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ALGEBRA 


AN 


ELEMENTARY  TEXT -BOOK 


Uniform   with  Part  I 


PART  II 


Completing  the  Work  and  containing  an  Index 

to  both  Parts. 

640  pp.,  post  8vo. 


BY  THE  SAME  AUTHOR 

AN     INTRODUCTION    TO    ALGEBRA 

For  the  Use  of  Secondary  Schools  and  Technical 
Colleges. 

Third  Edition.     Crown  8vo. 

Or  may  he  had  in  two  separate  Parts. 

I  have  kept  the  fundamental  principles  of  the 
subject  well  to  the  front  from  the  very  beginning. 
At  the  same  time  I  have  not  forgotten,  what 
every  mathematical  (and  other)  teacher  should 
have  perpetually  in  mind,  that  a  general  proposi- 
tion is  a  property  of  no  value  to  one  that  has  not 
mastered  the  particulars.  The  utmost  rigour  of 
accurate  logical  deduction  has  therefore  been  less 
my  aim  than  a  gradual  development  of  algebraic 
ideas.  In  arranging  the  exercises  I  have  acted 
on  a  similar  principle  of  keeping  out  as  far  as 
possible  questions  that  have  no  theoretical  or 
practical  interest. — Preface. 


AGENTS 

America    .     .      The   Macmillan   Company 

60   Fifth   Avenue,    New  York 

Australasia  .     Oxford  University   Press 

205    Flinders  Lane,   Melbourne 

Canada     .     .     The   Macmillan   Co.  of  Canada,   Ltd. 

St.  Martin's   House,  70  Bond   Street,  Toronto,  2 

India    .     .     .     Macmillan  Sc  Company,   Ltd. 
276   Hornby   Road,   Bombay 
294  Bow   Bazar   Street,   Calcutta 
North   Beach   Road,   Madras 


ALGEBEA 

AN    ELEMENTAEY    TEXT-BOOK 

FOR  THE 

HIGHER  CLASSES  OF  SECONDARY  SCHOOLS 
AND  FOR  COLLEGES 


BY 


G.  CHRYSTAL,  M.A.,  LL.D. 

HONORARY   FELLOW   OF   CORPUS   CHRISTI   COLLEGE,    CAMBRIDGE  ; 
PROFESSOR    OF    MATHEMATICS    IN    THE    UNIVERSITY    OF    EDINBURGH 


PART  I. 

FIFTH    EDITION 


A.  &  C.  BLACK,  Ltd. 

4,  5  &  6  SOHO  SQUARE,  LONDON,  W.l. 
1926 


Printed  in  Great  Britain. 


'■  I  should  rejoice  to  see  .  .  .  morphology  introduced  into  tha 
elements  of  Algebra.  '— Sylvester 


fa.  i 


9j 


PtihlUhed  July  1S86 

Reprinted,  with  corrections  and  additions,  1889 

New  impressions  1893  and  1898 

Reprinted,  with  corrections  and  additions,  1904  and  1910 

Reprinted  in  1920  and  1926 


PKEFACE  TO  THE  FIFTH  EDITION. 

In  this  Edition  considerable  alterations  have  been  made 
in  chapter  xii.  In  particular,  the  proof  of  the  theorem 
that  every  integral  equation  has  a  root  has  been  amplified, 
and  also  illustrated  by  graphical  considerations. 

An  Appendix  has  been  added  dealing  with  the  general 
algebraic  solution  of  Cubic  and  Biquadratic  Equations ; 
with  the  reducibility  of  equations  generally ;  and  with  the 
possibility  of  solution  by  means  of  square  roots.  As  the 
theorems  established  have  interesting  applications  in  Ele- 
mentary Geometry,  it  is  believed  that  they  may  find  an 
appropriate  place  in  an  Elementary  work  on  Algebra. 

G.  CHEYSTAL. 

29th  June  1904. 


PEEFACE  TO  THE  SECOND  EDITION. 

The  comparatively  rapid  sale  of  an  edition  of  over  two 
thousand  copies  of  this  volume  has  shown  that  it  has,  to 
some  extent  at  least,  filled  a  vacant  place  in  our  educational 
system.  The  letters  which  I  have  received  from  many 
parts  of  the  United  Kingdom,  and  from  America,  containing 
words  of  encouragement  and  of  useful  criticism,  have  also 
strengthened  me  in  the  hope  that  my  labour  has  not  been 


VI  PREFACE 

in  vain.  It  would  be  impossible  to  name  here  all  the 
friends  who  have  thus  favoured  me ;  and  I  take  this  oppor- 
tunity of  offering  them  collectively  my  warmest  thanks. 

The  present  edition  has  been  thoroughly  revised  and 
corrected.  The  first  chapter  has  been  somewhat  simplified ; 
and,  partly  owing  to  experience  with  my  own  pupils,  partly 
in  consequence  of  some  acute  criticism  sent  to  me  by  Mr. 
Levett  of  Manchester,  the  chapters  on  Indices  have  been 
recast,  and,  I  think,  greatly  improved.  In  the  verification 
and  correction  of  the  results  of  the  exercises  I  have  been 
indebted  in  a  special  degree  to  the  Rev.  John  Wilson, 
Mathematical  Tutor  in  Edinburgh. 

The  only  addition  of  any  consequence  is  a  sketch  of 
Horner's  Method,  inserted  in  chapter  xv.  I  had  originally 
intended  to  place  this  in  Part  II. ;  but,  acting  on  a  sugges- 
tion of  Mr.  Hayward's,  I  have  now  added  it  to  Part  I. 

To  help  beginners,  I  have  given,  after  the  table  of 
contents,  an  index  of  the  principal  technical  terms  used  in 
the  volume.  This  index  will  enable  the  student  to  turn  up 
a  passage  where  the  "  hard  word  "  is  either  defined  or  other- 
wise made  plain. 

G.  CHKYSTAL. 

Edinburgh,  11th  October  1889. 


PREFACE  TO  THE  FIRST  EDITION. 

The  work  on  Algebra  of  which  this  volume  forms  the  first 
part,  is  so  far  elementary  that  it  begins  at  the  beginning  of 
the  subject.  It  is  not,  however,  intended  for  the  use  of 
absolute  beginners. 

The  teaching  of  Algebra  in  the  earlier  stages  ought  to 
consist  in  a  gradual  generalisation  of  Arithmetic ;  in  other 
words,  Algebra  ought,  in  the  first  instance,  to  be  taught  as 
Aritlimetica  Universalis  in  the  strictest  sense.  I  suppose 
that  the  student  has  gone  in  this  way  the  length  of,  say,  the 
solution  of  problems  by  means  of  simple  or  perhaps  even 
cpiadratic  equations,  and  that  he  is  more  or  less  familiar 
with  the  construction  of  literal  formulae,  such,  for  example, 
as  that  for  the  amount  of  a  sum  of  money  during  a  given 
term  at  simple  interest. 

Then  it  becomes  necessary,  if  Algebra  is  to  be  any- 
thing more  than  a  mere  bundle  of  unconnected  rules,  to 
lay  down  generally  the  three  fundamental  laws  of  the 
subject,  and  to  proceed  deductively — in  short,  to  introduce 
the  idea  of  Algebraic  Form,  which  is  the  foundation  of  all 
the  modern  developments  of  Algebra  and  the  secret  of  analy- 
tical geometry,  the  most  beautiful  of  all  its  applications. 
Such  is  the  course  followed  from  the  beginning  in  this 
work. 


Vlll  PREFACE 

As  mathematical  education  stands  at  present  in  this 
country,  the  first  part  might  be  used  in  the  higher  classes 
of  our  secondary  schools  and  in  the  lower  courses  of  our 
colleges  and  universities.  It  will  he  seen  on  looking  through 
the  pages  that  the  only  knowledge  required  outside  of 
Algebra  proper  is  familiarity  with  the  definition  of  the 
trigonometrical  functions  and  a  knowledge  of  their  funda- 
mental addition-theorem. 

The  first  object  I  have  set  before  me  is  to  develop 
Algebra  as  a  science,  and  thereby  to  "increase  its  usefulness 
as  an  educational  discipline.  I  have  also  endeavoured  so 
to  lay  the  foundations  that  nothing  shall  have  to  be  un- 
learned and  as  little  as  possible  added  when  the  student 
comes  to  the  higher  parts  of  the  subject.  The  neglect  of 
this  consideration  I  have  found  to  be  one  of  the  most 
important  of  the  many  defects  of  the  English  text -books 
hitherto  in  vogue.  Where  immediate  practical  application 
comes  in  question,  I  have  striven  to  adapt  the  matter  to 
that  end  as  far  as  the  main  general  educational  purpose 
would  allow.  I  have  also  endeavoured,  so  far  as  possible, 
to  give  complete  information  on  every  subject  taken  up,  or, 
in  default  of  that,  to  indicate  the  proper  sources ;  so  that 
the  book  should  serve  the  student  both  as  a  manual  and 
as  a  book  of  reference.  The  introduction  here  and  there  of 
historical  notes  is  intended  partly  to  serve  the  purpose  just 
mentioned,  and  partly  to  familiarise  the  student  with  the 
great  names  of  the  science,  and  to  open  for  him  a  vista 
beyond  the  boards  of  an  elementary  text-book. 

As  examples  of  the  special  features  of  this  book,  I  may 
ask  the  attention  of  teachers  to  chapters  iv.  and  v.  With 
respect  to  the    opening    chapter,   which    the    beginner    will 


PREFACE  IX 

doubtless  find  the  hardest  in  the  hook,  I  should  mention 
that  it  was  written  as  a  suggestion  to  the  teacher  how 
to  connect  the  general  laws  of  Algebra  with  the  former 
experience  of  the  pupil.  In  writing  this  chapter  I  hud  to 
remember  that  I  was  engaged  in  writing,  not  a  book  on  the 
philosophical  nature  of  the  first  principles  of  Algebra,  but 
the  first  chapter  of  a  book  on  their  consequences.  Another 
peculiarity  of  the  work  is  the  large  amount  of  illustrative 
matter,  which  I  thought  necessary  to  prevent  the  vagueness 
which  dims  the  learner's  vision  of  pure  theory ;  this  has 
swollen  the  book  to  dimensions  and  corresponding  price 
that  require  some  apology.  The  chapters  on  the  theory  of 
the  complex  variable  and  on  the  equivalence  of  systems  of 
equations,  the  free  use  of  graphical  illustrations,  and  the 
elementary  discussion  of  problems  on  maxima  and  minima, 
although  new  features  in  an  English  text- book,  stand  so 
little  in  need  of  apology  with  the  scientific  public  that  I 
offer  none. 

The  order  of  the  matter,  the  character  of  the  illustra- 
tions, and  the  method  of  exposition  generally,  are  the  result 
of  some  ten  years'  experience  as  a  university  teacher.  I 
have  adopted  now  this,  now  that  deviation  from  accepted 
English  usages  solely  at  the  dictation  of  experience.  It 
was  only  after  my  own  ideas  had  been  to  a  considerable 
extent  thus  fixed  that  I  did  what  possibly  I  ought  to  have 
done  sooner,  viz.,  consulted  foreign  elementary  treatises. 
I  then  found  that  wherever  there  had  been  free  considera- 
tion of  the  subject  the  results  had  been  much  the  same. 
I  thus  derived  moral  support,  and  obtained  numberless  hints 
on  matters  of  detail,  the  exact  sources  of  which  it  would  be 
difficult  to  indicate.      I  may  mention,  however,  as  specimens 


PREFACE 


of  the  class  of  treatises  referred  to,  the  elementary  text- 
books of  Baltzer  in  German  and  Collin  in  French.  Anion" 
the  treatises  to  which  I  am  indebted  in  the  matter  of  theory 
and  logic,  I  should  mention  the  works  of  De  Morgan,  Pea- 
cock, Lipschitz,  and  Serret.  Many  of  the  exercises  have 
been  either  taken  from  my  own  class  examination  papers 
or  constructed  expressly  to  illustrate  some  theoretical  point 
discussed  in  the  text.  For  the  rest  I  am  heavily  indebted 
to  the  examination  papers  of  the  various  colleges  in  Cam- 
bridge. I  had  originally  intended  to  indicate  in  all  cases 
the  sources,  but  soon  I  found  recurrences  which  rendered 
this  difficult,  if  not  impossible. 

The  order  in  which  the  matter  is  arranged  will  doubt- 
less seem  strange  to  many  teachers,  but  a  little  reflection 
will,  I  think,  convince  them  that  it  could  easily  be  justified. 
There  is,  however,  no  necessity  that,  at  a  first  reading,  the 
order  of  the  chapters  should  be  exactly  adhered  to.  I  think 
that,  in  a  final  reading,  the  order  I  have  given  should  be 
followed,  as  it  seems  to  me  to  be  the  natural  order  into 
which  the  subjects  fall  after  they  have  been  fully  com- 
prehended in  their  relation  to  the  fundamental  laws  of 
Algebra. 

With  respect  to  the  very  large  number  of  Exercises, 
I  should  mention  that  they  have  been  given  for  the  con- 
venience of  the  teacher,  in  order  that  he  might  have,  year 
by  year,  in  using  the  book,  a  sufficient  variety  to  prevent 
mere  rote-work  on  the  part  of  his  pupils.  I  should  much 
deprecate  the  idea  that  any  one  pupil  is  to  work  all  the 
exercises  at  the  first  or  at  any  reading.  We  do  too  much 
of  that  kind  of  work  in  this  country. 

I  have  to  acknowledge  personal  obligations  to  Professor 


TREFACE  XI 

Tait,  to  Dr.  Thomas  Muir,  and  to  my  assistant,  Mr.  R  E. 
Allardice,  for  criticism  and  suggestions  regarding  the 
theoretical  part  of  the  work ;  to  these  gentlemen  and  to 
Messrs.  Mackay  and  A.  Y.  Fraser  for  proof  reading,  and 
for  much  assistance  in  the  tedious  work  of  verifying  the 
answers  to  exercises.  In  this  latter  part  of  the  work  I 
am  also  indebted  to  my  pupil,  Mr.  J.  Mackenzie,  and  to 
my  old  friend  and  former  tutor,  Dr.  David  Rennet  of 
Aberdeen. 

Notwithstanding  the  kind  assistance  of  my  friends  and 
the  care  I  have  taken  myself,  there  must  remain  many 
errors  both  in  the  text  and  in  the  answers  to  the  exercises, 
notification  of  which  either  to  my  publishers  or  to  myself 

will  be  gratefully  received. 

G.  CHRYSTAL. 


Edinburgh,  2&h  June  1880. 


CONTENTS. 


CHAPTER   I. 


FUNDAMENTAL    LAWS    AND    PROCESSES    OF    ALGEBRA. 

PAGE 

Laws  of  Association  and  Commutation  for  Addition  and  Subtraction  2-7 

Essentially  Negative  Quantity  in  formal  Algebra         ...  8 

Properties  of  0  .             .             .             .             .             .             .             .  11 

Laws  of  Commutation  and  Association  for  Multiplication        .             .  12 
Law  of  Distribution      .              .             .             .             .             .             .13 

Laws  of  Association,  Commutation,  and  Distribution  for  Division       .  14-19 

Properties  of  1  .             .             .             .             .             .             .             .  17 

Synoptic  Table  of  the  Laws  of  Algebra              ....  20 

Exercises  I.        ........  22 

Historical  Note             .......  24 


CHAPTER   II. 

MONOMIALS — LAWS    OF    INDICES — DEGREE. 


Laws  of  Indices 

Theory  of  Degree,  Constants  and  Variables 

Exercises  II.      . 


25-29 
30 
31 


CHAPTER   III. 

THEORY   OF    QUOTIENTS — FIRST    PRINCIPLES    OF    THEORY  OF    NUMBERS. 


Fundamental  Properties  of  Fractions  and   Fundamental  Operations 
therewith  ...... 

Exercises  III.    ...... 

Prime  and  Composite  Integers  .... 

Arithmetical  G.C.M.     . 

Theorems  on  the  Divisibility  of  Integers 

Remainder  and  Residue,  Periodicity  for  Given  Modulus 

Arithmetical  Fractionality        .... 

The  Resolution  of  a  Composite  Number  into  Prime  Factors  is  unique 
General  Theorem  regarding  G.C.M.,  and  Corollaries    . 
The  Number  of  Primes  is  infinite 
Exercises  IV.     . 


33-36 
36 
38 
39 
41 
42 
43 
44 
44 
47 
48 


XIV 


CONTENTS 


CHAPTER   IV. 


DISTRIBUTION  OF  PRODUCTS ELEMENTS   OF   THE   THEORY   OF   RATIONAL 


INTEGRAL    FUNCTIONS. 

Generalised  Law  of  Distribution  ..... 

Expansion  by  enumeration  of  Products  ;  Classification  of  the  Products 

of  a  given  set  of  letters  into  Types ;  S  and  II  Notations 
Principle  of  Substitution 
Theorem  regarding  Sum  of  Coefficients 
Exercises  V. 

General  Theorems  regarding  the  Multiplication  of  Integral  Functions 
Integral  Functions  of  One  Variable 

Product  of  Binomials 

Binomial  Theorem     .... 

Detached  Coefficients 

Addition  rule  for  calculating  Binomial  Coefficients,  with  a  General 
isation  of  the  same 

xn±y7i  as  a  Product  .... 
Exercises  VI.     . 

Exercises  \Il.  .... 
Homogeneity    .... 

General  forms  of  Homogeneous  Integral  Functions 

Fundamental  Property  of  a  Homogeneous  Function 

Law  of  Homogeneity 

Most  general  form  for  an  Integral  Function 
Symmetry  ..... 

Properties  of  Symmetric  and  Asymmetric  Functions 

Rule  of  Symmetiy     .... 

Most  general  forms  of  Symmetric  Functions 
Principle  of  Indeterminate  Coefficients 
Table  of  Identities         .... 
Exercises  VIII. 


PAGE 

49 

51-54 
54 
55 
56 
57 

59-69 
60 
61 
64 

66 
68 
69 
70 

71-75 
72 
73 
74 
75 

75-79 
76 
77 
78 
79 
81 
83 


CHAPTER  V. 

TRANSFORMATION  OF  THE  QUOTIENT  OF  TWO  INTEGRAL  FUNCTIONS. 


Algebraic  Integrity  and  Fractionality  .... 

Fundamental  Theorem  regarding  Divisibility  . 

Ordinary  Division-Transformation,  Integral  Quotient,  Remainder 

Binomial  Divisor,  Quotient,  and  Remainder    . 

Remainder  Theorem      ...... 

Factorisation  by  means  of  Remainder  Theorem 
Maximum  number  of  Linear  Factors  of  an  Integral  Function  of  a; 
New  basis  for  the  Principle  of  Indeterminate  Coefficients 
Continued  Division       ...... 


85 
86 
86-93 
93 
96 
97 
98 
99 
102 


CONTENTS 


XV 


One  Integral  Function  expressed  in  powers  of  another . 

Expansion  in  the  form  Ao+Ai(aj  —  ai)  +  A%(x  —  «x)(a;  —  a2)  +  A$(x-ai) 

(x-(t2){x-a3)+  .  .  . 
Exercises  IX.    . 

CHAPTER   VI. 

GREATEST    COMMON    MEASURE    AND    LEAST    COMMON    MULTIPLE. 

G.C.M.  by  Inspection   .... 
Ordinary  process  for  Two  Functions     . 
Alternate  destruction  of  highest  and  lowest  terms 
G.C.M.  of  any  number  of  Integral  Functions  . 
General  Proposition  regarding  the  Algebraical  G.C.M., 
regarding  Algebraic  Primeness 

L.C.M. 

Exercises  X.       . 

CHAPTER   VII. 


PAOE 

105 

107 
108 


with  Corollaries 


112 
113 

117 
119 

119 
122 
124 


FACTORISATION    OF    INTEGRAL    FUNCTIONS. 

Tentative  Methods        .  .  .  .  .  .  .126 

General  Solution  for  a  Quadratic  Function  of  a;  .  .  128-137 

Introduction  of  Surd  and  Imaginary  Quantity  .  .  130-133 

Progression  of  Real  Algebraic  Quantity        ....         130 

Square  Root,  Rational  and  Irrational  Quantity         .  .  .         132 

Imaginary  Unit         .......         132 

Progression  of  Purely  Imaginary  Quantity   ....         133 

Complex  Quantity     .......  133 

Discrimination    of    the    different    cases    in     the    Factorisation    of 

ax'2  +  bx  +  c  .......         134 

Homogeneous  Functions  of  Two  Variables       .  .  .  .136 

Use  of  the  Principle  of  Substitution     .  .  .  .  .136 

Use  of  Remainder  Theorem       .  .  .  .  .  .138 

Factorisation  in  general  impossible       .  .  .  .  .139 

Exceptional  case  of  ax2  +  2hxy  +  by2  +  2gx  +  2fy  +  c        .  .  .140 

Exercises  XI.    .  .  .  .  .  .  .  .142 

CHAPTER   VIII. 

RATIONAL    FRACTIONS. 

General  Propositions  regarding  Proper  and  Improper  Fractions  144-147 

Examples  of  Direct  Operations  with  Rational  Fractions  .  147-150 

Inverse  Method  of  Partial  Fractions     ....  151-159 

General  Theorem  regarding  decomposition  into  Partial  Fractions     .         151 
Classification   of  the   various   species   of  Partial    Fractions,   with 

Methods  for  determining  Coefficients     .  .  .  .153 

Integral  Function  expansible  in  the  form   2{au  +  ai(x-  a)+  .   .   .  + 

ar-.1(x-a)1—1}(x-pY(x-y)t.  .  .    .....  155 

Exercises  XII.  .......  159 


XVI 


CONTENTS 


CHAPTER   IX. 


FURTHER    APPLICATIONS    TO    THE    THEORY    OF    NUMBERS. 

TAOE 

Expression  of  an  Integer  as  an  Integral  Factorial  Series  .  .         163 

Expression  of  a  Fraction  as  a  Fractional  Factorial  Series  .  .         165 

Scales  of  Arithmetical  Notation  ....  167-175 

Expression  of  an  Integer  in  a  Scale  of  given  Radix  .  .  .         167 

Arithmetical  Calculation  in  various  Scales   .  .  .  .169 

Expression  of  any  Fraction  as  a  Radix  Fraction        .  .  .170 

Divisibility  of  a  Number  and  of  the  Sum  of  its  Digits  by  r  -  1  ;  the 

"Nine  Test"     .......         174 

Lambert's  Theorem  .  .  .  .  .  .176 

Exercises  XIII.  .......         177 


CHAPTER   X. 

IRRATIONAL    FUNCTIONS. 

Interpretation  of  scW"    .......         180 

Consistency  of  the  Interpretation  with  the  Laws  of  Indices  Examined         182 
Interpretation  of  a;0       .  .  .  .  .  .  .185 

Interpretation  of  x~m    .......         186 

Examples  of  Operation  with  Irrational  Forms  .  .  187-189 

Rationalising  Factors    ......  189-198 

Every  Integral  Function  of  \Jp,  \Jq,  \Jr,  &c,  can  be  expressed  in 
the  linear  form  A  +  B\Jp  +  C\/q  +  'D\Jr  +  .  .  .  +  ~E\/pq  +  .  .  . 
+Y"sfpqr+.  .  .  .  .  .  .  .  .193 

Rationalisation  of  any  Integral  Function  of  \Jp,  \Jq,  \Jr,  &c.         .         195 
Every  Rational  Function  of  \/p,  \Jq,  \/r,  &c,  can  be  expressed  in 

linear  form  .  .  .  .  .  .  .196 

General  Theory  of  Rationalisation         ....  197-198 

Exercises  XIV.  .......         199 

Historical  Note'  .......         201 


CHAPTER    XL 

ARITHMETICAL    THEORY    OF    SURDS. 

Algebraical  and  Arithmetical  Irrationality 

Classification  of  Surds  ..... 

Independence  of  Surd  Numbers 

Expression  of  \/{a  +  \/b)  in  linear  form 

Rational  Approximations  to  the  Value  of  a  Surd  Number 

Extraction  of  the  Square  Root 
Square  Root  of  an  Integral  Function  of  x 
Extraction  of  Roots  by  means  of  Indeterminate  Coefficients 
Exercises  XV.    ...... 


203 
204 

205-207 
207 

210-215 
211 
215 
217 
218 


CONTENTS 


XV11 


CHAPTER   XII. 

COMPLEX    NUMBERS. 

PACK 

Independence  of  Heal  and  Imaginary  Quantity           .             .             .  221 

Two-folduess  of  a  Complex  Number,  Argand's  Diagram         .             .  222 

If  x  +  yi  =  x'  +  y'i,  then  x  =  x',  y  =  y'     .....  224 

Every  Rational  Function  of  Complex  Numbers  is  a  Complex  Number    224-227 
If  <(>(x  +  yi)  =  X  +  Yi,  then  $(x-yi)=X-Yi  ;  if  <p(x  +  yi)  —  0,  then 

<f>(x-yi)  =  0            .......  226 

Conjugate  Complex  Numbers  ......  228 

Moduli.             ........  229 

If  x  +  yi  =  0,  then  |  x  +  yi  |  =  0  ;  and  conversely             .             .             .  229 

|  <p(x  +  yi)  |  =  \/{<P(x  +  yi)<P(x-yi)};  Particular  Cases  .             .             .  2l;0 
The  Product  of  Two  Integers  each  the  Sum  of  Two  Squares  is  the 

Sum  of  Two  Squares          ......  230 

Discussion  by  means  of  Argand's  Diagram      .  .  .  232-236 

Every  Complex  Number  expressible  in  the  form  r(cos  6  +  i  sin  d)  ; 

Definition  of  Amplitude    ......  232 

Addition  of  Complex  Numbers,  Addition  of  Vectors           .             .  233 
\z,  +  z2  +   .  .   .    +  zn\^\z1\  +  \z2\  +   .   .   .    +\zH\       .             .             .234 
The  Amplitude  of  a  Product  is  the  Sum  of  the  Amplitudes  of  the 

Factors  ;  Demoivre's  Theorem      .....  235 

Root    Extraction   leads   to    nothing   more    general    than    Complex 

Quantity 236-244 

Expression  of  ij{x  +  yi)  as  a  Complex  Number       .            .             .  237 

Expression  of  Mx  +  yi)  as  a  Complex  Number        .             .             .  238 

Every  Complex  Number  has  n  nth  roots  and  no  more         .             .  240 

Properties  of  the  nth  roots  of  ±1     .....  240 

Resolution  of  x"±  A  into  Factors      .....  243 
Every  Integral  Equation   has  at  least  one  root ;    Every   Integral 
Equation  of  the  ?ith  degree  has  n  roots  and  no  more  ;  Every 
Integral  Function  of  the  nth  degree  can  be  uniquely  resolved 
into  n  Linear  Factors         .....               244-250 

Upper  and  Lower  Limits  for  the  Roots  of  an  Equation        .             .  247 

Continuity  of  an  Integral  Function  of  z                    .             .             .  248 

Equimodular  and  Gradient  Curves  of/(r)  ....  248 

Argand's  Progression  towards  a  Root  .....  249 

Exercises  XVI. 251 

Historical  Note             .......  253 


CHAPTER   XIII. 

RATIO    AND    PROPORTION. 

Definition  of  Ratio  and  Proportion  in  the  abstract 
Propositions  regarding  Proportion 
Examples  ..... 

Exercises  XVII.  .... 

VOL.   I 


255 
257-264 
264-266 

267 

b 


XV111 


CONTENTS 


Ratio  and  Proportion  of  Concrete  Quantities 

Definition  of  Concrete  Ratio 

Difficulty  in  the  case  of  Incommensurables 

Euclidian  Theory  of  Proportion 
Variation  .... 

Independent  and  Dependent  Variables 

Simplest  Cases  of  Functional  Dependence 

Other  Simple  Cases  . 

Propositions  regarding  "Variation" 
Exercises  XVIII. 


CHAPTER   XIV. 


PAOE 

268-27.3 
269 
270 
272 

273-279 
273 
274 
275 
276 
279 


ON    CONDITIONAL    EQUATIONS    IN    GENERAL. 

General  Notion  of  an  Analytic  Function 
Conditional  Equation  contrasted  with  an  Identical  Equation 
Known  and  Unknown,  Constant  and  Variable  Quantities 
Algebraical  and  Transcendental  Equations  ;  Classification  of  Integral 

Equations  ..... 
Meaning  of  a  Solution  of  a  System  of  Equations 
Propositions  regarding  Determinateness  of  Solution 
Multiplicity  of  Determinate  Solutions 
Definition    of    Equivalent    Systems  ;    Reversible     and     Irreversible 

Derivations  ..... 

Transformation  by  Addition  and  Transposition  of  Terms 
Multiplication  by  a  Factor        .... 
Division  by  a  Factor  not  a  Legitimate  Derivation 
Every  Rational  Equation  can  be  Integralised  . 
Derivation  by  raising  both  sides  to  the  same  Power    . 
Every  Algebraical  Equation  can  be  Integralised  ;  Equivalence  of  the 

Systems,  Pj  =  0,  P2  =  0, . . .  P„  =  0,  and  L, P,  +  L2P2  +  . . .  +  LnP„  =  0, 

P2  =  0,  .   .   .  P„  =  0  .... 

Examination  of  the  Systems  P  =  Q,  R=S;  PR=QS,  R  =  S 
On  Elimination  .... 

Examples  of  Integralisation  and  Rationalisation 

Examples  of  Transformation 

Examples  of  Elimination 

Exercises  XIX.  .... 

Exercises  XX.    ..... 

Exercises  XXI.  .... 

CHAPTER   XV. 

VARIATION    OP   A    FUNCTION. 

Graph  of  a  Function  of  one  Variable    . 
Solution  of  an  Equation  by  means  of  a  Graph 
Discontinuity  in  a  Function  and  in  its  Graph 


281 
282- 

283 

283 

284 

286-288 

289 

289 
291 
292 
293 
294 
295 


296 
297 
298 
299-301 
302 
304 
305 
306 
308 


310 
313 
315 


CONTENTS 


XIX 


326 


PACK 

Limiting  Cases  of  Algebraic  Operation  .  318-322 

Definition  of  the  Increment  of  a  Function  ....  322 
Continuity  of  the  Sum  and  of  the  Product  of  Continuous  Functions  .  323 
Continuity  of  any  Integral  Function  .....  324 
Continuity  of  the  Quotient  of  Two  Continuous  Functions;  Exception  324 
General  Proposition  regarding  Continuous  Functions  .  .         325 

Number  of  Roots  of  an  Equation  between  given  limits  .  .         326 

An  Integral  Function  can  change  sign  only  by  passing  through  the 

value  0  ;  Corresponding  Theorem  for  any  Rational  Function 
Sign  of  the  Value  of  an  Integral  Function  for  very  small  and  for  very 

large  values  of  its  Variable  ;  Conclusions  regarding  the  Number 

of  Roots     ....... 

Propositions  regarding  Maxima  and  Minima    . 

Continuity  and  Graphical  Representation  of  f{x,  y) ;  Graphic  Surface 

Contour  Lines        ...... 

f(x,  y)  =  Q  represents  a  Plane  Curve      .... 

Graphical  Representation  of  a  Function  of  a  Single  Complex  Variabl 
Horner's    Method    for    approximating    to    the    Real    Roots   of    ar 

Equation    .... 
Multiplication  of  Roots  by  a  Constant 
Increase  of  Roots  by  a  Constant 
Approximate  Value  of  Small  Root 
Horner's  Process 
Example 

Extraction  of  square,  cube,  fourth,  .  . 
Exercises  XXII. 


roots  by  Horner's  Method 


328 
330 

331 
334 

335 

338-346- 
338 
339 
340 
341 

342-345 
346 
347 


CHAPTER   XVI. 

EQUATIONS    AND    FUNCTIONS    OF    FIRST    DEGREE. 

Linear  Equations  in  One  Variable         .... 

Exercises  XXIII.  ....... 

Linear  Equations  in  Two  Variables — Single  Equation,  One-fold  Infin 
ity  of  Solutions  ;  System  of  Two,  Various  Methods  of  Solution 
System  of  Three,  Condition  of  Consistency 

Exercises  XXIV.  ....... 

Linear  Equations  in  Three  Variables — Single  Equation,  Two-fold  In- 
finity of  Solutions  ;  System  of  Two,   One-fold  Infinity  of  Solu 
tions,  Homogeneous  System ;  System  of  Three,  in  general  Deter- 
minate,   Homogeneous  System,    Various  Methods  of  Solution 
S3'stems  of  more  than  Three  .... 

General  Theory  of  a  Linear  System       . 

General  Solution  by  means  of  Determinants     . 

Exercises  XXV.  ....... 

Examples  of  Equations  solved  by  means  of  Linear  Equations  . 

Exercises  XXVI.  ....... 


349, 

350 

351 

352- 

-364 

364 

365-372 
373 

374-376 
376 

379-383 
383 


XX 


CONTENTS 


PAGE 

Graph  of  ax  +  b              .......  385 

Graphical  Discussion  of  the  cases  6  =  0  ;  a  =  0  ;  a  =  0,  b  =  0      .             ».  388 

Contour  Lines  of  ax  +  by  +  c      ......  389 

Illustration  of  the  Solution  of  a  System  of  Two  Linear  Equations       .  390 
Cases   where   the    Solution   is    Infinite   or   Indeterminate    discussed 

graphically           .......  391 

Exceptional  Systems  of  Three  Equations  in  Two  Variables      .             .  393 

Exercises  XXVII.          ......  394 


CHAPTER   XVII. 

EQUATIONS    OF    THE    SECOND    DEGREE 
ax2  +  bx  +  c  =  0  has  in  general  just  two  roots 
Particular  Cases  .... 

General  Case,  various  Methods  of  Solution 
Discrimination  of  the  Roots 
Exercises  XXVIII.         .... 
Equations  reducible  to  Quadratics,  by  Factorisation,  by  Integralisa 

tion,  by  Rationalisation 
Exercises  XXIX.,  XXX. 
Exercises  XXXI. 

Reduction  by  change  of  Variable  ;  Reciprocal  Equations 
Rationalisation  by  introducing  Auxiliary  Variables 
Exercises  XXXII.  .... 

Systems  with  more  than  One  Variable  which  can  be  solved  by  means 
of  Quadratics  .... 

General  System  of  Order  1x2 

General  System  of  Order  2x2;  Exceptional  Cases 

Homogeneous  Systems 

Symmetrical  Systems 

Miscellaneous  Examples 
Exercises  XXXIII. 
Exercises  XXXIV. 
Exercises  XXXV. 


396 
397 
398 
400 

401 

402-406 
406 
407 

408-413 
413 
413 


414-427 
415 
416 
418 
420 
425 
427 
429 
430 


CHAPTER   XVIII. 

GENERAL    THEORY    OP    INTEGRAL    FUNCTIONS. 

Relations  between  Coefficients  and  Roots  ....  431 
Symmetric  Functions  of  the  Roots  of  a  Quadratic  .  .  .432 
Newton's  Theorem  regarding  Sums  of  Powers  of  the  Roots  of  any 

Equation    ........  436 

Symmetric  Functions  of  the  Roots  of  any  Equation  .  .  438 
Any  Symmetric  Function  expressible  in  terms  of  certain  elementary 

Symmetric  Functions         ......  440 


CONTENTS 


XXI 


Exercises  XXXYI. 

Special  Properties  of  Quadratic  Functions 

Discrimination  of  Roots,  Table  of  Results 

Generalisation  of  some  of  the  Results 

Condition  that  Two  Quadratics  have  Two  Roots  in  common 

Lagrange's  Interpolation  Formula    . 

Condition  that  Two  Quadratics  have  One  Root  in  common 

Exercises  XXXVII.       . 

Variation  of  a  Quadratic  Function  for  real  values  of  its  Variable  ; 

Analytical  and  Graphical  Discussion  of  Three  Fundamental  Cases, 

Maxima  and  Minima 


PAGE 

415 

447-453 

447 
449 
450 
451 
452 
453 


458 
461 
462 
463 


Examples  of  Maxima  and  Minima  Problems     . 

General  Method  of  finding  Turning  Values  by  means  of  Equal  Roots  . 

Example,  y  =  x3-  9x,2  +  24a;  +  3  .  ..... 

Example,  y=  (x2-  Sx  + 15)/*     ...... 

General  Discussion  of  y  =  (ax2  +  bx  +  c)j(a'x2  +  b'x  +  c'),  with  Graphs  of 

certain  Particular  Cases     .....  464-467 

Finding  of  Turning  Values  by  Examination  of  the  Increment  .         468 

Exercises  XXXVIII .469 


CHAPTER    XIX. 

SOLUTION    OF    PROBLEMS    BY    MEANS    OP    EQUATIONS. 

Choice  of  Variables  ;  Interpretation  of  the  Solution     . 
Examples  ....••• 

Exercises  XXXIX.         ....•• 

CHAPTER    XX. 

ARITHMETIC,    GEOMETRIC,    AND    ALLIED    SERIES. 

Definition  of  a  Series  ;  Meaning  of  Summation  ;  General  Term 
Integral  Series  .  .  .  .  ■ 

Arithmetic  Progression 

Sums  of  the  Powers  of  the  Natural  Numbers 

Sum  of  any  Integral  Series   . 

Arithmetic-Geometric  Series,  including  the  Simple  Geometric  Series 
as  a  Particular  Case 

Convergency  and  Divergency  of  Geometric  Series 
Properties  of  Quantities  in  A. P.,  in  G.P.,  or  in  H.P. 

Expression  of  Arithmetic  Series  by  Two  Variables 

Insertion  of  Arithmetic  Means 

Arithmetic  Mean  of  n  given  quantities 

Expression  of  Geometric  Series  by  Two  Variables 

Insertion  of  Geometric  Means 

Geometric  Mean  of  n  given  quantities 


471 

472-476 

476 


480 
482-488 

482 
484-487 

487 

489-494 
495 

496-502 
496 
497 
497 
499 
499 
500 


XX11 


CONTENTS 


Definition  of  Harmonic  Series  . 

Expression  in  terms  of  Two  Variables 

Insertion  of  Harmonic  Means 

Harmonic  mean  of  n  given  quantities 

Propositions  regarding  A.M.,  G.M.,  and  H.  M. 
Exercises  XL.    ..... 

Exercises  XLI.  ..... 

Exercises  XLII.  .... 

CHAPTEE    XXL 

LOGARITHMS. 

Discussion  of  ax  as  a  Continuous  Function  of  as 
Definition  of  Logarithmic  Function 
Fundamental  Properties  of  Logarithms 

Computation  and  Tabulation  of  Logarithms 
Mantissa  and  Characteristic  . 
Advantages  of  Base  10 
Direct  Solution  of  an  Exponential  Equation 
Calculation  of  Logarithms  by  inserting  Geometric  Means 
Alteration  of  Base     .... 

Use  of  Logarithms  in  Arithmetical  Calculation 

Interpolation  by  First  Differences 

Exercises  XLIII.  .... 

Historical  Note  .... 

CHAPTER    XXII. 


PAGE 
500 

501 
501 
501 
501 

502 
505 

507 


509 
511 
512 

513-519 
514 
515 

516 
517 
519 

519-523 


524 
527 
529 


THEORY    OP    INTEREST    AND    ANNUITIES. 

Simple  Interest,  Amount,  Present  Value,  Discount     .  .  531-532 

Compound   Interest,    Conversion -Period,    Amount,    Present    Value, 

Discount,  Nominal  and  Effective  Rate      .  .  .  533-535 

Annuities  Certain,  Accumulation  of  Forborne  Annuity,  Purchase  Price 
of  Annuity,  Terminable  or  Perpetual,  Deferred  or  Undeferred, 
Number  of  Years'  Purchase  ....  536-540 

Exercises  XLIV.  .......         540 


APPENDIX. 

Commensurable  Roots,  Reducibility  of  Equations 

Equations  Soluble  by  Square  Roots 

Cubic    ...... 

Biquadratic,  Resolvents  of  Lagrange  and  Descartes 
Possibility  of  Elementary  Geometric  Construction 
Exercises  XLV.  .... 


RESULTS   OF   EXERCISES. 


543-546 
546-548 
549 
550 
551 
553 

555 


INDEX  OF  PRINCIPAL  TECHNICAL  TEEMS 
USED  IN  PAET  I. 


Addition  Eule  for  binomial  coefficients, 
66 

Afline  of  a  complex  number,  223 

Algebraic  sum,  10 

Algebraical  function,  ordinary,  281 

Alternating  function,  77 

Amount,  532 

Amplitude  of  a  complex  number,  236 

Annuity,  certain,  contingent,  termin- 
able, perpetual,  immediate,  deterred, 
forborne,  number  of  years'  purchase, 
536  et  seq. 

Antecedent  of  a  ratio,  255 

Antilogaritlim,  518 

Argand-diagram,  222 

Argand's  progression,  249 

Argument,  524 

Arithmetic  means  and  arithmetic  mean, 
497 

Arithmetic  progression,  482 

Arithmetico-geometric  series,  491 

Association,  3,  12 

Auxiliary  variables,  380 

Base  of  an  exponential  or  logarithm,  511 
Binomial  theorem,  62 

Characteristic,  514 

Coefficient,  30 

Commensurable,  203 

Common  Measure  and  Greatest  Common 

Measure  (arithmetical  sense),  38,  39  ; 

algebraical  sense,  111 
Commutation,  4,  12 
Complex  number  or  quantity,  133,  221 
Conjugate  complex  numbers,  228 
Consequent  of  a  ratio,  2f>5 
Consistent  system  of  equations,  288 
Constant,  30 
Continued  division,  102 
Continued  proportion,  256 
Continuity  of  a  function,  317,  323,  324, 

336 
Contour  lines  of  a  function,  333 
Couvergency  of  a  series,  493 
Conversion-period  (for  interest),  533 

Degree,  30,  58 
Degree  of  an  equation,  284 
Derivation  of  equations,  290 
Detached  coefficients.  63   91 


Determiuateness  of  a  system  of  equa- 
tions, 286 
Differences  (first),  521 
Discontinuity  of  a  function,  317 
Discount,  532 
Discriminant,  134,  141 
Distribution,  13,  49 
Divergency  of  a  series,  493 
Divisibility  (algebraical  sense),  85 
Divisibility  (arithmetical  sense),  38 

Efjminant  (or  resultant),  415.  430 

Elimination,  298 

Equation,  conditional,  282 

Equation  and  equality  (identical),  22 

Equimodular  curves,  248 

Equiradical  surds,  204 

Equivalence    of   systems    of    equations, 

289 
Exponent,  25 
Exponential  function,  509 
Exponential  notation  (expa),  511 
Extraneous  solutions,  294 
Extremes  and    means  of  a  proportion, 

256 

Factor  (arithmetical  sense),  38 
Fractional  (algebraical  sense),  30,  85 
Fractional  (arithmetical  sense),  43 
Freehold,  value  of,  539 
Function,  analytical,  281 
Function,  rational,  integral,  algebraical, 
58 

Geometric  means  and  geometric  mean, 

499 
Geometric  series,  489 
Gradient  curves,  248 
Graph  of  a  function,  312,  333 
Graphical  solution  of  equations,  313 
Greatest  Common  Measure  (algebraical 

sense),  111 

Harmonic  means  and  harmonic  mean, 

501 
Harmonic  series,  500 
Homogeneity,  71 
Homogeneous  system  of  equations,  418 

Identity,  identical,  22 
Imaginary  unit  and  imaginary  quantity, 
132 


xxm 


XXIV 


INDEX 


Increment  of  a  function,  322 
Indeterminate  coefficients,  79,  100 
Indeterminate  forms,  318,  319,  320 
Indeterminateness  of  a  system  of  equa- 
tions, 286 
Index,  25 

Infinite  value  of  a  function,  315 
Infinitely  great,  318 
Infinitely  small,  318 
Integral  (algebraical  sense),  25,  85 
Integral  (arithmetical  sense),  37 
Integral  function,  58 
Integral  quotient  (algebraical  sense),  86 
Integral  series,  484 
Integralisation  of  equations,  296 
Integro-geometric  series,  492 
Interest,  simple  and  compound,  531,  533 
Interpolation,  524 
Inverse,  5,  14 

Irrationality  (algebraic),  203,  240 
Irrationality  (arithmetical),  203 
Irreducible  case  of  cubic,  549 
Irreducible  equation,  545 
Irreversible  derivation,  290 

Laws  of  Algebra,  fundamental,  20 
Least    Common    Multiple    (algebraical 

sense),  122 
Limiting  cases,  318 
Linear  (algebraic  sense),  138 
Linear  irrational  form,  193 
Logarithmic  function,  511 

Manifoldness,  496 
Mantissa,  514 

Maxima  values  of  a  function,  330 
Mean  proportionals,  256 
Minima  values  of  a  function,  330 
Modulus  (arithmetical  sense),  43 
Modulus  of  a  complex  number,  229 
Modulus  of  system  of  logarithms,  519 
Monomial  function,  30 

Negative  quantity,  9 
Nine-test,  175 

Operand  and  operator,  4 

Order  of  a  symmetric  function,  439 

Partial  fractions,  151 

Pascal's  triangle,  67 

Periodicity  of  integers,  43 

II-notation,  53 

l'rime  (arithmetical  sense),  38 

Primeness  (algebraical),  120 

Principal,  532 

Principal  value  of  a  root,  182 


Proper  fraction  (algebraical  sense),  86, 

144 
Proportion,  256,  269 
Proportional  parts,  526 

Quantity,  ordinary  algebraic,  130 

Rate  of  interest,  nominal  and  effective, 

535 
Ratio,  255,  268 
Rational  (algebraic  sense),  144 
Rational  fraction,  144 
Rationalisation  of  equations,  296 
Rationalising  factor,  190,  197 
Reciprocal  equations,  410 
Reducibility  of  an  equation,  545 
Remainder  (algebraical  sense),  86 
Remainder  (arithmetical  sense),  42 
Remainder  theorem,  93 
Residue  (arithmetical  sense),  42 
Resolvent  of  a  biquadratic,  550 
Resultant  equation,  415 
Reversible  derivation,  290 
Root  of  an  equation,  284 
Roots  of  a  function,  313 

Scales  of  notation,  168 

Series,  480 

Similar  surds,  204 

S-notation,  53 

Solution    of    an    equation,    formal    and 

approximate  numerical,  284 
Substitution,  principle  of,  18 
Sum  (finite)  of  a  series,  481 
Sum  (to  infinity)  of  a  series,  493 
Surd  number,  132 
Surd  number,  monomial,  binomial,  &c, 

203,  204 
Symmetrical  system  of  equations,  420 
Symmetry,  75 

Term,  30,  58 

Transcendental  function,  282 
Turning  values  of  a  function,  330 
Type  (of  a  product),  52 

Unity  (algebraical  sense  of),  17 

Variable,  30 

Variable,   independent  and  dependent, 

273 
Variation  of  a  function,  311 
"  Variation  "  (old  sense  of),  273,  275 

Weight  of  a  symmetric  function,  434 
Zero  (algebraical  sense  of),  11,  14 


CHAPTEK   I. 

The  Fundamental  Laws  and  Processes  of  Algebra 
as  exhibited  in  ordinary  Arithmetic. 

§1.1  The  student  is  already  familiar  with  the  distinction 
between  abstract  and  concrete  arithmetic.  The  former  is  con- 
cerned with  those  laws  of,  and  operations  with,  numbers  that  are 
independent  of  the  things  numbered ;  the  latter  is  taken  up 
with  applications  of  the  former  to  the  numeration  of  various 
classes  of  things. 

Confining  ourselves  for  the  present  to  abstract   arithmetic, 
let  us  consider  the  following  series  of  equalities  : — 
2623     1023     2623x3  +  1023x61 

ITT*- 3~~~~  61x3 

70272      00i 

= =  384. 

183 

The  first  step  is  merely  the  assertion  of  the  equivalence  of 
two  different  sets  of  operations  with  the  same  numbers.  The 
second  and  third  steps,  though  doubtless  based  on  certain  simple 
laws  from  which  also  the  first  is  a  consequence,  nevertheless 
require  for  their  direct  execution  the  application  of  certain  rules, 
of  a  kind  to  which  the  name  arithmetical  is  appropriated. 

We  have  thus  shadowed  forth  two  great  branches  of  the  higher 
mathematics: — one,  algebra,  strictly  so  called,  that  is,  the  theory  of 
operation  with  numbers,  or,  more  generally  speaking,  with  quanti- 
ties ;  the  other,  the  higher  arithmetic,  or  theory  of  numbers.  These 
two  science?  are  identical  as  to  their  fundamental  laws,  but  differ 
widely  in  their  derived  processes.  As  is  usual  in  elementary 
text-books,  the  elements  of  both  will  be  treated  in  this  work. 
VOL.  I  B 


2  REPRESENTATIVE  GROUPS  chap. 

§  2.]  Ordinary  algebra  is  simply  the  general  theory  of  those 
operations  with  quantity  of  which  the  operations  of  ordinary 
abstract  arithmetic  are  a  particular  case. 

The  fundamental  laws  of  this  algebra  are  therefore  to  be 
sought  for  in  ordinary  arithmetic. 

However  various  and  complex  the  operations  of  arithmetic 
may  seem,  it  appears  on  consideration  that  they  are  merely  the 
result  of  the  application  of  a  very  small  number  of  fundamental 
principles.  To  make  this  plain  we  return  for  a  little  to  the  very 
elements  of  arithmetic. 

ADDITION, 

AND   THE    GENERAL    LAWS    CONNECTED    THEREWITH. 

§  3.]  When  a  group  of  things,  no  matter  how  unlike,  is  con- 
sidered merely  with  reference  to  the  number  of  individuals  it 
contains,  it  may  be  represented  by  another  group,  the  individuals 
of  which  are  all  alike,  provided  only  there  be  as  many  individuals 
in  the  representative  as  in  the  original  group.  The  members  of 
our  representative  group  may  be  merely  marks  (l's  say)  on  a 
piece  of  paper.  The  process  of  counting  a  group  may  therefore 
be  conceived  as  the  successive  placing  of  l's  in  our  representa- 
tive group,  until  we  have  as  many  l's  as  there  are  individuals 
in  the  group  to  be  numbered.  This  process  of  adding  a  1  is 
represented  by  writing   +  1.      We  may  thus  have 

+  1,       +1  +  1,      +1  +  1  +  1,       +1  +  1  +  1  +  1,  &c, 

as  representative  groups  or  "numbers."  As  the  student  is  of 
course  aware,  these  symbols  in  ordinary  arithmetic  are  abbreviated 

int0  1,      2,      3,      4,&c. 

Hence  using  the  symbol  "  =  "  to  stand  for  "  the  same  as,"  or 
"replaceable  by,"  or  "equal  to,"  we  have,  as  definitions  of  1,  2, 
3,  4,  &c, 

1=  +1, 

2=  +1  +  1, 

3-  +1  +  1  +  1, 

4=  +  1  +  1  +  1  +  1,  &c. 


I  ASSOCIATION  IN  ADDITION  3 

And  there  is  a  further  arrangement  for  abridging  the  repre- 
sentation of  large  numbers,  which  the  student  is  familiar  with  as 
the  decimal  notation.  With  numerical  notation  we  are  not 
further  concerned  at  present,  but  there  is  a  view  of  the  above 
equalities  which  is  important.  After  the  group  +1  +  1  +  1  has 
been  finished  it  may  be  viewed  as  representing  a  single  idea  to 
the  mind,  viz.  the  number  "  three."  In  other  words,  we  may- 
look  at  +1  +  1  +  1  as  a  series  of  successive  additions,  or  we 
may  think  of  it  as  a  whole.  When  it  is  necessary  for  any 
purpose  to  emphasise  the  latter  view,  we  enclose  +1  +  1  +  1  in 
a  bracket,  thus  (  +  1  +  1  +  1) ;  and  it  will  be  observed  that  pre- 
cisely the  same  result  is  attained  by  writing  the  symbol  3  in 
place  of  +  1  +  1  +  1,  for  in  the  symbol  3  all  trace  of  the  for- 
mation of  the  number  by  successive  addition  is  lost.  We  might 
therefore  understand  the  equality  or  equation 

3=  +1  +  1  +  1 
to  mean  (  +  1  +  1  +  1)=  +1  +  1  +  1, 

and  then  the   equation  is   a  case   of  the   algebraical  Law   of 
Association. 

The  full  meaning  of  this  law  will  be  best  understood  by  con- 
sidering the  case  of  two  groups  of  individuals,  say  one  of  three 
and  another  of  four.  If  we  wish  to  find  the  number  of  a  group 
made  up  by  combining  the  two,  we  may  adopt  the  child's  process 
of  counting  through  them  in  succession,  thus, 

+  1  +  1  +  1  |    +1  +  1  +  1  +  1  =  7. 
But  by  the  law  of  association  we  may  write  for   +1  +  1  +  1 

(+1  +  1  +  1), 
and  for   +1  +  1  +  1  +  1 

(  +  1  +  1  +  1  +  1), 

and  we  have      +  (+  1  +  1  +  1)  +  (+  1  +  1  +  1  +1)  =  7, 

or  +3  +  4  =  7. 

It  will  be  observed  that  we  have  added  a  +  in  each  case  be- 
fore the  bracket,  and  it  may  be  asked  how  this  is  justified.  The 
answer  is  simply  that  setting  down  a  representative  group  of 
three  individuals  is  an   operation  of  exactly  the  same  nature  as 


4  COMMUTATION  IN  ADDITION  chap. 

setting  down  a  group  of  one.  The  law  of  association  for  addition 
worded  in  this  way  for  the  simple  case  before  us  would  be  this  : 
To  set  down  a  representative  group  of  three  individuals  is  the  same 
as  to  set  down  in  succession  three  representative  individuals. 

The  principle  of  association  may  be  carried  further.  The 
representative  group  +3  +  4  may  itself  enter  either  as  a  whole 
or  by  its  parts  into  some  further  enumeration :  thus, 

+  6  +  (  +  3  +  4)=  +6  +  3  +  4 
is  an  example  of  the  law  of  association  which  the  student  will 
have  no  difficulty  in  interpreting  in  the  manner  already  indi- 
cated. The  ultimate  proof  of  the  equality  may  be  regarded  as 
resting  on  a  decomposition  of  all  the  symbols  into  a  succession 
of  units.  There  is,  of  course,  no  limit  to  the  complication  of 
associations.     Thus  we  have 

+  [(  +  9  +  8)  +  {  +  6  +  (  +  5  +  3)}]  +  {  +  6  +  (  +  3  +  5)} 
"  =  +  (  +  9  +  8)  +  {  +  6  +  (  +  5  +  3)}  +  6  +  (  +  3  +  5), 
=  +9  +  8  +  6  +  (  +  5  +  3)  +  6  +  3  +  5, 
=  +9  +  8  +  6  +  5  +  3  +  6  +  3  +  5, 

each  single  removal  of  a  bracket  being  an  assertion  of  the  law 
of  association.  The  student  will  remark  the  use  of  brackets  of 
different  forms  to  indicate  clearly  the  different  associations. 

§  4.]  It  follows  from  the  definitions 

3=  +  1  +  1  +  1,      2  =  +1  +  1, 
that  +3  +  2=  +2  +  3; 

and  "by  a  similar  proof  we  might  show  that 

+  3  +  4  +  6=  +3  +  6  +  4=  +4  +  3  +  6,  &c. ; 
in  other  words,  the  order  in  which  a  series  of  additions  is  arranged 
is  indifferent. 

This  is  the  algebraical  Law  of  Commutation,  and  it  will 
be  observed  that  its  application  is  unrestricted  in  arithmetical 
operations  where  additions  alone  are  concerned.  The  statement 
of  this  law  at  once  suggests  a  principle  of  great  importance  in 
algebra,  namely,  the  attachment  of  the  "  symbol  of  operation  "  or 
"  operator  "  to  the  number,  or,  more  generally  speaking,  "  subject  " 
or  "  operand,"  on  which  it  acts.     Tims  in  the  above  equations 


I  SUBTEACTION  DEFINED  0 

the  +  before  the  3  is  supposed  to  accompany  the  3  when  it 
is  transferred  from  one  part  of  the  chain  of  additions  to  another. 
The  operands  in  +3,  +4,  and  +  6  are  already  complex  ;  and 
it  may  be  shown  by  a  further  application  of  the  reasoning  used 
in  the  beginning  of  this  article  that  the  operand  may  be  complex 
to  any  degree  without  interfering  with  the  validity  of  the  com- 
mutative law ;  for  example, 

+   {+3  +  (  +  2  +  3)}  +  (  +  6  +  8) 
=  +  (  +  G  +  8)  +  {  +  3  +  (  +  2  +  3)}  , 

of  which  a  proof  might  also  be  given  by  first  dissociating,  then 
commutating  the  individual  terms  +6,  +8,  '+  3,  &c,  and  then 
reassociating. 

The  Laiv  of  Commutation,  thus  suggested  by  arithmetical  considera- 
tions, is  noiv  laid  down  as  a  general  law  of  algebra ;  and  forms  a 
part  of  the  definition  of  the  algebraic  symbol  +  .* 

SUBTRACTION. 

§  5.]  For  algebraical  purposes  the  most  convenient  course  is 
to  define  subtraction  as  the  inverse  of  addition ;  or,  as  is  more 
convenient  for  elementary  exposition,  we  lay  down  that  addition 
and  subtraction  are  inverse  to  each  other,  t  By  this  we  mean 
that,  whatever  the  interpretation  of  the  operation  +  b  may  be, 
the  operation  -  b  annuls  the  effect  of  +  b  ;  and  vice  versa. 

Thus,  -  is  defined  relatively  to  +  by  the  equation 

+  a-  b  +  b=  +  a  (1), 

or  +  a  +  b-b-  +a  (2). 

These  might  also  be  written  f  f 


*  See  the  general  remarks  in  §  27. 

t  Here  we  virtually  assume  that  if  x  +  a  =  y  +  a,  then  x  =  y.  See  Hankel, 
Vorlcsungen  il.  d.  Complcxen  Zahlen  (Leipzig,  1867),  p.  19. 

tt  It  may  conduce  to  clearness  in  following  some  of  the  above  discussions  to 
remember  that  the  primary  view  of  a  chain  of  operations  written  in  any  order 
is  that  the  operations  are  to  be  carried  out  successively  from  left  to  right  ; 
for  example,  if  we  think  merely  of  the  last  addition,  +2  +  3  +  5  +  6  in  more  fully 
expressive  symbols  means  +  (+2  +  3  + 5) +  6,  that  is,  +  10  +  6;  +a+b+c  means 
+  (  +  a  +  b)  +  c;  +a~b  +  c  means  +(+a-b)  +  c;  and  so  on.  We  may  here  re- 
mind the  reader  that,  in  ordinary  practice,  when  +  occurs  before  the  first  member 
of  a  chain  of  additions  and  subtractions,  it  is  usually  omitted  for  brevity. 


6  LAWS  OF  COMMUTATION  AND  ASSOCIATION  chap. 

+  (  +  a-b)  +  b=  +  a  (T), 

+  (  +  a  +  b)-b  =  +  a  (2'). 

From  a  quantitative  point  of  view  we  might  put  the  matter 
thus  :  the  question,  What  is  the  result  of  subtracting  b  from  a  1 
is  regarded  as  the  same  as  the  question,  What  must  be  added  to 
+  b  to  produce  +  a  1  and  the  quantity  which  is  the  answer  to 
this  question  is  symbolised  by  +  a-b.  Starting  with  the  defini- 
tion involved  in  (1)  and  (2),  and  putting  no  restriction  upon  the 
operands  a  and  b,  or,  what  is  the  same  thing  from  a  quantitative 
point  of  view,  assuming  that  the  quantity  +  a-b  always  exists,  we 
may  show  that  the  laws  of  commutation  and  association  hold  for 
chains  of  operations  whose  successive  links  are  additions  and  sub- 
tractions. We,  of  course,  assume  the  commutative  law  for  addi- 
tion, having  already  laid  it  down  as  one  of  our  fundamental  laws. 
§  6.]  Since  +  a-  c  +  c=  +  a  by  the  definition  of  the  mutual 
relation  between  addition  and  subtraction,  we  have 

a+b-c=a-c+c+b-c; 
=  a  -  c  +  b  +  c  -  c, 

by  law  of  commutation  for  addition  ; 
=  a-c  +  b  (1), 

by  definition  of  subtraction. 
Also  a-b-c  =  a-c  +  c-b-c, 

by  definition  ; 
=  a-c-b  +  c-c, 

by  case  (1) ; 
=  a~c-b  (2). 

by  definition 

Equations  (1)  and  (2)  may  be  regarded  as  extending  the  law 
of  commutation  to  the  sign  -  .*     We  can  now  state  this  law 

fully  as  follows  : — 

±a±b=  ±b±a; 


*  It  might  be  objected  here  that  it  has  not  been  shown  that  -  c  may  come 
into  the  first  place  in  the  chain  of  operations.  The  answer  to  this  would  be 
that  +a-c-b  may  either  be  a  complete  chain  in  itself  or  merely  the  latter 
part  of  a  longer  chain,  say  p  +  a  -  c  -  b.  In  the  second  case  our  proof  would 
show  that  p+a-c-1>=p-c  +  a- b  J  and  the  nature  of  algebraic  generality 


i  FOR  ADDITION  AND  SUBTRACTION  7 

or,  in  words,  In  any  chain  of  additions  and  subtractions  the  different 
members  may  be  written  in  any  order,  each  with  its  proper  sign 
attached. 

Here  the  full  significance  of  the  attachment  of  the  operator 
to  the  operand  appears.  Thus  in  the  following  instance  the 
quantities  change  places,  carrying  their  signs  of  operation  with 
them  in  accordance  with  the  commutative  law  : — 

+  3-2  +  1-1=  +3  +  1-1-2, 
=  +3-1  +  1-2, 
=  -2-1  +  1+3. 

§  7.]  By  the  definition  of  the  mutual  relation  between  addi- 
tion and  subtraction,  we  have 

a  +  (  +  b-c)=  +  a  +  (  +  b-c)  +  c-c, 

=a+b-c  (1). 

Again,  by  the  definition, 

p  +  b-c  +  c-b  =p  +  b-b, 
=p. 
Hence  a-(  +  b-c)  =  a-(  +  b-c)  +  b-c  +  c-b; 

=  a-(  +  b-c)  +  (  +  b-c)  +  c-b, 

by  case  (1) ; 
=  a  +  c-b, 

by  the  definition  ; 
=  a-b+c  (2), 

by  the  law  of  commutation  already 
established. 
§  8.]  The  results  in  last  paragraph,  taken  along  with  those  of 
§  3  above,  may  be  looked  upon  as  establishing  the  law  of  associa- 
tion for  addition  and  subtraction.      This  law  may  be  symbolised 
as  follows  : — 

±(±a±b±c±  &c.)  =  ±  (  ±  a)  ±  (  ±  b)  ±  (  ±  c)  ±  &c, 
with  the  following  law  of  signs, 

+  (  +  «)=  +  a,      -(  +  «)=  -  a, 
+  (  -  a)  =  -  a,      -(-«)=+  a. 

requires  that  +a-c-b  should  not  have  any  property  in  composition  which  it 
has  not  per  se.     As  to  all  questions  of  this  kind  see  §  27. 


8  NON-ARITHMETICAL  CASES  chap. 

The  same  may  be  stated  in  words  as  follows : — If  any  number  of 
quantities  affected  with  the  signs  +  or  -  occur  in  a  bracket,  the  bracket 
may  be  removed,  all  the  signs  remaining  the  same  if  +  precede  the 
hracket,  each  +  being  changed  into  -  and  each  -  into  +  if  -precede 
the  bracket. 

In  the  above  symbolical  statement  double  signs  (  ±  )  have 
been  used  for  compactness.  The  student  will  observe  that  with 
three  letters  2x2x2x2,  that  is,  16,  cases  are  included.  Thus 
the  law  gives 

+  (  +  a  +  b  +  c)=  +  a  +  b  +  c, 
+  (-a  +  b  +  c)=  -  a  +  b  +  c, 
-(-a  +  b  +  c)=  +  a-b  -  c,  &c. 

§  9.]  It  will  not  have  escaped  the  student  that,  in  the  as- 
sumption that  +  a  -  b  is  a  quantity  that  always  exists,  we  have 
already  transcended  the  limits  of  ordinary  arithmetic.  He  will 
therefore  be  the  less  surprised  to  find  that  many  of  the  cases 
included  under  the  laws  of  commutation  and  association  exhibit 
operations  that  are  not  intelligible  in  the  ordinary  arithmetical 
sense. 

If  a  =  3  and  b  =  2, 

then  by  the  law  of  association  and  by  the  definition  of  sub- 
traction 

+  3-2=  +1  +  2-2, 
=  +1, 
in  accordance  with  ordinary  arithmetical  notions. 
On  the  other  hand,  if 

a  =  2  and  b  =  3, 

then  by  the  laws  of  commutation  and  association  and  by  the 
definition  of  subtraction 

+  2-3=  +2-(  +  2+l), 
=  +2-2-1, 
=  -  1  +  2  -  2, 
=  -  1. 

Here  we  have  a  question  asked  to  which  there  is  no  ordinary 
arithmetical  answer,  and  an  answer  arrived  at  which  has  no 
meaning  in  ordinary  arithmetic. 


I  ESSENTIALLY  NEGATIVE  QUANTITIES  9 

Such  an  operation  as  +  2  -  3,  or  its  algebraical  equivalent, 
-  1,  is  to  be  expected  as  soon  as  we  begin  to  reason  about 
operations  according  to  general  laws  without  regard  to  the  appli- 
cation or  interpretation  of  the  results  to  be  arrived  at.  It  must 
be  remembered  that  the  result  of  a  series  of  operations  may  be 
looked  on  either  as  an  end  in  itself,  say  the  number  of  in- 
dividuals in  a  group,  or  it  may  be  looked  upon  merely  as  an 
operand  destined  to  take  place  in  further  operations.  In  the 
latter  case,  if  additions  and  subtractions  be  in  question,  it  must 
have  either  the  +  or  the  -  sign,  and  either  is  as  likely  to  occur 
and  is  as  reasonably  to  be  expected  as  the  other.  Thus,  as  the 
results  of  any  partial  operation,  +  1  and  -  1  mean  respectively 
1  to  be  added  and  1  to  be  subtracted. 

The  fact  that  the  operations  may  end  in  results  that  have  no 
direct  interpretation  as  ordinary  arithmetical  quantities  need  not 
disturb  the  student.  He  must  remember  that  algebra  is  the 
general  theory  of  those  operations  with  quantity  of  which  ordinary 
arithmetical  operations  are  particular  cases.  He  may  be  assured 
from  the  way  in  which  the  general  laws  of  algebra  are  established 
that,  when  algebraical  results  admit  of  arithmetical  meanings, 
these  results  will  be  arithmetically  right,  even  when  some  of  the 
steps  by  Avhich  they  have  been  arrived  at  may  not  be  arithmetic- 
ally interpretable.  On  the  other  hand,  when  the  end  results 
are  not  arithmetically  intelligible,  it  is  merely  in  the  first  instance 
a  question  of  the  consistency  of  algebra  with  itself.  As  to  what 
the  application  of  such  purely  algebraical  results  may  be,  that 
is  simply  a  question  of  the  various  uses  of  algebra  •  some  of  these 
will  be  indicated  in  the  course  of  this  treatise,  and  others  will 
be  met  with  in  abundance  by  the  student  in  the  course  of  his 
mathematical  studies.  It  will  be  sufficient  at  this  stage  to  give 
one  example  of  the  advantage  that  the  introduction  of  algebraic 
generality  gives  in  arithmetical  operations.  +  a  -  b  asks  the  ques- 
tion what  must  be  added  to  +  b  to  give  +  a.  If  a  =  3  and  b  —  2, 
the  answer  is  1 ;  if  a  =  2  and  b  =  3,  then,  arithmetically  speaking, 
there  is  no  answer,  because  3  is  already  greater  than  2.  But  if 
we  regard  +  a  -  b  as  asking  what  must  be  added  to  or  subtracted 


10  REDUCTION  OF  AN  ALGEBRAICAL  SUM  OHAP. 

from  +  b  to  get  +  a,  then  the  evaluation  of  +  a-b  in  any  case 
by  the  laws  of  algebra  will  give  a  result  whose  sign  will  indicate 
whether  addition  or  subtraction  must  be  resorted  to,  and  to  what 
extent ;  for  example,  if  a  =  3  and  b  =  2,  the  result  is  +  1,  which 
means  that  1  must  be  added  ;  if  a  =  2  and  5  =  3,  the  result  is 
-  1,  which  means  that  1  must  be  subtracted. 

§  10.]  The   application  of  the  commutative  and  associative 
laws  for  addition  and  subtraction  leads  us  to  a  useful  practical 
rule  for  reducing  to  its  simplest  value  an  expression  consisting 
of  a  chain  of  additions  and  subtractions. 
We  have,  for  example, 

+a-b+c+d-e-f+g 

=  +  a  +  c  +  d  +  g-b-  e  -/, 

=  +  (a  +  c  +  d  +  g)  -  (b  +  e  +  /), 

=  +  {  +  (a  +  c  +  d  +  g)-(b  +  e+f)}  (1), 

=  -  {  +  (b  +  e+f)-(a  +  c  +  d  +  g)}  (2). 

If  a+c+d+g  be  numerically  greater  than  b  +  e+f,  (1)  is 
the  most  convenient  form ;  if  a  +  c  +  d  +  g  be  numerically  less 
than  b  +  e  +  f,  (2)  is  the  most  convenient.  The  two  taken  to- 
gether lead  to  the  following  rule  for  evaluating  a  chain  of 
additions  and  subtractions  : — * 

Add  all  the  quantities  affected  ivith  the  sign  +  ,  also  all  those 
affected  with  the  sign  -  ,•  take  the  difference  of  the  two  sums  and  affix 
t/ie  sign  of  the  greater. 

Numerical  example : — 

+3-5+6+8-9-10+2 

=  +  (3  +  6  +  8  +  2)-(5  +  9  +  10), 

=  +19-24, 

=  -(24-19)=  -5. 

§  11.]  The  special  case  +a-a  deserves  close  attention.  A 
special  symbol,  namely  0,  is  used  to  denote  it.  The  operational 
definition  of  0  is  therefore  given  by  the  equations 

+  a  -  a=  -  a  +  a  =  0. 

In  accordance  with  this  Ave  have,  of  course,  the  results, 

*  Such  a  chain  is  usually  spoken  of  as  an  "algebraical  sum." 


I  PROPERTIES  OF   0  H 

b  +  0  =  b  =  b  -  0, 
and  +  0  =  -  0, 

as  the  student  may  prove  by  applying  the  laws  of  commutation 
and  association  along  with  the  definition  of  0. 

§  12.]  It  will  be  observed  that  0,  as  operationally  defined,  is 
to  this  extent  indefinite  that  the  a  used  in  the  above  definition 
may  have  any  value  whatever. 

It  remains  to  justify  the  use  of  the  0  of  the  ordinary 
numerical  notation  in  the  new  meaning.  This  is  at  once  done 
when  we  notice  that  in  a  purely  quantitative  sense  0  stands  for 
the  limit  of  the  difference  of  two  quantities  that  have  been  made 
to  differ  by  as  little  as  we  please. 

Thus,  if  we  consider  a  +  x  and  a, 

+  (a  +  x)  —  a  =  +  a-a  +  x  =  x. 
If  we  now  cause  the  x  to  become  smaller  than  any  assignable 
quantity,  the  above  equation  becomes  an  assertion  of  the  identity 
of  the  two  meanings  of  0. 


MULTIPLICATION. 

§  13.]  The  primary  definition  of  multiplication  is  as  an  ab- 
breviation of  addition.  Thus  +  a  +  a,  +  a  +  a  +  a,  +  a  +  a  +  a  +  a, 
&c,  are  abbreviated  into  +  a  x  2,  +  a  x  3,  +  a  x  4,  &c. ;  and,  in 
accordance  with  this  notation,  +  a  is  also  represented  by  +  a  x  1. 
a  x  2  is  called  the  product  of  a  by  2,  or  of  a  into  2  ;  a  is  also 
called  the  multiplicand  and  2  the  multiplier.  Instead  of  the 
sign  x  ,  a  dot,  or  mere  apposition,  is  often  used  where  no  am- 
biguity can  arise.  Thus  a  x  2,  a.  2,  and  a2  all  denote  the  same 
thing. 

.§  14.]  So  long  as  a  and  b  represent  integral  numbers,  as  is 

supposed  in  the  primary  definition  of  multiplication,  it  is  easy  to 

prove  that 

a x  b  =  b x  a ; 

or,  adopting  the  principle  of  attachment  of  operator  and  operand, 

with  full  symbolism  (see  above,  §  4), 

x  a  x  b  =  x  b  x  a. 


12  COMMUTATION  AND  ASSOCIATION  chap. 

The  same  may  be  established  for  any  number  of  integers,  for 

example, 

x  a  x  b  x  c  —  x  a  x  c  x  b  =  x  b  x  c  x  a,  &c. 

In  other  words,  The  order  of  operations  in  a  chain  of  multiplication 
is  indifferent. 

This  is  the  Commutative  Law  for  multiplication. 

§  15.]  We  may  introduce  the  use  of  brackets  and  the  idea  of 
association  in  exactly  the  same  way  as  we  followed  in  the  case 
of  addition.  Thus  in  x  a  x  (  x  b  x  c)  we  are  directed  to  multiply 
a  by  the  product  of  b  by  c.  The  Law  of  Association  asserts 
that  this  is  the  same  as  multiplying  a  by  b,  and  then  multiplying 
this  product  by  c.     Thus 

x  a  x  (  x  b  x  c)  =  x  a  x  b  x  c. 

The  like  holds  for  a  bracket  containing  any  number  of  factors. 
In  the  case  where  a,  b,  c,  &c,  are  integers,  a  proof  of  the  truth 
of  this  law  might  be  given  resting  on  the  definition  of  multi- 
plication and  on  the  laws  of  commutation  and  association  for 
addition. 

§  16.]  Even  in  arithmetic  the  operation  of  multiplication  is 
extended  to  cases  which  cannot  by  any  stretch  of  language  be 
brought  under  the  original  definition,  and  it  becomes  important 
to  inquire  what  is  common  to  the  different  operations  thus  com- 
prehended under  one  symbol.  The  answer  to  this  question, 
which  has  at  different  times  greatly  perplexed  inquirers  into  the 
first  principles  of  algebra,  is  simply  that  what  is  common  is  the 
formal  laws  of  operation  which  we  are  now  establishing,  namely, 
the  commutative  and  associative  laws,  and  another  presently  to  be 
mentioned.  These  alone  define  the  fundamental  operations  of 
addition,  multiplication,  and  division,  and  anything  further  that 
appears  in  any  particular  case  (for  example,  the  statement  that 
|  x  |  is  \  of  §)  is  merely  a  matter  of  some  interpretation, 
arithmetical  or  other,  that  is  given  to  a  symbolical  result  demon- 
strably in  accordance  with  the  laws  of  symbolical  operation. 

Acting  on  this  principle  we  now  lay  down  the  laws  of  com- 
mutation and  association  as  holding  for  the  operation  of  multi- 
plication, and,  indeed,  as  in  part  defining  it. 


i  FOR  MULTIPLICATION LAW  OF  DISTRIBUTION  13 

§  1 7.]  The  consideration  of  composite  multipliers  or  com- 
posite multiplicands  introduces  the  last  of  the  three  great  laws 
of  algebra. 

It  is  easy  enough,  if  we  confine  ourselves  to  the  primary 
definition  of  multiplication,  to  prove  that 

+  ax(  +  b  +  c)  =  +  a  x  b  +  a  x  c, 
+  a*(  +  b-c)=  +  a  x  b  -  a  x  c, 
(  +  a-b)x(  +  c-d)=+axc-axd-bxc  +  bxd. 

These  suggest  the  following,  which  is  called  the  Distributive 
Law  : — 

The  product  of  two  expressions,  each  of  which  consists  of  a  chain 
of  additions  and  subtractions,  is  equal  to  the  chain  of  additions  and 
subtractions  obtained  by  multiplying  each  constituent  of  the  first  expres- 
sion by  each  constituent  of  the  second,  setting  down  all  the  partial 
products  thus  obtained,  and  prefixing  the  +  sign  if  the  two  constituents 
previously  had  like  signs,  the  -  sign  if  the  constituents  previously  had 
unlike  signs. 

Symbolically,  thus  : — 

(±a±b)  x(±c±d) 

=  (± a)  x  (± c)  +  (± a)  x  (± d)  +  (± b)  x  (± c) 

+  (  ±  b)  x  (  ±  d), 

with  the  following  law  of  signs  : — 

(  +  a)  x  (  +  c)  =  +  ac,         (  +  a)  x  (  -  c)  =  -  ac, 
(  -  a)  x  (  +  c)  =  -  ac,  (  -  a)  x  (  -  c)  -  +  ac. 

There  are  sixteen  different  cases  included  in  the  above  equation, 
as  will  be  seen  by  taking  every  combination  of  one  or  other  of 
the  double  signs  before  each  letter. 

Thus  (  +  a-b)(  +  c  +  d) 

=  +  ac  +  ad  -be-  bd ; 

(-a-b)(-c  +  d) 

=  +  ac-  ad  +  bc-bd  ; 
and  so  on. 

There    may,    of   course,   be   as   many   constituents    in    each 

bracket    as   we    please.     If,   for   example,   there   be  m    in    one 


14  PROPERTY  OF  0 


CHAP. 


bracket  and  n  in  the  other,  there  will  be  mn  partial  products 
and  2m+n  different  arrangements  of  the  signs. 

Thus  (  +  a-b  +  c)(-d  +  e) 

-  -  ad  +  bd  -  cd  +  ae  -  be  +  ce  ; 
and  so  on. 

The  distributive  law,  suggested,  as  we  have  seen,  by  the 
primary  definition  of  multiplication,  is  now  laid  down  as  a  law 
of  algebra.  It  forms  the  connecting  link  between  addition  and 
multiplication,  and,  along  with  the  commutative  and  associative 
laws,  completes  the  definition  of  both  these  operations. 

§  18.]  By  means  of  the  distributive  law  we  can  prove  another 
property  of  0.  For,  if  b  be  any  definite  quantity,  subject  without 
restriction  to  the  laws  of  algebra,  we  have 

+  ba-ba=  +  bx(  +  a-a)  =  (  +  a-a)x(  +  b), 

-  -bx(  +  a-a)  =  (  +  a-a)x(-b), 

whence     0  =  (  +  i)x0  =  0x(  +  J)  =  (-J)x0  =  0x(-J); 
or  briefly  b  x  0  =  0  x  b  =  0. 

DIVISION. 

§  19.]  Division  for  the  purposes  of  algebra  is  best  defined  as 
the  inverse  operation  to  multiplication :  that  is  to  say,  the 
mutual  relation  of  the  symbols  x  and  -f-  is  defined  by 

x  a-^-b  x  b-  x  a  (1), 


or 


* 


x  a  x  b  -r-  b  =  x  a  (2). 


From  a  quantitative  point  of  view,  this  amounts  to  defining 
the  quotient  of  a  by  b,  that  is,  a  -i-  b,  as  that  quantity  which, 
when  multiplied  by  b,  gives  a. 

In  a  -f-  b,  a  is  called  the  dividend  and  b  the  divisor.  Some- 
times a  is  called  the  antecedent  and  b  the  consequent  of  the 
quotient. 

Another  notation  for  a  quotient  is  very  often  used,  namely,  T  or 

'     b 

a/b.  As  this  is  the  notation  of  fractions,  and  therefore  has 
a  meaning  already  attached  to  it  in  the  case  where  a  and  b 
are  integers,  it  is  incumbent  upon  us  to  justify  its  use  in  another 

*  See  second  footnote,  p.  5. 


I  QUOTIENT  AND  FRACTION  15 

meaning.     To  do  this  we  have  simply  to  remark  that  b  times  =-, 

that  is,  b  times  a  of  the  bih  parts  of  unity,  is  evidently  a  times 
unity,  that  is,  a  ;  also,  by  the  definition  of  a^-b,  b  times  a-r-b  is  a. 

Hence  we  conclude  that  7  is  operationally  equivalent  to  a-^-b  in 

the  case  where  a  and  b  are  integers.     No  further  justification  is 

necessary,  for  when  either  a  or  b,  or  both,  are  not  integers,  7 

loses  its  meaning  as  primarily  defined,  and  there  is  no  obstacle 
to  resrardinc;  it  as  an  alternative  notation  for  a-^-b. 

In  the  above  definition  we  have  not  written  the  signs  +  or  - 
before  a  and  b,  but  they  were  omitted  simply  for  brevity,  and  one 
or  other  must  be  understood  before  each  letter.    We  shall  continue 
to  omit  them  until  the  question  as  to  their  manipulation  arises. 

§  20.]  Since  division  is  fully  defined  as  the  inverse  of  multi- 
plication, we  ought  to  be  able  to  deduce  all  its  laws  from  the 
definition  and  the  laws  of  multiplication. 

We  have* 

X  a  X  b-i-C  =    xdvCXCxt-rC, 

by  definition  ; 

=  x  a-^-c  x  b  x  c-f-r, 

by    law    of    commutation    for 
multiplication  ; 
—  x  a-^-c  x  b  (1), 

by  definition. 
Again,  x  a-^-b-^c  -  xdvCxo-f  J-i-c, 

by  definition ; 

=  xa-^rC~bxc-^-c, 
by  case  ( 1 )  ; 

=    XO-rC-fi  (2), 

by  definition. 
In  this  way  we  establish  the  law  of  commutation  for  division. 

*  Here  again  the  remark  made  in  the  third  note  at  the  foot  of  p.  5  applies, 
namely,  axb-i-c  primarily  means,  if  we  think  only  of  the  last  operation,  the 
same  as  (a x  b) -4- c  ;  a^-bxc  the  same  as  (a-T-b)x  c  ;  and  so  on. 

As  in  the  case  of  +  a,  when  x  a  comes  first  in  a  chain  of  operations,  x  i 
in  practice  usually  omitted  for  brevity. 


is 


16      COMMUTATION  AND  ASSOCIATION  IN  MULTIPLICATION     chap. 

Taking  multiplication  and  division  together  and  attaching 
the  symbol  of  operation  to  the  operand,  we  may  now  give  the 
full  statement  of  this  law  as  follows  : — 

In  any  chain  of  multiplications  and  divisions  the  order  of  the 
constituents  is  indifferent,  provided  the  proper  sign  be  attached  to  each 
constituent  and  move  with  it. 

Or,  in  symbols,  for  two  constituents, 

*a*b  =  *  b*a, 
there  being  4  cases  here  included,  for  example, 

H-«  xi=  x  b  -~a, 

-i-a-i-b  =  -T-b-~a>  and  so  on. 

§  21.]  By  the  definition  of  the  mutual  relation  between 
multiplication  and  division,  we  have 

xax(x&-j-c)=  x  a  x  (^  x  b  -7-  c)  x  c  -7-  c, 

=  x  a  x  b-r-c  (1). 

Again,  since 

x p  x  b-r-c  x  c—  b  =  x p  xb-h-b, 

=  xp, 

therefore       xa-i-(xb-7-c)=  x  a  -f-  (  x  b  -f-  c)  x  b  4-  c  x  c  —  b  ; 

=  xa-7-(xb-7-c)x(xb-~c)xc-7-b, 

by  case  (1) ; 
=  x  a  x  c-i-b, 

by  definition  ; 
=  x  a~b  x  c  (2), 

by    the    law    of    commutation 
already  established. 

These  are  instances  of  the  law  of  association  for  division  and 
multiplication  combined,  which  we  may  now  state  as  follows : — 

When  a  bracket  contains  a  chain  of  multiplications  and  divisions, 
the  bracket  may  be  removed,  every  sign  being  unchanged  if  x  precede 
the  bracket,  and  every  sign  being  reversed  if  ■—  precede  the  bracket. 

Or,  in  symbols,  for  two  constituents, 

l(lalb)  =  l(la)l{lb), 


I  AND  DIVISION PROPERTIES  OF    1  17 

with  the  following  law  of  signs  : — 

x  (  x  a)  -  x  a,        x(Tfl)=Td, 
4-  (  x  rt)  =  4-  a,       4-  ( 4-  a)  =    •  ". 

In  the  above  equation  eight  cases  are  included,  for  example, 

x(-i-ox})=  -4- a  x  6, 

4-  (  -r  a  x  6)  =    xfl-rJ, 

■4-  (  4-  a  4-  6)  =  x  a  x  b, 

and  so  on. 

§   22.]  Just  as   in  subtraction  we   denote  the   special   case 

+  a  -  a  by  a  separate  symbol  0,  so  in  division  we  denote  x  a  4-  a 

by  a  separate  symbol  1 .     From  this  point  of  view,  1  has  a  purely 

operational  meaning,  and  we  can  prove  for  it  the  following  laws 

analogous  to  those  established  for  0  in  §  11 ; — 

x  a-r-a=  -r-  a  x  a  =  1, 
6x  1=6  =  64-1, 

x  1  =   4-  1. 

Like  0,  1  has  both  a  quantitative  and  a  purely  operational 
meaning.  Quantitatively  we  may  look  on  it  as  the  limit  of  the 
quotient  of  two  quantities  that  differ  from  each  other  by  a 
quantity  which  is  as  small  a  fraction  as  we  please  of  either.  For 
example,  consider  a  +  x  and  a,  then  the  equation 
(a  +  x)  4-  a  =  a  4-  a  +z-r-a 

=  1  +  X  4-  H 

becomes,  when  x  is  made  as  small  a  fraction  of  a  as  we  please, 
an  assertion  of  the  compatibility  of  the  two  meanings  of  1. 

It  should  be  noted  that,  owing  to  the  one-sidedness  of  the 
law  of  distribution  (that  is,  owing  to  the  fact  that  in  ordinary 
algebra  6  +  (  x  a  -f-c)  =  x  (b  +  a)  4-  (6  +  c)  is  not  a  legitimate  trans- 
formation), there  is  no  analogue  for  1  to  the  equation 

b  x  0  =  0, 
which  is  true  in  the  case  of  0. 

§  23.]  If  the  student  will  now  compare  the  laws  of  commuta- 
tion and  association  for  addition  and  subtraction  on  the  one  hand 
and  for  multiplication  and  division  on  the  other,  he  will  find  them 
to  he  formally  identical.     It  follows,  therefore,  that  so  far  as  these 
VOL.  I  C 


18  PRINCIPLE  OF  SUBSTITUTION  chap. 

laws  are  concerned  there  is  virtually  no  distinction  between  addi- 
tion and  subtraction  on  the  one  hand  and  multiplication  and 
division  on  the  other,  except  the  accident  that  we  use  the  signs 
+  and  —  in  the  one  case  and  x  and  -r-  in  the  other, — a  conclusion 
at  first  sight  a  little  startling.  This  duality  ceases  wherever  the 
law  of  distribution  is  concerned. 

§  24.]  We  have  already  been  led  to  consider  such  expressions 
as  +  (  +  2)  and  +  (  -  2),  and  to  see  that  +  a  may,  according  to 
the  value  given  to  a,  be  made  to  stand  for  +  (  +  2),  that  is,  +  2,  or 
+  (  -  2),  that  is,  -  2.  The  mere  fact  that  a  particular  sign,  say 
+  ,  stands  before  a  certain  letter,  indicates  nothing  as  to  its 
reduced  or  ultimate  value ;  the  sign  +  merely  indicates  what 
has  to  be  done  with  the  letter  when  it  enters  into  operation. 

In  what  precedes  as  to  division,  and  in  fact  in  all  our  general 
formulae,  we  may  therefore  suppose  the  letters  involved  to  stand 
for  positive  or  negative  quantities  at  pleasure,  without  affecting 
the  truth  of  our  statement  in  the  least. 

For  example,  by  the  law  of  distribution, 

(a  -  b)  (c  +  d)  =  ac  +  ad  -be  -  bd ; 

here  we  may,  if  we  like,  suppose  d  to  stand  for  —  d'. 
We  thus  have 

(a  -  6)  {c  +  (  -  d')}  =  ac  +  a(-  d')  -bc-b{-  d'), 

which  gives,  when  we  reduce  by  means  of  the  law  of  signs 
proper  to  the  case, 

(a  -  b)  (c  -  d')  =  ac  -  ad'  -  be  +  bd', 

which  is  true,  being  in  fact  merely  another  case  of  the  law  of 
distribution,  which  we  have  reproduced  by  a  substitution  from 
the  former  case.  This  principle  of  substitution  is  one  of  the  most 
important  elements  in  the  science  ;  it  is  this  that  gives  to 
algebraic  calculation  its  immense  power  and  almost  endless 
capability  of  development, 

§  25.]  We  have  now  to  consider  the  effect  of  explicit  signs 
attached  to  the  constituents  of  a  quotient.  As  this  is  closely 
bound  up  with  the  operation  of  the  distributive  law  for  division, 
it  will  be  best  to  take  the  two  together. 


I  DISTRIBUTION  OF  A  QUOTIENT  19 

The  full  symbolical  statement  of  this  law  for  a  dividend 
having  two  constituents  is  as  follows  : — 

(±a±b)  +  (±c)  =  (±a)  +  (±c)  +  (±b)  +  (±c), 
with  the  following  law  of  signs, 

(  +  a) -T-  (  +  c) -  +  a  -f-  c,         (  +  a)  -f-  (  -  c)  =  - o-f- c, 

(  -  a)  -r-  (  +  c)  =  -a-r-e,         ( -  a)  -5-  (  -  c)  =  +  a  -f-  c. 

Or  briefly  in  words — 

In  division  the  dividend  may  be  distributed,  the  signs  of  the  partial 
quotients  following  the  same  law  as  in  multiplication. 

The  above  equation  includes  of  course  eight  cases.  It  will 
be  sufficient  to  give  the  formal  proof  of  the  correctness  of  the 
law  for  one  of  them,  say 

(  +  a  —  6)-t-(  —  c)=  -  a -f- e  +  6 -f  e. 

By  the  law  of  distribution  for  multiplication,  we  have 

(  —  a  —  c  +  b  -T-  c)  x  (  -  c)  =  +  (a  -f-  c)  x  t'  -  (b  -i-  c)  x  c  ; 

-  +  a-b, 

by  the  definition. 

Hence  (  +  a—  i)-r-(  —  c)  =  (  —  a-r-c  +  J-r-c)  *  ( -  c) -f- ( - c) ; 

=  — a-f-e  +  6-T-c, 

by  the  definition. 

§  26.]  The  law  of  distribution  has  only  a  limited  application 
to  division,  for  although,  as  just  proved,  the  dividend  may  be 
distributed,  the  same  is  not  true  of  the  divisor.  Thus  it  is  not 
true  in  general  that 

a  ~  (b  +  c)  =  a  -v-  b  +  a  ~  c, 
or  that  a  -f-  (b  —  c)  =  a  ■—  b  —  a  -f-  c, 

as  the  student  may  readily  satisfy  himself  in  a  variety  of  ways. 

§  27.]  As  we  have  now  completed  our  discussion  of  the 
fundamental  laws  of  ordinary  algebra,  it  may  be  well  to  insist 
once  more  upon  the  exact  position  which  the}^  hold  in  the 
science.  To  speak,  as  is  sometimes  done,  of  the  proof  of  these 
laws  in  all  their  generality  is  an  abuse  of  terms.  They  are 
simply  laid  down  as  the  canons  of  the  science.  The  best  evi- 
dence that  this  is  their  real  position  is  the  fact  that  algebras  ai'e 


20  POSITION  OF  THE  FUNDAMENTAL  LAWS  chap. 

in  use  whose  fundamental  laws  differ  from  those  of  ordinary 
algebra.  In  the  algebra  of  quaternions,  for  example,  the  law 
of  commutation  for  multiplication  and  division  does  not  hold 
generally. 

What  we  have  been  mainly  concerned  with  in  the  present 
chapter  is,  1st,  to  see  that  the  laws  of  ordinary  algebra  shall  be 
self-consistent,  and,  2nd,  to  take  care  that  the  operations  they  lead 
to  shall  contain  those  of  ordinary  arithmetic  as  particular  cases. 

In  so  far  as  the  abstract  science  of  ordinary  algebra  is  con- 
cerned, the  definitions  of  the  letters  and  symbols  used  are  simply 
the  general  laws  laid  down  for  their  use.  When  we  come  to  the 
application  of  the  formulae  of  ordinary  algebra  to  any  particular 
purpose,  such  as  the  calculation  of  areas,  for  example,  Ave  have 
in  the  first  instance  to  see  that  the  meanings  we  attach  to  the 
symbols  are  in  accordance  with  the  fundamental  laws  above 
stated.  When  this  is  established,  the  formulae  of  algebra  become 
mere  machines  for  the  saving  of  mental  labour. 

§  28.]  We  now  collect,  for  the  reader's  convenience,  the 
general  laws  of  ordinary  algebra. 

Definitions  connecting  the  Direct  and  Inverse 

Operations. 


Addition  and  subtraction- 

+  a  —  b  +  b=  +  a, 
+  a  +  b  —  b=  +  a. 


Multiplication  and  division- 

x  a  -f-  b  x  b  =  x  a, 

x.  a  *  b-i-b  -  x  a. 


For   addition   and   subtrac 
tion — 


Law  of  Association. 

For  multiplication  and  divi- 


sion— 


±(±a±b)=  ±  (  ±  a)  ±  (  ±  b), 

with  the  following  law  of  signs  :— 

The  concurrence  of  like  signs  gives  the  direct  sign  ; 
The  concurrence  of  unlike  signs  the  inverse  sign. 


SYNOPTIC  TABLE  OF  LAWS 


21 


Thus— 
+  (  +  a)  =  +  a,     +  (  -  a)  =  -  a,  \    x  (  x  a)  =  x  a,     x  ( -h  a)  =  -s-  a, 

-  (  -  a)  =  +  a,     -  (  +  a)  =  -  a.   j    -=-  ( -=-  a)  =  x  a,     -f-  (  x  a)  =  -4-  a, 

Law  of  Commutation. 


For  addition   and   subtrac- 


tion- 


sion- 


For  multiplication  and  divi- 
the  operand  always  carrying  its  own  sign  of  operation  with  it. 


±a±b=  ±b±a, 


Properties  of  0  and  1. 


0 

±5  +  0 

+  0 


+  a  —  a, 
±b-0  =  ±b, 

-0. 


1  =  x  a~-a, 
*bx  1  =  *£>-=- 1  =  *&, 

Xl=   -T-l. 


Law  of  Distribution. 
For  multiplication — 

(±  a  ±  b)  x  (±  c  ±  d)  =  +  (±  a)  x  (±  C)  +  (±  a)  x  (±  d) 
+  (±b)x(±c)  +  (±b)x(±  d), 

with  the  following  law  of  signs : — 

If  a  partial  product  has  constituents  with  like  signs,  it  must 
have  the  sign  +  ; 

If    the    constituents   have   unlike   signs,    it   must   have    the 
sign  -  . 

Thus— 

+  (  +  a)  x  (  +  c)  =  +ax  c,      +  (  +  a)  x  (  -  c)  =  -axe, 
+  (-a)x(-c)=  +  a  x  c,      +(-a)x(  +  c)=  -axe. 

Property  of  0. 

0x6  =  5x0-0. 
For  division — 

(  ±  a  ±  b)  -I-  (  ±  c)  =  +  (  ±  a)  -f  (  ±  e)  +  (  ±  6)  -*-  (  ±  c), 
with  the  following  law  of  signs  : — 


22 


EXERCISES  I 


CHAP. 


If  the  dividend  and  divisor  of  a  partial  quotient  have  like 
signs,  the  partial  quotient  must  have  the  sign  +  ; 

If  they  have  unlike  signs,  the  partial  quotient  must  have  tho 


sign  -  . 


Thus— 

+  (  +  a)  —  (  +  c)=  +  a~-c,      +(  +  a)-r-(-c)  = 

+ .(  -  a)  -7-  (  -  c)  =  +  a  +  c,      +  (  -  a)  4-  (  +  c)  = 

N.B. — The  divisor  cannot  be  distributed. 


-  a  -f-  c, 

—  a-T-c 


Property  of  0. 

0  -r-  6  =  0. 

N.B. — Nothing  is  said  regarding  &-r-0.     This  case  will  be 
discussed  later  on. 


The  reader  should  here  mark  the  exact  signification  of  the 
sign  =  as  hitherto  used.  It  means  "is  transformable  into  by 
applying  the  laws  of  algebra,  without  any  assumption  regarding 
the  operands  involved." 

Any  "  equation "  which  is  true  in  this  sense  is  called  an 
"Identical  Equation,"  or  an  "Identity";  and  must,  in  the  first 
instance  at  least,  be  carefully  distinguished  from  an  equation  the 
one  side  of  which  can  be  transformed  into  the  other  by  means  of 
the  laws  of  algebra  only  when  the  operands  involved  have  particular 
values  or  satisfy  some  particular  condition. 

Some  writers  constantly  use  the  sign  =  for  the  former  kind 
of  equation,  and  the  sign  =  for  the  latter.  There  is  much  to 
be  said  for  this  practice,  and  teachers  will  find  it  useful  with 
beginners.  We  have,  however,  for  a  variety  of  reasons,  adhered, 
in  general,  to  the  old  usage ;  and  have  only  introduced  the 
sign  =  occasionally  in  order  to  emphasise  the  distinction  in  cases 
where  confusion  might  be  feared. 

Exercises  I. 

[In  working  this  set  of  examples  the  student  is  expected  to  avoid  quoting 
derived  formulae  that  he  may  happen  to  recollect,  and  to  refer  every  step  to 
the  fundamental  principles  discussed  in  the  above  chapter.] 


i  EXERCISES  I  23 

(1.)  Point  out  in  what  sense  the  usual  arrangement  of  the  multiplication 
of  365  by  492  is  an  instance  of  the  law  of  distribution. 

(2.)  I  have  a  multiplying  machine,  but  the  most  it  can  do  at  one  time  is 
to  multiply  a  number  of  10  digits  by  another  number  of  10  digits.  Explain 
how  I  can  use  my  machine  to  multiply  13693456783231  by  46381239245932. 

(3.)  To  divide  5004  by  12  is  the  same  as  to  divide  5004  by  3,  and  then 
divide  the  quotient  thus  obtained  by  4.  Of  what  law  of  algebra  is  this  an 
instance  ? 

(4.)  If  the  remainder  on  dividing  X  by  a  be  R,  and  the  quotient  P,  and 
if  we  divide  P  by  6  and  find  a  remainder  S,  show  that  the  remainder  on 
dividing  N  by  ab  will  be  aS  +  R. 

Illustrate  with  5015+-12. 

(5.)  Show  how  to  multiply  two  numbers  of  10  digits  each  so  as  to  obtain 
merely  the  number  of  digits  in  the  product,  and  the  first  three  digits  on 
the  left  of  the  product. 

Illustrate  by  finding  the  number  of  digits,  and  the  first  three  left-hand 
digits  in  the  following  : — 

1st.  3659893456789325678  x  342973489379265  ; 
2nd.  264. 

(6.)  Express  in  the  simplest  form — 

-(-(-(-(  •   •   •  (-D  •   •   •   )))), 

1st.  Where  there  are  2«  brackets  ; 

2nd.  "Where  there  are  2?i  + 1  brackets  ;  n  being  any  whole  number  whatever. 
(7.)  Simplify  and  condense  as  much  as  possible — 

2a-  {3a-[a-(b-a)]}. 


(8.)  Simplify— 

1st. 

3  [4  -5[6-  7(8  -9.10-11)]}, 

2nd. 
(9.)  Simplify— 

*tt-t»-M-*-A-A)]}- 

l-(2-(3- 

(4-  .   .   .    (9-(10-ll))  .  .  .   ))). 

(10.)  Distribute    the 

following    products  : — 1st.     {a  +  b)  x  (a  +  b)  ; 

2nd 

(r*-6)x(a  +  6)  ;  3rd.  (3a- 66)  x  (3a +  66)  ;  4th.  (Ja-  £6)  x  (Ja  +  £6). 
(11.)  Simplify,  by  expanding  and  condensing  as  much  as  possible — 

{(m  +  l)a+(n  +  l)b}{{m-l)a  +  (n-l)b} 
+  {{m  +  l)a-(n  +  l)b}  {{m-l)a-(n-l)b}. 
(12.)  Simplify- 

K)K)+K)K> 

(13.)  Simplify— 

H)H)H)-H)B)H> 

(14.)  Expand  and  condense  as  much  as  possible — 





24  HISTORICAL  NOTE  chap,  i 

Historical  Xote. — The  separation  and  classification  of  the  fundamental  laws 
of  algebra  has  been  a  slow  process,  extending  over  more  than  2000  years.  It  is 
most  likely  that  the  first  ideas  of  algebraic  identity  were  of  geometrical  origin. 
In  the  second  book  of  Euclid's  Elements  (about  300  B.C.),  for  example,  we  have  a 
series  of  propositions  which  may  be  read  as  algebraical  identities,  the  operands 
being  lines  and  rectangles.  In  the  extant  works  of  the  great  Greek  algebraist 
Diophantos  (350  ?)  we  find  what  has  been  called  a  syncopated  algebra.  He  uses 
contractions  for  the  names  of  the  powers  of  the  variables  ;  has  a  symbol  f-  to 
denote  subtraction  ;  and  even  enunciates  the  abstract  law  for  the  multiplication 
of  positive  and  negative  numbers  ;  but  has  no  idea  of  independent  negative  quan- 
tity. The  Arabian  mathematicians,  as  regards  symbolism,  stand  on  much  the 
same  platform  ;  and  the  same  is  true  of  the  great  Italian  mathematicians  Ferro, 
Tartaglia,  Cardano,  Ferrari,  whose  time  falls  in  the  first  half  of  the  sixteenth 
century.  In  point  of  method  the  Indian  mathematicians  Aryabhatta  (476), 
Brahmagupta  (598),  Bhaskara  (1114),  stand  somewhat  higher,  but  their  works 
had  no  direct  influence  on  Western  science. 

Algebra  in  the  modern  sense  begins  to  take  shape  in  the  works  of  Regiomon- 
tanus  (1436-1476),  Rudolff  (about  1520),  Stifel  (1487-1567),  and  more  particularly 
Viete  (1540-1603)  and  Harriot  (1560-1621).  The  introduction  of  the  various 
signs  of  operation  now  in  use  may  be  dated,  with  more  or  less  certainty,  as 

follows :  -  and  apposition  to  indicate  multiplication,  as  old  as  the  use  of  the 

Arabic  numerals  in  Europe;  +  and  -,  Rudolff  1525,  and  Stifel  1544;  =, 
Recorde  1557  ;  vinculum,  Viete  1591  ;  brackets,  first  by  Girard  1629,  but  not 
in  familiar  use  till  the  eighteenth  century ;  <  > ,  Harriot's  Praxis,  published 
1631  ;    x  ,  Oughtred,  and  ^-,  Pell,  about  1631. 

It  was  not  until  the  Geometry  of  Descartes  appeared  (in  1637)  that  the  im- 
portant idea  of  using  a  single  letter  to  denote  a  quantity  which  might  be  either 
positive  or  negative  became  familiar  to  mathematicians. 

The  establishment  of  the  three  great  laws  of  operation  was  left  for  the  present 
century.  The  chief  contributors  thereto  were  Peacock,  De  Morgan,  D.  F.  Gregory, 
Hankel,  and  others,  working  professedly  at  the  philosophy  of  the  first  principles  ; 
and  Hamilton,  Grassmann,  Peirce,  and  their  followers,  who  threw  a  flood  of  light 
on  the  subject  by  conceiving  algebras  whose  laws  differ  from  those  of  ordinary 
algebra.  To  these  should  be  added  Argand,  Cauchy,  Gauss,  and  others,  who 
developed  the  theory  of  imaginaries  in  ordinary  algebra. 


CHAPTEE    II. 
Monomials — Laws  of  Indices—Degree. 

THEORY    OF    INDICES. 

§  1.]  The  product  of  a  number  of  letters,  or  it  may  be  num- 
bers, each  being  supposed  simple,  so  that  multiplication  merely 
and  neither  addition  nor  subtraction  nor  division  occurs,  is  called 
an  integral  term,  or  more  fully  a  rational  integral  monomial  (that 
is,  one-termed)  algebraical  function,  for  example,  ax3x6nxa 
xxxxxyxbxb. 

By  the  law  of  commutation  we  may  arrange  the  constituents 
of  this  monomial  in  any  order  we  please.  It  is  usual  and  con- 
venient to  arrange  and  associate  together  all  the  factors  that  are 
mere  numbers  and  all  the  factors  that  consist  of  the  same  letter ; 
thus  the  above  monomial  would  be  written 

(3  x  6)  x  (a  x  a)  x  (b  x  b)  x  (x  x  x  x  x)  x  y. 

3x6  can  of  course  be  replaced  by  18,  and  a  further  contrac- 
tion is  rendered  possible  by  the  introduction  of  indices  or  ex- 
ponents. Thus  a  x  a  is  written  a2,  and  is  read  "  a  square,"  or 
"a  to  the  second  power."  Similarly  b  x  b  is  replaced  by  b*,  and 
x  x  x  x  xhy  x3,  which  is  read  " x  cube,"  or  " x  to  the  third  power." 
We  are  thus  led  to  introduce  the  abbreviation  x11  for  x  x  x  x  x  x  .  .  . 
where  there  are  n  factors,  n  being  called  the  index  or  exponent* 
while  xn  is  called  the  nth  power  of  x,  or  x  to  the  nth.  power. 

§  2.]  It  will  be  observed  that,  in  order  that  the  above  defini- 
tion may  have  any  meaning,  the  exponent  n  must  be  a  positive 

*  In  accordance  with  this  definition  x1  of  course  means  simply  x,  and  is 
usually  so  written. 


26  RATIONAL  INTEGRAL  MONOMIAL  chap. 

integral  number.       Confining  ourselves  for  the  present  to  this 
case,  we  can  deduce  the  following  "laws  of  indices." 

I.   (a)  am  x  an  =  am+n, 

and  generally    a™  x  an  x  aP  x  .   .  .  =  am+n+p+  •  •  • 

(J3)  —  =  am~n  if  m>n, 

1 


an 


an-m 


if  m  <  n. 


II.  (am)n  =  amn  =  (ft'1)' 

III.  (a)  \ab)m  =  ambm, 

and  generally  (ahc  .  .   .  )m  =  ambmcm  .  . 


W 


¥1' 


To  prove  I.  (a),  we  have,  by  the  definition  of  an  index, 
am  x  an  =  (a  x  a  x  a  .  .   .  m  factors)  x  (a  x  a  x  a  .  .   .  n  factors), 
=  a  x  a  x  a  .   .  .  m  +  n  factors,  by  the  law  of  association, 
=  a,n+n,  by  the  definition  of  an  index. 

Having  proved  the  law  for  two  factors,  we  can  easily  extend 
it  to  the  case  of  three  or  more, 

for  am  x  an  x  ap  =  (am  x  a11)  x  ap,  by  law  of  association, 

_  am+n  x  ap^  \)y  case  already  proved, 
_  a(m+n)+p^  by  case  already  proved, 
_ am+n+p . 

and  so  on  for  any  number  of  factors. 

In  words  this  law  runs  thus :  The  product  of  any  number  of 
powers  of  one  and  the  same  letter  is  equal  to  a  power  of  that 
letter  whose  exponent  is  the  sum  of  the  exponents  of  these 
powers. 

To  prove  I.  (fi), 

am 

—  =  (a  x  a  x  .  .  ,m  factors)  -7-  (ft  x  ft  x   .  .  .  n  factors), 

by  definition  of  an  index, 


II 


LAWS  OF  INDICES  27 


I 

=  a  x  a  x  a  .  .   .  m  factors  -~  a  -f-  a  -j- .  .  .  w  divisions, 

by  law  of  association. 

Now  if  m  >  ?i  we  may  arrange  these  as  follows  : — 

am  

—  =  (a  x  a  x  .  .  .  m  —  n  factors)  x  (a  4-  a)  x  (a  -J-  a)  ...  w  factors, 

l>y  laws  of  commutation  and  association, 
=  a  x  a  x  .  .   .  m  -  «  factors,  by  the  properties  of  division, 
=  am~n. 

If  wi  <  n,  the  rearrangement  of  the  factors  may  be  effected 
thus : — 


—  =  -7- (a  y.  a  x  ...  n-  m  factors)  x  (a -f- a)  x  (a -r a)  . .  .  wi  factors 

=  -ha"-™, 
1 


,71-Ml 


It  is  important  to  notice  'that  I.  (ft)  can  be  deduced  from 
I.  (a)  without  any  further  direct  appeal  to  the  definition  of  an 
index.     Thus,  if  m  >  n,  so  that  m  -  n  is  positive, 

gm-n  x  an  _  am-n)+n    ^  J.  (a)} 


Hence 

Therefore,  by  the  definition  of  x  and  -J- : 


am"n  x  an  -4-  an  =  a'"  -f-  a". 


Again,  if  m  <  n,  so  that  n  -  m  is  positive, 

am  x  ftn-m  _  (jm+to-^  ty  J    ^ 

=  an,  by  the  laws  of  +  and  - 

Hence 

am  x  an  -  m  _j_  fln  -  m  _  a«  _l_  (fn  -  j» 

Therefore,  by  the  definition  of  x  and  ~ , 

am  =  an~an-m. 
Hence,  by  the  laws  of  x  and  -f- , 

am  -f-  an  =  an  -f-  an'm  -~  an, 
=  (an-7-an)-r-an-mt 
=  1  -r-an-m. 


28  LAWS  OF  INDICES 


CHAP. 


To  prove  II., 
(am)n  =  am  x  am  x  .  .   .  n  factors,  by  definition, 

=  (a  x  a  x  .    .    .7)i  factors)  x  (a  x  a  x  .   .    .  m  factors) 
x  .   .   .,  n  sets,  by  definition, 

ran  factors,  by  law  of  association. 


=  a  x  a  x 


=  amn,  by  definition. 

To  prove  III.  (a), 
(ab)m  =  (ab)  x  (ab)  x  .   .  .  m  factors,  by  definition, 

=  (a  x  a  x  ,   .    .  m  factors)  x  (6  x  b  x  .  .  .  m  factors), 

by  laws  of  commutation  and  association, 
=  ambm,  by  definition. 

Again,  (abc)m  =  {(ab)c}m, 

=  (ab)mcm,  by  last  case, 

=  (a™bm)c">,  by  last  case, 

=  ambmcm,  and  so  on. 
Hence  the  with  power  of  the  product  of  any  number  of  letters 
is  equal  to  the  product  of  the  wth  powers  of  these  letters. 

To  prove  III.  (ft), 

(a\m 
-A     =  (a  ~  b)  x(a~b)x.  .   .  m  factors,  by  definition, 

=  (a  x  a  x  .  .   .  m  factors)  -H  (b  x  b  x  .   .  .  m  factors), 

by  commutation  and  association, 
=  am  -^  bm, 

_  am 

In  words  :  The  mth  power  of  the  quotient  of  two  letters  is 
the  quotient  of  the  mt\\  powers  of  these  letters. 

The  second  branch  of  III.   may  be  derived  from   the   first 
without  further  use  of  the  definition  of  an  index.      Thus 

(d\  "l  /(l       \  "l 

v  x  bm  =  [b x  h)  ' by  IIL  (a)> 

=  a''\  by  definition  of  x  and  ~- . 
Hence  /a\ m 

t  1     x  b1"  +  bm  -  a11'  -J-  b"> 


that  is, 


ii  LAWS  OF  INDICES  29 

§  3.]  In  so  far  as  positive  integral  indices  are  concerned,  the 
above  laws  are  a  deduction  from  the  definition  and  from  the 
laws  of  algebra.  The  use  of  indices  is  not  confined  to  this  case, 
however,  and  the  above  are  laid  down  as  the  laws  of  indices 
generally.  The  laws  of  indices  regarded  in  this  way  become  in 
reality  part  of  the  general  laws  of  algebra,  and  might  have 
been  enumerated  in  the  Synoptic  Table  already  given.  In  this 
respect,  they  are  subject  to  the  remarks  in  chap,  i.,  §  27.  The 
question  of  the  meaning  of  fractional  and  negative  indices  is 
deferred  till  a  later  chapter,  but  the  student  will  have  no  diffi- 
culty in  working  the  exercises  given  below.  All  he  has  to  do  is 
to  use  the  above  laws  whenever  it  is  necessary,  without  regard 
to  any  restriction  on  the  value  of  the  indices. 

§  4.]  The  following  examples  are  worked  to  familiarise  the 
student  with  the  meaning  and  use  of  the  laws  of  indices.  At 
first  he  should  be  careful  to  refer  each  step  to  the  proper  law, 
and  to  see  that  he  takes  no  step  which  is  not  sanctioned  by 
some  one  of  the  laws  of  indices,  or  by  one  of  the  fundamental 
laws  of  algebra. 

Example  1. 

(a3b2c5)  x  (a5bscu)+(a4b3c15) 

=  asa5b-b*c5cu  4-  «4  4-  b3  4-  cls,  by  commutation  and  association, 

=  «!^'^"  4-  «4  4-  b3  -f-  c15,  by  law  of  indices,  I.  (a), 

=  (a3+5  4-  a*)  x  (b-+6  -f-  b3)  x  (c5+"  -=-  c15),  by  commutation  and 

association. 
=  «W-<x6W-3xcs+n-i5j  by  law  of  indices,  I.  (/3), 
=  a*bh. 

Example  2. 

(15-cVV)2  '<  (t^ttkY 

=  15V)V)V)a  x  nf£p>  b)' laws  of  indices,  III.  (a)  and  III.  (£), 

~(3x4)2(^vr  y  (a)' 

32  x  523,3,-6-10 

=  ~32 x  4--yyT'  by  l-  (a)  and  n-> 

=  3-  4-  32  x  i>-  4-  4-  x  xs  x  if  4 1/  x  z]0  4-  z™, 
=  5-~i2xxg  4-y2, 


30  ALGEBRAICAL  INTEGRALITY  AND  FRACTIONALITY        chap. 

THEORY  OF  DEGREE. 

§  5.]  The  result  of  multiplying  or  dividing  any  number  of 
letters  or  numbers  one  by  another,  addition  and  subtraction 
being  excluded,  for  example,  3  x  a  x  x  x  b  -~  c  —  y  x  d,  is  called  a 
(rational)  monomial  algebraical  function  of  the  numbers  and  letters 
involved,  or  simply  a  term.  If  the  monomial  either  does  not 
contain  or  can  be  so  reduced  as  not  to  contain  the  operation  of 
division,  it  is  said  to  be  integral;  if  it  cannot  be  reduced  so  as 
to  become  entirely  free  of  division,  it  is  said  to  be  fractional.  In 
drawing  this  distinction,  division  by  mere  numbers  is  usually 
disregarded,  and  even  division  by  certain  specified  letters  may  be 
disregarded,  as  will  be  explained  presently. 

§  6.]  The  number  of  times  that  any  particular  letter  occurs 
by  way  of  multiplication  in  an  integral  monomial  is  called  the 
degree  (or  dimension)  of  the  monomial  in  that  particular  letter ; 
and  the  degree  of  the  monomial  in  any  specified  letters  is  the 
siim  of  its  degrees  in  each  of  these  letters.  For  example,  the 
degree  of  6  x  a  x  a  x  x  x  x  x  x  x  y  x  y,  that  is,  of  6a2x3y2,  in  a  is  2, 
in  x  3,  in  y  2,  and  the  degree  in  x  and  y  is  5,  and  in  a,  x,  and  y  7. 

In  other  words,  the  degree  is  the  sum  of  the  indices  of  the 
named  letters.  The  choice  of  the  letters  which  are  to  be  taken 
into  account  in  reckoning  the  degree  is  quite  arbitrary  ;  one 
choice  being  made  for  one  purpose,  another  for  another.  When 
certain  letters  have  been  selected,  however,  for  this  purpose,  it 
is  usual  to  call  them  the  variables,  and  to  call  the  other  letters, 
including  mere  numbers,  constants.  The  monomial  is  usually 
arranged  so  that  all  the  constants  come  first  and  the  variables 
last;  thus,  x  and  y  being  the  variables,  we  write  32a2bcx3y' ;  and 
the  part  32a2bc  is  called  the  coefficient. 

In  considering  whether  a  monomial  is  integral  or  not,  division 
by  constants  is  not  taken  into  account. 

§  7.]  The  notion  of  degree  is  an  exceedingly  important  one, 
and  the  student  must  at  once  make  himself  perfectly  familiar 
with  it.  lie  will  find  as  he  goes  on  that  it  takes  to  a  large 
extent  in  algebra  the  same  place  as  numerical  magnitude  in 
arithmetic. 


IT 


NOTIONS  AND  LAWS  OF  DEGREE  31 


The  following  theorems  are  particular  cases  of  more  general 
ones  to  be  proved  by  and  by. 

The  degree  of  the  product  of  two  or  more  monomials  is  the  sum 
of  their  respective  degrees. 

If  the  quotient  of  two  monomials  be  integral,  its  degree  is  the  excess 
of  the  degree  of  the  dividend  over  that  of  the  divisor. 

For  let  A  =  cx[i/l":"ni>  .   .  . 

At  tjl    Ml'    »'      )>' 

=  cx  y  z  u'    ... 

where  c  and  c  are  the  coefficients,  x,  ij,  z,  u  .  .  .the  variables,  and 
/,  m,  v,p .  . .,  /',  m',  ri,p'  ■  ■  ■  are  of  course  positive  integral  numbers. 
Then  the  degree,  d,  of  A  is  given  by  d  =  I  +  m  +  n  +p  +  .  .  .,  and 
tbe  degree,  d',  of  A'  by  d'  =  1'  +  m'  +  n  +  p  +  .  .  . 

But       A  x  A'  =  (cxhf  nznuP  .  .  .)  x  (c'x  ym  zn up   .  .  .) 

/  a   l+V  m+»i'  n+n!    p+v' 

=  (c  x  c)x  y  z  ir  .  .  . 
the  degree  of  which  is  (I  +  V)  +  (m  +  m')  +  (w  +  n)  +  (p  +  p')  .  .  ., 
that  is,  (l  +  m  +  n+p  .  .  .)  +  (/'  +  m!  +  n'  +_//  +  .  .  . ),  that  is, 
d  +  d',  which  proves  the  first  proposition  for  two  factors.  The 
law  of  association  enables  us  at  once  to  extend  it  to  any  number 
of  factors. 

Again,  let  Q  =  A  -=-  A',  and  let  Q  be  integral  and  its  degree  8. 
Now  we  have,  by  the  definition  of  division,  Q  x  A'  =  A.  Hence, 
by  last  proposition,  the  degrees  of  A  and  A'  being  d  and  d',  as 
before,  we  have  d  =  8  +  d',  and  thence  8  =  d  -  d'. 

As  an  example,  let  A  =  G///,  A'  =  T.r7//3,  then  A  x  A'  = 
42x*y,  and  A  4-  A'  =  fc2/.  The  degree  of  A  x  A'  is  24,  that  is, 
14  +  10  ;  that  of  A-j- A'  is  4,  that  is,  14  -  10. 

The  student  will  probably  convince  himself  most  easily  of 
the  truth  of  the  two  propositions  by  considering  particular  cases 
such  as  these ;  but  he  should  study  the  general  proof  as  an 
exercise  in  abstract  reasoning  for  on  such  reasoning  he  will  have 
to  rely  more  and  more  as  he  goes  on. 

Exercises  II. 

[Wherever  it  is  possible  in  working  the  following  examples,  the  student 
should  verify  the  laws  of  degree,  §§  5-7.] 

11.)  Simplify—         57  x  124x  32-' x  (32  x  42  x  5)2 

(3  x  15  x  23)10 


32 


EXERCISES  II 


CHAP   II. 


(2. 
(3. 


(4. 

(5.: 

(6.: 
(7.: 
(8.; 

(9. 

(io.; 
(ii. 

(12. 
(13. 

(14. 
(15. 

(16.; 

(17. 


"Which  is  greater,  (22)2   or  2'-  ?     Find  the  difference  between  them, 
Simplify — 


2- 


Simplify- 


/       \a4b3x3y3J  ' 


2(22)2 
36W6W3 
81a4b3<?  * 
Express  in  its  simplest  form — 
cy    \2     /    a*Vh? 
<a3bWtf)    X  \aWc3x3y' 
Simplify—         /45«3&V\2     /2i3a4b4c4x\2 


Simplify — 
Simplify — 

Simplify — 
Simplify — 
Simplify — 


27a262c )   *\    180a2bc  J 
,„       *     x*y9     /3xV\2 


{.rhfz-j7  X  (;//l~Y)7  X  (A5/) 


S)7* 


gas/       Va;?// 

X"'J 


aj^J     x(y 


J  («p-?)«  x  (a^-ry-p  \ J 
I         (ar+»)r-«         / 

(z«-6  x  ^-c)a  x  C^) 


/r 


(a!aXic0)o-T-(jco+c)c 

Simplify—  /x^\p+*^  (xp^\v"-!<1 

Simplify — 

|  f  £*Y  x  /^' Y"  I  _i_  {(^  x  (Xm)m}  x    f^m)*  x  (jgljw^ 


Prove  that- 


{yz)^(zxYP(xy)P" 


_  {xyz)P+^-^ 


(yt~lzr-1)P{zr-'ixP-1Y{xP-lyi-lY       xPifzr 
Distribute  the  product — 


i  V       i 

aP  +  r-      a»  +  r- 


Distribute — 

If  ?n.  =  ft*,  n  =  aM,  az={mfnxY  ;  show  that  a:?/z  =  lc 


CHAPTEE    III. 

Fundamental  Formula  relating  to  Quotients  or 
Fractions,  with  Applications  to  Arithmetical 
Fractions  and  to  the  Theory  of  Numbers. 

OPERATIONS    WITH   FRACTIONS. 

§  1.]  Before  proceeding  to  cases  where  the  fundamental 
laws  are  masked  by  the  complexity  of  the  operations  involved, 
we  shall  consider  in  the  light  of  our  newly-acquired  principles 
a  few  cases  with  most  of  which  the  student  is  already  partly 
familiar.  He  is  not  in  this  chapter  to  look  so  much  for  new 
results  as  to  exercise  his  reasoning  faculty  in  tracing  the  opera- 
tion of  the  fundamental  laws  of  algebra.  It  will  be  well,  how- 
ever, that  he  should  bear  in  mind  that  the  letters  used  in  the 
following  formula?  may  denote  any  operands  subject  to  the  laws 
of  algebra ;  for  example,  mere  numbers  integral  or  fractional,  single 
letters,  or  any  functions  of  such,  however  complex. 

§  2.]  Bearing  in  mind  the  equivalence  of  the  notations  -, 

ajb,  and  a  —■  b,  the  laws  of  association  and  commutation  for 
multiplication  and  division,  and  finally  the  definition  of  a 
quotient,  we  have 

yb  =  O) -*- (Pb)  ^xa-rii-rJ, 

=  a  -7-  b  -r-p  x  p, 
—  a-r-b; 

that  is,  ^-7  =  7- 

pb     b 

VOL.  I  D 


34  ALGEBRAICAL  ADDITION  OF  FRACTIONS  chap. 

Kead  forwards  and  backwards  this  equation  gives  us  the 
important  proposition  that  ice  may  divide  or  multiply  the  numerator 
and  denominator  of  a  fraction  by  the  same  quantity  without  altering 
its  value. 

§  3.]  Using  the  principle  just  established,  and  the  law  of 
distribution  for  quotients,  we  have 


a 
±- 

6 

1 

±qa 
qb 

pb 

qb' 

±  qa 

±pb 

qb 
that  is,  To  add  or  subtract  two  fractions,  transform  each  by  multiplying 
numerator  and  denominator  so  that  both  shall  have  the  same  denomi- 
nator,  add   or  subtract  the  numerators,   and   write  underneath  the 
common  denominator. 

The  rule  obviously  admits  of  extension  to  the  addition  in 
the  algebraic  sense  (that  is,  either  addition  or  subtraction)  of  any 
number  of  fractions  whatever. 

Take,  for  example,  the  case  of  three  : — 

b     d    f         bdf     bdf     bdf    Yb    ' 

±  adf  ±  cbf  ±  ebd  ,     ,        ,  , .  ^  . . 

= J    ,,; ,  by  law  ol  distribution. 

bdf 

The  following  case  shows  a  modification  of  the  process,  which 
often  leads  to  a  simpler  final  result.  Suppose  b  -  Ic,  q-  lr;  then, 
taking  a  particular  case  out  of  the  four  possible  arrangements 
of  sign, 

a    p     a     p 
b     q     Ic     lr' 
_  ar     pc 
Icr     Ire 
_  ar  -  pc 
Icr 

Here  the  common  denominator  Icr  is  simpler  than  bq,  which  is 
Ihr. 

The  same  result  would  of  course  be  arrived  at  by  following 


in  MULTIPLICATION  AND  DIVISION  OF  FRACTIONS  35 

the  process  given  above,  and  simplifying  the  resulting  fraction 
at  the  end  of  the  operation,  thus  : — 

a     p     air  -  pic  . 

(ar  -  pc)l 
=      far     ' 

by  using  the  law  of  distribution  in  the  numerator,  and  the  laws 
of  association  and  commutation  in  the  denominator  ; 

ar  -cp 

§  4.]  The  following  are  merely  particular  cases  of  the  laws 
of  association  and  commutation  for  multiplication  and  division : — 


©«(a)->+«>"<H-A 


=  a  -J-  b  x  c  -f-  d, 
=  a  x  c-7-b  —el, 
=  (ac)  -t-  (bd), 

ac 
=  bd' 

or,  in  words,   To  multiply  two  fractions,  multiply  their  numerators 
together  for   the  numerator,  and  the  denominators   together  for  the 
denominator  of  the  product. 
Again, 

©  +  ©-<«■»> +<•+<>. 

=  a  x  d  -7-  b  -f-  c, 
-  (ad)  -7-  (be), 
ad 

=  Tc' 


also 

\C 


■© 


by  last  case.     In  words :  To  divide  one  fraction  by  another,  invert 
the  latter  and  then  midtiply. 

§  5.]  In  last  paragraph,    and   in   §   2   above,    we    have   for 


36  EXERCISES  III  CHAr. 

simplicity  omitted  all  explicit  reference  to  sign.  In  reality  we 
have  not  thereby  restricted  the  generality  of  our  conclusions,  for 
by  the  principle  of  substitution  (which  is  merely  another  name 
for  the  generality  of  algebraic  formulae)  we  may  suppose  the  p, 
for  example,  of  §  2  to  stand  for  -  w,  say,  and  we  then  have 

(  -  o>)a     a 
C^jb  =  b  ' 

that  is,  taking  account  of  the  law  of  signs, 

—  wa     a 

~-ub  =  b' 
and  so  on. 


Exercises  III. 
(1.)  Express  in  its  simplest  form — 


K»             V2 

x — y    y-x 

(2.)  Express  in  its 

simplest  form — 

a          h 

a-b    b-a 

(3.)  Simplify- 

P  +  Q    P-Q 

P-Q    P  +  Q' 

where 

T>  =  x  +  y,     Q=x~y, 

(4.)  Simplify— 

1     afl-tf 

x  +  y 

1+ 

x  +  y 

(5.)  Simplify— 

1       1       1 
ab    ac     be 

a?-(b-c? 

(6.)  Simplify- 


(  h"    \      I  h*    \ 

\       a  +  bj      \       a-b) 


(7.)  Simplify—  _1_     _J_        1x 

,8.)Siml,%-   fr^+iy^hly 

(9.)  Simplify—  fa    b\/f0    &\ 

\b    a)  •  \b*    a2)' 


Ill  ARITHMETICAL  INTEGRALITY  AND  DIVISIBILITY  37 

(10.)  Simplify—  a{a  -b)-  b{n  +  b) 


a+b     a- b 

(11.)  Simplify—  1-x  1+a: 

l+x  +  x2     1-x  +  x"' 

(12.)  Simplify-  x 

1+a.  {x  +  lf-x* 
1  x2  +  x+l  ' 

1  +  x 
(13.)  Simplify—  2_/l     1\ 

a-  +  b2     ab\a     b) 

w+  (k ' 

(14.)  Show  that  &_      (a2 -a2)2      (a2-^)2 

a2Ja+a2(aa-ft2)    W-ft2") 

is  independent  of  x. 

(15.)  Simplify—  «■ 


6--° 


'  -J 


(16.)  Simplify—  1 

1 


a -2b 


a -2b- 


a -2b 
(17.)  Simplify-  a  +  b 

1 

a  +  b  + 


1 
a  ~b  + 


a  +  b 


APPLICATIONS    TO   THE   THEORY    OF   NUMBERS. 

§  6.]  In  the  applications  that  follow,  the  student  should  look 
somewhat  closely  at  the  meanings  of  some  of  the  terms  employed. 
This  is  necessary  because,  unfortunately,  some  of  these  terms, 
such  as  integral,  factor,  divisible,  &c,  are  used  in  algebra  generally 
in  a  sense  very  different  from  that  which  they  bear  in  ordinary 
arithmetic  and  in  the  theory  of  numbers. 

An  integer,  unless  otherwise  stated,  means  for  the  present  a 
positive  (or  negative)  integral  number.  The  ordinary  notion  of 
greater  and  less  in  connection  with  such  numbers,  irrespective  of 
their  sign,  is  assumed  as  too  simple  to  need  definition.*     When 

*  This  is  a  very  different  thing  from   the  algebraical  notion  of  greater 
and   less.       See  chap.   xiii. ,    §    1.       It    may  not  he  superfluous  to   explain 


38  PRIME  AND  COMPOSITE  INTEGERS  chap. 

an  integer  a  can  be  produced  by  multiplying  together  two  others, 
b  and  c,  b  and  c  are  called  factors  of  a,  and  a  is  said  to  be  exactly 
divisible  by  b  and  by  c,  and  to  be  a  multiple  of  b  or  of  c.  Since 
the  product  of  two  integers,  neither  of  which  is  unity,  is  an 
integer  greater  than  either  of  the  two,  it  is  clear  that  no  integer 
is  exactly  divisible  by  another  greater  than  itself. 

It  is  also  obvious  that  every  integer  (other  than  unity)  has 
at  least  two  divisors,  namely,  unity  and  itself;  if  it  has  more,  it 
is  called  a  composite  integer,  if  it  has  no  more,  a  prime  integer. 
For  example,  1,  2,  3,  5,  7,  11,  13,  .  .  .  are  all  prime  integers, 
whereas  4,  6,  8,  9,  10,  12,  14  are  composite. 

If  an  integer  divide  each  of  two  others  it  is  said  to  be  a 
common  factor  or  common  measure  of  the  two.  If  two  integers 
have  no  common  measure  except  unity  they  are  said  to  be  prime 
to  each  other.  It  is  of  course  obvious  that  two  integers,  such  as 
6  and  35,  which  are  prime  to  each  other  need  not  be  themselves 
prime  integers.  We  may  also  speak  of  a  common  measure  of  more 
than  two  integers,  and  of  a  group  of  more  than  two  integers 
that  are  prime  to  each  other,  meaning,  in  the  latter  case,  a  set 
of  integers  no  two  of  which  have  any  common  measure. 

§  7.]  If  we  consider  any  composite  integer  N,  and  take  in 
order  all  the  primes  that  are  less  than  it,  any  one  of  these  either 
will  or  will  not  divide  N.  Let  the  first  that  divides  N  be  a, 
then  N  =  «N],  where  N,  is  an  integer  ;  if  N,  be  also  divisible  by  a 
we  have  Ni  =  «N2,  and  N  =  fl(</N2)  =  a2N2 ;  and  clearly,  finally, 
say  N  =  a*Na,  where  Na  is  either  1  or  no  longer  divisible  by  a. 
Na  (if  not  =1)  is  now  either  prime  or  is  divisible  by  some 
prime  >a  and  <Na,  and,  a  fortiori,  <N,  say  b ;  we  should  on 
the  last  supposition  have  N«  =  Z^N^,  where  N/3<Na,  and  so  on. 
The  process  clearly  must  end  with  unity,  so  that  we  get 

N  =  aW 

where  a,  b,  .  .   .  are  primes,  and  a,  /3,   .  .   .  positive  integers.    It 

here  the  use  of  the  inequality  symbols  4=,  >,  <,  >,  <f ;  they  mean 
respectively  "is  not  equal  to,"  "is  greater  than,"  "is  less  than,"  "is  not 
greater  than,"  "is  not  less  than."  Iustead  of  > ,  <t  we  may  use  <,>  which 
may  b;  read  "is  equal  to  or  less  than,"  "  is  equal  to  or  greater  than." 


in  ARITHMETICAL  G.C.M.  39 

is  to  be  observed  that  a",  b  ,  .  .  .  are  powers  of  primes,  and 
therefore,  as  we  shall  prove  presently,  prime  to  each  other.  It 
is  therefore  always  possible  to  resolve  every  composite  integer  into  factors 
that  are  powers  of  primes ;  and  we  shall  presently  show  that  this 
resolution  can  be  effected  in  one  way  only. 

§  8.]  If  a  be  divisible  by  c,  then  any  integral  multiple  of  a,  say  ma, 
is  divisible  by  c;  and,  if  a  and  b  be  each  divisible  by  c,  then  the  algebraic 
sum  of  any  integral  multiples  of  a  and  b,  say  ma  +  nb,  is  divisible  by  c. 

For  by  hypothesis  a  -  ac  and  b  =  fir,  where  a  and  ft  are  in- 
tegers, hence  ma  =  viae  -  (ma)c,  where  ma  is  an  integer,  that  is,  ma 
is  divisible  by  c.  And  ma  +  nb  =  mac  +  nfic  =  {ma  +  nfi)c,  where 
ma  +  n(3  is  an  integer,  that  is,  ma  +  nb  is  divisible  by  c.  The 
student  should  observe  that,  by  virtue  of  the  extension  of  the 
notion  of  divisibility  by  the  introduction  of  negative  integers, 
any  of  the  numbers  in  the  above  proposition  may  be  negative. 

§  9.]  From  the  last  article  we  can  deduce  a  proposition  which 
at  once  gives  us  the  means  of  finding  the  greatest  common  measure 
of  two  integers,  or  of  proving  that  they  are  prime  to  each  other. 

If  a  =pb  +  c,  where  a,  b,  c,  p  are  all  integers,  then  the  G.C.M.  of 
a  and  b  is  the  G.C.M.  of  b  and  c. 

To  prove  this  it  is  necessary  and  it  is  sufficient  to  show — 
1st,  that  every  divisor  of  b  and  c  divides  a  and  b,  and,  2nd,  that 
every  divisor  of  a  and  b  divides  b  and  r. 

Since  a  =  pb  +  c,  it  follows  from  §  8  that  every  divisor  of  b 
and  c  divides  a,  that  is,  every  divisor  of  b  and  c  divides  a  and  b. 

Again,  since  a  =  pb  +  c,  it  follows  that  c  —  a  —pb  •  hence,  again 
by  §  8,  every  divisor  of  a  and  b  divides  c,  that  is,  every  divisor 
of  a  and  b  divides  b  and  c.  Thus  the  two  parts  of  the  proof  are 
furnished. 

Let  now  a  and  //  be  two  numbers  whose  G.C.M.  is  required ; 
they  will  not  be  equal,  for  then  the  G.C.M.  would  be  either  of 
them.  Let  b  denote  the  less,  and  divide  a  by  b,  the  quotient 
beings  and  the  remainder  c,  where  of  course  c<b*  Next  divide 
b  by  c,  the  quotient  being  q,  the  remainder  d ;  then  divide  c  by 
d,  the  quotient  being  r,  the  remainder  e,  and  so  on. 

*  For  a  formal  definition  of  the  remainder  see  §  11. 


40  ARITHMETICAL  G.C.M. 


CHAP. 


Since  a  >  b,  b>c,  c>  d,  d>e,  &c,  it  is  clear  that  the  re- 
mainders must  diminish  down  to  zero.  We  thus  have  the 
following  series  of  equations  : — 

a  =pb  +  c 
b  =  qc  +  d 
c  =  rd  +  e 


I  =  vm  +  n 
m  =  ten. 
Hence  the  G.C.M.  of  a  and  b  is  the  same  as  that  of  b  and  c,  which 
is  the  same  as  that  of  c  and  d,  that  is,  the  same  as  that  of  d  and  e, 
and  finally  the  same  as  that  of  m  and  n.  But,  since  m  =  wn,  the 
G.C.M.  of  m  and  n  is  n,  for  n  is  the  greatest  divisor  of  n  itself. 
Hence  the  G.C.M.  of  a  and  b  is  the  divisor  corresponding  to  the 
remainder  0  in  the  chain  of  divisions  above  indicated. 

If  n  he  different  from  unity,  then  a  and  b  have  a  G.C.M.  in 
the  ordinary  sense. 

If  n  he  equal  to  unity,  then  they  have  no  common  divisor 
except  unity,  that  is,  they  are  prime  to  each  other. 

§  10.]  It  should  be  noticed  that  the  essence  of  the  foregoing 
process  for  finding  the  G.C.M.  of  two  integers  is  the  substitution 
for  the  original  pair,  of  successive  pairs  of  continually  decreasing 
integers,  each  pair  having  the  same  G.C.M.  All  that  is  necessary 
is  that  j),  q,  r,  .  .  .  be  integers,  and  that  a,  b,  c,  d,  e,  ...  be  in 
decreasing  order  of  magnitude. 

The  process  might  therefore  be  varied  in  several  ways. 
Taking  advantage  of  the  use  of  negative  integers,  we  may  some- 
times abbreviate  it  by  taking  a  negative  instead  of  a  positive 
remainder,  when  the  former  happens  to  be  numerically  less  than 
the  latter. 

For  example,  take  «  =  4323,  &  =  1595, 
we  might  take  4323  =  2  x  1595  +  1133 

or  4323  =  3x1595-462; 

the  latter  is  to  be  preferred,  because  462  is  less  than  1133.  In  practice  the 
negative  sign  of  462  may  be  neglected  in  the  rest  of  the  operation,  which  may 
be  arranged  as  follows,  for  the  sake  of  comparison  with  the  ordinary  process 
already  familiar  to  the  student : — 


Ill 


riUME  DIVISORS 


41 


1595)4323(3 
4785 


462)1595(3 
1386 


209)462(2 
418 

44)209(5 
220 

11)44(4 
44  • 

G.C.M.=11. 

By  means  of  the  process  for  finding  the  (x.C.M.  we  may  prove 
the  following  proposition,  of  whose  truth  the  student  is  in  all 
probability  already  convinced  by  experience  : — 

If  a  and  b  be  prime  to  each  other,  and  h  any  integer,  then  any 
common  factor  of  ah  and  b  must  divide  h  exactly. 

For,  since  a  and  b  are  prime,  we  have  by  §  9, 


a=pb  +  c 
b  =  qc  +  d 
c  =  rd  +  e 

I  -  vm  +  1 


>(1).    Hence  < 


r  ah- pbh  +  ch 
bh  =  qch  +  dh 
eh  =  rdh  +  eh 

Ih  =  vmh  +  h 


•(2). 


Now,  since  any  common  factor  of  ah  and  b  is  a  common 
factor  of  ah  and  bh,  it  follows  from  the  first  of  equations  (2)  that 
such  a  common  factor  divides  ch  exactly,  and  by  the  second  that 
it  also  divides  dh  exactly,  and  so  on ;  and,  finally,  by  the  last  of 
equations  (2),  that  any  common  factor  of  ah  and  b  divides  h 
exactly. 

In  particular,  since  b  is  a  factor  of  itself,  we  have 

Cor  1.  If  b  divide  ah  exactly  and  be  prime  to  a,  it  must  divide  h 
exactly. 

Cor.  2.  If  a'  be  prime  to  a  and  to  b  and  to  c,  &c,  then  it  is 
prime  to  their  product  abc  .  . . 

For,  if  a'  had  any  factor  in  common  with  abc  .  .  .,  that  is, 
with  a(bc .  .  .),  then,  since  a'  is  prime  to  a,  that  factor,  by  the 
proposition  above,  must  divide  be .  .  .  exactly  ;  hence,   since  a' 


42 


REMAINDER  AND  RESIDUE 


CHAP. 


is  prime  to  b,  the  supposed  factor  must  divide  c .  .  .  exactly,  and 
so  on.     But  in  this  way  we  exhaust  all  the  factors  of  the  pro 
duct,  since  all  are  prime  to  a'.     Hence  no  such  factor  can  exist, 
that  is,  a'  is  prime  to  abc  . .  . 

An  easy  extension  of  this  is  the  following  : — 
Cor.  3.  If  all  the  integers  a',  b',  c', .   .  .  be  prime  to  all  the  integers 
a,b,c,.  .  .,  then  the  product  a'b'c' .  .  .  is  prime  to  the  product  abc  .  .  . 
A  particular  case  of  which  is 

Cor.  4.  If  a'  be  prime  to  a  (and  in  particular  if  both  be  primes), 
then  any  integral  power  of  a'  is  prime  to  any  integral  power  of  a. 

§  11. J  It  is  obvious  that,  if  a  and  b  be  two  integers,  we  can 
in  an  infinite  number  of  ways  put  a  into  the  form  of  qb  +  r,  where 
q  and  r  are  integers,  for,  if  we  take  q  any  integer  whatever,  and 
find  r  so  that  a  -  qb  =  r,  then  a  =  qb  +  r. 

There  are  two  important  special  cases,  those,  namely,  where 
we  restrict  r  to  be  numerically  less  than  b,  and  either  (1)  positive 
or  (2)  negative.  In  each  of  these  cases  the  resolution  of  a  is 
always  possible  in  one  way  only.  For,  in  case  1,  if  qb  be  the 
greatest  multiple  of  b  which  does  not  exceed  a,  then  a  -  qb  —  r, 
where  r <b  ;  hence  a  =  qb  +  r ;  and  in  case  2,  if  qb  be  the  least 
multiple  of  b  which  is  not  less  than  a,  then  a  -  q'b-  -  r',  where 
r'  <  b.  Also  the  resolution  is  unique  ;  for  suppose,  in  case  1,  that 
there  were  two  resolutions,  another  being  a  =  \b  +  p,  say;  then 
qb  +  r  =  xb  +  p,  therefore  r  —  p  -  (x  -  q)b ;  hence  r  -  p  is  divisible 
by  b ;  but,  r  and  p  being  each  positive,  and  each  numerically  <b, 
r  -  p  is  numerically  less  than  b,  and  therefore  cannot  be  divisible 
by  b.  Hence  there  cannot  be  more  than  one  resolution  of  the 
form  1.     Similar  reasoning  applies  to  case  2. 

r  and  r'  are  often  spoken  of  as  the  least  positive  and  negative 
remainders  of  a  with  respect  to  b.  When  the  remainder  is  spoken 
of  without  qualification  the  least  positive  remainder  is  meant.  If 
a  more  general  term  is  required,  corresponding  to  the  removal 
of  the  restriction  r  numerically  <  b,  the  word  residue  is  used. 

It  is  obvious,  from  the  definitions  laid  down  in  §  6,  that  a  is 
or  is  not  exactly  divisible  by  b  according  as  the  least  remainder  of  a 
with  respect  to  b  does  or  does  not  vanish. 


ill  ARITHMETICAL  FRACTIONALITV  43 

The  student  will  also  prove  without  difficulty  that  if  the  re- 
mainders of  a  and  of  a'  with  respect  to  b  be  the  same,  then  a  -  a'  is 
divisible  by  b  ;  and  conversely. 

Cor.  If  q  be  a  fixed  integer  (sometimes  spoken  of  as  a  modulus), 
then  every  other  integer  can  be  expressed  in  one  or  other  of  the  forms 

bq,  bq+  1,  bq+  2,    .    .    .,  bq  +  (q-  I), 

where  b  is  an  integer. 

For,  as  we  have  seen,  we  can  put  any  given  integer  a  into 
the  form  bq  +  r,  where  r~^>q,  and  here  r  must  have  one  of  the 
values  0,  1,  2,   .   .   .,  (q-  \). 

Example.     Take  q  =  5,  then 

0  =  0.5,       1  =  0.5  +  1,       2  =  0.5  +  2,  3  =  0.5  +  3,       4  =  0.5+4; 

5  =  1.5,       6  =  1.5  +  1,       7  =  1.5  +  2,  8  =  1.5  +  3,       9  =  1.5  +  4; 

10  =  2.5,     11  =  2.5  +  1,     12  =  2.5  +  2,  13  =  2.5  +  3,     14  =  2.5  +  4; 
and  so  on. 

It  should  be  noticed  that,  since  bq  +  (q  -  1)  =  (b  +  \)q-  1, 
bq  +  (q  -  2)  =  (b  +  l)q  -  2,  &c,  we  might  put  every  integer  into 
one  or  other  of  the  forms 

bq,  bq±  1,  bq±  2,  .   .   .  ,  &c. 
For  example, 

8  =  2.5-2,     9  =  2.5-1,     10  =  2.5,     11  =  2.5  +  1,     12  =  2.5  +  2. 

The  above  principle,  which  may  be  called  the  periodicity  of 
the  integral  numbers  with  respect  to  a  given  modulus,  is  of  great 
importance  in  the  theory  of  numbers. 

§  12.]  When  the  quotient  a/b  cannot  be  expressed  as  an 
integer,  it  is  said  to  be  fractional  or  essentially  fractional ;  if  a>  b, 
a/b  is  called  in  this  case  an  improper  fraction;  if  a<b,  a  proper 
fraction. 

Hence  no  true  fraction,  proper  or  improper,  can  be  equal  to  an 
integer. 

Every  improper  fraction  a/b  can  be  expressed  in  the  form  q  +  rjb, 
where  q  is  an  integer  and  rjb  a  proper  fraction.  For,  if  r  be  the 
least  positive  remainder  when  a  is  divided  by  b,  a  =  qb  +  r,  and 
ajb  =  (qb  +  r)jb  =  q  +  rjb,  where  q  and  r  are  integers  and  r  <  b. 

If  two  improper  fractions  ajb  and  a'jb'  be  equal,  their  integral 
parts  and  their  proper  fractional  parts  must  be  equal  separately.     For, 


44  THEOREM  REGARDING  G.C.M.  CHAP. 

if    this  were    not    so,   we   should    have,   say   ajb  =  q  +  rjb,   a'jb' 
=  q1  +  r'/b',   and   q  +  rjb  =  q'  +  r'jb' ;    whence   q  -  q  =  r'/b'  -  r/b  = 
(r'6  -  rb')/bb'.     Now  r'b  <  b'b  and  rb'  <  bb',  hence  r'b  -  rb'  is  numeric- 
ally <  66'.     In  other  words,  the  integer  q  -  q'  is  equal  to  a  proper 
fraction,  which  is  impossible. 

§  13.]  We  can  now  prove  that  an  integer  can  be  resolved  info 
factors  which  are  powers  of  primes  in  one  way  only. 

For,  since  the  factors  in  question  are  powers  of  primes,  the}'' 
are  prime  to  each  other.  Let,  if  possible,  there  be  two  such 
resolutions,  namely,  a'b'c  . .  .  and  a"b"c"  ...  of  the  same  integer  N. 
Since  a'b'c!  .  . .  =  a"h"c"  . .  .  ,  therefore  a'b'c' ...  is  exactly  divisible 
by  a".  Now,  since  a"  is  a  power  of  a  prime,  it  will  be  prime  to 
all  the  factors  a',  b',  c,  .  .  .  save  one,  say  a',  which  is  a  power  of 
the  same  prime.  Moreover,  such  a  factor  as  a'  (that  is,  a  power 
of  the  prime  of  which  a"  is  a  power)  must  occur,  for,  if  it  did 
not,  then  all  the  factors  of  a'b'c' .  .  .  would  be  prime  to  a",  and 
a"  could  not  be  a  factor  of  N.  It  follows,  then,  that  a'  must  be 
divisible  by  a". 

Again,  since  a"b"c"  .  .  .=  a'b'c'  .  . .,  therefore  a"b"c" ...  is  divis- 
ible by  a',  and  it  follows  as  before  that  a"  is  divisible  by  a'. 

But,  if  two  integers  be  such  that  each  is  divisible  by  the 
other,  they  must  be  equal  (§  6) ;  hence  a"  =  a'. 

Proceeding  in  this  way  we  can  show  that  each  factor  in  the 
one  resolution  occurs  in  the  other. 

§  14.]  Every  remainder  in  the  ordinary  jwocess  for  finding  the 

G.C.M.  of  two  positive  integers  a  and  b  can  be  expressed  in  the  form 

±  (Art  -  Bo),  where  A  and  B  are  positive  integral  numbers.     The 

upper  sign  being  used  for  the  1st,  3rd,  5th,  &c,  and  the  lower  for  the 

2nd,  4th,  &c,  remainders. 

For,  by  the  equations  in  §  9,  we  have  successively — 

(i); 
(2); 


(3); 


c  = 

+ 

{a-pb} 

d  = 

h- 

-  qc  =  b  - 

q(a  -  pb), 

- 

- 

[qa  -  (1 

+  pq)b] 

e  = 

c  - 

-  rd, 

= 

{a 

-  pb]  +  ? 

•{qa-(\  + 

pq)b], 

= 

+ 

{(l+gr) 

a  -  (j)  +  r 

+pqr)b] 

in  THEOREMS  REGARDING  G.C.M.  45 

and  so  on.  It  is  evident  in  fact  that,  if  the  theorem  holds  for 
any  two  successive  remainders,  it  must  hold  for  the  next.  Now 
equations  (1),  (2),  and  (3)  prove  it  for  the  first  three  remainders; 
hence  it  holds  for  the  fourth  ;  hence  for  the  fifth  ;  and  so  on. 

In  the  chapter  on  Continued  Fractions,  a  convenient  process 
will  be  given  for  calculating  the  successive  values  of  A  and  B 
for  each  remainder.  In  the  meantime  it  is  sufficient  to  have 
established  the  existence  of  these  numbers,  and  to  have  seen  a 
straightforward  way  of  finding  them. 

Cor.  1.  Since  g,  the  G.C.M.  of  a  and  b,  is  the  last  remainder,  we 
can  always  express  g  in  the  farm — 

g  =  ±  (Aa  -  Bb)  (4), 

where  A  and  B  are  positive  integers. 

Cor.  2.  If  a  be  prime  to  b,  g  =  1 ;  hence,  If  a  and  b  be  two 
integers  prime  to  each  otlier,  two  positive  integers,  A  and  B,  can 
always  be  found  such  that — 

Aa  -  Bb  =  ±1  (5). 

X.B. — It  is  clear  that  A  must  be  prime  to  B.  For,  since  ajg 
and  b/g  are  integers,  I  and  m  say,  we  have,  from  (4), 

1  =  ±(Al-  Bm)  ; 
hence,  if  A  and  B  had  any  common  factor  it  would  divide  1  (by 
§  8  above). 

Cor.  3.  From  Cor.  1  and  §  8  we  see  that  every  common  factor 
of  a  and  b  must  be  a  factor  in  their  G.C.M. 

A  result  which  may  be  proved  otherwise,  and  will  probably 
be  considered  obvious. 

Cor.  4.  Hence,  To  find  the  G.C.M.  of  more  tlian  two  integers  a,  b, 
c,  d,  .  .  .,  we  must  first  find  g  the  G.C.M.  of  a  and  6,  then  g  the 
G.C.M.  of  g  and  c,  then  g"  the  G.C.M.  of  g  and  d,  and  so  on,  the  last 
G.C.M.  found  being  the  G.C.M.  of  all  the  given  integers. 

For  every  common  factor  of  a,  b,  c  must  be  a  factor  in  a  and 
b,  that  is,  must  be  a  factor  in  g ;  hence,  to  find  the  greatest  com- 
mon factor  iii  a,  b,  c,  we  must  find  the  greatest  common  factor 
in  g  and  c ;  and  so  on. 

From  Cor.  2  we  can  also  obtain  an  elegant  proof  of  the 
conclusions  in  the  latter  part  of  §  10. 


46  EXAMPLES  chap. 

Example  1.  To  express  the  G.C.M.  of  565  and  60  in  the  form  A565  -  B60. 
We  have  565  =  9x60  +  25,  60  =  2x25  +  10,  25  =  2x10  +  5,  10  =  2x5. 
Hence  the  G.C.M.  is  5,  and  we  have  successively 

25  =  565-9x60; 
10=60-2(565-9x60} 

=  -  {2x565-19x60}  ; 
5  =  25-2x10 
=  565  -  9  x  60  +  2  { 2  x  565  -  19  x  60 } 
=  5x565-47x60. 

Example  2.  Show  that  two  integers  A  and  B  can  be  found  so  that 

5A-7B  =  1. 

We  have  7  =  1x5  +  2,  5  =  2x2  +  1;  whence  2  =  7-5,  1  =  5-2(7-5) 
=  3x5-2x7. 

Hence  A  =  3,  B  =  2  are  integers  satisfying  the  requirements  of  the 
question. 

Example  3.  If  a,  b,  c,  d,  .  .  .  be  a  series  of  integers  whose  G.C.M.  is  g, 
show  that  integers  (positive  or  negative)  A,  B,  C,  D,  .  .  .  can  be  found 
such  that 

g  =  Aa  +  Bb  +  Cc  +  T)d  +  .  .  . 

(Gauss's  Disquisitioncs  Arithmetics,  Th.  40). 

Find  A,  B,  C,  D,  when  a=36,  6  =  24,  c=18,  ^=30. 

This  result  may  be  easily  arrived  at  by  repeated  application  of  corollaries 
1  and  4  of  this  article. 

Example  4.  The  proper  fraction  p/ab,  where  a  is  prime  to  b,  can  be  de- 
composed, and  that  in  one  way  only,  into  the  form 

a'    V     , 

-  +  -T-1; 
a      b 

where  a'  and  b'  are  both  positive,  a' <a,  V <b,  and  k  is  the  integral  jiart  of 
a'/a  +  b'/b  ;  that  is  to  say,  0  or  1,  according  to  circumstances. 

Illustrate  with  6/35. 

Since  a  is  prime  to  b,  by  Cor.  2  above, 

Aa -B6=±l  ; 
multiplying  this  equation  by  ^j/ab,  we  have 

±ph~=JLh  »)■ 

o    '   a      ab  ' 

If  the  upper  sign  has  to  be  taken,  resolve  pk  and^B  as  follows  (§  11) : — 

pA  =  lb  +  b'  (b'  positive  <b), 

pB—ma~a'  (a'  positive  <a). 

Then  (1)  becomes 

V      7  «'     b'  ' 

£-=:l-m+-+T  (2. 

ab  a      b 

Now,  since  p/ab  is  a  proper  fraction,  the  integral  part  on  the  right-hand  side 
of  (2)  must  vanish  ;  hence,  since  the  integral  part  of  a'/a  +  b'/b  cannot  exceed 
1 ,  we  must  have  I  -  m  =  0,  or  I  -  m  —  -  1 . 


in  NUMBER  OF  PRIMES  INFINITE  47 

If  the  lower  sign  has  to  be  taken  in  (1),  we  have  merely  to  take  the 
resolutions 

pA  =  lb-b'  (b'  positive  <b), 
pB  =  7)ia  +  a'  (a'  positive  <a), 

and  then  proceed  as  before.     We  leave  the  proof  that  the  resolution  is  unique 
to  the  ingenuity  of  the  reader. 

Illustration.  35  =  5  x  7. 

Now  3x5-2x7  =  1     (see  Example  2  above) ; 

whence  —  =  —(3  x  5  -  2  x  7), 

.55     .35 

_18    12 

~7       5' 
2x7+4     3x5-3 

~       7  5       * 

4  3 

-2+r-8+|, 

■W-j. 

5     7 

N.B. — If  negative  numerators  are  allowed,  it  is  obvious  that  p/ab  can 
always  be  decomposed  (sometimes  in  more  ways  than  one)  into  an  algebraic 
sum  of  two  fractions  a'/a  aud  b'/b,  where  a'  and  V  are  numerically  less  than 
a  and  b  respectively.     For  example,  we  have  6/35  =  3/5  -  3/7  =  4/7  -  2/5. 

Example  5.  If  the  n  integers  a,  b,  c,  d.  .  .  .  be  prime  to  each  other,  the 
proper  fraction  pjabed  .  .  .  may  be  resolved  in  one  way  only  into  the  form 

a     8    y     8  , 

abed 

where  a,  8,  y,  5,  .  .    .  are  all  positive,  a<a,  8<b,  y<c,  $<d,  .  .       and  £ 
has,  according  to  circumstances,  one  or  other  of  the  integral  values 

0,  1,  2,  .  .   „»-l. 

(Gauss's  Disquisitiones  Arithmetical,  Th.  310). 

This  may  be  established  by  means  of  Example  3. 

Example  6.  Work  out  the  resolution  of  Example  5  for  the  fraction 
10729/17017. 

§  15.]  We  conclude  this  chapter  with  a  proposition  which  is 
as  old  as  Euclid  (ix.  20),*  namely — 

The  number  of  prime  integers  is  infinite. 

For  let  a,  /3,  y,  .  .  .,  k  he  any  series  of  prime  integers  what- 
soever, then  we  can  show  that  an  infinity  of  primes  can  be 
derived  from  these. 

In  fact    the  integer  a/3y .  .  .  k  +  1   is  obviously  not  exactly 

*  Most  of  the  foregoing  propositions  regarding  integral  numbers  were 
known  to  the  old  Greek  geometers. 


48  EXERCISES  IV 


CHAP.    Ill 


divisible  by  any  one  of  the  primes  a,  (3,  y,  .  .  .,  k.  It  must 
therefore  either  be  itself  a  prime  different  from  any  one  of  the 
series  a,  (3,  y,  .  .  .,  k,  or  it  must  be  a  power  of  a  prime  or  a 
composite  integer  divisible  by  some  prime  not  occurring  among 
a,  (3,  y,  .  .  .,  k.  We  thus  derive  from  a,  /?,  y,  ,  .  .,  k  at  least 
one  more  prime,  say  A.  Then  from  a,  (3,  y,  .  .  .,  k,  A  we  can  in 
like  manner  derive  at  least  one  more  prime,  \x ;  and  so  on  ad 
infinitum.'" 

Exercises  IV. 

(1.)  If  the  two  fractions  A/B,  a/b  be  equal,  and  the  latter  be  at  its  lowest 
terms,  prove  that  A  =  /xa,  B  =  /Jib,  where  /x  is  an  integer. 

(2.)  Prove  that  the  sum  or  difference  of  two  odd  numbers  is  always  even  ; 
the  sum  or  difference  of  an  odd  and  an  even  number  always  odd  ;  the  product 
of  any  number  of  odd  numbers  always  odd  ;  the  quotient  of  one  odd  number 
by  another  always  odd,  if  it  be  integral. 

(3. )  If  a  be  prime  to  b,  then — 

1st.  (a  +  b)n  and  (a-b)m  have  at  most  the  G.C.M.  2m  ; 
2nd.  am  +  bm  and  am-bm  have  at  most  the  G.C.M.  2  ; 
3rd.  a  +  b  and  a2  +  b"  -  ab  have  at  most  the  G.  C.  M.  3. 

(4.)  The  difference  of  the  squares  of  any  two  odd  numbers  is  exactly 
divisible  by  8. 

(5.)  The  snm  of  the  squares  of  three  consecutive  odd  numbers  increased 
by  1  is  a  multiple  of  12. 

(6. )  If  each  of  two  fractions  be  at  its  lowest  terms,  neither  their  sum  nor 
their  difference  can  be  an  integer  unless  the  denominators  be  equal. 

(7.)  Resolve  45738  and  297675  into  their  prime  factors. 

(8.)  Find  the  G.C.M.  of  54643  and  91319,  using  negative  remainders 
whenever  it  is  of  advantage  to  do  so. 

(9.)  Trove  that  the  L. CM.  of  two  integers  is  the  quotient  of  their  product 
by  the  G.C.M. 

(10.)  If  pi,  g-i,  g3  be  the  G.C.M.  's,  h,  h,  h  the  L.C.M.'s,  of  b  and  c,  c  and 

a,  a  and  b  respectively,  G  the  G.C.M.,  and  L  the  L.C.M.,  of  the  three  a,  b, 

c,  show  that 

,  ,     T      abcG 
1st.   L  = ; 


2nd.  I;=  jm  , 
I*      V   \9tfsgi 


a). 

(11.)  When  x  is  divided  by  y,  the  quotient  is  u  and  the  remainder  u  ; 
show  that,  when  x  and  uy  are  divided  by  v,  the  remainders  are  the  same,  and 
the  quotients  differ  by  unity. 

*  On  this  subject  see  Sylvester,  Nature,  vol.  xxxviii.  (1888),  p.  261. 


CHAPTER    IV. 

Distribution  of  Products— Multiplication  of  Rational 
Integral  Functions— Resulting  General  Principles. 

GENERALISED    LAW    OF   DISTRIBUTION. 

§  1.]  We  proceed  now  to  develop  some  of  the  more  important 
consequences  of  the  law  of  distribution.  This  law  has  already  been 
stated  in  the  most  general  manner  for  the  case  of  two  factors, 
eacb  of  which  is  the  sum  of  a  series  of  terms :  namely,  we  multiply 
every  term  of  the  one  factor  by  every  term  of  the  other,  and  set 
down  all  the  partial  products  thus  obtained  each  with  the  sign 
before  it  which  results  from  a  certain  law  of  signs. 

Let  us  now  consider  the  case  of  three  factors,  say 
(a  +  b  +  c  +  .  .  .)(a'  +  b'  +  c'  +  .   .   .)(a"  +  b"  +  c"  +  .  .   .). 
First  of  all,  we  may  replace  the  first  two  factors  by  the  process 
just  described,  namely,  we  may  write 

(aa'  +  ah'  +  ac'  +  .  .  .  +  ba'  +  bb'  +  bc'  +  .  .  .)  (a"  +  b"  +  c"  +  .  .   .). 
Then  we  may  repeat  the  process,  and  write 

aa'a"  +  aa'b"  +  aa'c"  +  .  .  . 
+  ab'a"  +  ab'b"  +  ab'c"  +  .  .  . 
+  ac'a"  +  ac'b"  +  ac'c"  +  .  .   . 


+  baa"  +  ba'b"  +  ba'c"  +  .  .  .  &c, 
where  the  original  product  is  finally  replaced  by  a  sum  of 
partial  products,  each  of  three  letters.  AYe  have  simplified  the 
matter  by  writing  +  before  every  term  in  the  original  factors,  but 
the  proper  application  of  the  law  of  signs  at  each  step  will  pre- 
sent no  difficulty  to  the  student. 

VOL.  I  E 


50  GENERALISED  LAW  OF  DISTRIBUTION  chap. 

The  important  thing  to  remark  is  that  Ave  might  evidently 
have  arrived  at  the  final  result  by  the  following  process,  which 
is  really  an  extension  of  the  original  rule  for  two  factors : — 

Form  all  possible  partial  products  by  taking  a  term  from  each 
factor  (never  more  than  one  from  each) ;  determine  the  sign  by  the  law 
of  signs  (that  is,  if  there  be  an  odd  number  of  negative  terms  in  the 
partial  product,  take  the  sign  -  ;  if  an  even  number  of  such  vr  none, 
take  the  sign  +  ).     Set  down  all  the  partial  products  thus  obtained. 

Cor.  The  number  of  terms  resulting  from  the  distribution  of  a 
product  of  brackets  which  contain  I,  m,  n,  .  .  .  terms  respectively  is 
I  x  m  x  n  x  .  .  .  For,  taking  the  first  two  brackets  alone,  since 
each  term  of  the  first  goes  with  each  term  of  the  second,  the 
whole  number  of  terms  arising  from  the  distribution  of  these  is 
I  x  m.  Next,  multiplying  by  the  third  bracket,  each  of  the  I  x  m 
terms  already  obtained  must  be  taken  with  each  of  the  n  terms 
of  the  third.  We  thus  get  (I  x  m)  x  n,  that  is,  I  x  m  x  n  terms. 
By  proceeding  in  this  way  Ave  establish  the  general  result. 

It  should  be  noted,  hoAvever,  that  all  the  terms  are  supposed 
to  be  unlike,  and  that  no  condensation  or  reduction,  owing  to  like 
terms  occurring  more  than  once,  or  to  terms  destroying  each 
other,  is  supposed  to  be  made.  Cases  occur  in  §  2  below  in 
which  the  number  of  terms  is  reduced  in  this  Avay. 

If  the  student  have  the  least  difficulty  in  folloAving  the  aboATe, 
he  "will  quickly  get  over  it  by  working  out  for  himself  the  results 
stated  below,  first  by  successive  distribution,  and  then  by  apply- 
ing the  law  just  given. 

(a  +  b)(c  +  d)(e+f) 

—  ace  +  acf+  ade  +  adf+  bee  +  bcf+  bde  +  bdf 

(2x2x2  =  8  terms)  , 
(a-b)(c-d)(e-f) 

—  ace  -  acf-  ade  +  adf-  bee  +  br/+  bde  -  bdf ; 
(a-b)(c-d)(e+f+g) 

—  ace  +  acf  +  acg  -  ade  -  adf  -  adg  -  bee  -  bef  -  beg  +  bde  +  bdf+  bdg 

(2x2x3  =  12  terms). 

§  2.]  It  Avas  proved  above  that  in  the  most  general  case  of 
distribution  the  number  of  resulting  terms  is  the  product  of  the 
numbers  of  terms  in  the  different  factors  of  the  product.  An 
examination  of    the  particular  cases  where   reductions  may  be 


iv  ENUMERATION  OF  PRODUCTS  51 

afterwards   effected   will   lead   us    to   some   important    practical 
results,  and  will  also  bring  to  notice  certain  important  principles. 

Consider  the  product  (a  +  b)  (a  +  b).  By  the  general  rule  the 
distribution  will  give  2x2  =  4  terms.  We  observe,  however, 
that  only  two  letters,  a  and  6,  occur  in  the  product,  and  that 
only  three  really  distinct  products  of  two  factors,  namely,  a  x  a, 
a  x  b,  b  x  b,  that  is,  a3,  ab,  b3,  can  be  formed  with  these  ;  hence 
among  the  four  terms  one  at  least  must  occur,  more  than  once. 
In  fact,  the  term  a  x  b  (or  b  x  a)  occurs  twice,  and  the  result  of 
the  distribution  is,  after  collection, 

(a  +  b)(a  +  b)  =  a2  +  2ab  +  b\ 
This  may  of  course  be  written 

(a  +  b)2  =  a2  +  2ab  +  b2  (1). 

Similarly  (a  -  bf  =  a2  -  2ab  +  b2  (2). 

In  the  case       (a  +  b)  (a  —  b)  =  a  -  b2  (3), 

the  term  ab  occurs  twice,  once  with  the  +  and  again  with  the  - 
sign,  so  that  these  two  terms  destroy  each  other  when  the  final 
result  is  reduced. 

Before  proceeding  to  another  example,  let  us  write  down  all 
the  possible  products  of  three  factors  that  can  be  made  with  two 
letters,  a  and  b.     These  are  a3,  a2b,  ab2,  b3,  four  in  all. 

Hence  in  the  distribution  of  (a  +  b)3,  that  is,  of  (a  +  b)  (a  +  b) 
(a  +  b),  which  by  the  general  rule  would  give  2x2x2  =  8  terms, 
only  four  really  distinct  terms  can  occur.  Let  us  see  what  terms 
recur,  and  how  often  they  do  so.  a3  and  b3  evidently  occur  each 
only  once,  because  to  get  three  a's,  or  three  b's,  one  must  be 
taken  from  each  bracket,  and  this  can  be  done  in  one  way  only. 
a"b  may  be  got  by  taking  b  from  the  first  bracket  and  a  from 
each  of  the  others,  or  by  taking  the  b  from  the  second,  or  from 
the  third,  in  all  three  ways ;  and  the  same  holds  for  ab3.  Thus 
the  result  is 

(a  +  b)3  =  a3  +  3a2b  +  3ab2  +  b3  (4). 

In  a  similar  way  the  student  may  establish  for  himself  that 
(a  -  b)3  =  a3  -  Za2b  +  3ab2  -  b3  (5), 

(a  ±  by  =  a*  ±  ia3b  +  6a3b2  ±  lab3  +  b*  (6), 


52  COUNTING  OF  RECURRENCES  chap. 

and,  remembering  that  the  possible  binary  products  of  three 
letters,  a,  b,  c,  are  a2,  b2,  c2,  be,  ca,  ab,  six  in  number,  that — 

(a  +  b  +  c)*=  a2  +  b2  +  c2  +  2bc  +  2ca  +  2ab  (7), 

(a  +  b-  c)2  =  a2  +  b2  +  c2-2bc-2ca  +  2ab  (8), 

&c. 
The  ternary  products  of  three  letters,  a,  b,  c,  are  a3,  a2b,  a2c, 
ab3,  ac2,  abc,  b3,  b2c,  be2,  c3.  The  enumeration  is  made  more  certain 
and  systematic  by  first  taking  those  in  which  a  occurs  thrice, 
then  those  in  which  it  occurs  twice,  then  those  in  which  it  occurs 
once,  and,  lastly,  those  in  which  it  does  not  occur  at  all.* 

Bearing  this  in  mind,  the  student,  by  following  the  method 
we  are  illustrating,  Avill  easily  show  that 

(a  +  b  +  c)3  =  (a  +  b  +  c)  (a  +  b  +  c)  (a  +  b  +  e), 

=  a3+b3  +  c3  +  3b2c  +  Uc2  +  3c2a  +  3ca2 

+  3a%  +  3ab2  +  6abc  (9), 

from  which  again  he  may  derive,  by  substituting  (see  chap,  i., 
§  24)  -  c  for  c  on  both  sides,  the  expansion  of  (a  +  b  -  c)3,  and  so 
on.  He  should  not  neglect  to  verify  these  results  by  successive 
distributions,  thus  : — 

(a  +  b  +  c)3  =  (a  +  b  +  cf(a  +  b  +  c) 

=  (a2  +  b2  +  c2  +  2bc  +  2ca  +  2ab)  (a  +  b  +  c\ 
=  a3  +  ab2  +  ac2  +  2abc  +  2ca2  +  2a2b 
+  a%  +  b3+  be2  +  2b2c  +  2abc  +  2ab2 
+  ca2  +  b2c  +  c3  +  2bc2  +  2c2a  +  2abc 
=  &c. 

It  is  by  such  means  that  he  must  convince  himself  of  the 
coherency  of  algebraical  processes,  and  gain  for  himself  taste  and 
skill  in  the  choice  of  his  methods. 

*  There  is  another  way  of  classifying  the  products  of  a  given  degree  which 
is  even  more  important  and  which  the  student  should  notice,  namely,  according 
to  type.  All  the  terms  that  can  be  derived  from  one  another  by  interchanges 
among  the  variables  are  said  to  be  of  the  same  type.  For  example,  consider 
the  ternary  products  of  a,  b,  c.  From  a3  we  derive,  by  interchange  of  b  and  a,  b3 ; 
from  this  again,  by  interchange  of  b  and  c,  <?  :  no  more  can  be  got  in  this  way, 
so  that  a3,  b3,  c3  form  one  ternary  type  ;  b"c,  be",  ca,  car,  a"b,  ab",  form  another 
ternary  type  ;  and  abc  a  third.  Thus  the  ternary  products  of  three  variables 
fall  into  three  types. 


IV  S  AND  li  NOTATIONS  53 

Let  us  consider  one  more  case,  namely,  (b  +  c)  (c  +  a)  (a  +  b). 
Here  even  all  the  ten  permissible  ternary  products  of  a,  b,  c  cannot 
occur,  for  a3,  ba,  c3  are  excluded  by  the  nature  of  the  case,  since 
a  occurs  in  only  two  of  the  brackets,  and  the  same  is  true  of  b 
and  c.  In  fact,  by  the  process  of  enumeration  and  counting  of 
recurrences,  we  get 

(b  +  c)(c  +  a)  (a  +  b)  =  be  +  b2c  +  ca2  +  c2a  +  ab2  +  a2b  +  2abc  (10). 

In  the  product  (b  -  c)  (c  -  a)  (a  -  b)  the  term  abc  occurs  twice 
with  opposite  signs,  and  there  is  a  further  reduction,  namely, 

(b  -  c)  (c  -  a)  (a  -  b)  =  be2  -  b2c  +  ca2  -  c2a  +  ab2  -  a'b  (11). 

2  Notation. — Instead  of  writing  out  at  length  the  sum  of  all  the  terms  of 
the  same  type,  say  bc  +  ca  +  ab,  the  abbreviation  Hbc  is  often  used  ;  that  is  to 
say,  we  write  only  one  of  the  terms  in  question,  and  prefix  the  Greek  letter 
2,  which  stands  for  "sum,"  or,  more  fully,  "sum  of  all  terms  of  the  same 
type  as."  The  exact  meaning  of  2  depends  on  the  number  of  variables  that 
are  in  question.  For  example,  if  there  be  only  two  variables,  a  and  b,  then 
"Lab  means  simply  ab  ;  if  there  be  four  variables,  a,  b,  c,  d,  then  Hab  means 
ab  +  ac  +  ad  +  bc  +  bd  +  cd.  Again,  if  there  be  two  variables,  a,  b,  2«26  means 
a?b  +  ab~;  if  there  be  three,  a,  b,  e,  1a?b  means  a2b  +  ab2  +  a*c  +  ac2  +  b2c  +  bc*. 
Usually  the  context  shows  how  many  variables  are  understood  ;  but,  if  this 
is  not  so,  it  may  be  indicated  either  by  writing  the  variables  under  the  2, 
thus  2a6,  or  otherwise. 

abed 

This  notation  is  much  used  in  the  higher  mathematics,  and  will  be  found 
very  useful  in  saving  labour  even  in  elementary  work.  For  example,  the 
results  (4),  (9),  and  (10)  above  may  be  written— 

{a  +  b)3  =  Zas  +  3?,a-b; 
(a  +  b  +  c)3  =  2<t3  +  32a26  +  6abc  ; 
(b  +  c)  (c  +  a)  (a  +  b)  =  ~2,a-b  +  2abc. 
By  means  of  the  ideas  explained  in  the  present  article  the  reader  should 
find  no  difficulty  in  establishing  the  following,  which  are  generalisations  of 
(1)  and  (9)  :— 

(a  +  b  +  c  +  d+   .  .   .  )2  =  2a2  +  22«&  (12), 

(a  +  b  +  c  +  d+   .  .  .  )3  =  2«3  +  32«2&  +  62aZ>c  (13), 

the  number  of  variables  being  any  whatever. 

IT  Notation. — There  is  another  abbreviative  notation,  closely  allied  to  the 
one  we  have  just  been  explaining,  which  is  sometimes  useful,  and  which  often 
appears  in  Continental  works.  If  we  have  a  product  of  terms  or  functions  of 
a  given  set  of  variables,  which  are  all  different,  but  of  the  same  type  (that  is, 
derivable  from  each  other  by  interchanges,  see  p.  52),  this  is  contracted  by 
writing  only  one  of  the  terms  or  functions,  and  prefixing  the  Greek  letter  II, 
which  stands  for  "product  of  all  of  the  same  type  as."  Thus,  in  the  case  of 
three  variables,  a,  b,  c, 


54 


PRINCIPLE  OF  SUBSTITUTION 


CHAP. 


lla-b  means  a"b  x  air  x  arc  x  ac2  x  b'c  x  be" ; 
H(b  +  c)  means  (b  +  c)  {c  +  a)  (a  +  b) ; 
rifb  +  c\  (  b  +  c  \  (  c  +  a  \  (  a  +  b 

u{W+r?)  means  [FT?)  [*  +  *)  {*+-& 
and  so  on. 

"We  might,  for  example,  write  (10)  above — 

nib  +  c)  =  Zb2e  +  2abc. 
§  3.]  Hitherto  we  have  considered  merely  factors  made  up  of 
letters  preceded  by  the  signs  +  and  -  .  The  case  where  they  are 
affected  by  numerical  coefficients  is  of  course  at  once  provided 
for  by  the  principle  of  association.  Or,  what  comes  to  the  same 
thing,  cases  in  which  numerical  coefficients  occur  can  be  derived 
by  substitution  from  such  as  we  have  already  considered.  For 
example — 

(3a  +  2b)3  =  {(3a)  +  (2b)}3 

=  (3a)3  +  3(3a)2(2b)  +  3(3a)(2b)2  +  (2b)3, 
whence,  by  rules  already  established  for  monomials, 

=  27  a3  +  54a2b  +  36ab2  +  8b3. 
(a-2b  +  5c)2  =  {(a)  +  (-2b)  +  (5c)}2 

=  (af  +  (  -  2b)2  +  (5c)2  +  2(  -  2b) (5c)  +  2(5c)(a)  +  2(a) (  -  2b) 
=  a2  +  ib2  +  25c2  -  205c  +  lOca  -  iab. 

The  student  will  observe  that  in  the  final  result  the  general 
form  by  means  of  which  this  result  was  obtained  has  been  lost, 
so  far  at  least  as  the  numerical  coefficients  are  concerned. 

§  4.]   It   is  very  important  to  notice  that  the  principle  of 
substitution  may  also  be  used  to  deduce  results  for  trinomials 
from  results  already  obtained  for  binomials.    Thus  from  (a  +  b)3  = 
a3  +  3a2b  +  3ab2  +  b3,  replacing  b  throughout  by  b  +  c,  we  have 
{a  +  (b  +  c)}3  =  a3+  3a\b  +  c)  +  3a(b  +  cf  +  (b  +  c)3 
=  a3  +  3a2b  +  3a2c 

+  3a(b2  +  2bc  +  c2) 
+  b3+  3b2c  +  3bc2  +  c3 ; 
whence      (a  +  b  +  c)3  =  a3  +  b3  +  c3  +  3b2c  +  3bc2  +  3c2a  +  3ca2 

+  3a2b  +  3ab2  +  Qabc. 
By  association  of  parts  of  the  factors,  and  by  partial  distri- 
bution in  the  earlier  parts  of  a  reduction,  labour  may  often  be 
saved  and  elegance  attained. 


iv  SUMS  OF  COEFFICIENTS  DO 

For  example — 

{a  +  b  +  c  -  d)  (a  -  b  +  c  +  d) 

=  {(a+e)  +  (6  -  d)}  {(a  +  c)  -  (b  -  d)) ; 
=  (a  +  c)2-(b-dy2, 

by  formula  (3)  above  ; 
=  (a2  +  2ac  +  c2)  -  (bn-  -  2bd  +  cP)  ; 
=a?-P+(*-cP+2ac+2bd. 
Again, 

(a  +  b  +  c)  (b  +  c  -  a)  (c  +  a  -  b)  (a  +  b  -  c) 

=  {(b  +  c)  +  a}{(b  +  c)-a}{a-{b-c)}{a  +  (b-c)}; 
=  {(b+c)*-a?}{a?-(b-c)*\, 

by  a  double  application  of  formula  (3) ; 
=  Ji2  +  26c  +  c"  -  a-}  {a-  -  b2  +  2bc  -  c2} ; 
=  {2bc  +  {b"-  +  c"  -  a-)}  {2bc  -  (b2  +  c2  -  a")} ; 
=  {2bcf-{b2  +  c--a2)\ 

by  formula  (3); 
=  46V  -  (64  +  c '  +  a4  +  262c2  -  2c V  -  2a262) ; 
=  262c2  +  2c2a2  +  2a262  -  a*  -  ¥  -  c\ 
a  result  which  the  student  will  meet  with  again. 

§  5.]  There  is  an  important  general  theorem  which  follows 
so  readily  from  the  results  established  in  §§  1  and  2  that  we  may 
give  it  here.  If  all  the  terms  in  all  the  factors  of  a  product  be 
simple  letters  unaccompanied  by  numerical  coefficients  and  all  affected 
with  the  positive  sign,  then  the  sum  of  the  coefficients  in  the  distributed 
value  of  the  product  will  be  I  x  m  x  n  x  .  .  .,  where  I,  m,  n,  .  .  .  are 
the  numbers  of  the  terms  in  the  respective  factors. 

This  follows  at  once  from  the  consideration  that  no  terms 
can  be  lost  since  all  are  positive,  and  that  the  numerical  co- 
efficient of  any  term  in  the  distribution  is  simply  the  number  of 
times  that  that  term  occurs. 

Thus  in  formula?  (4),  (G),  and  (10)  in  §  2  above  we  have 

1+3  +  3  +  1  =2x2x2, 

1+4  +  6  +  4  +  1         =2x2x2x2, 
1  +  1  +  1  +  1  +  1  +  1  +  2  =  2x2x2, 

&c. 
In  formulae  (8)  and  (11)  of  §  2,  and  in  the  formula?  of  §  3, 
the   theorem  does   not  hold  on   account   of  the   appearance   of 
negative  signs  and  numerical  coefficients. 

The  following  more  general  theorem,  which  includes  the  one 
just  stated  as  a  particular  case,  will,  however,  always  apply : — 
The   algebraic  sum  of  the  coefficients   in   the   expansion  of  any 


56 


EXERCISES  V 


CHAP. 


product  may  be  obtained  from  the  product  itself  by  replacing  each  of 
the  variables  by  1  throughout  all  the  factors. 

Thus,  in  the  case  of 

(a  +  b  -  c)2  =  a2  +  b2  +  c2  -  2bc  -  2ca  +  2ab, 
we  have         (1  +  1  -  l)2  =  1  =  1  +  1  +  1  -  2  -  2  +  2. 

The  general  proof  of  the  theorem  consists  merely  in  this — 
that  any  algebraical  identity  is  established  for  all  values  of  its 
variables  :  so  that  we  may  give  each  of  the  variables  the  value  1. 
When  this  is  done,  the  expanded  side  reduces  simply  to  the 
algebraic  sum  of  its  coefficients. 

Exercises  V. 
(1.)  How   many   terms   are   there   in   the   distributed   product  (a^+a^) 
(h  +  b2  +  b3)  (Cl  +  0.,  +  %  +  c4)  (ih  +  d.2  +  d3  +  d4  +  d5)  ? 

Distribute,  condense,  and  arrange  the  following  : — 
(2.)  (x+y){x-y)(a?-y*)(a?+y*)*. 
(3.)  (x^  +  ,f){xi-f-)(xi  +  yi). 
(4.)  {x  +  y)\x-yf. 
(5.)  (x  +  2y)\x-2y)\ 

(6.)  (b  +  c){c  +  a){a  +  b)(b-e)(c-a)(a-b). 
(7.)  (x-  +  x  +  l)3. 
(8.)  (3a  +  26-l)3. 

(9.)   (x*+x  +  l  +  -  +  K 
\  X     x- 

(10.)  (a  +  b  +  cy,  and  {a-b-c)\ 

(11.)  Write  down  all  the  quaternary  products  of  the  three  letters  x,  y,  z ; 
point  out  how  many  diiferent  types  they  fall  into,  and  how  many  products 
there  are  of  each  type. 

(12.)  Do  the  same  thing  for  the  ternary  products  of  the  four  letters  a,  b,  c,  d. 

(13.)  Find  the  sum  of  the  coefficients  in  the  expansion  of  (2a  +  3b  +  Ac)3. 

Distribute  and  condense  the  following,  arranging  terms  of  the  same  type 
together  : — 

x     .     y  z    \  f   x         y 


(H.)     ~  +  -^- 


o - c    c- a     a- b 


b+c     c+a 


a  +  bj 


(15.)  [x  +  y  +  z)--x{y  +  z-x)-y(z  +  x-y)-z(x  +  y-z). 

(16. )  {b-c) {b  +  c- a)  +  {c- a)  (c  +  a -b)  +  {a-  b)(a  +  b-c). 

(17.)  (b  +  c)(y  +  z)  +  (c  +  a)(z  +  x)  +  (a  +  b)(x  +  y)-(a  +  b  +  c)(x  +  y  +  z). 

(18.)  2u(b  +  c-a)m(b+c-a).* 


*  "Wherever  in  this  set  of  exercises  the  abbreviative  symbols  S  and  IT  are 
used,  it  is  understood  that  three  letters  only  are  involved.  The  student  who 
finds  difficulty  with  the  latter  part  of  this  set  of  exercises,  should  postpone 
them  until  he  has  read  the  rest  of  this  chapter. 


IV 


EXERCISES  V  57 


Show  that 

(19.)  (x  +  yy  =  2(.r-  +  y")  (X  + y)2  -  (.'."  -  y- )-. 
(20.) 
ai(x  _  l)i  _  4a3b(x  -  a)(x  -  b)3  +  6a"b"{x  -  a)-(x  -  b)-  -  ial?{x  -  af{x-  b)  +  b*{x-a)* 
=  (a*  -  ia3b  +  6a"b-  -  iab3  +  6*)a^. 
(21.)  (x-  -  ay")  (.,■>"-  -  ay'-)  =  {xx'±ayy'f  -  a{xy,±yxf  ; 
(a-2 - ay-f  =  (x3  +  Zaxtff  - a[Zxhj  +  ay3)' ; 
(x~  -  By2  -  C;2  +  BCu-)  (x'2  -  By'2  -  Cz'2  +  BGu'-) 
=  {xx'  +  Byy'±C(zz'  +  Bmi')\2-B{a'y'  +  x'y±C(uz'  +  u'z)}2 

-Q{xz'  -Byu'±{zx'  -Buy')\2  +  BC{yz'  -xu'±{%ix' -zy'))2. 

Lagranrjc. 

The  theorems  (21.)  are  of  great  importance  in  the  theory  of  numbers  ;  they 
show  that  the  products  and  powers  of  numbers  having  a  certain  form  are 
numbers  of  the  same  form.  They  are  generalisations  of  the  formula;  numbered 
V.  in  the  table  at  the  end  of  this  chapter. 

Distribute,  condense,  and  arrange — 

(22.)  2a26c-II(6  +  c). 

(23.)  2a(2a2  +  26c)  +  2r/2a2  -  2(6  +  cf. 

(24. )  (6  -  e)  (6  +  cf  +  (c  -  a)  (c  +  a)3  +  {a-b)  (a  +  bf. 

(25.)  Distribute 

{{a  +  b)x*-abxy  +  {a-b)y2){{a-b)x2  +  abxy  +  (a  +  b)y2}; 

and  arrange  the  result  in  the  form 

Ax*  +  Bx?y  +  Cx2y2  +  Dxy3  +  Ey*. 

Show  that 

(26. )  { 3? -y3  +  Bxy(2x  +  y)}3+  { y3-x3  +  3xy(2y  +  x)}3 

=27xy{x  +  y)  (x2  +  xy  +  y1)3. 

(27.)  Z{2(x2  +  xy  +  y2)(x2  +  xz  +  z2)-(y2  +  yz  +  z2)2}=Z{Zyz}2. 

(28.)  i|2a2(6  +  c)2  +  2a6c2a}  =  {26c}2. 

(29.)  2(a-6)(a-c)={2a2-26c}. 

.      (3«6c  -  263  -  a2d)2  +  4(ac  -  b2)3 _  (Mtb  -  2c3  -  d2a)2  +  i(db  -  c2)3 
(30.) ^  -_  d.2 


general  theory  of  integral  functions. 

§  6.]  As  we  have  now  made  a  beginning  of  the  investigation 
of  the  properties  of  rational  integral  algebraical  functions,  it  will 
be  well  to  define  precisely  what  is  meant  by  this  term. 

We  have  already  (chap,  ii.,  §  5)  defined  a  rational  integral 
algebraical  term  as  the  product  of  a  number  of  positive  integral 
powers  of  various  letters,  x,  y,  z,  .  .  .,  called  the  variables,  multi- 
plied by  a  coefficient,  which  may  be  a  positive  or  negative  number, 
or  a  mere  letter  or  function  of  a  letter  or  letters,  but  must  not 
contain  or  depend  upon  the  variables. 


58  GENERAL  NOTIONS  REGARDING  chap. 

A  rational  integral  algebraical  function  is  the  algebraical  sum  of 
a  series  of  rational  integral  algebraical  terms.  Thus,  if  x,  y,  z,  ...  be 
the  variables,  /,  m,  n,  .  .  .,  /',  m',  n',  .  .  .,  I",  m",  n",  .  .  .  positive  in- 
tegral numbers,  and  C,  C,  C",  .  .  .  coefficients  as  above  defined, 
then  the  type  of  such  a  function  as  we  have  defined  is 

Cxlymzn  •  ■•  +  Casty*'*1' . . .  +  C"xl"ym"zn" ...+  &c. 
For  shortness,  we  shall,  when  no  ambiguity  is  to  be  feared,  speak 
of  it  merely  as  an  "  integral  function." 

To  fix  the  notion,  we  give  a  few  special  examples.  Thus 
(a)  dx3  +  dxy  +  2y2  is  an  integral  function  of  x  and  y  ; 
(/3)  ax2  +  bxy  +  cy-,  a,  b,  c  being  independent  of  x  and  y,  is  an  integral 

function  of  x  and  y  ; 
(7)  3X3  -  2.t2  +  3x  + 1  is  an  integral  function  of  x  alone  ; 

OS       If   -  % 

{5)  -  +  T  +  -  -1  is  an  integral  function,  if  x,  y,  z  be  regarded  as  the 

a     b     c  ° 

variables  ;  but  is  not  an  integral  function  if  the  variables  be 
taken  to  be  x,  y,  z,  a,  b,  c,  or  a,  b,  c  alone. 

Each  term  has  a  "degree,"  according  to  the  definition  of 
chap,  ii.,  §  6,  which  is  in  fact  the  sum  of  the  indices  of  the  vari- 
ables. The  decrees  of  the  various  terms  will  not  in  general  be 
alike  ;  but  the  degree  of  an  integral  function  is  defined  to  be  the 
degree  of  the  term  of  highest  degree  that  occurs  in  it. 

For  example,  the  degree  of  (a)  above  in  x  and  y  is  the  3rd,  of  (/3)  the 
2nd  in  x  and  y  and  the  1st  in  a,  b,  c,  of  (7)  in  x  the  3rd,  of  (5)  in  x,  y,  z  the  1st. 

§  7.]  From  what  has  already  been  shown  in  this  chapter  it 
appears  that,  in  the  result  of  the  distribution  of  a  product  of  any 
number  of  integral  functions,  each  term  arises  as  the  product  of 
a  number  of  integral  terms,  and  is  therefore  itself  integral. 
Moreover,  by  chap,  ii.,  §  7,  the  degree  of  each  such  term  is  the 
sum  of  the  degrees  of  the  terms  from  which  it  arises.  Hence 
the  following  general  propositions  : — 

The  product  of  any  number  of  integral  functions  is  an  integral 
function. 

The  highest  *  term  in  the  distributed  product  is  the  product  of  the 

*  By  "  highest  term  "  is  meant  term  of  highest  degree,  by  "  lowest  term  " 
term  of  lowest  degree.  If  there  be  a  term  which  does  not  contain  the  vari- 
ables at  all,  its  degree  is  said  to  be  zero,  and  it  of  course  would  be  the  lowest 
term  in  an  integral  function,  for  example,  +1  in  (7)  above. 


IV 


INTEGRAL  FUNCTIONS  59 


highest  terms  of  the  several  factors,  and  the  lowest  term  is  the  product 
of  their  lowest  terms. 

The  degree  of  the  product  of  a  number  of  integral  functions  is  the 
sum  of  tlie  degrees  of  the  several  factors. 

Every  identity  already  given  in  this  chapter,  and  all  those 
that  follow,  will  afford  the  student  the  means  of  verifying  these 
propositions  in  particular  cases.     It  is  therefore  needless  to  do, 
more  than  call  his  attention  to  their  importance.     They  form,  it 
may  he  said,  the  corner-stones  of  the  theory  of  algebraic  forms. 

INTEGRAL   FUNCTIONS    OF    ONE    VARIABLE. 

§  8.]  The  simplest  case  of  an  integral  function  is  that  where 
there  is  only  one  variable  x,  As  this  case  is  of  great  importance, 
we  shall  consider  it  at  some  length.     The  general  type  is 

2Wn+Pn-iXn~1  +  .  .  .  +pvr.+p0, 
where  p0,  plf  .  .  .,  pn  are  the  various  coefficients  and  n  is  a  posi- 
tive integral  number,  which,  being  the  index  of  the  highest  term, 
is  the  degree  of  the  function.  The  function  has  in  general  n  +  1 
terms,  but  of  course  some  of  these  may  be  wanting,  or,  which 
amounts  to  the  same  thing,  one  or  more  of  the  letters p0,pu  .  .  .,pn 
may  have  zero  value. 

§  9.]  When  products  of  integral  functions  of  one  variable 
have  to  be  distributed,  it  is  usually  required  at  the  same  time  to 
arrange  the  result  according  to  powers  of  as,  as  in  the  tj-pical 
form  above  indicated.  We  proceed  to  give  various  instances  of 
this  process,  using  in  the  first  place  the  method  described  in 
the  earlier  part  of  this  chapter.  The  student  should  exercise 
himself  by  obtaining  the  same  results  by  successive  distribution 
or  otherwise. 

In  the  case  of  two  factors  (x  +  a)  (x  +  b),  we  see  at  once  that 
the  highest  term  is  x2,  and  the  lowest  ab.  A  term  in  x  will  be 
obtained  in  two  ways,  namely,  ax  and  bx ;  hence 

(x  +  a)  (x  +  b)  =  x2  +  (a  +  b)x  +  ab  (1). 

This  virtually  includes  all  possible  cases  ;  for  example,  putting  -  a  for  a 

we  get 

(x  +  (  -  a))  {x  +  b)  =x-  +  ((  -  a)  +  b)x  +  (  -  a)b, 

=  x2  +  {-a  +  b)x  -  ab. 


60  DISTRIBUTION  OF  (x  -  ff  x)  (x  -  C(2)  .  .  .  (x  -  an)  CHAP. 

Similarly  (a:  -  a)  (x  -  b)  =  or  +  (  -  a  -  b)x  +  ab, 

=  o?  -(a  +  b)x  +  ab. 
(x  -  a)  (x  -  a)  =  o;"  +  ( -  a  t  a)x+  a2, 
=  or  -  lax  +  a",  &c. 
Cases  in  which  numbers  occur  in  place  of  a  and  b,  or  in  which  x  is  affected 
with  coefficients  in  the  two  factors,  may  be  deduced  by  specialisation  or  other 
modification  of  formula  (1),  for  example, 

U'-2)(.r+3)=.r2  +  (-2  +  3)z  +  (-2)(  +  3), 
=  or  +  x-6. 


(px  +  q)  (rx  +  s)  =p  (  x  + 


«\-'*+i 


=prx~+pri  -  +  -)x+pr  —  , 
=prx2  +  (rq  +ps)x  +  qs, 

which  might  of  course  be  obtained  more  quickly  by  directly  distributing  the 
product  and  collecting  the  powyers  of  x. 

In  the  case  of  three  factors  of  the  first  degree,  say  (x  +  ax) 
(x  +-  a2)  (x  +  a3),  the  highest  term  is  .r3 ;  terms  in  x2  are  obtained 
by  taking  for  the  partial  products  x  from  two  of  the  three  brackets 
only,  then  an  a  must  be  taken  from  the  remaining  bracket ;  we 
thus  get  axx2,  a2x2,  a^z2 ;  that  is,  {ax  +  aB  +  a3)x2  is  the  term  in  x2. 
To  get  the  term  in  x,  x  must  be  taken  from  one  bracket,  and  a's 
from  the  two  remaining  in  every  possible  way ;  this  gives 
(a^a2  +  a,{az  +  a2a3)x.  The  last  or  absolute  term  is  of  course  a^a^ 
Thus  (x  +  rtj)  (x  +  a.,)  (x  +  a3) 

=  x3  +  (a,  +  a2  +  a3)x2  +  (rt,a2  +  a,a3  +  a2a3)x  +  alaia3     (2). 

By  substitution  all  other   cases   may  be  derived  from  (2),  for 
example, 

(x  -  a,)  (x  -  a2)  (x  -  a3) 

=  x3  -  (a,  +  a2  +  a3)x2  +  (aaaa  +  a,a3  +  a2a3)x  -  axa2a3     (3) ; 
(x  +  1)  (x  +  2)  (x  -  3)  =  x  -  7x  -  G,  and  so  on. 

After  what  has  been  said  it  is  easy  to  find  the  form  of  the  dis- 
tribution of  a  product  of  n  factors  of  the  first  degree.    The  result  is 

(x  +  «,)  (x  +  a2) .  .  .  (x  +  an) 

=  xn  +  P.a:'1-1  +  P^'-2  +  .  .   .  +  P„_,a;  +  Pn  (4), 


IV 


BINOMIAL  THEOREM  61 


where  Px  signifies  the  algebraic  sum  of  all  the  a's,  P2  the  alge- 
braic sura  of  all  the  products  that  can  be  formed  by  taking  two 
of  them  at  a  time,  P3  the  sum  of  all  the  products  three  at  a  time, 
and  so  on,  Pn  being  the  product  of  them  all. 

§  10.]  The  formula  (4)  of  §  9  of  course  includes  (1)  and  (2) 
already  given,  and  there  is  no  difficulty  in  adapting  it  to  special 
cases  where  negative  signs,  &c,  occur.  The  following  is  par- 
ticularly important : — 

=  Xn  -  P,':"-1  +  P^-2  -...  +  (-  l)"-1^-!*  +  (  -  l)»Pn    (I)- 

Here  Tt  P2,  &c,  have  a  slightly  different  meaning  from  that 
attached  to  them  in  §  9  (4) :  P3,  for  example,  is  not  the  sum 
of  all  the  products  of  -a1}  -  a2,  .  .  .,  -  an,  taken  three  at  a 
time,  but  the  sum  of  the  products  of  +  a1}  +  a2,  .  .  .,  +  an,  taken 
three  at  a  time;  and  the  coefficient  of  a;n".3  is  therefore  -  P3, 
since  the  concurrence  of  three  negative  signs  gives  a  negative 
sign.     As  a  special  case  of  (1)  let  us  take 

(x  -  a) (x  -  2a)(x  -  Sa)(x  -  4a)  =  x*  -  Prx3  +  F2x2  -  P^  +  P4. 

Here  P,  =  a  +  2a  +  3a  +  4a  =  10a, 

P2  =  1  x  2a8  +  1  x  3a"  +  1  x  4a2  +  2  x  3«2  +  2  x  4a2  +  3  x  4a2 

=  35  a2, 
P3  -  2  x  3  x  4a3  +  1  x  3  x  4a  +  1  x  2  x  4a3  +  1  x  2  x  3a3 

-  50a3, 
P4=  1  x  2  x  3  x  4a'  =  24a4. 

So  that  (x  -  a)  (x  -  2a)  (x  -  3a)  (x  -  4a) 

-  x  -  Wax3  +  35a2/  -  50a3*  +  24«\ 

§  11.]  Another  important  case  of  §  9  (4)  is  obtained  by 
making  al  =  a2  =  a3  =  .  .  .  =  an,  each  =  a  say.  The  left-hand  side 
then  becomes  (x  +  a)n.  Let  us  see  what  the  values  of  Pn  P2,  .  .  ., 
Pn  become.  Pj  obviously  becomes  na,  and  Pn  becomes  an.  Con- 
sider any  other,  say  Pr;  the  number  of  terms  in  it  is  the  number 
of  different  sets  of  r  things  that  Ave  can  choose  out  of  n  things. 
This  number  is,  of  course,  independent  of  the  nature  of  the 
things  chosen  ;  and,  although  we  have  no  means  as  yet  of  calcu- 
lating it,  we  may  give  it  a  name.     The  symbol  generally  in  use 


62  BINOMIAL  COEFFICIENTS  chap. 

for  it  is  nCr,  the  first  suffix  denoting  the  number  of  things  chosen 
from,  the  second  the  number  of  things  to  be  chosen.  Again, 
each  term  of  Pr  consists  of  the  product  of  r  letters,  and,  since  in 
the  present  case  each  of  these  is  a,  each  term  will  be  ar.  All 
the  terms  being  equal,  and  there  being  nCr  of  them,  we  have  in 
the  present  case  Pr  =  nC/tr.     Hence 

(x  +  a)n  =  xn  +  nazn-1  +  nC2a2xn~2  +  nQ3azxn~z  +  .   .  .  +  an ; 

or,  if  we  choose,  since  nC\  —  n>  rfin  =  1,  we  may  write 

(x  +  a)n  =  xn  +  nC^x71'1  +  nC2a2xn~2  +  ...  +  nOn.lcfl-1x  +  nCnan  (1). 

This  is  the  "  binomial  theorem  "  for  positive  integral  exponents,  and 
the  numbers  nCM  nC2,  nC3,  .  .  .  are  called  the  binomial  coefficients  of 
the  nth  order.  They  play  an  important  part  in  algebra  j  in  fact, 
the  student  has  already  seen  that,  besides  their  function  in  the 
binomial  expansion,  they  answer  a  series  of  questions  in  the 
theory  of  combinations.  When  we  come  to  treat  that  subject 
more  particularly  we  shall  investigate  a  direct  expression  for  nCr 
in  terms  of  n  and  r.  Later  in  this  chapter  we  shall  give  a  pro- 
cess for  calculating  the  coefficients  of  the  different  orders  by 
successive  additions. 

By  substituting  successively  -a,  +1,  and  -  1  for  a  in  (1) 
we  get 

(x  -  a)n  =  xn  -  nGxaxn  ~ 1  +  nC2a2xn  -  2  -  nG3a3xn  -  3  +  .   .  . 

+  (  -  1)WW  (2) ; 

(x+l)n  =  xn  +  nC1xn-l  +  nC.p:n-2  +  .   .   .+„Cn  (3); 

(x-l)n  =  xn-nC1xn-1  +  nCfP-*-.   .  .  +  (-l)\Cn  (4); 

and  an  infinity  of  other  results  can  of  course  be  obtained  by 
substituting  various  values  for  x  and  a. 

§  12.]  In  expanding  and  arranging  products  of  two  integral 
functions  of  one  variable,  the  process  which  is  sometimes  called 
the  long  rule  for  multiplication  is  often  convenient.  It  consists 
simply  in  taking  one  of  the  functions  arranged  according  to 
descending  powers  of  the  variable  and  multiplying  it  successively 
by  each  of  the  terms  of  the  other,  beginning  with  the  highest 
and  proceeding  to  the  lowest,  arranging  the  like  terms  under 
one  another.     Thus  we  arrange  the  distribution  of 


iv  LONG  MULTIPLICATION  63 

(xa+2x2+2x+l)(x2-x+l) 
as  follows  : —  a?  +  2x2  +  2x  +  1 

x2  -    x  +  1 


x  +  2x*  +  2xa  +    of 
-    x4  -  2/  -  2x2  -    x 

+    z*  +  2x2  +  2x  +  1 


x*  + 

x*  +    x3  + 

x2 

+ 

x  + 

1 

or  again 

(px* 

+  qx  +  r)(rx2 

+ 

qx+p) 

px2 

+  qx 

+  r 

rx* 

+  qx 

+  p 

prx* 

+  qrx3 
+  pqx3 

2    2 

+  r  x 

2    2 

+  qx 

+  qrx 

+  px 

+  pqx 

+  pr 

prxK  +  (pq  +  qr)x3  +  (jf  +  q2  +  r2)x2  +  (pq  +  qr)x  +  pr. 

The  advantage  of  tins  scheme  consists  merely  in  the  fact  that 
like  powers  of  x  are  placed  in  the  same  vertical  column,  and  that 
there  is  an  orderly  exhaustion  of  the  partial  products,  so  that 
none  are  likely  to  be  missed.  It  possesses  none  of  the  funda- 
mental importance  which  might  be  suggested  by  its  prominent 
position  in  English  elementary  text-books. 

§  13.]  Method  of  Detached  Coefficients. — When  all  the  powers 
are  present  a  good  deal  of  labour  may  be  saved  by  merely 
writing  the  coefficients  in  the  scheme  of  §  12,  which  are  to  be 
multiplied  together  in  the  ordinary  way.  The  powers  of  x  can 
be  inserted  at  the  end  of  the  operation,  for  we  know  that  the 
highest  power  in  the  product  is  the  product  of  the  highest  powers 
in  the  two  factors,  and  the  rest  follow  in  order.  Thus  we  may 
arrange  the  two  multiplications  given  above  as  follows  : — 

1+2+2+1 
1-1  +  1 

1+2+2+1 
-1-2-2-1 

+1+2+2+1 

1+1+1+1+1+1; 


61 


DETACHED  COEFFICIENTS 


CHA1". 


•whence 

(x3  +  2.c2  +  2x  +  l)(x2  -  x  +  1)  =  Xs  +  x*  +  x3  +  %•  +  x  +  1. 
Again, 


p 

+  2 

+  r 

r 

+  1 

+  1> 

pr 

+  qr 

+  r~ 

+  M 

+  qr 

+  pq  +  pr 


pr  +  (qr  +  pq)  +  (p2  +  q2  +  r2)  +  (pq  +  qr)  +  pr  ; 
whence 

(px2  +  qx  +  r)(rx2  +  qx  +p) 

-  prx*  +  (pq  +  qr)x3  +  (p2  +  q2  +  r2)x~  +  (pq  +  qr)x  +  pr. 

The  student  should  observe  that  the  use  of  brackets  in  the 
last  line  of  the  scheme  in  the  second  example  is  necessary  to 
preserve  the  identity  of  the  several  coefficients. 

It  has  been  said  that  this  method  is  applicable  directly  only 
when  all  the  powers  are  present  in  both  factors,  but  it  can  be 
made  applicable  to  cases  where  any  powers  of  x  are  wanting  by 
introducing  these  powers  multiplied  by  zero  coefficients.  For 
example — 

(xi-2x"+l)(xi  +  2x2+l) 

=  (%*  +  Ox3  -  2x2  +  Ox  +  l)(x*  +  Ox3  +  2x2  +  Ox  +  1) ; 

1+0-2+0+1 
1+0+2+0+1 


whence 


1+0-2+0+1 
+0+0+0+0+0* 
+2+0-4+0+2 

+0+0+0+0+0* 
+1+0-2+0+1 

1 +0+0+0-2+0+0+0+1 

x*  +  O.c7  +  0x°  +  0/  -  2x*  +  0xa  +  0/  +  Ox  +  1  ; 

(x*  -  2x2  +  1)(^4  +  2x2  +  1)  =  x  -  2x*  +  1. 


iv  DETACHED  COEFFICIENTS  65 

The  process  might,  of  course,  be  abbreviated  by  omitting  the 
lines  marked  *,  which  contain  only  zeros,  care  being  taken  to 
place  the  commencement  of  the  following  lines  in  the  proper 
columns  ;  and,  in  writing  out  the  result,  the  terms  with  zero 
coefficients  might  be  omitted  at  once.  With  all  these  simplifica- 
tions, the  process  in  the  present  case  is  still  inferior  in  brevity 
to  the  following,  which  depends  on  the  use  of  the  identities 
(A  +  B)  (A  -  B)  =  A2  -  B2,  and  (A  +  B)2  =  A2  +  2AB  +  B2. 

(x*  -  2x*  +  1)  (x*  +  2x*  +  1)  =  {(x*  +  1)  -  2x*}{(x<  +  1)  +  2x2} 

=  (x*  +  I)2  -  (2xJ 
=  x  +  2x*  +  1  -  4a;4 
=  x*-2x*+l. 

The  method  of  detached  coefficients  can  be  applied  with  ad- 
vantage in  the  case  of  integral  functions  of  two  letters  which  are 
homogeneous  (see  below,  §  17),  as  will  be  seen  by  the  following 
example  : — 

(J  -  xy  +  f)  (x3  -  2x*y  +  2xf  -  f), 
1-2+2-1 
1-1  +  1 


1-2+2-1 
-14-2-2  +  1 
+1-2+2-1 

1-3  +  5-5  +  3-1, 
=  x"  -  Sx*y  +  Ssfy*  -  bx*y*  +  2>x>f  -  y. 

If  the  student  Avill  work  out  the  above  distribution,  arrange 
his  work  after  the  pattern  of  the  long  rule,  and  then  compare, 
he  will  at  once  see  that  the  above  scheme  represents  all  the 
essential  detail  required  for  calculating  the  coefficients. 

The  reason  of  the  applicability  of  the  process  is  simply  that 
the  powers  of  x  diminish  by  unity  from  left  to  right,  and  the 
powers  of  y  in  like  manner  from  right  to  left. 

We  shall  give  some  further  examples  of  the  method  of 
detached  coefficients,  by  using  it  to  establish  several  important 
results. 

VOL.  ]  F 


66  PASCAL'S  ARITHMETICAL  TRIANGLE  chap. 

§  14.]  Addition  Rule  for  calculating  the  Binomial  Coefficients. 
We  have  to  expand  (x  +  l)2,  (x  +  l)3,  .   .   .,  (x  +  l)n.     Let  us 
proceed  by  successive  distribution,  using  detached  coefficients. 

1  +  1  (The  coefficients  of  x  +  1 ), 

1  +  1 


1  +  1 

+  1  +  1 

1  +  2  +  1  (The  coefficients  of  (x  +  l)2), 

1  +  1 


1  +  2  +  1 

+1+2+1 

1  +  3  +  3+1   (The  coefficients  of  (x  +  l)3). 

The  rule  which  here  becomes  apparent  is  as  follows  : — 
To  obtain  the  binomial  coefficients  of  any  order  from  those  of  the 
previous  order — 1st,  Write  down  the  first  coefficient  of  the  previous  order; 
2nd,  Add  the  second  of  the  previous  order  to  the  first  of  the  same  ; 
3rd,  Add  the  third  of  the  previous  order  to  the  second  of  the  same  ; 
and  so  on,  taking  zeros  when  the  coefficients  of  the  previous  order  run 
out.  We  thus  get  in  succession  the  first,  second,  third,  &c,  coefficients 
of  the  new  order.     For  example,  those  of  the  fourth  order  are 

1  +  (1  +  3)  +  (3  +  3)  +  (3  +  1)  +  (1  +  0), 
that  is,  1+4  +6  +4  +1, 

which  agrees   with   the  result  obtained  by  a  different  method 
above,  §  2  (6). 

We  have  only  to  show  that  this  process  is  general.  Suppose 
we  had  obtained  the  expansion  of  (x  +  l)n,  namely,  using  the  nota- 
tion of  §  11, 

(.,  +  l)»  =  xn  +  nClXn-l  +  nC2.^-2  +  nC3.^-3  +  .   .    .  +  nC»_rT  +  nCn. 
Hence 
(z+  l)n+1  =  (a;+  l)'lx(.c+  1) 

=  (^  +  nCl.r'l-1  +  nCli^-2  +  .  •  .+*Cn_1a>  +  nCn)(a;+l) 


IV  PASCAL'S  TRIANGLE  GENERALISED  67 

using  detached  coefficients,  we  have  the  scheme 

1  +  n*~>i  +  nv-'g  +  n^3  +  •    •    •  +  tv^n-i  "i~  iv^n 
1  +  1 

I  +  »^i  +  n\-  -2 +  7V~  n 

1  +  (1  +  nC,)  +  (UC,  +  MC2)  +....+  (HCn_,  +  nC„)  +  (nGn  +  0). 
Hence  (s+l)»+1 

=  af+»  +  (1  +  WC>"  +  (.0,  +  „cgaf»-»  +  („C,  +  »C,)*»-a  +  .  .  ., 
in  which  the  coefficients  are  formed  from  the  coefficients  of  the 
nth.  order,  precisely  after  the  law  stated  above,  namely, 

This  law  is  therefore  general,  and  enables  us  whenever  we 
know  the  binomial  coefficients  of  any  rank  to  calculate  those  of 
the  next,  from  these  again  those  of  the  next,  and  so  on.  A 
table  of  these  numbers  (often  called  Pascal's  Triangle)  carried  to 
a  considerable  extent  is  given  at  the  end  of  this  chapter,  among 
the  results  and  formulae  collected  for  reference  there. 

§  15.]  "We  may  calculate  the  powers  of  x3  +  xz  +  x  +  1  by 
means  of  the  following  scheme,  in  which  the  lines  of  coefficients 
of  the  constantly-recurring  multiplier,  namely,  1  +  1  +  1  +  1,  are 
for  brevity  omitted. 


Tower. 

1st. 

1 

+  1 

+ 

1 

+ 

1 

+  1 

+ 

1 

+ 

1 

+ 

1 

+ 

1 

+ 

1 

+ 

1 

+ 

1 

1 

+  2 

+ 

1 

+ 

1 

+ 

1  + 

1 
1 

2nd. 

+ 

3 

+ 

4 

+ 

3 

+ 

2  + 

+  1 

+ 

2 

+ 

3 

+ 

4 

+ 

3  + 

2  + 

1 

+ 

1 

+ 

2 

+ 

3 

+ 

4  + 

3  + 

2+    1 

1 

+ 

1 

+ 

2 

+ 

3  + 

4  + 

3+    2+    1 

3rd. 

+  3 

+ 

6 

+ 

10 

+ 

12 

+ 

12  + 

10  + 

6+3+1 

+  1 

+ 

3 

+ 

0 

+ 

10 

+ 

12  + 

12  + 

10+    6+    3  + 

1 

+ 

1 

+ 

3 

+ 

6 

+ 

10  + 

12  + 

12  +  10+    6  + 

3  +  1 

+ 

1 

+ 

o 

+ 

6  + 

10  + 

12  +  12  +  10  + 

6  +  3  +  1 

4th.  1  +  4  +  10  +  20  +  31  +  40  +  44  +  40  +  31  +  20+10  +  4+1 

and  so  on. 


68  Xn  ±  if  AS  A  PRODUCT  chap. 

The  rule  clearly  is— Jo  get  from  the  coefficients  of  any  order 
the  rth  of  the  succeeding,  add  to  the  rth  of  that  order  the  three  preced- 
ing coefficients,  taking  zeros  when  the  coefficients  required  by  the  ride  do 

not  exist. 

The  rule  for  calculating  the  coefficients  of  the  powers  of 
xn  +  x71'1  +  x1l~2  +  .  .  .+x+l  is  obtained  from  the  above  by 
putting  n  in  place  of  3. 

These  results  may  be  regarded  as  a  generalisation  of  the  pro- 
cess of  tabulating  the  binomial  coefficients.  They  are  useful  in 
the  Theory  of  Probability. 

§  16.]  As  the  student  will  easily  verify,  we  have 

(x-y)(x2  +  xy  +  f)  =  x3-y3  (1), 

(as  +  y)  (x2  -  xy  +  f)  =  x3  +  y3  (2). 

The  following  is  a  generalisation  of  the  first  of  these : — 
If  n  be  any  integer, 

(a;  -  y)  (xn  - 1  +  xn  ~  %y  +  xn~3y2  +  .  .  .  +  xyn  ~ 2  +  yn  ~ a), 

1  +  1  +  1  +.  .  .+  1  +  1 
1-1 

1  +  1  +  1  +.  .  .  +  1  +  1 
-1-1-.   .   .-1-1-1 


1  +  0  +  0  +  .  .  .  +  0  +  0-1 

-  xn  -  yn  (3). 

Again,  n  being  an  odd  number, 

(x  +  y)  (xn ~ 1  -  xn ~hj  +  xn -3y2--  •  •  ~  Xlf  " 2  +  Vn ' *)> 
(  -  sign  going  with  odd  powers  of  y) 
1  -  1  +  1  -  .  .   .  -  1  +  1 
1  +  1 


1-1+1-. . .-1+1 
+  1-1+.   .   .  +  1-1  +  1 

1  +  0  +  0  +  .  .   .  +  0  +  0+1 

■  xtl  +  yn  (4). 


iv  EXERCISES  VI  69 

And,  similarly,  n  being  an  even  number, 

(x  +  y)  (xn  ~ l  -  xn  ~2y  +  xn  ~  hf  -  .  .  .  4  xf  ' 2  -  if  ~ l) 

=  xn  -if  (5). 

The  last  two  may  be  considered  as  generalisations  of  (2)  and  of 
(x  +  if)  (x  -  y)  =  x2  -  if  respectively. 

Exercises  VI. 

(1. )  The  variables  being  x,  y,  z,  point  out  the  integral  functions  among  the 
following,  and  state  their  degree  : — 

(a)  Zx"-  +  2xy+Sy~  ; 
,m3      2      3 
x-    xy    y- 
(7)  a?yz  +  y-zx  +  z"xy  +  x3  +  y3  +  z3  ; 

.„  x-y-z*    a?}/2*    oW 
X'yz       xyz       xyz- 

Distribute  the  following,  and  arrange  according  to  powers  of  x  : — 

(2.)  6{aj-J(a!-l)}{a!-S(a!-l)}+20{a!-|(a!-l)}{a;-|(a;-l)}. 

x(x  +  l)(x  +  3)    a;(a;+l)(2a:+l) 
(3.)  g . 

(4.)  {(aj-2)(a:-3)+<a;-3)(a;-l)  +  (a:-l)(a!-2)} 

x  {(a;+2)(a;+3)  +  (a;+3J(a;+l)  +  (a:+l)(ar+2)}. 

(5.)  {x  +  a}  {x-  +  (b  +  c)x  +  bc}  {x3 -  (a  +  b  +  c)x"  +  (be  +  ca  +  ab)x - abc] . 
(6.)  {(x+p)(x-q)(x  +  l)}{(x-p)(x  +  q)(x-l)}. 
(7. )  (z2  -  y")  (x*  -  2f)  (a?  -  3/)  (a?  -  4tf)  (a?  -  5y- ). 

(8.)  {az  +  (6-c)y}  {te  +  (c-a)?/}  {<.-.>■  +  («-%}  ;*    and    show   that   the 
sum  of  the  coefficients  of  x-y  and  y3  is  zero. 

(9.)  Show  that 

(x  +  4«)4  - 1  Oa(x  +  £«)3  +  35a2(.r  +  £a)2  -  50a3(a;  +  |a)  +  24a4 
=  (x2-i«2)(ar-|a2). 
(10.)  Show  that 

(-  +  ^)(-+^)(-  +  fl/)-(-  +  ^)(-  +  ?2/)(-  +  ^ 
_a;y(a;-2/)(g-r)(r-jp)(p-g) 

Distribute  and  arrange  according  to  powers  of  x,  the  following  : — 

(11.)  {(i+c)a!s+(c+a)aj+(a+J)}-{(&-c)arJ+(c-a)a;+(ffl-&)}. 
(12.)  (xn'-x  +  l){x2  +  x  +  l)(x'1-2x  +  l){xi  +  2x  +  l). 


*  In  working  some  of  these  exercises  the  student  will  find  it  convenient  to 
refer  to  the  table  of  identities  given  at  the  end  of  this  chapter. 


70  EXERCISES  VI,  VII  chap. 

(13.)-!  5x2  -  ix(x  -y)  +  {x  -y)2}  (2s  +  By). 
(14. )  (2x2  -  Zxy  +  2y2)  (2x2  +  Bxy  +  2if). 
(15.)  {(x-+x+l)(x--x  +  l)(x--l)}\ 
(16.)  (x3-x~  +  x-l)-{x*  +  x~  +  x+l)2. 

(17.)  {lx*-fr?  +  lx+%)(ix*+fr?-hx+i)- 

(18.)  (x*  -  ax*y  +  abx-y"  +  bxy3  +  y*)  (ax2  -  abxy  +  by"). 

(19.)  (x2  +  ax  +  b2)3  +  (x2  +  ax-  b2)3  +  (x2  -  ax  +  b2)3  +  (x2  -ax-  b2)3. 

(20.)  (xi-2a2x2  +  a*)\ 

(21.)  (.r4-a5)3. 

(22.)  (3*+|)'. 

(23.)  (a  +  bx2)*. 

(24.)  {(^  +  2/3)(^-2/3)}9. 

(25.)  (l+z  +  a:2  +  a;3  +  ai4)3. 

(26.)  Calculate  the  coefficient  of  a;4  in  the  expansion  of  (1+x  +  x2)8. 
(27. )  Calculate  the  coefficient  of  Xs  in  (1  -  2x  +  3x2  +  4x?-  xA)\ 
(28.)  Show  that 

{a  +  b)3(a5  +  b5)  +  5ab(a  +  b)2(a4  +  64)  +  I5a2b2(a  +  b)  {a3  +  b3) 
+  B5a3b3(a2  +  b2)  +  70aibi=(a  +  b)\ 
(29.)  Show  that 

«Ci  +  nC2  +  „C3+ .   .  .  +„C„  =  2"-1; 
1  +  «Co  +  nCi  +  .  .  .  =  »Cj  +  nC-3  +  nCs  +  .  .  .  ; 

(30. )  There  are  five  boxes  each  containing  five  counters  marked  with  the 
numbers  0,  1,  2,  3,  4  ;  a  counter  is  drawn  from  each  of  the  boxes  and  the 
numbers  drawn  are  added  together.  In  how  many  different  ways  can  the 
drawing  be  made  so  that  the  sum  of  the  numbers  shall  be  8  ? 

(31.)  Show  that 
(x-y)2(xn-2  +  xn-3y+  .  .  .  +xyn-3  +  yn-2)  =  xn-xn-ly-xyn-1  +  ijn. 


Exercises  VII. 

Distribute  the  following,  and  arrange  according  to  descending  powers 
of  x: — 

(1.)  (3.i'  +  4)(4;c  +  5)(5;e  +  6)(6a;  +  7). 

(2. )  (px  +  q-r) (qx  +  r-p) (rx  +p  - q). 

(3. )  [x  -  a)  (x  -  2a)  [x  -  3a)  {x  -  4a)  (x  +  a) (x  +  2a)  (x  +  3a)  (x  +  4a). 

(4. )  (x3  +  2,x2  +  2x  + 1)  (or3  -  3.x-2  +  Bx  -  1 ). 

(5. )  (ix3  +  \x2  +  \x  +  f )  (Ix3  +  \x2  +  kx  + 1 ). 

(6.)  (x-#{x*-ix+l)(x+lHx*+fr+i). 

7.  l-x2  +  -x+7)  (-x2  +  1x  +  -       -JX-  +  -X+-). 

(8.)  (2aj-3)» 

(9.)  {{x+y)(x*-xy+y*)}*. 

(10.)  (a;2-l)4(u;  +  l)10. 


iv  HOMOGENEOUS  FUNCTIONS  71 

(11.)  In  the  product  (x  +  a)(x+b)(z+e),  -r-  disappears,  and  in  the  product 
(x- a)(x+b)(x  +  c),  x  disappears;  also  the  coefficient  of  X  in  the  former  is 
equal  to  the  coefficient  of  a;2  in  the  latter.     Show  that  a  is  either  0  or  1. 

Prove  the  following  identities  : — 

(12.)  (b-c)(x-a)2+(c-a){x-b)2+(a-b){x-c)2  +  (b-c)(c-a){a-b)  =  0. 

(13. )  2(2a  -  b  -  c)  (h  -  6)  (h  -c)  =  2(6  -  c)-{h  -  a). 

(14.)  (s-af+(s-b)3  +  (s-c)*  +  3abc  =  s3, 
where  2s  =  a  +  b  +  c. 

(15.)  (s-a)*+(8-b)4+(8-c)* 

=  2(s  -  b)%s  -  c)2  +  2(s  -  c)2(s  -  a)2  +  2(s  -  a)2(s  -  b)2, 
where  3s  =  a  +  b  +  c. 

(16.)  (as+bc)(bs+ ca)  (cs  +  ab)  =  (b  +  c)2(c  +  a)2(a  +  6)2,  where  s  -  a  +  b  +  c. 

(17 '. )  s(s  -  a  -  d)(s  -  d-b)(s  -  c  -  d)  =  (s  -  a)(s  -b)(s  -  c)  {s  -  d)  -  abed, 
where  2s  =  a  +  b  +  c  +  d. 

(18. )  16(8  -  a) (s  -b)(s-  c)  (s -  d)  =  4(6c  +  ad)2 -  (62  +  c2  -  a2  -  d2)2, 
where  2s=a+b  +  c+d. 

(19. )  2(6  -  c)6=3n(i  -  cf  +  2(2«2  -  26c)3. 

(20.)  If  U„  =  (6-  c)n  +  (c  -«)"  +  («  -6)»,  then 

Un+3  -  (a2  +  b2  +  c2-bc-ca-  ab)Vn+1  -  (b  -  e)  (e  -  a)  (a  -  5)U„=  0. 
(21.)  If  pi  =  a  +  b  +  c,  p2  =  bc  +  ca  +  ab,  p3  =  abc,  sn  =  an  +  bn  +  cn,  show  that 
Si  =lh ,  s2  -piSi  -  2p-2 ,  ss  =piS-2  -  paSi  +  3p3 , 

S»  =PlS„-i  -p-fin-2  +PsSn-3- 

(22. )  If  j)-2=  (b  -c)(e-a)  +  (e-  a)  (a  -  6)  +  (a  -  6) (6  -  c), 
2i3=(b-c){c-a){a-b), 
sH  =  (b-  c)n  +  (c-  a)n  +  {a-  6)» 
show  that 

*2  =  -  S^pa ,     «3  =  3ps ,     Si = 2ps?,    ss=  -  5p»ps, 
sfi  =  - 2pa8  f  8pg8,     s7  =  7p-2ps 5     20S7S3  =  21s52. 


Homogeneity. 

§  17.]  An  integral  function  of  any  number  of  variables  is  said 
to  be  "  Homogeneous  "  when  Vie  degree  of  every  term  in  it  is  the  same. 
In  such  a  function  the  degree  of  the  function  (§  G)  is  of  course 
the  same  as  the  degree  of  every  terra,  and  the  number  of  terras 
which  (in  the  most  general  case)  it  can  have  is  the  number  of 
different  products  of  the  given  degree  that  can  he  formed  with 
the  given  number  of  variables.  If  there  be  only  two  variables, 
and  the  degree  be  n,  we  have  seen  that  the  number  of  possible 
terms  is  n  +  1. 


72  HOMOGENEOUS  FUNCTIONS  chap. 

For  example,  the  most  general  homogeneous  integral  functions  of  x  and  y 
of  the  1st,  2nd,  and  3rd  degrees  are  * 

Az+By  (1), 

Ax2  +  Bxy  +  Cy2  (2), 

Ax3  +  Bx2y  +  Cxy2  +  Vy3  ( 3), 

A,  B,  C,  &c. ,  representing  the  coefficients  as  usual. 
For  three  variables  the  corresponding  functions  are 

Ax  +  By  +  Cz  (4), 

A*2  +  By1  +  Cz2  +  Vyz  +  Esse  +¥xy  (5), 

Ax3  +  Bif  +  Cz3  +  Vyz2  +  P'tfz  +  Qzx2  +  Q,'z2x  +  Bxy2  +  Wx2y  +  Sxyz  ( 6 ), 

&c, 

As  the  case  of  three  variables  is  of  considerable  importance,  we  shall  in- 
vestigate an  expression  for  the  number  of  terms  when  the  degree  is  n, 

We  may  classify  them  into — 1st,  those  that  do  not  contain  x  ;  2nd,  those 
that  contain  x ;  3rd,  those  that  contain  x2 ;  .  .  . ;  n  +  lth,  those  that  contain  xn. 

The  first  set  will  simply  be  the  terms  of  the  ?ith  degree  made  up  with 
y  and  z,  n  +  1  in  number  ;  the  second  set  will  be  the  terms  of  the  (?i  —  l)th 
degree  made  up  with  y  and  z,  n  in  number,  each  with  x  thrown  in  ;  the  third 
set  the  terms  in  y  and  2  of  («-2)th  degree,  n-l  in  number,  each  with  x2 
thrown  in  ;  and  so  on.     Hence,  if  N  denote  the  whole  number  of  terms, 

N  =  (7!+l)+?l  +  (?l-l)+  .     .     .+2  +1. 

Reversing  the  right-hand  side,  we  may  write 

N=         1  +2+         3  +  .   .   .  +n  +  (n  +  l). 

Now,  adding  the  two  left-hand  and  the  two  right-hand  sides  of  these  equali- 
ties, we  get 

2N=(»+2)  +  (»+2)  +  (»  +  2)+.   .  .  +(h  +  2)  +  («  +  2); 

=  (n  +  l){n  +  2), 

since  there  are  n  +  1  terms  each  =n  +  2. 
Whence  N=4(»+l)(»+2). 

For  example,  let  n  =  3 ;  N=£(3+ 1)  (3  +  2)=  10,  which  is  in  fact  the  number 
of  terms  in  (6),  above. 

In  the  above  investigation  we  have  been  led  incidentally  to  sum  an 
arithmetical  series  (see  chap,  xx.)  ;  if  we  attempted  the  same  problem  for  4, 
5,  .  .  .,  7n  variables,  we  should  have  to  deal  with  more  and  more  complicated 
series.  A  complete  solution  for  a  function  of  the  ?i.th  degree  in  m  variables 
will  be  given  in  the  second  part  of  this  work. 

*  Homogeneous  integral  functions  are  called  binary,  ternary,  &c,  accord- 
ing as  the  number  of  variables  is  2,  3,  &c.  ;  and  quadric,  cubic,  &c,  according 
as  the  degree  is  2,  3,  &c.  Thus  (3)  would  be  called  a  binary  cubic  ;  (5)  a 
ternary  quadric  ;  and  so  on. 


IV  HOMOGENEOUS  FUNCTIONS  73 

The  following  is  a  fundamental  property  of  homogeneous 
functions  : — If  each  of  the  variables  in  a  homogeneous  function  of  the 
nth  degree  be  multiplied  by  the  same  quantity  p,  the  result  is  the  same 
as  if  the  function  itself  were  multiplied  by  pn. 

Let  us  consider,  for  simplicity,  the  case  of  three  variables ; 
and  let 

F  =  kxPtftf  +  A'«py tf'  +  .  .  ., 

where  p  +  q  +  r  =p'  +  q  +  r'  =  &c,  each  =  n. 

If  we  multiply  x,  y,  z  each  by  p,  we  have 

F  =  A(px)*(py)i(pzy  +  A'(pr)P'(pyy(P:y  +  .  .  . } 
=  ApP+<i+rxPy(}zr  +  A'pP'+<i'+r'xP'f'zr'+  .  .  ., 

by  the  laws  of  indices.     Hence,  since  p  +  q  +  r  =  p  +  q  +  r'  =  &c. 
=  n,  we  have 

F'  =  pn  {  AxPy?zr  +  A'xP'y<i'zr'  +...}, 

=  pnF, 

which    establishes    the    proposition   in   the    present    case.     The 
reasoning  is  clearly  general.* 


*  This  property  might  be  made  the  definition  of  a  homogeneous  function. 
Thus  we  might  define  a  homogeneous  function  to  be  such  that,  when  each 
of  its  variables  is  multiplied  by  p,  its  value  is  multiplied  by  pn  ;  and  define  n 
to  be  its  degree.  If  we  proceed  thus,  we  naturally  arrive  at  the  idea  of  homo- 
geneous functions  which  are  not  integral  or  even  rational  ;  and  we  extend  the 
notion  of  degree  in  a  corresponding  way.  For  example,  (.c3-  y3)/(x  +  y)  is 
a  homogeneous  function  of  the  2nd  degree,  for  ( (px)3  -  {py)3)j{  (px)  +  (py) ) 
=  pi(x3  -  y3)/(x  +  y).  Similarly  \Z(-t'3  +  V3)'  l/(*2  +  V") are  homogeneous  functions, 
whose  degrees  are  f  and  -2  respectively  (see  chap,  x.)  Although  these  ex- 
tensions of  the  notions  of  homogeneity  and  degree  have  not  the  importance  of 
the  simpler  cases  discussed  in  the  text,  they  are  occasionally  useful.  The 
distinction  of  homogeneous  functions  as  a  separate  class  is  made  by  Euler  in 
his  Introductio  in  Analysin  fnfinitorum  (1748),  (t.  i.  chap,  v.),  in  the  course 
of  an  elementary  classification  of  the  various  kinds  of  analytical  functions. 
He  there  speaks,  not  only  of  homogeneous  integral  functions,  but  also  of 
homogeneous  fractional  functions,  and  of  homogeneous  functions  of  fractional 
or  negative  degrees. 


74  LAW  OF  HOMOGENEITY  chap. 

Example. 

Consider   the  homogeneous  integral   function   3.>j2  -  2xy  +  y2,  of  the  2nd 
degree.     We  have 

3(/w)2  -  2(Px)  (Py)  +  (p2/)2= 3pV  -  2p"xy  +  p*y*, 
=P*(dxi-2vy+y2)> 
in  accordance  with  the  theorem  above  stated. 

The  following  property  is  characteristic  of  homogeneous  integral 
functions  of  the  first  degree. 

If  for   the  variables  x,  y,  z,  .  .  .  toe  substitute  Xx,  +  /j..r2,  kyx 
+  ayat   Xzx  +  fxz2,   .  .  .  respectively,  the  result  is  the  same  as   that 
obtained  by  adding  the  results  of  substituting  x„-yXi  zlt  .   .  .  and  x2, 
y,,  z2,  .  .  .  respectively  for  x,  y,  z,  .  .  .  in  the  function,  after  multi- 
plying these  results  by  X  and  fi  respectively. 

Example. 

Consider  the  function  Ax  +  By  +  Cz. 

We  have 

A(X.ri  +  fix.,)  +  B(\2/!  +  ^2)  +  C(Xzi  +  ftna) 

=  AXa'x  +  BXyi  +  C\Sj  +  Afix?  +  Bp.y-2  +  Cfiz* 
=  \(  Aa?i  +  Byx  +  Czi)  +  fi{Ax.2  +  By-2  +  Cz»). 

This  property  is  of  great  importance  in  Analytical  Geometry. 

§  18.]  Law  of  Homogeneity. — Since  every  term  in  the  product 
of  two  homogeneous  functions  of  the  mth  and  ?ith  degrees  re- 
spectively is  the  product  of  a  term  (of  the  mth  degree)  taken 
from  one  function  and  a  term  (of  the  «th  degree)  taken  from 
the  other,  we  have  the  following  important  law  : — 

The  product  of  two  homogeneous  integral  functions,  of  the  mth  and 
nth  degrees  respectively,  is  a  homogeneous  integral  function  of  the 
(m  +  n)th  degree, 

The  student  should  never  fail  to  use  this  rule  to  test  the 
distribution  of  a  product  of  homogeneous  functions.  If  he  finds 
any  term  in  his  result  of  a  higher  or  lower  degree  than  that 
indicated  by  the  rule,  he  has  certainly  made  some  mistake.  He 
should  also  see  whether  all  possible  terms  of  the  right  degree  are 
present,  and  satisfy  himself  that,  if  any  are  wanting,  it  is  owing 
to  some  peculiarity  in  the  particular  case  in  hand  that  this  is  so, 
and  not  to  an  accidental  omission. 

The  rule  has  many  other  uses,  some  of  which  will  be  illus- 
trated immediately. 


IV 


SYMMETRICAL  FUNCTIONS  75 


§  19.]  If  the  student  has  fully  grasped  the  idea  of  a  homo- 
geneous integral  function,  the  most  general  of  its  kind,  he  will 
have  no  difficulty  in  rising  to  a  somewhat  wider  generality, 
namely,  the  most  general  integral  function  of  the  nth.  degree  in 
in  variables,  unrestricted  by  the  condition  of  homogeneity  or 
otherwise. 

Since  any  integral  term  whose  degree  does  not  exceed  the 
nth  may  occur  in  such  a  function,  if  we  group  the  terms  into  such 
as  are  of  the  Oth,  1st,  2nd,  3rd,  .  .  . ,  nth  degrees  respectively, 
we  see  at  once  that  we  obtain  the  most  general  type  of  such  a 
function  by  simply  writing  down  the  sum  of  all  the  homogeneous 
integral  functions  of  the  m  variables  of  the  Oth,  1st,  2nd,  3rd,  .  .  ., 
nth  degrees,  each  the  most  general  of  its  kind. 

For  example,  the  most  general  integral  function  of  x  and  y  of  the  third 
degree  is 

A  +  Bx  +  Cy  +  Dx-  +  Exy  +  Fy2  +  Gx3  +  Hx-y  +  Ixrf  +  hf. 

The  student  will  have  no  difficulty,  after  what  has  been  done 
in  §  17  above,  in  seeing  that  the  number  of  terms  in  the  general 
integral  function  of  the  ?tth  degree  in  two  variables  is 

J(n+l)(n  +  2). 

Symmetry. 

§  20.]  There  is  a  peculiarity  in  certain  of  the  functions  we 
have  been  dealing  with  in  this  chapter  that  calls  for  special  notice 
here.  This  peculiarity  is  denoted  by  the  word  "  Symmetry  ";  and 
doubtless  it  has  already  caught  the  student's  eye.  What  we 
have  to  do  here  is  to  show  how  a  mathematically  accurate 
definition  of  symmetry  may  be  given,  and  how  it  may  be  used 
in  algebraical  investigations. 

1st  Definition. — An  integral  function*  is  said  to  be  symmetrical 
with  respect  to  any  two  of  its  variables  when  the  interchange  of  these 
two  throughout  the  function  leaves  its  value  unaltered. 

*  As  a  matter  of  fact  these  definitions  and  much  of  what  follows  are 
applicable  to  functions  of  any  kind,  as  the  student  will  afterwards  learn. 
According  to  Baltzer,  Lacroix  (1797)  was  the  first  to  use  the  term  Symmetric 
Function,  the  older  name  having  been  Invariable  Function. 


76  VARIOUS  KINDS  OF  SYMMETRY  chap. 

For  example,  2a  +  Bb  +  3c 

becomes,  by  the  interchange  of  b  and  c, 

2a + 3c +36, 

which  is  equal  to  2a  +  Sb  +  Be  by  the  commutative  law.  Hence  2a  +  3b  +  3c  is 
symmetrical  with  respect  to  b  and  c.  The  same  is  not  true  with  respect  to 
a  and  b,  or  a  and  c  ;  for  the  interchange  of  a  and  b,  for  example,  would 
produce  2b  +  Sa  +  3c,  that  is,  3a +  26  + 3c,  which  is  not  in  general  equal  to* 
2a +  36  + 3c. 

2nd  Definition. — An  integral  function  is  said  to  be  symmetrical 
(that  is,  symmetrical  with  respect  to  all  its  variables)  when  the  interchange 
of  any  pair  whatever  of  its  variables  would  leave  its  value  unaltered. 

For  example,  Sx  +  Sij  +  Bz  is  a  symmetrical  function  of  x,  y,  z.  So  are 
yz  +  zx  +  xy  and  2(x2  +  y-  +  z2)  +  Zxyz.  Taking  the  last,  for  instance,  if  we 
interchange  y  and  z,  we  get 

2(x°  +  z-  +  y-)  +  3xzy, 
that  is,  2(x2  +  y2  +  z2)  +  Sxyz, 

and  so  for  any  other  of  the  three  possible  interchanges. 

On  the  other  hand,  x'2y  +  y-z  +  z-x  is  not  a  symmetrical  function  of  x,  y,  z, 
for  the  three  interchanges  x  with  y,  x  with  z,  y  with  z  give  respectively 

y-x  +  x-z  +  z~y, 

o  o  o 

z-y  +  y-x  +  x-z, 

x-z  +  z-y  +  ifx, 

and,  although  these  are  all  equal  to  each  other,  no  one  of  them  is  equal  to  the 
original  function.  It  will  be  observed  from  this  instance  that  asymmetrical 
functions  have  a  property — which  symmetrical  functions  have  not — of  assuming 
different  values  when  the  variables  are  interchanged:  thus  x2y  +  y-z  +  z~x  is 
susceptible  of  two  different  values  under  this  treatment,  and  is  therefore  a 
two-valued  function.  The  study  of  functions  from  this  point  of  view  has 
developed  into  a  great  branch  of  modern  algebra,  called  the  theory  of  substitu- 
tions, which  is  intimately  related  with  many  other  branches  of  mathematics, 
and,  in  particular,  forms  the  basis  of  the  theory  of  the  algebraical  solution  of 
equations.  (See  Jordan,  Traiti  des  Substihitions,  and  Serret,  Cours  d'Alg&bre 
Superieure. ) 

All  that  we  require  here  is  the  definition  and  its  most  elementary  con- 
sequences. 

3rd  Definition. — A  function  is  said  to  be  collaterally  symmetrical 

\   X     X  X      ) 

iii  ttco  sets  of  variables  -  '  "    2'  '  r,  each  of  the  same  number, 

I  a,,a.2,.  .  .,  an  ) 

*  It  may  not  be  amiss  to  remind  the  student  that  for  the  present  "equal 
to"  means  "transformable  by  the  fundamental  laws  of  algebra  into." 


IV 


RULE  OF  SYMMETRY  77 


ivhen  the  simultaneous  interchanges  of  two  of  the  first  set  and  of  the 
corresponding  two  of  the  second  set  leave  its  value  unaltered. 

For  example,  a?x  +  bhj  +  <?z 

and  (b  +  c)x  +  (c  +  a)y  +  (a  +  b)z 

are  evidently  symmetrical  in  this  sense. 

Other  varieties  of  symmetry  might  be  defined,  but  it  is 
needless  to  perplex  the  student  with  further  definitions.  If  he 
fully  master  the  1st  and  2nd,  he  will  have  no  difficulty  with  the 
3rd  or  any  other  case.  At  first  he  should  adhere  somewhat 
strictly  to  the  formal  use  of,  say,  the  2nd  definition  ;  but,  after 
a  very  little  practice,  he  will  find  that  in  most  cases  his  eye  will 
enable  him  to  judge  without  conscious  effort  as  to  the  symmetry 
or  asymmetry  of  any  function.* 

§  21.]  From  the  above  definitions,  and  from  the  meaning  of 
the  word  "  ecpial "  in  the  calculation  of  algebraical  identities,  we 
have  at  once  the  following 

Rule  of  Symmetry. — The  algebraic  sum,  product,  or  quotient  of 
two  symmetrical  functions  is  a  symmetrical  function. 

Observe,   however,   that   the   product,  for   example,   of  two 

asymmetrical  functions  is  not  necessarily  asymmetrical. 

Thus,  a  +  b  +  c  and  bc  +  ca  +  ab  being  both  symmetrical,  their  product, 
(a  +  b  +  c)  ( be  +  ca  +  ab)  =  b"c  +  be2  +  c"a  +  ca-  +  orb  +  ab2  +  3abc, 
is  symmetrical. 

Again,  a-bc  and  ab-c2  are  both  asymmetrical  functions  of  a,  b,  c,  yet  their 
product, 

(<rbc)  x  (ab'2c")  —  a3b3c3, 
is  a  symmetrical  function. 

§  22.]  It  will  be  interesting  to  see  what  alterations  the 
restriction  of  symmetry  will  make  on  some  of  the  general  forms 
of  integral  functions  written  above. 

Since  the  question  of  symmetry  has  nothing  to  do  with 
degree,  it  can  only  affect  the  coefficients.     Looking  then  at  the 

*  There  is  a  class  of  functions  of  great  importance  closely  allied  to  sym- 
metrical functions,  which  the  student  should  note  at  this  stage,  namely,  those 
that  change  their  sign  merely  when  any  pair  of  the  variables  are  interchanged. 
Such  functions  are  called  "alternating."  An  example  is  [y  —  z)(z-x) (x  —  y). 
Obviously  the  product  or  quotient  of  two  alternating  functions  of  the  same 
set  of  variables  is  a  symmetric  function.  The  term  Alternating  Function  is 
due  to  Cauchy  (1812). 


78  APPLICATION  OF  THE  RULE  chap. 

homogeneous  integral  functions  of  two  variables  on  page  72,  we 

see  that,  in  order  that  the  interchange  of  x  and  y  may  produce 

no  change  of  value,  we  must  have  A  =  Bin§17(l);  A  =  C  in 

(2) ;  A  =  D  and  B  =  C  in  (3). 

Hence  the  symmetrical  homogeneous  integral  functions  of  x  and  y  of  1st, 
2nd,  3rd,  &c,  degrees  are 

Ax  +  Ay  (1), 

Ax2  +  Bxy  +  Ay2  (2), 

Ax*  +  Bx2y  +  Bxy2  +  Ay3  (3), 

&c 
The  corresponding  functions  of  x,  y,  z  are 

Ax  +  Ay  +  Az  (4), 

Ax2  +  Ay2  +  Az2  +  Byz  +  Bzx  +  Bxy  (5), 

Aa?  +  Ay3  +  Az*  +  Pyz2  +  ?y2z  +  Bzx"  +  Bz2x  +  Fxy2  +  T?x2y  +  Sxyz    (6), 

&c, 
The  most  general  symmetrical  integral  function  of  x,  y  of  the  3rd  degree 
will  be  the  algebraic  sum  of  three  functions,  such  as  (1),  (2),  and  (3),  together 
with  a  constant  term,  namely, 

F  +  Ax  +  Ay  +  Bx2  +  Cxy  +  By-  +  Bx3  +  Ex'2y  +  Exy2  +  By3. 
And  so  on. 

If  the  student  find  any  difficulty  in  detecting  what  terms 
ought  to  have  the  same  coefficient,  let  him  remark  that  they  are 
all  derivable  from  each  other  by  interchanges  of  the  variables. 
Thus,  to  get  all  the  terms  that  have  the  same  coefficient  as  a;3  in 
(6),  putting  y  for  x,  we  get  y* ;  putting  z  for  x,  we  get  z3 ;  and  we 
cannot  by  operating  in  the  same  way  upon  any  of  these  produce 
any  more  terms  of  the  same  type.  Hence  .r3,  if,  z3  form  one 
group,  having  the  same  coefficient.  Next  take  yz~ ;  the  inter- 
changes x  and  y,  x  and  z,  y  and  z  produce  xz2,  yx2,  yz2 ;  applying 
these  interchanges  to  the  new  terms,  we  get  only  two  more  new 
terms — zx2,  xy2 ;  hence  the  six  terms  yz2,  y2z,  zx2,  £x,  xy2,  x2y  form 
another  group ;  xyz  is  evidently  unique,  being  itself  symmetrical. 

§  23.]  The  rule  of  symmetry  is  exceedingly  useful  in  abbre- 
viating algebraical  work. 

Let  it  be  required,  for  example,  to  distribute  the  product  (a  +  b  +  c) 
(a?  +  b2  +  c2-bc- ca-ab),  each  of  whose  factors  is  symmetrical  in  a,  b,  c.  The 
distributed  product  will  be  symmetrical  in  a,  b,  c.  Now  we  see  at  once  that 
the  term  a?  occurs  with  the  coefficient  unity,  hence  the  same  must  be  true  of 
b3  and  c3.  Again  the  term  b'-c  has  the  coefficient  0,  so  also  by  the  principles 
of  symmetry  must  each  of  the  five  other  terms,  be2,  c"«,  cu1,  ab2,  a2b,  belonging 
to  the  same  type.  Lastly,  the  term  -abc  is  obtained  by  taking  a  from  the 
first  bracket,  hence  it  must  occur  by  taking  b,  and  by  taking  c,  that  is,  the 


iv  INDETERMINATE  COEFFICIENTS  79 

a&c-terni  must  have  the  coefficient  -  3.  We  have  therefore  shown  that 
(ct  +  b  +  c)  (a?  +  b2  +  c-  -bc-ca-  ab)  =  a?  +  b*  +  c3  -  Zabc  ;  and  the  principles  of 
symmetry  have  enahled  us  to  abbreviate  the  work  by  about  two-thirds. 

PRINCIPLE    OF    INDETERMINATE    COEFFICIENTS. 

§24.]  A  still  more  striking  use  of  the  general  principles  of 
homogeneity  and  symmetry  can  be  best  illustrated  in  conjunction 
with  the  application  of  another  principle,  which  is  an  immediate 
consequence  of  the  theory  of  integral  functions. 

We  have  laid  down  that  the  coefficients  of  ah  integral  function 
are  independent  of  the  variables,  and  therefore  are  not  altered  by 
giving  any  special  values  to  the  variables.  If,  therefore,  on  cither 
side  of  any  algebraic  identity  involving  integral  functions  we  determine 
the  coefficients,  either  by  general  considerations  regarding  the  forms  of 
the  functions  involved,  or  by  considering  particular  cases  of  the  identity, 
then  these  coefficients  are  determined  once  for  all.  This  has  (not  very 
happily,  it  must  be  confessed)  been  called  the  principle  of  inde- 
terminate coefficients.  As  applied  to  integral  functions  it  results 
from  the  most  elementary  principles,  as  we  have  seen  ;  when 
infinite  series  are  concerned,  its  use  requires  further  examination 
(see  the  chapter  on  Series  in  the  second  part  of  this  work). 

The  following  are  examples  : — 

(x  +  y)2  =  (x  +  y)(x  +  y),  being  the  product  of  two  homogeneous 
symmetrical  functions  of  x  and  y  of  the   1st  degree,  will  be  a 
homogeneous  symmetrical  integral  function  of  the  2nd  degree  ; 
therefore  (x  +  yf  =  Ax2  +  Bxy  +  Ay2  (1). 

"We  have  to  determine  the  coefficients  A  and  B. 

Since  the  identity  holds  for  all  values  of  x  and  y,  it  must 
hold  when  x  =  1  and  y  =  0,  therefore 

(1  +0)2  =  A12  +  B1  xO  +  AO2, 
1=A. 
We  now  have         (x  +  y)2  =  x2  +  Bxy  +  y2 ; 
this  must  hold  when       x  =  1  and  y  -  -  1, 
therefore  (1  -  1)8=  1 +B.1.(- 1)  +  1, 

that  is,  0  =  2  -  B, 

whence  B  =  2. 

Thus  finally  (x  +  y)2  =  x2  +  2xy  +  y2. 


80  INDETERMINATE  COEFFICIENTS  CHAr. 

This  method  of  working  may  seem  at  first  sight  somewhat  startling,  but 
a  little  reflection  will  convince  the  learner  of  its  soundness.  We  know,  by 
the  principles  of  homogeneity  and  symmetry,  that  a  general  identity  of  the 
form  (1)  exists,  and  we  determine  the  coefficients  l>y  the  consideration  that 
the  identity  must  hold  in  any  particular  case.  The  student  will  naturally  ask 
how  he  is  to  be  guided  in  selecting  the  particular  cases  in  question,  and 
whether  it  is  material  what  cases  he  selects.  The  answer  to  the  latter  part  of 
this  question  is  that,  except  as  to  the  labour  involved  in  the  calculation,  the 
choice  of  cases  is  immaterial,  provided  enough  are  taken  to  determine  all  the 
coefficients.  This  determination  will  in  general  depend  upon  the  solution  of 
a  system  of  simultaneous  equations  of  the  1st  degree,  whose  number  is  the 
number  of  the  coefficients  to  be  determined.  (See  below,  chap,  xvi.)  So  fat- 
as  possible,  the  particular  cases  should  be  chosen  so  as  to  give  equations  each 
of  which  contains  only  one  of  the  coefficients,  so  that  we  can  determine  them 
one  at  a  time  as  was  done  above. 

The  student  who  is  already  familiar  with  the  solution  of  simultaneous 
equations  of  the  1st  degree  may  work  out  the  values  of  the  coefficients  by 
means  of  particular  cases  taken  at  random.  Thus,  for  example,  putting  x=2, 
y  =  3,  and  x  =  l,  y  =  i  successively  in  (1)  above,  we  get  the  equations 

25  =  13A  +  6B, 
25  =  17A  +  4B, 

which,  when  solved  in  the  usual  way,  give  A  =  1  and  B  =  2,  as  before. 

We  give  one  more  example  of  this  important  process  : — 
By  the  principles  of  homogeneity  and  symmetry  we  must  have 
(x  +  y  +  z)  (x2  +  y2  +  z-  -  yz  -  zx  -  xy) 
=  A(.r>  +  y3  +  z3)  +  B(yz2  +  y2z  +  zx2  +  z2x  +  xy2  +  x*y)  +  Cyxz. 
Putting  sc=l,  y  =  0,  z  —  0,  we  get  1=A. 
Using  this  value  of  A,  and  putting  x=\,  y  =  l,  z  =  0,  we  get 

2xl  =  2  +  Bx2, 
that  is,  2  =  2  +  Bx2, 

therefore  2B  =  0, 

and  therefore  B  =  0. 

Using  these  values  of  A  and  B,  and  putting  x=1,  y=l,  2  =  1,  we  get 

3xO=3  +  C, 
that  is,  0  =  3  +  C, 

therefore  C  =  -  3  ; 

and  we  get  finally 

(x  +  y  +  z)  (x2  +  y2  +  z2-yz-zx-xij)  =  x3  +  if  +  zz-3xyz  (2), 

as  in  §  23. 

§  25.]  Reference  Table  of  Identities. — Most  of  the  results  given 
below  will  be  found  useful  by  the  student  in  his  occasional  calcu- 
lations of  algebraical  identities.     Some  examples  of  their  use 


TABLE  OF  IDENTITIES 


81 


have  already  been  given,  and  others  will  be  found  among  the 

Exercises    in   this  chapter.      Such  of  the   results   as   have  not 

already  been   demonstrated    above   may  be   established  by  the 
student  himself  as  an  exercise. 


(x  +  a)  (x  +  b)  =  x"  +  (a  +  b)x  +  ab  ; 
(x  +  a)  (x  +  b)  (x  +  c)  =  x3  +  (a  +  b  +  c)x* 

+  (be  +  ca  +  ab)x  +  abc  ; 
and  generally 
(x  +  «,) {x  +  a2)  ...(/•  +  an)  =  xn  +  P,.^1"1  +  P^"2 

+  .  .  .  +  Pn_^  +  Pw(see  §9). 

(x  ±  yf  -  x2  ±  2xy  +  if  ; 
(x  ±  yf  =  x3  ±  3x2y  +  Zxif  ±  if  j 
&c. ; 

the  numerical  coefficients  being  taken  from  the  following 
table  of  binomial  coefficients  : — 


> 


Hi-) 


Tower. 

Coefficients. 

1 

1 

1 

o 

1 

2     1 

3 

1 

3    3 

1 

4 

1 

4    6 

4 

1 

5 

1 

5  10 

10 

5 

1 

6 

1 

6  15 

20 

15 

6       1 

1 

7  21 

35 

35 

21       7       1 

8 

1 

8  28 

56 

70 

56    28      8       1 

9 

1 

9  36 

84  126  126    84    36       9 

1 

10 

1 

10  45  120 

210 

252  210  120     15 

10    1 

11 

1 

11  55 

165 

330  462  462  330  165 

55  11     1 

12 

1  12  G6 

220  495 

792  924  792  495 

220  66  12  1 

&c. 

Mil.) 


*  This  table  first  occurs  in  the  Arithmctica  Integra  of  Stifel  (1544),  in 
connection  with  the  extraction  of  roots.  It  does  not  appear  tli.it  he  was 
aware  of  the  application  to  the  expansion  of  a  binomial  The  table  was  dis- 
cussed and  much  used  by  Pascal,  and  now  goes  by  the  name  of  Pascal's 
Arithmetical  Triangle.  The  factorial  formula'  for  the  binomial  coefficients  (see 
the  second  part  of  this  work)  were  discovered  by  Newton. 

VOL.  I  G 


82 


TABLE  OF  IDENTITIES 


-  1in 


(x  ±  yf  t  %  =  (a  t  y)2- 
(x  +  y)  (x  -y)  =  x2-y2; 
(x  ±  y)  (x2  T  sqf  +  y2)  =  x3  ±  /  ; 
and  generally 

(x  _  y)  (x«  -i  +  xn~ h)  + .  .  .  +  «yn  ~ 2  +  f  ~ l)  =  a* 
(z  +  y)  (scn  -1  -  »n- 2y  + .  .  .  t  -™/n  " 2  ±  yn -1)  =  aJ«  ±  y» 
upper  or  lower  sign  according  as  w  is  odd  or  even. 

(x*  +  f)<f  +  y'2)  =  {xx'  T  yy')3  +  (^  ±  FT; 

(.<"  -  *■)(*"  -  2/'2)  =  (a*  ±  ^7  ~  (*y  ±  3*Ti 

(/  +  y2  +  «■)(*/■  +  y"  +  *'2)  =  ixx'  +  yy'  +  zz')2  +  (yz'  -  y'z)2 

+  (zx'-z'x)2  +  (xy'-x'y)2; 

(x2  +  y2  +  z2  +  u2)(x'2  +  y'2  +  z"  +  u'2)  =  (xx'  +  yy'  +  zz'  +  uu')2 

+  (xy  -  yx'  +  zu'  -  uz')2 
+  (xz'  -  yu'  -  zx'  +  uy')2 
+  (xu'  +  yz'  -  zy'  -  ux')2. 

(x2  +  xy  +  f)  (x2  -  xy  +  y2)  =  x*  +  x2y2  +  y\ 

(a  +  l)  +  c  +  d)2  =  a2  +  b2  +  c2  +  d2  +  2ab  +  2ac  +  2ad 
+  2bc  +  2bd  +  2cd  ; 
and  generally 
(al  +  a2  +  .   .  .  +  an)2  =  sixm  of  squares  of  ati  a2,  .  .  .,  a, 

+  twice  sum  of  all  partial  products  two  and  two. 

(a  +  b  +  c)3  =  a3  +  b3  +  c3  +  U2c  +  3bc2  +  Zc'a  +  Sea*  +  3a  b 
+  Sab2  +  Gabc 
=  a3  +  b3  +  c3  +  36c  (6  +  c)  +  3ca(c  +  a) 
+  Sab  (a  +  b)  +  Saba 

(a  +  b  +  c)  (a2  +  b2  +  c2-bc-  ca  -  ab)  -  a3  +  b3  +  c3  -  3abc 

(b  -  c)  (c  -  a)  (a-b)=  -  a\b  -  c)  -  b\c  -  a)  -  c\a  -  b), 
=  a(b2  -  c2)  +  b(c2  -  a2)  +  c(a2  -  b% 
-  -  bc(b  -c)-  ca(c  -  a)  -  ab(a  -  b), 
=  +  be2  -  b2c  +  ca2  -  c2a  +  ab2  -  a2b. 


CHAP. 


(III.) 


MIV.) 


Uy.y 


(VI.) 


I  (VII.) 


(VIII.) 
(IX.) 


*  These  identities  furnish,  inter  alia,  proofs  of  a  series  of  propositions  in 
the  theory  of  numbers,  of  which  the  following  is  typical :— If  each  of  two 
integers  he  the  ram  of  two  squares,  their  product  can  he  exhibited  in  two  ways 
as  the  sum  of  two  integral  squares. 


iv  EXERCISES  VIII  83 

(b  +  c)(c  +  a)(a  +  b)  =  as(b  +  c)  +  b2(c  +  a)  +  c2(a  +  b)  +  2abc,  \ 

=  bc(b  +  c)  +  ca(c  +  a)  +  ab(a  +  b)  +  2abc,  I  (XI.) 
=  be2  +  b2c  +  ca2  +  c2a  +  ab2  +  ab  +  2dbc.   J 

(a  +  b  +  c)  (a2  +  b2  +  c2)  =  bc(b  +  c)  +  ca(c  +  a)  +  ab(a  +  b)        \  , 

+  a3  +  b3  +  c\  j(XIL) 

(a  +  b  +  c)  (Lc  +  ca  +  ab)  =  a2(b  +  c)  +  b2(c  +  a)  +  c2(a  +  b)       \  /VTTT 

+  3abc,  J(X111) 

(b  +  c-  a)  (c  +  a-  b)  (a  +  b  -  c)  =  a2(b  +  c)  +  b2(c  +•«)  ( 

+  c\a  +  b)-a3-b3-c3-  2abc,    I  (  ' 

(a  +  6  +  c)(  -  a  +  6  +  c)(a  -  b  +  c)(a  +  b  -  c)  =  2b2c2  +  2c2a2   )  „ 

+  2a*b*-at-bi-c*.  /  (XV.)- 

(6  -  c)  +  (c  -  a)  +  (a  -  b)  =  0  ;  \ 

a(b  -c)+  b(c  -a)  +  c(a  -  b)  =  0 ;  V  (XVI.) 

(6  +  c)(fi  -  c)  +  (c  +  a)(c  -a)  +  (a  +  b) (a  -b)  =  0.  ) 

Exercises  VIII. 

(1.)  Write  down  the  most  general  rational  integral  symmetrical  function 
of  x,  y,  z,  u  of  the  3rd  degree. 

(2.)  Distribute  the  product  {x"y  +  y"z  +  z"x)  (xy'  +  yz^  +  zx2).  Show  that 
it  is  symmetrical ;  count  the  number  of  types  into  which  its  terms  fall  ;  and 
state  how  many  of  the  types  corresponding  to  its  degree  are  missing. 

(3.)  Construct  a  homogeneous  integral  function  of  x  and  y  of  the  1st 
degree  which  shall  vanish  when  x  =  y,  and  become  1  when  x  =5  and  ?/  =  2. 

(4.)  Construct  an  integral  function  of  x  and  y  of  the  1st  degree  which 
shall  vanish  when  x  =  x',  y  =  y',  and  also  when  x—x",  y  =  y". 

(5.)  Construct  a  homogeneous  integral  function  of  x  and  y  of  the  2nd 
degree  which  shall  vanish  when  x  =  x',  y  =  y',  and  also  when  x  —  x",  y  =  y",  and 
fchall  become  1  when  aj=l,  y  =  l. 

(6.)  If  A(a:-3)(iB-5)  +  B(aJ-5)(aj-7)  +  C(a!-7)(a!-3)=8iB-120  for  all 
values  of  x,  determine  the  coefficients  A,  B,  C. 

(7.)  Show  that  5.r2  +  19a;+18  can  be  put  into  the  form 

l{x  -  2)  {x  -  3)  +  m(x  -  3)  (x  -  1)  +  n{x  -  1 )  (x  -  2)  ; 
and  find  I,  m,  n. 

(8.)  Assuming  that  {x  -  1)  (x  -  2)  (a;-  3)  can  be  put  into  the  form 
l(x-l)  {x  +2){x  +  3)  +  vi{x-2)(x  +  B)(x  +  l)  +  n(x  -  3)  (*+ 1)  (»+  2), 
determine  the  numbers  7,  m,  n. 

*  Important  in  connection  with  Hero's  formula  for  the  area  of  a  plane] 
triangle. 


84  EXERCISES  VIII  chap,  iv 

(9.)  Find  a  rational  integral  function  of  x  of  the  3rd  degree  which  shall 
have  the  values  P,  Q,  R,  S  when  x  =  a,  x=b,  x  =  c,  x  =  d  respectively. 
(10.)  Find  the  coefficients  of  y-z  and  yz-  in  the  expansion  of 

(ax  +  by  +  cz)  (a-x  4  b-y  4  c2z)  (a3x  4  b3y  4  <?z). 
(11.)  Expand  and  simplify  2(</2  +  z2  -  x2)  (y  +  z  -  x). 

Trove  the  following  identities  :  — 

(12.)  (ad  +  bc)2  +  (a  +  b  +  c-d)(a  +  b-c  +  d)(b  +  d)(b-d)  =  (b2-d2  +  ab  +  cd)2. 
*(13.)  2(b2  +  c2-a2  +  bc  +  ca  +  ab)2(c2-b2)  =  4(b2-c2)(c2-a2)(a2-b2). 
(14. )  2(ca  -  b2)  (ab  -  c2)  =  (26c)  (26c  -  2a2). 
(15.)  2(&c'  -  b'c)  (be"  -  b"c)  =  2a22rt'«"  -  2aa'2W. 
(16.)  31%  4  z)  -  62?/~  =  2a-(2.c-  1)  (2jj-  2)  -  Saj(a-1)  (a!-2). 
(17.)  Z(b2  +  c2-a"-)/2bc=(ip12>-2-lh3-fy3)/ty3,    where  Pl  =  -  2a,  p,  =  Zbc, 
p3-  -abc. 

(18. )  1%  4 ;)2 4  2x2y2z2  -  2x*(y  4  z)2=  2(2r)3. 

(19.)  S(a:  +y-z){(y- z)2 -(z-x)(x- y)\  =  2a*- Zxyz. 

(20. )  n(a± b±c±d)  =  2a8  -  42a662 4  62«4i4 4  42aW  -  40a262c2rf2. 

(21.)  Show  that 

(x3  4  y3  4  s3  -  3ays)a  =  X3  4  Y3  4  Z3  -  3X YZ,  where  X  =  x2  4  2y;,  &c. ; 
also  that 

CZx3  -  3xyz)  (2a;'3  -  2>x'y'z)  =  S(a»'  4  ysf*  4  ?/~~)3  -  3II(»/  4  yz'  4  y'z). 
(These  identities  have  an  important  meaning  in  the  theory  of  numbers. ) 
(22.)  Show  that,  if  n  be  a  positive  integer,  then 

l-h+h~.   ■  .-!(»even)  =  2('^L  +  -L+.   .   .+!-)■ 

1-i+J-.  .  .  +  l(»odd)=2/-l-+_l_+.  .  .+1 

n  \n  +  l     n  +  3  2n 

(Blissard). 

*  In  this  example,  and  in  others  of  a  similar  kind,  2  is  not  used  in  its 
strict  sense,  but  refers  only  to  cyclical  interchanges  of  a,  b,  c;  that  is,  to 
interchanges  in  which  a,  b,  c  pass  into  b,  c,  a  respectively,  or  into  c,  a,  b 
respectively.  Thus,  2cr(&-c)  is,  strictly  speaking,  =0;  but,  if  2  be  used  in 
the  present  sense,  it  is  a2(b  -c)+  b2(c  -a)+  c2(a  -  b). 


CHAPTER    V. 

Division  of  Integral  Functions— Transformation  of 

Quotients. 

§  1.]  The  operations  of  this  chapter  are  for  the  most  part 
inverse  to  those  of  last.  Thus,  A  and  D  being  any  integral 
functions  of  one  variable  x*  and  Q  a  function  such  that 
D  x  Q  =  A,  then  Q  is  called  the  quotient  of  A  by  D  ;  A  is  called 
the  dividend  and  D  the  divisor.     We  symbolise  Q  by  the  nota- 

tion  A  -7-  D,  A/D,  or  =-,  as  explained  in  chap.  i. 

The  operation  of  finding  Q  is  called  division,  but  we  prefer 
that  the  student  should  class  the  operations  of  this  chapter  under 
the  title  of  transformation  of  quotients. 

A  and  D  being  both  integral  functions,  Q  will  be  a  rational 
function  of  x,  but  will  not  necessarily  be  an  integral  function. 

When  the  quotient  can  he  transformed  so  as  to  become  integral,  A 
is  said  to  be  exactly  divisible  by  D. 

IFhen  the  quotient  cannot  be  so  transformed,  the  quotient  is  said 
to  be  fractional  or  essentially  fractional. 

It  is  of  course  obvious  that  an  essentially  integral  function  cannot 
be  equal,  in  the  identical  sense,  to  an  essentially  fractional  function. 

§  2.]  When  the  quotient  is  integral,  its  degree  is  the  excess  of  the 
degree  of  the  dividend  over  tlie  degree  of  the  divisor.     For,  denoting 

*  For  reasons  partly  explained  below,  the  student  must  be  cautious  in 
applying  many  of  the  propositions  of  this  chapter  to  functions  of  more  vari- 
ables than  one  ;  or  at  least  in  such  cases  he  must  select  one  of  the  variables 
at  a  time,  and  think  of  it  as  the  variable  for  the  purposes  of  this  chapter. 


86  THEOREM  REGARDING  DIVISIBILITY  chap. 

the  degrees  of  the  functions  represented  bj7  the  various  letters 
by  suffixes,  we  have 

therefore,  by  chap,  iv.,  §  7,  m  =p  +  n,  that  is,  p  =  m  -  n. 

§  3.]  If  the  degree  of  the  dividend  be  less  than  that  of  the  divisor, 
the  quotient  is  essentially  fractional.  For,  m  being  <??,  suppose,  if 
possible,  that  the  cpiotient  is  integral,  of  degree  p  say,  then 

therefore  m=p  +  n;  but  p  cannot  be  less  than  0  by  our  hypo- 
thesis, and  m  is  already  less  than  n,  hence  the  cpiotient  cannot 
be  integral,  that  is,  it  must  be  fractional. 

§  4.]  If  A,   D,   Q,  R   be   all   integral  functions,   and  if  A  = 
QD  +  R,  then  R  will  be  exactly  divisible  by  D  or  not  according  as  A 
is  exactly  divisible  by  D  or  not. 

For,  since  A  =  QD  +  R, 

A  _  QD  +  R  R 

therefore  ~  =  j-  -  Q. 

Now,  if  A  be  exactly  divisible  by  D,  A/D  will  be  integral,  and 
A/D  -  Q  will  be  integral,  that  is,  R/D  will  be  integral,  that  is,  R 
will  be  exactly  divisible  by  D. 

Again,  if  A  be  not  exactly  divisible  by  D,  A/D  will  be 
fractional.  Hence  R/D  must  be  fractional,  for,  if  it  were 
integral,  Q  +  R/D  would  be  integral,  that  is,  A/D  would  be  in- 
tegral, which  is  contrary  to  hypothesis. 

INTEGRAL    QUOTIENT    AND    REMAINDER. 

§  5.]  The  following  is  the  fundamental  theorem  in  the 
transformation  of  quotients. 

A^  and  Dn  being  integral  functions  of  the  degrees  m  and  n  respect- 
ively, we  can  always  transform  the  quotient  A7n/D„  as  follows . — 

Affl  _  p         ^i 

XJn  XJn 


V  INTEGRAL  QUOTIENT  AND  REMAINDER  87 

where  PTO_n  is  an  integral  function  of  degree  m  -  n,  and  R  (if  it  do 
not  vanish)  an  integral  function  whose  degree  is  at  most  n-  1. 

This  transformation  is  effected  by  a  series  of  steps.     "We  shall 
first  work  out  a  particular  case,  and  then  give  the  general  proof. 

Let  Ah  =  8a*  +  8*-5  -  20a-4  +  40*3  -  50*2  +  30*  -10, 

D4  =  2*4  +  3*3-4*2  +  6*-8, 

multiply  the  divisor  D4  by  the  quotient  of  the  highest  term  of  the  dividend 
by  the  highest  term  of  the  divisor  (that  is,  multiply  D4  by  8*6/2*4  =  4*2),  and 
subtract  the  result  from  the  dividend  A6.     "We  have 

A6  =  8*fi  +    8*5  -  20k4  +  40*3  -  5  Ox-  +  30*  -  1 0 
4*2D4  =  Sxe  + 1 2*5  -  1 6*4  +  24.C3  -  32a? 


A6-4*'-D4  =       -   4ar»-    4*4  +  16*3-  18a;3 +  30*-  10 
=  A3  say  ; 
therefore  A6  =  4*2D4  +  A5  (1). 

Repeat  the  same  process  with  the  residue  A5  in  place  of  Ae,  and  we  have 

As=  -  4a*  -  is*  + 16*3  -  18*2  +  30*  -  10 
-  2*D4  =  -  4*5  -  6*4  +    8*'  -  1 2.7r  + 1  Qx 


A3  +  2*D4  =  2x*+   8X3-    Qx-  +  14*  -10 

=  A4  say; 
therefore  A5  =  -  2*D4  +  A4  (2). 

And  again  with  A4, 

A4  =  2x*  +  8x*  -  6*2  +  14*  -  10 
1  x  D4  =  2**  +  3*"  -  4*2  +   6*  -    8 


A4-D4=  5*3-2*2+    8*-    2 

=  A3 say  ; 
therefore  A4=D4  +  A3  (3). 

Here  the  process  must  stop,  unless  we  agree  to  admit  fractional  multi- 
pliers of  D4  ;  for  the  quotient  of  the  highest  term  of  A:!  by  the  highest  term  of 
D4  is  5*3/2*4,  that  is,  f/*,  which  is  a  fractional  function  of  *.  Such  a  con- 
tinuation of  the  process  does  not  concern  us  now,  but  will  be  considered  below. 

Meantime,  from  (1)  we  have 

A6=4*-D4  +  A5  (4)  • 

and,  using  (2)  to  replace  A3, 

A6  =  4*-D4  -  2*D4  +  A4  (5 )  ; 

and  finally,  using  (3), 

A6  =  4*2D4-2*D4  +  D4  +  A3, 

=  (4*2-2*  +  l)D4  +  A3  (6). 

Hence  A6=J4*2-2a;  +  l)D4  +  A, 

D4  D4 

=  4*2-2*  +  l  +  14>' ; 
•U4 


88  INTEGRAL  QUOTIENT  AND  REMAINDER  CHAP. 

or,  replacing  the  capital  letters  by  the  functions  they  represent, 

8,>;6  +  8a;5  -  20.r4  +  40.T3  -  50.r2  +  30.r  -  10 

2x*  +  3x:i  -  ix-  +  6x  -  8 

.  ,  5,r3-2x2  +  8a;-2  ... 

=  ^-2*+l+^  +  8a,_4a.+  fla,_3  (7). 

Since  6-4  =  2,  it  will  be  seen  that  we  hare  established  the  above  theorem 
for  this  special  case.  It  so  happens  that  the  degrees  of  the  residues  A5,  A4, 
A3  diminish  at  each  operation  by  unity  only  ;  but  the  student  will  easily  see 
that  the  diminution  might  happen  to  be  more  rapid  ;  and,  in  particular,  that 
the  degree  of  the  first  residue  whose  degree  falls  Tinder  that  of  the  divisor 
might  happen  to  be  less  than  the  degree  of  the  divisor  by  more  than  unity. 
But  none  of  these  possibilities  will  affect  the  proof  in  any  way. 

We  shall  return  to  the  present  case  immediately,  but  in  the  first  place  we 
may  give  a  general  form  to  the  proof  of  the  important  proposition  which  we 
are  illustrating. 

§  6.]  Let      Am  =  2Vm  +jalxm~1  +  p2xm~2  +  &c- 1 
Dn  —-qvxn  +  q^1'1  +  qaxn~2  +  &c. 

Multiplying  Dn  by  the  quotient  p$?njq0xn,  that  is,  by  (p0/qo)xm~n> 
and  subtracting  the  result  from  A,„,,  we  get 

=  Am_,  say, 
whence,  denoting  p0/q0  by  r  for  shortness,  we  get 

-A-m  =  tx        Dn  +  Am  _ !  ( I ). 

Treating  Am_t  in  the  same  way,  we  get 

Am_,  =  SX  Dn  +  Am_2  {-')• 

And  so  on,  so  long  as  the  degree  of  the  residue  is  not  less 
than  n,  the  last  such  equation  obtained  being — 

A„  =  m>D„  +  K  (3), 

where  E   is  of  degree   n  -  1   at  the   utmost.     Using  all   these 
equations  in  succession  we  get 

_  (rtfn-n  +  stfm-n-1  +   .    .    .   +  w)J)n  +  R  ; 

whence,    dividing   both   sides  by  Dn,   and   distributing  on   the 
right, 


A     _  -?-0  rm  -  »  T) 


v  THE  ORDINARY  DIVISION  TRANSFORMATION   UNIQUE  89 

A  R 

-^  =  rsm  - "  +  sxm  -n~1  +  .  .  .+«;+'=-, 

which,  if  we  bear  in  mind  the  character  of  R,  gives  a  general 
proof  of  the  proposition  in  cpiestion. 

§  7.]  We  have  shown  that  the  transformation  of  §  5  can 
always  be  effected  in  a  particular  way,  but  this  gives  no  assur- 
ance that  the  final  result  will  always  be  the  same.  The  proof 
that  this  really  is  so  is  furnished  by  the  following  proposition: — 

The  quotient  A/D  of  two  integral  functions  can  be  put  into  the 
form  P  +  R/D,  where  P  and  R  are  integral  functions  and  the  degree 
of  R  is  less  than  that  of  D,  in  one  way  only. 

If  possible  let 

1  A       TV       R' 

and  D  =  P+D' 

where  P,  R  and  P',  R'  both  satisfy  the  above  requirements  ; 

then  p  +  ?  =  P'  +  ^; 

D  D  ' 

subtracting  P'  +  =r  from  both  sides,  we  have 

R'     R  m 
r     r  ~  1 )      D  ' 

whence  — -  =  P  -  P'. 

D 

Now,  since  the  degrees  R  and  R  are  both  less  than  the  degree 
of  D,  it  follows  that  the  degree  of  R'  -  R  is  less  than  that  of  D. 
Therefore,  by  §  3,  the  left-hand  side,  (R'  -  R)/D,  is  essentially 
fractional,  and  cannot  be  equal  to  the  right,  which  is  integral, 
unless  R'  -  R  -  0,  in  which  case  we  must  also  have  P  -  P'  =  0, 
that  is,  R  =  R',  and  P  =  P\ 

§  8.]  The  two  propositions  of  §§  5,  7  give  a  peculiar  import- 
ance to  the  functions  P  and  R,  of  which  the  following  definition 
may  now  legitimately  be  given  : — 

If  the  quotient  A/D  be  transformed  into  V  +  R/D,   P  and  R  being 


90  CONDITIONS  FOR  EXACT  DIVISIBILITY  chap. 

integral  and  R  of  degree  less  than  D,  P  is  called  the  integral  quotient, 
and  R  the  remainder  of  A  when  divided  by  D. 

§  9.]  We  can  now  express  the  condition  that  one  integral 
function  A  may  be  exactly  divisible  by  another  D.  For,  if  E  be 
the  remainder,  as  above  denned,  we  have,  P  being  an  integral 
function, — 

^-P  +  ? 

whence,  subtracting  P  from  both  sides, 


-  Ax* - 

-  Ax*  - 

Ax*  +  16a;3-  18a;2  +  30a;  -10 
6a;4  +    8a;3- 12a;2  +  16a; 

2x*  +  8/-  6a;2  +  I  Ax-  10 
2»*  +    3a;3-    4a-2  +    63-    8 

2x4  +  Sx3  -  4/  +  6.r  -  8 


4a:2  -  2x  +  1 


A  B 

D  D 

Now,  if  A  be  exactly  divisible  by  D,  A/D  will  be  integral,  and 
therefore  A/D  -  P  will  be  integral.  Hence  R/D  must  be  integral ; 
but,  since  the  degree  of  R  is  less  than  that  of  D,  this  cannot  be 
the  case  unless  R  vanish  identically. 

The  necessary  and  sufficient  condition  for  exact  divisibility  is  there- 
fore that  the  remainder  shall  vanish. 

When  the  divisor  is  of  the  nth  degree,  the  remainder  will  in 
general  be  of  the  (n  -  l)th  degree,  and  will  contain  n  coefficients, 
every  one  of  which  must  vanish  if  the  remainder  vanish.  In 
general,  therefore,  when  the  divisor  is  of  the  nth  degree,  n  conditions 
are  necessary  to  secure  exact  divisibility. 

§  10.]  Having  examined  the  exact  meaning  and  use  of  the 
integral  quotient  and  remainder,  we  proceed  to  explain  a  con- 
venient method  for  calculating  them.  The  process  is  simply  a 
succinct  arrangement  of  the  calculation  of  §§  5,  G.  It  will  be 
sufficient  to  take  the  particular  case  of  §  5. 

The  work  may  be  arranged  as  follows  : — 
8x°  +    8x*  -  20a;4  +  40a;3  -  5  Ox2  +  3  Ox  -  10 
8a;6  +  1 2/- 16a:4  +  24a;3 -32a'2 


5x3-    2x2+    8x-    2 


v  DETACHED  COEFFICIENTS  91 

Or,  observing  that  the  term  -  10  is  not  waited  till  the  last 
operation,  and  therefore  need  not  be  taken  down  from  the  upper 
line  until  that  stage  is  reached,  and  observing  further  that  the 
method  of  detached  coefficients  is  clearly  applicable  here  just  as 
in  multiplication,  we  may  arrange  the  whole  thus  : — 

8+    8  -  20  +  40  -  50  +  30  -  10  |  2  +  3  -  4  +  6  -  6 

4-2  +  1 


8  +  12-16  +  24-32 

I 

-    4-    4  +  16-18  +  30 

-    4-    6  +    8-12  +  16 

2+    8-    6  +  14- 

10 

2+    3-    4+    6- 

8 

5-    2+8-    2 
Therefore,  Integral  quotient  =  4/  -  2x  +  1  \ 

Remainder  =  5x3  -  2x2  +  8x  -  2. 

The  process  may  be  verbally  described  as  follows  : — 

Arrange  both  dividend  and  divisor  according  to  descending  powers 
of  x,  filling  in  missing  powers  with  zero  coefficients.  Find  the  quotient 
of  the  highest  term  of  the  dividend  by  the  highest  term  of  the  divisor  ; 
the  result  is  the  highest  term  of  the  "  integral  quotient." 

Multiply  the  divisor  by  the  term  thus  obtained,  and  subtract  the 
result  from  the  dividend,  taking  down  only  one  term  to  the  right  beyond 
those  affected  by  the  subtraction ;  the  result  thus  obtained  will  be  less  in 
degree  than  the  dividend  by  one  at  least.  Divide  the  highest  term  of 
this  residt  by  the  highest  of  the  divisor  ;  the  result  is  the  second  term 
of  the  "  integral  quotient." 

Multiply  the  divisor  by  the  new  term  just  obtained,  and  subtract, 
&c,  as  before. 

The  process  continues  until  the  result  after  the  last  subtraction  is 
less  in  degree  than  the  divisor;  this  last  result  is  the  remainder  as 
above  defined. 

§  11.]  The  following  are  some  examples  of  the  use  of  the 
"  long  rule  "  for  division. 


92 


Example  1. 


EXAMPLES 


i.     19  „      5         l_ 

I         36         36r  +  36 

1  _  5    i    19  _     6      i      1 


,x---a;  +  4 


1-i  +  l 


5 

3ff 
"A 

i 

•B 

1 
V 

—     1-4-1 

J1"} 


CHAP. 


0   +  0 

The  remainder  vanishes,  therefore  the  division  is  exact,  and  the  quotient  is 


Example  2. 

l+p         +q 
I -a 


{x3+px2  +  qx  +  r)-i-[x-a). 
+r  1-a 


1  +  (a  +p)  +  {a2  +  ap  +  q) 


{a+p)  +  q 
(a+p)-{a2  +  ap) 

{a?  +  ap  +  q)  +  r 

(a2  +  ap  +  q)-  (a3  +  a2p  +  aq) 

(a3  +  a2p  +  aq  +  r) 
Hence  the  integral  quotient  is 

x2  +  (a+p)x  +  (a2  +  ap  +  q)  ; 
and  the  remainder  is 

a3  +  a2p  +  aq  +  r. 

The  student  should  observe  the  use  of  brackets  throughout  to  preserve  the 
identity  of  the  coefficients. 

Example  3. 

(re4  -  2>a3b  +  6a2b-  -  Zab3  + 1*)  4-  (a2  -ab  +  b2). 

1st.  Let  us  consider  a  as  the  variable.  Since  the  expressions  are  homo- 
geneous, we  may  omit  the  powers  of  b  in  the  coefficients,  and  use  the  numbers 
merely. 

1-3  +  6-3  +  1  I  1-1+1 


1-1  +  1 


-2+5-3 

-2+2-2 


1-2  +  3 
a2-2ab  +  Sb2 


3-1  +  1 
3-3  +  3 

"  2-2 
2ab3  -  2b* 


BINOMIAL  DIVISOR 


93 


whence 


ii-3a*b  +  6cr-b--Sab*  +  bi 


=  a?-2ab  +  M-  + 


2a't?  -  2b* 


a2-ab  +  b2' 

We  must  then  arrange  according 


a2-ab  +  b'- 

'2nd.  Let  us  consider  b  as  the  variable, 
to  descending  powers  of  b,  thus— 

(64  -  3ab3  +  6a-b°-  -  3a?b  +  a4)  +-  {b-  -ab  +  a-). 
Detach  the  coefficients,  and  proceed  as  before.  It  happens  in  this  particular 
case  that  the  mere  numerical  part  of  the  work  is  exactly  the  same  as  before  ; 
the  only  difference  is  in  the  insertion  of  the  powers  of  a  and  b  at  the  end. 
Thus  the  integral  quotient  is  b2-2ba  +  3a",  and  the  remainder  is  26a3  -2a4, 
whence 

— , ,      ,., =Za--2ab  +  b-  +  — — r. 

a2~ab  +  b1  a-  -  ab  +  b2 

§  12.]  The  process  of  long  division  may  be  still  further 
abbreviated  (after  expertness  and  accuracy  have  been  acquired) 
by  combining  the  operations  of  multiplying  the  divisor  and  sub- 
tracting. Then  only  the  successive  residues  need  be  written. 
Thus  contracted,  the  numerical  part  of  the  operations  of  Example 
3  in  last  paragraph  would  run  thus  : — 

1-3+6-3+1 1 1-1+1 
-2+5-3+i;i-2+3 
3-1  +  1 
2-2 


BINOMIAL    DIVISOR — REMAINDER   THEOREM. 

§  13.]  The  case  of  a  binomial  divisor  of  the  1st  degree  is  of 
special  importance.     Let  the  divisor  be  x  -  a,  and  the  dividend 


p^1  +  pxx 


n -i 


+  Pr 


,,«-2  + 


+  Pn-&+Pn- 


Then,  if  we  employ  the  method  of  detached  coefficients,  the 
calculation  runs  as  follows  : — 


P0+P1 

Po-Po«- 


+  Pa  + 


+  Pn-i+Pr. 


(P&+Pi)+F» 
(P&+Pi)-(Poa+Pi)a 


! 


+  (p<fl.+p1) 

+  (Po°-2+Pia+pJ 


(j><P+Pi*+P*)+pa 

(j><P+Pi*  +  Pi)  ~  (Po*  +pxo.+  pa)a 

(p0a  +  P,a   +  p,a  +  p3) 


94  RULES  FOR  COEFFICIENTS  OF  chap. 

The  integral  quotient  is  therefore 

pjF-l  +  {poa  +Pl)xn~*  +  {p/  +Pla  +pX'2  +  ••' 

The  law  of  formation  of  the  coefficients  is  evidently  as  follows: — 

The  first  is  the  first  coefficient  of  the  dividend  ; 

The  second  is  obtained  by  multiplying  its  predecessor  by  a  and 
adding  the  second  coefficient  of  the  dividend  ; 

The  third  by  multiplying  the  second  just  obtained  by  a  and  adding 
the  third  coefficient  of  the  dividend  ;  and  so  on. 

It  is  also  obvious  that  the  remainder,  xchich  in  the  present  case  is 
of  zero  degree  in  x  (that  is,  does  not  contain  x),  is  obtained  from  the 
last  coefficient  of  the  integral  quotient  by  multiplying  that  coefficient  by 
a  and  adding  the  last  coefficient  of  the  dividend. 

The  operations  in  any  numerical  instance  may  be  con- 
veniently arranged  as  follows  : — * 


Example  1. 


(2xi-Sx2  +  6x-4)  +  (x-2). 
2+0-3+    6-    4 
0  +  4  +  8  +  10  +  32 


2  +  4  +  5  +  16  +  28 

Integral  quotient  =  2a?  +  4a;2  +  5x  + 1 6  ; 
Remainder  =  28. 

The  figures  in  the  first  line  are  the  coefficients  of  the  dividend. 

The  first  coefficient  in  the  second  line  is  0. 

The  first  coefficient  in  the  third  line  results  from  the  addition  of  the  two 
ahove  it. 

The  second  figure  in  the  second  line  is  obtained  by  multiplying  the  first 
coefficient  in  the  third  line  by  2. 

The  second  figure  in  the  third  line  by  adding  the  two  over  it. 

And  so  on. 

Example  2. 

If  the  divisor  be  x  +  2,  we  have  only  to  observe  that  this  is  the  same  as 


*  The  student  should  observe  that  this  arrangement  of  the  calculation  of 
the  remainder  is  virtually  a  handy  method  for  calculating  the  value  of  an 
integral  function  of  x  for  any  particular  value  of  x,  for  28  is  2  x  24  -  3  x  23 
+  6x2-4,  that  is  to  say,  the  value  of  2x* -  Zx*  +  6x -  4  when  x-2  (see  §  14). 
This  method  is  often  used,  and  always  saves  arithmetic  when  some  of  the 
coefficients  are  negative  and  others  positive.  It  was  employed  by  Newton  ; 
see  Horsley's  edition,  vol.  i.  p.  270. 


v  DIVISOB,  AND  FOR  REMAINDER  95 

x-{-2);  and  we  see  that  the  proper  result  will  be  obtained  by  operating 
throughout  as  before,  using  -  2  for  our  multiplier  instead  of  +  2. 

(2a*  -  3a? + 6b -4) -Ha; +2) 

=  (2a,-4  -  3ar  +  6»  -  4)  -=-  (x  -  (  -  2)). 

2+0-3+   6-4 

0-4+8-10+8 


2-4  +  5-    4  +  4. 


Integral  quotient  =  1)?  -  Ax-  +  5x  -  4  ; 
Remainder  =4. 

Example  3. 

The  following  example  will  show  the  student  how  to  bring  the  case  of  any 
binomial  divisor  of  the  1st  degree  under  the  case  of  a;-  a. 

3-f  '  -  2X3  +  3x2  -  2x  +  3  _  3.x-4  -2j?  +  3 x2  -  2.v  +  3 
3a: +  2  ~  3(x  +  f) 

(  3b4 -2a;3 +  33? -2a; +  3  "1 

Transforming  now  the  quotient  inside  the  bracket  {  } ,  we  have 

3-2+  3-2+3 


0  —  0-1-    s    _  34    i    1 04 

S-iJ.n_58i.lS5 

I  ntegral  quotient  =  Sx3  -  4a?  +  ^-x  -  Af . 

Whence 

Remainder            —  y75-. 

3a:4- 

-2S5»+8a?-2a!+3        f          A-.it,     -  ,      W 

_te  +  2               =*t3a!      4x  +^x     ¥+«s-(-l 

185 

— ar*    ^x  +-5 -a.     #?+•>    ,  .>• 

Hence,  for  the  division  originally  proposed,  we  have — 

Integral  quotient  =a?-|a?  +  -^aj-  :];  ; 
Remainder  =  V\5-. 

The  process  employed  in  Examples  2  and  3  above  is  clearly 
applicable  in  general,  and  the  student  should  study  it  attentively 
as  an  instance  of  the  use  of  a  little  transformation  in  bringing 
cases  apparently  distinct  under  a  common  treatment. 

§  14.]  Reverting  to  the  general  result  of  last  section,  we  see 
that  the  remainder,  when  written  out  in  full,  is 

p0an  +_p1a"-1  +  .   .    .  +  £>„_!<_  +pn. 


96  REMAINDER  THEOREM  CHAP. 

Comparing  this  with  the  dividend 

IV'"  +  Pi*"  "    +  •    •    •  +  Pn  -  i x  +  Pn , 

we  have  the  following  "  remainder  theorem  " : — 

When  an  integral  function  of  x  is  divided  by  x  -  a,  the  remainder 
is  obtained  by  substituting  a  for  x  in  the  function  in  question. 

In  other  words,  the  remainder  is  the  same  function  of  a  as 
the  dividend  is  of  x. 

Partly  on  account  of  the  great  importance  of  this  theorem, 
partly  as  an  exercise  in  general  algebraical  reasoning,  we  give 
another  proof  of  it. 

Let  us,  for  shortness,  denote 

jj0x11  +  ptxn - l  +  .   .   ■+pn-1x+  pn  by  f(x), 

/'(a)  will  then,  naturally,  denote  the  result  of  substituting  a  for 
x  in  f(x),  that  is, 

p0on  +pla11-1  +  .  .   .  +!>„_, a  +pn. 

Let  x(-')  denote  the  integral  quotient,  and  R  the  remainder, 
when  f(x)  is  divided  by  x  -  a.  Then  x(x)  is  an  integral  function 
of  x  of  degree  n-l,  and  R  is  a  constant  (that  is,  is  independent 
of  ,»■),  and  we  have 

X- a      ^  X- a 

whence,  multiplying  by  x  -  a,  we  get  the  identity 

f(X)  =  (X  -  a)X(x)  +  R. 

Since  this  holds  for  all  values  of  x,  we  get,  putting  x  =  a 
throughout, 

/(a)  =  (a  -  a)X(a)  +  R, 

where  R  remains  the  same  as  before,  since  it  does  not  depend  on 
x,  and  therefore  is  not  altered  by  giving  any  particular  value 

to  .''. 

Since  x(«)  is  finite  if  a  be  finite,  (a  -  a)x(a)  =  0  x  x(«)  =  0  ; 
and  we  get  finally 

/(a)  =  R, 

which,  if  we  remember  the  meaning  of  /(a),  proves  the  "re- 
mainder theorem." 


v  FACTORISATION  BY  REMAINDER  THEOREM  97 

Cor.  1.   Since  x  +  a  -  x  -  (  -  a),  it  follows  that 
The  remainder,  when  an  integral  function  f(x)  is  divided  by 
X  +  a,  isf(-a). 

For  example,   the  remainder,  when  v4  -  2>x*  +  2a?  -  5x  +  6   is  divided   by 
as+10,  is  (-10)4-3(-10)3  +  2(-10)--5(-10)  +  6  =  13256. 

Cor.  2.  The  remainder,  when  an  integral  function  of  x,  f(x),  is 
divided  by  ax  +  b,  is  /(  -  bja). 

This  is  simply  the  generalisation  of  Example  3,  §  13,  above. 

By  substitution  we  may  considerably  extend  the  application 
of  the  remainder  theorem,  as  the  following  example  will  show: — 

Consider  pm(x")m  +pm-1(x» J"1-1  +  .  .  .  +Pi(x")+p0  and  xn  -  a".  Writing 
for  a  moment  £  in  place  of  xn,  and  a  in  place  of  a",  we  have  to  deal  with 
Pm$m  +pm-iZm~1  +  •  •  ■  +]h^+Po  and  £-<x.  Now  the  remainder,  when  the 
former  of  these  is  divided  by  the  latter,  is  pma"l+pm-iam-1+  .  .  .  +Pia  +  p0. 
Hence  the  remainder,  when  pm(x")m+pm-i{xn)m-1+  .  .  .  +piaf*+po  is  divided 
by  xn-an,  is  2}m(a")m+ pm-i(a»)m-1+  .  .  .  +pxan+2)o- 


APPLICATION    OF   REMAINDER   THEOREM    TO    THE    DECOMPOSITION 
OF   AN    INTEGRAL    FUNCTION    INTO    LINEAR    FACTORS. 

§  15.]  If  a„  a2,  .  .  . ,  ar  be  r  different  values  of  x,  for  which  the 
integral  function  of  the  nth  degree  f(x)  vanishes,  where  r  <  n,  then 
f{x)  -  (x  -  c^)  (x  -  Og)  .  . .  (x  -  a.r)cj>n_t(.r),  cf)n_r(x)  being  an  integral 
function  of  x  of  the  (n  -  r)th  degree. 

For,  since  the  remainder,  /(a,),  when  f(x)  is  divided  by  x  -  a„ 
vanishes,  therefore  f(x)  is  exactly  divisible  by  x  -  a„  and  we  have 

where  <£n_i(.>')  is  an  integral  function  of  x  of  the  (n  -  l)th  degree. 
Since  this  equation  subsists  for  all  values  of  x,  we  have 

/(a,)  =  (aa  -  a!)4>n-i(<h), 
that  is,  by  hypothesis,    0  =  (a.2  -  <*,)<£„_  ,(a2). 

Now,    since   a!  and   a2  are  different  by  hypothesis,  a.,  -  at  4=  0  ; 
therefore  <f>n-i(a2)  =  0. 

Hence,  <f>n-\(-1')  is  divisible  by  (x  -  a,), 
that  is,  </,„  _  v(x)  =  (x  -  a2)<f>n  _  .2(x) ; 

whence  f(x)  =  (x  -  at)  (x  -  a2)<j>n_2(x). 

VOL.  I  H 


98  FACTOKISATION  BY  MEANS  OF  chap. 

From  this  again, 

0  =/(a3)  =  (a3  ~  a0  (a3  ~  az)<£n_a(a3), 
which  gives,  since  an  a.2,  a3  are  all  unequal,  <$>n-2{a3)  =  0  ;  whence 
<£»-s(a)  =  (■'-'  -  a3)<£m-3(a)  J   so  that 

f(x)  =  (x  -  a,)  (x  -  os)  (a;  -  a3)<£w_3(.r). 

Proceeding  in  this  way  step  by  step,  we  finally  establish  the 
theorem  for  any  number  of  factors  not  exceeding  n. 

Cor.  1 .  If  an  integral  function  be  divisible  by  the  factors  x  -  a„ 
x  -  a2,  .  .  . ,  x  -  an  all  of  the  1st  degree,  and  all  different,  it  is 
divisible  by  their  product ;  and,  conversely,  if  it  is  divisible  by  the 
product  of  any  number  of  such  factors,  all  of  the  1st  degree  and  all 
different,  it  is  divisible  by  each  of  them  separately.  The  proof  of 
this  will  form  a  good  exercise  in  algebraical  logic. 

Cor.  2.  The  particular  case  of  the  above  theorem  where  the 
number  of  factors  is  equal  to  the  degree  of  the  function  is  of 
special  interest.     We  have  then 

f(x)  =  (x  -  a,)  (X  -  a3)  .  .  .  (X  -  a?l)P. 

Here  P  is  of  zero  degree,  that  is,  is  a  constant.  To  determine  it 
we  have  only  to  compare  the  coefficients  of  xn  on  the  left  and 
right  hand  sides,  which  must  be  equal  by  chap,  iv.,  §  24.  Now 
f(x)  stands  for  p^1  +  p^1'1  +  .  .  .  +pn-ix+Pw  Hence  V-p0, 
and  we  have 

In  other  words — If  n  different  values  of  x  can  be  found  for  which 
the  integral  function  fix)  vanishes,  then  f(x)  can  be  resolved  into  n 
factors  of  the  1st  degree,  all  different. 

The  student  must  observe  the  "if"  here.  We  have  not 
shown  that  n  such  particular  values  of  x  can  always  be  found, 
or  how  they  can  be  found,  but  only  that  if  they  can  be  found  the 
factorisation  may  be  effected.  The  question  as  to  the  finding  of 
aj,  a2,  ,  .  . ,  &c,  belongs  to  the  Theory  of  Equations,  into  which 
we  are  not  yet  prepared  to  enter. 

§  16.]  The  student  who  has  followed  the  above  theory  will 
naturally  put  to  himself  the  question,  "  Can  more  than  n  values 


v  THE  REMAINDER  THEOREM  99 

of  x  be  found  for  which  an  integral  function  of  x  of  the  nth  degree 
vanishes,  and,  if  so,  what  then  1 "  The  following  theorem  will 
answer  this  question,  and  complete  the  general  theory  of  factorisa- 
tion so  far  as  we  can  now  follow  it. 

If  an  integral  function  of  x  of  the  nth  degree  vanish  for  more  than 
n  different  values  of  x,  it  must  vanish  identically,  that  is,  each  of  its 
coefficients  must  vanish. 

Let  a„  a3,  .  .  .  ,  a,!  be  n  of  the  values  for  which  f(x)  vanishes, 
then  by  §  15  above,  if  p0  be  the  coefficient  of  the  highest  power 
of  x  in  f(x),  we  have 

f(x)  =  p0(x  -  a,)  (X  -  a2)  .  .  .  (x  -  an)  ( 1 ). 

Now  let  ft  be  another  value  (since  there  are  more  than  n)  for 
which /(.r)  vanishes,  then,  since  (1)  is  true  for  all  values  of  x,  we 
have 

0  =/(/?)  =MP  -  «,)  (fi  "  «.)  ...  08  -  «n)  (2). 

Since,  by  hypothesis,  a1}  a2,  .  .  .  ,  an  and  /?  are  all  different, 
none  of  the  differences  /5  -  a„  /3  -  a2,  .  .  .  ,  (3  -  an,  can  vanish, 
and  therefore  their  product  cannot  vanish.    Hence  (2)  gives p0  =  0. 

This  being  so,  f(x)  reduces  to  p^x11-1  +|)2a;'l~2  +  .  .  .  +pn-jX 
+  pn.  We  have  now,  therefore,  a  function  of  the  {n  -  l)th  degree 
which  vanishes  for  more  than  n,  therefore  for  more  than  (n  -  1), 
values  of  its  variable.  We  can,  by  a  repetition  of  the  above 
reasoning,  prove  that  the  highest  coefficient  J9,  of  this  function 
vanishes.  Proceeding  in  this  way  we  can  show,  step  by  step, 
that  all  the  coefficients  of  /(./•)  vanish. 

As  an  example  of  this  case  the  student  may  take  the  following : — 

The  integral  function 

Q3  -  7)  (3  -  0)  (3  -y)  +  (y-a)  (x  -  y)  (x  -  a)  +  (a  -  /3)  (x  -  a)  (x  -  /3) 
+  (/3-7)(7-0)(a-/3) 

vanishes  when  x  —  a,  when  x  =  p,  and  when  x  =  y  ;  but  it  is  only  of  the  2nd 
degree  in  x.  We  therefore  infer  that  the  function  vanishes  for  all  values  of  x, 
that  is  to  say,  that  we  have  identically 

{P-y){3B-p){x-y)  +  (y-a.){x-y){x-a)  +  (a-fl(x-a)(x-p) 

+  (/*-7)(7-a)(ft-/9)  =0. 

That  this  is  so  the  reader  may  readily  verify  by  expanding  and  arranging  the 
left-hand  side. 


100  INDETERMINATE  COEFFICIENTS  CHAP; 

Cor.  If  two  integral  functions  of  x,  whose  degrees  are  m  and  n 
respectively,  m  being  >  n,  be  equal  in  value  for  more  than  m  different 
values  of  x,  a  fortiori,  if  they  be  equal  for  all  values  of  x,  that  is  to 
say,  identically  equal,  then  the  coefficients  of  like  powers  of  x  in  the 
two  must  be  equal. 

We  may,  without  loss  of  generality,  suppose  the  two  functions 
to  be  each  of  degree  m,  for,  if  they  be  not  equal  in  degree,  this 
simply  means  that  the  coefficients  of  xn+1,  x1l+2,  .  .  . ,  xm  in  one 
of  them  are  zero.      We  have  therefore,  by  hypothesis, 

p(&m+plXm^1+   .    .    .    +pm  =  q<pim  +  qiZm~1+   •    •    .    +2m» 

and  therefore 

(p0~q0)xm+(p1-q1)xm-1+   .   .    .    +(pm-qm)  =  0, 

for  more  than  m  values  of  x. 
Hence  we  must  have 

Po-?o  =  0,    Pi-fr^O,    .  .  .,    pm-qm  =  0; 

that  is, 

Po  =  %     lh  =  So      •   •   •  »     Pm  =  2W 

This  is  of  course  merely  another  form  of  the  principle  of 
indeterminate  coefficients.  The  present  view  of  it  is,  however, 
important  and  instructive,  for  we  can  now  say  that,  if  any 
function  of  x  can  be  transformed  into  an  integral  function  of  x,  then 
this  transformation  is  unique. 

§  17.]  The  danger  with  the  theory  we  have  just  been  ex- 
pounding is  not  so  much  that  the  student  may  refuse  his  assent 
to  the  demonstrations  given,  as  that  he  may  fail  to  apprehend 
fully  the  scope  and  generality  of  the  conclusions.  We  proceed, 
therefore,  before  leaving  the  subject,  to  illustrate  very  fully  the 
use  of  the  remainder  theorem  in  various  particular  cases. 

To  help  the  student,  we  shall  distinguish,  in  the  following 
examples,  between  identical  and  conditional  equations  by  using 
the  sign  '*  =  "  for  the  former  and  the  sign  "  =  "  for  the  latter. 

Example  1.   To  determine  the  value  of  the  constant  k  in  order  that 

may  be  exactly  divisible  by  a; +  2. 

The  remainder,   after  dividing  by  x  +  2,  that  is,   by  x-  (  -  2),  is  (-2)s 


EXAMPLES 


101 


+  6(  -  2)2  +  4(  -  2)  + /-,  that  is,  8  +  k.     The  condition  for  exact  divisibility  is 
therefore  8  +  &  =  0,  that  is,  k=  -8. 
Example  2.  To  determine  whether 

80?- 2a-3 -7a -2  (1) 

is  divisible  by  (x  +  1)  (x-  2). 

If  we  put  x—  - 1  in  the  function  (1)  we  get 

-3-2  +  7-2  =  0, 

hence  it  is  divisible  by  x+1. 
If  we  put  x  =  2  we  get 

24-8-14-2  =  0, 

hence  it  is  divisible  by  X  -  2. 

Hence  by  §  15  it  is  divisible  by  (x  +  l)(x-2).  The  quotient  in  this  case 
is  easily  obtained,  for,  since  the  degree  of  (1)  is  the  3rd,  we  must  have 

Bx"-2a?-7x-2  =  (x+l){x-2){ax  +  b)  (2), 

where  a  and  b  are  numbers  to  be  determined. 

If  we  observe  that  the  highest  term  3a-3  on  the  left  must  be  equal  to  the 
product  x  x  x  x  ax  of  the  three  highest  terms  of  the  factors  on  the  right,  we 
see  that  SxP^ax3,  hence  a=3.  And,  since  the  product  of  the  three  lowest 
terms  of  the  factors  on  the  right  must  be  equal  to  -  2,  the  lowest  term  on  the 
left,  we  get  -  2&=  -  2,  that  is,  b  =  l.     Hence  finally 

3a3-  2x-  -  7x-2=(x+l)  (x  -  2)  (Bx+1). 


Example  3 

If  n  be  a  positive  integer, 

when 

is  divided  by 

the  rem.  is 

that  is 

xn  -  a'1 

X  -a 

a"  -  a" 

0  always. 

xn  -  a" 

x  +  a 

{-a)"-  a" 

0  if  n  be  even,  -  2an  if  n  be  odd. 

x"  +  «" 

x-a 

a"  +  a'1 

2a"  always. 

x"  +  a" 

x  +  a 

(  -  a)"  +  a" 

0  if  n  be  odd,  2a"  if  n  be  even. 

Hence  xn-a"  is  exactly  divisible  by  x-a  for  all  integral  values  of  n,  and  by 
x  +  a  if  n  be  even.  xn  +  a"  is  exactly  divisible  by  x  +  a  if  n  be  odd,  but  is 
never  exactly  divisible  by  z  —  a  (so  long  as  «=#0).  These  results  agree  with 
those  given  above,  chap,  iv.,  §  16. 

Example  4.  To  prove  that 

a"'{b  -  c)  +  b3{c  -a)  +  c^{a-b)=  -(a  +  b  +  c)  (b  -  c)  (c  -  a)  (a  -  b). 
First  of  all  regard  F^a^b  -  c)  +  b3{c-a)+cs(a-b)  as  a  function  of  a.     P 
is  an  integral  function  of  a  of  the  3rd  degree  ;  and,  if  we  put  a  =  b, 

Y  =  b3(b  -c)  +  ¥(c  -b)  +  cs(b  -  b) 
=  0; 


102  CONTINUED  DIVISION  chap. 

and  similarly,  if  we  put  a  =  c,  P  =  0  ;  therefore  P  is  exactly  divisible  both  by 
a  -  b  and  by  a  -  c. 

Again,  regard  P  as  a  function  of  b  alone.  It  is  an  integral  function  of  b, 
and  vanishes  when  b  —  c,  hence  it  is  exactly  divisible  by  b-c.  We  have, 
therefore, 

T  =  Q{a-b){a-c)(b-c). 

Since  P,  regarded  as  a  function  of  a,  b,  and  c,  is  of  the  4th  degree,  it 
follows  that  Q  must  be  an  integral  function  of  a,  b,  c  of  the  1st  degree. 
Hence,  I,  m,  n  being  mere  numbers  which  we  have  still  to  determine,  we 
have 

w\b  -  c)  +  b3(c  -  a)  +  c3(a  -  b)  =  (la  +  mb  +  nc)  {b-c)  (a-c)  (a-b) 

=  —{la  +  mb  +  nc)  (b  -c){c-  a)  (a  -  b). 
To  determine  I  we  have  merely  to  compare  the  coefficients  of  a3b  on  both 
sides.     It  thus  results  by  inspection  that  1  =  1;  and  similarly  m  =  l,  n  =  l; 
the  last  two  inferences  being  also  obvious  by  the  law  of  symmetry.     We  have 
therefore  finally 

as(b  -  c)  +  b\c  -a)  +  c3(a  -b)=  -  (a  +  b  +  c)(b-c)  (c-a)(a-  b). 
Example  5.   To  show  that 

Pee 2b2c2  +  2c2a2  +  2a2b2  -  a*  -  b*  -  c4 
=  (a  +  b  +  c)  (  -  a  +  b  +  c)  (a  -  b  +  c)  (a  +  b  -  c). 
First,  regarding  P  as  an  integral  function  of  a,  and  dividing  it  hy  a  +  b  +  c, 
that  is,  by  a  -  (  -  b  -  c),  we  have  for  the  remainder 
2J2c2+2c2(  -  b  -  cf  +  2b\  -  b- cf-  ( - 4-c)4-  6*-c* 

==  2b2c2  +  2b2<?  +  4.bcs  +  2c4  +  2¥  +  ib3c  +  2b2c2 
-  64  -  ib3c  -  6b2c2  -  Abe3  -c^b^-c4- 
=0. 
Hence  P  is  exactly  divisible  by  a  +  b  +  c. 

Observing  that  the  change  of  a  into  -  a,  or  of  b  into  -  b,  or  of  c  into  -  c 
does  not  alter  P,  all  the  powers  of  these  letters  therein  occurring  being  even, 
we  see  that  P  must  also  be  divisible  by  -a  +  b  +  c,  a-b  +  c,  and  a  +  b-c.  We 
have  thus  found  four  factors  of  the  1st  degree  in  a,  b,  c,  and  there  can  be  no 
more,  since  P  itself  is  of  the  4th  degree  in  these  letters.  This  being  estab- 
lished, it  is  easy  to  prove,  as  in  Example  4,  that  the  constant  multiplier  is 
+ 1 :  and  thus  the  result  is  established. 


EXPANSION    OF   RATIONAL   FRACTIONS    IN    SERIES   BY    MEANS    OF 

CONTINUED    DIVISION. 

§  18.]  If  we  refer  back  to  §§  5  and  6,  and  consider  the  analysis 
there  given,  we  shall  see  that  every  step  in  the  process  of  long 
division  gives  us  an  algebraical  identity  of  the  form 


V  DESCENDING  CONTINUED  DIVISION  103 

where  Q'  is  the  part  of  the  quotient  already  round,  and  R'  the 
residue  at  the  point  where  we  suppose  the  operation  arrested. 

For  example,  if  we  stop  at  the  end  of  the  second  operation, 
8/  +  8/  -  20/  +  40/  -  50/  +  30a  -  10 
2/  +  3/  -  4/  +  6.c  -  8 

*_  2/  +  8/ -  6/  +  14s- 10 

~~X+  2/+3/-4/+6*-8  ' 
Again,  instead  of  confining  ourselves  to  integral  terms  in  x,  and 
therefore  arresting  the  process  when  the  remainder,  strictly  so 
called,  is  reached,  we  may  continue  the  operation  to  any  extent. 
In  this  case,  if  we  stop  after  any  step  we  still  get  an  identity  of 
the  form 

where 

Q'  =  AxP  +  BxP-1  +  .  .  .  +  Kx  +  L  +  M/:c  +  .  .  .+T/&  (2), 
and 

R'  =  U^1-1  +  Vxn~2  +  .  .  .  +  Z  (3). 

This  process  may  be  called  Descending  Continued  Division. 

For  example,  consider 

^+2.r2  +  3a;+4 
x2  +  x  + 1 
and  let  us  conduct  the  division  in  the  contracted  manner  of  §  12,  but  insert 
the  powers  of  x  for  greater  clearness. 

a-2  +  a;+l 


x3  +  2x2  +  Sx  +  i 

+   x2  +  2x  +  4 

x  +  d 


.2      3      1_     2_ 

xi  +  x5 


X  +  1+-  +  ---.  +  -.  +  - 
X       iV"       ft, 


X 

3     2 


x    ar 

L     I. 

x2    x3 


2      1_ 

x* 
3      2 


+  ar*    a* 


whence        ^±g±|£±i=  1     2      3      1      2      ^fa-a^ 

ar+sc+l  a;    a;2    a,-5    ar4    a^5       a^+a+l 

an  identity  which  the  student  should  verify  by  multiplying  both  sides  by 
ar  +  a-+l.  ' 


104:  ASCENDING  CONTINUED  DIVISION  chap. 

§  19.]  When  we  prolong  the  operation  of  division  indefinitely 
in  this  way  we  may  of  course  arrange  either  dividend  or  divisor, 
or  both,  according  to  ascending  powers  of  x.  Taking  the  latter 
arrangement  we  get  a  new  kind  of  result,  which  may  be  illus- 
trated with  the  fraction  used  above. 
We  now  have 


i-x-x-  +  3x3-2x*-x5 


i  +  3x  +  2x-+   x3 

-   x-2x2  +   x3 

-   x-  +  2z3 

+  Bx3  +  xi 

-  2xi  -  3ar> 

-   xr'  +  2x6 

+  3x6  +  x7, 

wh  ence  5 =  4  -  x  -  x-  +  Bx3  -  2x*  -  x5  + ,  ,  ( o  )• 

x2  +  x+l  1+x  +  x2 

And,  in  general,  proceeding    in   a  similar  way  with    any   two 
integral  functions,  A^  and  Dn,  we  get 

where  Q"  =  A  +  Bx  +  .  .  .  +  Kafl  (7), 

K"  =  L  +  M.c  +  .  .  .  +  T.:"-1  (8). 

This  process  may  be  called  Ascending  Continued  Division. 

§  20.]  The  results  of  §§  18,  19  show  us  that  we  can,  by  the 
ordinary  process  of  continued  long  division,  expand  any  rational  fraction 
as  a  "series"  either  of  descending  or  ascending  powers  of  x,  continu- 
ing as  many  terms  as  ice  please,  plus  a  "  residue,"  which  is  itself  a 
rationed  fraction. 

And  there  is  no  difficulty  in  showing  that,  when  the  integer  q  is 
given,  each  of  the  expansions  (2)  and  (6)  o/§§  18  and  19  is  unique. 

The  proof  depends  on  the  theory  of  degree,  and  may  be  left 
as  an  exercise  for  the  reader. 

These  series  (the  Q'  or  Q"  parts  above)  belong,  as  we  shall 
see  hereafter,  to  the  general  class  of  "  Recurring  Series. " 

The  following  are  simple  examples  of  the  processes  we  have  been  describ- 
ing:— 

■  l+x  +  x2+.  .   .+.<"  f-n — -  (9). 


1 -x  \-x 

111  1      l'.<" 

— -5-3-?--  •  "x^^x  (10)- 


EXPANSION  THEOREMS  105 

-l-s+a?-.  .  .  +(-l)»x»-[    ?\  (11). 


1  +  a;  '  1  +  a: 

a;    a'2     a:3  a!"  1  +  x 


•i"r  -.3       •     •     •  ,,„  t    ,    .. 


l  +  ar  +  .   .  .  +xn 


=  1  -x+ x"**  -  a;»+2  +  a?»+2  -  ai2"+3  + .   .  . 

a/r+])(n+-l) 
i   riir+r  _  ^.nr+r+l    . . (13). 

1  +  x  + .   .   .  +  a;" 


1  ,     „       „  ,  ,       ,,         (/i  +  2)a;»+1-(n  +  l)a.'»+2 


(1  -a-)2-  '         v         '  (1  -a-)2 

(14). 


EXPRESSION    OF    ONE    INTEGRAL    FUNCTION    IN    POWERS    OF 

ANOTHER. 

§  21.]  "We  shall  Lave  occasion  in  a  later  chapter  to  use  two 
particular  cases  of  the  following  theorem. 

If  P  and  Q  be  integral  functions  of  the  rnth  and  nth  degrees 
respectively  (m  >  n),  then  P  may  always  he  put  into  the  form 

P  =  R0  +  R,Q  +  R2Q2  +  .  .  .  +  iy^  (1), 

where  R0,  E,,  .  .  . ,  R^  are  integral  functions,  the  degree  of  each  of 
which  is  re  — 1  at  most,  and  p  is  a  positive  integer,  which  cannot 
exceed  mjn. 

Proof. — Divide  P  by  Q,  and  let  the  quotient  be  Q0  and  the 
remainder  R0. 

If  the  degree  of  Q0  be  greater  than  that  of  Q,  divide  Q0  by 
Q,  and  let  the  quotient  be  Q,  and  the  remainder  Rj. 

Next  divide  Qi  by  Q,  and  let  the  quotient  be  Q.,  and  the 
remainder  R2,  and  so  on,  until  a  quotient  Qp_i  is  reached 
whose  degree  is  less  than  the  degree  of  Q.  Q^-,,  for  con- 
venience, we  call  also  R^.     "We  thus  have 

P  =  Q0Q  +  R0 
Qo  =  Q,Q  +  R, 

Hp-i  =  K-p- 


106  EXPANSION  THEOREMS  CHAP. 

Now,  using  in  the  first  of  these  the  value  of  Q0  given  by  the 

second,  we  obtain 

P  =  (Q,Q  +  R,)Q  +  R„, 

=  R0  +  R,Q  +  Q,Q2. 

Using  the  value  of  Q,  given  by  the  third,  we  obtain 

P  =  R0  +  R1Q  +  R,Q2  +  Q2Q3  (3). 

And  so  on. 

We  thus  obtain  finally  the  required  result ;  for,  R0,  R,,  .  .  ., 
Rp  being  remainders  after  divisions  by  Q  (whose  degree  is  n), 
none  of  these  can  be  of  higher  degree  than  n-1;  moreover, 
since  the  degrees  of  Q0,  Q„  Q.,  .  .  .,  Qp-i  are  m  -  n,  m  -  2n, 
m  -  3n,  .  .  .,  m-  np,  p  cannot  exceed  m/n. 

The  two  most  important  particular  cases  are  those  in  which  Q  =  a:-a  and 
Q  =  x2  +  (3x  +  y.     We  then  have 

T  =  a0  +  a1(x-a)  +  .   .  .+a„{x-a)", 

where  a0,  «i,  •   •  • ,  ««  ai'e  constants  ; 

P  =  (oo  +  b&)  +  (rti  +  hx)  (x°-  +  (3x  +  y)  +  .  .   . +(ap  +  bpx)(x"  +  fix  +  y) p, 
where  a0,  au  .  .   .,  ap,bo,h,  •  •  •,  ^  are  constants,  a,ndj»mj2. 

Example  1. 

Let  P=5«s-ll£c2+l0aj-2, 

Q  =  x-1. 

The  calculation  of  the   successive   remainders   proceeds   as   follows  (see 

§  13):— 

5  -11  +10  -2 

0  +    5  -    6+4 

5  -    6  +   4|  +  2 
0+5-1 


5  -    l|+    3 

0+5 


6|+    4 
0 

1  +  5; 

and  we  find 

5...3  -1U"  + 10a:-2  =  2  +  3(o;-  1)  +  4(3--  l)2+5{x     l)3. 

Example  2. 

P  =  x«  +  3x7  +  4z6  +  4a;2  +  Sx  + 1, 

Q  =  x2-x  +  l. 

The  student  will  find 

R0  =  11  x,  •  Ri  =  -  22a!  +  7,     R;  =  1 9a-  -  22,     R3  =  7x  +  15,     R4  =  1 


v  EXPANSION  THEOREMS  107 

so  that 

Y  =  n.r  +  {-22x+7)(x2-x+l)  +  {19x-22)(xi-x+l),i 
+  (7x  + 15)  (.c2  -  x  + 1  )8  +  (k2  -  x  + 1  )4. 

§  22.]  If  a,,  a9,  .  .  .,  art  &e  w  constants,  any  two  or  more  of 
which  may  be  equal,  then  any  integral  function  of  x  of  the  nth  degree 
may  be  put  into  the  form 

A0  +  A,(.c  -  a,)  +  A2(x  -  al)(x  -  a,2)  +  A3(x  -  ax)(x  -  a2)(x  -  a3)  +  .  .  . 

+  AH(x  -  a,)  (a;  -  a2) .  .  .  (x  -  an)  (1 ), 

where  A0,  A,,  A2,  .   .   . ,  An  are  constants,  any  one  of  which  except  An 
may  be  zero. 

Let  P?i,  be  the  given  integral  function,  then,  dividing  Pn  by 
x  -  a, ,  we  have 

P»  =  P»-i(s-  «,)  +  Ao  (2), 

where  A0  is  the  constant  remainder,  which  may  of  course  in  any 
particular  case  be  zero. 

Next,  dividing  Pn_!  by  (x  —  a.,),  we  have 

Pn-.^Pn-^-O  +  A,  (3); 

and  so  on. 

Finally,  P:  =  An(.?;  -  an)  +  An  _ ,  (n  +  1 ). 

Using  these  equations,  we  get  successively 

Pn  =  A0  +  A,(x  -  a,)  +  (x  -  a,)(x  -  a.,)?n_2, 
=  A0  +  A,(.?;  -  «,)  +  A2(x  -  at)  (x  -  «,) 

+  (x-a1)(x-as)(x-aa)'Pn-a, 

Pn  =  A0  +  A,(.?;  -  «,)  +  A,,(r  -  <?,)  (a-  -  a,)  +  A3(x  -  a,)  (x  -  a2)  (x  -  a3) 
+  .  .   .  +  An(x  -  «,)  (./•  -  a,2)  .  .  .  (x  -  an). 

This  kind  of  expression  for  an  integral  function  is  often 
useful  in  practice. 

Knowing  a  priori  that  the  expansion  is  possible,  we  can,  if  we  choose, 
determine  the  coefficients  by  giving  particular  values  to  x.  But  the  most 
rapid  process  in  general  is  simply  to  carry  out  the  divisions  indicated  in  the 
proof,  exactly  as  in  Example  1  of  last  paragraph. 

Thus,  to  express  a-3-!  in  the  form  A„  +  A\(x- 1)4-  A-..(.r- 1)  {x-  2) 
+  A3{x  -  1)  (,r  -  2)  (x  -  3),  we  calculate  as  follows  :  — 


108 


EXERCISES  IX 


CHAl'. 


1  +0  +0  -1 

0  +1  +1  +1 

1  +1  +l|0 
0  +2  +6 


1  +  3|  +  7 
0  +3 


1+6 


Henceo.-3-l  =  0  +  7(a--l)  +  6(a:-l)(a:-2)  +  (x-l)(a.'-2)(a;-3). 


Exercises  IX. 

Transform  the  following  quotients,   finding  both  integral  quotient  and 
remainder  where  the  quotient  is  fractional. 

(1.)  (sc5-5a8+5ar!-l)/(ar!+3a;+l). 

(2. )  (6a:6  +  2a;5  -  19a4  +  3lar5  -  37a;2  +  27a:  -  7)/(2a-2  -  3a-  + 1 ). 

(3. )  (4a;5  -  2x*  +  Zx3  -aj+1  )/(a;2  -  2a;  + 1). 

(4. )  (as5  -  8aj+ 15)  (x"  +  Sx  +  15)/(x-  -  25). 

(5. )  {(as- 1)  {x-  2)  (x  -  3)  (as  -  4) (x  -  5)  -  760(.i-  -  6)  +  120(a: -  7)}  +  (a!  -  C) 
(x-7). 

(6.)  (x6  +  4a:5 -  3a-4 -  16x3  +  2x2  +  x  +  3)/{x3+4x2  +  2x+l). 

(7.)  (27a*  +  10ass+l)/(3a?-2a:  +  l). 

(8. )  (x?  -  9a?  +  23a;  -  15)  (a:  -  7)/(ass  -  Sx  +  7). 

(9. )  (a;3  +  fix*  +  &&  +  t&  +  i)/(x"  ~  ix  + 1 ). 
(10.)  (a;4  +  fce3  +  ia-2  +  Aa:  +  i)/(x2  +  2aj  + 1 ). 
(11.)  (a/  +  T^)/(2a:+l). 
(12. )  (a;2  -  a;  + 1 )  (xs  -  1  )/{x*  +  ar»  + 1 ). 
(13.)  (ailV-fltyu)/(a:-y). 
(14. )  (9«4  +  2o2fis  +  &*)/(3aa  +  2«fe  +  62). 
(15.)  (a7  +  67)/(a  +  6). 
(16.)  (a;4  +  y4  -  7x-y°-)l{x>  +  Zxy  +  y"). 
(17.)  (x5  -  2afy  +  4.r32/2  -  8a*Y  + 1 6a-*/4  -  32ys)ftx*  -  8)/). 
(18. )  (a;4  +  5arfy  +  7a?V  +  15xif  +  12y4)/(a-  +  Ay). 
(19.)  (l+.r  +  x2  +  a?  +  a^  +  x6  +  x7  +  a*  +  a;9  +  a;15)/(l- 
(20.)  (a;6-5a^  +  8)/(a^  +  a;  +  2). 
(21 . )  {abx3  +  {ac  -  W )x2  -  (a/+  cd)x  +  <//}  /(aa:  -  d). 
(22. )  {a262  +  uV  +  fe2c2  +  2a?bc  -  2ab~c  -  2abc" }  4-  { «2  ■ 
(23. )  (1  +  b+c  -  be  -  Ve '-  bcn-)/(l  -  be). 
(24.)  {(ax  +  by)3  +  (ax-by)*-(ay-bxf+(ay  +  bx)3}/{(a  +  b)hr-3ab(x>-y-)}. 
(25. )  { (a2  +  b-)3  +  b3a3}j { (a  +  b)n-  -ba}. 
(26.)  {(x2  +  xy  +  yy-(xi-xy  +  i/-)i}l{xi  +  Zxhj-  +  yi}. 
(27. )  { (x  +  yY  -x>-  /}/(a?  +  *>/  +  2/2)2. 
(28.)  {(x+l)6-.r6-l}/{a?  +  x  +  l). 
(29.)  {o6(a?  +  i/)+arj/(os  +  62)}/{o6(ar'-ys)-a^(a2-  52)}. 
(30.)  (a!i  +  2a3b-  +  2a2b3-3b'i)/(ar-2ab  +  b-). 


t'5  +  X6). 


(«-S)(a-e)}. 


v  EXERCISES  IX  109 

(31.)  (xi-Zx2-2;r  +  4)/(.r  +  2). 

(32.)  (jc*- 4a?-Zia?+76x+V)5)f(x-7). 

(33. )  Find  the  remainder  when'  a?  -  6x2  +  8a:  -  9  is  divided  by  2x  +  3. 

(34.)  Find  the  remainder  when  pa?  +  qx2  +  qx+p  is  divided  by  x-  1  ;  and 
find  the  condition  that  the  function  in  question  be  exactly  divisible  by  x2-  1. 

(35.)  Find  the  condition  that  Ax2m  +  Bx">yn  +  Cy2"  be  exactly  divisible  by 
]\vm  +  Qy". 

(36.)  Find  the  conditions  that  x3  +  ax"  +  bx  +  c  be  exactly  divisible  by 
x-  +px  +  q. 

(37. )  If  x  -  a  be  a  factor  of  x2  +  2ax  -  36'-,  then  a .  =  ± b. 

(38.)  Determine  X,  /u,  v,  in  order  that  x4  +  Sx3  +  \x2  +  fix  +  v  be  exactly 
divisible  by  (x2-l)(x  +  2). 

(39.)  If  x4  +  Ax3  +  Qpx2  +  4 qx  +  r  be  exactly  divisible  by  x3  +  Bx2  +  9x  +  S, 
find  p,  q,  r. 

(40.)  Show  that  px3  +  (p2  +  q)x2  +  {2pq  +  r)x  +  q2  +  s  and  px3  +  (p2  -  q)x2 
+  rx-q2  +  s  either  both  are,  or  both  are  not,  exactly  divisible  by  x2  +p>x  +  q. 

(41.)  Find  the  condition  that  (xm  +  xm~l  +  .  .  .  +l)/(a,-"  +  a:n-1+  .  .  .  +1) 
be  integral. 

(42.)  Expand  l/(3.c  +  l)  in  a  series  of  ascending,  and  also  in  a  series  of 
descending,  powers  of  x  ;  and  find  in  each  case  the  residue  after  n  + 1  terms. 

(43.)  Express  l/iar-ax  +  x2)  in  the  form  A  +  Bz  +  Cx2  +  Dx3  +  R,  where  A, 
B,  C,  D  are  constants  and  R  a  certain  rational  function  of  x. 

(44.)  Divide  1+  x  +  ^  +  1^-3  +  •  •  ■  t>yl-sc 

(45.)  Show  that,  if  y<\,  then  approximately  1/(1  +y)  =  l  -y,  1/(1-  y) 
=  1  +  ?/,  the  error  in  each  case  being  100;/2  per  cent. 

Find  similar  approximations  for  1/(1+?/)"  and  1/(1 -y)n,  where  n  is  a 
positive  integer. 

(46.)  If  a>l,  show  that  «">1  +n{a- 1),  n  being  a  positive  integer. 
Hence,  show  that  when  n  is  increased  without  limit  an  becomes  infinitely 
great  or  infinitely  small  according  as«>  or  <1. 

(47.)  Show  that  when  an  integral  function  f(x)  is  divided  by  (x-ai) 
(x  —  ao)  the  remainder  is  {/(a-j)(a;-ai)  -/(ax)(a;-ao)}/(a2-  aj).  Generalise 
this  theorem. 

(48.)  Show  that  f(x)-/(a)   is  exactly  divisible  by  x-a;   and  that,   if 
f(x)=p0xn+piXn-1+p&cn-2+  .   .  . +pn,    then    the    quotient   is   x(x) -poxn~l 
+  (p0a+pi)xn-2  +  (pl)a2+pla.+2h2)xn-3+.   .   .  +(p0an~l +pxan~2+  .   .    .+pn-l). 

Hence   show   that   when  f(x)   is   divided   by    (x-a)2   the   remainder  is 
X(o)  (z-a)+/(a), 
where  f(a)=p0an+pian-1+.   .    .  +p„, 

x(a)-np0an-1  +  (n-l)2han-2+.   .   .  +pn-1. 

(49.)  If  x"+2hx"~1+.  •  .  +pn  and  x"-1  +  qxxn-2  + .  .  .  +q»-i  have  the 
same  linear  factors  with  the  exception  of  a: -a,  which  is  a  factor  in  the  first 
only,  find  the  relations  connecting  the  coefficients  of  the  two  functions. 

(50.)  If,  when  y  +  c  is  substituted  for  x  in  xn  +  aixn~1  +  .  .  .  +a„,  the 


110  EXERCISES  IX  chap.  V 

result  is  yn  +  &i2/n_1  + .  .  .  +bn,  show  that  bn ,  £>„_i,  .  .  . ,  bx  ai-e  the  remainders 
when  the  original  function  is  divided  by  x  -  c,  and  the  successive  quotients 
by  x-c.  Hence  obtain  the  result  of  substituting  y  +  3  for  x  in  a^-l&B* 
+  20x3-17x2-x  +  B. 

(51.)  Express  (x2  +  3x  +  l)*  in  the  form  A  +  B(a:  +  2)  +  C(a:  +  2)2  +  &c.,  and 
also  in  the  form  Ax  +  B  +  {Cx  +  B)(x2  +  x  +  l)  +  ('Ex  +  F)(x-  +  x  +  lf  +  kc. 

(52.)  Express  xA  +  x?  +  x2  +  x  +  l  in  the  form  A0  +  Ai(x  +  1)  +  A-2(x+l)(x+3) 
+  A3(a:  +  l)(a;  +  3)(a;  +  5)+A4(a:  +  l)(a;  +  3)(a;  +  5)(.r  +  7). 

(53.)  If,  when  P  and  P'  are  divided  by  D,  the  remainders  are  R  and  R', 
show  that,  when  PP'  and  RR'  are  divided  by  D,  the  remainders  are  identical. 

(54.)  When  P  is  divided  by  D  the  remainder  is  R  ;  and  when  the  integral 
quotient  obtained  in  this  division  is  divided  by  D'  the  remainder  is  S  and  the 
integral  c|uotient  Q.  R',  S',  Q'  are  the  corresponding  functions  obtained  by 
first  dividing  by  D'  and  then  by  D.  Show  that  Q  =  Q',  and  that  each  is  the 
integral  quotient  when  P  is  divided  by  DD';  also  that  SD  +  R  =  S'D'  +  R', 
and  that  each  of  these  is  the  remainder  when  P  is  divided  by  DD'. 


CHAPTEE    VI. 

Greatest  Common  Measure  and  Least  Common 

Multiple. 

§  1.]  Having  seen  how  to  test  whether  one  given  integral 
function  is  exactly  divisible  by  another,  and  seen  how  in  certain 
cases  to  find  the  divisors  of  a  given  integral  function,  we  are 
naturally  led  to  consider  the  problem — Given  two  integral 
functions,  to  find  whether  they  have  any  common  divisor  or  not. 

We  are  thus  led  to  lay  down  the  following  definitions  : — 

Any  integral  function  of  x  which  divides  exactly  two  or  more  given 
integral  functions  of  x  is  called  a  common  measure  of  these  functions. 

The  integral  function  of  highest  degree  in  x  zchich  divides  exactly 
each  of  two  or  more  given  integral  functions  of  x  is  called  the  greatest 
common  measure  (G.C.3I.)  of  these  functions. 

§  2.]  A  more  general  definition  might  be  given  by  suppos- 
ing that  there  are  any  number  of  variables,  x,  y,  z,  u,  &c.  ;  in 
that  case  the  functions  must  all  be  integral  in  x,  y,  z,  u,  &c,  and 
the  degree  must  be  reckoned  by  taking  all  these  variables  into 
account.  This  definition  is,  however,  of  comparatively  little 
importance,  as  it  has  been  applied  in  practice  only  to  the  case  of 
monomial  functions,  and  even  there  it  is  not  indispensable.  As 
it  has  been  mentioned,  however,  we  may  as  well  exemplify  its 
use  before  dismissing  it  altogether. 

Let  the  monomials  be  432aWy42,  270aWyV,  90a7v;3yV, 
the  variables  being  x,  y,  z,  then  the  G.C.M.  is  x2ifz,  or  C'V':, 
where  C  is  a  constant  coefficient  (that  is,  does  not  depend  on  the 
variables  x,  y,  z). 

The  general  rule,  of  which  the  above  is  a  particular  case,  is 
as  follows  : — 


112  G.C.M.  BY  INSPECTION 


CHAP. 


The  G.C.M.  of  any  number  of  monomials  is  the  product  of  the 
variables,  each  raised  to  the  lowest  power  *  in  which  it  occurs  in  any 
one  of  the  given  functions. 

This  product  may  of  course  be  multiplied  by  any  constant 
coefficient. 

G.C.M.    OBTAINED    BY    INSPECTION. 

§  3.]  Returning  to  the  practically  important  case  of  integral 
functions  of  one  variable  x,  let  us  consider  the  case  of  a  number 
of  integral  functions,  P,  P',  P",  &c,  each  of  which  has  been  re- 
solved into  a  product  of  positive  integral  powers  of  certain  factors 
of  the  1st  degree,  say  x  —  a,  x  -  (3,  x  -  y,  &c. ;  so  that 

P   =p(x-a)«(x-P)\x-yy..., 

P'  =p'(x  -  a)a'(x  -  (3)b'(x  -  yY'  ..., 
V"=p"{;x-ar'{x-pr{x-yr  ..., 

By  §  15  of  chap,  v.,  we  know  that  every  measure  of  P 
can  contain  only  powers  of  those  factors  of  the  1st  degree  that 
occur  in  P,  and  can  contain  none  of  those  factors  in  a  higher 
power  than  that  in  which  it  occurs  in  P,  and  the  same  is  true  for 
P',  P",  &c.  Hence  every  common  measure  of  P,  P',  P",  &c,  can 
contain  only  such  factors  as  are  common  to  P,  P',  P",  &c.  Hence 
the  greatest  common  measure  of  P,  P',  P",  &c,  contains  simply  all  the 
factors  that  are  common  to  P,  P',  P",  &c,  each  raised  to  the  lowest 
power  in  which  it  occurs  in  any  one  of  these  functions. 

Since  mere  numbers  or  constant  letters  have  nothing  to  do 
with  questions  relating  to  the  integrality  or  degree  of  algebraical 
functions,  the  G.C.M.  given  by  the  above  rule  may  of  course  be 
multiplied  by  any  numerical  or  constant  coefficient. 

Example  1. 

P=2x2-6a:  +    4  =  2(a--l)(a--2), 
P' =  6a:2  -  6z  -  12  =  6(x  + 1 )  (a;  -  2). 
Hence  the  G.C.M.  of  P  and  P'  is  a-  2. 
Example  2. 

P  =  a*  -  5as*  +  7a:3  +  x2 -  8x  +  4  =  (x  -  1  )-(x  +  l)[x-  2)2, 
P'  =  xe-  7x>+  17a-4  -  Ux3-  10a:2  +  20a;-  S  =  (x-  l)-(o.  +  l)  (a;-2)3, 
P"  =  x5  -Zx*-  a?  +  7a,"  -  4  =  (x  -  1 )  (x  +  l)2(x  -  2)2. 
The  G.  C.  M.  is  (a; - 1)  (a>+ 1)  (as  -  2)2,  that  is,  x4-4x3  +  3a;2  +  4x  -  4. 

*  If  any  variable  does  not  occur  at  all  in  one  or  more  of  the  given  func- 
tions, it  must  of  course  be  omitted  altogether  in  the  G.C.M. 


vi  CONTRAST  BETWEEN  ALGEBRAICAL  &  ARITHMETICAL  G.C.M.  113 

§  4.]  It  will  be  well  at  this  stage  to  caution  the  student 
against  being  misled  by  the  analogy  between  the  algebraical  and 
the  arithmetical  G.C.M.  He  should  notice  that  no  mention  is 
made  of  arithmetical  magnitude  in  the  definition  of  the  algebraical 
G.C.M.  The  word  "  greatest "  used  in  that  definition  refers 
merely  to  degree.  It  is  not  even  true  that  the  arithmetical 
G.C.M.  of  the  two  numerical  values  of  two  given  functions  of  x, 
obtained  by  giving  x  any  particular  value,  is  the  arithmetical 
value  of  the  algebraical  G.C.M.  when  that  particular  value  of  x 
is  substituted  therein ;  nor  is  it  possible  to  frame  any  definition 
of  the  algebraical  G.C.M.  so  that  this  shall  be  true.'1" 

The  student  will  best  satisfy  himself  of  the  truth  of  this  remark  by  study- 
ing the  following  example  : — 

The  algebraical  G.C.M.  of  x~-2,x  +  2  and  x2-x-2  is  x-2.  Now  put 
sc=31.  The  numerical  values  of  the  two  functions  are  870  and  928  respectively  ; 
the  numerical  value  of  x-  2  is  29  ;  but  the  arithmetical  G.C.M.  of  870  and  928 
is  not  29  but  58. 

LONG   RULE   FOR   G.C.M. 

§  5.]  In  chap.  v.  we  have  seen  that  in  certain  cases  in- 
tegral functions  can  be  resolved  into  factors ;  but  no  general 
method  for  accomplishing  this  resolution  exists  apart  from  the 
theory  of  equations.  Accordingly  the  method  given  in  §  3 
for  finding  the  G.C.M.  of  two  integral  functions  is  not  one  of 
perfectly  general  application. 

The  problem  admits,  however,  of  an  elementary  solution  by 
a  method  which  is  fundamental  in  many  branches  of  algebra. 
This  solution  rests  on  the  following  proposition : — 

If  A  =  BQ  +  R,  A,  B,  Q,  R  being  all  integral  functions  of  x, 
then  the  G.C.M.  of  A  and  B  is  the  same  as  the  G.C.M.  of  B  and  R. 

To  prove  this  we  have  to  show — 1st,  that  every  common 


*  To  avoid  this  confusion  some  writers  on  algebra  have  used  instead  of  the 
words  "greatest  common  measure"  the  term  "highest  common  factor."  We 
have  adhered  to  the  time-honoured  nomenclature  because  the  innovation  in 
this  case  would  only  be  a  partial  reform.  The  very  word  /actor  itself  is  used 
in  totally  dilferent  senses  in  algebra  and  in  arithmetic  ;  and  the  same  is  true 
of  the  words  fractional  and  integral,  with  regard  to  which  confusion  is  no  less 
common.  As  no  one  seriously  proposes  to  alter  the  whole  of  the  terminology 
of  the  four  species  in  algebra,  it  seems  scarcely  worth  the  while  to  disturb  an 
old  friend  like  the  G.C.M. 

VOL.  I  I 


114  LONG  KULE  FOR  G.C.M.  chap. 

divisor  of  B  and  R  divides  A  and  B,  and,  2nd,  that  every  common 
divisor  of  A  and  B  divides  B  and  R. 

Now,  since  A  =  BQ  +  R,  it  follows,  by  §  4  of  chap,  v.,  that 
every  common  divisor  of  B  and  R  divides  A,  hence  every  common 
divisor  of  B  and  R  divides  A  and  B. 

Again,  R  =  A  -  BQ,  hence  every  common  divisor  of  A  and  B 
divides  R,  hence  every  common  divisor  of  A  and  B  divides  B  and  R. 

Let  now  A  and  B  be  two  integral  functions  whose  G.C.M.  is  required; 
and  let  B  be  the  one  whose  degree  is  not  greater  than  that  of  the  other. 
Divide  A  by  B,  and  let  the  quotient  be  Q,,  and  the  remainder  R,. 

Divide  B  by  R,,  and  let  the  quotient  be  Q2,  and  the  remainder  R2. 

Divide  Ri  by  R2,  and  let  the  quotient  be  Q3,  and  the  remainder  R3, 
and  so  on. 

Since  the  degree  of  each  remainder  is  less  by  unity  at  least  than  the 
degree  of  the  corresponding  divisor,  R15  R2,  R3,  &c,  go  on  diminishing  in 
degree,  and  the  process  must  come  to  an  end  in  one  or  other  of  two  ways. 

I.  Either  the  division  at  a  certain  stage  becomes  exact,  and  the 
remainder  vanishes  ;  t 

II.  Or  a  stage  is  reached  at  which  the  remainder  is  reduced  to  a 
constant.  i  i 

Now  we  have,  by  the  process  of  derivation  above  described, 

A  =  BQX  +  R, 
B  -  R^a  +  R2 
R,  =  R2Q3  +  R3 


M1)- 


Hence  by  the  fundamental  proposition   the   pairs   of  functions 

A  (  B    |  R,  (  Ro  1  Rw-2  \R>i-i  (  ..li  v,flVP  fV,P  eomp  ci  HM 

B  IRJR,  jR,  /  •  *  •  RB_1  J |  R„     / 

In  Case  I.  Hn  =  0  and  R;i_2  =  Q,iR«-i.  Hence  the  G.C.M.  of 
R,t_2  and  Rn-u  that  is,  of  Q^R^-!  and  Rn_i,  is  R»_i,  for  this 
divides  both,  and  no  function  of  higher  degree  than  itself  can 
divide  R,t_i.      Hence  R7l_!  is  the  G.C.M.  of  A  and  B. 

In  Case  II.  R;l  =  constant.  In  this  case  A  and  B  have  no 
G.C.M.,  for  their  G.C.M.  is  the  G.C.M.  of  R;l_,  and  Rn>  that  is, 
their  G.C.M.  divides  the  constant  Rn.     But  no  integral  function 


VI 


MODIFICATIONS  OF  LONG  RULE 


115 


(other  than  a  constant)  can  divide  a  constant  exactly.     Hence 
A  and  B  have  no  G.C.M.  (other  than  a  constant). 

If,  therefore,  the  process  ends  with  a  zero  remainder,  the  last  divisor 
is  the  G.C.M. ;  if  it  ends  with  a  constant,  there  is  no  G.C.M. 

§  6.]  It  is  important  to  remark  that  it  follows  from  the 
nature  of  the  above  process  for  finding  the  G.C.M.,  which  con- 
sists essentially  in  substituting  for  the  original  pair  of  functions 
pair  after  pair  of  others  which  have  the  same  G.C.M.,  that  we 
may,  at  any  stage  of  the  process,  multiply  either  the  divisor  or  the 
remainder  by  an  integral  function,  provided  we  are  sure  that  this 
function  and  the  remainder  or  divisor,  as  the  case  may  be,  have  no 
common  factor.  We  may  similarly  remove  from  either  the  divisor  or 
the  remainder  a  factor  which  is  not  common  to  both.  We  may  remove 
a  factor  which  is  common  to  both,  provided  we  introduce  it  into  the  G.  C  M. 
as  ultimately  found.  It  follows  of  course,  a  fortiori,  tluit  a  numerical 
factor  may  be  introduced  into  or  removed  from  divisor  or  remainder  at  any 
stage  of  the  process.  This  last  remark  is  of  great  use  in  enabling  us 
to  avoid  fractions  and  otherwise  simplify  the  arithmetic  of  the  pro- 
cess. In  order  to  obtain  the  full  advantage  of  it,  the  student 
should  notice  that,  in  what  has  been  said,  "remainder"  may  mean, 
not  only  the  remainder  properly  so  called  at  the  end  of  each  sepa- 
rate division,  but  also,  if  we  please,  the  "  remainder  in  the  middle  of 
any  such  division''  or  "residue,"  as  we  called  it  in  §  18,  chap.  v. 

Some   of    these    remarks    are   illustrated    in    the 
examples  : — 


following 


Example  1. 

To  find  the  G.C.M.  of  x5 - 2x*  -  2x?  +  8x2 -  7x  +  2  audz4- 

x4  -  ix  +  3 


ix  +  3. 


X*- 
Xs 

-2xi-2x3  +   8x2~    1x  +  2 
-    Ax2  +   Zx 

-2) 

-  2x4  -  2r?  + 12x2 -  10a;  +  2 

ar*+  Xs-   6x2  +   5x- 1 
x*                     -    4a: +  3 

x3-   6x2+   9x-i 

x*                    -    4x  +  3 
xi-Qx3+   Qx2-   4x 

3)       6ar»-    9a;2           +3 

23?-    2.x2           +1 
2.r3-12a:2-l-18a:-8 

9)           9a^-18x  +  9 

X    +1 


a.3-6x-2  +  9a---4 
x  +2 


c2-    2x+l 


116 


EXAMPLES 


CHAP. 


X3- 

-  6a;2  +  9a;  -  4 

-  '2a;2  +   x 

-4)    - 

-4a;2+8a:-4 

a;2-2a;  +  l 
a-2-2a:+l 

x2-2a;+l 


a;  +1 


Hence  the  G.C.M.  is  xr-2x  +  l. 

It  must  be  observed  that  what  we  have  written  in  the  place 
of  quotients  are  not  really  quotients  in  the  ordinary  sense,  owing 
to  the  rejection  of  the  numerical  factors  here  and  there.  In 
point  of  fact  the  quotients  are  of  no  importance  in  the  process, 
and  need  not  be  written  down ;  neglecting  them,  carrying  out  the 
subtractions  mentally,  and  using  detached  coefficients,  we  may 
write  the  whole  calculation  in  the  following  compact  form : — 


_  o 


1-2-2+   8-   7  +  2 

-'2-2  +  12-10  +  2 

1  +  1-    6+   5-1 

1-    6+   9-4 


4  + 
1- 


8-4 
2  +  1 


0 


1+0+0-    4+3 

6-9+   0+3 

2-3+   0+1 

9-18  +  9 

1-    2  +  1 


-^3 
-j-9 


zx 


G.C.M.,  x2 

Example  2. 

Required  the  G.C.M.    of  4x4  +  26a,-3  +  41a;2-  2a;-  24  and  3a!*  +  20a?  +  32a;2 
-  8a;  -  32. 

Bearing  in  mind  the  general  principle  on  which  the  rule  for  finding  the 
G.C.M.  is  founded,  we  may  proceed  as  follows,  in  order  to  avoid  large  num- 
bers as  much  as  possible  : — 


4  +  26  +  41- 
x2  1+    6+   9  + 

2- 

6  + 

24 

8 

2  +  12  +  18+    12+    16 
7  +  44+   68+    16 
1+29  +  146  +  184 

-+23               23  +  138  +  184 

1+     6+     8 

3  +  20  +  32- 
2+    5- 


26- 


32 
56 


-53-318-424 

1+     6+     8 


-53 


The  G.C.M.  is  a2  +  6a: +  8. 

Here  the  second  line  on  the  left  is  obtained  from  the  first  by  subtracting 
the  first  on  the  right.  By  the  general  principle  referred  to,  the  function 
se4  +  6ar3  +  9a?  +  6a;  +  8  thus  obtained  and  3a;4  +  2033  +  32a;2  -  Sx  -  32  have  tlie 
same  G.C.M.  as  the  original  pair.  Similarly  the  fifth  line  on  the  left  is  the 
result  of  subtracting  from  the  line  above  three  times  the  second  line  on  the 
right. 


VI 


SECOND  RULE  FOR  G.C.M.  117 


If  the  student  be  careful  to  pay  more  attention  to  the  prin- 
ciple underlying  the  rule  than  to  the  mere  mechanical  application 
of  it,  he  will  have  little  difficulty  in  devising  other  modifications 
of  it  to  suit  particular  cases. 


METHOD    OF   ALTERNATE    DESTRUCTION    OF    HIGHEST    AND 

LOWEST   TERMS. 

§  7.]  If  /,  m.  p,  q  be  constant  quantities  (such  that  Iq  -  mp  is  not 
zero),  and  if 

P  =  ZA  +  mB  (1), 

Q  =  M  +  qB  (2), 

where  A  and  B,  and  therefore  P  and  Q,  are  integral  functions,  then 
the  G.C.M.  ofP  and  Q  is  the  G.C.M.  of  A  and  B. 

For  it  is  clear  from  the  equations  as  they  stand  that  every 
divisor  of  A  and  B  divides  both  P  and  Q.     Again,  we  have 

qP  -  wQ  =  q(IA  +  mS)  -  m  (pA  +  qB)  =  (Iq  -  mp)k         (3), 
-pP  +  ZQ  =  -p(IA  +  nzB)  +  I(pA  +  qB)  =  (Iq  -  mp)B         (4) ; 

hence  (provided  Iq  -  mp  does  not  vanish),  since  I,  p,  m,  q,  and 
therefore  Iq  -  mp,  are  all  constant,  it  follows  that  every  divisor  of 
P  and  Q  divides  A  and  B.      Thus  the  proposition  is  proved. 

In  practice  I  and  m  and  p  and  q  are  so  chosen  that  the 
highest  term  shall  disappear  in  I A  +  m*B,  and  the  lowest  in 
pA  +  qB.  The  process  will  be  easily  understood  from  the  follow- 
ing example  : — 

Example  1. 

Let  A  =  4ar*  +  26a-3  +  41a;2  -  2x  -  24, 
B  =  3a;4  +  20a?  +  32a;2  -  8x  -  32  ; 
then  -3A  +  4B  =  2ar>  +  5a;2-26a;-56, 

4 A  -  3B  =  7x*  +  44a.-3  +  68a;2  +  16a;. 

Rejecting  now  the  factor  x,  which  clearly  forms  no  part  of  the  G.C.M.,  we 
have  to  find  the  G.C.M.  of 

A'  =  7a;',  +  44a:2  +  68a;+16I 
B'  =  23?  + 5a;2 -26a: -56. 
Repeating  the  above  process — 

2A'-  7B'  =  53a-2  +  318a;  +424, 
7A'  +  2B'=53a-3  +  318.v2+424a\ 


118  TENTATIVE  PROCESSES 


CHAP. 


the  G.C.M.  of  which  is  53a;2  +  318a; +  424.  Hence  this,  or,  what  is  equivalent 
so  far  as  the  present  quest  is  concerned,  x2  +  Qx  +  8,  is  the  G.C.M.  of  the  two 
given  functions. 

When  the  functions  differ  in  degree,  we  may  first  destroy 
the  lowest  term  in  the  function  of  higher  degree,  divide  the 
result  by  x,  and  replace  the  function  of  higher  degree  by  the 
new  function  thus  obtained.  We  can  proceed  in  this  way  until 
we  arrive  at  two  functions  of  the  same  degree,  which  can  in 
general  be  dealt  with  by  destroying  alternately  the  highest  and 
lowest  terms. 

Detached  coefficients  may  be  used  as  in  the  following 
example : 

Example  2. 

To  find  the  G.C.M.  of  %A - 3ar>  +  2a;2  +  x -  1  and  x3 - x2 - 2x  +  2,  we  have 
the  following  calculation  : — 


A 
B 

1-3+2+1-1 
1-1-2+2 

A'  =         (2A  +  B)/* 
B'  =                   B 

2-5+3+0 
1-1-2+2 

A"  =                A'/x 
B"  =(-A'  +2B') 

2-5  +  3 

3-7  +  4 

A"'  =  (-4A"  +  3B")/x 
B'"=   -3A"  +  2B" 

1-1 
1-1 

Hence  the  G.C.M.  is  x-1. 

The  failing  case  of  the  original  process,  where  Jq -mp  =  0,  may  be  treated 
in  a  similar  manner,  the  exact  details  of  which  we  leave  to  be  worked  out  as 
an  exercise  by  the  learner. 

§  8.]  The  following  example  shows  how,  by  a  semi-tentative 
process,  the  desired  result  may  often  be  obtained  very  quickly : — 

Example. 

A  =  2a;4 -3a,-3 -3a;2 +  4, 
B  =  2xi-xs-9xi  +  ix  +  i. 

Every  common  divisor  of  A  and  B  divides  A  -  B,  that  is, 

-  2xa  +  6.c2  -  ix,   that    is,    rejecting    the    numerical    factor  -  2, 

x(x2  —  3x  +  2),  that  is,  x  (x  -  1)  (.c  -  2).    We  have  therefore  merely 

to  select  those  factors  of  x(x-\)(x-2)  which  divide  both  A 


VI  PROPOSITIONS  REGARDING  G.C.M.  119 

and  B.  x  clearly  is  not  a  common  divisor,  but  we  see  at  once, 
by  the  remainder  theorem  (§  13,  chap,  v.),  that  both  x—\  and 
x  -  2  are  common  divisors.  Hence  the  G.C.M.  is  (x  -  1)  (a;  —  2), 
or  x2  -  3a  +  2. 

§  9.]  The  student  should  observe  that  the  process  for  finding 
the  G.C.M.  has  the  valuable  peculiarity  not  only  of  furnishing 
the  G.C.M.,  but  also  of  indicating  when  there  is  none. 

Example. 

k=x--Sx  +  \, 
B  =  o;2-4a;+6. 

Arranging  the  calculation  in  the  abridged  form,  we  have 

1-3+1     I     1-4+6 
2+1  -1+5 


11     I 
The  last  remainder  being  11,  it  follows  that  there  is  no  G.C.M. 

G.C.M.    OF   ANY    NUMBER    OF    INTEGRAL    FUNCTIONS. 

§  10.]  It  follows  at  once,  by  the  method  of  proof  given  in 
§  5,  that  every  common  divisor  of  two  integral  functions  A  and  B  is 
a  divisor  of  their  G.  CM. 

This  principle  enables  us  at  once  to  find  the  G.C.M.  of  any 
number  of  integral  functions  by  successive  application  of  the 
process  for  two.  Consider,  for  example,  four  functions,  A,  B,  C,  D. 
Let  Gi  be  the  G.C.M.  of  A  and  B,  then  Gv  is  divisible  by  every 
common  divisor  of  A  and  B.  Find  now  the  G.C.M.  of  Gj  and 
C,  G,  say.  Then  Gr3  is  the  divisor  of  highest  degree  that  will 
divide  A,  B,  and  C.  Finally,  find  the  G.C.M.  of  G2  and  D, 
G3  say.     Then  G3  is  the  G.C.M.  of  A,  B,  C,  and  D. 

GENERAL   PROPOSITIONS    REGARDING    ALGEBRAICAL    PRIMENESS. 

§  11.]  We  now  proceed  to  establish  a  number  of  propositions 
for  integral  functions  analogous  to  those  given  for  integral 
numbers  in  chap,  iii.,  again  warning  the  student  that  he  must 
not    confound    the    algebraical    with    the    arithmetical    results ; 


120  PROPOSITIONS  REGARDING  G.C.M.  chav. 

although  he  should  allow  the  analogy  to  lead  him  in  seeking  for 
the  analogous  propositions,  and  in  devising  methods  for  proving 
them. 

Definition. — Two  integral  functions  are  said  to  be  prime  to  each 
other  when  they  have  no  common  divisor. 

Proposition. — A  and  B  being  any  two  integral  functions,  there 
exist  always  two  integral  functions,  L  and  M,  'prime  to  each  other,  such 
that,  if  A  and  B  have  a  G.C.M. ,  G,  then 

LA  +  MB  =  G ; 

and,  if  A  and  B  be  prime  to  each  other, 

LA  +  MB=1. 

To  prove  this,  we  show  that  any  one  of  the  remainders  in 
the  process  for  finding  the  G.C.M.  of  A  and  B  may  be  put  into 
the  form  PA  +  QB,  where  P  and  Q  are  integral  functions  of  x. 

We  have,  from  the  equalities  of  §  5, 

E^A-Q.B  (1), 

E,  =  B  -  Q2E,  (2), 

E3  =  Ex  -  Q3E3  (3), 

Equation  (1)  at  once  establishes  the  result  for  Ei  (only  here 

P  =  l,  Q=  -Q,). 

From  (2),  using  the  value  of  Et  given  by  (1), 

E2  =  B  -  Q,(A  -  QtB)  =  (  -  Q3)A  +  (  +  1  +  Q.Q^B, 

which  establishes  the  result  for  E2. 

From  (3),  using  the  results  already  obtained,  we  get 

E3  =  A  -  Q,B  -  Q,3{(  -  Qg)A  +  (  +  1  +  QlQB)B} 
=  (1  +  QA)A  +  (-<&-  Q3  -  QIQ,Q3)B, 

which  establishes  the  result  for  E3,  since  Q,,  Q2,  Q3  are  all  in- 
tegral functions.  Similarly  we  establish  the  result  for  E4,  E6, 
&c. 

Now,  if  A  and  B  have  a  G.C.M.,  this  is  the  last  remainder 
which  does  not  vanish,  and  therefore  we  must  have 

G  =  LA  +  MB  (L), 


vi  ALGEBRAIC  PRIMENESS  121 

where  L  and  M  are  integral  functions  ;  and  these  must  be  prime 
to  each  other,  for,  since  G  divides  both  A  and  B,  A/G  (  =  a  say) 
and  B/'G  (  =  b  say)  are  integral  functions ;  we  have  therefore, 
dividing  both  sides  of  (I.)  by  G-, 

1  =  La  +  M5  ; 

so  that  any  common  divisor  of  L  and  M  would  divide  unity. 

If  A  and  B  have  no  G.C.M.,  the  last  remainder,  Rrt,  is  a 
constant ;  and  we  have,  say,  Rn  =  L' A  +  M'B,  where  L'  and  M' 
are  integral  functions.  Dividing  both  sides  by  the  constant  Rn, 
and  putting  L  =  L'/Rw,  M  =  M'/Rn,  so  that  L  and  M  are  still 
integral  functions,  we  have 

1  =  LA  +  MB  (II.). 

Here  again  it  is  obvious  that  L  and  M  have  no  common  divisor, 
for  such  divisor,  if  it  existed,  would  divide  unity. 

The  proposition  just  proved  is  of  considerable  importance  in 
algebraical  analysis.  We  proceed  to  deduce  from  it  several  con- 
clusions, the  independent  proof  of  which,  by  methods  more 
analogous  to  those  of  chap,  iii.,  §  10,  we  leave  as  an  exercise 
to  the  learner.  Unless  the  contrary  is  stated,  all  the  letters 
used  denote  integral  functions  of  x. 

§  12.]  If  X  be  prime  to  B,  then  any  common  divisor  of  AH  and 
B  must  divide  H. 

For,  since  A  is  prime  to  B,  Ave  have 

LA  +  MB=1, 
whence 

LAH  +  MBH  =  H, 

which  shows  that  any  common  divisor  of  AH  and  B  divides  H. 

If  A  and  B  have  a  G.C.M.  a  somewhat  different  proposition 
may  be  established  by  the  help  of  equation  (I.)  of  §  11.  The 
discovery  and  proof  of  this  may  be  left  to  the  reader. 

Cor.  1.  IfB  divide  AH  and  be  prime  to  A,  it  must  divide  H. 

Cor.  2.  If  A'  be  prime  to  each  of  the  functions  A,  B,  0,  <&c,  it 
is  prime  to  their  product  ABC  .  .  . 


122  ALGEBRAIC  PPJMENESS  chav. 

Cor.  3.  If  each  of  the  functions  A,  B,  C,  .  .  .  be  prime  to  each 
of  the  functions  A',  B',  C,  .  .  .  ,  then  the  product  ABC  . . .  is  prime 
to  the  product  A'B'C  .  .  . 

Cor.  4.  If  A  be  prime  to  A',  then  Aa  is  prime  to  A'a',  a  and  a' 
being  any  positive  integers. 

Cor.  5.  If  a  given  set  of  integral  functions  be  each  resolved  into  a 
product  of  powers  of  the  integral  factors  A,  B,  C,  .  .  .,  which  are 
prime  to  each  other,  then  the  G.C.M.  of  the  set  is  found  by  uniting 
down  the  product  of  cdl  the  factors  that  are  common  to  all  the  given 
functions,  each  raised  to  the  lowest  power  in  which  it  occurs  in  any  of 
these  functions. 

This  is  a  generalisation  of  §  3  above. 

After  what  has  been  done  it  seems  unnecessary  to  add  de- 
tailed proofs  of  these  corollaries. 


LEAST   COMMON    MULTIPLE. 

§  13.]  Closely  allied  to  the  problem  of  finding  the  G.C.M.  of 
a  set  of  integral  functions  is  the  problem  of  finding  the  integral 
function  of  least  degree  which  is  divisible  by  each  of  them.  This 
function  is  called  their  least  common  multiple  (L.C.M.). 

§  14.]  As  in  the  case  of  the  G.C.M.,  the  degree  may,  if  we 
please,  be  reckoned  in  terms  of  more  variables  than  one ;  thus 
the  L.C.M.  of  the  monomials  Sx3yz2,  6.c2?/V,  8xyzu,  the  variables 
being  x,  y,  z,  u,  is  xsy3z*u,  or  any  constant  multiple  thereof. 

The  general  rule  clearly  is  to  write  down  all  the  variables,  each 
raised  to  the  highest  power  in  which  it  occurs  in  any  of  the  mono- 
mials. 

§  15.]  Confining  ourselves  to  the  case  of  integral  functions 
of  a  single  variable  x,  let  us  investigate  what  are  the  essential 
factors  of  every  common  multiple  of  two  given  integral  functions 
A  and  B.  Let  G  be  the  G.C.M.  of  A  and  B  (if  they  be  prime 
to  each  other  we  may  put  G  =  1)  ;  then 

A  =  aG,     B  =  bG, 

where  a  and  b  are  two  integral  functions  which  are  prime  to  each 


vi  LEAST  COMMON  MULTIPLE  123 

other.     Let  M  be  any  common  multiple  of  A  and  B.     Since  M 
is  divisible  by  A,  we  must  have 

M  =  PA, 

where  P  is  an  integral  function  of  x. 

Therefore  M  =  PaG. 

Again,  since  M  is  divisible  by  B,  that  is,  by  bG,  therefore 
M/bG,  that  is,  TaG/bG,  that  is,  ~Pa/b  must  be  an  integral  function. 
Now  b  is  prime  to  a;  hence,  by  §  12,  b  must  divide  P,  that  is, 
P  =  GJ),  where  Q  is  integral.      Hence  finally 

M  =  QabG. 

This  is  the  general  form  of  all  common  multiples  of  A  and  B. 

Now  a,  b,  G  are  given,  and  the  part  which  is  arbitrary  is  the 
integral  function  Q.  Hence  we  get  the  least  common  multiple 
by  making  the  degree  of  Q  as  small  as  possible,  that  is,  by  making 
Q  any  constant,  unity  say.  The  L.C.M.  of  A  and  B  is  therefore 
abG,  or  (aG)(bG)/G,  that  is,  AB/G.  In  other  words,  the  L.C.M. 
of  two  integral  functions  is  their  product  divided  by  their  G.C.M. 

§  16.]  The  above  reasoning  also  shows  that  every  common 
multiple  of  two  integral  functions  is  a  multiple  of  their  least  common 
multiple. 

The  converse  proposition,  that  every  multiple  of  the  L.C.M. 
is  a  common  multiple  of  the  two  functions,  is  of  course  obvious. 

These  principles  enable  us  to  find  the  L.C.M.  of  a  set  of  any 
number  of  integral  functions  A,  B,  C,  D,  &c.  For,  if  we  find 
the  L.C.M.,  L!  say,  of  A  and  B;  then  the  L.C.M.,  L2  say,  of  L, 
and  C ;  then  the  L.C.M.,  L3  say,  of  L2  and  D,  and  so  on,  until  all 
the  functions  are  exhausted,  it  follows  that  the  last  L.C.M.  thus 
obtained  is  the  L.C.M.  of  the  set. 

§  17.]  The  process  of  finding  the  L.C.M.  has  neither  the 
theoretical  nor  the  practical  importance  of  that  for  finding  the 
G.C.M.  In  the  few  cases  where  the  student  has  to  solve  the 
problem  he  will  probably  be  able  to  use  the  following  more  direct 
process,  the  foundation  of  which  will  be  obvious  after  what  has 
been  already  said. 

If  a  set  of  integral  functions  can  all  be  exhibited  as  powers  of  a 


124  EXERCISES  X  CHAP. 

set  of  integral  factors  A,  B,  C,  &e.,  which  are  either  all  of  the  1st 
degree  and  all  different,  or  else  are  all  prime  to  each  other,  then  the 
L.C.M.  of  the  set  is  the  product  of  all  these  factors,  each  being  raised 
to  the  highest  power  in  which  it  occurs  in  any  of  the  given  functions. 

For  example,  let  the  functions  be 

(,r-l)2(a;2  +  2)3(a:2  +  a-  +  l), 

(x-l)5{x-2)3(x-BY(x2  +  x  +  l)3, 
then,  by  the  above  rule,  the  L.C.M.  is 

(x-l)5(x-2)5(x-Z)i(x2+2f(x2  +  x  +  lf(x"-x  +  l)\ 

Exercises  X. 

Find  the  G.C.M.  of  the  following,  or  else  show  that  they  have  no  CM. 

(1.)  (x2-lf,     x6-l. 

(2.)  a:6-l,     xi-2x3  +  Zx2-2x  +  \. 

(3.)  z*-x2  +  l,     a-4  +  ar  +  l. 

(4.)  jc9  +  1,     xll  +  h 

(5.)  a?-x2-8x  +  \2,     sP+ia?- 3x- 18. 

(6.)  a:4-7a:3-22a:2  +  139x  +  105,     xA -8x* -Ux2  +  \l6x  +  70. 

(7.)  a4 -286a:2 +  225,     x*  +  140?-  480a:2-  690a:  -  225. 

(8.)  x6-x*-8x2  +  12,     a;6  +  4a;4 -3a;2 -18. 

(9.)  x> - 2a:4 -  2a:3  +  4ar  +  x -2,     x5  +  2xi -2x"' -  8x2-7x-2. 

(10.)  xs  +  6x6  -  8.C4  + 1 ,     a:12  +  7a:10  -  3a?  -  3a:2  -  2. 

(11.)  12x3  +  lBx2  +  6x  +  l,     16a:3  +  16a:2  +  7a:  +  l. 

(12.)  5ar3  +  38a:2  -195a;  -600,     4a;3-  15a:2-  38a; +  65. 

(13.)  16a4  -  56a,-3- 88a;2  +  278a; +105,     16a;4 -  64a;3  -  44a;2  +  232a; +  70. 

(14.)  7a4  +  6a:3 -8a;2- 6a; +  1,      lla:4+ 15a;3- 2a:2- 5;<;+ 1. 

(15.)  a4  +  64a4,     (a;  +  2a)4- 16«4. 

(16.)  9a;4+4a;2  +  l,     Zsj2x3  +  x2+l. 

(17.)  a;3  +  3i?a;2  -  (1  +  3p),     px3  -  3(  1  +  Zp)x  +  (3  +  8p). 

(18. )  x3  -  3(a  -  b)x2  +  (4a2  -  Zab)x  -  2a°{2a  -  3b), 

xi-{3a  +  b)x3+{5a2  +  2ab)x2-a2(5a  +  3b)x  +  2a3{a  +  b). 

(19. )  7iaf+1  -  (it  +  l)xn  + 1,     a"'  -  nx+{n  -  1 ). 

(20.)  Show  that  ar3+^a:2  +  g'a;  +  l,  x3  +  qx2  +  px  + 1  cannot  have  a  common 
measure,  unless  either  p  =  q  or  p  +  q  +  2  =  0. 

(21. )  Show  that,  if  ax2  +  bx  +  c,  ex2  +  bx  +  a  have  a  common  measure  of  the 
1st  degree,  then  a±b  +  c  —  0. 

(22.)  Find  the  value  of  a  for  which  {x3-aa;2  +  19a'-«-  4]  /{a:3-  (a+l)a-2 
+  23a;-a-7}  admits  of  being  expressed  as  the  quotient  of  two  integral 
functions  of  lower  degree. 

(23.)  If  ax3  +  3bx2  +  d,  bx3  +  Bdx  +  e  have  a  common  measure,  then 
(ae -4bd)3  =  27  {ad2 +  b2e)2. 


VI  EXERCISES  X  125 

(24.)  Ax2  +  Bxy  +  Cy2,  Ba?  -  2(A  -  C)xy  -  By8  cannot  have  a  common 
measure  unless  the  first  be  a  square. 

(25.)  ax3  +  bx2  +  cx  +  d,  dx3  +  cx2  +  bx  +  a  will  have  a  common  measure  of 
the  2nd  degree  if 

abc  -  a"b  -  b2d  +  acd     ac2  -  bed  -  a3  +  ad2     d(ac  -  b<l) 
ac-bd  ab-cd  a2-d? 

show  that  these   conditions  are  equivalent  to  only  one,  namely,    ac~bd  = 
or  -  dr. 

(26.)  Find  two  integral  functions  P  and  Q,  such  that 

P(^2  -  Zx  +  2)  +  Q(.x2  +  x  + 1)  =  1. 

(27.)  Find  two  integral  functions  P  and  Q,  such  that 

P(2^-7a;2  +  7^-2)  +  Q(2^  +  a;2  +  x-l)  =  2a;-l. 

Find  the  L.C.  M.  of  the  following  : — 

(28.)  a5-ab\     a?+a*b,     a6  +  b(i  +  a2b"-(a2  +  b2). 

(29.)  x3-x2-Ux  +  24,     x3 -2x2 -5x  +6,     x2-4a-  +  3. 

(00.)  3x3  +  x2-8x  +  4,     3x3  +  7x2-4,     x3  +  2a:2  -  x  -  2,     dx3  +  2,r2  -  3r  -  2. 

(31. )  x3  -  V2x  + 16,     xA  -  i.r3  -  x2  +  20,r  -  20,     x*  +  3x3  -  llx2  -  3x  +  10. 

(32.)  x6  +  2ax5  +  a2x4  +  5a5x  +  a6)     x3  +  crx  -  ax2  -  a3. 

(33.)  If  x2  +  ax  +  b,  x2  +  a'x  +  b'  have  a  common  measure  of  the  1st 
degree,  then  their  L.C.M.  is 

,     ab-a'V   .      /      ,     [b-V\*\      ,  ,.,«-«' 

(34.)  Show  that  the  L.C.M.  of  two  integral  functions  A  and  B  can  always 
be  expressed  in  the  form  PA  +  QB,  where  P  and  Q  are  integral  functions. 


CHAPTEE    VII. 

On  the  Resolution  of  Integral  Functions  into 

Factors. 

§  1.]  Having  seen  how  to  determine  whether  any  given 
integral  function  is  a  factor  in  another  or  not,  and  how  to  deter- 
mine the  factor  of  highest  degree  which  is  common  to  two  in- 
tegral functions,  it  is  natural  that  we  should  put  to  ourselves 
the  question,  How  can  any  given  integral  function  be  resolved 
into  integral  factors  ? 

TENTATIVE   METHODS. 

§  2.]  Confining  ourselves  at  present  to  the  case  where 
factors  of  the  1st  degree,  whose  coefficients  are  rational  integral 
functions  of  the  coefficients  of  the  given  function,  are  suspected 
or  known  to  exist,  we  may  arrive  at  these  factors  in  various  ways. 

For  example,  every  known  identity  resulting  from  the  distri- 
bution of  a  product  of  such  factors,  when  read  backwards,  gives 
a  factorisation. 

Thus  (x  +  y)  (x  -  y)  —  x2  -  y"  tells  us  that  of  -  y2  may  be  re- 
solved into  the  product  of  two  factors,  x  +  y  and  x  —  y.  In  a 
similar  way  we  learn  that  x  +  y  +  z  is  a  factor  in  x3  +  y3  +  z3  —  3xyz. 
The  student  should  again  refer  to  the  tables  of  identities  given 
on  pp.  81-83,  and  study  it  from  this  point  of  view. 

When  factors  of  the  1st  degree  with  rational  integral 
coefficients  are  known  to  exist,  it  is  usually  not  difficult  to  find 
them  by  a  tentative  process,  because  the  number  of  possible 
factors  is  limited  by  the  nature  of  the  case. 


chap,  vii         TENTATIVE  FACTORISATION EXAMPLES  127 

Example  1. 

Consider  a,2-12x  +  32,  and  let  us  assume  that  it  is  resolvable  into  (x-a) 
{x-b). 

Then  we  have 

a-2  -  12a!  +  32  =  x-  -  (a  +  b)x  +  ab, 

and  we  have  to  find  a  and  b  so  that 

«6=+32,  a  +  b- +12. 
"We  remark,  first,  that  a  and  b  must  have  the  same  sign,  since  their  pro- 
duct is  positive  ;  and  that  that  sign  must  be  +,  since  their  sum  is  positive. 
Further,  the  different  ways  of  resolving  32  into  a  product  of  integers  are 
1x32,  2x16,  4x8;  and  of  these  we  must  choose  the  one  which  gives 
a  +  b=  +12,  namely,  the  last,  that  is,  a  =  4,  b  —  8. 
So  that 

a-2-12a-  +  32  =  (a--4)(a--8). 
Example  2. 

x3  -  2a-2  -  23a:  +  60  =  (x  -a)(x-  b)  (x  -  c)  say. 
Here  -  abc  —  +  60. 

Now  the  divisors  of  60  are  1,  2,  3,  4,  5,  6,  10,  12,  15,  20,  30,  60  ;  and  we 
have  therefore  to  try  a-±l,  a1  ±2,  x±3,  &c.  The  theorem  of  remainders 
(chap.  v. ,  §  14)  at  once  shows  that  x  + 1,  x  - 1,  x  +  2,  x  -  2,  are  all  inadmissible. 
On  the  other  hand,  for  a- -3  we  have  (see  chap,  v.,  §  13) 

1-2-23  + GO 
0  +  3+    3-60 


1  +  1-20+   0 
that  is,  a- -3  is  a  factor  ;  and  the  other  factor  is  a;2  +  a;-20,  which  we  resolve 
by  inspection,  or  as  in  Example  1,  into  {x-  4)  {x  +  5). 
Hence  x*  -  2a-2  -  23a-  +  60  =  {x  -  3)  (a-  -  4)  (x  +  5). 

Example  3. 

&x-  -  1 9x  + 1 5  =  (ax  +  b)(cx  +  d). 

Here  ac=  +6,  bd=+  15  ;  and  we  have  more  cases  to  consider.  "We  might 
have  anyone  of  the  32  factors,  a;±l,  a; ±3,  a' ±5,  a' ±15,  2a; ±1,  2a- ±3, 
2x  ±  5,  2xzk  15,  &c.  A  glance  at  the  middle  coefficient,  -  19,  at  once  excludes 
a  large  number  of  these,  and  we  find,  after  a  few  trials, 
6x°-  -  19a-  +  15  =  (2a-  -  3)  (3a-  -  5). 
§  3.]  In  cases  like  those  of  last  section,  we  can  often  detect 
a  factor  by  suitably  grouping  the  terms  of  the  given  function. 
For  it  follows  from  the  general  theory  of  integral  functions 
already  established  that,  if  P  can  be  arranged  as  the  sum  of  a 
series  of  groups  in  each  of  which  Q  is  a  factor,  then  Q  is  a  factor 
in  P ;  and,  if  P  can  be  arranged  as  the  sum  of  a  series  of  groups 
in  each  of  which  Q  is  a  factor,  plus  a  group  in  which  Q  is  not  a 
factor,  then  Q  is  not  a  factor  in  P. 


128 


FACTORISATION  OF 


CHAP. 


Example  1. 

x3  -  2x"  -  23a;  +  60 

=  .>•■-(./■-  2)  -23(a:-  2)  +  14, 

that  is,  x  -  2  is  not  a  factor. 

a;3 -2«2 -23a- +  60 

=  a"(a;-3)+a:2-23a:  +  60 

=  x2(x-3)  +  x(x-Z)  -  20a;+  60 

=  x2{x  -  3)  +  x(x  -  3)  -  20(a;  -  3), 

that  is,  a; -3  is  a  factor. 

Example  2. 

-])x2  +  xy+pqxy  +  qy2 
=  x{px  +  y)  +  qy(px  +  y) , 
that  is,  px  +  y  is  a  factor,  the  other  being  x  +  qij. 

Example  3. 

x3  +  (m  +  n  + 1  )a,"a  +  (m  +  ?i  +  mn)xa2  +  mna? 
=  x3  +  a;2a  +  (w  +  ?i)  (ara  +  xa2)  +  mn(xa2  +  «3) 
=  ar^ai  +  a)  +  (m  +  n)xa(x  +  a)  +  mna2{x  +  a) 
=  {a;2  +  (m  +  yi)a'a  +  mrea2}  (x  +  a) 
=  {x(x  +  via)  +  ?ta(a;  +  ma)}  (x  +  a) 
=  (x  +  ma)  (x  +  ?ia)  (x  +  a). 


GENERAL    SOLUTION    FOR   A    QUADRATIC    FUNCTION. 

§  4.]  For  tentative  processes,  such  as  Ave  have  been  illustrat- 
ing, no  general  rule  can  be  given;  and  skill  in  this  matter  is  one 
of  those  algebraical  accomplishments  which  the  student  must 
cultivate  by  practice.  There  is,  however,  one  case  of  great  im- 
portance, namely,  that  of  the  integral  function  of  the  2nd  degree 
in  one  variable,  for  which  a  systematic  solution  can  be  given. 

We  remark,  first  of  all,  that  every  function  of  the  form 
x'+px  +  q  can  De  made  a  complete  square,  so  far  as  x  is  con- 
cerned, by  the  addition  of  a  constant.  Let  the  constant  in 
question  be  a,  so  that  we  have 

x2  +  px  +  q  +  a  =  (./•  +  /5)2  =  x"  +  2  fix  +  f32, 
(3  being  by  hypothesis  another  constant.     Then  we  must  have 

p  =  2f3,     q  +  a  =  ft2. 
The  first  of  these  equations  gives  (3-2>j2,  the  second  a  =  /32  -q 
-  (jpffi  ~  '1-    Thus  our  problem  is  solved  by  adding  to  x2  +px  +  q 
the  constant  (jj/2)2  -  q. 


vii  A  QUADRATIC  FUNCTION  129 

The  same  result  is  obtained  for  the  more  general  form, 
ax*  +  bx  +  c,  as  follows  : — 

2      ,  /  2     6         c 

ax  +  bx  +  c  =  a[x  +  -  x  +  - 

\        a       a 

Now,  from  the  case  just  treated,  we  see  that  x2  +  (b/a)x  +  c/a  is 
made  a  complete  square  in  x  by  the  addition  of  (b/2a)2  —  c/a, 
that  is,  (b2  -  4:0c)/iaa.  Hence  ax2  +  bx  +  c  will  be  made  a  com- 
plete square  in  x  by  the  addition  of  a(b2  —  lac)/ la2,  that  is, 
(b2  -  lac)/ la.     We  have,  in  fact, 

,     ,  b2-iac       (        b\2 

ax  +  bx  +  c  +  — ; =  a[x  +  -—)  ■ 

la  \       2aJ 

§  5.]  The  j)rocess  of  last  article  at  once  suggests  that 
aaf  +  bx  +  c  can  always  be  put  into  the  form  a{(x  +  I)2  -  m2}, 
where  I  and  m  are  constant. 

In  point  of  fact  we  have 

2i  f   «     b       c  ) 

ax  +  bx  +  c  =  a<  x~  +  - x  +  -  > 
I         a       a  ) 

..I  ,t+9>  .+  (*)'.(>)'+:] 

{  2a        \2aJ        \2aJ       a  ) 

In  other  words,  our  problem  is  solved  if  we  make  I  =  b/2a  and 
find  m,  so  that  m2  =  (b2  -  iac)/ia2. 

This  being  done,  the  identity  X2  -  A2  =  (X  -  A)  (X  +  A)  at 
once  gives  us  the  factorisation  of  ax2  +  bx  +  c ;  for  we  have 

ax2  +  bx  +  c  =  a  {(x  +  I)2  -  m2 } 

=  a  {(x  +  1)  +  m }  {(x  +  /)  -  m  }. 
Example  1. 
Consider  6x2-  19a; +  15  ;  we  have 

-{'-S-*(S)'-S*¥} 

19  / 1  \2  1 

Here  1=  -  — ,  and  m-=  (  —  )   ;  so  that  our  problem  is  solved  if  we  take  w  =  —  • 

VOL.  I  K 


130  REAL  ALGEBRAICAL  QUANTITY  chap. 

We  get,  therefore, 

"— +M(-S)4}{(--S)-£} 

=<¥)(^) 

=  (2as-3)(3«-5); 

the  same  result  as  we  obtained  above  (in  §  2,  Example  3),  by  a  tentative 
process. 

Example  2. 

Consider  x6  -  5x3  +  6.     We  may  regard  this  as  (x3)2  -  5(,r3)  +  6,  that  is  to 
say,  as  an  integral  function  of  x3  of  the  2nd  degree.     We  thus  see  that 

x6-5x3  +  6  =  (x3)2~5(xs)  +  6, 
=  (.k3-3)(.b3-2). 

INTRODUCTION    INTO    ALGEBRA    OF    SURD    AND 
IMAGINARY    NUMBERS. 

§  6.]  The  necessities  of  algebraic  generality  have  already  led 
us  to  introduce  essentially  negative  quantity.  So  far,  algebraic 
quantity  consists  of  all  conceivable  multiples  positive  or  negative 
of  1.  To  give  this  scale  of  quantity  order  and  coherence,  we 
introduce  an  extended  definition  of  the  words  greater  than  and 
less  than,  as  follows  : — a  is  said  to  be  greater  or  less  than  b,  according 
as  a-  b  is  positive  or  negative. 

Example. 

( +3)  -  ( +  2)=  + 1  therefore  +  3  >  +  2  ;  (-3) -(-5)  =+2  therefore  -  3  >  -  5  ; 
(  +  3)  -  (  -  5)  =  +  8  therefore  +3> -5;  (-7) -(-3)=  -  4  therefore  -7<  -3. 

Hence  it  appears  that,  according  to  the  above  definition,  any 
negative  quantity,  however  great  numerically,  is  less  than  any 
positive  quantity,  however  small  numerically ;  and  that,  in  the 
case  of  negative  quantities,  descending  order  of  numerical  magni- 
tude is  ascending  order  of  algebraical  magnitude. 

We  may  therefore  represent  the  whole  ascending  series  of 
algebraical  quantity,  so  far  as  we  have  yet  had  occasion  to  con- 
sider it,  as  follows  : — 


-   CO 


1  *  ..-£...  0  ...+£...  +1  ...+  oo 


* 


t 

*  The  symbol  oo  is  here  used  as  an  abbreviation  for  a  real  quantity  as 
great  as  we  please. 


vii  RATIONAL  AND  SURD  QUANTITY  131 

The  most  important  part  of  the  operations  in  the  last  para- 
graph is  the  finding  of  the  quantity  m,  whose  square  shall  be  equal 
to  a  given  algebraical  quantity.  We  say  algebraical,  for  we  must 
contemplate  the  possibility  of  (b2  -  4ac)/4as,  say  k  for  shortness, 
assuming  any  value  between  -  <x>  and  +  qo  .  When  m  is  such  that 
in2  =  k,  then  in  is  called  the  square  root  of  k,  and  we  write  in  =  \/k. 
We  are  thus  brought  face  to  face  with  the  problem  of  finding 
the  square  root  of  any  algebraical  quantity  ;  and  it  behoves  us 
to  look  at  this  question  somewhat  closely,  as  it  leads  us  to  a  new 
extension  of  the  field  of  algebraical  operations,  similar  to  that 
which  took  place  when  we  generalised  addition  and  subtraction 
and  thus  introduced  negative  quantity. 

1st.  Let  us  suppose  that  k  is  a  positive  number,  and  either 

a  square  integer  =  +  k,  say,  or  the  square  of  a  rational  number 

=  +  (*/A)2,  say,  where  k  and  A  are  both  integers,  or,  which  is 

the  same  thing  [since  (k/X)2  =  k'/'A2],  the  quotient  of  two  square 

integers.     Then  our  problem  is  solved  if  we  take 


in  the  one  case,  or 


m  —  +  k,  or  m  =  -  k 

m  =  +  k/X,  or  m  -  -  k/X 


in  the  other ; 

for  m*  -  (  ±  «)2  =  k  =  k, 


in 


-(^■-©■-* 


which  is  the  sole  condition  required. 

It  is  interesting  to  notice  that  we  thus  obtain  two  solutions 
of  our  problem  ;  and  it  will  be  afterwards  shown  that  there  are 
no  more.  Either  of  these  will  do,  so  far  as  the  problem  of 
factorisation  in  §  5  is  concerned,  for  all  that  is  there  required  is 
any  one  value  of  the  square  root. 

More  to  the  present  purpose  is  it  to  remark  that  this  is  the 
only  case  in  which  m  can  be  rational;  for  if  m  be  rational,  that 
is,  =  ±  k/X  where  k  and  A  are  integers,  then  m2  =  (k/A)3,  that  is, 
k  =  (k/X)2,  that  is,  k  must  be  the  square  of  a  rational  number. 

2nd.  Let  k  be  positive,  but  not   the   square   of   a   rational 


132  DEFINITION  OF  THE  IMAGINARY  UNIT  i  CHAP. 

number ;  then  everything  is  as  before,  except  that  no  exact 
arithmetical  expression  can  be  found  for  m.  We  can,  by  the 
arithmetical  process  for  finding  the  square  root,  find  a  rational 
value  of  m,  say  v,  such  that  m2  =  ( ±  v)2  shall  differ  from  k  by 
less  than  any  assigned  quantity,  however  small ;  but  no  such 
rational  expression  can  be  absolutely  exact.  In  this  case  m 
is  called  a  surd  number.  When  k  is  positive,  and  not  a  square 
number,  as  in  the  present  case,  it  is  usual  to  use  \/k  to  denote 
the  mere  (signless)  arithmetical  value  of  the  square  root,  which 
has  an  actual  existence,  although  it  is  not  capable  of  exact  arith- 
metical expression ;  and  to  denote  the  two  algebraical  values  of 
m  by  ±  \/k.  Thus,  if  k  =  +  2,  we  write  m  =  ±  v/2.  In  any 
practical  application  we  use  some  rational  approximation  of 
sufficient  accuracy ;  for  example,  if  k  =  +  2,  and  it  is  necessary 
to  be  exact  to  the  l/10,000th,  we  may  use  m-  ±  1-4142. 

A  special  chapter  will  be  devoted  to  the  discussion  of  surd 
numbers ;  all  that  it  is  necessary  in  the  meantime  to  say  further 
concerning  them  is,  that  they,  or  the  symbols  representing  them, 
are  of  course  to  be  subject  to  all  the  laws  of  ordinary  algebra.! 

3rd.  Let  k  be  negative  =  -  k',  say,  where  k'  is  a  mere  arith- 
metical number.  A  new  difficulty  here  arises ;  for,  since  the 
square  of  every  algebraical  quantity  between  -  co  and  +  oo  (ex- 
cept 0,  which,  of  course,  is  not  in  question  unless  k'  =  0)  is 
positive,  there  exists  no  quantity  m  in  the  range  of  algebraical 
quantity,  as  at  present  constituted,  which  is  such  that  m2  =  -  k'. 
If  we  are  as  hitherto  to  maintain  the  generality  of  all  algebraical 
operations,  the  only  resource  is  to  widen  the  field  of  algebraical  quantity 
still  farther.  This  is  done  by  introducing  an  ideal,  so-called  imaginary, 
unit  commonly  denoted  by  the  letter  i*  whose  definition  is,  that  it  is 
such  that 

i2=  -1. 

It  is,  of  course,  at  once  obvious  that  i  has  no  arithmetical 
existence  whatsoever,  and  does  not  admit  of  any  arithmetical 
expression,  approximate  or  other.  We  form  multiples  and  sub- 
multiples  of  this  unit,  positive  or  negative,  by  combining  it  with 

*  Occasionally  also  by  t.  t  See  vol.  ii.  chap.  xxv.  §  28-41. 


VII 


COMPLEX  NUMBERS  133 


quantities  of  the  ordinary  algebraical,  now  for  distinction  called 

real,  series,  namely, 

-oo...   -1...-|...0.  ..+!•..   +1...+CO. 
We  thus  obtain  a  new  series  of  purely  imaginary  quantity : — 
—  oo  *...—  *..  .  -  \i.  .  .  0* .  .  .  +  \i .  .  .  +  i  , .  .  +  co  i. 

These  new  imaginary  quantities  must  of  course,  like  every  other 
quantity  in  the  science,  be  subject  to  all  the  ordinary  laws  of 
algebra  when  combined  either  with  real  quantities  or  with  one 
another.  All  that  the  student  requires  to  know,  so  far  at  least  as 
operations  with  them  are  concerned,  beyond  the  laws  already  laid 
down,  is  the  defining  property  of  the  new  unit  i,  namely,  i2  —  —  1. 

When  purely  real  and  purely  imaginary  numbers  are  com- 
bined by  way  of  algebraical  addition,  forms  arise  like!?  +  qi,  where 
P  and  q  are  real  numbers  positive  or  negative.  Such  forms  are 
called  complex  numbers ;  and  it  will  appear  later  that  every  alge- 
braical function  of  a  complex  number  can  itself  be  reduced  to 
a  complex  number.  In  other  words,  it  comes  out  in  the  end 
that  the  field  of  ordinary  algebraical  quantity  is  rendered  com- 
plete by  this  last  extension. 

The  further  consequences  of  the  introduction  of  complex 
numbers  will  be  developed  in  a  subsequent  chapter.  In  the 
meantime  we  have  to  show  that  these  ideal  numbers  suffice  for 
our  present  purpose.  That  this  is  so  is  at  once  evident ;  for,  if 
we  denote  by  »Jk'  the  square  root  of  the  arithmetical  number 
k\  so  that  ijk'  may  be  either  rational  or  surd  as  heretofore,  but 
certainly  real,  then  m  -  ±i  Jk'  gives  two  solutions  of  the  problem 
in  hand,  since  we  have 

m2  =  (  ±  i  Jk')2 

=  (  ±  i  Jk')  x  (  ±  i  Jk'), 
upper  signs  going  together  or  lower  together, 

=  (i2)  x  ( </V  Y 
=  (-l)x(*') 

=  -k\ 

§  7.]  We  have  now  to  examine  the  bearing  of  the  discus- 
sions of  last  paragraph  on  the  problem  of  the  factorisation  of 
ax2  +  bx  +  c. 


134  FACTORISATION  OF  QUADRATIC  chap. 

It  will  prevent  some  confusion  in  the  mind  of  the  student  if 
we  confine  ourselves  in  the  first  place  to  the  supposition  that  a,  b,  c 
denote  positive  or  negative  rational  numbers.  Then  I  =  bj2a  is  in  all 
cases  a  real  rational  number,  and  we  have  the  following  cases  : — 

1st.  If  b2  -  4ac  is  the  positive  square  of  a  rational  number, 
then  m  has  a  real  rational  value,  and 

ox2  +  bx  +  c  =  a(z  +  I  +  m)(x  +  I  -  m) 
is  the  product  of  two  linear  factors  whose  coefficients  are  real  rational 
numbers.    Example  1,  §  5,  will  serve  as  an  illustration  of  this  case. 

2nd.  If  b2  —  iac  is  positive,  but  not  the  square  of  a  rational 
number,  then  m  is  real,  but  not  rational ;  and  the  coefficients  in 
the  factors  are  irrational. 

Example  1. 

x2  +  2x-l=x"  +  2x  +  l-2, 
=  (a;  +  l)2-(V2)2, 
=  (x  +  l  +  yj2)(x  +  l-^2). 

3rd.   If  b2  -  iac  is  negative,  then  m  is  imaginary,  and  the 
coefficients  in  the  factors  are  complex  numbers. 
Example  2. 


Example  3. 


a:2  +  2a:  +  5  =  a:2  +  2a'  +  l  +  4, 
=  (a-  +  l)2-(2i)2, 
=  {x  +  l  +  2i){x  +  l-2i). 


x-  +  2x  +  3  =  x2  +  2x  +  l  +  2, 

=  (x  +  lf-(i^2T~, 

=  (x  + 1  +  i\j2)  (x  + 1  --  i  V2). 

4th.  There  is  another  case,  which  forms  the  transition 
between  the  cases  where  the  coefficients  in  the  factors  are  real 
and  the  case  where  they  are  imaginary. 

If  b2  -  iac  =  0,  then  m  =  0, 
and  we  have  ax2  +  bx  +  c  =  a(x  +  I)2 ; 

in  other  words,  ax2  +  bx  +  c  is  a  complete  square,  so  far  as  x  is 
concerned.  The  two  factors  are  now  x  +  I  and  x  +  I,  that  is, 
both  real,  but  identical. 

We   have,   therefore,  incidentally  the  important   result  that 

ax2  +  bx  +  c  is  a  complete  square  in  x  ij '  tf  -  4ac  =  0. 

Example  4. 

3a;2  -  3a;  + 1  =  3(a;2  -  2.  \x  +  J),  =  8(»  -  h)2- 

*  I'^-iac  is  called  the  Discriminant  of  the  quadratic  function  ax-  +  bx+c. 


vil  FUNCTIONS  RESUMED  135 

§  8.]  There  is  another  point  of  view  which,  although  usually 
of  less  importance  than  that  of  last  section,  is  sometimes  taken. 

Paying  no  attention  to  the  values  of  a,  b,  c,  but  regarding 
them  merely  as  functions  of  certain  other  letters  which  they  may 
happen  to  contain,  we  may  inquire  under  what  circumstances  the 
coefficients  of  the  factors  will  be  algebraically  rational  functions  of 
those  letters. 

In  order  that  tins  may  be  the  case  it  is  clearly  necessary  and 
sufficient   that   b2  -  iac  be  a  complete  square  in  the  letters  in 
question,  =  P2  say. 
Then 

/        b       P\   /        b       P 
=  a  ( x  +  —  +  —  )  (x  +  —  -  — 

\       2a      la  J  \       2a      lo 

which  is  rational,  since  P  is  so. 

If  b2  -  iac  -  -  P2,  where  P  is  rational  in  the  present  sense, 
then 


/        b       P.\/        b       P  . 
=  a(x  +  — -  +  —  -n  (x  +  — -  -  —i 

V       2a      2a  /  \       2a      2a 

where  the  coefficients  are  rational,  but  not  real. 

Example  5. 

jtx2  +  {p  +  q)x-Jr  q 

«j»(«+i)(«+J). 

=  (x  +  l)(j>X  +  q); 

a  result  which  would,  of  course,  be  more  easily  obtained  by  the 
tentative  processes  of  §§  2,  3. 


136  HOMOGENEOUS  QUADRATIC  FUNCTIONS  chap. 

§  9.]  It  should  be  observed  that  the  factorisation  for 
ax2  +  bx  +  c  leads  at  once  to  the  factorisation  of  the  homogeneous 
function  ax2  +  bxy  +  cif  of  the  2nd  degree  in  two  variables  ;  for 

ax2  +  bxy  +  cf 

,f  z      b  ///"  -  lac  )    f  x      b  lb1  -  iuc  >  . 

(  /  b  lb2  -  \ac\     ")    f  /  b  lb1  -  4ac\    ) 

= "  { x+  (a; +  V  ~iH-"  \{r+  (s "  v  tt)  "I  • 

By  operating  in  a  similar  way  any  homogeneous  function  of 
two  variables  may  be  factorised,  provided  a  certain  non-homo- 
geneous function  of  one  variable,  having  the  same  coefficients, 
can  be  factorised. 

Example  1.   From 

a:2  +  2x  +  3={x+ 1  +  is/2)  {x  +  1  -  z'V2), 

we  deduce 

x2  +  2xy  +  3yn-  =  {x  +  (1  +  i\/2)y}  {x+(l  -  i\/2)y}. 
Example  2.   From 

xf  _  2x-  -  23a-  +  60  =  (x -  3) {x -  4)  (as  +  5), 
we  deduce 

a?  -  2a'2;/  -  23a-y2  +  60?/3  =  (.r  -  Zy)  [x  -  iy)  (x  +  5y). 

§  10.]  By  using  the  principle  of  substitution  a  great  many 
apparently  complicated  cases  may  be  brought  under  the  case  of 
the  quadratic  function,  or  under  other  equally  simple  forms. 
The  following  are  some  examples  : — 

Example  1. 
xt  +  xhf  +  y^^  +  y^-ixyT-, 

=  {x*+y*+xy)(x*+y*-xy), 

-{(•^'-(^^{(-W'-W}- 
-{.+G+^>}{.+G-^>H-+(-^>} 


vil  EXAMPLES  137 

Here  the  student  should  observe  that,  if  resolution  into  quadratic  factors  only 
is  required,  it  can  be  effected  with  real  coefficients  ;  but,  if  the  resolution  be 
carried  to  linear  factors,  complex  coefficients  have  to  be  introduced. 

Example  2. 

x3  +  y3={x  +  y)(x2-.ry  +  ij2) 


-*"»»{•+(-£+#>}{ 


-«-#>) 


Example  3. 

.<i  +  yi  =  (x2+y2)2-2x2y2 

=  (■<•-  +  j/2)2  -W-2xy? 

=  (x2  +  V&ey  +  y2)  [a?  -  ^2xy  +  y2). 

Again 

a?  +  s/2xy  +  y-=f  x  +  ^fy  Y +  ~y2 

V2  y  /V2. 


X+   21'       -\2iy 


x  +  ^(l  +  i)y]  {*+^(l-%}. 


The  similar  resolution  for  x2  -  \/2xy  +  y2  will  be  obtained  by  changing  the 
sign  of  \J2.     Hence,  finally, 

=  {^f(l  +  i)y}{^^l-i)y}{,-^lU)y}{x-^{l-i)y). 

Example  4. 

x^-i/^^y-iy6)2 

=  (xe-y,')(xG  +  yR) 

=  {(*2)3-(2/2)3}  {(*2)3  +  (ir)3} 

=  (x2  -  y2)  (x4  +  x2y2  +  y*)  (x2  +  y2)  (x*  -  x2y2  +  y4) 
=  {x  +  y){x-y)  (x  +  iy)  {x  -  iy)  (x4  +  x2y2  +  y*)  (x*  -  x2y2  +  y*), 
where  the  last  two  factors  may  be  treated  as  in  Example  1. 
Example  5. 

2i2c2  +  2cV  +  2a262  -  «4  -  ¥  -  c4 
=  4i2c2  -  (a-  -b2-  c2)2 
=  (2bc  +  a2  -  b2  -  c2)  (26c  -  d2  +  b2  +  c2) 
=  {a2-(b-c)2}  {(b  +  c)2-a2} 
=  (a  +  b  -  c)  (a  -  b  +  c)  (b  +  c  +  a)  (b  +  c  -  a). 


*  The  student  should  observe  that  the  decomposition  x2  +  y2  +  xy  = 
(x  +  y+  \Jxy)  (x  +  y-  \/xy),  which  is  often  given  by  beginners  when  they  are 
asked  to  factorise  x2  +  y2  +  xy,  although  it  is  a  true  algebraical  identity,  is  no 
solution  of  the  problem  of  factorisation  in  the  ordinary  sense,  inasmuch  as 

the  two  factors  contain  \Jxy,  and  are  therefore  not  rational  integral  functions 
of  a-  and  y. 


138  USE  OF  REMAINDER  THEOREM  chap. 


RESULTS  OF  THE  APPLICATION  OF  THE  REMAINDER  THEOREM. 

§  11.]  It  may  be  well  to  call  the  student's  attention  once 
more  to  the  use  of  the  theorem  of  remainders  in  factorisation. 
For  every  value  a  of  x  that  we  can  find  which  causes  the  integral 
function  f(x)  to  vanish  we  have  a  factor  x  -  a  off(x). 

It  is  needless,  after  what  has  been  shown  in  chap,  v.,  §§  13-16, 
to  illustrate  this  point  further. 

It  may,  however,  be  useful,  although  at  this  stage  we  cannot 
prove  all  that  we  are  to  assert,  to  state  what  the  ultimate  result 
of  the  rule  just  given  is  as  regards  the  factorisation  of  integral 
functions  of  one  variable.  If  f(x)  be  of  the  wth  degree,  its  coeffi- 
cients being  any  given  numbers,  real  or  imaginary,  rational  or 
irrational,  it  is  shown  in  the  chapter  on  Complex  Numbers 
that  there  exist  n  values  of  x  (called  the  roots  of  the  equation 
f(x)  =  0)  for  which  f(x)  vanishes.  These  values  will  in  general 
be  all  different,  but  two  or  more  of  them  may  be  equal,  and  one 
or  all  of  them  may  be  complex  numbers. 

If,  however,  the  coefficients  of  f(x)  be  all  real,  then  there 
will  be  an  even  number  of  complex  roots,  and  it  will  be  possible 
to  arrange  them  in  pairs  of  the  form  X  ±  jxi. 

It  is  not  said  that  algebraical  expressions  for  these  roots  in 
terms  of  the  coefficients  of  /(.<:)  can  always  be  found  ;  but,  if 
these  coefficients  be  numerically  given,  the  values  of  the  roots 
can  always  be  approximately  calculated. 

From  this  it  follows  that  f(x)  can  in  all  cases  be  resolved  into  n 
linear  *  factors,  the  coefficients  of  which  may  or  may  not  be  all  real. 

If  the  coefficients  of  f(x)  be  all  real,  then  it  can  be  resolved  into  a 
product  of  p  linear  and  q  quadratic  factors,  the  coefficients  in  all  of 
which  are  real  numbers  which  may  in  all  cases  be  calculated  approxi- 
mately. We  have,  of  course,  p  +  2q  =  n,  and  either  p  or  q  may  be 
zero. 

The  student  will  find,  in  §§  1-10  above,  illustrations  of  these 
statements  in  particular  cases ;   but  he  must  observe  that  the 

*    "  Linear"  is  used  here,  as  it  often  is,  to  mean  "of  the  1st  degree." 


VII  QUADRATIC  FUNCTION  WITH  TWO  VARIABLES  139 

general  problem  of  factorising  an  integral  function  of  the  nth. 
degree  is  coextensive  with  that  of  completely  solving  an  equation 
of  the  same  degree.  When  either  problem  is  solved  the  solution 
of  the  other  follows. 


FACTORISATION    OF   FUNCTIONS    OF   MURE    THAN    ONE    VARIABLE. 

§  12.]  Jflien  the  number  of  variables  exceeds  unity,  the  problem  of 
factorisation  of  an  integral  function  {excepting  special  cases,  such  as 
homogeneous  functions  of  two  variables)  is  not  in  general  soluble,  at 
least  in  ordinary  algebra. 

To  establish  this  it  is  sufficient  to  show  the  insolubility  of 
the  problem  in  a  particular  case. 

Let  us  suppose  that  x2  +  y2  + 1  is  resolvable  into  a  product  of  factors  which 
are  integral  in  x  and  y,  that  is,  that 

x"  +  y2  + 1  =  (px  +  qy  +  r)  (p'x  +  q'y  +  r'), 
then  x2  +  y2  +  l  =pp'x2  +  qq"y2  +  rr' 

+  (Pi'  +P'l)xy  +  (pr'  +p'r)x 

+  (qr'  +  q'r)y. 

Since  this  is,  by  hypothesis,  an  identity,  we  have 

pp'  =  1 
qq'  =  \ 
rr'  =  1 

First,  we  observe  that,  on  account  of  the  equations  (1)  (2)  (3),  none  of  the  six 
quantities p  q  r  p'  q'  r'  can  be  zero  ;  and  further,  p'  =  -,  <?'  =  -,  r'  —  -.    Hence, 


(1) 

Pi'  +  v'i  ~  o 

(4) 

(2) 

pr'  +  p'r  =  0 

(5) 

(3) 

q?''+q'r  =  0 

(6) 

as 

logical 

consequences 

of 

our 

hypothesis,  we 

^  +  2  =  0 
q   p 

r    p 

o*        n 

have 

from 

(4)  (5) 

and 

(6V- 

(7) 
(8) 
(9); 

T     q 

and,  from  these  again,  if  we  multiply  by  pq,  rp,  and  qr  respectively,  we  get 

p2  +  q2=0  (10) 

^2  +  r2  =  0  (H) 

q2  +  r2=0  (12). 
Now  from  (11)  and  (12)  by  subtraction  we  derive 

p2-q2=0  (13); 


140  QUADRATIC  FUNCTION  chap. 

and  from  (10)  and  (13)  by  addition 

2p3=0; 
from  this  it  follows  that  ^  =  0,  which  is  in  contradiction  with  the  equation  (1). 
Hence  the  resolution  in  this  case  is  impossible. 

§  13.]  Nevertheless,  it  may  happen  in  particular  cases  that 
the  resolution  spoken  of  in  last  article  is  possible,  even  when  the 
function  is  not  homogeneous.  This  is  obvious  from  the  truth 
of  the  inverse  statement  that,  if  we  multiply  together  two 
integral  functions,  no  matter  of  how  many  variables,  the  result 
is  integral. 

One  case  is  so  important  in  the  applications  of  algebra  to 
geometry,  that  we  give  an  investigation  of  the  necessary  and 
sufficient  condition  for  the  resolvability. 

Consider  the  general  function  of  x  and  y  of  the  2nd  degree,  and  write  it 

F  =  ax2  +  2hxy  +  by2  +  2gx  +  2/y  +  c. 
We  observe,  in  the  first  place,  that,  if  it  be  possible  to  resolve  F  into  two 
linear  factors,  then  we  must  have 

F  =  ( \Jax  +  ly  +  m)  (\Jax  +  I'y  +  to'), 
=  [sjax  +  >J(Z  +  Z')  +  h(l  -  I')} y  +  h(m  +  to')  +£(m- »»')] 

x[sjctx+{\{l+l')-l{l-l')}y  +  ii{m  +  m')-\{m-m')], 
=  { sjax  +  J(J  +  V)y  +  \{m  +  m')} 2  -  {h(l  -  l')y  +  i(m -  to')} 2- 

Hence,  when  F  is  resolvable  into  two  linear  factors,  it  must  be  expressible  in 
the  form  L2-M2,  where  L  is  a  linear  function  of  x  and  y,  and  M  a  linear 
function  of  y  alone  ;  and,  conversely,  when  F  is  expressible  in  this  form,  it 
is  resolvable,  namely,  into  (L  +  M)  (L- M). 

Let  us  now  seek  for  the  relation  among  the  coefficients  of  F  which  is 
necessary  and  sufficient  to  secure  that  F  be  expressible  in  the  form  L2  -  M2. 

1st.   Let  a  4=0,  then 

F  =  a[x*  +  2(hy  +  g)x/a  +(by"-  +  2/y  +  c)/a], 
=  a[  {x  +  (hy  +  g)/a} 2  -  {(hy  +  gf-  -  a(by*  +  2/y  +  c)}  /a"], 
=  a[ {x  +  (hy  +  g)/a} 2  -  {(^2  -  a%2  +2(gh -  af)y  +  (f  -  ac)} /«'-]. 

Hence  the  necessary  and  sufficient  condition  that  F  be  expressible  in  the  form 
L2  -  M2  is  that  (K2  -  ab)y"  +  2(gh  -  af)y  +  (g2  -  ac)  be  a  complete  square  as  regards 
y.     For  this,  by  §  7,  it  is  necessary  and  sufficient  that 

l{gh-af)*-4(h*-db)(g*-ac)  =  0; 

that  is,  -  a  {abc  +  2fgh  -  a/2  -  bg2  -  ch2)  —  0. 

Now,  since  a  4=0,  this  condition  reduces  to 

abc  +  2/gh  -  a/2  -bg2-ch2  =  0  { 1 ). 

2nd.  If  a  =  0,  but  b  4=0,  we  may  arrive  at  the  same  result  by  first  arranging 
F  according  to  powers  of  y,  and  proceeding  as  before. 


vii  OF  TWO  VARIABLES  HI 

3rd.  If  a  =  0,  6  =  0,  and  A#0,  the  present  method  fails  altogether,  but  F 
now  reduces  to 

F  =  2hxy  +  2gx  +  2fy  +  a, 

and  it  is  evident,  since  x2  and  y2  do  not  occur,  that  if  this  be  resolvable  into 
linear  factors  the  result  must  be  of  the  form  2h(x+p)(y  +  q).  We  must 
therefore  have  2g=2kq, 

2f=Zhp, 
c  =  2hpq. 

Now  the  first  two  of  these  give  fg  =  h-pq,  that  is,   2hpq=~- ;   whence 

using  the  third, 

ch=2fg, 
or,  since  h  *  0,  2fgh  -  cK2  =  0  (2) ; 

but  this  is  precisely  what  (1)  reduces  to  when  a  =  0,  6  =  0,  so  that  in  this  third 
case  the  condition  is  still  the  same. 

Moreover,  it  is  easy  to  see  that  when  (2)  is  satisfied  the  resolution  is 
possible,  being  in  fact 

2hxy  +  2gx  +  2fy  +  c  =  2hfx  +  fVy  +  ^\  (3), 

which  is  obviously  an  identity  if  c  =  2/g/h. 

4th.  If  a  =  0,  6  =  0,  h  =  0,  F  reduces  to  2gx  +  2/y  +  c.  In  this  case  we  may 
hold  that  F  is  resolvable,  it  being  now  in  fact  itself  a  linear  factor.  It  is 
interesting  to  observe  that  in  this  case  also  the  condition  (1)  is  satisfied. 

Returning  to  the  most  general  case,  where  a  does  not  vanish,  we  observe 
that,  when  the  condition  (1)  is  satisfied,  we  have,  provided  /i'2-«6  +  0, 

V{(#  -  ab),f-  +  2(gh  -  afjy  +  (g*  -  ac)}  =  VF^L+?p^Q, 

so  that  the  required  resolution  is 

f        h  +  \/l)?~-ab       g       gh-af     /r„ ,  "| 

Y=a\x+ y  +  -+  7£5 — ^-.\/h2-ab   [ 

I  a  a    a(h2  -  ab)  ) 


(        h-\/h2-ab       q        qh-af      /.« "|  r a\ 

I.  a  a     a{k-  -  ab)  ) 

To  the  coefficients  in  the  factors  various  forms  may  be  given  by  using  the 
relation  (1)  ;  but  they  will  not  be  rational  functions  unless  h2-ab  be  a  com- 
plete square,  and  they  will  be  imaginary  unless  h2-ab  is  positive. 

If  h2-ab  =  0,  then  (1)  gives  (gh-af ')2  =  0,  that  is,  gh-af—  0;  and  the 
required  resolution  is 

(        h       g     \'q- -ac\    |         h       g     \fg2-ac\  ,-> 

Y  =  a\  .T  +  -2/  +  -+  — * M  x+-y+- - h  (5). 

I       a       a  a       J   I       a fa  a       ) 

The  distinction  between  these  cases  is  of  fundamental  importance  in  the 
analytical  theory  of  curves  of  the  2nd  degree. 

The  function  abc  +  2fgh-af2-bg2-ch2,  whose  vanishing  is  the  condition 
for  the  resolvability  of  the  function  of  the  2nd  degree,  is  called  the  Discrimi- 
nant of  that  function. 


142 


EXERCISES  XI 


CHAP. 


It  should  be  noticed  that,  if 

F  =  ax2  +  2hxy  +  by2  +  2gx  +  2fy  +  c 

=(Ise+my+n)(l'x+m'y+n')  (6), 

then 

ax2  +  2hxy  +  by2=(lx  +  my)  (Vx  +  m'y), 

so  that  the  terms  of  the  1st  degree  in  the  factors  of  F  are  simply  the  factors 
of  ax2  +  2h xy  +  b y".  We  have  therefore  merely  to  find,  if  possible,  values  for 
n  and  n'  which  will  make  the  identity  (6)  complete. 

Example.  To  factorise  3a;2  +  2xy  -  y-  +  2x  -  2y  -  1 .     We  have  3a;2  +  2xy  -  y2 
=  (3x-y)  (x  +  y).     Hence,  if  the  factorisation  be  possible,  we  must  have 

3x2  +  2xy-y2  +  2x-2y-l  =  (3x-y  +  n){x  +  y  +  n')  (7). 

Therefore,  we  must  have 

»+3»'=2  (8), 

n-n'=-2  (9), 

«/;'=- 1  (10). 

Now,  from  (8)  and  (9),  we  get  n=  - 1,  and  n  =  +1.     Since  these  values 
also  satisfy  (10),  the  factorisation  is  possible,  and  we  have 

3x-2  +  2xy  -  y2  +  2x  -  2y  -  1  =  (3x  -  y  -  1 )  (x  +  y  + 1 ). 

It  should  be  noticed  that  the  resolvability  of 
F  =  ax2  +  2hxy  +  by2  +  2gx  +  2fy  +  c 
carries  with  it  the  resolvability  of  the  homogeneous  function  of 
three  variables  having  the  same  coefficients,  namely, 
F  =  ax5  +  by2  +  cz2  +  2fyz  +  2gzx  +  2hxy, 
as  is  at  once  seen  by  writing  xfz,  y/z,  in  place  of  x  and  y. 


Exercises  XL 
Factorise  the  following  functions  : — 


(1. 
(3. 
(5. 

(7. 
(10 
(13. 
(16. 
(18. 
(20. 
(22. 
(24. 
(23. 
(27. 
(28. 
(29. 
(30. 


(a  +  b)2  +  [a  +  c)2  -  (c+ d)2  -{b  +  d)2.         (2. )  ia2b2  -  {a2  +  b2  -  c2)2. 

(a2  -  2¥  -  c2)2  -  i(b2  -  c2)2.         (4. )  (5a2  -  11a;  +  12)a  -  (4.C2  -  15a;  +  6)3. 

{x2  -  03  +  y)x  +  fa}  2-(x-  yT-(x  -  a)2.  (6. )  a*  -  y6. 

x$-y\         (8.)  x2  +  Qxy  +  9y2-±.  (9.)  2a^  +  3a;-2. 

x2+6x-16.  (11.)  a;2-10a;  +  18.  (12.)  x2  +  a;-30. 

a;2  +  14a;  +  56.  (14.)  ar  +  4a;+7.  (15.)  2a;2  +  5a;-12. 

x2  +  2xs/(2J  +  q)  +  2q.         (17.)  x*-2bx/(b  +  c)  +  (b-c)/(b  +  c). 

[x2+pq)2-(p  +  q)2x2.         (19.)  ab(x2-y2)+xy(a2-b2). 

pq[x  +  y?-{p  +  q){x2-y2)  +  {x-y)2.         (21.)  a;3-15a;2  +  71a;- 105. 

a,J-14x2+148a;.         (23.)  a3-  13.^  +  54a; -72. 

3?  -  8.c2  +  x  -  8.  (25. )  x3  +  Zpx2  +  (3p2  -  q2)x  +p(p2  -  q2). 

(p  +  q)x3  +  (p-q)x2-(p  +  q)x-(p-q). 

x3  -  (1  +p  +p2)x2  +  (p  +p2  +p3)x  -p3. 

x*  -  (a  +  byx3  +  (a2b  +  ab2)x  -  a2b2. 

x6  +  xia  +  xta2  -  x2^  -  xas  -  a\ 

(l+x)2(l+i/2)-(l+y)2(l+ar!).         (31.)  x4  +  x2y2  +  y*. 


vii  EXERCISES  XI  143 

(32. )  Assuming  xl  +  yi=(x~  +pxy  +  y2)  (x2  +  qxy  +  y2),  determine  p  and  q. 
(33.)  Factorise  a4 +  y4-2(a-2  +  ?/2)  +  l. 

(34.)  Determine  r  and  s  in  terms  of  a,  p,  and  q  in  order  that  x~-  a2  may 
be  a  factor  in  x*  +px*  +  qx2  +  rx  +  s. 
Factorise 

(35. )  (xm+»)2  -  {x'"an)2  -  (x"am)2  +  («'»+»)-. 
(36. )  (x2  +  a2)2^  +  a2x2  +  a4)  -  (x*  +  a;4a4  +  a8). 
(37. )  xy2  -  2xy  -y2  +  x  +  2y-l.         (38. )  2a-2  +  xy  +  7x  +  3y  +  3. 
(39.)  2.)j2  +  a-2/-32/2-a;-47/-l.         (40.)  xy  +  7x  +  3y  +  21. 
(41.)  a:2-2!/2-3z2  +  7yz  +  2za;  +  a;#. 

(42.)  Determine  X  so  that  (x  +  6y -l){6x  +  y -l)+\(3x  +  2y  +  l)(2x  +  Sy+l) 
may  be  resolvable  into  two  linear  factors. 

(43.)  Find  an  equation  to  determine  X  so  that  ax2  +  by2  +  2hxy  +  2gx  +  2/y 
+  c  +  \xy  may  be  resolvable  into  two  linear  factors  ;  and  find  the  value  of  X 
when  c  =  0. 

(44.)  Find  the  condition  that  (ax  +  Py  +  yz)  {a'x  +  p'y  +  y'z)  -  (a"x  +  p"y 
+  y"z)2  break  up  into  two  linear  factors. 

(45.)  If  (x+p)  {x  +  2q)  +  (x  +  2p)  (x  +  q)  be  a  complete  square  in  a',  then 
9p2-Upq  +  9q2=0. 

(46. )  If  (x  4-  b)  (x  +  c)  +  (x  +  c)  (x  +  a)  +  (x  +  a)  (x  +  b)  be  a  complete  square  in 
x,  show  that  a  =  b  =  c. 

Factorise 

(47.)  a3  +  b3  +  c?-3abc.  (48.)  x3  +  3axy  +  ?/3  -  a3. 

(49.)  (x-x2)3  +  {x2-l)3  +  (l-x)3. 

Factorise  the  following  functions  of  a:,  y,  z: — * 

(50.)  ^(y2  +  x2)(z2  +  x2)(y-z). 

(51.)  2(^  +  ^)^-2/).         (52.)  2,xi(y2-z2).         (53.)  (2a-)3 -Zx3. 

(54.)  Simplify  {Z(x2  +  y2-z2)(x2  +  z2-y2)} /U{x±y±z). 

(55.)  Show  that  2(1/"^"  -  ynzm)  and  2,xn(ymzt>  -  yPzm)  are  each  exactly 
divisible  by  (y  -z)(z-  x)  (x  -  y). 

(56.)  Show  that  nxn+1  -  (n  + 1  )xn  + 1  is  exactly  divisible  by  (a*-!)2. 

(57.)  Show  that  ~Zx2(y  +  z  -  a:)3  is  exactly  divisible  by  2a;2-22j/z. 

(58.)  Show  that  (x  +  y  +  z)2n+1-x2n+1~y2rl+1-z2n+1  is  exactly  divisible  by 
{y  +  z){z  +  x)[x  +  y). 

(59. )  (y  -  z)2^1  +  {z-  a-)2"+1  +  (x  -  y)2'*1  is  exactly  divisible  by  {y  -  z)  (z  -  x) 

(x  ~  !/)■ 

(60. )  If  n  be  of  the  form  6m  -  1,  then  (,y  -  z)n  +  (z  -  x)n  +  (x  -  y)»  is  exactly 
divisible  by  2.x2 -Zxy  ;  and,  if  n  be  of  the  form  6»i  +  l,  the  same  function  is 
exactly  divisible  by  (2a:2  -  2a*i/)2. 

(61.)  Prove  directly  that  xy-\  cannot  be  resolved  into  a  product  of  two 
linear  factors. 

(62.)  If  a  and  b  be  not  zero,  it  is  impossible  so  to  determine  p  and  q  that 
x  +py  +  qz  shall  be  a  factor  of  x3  +  ay3  +  bz3. 

*  Regarding  the  meaning  of  2  in  (50),  (51),  &c,  see  the  footnote  on  p.  84. 


CHAPTER   VIII. 
Rational  Fractions. 

§  1.]  By  a  rational  algebraical  fraction  is  meant  simply  the 
quotient  of  any  integral  function  by  any  other  integral  function. 

Unless  it  is  otherwise  stated  it  is  to  be  understood  that  we 
are  dealing  with  functions  of  a  single  variable  x. 

If  in  the  rational  fraction  A/B  the  degree  of  the  numerator 
is  greater  than  or  equal  to  the  degree  of  the  denominator,  the 
fraction  is  called  an  improper  fraction,  if  less,  a  proper  fraction. 


GENERAL   PROPOSITIONS    REGARDING    PROPER   AND 
IMPROPER   FRACTIONS. 

§  2.]  Every  improper  fraction  can  be  expressed  as  the  sum  of 
an  integral  function  and  a  proper  fraction  ;  and,  conversely,  the  sum 
of  an  integral  function  and  a  proper  fraction  may  be  exhibited  as  an 
improper  fraction. 

For  if   in  '—  the   degree   m  of    Am  be  greater  than    the 

degree  n  of  Bn,  then,  by  the  division-transformation  (chap,  v.), 
we  obtain 

Aw  _  pj  J* 

n  -Dn 

which   proves   the   first  part  of  our   statement,  since   Qm.n  is 
integral,  and  the  degree  of  II  is  <  n. 

Again,  if  Fp  be  any  integral  function  whatever,  and  ATO/Bn  a 
proper  fraction  (that  is,  m<n),  then 


CHAP,  nil  PROPER  AND  IMPROPER  FRACTIONS  1-45 

A  P    P,    +  A 

P  -"Ml  _        P        n  "I 

p   K~~  "bT   ' 

which  is  an  improper  fraction,  since  the  degree  of  the  numerator, 
namely,  n  +  p,  is  >  n. 

Examples  of  these  transformations  have  already  been  given 
under  division. 

It  is  important  to  remark  that,  if  two  improper  fractions  be 
equal,  then  the  integral  parts  and  the  properly  fractional  parts  must  be 
equal  separately. 

For  let  ^•  =  QM  +  ^ 

A'  /  "R' 

am'  t>,      —  H  m'-n'  +  T3'    ' 

-t>  ,i'  -d  n' 

by  the  above  transformation. 

A         A'  , 
I  hen,  it 


B„      B'tt< ' 


R     ~  R' 


we  have  Qm  _„  +  =-=  Q'm<  _  M-  + 


B„     ^"l-"      BV 


'/i 


nence  h»/i-«     V»h'-)i'  —       t>   tv 

*> »  &  ri 

Now,  since  the  degrees  of  R'  and  R  are  less  than  n'  and  n 

respectively,  the   degree   of  the  numerator   on   the   right-hand 

side  of  this   last   equation  is   less   than  n  +  n' .     Hence,   unless 

Qm-n  —  Q'm'-ri  —  Q)    we   nave   an   integral   function    equal   to   a 

proper  fraction,  which  is  impossible  (see  chap,  v.,  §  1).    We  must 

therefore  have 

T>  TV 

Qm-n  =  Q'm'-n'j  and  consequently  ~-  =  ™~. 

-D/i      -°  ri 

X.B. — From  this  of  course  it  follows  that  m  -n=  m'  -  it'. 
As  an  example,  consider  the  improper  fraction  [a?  +  2x-  +  Zx  +  4)/(ar  +  x  +  1), 
and  let  us  multiply  both  numerator  and  denominator  by  ar  +  2x+  1  ;  we  thus 
obtain  the  fraction 

{a?  +  Ax4  +  8x*  +  12x-2  + 11«+  4)/(*4  +  Zx3  +  4.?2  +  3a?+ 1), 
which,  by  chap,  iii.,  §  2,  must  be  equal  to  the  former  fraction.     Now  transform 
each  of  these  by  the  long-division  transformation,  and  we  obtain  respectively 

£+3 


■+1+?+.+r 


VOL.  I 


146  DIRECT  OPERATIONS  chap. 

x3  +  5x2  +  7x  +  3 


and  X  +  1  + 


x4  +  3x3  +  ^-  +  3x  +  Y 


The  integral  parts  of  these  are  equal ;  and  the  fractional  parts  are  also  equal 
(see  next  section). 

The  sum  of  two  'proper  algebraical  fractions  is  a  proper  algebraical 
fraction. 

After  what  has  been  given  above,  the  proof  of  this  proposition  will  present 
no  difficulty.  The  proposition  is  interesting  as  an  instance,  if  any  were  needed, 
that  fraction  in  the  algebraical  sense  is  a  totally  different  conception  from 
fraction  in  the  arithmetical  sense  ;  for  it  is  not  true  in  arithmetic  that  the 
sum  of  two  proper  fractions  is  always  a  proper  fraction  ;  for  example,  f  +  i  =  |, 
which  is  an  improper  fraction. 

§  3.]  Since  by  chap,  iii.,  §  2,  we  may  divide  both  numerator 
and  denominator  of  a  fraction  by  the  same  divisor,  if  the  nu- 
merator and  denominator  of  a  rational  fraction  have  any  common 
factors,  we  can  remove  them.  Hence  every  rational  fraction  can 
be  so  simplified  that  its  numerator  and  denominator  are  algebraically 
prime  to  each  other ;  when  thus  simplified  the  fraction  is  said  to  be  at 
"its  lotvest  terms." 

The  common  factors,  when  they  exist,  may  be  determined  by 
inspection  (for  example,  by  completely  factorising  both  numerator 
and  denominator  by  any  of  the  processes  described  in  chap,  vii.) ; 
or,  in  the  last  resort,  by  the  process  for  finding  the  G.C.M.,  which 
will  either  give  us  the  common  factor  required,  or  prove  that 
there  is  none. 

Example  1. 

a? +53?+ 7s +3 


se*+3a8+4a!2+3a;+l' 

By  either  of  the  processes  of  chap.  vi.  the  G.  C.  M.  will  be  found  to  be  x-  +  2.r  + 1. 
Dividing  both  numerator  and  denominator  by  this  factor,  we  get,  for  the 
lowest  terms  of  the  given  fraction, 

a+3 
a,a+ss+r 

The  simplification  might  have  been  effected  thus.  Observing  that  both 
numerator  and  denominator  vanish  when  x=  -  1,  we  see  that  x+  1  is  a  com- 
mon factor.     Removing  this  factor  we  get 

.-•--}- ■!..•  + 3 
a*+2ar1+2a+l' 
Here  numerator  and  denominator  both  vanish  when  x=  -  1,  hence  there  is  the 
common  factor  as+1.     Removing  this  we  get 


vin  WITH  RATIONAL  FRACTIONS  147 

x+3 

aP  +  x  +  l' 
It  is  now  obvious  that  numerator  and  denominator  are  prime  to  each 
other  ;  for  the  only  possible  common  factor  is  x  +  3,  and  this  does  not  divide 
the  denominator,  which  does  not  vanish  when  x  =  -  3. 

§  4.]  The  student  should  note  the  following  conclusion  from 
the  above  theory,  partly  on  account  of  its  practical  usefulness, 
partly  on  account  of  its  analogy  with  a  similar  proposition  in 
arithmetic. 

If  two  rational  fractions,  P/Q,  P'/Q',  be  equal,  and  P/Q  be  at  its 
lowest  terms,  then  P'  =  AP,  Q'  =  AQ,  where  A  is  an  integral  function 
of  x,  which  will  reduce  to  a  constant  if  P'/Q'  be  also  at  its  lowest 
terms. 

To  prove  this,  we  observe  that 

p     p 

Q'~Q' 

whence  r  =  — ~-, 

Q 

that  is,  Q'P/'Q  must  be  integral,  that  is,  Q'P  must  be  divisible 

by  Q ;  but  P  is  prime  to  Q,  therefore  by  chap,  vi.,  §  1 2,  Q'  =  AQ, 

where  A  is  an  integral  function  of  x.     We  now  have 

Q 

so  that  P'  =  AP,  Q'  =  AQ. 

If  P'/Q'  be  at  its  lowest  terms,  P'  and  Q'  can  have  no  com- 
mon factor ;  so  that  in  this  case  A  must  be  a  constant,  which 
may  of  course  happen  to  be  unity. 

DIRECT    OPERATIONS    WITH    RATIONAL   FRACTIONS. 

§  5.]  The  general  principles  of  operation  with  fractions 
have  already  been  laid  down  ;  all  that  the  student  has  now  to 
learn  is  the  application  of  his  knowledge  of  the  properties  of 
integral  functions  to  facilitate  such  operation  in  the  case  of 
rational  fractions.  The  most  important  of  these  applications  is 
the  use  of  the  G.C.M.  and  the  L.C.M.,  and  of  the  dissection  of 
functions  by  factorisation. 


148  EXAMPLES  OF  DIRECT  OPERATIONS  chap. 

No  general  rules  can  be  laid  down  for  such  transformations  as  we  proceed 
to  exemplify  in  this  paragraph.  But  the  following  pieces  of  general  advice 
will  be  found  useful. 

Never  make  a  step  that  you  cannot  justify  by  reference  to  the  fundamental 
laws  of  algebra.  Subject  to  this  restriction,  make  the  freest  use  of  your  judg- 
ment as  to  the  order  and  arrangement  of  steps. 

Take  the  earliest  opportunity  of  getting  rid  of  redundant  members  of  a 
function,  unless  you  see  some  direct  reason  to  the  contrary. 

Cultivate  the  use  of  brackets  as  a  means  of  keeping  composite  parts  of  a 
function  together,  and  do  not  expand  such  brackets  until  you  see  that  some- 
thing is  likely  to  be  gained  thereby,  inasmuch  as  it  may  turn  out  that  the 
whole  bracket  is  a  redundant  member,  in  which  case  the  labour  of  expanding 
is  thrown  away,  and  merely  increases  the  risk  of  error. 

Take  a  good  look  at  each  part  of  a  composite  expression,  and  be  guided  in 
your  treatment  by  its  construction,  for  example,  by  the  factors  you  can  per- 
ceive it  to  contain,  by  its  degree,  and  so  on. 

Avoid  the  unthinking  use  of  mere  rules,  such  as  that  for  long  division, 
that  for  finding  the  G.C.M.,  &c. ,  as  much  as  possible  ;  and  use  instead  pro- 
cesses of  inspection,  such  as  dissection  into  factors  ;  and  general  principles, 
such  as  the  theorem  of  remainders.  In  other  words,  use  the  head  rather  than 
the  fingers.  But,  if  you  do  use  a  rule  involving  mechanical  calculation,  be 
patient,  accurate,  and  systematically  neat  in  the  working.  It  is  well  known 
to  mathematical  teachers  that  quite  half  the  failures  in  algebraical  exercises 
arise  from  arithmetical  inaccuracy  and  slovenly  arrangement. 

Make  every  use  you  can  of  general  ideas,  such  as  homogeneity  and  sym- 
metry, to  shorten  work,  to  foretell  results  without  labour,  and  to  control 
results  and  avoid  errors  of  the  grosser  kind. 

Example  1.   Express  as  a  single  fraction  in  its  simplest  form — 
2xs  +  4x-  +  3x  +  A     2ar>+4x2-3.c-2     „ 

— &n ^i — =F  say- 

Transform  each  fraction  by  division,  then 

F  =  (2x  +  4)  +-£-, ■-  (2x+ 4)  -  --£±?, 

x  +  1  a;  —  l 

_x{a?-1)-(-x  +  2){j?+l) 
.>-4-l 

_2x?-2xr-1 
~       x*-l      ' 

_2(33-a8-l) 

xA-l       ' 

Example  2.   Express  as  a  single  fraction 

111  1 


F= 


tf-Zxt+Zx-l     x*-a~-x+l     aA-2x3  +  2x~l     xi  -  2x*  +  2x:-~  2x+ 1" 


vin  WITH  RATIONAL  FRACTIONS  H9 

AVe  have 

x^-ofi-x+l     =x3  +  1-x(x+1)  =  (j:  +  1)(x2-x  +  1-x) 

=  (x+l)  (x-lf; 
x4  -  2:<3  +  2x  -  1  =x*  -  1  -  2x{x2  -  1), 
=  (*2-l)(.>'-l)-, 
=  (x-l)*(x+l); 
x*  -  2X3  +  2x2  -  2x  +  1  =  (a?  +  1 )2  -  2x(x-  + 1 ), 
=  (x*+l)(x-l)*. 
Whence 

ill  1 


F  = 


(x-1?     (jc+l)(a;-l)a     (x-lf(x+l)     (ar  +  lU:c-l)-' 

_(a;+l)-(.r~l)_(a;2  +  l)  +  (a--l)(a;+l) 
[x  + 1 )  (x  -  1  )3      [x  -  l)s  (aj+ 1)  (ar>  + 1) ' 

2  2^ 

(x  +  l)(a;-l)3     (a}-l)s(se+l)(a?+l)' 

x^+l-x* 
(x  +  l)(x2  +  l){x-lf 

2 


"(x*-l)(x--l)2' 
2 


x*-2xi  +  xi-  x2  +  2x  -  1 

Example  3. 

/.k  -  y    x3  -  y3\     /x  +  y    xs  +  y3\ 
\x  +  y    ar'  +  y3/     \x-y    x^-y3/' 

-(X-V\  (i     x*  +  x*/  +  y-\  (x+y\  /t  |  x2-xy  +  y2\ 
\x+yj  \       xP-xy  +  y2/  \x-y)  \       x2  +  xy  +  y2)' 

=(  ~2xy  \x(2^+yz)\ 

\x2-xy  +  y2J     \^  +  xij  +  y-)' 

ixy(x-  +  y") 
x4  +  x2y2  +  yf 

Example  4. 

^2              b-c  2  c-a  2  a-b 

*  =T~:+i \t~    m  +  r— :  +  r— 5T7T — -,  +  — ;  + 


b-c     (c-a)(a-b)     c-a     (a-b)(b-c)     a-b     (b-c)(c-a)' 

^2(c-a)(a-b)  +  (b-c)2  +  2(a-b)(b-c)  +  (c-a)2  +  2{b-c){c-a)  +  (a-b)2 

(b-c){c~a)(a-b) 

_{(b-c)  +  (c-a)  +  (a-b)}2 
&c. 

02  0 


&C.      (b-c)(c-a){a-b)        ' 
it  being  of  course  supposed  that  the  denominator  does  not  vanish. 


150  DIRECT  OPERATIONS  WITH  RATIONAL  FRACTIONS        CHAP. 

Example  5. 

«s  b3  -3 

■C  =7 tt~, ;  +7^ m r  + 


(a-b){a-c)     (b-c)(b~a)     (c-a)(c-b) 

_  - a3{b - c)-b3{c- a)  - <?{a-b) 
~  (b-c)(c-  a)  (a  -  b) 

Now  we  observe  that  when  b  =  c  the  numerator  of  F  becomes  0,  hence  b-c 
is  a  factor;  by  symmetry  c-a  and  a-b  must  also  be  factors.  Hence  the 
numerator  is  divisible  by  (b  -c){c-  a)  (a  -  b).  Since  the  degree  of  the  numer- 
ator is  the  4th,  the  remaining  factor,  owing  to  the  symmetry  of  the  expression, 
must  be  Pa  +  PS  +  Pc.     Comparing  the  coefficients  of  asb  in 

-  a3(b  -  c)  -  b3(c  -  a)  -  <?{a  -  b) 
and  F{a  +  b  +  c){b-c){c-a){a-b), 

we  see  that  P=  +1. 

Hence,  finally,  ¥  =  a  +  b  +  c. 

Example  6. 

^_  a2+pa  +  q  b2+pb  +  q  c2+pc  +  q 

~ (a-b)(a-c)(x-a)     {b-a)  {b-c)  (x-b)     {c-a)(c-b){x-c)' 
■p_(h-c)  (a2  +pa  +  q)(x-  b)  (x -  c)  +  &c.  +  &c. 
(b  -  c)  (c  -a)  (a-  b)  (x  -  a)  (x  -  b)  (x  -  c)    ' 
_(b  -  c)  (a?  +  pa  +  q) {x2 -  (b  +  c)x  +  bc}  +&c.  +&c. 
&c. 

Now,  collect  the  coefficients  of  x2,  x,  and  the  absolute  term  in  the  numerator, 
observing  that  the  two  &c.'s  stand  for  the  result  of  exchanging  a  and  b  and  a 
and  c  respectively  in  the  first  term.  We  have  in  the  coefficient  of  x2  a  part 
independent  of  p  and  q,  namely, 

a2(b  -c)  +  b2(c  -a)+c*(a-  b)=  -  (J  -  c)  (c  -  a)  (a  -  b)  (1). 

The  parts  containing  p  and  q  respectively  are 

{a(b  -c)  +  b(c  -a)+c{a-b))p  =  Q 
and  {(b-c)  +  (c-a)  +  (a-b)}q  =  0. 

The  coefficient  of  a?  therefore  reduces  to  (1). 

Next,  in  the  coefficient  of  x  we  have  the  three  parts, 

-  {a"-(b2  -  c2)  +  b2(c2  -  a2)  +  cV  -  b2)}  =  0, 

-  {a(b2  -c2)  +  b(c2  -  a2)  +  c(a2  -  b2))p 

=  -(b-c)(c-a)(a-b)p  (2), 

and  -  {(b2-c2)  +  (c2-a2)  +  {a2-b2)}q  =  0. 

Finally,  in  the  absolute  term, 

abc  {a(b  -c)  +  b(c  -a)+  c(a  -  b)}  =  0. 
abc  {{b  -c)  +  (c  -a)  +  (a-  b)}p  -  0, 
{bc(b  -  c)  +  ca(c  -a)+  ab(a  -b)}q 

=  -(b-c)(c-u)(a-b)q  (3). 


vin  INVERSE  METHODS  151 

Hence,  removing  the  common  factor  (b-c)  (c-a)(a-  b),  which  now  appears 
both  in  numerator  and  denominator,  and  changing  the  sign  on  both  sides,  we 
have 

,r-  +px  +  q 


F  = 


(x-a)  (x-  b)  (x  —  e) 


The  student  should  observe  here  the  constant  use  of  the  identities  on  pp. 
81-S3,  and  the  abbreviation  of  the  work  by  two-thirds,  effected  by  taking 
advantage  of  the  principle  of  symmetry.  In  actual  practice  the  greater  part 
of  the  reasoning  above  written  would  of  course  be  conducted  mentally. 


INVERSE    METHOD    OF   PARTIAL    FRACTIONS. 

§  6.]  Since  we  have  seen  that  a  sum  of  rational  fractions  can 
always  be  exhibited  as  a  single  rational  fraction,  it  is  naturally 
suggested  to  inquire  how  far  we  can  decompose  a  given  rational 
fraction  into  others  (usually  called  "partial  fractions")  having 
denominators  of  lower  degrees. 

O 

Since  we  can  always,  by  ordinary  division,  represent  (and  that 
in  one  way  only)  an  improper  fraction  as  the  sum  of  an  integral 
function  and  a  proper  fraction,  we  need  only  consider  the  latter 
kind  of  fraction. 

The  fundamental  theorem  on  which  the  operation  of  dissec- 
tion into  "  partial  fractions  "  depends  is  the  following  : — 

If  A/PQ  be  a  rational  proper  fraction  whose  denominator  contains 
two  integral  factors,  P  and  Q,  which  are  algebraically  prime  to  each 
other,  then  we  can  always  decompose  A/PQ  into  the  sum  of  two  proper 
fractions,  P'/P  +  Q'/Q. 

Proof. — Since  P  and  Q  are  prime  to  each  other,  we  can  (see 
chap,  vi.,  §  11)  always  find  two  integral  functions,  L  and  M, 
such  that 

LP  +  MQ=1  (1). 

Multiply  this  identity  by  A/PQ,  and  we  obtain 

A  _AL     AM 
PQ "  Q  +  "P"  (~}' 

In  general,  of  course,  the  degrees  of  AL  and  AM  will  be  higher 
than  those  of  Q  and  P  respectively.  If  this  be  so,  transform 
AL/Q  and  AM/P  by  division  into  S  +  Q'  Q  and  T  +  P'/P,  so  that 


152  PARTIAL  FRACTIONS  chap. 

S,  T,  Q',  and  P'  are  integral,  and  the  degrees  of  P'  and  Q'  less 
than  those  of  P  and  Q  respectively.     We  now  have 

PQ  P      Q  v  ;' 

where  S  +  T  is  integral,  and  P'/P  +  Q  Q  a  proper  fraction.  But 
the  left-hand  side  of  (3)  is  a  proper  fraction.  Hence  S  +  T  must 
vanish  identically,  and  the  result  of  our  operations  will  be  simply 

A^  +  g  (4). 

PQ     P     Q  w 

which  is  the  transformation  required. 

To  give  the  student  a  better  hold  of  the  above  reasoning,  we 
work  out  a  particular  case. 


Consider  the  fraction 

x*+l 


F=: 


"  (x3  +  &E2  +  2x  + 1 )  (Xs  +  x  + 1) ' 
Here  A=a*»+1>     F  =  x3  +  Bx2  +  2x  +  l,     Q=x"  +  x  +  l. 

Carrying  out  the  process  for  finding  the  G.  C.  M.  of  P  and  Q,  we  have 
1-1  +  1)1  +  3  +  2  +  1(1  +  2 
2  +  1-1 
-1-1)1  +  1  +  l(-l  +  0 
0  +  1 
+  1 

whence,  denoting  the  remainders  by  Ri  and  Ro, 

P  =  (x  +  2)Q  +  Ri,     Q=-  x&i  +  R* 

From  these  successively  we  get 

Ri  =  P-(a-  +  2)Q, 
l  =  R,  =  Q  +  a,R1, 

=  Q  +  xP-x{x  +  2)Q, 

=  (-xn--2x+l)Q +  .,;!>  (1). 

In  this  case,  therefore, 

M=-z*-2x+l,     L=x. 

Multiplying  now  by  A/PQ  on  both  sides  of  (1),  we  obtain  (putting  in  the 
actual  values  of  P  and  Q  in  the  present  case) 

(af'  +  l)(-a3-2g  +  l)      (z*  +  l)x . 
x2  +  Zx?  +  2x+\         x*+x+l' 
_  -xe-2x5  +  xi-x2-2x+l        j~ - x 

x3  +  3x?  +  2x+l  +a?  +  x+l  ' 

or,  carrying  out  the  two  divisions, 


viii  SPECIAL  CASES  153 

or,  seeing  that  the  integral  part  vanishes,  as  it  ought  to  do, 

which  is  the  required  decomposition  of  F  into  partial  fractions. 

Cor.  If  P,  Q,  R,  S,   .   .  .  be  integral  functions  of  x  which  are 

prime  to  each  other,  then  any  proper  rational  fraction  A/PQRS  .   .   . 
can   be  decomposed  into   a  sum  of  proper  fractions,  P'/P  +  Q'  Q  + 

R'/R  +  sys  +  .  .  . 

This  can  be  proved  by  repeated  applications  of  the  main 
theorem. 

§7.]  Having  shown  a  priori  the  possibility  of  decomposition 
into  partial  fractions,  we  have  now  to  examine  the  special  cases 
that  occur,  and  to  indicate  briefer  methods  of  obtaining  results 
which  we  know  must  exist. 

"We  have  already  stated  that  it  may  be  shown  that  every 
integral  function  B  may  be  resolved  into  prime  factors  with  real 
coefficients,  which  belong  to  one  or  other  of  the  types  (x  -  a)'', 

(/  +  0b  +  7y. 

1st.  Take  the  case  where  there  is  a  single,  not  repeated, 
factor,  X  -  a.      Then  the  fraction  F  =  A  B  may  be  written 

F         * 
(•!•  -  a)Q 

say,  where  X  -  a  and  Q  are  prime  to  each  other.     Hence,  by  our 
general  theorem,  we  may  write 

f-  F  +Q'  m 

each  member  being  a  proper  fraction. 

In  this  case  the  degree  of  P'  must  be  zero,  that  is,  P'  is  a 
constant. 

It  may  be  determined  by  methods  similar  to  those  used  in 
chap,  v.,  §  21.     See  below,  Example  1. 

P'  determined,  we  go  on  to  decompose  the  proper  fraction 
Q   Qi  by  considering  the  other  factors  in  its  denominator. 


154  SPECIAL  CASES  chap. 

2nd.  Suppose  there  is  a  repeated  factor  (x  -  a)r ;  say  B  = 
(.r  -  a)rQ,  where  Q  does  not  contain  the  factor  x  -  a.  "We  may, 
by  the  general  principle,  write 

r,  P'       +Q' 


(a;  -  a)'"     Q* 

P'  is  now  an  integral  function,  whose  degree  is  less  than  r\ 
hence,  by  chap,  v.,  §  21,  Ave  may  put  it  into  the  form 

P'  =  a0  +  di(z  -  a)  +  .   .  .  +ar_i(a;-a)r"1, 

and  therefore  write 

"         +  ...+^+g  (2), 


(x-af     (a; -a)'"1  x-a     Q 

where  a0,  alf  .  .  .,  a,._i  are  constants  to  be  determined.     See 
below,  Example  2. 

3rd.  Let  there  be  a  factor  (x2  +  fix  +  y)g,  so  that 

b  =  (x2  +  fix  +  yyq, 

Q  being  prime  to  x2  +  fix  +  y.     Now,  we  have 

P'  Q' 


(x2  +  px  +  7y    q- 

P'  is  in  this  case  an  integral  function  of  degree  2s  -  1  at  most. 
We  may  therefore  write,  see  chap,  v.,  §  21, 

P'  =  (a0  +  b0x)  +  (</,  +  bxx)  (x2  +  fix  +  y) 
t  (a2  +  kjx)  (x2  +  fix  +  y)2 

+  (ag„l  +  b8-1z)(x*  +  px  +  yy-1. 

We  thus  have 

_       a0  +  h„r  a,  +  bxx  at^  +  bg-tf     Q' 

(x2  +  /3x+  yy>     (x2  +  fix  +  y)*-1  x2  +  (3x  +  y      Q  {  ' ' 

where  the  2s  constants  am  b0,  &c,  have  to  be  determined  by  any 
appropriate  methods.      See  Examples  3  and  4. 

In  the  particular  case  where  s  =  1,  we  have,  of  course,  merely 

_     a0  +  &Q.T        Q' 


Viil  EXPANSION  THEOREM  155 

By  operating  successively  in  the  way  indicated  we  can  decompose 

every  rational  fraction  into  a  sum  of  partial  fractions,  each  of  which 

belongs  to  one  or  other  of  the  two  types  prj{x  -  a)r,  (as  +  bsx)/(x2  +  ftx 

+  y)s,  where  a,  ft,  y,  pr,  as,  b8  are  all  real  constants,  and  r  and  s 

positive  integers. 

It  is  important  to  remark  that  each  such  partial  fraction 
has  a  separate  and  independent  existence,  and  that  if  necessary 
or  convenient  the  constant  or  constants  belonging  to  it  can  be 
determined  quite  independently  of  the  others. 

Cor.  If  P  be  an  integral  function  of  x  of  the  nth  degree,  and 
a,  a,  .  .  .,  a;  ft,  (3,  .  .  . ,  ft ;  y,  y,  .  .  . ,  y,  .  .  .  constants  not  less 
than  n  +  1  in  number,  r  of  which  are  equal  to  a,  s  equal  to  ft,  t  equal 
to  y,  .  .  . ,  then  we  can  ahoays  express  P  in  the  form 

P  =  2{a0  +  a,(x  -«)+...+  ctr.^x  -  a)r"1}(a:  -  ft)%x  -  y)(  .  .  ., 

where  a0,  au  .  .  . ,  ar_u  .  .  .   are  constants.     In  particular,  if  r  =  1. 
s  =  1 ,  t  =  1, .  . . ,  we  have 

P  =  ?a0(x-ft)(x-y)  ... 

These    theorems    follow    at    once,  if   we   consider    the   fraction 

p/(x  -  ay(x-  fty(x  -7y... 

There  is  obviously  a  corresponding  theorem  where  x  -  a, 
x-  ft,  x  -  y  are  replaced  by  any  integral  functions  which  are 
prime  to  each  other,  and  the  sum  of  whose  degrees  is  not  less 
than  n  +  1. 

§  8.]  We  now  proceed  to  exemplify  the  practical  carrying 
out  of  the  above  theoretical  process ;  and  we  recommend  the 
student  to  study  carefully  the  examples  given,  as  they  afford  a 
capital  illustration  of  the  superior  power  of  general  principles  as 
contrasted  with  "rule  of  thumb"  in  Akebra. 

o 

Example  1.   It  is  required  to  determine  the  partial  fraction,  corresponding 
to  x-  1,  in  the  decomposition  of 

(Iv4-  16a»+17a?  -  8.r  +  7)/(.r  -  1)  (a  -  2)2(a-2  + 1). 
We  have 

r_4a^-16^  +  17x2-8a-  +  7_    p  Q' 

(a;-l)(a;-2)2(a;2+l)        a-l+(aj-2)2(£B2  +  l)  (  >' 

and  we  have  to  find  the  constant  p. 


156  EXAMPLES  CHAP. 

From  the  identity  (1),  multiplying  both  sides  by  (x-1)  (j;-2)2(a;2  +  l),  we 
deduce  the  identity 

±xA  -  16x3  + 1 7 xs  -  8.r  +  7  =p{x  -  2)2 («2  + 1)  +  Q'(x  - 1 )  (2). 

Now  (2)  being  true  for  all  values  of  x,  must  hold  when  o-=l  ;  in  this  case  it 
becomes 

4  =  2^),  that  is,p=2. 

Hence  the  required  partial  fraction  is  2/(x-  1). 

If  it  be  required  to  determine  also  the  integral  function  Q',  this  can  be 
done  at  once  by  putting  ^>  =  2  in  (2),  and  subtracting  2(.c-2)2(.£2  +  l)  from 
both  sides.     We  thus  obtain 

2x*  -  8a?  +  7,<"  -  1  =  Q'(x  -  1 )  (3). 

This  being  an  identity,  the  left-hand  side  must  be  divisible  by  x-1.*     It  is 
so  in  point  of  fact ;  and,  after  carrying  out  the  division,  we  get 

2,r3-6a:2  +  a:+l  =  Q'  (4), 

which  determines  Q'. 

The  student  may  verify  for  practice  that  we  do  actually  have 
4^-16^  +  1 7.x-2  -  8x  +  7  _  _2_     2a3  -  6x°  +  x  +  l 
(x-l){x-2)*(x*  +  l)        x -  1 +  (x -  2)s (x2  + 1 )  * 

Example  2.  Taking  the  same  fraction  as  in  Example  1,  to  determine  the 
group  of  partial  fractions  corresponding  to  (a;  -  2)2. 
1°.  "VVe  have  now 

4x*  -  1 6^  + 1 7a;2  -  8a:  +  7  _      an  ax  Q'  .. 

(a;-l)(a;-2)2(a;2+l)     ~  {x-2)-  + (x^2)  + (x-1)  (x2+l)         ^  " 
whence 

ixi-16x3  +  l7x'2-8x  +  7  =  a0(x-l)  (z2  + 1)  +  <n(x-  2)  (aj-1)  (x2  + 1) 

+  Q'(*-2)2  (2). 

In  the  identity  (2)  put  x  =  2,  and  we  get 

-  5  =  5«oi  that  is,  «0  =  -  1 . 
Putting  now  a0  =  -1  in  (2),  subtracting  ( -  1)  (.«-  1)  (.c2  +  l)  from  both  sides 
and  dividing  both  sides  by  x  -  2,  we  have 

4ri-7vi  +  2x-3  =  a1(x-l)(x-  +  l)  +  Q'{x-2)  (3). 

Put  x  =  2  in  this  last  identity,  and  there  results 

+  5  =  5cti,  that  is,  a,\  =  + 1. 
The  group  of  partial  fractions  required  is  therefore 

-l/(x-2T-  +  l/(x-2). 
If  required,  Q'  may  be  determined  as  in  Example  1  by  means  of  (3). 
2°.  Another  good  method  for  determining  a0  and  a\  depends  on  the  use  of 
"continued  division." 

If  we  put  x  =  y  +  2  on  both  sides  of  (1),  we  have  the  identity 

4(y  +  2)4-16(y  +  2)3  +  17(y  +  2)2-8(?/  +  2)  +  7  =  a0    ax  Q" 

(2/+l)2/2l(y  +  2)2+l}  y2     y+(y  +  l){{y  +  2f  +  \\' 

*   If  it  is  not,  then  there  lias  been  a  mistake  in  the  working. 


vin  EXAMPLES  157 

that  is, 

-5-4y  +  &c._fl0     ffl      _        Q"    

5y-  +  9f  +  kc.  y2+  y  (l+y)(3  +  iy  +  y-) 
Now,  by  chap,  v.,  §  20,  the  expansion  of  a  rational  fraction  in  descending 
powers  of  1/y  and  ascending  powers  of  y  is  unique.  Hence,  if  we  perform 
the  operation  of  ascending  continued  division  on  the  left,  the  first  two  terms 
must  be  identical  with  a0/if  +  ai/y  ;  for  Q"/(l  +y)  (3  +  4y  +  ?/2)  will  obviously 
furnish  powers  of  y  merely. 
AVe  have 

-5-4+...  5  +  9+  .  ,  .. 

+5+...       -1+1+... 

therefore  a0=  -1,  ai=  +1. 

The  number  of  coefficients  which  we  must  calculate  in  the  numerator  and 
denominator  on  the  left  depends  of  course  on  the  number  of  coefficients  to  be 
determined  on  the  right. 

Example  3.  Lastly,  let  us  determine  the  partial  fraction  corresponding  to 
7?  + 1  in  the  above  fraction. 
We  must  now  write 

4.7;* -I6x?  +  l7x2-8x  + 7  _ax  +  b  Q'  . 

(x-l)(x-2)*(x2+lj~~x2  +  l  +  (x-l)(x-2f  (  '• 

1°.  Whence,  multiplying  by  (x-  1)  (x-  2)2, 
4ar1-16x3  +  17x2-8^  +  7 _ jax  +  b)  (x-1)  {x- 2)2 

x*+l  ~  x-+l 

whence 


■  +  Q'  (2) 


4,,.2  _  1  6i,  +  13  +  84_J  =  {nx  +  b)(x_5  +  i£±l\  +  Q' 
X'+l  \  X1  + 1  / 


,         ,,,       rN     7ax-  +  (7b  +  a)x+b     _. 
=  (ax  +  b)  (x  -5)4 \,  +  1         -  +  <x>\ 

...       r,     „       (7b  +  a)x  +  (b-7a)     _,       . 
=  (ax  +  b)  .r-5  +7a  +  v ^—. \ '  +  Q        (3). 

ar  +  1 

Now  the  proper  fractions  on  the  two  sides  of  (3)  must  be  equal — that  u,  we 
must  have  the  identity 

( 7  b  +  a)x  +  (b  -  7a)  =  Sx  -  6, 
therefore  7b  +  a  —  8,     b-7a=  -  6. 

Multiplying  these  two  equations  by  7  and  by  1  and  adding,  we  get 

506  =  50,  that  is,  6=1. 
Either  of  them  then  gives  «=1,  heuce  the  required  partial  fraction  is 

(x+l)l(x*+l). 
2".  Another  method  for  obtaining  this  result  is  as  follows. 
Remembering  that  x2  + 1  =  [x  +  i)  (x -  I)  (see  chap,  vii.),  we  see  that  a;2 +1 
vanishes  when  x—i. 
Now  we  have 

lxi-16x"+l7x2-8x  +  7  =  (ax+b){x-l)(x-2)2  +  Q'{xn-+l) 

=  [ax  +  b)  (a?  -  5x2  +  8x -  4)  +  Q'(.>"  +  1 )       (4). 


158  EXAMPLES 


CHAP. 


Put  in  tins  identity  x=i,  and  observe  that 

ii  =  Pxi2  =  (-l)x(-l)=+l, 
^—■Px  i—(  -l)xi=  -  i  ; 
and  we  have  8i-G-(ai  +  b)  (7i+l), 

=  (7b  +  a)i+{b-7a) ; 
whence  (7b  +  a -  8)i=  -  b  +  7a-  6, 

an  equality  which  is  impossible  *  unless  both  sides  are  zero,  hence 

7b  +  a-8  =  0,      -b  +  7a-6-0, 
from  which  a  and  b  may  be  determined  as  before. 

3°.  Another  method  of  finding  a  and  b  might  be  used  in  the  present  case. 
We  suppose  that  the  partial  fractions  corresponding  to  all  the  factors 
except  ic2+ 1  have  already  been  determined.     We  can  then  write 

„        2  1  1        ax  +  b  /c. 

From  this  we  obtain  the  identity 
4.i4-16j3  +  17a;2-8a;  +  7 

=  2(x-2)2(x2  +  l)-(x-l)(x°+l)  +  (x-l)(x-2)(x2+l) 

+  (ax+b){x-rl){x-  2)8 ; 

whence 

%A  -  Ao?  +  Sx*  +  ix  -  4  =  (ax  +  b)  [x  -  1)  [x  -  2)2 ; 

and,  dividing  by  (x  -  1)  (x  -  2)2, 

x+l=ax  +  b. 
This  being  of  course  an  identity,  we  must  have 

a  =  l,     b  =  l. 

Another  process  for  finding  the  constants  in  all  the  partial  fractions  depends 
on  the  method  of  equating  coefficients  (see  chap,  v.,  §  16),  and  leads  to  their 
determination  by  the  solution  of  an  equal  number  of  simultaneous  equations 
of  the  1st  degree. 

The  following  simple  case  will  sufficiently  illustrate  this  method. 

Example  4. 

To  decompose  (3x-i)/(x-  l)(„e-2)  into  partial  fractions. 

We  have 

Zx  -  4  a  b 

{x-\)[x~2)~x^lJrx^~V 
therefore  3x-  l  =  a(x-2)  +  b(x-  1), 

=  (a  +  b)x  -  (2a  +  b). 
Hence,  since  this  last  equation  is  an  identity,  we  have 

a  +  b  =  3,     2a  +  b=i. 
Hence,  solving  these  equations  for  a  and  b  (see  chap.  xvi. ),  we  find  «=i, 
b  =  2. 

*  For  no  real  multiple  (differing  from  zero)  of  the  imaginary  unit  can  be  a 
real  quantity.  See  above,  chap,  vii.,  §  6.  The  student  should  recur  to  this 
case  again  after  reading  the  chapter  on  Complex  Numbers. 


VIII 


EXERCISES  XII 


159 


Example  5.   We  give  another  instructive  example.     To  decompose 


F=,- 


x-+px  +  q 


we  may  write 


x-  +px  +  q 


(x  -a)(x-  b)  (x-c)' 
C 


A         B 

+  - 


+  ■ 


(1), 


(x  -  a)  (x  -  b)  {x  -  c)     x-a    x-b    x-c 
where  A,  B,  C  are  constants. 
Now 

x2  +px  +  q  =  A(x  -b)(x-c)  +  B(x  -  e) {x-  a)  +  C{x  -  a)  (x  -  b)         (2). 

Herein  put  x  =  a,  and  there  results 

a2+pa  +  q=  A(a-  b)(a-c)  ; 


whence 

By  symmetry 

We  have  therefore 
x^+px  +  q 


A=  a2+Pa  +  9 
(a  -b)(a-c)' 

b2  +  pb  +  q 


B= 


(x-  a)(x-  b)(x-  c) 

a"  +pa  +  q 


+ 


(b-a)(b-c)' 

c2+pc  +  q 

(c~a)(c-  b)' 


b2+pb  +  q 


+  . 


c2  +pc  +  q 


(a-  b)(a-c)(x-  a)     (b-c){b-a)(x-b)     (c-a)(c-b)(x-c) 


(3), 


an  identity  already  established  above,  §  5,  Example  6.  It  may  strike  the 
student  as  noteworthy  that  it  is  more  easily  established  by  the  inverse  than 
by  the  direct  process.  The  method  of  partial  fractions  is  in  point  of  fact  a 
fruitful  source  of  complicated  algebraical  identities. 


Exercises  XII. 
Express  the  following  as  rational  fractions  at  their  lowest  terms. 


(1. 
(2. 

(3. 

(4. 
(5. 
(6. 
(7- 
(8. 

(9. 

(10. 


{x3  +  2x2-x  +  6)/(x*  -  x2  +  ix  -  4). 
(9ar»  +  53.T2  -  9a-  J  8)/(4x2  +  44«  +  120). 

z*+2x*-2x-l     _ x*_+  ,<a -  3<" - 5x-2 
x*  +  a*-3x*-5x-2        a?4  +  2x*  -  2x  - 1     " 

{3x*-x*-z- 1  )/(8a?  +  5x2  +  Zx  + 1 )  +  (se*  +  3a?  +  5x  +  3)/{x3  +  x2  +  x  -  3). 
(a-6  -  2a?  +  l)/(x2-2x  +  l)  +  {a?  +  2a?  + 1  )!(x2  +  2x + 1 ). 
(6a?  +  IZax2  -  9a2x  -  10«3)/(9x3  +  \2ax2  -  Ua2x  -  10a3). 
(l-a-)l{(l+ax)2-(a  +  x)2}. 
{(w  +  x  +  z)(w  +  x)-y(y  +  z)}/{(w  +  x  +  z)(w  +  z)-y(x  +  y)}. 

(\-x)(\-x2fl  {  (T^p "  (l-x)(l-x2) +  (l^tf)2  )  ' 
{ (al  +  bm)2  +  (am  -  bl)2 }  /  { (ap  +  bq)2  +  (aq  -  bpf } . 


160 


EXERCISES  XII 


CHAP. 


(11. 

(12. 

(14, 
(15. 

(16. 

(17. 
(18. 
(19. 
(20. 

(21. 

(22. 
(23. 

(24. 
(25. 
(26. 

(27. 

(28. 

(29. 

(30. 
(31. 
(32. 

(33. 
(34. 
(35. 


{px2  +  (k-s)x  +  r}2-  {px2+(k  +  s)x  +  r}2 
\p3?  +  {k  +  t)x  +  r}2-  {px2  +  (k-t)x  +  r}2' 

x         %-y 


2x  -2y     2y-2x 


(13.) 


■  +  ■ 


1 


a-b-(a-b)x    a  +  b  +  (a  +  b)x 


l/(a  -2b-  lj(a  -2b-  l/(a  -  2b) ) ). 
1/(6*  +  6)  -  l/(2a3  -  2)  +  4/(3  -  3a;2). 
x^-y3 


x*-y* 


x-y  _  ,  /  x  +  y 1_ ) 

x2-y2     t\x2  +  y2    x  +  y]' 
/    x       l-x\  I  /    x       \-x\ 
\\+x       x    )J  \l+a:       x    )' 


6a; 
3a;-2       9a,-2  +  4 


30a~+4a-        Ax 


2x  +1 
24(aY^l)  '  8(a;+l)  '  4(a-  +  l)2     2(a;+iy3"3(a;2  +  a;+l)• 

_1 1_      _2_      _2_ 

(a;+l)2(a;  +  2)2     (x  +  2f  +  x  +  l     x+2' 

{a  +  b)j{x  +  a)  +  {a  -  b)/(x  -a)-  2a{x  +  ty/ix2  +  a"). 

{(x-y)l{x+y)}  +  {{x-y)l{x  +  y)}2+  {(x-y)/(x+y)}*. 

/      a-3-3a-+2     \      /a-2  +  2a;+l\ 

\.ri  +  2x2  +  2x+l)  X  W-bx+i)' 

'a2  +  x2 


/a2  +  x2       \ 

(r^x-+1)x 


2ax 
x  +  y 


+ 


+  1 
x-y 


ax- 


-5a; +4, 

4a(a  +  x, 

a2  -  ax  +  x 


2' 


-2- 


x'  -  %f 


aP-y3    ar5  +  y3       xi  +  x2y2  +  y4 ' 
x2    y2 


1      1 

-  +  -. 
x-    y< 


I 


Ht   Hfi-'tts)(  t  -.) 


x°    y 


+  ; 


+  • 


2a(a-c)(x-a)     2a(a  +  c)(x  +  a)     (c2  -  a2)  (x  +  c) 

(        _20__180       420__280\      /i__20_     2?2  _  i2^      280  \ 

(.     +  a-+l     a-  +  2+a;  +  3     a'+4jXt        x-l+ x-2~  x^S+x- 4j 

{(xy-l)2  +  (x  +  y-2)(x  +  y-2xy)}/{(xy  +  l)2-(x  +  y)2}. 

{l+y*+*-Syz)/(l+y+z). 

{a{a  +  2b)  +  b(b  +  2c)  +  c(c  +  2a)} /  [a2  -b2-c2-  2bc) . 

(a  +  b)s+(b  +  c)s-(a  +  2b  +  c)i 


(a  +  b)(b  +  c)(a  +  2b  +  c) 

x6  +  a6 


■+- 


orx* 


(Ic  +  a6)  (a?  -  a2)  +  a2x2(x*  -  a4)    X*-  «G  -  «  V  Vs  -  a2)' 

a2  +  (2ac  -  b2)x2  +  c2xA  a2  +  (ac  -  b2)x2  -  bcx* 

a2  +  2abx  +  {2ac+b-  a  '     •zhcjF+c2xA  *  a-  +  \ac  ->>2  +  bex '■' 


VIII 


EXERCISES  XII 


161 


X2  +  y2+x  +  y-xy  +  l  |  x2  +  y2  +  x -y  +  xy  +  1 
x-y-1  x  +  y-1 


(37.) 


(38.) 


(■r5-10,cy  +  5.CT/4)2  +  (5afy  -  lOieV  +  //•-/-' 

(b  +  c)-  +  2(b2-c°-)  +  (b-cf 


(39.)  2(62  +  c2-a2)/(a-&)(<w). 
(41.)  2(6  +  c)/(c-o)(a-&). 
(43.)  2(&2  +  &c  +  c2)/(a-&)(«-c). 
(44.)  {II(l-a?)  +  n(a;-y2)}/(l-aj^). 
(45.)  {Z(J  +  c)s-3II(&  +  c)}/{2a3-3a&c}. 

(46.)  ]~x  i  g~*y  i y-1 1  (1-x)(x-y)(y-1) 


(40.)  (Zx)CZx2)/xyz-Z(y  +  z)/x. 
(42.)  2,bc{a  +  h)/{a-b){a-c). 


(47. 


1+x    x  +  y    y  +  1     (l+a:)(a:  +  ?/)(y  +  iy 
(y-2)2+(z-a;)2  +  (.r-y)2|  £/    1      [     1  1\ 

(y-2)(»-aj)(aj-y)  Vy-z    s-a:    a;-y/ 


ras  \  &-c  ,  c-«  ,  a-ft  ,  (b-c)(c-a)(a-b) 

148.) 1 -\ 1-7 r-j re, ,. 

x -  a    x-b     x-c     (x-a)(x-b)(x-c) 

(49.)  2(a+p)(a  +  q)f{a-b)(a-c)[a  +  h). 

(50.)  2a2/(a-b){a-c)(h-a).  (51.)  2a2/(a2-b°-)(o2-c2)(h2  +  a2). 

(52. )  Z(y2  +  0-  x2)/yz(x  -  y)  (x  -  z). 

a(b-c)3  +  b(c-a)3  +  c(a-b)s  +  {b2-c2)(b-c)  +  (c2-a2)(c-a)  +  (a2-b2)(a-b) 
a2(b-c)  +  b\c-a)  +  c2(a-b) 
{U)     {{x  +  yf  +  {y  +  zf)  {(z  +  xy>  +  (x  +  w)2} 

{(z  +  y){z  +  x)  +  (y  +  z)(x  +  w)}2+{(x+~y)(x  +  w)-{y  +  z){z  +  x)}2 


(53.) 


Prove  the  following  identities  : — 
(55.)  2a3/(a-b){a-c)  =  Za. 
(56.)  c(ic2-v)  =  au(l  -uv),     c{v2-u)  =  bv{l  -uv), 
where  tc  =  {ab-c2)j{bc-a2),     v=(ab-c2)/(ca-b2). 

(57. )  2  (a  +  a) (a  +  /3) (a  +  y)(a{a -b){a-c){a-d)=  - aPyfabcd. 

abed 

.  (b-c)3  +  (c-a)3  +  (a-bf  K        ' 


(59.) 


(60.) 


(ab  -  erf)  (a2  -  62  +  c2  -  rf2)  +  («c  -  bd)  (a2  +  b2-c2-  d2) 
(a2  -  b-  +  c-  -  W)  (a2  +  b2  -  c2  -  d2)  +  4.{ab  -  cd)  (fflc  -  bd) 

(b  +  c)(a  +  d) 
~(b  +  c)2+(a  +  df 
a5(c  -b)  +  b\a  -  c)  +  c5(6  -  a) 


(c-  b)(a-c)(b-a) 
(61.)  {2{y-8)8}/{2(y-^}-4n(y-Z)a={2a?-2^}». 


Decompose  the  following  into  sums  of  partial  fractions  :  — 
(62.)  0r2-l)/(x-2)(;«-3).  (63.)  x2/(x-  l)(x-2)(x-  3). 

(64.)  30a*/(a?-l)(a?-4).  (65.)  (.c2  +  4)/(a;  +  l)2(x-2)(x  +  3). 

VOL.  I  M 


1G2 


EXERCISES  XII 


CHAP.    VIII 


(66.)  (&-2)l(a?-l). 

(68.)  {2x-3)/(x-l)(x2  +  iy. 


(67.)  (z2  +  *  +  l)/(a;  +  l)(z2  +  l). 

(69.)  l/{x-a)(x-b)(x2-2px  +  q),  p*<q. 


(70.)  (l  +  aj  +  a?)/(l -»-»*  + a5).    (71.)  18/(ar*  +  4;e+8). 
(72.)  (*  +  3)/(^-l).  (73.)  lKafi  +  tf-rf-a*). 

(74.)  Express  (3a2  +  ic  +  l)/(a;8- 1)  as  the  sum  of  two  rational  fractions 
whose  denominators  are  xi-\  and  x4  +  l. 

(75.)  Expand  1/(3  -x)  (2  +  a?)  in  a  series  of  ascending  powers  of  x,  using 
partial  fractions  and  continued  division. 

(76.)  Expand  in  like  manner  1/(1  -x)2(l+x2). 

(77.)  Show  that 
2  (b  +  c  +  d)/(b-a)(c-ct)(d-a)(x -  a)  =  (x-a-b-c-d)J(x - a)(x -  b)(x -  c)(x -  d). 

abed 


CHAPTER    IX. 
Further  Application  to  the  Theory  of  Numbers. 

ON    THE   VARIOUS    WAYS    OF    REPRESENTING    INTEGRAL   AND 
FRACTIONAL    NUMBERS. 

§  1.]  The  following  general  theorem  lies  at  the  root  of  the 
theory  of  the  representation  of  numbers  by  means  of  a  systematic 
scale  of  notation  : — 

Let  rl}  r.,,  r3,  .  .  .,  rn,  rn+1,  .  .  .  denote  an  infinite  series  of 
integers*  restricted  in  no  way  except  that  each  is  to  be  greater  than  1, 
then  any  integer  N  may  be  expressed  in  the  finite  form — 

N  =p0  +plTl  +  p2r1r.2  +iW8ra  +  •  •  •  +iWa .  .  .  rn, 

where  p0<ru  px<rs,  p.2<r3,  .  .  .,  pn<rn+l.      When  ru  r.2,  ra,  .  .   . 
are  given,  this  can  be  done  in  one  way  only. 

For,  divide  N  by  rlt  the  quotient  being  N,  and  the  remainder 
p0 ;  divide  N\  by  r2,  the  quotient  being  N2  and  the  remainder 
pl}  and  so  on  until  the  last  quotient,  say  pn,  is  less  than  the  next 
number  in  the  series  which  falls  to  be  taken  as  divisor.  Then,  of 
course,  the  process  stops.     We  now  have 

N  =p0  +  T$1rl     (j?0<0  (1), 

Nt  =Pl  +  N2r2     (px<r3)  (2), 

N3=^2  +  N3r3     (pt<ra)  (3), 


N„  _ ,  =  pn  _ !  +  pnrn{  pn  _  !<r„)  (n). 

*  In  this  chapter,  unless  the  contrary  is  distinctly  implied,  every  letter 
used  denotes  a  positive  integral  number. 


164  FACTORIAL  SERIES  FOR  AN  INTEGER  chap. 

From  (1),  using  (2),  we  get 

N=Po  +  r1(p1  +  'N,r2), 
=Po  +  PiTi  +rjrJSr 
Thence,  using  (3), 

N  =p0  +P{>\  +  PJV2  +  W.N,, 
and  so  on. 

Thus  we  obtain  finally 
N  =p0  +PS\  +iWg  +  pj\r2r3  +  .  .   .  +  pnr1r2 . .  .  rn         (A). 
Again,  the  resolution  is  possible  in  one  way  only.     For  suppose 
we  also  had 

N  =p0'  +p1'r1  +  p2'r1r2  +  p3'r1r2r3  +  .  .  .  +pn'r1r2 .  .  .  rn     (B), 

then,  equating  (A)  and  (B),  and  dividing  both  sides  by  rlt  we 
should  have 

p0 

-  +  (Pi  +P*ra  +par2ra  +  .  .  .  +pnr3ra . . .  rn) 

'  i 

=  7  +  (ft'+ft''i+A'Vi  +  .  •  •  +Pn'rara . . .  rn)        (C). 
'  i 

But  the  two  brackets  on  the  right  and  left  of  (C)  contain  integers, 
and  p0fr}  and  p0'/rl  are,  by  hypothesis,  each  a  proper  fraction. 
Hence  we  must  have^,/^  -pdj^'i  ',  that  is, 

Po*=Po, 

px  +p2re  +  p3r2r3  +  .  .  .4  pnr2r3 . . .  rn 

=  Pi  +P*r*  +  pa'rara  +  .  .  .  +  pn'r2r3 .  . .  rn  (D). 

Proceeding  now  with  (D)  as  we  did  before  with  (C),  we  shall 
prove  Pi—pi';  and  so  on.  In  other  words,  the  two  expressions 
(A)  and  (B)  are  identical. 

Example.   Let  N  =  719,  and  let  the  numbers  r\,  r%,  rs,  .  .  .  be  the  natural 
series  2,  3,  4,  5,  .   .  .     Carrying  out  the  divisions  indicated  above,  we  have 

2)719 

3)359  ...    1 

4)119  ...   2 

5)29  ...  3 

5  ...  4. 


ix  FACTORIAL  SERIES  FOR  A  FRACTION  165 

Hence  Po  =  l,  2*1=2,  #s=3,  2>s=4,  Pi=5  ; 

and  we  have     719  =  1  +  2x2  +  3x2.3  +  4x2.3.4  +  5x2.3.4.5. 

§  2.]  There  is  a  corresponding  proposition  for  resolving  a 
fraction,  namely,  ru  r.,,   .  .   .,  rn,  &c,  being  as  before, 

Any  proper  fraction  A/B  can  be  expressed  in  the  form 

±  =  Pi+r±.  +  J!±-+.  .  .  +     *>»     +F 

B      r,     i\r2     r,r,2r3  i\r2 .  .  .  rn 

where  p^r^  p.2<r2,  .  .  .,  pn<rn;  and  F  is  either  zero  or  can  be  made 
as  small  as  we  please  by  taking  a  sufficient  number  of  the  integers 
ru  r2,  .  .  .,  rn.  When  o\,  r2,  .  .  .,  rn,  .  .  .  are  given,  this  resolution 
can  be  effected  in  one  way  only. 

The  reader  will  have  no  difficulty  in  deducing  this  proposition 
from  that  of  last  paragraph.     It  may  also  be  proved  thus  : — 

A  _  Ar,  _  Ar,/B 

b^bt;-"^-' 

Now  we  may  put  A^/B  into  the  form  pl  +  qJB,  where  g\<B. 
We  then  have 

A     px  +  g,/B 
B~       r>       ' 

where  pi<rXi  since,  by  hypothesis,  A<B. 
Hence 

-  =  ^  +  --^  (1) 

Treating  the  proper  fraction  ^,/B  in  the  same  way  as  we  treated 
A/B,  we  have 


(.2). 


B      r2  +  r2 

°2 

B' 

where 

2>*<rai  &<B 

Similarly, 

I2  =  il  +  I 
B      r3     ra 

ft 

B' 

"'"• 

Pa<ra,  23<~B,  &c 

(3). 


166  FACTORIAL  SERIES  FOR  A  FRACTION  chap. 

And,  finally, 

gn-i  =  Pn      2_  .  ?» 

B        7-M     r„    B' 
where  Ihi^n,  8»<B  (w). 

Now,  using  equations  (1),  (2),  .  .  .,   (n)  in  turn,  we  deduce 
successively 


B      r,     rxr2     r1raBf 


r,     r,r2     v/,     W.B' 


^'  +  A  +  _J?i_  +  ■         ^ 


+ q—  p  (A), 

r,r8 . . .  rnB 

where  p^r,,  p2<r.2,  .  .  .,  p?i<rn,  qn<B. 

It  appears  therefore  that  F  =  qn\r{r%  .  .  .  rnB,  which  can 
clearly  be  made  as  small  as  we  please  by  sufficiently  increasing 
the  number  of  factors  in  its  denominator.  This  of  course  in- 
volves a  corresponding  increase  in  the  number  of  the  terms  of 
the  preceding  series. 

It  may  happen,  of  course,  that  qn  vanishes,  and  then  F  =  0. 
We  leave  it  as  an  exercise  for  the  student  to  prove  that  this  case 
occurs  when  rfa  .  .  .  rn  is  a  multiple  of  B,  and  that  if  A/B  be 
at  its  lowest  terms  it  cannot  occur  otherwise.  He  ought  also  to 
find  little  difficulty  in  proving  that  the  resolution  is  unique  when 
fii  r„  •  •  .,  rn,   .  .  .  are  given. 

Example  1.  Let  A/B  =  444/576,  and  let  the  numbers  r\,  r%,  &c. ,  be  2,  4, 
6,  8,  &c. 

We  find  444     1       2       1_ 

57«~2  +  2.4  +  2.4.6' 
Example  2.  A/B  =  11/13,  r1;  r«,  &c.,  being  2,  3,  4,  5,  6,  .   .   .,  &c. 
11     1       2  0  1  3  3 


16     22,32. 8. 42. 3. 4. 52. 3. 4. 5. 62. 3. 4. 5. 6x13 

Since  T\,  r2,  &c,  are  arbitrary,  we  may  so  choose  them  that  the  numer- 
ators pit  ju,  &c,  shall  each  be  unity.  We  thus  have  a  process  for  decompos- 
ing any  fraction  into  a  sum  of  others  with  unit  numerators. 


IX  EXAMPLES                                                   1G7 

Example  3.             11  5                        1 

2x  3x                    13  x 

13)22(1  13)15(1              13~)l3(l 

13  13                      13 

9  2                         0 

2x  7x 

13)18(1  13)14(1 

13  13 


Whence 


5  1 


n_i    _i_       l         _i i 

13~2  +  2.2  +  2.2.3  +  2.2.3.7+2.2.3.7.13" 


Here  we  have  chosen  at  each  step  the  least  multiplier  possible.  When 
this  is  done,  it  may  be  shown  that  the  successive  remainders  diminish  down 
to  zero,  the  successive  multipliers  increase,  and  the  process  may  be  brought 
to  an  end.  If  this  restriction  on  the  multiplier  be  not  attended  to,  the  reso- 
lution may  be  varied  in  most  cases  to  a  considerable  extent.  Since,  however, 
we  always  divide  by  the  same  divisor  B,  there  are  only  B  possible  remainders, 
namely,  0, 1,  2,  .  .  .,  B  -  1 ;  hence  after  B  -  1  operations  at  most  the  remainder 
must  recur  if  the  operation  has  not  terminated  by  the  occurrence  of  a  zero. 

Example  4.  Thus  we  have 

2_1       1 

3~2  +  2.3  ' 

.  Ill  li 

also  =o+?r- 7  +  ^r-75+.  •  .+s— r„  +  ; 


2     2.4     2. 42  2.4"     2.  4". 3' 


Example  5. 

U  +  JU 


29     5     5  .  5     5  . 5  .  29  ' 

als°  4nV^  +  ^  +  CT  +  ^  +  5^+5T^  +  &C-  ; 

,  111  1 

also  =  -  +  t—z ■  +  ,    „   „  +  - 


66. 3     6. 3. 36.  3.  3. 29' 

and  so  on. 

§  3.]  The  most  important  practical  case  of  the  proposition  in 
§  1  is  that  where  r„  r2,  .  .  .  are  all  equal,  say  each  =r.  Then 
we  have  this  result — 

Every  integer  N  can  be  expressed,  and  that  in  one  tvay  only,  in 
the  form 

P*rn+Pn-Sn~1+  •   •  •  +2hr+p0, 
where _p0,  piy  .  .  .,  pn  are  each  < r. 

In  other  words,  detaching  the  coefficients,  and  agreeing  that 
their  position  shall  indicate  the  power  of  r  which  they  multiply, 
and  that  apposition  shall  indicate  addition  (and  not  multiplica- 
tion as  usual),  we  see  that,  r  being  any  integer  whatever  chosen 


168  SCALES  OF  NOTATION,  INTEGERS  CHAP. 

as  the  radix  of  a  scale  of  notation,  any  integer  whatever  may  be 
represented  in  the  form  pnpn-i  •  •  •  PiPol  where  each  of  the 
letters  or  digits  p0,  plf  .  .  .,  pn  must  have  some  one  of  the  integral 
values  0,  1,  2,  3,  .  .  .,  r  -  1. 

For  example,  if  r  =  1 0,  any  integer  may  be  represented  b.y 
PnJPn-i  ■  •  •  P\Po  where  p0,Pi,  •  •  -,pn  have  each  some  one  of 
the  values  0,  1,  2,  3,  4,  5,  G,  7,  8,  9. 

The  process  of  §  1  at  once  furnishes  us  with  a  rule  for  finding 
successively  the  digits  p0,P\,p2,  .  .  .,  namely,  Divide  the  given  integer 
N  by  the  chosen  radix  r,  the  remainder  will  be  p0 ;  divide  the  integral 
quotient  of  last  division  by  r,  the  remainder  will  be  pt ,  and  so  on. 

Usually,  of  course,  the  integer  N  will  be  given  expressed  in 
some  particular  scale,  say  the  ordinary  one  whose  radix  is  10; 
and  it  will  be  required  to  express  it  in  some  other  scale  whose 
radix  is  given.  In  that  case  the  operations  will  be  carried  on  in 
the  given  scale. 

The  student  will  of  course  perceive  that  all  the  rules  of  ordi- 
nary decimal  arithmetic  are  applicable  to  arithmetic  in  any  scale, 
the  only  difference  being  that,  in  the  scale  of  7  say,  there  are 
only  7  digits,  0,  1,  2,  3,  4,  5,  6,  and  that  the  "carriages"  go  by 
7's  and  not  by  10's. 

If  the  radix  of  the  scale  exceeds  10,  new  symbols  must  of 

course  be  invented  to  represent  the  digits.     In  the  scale  of  12, 

for  example,   digits  must  be  used  for  10  and  11,  say  t  for  10 

and  e  for  11. 

Example  1.  To  convert  136991  (radix  10)  into  the  scale  of  12. 

12)136991 


12)11415 

.   . 

.    e 

12)951 

.   . 

.   3 

12)79 

.   3 

6 

.   7 

The  result  is 

6733e. 

Example 

2.   To  convert  G733e  (radix 

12) 

into  the  scale  of  r. 

r)6733e 

T)7el7 

.   . 

.   1 

t-)9i;i 

.  9 

r)e4 

.    . 

.   9 

r)ll 

.   6 

1 

.   3 

The  result  is 

136991. 

IX  EXAMPLES  OF  ARITHMETICAL  OPERATION  1G9 

Although  this  method  is  good  practice,  the  student  may  very  probably 
prefer  the  following  : — 

6733e  (radix  12)  means 
6xl24  +  7xl23  +  3xl2a  +  3xl2  +  ll. 

Using  the  process  of  chap,  v.,  §  13,  Example  1,  we  have 

6+    7  +     3+         3+  11 

+  72  +  948  +  11412  +  136980 
6  +  79  +  951  + 11415  + 136991. 

§  4.]  From  one  point  of  view  the  simplest  scale  of  notation 
would  be  that  which  involves  the  fewest  digits.  In  this  respect 
the  binary  scale  possesses  great  advantages,  for  in  it  every  digit 
is  either  0  or  1.  For  example,  365  expressed  in  this  scale  is 
101101101.  All  arithmetical  operations  then  reduce  to  the 
addition  of  units.  The  counterbalancing  disadvantage  is  the 
enormous  length  of  the  notation  when  the  numbers  are  at  all 
large. 

"With  any  radix  whatever  we  can  dispense  with  the  latter 
part  of  the  digits  allowable  in  that  scale  provided  we  allow  the 
use  of  negative  digits.  For  let  the  radix  be  r,  then  whenever, 
on  dividing  by  r,  the  positive  remainder  p  is  greater  than  r/2,  we 
can  add  unity  to  the  quotient  and  take  -  (r  -  p)  for  a  negative 
remainder,  where  of  course  r-p<r/2.  For  example,  3978362 
(radix  10)  might  be  written  4022442,  where  2  stands  for  -2; 
so  that  in  fact  4022442  stands  for  4-10°  +  O'lO5  -  2"104  -  2-103 
+  4-102-4-10  +  2. 

Example  1.   Work  out  the  product  of  1698  and  314  in  the  binary  scale. 

1698  =  11010100010 
314=     100111010 


11010100010 
11010100010 
11010100010 
11010100010 
110101000100 

10000010001010110100  (  =  533172  radix  10). 

Example  2.  Express  1698  and  314  in  the  scale  of  5,  using  no  digit  greater 
than  3,  and  work  out  the  product  of  the  two  transformed  numbers. 


170  EXAMPLES  OF  ARITHMETICAL  OPERATION  chap. 

5)1698  5)314 


5)339  .  . 
5)68  .  . 
5)13  . 

.  3 
.  1 
.  3 

5)63  .  . 

5)12  .  . 

2  . 

.  1 
.  3 
.  2 

2  . 

.  3 

23313 

2231 

23313 
131111 
102111 

102111 

121121303     * 
The  student  may  verify  that  121121303  (radix  5)  =  533172  (radix  10). 

Example  3.  Show  how  to  weigh  a  weight  of  315  lbs.  :  first,  with  a  series 
of  weights  of  1  lb. ,  2  lbs.,  22  lbs.,  23  lbs.,  &c,  there  being  one  of  each  kind  ; 
second,  with  a  series  of  weights  of  1  lb.,  3  lbs.,  32  lbs.,  33  lbs.,  &c,  there  being 
one  only  of  each  kind. 

First.  Express  315  in  the  binary  scale.     We  have 
315  =  100111011, 
315  =  l+2  +  23  +  24  +  25  +  28. 
Hence  we  must  put  in  one  of  the  scales  of  the  balance  the  weights  1  lb.,  2  lbs., 
23  lbs.,  21  lbs.,  25  lbs.,  and  28  lbs. 

Second.  Express  315  in  the  ternary  scale,  using  no  digit  greater  than 
unity.     We  have 

315  =  110100. 

Hence  over  against  the  given  weight  we  must  put  the  weights  34  lbs.  and  35 
lbs. ;  and  on  the  same  side  as  the  given  weight  the  weight  32  lbs. 

§   5.]  If   we   specialise    the   proposition  of  §   2   by   making 

r,  =  r2  -  . . .  =  rn,  each  =  r  say,  we  have  the  following : — Every  proper 

fraction  A/B  can  be  expressed,  and  that  in  one  way  only,  in  the  form — 

A     Pi  ,  p*  ,  pa  ,  ,  pn 


+  " 


B      r      r2     r 


4.3  vn  > 


where  pu  p2,  .  .   .,  pn  are  each<r,  and  F  either  is  zero,  or  can  be 
made  as  small  as  we  please  by  sufficiently  increasing  n. 

If  r  be  the  radix  of  any  particular  scale  of  notation,  the  fraction 


r      r»  rn 


*  The  arrangement  of  the  multiplication  in  Examples  1  and  2  is  purposely 
varied,  because,  although  it  is  of  no  consequence  here,  sometimes  the  one  order 
is  more  convenient,  sometimes  the  other.  A  similar  variety  is  introduced  in 
§  6,  Examples  1  and  2. 


IX  IN  VARIOUS  SCALES  171 

is  usually  called  a  radix  fraction.  We  may  detach  the  coeffi- 
cients and  place  them  in  apposition,  just  as  in  the  case  of 
integers,  a  point  being  placed  first  to  indicate  fractionality. * 
Thus  we  may  write 

A 

where  px  in  the  first  place  after  the  radix  point  stands  for  px/r, 
p2  in  the  second  place  stands  for  pa/r*,  and  so'  on. 

Since  the  digits  pxp.zp3  .  .  .  pn  are  the  integral  part  of  the 
quotient  obtained  by  dividing  Arn  by  B,  the  radix  fraction  can- 
not terminate  unless  Arn  is  a  multiple  of  B  for  some  value  of  n. 
Hence,  if  we  suppose  A/B  reduced  to  its  lowest  terms,  so  that  A 
is  prime  to  B,  we  see  that  the  radix  fraction  cannot  terminate 
unless  the  prime  factors  of  B  (see  chap,  iii.,  §  10)  be  powers  of 
prime  factors  which  occur  in  r.  For  example,  since  r=10  =  2x5, 
no  vulgar  fraction  can  reduce  to  a  terminating  decimal  fraction 
unless  its  denominator  be  of  the  form  21"5'\ 

In  all  cases,  however,  where  the  radix  fraction  does  not 
terminate,  its  digits  must  repeat  in  a  cycle  of  not  more  than 
B  -  1  figures  ;  for  in  the  course  of  the  division  no  more  than  B  -  1 
different  remainders  can  occur  (if  we  exclude  0),  and  as  soon  as 
one  of  the  remainders  recurs  the  figures  in  the  quotient  begin 
to  recur. 

Example  1.  To  express  2/3  as  a  radix  fraction  in  the  scale  of  10  to  within 
l/100000th— 

2_  200000  _  66666+j 
3~3xl05~        L05      ' 

_6xl04  +  6xl03  +  6xl02  +  6xl0  +  6        2/3 

105  + 100000' 


6       6        6        6        6^ 
10     102     10J     104     103       ' 


where  F  = 


2/3     ^       1 

1000U0<100000' 


*  Napier  of  Merchiston  was  apparently  the  first  who  used  the  modern  form 
of  the  notation  for  decimal  fractions.  The  idea  of  the  regular  progression  of 
decimals  is  older.  Stevin  fully  explains  its  advantages  in  his  ArithmMique 
(1585);  and  germs  of  the  idea  may  be  traced  much  farther  back.  According 
to  those  best  qualified  to  judge,  Napier  was  the  first  who  fully  appreciated  the 


172  EXAMPLES  OF  RADIX  FRACTIONS  CHAP. 

In  other  words,  we  have  to  the  required  degree  of  accuracy 

~=  -66666. 
o 

It  is  ohvious  from  the  repetition  of  the  figures  that  if  we  take  n  6's  after  the 

point  we  shall  have  the  value  of  2/3  correct  within  l/10"th  of  its  value. 

Example  2.  Let  the  fraction  be  5/64.     Since  64  =  2s  this  fraction  ought 
to  be  expressible  as  a  terminating  decimal.     "We  have  in  fact 
5      5000000     78125 


64 

64  x  10s 
=  •078125 

106 

5 

Example   3 

.    To 

express 

2/3   as 

a  radix  fraction 

in 

the 

scale 

of 

2 

to 

within  l/23th. 

2 
3: 

2x26 
~3x2B_ 

128/3 
26 

42  +  2/3 
26      * 

Neglecting 

2/3      i  •  i,  ■ 

-p".  which  is  <  ^  and 

expressing  42  in 

the  scale  of  2, 

we 

have 

2 
3: 

101010 
26 

=  -101010  (radix  2). 

§  6.]  When  a  fraction  is  given  expressed  as  a  radix  fraction 
in  any  scale,  and  it  is  required  to  express  it  as  a  radix  fraction 
in  some  other  scale,  the  following  process  is  convenient. 

Let  <f>  be  the  fraction  expressed  in  the  old  scale,  r  the  new 
radix,  and  suppose 

.      .Pi  .iV-Pa  , 

^     r      r2     r 

then  r<b  =  p ,  +  -+^  +  .  .  . 

=  [\  +  <£i  say. 
Now  $,  is  a  proper  fraction,  hence  px  is  the  integral  part  of  r<f>. 

A         •  Pa 

Again  ?•</>!  =pa  +  — +  .    .   . 

=jpa  +  &  say. 
So  that pa  is  the  integral  part  of  r$u  and  so  on. 

It  is  obvious  that  a  vulgar  fraction  in  any  scale  of  notation 
must  transform  into  a  vulgar  fraction  in  any  other ;  and  we  shall 

operational  use  of  the  decimal  point  ;  and  in  his  Constructio  (written  long 
before  his  death,  although  not  published  till  1619)  it  is  frequently  used.  See 
Glaisher,  Art.  "  Napier, "  Encyclopaedia  Britannka,  9th  ed.;  also  Eae's  recent 
translation  of  the  Constructio,  p.  89. 


ix  EXAMPLES  173 

show  in  a  later  chapter  (see  Geometrical  Progression)  that  every 
repeating  radix  fraction  can  be  represented  by  a  vulgar  fraction. 
Hence  it  is  clear  that  every  fraction  which  is  a  terminating  or  a 
repeating  radix  fraction  in  any  scale  can  be  represented  in  any 
other  scale  by  a  radix  fraction  which  either  terminates  or  else 
repeats.  It  is  not,  however,  true  that  a  terminating  radix  fraction 
always  transforms  into  a  terminating  radix  fraction  or  a  repeater 
into  a  repeater.  Non-terminating  non-rejieating  radix  fractions 
transform,  of  course,  into  non-terminating  non-repeating  radix 
fractions,  otherwise  we  should  have  the  absurdity  that  a  vulgar 
fraction  can  be  transformed  into  a  non-terminating  non-repeating 
radix  fraction. 

It  is  obvious  that  all  the  rules  for  operating  with  decimal 
fractions  apply  to  radix  fractions  generally. 

Example  1.  Reduce  3*168  and  11  "346  to  the  scale  of  7,  and  multiply  the 
latter  by  the  former  in  that  scale  ;  the  work  to  be  accurate  to  l/1000th 
throughout. 

The  required  degree  of  accuracy  involves  the  5th  place  after  the  radical 
point  in  the  scale  of  7. 

•346 
7 


•168 

_7 
1)-176 

_7 
1)232 

_7 
l)-624 

_7 
4)-368 

_7 
2V576 


2)-422 

_7 
2) -954 

_7 
6)-678 

_7 
4)746 

_7 
5) -222 

3-168  =  3-11142  (radix  7).  11-346  =  14-22645. 


14-22645 
3-11142 

46-01601 

1-42265 

14227 

1423 

632 

32 

50-64146 


174  REMAINDER  ON  DIVIDING  BYf-1  chap. 

On  account  of  the  duodecimal  division  of  the  English  foot  into  12  inches, 
the  duodecimal  scale  is  sometimes  convenient  in  mensuration. 

Example  2.  Find  the  number  of  square  feet  and  inches  in  a  rectangular 
carpet,  whose  dimensions  are  21'  3|"  by  13'  llf".  Expressing  these  lengths 
in  feet  and  duodecimals  of  a  foot,  we  have 

21'  3|"  =  19-36. 
13'  ll|"=ll'e9. 

If,  following  Oughtred's  arrangement,  we  reverse  the  multiplier,  and  put  the 
unit  figure  under  the  last  decimal  place  which  is  to  be  regarded,  the 
calculation  runs  thus — 

19-36 
9ell 


19360 

1936 

1763 

13e 


20978 

209  (radix  12)  =  288 +  9  =  297  (radix  10)  feet. 
•78  (radix  12)  =  7  x  12  +  8  =  92  square  inches. 
Hence  the  area  is  297  feet  92  inches. 

§  7.]  If  a  number  N  be  expressed  in  the  scale  of  r,  and  if  we 
divide  N  and  the  sum  of  its  digits  by  r  -  1 ,  or  by  any  factor  of  r—  1 , 
the  remainder  is  the  same  in  both  cases. 

Let         N  =  p0  +  ptr  +  p2r*  +  .  .  .  +  pnrn. 
Hence  N  -  (p0 +i>x  +  •  •  -  +  Pn)  =  Pi{r  -  I)  +  p.2(r2  -  1)  +  .  .  . 

+  Pn(rn~l)  (1). 

Now,  m  being  an  integer,  rm  -  1  is  divisible  by  r  —  1  (see 
chap,  v.,  §  17).  Hence  every  term  on  the  right  is  divisible  by 
r  -  1,  and  therefore  by  any  factor  of  r  -  1.  Hence,  p  being  r  —  1, 
or  any  factor  of  it,  and  /x  some  integer,  we  have 

N-0'o  +;>,  +  .  •  -+pn)  =  W  (2). 

Suppose  now  that  the  remainder,  when  N  is  divided  by  p,  is  <r, 
so  that  N  =  vp  +  <t.     Then  (2)  gives 

p0  +  p,  +  .    .   .  +  pn  =  (v  -  fl)p  +  o-  (3), 

which  shows  that  when  p0+Pi  +  •   •  .  +pn  is  divided  by  p  the 
remainder  is  <r. 


IX  CASTING  OUT  THE  NINES  175 

Cor  1.  In  the  ordinary  scale,  if  we  divide  any  integer  by  9  or  by 
3,  the  remainder  is  the  same  as  the  remainder  we  obtain  by  dividing 
the  sum  of  its  digits  by  9  or  by  3. 

For  example,  31692-^9  gives  for  remainder  3,  and  so  does 
(3  +  1  +  G  +  9  +  2)  -+-  9. 

Cor.  2.  It  also  follows  that  the  sum  of  the  digits  of  every  midtiple 
of  9  or  3  must  be  a  multiple  of  9  or  3.     For  example, 

2x9-18  1  +  8  =  9  ■ 

13  x  9-117  1  +  1  +  7  =  9 

128x9  =  1152  1  +  1+5  +  2  =  9 
128x3  =  384  3  +  8  +  4  =  15  =  5x3. 

§  8.]  On  Cor.  1  of  §  7  is  founded  the  well-known  method 
of  checking  arithmetical  calculations  called  "  casting  out  the 
nines." 

Let  L  =  MN  ;  then,  if  L  =  19  +  L',  M  =  m9  +  M',  N  =  nd  +  N', 
so  that  L',  M',  N'  are  the  remainders  when  L,  M,  N  are  divided 
by  9,  we  have — 

19  +  L'  =  (m9  +  M')  (nd  +  N'), 

=  mra81  +  (M'w  +  N'm)9  +  M'N', 
=  (mn9  +  Wn  +  N'm)9  +  M'N' ; 

whence  it  appears  that  L'  and  M'N'  must  have  the  same  re- 
mainder when  divided  by  9.  L',  M',  N'  are  obtained  in  accord- 
ance with  Cor.  1  of  §  7  by  dividing  the  sums  of  the  digits  in  the 
respective  numbers  by  9. 

Example  1.  Suppose  we  wish  to  test  the  multiplication 
47923x568  =  27220264. 
To  get  the  remainder  when  47923  is  divided  by  9,  proceed  thus:  4  +  7  =  11, 
cast  out  9  and  2  is  left  ;  2  +  9  =  11,  cast  out  9;  2  +  2  +  3  =  7.  The  remainder 
is  7.  Similarly  from  563  the  remainder  is  1,  and  from  27220264,  7.  Now 
7x1  +  9  gives  of  course  the  same  remainder  as  7+^9.  There  is  therefore  a 
strong  presumption  that  the  above  multiplication  is  correct.  It  should  be 
observed,  however,  that  there  are  errors  which  this  test  would  not  detect  ;  if 
we  replaced  the  product  by  27319624,  for  instance,  the  test  would  still  be 
satisfied,  but  the  result  would  be  wrong. 

In  applying  this  test  to  division,  say  to  the  case  L/M  =  N  +  P/M,  since 
we  have  L  =  MN  +  P,  and  therefore  L-  P  =  MN,  we  have  to  cast  out  the  nines 
from  L,  P,  M,  and  N,  and  so  obtain  L',  P',  M',  and  N'  say.  Then  the  test  is 
that  L'  -  P'  shall  be  the  same  as  the  result  of  casting  out  the  nines  from  M'N'. 


176  LAMBERT'S  THEOREM  CHAF. 

Example  2.  Let  us  test — 

27220662+-568  =  47923  + 398  +  568, 
or  27220662  =  47923x568  +  398. 

Here  L'  -  P'  =  0-  2=  -2, 

M'.N'=7x  1=9-2. 
The  test  is  therefore  satisfied. 

§  9.]*  The  following  is  another  interesting  method  for  ex- 
panding any  proper  fraction  A/B  in  a  series  of  fractions  with 
unit  numerators  : — 

Let  (?!,  q,,  qa,  .  .  .,  qn,  and  rx,  r2,  ?-3,  .  .  .,  rn,  be  the  quotients  and 
remainders  respectively  when  B  is  divided  by  A,  rlt  r2,  .  .  .,  rn_,  re- 
spectively, then 

-  = + .  .  .  +  v i —  +  F  (1), 

B      ft      q,q2     q,q^3  q,q2...qn 

where  F  =  (  -  1  )ni "nJMi  •  •  •  on~B,  that  is,  F  is  numerically  less  than 
1/qfa  .  .  .  qn. 

For  we  have  by  hypothesis 

B  =  Aqx  +  ru  therefore  A/B  =  l/g1  -  rjqfi  (2), 

B  =  i\q2  +  rs,  therefore  rjB  =  l/q2-  r2/q2B  (3), 

B  =  r2q3  +  r3,  therefore  r„/B  =  l/q3  -  r3Jq3~B  (4), 

and  so  on. 

From  (2),  (3),  (4),  we  have  successively 
A.l     J_     J_AY\ 
B~?i     Mi    2&W' 

=  ±-±  +  -l LfcV 

2i     Mi     MA     Mzl^W' 
and  so  on. 

Since  rn  r2,  .  .   .,  rn  go  on  diminishing,  it  is  obvious  that,  if 

A  and  B  be  integers  as  above  supposed,  the  process  of  successive 

division  must  come  to  a  stop,  the  last  remainder  being  0.     Hence 

*  In  Lis  Essai  d' Analyse  Numirique  sur  la  Transformation  dcs  Fractions 
(CEuvres,  t.  vii.  p.  313),  on  which  the  present  chapter  is  founded,  Lagrange 
attributes  the  theorem  of  §  9  to  Lambert  (1728-1777).  Heis,  Sammlung  von 
Bcispielen  und  Au/gaber.  aits  dcr  allgemeinen  Arithmetik  und  Algebra  (1882),  p. 
322,  has  applied  series  of  this  character  to  express  incommensurable  numbers 
such  as  logarithms,  square  roots,  &c.  In  the  same  connection  see  also  Syl- 
vester, American  Jour.  Math.,  1880.  Sec  also  Cyp.  Stephanos,  Bull.  Soc. 
Math.  Fr.  7  (1879),  p.  81  ;  G.  Cantor,  Zeitsch.  f.  Math.  14  (1869),  p.  124  ; 
J.  Liiroth,  Math.  Ann.  21  (1883),  p.  411. 


IX 


EXERCISES  XIII  177 


every  vulgar  fraction  can  be  converted  into  a  terminating  series 
of  the  form 

1     JL      JL 


Example. 


113     1        1  1 

:  + 


244     2     2.13     2.13.24     2.13.24.61 


From  this  resolution  we  conclude  that  1/2-1/2.13  represents  113/244  within 
l/26th,  and  that  1/2-1/2.13  +  1/2.13.24  represents  113/244  within  l/624th. 


Exercises  XIII. 

(1.)  Express  16935  (scale  of  10)  in  the  scale  of  7. 
(2.)  Express  16-935  (scale  of  10)  in  the  scale  of  7. 
(3.)  Express  315  "34  (scale  of  10)  in  the  scale  of  11. 
(4.)   Express  r7e9ee  (scale  of  12)  in  the  scale  of  10. 
(5.)  Express  Ir8e54  (scale  of  12)  in  the  scale  of  9. 
(6.)  Express  345"361  (scale  of  7)  in  the  scale  of  3. 
(7.)  Express  112/315  (scale  of  10)  as  a  radix  fraction  in  the  scale  of  6. 
(8.)  Express  3169  in  the  form  ^  +  g3  +  r3.5+s3.5.7  +  &c,   where  ]i<3, 
2<5,  r<7,  &c. 

(9.)  Express   7/11    in    the    form  pl2  +  q/2.S  +  r/2.ZA  +  kc.,  where  p<2, 
q<3,  r<4,  &c. 

(10.)  Express  113/304  in  the  form ^3  +  ?/3.5  +  r/32.5  +  s/32.52-M/33.52  f  &r., 
where  p<  3,  q<5,  r<3,  &c. 

(11.)  Multiply  31263  by  56341  in  the  scale  of  7. 

(12.)  Find  correct  to  4  places  31  -3432  x  150323,  both  numbers  being  in 
the  scale  of  6. 

(13.)  Find  to  5  places  31  -3432-7-2  67312,  both  numbers  being  in  the  scale 
of  12. 

(14.)  Extract  the  square  root  of  365738  (scale  of  9)  to  3  places. 
(15.)  Express  887/1103  in  the  form  l/qi  -  l/qiq»  +  l/qiq«q3  -  &c- 
(16.)  Show  how  to  make  up  a  weight  of  35  lbs.  by  taking  single  weights 
of  the  series  1  lb.,  2  lbs.,  22  lbs.,  &c. 

(17.)  With  a  set  of  weights  of  1  lb.,  5  lbs.,  52  lbs.,  &c,  how  can  7  cwt.  be 
weighed  ?  First,  by  putting  weights  in  one  scale  only  and  using  any  number 
of  equal  weights  not  exceeding  four.  Second,  by  putting  weights  in  either 
scale  but  not  using  more  than  two  equal  weights. 

(18.)  Find  the  area  of  a  rectangle  35  ft.  3*  in.  by  23  ft.  6|  in. 
(19.)  Find  the  area  of  a  square  whose  side  is  17  ft.  4  in. 
(20.)  Find  the  volume  of  a  cube  whose  edge  is  3  ft.  9}  in. 
(21.)  Find  the  side  of  a  square  whose  area  is  139  sq.  ft.  130  sq.  in. 
(22.)  Expressed  in  a  certain  scale  of  notation,  79  (scale  of  10)  becomes  142  ; 
find  the  radix  of  that  scale. 

VOL.  I  N 


178  EXERCISES  XIII 


CHAP. 


(23.)  In  what  scale  of  notation  does  301  represent  a  square  integer  ? 

(24.)  A  number  of  3  digits  in  the  scale  of  7  lias  its  digits  reversed  when 
expressed  in  the  scale  of  9  ;  find  the  digits. 

(25.)  If  1  be  added  to  the  product  of  four  consecutive  integers  the  result 
is  always  a  square  integer  ;  and  in  four  cases  out  of  five  the  last  digit  (in  the 
common  scale)  is  1,  and  in  the  remaining  case  5. 

(26.)  Any  integer  of  four  digits  in  the  scale  of  10  is  divisible  by  7,  pro- 
vided its  first  and  last  digits  be  equal,  and  the  hundreds  digit  twice  the.  tens 
digit. 

(27. )  If  any  integer  be  expressed  in  the  scale  of  r,  the  difference  between 
the  sums  of  the  integers  in  the  odd  and  even  places  respectively  gives  the 
same  remainder  when  divided  by  r  +  1  as  does  the  integer  itself  when  so 
divided.     Deduce  a  test  of  multiplication  by  "casting  out  the  elevens." 

(28.)  The  difference  of  any  two  integers  which  are  expressed  in  the  scale 
of  10  by  the  same  digits  differently  arranged  is  always  divisible  by  9. 

(29.)  If  a  number  expressed  in  the  ordinary  scale  consist  of  an  even 
number  of  digits  so  arranged  that  those  equidistant  from  the  beginning  and 
end  are  equal,  it  is  divisible  by  11. 

(30.)  Two  integers  expressed  in  the  ordinary  scale  are  such  that  one  has 
zeros  in  all  the  odd  places,  the  other  zeros  in  all  the  even  places,  the  remaining 
digits  being  the  same  in  both,  but  not  necessarily  arranged  in  the  same  order. 
Show  that  the  sum  of  the  two  integers  is  divisible  by  11. 

(31.)  The  rule  for  identifying  leap  year  is  that  the  number  formed  by  the 
two  last  digits  of  the  year  must  be  divisible  by  4.  Show  that  this  is  a 
general  criterion  for  divisibility  by  4,  and  state  the  corresponding  criterion 
for  divisibility  by  2". 

(32.)  If  the  last  three  digits  of  an  integer  be^o^'o,  show  that  the  integer 
will  be  exactly  divisible  by  8,  provided  p$  +  2_£>i  +  4p-2  be  exactly  divisible  by  8. 

(33.)  Show  that  the  sum  of  all  the  numbers  which  can  be  formed  with  the 
digits  3,  4,  5  is  divisible  by  the  sum  of  these  digits,  and  generalise  the  theorem. 

(34.)  Itp/n  and  (n-j^/n,  p<n,  be  converted  into  circulating  decimals,  find 
the  relation  between  the  figures  in  their  periods. 

(35.)  If,  in  converting  the  proper  fraction  ajb  into  a  decimal,  a  remainder 
equal  to  b-a  occurs,  show  that  half  the  circulating  period  has  been  found, 
and  that  the  rest  of  it  will  be  found  by  subtracting  in  order  from  9  the  digits 
already  found.     Generalise  this  theorem. 

(36.)  In  the  scale  of  11  every  integer  which  is  a  perfect  5th  power  ends  in 
one  or  other  of  the  three  digits  0,  1,  t. 

(37.)  In  the  scale  cf  10  the  dilference  between  the  square  of  every  number 
of  two  digits  and  the  square  of  the  number  formed  by  reversing  the  digits,  is 
divisible  by  99. 

(38.)  A  number  of  six  digits  whose  1st  and  4th,  2nd  and  5th,  3rd  and  6th 
digits  are  respectively  the  same  is  divisible  by  7,  by  11,  and  by  13. 

(39.)  Show  that  the  units  digit  of  every  integral  cube  is  either  the  same 
as  that  of  the  cube  root  or  else  is  the  complementary  digit.  (By  the  comple- 
mentary digit  to  3  is  meant  10  -  3,  that  is,  7.) 

(40.)  If  in  the  scale  of  12  a  square  integer  (not  a  multiple  of  12)  ends 


ix  EXERCISES  XIII  179 

with  0,  the  preceding  digit  is  3,  and  the  cube  of  the  square  root  ends  with 
60. 

(41.)  If  a  be  such  that  am  +  a  —  r,  then  any  number  is  divisible  by  am, 
provided  the  first  m  integers  po,  pi,  ■  ■  ■  ,  pm-i  of  its  expression  in  the  scale  of 
r  are  such  that^0+2'i^+  •   •   •  +Pm-i^m~1  is  divisible  by  a"1. 

(42.)  The  digits  of  a  are  added,  the  digits  of  this  sum  added,  and  so  on, 
till  a  single  digit  is  arrived  at.  This  last  is  denoted  by  <p(u).  Show  that 
<p(a  +  b)  =  <f>  {</){a)  +  </>{b)} ;  and  that  the  values  of  <p(8n)  for  ft  =  1,  2,  .  .  .,  a, 
successively  consist  of  the  nine  digits  continually  repeated  in  descending 
order. 

(43.)  A  number  of  3  digits  is  doubled  by  reversing  its  digits  :  show  that 
the  same  holds  for  the  number  formed  by  the  first  and  last  digit,  and  that 
such  a  number  can  be  found  in  only  one  scale  out  of  three. 


CHAPTEK    X. 
Irrational  Functions. 

GENERALISATION    OF    THE    CONCEPTION    OF   AN    INDEX. 
INTERPRETATION    OF   z\  X^l,  X~m. 

§  1.]  The  definition  of  an  index  given  in  chap,  ii.,  §  1,  be- 
comes meaningless  if  the  index  be  other  than  a  positive  integer. 

In  accordance  with  the  generalising  spirit  of  algebra  we 
agree,  however,  that  the  use  of  indices  shall  not  be  restricted  to 
this  particular  case.  We  agree,  in  fact,  that  no  restriction  is  to 
be  put  upon  the  value  of  the  index,  and  lay  down  merely  that 
the  use  of  the  indices  shall  in  every  case  be  subject  to  the  laws 
already  derived  for  positive  integral  indices.  Less  than  this  we 
cannot  do,  since  these  laws  were  derived  from  the  fundamental 
laws  of  algebra  themselves,  to  which  every  algebraical  symbol 
must  be  subject. 

The  question  now  arises,  What  signification  shall  we  attri- 
bute to  xm  in  these  new  cases  ?  We  are  not  at  liberty  to  proceed 
arbitrarily,  and  give  any  meaning  we  please,  for  we  have  already 
by  implication  defined  xm,  inasmuch  as  it  has  been  made  subject 
to  the  general  laws  laid  down  for  indices. 

§  2  ]  Case  of  xp!?  where  p  and  q  are  any  positive  integers.     Let 
z  denote  the  value  of  xpto,  whatever  it  may  be  ;  then,  since  x^i  is 
to  be  subject  to  the  first  law  of  indices,  we  must  have — 
zV  =  zxzxzx  .   .  .  a  factors, 

=  xvli  x  xrti  x  xPlv  x  .  .  .   q  factors, 

-  3;P/?+P/?+.P/9+  •    •    •    1  terms, 
=  XP. 


chap,   x  INTERPRET ATION  OF  Xp,q  181 

Iii  other  words,  z  is  such  that  its  qt\\  power  is  x*}  that  is,  z 
is  what  is  called  a  qth  root  of  xP,  which  is  usually  denoted 
by  tfxP. 

Hence  x.p'9  =  *J&. 

In  particular,  if  p  -  1, 

We  have  now  to  consider  how  far  an  algebraical  value  of 
a  5th  root  of  every  algebraical  quantity  can  be  found. 

In  the  case  of  a  real  positive  quantity  k,  since  zi  passes  con- 
tinuously* through  all  positive  values  between  0  and  +  x>  as  z 
passes  through  all  positive  values  between  0  and  +  00  ,  it  is  clear 
that,  for  some  value  of  z  between  0  and  +  00  ,  we  must  have 
z?  -  k.     In  other  words,  there  exists  a  real  positive  value  of  %Jk. 

Unless  the  contrary  is  stated  we  shall,  when  k  is  positive, 
take  k1!i  as  standing  for  this  real  positive  value. 

The  student  should,  however,  remark  that  when  q  is  even, 
=  2r  say,  there  is  at  least  one  other  real  value  of  0/k ;  for,  since 
( -  z)2r  =  z2r,  if  we  have  found  a  positive  value  of  z  such  that 
z2r  =  k,  that  value  with  its  sign  changed  will  also  satisfy  the  re- 
quirements of  the  problem. 

Next  let  k  be  a  negative  quantity.  If  q  be  odd,  then,  since 
z?  passes  through  all  values  from  -  00  to  0  as  z  passes  through 
all  values  from  -  00  to  0,  there  must  be  some  one  real  negative 
value  of  z,  such  that  &  =  k.  In  other  words,  if  q  be  odd,  there 
is  a  real  negative  value  of  {/k. 

If  q  be  even,  then,  since  every  even  power  of  a  real  quantity 
(no  matter  Avhether  +  or  - )  is  positive,  there  is  no  real  value 
of  z.  Hence,  if  k  be  negative  and  q  even,  %/k  is  imaginary.  This 
case  must  be  left  for  future  discussion. 

It  will  be  useful,  however,  for  the  student  to  know  that 
ultimately  it  will  be  proved  that  */k  has  in  every  case  q  different 
values,  expressions  for  which,  in  the  form  of  complex  numbers, 
can  be  found.  Of  these  values  one,  or  at  most  two,  may  be  real, 
as  indicated  above  (see  chap,  xii.) 

*  For  a  fuller  discussion  of  the  point  here  involved  see  chaps,  xv.  and  xxv. 


182  VERIFICATION  OF  THE  LAWS  FOR  Xrlq  chap. 

Only  iii  the  case  where  h  is  the  pth  power  of  a  rational 
quantity  can   %/k  be  rational. 

Example. 

ltk=+h&>, 

2£>/k  has  two  real  values,  +h  and  -h. 

If  k=+h*P+\ 

ipt}/k  lias  one  real  value,  +h. 

HJc=  -J&+1, 

-v+Vk  has  one  real  value,  -  h. 

In  all  that  follows  in  this  chapter,  we  shall  restrict  the  radicand, 
I;  to  be  positive  ;  we  shall  regard  only  the  real  positive  value  of  the  qth 
root  of  k ;  and  this  (ivhich  is  called  the  PRINCIPAL  value  of  the 
root)  is  what  ice  understand  to  be  the  meaning  of  £1/? 

The  theory  of  fractional  indices  could  (as  in  the  first  edition  of  this  volume) 
he  extended  so  as  to  cover  the  case  of  a  negative  radicand,  hut  only  so  far  as  the 
order  of  the  root  is  odd.  The  practical  advantage  gained  by  this  extension  is 
not  worth  the  trouble  which  it  causes  by  complicating  the  demonstrations. 
We  think  it  better  also,  from  a  scientific  and  educational,  as  well  as  from  a 
practical  point  of  view,  to  consider  the  radication  of  negative  radicands  as  a 
particular  case  of  the  radication  of  complex  radicands  (see  chap,  xii.,  §  19). 

§  3.]  We  have  now  to  show  that  the  meaning  just  suggested 
for  xplq  is  consistent  with  all  the  Laws  of  Indices  laid  down  in 
chap.  ii.  The  simplest  way  of  doing  this  is  to  re-prove  these 
laws  for  the  newly  denned  symbol  x^i. 

We  remark  in  the  first  place  that  it  is  necessary  to  prove 
only  I.  (a),  II,  and  III.  (a)  ;  because,  as  has  been  shown  in  chap. 
ii.,  I.  (/8)  can  be  deduced  from  I.  (a),  and  III.  (J3)  from  III.  (a), 
without  any  appeal  to  the  definition  of  xm. 

To  prove  I.  (a),  consider  xpl?  and  xr/s,  where  p,  q,  r,  s  are 
positive  integers,  and  let 

z  =  xPb  xr's. 

Then,  since  x?1*  and  xr's  are,  by  hypothesis,  each  real  and 
positive,  z  is  also  real  and  positive.     Also 

z<i»  =  (xPlq  xrl*)is, 


X  VERIFICATION  OF  THE  LAWS  FOR  Xp,q  183 

all  by  the  laws  for  positive   integral  indices,   regarding   which 
there  is  no  question. 

Now,  by  the  meanings  assigned  to  aP^  and  xrls,  we  have 
(a^/«)9  =  %*  and  (xrls)a  =  xr.     Hence 

=  xPsxP, 
=  K*"+«r) 

hy  the  laws  for  positive  integral  indices. 

It  now  follows  that  0  is  the  qsth  root  of  a^JS+?'' ;  and,  since  z 
is  real  and  positive,  it  must  be  that  qsth  root  which  we  denote 
by  ofp*+9r)lv.     Therefore 

z  =  z(2«+ <?'•)/</■', 

that  is  to  say, 

z  =  ?pl<i+rls. 

The  proof  is  easily  extended  to  any  number  of  factors. 

To  prove  Law  II.,  consider  (x^)r's,  where  p,  q,  r,  s  are  posi- 
tive integers, 

and  let  z  =  (x^)r's. 

Then,  since,  by  hypothesis,  x*ti  is  real  and  positive,   therefore 
(xPtey1*,  that  is  z,  is  real  and  positive.     Also 
zv  =  [(xPlqyisy^ 

=  [{(ajP/s)*"/*}8]?, 

by  laws  for  positive  integral  indices ; 
=  [(xPte)r]i, 

by  definition  of  a  fractional  index ; 
=  (xvl*)9r, 

by  laws  of  positive  integral  indices  ; 

by  definition  of  a  fractional  index ; 
=  xv, 

by  laws  of  positive  integral  indices. 
Hence  z  is  a  qsth.  root  of  »*"",  and,  since  z  is  real  and  positive,  we 
must  have 

Z  =  o-Vrlqs, 

that  is,  z  =  a^/9)(r/»). 


184  PARADOXES  chap. 

Lastly,  to  prove  Law  III.  (a),  let 

Then,   since,   by  hypothesis,   x^i  and   yvli   are   each    real    and 
positive,  z  is  real  and  positive.     Also 

zq  =  (xplq  yplqy^ 

by  laws  for  positive  integral  indices  ; 
=  xPf, 

by  definition  for  a  fractional  index ; 

by  laws  for  positive  integral  indices. 

Hence  z  is  a  qi\\  root  of  (%y)p ;  and,  since  z  is  real  and  positive, 

we  must  have 

a  =  (.vy)pli. 

The  proof  is  obviously  applicable  where  there  is  any  number  of 
factors,  x,  y,   .  .   . 

§  4.]  Although  it  is  not  logically  necessary  to  give  separate 
proofs  of  Laws  I.  (/3)  and  III.  (/?),  the  reader  should  as  an 
exercise  construct  independent  proofs  of  these  laws  for  himself. 

It  should  be  noticed  that  in  last  paragraph  we  have  supposed 
both  the  indices  pjq  and  r/s  to  be  fractions.  The  case  where 
either  is  an  integer  is  met  by  supposing  either  q  —  1  or  s  =  1 ;  the 
only  effect  on  the  above  demonstrations  is  to  simplify  some  of 
the  steps. 

§  5.]  Before  passing  on  to  another  case  it  may  be  well  to 
call  attention  to  paradoxes  that  arise  if  the  strict  limitation  as  to 
sign  of  xPfo  be  departed  from. 

By  the  interpretation  of  a  fractional  index 

x*l2  =  Z/x*  =  ±  x\ 

But  x^  =  x\ 

which  is  right  if  we  take  x-4/2  to  stand  for  the  positive  value  of 
A2/V  ;  but  leads  to  the  paradox  x*  =  -  x~  if  we  admit  the  negative 
value. 

A  similar  difficulty  would  arise  in  the  application  of  the  law, 
(xm)n  =  xmn  =  (.'■")"' ; 


x  INTERPRETATION  OF  X°  185 

for  example,  (4*)9  =  (4*)' 

would  lead  to  (  ±  2f  =  ±  4, 

that  is,  4  =  ±  4, 

if  both  values  were  admitted.  Such  difficulties  are  always  apt 
to  arise  'with  x^i  where  the  fraction  pfq  is  not  at  its  lowest  terms. 
The  true  way  out  of  all  such  difficulties  is  to  define  and 
discuss  x11  as  a  continuously  varying  function  of  n,  which  is  called 
the  exponential  function.  In  the  meantime  fractional  indices  are 
introduced  merely  as  a  convenient  notation  in  dealing  with 
quantities  which  are  (either  in  form  or  in  essence)  irrational ; 
and  for  such  purposes  the  limited  view  we  have  given  will  be 
sufficient. 

§  6.]  Case  of  x°.  This  case  arises  naturally  as  the  extreme 
case  of  Law  I.  (/3),  when  n  =  m;  for,  if  we  are  to  maintain  that 
law  intact,  we  must  have,  provided  x  4=  0,* 

that  is,  X°  =  1. 

This  interpretation  is  clearly  consistent  with  Law  I.  (a),  for 

xm  n°  =  xm+° 
simply  means 

xm  x  1  =  xm, 

which  is  true,  whatever  the  interpretation  of  xm  may  be. 

Again,  a;'"0  =  (x,rt)°, 
that  is  x°  =  (xm)°, 

simply  means  1  =  1  by  our  interpretation  ; 

and  xm0  =  (x0)m, 
or  x°  =  (x°)m, 

gives  1  =  1™ 

which  is  right,  even  if  m  be  a  positive  fraction,  provided  we 
adopt  the  properly  restricted  interpretation  of  a  fractional  index 
given  above.  The  interpretation  is  therefore  consistent  with  II. 
The  interpretation  a;0  =  1  is  also  consistent  with  III.  (a),  for 

a?>f  =  (xyf 
simply  means  1x1  =  1, 


*  This  provision  is  important  since  the  form  0°  is  indeterminate  (see  chap, 
xxv.) 


186  NEGATIVE  INDICES  chap. 

§  7.]  Case  of  x~m,  where  m  is  any  real  positive  (or  signless) 
number,  and  x  4=  0. 

Let  z  =  x~m,  then,  since  xm^0,  Ave  have 
z  =  x~m  x  Zm-7-Xm, 

if  Law  I.  (u)  is  to  hold  for  negative  indices.     Whence 

,0  /-•>»>' 


z  =  ar/x 


/a*"» 


by  last  paragraph.      In  other  words,  x~m  is  the  reciprocal  of  xm. 

As  an  example  of  the  reconciliation  of  this  with  the  other 
laws,  let  us  prove  I.  (a),  say  that 


By 

our 

definition, 

X 

we 

~mx 

have 

-n  =  (\fo:m)(ljxn), 
=  l/xmxn, 

s=  l/xm+n, 

the    last  step  by 

the    laws 

already 

established  for  all  positive 

indices ; 

by  definition  of  a 

negative  index. 

Hei 

ice 

X' 

■mx 

-n  _  r*  -  vi  -  n 

In  like  manner  we  could  show  that 

rwm  v  -  n  _  g.m  -  n 

The  verification  of  the  other  laws  may  be  left  as  an  exercise. 

§  8.]  The  student  should  render  himself  familiar  with  the 
expression  of  the  results  of  the  laws  of  indices  in  the  equivalent 
forms  with  radicals  ;  and  should  also,  as  an  exercise,  work  out 
demonstrations  of  these  results  without  using  fractional  indices 
at  all. 

For  example,  he  should  prove  directly  that 

Vx*/z=P!/xP+*  (1); 

V{  VxPY  =  VxPr  =  Vi  V&Y         (2)  i 

yx&yyz=y(xyz)  (3); 

yxmj  yym  =    "/(^jy)™  (4). 


EXAMPLES  187 


EXAMPLES    OF   OPERATION    WITH    IRRATIONAL    FORMS. 

§  9.]  Beyond  the  interpretations  xpl^,  x°,  z~m,  the  student  has 
nothing  new  to  learn,  so  far  as  mere  manipulation  is  concerned, 
regarding  fractional  indices  and  irrational  expressions  in  general. 
Still  some  practice  will  he  found  necessary  to  acquire  the  requisite 
facility.  "We  therefore  work  out  a  few  examples  of  the  more 
commonly  occurring  transformations.  In  some  cases  we  quote 
at  each  step  the  laws  of  algebra  which  are  appealed  to ;  in  others 
we  leave  it  as  an  exercise  for  the  student  to  supply  the  omission 
of  such  references. 

Example  1. 

To  express  A  v  B  in  the  form  V  P. 

A  v/B  =  AB1/™  =  (Am),/"'B1/m,  by  law  of  indices  II., 
=  (A"'B)1;»',  by  law  of  indices  III.  (a), 
=  X/(A"'B). 
Example  2. 

'v/a=7a- 

for  v^A  =  A1/m  =  AP/mP, 

=  mVAP. 
Example  3. 

sJxPm+<l  =  x(Pm+tf''m 
=  xp+q!mi 

=  xPx  xn'm,  by  law  of  indices  I.  (a), 

m  / 

Example  4. 

To  express  \/x»\  y/y  as  the  root  of  a  rational  function  of  x  and  y. 

s/xp\  \/yr  =  xP!v/yr!»  =  xP^v/yW'Q', 
=  {xP'^lvftyvryiV, 

=  {xP'/yiry/q^ 

=  V{xP'lyr)- 
Example  5. 

V32=V(16x2), 
=  Vl6xV2, 

=  4x  V2. 


188 

EXAMPLES 

Example  6. 

2  x  V2  x  v"2  x  \A 

=  2x2"x2}x2', 

=  22, 
=  4. 

CHAP 


Example  7. 

=  («2)'"/2»(l-a-2/a2)m/2») 

=  amln(l-x2/a2)m'2n. 
Example  8. 

\/{yx  +  x")  x  ^(yz  +  ex) 

=  V  Hy  +  *)}  x  V  {2(2/  +  a-)} , 

=  V-Z  X  V(y  +  *)  X  \/z  X  \/(2/  +^); 

=  V(^)x{V(2/  +  ^)}2, 

=(y+«)x  V(a*)- 

Example  9. 

V240  +  V40 

=  V(16x3x5)  +  V(4x2x5), 
=  V16V3V5+ VW2V5, 
=  V5(4V3  +  2V2). 
Example  10. 

(V3  +  2V2  +  3V6)(V3-2N/2  +  3V6) 

=  (V3  +  3V6)2-(2V2)2, 
=  (V3)2  +  6V3V6  +  (3V6)2-(2V2)2. 
=  3  +  6V(3x6)  +  32x6-22x2, 
=  49  +  6\/18, 
=  49  +  18V2. 
Example  11. 

{V(l-a-)  +  V(l+.T)}4 

=  {(l-x)i  +  (l+x)i}*, 
=  (l-xf  +  {l+x)n- 

+  i(l-x)*(l+x)i+4(l-x)i(l+x)i 
+  6(l-x)(l+x), 

=  8  -  4x2  +  4(1  -x)h(l  +  x)\l  - x+l+x) 

=  8-4.t2+8V(l-tf2). 
Example  12. 

V    \x-y)      V   \x+y) 

_W(x  +  y)\2+{s/(x-y)}2 
\/{{x-y)(x  +  y)} 


RATIONALISING  FACTORS  189 

_x+y+x~y 
2a; 


Example  13. 


V(*2~2/2)' 


(a^-a^+a:   *- a;-*)  x  (;*:*+ 1+a:   *) 
=x*-7? +a:*-aT* 

+  ar  -  a;1  +  x    *  -  x    * 

Tit     "tC  V  X  «C  y 


5  1  _  1  _  5 

sx'+aT-a;      -a;    * 


Example  14. 
Show  that 


We  have 

g2  =  a+s/W-b)  +  a-yW-5)  +  2       /f  {a  +  V(a2  -  6)}  (a -  V(a2  -  5)}  ~| 

=  a  +  V[«2-{V(«2 -&)}'-'], 
=  re  +  \/6. 

Hence,  extracting  the  square  root,  we  have 

S=V(a+V&)- 


RATIONALISING    FACTORS. 

§  10.]  Given  certain  irrationals,  say  Jp,  *Jq,  y/r,  we  may 
consider  rational,  and  it  may  be  also  integral,  functions  of  these. 
For  example,  I  *Jp  +  m  \/q  +  n  yV,  and  /(  *Jp)s  +  m  \/{pq)  +  n{  s/qfy 
are  integral  functions  of  Jp,  *Jq,  Jr,  of  the  1st  and  2nd 
degrees  respectively,  provided  /,  m,  n  do  not  contain  Jp,  Jq,  Jr. 
Again,  (I  Jp  +  m  Jq)/(l  \/g  +  m  Jr)  is  a  rational,  but  not  integral, 
function  of  these  irrationals.  J  (I  \Jp  +  in  \/q),  on  the  other 
hand,  is  an  irrational  function  of  Jp  and  Jq. 

The  same  ideas  may  also  be  applied  to  higher  irrationals, 
such  us  pllm,  qlln,  &c. 

§  11.]  Confining  onrselves  for  the  present  to  quadratic 
irrationals,  we  shall  show  that  every  rational  function  of  a 
given    set    of   quadratic    irrationals,  Jp,  Jq,  ^/r,    &c,    can    be 


190  RATIONALISING  FACTORS  chap. 

reduced  to  a  linear  integral  function  of  the  square  roots  of  p,  q,  r, 
and  of  their  products,  pq,  pr,  gr,  pgr,  &c. 

This  reduction  is  effected  mainly  by  means  of  rationalising 
factors,  whose  nature  and  use  we  proceed  to  explain. 

If  P  be  any  integral  function  of  certain  given  irrationals,  and  Q 
another  integral  function  of  the  same,  such  that  the  product  QP  is 
rational  so  far  as  the  given  irrationals  are  concerned,  then  Q  is  called 
a  rationalising  factor  ofP  with  respect  to  the  given  irrationals. 

It  is,  of  course,  obvious  that,  if  one  rationalising  factor,  Q, 
has  been  obtained,  we  may  obtain  as  many  others  as  we  please 
by  multiplying  Q  by  any  rational  factor. 

§  12.]  Case  of  Monomials. 

1°.  Suppose  we  have  only  quadratic  irrational  forms  to  deal 
with,  say  two  such,  namely,  pi  and  qK 

Then  the  most  general  monomial  integral  function  of  these 
is 

i  =  A(pi)2m+\r)2n+\ 

where  A  is  rational.  There  is  no  need  to  consider  even  indices, 
since  (jpi)Zm=pm  is  rational. 

Now  I  reduces  to 

I  =  (Ap'YOiM 
where  the  part  within  brackets  is  rational. 

Hence  a  rationalising  factor  is  jj'-qK  for  we  have 

Ipigi  =  (Aj>mqn)pq, 

which  is  rational. 

Example.  A  rationalising  factor  of  16  .  2? .  3* .  5*  is  2*3-5',  that  is,  (30)  . 

2°.   Suppose  we  have  the  irrationals  pv*,  ql!t,  r^u,  say,  and 

consider 

I  =  ApVs  qm^  ?'"/"  * 

which  is  the  most  general  monomial  integral  function  of  these. 
A  rationalising  factor  clearly  is 

„  .1  -  l/s  f,\  -  in  It  rl  -  n/u 

p       q        '        i 
or  4*  -  0 >  (ft  -  "0. 't  >•(«  -  »)/« 


*  Where  of  course  l<s,  m<t,  «<«,  for  if  they  were  not  they  could  be 
reduced  by  a  preliminary  process  like  that  in  case  1°. 


x  RATIONALISING  FACTORS  191 

Example. 

1=81. 8*. 6*. 7*, 
=31.31+*.5*.7i+i, 
=(31.3.74).3*.5f.7*. 

5         2         1 

A  rationalising  factor  is  3  .  5  .  7  . 

§  13.]  Case  of  Binomials. 

1°.  The  most  general  form  when  only  quadratic  irrationals 
are  concerned  is  a  \/p  +  b  \/q,  where  a  and  b  are  rational ;  for,  if 
we  suppose  p  a  complete  square,  this  reduces  to  the  more  special 
form  A  +  B  \Aj,  where  A  and  B  are  rational. 

A  rationalising  factor  clearly  is  a  s/p  -  b  \/q.     For,  if 

I  =  a  */p  +  b  x/q, 

I(a  \  >  -  b  y/q)  =  (a  ^p)2  -  (b  s/q)\ 

=  ap  -  b'q, 
which  is  rational 

The  two  forms  a  \/p  +  b  \/q  and  a  \/p  -  b  *Jq  are  said  to  be  con- 
jugate to  each  other  with  reference  to  y/q,  and  we  see  that  any  binomial 
integral  function  of  quadratic  irrationals  is  rationalised  by  multiplying 
it  by  its  conjugate. 

2°.  Let  us  consider  the  forms  ap*l*  ±  bqW,  to  which  binomial 
integral  functions  of  given  irrationals  can  always  be  reduced.*    Let 

x  =  apaly,     y  =  bqffl, 
I  =  ap*b  -  hfr\ 
=  «  -  y- 

Let  m  be  the  L.C.M.  of  the  two  integers,  y,  8.  Now,  using 
the  formula  established  in  chap,  iv.,  §  16,  we  have 

(zm-1  +  xm  ~2y+.   .  .  +  xym  ~ 2  +  ym "1VI  =  xm  -  ym. 

Here  xm  -  y>"  =  (a'"  pmx^  -  b"<  tf&P),  where  ma/y  and  m/3/8  are 
integers,  since  m  is  divisible  by  both  y  and  S,  that  is,  x™  -  y'"  is 
rational. 

A    rationalising    factor    is    therefore    x1"  ~ 1  +  xm  ~  -y  +   .  .   . 
+  xym~2  +  ym~l,  in  which  x  is  to  be  replaced  by  ap ,  and  y  by  b<f' 

*  Tartaglia's  problem.    See  Cossali  Storia  dell'  Abjebra  (1797),  vol.  ii.  p.  266. 


192  RATIONALISING  FACTORS  chap. 

The  form   ap"ly  +  bqm   may  be   treated  in   like  manner  by 
means  of  formulas  (4)  or  (5)  of  chap,  iv.,  §  16. 

Example. 

1  =  3.2*-  4.3*. 

Here  m  =  6,     z=3.2*,     27  =  4.3*; 

and  a  rationalising  factor  is 

a5  +  xHj  +  x*if-  +  xhf  +  xyi  +  rf 

=  35.2S  +  3l.4.2l.3*  +  33.42.2.3*  +  32.43.2§.3*  +  3.44.2*.3§  +  4s.3i, 
=  35.2.23  +  34.8.2*.3*  +  33.32.3*  +  32.43.2S.3*  +  3.44.2*.3§  +  45.3f. 

§    14.]   Trinomials  with  Quadratic  Irrationals.      This  case    is 
somewhat  more  complicated.      Let 

I  =   \/p  +  \/q+   Jr  ;  * 
and  let  us  first  attempt  to  get  rid  of  the  irrational  Jr.     This 
Ave  can  do  by  multiplying  by  the  conjugate  of  \/p  +   sfq  +  s/r 
with  respect  to  *Jr,  namely,  sip  +  \'q  -  sir.     We  then  have 

(  Jp  +  Vg  -  v/r)I  =  (  Jp  +  JqY  -  ( vV)2, 

=  p  +  q-r+2j(pq)  (1). 

To  get  rid  of  nj(pq)  we  must  multiply  by  the  conjugate  of 
p  +  q-r  +  2  s/(p<j)  with  respect  to  \/(pq).     Thus  finally 
{^  +  2-r-2N  \pq)}{  s/p  +    Jq  ~  Jr)l  =  (p  +  q  -  r)2  -  {2  v/(  pq)}\ 

=f  +  ?2  +  r2  -  2j?2  -  2p-  -  2jr. 

Hence  a  rationalising  factor  of  I  is 

{p  +  q-r-  2  \/(j>g)}(  «/p  +    slq  -  Jr), 
or 
(Jp  -  Jq  +   */r)(vi>  -   s'q-   Jr)(Jp  +  v'2  -  v'r)       (2). 

Ey  considering  attentively  the  factor  (2)  the  student  will  see 
that  its  constituent  factors  arc  obtained  by  taking  every  possible 
arrangement  of  the  signs  +  and  -  in 

+   *Jp  ±    \fq±   \  V, 

except  the  arrangement  +  +  +  ,  which  occurs  in  the  given  trinomial. 

*  This  is  really  the  most  general  form,   for  a\/])  +  b\Jq  +  c\/r  may  be 
written  V(^)  +  V(&82)  +  vW- 


x  REDUCTION  TO  LINEAR  FORM  193 

Example  1.   A  rationalising  factor  of 

\/2  -  V3  +  V5 
is  (V2  -  \ft  -  V»)  (V2  +  V3  +  V5)  ( v'2  +  \/3-  yf5). 

Example  2.   A  rationalising  factor  of 

1+2V3-3V2 
is  (1  +  2V3+3V2)(1-2V3  +  3V2)(1-2V3-3V2). 

In  actual  practice  it  is  often  more  convenient  to  work  out 
the  rationalisation  by  successive  steps,  instead  of  using  at  once 
the  factor  as  given  by  the  rule.  But  the  rule  is  important, 
because  it  is  general,  and  will  furnish  a  rationalising  factor  for  a 
sum  of  any  number  of  quadratic  irrationals. 

Example  3.   A  rationalising  factor  of 

1  +  V2-V3  +  V4 

is  (1  +  V2-  V3-  \/4)(l+V2+V3  +  V4)(l+  V2  +  V3-  V*) 

x  (1  -  V2  -  \/3  +  \/4)  (1  -  V2  -  V3  -  V4)  (1  -  V2+  V3  +  V4) 
x  (1  -  sJ2  +  V3  -  V4). 

Before  giving  a  formal  proof  of  the  general  truth  of  this 
rule,  it  will  be  convenient  to  enunciate  one  or  two  general  pro- 
positions which  are  of  considerable  importance,  both  for  future 
application  and  for  making  clear  the  general  character  of  the 
operations  which  we  are  now  discussing. 

§    15.]  Ever)/    integral  function    of   a    series  of   square    roots, 

\/p,  -Jq,  \/r,  &c,  can  be  expressed  as  the  sum  of  a  rational  term 

and  rational  multiples  of  \tp,  \/q,  \/r,  &c,  and  of  their  products 

*J(P<l),  J(pr)>  v^Fi'').  &i* 

First,  let  there  be  only  one  square  root,  say  \/p,  and  consider 

any  rational  integral  function  of  \jp,  say  <£(  \''p).     Every  term 

of  even  degree  in  *Jp  will  be  rational,  and  every  term  of  odd 

degree,  such  as  A(  v//>)2w+1  may  be  reduced  to  (Kpm)  \/p,  that 

is,  will  be  a  rational  multiple  of  s/p.     Hence,  collecting  all  the 

even  terms  together,  and  all  the  odd  terms  together,  we  have 

</>(^)  =  P  +  Qv>  (l), 

where  P  and  Q  are  rational. 

*  Such  a  sum  is  called  a  "  Linear  Form." 
VOL.  I  0 


194  RATIONALISATION  OF  ANY  INTEGRAL  FUNCTION  chap. 

Next,  suppose  the  function  to  contain  two  square  roots,  say 
4>(  JPi  *Jq)'  First  of  all,  proceeding  as  before,  and  attending 
to  Jp  alone,  we  get 

«/>(  <Sp,   \/(L)  =  P  +  Qv/P, 

where  P  and  Q  are  rational  so  far  as  p  is  concerned,  but  are 

irrational  as  regards  q,  being  each  rational  integral  functions  of 

\/q.     Reducing  now  each  of  these  with  reference  to  Jq  we  shall 

obtain,  as  in  (1), 

P  =  F  +  QV2,     Q  =  P"  +  Q"vA;, 
and,  finally, 

<K  Jp,   Jq)  =  F  +  QVg  +  (P"  +  Q"  Jq)  y/p, 

=  F  +  P"  s/p  +  Q'  Jq  +  Q"  J(pq)        (2), 
which  proves  the  proposition  for  two  irrationals. 

If  there  be  three,  we  have  now  to  treat  P',  P",  Q',  Q"  by  means 
of  (1),  and  we  shall  evidently  thereby  arrive  at  the  form 
A+B  Jp  +  C  Jq+T>  vV+E^r)  +F  J(rp)+G  J(pq)  +  li  y/{pgr), 
and  so  on. 

Cor.  It  follows  at  once  from  the  process  by  which  we  arrived 
at  (1)  that 

4>(-     Jp)  =  P  -  Q    yip. 

Hence  if  <f>(  Jp)  he  any  integral  function  of  sip,  <£(  -  Jp)  is  a 
rationalising  factor  of  <£(  \/p) ;  and,  more  generally,  if  <f>(  sjp,  Jq, 
s/r,  .  .  .)  be  an  integral  function  of  \/p,  Jq,  Jr,  .  .  .,  then,  if  we 
take  any  one  of  them,  say  Jq,  and  change  its  sign,  the  product 
</>(  Jp>  Jq>  Jr>  •  •  •)  x  <K  J  Pi  ~  J°>  Jr>  •  •  •)  ?s  rational,  so  far 
as  Jq  is  concerned. 

Example    1.    If  <p(.r)=:x3  +  .r2  +  x+l,  find   the   values   of  0(l  +  \/3)   and 
0(1  -  V3)  and  0(1  +  \J3)  x  0(1  -  \JZ). 

0(1  +  V3)  =  (l  +  V3)3  +  (l  +  V3)2+  (1  +  V3)+  1, 
=  l  +  3\/3  +  3.3  +  3\/3 

+1+2V3+3 

+  1  +  V3 
+  1, 
=  16  +  9V3 

0(1  -  \/3)  is  deduced  by  writing  -  \JZ  in  place  of  +  \/3  everywhere  in  the 
above  calculation.     Hence 

0(1-V3)  =  16-9V3; 

0(1  +  V3)  x  0(1  -  V3)  =  (16)2  -  (9  V3)2, 
=  256-243, 
=  13. 


X  LINEAR  FUNCTION  OF  SQUARE  ROOTS  RATIONALISED       195 

Example   2.     Find    the    value   of    a?+yi-\-7?  —  xyzi    when    x=sjq-  \/r, 
y=sjr-  \/P>  z  =  s/p ~  \'<1- 

Since  x  +  y  +  z=\/q-  \Jr+\Jr-  \/p+s/p-\/q 

=  0, 
we  have  (chap.  iv. ,  §  25,  IX.) 

Sb*  -  3xyz  =  2a(Za:2  -  2xy), 
=  0. 
Therefore  Zx3  -  xyz = 2xyz, 

= 2(  V?  -  \Jr)  ( V  ~  Vi>)  ( Vl>  -  VsOi 
=  2(2  -  r)s/p  +  2(r  -^)  >/?  +  %(p  -  ?)Vr- 

Example  3.    Evaluate  (l+y+is)(l+2+a:)(l+as+y)  when  a:=  V2>  2/  =  V3> 
z=V5- 

(l+y+8)(l  +  «+a;)(l+a!+y) 

=  1  +  2(se  +  y  +  2)  +  x2  +  (y  +  z)x  +  yz  +  &c.  +  &c. 
+  x{y-  +  z2)  +  &c.  +  &c.  +  2xyz, 
=  1  +  x-  +  y2  +  z2  +  (2  +  y2  +  z2)x  +  (2  +  z2  +  x2)y 

+  (2  +  a;2  +  y2)z  +  %yz  +  3zx  +  Bxy  +  2xyz, 
=  11  + 10  V2  +  9  V3  +  7  V5  +  3V!5  +  3\/10  +  3V6  +  2V30. 

§  16.]  We  can  now  prove  very  easily  the  general  proposition 
indicated  above  in  §  14. 

If  P  be  the  sum  of  any  number  of  square  roots,  say  s/p,  \/q, 
sfr,  .  .  .,  a  rationalising  factor  Q  is  obtained  for  P  by  multiplying 
together  all  the  different  factors  that  can  be  obtained  from  P  as 
follows : — Keep  the  sign  of  the  first  term  unchanged,  and  tale  every 
possible  arrangement  of  sign  for  the  following  terms,  except  that  which 
occurs  in  P  itself. 

For  the  factors  in  the  product  Q  x  P  contain  every  possible 

arrangement  of  the  signs  of  all  but  the  first  term.      Hence  along 

with  the  +  sign  before  any  term,  say  that  containing  sjq,  there 

will  occur  every  possible  variety  of  arrangement  of  all  the  other 

variable  signs  ;  and  the  same  is  true  for  the  -  sign  before  \/q. 

Hence,  if  we  denote  the  product  of  all  the  factors  containing 

+   s!q  by  4>(  \/q),  the  product  of  all  those  factors  that  contain 

-  s/q  will  differ  from  <£(  \fa)  only  in  having  -  \/q  in  place  of 

+  s/q,  that  is,  may  be  denoted  by  <£(  -  s/q).     Hence  we  may 

write  Q  x  P  =  </)(  s/q)  x  <£(  -  s/q),  which,  by  §  15,  Cor.  1,  is  rational 

so  far  as  v^  is  concerned.     The  like  may  of  course  be  proved  for 

every  one  of  the  irrationals  \/q,  \fr,  .  .  .     Also,  for  every  factor 

in  Q  x  P  of  the  form  sip  +  k  there  is  evidently  another  of  the  form 


196  RATIONAL  FUNCTION   REDUCED  TO  LINEAR  FORM        chap. 

sip  -k;  so  that  Q  x  P  is  rational  as  regards  Jp.     Hence  Q  x  P 
is  entirely  rational,  as  was  to  be  shown. 

§  17.]  Every  rational  function,  whether  integral  or  not,  of  any 
number  of  square  roots,  s/p,  sjq,  s/r,  . . .,  can  be  expressed  as  the  sum 
of  a  rational  part  and  rational  midtiples  of  \/p>,  *Jq,  Jr,  &c,  and  of 
their  products  \/(pq),  y/(pr),  \/(qr),  J(pqr),  dr.* 

For  every  rational  function  is  the  quotient  of  two  rational 
integral  functions,  say  E/P.  Let  Q  be  a  rationalising  factor  of 
P  (which  we  have  seen  how  to  find),  then 

R     RQ 

P=PQ' 

But  PQ  is  now  rational,  and  RQ  is  a  rational  integral  function  of 
sip,  sjq,  \/r,  .  .  .,  and  can  therefore  be  expressed  in  the  required 
form.     Hence  the  proposition  is  established* 

Example  1.  To  express  1/(1  +  \J2  +  \J3)  as  a  sum  of  rational  multiples  of 
square  roots.     Rationalising  the  denominator  we  obtain  by  successive  steps, 

1  1  +  V2j!_\/3 

1  +  V2  +  V3     (1  +  \/2)2  -  (V3)2' 

_i+V2-ya 

2V2 

_V2(l  +  y2-V3) 

2x2 
=  4l(V2  +  2-V6), 

Example  2.  Evaluate  {x2  -x+1  )/(«2  +  x  + 1 ),  where  x  =  y3  +  \/5. 
x--x  +  l  _  9  +  2V15- V3- V5 
x2  +  x  + 1  ~  9  +  2  V15  +  \J3  +  v'5' 

_  (9  +  2Vl5)2-2(9  +  2V15)(V3  +  V5)  +  (V3  +  V5)2 
(9  +  2Vl5)2-(V3  +  V5)a 
149  -  38  V3  -  30\/5  +  38  y/15 

133  +  34V15 
(149-38V3-30V5  +  88yi5)(133-34yi5) 
1332-34-xl5  ' 

_  +  437  +  46y3  -  114y5  -  12yi5 
849 

*  Besides  its  theoretical  interest,  the  process  of  reducing  a  rational  func- 
tion of  quadratic  irrationals  to  a  linear  function  of  such  irrationals  is  important 
from  an  arithmetical  point  of  view  ;  inasmuch  as  the  linear  function  is  in 
general  the  most  convenient  form  for  calculation.  Thus,  if  it  be  required  to 
calculate  the  value  of  l/(l  +  y2  +  y3)  to  six  places  of  decimals,  it  will  be 
found  more  convenient  to  deal  with  the  equivalent  form  ^  +  jy2  -  \\J6. 


THEORY  FOR  IRRATIONALS  OF  ANY  ORDER  197 


GENERALISATION    OF   THE   FOREGOING   THEORY. 

§  18.]  It  may  be  of  use  to  the  student  who  has  already 
made  some  progress  in  algebra  to  sketch  here  a  generalisation  of 
the  theory  of  §§  13-17.  It  is  contained  in  the  following  pro- 
positions :  — 

I.  Every  integral  function  of  p1/n  can  he  reduced  to  the  form 
X0  +  A1pl!n  +  A2p2l'l+  .  .  .  +  An.lp^-^n,  where  Au,  A,,  .  .  ., 
An_,  are  rational,  so  far  as  j)^,n  is  concerned. 

After  what  has  been  done  this  is  obvious. 

II.  Every  integral  function  of  p111,  q1,m,  rlln,  &c,  can  he  ex- 
pressed as  a  linear  function  of  p1'1,  p2/l, .  .  .,  jfl-W  •  q1*'1",  q-/m, .  .  ., 
£m-i)lm;  yl/w    ,.2/n  _  _  ^  ,<n-i)/w  ;  £c^  ami  0f  tjie  products  of  these 

quantities,  two,  three,  &c,  at  a  time,  namely,  p111  q1/m,  p2'1  qllm,  &c, 
the  coefficients  of  the  linear  function  heing  rational,  so  far  as  p111,  qllm, 
rl!n,  &c,  are  concerned. 

Proved  (as  in  §  15  above)  by  successive  applications  of  I. 

III.  A    rationalising  factor    of   A0  +  A,^1/rt  +  A.2p2ln  +  .   .   . 
+  An_  jj/'i-i)/"  am  always  be  found. 

We  shall  prove  this  for  the  case  n  =  3,  but  it  will  be  seen 
that  the  process  is  general. 

Let  P  =  A0  +  A^  +  A2p%  ( 1 ), 

then  p$P  =pA2  +  A0p^  +  A^  (2), 

and  p%P  =joAi  +  pA.2p*  +  A0p?s  (3). 

Let  us  now  put  x  for  jp«,  and  y  for  p%,  on  the  right-hand  sides  of 
(1),  (2),  and  (3) ;  we  may  then  write  them 

(Ao-P)  +  A,*;  +  A2y  =  0  (1'), 

(M2-/P)  +  A^  +  A1^0  (2'), 

(M.  -i»*P)  +M^  +  A0y  =  0  (3'), 

whence,  eliminating  x  and  y,  we  must  have  (see  chap,  xvi.,  §  8) 

(A0  -  P)  (A02  -pA.A.,)  +  (pA.2  -pi?)  (pAf  -  A0A,) 

+  (PAl-piF)(A°-AuA2)  =  0  (4). 


198 


THEORY  FOR  IRRATIONALS  OF  ANY  ORDER 


C1IAV. 


Whence 

{(A02  -^AA)  +  (pV  -  A0At)/  +  (Ax2  -  AA^JP 

=  A0(A02  -j?AA)  +pA2(pA22  -  A0A,)  +  Mi(A,2  -  A0A2) 
=  A03  +  Mi3  +  /A/  -  3MAA,,  (5). 

Hence  a.  rationalising  factor  of  P  is 

(A02  -MA)  +  (M/  -  AA>*  +  (A,2  -  A0A.2)/      (6), 

and  the  rationalised  result  is 

A03  +  M.3  +  p2A.23  -  3;>Ao A, A2  (7). 

The  reader  -who  is  familiar  with  the  elements  of  the  theory 
of  determinants  will  see  from  the  way  we  have  obtained  them 
that  (6)  and  (7)  are  the  expansions  of 


and 


1 

A, 

A2 

1 

A0 

A, 

2 

M« 

A0 

A0 

A, 

A2 

pK 

A0 

A, 

Mi 

pA, 

A0 

(6'), 


(n 


and  will  have  no   difficulty  in  writing  down  the   rationalising 
factor  and  the  result  of  rationalisation  in  the  general  case. 

IV.  A  rationalising  factor  can  be  found  for  any  rational  integral 
function  of  p1/l,  qllm,  rlln,  .  .  . ,  &c,  by  first  rationalising  with 
respect  to  p111,  then  rationalising  the  result  with  respect  to  ql,m, 
and  so  on. 

V.  Every  rational  function  of  p1/l,  qVmt  r^*,  whether  integral  or 
not,  can  be  expressed  as  a  linear  function  of  p1!l,  pr11,  •  •  • ,  p^1'1^1 ; 
qVm,q2lm,  .  .  .,  (fi™-**!™,  &C  ;  and  of  the  products  p*'1  qt/nr*lm  .  .  ., 
the  coefficients  of  the  function  being  rational,  so  far  as  p1!l,  q1!m,  r1/n 
are  concerned. 

For  every  such  function  has  the  form  P/Q  where  P  and  Q 
are  rational  and  integral  functions  of  the  given  irrationals ;  and, 
if  R  be  a  rationalising  factor  of  Q,  PR  QR  will  be  of  the  form 
required. 


X  EXERCISES  XIV  199 

Example  1.  Show  that  a  rationalising  factor  of  a;  +  y  +  z   is 

(a;3  +  y3  +  z8  -  y  V  -  s3a;3  -  a:  y3) 

/I       3      i     ,,  4  J      1  i       4  4> 
x  (a-  +  y  +  z  +  2y333  -  z3x3  -  x 6y  ) 

,    i         3         9         4  4^44         i   is 

x  (ar  + 1/3  +  ;3  -  y  V  +  2z3ar  -  ary3) 

,3      9      3      44      4Jo4Sn 
x  (a;3  +  y3  +  23  -  y  V  -  z3a;5  +  2x6if) ; 

and  that  the  result  of  the  rationalisation  is  (x  +  y  +  z)3- 27 xyz. 

Exercises  XIV. 
Express  as  roots  of  rational  numbers — ■ 

(1.)  2!x3-*x4ix9*.  (2.)   {!/(**)}*+ {S/tf)}* 

(3.)  3V(Z/7)-2W?/7).  (4.)   {1/{W*)}  x  #(1S»)}. 

Simplify  the  following — 
(5.)   {(a-a/6-2)VW6)}    x  ^/(«1;<"-1,i1/("-1))- 

(6.)    (/fl/IHWM)  x  (a;(c+«)'(<»-»))l/(»-c)  X  (x(»+*)/(»-e))V(«-a). 

(7.)  Showthat  n/("%/,!+n/(''%=  ^v'+^x"^ 

Simplify — 

(S.)  [x^-y'^ix-t-y-h  (9.)  (ar»- 2 +  *-»)/(*- 2 4-ar1). 

(10.)  {x  +  x'^^-x'^-f. 

(11.)  (a^-a^+l)  (ar*+af*+  l){x-xh  +  l). 

(12.)  (xi  -  x  ~  V+  3*V )  (■**  -  2T  )• 

(13.)  (xl  +  4*/2)/(x3  +  2^3  +  2y). 

(14. )  23  - 1  +  23/(23  -  1)  + 1/(2*  + 1/(23  + 1)). 

(15. )  {x?  "  -  2./1 "  //'  "  +  y2/")  (x1 "  +  xl '-'"  y1  "-"  +  y1/n)  (aj1'"  -  y1  ")• 

(16.)  Show  that  x/{xi-l)-xi/{xi  +  l)-l/(x^-l)  +  l/(xh+l)=xi  +  2. 
(17.)  If  0(a-)  =  (ax -«"*)/(«* +  «"*)>     F(a-)  =  2/(a*  +  «T*), 
then  tf>(a; +y)=  {<fi(x)  +  <p(y) } / {1  +  £(a-)0(y) }  ; 

F(*  +  y)=  F(*)F(y)/  {1  +  tfaMy) } . 
(18.)  UxP/y=l,  then  xP-m/y9-n=xnJ''i-m=y"-m'''''. 
(19.)  If  m-ax,  n  =  ay,  m«nx  =  a-il,  then  xy;  =  l. 

Transform  the  following  into  sums  of  simple  irrational  terms  : — 

(20. )  V«/( \Ja  +  \/b)  +  V&/(  V«  ~  V6)- 
(21.)  (2V5-3V'^  +  W6)2. 

(22. )  {x  + 1  -  V2  +  \/3)  (a:  + 1  +  y/2  -  V3)  (a:  + 1  -  V2  -  V3),  arranging  ac- 
cording to  powers  of  x. 


200  EXERCISES  XIV  chap. 

(23. )  (1/ V»+ 1/  sja)  (xi  -  ah)l  {( V«  +  \/xf  -  ( V«  "  V*)2 }  ■ 
r24  v  V(«2+  {«(!  -  »0/3V»t}8)  +  o(to-  1)/2Vot 

K     ''  \/(a*+{a(\-m)lZsJm,y)-a{m-\)l2\/vi 

(C}r  v  \/(p/a  +  x)  +  *s/(p/a-z)  2pq 

(■to- )      „    t— — r — -,>  —, {,  where  a,x'=:  =- —  „. 

s/(p/a  +  x)  -  \/{p/a  -x)'  1  +  cf 

ton  \  P-a    p-b    p  +  a    p  +  b 

{to-) 1 r--— — r,  where  x-\/(nb). 

x-a     x-b     x  +  a    x  +  b  vv     ' 

(27.)  1/ {X/(P  -q)  +  y/p  +  V<?}  +  1/ !Mp  -q)-\/p-  \/?}  +  1/(VJP  -  V?)- 

(28)        /(l-*-^(2x  +  x*))  / /  1 -x+ V(2.r  +  ^)  )  . 

v     ''  V    U-a+V(2»+a*)/"r  V    ll-aj-V^+a:2)/ 

(29. )  ( V(«  +  &  +  c)  +  V(«  -  6  +  '0)7(  V(«  +  *  +  c)  -  V(«  -  6  +  c))2. 

(30.)  {U(p-q)  +  */p-<s/q)Ksf(p-q)-y/p-\/q)}. 

(31.)  (2.r5-6.r  +  5)/(4/2x'+  vA  +  l). 

(32. )  (a?  +  3  ^23  + 1  )/(.r  +  ^2  - 1). 

(33. )   { l/{a  +  b)-  l/(a  -  b) }  { [  y/{a  +  b)f  +  [  l/{u  -  i)]2  -  $/{<#  -  b-)  \ . 

Show  that 

<"•>  (r^r#  Gt^)-^^-  ve-*»- 

(35.)  (V(y-  +  i)  +  V(p2--i))-3  +  (V(^2  +  i)-V(y-i))-3=(y--i)V(r+i)- 

(36.)  V[\/{«2  +  \V&2)}  +  VF+  ^V&4)}]  =  («§  +  *<¥- 

Express  in  linear  form — 

(37.)  {Z/x-Z/y)/(l/x+i/y). 

(38. )  (1  +  V3  +  V5  +  V7)/(l  -  V3  -  \75  +  \/7)- 

(39.)  2(v&+ Vc)/(V&  +  Vc -  V«) - 42«(Vft  +  Vc)/n(\/ft  +  V<---  V«)- 

Rationalise  the  following  :  — 

(40.)  3.5*-  4^.  (41.)  2V(Hc-«). 

(42.)  V5  +  V3  +  V4 -  V6-  (43.)  3.2*  +  4.24-l. 

(44.)  a*  +  &J  +  c*.  (45.)  2*+2*  +  l. 

(46.)  If«  =  ;rV(l+i/2)  +  2/\/(l+*2).tlienV(l+«-)  =  -''2/  +  \/((l+»2)(1+2/2))- 

(47.)  Show  that  V(y..)  +  >/0,l,)  +  V(a>.yj 

=  (»/  -  z)%  +  (z  -  aQj  +  (a  -  y)1  +  (y  -  z)\z  -  x)\x  -  yY 
■'"  +  y2  +  z2  —  yz-zx-  xy 
(48. )  If  jr  =  l/(  Vi  +  \/c  -  \fa),      y  =  l/(\/c  +  s/a  -  \/£),      z=lf(s/a  +  V* 

-  /y/c),       U  =  l/(  V«  +  Vft  +  Vc)> 

then  Tl(-x+y  +  z  +  m)/(Ssb  -  ?t)3=  n(  ^  +  c  -  a)/8abc. 

xyz 

Historical  Note. — The  use  of  exponents  began  in  the  works  of  the  German 
"Cossists,"  Rudolf!  (1525)  and  Stifel  (1544),   who  wrote  over  the  contractions 


x  HISTORICAL  NOTE  201 

for  the  names  of  tbe  1st,  2nd,  3rd,  .  .  .  powers  of  the  variable,  which  had  been 
used  in  the  syncopated  algebra,  the  numbers  1,  2,  3,  .  .  .  Stifel  even  states 
expressly  the  laws  for  multiplying  and  dividing  powers  by  adding  and  subtracting 
the  exponents,  and  indicates  the  use  of  negative  exponents  tor  the  reciprocals  of 
positive  integral  powers.  Bombelli  (1579)  writes  _.,  ^,  „£,,  3>  •  •  •>  where 
we  should  write  .v°,.r, .-/;-,  .*.•■'',  .  .  .  Stevin  (1585)  uses  in  a  similar  way  @,  ©, 
©i  ©>•••>  and  suggests,  although  he  does  not  practically  use,  fractional 
powers  such  as  ©,   ©,  which  are  equivalent  to  the  x  ,  x  ,  of  the  present  day. 

Viete  (1591)  and  Oughtred  (1631),  who  were  in  lull  possession  of  a  literal 
calculus,  used  contractions  for  the  names  of  the  powers,  thus,  Aq,  Ac,  Aq</,  to 
signify  A'2,  A3,  A4.  Harriot  (1631)  simply  repeated  the  letter,  thus,  aa,  aaa, 
acuta,  for  ft2,  «:i,  a4.  Herigone  (1634)  used  numbers  written  after  the  letter, 
thus,  A,  A2,  A3,  .  .  .  Descartes  introduced  the  modern  forms  A,  A2,  A3,  .  .  . 
The  final  development  of  the  general  idea  of  an  index  unrestricted  in  magnitude, 
that  is  to  say,  of  an  exponential  function  ax,  is  due  to  Newton,  and  came  in 
company  with  his  discovery  of  the  general  form  of  the  binomial  coefficients  as 
functions  of  the  index.  He  says,  in  the  letter  to  Oldenburg  of  13th  June  1676, 
"Since   algebraists   write   a2,    ft3,   «',   &c,  for  aa,  aaa,   aaaa,   &c. ,   so   I    write 

a  ,  a",  a3,  for  \Ja,   \/as,  \/c.as:  and  I  write  a-1,  or-,  ar",  &c,  for  -,  — , 
1  «    aa 

—,kr." 

aaa 

The  sign  \/ was  first  used  by  Rudolff.;  both  he  and  Scheubel  (1551)  used 
/fj  to  denote  4th  root,  and  wJ  to  denote  cube  root.  Stifel  used  both  •sj'fr. 
and   \J  to  denote  square  root,  \/%%.   to   denote  4th  root,    and  so  on.     Girard 

(1633)  uses  the  notation  of  the  present  day,  \J,  \/,  &c.  Other  authors  of  the 
17th  century  wrote  y/2  :,  \/3  : ,  &c.  So  late  as  1722,  in  the  second  edition  of 
Newton's  Arithmetica  Universalis,  the  usage  fluctuates,  the  three  forms  \/3:, 

/3  3/ 

V     : ,   v'  all  occurring. 

In  an  incomplete  mathematical  treatise,  entitled  1)e  Arte  Logistica,  &c, 
which  was  found  among  the  papers  of  Napier  of  Merchiston  (1550-1617  ;  pub- 
lished by  Mark  Napier,  Edinburgh,  1839),  and  shows  in  every  line  the  firm  grasp 
of  the  great  inventor  of  logarithms,  a  remarkable  system  of  notation  for  irrationals 

is    described.      Napier    takes    the   figure   "       [_,  and  divides  it  thus    4J  |_5j  [6. 

'  •'  t-|  m  it 

He  then  uses  J,  \_J,  I ,  &c. ,  which  are  in  effect  a  new  set  of  symbols  for  the 

nine  digits  1,  2,  3,  &c,  as  radical  signs.  Thus  UlO  stands  for  \A0,  I-  10  for 
^10,  _i°10  for  ^/lO,  J!  10  for  ^10,  _]  ^j  or  =]  for  "Ao  ;  and  so  on. 

Many  of  the  rules  for  operating  with  irrationals  at  present  in  use  have  come, 
in  form  at  least,  from  the  German  mathematicians  of  the  16th  centuiy,  more 
particularly  from  Scheubel,  in  whose  Algebra  Compendiosa  Fo.cilisqiie  Descriptio 
(1551)  is  given  the  rule  of  chap,  xi  ,  §  9,  for  extracting  the  square  root  of  a 
binomial  surd.  Iu  substance  many  of  these  rules  are  doubtless  much  older  (as 
old  as  Book  X.  of  Euclid's  Elements,  at  least)  ;  they  were  at  all  events  more  or 
less  familiar  to  the  contemporary  mathematicians  of  the  Italian  school,  who  did 
so  much  for  the  solution  of  equations  by  means  of  radicals,  although  in  symbol- 
ism they  were  far  behind  their  transalpine  rivals.  See  Hutton's  Mathematical 
Dictionary,  Art.  "Algebra." 

The  process  explained  at  the  end  of  next  chapter  for  extracting  the  square  or 


202  HISTORICAL  NOTE  chap,  x 

cube  root  by  successive  steps  is  found  in  the  works  of  the  earliest  European 
writers  on  algebra,  for  example,  Leonardo  Fibonacci  (c  1200)  and  Luca  Pacioli  (c. 
1500).  The  first  indication  of  a  general  method  appears  in  Stifel's  Arithmetica 
Integra,  where  the  necessary  table  of  binomial  coefficients  (see  p.  81)  is  given. 
It  is  not  quite  clear  from  Stifel's  work  that  he  fully  understood  the  nature  of  the 
process  and  clearly  saw  its  connection  with  the  binomial  theorem.  The  general 
method  of  root  extraction,  together  with  the  triangle  of  binomial  coefficients,  is 
given  in  Napier's  De  Arte  Logistica.  He  indicates  along  the  two  sides  of  his 
triangle  the  powers  of  the  two  variables  (prsecedens  and  succedens)  with  which 
each  coefficient  is  associated,  and  thus  gives  the  binomial  theorem  in  diagram- 
matic form.  His  statement  for  the  cube  is — "  Supplementum  triplicationis  tribus 
constat  numeris  :  primus  est,  duplicati  prsecedentis  triplum  multiplicatum  per 
succedens  ;  secundus  est,  prsecedentis  triplum  multiplicatum  per  duplicatum  suc- 
cedentis  ;  tertius  est,  ipsum  triplication  succedentis."     In  modern  notation, 


CHAPTER    XL      . 
Arithmetical  Theory  of  Surds. 

ALGEBRAICAL   AND    ARITHMETICAL    IRRATIONALITY. 

§  1.]  In  last  chapter  we  discussed  the  properties  of  irra- 
tional functions  in  so  far  as  they  depend  merely  on  outward 
form ;  in  other  words,  we  considered  them  merely  from  the 
algebraical  point  of  view.  We  have  now  to  consider  certain 
peculiarities  of  a  purely  arithmetical  nature.  Let  p  denote  any 
commensurable  number ;  that  is,  either  an  integer,  or  a  proper  or 
improper  vulgar  fraction  with  a  finite  number  of  digits  in  its 
numerator  and  denominator ;  or,  what  comes  to  the  same  thing, 
letp  denote  a  number  which  is  either  a  terminating  or  repeating 
decimal.  Then,  if  a  be  any  positive  integer,  H/p  will  not  be 
commensurable  unless  p  be  the  nth  power  of  a  commensurable 
number  ;*  for  if  %/p  =  k,  where  k  is  commensurable,  then,  by  the 
definition  of  %/p,  p  =  kn,  that  is,  p  is  the  nth  power  of  a  commen- 
surable number. 

If  therefore p  be  not  a  perfect  nth  power,  %/p  is  incommensur- 
able. For  distinction's  sake  %/p  is  then  called  a  surd  number. 
In  other  words,  we  define  a  surd  number  as  the  incommensurable 
root  of  a  commensurable  number. 

Surds  are  classified  according  to  the  index,  n,  of  the  root  to 

be  extracted,  as  quadratic,  cubic,  biquadratic  or  quartic,  quintic, 

.   ,   .  w-tic  surds. 

The  student  should  attend  to  the  last  phrase  of  the  definition  of  a  surd  ; 
because  incommensurable  roots  might  be  conceived  which  do  not  come  under 

;;  This  is  briefly  put  by  saying  that  p  is  a  perfect  «th  power. 


204  CLASSIFICATION  OF  SURDS  chap. 

the  above  definition  ;  and  to  them  the  demonstrations  of  at  least  some  of  the 
propositions  in  this  chapter  would  not  apply.  For  example,  the  number  e  (see 
the  chapter  on  the  Exponential  Theorem  in  Part  II.  of  this  work)  is  incom- 
mensurable, and  \/c  is  incommensurable  ;  hence  \/e  is  not  a  surd  in  the  exact 
sense  of  the  definition.  Neither  is  V(  V2  + 1),  for  \/2  + 1  is  incommensurable. 
On  the  other  hand,  \/(  V2)>  which  can  be  expressed  in  the  form  tyl,  does  come 
under  that  definition,  although  not  as  a  quadratic  but  as  a  biquadratic  surd. 

He  should  also  observe  that  an  algebraically  irrational  function,  say  \/x, 
may  or  may  not  be  arithmetically  irrational,  that  is,  surd,  strictly  so  called, 
according  to  the  value  of  the  variable  x.     Thus  \J1  is  not  a  surd,  but  V2  is- 


CLASSIFICATION    OF    SURDS. 

§  2.]  A  single  surd  number,  or,  what  comes  to  the  same,  a 
rational  multiple  of  a  single  surd,  is  spoken  of  as  a  simple  mono- 
mial surd  number  ;  the  sum  of  two  snch  surds,  or  of  a  rational 
number  and  a  simple  monomial  surd  number,  as  a  simple  binomial 
surd  number,  and  so  on. 

The  propositions  stated  in  last  chapter  amount  to  a  proof  of 
the  statement  that  every  rational  function  of  surd  numbers  can 
be  expressed  as  a  simple  surd  number,  monomial,  binomial, 
trinomial,  &c,  as  the  case  may  be. 

§  3  ]  Two  surds  are  said  to  be  similar  when  they  can  be  expressed 
as  rational  multiples  of  one  and  the  same  surd  ;  dissimilar  when  this 
is  not  the  case. 

For  example,  >/18  and  N/8  can  be  expressed  respectively  in 
the  forms  3  N/2  and  2  J 2,  and  are  therefore  similar ;  but  J 6 
and  s/2  are  dissimilar. 

Again,  ^/54  and  £/16,  being  expressible  in  the  forms  3^2 
and  2  ^/2,  are  each  similar  to  1/2. 

All  the  surds  that  arise  from  the  extraction  of  the  same  nth  root 
are  said  to  be  equiradical. 

Thus  p*,  p*,  p*,  P*°  are  all  equiradical  with  p*. 

There  are  n  -  1  distinct  surds  equiradical  with  2>v'\  namely,  pl/n, 
P2!n,  .   .   .,  £>("■- D/'^  and  no  more. 

For,  if  we  consider  pmln  where  m>n,  then  Ave  have  pmln  = 
^*+»/n  -where  /x  and  v  are  integers,  and  v  <  n.  Hence  pm,n  = 
pft  pin  _  a  rational  multiple  of  one  of  the  above  series. 

All  the  surds  equiradical  with  pll*  are  rational  functions  (namely, 


xi  CLASSIFICATION  OF  SURDS  205 

positive  integral  powers)  of  plln  ;  and  every  rational  function  of  pl,n 
or  of  surds  equiradieal  with  pl,n  may  be  expressed  as  a  linear  function 
of  the  n  -  1  distinct  surds  which  are  equiradieal  with  pl,n,  that  is,  in 
the  form  A0  +  A^11'1  +  A.,p2ln  +  .  .  .  +  AM_1^n_1)/n,  where  A0,  Al5 
.  .  . ,  An  _  i  are  rational  so  far  as  plln  is  concerned. 

This  is  merely  a  restatement  of  §  18  of  chap.  x. 

§  4.]  The  p'oducl  or  quotient  of  two  similar  quadratic  surds  is 
rational,  and  if  the  product  or  quotient  of  the  two  quadratic  surds  is 
rational  they  are  similar. 

For,  if  the  surds  are  similar,  they  are  expressible  in  the 
forms  A  s/p  and  B  s/p,  where  A  and  B  are  rational ;  therefore 
A  \/p  x  B  s/p  -  ABp  ;  and  A  \/p/B  s/p  =  A/B,  which  proves  the 
proposition,  since  ABp  and  A/B  are  rational. 

Again,  if  s/p  x  \/q  =  A,  or  \/p/  \/q  =  B,  Avhere  A  and  B  are 
rational,  then  in  the  one  case  s/p  -  (AJq)  s^q,  in  the  other  s/p 
=  B  \'q.  But  A/q  and  B  are  rational.  Hence  s/p  and  \/q  are 
similar  in  both  cases. 

The  same  is  not  true  for  surds  of  higher  index  than  2,  but 
the  product  of  two  similar  or  of  two  equiradieal  surds  is  either  rational 
or  an  equiradieal  surd. 

INDEPENDENCE    OF    SURD    NUMBERS. 

§  5.]  If  p,  q,  A,  B  be  all  commensurable,  and  none  of  them  zero, 
and  s/p  and  sjq  incommensurable,  then  we  cannot  have 

s/p  =  A  +  B  sjq. 
For,  squaring,  we  should  have  as  a  consequence, 

p  =  A2  +  B2q  +  2AB  s/q  ; 
whence 

s/q  =  (p  -  A3  -  BV)/2AB, 

which  asserts,  contrary  to  our  hypothesis,  that  Jq  is  commen- 
surable. 

Since  every  rational  function  of  s/q  may  (chap,  x.,  §  15)  be 
expressed  in  the  form  A  +  B  Jq,  the  above  theorem  is  equivalent 
to  the  following  : — 

One  quadratic  surd  cannot  be  expressed  as  a  rational  function  of 
another  which  is  dissimilar  to  it. 


206  INDEPENDENCE  OF  SURD  NUMBERS  chap. 

Since  every  rational  equation  between  <Jp  and  Jq  which  is 
not  a  mere  equation  between  commensurables  (for  example, 
(  \/3)2  +  (  \/2)2  =  5)  is  reducible  to  the  form 

A  sj(pq)  +  B  x/jp  +  C  s/q  +  D  =  0, 

where  A,  B,  C,  D  are  rational ;  and,  since  this  equation  may  im- 
mediately be  reduced  to  another  of  the  form 

Jp  =  L  +  M  */q, 

where  L  and  M  are  rational,  it  follows  that 

No  rational  relation,,  which  is  not  a  mere  equation  between  rational 
numbers,  can  subsist  between  two  dissimilar  quadratic  surds. 

§6.]  7/"  the  quadratic  surds  >Jp,  \/q,  \/r,  \/{qr)  be  dissimilar  to 
each  other,  then  >Jp  cannot  be  a  rational  function  of  Jq  and  ijr. 

For,  if  this  were  so,  then  we  should  have 

s/p  =  A  +  B  *Jq  +  C  Jr  +  D  \/(gr), 

where  A,  B,  C,  D  are  all  rational. 

Now  we  cannot,  by  our  hypotheses,  have  three  of  the  four 
A,  B,  C,  D  equal  to  zero. 

In  any  other  case,  we  should  get  on  squaring 

p  =  {A  +  Bjq  +  C  Jr  +  D  J(qr)}°-, 

which  would  either  be  a  rational  equation  connecting  two  dis- 
similar quadratic  surds,  which  is  impossible,  as  we  have  just  seen  ; 
or  else  an  equation  asserting  the  rationality  of  one  of  the  surds, 
which  is  equally  impossible. 

An  important  particular  case  of  the  above  is  the  following  : — 

A  quadratic  surd  cannot  be  the  sum  of  two  dissimilar  quadratic 
surds. 

It  will  be  a  good  exercise  for  the  student  to  prove  this 
directly. 

§  7.]  The  theory  which  we  have  established  so  far  fur 
quadratic  surds  may  be  generalised,  and  also  extended  to  surds 
whose  index  exceeds  2.  This  is  not  the  place  to  pursue  the 
matter  farther,  but  the  reader  who  has  followed  so  far  will  find 
the  ideas  gained  useful  in  paving  the  way  to  an  understanding 
of  the  delicate  researches  of  Lagrange,  Abel,  and  Galois  regarding 


xi  INDEPENDENCE  OF  SURD  NUMBERS  207 

the  algebraical  solution  of  equations  whose  degree  exceeds  the 
4  th. 

§  8.]  It  follows  as  a  necessary  consequence  of  §§  5  and  6 
that,  if  we  are  led  to  any  equation  such  as 

A  +  Bs'p  +  C  v/g  +  D  ^(pq)  =  0, 
where  Jp  and  *Jq  are  dissimilar  surds,  then  we  must  have 

A  =  0,     B  =  0,     C  =  0,     D  =  0. 
One  case  of  this  is  so  important  that  we  enunciate  and  prove  it 
separately. 

If  x,  y,  z,  u  be  all  commensurable,  and  Jy  and  sju  incommen- 
surable, and  if  x  +  Jy  =  z  +  Ju,  then  must  x-z  and  y  =  u. 
For  if  x  =#  z,  but  =  a  +  z  say,  where  a  4=  0,  then  by  hypothesis 

a  +  z  +  \/y  =  z  +  \''u, 
whence  a  +  \/y  —  *Ju, 

a3  +  y  +  2a  s/y  -  u, 

s/y  =  («  -  a2  -  y)/2a, 
which  asserts  that  Jy  is  commensurable.     But  this  is  not  so. 
Hence  Ave  must  have  x  =  z ;  and,  that  being  so,  we  must  also 
have  Jy  —   \fu,  that  is,  y  =  u. 

SQUARE    ROOTS   OF   SIMPLE    SURD    NUMBERS. 

§  9.]  Since  the  square  of  every  simple  binomial  surd  number 
takes  the  form  p  +  Jq,  it  is  natural  to  inquire  whether  J(j>  +  *Jq) 
can  always  be  expressed  as  a  simple  binomial  surd  number,  that 
is,  in  the  form  *Jx  +  \'y,  where  x  and  y  are  rational  numbers. 
Let  us  suppose  that  such  an  expression  exists ;  then 

*J(jp+  s'q)=  \/x+  >Jy, 
whence  p  +  \'q  =  x  +  y  +  2  *J(xy). 

If  this  equation  be  true,  we  must  have,  by  §  8, 

x  +  y=p  (1), 

2^)=   s'q  (2); 

and,  from  (1)  and  (2),  squaring  and  subtracting,  we  get 
(x  +  y)3  -4xy=p*  -  q, 

that  is,  (z-y)2=p3~q  (3> 


208  LINEAR  EXPRESSION  FOR     </(«  +    \^)  chap. 

Xow  (3)  gives  either 

x-y  =  +  s!{/-q)  (4), 

or  x-y=  -  *S(p'-q)  (4*). 

Taking,  meantime,  (4)  and  combining  it  with  (1),  we  have 

(x  +  y)  +  (x-y)=p  +  s/{p*-q)  (5), 

(x  +  y)  -  (x  -y)=p-  s  '{f  -q)  (6) ; 

Avhence  2x  =p  +  \,'(p*  -  q), 

2y=p-  s/(p*-q); 
that  is,  x  =  h{p+   s'df-q)}  (7), 

V  =  HP  -  n;(/  "  ?)}  (8). 

If  we  take  (4*)  instead  of  (4),  we  simply  interchange  the  values 
of  x  and  y,  which  leads  to  nothing  new  in  the  end. 

Using  the  values  of  (7)  and  (8)  we  obtain  the  following 
result : — 

Since,  by  (2),  2  s/x  x  v/y  =  +  ^>  we  must  take  either  the  two 
upper  signs  together  or  the  two  lower. 

If  we  had  started  with  \/(p  -  */q),  it  would  have  been 
necessary  to  choose  \/x  and  \fy  with  opposite  signs. 

Finally  therefore  we  have 

(9), 

(9*). 

The  identities  (9)  and  (9*)  are  certainly  true  ;  we  have  in  fact 
already  verified  one  of  them  (see  chap,  x.,  §  9,  Example  14).  They 
will  not,  however,  furnish  a  solution  of  our  problem,  unless  the 
values  of  x  and  y  are  rational.  For  this  it  is  necessary  and 
sufficient  that  p*  -  q  be  a  positive  perfect  square,  and  that  p  be 


XI 


EXAMPLES  209 


positive.  Hence  the  square  root  of  p  +  *Jq  am  he  expressed  as  a 
simple  binomial  surd  number,  provided  p  be  positive  and  p*  -  a  be  a 
positive  perfect  square. 

Example  1.  Simplify  >/(19-4V21). 

Let  V(19-4V21)=V/a;  +  Vy- 

Then  aj+y=19, 

(cc-y)2  =  361-336 

=  25, 

x-y=  +5  say, 

x  +  y-19  ; 
whence  #  =  12,     y=7, 

*Jx  -  ±  VI 2,     \  //  =  T  \''7, 
so  that  V(l9-W21)=±(Vl2-\/7)- 

Example  2.   To  find  the  condition  that  \Z(VP+  V?)  ma}r  De  expressible 

4  / 

in  the  form  (\/x  +  \fy)  *Jp  we  have 

•s/NP  +  V?)  =  fa  x  V  U  +  V(?/l>)}  • 

Now  V{1  +  V((?/i°)}  "ill  t>e  expressible  in  the  form  \/x+\Jy,  provided 
1  -  q/p  be  a  positive  perfect  square  ;  this,  therefore,  is  the  required  condition. 
For  example, 

V(5V7  +  2V42)=  \/7x  V(5  +  2v'6) 

=  ±  4/7K/3  +  V2). 

Example  3.  It  is  obvious  that  in  certain  cases  V(.P  +  V?+  Vr+  N/'s)  roust 
be  expressible  in  the  form  \'x  +  \/y+  \  ~,  where  a1,  y,  z  are  rational.  To  find 
the  condition  that  this  may  be  so,  and  to  determine  the  values  of  x,  y,  z,  let 

V(P  +  \fl  +  V''  +  Vs)  =  \/x  +  \'y  +  Vs  C1 ). 

then  }i+\/q+\/r+\Js  =  x  +  y  +  z  +  2\/(yz)  +  2s/(zx)  +  2\/(xy)  (2). 

Now  let  us  suppose  that 

2V(yz)=V?  (3), 

2sJ{zx)  =  s/r  (4), 

2V(«y)=V*  (5). 

From  (4)  and  (5)  we  have  by  multiplication 

4x\/(yz)=*/(rs); 

whence,  by  using  (3),  x  =  hy/{>'s/q)  (6). 

Proceeding  in  like  manner  with  y  and  r,  we  obtain 

y=W(q*M  (7), 

~~=W(<7>7*)  («)• 

It  is  further  necessary,  in  order  that  (2)  may  hold,  that  the  values  (6),  (7), 
(8)  shall  satisfy  the  equation 

x  +  y  +  z=p  (9), 

VOL.  I  P 


210  ARITHMETICAL  SQUARE  ROOT  chap. 

that  is,  we  must  have 

V(W?)  +  VWO  +  s/iqr/s)  =  2p  (10), 

where  the  signs  throughout  must  be  positive,  since  x,  y,  z  must  all  be  positive. 
Also,  since  x,  y,  z  must  all  be  rational,  we  must  have 

rs      o     9s     as     W 
q  r  s 

where  a,  /3,  y  are  positive  rational  numbers,  such  that 

a  +  p  +  y  =  2p, 
whence,  in  turn,  we  obtain 

q  =  §y,     r  =  ya,     s  =  ap. 


ARITHMETICAL   METHODS    FOR   FINDING   APPROXIMATE    RATIONAL 
VALUES   FOR    SURD    NUMBERS. 

§  10.]  It  has  already  been  stated  that  a  rational  approxima- 
tion, as  close  as  we  please,  can  always  be  found  for  every  surd 
number.  It  will  be  well  to  give  here  one  method  at  least  by 
which  such  approximations  can  be  obtained.  We  begin  with 
the  approximation  to  a  quadratic  surd ;  and  we  shall  afterwards 
show  that  all  other  cases  might  be  made  to  depend  on  this. 

§  11.]  First  of  all,  we  may  point  out  that  in  every  case  we 
may  reduce  our  problem  to  the  finding  of  the  integral  part  of 
the  square  root  of  an  integer.  Suppose,  for  example,  we  wish 
to  find  the  square  root  of  3*689  correct  to  five  places  of  decimals. 
Then,  since  ^3-689  =  ^36890000000/10*,  we  have  merely  to 
find  the  square  root  of  the  integer  36890000000  correct  to  the 
last  integral  place,  and  then  count  off  five  decimal  places. 

§  12.]  The  following  propositions  are  all  that  are  required 
for  the  present  purpose  : — 

I.  The  result  of  subtracting  (A  +  B)2  from  N  is  the  same  as  the 
result  of  first  subtracting  A2,  then  2AB,  and  finally  B2. 

This  is  obvious,  since  (A  +  B)2  =  A2  +  2AB  +  B2. 

II.  If  the  first  p  out  of  the  n  digits  of  the  square  root  of  the 
integer  N  have  been  found,  so  that  P10n_^  is  a  first  approximation 
to  VN,  then  the  next  p  -  1  digits  ivill  be  the  first  p  -  1  digits  of  the 
integral  part  of  the  quotient  {N  -  (Pl0n-^)2}/2Pl0'1-^  with  a  possible 
error  in  excess  of  1  in  the  last  digit, 


xi                                  ARITHMETICAL  SQUARE  ROOT  211 

Let  the  whole  of  the  rest  of  the  square  root  be  Q.  Then 

x/N  =  P10»-"  +  Q, 
where  1 0*  - x  <  P  <  1 0*,  Q  <  1 0n  -*  ; 

whence  N  =  (P10w-*>)2  +  2PQ10*-*  +  Q2, 

N-(P10"-^)2_             Q2  (1). 
—  \°l  + 


2P10""^  ^     2P10n"^ 


Now 


Q72PlOn-^<102(,l-^/2  x  10J,-110n-*'<10n-*+1/2. 

Hence  Q2/2P10n--P  will  at  most  affect  the  (n  -  2p  +  l)th  place, 
and  the  error  in  that  place  will  be  at  the  utmost  5  in  excess. 
Therefore,  since  Q  contains  n-p  digits,  the  first  p  -  1  of  these 
will  be  given  by  the  first  p  -  1  digits  of  {N  -  (P10n-^)2}/2P10n"-P 
with  a  possible  error  in  excess  of  1  in  the  last  digit.* 

§  13.]  In  the  actual  calculation  of  the  square  root  the  first 
few  figures  may  be  found  singly  by  successive  trials,  Proposi- 
tion I.  being  used  to  find  the  residues,  which  must,  of  course, 
always  be  positive.  Then  Proposition  II.  may  be  used  to  find 
the  succeeding  digits  in  larger  and  larger  groups.  The  approxi- 
mation can  thus  be  carried  out  with  great  rapidity,  as  will  be 
seen  by  the  following  example  : — 

Let  it  be  required  to  find  the  square  root  of  N  =  680100000000000000, 
which,  for  shortness,  we  write  6801(14). 

Obviously  8(8)<\/N<9(8)  ;  in  other  words,  \/N  contains  9  digits,  and  the 
first  is  8. 

Now  N-  (8(8))2  =  401(14),  which  is  the  first  residue.  We  have  now  to 
find  the  greatest  digit  x  which  can  stand  in  the  second  place,  and  still  leave 
the  square  of  the  part  found  less  than  N,  that  is  (by  Proposition  I.),  leave  the 
residue  401(14)  -2  x  8(8)  xx(7)  -  {x(7)}2  positive.  It  is  found  by  inspection 
that»-  =  2.  Carrying  out  the  subtractions  indicated,  that  is,  subtracting 
|16(8)  +  2(7)}  x2(7)  =  162x2(14)  from  401(14),  we  have  now  as  residue 
7700(12). 

*  The  effect  of  such  an  error  would  be  to  give  a  negative  residue  in 
the  process  of  §  13  ;  so  that  in  practice  it  would  be  immediately  discovered 
and  rectified.  As  an  example  of  a  case  where  the  error  actually  occurs,  the 
reader  might  take  the  square  root  of  5558(12),  namely,  74551995,  and  attempt 
to  deduce  from  745  the  two  following  digits.  He  will  find  by  the  above  rule 
52  instead  of  51.  If  it  be  a  question  of  the  best  approximation,  the  rule  gives 
here,  as  always,  the  best  result ;  but  this  is  not  always  what  is  wanted. 


212 


EXAMPLES 


CHAP. 


The  double  of  the  whole  of  the  part  of  \J~N  now  found  is  164(7)  ;  and 

we  have  next  to  find  y  as  large  as  may  be,  so  that  7700(12)-  {164(7) +  2/(6)} 

x  ?/(6)  shall  remain  positive.     This  value  of  y  is  seen  to  be  4.     It  might,  of 

course,  be  found  (by  Proposition  II.)  by  dividing  7700(12)  by  164(7),  and 

taking  the  first  figure  of  the  quotient. 

The  residue  is  now  112400(10).     The   process  of  finding  the  first  four 
digits  in  this  way  may  be  arranged  thus  :  — 

8(8)  6801(14)  8(8) 

16(8)  6400(14) 

162(7)  401(14)  +2(7) 

164(7)  324(14) 

1644(6)  7700(12)  +4(6) 

1648(6)  6576(12) 

16486(5)  112400(10)         +6(5) 

16492(5)  98916(10) 

134840(9) 

We  might,  of  course,  continue  in  the  same  way,  figure  by  figure,  as  long  as 
we  please  ;  and  we  might  omit  the  records  in  brackets  of  the  zeros  in  each  line. 

Havino-,  however,  already  found  four  figures,  we  can  find  three  more  by 
dividing  the  residue  134840(9)  by  16492(5),  which  is  the  double  of  8246(5), 
the  part  of  VN  already  found. 


16492(5)      134840(9) 
131936 


817(2) 


29040 
16492 

125480 
115444 


10036000(4) 
The  next  three  digits  are  therefore  817.  10036000(4)  is  not  the  residue  ; 
for  we  have  only  subtracted  from  VN  as  yet  {8246(5)} 2  and  2x8246(5) 
x  817(2).  Subtracting  also  {817(2)}2  we  get  the  true  residue,  namely, 
93685110000.  We  may  now  divide  this  by  2x8246817(2),  that  is,  by 
1649363400,  and  thus  get  the  last  two  figures.     We  have  then 

10036000(4) 
667489(4) 


1649363400  I 


93685110000 
8246817000 
11216940000 
9896180400 

1320759600 


56 


We  have  now  found  the  whole  of  the  integral  part  of  V6801(14),  namely, 
824681756. 


XI 


RATIONAL  APPROXIMATION  TO  ANY  SURD 


213 


If  it  were  desired  to  carry  the  approximation  farther,  8  places  after  the 
decimal  point  could  at  once  be  found  by  dividing  the  true  residue 
(1320759600  -  562)  by  2  x  824681756.  If  we  require  no  more  places  than  those 
8  places,  then  the  residue  is  of  no  importance,  and  we  may  save  labour  by 
adopting  the  abbreviated  method  of  long  division  (see  Brook  Smith's  Arith- 
metic, chap.  vi. ,  §  153).     Thus 


nftiW$$V$ 


1320759600 
3136 

1320756464 
1319490810 

1265654 
1154554 


80076736 


111100 

98962 

12138 
11545 


593 
495 

"98 
98 

0 


We  thus  find  V6801(14)  =  824681756 '80076736. 
will  find  that  in  point  of  fact 


On  verifying,   the  reader 


(824681756 -80076736)2  =  680100000000000001 -82  .  .  . 

It  will  be  a  good  exercise  for  him  to  find  out  how  many  decimal  places  of 
the  square  root  of  a  given  integer  must  be  found  before  the  square  of  the 
approximation  ceases  to  be  incorrect  in  the  last  integral  place. 

§  14.]  By  continually  extracting  the  square  root  (that  is  to 
say,  hy  extracting  the  square  root,  then  extracting  the  square 
root  of  the  square  root,  and  so  on),  we  may  bring  any  number 
greater  than  unity  as  near  unity  as  we  please.  In  other  words, 
by  making  n  sufficiently  great,  W1*  may  be  made  to  differ  from  1 
by  less  than  any  assignable  quantity. 

For  let  it  be  required  to  make  NI/2  less  than  1  +  a,  where  a 
is  any  positive  quantity.  This  will  be  done  if  2n  be  made  such 
that  (1  +  afl>  N.  Now  (chap,  iv.,  §  1 1)  (1  +  a)2"  =  1  +  2'la  +  a 
series  of  terms,  which  are  all  positive.  Hence  it  will  be  sufficient 
if  we  make   1  +  2"u>  N,  that  is,  if  we  make  2na>N  -  1,  thut  is, 


214  EXAMPLES  chap. 

if  we  make  2n>(N-  l)/a,  which  can  always  be  done,  since  by 

making  n   sufficiently  great    2n  may  be  made   to   exceed   any 

quantity,  however  great. 

Example.    How  many  times  must  we  extract  the  square  root  beginning 
with  51  in  order  that  the  final  result  may  differ  from  1  by  less  than  -001  ? 

We  must  have 

2»  >  (51-1)/ -001, 
2"  >  50000. 
Now  215  =  32768,     216  =  65536, 

hence  we  must  make  ?i  =  16. 

In  other  words,  if  we  extract  the  square  root  sixteen  times,  beginning 
with  51,  the  result  will  be  less  than  1  "001. 

§  15.]  It  follows  from  §  14  that  we  can  approximate  to  any 
surd  whatever,  say  plln,  by  the  process  of  extracting  the  square 
root.  For  (see  chap,  ix.,  §  2)  let  1/n  be  expressed  in  the  binary 
scale,  then  we  shall  have 

1/n  =  a/2  +  /3/22  +  y/2'  +  .  .  ,+fjL, 

where  each  of  the  numerators  a,  ft,  y,  .  .  .  is  either  0  or  1,  and 
ix  is  either  absolutely  0  or  <  l/2r,  where  r  is  as  great  as  we 
choose. 

Hence 

=pt/2  x^/S/22  x^/23  x  x^»  ^y 

Now,  excepting  the  last,  each  of  these  factors  is  either  ] ,  or  of 
the  form  p*1"' ,  which  can  be  approximated  to  as  closely  as  we 
please  by  continued  extraction  of  the  square  root.  If  /i  =  0,  the 
last  factor  is  1  ;  and  if  ll<  \/2r,  since  r  may  be  as  great  as  we 
choose,  we  can  make  it  differ  from  1  by  as  small  a  fraction  as 
we  choose.  It  follows  therefore  that  the  product  on  the  right 
hand  of  (1)  may  be  found  in  rational  terms  as  accurately  as  Ave 
please. 

Example.  To  find  an  approximate  value  of  5V9. 
We  have 

i    i_    i    i     i     L    L    L   L    L   L 

3     2'2     2*     26     28"*"210"*~212"^  2U"^216  +  218"^2-""^'U' 
where  fi  <  1/220. 


XI  ALGEBRAICAL  SQUARE  ROOT  215 

Now  we  have,  correct  to  the  fourth  decimal  place,  the  following  values  :— 
5V*=  2-67234,  51^"= 1-00096, 

511/24=  1  -27857,  511"-'4  =  1  -00023, 

51^=1-06336,  51'2,6  =  1-00006, 

511  -8  =  1  -01548,  511"-'8  =  1  -00002, 

5H/2">  - 1  -00385,  511/220  <  1  -00001. 

Hence,  multiplying  the  first  nine  numbers  together,  we  get 

5V3  =  3  70841 
The  correct  value  is  3-708429  .  .   . 

§  16.]  The  method  just  explained,  although  interesting  in 
theory,  would  be  very  troublesome  in  practice. 

The  method  given  in  §  13  for  extracting  the  square  root  may 
be  easily  generalised  into  a  method  for  extracting  an  ?it\\  root 
directly,  figure  by  figure,  and  group  by  group  of  figures.  The 
student  will  be  able  to  establish  for  himself  two  propositions, 
counterparts  of  I.  and  II.,  §  12,  and  to  arrange  a  process  for 
the  economical  calculation  of  the  residues.  A  method  of  this 
kind  is  given  in  most  arithmetical  text-books  for  extracting  the 
cube  root,  but  it  is  needless  to  reproduce  it  here,  as  the  extrac- 
tion of  cube  and  higher  roots,  and  even  of  square  roots,  is  now 
accomplished  in  practice  by  means  of  logarithmic  or  other  tables 
(see  chap,  xxi.)  Moreover,  the  extraction  of  the  nth  root  of  a 
given  number  is  merely  a  particular  case  of  the  numerical  solu- 
tion of  an  equation  of  the  nth  degree,  a  process  for  which,  called 
Homer's  Method,  will  be  given  in  a  later  chapter. 

Our  reason  for  dwelling  on  the  more  elementary  methods  of 
this  chapter  is  a  desire  to  cultivate  in  the  mind  of  the  learner 
exact  ideas  regarding  the  nature  of  approximate  calculation — 
a  process  which  lies  at  the  root  of  many  useful  applications  of 
mathematics. 

SQUARE    BOOT    OF   AN    INTEGRAL    FUNCTION    OF   X. 

§  17.]  When  an  integral  function  of  x  is  a  complete  square 
as  regards  .r,  its  square  root  can  be  found  by  a  method  analogous 


216  ALGEBRAICAL  SQUARE  ROOT  chap. 

to  that  explained  in  §  12,  for  finding  the  square  root  of  a  number. 
Although  the  method  is  of  little  interest,  either  theoretically  or 
practically,  we  give  a  brief  sketch  of  it  here,  because  it  illustrates 
at  once  the  analogy  and  the  fundamental  difference  between 
arithmetical  and  algebraical  operations.* 

I.  We  may  restate  Proposition  I.  of  §  1 2,  understanding  now 
A  and  B  to  mean  integral  functions  of  x. 

II.  IfF  =p0x2n  +  p1x2n~1  +  .  .  .  +p,n,  and  if  JF  =  {q„xn  +  qxxn~x 
+  .  .  .  +  qn-p+xxn-p+1)  +  {qn-p*n~p  +  •  •  •  +  q0)  =  p  +  Q,say;  and  if 

we  suppose  the  first  p  terms,  namely,  P  =  q0xn  +  qxxn~l  +  .   .  .  +  qn-P+i 

xn~P+1,  of  \/F  to  be  biown,  then  the  next  p  terms  will  be  the  first  p 

terms  in  the  integral  part  of  (F  -  P2)/2P. 

for  we  have 

F  =  F  +  2PQ  +  Q2 ; 

,  F-F  Q2 

hence  —^  =  Q  +  ^ 

Now  the  degree  of  the  integral  part  of  Q2/2P  is  2(n-p)-n 
=  n-  2p.  Hence  Q2/2P  will  at  most  affect  the  term  in  xn~2p. 
Hence  (F  -  P2)/2P  will  be  identical  with  Q  down  to  the  term  in 
xn-2p+i  inclusive.  In  other  words,  the  first  n-p  -  (»  -  2p)  =p 
terms  obtained  by  dividing  F  -  P2  by  2P  will  be  the  p  terms  of 
the  square  root  which  follow  P. 

We  may  use  this  rule  to  obtain  the  whole  of  the  terms  one 
at  a  time,  the  highest  being  of  course  found  by  inspection  as  the 
square  root  of  the  highest  term  of  the  radicand  ;  or  we  may  ob- 
tain a  certain  number  in  this  way,  and  then  obtain  the  rest  by 
division. t 

The  process  will  be  understood  from  the  following  example, 

*  The  method  was  probably  obtained  by  analogy  from  the  arithmetical 
process.  It  was  first  given  by  Recorde  in  The  Whetstone  of  Witte  (black 
letter,  1557),  the  earliest  English  work  on  algebra. 

t  Just  as  in  division,  we  may,  if  we  please,  arrange  the  radicand  according 
to  ascending  powers  of  x.  The  final  result  will  be  the  same  whichever  arrange- 
ment be  adopted,  provided  the  radicand  is  a  complete  square.  If  this  is  not 
the  case  the  operation  may  be  prolonged  indefinitely  just  as  in  continued 
division.  We  leave  the  learner  to  discover  the  meaning  of  the  result  obtained 
in  such  cases.  The  full  discussion  of  the  matter  would  require  some  refer- 
ence to  the  theory  of  infinite  series. 


XI 


ALGEBRAICAL  SQUARE  ROOT 


217 


in  which  we  first  find  three  of  the  terms  of  the  root  singly,  and 
then  deduce  the  remaining  two  by  division  : — 

Exam]  ile. 

To  find  the  square  root  of 

a;io  +  6^9  +  13Z8  +  4a;7  -  18.x6  -  12a:5  +  14ar*  -  12k3  +  9a-2  -  2x  +  1. 


1 

2  +  3 
2  +  6  +  2 
2+6+4-4 

2+6+4-8 


1  +  6  +  13+   4-18-12  +  14-12  +  9-2  +  1 

1 


6  +  13+   4-18-12  +  14-12  +  9-2  +  1 

6+   9 

4+    4-18-12  +  14-12  +  9-2  +  1 
4  +  12+    4 


-  8-22-12  +  14-12  +  9-2  +  1 

-  8-24-16  +  16 


2+    4-    2-12+9-2+1 
2+    6+    4-    8 


+  1 
+  3 
+  2 


+  1-1 


-  2-    6-    4  +  9-^2  +  1 

-  2-    6-    4  +  8 

1-2  +  1 
Hence  the  square  root  is  x5  +  3a;4  +  2a*3  -  4a.*2  +  x  -  1  ;  and,  since  the  residue 
x*-2x+\  is  the  square  of  the  two  last  terms,  namely,  a;— 1,  we  see  that  the 
radicand  is  an  exact  square.     Of  course,  we  obtain  another  value  of  the  square 
root  by  changing  the  sign  of  every  coefficient  in  the  above  result. 

A  similar  process  can  be  arranged  for  the  extraction  of  the 
cube  root ;  but  it  is  needless  to  pursue  the  matter  further. 

§  18.]  The  student  should  observe  that  in  the  simpler  cases 
the  root  can  be  obtained  by  inspection ;  and  that  in  all  cases  the 
method  of  indeterminate  coefficients  renders  any  special  process 
for  the  extraction  of  roots  superfluous.  This  will  be  understood 
from  the  following  example. 


Example. 

To  extract  the  square  root  of 


,.io 


+  6a;9  +  13a:8  +  4a;7  -  18a:6 -  12a;5  +  Ux4  -  12a;3  +  9a:2  -  2x+ 1 


(1). 


If  the  radicand  be  a  complete  square,  its  square  root  must  be  of  the  form 

ar5  +pxi  +  qx*  +  rx"  +sx+ 1  (2 ). 

The  square  of  (2)  is 

xit)  +  '2px9+(p2  +  2q)xs  +  (22)q  +  2r)x7  +  (2pr  +  qii  +  2s)xe  +  .  .  .         (3). 

Now  this  must  be  identical  with  (1) ;  hence  we  must  have 

2p  =  G,    p2  + 2-7=13,     2pq+2r=4,     2pr+ga+2s=  -18. 


218  EXERCISES  XV 


CHAP. 


The  first  of  these  equations  gives  p  =  S  ;  p  being  thus  known,  the  second 
gives  q=2  ;  p  and  q  being  known,  the  third  gives  r—  -4  ;  andp,  q,  r  being 
known,  the  last  gives  8=1.  We  could  now  find  I  in  like  manner  ;  but  it  is 
obvious  from  the  coefficient  of  £  that  t=  —  1. 

Hence  one  value  of  the  square  root  is 

x5  +  3X4  +  2x*  -  Ax2  +  x  - 1 . 

N.B. — The  equating  of  the  coefficients  of  the  remaining  terms  of  (1)  and 
(3)  will  simply  give  equations  that  are  satisfied  by  the  values  of  p,  <7,  r,  s 
already  found,  always  supposing  that  the  given  radicand  is  an  exact  square. 

A  process  exactly  similar  to  the  above  will  furnish  the  root  of  an  exact 
cube,  an  exact  4th  power,  and  so  on. 


Exercises  XV. 

Express  the  following  as  linear  functions  of  the  irrationals  involved. 

(1.)  l/(VH  +  V3  +  \/14).  (2.)  x/12/(l  +  V2)(\/6-V3). 

(3.)  (1  -  V2  +  V3)/(l  +  V2+  V3)  +  (1  -  V2  -  V3)/(l  +  \/2  -  V3). 

(4.)  (3-V5)/(V3  +  V5)2  +  (3  +  \/5)/(V3-\/5)2. 

(5.)  V5/(V3  +  V5-2V2)-V2/(\/3  +  V2-\/5). 

(6.)  (7  -  2  V5)(5  +  V7)(31  +  13v'5)/(6  -  2V7)(3  +  V5)(H  +  4 V")- 

(7.)  V(25  +  10V6).  (8.)  V(3/2  +  v'2). 

(9.)  V(123-22V2).  (10.)  V(44V2  +  12V26). 

(11.)  V{(8  +  4VlO)/(8-4VlO)}. 
(12.)  V(7  +  4\/3)+V(5-2V6). 
(13.)  V(15-4V14)  +  1/V(15+4V14). 
(14. )  1/V(16  +  2  V63)  +  l/\/(16  -  2  V63). 
(15.)  l/V(16V3  +  6V21)  +  V(16v'3-6V21). 

(16.)  Calculate    to   five   places   of    decimals   the   value    of    {\/(5  +  2\/6) 

-V(5-2V6)}/{V(5  +  2\/6)+V(5-2V<5)}- 

(17.)  Calculate  to  seven  places  of  decimals  the  value  of  \/(\/15  +  \/13) 
+  VW15-V13). 

Simplify— 

(IS.)  V{3  +  V(9-i;2)}  +  V{3-V(9-^2)}. 
(19.)  ^{a  +  b-c+2^(b(a-c))}. 
(20.)  %/{«2-2  +  «V(«2-4)}. 

<-U/{(>-^Xr^-)}- 

(22.)  Show  that  V{2  +  V(2  -  V2)}  =  ./ {  2  +  V(^+n/2)  } 

(23. )  Express  in  a  linear  form  \/(5  +  V6  +  V^O  +  V15)- 
(24.)  „  ,,  V(25-4V3-12x/2  +  6V6). 


XI 


EXERCISES  XV  219 


(25.)  If  a-d  =  bc,  then  \/{a  +  \Jb  +  \Jc  +  \Jd)  can  always  be  expressed  in 
the  form  {\/x  +  sfy){\JX  +  sJY).  Show  that  this  will  be  advantageous  if 
a2  -  b  and  cr-c  are  perfect  squares. 

(26.)  If  f/(a  +  \Jb)  =  z+\/y,  where  a,  b,  x,  y  are  rational,  and  \Jb  and 
s/y  irrational,  then  f/{a -  \Jb)  =  x -  \/y.  Hence  show  that,  if  a2-b  =  z3i 
where  z  is  rational,  and  if  x  be  such  that  4xz-Zxz  =  a,  then  ^/(a  +  sjb) 
=x+»/(x*-z). 

(27.)  Express  in  linear  form  <i/{99  -  35\/8). 

(28.)  ,,  „  4/(395  + 93  V18). 

(29.)  „  „  4/(117V2  +  74V5).   ' 

(30.)  Show  that  4/(90 +  34V7)-  ^(90-Mv7)  =  2>/7. 

(31.)  If  x=  J/{p  +  q)+  </{p-q),  and  f-q-^r3,  show  that  ar3-3ra;-2^ 
=  0. 

(32.)  If  py*  +  qi/  +  r  =  0,  wherep,  q,  r,  y  are  all  rational,  and  y  irrational, 
then  p=0,  q  =  Q,  r=0.     Hence  show  that,  if  x,  y,  z  be  all  rational,  and 

x  ,  y  ,  z   all  irrational,  then  neither  of  the  equations  x+y=z,  x+y=z   is 
possible. 

(33.)  Find,  by  the  full  use  of  the  ordinary  rule,  the  value  of  \/10  to  5 
places  of  decimals  ;  and  find  as  many  more  figures  as  you  can  by  division 
alone.     Use  the  value  of  \/10  thus  found  to  obtain  \/-004. 

Extract  the  square  root  of  the  following  :  — 

(34.)  (yz  +  zx  +  xy)2-4xyz(z  +  x). 

(35. )  25a;2  +  9r/2  +  z2  +  6yz  -  lOzx -  SOxy. 

(36.)  9arl  +  24ar3+10a:2-8a;+l.  (37.)  af4-  4ar3  +  2a:2+4a;  +  l. 

(38.)  4xi-l2xiy  +  25xY-2ixy3  +  l6yi. 

(39.)  ars-6ar4  +  4ar3  +  9a;2-12a;  +  4. 

(40. )  4a;6  -  12a*  +  5ar*  +  22x?  -  23a;2  -  8a;  +16. 

(41. )  27(;a  +  qf(p"  +  q2)2  -  2(2r  +  ipq  +  q2?. 

(42.)  a;"3-2a:Va;  +  3a;-2v'a;+l- 

(43.)  Extract  the  cube  root  of 

8a;9  -  1 2a;8  +  6a;7  -  37a;6  +  36;^  -  9a,-1  +  54a-3  -  27a;2  -  27. 

(44.)  Extract  the  cube  root  of 

18(p3  +p2q  +pq2  +  y5) ±2  V3(5/  +  3p2q  -  Zpq2  -  5?3). 

(45.)  Show  that  X  can  be  determined  so  that  a4  +  6a?  +  7a;2  -  6a; +  X  shall  be 
an  exact  square. 

(46.)  Find  a,  b,  c,  so  that  xR  -  8zs  +  ax4  +  bx*  +  ex2  -  Ux  +  i  shall  be  an 
exact  square. 

(47.)  If  ax4  +  bx3  +  ca-2  be  subtracted  from  (x2  +  2a-  +  4)3  the  remainder  is  an 
exact  square  ;  find  a,  b,  c. 

(48. )  If  a^  +  ax5  +  tar4  +  car3  +  dx2  +  ex  +/  be  an  exact  square,  show  mat 
d  =  ^\«4  -  %a2b  +  \ b2  +  \ac, 
e  =  -  ^a5  +  \a?b  -  \a2c  -  \ab2  +  \be, 


-< 


220  EXERCISES  XV 


CHAP.   XI 


And  that  the  square  root  is 

ar*  +  iaa?  +  (  -  |«.2  +  \b)x  +  (&a?  -\db+  |c). 

(49.)  4a56+12.ri  +  5,r4-2.*::,  are  the  first  four  terms  of  an  exact  square  ;  find 
the  remaining  three  terms. 

(50.)  If  x^  +  Sdx^  +  ex^fx^  +  gx^  +  hx  +  P  be  a  perfect  cube,  find  its  cube 
root ;  and  determine  the  coefficients  e,f,  g,  h,  in  terms  of  d  and  k. 

(51.)  Show  that 

b%a  -b)(c  -b){(a-  6)2  +  (c-6)2}  -  ffJM^  +  O +  **(«•- & +  c) 
is  an  exact  cube. 

(52.)  Express  \/{l+x  +  a?+a?+.  .  .  ad  »}  in  the  form  a  +  bx  +  cx-  + 
...  as  far  as  the  4th  power  of  x.  To  how  many  terms  does  the  square  of 
your  result  agree  with  1  +  x  +  x2  +  x3  +.   .   .? 

(53.)  Express,  by  means  of  the  ordinary  rule  for  extracting  the  square 
root,  xAl  ~  ■*')  "s  an  ascending  series  of  integral  powers  of  x,  as  far  as  the 
4  th  power. 

(54.)  Express  \J(x+l)  as  a  descending  series  of  powers  of  x,  calculating 
six  terms  of  the  series. 

(55.)  Show  that  Lambert's  theorem  (chap,  ix.,  §  9)  can  be  used  to  find 
rational  approximations  to  surd  numbers.  Apply  it  to  show  that  \/'2  =  \  + 1/2 
-  1/2.5  +  1/2.5.7  -  1/2.5.7.197  approximately  ;  and  estimate  the  error. 


CHAPTEE   XII. 
Complex  Numbers. 

ON    THE    FUNDAMENTAL    NATURE    OF    COMPLEX    NUMBERS. 

§  1.]  The  attempt  to  make  certain  formulae  for  factorisation 
as  general  as  possible  has  already  shown  us  the  necessity  of  in- 
troducing into  algebra  an  imaginary  unit  i,  having  the  property 
i"  =  —  1.  It  is  obvious  from  its  definition  that  i  cannot  be  equal  to 
any  real  quantity,  for  the  squares  of  all  real  quantities  are  positive. 
The  properties  of  i  as  a  subject  of  operation  are  therefore  to  be 
deduced  entirely  from  its  definition,  and  from  the  general  laws 
of  algebra  to  which,  like  every  other  algebraical  quantity,  it 
must  be  subject. 

Since  i  must,  when  taken  along  with  other  algebraical  quan- 
tities, obey  all  the  laws  of  algebra,  we  may  consider  any  real 
multiples  of  i,  say  yi  and  y'i,  where  y  and  y'  are  positive  or 
negative,  and  we  must  have  yi  =  iy,  yi  +  y'i  -  (y  +  y')i  =  i(y  +  y'), 
and  so  on  ;  exactly  as  if  i  were  a  real  quantity. 

By  taking  all  real  multiples  of  i  from  -  go  i  to  +  go  i,  we  have 
a  continuous  series  of  purely  imaginary  quantity, 

-  oo  i  .   .   .  -  i  .  .   .  Oi  .   .  .  +  i  .  .  .  +  cc  i  I., 

whose   unit  is  i,  and  which  corresponds  to   the   series   of  real 
quantity, 

-co   ..   .-1.   .   .0.   .   .  +  1..   .  +  oo  II., 

whose  unit  is  1. 

No  quantity  of  the  series  I.  (except  Oi)  can  be  equal  to  any 
quantity  of  the  series  II.,  for  the  square  of  any  real  multiple  of  ?', 
say  yi,  is  y2i2  =  y2(  -  1)  =  -if,  that   is,   is  a   negative  quantity. 


222         FUNDAMENTAL  CHAKACTER  OF  COMPLEX  NUMBERS      chap. 


Hence  no  purely  imaginary  quantity  except  Oi  can  be  equal  to  a  real 
quantity.  Since  Oi  =  (  +  a  -  a)i  =  +  (ai)  -  (ai)  =  0,  if  the  same 
laws  are  to  apply  to  imaginary  as  to  real  quantity,  Ave  infer  that 
Oi  =  0.  Hence  0  is  the  middle  value  of  the  series  of  purely 
imaginary,  just  as  it  is  of  the  series  of  real  quantity ;  it  is,  in 
fact,  the  only  quantity  common  to  the  two  series. 

Conversely,  if  yi  =  0,  we  infer  that  y  =  0.  For,  since  yi  =  0, 
yixyi  =  0,  that  is,  -  y*  =  0 ;  hence  y  =  0. 

§  2.1  If  we  combine,  by  addition,  any  real  quantity  x  with  a 
purely  imaginary  quantity  yi,  there  arises  a  mixed  quantity  x  +  yi, 
to  which  the  name  complex  number  is  applied. 

We  may  consider  the  infinite  series  of  complex  numbers 
formed  by  giving  all  possible  real  values  to  x,  and  all  possible 
real  values  to  y.  We  thus  have  a  doubly  infinite  series  of  com- 
plex quantity.  The  student  should  note  at  the  outset  this  double 
character  of  complex  quantity,  on  account  of  the  contrast  which 
thus  arises  between  purely  real  or  purely  imaginary  quantity 
on  the  one  hand,  and  complex  quantity  on  the  other.  Thus  there 
is  only  one  way  of  varying  z  continuously  (without  repetition  of 
intermediate  values)  from  -  1  to  +  2,  say,  if  z  is  to  be  always 
real ;  and  only  one  way  of  varying  z  in  like  manner  from  -  i  to 
+  2i,  if  z  is  to  be  always  purely  imaginary.  But  there  are  an 
infinite  number  of  ways  of  varying  z  continuously  from  -1+4 
to  2  +  3i,  say,  if  there  be  no  restriction  upon  the  nature  of  z, 
except  that  it  is  to  be  a  complex  number. 

This  will  be  best  un- 
derstood if  we  adopt 
the  diagrammatic  method 
of  representing  complex 
numbers  introduced  by 
Argand. 

Let    XOX',    YOY'    be 
two  rectangular  axes.   We 
shall  call  XOX'  the  axis  of 
Fig.  i.  real   quantity,  or  z-axis  ; 

and  YOY'  the  axis  of  purely  imaginary  quantity,  or  y-axis.     To 


xil  argand's  diagram  223 

represent  any  complex  number  x  +  yi  we  measure  from  0  (called 
the  origin)  a  distance  OM,  containing  x  units  of  length,  to  the 
right  or  left  according  as  x  is  positive  or  negative ;  and  we  draw 
MP,  containing  y  units  of  length,  upwards  or  downwards  accord- 
ing as  y  is  positive  or  negative.  The  point  P,  or,  as  is  more 
convenient  from  some  points  of  view,  the  "  radius  vector  "  OP,  is 
then  said  to  represent  the  complex  number  x  +  yi.  It  is  obvious 
that  to  every  conceivable  complex  number  there  corresponds  one 
and  only  one  point  in  the  plane  of  XX'  and  YY' ;  and,  conversely, 
that  to  every  one  of  the  doubly  infinite  series  of  points  in  that 
plane  there  corresponds  one  and  only  one  complex  number.  P 
is  often  called  the  ajfixe  of  x  +  yi,  or  simply  the  "  Point  x  +  yi." 

If  P  lie  on  the  axis  XX',  then  y  =  0,  and  the  number  x  +  yi  is 
wholly  real.  If  P  lie  on  the  axis  YY',  then  x  =  0,  and  x  +  yi  is 
wholly  imaginary.  Now  there  is  only  one  way  of  passing  from 
any  point  on  XX'  to  any  other  point,  if  we  are  not  to  leave  the 
axis,  namely,  we  must  pass 
along  the  rr-axis  ;  and  the 
same  is  true  for  the  axis  YY'. 
If,  however,  we  are  not  re- 
stricted as  to  our  path,  there 
are  an  infinity  of  ways  of 
passing  from  one  point  in  the    X'  O 

plane  of  XX'  and  YY'  to  any 
other  point  in  the  same  plane.  Y 

If  we  draw  any  continuous  Fio-  - 

curve  whatever  from  P  to  Q,  and  imagine  a  point  to  travel  along 
it  from  P  to  Q,  the  value  of  x  corresponding  to  the  moving  point 
will  vary  continuously  from  the  value  OM  to  the  value  ON,  and 
the  value  of  y  in  like  manner  from  MP  to  NQ.  Hence  there  are 
as  many  ways  of  varying  x  +  yi  from  OM  +  MPi  to  ON  +  NQi  as 
there  are  ways  of  drawing  a  continuous  curve  from  P  to  Q. 

Similar  remarks  apply  when  P  and  Q  happen,  as  they  may 
in  particular  cases,  to  be  both  on  the  x-axis,  or  both  on  the 
y-axis,  provided  that  there  is  no  restriction  that  the  varying 
quantity  shall  be  always  real  or  always  imaginary.     There  are 


Q 


PM  QN 


224  RATIONAL  OPERATIONS  WITH  COMPLEX  NUMBERS       CHAi'. 

many  other  properties  of  complex  numbers,  which  are  best  under- 
stood by  studying  Argand's  diagram,  and  we  shall  return  to  it 
again  in  this  chapter.  In  the  meantime,  however,  to  prevent 
confusion  in  the  mind  of  the  reader,  we  shall  confine  ourselves 
for  a  little  to  purely  analytical  considerations. 

§  3.]  If  x  +  yi  =  0,  then  x  =  0,  y  =  0.*  For  it  follows  from 
x  +  yi  =  0  that  x  =  -  yi.  Hence,  if  y  did  not  vanish,  we  should 
have  a  real  quantity  x  equal  to  a  purely  imaginary  quantity  -  yi, 
which  is  impossible.  We  must  therefore  have  y  =  0  ;  and  conse- 
quently x—  -  Oi  =  0. 

Cor.  Hence  if  x  +  yi  =  x  +  y'i,  then  must  x  =  x  and  y  =  y . 

For  x  +  yi  =  x'  +  y'i  gives,  if  we  subtract  x  +  y'i  from  both  sides, 
(x  —  x)  +  (y  —  y')i  =  0. 
Hence  x  —  x'  —  0,     y  —  jf  =  0, 

that  is,  x  =  x',  y  =  y'. 

RATIONAL   FUNCTIONS    OF   COMPLEX    NUMBERS. 

§  4.]  We  have  seen  that  so  long  as  we  operate  upon  real 
quantities,  provided  we  confine  ourselves  to  the  rational  opera- 
tions— addition,  subtraction,  multiplication,  and  division,  we 
reproduce  real  quantities  and  real  quantities  only.  On  the 
other  hand,  if  we  use  the  irrational  operation  of  root  extraction, 
it  becomes  necessary,  if  we  are  to  keep  up  the  generality  of 
algebraical  operations,  to  introduce  the  imaginary  unit  i.  We  are 
thus  led  to  the  consideration  of  complex  numbers.  The  ques- 
tion now  naturally  presents  itself,  "  If  we  operate,  rationally  or 
irrationally,  in  accordance  with  the  general  laws  of  algebra  on 
quantities  real  or  complex  as  now  defined,  shall  we  always  re- 
produce quantities  real  or  complex  as  now  defined  ;  or  may  it 
happen  that  at  some  stage  it  will  be  necessary  in  the  interest  of 
algebraic  generality  to  introduce  some  new  kind  of  imaginary 
quantity  not  as  yet  imagined  1 "  The  answer  to  this  question 
is  that,  so  far  at  least  as  the  algebraical  operations  of  addition, 

*  Here  and  hereafter  in  this  chapter,  when  we  write  the  form  x  +  yi,  it  is 
understood  that  this  denotes  a  complex  number  in  its  simplest  form,  so  that 
x  and  y  are  real. 


XII  RATIONAL  FUNCTIONS  OF  COMPLEX  NUMBERS  225 

subtraction,  multiplication,  division,  and  root  extraction  are 
concerned,  no  further  extension  of  the  conception  of  algebraic 
quantity  is  needed.  It  is,  in  fact,  one  of  the  main  objects  of  the 
present  chapter  to  prove  that  algebraic  operations  on  complex 
numbers  reproduce  only  complex  numbers. 

§  5.]  The  sum  or  product  of  any  number  of  complex  numbers,  and 
the  quotient  of  two  complex  numbers,  may  be  expressed  as  a  complex 
number. 

Suppose  we  have,  say,  three  complex  numbers,  a;,  +  yj,,  x2  +  y2i, 
x3  +  y3i,  then 

(«i  +  ffii)  +  (x2  +  y2i)  -  (x3  +  y3i)  =  (.r,  +  x2-  x3)  +  (y,  +  y2  -  y3)i, 
by  the  laws  of  algebra  as  already  established. 

But  xl  +  x2  -  x3  and  yx  +  y2  -  y3  are  real,  since  xx,  x2,  x3,  yx,  y2,  y3 
are  so.  Hence  (#,  +  x,2  -  x3)  +  (yx  +y2-  y3)i  is  in  the  standard  form 
of  a  complex  number.  The  conclusion  obviously  holds,  however 
many  terms  there  may  be  in  the  algebraic  sum. 

Again,  consider  the  product  of  two  complex  numbers,  xx  +  yj, 
and  x2  +  yj.     We  have,  by  the  law  of  distribution, 

(«i  +  yd)  («» +  yd)  =  x&i  +  y<ij£  +  w  +  <w- 

Hence,  bearing  in  mind  the  definition  of  i,  we  have 

(a  +  yd)  (-r2  +  yj)  =  to  -  ysj»)  +  to  +  «Wi)i, 

which  proves  that  the  product  of  two  complex  numbers  can  be 
expressed  as  a  complex  number. 

To  prove  the  proposition  for  a  product  of  three  complex 
numbers,  say  for 

P  =  (.r,  +  yj)  (x,  +  yj)  (x3  +  y3i), 

Me  have  merely  to  apply  the  law  of  association,  and  write 

P  =  {(»i  +  yj)  («s  +  yd)}  («3  +  yd). 

We  have  already  shown  that  the  function  within  the  crooked 
brackets  reduces  to  a  complex  number ;  hence  P  is  the  product 
of  two  complex  numbers.  Hence,  again,  by  what  we  proved 
above,  P  reduces  to  a  complex  number.  In  this  way  we  can 
extend  the  theorem  to  a  product  of  any  number  of  complex 
numbers. 

VOL.  I  Q 


226  RATIONAL  FUNCTIONS  OF  COMPLEX  NUMBERS  chap. 

Lastty,  consider  the  quotient  of  two  complex  numbers.     We 
have 

Si  +  ffii  _  («i  +  yj)  («» -  yJ)  * 
x3  +  y2i  (x2f  -  (y2if     ' 

=  (^gg  +  vm)  -  fay»  -  %2!ti)i 
a*  +  y* 

xxx2  +  y^/nX      f^iV-i  ~ 


2 

Xo    t  y^     /  \   *^2    "■" 


— S~  ]' 

y2  / 


This   proves   that   the   quotient   of  two   complex  numbers   can 
always  be  reduced  to  a  complex  number. 

Cor.  1 .  Since  every  rational  function  involves  only  the  opera- 
tions  of   addition,    subtraction,   multiplication,   and  division,  it 
follows    from   what    has    just   been    shown    that    every   rational 
function  of  one  or  more  complex  numbers  can  be  reduced  to  a  com- 
plex number. 

Cor.  2.  If  <f>(x  +  yi)  be  any  rational  function  of  x  +  yi,  having  all 
its  coefficients  real,  and  if 

<j)(z  +  yi)  =  X  +  Yi, 
then 

<f>(x  -  yi)  =  X  -  Yi, 

X  and  Y  being  of  course  real. 

Cor.  3.  Still  more  generally,  if  <£(»,  +  yj,  x2  +  y2i,  .  .  .  ,  xn  +  yni) 
be  any  rational  function  of  n  complex  numbers,  having  all  its  coefficients 
real,  and  if 

4>{x,  +  yti,     x2  +  y2i,     .  .  .  ,     xn  +  yni)  =  X  +  Yi, 

then 

^{x.-y.i,     x2-y2i,     .  .  .  ,     xn-y,li)  =  X-Yi. 

Cor.  4.  If  all  the  coefficients  of  the  integral  function  <j>(z)  be 
reed,  and  if  cj>(z)  vanish  when  z  =  x  +  yi,  then  <f>(z)  vanishes  wlien 
z  =  x-yi. 

'  Here  we  perform  an  operation  which  we  might  describe  as  "realising" 
the  denominator  ;  it  is  analogous  to  the  process  of  rationalising  described  in 
chap.  x. 


xir  EXAMPLES  227 

For,  by  Cor.  1,  <f>(x  +  yi)  =  X  +  Yi  where  X  and  Y  are  real. 
Hence,  if  cf>(x  +  yi)  =  0,  we  have  X  +  Yi  =  0.  Hence,  by  §  3,  X  =  0 
and  Y  =  0.     Therefore  <j>(x  -  yi)  =  X  -  Yi  =  0  -  0/  =  0. 

Cor.  5.  If  all  the  coefficients  of  the  integral  function  <£(2„ 
zs,  .  .  .  ,  zn)  be  real,  and  if  the  function  vanish  when  zu  z.,,  .  .  . ,  zn 
are  equal  to  xx  +  yj,,  x2  +  y2i,  .  .  . ,  xn  +  yni  respectively,  then  the 
function  will  also  vanish  when  su  z.2,  .  .  .  ,  zn  are  equal  to  xx  -  yxi, 
xs  -  yi1,  '  •   ■  j  xn  -  Vni  respectively. 

Example  1. 

3(3  +  20  -  2(2  -  3i)  +  (6  +  80  =  9  +  6i-  4  +  6J+6+  Si, 

til  +  2Qi. 
Example  2. 

(2  +  30  (2  -  50  (3  +  20  =  (2  -  50  (6  -  6  +  9i  +  40, 
=  (2 -5013;', 
=  26i  +  65, 
=  65  +  26i. 
Example  3. 

(b  +  c  -  ai)  [c  +  a  -  bi)  (a  +  b-  ci) 

=  {U(b  +  c)-2bc(b  +  c)\  +  {abc-Za{a  +  b){a  +  c)}i, 

-  2abc  +  {abc  -  2a3  -  2a2(6  +  c)  -  Zabc}  i, 

—  2abc  -  {a3  +  b3  +  c3  +  (b  +  c)  [c  +  a)  {a  +  b)}  i. 
Example  4. 

To  show  that  the  values  of  the  powers  of  i  recur  in  a  cycle  of  4. 

We  have  i=i,  i2=-l,      i3  =  i2xi=  -i,        ii=(i~)-=+l! 

is=i4  x  i  =  i,     i6  =  i4  x  i-=  -  1,     i7  =  i4  x  i3—  -  i,     i8  =  {4  x  i4=  +  1  ; 

and,  in  general, 

i4n+l=i}  i*H-2=-l,  $*"+•=  -t,  l'4("+1)=+l. 

Example  5. 

3  +  5i_(3  +  5Q(2  +  3Q_6-15  +  19i_      9      19. 

2-3i~  4  +  9  13  13  +  13*' 

Example  6. 

(x  +  yi)"  =  x"  +  „Ci  xn~Hyi)  +  „C2  8»-2(yi)a  +  •   •   • . 

=(.?;«-, a z"-v2+»c.iz"-y-.  •  ■) 

+  (nC1x»-1y-nC3xn-3y3  +  „C5xn-hj5-.  .   .)*■ 

In  particular 

(jb  +  yt)*={a?  -  Sx-y°  +  2/4)  +  (4afy  -  to*/8)*. 
Example  7. 

If  <p(z)  =  Z" ' 


then  «/>(2  + 30 : 


'z-  +  z  +  V 
(2  +  3Q2-(2  +  3Q  +  l 

:"(2  +  302  +  (2  +  30  +  l' 
-5  +  12t-2-3i  +  l 
-5  +  12i  +  2  +  3i+l' 


228  CONJUGATE  COMPLEX  NUMBERS  CHAP. 

_j-6  +  9i  _3(-2  +  3Q(-2-15Q 
-2  +  15i~  229 

=  2§9{4  +  45_6'+30^' 
_U7     _72  . 
229    229  *' 
From  this  we  infer  that 

,.,     ...     147      72  . 
^(2-3l)  =  229-229i; 
a  conclusion  which  the  student  should  verify  by  direct  calculation. 

CONJUGATE   COMPLEX    NUMBERS,    NORMS,    AND   MODULI. 

§  6.]  Two  complex  numbers  which  differ  only  in  the  sign 
of  their  imaginary  part  are  said  to  be  conjugate.  Thus  —  3  —  2i 
and  -  3  +  2t  are  conjugate,  so  are  -  ii  and  +  ii ;  and,  generally, 
x  +  yi  and  x  -  yi. 

Using  this  nomenclature  we  may  enunciate  Cor.  3  of  §  5 
as  follows  : — 

If  the  coefficients  of  the  rational  function  <£  be  real,  then 
the  values  of 

4fa  +  yj,     x2  +  y.j,     .  .   .,     xn  +  yni) 

and  </>('ri-*/A     «»-yA     ■  •   •,     -rn  ~  ?/n0> 

where  the  values  of  the  variables  are  conjugate,  are  conjugate 

complex  numbers. 

The  reader  will  readily  establish  the  following : — 

The  sum  and  the  product  of  two  conjugate  complex  numbers  are  real. 

Conversely,  if  both  the  sum  and  the  product  of  two  complex  numbers 
be  real,  then  either  both  are  real  or  they  are  conjugate. 

§  7.]  By  the  modulus  of  the  complex  number  x  +  yi  is  meant 
+   J(x2  +  y2).     This  is  usually  denoted  by  |  x  +  yi  \* 

It  is  obvious  that  a  complex  number  and  its  conjugate  have  the 
same  modulus;  and  thai  this  modulus  is  the  positive  value  of  the 
square  root  of  their  product. 

Examples. 

|-3  +  4i|=+N/{(-3)2M2}=5. 
|-3-4;|=  +  v/{(-3)2  +  (-4)2}=5. 

|l+i|=  +  v/(l2+l2)=v/2.  

*  Formerly  by  mod  {x  +  yi). 


XII 


MODULI  229 


It  should  be  noticed  that  if  y  =  0,  that  is,  if  the  complex 
number  be  wholly  real,  then  the  modulus  reduces  to  +  Jx2, 
which  is  simply  the  value  of  x  taken  with  the  positive  sign,  or, 
say,  the  numerical  value  of  x.  For  example,  |  -  3  |  =  +  \/(  -  3)2 
=  +  3.  For  this  reason  Continental  writers  frequently  use  |  x  | 
where  x  is  a  real  quantity,  as  an  abbreviation  for  "  the  numerical 
value  of  SB."  We  shall  occasionally  make  use  of  this  convenient 
contraction. 

For  reasons  that  will  be  understood  by  referring  once  more  to  §  2,  the 
ordinary  algebraical  ideas  of  greater  and  less  which  apply  to  real  quantities 
cannot  be  attached  to  complex  numbers.  The  reader  will,  however,  find  that 
for  many  purposes  the  measure  of  the  "  magnitude  "  of  a  complex  number  is 
its  modulus.  We  cannot  at  the  present  stage  explain  precisely  how  "magni- 
tude" is  here  to  be  understood,  but  we  may  remark  that,  in  Argand's  diagram, 
the  representative  points  of  all  complex  numbers  whose  moduli  are  less  than 
p  lie  within  a  circle  whose  centre  is  at  the  origin  and  whose  radius  is  p. 

§  8.]  If  a  complex  number  vanish  its  modulus  vanishes ;  and, 
conversely,  if  the  modulus  vanish  the  complex  number  vanishes. 

For  if   x  +  yi  =  0,  then  by  §   3,  x  =  0   and  y  =  0.       Hence 
*J(x*  +  f)  =  0.  ' 

Again,  if  J(x"  +  y2)  =  0,  then  x2  +  y2  -  0  ;  but,  since  both  x 
and  y  are  real,  both  x2  and  y2  are  positive,  hence  their  sum  cannot 
be  zero  unless  each  be  zero.     Therefore  x  =  0  and  y  =  0. 

If  two  complex  numbers  are  equal  their  moduli  are  equal ;  but  the 
converse  is  not  true. 

For,  if  x  +  yi  =  x'  +  y'i,  then,  by  §  3,  x  =  x\  y  =  y.      Hence 
J(x2  +  f)  =  V(x'3  +  y'2). 

On    the    other   hand,    it    does    not    follow    from    J(x2  +  y2) 
=  J(x'2  +  y'2)  that  x  =  x',  y=-  y.     Hence  the  converse  is  not  true. 
§  9.]  Provided  all  the  coefficients  in  <£(x'  +  yi)  be  real,  we  have 
seen  (§  5,  Cor.  2)  that  if 

<p(x  +  yi)  =  X  +  Yi, 
where  X  and  Y  are  real,  then 

c/,(.c  -  yi)  =  X  -  Yi. 
Now      \cf>(x  +  yi)\=  v/(X2  +  Y2)=   J{(X  +  Yi)(X-Yi)}, 

=  J{<f>(x  +  yi)     <}>(x-yi)}, 


230  MODULI 


CHAP. 


In  like  manner  it  follows  from  §  5,  Cor.  3,  that 

I  <t>fa  +  yj,    %a  +  thh    •  ■  ■,    xn  +  yd)  | 

=  I  <M«i  -  Vih     x,  -  yj,     .   .  .,     xn  -  yni)  \ 
=  +  s/[<i>{xx  +  yxi,     x2  +  y2i,     .  .  .,     xn  +  yj) 

x  <f>(Xl  -  y,i,     x2  -  yj,     .   .  .,     xn  -  yni)]  (2). 

The  theorems  expressed  by  (1)  and  (2)  are  very  useful  in 
practice,  as  will  be  seen  in  the  examples  worked  below. 

It  should  be  observed  that  (1)  contains  certain  remarkable 
particular  cases.     For  example, 

I  («!  +  yj)  fa  +  yd)  •  •  •  fa  +  yj)  I 

=  +  ^[(jc,  +  yj)  (x2  +  yj)  .  .  .  fa  +  yni) 

*  (gi  -  yj)  fa  -  yai)  •  •  •  fa  -  yj)\ 

=  +  Vfa  +  y?)  fa  +  y2)  .  .  .  (xn2  +  yn2), 

=  I  fc  +  yj)  I x  I  fa  +  yd)  I x  •  •  •  x  I  fa  +  yj)  I       (3). 

In  other  words,  the  modulus  of  the  'product  of  n  complex  numbers 
is  equal  to  the  product  of  their  moduli. 
Also 


g,  +  yj> 

x2  +  y2i 


=  \/fa*  +  y.2)  _  ( g.  +  yj  1 

"  \/(x2+y22)     \x2  +  y2i\  (4). 


In  other  words,  the  modulus  of  the  quotient  of  two  complex  numbers 
is  the  quotient  of  their  moduli. 

§  10.]  The  reader  should  establish  the  results  (3)  and  (4)  of 
last  paragraph  directly. 

It  may  be  noted  that  we  are  led  to  the  following  identities  : — 

fa  +  y?)  fa  +  y.f)  =  fac,  -  yfo)'  +  {x,y2  +  ay/,)2. 

If  we  give  to  x„  yu  x2,  y2  positive  integral  values,  this  gives  us 
the  proposition  that  the  product  of  hoo  integers,  each  of  which  is  the 
sum  of  two  square  integers,  is  itself  the  sum  of  two  square  integers ; 
and  the  formula  indicates  how  one  pair  of  values  of  the  two 
integers  last  mentioned  can  be  found. 

Also 

fa2  +  y?)  fa2  +  y2)  fa  +  y.*)  =  zflp,  -  x,yjj3  -  xjj,y,  -  x^y,)* 

+  (yiWe  +  y&&i  +  y<FiXe  -  2W3)2- 


XII 


MODULI  231 


This  shows  that  the  product  of  three  sums  of  two  integral  squares 
is  the  sum  of  two  integral  squares,  and  shows  one  way  at  least  of 
finding  the  two  last-mentioned  integers. 

Similar  results  may  of  course  be  obtained  for  a  product  of 
any  number  of  factors. 

Example  1. 

Find  the  modulus  of  (2  +  3i)  (3  -  2i)  (6  -  4i). 
|(2  +  8i)(3-2i)(6-4t)| 

=|(2+3*)[x|(3-2*)[x|(6-4i)|> 

=  sf\lZ)x  ^(13)  x  ^(52), 

=26^/(13). 
Example  2. 
Find  the  modulus  of  ( ^2  +  ^3)  (-s/3  +  »  V5)/(V2  +  W&)- 

(v/2  +  rV3)(V3  +  tV5)| 

/r /( v/2  +  iv/3)(V3  +  ^v/5)\      r(N/2-W3)(x/3-i\/5)\-| 
=  VLl"  >/2  +  iV5  J      l  V2-W5  <U' 

-  V[(?±l^]=  7(f)- 

Example  3. 

Find  the  modulus  of  {(/3  +  7)  +  (/3  -  7)1}  {(7  +  a)  +  (7  -  a) i}  {(a  +  /3)  +  (a  -  /3)i} . 
The  modulus   is    J({((H-yT  +  (P-y)-}  {(y  +  *?  +  {y-a.f\  {(a  +  (3f  +  (a- p)*}) 
=  v/{8(^  +  72)(72+a2)(a2  +  ^)}. 
Example  4. 

To  represent  26  x  20  x  34  as  the  sum  of  two  integral  squares. 
Using  the  formula  of  §  10  we  have 
26  x  20  x  34  =  (l2+52)  (22  +  42)  (32  +  52), 

=  (1.2.3  -1.4.5-  2.5.5  -3.5.4)2  +  (5.2.3  +  4.3.1  +  5.1.2  -5.4.5)2, 
=  1242  +  482. 

§11.]   The  modulus  of  the  sum  of  n  complex  numbers  is  never 
greater  than  the  sum  of  their  moduli,  and  is  in  general  less. 

This  may  be  established  directly ;  but  an  intuitive  proof  will 
be  obtained  immediately  from  Argand's  diagram. 

§  12.]  We  have  seen  already  that,  when  PQ  =  0,  then  either 
P  =  0  or  Q  =  0,  provided  P  and  Q  be  real  quantities.  It  is 
natural  now  to  inquire  whether  the  same  will  hold  if  P  and  Q 
be  complex  numbers. 

If  P  and  Q  be  complex  numbers  then  PQ  is  a  complex 
number.  Also,  since  PQ  =  0,  by  §  8,  |  PQ  |  =  0.  But  |  PQ  | 
=  |pi*IQI»  by  §   10-      Hence   |P|xIQI  =  0.      Now   |P|  and 


232  argand's  DIAGRAM  chap. 

I  Q  |  are  both  real,  hence  either  |  P  |  =  0  or  |  Q  |  =  0.  Hence,  by 
§  8,  either  P  =  0  or  Q  =  0. 

We  conclude,  therefore,  that  if  PQ  =  0,  then  either  P  =  0  or 
Q  =  0,  whether  P  and  Q  be  real  quantities  or  complex  numbers. 

discussion  of  complex  numbers  by  means  of 
argand's  diagram. 

§  13.]  Returning  now  to  Argand's  diagram,  let  us  consider 
the  complex  number  x  +  yi,  which  is  represented  by  the  radius 
vector  OP  (Fig.  1).  Let  OP,  which  is  regarded  as  a  signless 
magnitude,  or,  what  comes  to  the  same  thing,  as  always  having 
the  positive  sign,  be  denoted  by  r,  and  let  the  angle  XOP, 
measured  counter-clock-wise,  be  denoted  by  6. 

We  have  seen  that  if  OP  represent  x  +  yi,  then  x  and  y  are 
the  projections  of  r  on  X'OX  and  Y'OY  respectively.  Hence 
we  have,  by  the  geometrical  definitions  of  cos  6  and  sin  9, 

r=  +  V(r  +  /)  (1), 

x/r-cos$,     y/r  =  sin  d,  (2). 

From  (1)  it  appears  that  r,  that  is  OP,  is  the  modulus  of  the 
complex  number.  The  equations  (2)  uniquely  determine  the 
angle  6,  provided  we  restrict  it  to  be  less  than  2ir,  and  agree 
that  it  is  always  to  be  measured  counter-clock- wise  from  OX.* 
We  call  6  the  amplitude  of  the  complex  number.  It  follows 
from  (2)  that  every  complex  number  can  be  expressed  in  terms 
of  its  modulus  and  amplitude  ;  for  we  have 

x  +  yi  =  r(cos  6  +  i  sin  6)  (3). 

This  new  form,  which  we  may  call  the  normal  form,  possesses 
many  important  advantages. 

*  Sometimes  it  is  more  convenient  to  allow  8  to  increase  from  -  ir  to  +  w  ; 
that  is,  to  suppose  the  radius  OP  to  revolve  counter-clock-wise  from  OX'  to 
OX'  again.  In  either  way,  the  amplitude  is  uniquely  determined  when  the 
coefficients  x  and  y  of  the  complex  number  are  given,  except  in  the  case  of  a 
real  negative  number,  where  the  amplitude  apart  from  external  considera- 
tions is  obviously  ambiguous. 


XII 


COMPOSITION    OF    VECTORS 


233 


Since  two  conjugate  complex  numbers  differ  only  in  the  sign 
of  the  coefficient  of  i,  it  follows 
that  the  radii  vectores  which  re- 
present them  are  the  images  of 
each  other  in  the  axis  of  x  (Fig.  3). 
Hence  two  such  have  the  same 
modulus,  as  we  have  already  shown 
analytically  ;  and,  if  the  amplitude 
of  the  one  be  6,  the  amplitude  of 
the  other  will  be  2tt  -  6.  In  other 
words,  the  amplitudes  of  two  con- 
jugate complex  numbers  are  con- 
jugate angles. 


Example. 


-1-i=V2("^2-^')  =  V2(C0ST  +  l'sinT)- 


§  14.]  If  OP,  OQ'  (Fig.  4)  represent  the  complex  numbers 

Y 

Q -,Q 


x  +  yi     and     x'  +  y'i,     and     if 
— > 
PQ  be  drawn  parallel  and  equal 


to  OQ',  then  OQ  will  represent 
the   sum   of   x  +  yi    and    x'  +  y'i. 

For  the  projection  of  OQ  on  the 
z-axis  is  the  algebraic  sum  of  the 


Yi 

I'lii.  4. 


projections  of  OP  and  PQ  on  the 
— > 
same  axis,  that  is  to  say,  the  projection  of  OQ  on  the  a-axis  is 

— > 
x  +  x.     Also  the  projection  of  OQ  on  the  y-axis  is,  by  the  same 
reasoning,  y  +  y'.      Hence  OQ  represents   the   complex  number 
(x  +  x)  +  (y  +  y')i,  which  is  equal  to  (x  +  yi)  +  (x'  +  y'i). 

By  similar  reasoning  we  may  show  that  if  OP„  OP2,  OP3,  OP4, 

OP5,  say,  represent  five  complex  numbers,  and  if  P,Q,  be  parallel 


234 


|  2i  +  Z3  + 


+  Zn\< 


+ 


+    \Zm 


CHAP. 


and  equal  to  0P2,  Q2Q3,  parallel  and  equal  to  0P3,  and  so  on,  then 
0Q5  represents  the  complex  number  which  is  the  sum  of  the 
complex  numbers  represented  by  OP,,  OP„,  OP3,  OP4,  OP5. 

This  is  precisely  what  is  known  as  the  polygon  law  for  com- 
pounding vectors.  Since  OQ5  is  never  greater  than  the  peri- 
meter OPjQ.jQaQ.jQs,  and  is  in  general  less,  Fig.  5  gives  us  an 
intuitive  geometrical  proof  that  the  modulus  of  a  sum  of  complex 
numbers  is  in  general  less  than  the  sum  of  their  moduli.  It  is 
equally  obvious  from  Fig.  4  that  the  modulus  of  the  sum  of  two  com- 


Fig.  5. 


plex  numbers  is  in  general  greater  than  the  difference  of  the  moduli. 
"  Sum  of  complex  numbers  "  in  these  theorems  means,  of  course, 
algebraic  sum. 

§  15.]  If  we  employ  the  normal  form  for  a  complex 
number,  and  work  out  the  product  of  two  complex  numbers, 
r,(cos  0,  +  i  sin  0:)  and  rt(cos  92  +  i  sin  02),  we  have 

r^cos  0,  +  i  sin  0])r»(cos  92  +  i  sin  B2) 

=  r,ra{(cos  0,  cos  6.2  -  sin  0,  sin  $,)  +  (sin  0,  cos  6.2  +  cos  9^  sin  92)i), 
=  r,r2{cos  (0,  +  02)  +  i  sin  (0,  +  9.2)}  (1). 

We  thus  prove  that  the  product  of  two  complex  numbers  is  a 
complex  number,  whose  modulus  r{r2  is  the  product  of  the  moduli 


xii  demoivre's  theorem  235 

of  the  two  numbers,  a  result  already  established ;  and  we  have 
the  new  theorem  that  the  amplitude  of  the  product  is,  to  a  multiple 
of  2tt,  the  sum  of  the  amplitudes  of  the  factors.  For  we  can  always 
find  an  angle  <£  lying  between  0  and  2rr,  such  that  cos  <f>  = 
cos  (0,  +  02)  and  sin  (f>  -  sin  {dx  +  02),  and  we  then  have  6Y  +  63 
=  2mr  +  cf>. 

This  last  result  is  clearly  general ;  for,  if  we  multiply  both 
sides  of  (1)  by  an  additional  factor,  r3(cos  03  +•  i  sin  03),  we  have 

r^cos  Qx  +  i  sin  01)r2(cos  0„  +  i  sin  02)r3(cos  03  +  i  sin  03) 

=  r^cos  (0,  +  62)  +  i  sin  (0t  +  62)}  r3(cos  63  +  i  sin  $3), 
=  rtr2r3{cos  ($x  +  d2+  d3)  +  i  sin  (01  +  62  +  03)}, 

by  the  case  already  proved, 

=  ?W3{cos  (0,  +  B2  +  93)  +  i  sin  (0:  +  02  +  03)}. 
Proceeding  in  this  way  we  ultimately  prove  that 

r,(cos  $!  +  i  sin  tf^r^cos  02  +  i  sin  02)  .  .  .  rn(cos  9n  +  i  sin  6n) 

=  r{r2 . .  .  ?-n{cos(#!  +  02  +  . .  .  +  9n)  +  i  sin(#,  +  62  +  .  . .  +  6n)}  (2). 

This  result  may  be  expressed  in  words  thus — 

The  pvduct  of  n  complex  numbers  is  a  complex  number  whose 
modulus  is  the  product  of  the  moduli,  and  whose  amplitude  is,  to  a 
multiple  of  2ir,  the  sum  of  the  amplitudes  of  the  n  complex  numbers. 

If  we  put  rl  =  r2  =  .  .  .  =  rn,  each  =  1  say,  we  have 

(cos  #!  +  i  sin  0j)  (cos  #3  +  i  sin  62)  .  .  .  (cos  6n  +  i  sin  dn) 

=  cos  (6,  +  62  +  .  .  .  +  0tl)  +  i  sin  (0,  +  02  + .  .  .  +  6n)   (3). 

This  is  the  most  general  form  of  what  is  known  as  Demoivre's 
Theorem. 

If  we  put  0,  =  62  -  .   .  .  -  6n,  each  =  0,  then  (3)  becomes 
(cos  0  +  i  sin  0)n  =  cos  nd  +  i  sin  nd  (4), 

which  is  the  usual  form  of  Demoivre's  Theorem.*     It  is  an  analy- 
tical result  of  the  highest  importance,  as  we  shall  see  presently. 

*  This  theorem  was  first   given   in  Demoivre's  Miscellanea  Analytica 
(Lond.  1730),  p.  1,  in  the  form 

^  =  i\/{^  +  \/(^-l)}+i/\/{^+v'(^-l)},  where  ar  =  cos0,  f  =  cos«0. 


236  QUOTIENT  OF  COMPLEX  NUMBERS  CHAP. 

Since  cos  0  -  i  sin  0  -  cos  (2r  -  0)  +  i  sin  (2ir  -  0), 

we  have,  by  (3)  and  (4), 

lT(cos  0,  -  i  sin  0,)  =  cos  (20,)  -  i  sin  (20,)  (3') ; 

and  (cos  0  -  i  sin  9)n  =  cos  n0  -  i  sin  «0  (4'). 

The  theorem  for  a  quotient  corresponding  to  (1)  may  be 
obtained  thus — 

r(cos  0  +  i  sin  0)  _  r(cos  0  +  i  sin  0)  (cos  0'  -  i  sin  0') 
/(cos  0'  +  i  sin  0')  =  r'(cos  20'  +  sin  a0')  ' 

=  -  {(cos  0  cos  0'  +  sin  0  sin  0') 

+  (sin  0  cos  0'  -  cos  0  sin  0')i}, 

=  -,  {cos  (0  -  0)  +  *  sin  (0  -  $')}  (5). 

Hence  $e  quotient  of  two  complex  numbers  is  a  complex  number 
ichose  modulus  is  the  quotient  of  the  moduli,  and  whose  amplitude  is 
to  a  multiple  of  2ir  the  difference  of  the  amplitude  of  the  two  complex 
numbers. 

IRRATIONAL   OPERATIONS    WITH   COMPLEX    NUMBERS. 

§  16.]  Since  every  irrational  algebraical  function  involves 
only  root  extraction  in  addition  to  the  four  rational  operations, 
and  since  we  have  shown  that  rational  operations  with  complex 
numbers  reproduce  complex  numbers  and  such  only,  if  we  could 
prove  that  the  nth.  root  of  a  complex  number  has  for  its  value, 
or  values,  a  complex  number,  or  complex  numbers  and  such  only, 
then  we  should  have  established  that  all  algebraical  operations 
with  complex  numbers  reproduce  complex  numbers  and  such 
only. 

The  chief  means  of  arriving  at  this  result  is  Demoivre's 
Theorem  ;  but,  before  resorting  to  this  powerful  analytical  engine, 
we  shall  show  how  to  treat  the  particular  case  of  the  square  root 
without  its  aid. 

Let  us  suppose  that 

J(x  +  yi)  =  X  +  Yi  (1). 


xii  SQUARE  ROOTS  OP  A  COMPLEX  NUMBER  237 

Then  x  +  yi  =  X2-Y2+2XYi. 

Hence,  since  X  and  Y  are  real,  we  must  have,  by  §  3, 

X2-Y2  =  .x  (2), 

2XY  =  y  (3). 

Squaring  both  sides  of  (2)  and  (3),  and  adding,  we  deduce 

(X2  +  Y2)2  =  x2  +  f  • 
whence,  since  X2  +  Y2  is  necessarily  positive,  we  deduce 

X2  +  Y2=  +  V'(/  +  /)  (4). 

From  (2)  and  (4),  by  addition,  we  derive 

2X2=  +   >J(x2  +  y2)  +  x, 

u.   v  ■                                   Y*      +  \  (x2  +  y2)  +  x 
that  is,  A  = - -• 

We  therefore  have  X=  ±  y    j 2 )      ^' 

In  like  manner  we  derive  from  (2)  and  (4),  by  subtraction,  &c, 

T.;y{±i^b'}  (6). 

Since  x2  +  y2  is  numerically  greater  than  x1,  +  ^(x2  +  y2)  is 
numerically  greater  than  x.  Hence  the  quantities  under  the  sign 
of  the  square  root  in  (5)  and  (6)  are  both  real  and  positive.  The 
values  of  X  and  Y  assigned  by  these  equations  are  therefore  real. 

Since  2XY  =  y,  like  signs  must  be  taken  in  (5)  and  (6),  or 
unlike  signs,  according  as  y  is  positive  or  negative. 

We  thus  have  finally 

(7). 

(8), 
if  y  be  negative. 

Example  1. 

Express  \/(8  +  6i)  as  a  complex  number. 

Let  ^{8  +  6i)  =  x  +  yi. 

Then  a~-i/2  =  8,     2xy=6. 

Hence  (*2  +  ?/2)2  =  64  +  36  =  100 

Hence  x!  +  if=\0; 

and  x~-y2  =  8; 


\ 


if  y  be  positive  ; 

=  ± 


238  EXAMPLES  chap. 

therefore  2x-2  =  18,     2y°  =  2. 

Hence  x=±3,      y==hl. 

Since  2a*y  =  6,  we  must  have  either  x  —  +3  and  y=+l,  or  ar=-3  and 
y=-l. 

Finally,  therefore,  we  have 

V(8  +  6i)=±(3  +  i); 
the  correctness  of  which  can  be  immediately  verified  by  squaring. 
Example  2. 

v<3-7o=±{y(»>^/(»)}. 

Example  3. 

Express  \/(  +  i)  and  \/(  ~  *)  as  complex  numbers. 
Let  \/{+i)=3:+#*; 

then  i  =  ar  -  2/2  +  2a;?/i. 

Hence  a.-2-2/2  =  0  (a),  2asy=l  (0). 

From  (a)  we  have  (x  +  y)(x-y)  =  0  ;  that  is,  either  ?/=  -a  or  y  =  x.  The 
former  alternative  is  inconsistent  with  (/3) ;  hence  the  latter  must  be  accepted. 
We  then  have,  from  (/3),  2a?=l,  whence  £2  =  l/2  and  a;=±l/\/2.  Since 
!/=£,  we  have,  finally, 

V+*=±^"  (7)- 

Similarly  we  show  that 

Example  4. 

To  express  the  4th  roots  of  + 1  and  - 1  as  complex  numbers. 

^/  +  1  =  V(V  +  1)  =  V±l  =  V  +  l  or  «s/-l  =  ±l  or  dbi. 
Hence  we  obtain  four  4th  roots  of  +  1,  namely,  +1,  -  1,  +  i,  -  i. 

Again  v  -  1  =  V(V-  l)=  V^- 

Hence,  by  Example  3, 

§  17.]  We  now  proceed  to  the  general  case  of  the  rcth  root 
of  any  complex  number,  r(cos  6  +  i  sin  6). 

Since  r  is  a  positive  number,  Vr  has  (see  chap,  x.,  §  2) 
one  real  positive  value,  which  we  may  denote  by  r1/n. 

Consider  the  n  complex  numbers — 

rVn[  cos  -  +  i  sin  -  )  (1), 

\       n  ii/  x 

2-rr+e      .    .     2tt  +  0N 

A  In  I 


(       2tt  +  9     .  .    2tt  +  9\  /t.x 

cos h  i  sin )  (2), 

\  n  n     J 


xii                       MTH  BOOTS  OF  ANY  COMPLEX  NUMBER  239 

..  /       Att  +  0      .   .    4-  +  0\  ... 

i '  "   cos +  t  sin )  (o), 

\  n  n     / 


2stt  +  6     .  .    2sir  +  8\  ,      . . 

r1'"    cos  -    +  *  sin  -         -  )  (s  +  1 ), 

n  n     J 


rVn  ( 


2(>i-l)-  +  e      .    .    2(n-  l)ir+0\  .  , 

cos  — +  %  sin  — hi). 

n  n  / 


i  rVnf 


No  two  of  these  are  equal,  since  the  amplitudes  of  any  two 
differ  by  less  than  2ir.  The  ?ith  power  of  any  one  of  them  is 
r(cos  6  +  i  sin  6) ;  for  take  the  (s  +  l)th,  for  example,  and  we  have 

2$ir  +  6     .  .    2stt  +  6 
cos +  ^  sm 

n  a 

(    ^.\n(  2STT+0         .      .       2S7T+8\n 

=  I  rxjn  )    [  cos +  i  sin 

\      /    \  n  n 

(         2sw  +  6     .  .       2S7T  +  8 

=  r  [  cos  n +  i  sin  n 

\  n  n 

by  Demoivre's  Theorem, 

=  r(cos  (25tt  +  6)  +  i  sin  (2stt  +  6) ), 

=  r(cos  0  +  i  sin  6). 

Hence  the  complex  numbers  (1),  (2),  .  .  .,  (n)  are  n  different 

nth  roots  of  r(cos  6  +  i  sin  6). 

We  cannot,  by  giving  values  to  5  exceeding  n—  1,  obtain 
any  new  values  of  the  ?tth  root,  for  the  values  of  the  series 
(1),  (2),  .  .  .,  (h)  repeat,  owing  to  the  periodicity  of  the 
trigonometrical  functions  involved.  We  have,  for  example, 
r,/H(cos.(2?i7r  +  6)1  n  +  i  sin.(2?i-  +  6)jn)  =  rln(cos.6!n  +  i  sin.  6jn) ; 
and  so  on. 

We  can,  in  fact,  prove  that  there  cannot  be  more  than  n 
values  of  the  ?ith  root.  Let  us  denote  the  complex  number 
r(cos  0  +  i  sin  6)  by  a,  for  shortness  ;  and  let  z  stand  for  any 
mth  root  of  a.  Then  must  zn  =  a,  and  therefore  zn  -  a  =  0. 
Hence  every  »th  root  of  a,  when  substituted  for  z  in  zn  -  a, 
causes  this  integral  function  of  z  to  vanish.     Hence,  if  «„  zs,  .  .  ., 


240  JITH  ROOTS  OF  ±  1  CHAP. 

~s  be  s  nth  roots  of  a,  z-zu  z-z2>  •  •  ■,  %  —  %*  will  all  be 
factors  of  zn  -  a.  Now  z11  -  a  is  of  the  ?(th  degree  in  z,  and 
cannot  have  more  than  n  factors  (see  chap,  v.,  §  10).  Hence  s 
cannot  exceed  n ;  that  is  to  say,  there  cannot  be  more  than  n 
nth  roots  of  a. 

We  conclude  therefore  that  every  complex  number  has  n  nth 
roots  and  no  more  ;  and  each  of  these  nth  roots  can  be  expressed  as  a 
complex  number. 

Cor.  1.  Since  every  real  number  is  merely  a  complex  num- 
ber whose  imaginary  part  vanishes,  it  follows  that  every  real 
number,  whether  positive  or  negative,  has  n  nth  roots  and  no  more, 
each  of  which  is  expressible  as  a  complex  number. 

Cor.  2.  The  imaginary  nth  roots  of  any  real  number  can  be 
arranged  in  conjugate  pairs.  For  we  have  seen  that,  if  x  +  yi  be 
any  nth  root  of  a,  then  (x  +  yi)n  -  a  =  0.  Hence,  if  a  be  real  (but 
not  otherwise),  it  follows,  by  §  5,  Cor.  4,  that  (x  -  yi)n  -  a  =  0  ; 
that  is,  x  -  yi  is  also  an  nth  root  of  a. 

N.B. — This  does  not  hold  for  the  roots  of  a  complex  number 
generally. 

§  IS.]  Every  real  positive  quantity  can  be  written  in  the 
form 

r(cos  0  +  i  sin  0)  (A) ; 

and  every  real  negative  quantity  in  the  form 

r(cos  7r  +  i  sin  7r)  (B) ; 

where  r  is  a  real  positive  quantity.  Hence,  if  we  know  the  n 
nth  roots  of  cos  0  +  ism  0,  that  is,  of  +1,  and  the  n  nth  roots  of 
cos  7r  +  isin7r,  that  is,  of  -  1,  the  problem  of  finding  the  n  nt\i 
roots  of  any  real  quantity,  whether  positive  or  negative,  is 
reduced  to  finding  the  real  positive  value  of  the  nth  root  of  a 
real  positive  quantity  r  (see  chap,  xi.,  §  15). 

By  means  of  the  nth  roots  of  +  1  we  can,  therefore,  com- 
pletely fill  the  lacuna  left  in  chap,  x.,  §  2.  In  addition  to  their 
use  in  this  respect,  the  nth.  roots  of  ±  1  play  an  exceedingly  im- 


XII  WTH  ROOTS  OF  ±1  241 

portant  part  in  the  theory  of  equations,  and  in  higher  algebra 
generally.  We  therefore  give  their  fundamental  properties  here, 
leaving  the  student  to  extend  his  knowledge  of  this  part  of 
algebra  as  he  finds  need  for  it. 

Putting  r-1  and  0  =  0  in  1,  .  .   .,  n  of  §  17,  and  remem- 
bering that  Vln  =  1,  we  obtain  for  the  n  nth  roots  of  +  1, 

cos  0  +  i  sin  0,     cos  —  +  %  sin  — , , 

n  n 

2(/i-1)tt      .   .    2(?i-1)tt 

cos  — J - — v  i  sin  — —  • 

n  n 

Putting  r=l,  6  =  tt,  we  obtain  for  the  nth  roots  of  -  l, 

TV  .      .        7T  StT  .      .        StT 

cos  -  +  i  sin  -,     cos  —  +  i  sin  — ,     ...,.., 
n  n  n  n 


(2w-  1W      .   .    (271-1W 

cos —  +  i  sin • 

n  n 

Cor.  1.   Since  cos .  2(?i  -  l)ir/w  =  cos .  27r/«,  sin  .  2(n  -  l)irjn  = 

-  sin  .  iTrjn;    cos  .  2(w  -  2)7r,?i  =  cos  .  iir/n,    sin  .  2(u  -  2)7rjn  = 

-  sin .  47r/»,   and    so    on,    we   can   arrange    the   roots   of   +1   as 
follows: — 

nth  roots  of  +  1,  n  even,  =2m  say, 

2tt       .    .     2tt  4ir       .    .     4-7T 

+  1,  cos  —  ±  x  sin  — ,     cos  —  ±  %  sin  — ,  .  .  ., 
n  n  n  n 

^a  2(^-iy           2(>u-lV  . 

cos ±isin- ,   -1  (L) ; 

7ith  roots  of  +  1,  n  odd,  =  2m  +  1  say, 

,  2ir      .    .     2tt  4:tt      .    .     4tt 

+  1,  cos — ±zsin — ,     cos  —  ±tsin — ,  .  .  ., 
n  n  n  n 

2nnr     .  .    2nnr  tir.. 

cos ±  i  sin (D). 

n  n  v    ' 

vol.  I  R 


242  WTH  ROOTS  OF  ±  1  chap. 

Similarly  we  can  arrange  the  roots  of  -  1  as  follows: — 
reth  roots  of  -  1,  «  even,  =  2m  say, 

cos  -  ±  i  sm  -,    cos  —  ±  i  sin  — ,  .  .  . , 
n  n  n  n 

(2m- 1W     .   .    (2m-  l>r 

cos '—  ±  i  sin ^-  (E) : 

n  n  v   ' 

?i th  roots  of  -  1,  n  odd,  =  2m  +  1  say, 

Ti         .      .       7T  37T         .      .       3~ 

cos  -  ±  i  sin  -,    cos  —  ±  i  sin  — ,  .... 
n  n  n  n 

(2m- 1W  L  .   .    (2m- 1W 

cos  v '—  ±  t  sin  v —     —  .  -  1  (F). 

11  n  v   ' 

From  (C),  (D),  (E),  (F)  we  see,  in  accordance  with  chap,  x., 
§  2,  that  the  ??th  root  of  +  1  has  one  real  value  if  n  be  odd,  and 
two  real  values  if  n  be  even  ;  and  that  the  »th  root  of  -  1  has 
one  real  value  if  n  be  odd,  and  no  real  value  if  n  be  even. 

We  have  also  a  verification  of  the  theorem  of  §  17,  Cor.  2, 
that  the  imaginary  roots  of  a  real  quantity  consist  of  a  set  of 
pairs  of  conjugate  complex  numbers. 

Cor.  2.  The  first  of  the  imaginary  roots  of  +  1  in  the  series 
(1),  .  .  .,(»),  namely,  cos.  2wjn  +  i  sin.  2ir/n,  is  called  a  primitive* 

rtth  root  of  +  1.     Let  us  denote  this  root  by  w. 
Then  since,  by  Demoivre's  Theorem, 

•2tt      .    .     2ttY  -2stt      .    .     2S7T 

cos  —  +  i  sin  —     -  cos  —  +  %  sm  — , 
n  n  /  it  n 

and,  in  particular, 


1%  n 


it 


2tt      .   .    2ir\ 
(on  =  (  cos  —  +  i  sin  —  I    ==  cos  2-n-  +  i  sin  2tt, 


1, 


*  By  a  primitive  imaginary  ?tth  root  of  +  1  in  general  is  meant  an  ?;th  root 
which  is  not  also  a  root  of  lower  order.  For  example,  cos.27r/3  +  isin.27r/3 
is  a  6th  root  of  +1,  but  it  is  also  a  cube  root  of  +1,  therefore  cos.27r/3-f 
»sin.2r/3  is  not  a  primitive  6th  root  of  +1.  It  is  obvious  that  cos.27r/«  + 
■i  sir\.2ir/n  is  a  primitive  «th  root ;  but  there  are  in  general  others,  and  it  may 
be  shown  that  any  one  of  these  has  the  property  of  Cor.  2. 


XII  FACTORISATION  OF  xn  ±  A  243 

we  see  that,  if  <o  be  a  primitive  imaginary  nth  root  of  +  1,  then  the 
n  nth  roots  of  +  1  are 

to  ,  u) ,  u) ,   .   .    . ,  wn  (Gr). 

Similarly,  i/"  w'  -  cos.ir/n  +  i  sin.7r/?t,  w/tic/i  we  may  call  a  primitive 
imaginary  nth  root  of  -  I,  then  the  n  nth  roots  of  -  1  are 


,./2n-l  /fj\ 


OJ 


§  19.]  The  results  of  last  paragraph,  taken  in  conjunction 
with  the  remainder  theorem  (see  chap,  v.,  §  15),  show  that 

Every  binomial  integral  function,  xn  ±  A,  can  be  resolved  into  n 
factors  of  the  1st  degree,  whose  coefficients  may  or  may  not  be  wholly 
real,  or  into  at  most  two  real  factors  of  the  1st  degree,  and  a  number 
of  real  factors  of  the  2nd  degree* 

Take,  for  example,  x2m  -  a2m.  This  function  vanishes  whenever  we  sub- 
stitute for  x  any  2»ith  root  of  a2m ;  that  is,  it  vanishes  whenever  x  has  any 
of  the  values  aw,  aw2,  .  .  . ,  aw2'"  where  w  stands  for  a  primitive  2?)ith  root 
of  +1. 

Hence  the  resolution  into  linear  factors  is  given  by 

To  obtain  the  resolution  into  real  factors,  we  observe  that,  corresponding 
to  the  roots  +a  and  —a,  we  have  the  factors  x-a,  x  +  a;  and  that,  corre- 
sponding to  the  roots  a(cos.STr/m±i sin .sir/m),  we  have  the  factors 


(St       .   .    sir\  / 
x-a  cos ai  sin  —  II 
m  m  J  \ 


sir        .   .    sw\ 

x-a  cos \-ai  sin  —  I, 

vi  m  J 


(  SW\"  „     .      0S7T 

=  I  x  -  a  cos  —  )  +  a-  sin"  — , 
\  to  /  TO 

o      0  Sir        „ 

=x-  -  2ax  cos h  a~. 

m 

Hence  the  resolution  into  real  factors  is  given  by 

x2m  -  a2m=(x  -a)(x  +  a)  (x2  -  lax  cos  —  +  a2)  lx2  -  lax  cos ha2)... 

m  m 

We  may  treat  x2m  +  aim,  x2m+l  -  a~m+1,  and  x2m+1  +  a2m+l  in  a  similar  way. 

Example  1. 

To  find  the  cube  roots  of  +  1  and  -  1.  We  have  +1  =1  {cos  O  +  i  sin  0}. 
Hence  the  cube  roots  of+1  are 

cos  0  +  i  sin  0,     cos .  27r/3  ±  i  sin .  27r/3, 
that  is  to  say ,  + 1 ,  - 1/2±  i*j3/2. 

*  The  solution  of  this  problem  was  first  found  in  a  geometrical  form  by 
Cotes  ;  it  was  published  without  demonstration  in  the  Harmonia  Mensurarum 
(1722),  p.  113.  Demoivre  (Misc.  Anal.,  p.  17)  gave  a  demonstration,  and  also 
found  the  real  quadratic  factors  of  the  trinomial  1  +  2  cos  Ox"  +  x'2". 


244  EXAMPLES  chap. 

Again  -1  =  1  {cos  ir  +  i  sin  jt} .      Hence  the  cube  roots  of  -  1  are 
cos .  ir/3  ±  i  sin .  ir/B,     cos  it  +  i  sin  w, 
that  is  to  say,  l/2±i\j3f2,   -  1. 

Example  2. 

To   find    the   cube   roots   of    1+i.      We   have    l+t=V2(Vv^+ll/V2) 
=  \/2(cos  45°  +  i  sin  45°).     Hence  the  cube  roots  of  1  +  i  are 

2J(cos  15°  +  i  sin  15°),     2*(cos  135°  +  i  sin  135°),     2*(cos  255°  +  i  sin  255°), 
that  is, 

2*(cos  15°  +  i  sin  1 5°),     2h{  -  cos  45°  +  i  sin  45°),     2*(  -  cos  75°  -  i  sin  75°), 
that  is, 

i/V3  +  l      V3-l\       1/       1        .   1  \     21/     V3-1      -\/3  +  l\ 
2r2V2_+  l"2V2~>    H"V2+    V2>    U~~2^      l2V2> 

«,„*;.  (V3  +  l)  +  (V3-l)f     -1+t         (V8-l)  +  CV3  +  l)t 

mat  is,  j ,    j — , -2 . 

93  93  9? 

Here  it  will  be  observed  that  the  roots  are  not  arranged  in  conjugate  pairs,  as 
they  would  necessarily  have  been  had  the  radicand  been  real. 

Example  3. 

To  find  approximately  one  of  the  imaginary  7th  roots  of  + 1.     One  of  the 
imaginary  roots  is 

cos  51°25'43"  +  i  sin  51°25'43". 

By  the  table  of  natural  sines  and  cosines,  this  gives 

•6234893+ -7818318?; 
as  one  approximate  value  for  the  7th  root  of  + 1. 

Example  4. 

If  a  be  one  of  the  imaginary  cube  roots  of  + 1,  to  show  that  1  +  w  +  co2=  0 
and  that  {ax  +  a2y){a2x  +  ay)  is  real. 

AVe  have  1  +w  + w2  =  (l  -  w3)/(l  -  w)  =  0,  since  co3=l  and  l-w#0. 
Again, 

{ax  +  a2y)  {a2x  +  ay)  =  a*x2  +  {a4  +  a2)xy  +  uPy'2. 

Now  u3=l  ;  and  w4  +  w2=w3u>  +  wa=«  +  a2—  -1,  since  l+«  +  w2  =  0. 

Hence 

( ax  +  a2y)  {a2x  +  ay)  =  x2  —  xy  +  y2. 


FUNDAMENTAL    PROPOSITION    IN    THE   THEORY    OF   EQUATIONS. 

§  20.]  If  /(2)sA0  +  A,«  +  A/+  •  •  •  +A„;n  be  an  integral 
function  of  z  of  the  nth  degree,  whose  coefficients  A0,  A,,  .  .  . ,  Aw 
are  given  complex  numbers,  or,  in  particular,  real  numbers,  where,  of 
course,  Aa  +  0,  then  f(z)  can  always  be  expressed  as  the  product  of  n 
factors,  each  of  the  1st  degree  in  z,  say  z  -  zl}  z-z.,,  z  -  z3,  .  .  ., 
z  -  zn,  ;.',,  z2,  .   .   .,  zn  being  in  general  complex  numbers. 


xii  FACTORISATION  OF  ANY  INTEGRAL  FUNCTION  245 

It  is  obvious  that  this  proposition  can  be  deduced  from  the 
following  subsidiary  theorem  : — 

One  value  of  z,  in  general  a  complex  number,  can  always  he  found 
which  causes  f{z)  to  vanish. 

For,  let  us  suppose  that  /(s,)  =  0,  then,  by  the  remainder 
theorem,  f(z)  =f(z)  (z  -  «,),  where  f(z)  is  an  integral  function  of  z 
of  the  (n  -  l)th  degree.  Now,  by  our  theorem,  one  value  of  z  at 
least,  say  z,,  can  be  found  for  which  f(z)  vanishes.  We  have, 
therefore,  /,(&)  =  0  ;  and  therefore  /,(*)  =fa(z)  (z  -  z2),  where  f2(z) 
is  now  of  the  (»  -  2)th  degree ;  and  so  on.     Hence  we  prove 

finally  that 

f(z)  s  k(z  -  *,)  (z  -  z2)  ...(z-  ztl), 

where  A  is  a  constant. 

§21.]  We  shall  now  prove  that  there  is  always  at  least  one 
finite  value  of  z,  say  z  =  a,  such  that  by  taking  z  sufficiently  near 
to  a,  that  is  by  making  \z  -  a\  small  enough,  we  can  make 
\f(z)  |  as  small  as  we  please.  So  that  in  this  sense  every 
integral  equation/^)  =  0  has  at  least  one  finite  root. 

Let  |  z  I  =  R.     Then,  since 

\f(z)  |  =  |  A. | R" 1 1  +  An_  JAnz  +    .  .  .    +  A0jAnzn  | , 
we  have,  by  §  14, 

\f(z)  |  >  |  An  |  R»{1  -  |  An_,/Anz  +    .  .  .  +  A0/A,,*"  | }, 
provided  |  z  |,  (i.e.  R),  be  large  enough ;  therefore 

|/(*)|>|A*|R»{1-C(1/R+   .  .  .    +  1/R»)}, 

where  C  is  the  greatest  of  |An_,/An|,  .   .  .,   [A0/Aw|.     There- 
fore, taking  provisionally  R>1,  we  have 

\f(z)  |  >  |  A. |  R»{1  -  CXI  -  1/R»)/R(1  -  1/R)}, 

>|An|R»{l-C/(R-l)}  (1), 

provided  R  >  C  +  1 . 

Hence,  by  taking  \z\  sufficiently  large,  we  can  make  \f(z)\  as  large 
as  we  please ;  and  we  also  see  that  there  can  be  no  root  of  f(z)  -  0 
whose  modulus  exceeds  C  +  1 . 

Let  now  w  be  the  value  of  z  at  any  finite  point  in  the 
Argand  Plane,  so  that  \f(ic)  |  is  finite.     It  follows  from  what  has 


246  EXISTENCE   OF  A   ROOT  CHAP. 

just  been  proved  that  we  can  describe  about  the  origin  a  circle 
S  of  finite  radius,  such  that,  at  all  points  on  and  outside  S, 
|/(~)  I  >  \f(w)  |  •  Then,  since  \f(w)  ]  is  real  and  positive,  if  we 
consider  all  points  within  S,  we  see  that  there  must  be  a  finite 
lower  limit  L  to  the  value  of  \f(w)  \ ;  that  is  to  say,  a  quantity 
L  which  is  not  greater  than  any  of  the  values  of  \f(w)  |  within  S, 
and  such  that  by  properly  choosing  u  we  can  make  \f(w)  |  =  L  +  e, 
where  e  is  a  real  positive  quantity  as  small  as  we  please. 

We  shall  show  that  L  must  be  zero.  For,  suppose  L  >  0, 
and  choose  w  so  that  \f(w)  |  =  L  +  e.  Let  h  be  a  complex  number, 
say  r(cos  0  +  i  sin  6).     Then 

f(w  +  h)  -  A0  +  A  (w  +  h)  +    .  .  .  +  An(w  +  h)n, 

=f(w)  +  BJi  +  BJf+    .  .  .+Anhn  (2), 

where  An  is  independent  both  of  w  and  h,  and  by  hypothesis 
cannot  vanish,  but  B„  .  .  .,  Bn_!  are  functions  of  w,  one  or  more 
of  which  may  vanish.  Suppose  that  Bm  is  the  first  of  the  B's 
that  does  not  vanish,  and  let  bm(cos  am  +  i  sin  <xm),  etc.,  be  the 
normal  forms  of  the  complex  numbers  Bm/f(w),  etc.  Then, 
since  \f{w)  |  is  not  zero,  bmi  etc.,  are  all  finite.  Also  we  have, 
by  Demoivre's  Theorem, 

f(w  +  h)ff(w)  =  1  +  bmr™em  +  bm+1r™+iQm+i  +  .  .  .  +  6nr»6n    (3), 
where  0m  =  cos  {md  +  am)  +  i  sin  (rnd  +  am),  etc. 

We  have  h,  and  therefore  both  r  and  6  at  our  disposal.  Let 
us  first  determine  0  so  that  cos  {m6  +  am)  =  -  1,  sin  (mO  +  am)  =  0 ; 
that  is,  give  6  any  one  of  the  m  values  {it  -  am)/m,  (Stt  —  am)/w, . . ., 
(2m  -  1.  7r  -  am)/m,  say  the  first.  Then  we  have  Qm=  -1; 
and  Qm+l,  etc.,  assume  definite  values,  say,  G'm+1>  etc.  We  now 
have 
f(w  +  h)/f(w)  =  1  -  bmr™  +  bm+1fm+10'm+1  +  .  .  .  +  bnr"Q'n  (A). 

Considering  the  right  hand  side  of  (4)  as  the  sum  of  1  -  bmrm 
and  bm+lrm+iQ'm+l  +  .  .  .  +  bnrnQ'n,  we  see,  by  §  14,  that  the 
modulus  of  f(w  +  h)jf(w)  lies  between  the  difference  and  the  sum 
of  the  moduli  of  these  two.     Also 


XII 


EXISTENCE   OF  A   ROOT  247 


\bm+lr™+lQ,m+l+  .  .  .  +  bnO'nrn\<bm+lrm+1  +  •  •  •  +&»'* 

<b(rm+1  +  .  .  .  +rn), 

where  b  is  the  greatest  of  bm+l,  .  .  .,  bn, 

<  («  -  m)brm+\ 

provided  we  take  r<  1,  so  that  rm+i>rm+2>  _  #  §    >rn 

Therefore  we  have 

I  -  bmrm  -(n-  m)b?-m+l  <  \f(w  +  h)/f(w)  | 

<  1  -  6TOrm  +{n  -  m)brm+l  (5) ; 

provided  r  be  so  chosen  that  1  -  bmrm  and  1  -  bmrm  -  (n  -  m)brm+1 
are  both  positive.  Let  us  further  choose  r  so  that  (n  -  m)hm+1 
<bmrm.  All  these  conditions  will  obviously  be  satisfied  if  we 
give  a  finite  value  to  r  less  than  the  least  of  the  three, 

1,     l/(26m)lM.     bm/(n-m)b.  (6). 

When  r  is  thus  chosen,  \f(w  +  h)/f(w)  |  will  lie  between  two 
positive  proper  fractions,  so  that  \f(w  +  h)jf(w)  |  =  1  —  /x,  where  /x 
is  a  positive  proper  fraction ;  and  we  have 
|/(w  +  A)|  =  (l-/t)|/HI  =  (l-/*)(L  +  €)  =  L  +  6-/t(L  +  e)(7). 

which,  since  e  may  be  as  small  as  we  please,  is  less  than  L  by  a 
finite  amount.  L  is  therefore  not  a  finite  lower  limit  as  sup- 
posed; in  other  words,  L  must  be  zero.  Our  fundamental 
theorem  is  thus  established. 

By  reasoning  as  above  we  can  easily  show  that,  if 

f(z)  =  A0  +  Ailz*+  .  .  .  +Anzn, 
then 
\Ao\{l-(n-s+l)d\z\»}<\f(z)\ 

<\A0\{l+(n-s+l)d\z\°}     (8), 

where  d  is  the  greatest  of  |  A«/A0 1 ,  .  .  .,  |  An/A0 1 ,  provided  [  z  \ 
is  less  than  the  lesser  of  the  two  quantities  1,  l/{(n  -  s  +  l)d}l>s. 

Combining  this  result  with  one  obtained  incidentally  above, 
we  have  the  following  useful  theorem  on  the  delimitation  of  the 
roots  (real  or  imaginary)  of  an  equation. 

Cor.  1,  The  equation  A0  +  AgZ8  +  .  .  .  +  Anzn  =  0  can  have  no  root 
whose  modulus  exceeds  the  greatest  of  the  quantities  1  +  |  A0/Aw  | , 


248  GRADIENT   AND    EQUIMODULAR    CURVES  CHAP. 

1  +  |  AsjAn  | ,  .  .  .,  1  +  |  An_JAn  | ,  or  whose  modulus  is  less  than  the 
least  of  1,  l/{(n  -  s  +  1)  |  As/A0 1  }V°,  .  . .,  l/{(«  -  s  +  1)  |  An/A0 1  }**. 

Cor.  2.  JFe  ca»  always  assign  a  positive  quantity  ?;,  such  that,  if 
|  A|<?7,  |/(2  +  h)  -f(z)  |<e,  w/tere  e  is  a  positive  quantity  as  small  as 
we  please. 

This  is  expressed  by  saying  that  the  integral  function  f(z)  is 
continuous  for  all  complex  values  of  its  argument  which  have  a 
finite  modulus.  The  proof  is  obvious  after  what  has  already 
been  done. 

The  above  demonstration  is  merely  a  version  of  the  proof  given  by 
Argand  in  his  famous  Essai,  *  amplified  to  meet  some  criticisms  on  the  briefer 
statement  in  earlier  editions  of  this  work.  The  criticisms  in  question  touch 
the  formulation,  but  not  the  essential  principle  of  Argand's  proof,  which  is 
both  ingenious  and  profound.  As  some  of  the  critics  appear  to  me  to  have 
missed  the  real  point  involved,  perhaps  the  following  remarks,  which  the 
student  will  appreciate  more  fully  after  reading  chap.  xv.  §§  17-19,  and 
chap,  xxix.,  may  be  useful. 

Taking  any  value  of  z=x  +  yi,  let  f(z)  —  u  +  vi,  where  u  and  v  are  real 
functions  of  the  real  variables  x  and  y.  Plot  u-  v-  and  x-  y-  Argand 
diagrams.  Then  to  each  point  (x,  y)  there  corresponds  one  point  (u,  v), 
although  it  may  happen  that  to  one  (u,  v)  point  there  correspond  more  than 
one  (x,  y)  point.  If  we  start  with  any  given  point  (x,  y),  and  consider 
\/(z)  I  =  \f(u2  +  v2)>  it  is  obvious  that  the  direction  in  which  \f(z)  \  varies  most 
rapidly  is  obtained  by  causing  (x,  y)  to  move  in  the  x-  y-  plane,  so  that 
(u,  v)  moves  along  the  radius  vector  towards  the  origin  in  the  u-  v-  plane  ; 
also  that  the  rate  of  variation  in  the  perpendicular  direction  is  zero.  If, 
therefore,  we  trace  one  of  the  curves  v\u  =  constant  in  the  x-  y-  plane,  the 
tangent  to  this  curve  at  every  point  z  on  it  is  the  direction  of  most  rapid 
variation.     We  may  call  these  curves  the  Gradient  Curves  of/(s).t 

*  See  in  particular  his  amplified  demonstration  given  in  a  note  in  Ger- 
gonne's  Ann.  de  Math.  t.  v.  pp.  197-209  (1814-15). 

t  These  curves,  together  with  the  curves  u^  +  v2  —  constant,  which  we 
may  call  the  Equimodular  Curves  of /(c),  possess  a  number  of  interesting 
properties.  Since  the  Equimodulars  and  Gradients  are  orthomorphosed  (see 
chap.  xxix.  §  36)  from  a  series  of  concentic  circles  and  their  pencil  of 
common  radii,  they  form  two  mutually  orthogonal  systems.  Through 
every  given  point  (x't  y'),  which  is  not  the  affixe  of  a  root  of /(s)  =  0,  there 
passes  one  equimodular  u2  +  v2  =  u"1  +  v'2  and  one  gradient  u'v-v'u  —  0. 
Every  gradient  u'v-v'u  —  0  passes  through  all  the  intersections  of  u  —  0, 
v  —  0,  i.e.  through  the  affixes  of  all  the  roots  of  /(z)  =  0.  Near  the  root 
points  the  equimodulars  take  the  form  of  small  ovals  enclosing  these  points. 


XII  ARGAND'S   PROGRESSION   TO   A   ROOT  249 

It  may  readily  be  shown  that  the  process  by  which  we  pass  from  v  to 
w  +  h  (—wv  say)  in  the  above  demonstration  simply  amounts  to  passing  a 
certain  distance  along  a  tangent  to  the  gradient  curve  through  the  point  w. 
We  may  repeat  this  process,  starting  from  wx  and  passing  along  the  tangent 
to  the  gradient  through  w1}  and  so  on.  We  shall  thus  ha.vef(to)>f(w1)> 
f{w0)  >  .  .  .  This  process  we  may  call  Argand's  Progression  towards  the  root 
of  an  equation. 

Since  bn<b,  bmrm  +  (n-  m)brm+l<\,  and  (n-m)brm+1<bmr'»,  it  follows 
that 

r  <  { \AW)  I  /2('1  -  m)  I  A»  I  !• '  /(m+1)  and  r  < !  B™  I  A*  _  m)  I  A»  I  • 

The  first  of  these  conditions  shows  that  the  longest  admissible  steps  of 
Argand's  Progression  become  smaller  and  smaller  as  we  approach  a  root. 
This  is  expressed  by  saying  that  the  Progression  becomes  asymptotic  as  we 
approach  a  root. 

But  the  second  condition  shows  that  Progression  also  becomes  asymptotic 
as  we  approach  a  point  at  which  Bj  =  0  ;  or  Bi  =  0,  B.2=:0  ;  or  B1  =  0,  B2=0, 
B3  =  0,  etc.  Such  points  are  stationary  points  for  the  variation  of  \J\z)  |  on 
any  path  which  passes  through  them.  They  are  also  multiple  points  on  the 
gradient  curves  which  pass  through  them  ;  so  that  at  them  we  have  2,  3,  4, 
etc.,  directions  of  most  rapid  variation  of  \f{z)  \ . 

If  the  original  progression  leads  towards  one  of  these  points  (for  which  of 
course  \f{iv)  |4=0),  we  must  infer  its  existence  from  the  asymptotic  approach, 
and  start  afresh  from  that  point  along  one  of  the  tangents  to  the  gradient 
that  passes  through  it ;  or  we  may  avoid  the  point  altogether  by  starting 
afresh  on  a  path  which  docs  not  lead  to  it. 

An  interesting  example  is  to  take  z2  -  z  + 1  =  0,  and  start  from  a  point  on 
the  real  axis  in  the  x-  y-  diagram.  Argand's  Progression  will  lead  first  to 
the  minimum  point  (1/2,  0)  on  the  x-  axis  ;  then  along  a  line  parallel  to  the 
y-  axis  to  the  points,  (1/2,  ±  *j3/2),  which  are  the  affixes  of  the  two  imaginary 
roots.  The  diagram  of  chap.  xv.  §  19  will  also  furnish  a  curious  illustration 
by  taking  initial  points  on  one  or  other  of  the  two  dotted  lines. 

It  should  be  noted  that  the  question  as  to  whether  |/(a)  |  actually  reaches 
its  lower  limit  is  not  essential  in  Argand's  proof,  if  we  merely  propose  to 
show  that  a  value  of  z  can  be  found  such  that  \f(z)  |  is  less  than  any  assigned 
positive  quantity,  however  small.  Nor  do  we  raise  the  question  whether 
the  root  is  rational  or  irrational,  which  would  involve  the  subtle  question  of 
the  ultimate  logical  definition  of  an  irrational  number  (see  vol.  ii.  (ed.  1900) 
chap.  xxv.  §§  28-41). 

§  22.]  We  have  now  shown  that  in  all  cases 

f(z)  =  A(z  -  2,)  (z  -  gg)  .  .  .  (z  -  zn), 

where  A  is  a  constant. 

zlf  z,,  .  .   .,  Zn  may  be  real,  or  they  may  be  complex  numbers 
of  the  general  form  x  +  yi.     They  may  be  all  different,  or  two 


250       EQUATION  OF  WTA  DEGREE  HAS  n   ROOTS      CHAP. 

or  more  of  them  may  be  identical,  as  may  be  easily  seen  by 
considering  the  above  demonstration. 

The  general  proposition  thus  established  is  equivalent  to  the 
following  : — 

If  f(z)  be  an  integral  function  of  z  of  the  nth  degree,  there  are 
n  values  of  z  for  which  f(z)  vanishes.  These  values  may  be  real  or 
complex  numbers,  and  may  or  may  not  be  all  unequal. 

We  have  already  seen  in  chap,  v.,  §  16,  that  there  cannot  be 
more  than  n  values  of  z  for  which  f(z)  vanishes,  otherwise  all  its 
coefficients  would  vanish,  that  is,  the  function  would  vanish  for 
all  values  of  z.  We  have  also  seen  that  the  constant  A  is  equal 
to  the  coefficient  An.     We  have  therefore  the  unique  resolution 

f(z)  =  An(z  -  zt)  (z  -  z2)  .  .  .  (z  -  zn). 

§  23.]  If  the  coefficients  of  f(z)  be  all  real,  then  we  have 
seen  that  if  f(x  +  yi)  vanish  f(x  -  yi)  will  also  vanish.  In  this 
case  the  imaginary  values  among  zu  z2,  .  .  .,  zn  will  occur  in 
conjugate  pairs. 

If  a  +  fii,  a  -  (3i  be  such  a  conjugate  pair,  then,  correspond- 
ing to  them,  we  have  the  factor 

(Z  -  a  -  (3i)  (z-a  +  (3i)  =  (z-  af  +  ft, 

that  is  to  say,  a  real  factor  of  the  2nd  degree. 

It  may  of  course  happen  that  the  conjugate  pair  a  ±  fti  is 
repeated,  say  s  times,  among  the  values  z„  z,,  .  .  .,  zn.  In  that 
case  we  should  have  the  factor  (z  -  a)2  +  (3s  repeated  s  times  ;  so 
that  there  would  be  a  factor  {(z  -  a)2  +  (32}s  in  the  function  f(z). 

Hence,  every  integral  function  of  z,  wlwse  coefficients  are  all  real, 
can  be  resolved  into  a  product  of  real  factors,  each  of  which  is  either 
a  positive  integral  power  of  a  real  integral  f  miction  of  the  1st  degree, 
or  a  positive  integral  power  of  a  real  integral  function  of  the  2nd 
degree. 

This  is  the  general  proposition  of  which  the  theorem  of  §  19 
is  a  particular  case. 


XII 


EXERCISES  XVI  951 


Exercises  XVI. 


Express  as  complex  numbers — 

(1.)  (a  +  bi)8  +  (a-bif. 

(2)    1+i   l   1~i 

2  +  36i  f7-26i 
{4m)    6  +  8i  +  3-4i' 

u)  (p±si\\(p^iY 

\p-qij     \p  +  viJ 

69-7V(15)  +  (V3-6V5)i 

{    '  3-(V3-3V5)i 

(6.)  Show  that 

if  n  be  any  integer  which  is  not  a  multiple  of  3. 

(7.)  Expand  and  arrange  according  to  the  powers  of  a; 

(as  -  1  -  i\J2)  (x-\  +  i\/2){x-2  +  i^/3)  (a;  -  2  -  i\/3). 

(8. )  Show  that 

\(2a-b-c)+i{b-c)^B}3={{2b-c-a)  +  i(c-aWS}3. 

(9.)  Show  that 

{(V3  +  1)  +  (V3-- W=16(l  +  i). 

(10.)  If  £  +  J?t  be  a  value  of  x  for  which  ax1  +  bx  +  c  =  0,  a,  6,  c  being  all 
real,  then  2a£rj  +  br)  =  0,  a??2  =  a£2  +  &£  +  c. 

(11.)  If  #(a?+2/*)=X.+Y*,  show  that  4(X2-Y2)  =  x/X  +  y/Y. 

(12.)  If  n  be  a  multiple  of  4,  show  that 

l+2i  +  3i2  +  .  .  .  +  (n  +  l)in=%(n  +  2-ni). 

(13.)  Showthat|o0  +  o15  +  .  .  . +anzn\^\an\  \z\n(l-nc/\z\),  provided  \z\ 
exceeds  the  greater  of  1  and  nc,  and  c  is  the  greatest  of  \aQ[a„\,  .  .  ., 

I  ««-]/««  |. 

(14.)  Find  the  modulus  of 

(2-3i)(3  +  4t) 
(6+4i)(15-8i)" 

(15.)  Find  the  modulus  of 

{x+  J&+W- 

(16.)  Find  the  modulus  of 

bc(b  -  ci)  +  ca(c  -  ai)  +  ab(a  -  bi). 
(17.)  Show  that 

1 1  +  ix  +  i~x-  +  iV  + .   .   .  ad  » |  =  1/  S!{1  +  x2)',  where  as<l. 
(18.)  Find  the  moduli  of  (x  +  yi)n  and  (x  +  yi)n/(x-yi)n. 

Express  the  following  as  complex  numbers  : — 
(19.)    \/-7  +  24f.  (20.)    \fQ  +  iJ13. 


(21.)   *J  -  7/36  +  2t/3.  (22.)    s'lab  +  2(oa  -  "Fjl 

(23.)    s!\+2x*]{x2-\)i.  (24.)    Vl  + i ^(x4  -  1 ). 

(25.)  Find  the  4th  roots  of  -  119  +  120;'. 


252  EXERCISES   XVI  CHAP. 

(26.)  Resolve  x*-  a6  into  factors  of  the  1st  degree. 

(27.)  Resolve  a;5+l  into  real  factors  of  the  1st  or  of  the  2nd  degree. 

(28.)  Resolve  xG  +  x5+  x4+x3  +  x2+x  +  l  into  real  factors  of  the  2nd 
degree. 

(29.)  Resolve  x2m-  2  cos  0amxm  +  a2m  into  real  factors  of  the  1st  or  of  the 
2nd  degree. 

(30.)  If  w  be  an  imaginary  nth  root  of  +1,  show  that  l  +  w  +  w2  +  .  .  .  + 
co"-1  =  0. 

(31.)  Show  that,  if  w  be  an  imaginary  cube  root  of  +1,  then 

x3  +  y3  +  z3  -  Sxyz  =  (x  +  y  +  z)  (x  +  wy  +  w2z)  (x  +  uPy  +  uz), 
and 

(x  +  wy  +  uhf  +  (x  +  w2y  +  wz)3  =  (2x-y -z)  {2y -z~x)  {2z-x-  y). 

(32. )  Show  that  (x  +  y)m  -xm-ym  is  divisible  by  x2  +  xy  +  y1  for  every  odd 
value  of  m  which  is  greater  than  3  and  not  a  multiple  of  3. 
(33.)  Show  that 

U„         2/-7T     -T    .     2nr\      („    .     2/7T     „         2rir\   .  ^ n     ,v     „.. 
Xcos Ysin )  +  (Xsin +  \  cos )i  V   =  (\+\i)n. 
n                  n  J     \            n                  n  J     J 

(34.)  Simplify 

(cos  2d  -  i  sin  20)  (cos  <£  +  i  sin  4>)2     (cos  20  +  i  sin  20)  (cos  <p  -  i  sin  <f>)2 
cos  (0 +  <p)  +  i  sin  {0  +  <p)  cos  (0  +  0) -i  sin  (0  +  0) 

(35.)  If  s/(a  +  bi)+  s/(c  +  di)=  s/(x  +  yi),  show  that 

(x-a-c)2+(y-b-d)2  =  4^J{(a2  +  b2)(e-  +  d2)}. 
(36.)  Prove  that  one  of  the  values  of  *J(a  +  bi)  +  £/(a  -  bi)  is 

v/[  J  \2a  +  2V(«2  +  b2)}  +  2  Z'(a2  +  b2)\ 
(37.)  If  w  =  cos  tt/7  +  i  sin  tt/7,  prove  that  {x  -  w)  {x  +  w2)  (x  -  it?)  (x  +  w4) 
(x  -  w5)  (x  +  w6)  =  x6  -  x5  +  x4  -  x3  +  x2  -  x  + 1 . 

(38.)  Find  the  value  of  wr1  +  w;''24  .  .  .  +wrn  ;  wlt  w2  .  .  .  w„  being  the 
nth  roots  of  1,  and  r  a  positive  integer.  What  modification  of  the  result  is 
necessary  if  r  is  a  negative  integer  ? 

Prove  that  1/(1 +«)!«) -f  1/(1  + «>2a;)  +  -  •  •  +l/(l+w„a:)=M/(l  -a;"). 

(39.)  Decompose  1/(1  +x  +  x2)  into  partial  fractions  of  the  form  aj(bx  +  c). 
Hence  show  that 

a:/(l  +  x  +  x1) -x  -  x2  +  x4  - x5  +  x1  - x8  + .  .  .  +  x3n+l  -  x3n+2  +  R, 
where  a^,  xe,  etc. ,  are  wanting  ;  and  find  R. 

(40.)  Find  the  equation  of  least  degree,  having  real  rational  coefficients, 
one  of  whose  roots  is  ^2  +  i. 

One  root  of  x4  +  3a;3-  30a;2  +  366.*:-  340  =  0  is  3 +  5?:,  find  the  other  three 
roots. 

(41.)  If  a  be  a  given  complex  number,  and  z  a  complex  number  whose 
affixe  lies  on  a  given  straight  line,  find  the  locus  of  the  affixe  of  a  +  z. 

(42.)  Show  that  the  area  of  the  triangle  whose  vertices  are  the  affixes  of 
ssii  s2,  z3  is  2  {(z2  -  z8)  |  zx  |2  /Uz-l}  . 

(43.)  If  2  =  (a +  7  cos  0)  +  i((i  +  y  sin  0),  where  a,  /3,  y  are  constant  and  0 
variable,  find  the  maximum  and  minimum  values  of  |  z  |  ;  and  of  amp  z 
when  such  values  exist. 


XII 


HISTORICAL  NOTE  253 


(44. )  If  the  affixe  of  x  +  yi  move  on  the  line  Sx  +  iy  +  5  =  0,  prove  that  the 
minimum  value  of\x  +  yi\  is  1. 

(45.)  If  u  and  v  are  two  complex  numbers  such  that  u  =  v+l/v,  show 
that,  if  the  affixe  of  v  describes  a  circle  about  the  origin  in  Argand's  diagram, 
then  the  aflixe  of  u  describes  an  ellipse  (x2/a2  +  ?/2/&2  =  l)  ;  and,  if  the  affixe  of 
u  describes  a  circle  about  the  origin,  then  the  affixe  of  v  describes  a  quartic 
curve,  which,  in  the  particular  case  where  the  radius  of  the  circle  described  by 
the  affixe  of  u  is  2,  breaks  up  into  two  circles  whose  centres  are  on  the  i-axis. 

(46.)  If  a;  and  y  be  real,  and  x  +  y  =  \,  show  that  the  affixe  of  xzl  +  yz2  lies 
on  the  line  joining  the  affixes  of  zx  and  ».,.  Hence  show  that  the  affixe  of 
xzx  +  yz2  lies  on  a  fixed  straight  line  provided  lx  +  my—l,  I  and  m  being 
constants. 

(47.)  If  £  +  ij£  be  an  imaginary  root  of  iE3  +  2cc  + 1  =  0,  prove  that  (£,  ij)  is 
one  of  the  intersections  of  the  graphs  of  ?j2  =  3£2+2  and  ??2  =  l/2  +  3/8£. 
Draw  the  graphs  :  and  mark  the  intersections  which  correspond  to  the  roots 
of  the  equation. 

If  o  be  the  real  root  of  this  cubic,  show  that  the  imaginary  roots  are 
H-a+*V(2-3/a)}. 

(48.)  If  £±r)i  be  a  pair  of  imaginary  roots  of  o?-px  +  q  =  0,  show  that 
(if,  tj)  are  co-ordinates  of  the  real  intersections  of  3£2-  i)2-p  =  0,  8^rj-  +  2p^- 
3q  =  0.  Hence  prove  that  the  roots  of  the  cubic  are  all  real,  or  one  real  and 
two  imaginary,  according  as  4p3<  >27ga.     What  happens  if  4ps=272a  ? 

(49.)  If  x3  +  qx  +  r  =  Q  has  imaginary  roots,  the  real  part  of  each  is  posi- 
tive or  negative  according  as  r  is  positive  or  negative. 

(50.)  The  cubic  x3  -  9a;2  +  33a:-  65  =  0  has  an  imaginary  root  whose 
modulus  is  N/13  ;  find  all  its  roots. 

(51.)  Find  the  real  quadratic  factors  of  x2n  +  x2"-1+  ...  +1  ;  and  hence 
prove  that 

o„    •        if        ■        27r  .       nir  ,,_       , . 

2    'Sm2„  +  1  Sin  S+l  '  "  '  Sm  2^Tl=  ^2"  +  1>- 


(52.)  Find  in  rational  integral  form  the  equation  which  results  by 
eliminating  6  from  the  equations  x  —  a  cos  0  +  b  cos  30,  y  =  a  smd+b  sin  36. 
(Use    Demoivre's    Theorem.)      Give   a   geometrical   interpretation    of  your 

analysis. 

Historical  Note. — Imaginary  quantities  appear  for  the  first  time  in  the  works 
of  the  Italian  mathematicians  of  the  16th  century.  Cardano,  in  his  Artie  Magna 
sive  de  Rcgvlis  Algebraicis  Liber  Units  (1545),  points  out  (cap.  xxxvii.,  p.  66) 
that,  if  we  solve  in  the  usual  way  the  problem  to  divide  10  into  two  parts  whose 
product  shall  be  40,  we  arrive  at  two  formula?  which,  in  modern  notation,  may 
be  written  5  +  *J  -  15,  5  -  N'  -  15.  He  leaves  his  reader  to  imagine  the  meaning 
of  these  "sophistic"  numbers,  but  shows  that,  if  we  add  and  multiply  them 
in  formal  accordance  with  the  ordinary  algebraic  rules,  their  sum  and  product 
do  come  out  as  required  in  the  evidently  impossible  problem  ;  and  he  adds 
"  hucusque  progreditur  Arithmetics  subtilitas,  cujus  hoc  extremum  ut  dixi  adeo 
est  subtile,  ut  sit  inutile."  Bombelli  in  his  Algebra  (1522),  following  Cardano, 
devoted  considerable  attention  to  the  theory  of  complex  numbers,  more  especially 
in  connection  with  the  solution  of  cubic  equations. 


254  HISTORICAL  NOTE 


CHAP  XII. 


There  is  clear  indication  in  the  fragment  De  Arte  Logistica  (see  above,  p.  201) 
that  Napier  was  in  possession  to  some  extent  at  least  of  the  theory.  He  was 
fully  cognisant  of  the  independent  existence  of  negative  quantity  ("quantitates 
defectives  minores  nihilo"),  and  draws  a  clear  distinction  between  the  roots  of 
positive  and  of  negative  numbers.  He  points  out  (Napier's  Ed.,  p.  85)  that 
roots  of  even  order  have  no  real  value,  either  positive  or  negative,  when  the 
radicand  is  negative.  Such  roots  he  calls  "  nugacia "  ;  and  expressly  warns 
against  the  error  of  supposing  that  J_|  -  9=  -  M  9.  In  this  passage  there  occurs 
the  curious  sentence,  "  Hujus  arcani  magni  algebraici  fundamentum  superius, 
Lib.  i.  cap.  6,  jecimus  :  quod  (quamvis  a  nemine  quod  sciam  revelatum  sit)  quan- 
tum tamen  emolumeuti  adferat  huic  arti,  et  cseteris  mathematicis  postea  patebit." 
There  is  nothing  farther  in  the  fragment  De  Arte  Logistica  to  show  how  deeply  he 
had  penetrated  the  secret  which  was  to  be  hidden  from  mathematicians  for  200 
years. 

The  theory  of  imaginaries  received  little  notice  \mtil  attention  was  drawn  to 
it  by  the  brilliant  results  to  which  the  use  of  them  led  Euler  (1707-1783)  and  his 
contemporaries  and  followers.  Notwithstanding  the  use  made  by  Euler  and 
others  of  complex  numbers  in  many  important  investigations,  the  fundamental 
principles  of  their  logic  were  little  attended  to,  if  not  entirely  misunderstood. 
To  Argand  belongs  the  honour  of  first  clearing  up  the  matter  in  his  Essai 
sur  une  maniere  de  representer  les  quantites  imaginaires  dans  les  constructions 
geometriques  (1806).  He  there  gives  geometrical  constructions  for  the  sum  and 
product  of  two  complex  numbers,  and  deduces  a  variety  of  conclusions  therefrom. 
He  also  was  one  of  the  first  to  thoroughly  understand  and  answer  the  question  of 
§  21  regarding  the  existence  of  a  root  of  every  integral  function.  Argand  was  an- 
ticipated to  a  considerable  extent  by  a  Danish  mathematician,  Caspar  Wessel,  who 
in  1797  presented  to  the  Royal  Academy  of  Denmark  a  remarkable  memoir  Om 
Direktionens  ancdytiske  Betegning,  et  Forslig,  anvendt  fwncmmelig  til  plane  og 
sphaeriske  Polygoners  Opliisning ,  which  was  published  by  the  Academy  in  1799, 
but  lay  absolutely  unknown  to  mathematicians,  till  it  was  republished  by  the 
same  body  in  1897.  See  an  interesting  address  by  Beman  to  Section  A  of  the 
American  Association  for  the  Promotion  of  Science  (1897).  Even  Argand's  results 
appear  to  have  been  at  first  little  noticed  ;  and,  as  a  matter  of  history,  it  was 
Gauss  who  first  initiated  mathematicians  into  the  true  theory  of  the  imaginaries  of 
ordinary  algebra.  He  first  used  the  phrase  com2>lex  number,  and  introduced  the 
use  of  the  symbol  i  for  the  imaginary  unit.  He  illustrated  the  twofold  nature  of 
a  complex  number  by  means  of  a  diagram,  as  Argand  had  done  ;  gave  a  masterly 
discussion  of  the  fundamental  principles  of  the  subject  in  his  memoir  on  Bi- 
quadratic Residues  (1831)  (see  his  Works,  vol.  ii.,  pp.  101  and  171)  ;  and  furnished 
three  distinct  proofs  (the  first  published  in  1799)  of  the  proposition  that  every 
equation  has  a  root. 

From  the  researches  of  Cauchy  (1789-1857)  and  Riemann  (1826-1866)  on 
complex  numbers  has  sprung  a  great  branch  of  modern  pure  mathematics,  called 
on  the  Continent  function  -  theory.  The  student  who  wishes  to  attain  a  full 
comprehension  of  the  generality  of  even  the  more  elementary  theorems  of  algebraic 
analysis  will  find  a  knowledge  of  the  theory  of  complex  quantity  indispensable  ; 
and  without  it  he  will  find  entrance  into  many  parts  of  the  higher  mathematics 
impossible. 

For  further  information  we  may  refer  the  reader  to  Peacock's  Algebra,  vol.  ii. 
(1845)  ;  to  De  Morgan's  Trigonometry  and  Double  Algebra  (1849),  where  a  list 
of  most  of  the  English  writings  on  the  subject  is  given  ;  and  to  Hankel's 
Vorlesungen  ilber  die  complexen  Zahlen  (1867),  where  a  full  historical  account 
of  Continental  researches  will  be  found.  It  may  not  be  amiss  to  add  that  the 
theory  of  complex  numbers  is  closely  allied  to  Hamilton's  theory  of  Quaternions, 
Grassmami's  Ausdehuuugslehre,  and  their  modern  developments. 


CHAPTER    XIII. 
Ratio  and  Proportion. 

RATIO   AND    PROPORTION    OF   ABSTRACT    QUANTITIES. 

§  1.]  The  ratio  of  the  abstract  quantity  a  to  the  abstract  quantity 
b  is  simply  the  quotient  of  a  by  b. 

When  the  quotient  a  -s-  b,  or  a/h,  or  y  is  spoken  of  as  a  ratio, 

it  is  often  written  a :  b ;  a  is  called  the  antecedent  and  b  the  con- 
sequent of  the  ratio. 

There  is  a  certain  convenience  in  introducing  this  new  name, 
and  even  the  new  fourth  notation,  for  a  quotient.  So  far,  how- 
ever, as  mere  abstract  quantity  is  concerned,  the  propositions 
which  we  proceed  to  develop  are  simply  results  in  the  theory 
of  algebraical  quotients,  arising  from  certain  conditions  to  which 
we  subject  the  quantities  considered. 

If  a  >  b,  that  is,  if  a  -  b  be  positive,  a  :  b  is  said  to  be  a  ratio 
of  greater  inequality. 

If  a  <  b,  that  is,  if  a  -  b  be  negative,  a  :  b  is  said  to  be  a  ratio 
of  less  inequality. 

When  two  ratios  are  multiplied  together,  they  arc  said  to  be 

compounded.     Thus,  the  ratio  aa' :  bb'  is  said  to  be  compounded  of 

the  ratios  a  :  b  and  a' :  V. 

The  compound  of  two  equal  ratios,  a :  b  and  a  :  b,  namely, 

a2 :  b2,  is  called  the  duplicate  of  the  ratio  a  :  b. 

Similarly,  of  :  b3  is  the  triplicate  of  the  ratio  a  :  5.* 

*  Formerly  a2  :  b-  was  spoken  of  as  the  double  of  the  ratio  a  :  b.     Similarly 

.i     * 
\Ja  :  \/b  was  called  the  half  or  subduplicate  of  a  :  b,  and  a2 :  b*  the  sesquipli- 

cate  of  a  :  b. 


256  PROPERTIES  OF  A  RATIO  chap. 

§  2.]  Four  abstract  numbers,  a,  b,  c,  d,  are  said  to  be  proportional 
when  the  ratio  a:b  is  equal  to  the  ratio  c :  d. 
We  then  write 

a  :  b  =  c  :  d* 

a  and  d  are  called  the  extremes,  and  b  and  c  the  means,  of  the  pro- 
portion,    a  and  c  are  said  to  be  homologues,  and  b  and  d  to  be 

homologu.es. 

If  a,  b,  c,  d,  e,  f,  &c,  be  such  that  a :  b  =  b  :  c  =  i :  d  =  d :  e  =  e  :f 
=  &c,  a,  b,  c,  d,  e,  f,  &c,  are  said  to  be  in  continued  proportion. 

If  a,  b,  c  be  in  continued  proportion,  b  is  said  to  be  a  mean 
proportional  between  a  and  c. 

If  a,  b,  c,  d  be  in  continued  proportion,  b  and  c  are  said  to  be 
two  mean  proportionals  between  a  and  d ;  and  so  on. 

§  3.]  If  b  be  positive,  and  a>b,  the  ratio  a:b  is  diminished  by 
adding  the  same  positive  quantity  to  both  antecedent  and  consequent  ; 
and  increased  by  subtracting  the  same  positive  quantity  (<b)  from 
both  antecedent  and  consequent. 

If  a<b,  the  words  "increased"  and  "diminished"  must  be  inter- 
changed in  the  above  statement. 

a  +  x     a     b(a  +  x)  -  a(b  +  x) 


For, 


b  +  x     b  b(b  +  x) 

x(b  -  a) 


b(b  +  x)' 

Now,  if  a  >  b,  b-a  is  negative  ;  and  x,  b,  b  +  x  are  all  positive 
by  the  conditions  imposed  ;  hence  x(b  -  a)jb(b  +  x)  is  negative. 

TT  a  +  x     a  . 

Hence  7 — ■ 7  is  negative, 

b  +  x     b 

,                                             a  +  x     a 
that  is,  t <  r. 

'  b  +  x     b 

a-  x     a     x(a  -  b) 

Ac;ain,  ■? t  =  777 r- 

0      '  b  -  x     b     b(b  -  x) 

But,  since  a  >  b,  a-b  is  positive,  and  x  and  b  are  positive,  and, 
since  x<b,  b-x  is  positive.     Hence  x(a  -  b)/b(b  -  x)  is  positive. 


*  Formerly  in  writing  proportions  the  sign  :  :  (originally  introduced  by 
Oughtred)  was  used  instead  of  the  ordinary  sign  of  equality. 


Xlll  PERMUTATIONS  OF  A  PROPORTION  257 

TT  a  —  x     a 

Hence  -. >  -. 

b  —  x     b 

The  rest  of  the  proposition  may  be  established  in  like  manner. 

The  reader  will  obtain  an  instructive  view  of  this  proposition 
by  comparing  it  with  Exercise  7,  p.  267. 

§  4.]  Permutations  of  a  Proportion. 

(1), 
(2), 
(3), 
(4). 


If 

a:b  =  c:d 

then 

b:a  =  d:c 

a  :c  =  b:d 

and 

c  :a  =  d  :b 

For,  from  (1),  we  have 

a     c 
b  =  d' 

Hence 

'b     V 

that  is, 

b_d 

a     c ' 

that  is, 

b  :  a-d:  c, 

which  establishes  (2). 

Again,  from  (1), 

a     c 
1  =  7v 

multiplying  both  sides  by  -,  we  have 

a     b     c     b 
b     c     d     c 

that  is,  -  =  - , ; 

c     d 

that  is,  a:c  =  b:  d, 

which  proves  (3). 

(4)  follows  from  (3)  in  the  same  way  as  (2)  from  (1). 

§  5.]  The  product  of  the  extremes  of  a  proportion  is  equal  to  the 
product  of  the  means  ;  and,  conversely,  if  the  product  of  two  quantities 
be  equal  to  the  product  of  two  others,  the  four  form  a  proportion,  the 
extremes  being  tlie  constituents  of  one  of  the  products,  the  means  the 
constituents  of  the  other. 

VOL.  J  S 


258 

RULE  OF  THREE 

For,  if 

a :  b  =  c  :  d, 

that  is, 

a     c 
b  =  d' 

then 

-  x  bd  =  - :  x  bd, 
b            d 

whence 

ad  =  be. 

Again,  if 

ad  =  be, 

then 

ad/bd  =  bc/bd, 

whence 

a     c 
b~d' 

CHAP. 


Cor.  If  three  of  the  terms  of  a  proportion  be  given,  the  remaining 
one  is  uniquely  determined. 

For,  when  three  of  the  quantities  a,  b,  c,  d  are  given,  the  equation 

ad  =  be, 

which  results  by  the  above  from  their  being  in  proportion,  be- 
comes an  equation  of  the  1st  degree  (see  chap,  xvi.)  to  deter- 
mine the  remaining  one. 

Suppose,  for  example,  that  the  1st,  3rd,  and  4th  terms  of  the  proportion 
are  I,  %,  and  f  ;  and  let  x  denote  the  unknown  2nd  term. 

Then  *:<*=*:*; 

whence  %y.x  =  \x%. 

Multiplying  hy  f ,  we  have  x=|xf  xf, 

_  o 

—  3TT- 

§  6.]  Relations  connecting  quantities  in  continued  proportion. 
If  three  quantities,  a,  b,  c,  be  in  continued  proportion,  then 

2       72  72         2 

a  :  c  =  a  :  b  =  b  :  c  ; 
and  b  =  \Z(ac). 

If  four  quantities,  a,  b,  c,  d,  be  in  continued  proportion,  then 
a:d  =  aa:  b'  =  b'  :  c3  =  c3 :  d3, 
and  b  =  'i/(a\l),     c  =  t/(ad*). 

For  the  general  proposition,  see  Exercise  12,  p.  267. 


XIII 


DETERMINATION  OF  MEAN  PROPORTIONALS 


259 


For,  if 

then 

Therefore 
whence 


a :  b 


b  :c, 
a  _b 
b~~c 


a     b     b     b 

~   X  -  =  -  X   -. 

0 


(!)• 


c     c     c 

c~  c2~  Ir 
Also  ac  =  b2, 

whence  b  =  \/(ac)  (2). 

Equations  (1)  and  (2)  establish  the  first  of  the  two  proposi- 


tions  above  stated. 

Again,  if 

a\b  =  b:c  =  c:d, 

then 

abac 
b     c     b     d" 

Also 

a     a 
b  =  b' 

hence 

a     a     a     a     b     c 

that  is, 

a3     a 
b3  =  d' 

therefore 

a     a3     b3     ca 
d~b3~c3~d3 

Further,  since 

a     a3 
d=b3' 

b3  —  ci'd ; 

whence 

b  =  l/(a*d). 

Also,  since 

a     c3 
d     d3' 

c3  =  ad2 ; 

whence 

c  =  l/{ad2) 

(3). 


(4> 


(5). 

It  should  be  noticed  that  the  result  (2)  shows  that  the  finding  of  a  mean 
proportional  between  two  given  quantities  a  and  c  depends  on  the  extraction 
of  a  square  root.     For  example,  the  mean  proportional  between  1  and  2  is 

V(l  x  2)  =  V2  =  1-4142  .   .   . 


260  DELTAN  PROBLEM 


CHAP. 


Again,  (i)  and  (5)  enable  us  to  insert  two  mean  proportionals  between  two 
given  quantities  by  extracting  certain  cube  roots.  For  example,  the  two 
mean  proportionals  between  1  and  2  are 

^(lx  2)  =4/2  =  1*2599  .  .  . 

and  V/(lx22)  =  ^- =1-5874  .  .   . 

Conversely,  of  course,  the  finding  of  the  cube  root  of  2,  which  again  corre- 
sponds to  the  famous  Delian  problem  of  antiquity,  the  duplication  of  the 
cube,  could  be  made  to  depend  on  the  finding  of  two  mean  proportionals,  a 
result  well  known  to  the  Greek  geometers  of  Plato's  time. 

§  7.]  After  what  has  been  done,  the  student  will  have  no 
difficulty  in  showing  that 


(2). 


if 

a  :b  =  c:d, 

then 

ma  :mb  =  nc:  nd 

and 

ma  :  nb  =  me  :  nd 

§8.] 
if 

Also  that 

al:bi  =  cl:d1, 
a±  \  o2  =  c2 :  «2> 

an  '.  on  =  en  :  an, 

then 

a,<i,2 . . .  an 

:  6,6S .  . .  bn  =  ca  .  .  .  cn 

■  d/h 

Cor. 

If 

a  •  b  =  c  :  d, 

then 

an  .  ^  =  cn  :  dn. 

.dn  (1). 


(Here  n,  see  chap,  x.,  may  he  positive  or  negative,  integral  or 
fractional,  provided  an,  &c,  be  real,  and  of  the  same  sign  as  a, 
&c.) 

§9.]  //  a:b  =  c:d, 

then  a±b  :b  =  c±d:d  (1), 

a  +  b:  a  -b  =  c  +  d  :  c  -  d  (2), 

la  +  mb  :  pa  +  qb  =  lc+  md  \pc  +  qd  (3), 

lar  +  mbr  :  par  +  qbr  =  lcr  +  mdr  :pcr  +  qd"  (4), 

where  I,  m,  p,  q,  r  are  any  quantities,  positive  or  negative. 


xiil  CONSEQUENCES  OF  PROPORTION  261 

Also,  if  a, :  b,  =  a2 :  ba  =  az :  b3  =  .   .  .  =  an  :  in, 

a,  +  a.,  +  .  .   .  +  an  :  6a  +  b3  +  .  .  .  +  &„  (5) ; 

and  afeo  fo 

;/(/,<  +  W  +  •  •  •  +  W) :  W  +  U>/  +  •  ■  ■  +  W)  (6). 

Though  outwardly  somewhat  different  in  appearance,  these 
six  results  are  in  reality  very  much  allied.  Two  different 
methods  of  proof  are  usually  given. 


FIRST    METHOD. 

Let  us  take,  for  example,  (1)  and  (2). 

„.  a     c 

bince  T  =  -, 

b     d 

in  a     i      c 

therefore  =-  ±  1  =  •=  ±  1  : 

b  a 

a±b     c  ±  d 
whence  — -= —  =  — 5—  ; 

b  d 

this  establishes  the  two  results  in  (1). 
Writing  these  separately  we  have 

a  +  b     c  +  d 


b           d    ' 

a  -  b     c  -  d 

b           d    ' 

whence 

(a  +  b), 

h      I 

'  (a-b)     (c  +  d)/  (c-  d) 
b             d    1        d     ' 

that  is, 

a+b     c+d 
a-b     c  —  d' 

which  establishes  (2). 

Similar 

treatment 

may  be  applied  to  the   rest  of   the   six 

results. 

2G2  EXPRESSION  IN  TERMS  OF  FEWEST  VARIABLES  chap. 


SECOND    METHOD. 

Let  us  take,  for  example,  (2). 

Since  a/b  =  c/d,  we  may  denote  each  of  these  ratios  by  the 
same  symbol,  p,  say.     We  then  have 


a 

c 

whence 

a  =  pb, 

c  =  pd 

Now, 

using  (a), 

Ave  have 

a  +  b 

pb  +  b 

a-b 

"  pb-b' 
b(P+l) 

~b(p-iy 

p  +  i 
-p-v 

In  exactly 

the  i 

same  way,  we 

!  have 

c  +  d 

pd  +  d 

c-d 

' pd-  d' 

p+l 
-p-V 

Hence 

a  +  b     p  + 
a-b     p- 

1      c  +  d 
1  "  c  -  d' 

Again 

,  let 

us  take  (5). 

We  h: 

ive 

a, 

a2     a3 

Zh~b3~  •   • 

.  =  — ,  each 

i  =P 

say, 

hence 

( 

h  =  p 

K    <k  =  ph, 

.   .   .,     an 

=  pbi 

l  5 

therefore 

«i 

+  do 

+  .  .   .  +an 

pbl  +  pb.2  + 
bx  +  b.2  + 

•  •  • 

+  pbn 

h 

+  K 

+  .  .   .  +  bn 

+  bn  ' 

p(K  +  h  + 

.  .  . 

+  bn) 

bl  +  bi+  . 

+  b»  ' 

hence 

=  P, 

a, 
6, 

a2 

-  &C    -  n  -  ffl 

+  a2+  .   .   . 

+  an 

—  iVL,   —  p  —    , 

+  b2  +  .  .   . 

+  bn 

(a). 


XIII 


GENERAL  THEOREM  2G3 


Finally,  let  us  take  (G). 

Since  a/  =  (tAY  =  p'V, 

a/  =  (ph2y  =  p>V,  &c. 

we  have 

y(ifi*  +  W+  ■  •  •  +  W)  =  V(pr(iAr  +  W+  ■  ■  ■  +inb/)), 

(see  chap,  x.,  §  4).     It  follows  that 

y(/,o,r  +  W  +  •  ■   ■  +  ln(hir)  =    _  a,  =  a*  _  &(j 

;/(ZAr  +  w  +  ■  ■  •  +  W«r)    p    ^    ^ 

Of  the  two  methods  there  can  be  no  doubt  that  the  second 
is  the  clearer  and  more  effective.  The  secret  of  its  power  lies 
in  the  following  principle  : — 

In  establishing  an  equation,  between  conditioned  quantities,  if  ice 
first  express  all  the  quantities  involved  in  the  equation  in  terms  of  the 
fewest  quantities  possible  under  the  conditions,  then  the  verification  of 
the  equation  involves  merely  the  establishment  of  an  algebraical  identity. 
In  establishing  (2),  for  instance,  we  expressed  all  the  quantities 
involved  in  terms  of  the  three  b,  d,  p,  so  many  being  necessary, 
by  §  5,  to  determine  a  proportion. 

A  good  deal  of  the  art  of  algebraical  manipulation  consists 
in  adroitly  taking  advantage  of  this  principle,  without  at  the 
same  time  destroying  the  symmetry  of  the  functions  involved. 

§  10.]  The  following  general  theorem  contains,  directly  or 
indirectly,  all  the  results  of  last  article  as  particular  cases  ;  and 
will  be  found  to  be  a  compendium  of  a  very  large  class  of 
favourite  exercises  on  the  present  subject,  some  of  which  will 
be  found  at  the  end  of  the  present  paragraph. 

If  <M''i>  ■''■_•>  •  •  .,  x„)  be  any  homogeneous  integral  function  of  the 
variables  it,,  x.2,  .  .  .,  xa  of  the  rth  degree,  or  a  homogeneous  function 
of  degree  r,  according  to  the  extended  notion  of  homogeneity  and 
degree  give<i  at  the  foot  of  p.  73,  and  if 

«!  :  bl  =  a.,:  b.,=  .   .   .  =  an  :  bn, 

then  each  of  these  ratios  is  equal  to 


264  EXAMPLES  chap. 

This  theorem  is  an  immediate  consequence  of  the  property 
of  homogeneous  functions  given  in  chap,  iv.,  p.  73. 

Example  1. 

AV  Inch  is  the  greater  ratio,  x2  +  y2  :  x  +  y,  or  x--y":x-y,  x  and  y  being 
each  positive  ? 

x2  +  y2    x2-y2_  (x2  +  y'2)  (x-y)-  {x2  -  y2)  (x  +  y) 
x  +  y  ~  x-y  ~  (x  +  y)(x-y) 

2xy2  -  2x2y 
~{x  +  y)(x-y)' 

_       2xy(x  -  y) 

{x  +  y)(x-y)' 
_       2xy  ^ 

x+y 

Now,  if  x  and  y  be  each  positive,  -2xyj(x  +  y)  is  essentially  negative. 
Hence 

x2  +  y2  :  x  +  y  <  x2  -  y2  :  x  -  y. 

Example  2. 

If  a:b=c;d,  and  A:B  =  C:D,   then   ci\/A  -  b\/B  :  c>s/C-ds/D  =  asJA 

+  6VB:cVC+dVD- 

Let  each  of  the  ratios  a :  b  and  c  :d  =  p,  and  each  of  the  two  A  :  B  and 
C  :  D  =  <r,  then  a  =  pb,  c  —  pd;  A  =  <rB,  C  =  crD.     A\7e  then  have 

as/ A  -  b  VB  _  pb  V(<rB)  -  b  VB 

(pV<r-l)&VB  _  K/B 

(p\/<r-l)d\/D    dsJV 
In  the  same  way  we  get 

a\/A  +  bK/B=  (PsJ<r  +  l)bsJB     K/B 

cVC  +  ^V^     (pV<r  +  l)rfv'D     rfV^ 
From  (a)  and  (j8)  the  required  result  follows. 


(a). 

(/3). 


Example  3. 

If  b  be  a  mean  proportional  between  a  and  c,  show  that 

(a+b  +  c)(a-b  +  c)  =  a2  +  b2  +  c2  (a), 

and  {a  +  b  +  c)2  +  d-  +  b2  +  c3  =  2(a  +  b  +  c){a  +  c)  (j8). 

Taking  (a)  we  have 

(a+i+c)(a-6+c)=(a+c+6)(a+c-6), 
=  (a+c)2-62. 
Now,  by  data,  a/b  =  b/c,  and  therefore  b'2  =  ac  ;  hence 

(«  +  c)2  -  b2 = (a  +  c)2  -  ac, 
=  a2  +  OC  +  C1, 
=  a-  +  b-  +  c-, 
since  b2  =  ac.     Hence  (a)  is  proved. 


XIII 


EXAMPLES  265 


Taking  now  (/3),  and,  for  variety,  adopting  the  second  method  of  §  9,  let 

us  put 

a     b 

b=C=P' 

Hence  a  —  pb,  b  —  pc;  so  that  a  =  pipe)  =  p~c. 
We  have  to  verify  the  identity 

(p-c  +  pc  +  cf  +  (j?cf  +  {pcf  +  c2  =  2(p-c  +  pc  +  c){p-c  +  c)  ; 
that  is  to  say, 

{(ffi  +  p+l)*  +  (j,*  +  l?  +  l)}<*  =  2(?  +  p  +  l)((?+l)c>  (7). 

Now 

{(p-  +  P  +  l)2  +  (^  +  r^-l)^•2=(p2+/»  +  l){(p2  +  p  +  l)  +  (/)••!-p  +  l)}c'•!, 

=  2(p2  +  p  +  I)(p2  +  l)c2, 
which  proves  the  truth  of  (7),  and  therefore  establishes  (j8). 

Example  4.* 

If  x/(b +e-a)  =  yl(c  +  0  -b)  =  zfta  +  b-c),  then  (b-c)x  +  (c-a)y  +  (a-b)z  =  0. 
Let  us  put 

a       _       V       _       z       _ 
b+c-a    c+a-b     a+b -c 

then  x  =  (b  +  c-a)p, 

y  =  (c  +  a-b)p, 
z  =  {a  +  b-  c)p. 
Now,  from  the  last  three  equations,  we  have — 
{b  -  c)x  +  (c  -  a)y  +  (a  -  b)z 

=  (b  -c)(b  +  c  -a)p  +  (c-a)(c  +  a  -  b)p+  (a-b)(a  +  b-c)p, 
=  {(S8  -  c2  +  c-  -  a2  +  a2  -  b'2)  -  (a(b  -c)  +  b(c  -  a)  +  e(a  -b))}p, 

=  {0-0}* 

=  0. 

Example  5. 

If  bz  +  cy  _cx  +  az  _ay  +  bx 

b-c        c-a        a- b 
then  (a  +  b  +  c)(x  +  y  +  z)=ax  +  by  +  cz  (2). 

Let  each  of  the  ratios  in  (1)  be  equal  to  p,  then 

bz  +  cy  =  p(b-c)  (3), 

cx  +  az  =  p(c-a)  (4), 

ay  +  bx  —  p(a-b)  (5). 

From  (3),  (4),  (5),  by  addition, 

(b  +  c)x+(c  +  a)y+  (a  +  b)z  =  p{  (b  -  c)  +  (c-a)  +  («  -b)}, 

=  p0, 

=  0  (6). 

If  now  we  add  ax  +  by  +  cz  to  both  sides  of  (6)  we  obtain  equation  (2). 

*  Examples  4,  5,  and  6  illustrate  a  species  of  algebraical  transformation 
which  is  very  common  in  geometrical  applications.  In  reality  they  are  ex- 
amples of  a  process  which  is  considered  more  fully  in  chap.  xiv. 


(1), 


266  EXAMPLES 

Example  6. 

If  cy  +  bz  az  +  cx  bx  +  ay 

qb  +  rc-  pa     re  +}M  -  qb    pa  +  qb-  re 
show  that 

x 
a  {pa(a  +  b  +  c)  -  qb(a  +  b-c)-  rc(a  -  b  +  c)  } 

y 


CHAI\ 


(1), 


b{qb(a  +  b  +  c)  -pa(a  +  b - c)  -rc(  -a  +  b  +  c)} 

z 


(2). 


c  {rc(a  +  b  +  c)-qb(- a  +  b  +  c)  -pa(a  -  b  +  c) } 
Let   each   of  the    fractions  of  (1)  be  =  p;  and    observe   that   the   three 

equations, 

cy  +  bz=(qb  +rc  -'pa)p  (a)  ~| 

az  +  ex  =  [re  +}>a  -  qb)p  (/3)   J-  (3), 

be  +  ay  —  {pa  +  qb  -  rc)p  (7)  J 

fa**) 

which  thus  arise  are  symmetrical  in  the  triple  set -J  abc  Y,  so  that  the  simul- 

[pqr) 

taneous  interchange  of  the  letters  in  two  of  the  vertical  columns  simply 
changes  each  of  the  equations  (3)  into  another  of  the  same  set.  It  follows, 
then,  that  a  similar  interchange  made  in  any  equation  derived  from  (3)  will 
derive  therefrom  another  equation  also  derivable  from  (3). 

Now,  if  we  multiply  both  sides  of  (j3)  by  b,  and  both  sides  of  (7)  by  c,  we 
obtain,  by  addition  from  the  two  equations  thus  derived, 

2bcx  +  a{cy  +  bz}  =p{b(rc+2>a-qb)  +  c{pa  +  qb-rc)}  (4). 

Now,  using  the  value  of  cy  +  bz  given  by  (a),  we  have 

2bcx  +  pa(qb  +  re  - 2m)  =  p {pa(b  +  c)  -  qb(b  -  c)  -rc(  -b  +  c)}         (5). 

Subtracting  pa(qb  +  rc-pa)  from  both  sides  of  (5),  we  have 

Ibex  =  p  {pa{a  +  b  +  c)-  qb(a  +  b-c)-  rc(a  -  b  +  e) }  (6). 

From  (6),  we  have 

? =P.  (7). 

a{pa{a  +  b  +  c)-qb[a  +  b-c)  -re(a-  b  +  c)}     2abc 

/xap\  /xap\ 

We  may  in  (7)  make  the  interchange   I  into  I,  or  I  into  I,  and  we  shall 

\  ybq  /  \  zcr  ' 

obtain  two  other  equations  derivable  from  (3)  by  a  process  like  that  used  to 
derive  (7)  itself.  These  interchanges  leave  the  right-hand  side  of  (7)  un- 
altered, but  change  the  left-hand  side  into  the  second  and  third  members  of 
(2)  respectively.  Hence  the  three  members  of  (2)  are  all  equal,  each  being  in 
fact  equal  to  pj2abc. 

This  is  a  good  example  of  the  use  of  the  principle  of  symmetry  in  compli- 
cated algebraical  calculations. 


xiii  EXERCISES  XVII  2G7 


Exercises  XVII. 

(1.)  Which  is  the  greater  ratio,  5 :  7  or  151  :  208  ? 

(2. )  If  the  ratio  3  :  4  be  duplicated  by  subtracting  x  from  both  antecedent 
and  consequent,  show  that  a'  =  lf. 

(3.)  What  quantity  x  added  to  the  antecedent  and  to  the  consequent  of 
a  :  b  will  convert  this  ratio  into  c  :  d  ? 

(4.)  Find  the  fourth  proportional  to  3£,  5|,  6| ;  also  the  third  proportional 
to  1  +  V2  and  3  +  2\/2. 

(5.)  Insert  a  mean  proportional  between  11  anil  19  ;  and  also  two  mean 
proportionals  between  the  same  two  numbers. 

(6.)  Find  a  simple  surd  number  which  shall  be  a  mean  proportional  be- 
tween \J7  -  \/5  and  11V7+ 13\/5- 

(7.)  If  x  and  y  be  such  that  when  they  are  added  to  the  antecedent  and 
consequent  respectively  of  the  ratio  a :  b  its  value  is  unaltered,  show  that 
x:y  =  a  :b. 

(8. )  If  x  and  y  be  such  that  when  they  are  added  respectively  to  the  ante- 
cedent and  consequent  and  to  the  consequent  and  antecedent  of  a  :  b  the  two 
resulting  ratios  are  equal,  show  that  either  x  =  y  or  x  +  y  =  -  a—b. 

(9.)  Find  a  quantity  x  such  that  when  it  is  added  to  the  four  given  quan- 
tities a,  b,  c,  d  the  result  is  four  quantities  in  proportion.  Exemplify  with 
3,  4,  9,  13  ;  and  with  3,  4,  1£,  2. 

(10.)  If  four  quantities  be  proportional,  the  sum  of  the  greatest  and  least 
is  always  greater  than  the  sum  of  the  other  two. 

(11.)  If  the  ratio  of  the  difference  of  the  antecedents  of  two  ratios  to  the 
sum  of  their  consequents  is  equal  to  the  difference  of  the  two  ratios,  then  the 
antecedents  are  in  the  duplicate  ratio  of  the  consequents. 

(12.)  If  the  n  quantities  d\,  a.2,  .  .  .,  on  be  in  continued  proportion,  then 
m  :  an  =  a1"-1 :  aan-1=aa"~1  :  a-i11'1  =  &c.  ;  and 

a,=  "'^(a1"--an),     as=  VW-V,,),     .   .   .,     «P=  "v/("i"-'Vr,1'-1). 
(13.)  If  (pa+qb+rc+sd)(pa-qb-rc+sd) 

=  {pa-qb  +  rc-  sd)  (pa  +  qb-rc-  sd), 
then  be  :  ad  =ps  :  qr  ; 

and,  if  either  of  the  two  sets  a,  b,  c,  d  or  p,  q,  r,  s  form  a  proportion,  the 
other  will  also. 

(14.)  If  a: b=c:d=e:f, 
then  a3  +  3an-b  +  b*:c3  +  Zc-d  +  cP  =  a*  +  &' :  c3  +  d3  (a)  ; 

//«V     «V     eV\  f(bd-     b"P     d-f-\ 

=  a\lf+  csb/+  c*bd  :  b3cc  +  tPae  +J*ac     (/3)  ; 
pa  -  qc  +  re:pb-qd+  rf=  ^/ace  :  y/bdf 

=  vV  -  c°-  + e"  +  2ac) :  V(&2  - cp  +f  +  -hd)    M- 


268  EXERCISES  XVII  chap. 

t 

(15.)  Ua:a'=b:b', 

then  «'"+"  +  a'"b"  +  &"•+"  : «'"'+"  +  a'mb'"  +  b>mr< " 

=  («.  +  ft)»'+":  («'  +  ft')"!+". 

(16.)  If  «:&  =  c  :  rf,  and  a  1/3  =  7:  5, 
then  «3a2  +  (a2ft  +  aft2)a/3  +  ft3/32  :  (a3  +  ft3)  (a2  +  /32) 

=  cV  +  (c2^  +  (5^)75  +  d382  :  (c3  +  d3)  (y~  +  8s). 

(17.)  If  a:  b  =  b  :c  =  c:d,  then 

[a?  +  ft2  +  e2)  (ft2  +  c2  +  d2)  =  (ab  +  be  +  cdf  (a)  ; 

(ft  -  c)2  +  (c  -  a)2  +  (d  -  ft)2  =  (a  -  d)2  (j8)  ; 

«ft  +  crf  +  ft^=(«  +  ft  +  c)(ft-c  +  f?)  (7); 

a  +  6-c-tf  =  (a  +  ft)(ft-f0/ft  (0); 

(a  +  6  +  c  +  a")  (a-  ft  -  6  +  0")  =  2(aft  -  erf)  (ac  -  bd)/(ad  +  ftc)  (e). 

(IS.)  If  a,  ft,  c  be  in  continued  proportion, 

then  a2  +  aft  +  ft2  :  b2  +  be  +  c2  =  a  :  c  (a); 

a2(«-ft  +  c)(a  +  ft  +  c)  =  «4  +  a2ft2  +  ft4  (/3)  ; 

(ft  +  c)2/(ft-f)  +  (c  +  «)2/(c-«)  +  (a  +  ft)2/(«-ft)  =  4ft(a  +  ft  +  c)/(«-c)  (7). 

(19.)  If  a,  ft,  c,  d  he  in  continued  proportion, 

then  («-c)(ft-rf)-(«-^)(?'-c)  =  (&-c)2  (a); 

V(a*)W(k)+V(«9=V{(« +*+«)(* +«+/>}  (£)■ 

(20.)  Uab=cd=ef,  then 

(ac  +  ce  +  ea)/dbf(d  +  ft  +/)  =  (a2  +  c2  +  e2)/(ft2d2  +  d2/2  +/'-ft-'). 

(21.)  If  (a-J)/(rf-e)=(6-c)/(e-/)1  then  each  of  them 

=  {b(f-d)  +  (cd-af)\/c(f-d). 

(22.)  Ul;/yx=vli?=tfyz,  thenx/^  =  y/e  =  ^vi-. 
(23.)  If        2a!+3y:3i/+4z:43+5aj=4a-56:3ft-o:26-3aJ 
then  7a;  +  6y+8«=0. 

(24.)  If  ax  +  cy  :by  +  dz  =  ay  +  cz:bz  +  dx  =  az  +  ex  :  bx  +  dy,  and  if 
x  +  y  +  z  +  0,  ab-cd  +  0,  ad-bc  +  0,  then  each  of  these  ratios  =a  +  c  :  ft  +  d  ; 
and  x2  +  y2  +  z2  =  yz  +  zx  +  xy. 

(25.)  If  (a  -  ny  +  mz)jl'  =  (b-7z  +  nx)/m'=(c  -  <mx  +  ly)/n',  then 
/  m'c-n'b      \n_f  ii'a-l'c       \,     _f  /'ft  -  m'a      \ ,    » 

V X  "  K'  +  mm'  +  MwV '       ^ y  '  U'+mm'+nn'J 'm~[z~U'  +  m m'  +  n n'J'71' 


RATIO    AND    PROPORTION    OF    CONCRETE    QUANTITIES. 

§  11.]  AVe  have  now  to  consider  how  the  theorems  Ave  have 
established  regarding  the  ratio  and  proportion  of  abstract  num- 
bers are  to  be  applied  to  concrete  quantities.     We  shall  base 

*  Important  in  the  theory  of  the  central  axis  of  a  system  of  forces,  &c. 


xill  CONCRETE  RATIO  AND  PROPORTION  2G9 

this  application  on  the  theory  of  units.  This,  for  practical  pur- 
poses, is  the  most  convenient  course,  but  the  student  is  not  to 
suppose  that  it  is  the  only  one  open  to  us.  It  may  be  well  to 
recall  once  more  that  any  theory  may  be  expressed  in  algebraical 
symbols,  provided  the  fundamental  principles  of  its  logic  are  in 
agreement  with  the  fundamental  laws  of  algebraical  operation. 

§  12.]  If  A  and  B  be  two  concrete  quantities  of  the  same  hind, 
which  are  expressible  in  terms  of  one  and  the  same  unit  by  the  com- 
mensurable numbers  a  and  b  respectively,  then  the  ratio  of  A  to  B  is 
defined  to  be  the  ratio  or  quotient  of  these  abstract  numbers,  namely, 
a  :  b,  or  ajb. 

It  should  be  observed  that,  by  properly  choosing  the  unit,  the  ratio  of 
two  concrete  quantities  which  are  each  commensurable  with  any  finite  unit  at 
all  can  always  be  expressed  as  the  ratio  of  two  integral  numbers.  For  ex- 
ample, if  the  quantities  be  lengths  of  Z\  feet  and  4f  feet  respectively,  then, 
by  taking  for  unit  |th  of  a  foot,  the  quantities  are  expressible  by  26  and  35 
respectively  ;  and  the  ratio  is  26  :  35.  This  follows  also  from  the  algebraical 
theorem  that  (3  +  £)/(4  +  |)  =  26/35. 

If  A,  B  be  two  concrete  quantities  of  the  same  kind,  whose  ratio  is 
a :  b,  and  C,  D  two  other  concrete  quantities  of  the  same  kind  {but  not 
necessarily  of  the  same  kind  as  A  and  B),  whose  ratio  is  c:d,  then 
A,  B,  C,  D  are  said  to  be  proportional  when  the  ratio  of  A  to  B  is 
equal  to  the  ratio  of  C  to  D,  that  is,  wht  n 

a:b  =  c:  d. 

We  may  speak  of  the  ratio  A :  B,  of  the  concrete  magnitudes 
themselves,  and  of  the  proportion  A  :  B  =  C  :  D,  without  alluding 
explicitly  to  the  abstract  numbers  which  measure  the  ratios  ;  but 
all  conclusions  regarding  these  ratios  will,  in  our  present  manner 
of  treating  them,  be  interpretations  of  algebraical  results  such  as 
we  have  been  developing  in  the  earlier  part  of  this  chapter, 
obtained  by  operating  with  a,  b,  c,  d.  The  theory  of  the  ratio 
and  proportion  of  concrete  quantity  is  thus  brought  under  the 
theory  of  the  ratio  and  proportion  of  abstract  quantities. 

There  are,  however,  several  points  which  require  a  nearer 
examination. 

§  13.]  In  the  first  place,  it  must  be  noticed  that  in  a  concrete 


270 


SPECIAL  POINTS  IN  CONCRETE  PROPORTION 


CHAP. 


ratio  the  antecedent  and  the  consequent  must  be  quantities  of  the 
same  kind  ;  and  in  a  concrete  proportion  the  two  first  terms  must 
be  alike  in  kind,  and  the  two  last  alike  in  kind.  Thus,  from  the 
present  point  of  view  at  least,  there  is  no  sense  in  speaking  of 
the  ratio  of  an  area  to  a  line,  or  of  a  ton  of  coals  to  a  sum  of 
money.  Accordingly,  some  of  the  propositions  proved  above — 
those  regarding  the  permutations  of  a  proportion,  for  instance — 
could  not  be  immediately  cited  as  true  regarding  a  proportion 
among  four  concrete  magnitudes,  unless  all  the  four  were  of  the 
same  kind. 

This,  however,  is  a  mere  matter  of  the  interpretation  of 
algebraical  formulae — a  matter,  in  short,  regarding  the  putting  of 
a  problem  into,  and  the  removing  of  it  from,  the  algebraical 
machine. 

§  14.]  A  more  important  question  arises  from  the  considera- 
tion that,  if  we  take  two  concrete 
magnitudes  of  the  same  kind  at  random, 
there  is  no  reason  to  expect  that  there 
exists  any  unit  in  terms  of  which  each 
is  exactly  expressible  by  means  of  com- 
mensurable numbers. 

Let  us  consider,  for  example,  the 
historically  famous  case  of  the  side  AB 
and  diagonal  AC  of  a  square  ABCD.  On  the  diagonal  AC  lay 
off  AF  =  AB,  and  draw  FE  perpendicular  to  AC.  It  may  be 
readily  shown  that 


3 

A 

E 

/ 

\ 

\ 

SF 

\ 

c 

\ 

D 

Hence 


BE  =  EF  =  FC. 
CF  =  AC  -  AB 
CE  =  CB  -  CF 


(2). 


Now,  if  AB  and  AC  were  each  commensurably  expressible  in 
terms  of  any  finite  unit,  each  would,  by  the  remark  in  §  1 2,  be  an 
integral  multiple  of  a  certain  finite  unit.  But  from  (1)  it  follows 
that  if  this  were  so,  CF  would  be  an  integral  multiple  of  the 
same  unit  j  and,  again,  from  (2),  that  CE  would  be  an  integral 
multiple  of  the  same  unit.  Now  CF  and  CE  are  the  side  and 
diagonal  of  a  square,  CFEG-,  whose  side  is  less  than  half  the  side 


xiu  COMMENSURABLES  AND  INCOMMENSURABLES  271 

of  ABCD;  and  from  CFEG  could  in  turn  be  derived  a  still 
smaller  square  whose  side  and  diagonal  would  be  integral  mul- 
tiples of  our  supposed  unit ;  and  so  on,  until  we  had  a  square 
as  small  as  we  please,  whose  side  and  diagonal  are  integral 
multiples  of  a  finite  unit;  which  is  absurd.  Hence  the  side 
and  diagonal  of  a  square  are  not  magnitudes  such  as  A  and  B 
are  supposed  to  be  in  our  definition  of  concrete  ratio. 

§  15.]  The  difficulty  which  thus  arises  in  the  theory  of  con- 
crete ratio  is  surmounted  as  follows  : — 

We  assume,  as  axiomatic  regarding  concrete  ratio,  that  if 
A'  and  A"  be  two  quantities  respectively  less  and  greater  than 
A,  then  the  ratio  A  :  B  is  greater  than  A' ;  B  and  less  than 
A"  :  B  ;  and  we  show  that  A'  and  A"  can  be  found  such  that, 
while  each  is  commensurable  with  B,  they  differ  from  each  other, 
and  therefore  each  differs  from  A  by  as  little  as  we  please. 

Suppose,  in  fact,  that  we  take  for  our  unit  the  nth  part  of  B, 
then  there  will  be  two  consecutive  integral  multiples  of  Bjn,  say 
mB/n  and  (m  +  l)Bfn,  between  which  A  will  lie.  Take  these 
for  our  values  of  A'  and  A" ;  then 

A"  -  A'  =  (m  +  1)B/tc  -  mBjn, 

=  B>. 

Hence  A"  -  A'  can,  by  sufficiently  increasing  n,  be  made  as  small 
as  Ave  please. 

We  thus  obtain,  in  accordance  with  the  definition  of  §  12, 
two  ratios,  m\n  and  (m  +  l)/n,  between  which  the  ratio  A  :  B  lies, 
each  of  which  may  be  made  to  differ  from  A  :  B  by  as  little  as 
we  please. 

Practically  speaking,  then,  we  can  find  for  the  ratio  of  two 
incommensurables  an  expression  which  shall  be  as  accurate  as 
we  please.     Regarding  this  matter,  see  vol.  ii.,  chap,  xxv.,  §§  26-41. 

Example. 

If  B  be  the  side  and  A  the  diagonal  of  a  square,  to  find  a  rational  value 
of  A  :  B  which  shall  be  correct  to  l/1000th. 

If  we  take  for  unit  the  l/1000th  part  of  B,  then  B  =  1000,  and  A2  = 
2,000,000.  Now  1414'-'=  1999396,  and  14152  =  2002225.  Hence  1414/I00O 
<A/B<  1415/1 000.  But  1415/1000-1414/1000  =  1/1000.  Hence  we  have 
A/B  =  1-414,  the  error  being  <  1/1000. 


272  EUCLIDIAN  THEORY  OF  PROPORTION  chap. 

§  16.]  The  theory  of  proportion  given  in  Euclid's  Elements  gets  over  the 
difficulty  of  incommensurables  in  a  very  ingenious  although  indirect  manner. 
No  working  definition  of  a  ratio  is  attempted,  but  the  proportionality  of  four 
magnitudes  is  defined  substantially  as  follows  : — 

If  there  be  four  magnitudes  A,  B,  C,  D,  such  that,  always, 

mk>,  =  ,  or  <«B, 
according  as  mC>,  =,  or  <?;D, 

m  and  n  being  any  integral  numbers  whatsoever,  then  A,  B,  C,  D  are  said  to 
be  proportional. 

Here  no  use  is  made  of  the  notion  of  a  unit,  so  that  the  difficulty  of  in- 
commensurability is  not  raised.  On  the  other  hand,  there  is  substituted  a 
somewhat  indirect  and  complicated  method  for  testing  the  subsistence  or  non- 
subsistence  of  proportion  ality. 

It  is  easy  to  see  that,  if  A,  B,  0,  D  be  proportional  according  to  the 

algebraical  definition,  they  have  the  property  of  Euclid's  definition.     For,  if 

a:b  and  c :  d  be  the  numerical  measures  of  the  ratios  A  :B  and"C:D,  we 

have 

a  _c 

b~d' 

,  ma    mc 

hence  — r  = — ,, 

no      nd 

from  which  it  follows  that  ma>,  —,  or  <nb,  according  as  mc> ,  =,  or  <nd. 

The  converse,  namely,   that,  if  A,  B,  C,  D  be  proportional  according  to 

Euclid's  definition,  then 

a  _c 

can  be  proved  by  means  of  the  following  lemma. 

Given  any  commensurable  quantity  ajb,  another  commensurable  quantity 
can  be  found  which  shall  exceed  or  fall  short  of  a/b  by  as  little  as  we  please. 

Let  n  be  an  integral  number,  and  let  mb  be  the  least  multiple  of  b  which 
exceeds  na,  so  that 

na—mb-r, 
where  r  <  b. 

Dividing  both  sides  of  this  equation  by  rib,  we  have 

a  _  in      r 
b     u     nb  ' 

,  m     a      r 

whence  T  =  _i;» 

n     b     vb 

so  that  m/n  exceeds  a/b  by  r/nb.  Now,  since  r  never  exceeds  the  given 
quantity  b,  by  making  n  sufficiently  great,  we  can  make  r/nb  as  small  as  we 
plea.se  ;  that  is  to  say,  we  can  make  m/n  exceed  a/b  by  as  little  as  we  please. 

Similarly  we  may  show  that  another  commensurable  quantity  may  be 
found  falling  short  of  a/b  by  as  little  as  we  please. 

From  this  it  follows  that,  if  two  commensurable  quantities  differ  by  ever  so 
little,  we  can  always  find  another  commensurable  quantity  which  lies  between 


xui  COMPARISON  OF  THEORIES  273 

them  ;  for  we  can  find  another  commensurable  quantity  which  exceeds  tlic 
less  of  the  two  by  less  than  the  difference  between  it  and  the  greater. 
Suppose  now  that 

ma  >,  =,  or  <nb, 
according  as  mo,  —,  or  <nd, 

m  and  n  being  any  integers  whatever,  then  we  must  have 

a  _  c 
b~d' 
For,  if  these  fractions  (which  we  may  suppose  to  be  commensurable  by 
virtue  of  §  15)  dilfer  by  ever  so  little,  it  will   be  possible  to  find  another 
fraction,  n/m  say,  where  n  and  m  are  integers,  which  lies  between  them. 
Hence,  if  a/b  be  the  less  of  the  two,  we  must  have 

t<  —  ,  that  is,  ma  <  nb  ; 
b    m 

->  — .  that  is,  mond. 
d    m 

In  other  words  we  have  found  two  integers,  m  and  n,  such  that  we  have 
at  once 

ma  <  nb 
and  mond. 

But,  by  hypothesis,  when  ma<nb,  we  must  have  mc<nd.     Hence  the 
fractions  a/b  and  c/d  cannot  be  unequal. 


VARIATION. 

§  17.]  There  are  an  infinite  number  of  ways  in  which  we 
may  conceive  one  quantity  y  to  depend  upon,  be  calculable  from, 
or,  in  technical  mathematical  language,  be  a  function  of,  another 
quantity  x.     Thus  we  may  have,  for  example, 

y  =  3&, 

y  =17/, 

y  =  ax  +  b, 

y  =  ax2  +  bx  +  c, 

y='2  \fx, 
and  so  on. 

For  convenience  x  is  called  the  independent  variable,  and  y  the 
dependent  variable  ;  because  we  imagine  that  any  value  we  please 
is  given  to  x,  and  the  corresponding  value  of  y  derived  from  it 
by  means  of  the  functional  relation.  All  the  other  symbols  of 
quantity  that  occur  in  the  above  equations,  such  as  3,  17,  a,  b,  c, 
VOL.  I  T 


274  INDEPENDENT  AND  DEPENDENT  VARIABLE  chap. 

2,  &c,  are  supposed  to  remain  fixed,  and  are  therefore  called 
constants. 

Here  we  attach  meanings  to  the  words  variable  and  constant 
more  in  accordance  with  their  use  in  popular  language  than 
those  given  above  (chap,  ii.,  §  6). 

The  justification  of  the  double  usage,  if  not  already  apparent, 
will  be  more  fully  understood  when  Ave  come  to  discuss  the 
theory  of  equations,  and  to  consider  more  fully  the  variations  of 
functions  of  various  kinds  (see  chaps,  xv.-xviii.) 

§  18.]  In  the  meantime,  we  propose  to  discuss  very  briefly 
the  simplest  of  all  cases  of  the  functional  dependence  of  one 
quantity  upon  another,  that,  namely,  which  is  characterised  by 
the  following  property. 

Let  the  following  scheme 


Values  of 
the  Independent  Variable. 

Corresponding  Values  of  the 
Dependent  Variable. 

X 

x' 

V 

y 

denote  any  two  corresponding  pairs  whatever  of  values  of  the 
independent  and  dependent  variables,  then  the  dependence  is  to 
be  such  that  always 

y:y'  =  x:x'  (1). 

It  is  obvious  that  this  property  completely  determines  the 
nature  of  the  dependence  of  y  upon  x,  as  soon  as  any  single  cor- 
responding pair  of  values  are  given.  Suppose,  in  fact,  that, 
when  x  has  the  value  x0,  y  has  the  value  y0,  then,  by  (1), 

y      x 

y0~x0' 

whence  y  =  (  —  )x. 

Now  we  may  keep  xu  and  y„  as  a  fixed  standard  pair,  for 
reference  as  it  were ;  their  ratio  y0/x0  is  therefore  a  given  con- 


Xlll  SIMPLEST  CASE  OF  FUNCTIONAL  DEPENDENCE  275 

stant  quantity,  which  we  may  denote  by  a,  say.  We  therefore 
have 

V  =  ax  (2), 

that  is  to  say,  y  is  a  given  constant  multiple  of  x ;  or,  in  the 
language  of  chap,  iv.,  §  17,  a  homogeneous  integral  function  of  x 
of  the  1st  degree. 

Example.  Let  us  suppose  that  we  have  for  any  two  corresponding  pairs 
y,  x  and  y',  x'  the  relation  y  :x  =  y'  :x'  ;  and  that  when  x=Z,  y  =  6-  Then 
since  6  and  3  are  corresponding  pairs  y  :x=6  :3.  Hence  y/x  —  6/B  =  2. 
Hence  y  =  2x. 

Conversely,  of  course,  the  property  (2)  leads  to  the  property 
(1).     For,  from  (2), 

y  =  ax ; 

hence,  if  x'  and  y'  be  other  two  corresponding  values, 

y'  =  ax'. 

y      ax      x 
Hence  '—~  — ,  =  —  • 

y      ax      x 

When  y  depends  on  x  in  the  manner  just  explained  it  is  said 
to  vary  directly  as  x,  or,  more  shortly,  to  vary  as  x. 

A  better  *  phrase,  which  is  also  in  use,  is  "  y  is  proportional 
to  x." 

This   particular   connection   between  y  and  x  is   sometimes 

expressed  by  writing 

y<^x. 

§  19.]  In  place  of  x,  we  might  write  in  equation  (2)  x2,  l/x, 
1/x2,  x  +  b,  and  so  on  ;  we  should  then  have 

y  =  ax2  (a), 

y  =  ajx  ((3), 

y  =  a\i  (y), 

y  =  a(x  +  b)  (8). 

*  The  use  of  the  word  "  Variation  "  in  the  present  connection  is  unfortunate, 
because  the  qualifying  particle  "  as  "  is  all  that  indicates  that  we  are  here 
concerned  not  with  variation  in  general,  as  explained  in  §  17,  but  merely  with 
the  simplest  of  all  the  possible  kinds  of  it.  There  is  a  tendency  in  uneducated 
minds  to  suppose  that  this  simplest  of  all  kinds  of  functionality  is  the  only 
one  ;  and  this  tendency  is  encouraged  by  the  retention  of  the  above  piece  of 
antiquated  nomenclature. 


276  OTHER  SIMPLE  CASES  chap. 

The  corresponding  forms  of  equation  (1)  would  then  be 

V  : :'/  =  X2 :  X"  (a'), 

y:y'  =  llx:l/x'  (ft'), 

T.y  =  1/aM/i"  (/), 

y.y'  =  x  +  b:  x'  +  b  (8'). 

y  is  then  said  to  vary  as,  or  be  proportioned  to,  x2,  l/'x,  Ijx2, 
x  +  b.  In  cases  (ft)  and  (y)  y  is  sometimes  said  to  vary  inversely 
as  x,  and  inversely  as  the  square  of  x  respectively. 

Still  more  generally,  instead  of  supposing  the  dependent 
variable  to  depend  on  one  independent  variable,  we  may  suppose 
the  dependent  variable  u  to  depend  on  two  or  more  independent 
variables,  x,  y,  z,  &c. 

For  example,  we  may  have,  corresponding  to  (2), 


and,  corresponding  to  (1), 


u  =  axy 

(4 

u  =  axyz 

(0, 

u  =  a(x  +  y) 

(v), 

u  =  ax/y 

{0); 

u :  to'  =  xy :  x'y' 

(0, 

u  :  m'  =  xyz :  x'y'z' 

(0, 

u:u'  =  x  +  y.  x'  +  y 

(v')> 

to  :  u'  =  xjy :  x'jy' 

(d'\ 

In  case  (e)  u  is  sometimes  said  to  vary  as  x  and  y  jointly ; 
in  case  (6)  directly  as  x  and  inversely  as  y. 

§  20.]  The  whole  matter  we  are  now  discussing  is  to  a  large 
extent  an  affair  of  nomenclature  and  notation,  and  a  little 
attention  to  these  points  is  all  that  the  student  will  require  to 
prove  the  following  propositions.  We  give  the  demonstrations 
in  one  or  two  specimen  cases. 

(1 .)  If  z°=y  and  y  ^  x,  then  z<=>=x. 

Proof. — By  data  z  =  ay,  y  =  bx,  where  a  and  b  are  constants  ; 
therefore  z  =  dbx.     Hence  z^x,  since  ah  is  constant. 

(2.)  If  yi'xxl  and  y2^x2,  then  yxy2 °=  ;<•/.,. 

Proof. — By  data  yt  =  axxlt  y2  =  a^,  where  a,  and  a2  are  con- 


XIII 


PROPOSITIONS  REGARDING  VARIATION 


277 


stants.  Hence  y$9  =  a^v^,  which  proves  the  proposition,  since 
ai«2  is  constant. 

In  general  if  y,^-x„  y,^x,,  .  .  .,  yn<=^xn,  then  yly2...yn 
oc  #,£2 . . .  xw     And,  in  particular,  if  y  cc  x,  then  yn  <^  xn. 

(3.)  If  y°zx,  then  zy°czx,  whether  z  be  variable  or  constant. 

(4.)  If  zozxy,  then  x^zjy,  and  y^zjx. 

(5.)  If  z  depend  on  x  and  y,  and  on  these  alone,  and  if  z^x 
when  y  is  constant,  and  z°^y  when  x  is  constant,  then  z  °=  xy  when 
both  x  and  y  wry. 

Proof. — Consider  the  following  system  of  corresponding 
values  of  the  variables  involved. 


Dependent  Variable. 

Independent  Variables. 

Z 

z' 

x,  y. 
x',  y. 
x',  y'. 

Then,  since  y  lias  the  same  value  for  both  z  and  zu  we  have, 

by  data, 

z      x 


2,       X 

Again,  since  x'  is  the  same  for  both  zl 

and  z',  we  have,  by 

data, 

»i    y 

z'     y- 

From  these  two  equations  we  have 

z      zx     x     y 

7  x  I7  =  v  x  7? ' 
Zi     z      x     y 

1.1.  l  •                                         z      xy 

thatls'                          ?-*?■ 

which  proves  that  z^xy. 

A  good  example  of  this  case  is  the  dependence  of  the  area  of  a  triangle 
upon  its  base  and  altitude. 


278  EXAMPLES  chap. 

"We  have 

Area  oc  base  (altitude  constant) ; 
Area  oc  altitude  (base  constant). 
Hence  area  oc  base  x  altitude,  when  both  vary. 

(6.)  In  a  similar  manner  we  may  prove  that  if  z  depend  on 
xl ,  x2,  .  .  . ,  xn,  and  on  these  alone,  and  vary  as  any  one  of  these  when 
the  rest  remain  constant,  then  z  oc  xxx2 .  .  .  xn  when  all  vary. 

(7.)  If  zee x  (y  constant)  and  z<^l/y  (x  constant),  then  z<>=x/y 
when  both  vary. 

For  example,  if  V,  P,  T  denote  the  volume,  pressure,  and  absolute  tem- 
perature of  a  given  mass  of  a  perfect  gas,  then 

V  oc  1/P  (T  constant),  V  oc  T  (P  constant). 
Hence  in  general  V  oc  T/P. 

Example  1. 

If  s  oc  t2  when/ is  constant,  and  s  oc/ when  t  is  constant,  and  2s=/ when 
t  =  \,  find  the  relation  connecting  s,  f,  t. 

It  follows  by  a  slight  extension  of  §  20  (5)  that,  when/ and  t  both  vary, 
s  <xft2.     Hence  s  =  aft",  where  a  is  a  constant,  which  we  have  to  determine. 

Now,  when  t  =  l,  s  =  \f,  hence  \f=afl2,  that  is,  \f—af\  in  other  words, 
we  must  have  a—h.     The  relation  required  is,  therefore,  s  —  \ffi. 

Example  2. 

The  thickness  of  a  grindstone  is  unaltered  in  the  using,  but  its  radius 
gradually  diminishes.  By  how  much  must  its  radius  diminish  before  the 
half  of  its  mass  is  worn  away  ?  Given  that  the  mass  varies  directly  as  the 
square  of  the  radius  when  the  thickness  remains  unaltered. 

Let  m  denote  the  mass,  r  the  radius,  then  by  data,  m  =  ar-,  where  a  is 
constant. 

Let  now  r  become  ?•',  and,  in  consequence,  m  become  Jm,  then  b>i  =  ar'2, 
hence 


ar'2 

_hn 

: 

ar2 

~  m' 

r>2 

r- 

=h; 

r' 

l 

— 

^  

r 

\A 

that  is, 

whence 

It  follows,  therefore,  that  the  radius  of  the  stone  must  be  diminished  in 
the  ratio  1 :  V2. 

Example  3. 

A  ami  B  are  partners  in  a  business  in  which  their  interests  are  in  the 
ratio  a  :  b.  They  admit  C  to  the  partnership,  without  altering  the  whole 
amount  of  capital,  in  such  a  way  that  the  interests  of  the  three  partners  in 
the  business  are  then  equal.     C  contributes  £c  to  the  capital  of  the  firm. 


XIII 


EXERCISES  XVIII  279 


How  is  the  sum  £c  which  is  withdrawn  from  the  capital  to  be  divided  between 
A  and  B  ?  and  what  capital  had  each  in  the  business  originally  ? 

Solution. — Since  what  C  pays  in  is  his  share  of  the  capital,  they  each  have 
finally  £c  in  the  business  ;  let  now  £x  be  A's  share  of  C's  payment,  so  that 
£{c-x)  is  B's  share  of  the  same.  In  effect,  A  takes  £x  and  B  £(c-x)  out 
of  the  business.  Hence  they  had  originally  £{c  +  x)  and  £(c  +  c-x)  in  the 
business.     By  data,  then,  we  must  have 

c  +  x  _a 
2c-x~b' 
hence  b(c  +  x)  =  a(2c-x) ; 

we  have,  therefore,  bc  +  bx  —  2ac  -  ax. 

From  this  last  equation  we  derive,  by  adding  ax  -  be  to  both  sides, 

{a  +  b)x=(2a-b)c. 

Heuce,  dividing  by  a  +  b,  we  have 

xJ2a-V)c 

a  +  b  v  ' 

Hence  c-x=c-- 


a  +  b 
(2b-a)c 
a  +  b 


(2). 


It  appears,  then,  that  A  and  B  take  £(2a  -  b)c/{a  +  b)  and  £{2b  -  a)c/(a  +  b) 
respectively  out  of  the  business.  C's  payment  must  be  divided  between  them 
in  the  ratio  of  these  sums,  that  is,  in  the  ratio  2a- b  :2b -a.  They  had  in 
the  business  originally  £3ac/(a  +  b)  and  £3bc/(a  +  b)  respectively. 


Exercises  XVIII. 

(1.)  Ifyccx,  and  if  y  =  3§  when  a;  =  6i,  find  the  value  of  y  when  a-=g. 

(2. )  y  varies  inversely  as  x2 ;  and  z  varies  directly  as  ,<:-.  When  x=  2,  y  +  z 
=  340  ;  when  ar=l,  ?/-c  =  1275.     For  what  value  of  a;  is  y  =  zl 

(3.)  zeeu-v;  uxx;  vecxr.  When  x  =  2,  s  =  48  ;  when  x  =  5,  z  =  30. 
For  what  values  of  x  is  c  =  0  ? 

(4.)  If  xy  oc  x2  +  y'2,  and  x  =  Z  when  y  =  4,  find  the  equation  connecting 
y  and  x. 

(5.)  If  x  +  y<xx-y,  then  x2  +  y2<x  xy  and  oP  +  y3  <x  .ri/(.>-±y). 

(6.)  If  {x  +  y  +  z)(x  +  y-z)(x-y  +  z)(  -x  +  y  +  z)  oc  x'hf,  then  either  x*  +  y2 
oc  zr  or  xr  ■>-  y  —  z-  oc  xy. 

(7.)  Hxxy,  then  x2  +  y2cc  xy. 

(8. )  If  a*  +  \  «  x3 -  i,  then  y  <x.  Ifx. 

(9. )  If  x  oc  y2,  y3  oc  z4,  z5  oc  ue,  tt7  oc  ^  then  (x/v)  (y/v)  (z/v)  (ujv)  is  constant. 
(10.)  Two  trains  take  3  seconds  to  clear  each  other  when  passing   in 
opposite  directions,  and  35  seconds  when  passing  in  the  same  direction  :  find 
the  ratio  of  their  velocities. 


280  EXERCISES  XVIII  chap,  xiii 

(11.)  A  watch  loses  2\  minutes  per  day.  It  is  set  right  on  the  15th  March 
at  1  p.m.  :  what  will  the  proper  time  be  when  it  indicates  9  A.M.  on  the  20th 
April  1 

(12.)  A  small  disc  is  placed  between  two  infinitely  small  sources  of  radiant 
heat  of  equal  intensity,  at  a  point  on  the  line  joining  them  equidistant  from 
the  two.  It  is  then  moved  parallel  to  itself  through  a  distance  aj2\/S  towards 
one  of  the  two  sources,  a  being  the  distance  between  them  :  show  that  the 
whole  radiation  falling  on  the  disc  is  trebled. 

(The  radiation  falling  on  the  disc  varies  inversely  as  the  square  of  the  dis- 
tance from  the  source,  when  the  disc  is  moved  parallel  to  itself  towards  or 
from  the  source.) 

(13.)  The  radius  of  a  cylinder  is  ?•,  and  its  height  h.  It  is  found  that  by 
increasing  either  its  radius  or  its  height  by  x  its  volume  is  increased  by  the 
same  amount.  Show  that  x  =  r(r-2h),'h.  "What  condition  is  there  upon  r 
and  h  in  order  that  the  problem  may  be  possible  ? 

(Given  that  the  volume  of  a  cylinder  varies  directly  as  its  height  when 
its  radius  is  constant,  and  directly  as  the  square  of  its  radius  when  its  height 
is  constant.) 

(14.)  A  solid  spherical  mass  of  glass,  1  inch  in  diameter,  is  blown  into  a 
shell  bounded  by  two  concentric  spheres,  the  diameter  of  the  outer  one  being 
3  inches.  Calculate  the  thickness  of  the  shell.  (The  volume  of  a  sphere 
varies  directly  as  the  cube  of  its  diameter. ) 

(15.)  Find,  the  radius  of  a  sphere  whose  volume  is  the  sum  of  the  volumes 
of  two  spheres  whose  radii  are  3^  feet  and  6  feet  respectively. 

(16.)  Two  equal  vessels  contain  spirits  and  water,  the  ratios  of  the  amount 
of  spirit  to  the  amount  of  water  being  p  :  1  and  p :  1  respectively.  The  con- 
tents of  the  two  are  mixed  :  show  that  the  ratio  of  the  amount  of  spirit  to  the 
amount  of  water  in  the  mixture  is  p  +  p'  +  2pp'  :2  +  p  +  p'. 


CHAPTER    XIV. 
On  Conditional  Equations  in  General. 

DEFINITIONS    AND    GENERAL    NOTIONS. 

§  1 .]  It  will  be  useful  for  the  student  at  this  stage  to  attempt 
to  form  a  wider  conception  than  we  have  hitherto  presupposed  of 
what  is  meant  by  an  analytical  function  in  general.  Dividing  the 
subjects  of  operation  into  variables  (x,  y,  z,  .  .  .)  and  constants 
(a,  b,  c,  .  .  .),  we  have  already  seen  what  is  meant  by  a  rational 
integral  algebraical  function  of  the  variables  x,  y,  z,  .  .  .;  and  we 
have  also  had  occasion  to  consider  rational  fractional  algebraical 
functions  of  x,  y,  z,  .  .  .  We  saw  that  in  distinguishing  the 
nature  of  such  functions  attention  was  paid  to  the  way  in  which 
the  variables  alone  were  involved  in  the  function.  We  have  already 
been  led  to  consider  functions  like  s/(x  +  Jy),  or  %/(x  +  >/y), 
or  ax*  +  bx-  +  c,  where  the  variables  are  involved  by  way  of  root 
extraction.  Such  functions  as  these  are  called  irrational  alge- 
braical functions.  These  varieties  exhaust  the  category  of  what 
are  usually  called  Ordinary  *  Algebraical  Functions,  In  short,  any 
intelligible  concatenation  of  operations,  in  which  the  operands  selected 
for  notice  and  called  the  variables  are  involved  in  no  other  ways  than 
by  addition,  subtraction,  multiplication,  division,  and  root  extraction,  is 
called  an  Ordinary  Algebraical  Function  of  these  variables. 

Although  Ave  have  thus  exhausted  the  category  of  ordinary 
algebraical  functions,  we  have  by  no  means  exhausted  the  possi- 

*  The  adjective  "  Ordinary  "  is  introduced  to  distinguish  the  class  of  func- 
tions here  defined  from  algebraical  functions  as  more  generally  denned  in 
chap,  xxx.,  §  10.  The  word  "Synthetic"  is  often  used  for  "Ordinary"  in 
the  present  connection. 


282 


CONDITIONAL  AND  IDENTICAL  EQUATIONS 


CHAP. 


bilities  of  analytical  expression.  Consider  for  example  a*  where, 
as  usual,  x  denotes  a  variable  and  a  a  constant.  Here  x  is  not 
involved  in  any  of  the  Avays  recognised  in  the  definition  of  an 
algebraical  function,  but  appears  as  an  index  or  exponent.  ax  is 
therefore  called  an  exponential  function  of  x.  It  should  be  care- 
fully noted  that  the  discrimination  turns  solely  on  the  way  in 
which  the  variable  enters.  Thus,  while  ax  is  an  exponential 
function  of  x,  x0,  is  an  algebraical  function  of  x.  There  are  other 
functions  in  ordinary  use, — for  example,  sin  a',  logic, — and  an 
infinity  besides  that  might  be  imagined,  which  do  not  come 
under  the  category  of  algebraical ;  all  such,  for  the  present,  we 
class  under  the  general  title  of  transcendental  functions,  so  that 
transcendental  simply  means  non-algebraical.  We  use  the  term 
analytical  function,  or  simply  function,  to  include  all  functions, 
Avhether  algebraical  or  transcendental,  and  we  denote  a  function 
of  the  variables  x,  y,  z,  .  .  .,  in  which  the  constants  a,  b,  c,  .  .  . 
are  also  involved,  by 

4>(x,  y,  z,  .  .  .  a,  b,  c,  .  .  .); 
or,  if  explicit  mention  of  the  constants  is  unnecessary,  by 

<f>(x,  y,  z,  .   .   .). 

§  2.]  Consider  any  two  functions  whatever,  say  cf>(x,  y,  z,  .  .  . 
a,  b,  c,  .  .  .),  and  if(x,  y,  z,  .  .  .  a,  b,  c,  .  .  .),  of  the  variables 
x,  y,  z,  .   .  .,  involving  the  constants  a,  b,  c,  .   .   . 

If  the  equation 
<f>(z,  y,z,  .  .  .  a,  b,  c,  .  .   .)  =  f(z,  y,  z,  .  .  .  a,  b,  c,  .  .  .)  (1) 
be  such  that  the  left-hand  side  can,  for  all  values  of  the  variables 
x,  y,  z,  .  .   .,  be  transformed  into  the  right  by  merely  apply- 
ing the  fundamental  laws  of   algebra,   it    is    called  an  identity. 
With  equations  of  this  kind  the  student  is  already  very  familiar. 

If,  on  the  other  hand,  the  left-hand  side  of  the  equation  (1) 
can  be  transformed  into  the  right  only  when  x,  y,  z,  .  .  .  have 
certain  values,  or  are  conditioned  in  some  way,  then  it  is  said  to  be 
a  Conditioned  Equation,  or  an  Equation  of  Condition.*     Examples 

*  "When  it  is  necessary  to  distinguish  between  an  equation  of  identity  and 
an  equation  of  condition,  the  sign  =  is  used  for  the  former,  and  the  sign  = 
for  the  latter.     Thus,  we  should  write  [x  + 1) (»- l)=u? - 1  j  but  1c  +  2  =  2. 


xiv  CLASSIFICATION  OF  EQUATIONS  283 

of  such  equations  have  already  occurred,  more  especially  in  chap, 
xiii.  One  of  the  earliest  may  be  seen  in  chap,  iv.,  §  24,  where, 
inter  alia,  it  was  required  to  determine  B  so  that  we  should 
have  2B  +  2  =  2  ;  in  other  words,  to  find  a  value  of  x  to  satisfy 
the  equation 

2x+2  =  2  (2). 

Here  2x  +  2  can  be  transformed  into  2  when  (and,  as  we 
shall  hereafter  see,  only  when)  x  =  0. 

Every  determinate  problem,  wherein  it  is  required  to  deter- 
mine certain  unknown  quantities  in  terms  of  certain  other  given 
or  known  quantities  by  means  of  certain  given  conditions,  leads, 
when  expressed  in  analytical  language,  to  one  or  more  equations 
of  condition ;  to  as  many  equations,  in  fact,  as  there  are  condi- 
tions. The  quantities  involved  are  therefore  divided  into  two 
classes,  known  and  unknown.  The  known  quantities  are  denoted 
by  the  so-called  constant  letters  ;  the  unknown  by  the  variable 
letters.  Hence,  in  the  present  chapter,  constant  and  known  are 
convertible  terms ;  and  so  are  variable  and  unknown.  The  con- 
stants may  be  actual  numerical  quantities,  real  and  positive  or 
negative  (-4,  -\,  0,  +1,  +  f ,  &c),  or  imaginary  or  complex 
numbers  (  -  i,  1  +  2i,  &c);  or  they  may  be  letters  standing  for 
any  such  quantities  in  general. 

§  3.]  Equations  are  classified  according  to  their  form,  and 
according  to  the  number  of  variables  that  occur  in  them. 

If  transcendental  functions  appear,  as,  for  example,  in 
2*  =  2>x  +  2,  the  equation  is  said  to  be  transcendental.  With 
such  for  the  present  we  shall  have  little  to  do. 

If  only  the  ordinary  algebraical  functions  appear,  as,  for 
example,  in  «/(jc  +  y)  +  \/(x  -  y)  =  1 ,  the  equation  is  called  an 
algebraical  equation.  Such  an  equation  may,  of  course,  be 
rational  or  irrational,  and,  if  rational,  either  fractional  or 
integral,  according  to  circumstances. 

It  will  be  shown  presently  that  every  algebraical  equation 
can  be  connected  with,  or  made  to  depend  upon,  an  equation 
of  the  form 


284  MEANING  OF  SOLUTION  chap. 

where  <t>  is  a  rational  integral  function.  Such  equations  are 
therefore  of  great  analytical  importance  ;  and  it  is  to  them  that 
the  "  Theory  of  Equations,"  as  ordinarily  developed,  mainly 
applies.  An  integral  equation  of  this  kind  is  described  by 
assigning  its  degree  and  the  number  of  its  variables.  The  degree 
of  the  equation  is  simply  the  degree  of  the  function  <f>.  Thus, 
of  +  Ixy  +  if  -  2  =  0  is  said  to  be  an  equation  of  the  2nd  degree 
in  two  variables. 

§  4.]  Equations  of  condition  may  occur  in  sets  of  one  or  of 
more  than  one.  In  the  latter  case  we  speak  of  the  set  as  a  set 
or  system  of  simultaneous  equations. 

The  main  problem  which  arises  in  connection  with  every  system  of 
equations  of  condition  is  to  find  a  set  or  sets  of  values  of  the  variables 
which  shall  render  every  equation  of  the  system  an  identity  literal  oi 
numerical. 

Such  a  set  of  values  of  the  variables  is  said  to  satisfy  the 
system,  and  is  called  a  solution  of  the  system  of  equations.  If 
there  be  only  one  equation,  and  only  one  variable,  a  value  of 
that  variable  which  satisfies  the  equation  is  called  a  root.  We 
also  say  that  a  solution  of  a  system  of  equations  satisfies  the  system, 
meaning  that  it  renders  each  equation  of  the  system  an  identity. 

It  is  important  to  distinguish  between  two  very  different 
kinds  of  solution.  When  the  values  of  the  variables  which  con- 
stitute the  solution  are  closed  expressions,  that  is,  functions  of 
known  form  of  the  constants  in  the  given  equations,  we  have 
what  may  be  called  a  formal  solution  of  the  system  of  equations. 
In  particular,  if  these  values  be  ordinary  algebraical  functions 
of  the  constants,  we  have  an  algebraical  solution.  Such  solutions 
cannot  in  general  be  found.  In  the  case  of  integral  algebraical 
equations  of  one  variable,  for  example,  if  the  degree  exceed  the  4th, 
it  has  been  shown  by  Abel  and  others  that  algebraical  solutions 
do  not  exist  except  in  special  cases,  so  that  the  formal  solution, 
if  it  could  be  found,  would  involve  transcendental  functions. 

When  the  values  of  the  variables  which  constitute  the  solution 
are  given  approximately  as  numbers,  real  or  complex,  the  solution 
is  said  to  be  an  approximate  numerical  solution.     In  this  case  the 


xiv  EXAMPLES  OF  SOLUTION  285 

words  "  render  the  equation  a  numerical  identity  "  are  understood 
to  mean  "reduce  the  two  sides  of  the  equation  to  values 
which  shall  differ  by  less  than  some  quantity  which  is  assigned." 
For  example,  if  real  values  of  the  two  sides,  say  P  and  P', 
are  in  question,  then  these  must  be  made  to  differ  by  less  than 
some  given  small  quantity,  say  1/100,000;  if  complex  values 
are  in  question,  say  P  +  Qi  and  P'  +  Q'i,  then  these  must 
be  so  reduced  that  the  modulus  of  their  difference,  namely, 
\/{(P  -  P')2  +  (Q  -  Q')2}>  shall  be  less  than  some  given  small 
quantity,  say  1/100,000.    (Cf.  chap,  xii.,  §  21.) 

As  a  matter  of  fact,  numerical  solutions  can  often  be  obtained 
where  formal  solutions  are  out  of  the  question.  Integral  alge- 
braical equations,  for  example,  can  always  be  solved  numerically 
to  any  desired  approximation,  no  matter  what  their  degree. 

Example  1. 

2x  +  2  =  2. 
jb=0  is  a  solution,  for  this  value  of  x  reduces  the  equation  to 

2x0  +  2  =  2, 
which  is  a  numerical  identity.     Strictly  speaking,  this  is  a  case  of  algebraical 
solution. 

Example  2. 

ax  —  b2  =  0. 

x  =  b-ja  reduces  the  equation  to 

a — b-  =  0, 
a 

which  is  a  literal  identity  ;  hence  x  =  b2/a  is  an  algebraical  solution. 

Example  3. 

x"  -  2  =  0. 

Here  x—  +  \/2  and  x=  -  \J2  each  reduce  the  equation  to  the  identity 

2-2=0 ; 
these  therefore  are  two  algebraical  solutions. 

On  the  other  hand,  a;=+l-4142  and  x  =  — 1*4142  are  approximate 
numerical  solutions,  for  each  of  them  reduces  x-~2  to  -  "00003836.  which 
differs  from  0  by  less  than  '00004. 

Example  4. 

0'-l)2  +  2  =  0. 
x  =  \  +  \/2i  and  x—l-\/2i   are   algebraical   solutions,  as  the   student  will 
easily  verify. 

.T  =  10001  +  l-4142i  and  a;=  1*0001  -  1  -4142i  are  approximate  numerical 
solutions,  for  they  reduce  (.r-  l)2  +  2  to  "00003837+  -00028284;:'  and  "00003837 
-  ,00028284t  respectively,  complex  numbers  whose  moduli  are  each  less  than 
"0003. 


286       CONDITIONAL  EQUATION  A  HYPOTHETICAL  IDENTITY    chap. 

Example  5. 

x-y-1. 

Here  se=l,  y=0,  is  a  solution  ;  so  is  a;=l"5,  y  =  5  ;  so  is  x  =  2,  y  —  1  ;  and, 
in  fact,  so  is  x  =  a+  1,  y  =  a,  where  a  is  any  quantity  whatsoever. 

Here,  then,  there  are  an  infinite  number  of  solutions. 

Example  6.   Consider  the  following  system  of  two  equations  : — 

x  —  y=\,     2x  +  y—5. 
Here  x=2,  y  =  l  is  a  solution  ;  and,  as  we  shall  show  in  chap,  xvi.,  there  is 
no  other. 

The  definition  of  the  solution  of  a  conditional  equation 
suggests  two  remarks  of  some  importance. 

1st.  Every  conditional  equation  is  a  hypothetical  identity.  In  all 
operations  with  the  equation  ive  suppose  the  variables  to  have  such 
values  as  will  render  it  an  identity. 

2nd.  The  ultimate  test  of  every  solution  is  that  the  values  which  it 
assigns  to  the  variables  shall  satisfy  the  equations  when  substituted  therein. 

No  matter  how  elaborate  or  ingenious  the  process  by  which 
the  solution  has  been  obtained,  if  it  do  not  stand  this  test,  it  is 
no  solution ;  and,  on  the  other  hand,  no  matter  how  simply 
obtained,  provided  it  do  stand  this  test,  it  is  a  solution.*  In 
fact,  as  good  a  Avay  of  solving  equations  as  any  other  is  to  guess 
a  solution  and  test  its  accuracy  by  substitution.! 

§  5.]  The  consideration  of  particular  cases,  such  as  Examples 
1-6  of  §  4,  teaches  us  that  the  number  of  solutions  of  a  system  of 
one  or  more  equations  may  be  finite  or  infinite.  If  the  number 
be  finite,  we  say  that  the  solution  is  determinate  (singly  determin- 
ate, or  multiply  determinate  according  as  there  are  one  or  more 
solutions) ;  if  there  be  a  continuous  infinity  of  solutions,  we  say 
that  the  solution  is  indeterminate. 

The  question  thus  arises,  Under  what  circumstances  is  the 
solution  of  a  system  of  equations  determinate  1  Part  at  least  of 
the  answer  is  given  by  the  following  fundamental  propositions. 

Proposition  I.  The  solution  of  a  system  of  equations  is  in  general 
determinate  (singly,  or  multiply  according  to  circumstances)  when  the 
number  of  the  equations  is  equal  to  the  number  of  the  variables. 


*  A  little  attention  to  these  self-evident  truths  would  save  the  beginner 
from  many  a  needless  blunder. 

t  This  is  called  solving  by  "inspection." 


xiv      PROPOSITIONS  AS  TO  DETERMINATENESS  OF  SOLUTION     287 

Rightly  considered,  this  is  an  ultimate  logical  principle  which 
may  be  discussed,  but  not  in  any  strictly  general  sense  proved. 
Let  us  illustrate  by  a  concrete  example.  The  reader  is  aware 
that  a  rectilinear  triangle  is  determinable  in  a  variety  of  ways 
by  means  of  three  elements,  and  that  consequently  three  condi- 
tions will  in  general  determine  the  figure.  To  translate  this  into 
analytical  language,  let  us  take  for  the  three  determining  elements 
the  three  sides,  whose  lengths,  at  present  unknown,  we  denote 
by  x,  y,  z  respectively.  Any  three  conditions  upon  the  triangle 
may  be  translated  into  three  equations  connecting  x,  y,  z  with 
certain  given  or  constant  quantities ;  and  these  three  equations 
will  in  general  be  sufficient  to  determine  the  three  variables, 
x,  y,  z.  The  general  principle  :VL  common  to  this  and  like  cases  is 
simply  Proposition  I.  The  truth  is  that  this  proposition  stands 
less  in  need  of  proof  than  of  limitation.  What  is  wanted  is  an 
indication  of  the  circumstances  under  which  it  is  liable  to  excep- 
tion. To  return  to  our  particular  case  :  What  would  happen, 
for  example,  if  one  of  the  conditions  imposed  upon  our  triangle 
were  that  the  sum  of  two  of  the  sides  should  fall  short  of  the 
third  by  a  given  positive  quantity  %  This  condition  could  be 
expressed  quite  well  by  an  equation  (namely,  x  +  y  =  z  -  q,  say), 
but  it  is  fulfilled  by  no  real  triangle,  f  Again,  it  might  chance 
that  the  last  of  the  three  given  conditions  was  merely  a  con- 
sequence of  the  two  first.  We  should  then  have  in  reality  only  two 
conditions — that  is  to  say,  analytically  speaking,  it  might  chance 
that  the  last  of  the  three  equations  was  merely  one  derivable  from 
the  two  first,  and  then  there  would  be  an  infinite  number  of 
solutions  of  the  system  of  three  variables.      Such  a  system  is 

x  +  y  +  z  =    6, 

3.c+  2y  +  z  =  10, 

2x  +  y=    4, 

for  example,  for,  as  the  reader  may  easily  verify,  it  is  satisfied 
by  x  =  a  -  2,  y  =  8  -  2a,  z  =  a,  where  a  is  any  quantity  whatsoever. 


*  A  name  seems  to  be  required  for  thi.s  all-pervading  logical  principle : 
the  Law  of  Determinate  Manifoldness  might  be  suggested. 
+  See  below,  chap.  xix. 


288    PROPOSITIONS  AS  TO  DETEEMINATENESS  OF  SOLUTION  chap. 

It  will  be  seen  in  following  chapters  how  these  difficulties  are 
met  in  particular  cases.  Meantime,  let  us  observe  that,  if  we 
admit  Proposition  I.,  two  others  follow  very  readily. 

Proposition  II.  If  the  number  of  equations  be  less  than  the  number 
of  variables,  the  solution  is  in  general  indeterminate. 

Proposition  III.  If  the  number  of  independent  equations  be 
greater  than  the  number  of  variables,  there  is  in  general  no  solution, 
and  the  system  of  equations  is  said  to  be  inconsistent. 

For,  let  the  number  of  variables  be  n,  and  the  number  of 
equations  to,  say,  where  to  <  n.  Let  us  assign  to  the  first  n  -  m 
variables  any  set  of  values  we  please,  and  regard  these  as  constant. 
This  we  may  do  in  an  infinity  of  ways.  If  we  substitute  any  such 
set  of  values  in  the  to  equations,  we  have  now  a  set  of  to  equa- 
tions to  determine  the  last  m  variables ;  and  this,  by  Proposition 
I.,  they  will  do  determinately.  In  other  words,  for  every  set  of 
values  we  like  to  give  to  the  first  n  -  to  variables,  the  to  equations 
give  us  a  determinate  set  of  values  for  the  last  to.  We  thus  get  an 
infinite  number  of  solutions  ;  that  is,  the  solution  is  indeterminate. 

Next,  let  to  be  >  n.  If  we  take  the  first  n  equations,  these 
will  in  general,  by  Proposition  I.,  give  a  determinate  set,  or  a 
finite  number  of  determinate  sets  of  values  for  all  the  n 
variables.  If  we  now  take  one  of  these  sets  of  values,  and 
substitute  it  in  one  of  the  remaining  to  -  n  equations,  that 
equation  will  not  in  general  be  satisfied  ;  for,  if  we  take  an 
equation  at  random,  and  a  solution  at  random,  the  latter  will 
not  in  general  fit  the  former.  The  system  of  to  equations  will 
therefore  in  general  be  inconsistent. 

It  may,  of  course,  happen,  in  exceptional  cases,  that  this 
proposition  does  not  hold ;  witness  the  following  system  of  three 
equations  in  two  variables  : — 

SB-y=l,     2x  +  y=5,     3x"+2«/=8, 
which  has  the  common  solution  x  =  2,  y  =  1. 

§  6.]  We  have  also  the  further  question,  When  the  system 
is  determinate,  how  many  solutions  are  there  ?  The  answer 
to  this,  in  the  case  of  integral  equations,  is  furnished  by  the 
two  following  propositions  : — 


xiv  MULTIPLICITY  OF  DETERMINATE  SOLUTIONS  289 

Proposition  I.  An  integral  equation  of  the  nth  degree  in  one 
variable  has  n  roots  and  no  more,  which  may  be  real  or  complex,  and 
all  unequal  or  not  all  unequal,  according  to  circumstances. 

Proposition  II.  A  determinate  system  ofm  integral  equations  with 
m  variables,  whose  degrees  in  these  variables  are  p,  q,  r,  .  .  .  respect- 
ively, has,  at  most,  pqr .  . .  solutions,  and  has,  in  general,  just  that 
number. 

Proposition  I.  was  proved  in  the  chapter  on  complex  num- 
bers, where  it  was  shown  that  for  any  given  integral  function 
of  x  of  the  nth  degree  there  are  just  n  values  of  x  and  no  more 
that  reduce  that  function  to  zero,  these  values  being  real  or 
complex,  and  all  unequal  or  not  as  the  case  may  be. 

Proposition  II.  will  not  be  proved  in  this  work,  except  in 
particular  cases  which  occur  in  chapters  to  follow.  General 
proofs  will  be  found  in  special  treatises  on  the  theory  of  equa- 
tions. We  set  it  down  here  because  it  is  a  useful  guide  to  the 
learner  in  teaching  him  how  many  solutions  he  is  to  expect. 
It  will  also  enable  him,  occasionally,  to  detect  when  a  system 
is  indeterminate,  for,  if  a  number  of  solutions  be  found  exceed- 
ing that  indicated  by  Proposition  II.,  then  the  system  is  certainly 
indeterminate,  that  is  to  say,  has  an  infinite  number  of  solu- 
tions. 

Example.  The  system  x2  +  y2=l,  x-y  =  \  has,  by  Proposition  II. ,  2x1  =  2 
solutions.     As  a  matter  of  fact,  these  solutions  are  x  =  0,  y  —  —  1,  and  x=l, 

y=o. 

EQUIVALENCE  OF  SYSTEMS  OF  EQUATIONS. 

§  7.]  Two  systems  of  equations,  A  and  B  (each  of  which  may  con- 
sist of  one  or  more  equations),  are  said  to  be  equivalent  when  every 
solution  of  A  is  a  solution  of  B,  and  every  solution  of  B  a  solution 
of  A. 

From  any  given  system,  A,  of  equations,  we  may  in  an  in- 
finity of  ways  deduce  another  system,  B;  but  it  will  not 
necessarily  be  the  case  that  the  two  systems  are  equivalent. 
In  other  words,  we  may  find  in  an  infinity  of  ways  a  system, 
B,  of  equations  which  will  be  satisfied  by  all  values  of  the 
VOL.  I  U 


290  DEFINITION  OF  EQUIVALENCE  chap. 

variables  for  which  A  is  satisfied  ;  but  it  will  not  follow  con- 
versely that  A  will  be  satisfied  for  all  values  for  which  B  is 
satisfied.  To  take  a  very  simple  example,  x  -  1  =  0  is  satisfied  by 
the  value  x=l,  and  by  no  other;  £(.t-1)  =  0  is  satisfied  by 
as=l,  that  is  to  say,  x(x  -  1)  =  0  is  satisfied  when  x  -  1  =  0  is 
satisfied.  On  the  other  hand,  x(x  -  1)  =  0  is  satisfied  either  by 
x  =  0  or  by  x  =  1,  therefore  x  —  1  =  0  is  not  always  satisfied  when 
x(x  -  1)  =  0  is  so  ;  for  x  =  0  reduces  x  -  1  to  —  1,  and  not  to  0. 
Briefly,  x(x  -  1)  =  0  may  be  derived  from  x-  1  =  0,  but  is  not 
equivalent  to  x  —  1  =  0. 

x(x  -  1 )  =  0  is,  in  fact,  more  than  equivalent  to  x  —  1  =  0, 
for  it  involves  x  -  1  =  0  and  x  =  0  as  alternatives.  It  will  be 
convenient  in  such  cases  to  say  that  x(x  -  1)  =  0  is  equivalent  to 

I        -01 

\;c-l  =  0j 

When  by  any  step  we  derive  from  one  system  another  which 
is  exactly  equivalent,  we  may  call  that  step  a  reversible  deriva- 
tion, because  we  can  make  it  backwards  without  fallacy.  If 
the  derived  system  is  not  equivalent,  we  may  call  the  step 
irreversible,  meaning  thereby  that  the  backward  step  requires 
examination. 

There  are  few  parts  of  algebra  more  important  than  the 
logic  of  the  derivation  of  equations,  and  few,  unhappily,  that 
are  treated  in  more  slovenly  fashion  in  elementary  teaching. 
No  mere  blind  adherence  to  set  rules  will  avail  in  this  matter ; 
while  a  little  attention  to  a  few  simple  principles  will  readily 
remove  all  difficulty. 

It  must  be  borne  in  mind  that  in  operating  with  conditional 
equations  we  always  suppose,  the  variables  to  have  such  values 
as  will  render  the  equations  identities,  although  we  may  not  at 
the  moment  actually  substitute  such  values,  or  even  know  them. 
We  are  therefore  at  every  step,  hypothetically  at  least,  applying  the 
fundamental  laws  of  algebraical  transformation  just  as  in  chap.  i. 

The  following  general  principle,  already  laid  down  for  real 
quantities,  and  carefully  discussed  in  chap,  xii.,  §  12,  for  com- 
plex quantities,  may  be  taken  as  the  root  of  the  whole  matter. 


xiv  ADDITION  AND  TRANSPOSITION  OF  TERMS  291 

Let  P  and  Q  be  two  functions  of  the  variables  x,  y,  z,  .  .  .,  vjhich 
do  not  become  infinite  *  for  any  values  of  those  variables  that  we  have 
to  consider.  J/PxQ=0  and  Q  4=  0,  then  mil  P  =  0,  and  ifP  x  Q  =  0 
and  P  =t=  0,  then  will  Q  =  0. 

Otherwise,  the  only  values  of  the  variables  which  make  P  x  Q  =  0 
are  such  as  make  either  P  =  0,  or  Q  =  0,  or  both  P  =  0  and  Q  =  0. 

§  8.]  It  follows  by  the  fundamental  laws  of  algebra  that  if 

P  =  Q  •  (l), 

then  P  ±  R  =  Q  ±  R  (2), 

where  R  is  either  constant  or  any  function  of  the  variables. 
We  shall  show  that  this  derivation  is  reversible. 

For,  if  P  ±  R  =  Q  ±  R, 

then  P±RtR  =  Q±RtR, 

that  is,  P  =  Q  ; 

in  other  words,  if  (2)  holds  so  does  (1). 

Cor.  1 .  If  we  transfer  any  term  in  an  equation  from  the  one  side 
to  the  other,  at  the  same  time  reversing  its  sign  of  addition  or  subtrac- 
tion, 07'  if  toe  reverse  all  the  signs  on  both  sides  of  an  equation,  we 
deduce  in  each  case  an  equivalent  equation. 

For,  if  P  +  Q  =  R  +  S,  say, 

then  P  +  Q-S  =  R  +  S-S, 

that  is,  P  +  Q  -  S  =  R. 

Again,  if  P  +  Q  =  R  +  S, 

then        P  +  Q-P-Q-R-S  =  R  +  S-P-Q-R-S, 

that  is,  -  R  -  S  =  -  P  -  Q, 

or  -P-Q=-R-S. 

Cor.  2.  Every  equation  can  be  reduced  to  an  equivalent  equation  of 
the  form — 

R=0. 

For,  if  the  equation  be      P  =  Q, 

*  In  all  that  follows  all  functions  of  the  variables  that  appear  are  supposed 
not  to  become  infinite  for  any  values  of  the  variables  contemplated.  Cases 
where  this  understanding  is  violated  must  be  considered  separately. 


292  MULTIPLICATION  BY  A  FACTOR  chap. 

we  have  P  -  Q  =  Q  -  Q, 

that  is  P  -  Q  =  0, 

which  is  of  the  form  R  =  0. 

Example. 

-  Za?  +  2x2  +  Sx = or  -  x  -  3. 

Subtracting  x-  -  x  -  3  from  both  sides,  we  have  the  equivalent  equation 

-3a;3  +  ar  +  4a:  +  3  =  0. 
Changing  all  the  signs,  we  have 

3.«3  -  x2  -  4x  -  3  =  0. 
In  this  way  an  integral  equation  can  always  be  arranged  with  all  its  terms  on 
one  side,  so  that  the  coefficient  of  the  highest  term  is  positive. 

§  9.]  It  follows  from  the  fundamental  laws  of  algebra  that 

if  P  =  Q  (1), 

then  PR  =  QR  (2), 

the  step  being  reversible  if  R  is  a  constant  differing  from  0,  but  not  if 
R  be  a  function  of  the  variables* 

For,  if  PR  =  QR, 

an  equivalent  equation  is,  by  §  8, 

PR  -  QR  =  0  (3), 

that  is,  (P  -  Q)R  =  0  (4). 

Now,  if  R  be  a  constant  4=  0,  it  will  follow  from  (4),  by  the 
general  principle  of  §  7,  that 

P-Q  =  o, 

which  is  equivalent  to  P  =  Q. 

But,  if  R  be  a  function  of  the  variables,  (4)  may  also  be  satisfied 

by  values  of  the  variables  that  satisfy 

R  =  0  (5)  ; 

and  such  values  Avill  not  in  general  satisfy  (1). 

In  fact,  (2)  is  equivalent,  not  to  (1),  but  to  (1)  and  (5)  as 
alternatives. 

*  This  is  spoken  of  as  "multiplying  the  equation  by  R."  Similarly  the 
process  of  §  8  is  spoken  of  as  "adding  or  subtracting  R  to  or  from  the  equa- 
tion." This  language  is  not  strictly  correct,  but  is  so  convenient  that  we 
shall  use  it  where  no  confusion  is  to  be  feared. 


XIV       DEDUCTION  OF  INTEGRAL  FROM  RATIONAL  EQUATION      293 

Cor.  1.  From  the  above  it  follows  that  dividing  both  sides  of 
an  equation  by  any  function  other  than  a  constant  not  equal  to  zero  is  not 
a  legitimate  process  of  derivation,  since  we  may  thereby  lose  solutions. 

Thus  PR  =  QR  is  equivalent  to  J  _     Y  ; 

whereas  PR/R  =  QR/R* 

gives  P  =  Q, 

which  is  equivalent  merely  to 

P-Q  =  0. 

Example.   If  we  divide  both  sides  of  the  equation 

(x~l)x2  =  i{x-l)  (a) 

by  £- 1,  we  reduce  it  to  x-  =  4  (/3), 

which  is  equivalent  to         (x  -  2)  (x  +  2)  =  0. 
(a),  on  the  other  hand,  is  equivalent  to 

(x-l)(w-2)(a;+2)=0. 

Hence  (a)  has  the  three  solutions  x-1,  x  =  2,  x=  -  2  ;  while  (/3)  has  only  the 
two  x  =  2,  x=  -  2. 

Cor.  2.  To  multiply  or  divide  both  sides  of  an  equation  by 
any  constant  quantity  differing  from  zero  is  a  reversible  process 
of  derivation.  Hence,  if  the  coefficients  of  an  integral  equation  be 
fractional  either  in  the  algebraical  or  in  the  arithmetical  sense,  we  can 
always  find  an  equivalent  equation  in  which  the  coefficients  are  all 
integral,  and  have  no  common  measure. 

Also,  we  can  always  so  arrange  an  integral  equation  that  the  co- 
efficient of  any  term  we  please,  say  the  highest,  shall  be  +  1 . 

Example  1. 

3a  +  2     6x  +  S_2x+_i 

~~4~~ +     5     -     8 

gives,  on  multiplying  both  sides  by  40, 

10(3x  +  2)  +  8(6i-  +  3)  =  5(2x-+4), 

that  is,  30^  +  20  +  48^  +  24  =  10x-  +  20, 

whence,  after  subtracting  lO.e  +  20  from  both  sides, 

68a; +  24  =  0  ; 

*  As  we  are  here  merely  establishing  a  negative  proposition,  the  reader 
may,  to  fix  his  ideas,  assume  that  all  the  letters  stand  for  integral  functions 
of  a  single  variable. 


294     DEDUCTION  OF  INTEGRAL  FROM  RATIONAL  EQUATION    chap. 


whence  again,  after  division  of  both  sides  by  68, 
Example  2. 


X+Tf=°- 


K    q         p~q'  J\    p         P  + 


-qy)=^y- 


If  we  multiply  both  sides  by  pq(p  -  q)  {p  +  q),  that  is,  by  pq(2>~  ~  <T)i  we  derive 
the  equivalent  equation 

{{p2-q2)x+pqy}  {{2r-q-)x+pqy)=2pq(p--q-)xy, 

that  is,  ( p2  -  q2)2x2  +  2pq{  p2  -  q2)xy  +p2q-y2  =  2pq{ p2  -  q2)xy, 

which  is  equivalent  to  [p2  -q2)2x2jrp2q2y2  =  Q. 

Cor.  3.  From  every  rational  algebraical  equation  an  integral  equa- 
tion can  be  deduced  ;  but  it  is  possible  that  extraneous  solutions  may 
be  introduced  in  the  process. 

Suppose  we  heave  P  =  Q  (a), 

where  P  and  Q  are  rational,  but  not  integral.  Let  L  he  the 
L.C.M.  of  the  denominators  of  all  the  fractions  that  occur  either 
in  P  or  in  Q,  then  LP  and  LQ  are  both  integral.  Hence,  if  we 
multiply  both  sides  of  (a)  by  L,  we  deduce  the  integral  equation 

LP  =  LQ  (/?). 

Since,  however,  the  multiplier  L  contains  the  variables,  it  is 
possible  that  some  of  the  solutions  of  L  =  0  may  satisfy  (ft),  and 
such  solutions  would  in  general  be  extraneous  to  (a).  We  say 
possible ;  in  general,  however,  this  will  not  hajjpp n,  because  P 
and  Q  contain  fractions  whose  denominators  are  factors  in  L. 
Hence  the  solutions  of  L  =  0  will  in  general  make  either  P  or  Q 
infinite,  and  therefore  (P  -  Q)L  not  necessarily  zero.  The  point 
at  issue  will  be  best  understood  by  studying  the  two  following 
examples  : — 

Example  1. 

.       0     z2-6a;  +  8     x-2 
2*'3+      x-2      =  x=S  (a)- 

If  we  multiply  both  sides  by  (x-  2)(x-  3),  we  deduce  the  equation 

(2x-3)(x-2)(x-3)  +  (x2-6x+8)(x-3)  =  (x-2)2  (/3), 

which  is  integral,  and  is  satisfied  by  any  solution  of  (a).  "We  must,  however, 
examine  whether  any  of  the  solutions  of  (x-  2)(x-  3)  =  0  satisfy  (/3).  These 
solutions  are  x=2  and  x  =  3.  The  second  of  these  obviously  does  not  satisfy 
(/3),  and  need  not  be  considered;  but  x=2  does  satisfy  (/3),  and  we  must 
examine  (a)  to  see  whether  it  satisfies  that  equation  also. 


XIV  RAISING  BOTH  SIDES  TO  SAME  POWER  295 

Now,  since  x2  -  6a: +  8  =  (as— 2)  (a;  -  4),  (a)  may  be  written  in  the  equivalent 

form 

x  —  2 
2x  -  3  +  x  -  4 : 


P  =  Q 

(1) 

P  -  Q  =  0 

(2). 

+  P»-2Q  +  P'l"3Q2  +  .  . 

. +Qn-\  ■ 

x-3 
which  is  obviously  not  satisfied  by  x  =  2. 

It  appears,  therefore,  that  in  the  process  of  integralisation  we  have  intro- 
duced the  extraneous  solution  x=2. 

Example  2. 

2x-B  +  2^^8  =  X~l  («<). 

x  -  2  x  -  3 

Proceeding  as  before,  we  deduce 

{2x  -  3)  (a;  -  2)  (x  -  3)  +  (2a:2  -  6x  +  8) (a;  -  3)  =  (x  -  2f  iff). 

It  will  be  found  that  neither  of  the  values  33=2,  a;  =  3  satisfies  (/3'). 
Hence  no  extraneous  solutions  have  been  introduced  in  this  case. 

N.B. — The  reason  why  a?  =  2  satisfies  (/3)  in  Example  1  is  that  the  numer- 
ator a,-2 -  6a:  +  8  of  the  fraction  on  the  left  contains  the  factor  x-2  which 
occurs  in  the  denominator. 

Cor.  4.  Raising  both  sides  of  an  equation  to  the  same  integral 
power  is  a  legitimate,  but  not  a  reversible,  process  of  derivation. 

The  equation 
is  equivalent  to 

If  we  multiply  by  P'1"1  +  Pn~2Q  +  P»-3Q2  +  .  .  .  +  QM~\  we 

deduce  from  (2) 

P*  _  Q»  =  0  (3), 

which  is  satisfied  by  any  solution  of  (1);  (3),  however,  is  not 
equivalent  to  (1),  but  to 

P  =  Q\ 

P»-1  +  P»-2Q  +  .    .    >  +  Q»-l  =  oj- 

It  will  be  observed  that,  if  we  start  with  an  equation  in  the 
standard  form  P  -  Q  =  0,  transfer  the  part  Q  to  the  right-hand 
side,  and  then  raise  both  sides  to  the  wth  power,  the  result  is  the 
same  as  if  we  had  multiplied  both  sides  of  the  equation  in  its 
original  form  by  a  certain  factor.  To  make  the  introduction  of 
extraneous  factors  more  evident  we  chose  the  latter  process  ;  but 
in  practice  the  former  may  happen  to  be  the  more  convenient.* 

If  the  reader  will  reflect  on  the  nature  of  the  process  described 
in  chap.  x.  for  rationalising  an  algebraical  function  by  means 
of  a  rationalising  factor,  he  will  see  that  by  repeated  operations  of 
this  kind  every  algebraical  equation  can  be  reduced  to  a  rational 

*  See  below,  §  12,  Example  3. 


296    EVERY  ALGEBRAICAL  EQUATION  CAN  BE  INTEGRALISED    chap. 

form  ;  but  at  each  step  extraneous  solutions  may  be  introduced. 
Hence 

Cor.  5.   From  every  algebraical  equation  we  can  derive  a  rational 
integral  equation,  which  will  be  satisfied  by  any  solution  of  the  given 
equation  ;  but  it  does  not  follow  that  every  solution^  or  even  that  any 
solution,  of  the  derived  equation  will  satisfy  the  original  one. 
Example  1.   Consider  the  equation 

V(z+l)  +  V(*-l)  =  l  (a), 

where  the  radicands  are  supposed  to  be  real  and  the  square  root  to  have  the 
positive  sign.  * 

(a)  is  equivalent  to  \J(x  +  l)  =  l  -  \J{x-  1), 

whence  we  derive,  by  squaring, 

x+l  =  \+x-l-2'sJ{x-\), 
which  is  equivalent  to  1  =  -  2\J(x  -  1). 

From  this  last  again,  by  squaring,  we  derive 

1  =  4(35-1), 

which  is  equivalent  to  the  integral  equation 

Ax  -5  =  0  (/3), 

the  only  solution  of  which,  as  Ave  shall  see  hereafter,  is  x  =  \. 

It  happens  here  that  x=\  is  not  a  solution  of  (a),  for  V(f +  1)  +  V(i"-  1) 

—  S    i    1  _o 

—  T  +  V  —  -■ 

Example  2. 

V(.c+i)-V(->,-i)  =  i  (o). 

Proceeding  exactly  as  before  we  have 

a;  +  l  =  l  +  a:-l  +  2V(*-l)i  ' 
1=+2V(*-1), 
1  =  4(3-1), 
4a- 5  =  0  (/3'), 

Here  (/?')  gives  a:=f,  which  happens  this  time  to  be  a  solution  of  the 
original  equation. 

We  conclude  this  discussion  by  giving  two  propositions 
applicable  to  systems  of  equations  containing  more  than  one 
equation.  These  by  no  means  exhaust  the  subject ;  but,  as  our 
object  here  is  merely  to  awaken  the  intelligence  of  the  student, 
the  rest  may  be  left  to  himself  in  the  meantime. 

§  10.]  From  the  system 

P,  =  0,     P2=0,     .  .  .,     Pn  =  0  (A) 

we  derive 

L1P1.+  IJPf+.    .    .+LnPn=  0,      P8  =  0,      .    .    .,      Pn  =  0      (B), 
and  the  two  will  be  equivalent  if  JJl  be  a  constant  differing  from  0. 


f  When  \Jx  is  imaginary,  its   "principal  value"  (see  chap,  xxix.)  ought 
to  be  taken,  unless  it  is  otherwise  indicated. 


XIV 


EXAMPLES  OF  DERIVATION  297 


Any  solution  of  the  system  (A)  reduces  P15  P2,  .  .  .,  Pn  all 
to  0,  and  therefore  reduces  L^  +  LP,  +  .  .  .  +  LnPn  to  0,  and 
hence  satisfies  (B). 

Again,  any  solution  of  (B)  reduces  P2,  P3,  .  .  .,  Pn  all  to  0, 
and  therefore  reduces  L,P,  +  L2P2  +  .  .  .  +  LnP„  =  0  to  L,P,  =  0, 
that  is  to  say,  if  L,  he  a  constant  4=  0,  to  Pj  =  0.  Hence,  in  this 
case,  any  solution  of  (B)  satisfies  (A). 

If  L,  contain  the  variables,  then  (B)  is  equivalent,  not  to  (A) 

simply,  but  to 

f  P,  =  0,    P2  =  0,    .  .  .,    Pw  =  0] 
tL.-O,    Ps  =  0,     .  .  ,     Pw  =  0j 

As  a  particular   case    of  the  above,  we  have  that  the  two 

systems 

P  =  Q,         R  =  S  j 

and  P  +  R  =  Q  +  S,  R  =  S 

are  equivalent.     For  these  may  be  written 

P-Q  =  0,  R~^S=0; 


P-Q  +  R-S  =  0,  R-S  =  0. 

If  I,  V,  m,  m!  he  constants,  any  one  of  which  may  he  zero,  hut 
which  are  such  that  lm'  -  I'm  =t=  0,  then  the  two  systems 

U  =  0,  U'  =  0, 

and  IV  +  IV  =  0,  mV  +  niV  =  0 

are  equivalent. 

The  proof  is  left  to  the  reader.      A  special  case  is  used  and 
demonstrated  in  chap,  xvi.,  §  4. 
§  11.]  Any  solution  of  the  system 

P  =  Q,     R  =  S  (A) 

is  a  solution  of  the  system 

PR  =  QS,  R  =  S  (B); 

but  the  two  systems  are  not  equivalent. 
From  P  =  Q,  we  derive 

PR  =  QR, 
which,  since  R  =  S,  is  equivalent  to 

PR  =  QS. 
It  follows  therefore  that  any  solution  of  (A)  satisfies  (B). 


298  EXAMPLES  OF  DERIVATION  CHAP. 

Starting  now  with  (B),  we  have 

PR  =  QS  (1), 

R  =  S  (2). 

Since  II  =  S,  (1)  becomes 

PR  =  QR, 
which  is  equivalent  to 

(P  -  Q)R  =  0, 
that  is,  equivalent  to 

fP-Q  =  0\ 

Hence  the  system  (B)  is  equivalent  to 

fP  =  Q,  R  =  S\ 

|R  =  0,  R  =  SJ" 
that  is  to  say,  to 

/P  =  Q,R  =  S\ 

\R  =  0,   S  =  0J" 
In  other  words,  (B)  involves,  besides  (A),  the  alternative  system, 

R  =  0,    S  =  0. 

Example.  From  x-2  =  l-y,  x  =  l+y, 

a  system  which  has  the  single  solution  x=2,  y==l,  we  derive  the  system 

x(x-2)  =  l-y\  x=l+y, 
which,  in  addition  to  the  solution  x  =  2,  y—l,  has  also  the  solution  x  =Q,y=  -1 
belonging  to  the  system 

2=0,  l  +  y  =  0. 

§  12.]  In  the  process  of  solving  systems  of  equations,  one  of 
the  most  commonly-occurring  requirements  is  to  deduce  from  two 
or  more  of  the  equations  another  that  shall  not  contain  certain 
assigned  variables.  This  is  called  "  eliminating  the  variables  in 
question  between  the  equations  used  for  the  purpose."  In  per- 
forming the  elimination  Ave  may,  of  course,  use  any  legitimate 
process  of  derivation,  but  strict  attention  must  always  be  paid  to 
the  question  of  equivalence. 
Example.  Given  the  system 

*2+r=i  (i), 

x+y=l  (2), 

it  is  required  to  eliminate  y,  that  is,  to  deduce  from  (1)  and  (2)  an  equation 
involving  x  alone. 


xiv  EXAMPLE  OF  ELIMINATION  299 

(2)  is  equivalent  to 

y  =  l-x. 
Hence  (1)  is  equivalent  to 

a?+(l-xf=l, 
that  is  to  sav,  to 

2x2-2x=0, 
or,  if  we  please,  to 

x*--x  =  0; 

and  thus  we  have  eliminated  y,  and  obtained  an  equation  in  x  alone. 

The  method  we  have  employed  (simply  substitution)  is,  of  course,  only 
one  among  many  that  might  have  been  selected. 

Observe  that,  as  a  result  of  our  reasoning,  we  have  that  the  system  (1)  and 
(2)  is  equivalent  to  the  system 

x2-x=0  (3), 

x  +  y=l  (4), 

from  which  the  reader  will  have  no  difficulty  in  deducing  the  solution  of  the 
given  system. 

§  13.]  Although,  as  we  have  said,  the  solution  of  a  system 
of  equations  is  the  main  problem,  yet  the  reader  will  learn, 
especially  when  he  comes  to  apply  algebra  to  geometry,  that 
much  information — very  often  indeed  all  the  information  that  is 
required— may  be  derived  from  a  system  without  solving  it, 
but  merely  by  throwing  it  into  various  equivalent  forms.  The 
derivation  of  equivalent  systems,  elimination,  and  other  general 
operations  with  equations  of  condition  have  therefore  an  im- 
portance quite  apart  from  their  bearing  on  ultimate  solution. 

We  have  appended  to  this  chapter  a  large  number  of  exercises 
in  this  branch  of  algebra,  keeping  exercises  on  actual  solution  for 
later  chapters,  which  deal  more  particularly  with  that  part  of 
the  subject.  The  student  should  work  a  sufficient  number  of  the 
following  sets  to  impress  upon  his  memory  the  general  principles 
of  the  foregoing  chapter,  and  reserve  such  as  he  finds  difficult  for 
occasional  future  practice. 

The  following  are  worked  out  as  specimens  of  various  artifices 
for  saving  labour  in  calculations  of  the  present  kind  : — 

Example  1.  Reduce  the  following  equation  to  an  integral  form  : — 

ax-  +  bx  +  c    ax  +  b  ,  . 

(a). 


px~  +  qx  +  r    px  +  q 
"We  may  write  (a)  in  the  form 

•  x(ax  +  b)  +  c  _  ax  +  b 
x{px  +  q)  +  r  ~px  +  q 


(0). 


300  EXAMPLES  OF  INTEGRALISATION  chap. 

Multiplying  (/3)  by  (px  +  q){x(px  +  q)  +  r},  we  obtain 

x(ax  +  b)  (px  +  q)+  c{px  +  q)  =  x(ax  +  b)  (px  +  q)  +  r(ax  +  b)     (7). 

Now,  (7)  is  equivalent  to 

c(px  +  q)  =  r(ax  +  b)  (5), 

which  again  is  equivalent  to 

(cp  -  ra)x  +  (cq  -  rb)  =  0  (e). 

The  only  possibly  irreversible  step  here  is  that  from  (/3)  to  (7). 

Observe  the  use  of  the  brackets  in  (/3)  and  (7)  to  save  useless  detail. 

Example  2. 
Integralise 

(a  -x)(x  +  m)_(a  +  x)  (x  -  m) 


x + n  x-n 


(a). 


Since  x  +  m  =  (x  +  n)  +  (m -  n),  x-m  =  (x-n)-  (m-n),  (a)  may  be  written 
in  the  equivalent  form, 

.         ./,  ,  m-n\     ,         ,  /,     m-v\  ,_, 


whence  the  equivalent  form 

{a-x)-(a  +  x)  +  (m-n)t + =0, 

\x+n    x-n) 

that  is, 


-2x  +  2{m-y{n  +  a)x=0  (7). 

x-  -  n- 

Multiplying  by  -£(a;2-?i2),  we  deduce  from  (7)  the  integral  equation 

x{x1-n'i-  (m  -  n)  (n  +  a))  =  0  (5). 

In  this  case  the  only  extraneous  solutions  that  could  be  introduced  are 
those  of  x1  -  n-  =  0. 

Note  the  preliminary  transformation  in  (/3)  ;  and  observe  that  the  order 
in  which  the  operations  of  collecting  and  distributing  and  of  using  any 
legitimate  processes  of  derivation  that  may  be  necessary  is  quite  unrestricted, 
and  should  be  determined  by  considerations  of  analytical  simplicity.  Note 
also  that,  although  we  can  remove  the  numerical  factor  2  in  (7),  it  is  not 
legitimate  to  remove  the  factor  x  ;  x  =  Q  is,  in  fact,  as  the  student  will  see  by 
inspection,  one  of  the  solutions  of  (a). 

Example  3. 

X,  Y,  Z,  U  denoting  rational  functions,  it  is  required  to  rationalise  the 

equation 

X/X  ±  \/ Y ±  y'Z  ±  VU  =  0  (a). 

We  shall  take  +  signs  throughout ;    but   the   reader  will    see,  on   looking 
through  the  work,  that  the  final  result  would  be  the  same  whatever  arrange- 
ment of  signs  be  taken. 
From  (a), 

VX+vy=-vz-\/u, 

whence,  by  squaring, 

X  +  Y  +  2V(XY)=Z+U+2V(ZTJ)  (/3). 


xiv  EXAMPLES  OF  RATIONALISATION  301 

From  (/3), 

X  +  Y-Z-U=-  2  V(XY)  +  2  V(ZU), 
whence,  by  squaring, 

(X+Y-Z-U)2=4XY+4ZU-8V(XYZU)  (7). 

We  get  from  (7), 

X2  +  Y3  +  Z-  +  U2  -  2XY  -  2XZ  -  2XU  -  2YZ  -  2YU  -  2ZU=  -  8 V(XYZU), 

whence,  by  squaring, 

J  Xs  +  Y2  +  Z2  +  U2  -  2XY  -  2XZ  -  2XU  -  2YZ  -  2YU  -  2ZU  j 2  =  64X  YZU   (5). 

Since  X,  Y,  Z,  U  are,  by  hypothesis,  all  rational,  (5)  is  the  required  result. 
As  a  particular  instance,  consider  the  equation 

V(2k+3)  +  V(&g+2)  -  V(2as+5)  -  \/{&c)=0  [a'). 

Here  X  =  2a: +  3,  Y=3a;+2,  Z  =  2a;  +  5,  U  =  Zx;  and  the  student  will  find, 
from  (5)  above,  as  the  rationalised  equation, 

(48^  +  112a,-  +  24)2=64(2a;+3)(3a:  +  2)(2a;  +  5)3a;  (8'). 

After  some  reduction  (5')  will  be  found  to  be  equivalent  to 

(z-3)2  =  0  (Y). 

It  may  be  verified  that  a;  =  3  is  a  common  solution  of  (a')  and  (e'). 

Although,  for  the  sake  of  the  theoretical  insight  it  gives,  we  have  worked 
out  the  general  formula  (5),  and  although,  as  a  matter  of  fact,  it  contains  as 
particular  cases  very  many  of  the  elementary  examples  usually  given,  yet 
it  is  by  no  means  advisable  that  the  student  should  work  particular  cases  by 
merely  substituting  in  (5)  ;  for,  apart  from  the  disciplinary  advantage,  it 
often  happens  that  direct  treatment  is  less  laborious,  owing  to  intervening 
simplifications.  Witness  the  following  treatment  of  the  particular  case  (a') 
above  given. 

From  (a'),  by  transposition, 

V(2aJ+8)+V(3a!+2)=V(2a!+5)  +  's/(3a5), 

whence,  by  squaring, 

5x  +  5  +  2\/(6ar  +  13a:  +  6)  =  5x  +  5  +  2  y/(6x-  +  15x), 
which  reduces  to  the  equivalent  equation 

^(6x2  +  lZx+6)=s/(6xi+l5x)  (£'). 

From  (/3'),  by  squaring, 

6X2  +  lBx  +  6  =  6a;2  +  15s, 
which  is  equivalent  to 

a;-3  =  0  (5"). 

Thus,  not  only  is  the  labour  less  than  that  involved  in  reducing  (5),  but 
(5")  is  itself  somewhat  simpler  than  (5'). 

Example  4.   If 

x  +  y  +  z=0  (o), 

show  that 

2(2/2  +  yz  +  z*f  =  3n(y2  +  yz  +  z")  (/3j. 


302  EXAMPLES  OF  TRANSFORMATION  chap. 

We  have 

vf  +  yz  +  z^if  +  ziy  +  z), 

=(-z-x)*+z{-x),by(a), 

=  Z2  +  ZX  +  X2, 

=  ir  +  xy  +  y2,  by  symmetry. 
It  follows  then  that 

2(f-  +  yz  +  z2)3  =  3(</2  +  yz  +  z*)*  (7), 

and  m(y-  +  ijz  +  z'>)  =  3(f-  +  yz  +  z*)3  (5). 

From  (7)  and  (5),  (/3)  follows  at  once. 

Example  5.   If 

x  +  y+z  =  0  (a), 

show  that 

(y  +  z)(z  +  x)  J 

From  (a),  y  +  z=-x  (7), 

whence,  squaring  and  then  transposing,  we  have 

y*+z*=a?-2yz  (5). 

Similarly  z  +  x=-y  (7'), 

zn-  +  x-  =  y"i-2zx  (5'). 

From  the  last  four  equations  we  have 

2  (y-  +  s2)  (z2  +  *2)  =  s  (a2  -  2yz)  (f-  -  2sc) 
(y+2)(«+a:)  a;?/ 

_     aPy2  -  2x?z  -  2y3z  +  ixyz1 


Z\xy-2 


xy 

(3?  +  y3ls 


3  +  4;2| 


xyz 

=  Xvy  +  42a,-2  -  J-  2.r%3  +  ,3)        (e). 
Now,  from  (a),  by  squaring  and  transposing, 

2x'!=-2?xy  (f). 

Also  2x2(y3  +  z3)EE2a:y2(a:  +  y), 

=  -  ^x-rfz,  by  (a), 

=  -  xyzZxy  (17). 

If  we  use  (f)  and  (r?),  (e)  reduces  to 

&+*)(*+*)  =_5 
(y  +  z)(z  +  x)  J' 

which  is  equivalent  to  (/3). 

The  use  of  the  principles  of  symmetry  in  conjunction  with  the  2  notation 
in  shortening  the  calculations  in  this  example  caunot  fail  to  strike  the 
reader. 


Example  6.   If 


yz-x^zx-f 
y+z       z+x 


xiv  EXAMPLES  OF  TRANSFORMATION  303 

and  if  x,  y,  z  be  all  unequal,  show  that  each  of  these  expressions  is  equal  to 
(xy  -  z2)/(x  +  y),  and  also  to  x  +  y  +  z. 

Denote  each  of  the  sides  of  (a)  by  U.     Then  we  have 

yz-x2 


y  +  z 
zx-y 
~z  +  x 


U  (/3), 

=  U  (7). 


Since  y  +  z  =  0  and  z  +  x  =  0  would  render  the  two  sides  of  (a)  infinite,  we 
may  assume  that  values  of  a-,  y,  z  fulfilling  these  conditions  are  not  in  ques- 
tion, and  multiply  (/3)  and  (7)  by  y  +  z  and  z+x  respectively.  We  then 
deduce 

ye-x*-(y+z)\J=0  (5), 

zx-yn--(z  +  x)U  =  0  (e). 

From  (5)  and  (e),  by  subtraction,  we  have 

z(x-y)  +  (x2-y2)-(x-y)V  =  0, 
that  is,  (x  +  y  +  z-V)(x-y)  =  0  (f). 

Now  x-y  —  0  is  excluded  by  our  data  ;  hence,  by  (f),  we  must  have 

x  +  y  +  z-U  =  0,  (,), 

that  is,  V=x+y+z  (6). 

We  have  thus  established  one  of  the  desired  conclusions.  To  obtain  the 
other  it  is  sufficient  to  observe  that  (77)  is  symmetrical  in  x,  y,  z.  For,  if  we 
start  with  (77)  and  multiply  by  x  -  z  (which,  by  hypothesis,  4=  0),  we  obtain 

y(x  -  z)  +  (x2  -  s«)  -  (x  -  Z)U  =  0  ; 

and,  combining  this  by  addition  with  (5), 

xy-i?-(z+y)U=Q; 

which  gives  (since  x  +  y  +  0) 

jj_xy-z* 


x  +  y 

The  reader  should  notice  here  the  convenient  artifice  of  introducing  an 
auxiliary  variable  U.  He  should  also  study  closely  the  logic  of  the  process, 
and  be  sure  that  he  sees  clearly  the  necessity  for  the  restrictions  x-y  +  Q, 
x  +  y  +  0. 

Example  7.   To  eliminate  x,  y,  z  between  the  equations 

y*+z*=ayz  (a), 

z2  +  x2  =  bzx  (£), 

xt+y*=cxy  (7), 

where  x  +  0,  w  +  0,  z  +  0. 

In  the  first  place,  we  observe  that,  although  there  are  three  variables,  yet, 
since  the  equations  are  homogeneous,  we  are  only  concerned  with  the  ratios 
of  the  three.  We  might,  for  example,  divide  each  of  the  equations  by  x2 ; 
we  should  then  have  to  do  merely  with  y/x  and  z/x,  each  of  which  might  be 
regarded  as  a  single  variable.  There  are  therefore  enough  equations  for  the 
purpose  of  the  elimination. 


304  EXAMPLES  OF  ELIMINATION  chap. 

From  (a)  and  (j3)  we  deduce,  by  subtraction, 

x*-y2={bx-ay)z  (8). 

We  remark  that  it  follows  from  this  equation  that  bx-  ay  +  0;  for  bx-ay  —  0 
would  give  x2  =  y2,  and  hence,  by  (7),  x  =  0  (at  least  if  we  suppose  c=t=±2). 
This  being  so,  we  may  multiply  (/3)  by  (bx  -  ay)2.     "We  thus  obtain 

z-(bx  -  ay)2  +  x2(bx  —  ay)2  =  bxz(bx  -  ay)2, 
whence,  using  (5),  we  have 

(a;2  -  y2)2  +  x2(bx  —  ay)2  =  bx(bx  -ay)  (x2  -  y2), 
which  reduces,  after  transposition,  to 

(x2  -  y2)2  =  xy(ax  -  by)  (bx  -  ay), 
that  is  to  say,  (x2  +  y2)2- ±x2y2  =  xy(ax-by)  (bx-ay)  (e). 

Using  (7),  we  deduce  from  (e) 

(c2  -  i)x2y2  =  xy(ax  -  by)  (bx  -  ay), 
whence,  bearing  in  mind  that  xy  +  0,  we  get 

(c-2  -i)xy  =  ab(x2  +  y2)  -  (a2  +  b2)xy, 
which  is  equivalent  to 

(a2  +  b2  +  c2  -  i)xy  =  ab(x2  +  y2)  (f). 

Using  (7)  once  more,  and  transposing,  we  reach  finally 

(a2  +  b2  +  c2  -  4  -  abc)xy  -  0, 
whence,  since  xy  +  0,  we  conclude  that 

a2  +  b2  +  c2-4:-abc  =  0  (v), 

so  that  (77)  is  the  required  result  of  eliminating  x,  y,  z  between  the  equations 
(a),  (/3),  (7).  Such  an  equation  as  (77)  is  often  called  the  eliminant  (or  re- 
sultant) of  the  given  system  of  equations. 

Example  8.   Show  that,  if  the  two  first  of  the  following  three  equations  be 
given,  the  third  can  be  deduced,  it  being  supposed  that  x  =t=  y  +  z  +  0. 

a2(y2  +  yz  +  z2)  -  ayz(y  +  z)  +  y2z2  =  0  (a), 

a2(z2  +  zx  +  x2)  -  azx(z  +  x)  +  z2x2  =  0  (p), 

a2(x2  +  xy  +  y"-)  -  axy(x  +  y)+  x2y2  =  0  (7). 

This  is  equivalent  to  showing  that,  if  we  eliminate  z  between  (a)  and  (/3),  the 
result  is  (7). 

Arranging  (a)  and  (/3)  according  to  powers  of  z,  we  have 

aY  -a(-ay  +  y2)z  +  (a2  -  ay  +  y2)z2  =  0  (5), 

a2x2  -a(-ax  +  x2)z  +  (a2  -ax  +  a?)z2  =  0  (e ). 

Multiplying  (5)  and  (e)  by  x2  and  y2  respectively,  and  subtracting,  we  get 

a2xy(x  -  y)z  +  {a2(x  +  y)  -  axy}  (x  -  y)z2  =  0, 
whence,  rejecting  the  factor  a(x-y)z,  which  is  permissible  since  x  +  y,  z#=0, 

axy+  {a(x  +  y)-xy}z  =  0  (f). 

Again,  multiplying  (5)  and  (e)  by  a2-ax  +  x2  and  a2-ay  +  y2  respectively, 
and  subtracting,  we  get,  after  rejecting  the  factor  a2, 

a(x  +  y)-xy+  \a-(x  +  y)}z=0  (77). 


XIV 


EXERCISES  XIX  305 


Finally,  multiplying  (f)  and  (v)  by  a{x  +  y)-xy  and  axy  respectively,  and 
subtracting,  we  get,  since  z=$=0, 

.      {a{x  +  y)-  xy) 2  -  axy  {a  -  (x  +  y)}  =  0, 
which  gives  a2(x2  +  xy  +  y2)  -  axy(x  +  y)  +  x2y2 = 0, 

the  required  result. 

Exercises  XIX. 
(On  the  Reduction  of  Equations  to  an  Integral  Form) 
Solve  by  inspection  the  following  systems  of  equations  :  — 
(1.)  ar-4-3(;r  +  2)  =  0. 

(2.)  £±j ;=«-. 

x  x—bx—a 

(3.)  (a-b)x-a2  +  b-  =  0. 

(4.)  x(b-c)+y(c-a)  +  (a-b)=0, 

ax(b  -c)  +  by(c  -a)  +  c(a-b)  =  0. 
(5.)  x  +  y  +  z  =  a  +  b  +  c, 

ax  +  by  +  cz  =  a2  +  b'-  +  c2, 
bx  +  cy  +  az  =  be  +  ca  +  ab. 

(6.)  For  what  values  of  a  and  b  does  the  equation 

(a:  -  a)  (3a:  -2)= Bx2  +  bx  + 10 
become  an  identity  ? 

Integralise  the  following  equations  ;  and  discuss  in  each  case  the  equiva- 
lence of  the  final  equation  to  the  given  one. 

(7.)  «±«+?»±"    14 

x  -  4       a;  -  2 


(8.) 


l-8/(g+l)  l  +  3/(a;-l) 

a;  + 1  +  l/fc+l)    as  -  1  +  l/(as  - 1)' 


/n  X  1111 

(9. )  + = + 

x+a    x-c     x-a    x+c 

,,~  x  flf         6"         ar       a-  +  b 

(10-)  : — =+:r-i=;r-;  + 


(11.) 
(12.) 


x-a    x—b    x-a      x-b 

(3 -a-)  (a; +  10)     (8  +  x)  (x  -  10) 

a;+ll  a- 11 

x2  +px  +  q  _  x2  +px  + 1 

x2  +  rx  +  2q  ~  x2  +  rx  +  2t 


(131  (x-a)3  (x-b)3  (x-c)3 

K     ''  (c-a)(a-b)     (a-b)(b-c)     (b-c)(c-a) 

(u)  x  +  T  +  U  a;  +  T-U 

1  x2  +  (2-t)x  +  s(2-s-t)     x2  +  (2-s)x  +  t(2-s-<)     A 
when  2T=s  +  t-s2-st-t2. 

VOL.  I 


(22.) 

(23.) 
(24.) 
(25.) 


306  EXERCISES  XIX,  XX  chap. 

,,_  .  x^  +  ax  +  b    x2  +  cx  +  d    x"  +  ax  +  b'     x"  +  cx  +  d' 

(15.)  1 —  = 1 . 

x  +  a  x  +  e  x  +  a  x  +  c 

Rationalise  the  following  equations  and  reduce  the  resulting  equation  to 
as  simple  a  form  as  possible  : — 

(16.)  \/X  +  \/Y  +  \JZ  =  0,  where  X,  Y,  Z  are  rational  functions  of  the 
variables. 

(17.)  \/{x  +  a)  +  \/(x  +  b)  +  \J(x  +  c)  =  0. 

(18.)  \/Q.+x)  +  *J(i  +  x)-y/(9  +  x)  =  0. 

(19.)  [x-c+  {(x-c)n-  +  f-'ii]/[x  +  c+  {(x-c)-  +  y°-}h]  =  m. 

(20. )  x  -  a  =  V  {a-  -  vV*2  -  <*)} . 

(21.)  VaB+V(a»-7)  =  21/V(*-7). 

V»  +  3"_Va;  +  29' 

\/{2+x)  V(2-a;) 

V2  +  V(2  +  ^O     V2  -  V(2  -  *) ' 
(24. )  \J{x  +  a)  +  V(se  -  a)  +  V(&  +  a")  +  V(6  -«)  =  0. 

V(l+a;  +  a;i!)  +  V(l-a:  +  a;2)_ 

V(i+*)  +  V(i-*) 

(26. )  (y  -  s)  (OSB4-  &)*  +  («-»)  (ay  +  ft)4  +  (a  -  ?/)  (az  +  &)*  =  0. 

(27.)  2V(y-~)  =  0;  and  show  that  2x=  V(322/~)  (three  variables  a-,  y,  z). 

<28-»   v{»w(»--i)(+v^-v^-i)rvl^+1)1- 

(29.)  sb* +53!* -22=0. 

,Qn  v  v/(a  +  a;)      \/(a  +  a:)      Va; 

^ou. ;  (-. 

a;  a  c 

(31. )  v/(a  +  V»)  +  \/(a  -  vfc)  =  #fc 

(32.)  a£+y*+z*=0, 

where  a; +  2/ +  2=0. 


Exercises  XX. 

(On  t%e  Transformation  of  Systems  of  Equations.) 

[In  working  this  set  the  student  should  examine  carefully  the  logic  of  every 
step  he  takes,  and  satisfy  himself  that  it  is  consistent  with  his  data.  He 
should  also  make  clear  to  himself  whether  each  step  is  or  is  not  reversible.] 

(1.)  If  y  +  s  +  zJ^  +  x±y  +  2  =  0,  x  +  y  +  z*0, 

x  y  z 

41  1111 

then  -H (--  =  ■ 


x    y     z    x+y+z 


xiv  EXERCISES  XX  307 

(2.)  If  a*  +  y*-=i?, 

then  {{a?  +  z*)y\ -  +  {(a*  -  ys)z) 3  =  {(if  +  a8)*} s  ( Tait). 

(3.)  If  x,  y,  z  be  real,  ami  it'  x\y  -  z)  +  yi(z- x) +z4{x-y)  =  0,  then  two  at 
least  of  the  three  must  be  equal. 

(4.)  If  (x  +  y  +  z)3  =  x*  +  y3  +  z\ 

then  (x  +  y  +  z)-^1  =  x2n+l  +  y-»+1  +  z2"+] . 

(5.)  If 

(2>2x  +  2pry  +  r2z)  (q2x  +  2qsy  +  s"z)  —  [pqx  +  (ps  +  qr)y  +  rsz) 2, 

then  either  y-  -zx  =  0  or  ps  -  qr  =  0. 


(6.)  if  jp^+*pr+*>=0i 

where  r2  =  a;2  +  y-  +  z2, 

.1  «2  V2  z2 

then  -3-., 5  +  -^ — a  +  -5Ki 5  =  0, 

b-cr  -  p"     era-  -  p-     a~b~  -  p- 

where  p2  =  a2x-  +  b2y2  +  c2z2. 

(Important  in  the  theory  of  the  wave  surface. —  Tait. 

(7.)  If  |±*=!±!!=*±£,  andas+y+*=0i 

b-c     c-a     a-b 

show  that  each  of  them  is  equal  to  \/{2a;2/2(2<(2-  S6c)}. 

a(&y  +  cz  -  ckc)  =  b(cz  +  ax-  by)  =  c(oa;  +  by-  cz), 
a  +  b  +  c  =  0, 
x  +  y  +  z  =  0. 
x  +  2y  _  y  +  2z  _  z  +  2x 
2a  +  b~2b  +  c~2c~+a 


(8.) 

If 

and  if 

then 

(9.) 

If 

then 

(10.) 

If 

then 

(11.) 

If 

then 

/ZxY-  _Xxy  _2x2 
\Za)   _2a6~2ft2" 
2ab  +  b2  a2-b- 

X~a2  +  ab  +  b2'     V~a'-  +  ab  +  b2 


x3  +  y  =  y-  +  x. 

(a  -b)2  a  +  b       ab 

x  =  a  +  b  +  y. — -—,      y  =  ——  +  —-, 
4(«  +  o)  4        a  +  b 

(x-a)2-(y-b)2  =  b2. 

(12.)  If  a  —  ax  +  by  +  cz  +  dw, 

(3  =  bx  +  ay  +  dz  +  cw, 

y  =  ex  +  dy  +  az  +  bio, 

d  =  dx  +  cy  +  bz  +  aw, 
and  if 

/{a,  ft  7,  5)  =  (a  +  /3  +  7  +  5)(a-i3  +  7-5)(a-/3-7  +  5)(a  +  /3-7-5), 

then 

/(«,  /3,  y,  5)  =/(«,  6,  c,  d)f{x,  y,  z,  w). 

(13.)  If  x+ y +2=0,  then  Zl/*2=(Zl/a;)2. 


308  EXERCISES  XX,  XXI  chap. 


and 


Qin+n       fyni-\-n       gvi+n 


show  that  (2aj™n/(",+»))  (2a,""2/<m+">)  =  dm. 

(15.)  If  a_^=&_J=c_^a.+0}y=#OjZ*0J 

.,  ,  w-  -  z-     ,     z-  -  xr  x*  -  y 

then  a  +  J-. —  b-] =  c  + f-. 

b-c  c- a  a-b 

(16.)  If  x  +  {yz  -  x2)j(x2  +  y2  +  z2)  be  unaltered  by  interchanging  x  and  y,  it 

will  be  unaltered  by  interchanging  x  and  z,  provided  x,  y,  z  be  all  unequal ; 

and  it  will  vanish  if  x  +  y  +  z=l. 

(17.)  If  zxy/(y  4  2)  -  7?  =  xyz/(z  +  x)  -  y2,  and  x  +  y,  then  each  of  these  is 

equal  to  xyz/(x  +  y)  -  z2  and  also  to  yz  +  zx  +  xy. 

(18.)  Of  the  three  equations 

__x y  +  z 

x2  -  w2  ~  (m  + 1  )w2  -  (n  + 1  )yz ' 

V      _ s  +  jg 

y2-w2     (m+l)iv2-(7i+l)zx' 

z     _  %  +  y 

z2-w2     {m  +  l)vr~(n  +  l)xy' 
where  x #=2/  +  z,  any  two  imply  the  third  (Cayley). 
(19.)  Given 

-1-  V        +  ^—  =  1, 


1  +  x  +  xz     l  +  y  +  xy     l+z  +  yz 

x  xy  1 

.  +  ,  ■  ...       +,  ■  .  ...  =h 


1+x  +  xz     l+y  +  xy     l+z  +  yz 
none  of  the  denominators  being  zero,  then  x  =  y  =  z. 

(20.)  Given  ■2(y  +  z)2/x  =  3Sx,  2a;  *0,  prove  Z(y  +  z-x)3  +  II{y  +  z-x)  =  0. 

(21.)  Given  2a;  =0,  prove  2(a?  +  y3)/(a:  +  ?/)  +  5a7/~2(l/ai)  =  0. 

(22.)  Given  2a;  =  0,  prove  that  Ske'Sa^/XB6  is  independent  of  a;,  y,  z, 

(23. )  If  2a;5  =  -  5xyzSxy,  then  2a  =  0,  or  2a,4  -  Safy  +  1.x2y2  +  2Zx2yz  =  0. 

(24.)  If  II(ar  +  l)  =  a2+l,  n(a^-l)=a2-l,  and  2a-y  =  0,  then  x+y+z=0 
or  =  ±«. 

(25.)  If  x  +  y  +  z  +  u=0,  then  42x*  +  32,(y  +  z)(u  +  y)(u  +  z)  =  0,  where  the 
2  refers  to  the  four  variables  a;,  y,  z,  u. 


Exercises  XXI. 
(On  Elimination.) 
(1.)  Eliminate  x  between  the  equations 

x  +  l/x  =  y,     xn+l/x5  —  z. 
(2.)  If  z= \/{ay--d2ly),  y  =  \J(ax2-a2/x),  express  \J(az2  -  a2[z)  in  terms 
of  a;. 


XIV 

(3.) 

If 

the  i 

I 

(i.) 

Given 

prove  that 

EXERCISES  XXI  309 

(p(x)  =  (ax  -  arx)l(ax  +  arx)\ 
F(x)=2/{a*+ar*), 

4>{x  +  y)  =  (<p(x)  +  <p(y)  )/(l  +  <p{x)4>{y) ), 
¥{x  +  y)  =  F(x)¥(y)/(l+<p(x)cl>(y)). 
x(y  +  z-x)  _y(z  +  x-y)  _z(x  +  y  -z) 

a  b  c 

a(b  +  c-a) _b{c  +  a-  b)  _c(a  +  b-c) 
x  y  z 

(5.)  Given    bz  +  cy  =  cx  +  az  —  ay  +  bx,   x2  +  y2  +  z2=2yz  +  2zx  +  2xy,    prove 
that  one  of  the  functions  «±£>±e  =  0. 

(6.)  Show  that  the  result  of  eliminating  x  and  y  between  the  equations 
x    y     ,      x2    y"     „  „ 

a+b  =  1>     S  +  ^=1'     Xy=r> 
is  (b"c"-  +  a"-cr2)-p*  +  2abc2cf-(b-c"  +  a"-dn-  -  2a2b"-)p2  +  arb^d^a2  -  c2)  (b2  -  d?)  =  0. 
(7.)  Eliminate  x,  y,  x',  y'  from 

ax  +  by  =  c2,        x-  +  y2  =  c~,  ,       ,   _ 

a'x'  +  by  =  c'2,     x'2  +  y'2  =  c'2,     Xy  +  X  V  ~ 
(8.)  If  l/(x  +  a)  +  l/(y  +  a)  +  l/(z  +  a)  =  l/a,  with  two  similar  equations  it 
which  b  and  c  take  the  place  of  a,  show  that  Z(l/«)  =  0,  provided  a,  b,  c  be  all 
different. 

(9.)  Show  that  any  two  of  the  following  equations  can  be  deduced  from 
the  other  three  : — 

ax  +  be  =  zu,     by  +  ca  =  nv,     cz  +  db  =  vx,     du  +  ec  =  xy,     ev  +  ad  =  yz. 
(10.)  Eliminate  x,  y,  z  from  the  three  equations 
(z  +  x-y){x  +  y-z)  =  ay~, 
(■''  sy-z){y  +  z-x)  =  bzx,     [y  +  z-  x)  {z  +  x-  y)  =  cxy  ; 
and  show  that  the  result  is  abc  —  {a  +  b  +  c- 4)2. 


CHAPTER    XV. 
Variation  of  Functions. 

§  1.]  The  view  which  we  took  of  the  theory  of  conditional 
equations  in  last  chapter  led  us  to  the  problem  of  finding  a  set 
of  values  of  the  variables  which  should  render  a  given  conditional 
equation  an  identity.  There  is  another  order  of  ideas  of  at  least 
equal  analytical  importance,  and  of  wider  practical  utility,  which 
we  now  proceed  to  explain.  Instead  of  looking  merely  at  the 
values  of  the  variables  x,  y,  z,  .   .  .  which  satisfy  the  equation 

f(x,  y,  z,  .  .  .)  =  0, 

that  is,  which  render  tlie  function /(x,  y,  z, .  .  .)  zero,  we  consider 
all  possible  values  of  the  variables,  and  all  possible  corresponding 
values  of  the  function  ;  or,  at  least,  we  consider  a  number  of  such 
values  sufficient  to  give  us  a  clear  idea  of  the  whole  ;  then,  among 
the  rest,  we  discover  those  values  of  the  variables  which  render 
the  function  zero.  The  two  methods  might  be  illustrated  by  the 
two  possible  ways  of  finding  a  particular  man  in  a  line  of  soldiers. 
We  might  either  go  straight  to  some  part  of  the  ranks  where 
a  preconceived  theory  would  indicate  his  presence ;  or  we  might 
walk  along  from  one  end  of  the  line  to  the  other  looking  till  we 
found  him.  In  this  new  Avay  of  looking  at  analytical  functions, 
the  graphical  method,  as  it  is  called,  is  of  great  importance. 
This  consists  in  representing  the  properties  of  the  function  in 
some  way  by  means  of  a  geometrical  figure,  so  that  we  can  with 
the  bodily  eye  take  a  comprehensive  view  of  the  peculiarities  of 
any  individual  case. 


CHAP.   XV 


THE  GRAPHICAL  METHOD 


311 


GENERAL    PROPOSITIONS    REGARDING   FUNCTIONS    OF    ONE 

REAL    VARIABLE. 

§  2.]  For  the  present  we  confine  ourselves  to  the  case  of  a 
function  of  a  single  variable,  fix)',  and  we  suppose  that  all  the 
constants  in  the  function  are  real  numbers,  and  that  only  real 
values  are  given  to  the  variable  x.  "We  denote,  as  in  chap, 
xiii.,  §  1 7,  f(x)  by  y,  so  that 

V  =/(■'■)  (IX 

and  we  shall,  as  in  the  place  alluded  to,  speak  of  x  and  y  as 
the  independent  and  dependent  variables  ;  we  are  now,  in  fact, 
merely  following  out  more  generally  the  ideas  broached  there. 

Y 


Fig.  1. 


To  obtain  a  graphical  representation  of  the  variation  of  the 
function  /(.»•)  we  take  two  lines  X'OX,  Y'OY,  at  right  angles  to 
each  other  (co-ordinate  axes).  To  represent  the  values  of  x  we 
measure  x  units  of  length,  according  to  any  convenient  scale, 
from  the  intersection  0  along  X'OX  to  the  right  if  x  have  a 
positive  value,  to  the  left  if  a  negative  value.  To  represent  the 
values  of  y  we  measure  lengths  of  as  many  units,  according  to 
the  same  or,  it  may  be,  some  other  fixed  scale,  from  X'OX 
parallel  to  Y'OY,  upwards  or  downwards  according  as  these 
values  are  positive  or  negative. 

For  example,  suppose  that,  when  Ave  put  x  =  -  20,  x  =  —  7, 
x=  +  IS,  x=  +  37,  the  corresponding  values  of 


312 


are 


CONTINUITY  OF  FUNCTION  AND  OF  GRAPH 

/(-20),     /(-7),    /(  +  18),    /(+37) 
+  4,  -  10,        +7,  -  6 


CHAP. 


respectively  ;    so  that  we  have   the  following  scheme  of  corre- 
sponding values  : — 


X 

y 

-20 

-    7 
+  18 
+  37 

+    4 

-  10 

+    7 

-  6 

l 

Then  we  measure  off  OM2  (left)  =20,  OM4  (left)  =  7,  OM7  (right) 
=  18,  OM9  (right)  =  37  ;  and  M2P2  (up)  =  4,  M4P4  (down)  =  10, 
M7P7  (up)  =  7,  M9P9  (down)  =  6. 

To  every  value  of  the  function,  therefore,  corresponds  a  re- 
presentative point,  P,  whose  abscissa  (OM)  and  ordinate  (MP) 
represent  the  values  of  the  independent  and  dependent  variables; 
that  is  to  say,  the  value  of  x  and  the  corresponding  value  of  /(./:). 
Now,  when  we  give  x  in  succession  all  real  values  from  —  oo  to 
+  qo  ,  y  will  in  general  *  pass  through  a  succession  of  real  values 
without  at  any  stage  making  a  sudden  jump,  or,  as  it  is  put,  without 
becoming  discontinuous.  The  representative  point  will  therefore 
trace  out  a  continuous  curve,  such  as  Ave  have  drawn  in  Fig.  1. 
This  curve  Ave  may  call  the  graph  of  the  function. 

§  3.]  It  is  obvious  that  when  Ave  Icuoav  the  graph  of  a 
function  we  may  find  the  value  of  the  function  corresponding  to  any 
value  of  the  independent  variable  x  Avith  an  accuracy  that  depends 
merely  on  the  scale  of  our  diagram  and  on  the  precision  of  our 
drawing  instruments.  All  Ave  have  to  do  is  to  measure  off  the 
value  of  x  in  the  proper  direction,  OM7  say ;  then  draw  a 
parallel  through  M7  to  the  axis  of  y,  and  find  the  point  P7  Avhere 
this  parallel  meets  the  graph  ;  then  apply  the  compasses  to  M7P7, 
and  read  off  the  number  of  units  in  M7P7  by  means  of  the  scale 
of  ordinates.     This  number,   taken  positive  if  P7  be  above  the 


We  shall  retina  to  the  exceptional  eases  immediately. 


xv  GRAPHICAL  SOLUTION  OF  AX  EQUATION  313 

axis  of  x,  negative  if  below,  will  be  the  required  value  of  the 
function. 

The  graph  also  enables  us  to  the  same  extent  to  solve  the 
converse  problem,  Given  the  value  of  the  function,  to  find  the  corre- 
sponding value  or  values  of  the  independent  variable. 

Suppose,  for  example,  that  Fig.  1  gives  the  graph  of  f(x), 
and  Ave  wish  to  find  the  values  of  x  for  which  f(x)  =  +  7.  All 
we  have  to  do  is  to  measure  ON7  =  7  upwards  from  0  on  the  axis 
of  y ;  then  draw  aline  (dotted  in  the  figure)  through  N7  parallel 
to  the  axis  of  x,  and  mark  the  points  where  this  line  meets  the 
graph.  If  P7  be  one  of  them,  we  measure  N7P7  (obviously  =  OM7) 
by  means  of  the  scale  of  abscissae,  and  the  number  thus  read  off 
is  one  of  the  values  of  x  for  which  f(x)  =  +  7 ;  the  others  are 
found  by  taking  the  other  points  of  intersection,  if  such  there  be. 

Observe  that  the  process  we  have  just  described  is  equivalent 
to  solving  the  equation 

f{x)  =  +  7. 

In  particular  we  might  look  for  the  values  of  x  for  which  /(./•) 
reduces  to  zero.  When/(a;)  becomes  zero,  that  is,  when  the  ordin- 
ate of  the  graphic  point  is  zero,  the  graph  meets  the  axis  of  x. 
The  axis  of  x,  then,  in  this  case  acts  the  part  formerly  played  by 
the  dotted  parallel,  and  the  values  of  x  required  are  -  OMj, 
-OM3,  +OM,  +OM8,  +OM10,  where  OM„  OM3,  Sec,  stand 
merely  for  the  respective  numbers  of  units  in  these  lengths  when 
read  off  upon  the  scale  of  abscissae.      Hence 

By  means  of  the  graph  of  the  function  /(.c)  we  can  solve  the 
equation 

/(■*)  =  0  (2). 

The  roots  of  this  equation  are,  in  point  of  fact,  simply  the  values 
of  x  which  render  the  function  f(x)  zero  ;  we  may  therefore, 
when  it  is  convenient  to  do  so,  speak  of  them  as  the  roots  of  the 
function  itself. 

§  4.]  The  connection  between  the  general  discussion  of  a 
function  by  means  of  the  graphical  or  any  other  method  and  the 
problem  of  solving  a  conditional  equation  will  now  be  apparent 
to  the  reader,  and  he  will  naturally  ask  himself  how  the  graph 


314 


EXAMPLE 


CHAP. 


is  to  be  obtained.  We  cannot,  of  course,  lay  down  all  the 
infinity  of  points  on  the  graph,  but  we  can  in  various  ways  infer 
its  form.  In  particular,  we  can  assume  as  many  values  of  the 
independent  variable  as  we  please,  and,  from  the  known  form  of 
the  function  f(x),  calculate  the  corresponding  values  of  y.  We 
can  thus  lay  down  as  many  graphic  points  as  we  please.  If  care 
be  taken  to  get  these  points  close  enough  where  the  form  of  the 
curve  appears  to  be  changing  rapidly,  we  can  draw  with  a  free 
hand  a  curve  through  the  isolated  points  which  will  approach 
the  actual  graph  sufficiently  closely  for  most  practical  purposes. 

When  the  form  of  the  function  is  unknown,  and  has  to  be 
determined  by  observation — as,  for  example,  in  the  case  of  the 
curve  which  represents  the  height  of  the  barometer  at  different 
times  during  the  day — the  course  we  have  described  is  the  one 
actually  followed,  only  that  the  value  of  y  is  observed  and  not 
calculated. 

Before  going  further  into  details  it  will  be  well  to  illustrate 
by  a  simple  example  the  above  process,  Avhich  may  be  unfamiliar 
to  many  readers. 

Example. 

Let  the  function  to  be  discussed  be  l-x",  then  the  equation  (1)  which 
determines  the  graph  is  y=  1  -  a?. 

We  shall  assume,  for  the  present  without  proof,  what  will  probably  be  at 
once  admitted  by  the  reader,  that,  as  x  increases  without  break  from  0  up  to 
+  oo,  x2  increases  without  break  from  0  up  to  +  oo  ;  and  that  a,2>  =  <1, 
according  as  x>  =  <  1. 

Consider,  in  the  first  place,  merely  positive  values  of  x.  When  x  =  0, 
y  =  l  ;  and,  so  long  as  x<l,  l-x-  is  positive.  When  x=l,  y  =  l  -1  =  0. 
When  x>l,  then  »,2>1  and  1  -x2  is  negative.  Hence  from  x  =  0  until  x=l, 
l-x"-  continually  decreases  numerically,  but  remains  always  positive.  When 
x  =  l,  l-x2  becomes  zero,  and  when  x  is  further  increased  l-x2  becomes 
negative,  and  remains  so,  but  continually  increases  in  numerical  value. 

We  may  represent  these  results  by  the  following  scheme  of  corresponding 
values  : — 


X 

y 

0 

i 

<+l 

+ 

+  1 

0 

>+l 

- 

+  0O 

—   CO 

XV 


EXAMPLE 


315 


The  general  form  of  the  graph,  so  far  as  the  right-hand  side  of  the  axis  of  y 
is  concerned,  will  be  as  in  Fig.  2. 

As  regards  negative  values  of 
x  and  the  left-hand  side  of  the 
axis  of  }i,  in  the  present  case, 
it  is  merely  necessary  to  notice 
that,  if  we  put  a;  =  -a,  the  re- 
sult, so  far  as  1  -  x2  is  concerned, 
is  the  same  as  if  we  put  x  =  +a; 
for  1  -  ( -  af=  1  -  (  +  a)-.  Hence 
for  every  point  P  on  the  curve, 
whose  abscissa  and  ordinate  are 
+  OM  and  +  MP,  there  will  be 
a  point  P',  whose  abscissa  and 
ordinate  are  -  OM  and  +  M  P.  P 
and  P'  are  the  images  of  each 
other  with  respect  to  Y'Y  ;  and  the  part  AP'B'  of  the  graph  is  merely  an 
image  of  the  part  APB  with  respect  to  the  line  Y'Y. 

Let  us  see  what  the  graph  tells  us  regarding  the  function  1  -x". 

First  we  see  that  the  graph  crosses  the  ar-axis  at  two  points  and  no  more, 
those,  namely,  for  which  x=  +  1  and  x=  -  1.  Hence  the  function  1  -x-  has 
only  two  roots,  +1  and  -  1  ;  in  other  words,  the  equation 

1-^  =  0 

has  two  real  roots,  x  —  -hi,  x=  -  1,  and  no  more. 

Secondly.  Since  the  part  BAB'  of  the  graph  lies  wholly  above,  and  the 
parts  C'B',  CB  wholly  below  the  a:-axis,  we  see  that,  for  all  real  values  of  x 
lying  between  -1  and  +1,  the  function  1  -ar  is  positive,  and  for  all  other 
real  values  of  x  negative. 

Thirdly.  We  see  that  the  greatest  positive  value  of  1  -x2  is  1,  correspond- 
ing to  x—0  ;  and  that,  by  making  x  sufficiently  great  (numerically),  we  can 
give  1  -x-  a  negative  value  as  large,  numerically,  as  we  please. 

All  these  results  could  be  obtained  by  direct  discussion  of  the  function, 
but  the  graph  indicates  them  all  to  the  eye  at  a  glance. 

§  5.]  Hitherto  we  have  assumed  that  there  are  no  breaks  or 
discontinuities  in  the  graph  of  the  function.  Such  may,  how- 
ever, occur ;  and,  as  it  is  necessary,  when  we  set  to  work  to 
discuss  by  considering  all  possible  cases,  above  all  to  be  sure 
that  no  possible  case  has  escaped  our  notice,  we  proceed  now  to 
consider  the  exceptions  to  the  statement  that  the  graph  is  in 
general  a  continuous  curve. 


f. 


The  function  f(x)  may  become  infinite  for  a  finite  value  of  x. 


316 


DIFFERENT  KINDS  OF  DISCONTINUITY 


CHAP. 


Example  1. 

Consider  the  function  1/(1 -a;).  "When  a;  is  a  very  little  less  than  +  1, 
say  x=  -99999,  then  y  =  \j(\-x)  gives  y  =  +  1/-00001  =  +100000  ;  that  is  to 
say,  y  is  positive  and  very  large  ;  and  it  is  obvious  that,  by  bringing  x  suffi- 
ciently nearly  up  to  + 1,  we  can  give  y  as  large  a  positive  value  as  we  please. 
On  the  other  hand,  if  a:  be  a  very  little  greater  than  +1,  say  x=  +1  '00001, 
then  2/=l/(-  "00001)=  -100000  ;  and  it  is  obvious  that,  by  making  x  ex- 
ceed 1  by  a  sufficiently  small  quantity,  y  can  be  made  as  large  a  negative 
quantity  as  we  please. 

The  graph  of  the  function  1/(1  -  x)  for  values  of  x  near  +  1  is  therefore  as 
follows : — 

The  branch  BC  ascends  to 
an  infinite  distance  along 
KAK'  (a  line  parallel  to  the 
2/-axis  at  a  distance  from  it 
=  +1),  continually  coming 
nearer  to  KAK',  but  never 
reaching  it  at  any  finite  dis- 
tance from  the  a;-axis.  The 
branch  DE  comes  up  from  an 
infinite  distance  along  the 
other  side  of  KAK'  in  a  similar 
manner. 

Here,  if  we  cause  x  to  in- 
crease from  a  value  OL  very 
little  less  than  + 1  to  a  value 
OM  very  little  greater,  the 
value  of  y  will  jump  from  a  very  large  positive  value  +  LC  to  a  very  large 
negative  value  -  WD  ;  and,  in  fact,  the  smaller  we  make  the  increase  of  x, 
provided  always  we  pass  from  the  one  side  of +  1  to  the  other,  the  larger  will 
be  the  jump  in  the  value  of  y. 

It  appears  then  that,   for  x= +\,   1/(1— a)  is  both  infinite  and  discon- 
tinuous. 

Example  2. 

y=  1/(1  -x)~. 

We  leave  the  discussion  to  the 
reader.    The  graph  is  as  in  Fig.  4. 

The  function  becomes  infinite 
when  x=  +1 ;  and,  for  a  very  small 
increment  of  x  near  this  value,  the 
increment  of  y  is  very  large.  In  fact, 
if  we  increase  or  diminish  x  from  the 
value  +  1  by  an  infinitely  small 
amount,  y  will  diminish  by  an  in- 
finitely great  amount. 

Here  again  we  have  infinite  value  of  the   function,   and  accompanying 
discontinuity. 


Y 

B 

K 

M 

O 

I 

k' 

\ 

X 

r 

Fig.  3. 


Fio.  1. 


XV 


DIFFERENT  KINDS  OF  DISCONTINUITY 


31 


Fio.  5. 


II.  The  value  of  the  function  may  make  a  jump  without  becoming 
infinite. 

The  graph  for  the  neighbourhood  of  such  a  value  would  be 
of  the  nature  indicated  in  Fig.  5,  where,  while  x  passes  through 
the  value  (DM,  y  jumps  from  MP 
to  MQ. 

Such  a  case  cannot,  as  we  shall 
immediately  prove,  occur  with  in- 
tegral functions  of  x.  In  fact  it  ol  M 
cannot  occur  with  any  algebraical 
function,  so  that  we  need  not 
further  consider  it  here. 

The  cases  we  have  just  considered  lead  us  to  give  the  follow- 
ing formal  definition. 

A  function  is  said  to  he  continuous  when  for  an  infinitely  small 
change  in  the  value  of  the  independent  variable  the  change  in  the  value 
of  the  function  is  also  infinitely  small ;  and  to  be  discontinuous  when 
for  an  infinitely  small  change  of  the  independent  variable  the  change  in 
the  value  of  the  function  is  either  finite  or  infinitely  great. 

III.  It  may  happen  that  the  value  of  a  function,  all  of  whose  con- 
stants are  real,  becomes  imaginary  for  a  real  value  of  its  variable. 

Example. 

This  happens  with  the  function  +  \J{1  -  x").  If  we  confine  ourselves  to  the 
positive  value  of  the  square  root,  so  that  we  have  a  single-valued  function  to 
deal  with,  the  graph  is  as  in  Fig.  6  : — 

a  semicircle,   in  fact,  whose  centre  is  at  the 
origin. 

For  all  values  of  a;>+l,  or  <— 1,  the 
value  of  y=  +  \/(l  -  ar)  is  imaginary  ;  and  the 
graphic  points  for  them  cannot  be  constructed 

-      in  the  kind  of  diagram  we  are  now  using. 

The  continuity  of  the  function  at  A  can- 
not, strictly  speaking,  be  tested  ;   since,  if  we 
attempt  to  increase  x  beyond  + 1,  y  becomes 
imaginary,  and  there  can  be  no  question  of  the 
magnitude  of  the  increment,  from  our  present  point  of  view  at  least.* 

No  such  case  as  this  can  arise  so  long  as /(.?•)  is  a  rational 

algebraical  function. 


Fio.  6. 


See  below,  §  18. 


318  LIMITING  CASES  chap. 

We  have  now  enumerated  the  exceptional  cases  of  functional 
variation,  so  far  at  least  as  is  necessary  for  present  purposes. 
Graphic  points,  at  which  any  of  the  peculiarities  just  discussed 
occur,  may  be  generally  referred  to  as  critical  points. 


ON    CERTAIN    LIMITING   CASES    OF    ALGEBRAICAL    OPERATION. 

§  6.]  We  next  lay  down  systematically  the  following  propo- 
sitions, some  of  which  we  have  incidentally  used  already.  The 
reader  may,  if  he  choose,  take  them  as  axiomatic,  although,  as 
we  shall  see,  they  are  not  all  independent.  The  important 
matter  is  that  they  be  thoroughly  understood.  To  secure  that 
they  be  so  we  shall  illustrate  some  of  them  by  examples.  In 
the  meantime  we  caution  the  reader  that  by  "  infinitely  small " 
or  "infinitely  great"  we  mean,  in  mathematics,  "  smaller  than 
any  assignable  fraction  of  unity,"  or  "  as  small  as  we  please,"  and 
"greater  than  any  assignable  multiple  of  unity,"  or  "as  great  as 
Ave  please."  He  must  be  specially  on  his  guard  against  treating 
the  symbol  <x> ,  which  is  simply  an  abbreviation  for  "  greater 
than  any  assignable  magnitude,"  as  a  definite  quantity.  There 
is  no  justification  for  applying  to  it  any  of  the  laws  of  algebra, 
or  for  operating  with  it  as  we  do  with  an  ordinary  symbol  of 
quantity. 

I.  If  P  be  constant  or  variable,  provided  it  does  not  become 
infinitely  great  when  Q  becomes  infinitely  small,  then  when  Q  becomes 
infinitely  small  PQ  becomes  infinitely  small. 

Observe  that  nothing  can  be  inferred  without  further  examin- 
ation in  the  case  where  P  becomes  infinitely  great  when  Q 
becomes  infinitely  small.  This  case  leads  to  the  so-called  inde- 
terminate form  oo  x  0.* 

Example  1. 

Let  us  suppose,  for  example,  that  P  is  constant,  =100000,  say.  Then,  if 
we  make  Q  =  l/100000,  we  reduce  PQ  to  1  ;  if  we  make  Q  =  1/100000000000, 
we  reduce  PQ  to  1/1000000  ;  and  so  on.  It  is  abundantly  evident,  therefore, 
that  by  making  Q  sufficiently  small  PQ  can  be  made  as  small  as  we  please. 


*  Indeterminate  forms  are  discussed  in  chap,  xxv 


ZV  LIMITING  CASES  319 

Example  2. 

LetP  =  x  +  l,     Q  =  a:-1. 

Here,  when  x  is  made  to  approach  the  value  + 1,  P  approaches  the  finite 
value  +  2,  while  Q  approaches  the  value  0.  Suppose,  for  example,  we  put  x  —  1 
+  1/100000,  then 

PQ  =  (2  + 1/100000)  x  1/100000, 
^2/100000  + 1/1010, 
and  so  on.     Obviously,  therefore,  by  sufficiently  diminishing  Q,  we  can  make 
PQ  as  small  as  we  please. 

Example  3. 

Y  =  l/(x--l),     Q=jb-1. 

Here  we  have  the  peculiarity  that,  when  Q  is  made  infinitely  small,  P  (see 
below,  Proposition  III.)  becomes  infinitely  great.  We  can  therefore  no  longer 
infer  that  PQ  becomes  infinitely  small  because  Q  does  so.  In  point  of  fact, 
PQ=(«-  l)/(x--  l)=l/(aj+l),  which  becomes  1/2  when  x=l. 

II.  If  ¥  be  either  constant  or  variable,  provided  it  do  not  become 
infinitely  small  when  Q  becomes  infinitely  great,  then  when,  Q  becomes 
infinitely  great  PQ  becomes  infinitely  great. 

The  case  where  P  becomes  infinitely  small  when  Q  becomes 
infinitely  great  must  be  further  examined ;  it  is  usually  referred 
to  as  the  indeterminate  form  0  x  oo . 

Example  1. 

Suppose  P  =  l/100000.  Then,  by  making  Q  =  100000,  we  reduce  TQ  to  1 ; 
by  making  Q  =  100000000000  we  reduce  PQ  to  1000000  ;  and  so  on.  It  is 
clear,  therefore,  that  by  sufficiently  increasing  Q  we  could  make  PQ  exceed 
any  number,  however  great. 

The  student  should  discuss  the  following  for  himself : — 

Example  2. 

Y=x  +  \,     Q  =  l/(z-l). 
PQ  =  oo  whena;=l. 
Example  3. 

P=(a;-l)a,     Q  =  l/(.*-l). 
PQ  =  0when  x=l. 

III.  If  P  be  either  constant  or  variable,  provided  it  do  not  become 
infinitely  small  when  Q  becomes  infinitely  small,  then  when  Q  becomes 
infinitely  small  P/Q  becomes  infinitely  great. 

The  case  where  P  and  Q  become  infinitely  small  for  the  same 
value  of  the  variable  requires  further  examination.     This  gives 

the  so-called  indeterminate  form  -• 


320  LIMITING  CASES 


CHAP. 


Example  1. 

Suppose  P  constant  =  1/100000.  If  we  make  Q  =  1/100000,  P/Q  becomes 
1 ;  if  we  make  Q  =  1/100000000000,  P/Q  becomes  1000000  ;  and  so  on.  Hence 
we  see  that,  if  only  we  make  Q  small  enough,  we  can  make  P/Q  as  large  as 
we  please. 

The  student  should  examine  arithmetically  the  two  following  cases  : — 

Example  2. 

T=x  +  1,     Q=a-1. 

P/Q  =  oo  when  x—1. 
Example  3. 

P=*-l,     Q=«-l. 
P/Q=l  whencc=l. 

IV.  If  P  be  either  constant  or  variable,  provided  it  do  not  become 
infinitely  great  when  Q  becomes  infinitely  great,  then  when  Q  becomes 
infinitely  great  P/Q  becomes  infinitely  small. 

The  case  where  P  and  Q  become  infinitely  great  together  re- 
quires further  examination.     This  gives  the  indeterminate  form 

00 
00 

Example  1. 

Suppose  P  constant  =  100000.  If  we  make  Q  =  100000,  P/Q  becomes  1; 
if  we  make  Q  =  100000000000,  P/Q  becomes  1/1000000  ;  and  so  on.  Hence  by 
sufficiently  increasing  Q  we  can  make  P/Q  less  than  any  assignable  quantity. 

Example  2. 

P=aj+1,     Q=l/(as-l). 

p/Q  =  0  when  x—1. 
Example  3. 

P  =  l/(a;-l)a,     Q  =  l/(.z-l). 

P/Q  =  oo  when  sc=l. 

V.  If  P  and  Q  each  become  infinitely  small,  then  P  +  Q  becomes 
infinitely  small. 

For,  let  P  be  the  numerically  greater  of  the  two  for  any 
value  of  the  variable.  Then,  if  the  two  have  the  same  sign,  and, 
a  fortiori,  if  they  have  opposite  signs,  numerically 

P  +  Q  <  2P. 

Now  2  is  finite,  and,  by  hypothesis,  P  can  be  made  as  small  as 
we  please.  Hence,  by  I.  above,  2P  can  be  made  as  small  as 
we  please.     Hence  P  +  Q  can  be  made  as  small  as  we  please. 

VI.  If  either  P  or  Q  become  infinitely  great,  or  if  P  and  Q  each 


XV 


LIMITING  CASES  321 


become  infinitely  great  and  both  have  finally  the  same  sign,  then  P  +  Q 
becomes  infinitely  great. 

Proof  similar  to  last. 

The  inference  is  not  certain  if  the  two  have  not  ultimately 
the  same  sign.  In  this  case  there  arises  the  indeterminate 
form  oo  -  co  . 

Example  1. 

?=x*/(x-l)*,     Q  =  (2x-\)/(x-ir-. 
When  x=  1,  we  ha ve  P  =  1/0  =  +  oo ,     Q ,  =  1  /0  =  +  oo  .     Also 

F  +  Q  =  rA^+2X~l     3S  +  2X~l 


(x-i)-'(z-iy     (x-iy 

Example  2. 


2  i  i 

=  -=oo,  when  x=l. 


P=a?/(a!-l)2,     q=-(2x-l)J(x-lf. 

Here  x=l  makes  P=+oo,  Q=-oo,  so  that  we  cannot  infer  r  +  Q  =  <». 
In  fact,  in  this  case, 

p.0__£! 2*-l_(a:-l)a 

L+K-(;c-lr<     (x-lf-ix-l)*-1 

for  all  values  of  x,  or,  say,  for  any  value  of  x  as  nearly  =  +  1  as  we  please.  In 
this  case,  therefore,  by  bringing  x  as  near  to  +1  as  we  please,  we  cause  the 
value  of  P  +  Q  to  approach  as  near  to  +1  as  we  please. 

§  7.]  The  propositions  stated  in  last  paragraph  are  the  funda- 
mental principles  of  the  theory  of  the  limiting  cases  of  algebraical 
operation.  This  subject  will  be  further  developed  in  the  chapter 
on  Limits  in  the  second  part  of  this  work. 

In  the  meantime  we  draw  the  following  conclusions,  which 
will  be  found  useful  in  what  follows  : — 

I.  If  P  =  P^  .  .  .  PJt,  then  P  will  remain  finite  if  P,,  P2,  .  .  ., 
Pn  all  remain  finite. 

P  will  become  infinitely  small  if  one  or  more  of  the  functions 
Pn  P2,  .  .  .,  ~Pn  become  infinitely  small,  provided  none  of  the  remain- 
ing ones  become  infinitely  great. 

P  will  become  infinitely  great  if  one  or  more  of  the  functions  Pn 
P2,  .  .  .,  Pn  become  infinitely  great,  provided  none  of  the  remaining 
ones  become  infinitely  small. 

II.  If  S  =  P,  +  P,  +  .  .  .  +  Pn,  then  S  will  remain  finite  if  P,, 
P2,  .  .  .,  P,j,  each  remain  finite. 

VOL.  I  Y 


322  LIMITING  CASES  chap. 

S  will  become  infinitely  small  if  Pu  P2,  .  .  .,  Pn  each  become  in- 
finitely small. 

S  vMl  become  infinitely  great  if  one  or  more  of  the  functions  P,, 
P3,  .  .  .,  Pn  become  infinitely  great,  provided  all  those  that  become 
infinitely  great  have  the  same  sign. 

III.   Consider  the  quotient  P/Q. 

p 

j-  xoill  certainly  be  finite  if  both  P  and  Q  be  finite, 

may  be  finite  if  P  =  0,  Q  =  0, 

or  if  P  —  oo  ,        Q  =  oo  . 

P 

pr  icill  certainly  =  0  if  P  =  0,         Q.  4=  0, 

or  ?/  P  4=  co  ,       Q  =  oo  • 

may  =0i/P  =  0,  Q  =  0, 

or  if  P  =  co  ,        Q  =  co  , 

P 

pr  will  certainly  =  co  (/*  P  =  oo  ,       Q  4=  oo , 

^  on/P  +  O,  Q  =  0 ; 

may  =  oo  if  P  =  0,         Q  =  0, 
or  ?/  P  =  oo  ,       Q  =  co . 


ON    THE   CONTINUITY    OF   FUNCTIONS,    MORE    ESPECIALLY    OF 
RATIONAL   FUNCTIONS. 

§  8.]  We  return  now  to  the  question  of  the  continuity  of 
functions. 

By  the  increment  of  a  function  f(x)  corresponding  to  an  increment 

h  of  the  independent  variable  x  we  mean  f(x  +  h)  -  f  {•>')■ 

For  example,  HfixJ—x1,  the  increment  is  (x  +  h)2-xi—2xh  +  Jr. 
lff(x)  =  l/x,  the  increment  is  l/{x  +  h)-l/x=  -h/x(x  +  h). 

The  increments  may  be  either  positive  or  negative,  according 
partly  to  choice  and  partly  to  circumstance.  The  increment  of 
the  independent  variable  x  is  of  course  entirely  at  our  disposal ; 
but  when  any  value  is  given  to  it,  and  when  x  itself  is  also 
assigned,  the  increment  of  the  function  or  dependent  variable 
is  determined. 


xv  CONTINUITY  OF  A  SUM  OR  PRODUCT  323 

Example. 

Let  the  function  be  1/x,  then  if  x=l,  h  =  3,  the  corresponding  increment 
ofl/.ris  -3/1(1+3)=  -3/4.  Ifz=2,  h  =  3,  the  increment  of  1/x  is  -3/2(2  +  3) 
~  -  3/10,  and  so  on. 

If  P  be  a  function  of  x,  and  p  denote  its  increment  when  x 
is  increased  from  x  to  x  +  h,  then,  by  the  definition  of  p,  P  +p  is 
the  value  of  P  when  x  is  altered  from  x  to  x  +  A. 

"We  can  now  prove  the  following  propositions  : — 

I.  The  algebraic  sum  of  any  finite  number  of  continuous  functions 
is  a  continuous  function. 

Let  us  consider  S  =  P  -  Q  +  R,  say.  If  the  increments  of  P, 
Q,  R,  when  x  is  increased  by  h,  be  p,  q,  r,  then  the  value  of  S, 
when  x  is  changed  to  x  +  h,  is  (P  +  p)  -  (Q  +  q)  +  (R  +  r)  ;  and  the 
increment  of  S  corresponding  to  h  is  p  -  q  +  r.  Now,  since  P,  Q, 
R  are  continuous  functions,  each  of  the  increments,  p,  q,  r,  becomes 
infinitely  small  when  h  becomes  infinitely  small.  Hence,  by  §  7, 
I.,  p  —  q  +  r  becomes  infinitely  small  when  h  becomes  infinitely 
small.     Hence  S  is  a  continuous  function. 

The  argument  evidently  holds  for  a  sum  of  any  number  of 
terms,  provided  there  be  not  an  infinite  number  of  terms. 

II.  The  p-oduct  of  a  finite  number  of  continuous  functions  is  a 
continuous  function  so  long  as  all  factors  remain  finite. 

Consider,  in  the  first  place,  PQ.  Let  the  increments  of  P 
and  Q,  corresponding  to  the  increment  h  of  the  independent  vari- 
able x,  be  p  and  q  respective^.  Then  when  x  is  changed  to  x  +  h 
PQ  is  changed  to  (P  +  p)  (Q,  +  q),  that  is,  to  VQ,  +  pQ,  +  q~P  +  pq. 
Hence  the  increment  of  PQ  corresponding  to  h  is 

jjQ  +  ^P  +pq. 

Xow,  since  P  and  Q  are  continuous,  p  and  q  each  become  in- 
finitely small  when  h  becomes  infinitely  smalL  Hence  by  §  7,  I. 
and  II.,  it  follows  that  pQ  +  qP  +  pq  becomes  infinitely  small 
when  h  is  made  infinitely  small ;  at  least  this  will  certainly  be 
so,  provided  P  and  Q  remain  finite  for  the  value  of  x  in  question, 
which  we  assume  to  be  the  case. 

It  follows  then  that  PQ  is  a  continuous  function. 

Consider  now  a  product  of  three  continuous  functions,  say 
PQR.     By  what  has  just  been  established,  PQ  is  a  continuous 


324  ANY  INTEGRAL  FUNCTION  CONTINUOUS  chap. 

function,  which  we  may  denote  by  the  single  letter  S ;   then 
PQR  =  SR  where  S  and  R  are  continuous.     But,  by  last  case,  SR 
is  a  continuous  function.     Hence  PQR  is  a  continuous  function. 
Proceeding  in  this  way,  we  establish  the  proposition  for  any 
finite  number  of  factors. 

Cor.  1.  If  A  be  constant,  and  P  a  continuous  function,  then  AP 
is  a  continuous  function. 

This  can  either  be  established  independently,  or  considered 
as  a  particular  case  of  the  main  proposition,  it  being  remembered 
that  the  increment  of  a  constant  is  zero  under  all  circumstances. 

Cor  2.  Axm,  where  A  is  constant,  and  in  a  positive  integer,  is  a 
continuous  function. 

For  xm  =  x  x  xx  .  .  .  x  x  (m  factors),  and  x  is  continuous,  being 
the  independent  variable  itself.  Hence,  by  the  main  proposi- 
tion, xm  is  continuous.  Hence,  by  Cor.  1,  At'"  is  a  continuous 
function. 

Cor.  3.  Every  integral  function  of  x  is  continuous ;  and  cannot 
become  infinite  for  a  finite  value  of  x. 

For  every  integral  function  of  x  is  a  sum  of  a  finite  number 
of  terms  such  as  Ax"1.  Now  each  of  these  terms  is  a  continuous 
function  by  Cor.  2.  Hence,  by  Proposition  I.,  the  integral  func- 
tion is  continuous.  That  an  integral  function  is  always  finite 
for  a  finite  value  of  its  variable  follows  at  once  from  §  7,  I. 

III.  If  P  and  Q  be  integral  functions  of  x,  then  P/Q  is  finite  and 
continuous  for  all  finite  values  of  x,  except  such  as  render  Q  =  0. 

In  the  first  place,  if  Q  4=  0,  then  (see  §  7,  III.)  P/Q  can  only 
become  infinite  if  either  P,  or  both  P  and  Q,  become  infinite  ;  but 
neither  P  nor  Q  can  become  infinite  for  a  finite  value  of  x,  because 
both  are  integral  functions  of  x.  Hence  P/Q  can  only  become 
infinite,  if  at  all,  for  values  of  x  which  make  Q  =  0. 

If  a  value  which  makes  Q  =  0  makes  P  4=  0,  then  P/Q  certainly 
becomes  infinite  for  that  A-alue.  But,  if  such  a  value  makes  both 
Q  =  0  and  also  P  =  0,  then  the  matter  requires  further  investi- 
gation. 

Next,  as  to  continuity,  let  the  increments  of  P  and  Q  corre 


XV  CONTINUITY  OF  A  RATIONAL  FUNCTION  325 

sponding  to  h,  the  increment  of  x,  be  p  and  q  as  heretofore. 
Then  the  increment  of  P  Q  is 

Y+p  _  P  _  pQ  -  gP 

Q  +  'l  Q~Q(Q  +  ?)" 
Now,  by  hypothesis,  ^  and  q  each  become  infinitely  small 
when  h  does  so.  Also  P  and  Q  remain  finite.  Hence  pQ  -  qP 
becomes  infinitely  small.  It  follows  then  that  (pQ  -  #P)/Q(Q  +  q) 
also  becomes  infinitely  small  when  h  does  so,  provided  always 
(see  §  6)  that  Q  does  not  vanish  for  the  value  of  x  in  question. 

Example. 

The  increment  of  l/(se— 1)  corresponding  to  the  increment,  h,  of  a:  is 
l/(x  +  h-l)-l/(x-l)=  -  h/(x - 1) (a*+ h - 1).  N ow,  if  x  =  2,  say,  this  becomes 
-  hftl+h),  which  clearly  becomes  infinitely  small  when  h  is  made  infinitely 
small.  On  the  other  hand,  if  x—1,  the  increment  is  -h/Oh,  which  is 
infinitely  great  so  long  as  h  has  any  value  differing  from  0  by  ever  so  little. 

§  9.]  When  a  function  is  finite  and  continuous  between  two 
values  of  its  independent  variable  x  =  a  and  x  =  b,  its  graph  forms 
a  continuous  curve  between  the  two  graphic  points  whose 
abscissas  are  a  and  b  ;  that  is  to  say,  the  graph  passes  from  the 
one  point  to  the  other  without  break,  and  without  passing  any- 
where to  an  infinite  distance. 

From  this  we  can  deduce  the  following  important  pro- 
position : — - 

Jff(x)  be  continuous  from  x  -  a  to  x  =  b,  and  iff(a)  =p,  f(b)  =  q, 
then,  as  x  passes  through  every  algebraical  value  between  a  and  b,  fix) 
passes  at  least  once,  and,  if  more  than  once,  an  odd  number  of  times 
through  every  algebraical  value  between  p  and  q. 

Let  P  and  Q  be  the  graphic  points  corresponding  to  x  =  a  and 
x  =  b,  AP  and  BQ  their  ordinates  ;  then  AP  =  p,  BQ  =  q.  We 
have  supposed  p  and  q  both  positive  ;  but,  if  either  were  negative, 
we  should  simply  have  the  graphic  point  below  the  a'-axis,  and 
the  student  will  easily  see  by  drawing  the  corresponding  figure 
that  this  would  alter  nothing  in  the  following  reasoning. 

Suppose  now  r  to  be  any  number  between  p  and  q,  and 
draw  a  parallel  UV  to  the  z-axis  at  a  distance  from  it  equal 
to  r  units  of  the  scale  of  ordinates,  above  the  axis  if  r  be 
positive,  below  if  r  be  negative.     The  analytical  fact  that  r  is 


326 


LIMITS  FOR  THE  ROOTS  OF  AN  EQUATION 


CHAP. 


intermediate  to  p  and  q  is  represented  by  the  geometrical  fact 
that  the  points  P  and  Q  lie  on  opposite  sides  of  UV. 


Y 

Q 

u 

f? 

R         R 



V 

p 

0 

A   M,     M2        Nlj     B                    X 

Fig.  7. 

Now,  since  the  graph  passes  continuously  from  P  to  Q,  it 
must  cross  the  intermediate  line  UV ;  and,  since  it  begins  on  one 
side  and  ends  on  the  other,  it  must  do  so  either  once,  or  thrice, 
or  five  times,  or  some  odd  number  of  times. 

Every  time  the  graph  crosses  UV  the  ordinate  becomes  equal 
to  r ;  hence  the  proposition  is  proved. 

Cor.  1.  If f(a)  be  negative  andf(b)  be  positive,  or  vice  versa,  then 
f(x)  has  at  least  one  root,  and,  if  more  than  one,  an  odd  number  of 
roots,  between  x  =  a  and  x  =  b,  provided  f{x)  be  continuous  from  x  =  a 
to  x-b. 

This  is  merely  a  particular  case  of  the  main  proposition,  for 
0  is  intermediate  to  any  two  values,  one  of  which  is  positive  and 
the  other  negative.  Hence  as  x  passes  from  a  to  bf(.r)  must  pass 
at  least  once,  and,  if  more  than  once,  an  odd  number  of  times 

through  the  value  0. 

In  fact,  in  this  case, 

the  axis  of  x  plays  the 

/    \       part  of  the  parallel  UV. 

Observe,  however,  in 

regard  to  the  converse  of 


12 


Fig.  8. 


Fio.  9. 


this  proposition,  that  a 
function  may  pass  through  the  value  0  without  changing  its  sign. 
For  the  graph  may  just  graze  the  re-axis  as  in  Figs.  8  and  9. 


XV  VALUES  FOR  WHICH  A  FUNCTION  CHANGES  SIGN  327 

Cor.  2.  Iff((i)  and  f(b)  have  like  signs,  then,  if  there  be  any  real 
roots  of  f(x)  between  x  =  a  and  x  —  b,  there  must  be  an  even  number, 
provided  f(x)  be  continuous  between  x  =  a  and  x  =  b. 

Since  an  integral  function  is  always  finite  and  continuous  for 
a  finite  value  of  its  variable,  the  restriction  in  Cor.  1  is  always 
satisfied,  and  we  see  that 

Cor.  3.  An  integral  function  can  change  sign  only  by  passing 
through  the  value  0. 

Cor.  4.  If  P  and  Q  be  integral  functions  of  x  algebraically  prime 
to  each  other,  P/Q  can  only  change  sign  by  passing  through  the  values 

0  or  oo  . 

"With  the  hint  that  the  theorem  of  remainders  will  enable 
him  to  exclude  the  ambiguous  case  0/0,  we  leave  the  reader  to 
deduce  Cor.  4  from  Cor.  3. 

Example  1. 

When  sb=0,   l-a?=+l;  and  when  x= +2,  l-ar=  -3.      Hence,  since 

1  -a;2  is  continuous,  for  some  value  of  x  lying  between  0  and  +2  1  —  a?  must 
become  0;  for  0  is  between  +1  and  -  3.  In  point  of  fact,  it  becomes  0  once 
between  the  limits  in  question. 

Example  2. 

y=a?-fa?+llx-6. 

Whenai=0,  y  —  -6;  and  when  x=  +  4,  y=  +6.  Hence,  between  x  =  0  and 
x=  +4  there  must  lie  an  odd  number  of  roots  of  the  equation 

a-3-6a;2+lla;-6  =  0. 
It  is  easy  to  verify  in  the  present  case  that  this  is  really  so;  for  x3-6xi 
+  llx  -  6  =  (x  -  1)  (x  -  2)  (x  -  3) ;  so  that  the  roots  in  question  are  x  —  1,  x  —  2, 
se=3. 

The  general  form  of  the  graph  in  the  present  case  is  as  follows  : — 


Fig.  io. 

Example  3. 

When  x  =  0,  l/(l-a;)=+l;  and  when  x=  +2,  l/(l-a:)=-]  :  but  since 
1/(1  —  x)  becomes  infinite  and  discontinuous  between  x  =  0 and  x=  +2,  namely, 
when  X=l,  we  cannot  infer  that,  for  some  value  of  x  between   0   and  +2, 


328  SIGN  OF  /(0)  AND  /(  ±  oo  )  chap. 

1/(1  -x)  will  become  0,  although  0  is  intermediate  to  + 1  and  -1.      In  fact, 
1/(1  —  x)  does  not  pass  through  the  value  0  between  x=0  and  x=  +2. 

§  10.]  It  will  be  convenient  to  give  here  the  following  pro- 
position, which  is  often  useful  in  connection  with  the  methods 
Ave  are  now  explaining. 

If  fix)  be  an  integral  function  of  x,  then  by  making  x  small 
enough  we  can  always  cause  f(x)  to  have  the  same  sign  as  its  lowest 
term,  and  by  making  x  large  enough  we  can  always  cause  f(x)  to  have 
the  same  sign  as  its  highest  term. 

Let  us  take,  for  simplicity,  a  function  of  the  3rd  degree,  say 
y  =  px3  +  qx2  +  rx  +  s. 
If  we  suppose  s  4=  0,  then  it  is  clear,  since  by  making  x  small 
enough  we  can  (see  §  7,  II.)  make  px3  +  qx2  +  rx  as  small  as  we 
please,  that  we  can,  by  making  x  small  enough,  cause  y  to  have 
the  same  sign  as  s. 

If  s  =  0, 

then  we  have  y  =px*  +  qx2  +  rx, 

=  (px2  +  qx  +  r)x. 
Here  by  making  x  small  enough  we  can  cause  px2  +  qx  +  r  to  have 
the  same  sign  as  r,  and  hence  y  to  have  the  same  sign  as  rx, 
which  is  the  lowest  existing  term  in  y. 

Again,  we  may  write 


ir- 

Here  by  making  x  large  enough  we  may  make  q/x  +  rjx2  +  s/x3  as 
small  as  we  please  (see  §  6,  IV.,  and  §  7,  II.),  that  is  to  say, 
cause  p  +  q/x  +  rjx2  +  s/x3  to  have  the  same  sign  as  p.  Hence  by 
making  x  large  enough  we  can  cause  y  to  have  the  same  sign 


as  px3 


If  we  observe  that,  by  chap,  xiv.,  §  9,  we  can  reduce  every 
integral  equation  to  the  equivalent  form 

f{x)  =  xn  +  pn _ ,  x"- *  +  .   .   .+^0  =  0, 
and  further  notice  that,  in  this  case,  if  n  be  odd, 

/(  +  oo  )  =  +  oo  ,     /(  -  oo  )  =  -  oo  , 
ami,  if  n  be  even, 

/(  +  oo  )  =  +  oo  ,     /(  -  oo  )  =  +  oo , 
we  have  the  following  important  conclusions. 


XV 


MINIMUM  NUMBER  OF  REAL  ROOTS 


329 


Cor.  1.  Every  integral  equation  of  odd  degree  with  real  co- 
efficients has  at  least  one  real  root,  and  if  it  has  more  than  one  it 
has  an  odd  number. 

Cor.  2.  If  an  integral  equation  of  even  degree  with  real  coefficients 
has  any  real  roots  at  all,  it  lias  an  even  number  of  such. 

Cor.  3.  Every  integral  equation  with  real  coefficients,  if  it  has  any 
complex  roots,  has  an  even  number  of  such. 

The  student  should  see  that  he  recognises  what  are  the  cor- 
responding peculiarities  in  the  graphs  of  integral  functions  of 
odd  or  of  even  degree. 

Example. 
„      Show  that  the  equation 

xi-6,3  +  llx--r-l  =  () 
has  at  least  two  real  roots. 
Let  y  =  xi-6x'i  +  llx--x-4. 

We  have  the  following  scheme  of  corresponding  values  : — 


X 

—  OO 

0 

+  oo 

V 

+  oo 
-  4 

+  oo 

Hence  one  root  at  least  lies  between  -  oo  and  0,  and  one  at  least  between 
0  and  +  oo .  In  other  words,  there  are  at  least  two  real  roots,  one  negative 
the  other  positive. 

We  can  also  infer  that,  if  the  remaining  two  of  the  possible  four  be  also 
real,  then  they  must  be  either  both  positive  or  both  negative. 

When  the  real  roots  of  an  integral  equation  are  not  very 
close  together  the  propositions  we  have  just  established  enable 
us  very  readily  to  assign  upper  and  lower  limits  for  each  of 
them ;  and  in  fact  to  calculate  them  by  successive  approxima- 
tion. The  reader  will  thus  see  that  the  numerical  solution  of 
integral  equations  rests  merely  on  considerations  regarding  con- 
tinuity, and  may  be  considered  quite  apart  from  the  question 
of  their  formal  solution  by  means  of  algebraical  functions  or 
otherwise.  The  application  of  this  idea  to  the  approximate 
determination  of  the  real  roots  of  an  integral  equation  will  be 
found  at  the  end  of  the  present  chapter. 


330 


MAXIMA  AND  MINIMA  ALTERNATE 


CHAP. 


GENERAL    PROPOSITIONS    REGARDING   MAXIMA   AND    MINIMA 
VALUES    OF   FUNCTIONS    OF   ONE    VARIABLE. 

§11.]  When  fix)  in  passing  through  any  value,  f(a)  say,  ceases  to 
increase  and  begins  to  decrease,  f(a)  is  called  a  maximum  value  of  f{x). 

When  fix)  in  passing  through  the  value  f (a)  ceases  to  decrease  and 
begins  to  increase,  f(a)  is  called  a  minimum  value  of  fix). 

The  points  corresponding  to  maxima  and  minima  values  of 
the  function  are  obviously  superior  and  inferior  culminating 
points  on  its  graph,  such  as  P2  and  P9  in  Fig.  1.  They  are 
also  points  where,  in  general,  the  tangent  to  the  graph  is  parallel 
to  the  axis  of  x.  It  should  be  noticed,  however,  that  points 
such  as  P  and  Q  in  Fig.  1 1  are  maxima  and  minima  points, 
according  to  our  present  definition,  although  it  is  not  true  in 
any  proper  sense  that  at  them  the  tangent  is  parallel  to  OX.     It 


Fig.  11. 


Fio.  12. 


should  also  be  observed  that  the  tangent  may  be  parallel  to  OX 
and  yet  the  point  may  not  be  a  true  maximum  or  minimum 
point.     Witness  Fig.  12. 

We  shall  include  both  maximum  and  minimum  values  as  at 
present  defined  under  the  obviously  appropriate  name  of  turning 
values. 

§  12.]  By  considering  an  unbroken  curve  having  maxima 
and  minima  points  (see  Fig.  1)  the  reader  will  convince  himself 
graphically  of  the  truth  of  the  following  propositions : — 

I.  So  long  as  f(x)  remains  continuous  its  maxima  and  minima 
values  succeed  each  other  alternately. 

II.  If  x  =  a,  x  =  b  be  two  roots  of  f(x)  (a  alg.<b),  then,  if  f(x)  be 
not  constant,  but  vary  continuously  between  x-a  and  x  =  b,  there  must 


XV 


CRITERION  FOR  TURNING  VALUES  331 


be  either  at  least  one  maximum  or  at  least  one  minimum  value  of  f(x) 
between  x  -  a  and  x  =  b. 

In  particular,  if  f(x)  become  positive  immediately  after  x 
passes  through  the  value  a,  then  there  must  he  at  least  one 
maximum  before  x  reaches  the  value  b ;  and,  in  like  manner,  if 
f(x)  become  negative,  at  least  one  minimum. 

§  1 3.]  It  is  obvious,  from  the  definition  of  a  turning  value, 
and  also  from  the  nature  of  the  graph  in  the  neighbourhood  of 
a  culminating  point,  that  we  can  always  find  two  values  of  the  func- 
tion, on  opposite  sides  of  a  turning  value,  which  shall  be  as  nearly 
equal  as  we  please.  These  two  values  will  be  each  less  or  each  greater 
than  the  turning  value  according  as  the  turning  value  is  a  maximum 
or  minimum. 

Hence,  if  p  be  infinitely  near  a  turning  value  of  fix)  (less  in 
the  case  of  a  maximum,  greater  in  the  case  of  a  minimum),  then 
two  roots  oi  fix)  -p  will  be  infinitely  nearly  equal  to  one  another. 
It  follows,  therefore,  that,  if  p  be  actually  equal  to  a  turning  value 
of  f(x),  the  function  f(x)  -p  will  have  two  of  its  roots  equal.  This 
criterion  may  be  used  for  finding  turning  values,  as  will  be  seen 
in  a  later  chapter. 

CONTINUITY    AND    GRAPHICAL    REPRESENTATION    OF   A 
FUNCTION    OF   TWO    INDEPENDENT   VARIABLES. 

§  14.]  Let  the  function  be  denoted  by  f(x,  y),  and  let  us 
denote  the  dependent  variable  b}r  z ;  so  that 

*=/(«,  y)- 

We  confine  ourselves  entirely  to  the  case  where  fix,  y)  is  an  integral 
function,  and  we  suppose  all  the  constants  to  be  real,  and  consider  mily 
real  values  of  x  and  y.     The  value  of  z  will  therefore  be  always  real. 

Since  there  are  now  two  independent  variables,  x  and  //, 
there  are  two  independent  increments,  say  h  and  k,  to  consider. 
Hence  the  increment  of  z,  that  is,  f(x  +  h,  y  +  k)  -f(x,  y),  now 
depends  on  four  quantities,  x,  y,  h,  k.  Since,  however,  f(x,  y) 
consists  of  a  sum  of  terms  such  as  Axmfn,  it  can  easily  be  shown 
by  reasoning,  like  that  used  in  the  case  oif(x),  that  the  increment 
of  z  always  becomes  infinitely  small  when  h  and  k  are  made  infinitely 


332 


GRAPHIC  SURFACE  FOR  Z  =/(»,  y) 


CHAP. 


small.  Hence,  as  x  and  y  pass  continuously  from  one  given  pair  of 
values,  say  (a,  b),  to  another  given  pair,  say  (a',  b'),  z  passes  continu- 
ously from  one  value,  say  c,  to  another,  say  c'. 

§  15.]  There  is,  however  a  distinct  peculiarity  in  the  case 
now  in  hand,  inasmuch  as  there  are  an  infinity  of  different  ways 
in  which  (x,  y)  may  pass  from  (a,  b)  to  (a',  b').  In  fact  we  re- 
quire now  a  two-dimensional  diagram  to  represent  the  variations  of 
the  independent  variables.     Let  X'OX,  Y'OY  be   two   lines   in  a 


Fio.  13. 

horizontal  plane  drawn  from  west  to  east  and  from  south  to 
north  respectively.  Consider  any  point  P  in  that  plane,  whose 
abscissa  and  ordinate,  with  the  usual  understanding  as  to  sign, 
are  x  and  y.  Then  P,  which  we  may  call  the  variable  point,  gives 
us  a  graphic  representation  of  the  variables  (x,  y). 

Let  us  suppose  that  for  P  x  =  a,  y  =  b,  and  that  for  another 
point  P'  x  =  a',  y  =  b'.  Then  it  is  obvious  that,  if  Ave  pass 
along  any  continuous  curve  whatever  from  P  to  P',  x  will  vary 
continuously  from  a  to  a',  and  y  will  vary  continuously  from 
b  to  1/  ;  and,  conversely,  that  any  imaginable  combination  of  a 
continuous  variation  of  x  from  a  to  a'  with  a  continuous  varia- 
tion of  y  from  b  to  V  will  correspond  to  the  passage  of  a  point 
from  P  to  P'  along  some  continuous  curve. 

It    is   obvious,   therefore,    that    the   continuous   variation   of 


XV  CONTOUR  LINES  333 

(x,  y)  from  (a,  h)  to  (a\  b')  may  be  accomplished  in  an  infinity 
of  ways.  We  may  call  the  path  in  which  the  point  which  repre- 
sents the  variables  travels  the  graph  of  the  variables. 

To  represent  the  value  of  the  function  z  =  f(x,  y)  we  draw 
through  P,  the  variable  point  representing  (x,  y),  a  vertical  line 
PQ,  containing  .:  units  of  any  fixed  scale  of  length  that  may  be 
convenient,  upwards  if  z  be  positive,  downwards  if  z  be  negative. 
Q  is  then  the  graphic  point  which  represents  the  value  of  the 
function  z  =/(•'",  y). 

To  every  variable  point  in  the  plane  XOY  there  corresponds 
a  graphic  point,  such  as  Q  ;  and  the  assemblage  of  graphic  points 
constitutes  a  surface  which  we  call  the  graphic  surface  of  the 
function  f{x,  y) 

When  the  variable  point  travels  along  any  particular  curve  S 
in  the  plane  XOY,  the  graphic  point  of  the  function  travels  along 
a  particular  curve  2  on  the  graphic  surface ;  and  it  is  obvious 
that  S  is  the  orthogonal  projection  of  2  on  the  plane  XOY. 

§  1 6.]  If  we  seek  for  values  of  the  variables  which  correspond 
to  a  given  value  c  of  the  function,  we  have  to  draw  a  horizontal 
plane  U,  c  units  above  or  below  XOY  according  as  c  is  positive 
or  negative  ;  and  find  the  curve  2  where  this  plane  U  meets  the 
graphic  surface.  This  line  2  is  what  is  usually  called  a  contour 
line  of  the  graphic  surface.  In  this  case  the  orthogonal  projection 
S  of  2  upon  XOY  will  be  simply  2  itself  transferred  to  XOY, 
and  may  be  called  the  contour  line  of  the  function  for  the  value  c. 
All  the  variable  points  upon  8  correspond  to  pairs  of  values  of 
(x,  y),  for  which  f(x,  y)  has  the  given  value  c. 

If  we  take  a  number  of  different  values,  c„  c2,  c3,  .  .  .,  c,„  we 
get  a  system  of  as  many  contour  lines.  Suppose,  for  example, 
that  the  graph  of  the  function  were  a  rounded  conical  peak,  then 
the  system  of  contour  lines  would  be  like  Fig.  14,  where  the 
successive  curves  narrow  in  towards  a  point  which  corresponds 
to  a  maximum  value  of  the  function. 

Any  reader  who  possesses  a  one -inch  contoured  Ordnance 
Survey  map  has  to  hand  an  excellent  example  of  the  graphic 
representation  of  a  function.     In  this  case  x  and  y  are  the  dis- 


334 


f(x,  y)=0  REPRESENTS  A  PLANE  CURVE 


CHAP. 


tances  east  from  the  left-hand  side  of  the  map,  and  north  from 
the  lower  side ;  and  the  function  z  is  the  elevation  of  the  land 


Fig.  14. 


at  any  point  above  the  sea  level.  The  study  of  such  a  map  from 
the  present  point  of  view  will  be  an  excellent  exercise  both  in 
geometry  and  in  analysis. 

An  important  particular  case  is  that  where  we  seek  the 
values  of  x  and  y  which  make  f(x,  y)  =  0.  In  this  case  the  plane 
U  is  the  plane  XOY.  This  plane  cuts  the  graphic  surface  in  a 
continuous  curve  S  {zero  contour  line),  every  point  on  which 
has  for  its  abscissa  and  ordinate  a  pair  of  values  that  satisfy 
f{x,  y)  =  0. 

The  curve  S  in  this  case  divides  the  plane  into  regions,  such  that 
in  any  region  f(x,  y)  has  always  either  the  sign  +  or  the  sign  — , 
and  S  always  forms  the  boundary  between  two  regions  in  which  f(x,  y) 
has  opposite  signs. 

If  we  draw  a  continuous  curve  from  a  point  in  a  +  region 
to  a  point  in  a  -  region,  it  must  cross  the  boundary  S  an  odd 
number  of  times.  This  corresponds  to  the  analytical  statement 
that  iff(a,  b)  be  positive  and  f(a,  b')  be  negative,  then,  if  (x,  y)  vary 
continuously  from  {a,  b)  to  (a',  b'),  f(x,  y)  will  pass  through  the  value 
0  an  odd  number  of  times. 

The  fact  just  established,  that  all  the  "  variable  points  "  for 
which  f(x,  y)  —  0  lie  on  a  continuous  curve,  gives  us  a  beautiful 
geometrical  illustration  of  the  fact  established  in  last  chapter,  that 
the  equation  f(x,  y)  =  0  has  an  infinite  number  of  solutions,  and 
gives  us  the  fundamental  idea  of  co-ordinate  geometry, namely,  that 


XV 


EXAMFLE 


335 


a  plane  curve  can  be  analytically  represented  by  means  of  a  single 
equation  connecting  two  variables. 

Example. 

Consider  the  function  z  =  x2  +  y2-  1.  If  we  describe,  with  0  as  centre,  a 
circle  whose  radius  is  unity,  it  will  be  seen  that  for  all  points  inside  this  circle 
z  is  negative,  and  for  all  points  outside  z  is  positive.  Hence  this  circle  is  the 
zero  contour  line,  and  for  all  points  on  it  we  have 

x2  +  if--l=0. 
Y 


Fig.  15. 


INTEGRAL   FUNCTIONS    OF   A    SINGLE    COMPLEX    VARIABLE. 

§  17.]  Here  we  confine  ourselves  to  integral  functions,  but  no  longer 
restrict  either  the  constants  of  the  function  or  its  independent  variable 
x  to  be  real. 

Let  us  suppose  that  x  =  £  +  ?ii,  and  let  us  adopt  Argand's 
method    of    representing    £  +  yi  H 

graphically,  so  that,  if  12 M  =  £, 
MP  =  ij,  in  the  diagram  of  Fig. 
1 6,  then  P  represents  £  +  tji. 

If  P  move   continuously  from 

any  position  P  to  another  P',  the  

complex  variable   is  said  to  vary 

continuously.      If    the   values    of 

(£,  rj)  at  P  and  P'  be  (a,  ft)  and 

(a',  ft')  respectively,  this  is  the  Fro.  16. 

same  as  saying  that  £  +  iji  is  said  to  vary  continuously  from  the 

value  a  +  fti  to  the  value  a  +  /3'i,  when  £  varies  continuously  from  a 

to  a,  and  tj  varies  continuously  from  ft  to  ft'.     There  are  of  course 


P 


Q 


M 


M'      2 


336 


CONTINUITY  OF  COMPLEX  FUNCTION 


CHAP. 


an  infinite  number  of  ways  in  which  this  variation  may  be 
accomplished. 

§  1 8.]  Suppose  now  we  have  any  integral  function  of  x  whose 
constants  may  or  may  not  be  real.  Then  we  have  f(x)  =f($  +  rji) ; 
but  this  last  can,  by  the  rules  of  chap,  xii.,  always  be  reduced 
to  the  form  £'  +  rji,  Avhere  £'  and  rj  are  integral  functions  of  £ 
and  ?;  whose  constants  are  real  (say  real  integral  functions  of 
(£,  rj)  ).  Now,  by  §  14,  £'  and  rj  are  finite  and  continuous  so 
long  as  (£,  ?/)  are  finite.  Hence  /(£  +  rfi)  varies  continuously  when 
£  +  r/i  varies  continuously. 

A  graphic  representation  of  the  function  /(£  +  rji)  can  be 
obtained  by  constructing  another  diagram  for  the  complex 
number  £'  +  iji.  Then  the  continuity  of  /(£  +  rji)  is  ex- 
pressed by  saying  that,  when  the  graph  of  the  independent  vari- 
able is  a  continuous  curve  S,  the  graph  of  the  dependent  variable  is 
another  continuous  curve  S'. 


Example. 
Let 


2/=+V(l-^). 


H 


12 


H 

$ 

1 

J 

B' 

C, 

0' 

A' 

c 

»— * 

Fig.  17. 


Fig.  18. 


For  simplicity,  we  shall  confine  ourselves  to  a  variation  of  x  which  admits 
only  real  values  ;  in  other  words,  we  suppose  r\  always  =0. 

The  path  of  the  independent  variable  is  then  IACBJ,  the  whole  extent 
of  the  £-axis.  In  the  diagram  we  have  taken  CA  =  CB  =  1  ;  so  that  A  and 
B  mark  the  points  in  the  path  for  which  the  function  begins  to  have,  and 
ceases  to  have,  a  real  value. 

Let  Fig.  18  be  the  diagram  of  the  dependent  variable,  ;/  =  £'  + t?7-  If 
A'C'-l  (A',  B',  and  W  are  all  coincident),  then  the  path  of  the  dependent 


XV 


COMTLEX  ROOTS  DETERMINED  GRAPHICALLY 


337 


variable   is  the  whole  of   the    77' -axis  above  fi,   together   with   A'C,   each 
reckoned  twice  over.     The  pieces  of  the  two  paths  correspond  as  follows  : — 


Independent 
Variable. 

Dependent  Variable. 

IA 

AC 
CB 
BJ 

FA' 
A'C 
CB' 
B'J' 

§  19.]  £'  and  rj  being  functions  of  £  and  >;,  we  may  represent 
this  fact  to  the  eye  by  writing 

r  =  </>(£  v),    v'  =  M  v)- 

If  we  seek  for  values  of  (£,  rj)  that  make  £'  =  0,  that  is  the  same 
as  seeking  for  values  of  (£,  rj)  that  make  <£(£,  rj)  =  0.  All  the 
points  in  the  diagram  of  the  independent  variable  corresponding 
to  these  will  lie  (by  §  16)  on  a  curve  S. 

Similarly  all  the  points  that  correspond  to  rj  =  0,  that  is,  to 
^(£,  rj)  =  0,  lie  on  another  curve  T. 

The  points  for  which  both  £'  =  0  and  ?/  =  0, — in  other  words, 
the  points  corresponding  to  roots  of  /(£  +  ?;?), — must  therefore  be 
the  intersections  of  the  two  curves  S  and  T. 


Example. 
If  we  jmtx=a+rri,  and  y=s'  +  7?'i  wu  have 

=m-$v)  +  (e-v-)i. 

Hence  £'=2(4  -£»;),  v'  =  ^-v". 

Hence  the  S  and  T  curves,  above  spoken  of,  are  given  by  the  equations 

2(4  -fr)  =  0  (S), 

?-v-=Q  (T). 


These  are  equivalent  to 


VOL.  I 


4 


(S), 

(T). 


338 


HORNER  S  METHOD 


CHAP. 


The  student  should  have  no  difficulty  in  constructing  these.    The  diagram 
that  results  is 

H 


\ 


N 


M 


Fir,.  19. 


The  S  curve  (a  rectangular  hyperbola  as  it  happens)  is  drawn  thick.  The 
T  curve  (two  straight  lines  bisecting  the  angles  between  the  axes)  is  dotted. 
The  intersections  are  P  and  Q. 

Corresponding  to  P  we  have  if  =  2,    ??  =  2;    corresponding  to  Q,  £=  -2, 


V- 


_  o 


It  appears  therefore  that  the  roots  of  the  function  are  +  2  +  2i  and  -  2  -  2i. 
The  student  may  verify  that  these  values  do  in  fact  satisfy  the  equation 

ix2  +  8  =  0. 


HORNER'S  METHOD  FOR  APPROXIMATING  TO  THE  VALUES  OF  THE 
REAL  ROOTS  OF  AN  INTEGRAL  EQUATION. 

§  20.]  In  the  following  paragraphs  we  shall  show  how  the 
ideas  of  §§  8-10  lead  to  a  method  for  calculating  digit  by  digit 
the  numerical  value  of  any  real  root  of  an  integral  equation.  It 
will  be  convenient  in  the  first  place  to  clear  the  way  by  estab- 
lishing a  few  preliminary  results  upon  which  the  method  more 
immediately  depends. 

§  21.]  To  deduce  from  the  equation 

p^n  +  pxXn  ~ l  +  .    .    .  +  pn  _  iX  +  pn  =0  (1 ) 

another  equation  each  of  wlwse  roots  is  m  times  a  corresponding  root 


xv  DIMINUTION  OF  ROOTS  339 

of  (1).    Let  x  be  any  root  of  (1) ;  and  let  £  =  mz.    Then  x  =  gjm. 
Hence,  from  (1),  we  have 

Pod  m)n  +p1(g/m)n-1  +  .  .  .  +pn-l($/m)  +pn  =  0. 

If  we  multiply  by  the  constant  in'1,  we  deduce  the  equivalent 
equation 

pg1  +  pMn  - 1  +  ■  ■  ■+  Pn  - .»"  "  *£  +JW»"  =  0       (2), 
which  is  the  equation  required. 

Cor.  The  equation  whose  roots  are  those  of  (1)  with  the  signs 
changed  is 

Po$"  -Pi?-1  +  •    •    ■  +  (-  r^Pn-^  +  (  -  )"Pn  =  0       (3). 

This  follows  at  once  by  putting  m  =  -  1  in  (2).  We  thus 
see  that  the  calculation  of  a  negative  real  root  of  any  equation 
can  always  be  reduced  to  the  calculation  of  a  positive  real  root 
of  a  slightly  different  equation. 

Example.  The  equation  whose  roots  are  10  times  the  respective  roots  of 

Sa?-15xi+5x  +  6  =  0 

is  3^ -150x2  +  500.c+ 6000  =  0. 

§  22.]  To  deduce  from  the  equation  (1)  of  §  21  another,  each  of 
xohose  roots  is  less  by  a  than  a  corresponding  root  of  (I). 

Let  x  denote  any  root  of  (1);  £  the  corresponding  root  of 
the  required  equation  ;  so  that  g  =  x  —  a,  and  x  =  £  +  a.  Then 
we  deduce  at  once  from  (1) 

P&  +  a)n  +;>,(£  +  a)""1  +  .  .  .  +pn-i($  +  «)  +Pn  =  0     (4). 
If  we  arrange  (4)  according  to  powers  of  £,  we  get 

ft£* +  $£*"*  + :  •  -  +  qn-i€  +  qn  =  o  (5), 

which  is  the  equation  required. 

It  is  important  to  have  a  simple  systematic  process  for 
calculating  the  coefficients  of  (5).  This  may  be  obtained  as 
follows. 

Since  £  =  x  -  a,  we  have,  by  comparing  the  left-hand  sides  of 
(1)  and  (5), 

p0xn  +plxn~1  +  .  .   .  +pn_lx  +pn 

=pQ(x-a)n  +  ql(z-a)n-1  +  .  .  .  +  ?»-i(a:-a)  +  ?»• 


340  APPROXIMATION  TO  ROOT  chap. 

The  problem  before  us  is,  therefore,  simply  to  expand  the 
function/(.T)  =p0xn  +p1xn~'1  +  .  .  .  +pn-iX  +pnm  powers  of  (x  -  a). 
Hence,  as  we  have  already  seen  in  chap,  v.,  §  21,  qn  is  the 
remainder  when  f{x)  is  divided  by  x  -  a ;  qn_^  the  remainder 
when  the  integral  quotient  of  the  last  division  is  divided  by 
x-  a ;  and  so  on.  The  calculation  of  the  remainder  in  any 
particular  case  is  always  carried  out  by  means  of  the  synthetic 
process  of  chap,  v.,  §  13. 

It  should  be  observed  that  the  last  coefficient,  qn,  is  the  value 
of  f(a). 

Example.  To  diminish  the  roots  of 

by  1. 

AVc  simply  reproduce  the  calculation  of  §  21,  Example  1,  in  a  slightly 

modified  form  ;  thus — 


5                 -11 

+  10 

-2  (1 

5 

-6 

4 

-6 

4 

1    2 

5 

-1 

-1 

1     3 

5 

1     4 

Hence  the  rerpiired  equation  is 

5f  +  4£2+3£  +  2  =  0. 

§  23.]  If  one  of  the  roots  of  the  equation  (1)  of  §  21  be  small, 

say  between  0  and  +  1,   then  an  approximate  value  of  that  root  is 

-Pn/Pn-v     For,    if  x  denote   the   root  in   question,   we  have, 

by  (i), 


x  =  - 


Pn 


(Pn-2+Pn-3V  +  -    ■    .+iV'""2)        (6). 


Pa- i       Pn-i 

Hence,  if  x  be  small,  we  have  approximately  z  =  -  pn;Pn-\- 

It  is  easy  to  assign  an  upper  limit  to  the  error.      We  have, 
in  fact, 

x=    -PnfPn-i  -5 

■II  _/• 

where  mode<^—  (1  +  x  +  .  .  .  +o:n~"), 

l'll-X 

pr  being  the  numerically  greatest  among  the  coefficients  p0  .   .  ., 
Pn-i,  Pn-2-     Hence,  since  x^>l,  we  have 

mode<(?i-  l)p,/pn-i- 


XV  iiokxek's  PROCESS  341 

It  would  be  easy  to  assign  a  closer  limit  for  the  error  ;  hut 
in  the  applications  which  we  shall  make  of  the  theorem  we  have 
indirect  means  of  estimating  the  sufficiency  of  the  approxima- 
tion ;  all  that  is  really  wanted  for  our  purpose  is  a  suggestion  of 
the  approximation. 

Example.  The  equation 

x"  +  8192ar  +  16036288a;  -  5969856  =  0 
has  a  root  between  0  and  1,  find  a  first  approximation  to  that  root. 
By  the  above  rule,  we  have  for  the  root  in  question 
a:  =  59S9856/160362S8-e 
=  "37227  -  e 
where  e<2  x  8192/16036288 <  -00103. 

Hence  o;=  *372,  with  an  error  of  not  more  than  1  in  the  last  digit. 
In  point  of  fact,  since  x<  '4,  we  have 

e<  |(-4)3  +  8192  x  (-4)2}/16036288, 
< 1311/16036288  < 1600/16000000, 
<-0001  ; 
so  that  the  approximation  is  really  correct  to  the  4th  place  of  decimals. 

§  24.]  Horner  s  Method.  Suppose  that  we  have  an  equation 
/(.'•)  =  0,  having  a  positive  root  235-67  .  .  .  This  root  would  be 
calculated,  according  to  Horner's  method,  as  follows  : — First  we 
determine,  by  examining  the  sign  of  f(x)}  that  /(.<•)  =  0  has  one 
root,  and  only  one,*  lying  between  200  and  300  :  the  first  digit 
is  therefore  2.  Then  we  diminish  the  roots  of f(z)  =  0  by  200, 
and  thus  obtain  the  first  subsidiary  equation,  say /,(.>•)  =  0.  Then 
fi(x)-0  has  a  root  lying  between  0  and  100.  Also  since  the 
absolute  term  of  ft(x)  is  /(200),  and  no  root  of  /(.»)  =  0  lies 
between  0  and  200,  the  absolute  term  of  f(x)  (that  is, /(0))  and 
the  absolute  term  oif^x)  must  have  the  same  sign.  By  examin- 
ing the  sign  of  /,(«)  for  x  =  0,  10,  20,  .  .  .,  90,  we  determine 
that  this  root  lies  between  30  and  40  :  the  next  digit  of  the 
root  of  the  original  equation  is  therefore  3.  The  labour  of  this 
last  process  is,  in  practice,  shortened  by  using  the  rule  of  §  23. 
Let  us  suppose  that  30  is  thus  suggested ;  to  test  whether  this 

*  For  a  discussion  of  the  precautions  necessary  when  an  equation  has  two 
roots  which  commence  with  one  or  more  like  digits,  see  Burnside  and  Pcmton's 
Theory  of  Equations,  §  104. 


3-42  HORNER'S  PROCESS  chap. 

is  correct  we  proceed  to  diminish  the  roots  of  /,(•>')  =  0  by  30, — 
to  deduce,  in  fact,  the  second  subsidiary  equation  fs(x)  =  0.  Since 
the  roots  of  /(.?:)  have  now  been  diminished  by  230,  the  absolute 
term  offa(x)  is/(230).  Hence  the  absolute  term  of  f,(.r)  must 
have  the  same  sign  as  the  absolute  term  of  /,(#),  unless  the  digit 
3  is  too  large.  In  other  words,  if  the  digit  3  is  too  large,  we 
shall  be  made  aware  of  the  fact  by  a  change  of  sign  in  the 
absolute  term.  In  practice,  it  does  not  usually  occur  (at  all 
events  in  the  later  stages  of  the  calculation)  that  the  digit 
suggested  by  the  rule  of  §  23  is  too  small ;  but,  if  that  were  so, 
we  should  become  aware  of  the  error  on  proceeding  to  calculate 
the  next  digit  which  would  exceed  9. 

The  second  subsidiary  equation  is  now  used  as  before  to 
find  the  third  digit  5. 

The  third  subsidiary  equation  would  give  "6.  To  avoid  the 
trouble  and  possible  confusion  arising  from  decimal  points,  we 
multiply  the  roots  of  the  third  (and  of  every  following)  subsidiary 
equation  by  10;  or,  what  is  equivalent,  we  multiply  the  second 
coefficient  of  the  equation  in  question  by  10,  the  third  coefficient 
by  100,  and  so  on;  and  then  proceed  as  before,  observing,  how- 
ever, that,  if  the  trial  division  for  the  next  digit  be  made  after 
this  modification  of  the  subsidiary  equation,  that  digit  will 
appear  as  6,  and  not  as  "6,  because  the  last  coefficient  has  been 
multiplied  by  10n  and  the  second  last  by  10B-1. 

The  fundamental  idea  of  Horner's  method  is  therefore  simply 
to  deduce  a  series  of  subsidiary  equations,  each  of  which  is  used 
to  determine  one  digit  of  the  root.  The  calculation  of  the 
coefficients  of  each  of  these  subsidiary  equations  is  accomplished 
by  the  method  of  §  22.  After  a  certain  number  of  the  digits  of 
the  root  have  been  found,  a  number  more  may  be  obtained  by  a 
contraction  of  the  process  above  described,  the  nature  of  which 
will  be  easily  understood  from  the  following  particular  case. 

Example.   Find  an  approximation  to  the  least  positive  root  of 

/(.-•)  =  .,"  +  2.v2-  5z-7  =  0  (1). 

Since  /(0)=-7,    /(l)=-9,    /(2)=-l,    /(3)=+23, 

the  root  in  cjuestion  lies  between  2  and  3.     The  first  digit  is  therefore  2. 


XV  EXAMPLE                                                 34.°, 

We  now  diminish  the  roots  of  (1)  by  2.     The  calculation  of  the  coefficients 
runs  thus : — 

1                 +  2  -5                 -7  (2 

_2  _8                 _6 

4  3               "\  - 1 

2  12 

~6  Tu 
2 


where  the  prefix  -|  is  used  to  mark  coefficients  of  the  first  subsidiary  equation. 
The  first  subsidiary  equation  is  therefore 

a?  +  8x*  +  l5x-l  =  0. 

Since  the  next  digit  follows  the  decimal  point,  we  multiply  the  roots  of 
this  equation  by  10.     The  resuming  equation  is  then 

a?  +  8(k-2  +  1500.*!  -1000  =  0  (2). 

Since  1000/1500  <1,  it  is  suggested  that  the  next  digit  is  0.     "We  there- 
fore multiply  the  roots  of  (2)  by  10,  and  deduce 

ar?  +  800x-2  +  150000.>;- 1000000  =  0  (3). 

Since  1000000/150000  =  6-  .  .   .,  the  next  digit  suggested  is  C.     We  now 
diminish  the  roots  of  (3)  by  6. 


+  800 

+  150000 

-1000000  (06 

6 

4836 

929016 

806 

154836 

4I  -70984000 

6 

4872 

812 

4i  15970800 

6 

8180 

The  resulting  subsidiary  equation,  after  the  multiplication  of  its  roots 
by  10,  is 

a?  +  8180a3  +  15970800a  -  70984000  (4). 

Since  70984000/15970800  =  4-  .  .  .,  the  next  digit  suggested  is  4.  The 
reader  should  notice  that,  owing  to  the  continual  multiplication  of  the  roots 
by  10,  the  coefficients  towards  the  right  increase  in  magnitude  much  more 
rapidly  than  those  towards  the  left :  it  is  for  this  reason  that  the  rule  of  §  23 
becomes  more  and  more  accurate  as  the  operation  goes  on.  Thus,  even  at  the 
present  stage,  the  quotient  70984000/15970800  would  give  correctly  more  than 
one  of  the  following  digits,  as  may  be  readily  verified. 

We  now  diminish  the  roots  of  (4)  by  4  ;  and  add  the  zeros  to  the  coefficients 
as  before. 


344  EXAMPLE  chap 


EXAMPLE 

+  8180 
4 

+  15970800 
32736 

-70984000  (4 
64014144 

8184 
4 

8188 
4 

81920 

16003536 
32752 
sl    1603628800 

b|- 6969856000 

Then  we  have  the  subsidiary  equation 

a;3  +  81920a-2  +  1603628800a  -  6969856000  (5). 

It  will  be  observed  that  throughout  the  operation,  so  far  as  it  has  gone, 
the  two  essential  conditions  for  its  accuracy  have  been  fulfilled,  namely,  that 
the  last  coefficient  shall  retain  the  same  sign,  and  that  each  digit  shall  come 
out  not  greater  than  9.  It  will  also  be  observed  that  the  number  of  the 
figures  in  the  working  columns  increases  much  more  rapidly  than  their  utility 
in  determining  the  digits  of  the  root.  All  that  is  actually  necessary  for  the 
suggestion  of  the  next  digit  at  any  step,  and  to  make  sure  of  the  accuracy  of 
the  suggestion,  is  to  know  the  first  two  or  three  figures  of  the  last  two 
coefficients. 

Unless,  therefore,  a  very  large  number  of  additional  digits  of  the  root  is 
required,  we  may  shorten  the  operation  by  neglecting  some  of  the  figures  in 
(5).  If,  for  example,  we  divide  all  the  coefficients  of  (5)  by  1000,  we  get  the 
equivalent  equation  * 

•001a3  +  81  -92a2  + 1603628  "8a  -  6969S56  =  0  (5'). 

Hence,  retaining  only  the  integral  parts  of  the  coefficients,  we  have 

0a-3  +  81a2  +  1603628a  -  6969856  =  0  (5"). 

It  will  be  noticed  that  the  result  is  the  same  as  if,  instead  of  adding  zeros, 
as  heretofore,  we  had  cut  off  one  figure  from  the  second  last  coefficient,  two 
from  the  third  last,  and  so  on.t 

Since  6969856/1603628  =  4-  .  .  .,  we  have  for  the  next  digit  4.  We  then 
diminish  the  roots  of  (5")  by  4.  In  the  necessary  calculation  the  first  working 
column  now  disappears  owing  to  the  disappearance  of  the  coefficient  of  a3 ;  we 
have  in  its  place  simply  81  standing  unaltered.  It  is  advisable,  however,  in 
multiplying  the  contracted  coefficients  by  4  to  carry  the  nearest  number  of 
tens  from  the  last  figure  cut  off  (just  as  in  ordinary  contracted  multiplication 
and  division  and  for  the  same  reason). 

*  If  the  reader  find  any  difficulty  in  following  the  above  explanation  of 
the  contracted  process,  he  can  satisfy  himself  of  its  validity  by  working  out 
the  above  calculation  to  the  end  in  full  and  then  running  his  pen  through  the 
unnecessary  figures. 

t  In  many  cases  it  may  not  be  advisable  to  carry  the  contraction  so  far  at 
each  step  as  is  here  done.  We  might,  for  instance,  divide  the  coefficients  of 
5  by  100  only.     The  resulting  subsidiary  equation  would  then  be 

Oa3  +  81 9a2  + 1 6036288a  -  09698560, 
with  which  we  should  proceed  as  before. 


XV 


EXAMPLE 


345 


The  next  step,  therefore,  runs  thus  : 

81  +1603628 

328 

1603957 

328 


6969856 

6415828 

-  554028 


(4 


(6); 
(6'). 


"I     1604285 
The  corresponding  subsidiary  equation  is 

81a2  +  16042850a-  -  55402800  =  0 
or,  contracted,  Ox-  + 160428.1-  -  554028  =  0 

The  next  digit  is  3  ;  and,  as  the  coefficient  of  x2,  namely  0-81,  still  has  a 
slight  effect  on  the  second  working  column,  the  calculation  runs  thus:  — 
0  +160428  -554028  (3 

2  481293 

71- 


160431 
2 


-72735 


'I    160433 
The  resulting  subsidiary  equation  after  contraction  is 

16043a; -72735  =  0  (7). 

The  rest  of  the  operation  now  coincides  with  the  ordinary  process  of 
contracted  division  ;  it  represents,  in  fact,  the  solution  of  the  linear  equation 
(7),  that  is  (see  chap,  xvi.,  §  1),  the  division  of  72735  by  16043. 

The  whole  calculation  may  be  arranged  in  practice  as  below.  But  the 
prefixes  2|,  3|,  &c,  which  indicate  the  coefficients  of  the  various  equations, 
may  be  omitted.  Also  the  record  may  be  still  farther  shortened  by  performing 
the  multiplications  and  additions  or  subtractions  mentally,  and  only  recording 
the  figures  immediately  below  the  horizontal  lines  in  the  following  scheme. 
The  advisability  of  this  last  contraction  depends  of  course  on  the  arithmetical 
power  of  the  calculator. 


+  2 

-5 

-7  (2-064434533 

2 

8 

6 

4 

3 

8|  - 1000000 

2 

12 

929016 

6 

"  3|  150000 

4|  -70984000 

2 

4836 

64014144 

3|  800 

154836 

1  -  6969856 

6 

4872 

6415828 

806 

1 15970800 

"1  -  554028 

6 

32736 

481293 

812 

16003536 

'1-72735 

6 

32752 

64173 

4|  8180 

bl  1603628^ 

"1  -  8562 

4 

328 

8022 

8184 

1603957 

9|-5l0 

4 

328 

481 

8188 

"1 160428$ 

10l-59 

4 

2 

48 

'I^N 

160431 
2 

-11 

16fc(^Sf 


346  EXERCISES  XXII 


i'H  U\ 


The  number  of  additional  digits  obtained  by  the  contracted  process  is  less 
by  two  than  the  number  of  digits  in  the  second  last  coefficient  at  the  beginning 
of  the  contraction.  Owing  to  the  uncertainty  of  the  carriages  the  last  digit 
is  uncertain,  but  the  next  last  will  in  such  a  case  as  the  present  be  abso- 
lutely correct.  In  fact,  by  substituting  in  the  original  equation,  it  is  easily 
verified  that  the  root  lies  between  2-064434534  and  2-064434535  ;  so  that  the 
last  digit  given  above  errs  in  defect  by  1  only.  The  number  of  accurate 
figures  obtained  by  the  contracted  process  will  occasionally  be  considerably 
less  than  in  this  example  ;  and  the  calculator  must  be  on  his  guard  against 
error  in  this  respect  (see  Horner's  Memoir,  cited  below). 

§  25.]  Since  the  extraction  of  the  square,  cube,  fourth,  .  .  . 
roots  of  any  number,  say  7,  is  equivalent  to  finding  the  positive 
real  root  of  the  equations,  x2  +  Ox  -  7  =  0,  xa  +  Ox2  +  Ox  -  7  =  0, 
x*  +  Ox3  +  (bf  +  Oo:  -  7  =  0,  .  .  .  respectively,  it  is  obvious  that 
by  Horner's  method  we  can  find  to  any  desired  degree  of 
approximation  the  root  of  any  order  of  any  given  number 
"whatsoever.  In  fact,  the  process,  given  in  chap,  xi.,  §  13,  for 
extracting  the  square  root,  and  the  process,  very  commonly 
given  in  arithmetical  text-books,  for  extracting  the  cube  root  will 
be  found  to  be  contained  in  the  scheme  of  calculation  described 
in  §  24.* 

*  Horner's  method  was  first  published  in  the  Transactions  of  the  Philoso- 
phical Society  of  London  for  1819.  Considering  the  remarkable  elegance, 
generality,  and  simplicity  of  the  method,  it  is  not  a  little  surprising  that  it 
has  not  taken  a  more  prominent  place  in  current  mathematical  text-books. 
Although  it  has  been  well  expounded  by  several  English  writers  (for  example, 
De  Morgan,  Todhunter,  Burnside  and  Panton),  it  has  scarcely  as  yet  found  a 
recognised  place  in  English  curricula.  Out  of  five  standard  Continental  text- 
books where  one  would  have  expected  to  find  it  we  found  it  mentioned  in  only 
one,  and  there  it  was  expounded  in  a  way  that  showed  little  insight  into  its 
true  character.  This  probably  arises  from  the  mistaken  notion  that  there  is 
in  the  method  some  algebraic  profundity.  As  a  matter  of  fact,  its  spirit  is 
purely  arithmetical ;  and  its  beauty,  which  can  only  be  appreciated  after  one 
has  used  it  in  particular  cases,  is  of  that  indescribably  simple  kind  which 
distinguishes  the  use  of  position  in  the  decimal  notation  and  the  arrangement 
of  the  simple  rules  of  arithmetic.  It  is,  in  short,  one  of  those  things  whose 
invention  was  the  creation  of  a  commonplace.  For  interesting  historical 
details  on  this  subject,  see  De  Morgan — Companion  to  British  Almanack,  for 
1839;  Article  "Involution  and  Evolution,"  Penny  Cyclopsedia  ;  and  Budget 
of  Paradoxes,  pp.  292,  374. 


XV 


EXERCISES  XXII  34" 


Exercises  XXII. 


[The  student  should  trace  some  at  least  of  the  curves  required  in  the 
following  graphic  exercises  by  laying  them  down  correctly  to  some  convenient 
scale.  He  will  find  this  process  much  facilitated  by  using  paper  ruled  into 
small  squares,  which  is  sold  under  the  name  of  Plotting  Paper.] 

Discuss  graphically  the  following  functions  : — 

(40  y=rz1Tvi-      (5.)  y=^i-      (6.)  y=-  x 


"(sb-1)3'         v    '  J     se-2  v  "'  *     J'2-9 

(7.)  Construct  to  scale  the  graph  of  y  =  -  x-  +  8x  -  9  ;  and  obtain  graphic- 
ally the  roots  of  the  equation  a-2  -  8a:  +  9  =  0  to  at  least  three  places  of 
decimals. 

(8.)  Solve  graphically  the  equation 

a?  -  16a;2  +  7Lc-  129  =  0. 
(9.)  Discuss  graphically  the  following  question.     Given  that  y  is  a  con- 
tinuous function  of  x,  does  it  follow  that  a;  is  a  continuous  function  of  y  ? 
(10.)  Show  that  when  h,  the  increment  of  x,  is  very  small,  the  increment  of 

p„x"  +pn-ix"-1  + .  .   .  +pxx  +p0 
is  (npnX"-1  +  (n  - 1  )pn-ix"-2  +  .  .  .  + 1  .pi)h. 

(11. )  If  h  be  very  small,  and  x=l,  find  the  increment  of  2a-*3  -  9ar  +  12a1  +  5. 

(12.)  If  an  equation  of  even  degree  have  its  last  term  negative,  it  has  at 
least  two  real  roots  which  are  of  opposite  signs. 

(13.)  Indicate  roughly  the  values  of  the  real  roots  of 

10a.-3-17ar  +  a;  +  3  =  0. 

(14.)  What  can  you  infer  regarding  the  roots  of 

a,-3-5a;  +  8  =  0? 

(15.)  Show  by  considerations  of  continuity  alone  that  a;" -1=0  cannot 
have  more  than  one  real  root,  if  n  be  odd. 

(16.)  If f{x)  be  an  integral  function  of  a;,  and  if/(a)=  -p,f{b)=  +q,  where 
p  and  q  are  both  small,  show  that  x  —  (qa+2^b)/{p  +  q)  is  an  approximation  to 
a  root  of  the  equation /(a:)  =  0. 

Draw  a  series  of  contour  lines  for  the  following  functions,  including  in 
each  case  the  zero  contour  line  :  — 

(17.)  z  =  xy.         (18.)  z  =  ~.  (19.)  z  =  x--f.  (20.)  z  =  ^±£ '. 

y  x 

Is  the  proposition  of  §  16  true  for  the  last  of  these  ? 

Draw  the  Argand  diagram  of  the  dependent  variable  in  the  following 
cases,  the  path  of  the  independent  variable  being  in  each  case  a  circle  of  radius 
unity  whose  centre  is  fi  : — 

<21.)  y=|.         (22.)y=  +  sjx.         (23.)  y=  ^x.         (24.)  y  =  \  -a-2. 


348 


EXERCISES  XXII 


CHAP.    XV 


Find  by  Horner's  method  the  positive  real  roots  of  the  following  equations 
in  each  case  to  at  least  seven  places  of  decimals  : — * 


(25.)  a? -2  =  0. 

(27.)  a3  +  x  -1000  =  0. 

(29.)  a4  +  x3  +  x"  +  x-  127694  =  0. 

(30. )  a4  -  80a3  +  24a:2  -  6a:  -  80379639  =  0. 


(26.)  x3-  2a-  5  =  0. 

(28. )  x3  -  46a;2  -  36a  +  18  =  0. 

(31.)  x5  -  4a-4  +  7a3  -863  =  0. 
(33.)  x5  -4a  -2000  =  0. 


(32.)  a5 -7  =  0. 

(34. )  4a6  +  7a5  +  9a:4  +  6a3  +  5a2  +  3a  -  792  =  0. 

(35.)  Find  to  twenty  decimal  places  the  negative  root  of  2a4  +  3a3  -  6x -  8 
=  0. 

(36.)  Continue  the  calculation  on  p.  344  two  stages  farther  in  its  uncon- 
tracted  form  ;  and  then  estimate  how  many  more  digits  of  the  root  could 
be  obtained  by  means  of  the  trial  division  alone. 

*  Most  of  these  exercises  are  taken  from  a  large  selection  given  in  De 
Morgan's  Elements  of  Arithmetic  (1854). 


CHAPTEE    XVI. 
Equations  and  Functions  of  the  First  Degree. 

EQUATIONS  WITH  ONE  VARIABLE. 

§  1.]  It  follows  by  the  principles  of  chap.  xiv.  that  every 
integral  equation  of  the  1st  degree  can  be  reduced  to  an  equiva- 
lent equation  of  the  form 

ax  +  b  =  0  (I); 

this  may  therefore  be  regarded  as  a  general  form,  including  all 
such  equations.  As  a  particular  case  b  may  be  zero ;  but  we 
suppose,  for  the  present  at  least,  that  a  is  neither  infinitely  great 
nor  infinitely  small. 

Since  a  4=  0,  we  may  write  (1)  in  the  form 

"{— ("«)}"°  (2>: 

whence  we  see  that  one  solution  is  x  =  -  bja.  We  know  already, 
by  the  principles  of  chap,  xiv.,  §  6,  that  an  integral  equation  of 
the  1st  degree  in  one  variable  has  one  and  only  one  solution.  Hence 
we  have  completely  solved  the  given  equation  (1). 

It  may  be  well  to  add  another  proof  that  the  solution  is  unique. 
Let  us  suppose  that  there  are  two  distinct  solutions,  x  —  a  and  x  =  §,  of  (1). 
Then  we  must  have 

aa  +  b  =  0, 

ap  +  b=0. 

From  these,  by  subtraction,  we  derive 

a(a  -  jS)  =  0. 

Now,  by  hypothesis,  «=t=0,  therefore  we  must  have  a-/S  =  0,  that  is,  a  =  /3; 
in  other  words,  the  two  solutions  are  not  distinct. 


350  TWO  LINEAR  EQUATIONS  IN  ONE  VARIABLE  chap. 

§  2.]  Two  equations  of  the  1st  degree  in  one  variable  will  in 
general  be  inconsistent. 

If  the  equations  be  ax  +  b  =  0  (1), 

a'x  +  b'  =  0  (2), 
the  necessary  and  sufficient  condition  for  consistency  is 

aV  -  a'b  =  0  (3). 

The  solution  of  (1)  is  x  =  -b/a,  and  the  solution  of  (2)  is 
x  =  -  b'/a'.  These  will  not  in  general  be  the  same ;  hence  the 
equations  (1)  and  (2)  will  in  general  be  inconsistent. 

The  necessary  and  sufficient  condition  that  (1)  and  (2)  be 
consistent  is 

b  V 

Since  a  4=  0,  a  4=  0,  (4)  is  equivalent  to 

a'b  -  ab', 
or  ab'  -  a'b  =  0. 

Obs.  1.  If  b  =  0  and  b'  =  0,  then  the  condition  of  consistency 
is  satisfied.  In  this  case  the  equations  become  ax  -  0,  a'x  =  0  ; 
and  these  have  in  fact  the  common  solution  x  =  0. 

Obs.  2.  When  two  equations  of  the  1st  degree  in  one  vari- 
able are  consistent,  the  one  is  derivable  by  multiplying  the  other 
by  a  constant.  In  fact,  since  a  4=  0,  if  we  also  suppose  b  4=  0,  we 
derive  from  (3),  by  dividing  by  ab  and  then  transposing, 

—  =  -r,  each  =  I;  say  ; 

a      b  '     J  ' 

hence  a'  =  ka,     b'  =  kb, 

so  that  a'x  +  b'  =  hax  +  kb, 

=  k(ax  +  b). 

If,  then,  (3)  be  satisfied,  (2)  is  nothing  more  or  less  than 

k(ax  +  b)  =  0 
where  k  is  a  constant. 

This  might  have  been  expected,  for,  transpositions  apart,  the 
only  way  of  deriving  from  a  single  equation  another  perfectly 
equivalent  is  to  multiply  the  given  equation  by  a  constant. 


XVI 


EXERCISES  XXIII  35  i 


Exercises  XXIII. 


Solve  the  following  equations  :  — 

l  +  (l-g)/2 
(2.)  3         =1 


(3.) 


51  62 


5  + 


3a; -1     12a;  +  5 
2  29 


(4.)  3-4-i-~5" 

i-X 

(5.)  -68(-32a;--5)  +  p—=3-694.r, 

find  x  to  three  places  of  decimals. 
(6.)  a/(l-bx)=b/(l-ax). 

(7. )  ("  +  x) (b  +  x)  -  a{b  +c)  =  (ca?  +  bx2)jb. 

x-a    x-c     _ 

(8-)  i, +i =  2- 

K    '  b- a     b-c 

x2-a"    x--b2    %*-<? 

(9.)  -  + r-  + =  a  +  b  +  c-3x. 

N    '  x-a       x - o       x-c 

(10.)  (a3  +  b3)x  +  a3-  bx  =  ft4  -b*  +  a  6(«3  +  b"). 

O  9  O  9 

a;^  -  or     ar  -  c- 

(11.)  -i i =c-a. 

^      >  b+a       b+c 

(12.)  (a?-l)(aJ+2)(2jj-2)=(2a;-l)(2a5+l)(a!/2+I). 


(13.) 

(14.) 
(15.) 
(16.) 
(17.) 
(18.) 


12  3  4 


as+1 

X  +  2 

x  +  3 

a;+4* 

x- 

1 

x-B 

x-2 

a;-  4 

x- 

2 

x-4 

x-  3 

a;-5" 

11 

12B  +  11 

5 
6a;  +~5~ 

7 
'4a;  +  7 

3- 
1- 

x 

X 

5-a: 
'T^x~ 

ar>-2 

1-Zx  +  x2 

2 

;  + 

14 

10 

r  + 

6 

aH-2     a-+10     a;  +  6     a-+14' 

a;2  -  4a;  4-  5 
a;- +  6a; +10 


\x+Zj 


352  ax  +  hj  +  c  =  0  HAS  do1  solutions  chap. 

rim  J-    J-       3(^+5)  6.r+i7 

1      ;  sc  +  l     .r  +  2    (s+l)(as+2)  tf  +  2  ' 

a;  +  2a     a:-2a_     4a& 
(20-)  2b~^x  +  2b  +  x~  ib2-x2' 

(a  +  b)x  +  c     (a-b)x  +  e_         iab 
(      '  (a-b)x  +  d    {a  +  b)x+f~(a  +  b){a-b) 

a+b     a-b       a  b 

(22.)  + ,= ;. 

v      '  x-a    x-b    x-a    x-b 

(23.)  -5-.+     *  "  +  * 


x-a     x-b    x(x-a-b)  +  ab' 


(24-)  --r^+  ~rr-  =  2- 

'                               x+a-bx+b-c 
(85)  X    _- ? 1 


(a;  -  a)  (x -  b)     (x  -a){x-  c)     (x  -b)(x-  c) 

1  2 


+  ; 


{x  +  a)(x  +  b)     (x  +  a)(x  +  c)     (x  +  b)(x  +  c) 


EQUATIONS   WITH    TWO  VARIABLES. 

§  3.]  A  single  equation  of  the  1st  degree  in  two  variables  has  a 
one-fold  infinity  of  solutions. 
Consider  the  equation 

ax  +  by  +  c  =  0  (1). 

Assign    to  y  any  constant    value  we    please,   say    (3,  then    (1) 
becomes 

ax  +  b/3  +  c  =  0  (2). 

We  have  now  an  equation  of  the  1st  degree  in  one  variable, 
which,  as  we  have  seen,  has  one  and  only  one  solution,  namely, 
x  =  -  (bp  +  c)ja. 

We  have  thus  obtained  for  (1)  the  solution  x=  -  (b(3  +  c)ja, 
y  =  f3,  where  ft  may  have  any  value  we  please.  In  other  words, 
we  have  found  an  infinite  number  of  solutions  of  (1). 

Since  the  solution  involves   the   one   arbitrary  constant   /?, 
we  say  that  the  equation  (1)  has  a  one-fold  infinity  (sometimes 
symbolised  by  oo  x)  of  solutions. 
Example. 

the  solutions  are  given  by 

2/3-1  . 


XVI 


TWO  LINEAR  EQUATIONS  IN  TWO  VARIABLES 


353 


we  have,  for  example,  for  /3=  -2,  0=  -  1,  j3  =  0,  /3=  +-,  /3=  + 1,  /3=  +  2,  the 
following  solutions  : — 


/3 

_2 

-1 

0 

1 
+  2 

+  1 

+  2 

5 

1 

1 

a; 

~3 

-1 

~3 

0 

+  3 

+  1 

y 

-2 

-' 

0 

1 

+  2 

+  1 

+  2 

And  so  on. 

§  4.]  We  should  expect,  in  accordance  with  the  principles  of 
chap,  xiv.,  §  5,  that  a  system  of  two  equations  each  of  the  1st 
degree  in  two  variables  admits  of  definite  solution. 

The  process  of  solution  consists  in  deducing  from  the  given 
system  an  equivalent  system  of  two  equations  in  which  the 
variables  are  separated ;  that  is  to  say,  a  system  such  that  x 
alone  appears  in  one  of  the  equations  and  y  alone  in  the 
other. 

We  may  arrive  at  this  result  by  any  method  logically  con- 
sistent with  the  general  principles  we  have  laid  down  in  chap 
xiv.,  for  the  derivation  of  equations.  The  following  proposition 
affords  one  such  method  : — 

If  I,  V,  m,  m'  be  constants,  any  one  of  ichich  may  be  zero,  but 
which  are  such  that  lm!  -  I'm  4=  0,  then  the  two  systems 

ax  +  by  +  c  =  0  (1), 

a'x  +  b'y  +  c'  =  Q  (2), 

and 

J(ax  +  by  +  c)+    l'(a'x  +  b'y  +  c')  =  0  (3), 

m(ax  +  by  +  c)  +  m'ia'x  +  b'y  +  c)  =  0  (4), 

are  equivalent. 

It  is  obvious  that  any  solution  of  (1)  and  (2)  will  satisfy  (3) 
and  (4)  ;  for  any  such  solution  reduces  both  ax  +  by  +  c  and 
a'x  +  b'y  +  c'  to  zero,  and  therefore  also  reduces  the  left-hand 
sides  of  both  (3)  and  (4)  to  zero. 

Again,  any  solution  of  (3)  and  (4)  is  obviously  a  solution  of 
VOL.  I  2  a 


354  SOLUTION  BY  CEOSS  MULTIPLICATION  chap. 

m'{  l(ax  +  by  +  c)  +   l'(a'x  +  b'y  +  c')} 

-  I'  {m(ax  +  by  +  c)  +  m'(a'x  +  b'y  +  c')}  =  0  (5), 

-  m  {  l(ax  +  by  +  c)  +   l'(a'x  +  b'y  +  c')} 

+  1   {m(ax  +  by  +  c)  +  m'(a'x  +  b'y  +  c')}  =  0  (6). 

Now  (5)  and  (6)  reduce  to 

(lm'  -  I'm)  (ax  +  by  +  c  )  =  0  (7), 

{lm!  -  I'm)  {ax  +  b'y  +  c')  =  0  (8), 

and,  provided  lm'  -  l'm^¥  0,  (7)  and  (8)  are  equivalent  to 

ax  +by  +  c  -  0, 
a'x  +  b'y  +  c'  -  0. 

We  have  therefore  shown  that  every  solution  of  (1)  and  (2)  is  a 
solution  of  (3)  and  (4) ;  and  that  every  solution  of  (3)  and  (4)  is 
a  solution  of  (1)  and  (2). 

All  we  have  now  to  do  is  to  give  such  values  to  I,  V,  m,  m' 
as  shall  cause  y  to  disappear  from  (3),  and  x  to  disappear  from 
(4).     This  will  be  accomplished  if  we  make 

I  =  +  V,     V  =  -b, 
m  =  -  a',     m'  =  +  a ; 
so  that  lm'  —  I'm  —  ab'  -  a'b. 

The  system  (3)  and  (4)  then  reduces  to 

(ab'  -  a'h)x  +  cb'  -  c'b  =  0  (3'), 

(ab'  -  a'b)y  +  c'a  -  ca'  =  0  (4') ; 

and  this  new  system  (3'),  (4')  will  be  equivalent  to  (1),  (2), 
provided 

ah'  -a'b^O  (9). 

But  (3')  and  (4')  are  each  equations  of  the  1st  degree  in  one 
variable,  and,  since  ab'  -  a'b  4=  0,  they  each  have  one  and  only 
one  solution,  namely — 

cb'  -  c'b  " 


X         ab'  -  a'b 

y 


ac'  -  a'c 
" ab'- a'b  J 


(10). 


XVI 


MEMORIA  TECHNICA  355 


It  therefore  follows  that  the  system 

ax  +  by  +  c  =  0  (1), 

a'x  +  b'y  +  c'=0  (2) 

has  one  and  only  one  definite  solution,  namely,  (10),  provided 

ab'  -  a'b  *  0  (9). 

The  method  of  solution  just  discussed  goes  by  the  name  of 
cross  multiplication,  because  it  consists  in  taking  the  coefficient 
of  y  from  the  second  equation,  multiplying  the  first  equation 
therewith  ;  then  taking  the  coefficient  of  y  from  the  first  equation, 
multiplying  the  second  therewith ;  and  finally  subtracting  the 
two  equations,  Avith  the  result  that  a  new  equation  appears  not 
containing  y. 

The  following  memoria  tcchnica  for  the  values  of  x  and  y  will  enable  the 
student  to  recollect  the  values  in  (10). 

The  denominators  are  the  same,  namely,  ab'  -  a'b,   formed  from  the  co- 
efficients of  x  and  y  thus 

a\       yb 


a'y       \6' 


the  line  sloping  down  from  left  to  right  indicating  a  positive  product,  that 
from  right  to  left  a  negative  product. 

The  numerator  of  x  is  formed  from  its  denominator  by  putting  c  and  c'  in 
place  of  a  and  a'  respectively. 

The  numerator  of  y  by  putting  c  and  c'  in  place  of  b  and  b'. 

Finally,  negative  signs  must  be  affixed  to  the  two  fractions. 

Another  way  which  the  reader  may  prefer  is  as  follows  :  — 

Observe  that  we  may  write  (10)  thus, 

_bc'-b'c  ca'  -  c'a 

X~abr-a'b'    y~ab'-a'b  (11)' 

where  the  common  denominator  and  the  two  numerators  are  formed  according 
to  the  scheme 


\ 


^a . 
It  is  very  important  to  remark  that  (1)   and    (2)  are  col 

laterally  symmetrical  with  respect  to  I    a,  b     ,  see  chap,  iv.,  §  20. 

V,  v) 

Hence,  if  we  know  the  value  of  x,  we  can  derive  the  value  of  y 
by  putting  everywhere  b  for  a,  a  for  b,  b'  for  a',  and  a  for  b'.    In 


356 


EXAMPLES 


CHAP. 


fact  the  value  of  y  thus  derived  from  the  value  of  x  in  (10)  is 
-  (ca  -  c'a)/(ba'  -  b'a) ;  and  this  is  equal  to  -  (ac'  -  a'c)/(ab'  -  a'b), 
which  is  the  value  of  y  given  in  (10). 


Example  1. 


3x+22/-3  =  0 
9x  +  iy  +  5  =  0 


(a), 
08). 


Proceeding  by  direct  application  of  (11),  we  have 

+  3\/+2X     /-3\/+3 


10  +  12     11 


9 


y=- 


27-15     2 


12  +  18     15'     "     12  +  18     5' 

Or  thus  :  multiply  (a)  by  2,  and  we  have  the  equivalent  system 

Sx  +  iy  -  6  =  0, 
-  9a;  +  4y  +  5  =  0  ; 
whence,  by  subtraction, 

15a;-ll=0, 


which  gives 


11 
*  =  I5- 


Again  multiplying  (a)  by  3,  and  then  adding  Q3),  we  have 

10y-4  =  0, 
which  gives 

4      2 

Example  2. 

a/3     *' 

a'V     7 

Multiplying  the  first  of  these  equations  by  -,  and  subtracting  the  second,  we 
obtain 

i    i\  _i  i 

a2/3  *       J87  ' 

<x2(7-/3) 


that  is, 
whence 


#  = 


7(«"/3) 


Since  the  equations  are  symmetrical  in  f  '  '       )  we  get  the  value  of  y  by 
interchanging  a  and  /3,  namely, 


y= 


7(/3-a) 


xvi  SPECIAL  CASES  357 

Sometimes,  before  proceeding  to  apply  the  above  method,  it 
is  convenient  to  replace  the  given  system  by  another  which  is 
equivalent  to  it  but  simpler. 

Example  3. 

a?x+b-y  =  2ab(a  +  b)  (a), 

b(2a  +  b)x  +  a(a  +  2%  =  a3  +  a?b  +  ab2  +  b*  (/3). 

By  adding,  we  deduce  from  (a)  and  (/3) 

(a  +  b)°~x  +  (a  +  b)2y  =  (a  +  b)3, 

which  is  equivalent  to 

x  +  y  =  a  +  b  (y). 

It  is  obvious  that  (a)  and  (7)  are  equivalent  to  (a)  and  (/3).     Multiplying 

(7)  by  b'2  and  subtracting,  we  have 

(a2-b2)x  =  2a2b  +  ab2-b3, 

=  b(2a-b){a  +  b). 

Hence  #=-— — =— . 

a-  b 

Since  the  original  system  is  symmetrical  in  {  '"'       J,  we  have 

a(2b  -  a) 

§  5.]  Under  the  theory  of  last  paragraph  a  variety  of  par- 
ticular cases  in  which  one  or  more  of  the  constants  a,  b,  c,  a\  b',  c' 
involved  in  the  two  equations 

ax  +  by  +  c  =  0, 
a'x  +  b'y  +  c'  =  0 

become  zero  are  admissible  ;  all  cases,  in  short,  which  do  not 
violate  the  condition  ab'  -  a'b  =t=  0. 

Thus  we  have  the  following  admissible  cases  : — 


'.-> 


a  =  0  (1),  b'  =  0                      (4), 

b  =  0  (2),  a  =  0  and  b'  =  0     (5), 

a'  -  0  (3),  a'  =  0  and  6  =  0     (G). 

The  following  are  exceptional  cases,  because  they  involve  ab'  -  a'b 

=  0:— 

a  =  0  and  a'  =  0  (I.),  a,  b,  a',  V  all  different 

a  =  0  and   b  =  0  (H.),  from  0,  but  such  that 

V  =  0  and  a'  =  0  (III.),  aJ'  -  a'J  =  0            (V.) 

b'  =  0  and   6  =  0  (IV.), 


358  HOMOGENEOUS  SYSTEM  chap. 

We  shall  return  again  to  the  consideration  of  the  exceptional 
cases.  In  the  meantime  the  reader  should  verify  that  the 
formulae  (10)  do  really  give  the  correct  solution  in  cases  (1)  to 
(6),  as  by  theory  they  ought  to  do. 

Take  case  (1),  for  example.     The  equations  in  this  case  reduce  to 
bi/  +  e-0,     a'x  +  b'y  +  c'  =  0. 
The  first  gives  y  —  -  c/b,  and  this  value  of  y  reduces  the  second  to 

a  x  -  -r  +  c  =  0, 

.  -  ,     •  b'c-bc' 

which  gives  x= n — ■• 

a  b 

It  will  be  found  that  (10)  gives  the  same  result,  if  we  put  a  =  0. 

There  is  one  special  case  that  deserves  particular  notice,  that, 

namely,  where  c  =  0  and  c'  =  0  ;  so  that  the  two  equations  are 

homogeneous,  namely, 

ax  +  by  =  0  (a), 

a'x  +  b'y  =  0  (ft). 

If  ab'  -  a'b  4=  0,  these  formula?  (10)  give  x  =  0,  y  =  0  as  the  only 
possible  solution.  If  ab'  -  a'b  =  0,  these  formulae  are  no  longer 
applicable  ;  what  then  happens  will  be  understood  if  we  reflect 
that,  provided  y  4=  0,  (a)  and  (/S)  may  be  written 

az  +  b  =  0  (a'), 

a'z  +  b'  =  0  ((3'), 

where  z  -  x/y. 

We  now  have  two  equations  of  the  1st  degree  in  z,  which 
are  consistent  (see  §  2),  since  ab'  —  a'b  =  0.  Each  of  them  gives 
the  same  value  of  z,  namely,  z  =  -  b/a,  or  z  =  -  b'/a'  (these  two 
being  equal  by  the  condition  ab'  -  a'b  =  0). 

If  then  ab'  —  a'b  4=  0,  the  only  solution  of  (a)  and  ((3)  is  x  =  0, 
y  =  0  ;  if  ab'  -  a'b  =  0,  x  and  y  may  have  any  values  such  that  the 
ratio  x/y  =  -b/a=  -  b'/a'. 

§  6.]  There  is  another  way  of  arranging  the  process  of  solu- 
tion, commonly  called  Bezoitt's  method*  which  is  in  reality  merely 
a  variety  of  the  method  of  §  4. 

*  For  an  account  of  Bezout's  methods,   properly  so   called,   see  Mini's 
papers  on  the  "  History  of  Determinants  ;"  Proc.  R.S.E.,  1886. 


&vi  USE  OF  UNDETERMINED  MULTIPLIER  359 

If  X  be  any  finite  constant  quantity  whatever*  then  any  solution  of  the 
system 

ax  +  by  +  c=0,     a'x  +  b'y  +  c'  =  0  (1) 

is  a  solution  of  the  equation 

[ax  +  by  +  c)  +  \(a'x  +  b'y  +  c')  =  0  (2), 

that  is  to  say,  of         (a  +  \a')x  +  (b  +  \b')y  +  (e  +  \c')  =  0  (3). 
Now,  since  X  is  at  our  disposal,  we  may  so  choose  it  that  y  shall  disappear 
from  (3) ;  then  must 

\b'  +  b  =  Q  (4), 

and  (3)  will  reduce  to  (a  +  \a')x  +  (c  +  \c')  =  0'  (5). 

From  (4)  we  have  \=  -  bjb',  and,  using  this  value  of  X,  we  deduce  from  (5) 

c_+\c'_      b'c  -  be' 
a  +  \a'         ab'-a'b' 
which  agrees  with  (10). 

The  value  of  y  may  next  he  obtained  by  so  determining  X  that  x  shall 
disappear  from  (3).     We  thus  get 

\a'  +  a  =  0  (6), 

(b  +  \b')y  +  (c  +  \c')  =  0  (7), 

and  so  on. 

To  make  this  method  independent  and  complete,  theoretically,  it  would 

of  course  be  necessary  to  add  a  proof  that  the  values  of  x  and  y  obtained  do 

in  general  actually  satisfy  (1)  and  (2);  and  to  point  out  the  exceptional  case. 

§  7.]  There  is  another  way  of  proceeding,  which   is   inter- 
esting and  sometimes  practically  useful. 
The  systems 

ax  +  by  +  c  =  0  ]  .  > 

a'x  +  b'y  +.  d  =  0  J  {  ' 

-i  ax  +  c  x 

aml  »-— J" }  (2) 

a'x  +  b'y  +  c'  =  0  J 

are  equivalent,  provided  b  4=  0,  for  the  first  equation  of  (2)  is 
derived  from  the  first  of  (1)  by  the  reversible  processes  of  trans- 
position and  multiplication  by  a  constant  factor. 

Also,  since  any  solution  of  (2)  makes  y  identically  equal 
to  -  (ax  +  c)/b,  we  may  replace  y  by  this  value  in  the  second 
equation  of  (2).      We  thus  deduce  the  equivalent  system, 

*  So  far  as  logic  is  concerned-  X  might  be  a  function  of  the  variables,  but 
for  present  purposes  it  is  taken  to  be  constant.  A  letter  introduced  in  this 
way  is  usually  called  an  "indeterminate  multiplier  "  ;  more  properly  it  should 
be  called  an  "undetermined  multiplier." 


360  SOLUTION  BY  SUBSTITUTION  CHAP. 

ax  +  c ' 

b'iax  +  c)       ,     „ 
a'a;  -  -^—7 — '-  +  c'  =  0 
0 

Now,  since  b  4=  0,  the  second  of  the  equations  (3)  gives 

(a'b  -  aJ>  +  (6c'  -  b'c)  =  0  (4). 

If  a'b  -  aft'  4=  0,  (4)  has  one  and  only  one  solution,  namely, 

be'  -b'c  .  . 

x  =  aY^7b  (5)' 

this  value  of  x  reduces  the  first  of  the  equations  (3)  to 

1  f  a(bc'  -  b'c)        } 

qj=~n-w^b-+c\' 

abc'  -  a'bc 


b(ab'  -  a'b)' 

that  is,  to  y  =  ca  ~  C  f  (6). 

*     ab  -  ao 

The  equations  (5)  and  (6)  are  equivalent  to  the  system  (3), 
and  therefore  to  the  original  system  (1).  Hence  we  have  proved 
that,  if  ab'  -  a'b  =1=  0  and  b  4=  0,  the  system  (1)  has  one  and  only 
one  solution. 

We  can  remove  the  restriction  b  4=  0 ;  for  if  b  =  0  the  first  of 

the  equations  (1)  reduces  to  ax  +  c  =  0.     Hence  (if  a  4=  0,  which 

must  be,  since,  if  both  a  =  0  and  b  =  0,  then  ab'  -  a'b  =  0)  we  have 

x  =  -  c/a,  and  this  value  of  x  reduces  the  second  of  equations 

(l)to 

a'c      ,,  ,      „ 
+  b'y  +  c  =  0, 

which  gives  (since  V  cannot  in  the  present  case  be  0  without 
making  ab'  -  a'b  =  0)  y  =  (ca'  -  c'a)/ab'.  Now  these  values  of  x 
and  y  are  precisely  those  given  by  (5)  and  (6)  when  b  =  0. 

The  excepted  case  b  =  0  is  therefore  included  ;  and  the  only 
exceptional  cases  excluded  are  those  that  come  under  the  condi- 
tion ab'  -  a'b  =  0. 


xvi  SYSTEM  OF  THREE  EQUATIONS  IN  X  AND  y  3G1 

The  method  of  this  paragraph  may  be  called  solution  -by 
substitution.  The  above  discussion  forms  a  complete  and 
independent  logical  treatment  of  the  problem  in  hand.  The 
student  may,  on  account  of  its  apparent  straightforwardness 
and  theoretical  simplicity,  prefer  it  to  the  method  of  §  4. 
The  defect  of  the  method  lies  in  its  want  of  symmetry  ;  the 
practical  result  of  which  is  that  it  often  introduces  needless 
detail  into  the  calculations. 

Example. 

3«+2y-  3  =  0  (a), 

-9ai  +  4i/  +  5  =  0  (/3). 

From  (a)  we  have  y= — ^ (y)- 

a 

Using  (y),  we  reduce  (/3)  to 

-9a!+2(-3a;+3)  +  5=0, 
that  is,  -15b+11=0; 

whence 

This  value  of  x  reduces  (7)  to 


15 


-3x^  +  3 
15 

y= — 2 — 

2 

=  5' 
The  solution  of  the  system  (a)  and  (J3)  is  therefore 

11  2 

X=15'     y  =  5 

§  8.]   Three  equations  of  the  1st  degree  in  two  variables,  say 

ax  +  by  +  c  =  0,     a'x  +  b'y  +  c'  -  0,     a"x  +  b"y  +  c"  =  0     (1 ), 

will  not  be  consistent  unless 

a" {be'  -  b'c)  +  b"(ca'  -  c'a)  +  c"(ab'  -  a'b)  =  0     (2) ; 

and  they  will  in  general  be  consistent  if  this  condition  be  satisfied. 

We  suppose,  for  the  present,  that  none  of  the  three  functions 
ab'  —  a'b,  a'b-ab",  a'b"  -  a'b'  vanishes.*  This  is  equivalent  to 
supposing  that  every  pair  of  the  three  equations  has  a  deter- 
minate finite  solution. 

If  we  take  the  first  two  equations  as  a  system,  they  have 
the  definite  solution 

*  See  below,  §  25. 


362  CONDITION  OF  CONSISTENCY  chap. 

be'  -  b'c  ca'  -  c'a 

X  =  ^b'~^rb'     V  =  ab'  -  a'b' 

The  necessary  and  sufficient  condition  for  the  consistency  of  the 
three  equations  is  that  this  solution  should  satisfy  the  third 
equation ;  in  other  words,  that 

be'  -b'c         erf  -ca 

a  -n -  +  b  -j-, +  e  =  0. 

ab  -  ab        ab  -  ab 

Since  ab'  -  a'b  4=  0,  this  is  equivalent  to 

a" {be'  -  b'c)  +  b"(ca'  -  c'a)  +  c"(ab'  -  a'b)  =  0  (3). 

The  reader  should  notice  that  this  condition  may  be  written  in 
any  one  of  the  following  forms  by  merely  rearranging  the 
terms : — 

a(b'c"  -  b"c')  +  b(c'a"  -  c"a')  +  c(a'b"  -  a'b')  =  0  (4), 

a'(bc"  -  b"c)  +  b'(ca"  -  c"a)  +  c'(ab"  -  a"b)  =  0  (5), 

a(b'c"  -  b"c')  +  a'(b"c  -  be")  +  a"(bc'  -  b'c)    =  0  (6), 

b(c'a"  -  c'a)  +  b'(c"a  -  ca")  +  b"(ca'  -  c'a)   =  0  (7), 

c(a'b"  -  a"b')  +  c'(a"b  -  ab")  +  c"(ab'  -  a'b)  =  0  (8), 

ab'c"-ab"c'  +  bc'a"   -bc"a'  +  ca'b"   -ca"b'  =  0  (9). 

The  forms  (4)  and  (5)  could  have  been  obtained  directly  by 
taking  the  solution  of  the  two  last  equations  and  substituting  in 
the  first,  and  by  solving  the  first  and  last  and  substituting  in  the 
second,  respectively.  Each  of  these  processes  is  obviously  logic- 
ally equivalent  to  the  one  actually  adopted  above. 

The  forms  (6),  (7),  (8)  would  result  as  the  condition  of  the 
consistency  of  the  three  equations 

ax  +  a'y  +  a"  =  0,     bx  +  b'y+b"  =  Q,     cx  +  c'y  +  c"  =  0     (10). 

We  have  therefore  the  following  interesting  side  result : — 

Cor.  If  the  three  equations  (I)  be  consistent,  then  the  three  equa- 
tions (10)  are  consistent. 

If  the  reader  will  now  compare  the  present  paragraph  with  §  2,  he  will 
see  that  the  function 

ab'  -  a'b 

plays  the  same  part  for  the  system 

ax  +  b  =  0,     a'.r  +  b'  =  0 


XVI 


DETERMINANT  OF  THE  SYSTEM 


363 


as  does  the  function 

a(b'c"  -  b"c')  +  b{c'a"  -  c"a')  +  c(a'b"  -  a"b') 
for  the  system 

ax  +  by  +  c  =  0,     a'x  +  b'y  +  c'  =  0,     a"x  +  b"y  +  c"  =  0. 
These  functions  are  called  the  determinants  of  the  respective  systems  of  equa- 
tions.    The}'  are  often  denoted  by  the  notations 

a      b 
a!     V 


for  ab'  -  a'b 


\a      b      c 
\a'     V     c' 


for  ab'c"  -  ab"c'  +  bc'a"  -  bc"a'  +  ca'b"  -  ca"b' 


(ii); 

(12). 


The  reader  should  notice— 

1st.  That  the  determinant  is  of  the  1st  degree  in  the  constituents  of  any 
one  row  or  of  any  one  column  of  the  square  symbol  above  introduced. 

2nd.  That,  if  all  the  constituents  be  considered,  its  degree  is  equal  to  the 
number  of  equations  in  the  system. 

A  special  branch  of  algebra  is  nowadays  devoted  to  the  theory  of  deter- 
minants, so  that  it  is  unnecessary  to  pursue  the  matter  in  this  treatise.  For 
the  sake  of  more  advanced  students  we  have  here  and  there  introduced  results 
of  this  theory,  but  always  in  such  a  way  as  not  to  interfere  with  the  progress 
of  such  as  may  be  unacquainted  with  them. 

The  reader  may  find  the  following  memoriae  technicse,  useful  in  enabling 

him  to  remember  the  determinant  of  a  system  of  three  equations  : — 

For  the  form  (4), 

a  b  c 


b' 


b" 


V 


b\ 


to  be  interpreted  like  the  similar  scheme  in  §  4. 
For  the  form  (9), 

b 


or  &"/         no- 

where the  letters  in  the  diagonal  lines  are  to  form  products  with  the  signs  -f 
or  - ,  according  as  the  diagonals  slope  downwards  from  left  to  right  or  from 
right  to  left. 

Example. 

To  show  that  the  equations 

3.r  +  5t/-2  =  0,     4ic  +  6?/-l=0,     2.r  +  4?/ -  3  =  0 

are  consistent. 

Solving  the  first  two  equations,  we  have  x=  -7/2,  j/  =  5/2.     These  values 


364 


EXERCISES  XXIV 


CHAP. 


reduce  2x  +  iy-B  to  -7  +  10-3,  which  is  zero.  Hence  the  solution  of  the 
first  two  equations  satisfies  the  third  ;  that  is,  the  three  are  consistent. 

We  might  also  use  the  general  results  of  the  above  paragraph. 

Since  3x6-5x4= -2,  5x2-3x4=-2,  4  x  4- 2  x  6= +4,  each  pair 
of  equations  has  by  itself  a  definite  solution.  Again,  calculating  the  deter- 
minant of  the  system  by  the  rule  given  above,  we  have,  for  the  value  of  the 
determinant,  -  54  -  10  -  32  +  24  + 12  +  60  =  0.  Hence  the  system  is  consistent. 
+  3+5  2+3+5 


+  2     + 


Exercises  XXIV. 
Solve  the  following  : — 

(1.)  £*+&=«,     |aj+Jy=6J. 

(2.)  &B+3y=18,     3x-2y  =  9. 

(3.)  -123.?+ -685?/ =  3 -34,     -893a!-  '59% =8 '71, 

find  x  and  y  to  five  places  of  decimals. 


(4.) 

(5.) 
(6.) 
(7.) 

(8.) 

(9.) 
(10.) 

(11.) 

(12.) 
(13.) 


x  +  y:x-y  =  5  : 3,     x  +  5y=Z6. 
Sx  +  l  =  2y  +  l  =  Zy  +  2x. 
{x+S)(y+S)  =  (x-l)(y+2),     8x  +  5  =  9y  +  2. 

x  +  y  =  a  +  b,     (x  +  a)l(y  +  b)  =  b/a. 


x       y 
la     mb 


2via~rZlb 


ax  +  by  =  0,     (a-b)x+(a  +  b)y  =  2c 
(a  +  b)x-  (a-b)y~c,     (a-b)x  +  (a  +  h)y=e. 

(a  +  b)x  +  (a  -b)y  =  a-  +  2ab  -  b2,     (a  -  by  +  [a  -  b)y  =  a2  +  b2. 


y 


-ab, 


V 


a-  -b2    a2  +  ab  +  b2~""''    a2+b2  '  a2-ab  +  b2 
(apm  +  bq'")x  +  {ii]imJrl  +  bqm+x)y  =  «/>"'+-  +  bqm+2, 
[npn  +  bq")x  +  {«2>"+l  +  bq"+^  )y  =  «^"+-  +  bq"+2. 


a{2a+b). 


(14.)  Find  \  and  p.  so  that  x3  +  Xx2  +  /xx  +  abc  may  be  exactly  divisible  by 
x  -  b  and  by  x  -  c. 

(15.)  If  X  4=0,  and  if  x-y  =  a-b,  -^—  +  -^—=1,  -X—+-!L=l,  be  con- 

J  a  +  X     b  +  X       '  a  -  X     b-\ 

sistent,  show  that  X=  ±\/aL 

(16.)  If  the  system  (b  +  c)x+{c  +  a)y  +  (a  +  b)  =  0,  (c  +  a)x+(a  +  b)y+  (b  +  c) 
—  0,  (a  +  b)x+{b  +  c)y  +  (c  +  a)~0,  be  consistent,  then  os8  + &*+<?- 3a&c=0. 

(17.)  Find  the  condition  that  ux-\-by  =  c,  a2x+b-i/  =  c'-,  a*x  +  b3y  =  c3  be 
consistent. 


xvi      SYSTEMS  OF  ONE  AND  OF  TWO  EQUATIONS  IN  X,  1J,  Z      365 

(18.)  Find  an  integral  function  of  a;  of  the  1st  degree  whose  values  shall 
be  +9  and  +10  when  x  has  the  values  -3  and  +  2  respectively. 

(19.)  Find  an  integral  function  of  x  of  the  2nd  degree,  such  that  the 
coefficient  of  its  highest  term  is  1,  and  that  it  vanishes  when  x=2  and  when 
x=  -3. 

(20.)  Find  an  integral  function  of  x  of  the  2nd  degree  which  vanishes 
when  .r=0,  and  has  the  values  -1  and  +  2  when  x—  -  1  and  x  =+3 
respectively. 


EQUATIONS  WITH  THREE  OR  MORE  VARIABLES. 

§  9.]  A  single  equation  of  the  1st  degree  in  three  variables  admits 
of  a  two-fold  infinity  of  solutions. 
For  in  any  such  equation,  say 

ax  +  by  +  cz  +  d  =  0, 

we  may  assign  to  two  of  the  variables  any  constant  values  we 
please,  say  y  =  ft,  z  —  y,  then  the  equation  becomes  an  equation 
of  the  1st  degree  in  one  variable,  which  has  one  and  only  one 
solution,  namely, 

b(3  +  cy  +  d 

x  =  — • 

a 

We  thus  have  the  solution 

bB  +  cy  +  d 

x= f — ■.    y  =  P,    *  =  y- 

Since  there  are  here  two  arbitrary  constants,  to  each  of 
which  an  infinity  of  values  may  be  given,  we  say  that  there  is 
a  two-fold  infinity  (oo  2)  of  solutions.  A  symmetric  form  is  given 
for  this  doubly  indeterminate  solution  in  Exercises  xxv.,  27. 

§  10.]  A  system  of  two  equations  of  the  1st  degree  in  three  vari- 
ables admits  in  general  of  a  one-fold  infinity  of  solutions. 

Consider  the  equations 

ax  +  by  +  cz  +  d  =  0,     a'x  +  b'y  +  c'z  +  d' =  0  (1). 

We  suppose  that  the  functions  be'  -  b'c,  ca  -  c'a,  ab'  -  a'b  do  not 
all  vanish,  say  ab'  —  a'b  4=  0. 

If  we  give  to  z  any  arbitrary  constant  value  whatever,  say 
z  =  y,  then  the  two  given  equations  give  definite  values  for  x  and 
y.     We  thus  obtain  the  solution 


366  HOMOGENEOUS  SYSTEM  OF  TWO  EQUATIONS  chap. 

(bc'-b'c)y  +  (bd'  -b'd)  (ca'  -  c'a)y  +  (da'  -  d'a)       _ 

X  =  ~~; abr^7b  ,V~  ab'-ab  »*     7  W- 

Since  we  have  here  one  arbitrary  constant,  there  is  a  one-fold 
infinity  of  solutions. 

Cor.  There  is  an  important  particular  case  of  the  above  that 
often  occurs  in  practice,  that,  namely,  where  d  =  0  and  d'  =  0. 
We  then  have,  from  (2), 

be'  -  b'c  ca'  -  c'a 

ab  -  ab '      *     ah  -  ab'  ' 

This  result  can  be  written  as  follows  : — 

x  y 


be'  -  b'c     ab'  -  aV 

V       =       7 
ca'  -  c'a     ab'  -  a'b' 

z       =       7 
ab'  -  a'b     ab'  -  a'b 

Now,  y  being  entirely  at  our  disposal,  we  can  so  determine 
it  that  y/(ab'  -  a'b)  shall  have  any  value  we  please,  say  p.  Hence, 
p  being  entirely  arbitrary,  we  have,  as  the  solution  of  the  system, 


ix  +by  +  cz  =0  )  .  v 

i'x  +  b'v  +  c'z  =  0)  ^  '* 


ax 

ax  +  by 
x  -  p(bc'  -  b'c),     y  =  p(ca'  -  c'a),     z  =  p(ab'  -  a'b)        (4). 

It  will  be  observed  that,  although  the  individual  values  of 
x,  y,  z  depend  on  the  arbitrary  constant  p,  the  ratios  of  x,  y,  z 
are  perfectly  determined,  namely,  we  have  from  (4) 

x :  y :  z  =  (be'  -  b'c) :  (ca'  -  c'a) :  (ab'  -  a'b). 

Example  1. 

2x  +  3y  +  4z=0, 

3x-2y-6z-0, 
x  y  z 


-2  -6  3  -2 

give  x:y:z-  -10  :  24  :  -13; 


xvi  SYSTEM  OF  THREE  EQUATIONS  IN  X,  If,  Z  367 

or,  which  is  the  same  thing, 

a;=-10p,     ?/  =  24/>,     z  —  -  ISp, 
p  being  any  quantity  whatsoever. 

Example  2. 

ax  +  by  +  cz  —  0, 
a2x  +  b2y  +  c2z=0, 
give  x  =  {be2  -  b2c)p  =  -  bcp(b  -  c), 

y  =  {ca2-c2a)p  =  -  cap(c  -  a) , 
z=  {ab2  -  a2b)p  —  -  abp(a  -  b): 

If  we  choose,  we  may  replace  -  abep  by  <r,  say,  and  we  then  have 

x-a(b-c)/a,     y  =  <r(c-a)/b,     z  —  a{a-b)\c, 

where  a  is  arbitrary. 

In  other  words,  we  have 

x  :y  :z  =  (b-  c)/a  :  (c  -  a)/b  :  (a  -  b)/c. 
§  11.]  A   system  of  three  equations  of  the    1st  degree  in  three 
variables,  say 

ax  +by  +  cz   +  d  =0  (1), 

a'x  +  b'y  +  c'z  +  6!  =  0  (2), 

a"x  +  b"y  +  c"z  +  d"  =  0  (3), 

has  one  and  only  one  solution,  provided 

ab'c"  -  ab"c'  +  be' a"  -  bc"a'  +  ca'b"  -  cab'  *  0  (4). 

The  three  coefficients  c,  c,  c"  cannot  all  vanish,  otherwise  we 
should  have  a  system  of  three  equations  in  two  variables,  x  and 
y,  a  case  already  considered  in  §  8. 

Let  us  suppose  that  c  =t=  0,  then  the  following  system 

ax  +by  +  cz  +  d    =0  (5), 

c'  (ax  +  by  +  cz  +  d)  -  c(a'x  +  b'y  +  c'z  +  d')  =  0  (6), 

c"(ax  +  by  +  cz  +  d)-  c(a"x  +  b"y  +  c"z  +  d")  =  0  (7), 

is  obviously  equivalent  to  (1),  (2),  and  (3).  Matters  are  so 
arranged  that  z  disappears  from  (6)  and  (7) ;  and  if,  for  short- 
ness, we  put 

A  -  ac'  -  a'c,        B  =  be'  -  b'c,       C  =  dc'  -  d'e, 
A'  -  ac"  -  a"c,     B'  =  be"  -  b"c,     C  =  dc"  -  d"c, 
we  may  write  the  system  (5),  (6),  (7)  as  follows  : — 

ax  +  by  +  cz  +  d  =  0  (5'), 

Ax  +  By  +  C  -  0  (6'), 

Ax  +  B'y  +  0'  =  0  (7'). 


368 


GENERAL  SOLUTION 


CHAP. 


(8), 

(9). 
(10). 

(11). 


Now,  provided  AB'  -  A'B  4=  0 

(6')  and  (7')  have  the  unique  solution 

,  _  BC  -  B'C 
X  ~  AB'  -  A'B 

_  CA  -  CA 

y  ~  AB'  -  A'B 

These  values  of  x  and  y  enable  us  to  derive  from  (5') 

g(BC  -  B'C)  +  b(CA'  -  CA)  +  d(AB'  -  A'B) 
Z  ~  f (AB'  -  A'B) 

(9),  (10),  and  (11)  being  equivalent  to  (5'),  (6'),  (7'),  that  is, 
to  (1),  (2),  (3),  constitute  a  unique  solution  of  the  three  given 
equations. 

It  only  remains  to  show  that  the  condition  (8)  is  equivalent 
to  (4). 

We  have 
AB'  -  A'B  =  {ad  -  a'c)  (be"  -  b"c)  -  (ac"  -  a"c)  (be'  -  b'c), 

=  c(ab'c"  -  ab"c'  +  be' a"  -  be" a'  +  ca'b"  -  ca"b')     (12). 
Hence,  since  c  4=  0,  (8)  is  equivalent  to  (4). 

Although,  in  practice,  the  general  formulae  are  very  rarely  used,  }ret  it  may 
interest  the  student  to  see  the  values  of  x,  y,  z  given  hy  (9),  (10),  (11)  ex- 
panded in  terms  of  the  coefficients.     We  have 

-  (BC  -  B'C)  =  {dc'  -  d'e)  (Id'  -  b"c)  -  (dc"  -  d"c)  (be'  -  b'c). 

Comparing  with  (12),  we  see  that  -(BC'-B'C)  differs  from  AB'-A'B 
merely  in  having  d  written  everywhere  in  place  of  a  (the  dashes  being 
imagined  to  stand  unaltered).     Hence 

-  (BC  -  B'C)=c(db'c" -  db"c'  +  be'd"  -  be'd'  +  cd'b"  -  cd"b'). 
So  that  we  may  write 


d(b'c"  -  b"c')  +  d'(b"c  -  be")  +  d"(bc'  -  b'c) 

X= 7- 


(13). 


a(b'c"  -  b"c')  +  a'(b"c  -  be")  +  a"(bc'  -  b'c) 

We  obtain  the  values  of  y  and  2  by  interchanging  a  and  b  and  a  and  c 
respectively,  namely, 

d(a'c"  -  a"c')  +  d'(a"c  -  ac")  +  d"(ac'  -  a'c) 


?/=  - 


b(a'c"  -  a"c')  +  b'(a"c  -  ac")  +  b"(ac'  -  a'c) 
d(b'a"  -  b"a')  +  d'(b"a  -  ba")  +  d"(ba'^  b'a) 
c(b'a" -  b"a')  +  c'(b"a-ba")  +  c"(ba'  -  b'a) 


(14), 
(15). 


XVI 


HOMOGENEOUS  SYSTEM  OF  THREE  EQUATIONS 


3G9 


Written  in  determinant  notation  these  would  become 


V  = 


d 

b 

c 

a 

b 

c 

d' 

V 

c 

-^ 

a' 

V 

e 

(13'), 

d" 

b" 

c 

a" 

b" 

c 

a 

d 

c 

a 

b 

c 

a' 

d' 

c' 

4- 

a' 

V 

c' 

an 

a" 

d" 

c" 

a" 

b" 

It 

c 

a 

h 

d 

a 

b 

c 

a' 

V 

d' 

4- 

a' 

b' 

c' 

(15'). 

a" 

b" 

d" 

a" 

b" 

c" 

§  12.]  In   the   special   case   where   d  —  0,  d'  =  0,  d"  =  0,  the 
equations  (1),  (2),  (3)  of  last  paragraph  become 

ax  +by  +  cz  =0  (1), 

a'x  +  b'y  +  c'z  =  0  (2), 

a"x  +  b"y  +  c'z  -  0  (3), 

which  are  homogeneous  in  x,  y,  z. 

If  the  determinant  of  the  system,  namely,  a" (be  -  b'c)  +  b"(ca'  -  c'a) 
+  c"(ab'  -  a'b),  do  not  vanish,  tee  see  from  §  11  (9),  (10),  (11)   (or 
more  easily  from  (13),  (14),  and  (15)  of  the  same  section)  that 

x  =  0,     y  -  0,     3  =  0. 
If  the  determinant  does  vanish,  this  conclusion  does  not  necessarily 
follow. 

In  fact,  if  we  write  (1),  (2),  (3)  in  the  form 


a  -  +  b  -  +  c 
z        z 


0 


«'-  +  ^  +  c'  =  0 

z        z 

a',X-  +  b"V-  +  c"  =  0 
z        z 


0'), 

(2'), 
(3'), 


and  regard  xjz  and  yjz  as  variables,  these  equations    are  con- 
sistent, since 

a" {be'  -  b'c)  +  b"(ca'  -  c'a)  +  c"(ab'  -  a'b)  =  0  (4), 

and  any  two  of  them  determine  the  ratios  xjz,  yjz ;  so  that  we 
have 

x:y:z-bc'  -b'c  :  at'  -  c'a  :  ab'  -  a'b, 
=  be"  -  b"c  :  ca"  -  c"a  :  ab"  -  ab, 
=  b:c"  -  b"d  :  c'a"  -  c"a'  :  a'b"  -  a"b'. 

VOL.  I  2  B 


370  EXAMPLES 


CHAP. 


These  different  values  of  the  ratios  are  in  agreement,  by  virtue 
of  (4),  as  the  student  should  verify  by  actual  calculation. 

Hence,  if  the  determinant  of  a  system  of  three  homogeneous  equa- 
tions of  the  1st  degree  in  x,  y,  z  vanish,  the  values  of  x,  y,  z  are  inde- 
terminate {there  being  a  one-fold  infinity  of  solutions),  but  their  ratios 
are  determinate. 

§  13.]  Knowing,  as  we  now  do,  that  a  system  of  three  equa- 
tions of  the  1st  degree  in  x,  y,  z  has  in  general  one  definite 
solution  and  no  more,  we  may  take  any  logically  admissible 
method  of  obtaining  the  solution  that  happens  to  be  convenient. 
(1)  We  may  guess  the  solution,  or,  as  it  is  put,  solve  by  inspec- 
tion, verifying  if  necessary.  (2)  We  may  carry  out,  in  the 
special  case,  the  process  of  §  11;  this  is  perhaps  the  most  gene- 
rally useful  plan.  (3)  We  may  solve  by  substitution.  (4)  We 
may  use  Bezout's  method.  (5)  We  may  derive  from  the  given 
system  another  which  happens  to  be  simpler,  and  then  solve 
the  derived  system.  The  following  examples  illustrate  these 
different  methods  : — 

Example  1. 

x  +  y  +  z  =  a  +  b  +  c,     (b-c)x  +  {c-a)y  +  {a-b)z  =  0,     -  +  \  +  -—3. 

'       v        '"  '  a     b     c 

A  glance  shows  ns  that  this  system  is  satisfied  by  x  =  a,  y  =  b,  z  —  c;  and, 
since  the  system  has  only  one  solution,  nothing  more  is  required. 

Example  2. 

Bx  +  5y-    7;- 2  =  0  (a), 

4af+8y-14z+3=0  (jS), 

Sx  +  6y-    8~-3  =  0  (7). 

Multiplying  (a)  by  4  and  (/3)  by  3,  and  subtracting,  we  obtain 

4^-143+17  =  0  (3). 

From  (a)  and  (7),  by  subtraction, 

2/-~-l  =  0  (e). 

Multiplying  (e)  by  4,  and  subtracting  (5),  we  have,  finally, 

l(b-21  =  0; 
whence  z=2'l. 

Using  this  value  of  z  in  (e),  we  find 

V  =  3-1; 

and,  putting  3/ =8  1,  z  =  2'\  in  (a),  we  find 

x  =-4. 
The  solution  of  the  system  (a),  (/3),  (7)  is  therefore 

x=-i,     t/  =  3-1,     ss=21. 


XVI 


EXAMPLES  371 


Example  3. 

Taking  the  equations  (a),  (/3),  (7)  of  last  example,  we  might  proceed  by 
substitution,  as  follows  :  — 
From  (a) 

5       7       2 
X=-3y  +  3Z  +  3- 


20       28       8 


This  value  of  x  reduces  (/3)  to 

which  is  equivalent  to 

4y-14z  +  17  =  0  (5')- 

Substituting  the  same  value  of  as  as  before  in  (7),  we  deduce 

2/-~-l=0  (e'). 

Now  (e')  gives 

y=z+l, 
and  this  value  of  y  reduces  (5')  to 

-102  +  21  =  0, 
hence  ~  =  21. 

The  values  of  y  and  x  can  now  be  obtained  by  using  first  (e')  and  then  (a). 

Example  4. 

Taking  once  more  the  equations  (a),  (^),  (7)  of  Example  2,  Ave  might  pro- 
ceed by  Bezout's  method. 

If  X  and  fi  be  two  arbitrary  multipliers,  we  derive  from  (a),  (/3),  (7), 
(3x  +  5y-7z-2)  +  \(ix  +  8y-liz  +  3)  +  /jL(3z  +  6y-8z-3)  =  0      (5'). 
Suppose  that  we  wish  to  find  the  value  of  x.     We  determine  X  and  /j.  so  that 
(5')  shall  contain  neither  y  nor  z.     We  thus  have 

8X  +  6/*+5  =  0  (e'), 

-14X-8/x-7  =  0  (D, 

(3  +  4X  +  3/4£-2  +  3X-3m=0  (if). 

If  we  solve  (e')  and  (f),  we  obtain 

X=--l,     ^=-7. 
The  last  equation  (rf)  thus  becomes 

(3--4-2-1).b-2-  -3  +  2-1  =  0, 
that  is,  'ox-  #2  =  0  ; 

whence  x=  -2/*5  =  -4. 

The  values  of  y  and  z  may  be  obtained  by  a  similar  process. 

Example  5. 

ax  +  by  +  cz  =  0  (a), 

(b  +  c)x  +  {c  +  a)y  +  (a  +  b)z=0  (|3), 

a2x  +  b*y  +  ch  =  a2{b  -  c)  +  b-{c  -  a)  +  c-(a  -  b)      (7). 
From  (a)  and  (/3)  we  derive,  by  addition, 

(a  +  b  +  c)(x  +  y  +  z)  =  0, 
which,  provided  «  +  i  +  c  +  0,  is  equivalent  to 

x  +  y  +  z  =  0  (5). 

We  can  now,  if  we  please,  replace  (a)  and  (/3)  by  the  equivalent  simpler  pair 
(a)  and  (5). 


372  EXAMPLES  chap. 

Now  (see  §  10),  by  virtue  of  (a)  and  (5),  we  have 

x         y  z  .  . 

b-c     c-a    a-b 
If  none  of  the  three,  b-c,  c-a,  a-b,  vanish,  we  may  write  (7)  in  the  form 

a2(b  -  c),—  +  b-(c  -  a)^—  +  c-(a  -  b) -^  =  a2(b  -c)  +  b2(c  -a)  +  c"(a  -  b). 
b  —  c  c  —  a  a  —  b 

Using  (e)  we  can  replace  y/{c-a)  and  zfta-b)  by  x/(b-c),  and  the  last  equa- 
tion becomes 

{a°-(b-c)  +  b-(c-a)  +  <?(a-b)},—  =  a"(b-c)  +  b*-(c-a)  +  c2(a-b); 

0      c 

and,  since  a"(b-c)  +  b-{c-a)+c-(a  -b)  =  -(b-c)  {c-a)  (a-  b),  which  does  not 

vanish,  if  our  previous  assumptions  be  granted,  it  follows  that 

b-c 
Hence  x  =  b-c,  and,  by  symmetry,  y  =  c-a,  z  =  a-b. 

This  solution  might  of  course  have  been  obtained  at  once  by  inspection. 

Example  6. 

x  +  ay  +  a2z  +  a3=0\ 

x  +  by  +  b2z  +  ¥  =  ol  (a). 

x  +  cy  +  c-z+c3-0J 
From  the  identity 

Z3+p£z+qZ+r={£-a)$-b){Z-c), 

(see  chap,  iv.,  §  9),  where 

2)= -a -b-c,     q  —  bc  +  ca  +  ab,     r=-abc, 
we  have 

r  +  aq  +  a2p  +  a?  =  0\ 

r  +  bq+b2j,+  b3=0l  (£). 

r  +  cq+c-p+  (^-0) 

It  appears,  therefore,  from  (,3)  that 

x-r,     y  =  q,     z=p 
is  a  solution  of  (a).     Hence,  since  (a)  has  only  one  solution,  that  solution  is 
x=-abc,     y=bc  +  ca  +  ab,     z='—a  —  b  —  c 
This  result  may  be  generalised  and  extended  in  various  obvious  ways. 

§  14.]  A  system  of  more  than  three  equations  of  the  1st  degree 
in  three  variables  will  in  general  be  inconsistent.  To  secure  consistency 
one  condition  must  in  general  be  satisfied  for  every  equation  beyond 
three.  This  may  be  seen  by  reflecting  that  the  first  three  equa- 
tions will  in  general  uniquely  determine  the  variables,  and  that 
the  values  thus  found  must  satisfy  each  of  the  remaining  equa- 
tions. Thus,  in  the  case  of  four  equations,  there  will  be  one 
condition  for  consistency.  The  equation  expressing  this  condition 
could  easily  be  found  in  its  most  general  form  ;  but  its  expression 
would  be  cumbrous  and  practically  useless  without  the  use  of 


xvi  GENERAL  THEORY  FOR  A  LINEAR  SYSTEM  373 

determinantal  or  other  abbreviative  notation.  There  is,  how- 
ever, no  difficulty  in  working  out  the  required  result  directly  in 
any  special  case. 

Example. 

Determine  the  numerical  constant  p,  so  that  the  four  equations 
2x~Zy+5z=18,     3x-y  +  lz  =  2Q,     4x  +  2y-z=5, 

{p+l)x+{p+2)y+(p  +  S)z=76 

shall  he  consistent. 

If  we  take  the  first  three  equations,  they  determine  the  values  of  x,  y,  z, 
namely,  x=l,     y  =  B,     2  =  5. 

These  values  must  satisfy  the  last  equation  ;  hence  we  must  have 
(p  +  l)  +  (p  +  2)3  +  (p  +  3)5  =  76, 
which  is  equivalent  to 

9p  =  5i. 
Hence  p  =  6. 

§  15.]  If  the  reader  will  now  reconsider  the  course  of  reason- 
ing through  which  we  have  led  him  in  the  cases  of  equations  of 
the  1st  degree  in  one,  two,  and  three  variables  respectively,  he 
will  see  that  the  spirit  of  that  reasoning  is  general ;  and  that, 
by  pursuing  the  same  course  step  by  step,  we  should  arrive  at 
the  following  general  conclusions  : — 

I.  A  system  of  n  -  r  equations  of  the  1st  degree  in  n  variables 
has  in  general  a  solution  involving  r  arbitrary  constants;  in  other 
words,  has  an  r-fold  infinity  of  different  solutions. 

II.  A  system  of  n  equations  of  the  1st  degree  in  n  variables  has 
a  unique  determinate  solution,  provided  a  certain  function  of  the  co- 
efficients of  the  system,  which  we  may  call  the  determinant  of  the 
system,  does  not  vanish. 

III.  A  system  of  n  +  r  equations  of  the  1st  degree  in  n  variables 
will  in  general  be  inconsistent.  To  secure  consistency  r  different  con- 
ditions must  in  general  be  satisfied. 

There  would  he  no  great  difficulty  in  laying  down  a  rule  for  calculating 
step  hy  step  the  function  spoken  of  above  as  the  determinant  of  a  system  of 
n  equations  of  the  1st  degree  in  n  variables  ;  hut  the  final  form  in  which  it 
would  thus  be  obtained  would  be  neither  elegant  nor  luminous.  Experience 
has  shown  that  it  is  better  to  establish  independently  the  theory  of  a  certain 
class  of  functions  called  determinants,  and  then  to  apply  the  properties  of 
these  functions  to  the  general  theory  of  equations  of  the  1st  degree.  A 
brief  sketch  of  this  way  of  proceeding  is  given  in  the  next  paragraph,  and 
will  be  quite  intelligible  to  those  acquainted  with  the  elements  of  the  theory 
of  determinants. 


374 


GENERAL  SOLUTION  OF  LINEAR  SYSTEM 


CHAP. 


GENERAL    SOLUTION    OF   A    SYSTEM    OF   LINEAR   EQUATIONS 
BY    MEANS    OF    DETERMINANTS. 


§16.]  Consider  the  system 

"D-!  =anxx  +  a12.r2  +  .  . 

.  +  amxn  +  c, 

=  0 

(1), 

KJ  2    ==  ^'21     1             ^22*   2      '     *      * 

•  +  CWEji   +  C-2 

=  0 

(2), 

U„  *  ffljuJB,  +  rt,!2a-2  +  .    .    .  +  fl^Bn  +  Cn  =  0  (»), 

where  there  are  n  variables,  2,,  x2,  .  .   .,  #«,  and  ra  equations  to 
determine  them. 


Let 


A  = 


an    a]2 


"«2 


and  let  AM  A2,  .  .  .,  An  denote  the  determinants  obtained  from  A 
by  replacing  the  constituents  of  the  1st,  2nd  .  .  .  nth  columns 
respectively,  by  the  set  r,,   c2,  .  .  .,  cn. 

Also  let  the  co-factors  of  a,„  aI2,  .  .  .,  am,  a21,  a22,  .  .  .,  am, 
&c.,  A  be  denoted  by  Au,  AI2)  .  .  .,  Am,  A21,  A22,  .  .  .,  A2n,  &c, 
as  usual. 

Then,  by  the  theory  of  determinants,  we  have 

OuA,,  +  OnAa   +  .    .    .  +  amAm  =  A    \ 
aISA„  +  rt23A21  +  .   .  .  +  an2Am  =  0 

(a), 

a,nAu  +  a.mA2i  +  .  .  .  +  annAm  =  0 

ciAi  +  £3-^1    +  .   .   .  +  <"nA,u    =  A,  J 
and  so  on. 

If  the  determinant  A,  which  we  call  the  determinant  of  the 
system  of  equations,  does  not  vanish,  then  Au,  A21,  .  .  .,  A,n 
cannot  all  vanish.  Let  us  suppose  that  A„  4=  0.  Then,  by 
chap,  xiv.,  §  10,  the  system 

AUU,  +  A21U2  +  .  .  .  +  A/UU„  =  0, 

U2=0,    u,  =  o,    .  .  .,    un=o, 

is  equivalent  to  the  system  (1),  (2)  .   .   .  (»).      If  we  collect  the 


XVI 


BY  MEANS  OF  DETERMINANTS 


375 


coefficients  of  the  variables  ar, ,  x2,  .  .  .,  xn  in  the  first  of  these 
equations,  and  attend  to  the  relations  (a),  that  equation  reduces  to 

A»,  +  At  =  0. 
Since  A  +  0,  this  is  equivalent  to 

*,=  -A/A. 

By  exactly  similar  reasoning  we  coidd  show  that  x2  =  -  A.,/ A,  .  .  . 
xn=  -  An/A.  Hence  the  solution,  and  the  only  solution,  of  (1), 
(2),  .  .  .,  (n)  is 

k,  =  -  A,/A,     x2  =  -  A2/A,     .  .   .,     xn=  -  A,,./ A    (ft). 

Although,  from  the  way  we  have  conducted  the  demonstration, 
it  is  not  necessary  to  verify  that  (ft)  does  in  fact  satisfy  (1), 
(2),  .  .  .,  (a),  yet  the  reader  should  satisfy  himself  by  substitu- 
tion that  this  is  really  the  case. 

We  have  thus  shoivn  that  a  system  of  n  equations  of  the  1st  degree 
in  n  variables  has  a  unique  determinate  solution,  provided  its  determin- 
ant does  not  vanish. 

Next,  let  us  suppose  that,  in  addition  to  the  equations  (1), 
(2),  .  .  .,  (n)  above,  we  had  another,  namely, 

0»+i,i  xi  +  a»+i,2  x2  +  •  •  •  +  aw+i,«  %n  +  Cn+i  =  Oj  (a  +  1 ), 
the  system  of  n  +  1  equations  thus  obtained  will  in  general  be 
inconsistent. 

The  necessary  and  sufficient  condition  for  consistency  is  that  the 
solution  of  the  first  n  shall  satisfy  the  n+lth,  namely,  ^/A=t=0, 


—  #71+1,1  A, 


tf»+i>2A2- 


a 


u 

a2l 


a™, 


an+i,n  Aji  +  C,!-)-! 

...     i 


A  =  0,  that  is, 


(1-2,1 


II 


rt+i,i     #n+2,s 


"  nil  '  II 

an+2,n  ("n+i 


=  0 


(y)- 


Lastly,  let  us  consider  the  particular  case  of  n  homogeneous 
equations  of  the  1st  degree  in  n  variables.  In  other  words,  let 
us  suppose  that,  in  equations  (1),  (2),  .  .  .,  (/<)  above,  we  have 
c,  =  0,  c2  =  0,   . 


.,    Cn=0. 


376     CONDITION  OF  CONSISTENCY HOMOGENEOUS  SYSTEM    chap. 


1st.  Suppose    A  4=  0,    then,  since   now  Al  =  0,   A.,  -  0, 
An  =  0,  (/3)  gives  Xy  =  0,  x2  =  0,  .  .  .,  xn  =  0. 
2nd.  Suppose  A  =  0. 
We  may  write  the  equations  in  the  form 


xx 


x, 


On—  +  «m—  +  •   •    •  +  am  =  0, 


■'  a 


X~ 


«2i—  +  «»—  +  .  .  .+am  =  0, 


"21  T    •*«! 


X\  x% 

Q"M  ^  ^W2  I" 


+  ann  =  0. 


These  may  be  regarded  as  a  system  of  n  equations  of  the  1st 
degree  in  the  n  —  1  variables  xfxm  x.,/xn,  .  .  .,  xn^\xn\  and,  since 
A  =  0,  they  are  a  consistent  system.  Using  only  the  last  n-\ 
of  them,  we  find 


x1 

Xn 


"'in     (*22     •      •     •      ®2,n  -  1 
^371     ^32     •      •      •      Q'3,n  -  1 


™"im  ™na 


ln,n-\ 


Clo,    do 


(I., 


J2\    "'22    •     •     •     "B,n  - 1 

^'31      ^32      •      "     *      "3,71—1 


0"K\       Q-1V2    .      •       •        tt 


n,n-i 


=    "("I)2 


A         A 

\2n-3  tt!L  -      n 

A         A     * 

In  a  similar  way  we  prove  that 

X2/Xn  =  A12| Am    .    .    .,       Xn-ljXn  =  Aijn_1/Aln. 

iZe/tce  we  /«we 

3/t  :  £2  •    •    •    •    •  -^n  ~  -"-li  •  -"-is  •    •    •    •  ■  Alrt  J 

and,  fo/  'parity  of  reasoning, 

xl  :  x.2:  .  .    .    :  xn  =  Arl  :  Ar2 :  .   .   .    :  Am 
where  r  =  2,  =  3,  .  .   .,  =  n,  as  we  please.     In  other  words,  the  ratios 
of  the    variables    are  determinate,    but  their  actual   values   are  in- 
determinate, there  being  a  one-fold  infin  iiy  of  different  solutions. 


Exercises  XXV 
Solve  the  following  systems  : — 

(1.) 


x    y    z 


a  ,  v 


3  +  4  +  6-^'     i5  +  20+9-10,     2  +  10  +  4_4,J- 


xvr 


EXERCISES  XXV  377 


(2.)       2x  +  %y  +  \z  =  2§,     3x+2y+5z=S2,     4.z  +  3?/  +  2i  =  25. 
(3.)  '8x+l-2y+6-8z=l,     SSx-2-5y-Z'82z=-5, 

•Ola:-  -003y-  -301;=  -013  ; 
calculate  as,  y,  z  to  four  places  of  decimals. 

(4.)  x  +  y  +  z  =  26,     x-y  =  <±,     x-z=6. 

(5.)  If  (x+l)a  _    A     |     B:r+C 


(x  +  2)(ar  +  x+l)~x  +  2    a?  +  x+V 
determine  the  numerical  constants  A,  B,  C. 

(6.)  Find  a  linear  function  of  x  and  y,  which  shall  vanish  when  x=x', 
y  =  y',  and  also  when  x  =  x",  y  =  y",  and  which  shall  have  the  value  +1  when 
x  =  x'",  y  =  y'". 

(7.)  An  integral  function  of  x  of  the  2nd  degree  vanishes  when  x  =  2, 
and  when  x=3,  and  has  the  value  -  1  when  x=  -  2  ;  find  the  function. 

Solve  the  following  systems  : — 
(8.)  y  +  z  =  a,     z  +  x  =  b,     x  +  y  —  c. 

(9.)  JL+    *    =2a,    -^-  +  —  =  26,     -X  .+-y-,=2c. 

b  +  c     b-c  c+a     c-a  a+b     a- b 

(10.)  An  integral  function  of  a;  of  the  2nd  degree  takes  the  values  A,  B,  C, 
when  x  has  the  values  a,  b,  c  respectively  ;  find  the  function. 

Solve  the  following  systems  : — 

(11.)  bc{b  -  c)x  +  ca(c  -  a)y  +  ab(a  -  b)z=0, 

(a  +  b-c)x  +  (b  +  c-a)y+(c  +  a-b)z  =  a2  +  b2  +  c2, 

b2c2x  +  c2a2y  +  a2b2z  =  abc(bc  +  ea  +  ab). 

(12.)  If  _^_+^_  +  _f_=l> 

a  +  a     b+a     c  +  a 

x  y  z        . 


«  +  /3     6  +  (3     c  +  /3 

x  y  z        . 


then 


a  +  y     b  +  y     c+y 
I  V  ■  z - Iz£. 


(a  +  a)(a  +  p)2"(b  +  a)(b  +  p)2     (c  +  a)  (c  +  /3)2     (a  +  j8)  (b  +  p)  (c  +  /3) 
(13.)  aa;  +  fa/  +  c3  =  «  +  &  +  c, 

a3x-  +  fe22/  +  c^  =  (a  +  6  +  c)-, 
bcx  +  cay  +  abz  =  0. 
(14.)      ax  +  cy  +  bz  =  ex  +  by  +  az  =  bx  +  ay  +  cz  =  a3  +  b*  +  c3  -  Zabc. 

(15.)  lx  +  my  +  nz  =  mn  +  nl  +  hn, 

x  +  y  +  z=l  +  m  +  n, 
(m-n)x  +  (n-  l)y  +  (l-  m)z—0. 

(16.)  h-  +  my  +  nz  =  0, 

(ra  +  n)x  +  (7i  +  ?)y  +  {l  +  m)z=l  +  m  +  n, 
Px  +  m2y  +  n2z =p2. 

(17.)  Show  that  (b- c)x  +  by-cz  =  0,  (c-a)y  +  cz-ax=Q,  (a-b)z  +  ax-by 
=  0,  are  consistent. 


378  EXERCISES  XXV  chap. 

(18.)  Show  that  the  system  cy-bz=f,  ass  —  cz—g,  bx-ay  =  h  has  no  finite 
solution  unless  af+bg  +  ch  =  0,  in  which  case  it  has  an  infinite  number  of 
solutions. 

Find  a  symmetrical  form  for  the  indeterminate  solution  involving  one 
arbitrary  constant. 

Solve  the  following  systems  : — 

(19.)  3x-2y  +  3u  =  0,  x-y+z=0,  3y  +  Sz-2u  =  0,  x  +  2y  +  Bz  +  4u  =  8. 
(20.)  Uax=p-r,  by—p-s,  cz  =  r-s,  d{y  +  z)  =  s-q,  e(z  +  x)  =  q-r,f(X  +  y) 
=  q-p  +  g,  find  z  in  terms  of  a,  b,  c,  d,  e,f,  g. 
iz  +  x     3u  +  x     5v  +  x 


(21.)  2y  +  x  = 


3  4  8 

x  +  y  +  z  +  u  +  v  -  1  _  5x  +  ly  +  Bz  +  2u  +  v  +  2 


4  9 

(22.)  ax  +  by=l,  cx  +  dz=l,  ez+fu  =  l,  gu  +  hv=l,  z  +  y  +  z  +  u  +  v  =  0. 

(23.)  Prove  that,  with  a  certain  exception,  the  system  U  =  0,  V  =  0,  W  =  0, 

and  \XJ  +  fiY  +  vW  =  0,  \'U  +  /x'V  +  k'W  =  0,  X"U  +  /j."V  +  p"W  =  0  are  equivalent. 

(24.)  If  x=by  +  cz  +  du,      y  =  ax  +  cz  +  du, 

z  =  ax  +  by  +  du,    u  =  ax  +  by  +  cz, 

„  a  b  c  d 

then  -  +  i — -H 7 +-5 — =r=l- 

a+l     6+1     c+1     d+l 

(25.)  Show  that  the  system  ax  +  by  +  cz  +  d  =  0,  a'x  +  b'y  +  c'z  +  d'  =  0, 
a"x  +  b"y  +  c"z  +  d"  =  0  will  be  equivalent  to  only  two  equations  if  the  system 
ax  +  a'y  +  a"-Q,  bx  +  b'y  +  b"  =  Q,  cx  +  c'y  +  e"  =  Q,  dx  +  d'y  +  d"  —  0  be  con- 
sistent, that  is,  if 

b'c"  -  b"c'  _  b"c  -  be"  _  be'  -  b'c 
a'd"  -  a"d'  ~  a"d  -  ad"  ~~ad'-  a'd' 

Show  that  in  the  case  of  the  system 

7  x    y    z     .        x      y     z      . 

x  +  y  +  z  =  a  +  b  +  c,     -  +  f  +  -=l,      -v.  +  pj  +  -^  =  0, 
a     b     c  a6     b-f     c8 

the  above  two  conditions  reduce  to  one  only,  namely, 

bc  +  ca  +  ab  =  Q. 
(26.)  Show  that  the  three  equations 

x  =  A  +  A'u  +  A"v,     y  =  B  +  B'u  +  B"v,     z  =  C  +  C'tc  +  C"v, 
where  u  and  v  are  variable,  are  equivalent  to  a  single  linear  equation  con- 
necting x,  y,  z;  and  find  that  equation. 
(27.)  If  ax  +  by  +  cz  +  d—0,  show  that 


y=(£+qye-a)-£ 


where  p  and  q  are  arbitrary  constants. 


xvi  EQUATIONS  REDUCIBLE  TO  LINEAR  SYSTEMS  379 

(28. )  If  ax  +  by  +  cz  +  d  =  0,     a'x  +  b'y  +  c'z  +  d'  =  0,  show  that 
x=p(bc!  -  b'c)  +  \{b' - c')d  -(b-  c)d'}/{a(b' -  c')  +  b(c'-a')  +c(a'  -b')}, 
y=p(ca'  ~  c'«)  +{(e'-  a')d  -  (c  -  a)d'\/{a(b'  -  c')  +  b(c'  -  a')  +  c(a'  -&')}, 
z=p(ab'  -  a'b)  +  { (a'  -  b')d  -(a-  b)d'}/{a{b'  -  c')  +  b(c'  -  a')  +  c(a'  -b')}, 
where  p  is  an  arbitrary  constant. 

EXAMPLES    OF   EQUATIONS    WHOSE    SOLUTION    IS    EFFECTED    BY 
MEANS    OF   LINEAR    EQUATIONS. 

§  17.]  We  have  seen  in  chap.  xiv.  that  every  system  of 
algebraical  equations  can  be  reduced  to  a  system  of  rational 
integral  equations  such  that  every  solution  of  the  given  system 
will  be  a  solution  of  the  derived  system,  although  the  derived 
system  may  admit  of  solutions,  called  "  extraneous,"  which  do  not 
satisfy  the  original  system.  It  may  happen  that  the  derived 
system  is  linear,  or  that  it  can,  by  the  process  of  factorisation, 
be  replaced  by  equivalent  alternative  linear  systems.  In  such 
cases  all  we  have  to  do  is  to  solve  these  linear  systems,  and  then 
satisfy  ourselves,  either  by  substitution  or  by  examining  the 
reversibility  of  the  steps  of  the  process,  which,  if  any,  of  the 
solutions  obtained  are  extraneous.  The  student  should  now 
re-examine  the  examples  worked  out  in  chap,  xiv.,  find,  wher- 
ever he  can,  all  the  solutions  of  the  derived  equations,  and 
examine  their  admissibility  as  solutions  of  the  original  system. 
"We  give  two  more  instances  here. 

Example  1. 

•  +  ./;.„     .L2     1U=V{2(^  +  D}  («)■ 


(Positive  values  to  be  taken  for  all  tbe  square  roots.) 

If  we  rationalise  the  two  denominators  on  the  left,  we  deduce  from  (a)  the 
equivalent  equation, 

V{^-V0«2-i)}+V{*  +  V(^-i)}=V{2(^+i)}         (/s). 

From  (|3)  we  derive,  by  squaring  both  sides, 

2x  +  2\f{x2-(x°-~l)}  =2(a*  +  l), 
that  is,  2.e  +  2  =  2x3  +  2  (y). 

Now  (7)  is  equivalent  to  x3-x  =  0, 

that  is,  to  x(x  - 1)  (se+ 1) =0  (8). 

Again  (5)  is  equivalent  to  the  alternatives 
that  is  to  say,  its  solutions  are  #  =  0,  x=l,  x  = 


380 


EXAMPLES 


niAP. 


Since,  however,  the  step  from  (fi)  to  (7)  is  irreversible,  it  is  necessary  to 
examine  which  of  these  solutions  actually  satisfy  (a). 

Now  x  =  Ogives  \f  -  i+ \J -\-i=\j2, 

that  is  (see  chap,  xii.,  §  17,  Example  3), 

which  is  correct. 

Also,  £=1  obviously  satisfies  (a). 

But  x=  -  1  gives  2i  =  0,  which  is  not  true,  hence  x=  - 1  is  not  a  solution 
of  (a). 

Remark  that  x=  -\  is  a  solution  of  the  slightly  different  equation, 

V{z+V(z2-D}  "  Vte-VC*8-!)} =  ^'^ + 1)' 

Example  2. 

x2~y2  =  x-y,     2x+3y-l  =  0  (a). 

Since  the  first  of  these  equations  is  equivalent  to  (x~y)(x  +  y-l)  =  0,  the 
system  (a)  is  equivalent  to 

/       x-y  =  0,  and  2x  +  3i/-l=0N 

\x  +  y-l  =  0,  an.l  2z  +  32/-l  =  0, 

now  the  solution  of  x-y  =  0,  2x+By-l~0  is  a: =1/5,  2/ =  1/5  ;  and  the  solu- 
tion of  a:  +  2/-l  =  0,  2»+3y-l  =  0  is  a;=2,  y—  -1.  Hence  the  solutions  of 
(a)  are 


a; 

y 

1/5 
2 

1/5 
-1 

§  18.]  The  solution  of  linear  systems  is  sometimes  facilitated 
by  the  introduction  of  Auxiliary  Variables,  or,  as  it  is  sometimes 
put,  by  changing  the  variables.  This  artifice  sometimes  enables  us 
to  abridge  the  labour  of  solving  linear  systems,  and  occasionally 
to  use  methods  appropriate  to  linear  systems  in  solving  systems 
which  are  not  themselves  linear.    The  following  are  examples  : — 

Example  1. 

(a). 


{x-af  _x-2a-b 


{x  +  b'f     x  +  a  +  2b 

Let  x  +  b  =  z,  so  that  x  =  z-b  ;  and,  for  shortness,  let  c  =  a  +  b. 
Then  (a)  may  be  written 

(z-c)3_z-2c 
2s      ~  z  +  c 
From  (/3)  we  derive 

{z-c)\z  +  c)  =  z3^z-2c\ 


(£)■ 


xvi  CHANGE  OF  VARIABLES  381 

that  is, 

z*  -  2z»c+  2z<?  -  c4  =  24  -  2rV, 
which  is  equivalent  to 

2cs3-c4=0  (7). 

Now  (7)  has  the  unique  solution  z=e/2,  which  evidently  satisfies  (a) 
Hence  x  =  c/2  -  b,  that  is,  x  —  (a-b)j2,  is  the  only  finite  solution  of  (a). 

Example  2. 

a(x  +  y)  +  b(x-y)+c  =  0,     a'(x  +  y)  +  b'(x-y)  +  c'  =  0  (a). 

Let  £  =  x  +  ?/,  -q  =  x-y,  then  the  system  (a)  may  be  written 

a^  +  bij  +  c-0,     a's  +  b'T]  +  e'  =  Q  (a'). 

Now  (a')  is  a  linear  system  in  £  and  7;,  and  we  have,  by  §  4, 

be' -b'c  _ca'  -  c'a 

*~ab'-a'b'     V~ab'-a'b  &>' 

Replacing  f  and  7;  by  their  values,  we  have 

be' - b'c  ca' -c'a  ,   . 

X  +  y  =  aV^b'     X~y=W^Tb  iy)- 

From  (7),  by  first  adding  and  then  subtracting,  we  obtain 

_  be'  -  b'c  +  ca'  -  c'a         _  be'  -  b'c  -  ca'  +  c'a 
X~       2{ab'-a'b)      '     V~       2(ab'  -  a'b)       ' 
Example  3. 

cy  +  bz  —  az  +  cx  —  bx  +  ay  —  abc. 

Dividing  by  be,  by  ca,  and  by  ab,  we  may  write  the  given  system  in  the 
following  equivalent  form 

!+-:-  » 

x    y  ,  . 

a+l=C  W 

Now,  if  we  add  the  equations  (/3)  and  (7),  and  subtract  (a),  we  have 

(MM;+s)-(K)-»+-^ 

x 

that  is,  2-  —  b  +  c-a\ 

a 

,                                                            a(b  +  c-a) 
wlience  x=  — — . 

By  symmetry,  we  have 

y  =  b{c  +  a-b)/2,     z  =  c{a  +  b-c)/2. 

Here  we  virtually  regard  x/a,  yjb,  z/c  as  the  variables,  although  we  have 
not  taken  the  trouble  to  replace  them  by  new  letters. 


382 


EXAMPLES 


CHAP. 


Example  4. 


x—ay—b    z-  c 
r 


(a), 

03). 

have 

(7). 


(*)• 


P  1 

Ix  +  my  +  nz  =  d 

Represent  each  of  the  three  equal  functions  in  (a)  by  p.     Then  we 
(x-a)/p  =  p,     (y-b)/q  =  p,     (z-c)/r  =  p, 
which  are  equivalent  to 

x  =  a+pp,     y  =  b  +  qp,     z-c  +  rp 

Using  (7),  we  reduce  (j8)  to 

l(a  +pp)  +  m[b  +  qp)  +  n(c  +  rp)  =  d, 
for  which  we  obtain,  for  the  value  of  the  auxiliary  p, 

_d-la-  mb  -  nc 

lp  +  mq  +  nr 

From  (7)  and  (5)  we  have,  finally, 

d—la  —  mb  -  nc 

x  =  a  +  v  -7 , 

lp  +  mq  +  nr 

_m{aq  -  bp)  +  n(ar  -  cp)  -\-})d 
lp  +  mq  +  nr 

The  values  of  y  and  z  can  be  similarly  found,   or  they  can  be  written 
down  at  once  by  considering  the  symmetry  of  the  original  system. 

Example  5. 

x-2y  +  Zz  =  0  (a), 

2a;-3y  +  4t  =  0  Q3), 

ia?  +  By3  +  z3-xyz  =  216  (7). 

From  (a)  and  (/3)  we  have  (see  §  10  above) 

x/l=y/2=z/l=p,  say. 
Hence  &  =  P,     y  —  %P>     ~  =  /}  (5). 

By  means  of  (5)  we  deduce  from  (7) 

27 p3  =  216, 
which  is  equivalent  to  p*  =  8.  (e). 

Now  the  three  cube  roots  of  8  are  (see  chap,  xii.,  §  20,  Example  1) 

2,     2(  -  1  +  V3i).     2(  -  1  -  \/30- 
Hence  the  solutions  of  (e)  are 

P  =  2,     p=2(-l  +  V3i).     p=2(-l-V8i)- 

Hence,  by  (5),  we  obtain  the  three  following  solutions  of  (a),  (/3),  (7)  ; — 


X 

V 

z 

2 
-  1  +  \J%i 

- 1  -  V3i 

4 
2(  - 1  +  V30 

2(  -  1  -  V30 

2 

-  1  +  V3* 

-  1  -  V3i 

xvi  EXERCISES  XXVI  383 

Since,  by  chap.  xiv. ,  §  6,  the  system  in  question  has  only  three  solutions, 
we  have  obtained  the  complete  solution. 

N.B.  —  In  general,  if  Ui,  w2,  •  •  •,  «n-i  be  homogeneous  functions  of  the 
1st  degree  in  n  variables,  and  v  a  homogeneous  function  of  the  nth  degree  in 
the  same  variables,  the  solution  of  the  system 

!/l  =  0,      W2  =  0,      .    .    .,      «n-i  =  0,      v  =  0 

may  be  effected  by  solving  a  system  of  n  -  1  linear  equations  in  n  -  1  variables, 
and  then  extracting  an  »th  root.     See  in  this  connection  §  16  above. 

Example  6. 

ax-  +  by2  +  c  =  0,     a'x?  +  b'y-  +  c'=0. 

If  we  regard  x?  and  y'2  as  the  variables,  we  have  to  do  with  a  linear  system, 
and  we  obtain    as  heretofore, 

x2={bc'  -  b'c)/(ab'  -  a'b),     y"-  =  (ca'  -  c'a)/(ab'  -  a'b). 
Hence 

x=±\/{M  -b'c)/(ab'  -a'b),     y=±\/(ca' -c'a)/{ab' -a'b). 

Since  either  of  the  one  pair  of  double  signs  may  go  with  either  of  the  other 
pair,  we  thus  obtain  the  full  number  of  2  x  2  =  4  solutions. 

Example  7. 

ay  +  bx  +  cxy  =  0,     a'y  +  b'x  +  c'xy=0. 

These  two  equations  evidently  have  the  solution  x=0,  y  =  0. 
Setting  these  values  aside,  we  may  divide  each  of  the  two  equations  by 
xy.     We  thus  deduce  the  system 

a-+b-  +  c  =  0,     a'-  +  b'-  +  c'  =  0, 
x       y  x       y 

which  is  linear,  if  we  regard  1/x  and  1/y  as  the  variables.     Solving  from  this 
point  of  view,  we  obtain 

1  _  be'  -  b'c     1  _  ca'  -  c'a  _ 

x~ab'-a'b'    y~ab'-a'b  ' 
for  which  we  have 

x  =  {aV  -  a'b)/(bc'  -  b'c),     y  =  {aV  -  a'b)/(ca'  -  c'a\ 

"We  have  thus  found  two  out  of  the  four  solutions  of  the  given  system.    There 
are  no  more  finite  solutions. 


Exercises  XXVI. 
Solve  the  following  by  means  of  linear  systems  :- 


,,  >  \Jox  +\/b_  \/a  +  \/b 

\/ax  -  yjb  ~      \/b 

,„  ,  Va;+4?>i  _  \/x  +  27H 

\/x  +  3)i  ~   \Jx  +  n  ' 
(3.)  ^/(x  +  22)-s/(x+ 11)  =  1. 

(4.)  V*+V(*+3)  =  12/V(*  +  3). 


384  EXERCISES  XXVI 

(5.)  V(^  +  2)  +  V(«-2)  =  5/V(a-  +  2). 

(6.)  Vaj+V(a  +  /3)-V(a-J8)=V(*+2/3). 

(7. )  \J{x  +  q-  r)  +  V(a;  +  r-p)  +  s/(x  +p  -q)  =  0. 

*j{x-p)-y/P + V(»-p)+Vp=  ^(x  ~p)~ 

(9.)  z=v>2-aV(&3  +  a;2--a2)}+a. 

(10. )  V( V-'c+  V«)  +  V(V*  -  V«)  =  V(2 V®  +  2\/b)- 

(11.)  \?x+^/{B-^(2x  +  x2)}  =  ^3. 

(12-)  V^'V^)^'     V(*-2)=|v(*-3). 

(13.)        \/{a-x)-^J{y-x)  =  sJy,     \J{b-x)  +  *J(y-x)~s/y. 

1  17 

\H.)  Va;-\/2/=4.     ^-y^^g- 

(15.)  (x-a)2-(y-6)2  =  0,     (a;  -6)  (y  -«)  =  «(  26  -a). 

(16.)  a-2/  =  3,     z2-7/2  =  45. 

(17.)  xfy  =  a/b,     x^-if  —  d. 

(18.)  a;  +  ay  +  a22  +  a3ii  +  a4=0, 

x  +  by  +  bh  +  bsu  +  b*  =  0, 
x  +  cy  +  <?z  +  <?u  +  c4 = 0, 
re  +  tf  y  +  cPz  +  d?u  +  d4  =  0. 

(19.)  x+y+z=0,     ax  +  by  +  cz-Q, 

bcx  +  cay  +  abz  =  (b-  -  c2)  (c2  -  a2)  (a2  -  b"). 

mx  -ly  _  ny  -mz  _  Iz-nx         1 
^     "'  lm{a-b)     mn(b  —  c)    nl(c-a)    hnn' 


CHAP. 


(21.) 


mnx  +  nly  +  hnz  —  a  +  b  +  c. 
x  +  7/  —  z    y  +  z-x    z  +  x-y  , 

b+c  c+a  a+b 


(22.)        Z(&-c)a;=0;     2a(62-c2)x=0,     2a(b-c)x=JI(b-c). 

(23.)  2sc=l,     2te/(6-c)=0J     2.<:/(i2-c2)  =  0. 

(24.)  ax  +  k(y  +  z  +  ic)-0,     by  +  k(z  +  u  +  x)  =  0, 

cz  +  k(u  +  x  +  y)-0,     du  +  k(x  +  y  +  z)  =  0. 
(25.)       x  +  y-\-z—a,     y  +  z  +  u  —  b,     z  +  u  +  x  =  c,     u  +  x  +  y=d. 
(26.)  3/»-2/y=i,    4»+7y=l|ay. 

1  1    _12       ay  +  2s  +  3y  +  2 

1      '  sb+5    y  +  7     35'  rry+1 

<28->  w+J-11-  L+h16- 


XL  M2  \2  +  M2       X2_M2 

y-    x-  +  y2  a:2--y-    ar  +  y- 


(29)  -^-  +■    M      -1        -^--      "^  =1 


XVI 


EXERCISES  XXVI 


385 


(30.) 

(31.) 
(32.) 

(33.) 


a(b  -y)  +  b(a  -  x)  =  c(a  -x)(b-  y), 
a\b  -y)  +  b\a  -x)  =  c2{a  -x)(b-  y). 

b  «2  ft2 

+     .  ,  .     =1, —  + 


c+a+x     c  +  b  +  y 

b2     c2     ,       6 

—  +  ~i  —  1, 

I/2     z2 


c+a+x    c+b+y 


-a  +  b. 


+*2=]' 


a2     b2     , 
— +— =1, 

yz    zx 


z2 

-+— =1, 

2a;    xy 


a2    62     , 

-3  +  -  =  l. 
x2     y- 

^2/     2/2 


(34. )     ayz  -  bzx  -  cxy  =  -  ayz  +  bzx  -  cry  —  -  ayz  -  bzx  +  cxy  =  xyz. 

(35.)  Show  that     (l  +  lx)  (l  +  ay)  =  l  +  lz.     {l+mx)[\  +  by)  =  l+mz, 
(1  +  nx)  (1  +cy)  =  l  \-nz  are  not  consistent  unless 

(6  -  c)  ajl  +  {c-  a)b/m  +  (a-b)  cfn  =  0. 

If  this  condition  be  satisfied,   then  x  =  (c/n-b/m)/(b -  c) ;  and  particular 
solutions  for  y  and  z  are  y—  -  \ja,  z=  -  l/l. 


GRAPHICAL    DISCUSSION    OF    LINEAR   FUNCTIONS    OF   ONE   AND 
OF   TWO    VARIABLES. 

§  19.]  The  graph  of  a  linear  function  of  one    variable    is    a 
straight  line. 

Consider  the  function 
y  =  ax+  b.  To  find  the 
point  where  its  graph  cuts 


Y 

B 

p 

N 

sk 

o            i\ 

ft                X 

Fio.  1. 

OY,  that  is,  to  find  the 
point  for  which  X  =  0, 

we    have    to    measure 

OB  =  b     upwards     op 

downwards,    according 

as    b    is     positive    or 

negative  (Figs.  1  and  2).    Through  B  draw  a  line  parallel  to  the 

x-axis. 

Let  OM  represent  any  positive  value  of  x,  and  MP  the  cor- 
responding value  of  if. 

vol.  I  2  c 


Fio.  2. 


386 


THE  GRAPH  OF  CLV  +  b 


CHAP. 


By  the  equation  to  the  graph,  we  have  (y  -  b)]x  =  a.    Now,  since 
b  =  +  OB  =  +  MN  in  Fig.  1,  -  -  OB  =  -  MN  in  Fig.  2,  we  have 

y-b  =  PM  -  MN  -  PN  in  Fig.  1, 
y  -  b  =  PM  +  MN  =  PN  in  Fig.  2. 
Hence  we  have  in  both  cases 

PN_PN_y-6 

BN  ~  OM  ~  " 


=  a. 


In  other  words,  the  ratio  of  PN  to  BN  is  constant ;  hence, 
by  elementary  geometry,  the  locus  of  P  is  a  straight  line.  If  a 
be  positive,  then  PN  and  BN  must  have  the  same  sign,  and  the 
line  will  slope  upwards,  from  left  to  right,  as  in  Figs.  1  and  2  ; 
if  a  be  negative,  the  line  will  slope  downwards,  from  left  to 
right,  as  in  Figs.  3  and  4.  The  student  will  easily  complete  the 
discussion  by  considering  negative  values  of  x. 
Y  Y 


M         X 


Fig.  3. 


Fio.  4. 


§  20.]  So  long  as  the  graphic  line  is  not  parallel  to  the  axis 
of  x,  that  is,  so  long  as  a  =#  0,  it  will  meet  the  axis  in  one  point, 
A,  and  in  one  only.  In  analytical  language,  the  equation 
ax  +  b  =  0  has  one  root,  and  one  only. 

Also,  since  a  straight  line  has  no  turning  points,  a  linear 
function  can  have  no  turning  values.  In  other  words,  if  we 
increase  x  continuously  from  -  oo  to  +  oo  ,  ax  +  b  either  increases 
continuously  from  -  oo  to  +  oo ,  or  decreases  continuously  from 
+  oo  to  -  oo  ;  the  former  happens  when  a  is  positive,  the  latter 
when  a  is  negative. 

Since  ax  +  b  passes  only  once  through  every  value  between 


XVI 


THE  GRAPH  OF  OX  +  b  387 


+  oo  and  -  oo  ,  it  can  pass  only  once  through  the  value  0.    We  have 
thus  another  proof  that  the  equation  ax  +  b  =  0  has  only  one  root. 

A  purely  analytical  proof  that  ax  +  b  has  no  turning  values 
may  be  given  as  follows  : — Let  the  increment  of  x  be  h,  then  the 
increment  of  ax  +  b  is 

{a(x  +  h)  +  b)  -  {ax  +  b)  =  ah. 
Now  ah  is  independent  of  x,  and,  if  h  be  positive,  is  always  posi- 
tive or  always  negative,  according  as  a  is  positive  or  negative. 
Hence,  if  a  be  positive,  ax  +  b  always  increases  as  x  is  increased  ; 
and  if  a  be  negative,  ax  +  b  always  decreases  as  x  is  increased. 

§  21.]  We  may  investigate  graphically  the  condition  that  the 
two  functions  ax  +  b,  a'x  +  b'  shall  have  the  same  root ;  in  other 
words,  that  the  equations,  ax  +  b  =  0,  a'x  +  b'  =  0,  shall  be  con- 
sistent. Denote  ax  +  b  and  a'x  +  V  by  y  and  y'  respectively,  so 
that  the  equations  of  the  two  graphs 
are  y  =  ax  +  b,  y'  =  a'x  +  b'.  If  both 
functions  have  the  same  root,  the 
graphs  must  meet  OX  in  the  same 
point  A.  Now,  if  P'M  PM  be  ordi- 
nates  of  the  two  graphs  corresponding 
to  the  same  abscissa  OM,  and  if  the 
graphs  meet  OX  in  the  same  point  A, 
it  is  obvious  that  the  ratio  P'M/PM 
is  constant.     Conversely,  if  P'M/PM  FlQ- 5- 

is  constant,  then  P'M  must  vanish  when  PM  vanishes ;  that  is, 
the  graphs  must  meet  OX  in  the  same  point.  Hence  the  neces- 
sary and  sufficient  analytical  condition  is  that  (a'x  +  b')j(ax  +  b) 
shall  be  constant,  =  k  say.     In  other  words,  we  must  have 

a'x  +  V  =  k(ax  +  b). 
From  this  it  follows  that 

a'  =  ka,     V  =  kb, 
and  ab'  -  a'b  =  0. 

These  agree  with  the  results  obtained  above  in  §  2. 

§  22.]  By  means  of  the  graph  we  can  illustrate  various  limiting 
cases,  some  of  which  have  hitherto  been  excluded  from  con- 
sideration. 


388 


GRAPHICAL  DISCUSSION  OF  LIMITING  CASES 


CHAP. 


I.  Let  b  =  0,  a  4=  0.     In  this  case  OB  =  0,  and  B  coincides 
with  0 ;  that  is  to  say,  the  graph  passes  through  0  (see  Figs. 

Y 


Fig.  6.  Fig.  7. 

6    and   7).     Here  the  graph  meets  OX  at  0,  and  the  root  of 
ax  =  0  is  x  =  0,  as  it  should  be. 

II.  Let  b  =¥  0  and  a  =  0.  In  this  case  the  equation  to  the 
graph  is  y  =  b,  which  represents  a  line  parallel  to  the  a-axis  (see 
Figs.  8  and  9).     In  this  case  the  point  of  intersection  of  the 


Y 

B 

O 

X 

o 


Fig.  8. 


B 


Fig.  9. 


graph  with  OX  is  at  an  infinite  distance,  and  OA  =  oo .  If  we 
agree  that  the  solution  of  the  equation  ax  +  b  =  0  shall  in  all 
cases  be  x  —  -  b/a,  then,  when  b  4=  0,  a  =  0,  this  will  give  x  =  oo , 

in  agreement  with  the  conclusion  just 
derived  by  considering  the  graph. 
This  case  will  be  best  understood 
-^  by  approaching  it,  both  geometric- 
— r    ally    and    analytically,    as    a    limit. 
Let  us   suppose    that   6=  —  1,  and 
that    a  is   very  small,  =1/100000, 
say.     Then   the    graph  correspond- 
ing  to    y  =  x/l 00000  -  1     is    something    like    Fig.    10,    where 


B 


Fio.  10. 


:cvi  INFINITE  ROOT  389 

the  intersection  of  BL  with  the  axis  of  x  is  very  far  to  the  right 
of  0  ;  that  is  to  say,  BL  is  nearly  parallel  to  OX. 
On  the  other  hand,  the  equation 

1=0 


100000 

gives  x  =  100000,  a  very  large  value  of  x.  The  smaller  we 
make  a  the  more  nearly  will  BL  become  parallel  to  OX,  and  the 
greater  will  be  the  root  of  the  equation  ax  +  b  =  0. 

If,  therefore,  in  any  case  where  an  equation  of  the  1st  degree  in 
x  was  to  be  expected,  we  obtain  the  paradoxical  equation 

6  =  0, 
where  b  is  a  constant,  this  indicates  that  the  root  of  the  equation  has 
become  infinite. 

III.  If  a  =  0,  b  =  0,  the  equation  to  the  graph  becomes  y  -  0, 
which  represents  the  axis  of  x  itself.  The  graph  in  this  case 
coincides  with  OX,  and  its  point  of  intersection  with  OX  becomes 
indeterminate.  If  we  take  the  analytical  solution  of  ax  +  b  =  0 
to  be  x  =  -  bja  in  all  cases,  it  gives  us,  in  the  present  instance, 
x  =  0/0,  an  indeterminate  form,  as  it  ought  to  do,  in  accordance 
with  the  graphical  result. 

§  23.]  Tho  graphic  surface  of  a  linear  function  of  two  inde- 
pendent variables  x  and  y,  say  z  =  ax  +  by  +  c,  is  a  plane.  It 
would  not  be  difficult  to  prove  this,  but,  for  our  present  pur- 
poses, it  is  unnecessary  to  do  so.  We  shall  confine  ourselves  to 
a  discussion  of  the  contour  lines  of  the  function. 

The  contour  lines  of  the  function  z  =  ax  +  by  +  c  are  a  series  of 
parallel  straight  lines. 

For,  if  k  be  any  constant  value  of  z,  the  corresponding  con- 
tour line  has  for  its  equation  (see  chap,  xv.,  §  1 6) 

ax  +  by  +  c-k  (1). 

Now  (1)  is  equivalent  to 

/     a\        k-  c 

r-(-j>+T  <2)- 

But  (2),  as  we  have  seen  in  §  19  above,  represents  a  straight 
line,  which  meets  the  axes  of  x  and  y  in  A  and  B,  so  that 


390 


CONTOUR  LINES  OF  ClX  +  by  +  C 


CHAP. 


b  b   I  b        a 


Fig.  11. 


Let  h'  be  any  other  value  of  z,  then  the  equation  to  the  corre- 
sponding contour  line  is 

ax  +  by  +  c  =  k'  (3), 


el- 


s' 


a\       k'  -  c 

-yx+-b- 


(4). 


Hence,  if  this  second  contour  line  meet  the  axes  in  A'  and  B' 
respectively,  we  have 


OB'  = 


Hence 


Jc'-c 

IT' 
OA  = 
OB~ 


OA'  = 
OA' 


k'-c 


OB' 


which  proves  that  AB  is  parallel  to  A'B'. 

The  zero  contour  line  of  z  =  ax  +  by  +  c  is  given  by  the  equa- 
tion 

ax  +  by  +  c  =  0  (5). 

This  straight  line  divides  the  plane  XOY  into  two  regions,  such 
that  the  values  of  x  and  y  corresponding  to  any  point  in  one  of 
them  render  ax  +  by  +  c  positive,  and  the  values  of  x  and  y  cor- 
responding to  any  point  in  the  other  render  ax  +  by  +  c  negative. 
§  24.]  Let  us  consider  the  zero  contour  lines,  L  and  I/,  of 
two  linear  functions,  z  =  ax  +  by  +  c  and  z'  =  a'x  +  b'y  +  c'.  Since 
the  co-ordinates  of  every  point  on  L  satisfy  the  equation 

ax  +  by  +  c  =  0  (1), 


XVI  GRAPHIC  ILLUSTRATION  OF  INFINITE  SOLUTION  391 

and  the  co-ordinates  of  every  point  on  L'  satisfy  the  equation 

a'x  +  Vy  +  ti  =  0  (2), 

it  follows  that  the  co-ordinates  of  the  point  of  intersection  of  L 
and  L'  will  satisfy  both  (1)  and  (2);  in  other  words,  the  co- 
ordinates  of   the  intersection  will  be  a  solution  of  the  system 

(1),  (2). 

Now,  any  two  straight  lines  L  and  L'  in  the  same  plane  have 

one  and  only  one  finite  point  of  intersection,  provided  L  and  L' 

be   neither  parallel   nor  coincident.      Hence  we  infer  that  the 

linear  system  (1),  (2)  has  in  general  one  and  only  one  solution. 

It  remains  to  examine  the  two  exceptional  cases. 

I.  Let  L  and  L'  (Fig.  1 1 )  be  parallel,  and  let  them  meet  the 
axes  of  X  and  Y  in  A,  B  and  in  A',  B'  respectively.  In  this  case 
the  point  of  intersection  passes  to  an  infinite  distance,  and  both 
its  co-ordinates  become  infinite. 

The  necessary  and  sufficient  condition  that  L  and  L'  be 
parallel  is  OA/OB  =  OA'/OB'.  Now,  OA  =  -  c/a,  OB  =  -  c/b  ; 
and  OA'  =  -  c'fa',  OB'  =  -  c'/b'.  Hence  the  necessary  and  suffi- 
cient condition  for  parallelism  is  bja  -  b'/a',  that  is,  ab'  -  a'b  -  0. 

We  have  thus  fallen  upon  the  excepted  case  of  §§  4  and  5. 
If  we  assume  that  the  results  of  the  general  formulae  obtained 
for  the  case  ab'  -  a'b  #  0,  namely, 

be'  -  b'c  ca'  -  c'a 


x=zr> — I7i>     y 


n  i 


ab'  -  a'b'     J     ab'  -  a'b 

hold   also  when  ab'  -  a'b  =  0,   we  see  that  in  the   present  case 

neither  of  the  numerators  be'  -  b'c,  ca'  -  c'a,  can  vanish.     For  if, 

say,  be'  -  b'c  =  0,  then  -  c/b  =  -  c'/b',  that  is,  OB  =  OB' ;  and  the 

two  lines  AB,  A'B',  already  parallel,  would  coincide,  which  is  not 

supposed. 

It  follows,  then,  that 

be'  -  b'c  ca'  -  c'a 

Z  =  — ^-  =  00,      y  =  _ -—  =co: 

and  the  analytical  result  agrees  with  the  graphical. 

II.  Let  L  and  L'  be  coincident,  then  the  intersection  becomes 
indeterminate.     The  conditions  for  coincidence  are 


392  INDETERMINATE  SOLUTION  CHAP. 


OA  =  OA',     OB  =  OB', 

whence 

-c/a  =  -c'/a',      -c/b=  -c'/b'. 

These  give 

a      b      c 
a'  =  b'  =  c" 

which  again  give 

be'  -  b'c  =  0,     ca'  -  c'a  =  0,     ab'  -  a'b  =  0. 

We  thus  have  once  more  the  excepted  case  of  §§  4  and  5,  but 
this  time  with  the  additional  peculiarit\r  that  be'  -  b'c  =  0  and 
ca'  -  c'a  ~  0. 

If  we  assert  the  truth  of  the  general  analytical  solution  in 

this  case  also,  we  have 

0  0 

*  =  o'    ?/  =  0' 
that  is,  the  values  of  x  and  y  are  indeterminate,  as  they  ought  to 
be,  in  accordance  with  the  graphical  result. 

§  25.]  Since  three  straight  lines  taken  at  random  in  a  plane 
have  not  in  general  a  common  point  of  intersection,  it  follows 
that  the  three  equations, 

ax  +  by  +  c  =  0,     a'x  +  b'y  +  c'  =  0,     a"x  +  b"y  +  c"  =  0     (1), 
have  not  in  general  a  common  solution.     When  these  have  a 
common  solution  their  three  graphic  lines,  L,  L',  L",  will  have  a 
common  intersection.      We  found   the  analytical  condition  for 
this  to  be 

ab'c"  -  ab"c  +  be  a"  -  be" a  +  ca'b"  -  ca'b'  =  0  (2). 

In  our  investigation  of  this  condition  we  left  out  of  account  the 
cases  where  any  one  of  the  three  functions,  ab'  —  a'b,  a"b  -  ab", 
a'b"  -  a'b',  vanishes. 

We  propose  now  to  examine  graphically  the  excepted  cases. 

First,  we  remark  that  if  two  of  the  functions  vanish,  the 
third  will  also  vanish ;  so  that  we  need  only  consider  (I.)  the 
case  where  two  vanish,  (II.)  the  case  where  only  one  vanishes. 

I.  ab'  -  a'b  =  0,     a'b  -  ab"  =  0. 

This  involves  that  L  and  L'  are  parallel,  and  that  L  and  L"  are 
parallel ;  so  that  all  three,  L,  L',  L",  are  parallel ;  and  we  have, 
in  addition  to  the  two  given  conditions,  also  a'b"  -  a'b'  =  0. 


xvi  EXCEPTIONAL  SYSTEMS  OF  THREE  EQUATIONS  393 

Hence,  since  the  condition  (2)  may  be  written 

c(a'b"  -  a"b')  +  c'(a"b  -  ab")  +  c"(ab'  -  a'b)  =  0, 

it  appears  that  the  general  analytical  condition  for  a  common 
solution  is  satisfied. 

This  agrees  with  the  graphical  result,  for  three  parallel 
straight  lines  may  be  regarded  as  having  a  common  intersection 
at  infinity. 

In  the  present  case  is  of  course  included  the  two  cases  where 
two  of  the  lines  coincide,  or  all  three  coincide.  The  corre- 
sponding analytical  peculiarities  in  the  equations  will  be  obvious 
to  the  reader. 

II.  ab'  -  a'b  =  0. 

Here  two  of  the  graphic  lines,  L  and  L',  are  parallel,  and  the 
third,  L",  is  supposed  to  be  neither  coincident  with  nor  parallel 
to  either. 

Looking  at  the  matter  graphically,  we  see  that  in  this  case 
the  three  lines  cannot  have  a  common  intersection  unless  L  and 
L'  coincide,  that  is,  unless 

a'  =  ka,     b'  =  kb,     c'  =  kc, 

where  k  is  some  constant. 

Let  us  see  whether  the  condition  (2)  also  brings  out  this 
result,  as  it  ought  to  do. 

Since  ab'  -  a'b  =  0, 

we  have  -  =  _  =  /•  say. 

a     b  J 

Hence  a'  =  ka,     b'  =  kb. 

Now,  by  virtue  of  these  results,  (2)  reduces  to 

a"(be'  -  b'c)  +  b"(ca  -  c'a)  =  0, 

that  is,  to 

a"(bc'  -  kbc)  +  b"(cka  -  c'a)  =  0, 
that  is,  to 

(a"b  -  ab")  (c'  -  kc)  =  0, 

which  gives,  since  a"b  -  ab"  4=  0, 

c  -  kc  =  0, 
that  is,  c'  =  kc. 


394  EXERCISES  XXVII  chap. 

Hence  the  agreement  between  the  analysis  and  the  geometry  is 
complete.* 

§  26.]  It  would  lead  us  too  far  if  we  were  to  attempt  here 
to  take  up  the  graphical  discussion  of  linear  functions  of  three 
variables.  We  should  have,  in  fact,  to  go  into  a  discussion  of 
the  disposition  of  planes  and  lines  in  space  of  three  dimensions. 

We  consider  the  subject,  so  far  as  we  have  pursued  it,  an 
essential  part  of  the  algebraic  training  of  the  student.  It  will 
help  to  give  him  clear  ideas  regarding  the  generality  and 
coherency  of  analytical  expression,  and  will  enable  him  at  the 
same  time  to  grasp  the  fundamental  principles  of  the  application 
of  algebra  to  geometry.  The  two  sciences  mutually  illuminate 
each  other,  just  as  two  men  each  with  a  lantern  have  more  light 
when  they  walk  together  than  when  each  goes  a  separate  way. 

Exercises  XXVII. 

Draw  to  scale  the  graphs  of  the  following  linear  functions  of  x : — 
(1.)  y=x  +  l.  (4.)  y  =  2x  +  3. 

(2.)  y=-x+\.  (5.)  y=-\x-\. 

(3.)  y=-2E-l.  (6.)  y=-Z[x-\). 

(7.)  Draw  the  graphs  of  the  two  functions,  3a;  -5  and  5a; +7 ;  and  by 
n>eans  of  them  solve  the  equation  Sx-  5  =  5»+7. 

(8.)  Draw  to  scale  the  contour  lines  of  z  =  2x-3y  +  l,  corresponding  to 

g=-2,    z=-l,     z  =  0,     z=+l,     z=+2. 
(9. )  Draw  the  zero  contour  lines  of  z  =  5x  +  6y  -  3  and  z'  =  8x  -  9y + 1 ;  and 
by  means  of  them  solve  the  system 

5x  +  6y-3  =  0,     8a:-9y+l=0. 

*  It  may  be  well  to  warn  the  reader  explicitly  that  he  must  be  careful  to 
use  the  limiting  cases  which  we  have  now  introduced  into  the  theory  of 
equations  with  a  proper  regard  to  accompanying  circumstances.  Take,  for 
instance,  the  case  of  the  paradoxical  equation  b  =  0,  out  of  which  we  manu- 
factured a  linear  equation  by  writing  it  in  the  form  0x  +  &  =  0;  and  to  which, 
accordingly,  we  assigned  one  infinite  root.  Nothing  in  the  equation  itself 
prevents  us  from  converting  it  in  the  same  way  into  a  quadratic  equation, 
for  we  might  write  it  Ox2  +  Ox  +  b  =  0,  and  say  (see  chap,  xviii.,  §  5)  that  it 
has  two  infinite  roots.  Before  we  make  any  such  assertion  we  must  be  sure 
beforehand  whether  a  linear,  or  a  quadratic  or  other  equation  was,  generally 
speaking,  to  be  expected.  This  must,  of  course,  be  decided  by  the  circum- 
stances of  each  particular  case. 


XVI 


EXERCISES  XXVII  395 


Also  show  that  the  two  contour  lines  divide  the  plane  into  four  regions, 
such  that  in  two  of  them  (5x  +  6y-Z)  (8x-9y  +  l)  is  always  positive,  and  in 
the  other  two  the  same  function  is  always  negative. 

(10.)  Is  the  system 

3x-4y  +  2  =  0,     6x-8y  +  3  =  0,     x-$y+l=0 
consistent  or  inconsistent  ? 

(11.)  Determine  the  value  of  c  in  order  that  the  system 

2se+y-l=0,     4.r  +  2y  +  3  =  0,     {c  +  1)x  +  (c  +  2)y  +  5  =  Q 
may  be  consistent. 

(12.)  Prove  graphically  that,  if  ab'  -a'b  —  0,  then  the  infinite  values  of  x 
and  y,  which  constitute  the  solution  of 

ax  +  by  +  c-0,     a'x  +  b'y  +  c'  =  0, 
have  a  finite  ratio,  namely, 

x/y=(bc'  -  b'c)j(ca'  -  c'a). 

(13. )  If  (ax  +  by  +  c)/{a'x  +  b'y  +  c')  be  independent  of  x  and  y,  show  that 
ab'-a'b-O,     ca'-c'a  =  0,     bc'-b'c  =  0; 
and  that  two  of  these  conditions  are  sufficient. 

(14.)  Illustrate  graphically  the  reasoning  in  the  latter  part  of  §  5  of  the 
preceding  chapter. 

(15.)  Explain  graphically  the  leading  proposition  in  §  6. 


CHAPTER    XVII. 
Equations  of  the  Second  Degree. 

EQUATIONS    OF    THE    SECOND    DEGREE    IN    ONE   VARIABLE. 

§  1.]  Every  equation  of  the  2nd  degree  (Quadratic  Equation) 
in  one  variable,  can  be  reduced  to  an  equivalent  equation  of 
the  form 

ax2  +  bx  +  c  =  0  (1). 

Either  or  both  of  the  coefficients  b  and  c  may  vanish ;  but 
we  cannot  (except  as  a  limiting  case,  which  we  shall  consider 
presently)  suppose  a  =  0  without  reducing  the  degree  of  the 
equation. 

By  the  general  proposition  of  chap,  xii.,  §  23,  when  a,  b,  c 
are  given,  two  values  of  x  and  no  more  can  be  found  which 
shall  make  the  function  ax2  +  bx  +  c  vanish  ;  that  is,  the  equation 
(1)  has  always  two  roots  and  no  more.  The  roots  may  be  equal  or 
unequal,  real  or  imaginary,  according  to  circumstances. 

The  general  theory  of  the  solution  of  quadratic  equations  is 
thus  to  a  large  extent  already  in  our  hands.  It  happens, 
however,  that  the  formal  solution  of  a  quadratic  equation  is 
always  obtainable  ;  so  that  we  can  verify  the  general  proposition 
by  actually  finding  the  roots  as  closed  functions  of  the  coefficients 
a,  b,  c. 

§  2.]  We  consider  first  the  following  particular  cases  : — 
I.  c  =  0. 

The  equation  (1)  reduces  to 

ax2  +  bx  =  0, 


chap,  xvn         BOOTS  EQUAL  AND  OF  OPPOSITE  SIGN  397 

that  is,  since  a  4=  0, 

az(z  +  ]|)  =  0, 

which  is  equivalent  to 

a:  =  0 

x  +  -b  =  0 
a 

Hence  the  roots  are  x  =  0,  x  =  -  bfa. 

II.  &  =  0,    e  =  0. 
The  equation  (1)  now  reduces  to 

ax  x  x  =  0, 
which,  since  a  4  0,  is  equivalent  to 

{:::}■ 

Hence  the  roots  are  x  =  0,  x  =  0.     This  might  also  be  deduced 
from  I. 

Here  the  roots  are  equal.  "We  might  of  course  say  that  there 
is  only  one  root,  but  it  is  more  convenient,  in  order  to  maintain 
the  generality  of  the  proposition  regarding  the  number  of  the 
roots  of  an  integral  equation  of  the  nth  degree  in  one  variable, 
to  say  that  there  are  two  equal  roots. 

III.  b  =  0. 

The  equation  (1)  reduces  to 

ax2  +  c  =  0, 
that  is,  since  a  =t=  0,  to 

W-IX*-v/-;H 

which  is  equivalent  to 

V        a 


i 


--  =  o 


a      J 

Hence  the  roots  are  x=  -  s/(-c/a),  x=  +   ^(-cja);    that  is, 
the  roots  are  equal,  but  of  opposite  sign.     If  cja  be  negative, 


398 


GENERAL  CASE 


CHAP. 


both  roots  will  be  real ;  if  c/a  be  positive,  both  roots  will  be 
imaginary,  and  we  may  write  them  in  the  more  appropriate  form 
x  =  -  i  \/(cJa),  x  =  +  i  \/(cJa). 

§  3.]  The  general  case,  where  all  the  three  coefficients  are 
different  from  zero,  may  be  treated  in  various  ways  ;  but  a  little 
examination  will  show  the  student  that  all  the  methods  amount 
to  reducing  the  equation 


ax2  +  bx  +  c  =  0 


(1) 


to  an  equivalent  form,  a(x  +  A)2  +  jm  =  0,  which  is  treated  like  the 
particular  case  III.  of  last  paragraph. 

1st  Method. — The  most  direct  method  is  to  take  advantage 
of  the  identity  of  chap,  vii.,  §  5.     We  have 

f        -b  +  J(b2-Aac))   (        -b-  J(l/-iac)) 

hence  the  equation  (1)  is  equivalent  to 

b+  J(b2-4:ac))   (        -  b  -  y/(62  -  iac)} 

-6+  ^(b'-Aac) 


a-lx- 
that  is,  to 


x- 


\ 


X- 


-b 


2a 
sl(b2  -  Aac) 


2a 


=  0 


=  0 


>■ 


The     roots    of    (1)    are    therefore    {-b+  s/(b2 -  iac)}/2a,    and 
{-h-  J(b2-iac)}/2a. 

2nd  Method. — We  may  also  adopt  the   ordinary  process  of 
"  completing  the  square."     We  may  write  (1)  in  the  equivalent  form 


x  +  ~x  =  — 
a  a 


(2), 


and  render  the  left-hand  side  of  (2)  a  complete  square  by  adding 
(b/2a)2  to  both  sides.     We  thus  deduce  the  equivalent  equation 


\X  +  2a)  ~ia*     a' 


b2  -  4«c 
4a* 


(3). 


xvn  VARIOUS  METHODS  OF  SOLUTION  399 

The  equation  (3)  is  obviously  equivalent  to 

/  fb2-Aac\ 


b 

2a 


i 


b  I  (b2  -  iac 


x  +  —  =  - 


y. 


2a  V    \     4  a* 

from  which  we  deduce 

x  =  {  -  b  +  */(!?  -  iac)  }/2a,     x={-b-  K/(b2  -  iac) }  /2a, 

as  before. 

3rd  Method. — By  changing  the  variable,  we  can  always  make 

(1)  depend    on   an   equation   of  the   form   az2  +  d  =  0.     Let  us 

assume  that  x  =  z  +  h,  where  h  is  entirely  at  our  disposal,  and  z 

is  to  be  determined  by  means  of  the  derived  equation.     Then, 

by  (1),  we  have 

a(z  +  Kf  +  b(z  +  h)  +  c  =  0  (4). 

It  is  obvious  that  this  equation  is  equivalent  to  (1),  provided  x 
be  determined  in  terms  of  z  by  the  equation  x  =  z  +  h. 
Now  (4)  may  be  written 

az2  +  (2ah  +  b)z  +  (ah2  +  bh  +  c)  =  0  (5). 

Since  h  is  at  our  disposal,  we  may  so  determine  it  that  2ah 
+  b-0 ;    that  is,  we  may  put  h  =  -  bj2a.     The  equation  (5) 
then  becomes 

'♦■(-sM-a)--* 

that  is,  az2 —  =  0  (6). 

From  (6)  we  deduce  z  =  +   J(b2  -  iac)/2a,  z  =  -  ^(b2  -  4ac)/2a. 
Hence,  since  x  =  z  +  h  =  -  b/2a  +  z,  we  have 

x  =  {-b+  s/(b2-iac)}j2a,     x={-b-   >J(b2  -  iac)} /2a, 

as  before. 

In  solving  any  particular  equation  the  student  may  either 
quote  the  forms  {  -  b  ±  *J(b2  -  iac)} /2a,  which  give  the  roots  in 
all  cases,  and  substitute  the  values  which  a,  b,  c  happen  to  have 
in  the  particular  case,  or  he  may  work  through  the  process  of 


az 


400  DISCRIMINATION  OF  THE  ROOTS  chap. 

the  2nd  method  in  the  particular  case.  The  latter  alternative 
will  often  be  found  the  more  conducive  to  accuracy. 

§  4.]  In  distinguishing  the  various  cases  that  may  arise  when 
the  coefficients  a,  b,  c  are  real  rational  numbers,  we  have  merely 
to  repeat  the  discussion  of  chap,  vii.,  §  7,  on  the  nature  of  the 
factors  of  an  integral  quadratic  function. 

We  thus  see  that  the  roots  of 

ax*  +  bx  +  c  =  0, 

(1)  Will  be  real  and  unequal  if  b2  -  lac  be  positive. 

(2)  Will  be  real  and  equal  if  b2  -  lac  =  0. 

(3)  Will  be  two  conjugate  complex  numbers  if  b2  -  lac 
be  negative.  The  appropriate  expressions  in  this  case  are 
{-b  +  i  s/(lac  -  b2)}/2a,  {-b-i  ^(lac  -  b2)}j2a. 

(4)  The  roots  will  be  rational  if  b2  -  lac  be  positive  and  the 
square  of  a  rational  number. 

(5)  The  roots  Avill  be  conjugate  surds  of  the  form  A  ±  JB 
in  the  case  where  b1  -  lac  is  positive,  but  not  the  square  of  a 
rational  number. 

(6)  If  the  coefficients  a,  b,  c  be  rational  functions  of  any 
given  quantities  p,  q,  r,  s,  .  .  .  then  the  roots  will  or  will  not 
be  rational  functions  of  p,  q,  r,  s,  .  .  .  according  as  b2  -  lac  is  or 
is  not  the  square  of  a  rational  function  of  p,  q,  r,  .?,... 

It  should  be  noticed  that  the  conditions  given  as  characterising 
the  above  cases  are  not  only  sufficient  but  also  necessary. 

The  cases  where  a,  b,  c  are  either  irrational  real  numbers,  or 
complex  numbers  of  the  general  form  a  +  a'i,  are  not  of  sufficient 
importance  to  require  discussion  here. 

Example  1. 

2jt2-3.7-  =  0. 

By  inspection  we  see  that  the  roots  are  x  =  0,  x=3j2. 
Example  2. 

This  equation  is  equivalent  to  #2  +  4  =  0,  whose  roots  are  x  =  2i,  x=  -2i. 

Example  3. 

35x2-2u;-l  =  0. 
The  equation  is  equivalent  to 

2    _  1 
X'-35X~T$' 


XVII 


EXAMPLES,  EXERCISES  XXVIII 


401 


that  is,  to 

Henca 

Hence 


(-& 


L\2    _1_      1__36_ 
:352  +  35~352' 


1  -+1 

*    35        35" 

1±6 
W 


x=- 


The  roots  are,  therefore,  + 1/5  and  - 1/7. 

Example  4. 

a?!-2a!-2=0. 

The  roots  are  1  +  v'3  and  1  -  \/3. 

Example  5. 

3a;2  +  2ix  +  48  =  0. 

The  given  equation  is  equivalent  to 

a?  +  8^  +  16  =  0, 
that  is,  to  (a;  +  4)2  =  0. 

Hence  x=  -  4±0 ;  that  is  to  say,  the  two  roots  are  each  equal  to  -  4, 

Example  6. 

a;2-4a;+7  =  0. 
This  is  equivalent  to 

a;2-4a;  +  4=-3) 

that  is,  to  (as-2)a=3**. 

Hence  the  roots  are  2  +  \jZi,  2  -  \JZi. 

Example  7. 

a;2  -  2{p  +  qfx  +  2p*  + 1 Iff  +  2qi  =  0. 

This  equation  is  equivalent  to 

{x  -  (p  +  q)*\  9=  (p +q)*  -  2p*  -  12pY  -  2q*, 
=  -(p-q)\ 
=  {p-q)H\ 

Hence  the  roots  are  (p  +  qf  +  {p-qfi,  (p  +  q^-ip-qfi- 


Exercises  XXVIII. 


(1.)  a:2  +  a;  =  0. 

(2.) 

(3.)  (a:+l)(as-l)+l=0. 

(4.) 

(5.)  (a;-l)2  +  (a--2)2  =  0. 

(6.) 

(7.)  p(x  +  a)2-q(x  +  p)*  =  0. 

(8.) 

(9.)  2a,-2  +  3a:+5  =  3a;2  +  4a:  +  l. 

(10.) 

(11.)  255a;2- 431a: +  182  =  0. 

(12.) 

(13.)  x*-  22a;  +170  =  0. 

(14.) 

(15.)  a?  +  102a;  +  2597  =  0. 

(16.) 

(17.)  a?  +  6\/7*  +  55  =  0. 

(18.) 

(19. )  a;2  +  (23  +  12i)x  +  97  + 137*'  =  0. 

(20.) 

VOL.  I 

(2a:-l)(3aj-2)  =  0. 

(a:-l)2  +  3(a;-l)  =  0. 
.3(x-l)2-2(a:-2)2=0. 
{px  +  q)2+{qx+p)2  =  0. 
ar>  +  8a:2  +  16a:-l  =  (a:  +  3)3. 
4a,-2  -40a;  +  107  =  0. 
a;2 -201a; +  200  =  0. 
a;2  -4a;  -2597  =  0. 
a.-2-2(l  +  V2)a;  +  2V2  =  0. 
a.-2-(8-2i)a:=38i-31. 
2  D 


402  EQUATIONS  REDUCIBLE  TO  QUADRATICS  chap. 

(21.)  («-l)(aj-2)  +  (aj-l)(a!-3)  +  (a!-2)(aJ-3)=0. 

(22.)  (x-l)3  +  {x-l)2(x-2)-2{x  +  l)3  =  0. 

(23.)  (x-i)(x-i)  +  (x-i)(x-l)  =  0. 

(24.)  {x-a)2  +  (x-b)2  =  a2  +  b2.  (25.)  a2  +  4aa;=(&-c)2  +  4(&c-a2). 

(26.)  x2+(b-c)x=a?  +  bc  +  ca  +  ab. 


w^i-K^+y|> 


(28.)  (a  +  b)(abx2-2)  =  (a2  +  b2)x. 

(29.)  (a-b)x2-(a2  +  ab  +  b2)x  +  ab(2a+b)  =  0. 

(30.)  (c  +  «-2Z>);z2+(a  +  &-2c),?+(&  +  c-2«)  =  0. 

(31. )  {a2  -  ax  +  c2)  (a2  +  ax  +  c2)  =  a4  +  aV  +  c4. 

(32. )  x-  -  2(a2  +  b2  +  c2)x  +  ai  +  bi  +  c4  +  b2c2  +  <?a*  +  a2b2  =  2abc(a  +  b  +  c). 

(33.)  (b-c){x-a)3+{c-a)(x-b)3  +  (a-b){x-c)3  =  0. 

(34.)  Evaluate  V(7  +  V(7  + V(7  +  V(7...  ad  oo...  )))). 


EQUATIONS    "WHOSE    SOLUTION    CAN    BE   EFFECTED    BY    MEANS    OF 

QUADRATIC    EQUATIONS. 

§  5.]  Reduction  by  Factorisation. — If  we  know  one  root  of  an 
integral  equation 

/(a)  =  0  (1), 

say  x  =  a,  then,  by  the  remainder  theorem,  we  know  that  f(x)  = 
(x  -  a)cj>(x),  where  <j>(x)  is  lower  in  degree  by  one  than  f(x). 
Hence  (1)  is  equivalent  to 

(2). 


tip) 

The  solution  of  (1)  now  depends  on  the  solution  of  <f>(x)  =  0.  It 
may  happen  that  <f>(x)  =  0  is  a  quadratic  equation,  in  which  case 
it  may  be  solved  as  usual ;  or,  if  not,  Ave  may  be  able  to  reduce 
the  equation  <f>(x)  —  0  by  guessing  another  root ;  and  so  on. 

Example  1. 

To  find  the  cube  roots  of  -  1. 

Let  x  be  any  cube  root  of  - 1,  then,  by  the  definition  of  a  cube  root,  we 
must  have  x3  —  - 1.     We  have  therefore  to  solve  the  equation 

3^  +  1  =  0. 

We  know  one  root  of  this  equation,  namely,  x=  -1 ;  the  equation,  in  fact,  is 

equivalent  to 

(x  +  l)(x2-x+l)  =  0, 

that  is,  to  {    .     X  +  }  =  °A. 

{  x2  -  x  +  1  =  0  J 

The  quadratic  x2-x  +  l  =  0,  solved  as  usual,  gives  a;=(l±t\/3)/2. 


xvii  INTEGKALISATION  AND  RATIONALISATION  403 

Hence  the  three  cube  roots  of  -  1  are  - 1,  (1  +  i\/S)/2,  (1  -  i\jZ)j2,  which 
agrees  with  the  result  already  obtained  in  chap.  xii.  by  means  of  Demoivre's 
Theorem. 

Example  2. 

This  equation  is  obviously  satisfied  by  x=l.     Hence  it  is  equivalent  to 

{7x2-6x-3)(x-l)  =  0. 
The  roots  of  the  quadratic  7x2-  6x-  3  =  0  are  (3±V30)/7.     Hence  the  three 
roots  of  the  original  cubic  are  1,  (3  +  V30)/7,  (3  -  V3lr)/7. 

It  may  happen  that  we  are  able  by  some  artifice  to  throw  an 

integral  equation  into  the  form 

PQR  .   .  .  =  0, 

where  P,  Q,  R,  .   .  .   are  all  integral  functions  of  x  of  the  2nd 

degree.     The  roots  of  the  equation  in  question  are  then  found 

by  solving  the  quadratics 

P  =  0,     Q=0,     R  =  0,      ... 

Example  3. 

p(ax2  +  bx  +  r)2  -  q(dx2  +  ex  +/  )2  =  0. 

This  equation  is  obviously  equivalent  to 

{^p(ax2  +  bx  +  c)  +  \Jq{dx2  +  ex+f)}  {^p(ax*+bx  +  c)  -  *Jq(dx2  +  ex+f)}  =  0. 

Hence  its  roots  are  the  four  roots  of  the  two  quadratics 

(a  sjp  +  dsjq)x2  +  (b\Jp  +  c\Jq)  x  +  {csjp  +f\Jq)  =  0, 
(a  \/p  -  d\/q)x2  +  {b\Jp  -  esjq)  x  +  (c\/p  -f\/q)  =  0, 
which  can  be  solved  in  the  usual  way. 

§  6.]  Integralisation  and  Rationalisation. — We  have  seen  in 
chap.  xiv.  that  every  algebraical  equation  can  be  reduced  to  an 
integral  equation,  which  will  be  satisfied  by  all  the  finite  roots  of 
the  given  equation,  but  some  of  whose  roots  may  happen  to  be 
extraneous  to  the  given  equation.  The  student  should  recur  to 
the  principles  of  chap,  xiv.,  and  work  out  the  full  solutions  of 
as  many  of  the  exercises  of  that  chapter  as  he  can.  In  the  exer- 
cises that  follow  in  the  present  chapter  particular  attention 
should  be  paid  to  the  distinction  between  solutions  which  are 
and  solutions  which  are  not  extraneous  to  the  given  equation. 

The  following  additional  examples  will  serve  to  illustrate  the 
point  just  alluded  to,  and  to  exemplify  some  of  the  artifices  that 
are  used  in  the  reduction  of  equations  having  special  peculiarities. 


404  EXAMPLES  chap. 

Example  1. 

1       =0. 


a-  b 

If  we  combine  the  first  and  last  terms,  and  also  the  two  middle  terms,  we 
derive  the  equivalent  equation 

2x  2x  _ 

>+.»    ,_     ra=0- 


x2-[a  +  bf    x'-{a-bf 
If  we  now  multiply  by  {x~  -  (a  +  b)2}  {x2  -(a-  b)2}  we  deduce  the  equation 

2x{2x2-2(a2  +  b2)}=0; 
and  it  may  be  that  we  introduce  extraneous  solutions,  since  the  multiplier 
used  is  a  function  of  x. 

The  equation  last  derived  is  equivalent  to 

\x2-{a2  +  b-)  =  0j- 
Hence  the  roots  of  the  last  derived  equation  are  0,  +  \/{a2  +  b2),  -  \/{a2  +  b2). 
Now,  the  roots,  if  any,  introduced  by  the  factor  \x2  -(a  +  b)2)  {x2  -(a-  b)2} 
must  be  ±(a  +  b)  or  ±(a-b).     Hence  none  of  the  three  roots  obtained  from 
the  last  derived  equation  are,  in  the  present  case,  extraneous. 

Example  2. 

a-x  a  +  x  .  i  \ 

\/a+\J{a-x)     \/a+^/{a  +  x) 
If  we  rationalise  the  denominators  on  the  left,  we  have 

(g-ar){Va-V(a-g)}  +  {a  +  x){^a-  s/ja  +  x)}  _    , 

x  -x  '  '' 

From  (^),  after  multiplying  both  sides  by  x,  and  transposing  all  the  terms 
that  are  rational  in  x,  we  obtain 

[a + as)t  -(«-«)?= 3a;  \/a  (7). 

From  (7),  by  squaring  and  transposing,  we  deduce 

2a3-3ax2  =  2(a2-x2)i  (5). 

From  (5),  by  squaring  and  transposing,  we  have  finally  the  integral  equation 

(4^-3«2)a^=0  (e). 

The  roots  of  (e)  are  0  (repeated  four  times,  but  that  does  not  concern  us  so  far 
as  the  original  irrational  equation  *  (a)  is  concerned)  and  ±a\/3/2. 

It  is  at  once  obvious  that  x  =  0  is  a  root  of  (a). 

If  we  observe  that  s/(l±s/Z/2)  =  (s/3±l)/2,  we  see  that  ±«V3/2  are  roots 

of  (a),  provided 

2:pV3  2±V3 

xl  +  \/3     2±l  +  \/3       ' 


that  is,  provided 


2^1  +  V^     2±l  +  \/3 
2- V3  ,  2  +  V3  = 

l  +  Vs^s  +  vs     ' 


which  is  not  true. 

Hence  the  only  root  of  (a)  is  x  =  0. 

*  For  we  have  established  no  theory  regarding  the  number  of  the  roots  of 
an  irrational  equation  as  such. 


xvil  EXAMPLES  405 

Example  3. 

V(ffl  +  a:)  \/(a-x) 

V«  +  V(re  +  x)     Va  _  V(«  ~  a:) 

By  a  process  almost  identical  with  that  followed  in  last  example,  we  deduce 

from  (a)  the  equation 

4z*-3ah?=0  (/3). 

The  roots  of  (/3)  are  0,  and  ±a\/3/2  ;  but  it  will  be  found  that  none  of  these 
satisfy  the  original  equation  (a). 

Example  4. 

V(2a;2  -  4aT+ 1)+  V(*'2  -5x+2)=  V(2a?  -  2a;  +  3)  +  V(«2  -  3a:  +  4)     (a). 
The  given  equation  is  equivalent  to 

V(2a?  -  4«+ 1)  -  V(>»2  ~  3a:  +  4)  =  s/(2x2  -  2x  +  3)  -  V(a*  -  Bas  +  2). 
From  this  last,  by  squaring,  we  deduce 


3a;2  -  7x  +  5  -  2V(2a:2  -  4a;  + 1)  (a;2  -  3a;  +  4) 

=  3a;2  -  7x  +  5  -  2V(2ar!  -  2a;  +  3)  (a-2  -  5a;  +  2), 
which  is  equivalent  to 

V(2a,4  -  10a?  +  21a?  -  19a;  +  4)  =  yj(2x*  -  12a?  +  17a?  -  19a-  +  6)       (j8). 
From  (/3),  by  squaring  and  transposing  and  rejecting  the  factor  2,  we  deduce 

a?+2a?-l=Q  (7). 

One  root  of  (7)  is  x  —  -  1,  and  (7)  is  equivalent  to 

(«+l)(aj2+a!-l)=0. 
Hence  the  roots  of  (7)  are  -  1  and  (  -  1  ±\/5)/2. 

Now  x=  -1  obviously  satisfies  (a).  We  can  show  that  the  other  two 
roots  of  (7)  are  extraneous  to  (a)  ;  for,  if  x  have  either  of  the  values 
(-l±\/5)/2,  then  x*  +  x-l  =  0,  therefore  a;2=  -a;  +  l.  Using  this  value  of 
a;2,  we  reduce  (a)  to  \/{  -  6x  +  3)=\J{  -  4a; +  5).  This  last  equation  involves 
the  truth  of  the  equation  -  6a;  +  3=  -  4ar+  5,  which  is  satisfied  by  x=  -  1,  and 
not  by  either  of  the  values  x—  (  -  1  ±  \J5)/2. 

N.B. — An  interesting  point  in  this  example  is  the  way  the  terms  of  (a) 
are  disposed  before  we  square  for  the  first  time. 


Example  5. 


1  -  \/(l  -  a;2)  __  27V(l+aQ  +  V(l-g)  (a)< 


1  +  V(l  - *2)  V(l  +*)  -  V(i  - x) 
Multiply  the  numerator  and  denominator  on  the  left  by  1  -  \/(l  -a:2),  and  the 
numerator  and  denominator  on  the  right  by  y/(l+x)  -  \/(l  -x),  and  we  ob- 
tain the  equivalent  equation 

(i_vr^)2_        x 

a?  -  1-V(I-^2)' 

Multiply  both  sides  of  the  last  equation  by  a-^l  -  Vl  -  x%  and  we  deduce 

{l-sj(l-x*)}3  =  27x3  08). 


406 


EXERCISES  XXIX,  XXX 


CHAP. 


If  1,  w,  u2  (see  chap,  xii.,  §  20)  be  the  three  cube  roots  of  4-1,  then  (/3)  is 
equivalent  to 

1-  \/(l-x2)  =  3x 

l-V(l-ar»)=3«a!  ! 

l-^/(l-x2)  =  Z<Jixj 
By  rationalisation  we  deduce  from  (7)  the  three  integral  equations 

10x2-6.r  =  (f 
{l  +  9w2)a?-6wx  =  0  -  (5). 

^l+QoO^-ear.x^O, 
The  roots  of  these  equations  (5)  are  0,  3/5  ;  0,  6w/(l  +9w2)  ;  0,  6w2/(l  +9w). 

The  student  will  have  no  difficulty  in  settling  which  of  them  satisfy  the 
original  equation  (a). 

Exercises  XXIX. 

(1.)    1X'6-1  =  (X2  +  |)2(X2-1). 

(2.)  x3-(a  +  b  +  c)x2-{a~  +  b-  +  c--bc-ca-ab)x  +  a3  +  P+c$-Babc=0. 

(3.)  x4- 40a;  +  39  =  0. 

(4.)  xA  +  2(a-2)xs+(a-2)n-x2  +  2a2(a-2)x  +  ai=0. 

(5.)  2a3 -a2 -2a; -8  =  0.  (6.)  ax3  +  x  +  a  +  l  =  0. 

(7.)  ar*-3a^  +  4a;2-3a;  +  l  =  0. 


x2  .  x  .  1     P    p2 


p     p2    p3     X2      X 
(9.)  a;4-6a,-3  +  10a^-8x  +  16  =  0.  (10.)  xi-6  =  5x(x2-x-l). 

(11.)  (x2  +  6x  +  9) (x2  +  8x  + 1 6)  =  (a;2  +  4a;  +  4) (x2-  12a;  +  36). 


(1.)  ax  =  2(l  +  l 


Exercises  XXX. 


1     !\ 
x  +  --T   . 
a     0/ 


(2.) 


b+x    a+x 


,n,2x2-x-l     2a?-3a;-8     8a;2-8 
(3.)  -ST-+- 


a;-2 


a;-3 


2a; -3 


9a; +  5     4a;-2_12a;  +  3     4a;  +  3     11 
(    '      12        7x-l_     16         7z  +  9     48' 


(5.)  a;-3  = 


a? -27 

a^  +  8  ' 


,.  .   ax  +  b    ax  +  b     2ax  +  d     b 

(6°  -r+<^+b=~2r-+-c 

ax  +  b     bx  +  a_(a  +  b)(x  +  2) 
cx  +  b     cx  +  a 


(8.)  |5±5+|"±»-5±? 

x - a      x-b    x-c 


cx  +  a  +  b 

n  r 


.,+ 


bx 


lex 


,n  .  x-a    x-b        b 

9.)  -=—  + =  - 

b  a       x-a    x-b 


a?-a2^x2-b2    x*-c2 
a 


XVII 


EXERCISES  XXX,  XXXI  407 


a-c       b-c      a  +  b-lc 


^l0''  2b  +  x  +  2a  +  x     a  +  b  +  :>:' 

x  +  a    x-a_x2  +  a?    32-«2 

(1L)  x~^a  +  x  +  a~xli-a-  +  x2  +  a^ 
(x  -  a) (x-b) _  (x  -c)(x-  d) 


(12.) 


x-a—b  x- c—d 

a  +  2x 


/gt  +  ax  +  x- 
^  \a2-ax  +  x' 


a-2x 

(      '       2z2  +  2a:  +  3  x  +  1 

x  74 


(15')  a2 -2a -15     cc2  +  2x-35     a;2  +  10a;  +  2l' 

2x+3a     2x-Sa_a  +  b    a-b 
^      '  2x-3a  +  2x+Sa~a-b     a  +  b' 

K  '''  (x-b){x-c)     (x-c){x-a)     {x-a){x-b) 


(1.) 


Exercises  XXXI. 

x+\/x_x(x-l) 
x-  \/x  4 


^  v^T2)=^+2)  +  2^- 

(4.)  (a2  +  bx)s/{a?  +  c-)  =  (a2  +  be) V(a2  +  *!). 

(5.)  6xtx-l)-2s/{Z{x-2)(x  +  l)-2(x-5)}=±{x+Z). 

(6. )  Viz  +  Vz)  +  V(*  -  V*)  =  aV*/V(*  +  Va). 

(7.)  (l+x)V(l-a;2)  +  (a:-1)  =  0- 

(8.)  (aj-8)M^-6*  +  86)  =  (aj-4)M^-8»  +  64). 

(9. )  (2a  -  a)/ V(«*  ~  «*  +  «2)  =  (2a; "  &V  V(-*2  "  hx  +  ^ 

wV(.4.H-y^)-y(£iO}- 

(ii.)  vV2 + 6a + 1)  -  V(3'2 + to + 4) + V(*2 + 6a" -  s)=o. 

(12.)  V(ff2  +  &x)  +  V(&2  +  a*)  =  3(«  +  &). 

(13.)  V {a(te- a2)/6}  +  V{ft(«* -  b')la)  =a ~  h- 

(14.)  ^/(a  +  x)  +  s/{b  +  x)  =  2s/(a  +  b  +  x). 

Consider  more  especially  the  case  where  a=b. 
(15.)  \/(x  +  i)-^(x-i)  =  ^(x-l). 
(16.)  2xs/{xi  +  a'2)  +  2x'sJ{xi  +  Vi)  =  a?-b-. 
(17. )  V(*2  +  4x  +  3)  -  V(*2  +  3*  +  2) = 2(x+ 1). 

Two  solutions,  x-  -  1  and  another. 

(18. )  a2  +  a2  +  V(-<-'4  +  «4)  -  2* V  {■<■"  +  V(*-4  +  «4) }  • 


408  CHANGE  OF  VARIABLE  chaP. 

(19.)  x=\J{ax  +  x2-a\/(ax  +  x2)}. 

(oqn  7  12  1  6 

y~  ''  V(a:-6)  +  4     V(«-6)  +  9     V(a'-6)-4  +  V(a;-6)-9_ 
(21.)  V(«2  +  a-'2)  +  V(2a»)  =  V(«2  +  3oaj)  +  VC*2  +  So*). 
(22.j_._l 1 


\/(a  +  x)-  \Ja     \Ja  +  \/(a  +  x)     \/(a  +  x)  -  \/{a - x) 

(23. )  V«  +  V(«  +  «)  -  V(«  - *)  =  ^/(«2  -  *2)- 

(24. )  BiV(a+a!)  +  »  V(« -«)=  V(™2  +  «2) #(«* - *2)- 

(25. )  Rationalise  and  solve  2,\J{x -b-c)  =  \Jx. 

(26.)  V{(^3  +  a2)(^  +  &2)}+x{V(a;2  +  a2)-\/(a;2  +  &2)}=:^2  +  a;2- 
(27.)  a  +  (a;  +  J)V{^2  +  «2)/(a;2  +  i2)}=6  +  (a:  +  a)v'{(a;2  +  i2)/(a;2  +  a2)}. 

§  7.]  Reduction  of  Equations  by  change  of  Variable.    If  we  have 
an  equation  which  is  reducible  to  the  form 

{_W  +*{/(*)} +2«0  (a), 

then,  if  we  put  £  =/(%),  we  have  the  quadratic  equation 

to    determine   £.      Solving    (/3),    we    obtain    for   £   the    values 
{  -p  ±  J(p2  -  4q)}/2.     Hence  (a)  is  equivalent  to 


< 


-p-J(p2-4q) 


m 


1 


(?)• 


If  the  function  f{x)  be  of  the  1st  or  2nd  degree  in  x,  the 
equations  (y)  can  be  solved  at  once  ;  and  all  the  roots  obtained 
will  be  roots  of  (a). 

Even  when  the  equations  (y)  are  not,  as  they  stand,  linear 
or  quadratic  equations,  it  may  happen  that  they  are  reducible  to 
such,  or  that  solutions  can  in  some  way  be  obtained,  and  thus 
one  or  more  solutions  will  be  found  for  the  original  equation  (a). 

In  practice  it  is  unnecessary  to  actually  introduce  the 
auxiliary  variable  £.  We  should  simply  speak  of  (a)  as  a 
quadratic  in  f(x),  and  proceed  to  solve  for  f(x)  accordingly. 

Example  1. 

<_*>/- +  _»*'- -12=0. 

We  may  write  this  equation  in  the  form 

(a5*-,.)_+4(_:_'/e)_12__0. 


XVII 


EXAMPLES  409 


It  may  therefore  be  regarded  as  a  quadratic  equation  in  o'J'i.    Solving,  we  find 

xp;,j=+2,     xi>''J=-6. 
From  the  first  of  these  we  have 

.rP  =  2'l. 

Hence,  if  1,  w,  or,  .  .  .,  w^-1  be  the  pth  roots  of  +1,  we  find  the  following  p 

values  for  x  : — 

2t'i\     oj2">'p,     w2-2i'p,     .   .   .,     wP-12i'p. 

In  like  manner,  from  xp:'<  =  -  6,  we  obtain,  if  q  be  even,  the  p  values 

&P,     w6«*      w26i'p,     .  .  .,     w*-16*'8; 

and,  if  q  be  odd,  the  p  values 

w'6«*.     w'36**s     w'56^(     .   .  .,     uPP-i&l*, 

where  &>',  w'3,  .  .   . ,  w'2^-1  are  the  ^?th  roots  of  -  1 . 

Example  2. 

x2  +  3  =  2  V(^'2  ~  2a  +  2)  +  2z. 

This  equation  may  be  written 

a?-2sB+2-2VO^-2a!+2)  +  l=0  ; 

that  is, 

{ VC-e2  -  2a  +  2) } 2  -  2  { VC*3  -  2x  +  2)}  + 1  =0, 

which  is  a  quadratic  in  \f(3?  -2x  +  2). 
Solving  this  quadratic  we  have 

x/(x2-2x  +  2)  =  l. 
Whence  ^-2*  + 2  =  1, 

that  is,  (x--l)2  =  0. 

The  roots  of  this  last  equation  are  1,  1,  and  x=l  satisfies  the  original  equation. 

Example  3. 

22*  _  3-2*4-2  +  32  =  0. 

We  may  write  this  equation  as  follows, 

(2*)2_  12(2*) +  32  =  0; 
that  is,  (2*-4)(2*-8)=0. 

Hence  the  given  equation  is  equivalent  to 

\2*=8J 

The  first  of  these  has  for  one  real  solution  x  =  2;  the  second  has  the  real 
solution  x=3. 

Example  4. 

(x  +  a)  (x  +  a  +  b)  (x  +  a  +  2b)  {x  +  a  +  3b)  =  c4. 

Associating  the  two  extreme  and  the  two  intermediate  factors  on  the  left, 
we  may  write  this  equation  as  follows, 

{a;2  +  (2«  +  3b)x  +  a(a  +  36) }  {sc*  +  {2a  +  %b)x  +  {a  +  b)  (a  +  26)}  =  c\ 


410  RECIPROCAL  BIQUADRATIC  chap. 

If  ^  =  xi  +  (2a  +  3b)x  +  {wi  +  dab),  the  last  equation  may  be  written 

^+26a)=c*; 

that  is,  ?  +  2b-2Z  +  bi  =  bi  +  ci. 

Hence  £=  -&±s/(&+ct). 

The  original  equation  is  therefore  equivalent  to  the  two  quadratics 

x-  +  (2a  +  3b)x  +  a2  +  3ab  +  bi=±\J{bi  +  ci). 

§  8.]  Reciprocal  Equations. — A  very  important  class  of  equa- 
tions of  the  4th  degree  (biquadratics)  can  be  reduced  to 
quadratics  by  the  method  we  are  now  illustrating. 

Consider  the  equations 

ax*  +  bx3  +  ex2  +  bx  +  a  =  0  (1), 

ax4  +  bx3  +  ex2  -  bx  +  a  =  0  (I.), 

where  the  coefficients  equidistant  from  the  ends  are  either  equal, 
or,  in  the  case  of  the  second  and  fourth  coefficients,  equal  or 
numerically  equal  with  opposite  signs.  Such  equations  are 
called  reciprocal* 

If  we  divide  by  x2,  we  reduce  (1)  and  (I.)  to  the  forms 


B(*+?) 

+  b(x  +  -j  +  c  =  0 

(2), 

a(x2+?J 

+  b(x--J  +c  =  0 

(II.) 

ralent  to 

a(x  +  l)  +b{ 

x  +  -J  +c-2a  =  0 

(3), 

«(«-!)  +b[ 

x  —  )  +  c+  2a  =  0 
\       xJ 

(III.) 

3  and  III.  are  quadratics  in  x  +  1  jx  and  x  -  l/x  respectively.     If 
their  roots  be  a,  /?,  and  y,  8  respectively,  then  (3)  is  equivalent  to 


*  If  in  equation  (1)  we  write  l/£  for  x,  we  get  an  equation  which  is  equiva- 
lent to  a?  +  b?  +  c?  +  bS  +  a  =  Q.  Hence,  if  f  be  any  root  of  (1),  l/£  is  also  a 
root.  In  other  words,  two  of  the  four  roots  of  (1)  are  the  reciprocals  of  the 
remaining  two.  In  like  manner  it  may  be  shown  that  two  of  the  roots  of  (I.) 
are  the  reciprocals  of  the  remaining  two  with  the  sign  changed. 


XViI  GENERALISED  RECIPROCAL  BIQUADRATIC  411 

that  is,  to 


j  X   -  aX  +  1  =  0  (^  ,.. 

|/-/fc+l=0j  W" 

Similarly,  III.  is  equivalent  to 

The  four  roots  of  the  two  quadratics  (4)  or  (IV.)  are  the  roots 
of  the  biquadratic  (1)  or  (I.) 

Generalisation  of  the  Reciprocal  Equation. — If  we  treat  the 
general  biquadratic 

ax*  +  bx3  +  ex2  +  dx  +  e  =  0 

in  the  same  way  as  we  treated  equations  (1)  and  (I.),  we  reduce 
it  to  the  form 

a { x2  +  — 5 )  -r  b(x  +  j-)  +  c  =  0. 
\        ax"/        \       ox/ 

Now,  if  e/a  =  cPjb2,  this  last  equation  may  be  written 

(       d\2     J       d\  nad     n 

a(x  +  E)   +b(x  +  -)+c-2T  =  0, 

which  is  a  quadratic  in  x  +  djbx. 

Cor.  It  should  be  noticed  that  the  following  reciprocal  equations 
of  the  5th  degree  can  be  reduced  to  reciprocal  biquadratics,  and  can 
therefore  be  solved  by  means  of  quadratics,  namely, 

ax*  +  bx*  +  ex3  ±  ex2  ±  bx  ±  a  =  0, 

where,  in  the  ambiguities,  the  upper  signs  go  together  and  the 
lower  signs  together. 

For  the  above  may  be  written 

a(x>  ±  1)  +  bx(x3  ±  1)  +  cx\x  ±  1)  =0, 

from  which  it  appears  that  either  x  +  1  orz-1  is  a  factor  on 
the  left-hand  side.  After  this  factor  is  removed,  the  equation 
becomes  a  reciprocal  biquadratic,  which  may  be  solved  in  the 
manner  already  explained.  The  roots  of  the  quintic  are  either 
+  1  or  -  1,  and  the  four  roots  of  this  biquadratic. 


412  EXAMPLES  CHaP. 

Ill  an  appendix  to  this  volume  is  given  a  discussion  of  the 
general  solution  of  the  cubic  and  biquadratic,  and  of  the  cases 
where  they  can  be  solved  by  means  of  quadratics. 

Example  1. 

To  find  the  fifth  roots  of  +1.    Let  x  be  any  fifth  root  of  + 1  ;  then  x5  =  l. 
Hence  we  have  to  solve  the  equation 

^-1  =  0. 
This  is  equivalent  to 

Xx^  +  a^  +  x^  +  x  +  l-OJ' 
The  latter  equation  is  a  reciprocal  biquadratic,  and  may  be  written 

H)2+H)-1=0- 

After  solving  this  equation  for  x  +  \jx,  we,  find 

1         1  +  V5  1         1  -  \/5 

x  2  x  2 

These  give  the  two  quadratics 

a?+1J^6a.+1=0j         ^  +  11^  +  1  =  0. 

These  again  give  the  following  four  values  for  x : — 

-  (1  +  V5)/4±»V(10  -  2V5)/4,      -  (1  -  V5)/4±*V(10  +  2V5)/4, 
these,  together  with  1,  are  the  five  fifth  roots  of +  1.     This  will  be  found  to 
agree  with  the  result  obtained  by  using  chap,  xii.,  §  19. 

Example  2. 

(cc  +  «.)4  +  (a:  +  Z>)4=17(a-Z>)4. 

This  equation  may  be  written 

(z  +  «)4  +  (a-  +  &)4=17{(a;  +  a)-(.r  +  &)}4, 
from  which,  by  dividing  by  (x  +  b)\  we  deduce 

or  £4  +  l  =  17(S-l)4, 

where  £ = (» + a)/(x  +  b). 

This  equation  in  £  is  reciprocal,  and  may  be  written  thus — 

Hence  *  +  F  =  2' 

,    1     7       • 
From  this  lust  pair  we  deduce 


{=2,  or  £  ;  and  £  =  - 


±iV(15) 


8 


xvii    RATIONALISATION  BY  MEANS  OF  AUXILIARY  VARIABLES    413 

Hence  we  have  the  four  equations 

x  +  a_         x  +  a_,       x  +  a_7±i\/(15) 
x~+b~'J'     aT+l>_*'      x~+~b~         < 8         ' 

From  these,  four  values  of  x  can  at  once  be  deduced.     The  real  values  are 
x  =  a-2b  and  x  =  b-  2a. 

§  9.]  By  introducing  auxiliary  variables,  we  can  always  make 
any  irrational  equation  in  one  variable  depend  on  a  system  of 
rational  equations  in  one  or  more  variables.     For  example,  if  we 

have 

s'(x  +  a)+   J(x  +  b)+  s/(x  +  c)  =  d, 

and  we  put  u  =  \/(x  +  a),  v=  sj(x  +  b),  w=  J(x  +  c),  then  we 
deduce  the  rational  system 

u  +  v  +  w  =  d,     n2  =  x  +  a,     v2  =  x  +  b,     w2  =  x  +  c. 
Whether  such  a  transformation   will  facilitate  the  solution  de- 
pends on  the  special  circumstances  of  any  particular  case.     The 
following  is  an  example  of  the  success  of  the  artifice  in  question. 
Example. 

(a +aj)*  +  («-»)=&. 
We  may  write  the  given  equation  thus — 

(re  +  «)*  +  (re  -  xy j  {(re  +z)  +  (a-  x)}  *. 

Hence  we  deduce 


\a-xj  /t)a\t  la  —  x       ) 


(2a) 
Let  now  y={(a  +  x)l(a-x)}*t 

we  then  have  y  + 1  = -Ay*  + 1 )*. 

(2a)* 
From  the  last  equation  we  deduce 

2a(y+l)i=V(y*+l), 

which  is  a  reciprocal  biquadratic,  and  can  therefore  be  solved  by  means  of 
quadratics.  Having  thus  determined  y,  we  deduce  the  value  of  x  by  means 
of  the  equation  (re  +  x)/(a  -x)  =  yi. 


Exercises  XXXII. 

(1. )  a;2"1  -  x'"(bm  +  cm)  +  bmcm  =  0. 

(2.)  e?*'2  +  qe~3xl'2=p  ;   show  that  the  sum  of  the  two  real  values  of  x  is 

°       7  2 

(3.)  2xH^)^=C^f~(x1'i>  +  x1^). 


4H  EXERCISES  XXXII  chap. 

(4.)  (9*)*  -  2(3*)*3*+1  =  B2*-^. 

(5.)  **-£l+*+ '£*=*• 

(6.)  (x  +  \)  +  l/(x  +  \)  =  fi. 

(7.)  (l-x  +  x!)l(l  +  a2-x)  =  (l  +  a2  +  x)/(l+x  +  xi). 

(8.)  6xi  +  5x3-Z8x2  +  5x  +  6  =  0.  (9.)  6a^-31x3  +  51a;2-31x  +  6  =  0. 

(10.)  2xi-7x3  +  7x2-7x  +  2  =  Q.  (11.)  8x4- 42ar*  +  29a:2  +  42a;  +  8  =  0. 

(12.)  ax3  +  bx2  +  bx  +  a-0.  (13.)  rta^  +  i>x2-6x-a=0. 

(14.)  aa^  +  6ar  +  c  =  0.  (15.)  ax*  +  bx3  -  bx  -  a  =  0. 

(16.)  a2xi  +  2abx3  +  b2x2-c2  =  0.  (17.)  a:5  +  l  =  0. 

(18.)  x5  +  7xi  +  9x3-9x2-7x-l  =  0. 
(19.)  12a5  +  x4  +  13a-3  -  13a;2  -x-  12  =  0. 

(20.)  Show  that  the  biquadratic  axi  +  bx3  +  cx2  +  dx  +  e  =  0  can  be  solved 
by  means  of  quadratics,  provided  b/2a  =  iad/(iac-  b2). 
(21.)  a;1  +  10ar3  +  22a;2-15a;+2  =  0. 

(22. )  xi  +  2(p-  q)x3  +  (p2  +  q2)x2  +  2pq{p  -  q)x  +pq(p2  +pq  +  q2)  =  0. 
(23.)  3/(x2-7x  +  B)-2/(x2  +  7x  +  2)  =  5. 

(24.)  at(l+lX-{to?+x)=7Q.         (25.)  VU  -o?)  =  \  +  *J(l+x2)/x. 
(26.)  N/(a?+l)  +  4=5/V(«2+l)-  (27-)  (x  +  5)i  +  (x  +  5)~h  =  2. 

™  {fc:M^-{(i*-:)*'-»W- 

(29.)  2ar  +  2v/(z2  +  4a;-5)  =  4x2  +  8a;-|-5. 
(30.)  x2  +  7x-3  =  s/(2x2+Ux  +  2). 

(31.)  (,z-7)i+(z  +  9)*  +  2(ar  +  2:c-63)i=70-2.r. 

(32. )  ^(x2  +px  +  a)  +  \J(x2  +px  +  b)  +  s/(x2  +px  +  c)  =  0. 

(33.)  Show  that  the  imaginary  7th  roots  of  +  1  are  the  roots  of 
x2  -  ax  + 1  =  0,  a;2  -  fix  + 1  =  0,  x2  -  yx  + 1  =  0,  where  a,  §,  y  are  the  roots 
of  the  cubic  x3  +  x2  -  2x  - 1  =  0. 

(34.)  ^  +  J  =  a;V2\/(^4-i)-  (35.)  5(l  +  ar>)/(l  -x3)=  {(1  +x)/(l  -x)}3. 

(36.)  {a-x)5  +  (x-b)5  =  (a-b)5.     (37.)    v'a;  +  v^a; -  1 )  =  \/(x  + 1 ). 

(38.)  (as  +  3)(»+8)(a!  +  13)(aj  +  18)  =  51. 


SYSTEMS  WITH  MORE  THAN  ONE  VARIABLE  WHICH  CAN  BE 
SOLVED  BY  MEANS  OF  QUADRATICS. 

§  10.]  According  to  the  rule  stated  without  proof  in  chap, 
xiv.,  §  6,  if  we  have  a  system  of  two  equations  of  the  Zth  and 
with  degrees  respectively  in  two  variables,  x  and  y,  that  system 
has  in  general  Im  solutions.  Hence,  if  we  eliminate  y  and 
deduce  from  the  given  system  an  equation  in  x  alone,  that  equa- 
tion will  in  general  be  of  the  Imth  degree,  since  there  must  in 


XVII         MOST  GENERAL  SYSTEM  HAYING  TWO  SOLUTIONS  415 

general  be  as  many  different  values  of  x  as  there  are  solutions  of 
the  original  systems.  We  shall  speak  of  this  equation  as  the 
Resultant  Equation  in  x. 

In  like  manner,  if  we  have  a  system  of  three  equations  of 
the  /th,  wth,  and  nth  degrees  respectively,  in  three  variables 
x,  y,  z,  the  sjrstem  has  in  general  Imn  solutions  ;  and  the  re- 
sultant equation  in  x  obtained  by  eliminating  y  and  z  will  be  of 
the  Imnth  degree  ;  and  so  on. 

From  this  it  appears  that  the  only  perfectly  general  case  in  which 
the  solution  of  a  system  of  equations  will  depend  on  a  quadratic  equation 
is  that  in  which  all  the  equations  hit  one  are  of  the  1st  degree,  and 
that  one  is  of  the  2nd. 

It  is  quite  easy  to  obtain  the  solution  in  this  case,  and  thus 
verify  in  a  particular  instance  the  general  rule  from  which  we 
have  been  arguing.  All  we  have  to  do  is  to  solve  the  n-\ 
linear  equations,  and  thereby  determine  n  -  1  of  the  variables  as 
linear  functions  of  the  nth.  variable.  On  substituting  these 
values  in  the  nth.  equation,  which  we  suppose  of  the  2nd 
degree  in  all  the  n  variables,  it  becomes  an  equation  of  the 
2nd  degree  in  the  nth  variable.  We  thus  obtain  two  values 
of  the  nth  variable,  and  hence  two  corresponding  values  for  each 
of  the  other  n  -  1  variables ;  that  is  to  say,  we  obtain  two  solu- 
tions of  the  system. 

Example  1. 

lx  +  my  +  n  =  0  (I), 

ax2  +  2hxy  +  by-  +  2gx  +  2fy  +  c=0  (2). 

(1)  is  equivalent  to 

Ix+n 
y=--m-  (3); 

and  this  value  of  y  reduces  (2)  to 

am2x*  -  2hmx{lx  +  n)  +  b(lx  +  rif  +  2gm-x  -  2fm(lx  +  n)  +  cm-  =  0, 
that  is, 

{am2 -  2hlm  +  bP)x2  +  2{gm'1  -  hmn  +  bnl  -flm)x  +  {bn~  -  2fmn  +  c??i2)  =  0    (4). 
The  original  system  (1),  (2)  is  therefore  equivalent  to  (3),  (4).     Now  (4)  gives 
two  values  for  x,  and  for  each  of  these  (3)  gives  a  corresponding  value  of  y. 
For  example,  the  two  equations 

3.c  +  2y  +  l=0,     x2  +  2xy  +  y--x  +  y  +  Z  =  0, 
will  be  found  to  be  equivalent  to 

y=-?x-\,     ar-8;c+ll-0. 


416  SYSTEM  IN  TWO  VARIABLES  chap. 

Hence  the  two  solutions  of  the  system  are 

x=      4  +    V5,  4-    s/5  ; 

2/=-¥-iV5,     -V+fs/6- 

Example  2. 

3a;+2y-i8=l>     x  +  y-3z  =  2,    x2  +  y2  +  z2=l. 
The  system  is  equivalent  to 

x=-5z-3,     y  =  8z  +  5,     90z2  + 1102  +  33  =  0. 
The  solutions  are 

the  upper  signs  going  together  and  the  lower  together. 

§  11.]  For  the  sake  of  contrast  with  the  case  last  considered, 
and  as  an  illustration  of  an  important  method  in  elimination,  let 
us  consider  the  most  general  system  of  two  equations  of  the 
2nd  degree  in  two  variables,  namely — 

ax*  +  2hxy  +  by2  +  2gx  +  2fy  +  c  =  0  (1), 

ax2  +  2h'xy  +  b'tf  +  2g'x  +  2fy  +  c'  =  0  (2). 

We  may  write  these  equations  in  the  forms — 

bif  +  2(hx  +f)y  +  (ax2  +  2gx  +  c)  =  0, 
b'y2  +  2(h'x  +f')y  +  (a'x2  +  2g'x  +  c')  =  0, 
say  by2+py  +  q  =  0  (1'), 

Vtf+ft  +  j-Q  (2'), 

Avhere  p  =  2(hx  +/),  q  =  ax2  +  2gx  +  c,  &c. 

If  we  multiply  (1')  and  (2')  by  b'  and  by  b  respectively,  and 
subtract,  and  also  multiply  them  by  q'  and  by  q  respectively,  and 

subtract,  we  deduce 

(pb'-p'b)y  +  (b'q-bq')  =  0  (3), 

(b'q-bq')y2+(p'q-pq')y  =  0  (4); 

and  provided  bq'  -  b'q^  0,  (3)  and  (4)  will  be  equivalent  to  (1') 
and  (2').  In  general,  the  values  of  x  which  make  bq'-b'q=0 
will  not  belong  to  the  solutions  of  (3)  and  (4),  nor  will  the  value 
y  -  0  belong  to  those  solutions.  Hence  we  may  say  that,  in 
general,  the  system 

{j>h'-p'b)y  +  (b'q-bq)  =  0  (3'), 

(b'q-bq')y  +  (p'q-pq')  =  0  (4'), 

is  equivalent  to  (1')  and  (2'). 

Again,  if  we  multiply  (3')  and  (4')  by  b'q  -  bq  and  by  pb'  - p'b 
respectively,  and  subtract,  we  deduce 

(b'q-bqy-(Pb'-p'b)(p'q~pq')  =  0  (5), 


XVII 


OF  THE  ORDER  (2,  2)  417 


and,  provided  bq  -  b'q  4=  0,  (4')  and  (5)  will  be  equivalent  to  (3') 
and  (4'). 

Hence  we  finally  arrive  at  the  conclusion  that,  in  general,  the 
system 
{b'(ax2  +  2gx  +  c)  -  b(a'a?  +  2g'x  +  c')}2  -  4={b'(hx  +/) 

-  b(h'x  +/)}{{h'x  +/')  (atca  +  2gx  +  c)  -  (hx  +/)  (a'af  +  2g'x  +  c')} 

-0     (6), 
{b'(ax2  +  2gx  +  c)  -  b(a'x2  +  2g'x  +  c')}y 

+  2{{h'x  +/')  (ax2  +  2gx  +  c)  -  (Iix  +/)  (ax2  +  2g'x  +  c')} 

=  0     (7), 
is  equivalent  to  (1)  and  (2). 

The  first  of  these  is  a  biquadratic  giving  four  values  for  x, 
and,  since  (7)  is  of  the  1st  degree  in  y,  for  each  value  of  x  we 
obtain  one  and  only  one  value  of  y.  We  have  therefore  four 
solutions,  as  the  general  rule  requires. 

In  general,  the  resultant  biquadratic  (6)  will  not  be  reducible 
to  quadratics.  It  may,  however,  happen  to  be  so  reducible  in 
particular  cases.  The  following  are  a  few  of  the  more  im- 
portant : — 

I.  If,  for  example,  b'/b  =/'//=  c'/c,  then  (6)  reduces  to 
x2[{b'(ax  +  2g)  -  b(a'x  +  2g')}2  -  i(b'h  -  bh'){(h'x  +  f)  (ax  +  2g) 

-  (hx+f)  (a'x  +  2g')  +  (h'c  -  he')}]  =  0, 
two  of  whose  roots  are  zero,  the  other  two  being  determinable 
by  means  of  a  quadratic  equation. 

II.  Again,  if  a' /a  =  b'/b  =  h'/h,  it  will  be  found  that  the  two 
highest  terms  disappear  from  (6).  Hence  in  this  case  two  of  its 
roots  become  infinite  (see  chap,  xviii.,  §  6),  and  the  remaining 
two  can  be  found  by  means  of  a  quadratic  equation. 

III.  If/=0,  g  =  0,f  =  0,  g'  =  0,  it  will  be  found  that  only 
even  powers  of  x  occur  in  (6).  The  resultant  then  becomes  a 
quadratic  in  x2. 

IV.  The  resultant  biquadratic  may  come  under  the  reciprocal 
class  discussed  in  §  8  above. 

Most  of  these  exceptional  cases  are  of  interest  in  the  theory 
of  conies,  because  they  relate  to  cases  where  the  intersection  of  two 
conies  can  be  constructed  by  means  of  the  ruler  and  compasses 
alone.     The  general  theory  is  given  in  the  Appendix  to  this  vol. 

VOL.  I  2  E 


418  EXAMPLES  chap. 

Example  1. 
The  system  3x2  +  2xy  +  y2=l7,     x2-2xy  +  5y2  =  5, 

is  equivalent  to     12.vy  +  14a;2-  80  =  0,     73a;4 -692a;2 +  1600  =  0. 
The  solutions  of  which  are 

x=+2,      -2,      +20/V(73),      -20/V(73); 

y=+l,      -1,     +1/V(73),       -1/V(73). 
Example  2. 

n{x2  +  2y)  =  1(1  +  2xy),     n(ij2  +  2x)  =  m(l  +  2xy). 
Here  the  elimination  is  easy,  because  the  first  equation  is  of  the  1st  degree 
in  y.     We  deduce  from  it 

?ia;2  - 1 
y~2{lx-n)' 
This  reduces  the  second  equation  to 

n(nx2-  l)2  +  8nx(lx-n)2  =  irn(lx-n)2+imx(lx-n)  (nx2-  I), 
which  is  equivalent  to 

(n2  -  4.lm)xi  +  4(2P  +  mn)x*  -  18nlx2  +  i(2n2  +  lm)x  +  (I2  -  4»m)  =  0. 
If  n  =  l,  this  biquadratic  is  reciprocal,  and  its  solution  depends  upon 

(Z-4m)f2  +  4(2Z  +  m)£+  (8m -200=0, 
where  £  =  a;  +  l/a;. 

In  general,  if  we  have  an  equation  of  the  1st  degree  in  x 
and  y  together  with  an  equation  of  the  nth.  degree  in  x  and  y, 
the  resultant  equation  in  x  will  be  of  the  wth  degree.  In  par- 
ticular cases,  owing  to  the  existence  of  zero  or  infinite  roots, 
or  for  other  special  reasons,  this  equation  may  be  reducible  to 
quadratics. 

Example. 

x  +  y  =  18,     a;3  +  y3=4914, 
is  equivalent  to 

y=lS-x,     ar!  +  (18-a;)3  =  4914. 
The  second  of  these  two  last  equations  reduces,  as  it  happens,  to 

a;2- 18a; +17  =  0. 
Hence  the  finite  solutions  of  the  given  system  are 

35=17,1; 
y=l,  17. 

§  12.]  A  very  important  class  of  equations  are  the  so-called 
Homogeneous  Systems.  The  kind  that  most  commonly  occurs  is 
that  in  which  each  equation  consists  of  a  homogeneous  function 
of  the  variables  equated  to  a  constant.  The  artifice  usually  em- 
ployed for  solving  such  equations  is  to  introduce  as  auxiliary 
variables  the  ratios  of  all  but  one  of  the  variables  to  that  one. 
Thus,  for  example,  if  the  variables  were  x  and  y,  we  should  put 
y  =  vx,  and  then  treat  v  and  x  as  the  new  variables. 


xvii  HOMOGENEOUS  SYSTEMS EXAMPLES  419 

Example  1. 

x2  +  xy  =  12,     xy  -2y2  =  l. 
Put  y  =  vx,  and  the  two  equations  become 

z2(l  +  fl)  =  12,     x2(v-2v2)  =  l. 
From  these  two  we  derive 

x2(l  +  v)-\2x2{v-2ir)  =  0, 
that  is, 

a?{24t?-llt>+l}=0. 
Since  x  =  0  evidently  affords  no  solution  of  the  given  system,  we  see  that  the 
original  system  is  equivalent  to 

a?(l+v)  =  12,     24b2-11v  +  1  =  0. 
Solving  the  quadratic  for  v,  we  find  v—l/S  or  1/8. 

Corresponding  to  v=l/3,  the  first  of  the  last  pair  of  equations  gives  x2  =  9, 
that  is,  x=  ±3. 

Corresponding  to  v—1/8,  we  find  in  like  manner  x=  ±4n/(2/3). 
Hence,  bearing  in  mind  that  y  is  derived  from  the  corresponding  value  of 
x  by  using  the  corresponding  value  of  v  in  the  equation  y  —  vx,  we  have,  for 
the  complete  set  of  solutious, 

*=+3,      -3,      +4V(2/3),      -4V(2/3); 
y=+l,      -1,      +1/V6,  -VV6. 

Example  2. 

x2  +  2yz=l,     y2  +  2zx  =  m,     z2  +  2xy  =  n. 

Let  x=uz,  y  —  vz,  then  the  equations  become 

(u2  +  2v)z2  =  l,     {v2  +  2u)z2  =  m,     (l  +  2uv)z2  =  n. 

Eliminating  z,  we  have,  since  2  =  0  forms  in  general  no  part  of  any  solution, 
n  ( v?  +  2v)  =  I  (1  +  2uv),     n  {v2  +  2u)  =  m  (1  +  2wi>). 

"We  have  already  seen  how  to  treat  this  pair  of  equations  (see  §  11, 
Example  2).  The  system  has  in  general  four  different  solutions,  which  can 
be  obtained  by  solving  a  biquadratic  equation  (reducible  to  quadratics  when 
n  =  I). 

If  we  take  any  one  of  these  solutions,  the  equation  (1  +2icv)z2  =  n  gives 
two  values  of  z.  The  relations  x  =  uz,  y  =  vz,  then  give  one  value  of  a;  and  one 
value  of  y  corresponding  to  each  of  the  two  values  of  z. 

We  thus  obtain  all  the  eight  solutions  of  the  given  system. 

There  is  another  class  of  equations  in  the  solution  of  which 
the  artifice  just  exemplified  is  sometimes  successful,  namely, 
that  in  which  each  equation  consists  of  a  homogeneous  function 
of  the  variables  equated  to  another  homogeneous  function  of  the 
variables  of  the  same  or  of  different  degree. 

Example  3. 
The  system 

ox2  +  bxy  +  cy2  =  dx  +  ey,     a'x2  +  b'xy  +  c'y2  =  d'x  +  e'y  (1) 

is  equivalent  to 

(a  +  bv  +  cv2)x2={d  +  ev)x,     (a'  +  b'v  +  c'v2)x2  =  (d'  +  e'v)x  (2) 

where  y  =  vx. 


420  EXAMPLES  chap. 

From  this  last  system  we  derive  the  system 

x*{(a  +  bv  +  cv°)  {d'  +  e'v)-  (a'  +  b'v  +  c'v>)(d  +  ev)}  =0\  ,„. 

£{(«  +  &u  +  cr2)a;-(d  +  er)}=0/  (6>> 

which  is  equivalent  (see  chap,  xiv.,  §  11)  to  (2),  along  with 

(a  +  bv  +  cv2)a?  =  0  (4), 

{d  +  ev)x  =  0  (5). 

If  we  observe  that  x=0,  y  —  0  is  a  solution  of  the  system  (1),  and  keep 
account  of  it  separately,  and  observe  further  that  values  of  v  which  satisfy  both 
(1)  and  (5)  do  not  in  general  exist,  we  see  that  the  system  (1)  is  equivalent  to 

(a  +  bv  +  cv2)  (d'  +  e'v)  -  {a'  +  b'v  +  c'v2)  (d  +  ev)  =  0  (6) 

along  with  (a  +  bv  +  ci?)x-  (d  +  ev)  =  0  (7) 

and  x  =  0,     y  =  0. 

The  solution  of  the  given  system  now  depends  on  the  cubic  (6).  The 
three  roots  of  this  cubic  substituted  iu  (7)  give  us  three  values  of  x,  and  y  =  vx 
gives  three  corresponding  solutions  of  (1).  Thus,  counting  x  =  0,  y  =  0,  we 
have  obtained  all  the  four  solutions  of  (1). 

The  cubic  (6)  will  not  be  reducible  to  quadratics  except  in  particular  cases, 
as,  for  example,  when  ad'  -a'd  =  Q  or  ce'  -  c'e  —  0. 
For  example,  the  system 

3a;2  -  2xy  +  3y2  =  x  + 1 2y,     6x2  +  2xy  -  2y2  -2x  +  29y, 
is  equivalent  to  x=0,  y  =  0,  together  with 

7>(llli>2  -  86*;+  8)  =  0,     (3  -  2v  +  3v-)x=  1  +  12t>. 
The  values  of  v  are  2/3,  4/37,  and  0.     Hence  the  solutions  of  the  system  are 

x=0,     3,     185/227,     1/3; 
y=0,     2,     20/227,       0. 

§  13.]  Symmetrical  Systems. — A  system  of  equations  is  said  to 

be  symmetrical  when  the  interchange  of  any  pair  of  the  variables 

derives  from  the  given  system  an  identical  system.    For  example, 

x  +  y  =  a,     x2  +  y2  =  b  ;  z3  +  y  =  a,     y3  +  x  -a  ; 

x  +  y  +  z  =  a,     x2  +  y2  +  z*  —  b,     yz  +  zx  +  xy  =  c, 

are  all  symmetrical  systems. 

There  is  a  peculiarity  in  the  solutions  of  such  systems,  which 
can  be  foreseen  from  their  nature.  Let  us  suppose  in  the  first  place 
that  the  system  is  such  that  it  would  in  general  have  an  even 
number  of  solutions,  four  say.    If  Ave  take  half  the  solutions,  say 

X  =  a1,  a2, 
V  =  Pn  Am 

then,  since  the  equations  are  still  satisfied  when  the  values  of  x 
and  y  are  interchanged,  the  remaining  half  of  the  solutions  are 

x  =  (3n  ft, 
y  =  au  a2. 


xvn  SYMMETRICAL  SYSTEMS  421 

If  the  whole  number  of  solutions  were  odd,  five  say,  then 
four  of  the  solutions  would  be  arranged  as  above,  and  the  fifth 
(if  finite,  which  in  many  cases  it  would  not  be)  must  be  such 
that  the  values  of  x  and  y  are  equal ;  otherwise  the  interchanges 
of  the  two  would  produce  a  sixth  solution,  which  is  inadmissible, 
if  the  system  have  only  five  solutions.* 

These  considerations  suggest  two  methods  of  solving  such 
equations. 

1st  Method. — Replace  the  variables  by  a  new  system  of  vari- 
ables, consisting  of  one,  say  x,  of  the  former,  and  the  ratios  to  it 
of  the  others,  u,  v,  .  .  .  say.  Eliminate  x,  v,  .  .  .  and  obtain 
an  equation  in  u  alone  ;  then  this  equation  will  be  a  reciprocal 
equation  ;  for  the  values  of  u  are 

al  Pi  a2  P-2       o  /  1       •  1  -i  \ 

u  =  — ,    — ,    -r-,    — ,  &c.  (and,  it  may  be,  u  =  1 ), 

Pi       «i       Pa       a2 

that  is  to  say,  along  with  each  root  there  is  another,  which  is  its 
reciprocal.  The  degree  of  this  resultant  equation  can  therefore 
in  all  cases  be  reduced  by  adjoining  a  certain  quadratic,  just  as 
in  the  case  of  a  reciprocal  biquadratic. 

2nd  Method. — Replace  the  variables  x,  y,  z,  .  .  .  by  an  equal 
number  of  symmetric  functions  of  x,  y,  z,  .  .  .,  say  by  Sic,  i>//, 
~2xyz,  .  .   .,   ifec,  and  solve  for  these. 

The  nature  of  the  method,  its  details,  and  the  reason  of  its 
success,  will  be  best  understood  by  taking  the  case  of  two 
variables,  x  and  y. 

Let  us  put  u  =  x  +  y,  v  =  xy.  After  separating  the  solutions, 
if  any,  for  which  x  =  y,  Ave  may  replace  the  given  system  by  a 
system  each  equation  of  which  is  symmetrical.  We  know,  by 
the  general  theory  of  symmetric  functions  (see  chap,  xviii.,  §  4), 
that  every  integral  symmetric  function  can  be  expressed  as  an 

*  We  have  supposed  that  for  all  the  solutions  (except  one  in  the  case  of 
an  odd  system)  x  +  y.  It  may,  however,  happen  that  x  =  y  for  one  or  more 
solutions.  Such  solutions  cannot  be  paired  with  others,  since  an  interchange 
of  values  does  not  produce  a  new  solution.  This  peculiarity  must  always 
arise  in  systems  which  are  symmetrical  as  a  whole,  but  not  symmetrical  in  the 
individual  equations.  As  an  example,  we  may  take  the  symmetrical  system 
x3  +  y=a,  y3  +  x-a,  three  of  whose  solutions  are  such  that  x  =  y. 


422  SYMMETRICAL  SYSTEMS  chap. 

integral  function  of  u  and  v.  Hence  it  will  always  be  possible  to 
transform  the  given  system  into  an  equivalent  system  in  u  and  v. 

We  observe  further  that,  in  general,  u  and  v  will  each  have 
as  many  values  as  there  are  solutions  of  the  given  system,  and 
no  more  ;  but  that  the  values  of  u  and  v  corresponding  to  two 
solutions,  such  as  x  =  au  y  =  ($„  and  x  =  /3l}  y  =  al}  are  equal. 
Hence  in  the  case  of  symmetrical  equations  the  number  of  solu- 
tions of  the  system  in  u  and  v  must  in  general  be  less  than  usual. 

Corresponding  to  any  particular  values  of  u  and  v,  say  u  =  a, 
v  =  (3,  we  have  the  quadratic  system  x  +  y  =  a,  xy  =  fi,  which  gives 
the  two  solutions 

X  =  {a  ±   v/(a2  -  4j8)}/2,      y={aT   */(aS  -  4/?)}/2. 

If  we  had  a  system  in  three  variables,  x,  y,  z,  then  we  should 
assume  u  =  x  +  y  +  z,  v  =  yz  +  zx  +  xy,  w  =  xyz,  and  attempt  to  solve 
the  system  in  u,  v,  w.  Let  u  =  a,  v  -  j3,  iv  -  y,  be  any  solution  of 
this  system  ;  then,  since 

(f-*)tf-y)tf-*)^-«f  +  «f-«i 

we  see  that  the  three  roots  of 

e-af'  +  /3$-y  =  0 

constitute  a  solution  of  the  original  system,  and,  since  the 
equations  are  symmetrical,  any  one  of  the  six  permutations  of 
these  roots  is  also  a  solution.  In  this  case,  therefore,  the  number 
of  solutions  of  the  system  in  u,  v,  to  would,  in  general,  be  less 
than  the  corresponding  number  for  the  system  in  x,  y,  z. 

The  student  should  study  the  following  examples  in  the  light 
of  these  general  remarks  : — 

Example  1.  A  (x-  +  y2)  +  Bxy  +C  (x  f  y)  +  T>  =0  \ 

A'(xo-  +  y"-)  +  B'xy  +  C'{z  +  y)  +  D'  =  0)  (  )- 

If  we  put  y  =  vx,  and  then  eliminate  x  by  the  method  employed  in  §11, 
the  resultant  equation  in  v  is 

{ (D'A)  +  (D'B)»  +  (D'AH-2} 2  =  (D'C)  (1  +  vf  { (C'A)  +  (C'B)«  +  (C'A)«2}     (2), 

where  (D'A)  stands  for  D'A  -  DA',  (D'B)  for  D'B  -  DB',  and  so  on. 

The  biquadratic  (2)  is  obviously  reciprocal,  and  can  therefore  be  solved  by 
means  of  quadratics. 

The  solution  can  then  be  completed  by  means  of  the  equation 

{(D'A)  +  (D'B)v  +  (D'A)^}x  +  (D'C)(l  +  v)  =  0  (3). 


i 


XVII 


EXAMPLES  423 


As  an  instance  of  this  method  the  student  should  work  out  in  full  the 

solution  of  the  system 

2(x2  +  y-)  -  3xy  +  2(x  +  y)  -  39  =  0, 
3(x2  +  y°-)-ixy  +   (x  +  i/)  -  50  =  0. 

"We  may  treat  the  above  example  by  the  second  method  of  the  present 
paragraph  as  follows.     The  system  (1)  may  be  written 
A(x  +  y)2+{B  -2A)xy  +  C(x  +  y)  +  T>  =  0, 
A'(x  +  y)2  +  (B'  -  2A!)xy  +  C'(x +y)  +  D'=0  ; 

Am2+(B  -2A)i-  +  Cm+D=0\  ... 

tnatis>  AV+(B'-2A>  +  C'«+D'=0j  v  h 

Eliminating  first  u2  and  then  v,  we  deduce  the  equivalent  system 

(A'B)i?+(A'C)M  +  (A'D)=0\ 
(A'B)u2  +  { (C'B)  -  2(C'A)  J  u  +  { (D'B)  -  2(D'A) }  =0  J 
where  (A'B),  &c,  have  the  same  meaning  as  above. 
The  system  (5)  has  two  solutions, 

u  =  a,  a', 

say,  corresponding  to  which  we  find  for  the  original  system 


x 


—  I 


;a±vV-4/3)}/2,      {a'±V("'2-4/3')}/2, 


in  all  four  solutions. 

This  method  should  be  tested  on  the  numerical  example  given  above. 

Example  2.  xi  +  yi  =  82,     x  +  y=4. 

We  have  xi  +  yi=(x  +  ijf  -  4xy(x2  +  y2)  -  6x2y2, 

=  (x  +  yf  -  ixy  { (x  +  yf  -  2xy }  -  6x2if, 
=  ui-4u2v  +  2v2. 
Hence  the  given  system  is  equivalent  to 

u4-4u*v  +  2v2  =  82,     u=i. 
Using  the  value  of  u  given  by  the  second  equation,  we  reduce  the  first  to 

f2-32w  +  87  =  0. 
The  roots  of  this  quadratic  are  3  and  29.     Hence  the  solution  of  the  u,  v 
system  is  u  =  4,  4, 

v=S,  29. 
From  x+y=i,  xy  =  29,  we  derive  {'--y)-=  -100,  that  is,  x-y-±10i; 
combining  this  with  x  +  y=4,  we  have  se=2±5i,  y  =  2:f  5i. 
From  x  +  y=i,  xy  =  2,  we  find  x  =  S,  y  =  l ;  x=l,  ?/  =  3. 
All  the  four  solutions  have  thus  been  found. 

Example  3.  xi=mx+ny,     y4  =  nx  +  my  (I}. 

Let  us  put  y  =  vx;  then,  removing  the  factor  x  in  both  equations,  and 
noting  the  corresponding  solution,  x  =  0,  y  =  0,  we  have 

x3  =  m  +  nv,     via?  =  n  +  mv. 
These  are  equivalent  to 

x3=m  +  nv,     v*(m  +  nr)  =  mv  +  n  (2). 


424  EXAMPLES  chap. 

The  second  of  these  may  be  written 

n(v°-l)  +  mv{v?-l)  =  0  (3), 

and  is  therefore  equivalent  to 

:"+iV+(5°i>+(5+i>+i=°}' 

The  second  of  these  is  a  reciprocal  biquadratic.     Hence  all  the  five  roots  of  (3) 
can  be  found  without  solving  any  equation  of  higher  degree  than  the  2nd. 

To  the  root  v—1  correspond  the  three  solutions, 

x  =  y  =  (m  +  m)"'3.     u{ni  +  n)llS,     to"(m  +  n)1!3, 
of  the  original  system,  where  (ra  +  n)1'3  is  the  real  value  of  the  cube  root,  and 
w,  or  are  the  imaginary  cube  roots  of  unity. 

In  like  manner  three  solutions  of  (1)  are  obtained  for  each  of  the  remain- 
ing four  roots  of  (3).  Hence,  counting  x  =  0,  y  =  0,  we  obtain  all  the  sixteen 
solutions  of  (1). 

The  reader  should  work  out  the  details  of  the  numerical  case 

xi  =  2x  +  By,     yi-3x  +  2y, 
and  calculate  all  the  real  roots,  and  all  the  coefficients  in  the  complex  roots, 
to  one  or  two  places  of  decimals. 

Example  4.  yz  +  zx  +  xy  =  26, 

yz(y  +  z)  +  zx(z  +  x)  +  xy(x  +  y)  =  1 62, 
yz{if  +  z2)  +  zx{z-  +  u?)  +  xy{x-  +  y2)  =  538. 
If  we  put  u  =  x  +  y  +  z,  v  =  yz  +  zx  +  xy,  w  =  xyz,  the  above  system  reduces  to 

i>=26,     M0-3w=162,     (u2-2v)v-uw  =  538. 
Hence  26t*-3w=162,     26ic--mc  =  1890. 

Hence  26m2  +81m-  2835  =  0. 

The  roots  of  this  quadratic  are  it  =  9  and  u=  —  315/26. 

We  thus  obtain  for  the  values  of  u,  v,  w,  9,  26,  24,  and  -  315/26,  26, 
-  159.     Hence  we  have  the  two  cubics 

£3-9£2  +  26£-24  =  0, 
£3  +  3^£2  +  26f  +  159  =  0. 

Twelve  of  the  roots  of  the  original  system  consist  of  the  six  permutations 
of  the  three  roots  of  the  first  cubic,  together  with  the  six  permutations  of  the 
roots  of  the  second  cubic. 

The  first  cubic  evidently  has  the  root  £  =  2  ;  and  the  other  two  are  easily 
found  to  be  3  and  4.     Hence  we  have  the  following  six  solutions  : — 

x=2,     2,     3,     3,     4,     4; 
y  =  3,     4,     4,     2,     2,     3; 
a  =  4,     3,     2,     4,     ?,     2. 
Other  six  are  to  be  found  by  solving  the  second  cubic. 

§  14.]  We  conclude  this  chapter  with  a  few  miscellaneous 
examples  of  artifices  that  are  suggested  merely  by  the  peculi- 


xvii  MISCELLANEOUS  EXAMPLES  425 

arities  of  the  particular  case.  Some  of  them  have  a  somewhat 
more  general  character,  as  the  student  will  find  in  working  the 
exercises  in  set  xxxiv.  A  moderate  amount  of  practice  in  solv- 
ing puzzles  of  this  description  is  useful  as  a  means  of  cultivating 
manipulative  skill ;  hut  he  should  beware  of  wasting  his  time 
over  what  is  after  all  merely  a  chapter  of  accidents. 

Example  1. 

ax         by       (a  +  b)c 


a  +  x     b  +  y    a  +  b  +  c' 
Let  a  +  x  =  (a  4-  b  +  c)£,     b  +  y  =  {a  +  b  +  c)-q  ; 

the  system  then  reduces  to 

a2^  +  b"lr,  =  (a  +  b)2,     £+ij=l. 
This  again  is  equivalent  to 

{(a  +  b)^a}2  =  0,     f+ij=l. 
Hence  we  have  the  solution  £  =  a/(a  +  b),  r)  =  b/(a  +  b)  twice  over. 

The  solutions  of  the  original  system  are  therefore  x  =  ac/(a  +  b),  y=bc/(a  +  b) 
twice  over. 

Example  2. 

ax2  +  bxy  +  cy2  =  bx2  +  cxy  +  ay2=d  (1). 

This  system  is  equivalent  to 

(a  -  b)x2  +  (b  -  c)xy  +  (c-a)y-  =  0  (2), 

ax2  +  bxy  +  cy2=d  (3). 

The  equation  (2)  (see  chap,  xvi.,  §  9)  is  equivalent  to 

x2  =  (c<x  +  l)P,     xy  =  (aa  +  l)p,     y2=(ba  +  l)P  (4), 

where  p  and  <r  are  undetermined. 
Since  x2y2  =  (xy)2,  we  must  have 

(C(r  +  l)(6(j  +  l)  =  (ffcr  +  l)2. 

J)  A-  n 0/t 

Hence  we  deduce  c  =  0,     a— — r1 — r~  (5). 

'  a- -be 

The  first  of  these,  taken  in  conjunction  with  (4),  gives  x  =  y  ;  and  hence 

4-       /         *~ . 

x  =  y  =  ±  A  /  i —  > 

J  V    a+b+c 

that  is  to  say,  two  solutions  of  (1).     If  we  take  the  second  value  of  a  we  find 
,2_pic-af  p{c-a){a-i)        „     p(«^)2  (6) 

x  ~  a2-bc'       J~       a? -be      '     T~  a? -be  K  >' 

where  it  remains  to  determine  p/(a2  -  be).     This  can  be  done  by  substituting 
in  (3).     We  thus  find 

p/(a2  -  be)  =  d/(a3  +  ac2  -  ca2  +  ab2  -  a2b  -  abc). 

We  now  deduce  from  (6) 

±(c-a)<P- 


x  =  : 


y=±,  &c. 


(a3  +  ac2  -  ca-  +  ab2  -  a2b  -  abc)1  ■-' 
two  more  solutions  of  the  original  system. 

The  system  (2),  (3)  could  also  be  solved  very  simply  by  putting  y  =  vx, 
as  in  §  12. 


426  MISCELLANEOUS  EXAMPLES  chap. 


Exam 
These 

pie  3. 
equations 

give 

yz  = 

-a2,     zx  = 
zxxxy 

■b2,     xy- 

b2xc2 

~     a2    ' 

b2c2 
~  a2' 

--c2. 

t  is, 

yz 

Hence  x=±bc/a  ;  the  two  last  equations  of  the  original  system  then  give 
y=±ca/b,  z=±ab/c.  The  upper  signs  go  together  and  the  lower  together  ; 
so  that  we  have  only  obtained  two  out  of  the  possible  eight  solutions. 

Example  4. 

x{y  +  z)  =  a2,     y(z  +  x)  =  b2,     z(x  +  y)=--c2. 

This  can  be  reduced  to  last  by  solving  for  yz,  zx,  xy. 

Example  5. 

x{x  +  y  +  z)  =  a2,     y(x  +  y  +  z)  =  b2,     z(x  +  y  +  z)  =  c2. 

Let  x  +  y  +  z  —  p.     Then,  if  we  add  the  three  equations,  we  have 

p2  =  a2  +  b2  +  c2. 
Hence  p  =  ±  \/(«2  +  b2  +  c2)  ;  and  we  have 

±a2  ±b2  ±c2 


X —      ///v-2   i   12  ,    »2\l        V~ 


«J(a2  +  b2  +  c2)'     J     ^{a2  +  b2  +  c2Y  V^'  +  ^  +  c2)' 

Example  6. 
To  find  the  real  solutions  of 

a*+tf+p=tp       (1),  ${y+z)+tf=bc         (4), 

tf'  +  ?-  +  e  =  b2        (2),  v{z  +  x)  +  tt=ca         (5)) 

z2  +  e  +  T  =  c2        (3),  fte+y)+|ij=a5        (6). 

From  (2),  (3),  and  (4)  we  deduce 

U(y+s)+i?f}2-  w+f+ewz'+e+v^^o ; 

that  is,  (l2-S»)8+(^-f2)a+(i?-w)3=0  (7). 

Every  solution  of  the  given  system  must  satisfy  (7).  Now,  since  (£2-yz)2, 
(£77 -zf)2,  (ft-yy)2  are  all  positive,  provided  x,  y,  z,  £,  77,  f  be  all  real,  it 
follows  that  for  all  real  solutions  we  must  have  ^2  —  yz,  §J7=fo  ff  =  777/. 

Hence,  from  the  symmetry  of  the  system,  we  must  have 

£2  =  yz,    ■n2  =  zx,    £2=xy,  (8), 

— £  '-?•   8=T  (9)- 

By  means  of  (8)  we  reduce  (1),  (2),  (3)  to 

x(x  +  y  +  z)  =  a2,     y(x  +  y  +  z)  =  b2,  z(x  +  y  +  z)  =  c2. 
Hence,  by  Example  5,  we  have 

±a2_                           ±b2  _       _±f 

X~^(a2  +  b2  +  c2y     y~^(a2  +  b2  +  c2)'  Z~^/(a2  +  b2  +  c2Y 
From  (8)  we  now  derive 

zkbc                                zkca  ,__           ±«£> 

*  "~  .  //_2  1  M  1   -2\'        V  ~~  .  J7Z.2  ,  la  .   .-2\'        i  — 


V(a2  +  *2  +  c2)'      ''-^/(a? +&+<?)'      s     V(a2  +  ^  +  0' 


xvil  MISCELLANEOUS  EXAMPLES  427 

If  we  take  account  of  (4),  (5),  (6)  we  see  that  the  upper  signs  must  go  to- 
gether throughout,  and  the  lower  together  throughout  ;  so  that  we  find  only 
two  real  solutions. 

Example  7. 

x(x-a)=yz,     y(y-b)  =  zx,     z(z-c)  =  xy  (1). 

From  the  first  two  equations  we  derive  (x  -y)  (x  +  y  +  z)  =  ax  -  by,  which, 
if  we  put  p  =  x  +  y  +  z,  may  he  written  (p-a)x=(p-b)y.  Hence,  bearing  in 
mind  the  symmetry  of  the  system,  we  have 

*= —  i    y= — i>    *= —  (2)> 

p-a      "    p-b  p-c 

where  p  and  a  have  to  he  determined. 
From  the  first  equation  of  (1)  we  have 

<x     f     cr 


p-a\p-a       )     {p~b)(p-c) 
Removing  the  factor  <r,  to  which  will  correspond  the  solution  x  —  y  =  z=0, 
we  find 

o- { (2a -  b -  c)p  +  (be  -  a") }=a(p~  a)(p  -b)(p-  c)  (3). 

Similarly  we  find 

<r{(2b-c-a)p+(ca-b"-)}=b(p-a)(p-b)(p-c)  (4). 

From  (3)  and  (4)  we  now  eliminate  <x,  observing  that  in  the  process  we 
reject  the  factors  <r,  p  -  a,  p-b,  p-c,  which  correspond  to  three  solutions, 
namely, 

x  =  a,  0,  0  ; 
y=0,  b,  0; 
2  =  0,      0,       c. 

We  thus  deduce  p  = . , 

r       a+b+c 

which    gives    one    more    solution.      We   have   in    fact    p-a  =  (bc-a")jZa, 
p-b  =  {ca-  b*)/2a,  p-c  =  (ab-  c2)IZa. 
Hence  (2)  gives 

<x    _(ca-b-)(ab-c-) 
p-a         Babe  -  2a3     ' 

and,  by  symmetry,  we  have  two  corresponding  values  for  y  and  z. 

This  example  is  worthy  of  notice  on  account  of  the  symmetrical  method 
which  is  used  for  treating  the  given  system  of  equations.  The  solution  might 
be  obtained  fully  as  readily  by  putting  x  =  u~,  y  =  vz,  and  proceeding  as  in 
§  13,  Example  3. 

Exercises  XXXIII. 

(1.)  x  +  y  =  30,     xy  =  2\Q.  (2.)  x-y=3,     x"  +  if  =  65. 

(3.)  x-+if-  =  5S,     xy  =  1\,  (4.)  x  +  y  =  8,     3x"-2xy  +  y'i=5i. 

(5.)  x  +  2y  =  x\     2x  +  y  =  y2. 

(6.)  x-  +  y-  +  2(x  +  y)  =  U,     Zxy  =  2(x  +  y). 

(7.)  x~ +  y~  —  a~,    x  +  y  =  b. 


428 


EXERCISES  XXXIII 


CHAP. 


and 


(8. 

(9. 

10. 

11. 

the 
(12. 
(14. 
(15. 
(16. 
(17. 
(18. 
(19. 

(20. 

(21. 

(22. 
(23. 
(24. 
(25. 
(26. 
(27. 
(28. 
(29. 
(30. 
(32. 
(33. 
(35. 
(36. 
(37. 
(38. 
(39. 
(40. 
(41. 
(42. 
(43. 
(44. 
(45. 
(46. 

(47. 
(48. 

(49. 
(50. 

(51. 

(52. 


a(x-  +  y2)  =px  -  qy,  b(x2  +  y2)  =  qx  -  py. 
(x  +  y)/(l+xy)=a,  {x-y)/(l  ~xy)  =  b. 
ax  +  by  =  e,     b/x  +  a/y  =  d. 

It  ax  +  by  =  1,  ex2  +  dy2  =  1,  have  only  one  solution,  then  arjc  +  b2/d  =  1, 
solution  in  question  is  x  =  a/c,  y—b/d. 

2x2-%xy  =  \,     y2  +  5xy  =  34.  (13.)  x2  +xy  =  8i,     xy  +  y2  =  60. 

x3+4xy  +  y3  =  38,     x  +  y  =  2. 
l/x2  +  l/xy  =  1/a2,     l/y2  +  l/xy  =  l/b2. 
(px  +  qy)  (x/p  +  y/q)  =  x2  +  y2  +p2  +  q2,     xjp  +  yjq  =  V5. 
x2  +  a2  =  y2  +  b2  =  {x  +  yf  +  (a  -  bf. 
(x-yf  =  a3(x  +  y),     {x  +  y)2  =  b3{x-y). 
(a2  -  b2)/(x2  +  y2)  +  (a2  +  b^/ix2  -y2)  =  l, 

3 


x2jp2-y2/q2  =  0. 


x+Z  ,y-3_0 
x-3+y+3~  ' 


x-Z       w  - 


;  =  1. 


2x+3     2y  +  3 
2(x-y)+xy  =  Bxy-(x-y)  =  7. 
(x  +  y)/7  =  8/(x  +  y  +  l),     xy=12. 
x+l/y=10/x,     y  +  l/x  =  l0x. 
Z{x2  +  y2)  -  2xy=27,     4(x2  +  y2)  -  6xy  =  16. 
cc3-?/  =  208,     x-y=L 
x2y  +  xy2  =  162,     a?  +  y3  =  243. 
x2y  +  xy2  =  30,     xiy2  +  x2y4=468. 
x3  +  y3  =  (a  +  b)(x-y),     x2  +  xy  +  y2  =  a-b. 
xi  +  x2if  +  y*=741,     x2-xy  +  y2  =  19 
xy(x  +  ij)  =  48,     x3  +  y3  =  72. 
xi  +  yi  =  Q7,     x  +  y=5. 


(31.)  x4  +  y4  =  a4,     x  +  y  =  b. 


xi  +  yi  =  {p2  +  2)x2y2,     x  +  y  =  a. 
x2-y2  =  2xy  +  x  +  y,     x3-y3  =  3xy(x  +  y). 
(x  +  y)  {x3  -  y3)  =  819,     (x  -  y)  {x3  +  y3)=  399. 
x2\y  +  y2\x  =  2,     x  +  y  =5. 


(34.)  xi  +  y5  =  33,     x  +  y=Z. 


x2y2(xi-yi)=a' 
xi-x2  +  yi-y2- 


xy(xi  +  y4)  (x2  -  y2)  =  a. 
84,     x2  +  x2y2  +  y2  =  49. 


ys/x=b2  -xy. 

i/2 


x3/y  =  a2-xy, 

x  +  y+  \J(xy)  =  14,     x2  +  y2  +  xy  =  84. 
V(l-«A')  +  V(l-«/2/)=\/(l+«/^)>     x  +  y  =  b. 
x+y+  VO*2  -  2/2)  =  a,     2ysJ{x2  -  y2)  =  V\ 
*J(x2  +  l2y)+sJ(y2  +  l2x)  =  33,     x  +  y  =  23. 

V(*/y)  +  V(y/*) = 5/2,    V(*W + V(s/7*) = 9 V2/2. 

\/{x  +  a)  +  V(2/  -  «)  =  Wa>     s/(x  ~a)  +  \/(y  -a)  =  f  \/a. 
Xs  +  y •  =a~, 


(x2  +  y2)h  +  (2xyf  =  b. 


a?+a?+y*+b*=>sl/2{z(La+y)-b{a-y)}, 

x2-a2-y2  +  b2='s/2{x(a-y)  +  b{a  +  y)\. 
(x2  +  a2)  {y2  +  b2)  =  m(xy  +  ab)2,     {x2  -  a2)  (y2  -  b2)  =  mJifix  -  ay)2. 

b      b      b 


x=y+^rr  z  ,  rr 


a     a     a 

y+  y+  y  + 

gmyn—^ym-n 

xz+y=y4a,     y 


y  =  x  + 


x+  x+  x  + 


'=uy 


*+:  '  =  :»•« 


xvii  EXERCISES  XXXIV  429 


Exercises  XXXIV. 

*(1.)  2e=0,     Saaj=0,     Zah?=ZIL{b-c). 

(2.)  (y-a){z-a)  =  bc,     (z-b)(x-b)  =  ca,     (x-e){y -c)  =  ab. 
(3.)  yz+2(y+z)=U,    zx+2{z+x)=8,     xy+2(x+y)=16. 

(4.)  ^  +  ^+;  =  4>     yz+xs+xy=tyxyz,     2zx  +  3yz=2xy. 

(5.)  z(j/  +  2)  =  24,     y{z  +  x) -18,     z(x  +  y)  =  20. 
,      (6.)  a<y+«)=y(«+a;)=a(a!+y)=l. 

(7.)  (2  +  a:)(a;  +  2/)  =  «2,     (a;  +  y) {y  +  z)  =  b2,     (y  +  z)(z  +  x)  =  c2. 
(8.)  ax  +  yz=ay  +  zx=az  +  xy=p2. 
(9.)  a;2  +  2?/2  =  128,     y2  +  2zx=15B,    z2  +  2xy=128. 
(10.)  a2(j/  +  2)2  =  a2a;2  +  l,     62(2  +  cc)2  =  &V  +  l,     c2(x  +  y)2  =  c2z2  +  1 . 
(11.)  a(i/  +  z-a;)  =  (a!  +  i/  +  z)2-2&2/,     b(z  +  x-y)  =  (x  +  y  +  zf-2cz, 

c(x  +  y-z)  =  (x  +  y  +  z)2-  2ax. 
(12. )  ZOc2  -  v/2)  -  2(a;2  -  yz)  =  a2,     ^(x2  -  yz)  -  2{y2  -zx)  =  b2, 

2(x2-yz)-2(z2-xy)  =  c2. 
(13.)  ,Zbcx=0,     2aijz  =  Q,     2a;2 =1. 

(14.)  a(x  +  yz)  =  b(y  +  zx)  =  c(z  +  xy),     x2  +  y2  +  z2  +  2xyz  =  l. 
(15.)  x(a  +  y  +  z)=y(a  +  z  +  x)  =  z(a  +  x  +  y)  =  3a(x  +  y  +  z). 
(16.)  a;2  +  ?/2  +  22=a2  +  2a;(?/4-2)-a;2,  and  the  two  equations  derived  from 

this  one  by  interchanging  -{  J- . 

(17.)  aa?=-+-t     by2  =  ~~~,     cz2=-  +  -. 
v      '  y     z'       "      z    x  x     y 

(18.)  y*z*+z*x*+xhj*=i9,     x2  +  if  +  z2  =  li,     x{y  +  z)  =  9. 

(19. )  (yz  -  **)/a?x=(zx  -  y2Wy=  {xy  -  z2)/Sz  =  l/xyz. 

(20.)  «2.c2(2/  +  2)2=(a2  +  a;2)2/222,  and  the  two   derived  therefrom  by  inter- 


changing-^}. 


(21.)  2x3  =  a{2x-2x)  =  b(2x-2y)  =  c(2x-2z). 

(22.)  (x-l)(y+z-5)=77,     (y-2)(z+x-  4)=.72,     (z-3){x+y-3)=65. 

(23.)  u{y-x)/(z-u)=a}     z(y-x)/{z-u)  =  b,     y(u-z)j{x-  y)  =  c, 

x(u-z)/(x-y)  =  d. 
(24. )  If  ar3  +  ^  +  z3  +  faeyz  =  a,      3(y2z  +  z2x  +  x2y)  =  b,      3(yz2  +  zx2  +  xy2)  =  c, 
show  that 

x  +  y  +  z  =  (a  +  b  +  c)  ,     x  +  wy  +  uPz  =  (a  +  wb  +  arc)  , 

X  +  u2y  +  uz  =  (a  +  u2b  +  wc)  , 

where  w2  +  w  +  l  =  0.     Find  all  the  real  solutions  when  a—  72,    b  =  75,    c=69. 

t  C\£     \  9  O  O  JO  o  o 

(25.)  xr-yz  —  a-,     y-  -zx  =  b",     z-  -xy  =  c-. 

*  In  this  set  of  exercises  2  and  II  refer  to  three  letters  only  ;  and  11(6 -c) 
stands  for  (b-c)(c-a)(a-b),  and  not  for  (b  -  c)  (c  -  a)  (a  -  b)  (c  -  b)(a  -c)(b~a), 
as,  strictly  speaking,  it  ought  to  do. 


430  EXERCISES  XXXV  CHAP,   xvn 

Exercises  XXXV. 
Eliminate  * 

(1.)  x  from  the  system 

ax  +  b  _  a'x  +  V  _  a"x  +  b" 

cx  +  d~c'x  +  d'~<7x  +  d"' 
(2. )  x  and  y  from 

Ix     my    a  +  b      al     bm  _a-b      x2    y2  _ 
a       b  ~ a  -  b       x       y      a+b      a2     b2 
(3.)  x  and  y  from 

x2  +  xy  =  a2,     y2  +  xy  =  b2,     x2  +  y2  —  c2. 
(4.)  x,  y,  z  from 

x(y  +  z)=a2,     y{z  +  x)  =  b2,     z(x  +  y)=c2,     xyz  =  d\ 

(5.)  x,  y,  z  from 

x     y     z     .       a.         .      b,         .     c,        . 
x  +  y  +  z=0,     -  +  |+-=0,     -(x-p)=-(y-l)=-{*-r). 

(6.)  x,  y,  z  from 

2Az2=0,     2A'x2  =  0,     2aa:=0, 

and  show  that  the  result  is 

21/  {b2(GA')  +  c2(AB')  -  «2(BC) }  =  0, 

where  (CA')-CA'  -  C'A,  &c. 

(7.)  Show  that  the  following  system  of  equations  in  x,  y,  z  are  inconsistent 

unless  r3  -  p3  =  Zrgp,  and  that  they  have  an  infinite  number  of  solutions  if  this 

condition  be  fulfilled. 

Skc3  -  Zxyz  =p3,     "Zyz  =  q2,     2z  =  r. 

Eliminate 
(8.)  x  and  y  from 

{a  -  x)  (a  -  y)  =p,     {b-x){b-y)  =  q,     (a-x)(b-y)/{b-x)(a-y)=c. 
(9.)  x,  y,  z  from 

x  +  y  -z  =  a,     x2  +  y2-z2  =  b2,     x3  +  y3-z3  —  c3,     xyz  —  a3. 
(10.)  x,  y,  z  from 

ax  +  yz  =  be,     by  +  zx  =  ca,     cz  +  xy  —  ab,     xyz  =  abc. 

(11.)  x,  y,  z  from 

2a;2 =p2,     2,3?  =  q3,     2x4  =  ?-4,     xyz  =  si. 
(12.)  x,  y,  z  from 
(x  +  a)(y  +  b){z  +  c)  =  abc,    (y-c)(z-b)  =  a2,    (z-a){x-c)  —  b2,    {x-b){y-a)  =  c2. 

(13.)  The  system 

X1X2  + y1y2  =  hi,     x&z  +  y2y3  =  kf,     .   .  .,     x„x1  +  y„y1  =  k,2, 
osi2  +  yi2  =  x-22  +  y.22=  .  .   .=xn2  +  yn2  =  a2, 
either  has  no  solution,  or  it  has  an  infinite  number  of  solutions. 

*  The  eliminant  is  in  all  cases  to  be  a  rational  integral  equation.  ' 


CHAPTEE  XVIII. 

General  Theory  of  Integral  Functions,  more 
particularly  of  Quadratic  Functions. 

RELATIONS  BETWEEN  THE  COEFFICIENTS  OF  A  FUNCTION  AND  ITS 
ROOTS — SYMMETRICAL  FUNCTIONS  OF  THE  ROOTS. 

§  1.]  By  the  remainder  theorem  (chap,  v.,  §  15),  it  follows 
that  if  a,,  a2,  .   .   .,  an  be  the  n  roots  of  the  integral  function 

p0Xn  +plXn~1  +p^n~2  +  .    .    .  +Pn-\X+  Pn  (1)> 

that  is  to  say,  the  n  values  of  x  for  which  its  value  becomes  0, 
then  we  have  the  identity 


PoXn  +  ptxn  ~ l  +  p.p:n  " L  +  .   .  .  +  pn 

=jp0(x  -  ax)(x  -  03)  .  .  .  (x-an)       (2). 

Now  we  have  (see  chap,  iv.,  §  10) 
(X  -  a,)(x  -  og)  .  .  .  (X  -  an)  =  Xn  -  P^"1  +  P2Z»-2  -...  +  (-  l)»Pn> 
where  Pt,  P2,  .  .  .,  Pn  denote  the  sums  of  the  products  of  the  n 
quantities  a,,  a2,  .  .  .,  an,  taken  1,  2,  .  .  .,  n  at  a  time  re- 
spectively. Hence,  if  we  divide  both  sides  of  (2)  by  p0,  we  have 
the  identity 

xn +Plxn-l +P*xn-2  +  ,    _       +Pn 
Pa  Pa  Pa 

=xn-Tlxn-1  +  T^n-2-.  .  . +  (-l)'lPn     (3). 
Since  (3)  is  an  identity,  we  must  have 

pl/p,=  -P„      Wl'o  =  P2,       •    •    -,      Pn/Pa  =  ( ~  1)BP«      (4). 

In  particular,  if  p0=  1,  so  that  we  have  the  function 

xn  +pl3-7l~1+p.2xn-2'  +  .   .   .  +  p,i  (5), 

then  i»1=-PlJ     #,  =  P8,     .  •  .,     i?»  =  (-l)nP«  (6). 


432  SYMMETRIC  FUNCTIONS  OF  TWO  VARIABLES  chap. 

Hence,  if  we  consider  the  roots  of  the  function 

xn  +  p&n  ~ l  +  p#n  " 2  +  .  .  .+pn_lX+  pn , 
or,  ivhat  comes  to  the  same  thing,  the  roots  of  the  equation 
xn+p1zn-1+pxn-2  +  .  .  .+pn.1x+pn  =  0, 
then  -pi  is  the  sum  of  the  n  roots;  pa  the  sum  of  all  the  products  of 
the  roots,  taken  two  at  a  time;  -p3  the  sum  of  all  the  products,  taken 
three  at  a  time,  and  so  on. 

Thus,  if  a  and  f3  be  the  roots  of  the  quadratic  function 
ax2  +  bx  +  c,  that  is,  the  values  of  x  which  satisfy  the  quadratic 
equation  ax2  +  bx  +  c  =  0,  then 

a  +  (3=  -  b/a,     a/3  =  cja  (7). 

Again,  -if  a,  /3,  y  be  the  roots  of  the  cubic  function  ax3  +  bx2 
+  c x  +  d,  then 

a  +  (3  +  y  =  -  b/a,       {3y  +  ya  +  af3  =  c/a,       a/3y=  -  d/a      (8). 

§  2.]  If  s1}  s2,  s3,  .  .  .,  sr  stand  f m-  the  sums  of  the  1st,  2nd, 
3rd,  .  .  . ,  rth  powers  of  the  roots  a  and  f3  of  the  quadratic  equation 

x2+p1x+p2  =  0  (1), 

we  can  express  s„  s,,  .  .   .,  sr  as  integral  functions  of  px  and  p2. 

In  the  first  place,  we  have,  by  §  1  (6), 

s1  =  a  +  /3=  -Pl  (2). 

Again 

S2  =  a2  +  (32  =  (a  +  (3)2-2a/3, 

=1K  -  2p2  (3). 

To  find  s3  we  may  proceed  as  follows.  Since  a  and  (3  are 
roots  of  (1),  we  have 

a2+^ia+^  =  0,     {32+p,{3+p3=0  (4). 

Multiplying  these  equations  by  a  and  [3  respectively,  and  adding, 
we  obtain 

s3  +pA+p.A  =  0  (5). 

Since  st  and  s2  are  integral  functions  of  px  and  p2,  (5)  determines 
53  as  an  integral  function  of  pl  and  p,.     We  have,  in  fact, 
h  =  -lh{p;-2p2)+p2p„ 
=  ~Px  +  3p>P*  (6). 


XVI 1 1 


SYMMETRIC  FUNCTIONS  OF.  TWO  VARIABLES  433 


Similarly,  multiplying  the  equations  (4)  by  a2  and  (?  respectively, 

and  adding,  we  deduce 

S4+P1S3 +#&=()  (7). 

Hence  s4  may  be  expressed  as  an  integral  function  of  px  and  pa, 
and  so  on. 

We  can  now  express  any  symmetric  integral  function  whatever  of 
the  roots  of  the  quadratic  (1)  as  an  integral  function  of  |>,  and  p.,. 

Since  any  symmetric  integral  function  is  a  sum  of  sym- 
metrical integral  homogeneous  functions,  it  is  sufficient  to  prove 
this  proposition  for  a  homogeneous  symmetric  integral  function 
of  the  roots  a  and  ft.  Tbe  most  general  such  function  of  the 
?-th  degree  may  be  written 

A(a'  +  ftr)  +  Ba/3(a'-2  +  jS*"2)  +  Ca2/3V~4  +^"4)  +  .    . 

that  is  to  say, 

Asr  -  Bp2  s,._2  +  Cp22  s,._4  +  .  .  .  (8), 

where  A,  B,  C  are  coefficients  independent  of  a  and  ft. 

Hence  the  proposition  follows  at  once,  for  we  have  already 
shown  that  sr,  sr.,,  sr_4,  .  .  .  can  all  be  expressed  as  integral 
functions  of  py  and  p.z. 

It  is  important  to  notice  that,  since  a  and  ft  may  be  any 
two  quantities  whatsoever,  the  result  just  arrived  at  is  really  a 
general  proposition  regarding  any  integral  symmetric  function  of 
two  variables,  namely,  that  any  symmetric  integral  function  of  two 
variables  a,  ft  can  be  expressed  as  a  rational  integral  function  of  the  two 
elementary  symmetrical  functions  px  =  -  (a  +  ft)  and  p.z  =  aft. 

There  are  two  important  remarks  to  be  made  regarding  this 
expression. 

1st.  If  all  the  coefficients  of  the  given  integral  symmetric  function 
be  integers,  then  all  the  coefficients  in  the  expression  for  it  in  terms  of 
l>i  and  p.,  will  also  be  integers. 

This  is  at  once  obvious  if  we  remark  that  at  ever)'  step  in 
the  successive  calculation  of  sly  s2,  s3,  .  .  .,  &c,  we  substitute 
directly  integral  values  previously  obtained,  so  that  the  only 
possibility  of  introducing  fractions  would  be  through  the  co- 
efficients A,  B,  C,   ...  in  (8). 

VOL.  I  2  F 


434  EXPRESSION  IN  TERMS  OF  p1  AND  p2  chap. 

2nd.  Since  all  the  equations  above  written  become  identities, 
homogeneous  throughout,  when  for  px  and  pg  we  substitute  their 
values  -  (a  + /3)  and  a/3  respectively;  and  since  ^,  is  of  the  1st 
and  p2  of  the  2nd  degree  in  a  and  /3,  it  follows  that  t?i  ever^ 
term  of  any  function  of  px  and  p2  which  represents  the  value  of 
a  homogeneous  symmetric  function,  the  sum  of  the  suffixes  *  of  the 
p's  must  be  equal  to  the  degree  of  the  symmetric  function  in  a  and  ft. 
Thus,  for  example,  in  the  expression  (6)  for  s3  the  sum  of  the 
suffixes  in  the  term  -p*,  that  is,  -piPiPi,  is  3  ;  and  in  the  term 
3p}p2  also  3. 

This  last  remark  is  important,  because  it  enables  us  to  write 
down  at  once  all  the  terms  that  can  possibly  occur  in  the  ex- 
pression for  any  given  homogeneous  symmetric  function.  All 
we  have  to  do  is  to  write  down  every  product  of  pt  and  ps,  or 
of  powers  of  these,  in  which  the  sum  of  the  suffixes  is  equal  to 
the  degree  of  the  given  function. 

Example  1. 

To  calculate  a4  +  /34  in  terms  of  p\  and#2. 

This  is  a  homogeneous  symmetric  function  of  the  4th  degree.     Hence,  by 
the  rule  just  stated,  we  must  have 

^ +  13*  =  Api*  +  Bj?^  +  Cpr, 

where  A,  B,  C  are  coefficients  to  be  determined. 

In  the  first  place,  let  /3  =  0,  so  that  ]h=  -  a,  #2=0.     We  must  then  have 

the  identity  a4sAa'.     Hence  A  =  l. 

We  now  have 

a4  +  /34s(a  +  /3)4  +  B(a  +  /3)2a/3  +  Ca2/32. 

Observing  that  the  term  a:!/3  does  not  occur  on  the  left,  we  see  that  B  must 
have  the  value  -  4. 

Lastly,  putting  a=  -/3=1,  so  that;>i  =  0,  p-2  =  -1,  we  see  that  C  =  2. 

Hence 

a'+p=pS-ipi-p»  +  2p.f. 

The  same  result  might  also  be  obtained  as  follows.     We  have 

Hence,  using  the  values  of  s2  and  s3  already  calculated,  we  have 

Si=  -]h(  -pf  +  ZpiPt)  -p-ilh2 ~  2?a)i 
=£i4-4pis.p»+2p8*. 
Example  2. 
Calculate  a6  +  ^  +  os/3sH  a'-'(f:  in  terms  ofjB]  and  jh. 

*  This  is  called  the  uxiylit  of  the  symmetric  function.     See  Salmon's 
Higher  Algebra,  §  5tJ. 


xvni  NEWTON'S  THEOREM  435 

We  have 

a5  +  /35  +  a3/32  +  a2/33  =  Kpx5  +  Efefa  +  Cpip-j1. 
Putting  /3  =  0,  we  find  A=  -  1 ;  considering  the  term  a4/i,  we  see  that  B  =  5; 
and,  putting  a  =  /3  =  l,  we  find  C=  -  6.     Hence 

a3  +  jS5  +  a*p2  +  a2^  =  -  p?  +  bpjfa  -  Spiff. 

Since  any  alternating  integral  function  *  of  a,  ft,  say  /(«,  ft), 
merely  changes  its  sign  when  a  and  ft  are  interchanged,  it  follows 
that  we  have  /(a,  ft)  =  -/(/?,  a).  Hence,  if  we  put  ft  =  a,  we 
have/(a,  a)  =  -/(a,  a);  that  is,  2/(a,  a)  =  0.  Therefore  /(a,  a)  =  0. 
It  follows  from  the  remainder  theorem  that  /(a,  ft)  is  exactly 
divisible  by  a  -  ft.  Let  the  quotient  be  <j(a,  ft).  Then  g(a,  ft) 
is  a  symmetric  function  of  a,  ft.     For  g(a,  ft)  =/(<*,  /3)/(<*  -  /?)>  and 

,/(/?,  a)  =/(/?,  a)/(/3-«)=    -f(a,ft)l(ft-a)  =  /(a,0)/(a  -  /3);  that  is, 

;/((z,  /?)  =  £(/?,  a).     Hence  any  alternating  integral  function  of  a  and 

/?  can  be  expressed  as  the  product  of  a  -  ft  and  some  symmetric 

function  of  a  and  ft.     Hence  any  alternating  function  of  a  and  ft  can 

be  expressed  without  difficulty  as  the  product  of  ±   >J(p*  -  4j»s),  and 

an  integral  function  of  p.  and  p.2. 

Example  3. 

To  express  a5/3-  a/35  in  terms  of  pi  and  ^2- 

We  have 

a5/3-  a/35=a/3(a4-  /34), 

=  (a-/3)a/3(a  +  /3)(a2  +  /32), 

=  ±  V( Pi2  -  4ft)  { Pi?'2 ( Pi*  -  2i?2)}  • 

Every  symmetric  rational  function  of  a  and  ft  can  be  ex- 
pressed as  the  quotient  of  two  integral  symmetric  functions  of 
a  and  ft,  and  can  therefore  be  expressed  as  a  rational  function 
of  px  and  p.,. 

Example  4. 

a:i  +  2a2/3  +  2a/32  +  ^     (a  +  /3)3  -  a/3(a  +  /3) 
a2/3  +  a/3*  a/3(a  +  /3) 

-7'i3  +  ;'i?'2 


_P?-Vz 
Pi 

§    3.]   The    general    proposition    established    for    symmetric 

functions  of  two  variables  can  be  extended  without  difficulty  to 

symmetric  functions  of  any  number  of  variables. 

*  See  p.  77,  footnote. 


436 


newton's  theorem 


chap. 


We  shall  first  prove,  in  its  most  general  form,  Newton's 
Theorem  that  the  sums  of  the  integral  powers  of  the  roots  of  any 
integral  equation, 

xn  +  p^xn - 1  +  paXn - 2  +  _    _    _  +  ^  _  q  (\^ 

can  be  expressed  as  integral  functions  of  px,  ps,  .  .   .,  pn,  whose  co- 
efficients are  all  integral  numbers. 

Let  the  n  roots  of  (1)  be  a,,  a2,  .  .  .,  an,  and  let  the  equation 
whose  roots  are  the  same  as  those  of  (1),  with  the  exception  of 
an  be 


y.n-1 


f'H  ii?i«        +  iPi 


.11-3 


+ 


+  iPn-i  =  0 


(2); 


also  let  the  equation  whose  roots  are  the  same  as  those  of  (1), 
with  the  exception  of  a.2,  be 

Xn~1  +  2p,Xn~2  +  2p.2Xn'3  +  .    .    .+spn-i  =  Q  (3), 

and  so  on. 
Then 

xn_1  +  j^a'1-2  +  ,p2xn~3  +  .  .   .  +  xpn-x 

=  (x?l  +p1Xn~1  +  p2Xn  ~  2  +  .    .    .  +  pn)K%  -  a,), 
=  Xn-1  +  (al+p])x^-2  +  (ai2+pla1+p.^Xn-s   .    .    . 
+  (a1r+p1a1r-1  +  .    .    .  +pr)xn-r~1  +  .    .    . 

by  chap,  v.,  §  13. 

Hence,  equating  coefficients,  we  have 

iP»  =  ai2       +?iai       +P»> 


r-l 


[pr  =  al1        +p1a1'     "  + 


+  P. 


iPn-i  =<    1+.2V*i 


«-2  + 


+Pn-i 


(3'). 


Similar   values  can    be    obtained    for  „j\,  aps,  2p3,  .  .  .,   gJ?n-i 
in  terms  of  a,  and  pltp„  .   .    .,  p»j  and  so  on. 

Taking  the  (r- l)th  equation  in  the  system  (3'),  and  multi- 
plying by  a,,  we  have 


r-l 


Similarly 
and  so  on. 


i£V-i«i  =  <*i   +j>W      + 


2pr-iOL2  =  a2r +pla2r    l  + 


+jpr-iai 


XVIII 


NEWTON  S  THEOREM 


43; 


Adding  the  11  equations  thus  obtained,  we  have 

iPr-i*i+2Pr-i<h  +  -    .    .  +  „pr-ian  =  Sr+2>lSr-l  +  .    .    .  +iV-l»j    (4)- 

Now  ,^r_,  is  the  sum  of  all  the  products  r—\  at  a  time  of  the 
n—  1  quantities  -  a,,  -  a3,  .  .  .,  -  an.  Hence  i/>r-iai  is  the  sum, 
with  the  negative  sign,  of  all  those  products  r  at  a  time  of  the 
n  quantities  -  a1?  -  a2,  .  .  .,  -  an  which  contain  a,.  Similarly 
the  next  term  contains  all  those  products  rat  a  time  in  which 
a2  occurs ;  and  so  on.  Hence  on  the  left  all  the  products  r  at 
a  time  of  the  n  quantities  -a,,  -  a2,  .  .  .,-an  occur,  each  as 
often  as  there  are  letters  in  any  such  product,  that  is  to  say,  r 
times.      Hence  the  equation  (4)  becomes 

-rpr  =  Sr+jt>1SrLl+    .    .    .    +pr-iSn 

Or  Sr+iVr-i+    •    •     •    +  Pr~  isi  +  rpr  =  0. 

This  will  hold  for  any  value  of  r  from  1  to  n  -  1,  both  inclusive. 

We  have  therefore  the  system 

si+pi  =0-| 

s2+pvst  +  2p2  =  0 

s3  +  pxsa  +pasl  +  3pa  =0  }■  (5). 


Sn-i  +PiSn-2  +  ■  •    •   (n-  l)i>»_i  =  0 


Again,  since  a,  is  a  root  of  (1),  we  have 

aIB  +  ^,a,n-1+  .    .   .  +pn  =  0. 

Similarly 


a/1  +  pta2 


+ 


■  +Pn  =  0; 

and  so  on. 

If  we  first  add  these  n  equations  as  they  stand,  then 
multiply  them  by  a,,  a2,  .  .  .,  aa  and  add,  then  multiply  them 
by  a,2,  a/,  .   .   .,  aa2  respectively,  and  add,  and  so  on,  we  obtain 

sn     +PiSn-i  +  •   •  •  +  npn  =0- 

Sn+i+Pi*n       +•    ■    •  +81pn=0    I 
Sn+a+PJn+i  +■    ■    -  +  S2pn  =  0    \ 


(6), 


and  so  on. 


J 


The  equations  (5)  and  (G)  constitute  Newton's  Formula  for 


438  INTEGRAL  SYMMETRIC  FUNCTION  CHAP. 

calculating  sn  s2,  s8,  .  .  .,  &c,  in  terms  ofpi,pa,  .  .  .,  pn.  It  is 
obvious  that  s,,  s,,  s3,  .  .  .  are  determined  as  rational  integral 
functions  of  p, ,  p2,  .  .  . ,  pn,  in  which  all  the  coefficients  are 
integral  numbers. 

A  little  consideration  of  the  formula?  will  show  that  in  the 
expression  for  sr  the  sum  of  the  suffixes  of  the  p's  in  each  term  will 
be  r. 

Hence  to  find  all  the  terms  that  can  possibly  occur  in  sr  we 
have  simply  to  write  down  all  the  products  of  powers  of  pn  p2, 
.   .  .,  pn  in  which  the  sum  of  the  suffixes  is  r. 

Example. 

To  find  the  sum  of  the  cubes  of  the  roots  of  the  equation 

a?  -  2a?  +  3a: +  1  =  0. 

We  have 

51-2  =  0,     s2-2s1  +  2x3  =  0,     53-  2s2  +  3s1  +  3  x  1  =  0. 
Hence  si  =  2,     s2=-2,     s3=-13. 

§  4.]  We  can  now  show  that  evqry  integral  symmetric  function 
of  the  roots  can  be  expressed  as  an  integral  function  of  pt,  p3,  .  .  .,  pn. 
The  terms  of  every  symmetric  function  can  be  grouped  into 
types,  each  term  of  a  type  being  derivable  from  every  other  of 
that  type  by  merely  interchanging  the  variables  a,,  a,,  .  .  .,  an 
(see  chap,  iv.,  §  22).  All  the  terms  belonging  to  the  same  type 
have  the  same  coefficient.  It  is  sufficient,  therefore,  to  prove  the 
above  proposition  for  symmetric  functions  containing  only  one 
type  of  terms.  Such  symmetric  functions  may  be  classed  as 
single,  double,  triple,  &c,  according  as  one,  two,  three,  &c, 
of  the  variables  au  a2,  .  .  .,  an  appear  in  each  term.  Thus 
^a,^,  ^a,^a/,  ^a^a^a/,  &c,  are  single,  double,  triple,  &c, 
symmetric  functions. 

For  the  single  functions,  which  are  simply  sums  of  powers, 
the  theorem  has  already  been  established.  We  can  make  the 
double  function  depend  on  this  case  as  follows : — 

Consider  the  distribution  of  the  product 

(tt,P  +  a.,P  +  .    .    .  +  aHP)  (a,?  +  aj  +  .    .    .  +  a^). 

Terms  of  two  different  types,  and  of  two  only,  can  occur,  namely, 


XVIII 


ORDER  AND  WEIGHT  439 


terms  derivable  from  a?a£,  that  is,  af+%  and  terms  derivable 
from  a^a22.     We  have  in  fact 

SpSq  =  SttjP+S  +  ^a.PaJ. 

Hence  Sa^cu?  =  spsq  -  sp+q. 

Now  sp,  sq,  sp+q  can  all  be  expressed  as  integral  functions  of 

PitPsi  •   ■  •>  Pn-     Hence  the  same  is  true  of  lafa^. 

Here  we  have  supposed  p  4=  q.  If  p  =  q,  then  the  term  a^a/ 
will  occur  twice,  and  we  have 

sp2  =  2ai2*  +  S2*?aJ>  ; 
but  this  does  not  affect  our  reasoning. 

The  case  of  triple  functions  can  be  made  to  depend  on  that 
of  double  and  single  functions  in  a  similar  way.  In  the  distri- 
bution of 

(ttj*  +  <%»  +  ...  +  a/)  (a,?  +  a?  +  .  .  .  +  a,?)  (a,r  +  a/  +  .  .   .  +  a/) 

every  term  is  of  the  form  aMpa/awr,  where  m,  v,  w  are,  1st,  all 
different ;  2nd,  such  that  two  are  equal ;  3d,  all  equal.  Any 
particular  term  can  occur  only  once  if  p,  q,  r  be  all  unequal. 
Hence  we  have 

SpSgSr  =  SoAsW  +  2af+W  +  Sa^+W  +  2<+2V  +  W+9+r- 
In  the  last  equation  every  term,   except  Safafaf,  can  be  ex- 
pressed as  an  integral  function  oiplfp2,  .  .  .,pn.     Hence  'Zafaja/ 
can  be  so  expressed. 

If  two  or  more  of  the  numbers  p,  q,  r  be  equal,  tlien  each 
term  of  lafa^a/  will  occur  a  particular  number  of  times ;  and 
the  same  is  true  of  certain  of  the  other  terms  in  the  equa- 
tion last  written.  But  this  does  not  affect  the  conclusion  in 
any  way. 

We  can  now  make  the  case  of  quadruple  symmetric  functions 
depend  on  the  cases  already  established ;  and  so  on.  Hence  the 
proposition  is  generally  true. 

It  is  obvious,  from  the  nature  of  each  step  in  the  above  pro- 
cess, and  from  what  has  been  already  proved  for  s,,  s.,,  s3,  .  .  ., 
that  in  the  expression  for  any  homogeneous  symmetric  function  of 
degree  r  the  sum  of  the  suffixes  of  the  p's  will  be  r  for  each  term ; 
so  that  we  can  at  once  write  down  all  the  terms  that  can  possibly 


440  GENERAL  STATEMENT  OF  THEORY  CHAP. 

occur  in  that  expression,  and  then  determine  the  coefficients  by 
any  means  that  may  happen  to  he  convenient. 

It  is  important  to  remark  that  the  degree  in  plt  p.,,  .  .  . ,  pn 
of  the  expression  for  'Eafa^a.f  .  .  .  in  terms  of  plt  ps,  .  .  .,pn 
must  be  equal  to  the  highest  of  the  indices  p,  q,  r  .  .  .  For,  let 
the  term  of  highest  degree  he  p^ipfo .  . .  p7^n,  then,  since 
P\  -  \P\  ~  «d  Pz  =  iPa  -  \P\0-ii  where  $lf  ,j?2,  &c,  do  not  contain  a1}* 
we  see  that  p^lp.2x* .  . .  pnXn,  when  expressed  in  terms  of 
a,,  a2,  .  .  .,  an,  will  introduce  the  power  a,^i  +  X2+'  '  +  *»  with 
the  coefficient  (  —  l)niPi^p3 3  . . .  i^n-i*"-  Now,  since  there 
are  no  terms  of  higher  degree  than  p^ipfo . .  .  p,^n,  if  the 
power  a^i  +  xi  +  -  ■  •+x»  occur  again,  it  must  occur  as  the  highest 
power,  resulting  from  a  different  term  of  the  same  degree  ;  that 
is  to  say,  it  will  occur  with  a  different  coefficient  and  cannot 
destroy  the  former  term.  Hence  the  index  of  the  highest 
power  of  any  letter  in  the  symmetric  function  must  be  equal 
to  the  degree  of  the  highest  term  in  its  expression  in  terms  of 

PoPm,    ■    ■    •,   VnA 

Although,  in  establishing  the  leading  theorem  of  this  para- 
graph, we  have  used  the  language  of  the  theory  of  equations, 
the  result  is  really  a  fundamental  principle  in  the  calculus  of 
algebraical  identities ;  and  it  is  for  this  reason  that  we  have 
introduced  it  here.     We  may  state  the  result  as  follows : — 

elementary  symmetric  functions  of  the  system  of  n  variables 
xux2,  .  .  .,  xn.  Then  we  caii  express  any  symmetric  integral  function 
of  sc, ,  o:2,  .  .  .,  xn  as  an  integral  function  of  the  n  elementary 
symmetric  functions ;  and  therefore  any  rational  symmetric  function 
of  these  variables  as  a  rational  function  of  the  n  elementary  symmetric 
functions. 

On  account  of  its  great  importance  we  give  a  proof  of  this 

*  They  are,  in  fact,  the  functions  of  a2,  ag, .  .  .,  a„  defined  in  §  3.     See 
Exercises  xxxvi.,  51. 

t  Salmon,  Higher  Algebra,  §  58. 


XVIII 


PROOF  OF  GENERAL  THEOREM  441 


proposition  not  depending  on  Newton's  Theorem  (which  is  itself 
merely  a  particular  case).* 

Let  nq„  nqa,  .  .  .,  n<ln  denote  the  n  elementary  symmetric 
functions  of  the  %  variables  xlt  x2,  .  .  .,  xm  that  is  to  say, 
2nK,,  2n.r,in,,  •  •  -,  xlxa...xn;  and  let  „_,&,  „_,&,  •  •  •»  n-tfn-i 
denote  the  n~\  elementary  symmetric  functions  of  xx,  x2,  .  .  .,%_,, 
that   is,    2a;,,   ?  x,r2,  .   .   .,  sea .  .  .  xn^.      It    is    obvious    that, 

?!  —  1  ?(— 1 

when  xn  =  0,  ££,,  nq2,  .  .  .,  n<ln-i  become  „_,£,,  „_,&,  .  .  .,  n-fln-i 
respectively. 

Let  us  now  assume  that  all  symmetric  integral  functions  not 
involving  more  than  n  -  1  variables  can  be  expressed  as  integral 
functions  of  „_,?,,  n-i?8j  .  .  .,  n-i?n-i-  Let/(:r.,,  a-a,  .  .  .,  »„_„  «w) 
be  any  symmetric  integral  function  of  the  «  variables  x„  x„  .  .  .,  £„, 
Then  /(a;,,  a:*,  .  .  .,  arn_,,  0)  is  a  symmetric  integral  function  of 
xu  x2,  .  .  .,  xn_„  and  can  therefore,  by  hypothesis,  be  expressed 
integrally  in  terms  of  „_,?„  »-,&,  •  •  •,  n-iin-i-  Let  this  ex- 
pression be  <K»-i?»  »-i2«  ■  •  •»  n-rfn-Oj  so  that  <£  is  a  known 
function. 

Now  assume 

+  xj/(xl,  x2,   .  .  .,  %_,,  .r„)     (7). 

Then,  since  <£(»&,  n</2,  .  .  .,  n3W-i)  is  a  symmetric  integral 
function  of  a,,  x2,  .  .  .,  xm  if/(x1}  x,,  .  .  .,  xn_„  a^)  is  obviously 
a  symmetric  integral  function  of  these  variables. 

If  we  put  xn  =  0  on  both  sides  of  the  identity  (7),  then 

J\XX,  X2,    .     .    .,    Xn_u   0)  —  <p{n-\(lu  n-^1-21    •    •    '}  n-iQn-i) 

+  xf (./-,,  Xs,   .    .    .,    Xn.\,  0)       (8). 

But/(.r,,  ..',,  .  .  .,  arB_„  0)  =  <f>(n_lq1,  w_,2„  .  .  .,  „_,£„_,)•  Hence, 
by  (8),  )/<(>,,  x2,  .  .  .,  a^_19  0)  =  0.  Therefore  the  integral 
function  \f/(xl}  x2,   .   .  .,  xn_u  xn)  is   exactly  divisible   by  some 


*  This  proof  is  taken  from  a  paper  by  Mr.  R.  E.  Allardice,  Pruc.  Edinb. 
Math.  Soc.  for  1889. 


442  PROOF  OF  GENERAL  THEOREM  chap. 

power  of  xn,  say  xn*  ;  hence,  on  account  of  its  symmetry,  also  by 
x*,  x",   .   .  .,  xn_".     We  may  therefore  put 

lf,(x1}  «b,    .    .    .,    Xn-1,Xn)=nqnfi(Vi,Xa,    •    ■    ■^n-i^n), 

where  /,  is  a  symmetric  integral  function  of  a,,  Kg,  .  .   .,  %  of 
lower  degree  than  / 

We  can  now  deal  with  fx  in  the  same  way  as  we  dealt  with 
f;  and  so  on.  We  shall  thus  resolve  f(xu  x2,  .  .  .,  xn_u  xn) 
into  a  closed  expression  of  the  form 

<f>  +  n2»"V.  +  nqnai+x%2  +  •   •   •  +  .fo"1  W  •  •  '  +K'n  *.     (9), 
where  <£,,   4>,,  .   .   .,  <f>m  are,  like  <f>,  all  known  functions  of  nqx, 
n<l>,  •  •   .,  «?«->,  or  else  constants. 

If,  therefore,  the  integral  expression  in  question  be  possible 
for  n  -  1  variables,  it  is  possible  for  n  variables. 

Now  every  integral  function  of  a  single  variable,  xn  is  a 
symmetric  function  of  that  variable,  and  can  be  expressed 
integrally  in  terms  of  //,,  which  is  simply  .t,.  Hence  it  follows 
by  induction  that  every  symmetric  integral  function  of  n  variables 
can  be  expressed  as  an  integral  function  of  the  n  elementary 
symmetric  functions. 

Cor.  It  follows  at  once,  by  induction,  from  the  form  of  (9)  that  the 
coefficients  of  the  expression  for  any  symmetric  integral  function 
/(»„  x,2,  .  .  .,  xn)  in  terms  of  nqu  nqa,  .  .  .,  nqn  are  integral 
functions  of  the  coefficients  off  In  particular,  if  the  coefficients  of  f 
be  integral  numbers,  the  coefficients  of  its  expression  in  terms  of 
n°i>  w&j  •   •  •>  nQn  w^  a^so  be  integral  numbers. 

We  now  give  a  few  examples  of  the  calculation  of  symmetric 
functions  in  terms  of  the  elementary  functions,  and  of  the  use  of 
this  transformation  in  establishing  identities  and  in  elimination. 

Example  1. 

If  a,  /3,  7  be  the  roots  of  the  equation 

gX-pja?  +p2x  -^3  =  0, 

express  /33>  +  fiy3  +  -/a  +  ya?  +  a?p  +  a/33  in  terms  of  ;j1;  p2,  ]h- 

Here  we  have;>i  =  Za,  p-i='Lap,  ps  =  af3y.     Remembering  that  no  term  of 
higher  degree  than  the  3rd  can  occur  in  the  value  of  2a3/3,  we  see  that 


XVIII 


EXAMPLES  443 


2a3£  =  Aprp-i  +  Bpa  &  +  Cp-r  ( 1 ), 

where  A,  B,  C  are  numbers  which  we  have  to  determine. 

Suppose  7  =  0  ;  then  2h  =  a  +  P,  P-2  =  *P,  J>s=0  ;  and  (1)  becomes 
a3(3  +  aps= A(o  +  /3)2a/3  +  Ca2/52  ; 
that  is  to  say,  a2  +  /32  =  A(a  +  /3)2  +  Ca/3. 

Hence  A  =  l,     C=-2. 

We  now  have  2a3/3  =^i2^2  +  Bpi p3  -  2p22. 

Let  a =/3=7 = 1,  so  that  pi = 3,  ^a = 3,  p» = 1 .     We  then  have 

6  =  27  +  3B-18. 
Hence  B=  - 1. 

Therefore,  finally,  2a3/3  =£1^2  -  p^  -  2i>22. 

In  other  words,  we  have  the  identity 

2a3/3=(2a)22a/3  -  a/372a  -  2(2a/3)2. 
Example  2. 
To  show  that 
{yz  -  xu )  (zx  -  yu)  (xy  -  zu) = (yzu  +  zux + uxy  +  xyzf  -  xyzu(x  +  y  +  z  +  u)2      (2). 
The  left-hand  side  of  (2)  is  a  symmetric  function  of  a,  y,  z,  u.     Let  us  calcu- 
late its  value  in  terms  of/?i  =  2a:,  /?2  =  2xy,  p3-Y.xijz,  pi  =  xyzu. 

Since  the  degree  of  U(yz  -  xu)  in  x,  y,  z,  u  is  6,  and  the  degree  in  z  alone 
is  3,  we  have 

U(yz  -  xu)  =  Api2pi  +  Bpip^&t  +  Cp23  +  BpsPi  +  Ep32  (3). 

If  we  put  u  =  0,  then  pi  =  ~Z3x,  p2  =  23xy,  p3  =  xyz,  pt=0,  where  the  suffix 
3  under  the  2  means  that  only  three  variables,  x,  y,  z,  are  to  be  considered.  If 
Pi,  lh,  Pz  have  for  the  moment  these  meanings,  then  (3)  becomes  the  identity 

^32 = BpiPsPa  +  Cpi  +  Ep32. 
Hence  B  =  0,     C=0,     E=l. 

Hence  Jl(yz  -  xu)  =  Aprp*  +  Vp-iPi  +  P3*  (4)- 

Now  let  x  =  y  =  l,  and  z  =  u- -\,  so  thatj9i  =  0,  #2= -2,  ^3=0,  pt  =  l. 

Then  (4)  becomes 

0=-2D. 

Hence  D  =  0. 

We  now  have  II  (yz  -  xu) = Apfp*  +p32. 

In  this  put  x  =  y  =  z-u  =  l,  and  we  have 

0  =  16A  +  16. 

Hence  A=  - 1. 

Hence,  finally,  H(yz - xu)=p32  - p^p*, 

which  establishes  the  identity  (2). 

Example  3. 

If  x  +  y  +  s  =  0,  show  that 
gn  +  yii  +  8u_^±^±j»    x*  +  f  +  z*    (xs  +  y^  +  z3)3    x2  +  y2  +  z2 

11  ~         3  "  2  9  2  '  ;' 

( Wolstcnholme.) 


444  EXAMPLES  chap. 

If^>1=Sar,  p2  =  ?,xy,  p3-xyz,  s3  =  2£2,  s3=2.r3,  &c,  then  we  are  required  to 
prove  that 

su     s$sa     s-/s2  ._,. 

11  _"6"  ""18  (    ,- 

We  know  that  sn  is  a  rational  function  of^i,  Pi,  lh-  I'1  the  present  case 
Pi  =  0,  and  we  need  only  write  down  those  terms  which  do  not  contain  px. 
We  thus  have 

9n  =  AfrY  +  Bpaps*  (6), 

provided  x  +  y  +  z=0. 

A  may  be  most  simply  determined  by  putting  z  =  -(x  +  y),  writing  out 
both  sides  of  (6)  as  functions  of  x  and  y,  dividing  by  xy,  and  comparing  the 
coefficients  of  a;9.     We  thus  find  A  =  11. 

We  have  therefore 

sn  =  llp24p3  +  B2]2P3S- 
In  this  last  equation  we   may  give  x,  y,  z  any  values   consistent   with 
x  +  y+z=0,  say  x=2,  y=  -1,  z=  -1.     We  thus  get  B=  -  11.     Hence 

Sn  =  1  lp24P3  ~  1  l&&£  (  7  )• 

In  like  manner  we  have 

s8  =  Ap2i  +  Bp2ps2- 
Putting  in  this  equation  first  x=l,  y=  -  1,  z  —  0,  and  then  x  =  2,  y  —  -  1, 
z=  -1,  we  find  A=2,  B=  -8. 

Hence                                 s8  =  Ip-t  -  8p-2p32  ( 8 ). 

We  also  find                             S3  =  3jt?3  (9), 

s,=  -2p2  (10). 

From  (8),  (9),  and  (10)  we  deduce 

T  -  IT  =^4  -  4^2)  +  3^' 

"IV 
which  is  the  required  equation. 

Since  we  have  four  equations,  (7),  (8),  (9),  (10),  and  only  two  quantities, 
P2,  Ps,  to  eliminate,  we  can  of  course  obtain  an  infinity  of  different  relations, 
such  as  (5) ;  all  these  will,  however,  be  equivalent  to  two  independent  equa- 
tions, say  to  (5),  and 

7258  =  952''  +  4.V:"  (11). 

Example  4. 

Eliminate  x,  y,  z  from  the  equations  x  +  y  +  z  =  0,  xi  +  y'i  +  z*  =  a,  x^  +  if  +  z5 
=  6,  x7  +  y7  +  z7  =  c. 

Using  the  same  notation  as  in  last  example,  we  can  show  that 

s3  =  3;>3 ,     SS  =  -  5;j2;>3  ,     $7  =  7prj>:i  ■ 
Our  elimination  problem  is  therefore  reduced  to  the  following  :  — 
To  eliminate p%  andf7s  from  the  equations 

3y'3 =a,      -  5pa  Pi  =  !>,     "p-fl  '3  =  <". 
This  can  be  done  at  once.     The  result  is 

2W  -25oc=0. 


xvin  EXERCISES  XXXVI  445 

Exercises  XXXVI. 

a  and  /3  being  the  roots  of  the  equation  x2+px  +  q  =  0,  express  the  follow- 
ing in  terms  of  p  and  q  : — 

(1.)  a»  +  /3»  (2.)(a«  +  /3«)/(a-/3)2.  (3.)  a~5  +  /3-3.  (1 )  a"5  - /3~5. 

(5. )  (a:1  +  /3s)-1  +  (a3  -  /3»)-i.  (6. )  (1  -  a)2/32  +  (1  -  /3)V. 

(7.)  If  the  sum  of  the  roots  of  a  quadratic  be  A,  and  the  sum  of  their 
cubes  B3,  find  the  equation. 

(8.)  If  s„  denote  the  sum  of  the  nth  powers  of  the' roots  of  a  quadratic, 
then  the  equation  is 

(SnS»-2  -  S„-i2)x2  -  (s„+iS„_o  -  SnSn_i)x  +  (sn+1Sn-i  -  Sn2)  =  0. 

(9.)  If  a  and  /3  be  the  roots  of  x2+px  +  q  =  0,  find  the  equation  whose 
roots  are  (a-h)2,  (/3-A)2. 

(10.)  Prove  that  the  roots  of 

x2  -  {2p-q)x+p2  -pq  +  q2  =  0 
are  p  +  uq,  p  +  u-q,  w  and  or  being  the  imaginary  cube  roots  of  1. 

(11.)  If  a,  /3  be  the  roots  of  x*  +  z  +  l,  prove  that  a"  +  /3"  =  2,  or  =  -  1, 
according  as  n  is  or  is  not  a  multiple  of  3. 

(12.)  Find  the  condition  that  the  roots  of  ax2  +  bx  +  c  =  0  may  be  deduc- 
ible  from  those  of  a'x2  +  b'x  +  c'  —  0  by  adding  the  same  quantity  to  each  root. 

(13.)  If  the  differences  between  the  roots  of  x3+px  +  q  =  0  and  x2  +  qx+p 
—  0  be  the  same,  show  that  either  p  =  q  or  p  +  q  +  4  =  0.  What  peculiarity  is 
there  when  p>  =  q1 

Calculate  the  following  functions  of  a,  j3,  y  in  terms  of^!  =  2a,  j?2  =  Sa/3, 
p3  =  aj3y:— 

(14.)  a.2/py  +  p2/ya  +  y2/ap.  (15.)  a~s  +  ^5  +  y-s. 

(16.)  (/ja+yxy+oW  +  Zn  (17.)  Z(a2  +  /37)/(a2-/37). 

(18.)  2(/3-7)'.  (19.)  Z(a-0)2(/3-7)2.  (20.)  2(/3  +  7)\ 

Calculate  the  following  functions  of  a,  /3,  7,  5  in  terms  of  the  elementary 
symmetric  functions  : — 

(21.)  Za\        (22.)  Sa-3.        (23.)  2a2/32.       (24.)  2a2/37.        (25.)  2(a+/3)* 

(26. )  If  a,  /3,  7,  3  be  the  roots  of  the  biquadratic  ar1  +p1x:i  +p2x2  +psx  +p4  =  0, 
find  the  equation  whose  roots  are  /37  +  a5,  ya  +  {15,  a^  +  yd. 

(27.)  If  the  roots  of  x2 -2hr+p2  —  0,  x2 -q1x  +  q2  =  Q,  x2-rix  +  r2  =  0,  be  /3, 
y ;  y,  a  ;  a,  /3  respectively,  then  a,  /3,  7  are  the  roots  of 

K3  -  Ki»i  +  ?i  +  ^i)*2  +  (#!  +  q-i+  r2)x  -  hiPilin  ~PiPa  -  q\q-i  -  nr2)  =  0. 
(28. )  If  a,  p,  y  be  the  roots  of  x3  +px  +  q  =  0,  show  that  the  equation  whose 
roots  are  a  +  /37,  /3  +  ya,  y  +  a/3,  is  Xs  -px2  +  {p  +  3q)x  +  q-(p  +  q)2  —  0. 
(29.)  If  a,  j8,  7  be  the  roots  of 

p/(a  +  x)  +  q/(b  +  x)  +  r/{c  +  x)  =  1, 
show  that  p  =  (a  +  a)  (a  +  /3)  (a  +  7)/(a  -  6)  (a  -  c). 

If  a,  /3  be  the  roots  of  x2+pix+p2  =  0,  and  a',  (3'  the  roots  of  x2+pi'x+p2 
=  0,  express  the  following  in  terms  of  p\,  p2,  p{,  p2  : — 
(30.)   (a'-a)(/3'-/3)+V-/3)(/3'-«). 


446  EXERCISES  XXXVI  CHAP. 

(31. )   (a'-a)'  +  (/?'  -  jB)«  +  (a'  -  /3)2  +  (/3'  -  a)*. 
(32.)  (a  +  a')(/3  +  /3')(a  +  /3')(/3  +  a'). 
(33.)   4(a-a')(a-/3')(/3-a')(/3-/3'). 
[The  result  in  this  case  is 

icft-y*)" + ♦(pi-ftO  (pip-2-piP2) = (2P-2 + 2p2'-PlPlr-{pi'2-  if*)  bi'2-  ^m 

(34.)  A,  A'  and  B,  B'  are  four  points  on  a  straight  line  whose  distances, 
from  a  fixed  point  0  on  that  line  (right  or  left  according  as  the  algebraic 
values  are  positive  or  negative),  are  the  roots  of  the  equations 
ax2  +  bx  +  c  =  0,     a'x2  +  b'x  +  c'  =  Q. 

If  AA'.BB'  +  AB'.BA'  =  0, 

show  that  1m'  +  2c 'a  -W  =  0; 

and  if  AA'.BA'  +  AB'.BB'=0, 

that  2c«'2  -  2cW  +  ab'2  -  a'W  =  0. 

(35.)  a,  j3  are  the  roots  of  x-~2ax  +  b2  =  0,  and  a',  (3'  the  roots  of 
x2  -  2cx  +  d-  =  0.     If  aa'  +  /3/3'  =  4w2,  show  that 

(a2-b2)(c2-d2)  =  {ae-2n-)2. 

(36.)  a,  /3,  a',  /3',  being  as  in  last  exercise,  form  the  equation  whose  roots 
are  aa'  +  /3/3',  a/3'  +  a'/3. 

(37.)  If  the  roots  of  ax2  +  bx  +  c  =  0  be  the  squai'e  roots  of  the  roots  of 
a'x2  +  b'x  +  c'  =  0,  show  that  a'b2  +  a-b'  =  2aa'c. 

(38.)  Show  that  when  two  roots  of  a  cubic  are  equal,  its  roots  can  always 
be  obtained  by  means  of  a  quadratic  equation. 

Exemplify  by  solving  the  equation  12a.13  -  56a;2  +  87a;  -  45  =  0. 

(39.)  If  one  of  the  roots  of  the  cubic  a?+pia?+p^xs+ps=0  be  equal  to  the 
sum  of  the  other  two,  solve  the  cubic.  Show  that  in  this  case  the  coefficients 
must  satisfy  the  relation 

Pi8-4pj#s+8p8=0. 

(40.)  If  the  square  of  one  of  the  roots  of  the  cubic  xs+piX2+p2X+2>3=0  be 
equal  to  the  product  of  the  other  two,  show  that  one  of  the  roots  is  -JJg/pi ; 
and  that  the  other  two  are  given  by  the  quadratic 

PiP-ix-  +2h(Pi"  -p-i)x  +2}i2P3  =  °- 
As  an  example  of  this  case,  solve  the  cubic 

x3  -9a;2-  63a;  +  343  =  0. 
(41.)  If  two  roots  of  the  biquadratic  xi+pix3+p<c2+p3x+pi  =  0  be  equal, 
show  that  the  repeated  root  is  a  common  root  of  the  two  equations 
4X3  +  ZpiX2  +  2p»z  +  ]>3  =  0,     ./;4  +  pX7?  +  p&p  +2)3x  +  p4  =  0. 
(42.)  If  the  three  variables  x,  y,  z  be  connected  by  the  relation  2x—xyz, 
show  that  22a:/(l  -  x2)  =  U2x/{1  -  x2). 

(43.)  If  2z  =  0,  show  that  22a.-7  =  1xijzZx\ 
(44.)  If  Saj=0,  show  that  Zxs=2{2yz)i  -  8x2ifz2Zyz. 

(45.)  If  Sa=0  (three  variables),  then  (2(6» - e?)/a3)  (Za^ft8 - <?) )  =s 
36-4(2a:,)(2a-3). 

(46.)  If  2ar*  =  Q,  2.t4  =  0  (three  variables),  show  that  Zx5  +  xyz{{y-z)(z-x) 


xviii        DISCRIMINATION  OF  THE  ROOTS  OF  A  QUADRATIC  447 

(47.)  Ifas+y+2+tt=0,  show  that  (2a?yi=9{2xyzf=m(yz-xu). 
(48.)  Under  the  hypothesis  of  last  exercise,  show  that 
ux{  u  +  xf  +  yziu-xf  +  uy(u  +  yf  +  zx(u  -  yf  +  uz(u  +  zf  +  xy(ic  -  zf  +  ixyzu  =  0. 
Eliminate  x,  y,  z  between  the  equations 

<»•><;)='.  *(:)*="■  =©'""•  KS)'-*1. 

(50.)  Sa?=aa,     Zxy  =  V,     2xhf  =  c\     Zx*  =  d\ 

(51.)  Show  that  Pi  =  Bp\-ai,  P2  =  >P2~  >P\*s,  •  •  ;  Pr= tPr~  »Pr-\**i  ■  ■  ; 
p„— - ,2hi-io.s,  where 2h> P2>  •  •  •>  tPi>  iPz>  •  •  •  have  the  same  meanings  as 
in  §  3. 

SPECIAL   PROPERTIES    OF    QUADRATIC    FUNCTIONS. 

§  5.]  Discrimination  of  Boots. — We  have  already  seen  (chap, 
xvii.,  §  4)  how,  without  solving  a  quadratic  equation,  to  dis- 
tinguish between  cases  where  the  roots  are  real,  equal,  or  imag- 
inary. There  are  a  variety  of  other  cases  that  occur  in  practice 
for  which  it  is  convenient  to  have  criteria.  These  may  be  treated 
by  means  of  the  relations  between  the  roots  and  the  coefficients 
of  the  equation  given  in  §  1  of  the  present  chapter.     If  a,  ft  be 

the  roots  of 

az*  +  bx+c  =  0  (1), 

then  a  +  ft  -  -  b/a,     aft  =  cja. 

If  both  a  and  ft  be  positive,  then  both  a  +  ft  and  aft  are  posi- 
tive. Conversely,  if  aft  be  positive,  a  and  ft  must  have  like 
signs ;  and  if  a  +  ft  be  also  positive,  each  of  the  two  signs  must 
be  positive ;  but  if  a  +  ft  be  negative,  each  of  the  two  signs 
must  be  negative.  Hence  the  necessary  and  sufficient  condition  that 
both  roots  of  (1)  be  positive  is  that  b/a  be  negative  and  cja  positive; 
and  the  necessary  and  sufficient  condition  that  both  roots  be  negative  is 
tin  if  hja  be  positive  and  cja  positive.  This  presupposes,  of  course, 
that  the  condition  for  the  reality  of  the  roots  be  fulfilled,  namely, 
b2  -  iac  >  0. 

Reality  being  presupposed,  the  necessary  and  sufficient  condition 
that  the  roots  have  opposite  signs  is  obviously  that  cja  be  negative. 

The  necessary  and  sufficient  condition  that  the  two  roots  be  numeric- 
ally equal,  but  of  opposite  sign,  is  a  +  ft  =  0,  that  is,  b/a  =  0. 

If  one  root  vanish,  then  aft  =  0  ;  and,  conversely,  if  aft  =  0, 
then  at  least  one  of  the  two,  a,  ft,  must  vanish.     Hence  the  neces- 


448  INFINITE  ROOTS 


CHAP. 


sary  and  sufficient  condition  for  one  zero  root  is  cja  -  0,  that  is,  c  =  0, 
a  being  supposed  finite. 

If  both  roots  vanish,  then  a/3  =  0  and  a  +  f3  =  0  ;  and,  con- 
versely, if  a/3  =  0  and  a  +  (3  =  0,  then  both  a  =  0  and  (3  =  0;  for 
the  first  equation  requires  that  either  a  =  0  or  (3  =  0,  say  a  =  0  ; 
then  the  second  gives  0  +  (3  =  0,  that  is,  (3  =  0  also.  Hence  the 
necessary  and  sufficient  condition  for  two  zero  roots  is  c/a  =  0,  b/a  =  0, 
that  is,  a  being  supposed  finite,  c  —  0,  b  =  0. 

The  two  last  conclusions  have  already  been  arrived  at  in 
chap,  xvii.,  §  2.  Perhaps  they  will  be  more  fully  understood  by 
considering  the  case  as  a  limit.  Let  us  suppose  that  the  root  a 
remains  finite,  and  that  the  root  (3  becomes  very  small.  Then 
a/3  becomes  very  small,  and  approaches  zero  as  its  limit,  while 
a  +  (3  approaches  a  as  its  limit.  In  other  words,  c/a  becomes 
very  small,  and  -  b/a  remains  finite,  becoming  in  the  limit  equal 
to  the  finite  root  of  the  quadratic. 

If  both  a  and  (3  become  infinitely  small,  then  both  a  +  (3  and 
a/3,  that  is  to  say,  both  -  b/a  and  c/a,  become  infinitely  small. 

Infinite  Boots. — If  the  quadratic  (1)  have  no  zero  root,  it  is 
equivalent  to 

that  is,  if  £=  1/x,  to 

c£2  +  b£  +  a  =  0  (2). 

The  roots  of  (2)  are  1/a  and  \/(3;  and  we  have  1/a+  1/(3 
=  -  b/c,  l/a/3  =  a/c.  Let  us  suppose  that  one  of  the  two,  a,  f3, 
say  (3,  becomes  infinitely  great,  while  the  other,  a,  remains  finite  j 
then  \/f3  becomes  infinitely  small,  and  l/a/3,  that  is,  a/c,  becomes 
infinitely  small,  while  l/a+l//3,  that  is,  -b/c,  approaches  the 
finite  value  1/a.  Hence  the  necessary  and  sufficient  condition 
that  one  root  of  (1)  be  infinite  is  a  =  0,  c  being  supposed  finite. 

In  like  manner,  the  condition  that  two  roots  of  (1)  become 
infinite,  that  is,  that  two  roots  of  (2)  become  zero,  is  a  =  0,  b  =  0. 

If  therefore  in  any  case  where  a  quadratic  equation  is  in 
question  we  obtain  an  equation  of  the  form  bx  +  c  =  0,  or  an  equa- 
tion of  the  paradoxical  form  c  =  0,  ice  conclude  that  one  root  of  the 


XVIII 


TABLE GENERAL  RESULTS CUBIC 


449 


quadratic  lias  become  infinite  in  the  one  case,  and  that  the  two  roofs 
have  become  infinite  in  the  other. 

For  convenience  of  reference  we  collect  the  criteria  for  dis- 
criminating the  roots  in  the  following  table  : — 


Roots  real 

i 
b"-4ac>0. 

Both  roots  negative 

c/a  +  ,    b/a  +  . 

Roots  imaginary 

b-  -  4ac  <  0. 

Roots    of    opposite 

Roots  equal    . 

b--4ac  =  0. 

signs  . 

c/a- . 

Roots    equal    with 

One  root   =0 

c  =  0. 

opposite  signs 

b  =  0. 

Two  roots  =  0 

b  =  0,  c  =  0. 

Both  roots  positive 

c/a  +  ,    bja- . 

One  root   =  qo 

a  =  0. 

Two  roots  =  oc 

b  =  0,  «  =  0. 

§  6.]  The  reader  should  notice  that  some  of  the  results  em- 
bodied in  the  table  of  last  paragraph  can  be  easily  generalised. 
Thus,  for  example,  it  can  be  readily  shown  that  if  in  the  equation 

p0xn+plxn-1+  .   .   .  +pn  =  0  (1) 

the  last  r  coefficients  all  vanish,  then  the  equation  will  have  r  zero 
roots  ;  and  if  the  first  r  coefficients  all  vanish  it  will  have  r  infinite 
roots. 

Again,  if  pt  =  0,  the  algebraic  sum  of  the  roots  will  be  zero ; 
and  so  on. 

It  is  not  difficult  to  find  the  condition  that  two  roots  of  any 
equation  be  equal.  AVe  have  only  to  express,  by  the  methods 
already  explained,  the  sjanmetric  function  TI(ai  -  a,)2  of  the  roots 
in  terms  of  p0,  pu  .  .  .,  pn,  and  equate  this  to  zero.  For  it  is 
obvious  that  if  the  product  of  the  squares  of  all  the  differences 
of  the  roots  vanish,  two  roots  at  least  must  be  equal,  and  con- 
versely. 

For  example,  in  the  case  of  the  cubic 

a?+pix2+p2x +2^3-0  (2), 

whose  roots  are  a,  /3,  7,  we  find 

(/3  -  7)2(7  -  a)2(a  -  /3)2  =  -  Wjh  +2hW  +  1  Zjhlh]h  ~  W  -  2"i>32. 
The  condition  lor  equal  roots  is  therefore 

-  4]h3p3+Pi-pr  +  18piP2i'3  ~  *Pa8  -  27j>32  =  0. 
Further,  if  all  the  roots  of  the  cubic  be  real,  (/3  -  7)2(7  -  a)2(a  -  /3)2  will  be 
positive,  and  if  two  of  them  be  imaginary,  say  /3=\H-^i,  y  =  \-/xi,  then 
(i3-7)2(7-a)2ia-^2=-4M2{(X-a)2  +  ^}2,  that  is,  (^ - 7)^(7 - «)2(a - /3)2  is 
negative.  Hence  the  roots  of  (2)  are  real  and  unequal,  such  that  two  at  least 
are  equal,  or  such  that  two  are  imaginary,  according  as 

VOL.  1  2  G 


450  TWO  QUADRATICS,  CONDITION  OF  EQUIVALENCE         CHAr. 

-  ipi3P3  +Pi~p-?  +  IZpiPiPz  ~  ±pi  -  27p32 
is  positive,  zero,  or  negative. 

The  further  pursuit  of  this  matter  belongs  to  the  higher  theory  of  equa- 
tions. 

§  7.]  If  the  two  quadratic  equations 

ax2  +  bx  +  c  -  0,     a'x2  +  b'x  +  c'  =  0 
be  equivalent,  then  b/a  =  b'/'a'  and  c/a  =  c'/a'.     For,  if  the  roots  of 
each  be  a  and  /3,  then 

bja  =  -  (a  +  /5)  =  b'/a',     cfa  =  afl  =  c'/a' ; 
and  this  condition  is  obviously  sufficient. 

The  above  proposition  leads  to  the  following  :  A  quadratic 
function  of  x  is  completely  determined  when  its  roots  are  given,  and 
also  the  value  of  the  function  corresponding  to  any  value  of  x  which  is 
not  a  root.  This  we  may  prove  independently  as  follows.  Let 
the  roots  of  the  function  y  be  a  and  (3  ;  then  y  =  A(x  -  a)  (x  -  /5). 
Now,  if  V  be  the  value  of  y  when  x  =  X,  say,  then  we  must  have 

V  =  A(A  -  a)  (A  -  /8). 

This  equation  determines  the  value  of  A,  and  we  have, 
finally, 

y-V(A-a)(A-/?)  W 

The  result  thus  arrived  at  is  only  a  particular  case  of  the 
following  :  An  integral  function  of  the  nth  degree  is  uniquely  deter- 
mined when  its  n  +  1  values,  V,,  V2,  .  .  .,  VM+1,  corresponding  re- 
spectively to  the  Ti+1  values  An  A2,  .  .  .,  Art+1  of  its  variable  x,  are 
given.  To  prove  this  we  may  consider  the  case  of  a  quadratic 
function. 

Let  the  required  function  be  ax2  +  bx  +  c  ;  then,  by  the  con- 
ditions of  the  problem,  we  have 

a  A,2  +  ?>A,  +  c-Yu     akf  +  bk2  +  c  =  V2,     a\.f  +  bXx  +  c  =  V3. 

Tbese  constitute  a  linear  system  to  determine  the  unknown 
coefficients  a,  b,  c.  This  system  cannot  have  more  than  one 
definite  solution.  Moreover,  there  is  in  general  one  definite 
solution,  for  we  can  construct  synthetically  a  function  to  satisfy 
the  required  conditions,  namely, 


xvnr  lagkange's  interpolation  formula  451 

=  v  Cg- A*K-C~  K)     v    (*- Ai)(s-Ag)     v  (■<•  -  a,)  (x  -  a2) 
'J       \K-\,^K  -  A3)        2(A,  -  A,)(A2-  A3)        3(A3-  A,)(A3-  A,) 

(2). 

The  reasoning  and  the  synthesis  are  obviously  general.  We 
obtain,  as  the  solution  of  the  corresponding  problem  for  an  in- 
tegral function  of  x  of  the  nth  degree, 

Vy  (■/-'    -     A2)     (■'■•    -     A3)     .      .     .      (X    -     A,t+1)  ,gX 

(A,  -  A.) (A!  -  A3) . .  .  (At  -  A)l+1) 
This  result  is  called  Lagrange's  Interpolation  Formula. 

Example  1. 

Find  the  quadratic  equation  with  real  coefficients  one  of  whose  roots  is 
5  +  6i. 

Since  the  coefficients  are  real,  the  other  root  must  be  5  -  6i.     Hence  the 

required  equation  is  

(x-5  +  6i)(x-5-6i)  =  0, 
that  is,  (x-5f+62  =  0, 

that  is,  x*-10x  +  61  =  Q. 

Example  2. 

Find  the  quadratic  equation  with  rational  coefficients  one  of  whose  roots 
is  3  +  v7. 

Since  the  coefficients  are  rational,*  it  follows  that  the  other  root  must  be 
3  -  \J7.     Hence  the  equation  is 


{x-3  +  ^/7)(x-3-^/7)  =  0, 
that  is,  a;2- 6^  +  2  =  0. 

Example  3. 

Find  the  equation  of  lowest  degree  with  rational  coefficients  one  of  whose 
roots  is  \J2  +  \J3. 

By  the  principles  of  chap,  x.*  it  follows  that  each  of  the  quantities 
\/2-  \J3,  -  \J2  +  \J3,  -  \/2-  \/3  must  be  a  root  of  the  required  equation. 
Hence  the  equation  is 

(x  -  V2  -  V3)  {x  -  V2  +  V3)  (*  +  V2  -  V3)  (x  +  s/2  +  s/3)  =  0, 
that  is,  a?-l0a?+l  =  0. 

Example  4. 

Construct  a  quadratic  function  of  x  whose  values  shall  be  4,  4,  6,  when 
the  values  of  x  are  1,  2,  3  respectively. 


*  This  we  have  not  explicitly  proved  ;  but  we  can  establish,  by  reasoning 
similar  to  that  employed  in  chap,  xii.,  §  5,  Cor.  4,  that,  if  a  +  b\fp  be  a  root  of 
f(x)  =  0,  and  if  a  and  b  and  also  all  the  coefficients  of  f(x)  be  rational  so  far  as 
\/p  is  concerned,  then  a  -  b\/p  is  also  a  root  of/(.t')  =  0. 


452         TWO  QUADRATICS,  CONDITION  FOR  COMMON  ROOT       chap. 

The  required  function  is 

(8-2)(g-8)        (■>:-!)  (a- -3)        (as-1)  (s-2) 

4(l-2)(l-3)  +  4(2-l)(2-3)+°(3-l)(3-2)' 

that  is,  a.'2  -  3.r  +  6. 

§  8.]  The  condition  that  the  two  equations 

ax2  +  bx  +  c  =  0,     ft  V  +  b'x  +  c'  =  0 
have  one  root  in  common  is  the  same  as  the  condition  that  the 
two  integral  functions 

y  =  ax2  +  bx  +  e,     y  =  a'x2  +  b'x  +  c' 

shall  have  a  linear  factor  in  common.     Now  any  common  factor 
of  y  and  y'  is  a  common  factor  of 

c'y  -  cy ',     and  ay'  -ay, 
that  is,  if  we  denote  ad  -  a'c  by  (ac'),  Sec,  a  common  factor  of 
(ac')x2  +  (bc')x,     and  (ab')x  +  (ac')  ; 

that  is,  since  x  is  i  ot  a  common  factor  of  y  and  y'  unless  c  =  0 
and  c'  =  0,  any  common  factor  of  y  and  y'  is  a  common  factor  of 

(uc')x  +  (be'),     and  (ab')x  +  (ac'). 

Now,  if  these  two  linear  functions  have  a  common  factor  of 
the  1st  degree  in  x,  the  one  must  be  the  other  multiplied  by  a 
constant  factor. 

Hence  the  required  condition  is 

(ac')  _  (be) 
(ab')~(ac'y 
or  (ac'  -  a'c)*  =  (be  -  b'c)  (ab'  -  a'b). 

The  common  root  of  the  two  equations  is,  of  course, 

be'  -  b'c  ac'  -  a'c 


x  =  - 


ac 


a'c         ab' -  a'b' 


By  the  process  here  employed  we  could  find  the  r  conditions 
that  two  integral  equations  should  have  r  roots  in  common. 

It  is  important  to  notice  that  the  process  used  in  the  demon- 
stration is  simply  that  for  finding  the  G.C.M.  of  two  integral 
functions — a  process  in  which  no  irrational  operations  occur. 
Hence 


xvm  EXERCISES  XXXVII  453 

Cor.  1.  If  two  integral  equations  have  r  roots  in  common,  these 
roots  are  the  roots  of  an  integral  equation  of  the  rth  degree,  whose  co- 
efficients are  rational  functions  of  the  coefficients  of  the  given  equations. 

In  particular,  if  the  coefficients  of  the  two  equations  be  real 
rational  numbers,  the  r  common  roots  must  be  the  roots  of  an 
equation  of  the  rth  degree  with  rational  coefficients. 

For  example,  two  quadratics  whose  coefficients  are  all  rational 
cannot  have  a  single  root  in  common  unless  it  be  a  rational  root. 

Cor  2.  We  may  also  infer  that  if  two  integral  equations  whose 
coefficients  are  rational  have  an  odd  number  of  roots  in  common,  then 
one  at  least  of  these  must  be  real. 

Exercises  XXXVII. 

Discriminate  the  roots  of  the  following  quadratic  equations  without  solving 
them  : — 

(1.)  4a;2-8a;  +  3  =  0.  (2.)  9x- -  12*-  1  =  0.  (3.)  ix*-4x+6  =  0. 

(4.)  9a;2- 36x4-36  =  0.        (5.)  la? -  ix  -  3  =  0.  (6.)  4a?+8x+8=0. 

(7.)  (a5-3)(aj+4)  +  (a;-2)(a:+3)=0. 

(8.)  Show  that  the  roots  of  {b2  -  4ac)x2  +  4(a  +  c)x  -  4  =  0  are  always  real  ; 
and  find  the  conditions— 1°  that  both  he  positive,  2°  that  they  have  opposite 
signs,  3°  that  they  be  both  negative,  4°  that  they  be  equal,  5°  that  they  be 
equal  but  of  opposite  sign. 

(9.)  Show  that  the  roots  of  x2  +  2(p  +  q)x  +  2(jj2  +  q2)  =  0  are  imaginary. 

(10.)  Show  that  the  roots  of 

{<?-2bc  +  l2}x2-2{c2-{a  +  b)c  +  ab}x+{2a2-2(b  +  e)a  +  b2  +  e2}=0 
are  imaginary. 

(11.)  Show  that  the  roots  of 

(a;  -  b)  [x  -c)  +  {x  -  e)  [x -  a)  +  (x  -  a)  [x-  b) =0 
are  real ;  and  that  they  cannot  be  equal  unless  a=b  =  c. 

(12. )  The  roots  of  a/(x  -a)  +  b/(x  -b)  +  c/(x  -  c)  =  0  are  real  ;  and  cannot  be 
equal  unless  either  two  of  the  three,  a,  b,  c,  are  zero,  or  else  a  =  b  =  c. 

(13.)  Find  the  condition  that  the  cubic  x3  +  qx  +  r  =  0  have  equal  roots. 

(14.)  Show  that  the  cubic  1 2x?-  52a;2  +  75a;  -  36  =  0  has  equal  roots;  and 
solve  it. 

(15.)  If  two  of  the  roots  of  a  cubic  be  equal,  and  its  coefficients  be  all 
rational,  show  that  all  its  roots  must  be  rational. 

(16.)  Find  the  condition  that  two  roots  of  the  biquadratic  axi  +  dx  +  e=0 
be  equal. 

(17.)  If  a/(x  +  a)  +  b/(x  +  b)-c/(x  +  c)  +  d/(x  +  d)  have  a  pair  of  equal  roots.. 
then  either  one  of  the  quantities  a  or  b  is  equal  to  c  or  d,  or  else  1/a  +  l/b 
=  l/c  +  l/d.  Prove  also  that  the  roots  are  then  -a.  -a,  0,  -  b,  -b,  0, 
or  0,  0,  -  2ab/(a  +  b). 


454  EXERCISES  XXXVII  chap. 

Write  down  and  simplify  the  equations  whose  roots  are  as  follows:  — 

(18.)  1,0.      (19.)  h  -|.  (20.)  3  +  V2,  3-V2. 

(21.)  (a+Va2-l)/(«-\/«2-l),     (a-  Va2  -  1 )/(«  +  Va2  -  1 ). 

Find  the  equations  of  lowest  degree  with  real  rational  coefficients  which 
have  respectively  the  following  for  one  root :  — 

(22.)  a+pi.  (23.)  1  +  V2-V3-  (21.)  s/2  +  i^3. 

(25.)    »/2  +  fyi.     (Result,  x3-  6x-  6  =  0.) 

(26. )    8/2  +  f/3.     ( Result,  x9  -  1 5x6  -  8 Tx3  -  1 25  =  0. ) 

(27.)  V(?'0  +  VM  +  V(i>9)- 

(28.)  Find  the  equation  of  the  6th  degree  two  of  whose  roots  are 
1  +  -y/2  and  1+^-1. 

(29.)  Find  an  equation  with  rational  coefficients  one  of  whose  roots  is 
ap2'3  +  bp1'3  +  c. 

Hence  show  how  to  find  the  greatest  integer  in  ap2/3  +  bp113  +  c  without 
extracting  the  cube  roots. 

(30.)  Form  the  equation  whose  roots  are  p  +  atf,  p  +  a2q,  .  .  .,  p  +  a2nq, 
where  a1;  a2,  .  .  .,  a2n  are  the  imaginary  (2?i  +  l)th  roots  of  1,  showing  that 
the  coefficients  are  all  rational,  and  finding  the  general  term  of  the  equation. 

(31.)  Construct  a  quadratic  function  whose  roots  shall  be  equal  with 
opposite  signs,  and  whose  values  shall  be  23  and  67  when  x=5  and  when 
x  =  6  respectively. 

(32.)  Construct  a  cubic  function  y  corresponding  to  the  following  table  ol 

values  :  — 

a:  =  2-5,     3,     35,       4; 

y=     6,     8,      15,     IS. 

(33.)  If  x3+ax  +  bc  =  0,  x2  +  bx  +  ca  =  0  have  a  common  root,  then  their 
other  roots  satisfy  x2  +  cx  +  ab  =  0. 

(34.)  If  2{p  +  q  +  r)  =  a2  +  p2  +  y2,  and  the  roots  of  a-2  +  aa: - ;;  =  0  be/3  and  y, 
and  the  roots  of  x2  +  fix  -  q  =  0  be  y  and  a,  then  the  equation  whose  roots  are 
a  and  /3  is  x2  +  yx -r—0. 


VARIATION    OF   QUADRATIC   FUNCTIONS    FOR    REAL   VALUES 
OF   THE   VARIABLE. 

§  9.]  The  quadratic  function 

y  =  ax2  +  bx  +  c 
may  be  put  in  one  or  other  of  the  three  forms 

y  =  a{(x  —  I)2  -  m]  I., 

y  =  a{(;x-iy}  II., 

y  =  a{(x  -  I)3  +  vi]  III., 

according    as    its    roots   «    and    ji    are    real    (say    a  =  l  +    Jin, 


xvni  VARIATION  OF  ca^  +  bx  +  c  455 

(3  =  I  -  \/m),  equal  (say  a  =  l,f$  =  l),  or  imaginary  (say  a  =  I  +  i  sjm, 
(3  =  1  -  i  x/m).  I  and  m  are  both  essentially  real  quantities,  and 
m  is  positive. 

Each  of  these  three  cases  may  be  farther  divided  into  two, 
according  as  a  is  positive  or  negative. 

In  all  three  cases  when  x  is  very  great  (x  -  I)3  is  very  great 
and  positive.  Hence,  in  all  three  cases,  y  is  infinite  when  x  is 
infinite,  and  it  has  the  same  sign  as  a. 

In  all  three  cases  the  function  within  the  crooked  bracket 
diminishes  in  algebraical  value  when  x  diminishes,  so  long  as 
x  >  I,  and  has  an  algebraically  least  value  when  x  =  I ;  for  (x  -  If, 
the  only  variable  part,  being  essentially  positive,  cannot  be  less 
than  zero.  When  x  is  diminished  beyond  the  value  x-l,  (x  -  If 
continually  increases  in  numerical  value. 

We  conclude,  therefore,  that  in  all  three  cases  the  quadratic 
function  y  has  an  algebraical  minimum  or  maximum  value  when  x  =  l, 
according  as  a  is  positive  or  negative;  and  that  the  function  has  no 
other  turning  value. 

In  Case  I.,  where  the  roots  are  real  and  unequal,  y  will  have  the 
same  sign  as  a  or  not,  according  as  the  value  of  x  does  not  or  does  lie 
between  the  roots. 

For  y  =  a(x  -  a)(x  -  (3) ;  and  (x  -  a)  (x  -  fS)  will  be  positive  if 
x  be  algebraically  greater  than  both  a  and  (3,  for  then  x  -  a  and 
x  -  (3  are  both  positive  ;  and  the  same  will  be  true  if  x  be  alge- 
braically less  than  both  a  and  (3,  for  then  x  -  a  and  x-  (3  are 
both  negative.  If  x  lie  between  a  and  (3,  then  one  of  the  two, 
x  -  a,  x-  (3,  is  positive  and  the  other  negative. 

In  Cases  II.  and  III,  where  the  roots  are  either  equal  or  imaginary, 
the  function  y  will  have  the  same  sign  as  a  for  all  values  of  x. 

For  in  these  cases  the  function  within  the  crooked  brackets 
has  clearly  a  positive  value  for  all  real  values  of  x. 

§  10.]  The  above  conclusions  may  be  reached  by  a  different 
but  equally  instructive  method  as  follows  : — 

Let  us  trace  the  graph  of  the  function 

y  =  axz  +  bx  +  c  (1); 

and,  for  the  present,  suppose  a  to  be  positive. 


456 


GRAPH  OF  A  QUADRATIC  FUNCTION 


CHAP. 


To  find  the  general  character  of  the  graph,  let  us  inquire 
where  it  cuts  a  parallel  to  the  axis  of  x,  drawn  at  any  given 
distance  y  from  that  axis.  In  other  words,  let  us  seek  for  the 
abscissa?  of  all  points  on  the  graph  whose  ordinatcs  are  equal  to  y. 

We  have 

y  =  ax"  +  bx  +  c, 

that  is,  ax2  +  bx  +  (c  -  y)  =  0  (2). 

We  have,  therefore,  a  quadratic  equation  to  determine  the 
abscissa?  of  points  on  the  parallel.  Hence  the  parallel  cuts  the 
graph  in  two  real  distinct  points,  in  two  coincident  real  points, 
or  in  no  real  point,  according  as  the  roots  of  (2)  are  real  and 
unequal,  real  and  equal,  or  imaginary. 

Since  a  is  positive,  it  follows  that  when  x=  -  <x> ,  y  =  +co; 
and  when  x-  +  ao  ,  y  =  +  oo  .  Moreover,  the  quadratic  function 
y  is  continuous,  and  can  only  become  infinite  when  x  becomes 
infinite.  Hence  there  must  be  one  minimum  turning  point  on 
the  graph.  There  cannot  be  more  than  one,  for,  if  there  were, 
it  would  be  possible  to  draw  a  parallel  to  the  &-axis  to  meet 
the  graph  in  more  than  two  points. 

The  graph  therefore  consists  of  a  single  festoon,  beginning 
and  ending  at  an  infinite  distance  above  the  axis  of  x. 

The   main    characteristic    point   to   be    determined    is    the 

minimum  point.  To  obtain  this  we 
have  only  to  diminish  y  until  the 
parallel  UV  (Fig.  1)  just  ceases  to 
meet  the  graph.  At  this  stage  it  is 
obvious  that  the  two  points  U  and 
V  run  together  ;  that  is  to  say,  the 
two  abscissa?  corresponding  to  y 
become  equal.  Hence,  to  find  //,  we 
have  simply  to  express  the  condition 
that  the  roots  of  (2)  be  equal.  This 
condition  is 
4a (c  -  y)  =  0. 

y=-hlz^  (3). 

J  4a  v 


V 

/ 

V^-f^M/ 

0 

/ 

/ 
/ 
/ 
/ 
/ 
/ 
/ 

/ 

'                A               S 

\ 
\ 
\ 

\ 

V 

\ 
\ 

\ 

Fig.  1. 


lr 


Hence 


XVIII 


THREE  FUNDAMENTAL  CASES 


457 


The  corresponding  value  of  x  is  easily  obtained,  if  we  notice 
that  the  sum  of  the  roots  of  (2)  is  in  all  cases  -  b/a,  and  that 
when  the  two  are  equal  each  must  be  equal  to  -  b/2a.  Hence 
the  abscissa  of  the  minimum  point  is  given  by 

b_ 

9.  a. 


X  = 


(0. 


There  are  obviously  three  possible  cases — ■ 

I.  The  value  of  y  given  by  (3)  may  be  negative.     Since  a  is 
supposed  positive,  this  will  happen  when  b2  -  iac  is  positive. 

In  this  case  the  minimum  point  A  will  lie  below  the  axis  of 
.<■,  and  the  graph  will  be  like  the  fully  drawn  curve  in  Fig.  1. 

Here  the  graph  must  cut  the  a'-axis,  hence  the  function  y 
must  have  two  real  and  unequal  roots,  namely,  x  =  OL,  x  =  OM  ; 
and  it  is  obvious  that  y  is  positive  or  negative,  that  is,  has  the 
same  sign  as  a  or  the  opposite, 
according  as  x  does  not  or  does 
lie  between  OL  and  OM. 

II.  The  value  of  y  given 
by  (3)  will  be  zero,  provided 
b2  -  inc  =  0. 


Fig.  2. 

In  this  case  the  minimum  point 
A  falls  on  the  axis  of  x,  and  the 
graph  will  be  like  the  fully  drawn 
curve  in  Fig.  2. 

Here  the  two  roots  of  the  function 
are  equal,  namely,  each  is  equal  to  OA. 
It  is  obvious  that  here  y  is  always 
positive,  that  is,  has  the  same  sign  as  a. 
III.   The  value  of  y  given  by  (3) 
will  be  positive,  provided  b2  -  iac  be  negative. 

In  this  case  the  graph  will  be  like  the  fully  drawn  curve  in 


Fig.  3. 


Fig. 


3. 


458  EXAMPLES 


CHAP. 


Here  the  graph  does  not  cut  the  axis  of  x,  so  that  the 
function  has  no  real  roots.  Also  y  is  always  positive,  that  is, 
has  the  same  sign  as  a. 

If  we  suppose  a  to  be  negative,  the  discussion  proceeds 
exactly  as  before,  except  that  for  positive  we  must  say  negative, 
and  for  minimum  maximum.  The  typical  graphs  in  the  three 
cases  will  be  obtained  by  taking  the  mirror-images  in  the  axis  of 
x  of  those  already  given.  These  graphs  are  indicated  by  dotted 
lines  in  Figs.  1,  2,  3. 

For  simplicity  we  have  supposed  the  abscissae  of  the  points 
L,  M,  N,  A  to  be  positive  in  all  cases.  It  will  of  course  happen  in 
certain  cases  that  one  or  more  of  these  are  negative.  The  cor- 
responding figures  are  obtained  in  all  cases  simply  by  shifting 
the  axis  of  y  through  a  proper  distance  to  the  right. 

Example  1. 

To  find  for  what  valuesof  x  the  function  y  =  2x2-  12.T  +  13  is  negative,  and 
to  find  its  turning  value. 

We  have  y  =  2(.r2  -  6ar  +  9)  -  5, 


=  2{(z-3)2- 


4i 


=  2{z-(3-Vf)}{a;-(3+Vf)}- 
Hence  ?/ will  be  negative  if  x  lie  between  3-  V(°/2)  and  3  +  \/(5/2),  and  will 
be  positive  for  all  other  values  of  x. 

Again,  it  is  obvious,  from  the  second  form  of  the  function,  that  y  is 
algebraically  least  when  (x-  3)2  =  0.  Hence  y=  -  5  is  a  minimum  value  of  y 
corresponding  to  x=Z. 

Example  2. 

To  find  the  turning  values  of  (a;0-  8a;  +  15)/a;. 

15     „ 


We  have  y—x  + 


x 


First,  suppose  x  to  be  positive,  then  we  may  write 


from   which   it  appears   that   y  has   a   minimum  value,  -8  +  2a/15,  when 
\Jx-  \/(15/.c)  =  0,  that  is,  when  x=\J\5. 

Next,  let  x  be  negative,  =  -£  say,  then  we  may  write 


»    15 


2Vi5-(vf-  V^)* 


win  MAXIMA  AND  MINIMA  459 

from  which  we  see  that  -  8  -  2\/15  is  a  maximum  value  of  y  corresponding  to 
£  =  /^/l  5,  that  is,  to  x  —  -  \/l  5. 

Example  3. 

If  a  and  y  be  both  positive,  then  — 

If  x  +  y  be  given,  the  greatest  and  least  values  of  xy  correspond  to  the 
least  and  greatest  values  of  (x-y)2;  so  that  the  maximum  value  of  xy  is 
obtained  by  putting  x=y,  if  that  be  possible  under  the  circumstances  of  the 
problem. 

If  xy  be  given,  the  greatest  and  least  values  of  x  +  y  correspond  to  the 
greatest  and  least  values  of  (x-y)-  ;  so  that  the  minimum  of  x  +  y  is  obtained 
by  putting  x  =  y,  if  that  be  possible  under  the  circumstances  of  the  problem. 

These  statements  follow  at  once  from  the  identity 

(x  +  y)2-(x-y)2=4xy. 


i,,y  =  c--(x-y)2. 


For,  iix  +  y  =  c,  then 

And,  if  xy=da,  then 

(x  +  y)2=id2  +  (.r-y)2. 

Hence  the  conclusions  follow  immediately,  provided  x  and  y,  and  therefore 
xy  and  x+y,  be  both  positive. 

These  results  might  also  be  arrived  at  by  eliminating  the  value  of  y  by 
means  of  the  given  relation.  Thus,  if  x  +  y  =  c,  then  xy  =  x(c-x)  =  cx-x2 
=  c2/4-(c/2-x)'2.  Hence  xy  is  made  as  large  as  possible  by  making  x  as 
nearly  =c/2  as  possible,  and  so  on. 

Many  important  problems  in  geometry  regarding  maxima 
and  minima  may  be  treated  by  the  simple  method  illustrated  in 
Example  3. 

Example  4. 

To  draw  through  a  point  A  within  a  circle  a  chord  such  that  the  sum  of 
the  squares  of  its  segments  shall  be  a  maximum  or  a  minimum. 

Let  r  be  the  radius  of  the  circle,  d  the  distance  of  A  from  the  centre,  x  and 
y  the  lengths  of  the  segments  of  the  chords. 

Then,  by  a  well-known  geometrical  proposition, 

xy=i*-d*  (1). 

Under  this  condition  we  have  to  make 

u  =  x-  +  y-  (2) 

a  maximum  or  minimum. 

Now,  if  we  denote  x"  and  y-  by  £  and  77,  then  £  and  77  are  two  positive 
quantities  ;  and,  by  (1),  we  have 

!;V=(i*-d*)*  (3). 

Hence,  by  Example  3,  { +  77  is  a  minimum  when  =  77,  and  is  a  maximum 
when  (£  -tj)2  is  made  as  great  as  possible.  If  we  diminish  77,  it  follows,  by 
(3),  that  I  increases.  Hence  (f-77)2  will  be  made  as  great  as  possible  by 
making  £  as  great  as  possible. 


460  GEOMETRICAL  MAXIMA  AND  MINIMA  chap. 

Hence  the  sum  of  the  squares  on  the  segments  of  the  chord  is  a  minimum 
when  it  is  bisected,  and  a  maximum  when  it  passes  through  the  centre  of 
the  circle. 

Example  5. 

A  and  B  are  two  points  on  the  diameter  of  a  circle,  FQ  a  chord  through 
B.  To  find  the  positions  of  PQ  for  which  the  area  APQ  is  a  maximum  or  a 
minimum. 

Let  0  be  the  centre  of  the  circle.  The  area  OPQ  bears  to  the  area  APQ 
the  constant  ratio  OB :  AB.  Hence  we  have  merely  to  find  the  turning 
values  of  the  area  OPQ. 

Let  OB  =  a,  and  let  x  denote  the  perpendicular  from  0  on  PQ.  Then,  if 
u  denote  the  area  OPQ,  u  =  x\J(r2-x2). 

We  have  therefore  to  find  the  turning  values  of  u.  Since  u  is  positive, 
this  is  the  same  thing  as  finding  the  turning  values  of  u2.     Now 

,.4        /  r2N 

u-  =  x-(r2  -  x-)  =  —  -  f  x-  -  — 

There  are  two  cases  to  consider.  First,  suppose  a>r/\J'2.  Then,  since 
the  least  and  greatest  values  of  x  allowable  under  the  circumstances  are  0  and 
a,  we  have,  confining  ourselves  to  half  a  revolution  of  the  chord  about  A, 
three  turning  values.  If  we  put  x=0  we  give  to  (*2-r2/2)2  the  greatest 
value  which  we  can  give  it  by  diminishing  x  below  r(\j2.  Hence  x  =  0  gives 
a  minimum  value  of  OPQ. 

If  we  put  x  =  rj\j2,  we  give  (x2-r2/2)2  its  least  possible  numerical  value. 
Hence,  for  x  =  r/\j2,  OPQ  is  a  maximum. 

If  we  put  x  =  a,  we  give  (ar-r2/2)2  the  greatest  value  which  we  can  give 
it  by  increasing  x  beyond  rj\j2.  Hence  to  x  =  a  corresponds  a  minimum 
value  of  OPQ. 

Next,  suppose  a<rj\j2.  In  this  case  we  cannot  make  x=  or  >rj\j2. 
Hence,  corresponding  to  a'  =  0,  we  have,  as  before,  OPQ  a  minimum.  But 
now  (x2  -  r2/\/2j2  diminishes  continually  as  x  increases  up  to  a.  Hence,  for 
x  =  a,  OPQ  is  a  maximum. 

Remark. — This  example  has  been  chosen  to  illustrate  a  peculiarity  that 
very  often  arises  in  practical  questions  regarding  maxima  and  minima, 
namely,  that  all  the  theoretically  possible  values  of  the  variable  may  not  be 
admissible  under  the  circumstances  of  the  problem. 

Example  6. 

Given  the  perimeter  of  a  right-angled  triangle,  to  show  that  the  sum  of 
the  sides  containing  the  right  angle  is  greatest  when  the  triangle  is  isosceles. 

Let  x  and  y  denote  the  two  sides,  p  the  given  perimeter.  Then  the 
hypotenuse  i&p-x-y ;  and  we  have,  by  the  condition  of  the  problem, 

{p-(x+y)}*=x*+y*. 

2 

Hence  xy-p{x+y)  =  -^-. 

This  again  may  be  written 

{p-x){p-y)j£  (1). 


XVIII 


MAXIMA  AND  MINIMA,  GENERAL  METHOD 


461 


Under  the  condition  (1)  we  have  to  make 

u  —  x-\-y 
a  maximum. 

If  we  put  £  —p  -  x,  f)  —p  -  y,  we  have 

to-2 


(2) 


(3); 


and  we  have  to  make  u  =  2p  -(£  +  *?) 

a  maximum  ;  this  is,  to  make  £  +  ??  a  minimum.     Now,  under  the  condition 

(3),  i  +  v  is  a  minimum  when  £  =  y.     Hence  x  +  y  is  a  maximum  when  v  —  y. 

§  11.]  The  method  employed  in  §  10  for  finding  the  turning 
points   of*  a   quadratic   function   is   merely  an   example   of   the 


Fm.  4. 


general   method   indicated   in   chap,    xv.,    §    13.     Consider  any 

function  whatever,  say 

?/=/('•)  (!)■ 

Let  A  be  a  maximum  turning   point   on   its  graph,   whose 

abscissa  and  ordinate  are  x  and  y.  If  we  draw  a  parallel  to  OX 
a  little  below  A,  it  will  intersect  the  graph  in  a  certain  number 
of  points,  TUVW  say.  Two  of  these  will  be  in  the  neighbour- 
hood of  A,  left  and  right  of  AL.  If  we  move  the  parallel  up- 
wards until  it  pass  through  A,  the  two  points  U  and  V  will  run 
together  at  A,  and  their  two  abscissae  will  become  equal.  If  we 
move  the  parallel  a  little  farther  upwards,  we  lose  two  of  the 
real  intersections  altogether. 

Hence  to  find  y  we  have  simply  to  express  the  condition  that  the 
roots  of  the  equation  «  v  _    _  (.  /0\ 


462 


EXAMPLES 


CHAP. 


be  equal,  and  then  examine  whether,  if  we  increase  y  by  a  small 
amount,  we  lose  two  real  roots  or  not.  If  we  do,  then  y  is  a  maximum 
value. 

If  it  appears  that  two  real  roots  are  lost,  not  by  increasing  but  by 
diminishing  y,  then  y  is  a  minimum  value. 

Example  1. 

To  find  the  turning  values  of 

y  =  xs-9x°  +  24x  +  3. 

The  values  of  x  corresponding  to  a  given  ordinate  y  are  given  by 

x3  -9x-  +  2ix  +  (3  -  y)  =  0. 

If  D  denote  the  product  of  the  squares  of  the  differences  of  the  roots  of  this 

cubic,  then  all  its  roots  will  be  real,  two  roots  will  be  ecpial  or  two  imaginary, 

according  as  D  is  positive,  zero,  or  negative. 

Using  the  value  of  D  calculated  in  §  6,  and  putting  pi=  -  9,  ^2=24, 

ps  =  3  -  y,  we  find 

T)=-2?(y-19)(y-2S). 

Hence  y  =  19,  ?/  =  23  are  turning  values  of  y.  If  we  make  y  a  little  less  than 
19,  D  is  negative,  that  is,  two  real  roots  of  the  cubic  are  lost.  Hence  19  is  a 
minimum  value  of  y.  If  we  make  y  a  little  greater  than  23,  D  is  again 
negative  ;  hence  23  is  a  maximum  value  of  y. 

It  is  easy  to  obtain 
the  corresponding  val- 
ues of  a;,  if  we  remember 
that  two  of  the  roots  of 
the  cubic  become  equal 
when  there  is  a  turning 
value.  In  fact,  if  the 
two  equal  roots  be  a,  a, 


and  the  third  root  y,  we 

have,  by  §  1, 

2a  +  7  =  9,      a2  +  2ct7  =  24. 

Hence 

a2  -6a  4-  8  =  0, 
which  gives 

a  =  2,  or  a  =  4. 


Fig.  6. 


It  will  be  found  that  x  =  i  corresponds  to  the  minimum  value  y  =  19  ;  and 
that  x=2  corresponds  to  the  maximum  y  =  23. 


XVIII 


EXAMPLES 


463 


Remark. — The  above  method  is  obviously  applicable  to  any  cubic  integral 
function  whatsoever,  and  we  see  that  such  a  function  has  in  general  two 
turning  values,  which  are  the  roots  of  a  certain  quadratic  equation  easily  ob- 
tainable by  means  of  the  function  D. 

If  the  roots  of  this  quadratic  be  real  and  unequal,  there  are  two  distinct 
turning  points,  one  a  maximum,  the  other  a  minimum. 

If  the  roots  be  equal,  we  have  a  point  which  may  be  regarded  as  an 
amalgamation  of  a  maximum  point  with  a  minimum,  which  is  sometimes 
called  a  maximum-minimum  point. 

If  the  roots  be  imaginary,  the  function  has  no  real  turning  point. 

If  the  coefficient  of  a?  be  positive,  the  graphs  in  the  first  two  cases  have 
the  general  characters  shown  in  Figs.  5  and  6  respectively. 

Example  2. 

To  discuss  the  turning  values  of 

ar-S.T  +  15  .... 

y= — —  (D- 

The  equation  for  the  values  of  x  corresponding  to  any  given  value  of  y  is 

ai2-(?/  +  8);r+15  =  0. 
Let  D  be  the  function  b2  -  Aac  of  §  5,  whose  sign  discriminates  the  roots  of  a 
quadratic.     In  the  present  instance  we  have 

D  =  (y  +  8)2-60={y-(-8-VG0)}{2/-(-8  +  V60)}  (2). 

Hence  the  turning  values  of  y  are 

y=  _8- V(60),  and  y=  -8  +  V(60). 

If  y  has  any  value  between 
these,  D  is  negative,  and  the 
roots  of  (1)  are  imaginary. 
Hence  the  algebraically  less  of 
the  two,  namely,  -  8  -  V(60), 
is  a  maximum  ;  and  the 
algebraically  greater,  namely, 
-  8  +  V(60),  a  minimum. 

The  values  of  x  correspond- 
iugtotheseare  atonce  obtained 
from  the  equation  x  =  {y  +  8)/2. 
They  are  x=  -  \J{15)  and 
x=  +  \/(15)  respectively. 

The  reader  should  examine 
carefully   the    graph   of    this 
function,  which  lias  a  discon- 
tinuity when  x=0  (see  chnp.  xv 
corresponding  values  : — 

»=-«,      -1,        -0, 


§  5). 


Fig.  7. 
We  have  the  following  series  of 


+  0, 


y=—ao,        -24,        —  00,        +  oo  , 

Hence  the  graph  is  represented  by  Fig.  7 


+  3, 
0, 


>3 
<5' 


>o, 


0,      + 


+  00, 

+  00. 


464  GENERAL  DISCUSSION  OF  chap. 

Example  3. 

To  discuss  generally  the  turning  values  of  the  function 

_  a,r2  +  b.v  +  c 
V~a'x2  +  b'x  +  c'  (1)' 

The  equation  which  gives  the  values  of  x  corresponding  to  any  given  value 
of  y  is 

(a  -  a'y)x2  +  (b-  b'y)x  +  (c  -  c'y)  =  0. 

Let  ~D  =  {b-b'yf-4{a-a'i/){c-c'y), 

=  (ft'2  -  ia'c')y2  +  2(2a'c  +  2ac'  -  W)y  +  (Ir  -  lac), 
=  Ay2  +  By  +  C,  say. 

Then  we  have  x=- (b-b'y)±^D 

2{a-ay)  K  ' 

The  turning  values  of  y  are  therefore  given  by  the  equation 

A2/2  +  By  +  C  =  0  (3). 

I.  If  B2-4AC>0,  this  equation  will  have  real  unequal  roots,  and  there 
will  be  two  real  turning  values  of  y. 

If  A  be  positive,  then,  for  real  values  of  x,  y  cannot  lie  between  the  roots 
of  the  equation  (3).  Hence  the  less  root  will  be  a  maximum  and  the  greater 
a  minimum  value  of  y. 

If  A  be  negative,  then,  for  real  values  of  x,  y  must  lie  between  the  roots  of 
(3).  Hence  the  less  root  will  be  a  minimum  and  the  greater  a  maximum 
value  of  y. 

II.  IfB2-4AC<0,  the  equation  has  no  real  root,  and  D  has  always  the 
same  sign  as  A.  In  this  case  the  sign  of  A  must  of  necessity  be  positive  ; 
for,  if  it  were  not,  there  would  be  no  real  value  of  x  corresponding  to  any 
value  of  y  whatever. 

Hence  there  is  a  real  value  of  x  corresponding  to  any  given  value  of  y 
whatever  ;  and  y  has  no  turning  values. 

III.  If  B2  -  4AC  =  0,  we  may  apply  the  same  general  reasoning  as  in  Case 
II.  The  present  case  has,  however,  a  special  peculiarity,  as  we  shall  see  im- 
mediately. 

The  criteria  for  distinguishing  these  three  cases  may  be  expressed  in  terms 
of  the  roots  a,  /3  and  a',  13'  of  the  two  functions  axr  +  bx-rC  and  a'x?  +  b'x  +  c', 
and  in  this  form  they  are  very  useful. 
We  have 
B2  -  4AC  =  4(2«c'  +  2a 'c  -  bb'f  -  4{b"  -  lac)  (6's  -  Aa'c'), 


f2i.^y-Cg-4iUS-^}, 


a'       a    a  a  J       \a-       aj  \a*       a' 
=  4aV2   [2ct'/3'  +  2a/3  -  (a  +  /S)  (a'  +  /3') ]2  -  (a  -  /3)2 (a'  -  /3')2} , 
=  4a2a'2  { 2a' 13'  +  2a/3  -  (a  +  j8)  (a'  +  /3')  -  (a  -  /3)  (a'  -  /3') } 

x  {2a'/3'  +  2ai8-(o  +  j8)(a'  +  j8')  +  (a-j8)(o'-j8')}, 
=  16feV2(a  -  a')  (a  -  /3')  (/3  -  a')  (/3  -  /3'). 
Hence  it  appears  that  the  sign  of  B2-  4  AC  depends  merely  on  the  sign  of 
E  =  (a-a')(a-/3')(/3-a')(/3-/3')  (4) 


xvi  ir  (ax~  +  bx  +  c)l(a'r  +  b'x  +  c')  465 

Since  ft,  b,  c,  a',  b',  c'  are  all  real,  the  roots  of  an?  +  bx  +  c  and  of 
a'x2  +  b'x  +  c',  if  imaginary,  must  be  conjugate  imaginaries.  Hence,  by 
reasoning  as  in  §  6,  we  see  that,  if  the  roots  of  ax2  +  bx  +  c,  or  of  a'x"  +  b'x  +  c', 
or  of  both,  be  imaginary,  E  is  positive. 

The  same  is  true  if  the  roots  of  either  or  of  both  of  these  functions  be 
equal. 

Consider,  next,  the  case  where  a,  /3,  a,  /3'  are  all  real  and  all  unequal. 

Since  the  sign  of  E  is  not  altered  if  we  interchange  both  a  with  a'  and  /3 
with  fi',  or  both  a  with  /3  and  a'  with  /3'.  we  may,  without  losing  generality, 
suppose  that  a  is  the  algebraically  least  of  the  four,  a,  /3,  a',  /?',  and  that  a'  is 
algebraically  less  than  /3'.  If  we  now  arrange  the  four  roots  in  ascending 
order  of  magnitude,  there  are  just  three  possible  cases,  namely,  a,  p,  a',  /3' ; 
a,  a',  /3',  /3  ;  a,  a',  /3,  /3'.  In  the  first  case,  a -a',  a-/3',  /3-a',  /3-/3'  have 
all  negative  signs  ;  in  the  second,  two  have  negative  signs,  and  two  positive  ; 
in  the  third,  three  have  negative  signs,  and  one  the  positive  sign.  It  is, 
therefore,  in  the  third  case  alone  that  E  has  the  negative  sign.  The  peculi- 
arity of  this  case  is  that  each  pair  of  roots  is  separated  as  to  magnitude  by 
one  of  the  other  pair.  We  shall  describe  this  by  saying  that  the  roots  inter- 
lace. 

Lastly,  suppose  E  =  0.  In  this  case  one  at  least  of  the  four  factors,  a  -  a', 
/?  -  /3',  (3  -  a',  /3  -  j8',  must  vanish  ;  that  is  to  say,  the  two  functions  ax2  +  bx  +  c 
and  a'x2  +  b'x  +  c'  must  have  at  least  one  root,  and  therefore  at  least  one  linear 
factor  in  common.* 

Hence,  in  this  case,  (1)  reduces  to 


say.     Hence  we  have 


ft(*-a) 
J     a'(x-a')  {0)> 

a:-a'  +  a'-a     a      a(a'  -  a) 
V  =  a  ■-«'(*--  a')"    =a'  +  a^^')  (6)" 


From  (6)  it  appears  that  y  has  a  discontinuity  when  x  =  a',  passing  from 
the  value  +  co  to  -  co ,  or  the  reverse,  as  X  passes  through  that  value  ;  but 
that,  for  all  other  values  of  x,  y  either  increases  or  decreases  continuously  as 
x  increases.  Hence  y  has  no  real  turning  values  in  this  case,  unless  we  choose 
to  consider  the  value  y  =  aja,  which  corresponds  to  x=  ±°o,  as  a  maximum- 
minimum  value. 

The  graph  in  this  case,  supposing  a/a',  a,  and  a'  -  a  to  be  both  positive,  is 
like  Fig.  8,  where  OA  =  a,  OA'  =  a',  OB=aJa', 

To  sum  up — 

Case  I.  occurs  when  the  roots  of  either  or  of  both  of  the  functions 
aa?  +  bx  +  c,  a'x2  +  b'x  +  c'  are  imaginary  or  equal,  and  when  all  the  roots 
are  real  but  not  interlaced. 

Case  II.  occurs  when  the  roots  of  both  quadratic  functions  are  real  and 
interlaced. 

*  In  the  case  where  they  have  two  linear  factors  in  common,  y  reduces  to 
a  constant,  a  case  too  simple  to  require  any  discussion. 

VOL.  I.  2  H 


466 


(ax*  +  bx  +  c)/(a'a?  +  b'x  +  c') 


CHAP. 


Case  III.  occurs  when  the  two  quadratic  functions  have  one  or  both  roots 
in  common.  In  this  case  y  reduces  to  the  quotient  of  two  linear  functions, 
or  to  a  constant,  and  has  no  maximum  or  minimum  value  properly  so  called. 

In  the  above  discussion  we  have  assumed  that  neither  a  nor  a'  vanish  ;  in 
other  words,  that  neither  of  the  two  quadratic  functions  has  an  infinite  root. 
The  cases  where  infinite  roots  occur  are,  however,  really  covered  by  the  above 


Y 

B 

^ 

X 

0 

M 

A' 

Fig.  8. 

statements,  as  may  be  seen  either  by  considering  them  as  limits,  or  by  work- 
ing out  the  expression  for  B2  -  4AC  in  terms  of  the  finite  roots  in  the  particular 
instances  in  question. 

In  stating  the  above  conclusions  so  generally  as  this,  the  student  must 
remember  that  one  of  the  turning  values  may  either  become  infinite  or  corre- 
spond to  an  infinite  value  of  x  ;  otherwise  he  ma}'  find  himself  at  a  loss  in 
certain  cases  to  account  for  the  apparent  disappearance  of  a  turning  value. 

A  great  variety  of  particular  cases  are  included  under  the  general  case  of 
this  example.  If  we  put  a'  =  0,  c'  =  0,  for  instance,  we  have  the  special  case 
of  Example  2. 

As  our  object  here  is  merely  to  illustrate  methods,  it  will  be  sufficient  to 
give  the  results  in  two  more  particular  cases. 

Example  4. 

To  trace  the  variation  of  the  function 

_a2-7a:  +  6 
V~x--8x  +  lo 
The  quadratic  for  x  in  terms  of  y  is 

(l-yy--(7-8ij)x+(6-15y)  =  Q. 
Hence 

D  =  (7-82/)2-4(l-2/)(6-152/)  =  4{2/-(t-V6)}{y-a+V6)}. 
Hence  7/2 -\/6  and  7/2  +  \/6  are  maximum  and  minimum  values  of  y  re- 
spectively.    The  corresponding  values  of  a;  are  given  by 


XVIII 


GRAPHS  FOR  PARTICULAR  CASES 


467 


X  =  is 


r-8y 
1-2/ 


and  are  9  +  2\/6  and  9  -  2\/6  respectively.  We  observe  farther  that  y  is  dis- 
continuous when  x  =  3  and  when  x  =  5  ;  that  when  a;  =  +  oo  or  =  —  oo ,  y  =  1  ; 
and  that  the  other  value  of  a-  for  which  ?/  =  l  is  a:=9. 

We  have  thus  the  following  table  of  corresponding  values  : — 
x=-co,  0,      +1,      +3-0,        +3  +  0,        +4-1, 


y= 

+  1,         +"4,          0, 

- 

°°, 

+  °°, 

+  5-9, 

mill. 

x= 

+  5-0,       +5  +  0, 

+  6, 

+  9, 

+  13-9, 

+  oo 

y= 

+  CO,                    -CO, 

o, 

+  1, 

+    1-05, 

+  1. 

The  graph  has  the 
general  form  indicated  in 
Fig.  9,  which  is  not 
drawn  to  scale,  but  dis- 
torted in  order  to  bring 
out  more  clearly  the 
maximum  point  15. 

Example  5. 
To  trace  the  variation 
of  the  function 


The  quadratic  for  x  is 


Y 

y 

i 
i 

i 

max. 

B 

„                  m                               ""         ™- 

\ 

/                  i           x 

0 

M 

1       " 

x?-5x+4 

'  x--8x+  15' 


Fig.  9. 


(l-y)x2-(5-8y)x  +  (i-15y)  =  0. 
Here  we  find 

D=4{(y-i)2+2}. 

Hence  there  are  no  real  turning  values. 

The  graph  will  be  found  to  be  as  in  Fig.  10. 


Y 

\ 

^__ 

0 

1 

X 

Fig.  10. 


468  MAXIMA  AND  MINIMA,  METHOD  OF  INCREMENTS        chap. 

Example  6. 

To  find  the  turning  values  of  z  =  x2  +  y2,  given  that  cut?+bxy+cy2=l. 

We  have,  since  ax2  +  bxy  +  cy2  —  l, 

x2  +  y2  £2  +  l 

~ ~  ax'2  +  bxy  +  cy2     a£-  +  b%  +  c' 
where  £  =  ,r/y. 

We  have  now  to  find  the  turning  values  of  z  considered  as  a  function  of  f. 
The  quadratic  for  £  is 

(az-l)£-  +  bz£  +  (cz-l)  =  0. 

Hence  the  turning  values  of  z  are  given  by 

&V=4(oa-l)(cs-l), 

that  is,  by 

(b2-4ac)z2+i(a  +  c)z-i  =  0. 

The  result  thus  arrived  at  constitutes  an  analytical  solution  of  the  well- 
known  problem  to  find  the  greatest  and  least  central  radii  (that  is,  the  semi- 
axes)  of  the  ellipse  whose  equation  is  ax2  +  bxy  +  cy2  =  1 . 

Remark. — The  artifice  used  in  this  example  will  obviously  enable  us  to 
find  the  turning  values  of  u=J{x,  y),  when  <p(x,  y)  =  c,  provided /(.r,  y)  and 
<p(x,  y)  be  homogeneous  functions  of  x  and  y  whose  degree  does  not  exceed 
the  2nd.  Indeed  it  has  a  general  application  to  all  cases  where  f(x,  y)  and 
<f>(x,  y)  are  homogeneous  functions  ;  the  only  difficulty  is  in  discriminating 
the  roots  of  the  resulting  equation. 

§  12.]  Examination  of  the  Increment. — There  is  yet  another 
method  which  is  very  useful  in  discussing  the  variation  of 
integral  functions.  Suppose  we  give  x  any  small  increment, 
h,  then  the  corresponding  increment  of  the  function  fix)  is 
f(x  +  h)  -f(x).  If  this  is  positive,  the  function  increases  when  x 
increases  ;  if  it  is  negative,  the  function  decreases  when  x  increases. 
The  condition  that  x  =  a  corresponds  to  a  maximum  value  of  f(x) 
is  therefore  that,  as  x  passes  through  the  value  a,  f(x  +  h)  -f(x) 
shall  cease  to  he  positive  and  begin  to  be  negative,  and  for  a 
minimum  shall  cease  to  be  negative  and  begin  to  be  positive. 

The  practical  application  of  the  method  will  be  best  under- 
stood by  studying  the  following  example  : — 

Example. 

To  find  the  turning  values  of 

y  =  x3-9x2  +  2ix  +  3. 
Let  I  denote  the  increment  of  y  corresponding  to  a  \  ery  small  increment, 
h,  of  x ;  then 

I  =  (./•  +  hf  -  9(a!  +  h)2  +  24(.c  +  h)  +  8  -  a?  +  9.r;  -  24a  -  3, 
=  (3z2-18a:  +  24)A  +  (3x-  9)/r  +  A:!. 


XVIII 


EXERCISES  XXXVIII  469 


Now,  since  for  our  present  purpose  it  does  not  matter  how  small  h  may 

be,  we  may  make  it  so  small  that  (3x  -  9)h"  +  h3  is  as  small  a  fraction  of 

(3a;2-  18x+24)A  as  we  please.     Hence,  so  far  as  determining  the  sign  of  I  is 

concerned,  we  may  write 

I  =  (3x2-18a;  +  24)A. 

Here  h  is  supposed  positive,  hence  the  sign  of  I  depends  merely  on  the  sign 

of  3ar-18a;  +  24.     Hence  I  will  change  sign  when,  and  only  when,  x  passes 

through  a  root  of  the  equation 

3a;2-  18a:  +  24  =  0. 

Hence  the  turning  values  of  y  correspond  to  x  =  2  and  x  =  i. 

Moreover,  we  have 

l=8(x-2)(x-4)h. 

Therefore,  when  a;  is  a  little  less  than  2,  I  is  positive  ;  and  when  x  is  a 
little  greater  than  2,  I  is  negative.  Hence  the  value  of  y  corresponding  to 
a' =  2  is  a  maximum. 

In  like  manner  we  may  show  that  the  value  of  y  corresponding  to  a;=4  is 
a  minimum. 

Exercises  XXXVIII. 

(1. )  Find  the  limits  within  which  x  must  lie  in  order  that  8(.r2  -  a2)  -  65xa 
may  be  negative. 

Trace  the  graphs  of 

(2.)  y  =  x2-5x  +  6.  (3.)  y= -Sx-  +  l2x-6. 

(4.)  y=  -  4a;2  +  20a;  -  25. 

Find  the  turning  values  of  the  following  ;    and  discriminate  between 
maxima  and  minima  : — 

(5.)  ae**  +  be~kx.  (6.)  afx+a/(a-x). 

(7.)  V(l+aO  +  V(l-*)-  (8-)  x-l  +  s/(x+l). 

Trace  the  graphs  of  the  following,  and  mark,  in  particular,  the  points 
where  the  graph  cuts  the  axes,  and  the  points  where  y  has  a  turning  value  : — 
(9.)  y  =  (a:2  +  8a;  +  16)/(a;2-7a;  +  12). 
(10.)  i/  =  (a;2-7a;  +  12)/(a;2+8a'  +  16). 
(11.)  y  =  (a;2  +  8a;  +  16)/(a;2-6a;+9). 
(12.)  y  =  (a-2-10aj  +  27)/(a;2-8,r  +  15). 
(13.)  y  =  (x2-8x  +  15)/(x2-\0x  +  27). 
(14.)  2/  =  (ar-10a:  +  27)/(a;2-14a;  +  52). 

(15.)  i/=(x2-9a:  +  14)/(a^  +  2a;-15).  (16.)  y  =  (a;2+a;-  6)/(se*-  1). 

(17.)  y  =  (x2  +  5x  +  Q)/{2x  +  3).  (18.)  y  =  l/(x?  +  $x  +  5). 

(19.)  y  =  (2a^  +  a;-6)/(2a;2+5a;-12). 

(20. )  Show  that  the  algebraically  greatest  and  least  values  of  (a;2  +  2x-  2)/ 
(x2  +  3a;  +  5)  are  \/(12Al)  an<i  ~  V(12/H)  J  an(l  n°d  the  corresponding  values 
of  a;. 

(21.)  Show  that  (ax-b)  (dz-c)/(bx-a)(cx- d)  may  have  all  real  values, 
provided  (a2  -  b-)  (c-  -  d2)  >  0. 

(22.)  Show    that    (ax2  +  bx  +  c)/(cx2  +  bx  +  a)   is    capable    of  all    values    if 


470  EXERCISES  XXXV1I1  CHAP,  xvtn 

b2>(a  +  c)2;  that  there  are  two  values  between  which  it  cannot  lie  if 
(a  +  c)2>b2>lac;  and  that  there  are  two  values  between  which  it  must  lie 
if  b2<  iac  (Wolstenholme). 

(23. )  If  ra  >pb,  tlien  the  turning  value  of  [ax  +  b)/(2}x  +  r)2  is  ar/4p(ra  ~pb). 

Find  the  turning  values  of  the  following ;  and  discriminate  maxima  and 
minima : — 

(24.)  (x-l)(x-3)jx2.  (25.)  (x-3)/(x2  +  x-3). 

(26. )  l(ax  +  b)2  +  l'(a'x  +  b'f  +  l"(a"x  +  b")2. 

(27. )  ax  +  by,  given  x2  +  y2  =  c2.  (28. )  a2x2  +  b"-y2,  given  x  +  y  =  a. 

(29.)  xy,  given  a2/x2  +  b2Jy2=l.  (30.)  x3y  +  x2y2  +  xy3,  given  xy  =  a2. 

(31. )  ax2  +  2hxy  +  by2,  given  Ax2  +  2Hxy  +  By2  =  1. 

(32.)  xy/^J(x2  +  y2).  (33.)  (2x  -  1)  (Bx  -  4)  (x  -  3). 

(34.)  \l\Jx  +  \j\Jy,  given  x  +  y  =  c. 

(35.)  To  inscribe  in  a  given  square  the  square  of  minimum  area. 

(36. )  To  circumscribe  about  a  given  square  the  square  of  maximum  area. 

(37.)  To  inscribe  in  a  triangle  the  rectangle  of  maximum  area. 

(38.)  P  and  Q  are  two  points  on  two  given  parallel  straight  lines.  PQ 
subtends  a  right  angle  at  a  fixed  point  0.  To  find  P  and  Q  so  that  the  area 
POQ  may  be  a  minimum. 

(39.)  ABC  is  a  right-angled  triangle,  P  a  movable  point  on  its  hypotenuse. 
To  find  P  so  that  the  sum  of  the  squares  of  the  perpendiculars  from  P  on  the 
two  sides  of  the  triangle  may  be  a  minimum. 

(40.)  To  circumscribe  about  a  circle  the  isosceles  trapezium  of  minimum 
area. 

(41.)  Two  particles  start  from  given  points  on  two  intersecting  straight 
lines,  and  move  with  uniform  velocities  u  and  v  along  the  two  straight  lines. 
Show  how  to  find  the  instant  at  which  the  distance  between  the  particles  is 
least. 

(42.)  OX,  OY  are  two  given  straight  lines  ;  A,  B  fixed  points  on  OX  ;  P  a 
movable  point  on  OY.     To  find  P  so  that  AP2  +  BP2  shall  be  a  minimum. 

(43. )  To  find  the  rectangle  of  greatest  area  inscribed  in  a  given  circle. 

(44.)  To  draw  a  tangent  to  a  given  circle  which  shall  form  with  two  given 
perpendicular  tangents  the  triangle  of  minimum  area. 

(45.)  Given  the  aperture  and  thickness  of  a  biconvex  lens,  to  find  the  radii 
of  its  two  surfaces  when  its  volume  is  a  maximum  or  a  minimum. 

(46. )  A  box  is  made  out  of  a  square  sheet  of  cardboard  by  cutting  four 
equal  squares  out  of  the  corners  of  the  sheet,  and  then  turning  up  the  flaps. 
Show  how  to  construct  in  this  way  the  box  of  maximum  capacity. 

(47.)  Find  the  cylinder  of  greatest  volume  inscribed  in  a  given  sphere. 

(48.)  Find  the  cylinders  of  greatest  surface  and  of  greatest  volume  in- 
scribed in  a  given  right  circular  cone. 

(49.)  Find  the  cylinder  of  minimum  surface,  the  volume  being  given. 

(50.)  Find  the  cylinder  of  maximum  volume,  the  surface  being  given. 


CHAPTEE   XIX. 

Solution  of  Arithmetical  and  Geometrical  Problems 
by  means  of  Equations. 

§  1.]  The  solution  of  isolated  arithmetical  and  geometrical 
problems  by  means  of  conditional  equations  is  one  of  the  most 
important  parts  of  a  mathematical  training.  This  species  of 
exercise  can  be  taken,  and  ought  to  be  taken,  before  the  student 
commences  the  study  of  algebra  in  the  most  general  sense.  It 
is  chiefly  in  the  applications  of  algebra  to  the  systematic  investi- 
gation of  the  properties  of  space  that  the  full  power  of  formal 
algebra  is  seen.  All  that  we  need  do  here  is  to  illustrate  one  or 
two  points  which  the  reader  will  readily  understand  after  what 
has  been  explained  in  the  foregoing  chapters. 

§  2.]  The  two  special  points  that  require  consideration  in 
solving  problems  by  means  of  conditional  equations  are  the 
choice  of  variables,  and  the  discussion  or  interpretation  of  the  solution. 

With  regard  to  the  choice  of  variables  it  should  be  remarked 
that,  while  the  selection  of  one  set  of  variables  in  preference  to 
another  will  never  alter  the  order  of  the  system  of  equations  on 
whose  solution  any  given  problem  depends,  yet,  as  we  have 
already  had  occasion  to  see  in  foregoing  chapters,  a  judicious 
selection  may  very  greatly  diminish  the  complexity  of  the  system, 
and  thus  materially  aid  in  suggesting  special  artifices  for  its 
solution. 

With  regard  to  the  interpretation  of  the  solution,  it  is  im- 
portant to  notice  that  it  is  by  no  means  necessarily  true  that 
all  the  solutions,  or  even  that  any  of  the  solutions,  of  the  system 
of  equations  to  which  any  problem  leads  are  solutions  of  the 


472  INTERPRETATION  OF  THE  SOLUTION  chap. 

problem.  Every  algebraical  solution  furnishes  numbers  which 
satisfy  certain  abstract  requirements  ;  but  these  numbers  may 
in  themselves  be  such  that  they  do  not  constitute  a  solution  of 
the  concrete  problem.  They  may,  for  example,  be  imaginary, 
whereas  real  numbers  are  required  by  the  conditions  of  the  con- 
crete case ;  they  may  be  negative,  whereas  positive  numbers  are 
demanded ;  or  (as  constantly  happens  in  arithmetical  problems 
involving  discrete  quantity)  they  may  be  fractional,  whereas 
integral  solutions  alone  are  admissible. 

In  every  concrete  case  an  examination  is  necessary  to  settle 
the  admissibility  or  inadmissibility  of  the  algebraical  solutions. 
All  that  we  can  be  sure  of,  a  priori,  is  that,  if  the  concrete 
problem  have  any  solution,  it  will  be  found  among  the  algebraical 
solutions ;  and  that,  if  none  of  these  are  admissible,  there  is  no 
solution  of  the  concrete  problem  at  all. 

These  points  will  be  illustrated  by  the  following  examples. 
For  the  sake  of  such  as  may  not  already  have  had  a  sufficiency 
of  this  kind  of  mental  gymnastic,  we  append  to  the  present 
chapter  a  collection  of  exercises  for  the  most  part  of  no  great 
difficulty. 

Example  1. 

There  are  three  bottles,  A,  B,  C,  containing  mixtures  of  three  substances, 
P,  Q,  11,  in  the  following  proportions  : — ■ 

A,  aP  +  «'Q  +  «"R; 

B,  bY  +  b'Q  +  b"R  ; 

C,  cP+c'Q  +  c"R. 

It  i3  required  to  find  what  proportions  of  a  mixture  must  be  taken  from  A, 
B,  C,  in  order  that  its  constitution  may  be  dP  +  d'Q  +  d"R  (Newton,  Arithmdica 
Universalis). 

Let  x,  y,  z  be  the  proportions  in  question  ;  then  the  constitution  of  the 
mixture  is 

{ax  +  by  +  cz)  P  +  (a'x  +  b'y  +  c'z)Q  +  [a"x  +  b"y  ■*-  c'z)R. 
Hence  we  must  have 

ax  +  by  +  cz-d,     a'x  +  b'y  +  c'z  =  d',     a"x  +  b"y  +  c"z  =  d". 

The  system  of  equations  to  which  we  are  thus  led  is  that  discussed  in 
chap,  xvi.,  §  11,  with  the  sole  difference  that  the  signs  of  d,  d',  d"  are  re- 
versed. 

If,  therefore,  ab'c"  -  ab"c'  +  bc'a"  -  be"  a'  +  ca'b"  -  ca"b'  4=  0,  we  shall  obtain  a 
unique  finite  solution.  Unless,  however,  the  values  of  x,  y,  z  all  come  out 
positive,  there  will  be  no  proper  solution  of  the  concrete  problem.     It  is  in 


XIX 


EXAMPLES  473 


fact  obvious,  a  priori,  that  there  are  restrictions  ;  for  it  is  clearly  impossible, 
for  instance,  to  obtain,  by  mixing  from  A,  P.,  C,  any  mixture  which  shall 
contain  one  of  the  substances  in  a  proportion  greater  than  the  greatest  in  which 
it  occurs  in  A,  B,  or  C. 

Example  2. 

A  farmer  bought  a  certain  number  of  oxen  (of  equal  value)  for  £350.  He 
lost  5,  and  then  sold  the  remainder  at  an  advance  of  £6  a  head  on  the  original 
price.     He  gained  £365  by  the  transaction  ;  how  many  oxen  did  he  buy  ? 

Let  x  be  the  number  bought ;  then  the  original  price  in  pounds  is  350/a:. 
The  selling  price  is  therefore  350/a- +  6.  Since  the  number  sold  was  as -5,  we 
must  therefore  have 

(x-5)(—+6j-  350=365. 

This  equation  is  equivalent  to 

6a;2-  395a;  -1750  =  0, 
which  has  the  two  roots  a;  =  70  and  x  =  -25/6.     The  latter  number  is  in- 
admissible, both  because  it  is  negative  and  because  it  is  fractional ;  hence  the 
only  solution  is  a;  =  70. 

Example  3. 

A'OA  is  a  limited  straight  line  such  that  OA  =  OA'  =  a.  P  is  a  point  in 
OA,  or  in  OA  produced,  such  that  OP=;?.  To  find  a  point  Q  in  A'A  such 
that  PQ2  =  AQ.QA'.  Discuss  the  different  positions  of  Q  asp  varies  from  0 
to  its  greatest  admissible  value. 

Let  OQ  =  a?,  a*  denoting  a  positive  or  negative  quantity,  according  as  Q  is 

right  or  left  of  O.    Then  PQ=±(aj-j>),  A'Q  =  a  +  x,  AQ=a-z;  and  we  have 

in  all  cases 

(x-pf  =  (a  +  x)(a-x)  =  a2-x-  (1). 

Hence  x2-px  +  h(p2-an-)  =  0  (2). 

The  roots  of  (2)  are  ^±V(i«2~  lP% 

These  roots  will  be  real  if  pr<2a- ;  that  is  to  say,  confining  ourselves  to 
positive  values  ofp,  \{p<\j2a. 

From  (1)  we  see  that  in  all  cases  where  x  is  real  it  must  be  numerically 
less  than  a.     Hence  Q  always  lies  between  A'  and  A. 

When  p  =  0,  the  roots  of  (2)  are  ±a\J2  ;  that  is  to  say,  the  two  positions  of 
Q  are  equidistant  from  O. 

So  long  as  p  is  <a,  ftp3  -  a?)  will  be  negative,  and  the  roots  of  (2)  will  be 
of  opposite  sign  ;  that  is  to  say,  the  two  positions  of  Q  will  lie  on  opposite 
sides  of  O.  Since  the  sum  of  the  two  roots  is  p(  =  OV),  if  QiQ2  be  the  two 
positions  of  Q,  the  relative  positions  of  the  points  will  be  as  in  Fig.  1,  where 
OQ2  =  PQi. 

i  n  m 

A'  Q20  PQiA 

Fig.  1. 

When  ,p  =  a,  Qa  moves  up  to  O,  and  Qi  up  to  A. 

If  p>a,  then  both  roots  are  positive,  and  the  points  will  be  as  in  Fig.  2, 
where  OQ2=QiP. 


474  EXAMPLES 


CHAP. 


I,  I  IMI  II 

A'  O  Q,>C<M         PB 

Fig.  2. 

If  OB  =  \/2a,  then  B  is  the  limiting  position  of  P  for  which  a  solution  of 
the  problem  is  possible.  When  P  moves  up  to  B,  Qi  and  Q2  coincide  at  C 
(OC  being  £OB). 

Example  4. 

To  find  four  real  positive  numbers  in  continued  proportion  such  that  their 
sum  is  a  and  the  sum  of  their  squares  b2. 

Let  us  take  for  variables  the  first  of  the  four  numbers,  say  x,  and  the 
common  value,  say  y,  of  the  ratio  of  each  number  to  the  preceding.  Then 
the  four  numbers  are  x,  xy,  xy2,  xy3.     Hence,  by  our  data, 

x  +  xy  +  xy2  +  xy3  =  a, 

x2  +  x2y2  +  xY  +  xhf  =  b2 ; 

that  is  to  say,  x{l+y){l+y2)-a  (1), 

x2(l  +  y2)(l  +  i/)  =  b2  (2). 

From  (1)  we  derive  x2(l  +y)\l  +  y2)"  =  ar  (3), 

and  from  (2)  and  (3),  rejecting  the  factor  y2+l,  which  is  clearly  irrelevant, 
we  derive 

a2(l+7/)  =  b%l+y2)(l+y)2  (4). 

The  equation  (4)  is  a  reciprocal  biquadratic  in  y,  which  can  be  solved  by  the 
methods  of  chap.  xvii. ,  §  8. 

For  every  value  of  y  (1)  gives  a  corresponding  value  of  x. 

The  student  will  have  no  difficulty  in  showing  that  there  will  be  two 
proper  solutions  of  the  problem,  provided  a  be  >  b.  Since,  however,  the  two 
values  of  y  are  reciprocals,  and  since  x(l  +y)  (1  +  y2)  =  xy3{l  +  l/y)  (1  +  l/i/2), 
these  two  solutions  consist  merely  of  the  same  set  of  four  numbers  read  for- 
wards and  backwards.  There  is,  therefore,  never  more  than  one  distinct 
solution. 

Newton,  in  his  Arithmctica  Universalis,  solves  this  problem  by  taking  as 
variables  the  sum  of  the  two  mean  numbers,  and  the  common  value  of  the 
product  of  the  two  means  and  of  the  two  extremes.  He  expresses  the  four 
numbers  in  terms  of  these  and  of  a  and  b,  then  equates  the  product  of  the 
second  and  fourth  to  the  square  of  the  third,  and  the  product  of  the  first  and 
third  to  the  square  of  the  second.  It  will  be  a  good  exercise  to  work  out  the 
problem  in  this  way. 

Example  5. 

In  a  circle  of  given  radius  a  to  inscribe  an  isosceles  triangle  the  sum  of 
the  squares  of  whose  sides  is  2b2. 

Let  x  be  the  length  of  one  of  the  two  equal  sides  of  the  triangle,  2y  the 
length  of  the  base. 

If  ABC  be  the  triangle,  and  if  AD,  the  diameter  through  A,  meet  BC  in 
E,  then,  since  ABD  is  a  right  angle,  we  have  AB2  =  AD  .  AE.     Hence 

x2  =  2as/(.l"-y2)  (1). 


XIX 


EXAMPLES  475 


Again,  by  the  conditions  of  the  problem,  we  have 

2x2  +  4y2=2i2, 

that  is,  x2  +  2y2=b2  (2). 

From  (1)  and  (2)  we  derive 

xi-6aW  +  2a2b'i  =  0  (3). 

The  roots  of  (3)  are 

*V{«y(l-5)}; 

and  the  corresponding  values  of  y  are  given  by  (2). 

The  necessary  and  sufficient  condition  that  the  values  of  x  and  of  y  be  real 
is  that  b<3a/\/2.  When  this  condition  is  satisfied,  there  are  two  real  posi- 
tive values  of  ,r,  and  if  b>2a  there  are  two  corresponding  real  positive  values 
ofy. 

It  follows  from  the  above  that,  for  the  inscribed  isosceles  triangle  the 
sum  of  the  squares  of  whose  sides  is  a  maximum,  b  =  Ba/\/2.  Corresponding 
to  this  we  have  x=\J2>a,  2y=\/3a  ;  that  is  to  say,  the  inscribed  triangle,  the 
sum  of  the  squares  of  whose  sides  is  a  maximum,  is  equilateral,  as  is  well 
known. 

Example  6. 

Find  the  isosceles  triangle  of  given  perimeter  2p  inscribed  in  a  circle  of 
radius  a  ;  show  that,  if  2p  be  less  than  3\/3,  and  greater  than  2a,  there  are 
two  solutions  of  the  problem  ;  and  that  the  inscribed  triangle  of  maximum 
perimeter  is  equilateral. 

Taking  the  variables  as  in  last  example,  we  find 

x*  =  2a^(x'>-y")  (1), 

x  +  y=p  (2). 

Hence  a-4  -  8a2px  +  idy"  =  0  (3). 

We  cannot  reduce  the  biquadratic  (3)  to  quadratics,  as  in  last  example  ; 
but  we  can  easily  show  that,  provided  p  be  less  than  a  certain  value,  it  has 
two  real  positive  roots. 

Let  us  consider  the  function 

y  =  x*-8a'ipx+iay-  (4); 

and  let  I  be  the  increment  of  y  corresponding  to  a  very  small  positive  incre- 
ment (h)  of  x.     Then  we  find,  as  in  chap,  xviii.,  §  12,  that 

l  =  4(.^-2a-p)h  (5). 

Hence,  so  long  as  xi<2a"p,  I  is  negative  ;  and  when  x3>2a2p,  I  is  positive. 
Hence,  observing  that  y—  +  <x>  when  x—  ±oo  ,  we  see  that  the  minimum  value 
ofy  corresponds  to  x=  ^/(2arp),  and  that  the  graph  of  (4)  consists  of  a  single 
festoon.  Hence  (3)  will  have  two  real  roots,  provided  the  minimum  point  be 
below  the  ar-axis  ;  that  is,  provided  y  be  negative  when  x=  ^/(2a2p) ;  that  is, 
provided 

4n-])U  — -«s  +p§  I 


476  EXERCISES  XXXIX  chap. 

be  negative  ;  that  is,  provided  2p<Z\J%a.  It  is  obvious  that  both  the  roots 
are  positive  ;  for  when  x  =  0  we  have  y  =  4a2p2,  which  is  positive  ;  hence  the 
graph  does  not  descend  below  the  axis  of  x  until  it  reaches  the  right-hand 
side  of  the  axis  of  y. 

From  the  above  reasoning  it  follows  that  the  greatest  admissible  perimeter 
is  SsjSa.  When  2p  has  this  value,  the  minimum  point  of  the  graph  lies  on  the 
axis  of  x,  and  x—  £/(2a2p>)  =  */(3\/3a3)=  \JBa  corresponds  to  two  equal  roots 
of  (3).  The  corresponding  value  of  2y  is  given  by  2y  =  2p  -  2x  =  B\/3a  -  2\/3a 
=  \jZa;  in  other  words,  the  inscribed  isosceles  triangle  of  maximum  peri- 
meter is  equilateral. 

Another  interesting  way  of  showing  that  (3)  has  two  equal  roots  is  to  dis- 
cuss the  graphs  (referred  to  one  and  the  same  pair  of  axes)  of  the  functions 

y  =  x*,  and  y  =  8a-px  -  iarp2. 
These  can  be  easily  constructed  ;  and  it  is  obvious  that  the  abscissae  of  their 
intersections  are  the  real  roots  of  (3). 

Exercises  XXXIX. 

(1.)  How  long  will  an  up  and  a  down  train  take  to  pass  each  other,  each 
being  44  yards  long,  and  each  travelling  30  miles  an  hour  ? 

(2.)  Diophantus  passed  in  infancy  the  sixth  part  of  his  life,  in  adolescence 
a  twelfth,  then  he  married  and  in  this  state  he  passed  a  seventh  of  his  life 
and  five  years  more.  Then  he  had  a  son  whom  he  survived  four  years  and 
who  only  reached  the  half  of  his  father's  age.  How  old  was  Diophantus  when 
he  died  ? 

(3.)  A  man  met  several  beggars  and  wished  to  give  25  pence  to  each  ;  but, 
on  counting  his  money,  he  found  that  he  had  10  pence  too  little  for  that ;  and 
then  made  up  his  mind  to  give  each  20  pence.  After  doing  this  he  had  25 
pence  over.     What  had  he  at  first,  and  how  many  beggars  were  there  ? 

(4.)  Two  bills  on  the  same  person  are  sent  to  a  banker,  the  first  for  £580 
payable  in  7  months,  the  second  for  £730  payable  in  4  months.  The  banker 
gives  £1300  for  the  two.  What  was  the  rate  of  discount,  simple  interest 
being  allowed  in  lieu  of  discount  ? 

(5. )  A  basin  containing  1 200  cubic  metres  of  water  is  fed  by  three  fountains, 
and  can  be  emptied  by  a  discharging  pipe  in  4  hours.  The  basin  is  emptied 
and  the  three  fountains  set  on  ;  how  long  does  it  take  to  fill  with  the  dis- 
charging pipe  open  ? — given  that  the  three  fountains  each  running  alone 
would  fill  the  basin  in  3,  6,  and  7  hours  respectively. 

(6. )  If  I  subtract  from  the  double  of  my  present  age  the  treble  of  my 
age  6  years  ago,  the  result  is  my  present  age.     What  is  my  age  ? 

(7.)  A  vessel  is  filled  with  a  mixture  of  spirit  and  water,  70%  of  which  is 
spirit.  After  9  gallons  is  taken  out  and  the  vessel  filled  up  with  water,  there 
remains  58  J°/0  °'  spirit :  find  the  contents  of  the  vessel. 

(8. )  Find  the  time  between  8  and  9  o'clock  when  the  hour  and  minute 
hands  of  a  clock  are  perpendicular. 

(9. )  A  and  B  move  on  two  paths  intersecting  at  O.     B  is  500  yards  short 


XIX 


EXERCISES  XXXIX  477 


of  0  when  A  is  at  0  ;  in  two  minutes  they  are  equidistant  from  0,  and  in  eight 
minutes  more  they  are  again  equidistant  from  0.  Find  the  speeds  of  A 
and  B. 

(10.)  I  have  a  sum  to  buy  a  certain  number  of  nuts.  If  I  buy  at  the  rate 
of  40  a  penny,  I  shall  spend  5d.  too  much,  if  at  the  rate  of  50  a  penny, 
lOd.  too  little.     How  much  have  I  to  spend  ? 

(11.)  If  two  numbers  be  increased  by  1  and  diminished  by  1  respectively, 
their  product  is  diminished  by  4.  If  they  be  diminished  by  1  and  increased 
by  2  respectively,  their  product  is  increased  by  16.     Find  the  numbers. 

(12.)  A  is  faster  than  B  by  p  miles  an  hour.  He  overtakes  B,  who  has 
a  start  of  h  miles,  after  a  run  of  q  miles.     Required  the  speeds  of  A  and  B. 

(13.)  To  divide  a  given  number  a  into  two  parts  whose  squares  shall  be 
in  the  ratio  m:  1. 

(14.)  Four  apples  are  worth  as  much  as  five  plums  ;  three  pears  as  much  as 
seven  apples  ;  eight  apricots  as  much  as  fifteen  pears  ;  and  five  apples  sell  for 
twopence.  I  wish  to  buy  an  equal  number  of  each  of  the  four  fruits,  and  to 
spend  an  exact  number  of  pence  ;  find  the  least  sum  I  can  spend. 

(15.)  A  man  now  living  said  he  was  x  years  of  age  in  the  year  x2.  What 
is  his  age  and  when  was  he  bom  .' 

Remark  on  the  nature  of  this  and  the  preceding  problem. 
(16.)  OABCD    are  five  points  in  order  on   a  straight  line.     If  OA  =  a, 
OB  =  6,     OC  =  c,    OB  =  d,    find   the   distance   of    P    from   O   in   order   that 
PA  :  PD  =  FB  :  PC.  (Assume  P  to  lie  between  B  and  C.) 

(17.)  A  man  can  walk  from  P  to  Q  and  back  in  a  certain  time  at  the  rate 
of  3£  miles  an  hour.  If  he  walks  3  miles  an  hour  to  and  4  miles  an  hour  back, 
he  takes  5  minutes  longer  ;  find  the  distance  PQ. 

(18.)  A  starts  to  walk  from  P  to  Q  half  an  hour  alter  B  ;  overtakes  B  mid- 
way between  P  and  Q  ;  and  arrives  at  Q  at  2  P.M.  After  resting  7i  minutes, 
he  starts  back  and  meets  B  in  10  minutes  more.  When  did  each  start 
from  P  ? 

(19.)  At  two  stations,  A  and  B,  on  a  line  of  railway  the  prices  of  coals  are 
£p  per  ton  and  £q  per  ton  respectively.  If  the  distance  between  A  and  B  be 
d,  and  the  rate  for  the  carriage  of  coal  be  £r  per  ton  per  mile,  find  the  distance 
from  A  of  a  station  on  the  line  at  which  it  is  indifferent  to  a  consumer  whether 
he  buys  coals  from  A  or  from  B. 

(20.)  A  merchant  takes  every  year  £1000  out  of  his  income  for  personal 
expenses.  Nevertheless  his  capital  increases  every  year  by  a  third  of  what 
remains  ;  and  at  the  end  of  three  years  it  is  doubled.  How  much  had  he  at 
first? 

(21.)  A  takes  m  times  as  long  to  do  a  piece  of  work  as  B  and  C  together  ; 
B  n  times  as  long  as  C  and  A  together  ;  C  x  times  as  long  as  A  and  B  together. 
Find  a;;  and  show  that  l/(se+l)  +  l/(m+l)+l(»+l)=l. 

(22.)  The  total  increase  in  the  number  of  patients  in  a  certain  hospital  in 
a  certain  year  over  the  number  in  the  preceding  year  was  2|%.  In  the 
number  of  out-patients  there  was  an  increase  of  4%  ;  but  in  the  number  of 
in-patients  a  decrease  of  11  %•  Find  the  ratio  of  the  number  of  out  to  the 
number  of  in-patients. 


478  EXERCISES  XXXIX  CHAP. 

(23.)  The  sum  of  the  ages  of  A  and  B  is  now  60;  10  years  ago  their  ages 
were  as  5  to  3.     Find  their  ages  now. 

(24.)  Divide  111  into  three  parts,  so  that  one-third  of  the  first  part  is 
greater  by  4  than  one-fourth  of  the  second,  and  less  by  5  than  one-fifth  of  the 
third. 

(25.)  In  a  hundred  yards'  race  A  can  beat  B  by  \"  ;  but  lie  is  handicapped 
by  3  yards,  and  loses  by  1TV  yards.     Find  the  times  of  A  and  B. 

(26.)  A  and  B  run  a  mile,  and  A  beats  B  by  100  yards.  A  then  runs  with 
C,  and  beats  him  by  200  yards.  Finally,  B  runs  with  C  ;  by  how  much  does 
he  beat  him  ? 

(27. )  A  person  rows  a  miles  down  a  river  and  back  in  t  hours.  He  can 
row  b  miles  with  the  stream  in  the  same  time  as  c  miles  against.  Find  the 
times  of  going  and  returning,  and  the  velocity  of  the  stream. 

(28. )  A  mixture  of  black  and  green  tea  sold  at  a  certain  price  brings  a 
profit  of  4°/0  on  the  cost  price.  The  teas  sold  separately  at  the  same  price 
would  bring  5%  and  3%  profit  respectively.  In  what  proportion  were  the 
two  mixed  ? 

(29. )  If  a  rectangle  were  made  a  feet  longer  and  b  feet  narrower,  or  a'  feet 
longer  and  V  feet  narrower,  its  area  would  in  each  case  be  unaltered.  Find 
its  area. 

(30.)  Two  vessels,  A  and  B,  each  contain  1  oz.  of  a  mixture  of  spirit  and 
water.  If  1/mth  oz.  of  spirit  be  added  to  A  and  l/?ith  oz.  of  spirit  to  B,  or  if 
l/;ith  oz.  of  water  be  added  to  A  and  1/mth  oz.  of  water  to  B,  the  percentages 
of  spirit  in  A  and  B  in  each  case  become  equal.  What  percentage  of  spirit 
is  there  in  each  ? 

(31.)  A  wine-merchant  mixes  wine  at  10s.  per  gallon  with  spirit  at  20s.  per 
gallon  and  with  water,  and  makes  25%  profit  by  selling  the  mixture  at  lis.  8d. 
per  gallon.  If  he  had  added  twice  as  much  spirit  and  twice  as  much  water,  he 
would  have  made  the  same  profit  by  selling  at  lis.  3d.  per  gallon.  How  much 
spirit  and  how  much  water  does  he  add  to  each  100  gallons  of  wine  ? 

(32. )  Find  the  points  on  the  dial  of  a  watch  where  the  two  hands  cross. 

(33.)  Three  gamesters  agree  that  the  loser  shall  always  double  the  capital 
of  the  two  others.  They  play  three  games,  and  each  loses  one.  At  the  end 
they  have  each  £«.     What  had  they  at  first  ? 

(34. )  A  cistern  can  be  filled  in  6  hours  by  one  pipe,  and  in  8  hours  by 
another.  It  was  filled  in  5  hours  by  the  two  running  partly  together  and 
partly  separately.  The  time  they  ran  together  was  two-thirds  of  the  time 
they  ran  separately.     How  long  did  each  run  ? 

(35.)  A  horse  is  sold  for  £24,  and  the  number  expressing  the  profit  per 
cent  expresses  also  the  cost  price.     Find  the  cost  price. 

(36.)  I  spent  £18  in  cigars.  If  I  had  got  one  box  more  for  the  money, 
each  box  would  have  been  5s.  cheaper.     How  many  boxes  did  I  buy  ? 

(37.)  A  person  about  to  invest  in  3%  consols  observed  that,  if  the  price 
had  been  £5  less,  he  would  have  received  ^°/0  more  interest  on  his  money. 
Find  the  price  of  consols. 

(38.)  Out  of  a  cask  containing  360  quarts  of  pure  alcohol  a  quantity  is 
drawn  and  replaced  by  water.     Of  the  mixture  a  second  quantity,  84  quarts 


XIX 


EXERCISES  XXXIX  479 


more  than  the  first,  is  drawn  and  replaced  by  water.     The  cask  now  contains 
as  much  alcohol  as  water.     "What  quantity  was  drawn  out  at  first  ? 

(39.)  Find  four  consecutive  integers  such  that  the  product  of  two  of  them 
may  be  a  number  which  has  the  other  two  for  digits. 

(40.)  The  consumption  of  an  important  commodity  is  found  to  increase  as 
the  square  of  the  decrease  of  its  price  below  a  certain  standard  price  (j>).  If 
the  customs'  duty  be  levied  at  a  given  percentage  on  the  value  (a)  of  the 
commodity  before  the  duty  is  paid,  show  that,  provided  the  rate  be  below  a 
certain  limit,  there  are  two  other  rates  which  will  yield  the  same  total 
revenue,  and  determine  the  rates  which  will  yield  the  greatest  and  least 
revenues. 

(41.)  A  number  has  two  digits,  the  sum  of  the  squares  of  which  is  130. 
If  the  order  of  the  digits  be  reversed  the  number  is  increased  by  18.  Find 
the  number. 

(42.)  Three  numbers  are  in  arithmetical  progression.  The  square  of  the 
first,  together  with  the  product  of  the  second  and  third,  is  16 ;  and  the  square 
of  the  second,  together  with  the  product  of  the  first  and  third,  is  14. 

(43. )  To  find  three  numbers  in  arithmetical  progression  such  that  their  sum 
is  2a,  and  the  sum  of  their  squares  462. 

(44.)  The  sides  of  a  triangle  are  the  roots  of  x3-ax2  +  bx-c  =  0.  Show 
that  its  area  is  \ \J {a( 4ab  -a3-  8c) } . 

(45. )  The.  hypotenuse  of  a  right-angled  triangle  is  h,  and  the  radius  of 
the  inscribed  circle  r.  Find  the  sides  of  the  triangle.  Find  the  greatest 
admissible  value  of  r  for  a  given  value  of  h. 

The  following  are  from  Newton's  Arithmetica  Universalis,  q.v.,  pp.  119 

ct  scq.  : — 

(46.)  Given  the  sides  of  a  triangle,  to  find  the  segments  of  any  side  made 
by  the  foot  of  the  perpendicular  from  the  opposite  vertex. 

(47.)  Given  the  perimeter  and  area  of  a  right-angled  triangle,  to  find  the 
hypotenuse. 

(48.)  Given  the  perimeter  and  altitude  of  a  right-angled  triangle,  to  find 

its  sides. 

(49.)  The  same,  given  the  hypotenuse  and  the  sum  of  the  altitude  and  the 

two  sides. 

(50.)  Find  the  sides  of  a  triangle  which  is  such  that  the  three  sides,  a,  b,  c, 
and  the  perpendicular  on  a  form  an  arithmetical  progression. 

(51.)  The  same,  the  progression  being  geometric. 

(52.)  To  find  a  point  in  a  given  straight  line  such  that  the  difference  of 
its  distances  from  two  given  points  shall  be  a  given  length. 


CHAPTER    XX. 

Arithmetic  and  Geometric  Progressions  and  the 
Series  allied  to  them. 

§  1.]  By  a  series  is  meant  the  sum  of  a  number  vf  terms  formed 
according  to  some  common  law. 

For  example,  if  f(n)  be  any  function  of  n  whatsoever,  the 
function 

/(l)  +/(2)  +/(3)  +  .  .  .+/(/•)  +  .  .  .+/(»)  (1) 

is  called  a  series. 

/(I)  is  called  the  first  term;  /(2)  the  second  term,  &c;  and/(r) 
is  called  the  rth,  or  general,  term. 

For  the  present  we  consider  only  series  which  have  a  finite 
number  n  of  terms. 

As  examples  of  this  new  kind  of  function,  let  f(n)  —  n,  then  we  have  the 
series 

1+2  +  3  +  .   .  .+%  (2)  ; 

let  f(n)  — I /(a +  bn),  and  we  have  the  series 

a  +  b  +  ^+T2  +  a  +  b3  +  •  •  •  +  ^Ui  (3)  ; 

let  f(n)  —  \Jnl{2-  \Jn),  and  we  have  the  series 


2-  VI     2- V2     2-V3     '  '        2-V» 
and  so  on. 

It  is  obvious  that  when  the  nth  term  of  a  series  is  given  we 

can  write  down  all  the  terms  by  simply  substituting  for  n  1,  2, 

3,   .  .  .  successively. 

Thus,  if  the  ?>th  term  be  n-  +  2n,  the  series  is 

(l'-!  +  2.1)  +  (22  +  2.2)  +  (3-,  +  2.3)  +  .  .  .+(»8+2tt), 

or  3  +  8  +  15  +  .  .   .+{n2  +  2n). 

It  is  not  true,  however,  that  when  the  first  few  terms  are 


CHAT\  xx  MEANING   OF   SUMMATION  481 

given  we  can  in  general  find  the  nth  term,  if  nothing  is  told  us 
regarding  the  form  of  that  term.  This  is  sufficiently  obvious 
from  the  second  form  in  which  the  last  series  was  written ;  for 
in  the  earlier  terms  all  trace  of  the  law  of  formation  is  lost. 

If  we  have  some  general  description  of  the  nth  term,  it  may 
in  certain  cases  be  possible  to  find  it  from  the  values  of  a  certain 
number  of  particular  terms.  If,  for  example,,  we  were  told  that 
the  nth  term  is  an  integral  function  of  n  of  the  2nd  degree, 
then,  by  chap,  xviii.,  §  7,  we  could  determine  that  function  if  the 
values  of  three  terms  of  the  series  of  known  order  were  given. 

§  2.]  If  we  regard  the  series 

/(l)+/(2)+.  .   .+/(») 
as  a  function  of  n,  and  call  it  <f>(n),  it  has  a  striking  peculiarity, 
shared  by  no  function  of  n  that  we  have  as  yet  fully  discussed, 
namely,  that  the  number  of  terms  in  the  function  <$>(n)  depends  on  the 
value  of  its  variable.     For  example, 

</>(l)=l,     0(2)  =  1  +  2,     <£(3)=l  +  2  +  3, 
and  so  on. 

It  happens  in  certain  cases  that  an  expression  can  be  found 

for  (f>(n)  which  has  not  this  peculiarity ;  for  example,  we  shall 

show  presently  that 

l2     02     02  a     n(n  +  1)  (2n+  1) 

1  +2  +3  +  .  .  .  +n  "  =  -* '-? '. 

o 

On  the  left  of  this  equation  the  number  of  terms  is  n ;  on  the 
right  we  have  an  ordinary  integral  function  of  n,  the  number  of 
terms  in  which  is  independent  of  n,  and  which  is  therefore  called 
a  closed  function  of  n. 

When,  as  in  the  example  quoted,  toe  can  find  for-  the  sum  of  a 
series  an  expression  involving  only  known  functions  and  constructed  by 
a  fixed  number  of  steps,  then  the  series  is  said  to  admit  of  summation  ; 
and  the  closed  expression  in  question  is  spoken  of  as  the  sum,  par 
excellence,  of  the  series. 

The  property  of  having  a  sum  in  the  sense  just  explained  is 

an  exceptional  one ;  and  the  sum,  where  it  exists,  must  always 

be  found  by  some  artifice  depending  on  the  nature  of  the  series. 

What  the  student  should  endeavour  to  do  is  to  group  together, 

VOL.  I  2  I 


482  ARITHMETIC  SERIES  chap. 

and  be  sure  that  he  can  recognise,  all  the  series  that  can  be 
summed  by  any  given  artifice.  This  is  not  so  difficult  as  might 
be  supposed ;  for  the  number  of  different  artifices  is  by  no  means 
very  large. 

In  this  chapter  we  shall  discuss  two  very  important  cases, 
leaving  the  consideration  of  several  general  principles  and  of 
several  interesting  particular  cases  to  the  second  part  of  this  work. 

SERIES   WHOSE    WTH   TERM    IS   AN    INTEGRAL   FUNCTION    OF   n. 

§  3.]  An  Arithmetic  Series,  or  an  Arithmetic  Progression,  as  it 
is  often  called,  is  a  series  in  which  each  term  exceeds  the  pre- 
ceding by  a  fixed  quantity,  called  the  common  difference.  Let 
a  be  the  first  term,  and  b  the  common  difference  ;  then  the  terms 
are  a,  a  +  b,  a  +  lb,  a  +  3b,  &c,  the  nth  term  being  obviously 
a  +  (n  -  1  )b. 

Here  a  and  b  may  be  any  algebraical  quantities  whatsoever, 
the  word  "  exceed  "  in  the  definition  being  taken  in  the  algebraical 
sense. 

Since  the  nth.  term  may  be  written  (a  —  b)  +  bn,  where  a  -  b 
and  b  are  constants,  we  see  that  the  nth.  term  of  an  arithmetical 
series  is  an  integral  function  of  n  of  the  1st  degree.  Such  a 
series  is  therefore  the  simplest  of  the  general  class  to  be  con- 
sidered in  this  section. 

The  usual  method  of  summing  an  A.P.  is  as  follows.     Let 
2  denote  the  sum  of  n  terms,  then 
2=      a+  {a  +  b)  +  {a  +  2b}+.   .   .+  {a  +  (n-l)b}. 

If  we  write  the  terms  in  the  reverse  order,  we  have 

2=    {a+(n-l)b}  +    {a  +  {n-2)b}+    {a  +  (n-3)b}  +.  ,  .  +      a. 

If  we  now  add,  taking  the  pairs  of  terms  in  the  same  vertical 

line  together,  we  find 

2S=  {&*  +  (»- 1)6}+  {2a  +  {n-l)b}  +  {2a  +  (n-l)b}+.  .  .  +  {2a  +  (n-l)b}. 

Hence,  since  there  are  n  terms, 

^  =  ~{2a  +  (n-l)b}  (1). 

This  gives  2  in  terms  of  n,  a,  b. 


xx  EXAMPLES  483 

If  we   denote   the   last   term  of   the   series   by  I,   we   have 
l  =  a  +  (n-l)b.     Hence 

^        a  + 1  /«\ 

2  =  »-y-  (2). 

That  is  to  say,  the  sum  of  n  terms  of  an  A. P.  is  n  times  the 
average  of  the  first  and  last  terms,  a  proposition  which  is  con- 
venient in  practice. 

Example  1. 

To  sum  the  arithmetical  series  5  +  3  +  1-1-3-  .   .  .   to  100  terms.     Here 
a  — 5  and  b=  -  2.     Hence 

S=a^{2x5+(100-1)(-2)}> 

=  50(10-198), 

=  -  9400. 
Example  2. 

To  find  the  sum  of  the  first  n  odd  integers. 
The  nth.  odd  integer  is  2n  -  1.     Hence 

2  =  1  +  3  +  5+  .  .   .  +(2»-l), 
l+(2n-l) 

=  n  2 ' 

=  n2. 
It  appears,  therefore,  that  the  sum  of  any  number  of  consecutive  odd  integers, 
beginning  with  unity,  is  the  scpuare  of  their  number.     This  proposition  was 
known  to  the  Greek  geometers. 

Example  3. 

Sum  the  series  1-2  +  3-4  +  5  .  .  .   to  n  terms.     First  suppose  n  to  be 
even,  —2m  say.     Then  the  series  is 

2  =  1-2  +  3-4+.   .  .  +  (2m -I) -2m, 
=  1+3+  .   .   .  +(2to-1) 
-  2  -  4  -  .   .  .  -2m. 

In  each  line  there  are  m  terms.  The  first  line  has  for  its  sum  m2,  by  Example  2. 
The  second  gives  -m(2  +  2m)/2,  that  is,  -m(m  +  l).     Hence 

2  =  wi2-m(m  +  l)=  -m=  —  ■=. 

Next  suppose  n  to  be  odd,  =2»i-  1,  say. 
Then  we  have 

2  =  1-2  +  3-4+  .   .   .  +(2m-l). 

To  find  the  sum  in  this  case,  all  we  have  to  do  is  to  add  2m  to  our  former 
result.     We  thus  find 

2  =  2to-to  =  wi, 
_n+\ 
2    • 
This  result  might  be  obtained  even  more  simply  by  associating  the  terms  of 
the  given  series  in  pairs. 


484  GENERAL  INTEGRAL  SERIES  chap. 

§  4.]  The  artifice  of  §  3  will  not  apply  to  the  case  where  the 
nth  term  of  a  series  is  an  integral  function  of  n  of  higher  degree 
than  the  1st.  We  proceed,  therefore,  to  develop  a  more  general 
method. 

Let  the  nth  term  of  the  series  be 

p0nr  +p1nr~1  +panr~2  +  .   .   .  +pr  (1), 

where_p0,  pl}  p.2,  .  .  .,  pr  are  independent  of  n. 

And  let  us  denote  the  sums  of  the  first,  second,  third,  .  .  ., 
rth  powers  of  the  first  n  integral  numbers  by  ns1}  ns2,  nsa,  .  .  ., 
nsr ;  so  that 


jjOj    —    x       -r    U      T    <J      T     .       .       .      T    l*j 

n*2=l2  +  22  +  32  +  .   .   .  +n\ 

n.S3=l3+23+33+  .   .   .  +n3, 
and  so  on. 

If  2  denote  the  sum  of  n  terms  of  the  series  whose  rath  term 
is  (1),  we  have, 

2=p0lr+plV-1+p2lr-2+  .  .  .  +pr, 
+  2V2r+pl2r~1+p22r-2+  .  .  .  +pr, 
+  p0y+pl3r-l+p23r~2+  .   .  .  +pr, 


+  p0nr  +pi7ir~1 +p2nr~2  +  .   .   .  +pr. 
Hence,  adding  in  vertical  columns,  we  have 

2  =  7WV  +  Pi nSr -  i  +  P»nSr-»  +  ■    •    ■  +  Wr  (2). 

From  this  formula  we  see  that  we  could  sum  the  series  whose 
general  term  is  (1)  if  oidy  we  knew  the  sums  of  the  first,  second, 
third,   .  .  .,  7th  powers  of  the  first  n  integers. 

These  sums  can  be  calculated  successively  by  a  uniform 
process,  as  we  shall  now  show. 

§  5.]  To  calculate  ns,. 

If  in  the  identity  (,c  +  1 )'  -  x'  =  2x  +•  1  we  put  successively 
z  =  n,  x  -  n  -  1 , .  .  .,  x  =  2,  x  -  1 ,  we  have  the  following  equations — 

(jh-  l)2  -  n'  =  2w  +1, 

n'  -(n~l)2  =  2(n-  1)4-1, 


3e-28=2.2         -t  1, 
22  -  12=  2  1         +1. 


XX 


SUMMATION  OF  lr  +  2r  +  .    .  .  +  nr  485 


If  we  add  all  these  equations,  the  terms  on  the  left  mutually 
destroy  each  other,  with  the  exception  of  two,  which  give 
(ft  +  l)2  -  1 ;  and  those  on  the  right,  added  in  vertical  columns, 
give  2nsl  +  n.     Hence 

(n+l)2-l  =  2ns1  +  ft  (1). 

From  this  we  have 

2ns1  =  (ft+l)2->+l),    . 
=  (ft  +  1)«, 


wOi     


ft(ft  +  1) 


(2); 


2 

a  result  which  we  might  have  obtained  by  the  method  of  §  3, 
for  1  +  2  + .  .  .  +  n  is  an  A.P. 

Cor.   The  sum  of  the  first  powers  of  the  first  n  integers  is  an 
integral  function  of  n  of  the  2nd  degree. 
§  6.]  To  calculate  ns2. 

In   the   identity  (x  +  l)3  -  z*  =  3x2  +  Sx  +  1    put    successively 
x  =  n,  x  =  n-l,  .  .   .,  x  =  2,  x=l,  and  we  have 

(ft  +  l)3  -  ft3  =  3ft2  +Sn  +1, 

ft3-(?i-l)3  =  3(ft-l)2  +  3(ft-l)fl, 


33-23  =  3.22  +3.2         +1, 

23-l3=3.12  +3.1         +1. 

Hence,  adding  all  these  equations,  we  have 

(n+lf-l  =  Sns2+Snsl  +  n  (1). 

Using  in  (1)  the  value  already  found  for  „*„  we  have 

3ns2  =  (ft+l)3-|n(ft+l)-(ft  +  l), 

=  ^{2(ft  +  l)2-3,i-2}, 


Hence 


=  — — (2n*  +  n). 


_n(n  +  l)(2ft+  1) 
~6~ 


(2) 


Cor.   The  sum  of  the  squares  of  the  first  n  integers  is  an  integral 
function  of  n  of  the  3rd  degree. 


486  SUMMATION  OF  V  +  2r  +  .  .  .  +  nf  chap. 

§  7.]  To  calculate  ns3. 

In  the  identity  (x  +  l)4  -  x*  =  4x3  +  6x2  +  Ax  +  1  put  success- 
ively x  =  n,  x  —  n  -  1,  .  .  .,  x—  2,  x=  I;  add  the  n  equations  so 
obtained,  and  we  find,  as  before, 

(n  +  l)4  -  1  =  4„s8  +  6„s2  +  4ns,  +  », 
or  (ra  +  l)4-(%+  l)  =  4nsa  +  6nSj  +  4ns,  (1). 

Using  the  values  of  ns2  and  nSj  already  found,  we  have 

4ws3  =  n(n  +l)(n2  +  3n+  3)-  n(n  +  1)  (2w  +  1)  -  2»(w  +  1 ), 
=  »i(w  +  1)  (n2  +  3n  +  3  -  2rc  -  1  -  2), 
=  n2(?i  +  If. 
Hence 

A=|«^i)|'  (3). 

Cor.  1.  w53  zs  aw  integral  function  of  n  of  the  4th  degree. 
Cor.  2.  T/je  swm  o/  <Ae  cubes  of  the  first  n  integers  is  the  square 
of  the  sum  of  their  first  powers. 

§  8.]  Exactly  as  in  §  7  we  can  show  that 

(n  +  l)5  -  (n  +  1)  =  5nst  +  10ns3  +  I0ns,  +  5ns,         (1); 

and  from  this  equation,  knowing  nSi,  ns2,  ns3,  we  can  calculate 
ns4.     The  result  is 

_  n(n  +  1)  (6n3  +  9?i2  +  n  -  1)  9v 

wS<  ~ "  "30-  W 

§  9.]  This  process  may  be  continued  indefinitely,  and  the 
functions  „s1}  ns2,  .  .   .,  nsr_l  .   .  .   calculated  one  after  the  other. 

Suppose,  in  fact,  that  nsu  ns2,  .  .  .,  nsr.x  had  all  been  cal- 
culated.    Then,  just  as  in  §§  5-8,  we  deduce  the  equation 
(n  +  l)r+1  -  (n  +  1)  =  r+iCinsr  +  r+1C2nsr_,  +.   .   . +r+1CrnS,     (1), 

where  r+iC,,  r+iC2,  &c,  are  the  binomial  coefficients  of  ther  +  1th 
order. 

The  equation  (1)  enables  us  to  calculate  nsr. 

Cor.  1.  nsr  is  an  integral  function  of  n  of  the  r  +  \th  degree,  so 
that  we  may  write 

nsr  =  q0nr+1  +  q^r  +  qjf-1  +  .   .  .  +  &■+, 

and  it  is  obvious  from  (1)  that 


-i ) 


XX  SUM  OF  ANY  INTEGRAL  SERIES  487 

1  1 

q°  ~  r+1C,  -  r  +  1  * 

Cor.  2.   nsr  is  divisible  by  n(n  +  1),  so  that  we  may  write 

[nr-1  1 

nsr  =  n(n  +  1)J  - —    +plnr-*  +  p.2nr~s  +  .  .  .  +^r_,  V  ; 

for  this  is  true  when  r  =  1,  r  =  2,  r  =  3,  r  =  4  ;  hence  it  must  be 
true  for  r  =  5,  for  we  have 

(n  +  1)'  -  (n  +  1)  =  6Cins5  +  6C2ns4  +  6C3nss  +  6C27isa  +  AiAi 

and  (■«  +  l)6  -  (/i  +  1)  is  divisible  by  »(%  +  1) ;  and  so  on. 

§  10.]  We  can  now  sum  any  series  whose  Tith  term  is  re- 
ducible to  an  integral  function  of  n.  By  §  4  and  §  9,  Cor.  1, 
we  see  that  the  sum  of  n  terms  of  any  series  whose  nth  term  is  an 
integral  function  of  n  of  the  rth  degree,  is  an  integral  function  of  n  of 
the  r  +  \th  degree.  We  may,  therefore,  if  we  choose,  in  summing 
any  such  series,  assume  the  sum  to  be  A?i,,+1  +  ~Bnr  +  .  .  .  +  K  ; 
and  determine  the  coefficients  A,  B,  .  .  .,  K  by  giving  particular 
values  to  ?7.  If  S,,  S2,  .  .  .,  Sr+2be  the  sums  of  1,  2,  .  .  .,  r  +  2 
terms  of  the  series,  then  it  is  obvious,  by  Lagrange's  Theorem, 
chap,  xviii.,  §  7,  that  the  sum  is 

r+2s  (n  -  1 )  (n  -  2) . .  .  (tt.  -  s  +  1)  (n  -  s  -  1) . . .  (n  -  r  -  2) 
\  '  \s~\)(s-2) 1  (-  1)         .. .  (s-r-  2)' 

The  following  are  a  few  examples  : — 


Example  1. 

To  sum  the  series  1,  =  a  +  (a  +  b)  +  (a  +  2b)  +  .   .  .  +  {a  +  {n-l)b}. 

The  ?ith  term  is  (a-b)  +  nb. 

The  n -  1th  term  is  (a - b)  +  (n -l)b. 


The  2nd  term  is  (a-b)  +  lb. 

The  1st  term  is  (a  -  b)  +  lb. 

Hence  2  =  (a-  b)7i  +  bnsi, 

=  (a  -  V)  n  +  b-~- — -, 


rn 


as  was  found  in  §  3. 


488  EXAMPLES 


CHAP. 


Example  2.                    2  =  l2  +  32  +  52  +  to  n 

terms. 

The  nth.  term  is  (2m  -  1  )2  =  4  m2  -  in  + 1 . 

Hence                                 2  =     4?i2         -  in 

+  1 

+  4(m-1)2-4(m- 

■1)  +  1 

+  4.22         -4.2 

+  1 

+  4.12         -4.1 

+1. 

Hence,  adding  in  vertical  columns,  we  have 

2  =  4„s2  -  4„si  +  n, 

?i(m  +  1)(2m  +  1) 
6 

-4^-2+1Vn, 

_(2;i-1)m(2m+1) 

3 
Example  3. 

2  =  2.3.4  +  3.4.5  +  4.5.6+.  .  .  to  n  terms. 

The  Mth  term  is  (m  +  1)  (?i  +  2)  (m  +  3)  =  m3  +  6?i2  +  11m  +  6. 

Hence  2  =  „s3  +  6„S2+11„Si  +  6m, 

=  |  (n4  +  10m3  +  35m2  +  50m). 

Example  4. 

A  wedge-shaped  pile  of  shot  stands  on  a  rectangular  base.  There  are  m 
and  n  shot  respectively  in  the  two  sides  of  the  lowest  rectangular  layer,  m  -  1 
and  m  -  1  in  the  two  sides  of  the  next  rectangular  layer,  and  so  on,  the  upper- 
most layer  being  a  single  line  of  shot.  Find  the  whole  number  of  shot  in  the 
pile,  m  being  greater  than  n. 

The  number  in  the  lowest  layer  is  mil  ;  in  the  next  (m  -  1)  (n  -  1)  ;  in  the 
next  {in -  2)  (m -  2),  and  so  on  ;  the  number  in  the  last  layer  is  {in-n-\) 
[n  -  m  -  1 ),  that  is,  (m  -n  +  1 ). 

Hence  we  have  to  sum  the  series 

S=m?i+(j»-l)(M-l)  +  (m-2)(»-2)+.  .  .  +(m-n-l)(n-n-  1), 
in  which  there  are  n  terms. 


The  rth  term  of  the  series  is  (m-r-l)(n-r-l),  that  is,  (m+l-r) 


(M  +  l-r),  that  is,  (wi  +  1)(m  +  1)-  (m  +  M  +  2)?-  +  r2. 
Hence  we  may  write  the  series  as  follows  : — 

2=     (wi  +  1)(m  +  1)    -(?>i  +  m  +  2)m  +m2 

+(m+l)(»+l)   -(mi  +  m  +  2)(?i-1)     +(m-1)2 


+  (wt  +  l)(/i  +  l)    -(m  +  M  +  2)2  +22 

+(m+l)(m+l)   -(??i  +  m  +  2)1  +12, 

=     n{m  +  l)(n  +  l)-(m  +  n  +  2)„si  +n«2> 

=  {in  +  l)n(n+l)-§{m  +  n+2)n{n+l)  +  l/t(n+~l)(2n  +  l), 
=  ln(n+l){Sm-n+l). 
Remark. — In  working  examples  by  this  method  the  student  must  be  care- 
ful to  see  that  the  scries  is  complete  ;  in  other  words,  that  there  are  exactly 
n  terms,  all  formed  according  to  the  same  law.  If  any  terms  are  wanting,  or 
if  there  are  redundant  terms,  allowance  must  be  made  by  adding  or  subtract- 
ing terms,  as  the  case  may  be. 


XX 


GEOMETRIC  SERIES  489 


SERIES    WHOSE   ftTH   TERM    IS   THE    PRODUCT    OF    AN    INTEGRAL 
FUNCTION  OF  ft  AND  A  SIMPLE  EXPONENTIAL  FUNCTION  OF  ft. 

§  11.]  The  typical  form  of  the  ftth  term  in  the  class  of  series 
now  to  be  considered  is 

(p0ng  +p1ns~1  +  .  •  •  +  P&n, 
where  p0,  pu  .  .  .,  p8,  r  are  all  independent  of  n,  and  s  is  any 
positive  integer. 

The  simplest  case  is  that  in  which  the  integral  function  re- 
duces to  a  constant.  The  ftth  term  is  then  of  the  form  psrn,  or 
sa,jpsr  .  i*"1,  that  is,  at*"1,  where  a  =p8r  is  a  constant. 

The  ratio  of  the  ftth  to  the  (ft  -  l)th  term  in  this  special  case 
is  arn/arn~l  =  r,  that  is  to  say,  is  constant. 

A  series  in  which  the  ratio  of  each  term  to  the  preceding  is  con- 
stant is  called  a  geometric  series  or  geometric  progression  ; 
and  the  constant  ratio  in  question  is  called  the  common  ratio. 

If  the  first  term  be  a  and  the  common  ratio  r,  the  second 
term  is  ar  •  the  third  (ar)r,  that  is,  ar2 ;  the  fourth  (ar*)r,  that  is, 
or3;  and  so  on.  The  ?ith  term  is  arn~l.  A  geometric  series 
is  therefore  neither  more  nor  less  general  than  that  particular 
case  of  the  general  class  of  series  now  under  discussion  which 
introduced  it  to  onr  notice. 

§  12.]  To  sum  a  geometrical  series. 

Let  2  =  a  +  ar  +  ar2  + .  .   .+arn~1  (1). 

Multiply  both  sides  of  (1)  by  1  -  r  and  we  have 
(1  -  r)2  =  a  +  ar  +  ar2  +  .   .  .  +  arn~l 

-  ar  -  ar2  -  ...  -  arn ~1  -  ar'1, 
=  a-  arn  (2). 

1  -  rn 

Hence  2  =  a (3). 

1  —  r 

Since  the  number  of  operations  on  the  right-hand  side  of  (3) 
is  independent  of  n*  we  have  thus  obtained  the  sum  of  the 
series  (1). 

Cor.  If  I  be  the  last  term  of  the  series,  then  l  =  arn-1  and 
arn  =  rl.     Hence  (3)  may  be  written 

*  Here  we  regard  the  raising  of  r  to  the  ttth  power  as  a  single  operation. 


490 


EXAMPLES 

a  -  rl 


CHAP. 


2  = 


Example  1. 


2=f+£+f+. 

In  this  case  «  =  $,  r  =  £.     Hence 


1  -r 

.  .  to  10  terms. 


(*>• 


Example  2. 
Here  a=l,  r 


2=1-2+4-8+16 
2.     Hence 

l-(-2)"_l-(-l)"2" 
S_1*  l-(-2)~  3  ' 

=i(l  -  2n),  if  ?i.  be  even, 
=  1(1+2"),  if  ?i  be  odd. 
Example  3. 

2  =  (a;  +  y)  +  (a;?+  xy  +  ?/2)  +  (a?  +  a%  +  xy2 +  ■>/)  +  . 
_x2-y"    x?-y3    xi-yi 
x-y      x-y       x-y 


to  n  terms. 


+ 


'WH~1  _  i/«+l 


a;  -1/ 


=  —  (x3  +  £c3  +  .   .  .+a-»+1)--^-(?/-  +  2/3  +  . 
x-y  '    aj-y 


to  ?i  terms, 


+  2/«+i), 


x-y 


{l+x- 


y 


Now 


and 
hnnce 


h.  .  .  +ic"-1)-^—  (l  +  w  +  .  .  .+7/"-1). 
x-y 

l+ai+.   .   .+xn~1  =  {l-xn)/(l-x), 

1  +  1/  +  .  .  .+2/m_1  =  (l-2/")/(l-2/). 

_    a:2(l  -  x71)  y-{\  -  yn) 


~{x-y){\-x)     {x-y){l-y)' 

§  13.]  "We  next  proceed  to  consider  the  case  where  the  integral 
function  which  multiplies  rn  is  of  the  1st  degree. 

The  general  term  in  this  case  is 

(a  +  bn)rn  (1  . 

where  a  and  b  are  constants. 

It  will  be  observed  that  a  term  of  this  form  would  result  if 
we  multiplied  together  the  wth  term  of  any  arithmetic  series  by 
the  nt\\  term  of  any  geometric  series.  For  this  reason  a  series 
whose  wth  term  has  the  form  (1)  is  often  called  an  arithmetico- 
geometric  series. 

The  series  may  be  summed  by  an  extension  of  the  artifice 
employed  to  sum  a  G.P. 

Let 

2  =  (a  +  b.  1>'  +  (a  +  b.  2)r2  +  (a  +  b.  3)/-s  +  .  .   .  +  (a  +  b.  n)rn. 


XX 


ARITHMETICO-GEOMETRIC  SERIES  491 


Multiply  by  1  -  r,  and  we  have 

(1-rJZ 

=  (a  +  b.iy  +  (a  +  b.  2)r2  +  (a  +  b.3)r3  +  .  .   .  +  (a  +  bn)rn 

-  (a  +  b.  l)r2  -  (a  +  b.  2)r3  -  .  .   .  -  (o  +  bn  -  1  )rn 

-  (a  +  bn)rn+\ 

=  (a  +  b.l)r  +  \br  +  br3  +.   .  .  +  brn\-  (a  +  bn)rn+l  (1). 

Looking  merely  at  the  terms  within  the  two  vertical  lines, 
we  see  that  these  constitute  a  geometric  series.  Hence,  if  we 
multiply  by  1  -  r  a  second  time,  there  will  be  no  series  left  on 
the  right-hand  side ;  and  we  shall  in  effect  have  found  the 
required  expression  for  2.     We  have,  in  fact, 

=  (1  -  r)  (a  +  b)r  +  h?  +  br3  +  .  .   .  +  brn 

-br3-.   .   .  -  brn  -  brn+1 

-  (1  -  r)  (a  +  bn)rn+\ 
=  (1  -  r)  (a  +  b)r  +  br2  -  brn+l  -  (1  -  r)  (a  +  bn)rn+\ 
=  (a  +  b)r  -  (a  +  b)r2  +  br2  -{<*  +  (»+  l)b}rn+l  +  (a  +  bn)rn+2  (2). 
Hence 

v     (a  +  b)r  -  (a  +  b)r2  +  br2  -  {a  +  (n  +  I  )6}r»+1  +  (a  +  bn)rn+2 
2  =  ~  (l-r)s  {6)- 

§  14.]  If  the  reader  has  not  already  perceived  that  the 
artifice  of  multiplying  repeatedly  by  1  -  r  will  sum  any  series  of 
the  general  form  indicated  in  §  11,  probably  the  following  argu- 
ment will  convince  him  that  such  is  the  case. 

Let  fs(n)  denote  an  integral  function  of  n  of  the  5th  degree  ; 
then  the  degree  of  fg(n)  -f/n  -  1)  is  the  (s  -  l)th,  since  the  two 
terms  in  ns  destroy  each  other.  Hence  we  may  denote  /,(n) 
-fin  -  1)  by  /,_,(»).  Similarly,  /,_,(«)  -/,_,(«  -  1)  will  be  an 
integral  function  of  n  of  the  (5  -  2)th  degree,  and  may  be  denoted 
by/,_g(n),  and  so  on. 

Consider  now  the  series 

2=/s(l>-'+/*(2>-2  +  .  •   .+//»>"  (I)- 

Multiply  by  1  -  r,  and  we  have 


492  INTEGRO-GEOMETRIC  SERIES  chap. 

(1-rjS 

=/s(iy+    //ay+  /s(3>-3 +//»>• 

-      fs(iy-     /,(2)r3.   .  .-/g(»-l)r»    -fJny»+\ 
=fs(\y  +  I  /,_1(2)r2  +fa.pY  +  .  .  .  +/..1(n>-  |  -/»"+1  (2). 

The  series  between  the  vertical  lines  in  (2)  is  now  simpler 
than  that  in  (1) ;  since  the  integral  function  which  multiplies  rn 
is  now  of  the  (s  -  l)th  degree  only. 

If  we  multiply  once  more  by  1  -  r  we  shall  find  on  the  right 
certain  terms  at  the  beginning  and  end,  together  with  a  series 
whose  nth.  term  is  now  fs_2(n)rn. 

Each  time  we  multiply  by  1  -  r  we  reduce  the  degree  of  the 
multiplier  of  rn  by  unity.  Hence  by  multiplying  by  (1  -  r)s+1 
we  shall  extirpate  the  series  on  the  right-hand  side  altogether, 
and  there  will  remain  only  a  fixed  number  of  terms. 

It  follows  that  any  series  whose  nth  term  consists  of  an  integral 
function  of  n  of  the  sth  degree  multiplied  by  rn  can  be  summed  by 
simply  multiplying  by  (1  —r)s+1. 

This  simple  proposition  contains  the  whole  theory  of  the  sum- 
mation of  the  class  of  series  now  under  discussion. 

Example  1.  2  =  IV  +  2  V2  +  3  V  + .  .   .  +  n2r". 

Here  the  degree  of  the  multiplier  of  rn  is  2.     Hence,  in  order  to  effect  the 
summation,  we  must  multiply  by  (1  -  r)3.     We  thus  find 
(1  -  r)32 
=  1V  +   2V  +      3V  +      4V  +  .   .  .+  »V» 

-3.1V2 -3.2V3 -3.  3V4-.  .   . -3(?i-l)V*-  2,n-rn+l 

+  3.  IV +  3.  2V4-.   .   .+3(7i-2)V"-l-3(?i-l)VI+1+        3/iV"+2 
-      IV-...-   (»-3)V*-   (?i-2)V"+1-(7(.-iyV»+2 

-  m  V+3, 
=  r  +  ,-2  _  (}l  + 1  frn+i  +  (2n-  +  2>i-  1  >-"+2  -  ?iV"+3. 

Hence 

_r  +  r"  -  (n  + 1 ) V"*1  +  (2?t2  +  2ra  -  I )rn+2  -  WV+3 

S-  (1-r)8 

Example  2.  2=1-  2r+3r9  -  4r3  +  .  .  .  -  2?ir2""1. 

Multiply  by  (1  +  r)2,  and  we.  have 
(l+r)22  =  l-2/-  +      3r2-      4r»+.  .  .  -  2»ir2"-1 

+  2;--2.2r2  +  2.3?-3-.   .   .  +2(2?i-  l)?-2"-1  -      2.2nr2" 

+       r2_      2r3  +  .   .   .-    (2n,-2)r2»-1  +  (2w-l>r2'!-2«r2',+1, 
=  1  -  (2n  +  l)r"n  -  27ir""+1. 
Hence 

^     l-(2»,+  l)r2't-2?tr2"+1 

2~  (1  +  r)2       ~~     " 


xx  CONVERGENCY  OF  GEOMETRIC  SERIES         493 

If  we  put  r=l,  we  deduce 

1-2  +  3-4  .  .   .  -2«=  -n, 
which  agrees  with  §  3,  Example  3,  above. 

CONVERGENCY   AND    DIVERGENCY    OF   THE    ABOVE    SERIES. 

§  15.]  We  have  seen  that  the  sum  of  n  terms  of  a  series 
whose  nth  term  is  an  integral  function  of  n  is  an  integral  function 
of  n  ;  and  we  have  seen  that  every  integral  function  becomes 
infinite  for  an  infinite  value  of  its  variable.  Hence  the  sum  of  n 
terms  of  any  series  whose  nth.  term  is  an  integral  function  of 
n  may  be  made  to  exceed  (numerically)  any  quantity,  however 
great,  by  sufficiently  increasing  n. 

This  is  expressed  by  saying  that  every  such  series  is 
divergent. 

§  16.]  Consider  the  geometric  series 

2  =  a  +  ar  +  ar2  +  .  .   .  +  arn  ~  \ 
If  r  =  1,  the  series  becomes 

"S  =  a  +  a  +  a  + .  .   .  +  a  =  na. 
Hence,  by  sufficiently  increasing  n,  we  may  cause  2  to  surpass 
any  value,  however  great. 

If  r  be  numerically  greater  than  1,  the  same  is  true,  for  we  have 

a(rn-  1) 


2  = 


r-1    ' 

irn         a 


r-1      r-1 
Now,  since  r>  1,  we  can,  by  sufficiently  increasing  n,  make  r", 
and  therefore  arn/(r  -  1),  as  great  as  we  please.      Hence,  by  suffi- 
ciently increasing  n,  we  can  cause  2  to  surpass  any  value,  how- 
ever great  (see  Ex.  ix.  46). 

In  these  two  cases  the  geometric  series  is  said  to  be  divergent. 

If  r  be  numerically  less  than  1,  we  can,  by  sufficiently  increas- 
ing n,  make  rn  as  small  as  we  please,  and  therefore  arn/(l  -  r)  as 
small  as  we  please.  Hence,  by  sufficiently  increasing  n,  we  can 
cause  2  to  differ  from  «/(l  -  r)  as  little  as  we  please.  This  is 
often  expressed  by  saying  that  when  r  is  numerically  less  than  1, 
the  sum  to  infinity  of  the  series  a  +  ar  +  ar2  +  ...  is  a! (I  -  r). 


494  EXAMPLE  OF  INFINITE  GEOMETRIC  SERIES  chai\ 

In  this  case  the  series  is  said  to  be  convergent,  and  to  converge  to 
the  value  a/ (I  -r). 

There  is  yet  another  case  worthy  of  notice. 
If  r  -  -  1 ,  the  series  becomes 

~2  =  a-a  +  a-a  +  .  .  . 

Hence  the  sum  of  an  odd  number  of  its  terms  is  always  a,  and 
the  sum  of  an  even  number  of  them  always  0.  The  sum,  there- 
fore, does  not  become  infinite  when  an  infinite  number  of  terms 
are  taken  ;  but  neither  does  it  converge  to  one  definite  value.  A 
series  having  this  property  is  sometimes  said  to  oscillate. 

Example  1. 

Find  the  limit  of  the  sum  of  an  infinite  number  of  terms  of  the  series 


For  n  terms  we  have 


1      1      1 


s=*lzi£=i. 


2    1-4    '  2"' 

Hence,  when  n  is  made  infinitely  great, 

2=1. 
This  case  may  be  illustrated  geometrically  as  follows  : — 

Let  AB  be  a  line  of  unit  length. 

|— j j j — — |  Bisect  AB  in  Px ;  bisect  PiB  in  P2, 

A  Pi  Po      P3  P4B         P2B  in  P3 ;  and  so  on  indefinitely. 

It  is  obvious  that  by  a  sufficient 
number  of  these  operations  we  can  come  nearer  to  B  than  any  assigned  dis- 
tance, however  small.  In  other  words,  if  we  take  a  sufficient  number  of 
terms  of  the  series 

AP1  +  P1P2  +  P2P3  +  P3P4+.   .   ., 

we  shall  have  a  result  differing  from  AB,  that  is,  from  unity,  as  little  as  we 
please. 

This  is  simply  a  geometrical  way  of  saying  that 

111  , 

2  +  2i  +  2»+-   •   *  adco=1- 
Example  2. 

To  evaluate  the  recurring  decimal  "34. 
Let 

^      S/      34       34        34 

s='34=Too  +  io^+ioo"3+-  -ad™' 

Then  2  is  obviously  a  geometric  series,  whose  common  ratio,  1/100,  is  less 
than  1.     Hence 

34        1  34 


2  = 


100  1-xfo     99 


xx  PROBLEMS  ON  ARITHMETIC  PROGRESSION  495 


PROPERTIES  OF  QUANTITIES  WHICH  ARE  IN  ARITHMETIC, 
GEOMETRIC,  OR  HARMONIC  PROGRESSION. 

§  17.]  If  a  be  the  first  term,  b  the  common  difference,  n  the 
number  of  terms,  and  2  the  sum  of  an  arithmetic  progression, 
we  have 

2  =  ^{2a  +  (n-l)b]  (1). 

This  equation  enables  us  to  determine  any  one  of  the  four  quan- 
tities, 2,  a,  b,  n,  when  the  other  three  are  given.  The  equation 
is  an  integral  equation  of  the  1st  degree  in  all  cases,  except 
when  n  is  the  unknown  quantity,  in  which  case  the  equation  is  a 
quadratic.  This  last  case  presents  some  points  of  interest,  which 
we  may  illustrate  by  a  couple  of  examples. 

Example  1. 

Given  2  =  36,  a  =  15,  &=-3,  to  find  n.  We  have  by  the  formula  (1) 
above 

36=|{S0-(»-l)3}. 

Hence  n2-  lira +  24  =  0. 

The  roots  of  this  equation  are  n  =  B  and  n  =  8.  It  may  seem  strange  that 
there  should  be  two  different  numbers  of  terms  for  which  the  sum  is  the  same. 
The  mystery  is  explained  by  the  fact  that  the  common  difference  is  negative. 
The  series  is,  in  fact, 

15  +  12  +  9|   +6  +  3  +  0-3-6]   -9-.   .   .; 
and,  inasmuch  as  the  sum  of  the  part  between  the  vertical  lines  is  zero,  the 
sum  of  8  terms  of  the  series  is  the  same  as  the  sum  of  3  terms. 

Example  2. 

2=14,      a  =  Z,     6  =  2. 

The  equation  for  n  in  this  case  is 

tt2  +  2?i  =  14. 

Hence  ji=  -  1±  V(15)= +2-87  .  .  .,  or  -4-87  .  .  . 

The  second  of  the  roots,  being  negative,  has  no  immediate  reference  to  our 
problem.  The  first  root  is  admissible  so  far  as  its  sign  is  concerned,  but  it  is 
open  to  objection  because  it  is  fractional,  for,  from  the  nature  ot  the  case,  n 
must  be  integral.  It  may  be  conjectured,  therefore,  that  we  have  set  our- 
selves an  impossible  problem.  Analytically  considered,  the  function  n2  +  2n 
varies  continuously,  and  there  is  in  the  abstract  no  difficulty  in  giving  to  it 
any  value  whatsoever.  The  sum  of  an  arithmetic  series,  on  the  other  hand, 
varies  per  saltum  ;  and  it  so  happens  that  14  is  not  one  of  the  values  that  2 
can  assume  when  a  —  B  and  b  —  2.     There  are,  however,  two  values  which  2 


496     DETERMINATION  OF  ARITHMETIC  SERIES  BY  TWO  DATA    chap. 

can  assume  between  which  14  lies  ;  and  we  should  expect  that  the  integers 
next  lower  and  next  higher  than  2  "87  would  correspond  to  these  values  of  2. 
So,  in  fact,  it  is  ;  for,  when  w  =  2  2  =  8,  and  when  n  =  3  2=15. 

§  18.]  An  arithmetic  progression  is  determined  when  its  first 
term  and  common  difference  are  given ;  that  is  to  say,  when 
these  are  given  we  can  write  down  as  many  terms  of  the  pro- 
gression as  we  please.  An  arithmetic  progression  is  therefore 
what  mathematicians  call  a  twofold  manifoldness ;  that  is,  it  is 
determined  by  any  two  independent  data. 

Bearing  this  in  mind,  we  can  write  the  most  general  arith- 
metic progressions  of  3,  4,  5,  &c.  terms  as  follows  : — 

a  -  (3,      a,      a.  +  {3, 

a  -  3/3,      a  -  (3,      a  +  fi,      a  +  3/?, 

a  -2(3,      a  -ft,      a,      a  +  (3,      a  +  2/3, 

&c, 

where  a  and  (3  are  any  quantities  whatsoever.  It  will  be 
observed  that  in  the  cases  where  we  have  an  odd  number  of 
terms  the  common  difference  is  (3,  in  the  cases  where  we  have 
an  even  number  2(3.  These  formulas  are  sometimes  useful  in 
establishing  equations  of  condition  between  quantities  in  A.P. 

Example  1. 

Given  that  the  ^th  term  of  an  A.P.  is  P,  and  that  the  qth  term  is  Q,  to 
find  the  A.P.  Let  a  be  the  first  term  and  b  the  common  difference  ;  then 
the  ^th  and  qth  terms  are  a  +  (j»  -  1  )b  and  a  +  [q  -  l)b  respectively.     Hence 

a  +  (p-l)b  =  ~P,     a  +  {q-l)b  =  Q. 
These  are  two  equations  of  the  1st  degree  to  determine  a  and  b. 
We  find 

&  =  (P-Q)/(i>-0).     ct={(p-l)Q-(q-l)?}l(p-q). 

Example  2. 

If  a,  b,  c  be  in  A.  P.,  show  that 

a\b  +  c)  +  b-{c  +  a)  +  c\a  +  b)  =  y(a  +  b  +  cf. 

We  may  put  a  =  a-p,     b  =  a,     c  =  a+/3. 

The  equation  to  be  established  is  now 

(a-/3)-(2a  +  /i)  +  a-.2a  +  (a  +  i3)2(2a-/3)=?(3cl)3, 

—  6as. 
Since  a  and  /3  are  independent  of  one  another,  this  equation  must  be  an 
identity.     The  left-hand  side  reduces  to 


XX  ARITHMETIC  MEANS  497 

2a  {(a  -  (3f-  +  (a  +  j8)2}  +  j8  {(a  -  /3)2  -  (a  +  0)*}  +  2a-\ 
=  2a{2a2  +  2/3'}  +  /3{-4a/3}  +2a3, 
=  6a:!. 
Hence  the  required  result  is  established. 

§  19.]  If  three  quantities,  a,  b,  c,  be  in  A. P.,  we  have 
b  -  a  =  c  -  b  by  definition.     Hence 

b  =  (c  +  «)/2. 

In  this  case  b  is  spoken  of  as  the  arithmetic  mean  between  a 
and  c.  The  arithmetic  mean  between  two  quantities  is  therefore 
merely  what  is  popularly  called  their  average. 

If  a  and  c  be  any  two  quantities  whatsoever,  and  Ax,  A2,  .  .  .,  An 
n  others,  such  that  a,  A,,  A2,  .  .  .,  An,  c  form  an  A. P.,  then  An  A2, 
.   .  .,  An  are  said  to  be  n  arithmetic  means  inserted  between  a  and  c. 

There  is  no  difficulty  in  finding  A,,  A2,  .  .  .,  An  when  a  and 
c  are  given.  For,  if  b  be  the  common  difference  of  the  A.P., 
a,  Au  A2,  .   .  .,  A,i;  c,  then 

A!  =  a  +  b,     A2  =  a  +  2b,     .  .   .,    An  =  a  +  nb, 
and  6  =  a  +  (n  +  1  )b. 

From  the  last  of  these  we  deduce  b  —  (c  -  a)j{n  +1).  Hence 
we  have 

A  C~a  A  O    C~a  S 

A,=a  + -,    A„  =  a  +  2 -,    6zc. 

n  +  1        "  n  +  1 

N.B. — By  the  arithmetic  mean  or  average  of  n  quantities  a,,  a2, 
.   .  .,  aa  is  meant  («,  +  a„  +  .   .   .  +  atl)/n. 

In    the  particular    case   where   two   quantities   only   are   in 

question,   the   arithmetic   mean   in   this    sense    agrees   with  the 

definitions  given  above  ;  but  in  other  cases  the  meanings  of  the 

phrases  have  nothing  in  common. 

Example  1. 

Insert  30  arithmetic  means  between  5  and  90  ;  and  find  the  arithmetic 

mean  of  these  means. 

Let  b  be  the  common   difference  of  the  A.  P.  5,  Ai,  A2,   .   .   .,  AM,  90. 

Then 

6=(90-5)/(80+l)=85/31. 

Hence  the  means  are 

,85  n   85  _    85      c 

5  +  3l'     5  +  2-3l'     5  +  3-3T     &C'; 

,.    t  .  240      325       410      . 

that  is,  — ,     — ,     — ,    &c. 

VOL.  I  2  K 


498  EXAMPLES  chap. 

We  have  A1  +  A2+ .  .  .  +A„  =  1  (  r  A^+A.  | 

n  n  \  2       J 

_A!  +  A» 
■~ 2~ ' 

_     85     nn     85  \  /„ 

=  (5  +  90)/2  =  95/2. 
Remark. — It  is  true  generally  that  the  arithmetic  mean  of  the  n  arith- 
metic means  between  a  and  c  is  the  arithmetic  mean  between  a  and  c. 

Example  2. 

The  arithmetic  mean  of  the  squares  of  n  quantities  in  A.  P.  exceeds  the 
square  of  their  arithmetic  mean  by  a  quantity  which  depends  only  upon  n 
and  upon  their  common  difference. 

Let  the  ?i  quantities  be 

a  +  b,     a  +  2b,     .  .  .,     a  +  nb. 
Then,  by  §§  5  and  6, 

{a  +  bT  +  {a  +  2b?+.  .  .  +(a  +  nbf 
n 


If.     ,     ,   ,     ,  .,  ,  ,.,« (n  +  1    2?i  +  l)\ 

:-■{  a-n  +  abnln  + 1)  +  b2  — ^ — -  V, 

n  I  6  J 


62 
=  a2  +  ab(n  +  l)  +  -{2n2  +  3n  +  l). 

.      .            f(a  +  b)  +  (a  +  2b)  +  .   .   .  +(a  +  nb)\ 3     /       ra  +  l,\a 
Again,        |-        —  )   a=^+__»ji 

TO 

=  «2  +  «&(  -,i  + 1 )  +  -( w2  +  2n  +  1 ). 

M2-  1 
Hence  A.  M.  of  squares  -  square  of  A.M.  =  52, 

which  proves  the  proposition. 

§  20.]  If  Z  be  the  sum  of  n  terms  of  a  geometric  progression 
whose  first  term  and  common  ratio  are  a  and  r  respectively,  we 
have 

rn  _  1 

When  any  three  of  the  four,  2,  a,  r,  n,  are  given,  this  equation 
determines  the  fourth.  "When  either  i:  or  a  is  the  unknown 
quantity,  we  have  to  solve  an  equation  of  the  1st  degree.  When 
r  is  the  unknown  quantity,  we  have  to  solve  an  integral  equation 
of  the  ?<th  degree,  which,  if  n  exceeds  2,  will  in  general  be 
effected  by  graphical  or  other  approximative  methods.  If  n  be 
the  unknown  quantity,  we  have  to  solve  an  exponential  equation 
of   the   form  r11  =  s,  where  r  and  s  are  known.     This   may  be 


xx       DETERMINATION   OF  GEOMETRIC  SERIES  BY  TWO  DATA     499 

accomplished  at  once  by  means  of  a  table  of  logarithms,  as  we 
shall  see  in  the  next  chapter. 

§  21.]  Like  an  A.P.,  a  G.P.  is  a  twofold  manifoldness,  and 
may  be  determined  by  means  of  its  first  term  and  common  ratio, 
or  by  any  other  two  independent  data. 

In  establishing  any  equation  between  quantities  in  G.P.,  it 
is  usual  to  express  all  the  quantities  involved  in  terms  of  the 
first  term  and  common  ratio.  Since  these  two  are  independent, 
the  equation  in  question  must  then  become  an  identity. 

Example  1. 

The  ^th  term  of  a  G.P.  is  P,  and  the  qth.  term  is  Q  ;  find  the  first  term 
and  common  ratio. 

Let  a  be  the  first  term,  r  the  common  ratio.     Then  we  have,  by  our  data, 

Prom  these,  by  division,  we  deduce 

?*-«=:  P/Q,  whence  r=(?/Q)1!(>>-<>K 

Using  this  value  of  r  in  the  first  equation,  we  find 

a  =  P/(P/Q)Ip-1V(p-«)  =  PP-d  /(/>-«)Q(i-*>)/(«-*). 

Hence  we  have 

a  =  YV-iV(p-q)Qj}-p)!(<i-p)}    r = pi/(i>-«)Qi/(«-j>). 

Example  2. 

If  a,  b,  c,  d  be  four  quantities  in  G.  P.,  prove  that 

4(«2  +  b2  +  c2  +  d')  -  (a  +  b  +  c  +  df={a -  bf  +  (c -  df  +  2(a - df. 
If  the  common  ratio  be  denoted  by  r,  we  may  put  b  —  ra,  c  =  r2a,  d  =  ria. 
The  equation  to  be  established  then  becomes 

4cr(l  +  >~  +  r4  +  Is)  -  a2{l  +  r  +  r2  +  r3)2  =  a'-'(l  -  r)2  +  aV(l  -  r)2  +  2a2(l  -  r3)2, 
that  is, 
4(1  +  r2  +r*+  r«)  -  (1  +  It  +  3r2  +  4r=  +  dr4  +  2r5  +  r6) 

=  l-2r  +  r2  +  ri-2r5  +  rK  +  2-  4r3  +  2r6, 
which  is  obviously  true. 

§  22.]  When  three  quantities,  a,  b,  c,  are  in  G.P.,  b  is  called  the 
geometric  mean  between  a  and  c. 

We  have,  by  definition,  c/b  =  b/a.  Hence  b2  =  ac.  Hence,  if 
we  suppose  a,  b,  c  to  be  all  positive  real  quantities,  b  =  +  \/(ac). 
That  is  to  say,  the  geometric  mean  between  two  real  positive  quantities 
is  the  positive  value  of  the  square  root  of  their  product. 

If  a  and  c  be  two  given  positive  quantities,  and  G1;  G2,  .  .  .,  Gn 
n  quantities,  such  that  a,  Glt  G2,  .  ,  .,  Gn,  c  form  a  G.P.,  then 
G„  G2,  .  .  .,  Gn  are  said  to  be  n  geometric  means  inserted  between  a 
and  c. 


500  GEOMETRIC  MEANS 


CHAP. 


Let  r  be  the  common  ratio  of  the  supposed  progression. 
Then  we  have  G,  =  ar,  G2  =  ar2,  .  .  .,  GM  =  arn,  c  =  arn+1.  From 
the  last  of  these  equations  we  deduce  r  =  (c/a)1/(-n+l\  the  real 
positive  value  of  the  root  being,  of  course,  taken.  Since  r  is  thus 
determined,  we  can  find  the  value  of  all  the  geometric  means. 

The  geometric  mean  of  n  positive  real  quantities  is  the  positive 
value  of  the  nth  root  of  their  product.  This  definition  agrees  with 
the  former  definition  when  there  are  two  quantities  only. 

Example. 

The  geometric  mean  of  the  n  geometric  means  between  a  and  c  is  the 
geometric  mean  between  a  and  c. 

Let  the  n  geometric  means  in  question  be  ar,  ar2,  .  .   .,  arn,  so  that 
c  =  arn+1.     Then 

{ar.  ar" .  .  .  arn)Vn  —  (a"rl^2+  "  ■  •  +»)i«, 

=  {a2r"+1)1'2, 

=  {acr-} 
which  proves  the  proposition. 

§  23.]  A  series  of  quantities  which  are  such  that  their  reciprocals 
form  an  arithmetic  progression  are  said  to  be  in  harmonic  progression. 

From  this  definition  we  can  deduce  the  following,  which  is 
sometimes  given  as  the  defining  property : — 

If  a,  b,  c  be  three  consecutive  terms  of  a  harmonic  progression,  then 

ajc  =  {a-b)l(b-c)  (1). 

For,  by  definition,  I /a,  1/6,  1/e  are  in  A.  P.,  therefore 

1_1      1 _1 

b      a     c      b 
a-b     b - c 


Hence 
Hence 


ah         be 
a-b     ab     a 
b  —  c     be     c  ' 
which  proves  the  property  in  question. 

§  24.]  A  harmonic  progression,  like  the  arithmetic  j)rogression, 
from  which  it  may  be  derived,  is  a  twofold  munifoldness.  The 
following  is  therefore  a  perfectly  general  form  for  a  harmonic 


xx  HARMONIC  PROGRESSION,  HARMONIC  MEANS  501 

series,  1  J(a  +  b),  l/(a  +  2b),  l/(a  +  36),  .  .  .,  lfca  +  rib),  .  .  ., 
for  it  contains  two  independent  constants  a  and  b ;  and  the 
reciprocals  of  the  terms  are  in  A. P. 

The  following  forms  (see  §  18)  are  perfectly  general  for 
harmonic  progressions  consisting  of  3,  4,  5,  .  .  .  terms  respect- 
ively : — 

l/(a-£),       1/a,      l/(a  +  P); 

l/(a-3/3),      l/(«-/3),      l/(a  +  /3),      l/(a+3/3); 
1/(0.-2(3),       l/(«-/3),       1/a,       l/(a  +  j8),      l/(a+2/3); 

&c. 

The  above  formulae  may  he  used  like  those  in  §  18. 

§  25.]  If  a,  b,  c  be  in  IIP.,  b  is  called  the  harmonic  mean 
between  a  and  c.  We  have,  by  definition,  1/c  —  1/6  =  1/b  —  1/a- 
Hence  2/b  -  1/a  +  1/c,  and  b  =  2ae/(a  +  c). 

If  a,  H,,  HB,  .  .  .,  H„,  c  form  a  harmonic  progression,  H,,  H,, 
.  .  .,  Hw  are  said  to  be  n  harmonic  means  inserted  between  a  and  c. 

Since  1/a,  1/H,,  1/H2,  .  .  .,  1/Hn,  1/c  in  this  case  form  an 
A. P.,  whose  common  difference  is  d,  say,  we  have 

d  =  (l/c-  l/a)/(n  +  1)  =  (a  -  c)j(n  +  \)ac. 
Hence 
1/H,  =  1/a  +  (a  -  c)/(n  +  l)ac,     1/Hg  =  1/a  *  2(a  -  c)j(n  +  l)ac,  &c; 
and     H,  =  (n  +  l)ae/(a  +  nc),     H2  =  (n  +  l)ac/(2a  +  (n  -  l)c),  &c. 

If  a  quantify  H  be  such  that  its  reciprocal  is  the  arithmetic  mean 
of  the  reciprocals  of  n  given  quantities,  H  is  said  to  be  the  harmonic 
mean  of  the  n  quantities. 

It  is  easy  to  see,  from  the  corresponding  proposition  regard- 
ing arithmetic  means,  that  the  harmonic  mean  of  the  n  harmonic 
means  between  a  and  c  is  the  harmonic  mean  of  a  and  c. 

§  26.]  The  geometric  mean  between  two  real  positive  quantities  a 
and  c  is  the  geometric  mean  between  the  arithmetic  and  the  harmonic 
means  between  a  and  c  ;  and  the  arithmetic,  geometric,  and  harmonic 
means  are  in  descending  order  of  magnitude. 

Let  A,  G,  H  be  the  arithmetic,  geometric,  and  harmonic 
means  between  a  and  c,  then 

A  =  (a  +  c)/2,     G  -  +  */(ac),     H  =  2ac/(a  +  c). 


502  ARITHMETIC,  GEOMETRIC,  AND  HARMONIC  MEANS       CHAP. 

XT                                    K-a      a  +  c       %ac  2 

Hence  AH  =  ——  x =  ac  =  G , 

2        a  +  c 

which  proves  the  first  part  of  the  proposition. 
Again,      A  -  G  =  — \/(oc)  =  h(  y/a  -  \U)2. 

G-H=  sl(ac)-  —  =^ks/a-  *Jc)\ 
a  +  c      a+c 

Now,  since  a  and  c  are  both  positive,  Ja  and  N/c  are  both  real, 
therefore  ( s/a  -  Jcf  is  an  essentially  positive  quantity ;  also 
*J(ac)  and  a  +  c  are  both  positive.  Hence  both  A  -  G  and  G  -  H 
are  positive. 

Therefore  A >G>H. 

The  proposition  of  this  paragraph  (which  was  known  to  the 
Greek  geometers)  is  merely  a  particular  case  of  a  more  general 
proposition,  which  will  be  proved  in  chap.  xxiv. 

§  27.]  Notwithstanding  the  comparative  simplicity  of  the 
law  of  its  formation,  the  harmonic  series  does  not  belong  to  the  cate- 
gory of  series  that  can  be  summed.  Various  expressions  can  be 
found  to  represent  the  sum  to  n  terms,  but  all  of  them  partake 
of  the  nature  of  a  series  in  this  respect,  that  the  number  of  steps 
in  their  synthesis  is  a  function  of  n. 

It  will  be  a  good  exercise  in  algebraic  logic  to  prove  that 
the  sum  of  a  harmonic  series  to  n  terms  cannot  be  represented 
by  any  rational  algebraical  function  of  n.  The  demonstration 
will  be  found  to  require  nothing  beyond  the  elementary  principles 
of  algebraic  form  laid  down  in  the  earlier  chapters  of  this  work. 

Exercises  XL. 

Sum  the  following  arithmetical  progressions  : — 

(1.)  5  +  9  +  13+  ...  to  15  terms.  (2.)  3  +  3^  +  4  +  ...  to  30  terms. 

(3.)  13  +  12  +  11+.   .   .  to  24  terms.       (4.)  i  +  l+ ■   ■   •  to  16  term* 

,-k  1  ,  n-  1 

(o.)   -  +  —       +  ...  to  7t  terms. 
n       n 

(6.)  {a~nyt  +  {a?  +  n-)  +  {a  +  n)-+  .  .  .  to  to  terms. 

r)  l  +  l,     41  7  + 

(<•)  T_r7  +  -n772+  •  •  •   to  (  terms. 

(8.)  The  20th   term  of  an  A. P.   is  100,  and  the  sum  of  30  terms  is  500  ; 
find  the  sum  of  1000  terms  of  the  progression. 


XX 


EXERCISES  XL  503 


(9.)  The  first  term  of  an  A. P.  is  5,  the  number  of  its  terms  is  15,  and  the 
sum  is  390  ;  find  the  common  difference. 

(10.)  How  many  of  the  natural  numbers,  beginning  with  unity,  amount 
to  500500  ? 

(11.)  Show  that  an  infinite  number  of  A.P.'s  can  be  found  which  have 
the  property  that  the  sum  of  the  first  2m  terms  is  equal  to  the  sum  of  the 
next  m  terms,  m  being  a  given  integer.  Find  that  particular  A.  P.  having 
the  above  property  whose  first  term  is  unity. 

(12.)  An  author  wished  to  buy  up  the  whole  1000  copies  of  a  work  which 
he  had  published.  For  the  first  copy  he  paid  Is.  '  But  the  demand  raised 
the  price,  and  for  each  successive  copy  he  had  to  pay  Id.  more,  until  the 
whole  had  been  bought  up.     What  did  it  cost  him  ? 

(13.)  100  stones  are  placed  on  the  ground  at  intervals  of  5  yards  apart. 
A  runner  has  to  start  from  a  basket  5  yards  from  the  first  stone,  pick  up  the 
stones,  and  bring  them  back  to  the  basket  one  by  one.  How  many  yards 
has  he  to  run  altogether  ? 

(14.)  AB  is  a  straight  line  100  yards  long.  At  A  and  B  are  erected  per- 
pendiculars, AL,  BM,  whose  lengths  are  4  yards  and  46  yards  respectively.  At 
intervals  of  a  yard  along  AB  perpendiculars  are  erected  to  meet  the  line  LM. 
Find  the  sum  of  the  lengths  of  all  these  perpendiculars,  including  AL  and  BM. 
(15.)  Two  travellers  start  together  on  the  same  road.  One  of  them 
travels  uniformly  10  miles  a  day.  The  other  travels  8  miles  the  first  day, 
and  increases  his  pace  by  half  a  mile  a  day  each  succeeding  day.  After  how 
many  days  will  the  latter  overtake  the  former  ? 

(16.)  Two  men  set  out  from  the  two  ends  of  a  road  which  is  I  miles  long. 
The  first  travels  a  miles  the  first  day,  a  +  b  the  next,  a  +  2b  the  next,  and  so 
on.     The  second  travels  at  such  a  rate  that  the  sum  of  the  number  of  miles 
travelled  by  him  and  the  number  travelled  by  the  first  is  always  the  same  for 
any  one  day,  namely  c.     After  how  many  days  will  they  meet  ? 
(17.)  Insert  15  arithmetic  means  between  3  and  30. 
(18.)  Insert  10  arithmetic  means  between  -  3  and  +3. 
(19.)  A  certain  even  number  of  arithmetic  means  are  inserted  between  30 
and  40,  and  it  is  found  that  the  ratio  of  the  sum  of  the  first  half  of  these 
means  to  the  second  half  is  137  :  157.     Find  the  number  of  means  inserted. 

(20.)  Find  the  number  of  terms  of  the  A. P.  1  +8  +  15+  .  .  .  the  sum  of 
which  approaches  most  closely  to  1356. 

(21.)  If  the  common  difference  of  an  A.  P.  be  double  the  first  term,  the 
sum  of  m  terms  :  the  sum  of  n  terms  =  m- :  n-. 

(22.)  Find  four  numbers  in  A.  P.  such  that  the  sum  of  the  squares  of  the 
means  shall  be  106,  and  the  sum  of  the  squares  of  the  extremes  170. 

(23.)  If  four  quantities  be  in  A. P.,  show  that  the  sum  of  the  squares  of 
the  extremes  is  greater  than  the  sum  of  the  squares  of  the  means,  and  that 
the  product  of  the  extremes  is  less  than  the  product  of  the  means. 

(24.)  Find  the  sum  of  n  terms  of  the  series  whose  rth  term  is  |(3r  + 1). 
(25. )  Find  the  sum  of  n  terms  of  the  series  obtained  by  taking  the  1st,  rth, 
2rth,  3rth,  &c.  terms  of  the  A.  P.  whose  first  term  and  common  difference  are 
a  and  b  respectively. 


504  EXERCISES  XL 


CHAP. 


(26.)  If  the  sum  of  n  terms  of  a  series  be  always  n(n  +  2),  show  that  the 
series  is  an  A. P.  ;  and  find  its  first  term  and  common  difference. 

(27.)  Show  by  general  reasoning  regarding  the  form  of  the  sum  of  an 
A.  P.  that  if  the  sum  of  p  terms  be  P,  and  the  sum  of  q  terms  Q,  then  the 
sum  of  n  terms  is  Pn(?i  -  q)/p{p  -q)  +  Qn(n  -p>)lq{<l  -p). 

(28.)  Any  even  square,  (2n)2,  is  the  sum  of  n  terms  of  one  arithmetic 
series  of  integers  ;  and  any  odd  square,  (2ft  +  l)2,  is  the  sum  of  n  terms  of 
another  arithmetic  series  increased  by  1. 

(29.)  Find  n  consecutive  odd  numbers  whose  sum  shall  be  nP. 

Show  that  any  integral  cube  is  the  difference  of  two  integral  squares. 

(30.)  Find  the  nth  term  and  the  sum  of  the  series 
1-3  +  6-10  +  15-21+  .... 

(31.)  Sum  the  series  3  +  6+  .  .  .  +3w. 

(32.)  If  si,  s2,  .  .  .,  sp  be  the  sums  of  p  arithmetical  progressions,  each 
having  n  terms,  the  fh-st  terms  of  which  are  1,  2,  .  .  .,  p,  and  the  common 
differences  1,  3,  .  .  .,  2p-l  respectively,  show  that  5i  +  sL.+ .  .  .  +gp  is 
equal  to  the  sum  of  the  first  np  integral  numbers. 

(33.)  The  series  of  integral  numbers  is  divided  into  groups  as  follows  : — 
1,  |  2,  3,  |  4,  5,  6,  |  7,  8,  9,  10,  |  .  .  .,  show  that  the  sum  of  the  nth  group 
is  |(?i3  +  ?i). 

If  the  series  of  odd  integers  be  divided  in  the  same  way,  find  the  sum  of 
the  ?ith  group. 

Sum  the  following  series  : — 

(34.)  42  +  72+  .   .  .  +(3u+l)2.  (35.)  2„(?i3-l)(?i-l). 

(36.)  Zn\p  +  q(n-l)}{p  +  q(n-2)}. 

(37.)  l2-22  +  32-  .  .  .  +  (2?i-l)2-(2ra)2. 

(38.)  as  +  (a  +  bf+.  .   .  +(a  +  n~^lb)*. 

(39.)  (l3-i)  +  (23_2)  +  (33-3)+.   .   .   tow  terms. 

(40.)  1.22+2.32  +  3.42+.  .   .  ton  terms. 

(41.)  l  +  2.32  +  3.52  +  4.72  +  5.92+.   .   .  to  n  terms. 

(42.)  1.3.7  +  3.5.9  +  5.7.11+ .   .  .  to  n  terms. 

(43.)  l2  +  (l2  +  22)  +  (l2  +  22  +  32)+ .  .  .  ton  terms. 

(44. )  A  pyramid  of  shot  stands  on  an  equilateral  triangular  base  having 
30  shot  in  each  side.     How  many  shot  are  there  in  the  pyramid  ? 

(45.)  A  pyramid  of  shot  stands  on  a  square  base  having  m  shot  in  each 
side.     How  many  shot  in  the  pyramid  ? 

(46.)  A  symmetrical  wedge-shaped  pile  of  shot  ends  in  a  line  of  m  shot 
and  consists  of  I  layers.     How  many  shot  in  the  pile  ? 

(47.)  IfBSr=l',+2'-+  .  .  .  +n',thenn8r=pon<+1+p1nr+.  .  .  +pr+h  where 
Po,  Pi,  •  .  .  can  be  calculated  by  means  of  the  equations 

r+lC3po  +  rCiJ?i  =  rQi, 
H-lQs  p0  +  pC2.Pl  +  r-lCi  ^2  =  rC» , 


„Cr  denoting,  as  usual,  the  rth  binomial  coefficient  of  the  nth  rank. 


XX 


EXERCISES  XLI 


505 


(48.)  Show  that 
„Sr=»(»+l)(n-l)(H-2)...(»-r)| 

r-lSr 


H 

rtnr 


r(r+l)(»-r)(r-l)! 

r-nOr 


(r-i)r(n-r+l)l\(r-2)\  '  (r-2)(r-l)(n-r  +  2)2!(r-3)! 

(  ~  )riSr  1 

1.2(7i-l)(r-l)!i  ' 

where  r  !  stands  for  1.2.3  .   .  .  ?•. 

(49.)  If  ?r  denote  the  sum  of  the  products  r  at  a  time  of  1,  2,  3,  .  .  .,  n, 
and  Sr  denote  lr  +  2r  +  .  .  .  +  W,  show  that  ?-Pr=SiPr_r-S2P,-2  +  S3Pr-3~  .  .  . 
Hence  calculate  P2  and  P3. 

(50.)  UJ[x)  he  an  integral  function  of  x  of  the  (?•-  l)th  degree,  show  that 
f(x)-rC1f(x-l)+rQif(x-2) . . .  (-)rf{n-r)=0,  rCi,  & 
coefficients. 

Exercises  XLI. 
Sum  the  following  geometric  progressions  : — 

(1.)  6  +  18  +  54+ .   .   .  to  12  terms.     (2.)  6-18  +  54- 

1      1 


being  binomial 


(3.)  -3333.  .  .  to  n  terms. 
(5.)  6-4+  .  .   .  to  10  terms 

^  V3  +  1     V3  +  2 


(4-)  J-i  +  P" 


.  to  12  terms, 
to  n  terms. 


to  20  terms. 


('■)  1+3+32+-  •  • 

(9.)  l-x  +  x2-x3  + 
(10.)  V2  +  ^+.   • 

(12.)  a±?-a-^  + 


to  n  terms. 

.  .  to  oo,  a;<l. 

to  00.  (11.) 

,    .   to  00  . 


(8.)  1-5+i- 


2     2' 

\/3 


V3 

V3  +  1  '  V3  +  3 


+ 


to  00 . 


+ 


to  00. 


a-x    a+x 

Sum,  by  means  of  the  formula  for  a  G.P.,  the  following  : — 
(13.)  l+x-x2-x3  +  x4  +  x5-x6-x7+  .   .   .  tooo,a;<l. 

(14.)  {x-y)+(l-^y(t3-ty.  .  .  to  *  terms. 

(15.)  l+(x  +  y)  +  (x2  +  o:y  +  y2){-{xi  +  x2y  +  xy2  +  y5)+.   .   .  to  n  terms. 

(16.)  -33  +-333+  -3333  +  .  .   .  to  n  terms. 

Sum  the  series  whose  ?ith  terms  are  as  follows  : — 

(17.)  2"3"+1.  (18.)  {xn  +  n)(xn-n). 

(19.)  Ae»-lVy»-.i).  (20.)  (jt»-gr)(p*+r). 

(21.)  2»(3"-1  +  3»-2+.  .   .+1).  (22.)  (-l)"a3''. 

(23. )  Sum  to  «  terms  the  series  (rn  +  l/>-")2  +  (r^1  +  l/r"+1)2  +  .   .   .     . 
(24.)  Sum  to  ?i  terms  (l  +  l//-)2  +  (l  +  l/r2)-+.   .   .     . 
(25.)  Show  that  {a  +  b)n-b"  =  abn~l  +  ab"~2(a  +  b)+.   .   .  +a(a  +  b)n-\ 
(26.)  If  S,  denote  the  sum  of  n  terms  of  a  G.P.  beginning  with  the  tth 
term,  sum  the  series  S1  +  S0+  .   .    .  +S(. 
(27.)  Show  that  £/('037)=-3. 


506  EXEECISES  XLI  chap. 

Sum  the  following  series  to  n  terms,  and,  where  admissible,  to  infinity  : — 

(28.)  l-2x  +  3x2-lxs+.   .   .     .         (29.)  1-f +  £-•£+.   .   .     . 
9-     S2     42  12     2  3     3  4 

(so.)  1-I44+-.  •  •       <31->  1+ir+1r+ir+-  ■  •  ■ 

(32.)  l3  +  23x  +  Ssx2+.   .   .     . 

12      3      12      3 
(33.)  =  +  =5  +  =;  +  =3  +  ss  +  =a+.  •   .  to    oo,    where    the    numerators   recur 

7     7-     iJ     i      r     r 

with  the  period  1,  2,  3. 

(34. )  -  +  — ,  +  -=  +  -:  +  —.  +  -a  +  .   .   .   to  3)i  terms,  where  the  numerators  recur 

with  the  period  a,  J,  c. 

(35.)  A  servant  agrees  to  serve  his  master  for  twelve  months,  his  wages  to 
be  one  farthing  for  the  first  month,  a  penny  for  the  second,  fourpence  for  the 
third,  and  so  on.     What  did  he  receive  for  the  year's  service  ? 

(36. )  A  precipitate  at  the  bottom  of  a  beaker  of  volume  V  always  retains 
about  it  a  volume  v  of  liquid.  It  was  originally  precipitated  in  an  alkaline 
solution  ;  find  what  percentage  of  this  solution  remains  about  it  after  it  has 
been  washed  n  times  by  filling  the  beaker  with  distilled  water  and  emptying 
it.     Neglect  the  volume  of  the  precipitate  itself. 

(37.)  The  middle  points  of  the  sides  of  a  triangle  of  area  Ai  form  the 
vertices  of  a  second  triangle  of  area  A2 ;  from  A2  a  third  triangle  of  area  A3  is 
derived  in  the  same  way  ;  and  so  on,  ad  infinitum.  Find  the  sum  of  the 
areas  of  all  the  triangles  thus  formed. 

(38.)  OX,  OY  are  two  given  straight  lines.  From  a  point  in  OX  a  perpend- 
icular is  drawn  to  OY  ;  from  the  foot  of  that  perpendicular  a  perpendicular 
on  OX  ;  and  so  on,  ad  infinitum.  If  the  lengths  of  the  first  and  second  per- 
pendicular be  a  and  b  respectively,  find  the  sum  of  the  lengths  of  all  the  per- 
pendiculars ;  and  also  the  sum  of  the  areas  of  all  the  right-angled  triangles  in 
the  figure  whose  vertices  lie  on  OY  and  whose  bases  lie  on  OX. 

(39.)  The  population  of  a  certain  town  is  P  at  a  certain  epoch.  Annually 
it  loses  d  per  cent  by  deaths,  and  gains  b  per  cent  by  births,  and  annually  a 
fixed  number  E  emigrate.     Find  the  population  after  the  lapse  of  n  years. 

2,  a,  r,  n,  I,  having  the  meanings  assigned  to  them  in  §  12,  solve  the 
following  problems  :  — 

(40. )  Express  2  in  terms  of  a,  n,  I ;  and  also  in  terms  of  r,  n,  I. 

(41.)  2=  4400,     «  =  11,     »=4,.findr. 

(42.)  2  =  180,        r  =  3,       n  =  5,  find  a. 

(43.)  2  =  95,         a  =  20,     n  =  S,  find  r. 

(44.)  2  =  155,       «  =  5,       »=3,  findr. 

(45.)  2  =  605,       a=5,       r  =  3,  find  n. 

(46.)  If  the  second  term  of  a  G.P.  be  40,  and  the  fourth  term  1000,  find 
the  sum  of  10  terms. 


XX 


EXEKCISES  XLI,  XLII  507 


(47.)  Insert  one  geometric  mean  between  \/3/\/2  and  3V3/2V2- 

(48.)  Insert  three  geometric  means  between  27/8  and  2/3. 

(49.)  Insert  four  geometric  means  between  2  and  64. 

(50.)  Find  the  geometric  mean  of  4,  48,  and  405. 

(51.)  The  geometric  mean  between  two  numbers  is  12,  and  the  arithmetic 
mean  is  25§ :  find  the  numbers. 

(52.)  Four  numbers  are  in  G.P.,  the  sum  of  the  first  two  is  44,  and  of  the 
last  two  396  :  find  them. 

(53.)  Find  what  common  quantity  must  be  added  to  a,  b,  c  to  bring  them 
into  G.P. 

(54.)  To  each  of  the  first  two  of  the  four  numbers  3,  35,  190,  990  is  added 
SB,  and  to  each  of  the  last  two  y.  The  numbers  then  form  a  G.P.  :  find  x 
and  y. 

(55.)  Given  the  sum  to  infinity  of  a  convergent  G.P.,  and  also  the  sum  to 
infinity  of  the  squares  of  its  terms,  find  the  first  term  and  the  common  ratio. 

(56.)  IfS=Oi  +  a2+.  .  .  +  «„be  a  G.P.,  then  S'  =  l/a1  +  l/a-2+  .  .  . +l/an 
is  a  G.P.,  and  S/S'  =  «!«„. 

(57.)  If  four  quantities  be  in  G.P.,  the  sum  of  the  squares  of  the  extremes 
is  greater  than  the  sum  of  the  squares  of  the  means. 

(58.)  Sum  In  terms  of  a  series  in  which  every  even  term  is  a  times  the 
term  before  it,  and  every  odd  term  c  times  the  term  before  it,  tire  first  term 

being  1. 

(59.)  If  x  =  a  +  a/r  +  a/r2+  .   .   .  ad  oo  , 

y  =  b-  b/r+  bjr2  -  .   .  .  ad  oo , 
z  =  c  +  clr2+cjri+  .   .   .  adoo, 
then  xylz  =  ab/c. 

(60. )  Find  the  sum  of  all  the  products  three  and  three  of  the  terms  of  an 
infinite  G.P.,  and  if  this  be  one-third  the  sum  of  the  cubes  of  the  terms,  show 
that  r=\. 

Exercises  XLII. 

(1.)  Insert  two  harmonic  means  between  1  and  3,  and  five  between  6  and  8. 

(2.)  Find  the  harmonic  mean  of  1  and  10,  and  also  the  harmonic  mean  of 
1,  2,  3,  4,  5. 

(3.)  Show  that  4,  6,  12  are  in  H.P.,  and  continue  the  progression  both 
ways. 

(4.)  Find  the  H.P.  whose  3rd  term  is  5  and  whose  5th  term  is  9. 

(5.)  Find  the  H.P.  whose  joth  term  is  P  and  whose  gill  term  is  Q. 

(6. )  Show  that  the  harmonic  mean  between  the  arithmetic  and  geometric 
means  of  a  and  b  is  2(a  +  b)/ {{a/b^  +  (b/a)i}n: 

(7.)  Four  numbers  are  proportionals  ;  show  that,  if  the  first  three  are  in 
G.P.,  the  last  three  are  in  G.P. 

(8.)  Three  numbers  are  in  G.P.  ;  if  each  be  increased  by  15,  they  are  in 
H.P. :  find  them. 

(9. )  Between  two  quantities  a  harmonic  mean  is  inserted  ;  and  between 
each  adjacent  pair  of  the  three  thus  obtained  is  inserted  a  geometric  mean. 


508  EXERCISES  XLII  chap,  xx 

It  is  now  found  that  the  three  inserted  means  are  in  A.  P. :  show  that  the  ratio 
of  the  two  quantities  is  unity. 

(10.)  The  sides  of  a  right-angled  triangle  are  in  A.  P. :  show  that  they  are 
proportional  to  3,  4,  5. 

(11.)  a,  b,  c  are  in  A.P.,  and  a,  b,  d  in  H.P.  :  show  that  c/d  = 
1  -  2(o  -  bflab. 

(12.)  If  x  be  any  term  in  an  A. P.  whose  two  first  terms  are  a,  b,  y,  the 
term  of  the  same  order  in  a  H.P.  commencing  with  the  same  two  terms,  then 
(x-a)/(y-x)  =  b/(y-b). 

(13.)  If  a2,  b\  c2  be  in  A. P.,  then  1/(5  +  c),  l/(c  +  a),  lfta  +  b)  are  in  A. P. 

(14.)  If  P  be  the  product  of  n  quantities  in  G.P.,  S  their  sum,  and  S'  the 
sum  of  their  reciprocals,  then  P2=(S/S')n. 

(15.)  If  a,  b,  c  be  the  pth,  qth,  and  rth  terms  both  of  an  A.P.  and  of  a 
G.P.,  then  a*-"  &*-»«»-» =1. 

(16.)  If  P,  Q,  R  be  the  .pth,  qth.,  rth  terms  of  a  H.P.,  then  2{PQ(j3-  q)} 
=  0,  and  {S(g2-r2)/P2}2  =  4{2to-r)/P2}{2?r(?-r)/F}. 

/17.)  If  the  sum  of  m  terms  of  an  A.P.  be  equal  to  the  sum  of  the  next  n, 
and  also  to  the  sum  of  the  next^J,  then  (m  +  n)  (1/n  -  l/p)  =  (n  +p)  (1/m  -  I/n). 

(18.)  If  the  squared  differences  of  p,  <?>  r  be  in  A.P.,  then  the  differences 
taken  in  cyclical  order  are  in  H.P. 

(19.)  If  a  +  b  +  c,  a2  +  &2  +  c2,  a?  +  bz  +  <?  be  in  G.P.,  prove  that  the  common 
ratio  is  ^2a  -  3a&c/226c. 

(20.)  If  x,  y,  z  be  in  A. P.,  ax,  by,  cz  in  G.P.,  and  a,  b,  c  in  H.P.,  then 
H.M.  of  a,  c:G.M.  of  a,  c  =  H.M.  oix,  z:G.M.  of  a,  z. 

(21.)  Ifa2  +  62-c2,  P  +  c--a",  c2-i-a2-&2  be  in  G.P.,  then  a2/c2  +  c2/i2, 
&2/c2  +  c2/62,  a2/62  +  62/c2  are  in  A.P. 

(22.)  If  a,  b,  c,  d  be  in  G.P.,  then  abcdl  2  -  ]  =  (2a)2,  and 

V(^  +  ^)  +  V(6*  +  c*)  +  V(c« +  *)_&«■     ^  „  4     m 

(23.)  The  sum  of  the  n  geometric  means  between  a  and  k  is 
{aVWik  -  aWl»W)l(tMn+1)  -  a1  (n+V). 

(24.)  If  Ai,  A2,  .  .  .,  A„  be  the  n  arithmetic  means,  and  H^  H2,  .  .  ., 
H„  the  n  harmonic  means,  between  a  and  c,  sum  to  n  terms  the  series  whose 
rth  term  is  (Ar-a)(Hr-«)/Hr. 

(25.)  If«i,a2,   .   .  .,  an  be  in  G. P. ,  then 
(^  +  a,2  +  03)-  +  {d2  +  a3  +  en)2  +  .   .   .  +  (a„_n  +  «.„_;,  +  anf 

=  («!2  +  «!«-,  +  «.o2)2(a!2«-4  -  «.22"-4)/(«l2  -  «2>15"-4. 

(26.)  If  ar,  br  be  the  arithmetic  and  geometric  means  respectively  between 
«r_i  and  br-i,  show  that 

a„-2-  {an *±(a„2-&„2)  }2, 
Z>„_2  =  {aj 2f{an2-bn-)  }2. 
(27.)  If  «j,  a2,  .  .   .,  an  be  real,  and  if 
(ai2  +  022+.  .  . +a„-i2)(a22  +  (T32+ .   .   .  +  a„2)  =  {aiao  +  a-2ai  +  .   .   .  +  a„-ia„),2 
then  ai,  a-2,   •   ■   -,  cin  are  in  G.P. 


CHAPTEE    XXI. 
Logarithms. 

§  1.]  It  is  necessary  for  the  purposes  of  this  chapter  to  define 
and  discuss  more  closely  than  we  have  yet  done  the  properties 
of  the  exponential  function  ax.  For  the  present  we  shall  sup- 
pose that  a  is  a  positive  real  quantity  greater  than  1.  AY  hat- 
ever  positive  value,  commensurable  or  incommensurable,  we  give 
to  x,  we  can  always  find  two  commensurable  values,  mjn  and 
(m  +  l)/n  (where  m  and  n  are  positive  integers),  between  which 
x  lies,  and  which  differ  from  one  another  as  little  as  we  please, 
see  chap,  xiii.,  §  15.  In  defining  ax  for  positive  values  of  x,  we 
suppose  x  replaced  by  one  (say  m/n)  of  these  two  values,  which 
we  may  suppose  chosen  so  close  together  that,  for  the  purpose 
in  hand,  it  is  indifferent  which  we  use.  We  thus  have  merely 
to  consider  a'",ln ;  and  the  understanding  is  that,  as  in  the 
chapter  on  fractional  indices,  we  regard  only  the  real  positive 
value  of  the  nth  root ;  so  that  am,n  may  be  read  indifferently  as 
(  Z/a)m,  or  as  yam. 

For  negative  values  of  x  we  define  ax  by  the  equation 
ax  =  lja~x,  in  accordance  with  the  laws  of  negative  indices. 

§  2.]  We  shall  now  show  that  ax,  defined  as  above,  is  a  continu- 
ous function  of  x  susceptible  of  all  positive  values  between  0  and  +  oo  . 

1st.  Let  y  be  any  positive  quantity  greater  than  1,  and  let 
n  be  any  positive  integer.  Since  a  >  1 ,  alln  >  1  ;  but,  by  suffi- 
ciently increasing  n,  we  may  make  a1!n  exceed  1  by  as  little  as 
we  please.  Also,  when  n  is  given,  we  can,  by  sufficiently  in- 
creasing w,  make  am!n  as  great  as  we  please.*     Hence,  whatever 

*  See  chap,  xi.,  §  14. 


510 


CC  CONTINUOUS ITS  GRAPH 


CHAP. 


may  be  the  value  of  y,  we  can  so  choose  n  that  a1/n<y ;  and  then 
y  will  lie  between  two  consecutive  integral  powers  of  al!n ;  say 
amin  <  y  <  a(»»+iy»  Now  the  difference  between  these  two  values 
of  ax  is  amln(a1/n  -  1);  and  this,  by  sufficiently  increasing  n,  we 
may  make  as  small  as  we  please.  Hence,  given  any  positive 
quantity  y  >  \,  we  can  find  a  value  of  x  such  that  ax  shall  be  as 
nearly  equal  to  y  as  we  please. 

2nd.  Let  y  be  positive  and  <  1  ;  then  1/y  is  positive  and 
greater  than  1.  Hence  we  can  find  a  value  of  x,  say  x',  such 
that  ax'  =  \jy  as  nearly  as  we  please.      Hence  a~x'  =  y. 

We  may  make  y  pass  continuously  through  all  possible  values 
from  0  to  +  oo  .  Hence  ax  is  susceptible  of  all  positive  values 
from  0  to  +  oo  .  It  is  obviously  a  continuous  function,  since 
the  difference  of  two  finite  values  corresponding  to  x  =  m  'n  and 
x  =  (wi  +  1  )/n  is  am!n(a1/n  -  1 ),  which  can  be  made  as  small  as 
we  please  by  sufficiently  increasing  n. 

Cor.   We  have  the  following  set  of  corresponding  values  : — 
X=  -oo,        -,       -1,      0,       +,      1,       +co; 
y  =  ax  =  0.     <  1,       1/a,      1,    >  1,      a,      +  oo . 


Fio.  1. 


In  Fig.    1   the  full-drawn   curve  is  the   graph   of  the   function 
y  ~  lO*  ;  the  dotted  curve  is  the  graph  of  y  =  100*. 


xxi  DEFINITION  OF  LOGARITHMIC  FUNCTION  511 

It  will  be  observed  that  the  two  curves  cross  the  axis  of  y 
at  the  same  point  B,  whose  ordinate  is  +  1  ;  and  that  for  one 
and  the  same  value  of  y  the  abscissa  of  the  one  curve  is  double 
that  of  the  other. 

§  3.]  The  reasoning  by  Avhich  we  showed  that  the  equation 
y  =  ax,  certain  restrictions  being  understood,  determines  y  as  a 
continuous  function  of  x,  shows  that  the  same  equation,  under 
the  same  restrictions,  determines  a;  as  a  contiimous  function  of  y. 
This  point  will  perhaps  be  made  clearer  by  graphical  considera- 
tions. If  we  obtain  the  graph  of  y  as  a  function  of  x  from  the 
equation  y  =  ax,  the  curve  so  obtained  enables  us  to  calculate  x 
when  y  is  given  ;  that  is  to  say,  is  the  graph  of  x  regarded  as  a 
function  of  y.  Thus,  if  we  look  at  the  matter  from  a  graphical 
point  of  view,  we  see  that  the  continuity  of  the  graph  means  the 
continuity  of  y  as  a  function  of  x,  and  also  the  continuity  of  x  as 
a  function  of  y. 

When  we  determine  x  as  a  function  of  y  by  means  of  the 
equation  y  =  ax,  we  obviously  introduce  a  new  kind  of  transcend- 
ental function  into  algebra,  and  some  additional  nomenclature 
becomes  necessary  to  enable  us  to  speak  of  it  with  brevity  and 
clearness. 

The  constant  quantity  a  is  called  the  base. 

y  is  called  the  exponential  of  x  to  base  a  (and  is  sometimes 
written  expa;r).* 

x  is  called  the  logarithm  of  y  to  base  a,  and  is  usually  written 

logay- 

The  two  equations 

y  =  a*  (1), 

z  =  logay  (2), 

are  thus  merely  different  ways  of  writing  the  same  functional 
relation.  It  follows,  therefore,  that  all  the  properties  of  our  new 
logarithmic  function  must  be  derivable  from  the  properties  of  our  old 
exponential  function,  that  is  to  say,  from  the  laws  of  indices. 

*  This  notation  is  little  used  in  elementary  text-books,  but  it  is  con- 
venient when  in  place  of  x  we  have  some  complicated  function  of  x.  Thus 
expa(l  +X  +  X2)  is  easier  to  print  than  a1+x+x2. 


512  FUNDAMENTAL  PEOPERTIES  OF  LOGARITHMS  chap. 

The  student  should  also  notice  that  it  follows  from  (1)  and 
(2)  that  the  equation 

y  =  a1****  (3) 

is  an  identity. 

§  4.]  If  the  same  hase  a  be  understood  throughout,  we  have 
the  following  leading  properties  of  the  logarithmic  function : — 

I.  The  logarithm  of  a  product  of  positive  numbers  is  the  sum  of 
the  logarithms  of  the  separate  factors. 

II.  The  logarithm  of  the  quotient  of  hvo  positive  numbers  is  the 
excess  of  the  logarithm  of  the  dividend  over  the  logarithm  of  the  divisor. 

III.  The  logarithm  of  any  power  {positive  or  negative,  integral 
or  fractional)  of  a  positive  number  is  equal  to  the  logarithm  of  the 
number  multiplied  by  the  power. 

Let  ?/,,  y2,  .  .  .,  yn  be  n  positive  numbers,  xlt  x3,  .  .  .,  xn  their 
respective  logarithms  to  base  a,  so  that 

«i  =  loga?/1)     x2  =  \ogay2,     .  .   .,     xn  =  logayn. 
By  the  definition  of  a  logarithm  we  have 

yx  =  ax\     y2  =  ax\     .  .  .,    yn  =  ax\ 
Hence         y^Ji-  ■  ■  II n  =  aXlax- .  . .  aXn  -  axi+x*+  •  ■  •  +Xn, 

by  the  laws  of  indices. 
Hence,  by  the  definition  of  a  logarithm, 

xx  +  x.2  +  .  .  .  +  xn  =  logafay, .  .  .  yn), 
that  is,     log^  +  loga?/2  +  .  .  .  +  logayn  =  log0(y,y9 .  . .  yn). 
We  have  thus  established  I. 

Again,  y1/y2  =  axi/ax~  =  ax^ _a'2, 

by  the  laws  of  indices. 
Hence,  by  the  definition  of  a  logarithm, 

xx  -xa  =  logaiyM, 
that  is,  logay,  -  \ogay,  =  logatyjyj), 

which  is  the  analytical  expression  of  II. 

Again,  y*  =  (axi)r  =  arx\ 

by  the  laws  of  indices. 


xxi  EXAMPLES  513 

Hence,  by  the  definition  of  a  logarithm, 

ra,  =  \ogayx\ 

that  is,  r  logay1  =  log*^, 

which  is  the  analytical  expression  of  III. 

Example  1. 

log  21  =  log  (7x3)  =  log  7  + log  3. 

As  the  equation  is  true  for  any  base,  provided  all  the  logarithms  have  the 
same  base,  it  is  needless  to  indicate  the  base  by  writing  the  suffix. 

Example  2. 

log  (113/29)= log  113  -log  29. 

Example  3. 

log  (540/539)  =  log  (22. 33.  5/72. 11), 

=  2  log2  +  3  log3  +  log5-2  log7-logll. 
Example  4. 

log  4/(49)/  7/(21)  =  log  (72'*/3^7n 

=  #log7-f  log3-f  log 7, 
=Hlog7-f  log 3. 


COMPUTATION    AND    TABULATION    OF   LOGARITHMS. 

§  5.]  If  the  base  of  a  system  of  logarithms  be  greater  than 
unity,  we  have  seen  that  the  logarithm  of  any  positive  number 
greater  than  unity  is  positive ;  and  the  logarithm  of  any  positive 
number  less  than  unity  is  negative. 

The  logarithm  of  unity  itself  is  always  zero,  whatever  the  base 
may  be. 

The  logarithm  of  the  base  itself  is  of  course  unity,  since  a  =  a1. 

The  logarithm  of  any  power  of  the  base,  say  ar,  is  r ;  and,  in 
particular,  the  logarithm  of  the  reciprocal  of  the  base  is  -  1. 

The  logarithm  of  +  oo  is  +  cc  ,  and  the  logarithm  of  0  is  -  oo  . 

It  is  further  obvious  that  the  logarithm  of  a  negative  number 
could  not  (with  our  present  understanding)  be  any  real  quantity. 
With  such,  however,  we  are  not  at  present  concerned. 

The  logarithm  of  any  number  which  is  not  an  integral  power 

of  the  base  will  be  some  fractional  number,  positive  or  negative, 

as  the  case  may  be.     For  reasons  that  will  appear  presently,  it  is 

usual  so  to  arrange  a  logarithm  that  it  consists  of  a  positive 

VOL.  I  2  L 


514 


DETERMINATION  OF  CHARACTERISTIC 


CHAP. 


fractional  part  less  than  unity,  and  an  integral  part,  positive  or 
negative,  as  the  case  may  be. 

The  positive  fractional  part  is  called  the  mantissa. 

The  integral  part  is  called  the  cliaracteristic. 

For  example,  the  logarithm  of  "0451  to  base  10  is  the  negative 
number  -  1  '3458235.    In  accordance  with  the  above  understand- 


ing, we  should  write 


log10-0451 


=  -  1-3458235  =  -  2  +  (1  -  -3458235), 
-  -  2  +  '6541765. 


For  the  sake  of  compactness,  and  at  the  same  time  to  prevent 
confusion,  this  is  usually  written 

log10-0451  =  2-6541765. 

In  this  case  then  the  characteristic  is  2  (that  is,  -  2),  and  the 
mantissa  is  -6541765. 

§  6.]  To  find  the  logarithm  of  a  given  number  y  to  a  given 
base  a  is  the  same  problem  as  to  solve  the  equation 

a*  =  y, 

where  a  and  y  are  given  and  x  is  the  unknown  quantity. 

There  are  various  ways  in  which  this  may  be  done ;  and  it 
will  be  instructive  to  describe  here  some  of  the  more  elementary, 
although  at  the  same  time  more  laborious,  approximative  methods 
that  might  be  used. 

In  the  first  place,  it  is  always  easy  to  find  the  characteristic 
or  integral  part  of  the  logarithm  of  any  given  number  y.  We 
have  simply  to  find  by  trial  hvo  consecutive  integral  powers  of  the 
base  between  which  the  given  number  y  lies.  The  algebraically  less  of 
these  two  is  the  characteristic. 

Example  1. 

To  find  the  characteristic  of  log3451. 

We  have  the  following  values  for  consecutive  integral  powers  of  3  : — 


Power 

1 

2 

3 

4 

5 

6 

Value 

3 

9 

27 

81 

243 

729 

XXI 


LOGARITHMS  TO  BASK  10 


515 


Hence  35<451<3fi.     Hence  log3451  lies  between  5  am!  6. 

log3451  =  5+a  proper  fraction. 
Hence  char.  log3451=5. 

Example  2. 

Find  the  characteristic  of  log3,0451.     We  have 


Therefore 


Powers  of  Base 

0 

-1 

-2 

-3 

Values 

1 

•333  .  .  . 

•111.  .  . 

•037  .  .  . 

Hence  3~3<  '0451  <3~2 
Hence 


;  that  is  to  say, 
log3-0451  =  -  3  +  a  proper  fraction, 
char.  log3-0451=3. 


When  the  base  of  the  system  of  logarithms  is  the  radix  of 
the  scale  of  numerical  notation,  the  characteristic  can  always  be 
obtained  by  merely  counting  the  digits. 

For  example,  if  the  radix  and  base  be  each  10,  then 

If  the  number  have  an  integral  part,  the  characteristic  of  its 
logarithm  is  +  {one  less  than  the  number  of  digits  in  the  integral 
part). 

If  the  number  have  no  integral  part,  the  characteristic  is  -  {one 
more  than  the  number  of  zeros  that  follow  the  decimal  point). 

The  proof  of  these  rules  consists  simply  in  the  fact  that,  if  a 
number  lie  between  10M  and  10n+1,  the  number  of  digits  by 
which  it  is  expressed  is  n  +  1  ;  and,  if  a  number  lie  between 
10 -(*+!)  and  10_ri,  the  number  of  zeros  after  the  decimal  point 
is  n. 

For  example,  351  lies  between  102andl03.  Heucechar.  logi0351  =  2  =  3  -  1, 
according  to  the  rule. 

Again,  -0351  lies  between  '01  and  T,  that  is,  between  10-2  and  10'1. 
Hence  char,  log w '0351=  -  2~  -  (1  +  1),  which  agrees  with  the  rule. 

The  rule  suggests  at  once  that,  if  1 0  be  adopted  as  the  base  of 
our  system  of  logarithms,  then  the  characteristic  of  a  logarithm  depends 
merely  on  the  position  of  the  decimal  point ;  and  the  mantissa  is  in- 
dependent of  the  position  of  the  decimal  point,  but  depends  merely  on 
the  succession  of  digits. 


516      COMPUTATION  OF  LOGARITHMS  BY  SOLUTION  OF  ax  =  y    chap. 

We  may  formally  prove  this  important  proposition  as 
follows  : — 

Let  N  be  any  number  formed  by  a  given  succession  of  digits, 
c  the  characteristic,  and  m  the  mantissa  of  its  logarithm.  Then 
any  other  number  which  has  the  same  succession  of  digits  as  N, 
but  has  the  decimal  point  placed  differently,  will  have  the  form 
10*N,  where  i  is  an  integer,  positive  or  negative,  as  the  case  may  be. 
But  log1010*N  =  log.JO1'  +  log10N,  by  §  4,  =  i  +  log10N  =  (i  +  c)  +  m. 
Now,  since  by  hypothesis  m  is  a  positive  proper  fraction,  and  c 
and  i  are  integers,  the  mantissa  of  logI010fN  is  m,  and  the 
characteristic  is  i  +  c.  In  other  words,  the  characteristic  alone 
is  altered  by  shifting  the  decimal  point. 

§  7.]  The  process  used  in  §  6  for  finding  the  characteristic 
of  a  logarithm  can  be  extended  into  a  method  for  finding  the 
mantissa  digit  by  digit. 

Example. 

To  calculate  log104-217  to  three  places  of  decimals. 

The  characteristic  is  obviously  0.  Let  the  three  first  digits  of  the  mantissa 
be  xyz.     Then  we  have 

4-217  =  10°-^,  hence  (4-217)10=10*-3«. 

We  must  now  calculate  the  10th  power  of  4-217.  In  so  doing,  however, 
there  is  no  need  to  find  all  the  significant  figures— a  few  of  the  highest  will 
suffice.     We  thus  find 

1778400  =  10^-^. 

We  now  see  that  x  is  the  characteristic  of  logi01778400.  Hencea:=6. 
Dividing  by  106,  and  raising  both  sides  of  the  resulting  equation  to  the  10th 
power,  we  find 

(l-77S)in  =  10J'-2  ;  hence  315'7  =  10^. 
Hence  y  =  2.     Dividing  by  102,  and  raising  to  the  10th  power,  we  now  find 

(3-16)10=102 ;  hence  99280  =  10*. 
Hence  z  =  5  very  nearly. 

Wc  conclude,  therefore,  that 

log104-217=-625  nearly. 

This  method  of  computing  logarithms  is  far  too  laborious  to 
be  of  any  practical  use,  even  if  it  were  made  complete  by  the 
addition  of  a  test  to  ascertain  what  effect  the  figures  neglected 
in  the  calculation  of  the  10th  powers  produce  on  a  given  decimal 
place   of  the  logarithm ;  it  has,  however,   a  certain  theoretical 


xxi  COMPUTATION  BY  INSERTING  GEOMETRIC  MEANS  517 

interest  on  account  of  its  direct  connection  with  the  definition  of 
a  logarithm. 

By  a  somewhat  similar  process  a  logarithm  can  he  expressed 
as  a  continued  fraction. 

§  8.]  If  a  series  of  numbers  be  in  geometric  progression,  their 
logarithms  are  in  arithmetic  progression. 

Let  the  numbers  in  question  be  y1}  y.2,  ya,  .  .  .,  yn.  Let  the 
logarithm  of  the  first  to  base  a  be  a,  and  the  logarithm  of  the 
common  ratio  of  the  G.P.  yl}  y2,  y.,,  .  .  .,  yn  to  the  same  base  be 
(3.    Then  we  have  the  following  series  of  corresponding  values  : — 

Vi,    y-2,     y*,  •  •  •,  Vu, 

ii      ii        ii  ii 

aa,     ax+?,    ax+-<\         a*+(».-i)^ 

from  which  the  truth  of  the  proposition  is  manifest. 

As  a  matter  of  history,  it  was  this  idea  of  comparing  two 
series  of  numbers,  one  in  geometric,  the  other  in  arithmetic  pro- 
gression, that  led  to  the  invention  of  logarithms ;  and  it  was  on 
this  comparison  that  most  of  the  early  methods  of  computing 
them  were  founded. 

The  following  may  be  taken  as  an  example.  Let  us  suppose 
that  we  know  the  logarithms  xx  and  a"9  of  two  given  numbers,  y, 
and  y9 ;  then  we  can  find  the  logarithms  of  as  many  numbers 
lying  between  yx  and  y9  as  we  please.      We  have 

Vi  =  aXl,     ft  =  a*3- 
Let  us  insert  a  geometric  mean,  y6,  between  yl  and  yg,  then 

%  =  (Mi.)*  =  «(*1+a"9)/2  =  «*,  say, 
where  xb  is   the  arithmetic  mean  between  x^  and  xa.     We  have 
now  the  following  system  : — 

Logarithm     xl     xs     xti, 

Number         yx     y,     y9. 
Next  insert  geometric  means  between  y},   yB  and  yu  y9.     The 
logarithms  of  the  corresponding  numbers  will  be  the  arithmetic 
means  between  xu  xb  and  xb,  xy.     We  thus  have  the  system — 

Logarithms     x1,     xs,     xb,     x7,     x9 
Numbers         yu     ya,     ys,     y7,     y9. 


^a  > 


518 


COMPUTATION  BY  INSERTING  GEOMETRIC  MEANS        chai\ 


Proceeding  in  like  manner,  we  derive  the  system — 


Logarithms 


wo 


/y*  /y  rv*  /■>•  iy  iy*  <y*     • 

[q,  a,2?  «^3  j  w4,  WfiJ  rt6,  .('7,  «^g,  «*/g  J 

Numbers         y„     y9J     y3J     yi}     y„     y6,     y7,     y8,     y9; 

and  so  on.  Each  step  in  this  calculation  requires  merely  a  multi- 
plication, the  extraction  of  a  square  root,  an  addition  accompanied 
by  division  by  2,  and  each  step  furnishes  us  with  a  new  number 
and  the  corresponding  logarithm. 

Since  x1}  x2,  .  .  .,  xn  form  an  A.P.,  the  logarithms  are  spaced 
out  equally,  but  the  same  is  not  true  of  the  corresponding  num- 
bers which  are  in  G.P.  It  is  therefore  a  table  of  antilogarithms  * 
that  we  should  calculate  most  readily  by  this  method.  It  will 
be  observed,  however,  that  by  inserting  a  sufficient  number  of 
means  we  can  make  the  successive  numbers  differ  from  each  other 
as  little  as  we  please ;  and  by  means  of  the  method  of  interpola- 
tion by  first  differences,  explained  in  the  last  section  of  this 
chapter,  we  could  space  out  the  numbers  equally,  and  thus  con- 
vert our  table  of  antilogarithms  into  a  table  of  logarithms  of  the 
ordinary  kind. 

As  a  numerical  example  we  may  put  a  =  10,  y1  =  l,ys  =  10;  thena^=0,  a'9=l. 
Proceeding  as  above  indicated,  we  should  arrive  at  the  following  table  : — 


Number. 

Logarithm. 

Number. 

Logarithm. 

1-0000 

o-oooo 

4-2170 

0-6250 

1-3336 

0-1250 

5-6235 

0-7500 

1-7783 

0-2500 

7-4990 

0-8750 

2-3714 

0-3750 

10-0000 

1  -oooo 

3-1622 

0-5000 

§  9.]  In  computing  logarithms,  by  whatever  method,  it  is 
obvious  that  it  is  not  necessary  to  calculate  independently  the 
logarithms  of  composite  integers  after  we  have  found  to  a  suffi- 
cient degree  of  accuracy  the  logarithms  of  all  primes  up  to  a 
certain  magnitude.  Thus,  for  example,  log  4851  =  log  32.7211 
=  2  log  3  +  2  log  7  +  log  11.  Hence  log  4851  can  be  found  when 
the  logarithms  of  3,  7,  and  1 1  are  known. 

*  By  the  antilogarithm  of  any  number  N  is  meant  the  number  of  which 
X  is  the  logarithm. 


XXI 


CHANGE  OF  BASE  519 


Again,  having  computed  a  system  of  logarithms  to  any  one  base 

a,  we  can  without  difficulty  deduce  therefrom  a  system  to  any  other  base 

b.  All  we  have  to  do  is  to  multiply  all  the  logarithms  of  the  former 
system  by  the  number  fx  =  l/\ogab. 

For,  if  x  =  logby,  then  y  =  Lx. 

Hence  logrty  =  loga^, 

=  ajloga&,  by  §  4. 
Hence  \ogby  =  x  =  loga?//loga&  (1). 

The  number  //,  is  often  called  the  modulus  of  the  system 
whose  base  is  b  with  respect  to  the  system  whose  base  is  a. 

Cor.  1.  If  in  the  equation  (1)  we  put  y=a,  we  get  the 
following  equation,  which  could  easily  be  deduced  more  directly 
from  the  definition  of  a  logarithm  : — 

log&«=  l/loga6, 

or  logaHog6a=l  (2). 

Cor.  2.  The  equation  y  =  bx  may  be  written 

y  =  axlos«b  or  y  =  ax!l0Bba. 

Hence  the  graph  of  the  exponential  bx  can  be  deduced  from  the 
graph  of  the  exponential  ax  by  shortening  or  lengthening  all  the  abscissce 
of  the  latter  in  the  same  ratio  1  :  logab. 

This  is  the  general  theorem  corresponding  to  a  remark  in  §  2. 

We  may  also  express  this  result  as  follows  : — 

Given  any  two  exponential  graphs  A  and  B,  then  either  A  is  the 
orthogonal  projection  of  B,  or  B  is  the  orthogonal  projection  of  A,  on  a 
plane  passing  through  the  axis  of  y. 

USE    OF    LOGARITHMS    IN   ARITHMETICAL   CALCULATIONS. 

§  10.]  We  have  seen  that,  if  we  use  the  ordinary  decimal 
notation,  the  system  of  logarithms  to  base  10  possesses  the  im- 
portant advantages  that  the  characteristic  can  be  determined  by 
inspection,  and  that  the  mantissa  is  independent  of  the  position 
of  the  decimal  point.  On  account  of  these  advantages  this 
system  is  used  in  practical  calculations  to  the  exclusion  of  all 
others. 


520 


SPECIMEN  OF  LOGARITHMIC  TABLE. 


Oil  A  P. 


No. 

0   12   3   4 

5   6   7   8   9 

Diff. 

3050 

484  2998  3141  32S3  342G  3568 

3710  3853  3995  4137  4280 

51 

4422  4564  4707  4849  4991 

5134  5276  5418  5561  5703 

52 

5845  5988  6130  6272  6414 

6557  6699  6841  6984  7126 

53 

7268  7410  7553  7695  7837 

7979  8121  8264  8406  8548 

54 

8690  8833  8975  9117  9259 

9401  9543  9686  9828  9970 

55 

485  0112  0254  0396  0539  0GS1 

0823  0965  1107  1249  1391 

56 

1533  1676  1818  1960  2102 

2244  2386  2528  2670  2812 

57 

2954  3096  3239  33S1  3523 

3665  3807  3949  4091  4233 

142 

58 

4375  4517  4659  4801  4913 

5085  5227  5369  5511  5053 

1   14 

59 

5795  5937  6079  6221  6363 

6505  6647  6788  6930  7072 

2  28 

3  43 

4  57 

60 

7214  7356  7498  7640  7782 

7924  8066  8208  8350  8491 

3061 

8633  8775  8917  9059  9201 

9343  9484  9626  9768  9910 

5   71 

62 

4860052  0194  0336  0477  0619 

0761  0903  1045  1186  1328 

6   85 

63 

1470  1612  1754  1895  2037 

2179  2321  2462  2604  2746 

7   99 

64 

2888  3029  3171  3313  3455 

3596  3738  3880  4021  4163 

8  114 

9  128 

65 

4305  4446  4588  4730  4872 

5013  5155  5297  5438  5580 

66 

5722  5863  6005  6146  62S8 

6430  6571  6713  6855  6996 

67 

7138  7279  7421  7563  7704 

7846  7987  8129  8270  8412 

68 

8554  8695  8837  8978  9120 

9261  9403  9544  9686  9827 

69 

9969  0110  0252  0393  0535 

0676  0818  0959  1101  1242 

70 

4871384  1525  1667  1808  1950 

2091  2232  2374  2515  2657 

3071 

2798  2940  3081  3222  3364 

3505  3647  3788  3929  4071 

72 

4212  4353  4495  4636  4778 

4919  5060  5202  5343  5484 

73 

5626  5767  5908  6050  6191 

6332  6473  6615  6756  6897 

74 

7039  7180  7321  7462  7604 

7745  7886  8027  8169  8310 

75 

76 

8451  8592  8734  8875  9016 
9863  0004  0146  0287  042S 

9157  9299  9440  9581  9722 

0569  0710  0852  0993  1134 

77 

488  1275  1416  1557  1698  1839 

1981  2122  2263  2404  2545 

78 

2686  2827  2968  3109  3251 

3392  3533  3674  3815  3956 

79 

4097  4238  4379  4520  4661 

4802  4943  5084  5225  5366 

80 

5507  5648  5789  5930  6071 

6212  6353  6494  6635  6776 

141 

1  14 

2  28 

3081 

6917  7058  7199  7340  7481 

7622  7763  7904  8045  8185 

82 

8326  8467  860S  8749  8890 

9031  9172  9313  9454  9594 

3   42 

83 

9735  9876  0017  0158  0299 

0440  0580  0721  0862  1003 

4   56 

84 

4891144  1285  1425  1566  1707 

1848  1989  2129  2270  2411 

5   71 

85 

2552  2692  2833  2974  3115 

3256  3396  3537  3678  3818 

6  85 

7  99 

8  113 

86 

3959  4100  4241  4381  4522 

4663  4804  4944  5085  5226 

87 

5366  5507  5648  5788  5929 

6070  6210  6351  6492  6632 

9  127 

88 

6773  6914  7054  7195  7335 

7476  7617  7757  7898  8038 

89 

8179  8320  8460  8C01  8741 

8882  9023  9163  9304  9444 

90 

9585  9725  9866  0006  0147 

0287  0428  0569  0709  0850 

3091 

4900990  1131  1271  1412  1552 

1693  1833  1973  2114  2254 

92 

2395  2535  2676  2816  2957 

3097  3238  3378  3518  3659 

93 

3799  3940  4080  4220  4361 

4501  4642  4782  4922  5063 

94 

5203  5343  5484  5624  5765 

5905  6045  6186  6326  6466 

95 

6G07  6747  6887  7027  7168 

7308  7448  7589  7729  7869 

96 

8010  8150  8290  8430  8571 

8711  8851  8991  9132  9272 

97 

9412  9552  9693  9833  9973 

0113  0253  0394  0534  0674 

98 

4910S14  0954  1094  1235  1375 

1515  1655  1795  1935  2076 

99 

2216  2356  2496  2636  2776 

2916  3057  3197  3337  3477 

3100 

3617  3757  3897  4037  4177 

4317  4457  4597  4738  4878 

xxl  USE  OF  LOGARITHMIC  TABLE  521 

la  printing  a  table  of  logarithms  to  base  10  it  is  quite  un- 
necessary, even  if  it  were  practicable,  to  print  characteristics. 
The  mantissa?  alone  are  given,  corresponding  to  a  succession  of 
five  digits,  ranging  usually  from  10000  to  99999.* 

A  glance  at  p.  520,  which  is  a  facsimile  of  a  page  of  the 
logarithmic  table  in  Chambers's  Mathematical  Tables,  will  show 
the  arrangement  of  such  a  table.  To  take  out  the  logarithm  of 
30715  from  the  table,  we  run  down  the  column  headed  "No." 
until  we  come  to  3071  ;  the  first  three  figures  of  the  mantissa 
are  487  (standing  over  the  blank  in  the  first  half  column) ;  the 
last  four  are  found  by  running  along  the  line  till  Ave  reach  the 
column  headed  5,  they  are  3505.  The  characteristic  is  seen  by 
inspection  to  be  4.     Hence  log  30715  =  4-4873505. 

To  find  the  number  corresponding  to  any  given  logarithm 
we  have  of  course  simply  to  reverse  the  process. 

To  find  the  logarithm  of  '030715  Ave  have  to  proceed  exactly 
as  before,  only  a  different  characteristic,  namely  2,  must  be  pre- 
fixed to  the  mantissa.      We  thus  find  log  -030715  =  2-4873505. 

If  we  Avish  to  find  the  logarithm  of  a  number,  say  3-083279, 
Avhere  we  have  more  digits  than  are  given  in  the  table,  then  we 
must  take  the  nearest  number  whose  logarithm  can  be  found 
by  means  of  the  table,  that  is  to  sa}r,  3-0833.  "We  thus  find 
log  3-0833  =  0-4890158f  nearly.  Greater  accuracy  can  be  at- 
tained by  using  the  column  headed  c'Diff,"  as  will  be  explained 
presently. 

Conversely,  if  a  logarithm  be  given  Avhich  is  not  exactly 
coincident  with  one  given  in  the  table,  Ave  take  the  one  in  the 
table  that  is  nearest  to  it,  and  take  the  corresponding  number  as 
an  approximation  to  the  number  required.  Greater  accuracy 
can  be  obtained  by  using  the  difference  column.  Thus  the 
number   whose    logarithm   is   1  -4872191    has   for  its   first   five 

*  For  some  purposes  an  extension  of  the  table  is  required,  and  such  ex- 
tensions are  supplied  in  various  ways,  which  need  not  be  described  here.  For 
rapidity  of  reference  in  calculations  that  require  no  great  exactness  a  short 
table  for  a  succession  of  3  digits,  ranging  from  100  to  999,  is  also  usually 
given. 

+  The  bar  over  0158  indicates  that  these  digits  follow  489,  and  not  48S. 


522  NUMBER  OF  FIGURES  REQUIRED  chap. 

significant  digits  30705  ;  but,  if  we  wish  the  best  approximation 
with  five  digits,  we  ought  to  take  30706.  Since  the  character- 
istic is  1,  the  actual  number  in  question  has  two  integral  digits. 
Hence  the  required  number  is  30'706,  the  error  being  certainly 
less  than  '0005. 

§  11.]  The  principle  which  underlies  the  application  of 
logarithms  to  arithmetical  calculation  is  the  very  simple  one 
that,  since  to  any  number  there  corresponds  one  and  only  one 
logarithm,  a  number  can  be  identified  by  means  of  its  logarithm. 

It  is  this  principle  which  settles  how  many  digits  of  the 
mantissa  of  a  logarithm  it  is  necessary  to  use  in  calculations 
which  require  a  given  degree  of  accuracy. 

Suppose,  for  example,  that  it  is  necessary  to  be  accurate 
down  to  the  fifth  significant  figure ;  and  let  us  inquire  whether 
a  table  of  logarithms  in  which  the  mantissae  are  given  to  four 
places  would  be  sufficient.  In  such  a  table  we  should  find  log 
3-0701  =0-4871,  log  3-0702  =  0-4871  ;  the  table  is  therefore 
not  sufficiently  extended  to  distinguish  numbers  to  the  degree 
of  accuracy  required.  Five  places  in  the  mantissa  would,  in  the 
present  instance,  be  sufficient  for  the  purpose;  for  log  3-0701 
=  0-48715,  log  3-0702  =  0-48716.  Towards  the  end  of  the 
table,  however,  five  places  would  scarcely  be  sufficient ;  for  log 
9-4910  =  0-97731  and  log  9-4911  =  0-97731. 

§  12.]  The  great  advantage  of  using  in  any  calculation 
logarithms  instead  of  the  actual  numbers  is  that  we  can,  in 
accordance  with  the  rules  of  §  4,  replace  every  multiplication  by 
an  addition,  every  division  by  a  subtraction,  and  every  operation 
of  raising  to  a  power  or  extracting  a  root  by  a  multiplication  or 
division. 

The  following  examples  will  illustrate  some  of  the  leading 
cases.     We  suppose  that  the  student  has  a  table  of  the  loga- 
rithms of  all  numbers  from  10000  to  100000,  giving  mantissa? 
to  seven  places. 
Example  1. 
Calculate  the  value  of  1-6843  x  -00132 -J- '3692. 

If  A  =  1-6843  x  -00132H--3692, 
log  A  =  log  1  -6843  +  log  -00132  -  log  -3692, 


XXI 


EXAMPLES  523 


log  1-6843   =    -2264194 
log -00132  =  3-1205739 


3*3469933 
log -3692   =1-5672617 
logA  =  3-7797316. 
Hence  A=    -0060219. 

Observe  that  the  negative  characteristics  must  be  dealt  with  according  to 
algebraic  rules. 

Example  2. 

To  extract  the  cube  root  of  -016843. 

Let  A  =  (-016843)1/3,  then 

log  A= |  log  -016843, 

=  i(2 -2264194), 

=  4(3  + 1-2264194), 

=  1-4088065. 

A=    -25633. 
Example  3. 

Calculate  the  value  of  A  =  (368)"'3/(439)5;9. 
Log  A =1  log  368 -flog  439. 

I  log  368  =  |(2 -5658478)  =  5-9869782 
$  log  439  =  f  (2  -6424645)  =  1  "4680358 
log  A  =  4-5189424 
A=     33033. 
Example  4. 

Find  how  many  digits  there  are  in  A  =  (l-01)10000. 
log  A=  10000  log  1-01, 

=  10000  x  -0043214, 
=  43-214. 
Hence  the  number  of  digits  in  A  is  44. 

Example  5. 

To  solve  the  exponential  equation  1-2*=1-1  by  means  of  logarithms. 
AVe  have  log  1  2*  =  log  1  •  1 . 

Therefore  a?logl'2=logl,L 

„  _  log  1-1  _  -0413927 

Ce  ""log  l-2~ -0791812 " 

Hence  log.r  =  l_og  -0413927 -log  -0791812, 

=  1-7183059. 
Therefore  x  —    -52276. 

Remark.—  It  is  obvious  that  we  can  solve  any  such  equation  as  a*2-*"**  =  &, 
where;,  q,  a,  b  are  all  given.     For,  taking  logarithms  of  both  sides,  we  have 

(x2  -px  +  q)  log  a  =  log  b. 
We  can  now  obtain  the  value  of  a:  by  solving  a  quadratic  equation. 


524  INTERPOLATION  BY  FIRST  DIFFERENCES  chap. 


INTERPOLATION  BY  FIRST  DIFFERENCES. 

§  13.]  The  method  by  which  it  is  usual  to  find  (or  "interpo- 
late ")  the  value  of  the  logarithm  of  a  number  which  does  not 
happen  to  occur  in  the  table  is  one  which  is  applicable  to  any 
function  whose  values  have  been  tabulated  for  a  series  of  equi- 
different  values  of  its  independent  variable  (or  "argument"). 

The  general  subject  of  interpolation  belongs  to  the  calculus 
of  finite  differences,  but  the  special  case  where  first  differences 
alone  are  used  can  be  explained  in  an  elementary  way  by  means 
of  graphical  considerations. 

We  have  already  seen  that  the  increment  of  an  integral 
function  of  x  of  the  1st  degree,  y  =  A.?;  +  B  say,  is  proportional 
to  the  increment  of  its  argument ;  or,  what  comes  to  the  same 
thing,  if  we  give  to  the  argument  x  a  series  of  ecpiidifferent 
values,  a,  a  +  h,  a  +  2h,  a  +  3/j,  &c,  the  function  y  will  assume  a 
series  of  equidifferent  values  Aa  +  B,  Aa  +  B  +  Ah,  Aa  +  B  +  2  Ah, 
Aa  +  B  +  3Ah,  &c. 

If,  therefore,  we  were  to  tabulate  the  values  of  Ax  +  B  for  a 
series  of  equidifferent  values  of  x,  the  differences  between  suc- 
cessive values  of  y  ("  tabular  differences ")  would  be  constant,  no 
matter  to  how  many  places  we  calculated  y. 

Conversely,  a  function  of  x  which  has  this  property,  that  the 
differences  between  the  successive  values  of  y  corresponding  to 
equidifferent  values  of  x  are  absolutely  constant,  must  be  an  in- 
tegral function  of  x  of  the  1st  degree. 

If,  however,  we  take  the  difference,  h,  of  the  argument  small 
enough,  and  do  not  insist  on  accuracy  in  the  value  of  y  beyond 
a  certain  significant  figure,  then,  for  a  limited  extent  of  the  table 
of  any  function,  it  will  be  found  that  the  tabular  differences  are 
constant. 

Bef erring,  for  example,  to  p.  520,  it  will  be  seen  that  the 
difference  of  two  consecutive  logarithms  is  constant,  and  equal 
to  -0000141,  from  log  30660  up  to  log  30S99,  or  that  there  is 
merely  an  accidental  difference  of  a  unit  in  the  last  place ;  that 
is  to  say,  the  difference  remains  constant  for  about  240  entries. 


XXI 


LIMITS  OF  THE  METHOD 


525 


A  similar  phenomenon  will  be  seen  in  the  following  extract 
from  Barlow's  Tables,  provided  we  do  not  go  beyond  the  7th 


significant  figure  :- 


Number. 

Cube  Root. 

Diff. 

2301 

13-2019740 

19122 

2302 

13-2038862 

19117 

2303 

13-2057979 

19111 

2304 

13-2077090 

19105 

2305 

13-2096195 

Let  us  now  look  at  the  matter  graphically.  Let  ACSDQB 
be  a  portion  of  the  graph  of  a  function  y  =  /(•>') ;  and  let  us 
suppose  that  up  to  the  nth  significant  figure  the  differences  of  y 
are  constant  for  equidifferent 
values  of  x,  lying  between 
OE  and  OH.  This  means 
that  in  calculating  (up  to  the 
nth  significant  figure)  values 
of  y  corresponding  to  values 
of  x  between  OE  and  OH  we 
may  replace  the  graph  by  the 
straight  line  AB.  Thus,  for 
example,  if  x  -  OM,  then 
/(OM)  =  MQ  ;  and  PM  is  the 
value  calculated  by  means  of  the  straight  line  AB.  Our  state- 
ment then  is  that  PM  -  QM,  that  is  PQ,  is  less  than  a  unit  in 
the  n  significant  place. 

If  this  be  so,  then,  a  fortiori,  it  will  be  so  if  Ave  replace  a 
portion  of  the  graph,  say  CD,  lying  between  A  and  B  by  a 
straight  line  joining  C  and  D. 

In  other  words,  if  up  to  the  nth  place  the  increment  of  the  func- 
tion for  eqiudifferent  values  of  x  be  constant,  between  certain  limits, 
then,  to  that  degree  of  accuracy  at  least,  the  increment  of  the  function 
will  be  proportional  to  the  increment  of  the  argument  fcrr  all  values 
within  those  limits. 

§  1 4.]  Let  us  now  state  the  conclusion  of  last  article  under 


Fig.  2. 


526  RULE  OF  PROPORTIONAL  PARTS  chap. 

an  analytical  form,  all  the  limitations  before  mentioned  as  to 
constancy  of  tabular  (or  first)  difference  being  supposed  fulfilled. 
Let  h  be  the  difference  of  the  arguments  as  they  are  entered 
in  the  table,  D  the  tabular  difference  f(a  +  h)  -/(«),  a  +  h'  a  value 
of  the  argument,  which  does  not  occur  in  the  table,  but  which 
lies  between  the  values  a  and  a  +  h,  which  do  occur,  so  that  h'<h. 
Then,  by  last  paragraph, 

f(a  +  h')  -f(a)  _  (a  +  h')  -  a 
f(a  +  h)  -f(a)      (a  +  h)  -  a 

Hence  f{a  +  h')-f(a)     K 

D  h 

Since  in  (1)  f(a),  D,  h  are  all  known,  it  gives  us  a  relation 
between  h'  and  f(a  +  h').  When,  therefore,  one  or  other  of  these 
is  given,  we  can  calculate  the  other.     We  have  in  fact 

f(a  +  h')=f(a)  +  ^J)  (2), 

and  a  +  h^a+f(a  +  h^-f(a)h  (3). 

From  (2)  we  find  a  value  of  the  function  corresponding  to  a 
given  intermediate  value  of  the  argument.  From  (3)  we  find  an 
intermediate  value  of  the  argument  corresponding  to  a  given 
intermediate  value  of  the  function. 

The  equations  (2)  and  (3)  are  sometimes  called  the  Rule  of 
Proportional  Parts. 

Example  1. 

To  find  by  means  of  first  differences  the  value  of  ^/(2303,45)  as  accurately 

as  Barlow's  Table  will  allow. 

By  the  rule  of  proportional  parts,  we  have 

^'(2303  -45)  =  ^(2303  -00)  +  T<&(  -00191), 
=  13-20580+ -00086, 
=  13-20666, 
which  will  be  found  correct  down  to  the  last  figure. 

The  only  labour  in  the  above  calculation  consists  in  working 
out  the  fraction  45/100  of  the  tabular  difference.     In  tables  of 


XXI 


EXAMPLES  527 


logarithms  even  this  labour  is  spared  the  calculator  ;  for  under 
each  difference  there  is  a  small  table  of  proportional  parts,  giving 
the  values  of  1/10,  2/10,  3/10,  4/10,  5/10,  6/10,  7/10,  8/10, 
9/10  of  the  difference  in  question  (see  the  last  column  on  p.  520). 
It  will  be  observed  that,  if  we  strike  the  last  figure  off  each  of 
the  proportional  parts  (increasing  the  last  of  those  left  if  the 
one  removed  exceeds  5),  we  have  a  table  of  the  various  hun- 
dredths, and  so  on.  Hence  Ave  can  use  the  table  twice  over  (in 
some  cases  it  might  be  oftener),  as  in  the  following  example : — 

Example  2. 
To  find  log  30 -81 345. 

We  may  arrange  the  corresponding  contributions  as  follows ' — 

30-81300     1-4887340 

40  56 

5  7 


log  30 -81345  =  1-4887403 
Example  3. 

To  find  the  number  whose  logarithm  is  1-4871763. 

1-4871763 

1-4871637     -3070200 
96 

85  60 

11  8 


antilog  1  -4871763  =  -3070268 

Here  we  set  down  under  the  given  logarithm  the  next  lowest  in  the  table, 
and  opposite  to  it  the  corresponding  number  -30702. 

Next,  we  write  down  -0000096,  the  difference  of  these  two  logarithms,  and 
look  for  the  greatest  number  in  the  table  of  proportional  parts  which  does  not 
exceed  96— this  is  85.  We  set  down  85,  and  opposite  to  it  the  corresponding 
figure  6. 

Lastly,  we  subtract  85  from  96,  the  result  being  -0000011.  We  then 
imagine  a  figure  struck  off  every  number  in  the  table  of  proportional  parts, 
look  for  the  remaining  one  which  stands  nearest  to  11,  and  set  down  the 
figure,  namely  8,  corresponding  to  it,  as  the  last  digit  of  the  number  we  are 
seeking. 

Exercises  XLIII. 
(1.)  Find  the  characteristics  of  log1036983,  logi058,  logi05-3,  log10  '00068 
(2.)  Find  the  characteristics  of  log51067,  log5-0138,  log^,  logvAjl/8 
(3.)  Find  log28  ^2. 
(4.)  Calculate  log236'432  to  two  places  of  decimals. 


528  EXERCISES  XLIII 


CHAP. 


Calculate  out  the  values  of  tlio  following  as  accurately  as  your  tables  will 
allow: — 

(5.)  4163x7-835.  (6.)  *3068  x -0015^-0579. 

(7.)  (5-0063745)5.  (8.)    ^/(5 -0063745). 

(9.)  (-01369)12.  (10.)  (-001369)*. 

(11.)    {15(*318)fyl6}^.  (12.)   {(1-035)7-  1}/ {1-035  -  1}. 

(13.)  The  population  of  a  country  increases  each  year  by  *13  %  0I"  its 
amount  at  the  beginning  of  the  year.  By  how  much  °/0  will  it  have  increased 
altogether  after  250  years  ? 

(14.)  If  the  number  of  births  and  deaths  per  annum  be  3*5  and  1*2  °/0 
respectively  of  the  population  at  the  beginning  of  each  year,  after  how  many 
years  will  the  population  be  trebled  ? 

(15.)  Calculate  the  value  of  ^(326-8+553-6). 

(16.)  Calculate  the  value  of  1  +  c  +  c-  + .  .  .  +e19,  where  e= 2 71828. 

(17.)  Find  a  mean  proportional  between  3*17934  and  3*987636. 

(18.)  Insert  three  mean  proportionals  between  65"342  and  88*63. 

(19.)  The  1st  and  13th  terms  of  a  geometric  progression  are  3  and  65 
respectively  :  find  the  common  ratio. 

(20.)  The  4th  and  7th  terms  of  a  geometric  progression  are  31  and  52 
respectively  :  find  the  5  th  term. 

(21.)  How  many  terms  of  the  series  s  +  p+p+  ■   •   •   must  be  taken  in 

order  that  its  sum  may  differ  from  unity  by  less  than  a  millionth  ? 

(22.)  Given  log105=  *69897,  find  the  number  of  digits  in  (\/5)9a. 

(23.)  Given  log  2673  =  3*427,  and  log 3267  =  3*51415,  find  log  11. 

(24.)  Find  the  first  four  significant  figures  and  the  number  of  digits  in 
1.2.3.4.  .  .  20. 

(25.)  How  many  terms  of  31,  3-,  33,  .  .  .  must  I  take  in  order  that  the 
product  may  just  exceed  100000  ? 

(26.)  Given  logx36  =  1*3678,  find  a:. 

(27.)  Given  loga:6£  =  2,  find  x. 

Solve  the  following  equations  : — 

(28.)  21*  =  20.  (29.)  2*  15*= 5.  (30.)  2*2  =  5  x  2*. 

(31.)  6*  =  5y,     7*=3y.  (32.)  3*-3-*=5. 

(33.)  23*+2»=5,     42*=22<'+;!.  (34.)  &*&*-* ->;»-\ip-xm 

(35. )  (a  +  b)^(a4  -  2a-u-  +  b*)*-1  =  {a-  bf*. 
(36.)  xx+y  =  yia,     yx+«  =  xa. 

(37.)  Find  by  means  of  a  table  of  common  logarithms  loge16.345,  where 
«  =  2*71828. 

(38.)  Show  that  x—a  ;  and  that  x = a 

(39.)  Show  that 

log„(log„N)  _  h^(k>gj^ 

V(l0ga"i)  V(log*'0     :  V(l<>go&)  \/(l0g»rt) 

(40.)  Show  that  the  logarithm  of  any  number  to  base  an  is  a  mean  pro- 

g 
portional  between  its  logarithms  to  the  bases  a  and  a"  . 


xxr  HISTORICAL  NOTE  529 

(41.)  If  P,  Q,  R  be  the  pth,  qth,  rth  terms  of  a  geometric  progression, 
show  that  2(y  -  r)  log  P  =  0. 

(42.)  If  ABC  be  in  harmonic  progression,  show  that  log(A  +  C) 
+  log(A  +  C-2B)  =  2log(A-C). 

(43.)  If  a,  b,  c  be  in  G.P.,  show  that  S{log0(6/c)}-1=-3{log4(c/a)}-1. 

(44.)  If  a,  b,  c  be  in  G.P.,  and  logc«,  log6c,  logab  in  A. P.,  then  the 
common  difference  of  the  latter  is  3/2. 

(45.)  If  a2  +  b2  =  c-,  then  log6+c«  +  logc_&a  =  2iog6+crelogc_6«. 

/  a  /»  \  re  x(v +a  —  x)    y(z + x  -  y)    z(x  +  y  -  z)    . ,      •     „      „  .      „  . 

(46.)  If-5^. =^-r -=-■     ,    -,  then  y*0'=f?!x*=x*y*. 

log  a;  logy  logs      '  J  a 

(47.)  If  :c2  =  \ogxnXi,  xz=\ogXlx2)  K4=logx2a!s,  .  .  .,  av,=logrB_2a3„-i,  x1  = 

l°S*n-\x»>   then  XlX-'  ■  ■  'T»  =  1- 

Historical  Note. — The  honour  of  devising  the  use  of  logarithms  as  a  means  of 
abbreviating  arithmetical  calculations,  and  of  publishing  the  first  logarithmic 
table,  belongs  to  John  Napier  (1550-1617)  of  Merchiston  (in  Napier's  day  near, 
iu  our  day  in,  Edinburgh).  This  invention  was  not  the  result  of  a  casual  inspira- 
tion, for  we  learn  from  Napier's  Rabdolorjla  (1617),  in  which  he  describes  three 
other  methods  for  facilitating  arithmetical  calculations,  among  them  his  calculat- 
ing rods,  which,  uuder  the  name  of  "  Napier's  Bones,"  were  for  long  nearly  as 
famous  as  his  logarithms,  that  he  had  devoted  a  great  part  of  his  life  to  the  con- 
sideration of  methods  for  increasing  the  power  and  diminishing  the  labour  of 
arithmetical  calculation.  Napier  published  his  invention  in  a  treatise  entitled 
"Mirifici  Logarithmorum  Cauonis  Descriptio,  ejusque  usus,  in  utraque  Trigo- 
nometria  ut  etiam  in  omni  Logistica  Mathematica,  Amplissimi,  facillimi,  et 
expeditissimi  explicatio.  Authore  ac  Inventore  Ioanne  Nepero5  Barone  Merchis- 
tonii,  &c,  Scoto,  Edinburgi  (1614)."  In  this  work  he  explains  the  use  of 
logarithms  ;  and  gives  a  table  of  logarithmic  sines  to  7  figures  for  every  minute 
of  the  quadrant.  In  the  Canon  Mirificus  the  base  used  was  neither  10  nor  what 
is  now  called  Napier's  base  (see  the  chapter  on  logarithmic  series  in  the  second 
part  of  this  work).  Napier  himself  appears  to  have  been  aware  of  the  advantages 
of  10  as  a  base,  and  to  have  projected  the  calculation  of  tables  on  the  improved 
plan  ;  but  his  infirm  health  prevented  him  from  carrying  out  this  idea  ;  and  his 
death  three  years  after  the  publication  of  the  Canon  Mirificus  prevented  him  from 
even  publishing  a  description  of  his  methods  for  calculating  logarithms.  This 
work,  entitled  Mirifici  Logarithmorum  Canonis  Constructio,  &c. ,  was  edited  by 
one  of  Napier's  sons,  assisted  by  Henry  Briggs. 

To  Henry  Briggs  (1556-1630),  Professor  of  Geometry  at  Gresham  College,  and 
afterwards  Savilian  Professor  at  Oxford,  belongs  the  place  of  honour  next  to 
Napier  in  the  development  of  logarithms.  He  recognised  at  once  the  merit  and 
seized  the  spirit  of  Napier's  invention.  The  idea  of  the  superior  advantages 
of  a  decimal  base  occurred  to  him  independently  ;  and  he  visited  Napier  in 
Scotland  in  order  to  consult  with  him  regarding  a  scheme  for  the  calculation 
of  a  logarithmic  table  of  ordinary  numbers  on  the  improved  plan.  Finding 
Napier  in  possession  of  the  same  idea  in  a  slightly  better  form,  he  adopted  his 
suggestions,  and  the  result  of  the  visit  was  that  Briggs  undertook  the  work  which 
Napier's  declining  health  had  interrupted.  Briggs  published  the  first  thousand 
of  his  logarithms  in  1617  ;  and,  in  his  Arithmetica  Logarithmica,  gave  to  14 
places  of  decimals  the  logarithms  of  all  integers  from  1  to  20,000,  and  from 
90,000  to  100,000.  In  the  preface  to  the  last-mentioned  work  he  explains  the 
methods  used  for  calculating  the  logarithms  themselves,  and  the  rules  for  using 
them  in  arithmetical  calculation. 

VOL.  I  2  M 


530  HISTOKICAL  NOTE  chap,  xxi 

While  Briggs  was  engaged  in  filling  up  the  gap  left  in  his  table,  the  work  of 
calculating  logarithms  was  taken  up  in  Holland  by  Adrian  Vlacq,  a  bookseller  of 
Gouda.  He  calculated  the  70,000  logarithms  which  were  wanting  in  Briggs' 
Table  ;  and  published,  in  1628,  a  table  containing  the  logarithms  to  10  places  of 
decimals  of  all  numbers  from  1  to  100,000.  The  work  of  Briggs  and  Vlacq  has 
been  the  basis  of  all  the  tables  published  since  their  day  (with  the  exception  of 
the  tables  of  Sang,  1871) ;  so  that  it  forms  for  its  authors  a  monument  both 
lasting  and  great. 

In  order  fully  to  appreciate  the  brilliancy  of  Napier's  invention  and  the  merit 
of  the  work  of  Briggs  and  Vlacq,  the  reader  must  bear  in  mind  that  even  the 
exponential  notation  and  the  idea  of  an  exponential  function,  not  to  speak  of  the 
inverse  exponential  function,  did  not  form  a  part  of  the  stock-in-trade  of  mathe- 
maticians till  long  afterwards.  The  fundamental  idea  of  the  correspondence  of 
two  series  of  numbers,  one  in  arithmetic,  the  other  in  geometric  progression,  which 
is  so  easily  represented  by  means  of  indices,  was  explained  by  Napier  through 
the  conception  of  two  points  moving  on  sejjarate  straight  lines,  the  one  with 
uniform,  the  other  with  accelerated  velocity.  If  the  reader,  with  all  his  acquired 
modern  knowledge  of  the  results  to  be  arrived  at,  will  attempt  to  obtain  for  him- 
self in  this  way  a  demonstration  of  the  fundamental  rules  of  logarithmic  calcula- 
tion, he  will  rise  from  the  exercise  with  an  adequate  conception  of  the  penetrating 
genius  of  the  inventor  of  logarithms. 

For  the  full  details  of  this  interesting  part  of  mathematical  history,  and 
in  particular  for  a  statement  of  the  claims  of  Jost  Biirgi,  a  Swiss  contemporary 
of  Napier's,  to  credit  as  an  independent  inventor  of  logarithms,  we  refer  the 
student  to  the  admirable  articles  "Logarithms"  and  "Napier,"  by  J.  W.  L.  Glaisher, 
in  the  Encyclopaedia  Britannica  (9th  ed.).  An  English  translation  of  the 
Constnictio,  with  valuable  bibliographical  notes,  has  been  published  by  Mr.  W. 
R.  Macdonald,  F.F.A.  (Edinb.  1889). 


CHAPTEE    XXII. 

Theory  of  Interest  and  Annuities  Certain. 

§  1.]  Since  the  mathematical  theory  of  interest  and  annuities 
affords  the  best  illustration  of  the  principles  we  have  been  dis- 
cussing in  the  last  two  chapters,  we  devote  the  present  chapter 
to  a  few  of  the  more  elementary  propositions  of  this  important 
practical  subject.  What  we  shall  give  will  be  sufficient  to  enable 
the  reader  to  form  a  general  idea  of  the  principles  involved. 
Those  whose  business  requires  a  detailed  knowledge  of  the 
matter  must  consult  special  text-books,  such  as  the  Text-Book  of 
the  Institute  of  Actuaries,  Part  I.,  by  Sutton.* 

SIMPLE    AND    COMPOUND    INTEREST. 

§  2.]  When  a  sum  of  money  is  lent  for  a  time,  the  borrower 
pays  to  the  lender  a  certain  sum  for  the  use  of  it.  The  sum 
lent  is  spoken  of  as  the  capital  or  principal ;  the  payment  for 
the  privilege  of  using  it  as  interest.  There  are  various  ways  of 
arranging  such  a  transaction ;  one  of  the  commonest  is  that  the 
borrower  repays  after  a  certain  time  the  capital  lent,  and  pays 
also  at  regular  intervals  during  the  time  a  stated  sum  by  way  of 
interest.  This  is  called  paying  simple  interest  on  the  borrowed 
capital.  The  amount  to  be  paid  by  way  of  interest  is  usually 
stated  as  so  much  per  cent  per  annum.  Thus  5  per  cent  (5  %) 
per  annum  means  £5  to  be  paid  on  every  £100  of  capital,  for 


*  Full  references  to  the  various  sources  of  information  will  be  found  in 
the  article  "Annuities"  (by  Sprague),  Encyclopaedia  Britamica,  9th  edition, 
vol.  ii. 


532  AMOUNT PRESENT  VALUE DISCOUNT  chap. 

every  year  that  the  capital  is  lent.  In  the  case  of  simple 
interest,  the  interest  payable  is  sometimes  reckoned  strictly  in 
proportion  to  the  time ;  that  is  to  say,  allowance  is  made  not 
only  for  whole  years  or  other  periods,  but  also  for  fractions 
of  a  period.  Sometimes  interest  is  allowed  only  for  integral 
multiples  of  a  period  mutually  agreed  on.  We  shall  suppose 
that  the  former  is  the  understanding.  If  then  r  denote  the 
interest  on  £1  for  one  year,  that  is  to  say,  one-hundredth  of 
the  named  rate  per  cent,  n  the  time  reckoned  in  years  and 
fractions  of  a  year,  P  the  principal,  I  the  whole  interest  paid,  A 
the  amount,  that  is,  the  sum  of  the  principal  and  interest,  both 
reckoned  in  pounds,  we  have 

I  =  nrP         (1);  A  =  I  +  P  =  P(1  +  nr)         (2). 

These  formulae  enable  us  to  solve  all  the  ordinary  problems  of 
simple  interest. 

If  any  three  of  the  four  I,  n,  r,  P,  or  of  the  four  A,  n,  r,  P, 
be  given,  (1)  or  (2)  enables  us  to  find  the  fourth. 

Of  the  various  problems  that  thus  arise,  that  of  finding  P 
when  A,  n,  r  are  given  is  the  most  interesting.  We  suppose 
that  a  sum  of  money  A  is  due  n  years  hence,  and  it  is  required 
to  find  what  sum  paid  down  at  once  would  be  an  equitable 
equivalent  for  this  debt.  If  simple  interest  is  allowed,  the 
answer  is,  such  a  sum  P  as  would  at  simple  interest  amount  in  n 
years  to  A.  In  this  case  P  =  A/(l  +  nr)  is  called  the  present 
value  of  A,  and  the  difference  A-P  =  A{1-  1/(1  +  nr)} 
=  A?w/(1  +  nr)  is  called  the  discount.  Discount  is  therefore  the 
deduction  allowed  for  immediate  payment  of  a  sum  due  at  some 
future  time.  The  discount  is  less  than  the  simple  interest 
(namely  Anr)  on  the  sum  for  the  period  in  question.  When  n 
is  not  large,  this  difference  is  slight. 

Example. 

Find  the  difference  between  the  interest  and  the  discount  on  £1525 
due  nine  months  hence,  reckoning  simple  interest  at  3£  %•  The  difference 
in  question  is  given  by 

Anr  -  An?i(l  +  nr)  =  An-r-/(l  +nr). 


XXH  COMPOUND  INTEREST  533 

In  the  present  case  A *=  1525,     n  =  9/12  =  3/4,     r= 3-5/100= -035.     Hence 
Difference  =  1525  x  ( -02625)2-f-(l  -02625), 
=  £1  :0:5£. 

§  3.]  In  last  paragraph  we  supposed  that  the  borrower  paid 
up  the  interest  at  the  end  of  each  period  as  it  became  due.  In 
many  cases  that  occur  in  practice  this  is  not  done ;  but,  instead, 
the  borrower  pays  at  the  end  of  the  whole-  time  for  which  the 
money  was  lent  a  single  sum  to  cover  both  principal  and 
interest.  In  this  case,  since  the  lender  loses  for  a  time  the  use 
of  the  sums  accruing  as  interest,  it  is  clearly  equitable  that  the 
borrower  should  pay  interest  on  the  interest ;  in  other  words, 
that  the  interest  should  be  added  to  the  principal  as  it  becomes 
due.  In  this  case  the  principal  or  interest-bearing  capital 
periodically  increases,  and  the  borrower  is  said  to  pay  compound 
interest.  It  is  important  to  attend  carefully  here  to  the  under- 
standing as  to  the  period  at  which  the  interest  is  supposed  to 
become  due,  or,  as  it  is  put  technically,  to  be  convertible  (into 
principal) ;  for  it  is  clear  that  £100  will  mount  up  more  rapidly 
at  5  %  compound  interest  convertible  half-yearly  than  it  will  at 
5  %  compound  interest  payable  annually.  In  one  year,  for  in- 
stance, the  amount  on  the  latter  hypothesis  will  be  £105,  on  the 
former  £105  plus  the  interest  on  £2  :  10s.  for  a  half-year,  that 
is,  £105  :  1  :3. 

In  what  follows  we  shall  suppose  that  no  interest  is  allowed 
for  fractions  of  the  interval  (conversion -period)  between  the 
terms  at  which  the  interest  is  convertible,  and  we  shall  take  the 
conversion-period  as  unit  of  time.  Let  P  denote  the  principal,  A 
the  accumulated  value  of  P,  that  is,  the  principal  together  with 
the  compound  interest,  in  n  periods  ;  r  the  interest  on  £1  for 
one  period  ;   1  +  r  =  R  the  amount  of  £1  at  the  end  of  one  period. 

At  the  end  of  the  first  period  P  will  have  accumulated  to 
P  +  Pr,  that  is,  to  PR.  The  interest-bearing  capital  or  principal 
during  the  second  period  is  PR ;  and  this  at  the  end  of  the 
second  period  will  have  accumulated  to  PR  +  PRr,  that  is,  to 
PR2.  The  principal  during  the  third  period  is  PR2,  and  the 
amount  at  the  end  of  that  period  PR3,  and  so  on.     In  short,  the 


534  EXAMPLES  CHA1\ 

amount  increases  in  a  geometrical  progression  whose  common  ratio  is 
R ;  and  at  the  end  of  n  periods  we  shall  liave 

A  =  PR»  (1). 

By  means  of  this  equation  we  can  solve  all  the  ordinary 
problems  of  compound  interest ;  for  it  enables  us,  when  any  three 
of  the  four  quantities  A,  P,  R,  n  are  given,  to  determine  the 
fourth.  In  most  cases  the  calculation  is  greatly  facilitated  by 
the  use  of  logarithms.      See  the  examples  worked  below. 

Cor.  I.  If  I  denote  the  whole  compound  interest  on  P  during  the 
n  periods,  we  have 

I=A-P  =  P(R"-1)  (2). 

Cor.  2.  If  P  denote  the  present  value  of  a  sum  A  due  n  periods 

hence,  compound  interest  being  allowed,  then,  since  P  must  in  n  periods 

amount  to  A,  we  have 

A  =  PR", 

so  that  P  =  A/RJl  (3). 

The  discount  on  the  present  understanding  is  therefore 

A(l  -  1/R'1)  (4). 

Example  1. 

Find  the  amount  in  two  years  of  £2350  :  5  :  9  at  Z\  %  compound  interest, 
convertible  quarterly. 

Here  P  =  2350-2875,     n  =  S,    r  =  3-5/400  =-00875,     R  =  l-00875. 
log  A  =  log  P  +  n  log  R, 
log  P  =  3-3711210 
?ilogR*  =    -0302684 


3-4013894 
A  =  £2519-936  =  £2519  :  18  :  8. 
Example  2. 

How  long  will  it  take  £186  :  14  :  9  to  amount  to  £216  :  9  :  7  at  6  %  com- 
pound interest,  convertible  half-yearly. 

*  When  n  is  very  large,  the  seven  figures  given  in  ordinary  tables  hardly 
afford  the  necessary  accuracy  in  the  product  n  log  R.  To  remedy  this  defect, 
supplementary  tables  are  usually  given,  which  enable  the  computer  to  find 
very  readily  to  9  or  10  places  the  logarithms  of  numbers  (such  as  R)  which 
differ  little  from  unity. 


xxn  NOMINAL  AND  EFFECTIVE  RATE  .535 

Here  P= 186 -7375,     A  =  216"4792,     R=1'03. 
»=(logA-logP)/logR 

•0641847 


=  5-00 
•0128372 


Hence  the  required  time  is  five  half-years,  that  is,  1\  years. 

Example  3. 

To  find  the  present  value  of  £1000  due  50  years  hence,  allowing  compound 
interest  at  4  %>  convertible  half-yearly. 

HereA  =  1000,     ?i  =  100,     R  =  l-02.     We  have  P=A/R». 
log  P  =  log  1000  - 100  log  1-02, 
=  3  -  100  x -0086002, 
=  2-1399800. 
P  =  £138-032  =  £138  :  0  :  8. 

§  4.]  In  reckoning  compound  interest  it  is  very  usual  in 
practice  to  reckon  by  the  year  instead  of  by  the  conversion- 
period,  as  we  have  done  above,  the  reason  being  that  different 
rates  of  interest  are  thus  more  readily  comparable.  It  must  be 
noticed,  however,  that  when  this  is  done  the  rate  of  interest  to 
be  used  must  not  be  the  nominal  rate  at  which  the  interest  due 
at  each  period  is  reckoned,  but  such  a  rate  (commonly  called  the 
effective  rate)  as  would,  if  convertible  annually,  be  equivalent  to 
the  nominal  rate  convertible  as  given. 

Let  rn  denote  the  effective  rate  of  interest  per  pound  which 
is  equivalent  to  the  nominal  rate  r  convertible  every  l/?ith  part 
of  a  year ;  then,  since  the  amount  of  £  1  in  one  year  at  the  two 
rates  must  be  the  same,  we  have 

(l+r)n=l+rn, 
that  is,  rn  =  (\+r)'l-l  (1), 

and  r  =  (l+rn)1/B-l  (2). 

The  equations  (1)  and  (2)  enable  us  to  deduce  the  effective  rate 
from  the  nominal  rate,  and  vice  versa. 

Example. 

The  nominal  rate  of  interest  is  5  %>  convertible  monthly,  to  find  the 
effective  rate. 

Here  r=    -05/12=  -004166. 

Hence  ?-12=(l-004166)12- 1, 

=  1-05114-1. 
r12=     -05114. 
Hence  the  effective  rate  is  5  "11 4  °/0. 


536  ANNUITIES  TERMINABLE  OE  PERPETUAL  CHAP. 


ANNUITIES  CERTAIN. 


§  5.]  When  a  person  has  the  right  to  receive  every  year  a 
certain  sum  of  money,  say  £A,  he  is  said  to  possess  an  annuity 
of  £A.  This  right  may  continue  for  a  fixed  number  of  years  and 
then  lapse,  or  it  may  be  vested  in  the  individual  and  his  heirs 
for  ever ;  in  the  former  case  the  annuity  is  said  to  be  terminable, 
in  the  latter  perpetual.  A  good  example  of  a  terminable  annuity 
is  the  not  uncommon  arrangement  in  lending  money  where  B 
lends  C  a  certain  sum,  and  C  repays  by  a  certain  number  of 
equal  annual  instalments,  which  are  so  adjusted  as  to  cover  both 
principal  and  interest.  The  simplest  example  of  a  perpetual 
annuity  is  the  case  of  a  freehold  estate  which  brings  its  owner  a 
fixed  income  of  £A  per  annum. 

Although  in  valuing  annuities  it  is  usual  to  speak  of  the 
whole  sum  which  is  paid  yearly,  yet,  as  a  matter  of  practice,  the 
payment  may  be  by  half-yearly,  quarterly,  &c.  instalments ;  and 
this  must  be  attended  to  in  annuity  calculations.  Just  as  in 
compound  interest,  the  simplest  plan  is  to  take  the  interval 
between  two  consecutive  payments,  or  the  conversion-period,  as 
the  unit  of  time,  and  adjust  the  rate  of  interest  accordingly. 

In  many  cases  an  annuity  lasts  only  during  the  life  of  a  cer- 
tain named  individual,  called  the  nominee,  who  may  or  may  not 
be  the  annuitant.  In  this  and  in  similar  cases  an  estimate  of 
the  probable  duration  of  human  life  enters  into  the  calculations, 
and  the  annuity  is  said  to  be  contingent.  In  the  second  part  of 
this  work  we  shall  discuss  this  kind  of  annuities.  For  the 
present  we  confine  ourselves  to  cases  where  the  annual  payment 
is  certainly  due  either  for  a  definite  succession  of  years  or  in 
perpetuity. 

§  6.]  One  very  commonly  occurring  annuity  problem  is  to 
find  the  accumulated  value  of  a  FORBORNE  annuity.  An  annuitant 
B,  who  had  the  right  to  receive  n  successive  payments  at  n  suc- 
cessive equidistant  terms,  has  for  some  reason  or  other  not 
received  these  payments.  The  question  is,  What  sum  should  he 
receive  in  compensation  ? 


XXII 


ACCUMULATION  OF  FORBORNE  ANNUITY  537 


To  make  the  question  general,  let  us  suppose  that  the  last  of 
the  n  instalments  was  due  m  periods  ago. 

It  is  clear  that  the  whole  accumulated  value  of  the  annuity 
is  the  sum  of  the  accumulated  values  of  the  n  instalments, 
and  that  compound  interest  must  in  equity  be  allowed  on  each 
instalment. 

Now  the  nth  instalment,  due  for  m  periods,  amounts  to  AR"!, 
the  n  -  1th  to  AE"l+1,  the  n  -  2th  to  ARm+2;  and  so  on.  Hence, 
if  V  denote  the  whole  accumulated  value,  we  have 

V  =  ARm  +  ARw+1  +  .  .  .  +ARm+»-1  (1). 

Summing  the  geometric  series,  we  have 

V  =  AR™(Rn-l)/(R-l)  (2). 

Cor.  If  the  last  instalment  be  only  just  due,  m  =  0,  and  the 
accumulated  value  of  the  forborne  annuity  is  given  by 

V  =  A(R»-1)/(R-1)  (3). 
Example. 

A  farmer's  rent  is  £156  per  annum,  payable  half-yearly.  He  was  unable 
to  pay  for  five  successive  years,  the  last  half-year's  rent  having  been  due  three 
years  ago.  Find  how  much  he  owes  his  landlord,  allowing  compound  interest 
at  3%. 

HereA  =  78,     R  =  l-015,     m  =  6,     n  =  10. 

V  =  78  x  1-0156(1-01510-1)/-015. 
10  log  1-015  =-0646600, 

1-01510=  1-16054. 

V  =  78  x  l-0156x  -16054/-015. 
log  78         =1-8920946 

6  log  1-015    =    -0387960 


log  -16054 

=  1-2055833 

log  -015 

1-1364739 
=  2-1760913 

logV 

=  2-9603826 
Y  =  £912-814  =  £912 

16  :  3. 

§  7.]  Another  fundamental  problem  is  to  calculate  the  purchase 
price  of  a  given  annuity.  Let  us  suppose  that  B  wishes,  by  paying 
down  at  once  a  sum  £P,  to  acquire  for  himself  and  his  heirs  the 
right  of  receiving  n  periodic  payments  of  £A  each,  the  first  pa}*- 
ment  to  be  made  m  periods  hence.     We  have  to  find  P. 

P  is  obviously  the  sum  of  the  present  values  of  the  n  pay- 


538  PURCHASE  PRICE  OF  AX  ANNUITY  chap. 

ments.  Now  the  first  of  these  is  due  m  years  hence  ;  its  present 
value  is  therefore  A/K"1.  The  second  is  due  ra  +  1  years  hence ; 
A's  present  value  is  therefore  A/K,n+1,  and  so  on.     Hence 

V-—       A  A  . 


Hence 


P  =  K^(1"^)/(1"F. 

A—l(Rn_l)/(R_l)  (2). 


Km+r 

Cor.  1.  The  ratio  of  the  purchase  price  of  an  annuity  to  the 
annual  payment  is  often  spoken  of  as  the  number  of  years'  purchase 
which  the  annuity  is  worth.  If  the  "period  "  understood  in  the 
above  investigation  be  a  year,  and  p  be  the  number  of  years'  purchase, 
then  we  have  from  (2) 

p  =  (R«  -  l)[Rm+n-x(T&  -  1)  (3). 

If  the  period  be  1/qth  of  a  year,  since  the  annual  payment  is  then 

qA.,  we  have 

p  =  (Rn  -  1  )/qRm +n-\R-l)  (4 ) . 

Cor.  2.  If  the  annuity  be  not  " deferred"  as  it  is  called,  but 
begin  to  run  at  once,  that  is  to  say,  if  the  first  payment  be  due  one 
period  hence*  then  m-  1,  and  we  have 

P  =  A(R»-1)/R"(R-1), 
=  A(l-R-»)/(R-l)  (5). 

Also 

2>  =  (R"-1)/R»(R-1), 
=  (l-R-»)/(R-l)  (6); 

or  p  =  (\-B-n)/q(R-l)  (7), 

according  as  the  period  of  conversion  is  a  year  or  the  qth  part  of  a  year. 
Cor.  3.  To  obtain  the  present  value  of  a  deferred  perpetual 
annuity,  or,  as  it  is  often  put,  the  present  value  of  the  reversion  of  a 
perpetual  annuity,  we  have  merely  to  make  n  infinitely  great  in  the 
equation  (2).      We  thus  obtain 

*  This  is  the  usual  meaning  of  "heginning  to  run  at  once."     In  some 
cases  the  tir*t  payment  is  made  at  once.     In  that  case,  of  course.  ?n.  =  0. 


xxu  NUMBER  OF  YEARS'  PURCHASE  OF  A  FREEHOLD 


539 


p-4/fi-1 


=  A/R'«-1(R-1)  (8). 
Hence,  for  the  number  of  years'  purchase,  we  have 

p  =  l/E^-^R  -  1)  (9), 

or                                   p=l/ffRTO-1(E-l)  (10), 

according  as  the  period  of  conversion  is  a  year  or  1/qth  of  a  yea?: 

Cor.  4.    JFlien  the  perpetual  annuity  begins  to  run  at  once  the 
formulce  (8),  (9),  (10)  become  very  simple.     Putting  m=  1  we  have 

P  =  A/(R-1), 
=  A/(l+r-l), 

=  A/r  (11). 

For  the  number  of  years'  purchase 

p=\jr  (12); 

or  p=l/qr  (13), 

according  as  the  period  of  conversion  is  a  year  or  1/qth  of  a  year. 

If  the  period  be  a  year,  remembering  that,  if  s  be  the  rate 
per  cent  of  interest  allowed,  then  r  =  sj  100,  we  see  that 

p=100/s  (14). 

Hence  the  following  very  simple  rule  for  the  value  of  a  perpetual 
annuity.  To  find  the  number  of  years'  purcfoise,  divide  100  by  the 
rate  per  cent  of  interest  corresponding  to  the  kind  of  investment  in 
question.  This  rule  is  much  used  by  practical  men.  The  following 
table  will  illustrate  its  application  : — 


Rate  %         .         .         . 

3 

H 

4 

4|  i       5            5i  '       6 

1 

No.  of  years'  purchase  . 

33 

28 

25 

22 

20 

18 

17 

Example. 

A  sum  of  £30,000  is  borrowed,  to  be  repaid  in  30  equal  yearly  instalments 
which  are  to  cover  both  principal  and  interest.  To  find  the  yearly  payment, 
allowing  compound  interest  at  4|  %. 

Let  A  be  the  annual  payment,  then  £30,000  is  the  present  value  of  an 


540  INTEREST  AND  ANNUITY  TABLES  CHAf. 

annuity  of  <£A  payable  yearly,  the  annuity  to  begin  at  once  and  run  for  30 
years.     Hence,  by  (5)  above, 

30,000  =  A(l  -  r045-30)/-045, 
A  =  1350/(l-l-045-30), 
-  30  log  1  -045  =  1  -4265110, 
l-045~so=  -267000. 
A  =  1350/-733, 
=  £1841  :  14  :  11. 

§  8.]  It  would  be  easy,  by  assuming  the  periodic  instalments 
or  the  periods  of  an  annuity  to  vary  according  to  given  laws,  to 
complicate  the  details  of  annuity  calculations  veiy  seriously ; 
but,  as  we  should  in  this  way  illustrate  no  general  principle  of 
any  importance,  it  will  be  sufficient  to  refer  the  student  to  one 
or  two  instances  of  this  kind  given  among  the  examples  at  the 
end  of  this  chapter. 

It  only  remains  to  mention  that  in  practice  the  calculation 
of  interest  and  annuities  is  much  facilitated  by  the  use  of  tables 
(such  as  those  of  Turnbull,  for  example),  in  which  the  values  of  the 
functions  (1  +  r)n,  (1  +r)~n,  {(1  +  r)n  -  1  }jr,  {1  -  (1  +  r)-n}jr, 
rj{\  -(1  +r)~n},  &c,  are  tabulated  for  various  values  of  lOOr 
and  ii.  For  further  information  on  this  subject  see  the  Text-Book 
of  the  Institute  of  Actuaries,  Part  I.,  p.  151. 

Exercises  XLIV. 

^1.)  The  difference  between  the  true  discount  and  the  interest  on  £40,400 
for  a  period  x  is  £4,  simple  interest  being  allowed  at  4  %  >  fiud  x. 

(2.)  Find  the  present  value  of  £15,000  due  50  years  hence,  allowing  4i  °/B 
compound  interest,  convertible  yearly. 

(3.)  Find  the  amount  of  £150  at  the  end  of  14  years,  allowing  3  °/0  com- 
pound interest,  convertible  half-yearly,  and  deducting  6d.  per  £  for  income- 
tax. 

(4.)  How  long  will  it  take  for  a  sum  to  double  itself  at  6  %  compound 
interest,  convertible  annually  ? 

(5.)  How  long  will  it  take  for  one  penny  to  amount  to  £1000  at  5  °/0  com- 
pound interest,  convertible  annually  ? 

(6.)  On  a  salary  of  £100,  what  difference  does  it  make  whether  it  is  paid 
quarterly  or  monthly  ?  Work  out  the  result  both  for  simple  and  for  compound 
interest  at  the  rate  of  4-2  °/0. 

(7.)  A  sum  £A  is  laid  out  at  10  %  compound  interest,  convertible  annually, 
arid  a  sum  £2.V  at  5  %  compound  interest,  convertible  half-yearly.  After 
how  many  years  will  the  amounts  be  ecpual  ? 


XXII 


EXERCISES  XLIV  541 


(8.)  Show  that  the  difference  between  bankers'  discount  and  true  discount, 
simple  interest  being  supposed,  is 

A?)  V2  {1  -  nr  +  nh-2  -  iflr3  + .   .  .   ad  oo  } . 

(9.)  If  r>  5/100,  n ■>  10,  find  an  upper  limit  for  the  error  in  taking 
100(1  +nCir  +  nC-2r2-  +  nC3r:])  as  the  amount  of  £100  in  n  years  at  100/-  %  com- 
pound interest,  convertible  annually. 

(10.)  If  £IC  and  £ls  denote  the  whole  compound  and  the  whole  simple 
interest  on  £P  for  n  years  at  100?-  %>  convertible  annually,  show  that 
Ir-Is  =  P(,1C2r2  +  „C3r!+  .    .   .+  '/■»). 

(11.)  A  man  owes  £P,  on  which  he  pays  lOOr  %  annually,  the  principal 
to  be  paid  up  after  n  years.  What  sum  must  he  invest,  at  100r'  °/0,  so  as  to  be 
just  able  to  pay  the  interest  annually,  and  the  principal  £P  when  it  falls  due  ? 

(12.)  B  has  a  debenture  bond  of  £500  on  a  railway.  When  the  bond  lias 
still  five  years  to  run,  the  company  lower  the  interest  from  5  %>  which  was 
the  rate  agreed  upon,  to  4  °/0,  and,  in  compensation,  increase  the  amount  of 
B's  bond  by  x  °/a.  Find  x,  supposing  that  B  can  always  invest  his  interest 
at  5  %. 

(13.)  A  person  owes  £20,122  payable  12  years  hence,  and  offers  £10,000 
down  to  liquidate  the  debt.  What  rate  of  compound  interest,  convertible 
annually,  does  he  demand  ? 

(14.)  A  testator  directed  that  his  trustees,  in  arranging  his  affairs,  should 
set  apart  such  sums  for  each  of  his  three  sons  that  each  might  receive  the 
same  amount  when  he  came  of  age.  When  he  died  his  estate  was  worth 
£150,000,  and  the  ages  of  his  sons  were  8,  12,  and  17  respectively.  Find 
what  sum  was  set  apart  for  each,  reckoning  4  %  compound  interest  for 
accumulations. 

(15.)  B  owes  to  C  the  sums  Ai,  A-2,  .  .  .,  Ar  at  dates  Bi,  n2,  .  .  .,  »r 
years  hence.  Find  at  what  date  B  may  equitably  discharge  his  debt  to  C 
by  paying  all  'the  sums  together,  supposing  that  they  all  bear  the  same  rate 
of  interest ;  and 

1st.  Allowing  interest  and  interest  in  lieu  of  discount  where  discount  is  due. 

2nd.  Allowing  compound  interest,  and  true  discount  at  compound  interest. 

(16.)  Required  the  accumulated  value  at  the  end  of  15  years  of  an  annuity 
of  £50,  payable  in  quarterly  instalments.     Allow  compound  interest  at  5  %• 

(17.)  A  loan  of  £100  is  to  be  paid  off  in  10  equal  monthly  instalments. 
Find  the  monthly  payment,  reckoning  compound  interest  at  6  %• 

(18.)  I  borrow  £1000,  and  repay  £10  at  the  end  of  every  month  for  10 
years.  Find  an  equation  for  the  rate  of  interest  I  pay.  What  kind  of 
interest  table  would  help  you  in  practically  solving  such  a  question  as  this  ? 

(19.)  The  reversion  after  2  years  of  a  freehold  worth  £168  :  2s.  a  year  is  to 
be  sold  :  find  its  present  value,  allowing  interest  at  2  %>  convertible  annually. 

(20.)  Find  the  present  value  of  a  freehold  of  £365  a  year,  reckoning  com- 
pound interest  at  3J  %,  convertible  half-yearly,  and  deducting  6d.  per  £  of 
income-tax. 

(21.)  If  a  perpetual  annuity  be  worth  25  years'  purchase,  what  annuity  to 


542  EXERCISES  XLIV  chap,   xxii 

continue  for  3  years  can  be  bought  for  £5000  so  as  to  bring  the  same  rate  of 
interest  ? 

(22. )  If  20  years'  purchase  be  paid  for  an  annuity  to  continue  for  a  certain 
number  of  years,  and  24  years'  purchase  for  one  to  continue  twice  as  long,  find 
the  rate  of  interest  (convertible  annually). 

(23.)  Two  proprietors  have  equal  shares  in  an  estate  of  £500  a  year.  One 
buys  the  other  out  by  assigning  him  a  terminable  annuity  to  last  for  20  years. 
Find  the  annuity,  reckoning  3|  %  compound  interest,  convertible  annually. 

(24.)  The  reversion  of  an  estate  of  £150  a  year  is  sold  for  £2000.  How 
long  ought  the  entry  to  be  deferred  if  the  rate  of  interest  on  the  investment 
is  to  be  4|  %>  convertible  annually  ? 

(25.)  If  a  lease  of  19  years  at  a  nominal  rent  be  purchased  for  £1000,  what 
ought  the  real  rent  to  be  in  order  that  the  purchaser  may  get  4  °/0  on  his 
investment  (interest  convertible  half-yearly)  ? 

(26.)  B  and  C  have  equal  interests  in  an  annuity  of  £A  for  2n  years  (pay- 
able annually).  They  agree  to  take  the  payments  alternately,  B  taking  the 
first.     What  ought  B  to  pay  to  C  for  the  privilege  he  thus  receives  ? 

(27. )  A  farmer  bought  a  lease  for  20  years  of  his  farm  at  a  rent  of  £50, 
payable  half-yearly.  After  10  years  had  run  he  determined  to  buy  the  free- 
hold of  the  farm.  "What  ought  he  to  pay  the  landlord  if  the  full  rent  of  the 
farm  be  £100  payable  half-yearly,  and  3  %  be  the  rate  of  interest  on  invest- 
ments in  land  ? 

(28.)  What  annuity  beginning  n  years  hence  and  lasting  for  n  years  is 
equivalent  to  an  annuity  of  £A,  beginning  now  and  lasting  for  n  years  ? 

(29.)  A  testator  left  £100,000  to  be  shared  equally  between  two  institu- 
tions B  and  C  ;  B  to  enjoy  the  interest  for  a  certain  number  of  years,  C  to 
have  the  reversion.  How  many  years  ought  B  to  receive  the  interest  if  the 
rate  be  3^  %>  convertible  annually  ? 

(30.)  If  a  man  live  m  years,  for  how  many  years  must  he  pay  an  annuity 
of  £A  in  order  that  he  may  receive  an  annuity  of  the  same  amount  for  the 
rest  of  his  life  ?  Show  that,  if  the  annuity  to  be  acquired  is  to  continue  for 
ever,  then  the  number  of  years  is  that  in  which  a  sum  of  money  would  doublo 
itself  at  the  supposed  rate  of  interest. 

(31.)  A  gentleman's  estate  was  subject  to  an  annual  burden  of  £100.  His 
expenses  in  any  year  varied  as  the  number  of  years  he  had  lived,  and  his 
income  as  the  square  of  that  number.  In  his  21st  year  he  spent  £10,458, 
and  his  income,  before  deducting  the  annual  burden,  was  £4410.  Show  that 
he  ran  in  debt  every  year  till  he  was  50. 

(32.)  A  feu  is  sold  for  £1500,  with  a  feu-duty  of  £18  payable  annually, 
and  a  casualty  of  £100  payable  every  50  years.  What  would  have  been  the 
price  of  the  feu  if  it  had  been  bought  outright  ?     Beckon  interest  at  4£  %• 

(33.)  Find  the  accumulation  and  also  the  present  value  of  an  annuity 
when  the  annual  payments  increase  in  A.r. 

(34.)  Solve  the  same  problem  when  the  increase  is  in  G.P. 

(35.)  The  rental  of  an  estate  is  £mA  to  begin  with  ;  but  at  the  end  of 
every  q  years  the  rental  is  diminished  by  £A,  owing  to  the  incidence  of  fresh 
taxation.     Find  the  present  value  of  the  estate. 


APPENDIX 

ON  THE  GENERAL  SOLUTION  OF  CUBIC  AND  BIQUAD- 
RATIC EQUATIONS;  AND  ON  THE  CASES  WHERE 
SUCH  EQUATIONS  CAN  BE  SOLVED  BY  MEANS  OF 
QUADRATIC  EQUATIONS. 

§  1.]  Since  cubic  and  biquadratic  equations  are  of  frequent 
occurrence  in  elementary  mathematics,  and  many  interesting 
geometric  problems  can  be  made  to  depend  on  their  solution,  a 
brief  account  of  their  leading  properties  may  be  useful  to  readers 
of  this  book.  Incidentally,  we  shall  meet  with  some  principles 
of  importance  in  the  General  Theory  of  Equations. 


COMMENSURABLE    ROOTS   AND    REDUCTIBILITY. 

§  2.]  We  shall  suppose  in  all  that  follows  that  the  coefficients 
Po  •  •  •>  Pn  °f  any  equation, 

p0xn  +p,xn-1  +  .  .  .  +  p„,  =  0  (1), 

are  all  real  commensurable  numbers.  If,  as  in  chap,  xv.,  §  21, 
we  put  x  =  £/m,  we  derive  from  (1)  the  equivalent  equation 

Poim  +plm$'1-1  +  .  .  .  +pn-,mn'1$  +pnmn  =  0       (2), 

each  of  whose  roots  is  m  times  a  corresponding  root  of  (1).  If 
we  then  choose  m  so  that  mp,jp0,  .  .  .,  mn~1pn.1/p0,  mnpnfp0  are 
all  integral — for  example,  by  taking  for  m  the  L.C.M.  of  the  de- 
nominators of  the  fractions  pxjpm  .  .  .,  pn-i/Po>  Pn/po — we  shall 
reduce  (2)  to  the  form 

£■  +  },£»-!  +  .  .  .+qn  =  0  (3), 

in  which  all  the  coefficients  are  positive  or  negative  integers,  and  the 


544  APPENDIX 

coefficients  of  the  highest  term  unity.  We  may  call  this  the  Special 
Integral  Form. 

§  3.]  If,  as  in  chap,  xv.,  §  22,  we  put  x  =  £  +  a,  we  transform 
the  equation  (1)  into 

i>o£"  +  fl,i£"~1  +  .  •  -  +  <z»  =  o, 

where  q1  =  npt)a+p1.  Hence,  if  we  take  a=  —pijnpm  the  trans- 
formed equation  becomes 

&?+.?&-*  +  •  •  .  +  qn  =  o  (4), 

wherein  q2,  .  .  .,  q'n  have  now  determinate  values.  It  follows 
that 

By  a  proper  linear  transformation,  we  can  always  deprive  an 
equation  of  the  nth  degree  of  its  highest  term  but  one. 

We  can,  of  course,  combine  the  transformations  of  §§  2,  3, 
and  reduce  an  equation  to  a  special  integral  form  wanting  the 
highest  term  but  one. 

§  4.]  If  an  equation  of  the  special  integral  form  has  commensurable 
roots,  these  roots  must  be  integral,  and  can  only  be  exact  divisors  of 
its  absolute  term.  For,  suppose  that  the  equation  (3)  has  the 
fractional  commensurable  root  a/b,  where  a  may  be  supposed  to 
be  prime  to  b.     Then  we  have  the  identity 

(a/b)n  +  qi(alb)n-i  +  .  .  .+qn  =  0, 
whence 

an/b=  -  q.a11-1  -  qaan~2b  -  ...  -  qnbn~x, 

which  is  impossible,  since  the  left-hand  side  is  a  fraction  and  the 
right-hand  side  an  integer. 

Also,  if  x  =  a  be  any  integral  root,  we  must  have 

qn/a=  -a'1"1-^-2-.  .   .-qn.v 

Hence,  since  the  right-hand  side  is  obviously  an  integral  number, 
a  must  be  an  exact  divisor  of  qn. 

The  commensurable  roots  of  an  equation,  if  any  exist,  can  therefore 
always  be  found  by  a  limited  number  of  arithmetical  operations. 

We  have  merely  to  reduce  the  equation  to  an  equivalent 
special  integral  form,  and  substitute  the  divisors  of  its  absolute 
term  one  after  the  other  in  the  characteristic.  The  number  of 
trials  may  in   most  cases  be  reduced  by  obtaining  upper  and 


APPENDIX  545 

lower  limits  for  the  roots  by  means  of  the  theorem  of  chap,  xii., 
§  21,  by  graphical  methods,  or  otherwise. 

Example.  a;3-  10x2  + 31a; -30  =  0.  This  equation  is  already  in  the 
special  integral  form.  Hence  the  only  possible  commensurable  roots  are 
±1,  ±2,  ±3,  ±5,  ±6,  ±10,  +15,  ±30.  It  is  obvious  that  the 
equation  has  no  negative  roots  ;  and,  since  ai(ar  +  31)  =  10(a;2  +  3),  it  is 
useless  to  try  x  =  10  or  any  larger  number.  Of  the  remaining  possible 
numbers,  +1,  +  2,  +3,  +5,  it  is  immediately  found  that  +2,  +3,  and  +5 
are  roots. 

§  5.]  An  equation  is  said  to  be  reducible  when  it  has  a  root  or 
roots  in  common  with  an  equation  of  lower  degree  (having  of 
course  commensurable  coefficients) ;  irreducible  if  it  has  no  root  in 
common  with  any  equation  of  lower  degree. 

If  an  equation  f(x)  =  0  have  roots  in  common  with  an 
equation  of  lower  degree  <f>(x)  =  0,  then  the  product  of  the  linear 
factors  corresponding  to  all  such  common  roots,  say  g(x),  is  the 
G.C.M.  of  the  characteristics  f(x)  and  <£(.r),  which  can  be  deduced 
from  these  functions  by  purely  rational  operations.  It  follows 
that  f(x)  =  g(x)h(x),  where  g(x)  and  h(x)  are  integral  functions  of 
x  having  commensurable  coefficients.  The  roots  of  f(x)  =  0  are 
therefore  the  aggregate  of  the  roots  of  the  two  equations  g(x)  =  0, 
h(x)  =  0,  each  of  lower  degree  than  the  original  equation.  Each 
of  these  new  equations  may  be  reducible  or  irreducible ;  but  it 
is  obvious  that  at  last  we  must  arrive  at  a  series  of  irreducible 
equations  the  aggregate  of  whose  roots  are  the  roots  of  f(x)  =  0  ; 
and  the  characteristics  of  these  equations  are  the  irreducible 
factors  of  f(x),  irreducible  in  the  sense  that  they  cannot  be 
decomposed  into  integral  factors  of  lower  degree  having  com- 
mensurable coefficients. 

§  6.]  The  following  theorem,  often  appealed  to  in  the  theory 
of  equations,  is  an  immediate  consequence  of  the  notion  of  irre- 
ducibility  explained  in  the  last  paragraph. 

If  an  irreducible  equation  A  have  a  root  in  common  with  an 
equation  B  (reducible  or  irreducible),  then  every  root  of  A  is  a  root 
ofB. 

For,  if  only  some  of  the  roots  of  A  were  roots  of  B,  then  a 
common  commensurable  factor  of  the  characteristics  of  A  and  B 
could  be  found  of  less  degree  than  A  itself ;  and  A  would  not 
be  irreducible. 

§  7.]  When  an  equation  is  reducible  it  can  be  reduced  by  a  finite 
number  of  arithmetical  operations. 

VOL.  I  2  N 


546  APPENDIX 

Consider  the  equation 

f{x)=x"  +iV;"-1  +  .   .  .  +pn  =  0  (5), 

whose  roots  are  a„  a2,  .  .   .  an. 

If  (5)  be  reducible,  then  f(x)  must  have  a  commensurable  factor 
of  the  1st,  or  2nd,  .  .  .,  or/th  degree,  where  (/)  is  the  greatest 
integer  in  n/2. 

If/(x)  has  a  commensurable  factor  of  the  1st  degree,  (5)  has 
a  commensurable  root,  which  can  be  found  as  explained  in  §  4. 

If  f(x)  has  a  commensurable  factor  of  the  sth  degree,  let 
o„  aa  .  .  .,  as  be  the  corresponding  roots ;  and  let 

(x - a^x - Og)  .  .  .  (x-at)  =  x'-qix*-1  +  .  .  ,±q,      (6), 

s  s 

where  qi  =  2a„  q2  =  2a,a2,  .    .   .,  qs  =  a^  .    .    .    ag, 

l  l 

are  by  hypothesis  all  commensurable.     If  we  form  the  equations 

n  s  n  s  n 

U(x  -  2a,)  =  0,  U(x  -  2a,a2)  =  0,  .  .  .  U(x  -  aia2  .  .  .  a»)=  0     (7), 
llil  l 

the  roots  of  which  are  respectively  all  the  different  values  of 

s  s 

2aI}      ^a,a2,      .    .    .,      O-iC-2   •    •    •    as 

1  1 

obtained  by  taking  every  possible  selection  of  s  of  the  roots  of 
(5),  then  the  coefficients  of  these  equations  are  symmetric 
functions  of  the  roots  of  (5),  therefore  rational  functions  of  the  co- 
efficients of  (5),  and  therefore  commensurable.  But  ql}  q2,  .  .  .,  qs 
are  obviously  roots  of  the  respective  equations  (7),  and,  being 
commensurable,  can  be  found  by  a  finite  number  of  trials. 

In  point  of  fact,  it  is  in  general  sufficient  to  determine  q  as 
a  commensurable  root  of  the  first  of  (7),  and  then  determine  the 

n  5-1 

function  (6)  as  the  G.C.M.  oif(x)  and  II(a;  -  J,  +  2a,).     The  proof, 

i  i 

and  the  discussion  of  possible  exceptions,  may  be  left  to  the 
reader. 

EQUATIONS    SOLUBLE   BY   MEANS    OF   SQUARE    ROOTS. 

§  8.]  Reference  to  the  theory  of  irrational  operations  laid 
down  in  chap.  x.  will  show  that  any  function  which  is  constructed 
by  means  of  a  finite  number  of  the  operations  +  ,  —  ,  x  ,  -=- ,  */ 
may  without  loss  of  generality  be  supposed  to  be  constructed 
as  follows  : — 


APPENDIX  547 

Starting  with  the  series  of  rational  numbers,  we  construct  a 
number  of  quadratic  irrationals,  say  \/a„  Ja3,  .  .  .  Any 
rational  functions  of  these  may  be  reduced  to  linear  forms,  such 
as  A  +  B^/a,  +  .  .  .  +  C\/a,\/a2  +  .  .  .,  which  we  may  describe 
as  quadratic  irrationals  of  the  first  order.     We  suppose  that   \ZaM 

N  «,,  .  .  .  are  independent,  in  the  sense  that  there  is  no  linear 
relation,  such  as  P  +  Qs/a,  +  .  .  .  +  Hja^a,  +  .  .  .  =  0,  con- 
necting them ;  for,  if  there  were  any  such  relation,  we  could  use 
it  to  get  rid  of   \/a,  by  expressing  it  as   a  linear  function   of 

\/a3  .  .  .,  and  thus  reduce  the  number  of  independent  square 
roots. 

Next  consider  >Jbu  >/&2,  .  .  .,  where  &„  &„,...  are  quadratic 
irrationals  of  the  first  order  reduced  as  above.  Then  take 
rational  functions  of  these,  and  reduce  them  to  linear  forms  con- 
taining only  independent  square  roots  as  before.  These  we  may 
call  quadratic  irrationals  of  the  second  order. 

Proceeding  in  this  way,  we  can  build  up  quadratic  irrational 
functions  of  any  order;  and  it  is  obvious  that  every  function  which 
is  constructed  by  means  of  a  finite  number  of  the  operations  +  ,  -  , 

x  ,  h-  ,  \f  is  a  quadratic  irrational  of  a  finite  order  in  the  above  scale. 

For  example,  3+^/2  +  2  */2  N/3,  N'(  N/2  +  N/3)  +  J(  s>2  -  N'3),  ^2  +  N'{3  + 
N'(  N'2+  ^/3)}  are  quadratic  irrationals  of  the  first,  second,  and  third  orders 
respectively. 

Def.  If  we  give  every  possible  arrangement  of  signs  to  the 
square  roots  in  a  quadratic  irrational  function  which  contains  p 
square  roots,  we  get  2^  values,  which  are  said  to  be  conjugate  to 
one  another.  It  should  be  noticed  that  the  conjugates  may 
not  be  all  different;  e.g.,  N/(  \/2  +  «/3)  +  \/(  J2  -  J 3)  and 
\/(  \/2  -  v/3)  +  \/(  \>'2  +  \/3)  are  conjugate  with  respect  to 
\/3,  but  they  are  not  distinct. 

§  9.]  If  any  quadratic  irrational  x„  containing  p  square  roots,  is 
a  root  of  an  irreducible  equation  f(x)  =  0,  then  all  its  conjugates, 
x2,  .   .  .,  x^,  (fj.  -  2P)  are  also  roots  of  the  same  equation. 

For,  if  we  substitute  .r,  in  the  equation,  we  shall  in  the  first 
place  get  an  identity  the  left-hand  side  of  which  will  be  a  linear 
quadratic  irrational  function  of  say  the  kih  order.  Since  our 
square  roots  are  independent,  such  a  relation  cannot  exist  unless 
each  term  is  zero  independently.  We  are  thus  led  to  a  series  of 
identities  involving  quadratic  irrational  functions  of  order  h—  1, 
or  lower.     Applying  the  same  reasoning  again  and  again,  we  are 


548  APPENDIX 

at  last  led  to  a  series  of  identities  in  which  there  are  no  square 
roots  at  all.  These  must  hold  whatever  the  signs  of  the  square 
roots  originally  involved  may  have  been.  Hence,  if  x,  nullify 
f(x),  so  must  also  x2,  .   .   .,  x^. 

It  is  easy  to  see,  by  reasoning  similar  to  that  employed  in 
chap,  x.,  §  1 6,  that  the  function 

\p(x)  =  (x-  x^){x  -  x2)  .  .   .   (x-  xj 

is  an  integral  function  of  degree  /x  =  2p  in  x,  whose  coefficients 
are  commensurable. 

If  xu  .  .  .,  x^  are  all  unequal,  then,  since  these  are  all  roots 
of /(»)  =  (),  \f>(x)  and  f(x)  can  only  differ  by  a  constant  factor. 
Therefore  the  degree  of  f(x)  is  2^. 

If  x„  .  .  .,  x  are  not  all  unequal,  then  each  of  them  must 
be  repeated  the  same  number  of  times ;  otherwise,  by  dividing 
\f(x)  by  a  proper  power  of  f{x)  we  should  obtain  the  characteristic 
function  of  an  equation  which  has  some  but  not  all  of  the  roots 
of  f(x)  =  0,  which,  by  §  6,  is  impossible,  since  f(x)  =  0  is  irre- 
ducible. It  follows  that  the  degree  of  f(x)  is  a  factor  of  2-P,  that 
is  to  say,  is  some  power  of  2  lower  than  the  ^th.  Hence  the 
following  important  result : — 

The  degree  of  an  irreducible  equation  which  can  be  solved  by  means 
of  square  roots  must  be  a  power  of  2  ;  and  its  roots  can  all  be  deduced 
from  any  one  by  -varying  the  signs  of  the  square  roots  involved  in  the 
expression  for  that  root. 

By  a  process  of  continually  pairing  factors  which  are  con- 
jugate with  respect  to  any  particular  square  root,  we  can  reduce 
the  characteristic  of  any  equation  soluble  by  means  of  square 
roots  to  the  product  of  two  conjugate  factors,  each  of  which  con- 
tains only  the  square  root  of  a  commensurable  number.  Hence 
any  such  equation  can  be  put  into  the  form 

(xn  +  pxxn~x  +  .   .   .+pn)2-p(xn-1  +  q1xn-2  +  .   .   . +?„_1)2  =  0, 

where  p.,  .  .  .,  pn-»  2u  •  •  •>  ?»-u  anc^  P  are  au  commensurable. 
This  transformation  may  be  regarded  as  the  first  step  in  the 
solution  of  the  equation.* 


*  For  further  discussion  of  this  matter,  see  Petersen's  Thtorie  des 
Equations  Algtbriques  (trans,  by  Laurent,  1897),  chap,  vii.,  from  which  the 
substance  of  §§  8,  9  are  taken. 


APPENDIX  549 


THE    CUBIC    EQUATION. 

§  10.]  We  have  seen  (§  3)  that  every  cubic  equation  can  be 
reduced  to  the  form 

z3  +  qz-rr  =  0  (1). 

If  (a  be  an  imaginary  cube  root  of  unity,  we  have  the  identity 

x3  +  y3  +  z3  -  3xyz=(x  +  y  +  z)(x  +  u>y  +  uz)  (x  +  wy  +  wz). 

It  follows  that  the  roots  of  the  equation 

x3  -  (3yz)x  +  (y3  +  z3)  =  0  (2) 

are  -  y  -  z,   —<ay—  ufz,  -  u>sy  -  wz. 
Now,  if 

yz=  -q/S,     y3  +  z3  =  r  (3), 

the  equations  (1)  and  (2)  are  identical. 

From  (3)  we  see  that  y3  and  z3  are  the  roots  of  the  quadratic 

?-r$-q3l27  =  Q  (4). 

Hence,  if 

H-'(t4)'m4^(t4)     « 

then  the  roots  of  (1)  are 

-  f/L  -  4/M,  -  (o  £/L  -  or  4/M,  -  «r  */L  -  w  #M      (6). 

When  r2/4  +  g'3/27  is  positive,  (6)  gives  the  roots  of  the  cubic  in  a  con- 
venient form  for  computation  ;  and  in  this  case  one  root  is  real  and  two 
imaginary.  -  ijh  -  ^/M  is  the  famous  expression  of  Cardan  for  the  root  of 
a  cubic  equation,  which  formed  the  subject  of  a  notorious  controversy 
between  him  and  his  countryman  Tartaglia. 

If  r2l±  +  qs/27  is  negative,  so  that  q  must  be  a  negative  number,  the 
expressions  (6)  in  their  algebraic  form  are  useless  for  the  purposes  of 
numerical  calculation.  We  may,  however,  use  the  circular  functions,  as  in 
chap,  xii.,  §  17,  for  finding  the  principal  values  of  £/L  and  £/M.  We  thus 
find  that  the  roots  are  -  2p*  cos  0/3,  -  2p*  cos  (2tt  +  6)13,  -  2pi  cos  (4tt  +  0)/3, 
where  p  =  (  -g-)3/27i,  and  cos0  =  r27V2(  -?)'.  The  three  roots  are  therefore 
all  real  (Cardan's  Irreducible  Case).* 

If  r/4  + <f/27  be  zero,  two  of  the  roots  are  equal,  and  all 
three  real. 

*  See  also  Pressland  and  Tweedie's  Trigonometry,  §  124. 


550  APPENDIX 

§  11.]  Since  3  is  not  a  power  of  2,  it  follows  from  §  8  that  a 
cubic  cannot  be  solved  by  means  of  square  roots  unless  it  is 
reducible :  in  other  words,  unless  it  has  a  commensurable  root. 
In  that  case  it  may  happen  that  the  other  two  roots  are  also 
commensurable,  so  that  no  irrational  operations  at  all  are 
required  for  the  solution. 

It  follows  from  the  result  of  §§  9  and  10,  that  an  irreducible 
cubic  requires  both  square  and  cubic  roots  for  its  formal  solution. 


THE    BIQUADRATIC    EQUATION. 

§  12.]  The  solution  of  the  biquadratic 

x4  +  pa?  +  qx2  +  rx  +  s  =  0  (1 ) 

can  always  be  made  to  depend  on  the  solution  of  a  cubic  and  two 
quadratic  equations. 

For  we  may  conjoin  with  (1)  the  equation 

x*-y  =  0  (2), 

and  regard  (1)  as  the  z-eliminant  of  the  system  (1)  (2).  Now, 
using  (2)  to  transform  (1),  we  see  that  the  system  (1)  (2)  is 
equivalent  to  the  system 

qx2  +  pxy  +  y2  +  rx  +  s  =  0,     x2  -  y  =  0  ; 
and  this  system  again  to 

(q  -  X)x2  +  pxy  +  y2  +  rx  +  Xy  +  s  =  0  (3), 

and  x2  -  y  =  0  (4). 

Now  (see  chap,  vii.,  §  13)  we  can  always  determine  X  so  that  (3) 
shall  break  up  into  two  linear  equations.  We  have  merely  to 
choose  A  so  that 

In  other  words,  X  must  be  a  root  of  the  cubic  equation 

A3  -  qX2  +  (pr  -  4s)X  +  iqs  -  r2  -  p2s  =  0  (5), 

called  Lagrange's  Resolvent. 

If  we  substitute  in  (3)  for  A  any  one  of  the  three  roots  of  (5), 
then  (3)  takes  the  form 

(y  +  ax  +  ft)(y  +  yx+S)  =  0; 


APPENDIX  551 

and  the  system  (3)  (4)  leads  to  the  two  quadratics 

a?  +  ax  +  p=  0,  x*  +  yx  +  8  =  0  (6), 

the  roots  of  which  are  the  four  roots  of  the  biquadratic  (1). 

If  xly  x2,  x3,  xt  be  the  roots  of  the  biquadratic  taken  in  a 
certain  order,  then  we  see  from  (6)  that  (3  +  8  =  Xfa  +  xjct.     Also 
from    the    identity    (q  -  X)x2  +  pxy  +  if  +  rx  +  Xy  +  s  =  (y  +  ax  +  /3) 
(i/  +  yx  +  8)  we  see,  by  comparing  coefficients  of  y,  that  X  =  (3  +  8  = 
xxx2  +  xg,v     Hence  the  following  interesting  result  : — 

Cor.    The   roofs   of  Lagrange's   cubic   resolvent   are   xxxa  +  x3x4, 

13  "*     *^2    4)    *^i*^'4     i     *^2*   3* 

The  above  method  for  solving  a  biquadratic  is  merely  an  analytical 
translation  of  the  geometrically  obvious  fact  that  the  four  points  of  inter- 
section of  two  conic  sections  can  be  determined  by  finding  the  intersections 
with  either  of  the  conies  of  any  one  of  the  three  pairs  of  straight  lines  which 
contain  all  the  four  points. 

Example. 

sc4-5<Es+538  +  5a;-6  =  0  (1). 

Conjoin  x2-y  =  0  (2). 

Then  we  have  the  system 

5x2 -5xy  +  y2  +  5x-  6  =  0,     x--y  =  0, 
equivalent  to 

{5-\)x2-5xy  +  y*  +  5x  +  \y-6  =  0  (3). 

cc2-2/  =  0  (4). 

The  cubic  resolvent  is 

\3-5A2-\  +  5  =  0; 

that  is  (\-5)(\2-l)  =  0  (5), 

which  happens  to  have  three  commensurable  roots.     We  take  the  simplest, 
X  =  l,  and  find  that  (3)  becomes 

(y-lx  +  3)(y-x-2)  =  Q; 

so  that  the  roots  of  (1)  are  given  by 

x°--4x  +  3  =  0,  x~-x-2  =  0  (6). 

They  are  in  fact  1,  3,  2,  -  1. 

§  13.]  If  the  cubic  resolvent  is  irreducible,  X  will  involve  an 
incommensurable  cube  root,  and  the  roots  of  the  biquadratic  will 
not  be  expressible  by  means  of  square  roots  alone.  Hence,  in 
order  that  the  roots  of  the  biquadratic  may  be  expressible  by 
means  of  square  roots  alone,  it  is  necessary  that  the  cubic 
resolvent  should  have  a  commensurable  root,  which  can  always 
be  found  as  explained  in  §  4.* 


See  also  Ex.  xlv.  (21). 


552  APPENDIX 

This  condition  is  obviously  sufficient ;  for,  if  we  use  the  value 
of  A,  then  a,  /?,  y,  8  will  all  be  expressible  by  means  of  a  single 
square  root  (see  chap,  xii.,  §  13),  viz.  J{p2 -  i(q-  X)};  and  each 
of  the  two  quadratics  (6)  will  be  soluble  by  means  of  an  addi- 
tional square  root.  The  expression  for  a  root  will  in  general 
be  a  quadratic  irrational  of  the  second  order  of  the  form 
A  +  \\B  +  sJC),  where  A,  B,  C  are  rational  functions  of  the 
coefficients ;  but  in  particular  cases  it  may  reduce  to  the  simpler 
form  A  +  \/B  +  \/C  +  D  \/B  \/C  ;  or  it  may  happen  that  two 
or  four  of  the  roots  may  be  commensurable. 

§  14.]  If  a  biquadratic  be  reducible,  it  may  reduce  (i.)  to  a 
linear  equation  and  a  cubic  ;  (ii.)  to  two  quadratics  ;  (iii.)  to  two 
linear  equations  and  a  quadratic  ;  (iv.)  to  four  linear  equations. 

It  should  be  noticed  as  regards  a  biquadratic  that  reducibility 
and  solubility  by  means  of  square  roots  (i.e.  by  means  of 
quadratic  equations)  alone  are  not  the  same  thing.  For  example, 
a  biquadratic  may  have  one  commensurable  root,  and  its  other 
roots  may  be  the  roots  of  an  irreducible  cubic.  Again, 
(x2  +  3x  +  l)2  -  2(2/  -  2x  +  l)2  =  0  is  evidently  soluble  by  means 
of  square  roots ;  but  it  is  not  reducible,  for  we  cannot  factorise 
the  characteristic  without  introducing  the  surd  \/2. 

§  15.]  There  is  another  way  of  solving  a  biquadratic  which  is 
often  convenient  in  practice.  Suppose  the  biquadratic  reduced 
to  the  form 

x4  +  qx2  +  rx  +  s  =  0  (1). 

Then  xx  +  x2  +  xii  +  xi  =  0  ;  and  we  can  reduce  the  characteristic  to 
the  form 

{x2  -  (a,  +  x2)x  +  x1x2}{x2  +  (a;,  +  x2)x  +  x3x4]  (2). 

Hence,  if  Ave  put 

«,  +  .'-o  =  s/p,  xxx2  =  (3-  Jyp,  x&t  =  (3  +  sfyp  (3), 

we  have 

(/'  +  p)2  -  p(x  +  yf  =  x*  +  qx2  +  rx  +  s  (4 ).  * 

Therefore 

2P-P  =  q,  -2py  =  r,(32-py2  =  s  (5), 

which  are  equivalent  to 

(B  =  (q  +  P)/2,     y  =  -  r/2p  (6) ; 

*  The  whole  of  the  present  process  is  a  natural  application  of  the  last 
remark  in  §  9. 


APPENDIX  553 

together  with 

p3  +  2qP2  +  (q2  -  4s)P  -  r2  =  0  (7), 

which  is  Descartes'  Cubic  Resolvent. 

"When  any  root  of  (7)  is  known,  the  values  of  /3  and  y  are 
given  by  (6)  and  the  roots  of  the  biquadratic  are  given  by 

x2  -  \fpx  +  (3-  Jyp  =  0,  X2  +  s/p  X  +  f3  +  Jyp  =  0       (8). 

As  before,  the  necessary  and  sufficient  condition  for  solubility 
by  means  of  square  roots  is  that  the  resolvent  shall  have  at  least 
one  commensurable  root. 

Cor.  1.  The  roots  of  Descartes'  resolvent  are  three  of  the  six 
quantities 

(.r1  +  a-2)2,    (^  +  .r3)2,    (»,  +  x4)2,    (x3  +  xt)2,    (x2  +  x4)2,    (x2  +  x3)2, 

which  are  equal  in  pairs. 

Cor.  2.  If  the  biquadratic  be  reducible  to  two  quadratics,  one  of 
the  roots  of  Descartes'  resolvent  must  be  a  perfect  square;  and  this 
condition  is  sufficient. 

§  16.]  If  the  solution  of  a  geometric  problem  be  expressed  by 
a  series  of  equations,  the  necessary  and  sufficient  condition  for 
solubility  by  means  of  the  ruler  and  compass  alone  is  that  these 
equations  either  are,  or  are  replaceable  by  a  series  of  linear  and 
quadratic  equations  (see  Introduction,  §  240).  The  foregoing 
considerations  often  enable  us  to  settle  the  possibility  or  impossi- 
bility of  such  a  solution.  For  example,  the  abscissa,  or  ordinate, 
of  the  intersection  of  two  conies  is  in  general  the  root  of  a  bi- 
quadratic equation  :  hence  the  intersections  of  two  conies  cannot 
be  constructed  by  the  ruler  and  compass  alone,  unless  the  cubic 
resolvent  of  this  biquadratic  have  a  commensurable  root. 

Exercises  XLV. 

(1.)  Prove  that  the  biquadratic  x4+px3  +  qx2  +  rx+s  =  0  is  soluble  by- 
square  roots  if  j)3-4^  +  8r  —  0. 

(2.)  Discuss  the  Lagraugian  resolvent  of  x*  +pxs  +  qx2  ±px  + 1  =  0. 

Solve  the  following  biquadratics  : — 
(3.)  .T4+10a;3-l-22.'c2-15a;  +  2  =  0. 
(4.)  a;4  +  10a;3-l-35.r2-t-  50* +  4  =  0. 

(5. )  x4  +  2{p  -  q)x3  +  {p2  +  q2)x2  +  2pq(p  -  q)x  +pq(p2  +pq  +  q~)  =  0. 
(6.)  2a;4-ar5-9x2  +  4x  +  3  =  0. 


554  APPENDIX 

(7.)  2*4 -far5 -3a;2 -So; -12  =  0. 
(8.)  2zA  +  5x3  +  6x-  -a?-6=0. 
(9.)  2cc4  +  3a;3  +  16ic  +  6  =  0. 

(10.)  xi-4xs-4x2  +  16x-8  =  0. 

(11.)  x4-6a;2+8a;-3  =  0. 

(12. )  If  an  equation  of  the  special  integral  form  of  §  2  reduce  to  equations 
of  lower  degree,  prove  that  each  of  these  equations  is  also  of  the  special  in- 
tegral form  (see  Weber's  Algebra,  §2). 

(13.)  Show  that,  without  solving  equations  of  higher  degree  than  the 
second,  we  can  determine  a,  j3,  y  so  that  the  substitution  y  —  a  +  fix  +  yx2 
shall  transform  any  cubic  equation  into  the  form  y's  +  A  —  0. 

(14.)  Show  that,  without  solving  equations  of  higher  degree  than  the 
third,  we  can  determine  a,  /3,  y,  5  so  that  the  substitution  y  =  a  +  /3x  +  yx"  +  5x* 
shall  transform  any  biquadratic  into  the  form  2/4  +  A?/2  +  B  =  0. 

(15.)  Show  that  ^/{r/2  +  sJ(r2/4  +  q3/27)}  is  expressible  in  the  form 
%+s/y  where  x  and  y  are  rational,  when,  and  only  when,  the  cubic 
x3  +  qx  +  r  =  0  has  a  commensurable  root.  What  bearing  has  this  on  the 
solution  of  a  cubic  equation  ? 

(16.)  Show  that  one  root  of  Descartes'  resolvent  of  the  biquadratic 
xi  +  qx2  +  rx  +  s  =  0  is  always  real  and  positive;  and  that  the  roots  of  the 
biquadratic  are  1°  all  real,  if  the  other  two  roots  (p2,  p3)  of  the  resolvent  are 
both  real  and  positive  ;  2°  all  imaginary,  if  p2  and  p3  are  both  real,  negative, 
and  unequal ;  3°  two  real  and  two  imaginary,  if  p<i  and  p3  are  both  real, 
negative,  and  equal,  or  if  p2  and  p3  are  both  imaginary. 

(17.)  If  the  roots  of  Lagrange's  resolvent  be  all  real  and  unequal,  show 
that  the  roots  of  the  biquadratic  are  either  all  real,  or  else  all  imaginary  ; 
and  that,  if  only  one  root  of  the  resolvent  is  real,  then  two  roots  of  the 
biquadratic  are  real  and  two  imaginary. 

(18.)  Show  that  a  regular  heptagon  cannot  be  inscribed  in  a  circle  by 
means  of  the  ruler  and  compasses  only  (see  Ex.  xxxii.,  33). 

(19.)  Show  that  the  inscription  in  a  circle  of  a  regular  polygon  of  11 
sides  depends  on  an  irreducible  quintic  equation. 

(20.)  Show  that,  if  A,  B  be  two  given  points  in  a  straight  line,  we 
can  by  the  ruler  and  compass  alone  find  a  point  on  the  line  such  that 
AP  +  BP:AP-BP  =  AP3:BP3. 

(21.)  Starting  from  the  remark  at  the  end  of  §  8,  prove  that,  if  a 
biquadratic  equation  be  soluble  by  square  roots  alone,  then  its  Lagrangian 
resolvent  must  have  at  lease  one  commensurable  root. 

(22.)  Show  that,  if  the  roots  of  the  biquadratic  x4  +  qx2  +  rx  +  s  =  0  be 
rational  functions  of  two  quadratic  surds,  then  the  cubic  y'i-4qy2  + 
4(q'-  -  4s)y+8r2  =  0  must  have  a  commensurable  root,  say  y  =  m;  and 
(q/2  -  m/8)2  +  r2/2m  must  be  the  square  of  a  rational  number.  Are  these 
conditions  sufficient  ? 


RESULTS    OF    EXERCISES. 


I. 

(5.)  1st.  The  number  of  digits  is  34  ;  for  the  best  approximation  the  first 
three  digits  are  126.  2nd.  The  number  of  digits  is  20  ;  the  first  three  184. 
(6.)  -1,  +1.  (7.)  a -b.  (8.)  1707  ;  30521/415800.  (9.)  6.  (10.)  aa  +  Zab 
+  bb;aa-bb;  9aa-36bb;  laa-^bb.  (11.)  2(mm-  l)cta  +  2{nn-  l)bb.  (12.) 
2xy  +  2/xy.     (13. )  2yz/x  +  2zxjy  +  2xyjz  +  2jxyz.     (14.  )\xx  +  \zx-  ^yy  +  fazz. 

II. 

(1.)  1/24.312.5  =  1/42515280.  (2.)  The  second  is  greater  by  65280.  (3.) 
1/2.  (4.)  16«W-.  (5.)  <?/aliVii*yu.  (6.)  (81/16)aW2.r2.  (7.)  j/V/a:5. 
(8.)  (xyz)49.  (9.)  1.  (10.)  nP+i-°-r.  (11.)  asl*-*) (*-«>.  (12.)  l/xi'^2.  (13.) 
1.  (15.)  i+x2"-l'-c-x-2a+>*<:  +  x-a+2<>-c  +  xa--b+c-x-a-b+2c  +  xa+i-2c.  (16.) 
ap+2?  +  2ar+«/br  +  aP/b2P  +  cfo/bi  +  2atjbP+i  +  l/b2r+*. 

III. 

(1.)  x  +  y.  (2.)  1.  (3.)  (x2-y2)/xy.  (4.)  y.  (5.)  l/bc(-a  +  b-c).  (6.) 
(a*-a2b2  +  2aV-bi)/(a2-b2).  (7.)  ixy-/(x* -y*).  (8.)  2(b2x2  +  a2y2)/abxy. 
(9.)  abl(a?  +  bn~).  (10.)  a2-  b2.  (11.)  -  (4*+2a?)/(l  +x2  +  xi).  (12.)  1.  (13.) 
1.  (14.)  The  function  is  =1.  (15.)  (adf-ae)/(bdf-  be-cf).  (16.)(a2-4a& 
+  ib2  -  l)/(a3  -  6a?b  +  I2ab2 -  Sb3  -2a  +  ib).     (17. )  (a2  -b2  +  l)/(a2 -  b2  +  2). 

IV. 

(7.)  2.33.7.112;  35.52.72.     (8.)  53. 

V. 

(1.)  120.  (2.)  x*-2x4y*  +  y8.  (3.)  Xs -ys.  (4. )  x*  -  3aV  +  3a V  -  i/. 
(5.)  x8-16^i/2  +  96r1!/4-256a;V  +  256^.  (6.)  JV-64c2  +  c2a4-c4a2  +  rt261 
-tf*i>.  (7.)  a-6  +  3^5  +  6x-4  +  7^3  +  6x2  +  3x+l.  (8.)  27a3 +  863-  1  +  54a2b 
+  36ab2  -  12b2  +  66  +  9a  -  27a2  -  36a&.  (9. )  x*  +  2a?  +  Zx2  +  4x  +  5  +  4/x  +  3/x3 
+  2/xs+l/xi. 

(10>  )  +  a4  +  64  +  c4  +  4a3&  +  4a  J3  +  4J3C  +  4&c3  +  4ca3  +  4c3a  +  6a2J2 

+  66V  +  6c2a2  +  12a26c  + 1 2ab2c  + 1 2«6c2  ; 

+     +     +     -         -         +        +         --         + 
+  +  + 

(11.)  Four  types;  3  like   xi ;    6  like  a.-3//;  3  like  x2yz  ;  3  like  x2y2.      (12. ) 


556  RESULTS  OF  EXERCISES 

Three  types;  4  like  a3;  12  like  a2b  ;  4  like  abc.      (13.)  (2  +  3  +  4^  =  729. 

(14.)  a;2/(62-c2)  +  &c.+&c.+2(ca-a&)2/2/(a2-62)(c2-«2)  +  &c.+&c.  (15.)  2(a;2 
+  y2  +  z2).  (16.)  0.  (17.)  ax  +  by  +  cz.  (18.)  -2a6  +  22a5&  +  2a4&2-102a4&c 
-42«3&3  +  82a3&2c-18a2&2c2.  (22.)  abc.  (23.)  3a6c.  (24.)  2(&3c-fc3  +  c3a 
-ca3  +  a36-a&3).  (25.)  (a2-&2)af»  +  2a&2arV  +  (2a2  +  2&2-  a2b2)x2y2-2ab2xy3 
+  (a2-b2)y\ 

VI. 

(l.)(«)2nd.  (/3)  Fractional.  (7)  4th.  (3)  2nd.  (2.)  2a;2  +  10a?  +  14.  (3.) 
fx2  +  |a;.  (4. )  9a*4  -  78a;2  + 121.  (5. )  x6  -  a:42a2  +  a;22a262  -  aW.  (6. )  x6  - 
(p2  +  q2+l)xi+(p2q2+p2  +  q2)x2-p2q2.  (7.)  xi0-15xsy2  +  85xsyi-225xitf  + 
274x2y9  -  120tj10.  (8. )  a&ca;3  -  (b  -  c)  (c  -  a)  (a  -  b)x2y  +  (2a26  -  2a3  -  3abc)xy2 
+  (b-c){c-a){a-b)y3.  (11.)  (b'2-c")xi  +  2c(b-a)x3+(c-a)(c  +  a-  2b)x2  + 
2a{c-b)x  +  (a2-b2).  (12.)  a-8- a6- a;2 +  1.  (13.)  4a?  +  10arV  +  8a;?/2  +  3?/3.  (14.) 
ixi-xhj2  +  ±yi.  (15.)  a;12-2a;6  +  l.  (16.)  a-12  +  2aJ0  -  a8  -  4a6-a;4  +  2a:2+l. 
(17.)  T%x6-ixi  +  -^x3-^\x2  +  -ij:.  (18.)  ax6-a{a  +  b)x5y  +  b(2a2  +  l)xitj2-a2b2xsy3 
+  ax2yi-b(a-b)xy5  +  by6.  (19.)  4a6+12a2a;4  +  12&4a-2.  (20.)  a;24-12a2x22 
+  66a4ar°  -  220a6x18  +  495a8 a;16  -  792a10a-14  +  924a12a12  -  &c.  (21. )  a'12  -  3a8a5 
+  data™  -  a15.  (22.)  2187a? +  1701a'6  +  567a5  +  105a^  +  ^x3  +  |a? + ^x + ^Vr- 
(23.)  a8  +  8a7&a2  +  28a6&2a;4  +  56a5&3a*i+70a4&4a;8  +  &c.  (24.)    ^-Qx^tf 

+  36.r8V2  -  84a:7V8  +  126a;60j/24  -  &c.  (25. )  1  +  3a;  +  6a;2  +  10a-3  +  15a-4+  18a-5 
+  19a?  +  &c.     (26.)  266.     (27.)  -1975.     (30.)  320. 

VII. 

(1.)    360a-4 +1 782a*5  +  3305a;2  +  2722a:  +  840.  (2.)    pqrx3  -(q-r)(r-p) 

(p-q)x2+(-2p3  +  -2p2q-Spqr)x+(q-r){r-p)(p-q).  (3.)    Xs  -  30a2 a-6 

+  273a4a4--820a6a:2  +  576a8.  (4.)  a6- 3a-4  +  3a-2-l.  (5.)  ix6  +  U^  +  U^A 
+  H W  + 1 ^2  +  &  +  !•  (6. )  a;6  -  &.  (7. )  a-«  +  (2Z2/»m)  x5  +  22(mnJP)  x*  +  (l 
+  l3lm3  +  m3jn3  +  n3/l3) x3  +  2(2Z2/mn) x2  +  (2mn/P)x  +  1.  (8. )  2048a;11  -  33792a;10 
+  253440a9  -  1140480a;8  +  3421440a;7  -  7185024a;6  +  10777536a-5  -  11547360a-4 
+  8660520ar>- 43302603?  +  1299078a;  -177147.  (9.)  x24  +  8x21y3 +  28x18y6 
+  56aJV  +  70a1V2  +  &c.  (10.)  a;18+  10a-17  +  41a:16  +  80a15  +  36a14  +  168a;13 
-  364a;12  -  208a;11  +  286^°  +  572a;9  +  &c. 

VIII. 

(1.)  A  +  B2a;  +  C2a;2  +  D2a;2/  +  E2a?  +  F2a22/  +  G2a-^.  (2.)  ZoY+Xetya 
+  Zx2y2z2.  Three  types  present,  four  missing,  viz.,  a-6,  x5y,  a*4?/2,  oPy'h.  (3.) 
^x-^y.  (4.)  P {(y" - y')  (a- -a') -(a" -x')  (y -y')},  where  P  is  any  constant. 
This  may  also  be  written  P {(y" -  y') x -  (x" -x')y  +  x"y'  - x'y") .  (5. )  (y'x - x'y) 
{y"x-x"y)l{x'-y'){x"-y").  (6.)  A=  -8,  B=  -12,  C=20.  (7.)Z=21, 
m=-76,  ?i  =  60.  (8.)  7=6,  m=  -15,  «  =  10.  (9.)  2P(a- - b)  (x - c)  (x - d)/ 
{a-b){a-c){a-d).     (10.)  b3c3  +  /A-2  +  b5c,  b3c3  +  b2c*  +  be5.     (11.)  32ar5-2a2!/. 

IX. 

(1.)  Q=a?-3a:2  +  3a:-l,  R  =  0.        (2.)  Q=3a!*+V^-¥«2+¥*-&,    R 

=  t^-tI-  (3.)  Q  =  4a3  +  6a?+lla+16,  R  =  20a--15.  (4.)a;2-9.  (5.] )  The 
function  =  a-3-2a:2  +  17a;  +  80-40/(a;-7).      (6.)  Q  =  a3-5a-  +  3,  R  =  0.      (7.)  Q 


ax 


RESULTS  OF  EXERCISES  557 

=  9x*  +  6x'i  +  xS  +  2x  +  l)  R  =  0.  (8.)  Q  =  a;2-  8a;+15,  R  =  0.  (9.)  Q=x3+)ix2 
+  &  +  1  R  =  0.  (10.)  Q  =  a;2-fa;  +  -y-,  R=_J^aj-ff.  (n.)  Q^a;6-^ 
+  i*4  -  A*8  +  ttV*2  -  -hx  +  tIts,  R  =  0.  (12.)  as  - 1.  (13. )  aV(*6  +  x?y  +  xhj2 
+  .  .  .+y6).  (14.)  3a2-2ab  +  b2.  (15.)  a6  -  a5b  +  a4b2  - .  .  .+bs.  (16.)  x1 
-Bxy  +  y2.  (17.)  aj2  -  2xy  +  ty2.  (18.)  x3  +  x2y  +  3xy2  +  3?/3.  (19.)  l+a;  +  x2 
+  .  .  .+x9.  (20.)  ct'1-c»3-a32-2a;  +  4.  (21.)  bx2  +  cx-f.  (22.)  a&  +  ac-Z>c. 
(23.)  1+6  +  c.  (24.)  2{a  +  b)x.  (25.)  a4 - a?b  +  Za2b2 - ab3  +  bK  (26.)  8xy(x2 
+  y2).  (27.)7xy(x  +  y).  (28.)  Q  =  6ar*  +  9a;2  +  5a;  + 1,  R=  -  1.  (29.)  (bx  +  mj)/ 
(bx-ay)  =  l  +  2ay/(bx-ay)—  ~l  +  2bx/(bx-ay).  (30.)  If  a  be  variable,  the 
transformed  result  is  a?  +  2a26  +  5a&2  +  1063  +  (15«&4'-  1365)/(a2-  2a&  +  &2).  (31.) 
Q  =  ars-2a;2  +  x-4,  R=12.       (32.)  tf  +  Zx2-  13a;-  15.      (33.)  -303/8.      (34.) 

%(p+q);  p+q=o.     (35.)  aq2-bpq  +  cp2=o.     (36.)  p2-a1)-q+b=o, 

pq-aq  +  c  =  0.  (38.)  X=l,  /i=-3,  y=-2.  (39.)  _p  =  2,  g-=3,  r  =  3.  (40.) 
The  remainder  in  each  case  is  ra  +  s.     (41.)  m  +  1  must  be  a  multiple  of  n  +  1. 

(42.)  l-te+fc#-27aM-.  .  .  +(  -  3)»a--(  -ZyWftSx  +  l) ;   A-J^+J-g 

+  x2).  (44.)  l  +  2ai  +  5a;2/l. 2  +  16^/1. 2. 3  +  65^/1. 2.3.4  +  .  .  .  («.)l-»y; 
1  +  ny.  (50. )  a;5  -  70a?  -  377a;2  -  778a;  -  585.  (51. )  P8  -  4P7  +  2P6  +  8P5  -  5P4 
-8P3  +  2P2  +  4P  +  1,  where  P  =  a;  +  2;  Q4  +  (8a;  +  24)Q3  +  (8a:-40)Q2  +  (  -32a; 
+  16)Q  +  16;c,  where  Q=a;2  +  a;  +  l. 

X. 

(l.)ar»-l.  (2.)  aP-x+ 1.  (3.)  No  CM.  (4.)a;+l.  (5. )  x2  +  x  -  6. 
(6.)  x2  -\2x  +  35.  (7.)  x2  -16a;  -15,  use  §  7.  (8.)  x*  +  x2-  6  ;  compare  with 
Example  5.  (9.)  %*-  3a;-2.  (10.)  a?- 1.  (11.)  4a;2  +  3a;+l.  (12.)  a; -5. 
(13.)  4a;2 -24a; +  35.  (14.)  x2  +  2x+l.  (15.)  x2  +  4aa:  +  8a2.  (16.)  3a;2- 
sj2x+l.  (17.)as-l.  (18.)  a:2-«a;  +  2a2.  (19.)  (x- 1)2.  (20.)  The  G.C.M. 
would  be  a  measure  of  (2)-q)x(x-  1),  neither  of  the  factors  of  which  is  in 
general  a  measure  of  either  of  the  given  functions.  If,  however,  p  +  q  +  2  =  0, 
then  x  —  1  is  a  measure  of  both.  (22. )  a  —  8,  there  is  then  a  factor  x2  -  4x  +  3 
common  to  numerator  and  denominator.  (23.)  Use  §  7.  (25.)  Use  §§  6 
and  7  ;  the  first  gives  the  conditions  in  the  first  form,  the  second  gives  the 
single  condition.  (26.)  P  =  ^  +  -rr>  Q=-/Ta-'  +  ir-  (27-)  ?  =  &%  +  &, 
Q=-Jrx  +  i\.  (28.)  a\a -b){a  +  b) (a2  +  b2) (a4  +  64).  (29.)  («-l)(a:-2) 
(x-  3)  (x  +  2)  (x  +  4).  (30.)  (a;-l)(a;  +  l)(a;  +  2)(3a;-2)(3a;  +  2).  (31.)(ar-l) 
(a;-2)2(s;  +  4)(a;  +  5)(a:2-5).     (32.)  The  product  of  the  given  functions. 


XI. 

(1.)  2{a-d)(a  +  b  +  c  +  d).  (2.)  (a  +  b  +  c)  (  - a  +  b  +  c)(a-b  +  c)  (a  +  b-c). 
(3. )  (a2  -  3c2)  (a2  -  4b2  +  c2).  (4. )  i(x  +  2  +  *j2i)  {x  +  2-  ^2i)  {9x  -  13  +  sJ7) 
(9x-13-V7).  (5.)  (a-/3)(2a;-a-/3)(a;-7)2.  (6.)  (x  +  y)(x-y){x- 


558  KESULTS  OF  EXERCISES 

(x  +  y)(x -y)(x  +  iy) (x  -  iy) {x +y(l  +  i)/^2}  {x  + 1/(1  -  i)f*j2)  {x - y{\  +  i)/s/2} 
{x-y(l-i)/^2}.  (8.)  (x  +  Zy+2)(x  +  By-2).  (9.)  2(aj  +  2)(aj-i).  (10.) 
(x+8)(x-2).  (ll.)(^-5  +  V7)(a;-5-V7)-  (12.)  (a: +  6)  (a: -5).  (13.)  {x  +  7 
+  i\f7)(x  +  7-W7).  J14.)  (x  +  2+js/3)(x  +  2-i^S).  (15.)  2(a-  +  4)(a:-f). 
(16.)    (x+\/p  +  q  +  \/p-q)(x+\/p  +  q-\/p-q).  (17.)    (x-l){x-(b- c)/ 

{b  +  c)}.  (18.)  (x+p)(x  +  q)(x-p)(x-q).  (19.)  {ax- by)  (bx  +  ay).  (20.) 
{(l-p)x-(l+p)y\{(l-q)x-(l  +  q)y}.  (21.)  [x- B)  (x- 5)  (x-7).  (22.) 
a;(a;-7  +  3iVll)(^-7-3iVll)-  (23.)  (a -3) (a; -4) (a; -6).  (24.)  (x-  8)(x  +  i) 
(x-i).  (25.)(x+p)(x  +  p  +  q)(x+p-q).  (26.)  (x  +  l)(x -l){(p  +  q)x+ (p-q)}. 
(27.)  (x-l)(x-p)(x-p2).  (28.)  (x- a)  (x-b)(x+ \fab)(x-\/ ab).  (29.) 
(a:4  -  a4)  (a;2  +  xa  +  a2)  =  &c.  (30. )  2(x  -  y)  (1  -  xy).  (31. )  (a;2  +  xy  +  y2)  (x2  -  xy 
+  y2)  =  kc.  (32.)  p=  +V2»  9=  ~  V2-  (33.)  (a:2  + V2^  +  ^2-l)  (a:2- V2iC2/ 
+  2/2-l).  (34.)  r=  -jm2,  s=  -qa2-ai.  (35.)  (xm  +  am)  (xm  -  am)  (xn  +  an) 
(xP-a").  (36.)  3a2ai2(a;2  +  ax  +  a2)(a:2-aa;  +  a2)  =  &c.  (37.)  (x-l)(y-l)'\ 
(38.)  (a;+ 3)  (2x+y  +  l).  (39.)  (2aj  +  3y  +  l)(oj-y-l).  (40.)  (aj+3)  (y+7). 
(41. )  (a;  +  2i/  -  2)  (x  -  y  +  3s).  (42. )  Equate  the  discriminant  of  the  function  to 
zero  and  thus  obtain  a  cubic  equation  for  X.  (43.)  When  c  =  0,  \  =  (af2  +  bg2 
-2fgh)lfg.  (44.)  a((3'y"  -  (3"y')  +  l3(y'a" -y"a')  +  y(a'p' -a"p')  =  0.  (47.)  (a 
+  b  +  c)(a2  +  b2  +  c2-bc-ca-ab).  (48.)  (x+y-a)(x2  +  y2  +  a2-xy  +  ax  +  ay). 
(49.)  Zx(x  +  l)(x-l)3.  (50.)  -CZx2  +  -2yz)(y-z)(z-x)(x-y).  (51.)  (as  +  y 
+«) (y -«)(«- a) (aj-y).  (52.)  -(jr+a)(z+a;) (x+y)(y-z)(z-x)(x-y).  (53.) 
3(y  +  2)  (2  +  a;)  (a:  +  y).     (54. )  -  1. 

(60.)  If  p2  =  -2(y-2)(2-a;)  =  2(2a;2-2a;2/), 

and  p3  =  (y-z)(z-x)(x-y),     sn='Z(y-z)n, 

then  it  may  be  shown  (see  chap,  xviii.,  §  4)  that 

s6m+1  =  Ap3p2Sm-1  +  Bps3p2s(m-V-1  +  .  .  .  +  Lp32m-W, 

s6m-1  =  A2}3p2Sm'2  +  Bpsspi{m-1}-2  +  -  •  •  +  Lpg2™-1^, 

where  A,  B,  .  .  .,  L  are  numerical  coefficients.     Hence  the  theorem  follows. 

XII. 

(1.)  (a;  +  3)/(a;2  +  a;-2).  (2.)  (9a:2 -a;-  8)/4(aj  +  5).  (3.)  (2a: -  3)/(a;2 -  3a; 
+  2).  (4.)2(a;2  +  l)/(a:2-l).  (5.)  2a?  +  6x*  +  2.  (6.)  (2x  +  5a)/(Zx  +  5a).  (7.) 
l/(l-x2).  (S.)(w  +  x-y)/{w+z-y).  (9.)  1/(1 -a3).  (10.)  (l2  +  m2)l(p2  +  q2). 
(11.)  -sit.  (12.)  y/2(x-y).  (13.)  2(«  +  bx)/(a2 -  b2)  (1  - x2).  (14.)  («2 -  iab 
+  <Lb2-l)/(as-6a2b  +  12ab2-8b*-2a  +  4b).  (15.)  (6  +  a-)/3(l -a;2).  (16.)  0. 
(17.)  l/(2.r2-l).  (18.)  (240a^+32a:)/(81a^-16).  (19.)  (3a;+2)/a:(a;  +  l)3. 
(20.)  a*2/(a:-l)(a;+l)3(a:2  +  a;+l).  (21.)  l/(a:  +  l)2.  (22.)  4«a-(-&a;  +  a2)/ 
(a^-a4).  (23.)  (Bx2  +  y2)(x-y)/(x  +  yf.  (24.)  (x  +  2)  {x2-  l)/(x2  +  x  +  l)  (x2 
+  x-A).  (25.)  x/8a.  (26.)  4a'V/(a:6  -  2/6).  (27.)  -1.  (28.)  (203!  +  ^  +  a2)/ 
(a2-c2)(a:2-a2)(a:  +  c).  (29.)  1.  (30.)  (x-l)(y -l)/(x+l)  (y +  1).  (31.) 
l+yS+tf-y-z-ya  (32.)  (a  +  b  +  c)/(a  -  b  -  c).  (33.)  -  3.  (34.)l/(a:2-a2). 
(35.)  (a -&«)/(« +  &c).  (36.)  2(a<3  -  l)/{(x-  l)2-  y2}.  (37.)  (x°-  +  y2)2.  (38.)  1. 
(39.) -2.  (40.)  2a?/xyz.  (41.)  0.  (42.)  A.  (43.)  0.  (44. )  1  -  2a:2  +  2xyz.  (45.) 
2.  (46.)  0.  (47.)  0.  (48.)  0.  (49.)  (h  -p)  (h- q)/H(h  +  a).  (50.)  h2/U(h-  a). 
(51.)  -Jrjn(h2  +  a2).       (52. )  -  2Xx/xyz.      (53.)  1 -a-b- c.       (54.)  1.       (62.1 


RESULTS  OF  EXERCISES  559 

l-3/(a;-2)  +  8/(aj-3).  (63.)  l/2(« - 1)  -  i/(x -  2)  +  9/2(« -  3).  (64.)  30x-5/ 
(a?+l)-5/(a!-l)  +  80/(aj  +  2)  +  80/(a!-2).  (65.)  17/36(a?  +  lJ-  5/6(x+l)2  +  8/45 
(»-2)-13/20(a:  +  3).  (66.)  (4x  +  5)/3(ar  +  a;+l)  -  1/S{x-  1).  (67.)  1/2(8+1) 
+  (a:  +  l)/2(x2  +  l).  (68.)-l/4(a:-l)  +  (z  +  l)/4(a;2  +  l)  +  (2:  +  5)/2(a;2  +  l)2.  (69.) 
l/(a-b)  (a2-2pa  +  q)  (x-a)  -  l/(a-b)  {b- -  2pb  +  q)  {x-b)+{(a  +  b  -  2p)x  + 
(2p-a)(2p-b)-q}/(a2-2pa  +  q)  (b2-  2pb  +  q)  (x2-  2px  +  q).  (70.)  3/4(a:-l)2 
-3/8(it--l)  +  l/8(a;+l)  +  (a;-l)/4(a:2  +  l).  (71.)  2/(x+l)  +  3/(x+l)2- (2x-3)/ 
(x2-2x  +  S).  (72.)  l/(z-l)-l/2(z  +  l)-(a;  +  3)/2(a;2  +  l).  (73.)  -1/x+l/x2 
-l/x3+l/8(x-l)  +  9/8(x+l)  +  l/i{x+l)2-(x  +  l)/i(x2  +  l).  (74.)(3a;2  +  a;  +  l)/ 
2(^-l)-(3a;2  +  £f  +  l)/2(a;4  +  l).  (75.)     l/6  +  S{*l/15.3n  +  (  -  l)"/10.2»}a;n. 

(76. )  1  +  JS  { (n  +  2)xn  +  ( -  1  fx2^1} . 


XIII. 

(1.)  100242.  (2.)  22-6354.  (3.)  267 '3861249.  (4.)  2653919.  (5.) 
788001.  (6.)  20200-1122212  ..  .  (7.)  -204.  (8.)  1  +  1  x  3  +  1  x  3.5  +  3  x  3.5.7 
+  3x3.5.7.9.  (9.)  l/2!  +  0/3!  +  3/4!  +  l/5!  +  2/6!  +  l/7!  +  2/8!  +  l/9!  +  6/10! 
+  4/11!.*  (10.)  l/3  +  0/3.5  +  l/32.5  +  3/32.52  +  l/33.52  +  4/33.53  +  l/34.53+ .  .. 
(11.)  2466411243.    (12.)  100-1431.    (13.)  127«50.    (14.)  18 "355.     (15.)1-| 

111  1  1 


5.47  5.47.50  5.47.50.367  5.47. 50. 367. 551  5.  47.  50. 367.551. 1103 
(16.)  1  +  2  +  25.  (17.)4.1  +  1.5  +  1.52  +  1.53  +  1.54;-l  +  2.5  +  1.52  +  1.53+1.54. 
(18.)  831'80f".  (19.)  300'64".  (20.)  53-617  cubic  ft.  (21.)  11'9#".  (22.) 
r=7.  (23.)r=4,  &c.  (24.)  503.  (25.)  x(x+l)(x  +  2)  (z  +  3)  +  l  =  (z2  +  3a:+l)2. 
Since  x=10m+p  where  7;  =  0,  1,  2,  .  .  .,  9,  we  have  only  10  different  cases  to 
consider.  It  will  be  found  that  the  last  digit  is  5  when^=l  or  =6  ;  in  all 
other  cases  the  last  digit  is  1.  (28.)  Since  2^(10r~10s)  =  2^10s(10r-«- 1)  is 
always  divisible  by  10-1  =  9.  (31.)  Since  10"  and  all  higher  powers  of  10 
are  divisible  by  2",  it  follows  thatjp0+.Pil0  +  .  .  .  +  j0n_1lOn~1  must  be  divisible 
by  2".  (32.)  j0o+i>ilO+p2lO2=2>o  +  2pi  +  4^2  +  8(;>i  +  12p2)  must  be  divisible 
by  8,  therefore,  &c.  (34.)  If  the  digits  in  the  period  of  p/n  be  qi,  qi,  .  .  .,  qs, 
those  in  the  period  of  1  -p/n  are  9  -  qh  9  -  q2,  .  .  .,  9-qs-  (36.)  Since  any 
number  may  be  written  11m +p  where  p  =  0,  1,  .  .  .,  10,  we  have  merely  to 
show  that  05,  l5,  25,  .  .  .,  t5  all  end  in  one  or  other  of  the  digits  0,  1,  r. 
We  proceed  to  test  thus  :  92  ends  in  4  ;  therefore  94  ends  in  5  ;  therefore  95 
ends  in  1  ;  and  so  on.  (38.)  pqrpqr  =  (101i+l)])qr=7.11.1B.pqr.  (39.)  03  ends 
in  0,  l3  in  1,  23  in  8,  33  in  7,  43  in  4,  53  in  5.  Hence  the  theorem  ;  for  every 
number  can  be  written  lOwidbp,  P>§-  (40.)  I2=(12?;i+^>)2,  hence p  =  0 
or  6.  The  latter  only  is  admissible.  Hence  I2  =  (12m  +  6)2  =  0  +  3.12  +  ya.l22; 
I3=(12m  +  6)3  =  0  +  6.12  +  i>.122.  (41.)  TS-po-pia- '.  .  .  - pn^a"-1  -  (pmam 
+pm+iam+1+  .  .  .)=2h{r-a)+2h{f2-a2)+  .  .  .  =  /x(r  -  a)  =  fxam  ;  therefore,  &c. 
(42.)  <p{a)  is  simply  the  result  of  casting  out  the  nines  in  the  sum  of  the 
digits  of  a,  that  is,  <p(a)  is  the  remainder  when  a  is  divided  by  9.  Hence,  &c. 
(43. )  We  must  have  2xr2  +  2yr  +  2z  —  zr2  +  yr  +  x;  whence  (2x -  z)r  +  y  +  (2z~x)/ 

*  3!  stands  for  1.2.3,   4!  for  1.2.3.4,  &c. 


560  RESULTS  OF  EXERCISES 

r  =  0  ;  therefore  (2z-x)jr  must  be  an  integer.  Now  2z-x<2r,  hence  either 
2z-x  =  0  or  =  r.  The  former  can  be  shown  to  be  inadmissible.  The  latter 
leads  finally  to  z  —  2t  +  l,  y=Bt  +  l,  x=t,  r  —  Zt  +  2,  where  t  is  any  positive 
integer.     Hence  the  theorem. 

XIV. 

(1.)  18^/3.  (2.)  1.  (3.)  71/6°.  (4.)  jy(57.331).  (5.)  (a*-s»(»-i)j4+3n(»-i)) 
i/4n(«-i),  (6.)  i.  (7.)  Each  =a;2/"("+1»(»+2).  (8.)  x'2'3  +  x^y1'3  +  y~2'3.  (9.) 
x2  +  2x  +  3  +  2aH  +  x-2.  (10. )  x7'2  -  Sx5'2  +  5x3'2  -  7x1/2  +  Ix-1'2  -  5x-3'2 
+  3x-5l2-x-712.  (11.)  x2  +  x  +  l.  (12.)  x7l10-2x1'5yll2  +  3x9<'lY'5  +  x~moy 
-3x2'5y7'10.  (13.)  x2'3  -  2xliy2  +  2y.  (14.)  2(2^  +  22'3).  (15.)  a*'" 
+  x7/2nyV2n  -  2x3,"y1'n  -  Sx52ny3'2n  +  Za?l2nifl2n  +  2xVny3ln  -  xll2ny7'2n  -  y4'".  ( 20. ) 
{a  +  b)/(a-b).  (21.)  39|  -  6  V3  -  12  V10  +  2\/30.  (22.)  x3  +  (3  -  V2 
-  s/3)x2 +(- 2  -  2^/2- 2^/3 +  2s/6)x  +  (-i- 2^/2 +  2^6).  (23- )  {x-a)l±ax. 
(24.)  (13m2  +  10to+  13  +  12(m-  l)Vr?i2  +  7m  + 1)/(  -  5m2  +  46m -  5).  (25.)  1/q. 
(26. )  0.  (27.)  (j VJP  +  ? V?  +  ? VF^?  -  Vj?g(j>  -  g))fg{p  -  g).  (28.)  2  {(1  -  a;)/ 
(l-4x)}V(l-4a-).  (29.)  {2(a  +  c)2-&2  +  2(ffl  +  c)V(CT  +  c)2-&2}/52.  (30.) 
{-q{p-g)+{p-q)\/pq+p\fq{p-q)-g^p{p-g)}lg{g-p)-  (31.)     22%2 

-(2«»  +  2)sb  +  (2*"-2P»  +  1).  (32.)  a;2-  (21/3  -  l)a;  +  (22/3  +  21/3  +  1).  (33.) 
2b-2sy{(a  +  b)2(a-b)}+23y{(a-b)2(a  +  b)}.  (37.)  (a;  -  2x3'yi  +  2^Y'2 
-2x1>iifii  +  y)/(x-y).  (38.)  -  |{ll  +  6\/3  +  5\/5'  +  4V7  +  4V15  +  3V21 
+  2V35  +  V105}.  (39.)  22a(2a  +  22\/£c)/(2a2-22&c).  (40.)  The  rational- 
ised product  is  31555  -  43.  (41. )  A  rationalising  factor  is  2(3a  -  b  -  c)\J(b  +  c-a) 
-2\J{U(b  +  e-a)}  ;  theresultis  -52«2+62a&.  (42.)  A  rationalising  factor  is 
(2\J5  -  3 V'2)  (V5  +  2  -  V3  +  V6)  5  tne  result  4.  (43. )  A  rationalising  factor 
is  19.22'3  +  22.21/3-  23  ;  the  result  307.  (44.)  The  result  2a3  +  32a26-21a&c. 
(45.)  A  rationalising  factor  is  23/4  +  2.22''4-3.21/4  +  l  ;  the  result  7. 


XV. 

(1.)  A(H\/3  +  3\/ll-\/462).  (2.)  2.  (3.)-2V2-  (4.)12  +  5\/3. 
(5.)  |\/6.  (6.)  14*.  (7.)  ±(V10  +  V15)-  (8.)  ±(1  +  1/V2)-  («•) 
±(11 -V2)-  (10.)  23'4(3  +  131/--).  (11.)  ±i(V6  +  V15)/3.  (12.)  2-V2 
+  2V3.  (13.)  4V2-2V7.  (14.)  3.  (15.)  (3  +  6V3  -  V?  -  2V21)/2  V3' 
(16.)  *V6=  -81649.  (17.)  3-2518293.  (18.)  \/(6  +  2p).  (19.)  *s/{a-e)  +  y/b. 
(20.)  {a+V(«2-4)}/V2-  (210  x/(l-x2).  (23.)  1  +  V(3/2)  +  V(5/2)-  (24.) 
2-V3-3V2-  (27.)  3-2V2-  (28.)  5  +  V18.  (29.)  21'6(3  +  101/2).  (33.) 
3-162277660;  -0632455532.  (34.)  ±(yz-zx  +  xy).  (35.)  ±(5x-3y-x). 
(36.)  ±(SaP  +  4as-l).  (37.)  ±(a:2- 2x- 1).  (38.)  ±(2x2-3xy  +  4Ly2).  (39.) 
±(^-8aH-2).  (40.)  ±(2^-3a!2-a;+4).  (41.)  ±(5p3  +  3p2q-  Spq2-  bq3). 
(42.)  ±(x-V*+l).  (43.)  (2ar»-aj8-3).  (44.)  {(3±  V3)p  +  (3tV3M/  $/8. 
(46.)X=1;  the  square  root  is  ±(a.-2  +  3a-- 1).  (46.)  -6,  92,105;  or  38, 
-92,  137.  (47.)  3,  4,  12  ;  or  27,  108,  108.  (49.)  7z2-2a;+l.  (50.)  The 
cube  root  is  x2  +  dx  +  fc  ;    e=3k+3d?,  f=6dk  +  d3,    cj  =  3#>  +  3M2,    h  =  dk2d. 


11ESULTS  OF  EXERCISES  5G1 

(51.)  It  is  {b2-b(c  +  a)}3.  (52.)  l+$x+%a?+£sa*'+&s<*.  .  .  (53.)  1- 
i«-Arf-Thfl*-TJt1flS»-  .  .  .  (54.)  s/x{l  +  l/2a!  -  l/8z2  +  l/lOa,-3  - 
5/128.i-1  +  7/256a;5.  .  . }. 

XVI. 

(1.)  2(a8-28a6&2  +  70a^-28a2&8  +  68).  (2.)  6/5.  (3.)  8.  (4.)  {Spq(p2-q2)/ 
(p2  +  q2?}i-  (5-)  2  +  (V3-4V5)t.  (7.)  a-4-6x3  +  18^-26.v+21.  (14.)  &. 
(15.)  x2+\/2iV{\/(^  +  y4)+a;2}+V(«4  +  2/4)-  ("■ )  V(2a462  +  2«6c2«2&). 
(18.)  (a-2  +  y-)nl- ;  1.  (19.)  ±(3+4i).  (20.)  ±(V13  +  i)/V2-  (21-) 
±K3  +  4i).  (22.)  ±  {(«  +  &)  + (a -&)i}.  (23.)  ±  {a-  +  V(*2-  I)*}-  <24-) 
±[V!(*2  +  l)/?}+^\/{(^-l)/2n-  (25.)  ±(3  +  2t),  ±(2-3i).  (26.) 
(aj  +  a)  («-«)  (.r-wa)  (aj-w'a)  (a--w2a)  (a-w'3«),  where  «=(-l+  V3*)/2> 
a/=(l  +  V3i)/2.  (27.)  (,r  +  l)  (x2-.t(V5  +  1)/2  +  1)  (xi  +  x(^/5  -  l)/2  +  l). 
(28.)   {a:2 -2a:  cos.  2ir/7  +  l}  {a-2 -2a:  cos.  4tt/7  +  1}  {a-2 -2a;  cos.  6w/7  +  l}. 

(29.)  n      |  r=-2ascos  t/  +  "A7r  +  a2    . 

fc=o    L  TO  J 


XVII. 

(1.)  151/208  >  5/7.  (3.)  {ad-bc)/(c-d).  (4.)  10*1;  7  +  5\/2.  (5.) 
14-456  .  .  .,  13-198  .  .  .,  15-835  .  .  .  (6.)  \/7  +  \/5.  (9-)  {ad-bc)l 
(b  +  c-cc-d);    -1  ;  0. 

XVIII. 

(1.)  145/416.  (2.)  The  real  values  of  a- are  ±  4.  (3.)  0,  6.  (4.)  25«y 
=  \2(x2  +  y-).  (10.)  19:16.  (11.)  29H  m™.  past  10.  (13.)  r>2h. 
(14.)   -01875  in.     (15.)  6 "373  ft. 

XIX. 

(1.)  -2,5.  (2.)  a+26.  (3.)  a+b.  (4.)  1,  1.  (5.)  a,  b,  c  (6.)  a  =  5, 
b=-l7.  (7.)  11a;2 -87a; +  160  =  0.  (8.)a*2+l  =  0.  (9.)  a2  +  rtc  =  0.  (10.) 
(x-a){x2  +  {a-b)x-ab  +  a?}=Q.  (11.)  x(x2-  107)  =  0.  (12.)  »(aj+2p-r)=0. 
(13.)3a;-(a+_6+_c)  =  0.  (14.)  xs-i(s  +  t){s  +  t-s2  +  st-t2} +2st  +  Vs-Ut  =  0. 
(15.)  (M^ -  ft' +  d> +  <#»-*')  +  «(<*- <*')=<>■  (16.)  X2  +  Y2  +  Z2-2YZ-2ZX 
-2XY  =  0.  (17.)  3a;2  +  2(a  +  &  +  c)a;-(a'-  +  &2  +  c2-2a&-2&c-2ca)  =  0.  (18.) 
3a;2  +  28a;  =  0.  (19. )  4cm(l  -  m)x  +  (1  -  mfy2  =  ivic2.  (20. )  ar(2aj2  -  iax  +  3a2)  =  0. 
(21.)  x- 16=0.  (22.)  49a;-  1936  =  0.  (23.)  a?*-3a;2  =  0.  (24.)  5xA-ibx* 
-2a2x2-ia2bx  +  ai+4a2b2=0.  (25.)  a6  =  0.  (26.)  2{a?(y-z)*-  2yz{z-xf 
(x-y?}=0.  (27.)  x*  +  y*  +  #-xy-yz-sx=0.  (28.)  a:(a:2-l)  =  0.  (29.) 
625a?- 24641a:  +  234256  =  0.  (30.)  c"(a:  +  a)«+1  =  a"a:'!+1.  (31.)  27b(a- --' 
= (&  -  2a)3.     (32. )  xy{x  +  y)  (a2  +  xy  +  y2)  =  0. 

XXI. 

(1.)  s  =  j/5 - 5y3  +  5t/.     (7.)  (ab'  +  a'b)2  =  {ac'Ta'c)"-  +  (bc'±b'c)2. 
VOL.  I  2  O 


562  RESULTS  OF  EXERCISES 


XXII. 

(7.)  1-3543,  6-6457.  (8.)  2-0508.  (11.)  -  6h2.  (13.)  +-55826  .  .  ., 
-•35826  .  .  .,  and  1-5  exactly.  (14.)  One  between -2  and -3,  namely, 
-2-8025  ;  the  rest  imaginary.  (25.)  1  "259921049894873.  (26.) 
2-094551481542326.  (27.)  9-96666679.  (28.)  46  7616301847,  '3471623192. 
(29.)  18-64482373095.  (30.)  123.  (31.)  4-5195507.  (32.)  1-475773161. 
(33.)  4-581400362.    (34.)  2-0520421768796.    (35.)  -1-4142135623730950488. 


XXIII. 

(1.)  iU-       (2.)  21.       (3.)    -HI       (4.)  2.     (5.)    -1-455.     (6.)  l/(a  +  b). 
(7.)  ac/b.    (8.)  b.     (9.)  0.    (10.)  {(a° +  b2)  (a*- b*  +  ab)~ as +  b3}l(as+P).    (11.) 
±b.     (12.)    -2,  f.      (13.)0,-£.      (14.)  f      (15.)    -I.      (16.)   -fc     (17.)  4. 
(18.)    -£.      (19.)  {.      (20.)  ab/(a  +  b). 
(2i)  iabfd-(a?-F)(cf-dc) 

(a--b~){(c+/)(a  +  b)-(c  +  d)(a-b)}-4ab{d(a  +  b)+/(a-b)}' 
(22.)  (a2  +  b2)/(a  +  b).       (23.)    a  +  b.       (24.)    2(a -b)(b-  c)/(c-  a).       (25.)    0, 
±\/(-ab-bc-  ca). 

XXIV. 

(1.)  6,  9.  (2.)  $f,  f|-  (3.)  6-60485,  3-68993.  (4.)  16,  4.  (5.)  f,  f 
(«■)  -Wi  --W-  (7-)  26 -a,  2a -b.  (8.)  2lm(m  -  3l)a/(2m2 -  SP),  3hn(2m 
-l)b/(2m2-3P).  (9.)-2&c/(a2  +  62),  2ac/(a2  +  b2).  (10.)  acj  (a? +  b2),  bc/(a?  +  b2). 
(11.)  a -6,  2ab/(a-b).  (12.)  a4-64,  a'  +  a^  +  fc4.  (13.)  -p$  p  +  q.  (14.) 
X=a-6-c,/t=-a6+fc-ca.  (17.)  aJc(5-c)(c -a) (a- b)  =  0.  (18.)^  +  ^. 
(19.)  X-  +  X-6.      (20.)  -^-fi^c. 


XXV. 

(1.)  60,  40,  36.     (2.)  2,  3,  4.     (3.)   7293,  '8039,  - -0269.     (4.)  12,  8,  6. 
(5.)  A  =  i,   B  =  f,   C=*.      (6.)   {(2/"-y>-(a;"-x')2/-.Ty  +  a/y}/{(y"-2/V" 

-  (a*  -  a;')2/'"  -  aty"  +  *Y} .  (7. )  -  ?\x>  +  \x-  TV  (8. )  x=\(b  +  c  -  a),  &c.  (9. ) 
x=2bc(c*-a2)(a  +  b)/(bc2  +  ca?  +  ab3  +  abc),  be.  (10.)  2 A(a  -b)  (x  -  c)/(a  -  b) 
(a-c).  (11.)  a,  6,  c.  (12.)  a?=(a  +  a)(a  +  /3)(a  +  7)/(a-6)(a-c),  &c.  (13.) 
%  =  a(a  +  b  +  c)/(a-b)(a-c),bc.     (14.)  a;=2/=z  =  Sa2-  S&c.     (15.)  a;  =  (m3  +  M3 

-  2Zmn  -  Zwz.2  +  Pm  -  /?i2  +  Pn)/2C2P  -  Smn)  =  (m  +  n)/2,  be.  (16.)  *=  (p-  +  mn)[ 
(l-m)(l-n),  be.  (17.)  x  :y:z  =  b  +  c-a  ic  +  a-b  :a  +  b-c.  (18.)  Put  a; +  y 
+*=/>,    then    x  =  Pa/(a  +  b  +  c)-(g-h)/(a  +  b  +  c).       (19.)    -%*,  -|£,  |f,  ff 

(20.)  Express  jj,  g-,  r  in  terms  of  .?,  y,  z,  s,  then  eliminate  p,  q,  r,  and  there 
Jesuits  a  system  of  three  equations  in  x,  y,  z ;    z=g(ad  +  bc)/{bce  +  bde-bcf 

-  ftd/"-  &<?/■+  cde  +  cef-  cdf-  abc  -  abd  -  abe  -  acd  -  ade  -  adf-  acf-  aef) .  (21. ) 
1,  3,  5,  9,  11.  (22.)  By  means  of  the  first  four  equations  express  all  the 
variables  in  terms  of  z  ;  the  last  equation  then  gives 

z  =  (afh  +  bey  -  bef-  cfh  -  bfh  -  bch)+(adfh  +  bug  +  befh  -  bfdh  -  bceh). 


RESULTS  OF  EXERCISES  563 

(24.)  x:y:z  :u  =  1/(1+  a)  :1/(1  +  6) :  1/(1  +c):  1/(1+0*).  (25.)  The  required 
equation  is  (B"0  +  (A'C")y  +  (A"B')8  =  A(B"C)  +  A'(BC")  +  A"(B'C).  where 
(B"C')  =  B"C'-B'C",  &c. 

XXVI. 

(1.)  b{a+ib  +  i\/aT)/a2.  (2.)  mV/(m-n)?.  (3.)  14.  (4.)  "T7-.  (5.)  *£. 
(6.)  a- /?.  (7.)  x=  ±  VfrfC^i?2-^^)}.  This  solution  is  extraneous  if  all  the 
radicals  be  taken  positively.  (8.)  ]>,  2p  +  2.  (9.)  (5a2-62)/4a.  (10.)  a  +  5. 
(11.)  0,   |f.       (12.)  W,    11.       (13.)  o6/(«  +  6),    (a  +  6)/4.       (14.)  |f,   AV 

»  =  «-&,     a  +  &,     a±\/a{a-2b)  ; 

(15.)  -J  , 

1  .?/=       0,         2&,     b^\/a{a-2b). 


(16)9     6         (17)    JB=flyWCflF-^.     w&C->     w2&c- 
1y=  &,«/{<*/(«*-*)},     w&c,     w2&c. 

(18.)  x  =  abcd,y=  -2abc,z=2db,u=  -2a.  (19.)  cc=  -(&2-c2)  (a +  6)  (a  +  c), 
&c.  (20.)  x=a/mn,  &c.  (21.)  #  =  £2a(2a  +  o),  &c.  (22.)  -a,  -  6,  -  c.  (23.) 
ce  =  (6  -  c)  (b2  -  c2)/(22«3  -  2a26),  &c.  (24.)  In  order  that  the  system  be  consistent 
we  must  have  \jk  =  l/{k  -  a)  +  lf(k  -b)  +  l/{k  -  c)  +  l/{k  -  d)  ;  then  x :  y :  z :  u 
=  l/{k~a):l/(k-b):l/(k-c):l/(k-d).  (25.)  x=\(a  +  c  +  d-2b),  to.  (26.) 
6,  8.  (27.)  0,  0;  and  fj,  -ff  (28.)  &,  IS-  (29.)  a?=  ± VIM^  +  M4) 
(l/X2  +  l//a2)!-2/=±V{2^4  +  M4)(lA2-VM2)}.  (30.)  a,  6;  and  a-a(a-b)/ 
c(c-b),  b-b(b-a)/c(e-a).  (31.)  -J-c,  -a-c.  (32.)  z=±^2a,  &c 
(33.)  x-±\j2bc/a,  &c.     (34.)  -a,  -b,  -e. 

XXVIII. 
(1.)  0,  -1.  (2.)  h  f.  (3._)_0,  0.  (4.)  1,  -2.  (5.)  |(3±i).  (6.) 
-1±V«.  (7.)  {-^a  +  ^iV^^-a)}/^-^.  (8.)  {  -  2pq±(p*  -  a2)i}/ 
(?2  +  <Z2).  (9.)  K-1±V17).  (10.)  -4,  -7.  (11.)  |i,  if  (12.) 
±(10±V'0-  (13.)  11±7'.  (14.)  200,  1.  (15.)  -53,  -49.  (16.)  53, 
-49.  (17.)  -3V7±2x/2.  (18.)  l  +  \/2±V3.  (19.)  -ll-5i,  -12-7i. 
(20.)  7  +  ii,  1-6/.  (21.)  2±JV3.  (22.)  (l±8i)/13.  (23.)  f,  |.  (24.) 
0,  a  +  b.  (25.)  -2a±(J+c).  (26.)  a  +  c,  -a-b.  (27.)  vW»).  \/(n/m). 
(28.)  (a  +  b)/ab,  -2/(a  +  b).  (29.)  a,  6(2a  +  6)/(a-5).  (30.)  1,  (b  +  c-2a)/ 
(c  +  a-26).  (31.)  c,  -&  (32.)  2a2±2a6.  (33.)  (a  +  &  +  c)/3.  (34.)  £(1 
+  V29). 

XXIX. 

(1.)    ±1,     ±VI»-        (2.)    ±V(Za2-2a&),    2a,        (3.)    -  2  ±  3i,    1,    3. 
(4.)  £[-(a-2)±aV2  +  \/{4-4a-a2=F2V2«(a-2)}], 

hi- (a-  2)±a\/2  -  V{4  -  4a  -  a2^2V2a(a  -  2)}  ]. 
(5.)  2,    i(-3±i'V23).       (6.)    -1,   (Va±tV(3a  +  4))/2V«.       (7.)    -«,    -w2, 
1,1.     (8.)  u/p,  u?/p,p*,  -p2. 

(9.)  £{3±V(\Al  +  4)}+A*-l±V(\/41-4)}', 

|{3±V(V41  +  4)}-4{-ld=V(V41-4)}i. 

(10.)  2,3,  1,  -1.     (11.)  -fi,  0,  -f 

vol.  i  2  o  2 


564  RESULTS  OF  EXERCISES 


XXX. 

(1.)  1/a  +  l/b,  -2/a.  (2.)  ±^(a2-ab  +  b-).  (3.)  (l±\/l9)/2.  (4.)  3. 
(5.)  3,  -£.  (6.)  (bd-2bc)j(2ca-cd).  (7.)  0,  {c(a2  +  b°-)  -  (as  +  P)}  /  {c(a2  +  F) 
-c"-(a  +  b)}.  (8.)  ±V{(2«2&2-c2a2-&2e2)/(«2  +  &2-2c2)},  0.  (9.)  (a2  +  62)/ 
(a  +  fc),  a  +  &,  0.  (10.)  -2{a  +  b)  +  2c,  (11.)  0,  0.  (12.)  {ab{c  +  d)-cd 
(a  +  b)}/{ab-cd).  (13.)  ±sj2ai,  0.  (14.)  2.  (15.)5,  -3i.  (16.)  ±la2/6. 
(17.)  Pa. 

XXXI.* 

(1.)  4,  |(-3±V"0-  (2.)  M-6  +  4V3).  (3.)  4(1-V5)a.  (4.)  c,  (2a2b 
+  tfc-a\)]{a?  +  2bc-b%  (5.)  [J(5±  x/52),  -|],3.  (6.)  (a2-  2a  +  2)2/4(a-  l)2. 
(7.)  0,  1,  [M-3=fcV7i)].  (8.)  [VI  0.  (9.)  [a&/(a  +  &)],  0.  (10.)  (3±V22)/2. 
(11.)  -3±V\5-  +  fV37.  (12.)  4(a  +  i),  [8(a  +  &)(2a  +  o)(a  +  26)/(a-o)2j. 
(13.)  [(«3  +  J3)/«H(«  +  ^)(«2  +  3a&  +  &'2)M  (14.)  [-(9a2+14a&  +  9&2)/8(a  +  &)]; 
if  6  =  a,  x=-2a,  which  does  not  satisfy  the  equation.  (15.)  5,  [  —  ■¥]. 
(16.)  +{a--b2)/2\/2(a2  +  b-).  (17.)  -ff,  -1.  (18.)  +  2a/V3.  (19.)  0,  oo . 
(20.)  42,  15.  (21.)  Reduces  to  x  =  0,  along  with  a  reciprocal  biquadratic 
whose  roots  a,  a,  (9±4\/5)a  are  all  extraneous.  (22.)  &a(m-  2)l(m"-  4m +  8). 
(23.)  0,  [±4V5«M  (24-)  a[-{m+n)/2(m-n)±bs/{l-lmnffa?+n?)}l 
(25.)  (2ib)*l4abc.     (26.)  ±{a2  -  n%2)/2^/ {n(n -  1)  (a2 -  nb1)} .     (27.)  -  V(a6), 

XXXII. 

(1.)  &,  c,  &c.  (2.)  |logeJ{p±V(2>2-4g)}.  (3.)  {a +S)/(a-  6)} WW, 
{(a-6)/(a  +  6)}^wt»-t),  &c.  (4.)  2,  -1.  (5.)  2  +  i  log  y/log  3.  (6.)  -A+ 
l^i^a-4)}.  (7.)  ±a,  ±^/(«2  +  2)i.  (8.)  2,  1/2,  -3,  -1/3.  (9.)  §, 
f,  4(3 ±  -s/5).  (10.)  J(3+>/5),  i(l±^/16<).  (11.)  4,  -1/4,  2,  -1/2. 
(12.)  {a-b±sJ{Ui-2ab-2,a-)}j2a,  -  1.  (13.)  {  -  (a  +  6)±  V(&2  +  2ao-  3a2)}/ 
2a,  1.  (14.)  ±s/{(-b±\/bi-4ac)/2a}.  (15.)  {-  6± \/(b--  4a2)} /2a,  ±1. 
(16.)  {-ft±V(^±4ac)}/2a  (4  solutions).  (17.)  J{1±V5  +  V(10:F2V5)*}, 
|{l±V5-V(10=F2V5)i}>  -1.  (18.)  i(-3±V5),  J(-5±V21),  1.  (19.) 
iV{-13±V73  +  V(-2062T26V73)},  &{kc.-kc.}.  (21.)  i(-5±V33), 
^,(-5±\/29)-  (22.)  The  equation  is  equivalent  to  x2  +  (p-q)x+pq=  ±i'\/ 
{^(p2+g2)}.  (23.)  ±V{iV(221±V48241)}.  (24.)  -  V,  3,  J(  -  l±V251t). 
(25.)  Reduces  to  a  reciprocal  biquadratic,  the  roots  of  which  are  extraneous. 
(26.)  0,  [±V24].  (27.)  -4.  (28.)  Tut  £=  {(a?-a)/(a!  +  a)}* j  the  equation 
then  becomes  a  reciprocal  cubic.  (29.)  -  2±£{\/(\/45  +  4)±  V(\/45  -  4)/}. 
(30.)  i(-7±V?7),  [i(-7±V53)].  (31.)  16,  [«,W].  (32.)  l\-p±^(}fi 
+  4q)),  where  ^  =  £  {  -  2a±2\/(2«2-  So&)}.  (34.)  Reduces  to  a  reciprocal 
biquadratic,  all  the  roots  of  which  are  extraneous  except  ^\/(2  +  2\/2).  (35.) 
±1,  2±V3,  J(l±V15i).  (36.)  ^{a  +  b±^/S(a-b)i},  a,  b,  w.  (37.)  ±2/ 
V(20V6-45),  ±2//y'(20x/6  +  4.r>).      (38.)    -^±^229,  -  -V-±\^/21. 


*  When  extraneous  solutions  are  given  at  all,  they  are  in  most  cases  dis- 
tinguished by  enclosing  them  in  square  brackets,  thus  [  -  y-g-]. 


RESULTS  OF  EXERCISES  565 


XXXIII. 

(1.)  12,18;  (2.)  7,-4;  (3.)  7,3,-7,-3;  (4.)  J,  5  ;  (5.)  0,  3,  h(  -  1± sjli) ; 
18,  12.  4,  -  7.  3,  7,  -  3,  -  7.  Vi  3-  °.  3»  M  -  IT  \#*)- 

(6.)  1,     2,     J(-11±VZ09);  (7.)  i;6±a-(2&-«)4}; 

2,     1,     i(-llT\/2°9)-  J^Ta^J-a)*}. 

(8. )  0,  (bq  -  ap)  (?2  -p«)/  {(a2  +  62)  (f.  +  gS)  _  4^}  . 

0,  (6p  -  ag)(q--2"-)/  {(a2  +  &2)  (^  +  f)  -  4«6P?}  • 
(9.)  {l+rt5±V(a2-l)(62-l)}/(a  +  i); 

{1  -  a6±V(a2-l)(62-l)}/(a  -  &)  ;  two  solutions. 
(10.)  {c±Vc(frf  -  lab)/d}/2a  ; 

{cT  &c.  }/26. 

(12.)         aj=±V{(325±3VH721)/68},     j//a:=(-107±\Al721)/2. 
(13.)  7,-7;  (14.)  5,-3;  (15.)  ±asj(a*+b")/b  ; 

5,   -5.  -3,      5.  ±b\Z(a2  +  b2)/a ;  two  solutions. 

(16.)  i(V5±l]P5  (17-)  ±K/3(2&-«),  ±«i; 

i(V5=Fl)?.  ±iv/3(2a-6),  T«. 

(18.)  0,  },ab(bw  +  aio°) ; 

0,  \ab{bw  -  aui2) ;  where  w3=  1. 

(19.)  ±{2p2(aV+623a)/(i»4-S'*)}*;  (20.)  f,   -f.         (21.)  3,-1; 

±  {223(aV  +  &V)/(l>*  -  g4)}  * ;  4  solutions.  1,-3. 

(22.)  4,  3,  -6,  -2;  (23.)  ±(x/3±\/2),  ±(9\/3±lW2)  5  4  solutions. 

3,  4,  -  2,  -  6. 
(24.)   ±3,  ±2;  (25.)  6,-2;  (26.)  3,  6,  3w,  6w,  3w2,  6ur  ; 

±2,  ±3;  4  solutions.  2,  -6.  6,  3,  6w,  3co,  6o2,  3w2. 

(27.)  2,  3,  2w,  3»,  2w2,  3ar  ;  (28.)   ±a*(a* - «&*)*,  ±  «&*(«* -<"&*)*■ 

3,  2,  3a>,  2w,  3w2,  2w2. 
(29.)  5,  2,    -5,   -2;  (30.)  2,  4,  2w,  4w,  2ar,  4ar  ; 

2,  5,  -  2,   -  5.  4,  2,  4u,  2w,  4u>2,  2w2. 

(31.)  i[6±V!-362±2V(2a4  +  264)!]; 

i[6TV{-3&2±2V(2a4  +  2&4)}]. 
(32.)  3,  2,  i(5±Vl510  5  /„  ,  2« 

2,  3,  i(5TV151*").  •X-2±/±V(^2  +  4)' 

(34.)  1,  2,  J(3±Vl9t);  (35. )  (2*+2Sw+«8)/2*j 

2,  1,  |(3=FV19*)-  w724- 

(36.)  i>v.  2c'  ;  where  u4  =  +1,  (37.)  &(17±\ 7,1/)  ; 

2v,  W\  i/*=-l.  &(17T\/510- 

(38.)  If  v  =  y/x,  then  u(l  +  u2)  =  a8(l  +  i/*),  a  reciprocal  biquadratic. 

(39.)  ±3,  ±2;  „     ,     .  .„  ,      x+y=±\/(-U±6'J7); 

_i_«    j-o     8  solutions  :  and  8  more  given  by  ,      .;  .    .„. 

±2,  ±3;  x-?/=±\/(- 14zp6\/7). 

(40.)  ±«Va6/(aa  +  63),  ±u»Va6/(a2  +  62);  (41.)  2,  8  ; 

±b\/abl{ar  +  V2),   ^fib\/ab/{a-  +  b-).  8,  2. 

(42.)  Rationalise  the  first  equation,  using  the  second  in  the  process,  and  thus 

find  a  quadratic  for  xy.         (43.)  {a--b-)/2a  ;  {a2  +  62±  V(«4"  6a2Z-2  +  64)}/4«. 


566  RESULTS  OF  EXERCISES 

(44.)  10,  13;  (45.)  2,  8;  (46.)  £  a  ; 

13,  10.  8,  2.  2a. 

(47. )  We  can  derive  (x  -  y)2  -  2a(x  +  y)     +  a2  =  0  ; 

(as  -  yf  -  \j2b(x  +  y)  +  sJ2ab  -  b2  =  0. 
(48.)  ±bi,  \/2a  +  b(bis); 

=p«i,  \J2b  +  a  (bis). 
(49.)  If  u  =  xy/ab,  v  =  x2/a2  +  y2/b2,  we  can  derive 

(m-  2)u2  +  2(m-n)u+(m-  2)  +  ?w  =  0  ; 
mu2  +  2{m  +  n)u  +  m-  {n  +  2)v  =  0. 
(50.)   ±als/(a  +  b);  (51.)  f; 

T6/V(«  +  6).  I- 

(52.)  One  real  solution  is  %{4a  +  l±yJ{8a  +  l)}  ; 

i{    -iTy(8«+i)}. 

Another  is  given  by  ?/3  +  2«?/2  + 1  =  0,  x  =  y~2. 

XXXIV. 

(1.)  as=  +(b-c)/(abcY,  y=  +(c-a)/(dbcf,  z=&c; 

a;  =  w(i  -  c)j(abc)  ,  y=w(c-a)/(abc)  ,  z = &c. ; 

x  =  u2(b-c)/{abc)  ,  y  =  &c.  2  =  &c. ; 

where  w3=+l.  (2.)  Eliminate  s  between  the  first  two  equations,  and  put 
£  =  x-  c,  T)  =  y  -c.     The  following  are  solutions  :  — 

x  =  b  +  c,  y  =  c  +  a,         z  =  a  +  b, 

x=  {b2  +  c2-a(b  +  c)}/(b  +  c-a),       y  =  kc,  z  =  kc. 

(3.)  as=2,    2/  =  3,    z=l;    or  as=-6,    y=-7,   z=-5.  (4.)  as =3,   2/  =  2, 

s=l.  (5.)  a;=±}V(1001).  2/=±tW(1001)>  2=  ±TVV(1001),  two  solutions. 
(6.)as=#=z=±V2/2.  (7.)a;=±(a-6-  +  «2c2-&2c2)/2a&c,  2/=±&c,  «=±&a, 
two  solutions.  (8.)  We  derive  by  subtraction  from  the  first  two  equations 
(x-y)(a-z)  =  0,  and  from  the  first  and  third  (x-z)(a-y)  =  0.  Combining 
these  two  with  one  of  the  original  equations,  we  obtain  the  following  fire 
solutions  (the  last  three  twice  over) : — 

x—a,  (},         (p2-a2)/a,  a,  a; 

y=a,  fi,  a,  (p2-a2)/«,  a  ; 

z  =  a,  /3,  a,  a,  (p2-a2)/a; 

where  a  and  /3  are  the  roots  of  x2  +  ax  -  j?  —  0.  (9.)  Eight  solutions,  as 
follows : — 

aj=«=(±5  +  V409)/3,  y=(zpl0  +  Vi09)/3  ; 

as=2=(±5-/s/409)/3,  ?/ =  ( ±  1 0  -  V409 )/3  ; 

a;  =  (±\/l635  +  23V/33)/6,            2  =  (±Vi635-t'3V33)/6, 
</=±V(1635)/6;        

ar=(±Vl635-i3V33)/6,  a  =  (±Vl635  +  ?3v/33)/6, 

2/=±V(1635)/6; 
upper  signs  together  and  lower  together  throughout. 

(10.)  x=±{^  +  \)/2(\  +  k  +  \y,  y=bc,  z  =  kc.      (11.)  If  we  add  the 


RESULTS  OF  EXERCISES  567 

three  equations,  we  obtain  the  equation  (a  +  b  +  c)(x  +  y  +  z)  =  Z{x  +  y  +  z)2. 
Hence  x+y+z=0,  or  =(a+6+c)/3.  The  three  equations  can  therefore  be 
replaced  by  three  linear  equations  :  x  =  0,  y=0,  2=0,  and  x=(Sbc  +  2ca  +  ab 
+  b2-c2)/2(bc  +  ca  +  ab),  &c,  are  solutions.  (12.)  The  equations  are  linear  in 
x'2  -  yz,  y-  -  zx,  z-  -  xy.  Solving,  we  obtain,  x2  -  yz  =p,  y2  -zx=q,  z2-  xy  =  r, 
say.  If  we  now  put  x  =  uz,  y  =  vz,  we  obtain  the  following  biquadratics  for 
u  and  v  : — 

(r2  -  x>q)  "4  -  ( V"  -  ir)uS  -  (?"  -pi)u  +  (p2-  ??')  =  °> 

(r2  -pq)v*  -  ( <f  -  rp)i?  -  (r2  -pq)v  +  (  q2  -  rp)  =  0. 
We  thus  find  the  following  values  for  ic  and  v  : — 

u=l,     to,      or,     {p*-qr)l{r*-pq), 

v=l,     ur,     a,       (q2-rp)/(7-2-pq). 

The  first  three  pairs  give  aj=w,  y=<*>,  2=00.  The  last  pair  gives 
x=±(p2-qr)/\/(p3  +  q3  +  r3-Spqr),  y=±kc,  z=±kc.  (13.)  From  the  first 
equation  we  see  that  x  =  pa(b-c)(<r  +  a),  y  =  pb[c-a)(cr  +  b),  z  =  kc,  where  p 
and  <r  are  arbitrary.  The  second  equation  gives  the  following  quadratic  for  <r, 
{2a2  -  26c}  o-2  +  {2re2(6  +  c)  -  6abc}  a  +  {262c2  -  abcZa]  =  0.  When  <r  is  known,  the 
third  equation  gives  p=±l/ V2a2(0-c)2(<r  + re)2.  Hence  we  obtain  four  sets 
of  values  for  x,  y,  z.  (14.)  From  the  first  three  equations  we  have  x  +  yz 
=  p/ft,  &c.  From  these,  squaring  and  using  the  last  equation,  we  deduce 
{l-y2)(l-z2)  =  p2/a2,  &c.  From  these  last  we  deduce  x-  ±sf(l±pa/bc), 
±&c.  ±&c.  Substituting  these  values  in  the  last  equation  we  find  p  =  0 
and  p=±(2ft4-22&2c2)/4«&c.  Hence  x  =  y  =  z= -1  ;  and  x=  -(a2-  b2-c2)/ 
2bc,  y=  -&c.  z=  -&c. 
(15.)  x  =  0,  4a,  fa,     -re,      -re; 

y  =  0,  4re,        -re,       fa,      -re; 

2=0,  4re,  -re,  —re,  fa. 
(16.)  The  given  equations  may  be  written  (x~y)2  +  (y-z)2  =  a2,  &c.  Hence 
we  have(?/-2)2  =  (62  +  c2-re2)/2,  &c.  Hence  y-z=±  V^J  +  <r  -  a-)/2,  &c.  The 
system  is  therefore  insufficient  to  determine  the  three  variables  ;  in  fact  it  will 
not  be  a  consistent  system  unless  2ft4- 262c2=0.  (17.)  If  p  =  xyz,  x  =  uz,y  =  vz, 
we  may  write  the  equations  ap  =  (v+l)/u,  fy)  =  (w- l)/v,  ep  =  u  +  v.  Elim- 
inating u  and  v  we  find  p2=(b  +  c-a)/abc  ;  and  so  on.  (18.)  If  x  be 
eliminated,  the  resulting  equations  may  be  written 

2£v  +  v2-  Utj  -28|-81=0, 
^-(v-7f  =0, 

where  £  =  yz,  r)  =  y2  +  z2;  one  set  of  solutions  is  x  =  3,  y=l,  2  =  2;  another 
x  =  Z,  y  =  2,  2  =  1;  &c.  (19.)  From  the  given  equations  we  can  deduce 
(bhj  -  (rz)/(y  -  z)  =  &c.  =  &c.  =  <r,  say.  Whence  (re4  -  <r)x  =  (o4  -  <x)y  =  (c4  -  <r)z 
=  t,  say.     We  can  then  determine  <x  and  r  by  means  of  the  given  equations. 

Result,  a-  =  p{n(re8-&4c4)}-/(ft8-J4c4)(2re12-3«464c4)i,  where  p  is  any  one  of 
the    4th   roots   of    +1.       (20.)  The   equations   can   be   written    xy  +  xz-yz 

=  P/a2,  &c,  where  p  =  x2y2z2/{yz  +  zx  +  xy).     Result,  x=  ±2bc(Zb2c°-)i/a(b2  +  c2), 

y=±kc.,z=±kc,  two  solutions.     (21.)  x=±\/2ahic\b  +  c)/{2a3{b  +  c)3}i, 


568  RESULTS  OF  EXERCISES 

y=±kc,  3=±&c.  (22.)  x-y  =  z=8;  &ndx= -6,  y= -4,  z= -2.  (23.) 
z=d(b  —  a)f(c-d),  y  =  c(b-a)/(c-d),  z  =  b(c-d)/(b-a),  u  =  a(c-d)/(b-a). 
(24.)  The  real  solutions  are  .r=3,  1,  2  ; 

y  =  2,  3,  1; 

(25. )  We  have  (a;2  -  yz)2  -  (y2  -  zx)  (z2  -  xy)  =  a4-  b2c2. 

Hence  x  =  p(a4-b2c2),     y  =  p(b4-c2a2),  &c. 

»  =  ±(a4  -  i2c'-)/V(2aG  -  3a2&2c2),  &c. 


XXXV. 

(1.)  [(ac'){(ad")  +  (be")}  -  (ac")  {(ad')  +  (be')}]  x  [(bd"){(ad')  +  (be')}  -  (bd') 
{(ad")  +  (be")\]  =  [(ae')(bd")  -  (ac")(bd')f.  (2.)  (l2  +  m2-  l)2(a  +  b)2-  (l2  +  m2-  1) 
{(l2-m2)2-l2-m2}(a2-b2)2  +  l2m2(a-b)2  =  0.  (3.)  «4  +  &4  =  c2(«2  +  &2).  (4.) 
8ds  =  Il(b2  +  c2-a2).  (5.)p+q  +  r  =  0.  (8.)  c(a-&)4-2c(^  +  ^)(a-&)2  +  (c^-^) 
(p-cq)  =  0.  (9.)  Eliminate  «,  and  put  ^  =  x  +  y,  yj=xy,  in  the  three  resulting 
equations,  then  eliminate  £ ,  and  there  results  two  quadratics  in  77,  &c.  (10. ) 
~Za?bz=Za2b2c2.  (11.)  Put  u  =  ~2,x,  v  =  2xy,  w  =  xyz,  eliminate  v  and  to,  and 
reduce  the  resulting  equations  to  two  quadratics  in  u.  (12.)  Let  %  =  x  +  a, 
V  =  y  +  b,  $=z  +  c,  then  ^=abc.  We  have  7?f-  (&  +  c)(i?  +  f)  =  «2-  (&  +  c)2, 
&c.  These  give  £,  17,  f  in  terms  of  77^,  f£,  £77.  Again  multiplying  the  last 
three  equations  by  £,  17,  f,  we  have  a&c-(J  +  c)(£?7  +  f£).  These  give  £,  17,  f 
again  in  terms  of  77^,  f£,  £77.  We  thus  get  three  linear  equations  for  £,  77,  f, 
&c.  (13.)  We  can  deduce  x-2xn  +  y.Yyn  =  const.  =2kn2  say;  x%xn  +  y3yn  =  3k„2, 
.  .  .  ;  and  finally  xn-ixn  +  yn-i yn  =  n-ikn2-  Now  either  n-i7cn2  —  kn2,  in  which 
case  the  system  is  indeterminate,  or  n_i£„24=£„2,  in  which  case  the  system 
is  inconsistent. 

XXXVI. 

(1.)  -pB  +  5psq~5pq3-  (2.)  (pG~6p4q  +  9p2q2-2q3)/(p2-4q).  (3.)  ( -f 
+  5p3q-5pq2)/q\  (4.)    ±(p4  -  3p2q  +  q2)  sj(p2  -  4q)/q\  (5.)    {-^(^-38) 

Mpi-q)^(p*-4q)}/TP(P2-q)(P*-Z<lW(Pi-4q)-  (G.)  p2-2q  +  2pq  +  2q2. 
(7. )  3A.c2  -  3 A2x  +  A3  -  B3  =  0.  (9. )  x?  -  (2h2  +  2ph  +p*  -  2q)x  +  h4  +  2phs  +  ( p2 
+  2q)h2  +  2pqh  +  q2=0.  (12.)  4aa'(c'a)  +  (a'2b2)  =  0.  (14.)  (pf-  Sp^  +  Sps^fps. 
(15. )    ( pf  -  5p,p23p3  +  §p?p.2p32  +  5p2V  -  5Plp3s)/p35.  (16. )    p^pJ  -  2p.? 

-2pi3P3  +  4piP-2Ps-P32-  (I7-)  (^PiP^3~P23-pi3P-i)/(2h3P3-p-23)-  (18.)  2;>i2 
-6pa.  (19.)  2hi-6p12p,  +  9p-P.  (20.)  2p13-3Plp.,-3p3.  (il.)  pi'-ipfa 
+  2p-?  +  4p1p3-4pi.  (22.)  {2piP42-Sj?iP3Pi+Pa*)/P4*.  (2Z.)  pi-2pxp3 

+  2p4.  (24.)  plp3-4Pi.  (2b.)  2,p14-%pl2p2  +  4p,2-4plp3  +  \Qpi.  (26.) 
K3-j3./c2  +  (jB1^3-4?4)^-^i2^4+4jo2i54-iV  =  0.  (30.)  2p2' +  2p2  -  plPl' .  (31.) 
=  2( ft"  +  px2')  -4(p2  +  p.{)  -  2plPl'.  (32. )  (j>2  - #j')a  +  ftft'( ^ +•#>')  +  fiV 
+Prp-2 ■  ( 36. )  .r2  -  4ocx  +  4a2d2  +  4b"-c2  -  4b2d2  =  0.  (37. )  a2V  +  a'b2  =  2aa'c. 
(38.)  The  roots  are  §,  f,  f.  (40.)  The  roots  are  -7,  8±V15-  (46-)  Fl'om 
the  first  two  equations  we  deduce  p-2=2h~/\/6,  3p3  =  (3/\/6-  1)Pi3,  &c.  (49.) 
I4  +  3 w4  -  6^m2  -f  8Jn3  -  6j»4  =  0.     (50. )  (2a4-b4  +  2d2b2  -  c4)2  =  4d6(a2  +  2b2). 


RESULTS  OF  EXERCISES 


569 


XXXVII. 

(1.)  Roots  real,  +  ,  +.  (2.)  Roots  real,  +(nurn.  greater),  -.  (3.)  Roots 
imaginary.  (4.)  Roots  equal,  +.  (5.)  Roots  real,  +(num.  greater),  -. 
(6.)  Roots  real,  -,  -.  (7.)  Roots  real  +,  -  (num.  greater).  (8.)  1°  b2-  iac, 
-  ;  a  +  c,  +  .  2°  b--iac,  +  .  3°  b2 -  iae,  -  ;  a  +  c,  -.  4°  &  =  0,  a  =  c. 
5°«  +  c  =  0.  (9.)  D  (the  discriminant)  = -4(;)-^)2.  (10.)  D=  -  4(e-  bf 
{a-b)°:  (11.)  D  =  2Z(6-c)2.  (12.)  T>  =  2Za-(b-  c)-.  (13.)  4^  +  27r2=0. 
(14.)  The  roots  are  f,  f,  |.  (16.)  256«e3- 27d4=-0.  (18.)  x*-x=0.  (19.) 
6z2  +  a:-2  =  0.        (20.)  a-2-6a:+7  =  0.        (21.)  ar- 2(2«2- l)a+ 1  =  0.        (22.) 


■2ax  +  cr  +  /32  =  0.      (23. 


(27.) 


-x 
qr 
rp 
pq 


1 

-x 
V 
V 


1 

<7 
-x 


q      —x 


(30.)  (x-1>)2»+1-q2"+1  =  0.     (31.)   4a2- 77 


x4  -  4x3  -  4a-2  +  16a;  -  8  =  0.     (24. )  x*  +  2x2  +  25  =  0. 
(28. )  x*  -  2a5  -x4  +  x2-  2x  -1=0. 

c  —  x  b  i> 

(29.)         ap      c-x  b    =  0. 

bp  ap      c-x 

(32.)  -123?  + 118a;2 -372a- +  386. 


=  0. 


(15. )  He  was  43  years 
(17.)  7  miles.     (18.) 

(20.)  £14,800.  (21.) 
(24.)  25*,    18,    67*. 


XXXIX. 

(1.)  3  seconds.  (2.)  84.  (3.)  13s.  9d.,  7.  (4.)  172%.  (5.)  2T<V  hours. 
(6. )  9.  (7. )  54  gallons.  (8. )  8  h.  27  m.  16  sec.  + .  (9. )  100  yards  per  minute ; 
150  yards  per  minute.  (10.)  5s.  lOd.  (11.)  15,  12.  (12.)  pq/h,  pq\h-p. 
(13.)  a\Jm){\  +  \Jm),  a/{l  +  \/m).  (14.)  1021  pence, 
of  age  in  the  year  1849.  (16.)  [ac  -  hi) /(a  -b  +  c-d). 
A  at  10  a.m.,  B  at  9.30  a.m.  (19.)  (q-p)/2r  +  d/2. 
x={m  +  n  +  2)/(mn-l).  (22.)  9  :  1.  (23.)  35,  25. 
(25.)  10-088",  10-288".  (26.)  106  yards,  very  nearly.  (27.)  ct/(b  +  c),  bt/{b  +  c), 
a(b2-c2)/2bci.  (28.)  10815:10827.  (29.)  aba'b'(a-  a')  (b  -  b')/(ab'  -  a'b)2. 
(30.)  In  A  100 m(ji+l)/(2mra+m  +  w),in  B  100  n{m  +  l)/{2mn  +  m  +  n).  (31.) 
20,  30.  (32.)  The  distances  from  XII  are  given  by  x—60p/ll,  where p  =  0, 
1,  2,  .  .  .,  11.  (33.)  If  A,  B,  Close  in  order,  they  had  originally  £13«/8, 
£7aj8,  £4«/8.  (34.)  3  hours,  and  4  hours.  (35.)  £20.  (36.)  8.  (37.)  80. 
(38.)  60  quarts.  (39.)  1,  2,  3,  4;  or  5,  6,  7,  8.  (40.)  The  duties  corre- 
sponding to  maximum  and  minimum  revenues  are  100(/>-a)/3a  %  and 
100(p-a)/a%  respectively.  (41.)  79.  (42.)  1,3,  5.  (43.)  %a~s/{2(b2 
-  KJ)} ,  f«i  ^  +  V {2(&2  "  W)}  •  (45. )  r  +  h[l±  V {2  -  (1  +  27-/*.)2}  ]/2,  r = ( V2 
-l)h/2. 


(1.)  495. 


(2.)  307J. 


XL. 

(3.)  36.        (4.) 


r.i 


(5.)  ^2-3«  +  4).       (6.) 


n\a2  +  n{n-Z)a  +  n2\.         (7.)    {Bl+F  +  bP-  l*)/2(l  -  P).         (8.) 


8998148^- 


(9.)  3.  (10.)  1000.  (11.)  Any  A. P.  whose  first  term  is  a  and  whose  CD. 
is  2a/(m  +  1)  has  the  required  property.  (12.)  £2131  :  5s.  (13.)  50,500  yards. 
(14.)  2525  yards.  (15.)  9.  (16. )  l/e.  (17. )  ft,  -W,  &c.  (18. )  -  f  I,  -  U,  &c. 
(19.)  20.  (20.)  20.  (22.)  1,  5,  9,  13.  (24.)  |w(3?i  +  5).  (26.)  6  + (a -ft 
-  hrb)n  +  \rbn2.     (26. )  3,  2.     (28. )  (2n)2  =  4  +  12  + .   .   .  +  (8»i  -  4),  (2/t  +  If  -  1 


570  RESULTS  OF  EXERCISES 

=  8  + 16  + .  .  .  +  8k-.  (29.)  The  first  odd  number  is  n?-1  - n+ 1.  The  second 
part  follows  from  §  7.    (30.)  T„=J(-1)»-1»(»+1);2^=  -  £»(re+2)or4(»  +  l)2, 

according  as  n  is  even  or  odd.  (31.)  f»(»  +  l).  (33.)  ns.  (34.)  ^?i(6rt2+15?i 
+  11).  (35.)  ns4  -  n«3  -  »-5i  +  n.  (36.)  (j3  -?)  (p-  2q)n  +  q( 2p  -iq),^  +  q2ns2. 
(37.)  -2n2-n.  (38.)  (re-  &)3»  +  3&(a-6)3nSi  +  362(a-  b)ns2  +  bsns3.  (39.) 
J(»-l)»(n  +  l)(»+2).  (40.)  TVi(«  +  l)(?i  +  2)(3?i  +  5).  (41.)  £n(?i  +  l)  (6?i2 
-2;i-l).  (42.)  i»(6?i3+32?i2  +  33«.-8).  (43.)  tVKh,  +  1)2(h,  +  2).  (44.)  4960. 
(45.)  J?n(m  +  l)(2??i  +  l).     (46.)  &(l  +  l)  (3m  +  2l-  2). 


XLI. 

(1.)  313-3.  (2.)  - i(313 - 3).  (3.)  J(l-  1/10").  (4.)  *(l-(-l)'V4»). 
(5.)  ^{l-(2/3)10}.  (6.)  |(3  +  V3){1-(V3-1)-0}.  (7.)  |(1  -  1/3").  (8.)  f . 
(9.)  1/(1+ a;).  (10.)  2V2.  (11.)  f.  (12.)  (a  +  x)s/2{a-x)(a2  +  x2).  (13.) 
(l+a)/(l  +  a:2).  (14.)  (x2n-y2")j(x  +  y)x2"-2.  (15.)  x{l  -xn)/(x -y)  (1  -x) 
-y(l-yn)l(x-y)(l-y).  (16.)  ^{9n-l/10  +  l/10-+i}.  (17.)  ^(6»-l). 
(18.)  a;2(.c2»-l)/(a;2-l)-^i(?i+l)(2?i+l).  (19.)  {{xy)^1-  (xy)-«}/(xy-  1) 
-  {*{x/y)«-y{y/x)«}l(x-y).  (20.)^(i>»-l)/(^2-l)-2%2»-l)/(a2-l).  (21.) 
|6»_2»+f.  (22.)-a3(l-(-l)"a3»)/(l+«3).  (23.)  2?i  +  (r2»  +  l/r*»-3) (r2"-  1)/ 
(r2-l).  (24.)?i  +  2(l-?-")/(r-l)+(l-?-2»)/(r2-l).  (26.)  a(r»-l)(r«-l)/ 
(>--l)2.  (28.)2„={l-(-)»(7i  +  l)x»-(-)-^«+1}/(l  +  a;)2,Sa3=l(l  +  af.  (29.) 
2„  =  |  +  (-)"-1(6«  +  l)/9.2»-1,  200=f.  (30.)  Sn  =  ^  +  (-)«-i(9«2  +  12^  +  2)/ 
27.2"-1,  S00=^V.  (31.)2„  =  l  +  2a:2/(a;-l)3-  {(»2  +  ?i)z2- (2«2-2)a;  +  (?i2-j0!7 
a»-1(a!-l)8,Sa)=l  +  2ar,/(a!-l)s.  (32.)  2(!0=(l  +  4a;+a3)/(l-*)4.  (38.)  2, 
=  11/57.  (34.)  (ar2  +  &r  +  c)(l-?-3")/(/-3-l).  (35.)  £5825  :  8  :5|.  (36.) 
100(w/V)».  (37.)JAi.  (38.)a2/(«-J).  (39.)  a"P-  (1  -a")E/(l  -a),  where  a  =  l 
-(rf-6)/100.  (41.)  7.  (42.)  180/121.  (43.)-forf.  (44.)  5,  or -6.  (45.)  5. 
(46.)  2(510-l),or£(510-l).  (47.)  f.  (48.)  I  f,  1.  (49.)  4,  8,  16,  32.  (50.) 
12^45.  (51.)  3,  48.  (52.)  11,  33,  99,  297;  or  -22,  66,  -198,  594.  (53.) 
(ac -  b2)/{2b  -a-c).  (54. )  5,  10 ;  or  -  25/3,  -  970/3.  (55. )  lip  and  q  be  the 
given  sums,  the  results,  are  2pq\{p2-\-q),  {p2-q)l(p2  +  q).  (58.)  (1  +  ffl) 
{l-(«c)"!/(l-rtc).     (60.)  aV7(l+r)(l-r)2(l-rl). 


XLII. 

(i.)f.f;  W,  W»  &e.    (2. )  ffc  f|f    (3. )  -VS  V,  -V-.  ¥,  ¥,  ¥.  - ¥,  &c. 

(4.)  For  the  corresponding  A. P.  a=\%,  b=-fz.  (5.)  For  the  correspond- 
ing A.P.  a={(p-l)V-(q-l)Q}/(p-q)rQ,  b=(Q-T)/(p-q)VQ.  (8.) 
h  {?>  -  VC?'2  -  90°) } »  15>  \  {P  +  V(^  -  90°)} .  where  p  is  arbitrary. 

XLIII. 

(1.)  4,  5,  3,  4.  (2.)  4,  3,  3,  4.  (3.)  3J.  (4.)  5-1871  .  .  .  (5.)  32617-105. 
(6.)  -00794818.  (7.)  3144-973.  (8.)  1-3800812.  (9.)  -0  ...  (22  cyphers) 
433352.  (10.)  -2674734.  (11.)  -979467.  (12.)  77794.  (13.)  38"37. 
(14.)  48-3.  (15.)  4-81213.  (16.)  282351500.  (17.)  3'560625.  (18.) 
The  common  ratio  is  1-079188.     (19.)  1-2921592.     (20.)  36-833432.     (21.)  20. 


RESULTS  OF  EXERCISES  571 

(22.)  35.  (23.)  1-041393.  (24.)  2432,  number  of  digits  19.  (25.)  5.  (26.) 
13-73454.  (27.)  }.  (28.)  -98397.  (29.)  -47320.  (30.)  2-10372,-1-10372. 
(31.)  x=  -3-313811,  y  =  -000527696.  (32.)  1-49947.  (33.)  £=76028, 
?/=-02060.  (34.)  1-24207.  (86.)  log  (o8-  ¥)/2  log  (a  +  b).  (36.)  x  +  y=  ±2a, 
x=y1.     (37.)  2-793925. 

XLIV. 

(1.)  3  months.  (2.)  £1660  :  12  :  10.  (3.)  £225  :  4  :  10.  (4.)  12  years. 
(5.)  254  years.  (6.)  7s.,  7s.  6d.  (7.)  15  years.  •  (11.)  Y{l+nr)/(l+nr')  it 
the  surplus  interest  be  not  reinvested  ;  otherwise  P{(1  -r/r')/(l  +r')n  +  r/r'\. 
(12.)  4-526  %.  (13.)  6  %.  (14.)  £41,746,  £48,837,  £59,417.  (15.)  2Arnr/2Ar, 
(log2Ar-logSArR-"r)/logR.  (16.)  £1107  :  3  :  7.  (17.)  £10  :  5  :  6.  (19.) 
£8078.  (20.)  £11,231.  (21.)  £1801  :  14  :  10.  (22.)  4%.  (23.)  £479  :  14  :  11. 
(24.)  10  years.  (25.)  £75  :  12  :  10.  (26.)  A(l -R"2")/2(R  +  1).  (27.) 
£2904:2:5.  (28.)  AR".  (29.)  20  years.  (30.)  {log  2-  log  (1  +  R-"1)}/ 
log R years.  (32.)  £1912 : 8 :  11.  (33. )  Present  value  =  a/(R  -  1)  +  b(l  -  B~n+1)/ 
(R-l)2-  {«+(»- 1)  6}  R-*/(R-l).  (34.)  Present  value  =  a  {1  -(&/R)»}/(R-  b). 
(35. )  A  j  mlK"^?  -  (m  +  1)R"*?  + 1 }  /R"*«(R»  -  1)  (R  -  1). 

XLV. 

(X  and  p  denote  roots  of  the  resolvents  of  Lagrange  and  Descartes.) 

(L)  X=2r/p.     (2.)X=±2.     (3.)X=-3.     (4.)  X=10.      (5.)  \=pq.      (6.) 
3/2  is  a  root.      (7.)  2  and   -3/2  are  roots.      (8.)  The  equation  reduces  to 
(.c2  +  2a;  +  3)(2;z2  +  :r-2)  =  0.       (9.)  X  =  ^566.       (10.)  x  =  l  +  V2  +  V3,    etc 
(11.)  />  =  4. 


END  OF  PART  I. 


Printed  in  Great  Britain  by  R.  &  R.  Clark,  Limiteo,  Edinburgh. 


BINDING  SECT.       DEC     6  TO 


QA 

Chrystal,  George 

152 

Algebra 

G^f 

1889 

pt.l 

cop. 2 

P&ASci 

so. 

■*•