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THE  THEORY  OF  FUNCTIONS  OF 
REAL  VARIABLES 

Jk 

VOLUME  II 


. JAMIE: S    Pif;RPONT 


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Edward  Bright 


Mathematics  Dept 


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LECTURES 

ON 

THE  THEORY  OF  FUNCTIONS  OF 
REAL  VARIABLES 

c 

VOLUME  II 


BY 

JAMES  PIERPONT,  LL.D. 

PROFESSOR  OF  MATHEMATICS  ix  YALE  UNIVERSITY 


GINN  AND  COMPANY 

BOSTON  •  NEW  YORK  •  CHICAGO  •  LONDON 


Qfi 


\f 


»7 


COPYRIGHT,  1912,  BY 
JAMES  PIERPONT 


ALL   RIGHTS   RESERVED 
923.4 


fltftenaum 


GINN  AND  COMPANY  •  PRO 
PRIETORS  •  BOSTON  •  U.S.A. 


TO 

ANDREW  W.  PHILLIPS 
THESE  LECTURES 

ARE  INSCRIBED 
WITH  AFFECTION  AND  ESTEEM 


773668 


PREFACE 

THE  present  volume  has  been  written  in  the  same  spirit  that 
animated  the  first.  The  author  has  not  intended  to  write  a 
treatise  or  a  manual ;  he  has  aimed  rather  to  reproduce  his  uni 
versity  lectures  with  necessary  modifications,  hoping  that  the 
freedom  in  the  choice  of  subjects  and  in  the  manner  of  presenta 
tion  allowable  in  a  lecture  room  may  prove  helpful  and  stimulating 
to  a  larger  audience. 

A  distinctive  feature  of  these  Lectures  is  an  attempt  to  develop 
the  theory  of  functions  with  reference  to  a  general  domain  of 
definition.  The  first  functions  to  be  considered  were  simple 
combinations  of  the  elementary  functions.  Riemann  in  his  great 
paper  of  1854,  "  Ueber  die  Darstellbarkeit  einer  Function  (lurch 
eine  trigonometrische  Reihe,"  was  the  first  to  consider  seriously 
functions  whose  singularities  ceased  to  be  intuitional.  The  re 
searches  of  later  mathematicians  have  brought  to  light  a  collection 
of  such  functions,  whose  existence  so  long  unsuspected  has  revolu 
tionized  the  older  notion  of  a  function  and  made  imperative  the 
creation  of  finer  tools  of  research.  But  while  minute  attention 
was  paid  to  the  singular  character  of  these  functions,  practically 
none  was  accorded  to  the  domain  over  which  a  function  may  be 
defined.  After  the  epoch-making  discoveries  inaugurated  in  1874 
by  G.  Cantor  in  the  theory  of  point  sets,  it  was  no  longer  neces 
sary  to  consider  a  function  of  one  variable  as  defined  in  an  in 
terval,  a  function  of  two  variables  as  defined  over  a  field  bounded 
by  one  or  more  simple  curves,  etc.  The  first  to  make  use  of  this 
new  freedom  was  C.  Jordan  in  his  classic  paper  of  1892.  He 
has  had,  however,  but  few  imitators.  In  the  present  Lectures  the 
author  has  endeavored  to  develop  this  broader  view  of  Jordan, 
persuaded  that  in  so  doing  he  is  merely  carrying  a  step  farther 
the  ideas  of  Dirichlet  and  Riemann. 

Often  such  an  endeavor  leads  to  nothing  new,  a  mere  statement 
for  any  n  of  what  is  true  for  n  =  1,  or  2.  A  similar  condition 


vi  PREFACE 

prevails  in  the  theory  of  determinants.  One  may  prefer  to  treat 
only  two  and  three  rowed  determinants,  but  he  surely  has  no 
ground  of  complaint  if  another  prefers  to  state  his  theorems  and 
demonstrations  for  general  n.  On  the  other  hand,  the  general 
case  may  present  unexpected  and  serious  problems.  For  example, 
Jordan  has  introduced  the  notion  of  functions  of  a  single  variable 
having  limited  variation.  How  is  this  notion  to  be  extended  to 
two  or  more  variables  ?  An  answer  is  far  from  simple.  One  was 
given  by  the  author  in  Volume  I ;  its  serviceableness  has  since 
been  shown  by  B.  Camp.  Another  has  been  essayed  by  Lebesgue. 
The  reader  must  be  warned,  however,  against  expecting  to  find 
the  development  always  extended  to  the  general  case.  This, 
in  the  first  place,  would  be  quite  impracticable  without  greatly 
increasing  the  size  of  the  present  work.  Secondly,  it  would  often 
be  quite  beyond  the  author's  ability. 

Another  feature  of  the  present  work  to  which  the  author  would 
call  attention  is  the  novel  theory  of  integration  developed  in 
Chapter  XVI  of  Volume  I  and  Chapters  I  and  II  of  Volume  II. 
It  rests  on  the  notion  of  a  cell  and  the  division  of  space,  or  in  fact 
any  set,  into  unmixed  partial  sets.  The  definition  of  improper 
multiple  integrals  leads  to  results  more  general  in  some  respects 
than  yet  obtained  with  Riemann  integrals. 

Still  another  feature  is  a  new  presentation  of  the  theory  of 
measure.  The  demonstrations  which  the  author  has  seen  leave 
much  to  be  desired  in  the  way  of  completeness,  not  to  say  rigor. 
In  attempting  to  find  a  general  and  rigorous  treatment,  he  was 
at  last  led  to  adopt  the  form  given  in  Chapter  XI. 

The  author  also  claims  as  original  the  theory  of  Lebesgue 
integrals  developed  in  Chapter  XII.  Lebesgue  himself  considers 
functions  such  that  the  points  e  at  which  a  <f(x)  <6,  for  all  a,  b 
form  a  measurable  set.  His  integral  he  defines  as 

lim  2lmerm 

W=«     1 

where  lm<f(x)<lm+l  in  em  whose  measure  is  e'm,  and  each 
lm+1  —  lm=  0,  as  n  =  oo.  The  author  has  chosen  a  definition  which 
occurred  to  him  many  years  ago,  and  which  to  him  seems  far 
more  natural.  In  Volume  I  it  is  shown  that  if  the  metric  field  ^ 


PREFACE  vii 

be  divided  into  a  finite  number  of  metric  sets  Sv  S2  •••  of  norm  d, 
then 

=  Min 


where  m^  M,  are  the  minimum  and  maximum  of/  in  St.  What 
then  is  more  natural  than  to  ask  what  will  happen  if  the  cells 
Bv  S2>"  are  infinite  instead  of  finite  in  number?  From  this 
apparently  trivial  question  results  a  theory  of  ^-integrals  which 
contains  the  Lebesgue  integrals  as  a  special  case,  and  which, 
furthermore,  has  the  great  advantage  that  riot  only  is  the  relation 
of  the  new  integrals  to  the  ordinary  or  Riemannian  integrals 
perfectly  obvious,  but  also  the  form  of  reasoning  employed  in 
Riemann's  theory  may  be  taken  over  to  develop  the  properties 
of  the  new  integrals. 

Finally  the  author  would  call  attention  to  the  treatment  of 
the  area  of  a  curved  surface  given  at  the  end  of  this  volume. 
Though  the  above  are  the  main  features  of  novelty,  it  is  hoped 
that  the  experienced  reader  will  discover  some  minor  points,  not 
lacking  in  originality,  but  not  of  sufficient  importance  to  em 
phasize  here. 

It  is  now  the  author's  pleasant  duty  to  acknowledge  the  in 
valuable  assistance  derived  from  his  colleague  and  former  pupil, 
Dr.  W.  A.  Wilson.  He  has  read  the  entire  manuscript  and 
proof  with  great  care,  corrected  many  errors  and  oversights  in 
the  demonstrations,  besides  contributing  the  substance  of  §§  372, 
373,  401-406,  414-424. 

Unstinted  praise  is  also  due  to  the  house  of  Ginn  and  Com 
pany,  who  have  met  the  author's  wishes  with  unvarying  liberality, 
and  have  given  the  utmost  care  to  the  press  work. 

JAMES  PIERPONT 

NEW  HAVEN,  December,  1911 


CONTENTS 


CHAPTER   I 

POINT  SETS  AND  PROPER  INTEGRALS 

ARTICLES 

1-10.     Miscellaneous  Theorems    .         .        .  .        . 

11-15.     Iterable  Fields  .        .        .        .        .  ... 

16-25.     Union  and  Divisor  of  Point  Sets        .  .        . 


PAGE 

1 

14 
22 


26-28. 

29. 

30. 

31-61. 
62-69. 
70-78. 


CHAPTER   II 
IMPROPER  MULTIPLE  INTEGRALS 

Classical  Definition    .        .        .        .        .        ... 

Definition  of  de  la  Valle"e-Poussin     .... 

Author's  Definition  .         .        ... 

General  Theory         .        .'       .    '     .        . 
Relation  between  Three  Types .         .  .        . 

Iterated  Integrals      .  .        ..        .        . 


30 
31 
32 
32 
59 
63 


CHAPTER  III 
SERIES 

79-80.  Preliminary  Definitions  and  Theorems     .         .  .      .       r.        .         .77 

81.  Geometric,  General  Harmonic,  Alternating,  and  Telescopic  Series  .       81 

82.  Dini's  Series      .        .        .        ,        .       '......        .86 

83.  Abel's  Series      .         .        .        .        .         ...        .        ..       .     '   .      87 

84.  Trigonometric  Series         .........       88 

85.  Power  Series     .        .  . 89 

86.  Cauchy's  Theorem  on  the  Interval  of  Convergence  ....      90 
87-91.  Tests  of  Convergence.     Examples     .         .        .         .        .        .        .91 

92.  Standard  Series  of  Comparison          .        .        .        .         .         .         .     101 

93-98.  Further  Tests  of  Convergence   .        . 104 

99.  The  Binomial  Series .         .110 

100.  The  Hypergeometric  Series 112 

101-108.  Pringsheim's  Theory .        .         .113 

109-113  Arithmetic  Operations  on  Series        .         ......     125 

114-115.  Two-way  Series .         .133 

ix 


CONTEXTS 


CHAPTER   IV 


MULTIPLE  SERIES 


ARTICLES 

PAGE 

116-125. 

General  Theory          

.     137 

126-133. 

148 

CHAPTER   V 

SERIES   OF  FUNCTIONS 

134-145. 

156 

146. 

The  Moore-Osgood  Theorem      ....... 

.     170 

147-149. 

Continuity  of  a  Series        

.     173 

150-152. 

Termwise  Integration         ........ 

.     177 

153-156. 

Termwise  Differentiation  .        ... 

.     181 

CHAPTER   VI 

POWER  SERIES 

157-158. 

Termwise  Differentiation  and  Integration 

.     187 

159. 

Development  of  log  (1  +  E),  arcsin  x,  arctan  »,  e1,  sin  x,  cosse 

.     188 

160. 

Equality  of  two  Power  Series    ....... 

.     191 

161-162. 

Development  of  a  Power  Series  whose  Terms  are  Power  Series 

.     192 

163. 

Multiplication  and  Division  of  Power  Series     . 

.     196 

164-165. 

Undetermined  Coefficients         ....... 

.     197 

166-167. 

Development  of  a  Series  whose  Terms  are  Power  Series  . 

.     200 

168. 

Inversion  of  a  Power  Series       

.     203 

169-171. 

Taylor's  Development        .         .         . 

.     206 

172. 

Forms  of  the  Remainder   .         .         . 

.     208 

173. 

Development  of  (l+sc)'*  ........ 

.     210 

174. 

Development  of  log  (1  -f  x),  etc.        .         .        .        . 

.     212 

175-181. 

Criticism  of  Current  Errors        .         .         ... 

.     214 

182. 

Pringsheim's  Necessary  and  Sufficient  Condition 

.     220 

183. 

Circular  Functions     ......... 

.     222 

184. 

Hyperbolic  Functions        ........ 

.     228 

185-192. 

Hypergeometric  Function           ....... 

.     229 

193. 

Bessel  Functions        ......... 

.     238 

CHAPTER   VII 

INFINITE  PRODUCTS 

195-202. 

242 

203-206. 

260 

207-212. 

Uniform  Convergence        ........ 

.     254 

213-218. 

Circular  Functions    ......... 

.     257 

CONTENTS 


XI 


ARTICLES  PAGE 

219.     Bernouillian  Numbers 266 

220-228.     B  and  T  Functions 267 

CHAPTER   VIII 

AGGREGATES 

229-230.     Equivalence "     •  '•    .v        •  -•  •  •     276 

231.     Cardinal  Numbers      .        .        .        ...        .    ...  .  .  .  .     278 

232-241.     Enumerable  Sets        .         *;       •        •        •        •     .    •  •  •  -280 

242.     Some  Space  Transformations    .         .                 .        .  .  •  •     286 

243-250.     The  Cardinal  c v  •  •  •     287 

251-261.     Arithmetic  Operations  with  Cardinals       .         .    •     .  ...  .292 

262-264.     Numbers  of  Liouville         .        .        *        .        .        .  .  •  -299 

CHAPTER   IX 
ORDINAL  NUMBERS 

265-267.     Ordered  Sets      .         .        •        •        •        •        •      :  '  •  '  .302 

268-270.     Eutactic  Sets     .        .       ...        .        .        .        .  .  .  .304 

271-279.     Sections     .        . •  •  •     307 

280-284.     Ordinal  Numbers       .         .        .        .      ..'      .        .  .  .  .310 

285-288.     Limitary  Numbers     .      *  ."        .         .         .         ...  •  •  •     314 

289-300.     Classes  of  Ordinals     .        .        .        .        .        .        •  *  .  .     318 

CHAPTER   X 
POINT  SETS 

301-312.     Pantaxis  .         .         .        • 824 

313-320.     Transfinite  Derivatives      .         .         .         .         •         •  •  •  •     330 

321-333.     Complete  Sets    .        .        .        .        .                 .        .  .  .  .337 

CHAPTER   XI 
MEASURE 

334-343.     Upper  Measure .        .        .        .        .        .        •        •  •  •  .343 

344-368.     Lower  Measure          .         .         .         .         ...  .  .  -     348 

369-370.     Associate  Sets   .        .         ...        ...         .  .  •  •     365 

371-376.     Separated  Sets  .        .        .        .        .        .        ..       •  •  •  .366 

CHAPTER   XII 
LEBESGUE  INTEGRALS 

377-402.     General  Theory _•  •  .371 

403-406.     Integrand  Sets •  ....     385 


Xll 


CONTENTS 


ARTICLES 

407-409.  Measurable  Functions 

410.  Quasi  and  Semi  Divisors 

411-413.  Limit  Functions 

414-424.  Iterated  Integrals 


IMPROPER  L-!NTEGRALS 


425-428.     Upper  and  Lower  Integrals 
429-431.     Z-Integrals 
432-435.     Iterated  Integrals      . 


PAGE 

388 
390 
392 
394 


402 
405 
409 


CHAPTER   XIII 

FOURIER'S  SERIES 

436-437.  Preliminary  Remarks        .... 

438.  Summation  of  Fourier's  Series  . 

439-442.  Validity  of  Fourier's  Development  . 

443-446.  Limited  Variation 

447-448.  Other  Criteria 

449-456.  Uniqueness  of  Fourier's  Development 


415 
420 
424 
429 
437 
438 


CHAPTER   XIV 
DISCONTINUOUS  FUNCTIONS 

457-462.  Properties  of  Continuous  Functions  . 

463-464.  Pointwise  and  Total  Discontinuity    .         .        . 

465-473.  Examples  of  Discontinuous  Functions 

474-489.  Functions  of  Class  1 

490-497.  Semicontinuous  Functions         .... 


452 
457 
459 

468 
485 


CHAPTER   XV 
DERIVATES,  EXTREMES,    VARIATION 


498-518.  Derivates  . 

519-525.  Maxima  and  Minima 

526-534.  Variation  . 

535-537.  Non-intuitional  Curves 

538-539.  Pompeiu  Curves 

540-542.  Faber  Curves 


493 
521 
531 
537 
542 
546 


CHAPTER   XVI 
SUB-  AND  INFRA-UNIFORM  CONVERGENCE 


543-550.     Continuity 
551-556.     Integrability 
557-561.     Differentiability 


555 
562 
570 


CONTENTS 


Xlll 


CHAPTER   XVII 


GEOMETRIC  NOTIONS 

ARTICLES  PAGE 

562-563.     Properties  of  Intuitional  Plane  Carves 578 

564.  Motion 579 

565.  Curve  as  Intersection  of  Two  Surfaces 579 

566.  Continuity  of  a  Curve 580 

567.  Tangents 580 

568-572.     Length '.      .  .         .581 

573.     Space-filling  Curves .        .  ~     .        .     588 

.574.  Hilbert's  Curve           .         .         .         .         .         .         .         .         .         .590 

575.     Equations  of  a  Curve •  '•       .     593 

576-580.     Closed  Curves .         .        .        .         .594 

581.  Area 599 

582.  Osgood's  Curve  .        .        .        .        .        .        .        .        •'        .600 

583.  Re-sums' .        ....     603 

584-585.     Detached  and  Connected  Sets 603 

586-591.     Images '       .        .        .        .  '      .        .605 

592-597.  Side  Lights  on  Jordan  Curves  .         .        .        .    .    .       '•       .  •  •      •     610 

598-600.  Brouwer's  Proof  of  Jordan's  Theorem      .-'•-,.        .  •      .        .        .     614 

601.  Dimensional  Invariance     .       ..        .        .        ...        .        .     619 

602.  Schonfliess'  Theorem         .        .        .        .        .        .    '     .        .         .     621 

603-608.     Area  of  Curved  Surfaces 623 

Index .        .        .        .        .        .        .         .639 

List  of  Symbols 644 


FUNCTION  THEORY   OF  REAL 

VARIABLES        :  v^  U; 

CHAPTER   I 
POINT   SETS   AND   PROPER   INTEGRALS 

1.  In  this  short  chapter  we  wish  to  complete  our  treatment  of 
proper  multiple  integrals  and  give  a  few  theorems  on  point  sets 
which  we  shall  either  need  now  or  in  the  next  chapter  where  we 
take  up  the  important  subject  of  improper  multiple  integrals. 

In  Volume  I,  702,  we  have  said  that  a  limited  point  set  whose 
upper  and  lower  contents  are  the  same  is  measurable.  It  seems 
best  to  reserve  this  term  for  another  notion  which  has  come  into 
great  prominence  of  late.  We  shall  therefore  in  the  future  call 
sets  whose  upper  and  lower  contents  are  equal,  metric  sets.  When 
a  set  51  is  metric,  either  symbol 

I     or     51 

expresses  its  content.  In  the  following  it  will  be  often  con 
venient  to  denote  the  content  of  51  by 

a. 

This  notation  will  serve  to  keep  in  mind  that  51  is  metric,  when 
we  are  reasoning  with  sets  some  of  which  are  metric,  and  some 
are  not. 

The  frontier  of  a  set  as  51,  may  be  denoted  by 

Front  51. 

2.  1.    In  I,  713  we  have  introduced  the  very  general  notion  of 
cell,  division  of  space  into  cells,  etc.      The  definition  as  there 

1 


2  POINT   SETS   AND   PROPER  INTEGRALS 

given  requires  each  cell  to  be  metric.  For  many  purposes  this 
is  not  necessary  ;  it  suffices  that  the  cells  form  an  unmixed  divi 
sion  of  the  given  set  51.  Such  divisions  we  shall  call  unmixed  di 
visions  of  norm  8.  [I,  711.]  Under  these  circumstances  we  have 
now  theorems  analogous  to  I,  714,  722,  723,  viz  : 

2.  Let  3?  contain  the  limited  point  set  51.  Let  A  denote  an  un 
mixed  division  of  $8  of  norm  8.  Let  515  denote  those  cells  of  33  con 
taining  points  of  5L  Then 


8=0 

The  proof  is  entirely  analogous  to  I,  714. 

3.  Let  $8  contain  the  limited  point  set  51.  Let  f(x^  •  •  •  xm)  be 
limited  in  51.  Let  A  be  an  unmixed  division  of  ^Q  of  norm  8  into 
cells  Sr  S2,  •  •  •  .  Let  9ftt,  mt  be  respectively  the  maximum  and  mini 
mum  off  in  St.  Then 

lim  £A  =  lira  29HA  =  f  /«,  (1 

6=0  8=0  */SI 

lira  flA  =  lim  2mA  =  f/*  (2 

5=0  S=0  ^H 

Let  us  prove  1)  ;  the  relation  2)  may  be  demonstrated  in  a  similar 
manner.  In  the  first  place  we  show  in  a  manner  entirely  analo 
gous  to  I,  722,  that 

.  (3 

The  only  modifications  necessary  are  to  replace  8t,  8[,  Sl)C,  by  their 
upper  contents,  and  to  make  use  of  the  fact  that  A  is  unmixed,  to 
establish  5). 

To  prove  the  other  relation 

,  (4 

we  shall  modify  the  proof  as  follows.  Let  E  be  a  cubical  division 
of  space  of  norm  e  <  eQ.  We  may  take  eQ  so  small  that 


PROPER  INTEGRALS  3 

The  cells  of  E  containing  points  of  21  fall  into  two  classes. 
1°  the  cells  eltt  containing  points  of  the  cell  St  but  of  no  other  cell 
of  A ;  2°  the  cells  e(  containing  points  of  two  or  more  cells  of  A. 
Thus  we  have 


where  MM  M(,  are  the  maxima  of  /  in  et(C,  e[.     Then  as  above  we 
have 


if  eQ  is  taken  sufficiently  small. 
On  the  other  hand,  we  have 


Now  we  may  suppose  S0,  eQ  are  taken  so  small  that 


differ  from  51  by  as  little  as  we  choose.     We  have  therefore  for 
properly  chosen  S0,  e0, 


This  with  6)  gives 

which  with  5)  proves  4). 

4.    Let  f(xl  •  •  -  xm)  be  limited  in  the  limited  field  21.     Let  A  be 
an  unmixed  division  oftyiof  norm  8,  into  cells  Sv  S2  •  •  • .     Let 


where  as  usual  mt,  Jf[  are  the  minimum  and  maximum  of  f  in  8t. 

Then 

=  Max  £A,  yrfa  =  Min  S*. 


The  proof  is  entirely  similar  to  I,  723,  replacing  the  theorem 
there  used  by  2,  3. 

5.  In  connection  with  4  and  the  theorem  I,  696,  723  it  may  be 
well  to  caution  the  reader  against  an  error  which  students  are  apt 
to  make.  The  theorems  I,  696,  1,  2  are  not  necessarily  true  if  / 


4  POINT   SETS   AND   PROPER  INTEGRALS 

has  both  signs  in  51.  For  example,  consider  a  unit  square  S 
whose  center  call  O.  Let  us  effect  a  division  E  of  S  into  100 
equal  squares  and  let  51  be  formed  of  the  lower  left-hand  square  s 
and  of  (7.  Let  us  define  /  as  follows  : 

/  =  1  within  s 
=  - 100  at  0. 

For  the  division  E, 

Hence,  Min  ^  <  _ 

On  the  other  hand,          ^m  g  __  _\ 


d=0 


The  theorems  I,  723,  and  its  analogue- 4  are  not  necessarily  true 
for  unmixed  divisions  of  space.  The  division  A  employed  must 
be  unmixed  divisions  of  the  field  of  integration  51.  That  this  is 
so,  is  shown  by  the  example  just  given. 

6.  In  certain  cases  the  field  51  may  contain  no  points  at  all. 
In  such  a  case  we  define  „ 

f/=o. 

J% 

7.  From  4  we  have  at  once  : 

Let  A  be  an  unmixed  division  of  51  into  cells  Sv  £2,  •••     Then 

%  =  Min  2£t, 
with  respect  to  the  class  of  all  divisions  A. 

8.  We  also  have  the  following  : 

Let  D  be  an  unmixed  division  of  space.  Let  d±,  d^--  denote  those 
cells  containing  points  of  51.  •  Then 

^  =  Min  24, 
with  respect  to  the  class  of  the  divisions  D. 

For  if  we  denote  by  S,  the  points  of  51  in  d,  we  have  obviously 

5<2,. 

Also  by  I,  696,  S  =  Min  2et 


PROPER   INTEGRALS  5 

with  respect  to  the  class  of  rectangular  division  of  space  E  =  \e,\. 
But  the  class  E  is  a  subclass  of  the  class  D. 
Thus 

Min  28t  <  Min  2^  <Min  2«c. 

A  D  E 

Here  the  two  end  terms  have  the  value  51. 


3.  Let/^j  •••  zm),  g(x^  •••  xm)  be  limited  in  the  limited  field  51. 
We  have  then  the  following  theorems  : 

1.  Letf  =  g  in  51  except  possibly  at  the  points  of  a  discrete  set  £). 
Then,  _  _ 

//=//• 

For  let  |  /  1,  \g\<M.  Let  D  be  a  cubical  division  of  norm  d. 
Let  MU  N,  denote  the  maximum  of/,  g  in  the  cell  d,.  Let  A  de 
note  the  cells  containing  points  of  £),  while  A  may  denote  the 
other  cells  of  5l/>. 

Then, 


Hence, 


^  _    ^-^    <  2  -flf,  -  #    dt  <  2 


and  the  term  on  the  right  =  0  as  d  =  0. 

2.    Let  f  >  g  in  51  except  possibly  at  the  points  of  a  discrete  set 
Then 


Forlet 

But  in  J.,  f>g,  hence 


The  theorem  now  follows  at  once. 


POINT  SETS  AND   PROPER  INTEGRALS 

,_.,, 


For  in  any  cell  dt 

•,-    Max  •  cf=c  Max/;         Min  •  cf  =  c  Min/ 
when  c  >  0  ;  while 

Max  •  </  =  <?Min/;          Min  •  <?/=<?  Max/ 
when  c  <  0. 

4.    If  g  is  integrable  in  51, 


For  from 

Max  /  +  Min  g  <  Max  (/  +  g)  <  Max  /  +  Max  g, 

we  have 

(2 


But  g  being  integrable, 
Hence  2)  gives 


which  is  the  first  half  of  1).     The  other  half  follows  from  the 

relation 

Min  /  +  Min  g<M'm  (/  +  g)  <  Min  /  +  Max  g. 

5.    The  integrands  /,  g  being  limited, 


For  in  any  cell  d, 


PROPER  INTEGRALS 

6.    Let  f  =  g  +  h,  \h\<H  a  constant,  in  51      Then, 


Then  by  2  and  4 


or 


fff<      /<       <7  +  ftf, 

^/2i          ^l  ~2l         J% 

r 
g<  \  f< 


4.    Letf(xl  •••  a:TO)  be  limited  in  limited  51.      Then, 


|/  1  <  Jf,  wg  have  also, 

fl/l<.JrtC 


(2 
(3 
(4 

(5 


Let  us  effect  a  cubical  division  of  space  of  norm  S. 
To  prove  1)  let  JVt  =  Max|/|  in  the  cell  dL.     Then  using  the 
customary  notation, 


Hence 

Letting  8=0,  this  gives 


\vhich  is  1). 


< 


8  POINT  SETS  AND   PROPER  INTEGRALS 

To  prove  3),  we  use  the  relation 

-I/I  </<!/!• 

Hence 


from  which  3)  follows  on  using  3,  3. 
The  demonstration  of  4)  is  similar. 
To  prove  5),  we  observe  that 


5.    1.    Let  f>  0  be  limited  in  the  limited  fields  33,  (L     Let  91  be 
the  aggregate  formed  of  the  points  in  either  33  or  (L      Then 


This  is  obvious  since  the  sums 


may  have  terms  in  common.  Such  terms  are  therefore  counted 
twice  on  the  right  of  1)  and  only  once  on  the  left,  before  passing 
to  the  limit. 

Remark.     The  relation  1)  may  not  hold  when  /  is  not  >  0. 

Example.     Let  $  =  (0,  1),  55  =  rational  points,  and  (£  =  irra 
tional  points  in  $.     Let/=  1  in  55,  and  -  1  in  g.     Then 


and  1)  does  not  now  hold. 

2.    Let  51  be  an  unmixed  partial  aggregate  of  the  limited  field 

Let  (5  =  55  -  51.     If 

g  =/         in  51 

=  0         in  (5, 


PROPER  INTEGRALS 
For 


*  *  * 

J  0=J  7+JL* 

«/23          */2i         »£(£ 
But 


and  obviously 


3.    The  reader  should  note  that  the  above  theorem  need  not  be 
true  if  51  is  not  an  unmixed  part  of  33. 

Example.     Let  51  denote  the  rational  points  in  the  unit  square 
8. 

Let 


/  =  9  =  ~  *- 
Then 

^M 


=-L 


4.    Let  Vibe  a  part  of  the  limited  field  $.     Letf^O  be  limited  in 
.     Let  g=f  in  51  and  =  0  in  (£  =  33  -  51. 


//>  r^.  (2 

aar      «^s 

For  let  Jft,  JVt  be  the  maxima  of/,  g  in  the  cell  c?t.     Then 


21 

Passing  to  the  limit  we  get  1). 

To  prove  2)  we  note  that  in  an}^  cell  containing  a  point  of  51 

Min/>  Min  </. 

6.     1.    Letf(x^  "-  xm)  be  limited  in  the  limited  field  51.     Let 
be  an  unmixed  part  of  51  such  that  §M  ==  51  as  u  =  0.      Then 


f/=Hmf/. 

»/2l          "^J^Su 


10  POINT   SETS   AND  PROPER  INTEGRALS 

For  let   /<  Jfin^l.     Let  £  =  51  -  $.     Then 


But 

by  4,  1),  5). 


Hence  passing  to  the  limit  u  =  0  in  2)  we  get  1). 

2.  We  note  that  1  may  be  incorrect  if  the  $&u  are  not  unmixed. 
For  let  51  be  the  unit  square.  Let  $QU  be  the  rational  points  in  a 
concentric  square  whose  side  is  1  —  u.  Let/=  1  for  the  rational 
points  of  51  and  =  2  for  the  other  points.  Then 


ff-2          limff-l 
L/--»        „=*!  /-i. 


7.    In  I,  716  we  have  given  a  uniform  convergence  theorem 
when  each  33M  <  5(.     A  similar  theorem  exists  when  each  33  M  >. 
viz.  : 


33M  <  33M,  ^7  M  <  t/.     .L^  51  be  a  part  of  each  $u.     Let  <gM  = 
as  u  ==  0.      Then  for  each  e>  0,  there  exists  a  pair  %0,  dQ  such  that 


For  Stto  <  1  +  ^,         %  sufficiently  small. 

2 

Also  for  any  division  D  of  norm  ^  <  some  d0. 


»^  z><#«0+ |- 
But 

Hence 


8.  1.  Let  51  be  a  point  set  in  m  =  r  +  s  way  space.  Let  us  set 
certain  coordinates  as  xr+l .» xm=  0  in  each  point  of  51.  The 
resulting  points  53  we  call  a  projection  of  51-  The  points  of  51 


PROPER  INTEGRALS  11 

belonging  to  a  given  point  b  of  33,  we  denote  by  (£6  or  more  shortly 
by  (5-     We  write 

*  =  «•€, 

and  call  33,  &  components  of  51. 

We  note  that  the  fundamental  relations  of  I,  733 


hold  not  only  for  the  components  £,  $,  etc.,  as  there  given,  but 
also  for  the  general  components  21,  33. 

In  what  follows  we  shall  often  give  a  proof  for  two  dimensions 
for  the  sake  of  clearness,  but  in  such  cases  the  form  of  proof  will 
admit  an  easy  generalization.  In  such  cases  33  will  be  taken  as 
the  ^-projection  or  component  of  21- 

2.    7f  21  =  33  •  (£  is  limited  and  33  is  discrete,  21  is  also  discrete. 

For  let  21  lie  within  a  cube  of  edge  J  (7  >  1  in  m  —  r  +  s  way 
space.  Then  for  any  d  <  some  d^ 


Then  1^  <  0s®  D  <  e. 

3.    That  the  converse  of  2  is  not  necessarily  true  is  shown  by 
the  two  following  examples,  which  we  shall  use  later  : 

Example  1.     Let  2(  denote  the  points  re,  y  in  the  unit  square 
determined  thus  : 

For 

0»~,         n=l,  2,  3,  ..-,         m  odd  and  <  2n, 

let 

' 


Here  21  is  discrete,  while  33  =  1,  where  33  denotes  the  projection 
of  21  on  the  z-axis. 

4.    Example  2.     Let  21  denote  the  points  x<  y  in  the  unit  square 
determined  thus  : 


12  POINT  SETS   AND   PROPER  INTEGRALS 

For 

/yy* 

x  =  —,         m,  n  relatively  prime, 
ft 

let  1 

o<,<l. 

Then,  33  denoting  the  projection  of  5l  on  the  #-axis,  we  have 
f=0,         #  =  1. 

9.    1.    Let  91  =  $  •  (£  be  a  limited  point  set.      Then 


For  let/=l  in  5L     Let  g  =  l  at  each  point  of  51  and  at  the 
other  points  of  a  cube  A  =  B  -  0  containing  51,  let  g  =  0.     Then 


By  I,  733,  ' 
But  by  5,  4, 


Thus 


which  gives  1),  since 


2.    7/i  case  51  ^s  metric  we  have 

S=J8S,  (2 

is  an  integrable  function  over  3$. 
This  follows  at  once  from  1). 


PROPER  INTEGRALS  13 

3.  In  this  connection  we  should  note,  however,  that  the  converse 
of  2  is  not  always  true,  i.e.  if  (£  is  integrable,  then  51  has  content 
and  2,  2)  holds.  This  is  shown  by  the  following  : 

Example.     In  the  unit  square  we  define  the  points  x,  y  of  51  thus  : 
For  rational  x, 


For  irrational  x,  1  <     <  1 

Then  (£  =  J  for  every  x  in  23.     Hence 


But  51  =  0,        51  =  1. 

10.    1.    Letf(xl  •••  x^  be  limited  in  the  limited  field  51  =  23 


Let  us  first  prove  1).  Let  51,  23,  £  lie  in  the  spaces  9?m,  9^  9?a, 
r  +  s  =  m.  Then  any  cubical  division  D  divides  these  spaces  into 
cubical  cells  c?t,  d[,  d['  of  volumes  d,  cZ',  d"  respectively.  Ob 
viously  d  =  d'd".  D  also  divides  23  and  each  Q.  into  unmixed  cells 
8',  8".  Let  ^t  =  Max/  in  one  of  the  cells  d»  while  JtfJ'  =  Max/ 
in  the  corresponding  cell  &['.  Then  by  2,  4, 


since  M«  M'  >  0.     Hence 

p'jT/<| 

Letting  the  norm  of  D  converge  to  zero,  we  get  1).     We  get 
2)  by  similar  reasoning  or  by  using  3,  3  and  1). 


14  POINT  SETS   AND  PROPER  INTEGRALS 

2.  To  illustrate  the  necessity  of  making/ >0  in  1),  let  us  take 
51  to  be  the  Pringsheim  set  of  I,  740,  2,  while  /  shall  =  -  1  in  51. 
Then 


On  the  other  hand 
Hence 
and  the  relation  1)  does  not  hold  here. 

Iterable  Fields 

11.    1.    There  is  a  large  class  of  limited  point  sets  which  do  not 
have  content  and  yet  — 

«=(*£.  (1 

•£» 

Any  limited  point  set  satisfying  the  relation  1)  we  call  iterable, 
or  more  specifically  iterable  with  respect  to  33- 

Example  1.     Let  51  consist  of  the  rational  points  in  the  unit 
square.     Obviously  —          —  _ 

8=  f<£=  fg»l, 

ji/33  ji/Q£ 

so  that  5(  is  iterable  both  with  respect  to  33  and  (£. 

Example  2.     Let  51  consist  of  the  points  x,  y  in  the  unit  square 

defined  thus : 

For  rational  x  let      0  <  y  <  1. 
For  irrational  x  let    0  <  y  <  1. 

Here     1  =  1. 


Thus  51  is  iterable  with  respect  to  (£  but  not  with  respect  to  33- 


ITERABLE   FIELDS  15 

Example  3.     Let  51  consist  of  the  points  in  the  unit  square  de 

fined  thus:  ,,  .       i      -I  .       A  ^     ^  o 

b  or  rational  x  let      0  <  y  <  |. 

For  irrational  a;  let  -J  <  ?/  <  1. 
Here  51  =  1,  while     - 


Hence  51  is  iterable  with  respect  to  d  but  not  with  respect  to  33. 

Example  4-     Let  51  consist  of  the  sides  of  the  unit  square  and 
the  rational  points  within  the  square. 
Here  51  =  1,  while 


and  similar  relations  for  (L     Thus  51  is  not  iterable  with  respect 
to  either  33  or  (£. 

Example  5.     Let  51  be  the  Pringsheim  set  of  I,  740,  2. 
Here  51  =  1,  while 


Hence  51  is  not  iterable  with  respect  to  either  33  or  Q. 

2.   Every  limited  metric  point  set  is  iterable  with  respect  to  any  of 

its  projections. 

This  follows  at  once  from  the  definition  and  9,  2. 

12.  1.  Although  51  is  not  iterable  it  may  become  so  on  remov 
ing  a  properly  chosen  discrete  set  £). 

Example.  In  Example  4  of  11,  the  points  on  the  sides  of  the 
unit  square  form  a  discrete  set  £)  ;  on  removing  these,  the  deleted 
set  51*  is  iterable  with  respect  to  either  33  or  (£. 

2.  The  reader  is  cautioned  not  to  fall  into  the  error  of  suppos 
ing  that  if  5lx  and  5^  are  unmixed  iterable  sets,  then  51  =  5lj  +  512 
is  also  iterable.  That  this  is  not  so  is  shown  by  the  Example  in  1. 

For  let  5ti  =  51*,  512=  1)  in  that  example.  Then  £5  being  dis 
crete  has  content  and  is  thus  iterable.  But  5(  =  5^  -h  512  is  not 
iterable  with  respect  to  either  33  or  (L 


16  POINT   SETS  AND   PROPER  INTEGRALS 

13.  1.  Let  51  be  a  limited  point  set  lying  in  the  m  dimensional 
space  ffim.  Let  33,  (£  be  components  of  51  in  9?r,  9^,  r  +  s  =  m. 
A  cubical  division  D  of  norm  8  divides  3?OT  into  cells  of  volume 
d  and  9?r  and  9?s  into  cells  of  volume  dr,  d#  where  d  =  drds.  Let 
b  be  any  point  of  33,  lying  in  a  cell  dr.  Let  ^ds  denote  the  sum 

6 

of  all  the  cells  ds,  containing  points  of  51  whose  projection  is  b. 
Let  2c?5  denote  the  sum  of  all  the  cells  containing  points  of  51 

dr 

whose  projection  falls  in  dr,  not  counting  two  da  cells  twice. 
We  have  now  the  following  theorem  : 
If  51  is  iterable  with  respect  to  33> 


F°r 
Hence 


Let  now  8=0.  The  first  and  third  members  =  51,  using  I,  699, 
since  51  is  iterable.  Thus,  the  second  and  third  members  have 
the  same  limit,  and  this  gives  1). 

2.  If  51  is  iterable  with  respect  to  33» 

lim  2dr2d.  =  g. 

fi=o   33      6 

This  follows  at  once  from  1). 

3.  Let  51  =  33  •  (5  be  a  limited  point  set,  iterable  with  respect  to  33- 
Then  any  unmixed  part  &  of  51  is  also  iterable  with  respect  to  the 
^-component  o 


For  let  b  =  a  point  of  33  ;  (5'  points  of  51  not  in  (5  ;  Cb=  points 
of  @j  in  (5,  (7^  =  points  of  (E6  in  (£'.  Then  for  each  @>Q  there 
exist  a.  pair  of  points,  bv  52,  distinct  or  coincident  in  any  cell  dr 
such  that  as  b  ranges  over  this  cell, 

+  /3',     C  =  Max  Ob  +  13", 


ITERABLE   FIELDS  17 

Let  S  denote,  as  in  13,  l,  the  cells  of  2c£,  which  contain  points  of  G?', 

and  F  the  cells  containing  points  of  both  (5,  &  whose  projections 
fall  in  dr.     Then  from 

Cb^C'^<Cb^S<Cb 
we  have 

5*,  <  Obi  +  Cbi  <  Min  Cb  +  /3'  +  #<  Max 
Multiplying  by  c?r  and  summing  over  33  we  have, 
i  <  2  rfr  Min  ^  +  2  £;dr  4-  (!i  <  2  d  r  Max  <76 


Passing  to  the  limit,  we  have 

+  7;"  +  S<i,  (2 


the  limit  of  the  last  term  vanishing  since  (5,  ($'  are  unmixed  parts 
of  21.  Here  r)',  rjrf  are  as  small  as  we  please  on  taking  0  sufficiently 
small.  From  2)  we  now  have 


f  (7=S-(!'  = 
J 


4.  Let  51  =  33  •  £  £e  iterable  with  respect  to  33.  Ze£  £  be  a  part 
of  33  a/ic?^l  aZ£  those  points  of  21  wA0S£  projection  falls  on  B.  Then 
A  is  iterable  with  respect  to  B. 

For  let  D  be  a  cubical  division  of  space  of  norm  d.     Then 


where  the  sum  on  the  right  extends  over  those  cells  containing 
no  point  of  A.     Also 


where  the  second  sum  on  the  right  extends  over   those    cells  dr 
containing  no  point  of  B. 
Subtracting  1),  2)  gives 

0  =  lim  {  AD  -  ZdM]  +  lim  {  ^drds  - 

d=U    I  B  »          d=&    ^r.s 


18  POINT   SETS   AND   PROPER   INTEGRALS 

As  each  of  the  braces  is  >  0  we  have 


14.    We  can  now  generalize  the  fundamental  inequalities  of  I, 
733  as  follows  : 

Let  /(#!  ...  xm)  be  limited  in  the  limited  field  $  =  23  •  (5,  iterable 
with  respect  to  33-      Then 


For  let  us  choose  the  positive  constants  A,  B  such  that 


,          n  31. 

Let  us  effect  a  cubical  division  of  the  space  of  $ftm  of  norm  8  into 
cells  d.  As  in  13,  this  divides  9^.,  $ts  into  cells  which  we  denote, 
as  well  as  their  contents,  by  c?r,  ds.  Let  b  denote  any  point  of  33. 
As  usual  let  w,  M  denote  the  minimum  and  maximum  of  /  in  the 
cell  d  containing  a  point  of  31.  Let  ra',  M'  be  the  corresponding 
extremes  of  /  when  we  consider  only  those  points  of  51  in  d  whose 
projection  is  b.  Let  |/|  <  F  in  $. 
Then  for  any  b,  we  have  by  I,  696, 


or 

-  B(^ds  -  g)  +  ^mds  <  )J,  (2 

since  m^m1. 

In  a  similar  manner 


-<£)•  (3 

Thus  for  any  b  in  33,  2),  3)  give 


6 


Let  /3  >  0  be  small  at  pleasure.     There  exist  two  points  bv  b%  dis 
tinct  or  coincident  in  the  cell  dr,  for  which 


ITERABLE   FIELDS  19 

where  |  ^  ,    /32  1  <  £  and  6X,  and  Ct2  stand  for  (£v  @6j,  and  finally 
where 

,         J-=MaxJ/ 
for  all  points  b  in  <fr. 

Let  c  =  Min  £  in  dr,  then  4)  gives 


,  -  c)  +  2widf  <  y  +  /?!  <  <7  +  /32  <  ^Mds  +  4(2d,  -  c) 

11  22 

where  the  indices  1,  2  indicate  that  in  2  we  have  replaced  b  by 


Multiplying  by  dr  and  summing  over  all  the  cells  dr  containing 
points  of  33,  the  last  relation  gives 


-  0.  (5 

20  50  33      2  33         2 

NOW  aS  8  =  0,  V,7V7      •    O?  V  7  V,7      •    W  1,-IQo 

Zdrz,as  =  51,         2,ar2,as  =  VI,         by  lo,  2. 
33       1  33      2 


=  1  S  =  5t,        since  51  is  iterable. 


Thus  the  first  and  last  sums  in  5)  are  evanescent  with  8.     On 
the  other  hand 


2(dr2d,wi  -  2<*,w)  I  <  F^dr(^ds  -  2ds) 

%        df  I  33        ds  1 

=  0  as  8=0,         by  13,  1. 
Thus 


^ 
lim  2rfr2d,w  =|   /.  (6 


(7 


Hence  passing  to  the  limit  3=0  in  5)  we  get  1),  since  2£1dfr, 
2/32t?r  have  limits  numerically  <yQ(5  which  may  be  taken  as  small 
as  we  please  as  /3  is  arbitrarily  small. 


20  POINT  SETS   AND   PROPER   INTEGRALS 

2.  If  51  is  not  iterable  with  respect  to  33,  let  it  be  so  on  remov 
ing  the  discrete  set  T).     Let  the  resulting  field  A  have  the  com 
ponents  B,  0.     Then  1  gives 

since  -         - 

(/=/>• 
c/51       JA 

3.  The  reader  should  guard  against  supposing  1)  is  correct  if 
only  51  is  iterable  on  removing  a  discrete  set  £).     For  consider 
the  following : 

Example.  Let  the  points  of  51  =  5lx  +  T)  lie  in  the  unit  square. 
Let  5lj  consist  of  all  the  points  lying  on  the  irrational  ordinates. 
Let  £)  lie  on  the  rational  ordinates  such  that,  wrhen 

m,  n  relatively  prime, 
Let  us  define/  over  51  thus  : 


•<„<! 


/=        in     5Ir 

/=0     in     £). 

The  relation  1)  is  false  in  this  case.     For 


//=!, 

^21 


while  — 

f  f  /=°- 

*/s  */e 

15.  1.  Let  /(ajj  •  •  •  #TO)  be  limited  in  the  limited  point  set  51. 
Let  D  denote  the  rectangular  division  of  norm  d.  All  the  points 
of  5t/>  except  possibly  those  on  its  surface  are  inner  points  of  51. 
[1,702.] 

The  limits  Hm  Cf    ,     nm  f  /  (1 

rf=o  «/9i  rf=o  «/2f 

-D  -D 

exist  and  will  be  denoted  by 

/*/  ,  JV  ,  (2 

-^  ^21 

and  are  called  the  inner,  lower  and  upper  integrals  respectively. 


ITERABLE   FIELDS  21 

To  show  that  1)  exist  we  need  only  to  show  that  for  each  6  >  0 
there  exists  a  dQ  such  that  for  any  rectangular  divisions  D1,  D'f  of 
norms  <  d 0  (  -  - 

<€. 


To  this  end,  we  denote  by  E  the  division  formed  by  superimpos 
ing  D"  on  Df.     Then  E  is  a  rectangular  division  of  norm  <  d0. 
T  pf 

«,-!,,  =  4',       *,-«,,  =  4". 

If  d0  is  sufficiently  small,       .,     .„ 

-A  ,  A.     <«  ^ 

an  arbitrarily  small  positive  number.     Then 

A  =  |ff     -/    V-(f    -f 
|V-;^     Jjyy     Wgy   j5 

if  97  is  taken  small  enough. 
2.    The  integrals 


Cf,  f /, 

%/2I  Jw 


heretofore  considered  may  be  called  the  outer,  lower  and  upper  in 
tegrals,  in  contradistinction. 

3.    Let  f  be  limited  in  the  limited  metric  field  51.      Then  the  inner 
and  outer  lower  (upper)  integrals  are  equal. 

For  W.D  is  an  unmixed  part  of  51  such  that 


Then  by  6,  l,  r  r 

limj    /-// 
rf=o  J%D        J% 

But  the  limit  on  the  left  is  by  definition 


4.     When  51  has  no  inner  points, 

JV=o. 

t/SM 


22.  POINT   SETS   AND   PROPER  INTEGRALS 

For  each  $/>  =  0,  and  hence  each 


Point  Sets 

16.  -Le£  51  =  33  +  £  £>e  metric.      Then 

g  =  33  +  g.  (1 

For  let  .Z)  be  a  cubical  division  of  space  of  norm  d.  The  cells 
of  51^  fall  into  three  classes  :  1°,  cells  containing  only  points  of  33; 
these  form  33/>.  2°,  cells  containing  points  of  (£ ;  these  form  &D. 
3°,  cells  containing  frontier  points  of  33,  not  already  included  in  1° 
or  2°.  Call  these  \D.  Then 

^  =  %D  +  &D  +  \D.  (2 

Let  now  d  =  0.  As  51  is  metric,  f^  =  0,  since  \D  is  a  part  of 
Front  51  and  this  is  discrete.  Thus  2)  gives  1). 

17.  1.    Let  51,  33,  G  -  (1 
be  point  sets,  limited  or  not,  and  finite  or   infinite   in   number. 
The  aggregate  formed  of  the  points  present  in  at  least  one  of  the 
sets  1)  is  called  their  union,  and  may  be  denoted  by 

U(K,  33,  (5  •••), 
or  more  shortly  by  ,<*   ™   ^      x 

If  51  is  a  general  symbol  for  the  sets  1),  the  union  of  these  sets 
may  also  be  denoted  by  77  5  91  [ 

or  even  more  briefly  by  r^> 

If  no  two  of  the  sets  1)  have  a  point  in  common,  their  union 
may  be  called  their  sum,  and  this  may  be  denoted  by 

51  +  33  +  S+  - 

The  set  formed  of  the  points  common  to  all  the  sets  1)  we  call 
their  divisor  and  denote  by 


POINT   SETS  23 


if  51  is  a  general  symbol  as  before. 

2.    Examples. 

Let  51  be  the  interval  (0,  2);   S3  the  interval  (1,  oo).      Then 

Z7(2l,  «)  =  (0,  oo),         Dv($(,  33)  =  (1,  2). 
Let  ^  =  (0,  1),         5I2  =  (1,  2).-. 

Then 


Let        ^=(1,  i),      5i2=(i  j),      5 

Then  ^(512,512-0  =  (0*,  1), 

!)»(«!,  «a  -)  =  0. 

Let      *i  = 
Then 

3'    Let 

Let 

Let  21  =  ^  +  ^,  2li  =  ^2  +  ^- 

Then  21  =  -D  +  (E!  +  (£2  H-  - 

Let  us  first  exclude  the  =  sign  in  1).  Then  every  element  of 
51  which  is  not  in  £)  is  in  some  5ln  but  not  in  5ln+r  It  is  therefore 
in  (EB+1  but  not  in  £n+2>  £n+3^  "•  The  rest  now  follows  easily. 

4.  Some  writers  call  the  union  of  two  sets  51,  53  their  sum, 
whether  51,  33  have  a  point  in  common  or  not.  We  have  not  done 
this  because  the  associative  property  of  sums,  viz.  : 


does  not  hold  in  general  for  unions. 


24  POINT  SETS  AND  PROPER  INTEGRALS 

Example.     Let         51  =  rectangle  (1234), 

<8  =  (5678), 

(£  =  (5  8  «  /3)  = 
Then  0W» 

and  (OX*  »)-<£),  (2 

are  different. 

Thus  if  we  write  -f-  for  £7",  1),  2)  give 


18.    1.    -Le£  511>512>513  "*  ^e  a  8e^  °/  limited  complete  point 
aggregates.     Then 

33  =  ^(51!,  512  -'OX)' 
Moreover  33  as  complete. 

Let  an  be  a  point  of  3ln,  w  =  1,  2,  ...  and  51  =  «p  «2'  ^3  '** 
Any  limiting  point  a  of  51  is  in  every  5ln.     For  it  is  a  limit 
ing  point  of 


But  all  these  points  lie  in  5lm,  which  is  complete.  Hence  a  lies  in 
5lm,  and  therefore  in  every  y(v  $[2,  •••  Hence  a  lies  in  23,  and 
»  >  0. 

33  i*  complete.     For  let  /3  be  one  of  its  limiting  points.     Let 


V     2'     3'  - 

As  each  bm  is  in  each  2ln,  and  5(n  is  complete,  y8  is  in  5ln-     Hence  ft 
is  in  33- 

2.    Let  W.  be  a  limited  point  set  of  the  second  species.      Then 


s  complete. 
For  5((n)  is  complete  and  >  0.     Also  5l(n)  .> 


19.  i««  5lr  212  •••  &«  *^  33;  let  51  =  ^7S5lni.  i«<  An  be  the  com 
plement  of  5ln  with  respect  to  33>  so  that  An  +  2In  =  33-  ^ 
^1  =  Dv\An\  .  Then  A  and  51  are  complementary,  so  that  A  4-  51  =  33 


POINT   SETS  25 

For  each  point  b  of  33  lies  in  some  5ln,  or  it  lies  in  no  5In,  and 
hence  in  every  An.  In  the  first  case  b  lies  in  51,  in  the  second  in 
A.  Moreover  it  cannot  lie  in  both  A  and  51- 

20.    1.    Let  2lj  <512<  513  •••  (1 

be  an  infinite  sequence  of  point  sets  whose  union  call  51.     This 
fact  may  be  more  briefly  indicated  by  the  notation 


Obviously  when  51  is  limited, 

1  >  lim  ln.  (2 

That  the  inequality  may  hold  as  well  as  the  equality  in  2)  is 
shown  by  the  following  examples. 

Example  1.     Let  5ln  =  the  segment  (-,  1  ]  • 

\H       I 

Then  5l  =  Z7j5U  =  (0*,  1). 


Example  2.     Let  an  denote  the  points  in  the  unit  interval  whose 
abscissae  are  given  by 

x  =  —  ,  m  <  n  =  1,  2,  3,  •••  m,  n  relatively  prime. 
n 

Let  5ln  =  a  +  -  +  an. 

Here  2i 

is  the  totality  of  rational  numbers  in  (0*,  1*). 

A  c 

21  =  1  and  5ln  =  0,  we  see 

51  >  lim  ln. 

2.    Let  «i>_«2>- 

Let  33  be  their  divisor.     This  we  may  denote  briefly  by 


Obviously  when  33X  is  limited, 

8  <  lim  Sn. 


26  POINT   SETS  AND   PROPER  INTEGRALS 

Example  1.     Let  33n  =  the  segment  ( 0,  -V 

Then  ^  =  ^533^  =  (0),   the  origin. 

Here  • •  •      1 

n 

and  S  =  lim  gn. 

Example  2.     Let  2ln  be  as  in  1,  Example  2.     Let  bn  =  21  —  2ln. 

$A      —  f~\     9^\  _l_  fi 

Here  ^  _  the  gegment  (^  2)  and  «„  =  2. 

Hence  g  <  lim  ».. 

3.    ie^  33j  <  332  <  •••  ^^  unmixed  parts  of  21.     -£e£  Sn  =  21. 
LJ.     Then  (£  =  21  —  33  i*  discrete. 


For  let  31  =  $n  +  (£n  ;  then  (5n  is  an  unmixed  part  of  21.     Hence 

s=sw+c. 

Passing  to  the  limit  n  =  oo,  this  gives 

limgn=0. 
Hence  (5  is  discrete  by  2. 

4.  We  may  obviously  apply  the  terms  monotone  increasing, 
monotone  decreasing  sequences,  etc.  [Cf.  1,  108,  211]  to  sequences 
of  the  type  1),  3). 


21.    Let&  =  2(  +  33.     If  51,  33  are  complete, 

£  =  S+S.  (1 

For  S  =  Dist  (21,  33)  >  0, 

since  21,  33  are  complete  and  have  no  point  in  common.  Let  D  be 
a  cubical  division  of  space  of  norm  d.  If  d  is  taken  sufficiently 
small  2l/),  33/>  have  no  cells  in  common.  Hence 


Letting  d=  0  we  get  1). 


POINT   SETS  27 

22.    1.   If  51,  33  fl/*e  complete,  so  are  also 
£  =(21,33),        £) 


Let  us  first  show  that  £  is  complete.  Let  c  be  a  limiting  point 
of  £.  Let  Cj,  £2,  ••«  be  points  of  (5  which  =  c.  Let  us  separate 
the  cn  into  two  classes,  according  as  they  belong  to  51,  or  do  not. 
One  of  these  classes  must  embrace  an  infinite  number  of  points 
which  =  c.  As  both  51  and  33  are  complete,  c  lies  in  either  51  or 
33-  Hence  it  lies  in  g. 

To  show  that  £)  is  complete.  Let  dv  d2,  •••  be  points  of  £)  which 
=  d.  As  each  dn  is  in  both  5(  and  33,  their  limiting  point  d  is  in 
51  and  33,  since  these  are  complete.  Hence  d  is  in  £). 

2.    If  51,  23  are  metric  so  are 


For  the  points  of  Front  £  lie  either  in  Front  51  or  in  Front  33, 
while  the  points  of  Front  £)  <  Front  51  and  also  <  Front  33.  But 
Front  5(  and  Front  33  are  discrete  since  51,  33  are  metric. 

23.  Let  the  complete  set  51  have  a  complete  part  33.  Then  hoiv- 
ever  small  e  >  0  is  taken,  there  exists  a  complete  set  &  in  51,  having  no 
point  in  common  with  33  such  that 

£>5(-5-e.  (1 

Moreover  there  exists  no  complete  set  d,  having  no  point  in  common 
with  33  such  that 


The  second  part  of  the  theorem  follows  from  21.  To  prove  1) 
let  D  be  a  cubical  division  such  that 

5^=51  +  6',         ^  =  2)  +  e",         0<e',  €"<e.  (2 

Since  33  is  complete,  no  point  of  33  lies  on  the  frontier  of  33z>- 
Let  £  denote  the  points  of  51  lying  in  cells  containing  no  point  of 
33.  Since  51  is  complete  so  is  (S,  and  33,  (£  have  no  point  in  common. 

Thus 

.  (3 


28  POINT  SETS  AND  PROPER  INTEGRALS 

But  the  cells  of  &D  may  be  subdivided,  forming  a  new  division  A, 
which  does  not  change  the  cells  of  $QD,  so  that  $8D  =  $3A,  but  so  that 

1A  =  !  +  €'",         0<e'"<€.  (4 

.     Thus  2),  3),  4)  give 


24.    Let  51,  33  be  complete.     Let 


Forlet  II  =  51  +  A. 

Then  A  contains  complete  sets  (7,  such  that 

^>U-S-e,  (2 

but  no  complete  set  such  that 

c>u-a,  (3 

by  23.     On  the  other  hand, 

»*A  +  $. 

Hence  ^4  contains  complete  sets  (7,  such  that 

a>®-s>-€,  (4 

but  no  complete  set  such  that 

<7>S-£.  (5 

From  2),  3),  and  4),  5)  we  have  1),  since  6  is  arbitrarily  small. 

25.    Let 


each  $n  being  complete  and  such  that  5ln  >  some  constant  k. 
Then 


POINT   SETS  29 

For  suppose  l  =  k-®>0. 

Let  Z  =  e+7,;          e,  7,>0. 

Then  by  23  there  exists  in  5lj  a  complete  set  Q^,  having  no  point 
in  common  with  £)  such  that 

Sj  >  Sj  -  T)  -  e  ; 
or  as  5tj  >  A:,  such  that  ^  > 

Let  (5,),         U  =  (2I2,  eO- 


by  24, 
Thus 


Thus  $2  contains  the  non-vanishing  complete  set  @2  having  no 
point  in  common  with  £).  In  this  way  we  may  continue.  Thus 
5Ir  $2,  •••  contain  a  non-vanishing  complete  component  not  in  £), 
which  is  absurd. 

Corollary.     Let  31  =  (5Ij<  512<  •••)  Je  complete.      Then  Sn  =  3. 
This  follows  easily  from  23,  25. 


CHAPTER   II 
IMPROPER  MULTIPLE  INTEGRALS 

26.  Up  to  the  present  we  have  considered  only  proper  multiple 
integrals.     We  take  up  now  the  case  when  the  integrand  f(x1  -  •  •  xm) 
is  not  limited.     Such  integrals  are  called  improper.     When  m  =  1, 
we  get  the  integrals  treated  in  Vol.  I,  Chapter  14.     An  important 
application  of  the  theory  we  are  now  to  develop  is  the  inversion 
of  the  order  of  integration  in  iterated  improper  integrals.     The 
treatment  of  this  question  given  in  Vol.  I  may  be  simplified  and 
generalized  by  making  use  of  the  properties  of  improper  multiple 
integrals. 

27.  Let  51  be  a  limited  point  set  in  w-way  space  $lm.     At  each 
point  of  51  let  f(x1  •••#m)  have  a  definite  value  assigned  to  it. 
The  points  of  infinite  discontinuity  of  /  which  lie  in  51  we  shall 
denote  by  $.     In  general  $  is  discrete,  and  this  case  is  by  far  the 
most  important.     But  it  is  not  necessary.     We  shall  call  $  the 
singular  points. 

Example.     Let  51  be  the  unit  square.     At  the  point  #  =  —, 

y  =  -,  these  fractions  being  irreducible,  let  f=ns.     At  the  other 
s 

points  of  51  let  /=  1.     Here  every  point  of  51  is  a  point  of  infinite 
discontinuity  and  hence  Q  =  51- 

Several  types   of  definition  of   improper  integrals  have  been 
proposed.     We  shall  mention  only  three. 

28.  Type  I.     Let  us  effect  a  division  A  of  norm  8  of  9?m  into 
cells,  such  that  each  cell  is  complete.     Such  divisions  may  be 
called  complete.     Let  515  denote  the  cells  containing  points  of  51, 
but  no  point  of  Q ,  while  5l§  may  denote  the  cells  containing  a 
point  of  $•     Since  A  is  complete,  /  is  limited  in  5ls-     Hence  / 
admits  an  upper  and  a  lower  proper  integral  in  5ls«     The  limits, 

when  they  exist,  -^ 

lim   f  /,         lim   )    /,  (1 

6=0  c/2l  5=0  ^21 


GENERAL  THEORY  31 

for  all  possible  complete  divisions  A  of  norm  S,  are  called  the 
lower  and  upper  integrals  of  /  in  51,  and  are  denoted  by 


CfdK, 
« 


(2 
«l  «* 

or  more  shortly  by 


/• 


When  the  limits  1)  are  finite,  the  corresponding  integrals  2) 
are  convergent.  We  also  say/  admits  a  lower  or  an  upper  improper 
integral  in  51-  When  the  two  integrals  2)  are  equal,  we  say  that 
/  is  integrable  in  51  and  denote  their  common  value  by 


or  by         J/.  (3 


We  call  3)  the  improper  integral  of  f  in  51  ;  we  also  say  that 
/  admits  an  improper  integral  in  51  and  that  the  integral  3)  is 

convergent. 

The  definition  of  an  improper  integral  just  given  is  an  extension 
of  that  given  in  Vol.  I,  Chapter  14.  It  is  the  natural  develop 
ment  of  the  idea  of  an  improper  integral  which  goes  back  to  the 
beginnings  of  the  calculus. 

It  is  convenient  to  speak  of  the  symbols  2)  as  upper  and  lower 
integrals,  even  when  the  limits  1)  do  not  exist.  A  similar  remark 
applies  to  the  symbol  3). 

Let  us  replace  /by  l/|  in  one  of  the  symbols  2),  3).  The 
resulting  symbol  is  called  the  adjoint  of  the  integral  in  question. 
We  write 

(4 


When  the  adjoint  of  one  of  the  integrals  2),  3)  is  convergent, 
the  first  integral  is  said  to  be  absolutely  convergent.  Thus  if  4)  is 
convergent,  the  second  integral  in  2)  is  absolutely  convergent,  etc. 

29.  Type  II.  Let  X,  /u,>0.  We  introduce  a  truncated  func 
tion  /Afx  defined  as  follows  : 

/AM  =/Oi  •••#»)  when  -  X  </<  /* 
=  —  X  when  /  <  —  X 

=  p  when  /  >  fjL. 


32  IMPROPER  MULTIPLE   INTEGRALS 

We  define  now  the  lower  integral  as 

c  c 

J  f  =  Iim  J  /AM. 

A  similar  definition  holds  for  the  upper  integral.  The  other 
terms  introduced  in  28  apply  here  without  change. 

This  definition  of  an  improper  integral  is  due  to  de  la  Vallee 
Poussin.  It  has  been  employed  by  him  and  R.  G-.  D.  Richardson 
with  great  success. 

30.  Type  III.     Let  a,  /3  >  0.     Let  5la/3  denote  the  points  of  51 

We  define  now 

f /  =  Iim  f    f     ;       f /  =  Km    f    /.  (1 

tl2l  a,/3  =  °o^la/3  ^21  •,0—>*/*«0 

The  other  terms  introduced  in  28  apply  here  without  change. 
This  type  of  definition  originated  with  the  author  and  has  been 
developed  in  his  lectures. 

31.  When  the  points  of  infinite  discontinuity  -3  are  discrete 
and  the  upper  integrals  are  absolutely  convergent,  all  three  defini 
tions  lead  to  the  same  result,  as  we  shall  show. 

When  this  condition  is  not  satisfied,  the  results  may  be  quite 
different. 

Example.  Let  51  be  the  unit  square.  Let  5lr  512  denote  respec 
tively  the  upper  and  lower  halves.  At  the  rational*  points  53, 

x  =  —,  y  =  ~,  in  5L,  let/=  ns.     At  the  other  points  (£  of  5lr  let 
n    '       s 


/=-2.     In  51 

1°  Definition.     Here 
Hence 

2°  Definition.     Here 

T  . 

-  +  oo. 


*  Here  as  in  all  following  examples  of  this  sort,  fractions  are  supposed  to  be 
irreducible. 


GENERAL   THEORY  33 

3°  Definition.     Here  3la/3  embraces  all  the  points  of  2J2,  £  and  a 
finite  number  of  points  of  33  for  a  >  2,  /3  arbitrarily  large.     Hence 

//=-!,        //=-!, 

*£i  ^n 

and  thus 


32.  In  the  following  we  shall  adopt  the  third  type  of  definition, 
as  it  seems  to  lead  to  more  general  results  when  treating  the  im 
portant  subject  of  inversion  of  the  order  of  integration  in  iterated 
integrals. 

We  note  that  if /is  limited  in  21, 

lim     I  /  =  the  proper  integral   1  /. 

a, /3=»_2l  ^l2l 

For  a,  ft  being  sufficiently  large,  2la/J  =  21- 
Also,  if  31  is  discrete, 

//=//=  °- 

For  2la8  is  discrete,  and  hence 
r 

Hence  the  limit  of  these  integrals  is  0. 


33.    Let          m=|Min/|     ,     JJf=|Max/|     in  51. 
Then  -  - 

lim    I     /  =  lim  I       /,         m  finite. 
a,/3=oc^2laj3          ft-»*?Mm,p 

lim    f   /=lim  f      /,         M  finite. 

+fi-<*!mmj      a=^2ia)J/ 

For  these  limits  depend  only  on  large  values  of  a,  ft,  and  when 

is  finite. 

$OT  ^  =  $a ^     ,     for  all  a  >  7/1. 

Similarly,  when  Mis  finite 

^.6  =  3L*         f  or  all  /3  >  M. 


34  IMPROPER  MULTIPLE   INTEGRALS 

Thus  in  these  cases  we  may  simplify  our  notation  by  replacing 

CUT  (\f 

2U,  Jit       »        2im/3 
bj  3L.        ,        %ft        , 

respectively. 

2.  Thus  we  have: 

Xf  =  lim  I    /,         when  Min/  is  finite. 
j    *~A£ 

>  J  /  =  lim  J  /  ,         when  Max/  i«  finite. 

3.  Sometimes  we  have  to  deal  with  several  functions  /,#,  •  •• 
In  this  case  the  notation  5la/3  is  ambiguous.     To  make  it  clear  we 
let  21/,  a>  p  denote  the  points  of  51  where 


Similarly,  51^,  a>  ^  denotes  the  points  where 


34.     I    f  is  a  monotone  decreasing  function  of  a  for  each  ft. 
*f*«i 

I    f  is  a  monotone  increasing  function  of  ft  for  each  a. 
J**fi 

If  Max  /  is  finite 

|    /  are  monotone  decreasing  functions  of  a. 

•/«-« 

If  Uin  fit  finite 

I    /  are  monotone  increasing  functions  of  ft. 
J*e 

Let  us  prove  the  first  statement.     Let  a'  >  a. 
Let  D  be  a  cubical  division  of  space  of  norm  d. 
Then  ft  being  fixed, 

(    /=  lirn  2  wtc?t,  (1 

•f«M  <*=«    2la/3 

f   /=lim2w;^;,  (2 

•/tU'/l  rf=°    «a'^ 

using  the  notation  so  often  employed  before. 


GENERAL   THEORY  35 

But  each  cell  dt  of  5la/3  lies  among  the  cells  dj  of  2L  /s.     Thus  we 
can  break  up  the  sum  2),  getting 


Here  the  second  term  on  the  right  is  summed  over  those  cells 
not  containing  points  of  5la/3.  It  is  thus  <  0.  In  the  first  term 
on  the  right  ml  <mL.  It  is  thus  less  than  the  sum  in  1).  Hence 


Thus 


L^L: 


«'>«. 


In  a  similar  manner  we  may  prove  the  second  statement  ;  let 
us  turn  to  the  third. 

We  need  only  to  show  that 

|    /  is  monotone  decreasing. 
J2l_'a 

Let  «'>«.     Then 

=  lim  SJIf^.  (3 


As  before  'S.M'd'  =  ^M'd'  +  ^Mndn  f 5 

*-•  «-/ 

But  in  the  cells  d,,  MJ  =  ML.  Hence  the  first  term  of  5)  is 
the  same  as  2  in  3).  The  second  term  of  5)  is  <0.  The  proof 
follows  now  as  before. 

35.    If  Max  /  is  finite  and  I  fare  limited,  I  f  is  convergent  and 

_5tt  ^_2l 

f/<  f  /. 

•/•          j/2T_a 

If  Min  f  is  finite  and  I    are  limited,  I   tf  t«  convergent  and 


36  IMPROPER  MULTIPLE   INTEGRALS 

For  by  34  - 

f      /     ,     f   / 
J«L.  J** 

are  limited  monotone  functions.     Their  limits  exist  by  I,  277,  8. 
36.    If  M=  Max/  is  finite,  and  Jf  is  convergent,  the  correspond 
ing  upper  integral  is  convergent  and 


where  f  >_  —  a  in  5Ltt. 

Similarly,  if  m  =  Min  /  is  finite  and  J  f  is  convergent,  the  corre 
sponding  lower  integral  is  convergent  and 


Let  us  prove  the  first  half  of  the  theorem. 

We  have  /*  7* 

I  /=  lim  I 

Jjf  a=»J5l_a 

Now 


We  have  now  only  to  pass  to  the  limit. 
37.    If  if  is  convergent,  and  $8  <  51, 

" 


does  not  need  to  converge.     Similarly 


_ 

does  not  need  to  converge,  although  I  /  does. 

Example.     Let  21  be  the  unit  square  ;  let  8  denote  the  points 
for  which  x  is  rational. 


GENERAL   THEORY 

when  x  is  irrational 
when  x  is  rational 


37 


Then 


/=  1 

=  - 

y 

r  r 

I    /=!     ;      hence   I  /=!. 
J«/  Jtf 

On  the  other  hand, 


Hence 
is  divergent. 


X=  lim  I    =  lim  log  &  =  +  oo 
i       s=*  ^»s 


38.  1.  In  the  future  it  will  be  convenient  to  let  ty  denote  the 
points  of  51  where />  0,  and  9?  the  points  where/ <.  0.  We  may 
call  them  the  positive  and  negative  components 


2.    If  J  /converges,  so  do  \  f. 

If  I  /  converges,  so  do  I  /. 
*/H  *AR 


For  let  us  effect  a  cubical  division  of  space  of  norm  d.  Let 
fi'  >  /3.  Let  e  denote  those  cells  containing  a  point  of  ^  ;  e' 
those  cells  containing  a  point  of  ^  but  no  point  of  ^  ;  5  those 
cells  containing  a  point  of  9la/3  but  none  of  ^,. 

Then 


=  limJS^f. 

*/2la/3          d=0 


SJ. 


Obviously 
Hence 


,    M,,<0. 


~  ~ 

\      -\     »li 

^2l'         ^ 


38  IMPROPER  MULTIPLE  INTEGRALS 

We  find  similarly 

f    -  f   =lim{2(^-Jf.>  +  2JfXi- 
*Ap/3/         ^?B      d=° 

Now 


I          - 

ML* 


< 


for  a  sufficiently  large  a,  and  for  any  &  £'  >  j3Q. 
Hence  the  same  is  true  of  the  left  side  of  1). 

As  corollaries  we  have  : 

3.    If  the  upper  integral  off  is  convergent  in  51,  then 


If  the  lower  integral  off  is  convergent  in 


For 


< 


etc. 


4.    -?//  >:  0  ancZ   I  /  is  convergent,  so  is 
»/5l 


(1 


Moreover  the  second  integral  is  <  the  first. 
This  follows  at  once  from  3,  as  51  =  ty. 

39.    If  J  /  and  J  f  converge,  so  do  J  /. 

We  show  that  I  /  converges  ;  a  similar  proof  holds  for  I  . 

*/2t  ?±2l 

this  end  we  have  only  to  show  that 


e>0; 


L  -L 


<e;   «<«'<«", 


To 


(1 


GENERAL   THEORY  39 

Let  D  be  a  cubical  division  of  space  of  norm  d.  Let  typ  ,  typ- 
denote  cells  containing  at  least  one  point  of  2la'|8'  ,  2la"/j"  at  which 
/>0.  Let  tta-  i  tla"  denote  cells  containing  only  points  of  2la-/3'  , 
2la-0"  at  which/<  0.  We  have 


Subtracting, 

(2 


Let  jjf  [  =  Max  /  for  points  of  ^  in  c?t.     Then  since  /  has  one 
sign  in  9fc, 


|  .  (3 


Letting  d  =  0,     2)  and  3)  give 


" 


Now  if  13  is  taken  sufficiently  large,  the  first  term  on  the  right  is 
<  6/2.     On  the  other  hand,  sincej   /  is  convergent,  so  is  J  /  by 

36.     Hence  for  a  sufficiently  large,  the  last  term  on  the  right  is 
<e/2.     Thus  4)  gives  1). 

40.    Iff  is  integrable  in  21,  it  is  in  any  $3  <  21- 

Let  us  first  show  it  is  integrable  in  any  2laj3. 


Let  D  be  a  cubical  division  of  space  of  norm  d. 

Then  Aap  =  lira  2o>A     ,     <*>,  =  DSC/  in  dt. 

<*=o  2la/3 

Let  a'  >  a,  £'  >  0.     Then 

A'>  -  A     =  lim   2a>W:  -  2«A. 


40  IMPROPER  MULTIPLE  INTEGRALS 

Now  any  cell  dt  of  5laj8  is  a  cell  of  5la-j3',  and  in  d^  co(  >  co,. 
Hence  Aa>p  >  Aap.  Thus  Aa$  is  a  monotone  increasing  function 
of  a,  /3.  On  the  other  hand 

lim  Aap  =  0, 


by  hypothesis.     Hence  Aaft  =  0  and  thus  /is  integrable  in  5la/3- 
Next  let  /  be  limited  in  33,  then  |/|<some  7  in  33.     Then 

33  <  5lv,  r     But  /  being  integrable  in  5ly,  Y,  it  is  in  33  by  I,   700,  3. 
Let  us  now  consider  the  general  case.     Since  /  is  integrable  in  51 


f/    ,       f  /, 
J  J. 


both  converge  by  38.     Let  now  P,  N  be  the  points  of  ^P,  %l  lying 
in  33.     Then 


both  converge.     Hence  by  39, 


both  converge.     But  if  33a,6  denote  the  points  of  33  at  which 
-«</<&, 

r/=  iim  r  /, 

JjQ  a,b=*J®ab 

by  definition. 

But  as  just  seen,  C    _ 

£*# 

//- 

and  /is  integrable  in  33. 

41.    As  a  corollary  of  40  we  have  : 

1  .  Iff  is  integrable  in  51,  it  admits  a  proper  integral  in  any  part 
of  51  in  which  f  is  limited. 

2.  Iff  is  integrable  in  any  part  of  51  in  which  f  is  limited,  and  if 
either  the  lower  or  upper  integral  off  in  51  is  convergent,  f  is  integra 
ble  in  51. 


GENERAL   THEORY  41 

For  let  T:  ^ 

J   /=lim    j  /  (1 

JK      .tf—JiM 

exist.     Since 
necessarily 

exists  and  1),  2)  are  equal. 

42.    1.    In  studying  the  function/  it  is  sometimes  convenient  to 
introduce  two  auxiliary  functions  defined  as  follows : 

g=f  where/>0, 

=  0  where /<0. 

h=-f  where/<0, 

=  0  where />0. 

Thus  #,  h  are  both  >  0  and 


We  call  them  the  associated  non-negative  functions. 

2.  As  usual  let  5L/s  denote  the  points  of  51  at  which  —  a  <f<@. 
Let  510  denote  the  points  where  g<&,  and  5la  the  points  where  h<a. 
Then  -  - 

I   g  =  lim    I      g,  (1 

•'SI  a,^=oo»/$laj3 

f  A  =  lim    f    h.  (2 

C/QT  /> »y  91 

For  -  - 

I    9=    I     ^         by  5,  4. 

^%         ^2la^ 

Letting  a,  /Q  =  oo,  this  last  gives  1). 
A  similar  demonstration  establishes  2). 

3.  We  cannot  say  always 

C  C  C  7  C 

J  #  =  lim  J      g      ;      t  A  — lim    I      A, 

as  the  following  example  shows. 


42  IMPROPER  MULTIPLE  INTEGRALS 

Let          /  =  1  at  the  irrational  points  in  21  =  (0,  1), 

=  —  n,  for  x  =  —  in  21. 
n 

Then  ~  ~ 

^  ^2ta/3 

Again  let  /  =  —  1  for  the  irrational  points  in  21, 

=  n  for  the  rational  points  x  =  -  - 

n 

Then 


43.    1. 


f  A=0.  f    A=l. 

JM*  J.Kap 

1)     f</=f/;  /</<//;                           (2 

^2t          *7^  ^           ^ 

3)      f  A  =  -  f/;  f^<-    f/;                         (4 

c/21                 Jsjj17  c/^                  ^/g(j 


provided  the  integral  on  either  side  of  the  equations  converges,  or 
provided  the  integrals  on  the  right  side  of  the  inequalities  converge. 

Let  us  prove  1);  the  others  are  similarly  established.     Effecting 
a  cubical  division  of  space  of  norm  d,  we  have  for  a  fixed  ft, 


=  lim  2  Jft*  =    f  /.  (5 

d=Q   ^  ^0 

Thus  if  either  integral  in  1)  is  convergent,  the  passage  to  the 
limit  ft  =  QO  in  5),  gives  1). 


2.    If   I   f  is  convergent,    I  g  converge. 

J<£  v/21 

If   I  f  is  convergent,    \  h  converge. 
*/2l  c/21 

This  follows  from  1  and  from  38. 


GENERAL   THEORY  43 

3.    If   I  /  is  convergent,  we  cannot  say  that    I  /  is  always  con- 

•/g  *Syi 

vergent.     A  similar  remark  holds  for  the  lower  integral. 

For  let         jf=:l  at  the  rational  points  of  51  =  (0,  1) 


= at  the  irrational  points. 

x 


Then 


4.    That  the  inequality  sign  in  2)  or  4)  may  be  necessary  is 
shown  thus : 

Let  -I 

/=  -L  for  rational  x  in  51  =  (0,  1) 


= for  irrational  x. 


Then  r  r 

J>=0     ,     J/-i. 

44.    1.  ff=fg-  lim    f    A,  (1 

*^2I  *^2I  a    fi  =  xc'2I 

f/  =   lim    f   0-  (\  (2 

«^2t  a  i3  =  x*^2t  ** 

provided,  1°  ^e  integral  on  the  left  exists,  or  2°  fAe  integral  and  the 
limit  on  the  right  exist. 

For  let  us  effect  a  cubical  division  of  norm  d.     The  cells  con 
taining  points  of  51  fall  into  two  classes : 

a)  those  in  which /is  always  <  0, 

5)  those  in  which /is  >0  for  at  least  one  point. 

In  the  cells  a),  since /=  g  —  A, 

Max/  =  Max  (g-h)=  Max  g  -  Min  h,  (3 

as  Max#  =  0.     In  the  cells  b)  this  relation  also  holds  as  Min  h  =  0. 
Thus  3)  gives 

f  /=  f   £- J   A.  (4 

•^a?  "X0  -^ 


44  IMPROPER  MULTIPLE   INTEGRALS 

Let  now  a,  /3  =  oo.  If  the  integral  on  the  left  of  1)  is  conver 
gent,  the  integral  on  the  right  of  1^  is  convergent  by  43,  2.  Hence 
the  limit  on  the  right  of  1)  exists.  Using  now  42,  2,  we  get  1). 

Let  us  now  look  at  the  2°  hypothesis.     By  42,  2, 


lim 


g—   1  g. 

*  *V 


Thus  passing  to  the  limit  in  4),  we  get  1). 
2.    A  relation  of  the  type 

£-£-/.* 

does  not  always  hold  as  the  following  shows. 

Example.     Let/  =  n  at  the  points  x  —  — 

A  n 

f  m 

=  —  n  for  x  = 


22W-4-1 

=  —  1  at  the  other  points  of  51  =  (0,  1). 

Then  f/=-l  f#  =  0  fA  =  0. 

Ja  JsT  J» 

45.    If  (  f  is  convergent,  it  is  in  any  unmixed  part  33  0/21. 
c/2t 

Let  us  consider  the  upper  integral  first.     By  43,  2, 


exists.     Hence  a  fortiori, 

Jt' 

exists.     Since  51  =  48  -f  (£  is  an  unmixed  division, 
C  h=    C    h+    C  h. 

J*+  J®afi  JSafi 

Hence  C  h<    C  h. 


GENERAL  THEORY  45 

As  the  limit  of  the  right  side  exists,  that  of  the  left  exists  also. 
From  this  fact,  and  because  1)  exists, 


exists  by  44,  1. 

A  similar  demonstration  holds  for  the  lower  integral  over  $3. 


46.    If&v  212  •••  ^imform  an  unmixed  division  0/51,  then 
f/=   f/+  -+    f  /, 


JKm 

provided  the  integral  on  the  left  exists  or  all  the  integrals  on  the 
right  exist. 

For  if  2lm  a/3  denote  the  points  of  2la/3  in  5lm,  we  have 

JL-JU--+.L-          <2 

Now  if  the  integral  on  the  left  of  1)  is  convergent,  the  integrals 
on  the  right  of  1)  all  converge  by  45.  Passing  to  the  limit  in  2) 
gives  1).  On  the  other  hypothesis,  the  integrals  on  the  right  of 
1)  existing,  a  passage  to  the  limit  in  2)  shows  that  1)  holds  in 
this  case  also. 

47.    If  i  f  and   (  f  converge,  so  does   C  I/I,  and 
Jty  Jyi  c/21 

fl/l<  f/-  f/  (i 

si  9s         yi 

<£g  +  Jh.  (2 

For  let  AB  denote  the  points  of  51  where 

Then  since 


X  i'i  =1 

*/AB  «/A 


<    C  g+  Ch 
JAB        *^AB 

<fff+  f*  (3 

c/21          c/5( 

<f/-f/        by  43,1.  (4 

Jy        JM 


Passing  to  the  limit  in  3),  4),  we  get  1),  2). 


46  IMPROPER  MULTIPLE   INTEGRALS 

48.    1.    If  |    I/  1  converges,  loth   f  '/  converge. 
*%  JK 

For  as  usual  let  ^3  denote  the  points  of  5(  where  />0. 
Then  ' 


is  convergent  by  38,  3,  since   f  \f\  is  convergent. 
Similarly, 

f  (-/)=-   f/ 
•%  */3? 

is  convergent.     The  theorem  follows  now  by  39. 

2.  If  \    |  /|  converges,  so  do 

fff   ,    f*.  (i 

Ji/2t  j^2t 

For  by  1, 

J% 
both  converge.     The  theorem  now  follows  by  43,  2. 

3.  For 

f/  (2 

V* 

converge  it  is  necessary  and  sufficient  that 


is  convergent. 


For  if  3)  converges,  the  integrals  2)  both  converge  by  1. 
On  the  other  hand  if  both  the  integrals  2)  converge, 


converge  by  38,  2.     Hence  3)  converges  by  47. 
4.    If/is  integrable  in  21,  so  is  \f\. 
For  let  Aft  denote  the  points  of  5(  where  0  <  |/|  <  f}.     Then 


and  the  limit  on  the  right  exists  by  3. 


GENERAL   THEORY  47 

But  by  41,  I,/  is  integrable  in  A^.     Hence  |/|  is  integrable  in 
ft  by  I,  720.     Thus 


49.    From  the  above  it  follows  that  if  both  integrals 

.      b 

converge,  they  converge  absolutely.     Thus,  in  particular,  if 


converges,  it  is  absolutely  convergent. 

We  must,  however,  guard  the  reader  against  the  error  of  sup 
posing  that  only  absolutely  convergent  upper  and  lower  integrals 
exist. 

Example.     At  the  rational  points  of  31  =  (0,  1)  let 


At  the  irrational  points  let 
Here 


A,)-! 


// 


Thus,  /  admits  an  upper,  but  not  a  lower  integral.     On  the 
other  hand  the  upper  integral  of  /  does  not  converge  absolutely. 


For  obviously 

50.    We  have  just  noted  that  if 


J|/|  =  +  00. 


is  convergent,  it  is  absolutely  convergent.  For  m  =  1,  this  result 
apparently  stands  in  contradiction  with  the  theory  developed  in 
Vol.  I,  where  we  often  dealt  with  convergent  integrals  which  do 
not  converge  absolutely. 


48  IMPROPER  MULTIPLE  INTEGRALS 

Let  us  consider,  for  example, 

sin- 


If  we  set  x  =  -,  we  get 


sinu  -, 
u 

which  converges  by  I,  667,  but  is  not  absolutely  convergent  by 
I,  646. 

This  apparent  discrepancy  at  once  disappears  when  we  observe 
that  according  to  the  definition  laid  down  in  Vol.  I, 

J  =  R  Km  I  fdx, 

a=0  *^a 

while  in  the  present  chapter 

«7=   lim  J     fdx. 

Now  it  is  easy  to  see  that,  taking  a  large  at  pleasure  but  fixed, 
J      fdx  =  00         as  y3  =  oo, 

so  that  <7does  not  converge  according  to  our  present  definition. 

In  the  theory  of  integration  as  ordinarily  developed  in  works 
on  the  calculus  a  similar  phenomenon  occurs,  viz.  only  absolutely 
convergent  integrals  exist  when  m  >  1. 

51.    1.    If  j    |/|  is  convergent, 

I// £Xl/!-      :         (1 

For  5la/3  denoting  as  usual  the  points  of  51  where  —  «</</3 
we  have  -  -  - 

f   /    <  J     |/|<   f  I/I- 
'.5/21  ^21  21 

Passing  to  the  limit,  we  get  1). 


GENERAL   THEORY  49 

2.   If  §  l/l  is  convergent,  C  f  are  convergent  for  any  33  <2(. 
Ja  J% 

For  I   (/I  is  convergent  by  38,  4. 
*/$ 

Hence 


converge  by  48,  3. 

3.    If,  1°,   f"  |  / 1  is  convergent  and  Min  /  is  finite,  or  if,  2°,   f /  is 
convergent  and  Max  /  is  finite,  then 


is  convergent. 

This  follows  by  36  and  48,  3. 

52.    Letf>Q  inW.     Let  the  integral 


converge.     If 

then  for  any  unmixed  part  33  <  51, 


(2 


0  <«'<«.  (3 


For  let  21  =  55  4-  G>.     Then  51^  =  ^  +  ^/3  is  an  unmixed  division. 
Also 

*/9I  */«         c/ff 


=  f  +  «          by  1) 
s!*fi 

=/ 

V» 


+     +«. 


50 


IMPROPER  MULTIPLE  INTEGRALS 


Hence 
From  2) 


C  +   C  =  C  +  C  +  a. 

.5/33      ±:&      —  %$p      —  £/3 

-         - 

a'=    f  -    f 

«          J 


(4 


by4) 


which  establishes  3). 

53,    If  the  integral 
converges,  then 

<  31 


J"  I/I 


that 


><r. 


C1 
(2 
(3 


Let  us  suppose  first  that/>0.  If  the  theorem  is  not  true, 
there  exists,  however  small  o->0  is  taken,  a  53  satisfying  3)  such 
that 


Then  there  exists  a  cubical  division  of  space  such  that  those 
points  of  51,  call  them  (£,  which  lie  in  cells  containing  a  point  of 
53,  are  such  that  (5<<r  also.  Moreover  (£  is  an  unmixed  part  of  51. 
Then  from  4)  follows,  as/_>0,  that 


also. 

Let  us  now  take  /3  so  that 


Then 


and 

by  52.     But 


1=1+ «'' 


GENERAL  THEORY  51 

Let  now  /3<r  <  e,  then 


/  <•• 

*/CFo 


which  contradicts  5). 

Let  us  now  make  no  restrictions  on  the  sign  of/.     We  have 

/ 

But  since  1)  converges,  the  present  case  is  reduced  to  the  pre 
ceding. 

54.     1.    Let   I    |/ 1  converge. 
%/g 

Let  as  usual  2la/3  denote  the  points  of^at  which  —«</<#.  Let 
Aab  be  such  that  each  5la/3  lies  in  some  Aab  in  which  latter  f  is  limited. 
Let  £)a/3  =  Aab  —  2la/3  and  let  a,  b  =  ac  with  a,  /3.  Then 

lim  £)a/3  =  0. 

a,  0=30 

For  if  not,  let 

a,  /3=a> 

Then  for  any  0  <  X  <  Z,  there  exists  a  monotone  sequence  \an,  ftn\ 
such  that 

£W«  >  X         for  n  >  some  w. 


Let   /in=Min(an,  y8n),    then    \f    >  fj,n  in    X)an/3n^    an(l    Mn^00* 
Hence  ^ 

J        |/|>ASX^oo.  (1 

^D^fc 

X)an/3n  being  a  part  of  31 


by  38,  3.     This  contradicts  1). 

2.    Definition.     We  say  .Afli  6  is  conjugate  to  5la/3  with  respect  to/. 


55.    1.    J.s  wswaZ  let  -  a  </  <  /3  m  3la^.     Let  0<f</3  in  51^. 
i^^  ^4.^  5e  conjugate  to  2(a0  ^^A  reference  to  f  ;  and  Ab  conjugate 
to  51^  with  respect  to  |/|. 


52  IMPROPER  MULTIPLE  INTEGRALS 

V,  1°, 

or  (f,  2°, 


lim    f     /=    f/. 

a,  6=00  *d^a,  6  ^«l 


For,  if  2°  holds,  1°  holds  also,  since 


Thus  case  2°  is  reduced  to  1°.     Let  then  the  1°  limit  exist. 
We  have 

f   /»  f    tf-  f    *•  (2 

J2W  J*./       s4g 

as  4)  in  44,  1  shows.     Let  now 

£>,*.<-  4*  -**• 
Then, 


But  ^^  =  0,  as  «,  ft  =  oo,  by  54.     Let  us  now  pass  to  the  limit 
a,  yS  =  QO  in  3).     Since  the  limit  of  the  last  term  is  0  by  53,  54,  we 

-  - 

lim    L   #=lim     )     9-  (4 

«,  0=00  ^^  a,  6=ao  ^Aa,  b 

Similarly,  ~  ~ 

lim     I      h  =  lim    I      h.  (5 

o,  0=c»  ^a/3  a,  5=0=  ?Z^a6 

Passing  to  the  limit  in  2),  we  get,  using  4),  5), 
f    /=  lim   |  f    a-    f    h  I 

Ax/  «,6=oo     (^«/          ll^         J 

=  lim    f    / 

a,  ft  =  ao  ^^aft 

In  a  similar  manner  we  may  establish  1)  for  the  lower  integrals. 


GENERAL   THEORY  53 

2.  The  following  example  is  instructive  as  showing  that  when 
the  conditions  imposed  in  1  are  not  fulfilled,  the  relation  1)  may 
not  hold. 

Example.     Since  ^  , 

I    —=+oo, 

«/0      X 

there  exists,  for  any  bn  >  0,  a  0  <  bn+1  <  5n,  such  that  if  we  set 


then  n    ^  n 

Cr1<Cr2<  *••  =00, 

as  bn  =  0.     Let  now 

/  =  1  for  the  rational  points  in  51  =  (0, 1), 

=  -  for  the  irrational. 
x 

Then 
Let 

Let  An  denote  the  points  of  51  in  (£>n,  1)  and  the  irrational  points 
Then  C      r      ^ 

JA»  >  ^n+l 
But  obviously  the  set  An  is  conjugate  to  510.     On  the  other  hand, 


while  /• 

lim     1   /=  +  ». 


56.    Jf  £fo  integral 

.  // 

converges,  then 

e  >  0,         a-  >  0, 
/or  aw/  unmixed  part  $8  of  51 


/!<€  (2 

v 


54  IMPROPER  MULTIPLE  INTEGRALS 

Let   us   establish   the  theorem  for   the  upper  integral ;    similar 
reasoning  may  be  used  for  the  lower.     Since  1)  is  convergent, 

//  (3 

and  X=  lim    C  h  (4 

a(0==o«/5la/3 

exist  by  44,  l.     Since  3)  exists,  we  have  by  53, 


for  any  33  <  5t  such  that  33  <  some  cr'. 

Since  4)  exists,  there  exists  a  pair  of  values  a,  b  such  that 

X=  f    h  +  r)     ,      0<77<^-,  (6 

—  2ta6  ' 

since  the  integral  on  the  right  side  of  4)  is  a  monotone  increasing 
function  of  a,  b. 

Since  51  =  53  +  (£  is  an  unmixed  division  of  51, 

C  h=  C  h-}-  C  h. 

^5lal8         ^a/3         ^<£aj3 

Since  h  >  0,  and  the  limit  4)  exists,  the  above  shows  that 
p  =   lim     j      h     ,     v  =   lim     I      h 

a,  /3=ao  »^SJ3a|3  a,  /3=co  ^_(Sa(3 

exist  and  that 

x=M+".  a 

Then  a,  ft  being  the  same  as  in  6), 

M  =  J   A  +  V,  •  (8 

and  we  show  that 

n  ^    '  ^  „  (Q 

\j  <^  77     <»,  77  ^«-' 

as  in  52.     Let  now  c  >  a,  ft  ;  then 


if  we  take  ™  <  _e 

4 


GENERAL   THEORY  55 

Thus,  M<1          :  fe      B      (n 

But  ry  =  f^_^ 

by  44,  1.     Thus  2)  follows  on  using  5),  11)  and  taking  a-  <</,  cr". 

57.    If  the  integral    (  f  converges  and  $&u  is  an  unmixed  part  of 
21  such  that  $$u  =  21  as  u  =  0,  then 

limf/=f/.  (1 

u = 0  *Aw  *^9I 

For  if  we  set  21  =  93U  4-  £u,  the  last  set  is  an  unmixed  part  of  21 
and  (£„  =  0.     Now 


J%u     J.S* 
Passing  to  the  limit,  we  get  1)  on  using  56. 


58.    1.    Let  ®afi 

If,  1°,  the  upper  contents  of 

f  «P  ^  ^/a^  -  £>a0        ?        9a^  =  ^  a,3  ~  ^a^        >        ^a^  =  ^/+*  a/3  ~  ^a 

=  0  as  a,  /3  =00  , 
(f,  2°,  fAe  upper  integrals  off,  g,f+g  are  convergent,  then 


7/^1°  Ao?c?s,  awe?  {f,  3°,  ^Ae  Zower  integrals  off,  g,f  +  g  are  conver 
gent,  then 


Let  us  prove  2)  ;  the  relation  3)  is  similarly  established.  Let 
Z)a,  ft  be  a  cubical  division  of  space.  Let  (5a/3  denote  the  points  of 
£)a|8  lying  in  cells  of  Z>a/3,  containing  no  point  of  the  sets  1).  Let 


56  IMPROPER  MULTIPLE   INTEGRALS 

Then  Daft  may  be  chosen  so  that  gaj3  =  0. 
Now 


since  the  fields  are  unmixed.     By  56,  the  second  integral  on  the 
right  =  0  as  a,  &  =  oo  .     Hence 


lim  JT      /=   lim  /   /. 
i,H-«D«au«a        «,^-«»/««« 


Similar  reasoning  applies  to 
Again, 


Thus,  letting  a,  @  =00  we  get  2). 

2.    TTAe/i  fAe  singular  points  off,  g  are  discrete,  the  condition  1° 
holds. 


3.    7/#  is  integrable  and  the  conditions  1°,  2°,  3°  are  satisfied^ 


4.    If  f,  g  are  integrable  and  condition  1°  e's  satisfied,  f  +  g  is  in 
tegrate  and 


5. 

provided  the  integral  off  in  question  converges  or  is  definitely  infinite. 

LV+C^LS+L« 


Also 

lim  £)a/J  =  lim  2la/J 
where  2la/3  refers  to/. 

6.    When  condition  1°  is  not  satisfied,  the  relations  2)  or  3) 
may  not  hold. 


GENERAL   THEORY  ,  57 

Example.     Let  51  consist  of  the  rational  points  in  (0,  1). 

Let  /.      .,    .  .. 

/=  \+n    ,    g  =  \  —n 

at  the  point  x  =  ™.     Then 
n 

f  +  g=2         in  21. 
Now  qr  w 

*fi  «/i        »        *>  «/5 

embrace  only  a  finite  number  of  points  for  a  given  a,  /9.     On  the 
other  hand, 


Thus  the  upper  content  of  the  last  set  in  1)  does  not  =  0  as 
«,  ft  =  oo  and  condition  1°  is  not  fulfilled.  Also  relation  2)  does 
not  hold  in  this  case.  For 


,  jT/=o  , 


59.  #c>0,  Om-fjf;  (1 

(2 


provided  the  integral  on  either  side  is  convergent. 
For 


/       ifo<0.  (4 

Let  c>  0.     Since 

therefore  ~ 

--</<-         in  this  set. 

Hence  any  point  of  Hc/,  ap,  is  a  point  of  SI/,  -.  ^  and  conversely. 
Thus  2<cAa,=  2l,,^         whenoO. 


58  IMPROPER  MULTIPLE  INTEGRALS 

Similarly  ^=SI,,?,|         when  c  <  0. 

Thus  3),  4)  give 

f        e/=ef          /        c>0 

•         J 


?,,/   c<0- 

c'  c 

We  now  need  only  to  pass  to  the  limit  a,  0  =  <x>  . 
60.    Let  one  of  the  integrals 


converge.  Iff  =  #,  arc?^  a«  a  discrete  set  £)  m  51,  60^  integrals 
converge  and  are  equal.  A  similar  theorem  holds  for  the  lower 
integrals. 

For  let  us  suppose  the  first  integral  in  1)  converges.     Let 

*-. 

then 

Now 

=    lim  =     m  g 


f,  a/3 

Thus  the  second  integral  in  1)  converges,  and  2),  3)  show  that 
the  integrals  in  1)  are  equal. 


61.    1.    Let  f     /,       f  g  (1 

£8  ~2l 

converge.     Let  f  '>  g  except  possibly  at  a  discrete  set.     Let 


««,,,*)     ;  .f  =  2l/,aa-3X0     ;     Qa0  =  21^ -3V 

V  -  - 

fojs  =  0,  ga^  =0,   as  a,  yQ  =  oo, 
then  —          _ 


RELATION  BETWEEN  THE  INTEGRALS  OF  TYPES  I,  II,  III     59 

For  let  (Sa/3  be  defined  as  in  58,  1.     Then 


Let  a,  ft  =  <x>,  we  get  2)  by  the  same  style  of  reasoning  as  in 

58. 

2.  If  the  integrals  1)  converge,  and  their  singular  points  are  dis 
crete,  the  relation  2)  holds. 

This  follows  by  58,  2. 

3.  If  the  conditions  of  1  do  not  hold,  the  relation  2)  may  not 
be  true. 

Example.     Let  51  denote  the  rational  points  in  (0*,  1*).     Let 

/•  m    •      ca 

f=n         at  x  =  —  in  51. 
n 

g=l         in  51. 

Then  f>g         in  51. 

But 


Relation  betioeen  the  Integrals  of  Types  I,  //,  /// 

62.  Let  us  denote  these  integrals  over  the  limited  field  51  by 

0«     ,      V*     ,     At 

respectively.  The  upper  and  lower  integrals  may  be  denoted  by 
putting  a  dash  above  and  below  them.  When  no  ambiguity  arises, 
we  may  omit  the  subscript  51.  The  singular  points  of  the  inte 
grand/,  we  denote  as  usual  by  $• 

63.  If  one  of  the  integrals  P  is  convergent,  and  $  is  discrete,  the 
corresponding  0  integral  converges,  and  both  are  equal. 

T7^  * 

1  P%  =  p%s  +  paj,         using  the  notation  of  28, 

=  e*  +  p«j. 

Now  o        as  a  =  0        by  56. 


60  IMPROPER  MULTIPLE  INTEGRALS 

Hence  p   _  j.     Q 

5=0  5 

==  C%,         by  definition. 

64.    If  O  is  convergent,  we  cannot  say  that  P  converges.     A 
similar  remark  holds  for  tjie  lower  integrals. 

Example.     For  the  rational  points  in  51  =  (0,  1)  let 


for  the  irrational  points  let 

/oo  =  -  - 

x 
Then 


a=0 


On  the  other  hand,  _ 

PH  =  lim    f    / 

does  not  exist.     For  however  large  /3  is  taken  and  then  fixed, 

I    /=  —  oo         as  a  =  oo. 

65.    If  O  is  absolutely  convergent  and  $  is  discrete,  then  both  P 
converge  and  are  equal  to  the  corresponding  0  integrals. 

For  let  D  be  any  complete  division  of  51  of  norm  8.     Then 

/~Jt>j[L  (1 

using  the  notation  of  28.     Now  since 

£k  |/|  converges,         C%'&  |/|  =  0         as  8  =  0. 
But 


Again,  D  being  fixed,  if  «0/30  are  sufficiently  large, 
f    f=C^f        «>«0,        /S>/30. 

*/9I   « 


l«M 


RELATION  BETWEEN  THE  INTEGRALS  OF  TYPES  I,  II,  III      61 
Hence  1),  2)  give 

f   /=  #a,  +  e'          le'j  <  -         for  any  8  <  some  S0. 

J2lap  2 

On  the  other  hand,  if  S0  is  sufficiently  small, 

ft=  <£,  +  €"  |e"|<|         for  8<S0. 

Hence  f  /=<7a  +  €'"  |e'"|<e. 

^ajS 

Passing  to  the  limit  a,  /3  =  GO,  we  get 


66.    7/  Fa/  ^s  absolutely  convergent,  the  singular  points  $  are 
discrete. 

For   suppose  3  >  0.     Let   53  denote   the   points   of   51   where 
\f\>0.     Then  g  >  ^  for  any  ^.     Hence 


as  13  =  QO  unless  3  =  0. 

67.    If  V%f  is  absolutely  convergent,  so  is  C. 

For  let  D  be  a  cubical  division  of  space  of  norm  d. 

Then 

|/  1  <  some  /3in  2ld. 

Hence 


Hence  (7  is  absolutely  convergent. 

68.    Letf>0.     If  VyJ  is  convergent,  there  exists  for  each  e>0, 
a  a-  >  0  such  that 


for  any  53  such  that 

.  (2 


62  IMPROPER  MULTIPLE   INTEGRALS 

' 


for  X  sufficiently  large.     Let  X  be  so  taken,  then 

P»/=jQ/*  +  «"     ,     0<«»<|.  (3 

AIso> 


if  o-  is  taken  sufficiently  small  in  2). 
From  3),  4)  follows  1). 

69.    If  V^f  is  absolutely  convergent,   both  0  converge  and  are 
equal  to  the  corresponding  V  integrals. 

For  by  67,  0  is  absolutely  convergent.     Hence  (/converge  by  65. 

Thus 

(!<»f=  I     f  4- «     .     \n.'  <? 

Also 


=  1    /+«     »     |«'<-      for  some  d. 

®d  3 

L  4-  /3     ,      I  /3 1  <  |     for  some  X,  , 


Hence 


Now 
But 


and  7  <  |  if  d  is  sufficiently  small,  and  for  any  X,  /A,  by  68. 
o 

Taking  a  division  of  space  having  this  norm,  we  then  take  X, 
so  large  that 

/AM=/     mSIc,. 

Then 

T;  =  «  _  p  -  7, 

and  hence 

|77|<e. 

From  this  and  1)  the  theorem  now  follows  at  once. 


ITERATED  INTEGRALS  63 

Iterated  Integrals 

70.  1.    We  consider  now  the  relations  which  exist  between  the 
integrals 


and  -    ? 

If/,  (2 

~.<B«Ze 

where  51  =  53  •  (5  lies  in  a  space  9?m,  m  =  p  -f  ^,  and  53  is  a  projection 
of  51  in  the  space  9?p. 

It  is  sometimes  convenient  to  denote  the  last  q  coordinates  of  a 
point  x  =  (o^  •••  xp  xp+l  •••  xp+q)  by  yl-->  yq.  Thus  the  coordinates 
x1  •••  xp  refer  to  53  and  y^  •  ••  yg  to  (5.  The  section  of  51  correspond 
ing  to  the  point  x  in  53  may  be  denoted  by  (£x  when  it  is  desirable 
to  indicate  which  of  the  sections  (£  is  meant. 

2.    Let  us  set 

*(*! 

then  the  integral  2)  is 


It  is  important  to  note  at  once  that  although  the  integrand  /  is 
defined  for  each  point  in  51,  the  integrand  <f>  in  4)  may  not  be. 

Example.     Let  51  consist  of  the  points  (z,  y)  in  the  unit  square  : 

771  A   ^       ^  I 

x  =  -     ,      0<y<-. 
?i  n 

Then  51  is  discrete.     At  the  point  (x,  y)in  51,  let 


Then  i    *     A         by  32 


On  the  other  hand 
for  each  point  of  53-     Thus  the  integrals  2)  are  not  defined. 


64  IMPROPER  MULTIPLE   INTEGRALS 

To  provide  for  the  case  that  <f>  may  not  be  defined  for  certain 
points  of  53  we  give  the  symbol  2)  the  following  definition. 

f    (  /=    lim     f      I/,  (5 

J»J<r         a,0=ooJ|8a0Jr 

where  F  =  (£  when  the  integral  3)  is  convergent,  or  in  the  con 
trary  case  F  is  such  a  part  of  (£  that 

-«</*/<  A  (6 

^r 

and  such  that  the  integral  in  6)  .is  numerically  as  large  as  6)  will 
permit. 

Sometimes  it  is  convenient  to  denote  F  more  specifically  by  Fa/3. 

The  points  53a0  are  the  points  of  53  at  which  6)  holds.  It  will 
be  noticed  that  each  53a/3  in  5)  contains  all  the  points  of  53  where 
the  integral  3)  is  not  convergent.  Thus 


Hence  when  53  is  complete  or  metric, 

lim  Sais=S.  (7 

a, /3=ao 

Before  going  farther  it  will  aid  the  reader  to  consider  a  few 
examples. 

71.    Example  1.     Let  51  be  as  in  the  example  in  70,  2,  while/  =  n2 

at  x  =  -.     We  see  that 
n 


On  the  other  hand  53a/s  contains  but  a  finite  number  of  points 
for  any  a,  @.     Thus 


Thus  the  two  integrals  1),  2)  exist  and  are  equal. 

Example  2.  The  fact  that  the  integrals  in  Ex.  1  vanish  may 
lead  the  reader  to  depreciate  the  value  of  an  example  of  this  kind. 
This  would  be  unfortunate,  as  it  is  easy  to  modify  the  function  so 
that  thee.e  integrals  do  not  vanish. 


ITERATED   INTEGRALS  65 

Let  21  denote  all  the  points  of  the  unit  square.  Let  us  denote 
the  discrete  point  set  used  in  Ex.  1  by  £).  We  define  /  now  as 
follows  :  /  shall  have  in  £)  the  values  assigned  to  it  at  these  points 
in  Ex.  1.  At  the  other  points  A  =  21  —  £),/ shall  have  the  value  1. 

Then  C       C      C       C 

On  the  other  hand  33a/3  consists  of  the  irrational  points  in  $3  and 
a  finite  number  of  other  points.  Thus 

•  =  1.  _  (4 

Hence  again  the  two  3),  4)  exist  and  are  equal. 
Let  us  look  at  the  results  we  get  if  we  use  integrals  of  types  I 
and  II.     We  will  denote  them  by  C  and  F  as  in  62. 
We  see  at  once  that 

Let  us  now  calculate  the  iterated  integrals 

$B  Od,  (5 

and  Fs  F<£.  (6 

We  observe  that 

<7e  =  1         for  x  irrational 

=  +  oo    for  x  rational. 

Thus  the  integral  5)  either  is  not  defined  at  all  since  the  field 
33s  does  not  exist,  or  if  we  interpret  the  definition  as  liberally  as 
possible,  its  value  is  0.  In  neither  case  is 


Let  us  now  look  at  the  integral  6).      We  see  at  once  that 

- 


does  not  exist,  as  Fe  =  1  for  rational  #,  and   =  +00  for  irrational 
x.     On  the  other  hand 


Hence  in  this  case 


66  IMPROPER  MULTIPLE   INTEGRALS 

Example  3.     Let  51  be  the  unit  square. 

Let 

/f  m 

=  n   tor  x  =  —         n  even 
n 

=  -  n   for  x  =  ~          n  odd. 

At  the  other  points  of  51  let/=  1. 
Then  „  „   r 

//=/Je/=1- 

Here  every  point  of  51  is  a  point  of  infinite  discontinuity  and 
thus  $  =  51. 

Here  (7^  is  not  defined,  as  515  does  not  exist ;  or  giving  the 
definition  its  most  liberal  interpretation, 

<7st=0. 

The  same  remarks  hold  for  O^Og. 

On  the  other  hand  f^ 

FSI  =  4-  00, 

while  jr  y 

does  not  exist,  since  Jr  f  m 

Vg  =  ±  n    for  x  =  — 
n 

=  1  for  irrational  x. 
Moreover  77   TA  V  V 

Example  4.     Let  51  denote  the  unit  square.     Let 

~        9   £  m  A^^l 

f  =  n*   lor  a?  =  — ,    7i  even,  0<y<  — 

n  n 

=  —  n2   for  #  =  — ,    n  odd,    0  <  y  <  - . 
n  n 

At  the  other  points  of  5Ilet/=  1. 
Then 


ITERATED  INTEGRALS  67 

Let  us  look  at  the  corresponding  C  and  V  integrals. 

We  see  at  once  that 

n  --  v  —  i 
ca-  v*~  *• 

Again  the  integral  C^Cg  does  not  exist,  or  on  a  liberal  interpre 
tation  it  has  the  value  0.     Also  in  this  example 

(7^  and  C9Cz 

do  not  exist  or  on  a  liberal  interpretation,  they  =  0. 
Turning  to  the  F'  integrals  we  see  that 


while  V<g  Fjg  does  not  exist  finite  or  infinite. 

Example  5.  Let  our  field  of  integration  51  consist  of  the  unit 
square  considered  in  Ex.  4,  let  us  call  it  Gr,  and  another  similar 
square  g,  lying  to  its  right.  Let  /  be  defined  over  (S  as  it  was 
defined  in  Ex.  4,  and  let/=  1  in  g. 

Then 


Also  .    <t-*k-*  • 

Then  „  „       1 

^^B^S  ~  *' 

while  FsFg   does  not  exist, 

and 


72.    1.    In  the  following  sections  we  shall  restrict  ourselves  as 
follows: 

1°  51  shall  be  limited  and  iterable  with  respect  to  53. 

2°  53  shall  be  complete  or  metric. 

3°  The  singular  points  $  of  the  integrand  /shall  be  discrete. 

2.    Let  us  effect  a  sequence  of  superposed  cubical  divisions  of 
space 

A»  A*  ••• 

whose  norms  dn  =  0. 


68  IMPROPER  MULTIPLE   INTEGRALS 

Let  5ln  =  33n  •  (£n  denote  the  points  of  31  lying  in  cells  of  Dn 
which  contain  no  point  of  $.  We  observe  that  we  may  always 
take  without  loss  of  generality 

»„=». 

For  let  us  adjoin  to  51  a  discrete  set  £)  lying  at  some  distance 
from  51  such  that  the  projection  of  £)  on  $ftp  is  precisely  33. 

Let  ^  =  5l4-£)  =  33-<7    ,     (?=£+c     ,     c  =  0. 

We  now  set  ^  =/  in  ^ 

•=0   in  £). 

JL  hen  7*         7* 

J  4,=j   4 
•£1         ^-^ 


=// 

Similarly 


Hence 

~ 


3.    The  set  ^n  being  as  in  2,  we  shall  write 


73.    Ze£  BtT<  n  denote  the  points  of  33  at  which  cn  >  cr.      Then  if  51 
is  iterable,  with  respect  to  33, 

lim^.^O.  (1 

n=ao 

For  since  51  is  iterable, 

8  =  r  S          by  definition. 


Hence  (5  considered  as  a  function  of  x  is  an  integrable  function 
in  33. 

Similarly 


and  (£„  is  an  integrable  function  in  33. 


ITERATED   INTEGRALS  69 

We  have  now  7?      7?       -  -  ^  n 

£  =  @n  +  cn     ,     cn>0 

as  (£n,  cn  are  unmixed.     Hence  cn  is  an  integrable  function  in  53. 
But 


As  the  left  side  =  0  as  n  =  oo  , 

limj.=  0.  (2 

But 


As  the  left  side  =  0,  we  have  for  a  given  a 

lim  S^  =  0, 
which  is  1). 

74.    Let  %  =  <$>&  be  iterable.     Let  the  integral 

'  /^°  a 

be  convergent  and  limited  in  complete  53.     Let  (gn  denote  the  points 
of  53  at  which 


lim  (gn  =  S.  (3 


For  let  .  „ 

•••  =0. 


Since  jB^B  =  0  as  n  =  oo  by  48,  we  may  take  v1  so  large,  and 
then  a  cubical  division  of  $RP  of  norm  so  small  that  those  cells  con 
taining  points  of  SViVi  have  a  content  <rj/'2.  Let  the  points  of 
53  lying  in  these  cells  be  called  Bv  and  let  ^  =  SB  -  Bv  Then 
Bv  53X  form  an  unmixed  division  of  53  and 


is  complete  since  53  is. 


70  IMPROPER  MULTIPLE   INTEGRALS 

,    We  may  now  reason  on  ^  as  we  did  on  $,  replacing  7?/2  by  ??/22. 
We  get  a  complete  set  332 <$$i  such  that 


Continuing  we  get  ™   ^ 

Thus 


Let  now  b 

Then  b>23-77  (4 

by  25. 

Let  bn  denote  those  points  of  b  for  which  2)  does  hold.  Then 
b  =  Jbn(.  For  let  b  be  any  point  of  b.  Since  1)  is  convergent, 
there  exists  a  o~L  such  that 


at 


,  f/<€, 

^c 


for  any  c  such  that  c  <crt.     Thus  b  is  a  point  of  b^  and  hence  of 
{bj.     Thus  B~n=Fas  b  is  complete.      But  (Sn>bn. 

Hence  lim"gn>"b, 

which  with  4),  gives  3). 

75.    LetW  =  53  •  (£  5e  iterable.     Let  the  integral 


convergent  and  limited  in  complete  53. 

Then  /*    -^ 

lim    I      (   /=0.  (1 


For  let  D  be  a  cubical  division  of  $RP  of  norm  d. 
Then  C    C  C 

Let  d(  denote  those  cells  of  D  containing  a  point  of  (5n  where 
is  defined  as  in  74.  •  ' 


ITERATED   INTEGRALS  71 

Let  d['  denote  the  other  cells  containing  points  of  53.     Then 

St<Zd*€  +  2d?M, 

where  — 

0<  \f<M. 
•35 

Hence 


Letting  d  =  0,  we  get 

JJ> 

c/33  Jc» 


Letting  now  n  ==  oo  and  using  3)  of  74,  we  get  1),  since  e  is 
small  at  pleasure. 

76.    Let  51  =  33  •  (E  be  iterable  with  respect  to  $3,  which  last  is  com 
plete  or  metric.     Let  the  singular  points  $  of  f  be  discrete.      Then 


;  ::    .if,     f< 

Here  any  one  of  the  members  in  1)  may  be  infinite.      Then  all 
that  follow  are  also  infinite.     A  similar  remark  applies  to  2). 

Let  us  first  suppose  : 

f>  0     ,     33  is  complete     ,      j    j   f  is  convergent. 
We  have  by  14, 


Passing  to  the  limit  gives 

f  f  <  lim  f  f  /  (3 

Jr7          .J^^s/ 

and  also  r   T  r" 

lim  I     I     /  <   I    /    ,     finite  or  infinite.  (4 

— 


Now  e>0  being  small  at  pleasure,  there  exists  a  GrQ  such  that 

^ff-       (5 


72  IMPROPER  MULTIPLE   INTEGRALS 

But  for  a  fixed  n  ^ 

I  is  limited  in  53. 

*/(£ 

Hence  for  6r0  sufficiently  large, 

f  f<jf    ,     at  each  point  of  53,         G-Q<G-.  (6 

Then 


where  Fn,  yn  are  points  of  F  in  (£»,  cn. 

Hence 

J»<?J>»' 

Now  330  may  not  be  complete  ;  if  not  let  B0  be  completed  53^. 
As  53  is  complete, 


We  may  therefore  write  8),  using  5) 

-  .  +  f  /  </  /  +  f  /  <//+//- 

c/5B^       J&oJS*       JLBG^n        ^»^Sn       J.BGJ.yn 

By  75,  the  last  term  on  the  right  =  0  as  n  =  oo.     Thus  passing 
to  the  limit, 

n/<lim  f   f/,  (9 

_._y    -n=ao»/33^S/ 

since  e  >  0  is  small  at  pleasure. 

On  the  other  hand,  passing  to  the  limit  G-  =  oo  in  7),  and  then 
n  =  QO,  we  get 

lim  f   f  <  f   f  .  (10 

n^JjQj&n—  Jj&J& 

Thus  3),  10),  9),  and  4)  give  1). 

Let  us  now  suppose  that  the  middle  term  of  1)  is  divergent. 
We  have  as  before 


f     fciim       f  <(/ 

Jj8GJT        n=*>J%J£n       JK 

Hence  the  integral  on  the  right  of  1)  is  divergent. 


ITERATED   INTEGRALS  73 

Let  us  now  suppose  33  is  metric.  We  effect  a  cubical  division 
of  ftp  of  norm  rf,  and  denote  by  Bd  those  cells  containing  only 
points  of  23.  Then  Bd  is  complete  and 


Let  Ad  denote  those  points  of  31  whose  projections  fall  on  Bd. 
Then  Ad  is  iterable  with  respect  to  Ed  by  13,  3,  and  we  have  as 
in  the  preceding  case 

/<//</•  en 

^Ad      ^Bd^£      ^Ad 

If  the  middle  integral  in  11)  is  divergent,  I  is  divergent  and  1) 

*/2f 

holds,  also  if  the  last  integral  in  11)  is  divergent,  1)  holds.  Sup 
pose  then  that  the  two  last  integrals  in  11)  are  convergent. 
Then  by  57 

r=r  f. 

J          J 


Iimf    =  f. 

„      d=t)JAd      •** 


Thus  passing  to  the  limit  e?=  0  in  11)  we  get  1). 

Let  us  now  suppose  f  >  —  (r,  G  >  0. 

Then 


and  we  can  apply  1)  to  the  new  function  g. 


Now 


(13 


by  58,  5,  since  3  is  discrete.     Also  by  the  same  theorem, 

Cg=,   Cf+G-  lim  fT  =    f/  +  GT,  (14 

J&  J&  y  =  V  J_(l 

denoting  by  (Ey  the  points  of  (£  where 


and  setting 

T  =  lim  gy. 

y  =  x 


74  IMPROPER  MULTIPLE  INTEGRALS 

Now  for  any  n 


Hence  &%  =  lim   f    f  #=#li 

n  =  oo  c/58  *ASn  «= 

or  a  =  lim    fSn.  (15 

^  =  00  »/33 

Now  for  a  fixed  w,  7  may  be  taken  so  large  that  for  all  points 
of  33, 

Hence 

S  >  lim 


Hence 


Hence 


31 


and  thus  F  is  integrable  in  58. 

This  result  in  14)  gives,  on  using  58,  3, 


=  c  r 

*/58  Jg 
From  12),  13),  and  17)  follows  1). 

77.    As  corollaries  of  the  last  theorem  we  have,  supposing  H  to 
be  as  in  76, 

1.    Iffis  integrable  in  51  andf>  —  Gr,  then 


If  f<  ^  then  f/=  f    f/. 

*/2l          -/5I3  -^(S 

2.    J?//  >  —  ^  #nd    I    is  divergent,  then 


are  divergent, 


ITERATED   INTECxRALS 


75 


3.    If  f~>  —  G-  and  one  of  the  integrals    I      I  f  is  convergent,  then 

JJ 


is  convergent. 

78.    Let  51  =  33  •  (E  he  iterable  with  respect  to  33,  which  last  is  com 
plete  or  metric.     Let  the  singular  points  Q  be  discrete.     If 

f/,  (i 

J»a 
f  f*  <2 

•/*/( 


both  converge,  they  are  equal. 

For  let  Dr  D2  -••  be  a  sequence  of  superimposed  cubical  divisions 
as  in  72,  2.     We  may  suppose  as  before  that  each  $3re  =  33- 
Since  1)  is  convergent 

e>0,         »„,  f/_f/<l         „<«„.  (3 


(4 
(5 


Since /is  limited  in  5ln,  which  latter  is  iterable, 


This  shows  that 


* 


<2        »>«r 


is  an  integrable  function  in  58,  and  hence  in  any  part  of 
From  3),  4)  we  have 

f-ff 

*/2l        *^23  Jdr 

We  wish  now  to  show  that 

JJ-IX 

*^33*^C£         S3^Sj 

When  this  is  done,  6)  and  7)  prove  the  theorem. 
To  establish  7)  we  begin  by  observing  that 


(6 


n  >  nn. 


ff=lim    C     f. 

J%J<Z      ..s^oo^as^r 


76 


IMPROPER  MULTIPLE  INTEGRALS 


Now  for  a  fixed  n,  a,  0  may  be  taken  so  that  T  shall  embrace  all 
the  points  of  (gw  for  every  point  of  $.     Let  us  set 


Then 


JVM 


(8 


As 


lira    f      ( 

a,^  =  oo^J 

On  the  other  hand, 


I   724 

'-' 


Thus  7)  is  established  when  we  show  that 

,£jj/l<!         ">"„•  (9 

To  this  end  we  note  that  |/|  is  integrable  in  31  by  48,  4.     Hence 

by  77,  l, 

Also  by  I,  734, 

-C |/|  =-CX>|/!'  (i1 

From  10),  11)  we  have  for  n  >  n0, 


since  the  left  side  ==  0. 
But  as  in  8) 

.   LI  i/i  =4J>  +jro.j[i/i 

Passing  to  the  limit  (7=  oo  gives 


This  in  12)  gives  9). 


CHAPTER   III 

SERIES 
Preliminary  Definitions  and  Theorems 

79.    Let  av  a2,  ag  •  •  •  be  an  infinite  sequence  of  numbers. 

The  symbol  An  ^1 

J  JL  =  al  +  «2  +  a3  H-  •  •  •  (1 

is  called  an  infinite  series.     Let 

An=a1  +  a2  +  -'  +  an.  (2 

If  lim  An  (3 

n=w 

is  finite,  we  say  the  series  1)  is  convergent.  If  the  limit  3)  is  infi 
nite  or  does  not  exist,  we  say  1)  is  divergent.  When  1)  is  conver 
gent,  the  limit  3)  is  called  the  sum  of  the  series.  It  is  customary 
to  represent  a  series  and  its  sum  by  the  same  letter,  when  no  con 
fusion  will  arise.  Whenever  practicable  we  shall  adopt  the  fol 
lowing  uniform  notation.  The  terms  of  a  series  will  be  designated 
by  small  Roman  letters,  the  series  and  its  sum  will  be  denoted  by 
the  corresponding  capital  letter.  The  sum  of  the  first  n  terms  of  a 
series  as  A  will  be  denoted  by  An.  The  infinite  series  formed  by 
removing  the  first  n  terms,  as  for  example, 


4-  a,,+2  +  #»+3+  "•  4 

will  be  denoted  by  An,  and  will  be  called  the  remainder  after  n 
terms. 

The  series  formed  by  replacing  each  term  of  a  series  by  its  nu 
merical  value  is  called  the  adjoint  series.  We  shall  designate  it 
by  replacing  the  Roman  letters  by  the  corresponding  Greek  or 
German  letters.  Thus  the  adjoint  of  1)  would  be  denoted  by 

A  =  «!  -f-  «2  -f-  «3  +  •  .  .  =  Adj  A  (5 

where 


«»  = 

77 


78  SERIES 

If  all  the  terms  of  of  a  series  are  5  0»  it  is  identical  with  its 
adjoint. 

A  sum  of  p  consecutive  terms  as 

an+l  +  an+2+ f-n+p 

we  denote  by  An,p. 

Let  ^ 

B=  atl  +  #4  +  at3  +  •••      ,     t1<*2<*" 

£g  £Ae  8irie*  obtained  from  A  by  omitting  all  its  terms  that  vanish. 
Then  A  and  B  converge  or  diverge  simultaneously,  and  when  conver 
gent  they  have  the  same  sum. 

For  B  --A 

<&*  —  -*«»» 

Thus  if  the  limit  on  either  side  exists,  the  limit  of  the  other  side 
exists  and  both  are  equal. 

This  shows  that  in  an  infinite  series  we  may  omit  its  zero  terms 
without  affecting  its  character  or  value.  We  shall  suppose  this 
done  unless  the  contrary  is  stated. 

A  series  whose  terms  are  all  >  0  we  shall  call  a  positive  term 
series;  similarly  if  its  terms  are  all  <  0,  we  call  it  a  negative  term 
series.  If  an  >  0,  n  >  m  we  shall  say  the  series  is  essentially  a  pos 
itive  term  series.  Similarly  if  an <  0,  n>m  we  call  it  an  essen 
tially  negative  term  series. 

If  A  is  an  essentially  positive  term  series  and  divergent, 
lim  An  =  +  QO  ;  if  it  is  an  essentially  negative  term  series  and  di 
vergent,  lim  An=  -co. 

When  lim  An—  ±00,  we  sometimes  say  A  is  ±00. 

80.    1.    For  A  to  converge,  it  is  necessary  and  sufficient  that 

e>0,    m,    \An<p\<e,    n>m,  ^  =  1,2,—  (1 

For  the  necessary  and  sufficient  condition  that 

lim  An 

72  =  30 

exists  is  ~  .    ,  ,0 

€>0,    m,    \AV-  An\  <e,   v,   n>  m.  (2 

But  if  v  =  n+  p 

Av-  An=  An<p=an+1+  a-n+2+  •••  +an+p. 
Thus  2)  is  identical  with  1). 


PRELIMINARY   DEFINITIONS   AND   THEOREMS  79 

2.  The   two  series  A,  A,   converge   and  diverge  simultaneously. 
When  convergent, 

A  =  A,  +  A..  (3 

For  obviously  if  either  series  satisfies  theorem  1,  the  other 
must,  since  the  first  terms  of  a  series  do  not  enter  the  relation  1). 
On  the  other  hand,  .  A  A 

-"•«+p  —  •"•«  T  •***,  p" 

Letting  p  =  oo  we  get  3). 

3.  If  A  is  convergent,  An  =  Q. 

For  lim  An  =  lim  (A  -  An) 

—  A  —  lim  An  =  A  —  A 
=  0. 

For  A  to  converge  it  is  necessary  that  an  ==  0. 

For  in  1)  take  p  =  1  ;  it  becomes 

e         n  >  m 

We  cannot  infer  conversely  because  an  =  0,  therefore  A  is  con 
vergent.     For  as  we  shall  see  in  81,  2, 

1  +  J  +  1+  - 
is  divergent,  yet  lim  an  =  0. 

4.  The  positive  term  series  A  is  convergent  if  An  is  limited. 
For  then  lim  An  exists  by  I,  109. 

5.  A  series  whose  adjoint  converges  is  convergent. 
For  the  adjoint  A  of  A  being  convergent, 

e>0,    m,    |AB|P    <€,    n>m,  p  =1,  2,  3  ••• 
But 


Thus    '  l^d<« 

and  ^1  is  convergent. 

Definition.     A    series   whose   adjoint    is    convergent    is  called 
absolutely  convergent. 


80  SERIES 

Series  which  do  not  converge  absolutely  may  be  called,  when 
necessary  to  emphasize  this  fact,  simply  convergent. 

6.    Let  A  =  al  +  a^+  ••• 

be  absolutely  convergent. 

Let  B  =  a^  +  alt+  —      ;     i1<i2<  ••• 

be  any  series  whose  terms  are  taken  from  A,  preserving  their  relative 
order.      Then  B  is  absolutely  convergent  and 


choosing  n  so  large  that  An  contains  every  term  in  Bm.  Moreover 
for  m  >  some  m'  ,  An  —  Bm  >  some  term  of  A.  Thus  passing  to  the 
limit  in  1),  the  theorem  is  proved. 

7.    Let  A  =  a1  +  az  +  •••       The  series  B  =  ka1  +  ka2  +  ••- 
converges  or  diverges  simultaneously  with  A.      When  convergent, 

B  =  kA. 


We  have  now  only  to  pass  to  the  limit. 

From  this  we  see  that  a  negative  or  an  essentially  negative  term 
series  can  be  converted  into  a  positive  or  an  essentially  positive 
term  series  by  multiplying  its  terms  by  k  =  —  1. 

8.  If  A  is  simply  convergent,  the  series  B  formed  of  its  positive 
terms  taken  in  the  order  they  occur  in  A,  and  the  series  C  formed  of  the 
negative  terms,  also  taken  in  the  order  they  occur  in  A,  are  both 
divergent. 

If  B  and  0  are  convergent,  so  are  B,  F.     Now 
An  =  Bnv  +  Fna,         n  =  ^  +  n2. 

Hence  A  would  be  convergent,  which  is  contrary  to  hypothesis. 
If  only  one  of  the  series  B,  0  is  convergent,  the  relation 


shows  that  A  would  be  divergent,  which  is  contrary  to  hypothesis. 


PRELIMINARY   DEFINITIONS   AND   THEOREMS  81 

9.    The  following  theorem  often  affords  a  convenient  means  of 
estimating  the  remainder  of  an  absolutely  convergent  series. 


Let  A  =  al  -f-  #2  ~f~  '"  ^e  an  o^^olutely  convergent  series.  Let 
B  =  bl  +  b2  +  ••-  be  a  positive  term  convergent  series  whose  sum  is 
known  either  exactly  or  approximately.  Then  if  \  an  \  <  bn,  n  >  m 


<Bn<B. 


For 


<Bn<B. 

Letting  p  ==  oo  gives  the  theorem. 

EXAMPLES 

81.    1.    The  geometric  series  is  defined  by 


The  geometric  series  is  absolutely  convergent  when  |#|<1  and  di 
vergent  when  |$r|>l.      When  convergent, 

a=~  (2 


Hence  .,  „ 

ft-   —  & 

—  —      ~~ 


When  |#|<1,  lim  gn  =  0,  and  then 


When  |0|>1,  lim#ra  is  not  0,  and  hence  by  80,  3,  6r  is  not  conver 
gent. 

2.    The  series       ff=  1      1.       J_      1_      ^.  (3 


82  SERIES 

is  called  the  general  harmonic  series  of  exponent  /x.     When  /-i  =  1, 
it  becomes  J=l  +  i  +  .  +  {  +  ...  (4 

the  harmonic  series.     We  show  now  that 

The  general  harmonic  series  is  convergent  ivhen  IJL  >  1  and  is  di 
vergent  for  fJL  <  1. 

Let  /*>!.     Then 


Let  n  <  2".     Then 


Thus  lim  Hn  exists,  by  I,  109,  and 

'J<iI5'  C5 

Let  /*<!.     Then  1       -, 


Thus  3)  is  divergent  for  fi  <  1,  if  it  is  for  /z,  =  1. 
But  we  saw,  I,  141,  that 


lim  J 


n  =  oo, 


hence  J  is  divergent. 

It  is  sometimes  useful  to  know  that 


hm-^-=l.  (6 

log  n 

In  fact,  by  I,  180,  1 

log  n  log  n  -  log  O  -  1)  loef— 

*\n- 


n-l, 

=  1. 


PRELIMINARY  DEFINITIONS   AND   THEOREMS  83 

Since  *  n  >  log  n  >  lzn  •  •  -  we  have 

lim  —5=0      ;     lim  — -  =  oo     ,     r  >  1.  (7 

n  lrn 

Another  useful  relation  is 

11  1 

ffn=  1  -h  -  +  -  -h h  -  >log(7i -h  1).  (8 

2      6  n 

For  log(l  +  TW)  —  Iog7w  =  logf  1  H — )<— . 

\       mj      m 

Let  7/1  =  1,   2---71.     If   we  add   the  resulting   inequalities   we 
get  8). 

3.    Alternating  Series.     This  important  class  of  series  is  defined 
as  follows.     Let  a1  >  a2  >  a3  >  •••  =0. 

Then  ^  =  a1-a2  +  a3-a4  +  ...  (9 

whose  signs  are  alternately  positive  and  negative,  is  such  a  series. 
The  alternating  series  9)  is  convergent  and 

\An\<an+1.  (10 

For  let  p  >  3.     We  have 


If  p  is  even, 

P  =  On-fl  -  «n+2)  +   •"   +  On+P-l  ~  ^ 

If  p  is  odd, 


Thus  in  both  cases, 

P 
Again,  if  p  is  even, 

P  =  «n+1  -  (an+2  -  «n+a)  —  —  —  («n+p_2  -  #n+P-i)  ~  «n+P- 
*  In  I,  461,  the  symbol  "  lim  "  in  the  first  relation  should  be  replaced  by  Urn. 


84  SERIES 

If  p  is  odd, 

P  =  an+1  —  («n+2  —  aB+3)  —  ...  —  («n+p_!  —  an+p). 
Thus  in  both  cases, 


From  11),  12)  we  have 

0  <  an+1  -  an+2 
Hence  passing  to  the  limit  p=  oo, 


0  <  an+1  -  an+2  <  |  An,  p  |  <  an+l  - 


moreover,  .  n 

«n+l  =  0- 

Example  1.     The  series 

i-i+t-l+.v- 

being  alternating,  is  convergent.     The  adjoint  series  is 


which  being  the  harmonic  series  is  divergent.     Thus  13)  is  an 
example  of  a  convergent  series  which  is  not  absolutely  convergent. 


Example  2.     The  series 


_          _1_ 


'  V2  -  1      V2  +  1      V3  -  1      V3  +  1 

is  divergent,  although  its  terms  are  alternately  positive  and  nega 
tive,  and  an  =  0. 


m  — 
If  now  ^4.  were  convergent, 

lim  A  =  lim 


by  I,  103,  2. 


n 


PRELIMINARY  DEFINITIONS  AND   THEOREMS  85 

4.    Telescopic  Series.     Such  series  are 

A=(al-  aa)  +  (aa  -  «3)  +  («8  -  a4)  +  - 
We  note  that 

An=(a1-az)  +  -  +  (a»-an41) 

=  «i  -<W  (14 

Thus  the  terms  of  any  An  cancelling  out  in  pairs,  An  reduces  to 
only  two  terms  and  so  shuts  up  like  a  telescope. 
The  relation  14)  gives  us  the  theorem  : 

A  telescopic  series  is  convergent  when  and  only  ivhen  lim  an  exists. 

Let  ,  , 

A  =  al  +  «2  +  ...  denote  any  series. 

Then 

an  =  An  -  An_^     ,     A0  =  0. 

Hence 


This  shows  us  that 

-Awy  se?*^s  can  be  written  as  a  telescopic  series. 

This   fact,  as  we  shall  see,  is  of  great  value  in  studying  the 
general  theory  of  series. 

Example!.  A  =  —  —  I  —  -  —  u          -i  ____ 

^^^ 


—  in 

Thus  A  is  a  telescopic  series  and 

n 
Example  2.    Let  av  av  a8,  •-•  >  0.     Then 


(1  +  a,)  ... 

is  telescopic.     Thus 


and  J.  is  convergent  and  <  1. 


86  SERIES 

Examples.        A  =  ^] #=^0,  —1,  —2,  ••• 

-*•  *^  /"  „.  i  i  \  f  ™  i  „„  \ 


•4-  n  —  1     a:  H-  n 

is  telescopic. 

^  -1     1  -1. 

-  i  ,    —  •   ^—    —  * 


x      x  4-  n      x 

82.    Dini's  Series.      Let  A  =  al-\-a2-\-  •••  6e  a  divergent  positive 
term  series.      Then 


is  divergent. 
For 


_      m+l      , 
—     . 


>  ,  ^r    =1 


^  p  Am+p 


Letting  m  remain   fixed   and  _p  =  oo,    we    have    Dm>l,    since 
+p  ==  °°-     Hence  D  is  divergent. 

Lefc 


Hence  2)  =  i  +  i  +  i+...is  divergent. 

Let  A-1  +  J.4-J+.-: 

Then  -  -  -< 


is  divergent,  and  hence,  a  fortiori, 

v_l 


But  -^-n-l  >  log  W' 

Hence  -.  -,  -. 

V  _J__  =  _JL_  4.      1       _t_ 

^7  n  log  ^      2  log  2      3  log  3 


is  divergent,  as  J.5e/  first  showed. 


PRELIMINARY  DEFINITIONS   AND   THEOREMS  87 

83.    1.    Abels  Series. 

An  important  class  of  series  have  the  form 


As  Abel  first  showed  how  the  convergence  of  certain  types  of 
these  series  could  be  established,  they  may  be  appropriately  called 
in  his  honor.  The  reasoning  depends  on  the  simple  identity 
(Abel's  identity), 


p~l\fn+p-l~  ^n+p)  H~  ^n+p-^n,  pi  (^ 

where  as  usual  An^m  is  the  sum  of  the  first  m  terms  of  the  re 
mainder  series  An.  From  this  identity  we  have  at  once  the  fol 
lowing  cases  in  which  the  series  1)  converges. 

2.    Let   the   series   A  =  a^  +  a2  +  •••   and   the  series  2  tn+l  —  tn\ 
converge.    Let  the  tn  be  limited.     Then  B  =  afa  +  #2£2  4-  •••  converges. 

For  since  A  is  convergent,  there  exists  an  m  such  that 

An,p\<e\         n>m,        j0  =  1,  2,  3  .- 
Hence 


3.    Z/e^  the  series  A  =  a^  +  a%  4-  •••  converge.     Let  tr  tz,  t3  -•  be  a 
limited  monotone  sequence.      Then  B  is  convergent. 

This  is  a  corollary  of  2. 


4.  Let  A  =  al  +  a2  +  •  •  •  5e  swcA  iAa*  |  An  <  (7,  w  =  1,  2,  •  •  • 
2  1  ^n+1  —  ^w  |  converge  and  tn  =  0.     Then  B  is  convergent. 

For  by  hypothesis  there  exists  an  m  such  that 

I  tn+i  —  tn+z  |  4-  |  tn+2  —  tn+z  |  H-  •  •  •  +    tn+Ji  <  e 
for  any  n>m. 

5.  Let  \An\<&  and  ^  >  £2  >  ts  >  >-  =0.     Then  B  is  convergent. 
This  is  a  special  case  of  4. 


88  SERIES 

6.    As  an  application  of  5  we  see  the  alternating  series 

is  convergent.     For  as  the  A  series  we  may  take  A  =  l  — 1+1  — 
1  +  •••  as  \An\<l. 

84.    Trigonometric  Series. 

Series  of  this  type  are 

(7=  «0  +  a1  cos  x  +  a%  cos  2  x  +  aB  cos  3  x+  •••  (1 

S  =  al  sin  x  +  a2  sin  2  x  +  az  sin  3  x  +  ••«  (2 

As  we  see,  they  are  special  cases  of  Abel's  series.     Special  cases 
of  the  series  1),  2)  are 

r  =  J  +  cos  x  +  cos  2  x  +  cos  3  2;  -f-  .  •  . 
2  =  sin  x  +  sin  2  z  +  sin  3  x  +  ••• 
It  is  easy  to  find  the  sums  Tn,  Sn  as  follows.      We  have 


2  sin  mx  sin  j  -a?  =  cos     m  ~     x  -  cos 

2 

Letting  w  =  1,  2,  ...  w  and  adding,  we  get 

2  sin  1  x  •  2n  =  cos  |  2:  —  cos  ^  n  +     a:.  (5 

« 

Keeping  x  fixed  and  letting  n  =  oo,  we  see  Sn  oscillates  between 
fixed  limits  when  x  ^=  0,  ±  2  TT, 

Thus  2  is  divergent  except  when  x  =  0,  ±  TT,  ... 
Similarly  we  find  when  x  =£  2  WTT, 

r  _sinO-  j)a?  /« 

1  71  —  —  ;:  —  :  -  r^^  —  •  (  D 

2  sin  I  # 

Hence  for  such  values  Tn  oscillates  between  fixed  limits.     For 
the  values  x  =  2  rmr  the  equation  3)  shows  that  I\  =  +  oo. 
From  the  theorems  4,  5  we  have  at  once  now 

V  2  1  an+l  —  an  \  converges  and  an  =  0,  and  hence  in  particular  if 
ai>a2~  •"  ==  0,  the  series  1)  converges  for  every  x,  and  2)  converges 
for  x^2  mir. 


If  in  3)  we  replace  x  by  x  4-  TT,  it  goes  over  into 

A  =  \  —  cos  #  -J-  cos  2  a;  —  cos  3  x  +  ...  (7 


PRELIMINARY   DEFINITIONS   AND   THEOREMS  89 

Thus  An  oscillates  between  fixed  limits  if  x  =£  ±  (2  m  —  1)  TT, 
when  n  =  GO  .     Thus 

7f  2  |  0B+1  +  an    converges  and  an  =  0,  arcd  Aewce  in  particular  if 
a1>a2>  •  •  «  =0,  the  series  a0  —  ax  cos  x  +  «2  cos  2  z  —  a3  cos  3  x  -f 
converges  for  x  j=  (2  m  —  1)  TT. 

85.    Power  Series. 

An  extremely  important  class  of  series  are  those  of  the  type 


called  power  series.  Since  P  reduces  to  aQ  if  we  set  x  =  a,  we  see 
that  every  power  series  converges  for  at  least  one  point.  On  the 
other  hand,  there  are  power  series  which  converge  at  but  one 

point,  e.g. 

a0  +  l!(*-tf)  +  2!(:r-a)2  +  3!(*-a)3+  ...  (2 

For  if  x  =£  a,  lim  n\   x  —  a  \  n  —  ao,  and  thus  2)  is  divergent. 

1.    If  the  power  series  P  converges  for  x  =  b,  it  converges  absolutely 

within  -^  ,  ,  ,  , 

VK(a)     ,     \=\a-b\. 

If  P  diverges  for  x=b,  it  diverges  without  DA(a). 

Let  us  suppose  first  that  P  converges  at  b.     Let  #  be  a  point  in 
Z>A,  and  set  |  x  —  a  \  —  f  .     Then  the  adjoint  of  P  becomes  for  this 

point 


But  T  A 

lim  «nXn  =  0, 

since  series  P  is  convergent  for  x  =  b. 
Hence  .  ,,.- 


and  II  is  convergent.  X 

If  P  diverges  at  x  =  5,  it  must  diverge  for  all  5'  such  that 
|  b'  —  a  |  >  X.  For  if  not,  P  would  converge  at  b  by  what  we  have 
just  proved,  and  this  contradicts  the  hypothesis. 


90  SERIES 

2.  Thus  we  conclude  that  the  set  of  points  for  which  P  con 
verges  form  an  interval  (a  —  p,  a  +  p)  about  the  point  #,  called 
the  interval  of  convergence  ;  p  is  called  its  norm.  We  say  P  is 
developed  about  the  point  a.  When  a  =  0,  the  series  1)  takes  on 

the  simpler  form 

a 


which  for   many  purposes  is  just  as  general  as  1).     We  shall 
therefore  employ  it  to  simplify  our  equations. 

We  note  that  the  geometric  series  is  a  simple  case  of  a  power 
series. 

86.     Cauchy's  Theorem  on  the  Interval  of  Convergence. 

The  norm  p  of  the  interval  of  convergence  of  the  power  series, 


is  given  by  i 

-  =  hmVan         an  = 

We  show  H  diverges  if  f  >  p.     For  let 


Then  by  I,  338,  1,  there  exist  an  infinity  of  indices  iv  i2  •••  for 
which 


Hence 
and  thus 

since     3>l.     Hence 


v     fcln 

^ain£ 

71 

is  divergent  and  therefore  II. 

We  show  now  that  II  converges  if  f  <  p.     For  let 


Then  there  exist  only  a  finite  number  of  indices  for  which 


Let  m  be  the  greatest  of  these  indices.     Then 
V«n  </3        n>m. 


TESTS   OF  CONVERGENCE   FOR   POSITIVE   TERM  SERIES      91 
Hence 

d  «.? 

Thus 


and  H  is  convergent. 

Example  1.  2        * 

Here  -V^  =  _L  =  0         by  I,  185,  4. 

-faTf 

Hence  p  =  ao  and  the  series  converges  absolutely  for  every  x. 
Example  2.  *       * 

f-f+f-- 

1  O  c> 

Here  V^"n  =  -^L  =  1         by  I,  185,  3. 

Hence  /o=  1,  and  the  series  converges  absolutely  for  |  x  |<  1. 

Tests  of  Convergence  for  Positive  Term  Series 
87.    To  determine  whether  a  given  positive  term  series 

is  convergent  or  not,  we  may  compare  it  with  certain  standard 
series  whose  convergence  or  divergence  is  known.  Such  com 
parisons  enable  us  also  to  establish  criteria  of  convergence  of 
great  usefulness. 

We  begin  by  noting  the  following  theorem  which  sometimes 
proves  useful. 

1.    Let  A,  B  be  two  series  which  differ  only  by  a  finite  number  of 
terms.     Then  they  converge  or  diverge  simultaneously. 

This  follows  at  once  from  80,  2.     Hence  if  a  series  A  whose 
convergence  is  under  investigation  has  a  certain  property  only 


92  SERIES 

after  the  mill  term,  we  may  replace  A  by  Am,  which  has  this 
property  from  the  start.  • 

2.  The  fundamental  theorem  of  comparison  is  the  following  : 

Let  A  =  al  +  #2  +  ••-,  B  =  b1  +  62  -f  ••;•  be  two  positive  term  series. 
Let  r>0  denote  a  constant.  If  an<  rbn,  A  converges  if  B  does  and 
A  <  rB.  If  an  >  rbn,  A  diverges  if  B  does. 

For  on  the  first  hypothesis 

An<rBn. 
On  the  second  hypothesis 

An>rBn. 

The  theorem  follows  on  passing  to  the  limit. 

3.  From  2  we  have  at  once : 

Let  A  =  a1  -f  «2  -f-  •••,  B  =  bl  +  bz  +  •••  be  two  positive  term  series. 
Let  r,  s  be  positive  constants.  If 

a/n    .,  "i    o 

lim  -^ 

exists  and  is  3=-  0,  A  and  B  converge  or  diverge  simultaneously.  If 
B  converges  and  —  =  0,  A  also  converges.  If  B  diverges  and  -r=^ 
A  also  diverges. 

4.  Let  A  =  a1  -f-  a2  -f  •••,  B  =  b^  +  b2  +  •••  be  positive  term  series. 
If  B  is  convergent  and 

an+l  ^  °n+l  _  1      O     Q    ., 

<— —  n=  i,  ^,  o  ••• 

A  converges.     If  B  is  divergent  and 

an    ~~     °n 

A  diverges. 

For  on  the  first  hypothesis 


TESTS  OF   CONVERGENCE   FOR   POSITIVE   TERM   SERIES     93 

We  may,  therefore,  apply  3.     On  the  second  hypothesis,  we 
have 


and  we  may  again  apply  3. 

Exanplel.          A  =  ^2 
is  convergent.     For 


<  " 


n  •  n  -f 


and  V  —  is  convergent.    The  series  A  was  considered  in  81,  4,  Ex.  1. 
^  n2 

Example  2.        A  =  e~x  cos  x  +  e~2x  cos  2  x  -f  ••• 
is  absolutely  convergent  for  x  >  0. 

For 


which  is  thus  <  the  nth  term  in  the  convergent  geometric  series 


=  V  1  log 


is  convergent. 
For 


0<  «„  =  -        <. 

n2  \        n  y      w2 

Thus  ^4.  is  comparable  with  the  convergent  series  2~V 

~~l  TL 

88.  We  proceed  now  to  deduce  various  tests  for  convergence 
and  divergence.  One  of  the  simplest  is  the  following,  obtained 
by  comparison  with  the  hyperharmonic  series. 

Let  A  =  al  +  a2+  •••  be  a  positive  term  series.     It  is  convergent  if 

lim  ann^  <  oo     ,     JJL  >  1, 
and  divergent  if 

lim  nan  >  0. 


94  SERIES 

For  on  the  first  hypothesis  there  exists,  by  I,  338,  a  constant 
Gr  >  0  such  that 


Thus  each  term  of  A  is  less  than  the  corresponding  term  of  the 
convergent  series  GrZ^  —  • 

On  the  second  hypothesis  there  exists  a  constant  c  such  that 

an>-         ft  =  l,  2,  ... 
n 

and  each  term  of  A  is  greater  than  the  corresponding  term  of  the 

divergent  series  e  V  -. 
^  n 

Example  1.  A  =  V  -         w>0. 

^  log™  n 

Here  ^=-^  =  +  00,     by  I,  463. 

log™  ^ 

Hence  A  is  divergent. 

Example  2.  A  =  V  —  -  . 

^*  n  log  ft 

Here  nan=^-  =  0. 

log  ft 

Thus  the  theorem  does  not  apply.     The  series  is  divergent 
by  82. 

Example  8. 


where  /A  is  a  constant  and  |  6n  <  Gr. 

From  I,  413,  we  have,  setting  r  =  1  +  *, 


Hence 


TESTS  OF  CONVERGENCE   FOR  POSITIVE   TERM  SERIES     95 

and  L  is  divergent.     If  ^  >  0,  L  is  an  essentially  positive  term 
series.     Hence  L  =  +  00.     If  /*  <  0,  L  =  —  oo. 

Let     =  0.     Then 


which  is  comparable  with  the  convergent  series 


Thus  Z  is  convergent  in  this  case. 
Example  4-     The  harmonic  series 

1  +  J  +  J+  ••• 
is  divergent.     For  limnan  =  l. 

Example  5.  -, 

A  =  2    *i     a  ^  arbitrary. 

^^  Wa  lOgp  71 

Here  wl_a 

nan  =  -  —  -—  =  00      ,     a  <  1 


by  I,  463,  1.     Hence  A  is  divergent  for  a<  1. 
Example  6.  -, 

A  =v 


Here  -< 

wan  =  -fb  =  1         by  I,  185,  Ex.  3. 
vn 


7. 
Here,  if  /i  >  0, 


log(l  +  i 

\  /€- 


log  n          log 
Hence  A  is  divergent. 


l\n 

since  n*  >  loe^  n  and  ( 1  H —  ]   ==  e 

nj 


96  SERIES 

89.    D'Alemberfs  Test.      The  positive  term  series  A  =  a±  +  #2  +  •  •  ' 
converges  if  there  exists  a  constant  r  <  1  for  which 

^±l<r,  71  =  1,   2,  .- 

an 

/£  diverges  if 

«a±l>l. 
«» 

This    follows  from    87,  4,  taking  for  B   the   geometric   series 


Corollary.     Let  2a±la^.f.     J/*  /  <  1,  ^4.    converges.     If 

«« 
diverge*. 

Example  1.      The  Exponential  Series. 

Let  us  find  for  what  values  of  x  the  series 


is  convergent.     Applying  D'Alembert's  test  to  its  adjoint,  we  find 

xn     n-ll 


Thus  ^converges  absolutely  for  every  x. 

Let  us  employ  80,  9  to  estimate  the  remainder  En.     Let  x  >  0. 
The  terms  of  E  are  all  >  0.     Since 


^4-j[?         9^       fft 
we  have 


xn  f     x    V 
-yl     T~i~J   ' 


(2 


However  large  x  may  be,  we  may  take  n  so  large  that  x<n+  1. 
Then  the  series  on  the  right  of  2)  is  a  convergent  geometric  series. 
Let  x  <  0.     Then  however  large  |  z  |   is,  En  is  alternating  for 
some  m.     Hence  by  81,  3  for  n>^m, 

\W\^\X"  C\ 

-#nl<J— r-  0* 


TESTS   OF  CONVERGENCE   FOR  POSITIVE   TERM   SERIES     97 

Example  2.      The  Logarithmic  Series. 
Let  us  find  for  what  values  of  x  the  series 


is  convergent.     The  adjoint  gives 

"tn  *+i ' 

Thus  L  converges  absolutely  for  any   |z|<l,  and  diverges  for 
When  x  =  1,  L  becomes 


which  is  simply  convergent  by  81,  4. 
When  x  =  —  1,  L  becomes 


which  is  the  divergent  harmonic  series. 

Example  3.     A  =  —  +  —  +  —  +  — 

- 


an        \n  +  ij 

As  A  is  convergent  when  /x>l  and  divergent  if  p<1,  we  see 
that  D'Alembert's  test  gives  us  no  information  when  1  =  1.  It  is, 
however,  convergent  for  this  case  by  81,  2. 

Example  4- 


Here 

an4.i          » -h 


an        n  +  1  +  x 
and  D'Alembert's  test  does  not  apply. 

Example,  5. 

A  =  2 
Here 


*±!Y|- 


98  SERIES 

Thus  A  converges  for  |#|<1  and  diverges  for  \x\  >  1.  For 
\x\  =1  the  test  does  not  apply.  For  x  =  1  we  know  by  81,  2 
that  A  is  convergent  for  /-i  <  —  1,  and  is  divergent  for  /t  >  —  1. 

For  x  —  —  1,  A  is  divergent  for  /i  >  0,  since  an  does  not  =  0.  A 
is  an  alternating  series  for  p  <0,  and  is  then  convergent. 

90.  Cauchy's  Radical  Test.  Let  A  =  al  +  «2  -f  •••  be  a  positive 
term  series.  If  there  exists  a  constant  r  <  1  such  that 


A  is  convergent.     If,  on  the  other  hand, 


A  is  divergent. 

For  on  the  first  hypothesis, 

an<rn 

so  that  each  term  of  A  is  <,  the  corresponding  term  in 
r  _|_  r2  _j_  rs  _j_  . . .  a  convergent  geometric  series.  On  the  second 
hypothesis,  this  geometric  series  is  divergent  and  an>^rn. 

Corollary.     If  lim  \/an  =  I,  and  I  <  1,  A  is  convergent.     Ifl>\, 
A  is  divergent. 

Example  1.     The  series 

oo  1 

mr— \  -*-  \       sv         j 

Alogn7l  2 

is  convergent.     For 

1     =0. 


log  71 

Example  2. 

A. 


is  convergent.     For 

n-  nn  1         ^1 

e 


Example  3.     In  the  elliptic  functions  we  have  to  consider  series 
of  the  type 

6(v)  =  1  +  2  i0n'  cos  ZTrnv          0<q<l. 


TESTS  OF   CONVERGENCE   FOR   POSITIVE   TERM  SERIES      99 
This  series  converges  absolutely  if 

q  +  q*  +  q*+  "- 
does.     But  here 

Va*  =  Vq*  =  qn  =  Q. 

Thus  6(v)  converges  absolutely  for  every  v. 
Example  4-     Let  0  <  a  <6  <  1.     The  series 


n  =  2  m 


is  convergent.     For  if 

If  w  =  2m-f-l,  n_      2m+i  — 

Thus  for  all  n 

Va~n<b<l. 

Let  us  apply  D'Alernbert's  test.     Here 


Thus  the  test  gives  us  no  information. 

91.    Cauchy's  Integral  Test. 

Let  </>(#)  be  a  positive  monotone  decreasing  function  in  the  interval 
(«,  QO  ).      The  series 


is  convergent  or  divergent  according  as 


is  convergent  or  divergent. 

For  in  the  interval  (n,  n  +  1),         n>m>a, 


100  SERIES 

Hence 


rn+l 
<#>O  +  1)<  I      ^dx<4)(n). 

\s  n 

Letting  n  =  m,  m  +  1,  •••  m  +  j?,  and  adding,  we  have 


Passing  to  the  limit  p  =  GO,  we  get 

*«<    fV*^*-!.  (1 

*^m 

which  proves  the  theorem. 

Corollary.      When  <£  is  convergent 


Example  1.     We  can  establish  at  once  the  results  of  81,  2.     For, 
taking  *( 


is  convergent   or  divergent    according  as  /i  >  1,  or  /-i  <  1,  by  I, 
635,  636. 

We  also  note  that  if 

A-  JL      J_  .  J_  . 

~ 


—       (*™   1         11 
then  ^<  I     JL.i-.JL, 

*^n    a;1+'x      /x     w** 

Example  2.     The  logarithmic  series 

1 


_  1    9 
wZf  w  "I  *V   ^  fl\Y  Vf\ 

JN 

are  convergent  if  /A  >  1  ;  divergent  if  /4<1.  t  ^f1^  ^43 

We  take  here 


and  apply  I,  637,  638. 


TESTS   OF   CONVERGENCE   FOR   POSITIVE   TERM   SERIES  101 

92.  1.  One  way,  as  already  remarked,  to  determine  whether 
a  given  positive  term  series  A  =  al  +  a2+  •••  is  convergent  or 
divergent  is  to  compare  it  with  some  series  whose  convergence  or 
divergence  is  known.  We  have  found  up  to  the  present  the 
following  standard  series  S: 

The  geometric  series 


The  general  harmonic  series 

1  +  1  +  1+- •  (2 

1  n         £)(*.         QJU,  ^ 

The  logarithmic  series 


We  notice  that  none  of  these  series  could  be  used  to  determine 
by  comparison  the  convergence  or  divergence  of  the  series  follow 
ing  it. 

In  fact,  let  an,  bn  denote  respectively  the  nth  terms  in  1),  2). 
Then  for  g  <  1,  p  >  0, 

A_  =  J_  =  ^I±!!=00         by  I,  464, 
«n+i      n»g»         n» 

or  using  the  injinitary  notation  of  I,  461, 

bn  >  an. 

Thus  the  terms  of  2)  converge  to  0  infinitely  slower  than  the 
terms  of  1),  so  that  it  is  useless  to  compare  2)  with  1)  for  conver 
gence.  Let#>l.  Then 


«.>».. 


This  shows  we  cannot  compare  2)  with  1)  for  divergence. 


102  SERIES 

Again,  if  «n,  bn  denote  the  nth  terms  of  2),  3)  respectively,  we 
have,  if  /i  >  1, 

^  =  -^-  =  00         by  I,  463, 
an     log'*  n 

or  7    , 


^5  =  log  n  =  QO, 


Thus  the  convergence  or  divergence  of  3)  cannot  be  found 
from  2)  by  comparison.  In  the  same  way  we  may  proceed  with 
the  others. 

2.  These  considerations  lead  us  to  introduce  the  following 
notions.  Let  A  =  al  +  a2+  •••,  B  =  bl  +  62  +  •••  be  positive  term 
series.  Instead  of  considering  the  behavior  of  an/bn,  let  us  gen 
eralize  and  consider  the  ratios  An  :  Bn  for  divergent  and  An  :  Bn 
for  convergent  series.  These  ratios  obviously  afford  us  a  measure 
of  the  rate  at  which  An  and  Bn  approach  their  limit.  If  now  A, 

B  are  divergent  and  .        ^ 

An  ~  J5n-> 

we.  say  A,  B  diverge  equally  fast  ;  if 

An<Bn, 

A  diverges  slower  than  B,  and  B  diverges  faster  than  A.     From 
I,  180,  we  have  : 

Let  A,  B  be  divergent  and 


According  as  I  is  0,  =£0,   oo,  A  diverges  slower,  equally  fast,  or 
faster  than  B. 

If  A,  B  are  convergent  and 


we  say  A,  B  converge  equally  fast  ;  if  A  converges  and 


TESTS  OF  CONVERGENCE   FOR  POSITIVE   TERM   SERIES    103 

B  converges  faster  than  A,  and  A  converges  slower  than  B.     From 
I,  184,  we  have  : 

Let  A,  B  be  convergent  and 

lira  ^=1 
on 

According  as  I  is  0,  =£  0,  oc,  A  converges  faster,  equally  fast,  or  slower 
than  B. 

Returning  now  to  the  set  of  standard  series  #,  we  see  that  each 
converges  (diverges)  slower  than  any  preceding  series  of  the  set. 
Such  a  set  may  therefore  appropriately  be  called  a  scale  of  con 
vergent  (divergent)  series.  Thus  if  we  have  a  decreasing  positive 
term  series,  whose  convergence  or  divergence  is  to  be  ascertained, 
we  may  compare  it  successively  with  the  scale  S,  until  we  arrive 
at  one  which  converges  or  diverges  equally  fast.  In  practice  such 
series  may  always  be  found.  It  is  easy,  however,  to  show  that  there 
exist  series  which  converge  or  diverge  slower  than  any  series 
in  the  scale  S  or  indeed  any  other  scale. 

Forlet  A,    S,     0,...     '  (2 

be  any  scale  of  positive  term  convergent  or  divergent  series. 
Then,  if  convergent, 


if  divergent,  An>  Bn>  Cn>  ... 

Thus  in  both  cases  we  are  led  to  a  sequence  of  functions  of  the 


Thus  to  show  the  existence  of  a  series  ft  which  converges  (di 
verges)  slower  than  any  series  in  2,  we  have  only  to  prove  the 
theorem  : 

3.    (Du  Bois  Reymond.^)     In  the  interval  (a,  oo)  let 


denote  a  set  of  positive  increasing  functions  which   =00  as  x  =  oo  . 

Moreover,  let  /. 

J\ 


104  SERIES 

Then  there  exist  positive  increasing  functions  which  =  oc  slower  than 
anyfn. 

Foras/1>/2  there  exists  an  a1>a  such  that  /1>/2  +  l  for 
x>  ar  Since  /2  >/3,  there  exists  an  a2  >  a1  such  that  /2  >/3  +  2 
for  x>a%.  And  in  general  there  exists  an  an>an_1  such  that 

fn  >fn+l  +  n    f°r  X  >  an'        Let  HOW 

g(x)  =  fn(x)+n-l         in  (an_x,  <*„)• 

Then  g  is  an  increasing  unlimited  function  in  (a,  oo)  which 
finally  remains  below  any  fm(x)  +  m  —  1,  w  arbitrary  but  fixed. 


Thus  Q<ijm  yvv   =ijm y\^i <lim   jm+i-r"«   =  0> 

Hence  g<fm- 

93.    From  the  logarithmic  series  we  can  derive  a  number   of 
tests,  for  example,  the  following : 

1.    (Bertram's  Tests.)     Let  A  =  al  +  a2  +  •••  be  a  positive  term 
series. 

Let  log-      -1-y— 

ft(M)=        «n^-  l.-in         s==l,  2,  ...         I0n=l. 

If  for  some  s  and  m, 

Q8(.n)  ^  A1  >  1         71  >  w,  (1 

^4.  ^s  convergent.     If,  however, 

&O)<1,  (2 

^1  ^s  divergent. 

For  multiplying  1)  by  Z8+1n,  we  get 


i 


Hence 


or 


TESTS  OF   CONVERGENCE   FOR  POSITIVE   TERM   SERIES  105 

Thus  A  is  convergent. 

The  rest  of  the  theorem  follows  similarly. 


2.    For  the  positive  term  series  A=al  +  a%  +  --to  converge  it  is 
necessary  that,  for  n  =  oo, 

lim  an  =  0,       lim  nan  =  0,       lira  na^n  =  0,       lim^naj^nl^n  =  0,  ••• 
We  have  already  noted  the  first  two.     Suppose  now  that 

lim  nanl^n  •••  l,n  >  0. 
Then  by  I,  338  there  exists  an  m  and  a  c  >  0,  such  that 

naj-^n  •••  l,n  >  c     ,     n  >  m, 
or 


Hence  A  diverges. 
Example  1. 


««>^-r 

nl^n  •••  l,n 


- 

na  log*3  n 


We  saw,  88,  Ex.  5,  that  A  is  divergent  for  a  <  1.  For  «=  1, 
A  is  convergent  for  fi  >  1  and  divergent  if  yS  ^  1,  according  to 
91,  Ex.  2. 

If  a  >1,  let  a=a'  +  a"  a">l 

Then  if  /3  >  0,  -,  -, 

<—     ,     n  >  2, 


and  A  is  convergent  since  ^  —  is.     If  ft  <  0,  let 


Then  1     „,  n       1 

a"~     n0-'      '  n?'' 

But  log^'n<n«'         by  I,  463,  1 ; 

and  A  is  convergent  since  2  — ~  is- 


106  SERIES 

Example  2.  -,  ., 

A        \^  1  ^       1 

^  =  x — — : jT  =  2, — F' 

I    1  -f-        -4      ...-!__     1  ^^    ->i  ^/>      tl 

^?M/?  2  ^ 

Here  . 

^  aMft      -  log  n  +  A*  log  7i+  IT, 

Vl ; ~ ^ 

62ft  t2/l 

/x-14--^}^^^          by  81,  6). 
log  ft  J 

Hence  J.  is  convergent  for  ft  >  0  and  divergent  for  /A  <  0.     No 
test  for  fi  =  0. 

But  for  /i  =  0,  1 

log _ 

/Tf     ^77     >7,  /•/          __r     /    'M /    ,vi 

2  Lw  Z0^ 


since  I2n  >  I3n.     Thus  A  is  divergent  for  /a  =  0. 

94,    A  very  general  criterion  is  due  to  Kummer,  viz. : 

Let  A  =  al  +  a2  4-  •>•  be  a  positive  term  series.     Let  kv  &2,  •••  be  a 

set  of  positive  numbers  chosen  at  pleasure.     A  is  convergent,  if  for 

some  constant  k  >  0. 

<w .  =  1     9    . 


«*+! 

^4.  ^s  divergent  if 


is  divergent  and 

For  on  the  first  hypothesis 

1, 


TESTS   OF   CONVERGENCE   FOR  POSITIVE  TERM   SERIES    107 
Hence  adding, 


and  A  is  convergent  by  80,  4. 
On  the  second  hypothesis, 


^±1>«1 

«»     "^n1 

Hence  JL  diverges  since  ^  is  divergent. 

95.    1.    From  Rummer's  test  we  may  deduce  D'Alembert's  test 
at  once.     For  take 

k1  =  kt=  ..-  =1. 

Then  A  =  a^  +  «2  -f-  •••  converges  if 

t.«.  if 

?2 

« 

Similarly  A  diverges  if  ^»±i  >^1. 

«• 

2.   To  derive  Raabe's  test  we  take 

~kn  —  n. 
Then  A  converges  if 


j.  if 


Similarly  A  diverges  if 


108  SERIES 

96.    1.    Let  A  =  a1  +  a2  +  •••  be  a  positive  term  series.     Let 


X2O)  =  I2n 


Then  A  converges  if  there  exists  an  s  such  that 

\(n)  >  S  >  1        for  some  n>m\ 

it  diverges  if  ^  /  N    .  ^  /. 


We  have  already  proved  the  theorem  for  X0(w).     Let  us  show 
how  to  prove  it  for  Xj(^).     The  other  cases  follow  similarly. 
For  the  Kummer  numbers  kn  we  take 

kn  =  n  log  n. 
Then  A  converges  if 


As 


-  log( 


l  4-        - 


1V+1 
n) 


Thus  ^1  converges  if  Xj(^)  >  8  >  1  for  n>m. 

In  this  way  we  see  that  .A  diverges  if  \(n)  <  1,  n>m. 

2.     Oahens   Test.     For  the  positive  term  series  to  converge  it  is 
necessary  that 


TESTS  OF   CONVERGENCE   FOR   POSITIVE   TERM   SERIES    109 

For  if  this  upper  limit  is  not  +  oo, 


for  all  n.     Hence 


But  the  right  side  =0.      Hence  X1(^)<1  for  w>some  w,  and 
A  is  divergent  by  1. 

Example.    We  note  that  Raabe's  test  does  apply  to  the  harmonic 

series  i  4.  i  _i_  i  4.  (\ 

Here 


Hence  Pn  =  0,         and 

lim  Pn  =  0. 
Hence  the  series  1)  is  divergent. 

97.     Grauss'  Test.     Let  A  =  «j  +  «2  -f   •••  be  a  positive  term  series 

such  that  , 

an  =ns  +  aji*-i+  •••  +  a, 

where  s,  a^  •••  b1  •••  do  not  depend  on  n.      Then  A  is  convergent  if 
al  —  bl  >  1,  and  divergent  if  al  —  b1  <  1. 

Using  the  identity  I,  91,  2),  we  have 

T  _L      (  1 


Thus  lim  X0(V)  =  a1  —  br  Hence,  if  a1  —  b1  >  1,  A  is  Conver 
gent ;  if  a1  —  #!<!,  it  is  divergent.  If  al  —  b1  =  1,  Raabe's  test 
does  not  always  apply.  To  dispose  of  this  case  we  may  apply 
the  test  corresponding  to  ^(V).  Or  more  simply  we  may  use 
Cahen's  test  which  depends  on  X^n).  We  find  at  once 

lim  Pn  —  #2  —  b2  —  bl  <  QO  ; 
and  A  is  divergent. 


110  SERIES 

98.    Let  A  =  a±  -f  #2  -f-  •••  be  a  positive  term  series  such  that 


.A  «*  convergent  if  a  >  1  cwd  divergent  if  a<  1. 


For 


_^L__1    =  «  +  J^  = 
an^        J  n^'1 


and  A  converges  if  a  >  1  and  diverges  if  a  <  1.     If  a  =  1, 
and  A  is  divergent. 

EXAMPLES 

99.    The  Binomial  Series.     Let  us  find  for  what  values  of  x  and 
Ai  the  series 


converges.  If  ft  is  a  positive  integer,  B  is  a  polynomial  of  degree  ft, 
For  ft  =  0,  5=1.  We  now  exclude  these  exceptional  values  of  ft. 
Applying  D'Alembert's  test  to  its  adjoint  we  rind 

—  n+  1 


*   =  \x  . 


Thus  5  converges  absolutely  for  x  \  <  1  and  diverges  for  \x\  >  1 
Letx  =  l.     Then 


Here  D'Alembert's  test  applied  to  its  adjoint  gives 


As  this  gives  us  no  information  unless  p<  —  1,  let  us  apply 
Raabe's  test.     Here 


,  for  sufficiently  large  n 


n 


TESTS   OF   CONVERGENCE   FOR   POSITIVE   TERM   SERIES  111 

Thus  B  converges  absolutely  if  /*  >  0,  and  its  adjoint  diverges 
if  fi<  0.  Thus  B  does  not  converge  absolutely  for  ft  <  0. 

But  in  this  case  we  note  that  the  terms  of  B  are  alternately 
positive  and  negative.  Also 


1- 


n 


so  that  the  |an|  form  a  decreasing  sequence  from  a  certain  term. 
We  investigate  now  when  an  =  0.     Now 


In  I,  143,  let  a  =  —  /*,  /3  =  1.  We  thus  find  that  lim  an  =  0  only 
when  /*>  —  1.  Thus  -B  converges  when  /*>  —  1  and  diverges 
when  /!<  —  !. 

=  -l.     Then 


1-2  1-2.3 

If  /A  >  0,  the  terms  of  B  finally  have  one  sign,  and 

"(fc-'>- 

Hence  B  converges  absolutely. 

If  n  <  0,  let  fj,  =  -  X.     Then  B  becomes 


.*    ,  X-X  +  1  ,  X-X 

~r  A,  -| 1 


1-2 


1.2-3 


Here 


Hence  ^  diverges  in  this  case.     Summing  up : 

The  binomial  series  converges  absolutely  for  \x\<1  and  diverges 
for  \x\  >  1.  When  x  =  \  it  converges  for  p >  —  1  and  diverges  for 
fji  <  —  1 ;  it  converges  absolutely  only  for  /JL  >  0.  When  x  =  —  1,  & 
converges  absolutely  for  p  >  0  awd  diverges  for  p  <  0. 


112  SERIES 

100.     The  Hypergeometric  Series 
A  7,  *)=l  +  s  +  « 


o 


Let  us  find  for  what  values  of  x  this  series  converges.     Passing 
to  the  adjoint  series,  we  find 


X     =     X  . 


Thus  .F  converges  absolutely  for    x  \  <  1  and  diverges  for  |  x  \  >  1. 
Let  x=1.     The  terms  finally  have  one  sign,  and 
qn+1  _  n2  +  n(l  +  7)  +  7 


Applying  Gauss',  test  we  find  ^  converges  when  and  only  when 


a;  =  —  1.     The  terms  finally  alternate  in  sign.     Let  us  find 
when  an  =  0.     We  have 


Now 


m 


—  )     , 
mj 


Thus 

K+2|  =  n^ 

But  by  I,  91,  1), 

1  1 


mj\        m 


m 


1  + 


m 


1+^ 


m< 


where  crm  =  1,  rm  =  72  as  w  =  oo. 


PRIXGSHELM'S   THEORY  113 

Hence 


m 
Hence 


and  thus 

Z  =  lira  log 

i 

Now  for  an  to  =  0  it  is  necessary  that  Ln  =  —  so.     In  88,  Ex.  3, 
we  saw  this  takes  place  when  and  only  when  «  +  /3  —  7—  1<0. 
Let  us  find  now  when    an+l  \  <  |  an  \.     Now  1)  gives 


Thus  when  «  +  /3  —  7  —  1<0,  |  «n+2 1  <  |  an+l  .  Hence  in  this 
case  F  is  an  alternating  series.  We  have  thus  the  important 
theorem : 

The  hypergeometric  series  converges  absolutely  when  x\<\  and 
diverges  when  \x\>\.  When  x  =  \,  F  converges  only  when  a  +  /3 
—  7<0  and  then  absolutely.  When  x  =  —  1,  F  converges  only 
when  ct  +  /3  —  7  —  1<0,  and  absolutely  if  a.  -f-  @  —  7  <  0. 

Pnngsheims   Theory 

101.  1.  In  the  35th  volume  of  the  Mathematische  Annalen 
(1890)  Pringsheim  has  developed  a  simple  and  uniform  theory  oi 
convergence  which  embraces  as  special  cases  all  earlier  criteria, 
and  makes  clear  their  interrelations.  We  wish  to  give  a  brief 
sketch  of  this  theory  here,  referring  the  reader  to  his  papers  for 
more  details. 

Let  Mn  denote  a  positive  increasing  function  of  n  whose  limit 
is  4-  oo  for  n  =  DO  .  Such  functions  are,  for  example,  p  >  0, 

n»     ,     log'1  n     ,     l$n     ,     l-^nl^n  •••  Ig^nl^n 


114  SERIES 

A^t  where  A  is  any  positive  term  divergent  series. 
Bn~*  where  B  is  any  positive  term  convergent  series. 


It  will  be  convenient  to  denote  in  general  a  convergent  positive 
term  series  by  the  symbol 

0=^+%+  ... 

and  a  divergent  positive  term  series  by 

D  =  dl  +  di  +  ... 
2.    The  series 


is  convergent,  and  conversely  every  positive    term  convergent  series 
may  be  brought  into  this  form. 

For 


and  C  is  convergent. 

Let   now  conversely    C—  cl  -f-  c2  4-  ..-be   a    given   convergent 
positive  term  series.     Let 

tf»-l  =  —  • 

Then 
3. 


rn         M.+1 

1-^n)  -  (2 

i*  divergent,  and  conversely  every  positive  term  divergent  series  may 
be  brought  into  this  form. 
For 


PRINGSHEIM'S   THEORY  115 

Let  now  conversely  D  =  dl  +  d^-{-  •••  be  a  given  positive  term 
divergent  series.  Let  M  -  T) 

Then  d  =M       -M 

102.  Having  now  obtained  a  general  form  of  all  convergent 
and  divergent  series,  we  now  obtain  another  general  form  of  a 
convergent  or  divergent  series,  but  which  converges  slower  than 
1)  or  diverges  slower  than  101,  2).  Let  us  consider  first  con 
vergence.  Let  M'n  <  Mn,  then 

-<     \ 

(i 


is  convergent,  and  if  M'n  is  properly  chosen,  not  only  is  each 
term  of  1)  greater  than  the  corresponding  term  of  101,  1),  but  1) 
will  converge  slower  than  101,  1).  For  example,  for  M'n  let  us 
take  M*,  0  <  /*  <  1.  Then  denoting  the  resulting  series  by 
C'  =  2c',  we  have 


n         urn  nr*       w         M 

On          M^M*+l     lYLn+l  —  Mn 

=  ^  ^n"M       »       r  =  <  I*  (2 

1  -  r  Mn+1 

Thus   C'  converges  slower  than   0.     But   the   preceding   also 
shows  that  0'  and  ,..          ,- 

^        '  ~M*H  (B 

converge  equally  fast.     In  fact  2)  states  that 

Since  Mn  is  any  positive  increasing  function  of  n  whose  limit 
is  oo,  we  may  replace  Mn  in  3)  by  lrMn  so  that 


is  convergent  and  a  fortiori 

^lrMn+]-lrMn         r  =  1  2    ..  (4 

A      Q+"3f.+1 
is  convergent. 


116  SERIES 

Now  by  I,  413,  for  sufficiently  large  n, 

log  Mu+l  -  log  Mn  =  -  log(l  - 

V  -" 

Replacing  here  Mn  by  log  7ffn,  we  get 

Z  M 

fc2^"»+l  ~ 

and  in  general 


Thus  the  series 
V 


f f\ 

V 


converges  as  is  seen  by  comparing  with  4).     We  are  thus  led  to 
the  theorem  : 


MnMa+l 


. 
=    '    '  •••' 


form,  an  infinite  set  of  convergent  series;    each  series  converging 
slower  than  any  preceding  it. 

The  last  statement  follows  from  I,  463,  l,  2. 

Corollary  1  {Abel).     Let  D  =  d-^  +  d2  -f-  •••  denote  a  positive  term 
divergent  series.      Then 


is  convergent. 

Follows  from  3),  setting  Mn+1  =  Dn. 

Corollary  2.     If  we  take  Mn  =  n  we  get  the  series  91,  Ex.  2. 

Corollary  3.  Being  given  a  convergent  positive  term  series 
C  =  cl  +  c2  4-  •••  we  can  construct  a  series  which  converges  slower 
than  C. 


PRINGSHEIM'S   THEORY  117 

For  by  101,  2  we  may  bring  Q  to  the  form 


Then  any  of  the  series  7)  converges  slower  than  0. 

103.     1.    Let   us    consider   now   divergent   series.       Here    our 
problem  is  simpler  and  we  have  at  once  the  theorem  : 

The  series  ™    TUT          ^ 

J>-|^^=?4,  a 

diverges  sloiver  than 

(2 


That  1)  is  divergent  is  seen  thus  :     Consider  the  product 

fA 

i    M 


which  obviously  =  oc. 
Now 


Hence  Dn  =  oo  and  Z>  is  divergent. 

As  ^  =  JL=0 

di     Mn 

we  see  that  1)  converges  slower  than  2). 

2.    Any  given  positive  term  series  D  =  d^  +  d2  +  .-•  caw 
the  form  -Z). 

For  taking  J^  >  0  at  pleasure,  we  determine  Jf2,  J[f3  ...  by  the 
relations  T 


118  SERIES 

Then  Mn+1  >  Mn  and 

,  _  Mn+l  —  Mn 
—         n/r 

•L'J-n 

Moreover  Mn  =  oo.     For 


>!  +  !>„         by  I,  90,  1. 
But  Dn  =  oo. 

3.    The  series 


t^m    '='0«1'2'" 

form  an  infinite  set  of  divergent  series,  each  series  divergent  slower 
than  any  preceding  it.     l^Mn  =  Mn. 

For  log  Mn+l  -  log  Mn  =  log  (l  +  Mn^~Mn^ 


Mn 

This  proves  the  theorem  for  r  =  0.     Hence  as  in  102  we  find, 
replacing  repeatedly  Mn  by  log  Mm 


Corollary  1.     If  we  take  Mn  =  n,  we  get  the  series  91,  Ex.  2. 
Corollary  2  {Abel).     Let  D  =  d1  4-  d2  +  ••«  be  a  divergent  positive 
term  series.      Then  , 


is  divergent. 

We  take  here  Jlfn  =  Dw. 

Corollary  3.     Being  given  a  positive  term  divergent  series  D,  we 
can  construct  a  series  which  diverges  slower  than  D. 
For  by  101,  3  we  may  bring  D  to  the  form 


Then  1)  diverges  slower  than  D. 


PRINGSHEIM'S   THEORY  119 

104.    In  Ex.  3  of  I,  454,  we  have  seen  that  Mn+i  is  not  always  ~ 
Mn.     In  case  it  is  we  have 

1.    The  series 


^s  convergent. 

Follows  from  102,  3). 

2.    The  series 


is  convergent  if  \i  >  0  ;  #  ?'s  divergent  if  /x<  0. 

For  ^«  >  I  /iWn2  -  Ml         p>  0. 

Thus 


If/i<0 


3.    jy  J^+1  ~  Mn,  we  have 
I     M     -I     M 


For  by  102,  5),  103,  3), 

7       W  7       AT  ~ 

~ 


7         TI^-  7         AT 

r+l    n+l~  r+l    n' 
Now  since  Mn+l~  Mn,  we  have  also  obviously 
lmMn~lmMn+l        m=l,2,-r. 

105.  Having  obtained  an  unlimited  set  of  series  which  converge 
or  diverge  more  and  more  slowly,  we  show  now  how  they  may  be 
employed  to  furnish  tests  of  ever  increasing  strength.  To  ob 
tain  them  we  go  back  to  the  fundamental  theorems  of  comparison 
of  87.  In  the  first  place,  if  A=  a^  +  a2  -f  •••  is  a  given  positive 
term  series,  it  converges  if 


120  SERIES 

It  diverges  if 


(2 

**» 

In  the  second  place,  A  converges  if 

^±i_£n±a<0,  (3 

«n  Cn 

and  diverges  if  , 

an         dn 

The  tests  1),  2)  involve  only  a  single  term  of  the  given  series 
and  the  comparison  series,  while  the  tests  3),  4)  involve  two 
terms.  With  Du  Bois  Reymond  such  tests  we  may  call  respec 
tively  tests  of  the  first  and  second  kinds.  And  in  general  any 
relation  between  p  terms 

&ni  ^«+l»   *"*  an+p-l 

of  the  given  series  and  p  terms  of  a  comparison  series, 


•'   Cn+p-\'>       Or      n>  <+i        "'   <+p-l 

which  serves  as  a  criterion  of  convergence  or  divergence  may  be 
called  a  test  of  the  pth  kind. 

Let  us  return  now  to  the  tests  1),  2),  3),  4),  and  suppose  we 
are  testing  A  for  convergence.  If  for  a  certain  comparison 
series  0 

—         not  always  <_6r     ,     n  >  m 

cn 

it  might  be  due  to  the  fact  that  cn  =  0  too  fast.  We  would  then 
take  another  comparison  series  (7'=  ^cfn  which  converges  slower 
than  (7.  As  there  always  exist  series  which  converge  slower  than 
any  given  positive  term  series,  the  test  1)  must  decide  the  con 
vergence  of  A  if  a  proper  comparison  series  is  found.  To  find 
such  series  we  employ  series  which  converge  slower  and  slower. 
Similar  remarks  apply  to  the  other  tests.  We  show  now  how 
these  considerations  lead  us  most  naturally  to  a  set  of  tests  which 
contain  as  special  cases  those  already  given. 

106.  1.  G-eneral  Criterion  of  the  First  Kind.  The  positive  term 
series  A  =  a^  -f  «2  4-  •••  converges  'if 


PRINGSHEIM'S   THEORY  121 

It  diverges  if  }[m        Mn  >  Q<  2 

-Mn+1-Mn 

This  follows  at  once  from  105,  1),  2);  and  101,  2;  103,  1. 

2.    To  get  tests  of  greater  power  we  have  only  to  replace  the 

^    nr     M       ' 


series 


just  employed  in  1),  2)  by  the  series  of  102  and  103,  3  which  con 
verge  (diverge)  slower.     We  thus  get  from  1  : 

The  positive  term  series  A  converges  if 


It  diverges  if          ^  Mnl,Mn  .-  lrMn  ^  >  ^ 

Mn^  -  Mn 

Bonnets  Test.      The  positive  term  series  A  converges  if 

lira  n^n  •••  lr-^nl}.+ttn  •  an  <  oo     ,     IJL  >  0. 
It  diverges  if  ihp  ^  ...  ^  .  fln>0. 

Follows  from  the  preceding  setting  Mn  =  n. 
3.    The  positive  term  series  A  converges  or  diverges  according  as 

^""V  <  1    ,     M>0,  (3 

Mn+l-Mn  Mn+1~Mn. 

<1     ,     /*<0. 
For  in  the  first  case 


and  in  the  second  case 


The  theorem  follows  now  by  104,  2. 
4.    The  positive  term  series  A  converges  if 
log  #.+!-•%.  loff  -  _ 

-  g 


122  SERIES 

It  diverges  if 


, 

t 


p-  n  <()  orl  rnn 

hm  -  TUT  -  <()          or  inn  -  -  —  -j^  -  <o. 

2Un  (,r+llUn 

Here  r  =  0,  1,  2,  •••  awe?  as  6e/0re  /0M"n  =  7ffn. 
For  taking  the  logarithm  of  both  sides  of  3)  we  have  for  con 
vergence  Mn+l  -  Mn 


As  p  is  an  arbitrarily  small  but  fixed  positive  number,  A  con 
verges  if  lim  q  >  0.  Making  use  of  104,  3  we  get  the  first  part 
of  the  theorem.  The  rest  follows  similarly. 

Remark.  If  we  take  Mn  —  n  we  get  Cauchy's  radical  test  90 
and  Bertram's  tests  93. 

Forif        log!  . 


it  is  necessary  that 
Also  if 


annlln~-lrn_ 

0                 7                      7                      1       1U6    7     " 

annl^n  •••  lr^n            lrn 

lr+1n 

lr+ln 
loo*1 

1  4.             n     1     '  'r-l> 

r+l 
it  is  necessary  that  -^ 


lr+ln 

107.  In  94  we  have  given  Rummer's  criterion  for  the  conver 
gence  of  a  positive  term  series.  The  most  remarkable  feature 
about  it  is  the  fact  that  the  constants  kv  k2-~  which  enter  it  are 
subject  to  no  conditions  whatever  except  that  they  shall  be  positive. 
On  this  account  this  test,  which  is  of  the  second  kind,  has  stood 
entirely  apart  from  all  other  tests,  until  Pringsheim  discovered  its 
counterpart  as  a  test  of  the  first  kind,  viz.  : 


PRINGSHEIM'S   THEORY  123 

Pringsheims  Criterion.  Let  pr  p2---  be  a  set  of  positive  numbers 
chosen  at  pleasure,  and  let  Pn—p^  +  •••  +  pn.  The  positive  term 
series  A  converges  if 


For  A  converges  if 


lim  _  ^L>0.  (1 

* 


lim — ^ >  0     ,     by  106,  4.  (2 

But  Mn+1  —  Mn  =  dn  is  the  general  term  of  the  divergent  series 
Thus  2)  may  be  written 

~#T 

Moreover  A  converges  if 

an~ 

that  is,  if  v     cn      ^ 

lim  —  >Q, 

where  as  usual  0=  cl-\-  c2  +  •••  is  a  convergent  series. 
Hence  A  converges  if  Cn 

lim^>0.  (4 

But  now  the  set  of  numbers  pv  p2  •••  gives  rise  to  a  series 
P  =  p1  -f  p2  +  •••  which  must  be  either  convergent  or  divergent. 
Thus  3),  4)  show  that  in  either  case  1)  holds. 

108.  1.  Let  us  consider  now  still  more  briefly  criteria  of  the 
second  kind.  Here  the  fundamental  relations  are  3),  4)  of  105, 
which  may  be  written  : 

cn+l— cn  >  0  for  convergence;  (1 

dn+l— —  dn  <^0  for  divergence.  (2 


124  SERIES 

Or  in  less  general  form  : 

The  positive  term  series  A  converges  if 


___.  (3 

«»+i         / 
It  diverges  if 

(4 


Here  as  usual  0=^+%+  •••  is  a  convergent,  and  D=d1  +  d%-\  ---- 
a  divergent  series. 

2.  Although  we  have  already  given  one  demonstration  of 
Rummer's  theorem  we  wish  to  show  here  its  place  in  Pringsheim's 
general  theory,  and  also  to  exhibit  it  under  a  more  general  form. 
Let  us  replace  <?n,  cn+l  in  1)  by  their  values  given  in  101,  2. 
We  get 

Jfn     -  JEf          a         M-M 


_ 

an+1  Mn 


or  snce 


or  by  103,  2 


Mn+l  an+1  Mn 


where  Z>  =  a1-fc?2+  •••  is  any  divergent  positive  term  series. 
Since  any  set  of  positive  numbers  &x,  &2,  •••  gives  rise  to  a  series 
&!  +  &2  -f  •••  which  must  be  either  convergent  or  divergent,  we  see 
from  1)  that  5)  holds  when  we  replace  the  cTs  by  the  &'s.  We 
have  therefore: 

The  positive  term  series  A  converges  if  there  exists  a  set  of  positive 
numbers  &x,  &2  •••such  that 

kn+lf*—k*>0.  (<3 

It  diverges  if 


where  as  usual  6?j  +  d%  -f  •••  denotes  a  divergent  series. 


ARITHMETIC   OPERATIOXS   ON   SERIES  125 

Since  the  Fs  are  entirely  arbitrary  positive  numbers,  the  rela 
tion  6)  also  gives 

A  converges  if 


as  is  seen  by  writing 

*»  =  F 

K  n 

reducing,  and  then  dropping  the  accent. 

3.    From  Rummer's  theorem  we  may  at  once  deduce  a  set  of 
tests  of  increasing  power,  viz.  : 

The  positive  term  series  A  is  convergent  or  divergent  according  as 

M-M  a  M     -  M 


L    an+1      Mnl^Mn  ...  Zr^n 
is  >Q  or  is  <^  0. 

For  kl,  &2  ...  we  have  used  here  the  terms  of  the  divergent 
series  of  103,  3. 

Arithmetic  Operations  on  Series 
109.    1.    Since  an  infinite  series 

is  not  a  true  sum  but  the  limit  of  a  sum 

A=  lim  J.n, 

we  now  inquire  in  how  far  the  properties  of  polynomials  hold  for 
the  infinite  polynomial  1).  The  associative  property  is  expressed 
in  the  theorem  : 

Let  A  =  al  4-  a2  +  •  •  •  be  convergent.  Let  b^  =  a1  -j-  •  •  •  -f  am  , 
^)2  —  am1+i+  •"  +«/»,!-••  Then  the  series  £  =  bl  +  b2-}-  ••>  is  con 
vergent  and  A  =  B.  Moreover  the  number  of  terms  which  bn  em 
braces  may  increase  indefinitely  with  n. 

For  B  -A 

and  lim  A     =A        by  I,  103,  2. 


126  SERIES 

This  theorem  relates  to  grouping  the  terms  of  A  in  parentheses. 
The  following  relate  to  removing  them. 

2.  Let  B  =  b1  +  b2  +  •»  be  convergent  and  let  b1  =  al  +  •  •  •  +  am  , 
62  =  anh+l  +  •••  +  am^  ••-  If  1°  A  =  a1  +  a2  +  •••  is  convergent, 
A  =  B.  2°  Jf  *Ae  terms  an>0,  J.  i«  convergent.  3°  7f  ea^A 
mn  —  mn_i  <_p  a  constant,  and  an  =  0,  A  is  convergent. 

On  the  first  hypothesis  we  have  only  to  apply  1,  to  show 
A  —  B.  On  the  second  hypothesis 

e  >  0,         m,         Bn  <  e,         n>m. 
Then  5-^.<e,         *>»*„. 

On  the  third  hypothesis  we  may  set 

A,  =  Br+Vr+l 

where  b'r+1  denotes  a  part  of  the  a-terms  in  br+l.     Since  br+l  con 
tains  at  most  p  terms  of  A,  b'r+l  =  0. 

Hence  lim  ^1.  =  lira  J9r     ,     or     A  =  B. 

Example  1.   The  series 

JB=(l-l)  +  (l-l)  +  (l-l)+- 
is  convergent.     The  series  obtained  by  removing  the  parentheses 

4  =  1-1  +  1-1+  ... 
is  divergent. 

Example  2. 


As  ^  is  comparable  with  *?.  —  ,  it  is  convergent.     Hence  A  is 

""*  nz 

convergent  by  3°. 

110.    1.    Let  us  consider  now  the  commutative  property. 

Here    Riemann     has    established     the     following    remarkable 
theorem  : 


ARITHMETIC   OPERATIONS  OX   SERIES  127 

The  terms  of  a  simply  convergent  series  A  =  al  +  a2  -f-  •••  can  be 
arranged  to  form  a  series  S,  for  which  lim  Sn  is  any  prescribed 
number,  or  ±00. 

For  let  7?      i     ,   i 

B  =  ol  +  o2  +  ••• 

(7=  <?!  +  <?,,+  •«• 

be  the  series  formed  respectively  of  the  positive  and  negative 
terms  of  A,  the  relative  order  of  the  terms  in  A  being  preserved. 
To  fix  the  ideas  let  I  be  a  positive  number  ;  the  demonstration 
of  the  other  cases  is  similar.  Since  Bn  =  +00,  there  exists  an  m1 
such  that 

Bmi  >  I.  (1 

Let  ml  be  the  least  index  for  which  1)  is  true.  Since  Cn=  —  oo, 
there  exists  an  m^  such  that 

Bmi+C^<l.  (2 

Let  m2  be  the  least  index  for  which  2)  is  true.  Continuing, 
we  take  just  enough  terms,  say  m3  terms  of  B,  so  that 


Then  just  enough  terms,  say  m±  terms  of  (7,  so  that 

J^+0«+^*  +<&».»<  4 

etc.     In  this  way  we  form  the  series 


whose  sum  is  I.     For 

|  aa  |  <  e         s  >  <r  ; 

rn  =  ml  +  wa  +  •••  +™ 


A  =  al  +  a2  +  •  *  be  absolutely  convergent.  Let  the  terms 
of  A  be  arranged  in  a  different  order,  giving  the  series  B.  Then  B 
is  absolutely  convergent  and  A  =  B. 

For  we  may  take  m  so  large  that 

Am  <  e. 


128  SERIES 

We  may  now  take  n  so  large  that  An  —  Bn  contains  no  term 
whose  index  is  <_  m.  Thus  the  terms  of  An  —  Bn  taken  with 
positive  sign  are  a  part  of  ATO  and  hence 


An  —  Bn 


n  >  m. 


Thus  B  is  convergent  and  B  =  A. 

The  same  reasoning  shows  that  B  is  convergent,  hence  B  is 
absolutely  convergent. 

3.    If  A  =  tfj  -h  a2  -f  ••>  enjoys   the    commutative  property,  it   is 
absolutely  convergent. 

For  if  only  simply  convergent  we  could  arrange  its  terms  so  as 
to  have  any  desired  sum.     But  this  contradicts  the  hypothesis. 


Addition  and  Subtraction 

111.    Let   A  =  a1  +  a2  +  --      ,      B  =  bl  +  b2  4-  •••  be    convergent. 
The  series 


are  convergent  and  O=A±B. 

For  obviously  Cn  =  An  ±  Bn.     We  have  now  only  to  pass  to  the 
limit. 

Example.    We  saw,  81,  3,  Ex.  1,  that 

^=1-1  +  1-1  +  ... 

is  a  simply  convergent  series.     Grouping  its  terms  by  twos  and 
by  fours  [109,  l]  we  get 


^\2n  —  1      2nJ      —?\-±n  —  3      4n  —  2      4  n  —  1      4fi/ 

Let  us  now  rearrange  A,  taking  two  positive  terms  to  one  nega 
tive.     We  get 


ADDITION    AND  SUBTRACTION  129 

We  note  now  that 


n_a     4n-2     4n-l      4n/      --U  -  2 


n 


n  -  1      4  n  -  3      2 
=  B         by  109,  2. 
Thus  B  =  I  A. 

This  example,  due  to  Dirichlet,  illustrates  the  non-commutative 
property  of  simply  convergent  series.  We  have  shown  the  con 
vergence  of  B  by  actually  determining  its  sum.  As  an  exercise  let 
us  proceed  directly  as  follows  : 

The  series  1)  may  be  written : 

Sn-  3  ^1  ~n 


n 

Comparing  this  with 


we  see  that  it  is  convergent  by  87,  3.  Since  1)  is  convergent,  B 
is  also  by  109,  2. 

112.  1.  Multiplication.  We  have  already  seen,  80,  7,  that  we 
may  multiply  a  convergent  series  by  any  constant.  Let  us  now 
consider  the  multiplication  of  two  series.  As  customary  let 

2at^  i,  *  =  1,  2,  3,  -  (1 

IK 

denote  the  infinite  series  whose  terms  are  all  possible  products 
a,  •  bK  without  repetition.  Let  us  take  two  rectangular  axes  as  in 
analytic  geometry  ;  the  points  whose  coordinates  are  x  =  t,  y  =  K 
are  called  lattice  points.  Thus  to  each  term  aJbK  of  1),  cor- 


130  SERIES 

responds  a  lattice  point  t,  K  and  conversely.     The  reader  will  find 
it  a  great  help  here  and  later  to  keep  this  correspondence  in  mind. 

Let  A  =  «!  -f  #2  H  ----  •>   •&  —  ^i  +  ^2  +  '"   be  absolutely  convergent. 
Then  O  =  ^LaJ)K  is  absolutely  convergent  and  A  •  B  =  C. 

Let  m  be  taken  large  at  pleasure  ;   we  may  take  n  so  large  that 
Tn  —  Am  •  Bm  contains  no  term  both  of  whose  indices  are  <.  m. 

Then  —  —  — 

Tn  -  ATOBm  <  «1Bm  +  «2BOT  +  ..  .  +  «mBro 


AmBm 


<  e  for  m  sufficiently  large. 


Hence  limr 


and  C  is  absolutely  convergent. 

To  show  that  0=  A  -  B,  we  note  that 

\Cn-AmBm   <Tn-AmBm<€ 

2.    We  owe  the  following  theorem  to  Mertens. 

If  A  converges  absolutely  and  B  converges  (not  necessarily  abso 
lutely),  then 


0  =  a1b1 
is  convergent  and  0  =  A  •  B. 

We  set  C—  c1-\-  <?2  + 

where  cl  =  a1b1 


4- 


Adding  these  equations  gives 


ADDITION   AND   SUBTRACTION  131 

But 

Bm  =  B-Bm         w  =  l,  2,  -. 

Hence  _ 


where 


The  theorem  is  proved  when  we  show  dn  =  0.     To  this  end  let 
us  consider  the  two  sets  of  remainders 


sl  , 


=  n. 


Let  *  each  one  in  the  first  set  be  |  <    Mv  and  each  in  the  second 
set     <    M.     Then  since 


Now  for  each  e  >  0  there  exists  an  n^  such  that 

also  a  i/,  such  that 

Thus  1)  shows  that       ,   ,   , 

I  da  |  <  e. 

3.  When  neither  A  nor  B  converges  absolutely,  the  series  C 
may  not  even  converge.  The  following  example  due  to  Cauchy 
illustrates  this. 


VI      V2      V3      V4 

5  =  J=-^-_  +  A__JL+...=A 

VI      V2      V3      V4 
*The  symbols  |  <  |,  |  <  |  mean  numerically  <,  numerically  <. 


132  SERIES 

The   series  A  being   alternating  is  convergent   by  81,  3.     Its 
adjoint  is  divergent  by  81,  2,  since  here  /LI  =  1.     Now 


VI  VI     VV1V2     V2V1 

^J_J 

VVlVS     V2V2     VSV 
=  c2  +  c8  +  £4  +  - 

and 


Vw-1      VI 


By  I,  95, 
Hence 

2 
1          -^2           ,      ,      2O-1) 

Hence  (7  is  divergent  since  cn  does  not  =  0,  as  it  must  if  0 
were  convergent,  by  80,  3. 

4.  In  order  to  have  the  theorems  on  multiplication  together, 
we  state  here  one  which  we  shall  prove  later. 

If  all  three  series  A,  B,  0  are  convergent,  then  C  =  A  •  B. 

113.  We  have  seen,  109,  1,  that  we  may  group  the  terms  of  a 
convergent  series  A  =  a^  +  «2  4-  —  into  a  series  B  =  bl  +  52  +  ••• 
each  term  bn  containing  but  a  finite  number  of  terms  of  A.  It  is 
easy  to  arrange  the  terms  of  A  into  a  finite  or  even  an  infinite 
number  of  infinite  series,  B1  ',  B",  B1"  •••  For  example,  let 

B'  =  «j  +  ap+1 
B"  = 


Then  every  term  of  A  lies  in  one  of  these  p  series  B.  To  decom 
pose  A  into  an  infinite  number  of  series  we  may  proceed  thus : 
In  B'  put  all  terms  an  whose  index  n  is  a  prime  number  ;  in  B" 
put  all  terms  whose  index  n  is  the  product  of  two  primes  ;  in 


TWO-WAY   SERIES  133 

B(m)  all  terms  whose  index  is  the  product  of  m  primes.  We  ask 
now  what  is  the  relation  between  the  original  series  A  and  the 
series  B'  ,  B"  >~ 

If  A  =  a1  +  #2  -h  •••  is  absolutely  convergent,  we  may  break  it  up 
into  a  finite  or  infinite  number  of  series  Bf,  B",  Bfrf,  •  ••  Each  of 
these  series  converges  absolutely  and 


'" 


That  each  B(m}  converges  absolutely  was  shown  in  80,  6.  Let 
us  suppose  first  that  there  is  only  a  finite  number  of  these  series, 
say  p  of  them.  Then 

An  =  £'nt  +  JB£  +  -  4-  B$        n  =  n,  +  ...  4-  »,. 

As  n=oo,  each  nr  7i2-..=oo.  Hence  passing  to  the  limit 
n  =  oo  ,  the  above  relation  gives 


=      +        +  ... 
Suppose  now  there  are  an  infinite  number  of  series  B(m). 
Set  B  =  B'  +  £"  +  £'"  +  ... 


We  take  v  so  large  that  A  —  Bn,  n>v,  contains  no  term  an  of 
index  <  m,  and  m  so  large  that 

Am<e. 

Then 

I A  —  Bn  |  <  Am  <  €.     n  >  v. 

Two-way  Series 

114.  1.  Up  to  the  present  the  terms  of  our  infinite  series  have 
extended  to  infinity  only  one  way.  It  is,  however,  convenient 
sometimes  to  consider  series  which  extend  both  ways.  They  are 
of  the  type 

•••  a_3  +  a_2  +  a_!  H-  a0  +  a1  +  a2  +  «3  -f-  ... 

which  may  be  written 


or 


134  SERIES 

Such  series  we  called  two-way  series.     The  series  is  convergent 

if 

lim    Zan  (2 


is  finite.  If  the  limit  2)  does  not  exist,  A  is  divergent.  The  ex 
tension  of  the  other  terms  employed  in  one-way  series  to  the 
present  case  are  too  obvious  to  need  any  comment.  Sometimes 
n  =  0  is  excluded  in  1)  ;  the  fact  may  be  indicated  by  a  dash, 

thus  2'an. 

—  00 

2.    Let  m  be  an  integer ;  then  while  n  ranges  over 
o         o         1    0    1    ^    Q 

—  O,    —  4,    —  JL)    v,    1,    *j,    O 

v  =  n  +  m  will  range  over  the  same  set  with  the  difference  that  v 
will  be  m  units  ahead  or  behind  n  according  as  m  ^  0.  This 
shows  that 


Similarly,  So.  =  fa... 

fl=-GC  7J=-00 

3.    Examine  1.     @  =  |^x+an2 

—  ao 

4- 


This  series  is  fundamental  in  the  elliptic  functions, 
Example  2. 


.       ^        »     /     -^  -^x 

a;      ^  Va;  +  w      n/ 


The  sum  of  this  series  as  we  shall  see  is  TT  cot  TTX. 


TWO-WAY   SERIES  135 

115.  For  a  two  way  series  A  to  converge,  it  is  necessary  and 
sufficient  that  the  series  B  formed  with  the  terms  with  negative  indices 
and  the  series  C  formed  with  the  terms  with  non-negative  indices  be 
convergent.  If  A  is  convergent,  A  =  B  4-  C. 

It  is  necessary.     For  A  being  convergent, 

\A-Br-Cs\<e/'2     ,     \A-Br-  C8,  <e/2 
if  s,  s'  >  some  a-  and  r  >  some  p.     Hence  adding, 

\C,-C,    <e, 

which  shows  C  is  convergent.     Similarly  we  may  show  that  B  is 
convergent. 

It  is  sufficient.     For  B,  C  being  convergent, 

B-BT  <e/2    ,     \0-0.\<t/-2 
for  r,  s  >  some  p.      Hence 


r\  T» 


Thus  lim2a.=  B+C. 


Example  1.     The  series 


rr>  ^"^       \      >•       i_     vi  /vi 


x      ^  \x-\-  n      n> 


is  absolutely  convergent  if  x  ^  0,  ±1,  ±  2, 

For 

I  a.  I  = 


+  n      n 

Hence  *  ,     ~J 

2an     and     Zan 

o  -» 

are  comparable  with  V  — • 

7* 

Example  2.     The  series 

®(a;)  =  igna;+a"2          rr  arbitrary  (2 

is  convergent  absolutely  if  a  <  0.     It  diverges  if  a  >  0. 


136  SERIES 

Here 


n  >  0,         Van  =  e*ean  =  0  if  a  <  0 

==  QO          if  a  >  0  ; 
n  =  —  n',nr>0         n^/~an  =  e~xean'  =  0         ifa<0 

=  00          if  a  >  0. 
The  case  a  =  0  is  obvious. 

Thus  the  series  defines  a  one-valued  function  of  x  when  a  <  0. 
As  an  exercise  in  manipulation  let  us  prove  two  of  its  properties. 

1°   <H)(V)  is  an  even  function. 

For 

®(-20=2«-«*+"*.  (3 

-  00 

If  we  compare  this  series  with  2)  we  see  that  the  terms  corre 
sponding  to  n  =  m  and  n  =  —  m  have  simply  changed  places,  as  the 
reader  will  see  if  he  actually  writes  out  a  few  terms  of  2),  3). 
Of.  114,  2. 

2°    <8>O  +  2ma-)=  e-^x+ma^x).     m=±l,  ±2,  ... 
For  we  can  write  2)  in  the  form 

_x*      ^     (.r+2na)2 

e(aO=e  4a    2e     4a         •  (4 

n  =—  oo 
(#+2/na)2     ,.     (r+2(m+n)o)8 


g    4a     ^^      4a 

f=— 00 

which  with  4)  gives  3). 


•  CHAPTER   IV 
MULTIPLE   SERIES 

116.  Let  x  =  xr  •"  xm  be  a  point  in  ra-way  space  9?m.  If  the 
coordinates  of  x  are  all  integers  or  zero,  x  is  called  a  lattice  point, 
and  any  set  of  lattice  points  a  lattice  system.  If  no  coordinate  of 
any  point  in  a  lattice  system  is  negative,  we  call  it  a  non-negative 
lattice  system,  etc.  Let  f(x^  •••  z-m)  be  denned  over  a  lattice 
system  1  =  ^,...^.  The  set  {/(vOJ  is  called  an 
sequence.  It  is  customary  to  set 


Then  the  sequence  is  represented  by 


The  terms  Um  A     ,     IfS  A     ,     lim 


as  tj  •  •  •  im  converges  to  an  ideal  point  have  therefore  been  denned 
and  some  of  their  elementary  properties  given  in  the  discussion 
of  I,  314-328  ;  336-338. 

Let  x  =  x1  —  xn  y  =  yi-~ym  be  two  points  in  Wm.  If 
y\  >  x\  "•  Vm  >  xm  we  shall  write  more  shortly  y  >  x.  If  x 
ranges  over  a  set  of  points  x'  >  x"  >  x'"  •••  we  shall  say  that  x  is 
monotone  decreasing.  Similar  terms  apply  as  in  I,  211. 

Ifnow  /(*•••  y.)>/(*,~<0 

when  y  _>  a?,  we  say  f  is  a  monotone  increasing  function.     If 


we  say  f  is  a  monotone  decreasing  function. 

Similar  terms  apply  as  in  I,  211. 

137 


138  MULTIPLE   SERIES 

117.  A  very  important  class  of  multiple  sequences  is  connected 
with  multiple  series  as  we  now  show.  Let  «tl...tm  be  defined  over 
a  non-negative  lattice  system.  The  symbol 


or  2atl...lm     ,     or  AVl...;m 


denotes  the  sum  of  all  the  a's  whose  lattice  points  lie  in  the  rec 
tangular  cell          Q<XI<VI         -0<xm<vm. 

Let  us  denote  this  cell  by  RVl...vn  or  by  Rv.     The  sum  1)  may  be 
effected  in  a  variety  of  ways.     To  fix  the  ideas  let  m  =  3.     Then 


A,  „  „  = 


etc.  In  the  first  sum,  we  sum  up  the  terms  in  each  plane  and 
then  add  these  results.  In  the  second  sum,  we  sum  the  terms  on 
parallel  lines  and  then  add  the  results.  In  the  last  sum,  we  sum 
the  terms  on  the  parallel  lines  lying  in  a  given  plane  and  add  the 
results;  we  then  sum  over  the  different  planes. 
Returning  now  to  the  general  case,  the  symbol 

A  =  2all...tn         iv  •••  im=  0,  1,  •••  oo, 

00 

or  4  =  2^...^ 

o 

is  called  an  w-tuple  infinite  series.     For  m  =  2  we  can  write  it 
out  more  fully  thus 


^12+ 


In  general,  we  may  suppose  the  terms  of  any  m-tuple  series  dis 
played  in  a  similar  array,  the  term  atl...lw  occupying  the  lattice 
point  t  =  (i1-«-tm).  This  affords  a  geometric  image  of  great 
service.  The  terms  in  the  cell  Rv  may  be  denoted  by  Av. 

If  lim  AVl...Vm  =  lim  A,  (2 


GENERAL   THEORY  139 

is  finite,  A  is  convergent  and  the  limit  2)  is  called  the  sum  of  the 
series^..  When  no  confusion  will  arise,  we  may  denote  the  series 
and  its  sum  by  the  same  letter.  If  the  limit  2)  is  infinite  or  does 
not  exist,  we  say  A  is  divergent. 

Thus  every  w-tuple  series  gives  rise  to  an  ra-tuple  sequence 
{AVl...Vm\.  Obviously  if  all  the  terms  of  A  are  >  0  and  A  is  diver 
gent,  the  limit  2)  is  -f  oo.  In  this  case  we  say  A  is  infinite. 

Let  us  replace  certain  terms  of  A  by  zeros,  the  resulting  series 
may  be  called  the  deleted  series.  If  we  delete  A  by  replacing  all 
the  terms  of  the  cell  RVl...VM  by  zero,  the  resulting  series  is  called 
the  remainder  and  is  denoted  by  AVl...vm  or  by  Av.  Similarly  if 
the  cell  Rv  contains  the  cell  R^  the  terms  lying  in  Rv  and  not  in 
Rp  may  be  denoted  by  A^  „. 

The  series  obtained  from  A  by  replacing  each  term  of  A  by  its 
numerical  value  is  called  the  adjoint  series.  In  a  similar  manner 
most  of  the  terms  employed  for  simple  series  may  be  carried  over 
to  m-tuple  series.  In  the  series  2atl...llB  the  indices  t  all  began 
with  0.  There  is  no  necessity  for  this;  they  may  each  begin  with 
any  integer  at  pleasure. 


118.    The  Geometric  Series.     We  have  seen  that 
=  1  -f  a  +  a2  +  •••  a    <  1, 


1-  b 

Hence 


1 


for  all  points  a,  b  within  the  unit  square. 
In  general  we  see  that 


1  "2  *• 

is  absolutely  convergent  for  any  point  x  within  the  unit  cube 


and 


140  MULTIPLE   SERIES 

119.  1.    It  is  important  to  show  how  any  term  of  A  =  2atl...lm  can 
be  expressed  by  means  of  the  AVr..Vn. 

Let  Dl/il/2...%_i  =  AVlVt...Vm  —  Av^...Vm_^  (1 

Then  D^2. ..I/m_1_1  =  AVlVt... ,m  ^Vm  -  AVlVs...VM_^lt  ,m_r      (2 

Let  &w.'i'm-2  =  A^-^-i  -  ^w^-i-r  (3 

Similarly 


",-,-n 

(5 


Finally  ^  =  DViVf  -  !>„,„,_!,  (6 

and  «IV,...I/M  =  A't  —  DVl-i*  (7 

If  now  we  replace  ,the  D's  by  their  values  in  terms  of  the  As, 
the  relation  7)  shows  that  «„,...„„  may  be  expressed  linearly  in 
terms  of  a  number  of  AIJLl...IJim  where  each  pr  =  vr  or  vr  —  1.  •  . 

For  m  =  2  we  find 

aVlVa  =  AVtVf  +  ^-1,^-1  —  AVlt  V2_x  —  AVl_^Vf.  (8 

2.  From  1  it  follows  that  we  may  take  any  sequence  \Alt...ltlt\ 
to  form  a  multiple  series 

-^i  —  ^^ij  •••  im* 

This  fact  has  theoretic  importance  in  studying  the  peculiarities 
that  multiple  series  present. 

120.    We  have  now  the  following  theorems  analogous  to  80. 

1.  For  A  to  be  convergent  it  is  necessary  and  sufficient  that 

2.  If  A  is  convergent,  so  is  A^  and 

A  -A  \  —  1 1  tv»       1 

-/Xj^  —  ^1.  ^~  *^-*-/x   ~~"   ^•**1I   -*jLix    j/» 

Conversely  if  A^  is  convergent,  so  is  A. 


GENERAL   THEORY  141 

3.  For  A  to  converge  it  is  necessary  and  sufficient  that 

lim  Av  =  0. 

4.  A  series  ivhose  adjoint  converges  is  convergent. 

5.  Let  A  be  absolutely  convergent.     Any  deleted  series  B  of  A  is 
absolutely  convergent  and  \  B  \  <  A. 

6.  If  A  =  2ati...lm  is  convergent,  so  is  B  —  2&«ti...,,n  and 

B  =  kA,         k  a  constant. 

121.      1.    For  A  to  converge  it  is  necessary  that 

-A^...,.*,-!     ,     -Z>ri,2...,m_2     ,     —Dvi    ,    avil.2.  ..,,  =  (),  as  v  =  cc  . 
For  by  120,  l  A  , 

I    ylA,  •••  Am  ^fM-'Mm    |    V   c 

if  X1..-Aro,      /*!  .../*m  >jo. 
Thus  by  119,  1) 

Hence  passing  to  the  limit  p  =  00  , 

IrniA,...,  „_,<.*. 

As  e  is  small  at  pleasure,  this  shows  that  DVl...Vm_^  =  0.     In  this 
way  we  may  continue. 

2.    Although  ,.  n 

lim  av  ...  ,,m  =  0 

»i  •••  >'m=» 

when  A  converges,  we  must  guard  against  the  error  of  supposing 
that  av=  0  when  v  =  (yl  •••  vm)  converges  to  an  ideal  point,  all  of 
whose  coordinates  are  not  cc  as  they  are  in  the  limits  employed 
in  1. 

This  is  made  clear  by  the  following  example  due  to  Pringsheim. 


Then  by  119,  8)  I  ^,-1  +  1 

ar      as 


142  MULTIPLE   SERIES 

AS  lim  A-,.  =  0 

r,  5=» 

A  is  convergent.     But 

lim    aftS\  =—      ,     lim  |  ars  \  =-. 
r=x>  a  s=™  ar 

That   is  when   the  point  (r,  s)    converges  to   the   ideal   point 
(oo,  s),  or  to  the  ideal  point  (r,  GO  ),  ars  does  not  =  0. 

3.    However,  we  do  have  the  theorem  : 

Let  .      ~  ^  ~ 

A  =  2at  ...  l  at  >  0 


converge.      Then  for  each  e  >  0  ^m?  e:m£s  a  X  swcA  that  «tl...t    <  e 
/or  «?i?/  t  outside  the  rectangular  cell  R^. 


This  follows  at  once  from  120,  1,  since 

*£•*»*• 

122.      1.    Letf(x^  •••  xm)  be  monotone.      Then 

^  •••  xm)  =1         xl<  av  •••  xm  <  am,  a  may  be  ideal.     (1 


exists,  finite  or  infinite.  Iff  is  limited,  I  is  finite.  If  f  is  unlim 
ited,  I  =  4-  QO  when  f  is  monotone  increasing,  and  I  =  —  GO  whenf  is 
monotone  decreasing. 

For,  let/  be  limited.     Let  A  =  «:  <  <*2  <  •••  =  a. 

Then  T      />x    N      7 

l]m/(«n)  =  I 

n=cc 

is  finite  by  I,.  109. 

Let  now  B  =  ftv  /32,  •••  =  a  be  any  other  sequence. 

T  pf 

lim/G8n)  =  I         lim  f  (&)  =  f. 

~«~  ^  " 

Then   there   exists    by   I,   338  a   partial    sequence    of   B,    say 
O=j1,  72  •••  such  that 


also  a  partial  sequence  D—  S1,  S2  •••  such  that 

lim/(S,,)  =  I 


GENERAL   THEORY  143 

But  for  each  an  there  exists  a  yln  _>  an  ; 

/(7  J  >/(«») 

and  therefore  J  >  I-  (2 

Similarly,  for  each  dn  there  exists  an  a,a  >  Sn  ; 

hence  /(8.)  </(«,.) 

and  therefore  7  <  Z  (3 

Thus  2),  3)  give  lim/(~)'=/. 

.8 

Hence  by  I,  316,  2  the  relation  1)  holds. 

The  rest  of  the  theorem  follows  along  the  same  lines. 

2.    As  a  corollary  we  have 

The  positive  term  series  A  =  ^,ali,..ln  is  convergent  if  Av^tfl,m  is 
limited. 

123.  1.  Let  A=2all...ls  =  2at  ,  B  =  26tl...t-  =  2J4  be  tivo  non- 
negative  term  series.  If  they  differ  only  by  a  finite  number  of 
terms,  they  converge  or  diverge  simultaneously. 

This  follows  at  once  from  120,  2. 

2.  Let  A,  B  be  two  non-negative  term  series.     Let  r  >  0  denote 
a  constant.     If  aL  <  rbL  ,  A  converges  if  B  is  convergent  and  A  <  rB. 
If  a,  >  rbL,  A  diverges  if  B  is  divergent. 

For  on  the  first  hypothesis 

AK 

and  on  the  second  A 

A* 

3.  Let  A,  B  be  two  positive  term  series.       Let  r,  s  be  positive 
constants.     If 


r     fl| 
hm  —  l 

1=00  6t 

exists  and  is  =£  0,  A  and  B  converge  or  diverge  simultaneously.     If 
B  converges  and  —  =  0,  A  is  convergent.     If  B  diverges  and  -*  =  <», 

bn  bn 

A  is  divergent. 


144 


MULTIPLE   SERIES 


4.  The  infinite  non-negative  term  series 

2#t,...lg     and     2  log  (1 
converge  or  diverge  simultaneously. 
This  follows  from  2. 

5.  Let  the  potver  series 

P  —  S/>  rw7irm,   . 

;       —  ^^-'-- 


converge  at  the  point  a  =  («j,  •••  «a),  then  it  converges  absolutely  for 
all  points  x  within  the  rectangular  cell  R  whose  center  is  the  origin, 
and  one  of  whose  vertices  is  a;  that  is  for  \  x,  \  <  |  a,  ,  i=l,  2,  •••  a. 

For  since  P  converges  at  a, 

lim  cmim2...a™i  •••<'•  =  0. 

Thus  there  exists  an  J^such  that  each  term 
I  c       a7!*1  "•  am*  I  "^  ]\T 

|     TO!  •••  "~l  "»j      |    —  •<•'-' 

Hence 


,           nm\          nm* 

1 

mi 

xa 

m\  ...  ^J             **s 

«T 

" 

OH 

x.\ 

""... 

X. 

ma 

ai 

aa 

Thus  each  term  of  P  is  numerically  <  than  M  times  the  cor 
responding  term  in  the  convergent  geometric  series 


We  apply  now  2. 

We  shall  call  R  a  rectangular  cell  of  convergence. 

124.  1.  Associated  with  any  w-tuple  series  A  =  ^aL  ...,_  are 
an  infinite  number  of  simple  series  called  associate  simple  series, 
as  we  now  show. 

Let  7?  7?  7? 

be  an   infinite   sequence  of  rectangular  cells  each  lying  in  the 
following.     Let 


be  the  terms  of  ^1  arranged  in  any  order  lying  in 


Let 


GENERAL  THEORY  145 

be  the  terms  of  A  arranged  in  order  lying  in  R^—  R\^  and  so  on 

indefinitely. 

Then  SI  =  ^  4- «a  +  -  +  a.v  +  a.l+1  +  - 

is  an  associate  simple  series  of  A. 

2.  Conversely  associated  with  any  simple  series  51  =  2an  are  an 
infinity  of  associate  m-tuple  series.     In  fact  we  have  only  to  arrange 
the  terms  of  51  over  the  non-negative  lattice  points,  and  call  now 
the  term  an  which  lies  at  the  lattice  point  ^  •••  im  the  term  atl...lw. 

3.  Let  51  be  an  associate  series  of  A  =  2ah ...  l|B.     If  51  is  convergent, 
so  is  A  and  J.  =  51 

For  AVl...Vm  =  %n. 

Let  now  v  =  oo,  then  n  =  <x>.     But  5l7i  =  51,  hence  ^ ...  Vm  =  51. 

4.  If  the  associate  series  51  is  absolutely  convergent,  so  is  A. 
Follows  from  3. 

5  If  A  =  2ari ...  Vfn  is  a  non-negative  term  convergent  series,  all  its 
associate  series  51  converge. 

For,  any  51^^  lies  among  the  terms  of  some  A^v.     But  for  X 
sufficiently  large          A*9<*         \<n<v. 
Hence  ar 

*«•.*<«         m>mQ. 

6.  Absolutely  convergent  series  are  commutative. 

For  let  B  be  the  series  resulting  from  rearranging  the  given 
series  A. 

Then  any  associate  53  of  B  is  simply  a  rearrangement  of  an 
associate  series  51  of  A.  But  51  =  SB,  hence  A  =  B. 

7.  A    simply   convergent   m-tuple   series   A    can    be   rearranged, 
producing  a  divergent  series. 

For  let  51  be  an  associate  of  A.  51  is  not  absolutely  convergent, 
since  A  is  not.  We  can  therefore  rearrange  51,  producing  a  series 
53  which  is  divergent.  Thus  for  some  53 

lim  $„ 

does  not  exist.     Let  53'  be  the  series  formed  of  the  positive,  and 
53"  the  series  formed  of  the  negative,  terms  of  53  taken  in  order. 


146  MULTIPLE   SERIES 

Then  either  Wn  =  +  oo  or  ^  =  -00,  or  both.  To  fix  the  ideas 
suppose  the  former.  Then  we  can  arrange  the  terms  of  33  to 
form  a  series  (£  such  that  &n  =  -h  oo.  Let  now  (£  be  an  associate 
series  of  O.  Then 

t;  =  cv,...  ,„  =  <£„ 

and  thus 

Km  Cv  =  lim  (£„  =  +  oo. 

Hence  0  is  divergent. 

8.  If  the,  multiple  series  A  is  commutative,  it  is  absolutely  con 
vergent. 

For  if  simply  convergent,  we  can  rearrange  A  so  as  to  make  the 
resulting  series  divergent,  which  contradicts  the  hypothesis. 

9.  In   121,  2  we  exhibited  a  convergent  series  to  show  that 
«tl...lw  does  not  need  to  converge  to  0  if  ^  •••  im  converges  to  an  ideal 
point  some  of  whose  coordinates  are  finite.     As  a  counterpart  we 
have  the  following  : 

Let  A  be  absolutely  convergent.  Then  for  each  e  >  0  there  exists 
a  \,  such  that  any  finite  set  of  terms  B  lying  without  E^  satisfy  the 
relation 


and  conversely. 

For  let  51  be  an  associate  simple  series  of  Adj  A.     Since  51  is 
convergent  there  exists  an  n,  such  that 


But  if  X  is  taken  sufficiently  large,  each  term  of  B  lies  in  5ln, 
which  proves  1). 

Suppose  now  A  were  simply  convergent.  Then,  as  shown  in  7, 
there  exists  an  associate  series  £)  which  is  infinite. 

Hence,  however  large  n  is  taken,  there  exists  a  p  such  that 


Hence,  however  large  X  is  taken,  there  exist  terms  J?=  £)Wip  which 
do  not  satisfy  1). 

10.    We  have  seen  that  associated  with  any  m-tuple  series 


GENERAL   THEORY  147 

extended  over  a  lattice  system  2ft  in  9f?m  is  a  simple  series  in  9?r 
We  can  generalize  as  follows.  Let  2ft  =  \i\  be  associated  with  a 
lattice  system  2ft  =  \j\  in  ^Rn  such  that  to  each  i  corresponds  a,j  and 
conversely. 

If  i  ~y  we  set  «4i  ...  lm  =  a^  ...  jn  . 

Then  A  gives  rise  to  an  infinity  of  w-tuple  series  as 


We  say  B  is  a  conjugate  n-tuple  series. 
We  have  now  the  following  : 

Let  A  be  absolutely  convergent.  Then  the  series  B  is  absolutely 
convergent  and  A  =  B. 

For  let  A\  B'  be  associate  simple  series  of  A,  B.  Then  A',  B1 
are  absolutely  convergent  and  hence  A'=B'.  But  A  =  A\  B  =  B'. 
Hence  A  =  B,  and  B  is  absolutely  convergent. 

11.  Let  A  =  2atl...  tm  be  absolutely  convergent.  Let  B=  Sa^...^ 
be  any  p-tuple  series  formed  of  a  part  or  all  the  terms  of  A.  Then 
B  is  absolutely  convergent  and 

Ad   A. 


For  let  A',  B'  be  associate  simple  series  of  A  and  B.     Then  B' 
converges  absolutely  and  |  B'  \  <  Adj  A. 

125.    1.    Let  4  =  2«ll......  (1 

Set 

in  the  cell 

Then 

(2 


Let  72  denote  that  part  of  9?m  whose  points  have  non-negative 
coordinates.     Let  ^ 

J=\        fdX,:-dXm.  (3 

•X  ^2 

If  «7is  convergent,  A  =  J.     We  cannot  in  general  state  the  con 
verse,  for  A  is  obtained  from  Av  by  a  special  passage  to  the  limit,  viz. 


148  MULTIPLE   SERIES 

by   employing   a   sequence    of    rectangular   cells.      If,    however, 
av  >_  0  we  may,  and  we  have 

For  the  non-negative  term  series  1)  to  converge  it  is  necessary  and 
sufficient  that  the  integral  3)  converges. 

2.  Let  /(#!  •••  XM)  >  0  be  a  monotone  decreasing  function  of 
x  in  R,  the  aggregate  of  points  all  of  whose  coordinates  are  non- 
negative.  Let 


The  series  A  =  ^ 

is  convergent  or  divergent  with 

J» 
fdxl  "-  dxm. 
R 

For  let  R},  R2,  •••  be  a  sequence  of  rectangular  cubes  each  Rn 
contained  in  Rn+i. 

Let  RntS=Rt-Ra        s>n. 

Then  X,  ft  being  taken  at  pleasure  but  >  some  v,  there  exist  an 
Z,  m  such  that 


But  the  integral  on  the  right  can  be  made  small  at  pleasure  if  J 
is  convergent  on  taking  I  >  m  >  some  n.  Hence  A  is  convergent 
if  J"is.  Similarly  the  other  half  of  the  theorem  follows. 

Iterated  Summation  of  Multiple  Series 
126.    Consider  the  finite  sum 


One  way  to  effect  the  summation  is  to  keep  all  the  indices  but 
one  fixed,  say  all  but  tx,  obtaining  the  sum 


Then  taking  the  sum  of  these  sums  when  only  *2  is  allowed  to 
vary  obtaining  the  sum 

2     2ah...t  m 

ia=0  «j=0 


ITERATED   SUMMATION   OF   MULTIPLE   SERIES  149 

and  so  on  arriving  finally  at 

ml 

...^  (2 


whose  value  is  that  of  1).  We  call  this  process  iterated  summa 
tion.  We  could  have  taken  the  indices  ^  •••  im  in  any  order 
instead  of  the  one  just  employed  ;  in  each  case  we  would  have 
arrived  at  the  same  result,  due  to  the  commutative  property  of 
finite  sums. 

Let  us  see  how  this  applies  to  the  infinite  series, 

^i  =  2ati...,m,         ij  — tm=0,  1,  ...oo.  (3 

The  corresponding  process  of  iterated  summation  would  lead  us 
to  a  series  31=  2  2  •••  fa  (4 

_..  ll  *  *  "  lm  '  ^ 

which  is  an  m-tuple  iterated  series.     Now  by  definition 

"m  "m  •  1  "i 

31  =  lim     2       lim        2      •••     lim    2ati...(m  (5 

=   lim     lim    •••  lim  AVi...Vm^  (6 

while  A        ,.  /rj 

A=   lim    AVi...Vm.  (J 

Thus  A  is  defined  by  a  general  limit  while  31  is  defined  by  an 
iterated  limit.  These  two  limits  may  be  quite  different.  Again 
in  6)  we  have  passed  to  the  limit  in  a  certain  order.  Changing 
this  order  in  6)  would  give  us  another  iterated  series  of  the  type 
4)  with  a  sum  which  may  be  quite  different.  However  in  a  large 
class  of  series  the  summation  may  be  effected  by  iteration  and  this 
is  one  of  the  most  important  ways  to  evaluate  3). 

The  relation  between  iterated  summation  and  iterated  integra 
tion  will  at  once  occur  to  the  reader. 

127.  1.  Before  going  farther  let  us  note  some  peculiarities  of 
iterated  summation.  For  simplicity  let  us  restrict  ourselves  to 
double  series.  Obviously  similar  anomalies  will  occur  in  m-tuple 
series. 


150  MULTIPLE   SERIES 

^  =  «00  +  a01  +  S2+    -+«10+all  + 

be  a  double  series.     The  mih  row  forms  a  series 


and  the  wth  column,  the  series 


»i=0 


7M=0  MJ=O  »=0 

are  the  series  formed  by  summing  by  rows  and  columns,  respec 
tively. 

2.  A  double  series  may  converge  although  every  row  and  every 
column  is  divergent. 

This  is  illustrated  by  the  series  considered  in  121,  2.     For  A 

00  00 

is  convergent  while  2ar,,  2ar,  are  divergent,  since  their  terms  are 

r=0  s=Q 

not  evanescent. 

3.  A  double  series  A  may  be  divergent  although  the  series  R  ob 
tained  by  summing  A  by  rows  or  the  series  C  obtained  by  summing 
by  columns  is  convergent. 

For  let  Ars=0         if  r  or  s  =  0 

r  .» 

= if  r,  s>0. 

r  -f  s 

Obviously  by  I,  318,  lim  Ars  does  not  exist  and  A  =  2#ra  is  di 
vergent. 

On  the  other  hand, 

R  =  lim  lim  Ars  —  0, 


r=oo    5=3 


(7=  lim  lim  Ars  =  1. 


S=00        r=3 


Thus  both  R  and  (7  are  convergent. 


ITERATED   SUMMATION   OF   MULTIPLE   SERIES  151 

4.  In  the  last  example  R  and  C  converged  but  their  sums  were 
different.  We  now  show  : 

A  double  series  may  diverge  although  both  R  and  C  converge  and 
have  the  same  sum. 

For  let  Art,  =  0         if  r  or  s  =  0 


rs 


if  r,  «  >  0. 


Then  by  I,  319,  lim  A,,  does  not  exist  and  A  is  divergent.     On 
the  other  hand,  R  =  \{m  \{m  Ar,  =  0, 

(7=  lim  lim  Ara  =  0. 
Then  R  and  S  both  converge  and  have  the  same  sum. 

128.    We  consider  now  some  of  the  cases  in  which  iterated  sum 
mation  is  permissible. 

Let  A  =  2ati ...  ,w  be  convergent.     Let  i\,  i2,-~  i'm  be  any  permutation 
of  the  indices  ir  iv  •••  im.     If  all  the  m  -  l-tuple  series 


.'=0        t'  =0 


are  convergent,  A  = 

This  follows  at  once  from  I,  324.  For  simplicity  the  theorem 
is  there  stated  only  for  two  variables ;  but  obviously  the  demon 
stration  applies  to  any  number  of  variables. 

129.  1.  Let  f(x1-"Xm)  be  a  limited  monotone  function.  Let  the 
point  a=  (04  •••#,»)  be  finite  or  infinite.  When  f  is  limited,  all  the 
s-tuple  iterated  limits 


exist.      When  s  =  m,  these  limits  equal 

..-^).  (2 


In  these  limits  we  suppose  x<a. 


152  MULTIPLE   SERIES 

For  if /is  limited,        Hm/    >     ^^ 


exists  by  122,  l.     Moreover  3)  is  a  monotone  function  of  the  re 
maining  m  —  1  variables. 

Hence  similarly  ]im        Hm  f 

JTia_l=ais_l    xis=ctis 

exists  and  is  a  monotone  function  of  the  remaining  m  —  2  vari 
ables,  etc.     The  rest  of  the  theorem  follows  as  in  I,  321. 

2.  As  a  corollary  we  have 

Let  Abe  a  non-negative  term  m-tuple  series.  If  A  or  any  one  of 
its  m-tuple  iterated  series  is  convergent,  A  and  all  the  ml  iterated 
m-tuple  series  are  convergent  and  have  the  same  sum.  If  one  of  these 
series  is  divergent,  they  all  are. 

3.  Let  a  be  a  non-negative  term  m-tuple  series.     Let  s<m.      All 
the  s-tuple  iterated  series  of  A  are  convergent  if  A  is,  and  if  one  of 
these  iterated  series  is  divergent,  so  is  A. 

130.  1.  Let  A  =  2ati...tm  be  absolutely  convergent.  Then  all  its 
s-tuple  iterated  series  s  =  l,  2  •••  m,  converge  absolutely  and  its 
m-tuple  iterated  series  all  =  A. 

For  as  usual  let  «ti...lm=  atl...im\.  Since  A  =  Adj  A  is  con 
vergent,  all  the  s-tuple  iterated  series  of  A  are  convergent. 

OD  ao 

Thus  sl  =  2  fltl...im  is  convergent  since  2  atl.  .  (TO  =  tr1.     Moreover 
II=Q  l  4=0 

00  00 

I  sl  I  <  crr       Similarly     2     2«lf...lm  =  2st    is    convergent    since 

i,=0  4=0  i? 

OO  QO 

2  2«M...  ,w  =20-^8  convergent;  etc.     Thus  every  s-tuple  iter- 

'2=0   4=0  i2 

ated  series  of  ^4.  is  absolutely  convergent.     The  rest  follows  now 
by  128. 

2.  Let    A  =  2alt...,m.     /f  one    of  i^e  m-tuple  iterated  series   B 
formed  from  the  adjoint  A  of  A  is  convergent,  A  is  absolutely  con 
vergent. 

Follows  from  129,  2. 

3.  The  following  example  may  serve  to  guard  the  reader  against 
a  possible  error. 


ITERATED   SUMMATION   OF   MULTIPLE   SERIES  153 

Consider  the  series 


and  R  =  ea  +  e*a  +  e3a  -h 

This  is  a  geometric  series  and  converges  absolutely  for  a  <  0. 
Thus  one  of  the  double  iterated  series  of  A  is  absolutely  conver 
gent.  We  cannot,  however,  infer  from  this  that  A  is  convergent, 
for  the  theorem  of  2  requires  that  one  of  the  iterated  series  formed 
from  the  adjoint  of  A  should  converge.  Now  both  those  series 
are  divergent.  The  series  A  is  divergent,  for  |  arg  \  =  <x>  ,  as 
r,  s  =  oo  . 

131.    1.   Up  to  the  present  the  series 

2*.,.....  (1 

have  been  extended  only  over  non-negative  lattice  points.  This 
restriction  was  imposed  only  for  convenience  ;  we  show  now  how 
it  may  be  removed.  Consider  the  signs  of  the  coordinates  of  a 
point  x=  (xv  •••  xm).  Since  each  coordinate  can  have  two  signs, 
there  are  2m  combinations  of  signs.  The  set  of  points  x  whose 
coordinates  belong  to  a  given  one  of  these  combinations  form  a 
quadrant  for  m  =  2,  an  octant  for  m  =  3,  and  a  2m-tant  or  polyant 
in  9?m.  The  polyant  consisting  of  the  points  all  of  whose  coordi 
nates  are  >  0  may  be  called  the  first  or  principal  polyant. 

Let  us  suppose  now  that  the  indices  i  in  1)  run  over  one  or  more 
polyants.  Let  R^  be  a  rectangular  cell,  the  coordinates  of  each  of 
its  vertices  being  each  numerically  <  \.  Let  A^  denote  the  terms 
of  A  lying  in  72A.  Then  I  is  the  limit  of  A^  for  X  =  oo,  if  for  each 
e  >  0  there  exists  a  \0  such  that 

\A,-A,n\<e        X>\0.  (2 


154  MULTIPLE   SERIES 

If  lim  At  (3 


A=ao 


exists,  we  say  A  is  convergent,  otherwise  A  is  divergent.  In  a 
similar  manner  the  other  terms  employed  in  multiple  series  may 
be  extended  to  the  present  case.  The  rectangular  cell  72Ao  which 
figures  in  the  above  definition  may  without  loss  of  generality  be 
replaced  by  the  cube 


Moreover  the  condition  necessary  and  sufficient  for  the  exist 
ence  of  the  limit  3)  is  that 

|  A  -  4*  I  <  e        X,  p  >  X0. 

132.  The  properties  of  series  lying  in  the  principal  polyant 
may  be  readily  extended  to  series  lying  in  several  polyants.  For 
the  convenience  of  the  reader  we  bring  the  following  together, 
omitting  the  proof  when  it  follows  along  the  same  lines  as  before. 

1.  For  A  to  converge  it  is  necessary  and  sufficient  that 

lim  AI  =  0. 

A=oo 

2.  A  series  whose  adjoint  converges  is  convergent. 

3.  Any  deleted  series  B  of  an  absolutely  convergent  series  A  is 
absolutely  convergent  and 

\B\<  Adj  A. 

4.  If  A  =  Sdtij  ...  ,n  is  convergent,  so  is  B  =  2&#(J  ...,M  and  A  =  kB. 

5.  The  non-negative  term  series  A  is  convergent  if  A^  is  limited, 
X  =  oo. 

6.  If  the  associate  simple  series  51  of  an  m-tuple  series  A  converges, 
A  is  convergent.     Moreover  if  21  is  absolutely  convergent,  so  is  A. 
Finally  if  A  converges  absolutely,  so  does  21. 

7.  Absolutely  convergent  series  are  commutative  and  conversely. 

8.  Let  f(x1  •••a;m)>.0  be  a  monotone  decreasing  function  of  the 
distance  of  x  from  the  origin. 

Let  ~ 


ITERATED   SUMMATION   OF  MULTIPLE   SERIES  155 

Then  A  =  Zat. 

1         m 

converges  or  diverges  ivith 


the  integration  extended  over  all  space  containing  terms  of  A. 

133.  1.  Let  B,  (7,  D  •••  denote  the  series  formed  of  the  terms  of  A 
lying  in  the  different  poly  ants.  For  A  to  converge  it  is  sufficient 
although  not  necessary  that  B,  C,  •••  converge.  When  they  do, 


For  if  i?A,  <7A  •••  denote  the  terms  of  B,  C  •••  which  lie  in  a 
rectangular  cell  72A, 

AI  =  BL+CI  +  - 

Passing  to  the  limit  we  get  1). 

That  A  may  converge  when  B,  (?,  •••  do  not  is  shown  by  the 
following  example.  Let  all  the  terms  of  A  =  2atl...tm  vanish  ex 
cept  those  lying  next  to  the  coordinate  axes.  Let  these  have  the 
value  +1  if  ir  L2-~  im>0  and  let  two  #'s  lying  on  opposite  sides 
of  the  coordinate  planes  have  the  same  numerical  value  but  opposite 
signs.  Obviously,  Ax  =  0,  hence  A  is  convergent.  On  the  other 
hand,  every  B,  C  •••  is  divergent. 

2.  Thus  when  B,  C  •••  converge,  the  study  of  the  given  series 
A  may  be  referred  to  series  whose  terms  lie  in  a  single  polyant. 
But  obviously  the  theory  of  such  series  is  identical  with  that  of 
the  series  lying  in  the  first  polyant. 

3.  The  preceding  property  enables  us  at  once  to  extend  the 
theorems  of  129,  130  to  series  lying  in  more  than  one  polyant. 
The  iterated  series  will  now  be  made  up,  in  general  of  two-way 
simple  series. 


CHAPTER   V 
SERIES  OF  FUNCTIONS 

134.  1.  Let  i  —  (tr  i2  •••  ip)  run  over  an  infinite  lattice  system  &. 
Let  the  one-valued  functions 

/.,...  .POi  •••*»)  =  /<»=/. 

be  denned  over  a  domain  51,  finite  or  infinite.     If  the  jt?-tuple  series 
F=F(x)=F(xi  »•  aw)  =2/., ...„(*!  •»*»,)  (1 

extended  over  the  lattice  system  %  is  convergent,  it  defines  a  one- 
valued  function  F(x1  •  •  •  #m)  over  51.  We  propose  to  study  the 
properties  of  this  function  with  reference  to  continuity,  differen 
tiation  and  integration. 

2.  Here,  as  in  so  many  parts  of  the  theory  of  functions  depend 
ing  on  changing  the  order  of  an  iterated  limit,  uniform  convergence 
is  fundamental. 

We  shall  therefore  take  this  opportunity  to  develop  some  of  its 
properties  in  an  entirely  general  mariner  so  that  they  will  apply 
not  only  to  infinite  series,  but  to  infinite  products,  multiple  inte 
grals,  etc. 

3.  In  accordance  with  the  definition  of  I,  325  we  say  the  series 
1)  is  uniformly  convergent  in  51  when  F^  converges  uniformly  to  its 
Kmit  F.     Or  in  other  words  when  for  each  e>0  there  exists  a  X 
such  that  |J--j;|<«         M>X, 

for  any  x  in  51.  Here,  as  in  117,  F^  denotes  the  terms  of  1)  lying 
in  the  rectangular  cell  72M,  etc. 

As  an  immediate  consequence  of  this  definition  we  have  : 

Let  1)  converge  in  51.  For  it  to  converge  uniformly  in  51  it  is 
necessary  and  sufficient  that  \  F^  is  uniformly  evanescent  in  51,  or  in 
other  words  that  for  each  e  >  0,  there  exists  a  \  such  that  F^  >  e  for 
x  in  51,  and  /JL>\. 

166 


GENERAL   THEORY  157 

135.    1.    Let 


in  51.  Here  51,  T  may  be  finite  or  infinite.  If  there  exists  an 
77  >0  such  that  f  =  (f>  uniformly  in  ^(V),  a  finite  or  infinite,  we 
shall  say  f  converges  uniformly  at  a  ;  if  there  exists  no  77  <  0.  \ve 
say  /  does  not  converge  uniformly  at  a. 

2.  Let  now  a  range  over  51.     Let  53  denote  the  points  of  51  at 
which  no  ??  exists  or  those  points,   they  may  lie  in  51  or  not,  in 
whose  vicinity  the  minimum  of  77  is  0.     Let  D  denote  a  cubical 
division  of  space  of  norm  d.     Let  $8D  denote  as  usual  the  cells  of 
D  containing  points  of  53.     Let  &D  denote  the  points  of  51  not  in 
53^.     Then/=<£  uniformly  in  &D  however  small  d  is  taken,  but 
then  fixed.     The  converse  is  obviously  true. 

3.  Iff  converges  uniformly  in  51,  and  if  moreover  it  converges  at  a 
finite  number  of  other  points  -03,  it  converges  uniformly  in  51  +  53. 

For  if  /  =  (f>  uniformly  in  51, 

f-<f>\<e         x  in  51,          t  in  F5o*(r). 
Then  also  at  each  point  b,  of  53, 

\f  -4>\<  e          x=bt          <inFif*(T). 

If  now  8  <  S0,  8V  S2  •••  these  relations  hold  for  any  x  in  51  +  53 
and  any  t  in  Vs*(r). 

4.  Let  /(#!  •••  xm,  fj  •••  tn)  =  $  (xl  •••  xm^  uniformly  in  51.     Let 
f  be  limited  in  51  for  each  t  in  F6*(r).      Then  <f>  is  limited  in  51- 

For  </>=/(*,  0  +€'          |«'|<«  C1 

for  any  x  in  51  and  t  in  F5*(r).  Let  us  therefore  fix  t.  The 
relation  1)  shows  that  (f>  is  limited  in  51. 

5.  If  2  \f^  ...  i  (tfj  •••  #m)  |  converges  uniformly  in  51,  so  c?oes  2/ti  ...t  . 
For  any  remainder  of  a  series  is  numerically  <  than  the  corre 

sponding  remainder  of  the  adjoint  series. 

6.  Let  the  s-tuple  series 


158  SERIES  OF   FUNCTIONS 

converge  uniformly  in  51.     Then  for  each  e  >  0  there  exists  a  X 
such  that  ,  _. 

\^\<e  (1 

for  any  Rv  >  R^  >  R^.     When  s  =  1,  these  rectangular  cells  re 
duce  to  intervals,  and  thus  we  have  in  particular 

I  /«Oi  —  aw)  |  <  e         for  any  n  >  n'. 
When  s  >  1  we  cannot  infer  from  1)  that 

\f^t.^i-xm)\<€     ,     in  51,  (2 

for  any  i  lying  outside  the  above  mentioned  cell  Rk. 

A  similar  difference  between  simple  and  multiple  series  was 
mentioned  in  121,  2. 

However  if  fL  >  0  in  51,  the  relation  does  hold.     Cf.  121,  3. 

136.      1.    Let  f(xv~xm^  t1"-  tn)  be  defined  for  each  x  in  51,  and  t 


T  finite  or  infinite.     The  convergence  is  uniform  if  for  any  x  in  51 

I/  -  <t>  I  <  V<*i  •  •  •  O          tin  Vt*  (r),  B  fixed 
while  Km  -fy  =  0. 

t=T 

For  taking  e>0    at    pleasure  there  exists  an   ?;>0  such  that 

|VI<*     »     ^in  ^,*(T). 
But  then  if  S  <  T/, 

l/-*l<« 
for  any  ^  in  V&*(r)  and  any  2:  in  51. 

Example. 

sin  a;  sin          n  .     Qr       .„       N 

°  =  *'         m  51  =  (0,  oo). 


Is  the  convergence  uniform  ? 
Let 

y 

then  u  =  0,  as  ^  =    - 


GENERAL   THEORY  159 

Then         f_  A  |  _  |  sin  x  cos  u  \  _  \  sin  x  cos  u  sin2  u  \ 
I  +  x  cot2  u  I         sin2  u  +  x  cos2  w  | 

^    sin  x  sin2  w  I  ^  ,     0      .   A 
< <  tan2  u  =  0. 

Hence  the  convergence  is  uniform  in  51- 
2.    As  a  corollary  we  have 

Weierstrass"1    Test.     For   each  point   in   51,   let   l/^... tp|  ^Mtl...lp 
The  series  ^/^...^(^  •••#„,)  is  uniformly  convergent  in  51  if  ^Mtl...ip 
is  convergent. 

Example  1. 
Here 


and  _F  is  uniformly  convergent  in  51  since 

2- 

—    on 

is  convergent. 

Example  2. 

F(x)  =  ^an  sin  An 

is  uniformly  convergent  for  (  —  00,  QO)  if 

Z.|o.| 

is  convergent. 


137.  1.  7%e  power  series  P  =  2amt...mpa;jli  •••  x™v  converges 
uniformly  in  any  rectangle  R  lying  within  its  rectangle  of  con 
vergence. 

For  let  b  =  (6r  •••  6P)  be  that  vertex  of  R  lying  in  the  principal 
polyant.  Then  P  is  absolutely  convergent  at  6,  i.e. 


is  convergent.     Let  now  x  be  any  point  of  R.     Then  each  term  in 

2<V...,nP  £?-&" 

is  <  than  the  corresponding  term  in  1). 


160  SERIES  OF   FUNCTIONS 

2.  If  the  power  series  P  —  aQ  +  a^x  +  a2x2  +  •••  converges  at  an 
end  point  of  its  interval  of  convergence,  it  converges  uniformly  at 
this  point. 

Suppose  P  converges  at  the  end  point  x  =  R  >  0.     Then 


however  large  n  is  taken.     But  for  0  <  x  <  R 


<  e         by  Abel's  identity,  83,  i. 

Thus  the  convergence  is  uniform  at  x  —  R.  In  a  similar 
manner  we  may  treat  x  =  —  R. 

3.  Let/n^j  •••  xm),  n  =  1,  2  •••  be  denned  over  a  set  5L     If  each 
\fn   <  some  constant  cn  in  21,  fn  is  limited  in  51.     If  moreover  the 
cn  are  all   <  some  constant   0,  we   say  the  fn(x)   are  uniformly 
limited  in  51.     In  general  if  each  function  in  a  set  of  functions 
\f\  denned  over  at  point  set  51  satisfy  the  relation 

\f  \  <  a  fixed  constant  0,  x  in  51, 
we  say  the  jf's  are  uniformly  limited  in  51. 

The  series  F=  ^gnhn  is  uniformly  convergent  in  51,  if  G  =ffi  -h  </2  -f-  •  • • 
is  uniformly  convergent  in  51,  while  2 1  ha+1  —  hn  \  and  hn  \  are 
uniformly  limited  in  51. 

This  follows  at  once  from  Abel's  identity  as  in  83,  2. 

4.  The  series  F=2gnhn  is  uniformly  convergent  in  51,  if  in  51, 
2  |  h,l+l  —  hn  |   is  uniformly  convergent,  hn  is  uniformly  evanescent, 
and  the  Grn  uniformly  limited. 

Follows  from  Abel's  identity,  83,  l. 

5.  The    series    F=  ^gnhn    is    uniformly    convergent    in    51    if 
Gr  =  gl  -f- g%  +  ••  •  is  uniformly  convergent  in  51  while  hv  h2  •••  are 
uniformly  limited  in  51  and  \hn\   is  a  monotone  sequence  for  each 
point  of  51. 

For  by  83,  l,  ,  ^      ,     ,  ^    ,  n       . 

**         <J**     &n< 


(JEXERAL   THEORY  101 

6.  The  series  F  =  ^gnhn  is  uniformly  convergent  in  51  if  Gl  =  gv 
6r2  =  gl  +  <72,  ~-  are  uniformly  limited  in  51  and  if  hr  A2,  •••  not  only 
form  a  monotone  decreasing  sequence  for  x  in  51  but  also  are  uni 
formly  evanescent. 

For  by  83,1,  |  J^,  |  <  |  ^     G.  . 

Example.  Let  A  =  al  +  a2  -f-  •••  be  convergent.  Let  5r  62  •-•  ^  0 
be  a  limited  monotone  sequence.  Then 


converges  uniformly  in  any  interval  51  which  does  not  contain  a 
point  of    |  —  [  • 

For  obviously  the  numbers 


form  a  monotone  sequence  at  each  point  of  51.     We  now  apply  5. 

7.  As  an  application  of  these  theorems  we  have,  using  the  re 
sults  of  84, 

The  series  0 

fl0  -f  «!  cos  x  +  a2  cos  2  x  + 

converges  uniformly  in  any  complete  interval  not  containing  one  of 
the  points  ±  2  mir  provided  2  an+l  —  an  is  convergent  and  an  =  0, 
and  hence  in  particular  if  a^^  #2  _>  •••  =  0. 

8.  The  series  ^ 

«0  —  a1  cos  x  +  a  2  cos  2  #  — 

converges  uniformly  in  any  complete  interval  not  containing  one  of 
the  points  ±  (2  m  —  I)TT  provided  2  |  an+1  +  an  is  convergent  and 
an  =  0,  and  hence  in  particular  if  al  >  a%  >  •  •  •  =  0. 

9.  The  series  .  .     0  .    0 

al  sin  x  +  «2  sin  is  2T  4-  ^3  sin  00:+  ••• 

converges  uniformly  in  any  complete  interval  not  containing  one  of 
the  points  ±  2  mir  provided  2  |  an+l  —  an  \  is  convergent  and  an  =  0, 
and  hence  in  particular  if  a±  >^  «2  21  •••  =  0. 


162  SERIES  OF  FUNCTIONS 

10.    The  series    ^  sill  ^  _  ^  2  *  +  ^sin  3*  -  ... 

converges  uniformly  in  any  complete  interval  not  containing  one  of 
the  points  ±(2w  —  I)TT  provided  £  |  an+l  +  an  is  convergent  and 
an  =  0,  and  hence  in  particular  if  a1^a2  >_  •••  =0. 

138.     1.    Let  F=^...^Xl...Xm) 

be  uniformly  convergent  in  51.     Let  A,  B  be  two  constants  and 

4«*)<^<X><^/.<X>         m  «• 
Then  (?  =  2^..,.(^...^) 

is  uniformly  convergent  in  51. 

For  then  j  T-T      ^  ^      ^ 

AJb  A,  M  <  CrA?  M  < 

But  ^  being  uniformly  convergent, 


2.  =l,...l8^ 

converge  uniformly  in  51.      Then 


is  uniformly  convergent  in  31.     Moreover  if  F  is  limited  in  51,  so 
is  L. 

For  /t  >  0  in  51,  hence 

l/i|<« 

for  any  i  outside  some  rectangular  cell  M\. 
Thus  for  such  i 

Af<  <  log  (1  +/)  <  £/         in  «. 

139.     1.    Preserving  the  notation  of  136,  let  g1,  #2,  •••  ^m  fo  chosen 
such  that  if  we  set 


formly  in  51, 

lim  A  =  lim  ...        *   M.       -          •-  ^nS  =  0. 


GENERAL   THEORY  163 

For  if  /=  <f>  uniformly  in  31, 

e>0,         S>0         |/_<£|<€ 

for  any  x  in  51  and  any  t  in  FS*(T),  8  independent  of  x. 
But  then  |  A  |  <  e         tin  Fi*(r). 

2.    As  a  corollary  we  have  : 

Let  «j,  #2,  ...  =  a.     Ze£  ^=  l/a  fo  uniformly  convergent  at  a. 

Then  .         JU<o=o. 

140.    Example  1. 

lim/=lim_8muBin2tL       ,(          [2  for*=0, 
«=o          «=o  sin2  -M  +  #  cos2  M  [  0  for  x  ^=  0. 

The  convergence  is  not  uniform  at  2;  =  0.     For 

/._      2cosw 

1  +  ^  cot2  w 
Hence  if  we  set  x  =  u2 

lim/=  1,         since  u2  cot2  u=  1. 

w  =  0 

Thus  on  this  assumption 


Example  2.     F=  l-x  +  x(l-x^  +  X2(l  _  x)+  ^(1  -  a:)  +  ••• 

Here  _      » 

^=1(1-^)  -2:". 

o 

Hence  F  is  uniformly  convergent  in  any  (—  r,  r),  0  <  r  <  1,  by 
136,  2. 

We  can  see  this  directly.     For 


Hence  F  is  convergent  for    —  1<#<1,   and    then   .F(V)=1, 
except  at  x  =  1  where  F  =  0. 

Thus  |  Fn  (x)  |  =  |  x  |n,  except  at  x  =  1. 
But  we  can  choose  m  so  large  that  rm<e. 
Then  |  ^,(2:)  |  <  e  for  any  x  in  (—  r,  r). 


164  SERIES  OF   FUNCTIONS 

We  show  now  that  F  does  not  converge  uniformly  at  x=\ 
For  let 


n 
Then 


and  F  does  not  converge  uniformly  at  x  —  1,  by  139,  2. 
Example  3.  «  2 


Here  -^  -^ 

^B  =  l  +  na;2~l+0i  + 
and  F  is  telescopic.     Hence 


x, 


=  0     ,     a;  =  0. 
Thus  -, 


Let  us  take 


Then 


and  JP  is  not  uniformly  convergent  at  x  =  0.  It  is,  however,  in 
(—00,  co  )  except  at  this  point.  For  let  us  take  x  at  pleasure 
such,  however,  that  |  x  \  >  &.  Then 


We  now  apply  136,  1. 
Example  4. 


GENERAL   THEORY  165 

Here 


.    -,  T 

=x    __  *_  n  +  1 

11  +  7iV        1  +(7i+  I)2*2  J 


and  F  is  telescopic.     Hence 

F  _      x          O 


1  +(W  +  1)2^2 

in  51  =  (-R, 


if 


1  + 
The  convergence  is  not  uniform  at  x  =  0. 

For  set  an  =  —  —  -.     Then 

71+1 

I  ^»(O  I  =  I,  does  not  =  0. 
It  is,  however,  uniformly  convergent  in  51  except  at  0.     For 


(*  +  l 


(n 


=-1  +  (W  +  1)2£2 

<  e         for  7i  >  some  m. 

141.  Let  us  suppose  that  the  series  F  converges  absolutely  and 
uniformly  in  51.  Let  us  rearrange  F,  obtaining  the  series  6r. 
Since  F  is  absolutely  convergent,  so  is  6r  and  F  =  (7.  We  can 
not,  however,  state  that  6r  is  uniformly  convergent  in  51,  as  Bocher 
has  shown. 


Example. 


jl-  1  +x-  x 

Here 


Hence  F  is  uniformly  convergent  in  31  =  (0,  1). 
Let  . 


Then 


166  SERIES   OF   FUNCTIONS 

Let  1 

n 
Then 


as  n  ==i  oo. 


-Yi-1^ 

A        ~e) 
Hence  Gr  does  not  converge  uniformly  at  x  =  1. 

142.  1.    Let  /==<#>  uniformly  in  a  finite   set   of  aggregates   5lx, 
512'  '"  ^P-      Then  f  converges  uniformly  in  their  union  (5Ij,  •••  5lp). 
For  by  definition 

€  >  0,  Bs  >  0,  |/  -  <f>  I  <  6         a:  in  5I8,          «  in  F5a*(r).        (1 

Since  there  are  only  p  aggregates,  the  minimum  B  of  S^  •••  8p 
is  >  0.     Then  1)  holds  if  we  replace  88  by  S. 

2.    The  preceding  theorem  may  not  be  true  when  the  number 
of  aggregates  5fx,  512  •••  is  infinite.     For  consider  as  an  example 

F=  2(1- sX, 
which  converges  uniformly  in  51  =  (0,  1)  except  at  x  =  1.     Let 

-19. 


s        s  + 

Then  .F  is  uniformly  convergent  in  each  5la»  but  is  not  in  their 
union,  which  is  5l- 

3.    Letf=  </>,  g  =  >/r  uniformly  in  51. 

TAew  /±  #  ==  <#>  ±  ^         uniformly. 

If  ^>,  ^  remain  limited  in  51, 

fg  =  (^^      uniformly.  (1 

Jf  moreover  \  ^r  \  >  some  positive  number  in  51, 

•£  =  2.      uniformly.  (2 

The  demonstration  follows  along  the  lines  of  I,  49,  50,  51. 


GENERAL   THEORY  167 

4.    To  show  that  1),  2)  may  be  false  if  <£,  ty  are  not  limited. 
Let  - 


/»jap*+*1         2l  =  (0*,  1),          r  =  0. 

QC> 

Then  <£  =  -^  =  -  and  the  convergence  is  uniform. 
x 

But  9  . 


Let    x  =  t.       Then    A  =  2    as    t  =  0,    and   fg  does    not 
uniformly. 

Again,  let  -^ 

the  rest  being  as  before. 
Then 


But  setting  x  =  £, 


Al  = 


=  —  oo  as  t  ==  0 


9 

and  •-  does  not  converge  uniformly  to  -£•  • 
^  t 

143.    1.    As  an  extension  of  I,  317,  2  we  have  : 
Let 


uniformly  in  51. 

lim^C^  •••  tn)  =  ij 

t=T 

Let  y  ^  rj  in  F*(T).      Then 


t=T 


=  ^(^  •••  «m),  uniformly. 


The  demonstration  is  entirely  analogous  to  that  of  I,  292. 


uniformly  in  51.     ie^  ^Ae  points 

v=  (vv  vv  —  vp) 


168  SERIES  OF   FUNCTIONS 

form  a  limited  set  33.     Let  F^  ««•  up)  be  continuous  in  a  complete 
set  containing  33.      Then 


Mj  ...  up)  =  F(v^^  Vp) 
uniformly  in  51. 

For  F,  being  continuous  in  the  complete  set  containing  33,  is 
uniformly  continuous.  Hence  for  a  given  e  >  0  there  exists  a 
fixed  a-  >  0,  such  that 

|  F(u)  -  F(v)    <e        u  in  V9(v)     ,     v  in  2$. 
But  as  wt  =  t\  uniformly  there  exists  a  fixed  8  >  0  such  that 
K  -  vt  |  <  €'     ,     x  in  51     ,     t  in 


Thus  if  e'  is  sufficiently  small,  w=(wj,  —  MP)    lies   in 
when  x  is  in  51  and  t  in  Fi*(r). 

144.    1.    Let 

t-r 

uniformly  in  51.      5T.  v       , 

lim  e7  = 

t  =  T 

uniformly  in  51,  if  (j>  is  limited. 
This  is  a  corollary  of  143,  2. 

-.    Let 


uniformly  in  51.     X^^  </>  6g  greater  than  some  positive  constant  in  51- 

TOert  ..     |       -     , 

lim  log/  =  log  <p, 

/=T 

uniformly  in  51,  if  c/>  remains  limited  in  51. 
Also  a  corollary  of  143,  2. 

3.    Let  f  =  c£  awe?  g  =  ^  uniformly,  as  t  ==  T. 

ig^  </>,  i/r  5g  limited  in  5t,  an(i  (/>  >  some  positive  number.      Then 

fa  =  ^         uniformly  in  51.  (1 

For 


GENERAL   THEORY  169 

But    by    2),    log/=log$   uniformly    in    21;    and    by    142,  3 
g  log/  =  T/T  log  <£,  uniformly  in  21.     Hence  2)  gives  1)  by  1. 

145.    1.    The  definition  of  uniform  convergence  may  be  given  a 
slightly  different  form  which  is  sometimes  useful.     The  function 


is  a  function  of  two  sets  of  variables  x  and  t,  one  ranging  in  an  9?m 
the  other  in  an  9?n. 

Let  us  set  now  w  =  (x^  —  xm,  ^  —  £n)  and  consider  w  as  a  point  in 
m  -f  p  way  space. 

As  x  ranges  over  21  and  t  over  FS*(T)>  let  w  range  over  $&&. 

Then 


t=T 

uniformly  in  21  when  and  only  when 

e>0,     S>0          |/-<£    <e         winSBa,     8  fixed. 

By  means  of  this  second  definition  we  obtain  at  once  the  follow 
ing  theorem: 

2.  Instead  of  the  variables  xl  —  xm,  fj  —  tn  let  us  introduce  the 
variables  y^  •••  ym,  u±  •••  un  so  that  as  w  ranges  over  58s, 

z  =  (y1~-ym,u1...un) 

ranges  over  (Es,  the  correspondence    between  33s,  (5s  being  uniform. 
Thenf  =  <f>  uniformly  in  21  when  and  only  when 

e>0,         ^>0          \f  —  <f>\<e     ,     zmgfi,      8  fixed. 

3.  Example.    Let /(#,  TI)  = 
where  a    / 

Then         ^(a;)  =  lim/(2J,  ri)=Q     ,     in  21  =  (0,  oo). 

Let  us  investigate  whether  the  convergence  is  uniform  at  the 
point  x  in  21- 

First  let  x  >  0.     If  0  <  a  <  x  <  b,  we  have 


170  SERIES   OF   FUNCTIONS 

As  the  term  on  the  right  =  0  as  n  =  oo  ,  we  see/=</>  uniformly 
in  (#,  b). 

When,  however,  a  =  0,  or  b  =  oo  ,  this  reasoning  does  not  hold. 
In  this  case  we  set  _  nfixp 

which  gives  ^  logl/|3    t 

n*& 
As  the  point  (x,  ri)  ranges  over  £  denned  by 

z^>0     ,     n>\, 
the  point  (£,  ?i)  ranges  over  a  field  £  defined  by 


and  the  correspondence  between  £  and  X  is  uniform.     Here 


The  relation  2)  shows  that  when  #  >  0,  t  =  en  asw-^oo;  also 
when  x  =  0,  £  =  1  for  any  n.  Thus  the  convergence  at  x  =  0  is 
uniform  when 

H- 

The  convergence  is  not  uniform  at  x  =  0  when  3)  is  not  satisfied. 
For  take  -, 

•  -•JL     ,     n=l,2,... 

n\/a. 

For  these  values  of  a:  ^ 


which  does  not  =  0  as  n  =  oo  . 
146.    1.    (Moore,  Osgood.)     Let 


uniformly  in  3(.     Let  a  be  a  limiting  point  of  21  and 
lim/ 

a-=a 

/or  gac^  f  iw  Fi*(r). 
c^lim 

ar=a 

exist  and  are  equal.     Here  a,  T  are  finite  or  infinite. 


GENERAL   THEORY  171 

We  first  show  <I>  exists.     To  this  end  we  show  that 
€>0     ,     S>0     ,     |  <£<V)  -  <£<V')  |  <  €         a/,  x"  in  F6*(»    (1 

Now  since  /(a:,  £)  converges  uniformly,  there  exists  an  77  >0 
such  that  for  any  x',  x"  in  51 

)  (2 


On  the  other  hand,  since/  =  -\/r  there  exists  a  &  >0  such  that 

/(*',  0  =  ^(0+*'"'  (4 


for  any  a;',  xrl  in  V&*(a)  ;  t  fixed. 

From  2),  3),  4),  5)  we  have  at  once  1).  Having  established 
the  existence  of  <l>,  we  show  now  that  3>  =  \f.  For  since  /  con 
verges  uniformly  to  0,  we  have 


/O,  0  -  £O)  I  <  |        *  in  «  •• ,    t  in  r,*(r).  (6 

Since /=  i/r,  we  have 
|  /(z,  0  -  ^  (0  I  <  I         *  in  TV  (a)     ,     t  fixed  in  F,*  (T).      (7 

Since  <f>  =  <£, 

I*W~*    <|         *»^»(a).  (8 

Thus  7),  8)  hold  simultaneously  for  8  <  8',  8". 
Hence  ,   ,  , ,s  _  -  , 

or  lim 

2.    Thus  under  the  conditions  of  1) 

lim  lim  /  =  lim  lim  / ; 

x=a    t=r  t=r    x—a 

in  other  words,  we  may  interchange  the  order  of  passing  to  the 
limit. 


172  SERIES   OF   FUNCTIONS 

3.  The  theorem  in  1  obviously  holds  when  we  replace  the  un 
restricted  limits,  by  limits  which  are  subjected  to  some  condition ; 
e.g.  the  variables  are  to  approach  their  limits  along  some  curve. 

4.  As  a  corollary  we  have  : 

Let  F  =  2/80*i  •••  %m)  t>e  uniformly  convergent  in  21,  of  which  x  =  a 
is  a  limiting  point.     Let  Iimf8  =  18,  and  set  L  =  ^L18.      Then 

X=(l 

Urn  F  =  L  ;         a  finite  or  infinite, 

x=a 

or  in  other  words 


lim  2jf,  =  2  limft. 
Example  1. 


**     %nenx 

converges  uniformly  in  51  =  (0,  oo)  as  we  saw  136,  2,  Ex.  1.     Here 

iimA=i=?n)         I  ; ' 

i  -r        "?  7  X^    1         ^ 

and  L  =  2L  =  >,  —  =1. 


Hence  lim  F(x)  =  1. 

a?=oo 

Also  1 


hence  R\\mF(x)=Q. 

Example  2. 


in        x 


converges  uniformly  in  any  interval  finite  or  infinite,  excluding 
x  —  0,  where  F  is  not  defined.     For 


and  -j      y\  1  _ 

^  n ! 

Hence  lim  JYaf)  =  e. 


GENERAL   THEORY  173 

Example  3. 


=  0  forz=0. 

Here  limJ(a 

*=0 

while 


Slim  /.(*)=  20  =  0. 


Thus  here  Hm 


«=0  35  =  0 


But  F  does  not  converge  uniformly  at  x  =  0.     On  the  other 
hand,  it  does  converge  uniformly  at  x—  ±  oo. 

Now 


and  lim  2/n(V>  =  2  lim  /„(*), 

a?=±x  at=j-x> 

as  the  theorem  requires. 

Example  4-      Wf  \  _  V  f  nx2      ( 

-- 


which  converges  about  x  =  0  but  not  uniformly. 
However,  iim  2/j|(!B)  =  2lim/.(*)  =  0. 


Thus  the  uniform  convergence  is  not  a  necessary  condition. 
147.    1.   Let   lim  /(^•••^ffl,  ^  •••  O  =  <£0i  •••#,»)   uniformly  at 

t-T 

x  =  a.     Let  /(#,  f)  6^  continuous  at  x=  a  for  each  t  in  Vf>*(r). 
Then  <f>  is  continuous  at  a. 

This  is  a  corollary  of  the  Moore-Osgood  theorem. 
For  by  146,  1 

lim  lim  /(a  +  h,  f)  =  lim  lim  /(a  +  h,t). 

h=o     t=r  t=r      h=o 

Hence  ]im  ^^  +  A)  =  lim  /(a,  f)  =  <£(a).  Q.E.D. 


174  SERIES   OF   FUNCTIONS 

A  direct  proof  may  be  given  as  follows  : 

/(«,  0  =  j>(x)  +  e'         |  €'  |  <  c,  x  in 

<K^-<K^')=/<X,  0  -/(*",  0+6 
But  |/(*",0-/<y>0    <*     ,     if  I  *'  - 

2.  Ze£  F  =  ^fSl...Sp(^x1  "•  xm)  be  uniformly  convergent  at  x=a. 
Let  each  fSl...Sp  be  continuous  at  a.      Then  F(xl  •••  xm*)  is  continuous 
at  x  =  a. 

Follows  at  once  from  1). 

3.  In  Ex.  3  of  140  we  saw  that 

=  V  _  ?L  _ 


is  discontinuous  at  x  =  0  and  does  not  converge  uniformly  there. 
In  Ex.  4  of  140  we  saw  that 


does  not  converge  uniformly  at  x  =  0  and  yet  is  continuous  there. 
We  have  thus  the  result  :    The  condition  of  uniform  convergence  in 
1,  is  sufficient  but  not  necessary. 
Finally,  let  us  note  that 


xa 


is  a  series  which  is  not  uniformly  convergent  at  x  =  0,  although 
F(x)  is  continuous  at  this  point. 

4.  Let  each  term,  of  F=  ^fSi...Sp(^x^  •••  xm)  be  continuous  at  x  =  a 
while  F  itself  is  discontinuous  at  a.  Then  F  is  not  uniformly 
convergent. 

For  if  it  were,  F  would  be  continuous  at  a,  by  2. 

Remark.  This  theorem  sometimes  enables  us  to  see  at  once 
that  a  given  series  is  not  uniformly  convergent.  Thus  140, 
Exs.  2,  3. 


GENERAL   THEORY  175 

5.  The  power  series  P=  2aSl...Sm  afr  •••  x£  is  continuous  at  any 
inner  point  of  its  rectangular  cell  of  convergence. 

For  we  saw  P  converges  uniformly  at  this  point. 

6.  The    power   series    P  =  aQ  +  a^x  +  a2x2  +  •••   is  a    continuous 
function  of  x  in  its  interval  of  convergence. 

For  we  saw  P  converges  uniformly  in  this  interval.  In  par 
ticular  we  note  that  if  P  converges  at  an  end  point  x  =  e  of  its 
interval  of  convergence,  P  is  continuous  at  e. 

This  fact  enables  us  to  prove  the  theorem  on  multiplication  of 
two  series  which  we  stated  112,  4,  viz.  : 

148.    Let  A  =  ^  +  fli  +  a^  +  _     ^     5  =  &0  +  &!  +  fta  +  - 

0=  aQbQ  +  (fl^j  +  a^)  +  (00£2  +  afa  +  a260)  +  ... 
converge.      Then  AB  =  C. 

For  consider  the  auxiliary  series 

F(x)  =  a0  +  «!•£  +  atf?  +  — 


x)  =  aQb0  -f  (a/1  +  aj^x  +  •" 

Since  A,  E,  0  converge,  F,  G-,  H  converge  for  x  =  1,  and  hence 
absolutely  for  |  x  \  <  1.     But  for  all  |  x  \  <  1, 


Thus  L  lim  H(x)  =  L  lira  F(x)  •  L  lira  G-  (x), 

x=\  x=l  x  =  i 


or 


149.  1.  We  have  seen  that  we  cannot  say  that/=  $  uniformly 
although  /  and  <£  are  continuous.  There  is,  however,  an  impor 
tant  case  noted  by  Dini. 

Let  f(x±  —  xm,  ^  —  tn)  be  a  function  of  two  sets  of  variables 
such  that  x  ranges  over  51,  and  t  over  a  set  having  r  as  limiting 
point,  T  finite  or  ideal.  Let 

lim/O,  f)=  </>O)       in  51. 

t=r 

Then  we  can  set          ...      ,.        ,,  ^  ,    ,  f     ,, 
f(x,t)=4>(x)++(x,  0- 


176  SERIES  OF   FUNCTIONS 

Suppose  now  |  ty(x,  t')\<\  ^(x,  t)  \  for  any  t'  in  the  rectangu 
lar  cell  one  of  whose  vertices  is  t  and  whose  center  is  r.  We  say 
then  that  the  convergence  of  /  to  <£  is  steady  or  monotone  at  x. 
If  for  each  x  in  51,  there  exists  a  rectangular  cell  such  that  the 
above  inequality  holds,  we  say  the  convergence  is  monotone  or 
steady  in  51. 

The  modification  in  this  definition  for  the  case  that  T  is  an  ideal 
point  is  obvious.  See  I,  314,  315. 

2.    We  may  now  state  Dini's  theorem. 

Let  /(#!  •••  zmi  *i  •••£»)==  0(^i  '••  xm)  steadily  in  the  limited  com 
plete  field  51  as  t  =  T;  T  finite  or  ideal.  Let  f  and  <j>  be  continuous 
functions  of  x  in  51.  Then  f  converges  uniformly  to  <£  in  51. 

For  let  x  be  a  given  point  in  51,  and 


We  may  take  t'  so  near  r  that  |  *fy(x,  t')  \  <  -• 

o 

Let  x'  be  a  point  in  V^x),     Then 

f(x<,  o  =  <K*')  +  tO',  O- 

As  /is  continuous  in  #, 


Similarly, 

Thus 

Hence  |  ./r<V>  0  I  <  €         for  any  *'  in  F.O) 

and  for  any  £  in  the  rectangular  cell  determined  by  t'  . 
As  corollaries  we  have  : 

3.  Let   Gr  =  2  |/tl...ia(^i  •••  Xm)  |  converge  in  the  limited  complete 
domain  51.     Let  G-  and  each  ft  be  continuous  in  51-      Then  G-  and 
a  fortiori  F=  2/tl...t-  converge  uniformly  in  51,  furthermore  ftl...ls=  0 
uniformly  in  51. 

4.  Let  Gr  =  2  |/tl...  ^(^  •••  rrm)  |  converge  in  the  limited  complete 
domain  51,  having  a  as  limiting  point.     Let  Gr  and  each  f,  be    con- 


GENERAL   THEORY  177 

tinuous  at  a.      Then  G  and  a  fortiori  F=  2/tl...la  converge  uniformly 
at  a. 

5.    Let   6r  =  2  |/tl...ta(^i  •••  2"m)  |  converge  in  the  limited  complete 
domain  21,  having  a  as  limiting  point.     Let  lim  Cr  and  each  lim/"t 

x=a  x=a 

exist.         Moreover,  let 


Then  Gr  is  uniformly  convergent  at  a. 

For  if  in  4  the  function  had  values  assigned  them  at  x  =  a  dif 
ferent  from  their  limits,  we  could  redefine  them  so  that  they  are 


continuous  at  a. 


150.    1  .    Let    lim  f(xt  •  •  •  a?m,  ^  •  •  •  tn~)  =  <£  (x^  •  •  •  xm)  uniformly  in 

t=r 

the  limited  field  21.     Xe£  0  be  limited  in  21. 


lim  f/=    f<£  =    film/. 

t=TJ%  ju%  «/g   #  =  T 


For  let  /=<^  +  ^r. 

Since  /=  <#>  uniformly          |^|  <  € 

for  any  t  in  some  V*(r)  and  for  any  z  in  21. 
Thus 


Remark.  Instead  of  supposing  <£  to  be  limited  we  may  suppose 
that/(#,  t)  is  limited  in  21  for  each  t  near  r. 

2.  As  corollary  we  have 

Let  lim/(^1  •••  xm,  tl"-t^)  =  <t>(%i  •-  xni)  uniformly  in  the  limited 

t=T 

field  2L     Letf  be  limited  and  integrable  in  2f  for  each  t  in  Tr5*(r). 
Then  <f>  is  integrable  in  21  and 

lim  f/=    f*=    flim/. 

«=T  ^$1  ^21  ^21  t=r 

3.  From  1,  2,  we  have  at  once: 

Let  F  =^flv..Ls(xl"-xm)  be  uniformly  convergent  in  the  limited 
field  21-  Let  each  /tl...ls  be  limited  and  integrable  in  2(.  Then  F  is 
integrable  and 


r»  /» 

I  F—  ^  (  f 

I  •*    —   ~     I    /»!•-«• 

Jgt  ^ 


178  SERIES   OF   FUNCTIONS 

If  the  f^...^  are  not  integrable,  we  have 


Example.  J&7—  V 

~ 


does  not  converge  uniformly  at  x  =  0.     Cf .  140,  Ex.  3. 
Here  _     J_ 


and  jYrN       fl         for 

~  10         for  x  =  0. 

Hence 


'* 


'*.*=  1-  /' 

*/o  1 


+  nx* 
—  1  _  arctg  Vn  ^_  .j 


Thus  we  can  integrate  F  termwise  although  F  does  not  converge 
uniformly  in  (0,  1). 

151.    That  uniform  convergence  of  the  series 

with  integrable  terms,  in  the  interval  51  =  (a  <  5)  is  a  sufficient 
condition  for  the  validity  of  the  relation 

Xb  fb  pb 

Fdx  =    \   f^dx  +    I   fjdx  +  •  •  • 

is  well  illustrated  graphically,  as  Osgood  has  shown.* 

Since  1)  converges  uniformly  in  H  by  hypothesis,  we  have 

and 

|  Fn  (x)  |  <  e         n  >  m  (3 

for  any  x  in  51. 

*  Bulletin  Amer.  Math.  Soc.  (2),  vol.  3,  p.  59. 


GENERAL  THEORY 


179 


In  the  figure,  the  graph  of  F(x)  is  drawn  heavy.  On  either 
side  of  it  are  drawn  the  curves  F—  e,  F -\- e  giving  the  shaded 
band  which  we  call  the  e-band. 

From  2),  3)  we  see  that  the  graph  of 
each  Fn<  n>m  lies  in  the  e-band.  The 
figure  thus  shows  at  once  that 


and 


X 
_ 


can    differ    at   most   by  the  area   of    the     a 
e-band,  i.e.  by  at  most 


Cb'2edx  =  2e(b- 

•Jo, 


152.     1.    Let  us  consider  a  case  where  the  convergence  is  not 
uniform,  as 

F(x^  -^  [nx  _  (n-l)x\  _ 
•*        -         - 


Here 


nx 


If  we  plot  the  curves  y  =  Fn(x),  we  observe  that  they  flatten 
out  more  and  more  as  n  ==  oo,   and  approach   the  #-axis  except 

near  the  origin,  where 
they  have  peaks  which 
increase  indefinitely  in 
height.  The  curves 
Fn(x),  n>m,  and  m  suf 
ficiently  large,  lie  within 
an  e-band  about  their 
limit  F(x)  in  any  inter 
val  which  does  not  in 
clude  the  origin. 

If  the  area  of  the 
region  under  the  peaks 
could  be  made  small  at 
pleasure  for  m  sufficiently  large,  we  could  obviously  integrate 
termwise.  But  this  area  is  here 


180  SERIES   OF   FUNCTIONS 


=  -         as  n  =  QO  . 

Thus  we  cannot  integrate  the  F  series  termwise. 

2.    As  another  example  in  which  the  convergence  is  not  uniform 
let  us  consider 


Here 

-r,       nx 


The  convergence  of  F  is  uniform  in  51  =  (0,  1)  except  at  x  =  0. 
The  peaks  of  the  curves  Fn(x)  all  have  the  height  e~l. 

Obviously  the  area  of  the 
region  under  the  peaks  can  be 
made  small  at  pleasure  if  m  is 
taken  sufficiently  large.  Thus 
in  this  case  we  can  obviously 
integrate  termwise,  although 
the  convergence  is  not  uniform 
in  21. 


We  may  verify  this  analytically.     For 

CXFndx=  CX—dx  =  --1  +  nx=Q       asn  =  oo. 
Jo  Jo    enx  n         nenx 

3.    Finally  let  us  consider 


Here  ,  n** 


1  +  *M 

The  convergence  is  not  uniform  at  x  =  0. 

The  peaks  of  Fn(x)  are  at  the  points  x  =  »"*,  at  which  points 

Fn  =  l  -Vn. 


GENERAL   THEORY  181 

Their  height  thus  increases  indefinitely  with  n.      But  at  the 
same  time  they  become  so  slender  that  the  area  under  them  =  0. 
In  fact 


We  can  therefore  integrate  termwise  in  (0  <  a). 

153.     1.    Let  Urn  G-(x,  ^  ...  fn)  =g(x)  in  51  =  (a,  a  +  $),  T  /m'te 

<=T 

or  infinite.     Let  each  G-'x(x,  t)  be  continuous  in  51  ;   also  let  Gr'x(x,  £) 
converge  to  a  limit  uniformly  in  51  as  t  =  r.      Then 

Urn  a'x(x,t)=g'(x)         m5l,  (1 

t=T 

and  g\x}  is  continuous. 
For  by  150,  2, 


By  I,  538,  ~, 

I      (jrxdx  =  CrCx,  t^)  —  GrCa*  £). 
*/ a 

Also  by  hypothesis,  ^  { &  ^  f}  _  &^  ()l=ffi 
Hence 


g(x)-g(a)  =  film  ^(a;,  «)<£«.  (2 

*^a       /=T 


But  by  147,  l,  the  integrand  is  continuous  in  51. 
Hence  by  I,  537,  the  derivative  of  the  right  side  of  2)  is  this  in 
tegrand.     Differentiating  2),  we  get  1). 

2.    Let  F(x)  =  2/tl ...  lt(x)  converge  in  51  =  (a,  a  +  S).     Let  each 
f'(x)  be  continuous,  also  let 

2/; (*) 

be  uniformly  convergent  in  51.      Then 

l?'(ar)  =  2//(aj),         in  %. 
This  is  a  corollary  of  1. 


182  SERIES  OF   FUNCTIONS 

3.    The  more  general  case  that  the  terms  /4...ls  are  functions  of 
several  variables  xv  •••  xm  follows  readily  from  2. 

154.    Example. 


Here 


a  function  whose  uniform  convergence  was  studied,  145,  3.    We  saw 

F(x)  =  0         for  any  x  >  0. 
Hence  F'(x)  =  0        x>0. 

Let  (?O)  =  ?//,(*)•  (1 


hence  J"(^)=2/^),  (2 

and  we  may  differentiate  the  series  termwise. 

If  a;  =  0,  and  «=1,  X>0;    (7n(0)  =  -  wx  =  -  oo  as  n  =  oo. 

In  this  case  2)  does  not  hold,  and  we  cannot  differentiate  the 
series  termwise. 

For  x=Q,  and  a>l,  6rn(0)=0,  and  now  2)  holds;  we  may 
therefore  differentiate  the  series  termwise.  But  if  we  look  at  the 
uniform  convergence  of  the  series  1),  we  see  this  takes  place  only 

when  «-l       X 

/S        // 

155.    1.   (Porter.)  Let  F^=^    ^ 

converge  in  51  =  (a,  J).     For  every  x  in  51  let  \fl(x)\  <  g^  a  constant. 
Let  G-  =  ^g,  converge.      Then  F(x)  has  a  derivative  in  51  and 

F'W^-Sf  „.....(*)  i  C1 

or  we  may  differentiate  the  given  series  termwise. 


GENERAL   THEORY  183 

For  simplicity  let  us  take  8  =  1.     Let  the  series  on  the  right  of 
1)  be  denoted  by  <#>(V).     ^or  eac^  x  m  ^  we  snow 


e>0,          .,.,          _         ^ 


<  e,         I  Az  I  <  S. 


For 


where  fn  lies  in  V?>(x 

Thus       D=. 

i 

But  G-  being  convergent,  6rm  <  e/3  if  m  is  taken  sufficiently  large. 
Hence 

|J>»I<  2  i/;a)l+  2  |/;c*)|< 2 <?.<}«. 

ff»+l  m-fl 

On  the  other  hand,  since  =«  ==/»(^)  and  since  there  are  only  ?w 

Az 

terms  in  Z)m,  we  may  take  5  so  small  that 

|l>J<e/8. 

Thus  |^> 

2.    Example  1.     Let 

TO---WtfO      ->l          0 


This  series  converges  uniformly  in  51  =  (0  <  6),  since 

I     /»    s      \  I 


Also  x     -^^         ^n 

-.• 


n  !        (1  +  «r 
Hence 


As    l^rn   converges,    we   may   differentiate    1)    termwise.      In 
general  we  have 


valid  in  51. 


184  SERIES  OF  FUNCTIONS 

3.    Example  2.     The  fl  functions. 
These  are  defined  by 

0j  (x)  =  2  i  (  -  1)  Yn+i)2  sin  (2  n  +  1)  TO 

o 

=  2  jl  sin  THE  —  2  2*  sin  3  THE  -f 
,V2  (a;)  ==  2  l^n+=)2  cos  (2/1  +  1)  TTX 

0 

=  2  <?*  cos  vrx  +  2q*  cos  3  TT.E  + 


,98  (a:)  =  1  4-  2  2?n2  cos  2 

=  14-2^  cos  2  ?ra;  +  2  ^*  cos  4  TTX  -f- 


»V0  (a;)  =  1  H-  2      (  -  l)n£n2  cos  2 
i 

=  1  —  2  <7  cos  2  THE  +  2  g-4  cos  4  THE  —  •  •  • 

Let  us  take  ,        .  -^ 

Then  these  series  converge  uniformly  at  every  point  x.     For 
let  us  consider  as  an  example  »vr     The  series 


is  convergent  since  the  ratio  of  two  successive  terms  is 


9* 

and  this  =  0.     Now  each  term  in  »vx  is  numerically 

<\q  (n+^<    q\n\ 
and  hence  <  the  corresponding  term  in  T. 

Thus  &i(x)  is  a  continuous  function  of  x  for  every  x  by  147,  2. 
The  same  is  true  of  the  other  .(/'s.  These  functions  were  discovered 
by  Abel,  and  were  used  by  him  to  express  the  elliptic  functions. 

Let  us  consider  now  their  derivatives. 

Making  use  of  155,  1  it  is  easy  to  show  that  we  may  differentiate 
these  series  termwise.  Then 


d  '  O)  =  2  -IT!  (  -  l)n(2  n  +  1)  0<»+*>*  cos  (2  w  +  1)  TTX 
o 

=  2?r(g*  cos  TTX  —  3<2*  cos  3  TTX  +  •••). 


GENERAL   THEORY  185 


^  (z)  =  _  2  TT    (2  n  +  1)  2<"+*)2  sin  (2  71  +  1)  TTZ 
o 

=  —  2^(9!  sin  TT#  •+-  3  q$  sin  3  THE  +  •••)• 

00 

#g'  (a;)  =  —  4  7r2  w^n2  sin  2  71772; 
i 

=  —  4  TT  (5-  sin  2  TTZ  +  2  ^*  sin  4  TTX  +  •  •  •)  . 


,^  (a;)  =  -  4  Tr     (  -  l)nnq^  sin  2 
i 

=  +  4  TT  (^  sin  2  TTX  —  2q*  sin  4  TTX  +  •••). 

To  show  the  uniform  convergence  of  these  series,  let  us  con 
sider  the  first  and  compare  it  with 


The  ratio  of  two  successive  terms  of  this  series  is 


,2n+1 


which  =  0.     Thus  S  is  convergent.     The  rest  follows   now  as 
before. 

156.    1.    Let 


t=r  h 

uniformly  for  0  <  |  A  |  <  17,  T  finite  or  infinite. 

Let 


'x(a,  0  ftw«* 
/or  each  t  near  r.      Then  g'  (a)  exists  and 


This  is  a  corollary  of  146,  1.     Here 

&O  +  A,  t)-GKa,  0 

A 
takes  the  place  of  f(x,  £). 

2.    From  1  we  have  as  corollary  : 


186  .         SERIES   OF   FUNCTIONS 

converge  for  each  x  in  51  which  has  x  =  a  as  a  proper  limiting  point. 
Letf((a)  exist  for  each  i  =  (iv  •••  tn).     Let 


converge  uniformly  with  respect  to  h.      Then 


CHAPTER   VI 
POWER    SERIES 

157.  On  account  of  their  importance  in  analysis  we  shall 
devote  a  separate  chapter  to  power  series. 

We  have  seen  that  without  loss  of  generality  we  may  employ 
the  series  a0  +  alX  +  a^  +  ...  (1 


instead  of  the  formally  more  general  one 

aQ  +  al(x  —  a)+  a^x-a)2-\-  - 

We  have  seen  that  if  1)  converges  for  x  =  c  it  converges  abso 
lutely  and  uniformly  in  (—7,  7)  where  0  <  7  <  |  c  |.  Finally, 
we  saw  that  if  c  is  an  end  point  of  its  interval  of  convergence,  it 
is  unilaterally  continuous  at  this  point.  The  series  1)  is,  of  course, 
a  continuous  function  of  x  at  any  point  within  its  interval  of 
convergence. 

158.    1.    Let  P(x)  =  a0  +  a^x  +  a2x2  +  •••  converge  in  the  interval 
$1  =  (—  «,  «)  which  may  not  be  complete.      The  series 

P.-l  .'  2  •  ...  M.  +  2  •  ft  •  —  (f»+  l)an+lx  +  - 

obtained  by  differentiating  each  term  of  P  n  times  is  absolutely  and 
uniformly  convergent  in  $8  =  (—  A  /3),  ft<  a,  and 


P.C?),         ins. 

For  since  P  converges  absolutely  for  x  =  /3, 
an{3n<M,         n=l,2,... 
Let  now  x  lie  within  33.     Then  the  adjoint  series  of  P^(x}  is 


Now  its  mih  term 

j  _  mctmQm  f  g\m~l  .  mM 
&     \£)        •  ft\ft 

187 


188  POWER   SERIES 

But  the  series  whose  general  term  is  the  last  term  of  the  pre 
ceding  inequality  is  convergent. 

2.    Let  P=a0  +  a1x  +  a%xz  +  ••• 

converge  in  the  interval  21.      Then 


where  «,  x  lie  in  21.     Moreover  Q  considered  as  a  function  of  x  con 
verges  uniformly  in  21. 

For  by  137,  P  is  uniformly  convergent  in  (a,  x).  We  may 
therefore  integrate  term  wise  by  150,  3.  To  show  that  Q  is  uni 
formly  convergent  in  21  we  observe  that  P  being  uniformly  con 
vergent  in  21  we  may  set 


where  i  D"  i  n         i 

I  Pm  I  <  <r,         m>m0,  o-  small  at  pleasure. 

Then 


on  taking  <r  sufficiently  small. 

159.  1.  Let  us  show  how  the  theorems  in  2  may  be  used  to 
obtain  the  developments  of  some  of  the  elementary  functions  in 
power  series. 

The  Logarithmic  Series.      We  have 


1  —  x 
for  any  x  in  21  =  (-  1*,  1*).     Thus 


l-x 
Hence 


This  gives  also 

a;    =  z-      +       -  -      ;     a;  in 


GENERAL   THEORY  189 

The  series  1)  is  also  valid  for  x  =  1.  For  the  series  is  conver 
gent  for  x  =  1,  and  log  (1  +  x)  is  continuous  at  x  =  1.  We  now 
apply  147,  6. 

For  x  =  1,  we  get 

2.    The  Development  of  arcsin  x.     We   have   by  the  Binomial 


for  x  in  51  =  (-!*,  1*).     Thus 


It  is  also  valid  for  x  =  1.     For  the  series  on  the  right  is  conver 
gent  for  x  —  1.     We  can  thus  reason  as  in  1. 
For  x  =  1  we  get 


Zr_  1  1.3          1.3.5 

2~      ^2-3      2.4.5      2.4.6-7 


3.    The  Arctan  Series.     We  have 

_J  —  =l_^  + 
1+  x2 

for  x  in  51  =  (-  1*,  1*).     Thus 


X      .    X  xo 

=  *~3-+5- 

valid  in  31.     The  series  3)  is  valid  for  x  =  1  for  the  same  reason  as 
in  2. 

For  x  =  1  we  get      TT  _  -,  _  1  ,  1  _  1  , 
4"          3  +  5      7~^ 

4.    The  Development  of  ex.     We  have  seen  that 


converges  for  any  #.     Differentiating,  we  get 


190  POWER   SERIES 

Hence  E'(x)=E(x)  (a) 

for  any  x.     Let  us  consider  now  the  function 


by  (a).     Thus  by  I,  400,/(V)  is  a  constant.     For  x  =  0,/(V)  =  1. 
Hence  r      ^      ~3 

?x  —  1  4-  —  -4-  —  4-         -|-  . 

hl!  +  2!  +  3!^ 
valid  for  any  #. 

5.    Development  of  cos  #,  sin  x. 

The  series  9         d        r 

(7=1-^  +  ^-^+... 
2  !  ^  4  !      6  ! 

converges  for  every  x.     Hence,  differentiating, 


Hence  adding,  (7+  (7"  =  0.  (b) 

Let  us  consider  now  the  function 

f(x)  =  (7  sin  x  +  C"  cos  #. 
Then 


sn  ^  _       sn  ^  +         cos  a; 
=  ((7+  <7")cosa; 
=  0         by  (b). 
Thus  /(V)  is  a  constant.     But  (7=1,   C"  =  0,  for  a;  =  0,  hence 

/(*)-o, 

or  C  sin  a:  +  C'  cos  2;=  0.  (c) 

In  a  similar  manner  we  may  show  that 
or  #0*0=  Ccosx—  0'  sin  x=  1.  (d) 


GENERAL   THEORY  191 

If  we  multiply  (c)  by  sin  x  and  (d)  by  cos  x  and  add,  we  get 
0=  cos  x.     Similarly  we  get  C'  —  —  sin  x.     Thus  finally 


.. 

valid  for  any  #. 

160.  1.  Let  P  =  amxm  +  am+1xm+1  +  •••  ,  am  =£  0,  converge  in 
some  interval  51  about  the  origin.  Then  there  exists  an  interval 
53  <  51  in  which  P  does  not  vanish  except  at  x  =  0. 


=  xmQ. 

Obviously  Q  converges  in  51.  It  is  thus  continuous  at  x  =  0. 
Since  Q  =£  0  at  x  =  0  it  does  not  vanish  in  some  interval  33  about 
3=0  by  I,  351. 

In  analogy  to  polynomials,  we  say  P  has  a  zero  or  root  of  order 
m  at  the  origin. 

2.  Let  P  —  aQ  4-  a^x  +  a2z2  4-  •••  vanish  at  the  points  bv  J2,  ...  =  0. 
Then  all  the  coefficients  an  =  0.  The  points  bn  are  supposed  to  be 
different  from  each  other  and  from  0. 

For  by  hypothesis  P(bn)  =  0.     But  P  being  continuous  at  x  =  0, 


Hence  P(0)=0, 


and  thus 
Hence 


p  = 


Thus  P1  vanishes  also  at  the  points  bn.  We  can  therefore 
reason  on  Pl  as  on  P  and  thus  a1  =  0.  In  this  way  we  may 
continue. 

3.    If  P  =  a0  +  aiz+- 


192  POWER  SERIES 

be  equal  for  the  points  of  an  infinite  sequence  B  whose  limit  is  x  =  0, 
then  an=  bn,  n  =  0,  1,  2  «•• 

For  P  —  Q  vanishes  at  the  points  B. 

Hence  i       A  A   -i    o 

«n-  bn  =  v     ,     w  =  0,  1,  2-.. 

4.  Obviously  if  the  two  series  P,  §  are  equal  for  all  x  in  a 
little  interval  about  the  origin,  the  coefficients  of  like  powers  are 
equal;  that  is  ^  =  ^  ?  n  =  0,l,2... 

161.    1.    Let  y  =  ao  +  <v;  +  v3+...  (1 

converge  in  an  interval  51.     As  #  ranges  over  51,  let  i/  range  over 
an  interval  $&.     Let 

'"  (2 


converge  in  35.     Then  z  may  be  considered  as  a  function  of  x  de 
nned  in  51.     We  seek  to  develop  z  in  a  power  series  in  x. 

To  this  end  let  us  raise  1)  to  the  2°,  3°,  4°  ...  powers  ;  we  get 
series  „  o 

y    =  ^20  +  a2lx  +  ^22^  +  "• 

wx*  +'~  (3 


which  converge  absolutely  within  51. 
We  note  that  amn  is  a  polynomial. 


in  «0,  ••-  #n  with  coefficients  which  are  positive  integers. 
If  we  put  3)  in  2),  we  get  a  double  series 


D=  (b  +  b)  +  b^x  -f  b^x2  + 

a21'7;  +  *2a222'2  + 

si^  +  V82232  + 
+        .....  .      V      • 


V20 


If  we  sum  by  rows,  we  get  a  series  whose  sum  is  evidently  0, 
since  each  row  of  D  is  a  term  of  z.     Summing  by  columns  we  get 

a  series  we  denote  by 

C  =  t'0  +  cx  +  czx*  +  •  •  •  (5 


GENERAL   THEORY  193 


cl  =  blal  +  62«21  4-  Vsi  -!  ----  (6 


We  may  now  state  the  following  theorem,  which  is  a  solution  of 
our  problem. 

.     Let  the  adjoint  y-series, 


converge  for  £  =  £0  to  the  value  T)  =  7/0.     Let  the  adjoint  z  series 

-  (8 


converge  for  77  =  ?;0.      T^e/i  the  z  series  2)  caw  be  developed  into  a 
power  series  in  x,  viz.  the  series  5),  which  is  valid  for  \  x  \  <  £0. 

For  in  the  first  place,  the  series  8)  converges  for  77  <.TJO.     We 
show  now  that  the  positive  term  series 


converges  for  £  <  f0.  We  observe  that  ^)  differs  from  Adj  D, 
at  most  by  its  first  term.  To  show  the  convergence  of  X)  we 
have,  raising  7)  to  successive  powers, 


7,2  = 


We  note  that  Amn  is  the  same  function  Fm%n  of  «0,  «j,  •••  «n  as 
amn  is  of  a0,  •••  aB,  i.e. 


As  the  coefficients  of  Fm^  n  are  positive  integers, 


194  POWER   SERIES 

Putting  these  values  of  ?;,  ??2,  rf  •••  in  8),  we  get 

A  =  8  + 


Summing  by  rows  we  get  a  convergent  series  whose  sum  is  ? 
or  8).  But  this  series  converges  for  £  <  f0  since  then  rj<rj^ 
and  8)  converges  by  hypothesis  for  rj  =  IJQ.  Now  by  9)  each 
term  of  £)  is  <  than  the  corresponding  term  in  A.  Hence  £) 
converges  for  f  <  £0. 

2.    As  a  corollary  of  1  we  have  : 

Let 

y  =  c 

converge  in  H,  and 


converge  for  all  —  oo  <  y  <  -f  °o«      2%ew  2  can  5e  developed  in  a 
poiver  series  in  x, 

z—  cQ  +  0^+  c%x2  +  ...  =  O 
for  all  x  within  51. 

3.    Let  the  series 

y  =  amxm  -f  am+1xm+l  H  ----  ,         w  >  1 
converge  for  some  x  >  0.     T/  fAg  series 

z  =  bQ+bly  +  btf*  +  ••• 
converges  for  some  y  >  0,  i'£  caw  ft^  developed  in  a  power  series 

Z=  CQ+  CjX  +  C2X2-\  ---- 

convergent  for  some  x  >  0. 

For  we  may  take  f  =  |  x  \  >  0  so  small  that 

V  =  «mfm  +  «»+if  ™+1  H-  -• 
has  a  value  which  falls  within  the  interval  of  convergence  of 


4.    Another  corollary  of  1  is  the  following  : 
y=  a9  +  a]x  +  a^x2  +  ... 


GENERAL   THEORY  195 

converge  in  21  =  (—  A,  A).      Then  y  can  be  developed  in  a  power 
series  about  any  point  c  of  21, 


which  is  valid  in  an  interval  53  whose  center  is  c  and  lying  within  21. 
162.     1.    As  an  application  of  the  theorem  161,  l  let  us  take 

s^  +  jL  +  ^  +  r  + 
i  !    2  r  3  r 

_  z__z^  ,  ^__ 
y      1  !      3  !      5  ! 

As  the  reader  already  knows, 

z  =  ev     ,     y  —  sin  a?, 
hence  z  considered  as  a  function  of  x  is 

z  = 


We  have 

z  =  1  +  z  +  0  •  z2  -  i  r3  +  0.*4  +  T|o  ^+  0  -a6  4- 

+  -i.^+    0    -  \x*  +      0      +^+.. 
H-j^-h     0     -iV^5    +      0     +  .. 


Summing  by  columns,  we  get 

Z=^n*=1  +  ^+j^_i^__l_^5__l_^... 

2.    As  a  second  application  let  us  consider  the  power  series 


z  = 

convergent  in  the  interval  21  =  (-  R,  R).     Let  z  be  a  point  in  21. 
Let  us  take  77  >  0  so  small  that  y  =  x  +  h  lies  within  21  for  all 

|*|<L* 

Then  ,. 

z  =  a0  +  flj  (x  +  h) 

+  a2  (z2  +  2  zA  +  A2) 


196  POWER   SERIES 

This  may  be  regarded  as  a  double  series.  By  161,  l  it  may  be 
summed  by  columns.  Hence 

P(x  +  h)  =  «0  +  ap  +  a2x2  +  a&*  +  ••• 

+  A(at  +  2  «2z  +  3  OgZ2  +  •••) 

+  |l(2«a  +  2.3a^  +  3.4fl42Ja  +  •••)  (2 

+  ............ 

=  P(x)+hP>(x)+^P"(x)  +  j;P'»W+.~  (3 

on  using  158,  1. 

This,  as  the  reader  will  recognize,  is  Taylor's  development  of 
the  series  1)  about  the  point  x.  We  thus  have  the  theorem  : 

A  power  series  1)  may  be  developed  in  Taylor  s  series  3)  about 
any  point  x  within  its  interval  of  convergence.  It  is  valid  for  all  h 
such  that  x+  h  lies  within  the  interval  of  convergence  0/1). 

163.  1.  The  addition,  subtraction,  and  multiplication  of  power 
series  may  be  effected  at  once  by  the  principles  of  111,  11:2.  We 

have  if  P  =  a  +  a 


converge  in  a  common  interval  31  : 
P+  Q  =  (aQ  +  b())  +  (a1  +  b1)x 

P  -  Q  =  («o  -  Jo)  +  Oi  - 
P  '  Q  =  «0^o  +  (aibo  +  aob 
These  are  valid  within  SI,  and  the  first  two  in  31. 

2.    Let  us  now  consider  the  division  of  P  by  R.     Since 

£-P.I 
R  R 

the  problem  of  dividing  P  by  R  is  reduced  to  that  of  finding  the 
reciprocal  of  a  power  series. 

P  =  a       ax      a  •••  «   ^  0 


converge  absolutely  in  R  =(—  -#, 
§  =  ^2;  + 
fo  numerically  <  \  a0  1  m  33  =  (  —  r,  r)         r  <  R. 


GENERAL   THEORY  197 


Then  1/P  can  be  developed  in  a  power  series 
1 
P 

valid  in  53.      The  first  coefficient  CQ  =  — . 

ao 

For  1111 


p 


for  all  x  in  53.     We  have  now  only  to  apply  161,  1. 
3.    Suppose 


To  reduce  this  case  to  the  former,  we  remark  that 


Then  ±^\_      I 

P~  xm  '  Q' 

But  \/Q  has  been  treated  in  2. 

164.  1.  Although  the  reasoning  in  161  affords  us  a  method  of 
determining  the  coefficients  in  the  development  of  the  quotient  of 
two  power  series,  there  is  a  more  expeditious  method  applicable 
also  to  many  other  problems,  called  the  method  of  undetermined 
coefficients.  It  rests  on  the  hypothesis  that  /(#)  can  be  developed 
in  a  power  series  in  a  certain  interval  about  some  point,  let  us  say 
the  origin.  Having  assured  ourselves  on  this  head,  we  set 

f(x)  =  aQ  +  a^x  +  atf?  +  ••• 

where  the  a's  are  undetermined  coefficients.  We  seek  enough 
relations  between  the  a's  to  determine  as  many  of  them  as  we 
need.  The  spirit  of  the  method  will  be  readily  grasped  by  the 
aid  of  the  following  examples. 

Let  us  first  prove  the  following  theorem,  which  will  sometimes 
shorten  our  labor. 


198  POWER   SERIES 

2'    ^      f(x~)  =  a0  +  alx  +  a<ix2  +  •••;     -E<x<R,  (1 

is  an  even  function,  the  right-hand  t<ide  can  contain  only  even  powers 
of  x;  iff(x)  is  odd,  only  odd  powers  occur  on  the  right. 

For  if/  is  even,  /(»)  -/<-•).  (2 

But  f(-x)  =  a0-a1z+<V*-  ...  (3 

Subtracting  3)  from  1),  we  have  by  2) 

0  =  2(a1a;  +  a#?  +  a#?  +  ..-) 
for  all  x  near  the  origin.     Hence  by  160,  2 

«i  =  «8=«6=  ••'  =°- 
The  second  part  of  the  theorem  is  similarly  proved. 

165.    Example  1.  /(a-)  =  tan  a. 

Since  gin  3. 

tan  x  =  —   —  , 


cos  x 
and  ^ 


we  have  ^3      ^ 


Since  cos  x  >  0  in  any  interval  33  =  f  —  -  +  S,  —  —  S  j  ,  S  >  0,  it 
follows  that  |  §  |  <  1         in  33. 

Thus  by  163,  2,  tana;  can  be  developed  in  a  power  series  about 
the  origin  valid  in  $&.     We  thus  set 

tan  x  =  a^c.  +  fl^r3  +  a^  -f  •••  (2 


GENERAL   THEORY  199 

since  tana:  is  an  odd  function.      From  1),  2)  we  have,  clearing 
fractions, 


Comparing  coefficients  on  each  side  of  this  equation  gives 


-  '    a  - 

3     2!~       FT  3~3' 


a        a. 


r  Q  , 

a-  --  ^H  —  a  --  1=  --  .        /.«_ 
7      2!     4!      6!          7!  7      315 


1  17 

7! 


__  __.  __ 

9      2!4!      6!      8!      9!'  9      2835 

Thus  21 


(3 


•) 
Example  2. 


sin  x 
\ 


Since 


we  see  that  I  O  I  <  1 

when  2;  is  in  ^=(-7r  +  S,  TT-^),  3>0.  Thus  xf(x)  = 
can  be  developed  in  a  power  series  in  58.  As  f(x)  is  an  odd 
function,  xf(x}  is  even,  hence  its  development  contains  only  even 
powers  of  x.  Thus  we  have 

xf(x)  =  rt0  4-  a^  -}-  a±x*  H  ---- 


200  POWER   SERIES 

Hence 


a   -       +  -t  _     s  +  , 

3!5!      7I>  8      3!      5!      7!+9! 


Comparing  like  coefficients  gives 


q-| 

8 !      5 !      7  !  3  •  7 

Thus  111  7  QI 


sina;      a;      6         360          3-7! 
valid  in  (—  TT*,  TT*). 

166.    Let  J<>)  =/!(*)  +/.CO+  - 

/.(*)  =  «n0  +  «.i*  +  «n2^2  +  -         »  =  1,  2 
Let  the  adjoint  series 


(4 


converge  for  %  =  R  and  have  </>n  as  sums  for  this  value  of  f  . 


converge.  Then  ^  converges  uniformly  in  H  =  (—  ^2,  ^2)  and  F 
may  be  developed  as  a  power  series,  valid  in  21,  by  summing  by 
columns  the  double  series 


GENERAL   THEORY  201 

F  converges  uniformly  in  21.     For  as  \x\  <  f, 


4  «nl      +  «n2        +    —    =  <V 

We  now  apply  136,  2  as  2$n  is  convergent  for  %  =  R. 

To  prove  the  latter  part  of  the  theorem  we  observe  that 

«    4  «    R  4  « 


4 


is  convergent,  since  summing  it  by  rows  it  has  <E>  as  sum.  Thus 
the  double  series  1)  converges  absolutely  for  |z|<f,  by  123,  2. 
Thus  the  series  1)  may  be  summed  by  columns  by  130,  l  and  has 
F(x)  as  sum,  since  1)  has  F  as  sum  on  summing  by  rows. 

167.    Example. 


This  series  we  have  seen  converges  in  51  =  (0,  5),  b  positive  and 
arbitrarily  large. 

Since  it  is  impossible  to  develop  the  fn(x)  in  a  power  series  about 
the  origin  which  will  have  a  common  interval  of  convergence,  let 
us  develop  F  in  a  power  series  about  XQ  >  0. 

We  have 

1  1  1 

=  F~W  1 1  ~  ^l^a^  +  (14  o»O2  ~  '"  J 
where  A  (—!)"«"" 


202  POWER  SERIES 

Thus  F  give  rise  to  the  double  series 
D  =  A'  -  * 


where  ,,    _(— l)n   A 

An*  —  - A.n  K   . 


The  adjoint  series  to/n(a:)  is,  setting  f  =  [a  — a;0|, 

,       ^  ^2-P 


T  n  \.9  /  i  I    -j 

nl  \1  +  c 
This  is  convergent  if 

^   a   n    <  1     or  if 
that  is,  if  02 

For  any  x  such  that  #0<#<2#0     ,     £  =  2 
Then  for  such  an  x 

*"=;ni+a-(L  - 

and  the  corresponding  series 


is  evidently  convergent,  since  <£n  < 

7Z  1 

We  may  thus  sum  D  by  columns ;  we  get 


K=0 

where  0       ^r_l)n+K          an« 


The  relation  1)  is  valid  for  0  <  x  <  2  :r0. 


GENERAL  THEORY  203 

168.    Inversion  of  a  Power  Series. 

Let  the  series  »     .   7  .  .  T  ,2  .  si 

v  =  o0  +  b1t  +  If  4-  •  •-  (1 

have  6X  =£  0,  and  let  it  converge  for  t  =  tQ.     If  we  set 

t  =  xt0,      U=V7+  °* 

°ico 
it  goes  over  into  a  series  of  the  form 

u  =  x  —  a^x2  —  a33?  —  •••  (2 

which  converges  for  x  =  1.  Without  loss  of  generality  we  may 
suppose  that  the  original  series  1)  has  the  form  2)  and  converges 
for  x—  1.  We  shall  therefore  take  the  given  series  to  be  2).  By 
I,  437,  2  the  equation  2)  defines  uniquely  a  function  x  of  u  which 
is  continuous  about  the  point  u  =  0,  and  takes  on  the  value  x=  0, 
for  u  =  0. 

We  show  that  this  function  x  may  be  developed  in  a  power 
series  in  w,  valid  in  some  interval  about  u  =  0. 

To  this  end  let  us  set 

x  =  u  4-  c2u?  4-  c3ifi  4-  •••  (3 

and  try  to  determine  the  coefficient  <?,  so  that  3)  satisfies  2) 
formally.  Raising  3)  to  successive  powers,  we  get 

x2  =  u?  4-  2  c&*  4-  (*22  +'  2  <?3>4  +  (2  c±  +  2  <y3X  +  - 

a*  =  M3  +  3  ^4  +  (3  ^2  +  3  <gw5  +  ...  (4 

x^  =  u*  -f  4  £2w5  -f-  •  •  • 

Putting  these  in  2)  it  becomes 

u  =  u  +  (ea  -  <z2)w2  -f  (<?8  -  2  a2c2  -  a3)w3 
+  (*4  -  «2(^22  4-  2  c8)  -  3  «3^2  -  a4)w* 
+  (<?6  -  2  a2(c4  +  ^2^3)  -  3  a3(6-22  4-  <?8)  -  4  «4^2  -  a6)  w5     (5 
4- 

Equating  coefficients  of  like  powers  of  w  on  both  sides  of  this 

equation  gives 

c2  —  #2 

c3  =  2  a2e2  4-  «8 

^4  =  «2(^22  +  2  c8)  4-  3  a^  4-  «4  (6 

*    =  2  «^    +  CC      +  3  ^^2  +  *      +  4  ^^    +  «    • 


204  POWER   SERIES 

This  method  enables  us  thus  to  determine  the  coefficient  c  in 
3)  such  that  this  series  when  put  in  2)  formally  satisfies  this 
relation.  We  shall  call  the  series  3)  where  the  coefficients  c  have 
the  values  given  in  6),  the  inverse  series  belonging  to  2). 

Suppose  now  the  inverse  series  3)  converges  for  some  wo9bO; 
can  we  say  it  satisfies  2)  for  values  of  u  near  the  origin  ?  The 
answer  is,  Yes.  For  by  161,  3,  we  may  sum  by  columns  the 
double  series  which  results  by  replacing  in  the  right  side  of  2) 

r       rr2       <r& 

Ox,  ^/    ,  ^/    , 

by  their  values  in  3),  4).  But  when  we  do  this,  the  right  side  of 
2)  goes  over  into  the  right  side  of  5),  all  of  whose  coefficients 
=  0  by  6)  except  the  first. 

We  have  therefore  only  to  show  that  the  inverse  series  con 
verges  for  some  u  =£  0.  To  show  this  we  make  use  of  the  fact  that 
2)  converges  for  x  =  1.  Then  an  =  0,  and  hence 

|fln|<some«        ft  =  2,  3,...  (7 

On  the  other  hand,  the  relations  6)  show  that 

*n=/»(«2,  «8»—  *»)  (8 

is  a  polynomial  with  integral  positive  coefficients.  In  8)  let  us 
replace  #2,  az>"  by  a,  getting 

7»=/n(a»  «>  —  «)•  (9 

Obviously  |  cn  \  <  yn.  (10 

Let  us  now  replace  all  the  a's  in  2)  by  a  ;   we  get  the  geometric 

series  2^4  x-n 

u  =  x  —  ax?  —  ax3  —  ax*  —  ...  (11 


The  inverse  series  belonging  to  11)  is 

x  =  u  +  y2u2  +  73^3  +  74^4  H  —  (13 

where  obviously  the  y's  are  the  functions  9). 

We  show  now  that  11)  is  convergent  about  u  =  0.     For  let  us 
solve  12)  ;  we  get 


_  1  +  u  +  VI  -  2(2  q  + 


2(1 


GENERAL   THEORY  205 

Let    us    set    1  —  2(2  a  -f  l)w  •+-  u2  =  1  —  v.       For  u   near  u  =  0, 
<  1.     Then  by  the  Binomial  Theorem 


VI  -  v  =  1  +  d^v  +  d2v2  H  ---- 

Replacing  v  by  its  value  in  w,  this  becomes  a  power  series  in  u 
which  holds  for  u  near  the  origin,  by  161,  3.  Thus  14)  shows  that 
x  can  be  developed  in  a  power  series  about  the  origin.  Thus  13) 
converges  about  u  =  0.  But  then  by  10)  the  inverse  series  3) 
converges  in  some  interval  about  u  =  0. 

We  may,  therefore,  state  the  theorem  : 

Let  U==b  +  b1x  +  b2x*  +  b3x*  +  ...     ,     fl^O,  (15 

converge  about  the  point  x  =  0.      TJien  this  relation  defines  x  as  a 
function  of  u  which  admits  the  development 

x=(u-  5)(i  +al(u-b)  +  a2(u-b)*+  •••  } 
I  o\  j 

about  the  point  u  =  b.      The  coefficients  a  may  be  obtained  from  15) 
by  the  method  of  undetermined  coefficients. 

Example.     We  saw  that 

T2         r3         r4         ^5 

M  =  log(l  +  ^)  =  ^-|+|-|  +  |--  (1 

If  we  set 

u  =  x  +  tf2z2  +  asx3  +  a4z4  +  •••  (2 

we  have  l  l  i  _  i 

«2  =  -l       ,        rt3  =  l       ,        «4=-t        ,        «5=i" 

If  we  invert  2),  we  get 

x  =  u  -f-  ^2'w2  +  c>3  ^3  +  •  •  • 
where  c's  are  given  by  6)  in  168.     Thus 


-  ^=  -  Ki  +  2  •  D+3  •*•*-*  =  -  A-      •••  ^  =  A- 

-^=2(-i)(-2L  +  |.i)+3 

=  -120-  •*•    Co  =120' 


206  POWER   SERIES 

Thus  we  get 

*=M+S+S+£+£+ 

But  from  1)  we  have 

i+*='"=i  +  n+f^+- 

which  agrees  with  3). 


Taylor  s  Development 

169.    1.    We  have  seen,  I,  409,  that  if  f  (x)  together  with  its 
first  n  derivatives  are  continuous  in  21  =  (a  <  6),  then 


+  ^/""O  +  OK)  (1 

Where  a<a  +  A<6     ,     0<0<1. 

Consider  the  infinite  power  series  in  h. 

^=/(«)  +  /j/'(*)  +  f*/>)+  -  (2 

We  call  it  the   Taylor  s  series  belonging  to  f(x).     The  first  n 
terms  of  1)  and  2)  are  the  same.     Let  us  set 

JZ.=  ^/*0» 

IV     • 

We  observe  that  Rn  is  a  function  of  n,  7i,  a  and  an  unknown 
variable  0  lying  between  0  and  1. 

We  have  ...     ,   ,,       m    ,    r> 

/(a  -f  A)  =  rn  +  ^u. 

F"rom  this  we  conclude  at  once': 

• 
//"  1°,  f(x)  and  its  derivatives  of  every  order  are  continuous  in 

51  =  (a,  6),  and  2° 

limJRn  =  lim  -^/(B)(a+  ^A)  =  0     ,     n  =  ac,  (4 


TAYLOR'S   DEVELOPMENT  207 

Then  7  TO 

/(«  +  A)  =/(")  +  -/(«)+  |j/"O)  +    -  (5 

The  above  theorem  is  called  Taylor's  theorem;  and  the  equa 
tion  5)  is  the  development  of  f(x)  in  the  interval  51  by  Taylor's 
series. 

Another  form  of  5)  ?s 


/  O)  =/(«)  +      ZLo)  +   ^-/"(a)  +  ...  (6 

When  the  point  a  is  the  origin,  that  is,  when  a  =  0,  5)  or  6) 
gives  2 

/(*)  =/(°)  +  */'(<>)  +  fr/"(0)  +  -  (7 

This  is  called  Maclauriris  development  and  the  right  side  of  7) 
Maclaurirfs  series.  It  is  of  course  only  a  special  case  of  Taylor's 
development. 

2.    Let  us  note  the  content  of  Taylor's  Theorem.     It  says  : 
If   1°  f(x)    can  be  developed  in  this  form  in  the   interval 

2l  =  (a<&); 
2°  if  f(x)    and  all  its  derivatives  are  known  at   the   point 

x  =  a  ; 

then  the  value  of  /  and  all  its  derivatives  are  known  at  every 
point  x  within  51. 

The  remarkable  feature  about  this  result  is  that  the  2°  condi 
tion  requires  a  knowledge  of  the  values  of  f(x)  in  an  interval 
(a,  a  -h  S)  as  small  as  we  please.  Since  the  values  that  a  func 
tion  of  a  real  variable  takes  on  in  a  part  of  its  interval  as  (a  <  e), 
have  no  effect  011  the  values  thatjf(#)  may  have  in  the  rest  of  the 
interval  (c  <  6),  the  condition  1°  must  impose  a  condition  on  f(x) 

which  obtains  throughout  the  whole  interval  51- 

v 

170.  Let  f(x)  be  developable  in  a  power  series  about  the  point  a, 
viz.  let 


Then  ,(n) 

"n      ~n^         ?i  =  0,  1,  ...  (2 

i.e.  the  above  series  is  Taylor's  series. 


208  POWER   SERIES 

For  differentiating  1)  n  times,  we  get 

/»>(*)  =  »!«„  +  "±11  a^(x  -  a)  +  ... 
Setting  here  x=  a,  we  get  2). 

The  above  theorem  says  that  if  f(x)  can  be  developed  in  a 
power  series  about  x  =  a,  this  series  can  be  no  other  than  Taylor's 
series. 

171.  1.  Let  f(n\x)  exist  and  be  numerically  less  than  some  con 
stant  M  for  all  a  <  x  <  6,  and  for  every  n.  Then  f(x)  can  be 
developed  in  Taylor  s  series  for  all  x  in  (a,  5). 

For  then  I  7?   I       M  ''" 

n ! 

But  obviously  ^.      hn  _  ^ 

n=x>  n ! 

2.    The  application  of  the  preceding  theorem  gives  at  once : 


(3 


which  are  valid  for  every  x. 
SinCe 


we  have 

«*=l+*l°£«  +  *21^+...  (4 

valid  for  all  x  and  a  >  0. 


172.  1.  To  develop  (1  +  #)'x  awe?  log  (1  +  #)  we  need  another 
expression  of  the  remainder  72n  due  to  Cauchy.  We  shall  con 
duct  our  work  so  as  to  lead  to  a  very  general  form  for  Rn. 

From  169,  1  we  have 


TAYLOR'S   DEVELOPMENT  209 

We  introduce  the  auxiliary  function  defined  over  (a,  £>). 


KO  =AO  +/'  (00*  -0  + 
Then  </(*)=/(*) 

and 


Hence         .          «.=K*)-K«0.  •      (2 

(f  we  differentiate  1),  we  find  the  terms  cancel  in  pairs,  leaving 

-/no-  (3 


We  apply  now  Cauchy's  theorem,  I,  448,  introducing  another 
arbitrary  auxiliary  function  &(x)  which  satisfies  the  conditions 
of  that  theorem. 

Then  9(x)-g(a)  =  /(g),  a  <  c  <  x. 


Using  2)  and  3),  we  get,  since  x  =  a  +  A, 


where  0  <  ^  <  1. 

2.    If  we  set  (?<»  =  (6-*)", 

we  have  a  function  which  satisfies  our  conditions.     Then  4)  becomes 


a  formula  due  to  Schlomilch  and  Roche. 
For  /A  =  1,  this  becomes 

A-O-^ 

r>  —  1  . 
which  is  Cauchy's  formula. 


210  POWER   SERIES 

For  IJL  =  n,  we  get  from  5) 


n  l 

which  is  Lagrange's  formula  already  obtained. 

k 

173.    1.     We  consider  now  the  development  of 

(1  +  x)*         x  ^  —  1     ,     p  arbitrary. 
The  corresponding  Taylor's  series  is 


We  considered  this  series  in  99,  where  we  saw  that  : 
T  converges  for  |  x  \  <  1  and  diverges  for  |  x  \  >  1. 
When  x  =  1,   T  converges  only  when  /*>—!;   when  x  =  —  1^ 
^converges  only  when  ft^O. 

We  wish  to  know  when 


The  cases  when  T  diverges  are  to  be  thrown  out  at  once.  Con 
sider  in  succession  the  cases  that  T  converges.  We  have  to 
investigate  when  lim  Rn  =  0. 

Case  1°.  0<  |  x  \  <  1.  It  is  convenient  to  use  here  Cauchy's 
form  of  the  remainder.  This  gives 


1  .  2  •  ••• 


setting  ., 

_^.M-1  .  ...M-M  +  1 

*" 


hence  lim  TFn  =  0. 


TAYLOR'S  DEVELOPMENT  211 


x, 

which  is  finite.     Hence  Un  is  <  some  constant  M. 

To  show  that  Km  Sn  =  0,  we  make  use  of  the  fact  that  the  series 
T  converges  for  the  values  of  x  under  consideration.  Thus  for 
every  /* 

lim  J"M-l--M-n  +  2  ^  = 
1  •  2  -  ...  n—  1 

since  the  limit  of  the  nih  term  of  a  convergent  series  is  0.     In 
this  formula  replace  /-t  by  ^  —  1,  then 


1-2 n-l  fMx 

Hence  ,.      0       A 

hm  Sn  =  0. 

Thus  n .      D 

hm  Rn  =  0. 

Hence  1)  is  valid  for  |  x  j  <  1. 

Case  2.     x=  1,  IJL>—  1.     We  employ  here  Lagrange's  form  of 
the  remainder,  which  gives 

±1(1 +  *)*-» 


1.2-  ... 
setting 


TT      _ 


1.2.  ... 


Consider  Wn.     Since  /i  increases  without  limit,  fi  —  n  becomes 
and  remains  negative.     As  6  >  0 

lim  Wn  =  0. 
For  Z7B,  we  use  I,  143.     This  shows  at  once  that 

lim  Un  =  0. 

Hence  ,.      ,, 

hm  Rn  =  0 

and  1)  is  valid  in  this  case,  i.e.  for  x—  1,  /x  >—  1. 


212  POWER  SERIES 

Case  3.    x  =  —  1,  ft  ^>  0.     We  use  here  for  p  >  0  the  Schlomilch- 
Roche  form  of  the  remainder  172,  5) .     We  set  a  =  0,  h  =  —  1  and  get 


( _  ly/*-1  •  /*-2  •  .../x-rc+1 
>  l,2...-n-l 


Applying  I,  143,  we  see  that  lim  -Rn  =  0. 
Hence  1)  is  valid  here  if  p  >  0. 

When  /i  =  0  equation  1)  is  evidently  true,  since  both  sides 
reduce  to  1. 

Summing  up,  we  have  the  theorem : 

The  development  of  (1  +  x)^  in  Taylor's  series  is  valid  when 
|  x  |  <  1  for  all  /x.  When  x  =  -h  1  it  is  necessary  that  /a  >  —  1  ; 
when  x=  —  1  it  is  necessary  that  fJi^>0. 

2.  We  note  the  following  formulas  obtained  from  1),  setting 
x  =  1  and  —  1. 


174.    1.     We   develop   now   log  (1  +  #).      The    corresponding 
Taylor's  series  is 

*  +  1  ~~  2"  +  ¥  " 

We    saw,   89,  Ex.  2,  that    T7  converges  when  and  only  when 
\x\<\  or  x  =  1. 

Let  0  <  x  <  1.     We  use  Lagrange's  remainder,  which  gives  here 


= 
n 
Thus 


Hence  lim  Rn  =  0. 


TAYLOR'S   DEVELOPMENT  213 

Let  _  l  <  x  <  0.     We    use   here    Cauchy's   remainder,  which 
gives,  setting  x  =  —  £,  0  <  f  <  1, 


if 


Evidently 

Also 


Finally  1  —  0 

lim  TFn  =  0         since <  1. 

1  —  6% 

We  can  thus  sum  up  in  the  theorem  : 

Taylor  s  development  of  log  (1  -f  x)  is  valid  when  and  only  when 
x\  <  1  or  x  =  1.     That  is,  for  such  values  of  x 


2.    We  note  the  following  special  case  : 

i  -  *  +  \  -  \  +  -  =  log  2. 
The  series  on  the  left  we  have  already  met  with. 

175.    We  add  for  completeness  the  development  of  the  follow 
ing  functions  for  which  it  can  be  shown  that  lim  Rn  =  0. 


which  is  valid  for  (—1,  1). 

arctan  x  ==  x \-  —  —  —+...  (2 

which  is  valid  for  (—  1*,  1). 

1  a*      1 .  3  *•      1.3.52? 


which  is  valid  for  (—  1*,  1*). 


214  POWER   SERIES 

176.  We  wish  now  to  call  attention  to  various  false  notions 
which  are  prevalent  regarding  the  development  of  a  function  in 
Taylor's  series. 

Criticism  1.  It  is  commonly  supposed,  if  the  Taylor's  series  T 
belonging  to  a  function  /(#)  is  convergent,  that  then 

/(*)  =  T. 

That  this  is  not  always  true  we  proceed  to  illustrate  by  various 
examples. 

Example  1.     For  f(x)  take  Cauchy's  function,  I,  335, 

-i 

*•+!, 

(7  00=  lime'    n 

w=oo 

_JL 

Forz=£0         O(x)=e  x*      ;     for  x  =  0         (7(a;)=0. 
1°  derivative.     For  x  *  0,         C'(x)  =  -    C(x). 


For,  =  0, 

A=O 

2°  derivative,     x  *  0,         £"'(*)  =  (7  (a;)  (  4  ~  4  I  ' 

[x*>      x*  ) 

x  =  0,          <7"0)  =  lim  ^Wll_^i2)  =  lim  1  «"*'  =  0. 


3°  derivative,     x  *  0,         C"'  (x)  =  0  (x)  \  -^  -  ^  +  ^ 

Id;9       a:'        z5 

*  =  0,        C""(0)=lim-^jp=0. 

/TI  general  we  have  : 

#  ^=  0,          C(n)(x')  =  C  (x)  | h  terms  of  lower  degree  i 

I  x?  J 

Thus  the  corresponding  Taylor's  series  is 

<r  r* 

T  —  (7(0)  +  —  <7'(0)  +  —  (7"(0)  +  ••• 
1 !  2  ! 

=  0  +  0  -x+  0  -x*+  0  •  a^+  — 


TAYLOR'S   DEVELOPMENT  215 

That  is,  T  is  convergent  for  every  #,  but  vanishes  identically. 
It  is  thus  obvious  that  C (x)  cannot  be  developed  about  the  origin 
in  Taylor's  series. 

Example  2.  Because  the  Taylor's  series  about  the  origin  be 
longing  to  <7(#)  vanishes  identically,  the  reader  may  be  inclined 
to  regard  this  example  with  suspicion,  yet  without  reason. 

Let  us  consider  therefore  the  following  function, 

/<»  =  C(x)  +  >  .  G(x)  +  g(x). 

Then  f(x)  and  its  derivatives  of  every  order  are  continuous. 
Smce  /(n)(a;)  =  c<n)^  +  g<n)^ 

71  =  1,   2   ... 

and  =0 


we  have  „ 

Hence  Taylor's  development  for  f  (x)  about  the  origin  is 

This  series  is  convergent,  but  it  does  not  converge  to  the  right 
value  since  rp_  x 

-L  —  &   • 

177.  1.  Example  3.  The  two  preceding  examples  leave  noth 
ing  to  be  desired  from  the  standpoint  of  rigor  and  simplicity. 
They  involve,  however,  a  function,  namely,  (7(#),  which  is  not 
defined  in  the  usual  way;  it  is  therefore  interesting  to  have  ex 
amples  of  functions  defined  in  one  of  the  ordinary  everyday 
ways,  e.g.  as  infinite  series.  Such  examples  have  been  given  by 
Pringsheim. 

The  infinite  series 


defines,  as  we  saw,  155,  2,  a  function  in  the  interval  21  =  (0,  5), 
b  >0  but  otherwise  arbitrary,  which  has  derivatives  in  51  of  every 
order,  viz. : 

°     /•        -f  ~\n  nn\ 

;p       «  (2 


216  POWER   SERIES 

The  Taylor's  series  about  the  origin  for  F(x)  is 

T(x)  =  ^—F^^)     ;     Xl  =  lforX=0, 

A=0  X  • 

and  by  2) 


Hence 

(3 

As  £*>0  and  lim  ^=0,  £A+I<£A,  this  series  is  an  alternate  series 
for  any  x  in  51.     Hence  T  converges  in  51. 

2.  Readers  familiar  with  the  elements  of  the  theory  of  func 
tions  of  a  complex  variable  will  know  without  any  further  reason 
ing  that  our  Taylor's  series  T  given  in  3)  cannot  equal  the  given 
function  F  in  any  interval  51,  however  small  b  is  taken.     In  fact, 
F(x)  is  an  analytic  function  for  which  the  origin  is  an  essentially 

singular  point,  since  F  has  the  poles  --  -     n  =  1,  2,  3    •••,  whose 
limiting  point  is  0. 

3.  To  show  by  elementary  means  that  F(x)  cannot  be  devel 
oped  about  the  origin  in  a  Taylor's  series  is  not  so  simple.      We 
prove  now,  however,  with  Pringsheim  : 

If  we    take   a^fi±lY«4.68  •••,    T(x)    does  not  equal   F(x) 
\e  —  I/ 

throughout  any  interval  51  =  (0,  5),  however  small  b  >  0  is  taken. 

We  show  1°  that  if  F(x)  =  T(x)  throughout  51,  this  relation  is 
true  in  53  =  (0,  25*). 

In  fact  let  0<xQ<b. 

By  161,  4  we  can  develop  I7  about  #0,  getting  a  relation 

^0*0  =  i<7JC<>-3b)''  (1 

0 

valid  for  all  x  sufficiently  near  x9.     On  the  other  hand,  we  saw  in 

167  that 

F(x)  =  ^BK(x-x«Y  (2 

o 

is  also  valid  for  0<z<2#0.     But  by  hypothesis,  the  two  power 
series  1)  and  2)  are  equal  for  points  near  x9.     Hence  they  are 


TAYLOR'S   DEVELOPMENT  217 

equal  for  0<x<2x0.  As  we  can  take  XQ  as  near  b  as  we  choose, 
F=Tin  33. 

By  repeating  the  operation  often  enough,  we  can  show  that  F  = 
T  in  any  interval  (0,  B)  where  B  >  0  is  arbitrarily  large. 

To  prove  our  theorem  we  have  now  only  to  show  F=£  T  for 
some  one  x  >0. 

Since 

1  1     V  /I        1  11 


we  have  -.  -, 

,FO)>— L — L. 

1  +  x      l  +  ax 

On  the  other  hand 


Hence  T(x)<-- 

e 

To  find  a  value  of  x  for  which  Gr^-   take    x—  a~*.      For    this 
value  of  x 


Observe  that  Cr  considered  as  a  function  of  a  is  an  increasing 
function.     For  /e  _j_  -|\ 2  ^ 

"~  \e  -  lj  ~  e  ' 

Hence  F>  T  tor  x  >«-*. 

178.  Criticism  2.  It  is  commonly  thought  if  f(x)  and  its 
derivatives  of  every  order  are  continuous  in  an  interval  H,  that 
then  the  corresponding  Taylor's  series  is  convergent  in  31. 

That  this  is  not  always  so  is  shown  by  the  following  example, 
due  to  Pringsheim. 

It  is  easy  to  see  that 


converges  for  every  x _>0,  and  has  derivatives  of  every  order  for 
these  values  of  #,  viz. : 


218  POWER   SERIES 

Taylor's  series  about  the  origin  is 


The  series  T  is  divergent  for  x  >  0,  as  is  easily  seen. 

179.  Criticism  3.  It  is  commonly  thought  if  f(x)  and  all  its 
derivatives  vanish  for  a  certain  value  of  x,  say  for  x  =  a,  that 
then/(V)  vanishes  identically.  One  reasons  thus: 

The  development  of/(V)  about  x—  a  is 

/oo^/oo+^fiVoo  +  (a;r,a)2/"(a)+  - 


As  /and  all  its  derivatives  vanish  at  a,  this  gives 
f(x)  =  0  +  0  -  O  -  a)  +  0  .  (x  -  a)2  +  •  -  - 
=  0  whatever  x  is. 

There  are  two  tacit  assumptions  which  invalidate  this  conclusion. 

First,  one  assumes  because  /  and  all  its  derivatives  exist  and 
are  finite  at  x  =  a,  that  therefore  f(x)  can  be  developed  in 
Taylor's  series.  An  example  to  the  contrary  is  Cauchy's  function 
C(x).  We  have  seen  that  C(x)  and  all  its  derivatives  are  0  at 
x  =  0,  yet  0(x)  is  not  identically  0  ;  in  fact  (7  vanishes  only  once, 
viz.  at  x  =  0. 

Secondly,  suppose  f(x)  were  developable  in  Taylor's  series  in  a 
certain  interval  51  =  (a—  A,  a  +  h).  Then  /  is  indeed  0  through 
out  H,  but  we  cannot  infer  that  it  is  therefore  0  outside  H.  In 
fact,  from  Dirichlet's  definition  of  a  function,  the  values  that  /has 
in  51  nowise  interferes  with  our  giving  /  any  other  values  we 
please  outside  of  51. 

180.  1.  Criticism  4-  Suppose  f(x)  can  be  developed  in  Taylor's 
series  at  a,  so  that 


for          H  =(«<*). 


TAYLOR'S   DEVELOPMENT  219 

Since  Taylor's  series  I7  is  a  power  series,  it  converges  not  only 
in  H,  but  also  within  53  =  (2  a  —  b,  a).  It  is  commonly  supposed 
that  f(x)  =  T  also  in  53.  A  moment's  reflection  shows  such  an 
assumption  is  unjustified  without  further  conditions  on  f(x). 

2.  Example.  We  construct  a  function  by  the  method  considered 
in  I,  333,  viz. 


Then          f(x)  =  cos  z,         in  5i  =  (0,  1) 

=  1  +  sin  x,         within  53  =  (0,  -  1). 

We  have  therefore  as  a  development  in  Taylor's  series  valid 
in  91  ~2       ~4       ~6 

/(*)-i-f>+fi-f>  +...-* 

It  is  obviously  not  valid  within  53,  although  T  converges  in  53. 

3.    We  have  given  in  1)  an  arithmetical  expression  for/  (x). 
Our  example  would  have  been  just  as  conclusive  if  we  had  said  : 

Let  /(#)  =  cos  x         in  H, 

and  =  1  +  sin  #         within  53- 

181.    1.    Criticism  5.     The  following  error  is  sometimes  made. 
Suppose  Taylor's  development 


valid  in  51  =  (a  < 

It   may  happen    that    jT   is   convergent   in    a   larger   interval 


One  must  not  therefore  suppose  that  1)  is  also  valid  in  53. 
2.    Example. 

Let  f(x)=e*          in  51  =  (a,  5), 

and  =  e*  +  sin  (x  -  b)         in  SB  =  (6,  5). 

Then  Taylor's  development 


is  valid  for  51.     The  series  T  converging  for  every  x  converges  in 
53  but  1)  is  not  valid  for  53. 


220  POWER  SERIES 

182.  Let  f(x)  have  finite  derivatives  of  every  order  in 
$[  =  (#<  5).  In  order  that/(V)  can  be  developed  in  the  Taylor's 
series  7  2 

/(*)=/(«  +  *)=/(«) +  ¥'00  +  ^ /"(«)  +  -  (1 

valid  in  the  interval  51  we  saw  that  it  is  necessary  and  sufficient 


that 


lim  Rn  =  0. 


But  Rn  is  not  only  a  function  of  the  independent  variable  A,  but 
of  the  unknown  variable  6  which  lies  within  the  interval  (0,  1) 
and  is  a  function  of  n  and  h. 

Pringsheim  has  shown  how  the  above  condition  may  be  replaced 
by  the  following  one  in  which  6  is  an  independent  variable. 

For  the  relation  1)  to  be  valid  for  all  h  such  that  §<Ji  <  H,  it  is 
necessary  and  sufficient  that  Cauchy'sform  of  the  remainder 


the  h  and  0  being  independent  variables,  converge  uniformly  to  zero 
for  the  rectangle  D  whose  points  (h,  6)  satisfy 


1°     It  is  sufficient.     For  then  there  exists  for  each  e  >  0  an  m 

such  that 

|  Rn(h,  0)  |  <  e          n  5  m 

for  every  point  (A,  6)  of  D. 

Let  us  fix  h  ;  then    Rn  \  <  e  no  matter  how  6  varies  with  n. 

2°     It  is  necessary.     Let  hQ  be  ah  arbitrary  but  fixed  number  in 

H  =  (0,JJ*> 

We  have  only  to  show  that,  from  the  existence  of  1),  for  h<_hQ, 

it  follows  that 


uniformly  in  the  rectangle  Z>,  defined  by 


TAYLOR'S   DEVELOPMENT  221 

The  demonstration  depends  upon  the  fact  that  Rn(h,  0)  is  h 
times  the  wth  term  /„(«,  &)  of  the  development  of  f'(x)  about  the 
point  a  +  «.  In  fact  let  h  =  a  +  k.  Then  by  158 

/'(a  +  A)  =/'(<,  +  «  +  *)  =  /'(*  +  «)  +  .••+i^/^a  +  «)+--- 
whose  nth  term  is 


Let  «  =  #A,  then 

«.(A,«)=A/m(o,*) 

as  stated. 

The  image  A0,  of  _Z>0  is  the  half  of  a  square  of  side  A0,  below  the 
diagonal. 

To  show  that  Rn  converges  uniformly  to  0  in  DQ  we  have  only 

to  show  that  ^^  ^  ^  Q         uniformly  in  A0  .        (2 

To  this  end  we  have  from  1)  for  all  t  in  H 

/'  (a  +  0  =/'(«)  +  (TOO  +  £  /"'(«)+-  (3 

Its  adjoint 


/'(a)  |  +«;/»(«)  |  +  ••• 
also  converges  in  31. 

By  161,  4  we  can  develop  4)  about  t  =  «,  which  gives 


But  obviously  (r(«,  Ar)  is  continuous  in  A0,  and  evidently  all  its 
terms  are  also  continuous  there.     Therefore  by  149,  3, 

("~])(«)  =  0         uniformly  in  A0  .  (5 


n  —  1  ! 
But  if  we  show  that 

|/<»>(a  +  «)    <_&*-»  (a)  (6 

it    follows    from    5)    that     2)    is    true.     Our   theorem   is   then 
established. 


222  POWER  SERIES 

To  prove  6)  we  have  from  1) 

/(n) f f,    I     ~\ f(n)(n\  _l_  r/f  (w-f-l)/    \  _i 
\u    i    **/       J        V^y  T"  *~/  v^v  T 

and  from  4) 

The  comparison  of  7),  8)  proves  6). 

Circular  and  Hyperbolic  Functions 

183.  1.  We  have  defined  the  circular  functions  as  the  length 
of  certain  lines ;  from  this  definition  their  elementary  properties 
may  be  deduced  as  is  shown  in  trigonometry. 

From  this  geometric  definition  we  have  obtained  an  arithmeti 
cal  expression  for  these  functions.  In  particular 

=  F!~37  +  5]~f!  +  Q 

cosrr=l  —  —  +- —  +...  /.? 

2 !     4 !     6 !  l 

valid  for  every  x. 

As  an  interesting  and  instructive  exercise  in  the  use  of  series 
we  propose  now  to  develop  some  of  the  properties  of  these  func 
tions  purely  from  their  definition  as  infinite  series.  Let  us  call 
these  series  respectively  8  and  O. 

Let  us  also  define  tan  x  =  sm  x ,  sec  x  =  — - ,  etc. 

cos  x  cos  x 

2.  To  begin,  we  observe  that  both  #and  C  converge  absolutely 
for  every  x,  as  we  have  seen.  They  therefore  define  continuous 
one-valued  functions  for  every  x.  Let  us  designate  them  by  the 
usual  symbols  . 


We  could  just  as  well  denote  them  by  any  other  symbols,  as 

4>O)     ,     *(*). 
3.    Since 


n     ^         £ 
,          (7=1         forz  =  0, 

we  have  .    ft      A 

smO  =  0     ,     cos  0  =  1. 


CIRCULAR   AND   HYPERBOLIC   FUNCTIONS  223 

4.  Since  S  involves  only  odd  powers  of  x,  and    C  only  even 
powers, 

sin  x  is  an  odd,         cos  x  is  an  even  function. 

5.  Since  S  and  C  are  power  series  which  converge  for  every  x, 
they  have  derivatives  of  every  order.     In  particular 


dC  =_z,??__3?_,&__  _  c  f 

dx"      18!     5!     7! 

Hence  dsinx  dcoxx 

—  =  cos  x    ,  —  =  —  sin  #.  (3 


6.    To  get  the  addition  theorem,  let  an  index  as  x,  y  attached  to 
S,  C  indicate  the  variable  which  occurs  in  the  series.     Then 


__         _ 

7!5!2!8!4!       6!  ) 


7!      o!2!      314! 
Adding, 


1 


=  x  +  y    _  (a;  +  y  )3      (^  +  5)5 
"      1!  3!  5! 


Thus  for  every  x,  y 

sin  (a;  -f-  y)  =  sin  #  cos  y  -f-  cos  #  sin  y  . 
In  the  same  way  we  find  the  addition  formula  for  cos  x. 


224  POWER   SERIES 

7.    We  can  get  now  the  important  relation 

sin2  x  -h  cos2  x  =  1  (4 

directly  from  the  addition  theorem.     Let  us,  however,  find  it  by 
aid  of  the  series.     We  have 


11     11 

+  +  + 


11  11  11 

l  +  6!2!+4!4!+6!2!+8! 


Hence 


Now  by  I,  96, 

Thus  £2         O2  =  ^2  x        cofc2  x  =  1 

8.  In  2  we  saw  sin  #,  cos  2;  were  continuous  for  x\  4)  shows 
that  they  are  limited  and  indeed  that  they  lie  between  ±  1. 

For  the  left  side  of  4)  is  the  sum  of  two  positive  numbers  and 
thus  neither  can  be  greater  than  the  right  side.  • 

9.  Let  us  study  the  graph  of  sin  #,  cos  #,  which  we  shall  call  2 
and  F,  respectively. 

Since  sin  x  =  0,  — s'n  x  =  cos  x  =  1,  for  x  =  0,  2  cuts  the  #-axis  at 
ax 

0  under  an  angle  of  45  degrees. 


CIRCULAR   AND   HYPERBOLIC   FUNCTIONS  225 

Similarly  we  see  y  —  1  for  x  =  0.     F  crosses  the  #-axis  there 
and  is  parallel  to  the  #-axis. 


and  each  parenthesis  is  positive  for  0  <  x2<  6, 

sin.r>0          for  0<:r<Vti=  2.449  ... 
Since 


,_  l  __  l 

21^4!^ 

T  1  7  p     O  O  Ck 

cosa:>0        for  0<*<  V2  =  1.414  «• 

Since 


cosa;<0         for  x  =  2. 

Since  Dx  cos  a:  =  —  sin  #  and  sin  x  >  0  for  0  <  x  <  V6,  we  see 
cos  x  is  a  decreasing  function  for  these  values  of  x.  As  it  is  con 
tinuous  and  >  0  for  x  =  V2,  but  <  0  for  x  =  2,  cos  x  vanishes  once 
and  only  once  in  (V2,  2). 

This  root,  uniquely  determined,  of  cos  x  we  denote  by  -  •  As  a 
first  approximation,  we  have 


From  4)  we  have  sin2  ?=  !•     As  we  saw  sin#>0  for  x<  V6, 
we  have 


Thus  sin  x  increases  constantly  from  0  to  1  while  cos  x  decreases 
from  1  to  0  in  the  interval  (  0,  ^  )=  Ir     We  thus  know  how  sin  #, 
cos  x  behave  in  Ir 
From  the  addition  theorem 

sin  (  ~  +  x  )  =  sin  ^  cos  x  +  cos  ^  sin  x  =  cos  z. 

\<A  /  2  J 

-|-  a;=  cos     cos  a:  —  sin     sin  a;  =  —  sin  a:. 


226  POWER  SERIES 

Knowing  how  sin#,  cosx  march  in  7j,  these  formulae  tell  us 
how  they  march  in  J2  =  (-,  77-). 

From  the  addition  theorem, 

sin  (TT  +  x)  =  —  sin  x,          cos  (TT  +  x)  =  —  cos  x. 

Knowing  how  sin  x,  cos  x  march  in  (0,  TT),  these  formulae  inform 
us  about  their  march  in  (0,  2  TT). 
The  addition  theorem  now  gives 

sin  (x  +  2  TT)  =  sin  x,         cos  (x  +  2  TT)  =  cos  x. 

Thus  the  functions  sin  ar,  cos  #  are  periodic  and  have  2  TT  as  period. 

The  graph  of   sin  x  cos  x  for  negative  x   is   obtained    now  by 
recalling  that  sin  x  is  odd  and  cos  x  is  even. 

10.    As  a  first  approximation  of  TT  we  found 

V2  <  |  <  2. 
By  the  aid  of  the  development  given  159,  3 

=  *-!  +    i-+-  5) 


we  can  compute  TT  as  accurately  as  we  please. 

In  fact,  from  the  addition  theorem  we  deduce  readily 

n4==vl     '        >S4=vl' 

Hence  TT 

tan  — =  1. 

This  in  5)  gives  Leibnitz  s  formula, 

4  =    '  ~  3  +  5  ~  7  +  ' 

The  convergence  of  this  series  is  extremely  slow.  In  fact  by 
81,  3  we  see  that  the  error  committed  in  stopping  the  summation 

at  the  nth  term  is  not  greater  than  — ' — .  How  much  less  the 
error  is,  is  not  stated.  Thus  to  be  sure  of  making  an  error  less 
than  — —  it  would  be  necessary  to  take  |  (10W  +  2)  terms. 


CIRCULAR  AND   HYPERBOLIC  FUNCTIONS  227 

11.    To  get  a  more  rapid  means  of  computation,   we  make   use 
of  the  addition  theorem. 

To  start  with,  let  , 

a  =  arctg  £. 

Then  5)  gives  1^11^11      11 

~5      35S  +  555      757  ^ 
a  rapidl}7  converging  series. 

The  error  Ea  committed  in  breaking  off  the  summation  at  the 
wth  term  is  .,  _, 


By  virtue  of  the  formula  for  duplicating  the  argument 

0  2  tan  « 

tan  2  a  =  —  -     —  —, 
1  — 


wehave 

Similarly          .  tan  4  «  =  if-o. 

Let 

^  =  4«-|.  (7 

The  addition  theorem  gives 

tan  4  a  -  1         1 


tan  13 


1  +  tan  4  «      239 ' 


Then  5)  gives  111         11 

r)  |     -I  xo 

~~  289     3239*     5289* 

also  a  very  rapidly  converging  series. 

We  find  for  the  error 


"2w-12392"-i' 

The  formula  7)  in  connection  with  6)  and  8)  gives  - .     The 
error  on  breaking  off  the  summation  with  the  wth  term  is 


228  POWER   SERIES 

184.  The  Hyperbolic  Functions.  Closely  related  with  the  cir 
cular  functions  are  the  hyperbolic  functions.  These  are  defined 
by  the  equations 


£>X      I      a  -  X 

cosh  x  =  -      '  -  -  (2 


tanh  x  = 


2 
sinh  x      ex  —  e~x 


cosh  a;      ex  +  e~x 


sech  x  =  — : —     ,     cosech  x- 


cosh  x  sinh  x 

Since  „ 


we  have  ,         , 

=  _+|j+|I+...  .  .  (3 

=l  +  g  +  i£  +  ...  -'.  (4 

valid  for  every  x.     From  these  equations  we  see  at  once  : 
sinh  (  —  x)  =  —  sinh  x     ;     cosh  (  —  x)  =  cosh  x. 
sinh  0  =  0.  coshO=  1. 

-—  sinh  a;  =1+  —  +  ^7+   —  =  cosh  x.  (5 

dx  214! 


Let  us  now  look  at  the  graph  of  these  functions.  Since  sinh  #, 
cosh  x  are  continuous  functions,  their  graph  is  a  continuous  curve. 
For  x  >  0,  sinh  x  >  0  since  each  term  in  3)  is  >  0.  The  relation 
4)  shows  that  cosh  x  is  positive  for  every  x. 

If  x'  >  x  >  0,  sinh  x'  >  sinh  #,  since  each  term  in  3)  is  greater 
for  x'  than  for  x.  The  same  may  be  seen  from  5). 


THE   HYPERGEOMETRIC   FUNCTION  229 

Evidently  from  3),  4) 

lim  sinh  x  =  +  oo      ,     lim  cosh  x  =  +  oo  . 

X=+30  X=+X> 

At  x  =  0,  cosh  2:  has  a  minimum,  and  sinh  x  cuts  the  2>axis 
at  45°. 

For  x  >  0,  cosh  x  >  sinh  #  since 


The  two  curves  approach  each  other  asymptotically  as  x  =  -hoc  . 

For  the  difference  of  their  ordinates  is  e~x  which  =  0  as  x  =  +  oo  . 

The  addition  theorem  is  easily  obtained  from  that  of  ex.    In  fact 

.   ,  ,  e*  —  e~x 

sinh  x  cosh  y  =  -  -  -- 

-)imi  ar  y 


=      ^y—  ex~v  +  e~x+v  —  e~x~v). 
Hence 

sinh  x  cosh  y  +  cosh  2:  sinh  y  =  \(ex^v  —  e~(x+y))  =  sinh  (x  + 
Similarly  we  find 

cosh  (2:  +  ?/)  =  cosh  a:  cosh  ?/  +  sinh  x  sinh  y. 
In  the  same  way  we  may  show  that 

cosh2  x  —  sinh2  x  =  1. 


Hyper  geometric  Function 

185.  This  function,  although  known  to  "Wallis,  Euler,  and  the 
earlier  mathematicians,  was  first  studied  in  detail  by  Gauss.  It 
may  be  defined  by  the  following  power  series  in  x: 


- 


The  numbers  a,  /3,  7  are  called  parameters.  We  observe  that 
a,  (B  enter  symmetrically,  also  when  a.  =  1,  ft  =  7  it  reduces  to 
the  geometric  series.  Finally  let  us  note  that  7  cannot  be  zero  or 
a  negative  integer,  for  then  all  the  denominators  after  a  certain 
term  =  0. 


230  POWER  SERIES 

The  convergence  of  the  series  F  was  discussed  in  100.  The 
main  result  obtained  there  is  that  F  converges  absolutely  for  all 
|  x  |  <  1,  whatever  values  the  parameters  have,  excepting  of  course 
7  a  negative  integer  or  zero. 

186.  For  special  values  of  the  parameters,  F  reduces  to  ele 
mentary  functions  in  the  following  cases  : 

1.  If  a  or  /?  is  a  negative  integer  —  n,  F  is  a  polynomial  of 
degree  n. 

2.  ^(1,1,  2;  -x)=      log  (1  +  rc).  (1 


Also 


The  relation  1)  is  now  obvious. 
Similarly  we  have 


,l,  2;  *)  =  —  log  (I-*)- 


4.  s-FC},  -|-,  |,  a:2)  =  arcsin  x. 

5.  2^(1>  1»  f  »  —  ^2)  =  arc  tan  ^. 

6.  Km  jpf  «,  1,  1,  -}  =  e*.  (2 

a=+oo        \  Ct/ 

For 


•  2  •  1  •  2 


t     t*  -  t*     j     •»-       i*     i     *       •         -  /I        I 

~1 . 2  .  3      "  1 .2-8W  " 


THE   HYPERGEOMETRIC   FUNCTION  231 

Let  0  <  Gr  <  0.     Then 


is  convergent  since  its  argument  is  numerically  <  1.  Comparing 
3),  4)  we  see  each  term  of  3)  is  numerically  <  the  corresponding 
term  of  4)  for  any  \x  <  G-  and  any  a  >  0.  Thus  the  series  3) 
considered  as  a  function  of  a  is  uniformly  convergent  in  the 
interval  (/3  +  co  )  by  136,  2  ;  and  hereby  x  may  have  any  value 
in  (—  G,  G-).  Applying  now  146,  4  to  3)  and  letting  a=  +  00, 
we  see  3)  goes  over  into  2). 

7.  lim  xF(  «,«,-;  -  —  -  ]  =  sin  x.  (5 

a=+»         \  A  4  arj 

For 


Let  x  =  G-  >  0  and  a  =  a.     Then 


is  convergent  by  185.     We  may  now  reason  as  in  6. 
8.    Similarly  we  may  show  : 

/  "I  2     \ 

lim  F(  «,  a,  -  ;  -  -—5]  =  cos  x. 

a=+oo        \  2  4  «2/ 

lim  El  a,  «,  1  ,  —  -  )  =  sinh  x. 
a=+oo     \          2    4  a2/ 

lim  F(a,  «,  -,  T—  i)  =  cosh  ^. 

a=+30     V         2    4«V 

187.    Contiguous  Functions.     Consider  two  F  functions 
-F(a,&7;   x)     ,     JT(«f,  /3',  7'  ;   *). 

If  a  differs  from  a!,  by  unity,  these  two  functions  are  said  to  be 
contiguous.  The  same  holds  for  0,  and  also  for  7.  Thus  to 
F  (afiyx)  correspond  6  contiguous  functions, 

-F(a±l,£±l,  7±1;  x). 


232  POWER   SERIES 

Between  F  and  two  of  its  contiguous  functions  exists  a  linear 
relation.     As  the  number  of  such  pairs  of  contiguous  functions  is 

6-5,, 
172-  L5' 

there  are  15    such   linear   relations.     Let  us  find  one   of   them. 

We  set  4- 1  •  a  -I-  2       •  a  4-     — 1    S    R  4-1         fl  4-     —  9 

1  •  2  •  •  •  •  ft  •  7  •  7  4- 1  •  •••74-71— 1 

Then  the  coefficient  of  xn  in  F(a.@vx}  is 
in  F(a  +  1,  ft  7,  x)  it  is 
in  ^(«,  ft  7  —  1,  x)  it  is 


I  n 

, 

Thus  the  coefficient  of  #n  in 

(7  _  «  _  1)^(«,  ft  7,  x)  +  a.F(a  +  1,  ft  7,  z) 

+  (l-7)JF(a,  ft  7-1, 
is  0.     This  being  true  for  each  n,  we  have 

(7  _  «  _  1)  Jf  (a,  ft  7,  z)  +  «JP  (a  +  1,  ft  7,  x) 

a,  ft  7-1,  aO= 


Again,  the  coefficient  of  a;n  in  JP(a,  /3  —  1,  7,  a;)  is  «(/3  — 
in  a?^(a  -f-  1,  ft  7,  a;)  it  is  71(7  +  w  —  1)  §n. 
Hence  using  the  above  coefficients,  we  get 

«,  ft  7,  »)  +  «(1  -  a;)F(a  +  1,  ft  7,  ») 


From  these  two  we  get  others  by  elimination  or  by  permuting 
the  first  two  parameters,  which  last  does  not  alter  the  value  of 
the  function 


Thus  permuting  «,  ft  in  1)  gives 

(7  -  £  -  1)^(«,  ft  %  s)  +ft*T(«1  £  +  1,  7,  s) 

ft  7  ~  1,  *0  =  0.      (3 


THE   HYPERGEOMETRIC   FUNCTION  233 

Eliminating  F  '(<*,  /3,  7—  1,  x)  from  1),  3)  gives 

(£-a)jF(«,  &  7,  a-)  +  «.F(a  +  l,  &  7,  z) 

-  AF(a,  £  +  1,  7,  a:)  =  0.       (4 
Permuting  a,  /9  in  2)  gives 

OX-  *-  /3)^(«,  £,  7,  *)  +  £(1  -  x)F(a,  0  +  1,  7,  *0 

a-l,  £,  7,2r)  =  0.      (5 


From  3),  5)  let  us  eliminate  jP(«,  /S  +  1,  7,  a;),  getting 
(«  _  1  _  (7  _  ff  _  1»^(>,  A  7,  a;)  +  (7  -  «)JP(«  -  1,  A  7,  a;) 

+  (l_7)(l_aOJFT(«,  /3,  7-l,af)=0.      (6 
In  1)  let  us  replace  a  by  a  —  1  and  7  by  7  +  1  ;   we  get 

(7  -  a  +  1)^(«  -  1,  &  7  +  1*  *)  +  O  -  1)^(«'  A  7  +  1,  a) 

_7^(«-l,  A  7,  x)=Q.  (a) 

In  6)  let  us  replace  7  by  7  +  1  ;   we  get 


/3,7,  aO  =  0.     (b) 

Subtracting  (b)  from  (a),  eliminates  F(^a  —  1,  /8,  7  +  1,  a;)  and 
gives 

7(1  -  aO^O/^z)  -  7^(«  -  1,  A  7,  a;) 

+  (7  -  /8)^(«,  A  7  +  1,  *)  =  0.      (7 
From  6),  7)  we  can  eliminate  F(a—  1,  /?,  7,  z),  getting 
7!7-l+C«H-/8+l-27>SJF(«,  A  7,3;) 

+  (7  -  «)(7  -  P)zF(a,  /3,  7  +  1.  *0 
+  7(1  -  7)(1  -  aO^Ca,  A  7  -  1,«)  =  0.     (8 
In  this  manner  we  may  proceed,  getting  the  remaining  seven. 

188.  Conjugate  Functions.  From  the  relations  between  con 
tiguous  functions  we  see  that  a  linear  relation  exists  between  any 
three  functions 


whose  corresponding  parameters  differ  only  by  integers.     Such 
functions  are  called  conjugate. 


234  POWER  SERIES 

For  let  jo,  q,  r  be  any  three  integers.     Consider  the  functions 
JF(a#y30,         JF(«  +  1,  ft  7,  x)  •••  F(a+p,  ft  7,  x), 

+  2>  7,  *)  •'•  ^ 


We  have  jt?  +  q  +  r  +  1  functions,  and  any  3  consecutive  ones 
are  contiguous.  There  are  thus  p  +  q  -f  r  —  1  linear  relations 
between  them.  We  can  thus  by  elimination  get  a  linear  relation 
between  any  three  of  these  functions. 

189.    Derivatives.     We  have 


1.2.  ... 


~~r~   ^^  /„   _i     1  \  '  i  ~,n 

==  X     V       "l         7  — -i ?» — ~~  -i -i — 

=  ^JF(a  +  l,  /3+1,  7  +  1,  x~). 

7 
Hence 

7^//  /^..      Q     ,        _N  a  '   P    Til  S~     i     1       /Oil       .  .     i     1       ^,\ 


^ 

7  •  7 

and  so  on  for  the  higher  derivatives.     We  see  they  are  conjugate 
functions. 

190.  Differential  Equation  for  F.  Since  F,  F1  ,  F"  are  conju 
gate  functions,  a  linear  relation  exists  between  them.  It  is  found 
to  be 


+  {(«  +  13  4-  l)z  -  7}  ^'  +  «/3^=  0.  (1 

To  prove  the  relation  let  us  find  the  coefficient  of  xn  on  the  left 
side  of  1).     We  set 

p  _«•«  +  !•  —  «  +  n-l-£-ff  +  l-—  ff  +  ro-l_ 

~~ 


THE   HYPERGEOMETRIC   FUNCTION  235 

The  coefficient  of  xn  in  x2F"  is 

n(n-l)PB, 
in  —  xF"  it  is 


7+n 
in  (a  +  £  +  l)a;jF'  it  is 

w«  +      + 
in  —  7.F'  it  is 

in  a/3P  it  is 

Adding  all  these  gives  the  coefficient  of  xn  in  the  left  side  of  1). 
We  find  it  is  0. 

191.    Expression  of  F(a/3yx')  as  an  Integral. 
We  show  that  for  |  x  \  <  1, 

B(fri-P)-F(ap<ix)=    fV-^l  -uy-P-id-xu^-'du   (1 

«^o 

where  ^(jt?,  ^)  is  the  Beta  function  of  I,  692, 

B(p,  q)  =   f  nr-i(l  -  u)«-ldu. 
For  by  the  Binomial  Theorem 

N  -,         .a  ,«•«+!         •«.«»«4-l«« 

(1  -  zw)-*  =  1  +  -  xu  +  -y-  1-  A2  +  -      1.2.3 
for  |  xu  \  <  1.     Hence 

,7 


7  -  /?)  +  ^5(/3  +  1,  7  ~  ^) 

2,7-/3)+...  (2 


236  POWER  SERIES 

Now  from  I,  692,  10) 

Hence 


7+1  ry   .    ry  _|_ 

etc.     Putting  these  values  in  2)  we  get  1). 

192.     Value  of  F  (a,  £,  7,  x)  for  x  =  I. 

We  saw  that  the  F  series  converges  absolutely  for  x  =  1  if 
a  +  P  —  7  <  0.  The  value  of  F  when  x  =  1  is  particularly  in 
teresting.  As  it  is  now  a  function  of  a,  &  7  only,  we  may  denote 
it  by  .F(«,  /3,  7).  The  relation  between  this  function  and  the  T 
function  may  be  established,  as  Gauss  showed,  by  means  of  187,  8) 

viz  * 

7!7-l+O  +  /3  +  l-27)zJ  F(afax) 

+  (7  -  «)  (7  -  &)xF(a,  #7  +  1,  x) 

7(1  ~  7)  (1  -  *0^(«,  /3,  7  -  1,  *)  =  0.        (1 


Assuming  that  n  A 

«  +  £  -  7  <  0,  (2 

we  see  that  the  first  and  second  terms  are  convergent  for  x  =  1  ; 
but  we  cannot  say  this  in  general  for  the  third,  as  it  is  necessary 
for  this  that  a  +  /3  —  (7  —  1)  <  0.  We  can,  however,  show  that 

L  lim  (1  -  x)  JF(«,  /?,  7  -  1,  x)  =  0,  (3 

supposing  2)  to  hold.     For  if    x\  <  1, 

^(«,  &  7  -  1»  *)  =  «0  +  V  +  a2z2  +  ...  (4 

Now  by  100,  this  series  also  converges  for  x  =  —  1.     Thus 

lim  an  =  0.  (5 

n=  oo 

From  4)  we  have 

£,  7  -  1,  «)  =  «0  +  O    -  «)^  +  («    -  ^)^  +  •" 


Let  the  series  on  the  right  be  denoted  by  6r(».  As 
6?n+1(l)  =  an,  we  see  6r(l)  is  a  convergent  series,  by  5),  whose 
sum  is  0.  But  then  by  147,  6,  Cr(x)  is  continuous  at  x  =  1. 

Hence  ilirn  6^jc 


THE   HYPERGEOMETRIC   FUNCTION  237 

and  this  establishes  3).     Thus  passing  to  the  limit  x  =  1  in  1) 
gives 

7  O  +  /3  -  7)  F(«,  &  7)  +  (7  -  «)  (7  -  £)-F(«,  /3,  7  +  1)  =  0, 


*(«,  A  7)  = 


7(7  -  a- 
Replacing  7  by  7  +  1,  this  gives 


etc.     Thus  in  general 
7)  = 


-.?(«,&  7  +  »)• 

Gauss  sets  now 

71    !    71^ 

;  >5  I}  =  («+!)(*  +  2)  ...(*  +  »)' 
Hence  the  above  relation  becomes 
jfro  )  =  n(>i.y-l-)n(n.7-«-ff-l)  J(      p  }      (g 

n(w,7-«-i)n(w,7-/3-i) 

N°W 


lira  J(«,  A  7  +  »)  =  1.  (7 

7l  =  OC 

For  the  series 

)=l+          +  IL±±l+..  (8 


converges  absolutely  when  2)  holds.     Hence 

'!*"'+1| 


In  n      o      n     n    \    1 

•   Cr  1  •  1  -   Or  •  Or  +  1 

is  convergent.  Now  each  term  in  8)  is  numerically  <  the  corre 
sponding  term  in  9)  for  any  7  >  6r.  Hence  8)  converges  uni 
formly  about  the  point  7  =  -f  oc.  We  may  therefore  apply  146,  4. 
As  each  term  of  8)  has  the  limit  0  as  7  =  +  oc,  the  relation  7) 
is  established. 


238  POWER  SERIES 

We  shall  show  in  the  next  chapter  that 

lim  II  (n,  x) 

n=oo 

exists  for  all  x  different  from  a  negative  integer.     Gauss  denotes 
it  by  II  (x)  ;  as  we  shall  see, 

rO)  =  n<>-l)     ,     fora>0. 
Letting  n  =  GO,  6)  gives 

*(«,  A  7)  =  n  c-y  -  i)n(7  -«-  0-1) 

n(y-«-l)n(7-/3-l) 
We  must  of  course  suppose  that 

7,          7  -  «,          7  -  &          7  -  a  -  £, 

are  not  negative  integers  or  zero,  as  otherwise  the  corresponding 
II  or  F  function  are  not  defined. 

Bessel  Functions 
193.    1.    The  infinite  series 


converges  for  every  x.     For  the  ratio  of  two  successive  terms  of 
the  adjoint  series  is  \x  2 


which  =  0  as  s  =  GO  for  any  given  x. 

The  series  1)  thus  define  functions  of  x  which  are  everywhere 
continuous.     They  are  called  Bessel  functions  of  order 

n=0,  1,  2  ... 
In  particular  we  have 

^oW  =  *  - 7772  +  2271^  ~  22 .  42  •  62  +  '"  ^ 

j  (x\  =  %_     x8  x5 tf_ sn 

2      22  •  4      22  •  42  •  6      22  •  42  •  62  •  8 

Since  1)  is  a  power  series,  we  may  differentiate  it  termwise  and 
' _  V  (-lV( 


BESSEL  FUNCTIONS  239 

2.    The  following  linear  relation  exists  between  three  consecutive 
Bessel  functions  : 


For     ,.  xn~l       .1.  sr-iv          afr+n~1  rr 

71-1         -'-  ;     »+*-1-  ' 


Hence 


—  1  «  ,~2a+n—  1   ( 

4-2C—  IV-  _  |  _ 

-l!       iv       y  2«+2*-M8:- 


3.    We  show  next  that 

2^2(8!)  =  «/_!(*)  -J-.+1(*)        «>0.  (8 

For  subtracting  7)  from  6)  gives 


From  8)  we  get,  on  replacing  Jn+1  by  its  value  as  given  by  5)  : 
Ji(x)  =  -  Vn(»  +  ^(2:),         TI  >  0.  (9 

X 

From  5)  we  also  get 

«£(*)=•  -Jr,,co-«W*)      w>°-  (10 

X 

4.    The  Bessel  function  Jn  satisfies  the  following  linear  homo 
geneous  differential  equation  of  the  2°  order  : 

n  =  o.  (ii 


240  POWER   SERIES 

This  may  be  shown  by  direct  differentiation  of  1)  or  more  sim 
ply  thus  :    Differentiating  9)  gives 


,.  (12 

X  X 

Equation  10)  gives 


Replacing  here  Jn_^  by  its  value  as  given  by  9),  we  get 


Putting  this  in  12)  gives  11). 


5.  e*-2~  =  ^unJn(x)  (13 

—  00 

for  any  #,  and  for  u  =£  0. 
For 


e      2     =  e      e 


(1  _i_ xu  j_    ^u* 
1   "T  +  ^TTi 


Now  for  any  x  and  for  any  u  =£  0,  the  series  in  the  braces  are 
absolutely  convergent.  Their  product  may  therefore  be  written 
in  the  form  '  ^  (x*  1  \ 

22     \2y  2!  2!       'V 


3  !  2 ! V2 


Jx  _  j^ 

V2      r\ 


( 


BESSEL  FUNCTIONS  241 

194.    1.    Expression  of  Jn(x}  as  an  Integral. 

'         (X  COS 


Hence  -r,    ,  _  -,  x  g 

cos  (a;  cos  <£)  =  ]T  ^-  —  ^  a^*  cos2*  </> 

o     (-s)- 
and  thus 

CC  X-  -J     N    8 

cos  (a:  cos  </>)  sin2n  ^  =  V  ^  ~    ^  2^«  cos2*  (^  sin2n  </>. 

o     (^  s)  • 

As  this  series  converges  uniformly  in  (0,  TT)  for  any  value  of  re, 
we  may  integrate  termwise,  getting 

j[cos  (a?  cos  </>)  sin2"  <j>d<t>  =  ^  ^~  1)f*  <&  j'cos2'  (/>  sin2" 


o    (2«)I 
We  shall  show  in  225,  6,  that 


r(l£±l).l.8.5....8.-lv5: 


Thus  the  last  series  above 


9 

0 

Thus 

™n 


2     ) 


CHAPTER   VII 
INFINITE    PRODUCTS 

195.  1.  Let  {a^... tj  be  an  infinite  sequence  of  numbers,  the 
indices  i  =  (t1-..t8)  ranging  over  a  lattice  system  £  in  s-way 

space.     The  symbol       p  —T\  -  TT  (1 

=  gatl ...,,_  ^ 

is  called  an  infinite  product.  The  numbers  at  are  its  factors.  Let 
PM  denote  the  product  of  all  the  factors  in  the  rectangular  cell 

**     "  '  lirnP,  (2 

is  finite  or  definitely  infinite,  we  call  it  the  value  of  P.  It  is 
customary  to  represent  a  product  and  its  value  by  the  same  letter 
when  no  ambiguity  will  arise. 

When  the  limit  2)  is  finite  and  =£  0  or  when  one  of  the  factors 
=  0,  we  say  P  is  convergent,  otherwise  P  is  divergent. 

We  shall  denote  by  P^  the  product  obtained  by  setting  all  the 
factors  a,  =  1,  whose  indices  t  lie  in  the  cell  R^.  We  call  this  the 
co-product  of  PM. 

The  products  most  often  occurring  in  practice  are  of  the  type 

P  =  a1-a2.aB.  •••  =  TLan.  (3 

The  factor  P^  is  here  replaced  by 

and  the  co-product  PM  by 

•*   m  ==  &m+l  '  ^m+2  "  ^wi+3  " 

Another  type  is  +00 

P=Han.  .        (4 

The  products  3),  4)  are  simple,  the  product  1)  is  s-tuple.  The 
products  3),  4)  may  be  called  one-way  and  tivo-way  simple  products 
when  necessary  to  distinguish  them. 

242 


GENERAL   THEORY  243 


p  —  i  .  1  .  2  .  3  .  4.  .     .  . 
*      *1      2      3      ¥      6 

Obviously  the  product  P  =  0,  as 

p.  =  I  =  o. 

/i 

Hence  P  =  0,  although  no  factor  is  zero.  Such  products  are 
called  zero  products.  Now  we  saw  in  I,  77  that  the  product  of  a 
finite  number  of  factors  cannot  vanish  unless  one  of  its  factors 
vanishes.  For  this  reason  zero  products  hold  an  exceptional  posi 
tion  and  will  not  be  considered  in  this  work.  We  therefore  have 
classed  them  among  the  divergent  products.  In  the  following 
theorems  relative  to  convergence,  we  shall  suppose,  for  simplicity, 
that  there  are  no  zero  factors. 

196.  1.    For  P  =  Tlatl...lt  to  converge  it  is  necessary  that  each  PM 
is  convergent.     If  one  of  these  PM  converges,  P  is  convergent  and 

P  —  P    •  P 

M   —  -*•  fj.    -*•  fj.  • 

The  proof  is  obvious. 

2.  If  the  simple  product  P  =  al  •  «2  •  a3  >••  is  convergent,  its  fac 
tors  finally  remain  positive. 

For,  when  P  is  convergent,  Pn  j  >  some  positive  number,  for 
n  >  some  m.  If  now  the  factors  after  am  were  not  all  positive,  Pn 
and  Pv  could  have  opposite  signs  v>n,  however  large  n  is  taken. 
Thus  Pn  has  no  limit. 

197.  1.   To  investigate  the  convergence   or  divergence    of   an 
infinite  product  P  =  Ila^...,,  when  at  >  0,  it  is  often  convenient  to 
consider  the  series 


called  the  associate  logarithmic  series.     Its  importance  in  this  con 
nection  is  due  to  the  following  theorem  : 

The  infinite  product  P  with  positive  factors  and  the  infinite  series 
L  converge  or  diverge  simultaneously.  When  convergent,  P  =  eL, 
L  =  log  P. 

For  logPM  =  £M,  (1 

P,  =  *V  (2 


244  INFINITE   PRODUCTS 

If  P  is  convergent,  P^  converges  to  a  finite  limit  =£  0.  Hence 
L^  is  convergent  by  1).  If  L^  is  convergent,  P^  converges  to  a 
finite  limit  =?t  0  by  2). 

2.    Example  1. 

p  =  n  (  i  +  -  V  »  =  nan      7i  =  i,  2,  ... 
\     »/ 

is  convergent  for  every  x. 

For,  however  large  |  x  \  is  taken  and  then  fixed,  we  can  take  m 
so  large  that 


n>m. 
n 


Instead  of  P  we  may  therefore  consider  Pm. 

Then 

But  by  I,  413 


Hence  Lm  =  2^  Mnz?  •  — 

m+\  %« 

which  is  convergent. 

The  product  P  occurs  in  the  expression  of  sin  x  as  an  infinite 
product. 

Let  us  now  consider  the  product 


Q  =  nf  1  +  -}e  n         n  =  ±  1,  ±  2, 
V        n) 


The  associate  logarithmic  series  L  is  a  two-way  simple  series. 
We  may  break  it  into  two  parts  U,  L",  the  first  extended  over 
positive  ft,  the  second  over  negative  n.  We  may  now  reason  on 
these  as  we  did  on  the  series  3),  and  conclude  that  Q  converges 
for  every  x. 

3.    Example  2. 


n 
is  convergent  for  any  x  different  from 

0,  -  1,  -  2,  -  3, 


GENERAL   THEORY  245 

For  let  p  be  taken  so  large  that  \x\  <  p.     We  show  that  the 
co-product 


converges  for  this  2;.     The  corresponding  logarithmic  series  is 

QO 

L  =  Z,  I  x  logf  1  +  1)  -  logf  1  +  ^  1 
j>+i  I  V        n/  V        »/  J 


As  each  of  the  series  on  the  right  converges,  so  does  L.  Hence 
Gr  converges  for  this  value  of  x. 

198.    1.    When  the  associate  logarithmic  series 

Zr=21ogatl...lf     ,     aL>0 
is  convergent,          Um  log  ^  _    _  Oj         b    121>  ^ 

|t|=QO 

and  therefore  -,. 

limati...ls  =  l. 

|l|=00 

For  this  reason  it  is  often  convenient  to  write  the  factors 
ati...l4  of  an  infinite  product  P  in  the  form  1  +  6tl...tj.  When  P  is 
written  in  the  form 

p  =  n(i  +  ^...ts), 

we  shall  say  it  is  written  in  its  normal  form.     The  series 

2J,,..,,  =  2J. 

we  shall  call  the  associate  normal  series  of  P. 
2.    The  infinite  product 


z'^s  associate  normal  series 


converge  or  diverge  simultaneously. 


246  INFINITE   PRODUCTS 

For  P  and  £  =  2  log  (1  +  «.) 

converge  or  diverge  simultaneously  by  197.     But  A  and  L  con 
verge  or  diverge  simultaneously  by  123,  4. 

3.    If  the  simple  product  P  —  al  -  a2  •  a3  •••  is  convergent,  an=l. 

For  by  196,  2  the  factors  an  finally  become  >  0,  say  for  n  >  m. 
Hence  by  197,  l  the  series 

oo 

2  log  an         an  >  0 

n=m 

is  convergent.    -Hence  log  an  =  0.     .-.  an  =  1. 

199.    Let  R^  <  R^  <  •  ••  X  |  =  oo  be  a  sequence  of  rectangular 

cells.      Then  if  P  is  convergent, 


For  P  is  a  telescopic  series  and 


200.     1.    Let     P 

We  call  (?=n(l  +  all...l8       ,     «t  =    «4 

the  adjoint  of  P,  and  write 

¥  =  Adj  P. 
2.    P  converges,  if  its  adjoint  is  convergent.      We  show  that 

€  >  0,      X,  \Pp-Pv\<€  p,V>\. 

Since  $  is  convergent, 


is  also  convergent  by  199.     Hence 

0<^,-(ipM<€         \<n<v. 

But  Pv  —  PM  is  an  integral   rational  function  of  the  a's   with 
positive  coefficients.     Hence 

IP,  -.p.  i  <*,-$,•  ci 


GENERAL   THEORY  247 

3.  When  the  adjoint  of  P  converges,  we  say  P  is  absolutely 
convergent. 

The  reader  will  note  that  absolute  convergence  of  infinite 
products  is  defined  quite  differently  from  that  of  infinite 
series.  At  first  sight  one  would  incline  to  define  the  adjoint  of 

P  =  Hatl...  18 

to  be  «i  __  jj  I  a        I 

With  this  definition  the  fundamental  theorem  2  would  be  false. 
For  let  P=n(-l)»; 

its  adjoint  would  be,  by  this  definition, 

Now  $n  =  1.  .*.  $  is  convergent.  On  the  other  hand, 
_Pn=(—  l)n  and  this  has  no  limit,  as  n=cc.  Hence  P  is 
divergent. 

4.  In    order    that    P=  TI(1  +  atl...ls)    converge    absolutely,  it  is 
necessary  and  sufficient  that       ^ 

converges  absolutely. 

Follows  at  once  from  198,  2. 
Example.  /        ^ 

nd--. 


converges  absolutely  for  every  x. 

For  y*2.  avl 

^  n2          *~  n2 
is  convergent. 

201.    1.    Making  use  of  the  reasoning  similar  to  that  employed 
in  124,  we  see  that  with  each  multiple  product 

are  associated  an  infinite  number  of  simple  products 
and  conversely. 


248  INFINITE   PRODUCTS 

We  have  now  the  following  theorems  : 

2.  If  an  associate  simple  product  Q  is  convergent,  so  is  P,  and 
P=Q. 

For  since  Q  is  convergent,  we  may  assume  that  all  the  a's  are 
>  0  by  196,  2.  Then 


_  g2  log  CV  i.  by   124,   3, 

=  P          by  197,  1. 

3.    If  the  associate  simple  product   Q  is  absolutely  convergent,  so 
is  P. 

Forlet 


Since  Q  is  absolutely  convergent, 


is  convergent.     Hence  11(1  +  atl...t  )  is  convergent  by  2. 

4.  Let  P=  H(l  H-  «it...i  )  fo  absolutely  convergent.      Then  each 
associate  simple  product  Q=  11(1  +  #n)  ^s  absolutely  convergent  and 

p=<?. 

For  since  P  is  absolutely  convergent, 

2«^...^ 

converges  by  200,  4.     But  then  by  124,  5 

2«n 
is  convergent.     Hence  Q  is  absolutely  convergent. 

5.  If  P=  natl...lg  is  absolutely  convergent,  the  factors  flj.-i,  >0 
^y  ^Aei/  ^'g  outside  of  some  rectangular  cell  R^. 

For  since  P  converges  absolutely,  any  one  of  its  simple  associ 
ate  products  Q=llan  converges.  But  then  an>Q  for  n>m,  by 
198,  3.  Thus  a(i...t  >  0  if  i  lies  outside  of  some  R^. 

6.  From  5  it  follows  that  in  demonstrations  regarding  abso 
lutely   convergent  products,  we  may  take   all   the    factors  >  0, 
without  loss  of  generality. 


GENERAL   THEORY  249 


For 


and  all  the  factors  of  PM  are  >  0,  if  JJL  is  sufficiently  large.     This 
we  shall  feel  at  liberty  to  do,  without  further  remark. 

T.  4  =11(1  +  *,,...„)         «t>0 


converge  or  diverge  simultaneously. 

For  if  A  is  convergent, 

2a,,..... 

is  convergent  by  200,  4.     But  then  L  is  convergent  by  123,  4. 
The  converse  follows  similarly. 

202.     1.    As   in    124,  10  we  may  form   from  a   given   m-  tuple 
product  A=Ua 

l  '     m 

as  infinite  number  of  conjugate  w-tuple  products 

*-™*~t. 

where  a,  =  bj  if  i  andy  are  corresponding  lattice  points  in  the  two 
systems. 

We  have  now  : 

2.    If  A  is  absolutely  convergent,  so  is  B,  and  A  —  B. 
For  by  201,  6,  without  loss  of  generality,  we  may  take  all  the 
factors  >  0. 

Then  sioga... 


=  B. 

3.    Let  A-\\a 

A  -  llah...lwi 

be  an  absolutely  convergent  m-tuple  product. 


be  any  p-tuple  product  formed  of  a  part  of  or  all  the  factors  of  A. 
Then  B  is  absolutely  convergent. 


250  INFINITE   PRODUCTS 

For  2  log  a,  is  convergent. 

Hence  2  log  fy  is. 

Arithmetical  Operations 

203.    Absolutely  convergent  products  are  commutative,  and  con 
versely. 

For  let  ,        ,  , 

^.  =  IK...lm 

be  absolutely  convergent.     Then  its  associate  simple  product 

2l=Han 

is  absolutely  convergent  and  A  =  51,  by  201,  4.  Let  us  now  re 
arrange  the  factors  of  A,  getting  the  product  B.  To  it  corre 
sponds  a  simple  associate  series  23  and  B  =  $8.  But  21  =  23  since 
51  is  absolutely  convergent.  Hence  A  =  B. 

Conversely,  let  A  be  commutative.     Then  all  the  factors  atl..., 
finally  become  >  0.     For  if  not,  let 

E1<E2<  ...  =00  (1 

be  a  sequence  of  rectangular  cells  such  that  any  point  of  9?m  lies 
in  some  cell.  We  may  arrange  the  factors  a,  such  that  the  partial 
products  corresponding  to  1), 

1       '       ^2       '  3  "" 

have  opposite  signs  alternately.  Then  A  is  not  convergent,  which 
is  a  contradiction.  We  may  therefore  assume  all  the  a's  >  0. 

Then  A         2iogat...t 

*a.  —  e  m 

remains  unaltered  however  the  factors  on  the  left  are  rearranged. 

Hence  v  n 

21og<v..lwt 

is  commutative  and  therefore  absolutely  convergent  by  124,  8. 
Hence  the  associate  simple  series 

«  =  2  log  a,  =  2  log  (1  +  6.) 

is  absolutely  convergent  by  124,  5.     Hence 


is  convergent  and  therefore  A  is  absolutely  convergent. 


ARITHMETICAL  OPERATIONS  251 

204.    1.    Let  A  =  u 

ll       lt 

be  absolutely  convergent.      Then  the  s-tuple  iterated  product 


is  absolutely  convergent  and  A  =  B  where  i\  •-  ij  is  a  permutation  of 
ir  ia  •••  i,. 

For  by  202,  3  all  the  products  of  the  type 
Ha  UaL 

Vl«  li"-'« 

i«-ii«  i« 

are  absolutely  convergent,  and  by  I,  324 

n  =  nn. 

»«-i»«  i«-i  i« 

Similarly  the  products  of  the  type 

n 

'«-ll«-2t«-S 

are  absolutely  convergent  and  hence 

n=  n   n   n. 


In  this  way  we  continue  till  we  reach  A  and  B. 
2.    We  may  obviously  generalize  1  as  follows  : 

Let  A-IK-- 

5e  absolutely  convergent.  Let  us  establish  a  1  to  1  correspondence 
between  the  lattice  system  £  oi'er  which  i  =  (ix  —  O  ranges,  and  the 
lattice  system  9)1  over  which 


ranges.      Then  the  p-tuple  iterated  product 
B  =  tt  •  n  -  ...  Ila.  , 

1          2  r      ;n>n" 

2*s  absolutely  convergent,  and 


252  INFINITE   PRODUCTS 

3.    An  important  special  case  of  2  is  the  following: 
Let  A  =  Tlan     ,     w=l,2,... 

converge  absolutely.     Let  us  throw  the  an  into  the  rectangular  array 

an     ,     ala... 

^21       '        ^22  *'* 


converge  absolutely,  and 


4.    7%e  convergent  infinite  product 


associative. 

Forlet  '""«!<  OT2<-..=  oo. 

•L^et  -i   i   z.       /"i   i   —  \       /^i   i 


We  have  to  show  that 

<?=(i+ 

is  convergent  and  P  =  Q. 

This,  however,  is  obvious.     For 


=  P,,  v  =  ml+  ...  +wn. 

But  when  n  =  oo  so  does  v. 
Hence  ;  lim(?n  =  limPn. 

Remark.     We  note  that  mm+1  —  mm  may  =  oo  with  n. 


ARITHMETICAL   OPERATIONS  253 

205.    Let  A  =  IIati...t.     ,     B  =  Tlb^...^ 

be  convergent.      Then 

C=UaL-bt    ,     D=U^ 
ft. 

are  convergent  and 

C=A.B  ,   D  =  4 

B 

Moreover  if  A,  B  are  absolutely  convergent,  so  are  <?,  D. 

Let  us  prove  the  theorem  regarding  (7;  the  rest  follows  simi 

larly.     We  have  n  D 

Cjt  =  ^cL^  •  .o^. 

Now  by  hypothesis  A^  =  A,  B^  =  B  as  p  =  oo. 

Hence  C,  =  A.B. 

To  show  that  O  is  absolutely  convergent  when  A,  B  are,  let  us 
write  a,  =  1  +  at     ,     5t  =  1  +  bt       and  set  |  at  |  =  «t     ,      bt  |  =  ft. 
Since  A,  B  converge  absolutely, 


+  O     ,     2  log  (1  +  &) 
are  convergent.     Hence 

2  {log  (1  +  <*)  +  log  (1  +  #)  i  =  2  log  (1  +  «t)  (1  +  &) 

is   absolutely  convergent.       Hence    C  is    absolutely    convergent 
by  201,  7. 

206.    Example.     The    following  infinite  products  occur  in  the 
theory  of  elliptic  functions  : 


<?2  =  n  (i  +  j2"-1) 
§3  =n  (i-j2-1). 

They  are  absolutely  convergent  for  all  |  q\  <  1. 
For  the  series  ^^     ^     ^\qZn~l\ 

are  convergent.     We  apply  now  200,  4. 

As  an  exercise  let  us  prove  the  important  relation 

P  =   <?,<?2<?3  =  1- 


254  INFINITE   PRODUCTS 

For  by  205,  p  =  n  (1  +  ?2n)(l  4-  fn~l)(l  -  q2n~l 


Now  all  integers  of  the  type  2  w,  are  of  the  type  4^  —  2  or  4 
Hence  by  204,  3, 

n  (i  -  0a»)  =  n  (i  -  ?4n)  n  (i  -  ^-2), 


Thus  p^n 

=  1 


Uniform   Convergence 
207.    Jn  ^Ae  limited  or  unlimited  domain  51,  let 


uniformly  convergent  and  limited.      Then 


^8  uniformly  convergent  in  H. 

For  L 

J^A  =  eLx- 

Now  LK  =  L  uniformly.     Hence  by  144,  1,  F  is  uniformly  con 
vergent. 

208.    If  the  adjoint  of 


is  uniformly  convergent  in   51  (finite  or  infinite),  F  is  uniformly 
convergent. 

For  if  the  adjoint  product, 


is  uniformly  convergent,  we  have 

|^-^|<e 
for  any  x  in  51- 


UNIFORM   CONVERGENCE  255 

But  as  already  noticed  in  200,  2,  1) 

I  P  —  P  I  <     $  —  %  I 

I    •*    M  -*    v    I    —          rV  Fr  |« 

Hence  .F  is  uniformly  convergent. 
209.     The  product 


uniformly  convergent  in  the  limited  or  unlimited  domain  51,  if 

*  =  2*.,  .....Ov..<0    ,    *.=  !/,! 

limited  and  uniformly  convergent  in  51. 
For  by  138,  2  the  series 


is  uniformly  convergent  and  limited   in   51-     Then   by  207,  the 
adjoint  of  F  is  uniformly  convergent,  and  hence  by  208,  F  is. 

210.  Let  -p,  A      TT  r 

**(*,  —  O  =  n/H  ...t.(*i  ...  rrm) 

fo  uniformly  convergent  at  x  =  a.     //  eaeA  /t  t*  continuous  at  a,  F 
is  also  continuous  at  a. 

This  is  a  corollary  of  147,  1. 

211.  1.    Let  G  =  S  |  /^...^(X  •••  zw)  |  converge    in    the     limited 
complete  domain  51  having  a  as  a  limiting  point.     Let  Gr  and  each 
/t  be  continuous  at  a.      Then 


is  continuous  at  a. 

For  by  149,  4,  Gr  is  uniformly  convergent.     Then  by  209,  F  is 
uniformly  convergent,  and  therefore  by  210,  F  is  continuous. 

2.    Let  Gr  =2  l/i^-i.C*?!  •••  #m)  |  converge  in  the  limited  complete 
domain  51,  having  x  =  a  as  limiting  point.     Let 

lim/c=at     ,     lira  G  =  2at. 
lira 


256  INFINITE   PRODUCTS 

For  by  149,  5,  6r  is  uniformly  convergent  at  x  =  a.     It  is  also 
limited  near  x—  a.     Thus  by  209, 


is  uniformly  convergent  at  a.     To  establish  1)  we  need  now  only 
to  apply  146,  l. 


212.     1.    Let  F=TlfLi...,a(x)     ,    />0  (1 

converge  in  51=  (a,  a  +  8).     Then 

logJ=i  =  21og/..  (2 

If  we  can  differentiate  this  series  termwise  in  51  we  have 

Thus  to  each  infinite  product  1)  of  this  kind  corresponds  an  infi 
nite  series  3).  Conditions  for  termwise  differentiation  of  the  series 
2)  are  given  in  153,  155,  156.  Other  conditions  will  be  given  in 
Chapter  XVI. 

2.    Example.     Let  us  consider  the  infinite  product 

0(x)  =2q*Q  sin  7nzfl(l  -  2  q2n  cos  2  TTX  +  q*n)  (1 


which  occurs  in  the  elliptic  functions. 

Let  us  set 

1  -  un  =  1  -  2  <fn  cos  2  TTX  +  (fn. 

Then  \un\<2\q\*n+\q\*n. 

Thus  if  |  q  \  <  1,  the  product  1)  is  absolutely  convergent  for  any  x. 
It  is  uniformly  convergent  for  any  x  and  for  |  q  \  <  r<  1. 

If  it  is  permissible  to  differentiate  termwise  the  series  obtained 
by  taking  the  logarithm  of  both  sides  of  1),  we  get 


0(x)  ^1  —  2  (fn  COS  2  7TX  +  <?4" 

If  we  denote  the  terms  under  the  2  sign  in  2)  by  vn  we  have 


THE   CIRCULAR   FUNCTIONS 


257 


Now  the  series  2an  converges  if    q  \  <  1.     For  setting  bn=  \  <?2n|, 
the  series  25ra  is  convergent  in  this  case.     Moreover, 

lira  £»  =  1. 

7i-=oo    0  ^ 

H 

Thus  we  may  differentiate  termwise. 


The  Circular  Functions 
213.     1.    Sin  z  and  cos  x  as  Infinite  Products. 
From  the  addition  theorem 

sin  (nix  -f  x)  =  sin  (m  -f  1)  a:  =  sin  raz  cos  2:  4-  cos  mx  sin  2: 
m  =  1,  2,  3  •••  we  see  that  for  an  odd  n 

sin  rcz  =  a0  sinn  z  +  a1  sin""1  a?  +  •••  4-  «n-i  sin  x 
where  the  coefficients  a  are  integers.      If  we  set  t  =  sin  x,  we  get 

sin  nx  =  Fn(t)  =  aQtn  +  a^  +  .  .  .  +  «n_^.  (1 

Now  J"n  being  a  polynomial  of  degree  n,  it  has  n  roots.     They  are 
0,      ±sin^      ±sin^,     ...  isini^, 


n 


n 


corresponding  to  the  values  of  x  which  make  sin  nx  =  0.     Thus 


t*  -  sin2  -    •  •  .    i*  -  sin*    - 
»         \  n 


Dividing  through  by 


sin  -  sin 
n  n 


.  n 

sin2 


n  —     TT 


n 


and  denoting  the  new  constant  factor  by  a,  1),  2)  give 


sin  nx  =  a  sin  x 


I  _ 


sin2  x 


77 

sm*  — 
n 


!1  Il2 


..l*i ss!*   1 

.     97l  —  1  7T 

S1"^-2j 


258 


INFINITE   PRODUCTS 


To  find  a  we  observe  that  this  equation  gives 
sin  nx 


sin  x 


I".,       sin2  x 
a    1 

.     27T 

snr  — 
n_ 


Letting  x  =  0  we  now  get  a  =  n.     Thus  putting  this  value  of  a. 

y 
in  3),  and  replacing  x  by  -,  we  have  finally 


sin  x  =  n  sin  -  P  (x,  n) 


where 


1 

sin2-" 
n 

r       1     °    .  ,.  U 

•     2T7r 

n  - 

•  ~            2 

We  note  now  that  as  n  =  oo, 


Similarly 


x 

sin  - 
.    #  n  . 

n  sin  -  =  x =  x. 

n  x 

n 


sm  "         ^ 
n    .     x* 


It  seems  likely  therefore  that  if  we  pass  to  the  limit  n  =  oo  in 
4),  we  shall  get  gin  x  _  xp^  (5 

where  P(  ^  —  \ 

The  correctness  of  5)  is  easily  shown. 
Let  us  set 


L  (x,  n)  =  log  P  (x,  ri)  =  2  log 


1- 


n 


,'r.2 


sn 


=  log  P(x)  =  2  log    l  - 


THE   CIRCULAR  FUNCTIONS 
We  observe  that 

lim  P  (x,  ri)  =  lim  e**> n)  =  e™  =  P  (x) 


259 


provided 


lim  L(x,  ti)  =  L(x). 


We  have  thus  only  to  prove  7).  Let  us  denote  the  sum  of  the 
first_w  terms  in  6)  by  Ln(x,  n)  and  the  sum  of  the  remaining 
byZm(z,  rc).  Then 


|ZO,M)-£O)|< 

Since  for 


we  have 


(8 


-  <  sin  x  <  x, 


sin2- 


n       4  n2         x2 


n         n 


and  hence  for  an  m1  so  large  that  -  -  <  1,  we  have, 


-log 
But  the  series 


1- 


sin2- 
n 

I'TT 


sin2 


n  _ 


r  >  m. 


is  convergent.     Hence  for  a  sufficiently  large  m 


mx,n<-    ,          m*<- 

Now  giving  m  this  fixed  value,  obviously  for  all  n  >  some  v  the 
first  term  on  the  right  of  8)  is  <  e/3,  and  thus  7)  holds. 


260  INFINITE   PRODUCTS 

2.    In  algebra  we  learn  that  every  polynomial 

«0  +  a^x  +  a2z2  +  ...  +  anxn 
can  be  written  as  a  product 

««O  -  «i)0*  -  «2)  •••  O  -  «„), 
where  a    «    ""  are  ^s  r°°ts.     Now 


is  the  limit  of  a  polynomial,  viz.  the  first  n  terms  of  9).  It  is 
natural  to  ask,  Can  we  not  express  sin  x  as  the  limit  of  a  product 
which  vanishes  at  the  zeros  of  sin  x  ?  That  this  can  be  done  we 
have  just  shown  in  1. 

3.    If  we  set  x  =  TT/%  in  5),  it  gives, 


2"V        4r*J      2  2r.2r 

Hence     TT      ,,  2r.2r  2- 2. 4- 4- 6- 6- 


2/9  ,».        1  \/9  «  _|_  1  \        1      Q      Q      e      c      7        * 
c  ^  /  —  j.  )  i  ^  /  "f"  x)      A*O*O*O*O*  i  ... 

a  formula  due  to  Wallis. 

4.    From  5)  we  can  get  another  expression  for  sin  z,  viz.  : 

sin  x  =  #11(1 — —}ern         r=±l,  ±2,  •••  (11 

V        rirj 

For  the  right  side  is  convergent  by  197,  2.     If  now  we  group 
the  factors  in  pairs,  we  have 


rvr, 
This  shows  that  the  products  in  5)  and  11)  are  equal. 

5.    From  5)  or  11)  we  have 

sin  x  =  lim  Pn(x)  =  lim  x  IT'  x+87r  (12 

n=oo  s=-n       87T 

where  the  dash  indicates  that  s  =  0  is  excluded. 


\ 

THE   CIRCULAR  FUNCTIONS  261 

214.     We  now  show  that 

coss  =  nfi-       4a;      V  (i 


To  this  end  we  use  the  relation 

sin  2  x  ==  2  sin  x  cos  x. 
Hence 


n?r 
2 


(2«-i) 


from  which  1)  is  immediate. 
From  1)  we  have,  as  in  213,  4, 


cos  x  =  ul  -       n,1)g'         n  =  0,  ±1,  ±2,  ...     (2 

215.    From  the  expression  of   sin  #,  cos  x  as  infinite  products, 
their  periodicity  is  readily  shown.     Thus  from  213,  12) 

sina:  =  lim  Pn(x). 


Hence 

or  •   >          N  • 

sin  (a:  -f  TT)  =  —  sin  a:. 

Hence  sin(x  +  2  TT)  =  sin  x 


and  thus  sin  a;  admits  the  period  2  TT. 

216.    1.    Infinite  Series  for  tana:,  cosec  #,  e^c. 

If  0<a;<7r,  all  the  factors  in  the  product  213,  5)  are  positive. 

TllUS    log  sin  x  =  log  x  +     log    l-  ,    0<a:<7r.  (1 


262  INFINITE  PRODUCTS 

Similarly  214,  1)  gives 


log  cos.  =    log    l-2      ,     0<,<.  (2 


To  get  formulae  having  a  wider  range  we  have  only  to  square 
the  products  213,  5)  and  214,  1).     We  then  get 

log  sin2  z  =  log  z2  +  2  log  (l  -  -f^-Y,  (3 

i          \ 


valid  for  any  x  such  that  sin  x  =£  0  ;  and 

A   ^,2  \  2 

l-^-M^),  (4 

valid  for  any  x  such  that  cosx=£  0. 
If  we  differentiate  3),  4)  we  get 

.  9- 

(5 

(6 


, 
j  a;2  —  «  V 

* 


'c?  «s  iw  3),  4). 

Remark.  The  relations  5),  6)  exhibit  cot  x,  tan  x  as  a  series  of 
rational  functions  whose  poles  are  precisely  the  poles  of  the  given 
functions.  They  are  analogous  to  the  representation  in  algebra 
of  a  fraction  as  the  sum  of  partial  fractions. 

2.    To  get  developments  of  sec  #,  cosec  a?,  we  observe  that 

cosec  x  =  tan  \  x  +  cot  x. 
Hence 


1      ^  4 

=  ~~*~  *j  fv  0 _  1 


s-l)27T2- 


a^ 
valid  for  x^±  STT. 


THE   CIRCULAR   FUNCTIONS 
3.    To  get  sec  x,  we  observe  that 

cosec  f  ^  —  x  J  =  sec  x. 


263 


Now 


Hence 


cosec 


x        i  (STT  —  x      STT  +  X] 


H.cfe-sV— +±(- 


cosec 


=s. 


^     J   |_,    , 


7T 


Let  us  regroup  the  terms  of  S,  forming  the  series 


As 


=  o, 


:TT  —  a; 


we  see  that  T7  is  convergent  and  =  S.     Thus 


wr—'Zf 
sec  a;  —  2,^  — 


valid  for  all  a;  such  that  cos  a;  ^=  0. 

217.    As  an  exercise  let  us  show  the  periodicity  of  cot  x  from 
216,  5).     We  have 


Now 


TO  ^ 

cot  a;  =  lim  Fn(x)  =  lim  V a:  =£  STT, 

"=»  ^nx  H-  *T 


1 


a;  4-  (n+  l)?r      x  —  nir 


Letting  TI  =  oo  we  see  that 

lim  ^(2:  +  TT)  =  lim  Fn(x) 
cot  (x  4-  ?r)  =  cot  a;. 


and  hence 


264  INFINITE  PRODUCTS 

218.    Development  of  log  sin  #,  tan  x,  etc.,  in  power  series. 
From  216,  1) 


sn  x 


If  we  give  to  -^-^its  limiting  value  1  as  x  =  0,  the  relation  1) 
x 

holds  for  |  x  \  <  TT. 
Now  for  I  x  I  <  TT 


Thus 

sin  x      x2   .  1  x*   .  1  XQ 


227T2         2247T4         3267T6 

^2     i  1    ^     ,  1   a* 

327T2         2347T4         3367T6 


provided  we  sum  this  double  series  by  rows.  But  since  the  series 
is  a  positive  term  series,  we  may  sum  by  columns,  by  129,  2. 
Doing  this  we  get 


+...         ,       .        (2 
where  1111 

^=i+i+i^+-  '     ,;•";; 

The  relation  2)  is  valid  for  \  x  |  <  TT. 

In  a  similar  manner  we  find 

96  ^6 
£(?6+...  (3 


valid  for  |  »|  <•     Here 


VT^  7T 


THE   CIRCULAR  FUNCTIONS  265 

The  terms  of  G-n  are  a  part  of  Hn.     Obviously 


These  coefficients  put  in  3)  give 


valid  for  |  x  \  <  -  •     If  we  differentiate  4)  and  2),  we  get 

Zt 

tan  x=  2(22  _  1>F  ^  +  2(2<  _  1)^  +  2(2«-  1)^  +  ...  (5 

7T*  7T*  7T" 

valid  for  |a?|  <—  ; 

2i 

eot*=i-2^-2J?i^-2J.g-...  (6 

£  7T  7T  7T 

valid  for  0  <  \x\  <  TT. 

Comparing  5)  with  the  development  of  tan  x  given  165,  3) 
gives 


a, 

i 

"12 
1 

1 

1   , 

1 

32 

1 

=  6 

7T4 

1   2?r2-» 

6*2!" 

1          237T4 

.    2?r2. 
L         t^  y 

1*    ' 

1     , 

2* 

1   , 

„  .  i 

i  , 

90 

7T6 

30       4! 

1           257T6 

3      4! 

i?         257T6 

'I'1 

1     , 

1 

36  + 

!+... 

945 

7T8 

42        6! 

1          27  7T8 

5      6! 

07  ,,.8 

z? 

8 

1'    ' 

28    ' 

9450 

30       8! 

7      8! 

Let  u 

.s  set 

jy     — 

2*-V- 

1  J&2 

Then 

n  T.  — 

5)  gi\ 

res 

:24-i) 

-1) 

(8 


valid  for  |  a;  |  <  ^  •     The  coefficients  B^  B3  -  •  -  are  called    Ber- 
nouillian  numbers.     From  7)  we  see 

A  =6       '       ^3  =  A       '       ^5  =  A       '       A  =  A' 


266  INFINITE  PRODUCTS 

From  6),  8)  we  get 

cota»H=-|(f^»-^-'  do 

valid  for  0  <    x  \  <  ?r. 

219.    Recursion  formula  for  the  Bernouillian  Numbers. 
If  we  set  f(x)  =  tan  x, 

we  have  by  Taylor's  development 


o  !  51 

where       /2n-i,(0)        2(2'-  -  I)g2n     22"(22"  -  1)  R 

(2w-l)!  ,T2»  (2re)!          2-1 

Now  by  I,  408, 

/o»-i>(0)-  (2  Y 
From  1),  2)  we  get 


2 

^Y1)^^^^,A..(-1)          (3 

We  have  already  found  ^,  ^3,  .B.,  ^7  ;    it  [s  now  easy  to  find 
successively  : 


Thus  to  calculate  J59,  we  have  from  3) 

2io  -  1)  B    _  ^8  27(28  -  1)    J_       9.8.7.6  25(26-1)  ^ 
5  "  1  •  2  "       4          '  30       1  .  2  .  3  .  4          3          42 

Q  .  Q  .  7    93/^94         1\        1  -t 

_   V      O       j     £   ^     -    JJ      J_  1 

1-2.3  2  30  ^  C  }  '  6 

Thus 


512 

5  .  7936        _5^ 
512  .  1023  ~  66' 


~  2°16 


THE   B   AND   T   FUNCTIONS  267 


The  B  and  F  Functions 

220.    In  Volume  I  we  defined  the  B  and  F  functions  by  means 
of  integrals:  r*      u_1  -, 

B  (u,  v)  =  \     —  (1 

r<V)=  Ce-xxu~ldx  (2 


(u)= 

^0 


which  converge  only  when  u,  v  >  0.     Under  this  condition  we  saw 


We  propose  to  show  that  T(u)  can  be  developed  in  the  infinite 
product  /        j 


(4 

n        « 


This  product  converges,  as  we  saw,  197,  3,  for  any  u  =£  0,  —  1, 
—  2,  •••  From  201,  7  and  207  it  is  obvious  that  G-  converges  abso 
lutely  and  uniformly  at  any  point  u  different  from  these  singular 
points.  Thus  the  expression  4)  has  a  wider  domain  of  definition 
than  that  of  2).  Since  G-  =  F^  as  we  said,  for  w>0,  we  shall  ex 
tend  the  definition  of  the  F  function  in  accordance  with  4),  for 
negative  u. 

It  frequently  happens  that  a  function  f(x)  can  be  represented 
by  different  analytic  expressions  whose  domains  of  convergence 
are  different.  For  example,  we  saw  218,  9),  that  tan  x  can  be  de 
veloped  in  a  power  series 


92/92 
^  ^~ 


92 


valid  for   a?<?«     On  the  other  hand, 


tan  x  = 


X  X*          X° 

II      81      51*  '"      sin  a; 


r2 


cosz 


_ 
214! 


268  INFINITE   PRODUCTS 

and  w  x 

tanz  =  227oT — 1x2 ^  216'  6) 


are  analytic  expressions  valid  for  every  x  for  which  the  function 
tan  x  is  denned. 

221.  1.  Before  showing  that  Gr  and  F  have  the  same  values  for 
u  >  0,  let  us  develop  some  of  the  properties  of  the  product  Gr  given 
in  220,  4).  In  the  first  place,  we  have,  by  210: 

The  function  Cr(u)  is  continuous,  except  at  the  points  u  =  0,  —  1, 

-2,  ... 

Since  the  factors  of  4)  are  all  positive  for  u  >  0,  we  see  that 

Gr(u)  is  positive  for  u  >  0. 

2.    In  the  vicinity  of  the  point  x  =  —  m,      m  =  0,  1,  ••• 


x  +  m 

where  H(u)  is  continuous  near  this  point,  and  does  not  vanish  at 
this  point. 
For 

'!  +  - 
m 


m 

where  If  is  the  infinite  product  G-  with  one  factor  left  out.  As  we 
may  reason  on  .ZTas  we  did  on  G-,  we  see  .ZT  converges  at  the  point 
x  =  —  m.  Hence  ff=£  0  at  this  point.  But  ^Talso  converges  uni 
formly  about  this  point;  hence  H is  continuous  about  it. 

222>  „      r     1  1.2.-O-1) 

G-  =  lim ^ ^ nu.  (1 

n=*  u  (u  +  1)  (u  +  2)  • .  -  (u  +  n  —  1) 

To  prove  this  relation,  let  us  denote  the  product  under  the  limit 
sign  by  Pn.     We  have 

2  3  4         n 


THE  B  AND  T  FUNCTIONS  269 

Also 


Thus  Pn  =  Grn.     But  Grn  =  G-,  hence  Pn,  is  convergent  and  Gr  = 
limPn. 

223.    Uuler's  Constant.     This  is  defined  by  the  convergent  series 


It  is  easy  to  see  at  once  that 


\        n. 

where  C  is  the  Eulerian  constant. 

For  when  a  >  0,         au  =  eu  loga. 
Hence 

1     *'U< 


u 


Now 
and 


by  218,  7).     By  calculation  it  is  found  that 

C^  .577215  — 

224.    Another  expression  of  G-  is 

"c      .   ,   ^  =  1,2,...  (i 


270  INFINITE   PRODUCTS 

are  convergent.     Hence 


/ 

from  which  1 )  follows  at  once,  using  223. 
225.    Further  Properties  of  G-. 


Let  us  use  the  product 

P.00-1  __  fr"1"  __  »• 
u     («  +  !)•••  ,(«+•»  -?!) 

employed  in  222.     Then 

Pn(tt  +  l)  =  ^P^i».  (2 

w  4-  n 

As 


=  u         as  w  =  QO 


M  4-  n 
we  get  1)  from  2)  at  once  on  passing  to  the  limit. 

2.  #O  +  rc)=tt(i*  +  l)  ...  O  +  ra-l)#O).  (3 
This  follows  from  1)  by  repeated  applications. 

3.  #00=1.2.  ...w-l=(w-l)I  (4 

where  n  is  a  positive  integer. 


sin  TTU 
For  G(l-u)=-uG(-u)         b    1 

= — ,     by  224,  1). 

Hence 


n 


THE   B   AND  T  FUNCTIONS  271 

We  now  use  213,  5). 

Let  us  note  that  by  virtue  of  1,  2  the  value  of  Gr  is  known  for 
all  u  >  0,  when  it  is  known  in  the  interval  (0,  1).  By  virtue  of 
5)  G-  is  known  for  u  <  0  when  its  value  is  known  for  u  >  0. 
Moreover  the  relation  5)  shows  the  value  of  6r  is  known  in  (J,  1) 
when  its  value  is  known  in  (0,  J). 

As  a  result  of  this  we  see  G-  is  known  when  its  values  in  the 
interval  (0,  J)  are  known  ;  or  indeed  in  any  interval  of  length  J. 

Gauss  has  given  a  table  of  log  Gr(u)  for  l<w<1.5  calculated 
to  20  decimal  places.  A  four-place  table  is  given  in  "  A  Short 
Table  of  Integrals  "  by  B.  0.  Peirce,  for  1  <  u  <  2. 

5.  &($)  =  V^.  (6 

For  in  5)  set  u  =  ^.     Then 


Hence  &(£)  = 

We  must  take  the  plus  sign  here,  since  G-  >  0  when  u  >  0,  by  221 

1-3.  5-  ..27i- 


where  n  is  a  positive  integer. 

For 


226.    Expressions  for  log  6r(w),  a?ic?  ^8  Derivatives 
From  224,  1)  we  have  for  w  >  0, 

ZO)  =  log  (?  O)  =  -  CW 

Differentiating,  we  get 


U          l     VH        M  + 

That  this  step  is  permissible  follows  from  155,  1. 


272  INFINITE   PRODUCTS 

We  may  write  2) 


(3 


That  the  relations  2),  3)  hold  for  any  u=£  0,  -  1,  -  2  •••  follows 
by  reasoning  similar  to  that  employed  in  216.     In  general  we  have 

^-(-lyO-')'^,1.!),    .    r>L  (4 

In  particular, 

-  (7.  (5 


-iyo-i)iSi.(-i)'oi-i)!Jt. 


227.    Development  of  log  #(%)  m  a  Power  Series.     If  Taylor's 
development  is  valid  about  the  point  u  =  1,  we  have 


log  0(«)  =  £ 

or  using  226,  5),  and  setting  u  =  1  +  #, 
log 


n 


We  show  now  this  relation  is  valid  for  —  J  <  x  <  1,  by  proving 
that 


converges  to  0,  as  s  =  oo  . 
For,  if  0<z<l,  then 


Also  if  -i<o;<0, 


x 


Ox 


The  relation  1)  is  really  valid  for  —  1  <  a;<  1,  but  for  our  pur 
pose  it  suffices  to  know  that  it  holds  in  51  =  (—  J,  1).     Legendre 


THE   B   AND   T   FUNCTIONS  273 

has   shown   how  the    series  1)   may  be  made  to  converge  more 
rapidly.     We  have  for  any  x  in  51 


2  n 

This  on  adding  and  subtracting  from  1)  gives 
log  0(1  +  x)  =  -  log  (1  +  x)  +  (1  -  C)x  +  I(  -  ! 

2 

Changing  here  x  into  —  a;  gives 
log  <?(!  -  T)  =  -  log  (1  -  *)  -  (1  -  C)x  +  2(J5T.-  I)?" 

71 

Subtracting  this  from  the  foregoing  gives 
log  0(1  +  a)  -  log  (7(1  -  *) 


From  225,  4 

log  (7(1  +  x) 


sin  TTX 

This  with  the  preceding  relation  gives 
log  (7(1  +  z) 

valid  in  51. 


This  series  converges  rapidly  for  0<#<i,  and  enables  us  to 
compute  G-(u)  in  the  interval  l<w<|.  The  other  values  of  (7 
may  be  readily  obtained  as  already  observed. 

228.  1.  We  show  now  with  Pringsheim*  that  Gr(u)  =r(w),/0r 
u>0. 

We  have  for  0<><ll, 

r(w  +  ?i)  =  f  Vzzu+n-1<fa 


0 

.  Annalen,  vol.  31,  p.  455. 


274  INFINITE  PRODUCTS 

Now  for  any  x  in  the  interval  (0,  ri), 

xu<nu     ,     xu>xnu~1 
since  u  >  0  and  u  —  1  <  ;  0. 

Also  for  any  x  in  the  interval  (n,  oo  ) 

xu<xnu~l     ,     xu>^nu. 


Hence 

/•n 

nu-ij  e 

r*n  s+<*> 

<nu\  e~xxn-ldx  +  nu-l\  e~xxndx. 

»/0  Jn 

Thus 


/*ra  1     /^a° 

I    e-^71-1^^-  I 

^0  ^^/O 


—  ±  I    e-*x*dx. 


Let  us  call  these  integrals  ^4,  ^,  (7  respectively. 
We  see  at  once  that 

=  n\  = 


n  n 

Also,  integrating  by  parts, 


Thus 
Similarly 

Hence 
where 


e*(n-l)\      enn\ 
Now 


THE   B   AND   T   FUNCTIONS  275 

But 

svi  mm 

vn  >  1  H T  +  —  + 7  — ^     ,     for  any  m 

n+l  O  +  l)  ...  (n  +  m) 

mnm  m  m 


(n  +  1)  -.  O  +  m)      A  +  ^  ~  /t  ~  wA      fl  +  m\n 
\        nj       \        nj     \        n) 


Let  us  take 

n>m*    or     *< 

?i        7W 

Then 

m  m 


Since  m  may  be  taken  large  at  pleasure, 

lim  vn  =  oo 

and  hence  ,. 

lim  qn  =  0. 

Thus 

But  from  T(u  +  1)  =  uT(u)  we  have 

T(u  +  1  +ri)  _  u  +  n  Y(u  +  n)    __  -, 

also,  as  n  =  oo  .     Thus  the  relation  1)  holds  for  1  <  u<_ 2,  and  in 
fact  for  any  u  >0. 

A«a 

-iXO  Tl  /^/i*      )       .,_  "\ /\    f  I       "1  \  /^  I 

we  have 


Hence  using  1),  1N  .  ^. 

(M.-l)!n«  F(M  +  n) 


u(u  +  1)  ..«  (w  +  n-  1)      (w-1)!^ 

Letting  w=  oo  ,  we  get  F(w)=  (r(w)  for  any  w>0,  making  use 
of  1)  and  222,  1). 

2.    Having  extended  the  definition  of  F(w)  to  negative  values 
of  w,  we  may  now  take  the  relation 


as  a  definition  of  the  B  function.  This  definition  will  be  in 
accordance  with  220,  1)  for  w,  v  >  0,  and  will  define  B  for  negative 
w,  v  when  the  right  side  of  2)  has  a  value. 


CHAPTER   VIII 
AGGREGATES 

Equivalence 

229.  1.  Up  to  the  present  the  aggregates  we  have  dealt  with 
have  been  point  aggregates.  We  now  consider  aggregates  in 
general.  Any  collection  of  well-determined  objects,  distinguish 
able  one  from  another,  and  thought  of  as  a  whole,  may  be  called 
an  aggregate  or  set. 

Thus  the  class  of  prime  numbers,  the  class  of  integrable  func 
tions,  the  inhabitants  of  the  United  States,  are  aggregates. 

Some  of  the  definitions  given  for  point  aggregates  apply  obvi 
ously  to  aggregates  in  general,  and  we  shall  therefore  not  repeat 
them  here,  as  it  is  only  necessary  to  replace  the  term  point  by 
object  or  element. 

As  in  point  sets,  51  =  0  shall  mean  that  51  embraces  no  elements. 

Let  51,  33  be  two  aggregates  sucli  that  each  element  a  of  51  is 
associated  with  some  one  element  b  of  33,  and  conversely.  We  say 
that  51  is  equivalent  to  33  and  write 

51-33. 

We  also  say  51  and  33  are  in  one  to  one  correspondence  or  are  in 
uniform  correspondence.  To  indicate  that  a  is  associated  with  b 
in  this  correspondence  we  write 

a~b. 

2.  If  51  ~  33  and  33  ~  6,  then  51  ~  {£. 

For  let  a  ~  b,  b  ~  c.  Then  we  can  set  51,  (£  in  uniform  corre 
spondence  by  setting  a  ~  c. 

3.  Let  5(  =  33  +  £  +  £)+  - 

A  =  B  +  C+D  +  ••• 

//  33  ~  B,  6  ~  C\  •••,  then  51  ~  A. 

276 


EQUIVALENCE  277 

For  we  can  associate  the  elements  of  51  with  those  of  A  by 
keeping  precisely  the  correspondence  which  exists  between  the 
elements  of  33  and  B,  of  £  and  (7,  etc. 

Example  1.  51  =  1,  2,  3,  ... 

33  =  aj,  &2,  a3,  ... 
If  we  set  an~  n,  51  and  33  will  stand  in  1,  1  correspondence. 

Example  2.  51  =  1,  2,  3,  4,  ••• 

33  =  2,4,6,8,  - 

If  we  set  n  of  51  in  correspondence  with  2  n  of  33,  51  and  33  will 
be  in  uniform  correspondence. 

We  note  that  33  is  a  part  of  5t  ;  we  have  thus  this  result  :  An 
infinite  aggregate  may  be  put  in  uniform  correspondence  with  a 
partial  aggregate  of  itself. 

This  is  obviously  impossible  if  51  is  finite. 

Example  3.  51  =  1,  2,  3,  4,  ... 

33  =  101,  102,  103,  104,  ... 

If  we  set  n  ~  10n,  we  establish  a  uniform  correspondence  be 
tween  51  and  33.  We  note  again  that  31  ~  33  although  51  >  33. 

Example  4-     Let  (E  =  \%  j,  where,  using  the  triadic  system, 

f=-«A-        f.=  0,2 
denote  the  Cantor  set  of  I,  272.     Let  us  associate  with  %  the  point 


where  xn  =  0  when  fn  =0,  and  =1  when  f  n  =  2  and  read  1)  in 
the  dyadic  system. 

Then  \x\  is  the  interval  (0,  1).  Thus  we  have  established  a 
uniform  correspondence  between  (E  and  the  points  of  a  unit  interval. 

In  passing  let  us  note  that  if  f  <  f  '  and  a;,  a/  are  the  correspond 
ing  points  in  \x\,  then  x  <  x'  . 

This  example  also  shows  that  we  can  set  in  uniform  correspond 
ence  a  discrete  aggregate  with  the  unit  interval. 

We  have  only  to  prove  that  (E  is  discrete.  To  this  end  consider 
the  set  of  intervals  C  marked  heavy  in  the  figure  of  I,  272.  Ob- 


278  AGGREGATES 

viously  we  can  select  enough  of  these  deleted  intervals  so  that 
their  lower  content  is  as  near  1  as  we  choose.     Thus 

Cont  0=1. 

As  Cont  C  <  1,  O  is  metric  and  its  content  is  1.  Hence  (£  is 
discrete. 

230.  1.  Let  tyi=a  +  A,  33  = /3 -f  .#,  where  a,  b  are  elements 
of  SI,  33  respectively.  7/1  SI  ~-  33,  then  A~B  avid  conversely. 

For,  since  SI  ~  33,  each  element  a  of  51  is  associated  with  some 
one  element  b  of  33,  and  the  same  holds  for  33.'  If  it  so  happens 
that  a  ~  /3,  the  uniform  correspondence  of  A,  B  is  obvious.  If 
on  the  contrary  «  ~  b'  and  /3  ~  a',  the  uniform  correspondence  be 
tween  A,  B  can  be  established  by  setting  a'  ~  b'  and  having  the 
other  elements  in  A,  B  correspond  as  in  51  ~  33. 

2.  We  state  as  obvious  the  theorems: 
No  part  33  of  a  finite  set  SI  can  be  ~  SI. 
No  finite  part  33  of  an  infinite  set  51  can  be  ~  SI. 


Cardinal  Numbers 

231.  1.  We  attach  now  to  each  aggregate  SI  an  attribute 
called  its  cardinal  number,  which  is  defined  as  follows  : 

1°  Equivalent  aggregates  have  the  same  cardinal  number. 

2°  If  SI  is  —  to  a  part  of  33,  but  33  is  not  ~  SI  or  to  any  part 
of  SI,  the  cardinal  number  of  SI  is  less  than  that  of  33,  or  the 
cardinal  number  of  33  is  greater  than  that  of  SI.  The  cardinal 
number  of  SI  may  be  denoted  by  the  corresponding  small  letter 
a  or  by  Card  SI. 

The  cardinal  number  of  an  aggregate  is  sometimes  called  its 
power  or  potency. 

If  SI  is  a  finite  set,  let  it  consist  of  n  objects  or  elements. 
Then  its  cardinal  number  shall  be  n.  The  cardinal  number  of 
a  finite  set  is  said  to  be  finite,  otherwise  transfinite.  It  follows 
from  the  preceding  definition  that  all  transfinite  cardinal  num 
bers  are  greater  than  any  finite  cardinal  number. 


CARDINAL   NUMBERS  279 

2.  It  is  a  property  of  any  two  finite  cardinal  numbers  a,  b  that 

either 

a  =  b    ,     or  a  >  b    ,     or  a  <  b.  (1 

This  property  has  not  yet  been  established  for  transfinite  car 
dinal  numbers.  There  is  in  fact  a  fourth  alternative  relative  to 
21,  33,  besides  the  three  involved  in  1).  For  until  the  contrary 
has  been  shown,  there  is  the  possibility  that  : 

No  part  of  21  is  ~  23,  and  no  part  of  23  is  ~  21. 

The  reader  should  thus  guard  against  expressly  or  tacitly 
assuming  that  one  of  the  three  relations  1)  must  hold  for  any 
two  cardinal  numbers. 

3.  We  note  here  another  difference.     If  21,  23  are  finite  with 
out  common  element, 

Card  (21  +  23)  >  Card  21.  (2 

Let  now  21  denote  the  positive  even  and  23  the  positive  odd 
numbers.  Obviously 

Card  (21  +  23)  =  Card  21  =  Card  23 
and  the  relation  2)  does  not  hold  for  these  transfinite  numbers. 

4.  We  have,  however,  the  following  : 

Let  21  >  23,  then 

Card  21  >  Card  23. 

For  obviously  23  is  ~  to  a  part  of  21,  viz.  23  itself. 

5.  This  may  be  generalized  as  follows  : 

Let 


If  Card  23  <  Card  B     ,     Card  <£  <  Card  (7,  etc., 

then  Card  21  <  Card  A. 

For  from  Card  23  <.  Card  B  follows  that  we  can  associate  in  1, 
1  correspondence  the  elements  of  23  with  a  part  or  whole  of  B. 

The  same  is  true  for  (£,  (7;  $),  D  ;  ••• 

Thus  we  can  associate  the  elements  of  21  with  a  part  or  the 
whole  of  A. 


280  AGGREGATES 

Enumerable  Sets 

232.  1.  An  aggregate  which  is  equivalent  to  the  system  of 
positive  integers  $  or  to  a  part  of  3  ig  enumerable. 

Thus  all  finite  aggregates  are  enumerable.  The  cardinal  num 
ber  attached  to  an  infinite  enumerable  set  is  K0,  aleph  zero. 

At  times  we  shall  also  denote  this  cardinal  by  e,  so  that 

e  =  V 

2.    Every  infinite  aggregate  51  contains  an  infinite  enumerable  set  $&. 
For  let  a1  be  an  element  of  51  and 


Then  5tj  is  infinite ;  let  az  be  one  of  its  elements  and 

Then  512  is  infinite,  etc. 

Then  $  =  a 

is  a  part  of  21  and  forms  an  infinite  enumerable  set. 
3.    From  this  follows  that 

K0  is  the  least  transfinite  cardinal  number. 

233.      The  rational  numbers  are  enumerable. 
For  any  rational  number  may  be  written 

r  =  ™  (1 

n 

where,  as  usual,  m  is  relatively  prime  to  n. 
The  equation 

admits  but  a  finite  number  of  solutions  for  each  value  of 

^  =  2,3,4,  .- 

Each  solution  m,  n  of  2),  these  numbers  being  relatively  prime, 
gives  a  rational  number  1).     Thus  we  get,  e.g. 
p=2     ,      ±1. 

O  i     O  i      1 

P  =  o     •>      ±2,          ±  -J. 

P  =  4:       ,         ±3,  ±J. 

J>  =  5    ,     ±4,         ±J    ,     ±|          ±J. 


ENUMERABLE   SETS  281 

Let  us  now  arrange  these  solutions  in  a  sequence,  putting  those 
corresponding  to  p  =  q  before  those  corresponding  to  p  =  q  +  1. 

We  get 

r\     >     r2     »     r3  .-  (3 

which  is  obviously  enumerable. 

234.    Let  the  indices  tj,  t2,  '••  *p  range  over  enumerable  sets.     Then 

«VK-^J 

z*  enumerable. 

For  the  equation 

"i  +  "2  +  "•  +  "*  =  w, 

where  the  i/'s  are  positive  integers,  admits  but  a  finite  number 
of  solutions  for  each  n  =  p,  jo  +  1,  p  +  2,  jt?  +  3  «•«  Thus  the 
elements  of  $»_$/,  ? 

may  be  arranged  in  a  sequence 


by  giving  to  n  successively  the  values  p,  p  +  1,  •••  and  putting  the 
elements  bVl...Vp  corresponding  to  n  =  q+  1  after  those  correspond 
ing  to  n  =  q. 

Thus  the  set  35  is  enumerable.  Consider  now  51.  Since  each 
index  im  ranges  over  an  enumerable  set,  each  value  of  im  as  i'm  is 
associated  with  some  positive  integer  as  m'  and  conversely.  We 
may  now  establish  a  1,  1  correspondence  between  31  and  33  by 
setting 

£/»x-™;~aiX-v 

Hence  21  is  enumerable. 

235.  1.  An  enumerable  set  of  enumerable  aggregates  form  an 
enumerable  aggregate. 

For  let  5t,  33,  (£  •••  be  the  original  aggregates.  Since  they  form 
an  enumerable  set,  they  can  be  arranged  in  the  order 

*!,«,**,,      -  (1 

But  each  $Im  is  enumerable  ;  therefore  its  elements  can  be 
arranged  in  the  order 

am\       >       «m2       »       ^m3       »       ^m*       »        '" 


282  AGGREGATES 

Thus  the  a-elements  in  1)  form  a  set 

\amn\         m,  n,=  1,  2,  ••• 
which  is  enumerable  by  234. 

2.  The  real  algebraic  numbers  form  an  enumerable  set. 

For  each  algebraic  number  is  a  root  of  a  uniquely  determined 
irreducible  equation  of  the  form 

xn+aiXn-l+   ...    +an=0, 

the  a's  being  rational  numbers.     Thus  the  totality  of  real  algebraic 
numbers  may  be  represented  by 

\Pn,  aidf-  an\ 

where  the  index  n  runs  over  the  positive  integers  and  a1  •••  an  range 
over  the  rational  numbers. 

3.  Let  51,  33  ^  two  enumerable  sets.      Then 

Card  51= 


And  in  general  if^,  512  —  are  an  enumerable  set  of  enumerable 
aggregates,  Card  (5^  ,  512  ,•••)  =  K0. 

This  follows  from  1. 

236.  Every  isolated  aggregate  91,  limited  or  not,  forms  an  enumer 
able  set. 

For  let  us  divide  9?m  into  cubes  of  side  1.  Obviously  these  form 
an  enumerable  set  C\,  <72'».  About  each  point  a  of  91  in  any  <7n 
as  center  we  describe  a  cube  of  side  er,  so  small  that  it  contains  no 
other  point  of  91.  This  is  possible  since  91  is  isolated.  There  are  but 

a  finite  number  of  these  cubes  in  On  of  side  a-  =  -,  v  =  1,  2,  3,  ••• 

v 

for  each  v.     Hence,  by  235,  l,  91  is  enumerable. 

237.  1.  Every  aggregate  of  the.  first  species  91,  limited  or  not,  is 
enumerable. 

For  let  91  be  of  order  n.     Then 

91  =  91  +  9i; 


ENUMERABLE   SETS  283 

where  5lt  denotes  the  isolated  points  of  51  and  51^  the  proper  limit 
ing  points  of  51- 
Similarly, 


Thus, 

5i  =  5t;  +  5i;,t  +  5r;,t  +  -  +  a?). 

But  5l(n)  is  finite  and  51<;1)  <  5I(n). 

Thus  51  being  the  sum  of  n  4-  1  enumerable  sets,  is  enumerable. 

2.    .Tjf  51'  is  enumerable,  so  is  51. 
For  as  in  1, 

*  »  X  +  9£ 

and  5i;<5{'. 

238.    1.   Every  infinite  aggregate  51  contains  a  part  53  swc?A  £^a£ 
53-51. 

For  let  &  =  («j,  a2,  «3  •••)  be  an  infinite  enumerable  set  in  51, 
so  that 

51  =  (5  +  g. 

Let  (g  =  d    +  .#. 


To   establish  a  uniform   correspondence   between  .#,  (5  let  us 
ociate  an  in 
We  now  set 


associate  an  in  @  with  an+1  in  J^.     Thus 


Obviously  51  ~  53  since  .Z7~  (5,  and  the  elements  of  5  are  common 
to  51  and  53.  - 

2.    -Zjf  5l~53  are  infinite,  each  contains  a  part  5lj,  53i  such  that 


For  by  1,  51  contains  a  part  5^  such  that  51  —  51J.  Similarly, 
53  contains  a  part  53:  such  that  53—  53r  As  51  —  33,  we  have  the 
theorem. 


284  AGGREGATES 

239.  1.  A  theorem  of  great  importance  in  determining 
whether  two  aggregates  are  equivalent  is  the  following.  It  is 
the  converse  of  238,  2. 


then  ^^^ 

In  the  correspondence  3^  ~  33,  let  512  be  the  elements  of  5Ij 
associated  with  33X  .  Then 

5I2  ~  $!  ~  31 

and  hence  or       <ar  /1 

&  «v  eig*  (.1 

But  as  Slj  >  $12  ,  we  would  infer  from  1)  that  also 

21  ~V  (2 

As  ^  ~  33  by  hypothesis,  the  truth  of  the  theorem  follows  at 
once  from  2). 

To  establish  2)  we  proceed  thus.  In  the  correspondence  1),  let 
5(3  be  that  part  of  $12  which  ~  ^  in  51.  In  the  correspondence 
^  ~  513,  let  514  be  that  part  of  5t3  which  ~  512  in  5lx  . 

Continuing  in  this  way,  we  get  the  indefinite  sequence 

51  >  5Ij  >  512  >  313  >  ••. 

SUCh    that  rw  rvf  af 

S4  ~  <!12  ~  ^14  ~  ••• 

3^-213-21,-... 

Let  now 


Then  3l  =  D  +  G1H-G2  +  68  +  C4+  -  (3 

and  similarly  «,  =  ®  +  G,  +  G,  +  G4  +  S5  +  •" 

We  note  that  we  can  also  write 

2l1  =  £)+G3  +  l£2  +  e6  +  G4+  ».  (4 

Now  from  the  manner  in  which  the  sets  513,  514  •••  were  obtained, 
it  follows  that 

£i~£3     »     e8-@6-  (5 

Thus  the  sets  in  4)  correspond  uniformly  to  the  sets  directly 
above  them  in  3),  and  this  establishes  1). 


ENUMERABLE   SETS  285 

2.  In  connection  with  the  foregoing  proof,  which  is  due  to 
Bernstein,  the  reader  must  guard  against  the  following  error.  It 
does  not  in  general  follow  from 

that  £    ~  (5 

which  is  the  first  relation  in  5). 

Example.     Let  51  =  (1,  2,  3,  4,  •••). 

511=(2,  3,  4,  5".)     ,     512=(3,  4,  5,  6  ...) 

513=(5,  6,  7,  8  •••). 

Then  £  =  1         6  =  (3,  4). 

Now  5(,  51  r  51 2  ,  513  are  all  enumerable  sets ;  hence 
9T  <~  91  91    ~-  31 

But  obviously  C^  is  not  equivalent  to  (E3,  since  a  set  containing 
only  one  element  cannot  be  put  in  1  to  1  correspondence  with  a 
set  consisting  of  two  elements. 


240.    1.    If%>$> 
For  by  hypothesis  a  part  of  23,  viz.  (£,  is  ~2L     But  a  part  of 
is  ~33,  viz.  33  itself.     We  apply  now  239. 
2.    Let  a  be  any  cardinal  number.     If 


then  a  =  Card  $. 

For  let  Card  51  =  «.     Then  from 

a  <  Card  33 
it  follows  that  51  ~  a  part  or  the  whole  of  33  ;   while  from 

Card  33  <  « 
it  follows  that  33  is  ~  a  part  or  the  whole  of  51. 

3.    Any  part  33  of  an  enumerable  set  51  is  enumerable. 
For  if  33  is  finite,  it  is  enumerable.      If  infinite, 

Card33>K0- 
On  the  other  hand 

Card  33  <  Card  51  =  K0. 


286  AGGREGATES 

4.    Two  infinite  enumerable  sets  are  equivalent. 

For  both  are  equivalent  to  $,  the  set  of  positive  integers. 

241.  1.    Let  (£  be  any  enumerable  set  in  51 ;  set  51  =  (£  +  23.     If 
23  ^s  infinite,  51  —  53. 

For  23  being  infinite,  contains  an  infinite  enumerable  set  g. 
Let  23  =  g  +  ®.  Then 

51  =  (5  +  g  +  ®, 

8  -.  8  +'ft 

But  <g  +  g  ~  g.     Hence  51-23. 

2.  We  may  state  1  thus  : 

Card  (31 -(S)=  Card  51 
provided  51  —  (5  i«  infinite. 

3.  From  1  follows  at  once  the  theorem : 

.Let  51  be  any  infinite  set  and  (5  an  enumerable  set.      Then 
Card  (51  +  <g)  =  Card  51. 

Some  Space   Transformations 

242.  1.    Let  T  be  a  transformation  of  space  such  that  to  each 
point  x  corresponds  a  single  point  XT,  and  conversely. 

Moreover,  let  #,  y  be  awy  two  points  of  space.  After  the  trans 
formation  they  go  over  into  XT,  yT.  If 

Dist(>,  y)=  DistOy,  yT) 
we  call  jTa  displacement. 

If  the  displacement  is  defined  by 

x'1  =  xl  +  al     ,     ...     x'm  =  xm  +  am 
it  is  called  a  translation. 

If  the  displacement  is  such  that  all  the  points  of  a  line  in  space 
remain  unchanged  by  T,  it  is  called  a  rotation  whose  axis  is  the 
fixed  line. 


THE   CARDINAL   c  287 

If  9?  denotes  the  original  space,  and  9?r  the  transformed  space 
after  displacement,  we  have,  obviously, 


2.  Let  =tx  =  tx  t      Q  ^ 

Then  when  x  ranges  over  the  w-way  space  3E,  y  ranges  over  an 
w-way  space  9).     If  we  set  x  ~  y  as  defined  by  1), 

Alcn 

Dist  (0,  y)  =t  Dist  (0,  x). 

We  call  1)  a  transformation  of  similitude.     If  t  >  1,  a  figure  in 
space  is  dilated  ;  if  t  <  1,  it  is  contracted. 

3.  Let  Q  be  any  point  in  space.     About  it  as  center,  let  us  de 
scribe  a  sphere  S  of  radius  R.     Let  P  be  any  other  point.     On  the 
join  of  P,  Q  let  us  take  a  point  P'  such  that 

Dist  (P',  Q)  = 


Dist  (P,  Q) 

Then  P'  is  called  the  inverse  of  P  with  respect  to  S.  This  trans 
formation  of  space  is  called  inversion.  Q  is  the  center  of  inversion. 

Obviously  points  without  S  go  over  into  points  within,  and  con 
versely.  As  P  =  x  ,  P'  =  Q. 

The  correspondence  between  the  old  and  new  spaces  is  uniform, 
except  there  is  no  point  corresponding  to  Q. 


TJie  Cardinal  c 

243.  1.  All  or  any  part  of  space  &  may  be  put  in  uniform  cor 
respondence  with  a  point  set  lying  in  a  given  cube  C. 

For  let  @t  denote  the  points  within  and  on  a  unit  sphere  S  about 
the  origin,  while  &e  denotes  the  other  points  of  space.  By  an  in 
version  we  can  transform  @e  into  a  figure  @/  lying  in  S.  By  a 
transformation  of  similitude  we  can  contract  @t,  &f  as  much  as  we 
choose,  getting  ^',  (gy-  We  may  now  displace  these  figures  so 
as  to  bring  them  within  C  in  such  a  way  as  to  have  no  points  in 
common,  the  contraction  being  made  sufficiently  great.  The 


288  AGGREGATES 

correspondence  between  <S  and  the  resulting  aggregate  is  obviously 
uniform  since  all  the  transformations  employed  are. 

As  a  result  of  this  and  240,  l  we  see  that  the  aggregate  of  all 
real  numbers  is  ~  to  those  lying  in  the  interval  (0, 1);  for  example, 
the  aggregate  of  all  points  of  SRm  is  ~  to  the  points  in  a  unit  cube, 
or  a  unit  sphere,  etc. 

244.  1.  The  points  lying  in  the  unit  interval  5t  =  (0*,  1*)  are 
not  enumerable. 

For  if  they  were,  they  could  be  arranged  in  a  sequence 

«i,  «2'  a3  "•  0- 

Let  us  express  the  as  as  decimals  in  the  normal  form.     Then 

an  =    '  anian2ana   '" 

Consider  the  decimal 

b  =  •  &J&2&3  ... 

also  written  in  the  normal  form,  where 

^1^^1,1       '       ^2^^2,2       '       ^3^^3,3       i       "• 

Then  b  lies  in  5(  and  is  yet  different  from  any  number  in  1). 

2.  We  have         (0*,  1*)  ~  (0,  1)     ,     by  241,  3, 

-(a,  6)     ,     by  243, 

where  a,  b  are  finite  or  infinite. 

Thus  the  cardinal  number  of  any  interval,  finite  or  infinite, 
with  or  without  its  end  points  is  the  same. 

We  denote  it  by  c  and  call  it  the  cardinal  number  of  the  recti 
linear  continuum,  or  of  the  real  number  system  $1. 

Since  9^  contains  the  rational  number  system  R,  we  have 

OKo- 

3.  The  cardinal  number  of  the  irrational  or  of  the  transcendental 
numbers  in  any  interval  51  is  also  c. 

For  the  non-irrational  numbers  in  51  are  the  rational  which  are 
enumerable ;  and  the  non-transcendental  numbers  in  51  are  the 
algebraic  which  are  also  enumerable. 


THE   CARDINAL   C  289 

4.    The  cardinal  number  of  the  Cantor  set  (£  of  I,  272  is  c. 

For  each  point  a  of   (E  has  the  representation '  in   the   triadic 

system  n   0 

J  a  =  •  a-,a9ao  •••     ,     a  =  U,  ^. 


But  if  we  read  these  numbers  in  the  dyadic  system,  replacing 
each  an  =  2  by  the  value  1,  we  get  all  the  points  in  the  interval 
(0,  1).  As  there  is  a  uniform  correspondence  between  these  two 
sets  of  points,  the  theorem  is  established. 

245.  An  enumerable  set  51  is  not  perfect,  and  conversely  a  perfect 
set  is  not  enumerable. 

For  suppose  the  enumerable  set 

51  =  ^,  «a  —  (1 

were  perfect.  In  D^^a^)  lies  an  infinite  partial  set  51  x  of  51, 
since  by  hypothesis  51  is  perfect.  Let  a^  be  the  point  of  lowest 
index  in  5lj  .  Let  us  take  r2  <  rl  such  that  D^(a^)  lies  in 
D*  (ai)-  In  -A-fC^mi)  ^es  an  infinite  partial  set  512  of  5lr  Let 
am3  be  the  point  of  lowest  index  in  512,  etc. 
Consider  now  the  sequence 


It  converges  to  a  point  a  by  I,  127,  2.  But  a  lies  in  51,  since  this 
is  perfect.  Thus  a  is  some  point  of  1),  say  a  =  a,.  But  this 
leads  to  a  contradiction.  For  a,  lies  in  every  .Z)r*n(#™n);  on  the 
other  hand,  no  point  in  this  domain  has  an  index  as  low  as  mn 
which  =  oo,  as  n  =  GO.  Thus  51  cannot  be  perfect. 

Conversely,  suppose  the  perfect  set  51  were  enumerable.  This 
is  impossible,  for  we  have  just  seen  that  when  51  is  enumerable  it 
cannot  be  perfect. 

246.  Let  51  be  the  union  of  an  enumerable  set  of  aggregates  5ln 
each  having  the  cardinal  number  c.  Then  Card  51  =  c. 

For  let   33n  denote  the  elements  of  5ln  not  in  5lj,5l2  •••  5ln_j. 


Let  (£B  denote   the   interval   (w  —  1,  w*).      Then   the   cardinal 
number  of  Q    -f-  £  +  ...  is  c. 


290  AGGREGATES 

But  Card33n<  Card£n. 

Hence  Card  21  <  c     ,     by  231,  6.  (1 

On  the  other  hand, 

Card  SI  >  Card  21!  =  c.  (2 

From  1),  2)  we  have  the  theorem,  by  240,  2. 

247.  1.  As  already  stated,  the  complex  x=  (2^,  #2,  •••  #n)  de 
notes  a  point  in  n-  way  space.  Let  x±,  #2,  •••  denote  an  infinite 
enumerable  set.  We  may  also  say  that  the  complex 

x—  (2^,  #2,  •  ••  in  inf.) 
denotes  a  point  in  oo  -way  space  9^. 

2.    Let  21  denote  a  point  set  in  $Rn,  n  finite  or  infinite.      Then 

Card  21  <  c.  (1 

For  let  us  first  consider  the  unit  cube  (£  whose  coordinates  xm 
range  over  33  =  (0*,  1*).  Let  £)  denote  the  diagonal  of  (L  Then 

c  =  Card  £)  <  Card  <£.  (2 

On  the  other  hand  we  show  Card  (£  <  c. 

For  let  us  express  each  coordinate  xm  as  a  decimal  in  normal 
form.  Then 


Let  us  now  form  the  number 


obtained  by  reading  the  above  table  diagonally.     Let  9)  denote  the 
set  of  ?/'s  so  obtained  as  the  #'s  range  over  their  values.     Then 


For  the  point  y,  for  example,  in  which  aln=  0,  n  =  1,  2,  •••  lies 
in  33  but  not  in  9)  as  otherwise  xl  =  0.  Let  us  now  set  x  ~  y. 
Then  |£  ~  9  and  hence  Car(J  g  <  £  (3 

From  2),  3)  we  have         Card  G>  =  c. 


THE   CARDINAL   c  291 

Let  us  now  complete  (E  by  adding  its  faces,  obtaining  the  set  C. 
By  a  transformation  of  similitude  T  WQ  can  bring  CT  within  (£. 

Hence  Card  S>  Card  C. 

On  the  other  hand,  (£  is  a  part  of  (7,  hence 

Card  £  <  Card  C. 
Thus  Card  C  =  c.     The  rest  of  the  theorem  follows  now  easily. 

248.    Let  g  =  j/J   denote  the  aggregate  of  one-valued  continuous 
functions  over  a  unit  cube  &  in  9?n. 

Then 


Let  C  denote  the  rational  points  of  (5,  i.e.  the  points  all  of 
whose  coordinates  are  rational.  Then  any  /  is  known  when  its 
values  over  0  are  known.  For  if  a  is  an  irrational  point  of  (5, 
we  can  approach  it  over  a  sequence  of  rational  points  alf  #2  •••  =  a. 
But  /  being  continuous,  /(a)  =  lim/(an),  and  /  is  known  at  «. 
On  the  other  hand,  0  being  enumerable,  we  can  arrange  its  points 

in  a  sequence  n 

O=c^  c^  ... 

Let  now  9^  be  a  space  of  an  infinite  enumerable  number  of 
dimensions,  and  let  y  =  (^,  y^  •  ••)  denote  any  one  of  its  points. 

Let  /  have  the  value  vl  at  c1,  the  value  7/2  at  cz  and  so  on  for 
the  points  of  C.  Then  the  complex  T/J,  ?;2,  ...  completely  deter 
mines  /  in  (£.  But  this  complex  also  determines  the  point 
V  =  C7?!^  ^2  '")  i'n  ^x-  W°  now  associate  /  with  77.  Thus 

Card  g  <.  Card  ft    =  c. 

But  obviously  Card  g  >  c,  for  among  the  elements  of  g  there 
is  an/  which  takes  on  any  given  value  in  the  interval  (0,  1),  at 
a  given  point  of  (L 

249.  There  exist  aggregates  whose  cardinal  number  is  greater 
than  any  given  cardinal  number. 

Let  33=  \b\  be  an  aggregate  whose  cardinal  number  b  is  given. 
Let  a  be  a  symbol  so  related  to  33  that  it  has  arbitrarily  either 
the  value  1  or  2  corresponding  to  each  b  of  33.  Let  51  denote  the 


292  AGGREGATES 

aggregate  formed  of  all  possible  a's  of  tins  kind,  and  let  a,  be  its 
cardinal  number. 

Let  ft  be  an  arbitrary  element  of  33.  Let  us  associate  with  ft 
that  a  which  has  the  value  1  for  b  =  ft  and  the  value  2  for  all 
other  5's.  This  establishes  a  correspondence  between  33  and  a 

part  of  51.     Hence 

a^b. 

Suppose  a  =  b.  Then  there  exists  a  correspondence  which 
associates  with  each  b  some  one  a  and  conversely.  This  is 
impossible. 

For  call  ab  that  element  of  51  which  is  associated  with  b.  Then 
ab  has  the  value  1  or  2  for  each  ft  of  33.  There  exists,  however, 
in  51  an  element  a'  which  for  each  ft  of  33  has  just  the  other 
determination  than  the  one  ab  has.  But  a'  is  by  hypothesis 
associated  with  some  element  of  33,  say  that 


Then  for  b  =  br,  a1  must  have  that  one  of  the  two  values  1,  2 
which  ab'  has.  But  it  has  not,  hence  the  contradiction. 

250.  The  aggregate  of  limited  integrable  functions  $  defined  over 
5(  =  (0,  1)  has  a  cardinal  number  f  >  c. 

For  let  f(x)  =  0  in  51  except  at  the  points  (5  of  the  discrete 
Cantor  set  of  I,  272,  and  229,  Ex.  4.  At  each  point  of  {£  let  / 
have  the  value  1  or  2  at  pleasure.  The  aggregate  ®  formed  of 
all  possible  such  functions  has  a  cardinal  number  >  c,  as  the 
reasoning  of  249  shows.  But  each  /  is  continuous  except  in  (5, 
which  is  discrete.  Hence  /  is  integrable.  But  gf  >  ®.  Hence 

.':     ."••"..    .'        ;.  f><-  '•-'     "      .'"'.'••      , 

Arithmetic   Operations  with  Cardinals 

251.  Addition  of  Cardinals.     Let  51,  33  be  two  aggregates  with 
out  common  element,  whose  cardinal  numbers  are  a,  b.     We  define 
the  sum  of  a  and  b  to  be 

Card  (51,  33)=  a  +  b. 


ARITHMETIC   OPERATIONS   WITH   CARDINALS  293 

We  have  now  the  following  obvious  relations: 

K0  +  n  =  K0     ,     n  a  positive  integer.  (1 

+  •••  +  K0  =  K0     ,     w  terw*.  (2 

+  K0  +  •"  =  KO     ,     aw.  infinite  enumerable  set  of  terms.  (3 
cardinal  numbers  of  51,  23,  (?  are  a,  b,  c, 


The  first  relation  states  that  addition  is  associative,  the  second 
that  it  is  commutative. 

252.    Multiplication. 

1.  LetH  =  {a{,  ^3  =  J5J  have  the  cardinal  numbers  a,  b.     The 
union  of  all  the  pairs  (a,  b)  forms  a  set  called  the  product  of  51  and 
23.     It  is  denoted  by  51  •  23.     We  agree  that  (a,  6)  shall  be  the 
same  as  (5,  a).     Then 

51-23  =  23-51. 
We  define  the  product  of  a  and  b  to  be 

Card  51  -  23  =  Card  23  •  5T  =  a  .  b  =  b  -  a. 

2.  We  have  obviously  the  following  formal  relations  as  in  finite 

cardinal  numbers  : 

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

a  •  b  =  b  •  a, 
a(b  +  c)  =  ab  +  ac, 

which  express  respectively  the  associative,  commutative,  and  dis- 
tripulative  properties  of  cardinal  numbers. 

Example  1.     Let   5l=jaj,   %>  =  \l\    denote   the   points   on   two 
indefinite  right  lines.     Then 


If  we  take  a,  b  to  be  the  coordinates  of  a  point  in  a  plane  9?2, 


*  The  reader  should  note  that  here,  as  in  the  immediately  following  articles,  c  is 
simply  the  cardinal  number  of  (£  which  is  any  set,  like  31,  53  ••• 


294  AGGREGATES 

Example  2.     Let  21  =  \a\  denote  the  family  of  circles 


Let  33  =  5^!  denote  a  set  of  segments  of  length  b.  We  can 
interpret  (#,  6)  to  be  the  points  on  a  cylinder  whose  base  is  1) 
and  whose  height  is  I.  Then  91-33  is  the  aggregate  of  these 
cylinders. 

253.    1.  K0  =  ra.K0     ,     or  nt  =  t.  (1 

For  let  ^      ,       ^     _v 

(§  =  (<?!,  £2  •••  in  inf.) 

Then      K--c~<;«t,'o  ,   («i,«a)  ,   («i» «•)••• 

(/7          ^    ^  ^/7          />    ^  r/7          ^    "\    .  . 

2'      lx       '        v^'     2^        '        VM/21      3x 


The  cardinal  number  of  the  set  on  the  left  is  n£0,  while  the 
cardinal  number  of  the  set  on  the  right  is  K0  . 

2.  ec  =  c.  (2 

For  let  (£  =  {c}  denote  the  points  on  a  right  line,  and  (5  =  (1,  2, 


Then  (S£ 

may  be  regarded  as  the  points  on  a  right  line  ln.       Obviously, 

Card  JU=c. 
Hence 

ec  =  Card  (g(£  =  c. 

254.  Exponents.  Before  denning  this  notion  let  us  recall  a 
problem  in  the  theory  of  combinations,  treated  in  elementary 
algebra. 

Suppose  that  there  are  7  compartments 

n     n          n 

^ii  v25  *"  ^y> 

and  that  we  have  k  classes  of  objects 


ARITHMETIC   OPERATIONS   WITH   CARDINALS  295 

Let  us  place  an  object  from  any  one  of  these  classes  in  (7r  an 
object  from  any  one  of  these  classes  in  <72---  and  so  on,  for  each 
compartment.  The  result  is  a  certain  distribution  of  the  objects 
from  these  k  classes  K,  among  the  y  compartments  O. 

The  number  of  distributions  of  objects  from  k  classes  among  y 
compartments  is  &. 

For  in  O1  we  may  put  an  object  from  any  one  of  the  k  classes. 
Thus  (7j  may  be  tilled  in  k  ways.  Similarly  (72  may  be  filled  in 
k  ways.  Thus  the  compartments  (Tp  <72  may  be  filled  in  k2  ways. 
Similarly  (7-p  (72,  <73  may  be  filled  in  A?  ways,  etc. 

255.  1.  The  totality  of  distributions  of  objects  from  k  classes 
K  among  the  7  compartments  0  form  an  aggregate  which  may  be 
denoted  by  TTC 

We  call  it  the  distribution  of  K  over  O.  The  number  of  distri 
bution  of  this  kind  may  be  called  the  cardinal  number  of  the  set, 
and  we  have  then  Card  K°  =  & 

2.  What  we  have  here  set  forth  for  finite  0  and  .STmay  be  ex 
tended  to  any  aggregates,  51  =  |a|,  33  =  \b\  whose  cardinal  num 
bers  we  call  a,  b.  Thus  the  totality  of  distributions  of  the  a's 
among  the  5's,  or  the  distribution  of  51  over  93,  is  denoted  by 

21®, 

and  its  cardinal  number  is  taken  to  be  the  definition  of  the  symbol 
ab-     Thus' 


256.    Example  1.     Let 

X*  +   djZ*-1*   >•'    +   «n=   0  (1 

have  rational  number  coefficients.  Each  coefficient  a8  can  range 
over  the  enumerable  set  of  elements  in  the  rational  number 
system  R  =  jr{,  whose  cardinal  number  is  K0.  The  n  coefficients 
form  a  set  21  =  (at,  •••  an)  =  \a\.  To  the  totality  of  equations  1) 
corresponds  a  distribution  of  the  r's  among  the  a's,  or  the  set 

R* 

whose  cardinal  number  is 

K5  =  c». 


296  AGGREGATES 

As  Card  R*  =  *0  =  e 

we  have  the  relation : 

K£  =  K0    ,     or  en  =  e 
for  any  integer  n. 

On  the  other  hand,  the  equations  1)  may  be  associated  with 
the  complex 

(flj,  ...  an), 

and  the  totality  of  equations  1)  is  associated  with 

<£  =  fOi>  •'•  «n)j- 

But  K«i.4)1-f«ii»f*j« 

JOi,  «2'  as)i  =  IOi»  °2){  •  \az\     »     etc. 
N  C^f^^KJvJa.]. 

Card  (£  =  e  •  e  «  ••«  e     ,     n  times  as  factor. 
But  Card  (^  =  Card  J2* 

since  each  of  these  sets  is  associated  uniformly  with  the  equations 

1).     Thus  ..  - 

en  =  e-e--"e     ,     n  times  as  factor. 

257.  Example  2.  Any  point  x  in  m-way  space  $Rm  depends  on 
m  coordinates  xl^  x%,  •••  xm,  each  of  which  may  range  over  the  set 
of  real  numbers  9t,  whose  cardinal  number  is  c.  The  m  coordi 
nates  xl  ...  xm  form  a  finite  set 

I  =(>!,  -..  a;,,). 

Thus  to  $lm  =  \x\  corresponds  the  distribution  of  the  numbers  in 
$R,  among  the  m  elements  of  £,  or  the  set 

K* 

whose  cardinal  number  is 

cm. 

As  Card  M*  =  c 

we  have 

cm  =  c         for  any  integer  m.     (1 
As  in  Example  1  we  show 

cm  =  c  •  c  *  • « •  c     ,     m  times  as  factor. 


ARITHMETIC   OPERATIONS   WITH   CARDINALS  297 

258.  ab+c  =  ab.ac.  (1 

To  prove  this  we  have  only  to  show  that 

and  31s8  •  21s 


can  be  put  in  1-1  correspondence.  But  this  is  obvious.  For 
the  set  on  the  left  is  the  totality  of  all  the  distributions  of  the 
elements  of  51  among  the  sets  formed  of  33  and  (L  On  the  other 
hand,  the  set  on  the  right  is  formed  of  a  combination  of  a  distri 
bution  of  the  elements  of  51  among  the  93,  and  among  the  (£.  But 
such  a  distribution  may  be  regarded  as  the  distribution  first  con 
sidered. 

259.  (a*)'  =  aK  (1 

We  have  only  to  show  that  we  can  put  in  1-1  correspondence 
the  elements  of 

(3158/  and  2l*-e.  (2 

Let  51=  \a\,  33  =  {6j,  6=  \c\.  We  note  that  51s  is  a  union  of 
distributions  of  the  as  among  the  J's,  and  that  the  left  side  of  2) 
is  formed  of  the  distributions  of  these  sets  among  the  c's.  These 
are  obviously  associated  uniformly  with  the  distributions  of  the 
a's  among  the  elements  of  33  •  (L 

260.  1.  cn  =  (mc)n  =  mn*  =  m*  =  c  (1 
where  m,  n  are  positive  integers. 

For  each  number  in  the  interval  &  =  (0,  1*)  can  be  represented 
in  normal  form  once  and  once  only  by 

•  a^a^  •••in  the  ra-adic  system,  (2 

where  the  0  <  as  <  m.         [I,  145]  . 

Now  the  set  of  numbers  2)  is  the  distribution  of  3ft  =(0,  1,  2, 
•  ••  m  —  1)  over  (5  =  (ax,  a2,  «3  •••),  or 


whose  cardinal  number  is 

m< 

On  the  other  hand,  the  cardinal  number  (£  is  C. 


298  AGGREGATES 

Hence,  mc  =  c. 

As  n*  =  e,  we  have  1),  using  1)  in  257. 

2.  The  result  obtained  in  247,  2  may  be  stated: 

V  =  c.  (3 

3.  t*  =  c.  (4 
For  obviously                    ne  <  ec  <  ce. 

But  by  3),  cc  =  c  and  by  1)  n*  =  c. 

261.  1.  The  cardinal  number  t  of  all  functions  f  (xl  •••  xm)  which 
take  on  but  two  values  in  the  domain  of  definition  31,  of  cardinal  num 
ber  a,  is  2  2*. 

Moreover,  2  21  >  a. 

This  follows  at  once  from  the  reasoning  of  249. 

2.  Let  f  be  the  cardinal  number  of  the  class  of  all  functions  de 
fined  over  a  domain  31  whose  cardinal  number  is  c.      Then 

f  =  cc=2c>c.  (1 

For  the  class  of  functions  which  have  but  two  values  in  21  is  by 
1,  2c. 

On  the  other  hand,  obviously 

f  =  cc. 
But 

cc  =  (2e)c,         by  260,  1) 

=  2",  by  259,  1) 

=  2S  by  253,  2). 

Thus,  cc  =  2c. 

That  f  >  c 

follows  from  250,  since  the  class  of  functions  there  considered  lies 
in  the  class  here  considered.  ' 

3.  The  cardinal  number  t  of  the  class  of  limited  integrable  func 
tions  in  the   interval  31  is  =  f,  the   cardinal  number  of  all  limited 
functions  defined  over  31. 


NUMBERS  OF   LIOUVILLE  299 

For  let  &  be  a  Cantor  set  in  51  [I,  272].  Being  discrete,  any 
limited  function  defined  over  £)  is  integrable.  But  by  229,  Ex.  4, 
the  points  of  51  may  be  set  in  uniform  correspondence  with  the 
points  of  £). 

4.  The  set  of  all  functions 

/O)  =/,(*)  +/,(*)+...  (2 

which  are  the  sum  of  convergent  series,  and  whose  terms  are  continu 
ous  in  5(,  has  the  cardinal  number  c. 

For  the  set  g  of  continuous  functions  in  51  has  the  cardinal 
number  c  by  248.  These  functions  are  to  be  distributed  among 
the  enumerable  set  &  of  terms  in  2).  Hence  the  set  of  these 

functions  is  ~ 

u  > 
whose  cardinal  number  is  c 

Remark.  Not  every  integrable  function  can  be  represented  by 
the  series  2). 

For  the  class  of  integrable  functions  has  a  cardinal  number  >  c, 
by  250. 

5.  TJie  cardinal  number  of  all  enumerable  sets  in  an  m-way  space 
Wm  is  c. 

For  it  is  obviously  the  cardinal  number  of  the  distribution  of 
9?m  over  an  enumerable  set  (5,  or 

Card  ft®  =  ce  =  c. 


Numbers  of  Liouville 

262.    In  I,  200  we  have  defined  algebraic  numbers  as  roots  of 
equations  of  the  type 


where  the  coefficients  a  are  integers.  All  other  numbers  in  $ft  we 
said  were  transcendental.  We  did  not  take  up  the  question 
whether  there  are  any  transcendental  numbers,  whether  in  fact, 
not  all  numbers  in  9?  are  roots  of  equations  of  the  type  1). 


o'X'  AGGREGATES 

The  first  to  actually  show  the  existence  of  transcendental  num 
bers  was  Liouville.  He  showed  how  to  form  an  infinity  of  such 
numbers.  At  present  we  have  practical  means  of  deciding 
whether  a  given  number  is  algebraic  or  not.  It  was  one  of  the 
signal  achievements  of  Hermite  to  have  shown  that  e  =  2.71818  ••• 
is  transcendental. 

Shortly  after  Lindemann.  adapting  Hermite's  methods,  proved 
that  TT  =  3.14159  •••  is  also  transcendental.  Thereby  that  famous 
problem  the  Quadrature  of  the  Circle  was  answered  in  the  negative. 
The  researches  of  Hermite  and  Lindemann  enable  us  also  to  form 
an  infinity  of  transcendental  numbers.  It  is,  however,  not  our  pur 
pose  to  give  an  account  of  these  famous  results.  We  shall  limit 
our  considerations  to  certain  numbers  which  we  call  the  numbers 
of  Liouville. 

In  passing  let  us  note  that  the  existence  of  transcendental  num 
bers  follows  at  once  from  285,  2  and  244,  2.  fe  -X  ^  ? 

For  the  cardinal  number  of  the  set  of  real  algebraic  number  is 
e,  and  that  of  the  set  of  all  real  numbers  is  c,  and  c  >  e. 

263.  In  algebra  it  is  shown  that  any  algebraic  number  a  is  a 
root  of  an  irreducible  equation, 


f-  +  <i.  =  o  a 

whose  coefficients  are  integers  without  common  divisor.     We  say 
the  order  of  a  is  ni. 

We  prove  now  the  theorem 


r«  =  ^      ,    Pn*qm  relatively  prime, 
=  a,  an  algebraic  number  of  order  m,  as  n  =  x  .      Then 

]«-r.]>-i_     ,     „>„.  (2 

For  let  a  be  a  root  of  1).     We  may  take  S>0  so  small  that 
/(x)=#=0  in  Dj*(«),  and  *  so  large  that  rn  lies  in  ^(a),  for  n>9. 

,  (3 


NUMBERS   OF   LIOUVILLE  301 

for  n  >  i,  since  the  numerator  of  the  middle  member  is  an  integer, 
and  hence  >  1  . 

On  the  other  hand,  by  the  Law  of  the  Mean  [I, 


where  £  lies  in  !>«<»     Now  /(«)=0   and  /'(£)<   some  M. 
Hence  -,    x        - 

--"^4-  (4 

on  using  3).     Bat  however  large  Jf  in,  there  exists  a  v,  such  that 
qn>M,  for  any  n  >  v.     This  in  4)  gives  2). 

264.    1.    The  numbert 


where  an<  10»,  and  not  aR  of  them  vanish  after  a  certain  index,  are 
transcendental. 

For  if  L  is  algebraic,  let  its  order  be  m.     Then  if  Ln  denotes 
the  sum  of  the  first  n  terms  of  1),  there  exists  a  v  such  that 

^.li-AOjjjjl-     ,     forn>,.  (2 

But  ^  l 

^"lO-'-V:  +  C  10(»+l>»!      '      »»>v;, 

v^  being  taken  sufficiently  large.     But  3)  contradicts  2). 
The  numbers  1)  we  call  the  numbers  of  Lioumtte. 

2.    The  set  of  Lioumlle  numbers  AM  the  cardinal  number  c. 

For  all  real  numbers  in  the  interval  (0*,  1)  can  be  represented 

/i-w+fe+^+-  •  °^9' 

where  not  all  the  6Ts  vanish  after  a  certain  index.     The  numbers 

*- 


can  obviously  be  put  in  uniform  correspondence  with  the  set 
Thus  Card  \\\  =c.  But  \L\  >  }X(,  hence  Card  \L\  >c.  On  the 
other  hand,  the  numbers  \L\  form  only  a  part  of  the  numbers  in 
(0*,  1).  Hence  Card  {L\  <  c. 


CHAPTER   IX 
ORDINAL   NUMBERS 

Ordered  Sets 

265.  An  aggregate  51  is  ordered,  when  a,  b  being  any  two  of 
its  elements,  either  a  precedes  5,  or  a  succeeds  5,  according  to  some 
law  ;  such  that  if  a  precedes  5,  and  b  precedes  <?,  then  a  shall  pre 
cede  c.  The  fact  that  a  precedes  b  may  be  indicated  by 

a<b. 

Then  a>b 

states  that  a  succeeds  b. 

Example  1.     The  aggregates 

1,  2,  3,  ... 
2,4,6,... 


-3,  -2,  -1,0,1,2,3, 


are  ordered. 


Example  2.  The  rational  number  system  R  can  be  ordered  in 
an  infinite  variety  of  ways.  For,  being  enumerable,  they  can  be 

arranged  in  a  sequence      -     «.     * 

ri  •>  ri  '  ra  »  *  "  rn  •  • 

Now  interchange  r^  with  rn.  In  this  way  we  obtain  an  infinity 
of  sequences. 

Example  3.  The  points  of  the  circumference  of  a  circle  may  be 
ordered  in  an  infinite  variety  of  ways. 

For  example,  let  two  of  its  points  Pl,  P2  make  the  angles  a+6r 
a  4-  02  with  a  given  radius,  the  angle  6  varying  from  0  to  2  ?r. 
Let  Pl  precede  P2  when  61  <  02. 

302 


ORDERED   SETS  303 

Example  4>  The  positive  integers  $  may  be  ordered  in  an  infi 
nite  variety  of  ways  besides  their  natural  order.  For  instance,  we 
may  write  them  in  the  order 

1,  3,  5,  ...  2,  4,  6,  -. 

so  that  the  odd  numbers  precede  the  even.     Or  in  the  order 
1,  4,  7,  10,  ...  2,  5,  8,  11,  ...  3,  6,  9,  12,  ... 

and  so  on.  We  may  go  farther  and  arrange  them  in  an  infinity 
of  sets.  Thus  in  the  first  set  put  all  primes ;  in  the  second  set 
the  products  of  two  primes ;  in  the  third  set  the  products  of 
three  primes;  etc.,  allowing  repetitions  of  the  factors.  Let  any 
number  in  set  m  precede  all  the  numbers  in  set  n>m.  The  num 
bers  in  each  set  may  be  arranged  in  order  of  magnitude. 

Example  5.  The  points  of  the  plane  9?2  may  be  ordered  in  an 
infinite  variety  of  ways.  Let  Ly  denote  the  right  line  parallel  to 
the  z-axis  at  a  distance  y  from  this  axis,  taking  account  of  the  sign 
of  y.  We  order  now  the  points  of  9?2  by  stipulating  that  any 
point  on  Lv,  precedes  the  points  on  any  L^,  when  y1  <y" ,  while 
points  on  any  Ly  shall  have  the  order  they  already  possess  on  that 
line  due  to  their  position. 

266.  Similar  Sets.  Let  21,  33  be  ordered  and  equivalent.  Let 
a  ~  b,  a  ~  y3.  If  when  a  <  a  in  21,  b  <  /9  in  33,  we  say  21  is  similar 
to  33,  and  write  or  m 

VI  —  1O' 

Thus  the  two  ordered  and  equivalent  aggregates  are  similar 
when  corresponding  elements  in  the  two  sets  occur  in  the  same 
relative  order. 

Example  1.     Let  ar       100 

g  =  1,  J,  d,  ... 

33  =  a1,  a2,  az,  ••• 

In  the  correspondence  21  ~  33,  let  n  be  associated  with  an.  Then 
31^33- 

Example  2.     Let  or  _  1    9   Q 

VI  —  A,  ^j,  o,  «• 

33=  «x  a2  ...  am,  b1,  52,  b3  «•« 


304  ORDINAL   NUMBERS 

In  the  correspondence  21  ~  33,  let  ar~r  for  r  =  1,  2,  •••  m;  also 
let  bn~m  +  n,n  =  1,  2  •••  Then  51  ^  53. 

Example  3.     Let  91  —  1    9   3 

53  =  ^,  62  •••  a1?  «2  ...  am. 

Let  the  correspondence  between  21  and  53  be  the  same  as  in 
Ex.  2.  Then  21  is  not  similar  to  53.  For  1  is  the  first  element  in 
21  while  its  associated  element  al  is  not  first  in  53. 

Example  4.     Let  w  —  1    9   q 

<\  —  i,  .<£,  o,  •«« 

53=  a1?  «2  •••  6j,  52  ... 
Let  an  ~  2  w,  bn  ~  2  n  -  1.     Then  21  -  53  but  51  is  not  a*  53. 


267.  Let  21  ^53,  53  ^(L     7%^  21  ^  £. 

For  let  a  ~  5,  a'~6'  in  21-53.  Let  b  ~  c,  V  ~  c'  in  53  ~  &.  Let 
us  establish  a  correspondence  21  ~  S  by  setting  a  ~  c,  a!  ~c'  .  Then 
if  a  <a'  in  21,  £<  c'  in  S.  Hence  21  ~  (5. 

Eutactic  Sets 

268.  Let  21  be  any  ordered  aggregate,  and  53  a  part  of  21,  the 
elements  of  53  being  kept  in  the  same  relative  order  as  in  21.    If  21 
and  each  53  both  have  a  first  element,  we  say  that  21  is  well  ordered, 
or  eutactic. 

Example  1.  21  =  2,  3,  •••  500  is  well  ordered.  For  it  has  a  first 
element  2.  Moreover  any  part  of  21  as  6,  15,  25,  496  also  has  a 
first  element. 

Example  2.  21  =  12,  13,  14,  ..-in  inf.  is  well  ordered.  For  it 
has  a  first  element  12,  and  any  part  53  of  21  whose  elements  pre 
serve  the  same  relative  order  as  in  21,  has  a  first  element,  viz. 
the  least  number  in  53. 

The  condition  that  the  elements  of  53  should  keep  the  same  rel 
ative  order  as  in  21  is  necessary.  For  B  =  •••  28,  26,  24,  22,  20, 
21,  23,  25,  27,  ...  is  a  partial  aggregate  having  no  first  element. 
But  the  elements  of  B  do  not  have  the  order  they  have  in  21. 


EUTACTIC   SETS  305 

Example  3.  Let  51  =  rational  numbers  in  the  interval  (0,  1) 
arranged  in  their  order  of  magnitude.  Then  51  is  ordered.  It 
also  has  a  first  element,  viz.  0.  It  is  not  well  ordered  however. 
For  the  partial  set  53  consisting  of  the  positive  rational  numbers  of 
51  has  no  first  element. 

Example  4-  An  ordered  set  which  is  not  well  ordered  may  some 
times  be  made  so  by  ordering  its  elements  according  to  another 
law. 

Thus  in  Ex.  3,  let  us  arrange  51  in  a  manner  similar  to  233. 
Obviously  51  is  now  well  ordered. 

Example  5.  51  =  ar  a2  •  -  b^  b%  •••  is  well  ordered.  For  al  is  the 
first  element  of  51  ;  and  any  part  of  51  as 


has  a  first  element. 

269.  1.  Every  partial  set  53  of  a  well-ordered  aggregate  51  is  well 
ordered. 

For  53  has  a  first  element,  since  it  is  a  part  of  51  which  is  well 
ordered.  If  £  is  a  part  of  53,  it  is  also  a  part  of  51,  and  hence  has 
a  first  element. 

2.  If  a  is  not  the  last  element  of  a  well-ordered  aggregate  51,  there 
is  an  element  of  51  immediately  following  a. 

For  let  53  be  the  part  of  51  formed  of  the  elements  after  a.  It 
has  a  first  element  b  since  51  is  well  ordered.  Suppose  now 

a  <  c  <  b. 

Then  b  is  not  the  first  element  of  53,  as  c  <  b  is  in  53. 

3.  When  convenient  the  element  immediately  succeeding  a  may 
be  denoted  by 

a  +  1. 

Similarly  we  may  denote  the  element  immediately  preceding  a, 
when  it  exists,  by 

a-1. 


306  ORDINAL  NUMBERS 

For  example,  let 

5(  =  a^a2  •'•  5j£>2  ••' 
Then  an+l  =  an+1     ,     bm  +  1  =  bm+1 

an—l  =  an-l        »        bm—  l  =  bm_v 

There  is,  however,  no  b1  —  1. 

270.  1.  If  51  is  well  ordered,  it  is  impossible  to  pick  out  an  in 
finite  sequence  of  the  type 

a1  >  a2  >  a3  >  •••  (1 

For  ™ 

20  =  •••  a8,  0^,  Oj 

is  a  part  of  51  whose  elements  occur  in  the  same  relative  order  as 
in  51,  and  33  has  no  first  element. 

2.  A  sequence  as  1)  may  be  called  a  decreasing  sequence,  while 

a1  <  a2  <  as  ... 
may  be  called  increasing. 

In  every  infinite  well  ordered  aggregate  there  exist  increasing 
sequences. 

3.  Let  51,  33,  (£,  •••  be  a  well  ordered  set.     Let  5l  =  .JaJ  be  well 
ordered  in  the  a's,  -53  =  \b\  be  well  ordered  in  the  b's,  etc.      The  set 

U  =  Sl,  «,  6  - 
is  well  ordered  with  regard  to  the  little  letters  a,  b 

For  U  has  a  first  element  in  the  little  letters,  viz.  the  first  ele 
ment  of  51.  Moreover,  any  part  of  U,  as  S3,  has  a  first  element  in 
the  little  letters.  For  if  it  has  not,  there  exists  in  33  an  infinite 
decreasing  sequence 

t  >  s  >  r  >  ••• 

This,  however,  is  impossible,  as  such  a  sequence  would  deter 
mine  a  similar  sequence  in  U  as 

£><S>ft  >  ••• 

which  is  impossible  as  U  is  well  ordered  with  regard  to  21,  33  ••• 

4.  Let  9l<33<£<  -..  (1 
Let  each  element  of  51  precede  each  element  of  33,  etc. 


SECTIONS  307 


Let  each  51,  33,  •••  be  well  ordered. 

Let 


&  =  %  +  £+  C+   .- 

is  a  well   ordered  set,  3  preserving  the  relative  order  of  elements 
intact. 

For  @  has  a  first  element,  viz.  the  first  element  of  51.  Any 
part  S  of  &  has  a  first  element.  For,  if  not,  there  exists  in  @ 
an  infinite  decreasing  sequence 

r  >  q>  p  >  •••  (2 

Now  r  lies  in  some  set  of  1)  as  9?.  Hence  <?,  jt?,  •••  also  lie  in 
Sft.  But  in  $ft  there  is  no  sequence  as  2). 

5.  Let  5(,  23,  S,  •••  be  an  ordered  set  of  well  ordered  aggre 
gates,  no  two  of  which  have  an  element  in  common.  The  reader 
must  guard  against  assuming  that  51  +  33  +  Q[  +  •••»  keeping  the 
relative  order  intact,  is  necessarily  well  ordered. 

For  let  us  modify  Ex.  5  in  265  by  taking  instead  of  all  the 
points  on  each  Lv  only  a  well  ordered  set  which  we  denote  by  5lj,- 

Then  the  sum  0,      Var 

21  =  <fcflg 

has  a  definite  meaning.     The  elements  of  51  we  supposed  arranged 
as  in  Ex.  5  of  265. 

Obviously  51  is  not  well  ordered. 


Sections 

271.  We  now  introduce  a  notion  which  in  the  theory  of  well- 
ordered  sets  plays  a  part  analogous  to  Dedekind's  partitions  in 
the  theory  of  the  real  number  system  $ft.  Cf.  I,  128. 

Let  51  be  a  well  ordered  set.  The  elements  preceding  a  given 
element  a  of  51  form  a  partial  set  called  the  section  of  51  generated 
by  a.  We  may  denote  it  by 

So, 

or  by  the  corresponding  small  letter  a. 


308  ORDINAL   NUMBERS 

Example  1.     Let  51  =  1   2  3 

Then 

£100=1,  2,  -99 

is  the  section  of  51  generated  by  the  element  100. 

Example  2.     Let 

51  =  1^,  a2--.  6j,  b2-> 
Then 

Sb5  =  ala2'"blb2b3b4i 

is  the  section  generated  by  b5. 

tSb-^  =  a^a^  •  •  • 
that  generated  by  b1,  etc. 

272.    1.  Every  section  of  a  well  ordered  aggregate  is  well  ordered. 
For  each  section  of  51  is  a  partial  aggregate  of  51,  and  hence 
well  ordered  by  269,  1. 

2.  In  the  well  ordered  set  51,  let  a<b.      Then  Sa  is  a  section 
ofSb. 

3.  Let  @  denote  the    aggregate    of  sections   of  an   infinite   well 
ordered  set  51.     If  we  order  ©  such  that  Sa  <  Sb  in  ©  wAew  a  <  b  in 
51,  @  is  well  ordered. 

For  the  correspondence  between  51  and  @  is  uniform  and  similar. 


273.  ie£   51,    93    fo   we#   ordered   and   51^33.      If  a^b,    then 

Sa  ~  £6. 

For   in   51   let   a"<a'>a.     Let    b'  ~  a1    and   b"^an.     Since 

51  ^  53,  we  have 

&"<£'<&; 
hence  the  theorem. 

274.  If  51  is  well  ordered,  51  is  not  similar  to  any  one  of  its 
sections. 

For  if  51  ^  Sa,  to  a  in  51  corresponds  an  element  a1  <  a  in  Sa. 
To  al  in  51  corresponds  an  element  a2  in  Sa,  etc.  In  this  way  we 
obtain  an  infinite  decreasing  sequence 

a>  a1>a2>  •••, 
which  is  impossible  by  270,  1. 


SECTIOXS  309 

275-  Let  51,  53  be  well  ordered  and  51  =*  53.  2%ew  to  #a  w  31  can 
not  correspond  two  sections  Sb,  S/3  each  ^  $a. 

For  let  b  <  &  and  £a  ^  £6,  £a  ^  /SJS.     Then 

Sb  a*  $8,         by  267.  (1 

But  1)  contradicts  274. 

276.  Let  51,  53  be  two  well  ordered  aggregates.     It  is  impossible 
to  establish  a  uniform  and  similar  correspondence  betiveen  51  and  53 
in  more  than  one  way. 

For  say  Sa  ^  Sb  in  one  correspondence,  and  Sa  ^  S/3  in  an 
other,  b,  /3  being  different  elements  of  53.  Then 

Sb  ^  Sfr         by  267. 
This  contradicts  275. 

277.  1.    We  can  now  prove  the  following  theorem,  which  is 
the  converse  of  273. 

Let  51,  53  be  well  ordered.  If  to  each  section  of  81  corresponds  one 
similar  section  of  53,  and  conversely,  then  53  —  51. 

Let  us  first  show  that  51  ~  53.  Since  to  any  Sa  of  51  corre 
sponds  a  similar  section  Sb  in  53,  let  us  set  a  ~  b.  No  other 
a1  ~  5,  and  no  other  b'  ~  a,  as  then  Sa'  ^  Sb  or  Sb'  ^  Sa,  which 
contradicts  274.  Let  the  first  element  of  51  correspond  to  the 
first  of  53.  Thus  the  correspondence  we  have  set  up  between  21 
and  53  is  uniform  and  51  ~  53. 

We  show  now  that  this  correspondence  is  similar.     For  let 

a  ~  b  and  a'  ~~  b',  a'  <  a. 

Then  b'  <  b.     For  a'  lies  in  Sa  ^  Sb  and  br  —  a'  lies  in  Sb. 
2.    From  1  and  273  we  have  now  the  fundamental  theorem  : 

In  order  that  two  well-ordered  sets  51,  53  be  similar,  it  is  necessary 
and  sufficient  that  to  each  section  of  51  corresponds  a  similar  section 
of  53,  and  conversely. 

278.  Let  51,  53  be  well  ordered.     If  to  each,  section  of  51  corre 
sponds  a  similar  section  of  53i  but  not  conversely,  then  5(  is  similar  to 
a  section  of  53. 


310  ORDINAL  NUMBERS 

Let  us  begin  by  ordering  the  sections  of  51  and  53  as  in  272,  3. 
Let  B  denote  the  aggregate  of  sections  of  53  to  which  similar  sec 
tions  of  51  do  not  correspond.  Then  B  is  well  ordered  and  has  a 
first  section,  say  Sb.  Let  /9  <  b.  Then  to  <S/3  in  53  corresponds 
by  hypothesis  a  similar  section  Sa  in  5L  On  the  other  hand,  to 
any  section  Sa'  of  51  corresponds  a  similar  section  Sb'  of  53.  Ob 
viously  b'  <  b.  Thus  to  any  section  of  51  corresponds  a  similar 
section  of  Sb  and  conversely.  Hence  51^>S7>  by  277,  1. 

279.  Let  51,  53  be  well  ordered.     Either  5t  is  similar  to  53  or  one 
is  similar  to  a  section  of  the  other. 

For  either : 
1°   To  each  section  of  51  corresponds  a  similar  section  of  53 

and  conversely ; 
or  2°    To  each  section  of  one  corresponds  a  similar  section  of 

the  other  but  not  conversely ; 

or  3°   There  is  at  least  one  section  in  both  51  and  53  to  which  no 
similar  section  corresponds  in  the  other. 

If  1°  holds,  51  =*  53  by  277,  1.  If  2°  holds,  either  51  or  53  is  similar 
to  a  section  of  the  other. 

We  conclude  by  showing  3°  is  impossible. 

For  let  A  be  the  set  of  sections  of  51  to  which  no  similar  section 
in  53  corresponds.  Let  B  have  the  same  meaning  for  53.  If  we 
suppose  51,  53  ordered  as  in  272,  3,  A  will  have  a  first  section  say 
Sa,  and  B  a  first  section  Sft. 

Let  a  <  a.  Then  to  Sa  in  51  corresponds  by  hypothesis  a  sec 
tion  Sb  of  Sfl  as  in  278.  Similarly  if  b'  <  #,  to  Sb'  of  53  corre 
sponds  a  section  Sa'  of  Sa.  But  then  Sa^-Sft  by  277,  l,  and  this 
contradicts  the  hypothesis. 

Ordinal  Numbers 

280.  1.    With  each  well  ordered  aggregate  51  we  associate  an 
attribute  called  its  ordinal  number,  which  we  define  as  follows  : 

1°    If  5(^53,  they  have  the  same  ordinal  number. 
2°    If  5t  2-a  section  of  53,  the  ordinal  number  of  5(  is  less  than 
that  of  53. 


ORDINAL   NUMBERS  311 

3°   If  a  section  of  51  is  ^  23,  the  ordinal  number  of  51  is  greater 
than  that  of  S3. 

The  ordinal  number  of  5(  may  be  denoted  by 

Orel  51, 

or  when  no  ambiguity  can  arise,  by  the  corresponding  small  letter  a. 
As  any  two  well  ordered  aggregates  51,  53  fall  under  one  and  only 
one  of  the  three  preceding  cases,  any  two  ordinal  numbers  a,  b 
satisfy  one  of  the  three  following  relations,  and  only  one,  viz.  : 

a  =  b     ,     a<b     ,     a>b, 
and  if  a  <  b,  it  follows  that  b  >  a- 

Obviously  they  enjoy  also  the  following  properties. 

2  If 

J  a  =  b     ,     b  =  c     ,     then  a  =  c. 

For  if  c  =  Ord  £,  the  first  two  relations  state  that 

• 

31^33    ,    SB^S. 
But  then  ^g    t    by267_ 

Hence 

n  =  c. 

3  If 

J  a  >  b     ,     b  >  c     ,     then  a  >  c. 

281.    1.    Let  51  be  a  finite  aggregate,  embracing  say  n  elements. 

Then  we  set  ~    -,  w 

Ord  51  =  n. 

Thus  the  ordinal  number  of  a  finite  aggregate  has  exactly  similar 
properties  to  those  of  finite  cardinal  numbers.  The  ordinal  num 
ber  of  a  finite  aggregate  is  called  finite,  otherwise  transfinite. 

The  ordinal  number  belonging  to  the  well  ordered  set  formed 
of  the  positive  integers  •  c\  _  1  9  Q 

x)    —   ^   ^->    **l    "* 

we  call  co. 

2.    The  least  transfinite  ordinal  number  is  co. 

For  suppose  a  =  Ord  51  <  co,  is  transfinite.  Then  51  is  ^  a 
section  of  Q.  But  every  section  of  $  is  finite,  hence  the 
contradiction. 


312  ORDINAL   NUMBERS 

3.  The  cardinal  number  of  a  set  51  is  independent  of  the  order 
in  which  the  elements  of  51  occur.  This  is  not  so  in  general  for 
ordinal  numbers. 

For  example,  let      Qr      -,    0   Q 

&SS    1,    Z,   $,   «•• 

33=1,3,5,...  2,4,6,  ... 
Here  Card  1  =  Card  %  =  K0. 

But  Ord  21  <  Ord  33, 

since  51  is  similar  to  a  section  of  33,  viz.  the  set  of  odd  numbers, 
1,  3,  5,  ... 

282.  1.  Addition  of  Ordinals.  Let  51,  33  be  well  ordered  sets 
without  common  elements.  Let  (£  be  the  aggregate  formed  by 
placing  the  elements  of  33  after  those  of  51,  leaving  the  order  in  33 
otherwise  unchanged.  Then  the  ordinal  number  of  (£  is  called  the 

sum  of  the  ordinal  numbers  of  51  and  33,  or 

• 

Ord  <£  =  Ord  51  +  Ord  33, 
or  c  =  a  +  b. 

The  extension  of  this  definition  to  any  set  of  well-ordered  aggre 
gates  such  that  the  result  is  well  ordered  is  obvious. 

2.  We  note  that          a  +  j  >  „,         a  +  f,  >  b.  .      .        . 

For  51  is  similar  to  a  section  of  (£,  and  33  is  equivalent  to  a  part 
of  ft 

3.  The  addition  of  ordinal  numbers  is  associative. 

This  is  an  immediate  consequence  of  the  definition  of  addition. 

4.  The  addition  of  ordinal  numbers  is  not  always  commutative. 
Thus  if      a=  (^2...  in  inf.),  Ord  5i  =  *>, 

33  =  (^2  ...  5n),  Ord  33  =  rc; 

let 


$)=:(&!...  bnafy  ..-),  Ord£) 

Then  c  =  a  +n     ,     b  =  ™  +  &>. 


ORDINAL   NUMBERS  313 

But  51  —  a  section  of  (5,  viz.  :    ^  ^S^,  while  £)  ^  51.     Hence 

a  <  c     ,     «  =  b, 
<w  +  n  >  &>     ,     n  +  a)  =  a). 


5.    Tjf  a  >  b,  fAett  c  -f  a  >  c  -f  b,  and  a  +  c  >  b  4-  c. 
For  let         a  =  Ord  5(,        b  =  Ord  33,         c  =  Ord  (L 
Since  a  >  b,  we  can  take  for  53  a  section  Sb  of  51.     Then  c  -f  a  is 

the  ordinal  number  of         AT   ,   or  /^i 

^  +  zl?  V-L 

and  c  +  b  is  the  ordinal  number  of 

6  +  Sb,  (2 

preserving  the  relative  order  of  the  elements. 

But  2)  is  a  section  of  1),  and  hence  c  +  a  >  c  -h  b. 
The  proof  of  the  rest  of  the  theorem  is  obvious. 

283.    1.    The  ordinal  number  immediately  following  a  is  a  +  1. 

For  let  a  =  Ord  51.  Let  53  be  a  set  formed  by  adding  after  all 
the  elements  of  51  another  element  b.  Then 

a  +  1  =  Ord  53  =  b. 
Suppose  now 

a<c<b     ,     c=Ord£.  (1 

Then  (5  is  similar  to  a  section  of  53.  But  the  greatest  section 
of  53  is  Sb  =  51.  Hence 

c  <  a, 
which  contradicts  1). 

2.    Let  a  >  b.      Then  there  is  one  and  only  one  ordinal  number  b 

such  that  ,       , 

a  =  D  +  o. 

Forlet  a  =  Ord  51     ,     b  =  Ord53. 

We  may  take  53  to  be  a  section  Sb  of  51.  Let  X)  denote  the  set 
of  elements  of  51,  coming  after  Sb.  It  is  well  ordered  and  has  an 
ordinal  number  b-  Then 

3l  =  53  +  £), 

preserving  the  relative  order,  and  hence 

a  =  b  +  b. 
There  is  no  other  number,  as  282,  5  shows. 


314  ORDINAL   NUMBERS 

284.  1.  Multiplication  of  Ordinals.  Let  51,  53  be  well-ordered 
aggregates  having  a,  b  as  ordinal  numbers.  Let  us  replace  each 
element  of  51  by  an  aggregate  ^  53.  The  resulting  aggregate  (£ 

we  denote  by  «*    w 

53  •  21. 

As  (5  is  a  well-ordered  set  by  270,  3  it  has  an  ordinal  number  c. 
We  define  now  the  product  b  •  a  to  be  c,  and  write 

b  •  a  =  c. 

We  say  c  is  the  result  of  multiplying  a  by  b,  and  call  a,  b  factors. 
We  write 

a  «  a  =  a2    ,     a  •  a  •  a  =  a3    ,     etc. 

2.  Multiplication  is  associative. 

This  is  an  immediate  consequence  of  the  definition. 

3.  Multiplication  is  not  always  commutative. 
For  example,  let 


53  =  (1,  2,  3  ...  in  inf.). 

-L  llGH  fv\  CYf  /•  7      7       7 


Hence       Ord  (53  •  51)  =  a,  .  2  >  o>, 

Ord(H«53)=  2  &>  =  &). 
4.   If  a  <  b,  ^ew  ca  <  cb. 
For  (5  •  51  is  a  section  of  £  •  53. 


Limitary  Numbers 

285.    1.    £«« 

al<  «2<«3<  ...  ( 

&e  «n  infinite  increasing  enumerable  sequence  of  ordinal  numbers 
There  exists  a  first  ordinal  number  a  greater  than  every  an. 

J-^v3u  /~\        i    rw" 

an=  Ord5ln. 


LIMITARY  NUMBERS  315 

Since  an_i  <  «n,  2ln_!  is  similar  to  a  section  of  2ln.     For  simplicity 
we  may  take  2ln_!  to  be  a  section  of  2ln.     Let,  therefore, 


Consider  now  w      qr        ™        ™ 

21  =  Slj  +  *B2  +  £}g  +  ... 

keeping  the  relative  order  of  the  elements  intact.     Then  21  is  well 
ordered  and  has  an  ordinal  number  «. 
As  any  5ln  is  a  section  of  21, 

«„<«. 

Moreover  any  number  y8<«  is  also  <  some  am.  For  if  33  has 
the  ordinal  number  &  33  must  be  similar  to  a  section  of  21.  But 
there  is  no  last  section  of  21. 

2.  The  number  a  we  have  just  determined  is  called  the  limit  of 
the  sequence  1).      We  write 

a  =  Km  an     ,     or  an  =  a. 

We  also  say  that  a  corresponds  to  the  sequence  1). 
All  numbers  corresponding  to   infinite   enumerable   increasing 
sequences  of  ordinal  numbers  are  called  limitary. 

3.  If  every  an  in  1)  is  <  &  then  a  <  ft. 

For  if  £<  a,  a  is  not  the  least  ordinal  number  greater  than 
every  «n. 

4.  If  /3<«,  fi  is  <  some  an. 

286.    In  order  that  n 

' 


define  the  same  number  \   it  is  necessary  and  sufficient  that  each 
number  in  either  sequence  is  surpassed  by  a  number  in  the  other. 

For  let  .  o    •   Q 

an  =  a     ,     pn—  p- 

If  no  Pn  is  greater  than  «TO,     /3  <  «m  <  a,  by  285,  3,  and  «  =£  /3. 
On   the   other  hand,  if  each  «m<    some  /3n,  a</3.     Similarly 


316  ORDINAL   NUMBERS 

287.  Cantor's  Principles  of  Generating  Ordinals.  We  have  now 
two  methods  of  generating  ordinal  numbers.  First,  by  adding  1 
to  any  ordinal  number  a.  In  this  way  we  get 

a,  a  +  1,  a  +2,  ... 

Secondly,  by  taking  the  limit  of  an  infinite  enumerable  increas 
ing  sequence  of  ordinal  numbers,  as 

«!  <  «2  <  «3  <  "• 

Cantor  calls  these  two  methods  the  first  and  second  principles 
of  generating  ordinal  numbers. 

Starting  with  the  ordinal  number  1,  we  get  by  successive  appli 
cations  of  the  first  principle  the  numbers 

1,2,3,4,... 

The  limit  of  this  sequence  is  co  by  285,  l.  Using  the  first  prin 
ciple  alone,  this  number  would  not  be  attained  ;  to  get  it  requires 
the  application  of  the  second  principle.  Making  use  of  the  first 
principle  again,  we  obtain 

<w  +  l,         a>  +  2,         w  +  3,  ... 

The  second  principle  gives  now  the  limitary  number  CD  -f  o>  =  a>2 
by  285,  1.  From  this  we  get,  using  the  first  principle,  as  before, 

tt>2  +  l,         6)2  +  2,         0)2  +  3,... 
whose  limit  is  ft)3.     In  this  way  we  may  obtain  the  numbers 

com  +  n     ,     m,  n  finite. 
The  limit  of  any  increasing  sequence  of  these  numbers  as 

CO        ,        ft)  2        ,        ft)3        ,        0)4:,    «•• 

is  a)  «  ft)  =  a)2,  by  285,  1. 

From  a)2  we  can  get  numbers  of  the  type 

caPl  +  com  4-  n         Z,  m,  n  finite. 

Obviously  we  may  proceed  in  this  way  indefinitely  and  obtain 
all  numbers  of  the  type 


where  a0,  al  •>•  an  are  finite  ordinals. 


LIMITARY  NUMBERS  317 

But  here  the  process  does  not  end.     For  the  sequence 

O)  <   ft)2  <  O)3  <    ••• 

has  a  limit  which  we  denote  by  &)w. 
Continuing  we  obtain 

(i)"™,     ft)""  ,     etc. 

288.  It  is  interesting  to  see  how  we  may  obtain  well  ordered 
sets  of  points  whose  ordinal  numbers  are  the  numbers  just  con 
sidered. 

In  the  unit  interval  51  =  (0,  1),  let  us  take  the  points 

•  :•*.'..  t  »  * '»  if--  .a 

These  form  a  well  ordered  set  whose  ordinal  number  is  to. 
The  points  1)  divided  51  into  a  set  of  intervals, 

*!    ,    «a    ,     213-  (2 

In  m  of  these  intervals,  let  us  take  a  set  similar  to  1).  This 
gives  us  a  set  whose  ordinal  number  is  com. 

In  each  interval  2),  let  us  take  a  set  similar  to  1).  This  gives 
us  a  set  whose  ordinal  number  is  &>2.  The  points  of  this  set 
divide  51  into  a  set  of  o>2  intervals.  In  each  of  these  intervals, 
let  us  take  a  set  of  points  similar  to  1).  This  gives  a  set  of 
points  whose  ordinal  number  is  &>3,  etc. 

Let  us  now  put  in  5Ij  a  set  of  points  33X  whose  ordinal  number 
is  co.  In  512  let  us  put  a  set  332  whose  ordinal  number  is  o>2,  and 
so  on,  for  the  other  intervals  of  2). 

We  thus  get  in  51  the  well  ordered  set 

#  =  2^  +  ®a  +  88  +  - 
whose  ordinal  number  is  the  limit  of 

CO        ,        ft)  4-   CO2       ,        CO  +    CO2  +    CO3       ,       ... 

This  by  286  has  the  same  limit  as 

a)     ,     co2     ,     w3     ,     •••     or     co". 

With  this  set  we  may  now  form  a  set  whose  ordinal  number  is 
o)wft>,  etc. 


318  ORDINAL   NUMBERS 

Classes  of  Ordinals 

289.    Cantor  has  divided  the  ordinal  numbers  into  classes. 

Class  1,  denoted  by  Z^  embraces  all  finite  ordinal  numbers. 

Class  2,  denoted  by  Z2,  embraces  all  transfinite  ordinal  numbers 
corresponding  to  well  ordered  enumerable  sets  ;  that  is,  to  sets 
whose  cardinal  number  is  K0  .-  For  this  reason  we  also  write 


It  will  be  shown  in  293,  1  that  Z^  is  not  enumerable.     Moreover 

if  we  set  ~     ,  „ 

K!  =  Card  Z2  , 

there  is  no  cardinal  number  between  K0  and  Kj  as  will  be  shown  in 
294.  We  are  thus  justified  in  saying  that  Class  3,  denoted  by 
Z%  or  ^(Kj),  embraces  all  ordinal  numbers  corresponding  to  well 
ordered  sets  whose  cardinal  number  is  Kj,  etc. 

Let  j3  =  Ord  33  be  any  ordinal  number.  Then  all  the  numbers 
a  <  0  correspond  to  sections  of  33.  These  sections  form  a  well 
ordered  set  by  272,  3.  Therefore  if  we  arrange  the  numbers 
«  <  /3  in  an  order  such  that  a1  precedes  a  when  Sa'  <  Sa,  they  are 
well  ordered.  We  shall  call  this  the  natural  order.  Then  the 
first  number  in  Z-^  is  1,  the  first  number  of  Z%  is  at.  The  first 
number  in  Z3  is  denoted  by  H. 

290.  As  the  numbers  in  Class  1  are  the  positive  integers,  they 
need  no  comment  here.     Let  us  therefore  turn  to  Class  2. 

If  a  is  in  Z2  ,  so  is  a  -f  1  • 

For  let  a  =  Ord  51.  Let  53  be  the  well  ordered  set  obtained 
by  placing  an  element  b  after  all  the  elements  of  21.  Then 

a  +  1  =  Ord  53. 

But  53  is  enumerable  since  31  is. 
Hence  a  -f  1  lies  in  Z%  . 

291.  Let  •^«1<«2<«3<... 

be  an  enumerable  infinite  set  of  numbers  in  Z2.  Then  a  =  lim  an  lies 
in  Z2. 


CLASSES  OF  ORDIXALS  319 

For  using  the  notation  employed  in  the  proof  of  285,  1,  a  is  the 
ordinal  number  of 

«=«!  +  »,  +  »,+  ••• 

But  2lr  SBj,  332"*  are  eacn  enumerable. 

Hence  21  is  enumerable  by  235,  1,  and  a  lies  in  Zv 

292.  We  prove  now  the  converse  of  290  and  291. 

Each  number  a  in  Z^,  except  &>,  is  obtained  by  adding  1  to  some 
number  in  Z%;  or  it  is  the  limit  of  an  infinite  enumerable  increasing 
set  of  numbers  in  Z^ 

For,  let  a  =  Ord  21.  Suppose  first,  that  21  has  a  last  element, 
say  a.  Since  21  is  enumerable,  so  is  Sa.  Hence 

yS=Ord  -  Sa 
is  in  Z%.     Then  a=  8  +  1 

Suppose  secondly,  that  21  has  no  last  element.  All  the  numbers 
ft  <  a  in  Z%  belong  to  sections  of  21.  Since  21  is  enumerable,  the 
numbers  ft  are  enumerable.  Let  them  be  arranged  in  a  sequence 

/?!,  /32,  /V"  C1 

Since  they  have  no  greatest,  let  $[  be  the  tirst  number  in  it 
>/?!,  let  ft%  be  the  first  number  in  it  >  ft{,  etc.  We  get  thus  the 
sequence  ^  ^<^<  ...  (2 

whose  limit  is  X,  say. 

Then  X  =  «.  For  X  is  >  any  number  in  1),  which  embraces  all 
the  numbers  of  Z^  <  a.  Moreover  it  is  the  least  number  which 
enjoys  this  property. 

293.  1.    The  numbers  of  Z2  are  not  enumerable. 

For  suppose  they  were.     Let  us  arrange  them  in  the  sequence 

«i»  «a»  as  •"  C1 

Then,  as  in  292,  there  exists  in  this  sequence  the  infinite  enu- 
merable  sequence  ^  < «;  <  «^  <  . . .  (2 

such  that  there  are  numbers  in  2)  greater  than  any  given  number 
in  1). 


320  ORDINAL   NUMBERS 

Let  <  =  «'.  Then  a'  lies  in  Z2  by  291.  On  the  other  hand,  by 
285,  a'  is  >  any  number  in  2),  and  therefore  >  any  number  in 
1).  But  1)  embraces  all  the  numbers  of  Z2,  by  hypothesis.  We 
are  thus  led  to  a  contradiction. 

2.   We  set 


294.  There  is  no  cardinal  number  between  K0  and  $r 

For  let  «=Card  5(  be  such  a  number.  Then  5Hs  ~  an  infinite 
partial  aggregate  of  Z%,  which  without  loss  of  generality  may  be 
taken  to  be  a  section  of  Z^.  But  every  such  section  is  enumer 
able.  Hence  51  is  enumerable  and  «=X0,  which  is  a  contradiction. 

295.  We  have  just  seen  that  the  numbers  in  Z2  are  not  enumer 
able.     Let  us  order  them  so  that  each  number  is  less  than  any 
succeeding  number.     We  shall  call  this  the  natural  order. 

1.  The  numbers  of  Z%  when  arranged  in  their  natural  order  form 
a  well  ordered  set. 

For  Z%  has  a  first  element  co.  Moreover  any  partial  set  Z,  the 
relative  order  being  preserved,  has  a  first  element.  For  if  it  has 
not,  there  exists  an  infinite  enumerable  decreasing  sequence 


This,  however,  is  not  possible.     For  /3,  7,  •••  form  a  part  of  Sa 
which  is  well  ordered. 

There  is  thus  one  well  ordered  set  having  Xj  as  cardinal  num- 

ber-    Let 


Let  now  51  be  an  enumerable  well  ordered  set  whose  ordinal 

number  is  a.     The  set  ^       w 

^2  4-  «i 

the  elements  of  51  coming  after  Z^,  has  the  cardinal  number  Kj  by 
241,  3.  It  is  well  ordered  by  270,  3.  It  lias  therefore  an  ordinal 
number  which  lies  in  Z3,  viz.  n  -f  «  by  282,  l.  Thus  Z3  embraces 
an  infinity  of  numbers. 

2.    The  least  number  in  Z%  is  H. 

For  to  any  number  a<  H  corresponds  a  section  51  of  Z^.     Hence 
a  lies  in  Z 


CLASSES   OF   ORDINALS 


321 


296.    1.    An  aggregate  formed  of  an  Kj  set  of  ^1  sets  is  an  Kj  set. 
Consider  the  set 


A  = 


la 


«< 


Here  each  row  is  an  ^  set.  As  there  are  an  Kx  set  of  rows,  A 
is  an  Kj  set  of  Xj  sets.  To  show  that  A  is  an  ^  set,  we  associate 
each  allt  with  some  number  in  the  first  two  number  classes. 

In  the  first  place  the  elements  alK  where  i  tc  <  o>  may  be  associ 
ated  with  the  numbers  1,  2,  3,  •••  <  <w.  The  elements  al<0,  aM 
lying  just  inside  the  &>th  square  and  which  are  characterized 
by  the  condition  that  i  =  1,  2,  •••  o>;  /c=l,  2  •••  <  o>  form  an 
enumerable  set  and  may  therefore  be  associated  with  the  ordinals 
co,  o>  +  1,  •••  <  G)2.  For  the  same  reason  the  elements  just  inside 
the  a)  +  1st  square  may  be  associated  with  the  ordinals  o>2,  o>2  +  1, 
...  <  6)3.  In  this  way  we  may  continue.  For  when  we  have 
arrived  at  the  «th  row  and  column  (edge  of  the  ath  square)  we 
have  only  used  up  an  enumerable  set  of  numbers  in  the  sequence 

i,  2,  ...  a,...  <n  (i 

in  our  process  of  association.     There  are  thus  still  an  Kx  set  left 
in  1)  to  continue  the  process  of  association. 

2.    As  a  corollary  of  1  we  have  : 
The  ordinal  numbers 

n2,      n3,      o4,  ... 

lie  in  Z~  . 


297.    I.    Let  a  <  /3  <  7  <  ••• 

be  an  increasing  sequence  of  numbers  in  Z3  having 


(1 

as  cardinal 

number    and    such    that  any  section  of  1)   has  K0  as    its  cardinal. 
There  exists  a  first  ordinal  number  \  in  Z3  greater  than  any  number 
in  1). 
For  let 


=  Ord 


7=Ord6  — 


322  ORDINAL   NUMBERS 

Since  a  <  /3  we  may  take  51  to  be  a  section  of  53.  Similarly 
we  may  suppose  53  is  a  section  of  (£,  etc. 

Let  now  %  =  %  +  B,         <5  =  »+(7,... 

Consider  now  8  =  « +  .B+ (7+  - 

keeping  the  relative    order  intact.     Then  8  is  well   ordered  by 
270,  4.     Let 

X  =  Ord  8. 

Since  Card  8  =  Kx,  by  296,  1,  X  lies  in  Z3. 
As  any  51,  53,  •••  is  a  section  of  8, 

«<  /3<  •••  <  X. 

Moreover,  any  number  n  <  X  is  also  <  some  a,  /3,  7  •••  For  if 
9ft  has  ordinal  number  /A,  9ft  must  be  similar  to  a  section  of  8. 
But  there  is  no  last  section  in  8. 

2.  We  shall  call  sequences  of  the  type  1),  an  Kj  sequence. 
The  number  X  whose  existence  we  have  just  established,  we  shall 
call  the  limit  ofV).  We  shall  also  w^rite 

a  <  @<  7  •••  =X 
to  indicate  that  a,  /3,  •••  is  an  Kj  sequence  whose  limit  is  X. 

298.  1.  The  preceding  theorem  gives  us  a  third  method  of 
generating  ordinal  numbers.  We  call  it  the  third  principle. 

We  have  seen  that  the  first  and  second  principles  suffice  to  gen 
erate  the  numbers  of  the  first  two  classes  of  ordinal  numbers  but 
do  not  suffice  to  generate  even  the  first  number,  viz.  O  in  Z3.  We 
prove  now  the  following  fundamental  theorem  : 

2.  The  three  principles  already  described  are  necessary  and  suffi 
cient  to  generate  the  numbers  in  Z3. 

For  let  a  =  Ord  be  any  number  of  Z3.  If  31  has  a  last  element, 
reasoning  similar  to  292,  i  shows  that 

«  =  £  +  1. 

If  51  has  no  last  element,  all  the  numbers  of  Z3<a  form  an  X0 
or  K  set.  In  the  former  case 


CLASSES  OF  ORDINALS  323 

where  ft  lies  in  Z2.     In  the  latter  case,  reasoning  similar  to  292,  l 
shows  that  we  can  pick  out  an  Kj  increasing  sequence 


299.  1.    The  numbers  of  Z3  form  a  set  whose  cardinal  number  a 
is  >Kr 

The  proof  is  entirely  similar  to  293,  1.  Suppose,  in  fact,  that 
a  =  Kj  .  Let  us  arrange  the  elements  of  Z3  in  the  Kx  sequence 

«i     ,     «2  •••««•••  «n  •••  (1 

As  in  292,  there  exists  in  this  sequence  an  ^  increasing  sequence 

a[<ai<  .-.  -«'.  (2 

Then  «'  lies  in  Z%  by  297,  l.  On  the  other  hand  ex!  is  greater  than 
any  number  in  2)  and  hence  greater  than  any  number  in  1). 
But  1)  embraces  all  the  numbers  in  Z3  by  hypothesis.  We  are 
thus  led  to  a  contradiction. 

2.  We  set  K2 

3.  There  is  no  cardinal  number  between  Kj  and  K2  . 

For  let  a  =  Card  51  be  such  a  number.  Then  31  is  equivalent  to 
a  section  of  Z3.  But  every  such  section  has  the  cardinal  num 
ber  Xr 

300.  The  reasoning  of  the    preceding  paragraphs  may  be  at 
once  generalized.      The  ordinal  numbers  of  Zn  corresponding  to 
well  ordered  sets  of  cardinal  number  Kn_2  form  a  well  ordered  set 
having  a  greater  cardinal  number  a  than  Kn_2  •     Moreover  there  is 
no  cardinal  lying  between  Xn_2  and  «.     We  may  therefore  ap 
propriately   denote    a   by   KB_r     The    KM_2   sequence    of   ordinal 
numbers 


lying  in  Zn  has  a  limit  lying  in  Zn,  and  this  fact  embodies  the 
nth  principle  for  generating  ordinal  numbers.     The  first  n  prin 
ciples  are  just  adequate  to  generate  the  numbers  of  Zn.     They  do 
not  suffice  to  generate  even  the  first  number  in  Zn+l  . 
Finally  we  note  that  an  Kn  set  of  Kn  sets  forms  an  KM  set. 


n 


CHAPTER   X 
POINT  SETS 

Pantaxis 

301.  1.  (Borel.)  Let  each  point  of  the  limited  or  unlimited  set 
51  lie  at  the  center  of  a  cube  (L  Then  there  exists  an  enumerable  set 
of  non- overlapping  cubes  \c\  such  that  each  c  lies  within  some  (5,  and 
each  point  of  51  lies  in  some  c.  If  51  is  limited  and  complete,  there 
is  a  finite  set  jc|  having  this  property. 

For  let  D-p  D2  •••  be  a  sequence  of  superposed  cubical  divisions 
of  norms  =  0.  Any  cell  of  Dl  which  lies  within  some  (5  and 
which  contains  a  point  of  21  we  call  a  black  cell ;  the  other  cells 
of  D  we  call  white.  The  black  cells  are  not  further  subdivided. 
The  division  D2  divides  each  white  cell.  Any  of  these  subdivided 
cells  which  lies  within  some  (£  and  contains  a  point  of  51  we  call  a 
black  cell,  the  others  are  white.  Continuing  we  get  an  enumer 
able  set  of  non-overlapping  cubical  cells  Jc[. 

Each  point  a  of  51  lies  within  some  c.  For  a  is  the  center  of 
some  (5.  But  when  n  is  taken  sufficiently  large,  a  lies  in  a  cell  of 
Dn,  which  cell  lies  within  ($. 

Let  now  51  be  limited  and  complete.  Each  a  lies  within  a  cube  c, 
or  on  the  faces  of  a  finite  number  of  these  c.  With  a  we  associ 
ate  the  diagonal  8  of  the  smallest  of  these  cubes.  Suppose 
MinS  =  0  in  51.  As  51  is  complete,  there  is  a  point  a  in  51  such 
that  Min  S  =  0,  in  any  F^(cc).  This  is  not  possible,  since  if  ??  is 
taken  sufficiently  small,  all  the  points  of  Vj,  lie  in  a  finite  number 
of  the  cubes  c. 

Thus  Min  S  >  0.  As  the  c's  do  not  overlap,  there  are  but  a 
finite  number. 

2.  In  the  foregoing  theorem  the  points  of  51  are  not  necessarily 
inner  points  of  the  cubes  c.  Let  a  be  a  point  of  51  on  the  face  of 
one  of  these  c.  Since  a  lies  within  some  (5,  it  is  obvious  that  the 

324 


PANTAXIS  325 

cells  of  some  Dn,  n  sufficiently  large,  which  surround  a  form  a 
cube  (?,  lying  within  d.  Thus  the  points  of  51  lie  within  an 
enumerable  set  of  cells  J<?j,  each  c  lying  within  some  (£.  The 
cells  c  of  course  will  in  general  overlap.  Obviously  also,  if  51  is 
complete,  the  points  of  51  will  lie  within  a  finite  number  of 
these  <?'s. 

302.  If  51  is  dense,  51'  is  perfect. 

For,  in  the  first  place,  51'  is  dense.  In  fact,  let  a  be  a  point  of 
51'.  Then  in  any  D*(«)  there  are  points  of  51.  Let  a  be  such  a 
point.  Since  51  is  dense,  it  is  a  limiting  point  of  51  and  hence  is  a 
point  of  51'.  Thus  in  any  D*(a)  there  are  points  of  51'. 

Secondly,  51'  is  complete,  by  I,  266. 

303.  Let  $8  be  a  complete  partial  set  of  the  perfect  aggregate  51. 
Then  6  =  51  -  53  is  dense. 

For  if  (£  contains  the  isolated  point  c,  all  the  points  of  51  in  Dr*(c) 
lie  in  53,  if  r  is  taken  sufficiently  small.  But  53  being  com 
plete,  c  must  then  lie  in  53. 

Remark.  We  take  this  occasion  to  note  that  a  finite  set  is  to  be 
regarded  as  complete. 

304.  1.    J/51  does  not  embrace  all  9?n,  it  has  at  least  one  frontier 
point  in  $ln. 

For  let  a  be  a  point  of  51,  and  b  a  point  of  $Rn  not  in  5(.  The 
points  on  the  join  of  a,  b  have  coordinates 

2^  =  ^  +  0(^-0  =  ^(0),  0<0<1,  i  =  l,  2,. ..n. 

Let  6'  be  the  maximum  of  those  0's  such  that  #(0)  belongs  to 
5t  if  9  <  0'.  Then  x(6')  is  a  frontier  point  of  51. 

2.  Let  51,  33  have  no  point  in  common.  If  Dist  (51,  53)  >0,  we 
say  51,  53  are  exterior  to  each  other. 

305.  1.    Let  51  =  \a]   be  a  limited  or  unlimited  point  set  in  $lm. 
We  say  53  <  51  is  pantactic  in  51,  when  in  each  Dg(a)  there  is  a 
point  53. 

We  say  53  is  apantactic  in  51  when  in  each  D^a)  there  is  a  point 
a  of  51  such  that  some  D^t)  contains  no  point  of  53. 


326  POINT  SETS 

Example  1.  Let  21  be  the  unit  interval  (0,  1),  and  $8  the  ra 
tional  points  in  21.  Then  $8  is  pantactic  in  21. 

Example  2.  Let  21  be  the  interval  (0,  1),  and  33  the  Cantor  set 
of  I,  272.  Then  53  is  apantactic  in  21. 

2.  If  53  <  21  is  pantactic  in  21,  21  contains  no  isolated  points  not 
in®. 

For  let  a  be  a  point  of  21  not  in  53.  Then  by  definition,  in  any 
Z)5(#)  there  is  a  point  of  53.  Hence  there  are  an  infinity  of  points 
of  53  in  this  domain.  Hence  a  is  a  limiting  point  of  21. 

306.  Let  21  be  complete.     We  say  53  <  21  is  of  the  1°  category 
in  21,  if  53  is  the  union  of  an  enumerable  set  of  apantactic  sets 
in  21. 

If  53  is  not  of  the  1°  category,  we  say  it  is  of  the  2°  category. 
Sets  of  the  1°  category  may  be  called  Baire  sets. 

Example.  Let  21  be  the  unit  interval,  and  53  the  rational 
points  in  it.  Then  53  is  of  the  1°  category. 

For  53  being  enumerable,  let  53  =  \on\.     But  each  bn  is  a  single    f  k 
point  and  is  thus  apantactic  in  21. 

The  same  reasoning  shows  that  if  53  is  any  enumerable  set  in 
21,  then  53  is  of  the  1°  category. 

307.  1.    If  53  is  of  the  1°  category  in  21,  21  -  53  =  B  is  >  0. 

For  since  53  is  of  the  1°  category  in  21,  it  is  the  union  of  an 
enumerable  set  of  apantactic  sets  {53nj.  Then  by  definition  there 
exist  points  a^  a2,  •••  in  21  such  that 


where  D(a^)  contains  no  point  of  53X,  -#(«2)  no  point  of  532?  etc. 
Let  b  be  the  point  determined  by  1).  Since  21  is  complete  by 
definition,  b  is  a  point  of  21.  As  it  is  not  in  any  53n,  it  is  not 
in  53.  Hence  B  contains  at  least  one  point. 

2.    Let  21  be  the  union  of  an  enumerable  set  of  sets  J2lnj,  each  2ln 
being  of  the  1°  category  in  53-      Then  21  is  of  the  1°  category  in  53. 

This  is  obvious,  since  the  union   of  an  enumerable  set  of  enu 
merable  sets  is  enumerable. 


PANTAXIS  327 

3.  Let  33  be  of  the  1°  category  in  21.     Then  B  =  21  -33  is  of  the 
2°  category  in  21. 

For  otherwise  $8  +  -5  would  be  of  the  1°  category  in  21-     But 

51  -  (53  +  B)  =  0, 
and  this  violates  1. 

4.  It  is  now  easy  to  give  examples  of  sets  of  the  2°  category. 
For  instance,  the  irrational  points  in  the  interval  (0,  1)  form  a 
set  of  the  2°  category. 

308.  Let  21  be  a  set  of  the  1°  category  in  the  cube  Q.  Then 
A  =  Q  —  21  Aas  the  cardinal  number  c. 

If  A  has  an  inner  point,  Da(a),  for  sufficiently  small  8,  lies  in  .A. 
As  Card  D&  =  c,  the  theorem  is  proved. 

Suppose  that  A  has  no  inner  point.  Let  51  be  the  union  of  the 
apantactic  sets  2lj  <  2(2  <  •••  in  Q.  Let  An  =  Q  —  2ln.  Let  qn  be 
the  maximum  of  the  sides  of  the  cubes  lying  wholly  in  An.  Ob 
viously  qn  =  0,  since  by  hypothesis  A  has  no  inner  points.  Let  Q 
be  a  cube  lying  in  Al.  As  qn  =  0,  there  exists  an  n^  such  that  Q 
has  at  least  two  cubes  lying  in  Ani  ;  call  them  $0,  Qlt  There  ex 
ists  an  n2  >  Wj  such  that  $0,  Ql  each  have  two  cubes  in  A^\  call 

them  Q  Q         •      O  Q 

Vo,  o     »     Vo,  i     >      Vi,  o     i     Vi,  i  » 

or  more  shortly  (>tli  tj. 

Each  of  these  gives  rise  similarly  to  two  cubes  in  some  An&, 
which  may  be  denoted  by  ftit  tji  ls,  where  the  indices  as  before  have 
the  values  0,  1.  In  this  way  we  may  continue  getting  the  cubes 

Qn     »     ftji,     »     &**•"• 

Let  a  be  a  point  lying  in  a  sequence  of  these  cubes.  It  obvi 
ously  does  not  lie  in  21,  if  the  indices  are  not,  after  a  certain  stage, 
all  0  or  all  1.  This  point  a  is  characterized  by  the  sequence 


which  may  be  read  as  a  number  in  the  dyadic  system.     But  these 
numbers  have  the  cardinal  number  c. 

309.  Let  21  be  a  complete  apantactic  set  in  a  cube  Q.  Then  there 
exists  an  enumerable  set  of  cubical  cells  jq}  such  that  each  point  of 
21  lies  on  a  face  of  one  of  these  q,  or  is  a  limit  point  of  their  faces. 


328  POINT   SETS 

For  let  D^  >  D2  >  •••  be  a  sequence  of  superimposed  divisions 
of  O,  whose  norms  5n  =  0.     Let 


be  the  cells  of  Dl  containing  no  point  of  51  within  them.     Let 

dzl,  d22,  c723  ...  (2 

denote  those  cells  of  D2  containing  no  point  of  51  within  them  and 
not  lying  in  a  cell  of  1).  In  this  way  we  may  get  an  infinite  se 
quence  of  cells  £)  =  \dmn\,  where  for  each  m,  the  corresponding  n 
is  finite,  and  m  =  cc.  Eacli  point  a  of  A  lies  in  some  dm^  n  .  For  51 
being  complete,  Dist  (a,  51)  >  0.  As  the  norms  Bn  =  0,  a  must  lie 
in  some  cell  of  Z>n,  for  a  sufficiently  large  n.  The  truth  of  the 
theorem  is  now  obvious. 

310.  Let  33  be  pantactic  in  51.      Then  there  exists  an  enumerable 
set  (£<_  33  which  is  pantactic  in  51. 

For  let  D1  >  Z>2>  «••  be  a  set  of  superimposed  cubical  divisions 
of  norms  dn  =  0.  In  any  cell  of  Dl  containing  within  it  a  point 
of  51,  there  is  at  least  one  point  of  53.  If  the  point  of  51  lies  on 
the  face  of  two  or  more  cells,  the  foregoing  statement  will  hold 
for  at  least  one  of  the  cells.  Let  us  now  take  one  of  these  points 
in  each  of  these  cells;  this  gives  an  enumerable  set  (S^.  The 
same  holds  for  the  cells  of  D2.  Let  us  take  a  point  in  each  of 
these  cells,  taking  when  possible  points  of  @j.  Let  (52  denote  the 
points  of  this  set  not  in  (S^.  Continuing  in  this  way,  let 

(S  =  (£1  +  (*2+  ... 
Then  (5  is  pantactic  in  51,  and  is  enumerable,  since  each  (5n  is. 

Corollary.     In  any  set  51,  finite  or  infinite,  there  exists  an  enumer 
able  set  &  which  is  pantactic  in  51. 

For  we  have  only  to  set  53  =  51  in  the  above  theorem. 

311.  1.    The  points  (£  where  the  continuous  function  f(xl  •  •  •  xm) 
takes  on  a  given  value  g  in  the  complete  set  tyi,form  a  complete  set. 

For  let  cv  c2  ...  be  points  of  (5  which  =  c.  We  show  c  is  a 
point  of  (5.  For  --  - 


PANTAXIS  329 

As /is  continuous,  »f    \^ff\ 

J\Cn)  —J\C)' 

Hence  /<*)** 

and  c  lies  in  (L 

2.  Letf(xl  "•  xm)  be  continuous  in  the  limited  or  unlimited  set  51. 
If  the  value  of  f  is  known  in  an  enumerable  pantactic  set  &  in  51, 
which  contains  all  the  isolated  points  of  51,  in  case  there  be  such,  the 
value  off  is  known  at  every  point  of  5(. 

For  let  a  be  a  limiting  point  of  51  not  in  (£.  Since  (5  is  pantactic 
in  51,  there  exists  a  sequence  of  points  e^  e2--  in  (S  which  =  a. 
Since  /  is  continuous,  /(#„)  = /(a).  As  /  is  known  at  each  en, 
it  is  known  at  a. 

3.  Let  g  =  J/j   be  the  class  of  one-valued  continuous  functions 
defined  over  a  limited  point  set  51.      Then 

f  =  Card  g  =  c. 

For  let  SH^  be  a  space  of  an  infinite  enumerable  number  of 
dimensions,  and  let  A 

r— (TII  #2»  •••) 

denote  one  of  its  points.     Let/ have  the  value  rjl  at  e^  the  value 
?72  at  £2  •••  for  the  points  of  (5  defined  in  2.     Then  the  complex 

0?i»  ^2  ••') 

completely  determines  /.     But  this  complex  determines  also   a 
point  77  in  ^  whose  coordinates  are  rjn.     We  now  associate  /  with 

•     Hence 


On  the   other   hand,   f>c,   since   in    g    there   is    the   function 
/(#!  •••  xm)  =  g  in  51,  where  g  is  any  real  number. 

312.    Let  53  denote  the  class  of  complete  or  perfect  subsets  lying  in 
the  infinite  set  51,  which  latter  contains  at  least  one  complete  set. 

Then  «      n     ^  cu 

b  =  Card  53  =  c. 

For  let  alt  a2,  •  ••  =  a,  all  these  points  lying  in  51.     Then 

But  for  tj  we  may  take  any  number  in  ^  =  (1,  2,  3,  •••)  ;   for  i% 
we  may  take  any  number  in  $2  =  (^  +  1.  ^  +  2,  •••),  etc. 


330  POINT   SETS 

Obviously  the  cardinal  number  of  the  class  of  these  sequences 
l)ise<  =  c.     But  («,«^;.«;,..) 

is  a  complete  set  in  51.     Hence  b.>c.     On  the  other  hand,  b<c. 

Forlet  A  >-»•>•••  (2 

be  a  sequence  of  superimposed  cubical  division  of  norms  =  0. 
Each  Dn  embraces  an  enumerable  set  of  cells.  Thus  the  set  of 
divisions  gives  an  enumerable  set  of  cells.  Each  cell  shall  have 
assigned  to  it,  for  a  given  set  in  53,  the  sign  +  or  —  according  as 
33  is  exterior  to  this  cell  or  not.  This  determines  a  distribution 
of  two  things  over  an  enumerable  set  of  compartments. 

The  cardinal  number  of  the  class  of  these  distributions  is  2c  =  c. 
But  each  53  determines  a  distribution.     Hence  b<c. 


Transfinite  Derivatives 

313.    1.    We  have  seen,  I,  266,  that 

%'>%">%'">  .-. 
Thus  2l(n)  =  Dv(2l',  a"  •..  2irn)>  (1 

Let  now  51  be  a  limited  point  aggregate  of  the  second  species. 
It  has  then  derivatives  of  every  finite  order.  Therefore  by  18, 

D<21',  21",  51'",  •••)  (2 

contains  at  least  one  point,  and  in  analogy  with  1),  we  call  the 
set  2)  the  derivative  of  order  co  of  21,  and  denote  it  by 

2l(w), 
or  more  shortly  by 

2K 

Now  we  may  reason  on  2lw  as  on  any  point  set.  If  it  is  infinite, 
it  must  have  at  least  one  limiting  point,  and  may  of  course  have 
more.  In  any  case  its  derivative  is  denoted  by 

(«+i)  or  5lw+1. 


The  derivative  of  5lw+1  is  denoted  by 


or 


Making  use  of  o>  we  can  now  state  the  theorem  : 


TRANSFINITE   DERIVATIVES  331 

In  order  that  the  point  set  51  is  of  the  first  species  it  is  necessary 
and  sufficient  that  5lu;  =  0. 

2.  We  have  seen  in  18  that  51"'  is  complete.  The  reasoning  of 
I,  266  shows  that  5lw+1,  5lw+2,  •••,  when  they  exist,  are  also  complete. 
Then  18  shows  that,  if  5lw+71  n  =  1,  2,  ...  exist, 

Dw(aw>aw+1>aw+2>  •••)  (3 

exists  and  is  complete.     The  set  3)  is  called  the  derivative  of  order 

ft>  •  2  and  is  denoted  by 

§j(«2)  or  5^ 

Obviously  we  may  continue  in  this  way  indefinitely  until  we 
reach  a  derivative  of  order  a  containing  only  a  finite  number  of 
points.  Then  ^a+1  =  Q 

That  this  process  of  derivation  may  never  stop  is  illustrated  by 
taking  for  51  any  limited  perfect  set,  for  then 


3.    We  may  generalize  as  follows  :   Let  a  denote  a  limitary  ordi 
nal  number.     If  each  51^  >  0,  /3  <  a,  we  set 


when  it  exists. 

4.    If  5la  >  0,  while  51  +  1  =  0,  we  say  5t  is  of  order  a. 

314.     1.    Let  a  be  a  limiting  point  of  51.     Let 


Obviously  as  is  monotone  decreasing  with  8.      Suppose  that 
there  exists  an  a  and  a  BQ  >  0,  such  that  for  all  0  <  8  <  S0 

«=  Card  F<». 

We  shall  say  that  a  is  a  limiting  point  of  rank  a. 
If  every  «5  >  a,  we  shall  say  that 

Rank  a  >  «. 
If  every  as  >  a,  we  shall  say  that 

Rank  a  >  a. 


332  POINT   SETS 

2.  Let  51  be  a  limited  aggregate  of  cardinal  number  a.      Then  there 
is  at  least  one  limiting  point  of  5(,  of  rank  a. 

The  demonstration  is  entirely  similar  to  I,  264.  Let  S1  > 
£2  >  ...  =0.  Let  us  effect  a  cubical  division  of  51  of  norm  8^.  In 
at  least  one  cell  lies  an  aggregate  5lx  having  the  cardinal  num 
ber  a.  Let  us  effect  a  cubical  division  of  5^  of  norm  £2 .  In  at 
least  one  cell  lies  an  aggregate  512  having  the  cardinal  number  a, 
etc.  These  cells  converge  to  a  point  #,  such  that 

Card  F5O)  =  a, 
hoAvever  small  S  is  taken. 

3.  If  Card  51  >  e,  there  exists  a  limiting  point  oftyt  of  rank  >  e. 
The  demonstration  is  similar  to  that  of  2. 

4.  If  there  is  no  limiting  point  of  51  of  rank  >  e,  51  is  enumerable. 
This  follows  from  3. 

5.  Let  Card  51  be  >  e.      Let  33  denote  the  limiting  points  of  51 
whose  ranks  are  >  e.      Then  33  is  perfect. 

For  obviously  33  is  complete.  We  need  therefore  only  to  show 
that  it  is  dense.  To  this  end  let  b  be  a  point  of  33.  About  b  let 
us  describe  a  sequence  of  concentric  spheres  of  radii  rn  =  0.  These 
spheres  determine  a  sequence  of  spherical  shells  S$n5,  no  two  of 
which  have  a  point  in  common.  If  5ln  denote  the  points  of  51  in  $n, 
we  have  y  =  y^  .=  ^  +  ^  +  ^  +  ... 

Thus  if  each  5(m  were  enumerable,  V  is  enumerable  and  hence 
Rank  b  is  not  >  e.  Thus  there  is  one  set  5lm  which  is  not  enu 
merable,  and  hence  by  3  there  exists  a  point  of  33  in  Sm.  But  then 
there  are  points  of  33  in  any  F^*(5),  and  b  is  not  isolated. 

6.  A  set  51  which  contains  no  dense  component  is  enumerable. 
For  suppose  51  were  not  enumerable.      Let  ty  denote  the  proper 

limiting  points  of  51.  Then  ^  contains  a  point  whose  rank  is  >  e. 
But  the  set  of  these  points  is  dense.  This  contradicts  the  hy 
pothesis  of  the  theorem. 

315.    Let  a  lie  in  Zn.     -Zf5la  >  0,  it  is  complete. 
For  if  a  is  non-limitary,  reasoning  similar  to  I,  266  shows  that 
5la  is  complete.      Suppose  then  that  a  is  limitary,  and  5la  is  not 


TRANSFINITE   DERIVATIVES  333 

complete.  The  derivatives  of  51  of  order  <  a  which  are  not  com 
plete,  form  a  well  ordered  set  and  have  therefore  a  first  element 
91^,  where  &  is  necessarily  a  limitary  number.  Then 


But  every  point  of  51^  lies  in  each  5IY.  Hence  every  limiting 
point  of  W  is  a  limiting  point  of  each  51*  and  hence  lies  in  2F3. 
Hence  2C3  is  complete,  which  is  a  contradiction. 

316.  Let  a    be  a    limitary  number   in  Zn.     If  ^  >  0  for  each 
/3  <  «,  5la  exists. 

For  there  exists  an  Km,      ra  j<  n  —  2,  sequence 

7<  &  <e<  77  <  •••=«.  (1 

Let  c  be  a  point  of  21?,  d  a  point  of  21s,  e  a  point  of  51%  etc. 
Then  the  set  ^  ^  ,,/,...) 

has  at  least  one  limiting  point  I  of  rank  XTO.  Let  e  be  any  number 
in  1).  Then  Hs  a  limiting  point  of  rank  Xm  of  the  set 

(«./»•••)- 

Thus  I  is  a  limiting  point  of  every  21^,  /3  <  «,  and  hence  of  5la. 

317.  Let  us  show  how  we  may  form  point  sets  whose  order  a 
is  any  number  in  Z1  or  Z2. 

We  take  the  unit  interval  51  =  (0.  1)  as  the  base  of  our  con 
siderations. 

In  51,  take  the  points 

»i-i   .  I  .  f  •  tf   •••  C1 

Obviously  $[  =  1,  ${'  =  0.  Hence  ^  is  of  order  1.  The  set 
SBj  divides  51  into  a  set  of  intervals 

5lx    ,     5I2    ,    513     -.  (2 

In  5lj  =  (0,  l)  take  a  set  of  points  similar  to  1)  which  has  as 
single  limiting  point,  the  point  J.  In  512  =  Q-,  |)  take  a  set  of 
points  similar  to  1)  which  has  as  single  limiting  point,  the  point 
|,  etc.  Let  us  call  the  resulting  set  of  points  332. 


334  POINT   SETS 

Obviously       ™,       l  3  * 

^2  =  i    »    f    '    t    '    "* 

Hence  ^  =  ^  =  j  and  $  w  =  0 

Thus  <B2  is  of  order  2. 


In  each  of  the  intervals  2)  we  may  place  a  set  of  points  similar 
to  332,  such  that  the  right-hand  end  point  of  each  interval  5{n  is  a 
limiting  point  of  the  set.  The  resulting  set  233  is  of  order  3,  etc. 

This  shows  that  we  may  form  sets  of  every  finite  order. 

Let  us  now  place  a  set  of  order  1  in  5lx,  a  set  of  order  2  in  512, 
etc.  The  resulting  set  5L  is  of  order  o>.  For  33^  has  no  points 
in  Slj,  212  ...  $„_!,  while  the  point  1  lies  in  every  ^?l). 


Hence  $(.+i>  =  o, 

and  ^w  is  of  order  o>. 

Let  us  now  place  in  each  5ln  a  set  similar  to  $BW,  having  the 
right-hand  end  point  of  $ln  as  limiting  point.  The  resulting  set 
33W+1  is  of  order  o>  -f  1.  In  this  way  we  may  proceed  to  form  sets 
of  order  o>  +  2,  o>  +  3,  •••  just  as  we  did  for  orders  2,  3,  •••  We 
may  also  form  now  a  set  of  order  o>2,  as  we  before  formed  a  set 
of  order  co. 

Thus  we  may  form  sets  of  order 

w     ,     a)  •  2     ,     a)  •  3     ,     a)  •  4 

and  hence  of  order  &)2,  etc. 

318.  1.  Let  51  be  limited  or  not,  and  let  2ltw  denote  the  isolated 
points  of  2F.  Then 


ft 
For  t        i        'i 

.L  flUS  nfl          c\fi     .     nv;  /    .  CW/'YI—-!'* 


that  is,  51'  is  the  sum  of  the  points  of  51'  not  in  51",  of  the  points 
of  51"  not  in  2T",  etc.  If  now  there  are  points  common  to  every 
H<->wehave  <»,  M  .. 


TRANSFINITE   DERIVATIVES  335 

On  5lw  we  can  reason  as  on  51',  and  in  general  for  any  a  <  fl  we 

have  a, 

/3<a 

which  gives  1). 


2.    #*5P  =  0,  51  tmd  51'  are  enumerable. 
For  not  every       ^  >  Q         .<ftb 

Hence  there  is  a  first  a,  call  it  7,  such  that  51Y  =  0.     Then  1) 
reducesto 


But  the  summation  extends  over  an  enumerable  set  of  terms, 
each  of  which  is  enumerable  by  289.  Hence  51'  is  enumerable. 
But  then  51  is  also  enumerable  by  237,  2. 

3.  Conversely,  if  51'  is  enumerable,  5ln  =  0. 

For  if  51"  >  0,  there  is  a  non-enumerable  set  of  terms  in  1),  if 
no  5l(^)  is  perfect  ;  and  as  each  term  contains  at  least  one  point, 
51'  is  not  enumerable.  If  some  5l(/3)  is  perfect,  51'  contains  a  per 
fect  partial  set  and  is  therefore  not  enumerable  by  245. 

4.  From  2,  3,  we  have  : 

For  51'  to  be  enumerable,  it  is  necessary  and  sufficient  that  there 
exists  a  number  a  in  Z1  or  Z2  such  that  5la  =  0. 

5.  If  51  is  complete,  it  is  necessary  and  sufficient  in  order  that  51 
be  enumerable,  that  there  exists  an  a  in  Z^  or  Z2  such  that  5la  =  0. 

F°r  51  =  5lt  +  51', 

and  the  first  term  is  enumerable. 

6.  If  51^  =  0  for  some  ft  <  H,  we  say  51  is  reducible,  otherwise  it 
is  irreducible. 

319.    If  5In  >  0,  it  is  perfect. 

By  315  it  is  complete.  We  therefore  have  only  to  show  that 
its  isolated  points  51"  =  0.  Suppose  the  contrary  ;  let  a  be  an 
isolated  point  of  5ln. 

Let  us  describe  a  sphere  S  of  radius  r  about  a,  containing  no 
other  point  of  5ln.  Let  53  denote  the  points  of  51'  in  S.  Let 

r  >r   >r>  •••  =  0. 


POINT   SETS 


Let  Sn  denote  a  sphere  about  a  of  radius  rn.  Let  53n  denote  the 
points  of  53  lying  between  /S^,  $n,  including  those  points  which 
may  lie  on  Sn_lf  Then 


-i-  a. 


Each  53m  is  enumerable.  For  any  point  of  53,"  is  a  point  of 
53"  =  a.  Hence  53"  =  0  and  53TO  is  enumerable  by  318,  2. 

Thus  53  is  enumerable.  This,  however,  is  impossible  since 
53"  =  a,  and  is  thus  >  0. 

320.    1.    In  the  relation 

5T  =  S^  +  51"         £=1,2,-..  <fl, 

ft 
the  first  term  on  the  right  is  enumerable. 

For  let  us  set 


«*  _  ?9fo)  . 

r1>rt>-  =0.  •          '    '     V'    . 

Let  53n  denote  the  points  of  53  whose  distance  B  from  5P  satis 
fies  the  relation  ^  ?>  ^ 


n+1 


Then  the  distance  of  any  point  of  53J>  from  51"  is  >  rn+1  .     If  530 
includes  all  points  of  53  whose  distance  from  $P  is  >  r1,  we  have 


Each  53n  is  enumerable.     For  if  not,  53"  >  0.     Any  point  of 
53£  as  b  lies  in  51".     Hence 

Dist  (5,  51")  =  0. 

On  the  other  hand,  as  b  lies  in    53^,  its    distance    from  51°  is 
>  rn+1,  which  is  a  contradiction. 

2.  If  51'  is  not  enumerable,  there  exists  a  first  number  a  in  Zl  or 
Z%  such  that  5la  is  perfect. 

This  is  a  corollary  of  1. 

3.  If  51  is  complete  and  not  enumerable,  there  exists  a  first  number 
a  in  Zl  +  Z%  such  that  5T  is  perfect. 

is  complete,  . 


where  (5  is  enumerable,  and  ^  is  perfect.     If  51  is  enumerable,  ^  =  0. 


COMPLETE   SETS  337 

Complete  Sets 

321.  Let  us  study  now  some  of  the  properties  of  complete  point 
sets.      We  begin  by  considering  limited  perfect  rectilinear  sets. 
Let  51  be  such  a  set.     It  has  a  first  point  a  and  a  last  point  b.     It 
therefore  lies  in  the  interval  /=(«,  £).     If  51  is  pantactic  in  any 
partial  interval  J=  (a,  /3)  of  J,  51  embraces  all  the  points  of  «7, 
since  51  is  perfect.     Let  us  therefore  suppose  that  51  is  apantactic 
in  /.     .An  example  of  such  sets  is  the  Cantor  set  of  I,  272. 

Let  D  =  \  S  I  be  a  set  of  intervals  no  two  of  which  have  a  point 
in  common.  We  say  D  is  pantactic  in  an  interval  /,  when  I  con 
tains  no  interval  which  does  not  contain  some  interval  8,  or  at 
least  a  part  of  some  8. 

It  is  separated  when  no  two  of  its  intervals  have  a  point   in    ^£/ 
common. 

322.  1.    Every  limited  rectilinear  apantactic  perfect  set  51  deter 
mines  an  enumerable  pantactic  set  of  separated   intervals  D—  \S\, 
whose  end  points  alone  lie  in  51. 

For  let  51  lie  in  /=(«,  $),  where  «,  ft  are  the  first  and  last 
points  of  51.  Let  93  =  /—  51.  Each  point  b  of  33  falls  in  some  in 
terval  S  whose  end  points  lie  in  51.  For  otherwise  we  could 
approach  b  as  near  as  we  chose,  ranging  over  a  set  of  points  of  51. 
But  then  b  is  a  point  of  51,  as  this  is  perfect.  Let  us  therefore 
take  these  intervals  as  large  as  possible  and  call  them  B. 

The  intervals  8  are  pantactic  in  J,  for  otherwise  51  could  not  be 
apantactic.  They  are  enumerable,  for  but  a  finite  set  can  have 
lengths  >  I/n  +  1  and  <  I/n,  n  =  1,  2  ••• 

It  is  separated,  since  51  contains  no  isolated  points. 

2.    The  set  of  intervals  D  =  \S\   just  considered  are  said  to  be    I    v 
adjoint  to  51,  or  determined  by  51,  or  belonging  to  51.  I         ^1 

323.  Let  51  be  an  apantactic  limited  rectilinear  perfect  point  set,  to 
ichich  belongs  the  set  of  intervals  D=  |8j.      Then  51  is  formed  of  the 
end  points  E=  \e\  of  these  intervals,  and  their  limiting  points  E' . 

For  we  have  just  seen  that  the  end  points  e  belong  to  51.  More 
over,  51  being  perfect,  E'  must  be  a  part  of  51. 


338  POINT  SETS 

51  contains  no  other  points.  For  let  a  be  a  point  of  51  not  in  E, 
E'  .  Let  a  be  another  point  of  31.  In  the  interval  (a,  a)  lies  an 
end  point  e  of  some  interval  of  D.  In  the  interval  (a,  e)  lies  an 
other  end  point  er  In  the  interval  (a,  gj)  lies  another  end  point 
02,  etc.  The  set  of  points  e,  e^  e^--  =  a.  Hence  a  lies  in  E'  , 
which  is  a  contradiction. 

324.  Conversely,  the  end  points  E  =  \e\  and  the  limiting  points  of 
the  end  points  of  a  pantactic  enumerable  set  of  separated  intervals 
D  =  j  8  \  form  a  perfect  apantactic  set  51. 

For  in  the  first  place,  51  is  complete,  since  51  =  (E,  E').  51  can 
contain  no  isolated  points,  since  the  intervals  S  are  separated. 
Hence  51  is  perfect.  It  is  apantactic,  since  otherwise  51  would  em 
brace  all  the  points  of  some  interval,  which  is  impossible,  as  D  is 
pantactic. 

325.  Since  the  adjoint  set  of  intervals  D  =  \S\  is  enumerable,  it 
can  be  arranged  in  a  1,  2,  3,  •••  order  according  to  size  as  follows. 

Let  8  be  the  largest  interval,  or  if  several  are  equally  large,  one 
of  them.  The  interval  8  causes  Jto  fall  into  two  other  intervals. 
The  interval  to  the  left  of  8,  call  IQ,  that  to  the  right  of  £,  call  Ir 
The  largest  interval  in  /0,  call  S0,  that  in  Iv  call  Sv  In  this  way 
we  may  continue  without  end,  getting  a  sequence  of  intervals 

S,  80,  Sj,  S00,  S01,  S10,  Sn-..  (1 

and  a  similar  series  of  intervals 

•*i    ^0'      1»       00'      01"* 

The  lengths  of  the  intervals  in  1)  form  a  monotone  decreasing 
sequence  which  =  0. 

If  v  denote  a  complex  of  indices  ij/c  -•• 


326.    1.    The  cardinal  number  of  every  perfect  limited  rectilinear 
point  set  51  is  c. 

For  if  51  is  not  apantactic,  it  embraces  all  the  points  of  some  in 
terval,  and  hence  Card  51  =  c.      Let  it  be  therefore  apantactic. 


COMPLETE  SETS  339 

Let  D=  JS,;  be  its  adjoint  set  of  intervals,  arranged  as  in  325. 
Let  (£  be  the  Cantor  set  of  I,  272.  Let  its  adjoint  set  of  intervals 
be  H=  \r]v\,  arranged  also  as  in  325.  If  we  set  8V^>  77,,  we  have 
D^H.  Hence  Card  51  =  Card  £. 

But  Card  6  =  c  by  244,  4. 

2.    The  cardinal  number  of  every  limited  rectilinear  complete  set  51 
i  %o.  is  either  e  or  c. 

For  we  have  seen,  320,  4,  that 


where  (£  is  enumerable  and  ^3  is  perfect, 

If  $  =  0,         Card  51  =  e. 

If  $>0,          Card  51  =  c. 

For  Card  51  =  Card  (g  +  Card  $  =  e  +  c  =  c. 

327.  The  cardinal  number  of  every  limited  complete  set  51  in  ^Rn  is 
either  e  or  c.     It  is  c,  ^/5^  Aas  a  perfect  component. 

The  proof  may  be  made  by  induction. 

For  simplicity  take  m  =  2.  By  a  transformation  of  space  [242], 
we  may  bring  51  into  a  unit  square  S.  Let  us  therefore  suppose 
51  were  in  S  originally.  Then  Card  51  <  c  by  247,  2. 

Let  (£  be  the  projection  of  51  on  one  of  the  sides  of  #,  and  $3  the 
points  of  51  lying  on  a  parallel  to  the  other  side  passing  through  a 
point  of  £.  If  33  has  a  perfect  component,  Card  33  =  c,  and  hence 
Card  51  =  c.  If  33  does  not  have  a  perfect  component,  the  cardinal 
number  of  each  33  is  e.  Now  (£  is  complete  by  I,  717,  4.  Hence 
if  (E  contains  a  perfect  component,  Card  (S  =  c,  otherwise  Card 
(5  =  e.  In  the  first  case  Card  51  =  c,  in  the  second  it  is  e. 

328.  1.    Let  51  be  a  complete  set  lying  within  the  cube  Q.     Let 
DI  >  D%  >  ...  denote  a  set  of  superimposed  cubical  divisions  of  Q 
of  norms  =  0.      Let  d1  be  the  set  of  those  cubes  of  Dl  containing 
no  point  of  51.     Let  d2  be  the  set  of  those  cubes  of  D2  not  in  dl  , 
which  contain  no  point  of  51.     In  this  way  we  may  continue.     Let 
&  =  \dn\.     Then  every  point  of  A  =  O  -  51  lies  in  33.     For  51  being 


340  POINT   SETS 

complete,  any  point  a  of  A  is  an  inner  point  of  A.     Hence  2>p(a) 
lies  in  A,  for  some  p  sufficiently  small.     Hence  a  lies  in  some  dm. 
We  have  thus  the  result  : 

Any  limited  complete  set  is  uniquely  determined  by  an  enumerable 
set  of  cubes  \dn\,  each  of  which  is  exterior  to  it. 

We  may  call  33  =  \dn\  the  border  of  51,  and  the  cells  dn,  border 
cells. 

2.  The  totality  of  all  limited  perfect  or  complete  sets  has  the  car 
dinal  number  c. 

For  any  limited  complete  set  (E  is  completely  determined  by  its 
border  \dn\.  The  totality  of  such  sets  has  a  cardinal  number 
<  ce  =  c.  Hence  Card  j(S  J  <  c.  Since  among  the  sets  (5  is  a  c-set 
of  segments,  Card  (£  >  c. 

329.  If  5lt  denote  the  isolated  points  of  51,  and  5(A  its  proper 
limiting  points,  we  may  write 

51  =  51  +  5(A. 
Similarly  we  have 

5lA=5lAl 


51A,  =  5U  +  HA3,  etc. 
We  thus  have 

51  =  5It  +  5lAt  +  5U  +  -  -  -  +  5IAn-it  +  ?1A«  . 

At  the  end  of  each  step,  certain  points  of  51  are  sifted  out.  They 
may  be  considered  as  adhering  loosely  to  51,  while  the  part  which 
remains  may  be  regarded  as  cohering  more  closely  to  the  set.  Thus 
we  may  call  2lA«-it,  the  nih  adherent,  and  21AW  the  nth  coherent. 

If  the  nth  coherent  is  0,  51  is  enumerable. 

If  the  above  process  does  not  stop  after  a  finite  number  of  steps, 

let  5 


If  5lw  >  0,  we  call  it  the  coherent  of  order  &>. 
Then  obviously  9f  —  "S9f  n  4-  9f 

We  may  now  sift  5L  as  we  did  51. 


COMPLETE   SETS  341 

If  a  is  a  limitary  number,  defined  by 


we  set  5la 

and  call  it,  when  it  exists,  the  coherent  of  order  a.     Thus  we  can 

write  +  2^         «=1,  2,  ...</3  (1 


where  /3  is  a  number  in  Z2. 

330.    1.     When  51  is  enumerable, 


,  2,  .-. 


ivhere  $  i§  the  sum  °f  an  enumerable  set  of  isolated  sets,  and  £),  when 
it  exists,  is  dense. 

For  the  adherences  of  different  orders  have  no  point  in  common 
with  those  of  any  other  order.  They  are  thus  distinct.  Thus  the 
sum  $  can  contain  but  an  enumerable  set  of  adherents,  for  other 
wise  51  could  not  be  enumerable.  Thus  there  is  a  first  ordinal 
number  j3  for  which 

5lA  =  0. 
As  now  in  general 

8t^=  2U  +  8x0+1, 
we  have  ^  =  ^/+1  =  ^,+2  =  ... 

As  21A0  thus  contains  no  isolated  points,  it  is  dense,  when  not  0, 
by  I,  270. 

2.  Wlien  51  is  not  enumerable,  X)  >  0.  For  if  not,  21  =  3'  and  3 
is  enumerable. 

331.  8  =  S'.  (1 

For  let  D  be  a  cubical  division  of  space.     As  usual  let 

or  Of' 

«•/)         9         <^Z> 

denote  those  cells  of  D  containing  a  point  of  51,  5T  respectively. 
The  cells  of  5(i  not  in  51^  will  be  adjacent  to  those  of  51^,  and 


342  POINT   SETS 

these  may  be  consolidated  with  the  cells  of  D,  forming  a  new  di 
vision  A  of  norm  8  which  in  general  will  not  be  cubical.     Then 


21A  =  211  +  21 


The  last  term  is  formed  of  cells  that  contain  only  a  finite  number 
of  points  of  21.  These  cells  may  be  subdivided,  forming  a  new 
division  U  such  that  in 

%E  =  2fi  +  %E*  (2 

the  last  term  is  <  e/3-     Now  if  8  is  sufficiently  small, 

aA-S<!    ,   H  -«'<!•  (3 

o  o 

Hence  from  2),  3)  we  have  1). 

332.    -7f2l>0,  Card  21  =  c. 


For  let  93  denote  the  sifted  set  of  21  [I,  712].  Then  $  is  per 
fect.  Plence  Card  53  =  c,  hence  Card  21  =  c. 

333.  Let  21  =  JaJ,  where  each  a  is  metric  and  not  discrete.  If  no 
two  of  the  as  have  more  than  their  frontiers  in  common,  21  is  an 
enumerable  set  in  the  d's.  21  may  be  unlimited. 

Let  us  first  suppose  that  21  lies  in  a  cube  O.  Let  a  denote  a  on 
removing  its  proper  frontier  points.  Then  no  two  of  the  a's  have 
a  point  in  common.  Let 


where  the  first  term  ql  =  Q.     There  can  be  but  a  finite  number  of 
sets  a,  such  that  their  contents  lie  between  two  successive  ^'s. 

For  if  ^  ^ 

«4     »     "*~'>q, 

we  have  ^+^+  .~  +«tn>nq.. 

But  the  sum  on  the  left  is  <  O,  for  any  n. 

As  n  may  =  oo,  this  makes  O  =  oo,  which  is  absurd. 

If  21  is  not  limited,  we  may  effect  a  cubical  division  of  9?m. 
This  in  general  will  split  some  of  the  a's  into  smaller  sets  b.  In 
each  cube  of  this  division  there  is  but  an  enumerable  set  of  the  b's 
by  what  has  just  been  proved. 


CHAPTER   XI 
MEASURE 

Upper  Measure 

334.  1.  Let  51  be  a  limited  point  set.  An  enumerable  set  of 
metric  sets  D=  {e?tj,  such  that  each  point  of  51  lies  in  some  d^  is 
called  an  enclosure  of  51.  If  each  point  of  51  lies  within  some  c?0  D 
is  called  an  outer  enclosure.  The  sets  dt  are  called  cells.  To  each 
enclosure  corresponds  the  finite  or  infinite  series 

23,  (1 

which  may  or  may  not  converge.  In  any  case  the  minimum  of  all 
the  numbers  1)  is  finite  and  <_0.  For  let  A  be  a  cubical  division 
of  space,  51A  is  obviously  an  enclosure  and  the  corresponding  sum 
1)  is  also  51A,  since  we  have  agreed  to  read  this  last  symbol  either 
as  a  point  set  or  as  its  content. 

We  call  ,».    v  , 

Mm  2at, 

with  respect  to  the  class  of  all  possible  enclosures  D,  the  upper 
measure  of  51,  and  write 

I  =  Meas  51  =  Min  2rft. 

D 

2.  The  minimum  of  the  sums  1)  is  the  same  when  we  restrict  our 
selves  to  the  class  of  all  outer  enclosures. 

For  let  D=  \dt\  be  any  enclosure.  For  each  c?t,  there  exists  a 
cubical  division  of  space  such  that  those  of  its  cells,  call  them  d^ 

*~*  £ 

containing  points  of  d^  have  a  content  differing  from  dt  by  <  «;• 
Obviously  the  cells  \diK\  form  an  outer  enclosure  of  51,  and 


343 


344  MEASURE 

As  e  is  small  at  pleasure,  Min  2c?t  over  the  class  of  outer  en 
closures  =  Min  2c?t  over  the  class  of  all  enclosures. 

3.  Two  metric  sets  whose  common  points  lie  on  their  frontiers 
are  called  non-overlapping.     The  enclosure  D  =  2dt  is  called  non- 
overlapping,  when  any  two  of  its  cells  are  non-overlapping. 

Any  enclosure  D  may  be  replaced  by  a  non-overlapping  enclosure. 
For  let  U(d1^  c?2)  =  d1  4-  «2, 

U(d^  dz<  d3)  =  d1  +  e2  +  08, 
U(dl  d2  d3  d±)  =  d1  -h  ez  +  e3  +  «4,  etc. 

Obviously  each  en  is  metric.  For  uniformity  let  us  set  dj  =  er 
Then  E  =  \en\  is  a  non-overlapping  enclosure  of  31.  As 

£%.<*& 

we  see  that  £^#  minimum  of  the  sums  1)  ^s  the  same,  when  we  restrict 
ourselves  to  the  class  of  non-  overlapping  enclosures. 

Obviously  we  may  adjoin  to  any  cell  en,  any  or  all  of  its 
improper  limiting  points. 

4.  In  the  enclosure  E=  \en\  found  in  3,  no  two  of  its  cells 
have  a  point  in  common.     Such  enclosures  may  be  called  distinct. 

335.  1.  Let  D  =  \dt\,  E  =  \eK\  be  tivo  non-  overlapping  enclosures 
of%.  Let 

^  *!>»(<,  O- 

Then 

A=  5^1,        *,*  =  !,  2,  ... 

is  a  non-  over  lapping  enclosure  of  51. 

For  SiK  is  metric  by  22,  2.  Two  of  the  S's  are  obviously  non- 
overlapping.  Each  point  of  51  lies  in  some  dL  and  in  some  eK, 
hence  a  lies  in  8t(C. 

2.    We  say  A  is  the  divisor  of  the  enclosures  D,  E. 


336. 

For  let  E=  \e,\  be  an  enclosure  of  53.  Those  of  its  cells  dt  con 
taining  a  point  of  H  form  an  enclosure  D  =  \dt\  of  H.  Now  the 
class  of  all  enclosures  A  =  \B^  of  51  contains  the  class  D  as  a  sub 
class. 


UPPER  MEASURE  345 


As  2<2?t, 

we  have 

Min  2St<  Min  Zdt<  Min 

A  />  £• 

from  which  1)  follows  at  once. 
337.    If  21  w 


21  =  51.  (l 

For  let  D  be  a  cubical  division  of  space  such  that 

a/)_a<€  ,  a  -«/><€.  (2 

Let  us  set  33  =  1^.  Let  -#=JetJ  be  an  outer  enclosure  of  33. 
Since  33  is  complete,  there  exists  a  finite  set  of  cells  in  E  which 
contain  all  the  points  of  33  by  301.  The  volume  of  this  set  is 
obviously  >  33  ;  hence  a  fortiori 

2?t  >  8. 

Hence  =      - 

33>33. 

BUt  I>i,by336, 

>»  =  !i, 

>g-€,by2).  (3 

On  the  other  hand,      = 

2l<2U<2l  +  e,  by  2).  (4 

From  3),  4)  we  have  1),  since  e  is  arbitrarily  small. 

338.    If%  is  complete,     = 

31  =  21. 
For  by  definition  = 

21  =  Min  2aM 

with  respect  to  all  outer  enclosures  D  =  \dt\.  But  21  being  com 
plete,  we  can  replace  D  by  a  finite  set  of  cells  F=  \f,\  lying  in  D, 
such  that  F  is  an  enclosure  of  21.  Finally  the  enclosure  F  can  be 
replaced  by  a  non-overlapping  enclosure  G-  =  \g,}  by  334,  3. 


with  respect  to  the  class  of  enclosures    6r.     But  this  minimum 
value  is  also  21  by  2,  8. 


346  MEASURE 

339.    Let  the  limited  set  21  =  \Un\  be  the  union  of  a  finite  or  infinite 
enumerable  set  of  sets  2In.      Then 


For  to  each  ?Jfn  corresponds  an  enclosure  Dn  =  \  dni  \  such  that 
Sc?m  <  2In  +  —     •>     e  >  0,  arbitrarily  small. 

But  the  cells  of  all  the  enclosures  Z>n,  also  form  an  enclosure. 
Hence 


This  gives  1),  as  e  is  small  at  pleasure. 

340.    Let  n  lie  in  the  metric  set  2ft.     Let  A  =  2ft  -  21,  be  the 
complementary  set.      Then 


For  from  m  =  K  +  A, 

follows  =      _      = 

m<K  +  A,        by  339. 

But  .      _ 

9W  =  2ft,        by  337. 


341.    If  51  =  53  +  6,  awe?  53,  (£  are  exterior  to  each  other, 

1  =  S  +  f  .  (1 

For,  if  any  enclosure  D  —  \d^  of  51  embraces  a  cell  containing 
a  point  of  53  and  (£,  it  may  be  split  up  into  two  metric  cells  c?[, 
c?[',  each  containing  points  of  53  only,  or  of  (£  only.  Then 


Thus   we   may   suppose    the    cells    of    D   embrace   only  cells 

D'  =  \d(\    containing   no   point   of   (£,  and  cells  Df'  =  \d['l  con 
taining  no  point  of  53.     Then 

s5t  =  25;  +  25;'.  (2 


UPPER  MEASURE  347 

By  properly  choosing  D,  we  may  crowd  the  sum  on  the  left 
down  toward  its  minimum.  Now  the  class  of  enclosures  D'  is 
included  in  the  class  of  all  enclosures  of  33,  and  a  similar  remark 
holds  for  D". 

Thus  from  2)  follows  that 


This  with  339  gives  1). 

342.    If  51  =  23  +  9ft,  2ft  being  metric, 


For  let  D  be  a  cubical  division  of  norm  d.  Let  n  denote  points 
of  9ft  in  the  cells  containing  points  of  Front  9ft.  Let  tn  denote 
the  other  points  of  Oft-  Then  tn  and  33  are  exterior  to  each  other, 
and  by  337  and  341, 

Meas(33  +  m)  =  i  +  m. 
As  2l  =  33  +  tn  +  tt, 

Meas(33  +  m)<I         by  336. 
Als°  l<i  +  m  +  n         by  339. 

Thus  S  +  m<I<i  +  m  +  n.  (2 

Now  if  d  is  sufficiently  small, 

9ft-e<m     ;    tt<e. 
Thus  2)  gives,  as  rn<9ft, 


which  gives  1),  as  e>0  is  arbitrarily  small. 

343.     1.    Let  51  lie  in  the  metric  set  53,  and  also  in  the  metric  set 
£•     Let  £  =  %-%    ,     <7=<S-a. 

Then  §-J=§-5. 

For  let 

3)  = 


348  MEASURE 

Thus 

§  -  H  =  £  +  81  -  (§1  +  5)  =  S  -  5 
g  -  <7  =  S  +  Sj  -  (ii  4-  5)  =  S  -  S. 

2.    If   5l<53,   the    complement    of   51   with    respect   to  53  will 
frequently  be  denoted  by  the  corresponding  English  letter.     Thus 

Mod  53 


Lower  Measure 

344.  1.  We  are  now  in  position  to  define  the  notion  of  lower 
measure.  Let  51  lie  in  a  metric  set  2ft.  The  complementary  set 
A  =  2ft  —  51  has  an  upper  measure  A.  We  say  now  that  2ft  —  3 
is  the  lower  measure  of  51,  and  write 


By  343  this  definition  is  independent  of  the  set  2ft  chosen. 
When  |  _  ^ 

we  say  51  is  measurable,  and  write 


A  set  whose  measure  is  0  is  called  a  null  set. 

2.  Let  U=  [e,]  be  an  enclosure  of  A. 
Then  51  =  Max  (§*  -  25,)  » 

m'^  respect  to  the  class  of  all  enclosures  E. 

3.  If  (g  =  |et}  is  an  enclosure  of  51,  the  enclosures  ^  and  <g  may 
obviously,  without  loss  of  generality,  be  restricted  to  metric  cells 
which  contain  no  points  not  in  2ft.     If  this  is  the  case,  and  if  @, 
^are  each  non-overlapping,  we  shall  say  they  are  normal  enclosures. 

If  (§:,  8  are  two  normal  enclosures  of  a  set  51,  obviously  their 
divisor  is  also  normal. 


LOWER  MEASURE  349 

345.     1.  51  >0. 

For  let  51  lie  in  the  metric  set  $[)?. 

Then        /          2  =  ®-Z  "'.- 

But  by  336,  2<§, 

hence  2K-1>0. 

2.  5l<i. 

For  let  51  lie  in  the  metric  set  9ft. 
Then 


by  340. 
Hence  51  =  §?- 


346.    1.    For  any  limited  set  51, 

51  <  5j[*<  I  <  5l  (1 

For  let  Z>=  §dtj  be  an  enclosure  of  51.     Then 

51  =  Min  2<?t, 

,0 

when  Z>  ranges  over  the  class  F  of  all  ^wzVe  enclosures.     On  the 
other  hand, 

I  =  Min  2  d, 

D 

when  D  ranges  over  the  class  E  of  all  enumerable  enclosures. 
But  the  class  E  includes  the  class  F.     Hence  I  <  S. 

To  show  that  ™  ^  or  f  9 

21  <  <H,  V^ 

we  observe  that  as  just  shown 

A>I. 
Hence,  A  ^^ 

sw-A<sw»^  =  a.  (3 

A  +  5t  =  %        by  16. 
This  with  3)  gives  2). 


350  MEASURE 

2.    If  51  is  metric,  it  is  measurable,  and 

This  follows  at  once  from  1). 

347.    Let  51  be  measurable  and  lie  in  the  metric  set  9ft.      Then  A 
is  measurable,  and  «,      «>      ^ 

For 

A  =  9ft  -  5t.  (2 

since  51  is  measurable.     This  last  gives 


This  with  2)  shows  that  J  =  A  ;  hence  ^4.  is  measurable.     From 
2)  now  follows  1). 

348.  If    %<%,then  5T<<8.  (1 

For  as  usual  let  A,  B  be  the  complements  of  51,  23  with  respect 
to  a  metric  set  9ft.     Since  51  <  53,  A  >  B. 

Hence,  by  336, 

A>B. 

Thus,  ^      =      ^ 

9ft  -  4  <  9ft  -  B, 
which  gives  1). 

349.  For  51  to  be  measurable,  it  is  necessary  and  sufficient  that 


where  9ft  is  any  metric  set  >  51,  and  A  =  9ft  —  51. 
It  is  sufficient,  for  then  1)  shows  that 

!  =  §£-!. 

But  the  right  side  is  by  definition  51  ;  hence  3  =  5(. 
It  is  necessary  as  347  shows. 

350.    Let  51  =  {aj   be    the  union  of  an   enumerable  set  of  non 
overlapping  metric  sets.      Then  51  is  measurable,  and 

S  =  2an.  1 


LOWER  MEASURE  351 

Let  S  denote  the  infinite  series  on  the  right  of  1).     As  usual 
let  Sn  denote  the  sum  of  the  first  n  terms.     Let  5ln  =  (c^,  •••  an). 
Then  5ln  <  51  and  by  336, 

§n  =  #n<!     ,     for  any  n.  (2 

Thus  S  is  convergent  and 

£<I.  (3 

On  the  other  hand,  by  339, 

1  <  S.  (4 

From  3),  4)  follows  that 

S  =  I  =  lim  Sn  =  lim  Sn.  (5 

We  show  now  that  51  is  measurable.     To  this  end,  let  9ft  be  a 
metric  set  >  51,  and  2ln  +  An  =  9ft  as  usual. 

Then      I  in  +  2n  =  St     .  (6 

But  A  <  An     ,     hence  A  <  An. 

Thus  6)  gives  =      ^        ^ 

A  +  2ln  <  3ft, 
for  any  n.     Hence 


Hence  by  339,  J+8aafi|. 

Thus  by  349,  51  is  measurable. 


351.    Let 


For  let  9ft  be  a  metric  set  >  51.     Let  A,  B,  0  be  the  comple 
ments  of  51,  53,  S,  with  reference  to  9ft. 

Let  E=  \em\     ,     F=  \fn\ 

be  normal  enclosures  of  B,  C.     Let 


and  D  =  j^mn|  the  divisor  of  E,  F. 


352  MEASURE 

As  all  the  points  of  A  are  in  B,  and  also  in  (7,  they  are  in  both 
E  and  F,  and  hence  in  the  cells  of  D,  which  thus  forms  a  normal 
enclosure  of  A.  Let 

Let  us  set  _  /.  _        .   j 

m    '~       /in     I     t/  wi        '       */  TI  in     I         ?i  * 

Then  by  350,        -    _     -  - 

By  347,  _     !   ^  I       ^ 

?»  =   7m   +  9m        ,       /n  =   ??n  +  AB  . 

Hence  ^  ^ 


, 

Hence  adding, 

(^-2/n) 

rfmn)].       (2 

Thus  by  339,  the  term  in  [     ]  is  <  0.     Thus  2)  gives 


Now  ^  =  U\gm,  hn,  dmn\         m,n=l,  2, 


2n)  <       -  2wn  <  a.  (3 

But  ^ 

33  =  Max  (2ft  -  2?m) 


2  =  Max  (- 
Thus  3)  gives  1)  at  once. 

Measurable  Sets 

352.    1.    Let  H  =$  +  (£.     7f  53,  S   are    measurable,    then    51  i 
measurable,  and 

f  =  5  +  i.  ( 

For  <£  +  (£<  51     ,     by  351 

<  I  <  i  +  S     ,     by  339. 

*D      -i. 


LOWER  MEASURE  353 

2.    Let  51  =  33  +  (£.      If  51,  53  are  measurable,  so  is  &  and 

i  =  i-5.  (2 

For  let  51  lie  in  the  metric  set  9}?.      Then 

2fl  -  a  =  2K  -  OB  +  S)  =  (2»  -  G)  -  53- 
Thus  A  =  C-S; 

Hence  <7=S  +  A 

Thus  (7  is  measurable  by  1.     Hence  £  is  measurable  by  347, 
and 

5l  =  33  +  G. 

From  this  follows  2)  at  once. 

353.    1.    Let  51  =  25ln  be  the  sum  of  an  enumerable  set  of  measur 
able  sets.      Then  51  is  measurable  and 


If  51  is  the  sum  of  a  finite  number  of  sets,  the  theorem  is  obvi 
ously  true  by  352,  1.  In  case  51  embraces  an  infinite  number  of 
sets,  the  reasoning  of  350  may  be  employed. 

2.  Let  $1  =  \yin]  be  the  union  of  an  enumerable  set  of  null  sets. 
Then  $1  is  a  null  set. 

Follows  at  once  from  1. 

3.  Let  51=  J5InJ   be  the  union  of  an  enumerable  set  of  measurable 
sets  whose  common  points  two  and  two,  form  null  sets.      Then  51  is 
measurable  and 

§  =  25ln. 

4.  Let  G  =  \tn\  be  a  non-  overlapping  enclosure  0/51.      Then  (§:  is 

measurable,  and 

S  =  2en. 

5.  Let  53  <  51.     Those  cells  of  (£  containing  a  point  of  33  may 
be  denoted  by  33e,  and  their  measure  will  then  be  of  course 


If  $  =  51,  this  will  be  §.     This  notation  is  analogous  to  that 
used  in  volume  I  when  treating  content. 


354  MEASURE 

6.    If  g=  \\n\  is  another  non-overlapping  enclosure  of  some  set 
then 

T)  =  Dw((g,  g) 

is  measurable. 

For  the  cells  of  £)  are 

&. 

Thus  Stlt  is  metric,  and 


354.    1.    Harnack  Sets.     Let  21  be  an  interval  of  length  I.     Let 

X  =  Zx  +  Z2  +  ... 

be  a  positive  term  series  whose  sum  X  >  0  is  <_  I.  As  in  defining 
Cantor's  set,  I,  272,  let  us  place  a  black  interval  of  length  ^  in  the 
middle  of  21.  In  a  similar  manner  let  us  place  in  each  of  the  re 
maining  or  white  intervals,  a  black  interval,  whose  total  lengths 
=  Z2.  Let  us  continue  in  this  way;  we  get  an  enumerable  set  of 
black  intervals  53,  and  obviously 

§  =X. 

If  we  omit  the  end  points  from  each  of  the  black  intervals  we  get 
a  set  53*,  and  obviously 


The  set  £  =  51  -  53* 

we  call  a  Harnack  set.     This  is  complete  by  324  ;  and  by  338,  347, 


When  X  =  Z,  ^p  is  discrete,  and  the  set  reduces  to  a  set  similar 
to  Cantor's  set.  When  \<l,  we  get  an  apantactic  perfect  set 
whose  upper  content  is  I  —  X  >  0,  and  whose  lower  content  is  0. 

2.  Within  each  of  the  black  intervals  let  us  put  a  set  of  points 
having  the  end  points  for  its  first  derivative.  The  totality  of 
these  points  form  an  isolated  set  $  anc^  3'  =  €>•  But  b}r  331, 
3  =  $•  If  now  ^j  is  not  discrete,  <J  is  n°t-  We  have  thus  the 
theorem  : 

There  exist  isolated  point  sets  which  are  not  discrete. 


LOWER  MEASURE  355 

3.  It  is  easy  to  extend  Harnack  sets  to  $„.  For  example,  in  9?2, 
let  S  be  the  unit  square.  On  two  of  its  adjacent  sides  let  us  place 
congruent  Harnack  sets  $>.  We  now  draw  lines  through  the  end 
points  of  the  black  intervals  parallel  to  the  sides.  There  results 
an  enumerable  set  of  black  squares  @  =  \<Sn\.  The  sides  of  the 
squares  @  and  their  limiting  points  form  obviously  an  apantactic 
perfect  set  $. 

Let  af  +  a|+...  =  w 

be  a  series  whose  sum  0  <  m  <  1. 

We  can  choose  §  such  that  the  square  corresponding  to  its  larg 
est  black  interval  has  the  area  a\  ;  the  four  squares  corresponding 
to  the  next  two  largest  black  intervals  have  the  total  area  &\,  etc. 

Then  = 


Henoe         ... 

355.    1.    If  (g  =  \tm\  is  an  enclosure  of  %  such  that 


it  is  called  an  e-enclosure.  Let  A  be  the  complement  of  SI  with 
respect  to  the  metric  set  9D?.  Let  E  =  \en\  be  an  e-enclosure  of  A. 
We  call  (g,  E  complementarg  e-enclosures  belonging  to  SI. 

2.    //^  SI   is    measurable,   then  each  pair  of  complementary  e/2 
normal  enclosures  @,  ^,  wAosg  divisor  $)  = 


!5)  <  e,         e  small  at  pleasure.  (1 

For  let  (£,  J^  be  any  pair  of  complementary  e/2  normal  enclo 
sures.     Then 

t-f<{   ,  !-.!.<  f 

Adding,  we  get       0  <  S  +  2-  (84-2)<  c; 

0<S-h^-^<e.  (2 

But  the  points  of  9Q?  fall  into  one  of  three  classes  :  1°  the  points 
of  S)  ;  2°  those  of  (g  not  in  £)  ;  3°  those  of  j^  not  in  £).     Thus 

i  +  .f  =  ^  +  S. 

This  in  2)  gives  1). 


356  MEASURE 

356.  1.  Up  to  the  present  we  have  used  only  metric  enclosures 
of  a  set  21.  If  the  cells  enclosing  21  are  measurable,  we  call  the 
enclosure  measurable. 

Let  (£  =  \tn\  be  a  measurable  enclosure.  If  the  points  common 
to  any  two  of  its  cells  form  a  null  set,  we  say  (£  is  non- 
overlapping.  The  terms  distinct,  normal,  go  over  without 
change. 

2.     We  prove  now  that      |=  Min  ^  (1 

with  respect  to  the  class  of  non-overlapping  measurable  enclosures. 

For,  as  in  339,  there  exists  a  metric  enclosure  mn  =  \dnK\   of 

each  en  such  that  2  dnll  differs  from  ?n  by  <  e/2n.       But  the  set 

• 

\mn\  forms  a  metric  enclosure  of  21.     Tims 


<  2  <  K  <  2   en  +        =  2n  4-  e, 

ft  ,  K 

which  establishes  1). 


357.  Z0£  @  be  a  distinct  measurable  enclosure  of  21.  Let  \  denote 
those  cells  containing  points  of  the  complement  A.  If  for  each  e  >  0 
there  exists  an  (£  such  that  f  <•  e,  £  Aew  21  ^s  measurable. 

For  let  (g  =  e  +  f.     Then  e  <  21.     Hence  e  <  21  by  348.      But 


Hence  l 

and  thus  S  =  21 

358.    1.  .  The  divisor  £)  of  two  measurable  sets  2(,  53  ^ 


For  let  ($,  ^  be  a  pair  of  complementary  e/4  normal  enclosures 
belonging  to  21  ;  let  g,  F  be  similar  enclosures  of  53.     Let 


e  =  Dt;(<g,  J£)     ,     f  = 
Then 

?<e/2     ,    ?<€/:,         by  355,  2, 


LOWER   MEASURE  357 

Now  ©  =  Dv(&,  g)  is  a  normal  metric  enclosure  of  £).  More 
over  its  cells  g  which  contain  points  of  3)  and  (7(3)  )  lie  among 
the  cells  of  e,  f.  Hence 


Thus  b}r  357,  2)  is  measurable. 
2.    Let  51,  $8  be  measurable. 

Let  )     ,     II  = 


For 
Hence 


U  =     +  Meas  (53  - 


359.  Xe/  SI  =  U  \  5Im  j  be  the  union  of  an  enumerable  set  of 
measurable  cells  ;  moreover  let  51  be  limited.  Then  51  is  measurable. 
If  we  set 


For  2)  =  Dy^,  512)  is  measurable  by  358. 
T  »f 

51,  =  ^  +  ^    ,    5l2  =  £  +  a2. 
Then  ax,  a2  are  measurable  by  352,  2. 

AQ 

U  =  (5^,512)  =  2)4-^  +  02, 

U  is  measurable.     As  U  and  ^31  are  measurable,  so  is  332.     In  a 
similar  manner  we  show  that  $3,  534  •••  are  measurable.     As 


SI  is  measurable  by  353,  1,  and  the  relation  1)  holds  by  the  same 
theorem. 

360.     Let  5Tj  <  5I2  <  •••  be  a  set  of  measurable  aggregates  whose 
union  51  is  limited.      Then  51  is  measurable,  and 

5=limin. 


358  MEASURE 

For  let  Qf       «r  w       or 

a2  =  ^2-^i     >     ^3  =  ^3-^2  ••• 

For  uniformity  let  us  set  a:  =  21.     Then 

a  =  2o_. 

As  each  an  is  measurable 

t  =  2aw 

=  lim  (aj+  •••  +  an) 

n=oo 

=  lim  Sn  . 

361.  .Le£  Stj,  5I2  "*  ^  measurable  and  their  union  H  limited.  If 
£)  =  Dv  52IBj  >  0,  &  is  measurable. 

For  let  21  lie  in  the  metric  set  $ft; 
let  2)  +  D  =  2ft     ,     %n+An  =  m 

as  usual. 

Now  $)  denoting  the  points  common  to  all  the  2ln,  no  point  of 
D  can  lie  in  all  of  the  $(n,  hence  it  lies  in  some  one  or  more  of  the 
An.  Thus  D<\An\.  (1 

On  the  other  hand,  a  point  of  \An\  lies  in  some  Am,  hence  it 
does  not  lie  in  2lm.  Hence  it  does  not  lie  in  £).  Thus  it  lies  in 
D.  Hence  \An\<D.  (2 

From  1),  2)  we  have         D  =  $A  \ 

As  each  An  is  measurable,  so  is  D.     Hence  3)  is. 


362.    If  Hj^E^  •••  is   an  enumerable  set  of  measurable  aggre 
gates,  their  divisor  $)  is  measurable,  and 


For  as  usual  let  D,  An  be  the  complements  of  2),  2ln  with  respect 
to  some  metric  set  3ft. 

Then  D=\An\     ,     An<A»+l. 

Hence  by  360, 


LOWER   MEASURE  359 


As  $D  =  m  -  D, 

wehave  5  =  ^-5 

=  lim   §?- 


363.    1.    The  points  x  =  (x±  ••>  xm)  such  that 


form  a  standard  rectangular  cell,  whose  edges  have  the  lengths 
e1  =  bl  —  a1     ,     •••     ,     ^m  =  ^  —  am. 

When  e^  =  ez  =  •••  =  em,  the  cell  is  a  standard  cube.  A  normal 
enclosure  of  the  limited  set  SI,  whose  cells  S  =  Jenj  are  standard 
cells,  is  called  a  standard  enclosure. 


2.    For  each  e  >  0,  £fore  are  standard  e-enclosures  of  any  limited 

m*. 

For  let  (£  =  jenj  be  any  ry-enclosure  of  SI.     Then 

2en-i<)?.  (2 

Each  en  being  metric,  may  be  enclosed  in  the  cells  of  a  finite 
standard  outer  enclosure  Fn  ,  such  that 

Fn-tn<-n/ln    ,    ™  =  l,  2,... 

Then  g  =  \Fn\  is  an  enclosure  of  SI,  and 


<i+27;,         by  2). 

But  the  enclosure  .F  can  be  replaced   by  a   non-overlapping 
standard  enclosure  ©  =  5gn|,  as  in  334,  3.     But  ©  <  ^Fn. 
Hence  if  2  77  is  taken  <  e, 


and  ©  is  an  e-enclosure. 

3.    Let  £=!emj,         8=SW 

be  two  non-overlapping   enclosures  of  the  same  or  of   different 
sets.     Let  emn  =  Dv(tm,  fn). 


360  MEASURE 

^m==\^m,  !">    ^m.21    ^wi,  3  "  -V  ~^~  ^m">  C" 

then  0OT  is  measurable.  By  this  process  the  metric  or  measurable 
cell  tm  falls  into  an  enumerable  set  of  non-overlapping  measur 
able  cells,  as  indicated  in  3).  If  we  suppose  this  decomposition  to 
take  place  for  each  cell  of  (§,  we  shall  say  we  have  superimposed  g 
on  (£. 

364.    (IF".  H.  Young.}     Let  (£  be  any  complete  set  in  limited  21. 
2%era 

|  =  Max  <£.  (1 

For  let  8  lie  within  a  cube  2ft,  and  let  ^  =  90?  -  51,  (7=  2ft  -  (£ 
be  as  usual  the  complementary  sets. 

Let  53=  |bB}  be  a  border  set  of  (£  [328].  It  is  also  a  non- 
overlapping  enclosure  of  (7;  we  may  suppose  it  is  a  standard  en 
closure  of  C.  Let  E  be  a  standard  e-enclosure  of  A.  Let  us 
superimpose  E  on  53,  getting  a  measurable  enclosure  A  of  both  0 
and  A.  Then 

(7=  (7A>^A. 
Hence 

&  =  m-C=m-  (7A<9^-^A. 
Thus 

<£  =  (£,         by  338 

<  Meas  (2ft  -  ^4A) 

!A,         by  352,  2 


Hence 

(£<«, 

and  thus 

Maxg<|-  (2 

On  the  other  hand,  it  is  easy  to  show  that 

Max§>2t.  (3 

For  let  AD  be  an  e-outer  enclosure  of  A,  formed  of  standard 
non-overlapping  cells  all  of  which,  after  having  discarded  certain 
parts,  lie  in  2ft. 


LOWER   MEASURE  361 

Let  $  =  9ft  -  AD  +  ft,  (4 

where  g  denotes  the  frontier  points  of  AD  lying  in  21.  Obviously 
$  is  complete.  Since  each  face  of  D  is  a  null  set,  g  is  a  null  set. 
Thus  each  set  on  the  right  of  4)  is  measurable,  hence 

I  =  m  -  AD  +  § 

=  m-ID 

=  2JJ-2-e'     ,     0<e'<e 


Thus  Max  (£>$  =>|-e, 

from  which  follows  3),  since  e  is  small  at  pleasure. 

365.  1.  If  21  is  complete,  it  is  measurable,  and 

8  =  8. 
For  by  364, 

|  =  2I. 
On  the  other  hand, 

S=l,         by  338. 

2.    Let  33  be  any  measurable  set  in  the  limited  set  21.      Then 

|  =  Max  5.  (1 

For  |>33  =  §. 

Hence,  21  >  Max  5.  (2 

But   the   class  of  measurable   components    of   21    embraces  the 
class  of  complete  components  (£,  since  each  (£  is  measurable  by  1. 

Thus  Max  5  >  Max  £  (3 

From  2),  3)  we  have  1),  on  using  364. 

366.  Van  Week  Sets.     Let  (E  denote  the  unit  interval  (0,  1), 
whose  middle  point  call  M.     Let  3  denote  the  irrational  points  of 
(5.     Let  the  division  Dn,  w  =  1,  2,  •••  divide  (g  into  equal  intervals 

$n  of  length  l/2n. 


3(32  MEASURE 

We  throw  the  points  3  into  two  classes  51  =  \a  j,  53  =  \b\  having 
the  following  properties  : 

1°  To  each  a  corresponds  a  point  b  symmetrical  with  respect 
to  M,  and  conversely. 

2°  If  a  falls  in  the  segment  &  of  J9n,  each  of  the  other  seg 
ments  B'  of  Dn  shall  contain  a  point  a'  of  51  such  that  a'  is  situated 
in  S'  as  a  is  situated  in  B. 

3°  Each  S  of  Dn  shall  contain  a  point  a'  of  51  such  that  it  is 
situated  in  8,  as  any  given  point  a  of  51  is  situated  in  (g. 

4°  51  shall  contain  a  point  a  situated  in  (£  as  any  given  point 
a'  of  51  is  in  any  8n. 

The  1°  condition  states  that  51  goes  over  into  53  on  rotating  & 
about  M.  The  2°  condition  states  that  51  falls  into  n  =  1,  2,  22, 
23,  •••  congruent  subsets.  The  3°  condition  states  that  the  subset 
2ln  of  51  in  Bn  goes  over  into  51  on  stretching  it  in  the  ratio  2n  :  1. 
The  condition  4°  states  that  51  goes  over  into  5ln  on  contracting  it 
in  the  ratio  1  :  2n. 

We  show  now  that  51,  and  therefore  53  are  not  measurable.  In 
the  first  place,  we  note  that 

1-8, 

by  1°.     As  3  =  51  +  53,  if  51  or  53  were  measurable,  the  other  would 
be,  and  ^      ^ 

«=*-$. 

Thus  if  we  show  51  or  53  =  1,  neither  51  nor  53  is  measurable. 
We  show  this  by  proving  that  if  21  =  «<  1,  then  53  is  a  measurable 

set,  and  S3  =  1.     But  when  53  is  measurable,  $8  =  |-  as  we  saw,  and 
we  are  led  to  a  contradiction. 

Let  e  =  el  +  e2  -}-  •••  be  a  positive  term  series  whose  sum  e  is 
small  at  pleasure.  Let  ^  =  \en\  be  a  non-overlapping  ej-enclosure 
of  51,  lying  in  <g.  Then 

i1  =  2en  =  «  +  e;  =  «1     ,     0 
Let  53!  =  3  -  (gj  ;  then  53j  <  53,  and 


=  1  —  «  —  €j>l   —  «  — 


.    LOWER  MEASURE  363 

Each  interval  en  contains  one  or  more  intervals  7;nl,  ?/n2,  ...  of 
some  Z>,,  such  that 

f*?nm  =  en-0-n        ,         0  <  (7n 

where  v 

&  =  Zcrn 

may  be  taken  small  at  pleasure. 

Now  each  rjnm  has  a  subset  5lnTO  of  21  entirely  similar  to  21. 
Hence  there  exists  an  enclosure  (£nm  of  5lnra,  whose  measure  «nm  is 
such  that 


But   @2  =  {^n>«S    is  a    non-overlapping   enclosure   of   21,   whose 
measure  v~  ^^  . 

«2  =  «!Sr7nW  =  «l^  'On  -  ^n) 


if  <r  is  taken  sufficiently  small. 

Let  932  denote  the  irrational  points  in  (^  —  C?2.     It  is  a  part  of 
53,  and  332  has  no  point  in  common  with  ^&l.     We  have 


In  this  way  we  may  continue.     Thus  53  contains  the  measurable 
component  ^       ^ 

whose  measure  is 


>!-€. 
As  e  is  small  at  pleasure,  53  =  1. 

367.    (If.  H.  Young.)     Let 

«!,**,      V"  C1 

6e  an  infinite  enumerable  set  of  point  sets  whose  union  51  is  limited. 
Let  5ln>a>0  ,  n  =  1,  2  «••  Then  there  exists  a  set  of  points  each 
of  which  belongs  to  an  infinity  of  the  sets  1)  and  of  lower  measure  >  a. 


364  MEASURE 

For  by  365,  2,  there  exists  in  the  sets  1),  measurable  sets 

G,     ,    <52    ,    6,—          .  (2 

each  of  whose  measures  (£n  >  a.     Let  us  consider  the  first  n  of 
these  sets,  viz.:  ^     >     ^     _     ^  (g 

The  points  common  to  any  two  of  the  sets  3)  form  a  measurable 
set  £5^  by  358,  1.  Hence  the  union  (£ln  =  {  $)l(C  j  is  measurable,  by 
359.  The  difference  of  one  of  the  sets  3),  as  (^  and  Dv(&v  (Sln), 
is  a  measurable  set  cx  which  contains  no  point  in  common  with  the 
remaining  sets  of  3).  Moreover 

/».  <K. 

cx  >  a  -  (Slfl. 

In  the  same  way  we  may  reason  with  the  other  sets  (£2,  (E3  ••• 
of  3).  Thus  51  contains  w  measurable  sets  Cj,  C2  •••  cn  no  two  of 
which  have  a  common  point. 

Hence  c  =  Cl  +  ...  +  c. 

is  a  measurable  set  and 


The  first  and  last  members  give 

£,„>«-  la. 

n 
Thus  however  small  a  >  0  may  be,  there  exists  a  p  such  that 

Si,,       l-«.  •      ,  (4 


Let  us  now  group  the  sets  2)  in  sets  of  /a.     These  sets  give  rise 
to  a  sequence  of  measurable  sets 


such  that  the  points  of  each  set  in  5)  belong  to  at  least  two  of  the- 
sets  1)  and  such  that  the  measure  of  each  is  >  the  right  side  of  4). 
We  may  now  reason  on  the  sets  5)  as  we  did  on  those  in  2). 
We  would  thus  be  led  to  a  sequence  of  measurable  sets 


ASSOCIATE  SETS  365 

such  that  the  points  of  each  set  in  6)  lie  in  at  least  two  of  the  sets 
5),  and  hence  in  at  least  22  of  the  sets  1),  and  such  that  their 
measures  are. 


In  this  way  we  may  continue  indefinitely.  Let  now  ^3l  be  the 
union  of  all  the  points  of  51,  common  to  at  least  two  of  the  sets  1). 
Let  332  be  the  union  of  the  points  of  51  common  to  at  least  22  of 
the  sets  1),  etc.  In  this  way  we  get  the  sequence 

«!>«2>    ••• 
each    of   which   contains    a    measurable    set   whose    measure    is 


We  have  now  only  to  apply  25  and  364. 

368.  As  corollaries  of  367  we  have: 

1.  Let  Cj,  Q2  •••  be  an  infinite  enumerable  set  of  non-overlapping 
cubes  whose  union  is  limited.     Let  each  Qn  >  a  >  0.      Then  there 
exists  a  set  of  points  b  whose  cardinal  number  is  c,  lying  in  an  infin 
ity  of  the  On  and  such  that  b  >  a. 

2.  (Arzeld.)     Let  ^  ,  ?/2  •••  =77.      On  each  line  yn  there  exists  an 
enumerable  set  of  intervals  of  length  £„.     Should  the  number  of  inter 
vals  vn  on  the  lines  yn  be  finite,  let  vn  =  cc.     In  any  case  Bn  >  a  >  0, 
n  =  1,  2,  ...  and  the  projections  of  these  intervals  lie  in  51  =  (a,  5). 
Then  there  exists  at  least  one  point  x  =  f  in  51,  such  that  the  ordinate 
through  £  is  cut  by  an  infinity  of  these  intervals. 

Associate  Sets 

369.  1.    Let  e^e^eg  •••  =0.  (1 
Let  (gn  be  a  standard  en-enclosure  of  2ln.     If  the  cells  of  Q?n+1  lie  in 
<gn,  we  write                           @1>@2>-"                                               (2 
and  call  2)  a  standard  sequence  of  enclosures  belonging  to  1). 

Obviously  such  sequences  exist.     The  set 

%e  =  Vvl®n\ 

is  called  an  outer  associated  set  of  51.     Obviously 

51<5L. 


366  MEASURE 

2.    Each  outer  associated  set  5le  is  measurable,  and 
f=ie=limin. 

n=x> 

For  each  (gn  is  measurable;  hence  5le  is  measurable  by  362,  and 


=    ,         asen=0. 

370.    1.    Let  A  be  the  complement  of  51  with  respect  to  some 
cube  O  containing  5(.     Let  ,4.e  be  an  outer  associated  set  of  A. 

Then  a.=  o-^. 

is  called  aw  inner  associated  set  of  51.     Obviously 


2.    The  inner  associated  set  5It  is  measurable,  and 

§1=2. 

For  Ae  is  measurable  by  369,  2.     Hence  5lt  =  G  —  ^4.e  is  meas 
urable.     But 

Ae  =  A 
by  369,  2.     Hence 


Separated   Sets 

371.  Let  H,  53  be  two  limited  point  sets.  If  there  exist 
measurable  enclosures  (£,  g  °f  H,  53  such  that  3)  =  Dv(@,  g)  is  a 
null  set,  we  say  51,  53  are  separated. 

If  we  superimpose  g  on  (§,  we  get  an  enclosure  of  (£  =  (51,  53) 
such  that  those  cells  containing  points  of  both  51,  53  form  a  null 
set,  since  these  cells  are  precisely  £).  We  shall  call  such  an  en 
closure  of  (£  a  null  enclosure. 

Let  5l  =  {5ln}  ;  we  shall  call  this  a  separated  division  of  51  into 
the  subsets  5ln,  if  each  pair  5lm,  5ln  is  separated.  We  shall  also 
say  the  5ln  are  separated. 


SEPARATED   SETS  367 

372.    For  21,  53  to  be  separated,  it  is  necessary  and  sufficient  that 

2)  =  ZH2le,  53e) 
is  a  null  set. 

It  is  sufficient.     For  let 


Then  G  =  (a,b,5» 

is  a  measurable  enclosure  of  (£,  consisting  of  three  measurable 
cells.  Of  these  only  £)  contains  points  of  both  21,  53.  But  by 
hypothesis  £)  is  a  null  set.  Hence  21,  53  are  separated. 

It  is  necessary.  For  let  9D?  be  a  null  distinct  enclosure  of  (E, 
such  that  those  of  its  cells  9?,  containing  points  of  21,  $8  form  a 
null  set.  Let  us  superimpose  9#  on  the  enclosure  (£  above,  get 
ting  an  enclosure  g  of  21. 

The  cells  of  g  arising  from  a  contain  no  point  of  53  ;  similarly 
the  cells  arising  from  b  contain  no  point  of  21.  On  the  other 
hand,  the  cells  arising  from  £),  split  up  into  three  classes 


The  first  contains  no  point  of  53,  the  second  no  point  of  21,  the 
cells  of  the  last  contain  both  points  of  21,  53.      As  £)a,6<  W, 

$a.6  =  0.  (1 

On  the  other  hand, 

He  =  a  +  2>?l; 

hence  «+*>.+5>*>a. 

Thus  a  +  §0>S,  (2 

byl).     Also  g.=a  +  £=I        by  369,  2. 

This  with  2)  gives        ^      ^       ^      ^ 

a+  :Ta^>a  +  :I). 
Hence  3^^  (3 

But  l).>f}a  +  §6. 

This  with  3)  gives  £>6  =  0. 

In  a  similar  manner  we  find  that  £)a  =  0.     Hence  3)  is  a  null 
set  by  3). 


368  MEASURE 


373.    1.   J/  51,  $  are  separated,  then  £)  =  Dv($l,  $8)  is  a  null  set. 
For  S)e  =  Dv         23     is  a  nul1  set  b    3?2-     But  £)  <  2). 


2.  Let  51,  23  be  the  Van  Vleck  sets  in  366.  We  saw  there  that 
1  =  8  =  1.  Then  by  369,  2,  §c  =  5e  =  1.  The  divisor  of  5Ie,  23e  is 
not  a  null  set.  Hence  by  372,  51,  33  are  not  separated.  Thus  the 
condition  that  ^  be  a  null  set  is  necessary,  but  not  sufficient. 

374.  1.  Let  J51J,  \y$n\  oe  separated  divisions  of  51.  Let 
(£IK  =  Zhj(5It,  $3*).  Then  \&IK\  is  a  separated  division  0/"5l  also. 

We  have  to  show  there  exists  a  null  enclosure  of  any  two  of  the 
sets  <£„,  £mn.  Now  <£„  lies  in  51  and  53.  ;  also  £mn  lies  in  5Tm,  23n. 
By  hypothesis  there  exists  a  null  enclosure  &  of  5lt,  5lm;  and  a  null 
enclosure  g  of  23*,  23n.  Then  ©  =  Dv(&,  g)  is  a  null  enclosure  of 
5It,  5Im  and  of  58.,  33n.  Thus  those  cells  of  ®,  call  them  ®a,  con 
taining  points  of  both  5It,  5Tm  form  a  null  set;  and  those  of  its  cells 
©6,  containing  points  of  both  53K,  23n  also  form  a  null  set. 

Let  Gr—  \g\  denote  the  cells  of  ©  that  contain  points  of  both 
(£„,  (Smn.  Then  a  cell  g  contains  points  of  5ft  5TTO  53K  53n.  Thus  g 
lies  in  @a  or  ©6.  Thus  in  either  case  G-  is  a  null  set.  Hence  \&lK\ 
form  a  separated  division  of  51. 

2.  Let  D  be  a  separated  division  of  51  into  the  cells  d^  d2  -•• 
Let  E  be  another  separated  division  of  51  into  the  cells  e1,  e2--- 
We  have  seen  that  F  =  \flK\  where  fllt  =  Dv(dt,  eK~)  is  also  a  sepa 
rated  division  of  51.     We  shall  say  that  F  is  obtained  by  superim 
posing  E  on  D  or  D  on  ^,  and  write  F  '=  D  +  E=  E+  D. 

3.  Let  E  be  a  separated  division  of  the  separated  component  53 
of  51,  while  D  is  a  separated  division  of  51.     If  dt  is  a  cell  of  D,  eK 
a  cell  of  E,  and  c?t((  =  Dv(dL,  eK),  then 


Thus  superposing  E  on  D  causes  each  cell  c?t  to  fall  into  sepa 
rated  cells  e?tl,  c?tl  •••  St.  The  union  of  all  these  cells,  arising  from 
different  dt,  gives  a  separated  division  of  5(  which  we  also  denote 
by  D  +  E. 

375.  Let  J5tn|  be  a  separated  division  of  51.  Let  23  <  51,  and  let 
23n  denote  the  points  of  23  in  5(n.  TAew  J23nj  ^s  a  separated  division 
of*. 


SEPARATED   SETS  369 

For  let  $)  be  a  null  enclosure  of  5lm,  5In.  Let  S)^  denote  the 
cells  of  &  containing  points  of  both  5im,  5ln.  Let  (£  denote  the 
cells  of  2)  containing  points  of  $8  ;  let  (£a)6  denote  the  cells  con 
taining  points  of  both  53m,  53n.  Then 


As  $Da&  is  a  null  set,  so  is  (£«&. 

376.    1.    Letn  =  (53,  <£)  fo  a  separated  division  of  51. 

i  =  i  +  I  .  (i 

For  let  e1  >  €2  >  •••  =  0.  There  exist  en-measurable  enclosures 
of  5t,  53,  <£  ;  call  them  respectively  An,  Bn,  Cn.  Then  &n  =  An  + 
Bn  +  (7n  is  an  en-enclosure  of  51,  33,  (S  simultaneously. 

Since  53,  (S  are  separated,  there  exist  enclosures  B,  0  of  53,  & 
such  that  those  cells  of  D  =  B  +  0  containing  points  of  both  53 
and  (E  form  a  null  set.  Let  us  now  superpose  D  on  ($n  getting 
an  en-enclosure  En=\ena\  of  51,  53,  &  simultaneously.  Let  ebn 
denote  the  cells  of  En  containing  points  of  53  alone  ;  ecn  those 
cells  containing  only  points  of  (£  ;  and  ebc  those  cells  containing 
points  of  both  53,  (£.  Then 

2"ns  =  2?fen  +  Zecn  +  tebc  .  (2 

s 

As  2e6c  =  0,  we  see  that  as  n  ==  oo, 


Hence  passing  to  the  limit  w=  oo,  in  2)  we  get  1). 

2.    Let  51  =  f53nj  fo  a  separated  division  of  limited  51.      Then 

l  =  2g..  (1 

For  in  the  first  place,  the  series 

B  =  2§n  (2 

is  convergent.     In  fact  let  5In  =  (53X  ,  532  •  •  -  53n). 
Then  5IW  <  5T,  and  hence  In  <  I. 


370  MEASURE 

On  the  other  hand,  by  1 

in=i1+ ...  +  §„=£„, 

the  sum  of  the  first  n  terms  of  the  series  2).     Thus 

^n<I, 

and  hence  B  is  convergent  by  80,  4.     Thus 

^<i. 

On  the  other  hand,  by  339, 

£>i. 

The  last  two  relations  give  1). 


CHAPTER   XII 
LEBESGUE    INTEGRALS 

General  Theory 

377.  In  the  foregoing  chapters  we  have  developed  a  theory  of 
integration  which  rests  on  the  notion  of  content.     In  this  chapter 
we  propose  to  develop  a  theory  of  integration  due  to  Lebesgue, 
which  rests  on  the   notion  of  measure.     The  presentation  here 
given  differs  considerably  from  that  of  Lebesgue.     As  the  reader 
will  see,  the  theory  of  Lebesgue  integrals  as  here  presented  differs 
from  that  of  the  theory  of  ordinary  integrals  only  in  employing 
an  infinite  number  of  cells  instead  of  a  finite  number. 

378.  In  the  following  we  shall  suppose  the  field  of  integration 
SI  to  be  limited,  as  also  the  integrand  SI  lies  in  Sftm  and  for  brevity 
we  set/(#)  =f(xl  >••  xm).     Let  us  effect  a  separated  division  of 
SI  into  cells  Sj,  S2  •  ••.     If  each  cell  8t  lies  in  a  cube  of  side  d,  we 
shall  say  D  is  a  separated  division  of  norm  d. 

As  before,  let 


,     &>t  =  Osc/=  M,  -  m,     in  8t. 
Then  SD  =  I,Mfg    ,     ^,=  20*  A, 

the  summation  extending  over  all  the  cells  of  SI,  are  called  the 
upper  and  lower  sums  off  over  SI  with  respect  to  D. 
The  sum 


is  called  the  oscillatory  sum  with  respect  to  D. 
379.    If  m  =  Min  f,M=  Max  /  in  SI,  then 


m  <  mt  <M^<M. 

371 


372  LEBESGUE   INTEGRALS 

Hence 
Thus 


t  <SD<8j>< 

But  2lt  =  l, 

by  376,  2. 

380.     1.    Since  /is  limited  in  51, 

Max  $0     ,     Min  Sj) 

with  respect  to  the  class  of  all  separated  divisions  D  of  31,  are 
finite.  We  call  them  respectively  the  lower  and  upper  Lebesgue 
integrals  of  /over  the  field  51,  and  write 


=U*xSD     ;  /=Min^. 

In  order  to  distinguish  these  new  integrals  from  the  old  ones, 
we  have  slightly  modified  the  old  symbol  (  to  resemble  somewhat 
script  L,  or  I  ,  in  honor  of  the  author  of  these  integrals. 

J^i       JL^K 
we  say  /is  L-integrable  over  51,  and  denote  the  common  value  by 


which  we  call  the  L-integral. 

The  integrals  treated  of  in  Vol.  I  we  will  call  R-integrals,  i.e. 
integrals  in  the  sense  of  Riemann. 

2.    Letf  be  limited  over  the  null  set  51.      Then  f  is  L-integrable  in 
51,  and 


This  is  obvious  from  379. 

381.    Let  51  be  metric  or  complete.      Then 


GENERAL   THEORY  373 

For  let  dj,  c?2  •••  be  an  unmixed  metric  or  complete  division  of 
31  of  norm  d.     Let  each  cell  dk  be  split  up  into  the  separated  cells 

Then  since  d^  is  complete  or  metric, 

(*     =:  (I    =    2-.(1. 
i  t  ue 

Hence  using  the  customary  notation, 


Thus  summing  over  K, 

»,5.  < 

Summing  over  A  gives 
2wt3t  < 
Thus  by  definition, 


Letting  now  (^=0,  we  get  1). 

2.    Ze£  H  i«  metric  or  complete.     If  f  is  R-integrable  in  31,  it  is 
L-integrable  and 

(2 


3.    In  case  that  H  is  not  metric  or  complete,  the  relations  1),  2) 
may  not  hold. 

Example  1.     Let   31  denote  the  rational  points  in  the  interval 
(0,  1). 
Let 

/=  1,  for  x  =  —  ,  n  even 
n 

=  2,  when  n  is  odd. 
Then 

f/-l     ,      (T/-2; 

Ja  Jr 

while 


since  31  is  a  null  set.     Thus  1)  does  not  hold. 


374  LEBESGUE  INTEGRALS 

Example  2.     Let/=  1  at  the  rational  points  51  in  (0,  1).     Then 

=°  '  ^Lf<&-      (3 

Let  g=  —  1  in  51.     Then 


Thus  in  3)  the  i-integral  is  less  than  the  ^-integral,  while  in 
4)  it  is  greater. 

Example  3.     Let  /=  1    at   the    irrational   points  51  in  (0,  1). 
Then 


although  51  is  neither  metric  nor  complete. 

382.    Let  2),  A  be  separated  divisions  of  51.     Let 
E=D  +  &=  \et\. 


For  any  cell  d,  of  D  splits  up  into  c?tl,  dl9  •••  on  superimposing 
A,  and  =         = 

But  =       *    = 

and  =  = 

Thus  v  <  v  >  s 

383.    1.    Extremal  Sequences.     There  exists  a  sequence  of  sepa 
rated  divisions  n  r>  r>  (\ 

**\       •>       ^2       '       ^3  " 

each  Dn+1  being  obtained  from  Dn  by  superposition,  such  that 

(2 


GENERAL  THEORY  375 

For  let  el  >  e2  >  •••  =0.     For  each  en,  there  exists  a  division 
En  such  that 


Let  JSi  +  D!  =  Da     ,     ^3+D2  = 

and  for  uniformity  set  El  =  Dr     Then  by  382, 

sDn^<sDn  ,   SD^<SE^ 

Hence 


Letting  n  =  oo  we  get  2). 

Thus  there  exists  a  sequence  \D'n}  of  the  type  1)  for  2),  and  a 
sequence  \D'i  \  of  the  same  type  for  3).  Let  now  Dn  =  D'n  +  #'„'• 
Obviously  2),  3)  hold  simultaneously  for  the  sequence  \Dn\. 

2.  The  sequence  1)  is  called  an  extremal  sequence. 

3.  Let  \Dn}  be  an  extremal  sequence,  and  E  any  separated  divi 
sion  of  2(.      Let  En  =  Dn  +  E.      Then  E^  E^---  is  an  extremal 
sequence  also. 

384.    Let  f  be  L-integrable  in  31.      Then  for  any  extremal  sequence 

MU, 


inhere  dt  are  the  cells  of  Dn,  and  £  any  point  o/8(  in 
F°r 


Passing  to  the  limit  we  get  1). 

385.    1.    Let  m  =  Min/,  M=  Max/  tw  3[. 

Jfl. 
This  follows  at  once  from  379  and  383,  1. 


<  Af< 


376  LEBESGUE  INTEGRALS 

2.    Let  F  =  Max  \f\in  21,  then 

// 


< 


This  follows  from  1. 


386.    In  order  that  f  be  L-integrable  in  21,  it  is  necessary  that,  for 
each  extremal  sequence  \  Dn  \  , 

lim  flDf=  0; 


^s  sufficient  if  there  exists  a  sequence  of  superimposed  separated 
divisions  \  En  \  ,  such  that 

lim  £1EJ  =  0. 

n=ao 

It  is  necessary.     For 

/T 

lim  iS  I  =  lim 


As  /is  X-integrable, 

0=    f-    r=lirn(^n-^n)  =  limflz)n 
JL%    5^21 

It  is  sufficient.     For 


Both  \SEn\,  \&sn\  are  limited  monotone  sequences.  Their 
limits  therefore  exist.  Hence 

0  =  lim  £1E  =  lim  SE   —  lim  SE  . 

n  H  . H 

Thus 

oC'ffi       ow2l 

387.  J^i  order  that  f  be  L-integrable,  it  is  necessary  and  sufficient 
that  for  each  e  >  0,  there  exists  a  separated  division  D  of  H,  for 
which 


It  is  necessary.     For  by  386,  there  exists  an  extremal  sequence 
Dn\,  such  that 

0  <_  fl/>  /<  e     ,     for  any  n  >  some  m. 
Thus  we  may  take  Dm  for  D. 


GENERAL   THEORY  377 

It  is  sufficient.       For   let   e1>e2>  •••  =  0.     Let    \Dn\    be    an 
extremal  sequence  for  which 


Let  Aj  =  D1,  A2  =  Ax  +  Z>2,  A3  =  A2  +  D3  •••      Then    JAnj    is  a 
set  of  superimposed  separated  divisions,  and  obviously 


Hence  /  is  l/-iiitegrable  by  386. 

388.  In  order  that  f  be  L-integrable,  it  is  necessary  and  sufficient 
that,  for  each  pair  of  positive  numbers  o>,  cr  there  exists  a  separated 
division  D  of  21,  such  that  if  77^  ?;2,  •••  are  those  cells  in  which 
Osc/>  o>,  then 

2f.  <  <r.  (1 

It  is  necessary.  For  by  387  there  exists  a  separated  division 
D  =  JSJ  for  which 

flDf  =  SwA  <  G)(T.  (2 

If  ^,  ^2  ...  denote  the  cells  of  D  in  which  Osc/  <.&), 


This  in  2)  gives  1). 

It  is  sufficient.     For  taking  e  >  0  small  at  pleasure,  let  us  then 
take 

r-A     .     —  ^  (4 

2^1 

where  II  =  Osc  /in  51. 

From  1),  3),  and  4)  we  have,  since  COL  <  H, 

o-n  H-  aM  =  e. 


We  now  apply  387. 

389.    1.    Iff  is  L-integrable  in  H,  it  is  in  53  <  H. 

For  let  \Dn\  be  an  extremal  sequence  of  /relative  to  SI.     Then 
by  386, 


378  LEBESGUE  INTEGRALS 

But  the  sequence  \Dn\  defines  a  sequence  of  superposed  sepa 
rated  divisions  of  33,  which  we  denote  by  \En\.  Obviously 

nej<  nDj. 

Hence  by  1), 

<W=o, 

and  /  is  .L-integrable  in  23  by  386. 

2.    If  f  is  L-integrable  in  51,  so  is  |/|. 

The  proof  is  analogous  to  I,  507,  using  an  extremal  sequence 
for  /. 

390.  1.  Let  j5lnj  be  a  separated  division  of  51  into  a  finite  or  in 
finite  number  of  subsets.  Letf  be  limited  in  51.  Then 

//=//+//+-  a 

<£%         4^        ^2I2 

For  let  us  1°  suppose  that  the  subsets  5^  •••  5(r  are  finite  in  num 
ber.  Let  \Dn\  be  an  extremal  sequence  of/  relative  to  51,  and 
]Dmn\  an  extremal  sequence  relative  to  5Im.  Let 

En=Dn  +  Dln+  ...  +Drn. 

Then  \En\  is  an  extremal  sequence  of /relative  to  51,  and  also 
relative  to  each  51TO. 

Now  -  - 

*.JL-f*»Wt    •"    +^K^n- 

Letting  71  =  00,  we  get  1),  for  this  case. 
Let  now  r  be  infinite.     We  have 

i=flm.  (2 

Let  «„=(?!!  ...?in)   ,  en=?r-93n- 

Then  53n,  Sn  form  a  separated  division  of  51,  and 

S =€„  +  !„. 

If  v  is  taken  large  enough,  2)  shows  that 

^n<~     ,     rc>"     ,     jlf=Max|/|     in5T. 


GENERAL   THEORY  379 

Th  as  by  case  1°, 

' 


(3 

2In 

where  by  385,  2 

|e'|<Mn<e     ,     n>v. 

Thus  1)  follows  from  3)  in  this  case. 

2.    Let  l^inl  be  a  separated  division  0/51.      Then 


iffis  L  integrable  in  51,  or  if  it  is  in  each  2In,  and  limited  i 
391.    1.    Letf  =  ^  i/i  51  except  at  the  points  of  a  null  set 


in 


:21 
Forlefc 


//=/,.  a 

^21         4:21 
=8+  ft.     Then 

f/=  f/+f/=//.  (2 

4:21         ilJ         4SJ?         4^8 

Similarly  //=J/  (3 

But/  =  ^  in  83.     Thus  2),  3)  give  1). 
392.    1.    7/00; 

If  e  <  0  ;         Jc/  =  c  J/,         £cf  =  e  jf. 


The  proof  is  similar  to  3,  3,  using  extremal  sequences. 
2.    Iffis  L-  integrable  in  51,  so  is  cf,  and 


^s  a  constant. 


380  LEBESGUE  INTEGRALS 

393.    1.    Let  F(x)  =  fl(x)  +  •••  +/„<»,  each  fm  being  limited 
in  2i.     Then 


For  let  jDnj  be  an  extremal  sequence  common  to  F^fv  •••/„.     In 
each  cell 

dn\       »        ^n2  '  '  ' 

of  Dn  we  have 

2  Min/m  <  Min  F  <  Max  F  <  2  Max/m  . 

Multiplying   by   dns,    summing  over    s   and   then   letting  w  =  oo, 
gives  1). 


2.    Iff^x),  •••/„(«)  are  each  L-integrable  in  31,  so  u 
and 

394.    1. 


For  using  the  notation  of  393, 
Min  (/+#)  <  Min/+ 


in  each  cell  dns  of  Dn. 


2.    If  g  is  L-integrable  in  51, 

f  (/+< 

^21 
Reasoning  similar  to  3,  4,  using  extremal  sequences. 

3-  f(f-g)<ff-fg. 

^21  <X2l         ^2t 

ff-  f 

JLw        JLw, 


g< 


GENERAL   THEORY  381 

f  (/-*)  <  f /  +  /'(-</)  <  ff-  fg; 

<^2l  <=L>y(          s^2l  «^2l          «^2l 

etc. 

4.    Iff,  g  are  L-integrable  in  Si,  so  isf  —  g,  and 

L(f~9)=Lf~ 

^ . .  ^  . 


395.  -/f/,  #  are  L-integrable  in  SI,  so  is./-  (/. 

J.?so  ^eir  quotient  f/g  is  L-integrable  provided  it  is  limited  in  51. 

The  proof  of  the  first  part  of  the  theorem  is  analogous  to  I, 
505,  using  extremal  sequences  common  to  both  /  and  g.  The 
proof  of  the  second  half  is  obvious  and  is  left  to  the  reader. 

396.  1.    Let  f,  g  be  limited  in  SI,  and  f  <^g,  except  possibly  in  a 
null  set  yi.      Then  -^  -^ 

I  f<  I  g-  (i 

Xsi        ^,21 
Let  us  suppose  first  that/<:  #  everywhere  in  SI. 

Let   \Dr\   be  an  extremal  sequence  common  to  both  /  and  g. 

Then  „     f^  u   , 

b/)nj  <-&Dng. 

Letting  n  =  oo ,  we  get  1). 

We  consider  now  the  general  case.     Let  SI  =  53  4-  $1-     Then 


since 


//=// ,  /,=/ 

^21         ^33  <^2l         =^33 

lf-fc-* 


But  in  53,  f<g  without  exception.     We  may  therefore  use  the 
result  of  case  1°. 

2.    Letf>Qin%.     Then 


382  LEBESGUE   INTEGRALS 

397.    The  relations  of  4  also  hold  for  L-integrals,  viz.  : 

Iff  </!/!•  (i 

l^fca       £%. 

f/<    f/-  (2 

^51  <^2l 

<  f/<  fl/l-  (3 

«L2l         ^21 

(4 


The  proof  is  analogous  to  that  employed  for  the  72-integrals, 
using  extremal  sequences. 

398.    Let  2l  =  08u,  @«)  t>e  a  separated  division  for  each  u  =  0. 
Let  ltt  =  0.      Then 


lim 
«=0 
For  by  390,  l, 


im    f  /  =   f  / 
=0  ^33M       4^21 


But  by  385,  2,  the  last  integral  =  0,  since  (£„  =  0,  and  since  /is 
limited. 


399.  Xe^  f  be  limited  and  continuous  in  51,  except  possibly  at  the 
points  of  a  null  set  $ft.  Then  f  is  L-integrable  in  5(. 

Let  us  first  take  91  =  0.  Then/  is  continuous  in  51.  Let  51  lie 
in  a  standard  cube  £}.  If  Osc/  is  not  <  e  in  51,  let  us  divide  Q 
into  2n  cubes.  If  in  one  of  these  cubes 

Osc/<  e,  (1 

let  us  call  it  a  black  cube.  A  cube  in  which  1)  does  not  hold  we 
will  call  white.  Each  white  cube  we  now  divide  in  2n  cubes. 
These  we  call  black  or  white  according  as  1)  holds  for  them  or 
does  not.  In  this  way  we  continue  until  we  reach  a  stage  where 
all  cubes  are  black,  or  if  not  we  continue  indefinitely.  In  the 
latter  case,  we  get  an  infinite  enumerable  set  of  cubes 

<h>  <fe'  ^3  •"  (2 


GENERAL   THEORY  383 

Each  point  a  of  51  lies  in  at  least  one  cube  2).  For  since  /  is 
continuous  at  x  =  a, 

!/CO-/OOI<«/2     ,     x  in    r,(«). 

Thus  when  the  process  of  division  has  been  carried  so  far  that 
the  diagonals  of  the  corresponding  cubes  are  <  8,  the  inequality 
1)  holds  for  a  cube  containing  a.  This  cube  is  a  black  cube. 

Thus,  in  either  case,  each  point  of  51  lies  in  a  black  cube. 

Now  the  cubes  2)  effect  a  separated  division  D  of  51,  and  in 
each  of  its  cells  1)  holds.  Hence  /is  .L-integrable  in  5T. 

Let  us  now  suppose  %l  >  0.     We  set 

5l  =  £  +  ft. 

Then  /is  Z-integrable  in  (£  by  case  1°.  It  is  L-integrable  in  $1 
by  380,  2.  Then  it  is  L-integrable  in  51  by  390,  1. 

2.  If  /  is  L-integrable  in  51,  we  cannot  say  that  the  points  of 
discontinuity  of/  form  a  null  set. 

Example.     Let/=  1  at  the  irrational  points  $,  in  51  =  (0,  1)  ; 

=  0  at  the  other  points  9?,  in  51. 
Then  each  point  of  51  is  a  point  of  discontinuity.     But  here 


since  tit  is  a  null  set.     Thus  /is  L-integrable. 

400.    Iff(xl  •••  xni)  has  limited  variation  in  51,  it  is  L-integrable. 

For  let  D  be  a  cubical  division  of  space  of  norm  d.     Then  by  I, 
709,  there  exists  a  fixed  number  V,  such  that 

2a>(dm-l<  V 

for  any  D.     Let  o>,  cr  be  any  pair  of  positive  numbers.     We  take 
d  such  that 

.  a 


Let  d(  denote  those  cells  in  which  Osc/>&>,  and  let  the  number 
of  these  cells  be  v.     Let  rj,  denote  the  points  of  51  in  d{  .     Then 

l<^,(odm-l<  V. 


384  LEBESGUE   INTEGRALS 


Hence 

v< 

Thus 


ox 

2), 


••         <Va<*    .    by*)-      ' 

Hence /is  .L-integrable  by  388. 

401.    Let  <t>  =/,  in  51  <  33  ; 

=  0,  in  A  =  33  -  5t. 

f /-  /V     - 

<X2t  els 

if  1°,  <f)  is  L-integrable  in  33  ;   or  2°,  /  is  L-integrable  in  51, 
are  separated  parts  of  33. 

On  the  1°  hypothesis  let  J(SS|  be  an  extremal  sequence  of  </>. 
Let  the  cells  of  @8  be  e^,  ez  •••  They  effect  a  separated  division 
of  51  into  cells  d^  d%  •••  Let  mt,  M~t  be  the  extremes  of /in  c?t  and 
wt,  JV[  the  extremes  of  (/>  in  et.  Then  for  those  cells  containing  at 
least  a  point  of  5(, 

is  obviously  true  when  et  =  d^.     Let  dk  <  et.     If  mt  <  0, 

nt^t  <^ mtc?t ,         since  mi  =  ni.  (3 

If  mt  >  0,  wt  =  0,  and  3)  holds. 

If  Mt  <_  0,  Jftc?t  <  Nfc ,         since  ^Vt  =  0.  (4 

If  M^  >  0,  4)  still  holds,  since  ML  =  Nt. 
Thus  2)  holds  in  all  these  cases.     Summing  2)  gives 


for  the  division  ($a,  since  in  a  cell  e  of  (§,  containing  no  point  of 
<t>  =  0.     Letting  s  =  oo,  we  get  1),  since  the  end  members 


INTEGRAND   SETS  385 

On  the  2°  hypothesis, 

f  </>=  r*+  r*=  r*=  r /, 

<X«B  <^2l  <^J.  •&*  el/t 

since  0  being  =  0  in  A,  is  .L-integrable,  and  we  can  apply  390. 
402.     1.    If 


/=o, 

we  call /a  null  function  in  51. 

2.    Iff>  0  is  a  null  function  in  51,  the  points  ty  where  f  >  0  form 


o 


For  let  51  =  3  +  ?,  so  that/=  0  in  3. 
By  401,  .  ^ 

=  //=//•  a 

«z«     x* 


Let  €j  >  e2  >  •••  =  0.     Let  ^3n  denote   the   points  of  $  where 
/>€n.     Then 

%f  =  0,         byl). 


Each  <>pn  is  a  null  set.     For 


Hence  ^n  =  0. 

Then  *  =  J?nJ=Gi+C2+- 

where          ^  =  ^,          $2=^2-^,          $3=^33-$3... 
As  each  §n  is  a  null  set,  $  is  a  null  set. 

Integrand  Sets 

403.  Let  51  be  a  limited  point  set  lying  in  an  w-way  space  $ftm. 
Let  f  (xl  •••  xm)  be  a  limited  function  denned  over  51.  Any 
point  of  21  may  be  represented  by 

a  =  (flj  ...  «m). 


386  LEBESGUE   INTEGRALS 

The  point  x  =  ^  •••  amxm+l) 

lies  in  an  m  +  1  way  space  $ftm+1.  The  set  of  points  J  x\  in  which 
xm+1  ranges  from  —  oo  to  +00  is  called  an  ordinate  through  a.  If 
xm+1  is  restricted  by  Q  <  ^  ^  ^ 

we  shall  call  the  ordinate  a  positive  ordinate  of  length  I  ;  if  it  is  re 
stricted  by  _  l<Xm+l<0, 

it  is  a  negative  ordinate.  The  set  of  ordinates  through  all  the 
points  a  of  H,  each  having  a  length  =/(«),  and  taken  positively 
or  negatively,  as  /(a)  is  ^  0,  form  a  point  set  $  in  9?m+1  which 
we  call  an  integrand  set.  The  points  of  $  f°r  which  xm+1  has  a 
fixed  value  xm+1  =  e  form  a  section  of  3,  and  is  denoted  by  3(<?)  or 

by  a- 


404.  Z0£  21=  j#J  fo  a  limited  point  set  in  9?TO.  Through  each 
point  «,  let  us  erect  a  positive  ordinate  of  constant  length  /,  getting  a 
set  £),  in  Wm+1  .  Then  g  =  ;fj  (\ 

For  let  Q?!  >  (£2  >  •••  form  a  standard  sequence  of  enclosures  of 

O,  such  that  j^  ^  ^  ^ 

Let  us  project  each  section  of  (£n  corresponding  to  a  given  value 
of  zm+  on  $m,  and  let  5ln  be  their  divisor.  Then  5ln  >  31.  Thus 


Letting  n  =  oo  ,  and  using  2),  we  get 

6  =  1  •  i. 

To  prove  the  rest  of  1),  let  0  be  the  complement  of  D  with  re 
spect  to  some  standard  cube  Q  in  9^TO+1,  of  base  Q  in  9?m. 
Then,  as  just  shown, 

0  =IA    ,     where  .4  =  Q  -  51. 
Hence 


INTEGRAND   SETS  387 

405.    Letf  >0  be  L-integralle  in  21.      Then 


where  $  is  the  integrand  set  corresponding  to  f. 

For  let   J£tj   be  a  separated  division  .Z)  of  21.      On  each  cell 
erect  a  cylinder  (£t  of  height  Mt  =  Max/  in  St.     Then  by  404, 


Let  (£=  {(SJ  ;  the  (£t  are  separated.     Hence,  e>0  being  small 
at  pleasure, 


for  a  properly  chosen  D.     Thus 

§<  f/.  (2 

^21 
Similarly  we  find 

f/<5.  (3 

^2t 

From  2),  3)  follows  1). 

406.    Letf>0  be  L-integrable  over  the  measurable  field  21.      Then 
the  corresponding  integrand  set  3  is  measurable,  and 


For  by  2)  in  405, 

§<  f  /• 

x« 

Using  the  notation  of  405,  let  cn  be  a  cylinder  erected  on  8n  of 
height  mn  =  Min/  in  8B.     Let  c  =  JcJ.     Then  c  <  3,  and  hence 

c<3-  (2 

But  21  being  measurable,  each  cn  is  measurable,  by  404.     Hence 
c  is  by  359.     Thus  2)  gives 

c<3-  (3 

Now  for  a  properly  chosen  Z>, 

-*+  r/<27wtst=T. 


388  LEBESGUE   INTEGRALS 

Hence 


. 

as  e  is  arbitrarily  small.     From  2),  3),  4) 


from  which  follows  1). 


Measurable  Functions 

407.    Let/Oj  •••  xm)  be  limited  in  the  limited  measurable  set  51. 
Let  2(v  denote  the  points  of  51  at  which 


If  each  5lxM  is  measurable,  we  say/z's  measurable  in  5(. 

We  should  bear  in  mind  that  when  /is  measurable  in  5(,  neces 
sarily  51  itself  is  measurable,  by  hypothesis. 

408.    1.    Iff  is  measurable  in  51,  the  points  &  of  51,  at  which  f  —  0, 
form  a  measurable  set. 

For  let  5ln  denote  the  points  where 


where  €l>62>...=o. 

Then    by    hypothesis,    5ln    is    measurable.      But    ^  — 
Hence  (£  is  measurable  by  361. 

2.    Iffis  measurable  in  51,  the  set  of  points  where 


is  measurable,  and  conversely. 
Follows  from  1,  and  407. 

3.    If  the  points  5IA  in  51  where  f>\  form  a  measurable  set  for 
each  X,  /  is  measurable  in  51. 

For  51^  having  the  same  meaning  as  in  407, 

5lx,  =  5Tx-5TM. 
Each  set  on  the  right  being  measurable,  so  is  5lxM  • 


MEASURABLE   FUNCTIONS  389 

409.    1.    Iffis  measurable  in  21,  it  is  L-integrable. 

For  setting  m  =  Min  /,  M  =  Max  /  in  21,  let  us  effect  a  division 
D  of  the  interval  g  =  (w,  M)  of  norm  c?,  by  interpolating  a  finite 
number  of  points 

7W1<7W2<Wg<    -•• 

Let  us  call  the  resulting  segments,  as  well  as  their  lengths, 

dl,  d%,  d3  "- 
Let  2lt  denote  the  points  of  21  in  which 

ml-i<f<ml     ,     i  =  l,  2,  ...  ;  mQ  =  m. 
We  now  form  the  sums 

SD  =  2wt-iit     ,     */,  =  2wtit. 
Obviously 


But     t/>-t^  =  m151  +  «A 

=  5(i(mi  -  ™)  4- 


=  0     ,     asrf  =  0.  (2 

We  may  now  apply  387. 

2.    Iff  is  measurable  in  21 

**  A 

/=lim 


L 


using  the  notation  in  1. 

This  follows  from  1),  2)  in  1. 

3.  The  relation  3)  is  taken  by  Lebesgue  as  definition  of  his 
integrals.  His  theory  is  restricted  to  measurable  fields  and  to 
measurable  functions.  For  Lebesgue's  own  development  of  his 
theory  the  reader  is  referred  to  his  paper,  IntSgrale,  Longueur •, 
Aire,  Annali  di  Mat.,  Ser.  3,  vol.  7  (1902)  ;  and  to  his  book, 
Lemons  sur  I1  Integration.  Paris,  1904.  He  may  also  consult  the 
excellent  account  of  it  in  Nobsons  book,  The  Theory  of  Functions 
of  a  Real  Variable.  Cambridge,  England,  1907. 


390  LEBESGUE   INTEGRALS 


Semi-Divisors  and  Quasi-  Divisors 

410.    1.    The  convergence  of   infinite   series  leads  to  the  two 
following  classes  of  point  sets. 

T  of 

Let 


F=  2/.C*,  ...  xj  =  2/;  +  2/.  =  Fn 

1  n+1 


each/t  being  defined  in  21. 

Let  us  take  e  >  0  small  at  pleasure,  and  then  fix  it. 
Let  us  denote  by  2ln  the  points  of  H  at  which 

-  e  <  Fn(x)  <  e.  (2 
Of  course  5ln  may  not  exist.     We  are  thus  led  in  general  to  the 

Sets                                               or               or               or  /•* 

*»|      ?      <^2      »      ^3  v*3 

The    complementary  set   An  =  51  —  5ln  will   denote  the   points 

where                    !>«.  ..•  (4 


If  now  F  is  convergent  at  #,  there  exists  a  i>  such  that  this  point 

lies  in  or  or  or  sz 

<*v     »     ^+1     ^     -u-v+2  \° 

The  totality  of  the  points  of  convergence  forms  a  set  which  has 
this  property  :  corresponding  to  each  of  its  points  #,  there  exists 
a  v  such  that  x  lies  in  the  set  5).  A  set  having  this  property  is 
called  the  semi-divisor  of  the  sets  3),  and  is  denoted  by 

Sdv  J2IJ. 

Suppose  now,  on  the  other  hand,  that  1)  does  not  converge  at 
the  point  x  in  51.  Then  there  exists  an  infinite  set  of  indices 

^i  <  n%  <  •••  =  oo, 

such  that  = 

I  -F»aO)  I   >  €. 

Thus,  the  point  x  lies  in  an  infinity  of  the  sets 

Al    ,     A2    ,    A3  •••  (6 

The  totality  of  points  such  that  each  lies  in  an  infinity  of  the 
sets  6)  is  called  the  quasi-divisor  of  6)  and  is  denoted  by 

QdrM,!. 

Obviously, 

HnS  +  QdvJ^nS  =  3l.  (7 


SEMI-DIVISORS   AND   QUASI-DIVISORS  891 

We    may  generalize   these    remarks  at   once.     Since  F(x)   is 
nothing  but 


we  can  apply  these  notions  to  the  case  that  the  functions/,^  •••  xm) 
are  defined  in  51,  and  that 


2.    We  may  go  still  farther  and  proceed  in  the  following  abstract 
manner. 

The  divisor  £)  of  the  point  sets 

HI  ,  v-  •  a 

is  the  set  of  points  lying  in  all  the  sets  1). 

The  totality  of  points  each  of  which  lies  in  an  infinity  of  the  sets 
1)  is  called  the  quasi-divisor  and  is  denoted  by 


(2 


The  totality  of  points  a,  to  each  of  which  correspond  an  index  m 
such  that  a  lies  in 


forms  a  set  called  the  semi-divisor  of  1),  and  is  denoted  by 

Sdv  {'«.}.  (3 

If  we  denote  2),  3)  by  G  and  @  respectively,  we  have,  obviously, 

£)  <  @  <  O.  (4 

3.    In  the  special  case  that  2Ij  >212  >  •••  we  have 

Q  =  @  =  5).  (5 

For  denoting  the  complementary  sets    by  the  corresponding 
Roman  letters,  we  have 


But  Q  has  precisely  the  same  expression. 
Thus  G  =  S),  and  hence  by  4),  @  =  £). 


392  LEBESGUE   INTEGRALS 

4.    Z^5ln  +  A»  =  93>     ra  =  l,2,...     Then 


For  each  point  b  of  93  lies 

either  1°  only  in  a  finite  number  of  5ln,  or  in  none  at  all, 
or  2°  in  an  infinite  number  of  5ln. 

In  the  1°  case,  b  does  not  lie  in  518,  5ls+1  •••  ;  hence  it  lies  in 
A,,  Aa+1  •••     In  the  2°  case  b  lies  obviously  in  Qdv  [51J. 

5.  If  5^,  5f2  •••  are  measurable,  and  their  union  is  limited, 

n  =  Qdvj5u   ,  e  =  sdvj5u 

are  measurable. 

For  let  S)n  =  Dw(3Cn,  5In+1  •••)  .     Then  @  =  j$nj  . 

But  @  is  measurable,  as  each  £)n  is.     Thus  Sdv  J  J.nJ  is  measur 
able,  and  hence  Q  is  by  4. 

6.  £e£  O  =  Qdv  55ln|  ,  c«(?A  Hn  6ezw^  measurable,  and  their  union 
limited.     If  there  are  an  infinity  of  the  5ln,  say 


measure  is  >  a, 

Q>«.  (6 


For  let  53n  =  (5(ln,  5lln+1  .••),  then 
Let  53  =  Dw{«»}  .     As  «n  >  »B+1, 

S  =  limSn>«  (7 

by  362.     As  O>93  we  have  6)  at  once,  from  7). 


Limit  Functions 
411.    Let 


as  x  ranges  over  51,  r  finite  or  infinite.  Let  f  be  measurable  in  51 
and  numerically  <M,for  each  t  near  r.  Then  <j>  is  measurable  in 
51  also. 

To  prove  this  we  show  that  the  points  93  of  51  where 


LIMIT  FUNCTIONS  393 

form  a  measurable  set  for  each  X,  p.  For  simplicity  let  T  be  finite. 
Let  £1?  t2~.  =T;  also  let  €1>e2>  •  ••  =0.  Let  (£„,,  denote  the 
points  of  21  where 

.)  </*  +  «»•  (2 


Then  for  each  point  x  of  33,  there  is  an  «0  such  that  2)  holds  for 
any*,,  if  s>  v     Let  £n  =  Sdv  f(£n,J  .     Then  8  <  <£B  .     But  the  &M 

being  measurable,  (£ft  is  by  410,  5.     Finally  23  =  Dv  J(£J  ,  and  hence 
53  is  measurable. 

412.    Let 


for  x  in  51,  and  r  finite  or  infinite.  Let  tf,  t"  •  ••  =T.  Let  each 
fs  =/(#,  t(9))  be  measurable,  and  numerically  <  M.  Let  <f>=fg  +  g8. 
Let  ©8  denote  the  points  where 

9.\>*- 

Then  for  each  e  >  0,  Um  ^  =  Q>  (1 

*=*> 

For  by  411,  <^>  is  measurable,  hence  gt  is  measurable  in  51,  hence 
®,  is  measurable. 

Suppose  now  that  1)  does  not  hold.     Then 


Then   there    are    an    infinity   of    the   ®8,   as    ®,t,  ®a2---   whose 
measures  are  >X>0.     Then  by  410,  6,  the  measure  of 


is  >  X.     But  this  is  not  so,  since/,  =  (/>,  at  each  point  of  SI. 
413.    1.    Let   v 


for  x  in  51,  and  T  finite  or  infinite. 


Ifeachf,=f(x,  #a))  is  measurable,  and  numerically  <M  in 
each  sequence  1),  then 

/-»  /-a 

0-  (2 


394  LEBESGUE   INTEGRALS 

For  set  ,       /. 

£=/.+#n 

and  let  \      \  ^  -\r  -in 

|&|:$-y    ,     «=!,  2  ... 

Then  as  in  412,  <£  and  #8  are  measurable  in  51.     Then  by  409, 
they  are  Z-integrable,  and 


(3 

Let  $3a  denote  the  points  of  51,  at  which 

and  let  $88  +  B8  —  51.     Then  238,  B8  are  measurable,  since  ga  is. 
Thus  by  390,  ~  „  „ 

J  ^=2  gs+l/8' 
Hence  .,  _ 

i/8  - 

ovii 

By  412,  58  =  0.     Thus 


Hence  passing  to  the  limit  in  3),  we  get  2),  for  the  sequence 
1).  Since  we  can  do  this  for  every  sequence  of  points  t  which 
=  T,  the  relation  2)  holds. 

it* 


converge  in  51.     If  each  term  /t  is  measurable,  and  each 
then  F  is  L-integrable,  and 


Iterated  Integrals 
414.    In  Vol.  I,  732,  seq.  we  have  seen  that  the  relation, 


holds  when  /is  72-integrable  in  the  metric  field  51.     This  result 
was  extended  to  iterable  fields  in  14  of  the  present  volume.     We 


ITERATED  INTEGRALS  395 


wish  now  to  generalize  still  further  to  the  case  that  f  is  j 
grable  in  the  measurable  field  51.  The  method  employed  is  due  to 
Dr.  W.  A.  Wilson,*  and  is  essentially  simpler  than  that  employed 
by  Lebesgue. 

1.  Let  x  =  (Zj  •••  z,)  denote  a  point  in  s-way  space  Sft,,  s  =  m  +  n. 
If  we  denote  the  first  m  coordinates  by  x1  •••  xm,  and  the  remaining 
coordinates  by  ^  •••  #„,  we  have 


The  points 


*= 


range  over  an  ra-way  space  $Rm,  when  2  ranges  over  9?8.     We  call 
x  the  projection  of  z  on  $TO  . 

Let  z  range  over  a  point  set  51  lying  in  $Ra,  then  x  will  range 
over  a  set  53  in  $m,  called  the  projection  of  51  o?i  9?m.  The  points 
of  51  whose  projection  is  x  is  called  the  section  of  51  corresponding 
to  x.  We  may  denote  it  by 

5l(z),  or  more  shortly  by  (£. 
We  write  «  =  ».<£ 

to  denote  that  51  is  conceived  of  as  formed  of  the  sections  (E,  cor 
responding  to  the  different  points  of  its  projection  53. 

2.  Let  O  denote  a  standard  cube  containing  51,  .let  q  denote  its 
projection  on  Sftm.  Then  53  <.q.  Suppose  each  section  5I(z)  is 
measurable.  It  will  be  convenient  to  let  5l(X)  denote  a  function 
of  x  defined  over  q  such  that 

/«,  /«> 

5l(V)  =  Meas  5l(z)  =  S         when  #  lies  in  53, 

=  0         when  x  lies  in  q  —  53. 

This  function  therefore  is  equal  to  the  measure  of  the  section  of 
51  corresponding  to  the  point  z,  when  such  a  section  exists  ;  and 
when  not,  the  function  =  0. 

When  each  section  5l(#)  is  not  measurable,  we  can  introduce 
the  functions 


*  Dr.  Wilson's  results  were  obtained  in  August,  1909,  and  were  presented  by  me 
in  the  course  of  an  address  which  I  had  the  honor  to  give  at  the  Second  Decennial 
Celebration  of  Clark  University,  September,  1909. 


396  LEBESGUE  INTEGRALS 

Here  the  first  =  (£  when  a  section  exists,  otherwise  it  =  0,  in  q. 
A  similar  definition  holds  for  the  other  function. 

3.    Let  us  note  that  the  sections 


where  He,  2L  are  the  outer  and  inner  associated  sets  belonging  to  31, 
are  always  measurable. 

For  2Ie  =  Dv  \  (£„  \  ,  where  each  G?n  is  a  standard  enclosure,  each 
of  whose  cells  tnm  is  rectangular.  But  the  sections  enm(V)  are 
also  rectangular.  Hence 


being  the  divisor  of  measurable  sets,  is  measurable. 

415.    Let  $te  be  an  outer  associated  set  of  tyt,both  lying  in  the  stand- 

0t 

ard  cube  O.      Then  2le(V)  is  L-integrable  in  q,  and 


=  f  ioo-  a 

«4/ 


For  let  j@nj  be  a  sequence  of  standard  enclosures  of  51,  and 
@n=5enni;.  Then 

£n  =  2enm  (2 

m 

and  «.(*)  =  2e»(*).  (3 

TO 

Now  enm  being  a  standard  cell,  enm(^)  nas  a  constant  value  >  0 
for  all  x  contained  in  the  projection  of  enm  on  q.  It  is  thus  con 
tinuous  in  q  except  for  a  discrete  set.  It  thus  has  an  ^-integral, 
and 


This  in  2)  gives 

enm<»,         by  413,  2, 


f  €,0), 

oLa 


(4 
by  3). 


ITERATED  INTEGRALS  397 

On  the  other  hand,  (S(z)  is  a  measurable  function  by  411.     Also 
1  =  Se  =  lim  <fn 


=  Aim  in(z),         by  413,  1.  (5 

<X 


Thus  this  in  5)  gives  1). 

416.    Let  51  lie  in  the  standard  cube  O.     Let  Hi  50  a/i  inner  asso 
ciated  set.      Then  §t(V)  is  L-integraUe  in  q,  and 


For  0  =  21.  +  A- 

Thus  flCr)  =  SCO  -  A.(x). 

Hence  H^x)  is  i-integrable  in  q,  and 

f*{x)  =  fSO)  -  p.(*) 

oLq  0Lq  —  q 

=  S-A     ,     by  415, 
=  St  =  a         by  370,  2. 

417.    ie£  measurable  21  fo'e  iw  #Ae  standard  cube  O. 


For  a. 

Hence          ^  =   T^^)  <  Tf^)  <  fi/^)  =  f,  (2 

~       <Zq  iq~  «^q 

using  396,  1,  and  415,  416.     From  2)  we  conclude  1)  at  once. 
418.    Let  H  =  $8  •  (S  ^  measurable.     Then  S  are  L-integrable  in 


398  LEBESGUE   INTEGRALS 

For  by  41 7,  ~ 


by  401. 

419.    If  51  =  53  •  (£  is  measurable,  the  points  of  53  at  which  &  is  not 
measurable  form  a  null  set  $1. 

For  by  418,  g=  f  =  =  f 

i  i 

Hence 


=  f  (f-<£). 

<X$ 


Thus 


is  a  null  function  in  53,  and  by  402,  2,  points  where  </>  >  0  form  a 
null  set. 

420.    Let  51  =  53  •  (S  £>e  measurable.     Let  b  denote  the  points  of  53 
/or  which  the  corresponding  sections  (£  are  measurable.     Then 


= 

For  by  419,  53=b  + 

and  9?  is  a  null  set.     Hence  by  418, 


=/s. 

<Xb 


421.    Let  f>0  in  51.     .Zf  £Ae  integrand  set  3s?  corresponding  to  f 
be  measurable,  then  f  is  L-integrable  in  51, 


3-J/ 

For  the  points  of  Q  lying  in  an  m  -f-  1  way  space  9?m+1  may  be 
denoted  by  x  =  (v  •- y    z} 

where  y  =  (yl  -  •  •  ?/m)  ranges  over  9?m,  in  which  51  lies.     Thus  51 
may  be  regarded  as  the  projection  of  Q  on  9?m.     To  each  point  y 


ITERATED   INTEGRALS  399 

of  21  corresponds  a  section  3G/),  which  for  brevity  may  be  denoted 
by  $.     Thus  we  may  write 

$»*-*. 

As  ft  is  nothing  but  an  ordinate  through  y  of  length  /Q/),  we 
have  by  419,  ^  /»= 

§«/I 

at* 

422.  Ze£  /  6e  L-integraUe  over  the  measurable  field  21  =  53  •  (£. 
ie£  b  denote  those  points  of  33,  /or  which  f  is  L-integralle  over  the 
corresponding  sections  (£.  2%era 

f /=///.  a 

^21         otb^S 
Moreover  $ft  =  55  —  b  is  a  null  set. 

Let  us  1°  suppose  f>  0.     Then  by  406,  3  is  measurable  and 

§=r/.  (2 

•£« 

Let  0  denote  the  points  of  23  for  which  3(z)  is  measurable. 
Then  by  420, 

5  =  f§(*).  (3 

Jip 
By  419,  the  points 

^  =  53  -  /3  (4 

form  a  null  set. 

On  the  other  hand,  $(x)  is  the  integrand  set  of/,  for  SI (V)  =  6. 
Hence  by  421,  for  any  z  in  /3, 

,  (5 

and  /3  <  b.  (6 

From  2),  3),  5)  we  have 

w.     Jlp  J*& 

From  6)  we  have 

^=33-b<23-/3  =  ^, 

a  null  set  by  4).     Let  us  set 

b  =  J3  +  n. 


400  LEBESGUE   INTEGRALS 

Then  tt  lying  in  the  null  set  $,  is  a  null  set.     Hence 

JLp  JL&   JLn  JL(s,   JL\)  cXg 

This  with  7)  gives  1). 

Let  f  be  now  unrestricted   as  to  sign.     We  take   0  >  0,  such 
that  the  auxiliary  function 

ff=f+C>0,        in  St. 

Then  /,  g  are  simultaneously  Z-integrable  over  any  section  (£. 
Thus  by  case  1° 

f  (/+<?)=  c  fcf+o).          (8 

e£/2l  oC'b  ^S 

Now  r  /»/»./»- 

(9 
(10 

By  418,  (£  is  Z-integrable  in  ^3,  and  hence  in  b.     Thus 
/*    /*  /»    /»  /»= 

Li^f+c^=Llf+0l^"        (11 

As  b  differs  from  33  by  a  null  set, 

ri=ri=s,  (12 

by  418.     From  8),  9),  10),  11),  12)  we  have  1). 

423.    If  f  is  L-integrable  over  the  measurable  set  51  =  53  •  (£,  £Aew 

/*  /*     /T 

J /=///.  a 

Xx      «X^3  oC$ 

For  by  422, 

/»       /»    /» 

(2 


As  ^3  —  b  =  yt  is  a  null  set, 

"/=o 


ITERATED   INTEGRALS  401 

may  be  added  to  the  right  side  of  2)  without  altering  its  value. 
Thus 


JLn     JLbJ&     °LftcL(§.     JLsQcLd 


424.  1.  (TF.  A.  Wilson.)  If  f  (^  •  -  -  xm~)  is  L-integrable  in 
measurable  21,  f  is  measurable  in  21. 

Let  us  first  suppose  that/>  0.  We  begin  by  showing  that  the 
set  of  points  21A  of  21  at  which  /  >  X,  is  measurable.  Then  by 
408,  3,  /is  measurable  in  21. 

Now  /  being  Z-integrable  in  21,  its  integrand  set  3>  is  measur 
able  by  406.  Let  QA  be  the  section  of  3  corresponding  to  xm+l=  \. 
Then  the  projection  of  3A  on  3tm  is  21A.  Since  3  is  measurable,  the 
sections  3?A  are  measurable,  except  at  most  over  a  null  set  L  of 
values  of  X,  by  419.  Thus  there  exists  a  sequence 

Xj  <  \2<  ...  =X 

none  of  whose  terms  lies  in  L.     Hence  each  3xM  is  measurable,  and 
hence  2lAjt  is  also. 

As  2lAn+1  <  2lAn,  each  point  of  21A  lies  in 


so  that  '   «A<5>.  (2 

On  the  other  hand,  each  point  d  of  3)  lies  in  21A.     For  if  not, 
f(d)<\. 

There  thus  exists  an  s  such  that 


<  X.  <  X.  (3 

But  then  d  does  not  lie  in  2IA,,  for  otherwise  f  (d)  >  X,,  which 
contradicts  3).  But  not  lying  in  2IA,,  d  cannot  lie  in  £),  and  this 
contradicts  our  hypothesis.  Thus 

£)<21A.  (4 

From  2),  4)  we  have 

$«*A< 

But  then  from  1),  21A  is  measurable. 
Let  the  sign  off  be  now  unrestricted. 


402  IMPROPER   L-INTEGRALS 

Since  f  is  limited,  we  may  choose  the  constant  C,  such  that 


Then  g  is  Z-integrable,  and  hence,  by  case  1°,  g  is  measurable. 
Hence/,  differing  only  by  a  constant  from  g,  is  also  measurable. 

2.  Let  51  be  measurable.     Iff  *'*  L-integrable  in  51,  i£  i*  measur 
able  in  51,  a/ic?  conversely. 

This  follows  from  1  and  409,  l. 

3.  From  2  and  409,  3,  we  have  at  once  the  theorem  : 

When  the  field  of  integration  is  measurable,  an  L-integrable  func 
tion  is  integrable  in  Lebesgue's  sense,  and  conversely;  moreover,  both 
have  the  same  value. 

Remark.  In  the  theory  which  has  been  developed  in  the  fore 
going  pages,  the  reader  will  note  that  neither  the  field  of  integra 
tion  nor  the  integrand  needs  to  be  measurable.  This  is  not  so  in 
Lebesgue's  theory.  In  removing  this  restriction,  we  have  been 
able  to  develop  a  theory  entirely  analogous  to  Riemann's  theory  of 
integration,  and  to  extend  this  to  a  theory  of  upper  and  lower  in 
tegration.  We  have  thus  a  perfect  counterpart  of  the  theory 
developed  in  Chapter  XIII  of  vol.  I. 

4.  Let  51  be  metric  or  complete.     If  f  \xl  •••  xni)  is  limited  and 
R-integrable,  it  is  a  measurable  function  in  51. 

For  by  381,  2,  it  is  .L-integrable.  Also  since  51  is  metric  or 
complete,  51  is  measurable.  We  now  apply  1. 


IMPROPER  L-INTEGRALS 

Upper  and  Lower  Integrals 

425.  1.  We  propose  now  to  consider  the  case  that  the  integrand 
/(#!•••  #w)  is  not  limited  in  the  limited  field  of  integration  51-  In 
chapter  II  we  have  treated  this  case  for  ^-integrals.  To  extend 
the  definitions  and  theorems  there  given  to  X-integrals,  we  have 
in  general  only  to  replace  metric  or  complete  sets  by  measurable 
sets;  discrete  sets  by  null  sets;  unmixed  sets  by  separated  sets; 


UPPER   AND   LOWER   INTEGRALS  403 

finite  divisions  by  separated  divisions  ;  sequences  of  superposed 
cubical  divisions  by  extremal  sequences;  etc. 

As  in  28  we  may  define  an  improper  .//-integral  in  any  of  the 
three  ways  there  given,  making  such  changes  as  just  indicated. 
In  the  following  we  shall  employ  only  the  3°  Type  of  definition. 
To  be  explicit  we  define  as  follows  : 

Let/  (2^  ...  xm)  be  defined  for  each  point  of  the  limited  set  51. 
Let  5la/3  denote  the  points  of  21  at  which 


The  limits 


„  /- 

lim    /   /    ,     lim    /  /  (2 

a,  0=*  cL^p  a,  0=  *  o^SJa/S 


in  case  they  exist,  we  call  the  lower  and  upper  (improper)  L-in- 
tegrals,  and  denote  them  by 


In  case  the  two  limits  2)  exist  and  are  equal,  we  denote  their 
common  value  by 


and  say/  is  (improperly)  L-integrable  in  51,  etc. 

2.  In  order  to  use  the  demonstrations  of  Chapter  II  without  too 
much  trouble,  we  introduce  the  term  separated  function.  A  func 
tion  /  is  such  a  function  when  the  fields  5la0  defined  by  1)  are 
separated  parts  of  51. 

We  have  defined  measurable  functions  in  407  in  the  case  that 
/  is  limited  in  51.  We  may  extend  it  to  unlimited  functions  by 
requiring  that  the  fields  5ltt/3  are  measurable  however  large  a,  ft  are 
taken. 

This  being  so,  we  see  that  measurable  functions  are  special  cases 
of  separated  functions. 

In  case  the  field  51  of  integration  is  measurable,  5la0  is  a  meas 
urable  part  of  51,  if  it  is  a  separated  part.  From  this  follows  the 
important  result  : 

Iff  is  a  separated  function  in  the  measurable  field  51,  it  is  L-in 
tegrable  in  each  5la/3. 


404  IMPROPER  L-INTEGRALS 

From  this  follows  also  the  theorem: 

Letf  be  a  separated  function  in  the  measurable  field  51.  If  either 
the  lower  or  upper  integral  off  over  51  is  convergent,  f  is  L-integrable 

in  51,  and  /»  /» 

/  /=   lim    /  /. 

JLK  «,  0-=°^2la/3 

426.  To  illustrate  how  the  theorems  on  improper  .72-integrals 
give  rise  to  analogous  theorems  on  improper  .//-integrals,  which 
may  be  demonstrated  along  the  same  lines  as  used  in  Chapter  II, 
let  us  consider  the  analogue  of  38,  2,  viz. : 

£7* 
f  converges,  so  do   I   f. 
cly 

Let  \En\  be  an  extremal  sequence  common  to  both 
f      ,      r  /3'>/3- 

<^2la/3'  ^2la/3 

Let  e  denote  the  cells  of  En  containing  a  point  of  ^ ;  e*  those 
cells  containing  a  point  of  typ ;  8  those  cells  containing  a  point  of 
5Iaj3  but  none  of  ^-.  Then 


L 


=  lim  {2JC  •  e  +  1MI  •  e' 


In  this  manner  we  may  continue  using  the  proof  of  38,  and  so 
establish  our  theorem. 

427.    As  another  illustration  let  us  prove  the  theorem  analogous 
to  46,  viz.  : 

Let  Sfj,  512,  •••  5ln  form  a  separated  division  of  5(.     If  f  is  a 
separated  function  m  51,  then 


//=//+-+//, 

4^21         4/2li  <?k2l» 


provided  the  integral  on  the  left  exists,  or  all  the  integrals  on  the 
right  exist. 

For  let  51,,  aft  denote  the  points  of  5lap  in  51,.     Then  by  390,  l, 


,a/3  oSLn,  aft 

In  this  way  we  continue  with  the  reasoning  of  46. 


L-INTEGRALS  405 

428.  In  this  way  we  can  proceed  with  the  other  theorems  ;  in 
each  case  the  requisite  modification  is  quite  obvious,  by  a  con 
sideration  of  the  demonstration  of  the  corresponding  theorem  in 
.R-integrals  given  in  Chapter  II. 

This  is  also  true  when  we  come  to  treat  of  iterated  integrals 
along  the  lines  of  70-78.  We  have  seen,  in  425,  2,  that  if  31  is 
measurable,  upper  and  lower  integrals  of  separated  functions  do 
not  exist  as  such  ;  they  reduce  to  .//-integrals.  We  may  still 
have  a  theory  analogous  to  iterated  72-integrals,  by  extending  the 
notion  of  iterable  fields,  using  the  notion  of  upper  measure.  To 
this  end  we  define  : 

A  limited  point  set  at  31  =  33  •  (£  is  submeasurable  with  respect 
to  33,  when 

1=  f  I. 


f 


We  do  not  care  to  urge  this  point  at  present,  but  prefer  to  pass 
on  at  once  to  the  much  more  interesting  case  of  ^-integrals  over 
measurable  fields. 

Lrlntegrals 

429.    These  we  may  define  for  our  purpose  as  follows  : 
Let/(a:1  •••  xm)  be  defined  over  the  limited  measurable  set  31. 
As  usual  let  3L0  denote  the  points  of  31  at  which 

-«</<&          «,  £>0. 

Let  each  3la/3  be  measurable,  and  let  /  have  a  proper  Z-integral 
in  each  3L0-  Then  the  improper  integral  of  f  over  31  is 

f/  =   Km    C  f,  (1 

Ji%          «.0=*<X2U/3 

when  this  limit  exists.     We  shall  also  say  that  the  integral  on 
the  left  of  1)  is  convergent. 

On  this  hypothesis,  the  reader  will  note  at  once  that  the  dem 
onstrations  of  Chapter  II  admit  ready  adaptation  ;  in  fact  some 
of  the  theorems  require  no  demonstration,  as  they  follow  easily 
from  results  already  obtained. 


406  IMPROPER  L-INTEGRALS^ 

430.    Let  us  group  together  for  reference  the  following  theo 
rems,  analogous  to  those  on  improper  .R-integrals. 

1.  Iff  is  (improperly')  L-integrable  in  H,  it  is  in  any  measurable 
part  of  21. 

2.  If  g,  h  denote  as  usual  the  non-negative  functions  associated 
withf,  then 


3.  If  I   f  is  convergent,  so  is   I    \f\,  and  conversely. 

eW$l  o*^2l 

4.  When  convergent, 

Lf^Lf-  (2 

5.  If  I    f  is  convergent,  then 

e  >  0,         <r  >  0, 


for  any  measurable  53  <  51,  such  that  $8  <  cr. 

6.  Let  $[  =  ($(!,  H2  •••  5In)  be  a  separated  division  of  21,  each  5lt 
being  measurable.     Then 

f/=  r /+-  +  r/,  (3 

alf[  JL*l  JL%n 

provided  the  integral  on  the  left  exists,  or  all  the  integrals  on  the 
right  exist. 

7.  Let  51  =  \tyin\  be  a  separated  division  of  51,  into  an  enumerable 
infinite  set  of  measurable  sets  5ln.      Then 

-  (4 

212 
provided  the  integral  on  the  left  exists. 

8.  Iff<9  in  ^  except  possibly  at  a  null  set,  then 

ff<  Cff,  (5 

,,    .,  ^51          ei* 

when  convergent. 


L-INTEGRALS  407 

431.  1.  To  show  how  simple  the  proofs  run  in  the  present 
case,  let  us  consider,  in  the  first  place,  the  theorem  analogous  to 
38,  2,  viz.  : 


If  I   f  converges,  so  do   I   f  and   I  f. 

JLyi  J*  JLm 


The  rather  difficult  proof  of  38,  2  can  be  replaced  by  the  follow 
ing  simpler  one.     Since 


is  a  separated  division  of  2la/s>  we  have 

/=/+/• 

<**<#    JL        JL^ 


Hence 


\f  L  =\f-f 

\£%ap         aU^r  \^        «tf^ 


But  the  left  side  is  <  e,  for  a  sufficiently  large  a,  and  /3,  /?'  > 

some  y£0.     This  shows  that   /    is  convergent.     Similarly  we  show 

^ 

the  other  integral  converges. 

2.  This  form  of  proof  could  not  be  used  in  38,  2,  since  1)  in 
general  is  not  an  unmixed  division  of  2fa/3. 

3.  In  a  similar  manner  we  may  establish  the  theorem  analo 
gous  to  39,  viz.  : 


If  i    f  and   I  f  converge,  so  does   I  f. 

Jiy          JL&  JL* 


4.    Let  us  look  at  the  demonstration  of  the  theorem  analogous 
to  43,  1,  viz.  : 


provided  the  integral  on  either  side  of  these  equations  converges. 


408  IMPROPER  L-INTEGRALS 

Let  us  prove  the  first  relation.     Let  53^  denote  the  points  of 
at  which  f</3.     Then 

8*  «'R  +  ft 

is  a  separated  division  of  $8^,  and  hence 


=   Cf,     etc. 

cL 


5.  It  is  now  obvious  that  the  analogue  of  44,  l  is  the  relation  1) 
in  430. 

6.  The  analogue  of  46  is  the  relation  3)  in  430.     Its  demon 
stration  is  precisely  similar  to  that  in  46. 

7.  We  now  establish  430,  7.     Let 

Q>(ftt!fc»<lri>. 

Then  2t  =  $m  +  ^m 

is  a  separated  division  of  21,  and  we  may  take  m  so  large  that 
Bm  <  <r,  an  arbitrarily  small  positive  number.  Hence  by  430,  5, 
we  may  take  m  so  large  that 


f 


J»Bm 

f/=//+/ 

«t2l         J*%m        J*B 

r* 


<  €. 


From  this  our  theorem  follows  at  once. 

Iterated  Integrals 

432.  1.  Let  us  see  how  the  reasoning  of  Chapter  II  may  be 
extended  to  this  case.  We  will  of  coarse  suppose  that  the  field 
of  integration  51  =  93  •  &  is  measurable.  Then  by  419,  the  points 
of  58  for  which  the  sections  are  not  measurable  form  a  null  set. 
Since  the  integral  of  any  function  over  a  null  set  is  zero,  we  may 
therefore  in  our  reasoning  suppose  that  every  (£  is  measurable. 

Since  21  is  measurable,  there  exists  a  sequence  of  complete  com 
ponents  Am=  BmOm  in  H,  such  that  the  measure  of  A  =  \Am\  is  S. 


ITERATED   INTEGRALS  409 

Since  An  is  complete,  its  projection  Bn  is  complete,  by  I,  717,  4. 
The  points  of  Bm  for  which  the  corresponding  sections  Om  are  not 
measurable  form  a  null  set  vm.  Hence  the  union  \vm\  is  a  null 
set.  Thus  we  may  suppose,  without  loss  of  generality  in  our 
demonstrations,  that  21  is  such  that  every  section  in  each  Am  is 
measurable. 
Now  from 


we  see  that  those  points  of  53  where  (£  >  C  form  a  null  set.  We 
may  therefore  suppose  that  (£  =  0  everywhere.  Then  (£  —  C  is  a 
null  set  at  each  point  ;  we  may  thus  adjoin  them  to  C.  Thus  we 
may  suppose  that  &  =  C  at  each  point  of  53,  and  that  53  =  B  is  the 
union  of  an  enumerable  set  of  complete  sets  Bm. 

As  we  shall  suppose  that 

/» 


is  convergent,  let 

«!  <  «2  <  •  •  •  =  oo  , 


=  00. 


Let  us  look  at  the  sets  5lan,  53^,  which  we  shall  denote  by  2In. 
These  are  measurable  by  429.  Moreover,  the  reasoning  of  72,  2 
shows  that  without  loss  of  generality  we  may  suppose  that  21  is 
such  that  53n  =  53.  We  may  also  suppose  that  each  (£„  is  measur 
able,  as  above. 

2.    Let  us  finally  consider  the  integrals 

'/•  (i 


These  may  not  exist  at  every  point  of  53,  because  /  does  not 
admit  a  proper  or  an  improper  integral  at  this  point.  It  will 
suffice  for  our  purpose  to  suppose  that  1)  does  not  exist  at  a  null 
set  in  53.  Then  without  loss  of  generality  we  may  suppose  in  our 
demonstrations  that  1)  converges  at  each  point  of  53. 

On  these  assumptions  let  us  see  how  the  theorems  73,  74,  75, 
and  76  are  to  be  modified,  in  order  that  the  proofs  there  given 
may  be  adapted  to  the  present  case. 


410  IMPROPER  L-INTEGRALS 

433.    1     The  first  of  these  may  be  replaced  by  this  : 
Let  B^  n  denote  the  points  of  $8  at  which  Tn  >  a.      Then 


21=         , 


For  by  419, 


as  by  hypothesis  the  sections  (£  are  measurable.     Moreover,  by 
hypothesis 

is  a  separated  division  of  (£,  each  set  on  the  right  being  measur 
able.     Thus  the  proof  in  73  applies  at  once. 

2.    The  theorem  of  74  becomes  : 

Let  the  integrals 

,    />0 

be  limited  in  the  complete  set  53.     Let  (gn  denote  the  points  of  53  at 
which 


Then 

HmS^B. 

n=ao 

The  proof  is  analogous  to  that  in  74.  Instead  of  a  cubical 
division  of  the  space  9?p,  we  use  a  standard  enclosure.  The  sets 
33n  are  now  measurable,  and  thus 


is  measurable.     Thus  bn  =  IT.     The  rest  of  the  proof  is  as  in  74. 

3.    The  theorem  of  75  becomes  : 

Let  the  integral  ^ 

f    ,    />0 

XG 

be  limited  in  complete  53.      Then 

lim  T    //=0. 


n= 


ITERATED   INTEGRALS  411 

The  proof  is  entirely  similar  to  that  in  75,  except  that  we  use 
extremal  sequences,  instead  of  cubical  divisions. 

4.    As  a  corollary  of  3  we  have 
Let  the  integral 


be  limited  and  L-integrable  in  53.     Let  ^3  =  \Sm\  the  union  of  an 
enumerable  set  of  complete  sets.      Then 

lira  f    f/=0. 

•"•JUftatc. 

For  if  53m  =  (#!,  £2  ...  Bm),  and  %  =  53m  4-  £)„,  we  have 


/ 

But  for  w  sufficiently  large,  £)m  is  small  at  pleasure.     Hence 


We  have  now  only  to  apply  3. 

434.    1.    We   are   now  in   position  to   prove  the  analogue  of 
76,  viz.  : 

Let  51  =  53  •  (£  be  measurable.     Let   I   f  be  convergent.     Let  the 

/»  0^21 

integrals    I  f  converge  in  53,  except  possibly  at  a  null  set.      Then 

JL* 

ff=f!f>  (1 

«C21         vL$&°L($ 
provided  the  integral  on  the  right  is  convergent. 

We  follow  along  the  line  of  proof  in  76,  and  begin  by  taking 
/  >  0  in  a.     By  423,  we  have 

•  •  U-LU-- 

hence  ,,  ,,     ,, 

/=limj      if.  (2 

I          n=QOoL33  =£(£„ 


412  IMPROPER  L-INTEGRALS 

Now  e  >  0  being  small  at  pleasure, 

-e+f    (/<f      Cf    ,     for  a  >  some 
<£%  aid       aL^G  JL*i 


Since  we  have  seen  that  we  may  regard  33  as  the  union  of  an 
enumerable  set  of  complete  sets,  we  see  that  the  last  term  on  the 
right  =  0,  as  n  =  oo,  by  433,  4.  Thus 

c  r  <iim  c  r  =  r,  (3 

JL<$>  0&C  JL^&  JL&n    JUK 

by  2).     On  the  other  hand, 


From  3)  and  4)  we  have  1),  when/>  0. 
The  general  case  is  now  obviously  true.     For 

where  f>  0  in  ^P,  and  <  0  in  ft.  Here  ^  and  ft  are  measurable. 
We  have  therefore  only  to  use  1)  for  each  of  these  fields  and  add 
the  results. 

2.    The  theorem  1  states  that  if 

1  /*     /* 

/  ,   /  If, 


loth  converge,  they  are  equal.  Hobson*  in  a  remarkable  paper  on 
Lebesgue  Integrals  has  shown  that  it  is  only  necessary  to  assume 
the  convergence  of  the  first  integral ;  the  convergence  of  the  second 
follows  then  as  a  necessary  consequence. 

*  Proceedings  of  the  London  Mathematical   Society,    Ser.    2,   vol.   8    (1909), 
p.  31. 


ITERATED  INTEGRALS  413 

435.  We  close  this  chapter  by  proving  a  theorem  due  to 
Lebesgue,  which  is  of  fundamental  importance  in  the  theory  of 
Fourier's  Series. 

Letf(x)  be  properly  or  improperly  L-integrable  in  the  interval 
2l  =  a<5.  Then 


im  r\ 

=0  JLa 


For  in  the  first  place, 

*)l«fc+  r\f\dx<^r\f\dx.      (2 

JLa  JLa 

Next  we  note  that 


Hence 


Or  f—g<f-g' 

From  2),  3)  we  have 

J,<J.  +  2£\f-g\d*.  (4 

Let  now  ^=/        fo"r  |/|  <  (?, 

=  0         for  |/|  >#. 
Then  by  4),  r 


where  e'  is  small  at  pleasure,  for  Cr  sufficiently  large.     Thus  the 
theorem    is   established,  if   we   prove  it  for   a   limited  function, 

\g(*)\<&. 

Let  us  therefore  effect  a  division  of  the  interval  F  =  (—  6r,  6r), 
of  norm  d,  by  interpolating  the  points 

-  a<  cl<  cz<  ...  <a, 

causing  F  to  fall  into  the  intervals 

7i<  72'  7s  ••' 


414  IMPROPER  L-INTEGRALS 

Let  hm  =  cm  for  those  values  of  x  for  which  g(x)  falls  in  the  in 
terval  7m,  and  =  0  elsewhere  in  21.     Then 


<  2  J^t  +  e',         e'  small  at  pleasure, 
for  d  sufficiently  small. 

Thus  we  have  reduced  the  demonstration  of  our  theorem  to  a 
function  h(x)  which  takes  on  but  two  values  in  21,  say  0  and  7. 

Let  (£  be  a  <r/4  enclosure  of  the  points  where  h  =  7,  while  g  may 
denote  a  finite  number  of  intervals  of  (§  such  that  g  —  ($  <  o-/4. 

Let  <£  =  7  in  (§:,  and  elsewhere  =  0  ;  let  i/r  =  7  in  g,  and  else 
where  =  0.  Thus  using  4), 


since  h=</)in  (a,  /3),  except  at  points  of  measure  <  <r/4.     Similarly 

^  <  J^  rf  I  7. 

Thus  Jh  <  J^  +  0-7  <  J^  +  e, 

for  <r  sufficiently  small. 

Thus  the  demonstration  is  reduced  to  proving  it  for  a  i/r  which 
is  continuous,  except  at  a  finite  number  of  points.  But  for  such  a 
function,  it  is  obviously  true. 


CHAPTER   XIII 

FOURIER'S   SERIES 

Preliminary  Remarks 

436.    1.    Let  us  suppose  that  the  limited  function  f(x)  can  be 
developed  into  a  series  of  the  type 

f(x)  =  a0  +  #!  cos  x  4-  02  cos  2  x  4-  03  cos  3  #  -f-  ••• 

4-  bl  sin  a:  4-  62  sin  2  z  +  Z>3  sin  3  x  4-  •••  (1 

which  is  valid  in  the  interval  51  =  (—  TT,  TT).  If  it  is  also  known 
that  this  series  can  be  integrated  termwise,  the  coefficients  an,  bn 
can  be  found  at  once  as  follows.  By  hypothesis 


cos 


r  fdx=a,Tdx+al  r 

JL-K  JL-*  JL-* 

sin  xdx  4-  •  •  • 

r 

As  the  terms  on  the  right  all  vanish  except  the  first,  we  have 


I 


Let  us  now  multiply  1)  by  cos  nx  and  integrate. 
I     /(V)  cos  nxdx  =  «0  /     cos  rz^Ja;  +  al  I     cos  ^  cos  nxdx  4- 

/^ff 
4- ^!  i      si n  2;  cos  wa;4-  ••• 

/     cos  ma:  cos  nxdx  =0     ,     m=£n, 


r. 

£- 


cos2  nzcfo  = 


sin  mx  cosna:=0. 
415 


416  FOURIER'S   SERIES 

Thus  all  the  terms  on  the  right  of  the  last  series  vanish  except 
the  one  containing  an.     Hence 


a   —  - 


/(V)cos  nxdx.  (2 


Finally  multiplying  1)   by  sin  712:,  integrating,  and  using  the 

relations  „* 

i     sin  mx  sin  nxdx  =  0     ,     m^n, 


fsi: 
•7T 


sin2  nxdx  —  TT, 

fJU— 

we  get 


bn  =  -  T  V  (a;)  sin  nxdx.  (2 

TToC'-TT 

Thus  under  our  present  hypothesis, 

1     /*"•  1  «  /*"' 

/W  =  o~  l     f  (u)du  +  —  -%  cos  nx   I     f(u)  cc 

^^JL-rr  TT    1  ^-'r 


'" 


1    oo 

H —  2  sin 

7T    l 


f» 
/ » V*         N.  *  T  /"  Q 

/^    ^ 


The  series  on  the  right  is  known  as  Fourier's  series  ;  the  coeffi 
cients  2)  are  called  Fourier's  coefficients  or  constants.  When  the 
relation  3)  holds  for  a  set  of  points  33,  we  say/(#)  can  be  de 
veloped  in  a  Fourier's  series  in  33,  or  Fourier's  development  is  valid 
in  $. 

2.  Fourier  thought  that  every  continuous  function  in  51  could 
be  developed  into  a  trigonometric  series  of  the  type  3).  The 
demonstration  he  gave  is  not  rigorous.  Later  Dirichlet  showed 
that  such  a  development  is  possible,  provided  the  continuous 
function  has  only  a  finite  number  of  oscillations  in  51.  The  func 
tion  still  regarded  as  limited  may  also  have  a  finite  number  of 
discontinuities  of  the  first  kind,  i.e.  where 

/(a+O)     ,    /(a-0)  (4 

exist,  but  one  at  least  is  =£/(#). 

At  such  a  point  a,  Fourier's  series  converges  to 


PRELIMINARY  REMARKS  417 

Jordan  has  extended  Dirichlet's  results  to  functions  having 
limited  variation  in  51.  Thus  Fourier's  development  is  valid  in 
certain  cases  when  /  has  an  infinite  number  of  oscillations  or 
points  of  discontinuity.  Fourier's  development  is  also  valid  in 
certain  cases  when/  is  not  limited  in  51,  as  we  shall  see  in  the 
following  sections. 

We  have  supposed  that  /(#)  is  given  in  the  interval 
31  =  ( —  TT,  TT).  This  restriction  was  made  only  for  convenience. 
For  if/(V)  is  given  in  the  interval  3  =  (a  <  b),  we  have  only  to 
change  the  variable  by  means  of  the  relation 


b-a 

Then  when  x  ranges  over  3k  u  will  range  over  H. 
Suppose  f  is  an  even  function  in  51;  its  development  in  Fourier's 
series  will  contain  only  cosine  terms.     For 

00 

f(x)  —  2(an  cos  nx  +  bn  sin  nx), 

o 

GO 

/(—  x)  =  2(an  cos  nx—  bn  sin  nx). 

o 

Adding  and  remembering  that  f(x)  =/(  —  x)  in  51,  we  get 

GO 

f(x)  =  J2#n  cos  nx,        f  even. 

"  o 

Similarly  if  f  is  odd,  its  development  in  Fourier's  series"  will 
contain  only  sine  terms ; 

po 

f(x)  =  -J-S5n  sin  nx,        f  odd. 

"  i 

Let  us  note  that  if  f(x)  is  given  only  in  53  =  (0,  TT),  and  has 
limited  variation  in  53,  we  may  develop  /  either  as  a  sine  or  a 
cosine  series  in  53.  For  let 

g(.x)=f(x)     »     a:  in  93 

Then  g  is  an  even  function  in  51  and  has  limited  variation. 
Using  Jordan's  result,  we  see  g  can  be  developed  in  a  cosine 
series  valid  in  51.  Hence  /  can  be  developed  in  a  cosine  series 
valid  in  53. 


418  FOURIER'S   SERIES 

In  a  similar  manner,  let 

h(x)=f(x)     ,     x  in  $ 


Then  h  is  an  odd  function  in  21,  and  Fourier's  development 
contains  only  sine  terms. 

Unless  /(0)=  0,  the  Fourier  series  will  not  converge  to  /(O) 
but  to  0,  on  account  of  the  discontinuity  at  x  =  0.  The  same  is 
true  for  x  =  TT. 

If  /can  be  developed  in  Fourier's  series  valid  in  5l  =  (—  ?r,  TT), 
the  series  8)  will  converge  for  all  #,  since  its  terms  admit  the 
period  2  TT.  Thus  3)  will  represent  f(x)  in  H,  but  will  not 
represent  it  unless  f  also  admits  the  period  2  TT.  The  series  3) 
defines  a  periodic  function  admitting  2  TT  as  a  period. 

EXAMPLES 

437.  We  give  now  some  examples.  They  may  be  verified  by 
the  reader  under  the  assumption  made  in  436.  Their  justifica 
tion  will  be  given  later 

Example  1.  f(x)~x     ,     for  —7r<x<7r. 

Then 


I  sin  x      sin  2  x      sin  3  x          \ 
t     1          ~2~        ~^~       "J 


If  we  set  x  =  —  ,  we  get  Leibnitz  s  formula, 


_        _ 

4      1      35      7 
Example  2.  f(x)—x     ,     0<z<?r 

=   -X       ,         -7T<Z<0. 

Then 

*  s  -       TT      4  f  cos  x      cos  3  rr      cos  5  a; 


If  we  set  x  =  0,  we  get 

8      1*     8*     5* 


PRELIMINARY   REMARKS  419 

Example  3.  f  (V)  =  1  •    • ,     0  <  x  <  TT 

=  0     ,     x  =  0,  ±  TT 

=    -1        ,         -7T<Z<0. 

Then 

/.  ,  N  _  4  f  sin  a;  ,  sin  3  a:      sin  5  a;  1 

/  \x)  —  —  I  ~~q I        5        I         r        r  " '  f* 

7T   I       1  3  O  J 

Example  4.  f  (x)  =  x     ,     0  <  a;  <  ^ 


=  7T  —  X 


By  defining /as  an  odd  function,  it  can  be  developed  in  a  sine 
series,  valid  in  (0,  TT).      We  find 

/Y  N_4  fsin  a:      sin  3 x      sin  5 x _       1  .  ;r 

Examples.  /(^)  =  1     ,     0  .<#'<.--- 

=  -1     ,     !<*<7r. 

By  defining  /  as  an  even  function,  we  get  a  development   in 

cosines, 

/, .  ^  _  4  f  cos  x      cos  3  a:      cos  5  x  _ 


W  iw  (0,  TT). 
Example  6.  /(«)  =  K71"  ~  *)     '     O<Z<TT. 

By  defining  /  as  an  odd  function   we   get   a    development   in 
sines, 

/  (x)  =  sin  #  +  J  sin  2  #  +  J  sin  3  a;  -f  •  •  • 


zc?  in  (—  TT,  TT). 


>  s"!  i 
A.         v 


Example  7.  Let  f(x)  =  -     ,     0  <  a:  <  ^ -•;  . 

3  3 


2Z  ^)\ 

3 


^  2?r 

3     '      3 


420  FOURIER'S   SERIES 

Developing/ as  a  sine  series,  we  get 


valid  in  (0,  TT). 

Example  8.  /CO  =  e*     »     in  (—  TT,  TT), 

We  find 


valid  for  —  TT  <  x  <  TT. 

Example  9.    We  find 

2  /i    .  f    1          cos  :r       cos  2  a:      cos  3  x    ,         ] 

cos  /iz  =  -  £  sin  7r/i     —  -  -  —  —  -  +  —  —  —  --  -  -  -  +  ... 
TT  1  2  /A2     /i2  —  1      /A2  —  22     /i2  —  3a  J 


Let  us  set  x  =  TT,  and  replace  /*  by  a;  ;  we  get 

1  |  1  | 

o     "^      o  10    "^      o          OQ    ' 


s  „          -i  o  o  10    "        o          OQ 

2a;  2^      ir2—  I2      r*  —  22     ar2  —  32 

a  decomposition  of  cot  irx  into  partial  fractions,  a  result  already 
found  in  216. 

Example  10.    We  find 

2  2  cos  2  ^     2  cos  4  #      2  cos  6  a; 


valid  for  Q  <  x  <TT. 

Summation  of  Fourier's  Series 

438.  In  order  to  justify  the  development  of  f(x)  in  Fourier's 
series  F,  we  will  actually  sum  the  F  series  and  show  that  it  con 
verges  to  /(of)  in  certain  cases.  To  this  end  let  us  suppose  that 
f(x)  is  given  in  the  interval  5l  =  (—  TT,  TT),  and  let  us  extend/  by 
giving  it  the  period  2  TT.  Moreover,  at  the  points  of  discontinuity 
of  the  first  kind,  let  us  suppose 


SUMMATION   OF   FOURIER'S   SERIES  4'2\ 

Then  the  function 

<K«)  =  /O  +  2  u)  4- /Or  -  2  *)  -  2/(*) 

is  continuous  at  u  =  0,  and  has  the  value  0,  at  points  of  continuity, 
and  at  points  of  discontinuity  of  1°  kind  of/.  Finally  let  us  sup 
pose  that  /  is  (properly  or  improperly)  Z-integrable  in  21  ;  this 
last  condition  being  necessary,  in  order  to  make  the  Fourier  co 
efficients  aB,  bn  have  a  sense. 

Let 

F=F(x)  =  \  004-  aa  cos  x  4-  03  cos  2  x  4-  — 

+  ^sin  .r  +  52sin  2  2-  4-  •••  (1 

X 

=  \  a0  4-  2(am.cos  war  +  6m  sin  na:), 
where  we  will  now  write 

1  /***•» 
««  =  -  /    /O)eosw2*Za?,  (2' 

£w  =  ^  r'/C^)  sin  «w^-  (2; ' 

Since /(z)  is  periodic,  the  coefficients  an,  5m  have  the  same  value 
however  c  is  chosen.  If  we  make  c  =  —  TT,  these  integrals  reduce 
to  those  given  in  436. 

We  may  write 

F=  —  I    f  (f)tfr  \  I  +  2(cos  nx  cos  nt  -h  sin  nx  sin  nt)  \ 

2  COS  »(«  -  2")  \f  (t)dt.  (3 


Thus                F  _i/v.f(0(ft 

where        p.-i~*&»m(t-z). 

c-t 

1 

Provided                           .     , 
sin  J(f  —  2-)  =£0, 

(5 

we  may  write 

L-  sin  2  C  ^  —  "^)                             ^ 

-f  2  I  sin  ^-^ (f  —  2-)  —  sin  ^^ (f  —  a:)  J  L 


422  FOURIER'S   SERIES 

ThUS 


sn  -  ,fi 


if  5)  holds.  Let  us  see  what  happens  when  5)  does  not  hold. 
In  this  case  %(t  —  x)  is  a  multiple  of  TT.  As  both  £  and  x  lie  in 
(<?,  c  +  2  TT),  this  is  only  possible  for  three  singular  values  : 

t  =  x     ;     t  =  c,     x  =  c  -f-  2  TT     ;     £  =  c  +  2  TT,     a;  =  c. 
For  these  singular  values  4)  gives 


n 


As  Pn  is  a  continuous  function  of  £,  #,  the  expression  on  the 
right  of  6)  must  converge  to  the  value  7)  as  #,  t  converge  to  these 
singular  values.  We  will  therefore  assign  to  the  expression  on 
the  right  of  6)  the  value  7),  for  the  above  singular  values.  Then 

in  all  cases 

1  p*glPy2n  +  lXt-aO  /(Q(ft. 

irJic  2  sin  ^(t  —  x) 

Let  us  set  2     -I-  1  —  t  —     — 

Then 

Fn^-\  f(x  +  2uY-^^du. 


sin 

Let  us  choose  c  so  that 

c  —  x  =  —  TT, 

then  ~f 

<X_JT  J,_7T 

2  2 

Replacing  w  by  —  u  in  the  first  integral  on  the  right,  it  becomes 

-,        o    ^  sin  vu  -, 

f(x  —  2  u) du. 

„ .  "  sin  u 

Thus  we  get 

7T 

TT^io  gin  W 

Let  us  now  introduce  the  term  —  2/(z)  under  the  sign  of  inte 
gration  in  order  to  replace  the  brace  by  <£(w).     To  this  end  let  us 


SUMMATION  OF   FOURIER'S   SERIES  423 

give  x  an  arbitrary  but  fixed  value  and  consider  the  Fourier's 
series  for  the  function 


f(x),  a  constant. 

If  we  denote  the  Fourier  series  corresponding  to  the  g  function 
by  =  r 


4-  h1  sin  t  +  h%  sin  2  t  + 
we  have 


cos  ntdt  =  0, 


f(x\     /^c+2w 

-^L 


7T      ^^ 

sin  ntdt  =  0. 


7T 

Thus  the  sum  of  the  first  n  -f  1  terms  of  the  Fourier  series 
belonging  to  g(f)  reduces  to 

<?.  =/(*)•  (9 

But  this  sum  is  also  given  by  8),  if  we  replace 

by  <?(*42M; 

since  g  is  a  constant.      We  get  thus 


Sin  W 

Let  us  therefore  subtract  f(x)  from  both  sides  of  8),  using  9), 
10).     We  get 

IT 

F.(x)  -f(x)  =  -T  {/(*  +  2  «)  +f(x  -  2  t.)  -  2/O)  j  b 


sin 


Settin&  AW  =  Trl^W  -/(*)},  (11 


We  have  thus  the  theorem  : 

For  the  Fourier  Series  to  converge  to  f(x)  at  the  point  x,  it  is 
necessary  and  sufficient  that  Dn(x)  =0,  as  n  ==  oo. 


424  FOURIER'S  SERIES 

Validity  of  Fourier's  Development* 

439.  The  integral  on  the  right  side  of  438,  12),  on  which  the 
validity  of  Fourier's  development  at  the  point  x  depends,  is  a 
special  case  of  the  integral 


In  fact  Jn  goes  over  into  Dn,  if  we  set 


, 
sin  u  2 

To  evaluate  Jn  let  us  break  23  up  into  the  intervals 


-.r=ar 
n 


These  intervals  are  equal  except  the  last,  which  is  shorter  than 
the  others  unless  b  —  a  is  a  multiple  of  ir/n.     We  have  thus 


If  we  set 

v  =  M  +  - 

71 


we  see  that  while  v  ranges  over  3325,  u  ranges  over  332*-i-  This 
substitution  enables  us  to  replace  the  integrals  over  332<s  by  those 
over  SBfc-n  since 

I     g  (v)  sin  nvdv  —  —  I        g(u  +  —  )  sin  nudu. 

JL%2S  £®2s-l     *  U' 

Hence  grouping  the  integrals  in  pairs,  we  get 
Jn=  I     g(u)  sin  nudu  +  2  I  1 9(.u)  ~~  9\u  +  ~  )  r  s^n  ww^w 

f   O3  ^^^      f  c*j  I  \  M.  /  I 

e^*50  *     oL202«-l       L  \  ft/  J 

/-» 

+    I     g  (u)  sin  nudu, 

JLw 

*  The  presentation  given  in  439-448  is  due  in  the  main  to  Lebesgue.  Cf.  his 
classic  paper,  Mathematische  Annalen,  vol.  61  (1905),  p.  251.  Also  his  Lemons  sur 
les  Series  Trigonometriques,  Paris,  1906. 


VALIDITY  OF   FOURIER'S   DEVELOPMENT  425 

where  W  is  33r  or  $,._!  -f  $r,  depending  on  the  parity  of  r.     Now 

I,  (2 


du 


du. 


IsC,  {'<->-'("+i)J™ 


n 


\L 


Thus  Jn  =  0,  if  the  three  integrals  2),  3),  4)  =  0.  Moreover, 
if  these  three  integrals  are  uniformly  evanescent  with  respect  to 
some  point  set  (£  <  33,  Jn  is  also  uniformly  evanescent  in  (£.  In 
particular  we  note  the  theorem 

Jn  =  0,  if  g  is  L-integrable  in  53. 

We  are  now  in  a  position  to  draw  some  important  conclusions 
with  respect  to  Fourier's  series. 

440.  1.  Let  f(x)  be  L-integraUe  in  (c,  C  +  ^TT).  Then  the 
Fourier  constants  an,  bn  =  0,  as  n  =  oo. 


For 


-^      />c+2jr 

an  =  -  f 

irJic 


cos  nxdx 


is  a  special  case  of  the  Jn  integral.  As /is  L-integrable,  we  need 
only  apply  the  theorem  at  the  close  of  the  last  article.  Similar 
reasoning  applies  to  bn. 

2 .    For  a  given  value  of  x  in  51  =  ( —  TT,  TT)  let 


sn  u 


IT 


be  L-integrable  in  33  =  f  0,  —  j.      Then  Fourier  s  development  is  valid 
at  the  point  x. 


426  FOURIER'S   SERIES 

For  by  438,  Fourier's  series  =  /(#)  at  the  point  x,  if  Dn(x)  =  0. 
But  Dn  is  a  special  case  of  Jn  for  which  the  g  function  is  in- 
tegrable.  We  thus  need  only  apply  439. 

3.    For  a  given  x  in  21  =  (—  vr,  TT),  let 

u 

/        \ 
be  L-integrable  in  33  =  f  0,  —  j.      Then  Fourier  s  development  is  valid 

at  the  point  x. 
^For  let  S>0,  then   : 


sm 


u 


=  0     ,     as  S  =  0     ,     by  hypothesis. 
4.    For  a  given  x  in  51  =  (—  TT,  TT),  Ze£ 

)-/C»)  (8 


fte  L-integrable  in  51.      2TAe?^  Fourier  s  development  is  valid  at  the 
point  x.  .  .  , 

f(x-2u)-f(x) 


x 

J  u 


f         7T\ 

Thus  x  ig  -Zy-integrable  in  f  0,  —  j,  as  it  is  the  difference  of  two 
integrable  functions. 

441.    (Lebesgue).     For  a  given  x  in  5l  =  (—  TT,  TT)  let 

7T 
/»« 

«=«        oto 

P* 

2°  Km  I    |^(w  +  o)  —  ty(u)  \du  =  0 

*-«aW 

/br  some  y  such  that 


VALIDITY  OF  FOURIER'S  DEVELOPMENT 


427 


Then  Fourier's  development  is  valid  at  the  point  x. 
For  as  we  have  seen, 


\X)\< 


sin  M 


it_ 

f 
X. 


du 


du<D' 


\srnu 
where  &,  is  a  certain  number  which  =     »  as  n  =  oo. 


us  first  consider  Dr.     Since  0<w<—  ,  we  have 


Hence 


z/%4 


sin 


sin 


, 

u h  T  — 

6         24 


|t,          0«r,   T< 


=    r- 


4  7 


=  V 


'u     -.       TM  \  ~>        .  a 

~6\Ty        ~*? 


<z^,  provided  s>t. 
But  this  is  indeed  so.     For 


«  _  vau  ^  -.  _  TT 


Hence 


Thus 


Df  <  v  I     |0|  C?M  =  0,  by  hypothesis. 

eio 

w0?#  <i«rw  ^o  D'r.     We  have 


428  FOURIER'S   SERIES 

Now  /  being  L-integrable, 

*(•+?)-*<•> 

is  £-integrable  in  f  77,  1L  \  .     Thus 


lim        =  0. 
But  by  condition  2°, 


lim  f"  = 

•^•oLir 


Thus  lim  IX  '  =  0. 

s=o 

Finally  we  consider  Dfff.      But  the  integrand  is  an  integrable 
function  in  f  /3,  ^  J  .     Thus  it  =  0  as  n  =  GO  . 


442.  1.  7^0  validity  of  Fourier's  development  at  the  point  x  de 
pends  only  on  the  nature  off  in  a  vicinity  of  x,  of  norm  $  as  small  as 
we  please. 

For  the  conditions  of  the  theorem  in  441  depend  only  on  the 
value  of  /in  such  a  vicinity. 

2.    Let  us  call  a  point  x  at  which  the  function 


is  continuous  at  u  =  0,  and  has  the  value  0,  a  regular  point. 

In  438,  we  saw  that  if  #  is  a  point  of  discontinuity  of  the  first 
kind  for  /(#),  then  #  is  a  regular  point. 

3.    Fourier's  development  is  valid  at  a  regular  point  x,  provided 
for  some  ij 

lim 

6=0 

For  at  a  regular  point  x,  $(u)  is  continuous  at  u  =  0,  and  =  0 
for  u  =  0.     Now 

lim  1  /**!  <K«)  1  du= 
A=o  hJio 


LIMITED   VARIATION  429 

7T  77 

Thus 

du  =  TT  •  — 


Hence  condition  1°  of  441  is  satisfied. 

Limited  Variation 

443.  1.  Before  going  farther  we  must  introduce  a  few  notions 
relative  to  the  variation  of  a  function  f(x)  defined  over  an  interval 
$1  =(#<£>).  Let  us  effect  a  division  D  of  21  into  subintervals, 
by  interpolating  a  finite  number  of  points  al  <  a2  <  •••  The  sum 

F,-  2  |/(«.)  -/(«.+!)  I  (1 

is  called  the  variation  of  fin  51  for  the  division  D.     If 

Max  VD  (2 

is  finite  with  respect  to  the  class  of  all  finite  divisions  of  21,  we  say 
/  'has  finite  variation  in  21.     When  2)  is  finite,  we  denote  its  value  by 

Var/,     or      Vf,     or      V 
and  call  it  the  variation  of  f  in  31. 

We  shall  show  in  5  that  finite  variation  means  the  same  thing 
as  limited  variation  introduced  in  I,  509.  We  use  the  term  finite 
variation  in  sections  1  to  4  only  for  clearness. 

2.  A  most  important  property  of  functions  having  finite  vari 
ation  is  brought  out  by  the  following  geometric  consideration. 

Let  us  take  two  monotone  increasing  curves  A,  B  such  that  one 
of  them  crosses  the  other  a  finite  or  infinite  number  of  times.  If 
f(x),  g(x)  are  the  continuous  functions  having  these  curves  as 
graphs,  it  is  obvious  that 


is  a  continuous  function  which  changes  its  sign,  when  the  curves 
A,  B  cross  each  other.  Thus  we  can  construct  functions  in  infinite 
variety,  which  oscillate  infinitely  often  in  a  given  interval,  and 
which  are  the  difference  of  two  monotone  increasing  functions. 


430  FOURIER'S   SERIES 

For  simplicity  we  have  taken  the  curves  A,  B  continuous.  A 
moment's  reflection  will  show  that  this  is  not  necessary. 

Since  d(x)  is  the  difference  of  two  monotone  increasing  functions, 
its  variation  is  obviously  finite.  Jordan  has  proved  the  following 
fundamental  theorem. 

3.  If  f(x)  has  finite  variation  in  the  interval  51  =  (a  <  5),  there 
exists  an  infinity  of  limited  monotone  increasing  functions  g(x),  h(x} 
such  that  f—o_h  (\ 

For  let  D  be  a  finite  division  of  St.     Let 

PD=  sum  of  terms  J/OWj)—  /(<OS  which  are  >  0, 


Then  VB  =  2  l/Ow,)  -/(«-)  \=P0  +  ND.  (2 


Also 

)  -/(«)!  +  !/<X)-/(«i)i  +  -  +  \f(V)  -f(an)\=PD-ND. 
On  the  left  the  sum  is  telescopic,  hence 

f(V)-f  (.<*)=  PD-ND.  (3 

From  2),  3)  we  have 

VD  =  2  PD  +/(a)-/(J)  =  2  Na  +/(6)  -/(«).  (4 

Let  now  MaxPB  =  P     ,     Max^  =  ^ 

with  respect  to  the  class  of  finite  divisions  D. 

We  call  them  the  positive  and  negative  variation  of  f(x)  in  51. 
Then  4)  shows  that 


/(a).  (5 

Adding  these,  we  get       jr=  p  +  jy.  (6 

From  5)  we  have 


-/(«)  =  P-JV.  (7 

Instead  of  the  interval  21  =  («<&),  let   us   take    the    interval 
(a  <  x),  where  x  lies  in  St.     Replacing  5  by  a:  in  7),  we  have 

/(*)=/(«)  +  P(x)-JIT(*).  (8 


LIMITED   VARIATION  431 

Obviously   P(x),   -ZV(#)    are    monotone    increasing    functions. 
Let  p(x)  be  a  monotone  increasing  function  in  21.     If  we  set 


(9 


we  get  1)  from  8)  at  once. 
4.    From  8)  we  have 

I  < 


5.    We  can  now  show  that  when  f(x)  has  finite  variation  in  the 
interval  51  =  (a  <  6)  it  has  limited  variation  and  conversely. 

For  if  /  has  finite  variation  in  21  we  can  set 

/CO  =  *(*)  -*(*), 

where  <£,  ty  are  monotone  increasing  in  21.     Then  if  21  is  divided 
into  the  intervals  Sx,  S2  •••  we  have 

Osc/< 


Osc  4>  =  A<£     ,     Osc  ^  =  A^     ,     in  St 

since  these  functions  are  monotone.     Hence  summing  over  all  the 

intervals  S,,       vrx     *  ^  <**         ^  A 

2  Osc/<  2A0  H-  SA-v/r 

<  {0(5)-  ^(a)}  +  {^(ft)  -  t(a)  j 

<  some  $f,  for  any  division. 
Hence  /  has  limited  variation. 

If  /  has  limited  variation  in  21, 

|  A/I  <0sc/    ,     in£t. 

Hence  2  |  A/  1  <  2  Osc/  <  some  M. 

Hence  /has  finite  variation. 

6.    If  f(x)  has  limited  variation  in  the  interval  21,  its  points  of 
continuity  form  a  pant  act  ic  set  in  21. 

This  follows  from  5,  and  I,  508. 


432  FOURIER'S   SERIES 

7.    Let  a<b<  c  ;  then  iff  has  finite  variation  in  (a,  c), 

JW+  v»,J=  va,j,  (ii 

^>6  means  the  variation  of  f  in  the  interval  (a,  5),  efa. 
r«/=  Max  VBf 

with  respect  to  the  class  of  all  finite  divisions  D  of  (a,  <?).  The 
divisions  D  fall  into  two  classes  : 

1°  those  divisions  E  containing  the  point  5, 

2°  the  divisions  F  which  do  not. 

Let  A  be  a  division  obtained  by  interpolating  one  or  more 
points  in  the  interval.  Obviously 


Let  now  Gr  be  obtained  from  a  division  F  by  adding  the  point 

Then 


Hence  Max  Fi>Max  VF. 

E  F 


Hence  to  find  F^fC/,  we  may  consider  only  the  class  E.  Let 
now  E^  be  a  division  of  (a,  5),  and  E%  a  division  of  (5,  <?).  Then 
^  +  EI  is  a  division  of  class  E.  Conversely  each  division  of  class 
Ogives  a  division  of  (a,  5),  (5,  c).  Now 


From  this  11)  follows  at  once. 

444.    We  establish  now  a  few  simple  relations  concerning  the 
variation  of  two  functions  in  an  interval  51  =  (a  <  ft). 


F°r 

where  for  brevity  we  set  /.  _  ff    . 

/i  —  J\aJ' 

|iy.  (2 


LIMITED   VARIATION  433 

3.    Letf,  g  be  monotone  increasing  functions  in  21.      Then 

n/+<7)  =  Vf+  Vg.  (3 

For 


4.    .For  any  two  functions  f,  g  having  limited  variation, 

Vf+Vg.  (4 


5.    Letf,^  have  limited  variation  in  21  =  («,  £). 
7W 

«=!/(«)!    ,   «i=l/iO)|. 

^(//i)  <(«  +  fy)(«!  +  vfo  (5 

For  by  443,  8)  we  have 


where 
Thus 


Hence  by  2,  4, 

<  ^PA  +  ^y^  +  VPAl  +  ... 
-)     ,     by  3 


But  Vf=P  +  N    ,     hence,  etc. 

445.    Fourier's  development  is  valid  at  the  regular  point  x,  if  there 

exists  a  0  <  f  <~,  such  that  in  (0,  f)  £Ae  variation  V(u)  of  i/r(V) 

-j 

m  awy  (u,  f  )  zs  limited^  and  such  that  u  V(u)  =  0,  u  =  0. 
By  442,  we  have  only  to  show  that 


2 

is  evanescent  with  B. 


434  FOURIER'S   SERIES 

Let  us  first  suppose  that  ty(u)  is  monotone  in  some  (0,  £),  say 
monotone  increasing.  Similar  reasoning  will  apply,  if  it  is  mono 
tone  decreasing.  Then,  taking  0  <  rj  +  B  <  £ , 

^=  r\^u  +  §)-^(u)\du  =  (  ^(u+S)du-  I    ^(u)du. 
In  the  second  integral  from  the  end,  set  v  =  u  +  S. 

Xrj  /*17+5 

^(u  +  tydu  =  /       ty(v)dv. 
aW 

Hence, 


r 
ltl<^ 


We  will  consider  the  integrals  on  the  right  separately.     Let 

^m  =  Max  |^|,         in 
Then 


Hence,  -,         -i 

1  -  <  some  M. 


=  -  +  o-u     , 


sin  u      u 
Thus, 


=  0     ,     as  8  =  0     ,     since  </>(w)  =  0, 
as  a:  is  a  regular  point. 

TTe  iwrw  wow  to  %.     In  (17,  77  +  8),  3,  ??  sufficiently  small, 
sin  u  >  M  -     ^3  >  ri(I  -  ??2). 


LIMITED  VARIATION  435 

Thus,  if  <#v  =  Max  |  0'|  in  (77,  77  +  S),  >>* 


with  S. 

Thus,  when  ty  is  monotone  in  some  (0,  f),  Fourier's  develop 
ment  is  valid.  But  obviously  when  -ty  is  monotone,  the  condition 
that  uV(u)=0  is  satisfied.  Our  theorem  is  thus  established  in 
this  case. 

Let  us  now  consider  the  case  that  the  variation    r(v)  of  i/r  is 

limited  in  (u,  f). 

From  443,  10),  we  have 


As  before  we  have 


By  hypothesis  there  exists  for  each  €  >  0,  a  S0  >  0,  such  that 

u  V(u)  <  e     ,     for  any  0  <  u  <  80  . 
Hence, 

PX*)^1   ' 

u 


s  turn  now  to  ^2.     Since   V(u)  is  the  sum  of  two  limited 
monotone  decreasing  functions  P,  Nin.  (u,  f)'  ^  ig  integrable. 
Thus, 


/»7 

I  / 

ot'T? 


is  evanescent  with 


436  FOURIER'S   SERIES 

446.    1.    Fourier's  development  is  valid  at  the  regular  point  x,  if 
^>(u)  has  limited  variation  in  some  interval  (0  <  f  ),      f  <  —  . 
For  let  0  <  u  <  7  <  ?,  then 


Now  T/r=<f>(X)  •  - 

sm  u 

Hence      Vuy+  <  j  V^  + 
But  sin  w  b.eing  monotone, 


__  ___  _ 

MY  sin  w      sin  w      sin  7 


Thus 


sm 

Similarly'         r*<S**±. 

vfr—          sin  7  2* 

Now 

0<-^-<^f    ,     in  (0*,  n. 
sin  w 

The  theorem  now  follows  by  445.     For  we  may  take  7  so  small 

that  T-r      ,  € 


Thus  for  any  u  <  7, 


On  the  other  hand,  3)^  being  sufficiently  large,  and  7  chosen  as 
in  1)  and  then  fixed, 

Thus 


for  w<some  5r.     Hence 

for  0  <  u  <  some  B. 

2.    (Jordan.  )     Fourier's  development  is  valid  at  the  regular  point 
x,  *ff(v)  has  limited  variation  in  some  domain  of  x. 


OTHER  CRITERIA  437 

For       <K«)  =  !/(*  +  2  «)-/O)!+  {/(*-  2  «)-/(»)} 

has  limited  variation  also. 

3.    Fourier's  development  is  valid  at  every  point  of  21  =  (0,  2  TT), 
iff  is  limited  and  has  only  a  finite  number  of  oscillations  in  21. 


Other  Criteria 
447.    Let    X= 


.Zf  X  =  0  rts  S  =  0,  so  does  "^,  awe?  conversely. 
For  ,   ^x         xA  ,    <xx  sinfw  4- 


U  +  0 

•  /-   N  >  sin 


Obviously   X    and   "^   are    simultaneously  evanescent   with 
provided 

R  =  =  0     ,     as  8  =  0. 


Let 

r*,     v        Sin  U 

Z(u)  =  - 
u 

Then  .  f  N  <  r*s     .   ^^ 


Now 


v  cos  v  —  sin  v 


tf 
Thus 


438 
Hence 

As 


FOURIER'S   SERIES 


sin  u 


- 


!J>|iO    , 


with  8. 


448.  (Lipschitz-Dini.)  At  the  regular  point  x,  Fourier's  devel 
opment  is  valid,  if  for  each  e  >  0,  there  exists  a  S0  >  0,  swcA  that  for 
each  0  <  8  <  S0  , 


For 


l       . 
log  5 


n 


, 


Now  a:  being  a  regular  point,  there  exists  an  rjf  such  that 

I  $00  I  <  €>         f°r  w  in  any  (^»  ^')' 

Thus  taking  ^       , 

^7  >  o,  V, 


<e 


Thus 


,  log  B  |          e  VS 
<  2  e,         for  any  8  <  ?;. 
X  =  0,  as  8  =  0. 


I  _1\ 

o     V 


Uniqueness  of  Fourier's  Development 
449.    Suppose  /(V)  can  be  developed  in  Fourier's  series 


1    /1|r 
an=  -  I       /(a?) 

T^cX-TT 


cos 


sn 


,      (2 


UNIQUENESS  OF   FOURIER'S   DEVELOPMENT  439 

valid  in  51  =  (—  TT,'  TT).      We  ask  can/"  (V)  be  developed  in  a  simi- 
/  (x)  =  I  a0'  +  2(an'  cos  n#  +  £„'  sin  712:),  (3 

also  valid  in  51,  where  the  coefficients  are  not  Fourier's  coefficients, 
at  least  not  all  of  them. 

Suppose  this  were  true.     Subtracting  1),  3)  we  get 

0  =  £  O0  -  O  +  2  {  (an  -  <)  cos  war  +  (&„  -  &i)  sin  r?:r  J  =  0, 

?0  +  2  jtfn  cos  tt#  -f  c?n  sin  /i^j  =  0,          in  51.  (4 

Thus  it  would  be  possible  for  a  trigonometric  series  of  the  type 
4)  to  vanish  without  all  the  coefficients  cm,  dm  vanishing. 
For  a  power  series 


to  vanish  in  an  interval  about  the  origin,  however  small,  we  know 
that  all  the  coefficients  pm  in  5)  must  =>  0. 

We  propose  to  show  now  that  a  similar  theorem  holds  for  a 
trigonometric  series.  In  fact  we  shall  prove  the  fundamental 

Theorem  1.  Suppose  it  is  known  that  the  series  4)  converges  to  0 
for  all  the  points  of  51  =  (—  TT,  TT),  except  at  a  reducible  set  9?. 
Then  the  coefficients  cm,  dm  are  all  0,  and  the  series  4)  =  0  at  all  the 
points  o/5l. 

From  this  we  deduce  at  once  as  corollaries  : 

TJieorem  2.     Let  $1  be  a  reducible  set  in  51.      Let  the  series 

«0  +  2  \an  cos  nx  +  @n  sin  nx\  (6 

converge  in  51,  except  possibly  at  the  points  Si.      Then  6)  defines  a 
function  l?(x)  in  51  -  3t 

If  the  series  ,      v<    ,  Ql  . 

«0  +  2  \  «„  cos  nx  +  fin  sin  nx  \ 

converges  to  F(x)  in  51  —  9?,  its  coefficients  are  respectively  equal  to 
those  in  6). 


Theorem  3.  If  f(^x)  admits  a  development  in  Fourier1  %  series  for 
the  set  51  —  9?,  any  other  development  of  f(x)  of  the  type  6),  valid  in 
51  —  9£  is  necessarily  Fourier's  series,  i.e.  the  coefficients  «TO,  fim  have 
the  values  given  in  2). 


440  FOURIER'S  SERIES 

In  order  to  establish  the  fundamental  theorem,  we  shall  make 
use  of  some  results  due  to  Riemann,  Gr.  Cantor,  Harnack  and 
Schwarz  as  extended  by  later  writers.  Before  doing  this  let  us 
prove  the  easy 

Theorem  4-  If  /(#)  admits  a  development  in  Fourier  s  series 
which  is  uniformly  convergent  in  21  =  (  —  TT,  TT),  it  admits  no  other 
development  of  the  type  3),  which  is  also  uniformly  convergent  in  51. 

For  then  the  corresponding  series  4)  is  uniformly  convergent 
in  21,  and  may  be  integrated  termwise.  Thus  making  use  of  the 
method  employed  in  436,  we  see  that  all  the  coefficients  in  4) 
vanish. 

450.  1.  Before  attempting  to  prove  the  fundamental  theorem 
which  states  that  the  coefficients  #n,  bn  are  0,  we  will  first  show 
that  the  coefficients  of  any  trigonometric  series  which  converges 
in  21,  except  possibly  at  a  point  set  of  a  certain  type,  must  be  such 
that  they  =  0,  as  n  =  oo.  We  have  already  seen,  in  440,  1,  that 
this  is  indeed  so  in  the  case  of  Fourier's  series,  whether  it  con 
verges  or  not.  It  is  not  the  case  with  every  trigonometric  series 
as  the  following  example  shows,  viz.  : 

§  sin  n  \  x.  (1 

i 

When  x  =  r^  all   the  terms,  beginning  with  the  r  !th,   vanish, 
r  I 

and  hence  1)  is  convergent  at  such  points.  Thus  1)  is  conver 
gent  at  a  pantactic  set  of  points.  In  this  series  the  coefficients  an 
of  the  cosine  terms  are  all  0,  while  the  coefficients  of  the  sine 
terms  6n,  are  0  or  1.  Thus  bn  does  not  =  0,  as  n  =  oo. 

2.  Before  enunciating  the  theorem  on  the  convergence  of  the 
coefficients  of  a  trigonometric  series  to  0,  we  need  the  notion  of 
divergence  of  a  series  due  to  Harnack. 

Let  A=a1  4-  a2+  •••  (2 

be  a  series  of  real  terms.  Let  gn,  Grn  be  the  minimum  and  maxi 
mum  of  all  the  terms 

-^n+l        »       -An+2       , 

where  as  usual  An  is  the  sum  of  the  first  n  terms  of  2).     Obviously 


UNIQUENESS   OF   FOURIER'S   DEVELOPMENT  441 

Thus  the  two  sequences  \gn\,  [Grn\  are  monotone,  and  if  limited, 
their  terms  converge  to  fixed  values.     Let  us  say 


The  difference 

b  =  #-<7 

is  called  the  divergence  of  the  series  2). 

3.    For  the  series  2)  to  converge  it  is  necessary  and  sufficient  that 
its  divergence  b  =  0. 

For  if  A  is  convergent, 


Thus  -e  +  A<gn<G-n<A  +  €. 

Thus  the  limits  Gr,  g  exist,  and 

G-g<2e     ;     or  G-  =  g, 
as  e  >  0  is  small  at  pleasure. 

Suppose  now  b  =  0.     Then  by  hypothesis,  Gr,  g  exist  and  are 
equal.     There  exists,  therefore,  an  n,  such  that 

<7-*<<7n<#n<#  +  e, 
or  #n-<7n<2e. 

Thus  \An+p-An\<2e     ,    p=l,2-. 

and  A  is  convergent. 

451.    Let  the  series 

GO 

2  (an  cos  nx  +  bn  sin  nx) 

o 

be  such  that  for  each  8  >  0,  there  exists  a  subinterval  of 

Sl  =  (-ir,  TT) 
fa  divergence  b  <  S.      Men  an,  6n  =  0,  as 


=  QO. 


For,  as  in  450,  there  exists  for  each  x  an  wz,  such  that 

£ 
|  0n  cos  nx  +  5n  sin  nx  \  <  -     ,     n>  mx  (1 


442  FOURIER'S  SERIES 

for  any  point  x  in  some  interval  $3  of  21.  Thus  if  b  is  an  inner 
point  of  23,  x=-b  +  @  will  lie  in  33,  if  0  lies  in  some  interval 
B  =  (p,  q).  Now 

an  cos  ft  (b  +  /3)  +  6n  sin  n(b  +  j3) 

=  (an  cos  716  +  &„  sin  w&)  cos  n/3  —  (an  sin  nb  —  bn  cos  ^6)  sin  n/3. 
an  cos  n(b  —  (3}  +  bn  sin  w (6  —  /3) 
v;^  r=  (.ancosnb  +  &„  sin  w5)  cos  w/3  +  («n  sin  nb  -  5n  cos  ^6)  sin  nj3. 

Adding  and  subtracting  these  equations,  and  using  1)  we  have 

•  8 

. ,   |.  (an  cos  nb  +  ;5n  sin  nb)  cos  n/5  |  <  -, 

^ 
|  (an  sin  nb  —  ln  cos  w5)  sin  n@    <  -, 

for  all  n>mx.  Let  us  multiply  the  first  of  these  inequalities  by 
cos  nb  sin  nf$,  and  the  second  by  sin  nb  cos  nft,  and  add.  •  We  get 

|  an  sin  w£J  <  8     ,     /^  =  2  £     ,     n  >  mx.  (2 

Again  if  we  multiply  the  first  inequality  by  sin  nb  sin  n/3,  and 
the  second  by  cos  nb  cos  n/3,  and  subtract,  we  get 

bnsmn/3l\  <S   \     n>mx.  (3 

From  2),  3),  we  can  infer  that  for  any  e  >  0 

|  an'\  <  e  '  y   ;,|  bn  |  <  e.    ,     n  >  some  ?w,  (4 

or  what  is  the  same,  that  an,  Jn  =  0. 

For  suppose  that  the  first  inequality  of  4)  did  not  hold.     Then 
there  exists  a  sequence 

n\  <  n2  <  ...  =  oo  (5 

such  that  on  setting 

i«^1  =  «+«ir     ,     e-S  =  S' 
we  will  have 

«.,  >  «'•  (6 

If  this  be  so,  we  can  show  that  there  exists  a  sequence 

J:,  V.l  <  V2  <  '••   =  °° 

in  5),  such  that  for  some  ft'  in  B, 

\aVrsmvr{3'\  >B,  (7 


UNIQUENESS   OF   FOURIER'S   DEVELOPMENT  443 

which  contradicts  2).     To  this  end  we  note  that  70  >  0  may  be 
chosen  so  small  that  for  any  r  and  any  |  7  |  <  70  , 

|  aVr  |  cos  7  >  (B  -f  £')  cos  70  >  B.  (8 

Let  us  take  the  integer  vl  so  that 

Vl>7L±2h.  (9 

9-f 

Then  2^^  N       n     N  -^  r> 

-Oi  (?-?)-  270)^2- 


7T 


Thus  at  least  one  odd  integer  lies  in  the  interval  determined  by 
the  two  numbers 

9  9 


Let  ml  be  such  an  integer.     Then 

9  9 

j(M'  +  W<%  <  ^Oi  -  70)- 
If  we  set 


we  see  that  the  interval  Bl=(pr  q^  lies  in  B.     The  length  of 
Bl  is  270/i/j.      Then  for  any  /3  in  .B^ 

"i/3  =  mi^  +  f>'i     '     |7il<70- 

Thus  by  8), 

|  avi  sin  i/j/3  j  =  1^1  cos  j1  >  8.  (12 

But  we  may  reason  on  Bl  as  we  have  on  B.  We  determine  z>2 
by  9),  replacing  jt?,  q  by  JPX,  ^j.  We  determine  the  odd  integer  m2 
by  10),  replacing^,  q,  vl  by  p1,  q1,  v2.  The  relation  11)  deter 
mines  the  new  interval  B2  =  (jt?2,  ^2),  on  replacing  m^  vl  by  w2,  z^2. 
The  length  of  B2  is  2jQ/v2,  and  52  lies  in  ^j.  For  this  relation 
of  v2  ,  and  for  any  /3  in  B.2  we  have,  similar  to  12), 

|  avt  sin  z/2/3  |  >  B. 

In  this  way  we  may  continue  indefinitely.  The  intervals 
Bl  >  ^2  >  ...  =  to  a  point  /3',  and  obviously  for  this  (S\  the  rela- 


444  FOURIER'S   SERIES 

tion  7)  holds  for  any  x.     In  a  similar  manner  we  see  that  if  bn  does 
not  =  0,  the  relation  3)  cannot  hold. 

452.    As  corollaries  of  the  last  theorem  we  have  : 
1.    Let  the  series 

00 

bn  sin  nx)  (1 


be  such  that  for  each  &  >  0,  the  points  in  5l  =  (  —  TT,  TT)  at  which 
the  divergence  of  1)  is  >8,  form  an  apantactic  set  in  51.  Then 
an,  bn  =  0,  as  n  =  oo  . 

2.  Let  the  series  1)  converge  in  51,  except  possibly  at  the  points  of 
a  reducible  set  ^R.  Then  an,  bn  =  0. 

For  9t  being  reducible  [318,  6],  there  exists  in  51  an  interval  33 
in  which  1)  converges  at  every  point.  We  now  apply  451. 

453.  Let 

at  the  points  of  51  =  (—  TT,  TT),  where  the  series  is  convergent.  At  the 
other  points  of  51,  let  F(x)  have  an  arbitrarily  assigned  value,  lying 
between  the  two  limits  of  indetermination  g,  Gr  of  the  series.  If  F  is 
R-integrable  in  51,  the  coefficients  an,  bn  =  0. 

For  there  exists  a  division  of  51,  such  that  the  sum  of  those  in 
tervals  in  which  Osc  F>  o>  is  <  cr.  There  is  therefore  an  interval 
3  in  which  Osc  F  <  o>.  If  &  is  an  inner  interval  of  3,  the  di 
vergence  of  the  above  series  is  <  w  at  each  point  of  $.  We  now 
apply  451. 

454.  Riemanrfs  Theorem. 

Let  F(x)  =  ^  a0  +  2(an  cos  nx  +  bn  sin  nx)  =  2J.n    converge   at 

each  point  of  51  =  (—  TT,  TT),  except  possibly  at  the  points  of  a  redu 
cible  set  9?.  The  series  obtained  by  integrating  Ms  series  termwise, 
we  denote  by 

a(x)  =  -  a^  -  JJ  —  (an  cos  nx  +  bn  sin  nx)  =  -  AQx2  -  %  -f- 
~t  -i  n  M  •«    n 

Then  Q-  is  continuous  in  51. 


UNIQUENESS   OF   FOURIER'S   DEVELOPMENT  445 

Let  <b(u)  =  G-(x  +  2  u)  +  #(z  -  2  w)  -  2  G(x).  (1 

£  eacA  point  of  33  =  21  —  9?, 

lira  ^^  =  ^0)  ;  (2 

«=o     4  IT 

edch  point  oj  21, 

lim^^  =  0.  (3 

t*=o      w 

For,  in  the  first  place,  since  9?  is  a  reducible  set,  an,  bn  =  0.  The 
series  6r  is  therefore  uniformly  convergent  in  21,  and  is  thus  a 
continuous  function. 

Let  us  now  compute  <l>.     We  have 

an  cos  n(x  +  2  w)  +  an  cos  /i(a:  —  2  w)  —  2  an  cos  wa; 
=  2  an  cos  no:  (cos  2  nu  —  1) 
=  —  4  an  cos  w#  sin2  nu. 

Also        6n  sin  n(>  +  2  w)  -f  6n  sin  w(z  -  2  ^)  -  2  on  sin  wa; 

=  '2bn  sin  /ix(cos  2  ww  —  1) 

=  —  4  bn  sin  nx  sin2  ww. 
Thus 


4  u2         o        \    nu 

if  we  agree  to  give  the   coefficient   of  A^  the  value   1.      Let  us 
give  x  an  arbitrary  but  fixed  value  in  53.     Then  for  each  e  >  0, 

there  exists  an  w  such  that      •- 


en     ,       €B<€,     n>i 
Thus  ^ 


(4 


446  FOURIER'S  SERIES 

The  index  m  being  determined  as  above,  let  us  take  u  such  that 

u  <  —     ,     so  that     m  <  —  ; 
m  u 

and  break  jS  into  three  parts 


1  m+l  K+I 

where  K  is  the  greatest  integer  <  TT/U,  and  then  consider  each  sum 
separately,  as  u  =  0. 

Obviously  lim  S1  =  0. 

u=Q 

As  to  the  second  sum,  the  number  of  its  terms  increases  indefin 
itely  as  u  =  0. 
For  any  u, 


(i—     •  —19  i—    •  — 19  x 

p^>-?_r~7 
mu    J  KU    J  J 


<,r!»2!.P.<« 

WW 


since  each  term  in  the  brace  is  positive.     In  fact 

sin  v 

v 

is  a  decreasing  function  of  v  as  v  ranges  from  0  to  TT,  and 
nu  <  KU  <_TT     ,     n  OB  we,  tn  -f- 1,  ...  *. 

Finally  we  consider  Sy      We  may  write   the  general  term  as 
follows  : 


[rsin(n-l>"|2    _rsi 
€n   lL    (n-l)w    J   "    L 


jTsin  (n  -  l)^"]2     fsin  nu~V\ 
'  €n  IL~"      nu         J      L   W    J  J 

sin2  (yi  —  1)u  —  s\ii2nu  _  —  sin  (2n  —  l)u  sin  w  ,  ^  ,     1 


UNIQUENESS  OF   FOURIER'S  DEVELOPMENT  447 

Thus 


<^-T( 


O-l)2      n*\       u 

6  € 


since 


But  K  >_  —  —  1     ,     or  KU  _>  TT  —  w. 

M 

Thus  I . y  <  c  f     1      i     1    I  - 

1  (TT  —  w)2      TT  —  u) 

Hence  e       o        „        ^  -  n   .      ,   •   n 

o  =  Oj  -(-  o2  +  A33  —  u,  as  u  =  u, 

which  proves  the  limit  2),  on  using  4). 
To  prove  the  limit  3),  we  have 


Let  us  give  wa  definite  value  and  break  ^Tinto  three  sums. 

m 

T±  =  2, 
where  m  is  chosen  so  that 

\A  n  I  <  e     ,     n  >  m  ; 


TO+l 

where  \  is  the  greatest  integer  such  that 

\U<_1', 

and 

A+l 

Obviously  for  some  M, 

|  Z\|  <.w^f. 
Also 

since 


448  FOURIER'S   SERIES 

As  to  the  last  sum, 

u  A+1.v 
Thus  T  ^  Q          as  M  =  0. 

455.    Schwarz-Luroth  Theorem.  • 

In  ty,  =  (a  <  b}  let  the  continuous  function  f  (x)  be  such  that 

except  possibly  at  an  enumerable  set  &  in  51.     At  the  points  ($,  let 

uS(x,  u)  =  0         as  u  =  0.  (2 

Then  f  is  a  linear  function  in  51. 

Let  us  first  suppose  with  Schwarz  that  (g  =  0.     We  introduce 
the  auxiliary  function, 

where  _ 

?;  =  ±  1,  and  c  is  an  arbitrary  constant. 

The  function  g  (V)  is  continuous  in  51,  and  <?  (a)  =  </ (5)  =  0. 
Moreover  ,  >.    ,      ,  N       0    /•  -\ 

flr(^4-1*)4-Q'(^  —  tt  J  —  !Z<7(2?).  -n 

e_v ! : — ! — ii_i . — L £_! — L  =  <?,  as  U  =  U. 

Thus  for  all  0<u<  some  8, 

(3 


From  this  follows  that  g(x)<0  in  51.     For  if  #(V)>0,  at  any 
point  in  51,  it  takes  on  its  maximum  value  at  some  point  f  within  51. 

Thus 


for  0  <  w  <  8,  8  being  sufficiently  small.     Adding  these  two  in 
equalities  gives  6r  <_0,  which  contradicts  3).     Thus  #.<  0  in  51. 
Let  us  now  suppose  L=fcO  for  some  x  in  51.     We  take  c  so  small 

that  T  r 

sgn#  =  sgn  ?;£  =  77  sgn  .L. 


UNIQUENESS  OF  FOURIER'S   DEVELOPMENT  449 

But  77  is  at  pleasure   ±  1,  hence  the  supposition  that  L  =£  0  is 
not  admissible.     Hence  L  =  0  in  21,  or 

/<X)=/00-f5|j/(i)-/00!  (4 

is  indeed  a  linear  function. 

Let  us  now  suppose  with  Liiroth  that  (g>0.     We  introduce  the 
auxiliary  continuous  function. 


Thus  A(a)=0     , 

Suppose  at  some  inner  point  £  of 


This  leads  to  a  contradiction,  as  we  proceed  to  show.     For  then 
provided 


We  shall  take  c  so  that  this  inequality  is  satisfied,  i.e.  c  lies  in 
the  interval®  =  (0*,  (7*).     Thus 


Hence  A(V)  takes  on  its  maximum  value  at  some  inner  point  e 
of  31.     Hence  for  B  >  0  sufficiently  small, 

<S.      (6 
(7 


Now  if  e  is  a  point  of  H  —  (S, 


«=o 

But  this  contradicts  7),  which  requires  that 
\\mH(e,  w)<0. 


450  FOURIER'S   SERIES 

Hence  e  is  a  point  of  (£.     Hence  by  2), 

h(e  +  u)-h(e)  +  AQ  -  M)  -  &(e)  ^  Q          as  w  ^  Q. 
w  w 

By  6),  both  terms  have  the  same  sign.     Hence  each  term  =  0. 
Thus  f  or  u  >  0 

0  =  lim  h(e  ±M^~  h^  =  lim  f(e 


±u  ±u  b  —  a 

+  2*0-a). 

Thus  to  each  c  in  the  interval  (£,  corresponds  an  e  in  (£,  at  which 
point  the  derivative  of  f(x)  exists  and  has  the  value  given  on  the 
right  of  8).  On  the  other  hand,  two  different  <?'s,  say  c  and  c' ,  in 
(£  cannot  correspond  to  the  same  e  in  (S. 

For  then  8)  shows  that 

c  (e  —  a)  =  c'(e  —  #), 
or  as  >  ,  _ 

Thus  there  is  a  uniform  correspondence  between  (£  whose  cardi 
nal  number  is  c,  and  (£  whose  cardinal  number  is  e,  which  is  absurd. 
Thus  the  supposition  5)  is  impossible.  In  a  similar  manner,  the 
assumption  that  L  <  0  at  some  point  in  51,  leads  to  a  contradiction. 
Hence  L  =  0  in  51,  and  4)  again  holds,  which  proves  the  theorem. 

456.    Cantor  s  Theorem.     Let 

J  a0  +  2)(#n  cos  nx  +  bn  sin  nx)  (1 

i 

converge  to  0  in  5l  =  (—  TT,  TT),  except  possibly  at  a  reducible  set  9?, 
where  nothing  is  asserted  regarding  its  convergence.  Then  it  con 
verges  to  0  at  every  point  in  51,  and  all  its  coefficients 

For  by  452,  2,  an,  5n  =  0.     Then  Riemann's  function 

^v  N      i  V  1  A  * 

/  (V)  =  -J-  aQx2  —  V  —  (an  cos  w#  H-  6n  sin  712:) 

^  n^ 


UNIQUENESS   OF   FOURIER'S   DEVELOPMENT  451 

satisfies  the  conditions  of  the  Schwarz-Liiroth  theorem,  455,  since  9? 
is  enumerable.  Thus  f(x)  is  a  linear  function  of  x  in  51,  and  has 
the  form  a  +  fix.  Hence 

«    1 
a  +  fix  —  |  aQx2  =  —  2,  -g  («B  cos  W2:  +  ^n  sin  712:) .  (2 

The  right  side  admits  the  period  2  TT,  and  is  therefore  periodic. 

Its  period  o>  must  be  0.  For  if  &>  >  0,  the  left  side  has  this 
period,  which  is  absurd.  Hence  co  =  0,  and  the  left  side  reduces 
to  a  constant,  which  gives  /3=0,  a0=  0.  But  in  51  —  9?,  the  right 
side  of  1)  has  the  sum  0.  Hence  «=  0.  Thus  the  right  side  of 
2)  vanishes  in  51.  As  it  converges  uniformly  in  51,  we  may  deter 
mine  its  coefficients  as  in  436.  This  gives 


CHAPTER   XIV 
DISCONTINUOUS  FUNCTIONS 

Properties  of  Continuous  Functions 

457.  1.  In  Chapter  VII  of  Volume  I  we  have  discussed  some 
of  the  elementary  properties  of  continuous  and  discontinuous 
functions.  In  the  present  chapter  further  developments  will  be 
given,  paying  particular  attention  to  discontinuous  functions. 
Here  the  results  of  Baire  *  are  of  foremost  importance.  Le- 
besgue  f  has  shown  how  some  of  these  may  be  obtained  by  sim 
pler  considerations,  and  we  have  accordingly  adopted  them. 

2.  Let  us  begin  by  observing  that  the  definition  of  a  continu 
ous  function  given  in  I,  339,  may  be  extended  to  sets  having  iso 
lated  points,  if  we  use  I,  339,  2  as  definition. 

Let  therefore/0^  •••  xm)  be  defined  over  51,  being  either  limited 
or  unlimited.  Let  a  be  any  point  of  21.  If  for  each  e  >  0,  there 
exists  a  8  >  0,  such  that 

I/O)  -/O)  |  <  e,         for  any  x  in  F5(a), 
we  say  /  is  continuous  at  a. 

By  the  definition  it  follows  at  once  that  /  is  continuous  at  each 
isolated  point  of  21.  Moreover,  when  a  is  a  proper  limiting  point 
of  21,  the  definition  here  given  coincides  with  that  given  in  I,  339. 
If /is  continuous  at  each  point  of  21,  we  say  it  is  continuous  in  21. 
The  definition  of  discontinuity  given  in  I,  347,  shall  still  hold, 
except  that  we  must  regard  isolated  points  as  points  of  con 
tinuity. 

*  "  Sur  les  Functions  de  Variables  reeles,"  Annali  di  Mat.,  Ser.  3,  vol.  3 
(1899). 

Also  his  Lemons  sur  les  Functions  Discontinues.     Paris,  1905. 
t  Bulletin  de  la  Societe  Mathematique  de  France,  vol.  32  (1904),  p.  229. 

452 


PROPERTIES  OF   CONTINUOUS  FUNCTIONS  453 

3.  The  reader  will  observe  that  the  theorems  I,  350  to  354 
inclusive,  are  valid  not  only  for  limited  perfect  domains,  but  also 
for  limited  complete  sets. 

458.  1.  If  f(x^  •••  #m)  is  continuous  in  the  limited  set  51,  and  its 
values  are  known  at  the  points  of  53  <  51,  then  f  is  known  at  all 
points  of  53'  lying  in  51. 

For  let  5j,  b2,  b3  •••  be  points  of  53,  whose  limiting  point  b  lies 
in  5i.  Then 


2.  If  f  is  known  for  a  dense  set  53  in  5(,  and  is  continuous  in  51, 
/  is  known  throughout  51. 

For  g,  >  3, 

3.  If  f(x1  -•-  xm)  is  continuous  in  the  complete  set  51,  the  points 
53  in  51  where  f=c,a  constant,  form  a  complete  set.     If  51  is  an 
interval,  there  is  a  first  and  a  last  point  0/53. 

For/=  c  at  x=  «1?  «2  •••  which  =  a;  we  have  therefore 
/(a)  =  lim/(an)  =  c. 


459.  The  points  of  continuity  (£  of  /(a:1---^m)  in  51  lie  in  a 
deleted  enclosure  $.  Ifty.  is  complete,  ft  =  (£. 

For  let  ex  >  e2  >  •••  =  0.  For  each  en,  and  for  each  point  of 
continuity  c  in  51,  there  exists  a  cube  Q  whose  center  is  c,  such  that 

Osc/<en,         in  O. 

Thus  the  points  of  continuity  of  /  lie  in  an  enumerable  non- 
overlapping  set  of  complete  metric  cells,  in  each  of  which 
Osc/<  en.  Let  Qn  be  the  inner  points  of  this  enclosure.  Then 
each  point  of  the  deleted  enclosure 

«  =  I*  {CU 

which  lies  in  51  is  a  point  of  continuity  of  /.     For  such  a  point  c 
lies  within  each  Qn. 

Hence  r\      *  ^  -     rr  s  \ 

Osc/<  e,         in  F6O), 

for  S  >  0  sufficiently  small  and  n  sufficiently  great. 


454  DISCONTINUOUS  FUNCTIONS 

Oscillation 
460'    Let  n 


This  is  a  monotone  decreasing  function  of  S.     Hence  if  o>5  is 

finite,  for  some  8  >  0, 

&)  =  lim  o>5 


6=0 


exists.     We  call  co  the  oscillation  off  at  x  =  a,  and  write 
T  W   v>  »^t» 


Should  o)s  =  -f  oo,  however  small  &  >  0  is  taken,  we  say  o>  =  -f  <x>. 
A  I  v\"\A^^nen  w  =  ^/  ig  continuous  at  x  =  a,  if  a  is  a  point  in  the  domain 
of  definition  of/.     When  o>  >  0,  /is  discontinuous  at  this  point. 
It  is  a  measure  of  the  discontinuity  off  at  x  =  a  ;  we  write 


461.    1. 

at  x  =  a.      Then 

\d-e\<  Disc  (/  ±  ^)  <  d  +  e. 

x—a 

For  in  F5  (a), 

|Osc/-  Osc^l  <  Osc(/±^)  <  OSG/+ 

2.  Tf/  is  continuous  at  x  =  a,  while  Disc  g  =  d,  then 

Disc  (/  +  9)  =  d. 

j:=a 

For  /being  continuous  at  a,         Disc/  =  0. 
Hence  Disc  ^  <  Disc  (/  +  g)  <  Disc  g  =  d. 

3.  If  c  is  a  constant, 

Disc  (c/)  =  |  c  |  Disc/    ,     at  x  =  a. 
For  Osc  (c/)  =  ;  c  |  Osc/    ,     in  any  F«(a). 

4.  When  the  limits 


OSCILLATION  455 

exist  and  at  least  one  of  them  is  different  from  /"(a;),  the  point  x 
is  a  discontinuity  of  the  first  kind,  as  we  have  already  said. 
When  at  least  one  of  the  above  limits  does  not  exist,  the  point  x 
is  a  point  of  discontinuity  of  the  second  kind. 

462.  1.  The  points  of  infinite  discontinuity  3  of  f,  defined  over 
a  limited  set  tyi,form  a  complete  set. 

For  let  i],  t2  •••  be  points  of  3,  having  k  as  limiting  point. 
Then  in  any  V(k)  there  are  an  infinity  of  the  points  in  and  hence 
in  any  V(lc),  Osc/=  +  oo.  The  point  k  does  not  of  course 
need  to  lie  in  51. 

2.  We  cannot  say,  however,  that  the  points  of  discontinuity  of 
a  function  form  a  complete  set  as  is  shown  by  the  following 

Example.  In  51  =  (0,  1),  let  f(x)  =  x  when  x  is  irrational,  and 
=  0  when  x  is  rational.  Then  each  point  of  51  is  a  point  of  dis 
continuity  except  the  point  x  —  0.  Hence  the  points  of  disconti 
nuity  of /do  not  form  a  complete  set. 

3.  Let  f  be  limited  or  unlimited  in  the  limited  complete  set  51. 
The  points  ^of^at  ivhich  Oscf>^kform  a  complete  set. 

For   let   ar  «2  •••  be   points  of   $   which  =  a.     However  small 
8  >0  is  taken,  there  are  an  infinity  of  the  an  lying  in  F«(a).     But 
at  any  one  of  these  points,  Oscf~>_k.     Hence  Qscf>_k  in  V&  (a) 
and  thus  a  lies  in  $. 

4.  Letf(x^  -•  :rm)  be  limited  and  R-integrable  in  the  limited  set  51. 
The  points  ft  at  which  Oscf>^kform  a  discrete  set. 

For  let  D  be  a  rectangular  division  of  space.  Let  us  suppose 
$D  >  some  constant  c  >  0,  however  D  is  chosen.  In  each  cell  8 
of  D, 

Osc/>fc. 

Hence  the  sum  of  the  cells  in  which  the  oscillation  is  _>  k  can 
not  be  made  small  at  pleasure,  since  this  sum  is  &#.  But  this 
contradicts  I,  700,  5. 

5.  Let  f(xl  •••  zm)  be  limited  in  the  complete  set  51.     If  the  points 
$  in  51  at  which  Osc  /  >  k  form  a  discrete  set,  for  each  k,  then  f  is 
R-integrable  in  51. 


456  DISCONTINUOUS  FUNCTIONS 

For  about  each  point  of  51  —  $  as  center,  we  can  describe  a  cube 
&  of  varying  size,  such  that  Osc/<  2  k  in  (£.  Let  D  be  a  cubical 
division  of  space  of  norm  d.  We  may  take  d  so  small  that 
&D  =  2c?t  is  as  small  as  we  please.  The  points  of  51  lie  now  within 
the  cubes  (£  and  the  set  formed  of  the  cubes  d,.  By  Borel's 
theorem  there  are  a  finite  number  of  cubes,  say 


such  that  all  the  points  of  51  lie  within  these  TJ'S.  If  we  prolong 
the  faces  of  these  ?;'s,  we  effect  a  rectangular  division  such  that 
the  sum  of  those  cells  in  which  the  oscillation  is  >  2  k  is  as  small 
as  we  choose,  since  this  sum  is  obviously  <  ®D.  Hence  by  I,  700, 
5,  /  is  72-integrable. 

6.  Letf(x^  •••  xm*)  be  limited  in  51;  let  its  points  of  discontinuity 
in  51  be  £).  If  f  is  R-integrable,  2)  is  a  null  set.  If  51  is  complete 
and  2)  is  a  null  set,  f  is  R-integrable. 

Let  /  be  jR-integrable.  Then  £)  is  a  null  set.  For  let  e:  >  e2 
>  ...  =  0.  Let  $)„  denote  the  points  at  which  Osc/>  en.  Then 
$)  =  {£)„}.  But  since/  is  72-integrable,  each  £)n  is  discrete  by  4. 
Hence  £)  is  a  null  set. 

Let  51  be  complete  and  £)  a  null  set.  Then  each  £)n  is  complete 
by  3.  Hence  by  365,  £n  =  £)„.  As  £)  =  0,  we  see  S)nis  discrete. 
Hence  by  5,  /is  JZ-integrable. 

If  51  is  not  complete,  /  does  not  need  to  be  .R-integrable  when 
£)  is  a  null  set. 

Example.     Let  5IX  =         l      ,     n  =  1,  2  ...  ;  m  <  2». 


Let  51  =  51}  +  5^ . 

Let  /(V)  =  —     ,     at  x  =  ^ 

=  1          in  512 . 

Then  each  point  of  51  is  a  point  of  discontinuity,  and  51 
But  5lj,  5Lj  are  null  sets,  hence  51  is  a  null  set. 


POINTWISE   AND   TOTAL   DISCONTINUITY  457 

On  the  other  hand, 

J/=l     ,      f/=0, 

^31  —21 

and  /  is  not  72-integrable  in  51. 

Pointwise  and  Total  Discontinuity 


463.  Let/^j  •••  2?m)  be  defined  over  51.  If  each  point  of  31  is  a 
point  of  discontinuity,  we  say  /is  totally  discontinuous  in  51. 

We  say  /  is  pointwise  discontinuous  in  51,  if  /  is  not  continuous 
in  51=  \a\,  but  has  in  any  V(a)  a  point  of  continuity.  If/  is 
continuous  or  pointwise  discontinuous,  we  may  say  it  is  at  most 
pointwise  discontinuous. 

Example  1.  A  function/^  •••  zm)  having  only  a  finite  number 
of  points  of  discontinuity  in  51  is  pointwise  discontinuous  in  51. 

Example  2.     Let 

f(x)  =  0     ,     for  irrational  x  in  51  =  (0,  1) 

1  £.  m 

=  -     ,     for  x  —  — 

n  n 

=  1     ,     for  x  =  0,  1. 

Obviously  /  is  continuous  at  each  irrational  x,  and  discontinuous 
at  the  other  points  of  51.  Hence  /  is  pointwise  discontinuous 
in  51. 

Example  3.  Let  £)  be  a  Harnack  set  in  the  unit  interval 
51  =  (0,  1).  In  the  associate  set  of  intervals,  end  points  included, 
let/(z)=l.  At  the  other  points  of  51,  let  /=  0.  As  S)  is 
apantactic  in  51,  /  is  pointwise  discontinuous. 

Example  4.  In  Ex.  3,  let  $)  =  (g  +  g,  where  (§  is  the  set  of  end 
points  of  the  associate  set  of  intervals.  Let  /=  I/ft  at  the  end 
points  of  these  intervals  belonging  to  the  nih  stage.  Let/=  0  in 
g.  Here  /  is  defined  only  over  £).  The  points  g  are  points  of 
continuity  in  £).  Hence/  is  pointwise  discontinuous  in  S). 

Example  5.  Let/(V)  be^irichlfit!s_function,  i.e.  /=  0,  for  the 
irrational  points  3  in  51  =  (0,  1),  and  =  1  for  the  rational  points. 


458      •  DISCONTINUOUS   FUNCTIONS 

As  each  point  of  21  is  a  point  of  discontinuity,/  is  totally  discon 
tinuous  in  21.  Let  us  remove  the  rational  points  in  21  ;  the  deleted 
domain  is  3.  In  this  domain/  is  continuous.  Thus  on  removing 
certain  points,  a  discontinuous  function  becomes  a  continuous 
function  in  the  remaining  point  set. 

This  is  not  always  the  case.  For  if  in  Ex.  4  we  remove  the 
points  g,  retaining  only  the  points  (£,  we  get  a  function  which  is 
totally  discontinuous  in  (£,  whereas  before  /  was  only  pointwise 
discontinuous. 

464.  1.  Iff(x1  •••  #m)  is  totally  discontinuous  in  the  infinite  com 
plete  set  21,  then  the  points  b^  where 

Disc/  >  co     ,     a)  >  0, 
form  an  infinite  set,  if  co  is  taken  sufficiently  small. 

For  suppose  bw  were  finite  however  small  co  is  taken.  Let 
o)1>ft)2>...  =0.  Let  Dj,  D2,  •••  be  a  sequence  of  superposed 
cubical  divisions  of  space  of  norms  dn  ==  0.  We  shall  only  con 
sider  cells  containing  points  of  21.  Then  if  d1  is  taken  sufficiently 
small,  D1  contains  a  cell  Sj,  containing  an  infinite  number  of 
points  of  21,  but  no  point  at  which  Disc/>ft>r  If  d2  is  taken 
sufficiently  small,  D2  contains  a  cell  S2<81,  containing  no  point 
at  which  Disc/><»2.  In  this  way  we  get  a  sequence  of  cells, 


which  ==  a  point  p.  As  21  is  complete,  p  lies  in  21.  But  /  is 
obviously  continuous  at  p.  Hence  /  is  not  totally  discontinuous 
in  21. 

2.    If  21  is  not  complete,  bw  .does  not  need  to  be  infinite  for 
any  co  >  0. 


Example.     Let  21  =  ,  n  =  1,  2,  •••  and  m  odd  and  <2".     At 

—  ,  let</=  —  •     Then  each  point  of  21  is  a  point  of  discontinuity. 
But  bo,  is  finite,  however  small  co  >  0  is  taken. 

3.    We  cannot  say  /is  not  pointwise  discontinuous  in  complete 
21,  when  bo>  is  infinite. 


EXAMPLES   OF   DISCONTINUOUS   FUNCTIONS  459 

Example.     At   the   points    |  -  \  =  %   let  /  =  0  ;    at    the   other 

(n) 

points  of  51  =  (0,  1),  let/=l. 

Obviously  /  is  pointwise  discontinuous  in  21.  But  bw  is  an 
infinite  set  for  &>  <  1,  as  in  this  case  it  is  formed  of  $ft,  and  the 
point  0. 

Examples  of  Discontinuous  Functions 

465.  In  volume  I,  330  seq.  and  348  seq.,  we  have  given  ex 
amples  of  discontinuous  functions.  We  shall  now  consider  a  few 
more. 

Example  1.     Riemanns  Function. 

Let  (x)  be  the  difference  between  x  and  the  nearest  integer; 
and  when  x  has  the  form  n  +  J,  let  (x)  =  0.  Obviously  (V)  has 
the  period  1. 

It  can  be  represented  by  Fourier's  series  thus  : 

sin  2  TTX      sin  2  •  2  TTX  .  sin  3  •  2  TTX 


Riemann  s  function  is  now 

This  series  is  obviously  uniformly  convergent  in  21  =  (—  oo,  oo). 
Since  (x)  has  the  period  1  and  is  continuous  within  (  —  J,  |), 

we  see  that  (nx)  has   the  period  -,   and  is   continuous  within 

n 

{  —  - — ,  —  j.     The  points  of  discontinuity  of  (nx)  are  thus 

®n=  \^-  +  -}      ,     «  =  0,  ±1,  ±2,... 
(  z  n      n  ) 

Let  (g=  5(gn{.  Then  at  any  a;  not  in  (£,  each  term  of  2)  is  a  con 
tinuous  function  of  x.  Hence  F(x)  is  continuous  at  this  point. 

On  the  other  hand,  F  is  discontinuous  at  any  point  e  of  (£.  For 
F  being  uniformly  convergent, 


R  lim  F(x)  =  ZR  lim  (3 


w 


i  lim  ^(a;)  =  2Z  lim  ^=^  (4 

x=€  ar=e       H2 


460  DISCONTINUOUS   FUNCTIONS 

We  show  now  that  3)  has  the  value 

jFO)--^         for  e=2*  +  1,         e  irreducible.  (5 

16  n2  2n 

and  4)  the  value 

||;  '  F^+w  <6 

Hence  2 

-OO-  (7 


To  this  end  let  us  see  when  two  of  the  numbers 
1    +£,      and      -L  +  i 


2mm  2 n     n 

are  equal.     If  equal,  we  have 


Thus  if  we  take  2  s  + 1  relatively  prime  to  n,  no  two  of  the  num 
bers  in  (§„  are  equal.  Let  us  do  this  for  each  n.  Then  no  two  of 
the  numbers  in  (g  are  equal. 

Let  now  x  =  e  = h  -  •    Then  (mx)  is  continuous  at  this  point, 

2  n     n 

unless  8)  holds;  i.e.  unless  m  is  a  multiple  of  n,  say  m=  In.  In 
this  case,  8)  gives 

Thus  I  must  be  odd  ;   I  =  1,  3,  5  •••     In  this  case  (mx)  =  0  at  e, 
while  .Rlim  (mx)  =  —  J.     When  m  is  not  an  odd  multiple  of  w, 

obviously  R  lim  (mx)  —  (me). 

Thus  when  m  =  In,  I  odd, 

7?r      (W)  1    1        (map      1  1       1 

«     m2    :        2  W~    m2    •    2  7*2  '  p' 

When  77i  is  not  a  multiple  of  n, 


m 


EXAMPLES   OF   DISCONTINUOUS   FUNCTIONS  461 

Hence 


This  establishes  5).     Similarly  we  prove   6).     Thus  F(x)  is 
discontinuous  at  each  point  of  (§.     As 


F  is   limited.     As  the   points  (S  form  an   enumerable  set,  F  is 
^-integrable  in  any  finite  interval. 


466.  Example  2.  Let/(V)=0  at  the  points  of  a  Cantor  set 
(7=  m  •  ^#2  •••  ;  m  =  0,  or  a  positive  or  negative  integer,  and  the 
a's  =  0  or  2.  Let  f(x)  =  1  elsewhere.  Since  /  (x)  admits  the 

period  I,/  (3  tt#)  admits  the  period  --     Let  01  be  the  points  of 

3  n 

C  which  fall  in  21  =(0,  1).  Let  Dl  be  the  corresponding  set  of 
intervals.  Let  <72  =  (7X  +  Fx,  where.  Tl  is  obtained  by  putting  a 
Cl  set  in  each  interval  of  D1  .  Let  Dz  be  the  intervals  correspond 
ing  to  <72.  Let  <73  =  (72  +  F2  where  F2  is  obtained  by  putting  a  <72 
set  in  each  interval  of  .Z>2,  etc. 

The  zeros  of/(3nz)  are  obviously  the  points  of  Cn.     Let 


The  zeros  of  F  are  the  points  of  (S  =  \  Cn\.  Since  each  (7n  is  a  null 
set,  (S  is  also  a  null  set.  Let  A  =  21  —  (L  The  points  J.,  (£  are 
each  pantactic  in  51.  Obviously  F  converges  uniformly  in  51, 
since  0</(3  nx)  <1.  Since  fn(x)  is  continuous  at  each  point  a 
of  -4,  F  is  continuous  at  a,  and 


462  DISCONTINUOUS   FUNCTIONS 

We  show  now  that  F  is  discontinuous  at  each  point  of  (£.     For 
let  em  be  an  end  point  of  one  of  the  intervals  of  Dm+1  but  not  of 


Dm.     Then 


-- 
7/1 


Hence 


As  the  points  ^4.  are  pantactic  in  21,  there  exists  a  sequence  in 
A  which  =  e.     For  this  sequence  F  =  H.     Hence 


Similarly,  if  rjm  is  not  an  end  point  of  the  intervals  Dm+1,  but  a 
limiting  point  of  such  end  points, 

Disc  =  5^ 

*=>?m 

The  function  F  is  jft-integrable  in  21  since  its  points  of  discon 
tinuity  (£  form  a  null  set. 

467.  Let  &  =  S«tl...la!  be  an  enumerable  set  of  points  lying  in  the 
limited  or  unlimited  set  21,  which  lies  in  $ftm.  For  any  x  in  21  and 
any  eL  in  (£,  let  x—  e^  lie  in  $8.  Let  g(x1  •••  #m)  be  limited  in  53  and 
continuous,  except  at  x  =  0,  where 

Disc  #(V)=  b. 
Let  (7=2cti...la  converge  absolutely.      Then 


is  continuous  in  A  =  21  —  (£,  and  at  x=  e^ 


For  when  #  ranges  over  21,  #  —  et  remains  in  $8,  and  g  is  limited 
in  33.  Hence  F  is  uniformly  and  absolutely  convergent  in  21. 

Now  each  g(x  —  ej)  is  continuous  in  A  ;  hence  ^  is  continuous 
in  A  by  147,  2. 


EXAMPLES   OF  DISCONTINUOUS   FUNCTIONS  463 

On  the  other  hand,  F  is  discontinuous  at  x  =  eK.     For 


where  If  is  the  series  F  after  removing  the  term  on  the  right  of 
the  last  equation.  But  H,  as  has  just  been  shown,  is  continuous 
at  x  =  eK  . 

468.    Example  1.     Let  (&  =  \en\   denote   the    rational    numbers. 


•JO 

=  0        ,        x=0. 
Then  rv  \      V*  1    /  N  -i 

^0*0=2,—  #O-O    >    /*>! 

?*M 

is  continuous,  except  at  the  points  (g.     At  x  =  en, 

Disc  ^  =  -^. 
n* 

Example  2.     Let  @  =  \en\  denote  the  rational  numbers. 

Let  "- 


=  0     , 
which  we  considered  in  I,  331. 

Then 


is  continuous,  except  at  the  rational  points,  and  at  x  =  em, 

Disc  F(x)  =  —  . 

m ! 

469.  In  the  foregoing  g(x)  is  limited.  This  restriction  may  be 
removed  in  many  cases,  as  the  reader  will  see  from  the  following 
theorem,  given  as  an  example. 

LetJ2=\eil...ls\  be  an  enumerable  apantactic  set  in  $(.  Let  (§  = 
(J£,  E'}.  For  any  x  in  51,  and  any  et  in  E,  let  x  —  et  lie  within  a 
cube  53.  Let  g^  •••  xm)  be  continuous  in  58  except  at  x=Q,  where 
9  ==  +  QO,  as  x=  0.  Let  2ctl...t<  be  a  positive  term  convergent  series. 


464  DISCONTINUOUS   FUNCTIONS 

Then  • 


is  continuous  in  A  =  H  —  (§.     On  the  other  hand,  each  point  of  ($  is  a 
point  of  infinite  discontinuity. 

For  any  given  point  x  =  a  of  A  lies  at  a  distance   >  0  from  (g. 
Thus 


as  x  ranges  over  some  F^(a),  and  et  over  E. 
Hence  |0(s-  Ol<  some  JK; 

for  a:  in  V^(a),  and  et  in  E.  Thus  .F  is  uniformly  convergent  at 
x  =  a.  As  each  g(x  —  et)  is  continuous  at  #  =  a,  F  is  continuous 
at  a. 

.Z/e£  next  x  =  eK.     Then  there  exists  a  sequence 

x\  x"  ...  =  eK  (1 

whose  points  lie  in  A.  Thus  the  term  g(x  —  eK)  ==  +  oo  as  x  ranges 
over  1).  Hence  a  fortiori  F  =  +  oo.  Thus  each  point  of  E  is  a 
point  of  infinite  discontinuity. 

Finally  any  limit  point  of  E  is  a  point  of  infinite  discontinuity, 
by  462,  1. 

470.   Example.      Let  g(x)  =  -     ,     an  =  --     ,  •   a  >  1. 

x  an 


n 
Then 


is  a  continuous  function,  except  at  the  points 

:':  '     "  :    o,-i,-^-v-      :  ••'•• 

a        a*        a6 
which  are  points  of  infinite  discontinuity. 

471.  Let  us  show  how  to  construct  functions  by  limiting 
processes,  whose  points  of  discontinuity  are  any  given  complete 
limited  apantactic  set  (£  in  an  m-way  space  9?m. 


EXAMPLES   OF   DISCONTINUOUS   FUNCTIONS  465 

1.  Let  us  for  simplicity  take  m  =  2,  and  call  the  coordinates  of 
a  point  #,  y. 

Let  Q  denote  the  square  wlxose  center  is  the  origin,  and  one  of 
whose  vertices  is  the  point  (1,  0). 

The  edge  of  Q  is  given  by  the  points  x,  y  satisfying 

|*|+|y|  =  l.  (1 

Thus  .,  f  J,  on  the  edge 


- 

LO,  outside 

of  the  square  Q.     Hence 

L  (     „)  =  ifl  -  lim     "tt-M-lyli    ]  =  (  i,  on  the  edge,      g 
2L        -=.l+njl-|*  -[y|d      10,  off  the  edge. 


edge. 

Thus  ff(*y)=0(*,y)  +  J(*,y)  =  {;'in.e' 

10,  without  (). 

2.  We  next  show  how  to  construct  a  function  g  which  shall  =  0 
on  one  or  more  of  the  edges  of  Q.  Let  us  call  these  sides  e^  <?2,  £3,  e±, 
as  we  go  around  the  edge  of  Q  beginning  with  the  first  quadrant. 
If  6r  =  0  on  et,  let  us  denote  it  by  Grl  ;  if  G-  =  0  on  «t,  eK  let  us 
denote  it  by  6rl(C,  etc.  We  begin  by  constructing  6rr  We  observe 
that 


=oo  1  +  w|<  !        10,  for  tj=  0. 
Now  the  equation  of  a  right  line  I  may  be  given  the  form 

x  cos  a  +  y  sin  a  =  p 
where  0<a<27r,  jt?>0.      Hence 

=  1  -  lim      n  I  g  COS  a  +  y  sin  a  ~  p  I       =  j1'  on  Z' 
n=x  1  +  w  |  a;  cos  a  +  ?/  sin  a  —  p  \        (  0,  off  I. 

If  now  we  make  I  coincide  with  ev  we  see  that 

y)  = 


Hence 


-  ^(^  y)  =     '  n  , 

0,  on  ex  and  without  Q. 


466  DISCONTINUOUS   FUNCTIONS 

In  the  same  way, 


By  introducing  a  constant  factor  we  can  replace  Q  by  a  square 
Qc  whose  sides  are  in  the  ratio  c :  1  to  those  of  Q. 

Tnus  i  H ,  on  the  edge  of  ft, 

Q^  y^  _  iim  Trn \~^~\\^  =  1 1»  inside, 


1  +  (  c    +    c)         l°'  °utside' 

We  can  replace  the  square  Q  by  a  similar  square  whose  center 
is  #,  b  on  replacing  |#|,  \y\  by  \x  —  a  ,  \y  —  b\. 

We  have  thus  this  result :  by  a  limiting  process,  we  can  con 
struct  a  function  g(x,  y)  having  the  value  1  inside  $,  and  on  any 
of  its  edges,  and  =  0  outside  ft  and  on  the  remaining  edges. 
Q  has  any  point  a,  b  as  center,  its  edges  have  any  length,  and  its 
sides  are  tipped  at  an  angle  of  45°  to  the  axes. 

We  may  take  them  parallel  to  the  axes,  if  we  wish,  by  replacing 


x 


,  |  y  |  in  our  fundamental  relation  1)  by 


Finally  let  us  remark  that  we  may  pass  to  w-way  space,  by  re 
placing  1)  by 

|  xl  |  4-  |*2  I  +  -  +  |*m|  =  l. 

3.  Let  now  Q  =  jqn|  be  a  border  set  [328],  of  non-overlapping 
squares  belonging  to  the  complete  apantactic  set  (£,  such  that 
d-f-  (£  =  9?  the  whole  plane.  We  mark  these  squares  in  the 
plane  and  note  which  sides  qn  has  in  common  with  the  preceding 
q's.  We  take  the  gn(xy)  function  so  that  it  is  =  l  in  qn,  except 
on  these  sides,  and  there  0.  Then 


has  for  each  point  only  one  term  ^=  0,  if  #,  y  lies  in  O,  and  no 
term  ^=  0  if  it  lies  in  (£. 
Hence 


_  { 1»  f°r  each  point  of  O, 
"  I  0,  for  each  point  of '<£. 


EXAMPLES  OF   DISCONTINUOUS    FUNCTIONS  467 

Since  &  is  apantactic,  each  point  of  (S  is  a  point  of  disconti 
nuity  of  the  2°  kind  ;  each  point  of  Q  is  a  point  of  continuity. 

4.    Let/(2#)  be  a  function  denned  over  51  which  contains  the 
complete  apantactic  set  (£. 

Then 


472.    1.    Let  51  =  (0,  1),    $B=  the  points  2  ™  +  l  in  51. 

Then  53n,  $„  have  no  points  in  common. 
Let/n(»  =  1  in  »n,  and  =  0  in  Bn  =  51  -  23n. 
Let«=[SBnJ.     Then 


The  function  J7  is  totally  discontinuous  in  33,  oscillating  be 
tween  0  and  1.  The  series  F  does  not  converge  uniformly  in 
any  subinterval  of  51. 

2.    Keeping  the  notation  in  1,  let 


At  each  point  of  23n,  G-  =  -,  while  Gr  =  0  in  ^. 

ft 

The  function  6r  is  discontinuous  at  the  points  of  93,  but  con 
tinuous  at  the  points  B.  The  series  G-  converges  uniformly  in 
51,  yet  an  infinity  of  terms  are  discontinuous  in  any  interval  in  51. 

473.  Let  the  limitecj.  set  51  be  the  union  of  an  enumerable  set 
of  complete  sets  £5ln5.  We  show  how  to  construct  a  function/, 
which  is  discontinuous  at  the  points  of  51,  but  continuous  else 
where  in  an  w-way  space. 

Let  us  suppose  first  that  51  consists  of  but  one  set  and  is  com 
plete.  A  point  all  of  whose  coordinates  are  rational,  let  us  call 
rational,  the  other  points  of  space  we  will  call  non-rational.  If  51 
has  an  inner  rational  point,  let  /=  1  at  this  point,  on  the  frontier 
of  51  let  /=  1  also  ;  at  all  other  points  of  space  let  /=  0.  Then 
each  point  a  of  51  is  a  point  of  discontinuity.  For  if  x  is  a  fron- 


468  DISCONTINUOUS   FUNCTIONS 

tier  or  an  inner  rational  point  of  91,  f(x)  =  1,  while  in  any  V(x) 
there  are  points  where  /=  0.  If  x  is  not  in  91,  all  the  points  of 
some  D(x)  are  also  not  in  91.  At  these  points  /=  0.  Hence  /is 
continuous  at  such  points. 

We  turn  now  to  the  general  case.     We  have 


where  A1  =  9^,  Az  —  points  of  912  not  in  9lx,  etc.  Let/j  =  1  at  the 
rational  inner  points  of  A^  and  at  the  frontier  points  of  9lj ;  at  all 
other  points  let  /x  =  0.  Let  /2  =  1  at  the  rational  inner  points  of 
A2,  and  at  the  frontier  points  of  A%  not  in  Al ;  at  all  other  points  H 
let  /2  =  0.  At  similar  points  of  Az  let/3  =  J,  and  elsewhere  =  0, 
etc. 

Consider  now  TJ 


Let  x  =  a  be  a  point  of  91.  If  it  is  an  inner  point  of  some  A,, 
it  is  obviously  a  point  of  discontinuity  of  F.  If  not,  it  is  a  proper 
frontier  point  of  one  of  the  A's.  Then  in  any  D  (#)  there  are  points 
of  space  not  in  91,  or  there  are  points  of  an  infinite  number  of  the 
As.  In  either  case  a  is  a  point  of  discontinuity.  Similarly  we 
see  F  is  continuous  at  a  point  not  in  91. 

2.  We  can  obviously  generalize  the  preceding  problem  by  sup 
posing  91  to  lie  in  a  complete  set  33,  such  that  each  frontier  point 
of  91  is  a  limit  point  of  A  =  33  —  91. 

For  we  have  only  to  replace  our  w-way  space  by  33. 

Functions  of  Class  1 

474.  1.  Baire  has  introduced  an  important  classification  of 
functions  as  follows  : 

Let  /(#!•••#,„)  be  defined  over  91 ;  /and  91  limited  or  unlimited. 
If /is  continuous  in  91,  we  say  its  class  is  0  in  91,  and  write 

Class  /=0     ,     orCl/=0     ,     Mod  91. 
If  ^. 


each/n  being  of  class  0  in  91,  we  say  its  class  is  1,  if/  does  not  lie 
in  class  0,  mod  91. 


FUNCTIONS  OF  CLASS  1  469 

2.    Let  the  series  F(x)  =  ?,fn(x) 

converge  in  51,  each  term/n  being  continuous  in  51.     Since 


we  see  F  is  of  class  0,  or  class  1,  according  as  F  is  continuous,  or 
not  continuous  in  51.     A  similar  remark  holds  for  infinite  prod- 

UCts  G(x)=Hgn(x). 

3.  The  derivatives  of  a  function  f(x)  give  rise  to  functions  of 
class  0  or  1.  For  let  f(x)  have  a  unilateral  differential  coeffi 
cient  g  (x)  at  each  point  of  51.  Both  /  and  51  may  be  unlimited. 
To  fix  the  ideas,  suppose  the  right-hand  differential  coefficient 
exists.  Let  h1>hz>  •  ••  =  ().  Then 


is  a  continuous  function  of  x  in  51.     But 

0O)=lim?.<» 

n=oo 

exists  at  each  x  in  51  by  hypothesis. 

A  similar  remark  applies  to  the  partial  derivatives 

<tf_      .   V_ 

3*1         dxm 
of  a  function  f(xl  •«•  #n). 

4- 


each/n  being  of  class  1  in  51.  Then  we  say,  Cl/=  2  if  /does  not 
lie  in  a  lower  class.  In  this  way  we  may  continue.  It  is  of 
course  necessary  to  show  that  such  functions  actually  exist. 


475.    Example  1. 

for  x  >  0, 
for  x  =  0. 


,  =  Um      nx     =  f  1, 
«=»  1  +  nx      \  0, 


This  function  was  considered  in  I,  331.  In  any  interval 
51  =  (0  <  b)  containing  the  origin  x  =  0,  Cl  jf  =  1  ;  in  any  inter 
val  (a  <  6),  a  >  0,  not  containing  the  origin,  Cl/=  0. 


470  DISCONTINUOUS   FUNCTIONS 

Example  2. 

n=oo  enx 

The  class  of  f(x)  is  0  in  51.     Although  each  fn  is  limited  in  51, 
the  graphs  of  fn  have  peaks  near  x  =  0  which  =  oo,  as  n  =  oo. 

Example  S.     If  we  combine  the  two  functions  in  Ex.  1,  2,  we 

get       f  art^um  J-JL     l-lna^l1'*01**0' 

""  n=™  \  1  +  nx      enx*  J  1  0,  for  x  =  0. 

Hence  Cl/(z)  =  1  for  any  set  53  embracing  the  origin  ;    =  0 
for  any  other  set. 

Example  4- 

Let  /<»  =  liin.™*+»     ,     in  21  =  (0,1). 

n=oo 

Then  /(aO=0     ,     for  ^  =  0 

i 
=  2;^*     ,     for  2;  >  0. 

We  see  thus  that  /  is  continuous  in  (0*,  1),  and  has  a  point  of 
infinite  discontinuity  at  x  =  0. 

Hence  Class  /  (a;)  =1,    in  51 

=  0,    in(OM). 
Example  5. 

Let  j  ^  =  Um  __!  in  ^  =  (0?  ^^ 


a:      - 


Then  f(x)=^     ,     for  2:  >  0 

•2/ 

=  -foo     ,     for  x  —  0. 
Here  lim/*^) 

n=co 

does  not  exist  at  x  =  0.  We  cannot  therefore  speak  of  the  class 
of  /(a?)  in  51  since  it  is  not  defined  at  the  point  x  =  0.  It  is 
defined  in  53  =  (0*,  oo),  and  its  class  is  obviously  0,  mod  53. 


FUNCTIONS   OF   CLASS   1 


471 


Example  6. 
Let 


f(x)  =  sin  -     ,     for  x  =£  0 
x 


=  a  constant  c     ,     for  x  =  0. 

We  show  that  Cl/=  1  in  51  =  (-  0,  oo).     For  let 

nx  (     1 


712: 


sin 


=  <7n  0*0 


n 


Now  by  Ex.  1, 


0,  for  a;  >  0, 

e,  for  x  =  0  ; 


lim 


sin  -,  for  x  >  0, 

x 


while  nmnnW=} 

0,  for  2=0. 

As  each  fn  is  continuous  in  51,  and 

1*  •£    f     \  -/?/"     *\    *         OY 

•/  TI  V.     y   ~~"  •/  V    x  "*^^ 

we  see  its  class  is  <  1.     As  /  is  discontinuous  at  x  =  0,  its  class 
is  not  0  in  51. 


Example  7.     Let        ...       ,.     1      .1 
f(x)  =  lim  -  •  sin  -• 


..—  n 

Here  the  functions  fn(x)  under  the  limit  sign  are  not  defined 
for  x=  0.  Thus /is  not  defined  at  this  point.  We  cannot  there 
fore  speak  of  the  class  of  /with  respect  to  any  set  embracing  the 
point  x—  0.  For  any  set  58  not  containing  this  point,  Cl  /=  0, 
since  f(x)  =  0  in  53. 


Let  us  set 


Let 


<j>(x)  =  sin  -     ,     for  x  =£  0 
x 


=  a  constant  c 


g(x)  =  lim  - 


lim  <f>n(x). 


472  DISCONTINUOUS  FUNCTIONS 

Here  g  is  a  continuous  function  in  51  =  (—  oo,  oo).  Its  class  is 
thus  0  in  51.  On  the  other  hand,  the  functions  <£n  are  each  of 
class  1  in  5(. 

Example  8. 


is  defined  at  all  the  points  of  (—00,  oo)  except  0,  —  1,  —  2,  ... 
These  latter  are  points  of  infinite  discontinuity.  In  its  domain 
of  definition,  F  is  a  continuous  function.  Hence  Cl  F(V)  =  0 
with  respect  to  this  domain. 

476.  1.  If  51,  limited  or  unlimited,  is  the  union  of  an  enumerable 
set  of  complete  sets,  we  say  51  is  liy  per  complete. 

Example  1.  The  points  S*  within  a  unit  sphere  $,  form  a 
hypercomplete  set.  For  let  Sr  have  the  same  center  as  S,  and 
radius  r<l.  Obviously  each  2r  is  complete,  while  J2r5  =  A7*,  r 
ranging  over  r^  <  r2  <  -  •  •  =  1  . 

Example  2.  An  enumerable  set  of  points  al,  a2  •••  form  a  hyper- 
complete  set.  For  each  an  may  be  regarded  as  a  complete  set, 
embracing  but  a  single  point. 

2.    If  5lx,  5I2"*  are  limited  hypercomplete  sets,  so  is  their  union 


For  each  5lm  is  the  union  of  an  enumerable  set  of  complete  sets 
,n.     Thus  51=  151^  „(   m,  n  =  1,  2  •-•  is  hypercomplete. 


Let  51  be  complete.  If  $8  is  a  complete  part  of  51,  A  =  51  —  53  is 
hypercomplete. 

For  let  Q=  JqJ  be  a  border  set  of  53,  as  in  328.  The  points 
An  of  A  in  each  qn  are  complete,  since  51  is  complete.  Thus 
A  —  \An\,  and  A  is  hypercomplete. 

Let  51=  J5lnj  be  hypercomplete,  each  5In  being  complete.  If  53  i* 
a  complete  part  of  51,  ^.  =  51  —  53  is  hypercomplete. 

For  let  An  denote  the  points  of  5In  not  in  53.  Then  as  above, 
An  is  hypercomplete.  As  A  —  \An\,  A  is  also  hypercomplete. 


FUNCTIONS   OF   CLASS   1  473 

477.  1.    (Se  Sets.     If  the  limited  or  unlimited  set  51  is  the  union 
of  an  enumerable  set  of  limited  complete  sets,  in  each  of  which 
Osc/<e,  we  shall  say  51  is  an  (ie  set.     If,  however  small  e>0  is 
taken,  51  is  an  (£€  set,  we  shall  say  51  is  an  @€  set,  e  =  0,  which  we 
may  also  express  by  (£e=o- 

2.  Let  f(x±  •  •  •  xm)  be  continuous  in  the  limited  complete  set  51. 
Then  51  is  an  (ge  set,  e  =  0. 

For  let  €>0  be  taken  small  at  pleasure  and  fixed.  By  I,  353, 
there  exists  a  cubical  division  of  space  7),  such  that  if  5ln  denote 
the  points  of  51  in  one  of  the  cells  of  D,  Osc/<  e  in  5ln.  As  5ln  is 
complete,  since  51  is,  51  is  an  (§€  set. 

3.  An  enumerable  set  of  points  51=  \an\  is  an  (£e=y)  8e^- 

For  each  an  may  be  regarded  as  a  complete  set,  embracing  but 
a  single  point.  But  in  a  set  embracing  but  one  point,  Osc/=  0. 

4.  The  union  of  an  enumerable  set  of  (§e  sets  51  =  \  51™  j  is  an  ^  set. 
For  each  51™  is  the  union  of  an  enumerable  set  of  limited  sets 

2lm  =  S5lm,nj,  ns=l>  2>  -  and  Osc/<e  in  each  5lmn. 

Thus  a  =  {8LJ     ,     f»,  n  =1,2,... 

But  an  enumerable  set  of  enumerable  sets  is  an  enumerable  set. 
Hence  51  is  an  (£e  set. 

5.  Letf(x^  "-  xm)  be  continuous  in  the  complete  set  51,  except  at  the 
points  £)  =  c?j,  dz  ...  dt.      Then  51  is  an  (£^o  set. 

For  let  e>0  be  taken  small  at  pleasure  and  fixed.  About  each 
point  of  £)  we  describe  a  sphere  of  radius  p.  Let  5lp  denote  the 
points  of  51  not  within  one  of  these  spheres.  Obviously  5lp  is  com 
plete.  Let  p  range  over  r1  >  r2  >  •••  =  0.  If  we  set  5(  =  A  -f-  2), 
obviously  A  =  \$[rn}.  As/  is  continuous  in  5lfn,  it  is  an  (§e  set. 
Hence  51,  being  the  union  of  A  and  £),  is  an  (£e  set. 

478.  1.    Let  51  be  an  @e  set.     The  points  £)  of  51  common  to  the 
limited  complete  set  $8  form  an  (£e  set. 

For  51  is  the  union  of  the  complete  sets  5(n,  in  each  of  which 
Osc/<e.  But  the  points  of  5ln  in  33  form  a  complete  set  An,  and 
of  course  Osc/<  e  in  An.  As  2)  =  J  An\,  it  is  an  (ge  set. 


474  DISCONTINUOUS   FUNCTIONS 

2.  Let  51  be  a  limited  (ge  set.     Let  23  be  a  complete  part  of  51. 
Then  A  =  %  -  S3  is  an  (ge  se£. 

For  51  is  the  union  of  the  complete  sets  5ln,  in  each  of  which 
Osc  /<e.  The  points  of  5ln  not  in  33  form  a  set  An,  such  that 
Osc  /<e  in  An  also.  But  J.  =  \An\,  and  each  ^4n  being  hyper- 
complete,  is  an  @e  set. 

3.  Let/(^  ...  xm}  be  defined  over  51,  either/  or  51  being  limited 
or  unlimited.     The  points  of  51  at  which 

<*</<£  (1 

may  be  denoted  by 

(«</<£).  (2 

If  in  1)  one  of  the  equality  signs  is  missing,  it  will  of  course  be 
dropped  in  2). 


479.    1.  Let^  ,/2,  •••  be  continuous  in  the  limited  complete  set  H. 
If  at  each  point  of  51,  Urn  fn  exists,  51  is  an  (£e^0  set  and  so  is  any 

n=oo 

complete  53  <  51. 

For   let   lim  fn  (^  •••  zm)  =f(xl  •  ••  xm)  in  51.     Let  us  effect  a 

division  of  norm  e/2  of  the  interval  (  —  00,  oo  )  by  interpolating 
the  points  •  •  •  m_2 ,  m_  ^ ,  m0  =  0,  m^ ,  m2  •  •  • 
Let  5lt  =  (wt  </<  wl+2),  then  51  =  j  51 J . 

Next  let         ~        -Dvlm+-<f<m       --} 

Then  ^=\^n,Pl     »     w,  jt?  =  l,  2-»  (1 

For  let  a  be  a  point  of  5lt ,  and  say  /(#)  =  a.     Then 


But  a  —  €</5(a)  <«+  e     , 

and  we  may  take  e  and  n  so  that 


Hence  a  is  in  £)ni2? . 

Conversely,  let  a  be  a  point  of   5£)w>pj.     Then  a  lies  in  some 

n^p.     Hence, 

i       -^     ^    J?     /*      N      ^^"  -^ 


FUNCTIONS  OF  CLASS  1  475 

But  as/n(a)  ==/(«),  we  have 


Hence  if  e  is  sufficiently  small, 


and  thus  a  is  in  5lt  . 

Thus  1)  is  established.  But  £)np  is  a  divisor  of  complete  sets, 
and  is  therefore  complete.  Thus  51  is  the  union  of  an  enumerable 
set  of  complete  sets  j53t5i  in  each  of  which  Osc/<e,  e  small  at 
pleasure. 

Let  now  53  be  any  complete  part  of  51.  Let  at  =  Dv  J53,  53tj. 
Then  at  is  complete,  and  Osc/<e,  in  at.  Moreover,  53  =  \^\. 

Hence  53  is  an  (S€^  set- 

2.  If  Class  /<  1  in  limited  complete  51,  /  limited  or  unlimited, 
51  is  an  (Se  set. 

This  is  an  obvious  result  from  1. 

3.  Let  /(#!•••  #m)  be  a  totally  discontinuous  function  in  the  non- 
enumerable  set  51.      Then  Class  f  is  not  0  or  1  in  51,  (f  b  =  Disc/a* 
0a£^  point  is  <  &  >  0. 

For  in  any  subset  53  of  51  containing  the  point  re,  Osc  f>k. 
Hence  Osc  /is  not  <e,  in  any  part  of  51,  if  e  <  k.  Thus  51  cannot 
be  an  (Se  set. 

4.  If  Class  /(«!«••  zm);<  1  m  fAe  limited  complete  set  5(,  ^e  se£ 
53  =  («</<  5)  is  a  hyper  complete  set,  a,  b  being  arbitrary  numbers. 

For  we  have  only  to  take  a  =  mt,b  =  mi+2.  Then  53  =  5It,  which, 
as  in  1,  is  hypercomplete. 

480.  (Lebesgue.)  Let  the  limited  or  unlimited  f  unction  f^  •••  zm) 
be  defined  over  the  limited  set  51.  //  51  may  be  regarded  as  an 
(£e-o  set  with  respect  to  f,  the  class  of  f  is  <  1. 

For  let  col>  o>2  >  ...  =  0.  By  hypothesis  51  is  the  union  of  a 
sequence  of  complete  sets 

5ln  ,  5I12  ,  5I13...  (^ 

in  each  of  which  Osc  /  <.  Wj  •  51  is  also  the  union  of  a  sequence 
of  complete  sets 

»„      ,      »«      ,      »W"  (1 


476  DISCONTINUOUS   FUNCTIONS 

in  each  of  which  Osc/<  o>2.  If  we  superpose  the  division  1)  of 
51  on  the  division  A^,  each  5llK  will  fall  into  an  enumerable  set 
of  complete  sets,  and  together  they  will  form  an  enumerable 
sequence 


in  each  of  wThich  Osc^^o^-     Continuing  in  this  way  we  see  that 
21  is  the  union  of  the  complete  sets 


such  that  in  each  set  of  Sn,  Osc/<  o>n,  and  such  that  each  set  lies 
in  some  set  of  the  preceding  sequence  ASrn_1. 

With  each  2ln>s  we  associate  a  constant  (7n.s,  such  that 


<».   ,   in  a..,  (2 

and  call  <7n,  the  corresponding  field  constant. 

We  show  now  how  to  define  a  sequence  of  continuous  functions 
/i  1/2  "*  which  =/.  To  this  end  we  effect  a  sequence  of  super 
imposed  divisions  of  space  Dj,  D2  •••  of  norms  =  0.  The  vertices 
of  the  cubes  of  Dn  we  call  the  lattice  points  Ln  .  The  cells  of  Dn 
containing  a  given  lattice  point  I  of  Ln  form  a  cube  Q.  Let  5Ilti 
be  the  first  set  of  Sl  containing  a  point  of  Q.  Let  5l2i2  be  the  first 
set  of  iS72  containing  a  point  of  jQ  lying  in  2lltl.  Continuing  in 
this  way  we  get 

%H  >*W^  •'•>*•%• 

To  5Inln  belongs  the  field  constant  (7n,n  ;  this  we  associate  with 
the  lattice  point  I  and  call  it  the  corresponding  lattice  constant. 

Let  now  (S  be  a  cell  of  Dn  containing  a  point  of  31.  It  has  2n 
vertices  or  lattice  points.  Let  P8  denote  any  product  of  8  differ 
ent  factors  2rn,  #r2,  •••  xrg.  We  consider  the  polynomial 

4>  =  APn  +  25Pn_j  +  2  OP,_  +  .-  +  S^Pj  +  i, 

the    summation    in    each   case    extending   over   all    the    distinct 
products  of  that  type.     The  number  of  terms  in  <f>  is,  by  I,  96, 


FUNCTIONS  OF  CLASS   1  477 

We  can  thus  determine  the  2n  coefficients  of  <£  so  that  the  values 
of  </>  at  the  lattice  points  of  @  are  the  corresponding  lattice  con 
stants.  Thus  c/>  is  a  continuous  function  in  Q,  whose  greatest  and 
least  values  are  the  greatest  and  least  lattice  constants  belonging 
to  (£.  Each  cube  (5  containing  a  point  of  31  has  associated  with  it 
a  <f>  function. 

We  now  define  fn(%i  •••%„)  by  stating  that  its  value  in  any 
cube  (£  of  Dn,  containing  a  point  of  21,  is  that  of  the  correspond 
ing  0  function.  Since  $  is  linear  in  each  variable,  two  <£'s  belong 
ing  to  adjacent  cubes  have  the  same  values  along  their  common 
points. 

We  show  now  that/n(V)  =f(x)  at  any  point  x  of  51,  or  that 

e>0,       v,         |/  (*)-/»<>)  I  <*     ,     n  >v.  (3 

Let  a)e  <  e/8.  Let  Hltl  be  the  first  set  in  iS^  containing  the  point  #, 
H2ll  the  first  set  of  Ss  lying  in  5Ilti  and  containing  x.  Continuing 
we  get  ^  >  ^  >  ^  £  ...  >  2lete. 

Let  tye  be  the  union  of  the  sets  in  $j  preceding  5Iit  ;  of  the  sets  in 
$2  preceding  2I2l2  and  lying  in  2llti,  and  so  on,  finally  the  sets  of 
Se  preceding  2lcte,  and  lying  in  $He_^  ^^  Their  number  being 
finite,  8=  Dist  (5let<,  ^e)  is  obviously  >  0.  We  may  therefore 
take  v  >  e  so  large  that  cubes  of  Dv  about  the  point  x  lie  wholly 
in  -/>,(»,  if  <  S. 

Consider  now/n(z),  n  >  v,  and  let  us  suppose  first  that  x  is  not 
a  lattice  point  of  Dn.  Let  it  lie  within  the  cell  (£  of  Dn.  Then 
fn(x)  is  a  mean  of  the  values  of 


where  I  is  any  one  of  the  2n  vertices  of  (E,  and  Cnjn  is  the  corre 
sponding  lattice  constant,  which  we  know  is  associated  with  the 
Bet**.. 

We  observe  now  that  each  of  the 

^<3te....  (4 

For  each  set  in  8n  is  a  part  of  some  set  in  any  of  the  preceding 
sequences.  Now  2ln7n  cannot  be  a  part  of  2I1A:,  k  <  ^,  for  none  of 


478  DISCONTINUOUS   FUNCTIONS 

these  points  lie  in  D^x).     Hence  H«yB  is  a  part  of  5114.     For  the 
same  reason  it  is  a  part  of  5l2i2,  etc.,  which  establishes  4). 
Let  now  x'  be  a  point  of  5I7y-J( .     Then 

I  Cnin  ~  C\f  |  <  |  Oa/n  -/(*')      + 


<fi>n +*>.<!     ,     by  2).  (5 

From  this  follows,  since  fn(x)  is  a  mean  of  these  Onjn,  that 

But  now 

I  f  (<r\         f  (r\  I   <    I  f  (r\          f1        I    J-    I    C1  f  ( <r\  (7 

\J   yGJ  ~~Jn\J'S  I  —  \J  \^J         ^njn  |   T    |   ^njn       J»\XJ     •  \  i 

As  x  lies  in  5lete, 

I/ GO  -  °«i,  I  <  /GO  -  C«.  I  +  I  ^,.  -  cm.  I 

<»«+|<|.  (8 

by  2),  5).     From  6),  8)  we  have  3)  for  the  present  case. 

The  case  that  #  is  a  lattice  point  for  some  division  and  hence 
for  all  following,  has  really  been  established  by  the  foregoing 
reasoning. 

481.  1.  Let  f  be  defined  over  the  limited  set  51.  If  for  arbitrary 
a,  5,  the  sets  53  =  («  </<  V)  are  hyper  complete,  then  Class  /<  1. 

For  let  us  effect  a  division  of  norm  e/2  of  (—00,  GO)  as  in 
479,1.  Then  5T=J5U,  where  as  before  5It  =  (mt  < / <  wl+2) . 
But  as  Osc/<e  in  5lt,  and  as  each  5lt  is  hypercomplete  by 
hypothesis,  our  theorem  is  a  corollary  of  480. 

2.  For  /(#!  •••  #m)  t°  t>e  °f  class  <  1  in  the  limited  complete  set 
51,  it  is  necessary  and  sufficient  that  the  sets  (a  </<  £>)  are  hyper- 
complete,  a,  b  being  arbitrary. 

This  follows  from  1  and  479,  2. 

3.  Let  limited  51  be  the  union  of  an  enumerable  set  of  complete  sets 
|5lnJ,  such  that  Cl/<  1  in  each  5In,  Mew  Cl/<  1  in  51. 


FUNCTIONS   OF   CLASS   1  479 

For  by  479,  1,  5(n  is  the  union  of  an  enumerable  set  of  complete 
sets  in  each  of  which  Oscf  <  e.  Thus  51  is  also  such  a  set,  i.e.  an 
l§e  set.  We  now  apply  480,  l. 

4.  If  Class/  <1  in  the  limited  complete  set  51,  its  class  is<~L, 
in  any  complete  part  $8  of  51. 

This  follows  from  479,  l  and  480,  1. 

482.  1.  Let  f(xl  "•  xm)  be  defined  over  the  complete  set  51,  and 
have  only  an  enumerable  set  (£  of  points  of  discontinuity  in  51. 
Then  Class/  =  1  in  51. 

For  the  points  E  of  51  at  which  Osc/  >  e/2  form  a  complete 
part  of  51,  by  462,  3.  But  E,  being  a  part  of  @,  is  enumerable 
and  is  hence  an  (ge  set  by  477,  3.  Let  us  turn  to  23  =  51  —  E.  For 
each  of  its  points  5,  there  exists  a  8  >  0,  such  that  Osc/<  e  in 
the  set  b  of  points  of  $8  lying  in  -A(6).  As  51  is  complete,  so  is  b. 
As  E  is  complete,  there  is  an  enumerable  set  of  these  b,  call  them 
bj,  b2  •••,  such  that  33  =  fbj.  As  51  =  53+  E,  it  is  the  union  of 
an  enumerable  set  of  complete  sets,  in  each  of  which  Osc/  <  e. 
This  is  true  however  small  e>  0  is  taken.  We  apply  now  480,  l. 

2.    We  can  now  construct  functions  of  class  2. 

Example.  Let  fn(x±  •••  xm)  —  1  at  the  rational  points  in  the 
unit  cube  Q,  whose  coordinates  have  denominators  <  n.  Else 
where  let/n  =  0.  Since  fn  has  only  a  finite  number  of  discontinu 
ities  in  O,  Cl/n  =  1  in  Q.  Let  now 


At  a  non-rational  point,  each  fn  =  0,  .-.  /=0.  At  a  rational 
point,  fn  =  1  for  all  n  >  some  s.  Hence  at  such  a  point  /=  1. 
Thus  each  point  of  O  is  a  point  of  discontinuity  and  Disc/=  1. 
Hence  Cl/is  not  1.  As  /  is  the  limit  of  functions  of  class  1,  its 
class  is  2. 

483.  Let  f(x±  •••  #m)  be  continuous  with  respect  to  each  #t,  at  each 
point  of  a  limited  set  51,  each  of  whose  points  is  an  inner  point. 
Then  Class  /<!. 


480  DISCONTINUOUS   FUNCTIONS 

For  let  21  lie  within  a  cube  Q.  Then  A  =  Q  —  H  is  complete. 
We  may  therefore  regard  21  as  a  border  set  of  A ;  that  is,  a  set  of 
non-overlapping  cubes  jqnj.  We  show  now  that  C1/<1  in  any 
one  of  these  cubes  as  q.  To  this  end  we  show  that  the  points  $8m 
of  q  at  which 


m  m 

form  a  complete  set.  For  let  6j,  52  •••  be  points  of  33m,  which  =  ft. 
We  wish  to  show  that  ft  lies  in  23m.  Suppose  first  that  6,,  £>,+1  ••• 
have  all  their  coordinates  except  one,  say  a?,  the  same  as  the  coordi 
nates  of  ft.  Since 

1  1 

w~~  m' 

therefore  -j  -. 

As /is  continuous  in  x1,  and  as  only  the  coordinate  xl  varies  in 
ba+p,  we  have 


Hence  /3  lies  in  53m. 

We  suppose  next  that  68,  68+1  •••  have  all  their  coordinates  the 
same  as  /?  except  two,  say  xl  ,  #2  . 

We  may  place  each  bn  at  the  center  of  an  interval  t  of  length  8, 
parallel  to  the  xl  axis,  such  that 


since  /is  uniformly  continuous  in  a^,  by  I,  352.  These  intervals 
cut  an  ordinate  in  the  a^,  a;2  plane  through  y8,  in  a  set  of  points 
ca+p  which  =  /3.  Then  as  before, 


m 


As  e  is  small  at  pleasure,  ft  lies  in  33m.      In  this  way  we  may 
continue. 

As  Cl/<  1  in  each  qn,  it  is  in  51,  by  481,  3. 


FUNCTIONS  OF  CLASS  1  481 

484.  (Volterra.)  Letf^f^  •••  be  at  most  po  bitwise  discontinuous 
in  the  limited  complete  set  51.  Then  there  exists  a  point  of  51  at 
which  all  thefn  are  continuous. 

For  if  51  contains  an  isolated  point,  the  theorem  is  obviously 
true,  since  every  function  is  continuous  at  an  isolated  point.  Let 
us  therefore  suppose  that  51  is  perfect. 

Let  e1>e2>---=0.     Let  a1   be   a  point  of  continuity  of  /r 

Then  Osc/!  <  e     ,     in  some  5l:  =  F5l(«i)- 

In  5lj  there  is  a  point  b  of  continuity  of  /r  Hence  Osc/j  <  e2 
in  some  F^),  and  we  may  take  b  so  that  F7?(6)<511.  But  in 
1^(6)  there  is  a  point  a2  at  which  /2  is  continuous.  Hence 

OSC/L  <  e2     ,     Osc/2  <  ej     ,     in  some  512  =  F«2(a2), 

and  we  may  take  az  such  that  512  <  5^  .     Similarly  there  exists  a 
point  a3  in  512,  such  that 

e3       ,       OsC/2  <  62       '       °SC/3  <  el       >       in  S0me  ^3=  ^3(^3)' 


and  we  may  take  a3  so  that  5I3  <  512  . 

In  this  way  we  may  continue.  As  the  sets  5ln  are  obviously 
complete,  Dv\y[n\  contains  at  least  one  point  a  of  51.  But  at  this 
point  each/m  is  continuous. 

485.  1.  Let  51  =  ^8  +  £  be  complete,  let  53,  £  be  pantactic  with 
reference  to  51.  Then  there  exists  no  pair  of  functions  f,  g  defined 
over  51,  such  that  if  53  are  the  points  of  discontinuity  of  f  in  51,  then 
53  shall  be  the  points  of  continuity  of  g  in  51. 

This  is  a  corollary  of  Volterra's  theorem.  For  in  any  Ffi(a)  of 
a  point  of  51,  there  are  points  of  53  and  of  (£.  Hence  there  are 
points  of  continuity  of  /and  g.  Hence/,  g  are  at  most  pointwise 
discontinuous  in  51.  Then  by  484,  there  is  a  point  in  51  where/ 
and  g  are  both  continuous,  which  contradicts  the  hypothesis. 

2.  Let  51=  53  +(£  be  complete,  and  let  53,  £  each  be  pantactic  with 
reference  to  51.  If  53  is  hypercomplete,  (£  is  not. 

For  if  53,  @  were  the  union  of  an  enumerable  set  of  complete 
sets,  473  shows  that  there  exists  a  function  /  defined  over  51 
which  has  53  as  its  points  of  discontinuity  ;  and  also  a  function  g 


482  DISCONTINUOUS  FUNCTIONS 

which  has  (£  as  its  points  of  discontinuity.     But  no  such  pair  of 
functions  can  exist  by  1. 

3.  The  non-rational  points  3  in  any  cube   O   cannot  be  hyper- 
complete. 

For  the  rational  points  in  O  are  hypercomplete. 

4.  As  an  application  of  2  we  can  state  : 

The  limited  function  f(xl--xm)  which  is  <  0  at  the  irrational 
points  of  a  cube  G,  and  >  0  at  the  other  points  3  of  £},  cannot  be 
of  class  0  or  1  in  O. 

For  if  Cl/  <  1,  the  points  of  O  where/  >  0  must  form  a  hyper- 
complete  set,  by  479,  4.  But  these  are  the  points  3. 

486.  1.  (Baire.^)  If  the  class  off(^xl"-xm)  is  1  in  the  com 
plete  set  51,  it  is  at  most  pointwise  discontinuous  in  any  complete 

8<H, 

If  Cl/  =  1  in  51,  it  is  <  1  in  any  complete  $  <  51  by  481,  4  ;  we 
may  therefore  take  33  =  51.  Let  a  be  any  point  of  51.  We  shall 
show  that  in  any  V  —  V^a)  there  is  a  point  c  of  continuity  of  /. 
Let  el  >  e2  >  •••  =  0.  Using  the  notation  of  479,  1,  we  saw  that 
the  sets  5lt  =  (wt  </<  mt+2)  are  hypercomplete.  By  473,  we  can 
construct  a  function  </>t(^i  •••  zm),  defined  over  the  w-way  space 
$ftOT  which  is  discontinuous  at  the  points  5ft,  and  continuous  else 
where  in  9?m.  These  functions  c^,  </>2  •••  are  not  all  at  most  point- 
wise  discontinuous  in  V.  For  then,  by  484,  there  exists  in  V  a 
point  of  continuity  #,  common  to  all  the  <£'s.  This  point  b  must 
lie  in  some  5lt,  whose  points  are  points  of  discontinuity  of  $t. 

Let  us  therefore  suppose  that  fa  is  not  at  most  pointwise  dis 
continuous  in  V.  Then  there  exists  a  point  cl  in  V,  and  an  rjl 
such  that  Vl  =  J^C^i)  contains  no  point  of  continuity  of  </>y  . 
Thus  F1<.5ly.  But  in  5Iy  and  hence  in  Fa,  Osc  f<e1.  The 
same  reasoning  shows  that  in  V\  there  exists  a  F^=  F^^),  such 
that  Osc/<  e2  in  F^.  As  51  is  complete,  V^>  V^>  •••  defines  a 
point  c  in  Fat  which  /is  continuous. 


2.    If  the  class  of  f(x^  •••  #m)  is  1  in  the  complete  set  51,  its  points 
of  discontinuity  3)  form  a  set  of  the  first  category. 


FUNCTIONS  OF   CLASS   1  483 

For  by  462,  3,  the  points  £)„  of  3)  at  which  Osc/>  -   form    a 

n 

complete  set.  Each  Dn  is  apantactic,  since  /  is  at  most  pointwise 
discontinuous,  and  £)„  is  complete.  Hence  3)  =  jOn(  is  the  union 
of  an  enumerable  set  of  apantactic  sets,  and  is  therefore  of  the  1° 
category. 

487.  1.  Let  f  be  defined  over  the  limited  complete  set  31.  If 
Class  f  is  not  <  1,  there  exists  a  perfect  set  3)  in  31,  such  that  f  is 
totally  discontinuous  in  3). 

For  if  Cl/  is  not  <1  there  exists,  by  480,  an  e  such  that  for 
this  e,  31  is  not  an  (£e  set.  Let  now  c  be  a  point  of  31  such  that 
the  points  a  of  31  which  lie  within  some  cube  q,  whose  center  is  <?, 
form  an  @€  set.  Let  53  =  {aj,  (£  =  \c\. 

Then  $8  =  (£.  For  obviously  (£  <  53,  since  each  c  is  in  some 
a.  On  the  other  hand,  33  <  (£.  For  any  point  b  of  53  lies  within 
some  q.  Thus  b  is  the  center  of  a  cube  q'  within  q.  Obviously 
the  points  of  31  within  q'  form  an  (ge  set. 

By  Borel's  theorem,  each  point  c  lies  within  an  enumerable  set 
of  cubes  Jcn|,  such  that  each  c  lies  within  some  q.  Thus  the 
points  an  of  31  in  cn,  form  an  (ge  set.  As  (£  =  5an|,  (£  is  an  (5e  set. 

Let  £)  =  31  -  6.  If  3)  were  0,  31  =  S  and  31  would  be  an  (g.  set 
contrary  to  hypothesis.  Thus  3)  >  0. 

3)  ^s  complete.  For  if  Z  were  a  limiting  point  of  3)  in  (£,  Z  must 
lie  in  some  c.  But  every  point  of  31  in  c  is  a  point  of  (£  as  we  saw. 
Thus  I  cannot  lie  in  (£. 

We  show  finally  that  at  any  point  d  of  £), 

Osc/>€,  with  respect  to  £). 

If  not,  Osc/<e  with  respect  to  the  points  b  of  £)  within 
some  cube  q  whose  center  is  d.  Then  b  is  an  (£e  set.  Also  the 
points  e  of  &  in  q  form  an  (5e  set.  Thus  the  points  b  -f  c,  that  is, 
the  points  of  31  in  q  form  an  (5e  set.  Hence  d  belongs  to  (£,  and 
not  to  £).  As  Osc/>e  at  each  point  of  3),  each  point  of  3)  is  a 
point  of  discontinuity  with  respect  to  3).  Thus/  is  totally  discon 
tinuous  in  £). 

This  shows  that  3)  can  .contain  no  isolated  points.  Hence  3)  is 
perfect. 


484  DISCONTINUOUS  FUNCTIONS 

2.    Let  f  be  defined  over  the  limited  complete  set  SI.    .If  f  is  at 
most  pointwise  discontinuous  in  any  perfect  58  <  SI,  its  class  is  <  1 


This  is  a  corollary  of  1.  For  if  Class  /  were  not  0,  or  1,  there 
exists  a  perfect  set  2)  such  that  /is  totally  discontinuous  in  £). 

488.  If  the  class  of  f,  g  <  1  in  the  limited  complete  set  SI,  the  class 
of  their  sum,  difference,  or  product  is  <  1  .  If  f  >  0  in  SI,  the  class 
of  <f> 


For  example,  let  us  consider  the  product  h  =fg.  If  Cl  h  is  not 
<  1,  there  exists  a  perfect  set  £)  in  SI,  as  we  saw  in  487,  l,  such 
that  h  is  totally  discontinuous  in  2).  But/,  #  being  of  class  <,  1, 
are  at  most  pointwise  discontinuous  in  £)  by  486.  Then  by  484, 
there  exists  a  point  of  £)  at  which/,  g  are  both  continuous.  Then 
h  is  continuous  at  this  point,  and  is  therefore  not  totally  discon- 
tinous  in  $). 

Let  us  consider  now  the  quotient  <f>.  If  Cl  <£  is  not  <  1,  0  is 
totally  discontinuous  in  some  perfect  set  $)  in  SI.  But  since  />  0 
in  £),  /  must  also  be  totally  discontinuous  in  £).  This  contradicts 
486. 

489.  1.  Let  F  =  ^f^...,t(xl  •••  #m)  converge  uniformly  in  the  com 
plete  set  SI.  Let  the  class  of  each  termft  be  <  1,  then  Class  J?<  1 
mSI. 

For  setting  as  usual  [117], 

1=1^  +  ^  (1 

there  exists  for  each  e  >  0,  a  fixed  rectangular  cell  72A,  such  that 

|  JA  |  <  e,         as  x  ranges  over  SI.  (2 

As  the  class  of  each  term  in  FK  is  <  1,  Cl  J^  <  1  in  SI.  Hence 
SI  is  an  (ge  set  with  respect  to  FK. 

From  1),  2)  it  follows  that  SI  is  an  (ge  set  with  respect  to  F. 


2.    .Letf  ^  =  II/^...^^  •••  #m)  converge  uniformly  in  the  complete 
set  SI.     /f  the  class  of  eachf^  is  <  1,  then  Cl  ^<  1  in  SI. 


SEMICONTINUOUS  FUNCTIONS  485 


Semicontinuous  Functions 

490.  Let  f(xl  ••-  XM)  be  defined  over  21.     If  a  is  a  point  of  51, 
Max/ in  F"8(a)  exists,  finite  or  infinite,  and  may  be  regarded  as  a 
function  of  8.     When  finite,  it  is  a  monotone  decreasing  function 
of  8.     Thus  its  limit  as  8  =  0  exists,  finite  or  infinite.     We  call 
this  limit  the  maximum  off  at  x=  a,  and  we  denote  it  by 

Max/. 

x=a 

Similar  remarks  apply  to  the  minimum  of /in  Fa(a).  Its  limit, 
finite  or  infinite,  as  8  ==  0,  we  call  the  minimum  of  f  at  x  =  a,  and 
we  denote  it  by 

Min/ 

x=a 

The  maximum  and  minimum  of /in  Fg(a)  niay  be  denoted  by 
Max/    ,     Min/ 

a,  S  a,  S 

Obviously,  Max  (-/)=- Min/, 

x=a  x=a 

Min  (-/)=-  Max/. 

x=a  x=a 

491.  Example  1.  -, 

/O)  =  ±in(-l,  1)     ,     for 
*c 

=  0     ,     forz=0. 
Then  Max/=+sc     ,     Min/=-oo. 

^=0  r=o 

Example  2.  -, 

/(V)  =  sin  -  in  (—  1,  1)     ,     for  x  =£  0 

^c/ 

=  0     ,     for  x  =  0. 
Then  Max/=l     ,     Min/=-l. 

;r=o  x=Q 

Example  3.  /(„)  =  l  in  (_  !,  l)     ,     f or 

=  2     ,     for  x  =  0. 
Then  Max/ =2     .     Min/=l. 

" 


486  DISCONTINUOUS   FUNCTIONS 

We  observe  that  in  Exs.  1  and  2, 

Iim/=Max/    ,     lim/=Min/; 

x=Q  x=Q  x=Q  z=o 

while  in  Ex.  3, 

lim/=  1     ,     and  hence  Max/  >  lim/. 

X=Q  X=Q  X=Q 

Also  lim/  =  Min/. 


Example  4-  -i 

f(x)  =  (z2  +  1)  sin  -  in  (-  1,  1)     ,     for  x*  0 
x 

=  -  2     ,     for  x  =  0. 
Here  Max/=  1     ,     Min/=  -  2, 

x=0  x=0 

lim/=l     ,     lim/==  —  1. 

X=Q  #=0 

Examples.     Let        f^  =  x    ,     for  rational  rr  in  (0,  1) 

=  1     ,     for  irrational  x. 
Here  Max/=l     ,     Min/=0, 

z=0  x=0 

lhn/=l. 

2^=0 

492.    1.    For  M  to  be  the  maximum  of  f  at  x  =  a,  it  is  necessary 
and  sufficient  that 

1°  e  >  0,         8  >  0,        /(z)  <  M  +  e,        for  any  x  in  V8(a)  ; 

2°  there  exists  for  each  e  >  0,  and  in  any  Fg(a),  a  point  a  such 
that 


These  conditions  are  necessary.     For  M  is  the  limit  of  Max/ 
in  Fs(a),  as  B  =  0.     Hence 

e>0,         o>0, 


a,fi 

But  for  any  x  in  Fs(a), 

f(x)  <  Max/. 


SEMICONTINUOUS   FUNCTIONS  487 

Hence  f^  <M+e    ?     x  in  y^ 

which  is  condition  1°. 

As  to  2°,  we  remark  that  for  each  e  >  0,  and  in  any   Fi(a), 
there  is  a  point  a,  such  that 

-e  +  Max/  </(«). 

a,  6 

But  M  <  Max/. 

Hence 


which  is  2°. 

These  conditions  are  sufficient.     For  from  1°  we  have 


a,  8 

and  hence  letting  £  =  0, 


since  e  >  0  is  small  at  pleasure. 
From  2°  we  have 

Max/>  M-e, 

a,  5 

and  hence  letting  S  =  0, 

Max/  >  Jtf.  (2 

x=a 

From  1),  2)  we  have  M=  Max/. 

j^=a 

2.    For  m  to  be  the  minimum  of  f  at  x  =  a,  it  is  necessary  and 
sufficient  that 

1°  e  >  0,         8  >  0,         m  -  e  </O),      for  any  x  in  V&(a)  ; 

2°  that  there  exists  for  each  e  >  0,  and  in  any  VI  (a),  a  point  a 
such  that 

/(«)  <  m  +  e. 

493.    When  Max/  =  /(#),  we  say  /  is  supracontinuous  at  x  =  a. 

x=a 

When  Min/  =  /(a),  we  say  /  is  infracontinuous  at  a.     When/  is 

x=a 

supra  (infra)  continuous  at  each  point  of  51,  we  say  /  is  supra 
(infra)  continuous  in  51.  When  /  is  either  supra  or  infracontinu 
ous  at  a  and  we  do  not  care  to  specify  which,  we  say  it  is  semi- 
continuous  at  a. 


488  DISCONTINUOUS  FUNCTIONS 

The  function  which  is  equal  to  Max  /at  each  point  x  of  51  we 
call  the  maximal  function  of/,  and  denote  it  by  a  dash  above,  viz. 
f(x).  Similarly  the  minimal  f  unction  /(V)  is  defined  as  the  value 
of  Min  /  at  each  point  of  21. 

Obviously  Qsc/=  Max/_  M;n/=  D.sc/ 

x=a  x=a  x=a          -      x—a 

We  call  - 

<*)=/<>)-/<>) 

the  oscillatory  function. 

We  have  at  once  the  theorem  : 

For  f  to  be  continuous  at  x  —  a,  it  is  necessary  and  sufficient  that 

/00=  700  =/(«). 

For  Min  /  <  f(a)  <  Max  /. 

a,  6  a,  8 

Passing  to  the  limit  x  =  a,  we  have 

Min  /</<»  <  Max/, 

x=a  x=a 

or 

/(«)</(«)</(«). 

But  for  /  to  be  continuous  at  x  —  a,  it  is  necessary  and  suffi 
cient  that 

«(V)  =  Osc/=  0. 

x=a 

494.  1.  For  f  to  be  supracontinuous  at  x  =  a,  it  is  necessary  and 
sufficient  that  for  each  e  >  0,  there  exists  a  S  >  0,  such  that 

/O)  <  /O)  +  €     »    for  any  x  in  V^a).  (1 

Similarly  the  condition  for  infracontinuity  is 

f(a)  -  e  <  /(»     ,    for  any  x  in  V^a).  (2 

Let  us  prove  1).  It  is  necessary.  For  when  /is  supracontinu 
ous  at  a, 


Then  by  492,  1, 

€>0     ,     S>0     ,    /(aO</(<0  +  €     ,     for  any  x  in 
which  is  1). 


SEMICONTINUOUS  FUNCTIONS  489 

It  is  sufficient.     For  1)  is  condition  1°  of  492,  l.     The  condition 
2°  is  satisfied,  since  for  a  we  may  take  the  point  a. 

2.    The  maximal  function  f(x)  in  supracontinuous  ;  the  minimal 
function  f(x)  is  infracontinuous,  in  31. 

To  prove  that  /is  supracontinuous  we  use  1,  showing  that 

f(x)  <  /(«)  +  e     ,     for  any  x  in  some  V^d). 
Now  by  492,  l, 

e'  >  0,  8  >  0     ,    f(x)  <  /(a)  +  e'     ,     for  any  x  in  F«(a). 
Thus  if  e'  <  e 

f(x)  <  /(a)  +  e     ,     f  or  any  x  in  F,  (a)      ,     17  =  |. 


3.    jT/ie  swm  (>/  ^wo  supra  (infra)  continuous  functions  in  31  is  a 
supra  (infra)  continuous  function  in  31. 

For  let/,  g  be  supracontinuous  in  31  ;  let/-f  g  =  h.    Then  by  1, 


for  any  a;  in  some  Fs(a)  ;  hence 


This,  by  1,  shows  that  h  is  supracontinuous  at  x=  a. 

4.    If  f(x)  is  supra  (infra)  continuous  at  z  =  a,  g(jz)=—f(%) 
is  infra  (supra)  continuous. 

Let  us  suppose  that  /is  supracontinuous.     Then  by  1, 

/(V)</(a)-|-  e     ,     for  any  x  in  some  Fs(a). 
Hence  -/(«)-,€<-/(*),        ,     . 

g(a)  -  e  <  ^(2:)     ,     for  any  x  in  F«(a). 
Thus  by  1,  #  is  infracontinuous  at  a. 


490  DISCONTINUOUS  FUNCTIONS 

495.  If  /(#!  •••  Xm)  i8  supracontinuous  in  the  limited  complete 
set  51,  the  points  33  of  51  at  which  />  c  an  arbitrary  constant  form  a 
complete  set. 

For  let  f  >  c?  at  6j,  bz  •••  which  ==  b  ;  we  wish  to  show  that  b  lies 
in  $. 

Since/ is  supracontinuous,  by  494,  l, 

/(V)  </(£>)  +  e     ,     for  any  x  in  some  F6(5)=  V. 

But  <?</(&„),  by  hypothesis  ;  and  bn  lies  in  Fi  for  n>  some  m. 
Hence 


*-«</(a). 

As  e  >  0  is  small  at  pleasure, 
and  b  lies  in  33. 

496.    1.    The  oscillatory  function  oy(x)  is  supracontinuous. 
For  by  493,  „(*)=  Max/- Min/ 

=  Max/+Max(-/). 

But  these  two  maximal  functions  are  supracontinuous  by  494,  2. 
Hence  by  494,  3,  their  sum  a>  is  supracontinuous. 

2.  The    oscillatory   function    o>    is    not    necessarily    infracon- 
tinuous,  as  is  shown  by  the  following 

Example.    /=  1   in   (-1,   1),   except  for  z  =  0,   where /=  2. 
Then  co(x)  =  0,  except  at  x  =  0,  where  o»  =  1.     Thus 

Min  &>(>)  =  0     ,     while  o>(0)  =  1. 

Hence  &>(a?)  is  not  infracontinuous  at  x  =  0. 

3.  Let  o>(V)  be  the  oscillatory  function  of  f(xl  •••  xm)  in  51.     For 
f  to  be  at  most  pointwise  discontinuous  in  51,  it  is  necessary  that 
Min  &)  =  0  at  each  point  of  51.     If  51  is  complete,  this  condition  is 
sufficient. 


SEMICONTINUOUS  FUNCTIONS  491 

It  is  necessary.  For  let  a  be  a  point  of  H.  As  /  is  at  most 
pointwise  discontinuous,  there  exists  a  point  of  continuity  in  any 
Ffi(a).  Hence  Min  o>(V)  =  0,  in  F6(a).  Hence  Min  o>(V)  =  0. 

x=a 

It  is  sufficient.     For  let  €1>e2>  •••  =0.      Since  Min  0(2:)  =  0, 

jr=a 

there  exists  in  any  Fs(a)  a  point  al  such  that  &>(«!)  <|e1. 
Hence  o>(V)  <  el  in  some  ^(aj)  <  F6.  In  VSl  there  exists  a  point 
«2  such  that  o>O)  <  e2  in  some  F52(«)  <  F6l,  etc.  Since  21  is  com 
plete  and  since  we  may  let  Sn  =  0, 

V^  >  Ffi2  >  •••  =  a  point  «  of  51, 

at  which  f  is  obviously  continuous.  Thus  in  each  Fs(tf)  is  a  point 
of  continuity  of/.  Hence  /is  at  most  pointwise  discontinuous. 

497.    1.    At  each  point  x  of  31, 

<#>  =  Min  \f(x)  -/(*)},  and  t  =  Min  j/<»  -/(*){ 
=  0. 


Let  us  show  that  $  =  0  at  an  arbitrary  point  a  of  51.     By  494, 
2,  /(V)  is  supracontinuous  ;  hence  by  494,  1, 

f(x)  </(«)  +  e     ,     for  any  a:  in  some  Fs(a)  =  F".  (1 

Also  there  exists  a  point  a  in  Fsuch  that 

_€+/(«)  </(„).  (2 

Also  by  definition 

/(«)  </(«)•  (3 

If  in  1)  we  replace  #  by  a  we  get 

/(«)</(«)  +  e.  (4 

From  2),  3),  4)  we  have 

-e  +/(a)  </(«)  </(«)  </(«)  +  e, 


or 

0  </(«)-/(«)<  2  €. 

As  e  >  0  is  small  at  pleasure,  this  gives 

</><»  =  o. 


492  DISCONTINUOUS  FUNCTIONS 

2.    Iff  is  semicontinuous  in  the  complete  set  51,  it  is  at  most  point- 
wise  discontinuous  in  51. 

'  »CO=/CO-/CO 

=  [/CO  -/CO]  +  [/co  -/CO]    (1 


To  fix  the  ideas  let  /  be  supracontinuous.     Then  <£  ==  0  in  51. 
Hence  1)  gives 

Min  o>(V)  =  Min  ^(z)  =  0,         by  1. 

Thus  by  496,  3,  /  is  at  most  pointwise  discontinuous  in  51. 


CHAPTER   XV 
DERIVATES,   EXTREMES,   VARIATION 

Derivates 

498.  Suppose  we  have  given  a  one-valued  continuous  function 
f(x)  spread  over  an  interval  51  =  (a<6).     We  can  state  various 
properties  which  it  enjoys.     For  example,  it  is  limited,  it  takes 
on  its  extreme  values,  it  is  integrable.     On  the  other  hand,  we 
do  not  know  1°  how  it  oscillates  in  51,  or  2°  if  it  has  a  differ 
ential  coefficient  at  each  point  of  51.     In  this  chapter  we  wish  to 
study  the  behavior  of  continuous  functions  with  reference  to  these 
last  two  properties.     In  Chapters  VIII  and  XI  of  volume  I  this 
subject  was  touched  upon  ;  we  wish  here  to  develop  it  farther. 

499.  In  I,  363,  364,  we  have  defined  the  terms  difference  quo 
tient,  differential  coefficient,  derivative,  right-  and  left-hand  dif 
ferential  coefficients  and  derivatives,  unilateral  differential  coeffi 
cients  and  derivatives.     The  corresponding  symbols  are 

,    /'(a)     , 


Lf(a)     , 

The  unilateral  differential  coefficient  and  derivative  may  be  de 
noted  by 

Uf'(a)     ,     Uf'(x).  (1 

When  .  , 


does  not  exist,  finite  or  infinite,  we  may  introduce  its  upper  and 
lower  limits.     Thus 


A=O 


(2 


always  exist,  finite  or  infinite.     We  call  them  the  upper  and  lower 
differential  coefficients  at  the  point  x  =  a.    The  aggregate  of  values 

493 


494  DERIVATES,   EXTREMES,    VARIATION 

that  2)  take  on  define  the  upper  and  lower  derivatives  of  /(#),  as 
in  I,  363. 

In  a  similar  manner  we  introduce  the  upper  and  lower  right- 
and  left-hand  differential  coefficients  and  derivatives, 

Rf>     ,     Rf     ,    Lf     ,    Lf.  (3 

Thus,  for  example, 


finite  or  infinite.     Cf.  I,  336  seq. 

If  f(x)  is  defined  only  in  51  =  (a  <  /3),  the  points  a,  a  +  A  must 
lie  in  51.  Thus  there  is  no  upper  or  lower  right-hand  differential 
coefficient  at  x  =  fB  ;  also  no  upper  or  lower  left-hand  differential 
coefficient  at  x  =  a.  This  fact  must  be  borne  in  mind.  We  call 
the  functions  3)  derivates  to  distinguish  them  from  the  deriva 
tives  Rf,  Lf.  When  Rf(a)=Ef'(a)i  finite  or  infinite, 
Rf(cC)  exists  also  finite  or  infinite,  and  has  the  same  value.  A 
similar  remark  applies  to  the  left-hand  differential  coefficient. 

To  avoid  such  repetition  as  just  made,  it  is  convenient  to  in 
troduce  the  terms  upper  and  lower  unilateral  differential  coeffi 
cients  and  derivatives,  which  may  be  denoted  by 

Uf>    ,     Uf.  (4 

The  symbol   U  should  of  course  refer  to  the  same  side,  if  it  is 
used  more  than  once  in  an  investigation. 

When  no  ambiguity  can  arise,  we  may  abbreviate  the  symbols 
3),  4)  thus: 

R    ,     R    ,     L    ,    L    ,     U    ,     U. 

The  value  of  one  of  these  derivates  as  R  at  a  point  x  —  a  may 
similarly  be  denoted  by 

5(«). 

The  difference  quotient 


a-b 
may  be  denoted  by 

A(a,  b). 


DERIVATES  495 

1 

Example  1.  /(V)  =  zsin-     ,     x=£  0  in  (—  1,  1) 

=  0     ,     x=0. 

li  sin  - 
Here  f  or  x  =  0,        -^  =  — . —  =  sin  r- 


Hence  - 

"i 

Z/'(0)  = 


Example  2.  f(x)  =  z*  sin  -     ,     a;  ^  0  in  ( -  1, 

x 

=  0     ,     a:  =  0. 

.     1 

A/        n  4 
Here  for  x  =  0     ,     —  =  — 5 — 

Hence 


+  QO          ,        Z/'(0)=:-QO, 

/'(O)  =  +  oo       , 


Example  8.  f(x)  =  a;  sin  -     ,     f  or  0  <  x  <  1 

=  x*  sin  -     ,     for  —  1  <  x  <  0 
x 

=  0     ,     for  x  =  0. 
Here 


500.  1.  Before  taking  up  the  general  theory  it  will  be  well 
for  the  reader  to  have  a  few  examples  in  mind  to  show  him  how 
complicated  matters  may  get.  In  I,  367  seq.,  we  have  exhibited 
functions  which  oscillate  infinitely  often  about  the  points  of  a  set 


496  DERIVATES,   EXTREMES,   VARIATION 

of  the  1°  species,  and  which  may  or  may  not  have  differential  co 
efficients  at  these  points. 

The  following  theorem  enables  us  to  construct  functions  which 
do  not  possess  a  differential  coefficient  at  the  points  of  an  enumer 
able  set. 

2.  Let  @  =  \en\  be  an  enumerable  set  lying  in  the  interval  SI.  For 
each  x  in  SI,  and  en  in  (£,  let  x  —  en  lie  in  an  interval  33  containing 
the  origin.  Let  g(x)  be  continuous  in  33.  Let  g\x)  exist  and  be 
numerically  <_  M  in  33,  except  at  x  =  0,  where  the  difference  quotients 
are  numerically  <.  M.  Let  A  =  San  converge  absolutely.  Then 


is  a  continuous  function  in  SI,  having  a  derivative  in  (£  =  SI  —  G£. 
At  the  points  of  (§,  the  difference  quotient  of  F  behaves  essentially  as 
that  of  g  at  the  origin. 

For  g(x)  being  continuous  in  33,  it  is  numerically  <  some  con 
stant  in  SI.  Thus  F  converges  uniformly  in  SI.  As  each  term 
g(x  —  #n)  is  continuous  in  SI,  F  is  continuous  in  SI. 

Let  us  consider  its  differential  coefficient  at  a  point  x  of  (£. 
Since  g'(x—  en)  exists  and  is  numerically  <  M, 

^'(20=2«n</(*-O     ,     by  156,  2. 
Let  now  x  =  em,  a  point  of  (£, 

W(x)  =  amg(x  -  em)  +  2*a^C*  -  *»)     £*  i  *%  M*$ 

- 


The  summation  in  2*  extends  over  'dl\n=^m.     Hence  by  what 
has  just  been    shown,  G-  has  a  differential  coefficient  at  x  =  em. 

Thus  —  —  behaves  at  x  =  em,  essentially  as  —  at  x  =  0.     Hence 


501.    Example  1.     Let 

^r(V)  =  a#     ,     a:  >  0 

b  <  0  <  a. 

=  bx 


DERIVATES  497 

Then 


is  continuous  in  any  interval  SI,  and  has  a  derivative 

-$r'O-en) 
at  the  points  of  SI  not  in  (£.     At  the  point  em, 

r>  TT/ /„  \  .     >T^*    J-       is  \ 

H±  (x)  =  ama  +  >     —og(em-en), 


Let  &  denote  the  rational  points  in  SI.  The  graph  of  F(x)  is  a 
continuous  curve  having  tangents  at  a  pantactic  set  of  points  ; 
and  at  another  pantactic  set,  viz.  the  set  (S,  angular  points  (I,  366). 

A  simple  example  of  a  g  function  is 


Example  2.    Let  g(x)  =  x2sin-     ,     x  =£  0 

=  0     ,     z=0. 
This  function  has  a  derivative 

#'(z)  =  2zsin--7rcos-     , 

X  X 

=  0     ,     z  =  0. 

Thus  if  2cn  is  an  absolutely  convergent  series,  and  Q?=  \en\  an 
enumerable  set  in  the  interval  31  =  (0,  1), 


is  a  continuous  function  whose  derivative  in  SI  is 


Thus  F  has  a  derivative  which  is  continuous  in  SI  —  (S,  and  at 
the  point  x  =  em 

Disc  F'  =  2  <?m7r, 

since  -'(*)=  2-         Mtf.  451     ' 


498  DERIVATES,   EXTREMES,   VARIATION 

If  (£  is  the  set  of  rational  points  in  31,  the  graph  of  F(x)  is  a 
continuous  curve  having  at  each  point  of  31  a  tangent  which  does 
not  turn  continuously  as  the  point  of  contact  ranges  over  the 
curve;  indeed  the  points  of  abrupt  change  in  the  direction  of  the 
tangent  are  pantactic  in  31. 

Example  3.    Let  g(x)  =  x  sin  log  x2     ,     x  =£  0 

=  0     ,     x=0. 
Then  g '(x)  =  sin  log  x1  +  2  cos  log  x2     ,     x  j=  0. 

At  x  =  0,  ^  =  sin  log  h2 

which  oscillates  infinitely  often  between  ±  1,  as  h  =  A#  =  0.     Let 
(g  =  \en\  denote  the  rational  points  in  an  interval  31.     The  series 

-    *%•        /%P         ^   ^  ein   Inrp  (v  _  p  ^2 

==       /      (  •C    "r,  I    olll    H.^ii    I  Js    "n  I 


satisfies  the  condition  of  our  theorem.     Hence  F(x)  is  a  continu 
ous  function  in  31  which  has  a  derivative  in  31  —  (§.     At  £  =  em, 


Thus  the  graph  of  ^  is  a  continuous  curve  which  has  tangents  at 
a  pantactic  set  of  points  in  31,  and  at  another  pantactic  set  it  has 
neither  right-  nor  left-hand  tangents. 

502.  Weierstrass'  Function.  For  a  long  time  mathematicians 
thought  that  a  continuous  function  of  x  must  have  a  derivative,  at 
least  after  removing  certain  points.  The  examples  just  given 
show  that  these  exceptional  points  may  be  pantactic.  Weierstrass 
called  attention  to  a  continuous  function  which  has  at  no  point  a 
differential  coefficient.  This  celebrated  function  is  defined  by  the 
series 

F  (x)  =  2  an  cos  bnirx  =  cos  TTX  -f-  a  cos  ITTX  +  a2  cos  WTTX  +  -  •  •    (1 

0 

where  0  <  a  <  1  ;  b  is  an  odd  integer  so  chosen  that 

a5l  +     7r.  (2 


DERIVATES  499 

The  series  F  converges  absolutely  and  uniformly  in  any  interval 


Hence  .F  is  a  continuous  function  in  2(.     Let  us  now  consider 
the  series  obtained  by  differentiating  1)  termwise, 

Q(x)  =  -  7r2(«6)nsin  bnirx. 

If  ab  <  1,  this  series  also  converges  absolutely  and  uniformly, 
and  F'(x)  =  <?O), 

by  155,  1.     In  this  case  the  function  has  a  finite  derivative  in  21. 
Let  us  suppose,  however,  that  the  condition  2)  holds.     We  have 


v      ^  ,  c  <«-hA)  -  cos  bn7rx\  =  Qm+  Qm.        (3 

A*  7  A 

Now  Tn_1   n 

§m  =  Vs  —  5  cos  bn7r(x  +  7t)  —  cos  ftn7T2:| 
<*4   A 

0 


»       /*JT+/i 

-  I       sin  bn7rudu. 
^      A    * 

Since 


I    fx+h  I     /*x+h 

I       sin  bn7rudu    <  I  I 


I  <M  <  '    W—-    -' if 

Consider  now  *     n 

§ro  =  2J  ^  jcos  bnrjr(x  +  h)  —  cos  l>nTrx\. 

m     ft 

Up  to  the  present  we  have  taken  h  arbitrary.  Let  us  now 
take  it  as  follows  ;  the  reason  for  this  choice  will  be  evident  in  a 
moment. 

Let  *-*=i.+f., 

where  im  is  the  nearest  integer  to  bmx.     Thus 

-*<£.<!• 

Then  6-(*  +  A)  =  *.  +  f »  +  Ai-  =  .»  +  ij. . 


500  DERIVATES,  EXTREMES,   VARIATION 

We  choose  h  so  that 

Vm  =  £  m  4-  hbm  is  ±  1,  at  pleasure. 

Then  _* 

h  =  ^m      ^m  =  0,  as  m=cc  ; 
om 

moreover  ,     and    „_  -    .    <    . 


This  established,  we  note  that 

cos  bnTr(x  +  h)  =  cos  bn~m7r  -  bm(x  +  h)  =  cos  6n~m(tm  -f-  rjm)7r 
=  cos  (tm  +  ^m)7r     ,     since  6  is  odd 
=  (  —  l)l»+1     ,     since  T;TO  is  odd. 

Also         cos  bn7rx  =  cos  bn~m(tm  +  f  m)?r 


bn~m^m7T. 

Thus 


where  :••;         ««  =  (-i>+'. 

Now  each  5  j  >  0  and  in  particular  the  first  is  >  0.     Thus 

sgn  Qm  =  sgn  e-f  =  sgn  emrjm, 
h 

and  ,  ,xm 

i^i>f=^->iW" 

»          ^m  —  ^m 

Thus  if  2)  holds,  |  ^TO  |  >  |  Qm  |.     Hence  from  3), 

sgn  Q  =  sgn  Qm  =  sgn  ^m?;m, 
and 


Let  now  m  =  QO  .  Since  ?;m  =  ±  1  at  pleasure,  we  can  make 
Q  =  -j-oo,  or  to  —  oo  ,  or  oscillate  between  ±  oo,  without  becoming 
definitely  infinite.  Thus  F  (x)  has  at  no  point  a  finite  or  infinite 
differential  coefficient.  This  does  not  say  that  the  graph  of  F  does 
not  have  tangents;  but  when  they  exist,  they  must  be  cuspidal  tangents. 


DERIVATES  501 

503.    1.     Vblterra's  Function. 

In  the  interval  51  =  (0,  1),  let  <£>  =  \r)l  be  a  Harnack  set  of 
measure  0<A<1.  Let  A  =  |8nj  be  the  associate  set  of  black 
intervals.  In  each  of  the  intervals  £n  =  (a  <  /8),  we  define  an 
auxiliary  function  fn  as  follows  : 

/„(*)  =  (*-  «)2  sin-          ,     in  («*,  7),  (1 


where  7  is  the  largest  value  of  x  corresponding  to  a  maximum  of 
the  function  on  the  right  of  1),  such  that  7  lies  to  the  left  of  the 
middle  point  /z  of  Sn.  If  the  value  of  /„(#)  at  7  is  g,  we  now 


Finally  fn(a)=  0.  This  defines  fn  (x)  for  one  half  of  the  inter 
val  Sn.  We  define  /„(#)  for  the  other  half  of  Sn  by  saying  that  if 
x<x'  are  two  points  of  Sn  at  equal  distances  from  the  middle 
point  ft  then  . 


With  Volterra  we  now  define  a  function  f(x)  in  51  as  follows: 
f(x)  =  fn(x)     ,     inSn     ,     7i  =  l,2,... 

=  0     ,     in  $. 

Obviously/^)  is  continuous  in  51. 
At  a  point  x  of  51  not  in  &,f(x)  behaves  as 

1  1 

2  x  sin  --  cos-, 
x  x 

as  is  seen  from  1).  Thus  as  x  converges  in  8n  toward  one  of  its 
end  points  a,  /3,  we  see  that  f(x)  oscillates  infinitely  often  be 
tween  limits  which  =  ±  1.  Thus 


similar  limits  exist  for  the  points  $. 

Let  us  now  consider  the  differential  coefficient  at  a  point  77  of 
&.     We  have 

M  =  /^  +  *)-/W  =  /0>  +  *)    ,   8ince/(,)=0. 


502  DERIVATES,   EXTREMES,    VARIATION 

If  rj  +  k  is  a  point  of  §,/(??  +  &)  =  0.  If  not,  rj  -f  k  lies  in  some 
interval  Sm .  Let  a;  =  e  be  the  end  point  of  8m  nearest  rj  +  k. 
Then 


1*1 

Thus  /'(??)=  0.  Hence  Volterra's  f  unction  f(x)  has  a  differen 
tial  coefficient  at  each  point  of  51;  moreover/' (x)  is  limited  in  51. 
Each  point  rj  of  &  is  a  point  of  discontinuity  of/' (V),  and 

Disc/  <»  >  2. 

Hence/' (V)  is  not  72-integrable,  as  &  =  h>0. 

We  have  seen,  in  I,  549,  that  not  every  limited  J2-integrable 
function  has  a  primitive.  Volterra's  function  illustrates  con 
versely  the  remarkable  fact  that  Not  every  limited  derivative  is 
R-integrable. 

2.  It  is  easy  to  show,  however,  that  The  derivative  of  Volterra's 
function  is  L-integrable. 

For  let  51A  denote  the  points  of  51  at  which  f  (x)  >  X.  Then 
when  X>l/m,  m  =  1,  2,  •••  51A  consists  of  an  enumerable  set  of 
intervals.  Hence  in  this  case  51A  is  measurable.  Hence  5(A,  X>0, 
is  measurable.  Now  51  ,  X>0,  differs  from  the  foregoing  by  add 
ing  the  points  3n  in  ea°h  &n  at  which/' (x)  —  0,  and  the  points  £>. 
But  each  3n  is  enumerable,  and  hence  a  null  set,  and  §  is  measur 
able,  as  it  is  perfect.  Thus  51A,  X>0,  is  measurable.  In  the 
same  way  we  see  51A  is  measurable  when  X  is  negative.  Thus  51A 
is  measurable  for  any  X,  and  hence  .L-integrable. 

504.  1.  We  turn  now  to  general  considerations  and  begin  by 
considering  the  upper  and  lower  limits  of  the  sum,  difference,  prod 
uct,  and  quotient  of  two  functions  at  a  point  x  =  a. 

Let  us  note  first  the  following  theorem  : 

Letf(xl  -••  XM)  be  limited  or  not  in  51  which  has  x  =  a  as  a  limiting 
point.  Let  <£fi  =  Max/  (f>&  —  Min/m  Ffi*(a).  Then 


This  follows  at  once  from  I,  338. 


DERIVATES  503 

2.    Letf(x^  "•  xm~),  g(x^  -•  xm)  be  limited  or  not  in  21  which  has 
x  =  a  as  limiting  point. 

Let  limf=a     ,     limg  =  0 

\imf=A    ,     Km  g  =  B 
as  x=  a.      Then,  these  limits  being  finite, 

,  (1 


«  -  B  <  Hm  (/  -  g)  <  A  -  0.  (2 

For  in  any  F^*(a), 
Min  /  +  Min  g  <  Min  (/  -f  y)  <  Max  (/+#)<  Max  /  +  Max  g. 

Letting  S  =  0,  we  get  1). 
Also  in 


Min  /  —  Max  g  <  Min  (/  —  g)  <  Max  (/  —  g)  <  Max  /—  Min  g. 

Letting  8  =  0,  we  get  2). 

3*    If 


a/3  <  lim/#<  AS.  (3 

If 


(4 

/O)>Q     ,     ^)>*>0, 

l^^|-  (5 

a<Q<A     ,         2;>^>0, 


The  relations  3),  4),  5),  6)  may  be  proved  as  in  2.     For  exam 
ple,  to  prove  5),  we  observe  that  in  Fi*(«), 


g  g      Min  g 


504  DERIVATES,   EXTREMES,   VARIATION 

5.                              «  +  £<lim(/  +  0)<a  +  £.  (7 

a  +  Jg<Ihn~(/  +  #)  <.!  +  £.  (8 

a  -.£<  lim  (/-#)<«-£.  (9 

A-£<Km(f-g)<A-0.  (10 

J/  /O)>o   ,    <?(*)>  o, 

• 

a/3  <  limfg  <  *B,  (11 

(12 


(13 


6.    T/"  lira/  exists, 

=  lira  /  +  lira  #,  (15 

m^.  (16 


If  g(x)  >  &  >  0, 


11  m  ^  exists, 

Baifl  (17 


lim5r.  (18 

/(»)  >  0,  ^r(^)  >  0.     ie^  lim  ^  ftw*«.      Then 

.  lim  ^,  (19 


lim  fg  —  lira  /  •  lim  g.  (20 

g(x)  >  k  >  0, 

lim  //^  =  lim  //lim  ^,  (21 

Em  f/g  =  En  //lim  #.  (22 

505.  The  preceding  results  can  be  used  to  obtain  relations  be 
tween  the  derivates  of  the  sum,  difference,  product,  and  quotient 
of  two  functions  as  in  I,  373  seq. 


DERIVATES  505 


1.    Let  w2;=tt+va.     Tnen 


Aw  _  Aw      Av  ,-, 

Az      Az      A#  ' 

Thus  from  504,  1),  we  get  the  theorem: 

Uu'  +  v'U<Uw'<  Uu'  +  W.  (2 

7/  M  has  a  unilateral  derivative  Uu', 

Uw'  =  Uu1  +  Uv',  (3 

Uw'  =  CTw'  +  Uv'.  (4 

We  get  3),  4)  from  1),  using  504,  15),  16). 

2.   In  the  interval  51,  w,  v  arg  continuous,  u  is  monotone  increasing, 
v  is  >  0,  and  v'  exists.      Then,  if  w  =  wv, 


Uw1  =uv'  +vUuf.  (2 

For  from  A^  A  A^ 

—  -  =  (M  +  AM)  —  -h  v  —  , 

A^  Ao:         Ao: 

wehave 


/  ,      rri.        w 
=  wv   -|-  v  U  lim  — 

—  Aa: 

which  gives  1).     Similarly  we  establish  2). 

506.    1.    We  show  now  how  we  may  generalize  the  Law  of  the 
Mean,  I,  393. 

Let  f(x)  be  continuous  in  2I=(a<£>).     Let  m,  M  be  the  mini 
mum  and  maximum  of  one  of  the  four  derivates  of  f  in  51.      Then  for 


—  a 


To  fix  the  ideas  let  us  take  Rf'(x)  as  our  derivate.     Suppose 
now  there  exists  a  pair  of  points  a</3  in  SI,  such  that 

/(«>=  M  +e     ,     e>0. 


506  DERIVATES,    EXTREMES,   VARIATION 

We  introduce  the  auxiliary  function 

</>(*)  =/<X>-(^+<0*,  (2 

where  0<c<e  =  c+S. 

Then        -K/3)  -  »(«)  =  /Q8)  -/(«)      (  Jf  ;    .  _  ^ 
(3  —  a  /3  —  a 

Henoe 


Consider  now  the  equation 

<K/3)  -<£(*)  =  >?• 

It  is  satisfied  for  x  =  a.  If  it  is  satisfied  for  any  other  x  in  the 
interval  (a/3),  there  is  a  last  point,  say  x  =  7,  where  it  is  satisfied, 
by  458,  3. 

Thus  for  *>  7,  <K*0  is  >(/>(<*)• 

Hence 


(3 

Now  from  2)  we  have 


Hence  M  is  not  the  maximum  of  Rf'(x)  in  51.  Similarly  the 
other  half  of  1)  is  established.  The  case  that  m  or  M  is  infinite 
is  obviously  true. 

2.  Letf(x)  be  defined  over  51  =  (#  <  b).  Let  a1  <  «2  <  •••  <  an  lie 
in  21.  Let  m  and  M  denote  the  minimum  and  maximum  of  the  dif 
ference  quotients 

A(ara2)     ,     A(a2,  aB)     ,     •••  A(an_1,  aj. 
Then  m<^^an)<M.  (1 

For  let  us  first  take  three  points  a  <  @  <  7  in  2(.  We  have  iden 
tically  *  a  _ 

7). 


Now  the  coefficients  of  A  on  the  right  lie  between  0  and  1. 
Hence  1)  is  true  in  this  case.     The  general  case  is  now  obvious. 


DERIVATES  507 

507.    1.   Let  f(x)  be  continuous  in  H  =  (a  <  6).      The  four  deri- 
vates  off  have  the  same  extremes  in  21. 

To  fix  the  ideas  let 

Min  L  =  m     ,     Min  R  =  n,      in  21. 

We  wish  to  show  that  m  =  p.     To  this  end  we  first  show  that 


For  there  exists  an  a  in  21,  such  that 

L(a)  <  m  +  e. 
There  exists  therefore  a  0  <  a  in  21,  such  that 


a  —  /3 
Now  by  506,  l, 

ft  =  Min  R<q. 

Hence  ^  <  w, 

as  e>0  is  small  at  pleasure. 

TFe  s^o^  wow  ^Aa^  m<  u,  (2 

For  there  exists  an  a  in  H,  such  that 

R(a)  <  fji  +  €. 
There  exists  therefore  a  /3  >  «  in  21,  such  that 


a—  /3 

Thus  by  506,  l, 

m=  Min     ^ 

Hence  as  before  m<p.     From  1),  2)  we  have  m  =  /i. 

2.  In  499,  we  emphasized  the  fact  that  the  left-hand  derivates 
are  not  defined  at  the  left-hand  end  point  of  an  interval,  and  the 
right-hand  derivates  at  the  right-hand  end  point  of  an  interval 
for  which  we  are  considering  the  values  of  a  function.  The  fol 
lowing  example  shows  that  our  theorems  may  be  at  fault  if  this 
fact  is  overlooked. 


508  DERIVATES,  EXTREMES,   VARIATION 

Example.     Let/(V)  =  j  x  \. 

If  we  restrict  x  to  lie  in  21  =  (0, 1),  the  four  derivates  =  1  when 
they  are  defined.  Thus  the  theorem  1  holds  in  this  case.  If, 
however,  we  regarded  the  left-hand  derivates  as  denned  at  x  =  0, 
and  to  have  the  value 

i/'(0)  =  -  1, 

as  they  would  have  if  we  considered  values  of  /  to  the  left  of  21, 
the  theorem  1  would  no  longer  be  true. 

For  then  Min  £  =  -  1     ,     Min  ]R  =  +  1, 

and  the  four  derivates  do  not  have  the  same  minimum  in  SI. 

3.  Let  f  (x)  be  continuous  about  the  point  x=  c.     If  one  of  its 
four  derivates  is  continuous  at  x  =  c,  all  the  derivates  defined  at  this 
point  are  continuous,  and  all  are  equal. 

For  their  extremes  in  any  Fs(tf)  are  the  same.  If  now  R  is 
continuous  at  x  =  c, 

R(c)  -  e  <  R(x)  <  R(c)  +  e, 
for  any  x  in  some  F5(c). 

4.  Let  f(x)  be  continuous  about  the  point  x  =  c.     If  one  of  its 
four  derivates  is  continuous  at  x  =  c,  the  derivative  exists  at  this 
point. 

This  follows  at  once  from  3. 

.Remark.  We  must  guard  against  supposing  that  the  derivative 
is  continuous  at  x  =  c,  or  even  exists  in  the  vicinity  of  this  point. 

Example.     Let  F(x)  be  as  in  501,  Ex.  1.     Let 


21  =  (0,  1)  and  <g  =  |  - 
Let 

Then  RH'(x)  =  2  ^(a;)  +  x*RF'(x), 

LH'(x)  =  2  xF(x)  +  x*LF'(x~). 

Obviously   both    725"'    and   1/5'    are    continuous   at    x  =  0   and 
5'(0)  =  0.     But  H'  does  not  exist  at  the  points  of  (g,  and  lience 


DERIVATES  509 

does  not  exist  in  any  vicinity  (0,  8)  of  the  origin,  however  small 
S  >  0  is  taken. 

5.  If  one  of  the  derivates  of  the  continuous  function  f(x)  is 
continuous  in  an  interval  El,  the  derivative  fr(&)  exists,  and  is  con 
tinuous  in  El. 

This  follows  from  3. 

6.  If  one  of  the  four  derivates  of  the  continuous  function  f  \x)  is 
=  0  in  an  interval  El,  f(x)  =  const  in  El. 

This  follows  from  3. 

508.    1.    If  one  of  the  derivates  of  the  continuous  function  f(x)  is 
>  0  in  El  =  (a  <  £>),  f(x)  is  monotone  increasing  in  El. 

For  then  m  =  Min  Rf  >  0,  in  (a  <  z).     Thus  by  506,  i, 


2.  If  one  of  the  derivates  of  the  continuous  function  f(x)  is  >_  0 
in  El,  f(%)  is  monotone  decreasing. 

3.  If  one  of  the  derivates  of  the  continuous  function  f(x)  is  >  0 
in  El,  ivithout  being  constantly  0  in  any  little  interval  of  El,  f(x)  is 
an  increasing  function  in  El.     Similarly  f  is  a  decreasing  function 
in  El,  if  one  of  the  derivates  is  <^  0,  without  being  constantly  0  in  any 
little  interval  of  El. 

The  proof  is  analogous  to  I,  403. 

509.  1.  Letf(x)  be  continuous  in  the  interval  El,  and  have  a  deriv 
ative,  finite  or  infinite,  within  El.  Then  the  points  where  the  deriva 
tive  is  finite  form  a  pantactic  set  in  El. 

For  let  a  <  ft  be  two  points  of  El.  Then  by  the  Law  of  the 
Mean, 


—  a 


As  the  right  side  has  a  definite  value,  the  left  side  must  have. 
Thus  in  any  interval  (a,  ft)  in  El,  there  is  a  point  7  where  the 
differential  coefficient  is  finite. 


510  DERIVATES,   EXTREMES,   VARIATION 

2.    Let  f(x)   be   continuous   in   the  interval  2l  =  O<6).      Then 
Uf  (x)  cannot  be  constantly  -f  oo,  or  constantly  —  oo  in  51. 
For  consider 


which  is  continuous,  and  vanishes  for  x  =  a,  x  =  b.  We  observe 
that  <£O)  differs  from  f(x)  only  by  a  linear  function.  If  now 
£/f'(V)=-f-cc  constantly,  obviously  U<f>'(x)  =  +  oo  also.  Thus  </> 
is  a  univariant  function  in  51.  This  is  not  possible,  since  <£  has 
the  same  value  at  a  and  b. 

3.    ie£  /(z)  fo  continuous  in  51  =  (a  <  6),  awe?  Aave  a  derivative, 
finite  or  infinite,  in  51=  (a*,  6). 


For  the  Law  of  the  Mean  holds,  hence 


A 
Letting  now  A  =  0,  we  get  the  theorem. 

Remark.  This  theorem  answers  the  question  :  Can  a  continu 
ous  curve  have  a  vertical  tangent  at  a  point  x  =  a,  if  the  deriva 
tives  remain  <  M  in  V*(a)  ?  The  answer  is,  No. 

4.  Let  f(x)  be  continuous  in  5t  =  (a  <  5),  and  have  a  derivative, 
finite  or  infinite,  in  &*  =  («*,  b).  Iff  (a)  exists,  finite  or  infinite, 
there  exists  a  sequence  «j  >  «2  >  •  •  •  =  a  in  51,  such  that 

/'(«)  =  lim/'(«n)-  (1 

»=» 

For  /(a+AWfq),  ,     „<„,<,  +  ,.  (2 


Let  now  A  range  over  ^  >  A2  >  •••  =  0.  If  we  set  «n=  «//n  ,  the 
relation  1)  follows  at  once  from  2),  since  /'(a)  exists  by 
hypothesis. 

510.  1.  A  right-hand  derivate  of  a  continuous  function  f(x) 
cannot  have  a  discontinuity  of  the  1°  kind  on  the  right.  A  similar 
statement  holds  for  the  other  derivates. 


DERIVATES  511 

For  let  R(x}  be  one  of  the  right-hand  derivates.  It  it  has  a 
discontinuity  of  the  1°  kind  on  the  right  at  x  —  a,  there  exists  a 
number  I  such  that 

/  —e<_R(x)<^  I  -f  e     ,     in  some  (a  <  a  -f  S)  . 
Then  by  50G,  1, 


h 
Hence  R(a)=l, 

and  R(jc)  is  continuous  on  the  right  at  x  =  a,  which  is  contrary 
to  hypothesis. 

2.  It  can,  however,  have  a  discontinuity  of  the  1°  kind  on  the 
left,  as  is  shown  by  the  following 

Example.         Let/(ar)  =  |  x  =  +  Vx2     ,     in2I  =  (-l,l). 
Here  E(x)  =  +  1     ,     f  or  x  >  0  in  21 

=  -  1     ,     for  x  <  0. 

Thus  at  x  =  0,  R  is  continuous  on  the  right,  but  has  a  discon 
tinuity  of  the  1°  kind  on  the  left. 

3.  Let  f(x)   be  continuous  in  31  =  («,  5),  and  have  a  derivative, 
finite  or  infinite,  in  H*  =(a*,  £*).      Then  the  discontinuities  of  f  (x) 
in  51,  if  any  exist,  must  be  of  the  second  kind. 

This  follows  from  1. 

Example.  /0c)  =  aa8inl      ,     for  x*  0  in  51  =  (0,  1) 

=  0     ,     for  x  =  0. 

Then  -,  -, 

f(x)  =  2  a:  sin  -  -  cos  -      ,     x=^0 
x  x 

=  0     ,     a?=0. 
The  discontinuity  of  /'(#)  at  x  =  0,  is  in  fact  of  the  2°  kind. 

4.  Let  f(x)  be  continuous  in  2l  =  (a<6),  except  at  x=  a,  which 
is  a  point  of  discontinuity  of  the  2°  kind.     Let  f  (x)  exist,  finite  or 
infinite,  in  (a*,  6).      Then  x  =  a  is  a  point  of  infinite  discontinuity 
*//'(*> 


512  DERIVATES,   EXTREMES,   VARIATION 

For  if 

p  =  R  lim/  O)     ,     q  =  R  lim/  (», 

x==a  *=a 

there  exists  a  sequence  of  points  «1>«2  >•••=«,  such  that 
/(an)=jt>;  and  another  sequence  /^  >y£2  >  •••  =  «,  such  that 
/(/3n)  =  9.  We  may  suppose 

«n>/3»     ,     oran<^n     ,     rc=l,  2,  ... 
Then  the  Law  of  the  Mean  gives 


where  7n  lies  between  «n,  /3n.     Now  the  numerator  =p  —  q,  while 
the  denominator   =  0.     Hence  Qn  =  +  oo  ,  or  —  oo  ,  as  we  choose. 

5.  Let  f  (a?)  have  a  finite  unilateral  differential  coefficient  U  at 
each  point  of  the  interval  31.  Then  U  is  at  most  pointwise  discon 
tinuous  in  31. 

For  by  474,  3,  U  is  a  function  of  class  1.  Hence,  by  486,  l,  it  is 
at  most  pointwise  discontinuous  in  31. 

511.  Let  f  (x)  be  continuous  in  the  interval  (a  <  £»).  Let  R(x) 
denote  one  of  the  right-hand  derivates  of  f(x).  If  R  is  not  con 
tinuous  on  the  right  at  a,  then 


Q/JnPYP 

I  =  R  lim  R(x)     ,     m  —  R  lim  R(x)     ,     x  =  a. 

To  fix  the  ideas  let  R  be  the  upper  right-hand  derivate.     Let  us 
suppose  that  a  =  Rf'(a)  were  >m.     Let  us  choose  77,  and  c  such 

that 

<a.  (2 


We  introduce  the  auxiliary  function 

<£O)=  cx-f(x). 
1  )  =  c-3f'(x).         (3 


Now  if  8  >  0  is  sufficiently  small, 

Rf'(x)<m  +  r?     ,     for  any  x  in  31*  =  (a*,  a  +  8). 


DERIVATES  513 

Thus  2),  3),  show  that 

R<t>'(x)>(T     ,     <r>0. 
Hence  <$>(x)  is  an  increasing  function  in  51*.     But,  on  the  other 

hand'  4/"  oo  =£/"(«), 

since  a  >  m.     Hence 

'a=c  -  «<  0. 


Hence  <j>  is  a  decreasing  function  at  x  =  a.     This  is  impossible 
since  </>  is  continuous  at  a.     Thus  a<^m. 
Similarly  we  may  show  that  I  <  a. 

512.  1.  Let  f(x)  be  continuous  in  51  =  (a  <  £>),  and  have  a 
derivative,  finite  or  infinite.  //"«=/'(«),  £=/'(£),  then  f  (x) 
takes  on  all  values  between  a,  yS,  as  a:  ranges  over  51. 

For  let  «  <  7  <  /3,  and  let 


h>0. 


We  can  take  h  so  small  that 

<?O,  A)<7     ,     and 
Now  $(6,  -»).  Q(b-h,h). 

Hence  ^7       z,    IN  . 

§(6  -h,h)>  7. 

If  now  we  fix  A,  ()  (#,  ^)  is  a  continuous  function  of  #.  As  Q 
is  <  7,  for  x  =  a,  and  >  7,  for  z  =  b  —  h,  it  takes  on  the  value  7 
for  some  a;,  say  for  #  =  £,  between  a,  b  —  h.  Thus 


But  by  the  Law  of  the  Mean, 

<K6  *)= 

where  ,       , 

«<f<^<?  +  ^<^. 

Thus/f  (x)  =  7,  at  x  =  77  in  51. 

2.  ief  /(#)  3e  continuous  in  the  interval  51,  awe?  admit  a  deriva 
tive,  finite  or  infinite.  If  /'(x)  =  0  in  51,  except  possibly  at  an 
enumerable  set  (£,  ^£71  /'  =  0  a/so  t'w  (S. 


514  DER1VATES,   EXTREMES,   VARIATION 

For  if  /'(«)  =  0,  and  /'(£)  =  b  *  0,  then  f  (x)  ranges  over  all 
values  in  (0,  b),  as  x  passes  from  a  to  ft.  But  this  set  of  values 
has  the  cardinal  number  c.  Hence  there  is  a  set  of  values  in 
(a,  ft)  whose  cardinal  number  is  c,  where  f'(x)  =£  0.  This  is 
contrary  to  the  hypothesis. 

3.  Let  f(x),  g(x)  be  continuous  and  have  derivatives,  finite  or 
infinite,  in  the  interval  51.  //  in  51  there  is  an  a  for  which 

/'«>  </(<*)' 
and  a  ft  for  which 

then  there  is  a  7  for  which 


provided  gw=/(20 

has  a  derivative,  finite  or  infinite. 

For  by  hypothesis 

8'(«)>0     , 

Hence  by  1  there  is  a  point  where  8'  =  0. 

513.  1.  If  one  of  the  four  derivates  of  the  continuous  function 
f(x)  is  limited  in  the  interval  51,  all  four  are,  and  they,  have  the 
same  upper  and  lower  R-integrals. 

The  first  part  of  the  theorem  is  obvious  from  507,  1.  Let  us 
effect  a  division  of  51  of  norm  d.  Then 


Cli  =  lim  2M&     ,     M,  =  Max  ^t  in  d,. 

J%  <M) 

But  the  maximum  of  the  three  other  derivates  in  d,  is  also  M,  by 
507,  1.     Hence  the  last  part  of  the  theorem. 

2.    Let  f(x)  be  continuous  and  have  a  limited  unilateral  derivate 
m=&.     Then 


f  *&**</<?)  -/(«)  < 

J.a 

For  let  a  <  al  «*2  <  •••  <  b  determine  a  division  of  51,  of  norm  d. 


DERIVATES  515 

Then  by  506,  i, 


in  the  interval  (am,  am+1)  =  dm. 
Hence 

2dm  Min  -B<6    -«   <  2      Max  ^. 


Letting  <#=  0,  we  get  1). 

3.    If  f(x)  is  continuous,  and  Uf  is  limited  and  R-integrable  in 


JTI7  = 

514.     1.    Letf(x)  be  limited  in  51  =  (a  <  5), 
F(x)=   ffdx     ,      a<2:< 

«/a 


67  lira  /<  Z/JP'(M)  <  ^  lira/,  (1 

*=«  «=M 

/br  a?i^  u  within  51. 

To  fix  the  ideas  let  us  take  a  right-hand  derivate  atx=u.    Then 

£u+k 
fdx  <  h  Max  /    ,     in  (11  *,  u  +  A),  7i  >  0. 

Thus 

Letting  h  =  0,  we  get 


x=u  *=u    ' 

which  is  1)  for  this  case. 

2.    Let  f(x)  be  limited  in  the  interval  51  =  (a  <  6).     /f/O  +  0) 


R  derivative  Cfdx  =  f(x  +  0)  ; 

*/a 

and  iff(x  —  0)  exists,         a<x<b 

L  derivative  I  fdx  =/(#  —  0). 

•Ja 


516  DERIVATES,   EXTREMES,   VARIATION 

3.    Let  f(x)  be  limited  and  R-integrable  in  31  =(«<#).      The 
points  where 

F(x=        dx     ,     a<x<b 


does  not  have  a  differential  coefficient  in  tyi/orm  a  null  set. 
For  F<x)  =/O)        by  I,  537,  1, 

when/  is  continuous  at  x.     But  by  462,  6,  the  points  where/  is 
not  continuous  form  a  null  set*. 

515.    In  I,  400,  we  proved  the  theorem  : 

Let  f(x)  be  continuous  in  31  =  (a  <  £>),  and  let  its  derivative 
=  0  within  31.  Then  /is  a  constant  in  31.  This  theorem  we  have' 
extended  in  507,  6,  to  a  derivate  of  f(x).  It  can  be  extended  still 
farther  as  follows  : 

1.  (L.  Scheefer}.  If  f(x)  is  continuous  in  31  =  (a<  6),  and  if 
one  of  its  derivates  =  0  in  31  except  possibly  at  the  points  of  an 
enumerable  set  (g,  then  f  =  constant  in  31. 

If  /is  a  constant,  the  theorem  is  of  course  true.  We  show  that 
the  contrary  case  leads  to  an  absurdity,  by  showing  that  Card  (5 
would  =  c,  the  cardinal  number  of  an  interval. 

For  if  /  is  not  a  constant,  there  is  a  point  c  in  31  where 
p=f(c)—f(a)  is  =#=0.  To  fix  the  ideas  let  jt?>0;  also  let  us 
suppose  the  given  derivate  is  R  =  Rf'(x). 

Let  g(x,f)=f(x)-f<ji)-t(x-a)     ,     t>0. 

Obviously    g  \  is  the  distance/  is  above  or  below  the  secant  line, 

y  =  t(x-  «)+/(«). 
Thus  in  particular  for  any  £, 

g(a,  £)=0     ,     g(c>t)  =  p-t(c-a). 
Let  q  >  0  be  an  arbitrary  but  fixed  number  <  p.     Then 
g(c,  t)-q=p  -q-t(c-a) 


if  t  <  T,  where 

T= 

c—a 


DERIVATES  517 

Hence 

g(c,  0  >  q 

for  any  t  in  the  interval  £  =  (T,  T),  0  <  T  <  T7.      We  note  that 

Card  £  =  c. 

Since  for  any  £  in  £,  #(a,  £)  =  0,  and  g(c,  t)  >  q,  let  x  =  et  be 
the  maximum  of  the  points  <  c  where  g(x,  t)  =  q.  Then  e  <  <?, 
and  for  any  A  such  that  e  +  h  lies  in  (e,  c), 


Hence 


Thus  for  any  £  in  £,  et  lies  in  (g.  As  t  ranges  over  !£,  let  0* 
range  over  (^  <  (g.  To  each  point  e  of  (^  corresponds  but  one 
point  t  of  X.  For 

0  =g(e,  f)  -  g(e,  *')  =  («  -  ^')(«  ~  «)• 
Hence  . 

f  =  r     ,     as  e  >  a. 

Thus  Card  £  =  Card  @x  <  Card  <g, 

which  is  absurd. 

2.  Let  f  (x)  be  continuous  in  5(  =  (a<5).  Let  §  denote  the 
points  of  51  wAere  owe  o/  tfAe  derivates  has  one  sign.  If  £  exists, 

Card  (E  =  c,  ZAtf  cardinal  number  of  the  continuum. 

The  proof  is  entirely  similar  to  that  in  1.  For  let  c  be  a  point 
of  (£.  Then  there  exists  a  d  >  c  such  that 


We  now  introduce  the  function 

£(s»0=/(*)-/(<0-*<>-<0    ,    *>o, 

and  reason  on  this  as  we  did  on  the  corresponding  g  in  1,  using 
here  the  interval  (c,  c?)  instead  of  (a,  5).     We  get 

Card  ^  =  Card  £  =  c. 

3.  Letf(oi),  g(x)  be  continuous  in  the  interval  21.  Ze£  a  jt?az>  of 
corresponding  derivates  as  Rf,  Rg'  be  finite  and  equal,  except  pos 
sibly  at  an  enumerable  set  (g.  Then  f  —  g  +  C,  in  21,  where  C  is  a 
constant. 


518  DER1VATES,   EXTREMES,   VARIATION 

For  let  ^=f_g     f     ^_/B 

Then  in  A  =  %-& 

R(f>f  >  Rf-Rg'  =  o    ,    Jfy'  >  o. 


But  if  R(f>'  <  0  at  one  point  in  21,  it  is  <  0  at  a  set  of  points  33 
whose  cardinal  number  is  c.  But  $8  lies  in  (g.  Hence  R<f>  is 
never  <  0,  in  21.  The  same  holds  for  ty.  Hence,  by  508,  </>  and 
i/r  are  both  monotone  increasing.  This  is  impossible  unless 
$  ==  a  constant. 

516.  The  preceding  theorem  states  that  the  continuous  function 
/(#)  in  the  interval  21  is  known  in  21,  aside  from  a  constant,  when 
/'  (x)  is  finite  and  known  in  21,  aside  from  an  enumerable  set. 

Thus  f(x)  is  known  in  21  when  /'  is  finite  and  known  at  each 
irrational  point  of  21. 

This  is  not  the  case  when/7  is  finite  and  known  at  each  rational 
point  only  in  21. 

For  the  rational  points  in  21  being  enumerable,  let  them  be 

PI*  »2'  rs'~  0- 

Let  z  =  z1  +  /2+z3+... 

be  a  positive  term  series  whose  sum  I  is  <  21.  Let  us  place  rx 
within  an  interval  ^  of  length  <  ^  .  Let  r  be  the  first  number 
in  1)  not  in  Bv  Let  us  place  it  within  a  non-overlapping  interval 
S2  of  length  <  Z2,  etc. 

We  now  define  a  f  unction  /(V)  in  21  such  that  the  value  of  /at 
any  x  is  the  length  of  all  the  intervals  and  part  of  an  interval 
lying  to  the  left  of  x.  Obviously  f(x)  is  a  continuous  function  of 
x  in  21.  At  each  rational  point  /'  (x)  =  1.  But  f(x)  is  not  de 
termined  aside  from  a  constant.  For  2£n  <  I.  Therefore  when 
I  is  small  enough  we  may  vary  the  position  and  lengths  of  the 
S-intervals,  so  that  the  resulting  /'s  do  not  differ  from  each  other 
only  by  a  constant. 

517.  1.    Let  f(x)  be  continuous  in  21  =  (a  <  5)  and  have  a  finite 
derivate,  say  Rf',  at  each  point  of  21.     Let  S  denote  the  points  of  21 
where  R  has  one  sign,  say  >  0.     If  (S  exists,  it  cannot  be  a  null  set. 


DERIVATES  519 

For  let  c  be  a  point  of  (£,  then  there  exists  a  point  d  >  c  such 
that 


Let  (£n  denote  the  points  of  (£  where 

n  _  1  <  Rf'  <  n.  (2 

Then  (£  =  ^  +  (£2  4-  •••     Let  0  <  <?  <  p.     We  take  the  positive 
constants  qv  q2'"  such  that 


If  now  (£  is  a  null  set,  each  (£m  is  also.      Hence  the  points  of  (£m 
can  be  inclosed  within  a  set  of  intervals  Smn  such  that  2Smn  <  <?„». 

n 

Let  now  qm  (a:)  be  the  sum  of  the  intervals  and  parts  of  intervals 
$m,  m  w  =  1,  2  •••  which  lie  in  the  interval  (a  <  x).     Let 


Obviously  Q(x)  is  a  monotone  increasing  function,  and 

0  <<?<»<?•  (3 

Consider  now 

p<v>=/O)  -/(«)-  «(^). 

We  have  at  a  point  of  51  —  (S, 


Hence  at  such  a  point 

EP' 


But  at  a  point  x  of  (£,  jRP'  <  0  also.  For  x  must  lie  in  some 
(£m,  and  hence  within  some  Smn.  Thus  qm(%)  increases  by  at  least 
Az  when  x  is  increased  to  x  +  Az.  Hence  mqm(x),  and  thus 
(?(V)  is  increased  at  least  wAz.  Thus 


'  <Rf<  -m<Q,  by  2), 


520  DERIVATES,   EXTREMES,   VARIATION 

since  x  lies  in  (£m.     Thus  RP'  <  0  at  any  point  of  51.     Thus  P  is 
a  monotone  decreasing  function  in  51,  by  508,  2.     Hence 

P(c)-P(d)  >  0. 
Hence  /<*)  -  /(<*)-  i  «  (0  -  Q  W  S  >  0, 

or  using  1),  3) 

p  -  q  <  o, 

which  is  not  so,  as  p  is  >  <?. 

2.  (Lebesgue.)  Let  f(x),  g  (x)  be  continuous^in  the  interval  5(, 
and  have  a  pair  of  corresponding  derivates  as  Rf,  Rg'  which  are 
finite  at  each  point  of  51,  and  also  equal,  the  equality  holding  except 
possibly  at  a  null  set.  Thenf(x)  —  g(x)  =  constant  in  51. 

The  proof  is  entirely  similar  to  that  of  515,  3,  the  enumerable 
set  (£  being  here  replaced  by  a  null  set.  We  then  make  use  of  1. 

518.  Letf(x)  be  continuous  in  some  interval  A  =  (u  —  S,  u  -f-  8). 
Letf'(x)  exist,  finite  or  infinite,  in  A,  but  be  finite  at  the  point  x  =  u. 

Then 

where 


Let  us  first  suppose  that/'(V)  =  0.     We  have  for  0<h<rj<B, 

f(u-h)-f(ju)\ 
-h  } 

,     u<x'<u  +  h     ,     u-h<x"<u 


h 


where  |e'|,  |  e"|  are  <  e/2  for  ?;  sufficiently  small. 

Now  ^  -  u  ^  -,       I  x"  -  u  |  <  -, 

~T  ~h~~ 

while  /"(^)  =  0     ,     by  hypothesis. 

Hence  \Qf\<€     »     for 

and  1)  holds  in  this  case. 


MAXIMA   AND   MINIMA  521 

Suppose  now  that  f"  (u)  =  a  ^  0.     Let 

</(V)  =/(V)  —  q(x)     ,     where  q(x)  =  -J-  ax2  +  bx  +  c. 
Since  q"(u)  =  a     ,     #"(»=0. 

Thus  we  are  in  the  preceding  case,  and  lim  Qg  =  0. 
Bat  Qg=Qf-Qq- 

Hence  lim  Qf=  a. 

Maxima  and  Minima 

519.  1.  In  I,  466  and  476,  we  have  denned  the  terms  f(x)  as 
a  maximum  or  a  minimum  at  a  point.  Let  us  extend  these  terms 
as  follows.  Let/^j  •••  #m)  be  defined  over  51,  and  let  x=  a  be  an 
inner  point  of  21. 

We  say  f  has  a  maximum  at  x  =  a  if  I0,/  (a)  —  f(x)  >  0,  for  any 
x  in  some  V(a),  and  2°,  f(a)  —f(x)  >  0  for  some  x  in  any  F(a). 
If  the  sign  >  can  be  replaced  by  >  in  1°,  we  will  say  /  has  a 
proper  maximum  at  a,  when  we  wish  to  emphasize  this  fact;  and 
when  >  cannot  be  replaced  by  >,  we  will  -say  /  has  an  improper 
maximum.  A  similar  extension  of  the  old  definition  holds  for 
the  minimum.  A  common  term  for  maximum  and  minimum  is 
extreme. 

2.  If  f(x)  is  a  constant  in  some  segment  53,  lying  in  the  inter 
val  51,  53  is  called  a  segment  of  invariability,  or  a  constant  segment 
of  /in  «. 

Example.     Let  f(x)  be  continuous  in  51  =  (0,  1*). 

Lefc  x=  •  flj^ag  •••  (1 

be  the  expression  of  a  point  of  51  in  the  normal  form  in  the  dyadic 
system.     Let  - 


be  expressed  in  the  triadic  system,  where  an=an,  when  an  —  0, 
and  =2  when  an  =  l.  The  points  (£  =  S£5  form  a  Cantor  set, 
I,  272.  Let  j3nj  be  the  adjoint  set  of  intervals.  We  associate 


522  DERIVATES,   EXTREMES,   VARIATION 

now  the  point  1)  with  the  point  2),  which  we  indicate  as  usual  by 
x~%.  We  define  now  a  function  g(x)  as  follows  : 

#(O=/O)     ,     when  a;-  f. 

This  defines  g  for  all  the  points  of  (£.  In  the  interval  3n,  let  g 
have  a  constant  value.  Obviously  g  is  continuous,  and  has  a 
pantactic  set  of  intervals  in  each  of  which  g  is  constant. 

3.  We  have  given  criteria  for  maxima  and  minima  in  I,  468 
seq.,  to  which  we  may  add  the  following  : 

Let  f(x)  be  continuous  in  (a—  8,  a  +  £).  If  Rf  (a)  >  0  and 
Lf]  '(#)<  0,  finite  or  infinite,  f(x)  has  a  minimum  at  x  =  a. 

If  Ef'(a)<0  and  Lf'(a)>  0,  finite  or  infinite,  f(x)  has  a  maxi 
mum  at  x  =  a. 

For  on  the  1°  hypothesis,  let  us  take  a  such  that  R  —  a  >  0. 
Then  there  exists  a  8'  >  0  such  that 


Similarly  if  fi  is  chosen  so  that  L  +  /5<  0,  there  exists  a  S"  >  0, 

suchthat 


Hence  ^     «  +  ^  in  (a  _  5^,  a»). 


520.    Example  1.     Let  /(a?)  oscillate  between  the  #-axis  and  the 
two  lines  y  =  x  and  y  =  —  x,  similar  to 


y 


•      7T 

zsm  — 


In  any  interval  about  the  origin,  y  oscillates  infinitely  often,  hav 
ing  an  infinite  number  of  proper  maxima  and  minima.  At  the 
point  #  =  0,/has  an  improper  minimum. 

Example  2.  Let  us  take  two  parabolas  Pl,  P2  defined  by  y  —  x*, 
y  =  2x2.  Through  the  points  x=±\,  ±\-~  let  us  erect  ordi- 
nates,  and  join  the  points  of  intersection  with  Px,  P2,  alternately 
by  straight  lines,  getting  a  broken  line  oscillating  between  the 


MAXIMA   AND   MINIMA  523 

parabolas  Pl ,  P2 .     The  resulting  graph  defines  a  continuous  func 
tion  f(x)  which  has  proper  extremes  at  the  points  (£  =  j  ±  -  \  • 

However,  unlike  Ex.  1,  the  limit  point  x=  0  of  these  extremes  is 
also  a  point  at  which  f(x)  has  a  proper  extreme. 

Example  3.  Let  \S\  be  a  set  of  intervals  which  determine  a 
Harnack  set  ^  lying  in  51  =  (0,  1).  Over  each  interval  S  =  (a,  /3) 
belonging  to  the  nih  stage,  let  us  erect  a  curve,  like  a  segment  of 
a  sine  curve,  of  height  hn  =  0,  as  n  =  oo,  and  having  horizontal 
tangents  at  a,  /3,  and  at  7,  the  middle  point  of  the  interval  S.  At 
the  points  jf  j  of  51  not  in  any  interval  8,  let/(V)  =  0.  The  func 
tion/  is  now  defined  in  51  and  is  obviously  continuous.  At  the 
points  \y[,f  has  a  proper  maximum  ;  at  points  of  the  type  a,  y8, 
f, /has  an  improper  minimum.  These  latter  points  form  the  set 
&  whose  cardinal  number  is  c.  The  function  is  increasing  in  each 
interval  (a,  7),  and  decreasing  in  each  (7,  /3).  It  oscillates  in 
finitely  often  in  the  vicinity  of  any  point  of  &. 

We  note  that  while  the  points  where  /  has  a  proper  extreme 
form  an  enumerable  set,  the  points  of  improper  extreme  may  form 
a  set  whose  cardinal  number  is  c. 

Example  4-  We  use  the  same  set  of  intervals  \&\  but  change 
the  curve  over  S,  so  that  it  has  a  constant  segment  77  =  (\,  JJL)  in  its 
middle  portion.  As  before  /=0,  at  the  points  £  not  in  the 
intervals  8. 

The  function  f  (x)  has  now  no  proper  extremes.  At  the  points 
of  ^p,  /  has  an  improper  minimum  ;  at  the  points  of  the  type  \,  /*,  it 
has  an  improper  maximum. 

Example  5.  Weierstrass  Function.  Let  (5  denote  the  points  in 
an  interval  51  of  the  type 

x  =  —    ,     r,  s,  positive  integers. 

0s 

For  such  an  x  we  have,  using  the  notation  of  502, 

bmx  =  im  +  f  m  =  b»-'r. 

Hence  fm  =  0     ,     formes. 

Thus  e=    -l+i=     _i+i. 


524  DERIVATES,   EXTREMES,   VARIATION 

A  Ti1 
Hence  sgn  —  =  sgn  Q  =  sgn  emr)m  =  sgn  (  - 

Thus  sgn 


if  r  is  even,  and  reversed  if  r  is  odd.  Thus  at  the  points  @,  the 
curve  has  a  vertical  cusp.  By  519,  3,  F  has  a  maximum  at  the 
points  (£,  when  r  is  odd,  and  a  minimum  when  r  is  even.  The 
points  (£  are  pantactic  in  51. 

Weierstrass'  function  has  no  constant  segment  8,  for  then 
f'(x)  =  0  in  B.  But  ^'  does  not  exist  at  any  point. 

521.  1.  Let  f(xl  "-  xm)  be  continuous  in  the  limited  or  unlimited 
set  51.  Let  &  denote  the  points  of  51  where  f  has  a  proper  extreme. 
Then  d:  is  enumerable. 

Let  us  first  suppose  that  51  is  limited.  Let  S  >  0  be  a  fixed 
positive  number.  There  can  be  but  a  finite  number  of  points  a  in 
51  such  that 


For  if  there  were  an  infinity  of  such  points,  let  ft  be  a  limiting 
point  and  77  <  J  S.  Then  in  F^(/3)  there  exist  points  «',  a"  such 
that  F^(a'),  Fg(«")  overlap.  Thus  in  one  case 


and  in  the  other 


which  contradicts  the  first. 

Let  now  Sj  >  S2  >  -••  =0.  There  are  but  a  finite  number  of 
points  a  for  which  1)  holds  for  S  =  Sj,  only  a  finite  number  for 
£  =  &,,,  etc.  Hence  d:  is  enumerable.  The  case  that  51  is  unlim 
ited  follows  now  easily. 

2.  We  have  seen  that  Weierstrass'  function  has  a  pantactic  set 
of  proper  extremes.  However,  according  to  1,  they  must  be 
enumerable.  In  Ex.  3,  the  function  has  a  minimum  at  each  point 
of  the  non-enumerable  set  ^p;  but  these  minima  are  improper.  On 
the  other  hand,  the  function  has  a  proper  maximum  at  the  points 
57},  but  these  form  an  enumerable  set. 


MAXIMA   AND   MINIMA  525 

522.  1.  Let  f(x)  be  continuous  in  the  interval  51.  Letf  have  a 
proper  maximum  at  x  =  a,  and  x  =  ft  in  51.  Then  there  is  a  point  7 
between  a,  ft  where  f  has  a  minimum,  which  need  not  however  be  a 
proper  minimum. 

For  say  a  <  ft.  In  the  vicinity  of  a,  f(x)  is  </(«)  ;  also  in 
the  vicinity  of  ft,  f(x)  is  </(/8).  Thus  there  are  points  53  in 
(a,  yS)  where  /is  <  either /(a)  or/(y£).  Let  /it  be  the  minimum 
of  the  values  otf(x)i  as  #  ranges  over  53.  There  is  a  least  value 
of  #  in  (a,  /3)  for  which  f(x)  =  /z.  We  may  take  this  as  the 
point  in  question.  Obviously  7  is  neither  a  nor  ft. 

2.  That  at  the  point  7,  /  does  not  need  to  have  a  proper  mini 
mum  is  illustrated  by  Exs.  1,  or  3. 

3.  In  51  =  (#,  6)   let  f(x)  exist,  finite  or  infinite.     The  points 
within  51  at  which  f  has  an  extreme  proper  or  improper,  lie  among 
the  zeros  of  f  (x). 

This  follows  from  the  proof  used  in  I,  468,  2,  if  we  replace  there 
<  0,  by  <  0,  and  >  0,  by  >  0. 

4.  Let  f  (x)  be  continuous  in  the  interval  51,  and  let  f(x)  have 
no  constant  segments  in  51.      The  points  &  of  51  ivhere  f  has  an  ex 
treme,  form  an  apantactic  set  in  51.     Let  3  denote  the  zeros  of  f  (x) 
in  51.     If  53  =  fbnj  is  the  border  set  of  intervals  lying  in  51  corre 
sponding  to  &f(x)  is  univariant  in  each  bn. 

For  by  3,  the  points  (g  lie  in  3-  As  f'(x)  is  continuous,  S  *s 
complete  and  determines  the  border  set  53-  Within  each  bn, 
f  (x)  has  one  sign.  Hence  f(x)  is  univariant  in  bn. 

5.  Letf(x)  be  a  continuous  function  having  no  constant  segment 
in  the  interval  51.     If  the  points  Q,  ivhere  f  has  an  extreme  form  a 
pantactic  set  in  51,  then  the  points  53  ivhere  f(x)  does  not  exist  or  is 
discontinuous,  form  also  a  pantactic  set  in  51. 

For  if  53  is  not  pantactic  in  51,  there  is  an  interval  (£  in  51 
containing  no  point  of  53.  Thus  f'(x)  is  continuous  in  (E.  But 
the  points  of  @  in  (£  form  an  apantactic  set  in  (5  by  4.  This, 
however,  contradicts  our  hypothesis. 

Example.  Weierstrass'  function  satisfies  the  condition  of  the 
theorem  5.  Hence  the  points  where  F'  (x)  does  not  exist  or  is 


526  DERIVATES,   EXTREMES,   VARIATION 

discontinuous   form  a  pantactic  set.     This  is  indeed  true,  since 
F'  exists  at  no  point. 

6.  Let  f(x)  be  continuous  and  have  no  constant  segment  in  the 
interval  51.  Let  /'(#)  exist,  finite  or  infinite.  The  points  where 
f'(x)  is  finite  and  is  =^0form  a  pantactic  set  in  51. 

For  let  a  <  ft  be  any  two  points  in  51.  If  /(«)  =/(/3),  there  is 
a  point  a  <  7  <  ft  such  that  /(«)  T^/Oy),  since  /  has  no  constant 
segment  in  51.  Then  the  Law  of  the  Mean  gives 


a-y 

Thus  in  the  arbitrary  interval  (a,  ft)  there  is  a  point  f,  where 
f  (x)  exists  and  is  =£  0. 

7.  Let  f(x)  be  continuous  in  the  interval  51.  Then  any  interval 
53  in  51  which  is  not  a  constant  segment  contains  a  segment  (E  in  which 
f  is  univariant. 

For  since  /  is  not  constant  in  53,  there  are  two  points  a,  b  in  53 
at  which  /has  different  values.  Then  by  the  Law  of  the  Mean 

/(«)-/(*)=(«-  »)  AO    .    cin»- 

Hence  f  (c)  =£  0.     As  f'(x)  is   continuous,  it   keeps  its  sign  in 
some  interval  (c  —  8,  c  -f  8),  and  /is  therefore  univariant. 

523.  Letf(x)  be  continuous  in  the  interval  51,  and  have  in  any  in 
terval  in  51  a  constant  segment  or  a  point  at  which  f  has  an  extreme. 
If  f  (x)  exists,  finite  or  infinite,  it  is  discontinuous  infinitely  often  in 
any  interval  in  51,  not  a  constant  segment.  At  a  point  of  continuity 
of  the  derivative,  f  (x)  =  0. 

For  if  f  (x)  were  continuous  in  an  interval  53,  not  a  constant 
segment,  /  would  be  univariant  in  some  interval  (£:<53,  by  522,  7. 
But  this  contradicts  the  hypothesis,  which  requires  that  any  inter 
val  as  (£  has  a  constant  segment.  Hence  f'(x)  is  discontinuous 
in  any  interval,  however  small. 

Let  now  x  =  c  be  a  point  of  continuity.  Then  if  c  lies  in  a  con 
stant  segment,  /'(V)  =  0  obviously.  If  not,  there  is  a  sequence  of 
points  e1,  ez  •••  =  e  such  that  f(x)  has  an  extreme  at  en.  But  then 
/'(en)=0,  by  522,3.  As/'<»  is  continuous  at  z  =  <?,/'(»=  0 
also. 


MAXIMA   AND   MINIMA  ,527 

524.  (Konig.)  Letf^x)  be  continuous  in  51  and  have  a  pantactic 
set  of  cuspidal  points  (L  Then  for  any  interval  $8  of  $[,  there  exists 
a  ft  such  that  f(x)  =  ft  at  an  infinite  set  of  points  in  33.  Moreover, 
there  is  a  pantactic  set  of  points  \%\  in  33,  such  that  k  being  taken  at 


For  among  the  points  &  there  is  an  infinite  pantactic  set  c  of 
proper  maxima,  or  of  proper  minima.  To  fix  the  ideas,  suppose 
the  former.  Let  x  =  c  be  one  of  these  points  within  33.  Then 
there  exists  an  interval  b  <.33,  containing  c,  such  that 

/(<?)  >/(#)     ,     for  any  x  in  b. 
Let  fji  =  Min/(V),     in  b. 

Then  there  is  a  point  x  where  /  takes  on  this  minimum  value. 
The  point  c  divides  the  interval  b  into  two  intervals.  Let  (  be 
that  one  of  these  intervals  which  contains  #,  the  other  interval  we 
denote  by  m.  Within  m  let  us  take  a  point  c^  of  c.  Then  in  I 
there  is  a  point  c[  such  that 


The  point  c1  determines  an  interval  bx  ,  just  as  c  determined  b. 
Obviously  bj^tn,  and  bx  falls  into  two  segments  Ix  ,  n^  as  before 
b  did.  Within  ml  we  take  a  point  of  c.  Then  in  (  there  is  a 
point  c%,  and  in  (x  a  point  c'%,  such  that 


In  this  way  we  may  continue  indefinitely.     Let 


be  the  points  obtained  in   this  way  which  fall  in  (.     Let  c1  be  a 
limit  point  of  this  set.     Let 


be  the  points  obtained  above  which  fall  in  (j,  and  let  cn  be  a  limit 
point  of  this  set.  Continuing  in  this  way  we  get  a  sequence  of 
limiting  points  ^  cu  cnr  ...  (2 

lying  respectively  in  (,  (x,  I2  ... 


528  DERIVATES,    EXTREMES,   VARIATION 

Since  /is  continuous, 

-       /OO  =/(«")=/(<"')=-  (3 

Thus  if  we  set  /(<?')  =  fi  we  see  that  /(#)  takes  on  the  value  (S  at 
the  infinite  set  of  points  2),  which  lie  in  33. 

Let  7j,  72  •••  be  a  set  of  points  in  2)  which  =  7. 


/(y)  ~ 


p. 


7  -  7i  7  -  72 

Thus  if  /'(#)  exists  at  #  =  7,  the  equations  3)  show  that 
=  0.     If  f  does  not  exist  at  7,  they  show  that 


Let  now  k  be  taken  at  pleasure.      Then 

g(x)=f(x)-kx 
is  constituted  as/,  and 

?O)  =/(*)-*• 

This  gives  1). 

525.  1.  Lineo-  Oscillating  Functions.  The  oscillations  of  a  con 
tinuous  function  fall  into  two  widely  different  classes,  accord 
ing  as  f(x)  becomes  monotone  on  adding  a  linear  function 
l(x)  =  ax  +  6,  or  does  not. 

The  former  are  called  lineo-oscillating  functions.  A  continu 
ous  function  which  does  not  oscillate  in  2f,  or  if  it  does  is  lineo- 
oscillating,  we  say  is  at  most  a  lineo-oscillating  function. 

Example  1.     Let      /(_e)  =  8ina!     ,     Z(>)  =  :r. 

Ifwesefc  y  =/(*)+*(*) 

and  plot  the  graph,  we  see  at  once  that  y  is  an  increasing  function. 
At  the  point  x  =  TT,  the  slope  of  the  tangent  to  f(x)  =  sin  x  is 
greatest  negatively,  i.e.  sinx  is  decreasing  here  fastest.  But  the 
angle  that  the  tangent  to  sin  x  makes  at  this  point  is  —  45°,  while 
the  slope  of  the  line  l(x)  is  constantly  45°.  Thus  at  x  =  TT,  y  has 
a  point  of  inflection  with  horizontal  tangent. 

If  we  take  l(x)  =  ax,  a  >  1,  y  is  an  increasing  function,  increas 
ing  still  faster  than  before. 


MAXIMA   AND   MINIMA  529 

All  this  can  be  verified  by  analysis.     For  setting 

y  =  sin  x  +  ax     ,     a  >  1, 

we  sret  / 

y  =  a  -f-  cos  #, 

and  ,      Q 

Thus  y  is  a  lineo-oscillating  function  in  any  interval. 
Example  2.  f(x)  =  z2  sin  -     ,     x  3=  0 

=  0     ,     x=0. 

l(x)  =  ax  +  b     ,     y  =f(x)  +  l(x). 
Then  ^  1 

ni '     — .     "/   />«  QI  r-j     _-     ("*(~)G    |        ft  sy*   —t-~    O 

X  X 

=  a     ,     x  =  0. 

Hence,  if  a  >  1  -f  2  TT,  z/  is  an  increasing  function  in  51  =  (  —  TT,  TT). 
The  function /oscillates  infinitely  often  in  51,  but  is  a  lineo-oscil 
lating  function. 

Example  8.  /(#)  =  #  sin  -     ,     x  =£  0 

x 

=  0     ,     x  =  0. 

Here  111 

y'  =  sin cos  — f-  a     ,     #  ^=  0. 

For  x=Q,  yr  does  not  exist,  finitely  or  infinitely. 

Obviously,  however  great  a  is  taken,  y  has  an  infinity  of  oscilla 
tions  in  any  interval  about  x  =  0.  Hence /is  not  a  lineo-oscillat 
ing  function  in  such  an  interval. 

2.  If  on e  of  the  four  derivates  of  the  continuous  function  /(#)  is 
limited  in  the  interval  51,  f(x)  is  at  most  lineo-oscillating  in  51. 

For  say  Rf  >  -  a  in  51.      Let  0  <  a  <  £, 


530  DERIVATES,   EXTREMES,   VARIATION 

Then 


Hence  g  is  monotone  increasing  by  508,  1. 

3.  Letf^x)  be  at  most  lineo-oscillating  in  the  interval  31.  If  Uf 
does  not  exist  finitely  at  a  point  x  in  31,  it  is  definitely  infinite  at  the 
point.  Moreover,  the  sign  of  the  oo  is  the  same  throughout  31. 

For  if  /  is  monotone  in  31,  the  theorem  is  obviously  true.     If 


be  monotone.     Then 

Uf  =  W  -  a, 

and  this  case  is  reduced  to  the  preceding. 

Remark.  This  shows  that  no  continuous  function  whose  graph 
has  a  vertical  cusp  can  be  lineo-oscillating.  All  its  vertical  tan 
gents  correspond  to  points  of  inflection,  as  in 


Variation 

526.  1.  Letf(x)  be  continuous  in  the  interval  31,  and  have  limited 
variation.  Let  D  be  a  division  of  31  of  norm  d.  Then  using  the  no 
tation  of  443, 

\imVDf=Vf    ,     \imPDf=Pf    ,     YimNDf=Nf.         (1 

For  there  exists  a  division  A  such  that 


where  for  brevity  we  have  dropped  /  after  the  symbol  V.  Let 
now  A  divide  31  into  v  segments  whose  minimum  length  call  X. 
Let  D  be  a  division  of  31  of  norm  d<d0<\.  Then  not  more 
than  one  point  of  A,  say  aK,  can  lie  in  any  interval  as  (#t,  «l+1)  of 
D.  Let  E  =  D  +  A,  the  division  obtained  by  superposing  A  on  D. 
Then  ft  denoting  some  integer  <  i>, 

V-  r-i 


VARIATION  531 

If  now  dQ  is  taken  sufficiently  small,  Osc/  in  any  interval  of  D 

is  as  small  as  we  choose,  say  <  —  .     Then 

6  v 


But  since  E  is  got  by  superposing  A  on  Z>, 
Hence  for  any  D  of  norm  <  c?0, 

which  proves  the  first  relation  in  1.     The  other  two  follow  at 
once  now  from  443. 

527.    //  f(x)  is  continuous  and  has  limited  variation  in  the  in 
terval  31  =  (a  <  6),  then 

P(x)     ,     N(x)     ,     V(x) 
are  also  continuous  functions  of  x  in  31. 

Let  us  show  that  V(x)  is  continuous ;  the  rest  of  the  theorem 
follows  at  once  by  443. 

By  526,  there  exists  a  c?0,  such  that  for  any  division  D  of  norm 

d<dQ,  F"(6)  =  Fi(6)  +  e'     ,     0<e'<e/3. 

Then  a  fortiori,  for  any  x  <  b  in  31, 

V(X)  =  VD(X}  +  6j       ,        0<€!<€/3.  (1 

In  the  division  Z>,  we  may  take  x  as  one  of  the  end  points  of 
interval,  and  x  +  h  as  the  other  end  point.     Then 

On  the  other  hand,  if  dQ  is  taken  sufficiently  small, 

\ffx  +  A)  -f(x)  I  <  ^     ,     f or  0  <  h  <  B.  (3 

o 

From  1),  2),  3)  we  have 

0  <  V(x  +  A)  -  V(x)  <  e     ,     f  or  any  0  <  h  <  8.  (4 


an 


532  DERIVATES,   EXTREMES,   VARIATION 

But  in  the  division  .Z),  x  is  the  right-hand  end  point  of  some  in 
terval  as  (x  —k,x).     The  same  reasoning  shows  that 

\V(x-K)-V(x)\<€     ,     foranyO<&<£.  (5 

From  4),  5)  we  see  V(x)  is  continuous. 

528.    1.    If  one  of  the  derivates  of  the  continuous  function  f  (V)  is 
numerically  <  M  in  the  interval  51,  the  variation  Voffis  < 

For  by  definition  y=  Max  y 

with  respect  to  all  divisions  D=\di\  of  5L     Here 


Now  by  506,  1, 

or 

Hence  ^  <  M^  < 

2.    Letf(x)  be  limited  and  R-integrable  in  51  = 

has  limited  variation  in  51. 

For  let  D  be  a  division  of  51  into  the  intervals  dt  =  (at, 

Then 


a»+i)  -F(a,)  I  =2  |  I       /(fe 


Thus  Max  VD  -  F 

and  F  has  limited  variation. 

529.    1.    If  f  (x)    has  limited  variation  in  the   interval   51,  the 
points  $  where  Osc/>  &,  are  finite  in  number. 

For  suppose  they  were  not.     Then  however  large  G-  is  taken, 
we  may  take  n  so  large  that  nk  >  G-.     There  exists  a  division  D 


VARIATION  533 

of  H,  such  that  there  are  at  least  n  intervals,  each  containing  a 
point  of  $  within  it.     Thus  for  the  division  D, 


Thus  the  variation  of  /  is  large  at  pleasure,  and  therefore  is  not 
limited. 

2.  If  f  has  limited  variation  in  the  interval  51,  its  points  of  dis 
continuity  form  an  enumerable  set. 

This  follows  at  once  from  1. 

530.  1.  Let  Dj,  D2  •••  be  a  sequence  of  superposed  divisions,  of 
norms  dn  =  0,  of  the  interval  51.  Let  £lDn  be  the  sum  of  the  oscilla 
tions  of  f  in  the  intervals  of  Dn.  If  Max  flDn  is  finite,  f(x)  has 
limited  variation  in  51. 

For  suppose  /  does  not  have  limited  variation  in  51.  Then 
there  exists  a  sequence  of  divisions  E^,  E^  «••  such  that  if  £lEn  is 
the  sum  of  the  oscillations  of  /in  the  intervals  of  En,  then 

n^<n^<  ...  =  +00.  (i 

Let  us  take  v  so  large  that  no  interval  of  Dv  contains  more  than 
one  interval  of  En  or  at  most  parts  of  two  En  intervals.  Let 
Fn=  En  +  Dv.  Then  an  interval  8  of  Dv  is  split  up  into  at  most 
two  intervals  8',  8"  in  Fn.  Let  o>,  a/,  co"  denote  the  oscillation  of 
/in  8,  £',  8".  Then  the  term  co  in  Dv  goes  over  into 

a'  +  co'  '  <  2  co 
in  £lFn.     Hence  if  Max  £lDn  =  M, 

n£n  <  2  QDr  <  2  M, 
which  contradicts  1). 

2.  Let  VDn  =  2  |/(X)  —  /(at+1)  |  ,  the  summation  extended 
over  the  intervals  (at,  al+1)  of  the  division  Dn.  If  Max  VDn  is 

n 

finite  with  respect  to  a  sequence  of  superposed  divisions  \Dn\,  we 
cannot  say  that  /has  limited  variation. 

Example.  For  let  /  (z)  =  0,  at  the  rational  points  in  the  inter 
val  51  =  (0,  1),  and  =  1,  at  the  irrational  points.  Let  Dn  be 


534  DERIVATES,   EXTREMES,   VARIATION 

f)        i   -| 
obtained  by  interpolating  the  points  — — —  in  21.     Then  /=0 

at  the  end  points  a,,  al+l  of  the  intervals  of  Dn.  Hence  VDn  =  0. 
On  the  other  hand,  f(x)  has  not  limited  variation  in  21  as  is 
obvious. 

531.    Let  F(x)  =  lim/(>,  t),  r  finite  or  infinite,  for  x  in    the 
interval  21.     Let  Var  f(x,  t)  <  M  for  each  t  near  r. 
Then  F(x)  has  limited  variation  in  21. 
To  fix  the  ideas  let  T  be  finite.     Let 


Then  for  a  division  D  of  21, 

VDF<  VDf+  VDg. 
But 

)  -  g  (a 


where  (#m,  am+l)  are  the  intervals  of  D. 
But  for  some  t  =  t'  near  r,  each 


where  «  is  the  number  of  intervals  in  the  division  D. 

Tlms  . 

Hence 
and  F  has  limited  variation. 

532.    Let  f(x),  g(x)  have  limited  variation  in  the  interval  21,  then 
their  sum,  difference,  and  product  have  limited  variation. 

If  also  l#l>7>°     i     in^I 

thenf/g  has  limited  variation. 

Let  us  show,  for  example,  that  h=fg  has   limited  variation. 

Forlet  Min/=m     ,     Min<7  =  n 

in  the  interval  d,. 
Osc/=  (o     ,     Osc  g  =  r 


VARIATION  535 

rhen  /  =  m  +  «&>     ,     g  =  n  +  £r     ,     in  rft, 

0<«<1     ,     0<£<1. 

Thus  fg  =  mn  +  ra/3r  -f  wao>  -f  a/Scwr. 

Now 


Tim  —    Til   r  — 


a>  —  car  <      <   <  mn  +    m 


G>T. 


Hence  77  =  Osc  A  <  2  jr  |  m  |  -f  *>    n\  +  a>Tj. 

Bufc  |wi|,  |w|,  r<.some  JST. 

Thus  TA  <  4  7f  2a>  +  2 


<  some  6r, 
and  A  has  limited  variation. 

533.  1.  Let  us  see  what  change  will  be  introduced  if  we 
replace  the  finite  divisions  D  employed  up  to  the  present  by 
divisions  JE,  which  divide  the  interval  31  =  (a  <  £>)  into  an  infinite 
enumerable  set  of  intervals  («t,  al+i). 


and 


for  the  class  of  finite  or  infinite  enumerable  divisions 

Obviously  TT>  F; 

hence  if  IT  is  finite,  so  is  F. 

We  show  that  if  F  is  finite,  so  is  W.  For  suppose  W  were 
infinite.  Then  for  any  Q-  >  0,  there  exists  a  division  E,  and  an 
w,  such  that  the  sum  of  the  first  n  terms  in  1)  is  >  6r,  or 


(2 


Let   now    D   be  the  finite  division  determined  by  the  points  #j 
az  '"  an+i  which  figure  in  2). 

Then  VB>a, 

hence  F=  ao,  which  is  contrary  to  our  hypothesis. 


536 


DERIVATES,   EXTREMES,   VARIATION 


We  show  now  that  V  and  W  are  equal,  when  finite.     For  let 
E  be  so  chosen  that 

W  —  €  ^  W  ^  W 

~  \    rr  f    \     V  r  « 


Now 


6/2 


if  n  is  sufficiently  large. 

Let  D  correspond  to  the  points  a1  a2  •••  in  WE^n.     Then 

and  hence  Y  A-    '  >  W      -4-    '  —  W 

Hence  W-Vj,<e. 

We  may  therefore  state  the  theorem  : 

2.  Iff  has  limited  variation  in  the  interval  21  with  respect  to  the 
class  of  finite  divisions  Z>,  it  has  with  respect  to  the  class  of  enumer 
able  divisions  E,  and  conversely.  Moreover 

Max  VD  =  Max  VE. 

534.  Let  us  show  that  Weierstrass'  function  F,  considered  in 
502,  does  not  have  limited  variation  in  any  interval  2(  =  (a  <  /3) 
when  ab  >  1.  Since  F  is  periodic,  we  may  suppose  a.  >  0.  Let 


be  the  fractions  of  denominator  bm  which  lie  in  21. 
These  points  effect  a  division  Dm  of  21,  and 


,/=0 


bm 


-F(k-±L 

\     ¥ 


If  I  is  the  minimum  of  the  terms  Fi  under  the  S  sign, 


Now 
Hence 


bm 


-  2. 


NON-INTUITIONAL   CURVES  537 

On  the  other  hand,  using  the  notation  and  results  of  502, 


and  also          (      x 

h 

Let  us  now  take 


Then  r_£+/  h  _.   1 

"W  -& 

Hence  from  3),          -^  >    mf%_      ^ 

V3      ^6  -  1 

ThUS      r/>«  ^  am(~ — )(&"5  -  2)     ,     by  1),  2). 

As  a  <  1,  and  «£>  >  1,  we  see  that 

VDm  =  +  GO,  as  w  =  oo . 

Non-intuitional  Curves 

535.  1.  Let  /(#)  be  continuous  in  the  interval  21.  The  graph 
of  /  is  a  continuous  curve  0.  If  /  has  only  a  finite  number  of  os 
cillations  in  21,  and  has  a  tangent  at  each  point,  we  would  call  0  an 
ordinary  or  intuitional  curve.  It  might  even  have  a  finite  num 
ber  of  angle  points,  i.e.  points  where  the  right-hand  tangent  is 
different  from  the  left-hand  one  [cf.  I,  366].  But  if  there  were 
an  infinity  of  such  points,  or  an  infinity  of  points  in  the  vicinity 
of  each  of  which  /  oscillates  infinitely  often,  the  curve  grows  less 
and  less  clear  to  the  intuition  as  these  singularities  increase  in 
number  and  complexity.  Just  where  the  dividing  point  lies  be 
tween  curves  whose  peculiarities  can  be  clearly  seen  by  the  intui 
tion,  and  those  which  cannot,  is  hard  to  say.  Probably  different 
persons  would  set  this  point  at  different  places. 

For  example,  one  might  ask  :  Is  it  possible  for  a  continuous 
curve  to  have  tangents  at  a  pantactic  set  of  points,  and  no  tangent 
at  another  pantactic  set?  If  one  were  asked  to  picture  such  a 
curve  to  the  imagination,  it  would  probably  prove  an  impossibility. 


538 


DERIVATES,   EXTREMES,   VARIATION 


Yet  such  curves  exist,  as  Ex.  3  in  501  shows.  Such  curves  might 
properly  be  called  non-intuitional. 

Again  we  might  ask  of  our  intuition :  Is  it  possible  for  a  con 
tinuous  curve  to  have  a  tangent  at  every  point  of  an  interval  SI, 
which  moreover  turns  abruptly  at  a  pantactic  set  of  points  ?  Again 
the  answer  would  not  be  forthcoming.  Such  curves  exist,  how 
ever,  as  was  shown  in  Ex.  2  in  501. 

We  wish  now  to  give  other  examples  of  non-intuitional  curve's. 
Since  their  singularity  depends  on  their  derivatives  or  the  nature 
of  their  oscillations,  they  may  be  considered  in  this  chapter. 

Let  us  first  show  how  to  define  curves,  which,  like  Weierstrass' 
curve,  have  a  pantactic  set  of  cusps.  To  effect  this  we  will  extend 
the  theorem  of  500,  2,  so  as  to  allow  g(x)  to  have  a  cusp  at  x—  0. 

536.  Let  (£  =  \en\  denote  the  rational  points  in  the  interval 
51=  (—a,  a).  Let  g(x)  be  continuous  in  53  =  (  —  2  a,  2  a),  and 
=  0,  at  x  =  0.  Let  53*  denote  the  interval  53  after  removing  the 
point  x  =  0.  Let  g  have  a  derivative  in  53*,  such  that 

M 


\g'(*)\< 


Then 


a>  0. 


(1 


0 


is  a  continuous  function  in  SI,  and  -  -  behaves  at  x  =  em  essentially 

A# 

as  —9-  does  at  the  origin.* 

A# 

To  simplify  matters,  let  us  suppose  that  (5  does  not  contain  the 
origin.  Having  established  this  case,  it  is  easy  to  dispose  of  the 
general  case.  We  begin  by  ordering  the  en  as  in  233.  Then 
obviously  if 

en  =  -     t     q  >  0     ,    p  positive  or  negative, 

we  have 


Let 


p      r 

q       s 


qs 


mn 


(2 


*  Cf.  Dini,  Theorie  der  Functional,  etc.,  p.  192  seq.     Leipzig,  1892. 


NON-INTUITIONAL   CURVES  539 

Let  E(x)  be  the  F  series  after  deleting  the  mth  term.     Then 


We  show  that  E  has  a  differential  coefficient  at  x  =  em,  obtained 
by  differentiating  E  termwise.     To  this  end  we  show  that  as  h  =  0, 

(e-  +      ~grf*-)     ,'•'»*•          (3 


converges  to  ff  =  2a^'(O     ,     m*n.         <      '     .  '-          (4 

That  is,  we  show 

e>0      ,      rj>0      ,      |D(A)-#    <e      ,      0<|A|<i;.  (5 

Let  us  break  up  the  sums  3),  4)  which  figure  in  5),  into  three 

parts  r        s 

2  =  2  +  2  +  2.  (6 

1  1          r+l       5+1 

\D-a\<  Dr-ar\  +  \Dr,8-ar,a\  +  \Dt-aa\    (7 

<  A  +  B  +  C. 

Since  g'(emn)  exists,  the  first  term  may  be  made  as  small  as  we 
choose  for  an  arbitrary  but  fixed  r  ;  thus 


Let  us  noiv  turn  to  B.     We  have 

B<\Dr, 

j(0         ,( 


provided  g1  (x)  exists  in  the  interval  (emn,  emn  + 
But  by  2), 


mn         ms 

if 


Thus  by  1), 

|  ^'(^mn  4-  A')  |  <  2aMm«n«  <  M^*     ,     ^  a  constant. 


540 


Hence  a  fortiori, 
Now  the  sum 


DERIVATES,  EXTREMES,   VARIATION 

,  < 


(9 


converges  if  n  >  0.     Hence  Rp>  q  and  Hp  may  be  made  as  small  as 
we  choose,  by  taking  p  sufficiently  large.     Let  us  note  that  by  91, 

#,<--.  GO 

pf> 

Thus  if  /*  =  Min  (a,  /3), 

B<  I  A.I  +  Iff,.  I 
for  a  sufficiently  large  r. 


We  consider  finally  O.     We  have 


h    s+i 


From  9)  we  see  that 


<7 


8  .      -, 

for  s  sufficiently  large.     Since  g(x)  is  continuous  in 


Hence 


1 


JV 


2f 


if  s_>-r—  ,  on  using  10). 

I  h\ 

Taking  s  still  larger  if  necessary,  we  can  make 


Thus 


NON-IXTUITIOXAL   CURVES  541 

The  reader  now  sees  why  we  broke  the  sum  6)  into  three  parts. 
As  h  =  0,  the  middle  term  contains  an  increasing  number  of  terms. 
But  whatever  given  value  h  has,  *  has  a  finite  value. 

Thus  as  J.,  B,  C  are  each  <  e/3,  the  relation  5)  is  established. 

Hence  E  has  a  differential  coefficient  at  x  =  em,  and  as 


A(0) 

r-  —   am  -  7  --  --  T~> 

h  h  h 


our  theorem  is  established. 
537.    Example  1.     Let 


g(x)  =  Vz2. 


Then  for  x  *  0,  g'  (x)  =     —  .      Here  « 


Thus 


is  a  continuous  function,  and  at  the  rational  points  em  in  the  in 
terval  31, 

RF'  (a;)  =  +  oo     ,     X^'  (a;)  =  -  oo. 


Hence  the  graph  of  F  has  a  pantactic  set  of  cuspidal  tangents 
in  31.  The  curve  is  not  monotone  in  any  interval  of  31,  however 
small. 


^ 

g  (x)  =  x  sin  -     ,     x  =£  0 


Example  2.    Let 


Then  1       ,         -j 

#'<»  =  sin-  -  -cos-     , 

XX  X 

Here  a  =  1.      For  x  =  0, 


542  DERIVATES,    EXTREMES,   VARIATION 

Then  1  1 

*(*)-  2       (*-«.)  sin  -J-    ,    /3>0 


is  a  continuous  function  in  51,  and  at  the  rational  point  e 


w 


where  E  is  the  series  obtained  from  F  by  deleting  the  rath  term. 

538.  Pompeiu  Curves.*  Let  us  now  show  the  existence  of 
curves  which  have  a  tangent  at  each  point,  and  a  pantactic  set  of 
vertical  inflectional  tangents. 

We  first  prove  the  theorem  (Borel)  : 

Let  Ja 


where  (£  =  \en\  is  an  enumerable  set  in  the  interval  51,  and 


is  convergent.      Then  B  converges  absolutely  and  uniformly  in  a  set 
53  <  51,  and  S  is  as  near  51  as  we  choose. 

The  points  £)  where  adjoint  B  is  divergent  form  a  null  set. 

For  let  us  enclose  each  point  en  in  an  interval  Sn  of  length 
with  en  as  center. 

The  sum  of  these  intervals  is 


f  or  k  >  0  sufficiently  large.     Let  now  k  be  fixed.     A  point  x  of  51 
will  not  lie  in  any  Sn  if 

r    —  I  r  -  P    \  ->  ^an 

'n  —    \  •£          Vn  |    ^>  ~T-' 

Then  at  such  a  point, 

k 

Adjoint  B  <  2an—=.  =  £2  Van  =  kA. 
Van 

*  Math.  Annalen,  v.  03  (1907),  p.  326. 


NON-INTUITIONAL   CURVES  543 

As  S  >  51  —  e,  the  points  £)  where  B  does  not  converge  ab 
solutely  form  a  null  set. 

539.    1.    We  now  consider  the  function 

F(x)  =  I  an(x  -  erf  =  Z/»O)  (1 

i 

where  (5  =  \en\  is  an  enumerable  pantactic  set  in  an  interval  51,  and 

A  =  2«n  (2 

is  a  convergent  positive  term  series. 

Then  F  is  a  continuous  function  of  x  in  51.  For  |  x  —  en  |*  is  < 
some  M  in  51. 

Let  us  note  that  each  f  n(x)  is  an  increasing  function  and  the 
curve  corresponding  to  it  has  a  vertical  inflectional  tangent  at  the 
point  x  =  en  . 

We  next  show  that  F  (x)  is  an  increasing  function  in  51.  For  let 
x'  <  x".  Then 

/.(*')</.(*")• 

Hence 


Hence 

2.    Let  us  now  consider  the  convergence  of 


obtained  by  differentiating  F  termwise  at  the  points  of  21  —  @. 
Let  55  denote  the  points  in  31  where 

?»  —  (4 


diverges.     We  have  seen  £)  is  a  null  set  if 

(5 


544  DERIVATES,   EXTREMES,   VARIATION 

is   convergent.     Let  51  =  £)  +  (£.      Let  #  be  a  point  of  (£,  i.e.  a 
point  where  4)  is  convergent.     We  break  3)  into  two  parts 


such  that  in  Dr  each  fn  <  1.     Then  D2  is  obviously  convergent, 
since  each  of  its  terms 


where       = 


x—  e, 


tf 

and  the  series  2)  is  convergent. 

The  series  Dl  is  also  convergent.     For  as  fn<  1,  the  term 

M<l^ 

£n 

and  the  series  4)  converges  by  hypothesis,  at  a  point  x  in  (£. 
Hence  D(x)  is  convergent  at  any  point  in  (£,  and  S,  =  51  when  5)  is 
convergent. 

3.  Let  (7  denote  the  points  in  51  where  3)  converges.  Let 
51=  0+  A. 

J7e  Tieatf  sAow  #A«£  F'(x)  =  D(x),  for  x  in  0.  For  taking  a;  at 
pleasure  in  (7  but  fixed, 


We  now  apply  156,  2,  showing  that  Q  is  uniformly  convergent 
in  (0*,  ?;).     By  direct  multiplication  we  find  that 


Thus  6)  gives 

.OXTX   _ 


Let  us  set 
Then 


NOX-INTUITIONAL  CURVES  545 

for  0  <  |  h  <_?/,  77  sufficiently  small.  As  the  series  on  the  right  is 
independent  of  A,  Q  converges  uniformly  in  (0*,  77).  Thus 
by  156,  2 

F1  =  D     ,     for  any  x  in  C. 

4.    Let  now  x  be  a  point  of  A,  not  in  Q.     At  such  a  point  we  show 

that 

.F'(X)=  +  oo,  (8 

and  thus  the  curve  F  has  a  vertical  inflectional  tangent.  For  as 
D  is  divergent  at  #,  there  exists  for  each  M  an  w,  such  that 

A»>2  M. 

But  the  middle  term  in  7)  shows  that  for  |  h  \  <  some  rjr  each 
term  in  Qm  is  >  \  the  corresponding  term  in  Dm.     Thus 


M    ,     0<|A|<y. 
Since  each  term  of  Q  is  >  0,  as  7)  shows, 

Q(h)  >  M. 
Hence  8)  is  established. 

5.    Let  us  finally  consider  the  points  x=  em.     If  <1>  denotes  the 
series  obtained  from  F  by  deleting  the  mth  term,  we  have 


As  J7  is  increasing,  the  last  term  is  >  0. 
Hence  J"(:r)=+oo     ,     ing. 

As  a  result  ive  see  the  curve  F  has  at  each  point  a  tangent.  At  an 
enumerable  pantactic  set  V,  it  has  points  of  inflection  with  vertical 
tangents. 

7.  Let  us  now  consider  the  inverse  of  the  function  F,  which  we 
denote  by 

x=G(t).  (9 

As  x  in  1)  ranges  over  the  interval  51,  t  =F(x)  will  range  over 
an  interval  53,  and  by  I,  381,  the  inverse  function  9)  is  a  one- 
valued  continuous  function  of  t  in  53  which  has  a  tangent  at  each 


546  DERIVATES,   EXTREMES,   VARIATION 

point  of  53.  If  TTare  the  points  in  53  which  correspond  to  the 
points  V  in  51,  then  the  tangent  is  parallel  to  the  £-axis  at  the 
points  W,  or  Gr'  (£)  =  0,  at  these  points.  The  points  W  are  pan- 
tactic  in  53. 

Let  Z  denote  the  points  of  53  at  which  Gr'  (t)  =  0.  We  show 
that  Z  is  of  the  2°  category,  and  therefore 

Card£=c. 

For  G-1  '(£)  being  of  class  <  1  in  53?  its  points  of  discontinuity  5 
form  a  set  of  the  1°  category,  by  486,  2.  On  the  other  hand,  the 
points  of  continuity  of  Gr'  form  precisely  the  set  Z,  since  the 
points  W  are  pantactic  in  53  and  Gr'  =  0  in  W.  In  passing  let  us 
note  that  the  points  Z  in  53  correspond  1-1  to  a  set  of  points  3  afc 
which  the  series  3)  diverges.  For  at  these  points  the  tangent  to 
F  is  vertical.  But  at  any  point  of  convergence  of  3),  we  saw  in 
2  that  the  tangent  is  not  vertical. 

Finally  we  observe  that  3)  shows  that 

MinD(aO>-  •  —  2an     ,     in  51. 
3     gf 

Hence  Q  ^2 

Max 


Summing  up,  we  have  this  result  : 

8.  Let  the  positive  term  series  2V«n  converge.  Let  (&  =  \en\  be 
an  enumerable  pantactic  set  in  the  interval  51.  The  Pompeiu  curves 
defined  by 

F(x)=Zan(x-Crf 
have  a  tangent  at  each  point  in  51,  whose  slope  is  given  by 


when  this  series  is  convergent,  i.e.  for  all  x  in  51  except  a  null  set. 
At  a  point  set  3  of  the  2°  category  which  embraces  (5,  the  tangents 
are  vertical.  The  ordinates  of  the  curve  F  increase  with  x. 

540.    1.    Faber  Curves.*    Let  F(x)  be  continuous  in  the  interval 
${  ==  (0,    1).      Its   graph    AVC    denote   by    F.      For    simplicity   let 

*  Math.  Annalen,  v.  66  (1908),  p.  81. 


NON-INTUITIONAL   CURVES  547 

i  =  0,  .F(l)  =  /0.      We  proceed  to  construct  a  sequence  of 
broken  lines  or  polygons, 


which  converge  to  the  curve  F  as  follows : 

As  first  line  LQ  we  take  the  segment  joining  the  end  points  of 
F.     Let  us  now  divide  21  into  n^  equal  intervals 

of  length  1 

and  having 

as  end  points.  As  second  line  L^  we  take  the  broken  line  or 
polygon  joining  the  points  on  F  whose  abscissae  are  the  points  3). 
We  now  divide  each  of  the  intervals  2)  into  n2  equal  intervals, 
getting  the  n^nz  intervals 


of  length 
and  having 


(5 


as  end  points.     In  this  way  we  proceed  on  indefinitely.     Let  us 
call  the  points 

4-K.l 

terminal  points.     The  number  of  intervals  in  the  rth  division  is 

vr  =  nl-  n2.-  nr. 

If  Lm(x)  denote  the  one-valued  continuous  function  in  51  whose 
value  is  the  ordinate  of  a  point  on  Lm,  we  have 


,  (6 

since  the  vertices  of  Lm  lie  on  the  curve  F. 
2.    For  each  x  in  51, 


m(x)  =  F(x).  '  (7 

m=x> 

For  if  x  is  a  terminal  point,  7)  is  true  by  6). 


548  DERIVATES,   EXTREMES,   VARIATION 

If  x  is  not  a  terminal  point,  it  lies  in  a  sequence  of  intervals 

£i>s2>  ••• 

belonging  to  the  1°,  2°  •••  division  of  21. 
Let  5>  , 

0»=  (am,m  «m,tt+l)- 

Since  F(x)  is  continuous,  there  exists  an  «,  such  that 

|  F(x)  -F(am,  „)  |  <|,     m>s  (8 

for  any  a:  in  Sm.     As  Lm(x)  is  monotone  in  Sm, 

|  Zm(20  -  Lm(amn~)  \  <  |  Lm(amn)  -  Xm(aw,n+1)  | 


.'  ^|   >     by  8).  - 

|^(*)-^(«*n)|<|-  (9 

Hence  from  8),  9), 

which  is  7). 

3.    Tfe  m^  ^r^g  1)  as  a  telescopic  series.     For 


etc.     Hence 

.F 
If  we  set 


)  =  lim  Z.(a:)  =  i0<»  +  2 


we  have  F(x)  =  %fn(x)  , 

o  . 

and 


The  function  /n(V),  as  10)  shows,  is  the  difference  between  the 
ordinates  of  two  successive  polygons  Ln_^  Ln  at  the  point  x.  It 
may  be  positive  or  negative.  In  any  case  its  graph  is  a  polygon 


NON-INT  UITIOXAL   CURVES  549 

fn  which  has  a  vertex  on  the  z-axis  at  the  end  point  of  each 
interval  8n_lt  Let  In8  be  the  value  of  fn(x)  at  the  point  x  =  ana, 
that  is,  at  a  point  corresponding  to  one  of  the  vertices  of  fn.  We 
call  l^  the  vertex  differences  of  the  polygon  Ln. 

Let 

p.  -Mini/..  |     ,     ?n  =  Max|?n.|. 

*  5 

Then  l/nOOl<9n     ,     in  51.  (13 

In  the  foregoing  we  have  supposed  F(x)  given.  Obviously  if 
the  vertex  differences  were  given,  the  polygons  1)  could  be  con 
structed  successively. 

We  now  show  : 

2<?n  (14 

is  consent, 


is  uniformly  convergent  in  51,  and  is  a  continuous  function  in  5T. 

For  by  13),  14),  F  converges  uniformly  in  51.     As  each  fn(x) 
is  continuous,  F  is  continuous  in  51. 

The  functions  so  defined  may  be  called  Faber  functions. 

541.    1.   We  now  investigate  the  derivatives  of  Faber's  functions, 
and  begin  by  proving  the  theorem  : 

If  2n1  —  n.q.=*I,v.qt  (1 

converge,  the  unilateral  derivatives  of  F(x)  exist  in  51  =  (0,  1)  .     More 
over  they  are  equal,  except  possibly  at  the  terminal  points  A=  \amn\. 

For  let  x  be  a  point  not  in  A.     Let  x',  x"  lie  in  V=  V*(x)  ; 
lQtxf-x=h',x"  -x=h". 

Let  Q-F(x')-F^ 

V  h" 

Then  F'(x)  exists  at  x,  if 

e>0     ,     7;>0     ,     \Q\<e     ,     for  any  x',  x"  in  V.         (2 


550 

Now 

1  Q\  < 

DER1VATES,   EXTREMES,   VARIATION 
Fm(x')-Fm(x)      Fm(x")-Fm(x)        Fm(x*)-Fm(x) 

h'                                 h"                  ' 
+ 

h1 

h" 

But 
Hence 

Similarly 


/.<>')  -/.(*) 
x'-x 


00  _ 

<  2  2zy?«<  -     •>     m  sufficiently  large. 


Finally,  if  77  is  taken  sufficiently  small,  x,  x1 ',  x"  will  correspond 
to  the  side  of  the  polygon  Lm .  Hence  using  540,  12),  we  see 
that  Ql  =  0.  Thus  2)  holds,  and  F' (x)  exists  at  x. 

If  x  is  a  terminal  point  #mn,  and  the  two  points  x',  x"  are  taken 
on  the  same  side  of  amn ,  the  same  reasoning  shows  that  the  uni 
lateral  derivatives  exist  at  amn  .  They  may,  however,  be  different. 

2.  Let  n^  =  n2  =  •••  =  2.  For  the  differential  coefficient  F'(x)  to 
exist  at  the  terminal  point  x,  it  is  necessary  that 

Um2n^n<oo.  (3 

*f  Em  2npn  =  oo,  (4 

the  points  where  the   differential  coefficient   does   not   exist  form  a 
pantactic  set  in  SI. 

Let  us  first  prove  3).  Let  6<  a<  c  be  terminal  points.  Then 
they  belong  to  every  division  after  a  certain  stage.  We  will 
therefore  suppose  that  5,  c  are  consecutive  points  in  the  nth 
division,  and  a  is  a  point  of  the  n  +  1st  division  falling  in  the 
interval  Sn  =  (5,  c).  If  a  differential  coefficient  is  to  exist  at  a, 


(5 


a  —  b 


must  be  numerically  less  than  some  J/,  as  n  =  oo,  and  hence  their 
sum  Q  remains  numerically  <2M. 


NON-INTUITIONAL   CURVES  551 


Now 

.P  (a)  =£„+,(«)     , 


Thus  Q  =  2»+i  S2  in+1O)  -  [Z.(6)  + 


or  |  §  |  =  4  •  2nZn)8     ,     supposing  a  =  ana. 

Hence  2n?n  <  JJf, 

which  establishes  3). 

Let  us  noiv  consider  4).     By  hypothesis  there  exists  a  sequence 
<  •••  =  oc,  such  that 


(r  being  large  at  pleasure.  Hence  at  least  one  of  the  difference 
quotients  5)  belonging  to  this  sequence  of  divisions  is  numerically 
large  at  pleasure. 

3'   If  X  =  2?m.  (1 

i«  absolutely  convergent,  the  functions  F(x)  have  limited  variation  in 
& 

For/m(#)  is  monotone  in  each  interval  B^.     Hence  in  8^ 
Var/m  -|C-  ^,a+i  I  <  Km.  |  +  |  ?m,.+i  I- 

Hence  in  51,  Var  /„(*)<  2  2^. 

Hence  „ 

2\     ,     in  51. 


771=1  5 

We  apply  now  531. 


552 


DERIVATES,   EXTREMES,   VARIATION 


542.    Faber  Functions  without  Finite  or  Infinite  Derivatives. 

To   simplify  matters   let  us  consider  the   following  example. 
The  method  employed  admits  easy  generalization 
and  gives  a  class  of  functions  of  this  type.      We 
use  the  notation  of  the  preceding  sections. 

Let  /0(#)  have  as  graph  Fig.  1.  We  next 
divide  21  =  (0,  1)  into  21!  equal  parts  8n,  812  and 
take  f^(x)  as  in  Fig.  2.  We  now  divide  21  into 
22!  equal  parts  £21,  S22,  S23,  S24  and  take  /2 (x)  as 


The  height  of  the  peaks  is  12  = 


in  Fig.  3. 

In  the  mth  division  21  falls  into  2w!  equal  parts 


FIG.  1 


in 

FIG.  2 


one  of  which  may  be  denoted  by 


Its  length  may  be  denoted  by  the  same  letter, 
thus 


FIG.  3 


AAA/^ 


FIG.  4 


In   Fig.    4,   Sm   is  an   interval  of  the   m  —  1st 
division. 

The  maximum    ordinate  of  /m(V)   is  L  = =  -. The 

10TO      2    10m 

part  of  the  curve  whose  points  have  an  ordinate  <  J  lm  have  been 
marked  more  heavily.  The  x  of  such  points,  form  class  1.  The 
other  o;'s  make  up  class  2.  With  each  x  in  class  1,  we  associate 
the  points  am  <  /3m  corresponding  to  the  peaks  of  fm  adjacent  to  x. 
Thus  am<x<{3m.  If  #  is  in  class  2,  the  points  «m,  /3m  are  the 
adjacent  valley  points,  where  fm  =  0. 

Let  now  x  be  a  point  of  class  1.     The  numerators  in 


(1 


«.-* 


am-  x 


have  like  signs,  while  their  denominators  are  of  opposite  sign. 
Thus  the  signs  of  the  quotients  1)  are  different.  Similarly  if  x 
belongs  to  class  2,  the  signs  of  1)  are  opposite.  Hence  for  any  #, 


NON-INTUITIONAL  CURVES 


553 


the  signs  of  1)  are  opposite.     It  will  be  convenient  to  let  em  denote 
either  c^  or  /3m.     We  have 


Hence, 


m! 


On  the  other  hand,  for  any  x^x'  in  8TO, 


JU  As 

Hence  setting  x'  =  en,  and  letting  n  >  w, 

1       2m!       1      2n"1! 

—  1  Am  '   On!         1  i\m         On! 


(2 
(3 


10 


For  if  Iog2  a  be  the  logarithm  of  a  with  the  base  2, 


_  n  >     n     I0g2  10     ,     for  n  sufficiently  large. 


n-1 


Hence 
Thus 


On! 


and  this  establishes  4). 

Let  us  now  extend  the  definition  of  the  functions  fn(x)  by  giv 
ing  them  the  period  1.  The  corresponding  Faber  function  F(x) 
defined  by  540,  12)  will  admit  1  as  period.  We  have  now 


From  2)  we  have 


554  DERIVATES,   EXTREMES,   VARIATION 

As  to  T2,  we  have,  using  4)  and  taking  n  sufficiently  large, 


Similarly 

\T9\<    i 


-v_^      v_        __ 

*    *       "  ™         '      » 


<    2  2 

—   n-fl 


Thus  finally 


As 


Thus 


sgn 


-  X 


il>l*il  + 

F(x^ 

=  sgn 


en  —  x 


-  F(x) 


en  —  x 


As  gn  may  be  at  pleasure  «n  or  ^n,  and  as  the  signs  of  1)  are 
opposite,  we  see  that 


F(x)  has  neither  a  finite  nor  an  infinite  differential  coefficient 
at  any  point. 


CHAPTER  XVI 

SUB-  AND  INFRA-UNIFORM  CONVERGENCE 
Continuity 

543.  In  many  places  in  the  preceding  pages  we  have  seen  how 
important  the  notion  of  uniform   convergence   is  when  dealing 
with  iterated  limits.     We  wish  in  this  chapter  to  treat  a  kind  of 
uniform  convergence  first  introduced  by  Arzeld,  and  which  we 
will  call  subuniform.     By  its  aid  we  shall  be  able  to  give  condi 
tions  for  integrating  and  differentiating  series  termwise  much 
more  general  than  those  in  Chapter  V. 

We  refer  the  reader  to  Arzela's  two  papers,  "  Sulle  Serie  di 
Funzioni,"  R.  Accad.  di  Bologna,  ser.  V,  vol.  8  (1899).  Also 
to  a  fundamental  paper  by  Osgood,  Am.  Journ.  of  Math.,  vol.  19 
(1897),  and  to  another  b}^  Hobson,  Proc.  Lond.  Math.  Soc.,  ser.  2, 
vol.  1  (1904). 

544.  1.    Let/^j  ••«  xm,  ^  •••  tn)=f(x,  t)  be  a  function  of  two 
sets  of  variables.     Let  x  =  (xl>~xm}  range  over  Hi  in  an  w-way 
space,  and  t  =  (tl  •«•  £n)  range  over  £  in  an  rc-way  space.     As  x 
ranges  over  Hi  and  t  over  £,  the  point  (xl  •••  ^  ...)  =  (#,  £)  will 
range  over  a  set  51  lying  in  a  space  9?p ,  p  =  m  +  n. 

Let  r,  finite  or  infinite,  be  a  limiting  point  of  £. 

Let         v     f(  t        t^  =  6C  ">         in  £ 

t=T 

Let  the  point  x  range  over  53  <  X,  while  t  remains  fixed,  then 
the  point  (x,  £)  will  range  over  a  layer  of  ordinate  t,  which  we 
will  denote  by  %t.  We  say  x  belongs  to  or  is  associated  with  this 
layer. 

We  say  now  that/==  <£,  subuniformly  in  H  when  for  each  e>0, 

555 


556  SUB-  AND   INFRA-UNIFORM   CONVERGENCE 

1°  There  exists  a  finite  number  of  layers  £t  whose  ordinates  t 
lie  in  F;*(T). 

2°  Each  point  x  of  £  is  associated  with  one  or  more  of  these 
layers.  Moreover  if  x  =  a  belongs  to  the  layer  £,,  all  the  points 
x  in  some  V^a  also  belon  to  ?,. 


while  (#,  t)  ranges  over  any  one  of  the  layers  %t.  When  ra=  1, 
that  is  when  there  is  but  a  single  variable  #  which  ranges  over  an 
interval,0  the  layers  reduce  to  segments.  For  this  reason  Arzela 
calls  the  convergence  uniform  in  segments. 

2.    In  case  that  subuniform  convergence  is  applied  to  the  series 


convergent  in  51,  we  may  state  the  definition  as  follows : 

F  converges  subimiformly  in  51  when 

1°    For  each  e  >  0,  and  for  each  v  there  exists  a  finite  set  of 
layers  of  ordinates  >  v,  call  them 


8,,  «,-  (2 

such  that  each  point  x  of  51  belongs  to  one  or  more  of  them,  and  if 
x  =  a  belongs  to  £m,  then  all  the  points  of  51  near  a  also  belong 


as  the  point  (#,  w)  ranges  over  any  one  of  the  layers  2). 
545.    Example.     Let 

EVjA  _  y  f      MS  (n-l>     ]          in9J-r 

'          -^iTT^~l+(n-l)VJ 
Here 


The  series  converges  uniformly  in  51,  except  at  x  =  0.  The 
convergence  is  therefore  not  uniform  in  51  ;  it  is,  however,  sub- 
uniform.  For 


CONTINUITY  557 

Hence  taking  m  at  pleasure  and  fixed, 

Fm\<e     ,     a;  in  «!  =  (-$,  8), 
sufficiently  small.     On  the  other  hand, 


Thus  for  w  sufficiently  large, 


Hence  we  need  only  three  segments  s1,  s2,  s3  to  get  subuniform 
convergence. 

546.  1.  Let  /(^  -~xmi  V-'O^^Oi  '••*«)  m  £,  as  ?  =  T, 
finite  or  infinite.  Let  /(#,  t)  be  continuous  in  Hi  for  each  t  near  r. 
For  <f>  to  be  continuous  at  the  point  x  =  a  in  £,  it  is  necessary  that 
for  each  e  >  0,  there  exists  an  77  >  0,  and  a  dt  for  each  t  in  Fn*(r) 
such  that 


for  each  t  in  V^  and  for  any  x  in  Vd(a). 

It  is  sufficient  if  there  exists  a  single  t=/3  in  T/rT/*(r)  for  ivhich 
the  inequality  1)  holds  for  any  x  in  some  V^a). 

It  is  necessary.     For  since  </>  is  continuous  at  x  =  a, 

|  $(x)  —  <£(«)  |  <  |      ,     for  any  x  in  some  F^(«). 
o 

Also  since  /=  c/>, 

I/O  Q  -  <£(»  |  <  I     ,     for  any  f  in  some  r/(r). 
Finally,  since  /is  continuous  in  x  for  any  £  near  r, 

I/O>  0  -/O»  0|<  jj      ^     for  any  ^  in  some  1\(a). 
Adding  these  three  inequalities  we  get  1),  on  taking 


558  SUB-   AND  INFRA-UNIFORM   CONVERGENCE 

It  is  sufficient.     For  by  hypothesis 


and  hence  in  particular. 


»  n 

o 


Also  since  /O,  £)  *s  continuous  in  a;, 


I/O,  £)—/(«,  £)|  <        ,     for  any  a;  in  some  F6,,(». 
6 

Thus  if  8  <  8',  8",  these  unequalities  hold  simultaneously.     Add- 
ing  them  we  get 


—  <Ka)l  <  e   >   f°r  any  ^  i 

and  thus  <£  is  continuous  at  x  =  a. 
2.    As  a  corollary  we  get  : 
Let  ^O)=2/tl...lnOi-^) 

converge  in  21,  each  term  being  continuous  in  51.  For  F(x)  to  be  con 
tinuous  at  the  point  x  =  a  in  21,  it  is  necessary  that  for  each  e  >  0, 
and  for  any  cell  R^_  >  some  J2A,  there  exists  a  S^  such  that 


^8  sufficient  if  there  exists  an  R^  and  a  8  >  0 
|  ^O)l  <  e     ->    for  anV  x  in  V^( 


547.    1.    Let  limf^xl"-xm,  ^  •••  £n)  =  <^>Oi  "'  ^m)  ^  %,  r  finite 

x^ 

or  infinite.     Letf(x,  t)  be  continuous  in  Hfor  each  t  near  r. 
1°     Iff=  </>  subuniformly  in  £,  <#>  i*  continuous  in  3E- 
2°     ^  3E  ^8  complete,  and  <f>  is  continuous  in  £,/==  <t>  subuniformly 

in  X. 

To  prove  1°.     Let  x  =  a  be  a  point  of  £.     Let  e  >  0  be  taken  at 

pleasure  and  fixed.     Then  there  is  a  layer  %ft  to  which  the  point 

a  belongs  and  such  that 


CONTINUITY  559 

when  (x,  t)  ranges  over  the  points  of  8^.  But  then  1)  holds  for 
t  =  fi  and  x  in  some  F^(a).  Thus  the  condition  of  546,  l  is  satis 
fied. 

To  prove  2°.  Since  (f>  is  continuous  at  z=a,  the  relation  1) 
holds  by  546,  l,  for  each  t  in  Vf(j)  and  for  any  x  in  Vdt(a). 
With  the  point  a  let  us  associate  a  cube  Ca^  lying  in  D^a)  and 
having  a  as  center.  Then  each  point  of  £  lies  within  a  cube. 
Hence  by  Borel's  theorem  there  exists  a  finite  number  of  these 
cubes  (7,  such  that  each  point  of  £  lies  within  one  of  them,  say 


But  the  cubes  2)  determine  a  set  of  layers 

^     ,     V  (3 

such  that  1)  holds  as  (x,  £)  ranges  over  the  points  of  SI  in  each 
layer  of  3).  Thus  the  convergence  of /to  <f>  is  subuniform  in  £. 

2.    As  a  corollary  we  have  the  theorem  : 

Let  ps     •  .  a?  ^  =  2f       (x  •••  x  } 

converge  in  £,  each  /  fteiVigr  continuous  in  H.  If  F  converges  sub- 
uniformly  in  £,  F  is  continuous  in  £.  If  £  is  complete  and  F  is 
continuous  in  X,  F  converges  subuniformly  in  H. 

548.    1.    Let  F,  ,  _  2  -        (x  .  .  x  ^ 

*  \%)  —  "HMi—Si  VX1          ^m/ 

converge  in  SI. 

i^^  ^Ag  convergence  be  uniform  in  SI  except  possibly  for  the  points 
of  a  complete  discrete  set  53  =  55|.  .For  each  b,  let  there  exist  a  \0 
swcA  that  for  any  X  >  X0, 


.F  converges  subuniformly  in  SI. 

For  let  D  be  a  cubical  division  of  norm  d  of  the  space  9?TO  in 
which  SI  lies.  We  may  take  d  so  small  that  33^  is  small  at 
pleasure.  Let  BD  denote  the  cells  of  D  containing  points  of  SI 
but  none  of  33.  Then  by  hypothesis  ^converges  uniformly  in  BD. 
Thus  there  exists  a  /x0  such  that  for  any  ft  >  /x0, 

|  Fp  (x)  |  <  e     ,     for  any  z  of  SI  in  BD. 


560  SUB-   AND   INFRA-UNIFORM   CONVERGENCE 


At  a  point  b  of  $8,  there  exists  by  hypothesis  a  Fs(ft)  and  a  X0 


such  that  for  each  X  >  X0 


|  JFx(aO  !  <  €     ,     for  any  x  in  F«(i). 

Let  (7ftjX  be  a  cube  lying  in  D«(5),  having  b  as  center.     Since  33 
is  complete  there  exists  a  finite  number  of  these  cubes 


such  that  each  point  of  23  lies  within  one  of  them. 
Moreover  — 

l^.(*)l«i 

for  any  x  of  21  lying  in  tlie  /cth  cube  of  1). 

As  1?^  embraces  but  a  finite  number  of  cubes,  and  as  the  same 
is  true  of  1),  there  is  a  finite  set  of  layers  8  such  that 

\Fv(x)\<e     ,     in  each  8. 
The  convergence  is  thus  subuniform,  as  X,  p  are  arbitrarily  large. 

2.    The  reasoning  of   the  preceding  section  gives  us  also  the 
theorem  : 


in  £,  r  finite  or  infinite.  Let  the  convergence  be  uniform  in  £  except 
possibly  for  the  points  of  a  complete  discrete  set  (§  =  \e\.  For  each 
point  e<  let  there  exist  an  rj  such  that  setting  e(#,  t)  =/(^,  0  —  </>(^)» 

lim  e(x,  t)  =  0     ,    for  any  t  in  F^*(T). 

x=e 

Thenf=  <£  subuniformly  in  %. 

3.    As  a  special  case  of  1  we  have  the  theorem  : 

Let  *(*> 

converge  in  H,  and  converge  uniformly  in  51,  except  at  x  =  «1?  •••  a:  =  a,. 
^4.^  a;  =  at  Z^^  fA^re  g^z's^  «  j/t 


lim  J*ni(a;)  =0     ,     nt  >  i/t     ,     i  =  1,  2  ...  s. 

X=aL 

Then  F  converges  subuniformly  in  51. 


CONTINUITY  561 

4.    When  v      ~,     ,,        .  ,  x 

lim/O,  0  =  £(*) 

<=T 

we  will  often  set 

/(avO~*(*)4XM)i 

and  call  e  the  residual  function. 

549.    Example  1. 
/(^n)«^=£(a?)=0     ,     for  7i  =  oo  in  21  =  (0  «z), 

gW^.r" 

«,  /3,  X  >   0      ,      /I  >  0. 

The  convergence  is  suburiiform  in  81.      For  2;  =  0  is  the  only 
possible  point  of  non-uniform  convergence,  and  for  any  m, 

/-  ~\    i  H)\  OC       •     /\  •     /\ 

=  0     ,     as  x  =  0. 


Example  2.        f(x,  ri)  =  --  -  =  6  (x)  =  0     ,     as  n  =  oo, 

c  +  n^xP  f 

a;  in  31  =  (0  <  a)     ,     a,  /S,  X,  /*  >  0     ,     ^>X     ,     <?  >  0. 
The  convergence  is  uniform  in  iB  =  (e  <  a),  where  ^  >  0.     For 


"  c 

a»     7^ 

"  e^    n^ 

<  e     ,     for  n  >  some  m. 

Thus  the  convergence  is  uniform  in  81,  except  possibly  at  x  =  0. 
The  convergence  is  subuniform  in  51.     For  obviously  for  a  given  n 

lim/(#,  n)  =  0. 

-r=0 

550.    1.    Let  Hm/O^  •••  xm  tl  ...  fn)  =  ^(^  .-•  arm)  «»  Hi,  r  finite 

t=T 

or  infinite. 

Let  the  convergence  be  uniform  in  %  except  at  the  points 
85  =(*„*,,  -  J,). 


562  SUB-   AND   INFRA-UNIFORM   CONVERGENCE 

For  the  convergence  to  be  sub-uniform  in  £,  it  is  necessary  that  for 
each  b  in  33,  and  for  each  e  >  0,  there  exists  a  t=  fi  near  r,  such  that 


x=b 

For  if  the  convergence  is  subuniform,  there  exists  for  each 
and  77  >  0  a  finite  set  of  layers  £t,  t  in   FV"(r)  such  that 

|  e(#,  f)  |  <  e     ,     re  in  %t. 

Now  the  point  x=  b    lies  in  one    of   these   layers,  say  in   fy 
Then 

|  e(#,  /3)  |  <  e     ,     for  all  x  in  some  V*(b). 

But  then  1)  holds. 

"'        J^jOT  CL/YYL'Y)i r  I^Pt" 

0 

This  is  the  series  considered  in  140,  Ex.  2. 

F  converges  uniformly  in  21  =  (  —  1,  1),  except  at  x  =  1. 

As  y  ^  =  _  ^ 

we  see  that  y      XT  /^  \  _       -i 

Hence  ^  is  not  subuniformly  convergent  in  51. 

Integrdbility 
551.    1.    Infra-uniform  Convergence.     It  often  happens  that 


subuniformly  in  36  except  possibly  at  certain  points  (£=  \e]  form 
ing  a  discrete  set.  To  be  more  specific,  let  A  be  a  cubical  divi 
sion  of  $ftm  in  which  X  lies,  of  norm  5.  Let  JTA  denote  those  cells 
containing  points  of  X,  but  none  of  (£.  Since  (§,  is  discrete, 
JTA  =  36.  Suppose  now /"=(/>  subuniformly  in  any  ^TA  ;  we  shall 
say  the  convergence  is  infra-uniform  in  £.  When  there  are  no 
exceptional  points,  infra-uniform  convergence  goes  over  into  sub- 
uniform  convergence. 


INTEGRABILITY  563 

This  kind  of  convergence  Arzela  calls  uniform  convergence  by 
segments,  in  general. 

2.    We  can  make  the  above  definition  independent  of  the  set  (g, 
and  this  is  desirable  at  times. 


Let  £  =  (^T,  £)  be  an  unmixed  division  of  X  such  that  £  may  be 
taken  small  at  pleasure.  If  /=</>  subuniformly  in  each  X,  we 
say  the  convergence  is  infra-uniform  in  %. 

3.  Then  to  each  e,  77  >0,  and  a  given  Jf,  there  exists  a  set  of 
layers  (j,  I2  •••  ,  t  in  FV"(r),  such  that  the  residual  function  e(z,  f) 
is  numerically  <  e  for  each  of  these  layers.     As  the  projections  of 
these  layers  I  do  not  in  general  embrace  all  the  points  of  £,  we 
call  them  deleted  layers. 

4.  The  points  £  we  shall  call  the  residual  points. 

5.  Example  1.      ^     y* 


This  series  was  studied  in  150.     We  saw  that  it  converges  uni 
formly  in  21  =  (0,  1),  except  at  x—  0. 

As  . 


nx 


and  as  this  =  1  as  x  =  0  for  an  arbitrary  but  fixed  w,  F  does  not 
converge  subuniformly  in  51,  by  550.  The  series  converges  infra- 
uniformly  in  21,  obviously. 

6.    Example  X.  !•=  L.»(I  _*). 

0 

This  series  was  considered  in  550,  2.  Although  it  does  not 
converge  subuniformly  in  an  interval  containing  the  point  x  =  1, 
the  convergence  is  obviously  infra-uniform. 

552.    1.    Let  lira  /  (^  •••  xm  ^  ...  *n)  =  ^(^  •••  xm)  be  limited  in  X, 

x=r 

T  finite  or  infinite.  For  each  t  near  r,  let  f  be  limited  and  R-integrable 
in  H.  For  </>  to  be  R-integrable  in  X,  it  is  sufficient  thatf  =  <f>  infra- 
uniformly  in  Hi.  If  Hi  is  complete,  this  condition  is  necessary. 


564  SUB-  AND   INFRA-UNIFORM  CONVERGENCE 

It  is  sufficient.      We  show  that  for  each  e,  co  >  0  there  exists  a 
division  D  of  9?m  such  that  the  cells  in  which 

Osc  <f>  >  co  (1 

have  a  volume  <  <r.      For  setting  as  usual 


we  have  in  any  point  set, 

Oscc 
Using  the  notation  of  551, 


in    the    finite    set    of    deleted  layers    (x,    (2  •••  corresponding   to 

t=  t^  t2  -••     For  each  of  these  ordinates  £t,/(#,  Q  is  integrable 

in  H.     There  exists,  therefore,  a  rectangular  division  D  of  9?m, 
such  that  those  cells  in  which 


have  a  content  <  f  ,  whichever  ordinate  tL  is  used.     Let  JS  be  a 

division  of  9?m  such  that  the  cells  containing  points  of  the  residual 
set  £  have  a  content  <  <r/2.  Let  F  =  D  +  E.  Then  those  cells 
of  F  in  which 

Osc/C*,O>!<     or     Osc  '  €(s,  *0  I  >f 

t  =  l,  2  ...  have  a  content  <  <r.  Hence  those  cells  in  which  1) 
holds  have  a  content  <  cr. 

It  is  necessary,  if  £  is  complete.     For  let 

<1,  *2  V-  =  T' 

Since  <£  and/  (z,  fn)  are  integrable,  the  points  of  discontinuity  of 
<£O)  and  of  /(&,  «n)  are  null  sets  by  462,  6.  Hence  if  (£,  ^  denote 
the  points  of  continuity  of  <£(#)  and  /(#,  0  in  X, 


since  96  is  measurable,  as  it  is  complete. 


INTEGKABILITY 
Let  ©=QdvJ<£|}, 

then  5  =  f 

by  410,  6. 

Let  £)  =  Di»(6,  ®), 

then  f)  =  S, 

as  we  proceed  to  show.     For  if  G  =  X  — 

6T  =  S) 


565 


(1 


But    ^  is   a  null   set.       Hence  Meas   Dy((S,   6r)  =  0,    and    thus 
S  =  £  =  J),  which  is  1). 

Let  now  f  be  a  point  of  5),  let  it  lie  in  (£/,,  (£/2  •••  where  ^,  ^2  ... 
form  a  monotone  sequence  =  r.     Then  since 


there  is  an  m  such  that 


<  §     ,     for  any  n  >  w. 
o 


But  f  lying  in  2),  it  lies  in  (£  and  (£,  . 
Thus  « 


for  any  a:  in 


Now 


Hence 


n 


(3 


Hence  from  2),  8), 


<e     ,     for  any  a:  in 


Thus  associated  with  the  point  f,  there  is  a  cube  F  lying  in  DS(£), 
having  %  as  center.  As  D  =  £  —  5)  is  a  null  set,  each  of  its  points 
can  be  enclosed  within  cubes  (7,  such  that  the  resulting1  enclosure 


566  SUB-   AND   INFRA-UNIFORM   CONVERGENCE 

(£  has  a  measure  <  <r,  small  at  pleasure.  Thus  each  point  of  £  lies 
within  a  cube.  By  Borel's  theorem  there  exists  a  finite  set  of 
these  cubes 

1'       2   '"     .f        '  1'       2   '"       «' 

such  that  each  point  of  £  lies  within  one  of  them.  But  corre 
sponding  to  the  F's,  are  layers 

81,  8a,  -  8r 
such  that  in  each  of  them 

|€O,01<€. 

Thus/  =  <t>  subuniformly  in  X  =  (I\,  T2~-  Fr).  Let  £  be  the 
residual  set.  Obviously  ji  <  <r.  Thus  the  convergence  is  infra- 
uniform. 

2.    As  a  corollary  we  have  : 

Let  ^0^  =  2/tl...lnOi"-O 

converge  in  31.  Xe^  JP  be  limited,  and  each  f,  be  limited  and  R-in- 
tegrable  in  31.  For  F  to  be  R-integrable  in  31,  it  is  sufficient  that  F 
converges  infra-uniformly  in  31. 

If  31  is  complete,  this  condition  is  necessary. 

553.    Infinite  Peaks.     1.    Let  lira  f  (x {  "'Xmt1"-tn)  =  $(x)  in  £, 

t=T 

T  finite  or  infinite.  Although /(a;,  t)  is  limited  in  £  for  each  t 
near  T,  and  although  </>(»  is  also  limited  in  X,  we  cannot  say  that 

I/O,  01  <  some  ^  0- 

for  any  x  in  X  and  an}^  f  near  T,  as  is  shown  by  the  following 
Example.     Let/O>  0  =  -^  =  ^O)  =  °>    as    ^^^     for    *    in 

^  =  (-00,0)). 

It  is  easy  to  see  that  the  peak  of  /  becomes  infinitely  high  as 

flfssOQ. 

In  fact,  for  x  =  —-/=_.    Thus  the  peak  is  at  least  as  high 

V£  e 

Vz     , .  T 

as  — ,  which  =  QO  . 

e 


INTEGRABILITY  567 

The  origin  is  thus  a  point  in  whose  vicinity  the  peaks  of  the 
family  of  curves  f  (x,  £)  are  infinitely  high.  In  general,  if  the 

Peaksof  /CV^V'-O 

in  the  vicinity  Vs  of  x  =  f  become  infinitely  high  as  t  =  'T,  however 
small  8  is  taken,  we  say  f  is  a  point  with  infinite  peaks. 

On  the  other  hand,  if  the  relation  1)  holds  for  all  x  and  t  in 
volved,  we  shall  say/(#,  £)  is  uniformly  limited. 

2.  If  lim  /CV^    *1»-*»)  =  <Kai  •"*»)>    and  if  ffr  0   « 

<=T 

uniformly  limited  in  £,  £fo?w  $  z*  limited  in  Hi. 

For  2:  being  taken  at  pleasure  in  36  and  fixed,  $(x)  is  a  limit 
point  of  the  points  /(z,  £)  as  t  =  r.  But  all  these  points  lie  in 
some  interval  (—#,#)  independent  of  z.  Hence  <j>  lies  in  this 
interval. 

3.  IfH  is  complete,  the  points  $  in  Hi  with  infinite  peaks  also  form 
a  complete  set.     If  these  points  &  are  enumerable,  they  are  discrete. 

That  $  is  complete  is  obvious.  But  then  $  =  $  =  0,  as  $  is 
enumerable. 


554.  1.  Let  lim/0^  •••  xm  ^  •••  fn)  =  ^(^  •••«„)  in  I,  metric  or 
complete.  Let  f  (x,  t)  be  uniformly  limited  in  X,  and  R-integrable 
for  each  t  near  T.  For  the  relation 

Km 


fo  hold,  it  is  sufficient  thatf=(j>  infra-  uniformly  in  I.  If  X  is 
for  each  t  complete,  this  condition  is  necessary. 

For  by  552,  <f>  is  JZ-integrable  if  /=  £  iufra-uniformly,  and  when 
X  is  complete,  this  condition  is  necessary.  By  424,  4,  each  f(x,  t) 
is  measurable.  Thus  we  may  apply  381,  2  and  413,  2. 

2.    As  a  corollary  we  have  the  theorem  : 

Let  m     F(x)  =  -Sfli  .....  Or,-*.) 

converge  in  the  complete  or  metric  field  51.  Let  the  partial  sums  J\  be 
uniformly  limited  in  51-  Let  each  term  /t  fo  limited  and  R-integrable 
in  21.  Then  for  the  relation 


568  SUB-   AND   INFRA-UNIFORM   CONVERGENCE 

to  hold  it  is  sufficient  that  F  is  infra -uniformly  convergent  in  51.     If 
51  is  complete,  this  condition  is  necessary. 

555.    Example  1.     Let  us  reconsider  the  example  of  150, 


We  saw  that  we  may  integrate  termwise  in  51  =  (0,  1),  al 
though  F  does  not  converge  uniformly  in  51.  The  only  point  of 
non-uniform  convergence  is  x  ~  0.  In  551,  5,  we  saw  that  it  con 
verges,  however,  infra-uniformly  in  51.  As 


I  ^n(X)  I  <  1     •>     f°r  anv  x  m  ^  and  for  every  n, 

all  the  conditions  of  554  are  satisfied  and  we  can  integrate  the 
series  termwise,  in  accordance  with  the  result  already  obtained 
in  150. 

**      (n  ~*x 


Example  2.     Let     F(x)  =  V  -       ~  =  0. 

^     J          ^4    [  enx*  e(n-l)x*        j 

Then  ^  ,^  _  nx 

^w-p- 

We  considered  this  series  in  152,  i.  We  saw  there  that  this 
series  cannot  be  integrated  termwise  in  51  =  (0  <  «).  It  is,  how 
ever,  subuniformly  convergent  in  51  as  we  saw  in  549,  Ex.  1.  We 
cannot  apply  554,  however,  as  Fn  is  not  uniformly  limited.  In 
fact  we  saw  in  152,  l,  that  x  =  0  is  a  point  with  an  infinite  peak. 

Example  3.  F(x)  =  2^(1  -  x). 

o 

We  saw  in  551,  6,  that  F  converges  infra-uniformly  in  51  =  (0,  1). 
Here  Fn  (V)  =  |  1  -  x*  |  <  some  M, 

for  any  x  in  51  =  (0  <  w),  u  <^  1,  and  any  n.     Thus  the  Fn  are 
uniformly  limited  in  51. 

We  may  therefore  integrate  termwise  by  554,  2.  We  may 
verify  this  at  once.  For 


=  0 


INTEGRABILITY  569 

Hence  C*F(x)dai  =  u.  (1 

On  the  other  hand, 

Xu  lln+^ 

Fndx  =  u  --  --  =  u     ,     as  n  =  GO.  (2 

71+1 


+ 

From  1),  2)  we  have 


0     ,  n  +  1      n  H-  2 


556.    1.  //  l°/Oi  ••>  a?»  «!  -  O  =  *(«!  —  *.)  infra-uniformly 
in  the  metric  or  complete  field  36,  as  f  =  r,  r  ^wite  or  infinite  ; 

2°  /(#,  0  ^s  uniformly  limited  in  H  and  R-integrable  for  each  t 
near  r; 


uniformly  with  respect  to  the  set  of  measurable  fields  H  in  X- 

If  36  is    complete,  condition  1°  wa^  be   replaced   by  3°  <£(#)  is 
R-integrable  in  X. 

For  by  552,  l,  when  3°  holds,  1°  holds  ;  and  when  1°  holds,  <f> 
is  72-integrable  in  36. 

Now  the  points  <&t  where 

|  e  O,  tn)    >  e 
are  such  that  ^ 

lim  @t  =  0     ,     by  412. 


Let  £  =  £,+  £«.     Then 

Ce(x,t)=  /*€(«,  0+  f  «C 

«4/;e  -t^fc  otft 

I    f 

« 


But  lim  I,  =  0, 

?=T 

which  establishes  the  theorem. 
2.    As  a  corollary  we  have  : 

If  1°  F(x)=  ^fli...in(^x1  •••  ^m)   converges   infra-uniformly,    and 
each  of  its  terms  f,  is  R-integrable  in  the  metric  or  complete  field  51; 


570  SUB-  AND  INFRA-UNIFORM   CONVERGENCE 

2°  F>,(x)  is  uniformly  limited  in  51; 

Tken  r  *•(*)=  2  r/., 

J«  Jy 

and  the  series  on  the  right  converges  uniformly  with  respect  to  all 
measurable  SB  <  51. 


3.    Jf  1°  lim/(z,  ^  ...  fn)  =  <£(X)  i«  R-integrable  in  the  interval 

t=T 

5(  =  («  <  6),  T  finite  or  infinite  ; 

2°f(x,  £)  is  uniformly  limited,  and  R-integr  able  for  each  t  near  r; 

Thpw  Cx  fx 

lim  I/O,  0^=1    <KzVz  =  <£<>\ 

*=T    •/«  •/« 

uniformly  in  51,  anc?  <J>(a:)  is  continuous  in  51. 


termfL  are  R-integrable  in  the  interval  21  =  (a<  5); 
2°  jPx(^)  *'*  uniformly  limited  in  51; 

2%eft  xy,  N      v  r^-,  N  7 

^(a;)  =  2  I  f,(x)dx    ,     z  tw  51 

•OB 

continuous. 

For  6r  is  a  uniformly  convergent  series  in  51,  each  of  whose  terms 


/.*• 

%x  u 

i»  «  continuous  function  of  x. 

Differentiability 

557.    1.    J/  1°  lhn/(s,  <!-«„)=:  ^(«)  m  51  =  (a  <  6),  r  finite  or 
infinite  ; 

%°fx(.xi  0  *'*  R-integrable  for  each  t  near  T,  a/ic?  uniformly  limited 


3°  /j(a;,  «)=  i/r(V)  infra-  uniformly  in  5(,  a«  £  =  T; 
^  a^  a  point  x  of  continuity  of  i/r  in  51 

^(aO-^OO.  (1 


or  ttwa£  is  ^e  same 

-f/(*,0-  (2 

dx 


DIFFERENTIABILITY  571 

For  by  554, 

lim  f/J(z,  f)dx  =  F+(x)dx  (3 

t=r  "a  •/• 

=  lim[/0r,  0-/O,  0]     »     by  I,  538 

/=T 

=  <£<»-<»<»     ,     byl°. 
Now  by  I,  537,  at  a  point  of  continuity  of  i/r, 

(*)**  -*co-  (4 


From  3),  4),  we  have  1),  or  what  is  the  same  2). 

2.  /ft  the  interval  51,  if 

1°   F(x)=  2/tl...lB(a;)  converges;  (1 

2°    EacKf[(x)  is  limited  and  R-integrable  ; 

3°    .FA'  (a;)  t*  uniformly  limited  ; 

4°    G(x)=  2//  i«  infra-  uniformly  convergent; 

Then  at  a  point  of  continuity  of  6r(#)  m  51,  t^e  ??i(z?/  differentiate 
the  series  1)  termivise,  or  F'(x)=  G(x). 

3.  J/i  the  interval  51,  if 

1°  f(x,  t1  •-  tn)  =  (f>(x)  as  t  =  r,  r  finite  or  infinite  ; 

2°  /(#,  f)  is  uniformly  limited,  and  a  continuous  function  of  x  ; 

3°   ^(a:)  =  limy^a;,  £)  z*8  continuous; 

nen  .  *'(*)=*(*),  a 

or  w^a^  zs  ^6  same 

=  lim-    /(«,  0-  (2 


For  by  547,  l,  condition  3°  requires  that  /'  =  i|r  subuniformly 
in  K.  But  then  the  conditions  of  1  are  satisfied  and  1)  and  2) 
hold. 

4.    In  the  interval  51  let  us  suppose  that 

1°    F(x)  =  2/ti...tn<»  converges  ;  (1 


572  SUB-   AND  INFRA-UNIFORM   CONVERGENCE 

2°    Each  termf,  is  continuous; 

3°   Fl(x)  is  uniformly  limited  ; 

4°    G(x)  =  2/[(a;)  is  continuous  ; 

Then  we  may  differentiate  1)  termtvise,  or  F'(x)  =  6r(#), 

558.    Example  1.     We  saw  in  555,  Ex.  3  that 

'  *a-«U).        a 


The  series  got  by  differentiating  termwise  is 

#00  =  2zn(l-20=l     »     Q<z<l 

o  (2 

=  0     ,     x  =  0. 

Thus  by  557,  4,      ^^  =  ^^  in  (Q#?  1)  =  5p>  (g 

The  relation  3)  does  not  hold  for  x  =  0. 
Example  2. 


H- 


l  J 
1 


Here  ^(a:)  =  arctg  x,         for  any  z.  (1 


Hence   (r(^)  is  continuous  in  any  interval  51,  not  containing 
x  =  0.     Thus  we  should  have  by  557,  4, 

Ff(x)=G-(x),         zinH.  (3 

This  relation  is  verified  by  1),  2).     The  relation  3)  does  not 
hold  for  x  =  0,  since 


DIFFERENTIABILITY  573 

Example  3. 


=  1  log  (1  -f  x2)     ,     for  any  x. 


In  any  interval  51,  all  the  conditions  of  557,  4,  hold. 
Hence 


,     for 

In  case  we  did  not  know  the  value  of  the  sums  1),  2)  we  could 
still  assert  that  3)  holds.  For  by  545,  G-  is  subuniformly  con 
vergent  in  51,  and  hence  is  continuous. 

Example  4- 

F(  ^  —  V  I  ^  "*"  nx  —  1  +(n  +  1)^  }  _  1  +  #  s-t 

Here 

*'(*)= -5.  (2 

The  series  obtained  by  differentiating  jF  termwise  is 

*  (3 


•7  I     gi»-  enx 

and  hence 

/?•£  z>WX 

The  peaks  of  the  residual  function 
e(>,  n)=^x, 

are  of  height  =  \/e.  The  convergence  of  G-  is  not  uniform  at 
x  =  0.  The  conditions  of  557,  4,  are  satisfied  and  we  can  differ 
entiate  1)  termwise.  This  is  verified  by  2),  3). 


574  SUB-   AND  INFRA-UNIFORM   CONVERGENCE 


559.    1.    Ifl°  lim/O,  t1"-  tn)  =  <$>(x)  is  limited  and  R-integraUe 

t  =  T 

in  the  interval  51  =  (a  <  ft)  ; 

2°  f(x,  t)  is  limited,  and  R-integrable  in  51,  for  each  t  near  r  ; 

3°  ^(x)  =  lim  P/O,  0  =  lim  g(x,  t) 

t=r  */a  t=r 

is  a  continuous  function  in  51; 

4°   The  points  (g  in  51  in  whose  vicinity  the  peaks  of  f(x,  t)  as 
t  =  T  are  infinitely  high  form  an  enumerable  set  ; 

Then  Cx  Cx 

6(x)  =   I    ^(a;)  =  lim  (  /(*,  t)dx  =  ^O),          (1 

«/«  <=T  «^a 

°^"  fx  rx 

lim  I  /(a;,  t)dx  =  I    lim/(^,  <)c?a;, 
t=T  J<*  t/a    <=T 

ant?  the  set  (S  i*  complete  and  discrete. 

For  (g  is  discrete  by  553,  3. 

Let  a  be  a  point  of  A  =  51  —  (g.     Then  in  an  interval  a  about  a, 

|/(#,  t)  |  <  some  M    ,     a;  in  a,  any  £  near  r.  (2 

Now  by  556,  3,  taking  e  >  0  small  at  pleasure,  there  exists  an 
??  >  0  such  that 


for  any  x  in  a,  and  t  in  F^*(T).     If  we  set  x  =  a  4-  h,  we  have 

(3 


h 
Also  by  556,  3,  we  have 

P>O,  0^  =  f*<Kx)dx  +  e"     ,       €"  |  <  e 

*^a  ^a 

for  an?/  2:  in  a,  and  t  in  FT,*(T).     Thus 

(4 


A  h       Ax      h 

From  3),  4)  we  have 

i;=^+^          K|,|e"|<e. 
h      Ax      h 


DIFFERENTIABILITY  575 

Now  e  may  be  made  small  at  pleasure,  and  that  independent  of 
h.     Thus  the  last  relation  gives 


forarinA. 

z      Az 

As  this  holds  however  small  h  =  Az  is  taken,  we  have 

*±  =  M          for  x  in  A. 
dx      dx 

Hence  by  515,  3, 

-^(x)  =  6(x)  +  const     ,     in  21. 


For  x  =  a, 

and  thus 


,     in  21. 


2.    J.8  a  corollary  we  have  : 

If  1°  F(x)=  2/4...tn(z)  is  limited  and  R  integrable  in  the  inter- 


2°  1\(^)  ^s  limited  and  each  termf,  is  R-integrable; 
3°   &(x)=  Xf^  is  continuous; 


4°  The  points  @  i/i  21  wi  ^Aos^  vicinity  the  peaks  of  F^(x)  are  in 
finitely  high  form  an  enumerable  set; 

Then 


or  we  may  integrate  the  F  series  termivise. 

560.    1.   If  1°  lira  /(a,  «j  —  *»)  =  *(»)  *w  51  =  («  <  J>  T/w*fe  or 

<=T 

infinite  ; 

2°  /£(z,  «)  i8  limited  and  R-integrable  for  each  t  near  r; 

3°   The  points  (§.  of  21  m  w^o86  vicinity  f'x(x,  t)  has  infinite  peaks 
as  t  =  T  form  an  enumerable  set; 

4°  <£(V)  is  continuous  at  the  points  (g; 

5°  -^(a:)  =  lim/J(ir,  0  z*  limited  and  R-integrable  in  21; 


576  SUB-  AND   INFRA-UNIFORM   CONVERGENCE 

Then  at  a  point  of  continuity  of  ^(V)  in  51 

$(x)  =  ^o),  (l 

or  what  is  the  same 

-j-  lim/(^0  =  lim-f/<>,  0- 
ax  t=r  t=T  ax 

For  let  S  =  (a  <  /3)  be  an  interval  in  51  containing  no  point  of 
($.      Then  for  any  x  in  8 


X*CMfe:-/&Q~/C<Q    *    b72°- 

m^  i* 

Hence 


lim  I    f'x(x,  t)dx  =  lim\f(x,  £)  —  ./(«,  £)J 

=  c£(V)  -  </>(«)     ,     by  1°.  (2 

By  556,  3,  <f>(x)  is  continuous  in  S.  Thus  <£(#)  is  continuous 
at  any  point  not  in  (g.  Hence  by  4°  it  is  continuous  in  51. 

We  may  thus  apply  559,  1,  replacing  therein /(#,  £)  by /,£(#,  £). 
We  get 

/*x  /*x  /*x 

lim   I    f'x(x,£)dx=  I     lim/^(a;,  0^  =  I    ^(x)dx.  (3 

/=T   c/a  »/a  ^/a 

Since  2)  obviously  holds  when  we  replace  a  by  a,  this  relation 
with  3)  gives 


At  a  point  of  continuity,  this  gives  1)  on  differentiating. 

2.    Ifl°  F(x)  =  2/ti ...  tn(#)  converges  in  the  interval  51; 

2°   6r(:r)  =  2/[(a;)   aw^   ^ac^   o/  ^s   ^erws    ar^   limited    and   R- 
integrable  in  51; 

3°  TAe  points  of  51  zVi  whose  vicinity  Gr\(x)  has  infinite  peaks  as 
X  =  GO,  form  an  enumerable  set  at  which  F(x)  is  continuous; 

Then  at  a  point  of  continuity  of  G-(x)  we  have 


or  what  is  the  same 


DIFFERENTIABILITY  577 

561.    Example.  ^  /  n**  _  (n+1)^  1  _  z2 

TU"*2      ~  *' 

Hence  o 


The  series  obtained  by  differentiating  F  termwise  is 

1 

Here  ~  _ 


Hence  2  ^      9  ^ 

is  a  continuous  function  of  x. 

The  convergence  of  the  Gr  series  is  not  uniform  at  x  =  0.     For 
set  an  =  \/n.     Then 


I  en      en  J 

To   get   the    peaks    of   the  residual    function  we  consider  the 
points  of  extreme  of 

y  =  — •  f  3 

««• 

We  find  n(l-5nx*+OnW^ 

yr  = 2  . 

7jj;2 

Thus  y'  =  0  when 

2  nV  -  5  wa^  +  1  =  0, 

or  when  2;  =  — —  or  - — =     ,     a,  a  constants. 


V/i 
Putting  these  values  in  3),  we  find  that  y  has  the  form 


Hence  x  =  0  is  the  only  point  where  the  residual  function  has 
an  infinite  peak.  Thus  the  conditions  of  560,  2,  are  satisfied,  and 
we  should  have  F'  (JK)  =  G-(x)  for  any  x.  This  is  indeed  so,  as  1), 
2)  show. 


CHAPTER   XVII 
GEOMETRIC  NOTIONS 

Plane  Curves 

562.  In  this  chapter  we  propose   to  examine    the   notions  of 
curve  and  surface  together  with  other  allied  geometric  concepts. 
Like  most  of  our  notions,  we  shall  see  that  they  are  vague  and 
uncertain  as  soon  as  we  pass  the  confines  of  our  daily  experience. 
In  studying   some  of    their    complexities   and   even  paradoxical 
properties,  the  reader  will  see  how  impossible  it  is  to  rely  on  his 
unschooled  intuition.     HB  will  also  learn  that  the  demonstration 
of   a   theorem  in   analysis   which  rests  on   the   evidence    of  our 
geometric    intuition    cannot    be    regarded    as  binding    until   the 
geometric  notions  employed  have  been  clarified  and  placed  on  a 
sound  basis. 

Let  us  begin  by  investigating  our  ideas  of  a  plane  curve. 

563.  Without  attempting  to  define  a  curve  we  would  say  on 
looking  over  those  curves  most  familiar  to  us  that  a  plane  curve 
has  the  following  properties  : 

1°  It  can  be  generated  by  the  motion  of  a  point. 

2°  It  is  formed  by  the  intersection  of  two  surfaces. 

3°  It  is  continuous. 

4°  It  has  a  tangent  at  each  point. 

5°  The  arc  between  any  two  of  its  points  has  a  length. 

6°  A  curve  is  not  superficial. 

7°  Its  equations  can  be  written  in  any  one  of  the  forms 


(2 

(3 


and  conversely  such  equations  define  curves. 

678 


PLANE   CURVES  579 

8°  When  closed  it  forms  the  complete  boundary  of  a  region. 

9°    This  region  has  an  area. 

Of  all  these  properties  the  first  is  the  most  conspicuous  and 
characteristic  to  the  naive  intuition.  Indeed  many  employ  this 
as  the  definition  of  a  curve.  Let  us  therefore  look  at  our  ideas 
of  motion. 

564.  Motion.     In  this  notion,  two  properties  seem  to  be  essen 
tial.     1°  motion  is  continuous,  2°  it  takes  place  at  each  instant  in 
a  definite  direction  and  with  a  definite  speed.     The  direction  of 
motion,  we  agree,  shall  be  given  by  dy/dx,  its  speed  by  ds/dt. 
We  see  that  the  notion  of  motion  involves  properties  4°,  5°,  and  7°. 
Waiving  this  point,  let  us  notice  a  few  peculiarities  which  may 
arise. 

Suppose  the  curve  along  which  the  motion  takes  place  has  an 
angle  point  or  a  cusp  as  in  I,  366.  What  is  the  direction  of 
motion  at  such  a  point?  Evidently  we  must  say  that  motion  is 
impossible  along  such  a  curve,  or  admit  that  the  ordinary  idea  of 
motion  is  imperfect  and  must  be  extended  in  accordance  with  the 
notion  of  right-hand  and  left-hand  derivatives. 

Similarly  ds/dt  may  also  give  two  speeds,  a  posterior  and  an 
anterior  speed,  at  a  point  where  the  two  derivatives  of  s  ==  <£(£) 
are  different. 

Again  we  will  admit  that  at  any  point  of  the  path  of  motion, 
motion  may  begin  and  take  place  in  either  direction.  Consider 
what  happens  for  a  path  defined  by  the  continuous  function  in 
I,  367.  This  curve  has  no  tangent  at  the  origin.  We  ask  how 
does  the  point  move  as  it  passes  this  point,  or  to  make  the  ques 
tion  still  more  embarassing,  suppose  the  point  at  the  origin.  In 
what  direction  does  it  start  to  move?  We  will  admit  that  no 
such  motion  is  possible,  or  at  least  it  is  not  the  motion  given  us 
by  our  intuition.  Still  more  complicated  paths  of  this  nature  are 
given  in  I,  369,  371,  and  in  Chapter  XV  of  the  present  volume. 

It  thus  appears  that  to  define  a  curve  as  the  path  of  a  moving 
point,  is  to  define  an  unknown  term  by  another  unknown  term, 
equally  if  not  more  obscure. 

565.  2°  Property.     Intersection  of  Two  Surfaces.     This  property 
has  also  been  used  as  the  definition  of  a  curve.     As  the  notion 


580  GEOMETRIC   NOTIONS 

of  a  surface  is  vastly  more  complicated  than  that  of  a  curve,  it 
hardly  seems  advisable  to  define  a  complicated  notion  by  one  still 
more  complicated  and  vague. 

566.  3°  Property.     Continuity.     Over  this  knotty  concept  philos 
ophers  have  quarreled  since  the  days  of  Democritus  and  Aristotle. 
As  far  as  our  senses  go,  we  say  a  magnitude  is  continuous  when 
it  can  pass  from  one  state  to  another  by  imperceptible  gradations. 
The  minute  hand  of  a  clock  appears  to  move  continuously,  although 
in  reality  it  moves  by  little  jerks  corresponding  to  the  beats  of  the 
pendulum.     Its  velocity  to  our  senses  appears  to  be  continuous. 

We  not  only  say  that  the  magnitude  shall  pass  from  one  state 
to  another  by  gradations  imperceptible  to  our  senses,  but  we  also 
demand  that  between  any  two  states  another  state  exists  and  so 
without  end.  Is  such  a  magnitude  continuous  ?  No  less  a  mathe 
matician  than  Bolzano  admitted  this  in  his  philosophical  tract 
Paradoxien  des  Unendlichen.  No  one  admits  it,  however,  to-day. 
The  different  states  of  such  a  magnitude  are  pantactic,  but  their 
ensemble  is  not  a  continuum. 

But  we  are  not  so  much  interested  in  what  constitutes  a  con 
tinuum  in  the  abstract,  as  in  what  constitutes  a  continuous  curve 
or  even  a  continuous  straight  line  or  segment.  The  answer  we 
have  adopted  to  these  questions  is  given  in  the  theory  of  irra 
tional  numbers  created  by  Cantor  and  Dedekind  [see  Vol.  I, 
Chap.  II],  and  in  the  notion  of  a  continuous  function  due  to 
Cauchy  and  Weierstrass  [see  Vol.  I,  Chap.  VII]. 

These  definitions  of  continuity  are  analytical.  With  them  we 
can  reason  with  the  utmost  precision  and  rigor.  The  consequences 
we  deduce  from  them  are  sufficiently  in  accord  with  our  intuition 
to  justify  their  employment.  We  can  show  by  purely  analytic 
methods  that  a  continuous  function /(V)  does  attain  its  extreme 
values  [I,  354],  that  if  such  a  function  takes  on  the  value  a  at  the 
point  P,  and  the  value  b  at  the  point  Q,  then  it  takes  on  all  inter 
mediary  values  between  a,  b,  as  x  ranges  from  P  to  Q  [I,  357]. 
We  can  also  show  that  a  closed  curve  without  double  point  does 
form  the  boundary  of  a  complete  region  [cf.  576  seq.]. 

567.  4°  Property.     Tangents.     To  begin  with,  what  is  a  tangent  ? 
Euclid  defines  a  tangent  to  a  circle  as  a  straight  line  which  meets 


PLANE   CURVES  581 

the  circle  and  being  produced  does  not  cut  it  again.  In  com 
menting  on  tliis  definition  Casey  says,  "  In  modern  geometry  a 
curve  is  made  up  of  an  infinite  number  of  points  which  are 
placed  in  order  along  the  curve,  and  then  the  secant  through  two 
consecutive  points  is  a  tangent."  If  the  points  on  a  curve  were 
like  beads  on  a  string,  we  might  speak  of  consecutive  points.  As, 
however,  there  are  always  an  infinite  number  of  points  between  any 
two  points  on  a  continuous  curve,  this  definition  is  quite  illusory. 

The  definition  we  have  chosen  is  given  in  I,  365.  That  property 
3°  does  not  hold  at  each  point  of  a  continuous  curve  was  brought 
out  in  the  discussion  of  property  1°.  Not  only  is  it  not  necessary 
that  a  curve  has  a  tangent  at  each  of  its  points,  but  a  curve  does 
not  need  to  have  a  tangent  at  a  pantactic  set  of  points,  as  we  saw 
in  Chapter  XV. 

For  a  long  time  it  was  supposed  that  every  curve  has  a  tangent 
at  each  point,  or  if  not  at  each  point,  at  least  in  general.  Analytic 
ally,  this  property  would  go  over  into  the  following :  every  con 
tinuous  function  has  a  derivative.  A  celebrated  attempt  to  prove 
this  was  made  by  Ampere. 

Mathematicians  were  greatly  surprised  when  Weierstrass  ex 
hibited  the  function  we  have  studied  in  502  and  which  has  no 
derivative. 

Weierstrass*  himself  remarks:  "  Bis  auf  die  neueste  Zeit  hat 
man  allgemein  angenommen,  dass  eine  eindeutige  und  continuir- 
liche  Function  einer  reellen  Verandeiiichen  auch  stets  eine  erste 
Ableitung  habe,  deren  Werth  nur  an  einzelnen  Stellenunbestimmt 
oder  unendlich  gross  werden  konne.  Selbst  in  den  Schriften  von 
Gauss,  Cauchy,  Dirichlet  findet  sich  meines  Wissens  keine 
Ausserung,  aus  der  unzweifelhaft  hervorginge,  dass  diese  Mathe- 
matiker,  welche  in  ihrer  Wissenschaft  die  strengste  Kritik  iiberall 
zu  iiben  gewohnt  waren,  anderer  Ansicht  gewesen  seien." 

568.  Property  5°.  Length.  We  think  of  a  curve  as  having 
length.  Indeed  we  read  as  the  definition  of  a  curve  in  Euclid's 
Elements  :  a  line  is  length  without  breadth.  When  we  see  two 
simple  curves  we  can  often  compare  one  with  the  other  in  regard 
to  length  without  consciously  having  established  a  way  to  measure 

*  Werke,  vol.  2,  p.  71. 


582  GEOMETRIC   NOTIONS 

them.  Perhaps  we  unconsciously  suppose  them  described  at  a 
uniform  rate  and  estimate  the  time  it  takes.  It  may  be  that  we 
regard  them  as  inextensible  strings  whose  length  is  got  by 
straightening  them  out.  A  less  obvious  way  to  measure  their 
lengths  would  be  to  roll  a  straightedge  over  them  and  measure 
the  distance  on  the  edge  between  the  initial  and  final  points  of 
contact. 

We  ask  how  shall  we  formulate  arithmetically  our  intuitional 
ideas  regarding  the  length  of  a  curve  ?  The  intuitionist  says,  a 
curve  or  the  arc  of  a  curve  has  length.  This  length  is  expressed 
by  a  number  L  which  is  obtained  by  taking  a  number  of  points 
Pj,  P2,  P3--*  on  the  curve  between  the  end  points  P,  P',  and 
forming  the  sum 


The  limit  of  this  sum  as  the  points  became  pantactic  is  the 
length  L  of  the  arc  PP'. 

Our  point  of  view  is  different.  We  would  say  :  Whatever 
arithmetic  formulation  we  choose  we  have  no  a  priori  assurance 
that  it  adequately  represents  our  intuitional  ideas  of  length. 
With  the  intuitionist  we  will,  however,  form  the  sum  1)  and  see  if 
it  has  a  limit,  however  the  points  Pt  are  chosen.  If  it  has,  we  will 
investigate  this  number  used  as  a  definition  of  length  and  see  if  it 
leads  to  consequences  which  are  in  harmony  with  our  intuition. 

This  we  now  proceed  to  do. 

569.    1.    Let  Z 

be  one-valued  continuous  functions  of  t  in  the  interval  21  =  (a  <  5). 
As  t  ranges  over  51  the  point  x,  y  will  describe  a  curve  or  an  arc 
of  a  curve  O.  We  might  agree  to  call  such  curves  analytic,  in 
distinction  to  those  given  by  our  intuition.  The  interval  51  is 
the  interval  corresponding  to  O. 

Let  D  be  a  finite  division  of  21  of  norm  c?,  defined  by 


To  these  values  of  t  will  correspond  points 

p,p,,p,...e  (2 


PLANE   CURVES  583 

on  (7,  which  may  be  used  to  define  a  polygon  PD  whose  vertices 
are  2). 

Let  (m,  TTi  +  1)  denote  the  side  PmPm+1,  as  well  as  its  length. 
If  we  denote  the  length  of  PD  by  the  same  letter,  we  have 

1  ^  PD  (B 

exists,  it  is  called  the  length  of  the  arc  (7,  and  C  is  rectifiable. 

2.    (Jordan.)     For  the  arc  PQ  to  be  rectifiable,  it  is  necessary  and 
sufficient  that  the  functions  c/>,  ^  in  1)  have  limited  variation  in  51. 

For 


But  the  sum  on  the  right  is  the  variation  of  <f>  for  the  division  D. 
If  now  <f>  does  not  have  limited  variation  in  51,  the  limit  3)  does 
not  exist.  The  same  holds  for  ty.  Hence  limited  variation  is  a 
necessary  condition. 

The  condition  is  sufficient.     For 

PD<  2  |  Az  |  +  2  |  Ay  |  =  Var  <£  +  Var  ^. 

D  D 

As  <f>,  T/T  have  limited  variation,  this  shows  that 

P 
is  finite.      We  show  now  that 


P0  =  Max  PD 

D 


limPZ)  =  P0.  (4 

<f=0 


For  there  exists  a  division  A  such  that 


Let  A  cause  51  to  fall  into  v  intervals,  the  smallest  of  which  has 
the  length  X.  Let  D  be  a  division  of  51  of  norm  d<dQ<\. 
Then  no  interval  of  D  contains  more  than  one  point  of  A. 
Let  E=D  +  A. 


Obviously  PE>P 


or 


584  GEOMETRIC   NOTIONS 

Suppose  that  the  point  tK  of  A  falls  in  the  interval  (£t,  £t+1)  01 
D.  Then  the  chord  (t,  i  -f-  1)  in  PD  is  replaced  by  the  two  chords 
(t,  *),  (K,  i  +  1)  in  PE-  Hence 


where  ».£  C^)  +  (<•  +  1^  -  <•,  V+  1)  . 

Obviously  as  <£,  -^  are  continuous  we  may  take  dQ  so  small  that 
each 

G-K<£-     ,     for  any  d<d0. 

'-  V 

Hence  '  Pg-PD<e-.  (6 

From  5),  6)  we  have 

PQ-PD<€     ,     for  any  d  <  d0, 
which  gives  4). 

3.  If  the  arc  PQ  is  rectifiable,  any  arc  contained  in  PQ  is  also 
rectifiable. 

For  (/>,  i/r  having  limited  variation  in  interval  51,  have  a  fortiori 
limited  variation  in  any  segment  of  51. 

4.  Let  the  rectifiable  arc  C  fall  into  two  arcs  C1  ,  C2  .      If  s,  *j  ,  s2 
are  the  lengths  of  (7,  C\,  <72,  tf/ew, 

S    =     *j    +    8y  (T 

For  we  saw  that  (7X,  (72  are  rectifiable  since  (7  is.  Let  ^  ,  5I2 
be  the  intervals  in  51  corresponding  to  6\,  (72.  Let  Dv  D2  be 
divisions  of  ^,  ?12  °^  norm  ^-  Then 

«!  =  lim  PD.     ,     s2  =  limPn. 
d=o  rf=o 

But  Dj,  D2  effect  a  division  of  21,  and  since 

s  =  lim  PA,  (8 

e=0 

with  respect  to  the  class  of  all  divisions  of  51,  the  limit  8)  is  the 
same  when  E  is  restricted  to  range  over  divisions  of  the  type  of  D. 
Now 

Pj>-Pft+*V 

Passing  to  the  limit,  we  get  7). 


PLANE   CURVES  585 

The  preceding  reasoning  also  shows  that  if  Cl  ,  (72  are  rectifiable 
curves,  then  C  is,  and  7)  holds  again. 

5.    If  1)  define  a  rectifiable  curve,  its  length  s  is  a  continuous  func 
tion  s(f)  of  t. 

For  (f>,  ^r  having  limited  variation, 


where  the  functions  on  the  right  are  continuous  monotone  increas 
ing  functions  of  t  in  the  interval  51  =  («  <  ^). 

For  a  division  D  of  norm  d  of  the  interval  A21  =  (t,  t  +  A)  we 

have 

PD  =  2 


4- 


where  B^  =  c/>1(^  +  h)  —  <£(0>  an(i  similarly  for  the  other  func 
tions.  As  c^j  is  continuous,  8^  =  0,  etc.,  as  h  =  0.  We  may 
therefore  take  77  >  0  so  small  that  S^,  S(£2,  8-v^j,  3^2  <  e/4,  if  A  <  77. 

Hence  As  =  s(t  +  k)  -  s(t)  <  ^lax  P^  <  e     ,     if  0  <  h  >  77. 

Thus  s  is  continuous. 

6.  The  length  s  of  the  rectifiable  arc  C  corresponding  to  the  inter 
val  (a  <  t)  is  a  monotone  increasing  function  of  t. 

This  follows  from  4. 

7.  If  x,  y  do  not  have  simultaneous  intervals  of  invariability,  s(t) 
is  an  increasing  function  of  t.      The  inverse  function  is  one-valued 
and  increasing  and  the  coordinates  x,  y  are  one-  valued  functions  of  s. 

That  the  inverse  function  t  (s)  is  one-valued  follows  from  I,  214. 
We  can  thus  express  t  in  terms  of  s,  and  so  eliminate  t  in  1). 

570.    1.    If  <$>'  ,  ty'  are  continuous  in  the  interval  51, 

8=  fdt^^  +  ^'t.  (1 


s  =  Km  2Ac£2-f-  A^2.  (2 


586 
Now 


GEOMETRIC   NOTIONS 


where  ^,  £"  lie  in  the  interval  Af*. 

As  (//,  -*//  are  continuous  they  are  uniformly  continuous.    Hence 
for  any  division  D  of  norm  <  some  c?0, 


where  |  «K    ,    |  /3K  |  <  some  77,  small  at  pleasure,  for  any  K.     Thus 


and  we  may  take 


=  lim 


Hence 


j; 


< 


which  establishes  1). 

For  simplicity  we  have  assumed  <£',  ^'  to  be  continuous  in 
This  is  not  necessary,  as  the  following  shows. 

2.    Let  ar  «..  aB,  b^  --  bn>0  but  not  all  =  0. 
Then          , 


For 


=  1,  2 


Hence 


Vaf  + V5J 


But 


This  in  5)  gives  4). 


PLANE   CURVES  587 

Let  us  apply  4)  to  prove  the  following  theorem,  more  general 
than  1. 

3.    (Baire.)     If  <£',  -^  are  limited  and  R  integrable,  then 

8 

For  by  4), 


2 < 


4>K  _  yK  =  r 

where  ^j,  ??"  are  numerically  <1.      Thus 

!  S^K^AC  —  ^-&K^K  \  =  ^^/e7?*  Osc  (£>'  +  28K7^^'  Osc  ijr1 .  (6 

As  <£',  >/r'  are  integrable,  the  right  side  =  0,  as  d  =  0.     Now 

lira 


Thus  passing  to  the  limit  in  6),  we  have 

Km  SA^V(£'(^)2  +  A/r'(t')2=  f- 

^21 

This  with  2),  3)  gives  1)  at  once. 

571.  Volterra's  Curve.  It  is  interesting  to  note  that  there  are 
rectifiaUe  curves  for  which  <£'(£)>  V^CO  are  not  both  R-integr  able. 
Such  a  curve  is  Volterra's  curve,  discussed  in  503.  Let  its  equa 
tion  be  2/=/(z).  Then  f  (x)  behaves  as 

2  x  sin  --  cos  - 

X  X 

in  the  vicinity  of  a  non  null  set  in  31  =  (0,  1).      Hence  f'(x)  is 
not  ^-integrable  in  51.      But  then  it  is  easy  to  show  that 


does  not  exist.     For  suppose  that 


VI 


588  GEOMETRIC   NOTIONS 

were  .R-integrable.  Then  #2  =  1  +/'(V)2  is  ,R-integrable,  and 
hence  /'(^)2  also.  But  the  points  of  discontinuity  of  f'2  in  51  do 
not  form  a  null  set.  Hence  /'2  is  not  .K-integrable. 

On  the  other  hand,  Volterra's  curve  is  rectifiable  by  569,  2,  and 

528,  i. 

572.    Taking  the  definition  of  length  given  in  569,  1,  we  saw 
that  the  coordinates 


must  have  limited  variation  for  the  curve  to  be  rectifiable.  But  we 
have  had  many  examples  of  functions  not  having  limited  variation 
in  an  interval  21.  Thus  the  curve  defined  by 

y  =x  sin-     ,     x^  0 

(4 


does  not  have  a  length  in  21  =  (—  1,  1)  ;  while 

y  =  x2  sin  -     ,     x  =£  0 

x  (5 

=0     ,     x=0 
does. 

It  certainly  astonishes  the  na'ive  intuition  to  learn  that  the 
curve  4)  has  no  length  in  any  interval  8  about  the  origin  how 
ever  small,  or  if  we  like,  that  this  length  is  infinite,  however  small 
8  is  taken.  For  the  same  reason  we  see  that 

No  arc  of  Weierstrass'  curve  has  a  length  (or  its  length  is  infinite) 
however  near  the  end  points  are  taken  to  each  other,  ivhen  ab>l. 

573.  1.  6°  Property.  Space-filling  Curves.  We  wish  now  to 
exhibit  a  curve  whlcli  passes  through  every  point  of  a  square,  i.e. 
which  completely  fills  a  square.  Having  seen  how  to  define  one 
such  curve,  it  is  easy  to  construct  such  curves  in  great  variety,  not 
only  for  the  plane  but  for  space.  The  first  to  show  how  this  may 
be  done  was  Peano  in  1890.  The  curve  we  wish  now  to  define  is 
due  to  Hilbert. 

We  start  with  a  unit  interval  51  =  (0,  1)  over  which  t  ranges, 
and  a  unit  square  33  over  which  the  point  x,  y  ranges.  We  define 


PLANE   CURVES 


589 


as  one-valued  continuous  functions  of  t  in  51  so  that  xy  ranges  over 
53  as  t  ranges  over  51.  The  analytic  curve  O  defined  by  1)  thus 
completely  fills  the  square  53. 

We  do  this  as  follows.  We  effect  a  division  of  51  into  four 
equal  segments  SJ,  B'2,  S3,  8£,  and  of  53  into  equal  squares  77^,  77^, 
773,  774,  as  in  Fig.  1. 

We  call  this  the  first  division  or  D^.  The  corre 
spondence  between  51  and  53  is  given  in  first 
approximation  by  saying  that  to  each  point  P  in 
B[  shall  correspond  some  point  Q  in  v[ . 

We  now  effect  a  second  division  D2  by  dividing 
each  interval  and  square  of  J)1  into  four  equal 
parts. 

We  number  them  as  in  Fig.  2, 

X"  %"  W 

01       »       °2        •"       *M 


As  to  the  numbering  of  the  rfs  we  observe  the 
following  two  principles :  1°  we  may  pass  over  the 
squares  1  to  16  continuously  without  passing  the 
same  square  twice,  and  2°  in  doing  this  we  pass 
over  the  squares  of  Dl  in  the  same  order  as  in  FIG.  2. 

Fig.  1.     The  correspondence  between  5(  and  53  is 
given  in  second  approximation  by  saying  that  to  each  point  P  in 
B[f  shall  correspond  some  point  Q  in  rj{'.     In  this  way  we  continue 
indefinitely. 

To  find  the  point  Q  in  53  corresponding  to  P  in  51  we  observe 
that  P  lies  in  a  sequence  of  intervals 

8'  >S"  >B"r  >  •••  =0,  (2 

to  which  correspond  uniquely  a  sequence  of  squares 

V  >T,"  >r>'"  >..-  =0.  (3 

The  sequence  3)  determines  uniquely  a  point  whose  coordinates 
are  one-valued  functions  of  £,  viz.   the  functions  given  in  1). 

The  functions  1)  are  continuous  in  51. 

For  let  t'  be  a  point  near  t ;  it  either  lies  in  the  same  interval  as 
t  in  Dn  or  in  the  adjacent  interval.     Thus  the  point  Qf  corre- 


590  GEOMETRIC    NOTIONS 

spending  to  t'  either  lies  in  the  same  square  of  Dn  as  the  point  Q 
corresponding  to  £,  or  in  an  adjacent  square.  But  the  diagonal 
of  the  squares  =  0,  as  n  =  oo.  Thus 


Thus 
both  =  0,  as  t'  =  t. 

As  t  ranges  over  51,  the  point  x,  y  ranges  over  every  point  in  the 
square  53. 

For  let  Q  be  a  given  point  of  53.  It  lies  in  a  sequence  of 
squares  as  3).  If  Q  lies  on  a  side  or  at  a  vertex  of  one  of  the  rj 
squares,  there  is  more  than  one  such  sequence.  But  having  taken 
such  a  sequence,  the  corresponding  sequence  2)  is  uniquely  de 
termined.  Thus  to  each  Q  corresponds  at  least  one  P.  A  more 
careful  analysis  shows  that  to  a  given  Q  never  more  than  four 
points  P  can  correspond. 

2.  The  method  we  have  used  here  may  obviously  be  extended 
to  space.  By  passing  median  planes  through  a  unit  cube  we 
divide  it  into  23  equal  cubes.  Thus  to  get  our  correspondence 
each  division  Dn  should  divide  each  interval  and  cube  of  the  pre 
ceding  division  Dn_1  into  23  equal  parts.  The  cubes  of  each  divi 
sion  should  be  numbered  according  to  the  1°  and  2°  principles  of 
enumeration  mentioned  in  1. 

By  this  process  we  define 


as  one-valued  continuous  functions  of  t  such  that  as  t  ranges  over 
the  unit  interval  (0,  1),  the  point  a?,  #,  z  ranges  over  the  unit 
cube. 

574.  1.  Hilbert's  Curve.  We  wish  now  to  study  in  detail  the 
correspondence  between  the  unit  interval  51  and  the  unit  square 
53  afforded  by  Hilbert's  curve  denned  in  573.  A  number  of  inter 
esting  facts  will  reward  our  labor.  We  begin  by  seeking  the 
points  P  in  51  which  correspond  to  a  given  Q  in  53- 

To  this  end  let  us  note  how  P  enters  and  leaves  an  TJ  square. 
Let  B  be  a  square  of  Dn.  In  the  next  division  B  falls  into  four 


PLANE   CURVES  591 

squares  Bl  •••  B±  and  in  the  n  4-  2d  division  in  16  squares  StJ. 
Of  these  last,  four  lie  at  the  vertices  of  B ;  we  call  them  vertex 
squares.  The  other  12  are  median  squares.  A  simple  considera 
tion  shows  that  the  rj  squares  of  Dn+2  are  so  numbered  that  we 
always  enter  a  square  B  belonging  to  Dn,  and  also  leave  it  by  a 
vertex  square. 

Since  this  is  true  of  every  division,  we  see  on  passing  to  the 
limit  that  the  point  Q  enters  and  leaves  any  77  square  at  the  ver 
tices  of  ?;.  We  call  this  the  vertex  law. 

Let  us  now  classify  the  points  P,  Q. 

If  P  is  an  end  point  of  some  division  Dn  >  we  call  it  a  terminal 
point,  otherwise  an  inner  point,  because  it  lies  within  a  sequence 
of  8  intervals  B'  >  B"  >  •••  =  0. 

The  points  Q  we  divide  into  four  classes : 

1°  vertex  points,  when  Q  is  a  vertex  of  some  division. 

2°  inner   points,    when    Q   lies    within   a  sequence  of   squares 

y>7/'>...  =o. 

3°  lateral  points,  when  Q  lies  on  a  side  of  some  77  square  but 
never  at  a  vertex. 

4°  points  lying  on  the  edge  of  the  original  square  33.  Points 
of  this  class  also  lie  in  1°,  3°. 

We  now  seek  the  points  P  corresponding  to  a  Q  lying  in  one  of 
these  four  classes. 

Class  1°.  Q  a  Vertex  Point.  Let  Dn  be  the  first  division  such 
that  Q  is  at  a  vertex.  Then  Q  lies  in  four  squares  TJL,  ?/,•,  TJK,  ^  of 

!>,. 

There  are  5  cases  : 

a)  ij  k  I  are  consecutive. 

yS)  ij  k  are  consecutive,  but  not  I. 

7)  ij  are  consecutive,  but  not  k  I. 

8)  ij,  also  k  I,  are  consecutive, 
e)  no  two  are  consecutive. 

A  simple  analysis  shows  that  a),  /3)  are  not  permanent  in  the 
following  divisions ;  7),  8)  may  or  may  not  be  permanent ;  e)  is 
permanent. 


592  GEOMETRIC   NOTIONS 

Now,  whenever  a  case  is  permanent,  we  can  enclose  Q  in  a  se 
quence  of  7]  squares  whose  sides  =  0.  To  this  sequence  corre 
sponds  uniquely  a  sequence  cf  &  intervals  of  lengths  =  0.  Thus 
to  two  consecutive  squares  will  correspond  two  consecutive  inter 
vals  which  converge  to  a  single  point  P  in  21.  If  the  squares  are 
not  consecutive,  the  corresponding  intervals  converge  to  two  dis 
tinct  points  in  31.  Thus  we  see  that  when  7)  is  permanent,  to  Q 
correspond  three  points  P.  When  8)  is  permanent,  to  Q  corre 
spond  two  points  P.  While  when  Q  belongs  to  e),  four  points  P 
correspond  to  it. 

Class  2°.  Q  an  Inner  Point.  Obviously  to  each  Q  corresponds 
one  point  P  and  only  one. 

Glass  3°.  Q  a  Lateral  Point.  To  fix  the  ideas  let  Q  lie  on  a  ver 
tical  side  of  one  of  the  T/'S.  Let  it  lie  between  ??t,  r;;-  of  Dn.  There 
are  two  cases  : 

a)  j  =  i  +  1. 


We  see  easily  that  a)  is  not  permanent,  while  of  course  ft)  is. 
Thus  to  each  Q  in  class  3°,  there  correspond  two  points  P. 

Class  4°.  Q  lies  on  the  edge  of  33.  If  Q  is  a  vertex  point,  to  it 
may  correspond  one  or  two  points  P.  If  Q  is  not  a  vertex  point, 
only  one  point  P  corresponds  to  it. 

To  sum  up  we  may  say  : 

To  each  inner  point  Q  corresponds  one  inner  point  P. 

To  each  lateral  point  Q  correspond  two  points  P. 

To  each  edge  point  Q  correspond  one  or  two  points  P. 

To  each  vertex  point  Q,  correspond  two,  three,  or  four  points  P. 

2.  As  a  result  of  the  preceding  investigation  we  show  easily 
that  : 

To  the  points  on  a  line  parallel  to  one  of  the  sides  of  23  correspond 
in  51  an  apantactic  perfect  set. 

3.  Let  us  now  consider  the  tangents  to  Hilbert's  curve  which 
we  denote  by  H. 


PLANE   CURVES 


593 


$ 

7. 

ft+i 

Q 

%+i 

Let  Q  be  a  vertex  point.  We  saw  there  were  three  permanent 
cases  7),  S),  e). 

In  cases  7),  8)  we  saw  that  to  two  consecutive  B  intervals  cor 
respond  permanently  two  contiguous  ver 
tical  or  horizontal  squares. 

Thus  as   t  ranges   over  '  —  =  -  '  -  =  —  '     o 

Ot  0<+i 

ot,  ot+1,  the  point  #,  y  ranges 

over  these  squares,  and  the  secant  line 

joining  Q  and  this  variable  point  #,  y   oscillates  through   180°. 

There  is  thus  no  tangent  at  Q.     In  case  e)  we  see  similarly  that 

the  secant  line  ranges  through  90°.      Again  there  is  no  tangent 

at  Q. 

In  the  same  way  we  may  treat  the  three  other  classes.  We  find 
that  the  secant  line  never  converges  to  a  fixed  position,  and  may 
oscillate  through  360°,  viz.  when  Q  is  an  inner  point.  As  a  result 
we  see  that  Hubert's  curve  has  at  no  point  a  tangent,  nor  even  a 
unilateral  tangent. 

4.    Associated  with  Hilbert's  curve  ^Tare  two  other  curves, 
a;  =0(0     ,     and  ^  =  ^(0. 

The  functions  <£,  T/T  being  one-valued  and  continuous  in  H,  these 
curves  are  continuous  and  they  do  not  have  a  multiple  point.  A 
very  simple  consideration  shows  that  they  do  not  have  even  a 
unilateral  tangent  at  a  pantactic  set  of  points  in  31. 


Pro£$rty  7°.  Equations  of  a  Curve.  As  already  remarked, 
it  is  commonly  thought  that  the  equation  of  a  curve  may  be 
written  in  any  one  of  the  three  forms 


y  =/O), 


(i 

(2 


and  if  these  functions  are  continuous,  these  equations  define  con 
tinuous  curves. 

Let  us  look  at  the  Hilbert  curve  H.  We  saw  its  equation 
could  be  expressed  in  the  form  3).  H  cuts  an  ordinate  at  every 
point  of  it  for  which  0  <  y  <  1.  Thus  if  we  tried  to  define  H  by 


594  GEOMETRIC   NOTIONS 

an  equation  of  the  type  1),  /(V)  would  have  to  take  on  every 
value  between  0  and  1  for  each  value  of  x  in  51  =  (0,  1).     No  such 
.  —  ^    functions  are  considered  in  analysis. 

WVXf  u\   Again,  we  saw  that  to  any  value  x  =  a  in  21  corresponds  a  perfect 

apantactic  set  of  values  \ta\  having  the  cardinal  number  c.     Thus 

the  inverse  function  of  x  =  <£(£)  is  a  many-valued  function  of  x 

whose  different  values  form  a  set  whose   cardinal  number  is  c. 

^  —  -A  Such  functions  have  not  yet  been  studied  in  analysis. 

How  is  it  possible  in  the  light  of  such  facts  to  say  that  we  may 
pass  from  3)  to  1)  or  2)  by  eliminating  t  from  3).  And  if  we 
cannot,  how  can  we  say  a  curve  can  be  represented  equally  well 
by  any  of  the  above  three  equations,  or  if  the  curve  is  given  by 
one  of  these  three  equations,  we  may  suppose  it  replaced  by  one 
of  the  other  two  whenever  convenient.  Yet  this  is  often  done. 

In  this  connection  we  may  call  attention  to  the  loose  way 
elimination  is  treated.  Suppose  we  have  a  set  of  equations 


We  often  see  it  stated  that  one  can  eliminate  ^  •••  tn  and  obtain 
a  relation  involving  the  #'s  alone.  Any  reasoning  based  on  such 
a  procedure  must  be  regarded  as  highly  unsatisfactory,  in  view  of 
what  we  have  just  seen,  until  this  elimination  process  has  been 
established. 

576.  Property  8».  Closed  Curves.  A  circle,  a  rectangle,  an 
ellipse  are  examples  of  closed  curves.  Our  intuition  tells  us  that 
it  is  impossible  to  pass  from  the  inside  to  the  outside  without 
crossing  the  curve  itself.  If  we  adopt  the  definition  of  a  closed 
curve  without  multiple  point  given  in  I,  362,  we  find  it  no  easy 
matter  to  establish  this  property  which  is  so  obvious  for  the  simple 
closed  curves  of  our  daily  experience.  The  first  to  effect  the 
demonstration  was  Jordan  in  1892.  We  give  here  *  a  proof  due 
to  de  la  ValUe-Poussin.-\ 

Let  us  call  for  brevity  a  continuous  curve  without  double  point 

*  The  reader  is  referred  to  a  second  proof  due  to  Brouwer  and  given  in  598  seq. 
t  Cours  tf  Analyse,  Paris,  1903,  Vol.  1,  p.  307. 


PLANE   CURVES  595 

a  Jordan  curve.  A  continuous  closed  curve  without  double  point 
will  then  be  a  closed  Jordan  curve.  Cf.  I,  362. 

577.    Let  0  be  a  closed  Jordan  curve.      However  small  <r  >  0  is 
taken,  there  exists  a  polygonal  ring  R  containing  C  and  such  that 

1°  Each  point  of  R  is  at  a  distance  <  a  from  0. 

2°  Each  point  of  C  is  at  a  distance  <  a-  from  the  edges  of  R. 

For  let  x  =  0(0     ,     y  =  i/r(0  (1 

be  continuous  one-valued  functions  of  t  in  T  =(#<£>)  defining  C. 
Let  D  =  (a,  ax,  <z2  •••  6)  be  a  division  of  T  of  norm  d.  Let 
a,  «j,  «2  •••  be  points  of  0  corresponding  to  a,  al  •••  If  d  is  suffi 
ciently  small,  the  distance  between  two  points  on  the  arc 
<7t  =  (at_i,  at)  is  <e',  small  at  pleasure.  Let  A  be  a  quadrate 
division  of  the  x,  y  plane  of  norm  8.  Let  us  shade  all  cells  con 
taining  a  point  of  (7t.  These  form  a  connected  domain  since  C,  is 
continuous.  We  can  thus  go  around  its  outer  edge  without  a 
break.*  If  this  shaded  domain  contains  unshaded  cells,  let  us 
shade  these  too.  We  call  the  result  a  link  A,  .  It  has  only  one 
edge  En  and  the  distance  between  any  two  points  of  Et  is  ob 
viously  <  e'  +  2  V2  8.  We  can  choose  d,  &  so  small  that 

e'  +  2V2  8  <  0-,          arbitrarily  small.  (1 

Then  the  distance  between  any  two  points  of  A,  is  <  er.  Let  e" 
be  the  least  distance  between  non-consecutive  arcs  CL.  We  take 
8  so  small  that  we  also  have 

-  (2 


Then  two  non-consecutive  links  AL,  Aj  have  no  point  in  common. 
For  then  their  edges  would  have  a.  common  point  P.  As  P  lies 
on  EL  its  distance  from  OL  is  <  V2  5.  Its  distance  from  Cy-  is  also 
<  V2  8.  Thus  there  is  a  point  Pt  on  (7t,  and  a  point  Pj  on  Cf  such 
that 


*  Here  and  in  the  following,  intuitional  properties  of  polygons  are  assumed  as 
known. 


596  GEOMETRIC   NOTIONS 

But  by  hypothesis  e"  <_  rj.     Hence 

e"<2V2S, 
which  contradicts  2). 

Thus  the  union  of  these  links  form  a  ring  R  whose  edges  are 
polygons  without  double  point.  One  of  the  edges,  say  Gt,  lies 
within  the  other,  which  we  call  Gr€  .  The  curve  0  lies  within  R. 
The  inner  polygon  6rt  must  exist,  since  non-consecutive  links  have 
no  point  in  common. 

578.  1.  Interior  and  Exterior  Points.  Let  <r1  >  <r2  >  •••  =  0. 
Let  Rl,  R2~-  be  the  corresponding  rings,  and  let 


be  their  inner  and  outer  edges.  A  point  P  of  the  plane  not  on 
0  which  lies  inside  some  Gr,  we  call  an  interior  or  inner  point  of  C. 
HP  lies  outside  some  Gre,  we  call  it  an  exterior  or  outer  point  of  C. 

Each  point  P  not  on  C  must  belong  to  one  of  these  two  classes. 
For  let  p  =  Dist  (P,  (7);  then  p  is  >  some  <rn.  It  therefore  lies 
within  6r(tn)  or  without  6r<n),  and  is  thus  an  inner  or  an  outer  point. 
Obviously  this  definition  is  independent  of  the  sequence  of  rings 
\Rn\  employed.  The  points  of  the  curve  Care  interior  to  each 
G-™  and  exterior  to  each  G-(n). 

Inner  points  must  exist,  since  the  inner  polygons  exist  as  al 
ready  observed.  Let  us  denote  the  inner  points  by  3  and  the 
outer  points  by  O.  Then  the  frontiers  of  3  and  £)  are  the  curve  C. 

2.    We  show  now  that 

1°   Two  inner  points  can  be  joined  by  a  broken  line  Ll  lying  in  $. 
2°   Two  outer  points  can  be  joined  by  a  broken  line  Le  lying  in  £). 
3°  Any  continuous  curve  ®  joining  an  inner  point  i  and  an  outer 
point  e  has  a  point  in  common  with  C. 

To  prove  3°,  let 


be  the  equations  of   $,  the  variable  t  ranging   over  an  interval 
,  t=a  corresponding  to  i  and  t=@  to  e.     Let  t'  be 


T= 


PLANE   CURVES  597 

such  that  a<t<t'  gives  inner  points,  while  t  =  tf  does  not  give  an 
inner  point.  Thus  the  point  corresponding  to  t  =  t'  is  a  frontier 
point  of  3  and  hence  a  point  of  O. 

To  prove  1°.  If  A,  B  are  inner  points,  they  lie  within  some  6rt . 
We  may  join  A,  B,  6rt  by  broken  lines  Za,  Z&  meeting  (7t  at  the 
points  A',  B',  say.  Let  G-^  be  the  part  of  6rt  lying  between  A', 
B1.  Then 

La  +  aab  +  Lb 

is  a  broken  line  joining  A  to  B. 
The  proof  of  2°  is  similar. 

579.  1.  Let  P',  P"  correspond  to  t  =  tr,  t  =  t",  on  the  curve  0 
defined  by  577,  l).  If  t'  <t",  we  say  P'  precedes  P"  and  write 
P'<P". 

Any  set  of  points  on  C  corresponding  to  an  increasing  set  of 
values  of  t  is  called  an  increasing  set. 

As  t  ranges  from  a  to  £>,  the  point  P  ranges  over  C  in  a  direct 
sense. 

We  may  thus  consider  a  Jordan  curve  as  an  ordered  set,  in  the 
sense  of  265. 

2.  (De  la  Vallee-Poussin.)  On  each  arc  Ot  of  the  curve  C,  there 
exists  at  least  one  point  Pj  such  that 

Jp1<p2<p3<...  a 

may  be  regarded  as  the  vertices  of  a  closed  polygon  without  double 
point  and  whose  sides  are  all  <  e. 

For  in  the  first  place  we  may  take  S  >  0  so  small  that  no  square 
of  A  contains  a  point  lying  on  non-consecutive  arcs  (7t  of  C.  Let 
us  also  take  A  so  that  the  point  a  corresponding  to  t  =  a  lies 
within  a  square,  call  it  S^  of  A.  As  t  increases  from  t  =  #,  there 
is  a  last  point  Pl  on  C  where  the  curve  leaves  Sr  The  point  P^ 
lies  in  another  square  of  A,  call  it  S2<  containing  other  points  of 
C.  Let  P2  be  the  last  point  of  C  in  S2 .  In  this  way  we  may 
continue,  getting  a  sequence  1). 

There  exists  at  least  one  point  of  1)  on  each  arc  C, .  For  other 
wise  a  square  of  A  would  contain  points  lying  on  non-consecutive 
arcs  OK .  The  polygon  determined  by  1)  cannot  have  a  double 


598  GEOMETRIC   NOTIONS 

point,  since  each  side  of  it  lies  in  one  square.  The  sides  are  <  e, 
provided  we  take  SV2  <  e,  since  the  diagonal  is  the  longest  line 
we  can  draw  in  a  square  of  side  S. 

580.  Existence  of  Inner  Points.  To  show  that  the  links  form  a 
ring  with  inner  points,  Schonfliess*  has  given  a  proof  which  may 
be  rendered  as  follows  : 

Let  us  take  the  number  of  links  to  be  even,  and  call  them  Z^, 
L2,--L2n.  Then  L^  L3,  L5~-  lie  entirely  outside  each  other. 
Since  L^  L2  overlap,  let  P  be  an  inner  common  point.  Simi 
larly  let  Q  be  an  inner  common  point  of  Z2,  L3.  Then  P,  Q 
lying  within  L2  may  be  joined  by  a  finite  broken  line  b  lying 
within  L2.  Let  62  be  that  part  of  it  lying  between  the  last  point 
of  leaving  L^  and  the  following  point  of  meeting  L3.  In  this 
way  the  pairs  of  links 

T    T  T     T 

X/j^g        ,        ^3^5        I  ••' 

define  finite  broken  lines 


No  two  of  these  can  have  a  common  point,  since  they  lie  in 
non-consecutive  links.     The  union  of  the  points  in  the  sets 


we  call  a  ring,  and  denote  it  by  $.  The  points  of  the  plane  not 
in  $  fall  into  two  parts,  separated  by  $.  Let  2  denote  the  part 
which  is  limited,  together  with  its  frontier.  We  call  X  the  inte 
rior  of  9t  That  X  has  inner  points  is  regarded  as  obvious  since 
it  is  defined  by  the  links 


which  pairwise  have  no  point  in  common,  and  by  the  broken  lines 

fi2     ,     Z>4     ,     #6  ••• 

each  of  which  latter  lies  entirely  within  a  link. 
Let  £     =  l>v  (          £)     ••         m  =  1,  2,  ... 


*  Die  Entwickelung  der  Lehre  von  den  Punktmannigfaltigkeiten.     Leipzig,  1908, 
Part  2,  p.  170. 


PLANE   CURVES  599 

Then  these  £  have  pairwise  no  point  in  common  since  the  L2m 
have  not. 

Let  £  =  ?a  +  ?4+-  +82n  +  fl. 

Then  $  >  0.  For  let  us  adjoin  L2  to  Sft,  getting  a  ring  9?2  whose 
interior  call  £2.  That  £2  aas  inner  points  follows  from  the  fact 
that  it  contains  ?4,  £6  •••  Let  us  continue  adjoining  the  links 
L±<  L6  •-  Finally  we  reach  Z2n,  to  which  corresponds  the 
ring  $R2n,  whose  interior,  if  it  exists,  is  £2n.  If  £2n  does  not  exist, 
^2n-2  contains  only  £2n.  This  is  not  so,  for  on  the  edge  of  L^ 
bounding  <£,  is  a  point  P,  such  that  some  Dp(P)  contains  points 
of  no  L  except  Lr  In  fact  there  is  a  point  P  on  the  edge  of  Ll 
not  in  either  L2  or  Z2n,  as  otherwise  these  would  have  a  point  in 
common.  Now,  if  however  small  p  >  0  is  taken,  7>P(P)  contains 
points  of  some  L  other  than  L^  the  point  P  must  lie  in  LK  which 
is  absurd,  since  L^  has  only  points  in  common  with  £2,  L2n,  and 
P  is  not  in  either  of  these.  Thus  the  adjunction  of  L2,  L±,  ••• 
L2n  produces  a  ring  9?2n  whose  interior  £2n  does  not  reduce  to  0  ; 
it  has  inner  points. 

581.  Prggerti^  9°.  Area.  That  a  figure  defined  by  a  closed 
curve  without  double  point,  i.e.  the  interior  of  a  Jordan  curve, 
has  an  area,  has  long  been  an  accepted  fact  in  intuitional  geometry. 
Thus  Lindemann,  Vorlesungen  uber  G-eometrie,  vol.  2,  p.  557,  says 
"  einer  allseitig  umgrenzten  Figur  kommt  ein  bestimmter  Flachen- 
inhalt  zu."  The  truth  of  such  a  statement  rests  of  course  on 
the  definition  of  the  term  area.  In  I,  487,  702  we  have  given  a 
definition  of  area  for  any  limited  plane  point  set  51  which  reduces 
to  the  ordinary  definition  when  51  becomes  an  ordinary  plane  figure. 
In  our  language  51  has  an  area  when  its  frontier  points  form  a 
discrete  set.  Let 


define    a   Jordan    curve  (£,  as   t   ranges  over  T=(a<b).  The 

figure  51  defined  by  this  curve  has  the  curve  as  frontier.  In  I, 

708,   710,  we  gave  various  cases  in  which   (£  is  discrete.  The 
reasoning  of  I,  710,  gives  us  also  this  important  case  : 

If  one  of  the  continuous  functions  ^>,  -fy  defining  the  Jordan  curve 
(£,  has  limited  variation  in  T,  then  (£  is  discrete. 


600 


GEOMETRIC   NOTIONS 


It  was  not  known  whether  (£  would  remain  discrete  if  the  con 
dition*  of  limited  variation  was  removed  from  both  coordinates, 
until  Osgood  *  exhibited  a  Jordan  curve  which  is  not  discrete. 
This  we  will  now  discuss. 

.    582.    1.    Osgood' s    Curve.       We    start    with    a    unit    segment 
T '  =  (0,  1)  on  the  t  axis,  and  a  unit  square  S  in  the  xy  plane. 

We  divide  jTinto  17  equal  parts 


.12345  1C  17  rjj       F7J  rn  s~\ 

d 

and  the  square  $  into  9  equal 
squares 

by  drawing  4  bands  J?x  which 
are  shaded  in  the  figure.  On 
these  bands  we  take  8  segments, 

marked  heavy  in  the  figure. 

Then  as  t  is  ranging  from  left 
to  right  over  the  even  or  black 

intervals  T2,  T4,  •••  Tu  marked  heavy  in  the  figure,  the  point  x,  y 
on  Osgood's  curve,  call  it  £),  shall  range  univariantly  over  the 
segments  3). 

While  t  is  ranging  over  the  odd  or  white  intervals  2\,  T3  •••  T17 
the  point  xy  on  £)  shall  range  over  the  squares  2)  as  determined 
below. 

Each  of  the  odd  intervals  1)  we  will  now  divide  into  17  equal 
intervals  T^  and  in  each  of  the  squares  2)  we  will  construct 
horizontal  and  vertical  bands  E2  as  we  did  in  the  original  square 
$.  Thus  each  square  2)  gives  rise  to  8  new  segments  on  £) 
corresponding  to  the  new  black  intervals  in  T,  and  9  new  squares 
jSLJ>  corresponding  to  the  white  intervals.  In  this  way  we  may 
continue  indefinitely. 

The  points  which  finally  get  in  a  black  interval  call  /3,  the 
others  are  limit  points  of  the  /3's  and  we  call  them  X.  The  point 


*  Trans.  Am.  Math.  Soc.,  vol.  4  (1903),  p.  107. 


PLANE   CURVES  601 

on  D  corresponding  to  a  (3  point  has  been  defined.  The  point  of 
O  corresponding  to  a  point  X  is  defined  to  be  the  point  lying  in 
the  sequence  of  squares,  one  inside  the  other,  corresponding  to  the 
sequence  of  white  intervals,  one  inside  the  other,  in  which  X  falls, 
in  the  successive  divisions  of  T. 

Thus  to  each  t  in  T  corresponds  a  single  point  #,  y  in  8.  The 
aggregate  of  these  points  constitutes  Osgood's  curve.  Obviously 
the  #,  y  of  one  of  its  points  are  one-valued  functions  of  t  in  T,  say 

(4 


The  curve  D  has  no  double  point.  This  is  obvious  for  points  of 
£)  lying  in  black  segments.  Any  other  point  falls  in  a  sequence 
of  squares 

S,>S^>S^^ 

to  which  correspond  intervals 


in  which  the  corresponding  fs  lie.  But  only  one  point  t  is  thus 
determined. 

The  functions  4)  are  continuous.  This  is  obvious  for  points  j3 
lying  within  the  black  intervals  of  T.  It  is  true  for  the  points  X. 
For  X  lies  within  a  sequence  of  white  intervals,  and  while  t  ranges 
over  one  of  these,  the  point  on  £)  ranges  in  a  square.  But  these 
squares  shut  down  to  a  point  as  the  intervals  do.  Thus  $,  i/r  are 
continuous  at  t  =  X.  In  a  similar  manner  we  show  they  are  con 
tinuous  at  the  end  points  of  the  black  intervals. 

We  note  that  to  t  =  0  corresponds  the  upper  left-hand  corner 
of  S,  and  to  t  =  1,  the  diagonally  opposite  point. 

2.  Up  to  the  present  we  have  said  nothing  as  to  the  width  of 
the  shaded  bands  „  D 

-E>1      •>      B\  " 

introduced  in  the  successive  steps.     Let 

A  =  a1  +  a2  + 

be  a  convergent  positive  term  series  whose  sum  A<1.  We 
choose  Bl  so  that  its  area  is  a1^  B^  so  that  its  area  is  #2,  etc. 

Then  c->      A          cS      1        i  /£ 

£)  =  0,£j  =  l  —  -A,  (o 


602  GEOMETRIC   NOTIONS 

as  we  now  show.     For  £)  has    obviously    only    frontier    points ; 
hence  Q  =  0.     Since  £)  is  complete,  it  is  measurable  and 

5  =  6. 

Let  0=  #-O,  and  B=  \Bn\.  Then  0  <  B.  For  any  point 
which  does  not  lie  in  some  Bn  lies  in  a  sequence  of  convergent 
squares  ^  >  /Srt/  >  •••  which  converge  to  a  point  of  £).  Now 

S=S1+S2+  ...  =A. 

On  the  other  hand,  B  contains  a  null  set  of  points  of  O,  viz.  the 
black  segments.     Thus 

0  =  S  =  A     ,     and  hence  5  =  1  —  A 
and  5)  is  established. 

Thus  OsgoocTs  curve  is  continuous,  has  no  double  point,  and  its 
upper  content  is  1  —  A. 

3.  To  get  a  continuous  closed  curve  C  without  double  point 
we  have  merely  to  join  the  two  end  points  a,  ft  of  Osgood's  curve 
by  a  broken  line  which  does  not  cut  itself  or  have  a  point  in  com 
mon  with  the  square  S  except  of  course  the  end  points  a,  ft. 
Then  C  bounds  a  figure  g  whose  frontier  is  not  discrete,  and  g 
does  not  have  an  area.  Let  us  call  such  curves  closed  Osgood 
curves. 

Thus  we  see  that  there  exist  regions  bounded  by  Jordan  curves 
which  do  not  have  area  in  the  sense  current  since  the  Greek 
geometers  down  to  the  present  day. 

Suppose,  however,  we  discard  this  traditional  definition,  and 
employ  as  definition  of  area  its  measure.  Then  we  can  say  : 

A  figure  g  formed  of  a  closed  Jordan  curve  J  and  its  interior  ^ 
has  an  area,  viz.  Meas  g. 

For  Front  g  =  J.  Hence  g  is  complete,  and  is  therefore  rneas- 
ureable. 

We  note  that  &       T  ,  ^ 

tf  =  «/  +  J- 

We  have  seen  there  are  Jordan  curves  such  that 

J>0. 


DETACHED  AND  CONNECTED  SETS         603 

We  now  have  a  definition  of  area  which  is  in  accordance  with  the 
promptings  of  our  geometric  intuition.  It  must  be  remembered, 
however,  that  this  definition  has  been  only  recently  discovered, 
and  that  the  definition  which  for  centuries  has  been  accepted  leads 
to  results  which  flatly  contradict  our  intuition,  which  leads  us  to 
say  that  a  figure  bounded  by  a  continuous  closed  curve  has  an 
area. 

583.  At  this  point  we  will  break  off  our  discussion  of  the 
relation  between  our  intuitional  notion  of  a  curve,  and  the  con 
figuration  determined  by  the  equations 


where  $,  ty  are  one-valued  continuous  functions  of  t  in  an  interval 
T.  Let  us  look  back  at  the  list  of  properties  of  an  intuitional 
curve  drawn  up  in  563.  We  have  seen  that  the  analytic  curve 
1)  does  not  need  to  have  tangents  at  a  pantactic  set  of  points  on 
it;  no  arc  on  it  needs  have  a  finite  length;  it  may  completely  fill 
the  interior  of  a  square  ;  its  equations  cannot  always  be  brought 
in  the  forms  y=f(x)  or  F(xy)=Q,  if  we  restrict  ourselves  to 
functions  /or  F  employed  in  analysis  up  to  the  present;  it  does 
not  need  to  have  an  area  as  that  term  is  ordinarily  understood. 

On  the  other  hand,  it  is  continuous,  and  when  closed  and  with 
out  double  point  it  forms  the  complete  boundary  of  a  region. 

Enough  in  any  case  has  been  said  to  justify  the  thesis  that 
geometric  reasoning  in  analysis  must  be  used  with  the  greatest 
circumspection. 

• 

Detached  and  Connected  Sets 

584.  In  the  foregoing  sections  we  have  studied  in  detail  some 
of  the  properties  of  curves  defined  by  the  equations 


Now  the  notion  of  a  curve,  like  many  other  geometric  notions,  is 
independent  of  an  analytic  representation.  We  wish  in  the  fol 
lowing  sections  to  consider  some  of  these  notions  from  this  point 
of  view. 


604  GEOMETRIC   NOTIONS 

585.    1.    Let  51,  53  be  point  sets  in  w-way  space  9?m.     If 


we  say  51,  53  are  detached.  If  51  cannot  be  split  up  into  two  parts 
53,  (£  such  that  they  are  detached,  we  say  51  has  no  detached  parts. 
If  51  =  53  +  (£  and  Dist  (53,  £)>  0,  we  say  53,  (£  are  detached  parts 

of  a. 

Let  the  set  of  points,  finite  or  infinite, 

a,  ax,  «2,  •••  6  (1 

be  such  that  the  distance  between  two  successive  ones  is  <  e.  We 
call  1)  an  e-sequence  between  a,  b  ;  or  a  sequence  with  segments 
(«t,  «t+1)  of  length  <  e.  We  suppose  the  segments  ordered  so 
that  we  can  pass  continuously  from  a  to  b  over  the  segments  without 
retracing.  If  1)  is  a  finite  set,  the  sequence  is  finite,  otherwise 
infinite. 

2.  Let  51  have  no  detached  parts.     Let  a,  b  be  two  of  its  points. 
For  each  e  >  0,  there  exists  a  finite  e-sequence  between  a,  b,  and  lying 

•        c\v 

in  51. 

For  about  a  describe  a  sphere  of  radius  e.  About  each  point  of 
5(  in  this  sphere  describe  a  sphere  of  radius  e.  About  each  point 
of  51  in  each  of  these  spheres  describe  a  sphere  of  radius  e.  Let 
this  process  be  repeated  indefinitely.  Let  53  denote  the  points  of 
51  made  use  of  in  this  procedure.  If  53  <  51,  let  (£  =  51  —  53.  Then 
Dist  (53,  £)>€,  an(^  51  has  detached  parts,  which  is  contrary  to 
hypothesis.  Thus  there  are  sets  of  e-spheres  in  51  joining  a  and  b. 

Among  these  sets  there  are  finite  ones.  For  let  g  denote  the 
set  of  points  in  51  which  may  be  joined  to  a  by  finite  sequences  ;  let 
©  =  51  -  g.  Then  Dist  (g,  ®)  >  e.  For  if  <  e,  there  is  a  point  / 
in  g,  and  a  point  g  in  ®  whose  distance  is  <  e.  Then  a  and  g  can 
be  joined  by  a  finite  e-sequence,  which  is  contrary  to  hypothesis. 

3.  If  51  has  no  detached  parts,  it  is  dense. 

For  if  not  dense,  it  must  have  at  least  one  isolated  point  a. 
But  then  a,  and  51  —  a  are  detached  parts  of  51,  which  contradicts 
the  hypothesis. 

4.  Let  51,  53,  S  be  complete  and  51  =  (53,  6).     If  51  has  no  de 
tached  parts,  53,  (5  ^ave  at  least  one  common  point. 


IMAGES  605 

For  if  23,  (£  have  no  common  point,  8  =  Dist  (23,  d)  is  >  0. 
But  8  cannot  >  0,  -since  23,  (£  would  then  be  detached  parts  of  21. 
Since  &  =  0  and  since  23,  (£  are  complete,  they  have  a  point  in 
common. 


5.  If  21  i«  sw<?A  £A«£  any  two  of  its  points  may  be  joined   by  an 
e-sequence  lying  in  21,  where  e  >  0  is  small  at  pleasure,  21  has  no 
detached  parts. 

For  if  21  had  23,  <£  as  detached  parts,  let  Dist  (23,  <£)  =  8.  Then 
8  >  0.  Hence  there  is  no  sequence  joining  a  point  of  23  with  a 
point  of  (£  with  segments  <  8. 

6.  If  21  is  complete  and  has  no  detached  parts,  it  is  said  to  be 
connected.     We  also  call  21  a  connex. 

As  a  special  case,  a  point  may  be  regarded  as  a  connex. 

7.  If  21  is  connected,  it  is  perfect. 

For  by  3  it  is  dense,  and  by  definition  it  is  complete. 

8.  If  21  is  a  rectilinear  connex,  it  has  a  first  point  a  and  a  last 
point  /3,  and  contains  every  point  in  the  interval  (a,  /3). 

For  being  limited  and  complete  its  minimum  and  maximum 
lie  in  21  and  these  are  respectively  a  and  0.  Let  now 


There  exists  an  ersequence  Cl  between  a,  0.  Each  segment  has 
an  e2-sequence  (72.  Each  segment  of  (72  has  an  e3-sequence  (73, 
etc.  Let  O  be  the  union  of  all  these  sequences.  It  is  pantactic 
in  (a,  yS).  As  21  is  complete, 


Images 

586.    Let         ^./W-U     •••     *-n=/n(*i-O  (1 

be  one-valued  functions  of  t  in  the  point  set  £.     As  t  ranges  over 
X,  the  point  x  =  (xl  •••  xn)  will  range  over  a  set  21  in  an  w-way 
space  9JB.     We  have  called  21   the  image  of   X.     Cf.   I,  238j  3.    ^  |4 
If  the  functions  /  are  not  one-valued,  to  a  point  t  may  correspond 
several  images  xr,  x"  •••  finite  or  infinite  in  number.     Conversely 


606  GEOMETRIC   NOTIONS 

to  the  point  x  may  correspond  several  values  of  t.  If  to  each 
point  t  correspond  in  general  r  values  of  #,  and  to  each  x  in 
general  s  values  of  £,  we  say  the  correspondence  between  £,  31  is 
r  to  s.  If  r  =  s  =  1  the  correspondence  is  1  to  1  or  unifold  ;  if 
r  >  1,  it  is  manifold.  If  r  =  1,  31  is  a  simple  image  of  £,  other 
wise  it  is  a  multiple  image.  If  the  functions  1)  are  one- valued 
and  continuous  in  £,  we  say  31  is  a  continuous  image  of  £. 

587.    Transformations  of  the  Plane.     Example  1.     Let 

u  =  x  sin  y     ,     v  =  x  cos  y.  (1 

We  have  in  the  first  place 

u^  +  v2  =  x2. 

This  shows  that  the  image  of  a  line  x  =  a,  a  =£  0,  parallel  to  the 
?/-axis  is  a  circle  whose  center  is  the  origin  in  the  u,  v  plane,  and 
whose  radius  is  a.  To  the  ^/-axis  in  the  a?,  y  plane  corresponds 
the  origin  in  the  u,  v  plane. 

From  1)  we  have,  secondly, 

-  =  tan  y. 

v 

This  shows  that  the  image  of  a  line  y  =  6,  is  a  line  through  the 
origin  in  the  u,  v  plane. 

From  1)  we  have  finally  that  w,  v  are  periodic  in  y,  having  the 
period  2  TT.  Thus  as  x,  y  ranges  in  the  band  B,  formed  by  the 
two  parallels  y=  ±  TT,  or  —  TT  <  y  <  TT,  the  point  u,  v  ranges  over 
the  entire  u,  v  plane  once  and  once  only. 

The  correspondence  between  B  and  the  u,  v  plane  is  unifold, 
except,  as  is  obvious,  to  the  origin  in  the  it,  v  plane  corresponds 
the  points  on  the  y-axis. 

Let  us  apply  the  theorem  of  I,  441,  on  implicit  functions.  The 
determinant  A  is  here 


—  —  x. 


sin  ?/,          cos  y 
x  cos  y,  —  x  sin  y 

As  this  is •=£  0  when  x,  y  is  not  on  the  «/-axis,  we  see  that  the 
correspondence  between  the  domain  of  any  such  point  and  its 
image  is  1  to  1.  This  accords  with  what  we  have  found  above. 


IMAGES  607 

It  is,  however,  a  much  more  restricted  result  than  we  have  found  ; 
for  we  have  seen  that  the  correspondence  between  any  limited 
point  set  21  in  B  which  does  not  contain  a  point  of  the  y-axis  and 
its  image  is  unifold. 

588.    Example  2.     Let 


u 


the  radical  having  the  positive  sign.     Let  us  find  the  image  of  the 
first  quadrant  Q  in  the  #,  y  plane. 
From  1)  we  have  at  once 


Hence  the  image  of  Q  is  a  band  B  parallel  to  the  v-axis. 
From  1)  we  get  secondly 

y  =  uv     ,     x  =  wVl  —  u2.  (2 

Hence 


Thus  the  image  of  a  circle  in  Q  whose  center  is  the  origin  and 
whose  radius  is  a  is  a  segment  of  a  right  line  v  =  a. 

When  x  =  y  =  0,  the  equations  1)  do  not  define  the  correspond 
ing  point  in  the  u,  v  plane.  If  we  use  2)  to  define  the  corre 
spondence,  we  may  say  that  to  the  line  v  =  0  in  B  corresponds  the 
origin  in  the  x,  y  plane.  With  this  exception  the  correspondence 
between  Q  and  B  is  uniform,  as  1),  2)  show. 

The  determinant  A  of  1)  is,  setting 


r  = 


d(w,  v)  _        r3         r3  —  x 


for  any  point  x,  y  different  from  the  origin. 

589.  Example  3.  Reciprocal  Radii.  Let  0  be  the  origin  in  the 
x,  y  plane  and  H  the  origin  in  the  u,  v  plane.  To  any  point 
P  =  (#,  y)  in  the  x,  y  plane  different  from  the  origin  shall  cor 
respond  a  point  Q  =  (u,  v)  in  the  w,  v  plane  such  that  n  Q  has 


608  GEOMETRIC   NOTIONS 

the  same  direction  as  OP  and  such  that  OP  •  £IQ  =  1.     Analyti 
cally  we  have 

x=\y     ,     u  =  \v     ,     \  >  0, 
and 


From  these  equations  we  get 

u  v  f+ 

x  =  ~2 2     '     y  =  ~TT~2  v 

and  also 


The  correspondence  between  the  two  planes  is  obviously  unifold 
except  that  no  point  in  either  plane  corresponds  to  the  origin  in 
the  other  plane.  We  find  for  any  point  a?,  y  different  from  the 

origin  that  a(M,  v}  J 

d(x,y)'    -(J  +  fyf 

Obviously  from  the  definition,  to  a  line  through  the  origin  in 
the  #,  y  plane  corresponds  a  similar  line  in  the  w,  v  plane.  As  xy 
moves  toward  the  origin,  w,  v  moves  toward  infinity. 

Let  x,  y  move  on  the  line  x  =  a  =£  0.  Then  1)  shows  that  w,  v 
moves  along  the  circle 

a  (>2  +  v2)  -  u  =  0 

which  passes  through  the  origin.     A  similar  remark  holds  when 
z,  y  moves  along  the  line  y  =  b  =£  0. 

590.  Such  relations  between  two  point  sets  51,  33  as  defined  in 
586  may  be  formulated  independently  of  the  functions  /.  In  fact 
with  each  point  a  of  H  we  may  associate  one  or  more  points  51?  bz  ••• 
of  55  according  to  some  law.  Then  33  may  be  regarded  as  the 
image  of  SI.  We  may  now  define  the  terms  simple,  manifold,  etc., 
as  in  586.  When  b  corresponds  to  a  we  may  write  b  ~  a. 

We  shall  call  33  a  continuous  image  of  51  when  the  following  con 
ditions  are  satisfied.  1°  To  each  a  in  51  shall  correspond  but  one 
b  in  33,  that  is,  33  is  a  simple  image  of  H.  2°  Let  b  ~  a,  let  at,  «2  ••• 
be  any  sequence  of  points  in  51  which  =  #.  Let  bn  ~  an.  Then 
bn  must  =  Z>  however  the  sequence  \an\  is  chosen. 


IMAGES  009 

When  53  is  a  simple  image  of  51,  the  law  which  determines 
which  b  of  53  is  associated  with  a  point  a  of  51  determines  obviously 
n  one-valued  functions  as  in  586,  1),  where  ^  •••  tm  are  the  m  co 
ordinates  of  a,  and  xl  •••  xn  are  the  n  coordinates  of  b.  We  call  these 
functions  1)  the  associated  functions.  Obviously  when  53  is  a 
continuous  image,  the  associated  functions  are  continuous  in  51. 

591.  1.  Let  53  be  a  simple  continuous  image  of  the  limited  complete 
set  5(.  Then  1°  53  is  limited  and  complete.  If  2°  51  is  perfect  and 
only  a  finite  number  of  points  of  51  correspond  to  any  point  0/53,  then 
53  is  perfect.  -5^3°  51  is  a  connex,  so  is  53. 

To  prove  1°.  The  case  that  53  is  finite  requires  no  proof.  Let 
ftj,  £2  "•  be  points  of  53  which  =  /9.  We  wish  to  show  that  0  lies 
in  53.  To  each  bn  will  correspond  one  or  more  points  in  51;  call 
the  union  of  all  these  points  a.  Since  53  is  a  simple  image,  a  is  an 
infinite  set.  Let  av  #2  "'  be  a  set  of  points  in  a  which  =  «,  a 
limiting  point  of  51.  As  51  is  complete,  a  lies  in  51.  Let  b  ~  a. 
Let  b,n  ~  an.  As  an  =  a,  bln  =  /3.  But  53  being  continuous,  b^ 
must  =  b.  Thus  /3  lies  in  53.  That  53  is  limited  follows  from  the 
fact  that  the  associated  functions  are  continuous  in  the  limited 
complete  set  51.  To  prove  2°.  Suppose  that  53  had  an  isolated 
point  b.  Let  b  ~  a.  Since  51  is  perfect,  let  a^  a2>~  =  a.  Let 
bn  ~  an.  Then  as  53  is  continuous,  bn  =  5,  and  b  is  not  an  isolated 
point.  To  prove  3°.  We  have  only  to  show  that  there  exists 
an  e-sequence  between  any  two  points  a,  /3  of  53,  e  small  at  pleasure. 
Let  a  ~  a,  @  ~  b.  Since  51  is  connected  there  exists  an  ^-sequence 
between  a,  b.  Also  the  associated  functions  are  uniformly  con 
tinuous  in  51,  and  hence  77  may  be  taken  so  small  that  each  segment 
of  the  corresponding  sequence  in  53  is  >  e. 

2.  Let  f{t1  •••  £TO)  be  one-valued  and  continuous  in  the  connex  51, 
then  the  image  of  51  is  an  interval  including  its  end  points. 

This  follows  from  the  above  and  from  585,  8. 

3.  Let  the  correspondence  between  51,  53  be  unifold.     If  53  is  a 
continuous  image  of  51,  then  51  is  a  continuous  image  of  53. 

For  let  \bn\  be  a  set  of  points  in  53  which  =  b.  Let  an  ~  5n, 
a  ~  b.  We  have  only  to  show  that  an  =  a.  For  suppose  that  it 
does  not,  suppose  in  fact  that  there  is  a  sequence  ati,  ati  •••  which 


610  GEOMETRIC   NOTIONS 

=  a  3=  a.     Let  {3  ~  a.     Then  5tl,  ba  •••  =  /3.      But  any  partial  se 
quence  of  jfinj  must  =  b.     Tims  &  =  /3,  hence  a  =  «,  hence  an  =  a. 

4.  w4  Jordan  curve  J  is  a  unifold  continuous  image  of  an  interval 
T.  Conversely  if  J  is  a  unifold  continuous  image  of  an  interval  T, 
there  exist  two  one-valued  continuous  functions 


such  that  as  t  ranges  over  T,  the  point  x,  y  ranges  over  J.     In  case 
J  is  closed  it  may  be  regarded  as  the  image  of  a  circle  F. 

All  but  the  last  part  of  the  theorem  has  been  already  established. 
To  prove  the  last  sentence  we  have  only  to  remark  that  if  we  set 

x  =  r  cos  t     ,     y  =  r  sin  t 

we  have  a  unifold  continuous  correspondence  between  the  points 
of  the  interval  (0,  2  TT*)  and  the  points  of  a  circle. 

5.  The  first  part  of  4  may  be  regarded  as  a  geometrical  definition 
of  a  Jordan  curve.  The  image  of  a  segment  of  the  interval  T  or 
of  the  circle  F,  will  be  called  an  arc  of  J. 

592.  Side  Lights  on  Jordan  Curves.  These  curves  have  been 
defined  by  means  of  the  equations 


As  t  ranges  over  the  interval  T  =  (a  <  5),  the  point  P  =  (x,  y) 
ranges  over  the  curve  J.  This  curve  is  a  certain  point  set  in  the 
#,  y  plane.  We  may  now  propose  this  problem  :  We  have  given 
a  point  set  (£  in  the  a?,  y  plane  ;  may  it  be  regarded  as  a  Jordan 
curve  ?  That  is,  do  there  exist  two  continuous  one-valued  func 
tions  1)  such  that  as  t  ranges  over  some  interval  T,  the  point  P 
ranges  over  the  given  set  (£  without  returning  on  itself,  except 
possibly  for  t  =  a,  t  =  b,  when  the  curve  would  be  closed? 

Let  us  look  at  a  number  of  point  sets  from  this  point  of  view. 

593.    Example  1. 

L    Let  y  =  sin  -     ,     x  in  the  interval  %  =  (-  1,  1),  but  ^  0 
x 

=  0          for  x  =  Q. 


IMAGES  611 

Is  this  point  set  (£  a  Jordan  curve  ?  The  answer  is,  No.  For  a 
Jordan  curve  is  a  continuous  image  of  an  interval  51.  By  591,  1, 
it  is  complete.  But  (E  is  not  complete,  as  all  the  points  on  the 
y  axis,  —  1  <  y  <  1  are  limiting  points  of  (£,  and  only  one  of  them 
belongs  to  (£,  viz.  the  origin. 

2.  Let  us  modify  (£  by  adjoining  to  it  all  these  missing  limiting 
points,  and  call  the  resulting  point  set  (7.      Is  C  a  Jordan  curve  ? 
The  answer  is  again,  No.     For  if  it  were,  we  can  divide  the  inter 
val  T  into  intervals  8  so  small  that  the  oscillation  of  c£,  ^  in  any 
one  of  them  is  <  &>.     To  the  intervals  8,  will  correspond  arcs  Ot  on 
the  curve,  and  two  non-consecutive  arcs  Ct  are  distant  from  each 
other  by  an  amount  >  some  e,  small  at  pleasure.     This  shows  that 
one  of  these  arcs,  say  CK,  must  contain  the  segment  on  the  y-axis 
~~  1  ^  V  ^  !•     But  then  Osc  ^r  =  2  as  t  ranges  over  the  correspond 
ing  8K  interval.     Thus  the  oscillation  of  i/r  cannot  be  made  <  e, 
however  small  £K  is  taken. 

3.  Let  us  return  to  the  set  (£  defined  in  1.     Let  A,  B  be  the 
two  end  points  corresponding  to  x  =  —  1,  x  =  1.      Let  us  join  them 
by  an  ordinary  curve,  a  polygon  if  we  please,  which  does  not  cut 
itself  or  (£.     The  resulting  point  set  $  divides  all  the  other  points 
of  the  plane  into  two  parts  which  cannot  be  joined  by  a  contin 
uous  curve  without  crossing  $.     For  this  point  of  view  $  must  be 
regarded  as  a  closed  configuration.    Yet  $  is  obviously  not  complete. 

On  the  other  hand,  let  us  look  at  the  curve  formed  by  removing 
the  points  on  a  circle  between  two  given  points  a,  b  on  it.  The 
remaining  arc  %  including  the  end  points  a,  b  is  a  complete  set,  but 
as  it  does  not  divide  the  other  points  of  the  plane  into  two  sepa 
rated  parts,  we  cannot  say  £  is  a  closed  configuration. 

We  mention  this  circumstance  because  many  English  writers 
use  the  term  closed  set  where  we  have  used  the  term  complete. 
Cantor,  who  first  introduced  this  notion,  called  such  sets  abge- 
schlossen,  which  is  quite  different  from  geschlossen  =  closed. 

_! 

594.  Example  2.  Let  p  =  e  e ',  for  6  in  the  interval  31  =  (0,  1) 
except  6  =  0,  where  p  =  0.  These  polar  coordinates  may  easily  be 
replaced  by  Cartesian  coordinates 

-i  -1 

e  'cos  6     ,        =  e   9  sin  d     ,     in  51, 


612  GEOMETRIC    NOTIONS 

except  6  =  0,  when  x,  y  both  =  0.     The  curve  thus  denned  is  a 
Jordan  curve. 

Let  us  take  a  second  Jordan  curve 


with  p  =  0  for  6  =  0.  If  we  join  the  two  end  points  on  these 
curves  corresponding  to  6  =  1  by  a  straight  line,  we  get  a  closed 
Jordan  curve  J",  which  has  an  interior  <J,  and  an  exterior  O. 

The  peculiarity  of  this  curve  J  is  the  fact  that  one  point  of  it, 
viz.  the  origin  #  =  ;z/  =  0,  cannot  be  joined  to  an  arbitrary  point 
°f  3s  ky  a  finite  broken  line  lying  entirely  in  $  ;  nor  can  it  be 
joined  to  an  arbitrary  point  in  £)  by  such  a  line  lying  in  £)• 

595.    1.    It  will  be  convenient  to  introduce  the  following  terms. 
Let  31  be  a  limited  or  unlimited  point  set  in  the  plane.     A  set 
of  distinct  points  in  21 

«i     »     «2     »     <V"  (1 

determine  a  broken  line.  In  case  1)  is  an  infinite  sequence,  let  an 
converge  to  a  fixed  point.  If  this  line  has  no  double  point,  we  call 
it  a  chain,  and  the  segments  of  the  line  links.  In  case  not  only  the 
points  1)  but  also  the  links  lie  in  21,  we  call  the  chain  a  path.  If 
the  chain  or  path  has  but  a  finite  number  of  links,  it  is  called 
finite. 

Let  us  call  a  precinct  a  region,  i.e.  a  set  all  of  whose  points  are 
inner  points,  limited  or  unlimited,  such  than  any  two  of  its  points 
may  be  joined  by  a  finite  path. 

2.  Using  the  results  of  578,  we  may  say  that,  — 

A  closed  Jordan  curve  J  divides  the  other  points  of  the  plane  into 
two  precincts,  an  inner  $  and  an  outer  £)•  Moreover,  they  have  a 
common  frontier  which  is  J. 

3.  The  closed  Jordan  curve  considered  in  594  shows  that  not 
every  point  of  such  a  closed  Jordan  curve  can  always  be  joined  to 
an  arbitrary  point  of  3  or  O  by  a  finite  path. 

Obviously  it  can  by  an  infinite  path.  For  about  this  point,  call 
it  P,  we  can  describe  a  sequence  of  circles  of  radii  r  =  0.  Between 
any  two  of  these  circles  there  lie  points  of  Q  and  of  £),  if  r  is  suf- 


IMAGES  613 

liciently  small.  In  this  way  we  may  get  a  sequence  of  points  in  3, 
viz.  /j,  /2  ...  =  P.  Any  two  of  these  Im,  Im+1  may  be  joined  by  a 
path  which  does  not  cut  the  path  joining  /j  to  Im.  For  if  a  loop 
were  formed,  it  could  be  omitted. 

4.  Any  arc  &  of  a  closed  Jordan  curve  J  can  be  joined  by  a  path 
to  an  arbitrary  point  of  the  interior  or  exterior,  which  call  51. 

For  let  «7=  $  -f-  £•  Let  &  be  a  point  of  $  not  an  end  point. 
Let  S  =  Dist(&,  £),  let  a  be  a  point  of  51  such  that  Dist(a,  &) 

<  ^  B.     Then  ~.  ox       1  . 

??=  Dist(a,  £)  >  Jo. 

Hence  the  link  I  =  (a,  &)  has  no  point  in  common  with  £.  Let 
b  be  the  first  point  of  I  in  common  with  $.  Then  the  link 
m  =  (a,  £)  lies  in  31.  If  now  a  is  any  point  of  21,  it  may  be  joined 
to  a  by  a  path  p.  Then  p  +  m  is  a  path  in  51  joining  the  arbi 
trary  point  a  to  a  point  b  on  the  arc  $. 

596.    Example  3.     For  d  in  51  =  (0*,  1)  let 


and  -O^iX 

p  =  a(H-«  v     <"). 

These  equations  in  polar  coordinates  define  two  non-intersecting 
spirals  jS^  Sz  which  coil  about  p  =  a  as  an  asymptotic  circle  F. 
Let  us  join  the  end  points  of  the  spirals  corresponding  to  0  =  1 
by  a  straight  line  L.  Let  §  denote  the  figure  formed  by  the 
spirals  S^  $2,  the  segment  L  and  the  asymptotic  circle  F.  Is  £ 
a  closed  Jordan  curve  ?  The  answer  is,  No.  This  may  be  seen 
in  many  ways.  For  example,  §  does  not  divide  the  other  points 
into  two  precincts,  but  into  three,  one  of  which  is  formed  of  points 
within  F. 

Another  way  is  to  employ  the  reasoning  of  593,  2.  Here  the 
circle  F  takes  the  place  of  the  segment  on  the  y-axis  which  figures 
there. 

Still  another  way  is  to  observe  that  no  point  on  F  can  be  joined 
to  a  point  within  S  by  a  path. 

597.  Example  4-  Let  d  be  formed  of  the  edge  &  of  a  unit 
square,  together  with  the  ordinates  o  erected  at  the  points 


614  GEOMETRIC   NOTIONS 

x  =  ™ ,  of  length  ^,  ft  =  1,  2  -      Although  (£  divides  the  other 

points  of  the  plane  into  two  precincts  3  and  D,  we  can  say  that 
($  is  not  a  closed  Jordan  curve. 

For  if  it  were,  3  and  £)  would  have  to  have  (£  as  a  common 
frontier.  But  the  frontier  of  £)  is  (§,  while  that  of  3  is  (£. 

That  (£  is  not  a  Jordan  curve  is  seen  in  other  ways.  For 
example,  let  7  be  an  inner  segment  of  one  of  the  ordinates  o. 
Obviously  it  cannot  be  reached  by  a  path  in  £). 


Brouwers  Proof  of  Jordan's  Theorem 

598.  We  have  already  given  one  proof  of  this  theorem  in  577 
seq.,  based  on  the  fact  that  the  coordinates  of  the  closed  curve  are 
expressed  as  one-valued  continuous  functions 


Brouwer's  proof  *  is  entirely  geometrical  in  nature  and  rests 
on  the  definition  of  a  closed  Jordan  curve  as  the  unifold  continu 
ous  image  of  a  circle,  cf.  591,  5. 

If  51,  53,  •••  are  point  sets  in  the  plane,  it  will  be  convenient  to 
denote  their  frontiers  by  g^,  g^  •••  so  that 

%^  =  Front  H     ,     etc. 

We  admit  that  any  closed  polygon  ty  having  a  finite  number  of 
sides,  without  double  point,  divides  the  other  points  of  the  plane 
into  an  inner  and  an  outer  precinct  $t,  tye  respectively.  In  the 
following  sections  we  shall  call  such  a  polygon  simple,  and  usu 
ally  denote  it  by  ty. 

We  shall  denote  the  whole  plane  by  (§. 

Then  <g=  ?+$.+?.. 

Let  51  be  complete.  The  complementary  set  A  is  formed,  as 
we  saw  in  328,  of  an  enumerable  set  of  precincts,  say  A  =  \An\. 

*  Math.  Annalen,  vol.  69  (1910),  p.  169. 


BROUWER'S   PROOF  OF  JORDAN'S   THEOREM  615 

599.  1.  If  a  precinct  31  and  its  complement*  A  each  contain  a 
point  of  the  connex  (£,  then  g^  contains  a  point  of  (L 

For  in  the  contrary  case  c  =  Dv(2I,  (£)  is  complete.  In  fact 
33  =  21  +  Sgi  is  complete.  As  (£  is  complete,  Dv($8,  (S)  is  com 
plete.  But  if  §21  does  not  contain  a  point  of  Q,  c  =  Dv(33,  (£). 
Thus  on  this  hypothesis,  c  is  complete.  Now  c  =  Dv(A,  (E)  is 
complete  in  any  case.  Thus  (£  =  c  +  <?,  which  contradicts  585,  4. 

2.  If  ^^  ^$e,  the  interior  and  exterior  of  a  simple  polygon  ty  each 
contain  a  point  of  a  connex  (£,  then  ty  contains  a  point  of  (L 

3.  Let  $  be  complete  and  not  connected.      There  exists  a  simple 
polygon  $  such  that  no  point  of  $  lies  on  $,  while  a  part  of  $  lies  in 
$t  and  another  part  in  tye. 

For  let  $j,  $2  be  two  non-connected  parts  of  $  whose  distance 
from  each  other  is  p  >  0.  Let  A  be  a  quadrate  division  of  the 
plane  of  norm  8,  so  small  that  no  cell  contains  a  point  of  $j  and 
$2.  Let  A!  denote  the  cells  of  A  containing  points  of  $j.  It  is 
complete,  and  the  complementary  set  A2  =  @  —  Aj  is  formed  of  one 
or  more  precincts.  No  point  of  ^l  lies  in  A2  or  on  its  frontier. 

Let  Pj,  P2  be  points  in  $j,  $2  respectively.  Let  D  be  that 
precinct  containing  P2.  Then  g^  embraces  a  simple  polygon  ^3 
which  separates  Pl  and  P2. 

4.  Let  ®1,  $2  be  two  detached  connexes.      There  exists  a  simple 
polygon  $  which  separates  them.      One  of  them  is  in  ^  the  other  in 
$e,  and  no  point  of  either  connex  lies  on  ^3. 

For  the  previous  theorem  shows  that  there  is  a  simple  polygon 
$  which  separates  a  point  Pl  in  ®1  from  a  point  P2  in  $2  and  no 
point  of  $j  or  f  2  lies  on  $.  Call  this  fact  F. 

Let  now  Pl  lie  in  $t .  Then  every  point  of  $x  lies  in  % .  For 
otherwise  ^  and  $e  each  contain  a  point  of  the  connex  $j .  Then 
2  shows  that  a  point  of  $j  lies  on  $,  which  contradicts  F. 

5.  Let   53    be    a  precinct   determined   by    the   connex   (L      Then 
b  =  Front  53  is  a  connex. 

*  Since  the  initial  sets  are  all  limited,  their  complements  may  be  taken  with  ref 
erence  to  a  sufficiently  large  square  O  ;  and  when  dealing  with  frontier  points,  points 
on  the  edge  of  O  may  be  neglected. 


616  GEOMETRIC   NOTIONS 

For  suppose  b  is  not  a  connex.  Then  by  3,  there  exists  a  simple 
polygon  ty  which  contains  a  part  of  b  in  ^  and  another  in  ^3e, 
while  no  point  of  b  lies  on  ty.  Hence  a  point  fi'  of  b  lies  in  $t, 
and  another  point  /3"  in  $„.  As  53  is  a  precinct,  let  us  join  /3', 
fi'f  by  a  path  v  in  53-  Thus  ty  contains  at  least  one  point  of  v, 
that  is,  a  point  of  53  lies  on  $.  As  b  and  ty  have  no  point  in 
common,  and  as  one  point  of  ty  lies  in  53>  all  the  points  of  ^  lie 
in  53.  Hence  ^(^  e)  =  0>  (1 

As  b  is  a  part  of  (£  and  hence  some  of  the  points  of  (£  are  in  $e 
and  some  in  ^^  it  follows  from  2  that  a  part  of  $  lies  in  (£.  This 
contradicts  1). 

6.  Let  $1?  $2  be  two  connexes  without  double  point.     By  3 
there  exists  a  simple  polygon  ty  which  separates  them  and  has 
one  connex  inside,  the  other  outside  ^3. 

Now  $  =  $j  +  $2  is  complete  and  defines  one  or  more  precincts. 
One  of  these  precincts  contains  ty. 

For  say  $  lay  in  two  of  these  precincts  as  51  and  53.  Then  the 
precinct  51  and  its  complement  (in  which  53  lies)  each  contain  a 
point  of  the  connex  $.  Thus  g^  contains  a  point  of  $.  But  g^ 
is  a  part  of  $,  and  no  point  of  $  lies  on  $. 

That  precinct  in  Coinp  $  which  contains  ^3  we  call  the  inter 
mediate  precinct  determined  by  $x,  $2,  or  more  shortly  the  pre 
cinct  between  $x,  $2  and  denote  it  by  Inter  ($r  $2). 

7.  Let  $j,  $2  be  two  detached  connexes,  and  let  !  =  Inter  ($r  $2). 
Then  $!,  $2  can  I e  joined  by  a  path  lying  in  I,  except  its  end  points 
which  lie  on  the  frontiers  of  $v  $2  respectively. 

For  by  hypothesis  p  =  Dist($j,  $2)>0.  Let  P1  be  a  point  of 
5^  such  that  some  domain  b  of  Pl  contains  only  points  of  $j  and 
of  I.  Let  Q!  be  a  point  of  f  in  b.  Join  Px,  Ql  by  a  right  line,  let 
it  cut  g^j  first  at  the  point  P' .  In  a  similar  way  we  may  reason 
on  $2,  obtaining  the  points  P",  Q2.  Then  P' Q^P"  is  the  path 
in  question.  If  we  denote  it  by  v,  we  may  let  v*  denote  this 
path  after  removing  its  two  end  points. 

8.  Let  $j,  $2  t>e  ^wo  detached  connexes.     A  path  v  joining  $x, 
$2  and  lying  in  1=  Inter  ($j,  $2),  end  points  excepted,  determines 
one  and  only  one  precinct  in  f . 


BROUWER'S   PROOF   OF   JORDAN'S   THEOREM  617 

For  from  an  arbitrary  point  P  in  !,  let  us  draw  all  possible 
paths  to  v.  Those  paths  ending  on  the  same  side  (left  or  right) 
of  v  certainly  lie  in  one  and  the  same  precinct  fr  or  !j  in  f.  Then 
since  one  end  point  of  v  is  inside,  the  other  end  point  outside  ^)3, 
there  must  be  a  part  of  ty  which  is  not  met  by  v  and  which  joins 
the  right  and  left  sides  of  v.  We  take  this  as  an  evident  property 
of  finite  broken  lines  and  polygons  without  double  points. 

Thus  !j  and  !r  are  not  detached ;  they  are  parts  of  one  precinct. 

9.  Two  paths  v^  v2  without  common  point,  lying  in  I  and  joining 
$j,  $2,  split  t  into  two  precincts. 

Let  i  =  !  —  vl ;  this  we  have  just  seen  is  a  precinct.  From  any 
point  of  it  let  us  draw  paths  to  i>2.  Those  paths  ending  on  the 
same  side  of  v2  determine  precincts  tj,  tr  which  may  be  identical. 
Suppose  they  are.  Then  the  two  sides  of  v2  can  be  joined  by  a 
path  lying  in  I,  which  does  not  touch  v2  (end  points  excepted), 
has  no  point  in  common  with  v1,  and  together  with  a  segment  of 
v%  forms  a  simple  polygon  ty  which  has  one  end  point  of  vl  in  ^Pt, 
the  other  end  point  in  tye.  Thus  by  2,  $  contains  a  point  of  the 
connex  vr  This  is  contrary  to  hypothesis. 

Similar  reasoning  shows  that 

10.  The  n  paths  v^  •••  vn  pair  wise  without  common  point,  lying  in 
f,  and  joining  the  connexes  $j,  $2  split  !  into  n  precincts. 

Let  us  finally  note  that  the  reasoning  of  595,  4,  being  independ 
ent  of  an  analytic  representation  of  a  Jordan  curve,  enables  us  to 
use  the  geometric  definition  of  591,  5,  and  we  have  therefore  the 
theorem 

11.  Let  51  be  a  precinct  whose  frontier  g  is  a  Jordan  curve.     Then 
there  exists  a  path  in  $t  joining  an  arbitrary  point  of  5(  with  any  arc 

0/8- 

Having  established  these  preliminary  theorems,  we  may  now 
take  up  the  body  of  the  proof. 

600.  1.  Let  51  be  a  precinct  determined  by  a  closed  Jordan  curve 
J.  Then  g  =  Front  51  is  identical  with  J. 

If  J  determines  but  one  precinct  51  which  is  pantactic  in  (£,  we 
have  obviously  5  =  J, 


618  GEOMETRIC   NOTIONS 

Suppose  then  that  51  is  a  precinct,  not  pantactic  in  (£.  Let  53 
be  a  precinct  =£  21  determined  by  g.  Let  b  =  Front  53.  Then 
b  <_  g  <^J.  Suppose  now  b  <  J.  As  J" is  a  connex  by  591,  1,  g  is  a 
connex  by  599,  5.  Similarly  since  g  is  a  connex,  b  is  a  connex. 
Since  b  <  </,  let  b  ~  b  on  the  circle  F  whose  image  is  J.  We 
divide  b  into  three  arcs  5X,  £>2,  63  to  which  ~  b1?  b2,  b3  in  b. 

Let  /3=  Inter  (bx,  b3). 

Then  by  599,  11,  we  can  join  bx,  b3  by  a  path  vl  in  51,  and  by  a 
path  vz  in  53.  By  599,  9,  these  paths  split  /2  into  two  precincts 
ffii  A-  We  can  join  v1?  #2  by  a  path  wx  lying  in  /3X,  and  by  a 
path  w2  lying  in  /32 . 

Now  the  precinct  53  and  its  complement  each  contain  a  point  of 
the  connex  Wj.  Hence  by  599,  l,  b  contains  a  point  of  ur  Simi 
larly  b  contains  a  point  of  u2.  Thus  u^  u2  cut  b,  and  as  they 
do  not  cut  bx,  b3  by  hypothesis,  they  cut  b2.  Thus  at  least  one 
point  of  fit  and  one  point  of  02  lie  in  b2 . 

Let  p  be  a  point  of  /^  lying  in  b2,  let  p  ~p  on  the  circle.  Let 
b'  be  an  arc  of  b2  containing  p.  Let  b'  ~  b' .  As  the  connex  b' 
has  no  point  in  common  with  Front  /3X,  b'  must  lie  entirely  in  /31 
by  599,  1.  This  is  independent  of  the  choice  of  b',  hence  the 
connex  b2,  except  its  end  points,  lies  in  @v  Thus  /32  can  contain 
no  point  of  b2,  which  contradicts  the  result  in  italics  above. 

Thus  the  supposition  that  b  <  J  is  impossible.  Hence  b  =  J, 
and  therefore  g  =  J. 

As  a  corollary  we  have  : 

2.  A  Jordan  curve  is  apantactic  in  (§. 

3.  A  closed   Jordan  curve   J  cannot    determine  more    than   two 
precincts. 

For  suppose  there  were  more  than  two  precincts 

"a,,  a,,  a,-  (i 

Let  us  divide  the  circle  T  into  four  arcs  whose  images  call  «7j,  J%, 

Ji,/4- 

Then  by  1,  the  frontier  of  each  of  the  precincts  1)  is  J.  Thus 
by  599,  9,  there  is  a  path  in  each  of  the  precincts  2lx,  ^  •••  join 
ing  Jj  and  J"3.  These  paths  split 


DIMENSIONAL   INVARIANCE  619 

!  =  Inter  (Jv  <73) 
into  precincts  fj,  I2  ••'• 

Now  as  in  1,  we  show  on  the  one  hand  that  each  lt  must  contain 
a  point  of  «72  or  <74,  and  on  the  other  hand  neither  J2  nor  J~4  can 
lie  in  more  than  one  !t. 

4.    A  dosed  Jordan  curve  J  must  determine  at  least  tivo  precincts. 

Suppose  that  J  determines  but  a  single  precinct  21.  From  a 
point  a  of  21  we  may  draw  two  non-intersecting  paths  M15  w2  to 
points  6j,  #2  of  J. 

Since  the  point  a  may  be  regarded  as  a  connex,  a  and  J  are  two 
detached  connexes.  Hence  by  599,  9,  the  paths  u^  uz  split  21  into 
two  precincts  2lx,  2Lj-  Let  j  =  (w19  w2,  J").  The  points  6X,  b2 
divide  J"into  two  arcs  «7X,  J"2,  and 


are  closed  Jordan  curves.  Regarding  a  and  Jj  as  two  detached 
connexes,  we  see  y\  determines  two  precincts,  «j,  o^.  By  599,  l,  a 
path  which  joins  a  point  ax  of  ax  with  a  point  az  of  Og  must  cut  jl 
and  hence  y.  It  cannot  thus  lie  altogether  in  ^  or  in  212  .  Thus 
both  «j,  a2  do  not  lie  in  2lj,  nor  both  in  212.  Let  us  therefore 
say  for  example  that  2lj  lies  in  «x,  and  2^  in  «2.  Hence  by  2, 
2lj  is  pantactic  in  «j,  and  2(2  in  «2-  -^7  ^'  eac^  P°int  of  jl  is  com 
mon  to  the  frontiers  of  ctj  and  of  Og,  and  hence  of  2IX  and  of  212, 
as  these  are  pantactic. 

Let  P  be  a  point  of  J2  .  It  lies  either  in  «j  or  ct^.  Suppose  it 
lies  in  Oj.  Then  it  lies  neither  in  c^  nor  on  Front  a^  and  hence 
neither  in  212  nor  on  Front  2I2..  But  every  point  of  /2  and  also 
every  point  of  jl  lies  on  Front  212.  We  are  thus  brought  to  a 
contradiction.  Hence  the  supposition  that  J  determines  but  a 
single  precinct  is  untenable. 


Dimensional  Invariance 

601.  1.  In  247  we  have  seen  that  the  points  of  a  unit  interval 
/,  and  of  a  unit  square  S  may  be  put  in  one  to  one  correspondence. 
This  fact,  due  to  Cantor,  caused  great  astonishment  in  the  mathe 
matical  world,  as  it  seemed  to  contradict  our  intuitional  views 


620  GEOMETRIC   NOTIONS 

regarding  the  number  of  dimensions  necessary  to  define  a  figure. 
Thus  it  was  thought  that  a  curve  required  one  variable  to  define 
it,  a  surface  two,  and  a  solid  three. 

The  correspondence  set  up  by  Cantor  is  not  continuous.  On 
the  other  hand  the  curves  invented  by  Peano,  Hilbert,  and  others 
(cf.  573)  establish  a  continuous  correspondence  between  /and  S, 
but  this  correspondence  is  not  one  to  one.  Various  mathemati 
cians  have  attempted  to  prove  that  a  continuous  one  to  one  corre 
spondence  between  spaces  of  m  and  n  dimensions  cannot  exist. 
We  give  a  very  simple  proof  due  to  Lebesgue.* 

It  rests  on  the  following  theorem  : 


2.    Let  51  be  a  point  set  in  9?m  .     Let  O  <  21  be  a  standard  cube 
aL<'2<T     ,     4=1,  2-~m. 


Let  (Sj,  ^-"be  a  finite  number  of  complete  sets  so  small  that  each 
lies  in  a  standard  cube  of  edge  a.  If  each  point  of  51  lies  in  one  of 
the  (S's,  there  is  a  point  of  51  ivhich  lies  in  at  least  m  +  1  of  them. 

Suppose  first  that  each  (£t  is  the  union  of  a  finite  number  of 
standard  cubes.  Let  (^  denote  those  (Ts  containing  a  point  of 
the  face  \l  of  Q  lying  in  the  plane  xl  =  ar  The  frontier  gx  of  (^ 
is  formed  of  a  part  of  the  faces  of  the  GTs.  Let  Fl  denote  that 
part  of  gj  which  is  parallel  to  fj.  Let  Ox  =  i)y(O,  .Fj).  Any 
point  of  it  lies  in  at  least  two  (Ts. 

Let  @2  denote  those  of  the  GTs  not  lying  altogether  in  @x  and 
containing  a  point  of  the  face  f2  of  Q  determined  by  x%  =  a2.  Let 
JP2  denote  that  part  of  Front  @2  which  is  parallel  to  f2.  Let 
O2  =  Dt^Qj,  F^).  Any  point  of  it'  lies  in  at  least  three  of  the  (Ts. 

In  this  way  we  may  continue,  arriving  finally  at  Om,  any  point 
of  which  lies  in  at  least  m  -\-  1  of  the  GTs. 

Let  us  consider  now  the  general  case.  We  effect  a  cubical 
division  of  space  of  norm  d<a.  Let  O,  denote  those  cells  of  D 
which  contain  a  point  of  (£t.  Then  by  the  foregoing,  there  is  a 
point  of  51  which  lies  in  at  least  m  +  1  of  the  (7's.  As  this  is  true, 
however  small  d  is  taken,  and  as  the  (£'  s  are  complete,  there  is  at 
least  one  point  of  51  which  lies  in  m  +  1  of  the  GTs. 

*  Math  Annalen,  vol.  70  (1911),  p.  166. 


DIMENSIONAL   INVARIANCE  621 

3.  We  now  note  that  the  space  $lm  may  be  divided  into  congruent 
cells  so  that  no  point  is  in  more  than  m  -h  1  cells. 

For  m  =  1  it  is  obvious.  For  m  =  2  we  may 
use  a  hexagonal  pattern.  We  may  also  use 
a  quadrate  division  of  norm  B  of  the  plane. 
These  squares  may  be  grouped  in  horizontal 
bands.  Let  every  other  band  be  slid  a  distance 
^  8  to  the  right.  Then  no  point  lies  in  more 
than  3  squares.  For  m  =  3  we  may  use  a 
cubical  division  of  space,  etc. 

In  each  case  no  point  of  space  is  in  more  than  m  +  1  cells. 

Let  us  call  such  a  division  a  reticulation  of  9?m . 

4.  Let  51  be  a  point  set  in  $?OT  having  an  inner  point  a.      There  is 
no  continuous  unifold  image  $8  of  51  in  9?n,  n^=m,  such  that  b~a  is 
an  inner  point  of  $8. 

For  let  n  >  m.  Let  us  effect  a  reticulation  R  of  9?m  of  norm  p. 
If  B  >  0  is  taken  sufficiently  small  A  =  Z>26(a)  lies  in  51.  Let 
E  =  D^d)  ;  if  p  is  taken  sufficiently  small,  the  cells 

o^o.-.o.  (i 

of  R  which  contain  points  of  E,  lie  in  A.  Let  the  image  of  E  be 
(£,  and  that  of  the  cells  1)  be 

SpG.-C..  (2 

These  are  complete.  Each  point  of  (5  lies  in  one  of  the  sets  2). 
Hence  by  2,  they  contain  a  point  /3  which  lies  in  n  +  1  of  them. 
Then  a~/3  lies  in  n  4- 1  of  the  cells  1).  But  these,  being  part  of 
the  reticulation  R,  are  such  that  no  point  lies  in  more  than  m  +  1 
of  them.  Hence  the  contradiction. 

602.    1.    Schotifliesi  Theorem.     Let 

u  =/O,  #)     ,     v  =  g(x,  y*)  (1 

be  one-valued  and  continuous  in  a  unit  square  A  whose  center  is 
the  origin.  These  equations  define  a  transformation  T.  If  T  is 
regular,  we  have  seen  in  I,  742,  that  the  domain  Z>P(P)  of  a  point 
P  =  (x,  y}  within  A  goes  over  into  a  set  E  such  that  if  Q~P 
then  -Z>a((?)  lies  in  E,  if  cr  >0  is  sufficiently  small. 


622  GEOMETRIC   NOTIONS 

These  conditions  on  /,  g  which  make  T  regular  are  sufficient, 
but  they  are  much  more  than  necessary  as  the  following  theorem 
due  to  Schonfliess  *  shows. 

2.  Let  A  =  B  -f-  c  be  a  unit  square  in  the  x,  y  plane,  whose  center 
is  the  origin  and  whose  frontier  is  c. 

u  =/(?*  y)     ,     v  =  g(x,  y) 

be  one-valued  continuous  functions  in  A.  As  (x,  y}  ranges  over  A, 
let  (w,  v)  range  over  21  =  53  +  c  where  c  ~  c.  Let  the  correspondence 
between  A  and  51  be  uniform.  Then  c  is  a  closed  Jordan  curve  and 
the  interior  c,  of  c  is  identical  with  53. 

That  c  is  a  closed  Jordan  curve  follows  from  576  seq.,  or  598 
seq.  Obviously  if  one  point  of  53  lies  in  C0  all  do.  For  if  &,  j3e 
are  points  of  53,  one  within  c  and  the  other  without,  let  Jt~&, 
be~@e-  Then  5t,  be  lying  in  B  can  be  joined  by  a  path  in  B 
which  has  no  point  in  common  with  c.  The  image  of  this  path  is 
a  continuous  curve  which  has  no  point  in  common  with  c,  which 
contradicts  578,  2. 

Let 


be  the  equation  of  c  in  polar  coordinates. 
If  0  <  ft  <  1,  the  equation 

P  =  14(0) 

defines  a  square,  call  it  CM,  concentric  with  c  and  whose  sides  are 
in  the  ratio  /*  :  1  with  those  of  c.     The  equations  of  CM  ~  c^  are 


v=g\-  .•-.......    j=  00,  0). 

These  CM  curves  have  now  the  following  property  : 

If  a  point  (p,  q)  is  exterior  {interior)  to  cMo,  it  is  exterior  (in 
terior)  to  CM  ,  for  all  fA  such  that 

I  /*  —  MO  I  ^  some  e  >  0. 

For  let  /3M  be  the  distance  of  (/?,  <?)  from  a  point  (w,  v)  on  CM. 
Then 


*Goettingen  Nachrichten,  1899.     The  demonstration  here  given  is  due  to  Osgood, 
Goett.  Nachr.,  1900. 


AREA   OF   CURVED  SURFACES  623 

is  a  continuous  function  of  6,  p  which  does  not  vanish  for  //,  =  /*0, 
when  0  <  6  <  2  TT.  But  being  continuous,  it  is  uniformly  con 
tinuous.  It  therefore  does  not  vanish  in  the  rectangle 

-  e  +  /i0  <  AC  <  AIO  +  e     ,     0  <  0  <  2  TT. 

We  can  now  show  that  if  53<c0  it  is  identical  with  ct.  To  this 
end  we  need  only  to  show  that  any  point  ft  of  ct  lies  on  some  CM. 
In  fact,  as  /x  =  0,  CM  contracts  to  a  point.  Thus  ft  is  an  outer  point 
of  some  CM,  and  an  inner  point  of  others.  Let  /u0  be  the  maximum 
of  the  values  of  n  such  that  ft  is  exterior  to  all  cu,  if  ft  < /v 
Then  ft  lies  on  cMo.  For  if  not,  ft  is  exterior  to  cMo+«,  by  what  we 
have  just  shown,  and  /x0  is  not  the  maximum  of  ft. 

Let  us  suppose  that  23  lay  without  c.  We  show  this  leads  to  a 
contradiction.  For  let  us  invert  with  respect  to  a  circle  f,  lying 
in  ct.  Then  c  goes  over  into  a  curve  f,  and  51  goes  over  into 
3)  =  (S  -}-  f .  Then  &  lies  inside  f.  Let  f ,  77  be  coordinates  of  a 
point  of  £).  Obviously  they  are  continuous  functions  of  z,  y  in 

A,  and  <TN  «  •£        i 

A~x)     ,     c  ~  f ,         uniformly. 

By  what  we  have  just  proved,  (£  must  fill  all  the  interior  of  f. 
This  is  impossible  unless  51  is  unlimited. 

3.    We  may  obviously  extend  the  theorem  2  to  the  case 

u\  =/iOi  •••'O  "'um  = /«(*!•••*„) 

and  A  is  a  cube  in  m-way  space  9?m,  provided  we  assume  that  c,  the 
image  of  the  boundary  of  J.,  divides  space  into  two  precincts 
whose  frontier  is  c. 

Area  of  Curved  Surfaces 

603.  1.  TJie  Inner  Definition.  It  is  natural  to  define  the  area  of  a 
curved  surface  in  a  manner  analogous  to  that  employed  to  define 
the  length  of  a  plane  curve,  viz.  by  inscribing  and  circumscrib 
ing  the  surface  with  a  system  of  polyhedra,  the  area  of  whose 
faces  converges  to  0.  It  is  natural  to  expect  that  the  limits  of 
the  area  of  these  two  systems  will  be  identical,  and  this  common 
limit  would  then  forthwith  serve  as  the  definition  of  the  area  of 
the  surface.  The  consideration  of  the  inner  and  the  outer  sys- 


GEOMETRIC    NOTIONS 


terns  of  polyhedra  afford  thus  two  types  of  definitions,  which 
may  be  styled  the  inner  and  the  outer  definitions.  Let  us  look 
first  at  the  inner  definition. 

Let  the  equations  of  the  surface  S  under  consideration  be 


x  = 


v) 


y  =  ^r(w,  v) 


z  =  xO,  v), 


(1 


the  parameters  ranging  over  a  complete  metric  set  21,  and  a?,  y,  z 
being  one-valued  and  continuous  in  21. 

Let  us  effect  a  rectangular  division  D  of  norm  d  of  the  u,  v 
plane.  The  rectangles  fall  into  triangles  tK  on  drawing  the 
diagonals.  Such  a  division  of  the  plane  we  call  quasi  rectangular. 

Let     P0=(«0,«0)     ,     P,  =  Oo  +  M)     ,     P2  =  O0,  fo  +  'O 

be  the  vertices  of  tK.  To  these  points  in  the  u,  v  plane  corre 
spond  three  points  $«.  =  (#t,  y^  «t),  t=l,  2,  3,  of  £  which  form  the 
vertices  of  one  of  the  triangular  faces  TK  of  the  inscribed  polyhe 
dron  11^  corresponding  to  the  division  D.  Here,  as  in  the  follow 
ing  sections,  we  consider  only  triangles  lying  in  21.  We  may  do 
this  since  21  is  metric. 

Let  XK,  YK,  ZK  be  the  projections  of  TK  on  the  coordinate  planes. 
Then,  as  is  shown  in  analytic  geometry, 


where 


2/2 


2/2-2/0 


A'y       ,     A'z 


and  similar  expressions  for  y"K,  ZK. 
Thus  the  area  of  II ^  is 


the  summation  extending  over  all  the  triangles  tK  lying  in  the 
set  21. 

Let  x,  y,  z  have  continuous  first  derivatives  in  21-     Then 


dx 


AREA   OF   CURVED   SURFACES 


62;') 


with  similar  expressions  for  the  other  increments.     Let 


A  = 


du 

*y 

dv 


dz 
du 

dz 
dv 


Then 

X=(^K  +  «K)^ 


dz 
du 
dz 
~dv 


dz_ 
du 
dz 
dv 


dz 
du 

dx_ 
~dv 


du 


dv 


YK 


where  aK  /3K  yK  are  uniformly  evanescent  with  d  in  3(.  Thus  if 
^.,  .6,  C  do  not  simultaneously  vanish  at  any  point  of  21,  we  have 
as  area  of  the  surface  S 


2.  An  objection  which  at  once  arises  to  this  definition  lies  in 
the  fact  that  we  have  taken  the  faces  of  our  inscribed  polyhedra 
in  a  very  restricted  manner.  We  cannot  help  asking,  Would  we 
get  the  same  area  for  S  if  we  had  chosen  a  different  system  of 
polyhedra  ? 

To  lessen  the  force  of  this  objection  we  observe  that  by  replac 
ing  the  parameters  u,  v  by  two  new  parameters  u',  v'  we  may 
replace  the  above  quasi  rectangular  divisions  which  correspond  to 
the  family  of  right  lines  u  =  constant,  v  =  constant  by  the  infinitely 
richer  system  of  divisions  corresponding  to  the  family  of  curves 
u'  =  constant,  v'  =  constant.  In  fact,  by  subjecting  u',  v'  to  cer 
tain  very  general  conditions,  we  may  transform  the  integral  3) 
to  the  new  variables  u',  v'  without  altering  its  value. 

But  even  this  does  not  exhaust  all  possible  ways  of  dividing  51 
into  a  system  of  triangles  with  evanescent  sides.  Let  us  there 
fore  take  at  pleasure  a  system  of  points  in  the  u,  v  plane  having 
no  limiting  points,  and  join  them  in  such  a  way  as  to  cover  the 
plane  without  overlapping  with  a  set  of  triangles  tK.  If  each 
triangle  lies  in  a  square  of  side  d,  we  may  call  this  a  triangular 
division  of  norm  d.  We  may  now  inquire  if  SD  still  converges 
to  the  limit  3).  as  d  =  0,  for  this  more  general  system  of  divisions. 
It  was  generally  believed  that  such  was  the  case,  and  standard 
treatises  even  contained  demonstrations  to  this  effect.  These 
demonstrations  are  wrong ;  for  Schwarz  *  has  shown  that  by 

*  Werke,  vol.  2,  p.  309. 


626 


GEOMETRIC   NOTIONS 


properly  choosing  the  triangular  divisions  D,  it  is  possible  to 
make  SD  converge  to  a  value  large  at  pleasure,  for  an  extensive 
class  of  simple  surfaces. 

604.    1.    Schwarzs  Example.     Let  Q  be  a  right  circular  cylin- 
der  of  radius  1  and  height  1.     A  set  of  planes  parallel  to  the  base 


at  a  distance  -  apart  cuts  out  a  system  of  circles  rx,  F2 


Let 


us  divide  each  of  these  circles  into  m  equal 
arcs,  in  such  a  way  that  the  end  points  of 
the  arcs  on  Fx,  F3,  F6  •••  lie  on  the  same 
vertical  generators,  while  the  end  points  of 
F2,  F4,  F6  •••  lie  on  generators  halfway 
between  those  of  the  first  set.  We  now 
inscribe  a  polyhedron  so  that  the  base  of 
one  of  the  triangular  facets  lies  on  one 

circle  while  the  vertex  lies  on  the  next  circle  above  or  below,  as 

in  the  figure. 

The  area  t  of  one  of  these  facets  is 


t  =  1  bh 
Thus 


m 


=  \  A:+     1 


cos 
m 


m  '  w*                2m 
There  are  2  m  such  triangles  in  each  layer,  and  there   are   n 
layers.     Hence  the  area  of  the  polyhedron  corresponding  to  this 
triangular  division  D  is  

84  =  2^  =  2  mn  sin  —  \ — h  4  sin4  —  . 
m  *  M?  2m 

Since  the  integers  w,  n  are  independent  of  each  other,  let  us 
consider  various  relations  which  may  be  placed  on  them. 
Case  1°.    Let  n  =  \m.     Then 


S0  = 

2 

2 

<2 

9-v       •       7T       /      1 
7W   A.  ^sl  11         A  / 

+  4  sin4  — 
2  m 

•       7T 
Sill  — 

2       TT           m 

7T 

sin  
2m 

7T 

. 

m       TT        , 

'X2W2  1   ^w4 

m     V 
TT     ,     as  m  =  QO 

2m 

AREA   OF   CURVED   SURFACES 


627 


Case  2°.    Let  n  =  \m*.     Then 


+  4^f-4 


sin 


7T 


=  2  Try/1  +  —  X2     ,     as  w  =  x. 


Case  3°.    Let  w  =  Xw3.      Then 


sin  - 
m 

/  .,-..• 

sin^ 

TT 

l  +  ^m\ 

7T 

m    J 

V 

'2m 

,     as  m  =  x. 

=  +x> 

2.  Thus  only  in  the  first  case  does  SD  converge  to  2  TT,  which 
is  the  area  of  the  cylinder  C  as  universally  understood.  In  the 
2°  and  3°  cases  the  ratio  h/b  =  0.  As  equations  of  C  we  may 
take 


x  =  cos  u 


=  sin 


z  =  v. 


Then  to  a  triangular  facet  of  the  inscribed  polyhedron  will  cor 
respond  a  triangle  in  the  u,  v  plane.  In  cases  2°  and  3°  this  tri 
angle  has  an  angle  which  converges  to  TT  as  m  =  oo.  This  is  not 
so  in  case  1°.  Triangular  divisions  of  this  latter  type  are  of  great 
importance.  Let  us  call  then  a  triangular  division  of  the  u,  v 
plane  such  that  no  angle  of  any  of  its  triangles  is  greater  than 
7T  —  e,  where  e  >  0  is  small  at  pleasure  but  fixed,  positive  triangu 
lar  divisions.  We  employ  this  term  since  the  sine  of  one  of  the 
angles  is  >  some  fixed  positive  number. 

605.  The  Outer  Definition.  Having  seen  one  of  the  serious  diffi 
culties  which  arise  from  the  inner  definition,  let  us  consider  briefly 
the  outer  definition.  We  begin  with  the  simplest  case  in  which 
the  equation  of  the  surface  S  is 


=/(*, 


(1 


/  being  one-valued  and  having  continuous  first  derivatives.     Let 
us  effect  a  metric  division  A  of  the  #,  y  plane  of  norm  S,  and  on 


628  GEOMETRIC   NOTIONS 

each  cell  dK  as  base,  we  erect  a  right  cylinder  (7,  which  cuts  out  an 
element  of  surface  8K  from  S.  Let  *$„  be  an  arbitrary  point  of  SK 
and  !£„  the  tangent  plane  at  this  point.  The  cylinder  O  cuts  out 
of  XK  an  element  ASK .  Let  VK  be  the  angle  that  the  normal  to  £K 
makes  with  the  z-axis.  Then 

1 
C°S  "*  =      I 7]Tx2— -f^i 

^(IHD: 

and 


COS  VK 

The  area  of  &  is  now  defined  to  be 

lim  2A#K  (2 

5=0 

when  this  limit  exists.     The  derivatives  being  continuous,  we  have 
at  once  that  this  limit  is 


which  agrees  with  the  result  obtained  by  the  inner  definition  in 
603,  3). 

The  advantages  of  this  form  of  definition  are  obvious.  In  the 
first  place,  the  nature  of  the  divisions  A  is  quite  arbitrary  ;  however 
they  are  chosen,  one  and  the  same  limit  exists.  Secondly,  the  most 
general  type  of  division  is  as  easy  to  treat  as  the  most  narrow,  viz. 
when  the  cells  dK  are  squares. 

Let  us  look  at  its  disadvantages.  In  the  first  place,  the  elements 
A/S^  do  not  form  a  circumscribing  polyhedron  of  S.  On  the  con 
trary,  they  are  little  patches  attached  to  S  at  the  points  tyK,  and 
having  in  general  no  contact  with  one  another.  Secondly,  let  us 
suppose  that  S  has  tangent  planes  parallel  to  the  z-axis.  The  de 
rivatives  which  enter  the  integral  603,  3)  are  no  longer  continuous, 
and  the  reasoning  employed  to  establish  the  existence  of  the  limit 
2)  breaks  down.  Thirdly,  we  have  the  case  that  z  is  not  one- 
valued,  or  that  the  tangent  planes  to  S  do  not  turn  continuously, 
or  do  not  even  exist  at  certain  points. 


AREA  OF  CURVED  SURFACES  629 

To  get  rid  of  these  disadvantages  various  other  forms  of  outer 
definitions  have  been  proposed.  One  of  these  is  given  by  G-oursat 
in  his  Cours  d*  Analyse.  Instead  of  projecting  an  arbitrary 
element  of  surface  on  a  fixed  plane,  the  xy  plane,  it  is  projected  on 
one  of  the  tangent  planes  belonging  to  that  element.  Hereby  the 
more  general  type  of  surfaces  defined  by  603,  1)  instead  of  those 
defined  by  1)  above  is  considered.  The  restriction  is,  however, 
made  that  the  normals  to  the  tangent  planes  cut  the  elements  of 
surface  but  once,  also  the  first  derivatives  of  the  coordinates  are 
assumed  to  be  continuous  in  21.  Under  these  conditions  we  get 
the  same  value  for  the  area  as  that  given  in  603,  3). 

When  the  first  derivatives  of  #,  y,  z  are  not  continuous  or  do 
not  exist,  this  definition  breaks  down.  To  obviate  this  difficulty 
de  la  ValUe-Poussin  has  proposed  a  third  form  of  definition  in  his 
Cours  d  Analyse,  vol.  2,  p.  30  seq.  Instead  of  projecting  the 
element  of  surface  on  a  tangent  plane,  let  us  project  it  on  a  plane 
for  which  the  projection  is  a  maximum.  In  case  that  S  has  a  con 
tinuously  turning  tangent  plane  nowhere  parallel  to  the  2-axis,  de 
la  Vallee-Poussin  shows  that  this  definition  leads  to  the  same 
value  of  the  area  of  S  as  before.  He  does  not  consider  other  cases 
in  detail. 

Before  leaving  this  section  let  us  note  that  Jordan  in  his  Cours 
employs  the  form  of  outer  definition  first  noted,  using  the  paramet 
ric  form  of  the  equations  of  S.  In  the  preface  to  this  treatise  the 
author  avows  that  the  notion  of  area  is  still  somewhat  obscure,  and 
that  he  has  not  been  able  "a  definir  d'une  maniere  satisfaisante 
1'aire  d'une  surface  gauche  que  dans  le  cas  ou  la  surface  a  un  plan 
tangent  variant  suivant  une  loi  continue." 

606.  1.  Regular  Surfaces.  Let  us  return  to  the  inner  definition 
considered  in  603.  We  have  seen  in  604  that  not  every  system  of 
triangular  divisions  can  be  employed.  Let  us  see,  however,  if  we 
cannot  employ  divisions  much  more  general  than  the  quasi  rec 
tangular.  We  suppose  the  given  surface  is  defined  by 

x  =  </>(>,  v)     ,     y  =  \lr(u,  v)     ,     z  =  %(>,  v)  (1 


the  functions  </>,  i/r,  ^  being  one-  valued,  totally  differentiate  func 
tions  of  the  parameters  u,  v  which  latter  range  over  the  complete 


630 


GEOMETRIC   NOTIONS 


metric    set   SI.     Surfaces    characterized   by    these    conditions  we 
shall  call  regular.     Let 


be  the  vertices  of  one  of  the  triangles  tK,  of  a  triangular  division 
2>  of  norm  ^  of  SI.  As  before  let  $0,  ^x,  $2  be  the  corresponding 
points  on  the  surface  S.  Then 


and  similar  expressions  hold  for  the  other  increments.     Also 


du          dv 


+  2  jr.', 


where  X*  denotes  the  sum  of  several  determinants,  involving  the 
infinitesimals 

«i    ,    <    ,    ft    ,    ft. 

Similar  expressions  hold  for  J^,  ZK.     We  get  thus 

XK  =  AJK+X'K     ,     YK  =  £&+¥!    ,     Z^C^  +  Z't 

where  ^.,  5,  (7  are  the  determinants  2)  in  603.     Then  the  area  of 
the  inscribed  polyhedron  corresponding  to  this  division  D  is 


Let  us  suppose  that 


as  w,  v  ranges  over  SI.     Also  let  us  assume  that 

VI  V?  *7f 

^<  *K  ^K 


AREA  OF  CURVED  SURFACES 


631 


remain  numerically  <  e  for  any  division  D  of  norm  d<  c?0,  e  small 
at  pleasure,  except  in  the  vicinity  of  a  discrete  set  of  points,  that 
is,  let  3)  be  in  general  uniformly  evanescent  in  51,  as  d  =  0.  Then 


BI 


where  in  general 


If  now  A,  B,  Q  are  limited  and  ^-integrable  in  2(,  we  have  at 


once 


lim8D=fdudvJA* 


~    ^a 
as  in  603. 

2.  We  ask  now  under  what  conditions  are  the  expressions  3) 
in  general  uniformly  evanescent  in  51  ?  The  answer  is  pretty  evi 
dent  from  the  example  given  by  Schwarz.  In  fact  the  equation 
of  the  tangent  plane  X  at  ^30  is 

A(x  -  a-0)  +  B(y  -  #0)  +  C(z  -  z0)  =  0. 
On  the  other  hand  the  equation  of  the  plane   T=  ($0,  $j,  <$%) 

is  -    y 

^o  v»  z( 


or  finally 


Thus  for  3)  to  converge  in  general  uniformly  to  zero,  it  is  nec 
essary  and  sufficient  that  the  secant  planes  T  converge  in  general 
uniformly  to  tangent  planes.  Let  us  call  divisions  such  that  the 
faces  of  the  corresponding  inscribed  polyhedra  converge  in  general 
uniformly  to  tangent  planes  uniform  triangular  divisions.  For 
such  divisions  the  expressions  3)  are  in  general  uniformly  evanes 
cent,  as  c?=  0.  We  have  therefore  the  following  theorem  : 

3.  Let  51  be  a  limited  complete  metric  set.  Let  the  coordinates 
x,  y,  2  be  one-valued  totally  differentiable  functions  of  the  parame- 


632  GEOMETRIC   NOTIONS 

ters  u,  v  in  51,  such  that  A2  +  IP  +  O2  is  greater  than  some  positive 
constant,  and  is  limited  and  H-integrable  in  51.      Then 


tf  =  lim  SD  =      V^2+^2+  C*dudv, 
rf=o  ^21 

D  denoting  the  class  of  uniform  triangular  divisions  of  norms  d. 

This  limit  we  shall  call  the  area  of  S.  From  this  definition  we 
have  at  once  a  number  of  its  properties.  We  mention  only  the 
following  : 

4.  Let  5Ij,  •••  5lw  be  unmixed  metric  sets  whose  union  is  51.     Let 
$!,  •••  Sm  be  the  pieces  of  S  corresponding  to  them.      Then  each  SK 
has  an  area  and  their  sum  is  S. 

5.  Let  51A  be  a  metric  part  of  51,  depending  on  a  parameter  X=  0, 
such  that  SA  =  S.      Then 


6.  The  area  of  S  remains  unaltered  when  S  is  subjected  to  a  dis 
placement  or  a  transformation  of  the  parameters  as  in  I,  744  seq. 

607.  1.  Irregular  Surfaces.  We  consider  now  surfaces  which 
do  not  have  tangent  planes  at  every  point,  that  is,  surfaces  for 
which  one  or  more  of  the  first  derivatives  of  the  coordinates  #,  y,  z 
do  not  exist,  and  which  may  be  styled  irregular  surfaces.  We 
prove  now  the  theorem  : 

Let  the  coordinates  x,  y,  z  be  one-valued  functions  of  w,  v  having 
limited  total  difference  quotients  in  the  metric  set  51.  Let  D  be  a 
positive  triangular  division  of  norm  d<dQ.  Then 

Max  *S^ 
is  finite  and  evanescent  with  51. 

For  let  the  difference  quotients  remain  </JL.     We  have 


But 


cosec 


AREA   OF  CURVED   SURFACES  633 


where  0K  is  the  angle  made  by  the  sides  P$PI,  ^V^V     As  D  is  a 

positive  division,  one  of  the  angles  of  tK  is  such  that  cosec  6K  is 
numerically  less  than  some  positive  number  M.     Thus 


where  /-i,  M  are  independent  of  K  and  d.     Similar  relations  hold 
for    Y,  ,    ZK.     Hence 


77) 
where  77  >  0  is  small  at  pleasure,  for  dQ  sufficiently  small. 

2.  Let  31  and  x,  y,  z  be  as  in  606,  3,  except  at  certain  points  form 
ing  a  discrete  set  a,  the  first  partial  derivatives  do  not  exist.  Let 
their  total  difference  quotients  be  limited  in  31.  Then 


=  C 

J 


ivhere  D  denotes  a  positive  triajiyular  division  of  norm  d. 

Let  us  first  show  that  the  limit  on  the  left  exists.  We  may 
choose  a  metric  part  55  of  51  such  that  (§  =  51  —  53  is  complete  and 
exterior  to  31  and  such  that  53  is  as  small  as  we  please.  Let  /Sg 
denote  the  area  of  the  surface  corresponding  to  (5.  The  triangles 
tK  fall  into  two  groups  :  G1  containing  points  of  53  ;  6r2  containing 
only  points  of  (£•  Then 


SD  =  2  V  X2  +  17  +  Z  2  =  v  +  2 . 

«,      ff» 

But  53  may  be  chosen  so  small  that  the  first  sum  is  <  e/4  for 
any  d<dQ.  Moreover  by  taking  d0  still  smaller  if  necessary,  we 
have 

|2-SC  <e/4. 

0, 

HenCC  |^-^|<6/2     ,     d<d0.  (1 

Similarly  for  any  other  division  D'  of  norm  d', 

\SD,-Sg>\<€/2      ,      d'<d0 
decreasing  dQ  still  farther  if  necessary.     Thus 
|^-^|<€     ,     d,d'<dQ. 


634  GEOMETRIC   NOTIONS 

Hence  lim  SD  exists,  call  it  S.     Since  S  exists  we  may  take  dQ 

so  small  that 

\S-SD\<€/2 

This  with  1)  gives 

|tf 
that  is, 

S  =  lim  &k  =  lim  f  V^  +  ^ 
«/S 

=  C  ^/A?  + &  +  (Fdudv 

c/2l 
by  I,  724. 

608.  1.  The  preceding  theorem  takes  care  of  a  large  class  of 
irregular  surfaces  whose  total  difference  quotients  are  limited. 
In  case  they  are  not  limited  we  may  treat  certain  cases  as  follows: 

Let  us  effect  a  quadrate  division  of  the  u,  v  plane  of  norm  d, 
and  take  the  triangles  tK  so  that  for  any  triangular  division  D 
associated  with  c?,  no  square  contains  more  than  n  triangles,  and 
no  triangle  lies  in  more  than  v  squares ;  n,  v  being  arbitrarily 
large  constants  independent  of  d.  Such  a  division  we  call  a 
quasi  quadrate  division  of  norm  d.  If  we  replace  the  quadrate  by 
a  rectangular  division,  we  get  a  quasi  rectangular  division. 

We  shall  also  need  to  introduce  a  new  classification  of  functions 
according  to  their  variation  in  51,  or  along  lines  parallel  to  the 
u,  v  axes.  Let  D  be  a  quadrate  division  of  the  w,  v  plane  of  norm 
d  <  dQ .  Let 

COK  =  Osc/(w,  v)     ,     in  the  cell  dK. 

Then  Max  ^a)Kd 

is  the  variation  of  /  in  51.  If  this  is  not  only  finite,  but  evanes 
cent  with  51,  we  say/  has  limited  fluctuation  in  51.  Obviously  this 
may  be  extended  to  any  limited  point  set  in  m-way  space. 

Let  us  now  restrict  ourselves  to  the  plane.  Let  a  denote  the 
points  of  51  on  a  line  parallel  to  the  w-axis.  Let  us  effect  a  divi 
sion  D'  of  norm  df.  Let  co'K  =  Osc/(w,  v)  in  one  of  the  intervals 
of  D'.  Then 

?7a  =  Max  2o>^ 
is  the  variation  of /in  a- 


AREA  OF  CURVED  SURFACES  635 

Let  us  now  consider  all  the  sets  a  lying  on  lines  parallel  to  the 
M-axis,  and  let 

a  <_  a-    ,     (7  =  0. 

If  now  there  exists  a  constant  G-  independent  of  a  such  that 

1«<*#, 

that  is,  if  ?7a  is  uniformly  evanescent  with  <r,  we  say  that/(w,  v) 
has  limited  fluctuation  in  51  with  respect  to  u. 

With  the  aid  of  these  notions  we  may  state  the  theorems  : 

2.  Let  the  coordinates  x,  y,  z  be  one-valued  limited  functions  in 
the  limited  complete  set  51.  Let  x,  y  have  limited  total  difference 
quotients,  while  z  has  limited  variation  in  51.  Let  D  denote  a  quasi 
quadratic  division  of  norm  d<dQ.  Then 

Max  SD 

D 

is  finite. 

For,  as  before, 


But  p  denoting  a  sufficiently  large  constant, 

|  A;  '.,         |  A;'  |         are  <  pd. 

Let  ft>t=Osc2  in  the  square  st.     If  the  triangle  tK  lies  in  the 
squares  *tl,  •••  stjfc, 

I  A;  i,  i  A»  i<«.,+  -  +«... 

Thus,  n  denoting  a  sufficiently  large  constant, 


the  summation  extending  over  those  squares  containing  a  triangle 
of  D.     But  z  having  limited  variation, 

2&)tc?  <  some  M. 
Hence  *\XK\     ,     2  |  YK  \         are  < 

Finally,  as  in  607, 

2  |Z  |  <some  M'  . 

The  theorem  is  thus  established. 


636  GEOMETRIC   NOTIONS 

3.  The  coordinates  x,  y,  z,  being  as  in  2,  except  that  z  has  limited 
fluctuation  in  51,  and  D  denoting  a  quasi  quadrate  division  of 
norm  d  <  ^ 


D 

is  finite  and  evanescent  with  51. 

The  reasoning  is  the  same  as  in  2  except  that  now  M,  M'  are 
evanescent  with  51. 

4.  Let  the  coordinates  x,  y,  z  have  limited  total  difference  quo 
tients  in  51,  while  the  variation  of  z  along  any  line  parallel  to  the  u 
or  v  axis  is  <  M.  Let  51  lie  in  a  square  of  side  s  =  0.  Then 

Max/S^  <  sG-, 

D 

where  G  is  some  constant  independent  of  s,  and  D  is  a  quasi  rectan 
gular  division  of  norm  d  <  dQ  . 

For  here 

2  |  A»y    •  |  A'z  | 


where  M'  denotes  a  sufficiently  large  constant;  du,  dv  denote  the 
length  of  the  sides  of  one  of  the  triangles  tK  parallel  respectively 
to  the  u,  v  axes,  and  a)u,  a)v  the  oscillation  of  z  along  these  sides. 
Since  the  variation  is  <  M  in  both  directions, 


Ms. 

Similarly 

2o>A  <  M8. 

The  rest  of  the  proof  follows  as  before. 

5.    The  symbols  having  the  same  meaning  as  before,  except  that  z 
has  limited  fluctuation  with  respect  to  u,  v, 


The  demonstration  is  similar  to  the  foregoing.  Following  the 
line  of  proof  used  in  establishing  607,  2  and  employing  the 
theorems  just  given,  we  readily  prove  the  following  theorems  : 


AREA  OF  CURVED  SURFACES  637 

6.  Let  51  be  a  metric  set  containing  the  discrete  set  a.  Let  b  be 
a  metric  part  of  31,  containing  a  such  that  33  =  51  —  b  is  exterior  to  a, 
and  t>  =  0.  Let  the  coordinates  x,  y,  z  be  one-valued  totally  differ- 
entiable  functions  in  33,  such  that  A2  +  IP  +  C2  never  sinks  below  a 
positive  constant  in  any  33,  is  properly  R-integrable  in  any  53,  and 
improperly  integrable  in  51.  Let  x,  y  have  limited  total  difference 
quotients,  and  z  limited  fluctuation  in  b.  Then 


lim  S#  =    I  V^i2  +  B2  +  02dudv 
d=0  J% 

where  A,  B,  C  are  the  determinants  in  603,  2),  and  D  is  any  quasi 
quadrate  division  of  norm  d. 

7.    Let  the  symbols  have  the  same  meaning  as  in  6,  except  that 
1°  a  reduces   to  a  finite  set. 

2°  z  has  limited  variation  along  any  line  parallel  to  the  u,  v  axes. 
3°  D  denotes  a  uniform  quasi  rectangular  division.      Then 


\\mSD=      VA2  +  7>2  +  CPdudv. 

d=o  %/* 

8.    The  symbols  having  the  same  meaning  as  in  6,  except  that 

1°  z  has  limited  fluctuation  with  respect  to  w,  v  in  b. 

2°  D  denotes  a  uniform  quasi  rectangular  division.      Then 


lim  SD  =    I  V 'A*  +  B2  -f  C2dudv. 

9.    If  we  call  the  limits  in  theorems  6,  7,  8,  area,  the  theorems 
606,  3,  4,  5  still  hold. 


INDEX 


(Numbers  refer  to  pages) 


-x 

• 


tf 


AbeVs  identity,  87 

series,  87 
Absolutely  convergent  integrals,  31 

series,  79 

products,  247 
Addition  of  cardinals,  292 

ordinals,  312 

series,  128 
Adherence,  340 
Adjoint  product,  247 

series,  77,  139 

set  of  intervals,  337 
Aggregates,  cardinal  number,  278 

definition,  276 

distribution,  295 

enumerable,  280 

equivalence,  276 

eutactic,  304 

exponents,  294 

ordered,  302 

power  or  potency,  278 

sections,  307 

similar,  303 

transfinite,  278 

uniform  or  1-1  correspondence,  2" 
Alternate  series,  83 
Analytical  curve,  582 
Apantactic,  325 
Area  of  curve,  599,  602 

surface,  623 
Arzela,  365,  555 
Associated  simple  series,  144 

products,  247 

multiple  series,  145 

normal  series,  245 

logarithmic  series,  243 

inner  sets,  365 


Associated,  outer  sets,  365 
non-negative  functions,  41 

Baire,  326,  452,  482,  587 
Bernovillian  numbers,  265 
Bertram's  test,  104 
Bessel  functions,  238 
Beta  functions,  267 
Binomial  series,  110 
Bocher,  165 
Bonnet's  test,  121 
Borel,  324,  542 
Brouwer,  614 

Cohen's  test,  340 

Cantors  1°  and  2°  principle,  316 

theorem,  450 
Category  of  a  set,  326 
Cauchy's  function,  214 

integral  test,  99 

radical  test,  98 

theorem,  90 
Cell  of  convergence,  144 

standard  rectangular,  359 
Chain,  612 

Class  of  a  function,  468,  469 
Conjugate  functions,  238 

series,  147 

products,  249 
Connex,  605 
Connected  sets,  605 
Contiguous  functions,  231 
Continuity,  452 

infra,  487 

semi,  487 

supra,  487 
Continuous  image,  608 


639 


640 


INDEX 


Contraction,  287 

Convergence,  infra-uniform,  562 

monotone,  176 

uniform,  156 
at  a  point,  157 
in  segments,  556 

sub-uniform,  555 
Co-product,  242 
Curves,  analytical,  582 

area,  599,  602 

Faber,  546 

Jordan,  595,  610 

Hilbert,  590 

length,  579 

non-intuitional,  537 

Osgood,  600 

Pompeiu,  542 

rectifiable,  583 

space-filling,  588 

D'Alembert,  96 
Deleted  series,  139 
Derivates,  494 
Derivative  of  a  set,  330 

order  of,  331 
Detached  sets,  604 
Dilation,  287 
Dim,  176,  185,  438,  538 

series,  86 
Discontinuity,  452 

at  a  point,  454 

of  1°  kind,  416 

of  2°  kind,  455 

point  wise,  457 

total,  457 
Displacement,  286 
Distribution,  295 
Divergence  of  a  series,  440 
Division,  complete,  30 

separated,  366,  371 

unmixed,  2 

of  series,  196 

of  products,  253 
Divisor  of  a  set,  23 

quasi,  390 


Divisor,  semi,  390 
Du  Bois  Reymond,  103 


473 

Elimination,  594 
Enclosures,  complementary  e-,  355 

deleted,  452 

distinct,  344 

divisor  of,  344 

e,  355 

measurable,  356 

non-overlapping,  344 

null,  366 

outer,  343 

standard,  359 
Enumerable,  280 
Equivalent,  276 
Essentially  positive  series,  78 

negative  series,  78 
Euler's  constant,  269 
Eutactic,  304 
Exponents,  294 
Exponential  series,  96 
Extremal  sequence,  374 

Faber  curves,  546 
Fluctuation,  634,  635 
Fourier's  coefficient,  416 
constants,  416 
series,  416 
Function,  associated  non-negative  func 

tions,  41 
Bessel's,  238 
Beta,  267 
Cauchy's,  214 
class  of,  468,  469 
conjugate,  233 
contiguous,  231 
continuous,  452 
infra,  487 
semi,  487 
supra,  487 
discontinuous,  452 
of  1°  kind,  416 
of  2°  kind,  455 


INDEX 


641 


Function,  Gamma,  267 
Gauss'  HO),  238 
hyperbolic,  228 
hypergeometric,  228 
lineo-oscillating,  528 
maximal,  488 
measurable,  338 
minimal,  488 
monotone,  137 
null,  385 
oscillatory,  488 
pointwise  discontinuous,  457 
residual,  561 
Riemann's,  459 
totally  discontinuous,  457 
truncated,  27 

uniformly  limited,  160,  567 
Volterra's,  501,  583 
Weierstrass',  498,  523,  581,  588 

Gamma  function,  267 
Gauss'  function  !!(»,  238 

test,  109 
Geometric  series,  81,  139 

Harnack,  divergence  of  series,  440 

sets,  354 
Hermite,  300 
Httbert's  curves,  590 
Hobson,  389,  412,  555 
Hyperbolic  functions,  228 
Hypercomplete  sets,  472 
Hypergeometric  functions,  229 

series,  112 

Images,  simple,  multiple,  606 
unifold,  manifold,  606 
continuous,  606,  608 
Integrals,  absolutely  convergent,  31 
L-  or  Lebesgue,  proper,  372 

improper,  403,  405 
improper,  author's,  32 
classical,  26 

de  la  Vallee-Poussin,  27 
inner,  20 


Integrals,  R-  or  Riemannian,  372 
Integrand  set,  385 
Intervals,  of  convergence,  90 

adjoint  set  of,  337 

set  of,  belonging  to,  337 
Inversion,  geometric,  287 

of  a  series,  204 
Iterable  sets,  14 
Iterated  products,  251 

series,  149 

Jordan  curves,  595,  610 
variation,  430 
theorem,  436 

Kdnig,  527 

Rummer's  test,  106,  124 

Lattice  points,  137 

system,  137 

Law  of  Mean,  generalized,  505 
Layers,  555 

deleted,  563 
Lebesque  or  L-  integrals,  372 

theorems,  413,  424,   426,   452,   475, 

520,  619 

Leibnitz's  formula,  226 
Length  of  curve,  579    , 
Lindermann,  300,  599 
Lineo-oscillating  functions,  528 
Link,  612 

Liouville  numbers,  301 
Lipschitz,  438 
Logarithmic  series,  97 
Liiroth,  448 

Maclaurin's  series,  206 
Maximal,  minimal  functions,  488 
Maximum,  minimum,  521 

at  a  point,  485 
Measure,  348       — 

lower,  348 

upper,  343 
Mertens,  130 
Metric  sets,  1 


642 


INDEX 


Monotone  convergence,  176 

functions,  137 
Moore-Osgood  theorem,  170 
Motion,  579 
Multiplication  of  series,  129 

cardinals,  293 

ordinals,  314 

infinite  products,  253 

Normal  form  of  infinite  product,  245 
Null  functions,  385 

sets,  348 
Numbers,  Bernouillian,  265 

cardinal,  278 

class  of  ordinal  numbers,  318 

limitary,  314. 

Liouville,  301 

ordinal,  310 

rank  of  limitary  numbers,  331 

Ordered  sets,  302 

Order  of  derivative  of  a  set,  331 

Oscillation  at  a  point,  454 

Oscillatory  function,  488 

Osyood  curves,  600 
-Moore  theorem,  170 
theorems,  etc.,  178,  555,  622 

Pantactic,  325 
Path,  612 
Peaks,  179 

infinite,  566 
Poly  ant,  153 
Point  sets,  adherence,  340 

adjoint  set  of  intervals,  337 

apantactic,  325 

associated  inner  set,  365 
outer  set,  365 

Baire  sets,  326 

category  1°  and  2°,  326 

coherence,  340 

conjugate,  51 

connected,  605 

convex,  605 

detached,  604 


Point  sets,  divisor,  23 


Ilarnack  sets,  354 

hypercomplete,  472 

images,  605,  606 

integrand  sets,  385 

iterable,  14 

measurable,  343,  348 

metric,  1 

negative  component,  37 

null,  318 
-^  pantactic,  325 

positive  component,  37 

potency  or  power,  278 

projection,  10 

quasidivisor,  390 

reducible,  335 

reticulation,  621 

semidivisor,  390 

separated  intervals,  337 

sum,  22 

transfinite  derivatives,  330 

union,  27 

well-ordered,  304 
Polntwise  discontinuity,  457 
Pompeiu,  curves,  542 
Potency  or  power  of  a  set,  278 
Power  series,  89,  144,  187,  191 
Precinct,  612 
Pringsheim,  theory  of  convergence,  113 

theorems,  etc.,    141,  215,  216,  217, 

220,  273 
Projection,  10 
Products,  absolute  convergence,  247 

adjoint,  247 

associate  simple,  247 

conjugate,  249 

co-product,  242 

iterated,  251 

normal  form,  245 

Quasidivisor,  390 

Raabe's  test,  107 

Rank  of  limitary  numbers,  331 


INDEX 


643 


Rate  of  convergence  or  divergence,  102 
Ratio  test,  96 
Reducible  sets,  335 
Remainder  series,  77 

of  Taylor's  series,  209,  210 
Rectifiable  curves,  583 
Regular  points,  428 
Residual  function,  561 
Reticulation,  621 
Richardson,  32 
Riemann's  function,  459 

theorem,  444 

R-  or  Riemann  integrals,  372 
Rotation,  286 

Scheefer,  theorem,  516 
Schonfliess,  theorems,  598,  621 
Schicarz,  theorem,  etc.,  448,  626 
Section  of  an  aggregate,  307 
Segment,  constant,  or  of  invariability, 

521 

Semidii-isor,  390 
Separated  divisions,  366,  371 

functions,  403 

sets,  366 

of  intervals,  337 
Sequence,  extremal,  374 

m-tuple,  137 
Series,  Abel's,  87 

absolute  convergent,  79 

adjoint,  77,  139 

alternate,  83 

associate  logarithmic,  243 
normal,  245 
simple,  144 
multiple,  144 

Bessels,  238 

binomial,  110 

cell  of  convergence,  144 

conjugate,  147 

deleted,  139 

Dini's,  86 

divergence  of,  440 

essentially  positive  or  negative,  78 

exponential,  96 


Series,  Fourier's,  416 

geometric,  81,  139 

harmonic,  82 

general  of  exponent  /A,  82 

hypergeometric,  112 

interval  of  convergence,  90 

inverse,  204 

iterated,  149 

logarithmic,  97 

Maclaurin's,  206 

power,  89,  114,  187 

rate  of  convergence  or  divergence, 
102 

remainder,  77 

simple  convergence,  80 

Taylor's,  206 

tests  of  convergence,  see  Tests 

telescopic,  85 

trigonometric,  88 

two-way,  133 
Similar  sets,  303 
Similitude,  287 

Simple  convergence  of  series,  80 
Singular  points,  26 
Space-filling  curves,  588 
Steady  convergence,  176 
Submeasurable,  405 
Sum  of  sets,  22 
Surface,  area,  623 

irregular,  632 

regular,  629 

Taylor's  series,  206 
Telescopic  series,  85 
Tests  of  convergence,  Bertram,  104 

Bonnet,  121 

Cahen,  108 

Cauchy,  98,  99 

d'Alembert,  96 

Gauss,  109 

Rummer,  106,  124 

Pringsheim,  123 

Raabe,  107 

radical,  98 

ratio,  96 


644  INDEX 

Tests  of  convergence,  tests  of  1°  and  2°       Uniformly  limited  function,  160,  567 

kind,  120  Union  of  sets,  22 

Weierstrass,  120 

Theta  functions,  135,  184,  256  Vallee-Poussin  (de  la),  27,  594 

Total  discontinuity,  457  Van  Vleck  sets,  361 

Transjinite  cardinals,  278  Variation,  limited  or  finite,  429,  530 

derivatives,  330  positive  and  negative,  430 

Translation,  286  Volterra  curves,  501,  587 
Trigonometric  series,  88 

Truncated  function,  27  WaWs  tonnolo,  26° 

Two-way  series,  133  Weierstrats'  function,  498,  523,  588 

test,  120 

Undetermined  coefficients,  197  Well-ordered  sets,  304 

Unifold  image,  606  Wilson,  W.  A.,  vii,  395,  401 

Uniform  convergence,  156  youn^  w   H    theoremSj  360>  363 
at  a  point,  157 

correspondence,  276  Zeros  of  power  series,  191 


SYMBOLS  EMPLOYED   IN   VOLUME   II 

(Numbers  refer  to  pages) 

Front  31,  1.     Fa,  614  Xr  K2  ••• ,  318,  323 

2o  Z,,  Zg-,318 

gj(«)  -  2jw?  330 ;  9i<a)  -  s^a?  331 

fl,  1  1  =  Meas  2t,  343 ;  §  =  Meas  5t,  348 

U>{    I'22  S  =  Meas  a,  348 

£,,22  r    r    r 

Ad,J,81  /'    J,    J,  372,  403,  405 

/A,M'31  Sdv,  Qdv,  390 

2laij3,  32.     3(/,afp,  34  j/^  429;  Var/=  F/,  429 

31^,  s#_a,  34  QSC  j-  _  oscillation    in    a   given   set. 

A „,  A n,  Ad j  A ,  77.     A  „,  p,  78  QSC  y;  454 

f>   _             139  Disc/,  454 

51  ~  53,  276  ;  31  a*  53,  303  (S€,  @t±0»  473 

Card  51,  278  J(x)  y^)  433 

e  =  K  280;  c.287  /'(^./'(x),  493 

j/i^,  jyu  

Ord  31,  311  .ff(^),  494 

w,  311  ;  «,  318  A(a,  ft),  494 


INDEX 


645 


The  following  symbols  are  defined  in  Volume  I  and  are  repeated  here  for 
the  convenience  of  the  reader. 


Dist(a,  x)  is  the  distance  between 
a  and  x 

Z^(a),  called  the  domain  of  the  point 
a  of  norm  8  is  the  set  of  points  a:, 
such  that  Dist  (a,  x)  <  8 

Fg(rt),  called  the  vicinity  of  the  point 
a  of  norm  8,  refers  to  some  set  31, 
and  is  the  set  of  points  in  D^(a) 
which  lie  in  31 

Z>6*(tt),  V$*(a)  are  the  same  as  the 
above  sets,  omitting  a.  They  are 
called  deleted  domains,  deleted  vi 
cinities 

an  =  a  means  an  converges  to  a 


f(x)  =  a,  means /(z)  converges  to  a 

A  line  of  symbols  as : 

c  <  0,  wz,  |  a  -  an  |  <  e,  n  >  m 
is  of  constant  occurrence,  and  is  to 
be  read  :  for  each  e  >  0,  there  exists 
an  index  m,  such  that  |  a  —  an  \  <  e, 
for  every  n  >  m 

Similarly  a  line  of  symbols  as : 

00,  S>0,  !/(*)  -  a|<£,  x  in  F«*(«) 
is  to  be  read  :  for  each  e  >  0,  there 
exists  a  8  >  0,  such  that 

I /GO  -«|<€, 

for  every  x  in  Pr5*(a) 


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