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THE CALCULUS 



A SERIES OF MATHEMATICAL TEXTS 

EDITED BT 

EARLE RAYMOND HEDRICE 



THE CALCULUS 

By Elleby Williams Davis and William Chableb Bbenee. 

ANALYTIC GEOMETRY AND ALGEBRA 

By Alexander Ziwet and Louis Allen Hopkins. ' 

ELEMENTS OF ANALYTIC GEOMETRY 

By Alexander Ziwet and Louis Allen Hopkins. > 

PLANE AND SPHERICAL TRIGONOMETRY 
By Alfred Monroe Kenton and Louis Ingold. 

ELEMENTS OF PLANE TRIGONOMETRY 

By Alfred Monroe Keityon and Louis Ingold. . 

ELEMENTARY MATHEMATICAL ANALYSIS 

By John Wesley Young and Frank Millett Morgan. 

PLANE TRIGONOMETRY 

By John Wesley Young and Frank Millett Morgan. 

COLLEGE ALGEBRA 

By Ernest Brown Skinner. 

MATHEMATICS FOR STUDENTS OF AGRICULTURE AND 
GENERAL SCIENCE 

By Alfred Monroe Kenyon and William Vernon Lovitt. 

MATHEMATICS FOR STUDENTS OF AGRICULTURE 
By Samuel Eugene Rasor. 

THE MACMILLAN TABLES 

Prepared under the direction of Eable Raymond Hedrick. 

PLANE AND SOLID GEOMETRY 

By Wai/eer Burton Ford and Charles Ammerman. 

CONSTRUCTIVE GEOMETRY 

Prepared under the direction of Earle Raymond Hedrick. 

JUNIOR HIGH SCHOOL MATHEMATICS 

By William Ledley Vosburgh and Frederick William 

Gentleman. 

A BRIEF COURSE IN COLLEGE ALGEBRA 
By Walter Burton Ford. 



THE CALCULUS 



/ 



ELLERY WILLIAMS DAVIS 

It 
PBOFESBOR OF BCATHEMATICS IN THE UNIYEBSITT OF NEBRASKA 

AND 

WILLIAM CHARLES BRENKE 

PBOFE8BOB OF MATHEMATICS IN THE UNIVEBSITY OF NEBRASKA 



REVISED EDITION 



THE MACMILLAN COMPANY 

1924 

All rights reserved 



PRINTED IN THE UNITED STATES OF AMERICA 



Copyright, 1912 and 1922 
By the MACMILLAN COMPANY 



Set up and electrotyped 
Revised Edition published September. 1922 



'Sn. ,.:._:.. 638522 ••> : - -••;^' 



^j 




.T)^?2 



PREFACE TO THE FIRST EDITION 

The significance of the Calculus, the possibility of applying 
it in other fields, its usefulness, ought to be kept constantly 
and vividly before the student during his study of the subject, 
rather than be deferred to an uncertain future. 

Not only for students who intend to become engineers, but 
also for those planning a profound study of other sciences, the 
usefulness of the Calculus is universally recognized by teach- 
ers; it should be consciously realized by the student himself. 
It is obvious that students interested primarily in mathe- 
o? matics, particularly if they expect to instruct others, should 
recognize the same fact. 

To all these, and even to the student who expects only gen- 
^ eral culture, the use of certain types of applications tends to 
make the subject more real and tangible, and offers a basis for 
an interest that is not artificial. Such an interest is necessary 
to secure proper attention and to insure any real grasp of the 
essential ideas. 

For this reason, the attempt is made in this book to present 
as many and as varied applications of the Calculus as it is 
possible to do without venturing into technical fields whose 
subject matter is itself unknown and incomprehensible to the 
student, and without abandoning an orderly presentation of 
fundamental principles. 

The same general tendency has led to the treatment of 
topics with a view toward bringing out their essential useful- 
ness. Thus the treatment of the logarithmic derivative is 



^^ 



vi PREFACE 

vitalized by its presentation as the relative rate of change of a 
quantity; and it is fundamentally connected with the impor- 
tant "compound interest law," which arises in any phe- 
nomenon in which the relative rate of increase (logarithmic 
derivative) is constant. 

Another instance of the same tendency is the attempt, in 
the introduction of the precise concept of curvature, to explain 
the reason for the adoption of this, as opposed to other 
simpler but cruder measures of bending. These are only 
instances, of two typical kinds, of the way in which the effort 
to bring out the usefulness of the subject has influenced the 
presentation of even the traditional topics. 

Rigorous forms of demonstration are not insisted upon, es- 
pecially where the precisely rigorous proofs would be beyond 
the present grasp of the student. Rather the stress is laid 
upon the student's certain comprehension of that which is 
done, and his conviction that the results obtained are both 
reasonable and useful. At the same time, an effort has been 
made to avoid those grosser errors and actual misstatements 
of fact which have often offended the teacher in texts other- 
wise attractive and teachable. 

Thus a proof for the formula for differentiating a logarithm 
is given which lays stress on the very meaning of logarithms; 
while it is not absolutely rigorous, it is at least just as rigorous 
as the more traditional proof which makes use of the limit of 
(l+^/n)** as n becomes infinite, and it is far more convincing 
and instructive. The proof used for the derivative of the sine 
of an angle is quite as sound as the more traditional proof 
(which is also indicated), and makes use of fundamentally use- 
ful concrete concepts connected with circular motion. These 
two proofs again illustrate the tendency to make the subject 



PREFACE vii 

vivid, tangible, and convincing to the student; this tendency 
will be found to dominate, in so far as it was found possible, 
every phase of every topic. 

Many traditional theorems are omitted or reduced in im- 
portance. In many cases, such theorems are reproduced in 
exercises, with a sufficient hint to enable the student to 
master them. Thus Taylor's Theorem in several variables, 
for which wide applications are not apparent until further 
study of mathematics and science, is presented in this manner. 

On the other hand, many theorems of importance, both 
from mathematical and scientific grounds, which have been 
omitted traditionally, are included. Examples of this sort 
are the brief treatment of simple harmonic motion, the wide 
appUcation of Cavaheri's theorem and the prismoid formula, 
other approximation formulas, the theory of least squares 
(under the head of exercises in maxima and minima), and 
many other topics. 

The Exercises throughout are colored by the views ex- 
pressed above, to bring out the usefulness of the subject and 
to give tangible concrete meaning to the concepts involved. 
Yet formal exercises are not at all avoided, nor is this neces- 
sary if the student's interest has been secured through convic- 
tion of the usefulness of the topics considered. Far more 
exercises are stated than should be attempted by any one 
student. This will lend variety, and will make possible the 
assignment of different problems to different students and to 
classes in successive years. It is urged that care be taken in 
selecting from the exercises, since the lists are graded so that 
certain groups of exercises prepare the student for other 
groups which follow; but it is unnecessary that all of any 
group be assigned, and it is urged that in general less than 



viii ' PREFACE 

half be used for any one student. Exercises that involve 
practical applications and others that involve bits of theory 
to be worked out by the student are of frequent occurrence. 
These should not be avoided, for they are in tune with the 
spirit of the whole book; great care has been taken to select 
these exercises to avoid technical, concepts strange to the 
student or proofs that are too difficult. 

An effort is made to remove many technical difficulties by 
the intelligent use of tables. Tables of Integrals and many 
other useful tables are appended; it is hoped that these will 
be found usable and helpful. 

Parts of the book may be omitted without destroying the 
essential unity of the whole. Thus the rather complete treat- 
ment of Differential Equations (of the more elementary 
types) can be omitted. Even the chapter on Functions of 
Several Variables can be omitted, at least except for a few 
paragraphs, without vital harm; and the same may be said 
of the chapter on Approximations. The omission of entire 
chapters, of course, would only be contemplated where the 
pressure of time is unusual; but many paragraphs may be 
omitted at the discretion of the teacher. 

Although care has been exercised to secure a consistent 
order of topics, some teachers may desire to alter it; for 
example, an earlier introduction of transcendental functions 
and of portions of the chapter on Approximations may be 
desired, and is entirely feasible. But it is urged that the 
comparatively early introduction of Integration as a summa- 
tion process be retained, since this further impresses the 
usefulness of the subject, and accustoms the student to the 
ideas of derivative and integral before his attention is diverted 
by a variety of formal rules. 



PREFACE ix 

Purely destructive criticism and abandonment of coherent 
arrangement are just as dangerous as ultra-conservatism. 
This book attempts to preserve the essential features of the 
Calculus, to give the student a thorough training in mathe- 
matical reasoning, to create in him a sure mathematical 
imagination, and to meet fairly the reasonable demand for 
enlivening and enriching the subject through applications 
at the expense of piu-ely formal work that contains no essential 
principle. 

E. W. Davis, 
W. C. Brbnke, 

E. R. Hedrick, Editor. 
June, 1912. 



PREFACE TO THE REVISED EDITION 

The Davis Calculus was very favorably received by the 
mathematical world at the time of its original appearance 
in 1912. The necessity for some revision arose from the 
usual exhaustion of the old lists of exercises by repeated use 
of them in class-rooms, and from suggestions of minor changes 
of forms and of arrangement of the textual matter as a result 
of actual experience in its use. Professor Davis was intend- 
ing such a revision kt the time of his death, and it has re- 
mained for Professor Brenke, in collaboration with Professor 
E. R. Hedrick, to carry it out. 

The lists of exercises have been thoroughly revised. Most 
of the old formal exercises have been replaced by new ones, 
the lists have been extended or shortened, as experience 
indicated they should be, and some of the applications for- 
merly contained in the lists of problems have been trans- 
ferred to the body of the text. 

The spirit of the original text was to bring out to the 
student the real significance of the Calculus; and this was 
accomplished in an unusually effective manner. In the 
revision, every effort has been made to retain and to amplify 
this spirit. The technique, and mechanical drill, have not 
been neglected, but the reasons for learning this technique 
have been demonstrated to the student unmistakably. 

Some rearrangement of topics has occurred. Thus integra- 
tion as a simmiation has been postponed until after the 
technique of integration has been mastered. The latter half 
of the book has been somewhat simplified, and a few more 

xi 



xii PREFACE 

difficult topics that were not reached by many classes have 
been omitted. It is hoped that the revision will appeal to 
many and that it will do justice to the great teacher who 
was the principal author of the original edition. 

W. C. Brbnke, 
E. R. Hedrick. 



CONTENTS 

(Page numbers in roman type refer to the body of the book; those in italic type 
refer to pages of the Tables.) 

CHAPTER PAGE 

I. Functions — Slope — Speed 1 

II. Limits — Derivatives 14 

III. Differentiation of Algebraic Functions .... 24 

IV. Implicit Functions — Differentials 39 

V. Tangents — Extremes 49 

VI. Successive Derivatives 60 

VII. Reversal of Rates — Integration 79 

VIII. Logarithms — Exponential Functions .... 99 

IX. Trigonometric Functions 119 

X. Applications to Curves — Length — Curvature. . 133 

XL Polar Coordinates 147 

XII. Technique of Integration 156 

XIII. Integrals as Limits of Sums 192 

XrV. Multiple Integrals — Applications 208 

XV. Empirical Curves — Increments — Integrating Devices 234 

XVI. Law of the Mean — Taylor's Formula — Series . . 247 

XVII. Partial Derivatives — Applications 274 

XVIII. Curved Surfaces — Curves in Space 289 

XIX. Differential Equations 311 

TABLES 
TABLE 

I. Signs and Abbreviations 1 

II. Standard Formulas .......... 3 

III. Standard Curves 19 

IV. Standard Integrals 35 

V. Numerical Tables 61 

Index 61 



xui 



THE CALCULUS 

CHAPTER I 

FUNCTIONS — SLOPE — SPEED 

1. Variables. Constants. Functions. A quantity which 
changes is called a variable. The temperature at a given 
place, the annual rainfall, the speed of a falling body, the dis- 
tance from the earth to the sun, are variables. 

A quantity that has a fixed value is called a constarrt. 
Ordinary numbers, such as 2/3, n/2, — 7, tt, log 5, etc., are 
constants. 

If one variable, y, depends on another variable, x, in such 
a way that y is determined when x is known, y is called a 
function of z; the variable z is called the independent variable, 
and y is called the dependent variable. Thus the area A of a 
square is a function of the side a of the square, since A = s^. 
The volume of a sphere is a function of the radius. In 
general, a mathematical expression that involves a variable 
a: is a function of that variable. 

2. The Function Notation. A very useful abbreviation for a 
function of a variable x consists in writing / (x) (read / of x) 
in place of the given expression. 

Thus if fix) = a;2 + 3x + 1, we may write /(2) = 2^ + 
3- 2 + 1 = 11, that is, the value of x^ + 3 x + 1 when x = 2 
is 11. Likewise /(3) = 19, /(- 1) = - 1, /(O) = 1, etc. 
/(a) = a^ + 3 a + 1. f(u + v)==(u + vy + Siu + v) + 1. 

Other letters than / are often used, to avoid confusion, but 

/ is used most often, because it is the initial of the word func- 

1 



2 THE CALCULUS [I, § 2 

Hon, Other letters than x are often used for the variable. 
In any ease, given /(x), to find /(a), simply substitute a for 
X in the given expression. 

3. Graphs. In our study of variables and functions, much 
use will be made of graphs. To draw the graph of an equa- 
tion that contains two variables, we may determine by trial 
several pairs of numbers which satisfy the equation and plot 
these number pairs as points of the graph, as in elementary 
analytic geometry. 

Shorter methods for drawing certain graphs are indicated 

in some of the following exercises. Thus to draw the graph 

of the equation 

y = amx-\- cos x, 

first draw on the same sheet of paper the graphs of the two 

equations 

2/ = sin X and y = cos x, 

and add the corresponding ordinates. 

Certain standard graphs are shown in the tables at the 
back of this book. 

EXERCISES 

Calculate the values of each of the following functions for a suitably 
chosen set of values of x, and draw the graph. Estimate the values of 
X and / (x) at points where the curve has a highest or a lowest point. 
Also determine graphically the solutions of the equation f(x) = 0. 

1. fix) = aj2 - 5a; 4- 2. 2. fix) ^ x^ -2x + ^. 

3. /(x) = fr*-5x3 4-3a:2-2a:4-3. 4. fix) = ix + l)/i2x-S). 

6. fix) = logioo;. 6. fix) = (logioaj)^. 

7. fix) = sin X. 8. fix) = esc x, 

9. fix) = cos X. 10. fix) = sin a; + cos a:. 

11. fix) = a; + sin x. 12. fix) = sin 2 x. 



I, § 3] FUNCTIONS — SLOPE — SPEED 3 

13. If fix) = sin a; and <t>ix) = cosx, show that [f{x)\^ + [<l> (x)]2 = 1; 
/(a:)-?-<A(x)=tanx; fix + y) ==f{x) <t>(y) +f(y) 4>{x); <t>(x + y)=7; 
fix) = <^(x/2 - x); 4>ix) =/(x/2 - a;) = - <^ (x - x); /(- x) = 

14. If fix) = logio Xf show that 

fix) +f(y) ^fix-y); fix^) = 2 fix); 

/(m/n)-/(n/m) =2/(m)-2/(n); /(m/n) +/(n/m)=0. 

16. Jf fix) = tan a;, 4» ix) =» cos a;, draw the curves y — / (a;), y = <^ (x), 
y —fix) — <t>ix). Mark the points where fix) = ^ (x) and estimate the 
values of x and y there. 

16. Taking /(x) =x2, compare the graph of 2/ =/(x) with that of 
2/ = fix) + 1, and with that of 2/ = /(x + 1). 

17. Taking any two curves y =/(x), y = <^(x), how can you most 
easily draw y -fix) — <t>ix) ? 2/ = /(x) + <^ (x) ? Draw y - x^ -\- 1/x. 

18. How can you most easily draw 2/=/(x)+5? y=/(x + 5)? 
assuming that y = /(x) is drawn. 

19. Draw y = x^ and show how to deduce from it the graph of 
y — 2x^; the graph of y = — x^. 

Assuming that y—fix) is drawn, show how to draw the graph of 
y = 2/(x); that of y = —fix). 

20. From the graph oi y — x^, show how to draw the graph of 
2/ = (2 x)2; that of 2/ = x2 + 2; that of t/ = (x + 2)2; that of 2/ = (2x - 3)2. 

21. What is the effect upon a curve if, in the equation, x and y are 
interchanged? Compare the graphs of y =/(x), x ^fiy). 

Plot each of the following curves: 

22. 2/ + l = sin(3x-2). 23. 2^=2«+sinx. 

24. y = 2* + 2-*. 26. 2^ = 2-» cos x. 

Plot each of the following curves, using polar coordinates. 
26. r = sin 0. 27. r = sin 2 0. 

28. r = C06 3 ^. 29. r = 3 + 2 sin 0. 

30. r = 2 + 3 sin e, 31. r = 1 + cos 0. 

32. r = 0. 33. r = lA 

34. r = 2». 36. r = 2-«. 



THE CALCULUS 



n, H 



4. Rate of Increase. Slope. In the study of any quantity, 

its rate of increase (or decrease), when some related quantity 

changes, is a very important consideration. 

Graphically, the rate of increase of y with respect to z is 

shown by the rate of increase of the height 

of a curve. If the curve ia very flat, there 

is a small rate of increase; if steep, a lai^ 

j-ate. 

The steepness, or slope, of a curve shows 
the rate at which the dependent variable is 
increasing with respect to the independent 
variable. When we speak of the slope of 
a curve at any point P, we mean the slope 
of its tangent at that point. To find this, 
we must start, as in analytic geometry, with 
a secant through P. Let the equation of 
the curve, Fig. 1, he y = 3^, and let the 
point P at which the slope is to be found, be the point (2, 4). 
Let Q be any other point on the curve, and let Ax represent 
the difference of the values of x at the two points P and Q-* 
Then in the figure, OA = 2, AB = iix, and OB =2 + Ai. 
Moreover, since y = z" at every point, the value of y at Q is 
BQ = (2 + Az)^. The slope of the secant PQ is the quo- 
tient of the differences Ay and Ax: 

_ A^ _ MQ _ (2J 




Fig. 1. 



tan Z MPQ = ^ 

Ax 



MQ_ 
' PM~ 



Ax 



= 4 + Aar. 



The slope m trf the tangent at P, that is tan Z MPT, is the 

* Ax may be regarded aa an abbreviation of the phrase, "difference of 
,he x's," The quotient of two such differencea is called a difference ipio- 
ienl. Notice particularly that Axdoeanol mean A X z. Inateod of "differ- 
iiice of the x'a." the phrases "chaoge in x" and "increment of x" are ofteo 



I, § 4] FUNCTIONS — SLOPE — SPEED 5 

limit of the slope of the secant as Q approaches P. But it 
is clear that this limit as Q approaches P is 4, since Ax 
approaches zero when Q approaches P. Hence the slope 
m of the curve is 4 at the point P. At any other point the 
argument would be similar. If the coordinates of P are 
(a, o*), those of Q would be [(a + Aa;), (a + Aa;)^]; and the 
slope of the secant would be the difference quotient Ay -r- Ax: 

Ay ^ (g + AxY - a^ ^ 2aAx + Ax^ = 2a + Ax 
Ax Ax Ax 

Hence the slope of the curve at the point (a, a^) is * 

m = lim Ay /Ax = lim (2 a + Ax) = 2 a. 

On the curve y = x^, the slope at any point is numerically 
twice the value of x. When the slope can be found, as above, 
the equation of the tangent at P can be written down at 
once, by analytic geometry, since the slope m and a point 
(a, b) on a line determine its- equation: 

y —6 = m(x — a). 

The normal to a curve is defined to be the line through a 
point on the curve perpendicular to the tangent line at that 
point. Hence, if the slope of the tangent at a point (a, b) 
is m, the slope of the normal is -^ 1/m, and the equation of 
the normal is 

2/-6= --(x-a). 

Thus, in the preceding example, at the point (2, 4), where we found 
m=4, the equation of the tangent is 

(2/ — 4) = 4 (x — 2), or 4 a; — y = 4. 
The equation of the normal is 

y - 4 = - J (x - 2), or a; + 4 2/ = 18. 

* Read " Aa;-» 0'* "as Aa; approaches zero." A discussion of limits is given 
in Chapter II. 



6 THE CALCULUS [I, § 5 

6. General Rules. A part of the preceding work holds true 
for any curve, and all of the work is at least similar. Thus, 
for any curve, the slope is 

m = lim (Ay /Ax) ; 

Ax— K) 

tfiat is J the slope m of the curve is the limit of the difference quo- 
tient Ay /Ax. 

The changes in various examples arise in the calculation of 
the difference quotient, Ay 4- Ax, and of its limit, m. 

This difference quotient is always obtained, as above, by find- 
ing the value of y at Q from the value of x ai Q, from the equa- 
tion of the curve, then finding Ay by subtracting from this the 
value of y at P, and finally forming the difference quotient by 
dividing Ay by Ax. 

6. Slope Negative or Zero. If the slope of the curve is 
negative, the rate of increase in its height is negative, that is, 
the height is really decreasing with respect to the independent 
variable.* 

If the slope is zero, the tangent to the curve is horizontal. 
This is what happens ordinarily at a highest point (maximum) 
or at a lowest point (mininaum) on a curve. 

Example 1. Thus the curve 2/ = x^, as we have just seen, has, at any 
point X = a,a. slope w = 2 a. Since m is positive when a is positive, the 
curve is rising on the right of the origin; since m is negative when a is 
negative, the curve is falling (that is, its height y decreases as x increases) 
on the left of the origin. At the origin w = 0; the origin is the lowest 
point (a minimum) on the curve, because the curve falls as we come 
toward the origin and rises afterwards. 

* Increase or decrease in the height is always measured as we go toward 
the right, i.e. as the independent variable increases. 



I, §61 



FUNCTIONS — SLOPE — SPEED 



Example 2. Find the slope of the curye 



y— x* + 3x — 5 



(1) 

at the point where a; = — 2; also in general at a point a; = o. Use these 

values to find the equation of the tangent 

at a; = 2; the tangent at any point. 

When X = — 2, we find y = — 7 (P in 
Fig. 2); talcing any second point Q, (— 2 + 
Ax, — 7 + Ay), its coordinates must satisfy 
the given equation, therefore 

-7+A2/ = (-2+Ax)2 

+ 3 (- 2 + Ax) - 6, 
or 

Ay — — ^ Ax -j-Ax2 4- 3 Ax 

= — Ax + Ax^, 

where Ax^ means the square of Ax. Hence 
the slope of the secant PQ is 

Ay /Ax = — 1 + Ax. 

The slope m of the curve is the limit of Ay /Ax 

as Ax approaches zero; i.e. Fig. 2. 



\ 
















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Az 


M 












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T 
















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= lim ^ = lim (- 1+ Ax) = - 1. 

Aaf->0 Ax 



Ajp-»0 



It follows that the equation of the tangent at (— 2, — 7) is 

(y + 7) = - 1 (x + 2), or X + 2/ + 9 = 0, 

Likewise, if we take the point P (a, b) in any position on the curve 
whatsoever, the equation (1) gives 

5 = o2 + 3 a - 5. 

Any second point Q has coordinates (a + Ax, b + Ay) where Ax and 
Ay are the differences in x and in y, respectively, between P and Q. 
Since Q also lies on the curve, these coordinates satisfy (1) : 

. b + Ay={a+ Ax)2 + 3 (a + Ax) - 5. 

Subtracting the last equation from the preceding. 

Ay = 2 o Ax + Ax^ + 3 Ax, whence Ay /Ax = (2 o +3) + Ax, 
and 

m = lim ^ = lim [(2 o + 3) + Ax] = 2 a + 3. 

Ax— »0 Ax J^x-*Q ' 

Therefore the tangent at (o, b) is 
y-(a2 + 3o-5) = (2a4-3) (x-o), or (2a + 3)x - y = a^ _|. 5. 



8 THE CALCULUS [I, ! 6 

The slope m is zero when 2 o + 3 = 0, i.e. when a - — 3/2. Hence 
the tangent is horizontal at the point where x = — 3/2. 

Example 3. Consider the curve y = x' — 12 1 + 7. If the value of 
X at any point P is «, the value of y is o' — 12 o + 7. If the value of x 
at Q is a + Ax, the value of ji at G is (a + Ax)' ~ 12 (a + Ax) + 7. 

Hence 

Ay_ [(o + Ax)^~12(a + A3:)+71-[<i'-12a+7] 

= {3 a^ + 3 o Ax + Ax') - 12, 



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! 




K 




■^ 


4t 


m 


m 



For example, if i — 1, y = ~ 4; at this pomt (1, — 4) the slope 
is 3-1^ — 12 = —9; and the equation of the tangent is 

(y + 4) = - 9 (X - 1), or 9 1 + y - 5 =0. 

The points at which the slope is zero would be determined by the 
equation w = 3 a* - 12 = 0, which gives a = ± 2. When x has either 
of these values, the tangent is horizontal. From the equation of the 
curve, it X = + 2, y ■■ — 9; when x = — 2, y — 23. Hence the horizontal 
tangents are at the points (2, - 9) and (- 2, 23). (See Fig. 3.) 



I, § 7] FUNCTIONS — SLOPE — SPEED 9 

EXERCISES 

Find the slope and the equation of the tangent line to each of the 
following curves at the point indicated. Verify each result by drawing 
the graph of the curve and the graph of the tangent line from their 
equations. 

1. 2/ = a;2 - 2; (1, - 1). 2. 2/ = x^l2\ (2, 2). 

3. y = 2 x2 -3; (2, 5). 4. 2/ = a;2 - 4 a; + 3; (2, - 1). 

6. y = rr3; (1, 1). 6. y = x3 - 9 x; (2, - 10). 

7. 2/ = xs - 3 a; + 4; (0, 4). 8. 2/ = 2 a;3 - 3 x^\ (1, - 1). 

Draw each of the following curves, using for greater accuracy the 
precise values of x and y for which the tangent is horizont£d, and the 
knowledge of the values of x for which the curve rises or falls. 

9. 2^ = a;2 4- 5 a; — 5. \% y — 0^ ^ x^. 16. 2/ = ^^ 

10. y^Zx-Q^.j 13. 2/=a^-6a;. 16. y^x^ — 2x^. 

11. y = aj3-3x4-2. 14. 2/ =25' -6 a; + 5. 17. 2^ = a;* __ 3^. 

7. Speed. An important case of rate of change is the 
rate at which a body moves, — its speed. 

Consider the motion of a body falling from rest under the 
influence of gravity. During the first second it passes over 
16 ft., dining the next it passes over 48 ft., during the third 
over 80 ft. In general, if i is the niunber of seconds, and s 
the entire distance it has fallen, s = 16 /^ if the gravitational 
constant g be taken as 32. The graph of this equation (see 
Fig. 4) is a parabola with its vertex at the origin. 

The speed, that is the rate of increase of the space passed 
over, is the slope of this curve, i.e. 

,. As 
lim — • 

This may be seen directly in another way. The average 
speed for an interval of time A^ is found by dividing the dif- 
ference between the space passed over at the beginning and at 



10 



THE CALCULUS 



[I, §7 



the end of that interval of time by the difference in time: i.e. 
the average speed is the difference quotient As -7- A^ By the 
speed at a given instant we mean the limit of the average 
speed over an interval At beginning or ending at that instant 
as that interval approaches zero, i,e, 

speed =^ lim-r?- 

Taking the equation s = 16 ^, if ^ = 1/2, 8 = 4 (see point P in Fig. 4). 

After a lapse of time A^, the new 
values are 

t==l/2+At, 
and « = 16 (1/2 + M^ 
(Q in Fig. 4). 
Then 

As = 16 (1/2 4- AO^ - 4 

= 16 A< + 16 A?, 
As /At = 16 + 16 At. 

Whence 

As 



\ 










s 






/ 


\ 








-AA- 








// 










-w 




s- 


= 16<* 


■y/ 




\ 














/ 




A 












i 


k 




n 


L 










J 








V 










/ 








\ 




1ft 




1 


7 










V 




T> 


// 












\ 





^' 


\t-^ 


t 


1 










7 




\ 



speed = lim ^ ^ 



Fig. 4. 



= lim (16 + 16 AO = 16; 



that is, the speed at the end of the first half second is 16 ft. per second. 

Likewise, for any value of «, say « = T, s = 16 T^) while for 
< = T + Af, « = 16 (T + At)^\ hence 



awrages 



peerf-^ = ^^^^ + ^\'-^'^-32r+16A« 



A^ 



and 



As 



speed = lim —: = 32 T. 

^-^At 



Thus, at the end of two seconds, T = 2, and the speed is 32-2 = 64, in 
feet per second. 

8. Component Speeds. Any cm^e may be regarded as the 
path of a moving point. If a point P does move along a 
curve, both x and y are fixed when the time t is fixed. To 



I, §91 



FUNCTIONS — SLOPE — SPEED 



11 



specify the motion completely, we need equations which 
give the values of x and y in terms of L 

The horizontal speed is the rate of change of x with 
respect to the time. This may be thought of as the speed 
of the projection Af of P on the x-axis. Likewise, the 
vertical speed is the rate of change of y with respect to 
the time. It would be the speed of the projection of P on 
the 2/-axis. Hence, by § 7, we have 



and 



Ax 
horizontal speed = lim -r-t 

At-^^t 



Since 



vertical speed ^ lim -Ji 



Ay _^Ay . Ax 
Ax" A/"^ A/' 




it follows that 

m = (vertical speed) 4- (horizontal speed) ; 

that is, the slope of the curve is the ratio of the rate of increase 
of y to the rate of increase of x. 

9. Continuous Functions. In §§ 4-8, we have supposed that 
the curves used were smooth. All of the functions which 
we have used could be represented by smooth curves. Except 
perhaps at isolated points, a small change in the value of 
one coordinate has caused a small change in the value of 
the other coordinate. Throughout this text, unless the 
contrary is expressly stated, the functions dealt with will 
be of the same sort. Such functions are called continuous. 
(See § 10, p. 14.) 

The curve y = 1/x is continuous except at the point 
a? = 0. The curve y = tan x ig continuous except at the 



12 THE CALCULUS [I, § 9 

points X = =*= 7r/2, =t 3 7r/2, etc. Such exceptional points 
occur frequently. We do not discard a curve because of 
them, but it is understood that any of our results may fail at 
such points. 

EXERCISES 

1. From the formula a = 16 ^, calculate the values of s when ^ = 1, 
2, 1.1, 1.01, 1.001. From these values calculate the average speed between 
^ = 1 and ^ = 2; between t = 1 and t = 1.1; between ^ == 1 and t = 1.01; 
between ^ = 1 and t = 1.001. Show that these average speeds are 
successively nearer to the speed at the instant ^ = 1. 

2. Calculate as in Ex. 1 the average speed for smaller and smaller in- 
tervals of time after t ^2; and show that these approach the speed at the 
instant t ^=2. 

3. A body thrown vertically downwards from any height with an 
original velocity of 50 ft. per second, passes over in time t (in seconds) a 
distance s (in feet) given by the equation « = 50 < + 16 ^ (if ^ = 32, as 
in § 7). Find the speed v at the time ^ = 1; at the time t ^2; at the 
time < = 4; at the time t = T. 

4. In Ex. 3 calculate the average speeds for smaller and smaller m- 
tervals of time after * = 0; and show that they approach the original 
speed «o = 50. Repeat the calculations for intervals beginning with 
« = 2. 

Calculate the speed of a body at the times indicated in the follow- 
ing possible relations between 8 and t: 

6. a = f2j ^ = 1, 3, 20, T, 7. s = - 16 «« + 80 «; < = 0, 2, 5. 

6. a = 16 f2 - 50 <; « = 0, 2, r. 8. « = ^ - 6 « + 4; < = 0, 1/2, 1. 

9. The relation in Ex. 7 holds (approximately, since ^ = 32 ap- 
proximately) for a body thrown upward with an initial speed of 80 ft. 
per second, where s means the distance from the starting point coimted 
positive upwards. Draw a graph which represents this relation between 
the values of s and t 

In this graph mark the greatest value of a. What is the value of v at 
that point? Find exact values of s and t for this point. 

10. A body thrown horizontally with an original speed of 8 ft. per 
second falls in a vertical plane curved path so that the values of its hori- 



I, § 9] FUNCTIONS — SLOPE — SPEED 13 

zontal and its vertical distances from its original position are respec- 
tively, X ==St,y == Wt^, where y is measured downwards. Show that the 
vertical speed is 32 Tj and that the horizontal speed is 8, at the instant 
t = T, EUminate t to show that the path is the curve 4 y = x^. 

11. Find the component speeds and the resultant speed when the 
path is given by the equations 

x=t + l,y = fi'-l. 

Calculate their numerical values when < = 1; when ^ = 0; when t = 2, 
Plot the path. 

12. Proceed as in Ex. 11 when the path is given by the equations 

a; = 2 + <2, y = 2 - ^. 



CHAPTER II 

LIMITS — DERIVATIVES 

10. Limits. Infinitesimals. We have been led in what pre- 
cedes to make use of limits. Thus the tangent to a curve at 
the point P is defined by saying that its slope is the limit of 
the slope of a variable secant through P; the speed at a given 
instant is the limit of the average speed; the difference of the 
two values of x, Ax, was thought of as approaching zero; and 
so on. To make these concepts clear, the following precise 
statements are necessary and desirable. 

When the difference between a variable x and a constant a he- 
com£S and remains less, in absoliUe value* than any prea^signed 
positive quantity y however smaUy then a is the limit of the 
variable x. 

We also use the expression "x approaches a as a limit,'' or, 
more simply, "x approaches a." The symbol for limit is 
Urn; the symbol for approaches is — >; thus we may write 
lim X = a, or x— >a, or lim (a — x) =0, or a — a;— >0.t 

When the limit of a variable is zero, the variable is called 
an infinitesimal. Thus a — x above is an infinitesimal. 
The difference between any variable and its limit is always 
an infinitesimal. When a variable x approaches a limit a, 
any continuous function f (x) approaches the limit f (a) : 

* When dealing with real numbers, absolute value is the value without 
regard to signs, so that the absolute value of —2 is 2, for example. A con- 
venient symbol for it is two vertical lines; thus |3 — 7|=4. 

t The symbol = is often used in place of ->. 

14 



II, § II] LIMITS — DERIVATIVES 15 

thus, if y =/(x) and ft =/(«), we may write 
lim y = b, or lim f{x) =f (a) . 

This GonditioQ ia tho precise definition of continuity at the 
point x=a. (See § 9, p. 11.) 

11. Properties of Limits. The following properties of limits 
will be assumed as self-evident. Some of them have already 
been used in the article noted below. 

Theorem A. The limit of the sum of two varuAlesis the sum 
of the limits of the two variables. This is easily extended to the 
case of more than two variables. (Used in §§ 4, 6, and 7.) 

Theorem B. The limit of the jfroduct of two varieties is the 
product of the limOs of the variables. (Used in §§ 4, 6, and 7.) 

Theorem C. The limit of the quotient of one variable divided 
by another is the gu(^ient of the limits of the variables, provided 
the limit of the divisor is n,ot zero. (Used in § 8.) 

The exceptional case in Theorem C ia really the most in- 
teresting and important case of all. The exception arises 
because when zero occurs as a denominator, the division can- 
not be performed. In Boding the slope of a curve, we con- 
sider lim (Aj//Ai) as Ax approaches zero; notice that this is 
precisely the case ruled out in Theorem C, Again, fhe speed 
is lim (As/M) as At approaches zero. The limit of any such 
difference quotient is one of these exceptional cases. 

Theorem D. The limit of the ratio of two infinitesimals de- 
pends upon the law connecting them; otherwise it is quite inde- 
terminate. Of this the student will see many instances; for 
the Differential Calculus coTmsts of the consideration of just such 
limits. In fact, the very reason for the existence of the Differ- 



16 THE CALCULUS [H, § 11 

ential Calculus is that the exceptional case of Theorem C is 
important, and cannot be settled in an offhand manner. 

The thing to be noted here is, that, no matter how small 
two quantities may be, their ratio may be either small or 
large; and that, if the two quantities are variables whose 
limit is zero, the limit of their ratio may be either finite, zero, 
or non-existent. In oiu* work with such forms we shall try to 
substitute an equivalent form whose limit can be found. 

Theorem D accounts for the case when the numerator 
as well as the denominator in Theorem C is infinitesimal. 
There remains the case when the denominator only is 
infinitesimal. A variable whose reciprocal is infinitesimal is 
said to became infinite as the reciprocal approaches zero. 

Thus 

y = lA 

is a variable whose reciprocal is 2;. As x approaches zero, y 

is said to become infinite. Notice, however, that y has no 

value whatever when x == 0. 

Likewise 

y = sec X 

is a variable whose reciprocal, cos x, is infinitesimal as x 
approaches t/2. Hence we say that sec x becomes infinite 
as X approaches t/2. In any case, it is clear that a 
variable which becomes infinite becomes and remains larger 
in absolute value than any preassigned positive number, 
however large. 

The student should carefully notice that infinity is not a 
number. When we say that "sec x becomes infinite as x ap- 
proaches V2/' * we do not mean that sec (t/2) has a value, 
we merely tell what occurs when x approaches 7r/2. 

♦ Or, as is stated in short form in many texts, "sec (ir/2) « 00." 



II, § 11] LIMITS — DERIVATIVES 17 

EXERCISES 

1. Imagine a point traversing a line-segment in such fashion that it 
traverses half the segment in the first second, half the remainder in the 
next second, and so on; always half the remainder in the next following 
second. Will it ever traverse the entire line? Show that the remainder 
after t seconds is l/2<, if the total length of the segment is 1. Is this 
infinitesimal? Why? 

2. Show that the distance traversed by the point in Ex. Ivat seconds 
is 1/2 + 1/22 + ... + 1/2*. Show that this sum is equal to 1 - 1/2'; hence 
show that its limit is 1. Show that in any case the limit of the distance 
traversed is the total distance, as t increases indefinitely. 

3. Show that the limit of 3 — o^ as 2; approaches zero is 3. State this 
result in the symbols used in § 10. Draw the graph of y = 3 — x^ and 
show that y approaches 3 as 2; approaches zero. 

Evaluate the following limits: 



4. 


lim (7-5a;+3a;2). 


7. 


,. 3-2a;2 

i^24 + 2x2- 


® 


,. a;2 - 3 a; + 2 

x^2X^+2x-\-3' 


6. 


lim(7-5a;+3a;2). 

x-*2 


8. 


,. 2x 

um 7 • 

x-^ 4 — a; 


11. 


lim^J^. 


6. 


]im{k^+kx-2x^). 


9. 


,. 1 — X 
lim • 

X_>2 X 


12. 


y a + 6a;+ca;2 
x-^om-\-nx-\-lx^' 



If the numerator and denominator of a fraction contain a common 
factor, that factor may be canceled in finding a limit, since the value of 
the fraction which we use is not changed. Evaluate before and after 
canceling a common factor: 

^- ,. (x - 2) (x - 1) .^ ,. a;2(x-2) 

-j^_i(2 x — Z)(x—l) x-*2 (x2 + 1) (x — 2) 

a;2 lex ,. a;2-4a; + 3 />. ,. a;2+a;-2 



15. linl?-^ % lim ^^7^+^ rf7) Um 



x_>o X ^^* x-^1 a;2 — 1 v_/ x^i 2 x2 + X — 3 



4oi 1- ^X-hl -ft r X2(X--1)2 X« 

IBJ hm r^' 19. lim —7^ — jr-f-. 20. lim — = 

x^-i x + 1 x-*ox^ — 2x^ x-^ X 




0, n>l, 
ll,n = l. 



@ Show that 



,. 3x2 + 5 , 
lim « , . ;— = = 3. 

x-^ x2 + 4 X + 5 



[Hint. Divide numerator and denominator by x*; then such terms as 
5/x> approach zero as x becomes infinite.] 



18 



THE CALCULUS 



[11, § 11 



Evaluate: 
2x 



22 






-1 



-2 



23. lim 



5a;2-4 



25. lim 



2z 



«— >« 



ViT 



26. lim 



rr-Ko3 a;2 + 2 



24. lim 



aa; + 6 



X' 



X— MO Vaj^ — 4 



27. 



x—¥»mx -\-n 



lim 



px+g' 




28. Let be the center of a circle of radius r = 05, and let a = Z C0J5 

be an angle at the center (Fig. 6). Let BT be 
perpendicular to 05, and let BF be perpendic- 
* ular to OC, Show that OF approaches OC as a 
approaches zero; likewise arc CB-*0, arc 
DB^O, andFC-»0, asa-*0. 

29. In Fig. 6, show that the obvious 

Fig. 6. geometric inequality FB < arc CB <BT is 

equivalent to r sin a<r'a<r tan a, if a is measured in circular measure. 

Hence show that a/sin a lies between 1 and 1/cos a, and therefore 

that lim (a/sin a) = 1 as «-> 0. (Cf. § 72.) 

30. In Fig. 6, show that 

,. FB ^ ,. OF , ,. BT f. y FC ^ ,. arc 05 ^ 
Imi — = 0: Imi — =1; lim — = 0: lim — = lim = 0. 

12. Derivatives. While such illustrations as those in the pre- 
ceding exercises are interesting and reasonably important, 
by far the most important cases of the ratio of two infini- 
tesimals are those of the type studied in §§ 4-8, in which each 
of the infinitesimals is thq difference of two values of a varia- 
ble, such as Aiz/Ax or As/ At, Such a difference quotient 
Ay/AXj of y with respect to x, evidently represents the 
average rate of increase of y with respect to x in the interval 
Ax; if X represents time and y distance, then Ay /Ax is the 
average speed over the interval Ax (§ 7, p. 9); if y =/(x) 
is thought of as a curve, then Ay /Ax is the slope of a secant 
or the average rate of rise of the curve in the interval Ax 
(§ 4, p. 4). 



II, § 13] LIMITS — DERIVATIVES 19 

The limit obtained in such cases represents the instanta- 
neous rate of increase of one variable with respect to the 
other, — this may be the slope of a curve, or the speed of a 
moving object, or some other ratej depending upon the 
nature of the problem in which it arises. 

In general, the limit of the quotient Aiz/Ax of two infinitesim/il 
differences is called the derivative of y with respect to x; it is 
represented by the symbol dy/dx: 

JL s derivative of y with respect to x= lim = • 
ax Ax-^ Ax 

Henceforth we shall use this new symbol dy/dx or other 
convenient abbreviations; * but the student must not forget 
the real meaning: slope, in the case of curve; speed, in the 
case of motion; some other tangible concept in any new 
problem which we may undertake. In every case the meaning 
is the rate of increase of y mth respect to x. 

Any mathematical formulas we obtain will apply in any of 
these cases. We shall use the letters x and y, the letters s 
and t, and other suggestive combinations; but any formula 
written in x and y also holds true, for example, with the 
letters s and t, or for any other pair of letters. 

13. Formula for Derivatives. If we are to find the value of 
a derivative, as in §§ 4-7, we must have given one of the vari- 
ables 2/ as a function of the other x: 

(1) y=f(x). 

If we think of (1) as a curve, we may take, as in § 4, any 

* Often read "the x derivative of y." Other names frequently used are 
differerUial coefficient and derived function. Other convenient notations are 
Dxy, yx, fix) y', y; the last two are not safe unless it is otherwise clear 
what the independent variable is. 




20 THE CALCULUS [II, § 13 

point P whose coordinates are x and y, and join it by a secant 
PQ to any other point Q, whose coordinates are x + Ax, y + Ay. 

Here x and y represent fixed values 
of X and y. This will prove more 
convenient than to use new letters 
each time, as we did in §§ 4-7. 

Since P lies on the curve (1), its 
coordinates {x, y) satisfy the equa- 
tion {l),y —f {x). Since Q lies on 
(1), X + Ax and y + Ay satisfy the same equation; hence we 

must have 

(2) t/ + A2/=/(x + Ax). 

Subtracting (1) from (2) we get 

(3) Ai/=/(x + Ax)-/(x). 
Whence the difference quotient is 

fA^ ^y /(x + Ax) —fix) , „,^ 

(4) -^ = '^— — ' — -^ — ^-^^^ = average slope over PM, 

and therefore the derivative is 

(5) <k =lim^^lim ^(' + y--^('> =aopeatP* 
ax az-»oAjc az->o Ax 

14. Rule for Differentiation. The process of finding a de- 
rivative is called differentiation. To apply formula (5) of § 13: 

(A) Find (y + Ay) by substituting (x + Ax) for x in the given 
function or equation; this gives y + Ay = f{x + Ax). 

{B) Subtract y from y + Ay; this gives 

Ay=f{x + Ax) -fix). 

* Instead of slope, read speed in case the problem deals with a motion, 
as in § 7. In general, Ay /Ax is the average rate of increase, and dy/dx is 
the instantaneous rate. 



II, § 14] LIMITS — DERIVATIVES 21 

(C) Divide Ay by Ax to find the difference quotient Ay/Ax; 
simplify this result. 

(D) Find the limit of Ay /Ax as Ax approaches zero; this 
result is the derivative, dy/dx. 

Example 1. Given y ^f {x) ^x^^to find dy/dx, 

(A) / (a; + Aa;) = (a; + Aa;)2. 

(B) Ay=f(x+/^)-f{x) = (x + Aa;)2-a;2 =2xAx + Ix^, 

(C) Ay/Ax = (2xAx + A?) -^ Aa; = 2 a; + Aaj. 

(D) dy/dx = lim Ay /Ax = lim (2 x + Aa;) = 2 a;. 

Aap— ►O Ax— ►0 

Compare this work and the answer with the work of § 4, p. 5. 

Example 2. Given y =f(x) ^ofi — 12 a: + 7, to find dy/dx, 

}{x-YAx) = (a;+Aa;)3- 12 (a; + Ax) + 7. 
{B) Ay =/(a; + Ax)-/(x) = 3 x^ Ax + 3 x A? + Aa:' - 12 Ax. 

(C) Ay/Ax = 3 x2 + 3 X Ax + Ax^ - 12. 

(D) dy/dx = lim Ay/Ax = lira (3 x2 + 3 x Ax + Ax^ - 12) = 3 x2 - 12. 

A«— M) Ax— »0 

Compare this work and the answer with the work of Example 3, § 6. 

Example 3. Given y —fix) ^ l/x2, to find dy/dx, 

1 



(A) /(x+Ax) = 

{B) Ay=/(x + Ax)-/(x) = 



(x + Ax)2 

1 _ 1_ 2xAx + Ax 

(X + AX)2 X2 X2 (X + AX)2 



rn ^ = _ 2X + AX 

^^ AX X2(X+AX)2' 

(Z» dy/dx =^lim^g = mnj~ /(^ J^) j = - |f = " |' 

Example 4. Given y =/ (x) s Vx, to find dy/dx, or (^ {x)/dx. 
(A) / (x + Ax) = Vx + Ax. 

(5) A2/=/(x + Ax)-/(x) = Vx+Ax— y/x, 

(C) ^ = ^^ + Ax — Vx _ Vx + Ax -- Vx Vx + Ax + Vx 
Ax Ax "" Ax Vx + Ax + Vx 

1 

Vx + Ax + Vx 

(D) ^=ii„,^=lto 1 ?_. 



dx Ax-»o Ax Ax-»0 Vx + Ax + Vx 2Vx 



22 THE CALCULUS [II, § 14 

Example 5. Given ?/ = / (a;) ^ x^t ^ find ^/ {x)/dx. 
(A) / (x + Ax) = (x + Ax)7 = x7 + 7 x^ Ax + (terms with a factor A?). 
(5) Ay = / (x + Ax) — / (x) = 7 X® Ax+ (terms with a factor Ax^). 

(C) Ay/Ax = 7 X® + (terms with a factor Ax). 

(D) dy/cte = lim Ay /Ax = lim [7 x^ + (terms with a factor Ax)] = 7 x^. 

EXERCISES , 

Find the derivative, with respect to x, of each of the following 
functions: 



1. 


x2 - 4 X + 3. 


5. 8x — X*. 


2. 


X8+2X2. 


6. X4+X2+1. 


3. 


3x--x«. 


X-- 1 


4. 


• 

X4+2X2. 


^' A ^ o' 



10. 

11. 



X2 



x-1 
3x-2 



x + 2 

tt. VF=1. 

13. Find the equation of the tangent to the curve y = 4/x at the point 
where x = 3. 

14. Determine the values of x for which the curve y = x'--12x + 4 
rises, and those for which it falls. Draw the graph accurately. 

Proceed as in Ex. 14 for each of the following curves: 
16. x«-15x + 3. 17. 2x*--64x. 

16. x8-3x2. 18. x4-32x2. 

19. If a body moves so that its horizontal and its vertical distances 
from a point are, respectively, x = 15^, y = — 16^ + 15 1, find its hori- 
zontal speed and its vertical speed. Show that the path is 

2/ = - 16x2/225+x, 

and that the slope of this path is the ratio of the vertical speed to the 
horizontal speed. [These equations represent, approximately, the mo- 
tion of an object thrown upward at an angle of 45°, with a speed 15V2.] 

20. A stone is dropped into still water. The circumference c of the 
growing circular waves thus made, as a function of the radius r, is c = 2 irr. 

Show that dc/dr = 2 x, i.e. that the circumference changes 2 x times as 
fast as the radius. 



II, § 14] LIMITS — DERIVATIVES 23 

Let A be the area of the circle. Show ihsiidA/dr = 2 irr; i.e. the rate 
at which the area is changing compared to the radius is numerically 
equal to the circumference. 

21. Determine the rates of change of the following variables: 

(o) The surface of a sphere compared with its radius, as the sphere 
expands. 

(6) The volume of a cube compared with its edge, as the cube enlarges. 

(c) The volume of a right circular cone compared with the radius of 
its base (the height being fixed), as the base spreads out. 

22. If a man 6 ft. tall is at a distance x from the base of an arc light 
10 ft. high, and if the length of his shadow is s, show that «/6 = 05/4, or 
« = 3 x/2. Find the rate (ds/dx) at which the length s of his shadow 
increases as compared with his distance x from the lamp base. 



CHAPTER III 
DIFFERENTIATION OF ALGEBRAIC FUNCTIONS 

16. Classification of Functions. For convenience it is usual 
to classify functions into certain groups. 

A function which can be expressed directly in terms of the 
independent variable x by means of the three elementary 
operations of multipUcation, addition, and subtraction is 
called a polynomial in x. 

Thus, 2x^ + 4:31^ — 7x + 3y x^ — 4x + 6, etc., are poly- 
nomials. The most general polynomial is Oox" + aix^~^ + 
. . . + On-iX + a», where the coefficients a©, ai, . . . , On are 
constants, and the exponents are positive integers. 

A function which can be expressed directly in terms of 
the independent variable x by means of the four elementary 
operations of multiplication, division, addition, and sub- 
traction, is called a rational function oix. Thus, 1/x, {x^ — 
3 x)/{2 x+7), etc., are rational. The most general rational 
function is the quotient of two polynomials, since more than 
one division can be reduced to a single division by the rules 
for the combination of fractions. All polynomials are also 
rational functions. 

If, besides the four elementary operations, a function re- 
quires for its direct expression in the independent variable x 
at most the extraction of integral roots, it is called a simple 

algebraic function * of x. Thus, Vx, (Vx^ + 1 - 2)/(3 - v^x), 

* Since the expression "algebraic function" is used in the broader sense 
of § 25 in advanced mathematics, we shall call these simple algebraic 
functions. 

24 



Ill, § 16] ALGEBRAIC FUNCTIONS 25 

etc., are simple algebraic functions. All rational functions 
are also simple algebraic functions. 

Simple algebraic functions which are not rational are 
called irrational functions, 

A fimction which is not an algebraic function is called a 
transcendental function. Thus sinx, log x, e^, tan-^ (1 + x) + x^, 
etc., are transcendental. 

In this chapter we shall deal only with algebraic functions. 

16. Differentiation of Polynomials. We have differentiated 
a number of polynomials in Chapter I. To simplify the 
work to a mere matter of routine, we need four rules: 

The derivative of a constant is zero: 

The derivative of a constant times a function is equal to the 
constant times the derivative of the function: 

[H] i^ = c.*f. 

dx dx 

The derivative of the sum of two functions is equal to the sum 
of their derivatives: 

[III] d{u + v) ^^ dv^ 

dx dx dx 

The derivative of a power y x**, with respect to x is nx**""^: 

[IV] ^ = nxn-K 

dx 

[We shall prove this at once in the case when n is a positive integer; 
later we shall prove that it is true also for negative and fractional 
values of n.] 

Each of these rules was illustrated in Chapter II, § 14. 
To prove them we use the rule of § 14. 



26 THE CALCULUS [III, § 16 

Proof of [I]. Iiy=Cj a. change in x produces no change in 
y; hence Ay = 0. Therefore dy/dx = lim Ay /Ax = lim = 
as Ax approaches zero. Geometrically, the slope of the 
curve 2/ = c (a horizontal straight line) is everywhere zero. 

Proof of [H]. If y = C'U where w is a function of x, a 
change Ax in a: produces a change Au in u and a change Ay in 
y; following the rule of § 14 we find: 

(A) y + Ay = c (u + Au). 

(B) Ay = c Au. 

.-r,. dy ., r Aul ,. Au du 

(D) :^= lim \c'-r- = clim t— = c-t" 

ax Ax-»oL Ax J Aa^-♦oAa: dx 

Thus d{7x^)/dx = 7 • dix^)/dx = 7 • 2 x = 14 x. (See §§ 4, 
15.) 

Proof of [III]. If y = u + Vf where u and v are functions of 
X, a change Ax in x produces changes At/, Aiz, Ay in y, u, v, 
respectively, hence 

(A) y + Ay=(u + Au) + (v + Av); 

(B) Ay = Au + Av; 

^^Au Av_^ 
^^ Ax Ax "^ Ax ' 

(D) :j = li"^ T~ + li"^ T- = 3- + 3-- 

ax Aaj-*oAX Aa;-*oAx ttX OX 

Thus 

d{x^ - 12 X + 7) _ d(x3) _ d(12 x) ^ d{l) _ 3 ^ ^g 

dx dx dx dx , ' 

by applying the preceding rules and noticing that dx^/dx 
= 3x2. 



Ill, § 16] ALGEBRAIC FUNCTIONS 27 

Proof of [IV]. If 2/ = .r", we proceed as in Example 5, § 14. 

(A) y + Ay = {x + Ax)** = a:** + nx"~^Ax + (terms whicli 

liave a common factor Ax^). 

(B) Ay = nx'*~^Ax+ (terms with a common factor Ax^). 

(C) Ay /Ax = nx**"^ + (terms wliicli liave a factor Ax). 

(D) dy/dx = lim (AyJAx) = nx^~^. 

Tliis proof liolds good only for positive integral values of n. 
For negative and fractional values of n, see §§ 17, 21. 

Example 1. d {x^)/dx = 9 x^. 

Example 2. dx/dr = 1 • x° = 1, since a;® = 1. 

This is also evident directly: dx/dx = lim Ax/Ax = 1. Notice how- 
ever that no new rule is necessary. ^^»-»o 

Examples. $-(x*-7 x^ + 3x- 5) =4a;8- 14a; +3. 

dx 

Example 4. ^ (Ax» + Bx^ + C) = wAa;w-i + nBa;»-i. 

dx 

EXERCISES 

Calculate the derivative of each of the following expressions with re- 
spect to the independent variable it contains (x or r or 8 or t or y or u). 
In this list, the first letters of the alphabet, down to n, inclusive, repre- 
sent constants. 

1. y = Sx*. 5. s = 10t^-{-50t 9. g = 6<« + 3<«. 

2. y = a;V5. 6. « = - 4« + 2 «». 10. q = tT-8t^ + 10. 

3. y = 4a:5 + 5. 7. 8=Z{t*'-2fi). 11. g = 6(r8 + r2 + 1). 

4. y = 5(a;« - 3). 8. « = ??i<2 + nt\ 12. g = Ario + ^^6. 
13. u = v{v- 1). 14. w = (1 - f;2) (2 -f- ^2). 

16. w = v\v5 + 2). 16. M = (t;« + 2) (t;6 - 3). 

17. 3 = 02/5(2/8 -6t/4). (^ a = t*io(2 m7 - 5 1*9 + 8). 
19. 2 = A;a;» + ^». (^ r =cx»» -- (ia;2». 

21. r-«»(«2»_^2). 22. «=A-52/*"'. 



28 THE CALCULUS [III, § 16 

Locate the vertex of each of the following parabolas by finding the 
point at which the slope is zero. 

23. y = x^+4x + 4. 25. y = 5 + 2x-a:2. 

24. y =x^-6x + 2, 26. y = ax^+2bx+c, 

27. What is the slope of the curve j/ = 2 a;' — 3 x^ -|- 4 at a: = 0, ±2, 
± 4? Where is the slope 9/2? - 3/2? Where is the tangent hori- 
zontal? Draw the graph. 

28. What is the slope of the curve y = x*/4 — 2 x' + 4 a:^ at a: = 0, 
1,-1,-2? Where is the tangent horizontal? Where is the slope 
equal to eight times the value of x? 

29. Show that the function a;' — 3x2-f3a: — 1 alwa3rs increases 
with X. Where is the tangent horizontal? 

30. Find the angle between the curve y ^x^ and the straight line 
2/ = 9 a; at each of their points of intersection. 

17. Differentiation of Rational Functions. In order to dif- 
ferentiate all rational functions, we need only one more rule, 
— that for differentiating a fraction. 

The derivative of a quotient NJD of two functions N and D 
is equal to the denominator times the derivative of the numerator 
minus the numerator times the derivative of the denominator, aU 
divided by the square of the denominator: 

rvi VD/ _ dx dx 

^^ dx D2 

To prove this rule, let y = N/D, where N and D are func- 
tions of x; then a change Ax in x produces changes Ai/, AN, 
AD in y, N, and D, respectively. Hence, by the rule of § 14 : 

fB\ A ^ ^+^ N_ D'AN-N^D 



Ill, i 171 ALGEBRAIC FUNCTIONS 29 



(O 



(D) 



Ay__ Ax Ax , 
Ax"" D{D + AD) ' 

— = lim — = ^^ ^ . 



, ,_^3 (3.-7)|(x2 + 3)-(x^4-3)|(3.-7) 

^^^^^- &{.z^7) (S^T^^ 

(3a; -7)2 . (3a;-7)a 

Example 2. 



5 ^C^V 



(x2)2 a:* aft 

(Compare Example 3, § 14.) 

Examples. -^ (x-*) «^ (^^ j = -^^ =^, = -A:x-»-i. 

Note that fonnula IV holds also when n is a negative 
integer, for if n = — fc, formula IV gives the result we have 
just proved. 

EXERCISES 

Calculate the derivative of each of the following functions. 

1. y-iz^. e. i,-2x-»(=J). 

«• V-J+l- 8- *-— p 

A _ 3a!-4 - t« 

" x^ + % t^—1 

3 

6. y = -3 . 10. « = ^« - ktr^ 



30 THE CALCULUS [III, § 17 

11 2 ^* + l 01 2 2/ + 1 

11. t; = 1*2 5— ^« 21. X = f . 



t*2-l •*• •*' 2/3-1 y24.2,4_i- 

M ^2 r2/7 

13. t; = !^^jj2 23. 8 = («-»4-4)(«-«-5). 

14. 5 = ar^ + 6f-«. (M)r-a + &-5-(w + ^)- 

16. t. = -^. 2g-^° .;>^ '^'u'^a-M 

os^ ^ c (6w — an) (av + o) 

i.r 2,3 ^,- 2 ox + 6 

17. t^ = -5 + ir-rT- 27. 2/ = 



2S-r^2^.i- -• y 2 a2(ax 4-6)2* 

18. r.^(.2 + ;).(l-^). @^, = (^3 + 3'x4-l)^ - 

r2 — r + 1 3(2/ — 1)' 

20. .=4±l^^. 30..= ^^ 



2/2-22/4-6 (5-7a:5)2 

31. Compare the slopes of the family of curves y = a;», where n = 0, 
4- 1, 4- 2, etc., — 1,-2, etc., at the common point (1, 1). What is the 
angle between y = x^ and 2/ = aJ-i? See Tables ^ III, A, 

18. Derivative of a Product. The following rule is often 
useful in simplifying differentiations: 

The derivative of the product of two functions is equal to the 
first factor times the derivative of the second plus the second 
faxAor times the derivative of the first: 

rtm d(U ' V) dV . dU 

If y=u ' v where u and v are functions of x, a change Ax in 
X produces changes Ai/, Aw, Av in i/, w, and t;, respectively: 



Ill, § 191 ALGEBRAIC FUNCTIONS 31 

(A) y+Ay= (u + Au) (v + Av); 

(B) Ay= (u + Au) (v + Av) —u • v = uAv'\-vAu + AuAv\ 

Av 

(C) Ay /Ax = u{Av/Ax) + v{Au/Ax) + Au— ; 

(D) dy/dz = lim {Ay /Ax) = u{dv/dx) + v{du/dx). 

Example 1. To find the derivative of y = (x^ + 3)(x8 -f- 4). 
Meifwd 1. We may perform the indicated multiplication and write: 

^=^[(a;2+3)(a;3 + 4)] = —[0:5 + 3x8 + 4x2 + 12] =5x4 + 9a;2-f-8a:. 
dx dx ax 

Method 2. Using the new rule, we write: 

g-(x2 + 3)^(x8 + 4) + (x3 + 4)^(x2 + 3) 

= (x^ + 3)S x'^ + (x^ + 4)2 X -= 5 x^ + 9 x^ -{- S X. 

In other examples which we shall soon meet, the saving in labor due 
to the new rule is even greater than in this example. 

19. The Derivative of a Function of a Function. Another 
convenient rule is the following: 

The derivative of a function of a variable u, which itself is a 
function of another variable x, is found by multiplying the deriva- 
tive of the original function with respect to u by the derivative of 
u with respect to x. 

[vn] 3^ = 5^ •$^' 

dx du dx 

If 2/ is a function of w, and w is a function of x, a change Ax 
in x produces a change Au m u\ that in turn produces a 
change Ay my] hence: 

Ay _ Ay Alt 
Ax Au Ax 

Taking limits on both sides, we have formula [VII]. 



'32 • THE CALCULUS [III, § 19 

Example 1. To find the derivative of y = {x^ + 2)3. 
Method 1. We may expand the cube and write: 

^"S'^^^"*"^^^' =^(x« + 6a;4+12a;2+8) = 6a;5 + 24x8 + 24a;. 

Method 2. Using the new rule, we may simplify this work: let 
w = a;2 + 2, then y = {x^-\- 2)' = u^) rule [VI] gives 

dy^dydu^ d(v^ d(x^ + 2) ^ ^ ^j . 
dx du dx du dx 

= 3(x2 + 2)2 -(2 0;)= 3(a:4 _(_ 4 a;2 4. 4) . (2a;) = 6x5 + 24 x' + 24x. 

20. Parameter Forms. If x and y are given as functions 
of a third variable t, in the form 

the variable t is called a parameter , and the two given 
equations are called parameter equations. Elimination of t 
between these equations would give an equation connecting 
X and y, from which dy/dx might be found. But it is often 
desirable to find dy/dx without elimination of t. Since 

Ax "" !"« • M 
we have, in the limit as Ax approaches zero. 

This formula is essentially the same as the result of § 8, p. 11. 
If we replace thy y m [VII a], we obtain the following 
important special case: 

[VIIW *? = 1 ^ ^. 

^ ^ dx ^ ' dy 

Example, liy ^t^-\-2 and x = 3 < + 4, to find dy/dx. 
Method 1. We may solve the equation a; = 3 < + 4 for t and sub- 
stitute this value of t in the first equation: 

/x - 4\2 , ^ a:2 8 , 34 



Ill, § 20] 



ALGEBRAIC FUNCTIONS 



33 



dy 2 



^-2. 8__2« 
^ = ^(3^ + 4)-^=-^ 



Method 2. Using the new rule (with letters as used in §8, p. 11), 
we write: 

dy dy . dx _ d(fi + 2) . d&t + 4) ^. . o_2, 
dx~ dt ' dt ^ dt " dt -^« • ^-3'. 



1. y 

2. y 
8. y 
4. y 



EXERCISES 
2a;(a;2-l). 15. s 

xHa^ + 3). 16. li 

(2a: -3) (a: + 3). 17. m 

(l+a:) (l-a;.H-a:2). 18. m 



5. y = (4-aj2)(l+ir3). 



19. 2/ = 



= («»-/- 4)«. 
= (7-5t; + 2t;8)*. 
= (t;*+3t;2--2)*. 

= (a + &v + ct;^)®. 
1 



6. 2/ = (2 a; - a;2) (2 - 3 aj - x^). 20. 2/ = 



7. y = (a;2 - 1)». 



8. y = (2 a;2 + 3)2. 



21. y = 



22. 2/ 



9. 2/ = (a;»-2)«. 23. r 

10. y = (x« + 2)8. (fi) r 

11. y = {3x^ + 5)*. 25. m 

12. y = (5a;8-7)5. 26. u 

13. 8 =(l+2«-3«2)2. (27) « 

14. « = (<2 + 3 « + 7)8. 28. 8 
Determine dy/dx in each of the following 

6r-42« 



31. 



I" 



(«8 + l)2* 

1 

(<2 + ^ + l)t' 

a;« + 3 
(a:2 + 2)8' 

_ (2 x2 - 5)8 

(x8 + 3)* ' 

= (2s«-3)-«. 

= (l-«2 4.«4)-8. 

= («^ + 2)8(3t;-5)2 
= (^ _ 2)2 (2v- 1)8. 
= «(<* + 3) (<8 4. 4). 

= (l-0(l~5«2)(3-4^), 

pairs of equations: 

2, = 6w2-7i*- 1, 
li = x2 - 1/2. 

1-s 



{ 



5z2 
« = 2 — 4 X. 



y = 



2 = 



z 
1-x 

1+x* 



34 THE CALCULUS [III, § 20 



Draw each of the curves represented by the following pairs of 
parameter equations and determine dy/dx. 

as l^ = ^'» 34 [^ = 2< + 3/2, 

^' U = 3< + 2. ^- U = 2« + 4. 

What is the slope in each case when < = 1? Show this in your graphs. 
Find the value of the slope in each case at a point where th3 param- 
eter has the value 2. 

35. Draw the graph of the function y — (2 a: — 1)2(3 a; + 4)2. 
Determine its horizontal tangents. 

36. Proceed as in Ex. 35, for the function 

2/ = (2 a; - 1)2 -h (3 a; + 4)2. 

21. Differentiation of Irrational Functions. In order to 
differentiate irrational expressions, we proceed to prove that 
the formula for the derivative of a power (Rule [IV]) holds 
true for all fractional powers: 

[IVa] g = nx''-i, n=±^, 

where n is any positive or negative integer or fraction. 

The formula has been proved in § 17 for the case when n 
is a negative integer. Suppose next that 

(1) y = x^/^ 

where p and q are any positive or negative integers. If we 

set 

(2) X = ^, y = tP, 

which together are equivalent to i/ = ojp/*, and apply formula 

[Vila], we find: 

but since t = x^'^, substitution for t gives 

dx q q 

This proves [IV] for all fractional values of n. 



Ill, § 22] ALGEBRAIC FUNCTIONS 35 

The rule also holds when n is incommensurable; for 

example, given y = x^^y it is true that dy/dx = V2x ^^; 
we shall postpone the proof of this until § 85, p. 85. 

22. Collection of Formulas. Any formula may be combined 
with [VII], for in any example, any convenient part may be 
denoted by a new letter, as in § 20. For example. Rule [IV] 
may be written 

dw" du^ du u rTrxTi n-i du i rTTri 

^=d^-di'^yt^^J' =n«-.-,by[IV]. 
The formulas we have proved are collected below: 

m % - 0. 

inj **<' • "> - e . *!. 

dx dx 

[III] . ^ W'^d" ^^^^^ ^^^ subtraction also. 

[IV] ^ = nii"-i^. 
^ ^ dx dx 

./N\ dN dD j<^ ^W 

dx dy 

These formulas enable us to differentiate any simple alge- 
braic function. 



36 THE CALCULUS [III, § 23 

23. Illustrative Examples of Irrational Functions. In this 
article the preceding formulas are applied to examples. 

Example 1. -i — = — ^ — = ^x^/^-^ = -x~^/^ = 



dx dx 2 2 2Vx* 

(See Ex. 4, p. 21.) 

Example 2. Given y = Vs x^ + 4, to find dy/dx. 

Method 1. Set w = 3 a;2 + 4, then y * Vw ; by Rule [VII], 

dy _dy du _ 1 _ 6a; ^ 3 a; V3 o;^ + 4 

dx du' dx 2 Vw 2V3a;2^4 3 x^ -f- 4 

Method 2. Square both sides, and take the derivative of each side of 
the resulting equation with respect to x: 

d{y^) _ rf(3 x^ + 4) _ ^ ^^ 
dx dx 

But by Rule [IV], 

<^ W _ d{y^) ^dy _^ dy 
dx dy dx dx* 

hence, 

^ dy ^ dy Zx Sx 3 .t V3 x^ + 4 

dx dx y \/3 x^ + 4 3 x^ + 4 

This method, which is excellent when it can be applied, can be used to 
give a third proof of the Rule [IV] for fractional powers. The next 
example is one in which this method cannot be applied directly. 

Example 3. Given 2/ == x^ — 2 V3 x^ + 4, to find dy/dx. 



dx dx dx 3 x^ 4- 4 

Example 4. Given y = (x^ — 2)V3x2 + 4, to find dy/dx, 
J = V3x2 + 4£ (x3- 2) + (x3-2)£(V3x2 + 4) [by Rule VI] 

= V3^H:^.3x2+(x3-2)?^^^^ [byExample2] 

12x^-t-12x2-6x 
3x^ + 4 



= V3x« + 4 [3 x* + (a:^ - 2) . ^^^1 = \/3F+4 



Ill, § 23] ALGEBRAIC FUNCTIONS 37 



y/x 4-1 — v^x 
Example 6. Given y = . rr, to find dy/dx, 

V x -f 1 -f V a: 
First reduce 2/ to its simplest form: 

= "^x-\-l — Vx ^ y/x + l — y/x ^ 2x + l-'2Vx^-{'X 
^ " V^T^ + Vi VT+l-Vi (x + l)-x 

= 2 X + 1 - 2 Va^ + x. 
Then 

wherein = x^ + a?; hence 

f?=2-24.f^=2-— L=(2x + 1). 
cte 2ViiCto Vx^ + x 

This example may be done also by first appl3dng the rule for the 
derivative of a fraction [Rule V] ; but the work is usually simpler, as in 
this example, if the given expression is first simplified. 

EXERCISES 

Calculate the derivatives of 
1. 2/ = x*/». 3. « = 2 -Jx2. 5. 1/ = Vx Vx. 

« 6 10x» f^^ , 

(gp « = VS < - 4. 

15. V = 1/ V2 -f- 3 1*. 

17. « = Vf2 __ 3 ^. 
2 xVx8 . 3--. /^-v _ _ 5 + 3« 



'. J/ 


^ X — = ~" =r • 

Vx* Vx*» 


(5> " 


6 2 


9. 8 


= «»(2 (2/8 4- 3^-2/3). 


®? V 


= 2 ■^'SCxVs + xB/8). 



13. 2^ = V2+3x. "^0, y= \2x» + 4x. 



38 THE CALCULUS [III, § 23 

21. y « xWz x-4. 27. y = ^^^ "" 






22. 2/ = (5 + 3a;)V6a;-4. 28. y = (9 - 6 a: + 5 a;2) ^^^Tf^. 

23. t; = Vl-x + xK 29. s = (1 + ^2) vT^T^. 



(First rationalize the denominator.) 



25. y = Vl + Va; • 31. 2/ = 



26. 8 



vT+x2- 

- V iZTfi' 32. 2/ = 



X 



Draw the graphs of the equations below, and determine the tan- 
gent at the point mentioned in each case. 

33. 2/ = Vn^, (x = f). 36. y = V(l + x) (2 + 3 a;), (a; = 2). 

34. 2/ = VTT^, (a; = t). 37. y = xVTTx, {x = 1). 
36. y = Vx, (x = 2). 38. 2/ = xi/2 - a;i/3,(x = 1). 

39. Find the angle between the curves y = x^^^ and y = ar3/2 at (1, 1). 

40. Find the angle between the curves y = x^^^ and y = x^^^ at (1, 1). 

41. In compressing air, if no heat escapes, the pressure and volume 
of the gas are connected by the relation pv^'*^ = const. Find the rate of 
change of the pressure with respect to the volume, dp/dv. 

42. In compressing air, if the temperature of the air is constant, the 
pressure and the volume are connected by the relation pv = const. 
Find dp/dv J and compare this result with that of Ex. 41. 



CHAPTER IV 

IMPLICIT FUNCTIONS — DIFFERENTIALS 

24. Equations in Unsolved Form. An equation in two vari- 
ables X and y is often given in unsolved form; i.e. neither 
variable is expressed directly in terms of the other. Thus 

(1) , a:* + j/^ = l 

represents a circle of unit radius about the origin. 

Such an equation often can be solved for one variable in 
terms of the other; thus (1) gives 

(2) y = Vl-a^, or 2/ = - Vl - xK 

The first solution represents the upper half of the circle, the 
second the lower half. Now we can find dy/dx as in § 23: 

(3) ^^ -^ ,nr^y- +^ 



2 



dx Vl — x^ d^ Vl — X 

where the first holds true on the upper half, the second on 
the lower half, of the circle. 

By Rule [VII] such a derivative may be found directly 
without solving the equation. From (1) 

ax ax 

hence 

(4) 2x + 2y^ = 0, 

39 



40 THE CALCULUS [IV, § 24 

or 

(5) ^=-5. 

dx y 

This result agrees with (3), since y = =^ Vl — x^. 

This method is the same as that used in the second solution 
of Ex. 2, p. 36. It may be used whenever the given 
equation really has any solution, without actually getting 
that solution. 

Such a formula as (4) is much more convenient than (3), 
since it is more compact, and is stated in one formula instead 
of in two. But the student must never use (5) for values of x 
and y without substituting those values in (1) to make sure 
that the point (x, y) actually lies on the curve; and he must 
never use (5) when (5) does not give a definite value for 
dy/dx* Thus it would be very unwise to use (4) at the 
point x= 1, i/=2, for that point does not lie on the curve (1) ; 
it would be equally unwise to try to substitute x = 1, y = 0, 
since that would lead to a division by zero, which is impos- 
sible. 

26. Explicit and Implicit Functions. If one variable y is 
expressed directly in terms of another variable x, we say 
that y is an explicit function of x. 

If, as in § 24, the two variables are related to each other by 
means of an equation which is not solved explicitly for y, then 
y is called an implicit function of x. Thus, (1) in § 24 gives 
y as an implicit function of x; but either part of (2) gives y as 
an explicit function of x. 

Definition. If the original equation is a simple polynomial 

♦ These, precautions, which are quite easy to remember, are really suffi- 
cient to avoid all errors for all curves mentioned in this book, at least pro- 
vided the equation like (4) [not (5)] is used in its original form, before any 
cancelation has been performed. 



IV, §25] IMPLICIT FUNCTIONS — DIFFERENTIALS 41 

in X and y equated to zero, any explicit function of x obtained 
by solving it for y is called an algebraic function. See § 15. 

Example, x^ +y^ — Sxy = 0. (Folium of Descartes: Tables, III, 

/6.) 

This equation is diflScult to solve directly for y. Hence, as in § 24, 
we find dy/dx by Rule [VII] ; differentiating both sides with respect to 
X, we find: 

3^+3y«g-3y-3^g=0; 

dy' y — x^ 

wnence -r- ~ ~o • 

dx y^ — X 

At the point (2/3, 4/3), for example, dy/dx =4/5; hence the equation 
of the tangent at (2/3, 4/3) is {y - 4/3) = (4/5) (x - 2/3) or 4 a; - 
5 1/ + 4 = 0. Verify the fact that the point (2/3, 4/3) really lies on 
the curve. Note that this formula is useless at the point (0, 0) 
although that point lies on the curve. 

EXERCISES 

In each of these exercises the student should take some point on the 
curve, and find the equation of the tangent there. 

1. From the equation x^y = 1 find dy/dx by the two methods of 
§ 24, first solving for y, then ,v^ithout solving for y. Write the result in 
terms of x and y; and also in terms of x alone, when possible. 

Find dy/dx in the following examples by the two methods of § 24. 
2, s^y^lQ, 7. x8 -|_ y3 = o«. 

Z. x^ — xy ^ 5, 8. X* — 4 y2 = 4. 

4. 2xy +x + y =^0, 9. 3^+y^ — 3x=^0, 

5. x2 _ 4 2,2 = 36. 10. (x + y)2 - 2 X = 4. 

6. x^-y^^l. 11. xy^ -x^+y^=0. 

Find dy/dx in the following examples without solving for y: check 
the answers when possible by the other method of § 24. 

12. x'^+2xy + y^=2, 16. ax^ + 2 hxy + hy^ =- k. 

13. x^y^-Sxy + 7 = 0, 16. y*-2yH +x^ ==0, 

14. ax2 +2bxy+cy^+2dx + 2ey+f = 0, 

17. >/?+ V^ = Va. 18. ^3/2 _(. y3/2 == ^8/2. 



42 



THE CALCULUS 



[IV, § 25 



In the following pairs of parameter equations, find dyldx by § 20 : 
when possible eliminate i to find the ordinary equation, and show that 
the derivative found is correct. Regarding each pair of equations as 
defining the position of a point (x, y) at the time t, find the horizontal 
speed and the vertical speed at the time t, (See § 8.) Find also the 
total speed from the relation 



totoZ %'peQd == V (horizontal speed)^ -f- (vertical speed)^. 



19. 



a; = 4 <, 
, y = 8 <2. 



20. I^^^f/o' 21. j^ = 

U=4«-2. \y = 



= 3^ + 1, 
2^3. 



22. 



X = 



y = 



3t 



1 +t^' 



23. 



z = 



y = 



t^ + V 

-2t 

«2 + l* 



24. 






y = 



2t 



«2-l 



26. On a circle of unit radius about the origin dyldx — —x/y\ this is 
positive when x and y have different signs, negative when a; and y have 
the same sign. Show that this agrees with the fact that the circle rises 
in the second and fourth quadrants and falls in the first and third quad- 
rants as x increases. 

26. Show that the curve xy = 1 is falling at all its points. 

27. Show that the curve xh^ = 1 is rising in the second quadrant and 
falling in the first quadrant. 

28. The equation xV2 -f- y^/^ = 1 is the equivalent of the equation 
^.2 — 2 X2/ -t- y^ —2x — 2 2/4-1 = 0, if the radicals x^/^ and y^/^ be taken 
with both signs. Show that the values of dy/dx calculated from the two 
equations agree. By methods of analytic geometry, it is easy to see that 
the curve is a parabola whose axis is the line y ^ x, with its vertex at 
(1/4, 1/4). 

29. The curve of Ex. 28 is also represented by the parameter equa- 
tions 4 a; = (1 + 1)^, 4 2/ = (1 — t)^. Test this fact by substitution, 
and show that the value of dy/dx obtained from these equations agrees 
with the value obtained in Ex. 28. [The curve is most easily drawn 
from the parameter equations.] 

If t denotes the time in seconds since a particle moving on this curve 
passed the point (1/4, 1/4), find the total speed of the particle at any 
time. 



IV, §26] IMPLICIT FUNCTIONS — DIFFERENTIALS 43 




26. Differentials. Let the curve PQ (Fig. 8) be a part of 
the graph of the equation y =f(x). Let P be any point 
(x, y) on the curve, and let Q be a second point (x + Ax, 
y + Ay) on it. The change Ax = PM in x causes a change 
Ay = MQ in y. 

The slope of the tangent 
PT at the point P is given 
by the formula 

(1) m = tan a 

Ax-»oAx dx 

If this slope were main- 
tained over the interval 
Ax, the change produced in y would be 

(2) MK = m • Ax. 

When Ax is small, the change in y, MQ, will usually be 
nearly equal to MK. In many problems, it is a sufficiently 
exact approximation to Ay. Moreover, its value may be 
found readily by (2), whereas the actual calculation of Ay 
itself might be tedious or impracticable. 

This quantity MK, which is an approximation to Ay, is 
called the differential of y, and is denoted by the symbol dy. 
Hence we may write 

(3) dy 



m 



Ax = |.Ax. 



In particular, if the curve is the straight line y = x, we find 
m = 1; hence the differential of x is 

(4) c/x = 1 • Ax. 
If we divide (3) by (4) we find 

(5) dy -r- dx = m, 

where dy -r- dx now denotes a real division, since dy and dx 



44 THE CALCULUS [IV, § 26 

are actual quantities defined by the equations (3) and (4), 
and dx (= Ax) is not zero. 

Since m stands for the derivative of y with respect to x, it 
follows that that derivative is equal to the quotient of dy by 
dx, 

(6) g=di,^dx;^ 

this fact is the reason for our use of the symbol dy/dx to repre- 
sent a derivative originally. 
In the figure all quantities here mentioned are shown: 

cto = Aa; = AB, dy = MK, Ay = MQ,^ =. tan /3,^ = tan a. 

Ax dx 

The quantities dx(= Ax) ,dy(= mAx) , Ay, Ay — dy{= KQ) , are 
infinitesimal when Ax approaches zero, i.e, they approach 
zero as Ax approaches zero. 

27. Diflferential Formulas. For any given function y = f{x), 
dy can he computed in terms of dx(= Ax), by computing the 
derivative and multiplying it by dx. 

Every formula for diflferentiation can therefore be written 
as a differential formula; the first six in the list in § 22, p. 35, 
become after multiplication hy dx: 

[I] dc = 0. (The diflferential of a constant is zero.) 

[II] d{c -u) = c ' du. 

[III] d(u + v)-=du + dv. 

[IV] d (W) = nw^^du. 

[VI] d{U'V) = udv + vdu. 



IV, §271 IMPLICIT FUNCTIONS — DIFFERENTIALS 45 



Rules [VII], [Vila], and [VII6], of § 22, p. 35, appear as 
identities, since the derivatives may actually be used as 
quotients of the diflferentials. From the point of view of 
the differential notation Rule [VII] merely shows that we 
may use algebraic cancelation in products or quotients 
which contain differentials. 

Rules [I]-[VI] are sufficient to express all differentials of 
simple algebraic functions. A great advantage occurs in the 
case of equations not in explicit form, since all applications of 
Rule [VII] reduce to algebraic cancelation of differentials. 

Example 1. Given y = x^ __ 12 x + 7, to find dy and m. 
dy==d(xi-12x + 7) = d(2^) - d{l2x) +d(7) =3x^dx-12dXy 
whence m = dy-^dx = Sx^ — 12 aain Example 2, p. 21. 

a;2-f-3 



Example 2. Given y = 



3x-7 



, to find dy (Example 1, p. 29). 



(3x-7)d(x2 + 3)~(x2 + 3)d(3a;-7) 

^^ = (3x-7)2 : 

_ 3x2-14a;-9 ^ 
" (3x-7)2 ^' 

Example 3. Given y = (x^ + 2)3, to find dy (Example 1, p. 32). 

dy =d[(x2+2)3] =3(a;2+2)2d(a;2+2) 
= 3(x2+ 2)2.2 x-dx. 

Example 4. Given y — x^ — 2Vs x^ + 4, to find dy (Example 3 



p. 36). 



dy =d{3^)-2dVSx^+4: 

1 



= 3a;2da;-2 



2 V3 x2 + 4 

= ^"3x2 — L= 6 x) dx. 

V Va a:2 ^_ 4 / 



d (3x2 + 4) 



V3 x2 + 4 

Example 5. Given x^ + y^ = 1, to find dy in terms of dx (§ 24, p. 39). 
dix^+y^) =d(l) = 0; but d (x2 + 2^2) = d (x2) + d (j^2) 
= 2xdx + 2ydy; 
hence 2 x dx + 2 y dy = 0, or dy = — (x/y) dx, or m = dy/dx = — x/y. 



46 THE CALCULUS [IV, § 27 

Example 6. To Qnddy and m when a^ -{-y^ — Sxy =0. (Example, 
p. 41.) d (x3) + d (2/3) - 3 d (x2/) = 0, 

or 3x2 dx -{-3y^dy — Sxdy — 3y dx = 0, 

or (x2 —2/) dx + (2/^ — x) dy ^ 0, 

whence rfy = ^ dXyOrm = -f == ^ — - . 

2/2 — X dx y^ — X 

Example 7. To find dy in terms of dx when x = 3< + 4, y = ^ + 2. 
(Example, p. 32.) 

We find dx =^ d (S t + ^) = S dt; dy ^ d {fi + 2) = 2 t dt; 

hence w - dy -^ dx — (2/3) <, or d^ = (2/3) t dx; 

but since t — (x — 4)/3, this may be written: 

dy = (2/9) (X - 4)dx, or m = g = (2/9) (x - 4). 

EXERCISES 

[These exercises may be used for further drill in differentiation, and 
for reviews. It is scarcely advisable that all of them should be solved 
on first reading.] 

Calculate the differentials of the following expressions. 

1. y =^ax^ + bx+c. 15. u = l/V2v-\-v^. 

2. 2/ = (o2 + x2)2. 16. w = (1 - 2 t;2)/(2 - v^). 

3. 2/ = (ax^+bx+c)^, 17. u = '^^^\"^^ - 
4., = (a -6x2)5. 18. . = J^2^. 

3 



5. y=^l/(ax + b), 19. z = 1/V(2 ~ 2/3)4. 

6. y = l/(ax + 6)2. 20. s = l/\/(2/ - a)^. 

7. s = (1 + 2 /) (1 - 3 0. 21. 2 = 2//VT+7. 

8. s = (2 - 3 0M3 + 2 <2). 22. « = Va + by/y. 

9. s = <2 (o - ^)3. 23. r = {a + b^)P. 

10. s = «4 (3 - 2 «3)2 24. r = v^a -f 6s«. 

11. s = V3 t - t\ 25. r = l/(a + 6s'»)p. 

12. 8 = V<"4^n". 26. r = \/\/a + 6s». 

1 + Vx 



13. s = V(<3 - 3 0^ 27. 2/ = 



V: 



X 



14. 5 = v^(2<2 + l)2. 28. 2/ = |/^ 



bx 
bx 



IV, § 27] IMPLICIT FUNCTIONS — DIFFERENTIALS 47 



29. 


xy y -4.. 


30. 


x2- 2x2/- 32/2 = 0. 


31. 


x2-y2-^- 



Determine dy in terms of dx from the equations below. 

33. (1 - ax) (a;2 + y^) = 4. 

34. x2 + y2 = (ax + 6)2. 

* x2 a — hx 
32. 2/4 _ 2 2/2x - 1 = 0. ^36. (x + 2/)^^^ + (a; - 2/)^/^ = o^/^. 

37. Obtain the equation of the tangent at (2, — 1) to the curve 
4x2-2a:2/-5 2/2-6x-42/-7 = 0. 

^8. Obtain the equation of the tangent at (2, 1) to the curve 
x^ - 7 x^ - 5y^ + ^ x^- 10 xy + Sx-5y-\- 18=^0. 

Obtain the equation of the tangent at (xq, yo) to each of the following 
curves: 

CuBVE Tangent 

39. y^ =4ax; yyo'=2a(x+ Xq), 

40. x^-\r y^ = a2; xxq + yyo = a2. 



41 ?'+?^' = l- 

*^- 02 - 62 ^' 



^±^0 = 1 



a' 



62 



Find the derivative dy/dx for the curves defined by each of the 
pairs of parameter equations given below. 

S a — 2t 

at ' 
_4(a-t)^ 



42.^ 



X — 



-^6. 



y = 



x = 



2t 

1+^' 
1-t 

1-ht' 



43. 4 



a; = I V2 «3, 



44. 



X = 



e 



1 +0' 

[2/ = 0-1 + 0-2. 



46. 



X = 4 irr2, 
2/ =girr3. 



47. 



y = 



u- 



2/ = 



02^2 



4irr2» 

3 
4ir7^ 



48. Calculate the x and y components of the speed (% and Vy) at any 
time tf and the resultant speed "^Vx^ + /^^ for the motion 

2< _ l-/2 

49. If a particle moves so that its coordinates in terms of time are 

x = l-t + t\ 2/ = l+« + ^, 
show that its path is a parabola. Show that from the moment < = its 
speed steadily increases. 



48 THE CALCULUS [IV, § 27 

60. The electrical resistance of a platinum wire varies with the tem- 
perature, according to the equation 

calculate dRm terms of dd. What is the meaning of dR/dd? 

61. Van der Waal's equation giving the relation between the 
pressure and volume of a gas at constant temperature is 



(p+^) (P-^) =c. 



Draw the graph when a = .0087, 6 = .0023, c = 1.1. Express dv in 
terms of dp. What is the meaning of dv/dp? 

62. The crushing strength of a hollow cast iron column of length I, 
inner diameter d, and outer diameter D, is 

T = 46.65 (^:?i^) 

Calculate the rate of change qt T with respect to £>, d, and I, when 
each of these alone varies. 



CHAPTER V 



TANGENTS — EXTREMES 

28. Tangents and Normals. We have seen in § 4, p. 4, that 
if the equation of a curve C is given in explicit form: 

(1) y=f{x), 

the derivative at any point P on C represents the rate of rise, 
or slope, of C a.t P: 

(2) L^Jai p= t^^P^ ^f ^at p = ^^^P^ ^fP"^ = tow a = mp, 

where a is the angle XHT, counted from the positive direc- 
tion of the X-axis to the tangent PT, and where nip denotes 
the slope of C at P. 

Hence (§4, p. 5) the equation of 
the tangent is 

(3) iy-yp) = \_fX{x-xp), 

where the subscript P indicates that 
the quantity affected is taken with 
the value which it has at P, 

If the slope rrip is podtive, the curve is rising Sbt P; if mp is 
negative, the curve is falling; if nip is zero, the tangent is hori- 
zontal (§ 6, p. 6). Points where the slope has any desired 
value can be found by setting the derivative equal to the 
given number, and solving the resulting equation for x. 

Since, by analytic geometry, the slope n of the normal PN 
is the negative reciprocal of the slope of the tangent, we have, 

(4) np = slope of PN = = — fj-rrr' 

mp [ay/dx]p 

49 



r 


\ 










y 


\ / 


^T 






J^ 




« 


,^ 


:^ 


\ 


X 





/fl- 


A 


\N\ 





Fig. 9. 



50 THE CALCULUS [V, § 28 

hence the equation of the normal is: 

(5) ^y-y'^'-g^^^ -=""'>• 

29. Tangents and Normals for Curves not in Explicit Form. 
The equation of the curve may be given in the implicit 
form 

(1) F (x, y) = 0, 

as in §§24-25, pp. 39-41; or the equations in parameter 
form may be given: 

(2) x=f(t),y = <l>(t), 

as in § 20, p. 32. In either of these cases, dy/dx can be 
found, and this value may be used in the formulas of § 28. 
No new formulas are necessary. 

30. Secondary Quantities. In Fig. 9, § 28, since 

tan a (= nip = [dy/dx]p)f and AP (= i/p), 

are supposed to be known, the right triangles HAP and PAN 
can both be solved by trigonometry, and the lengths HA, 
AN, HP, PN can be found in terms of mp and ypi 

[Subtangent]p = HA = AP -r- tan a = yp-i- mp = [y/m]p. 
[Subnormal] p = AN = AP • tan a = [t/ • m]p, since a = Z APN, 

[Length of tangent]p = HP = '^Ap + W^ 

= ^y% + \ylm\\ = \y Vl + {Mmf\p. 



[Length of normaljp = PAT = ^ AP" + AN" 

= ^^yp+iymyp = [yVl + m^]p. 

It is usual to give these lengths the names indicated above; 
and to calculate the numerical magnitudes without regard to 
sigijs, unless the contrary is explicitly stated. 



V, 1 31] TANGENTS — EXTREMES 51 

31. Illustrative Examples. In this article, a few typical 
examples are solved. 

Example 1. Given the curve y = x^— 12x-\-7 (Ex. 2, p. 21), we 
have m = dy/dz = 3 a;^ — 12. 

(1) The tangent (T) and the normal (iV) at a point where x = a are 

(T)y- (a3-12o + 7) = (3 a2 - 12) (x - a), 

(iNr)2/-(a3-12a + 7)=j^^^(x-a); 

thus, at X = 3, the tangent and normal are 

(T) 2/ + 2 = 15(x-3), (N) 2/ + 2 = -A(a:-3). 

(2) The tangent has a given slope A; at points where 

3x2 - 12 = A;, i^e. x = ± ^ ^^^ ; 

there are always two points where the slope is the same, if A; > — 12; 
thus if A; = 0, a; = ± 2; if A; = - 9, x = ± 1; if A; = - 12, x = 0; if 
A; < — 12, no real value for x exists (see Fig. 15, p. 68). 

(3) The secondary quantities of § 30 may be calculated without 
using the formulas of § 30. Thus, at the point where x = 3, the 
tangent (T) cuts the x-axis where x = 47/15; the normal (iV) cuts the 
X-axis where x = — 27. If the student will draw a figure showing 
these points and lines, he will observe directly that t he subtange nt is 
2/15, the subnormal 30 , the len gth of the tangent V22 + (2/15)2, the 
length of the normal V302 + 22. These values agree with those given 
by §30. 

Example 2. Given the circle x2 + y2 = 1^ we have m = dy/dx = 
— x/y [see § 24]. 

(1) The tangent (T) and normal (N) at a point (xq, yo) are 

iT){y-yo)=-^{x-xo), (N) (y - yo) ^f {x- xo); 

yo *o 

or, since xo2 +yo^ ~ 1, 

(T) xxo + yyo = 1, i^) V^o = 2/oa;; 
thus, at the point (3/5, 4/5), which lies on the circle, we have 

(r) 3 X + 4 2/ = 5, (iV) 3 j^ = 4 X. 

(2) The tangent has a given slope A; at points where 

^ = A;, i.e. xq + kyo ~ 0. 

2/0 



52 THE CALCULUS [V, § 31 

The coordinates (xq, ^o) can be found by solving this equation simul- 
taneously with the equation of the circle, or by actually drawing the line 
xq + kyo = 0. Thus the points where the slope is -f 1 lie on the straight 
line X + y ^0; hence, solving x +j/ = and x^ -^y^ = 1, the co- 
ordinates are found to bea? = ± l/v^2, y — T 1/"^; but these points 
are most readily located in a figure by actually drawing the line 
x+y ^0. 

EXERCISES 

Find the equation of the tangent and that of the normal, and find 
the four quantities defined in § 30, for each of the ft^owing curves at 
the point indicated: 

1. y=xi-12x + 7; (1,-4). 6. x = j^«- 32/' + 5; (3,1). 

2- ^ = iSi^ (- ^^ ^)- «• {^ :(!;?}'• (^'^)- 

3. 9x^+2/2=25; (1,4). rx = <» + 4/-n 

4. xy + 2/2-2a;=5; (-4, 1). '* ly = ^ - 3 « + 5j ' ^' ^^• 

8. The curves of Exs. 1 and 3 pass through the point (1, — 4); 
at what angle do they cross? 

Determine the equation of the tangent and that of the normal to 
each of the following curves at any point (xo, 2/0) on it. 

9. j^ = kxK 13. 62a;2 ± a2y2 = ^262. 

10. y^ = 2px. 14. ax^-\-2bxy-{-cy^ =f. 

11. x2 + 2/2 = o2. 15. (m;2 + 2 6x2/ + C2/2 + 2 da; + 2 P2/ +/ = 0. 

12. y = kx^, 16. y = (ax-h h)/{cx + d). 

32. Extremes. In § 6, and in numerous examples, we have 
found points on a curve at which the tangent is horizontal, 
i,e, at which the slope is zero. If the slope of the curve 
y = f(x) is zero at the point where x = a, the curve may go 
through the point in any one of the ways illustrated in 
Fig. 10. 

In case (a),f(a) is called a maximum otf(x). 
In case (f)),f(a) is called a minimum oif(x). 



V, § 32] 



TANGENTS — EXTREMES 



53 



The value of f(x) at a point where x = a is a 4 . . I 

'' ^ '' ^ {minimum J 

value if it is i? ., l any other value of / (x) for values 

of X sufficiently near to x = a, 

A maximum or a minimum is called an extreme value, 
or an extreme oif(x). 

A value of x for which the slope m is zero is called a 
critical value. The corresponding point on the curve is 



y^^ 



yj^ 



^) 



fia) 



a 



X 



v^ 



(X) 



J(<t) 



a 



X 




(a) (6) (c) 

Fig. 10. 

called a critical point. At such a point, f(x) may be a 
maximum or a minimum, but it is not necessarily either. 
Thus, in cases (c) and (d), Fig. 10, the value of / (a) is neither 
a maximum nor a minimum of / (x) . 

On the other hand, extremes may also occur at points 
where the derivative has no meaning, or at points where the 
function becomes meaningless. 

Thus, the curve y = x^/s gives 
m = 2/(3 x^/^) : hence m is meaning- 
less when X = 0; in fact, the curve 
has a vertical tangent at that point. 
It is easy to see that this is, however, 
the lowest point on the curve. 

Again, if a duplicating apparatus costs $150, and if the running 
expenses are Ic. per sheet, the total costs of printing n sheets is / = 
150 + .01 n. This equation represents a straight line; geometrically 
there are no extreme values of t; but practically t is a. minimum when 
n = 0, since negative values of n are meaningless. Such cases are 
usually easy to observe. 




54 THE CALCULUS [V, § 33 

33. Fundamental Theorem. We proceed to show that a 
function / (x) cannot have an extreme except at a critical 
point; that is, assuming that/(a:) and its derivative have 
definite meanings at a: = a and everywhere near x = a^ no 
extreme can occur if the derivative is not zero atx = a. 

We are supposing that all our functions are continuous; 
if, then, the derivative m is positive at x = a, it cannot sud- 
denly become negative or zero. Hence m is positive on both 
sides of a: = a, and there can be no extreme there. 

Likewise if m is negative, the curve is falling near x = a 
on both sides of x = a; there can be no extreme. 

34. Final Tests. It is not certain that/ {x) has an extreme 
value at a critical point. To decide the matter, we proceed 
to determine whether the curve rises or falls to the left and to 
the right of the critical point: it rises if m > 0; it falls if 
m < 0. (See Fig. 10 in § 32.) 

Near a maximum, the curve rises on the left and falls on 
the right. 

Near a minimum, the curve falls on the left and rises on 
the right. 

If the curve rises on both sides, or falls on both sides, of the 
critical point, there is no extreme at that point. 

35. Illustrative Examples. 

Example 1. To find the extreme values of the function y ^J{x) = 
a;8 - 12 a; + 7. (See Ex. 3, p. 8.) 

{A) To find the Critical Values, Set the derivative equal to zero and 
solve for x\ 

w = ^ = 3 a;2 - 12; 3 a;2 - 12 = 0; X = 2 or a; = - 2. 
ax 

(B) Precautions, Notice that f(x) and its derivative each have a mean- 
ing for every value of x; hence a; = + 2 and x = — 2 are the only critical 
values. 



V,5 35] 



TANGENTS — EXTREMES 



(C) Final Tests, m - 3 1^* - 12 = 3 (i« - 
than 2, negative if x is slightly leas than 2; 
hence the curve rises on the right and fails 
ontheleftof3;-2, theretore/(2)=-9iBn 
TOiiumuQiof/(2). The student maj show 
that /(- 2) = 23 ia a maximum of f(x). 
(See Fig. 3, p. 8.) 

Example 2. To find the extremes of 
the fimction 

)/-/(i) =3H-12a^ + 50. 

(A) CTilical Values. Settiog dy/dx - 0, 
and solving, we find: 



^ = 12^- 



dx 



r*;12a^ 



-36a^ = 



= 0,01 



) iB positive if X 


s greater 








































A 






























t 






-- t 






. ^^ 




y- 


























t: 






1 






i 




i 






± 





FiQ. 12. 
1 the right, negative o 



(B) Precaviums. y and dy/dx have a 
meaning everj^vhere; the only critical 
values are and 3. 

<C) Fined Tests. Near i = 0, m - 
12i*(i — 3) is negative on both sides; 
hence there is no extreme there, though 
the tangent is horizontal. 

Near i = 3, m = 12 x'ix - 3) is positive o 
the left; hence /(3) = - 31 is a minimum. 

The information given above is of great assistance in accurate drawing. 
ElxAUPLE 3. Two raihiiad tracks cross at right angles; on one of 
them an eastbound train going 15 mi. per 
hour clears the crossing one minute before 
the engine of a southbound train running 
at 20 mi. per hour reaches the crossing. 
Find when the trains were closest together. 
Let X and y be the distance in miles of 
the rear end of the first train and the en- 
gine of the second one from the crossing, 
respectively, at a time t meaaured in min- 
utes beginning with the instant the first 



Fig. 13. 
train clears the crossing; then 

where D is the distance between the trains in miles. 



25, 



56 THE CALCULUS [V, § 35 

Since D is a positive quantity, it is a minimum whenever D^ is a mini-- 
mum; hence we write: 

_ d{D^) _ 2 , 25, _2,25. ^ .16 
"^^ dt " 9 "'"72^' 9 ■^72^"""' ^""25' 

when t <.16/25, m < 0; if /> 16/25, w> 0; hence D^ is diminishing 
before t = 16/25 and increasing afterwards. It follows that D is a 
minimum when t == 16/25. Substituting this value for <, we find the 
values X — 4/25, y = 3/25, D^ = 1/25; hence the minimum distance 
between the trains is 1/5 of a mile, and this occurs 16/25 of a minute 
after the first train clears the crossing. 

Example 4. To find the most economical shape for a pan with a 
square bottom and vertical sides, if it is to hold 4 cu. ft. 

Let X be the length of one side of the base, and let h be the height. 
Let V be the volume and A the total area. Then V = hx^ = 4, whence 
h = 4/a;2; and 

A =x2+4Aa;=a;2 + ^; 

X 

whence we find 

d A f^ 16. rt 16n«o o 

When a; < 2, m = 2(x^ — S)/x^ is negative; when x>2, m is positive; 
hence A is decreasing when x is increasing toward 2, and A is increasing 
as a; is increasing past 2; therefore x = 2 gives the minimum total area 
A = 12. Notice that the height is A=4/a;2=l. The correct 
dimensions are x = 2, A = 1 (in feet). 

EXERCISES 

Determine the maximum and minimum values of the following 
functions and draw the graphs, choosing suitable scales. 

1. j^ = a^ - 6 a;2 + 2. 2. s = 2 <3 - 6 ^ - 18 « + 15. 

3. p = g3 - 6 ^2 - 15 g. A. y = X!^ -{- 2 OX^ + G^X. 

6. x = 2/4 — 4 2/2 _f. 2. 6. t; = w4 - 4 w3 _j_ 4 ^2 _|. 3. 

7. m pn5-5w* + 5n8 + l. 8. A=^r8-6r4+4r3H-9r2-12r+4. 
9. s = (2^-l)(l-02. 10. V = h(h-1)K 

11. r=(s2-l)(a2-4). 12. a; = (2/ - 2)3 (2/ + 3)8. 

(a; + 2)2 ^. , a* 



V, § 35] TANGENTS — EXTREMES 57 



a;2-2a;+4 o/i^ + ft^ + c 

17. 2/ = ^!!^2 + r ^®- o = ^ + ^^r^- 

19. D = r VS^^. 20. 22 = ^^ + 6 - x. 

21. What is the largest rectangular area that can be inclosed by a line 
80 feet long? 

22. What must be the ratio of the sides of a right triangle to make its 
area a maximum, if the hypothenuse is constant? 

23. Determine two possible numbers whose product is a maximum 
if the sum of their squares is 98. Is there any minimum? 

24. Determine two numbers whose product is 100 and such that the 
sum of their squares is a minimum. Is there any maximum? Did you 
account for negative possible values of the two numbers? 

25. What are the most economical proportions for a cylindrical can? 
Is there any most extravagant type? Mention other considerations 
which affect the actual design of a tomato can. Is an ordinary flour 
barrel this shape? What considerations enter in making a barrel? 

26. What are the most economical proportions for a cylindrical pint 
cup? (1 pint = 28J cu. in.) Mention considerations of design. 

27. Determine the best proportions for a square tank with vertical 
sides, without a top. Is there any most extravagant shape? 

28. The strength of a rectangular beam varies as the product of the 
breadth by the square of the depth. What is the form of the strongest 
beam that can be cut from a given circular log? Mention some other 
practical considerations which affect actual sawing of timber. 

29. The stiffness of a rectangular beam varies as the product of the 
breadth by the cube of the depth. What are the dimensions of the 
stiffest beam that can be cut from a circular log? 

30. Is a beam of the commercial size 3" X 8*^ stronger (or stiffer) 
than the size 2* X 12*^ (1) when on edge, (2) when lying flat? 

[Conmiercial sizes of lumber are always a little short.] 

31. What line through the point (3, 4) will form the smallest triangle 
with the coordinate axes? Is there any other mininauin? maximum? 



58 THE CALCULUS [V, § 35 

32. Determine the shortest distance from the point (0, 3) to a point 
on the hyperbola x^ — y^ = 16. Show that it lies on the normal. 

[Hint. Use the square of the distance.] 

33. The distance D from the point (2, 0) to any point of the circle 
a;2 _j_ y2 — 1 ig given by the equation Z)^ = 5 — 4 a?. Discover the 
maximum and minimum values of Z)2, and show why the rule fails. 

34. Show that the maximum and minimum on the cubic y = x^ — ax 
-j- h are at equal distances from the y-axis. Compute y at these points. 

36. Show that the cubic x^ — ax -^b = has fhree real roots if the 
extreme values of the left-hand side (Ex. 34) have different signs. 
Express this condition algebraically by an inequality which states that 
the product of the two extreme values is negative. 

[Any cubic can be reduced to this form by the substitution x = a?' -j- A;; 
hence this test may be applied to any cubic] 

36. Show that if the equation x^ — ax -{-b = has two real roots, the 
derivative of the left-hand side (i.e. S x^ — a) must vanish somewhere 
between the two roots. Show that the convert is not true. 

37. The line y = mx passes through the origin for any value of m. 
The points (1, 2.4), (3, 7.6), (10, 25) do not lie on any one such line: 
the values of y found from the equation y = mx at a; = 1, 3, 10 are m, 
3 m, 10 w; the differences between these and the given values of y are 
(rn — 2.4), (3 m— 7.6), (10 m — 25). It is usual to assume that that 
line for which the sum of the squares of these differences 

S= (m- 2.4)2 -^ (Sm- 7.6)2 -f (lo m - 25)2 

is least is the best compromise. Show that this would give m = 2.50 
(nearly). Draw the figure. 

38. In an experiment on an iron rod the amount of stretching s (in 
thousandths of an inch) and the pull p (in hundreds of pounds) were 
found to be (p = 5, s = 4), (p = 10, s = 8), (p = 20, s = 17). Find 
the best compromise value for m in the equation s = m-p, under the 
assumption of Ex. 37. Ans. About 5/6.- 

39. A city's bids for laying cement sidewalks of uniform width and 
specifications are as follows: Job No. 1: length = 250 ft., cost, $110; 
Job No. 2: length, 600 ft., cost, $250; Job No. 3: 1500 ft., cost, $630. 
Find the price per foot for such walks, under the assumption of Ex. 37. 
How much does this differ from the arithmetic average of the price per 
foot in the three separate jobs? 



V, § 35] TANGENTS — EXTREMES 59 

40. The amount of water in a standpipe reaches 2000 gal. in 250 sec, 
5000 gal. in 610 sec. From this information (which may be slightly 
faulty). find the rate at which water was flowing into the tank, under 
assumption of Ex. 37. 

41. The values 1 in. = 2.5 cm., 1 ft. = 30.5 cm. are frequently 
quoted, but they do not agree precisely. The number of centimeters 
c, and the number of inches t, in a given length are surely connected by 
an equation of the form c = ki. Show that the assumptions of Ex. 37 
give k = 2.541. Is this the same as the average of the values in the 
two cases? Which result is more accurate? 

42. In experiments on the velocity of sound, it was found that sound 
travels 1 mi. in 5 sec, 3 mi. in 14.5 sec. These measurements do not 
agree precisely. Show that the compromise of Ex. 37 gives the velocity 
of sound 1088 ft. per second. How does this compare with the average 
of the two velocities found in the separate experiments? 

43. A quantity of water which at 0° C. occupies a volume vq, at 0° C. 
occupies a volume 

r = yo (1 - 10-4 X .5758^ + 10-6 X .756 6^ - 10-7 X .351 0^). 

Show that the volume is least (density greatest), at 4° C. (nearly). 

44. Determine the rectangle of greatest perimeter that can be in- 
scribed in a given circle. Is there any minimum? 

46. What is the largest rectangle that can be inscribed in an isosceles 
triangle? Is there any minimum? 

46. Find the area of the largest rectangle that can be inscribed in a 
segment of the parabola y^ = 4iax cut off by the line x == h. 

47. Determine the cylinder of greatest volume that can be inscribed 
in a given sphere. Is there also a minimum? 

48. Determine the cylinder of greatest convex surface that can be 
inscribed in a sphere. Is there a minimum? 

49. Determine the cylinder of greatest total surface (including the 
area of the bases) that can be inscribed in a given sphere. 

50. What is the volume of the largest cone that can be inscribed in a 
given sphere? 

61. What is the area of the maximum rectangle that can be inscribed 
in the ellipse x^/a^ -f- y^/b^ = 1? 



CHAPTER VI 
SUCCESSIVE DERIVATIVES 

36. Time-rates. In all the applications, derivatives are 
rates of increase (or decrease) of some quantity with respect 
to some other quantity which is taken as the standard of 
comparison, or independent variable. 

Among all rates, those which occur most frequently are 
time-rates, that is, rate of change of a quantity with respect 
to the time. 

37. Speed. Thus the speed of a moving bodv is the time- 
rate of increase of the distance it has traveled: 

(1) V = speed* = lim -r: = 37 , 

A<-^o A< at 

as in § 7, p. 9, and in numerous examples. 

38. Tangential Acceleration. The speed itself may change; 
the time-raie of change of speed is called the acceleration along 
the path, or the tangential acceleration^. 

A I? dv 

(2) Jt = tangential acceleration f = lim -r.= -y.' 

At— »o ^t at 

* The speed v is distinguished from the velocity t by the fact that the 
speed does not depend on the direction ; when we speak of velocity we shall 
always denote it by t (in black-faced type) and we shall specify the direc- 
tion. 

t The general acceleration J is also a directed quantity; when we speak 
of the acceleration J (not tangential acceleration jj,) we shall denote it by J, 
and give its direction. As in the case of speed, the letter j, in italic type, 
denotes the value of y without its direction. 

60 



VI, § 39] SUCCESSIVE DERIVATIVES 61 

Thus for a body falling from rest, if g represents the gravitational 
constant, 

hence 

da : 

and 

dv 

it follows that the tangential acceleration of a body falling from rest is 
constant; that constant is precisely the gravitational constant g.* 

In obtaining the tangential acceleration, we actually dififer- 
entiate the distance s twice, once to get v, and again to get 
dv/di or Jt, hence the tangential acceleration is also said to be 
the second derivative of the distance s passed over. 

39. Second Derivatives, Flexion. It often happens, as in 
§ 38, that we wish to differentiate a function twice. In any 
case, given y =f{x), the slope of the graph is 

ax Aa;-»0^ 

The slope itself may change (and it always does except on a 
straight line) ; the rate of change of the slope with respect to x 
will be called the flexion f of the curve: 

, n . dm ,. Am 

= flexion = -3- = lim -— » 

ax Aa;->0 AOJ 

and will be denoted by b, the initial letter of the word bend. 
Thus for y = x^jWe find m = 2x, 6 = 2;$ 

* The value of g is approximately 32.2 ft. per second per second = 981 
cm. per second per second. 

t The word curvature is used in a somewhat different sense. See § 86, 
p. 139. 

t The flexion for this parabola is constant; note that this means the 
rate of change of m per unit increase in x, not per unit increase in length 
along the curve. 



62 THE CALCULUS [VI, § 39 

for 2/ = x^, m = 3 x^, 6 = 6 x; 

for y = 3i^-l2x + 7, m = 3a^-12y 6 = 6a;; 

for any straight line y = fcx + c, m = fc, 6 ='0. 

The value of 6 is obtained by differentiating the given func- 
tion twice; the result is called a second derivative, and is 
represented by the symbol: 



cPy _ d^ /d^\ __ dm __ , 
dx^ dx \dx/ dx 



Likewise, the tangential acceleration in a motion is 

d^ _ d /ds\ _dv _ , 
de~dt\dt)''dt~^'^' 

If the relation between s and t is represented graphically, 
the speed is represented by the slope, the tangential acceleration 

m 

by the flexion, of the graph. Thus if s = gt^/2 be represented 
graphically, as in Fig. 4, p. 10, the slope of the (t, s) curve is 

m = slope — ~Jf — Q^ — speed = v, 

and the flexion of the (t, s) curve is 

, ^ . dm d!^s dv ^ ^-77^. 

b = flexion — ~17 — ~j^ — jf — 9"^ tangential acceleration =Jt' 

40. Speed and Acceleration. Parameter Forms. Let the 

equations 

x=f{t), y = 4>{t) 

represent the position of a moving point P in terms of time 
t as variable. Then, as in § 8, 

dx 

(1) ^x = -T. = horizontal component of the speed of P; 

dv 

(2) ^v= jf — vertical component of the speed of P; 



VI, S 401 SUCCESSIVE DERIVATIVES 



63 



(3) 



-wv. 



' + 0^ = total speed of P, 

in the direction tan-' (v^/vx). 
Further, 

<Px 

(4) jx= ;p- = horizontal acceleration of P; 

<Pv 

(5) jV = j2 = vertical acceleration of P; 

(6) j = Vj/ + j^ = total acceleration of P, 

in the direction tan-' (jg/jx). 

Note that the direction of v is aloi^ the tangent to the 
path of P, since v^/^ is equal to dy/dx, or m. But the total 
acceleration j m not, in general, in the direction of the path 
of P, since jy/j^ is ordinarily quite different from vjvx. 
Hence j and jV are usually different.* To get jr, calculate 
dv/dt from (3). 

Example. Let the parametric equations of the patb be 
a-=(*, !, = l/P(=(-s). 
To plot the path take a series of values 
of (: 



= 0, 


h 1, 3/2 


2, 




= o; 


h 1, 9/1 


4, 


■ ■; 


= OO 


4, 1, 4/9 


i- 




= 2 




Ji 


= 2, 


= - 


2H, 


jV 


=6H, 


-2v 


P+H. 


j 


=.2VH-9H. 


_dv 


2 i - 6 H 


(IIV), 1 22.) 




VJ+W >'■■"■"■' Fi«.14. 

• The reaaoQ for this difference is not difficult : jj, is the acceleration in 
the path itself; j ia the lolal acceleration, part of its effect being precisely 
to make the pa(A curved; heoce a part of / ia expended not t« increase the 
speed, but to change the direction of the speed, i.e. to bend the path. Notice 
that Ex. 33, p. 65, represents a straight line path; on itjj. = j; thia holds 
only on straight line paths. In uniform motion on a circle, tor eiample. 



64 THE CALCULUS [VI, § 40 

EXERCISES 

[In addition to this list, the second derivatives of some of the functions 
in the preceding exercises may be calculated.] 

Calculate the first and second derivatives in the following exercises. 
Interpret these exercises geometrically, and also as problems in motion, 
with 8 and t in place of y and x. 

1. 2/ = x2 + 5 a; - 4. 11. 2/ = >/F+ Vx^ + 1. 

2. 2/ = - x2 +4x - 4. 12. 2/ = (2 - 3x)2 (3 +x). 

3. 2/ = 2 x2 - X - 15. IZ. y = (x + 2)3 (x^ - 1). 

4. 2/ = — 5 x2 — X — 15. /14. y = Vl +x -r Vl — x. 
^6. y = x2— jx — 21. 16. y=^ax-\-b. 

6. y = — a;' + 3x2 _|_ i, 16. y = c (a constant). 

7. 2/ = 2 x8 + 3 x2 - 36 X - 20. 17. 2/ = oa;2 + 6x + c. 

8. 2/ = - a:^ + 8 x2 + 2. 18. 2/ = c (x - o)». 

9. 2/ = a:* - 2 x3 + 5 x2 + 2. 19. 2/ = (a; - o)"» (x - 6)». 
10. 2/ = (1 + a;) -^ (1 - x). 20. 2/ = Axr-K 

21. Show that the flexion of a straight line is everywhere zero. 

22. Show that if the distance passed over by a body is proportional 
to the time the tangential acceleration is zero. What is the speed? 

23. Show that the flexion of the curve y = ax2 + 6x + c is every- 
where the same, and equal to twice the coefficient of x'. 

24. Show that if the space-time equation is « = a^ + 6i + c, the 
acceleration is always the same and equal to twice the coefficient of <2. 
Is such a motion at all liable to occur in nature? 

26. Find the flexion of the curve y = 1/x. Show that it resembles y 
itself in some ways. Does the slope also resemble y? 

-*26. Can you interpret Ex. 25 as a motion problem? What is true 
at the beginning of the motion (t = 0)? Can a curve with a vertical 
asymptote represent a motion? Can a piece of such a curve? 

J27. Find the flexion of the curve y = (x- 2y (x + 3)« (x - 4). 
Show that the flexion has a factor (x — 2), while the slope has a factor 
(X - 2)2 (x + 3). 



VI, § 41] SUCCESSIVE DERIVATIVES 65 

28. Show that the flexion of the curve y =^^{x-\-aY (x^ -\-3) has a 
factor {x-\-a). 

29. If the function y = / (a;) , where / (x) is a polynomial, has a 
factor (x — a)3, show that' dy/dx has a factor {x — a)2, and d^/dx^ has 
a factor (x — a). 

30. If the equation x^ + ax^ -i- hx^ -^ cx^ -^ dx -\- e =0 has a triple 
root x — at show that the equation 20x^-{-12ax^-^Qbx-h2c=0 
has a factor x — a. 

^1. Show how to find the double and triple roots of any algebraic 
equation by the Highest Common Divisor process. 

C&2. If the equations of the curve in parameter form are x = fi, 
y = ^j find the slope m and the flexion b in terms of t. 

L * dx dt ' dt* dx dt ' dt J 

For each of the following curves, proceed as in Ex. 32. Calculate 
also the values, in terms of t, of each of the six quantities mentioned in 
§ 40, and the value of jr. Compare j and jt- 

S3. x = a + bt,y =^c + dt. ' 34. re = <2^ ^ = ^3. 

36. a; = <, y = <-2; < = 1 and 2. 36. x^l+t,y = ^^^ ; < = ± 2. 

41. Concavity. Points of Inflexion. If the flexion b = 
dm/dx is positive, the slope is increasing, and the curve turns 
upwards, or is concave upwards; if the flexion is negative, the 
slope is decreasing, and the curve is concave downwards. 

Thus y = x^ ia concave upwards everywhere, since 6 = 2 is positive. 
For y = x^ we find 6 = 6 x, which is positive when x is positive, and 
negative when x is negative; hence y — x^ ia concave upwards at the 
right, and concave downwards at the left of the origin. 

A point at which the curve changes from being concave up- 
wards to being concave downwards, or conversely, is called a 
point of inflexion. 

The value of the flexion 6 changes from positive to negative, 



66 THE CALCULUS [VI, § 41 

or conversely, in passing such a point; hence, the value of b at 
a paint of inflexion is zero, if it has any value there.* 

Thus the origin is a point of inflexion on the curve y =*= s^j for the 
curve is concave downwards on the left, concave upwards on the right, 
of the origin. 

42. Second Test for Extremes. In seeking the extreme 
values of a function y = /(x), we find first the critical points, 
i.e. the points at which the tangent is horizontal. 

If, at a critical point, b = (Py/dx^ > 0, the curve is also con- 
cave upwards,^ and the function has a minimum there; if 
6 < 0,the curve is concave downwards, and/ (x) has a maximum; 
that is, 

vr dy ^ , , cPv 
ifm = j^ = and b = -7-| 



> Ol . -, V . (minimum 



<0 



atx = a,f{a)isa 



maximum 



Whenever the flexion is not zero at a critical point, this 
method usually furnishes an easy final test for extremes. If 
the flexion is zero, no conclusion can be drawn directly by this 
method.J (See, however, § 34.) 

43. Illustrative Examples. 

Example 1. Consider the function y —3^ — I2x + 7. See Ex. 3, 
p. 8, and Ex. 1, p. 54. The slope and the flexion are, respectively, 

ax dx^ ax 

* Points where the tangent is vertical, for example, may be points of 
inflexion. 

t The curve is then also concave upwards on both sides of the point ; if 
the curve is concave upwards on one side and downwards on the othet*, b 
must be zero if it exists at the point. 

X Even in this case one may decide by determining whether the curve is 
concave upwards or downwards on both sides of the point; but the method 
of § 34 is usually superior. 



VI, § 43] SUCCESSIVE DERIVATIVES 67 

The critical points are x = ± 2. Since 6 a; is positive when x is 
positive, h is positive for x > 0; lilcewise 6 < when a; < 0. Hence 
the curve is concave upwards when a? > 0, and concave downwards 
when a; < 0. At a; = + 2, 6 > 0, hence by § 42, y has a minimum at 
X = + 2; at a; = — 2, 6 < 0, hence y has a maximum (compare p. 8 
and p. 54). 

To find a point of inflexion first set 6 = 0; 

h — -T- — T^ = 6 a; = 0, i,e. a; = 0. 
ax ax'' 

Since dm/dx is negative for x < and positive for a; > 0, the given 
curve is concave downwards on the left and concave upwards on the 
right of this point; hence a; = 0, y = 7 is a point of inflexion. (See 
Fig. 15, and § 44, p. 68.) 

Example 2. Consider the function y = 3a;*— 12a:» + 50 (Ex. 2, 
p. 55). 

The slope and the flexion are, respectively, 

m = ^ = 12a:3-36a:2; 6 = ^ = ^ = 36a:2 - 72a;. 
dx dx dx^ 

The critical points are x = 0, a; = 3. Ata; = 3, 6 = 108 > 0, hence 
y is a minimum there. At a; = 0, 6 = 0, and no conclusion is reached 
by this method (compare, however, p. 55). To find points of inflexion, 
first set 6=0; 

6 = ^ = f^ = 36x2 - 72x = 0, i^e. x = Cora; = 2. 
dx dx^ 

Near x = 0, at the left, dm/dx = 36 x(x — 2) is positive; at the right, 
negative; the given curve is concave upwards on the left, downwards 
on the right, and (x = 2, y = 2) is a point of inflexion. (See Fig. 13.) 

Example 3. For a body thrown vertically upwards, the distance s 
from the earth is: 

where vq is the speed with which it is thrown. 

The speed and the tangential acceleration are, respectively, 

ds ^ . . d^s dv 

If we draw a graph of the values of s and <, the speed v (slope of the 
graph) is zero when 

V = —gt + VQ-Oy i.e. t - vq/q, 



THE CALCULUS 



[VI, § 43 



I a critical point on the graph. The tangential 
of the graph) is negative everywhere, hence the 



that is, the point 

acceleration (Qexio 
graph is em. 

In particular, at the critical point just found, b is negative; hence 
has a maxim urn there; 

1 



Fig. 17 is drawn for the special values f o = 64 and g " 




44. Derived Curves. It is very instructive to draw in the 
same figure graphs which give the 
values of the original function, its 
derivative, and its second deriva- 
tive. 

These graphs of the derivatives 
are called the derived oaves; they 
represent the slope {or speed in 
case of a motion) and the flexion 
(or tangential acceleration). 
• .^-^--i -\- \ . I-,-- The figures for the curves of Era, 1 

and 2 of I 43 are appended. The stu- 
dent should show that each statement 
made in { 43 and each statement made 
on p. 67, for each of the examples, is illustrated and verified in these 
figures. 

The similar curves for space, speed, and acceleration are drawn in 
Fig. 17, for the motion of a body thrown upwards: 

a =• ~ i gP + V(,t Sor g = S2, v^ '• Qi. 
Verify the s4at«U)ents made in Ex. 3, { 43. 

In drawing such cur^•es, the second derivative should be 
drawn first of all; the information it gives should be used in 
drawing the graph of the first derivative, which in turn should 
be used in drawing the graph of the original function. 



Fio. 15. 



VI, i 441 SUCCESSIVE DERIVATIVES 69 





rim 


111! 


1 1 


' 1 1 1 ' M 


Is 




kP^. 


^ 


mm 


- 




d:^^.- 


zif-rWiT^ 


: 


TT'i- 


T^:^- 




^m 


: 


-^4 






M 


: 


/^'vX 




Eli^: 


- 


:/ \ 


\-;.:/ 


.X / :JJ~_ _ 


- 






. K.^ 


- 


f: 






J 


i : ;" i ■ 




' . j -- 







^ ~r ; ^-^"^ I 1 








































;_:^ rr.: i ■■-^\-r\ , ^-y\-t 



70 THE CALCULUS [VI, § 44 

EXERCISES 

1. Draw, in the order just indicated, the first and second derived 
curves in Ex. 1, p. 56, and show that each step of your work in that 
example is exhibited by these figures. 

2. Draw the derived curves for Exs. 2, 4, 6, 14, p. 56; and show 
their connection with your previous work. 

3. Draw the original and the derived curves for the function 
y =0:' — 6x2 — 15x — 6. Find the extreme values of y, and explain 
the figures. For what value of x is the flexion zero? Does this give a 
point of inflexion on the original curve? 

Find the extreme values of y and the points of inflexion on the fol- 
lowing curves; in each case draw complete figures: 

4. 2/ = 2 x8 - 3 x2 - 72 x. 9. y ^ Ax^ -\-Bx + C. 
6. y = 4 a:3 _j_ g a;2 _ 24 x. 10. y = mx-\-n, 

6. 2/ = x8_|.a;2. 11. 2/=Vx. 

7. 2/ = a:* — 6 a;2 — 40. 12. 2/ = a^ — px + 5. 

8. 2/ = x{x + 2)». 13. y = a;2 - 16/x. 

14. Show that the flexion of the h3rperbola xy ^ a^ varies inversely 
as the cube of the abscissa x, 

16. Show that the flexion of the conic Ax^ + By^ = 1 (ellipse or 
hjrperbola) varies inversely as the cube of the ordinate y, 

16. What is the effect upon the flexion of changing the sign of a in 
the equation y — ax^ -{■ hx -{■ cl 

17. A beam of uniform depth is said to be of ''uniform strength" 
(in resisting a given load) if the actual shape of its upper surface under 
the load is of the form y = ax^ + 6a; + c, where x and y represent 
horizontal and vertical distances measured from the middle point of 
the beam's surface in its original (unbent) position. Show that the 
flexion of such a beam is constant. 

18. Show that the addition of a constant to the value of y does not 
affect the slope or the flexion. 

19. Show that the addition of a term of the form A;a; + c to the 
value of y does not affect the flexion. What effect does it have upon 
the slope? 



VI, § 44l SUCCESSIVE DERIVATIVES 71 

20. Show, by means of Exs. 18 and 19, that any beam in which the 
flexion is constant has the form specified in Ex. 17. 

21. Show, by a process precisely similar to that of Ex. 20 that a 
motion in which the tangential acceleration is constant is defined by an 
equation of the form s = a^ -i-ht -^ c. 

22. Find, by the methods of Exs. 18-21, what the form of y must be 
if the slope is: 

«.)|=0; (5)|=-3; (c)|=6.; (^g=a. + 6. 

23. What is the form of y if the flexion is 6? if the flexion is 2 x + 3? 
if the flexion js zero? 

24. If a beam of length I is supported only at both ends, and loaded 
by a weight at its middle point, its deflection y at a distance x from one 
end is y = k (Sl^x — 4:X^)y provided the cross-section of the beam is 
constant. Find the flexion and show that there are no points of in- 
flexion between the supports. 

26. If the beam of Ex. 24 is rigidly fixed at both ends, and loaded 
at its middle point, the deflection of each half of the beam ia y = k 
(3 fa;* — 4 x^), where x is measured from either end. Show that there 
is a point of inflexion at a distance Z/4 from the end, and that the greatest 
deflection is at the middle point. 

Find the points of inflexion and the point of maximum deflection 
of a uniform beam of length I whose deflection is: 

26. 2/ = A;(3fa;2-a;8). 

[Beam rigidly embedded at one end, loaded at other end. Origin at 
fixed end.] 

27. y=k{3x^P-2x^), 

PBeam freely supported at both ends, loaded uniformly. Origin at 
lowest point.] 

28. y = A;(6Px2-4te3+x4). 

[Beam embedded at one end only; loaded uniformly. Origin at fixed 
end.] 

29. y^k(l^x-3lx^+2x^). 

[Beam embedded at one end, supported at the other end; loaded uni- 
formly. Origin at free end.] 



72 THE CALCULUS [VI, S 45 

46. Angular Speed. If a wheel turns, the angle 6 which a 
given spoke makes with its original position changes with 
the time, i.e. 5 is a function of the time: 

e = /(0- 

The time-rate of change of the angle is called the angular 
speed; it is dejwted by u: 

lu = anffular speed = 



~ dt " 



4 At 



46. Angular AcceleratioiL The angular speed may change; 
the time-rate of change of the angular speed is called the angular 
acceleration; it is denoted by a: 

a = angular acceleration = lim -r-r = 37 = t^ ■ 
iu-K> it at dr 

Example 1. A flywheel of an engine atarte from rest, and moves 
for 30 seconds according to the law 







1 1 










1 






1 




] 






- 
























































































































































































































































/ 


















-h -- 


. 




















' ^'1 






4. 














___ 












■„•;:,.. 1 














1 




















•^ 






-tu 



0"- 



(* + 



where 8 is measured in de- 
grees, after which it rotates 
uniformly. 
Then 



dl ' 



dt 



1 



160 



10 



This example furnishes 
an instaace id which the de- 
rived eta ma, i.e. the graphs 
which show the values of ui 
Fia. 18. and of a are more imparUmt 

than the original curve; for 
the total angle described is relatively unimportant. 
In the figure a scale is chosen which shows particularly well the 



VI, § 46] SUCCESSIVE DERIVATIVES 73 

variation of «; Bis allowed to run ofF of the figure completely, since its 
values are uninteresting. 

The acceleration a is so arranged that it does not suddenly drop to 
zero when the flywheel is allowed to run uniformly; and the values of 
a are never large. Something resembling this figure is what actually 
occurs in starting a large fl3rwheel. 

In actual practice with various machines, curves of this tj^pe are 
often drawn experimentally. The equationis serve only as approximations 
to the reality, but they are often indispensable in calculating other 
related quantities, such as the acceleration in this example. 

Curves which resemble the graph of w in this example occur fre- 
quently. (See §§ 87, 134.) 

EXERCISES 

1. A fljrwheel rotates so that ^ t^ -h 1000, where 6 is the angle of 
rotation (in degrees) and t is the time (in seconds). Calculate the 
angular speed and acceleration, and draw a figure to represent each of 
them. 

2. Suppose that a wheel rotates so that = fi -i- 1000 where 6 is 
measured in radians [1 radian = 180°/7r]. Is its speed greater than or 
less than that of the wheel in Ex. 1? What is the ratio of the speeds 
in the two cases? 

3. If a wheel moves so that 6 = — t^/lQ — </32, where 6 is measured 
in radians and t in minutes, find the angular speed and acceleration in 
terms of radians and minutes; in terms of revolutions and minutes; in 
terms of radians and seconds (of time). 

4. If a Ferris wheel turtis so that = 20 <2 while changing from rest 
to full speed, where d is in degrees and t in minutes, when will the speed 
reach 20 revolutions per hour? 

5. If the angular speed is co = A;<, as in Ex. 4, show that the accelera- 
tion a is constant. Conversely, show that if a = A;, and if < is the time 
since starting, co = kt. 

6. Express the linear speed of a point on the rim of a wheel 10 ft. 
in diameter when the angular speed is 4 R. P. M. 

7. Find the linear speed and the tangential acceleration of a point 
on the rim of the wheel of Ex. 1, § 46, if the wheel is 5 ft. in diameter. 
What are they when t = 30 sec? 



74 THE CALCULUS [VI, § 47 

47. Related Rates. If a relation between two quantities is 
known, the time-rate of change of one of them can be ex- 
pressed in terms of the time-rate of change of the other. 

Thus, in a spreading circular wave caused by throwing a 
stone into a still pond, the circumference of the wave is 

(1) * C = 2 TIT, 

where r is the radius of the circle. Hence 

® %-'"%■' 

or, the time-rate at which the circumference is increasing is 
2 TT times the time-rate at which the radius is mcreasing. 
Dividing both sides by dr/dt, we find 

dc dr ^ dc , , 
-t; -^ Ti = 2 TT = 3- = ac -^ ar: 
at dt dr ' 

that is, the ratio of the time-^ates is the derivative of c with re- 
spect to r; or, the ratio of the time-rates is equal to the ratio of 
the differentials. 

The fact just mentioned is true in general; if y and x are 
any two related variables which change with the time, it is 
true (Rule [Vila], p. 32) that: 

dy dx dy , , 

that is, the ratio of the time-rates of y and x is equal to the ratio 
of their differentials, i.e. to the derivative dy/dx. 

Example 1. Water is flowing into a cylindrical tank. Compare the 
rates of increase of the total volume and the increase in height of the 
water in the tanlc, if the radius of the base of the tank is 10 ft. Hence 
find the rate of inflow which causes a rise of 2 in. per second; and find 
Ibhe increase in height due to an inflow of 10 cu. ft. per second. Consider 
the same problem for a conical tank. 



VI, § 47] 



SUCCESSIVE DERIVATIVES 



75 



(A) 'Bhe volume F is given in terms of the height h by the formula: 



hence 



dV 
dt 



100 



IT 



dt' 



or, the rate of increase in volume (in cubic feet per second) is 100 ir times 
the rate of increase in height (in feet per second). 

If dh/dt = 1/6 (measured in feet per second), dV/dt = 100 7r/6 = 
(roughly) 52.3 (cubic feet per second). If dV/dt - 10, dh/dt = 10 -:- 
100 TT = (rou^ly) .031 (in feet per second) = 22.3 (in inches per 
minute). 

{B) If the reservoir is conical^ we have 

F = J Ttr^h = J 7r/i3tan2 «, 

where r is the radius of the water surface, h is the 
height of the water, and a is the half -angle of the 
cone; forr = h tan a. In this case 

dV I.04. o dh 
-TT — ir/i^tan'' a -j7 , 
dt dt 

which varies with h. If a = 45** (tana = 1), at a 
height of 10 ft., a rise 1/6 (feet per second) would 
mean an inflow of 7r/i2 x (1/6) = 100 7r/6 = 52.3 
(cubic feet per second). At a height of 15 feet, a rise 
of 1/6 (feet per second) would mean an inflow of 
225 7r/6 = (roughly) 117.8 (cubic feet per second). 
An inflow of 100 (cubic feet per second) means a rise 
in height of 100/ tt^^^ which varies with the height; at 
a height of 5 ft., the rate of rise is 4/7r = 1.28 (feet/ 
second). 




FiQ. 19. 



Example 2. A body thrown upward at an angle of 45**, with an 
initial speed of 100 ft. per second, neglecting the air resistance, etc., 
travels in the parabolic path 

r2 



2/ = - 



gz' 



10000 



+ x, 



where x and y mean the horizontal and vertical distances from the start- 
ing point, respectively; g is the gravitational constant = 32.2 (about); 

and the horizontal speed has the constant value 100/^2. Find the ver- 
tical speed at any time ^, and find a point where it is zero. 



76 THE CALCULUS [VI, § 47 

The horizontal speed and the vertical speed, i.e. the time-rate of 
change of x and y^ respectively, are connected by the relation (see 
§§8,20). 

^ _:- ^ = ^ = — ^ 4-1. 

dt ' dt dx 5000"^ ' 

, dy , gx , ^.dx gx , 100 

hence J = (- ^^ + i)_ = - ^ + _. 

This vertical speed is zero where 

gx .100 ^ . 5000 ,„o / u *^ 
— H 7= = 0, I.e. X = = 155.3 (about), 



50 v^ V2 ' ff 

which corresponds to y = 2500/^ = 77.7 (about). At this point the 
vertical speed is zero; just before this it is positive, just afterwards it is 
negative. When x — the value of dy/dt is 100/v^; when x = 
2500/^, dy/dt = 50/V2; when x = 7500/^, dy/dt = - 6O/V2. 



EXERCISES 

y^. Water is flowing into a tank of cylindrical shape at the rate of 
100 gal. per minute. If the tank is 8 ft. in diameter, find the rate of in- 
crease in the height of the water in the tank. 

^. A fimnel 12 in. across the top and 9 iA. deep is being emptied at 
the rate of 2 cu. in. per minute. How fast does the surface of the liquid 
fall? 

3. If water flows from a hole in the bottom of a cylindrical can of 
radius r into another can of radius r', compare the vertical rates of rise 
and fall of the two water surfaces. 

—4. If a fimnel is 12 in. wide and 9 in. deep and liquid flows from it at 
the rate of 5 cu. in. per minute, determine the time-rate of fall of the 
surface of the liquid. 

5. Compare the vertical rates of the two liquid surfaces when water 
drains from a conical funnel into a cylindrical bottle. Compare the 
time-rate of flow from the funnel with the time-rate of the decrease of 
the wet perimeter. 

6. If a wheel of radius R is turned by rolling contact with another 
wheel of radius R'y compare their angular speeds and accelerations. 



VI, § 47] SUCCESSIVE DERIVATIVES 77 

7. If the surface s of a cube increases at a given rate k (in square 
inches per second), what is the rate of increase of the volume? 

8. If a point moves on a circle so that the arc described in time t is 
ff = ^ — 1/^2 _j_ 1^ find the angular speed and acceleration of the radius 
drawn to the moving point. 

9. A point moves along the parabola y = 2x^—xin such a manner 
that the speed of the abscissa x is 4 ft. /sec. Find the general expression 
for the speed of y; and find its value when x = 1; when a; = 3. 

10. In Ex. 9, find the horizontal and vertical accelerations, the total 
speed, the tangential acceleration, and the total acceleration. 

11. A point moves on the cubical parabola y = x' in such a way that 
the horizontal speed is 10 ft. /sec. Find the vertical speed when a; = 6. 

12. In Ex. 11, find the horizontal, vertical, tangential, and total 
accelerations. 

13. If a person walks along a sidewalk at the rate of 4 ft. per sec. 
toward the gate of a yard, how fast is he approaching a house in the yard 
which is 50 ft. from the gate in a line perpendicular to the walk, when 
he is 100 ft. from the gate? When 10 ft. from the gate? 

14. Two ships start from the same point at the same time, one sailing 
due east at 10 knots an hour, the other due northwest at 12 knots an 
hour. How fast are they separating at any time? How fast, if the first 
ship starts an hour before the other? 

^ 15. If a ladder 13 ft. long rests against the side of a room, and its foot 
moves along the floor at a uniform rate of 2 ft. /sec, how fast is the top 
descending when it is 5 ft. above the floor? When the top is 1 inch 
from the floor? 

16. If the radius of a sphere increases as the square root of the time, 
determine the time-rate of change of the surface and that of the volume; 
the acceleration of the surface and that of the volume. 

17. If a projectile is fired at an angle of elevation a and with muzzle 
velocity vo, its path (neglecting the resistance of the air) is the parabola 

y = X tan a — 



2 v^ cos2 a * 

X being the horizontal distance and y the vertical distance from the point 
of discharge. Draw the graph, taking gr = 32, a = 20°, Vq = 2000 ft. /sec. 



78 THE CALCULUS [VI, § 47 

Calculate dy in terms of dx. In what direction is the projectile mov- 
ing when X = 5000 ft., 10,000 ft., 20,000 ft.? How high will it rise? 

18. If p'V — kj compare dp/dt and dv/dt in general; compare 
d^V/d^ and cPv/d^. 

19. If p • «» = ky compare dp/dt and dv/dt. [For air, in rapid com- 
pression, n = 1.41, nearly.] 

20. If 9 is the quantity of one product formed in a certain chemical 
reaction in time t, it is known that q = ckH/{l + ckt). The time-rate 
of change of g is called the speed v of the reaction. Show that 

" = (tSo^ = "(* - «^*- 

Show also that the acceleration a of the reaction is 



CHAPTER VII 
REVERSAL OF RATES — INTEGRATION 

48. Reversal of Rates. Up to this point, we have been 
engaged in finding rates of change of given functions. Often, 
the rate of change is known and the values of the quantity 
which changes are unknown; this leads to the problem of this 
chapter: to find the amount of a quantity whose rate of change is 
known. 

Simple instances of this occur in every one's daily experience. Thus, 
if the rate r (in cubic feet per second) at which water is flowing into a 
tank is known, the total amount A (in cubic feet) of water in the tanlc 
at any time can be computed readily, — at least if the amount originally 
in the tank is known: 

A = r . < + C, 

where t is the time (in seconds) the water has run, and C is the amount 

originally in the tank, i.e. C is the value of A at the time when < = 0. 

If a train runs at 30 miles per hour, its total distance d, from a given 

point on the track, is 

d = SO 't + Cy 

where t is the time (in hours) the train has run, and C is the original 
distance of the train from that point, i.e. C is the value of d when < = 0. 
(Notice that by regarding d as negative in one direction, this result is 
perfectly general; C may also be negative.) 

If a man is saving $100 a month, his total means is 100 'TI + Cj where 
n is the number of months counted, and C is his means at the beginning; 
i.e. C is his means when n = 0. 

If the cost for operating a printing press is 0.01 ct. per sheet the total 
expense of printing is 

T = 0.01-n + C 

where n is the number of copies printed, and where C is the first cost of 
the machine; t.e. C is the value of T when n = 0. 

79 



80 THE CALCULUS [VII, § 49 

49. Principle Involved. Such simple examples require no 
new methods; they illustrate excellently the following fact: 

The total amount of a variable quantity y at any stage is 
determined when its rate of increase and its original value C 
are known. 

We shall see that this remains true even when the rate 
itself is variable. 

50. Illustrative Examples. The rate R{x) at which any 
variable y increases with respect to an independent variable 
X is the derivative dy/dx] hence the general problem of §§ 48- 
49 may be stated as follows: given the derivative dy/dx, to find 
y in terms of x. 

In many instances our famiUarity with' the rules for obtain- 
ing rates of increase (differentiation) Qnsblo;^ us to set down at 
once a function which has a given rate of increase. 

Example 1. Thus, in each of the examples given in § 48, the rate is 
constant; using the letters of this article: 

where /: is a known fixed number; it is obVious that a function which 
has this derivative is 

(A) y = kx+C, 

where C is any constant chosen at pleasure. 

While the examples of § 48 can all be solved very easily without this 
new method, for those which follow it is at least very convenient. The 
value of C in any given example is found as in § 48; it represents the 
value of y when a; = 0. 

Example 2. Given dy/dx — x^, to find y in terms of x. 

Since we know that d (x^)/dx — 3 x^, and since multiplying a function 
by a number multiplies its derivative by the same number, we should 
evidently take: 

X X r ^x \ T 

y = -g , or else y =-^ +C; I check: ^ ( 3 + ^ ) = ^^cb\ » 



VII, § 501 REVERSAL OF RATES — INTEGRATION 81 

where C is some constant. As in § 48, some additional information 
must be given to determine C. In a practical problem, such as Ex. 3, 
below, information of this kind is usually known. 

Example 3. A body falls from a height 100 ft. above the earth's sur- 
face; given that the speed is v = — gt, find its distance from the earth 
in terms of the time t. 

Let s denote the distance (in feet) of the body from the earth; we are 

given that 

ds 

(1) V — -r. = — gt, or ds = vdt "= — gt dt, 

which is negative since s is decreasing. We know that d (^) =2tdt] 
hence it is evident that we should take: 

(2) s = - I <2 + C; [check: ds = - gt dt]. 

As the body starts to fall, ^ = and s = 100; substituting these 
values in (2) we find 100 = + C, or C = 100. Hence we have 

s = - I ^ + 100. 

Example 4. Given dy/dx — ic«, to find y in terms of x. 
Since we know that d(x«+i) = (n + 1) a;»»cte, we should take 

(B) y == —^x^+i + C; [check: dy = x^dx]. 

Since the rule for differentiation of a power is valid (§21, p. 34) 
for all positive and negative values of n, the formula (B) holds for all 
these values of n except n == — 1 ; when n — — I the formula (B) can 
not be used because the denominator n + 1 becomes zero. 

Special cases: 
dx 



w = 1, 5l = ^» y = 2 ^^ "^ ^' check: d f ^ ^^) =xdx. 



n = 0, -^ = 1, y =^x + C; check: d{x) = 1 -dx. 

n = ^» ^ = xi/2, y = 1^3/2 + C; check: d (l^^^^ = x^/^dx. 

n = - 2, ^ = a^^ y = - x-i + C; check: d (-1 a;-i) - x-^dx. 

Notice that these include Vx ( = xV^), l/a;2 ( = a;-2), etc. ; other special 
cases are left to the student. 



82 THE CALCULUS [VII, § 50 

Example 5. Given dyldx = x^ + 2 x^, to find y in terms of x. 

Since d {x^)/dx = 4 x^ and d {x^)/dx = 3 x^, and since the derivative of 
a sum of two functions is equal to the sum of their derivatives, it is 
evident that we should write * 



The check is 



X4 2x3 ^ 



S-e(?+¥+<^)=-+^-*^ 



such a check on the answer should be made in every exercise. 

In general, as in this example, if the given rate of increase (derivative) 
is the sum of two parts, the answer is found by adding the answers 
which would arise from the parts taken separately, since the sum of the 
derivatives of two variables is always the derivative of their sum. 



EXERCISES 

Determine functions whose derivatives are given below; do not 
forget the additive constant; check each answer. 

1. ^^ = 4x. 2.f = -5x. 3. ^=3x^ 4.^ = 2. 
dx dx dx dx 

6. ^^=-6x^.6. ^^ = -10x5. 7. f = -x*. 8. ^ = .01 a*. 
dx dx dx dx 

In the following exercises, remember that the derivative of a sum 
is the sum of the derivatives of the several terms; proceed as above. 

9. ^ = 4 + 5x2. 10. ^ = 4x2-2x + 3. 11. ^ = t^-4t + 7. 
dx dx dt 

12. 1 = 3x5-8x4.18. | = «x+6. 14. |=a^ + M + c. 

16. ^ = . 006 x2-. 004 x' + . 015x4. 16. ^ =■ - /» + St* - 6<« + 2 
ox at 

20. ^ = x2/8. 21. ^ = 2x1/2 - 3a;-i/2. 22. ^ = kv^-^\ 

dx dx dv 

* In all the Examples of this paragraph, we have had an equation which 
involves dy/dx; such an equation is often called a differential equation^ be- 
cause it contains differentials. See also Chapter XIX. 



VII, §511 REVERSAL OF RATES — INTEGRATION 83 

61. Integral Notation. If the rate of increase dyjdx = R (x) 
of one variable-!/ with respect to another variable x is given, a 
function y=I(x) which has precisely this given rate of increase 
is called an indefinite integral * of the rate R (x), and is repre- 
sented by the symbol t 

(1) I(x)^fR(x)dx; 
that is, 

(2) if ^[/(x)] = 2?W, thennx) = fR(x)dx, 

or, what amounts to the same thing, 

(3) if d [I (x)] = R (x) dx, then I (x) ^Jr (x) dx. 

The results of Examples 1, 2, 3, § 50, written with the new 
symbol, are, respectively, 

[A] Ck dx^kx + C. 

fa^dx^x^S + C. 

s =/« dt + C =/- gtdt + C = - gt^/2 + C. 
The first equation of Example 3 holds in general: 

[I] s= Cvdt + C, since ~=i;. 

•/ 4 at 

* The common English meaning of the word integrate is "to make whole 
again," "to restore to its entirety," "to give the sum or total." See any 
dictionary, and compare §§ 48-49. 

To integrate a rate R{x) is to find its integral; the process is called inte- 
gration. Often the rate function R(x) which is integrated is called the in- 
tegrand; thus the first part of equation (2) may be read: *'the derivative oj 
the integral is the integrand.'* This is the property used in checking answers. 

The first equation in (2) and the first in (3) are differential equations. 

t Note that dx is part of the symbol. As a blank symbol, it is J* (blank) 
dx; the function R{x) to be integrated {i.e. the integrand) is inserted in 
place of the blank. The origin of this ssrmbol is explained in § 120. 



84 THE CALCULUS [VII, § 51 

The result obtained in (B), Example 4, § 50, gives 

IB] rxndx=-^+C, HT^-l, 

%/ n "T 1 

for all positive and negative integral and fractional values of 
n except n = — 1, for which see § 65. 

As examples of the many special cases, we write: 

n = 1, J'x dx = -^ + C. 



n 



= 0, fx^dx =fldx =fdx =x + C. 

n=-2, fx-^dx =f^dx = -xr^ + C=---+C. 

From Example 5: 

/(a;3 + 2T')dx =fx^dx +f2x^dx =^ + ^ + C. 

The general principle used in this example is that the inte- 
gral of a sum of two functions is the sum of their integrals: 

[C\ ^[R (X) + S (X)] dx = J/2 {X) dx + Js (x) dx, 

which is true because the derivative of the sum R{x)+S (x) 
is the sum of the derivatives: 

d[R + S]/dx = dR/dx + dS/dx. 

The rules (A), (B), (C) are sufficient to integrate a large 
number of functions, including certainly all polynomials in x. 



VII, § 51] REVERSAL OF RATES — INTEGRATION 85 

EXERCISES 

1. Express the value of y if dy/dx = 4x^+ 3x by means of the 
new sign y (— ) <&. Then find y. Check the answer by differentiation. 

Proceed as in Ex. 1 if y dy/dx has one of the following values: 

2. 3^. 4. x-K 6. x^-2, 8. x^+3x-4, 10. mx - n. 

3. x-K 6. 4 X + 5. 7. 9. 9. x^ - x\ 11. a? + V5. 

In the following exercises express the given function as a sum of 
powers of x; then proceed as above. 

12. x^ (1 + x). 16. (1 + x^) (1 - x3). 20. (1 - x2) (1 + x-^). 

13. (x3 + 5 x2) -f- a;2. 17. (3 - x) (5 + 2 x). 21. x^Hx-x^). 

14. 3(1-2)2. 18. a;V2(2-x). 22. (x^-2x^+x)VK 
16. 3 a:8 (4 _ 3 ^)^ 19. (3 - 2 x) Vx, 23. (1 -|- \(x)2. 

Evaluate the following integrals: 

24. fx'^dx, 29. y(^H-^)<^«'- ^4. f 12 f^/^dt, 

26. ffi/^dt 80. f((ou-^-7u-^)du. 36. fsylr^dy, 

26. fba-^ds, 31. f{^/^-^z-^/^)dz. 36. f(5/Vu^)du, 

27. y (2 i^w - i*-i/2)dw. 32. /{yly^-^ y'^) dy. 37. f{y[u)^du. 

28. y3 r-2/3 dr. 33. / (j/^o/^ + 2 2^/*) rfy. 

Integrate the following expressions, making use of the principle of 
Exs. 12-23. 

38. y (1 - 0^ dt 44. y v^ (a + hx) dx. 

39. y^ (1 + y/x) dx. 46. y^" (a + 6a;) (te. 

40. fs (1 - >/«)2(fo. 46. f(a + &a;)2cte. 

41. y^ (1 - fi) dt, 47. y (^-5 - 2) r6 d<. 

42. yx-4(l4-x+x^)(^. 48.y.i-4(l+x2)2^. 

43. ya? (a + hx) dx. 49. fVt(l +2f)^dt. 



86 THE CALCULUS [VII, § 52 

62. Fundamental Theorem. If dyldx = 2 a;, the answers 
2/ = x^, 1/ = x^ + 5, 2/ = x^ + C are all correct. , To decide which 
one is wanted, additional information is needed. However, 
except for the additive constant C, all answers coincide. 
For practical purposes, there is but one answer. Stated 
precisely, this is the fundamental theorem of integral calculus: 

If the rate of increase 

(1) I = Ri^) 

of a variable quantity y which depends on x is given, then y is 
determined as a function of x,' I (x), except for a constant term: 

(2) y=fRix)dx + C = I (x) + C. 

63. Calculation by Integrals. In applications, we often care 
little about the actual total; it is rather the difference 
between two values which is important. 

Thus, in a motion, we care little about the real total 
distance a body has traveled; it is rather the distance it has 
traveled between two given instants. 

If a body falls from any height, the distance it falls is (Ex. 3, p. 81) 

s = vdt + C =fgtdt + C =-^ + C, 

where s is counted downwards. 

The value of s when < = is s]i=o = C; the value of s when < = 1 is 
s]i = i = g/2 + C. The distance traversed m^^^rs^ second is found by 
subtracting these values: 

where «]JlJ means the space passed over between the times < = and 
< = 1. 

In this calculation, we care little about where « is counted from; or 
its toted value. The result is the same for all bodies dropped from any 
height. 



VII, §54] REVERSAL OF RATES — INTEGRATION 87 
Likewise, the space passed over between the times ^ = 2 and ^ » 5 is 

.2|5.^.,.|.338(,u. 
In general the distance traversed between the times < = a and < = 6 is 

•]::-],..-'l-.-(^+'^)-(4+-)-4-4-i<'--)- 

64. Definite Integrals. The advantage realized in the 
example of § 53 in elinunating C can be gained in all problems. 

The numerical value of the total change in a quantity between 
two values of x, x = a and a; = 6, can be found if the rate of 
change dy/dx = R (x) is given. For, if 

y = I{x)=fR{x)dx + Cy 

the value of y for a; = a is 

and the value of y for x = 6 is 

The total change in y between the values x^ a and x = bis 

= [fR ix) dx\- [fR (x) dxl 

This difference, found by subtracting the values of the in- 
definite integral at x = a from its value at x = b, is called the 
definite integral of R (x) between x = a and x = 6; and is 
denoted by the symbol: 

r'^R{x)dx^\CR{x)dx\ - [ f^W^^l . 



lz»a 



88 THE CALCULUS [VII, § 54 

It should be noticed that, in subtracting, the unknown con- 
stant C has disappeared completely; this is the reason for 
calling this form definite. 

Example 1. Given dy/dx = x*, find the total change in y from 
X = 1 to a; = 3. 
Since 

y=^f2^dx =x4/4 + C, 

it follows that 

,?-'=,] -y\ =J] _J] =20. 
J«-l Jx-3 Jx-1 4Jx-3 4Jx-l 

Interpreted as a problem in motion, where x means time and y means 
distance, this would mean: the total distance traveled by a body be- 
tween the end of the first second and the end of the third second, if its 
speed is the cube of the time, is twenty units. 

Interpreted graphically, a curve whoise slope m is given by the 
equation m = rc^, rises 20 units between re = 1 and x = 3. The equa- 
tion of the curve is 2/ = ^/^ + C, 

EXERCISES 

1. If 'water pours into a tank at the rate of 300 gal. per minute, how 
much enters in the first ten minutes? how much from the beginning of 
the fifth minute to the beginning of the tenth minute? 

2. If a train is moving at a speed of 30 mi. per hour, how far does it 
go in two hours? Does this necessarily mean the distance from iis 
last stop? 

3. If a train leaves a station with a variable speed v = t/2 (ft./sec), 
find s in terms of t. How far does the train go in the first ten seconds? 
How far from the beginning of the fifth to the beginning of the tenth 
second? 

4. A falling body has a speed v = gt, where t is measiu^d from the 
instant it starts. How far does it go in the first four seconds? How far 
between the times t = 3 and < = 9? 

6. A wheel rotates with a variable speed (radians/sec.) <a = ^/lOO. 
How many revolutions does it make in the first fifteen seconds? How 
many between the times t = 1 and t = 10? 



VII, §54] REVERSAL OF RATES — INTEGRATION 89 

From the following rates of change determine the total change in 
the functions between the limits indicated for the independent variable. 
Interpret each result geometrically and as a problem in motion, and 
write your work in the notation used in the text. 

6. ^ = re, a; = 2 to X = 4. 11.^= ^^^ < = 1 to < = 3. 
dx at v^ 

7. f^ = ^x«,x = -2tox = 2.12. | = (l + ^,« = 4to« = 9. 
dx b at <»/2 ' 

8. T^ = rTi, a; = — 4 to a; = 4. 13. ^r = ^s , t = 0.1 to 1. 

dx 12 dt ^ 

9. ^ = 2-a^,a; = Otox = 10. 14. ^ = VtVl; < = 1 to « = 16. 

Determine the values of the following definite integrals. [In cases 
where no misunderstanding could possibly arise, only the numerical 
values of the limits are given. In every stich case, the numbers stated as 
limits are values of the variable whose differential appears in the integral,] 

Sxdx. 21. f x2/3 dx. 26. f sV} («2 -2s)ds. 

^xdx, 22. / iX + t)di. 27. / ^. 

18. r Zx^dx, 23. / 3(^-1) (ft. 28. / (.01 + .02^)<i&. 

19. J^^l^x^ dx. 24./_*^(H-a + 52)ds. ^ f^ (yie + 4^) dd. 

20. f^Vidx. 26. r^^J^ds. 30. f^'^ir-^^^ dv, 
•/o ^1 s^ J2.3 

31. A stone falls with a speed v = (7< + 10. Find « in terms of t and 
find the distance passed over between the times t ==2 and t = 7, 

32. A bullet is fired vertically with a speed v = — gt -\- 1500. How 
far does it go in ten seconds? How high does it rise? How long is it in 
the air? Make rough estimates of the answers in advance. 



90 



THE CALCULUS 



[VII, j 55 



, For any falling body, j = acceleration — ff = eonat. Find the 
speed in ten seconds. Does it matter what particular ten 
seconds are chosen? 

34. If, in Ex. 33, the speed is 100 ft./sec. when ( = 5, what is the 
speed when ( = 15? When will the speed be 250 ft./sec? Express v 
in t«nus of I. 

66. Area under a Curve, We saw in § 54 that the value of 
any quantity could be computed if its rate of change could 
be found. We shall proceed to illustrate this principle by 
showing how to find the area bounded by any given curve, 
the i-axis, and any two ordinates of the curve. 

Let the equation of the given curve be 

(1) S-/W, 

and let A denote the area FMQP between this curve, the 
X-axis, a fixed ordinate FP 
(Fig. 20), and a variable 
ordinate MQ. Since A will 
vary as the value of x at ilf 
changes, A is a function of x. 
If X changes by an amount 
ix = MN, the area A will 
change by an amount Jtf^fiQ, 
which we shall call AA. Then 



^Ay 




Fia.20. 



it is evident from the figure that if the curve rises from Q 
to R we shall have 

(2) redangU MNSQ<AA< rectangle MNRT. 

If the curve falls from Q to B, the inequalities would be 
reversed. From (2) we have 

(3) 1/ ■ Ax <a4 <(y + Ay) ■ Hx. 
Dividing by Ax, we find 

(4) 



VII, §55] REVERSAL OF RATES — INTEGRATION 91 

If the curve falls from Q to R, these inequaUties would 
simply be reversed. If we now let Ax approach zero, Ay will 
also approach zero, and we shall have, in either case, 



(5) 



dA ,. AA .. V 



It follows, by § 54, that the area under the curve (1), between 
any two fixed ordinates x = a and x = b, is given by the 
formula 

= 1 ydx=i f{x)dx. 

Example 1. To find the area under the 
curve* y =^x^ between the points where 
a; = and a; = 2. 

We have, by (2) 

A--fydx+C -=fx^dx +C^^+C, 

where A is counted from any fixed back 
boundary x = A; we please to assume, up to 
a movable boundary x = x. 

The area between a; = and a; = 2 is 
given by subtracting the value of A for yiq 21 

a; = from the value for A for a; = 2: 

aT'^a] -a] =/-%3^ = f.] -f] =|. 

Jx-O Ja;-2 Jx-0 •^ x^O oJ«-2 «>J«-0 «> 

Likewise the area under the curve between a; = 1 and a; = 3 is 

= / x^dx = — — — = 8f • 

aj-l -/x-i 3jx-3 3j«-i ' 

and the area under the curve between any two vertical lines x == a and 
a; = 6is 




AT-* = r-w=^i -I'l 



♦The phrase "the area under the curve" is understood in the sense 
used in § 55. When the curve is below the a;-axis, this area is counted as 
negative. 



92 THE CALCULUS [VII, § 55 

If the equation of the curve is given in parameter form 

i«=/(0, 



<" !:: 



«w, 



the equation (5) may be replaced by the equation 

, . dA _ dA dx _ dx 

^^^ dl~lx"M~'^' dA' 

or 

^^^ it-'^^^^'~dr' 

and the formula (6) takes the form 

or 

which gives the area above the x-axis, below the curve (7), 
and between the ordinates of the points at which t has the 
values ti and <2, respectively. 

Example 2. To find the area under the curve whose equations are 

between the ordinates of the points where t ^2 and < » 3. 
By (11), the required area is 

-31+< 



T" =/ 



.2 t 
3 



2tdt 



^ f (2 + 2t)dt=^7, 

J 2 

[Cautign. By calculating in a similar manner the area under the 
curve from ( = to ( = 1 we would find -AJJ"^ = 3. But this result 
would require justification by the considerations of § 115, p. 188 J 



VII, §55] REVERSAL OP RATES — INTEGRATION 93 

EXERCISES 

Find the area under each of the following curves between the ordi- 
nates x =0 and x — 1; between x = 1 and a; = 4. Draw the graph 
and estimate the answer in advance. 

1. 2/ = a;2. 4. 1/ = xVs. 7, y = VT+~x, 

2. 2/ = Vx, 6. 2/ = 1 — a;2. 8. y = x^l — x). 

3. 2/ = x3/2. 6. y = (I- x)2. 9. 2/ = xil - x^). 

Find the area under each of the following curves and check graphi- 
cally when possible. 

10. 2/ = i^ + 6 a;2 + 15 X, (x = to 2; a; = - 2 to + 2). 

11. y — x2/3, (x = — 1 to + 1; X = — a to + a). 

12. y =x^ + l/x2, (x = 1 to 3; X = 2 to 5; x = a to 6). 

Find the area under each of the following curves between the ordi- 
nates determined by the indicated values of t, and check graphically. 

13. X = < + 1, 2/ = < - 1; « = to 5. 

14. X = (< - 1)A y = fi/S; « = 2 to 4. 
16. X = 2 «, y = 3 VF; < = to 4. 

16. X = 1 + V?, 2/ =2 ^; < = to 9. 

17. X = (1+ 0^ 2/ = (1 - 0*; « = 1 to 2. 

18. X = 1 - «, 2/ = vT+1; < = - 1 to 3. 

19. X = VT+l, 2/ = ^^"^=1; « = 1 to 5. 

20. Show the area A bounded by a curve x =<l>(y), the 2/-axis> 
and the two lines 2^ = a and y = 6 is 



^= ] <t>(y)dy. 



21. Calculate the area between the 2/-axis, the curve x = y^, and the 
lines y = and y = 1. Compare this answer with that of Ex. 14. 

22. Find the area between the curve y — o^ and each of the axes 
separately, from the origin to a point (A;, W), Show that their sum is k^. 



d4 



THE CALCULUS 



[VII, § 56 



66. Volume of a Solid of Revolution. Let us next consider 
the volume of the solid of revolution which is described when 
the area MNLK (Fig. 22) under the curve- y = f{x) from 
X = a to X = b 18 revolved about the x-axis. Any section of 
this solid perpendicular to the x-axis will be a circle. 

Let us denote by V the volume from x = a to x = x, and 
by AV the increase in this volume as x increases to x + Ax. 
The radius of the circular section at any point is the ordinate 




Fig. 22. 

y of the curve. Hence the area of the section is wy^. If 
the curve is rising steadily from P to Q, it is evident that 

(1) 7ri/2.Ax<AF< TT (y + Ay)2 . Ax. 

Dividing by Ax, we have 

AV 



(2) 



Try < ^"^'^^y'^^y^ ' 



If the curve is falling, these inequalities are reversed. If we 
now let Ax approach zero, Ay will approach zero, and we 
shall have, in either case, 



(3) 



dv ,. ^v , 

-7- = lim -r- = 1^J/^ 



VII, §571 REVERSAL OF RATES — INTEGRATION 95 

It follows, by § 54, that the volume of the solid of revolution 
from X = a to X = fe, is given by the formula 



(4) 



]x^b /•x*6 /•x-6 

= 1 iry'dx= \ ir\fix)}»dx. 
x^a J xr»a J x» a 



Similarly, the volume F of a solid of revolution formed by 
revolving a curve x=<f>(y) around the y-axis satisfies the 
relations 

dV -^^"^ '•^"'^ 



(5) 



dy 



= TTX^, 



yJ-.J 



TX^dy. 



y— c 



Example. Find the volume generated when the area under the 
curve 2/ = 1 — x^ from a; = — ltoa; = +l revolves about the rc-axis. 

From the symmetry of the figure, we see that the total volimie re- 
quired is twice the volume generated by the area from x = to a; = 1. 

Hence 



= 2 / iry^dx 

J 
=-2jr(x- 



y-l-a;2 



2 0^ a;5\-[i 

3 "^5; Jo 
16^ 




[Fig. 23. 



57. Volume of a Frustum of a Solid. A frustum of a solid 
is the portion of that solid contained between two parallel 
planes. The solid itself, between the limiting parallel 
planes, may be thought of as generated by the motion of the 
cross-section parallel to these planes from one extremity to 
the. other, if the shape of the cross-section is supposed to 
vary in the correct manner during the motion. Thus, a 
frustum of a circular cone may be generated by the motion 
of a circle which remains parallel to its origiual position, if 



96 



THE CALCULUS 



[VII, § 57 



18^8 



the radius of the ckcle steadily increases (or diminishes) 

during the motion. 
In Fig. 24, let s denote the distance along a Une AB 

perpendicular to the variable cross-section, measured from 

some fixed point A. 
Let V denote the 
volume of the solid 
from 5 == a to s = s, 
-«+^« and let AV denote 
the increase in vol- 
ume as 5 changes to 
8 + As, Let As de- 
note the area of the 
cross-section at the 
position s = s, and 

let AA denote the increase in As as s changes from s to 

5 + As. Then, if As increases as s increases, we shall have 

(1) A,- As<AF<(il, + Ail) -As. 

This inequality will be reversed if As decreases. Dividing 
by As, and then allowing As to approach zero, AA will also 
approach zero, and we shall have 




Fig. 24. 



(2) 



^^ = lim^ = A„ 



ds A«-»o As 

whence, by § 54, the volume of the entire frustum from 
a; = a to a; = 6 is given by the formula 

(3) ^ = I '^» <'* 

The formulas (2) and (3) show that the rate of change of 
the volume with respect to* the distance s is equal to the 
area of the variable cross-section, and that the volume of 



VII, §57] REVERSAL OF RATES — INTEGRATION 97 

the entire frustum is obtained by integrating the area of 
the cross-section with respect to s. The formulas of § 56 
are special cases of the formula (3). 

Example. A circle moves with its center on a given straight Une, 
and its plane perpendicular to that hne. Its radius is proportional to 
the square of the distances of its center from a fixed point of the line. 
Find the volume of the frustum of the sohd generated as the circle 
moves from « = a to « = 6. 

If 8 denotes the distance from the fixed point to the center of the 
circle, the radius of the circle, which is to vary as the square of a, must 
be r = ks^f where A; is a constant. Hence the area of the circle is 

Then the volimie of the frustum from 8 = ato s = bia 

b Jb b 



V 



1 = / irA;2«4ds = irA;2 r 8*d8 



EXERCISES 

Find the volumes formed by revolving each of the following curves 
about the x-axis, between a; = to a; = 2; between a; = — ltoa;=+l. 

1. y = a^. 3. y = a^ — X. 5, y^ ^^ x +2y, 

2. y ^x^-l. 4. 2/ = (1 + a;)2 6. V^+l + Vy = 4. 

Proceed similarly for each of the following curves, between a? = 1 
and X = 3; between x = a and x = 6. 

7. 2/ = ^-^' 8. xy = 1+ a;2. 9. x* - x2y2 = 1. 

Find the volimies formed by revolving each of the following curves 
about the y-ajdSf between 2/ = and y = 2, 

10. X = ^. 12. X = 4 2/2 — 2^. 14. aj = ^2 — y^ 

11. x2 = 2/8. 13. x2 + 2/4 = 81. 16. X = 2/^/2 + 2/V4. 

16. Find by integration the volume of a frustum of a cone of height 
hf if the radii of the two bases are, respectively, r and R. 



98 THE CALCULUS [VII, § 57 

17. Find the volume of the paraboloid of revolution formed by 
revolving y^ = 4 ^ about the a;-axis, between x = and a; = 4; between 
X = 1 and a; = 5; between x = a and x = 6. 

18. Find the volume of a sphere by the formula of § 56. 

19. Find the volume of the ellipsoid of revolution formed by revolv- 
ing an ellipse (1) about its major axis; (2) about its minor axis. 

20. Find the volume of the portion of the hyperboloid of revolution 
formed by revolving about the 2/-axis the portion of the hyperbola 
ic2 _ y2 =s 1 between 2/ = and y = 2. 

21. Find the volume of the portion of the hyperboloid of revolution 
formed by revolving x^ — y^ — 1 about the rc-axis, between x = 1 and 
a; = 3. 

22. Find the voliune generated by a square of variable size perpen- 
dicular to the X-axis, which moves from x = Otox = 5, if the length of 
the side of the square is (1) proportional to x; (2) equal to x^, 

23. Find the volume generated by a variable equilateral triangle per- 
pendicular to the X-axis, which moves from x=0tox = 2, ifa side of 
the triangle is (1) equal to x^; (2) proportional to 2 — x. 

24. Find the volume generated by a variable circle which moves in a 
direction perpendicular to its own plane through a distance 10, if the 
radius varies as the cube of the distance from the original position. 

26. Find the mass of a right circular cylinder of variable density, if 
the density varies (1) directly as the distance from the base; (2) in- 
versely as the square root of the distance from the base. 



CHAPTER VIII 

LOGARITHMS — EXPONENTIAL FUNCTIONS 

58. Necessity of Operations on Logarithms. The necessity 
for the introduction of logarithms in the Calculus depends 
not only on their own general importance, but also upon the 
fact that integrals of algebraic functions may involve logarithms. 

Thus, in §51, in the case n = — 1 the integral yx^dx could 
not be found, although the integrand 1/x is comparatively 
simple. We shall see that this integral, J*x~^ dx, results in a 
logarithm. We shall see also in § 68 that numerous cases 
arise in science in which the rate of variation of a function 
/ (x) is precisely 1/x. 

69. Properties of Logarithms. The logarithm L of a num- 
ber N to any base B is defined by the fact that the two 
equations 

(1) iV = B^ logBN = L 

are equivalent. Thus if L = logBiV and l^logsn, the 
identity B^B^ = B^^^ is equivalent to the rule 

(2) logs (N-n) == logs N + logs n, 

where n and N are any two numbers. Likewise B^ -^B^ =^ 
B^'^ gives 

(3) logB (iV -^ w) = logs N - logs n; 
and (B^y = B^ becomes 

(4) logBiV" = nlogsiV, 
where n may have any value whatever. 

The relations (1), (2), (3), (4), are the fundamental rela- 
tions for logarithms. 

99 



100 



THE CALCULUS 



[VIII, § 60 



60. Computations. Graphs. To draw the graph of the 
equation 

(1) y^^logBX, 

for any fixed value of B, we may write the equation in the 
form 

(2) z = B^. 

To compute the value of x when y is given, we take the 
common logarithm of both sides of (2) : 

(3) logio X = logio B" -=y' logio B, 
by (4) § 59. But since y = logs Xy we have 

(4) logio X = logB X ' logio By 
or 

(5) logB X = logio X -4- logic B. 







y 






























3^_ 


- 




— 


























^ 


B 


5 




















"^ 




























^ 


-^ 














B 





2 


2.7 













y 


^ 












— 




— 


■D 


' 


e = 


*■ 








/ 


A 


^^ 


^ 


-^ 


' 






. — 




— 


D 


— ^ 












/ 


r 




-— ■ 


— - 


— 








— 






B 


= 


10 








1 


^ 









■ — 


— 


" 




















1 








5 








1 











1 


5 






X 


f 






































II 







































Fig. 25. 

The relations (4) and (5) enable us to compute logarithms 
to any base quickly by means of a table of common loga- 
rithms. The graphs of (1) for several values of B are shown 
in Fig. 25. 



VIII, § 601 LOGARITHMS 101 

The relation (3) enables us to compute fractional powers 
of any base. For, if B and y are given, as in (2), x may be 
found from (3) by means of a table of common logarithms. 

Similarly, if we take the logarithms of both sides of (2) with 
respect to any other base 6, we find the corresponding rela- 
tions 

(4) ' logs X = logB X ' logs B, 

(5)' logsx = logbX -4- logbB. 

If we set X = fe in (4)' and (5)', since log^fe = 1, we find 

(6) logsfe-logftS = 1 and log^fe = 1 -^ logjB. 

EXERCISES 

1. Find the value of 10* when x = 3; 0; 1.6; 2.7; - 1; - 1.9; 0.43. 

2. Plot the curve y = 10* carefully, using several fractional values 
of x. 

3. Plot the curve y = logio x by direct comparison with the figure of 
Ex. 2. Plot it again by use of a table of logarithms. 

Plot the graph of each of the following functions. 

4. logioxS. 6. logio-^. 6. logio (l/a;2). 7. logjoa:*/^ 
Do any relations exist between these graphs? 

Plot the graph of each of the following functions and explain its 
relation to graphs already drawn above. 

8. logio (1 + x)2. 9. logio yll+x, 10. logic (x ^1 + x). 

Plot the graphs of each of the following functions and show the 
relations between them. 

11. logjx. 12. logjx. 13. logja;2. 14. 3*. 

Show how to calculate most readily the values of the following ex- 
pressions, and find the niunerical value of each one. 

16. logii7. 17. V(5.4)6-2. 19. 100-5 H- 10-0-5. 21. logs 100. 

16. 24-53. 18. logieS. 20. 21og»5. 22. 10 logio 9. 



102 THE CALCULUS [VIII, § 61 

61. Napierian Logarithms. Base e. A careful examination 
of Fig. 25 will convince anyone that there must be a value of 
B for which the curve y = logsx has a slope equal to 1 at 
X = 1. Indeed, the equation (5), §60, shows that the 
slope of the curve y = logsX can be found by dividing the 
slope of the curve y = logiox by logioB. Hence if logio-B is 
equal to the slope of the curve y = logiox at the point (1, 0), 
the slope of the curve y = logsX will be 1 at (1, 0). 

Let this value of B be denoted by the letter e. Logarithms 
to the base e are called Napierian logarithms,* or natural 
logarithmsy or hyperbolic logarithms, (See Table V, C.) 

62. Differentiation of log« x. To find the derivative of log«a:, 

* let us write 

"^ y=log.x p^,^-^^" ^^^ ^ = ^^^^'^• 

^ (2) y + Ay=-loge{x + Ax). 

logiuh) 

X Hence 

Ay = loge (X + Ax)- logeX 

-.«g.(i+f), 
..d |.i,^(i+f).i.i,<^(i+f). 

Now let u = Ax/Xf so that we may write 

A^ ^ 1 loge (1 + ^) 

Ax X u ^ 

But the fraction {loge(l + u)}/u is simply the slope of 
the secant AP of the curve log«t^, and as Ax— ^0, so also 

* Named for Lord Napier, the inventor of logarithms. The value of c is 
stated below. No assumption is made at this point except that the logarithm 
curve has a tangent at (1,0). 




VIII, § 63] LOGARITHMS 103 

w— >0; hence the secant AP becomes the tangent at A and 
its slope has the limit 1, by the definition of e. Hence 

Therefore lim ^ = i • lim ^-^^i^l+i!^ = 1 • 1, 
or 

[vm] ^^ = ^. 

On account of the simplicity of this formula the base e will be 
used henceforth in this book for all logarithms and exponentials 
unless the contrary is explicitly stated. 

63. Differentiation of log^x. Since we have, by (4)', § 60, 

(1) y = logB X = loge X . logfi e, 

the derivative of log^x is found by multiplying the derivative 
of log«a; by log^e: 

dx X 

In particular, for common logarithms, since B = 10, we have 

(2) -^^ = --log.oe. 

The constant factor logio e is the value of the slope oi y = 

logioa: at (1, 0). It is called the modtdus of the system of 

common logarithms, and is denoted by the letter Af , that is 

logio e = M. Hence the preceding equation becomes 

[Vnib] dlogiox^M, 

dx X 

By means of formula VII, § 22, for change of variable, 

the formula VIII becomes 

,«s dlogeU _ 1 ^dw 

dx u dx 

The formulas Villa and Vlllb may be rewritten in a similar 

manner. 



104 THE CALCULUS [VIII, § 64 

64. Values of M and of e. To compute approximately the 
value of M, that is the slope of the curve y = logiox at (1, 0), 
let us draw the secant connecting the points P (1, 0) and 
Q (1 + Ax, + Ay) on that curve^ Let us denote the slope 
of this secant PQ by Mpq, Then 

Ay logio (1 + Ax) 
"^^^^Ai^ Ai 

If we choose for Ax a succession of smaller and smaller 

values, 

Ax = 0.1, 0.01, 0.001, ..., 

we find a corresponding succession of values of rripQi 

mpQ = 0.414, 0.432, 0.434, .... 

For the last of these values, a six or seven place logarithm 
table is required, while still higher place tables would be 
required to get a more accurate answer. Since the slope at 
(1, 0) is the limit of ttipq as Ax approaches zero, we have 

M = lim mpQ = 0.434 ... (approximately).* 

From this value of M, we can compute e, since 

logioe = M = 0.434 ... 

Hence, from a table of common logarithms, 

e = 2.72 ... (approximately). 

65. Illustrative Examples. 

Example 1. Given y = logi© (2 x^ + 3), to find dy/dx. 

Method 1. Derivative notation. Set u = 2 x^ + Sj then 

dy _dy du _ d logip u d(2x^ -\- 3) _M . _ 4: Mx 
dx" du dx du dx u "~2a;2-j-3 

* An independent method of calculating the values of M and of e will 
be given in §§ 147, 153. Logically, we might have waited until that time to 
state the value of M, but it is much more convenient, practically, to have 
an approximate value at once. To ten decimal places, the values are 
j»f = 0.4342944819, l/ifcf =2.3025850930, 6 = 2.7182818285. 



VIII, § 65] LOGARITHMS 105 

Method 2. Differential notation. 

dy = dlog,o(2x2 + 3) = 2^p^d(2x2 +3) = 2^%^^ 

Example 2. Find the area under the curve y = 1/x from a; = 1 to 
X =10, using formula [VIII] inversely: 

= / -dx=logex\ = logc 10 = ,—^ = j^ = 2.3026 * 

x-i J x~\ X ^ J-p.i '^ logio e M 

Example 3. If the rate of increase dy/dx of a quantity y with 
respect to a; is 1/x, find y in terms of x. 
Since dy/dr = l/x, 

2/ = /-^ = logcx+c, 

where c is a constant, — the value of y when x = 1. It should be noted 
that logarithms to the base e occur here in a perfectly natural manner; 
the same remark applies in Example 2. Note that 

logc X = logioX -r M. 

This case arises constantly in science. Thus, if a volume v of gas ex- 
pands by an amount AVj and if the work done in the expansion is ATT, 
the ratio aW/Av is approximately the pressure of the gas; and dW/dv 
T= p exactly. If the temperature remains constant pv — & constant; 
hence dW/dv = k/v. The general expression for W is therefore 

W — J - dv = k logc V -\-Cf 

and the work done in expanding from one volume vi to another volume 
V2 is 

TtT"*" = r""- dv^k \o^ vT = A; loge '^ = ^ logic ^• 

♦The number log« 10 =1 4- Af = 2.302585 is important because common 
logarithms (base 10) are reduced to natural logarithms (base e) by multi- 
plsring by this number, since log. iV"= logic ^Xlog* 10. Similarly, natural 
logarithms are reduced to common logarithms by multiplying by Af = 
log X e; since log i o iV = ifcf • log« iV". It is easy to remember which of these two 
multipliers should be used in transferring from one of these bases to the 
other by remembering that logarithms of numbers above 1 are surely 
greater when e is used as base than when 10 is used. 



106 THE CALCULUS [VIII, § 65 

EXERCISES 

Calculate the derivative of each of the following functions; when 
possible, simplify the given expression first. 

1. logioa;3. 2. logio >/J. 3. logw (1+ 2 a;). 

4. logio (1 + a^). 5. loge (1 + x)\ 6. loge V3 +-5x. 

I 

7. loge (l/x), 8. logio (x"^), 9. X loge x^, 

'^' '^^ (m) • ''' ^^«^« {' - r^^) • ''• ^^^ vi=^- 

13. ^^^ 14. logejlogex}. 15. (logcO*. 



Evaluate each of the following integrals.. 



16. /"^ -dx. 17. /"* '^ — ^dx. 18. f^ 

Jl X Jz x Js 



X3 



^^l-\-x^^ «-, /•^^(2-O^j, «- r^Qt^-2t^-l 



dx. 



dt. 



19. /•'" L±£!dx. 20. /""" ^^^<«. 21. r ^J^^ 
^10 a; •/lo 3^4 ^1 3/3 

26. Calculate the area between the hyperbola xy == 1 and the x-axis, 
from X = 1 to 10, 10 to 100, 100 to 1000; from x = 1 to a; = A;. 

26. Show that the slope of the curve y = logio x is a constant times 
the slope of the curve y = loge x. Determine this constant factor. 

27. Find the flexion of the curve y = loge x, and show that there are 
no points of inflexion on the curve. 

28. Find the maxima and minima of the curve 

y = logc(a;2-2« + 3). 

Find the maxima and minima and the points of inflexion (if anj' 
exist), on each of the following curves: 

29. y = x- loge X. 30. 2/ = X - logc (1 + x^). 
31. y = x2 - 4 loge x2. 32. t/ = (2 x + log x)2. 

Find the areas under each of the following curves between x = 2 
and X = 5: 

33. y=x + l/x. 34. y = (x^ + l)/x3. 35. y = (xi/2 - x)/x2. 



VIII, § 66] LOGARITHMS 107 

36. Find the volume of the solid of revolution formed by revolving 
that portion of the curve xy^ = 1 between a? = 1 and a? = 3 about the 
X-axis. 

37. If a body moves so that its speed v = < + 1/^, calculate the dis- 
tance passed over between the times ^ = 2 and 2 = 4. 

38. Find the work done in compressing 10 cu. ft. of a gas to 5 cu. ft., 
if po = .004. 

39. Find the areas under the hyperbola xy = A* between a; = 1 and 
X — CyC and c^, c^ and c^, & and c*. 

66. Differentiation of Exponential Functions. Let us con- 
sider first the function 

(1) V = B\ 

Taking the logarithms of both sides of this equation with 

respect to the base e, 

(2) loge 2/ = X • loge B. 

Differentiating both sides with respect to x, we have, by VIII, 

Hence we have the formula 

[IXa] ^^^B^log^B. 

For the special cases B = e and B = 10, we have 
[IX] — = e', 

[1X6] ^ = \{^ loge 10 = ^ = 10'(2.302585 . . .). 

If u denotes a function of x, we may combine any of these 
formulas with formula VII, § 22; thus the formula IX, 
which we shall use most often, becomes 
,M\ de^ du 



108" THE CALCULUS [VHI, § 67 

67. Illustrative Examples. 

Example 1. Given y = e^,to find dy/dx. 

Method 1. Set x^ = u; then 

dy dy du de^ d(a;2) « o ^ 

ax du dx du dx 

Method 2. dy^d^^^ d{x^) = 2 xe*'(to. 

Example 2. Find the slope of the curve 

(1) 2^ 2~' 

and determine its extreme values. 
Since de~^/dx = — e-*, we have 

(2) ^ = ^-^^ 

To determine the extreme values, first set dy/dx = 0: 

— 2 — =0> or e' =e * = -. 
Clearing of fractions, 

e2* = 1, whence x = 0. 

To determine whether y is really a maximum or a minimum at a; = 0, 
we find 

. d^y _ e^+e~^ . 

hence d^/dx^ = 1 when x = 0. Consequently y is a minimum 
(§ 42, p. 66) at a; = 0. 

The curve (1) is called a catenary. This curve is very important 
because it is the form taken by a perfect inelastic cord hung between 
two points. The given function is often called the hyperbolic cosine 
of Xf and is denoted by cosh x. The expression (e* — e-*)/2 in (2) is 
called the hyperbolic sine of Xj and is denoted by the symbol sinh x: 

U) ^Jihx = ^'^J~' , coshx = ?^!^t^. 

^^ 2 2 

The equations (2) and (3) show that 

^^v cf cosh X . 1. dsinhx * 

(5) « woix^ ^ gjjj^ ^^ *'°*~^ = cosh X. 

^ ^ dx dx 



VIII, § 67] LOGARITHMS 109 

Example 3. If a quantity y has a rate of change dy/dz with respect 
to X proportional to y itself, to find y in terms of x. Given 

dx ^' 
we may write 

,dx 1 

dy y 
hence • 

^ = fr.dy = *^8e y+Cf 

•/ y 

by § 65, Ex. 3. Transposing c, we have 

loge y — kx — Cj or ^ = e**^ = e^e** = Ce**, 

where C( = e^)is again an arbitrary constant. 

TAe only quantity y whose rate of change is proportioned to itself is 
Cc** where C and k are arbitrary , and k is the factor of proportumality. 
This principle is of the greatest importance in science; a detailed dis- 
cussion of concrete cases is taken up in § 68. 

£X£RCIS£S 

Find the derivative of each of the following functions: 
1. c3x. 2. e^^+^\ 3. e^^^i+5. 4. c><«^. 

5. a;2e*. 6. (l-x)^€^. 7. 103^^+4. 8. a^^+^K 

9. loge*. 10. log (l+e*). 11. loge"**. 12.. {loge^^)* 

13. (e- + l)2. 14. e:!L±±^. 16. ^^^"^"^. 16. ''-''\ 

2 2 e*+er* 

17. Show that the slope of the curve y — e^ ia equal to its ordinate. 

18. Show that the area under the curve ^ = e* between the ^-axis 
and any value of a; is y — 1. 

19. Find the area under the catenary from a; = to a? = 3; from 
ir = — ltoa; = +l; from a; = to a; = a. [See Tables, V, C.] 

20. Find the area under the curve y = sinh x from a; = to a; = 3; 
from X = tox — a. 

Find the maxima and minima and the points of inflexion (if any 
exist) on each of the following curves: 

21. y = x€^. 22. y = x^e^. 23. y = sinh x. 

24. y = e-^. 26. y = xer^, 26. y = sech a; = 1 -^ cosh x. 



110 THE CALCIJLUS [VIII, § 67 

27. Show that the pair of parameter equations x — cosh t^y = sinh t 
represent the rectangular hyperbola x^ — y2 = i. Hence show that the 
area under the h3rperbola x^ — y^ = 1 from a; = ltoa; = ais represented 
(see (9) § 55) by the integral 

f '\mh^ tdt-- f f(cosh 2 t - 1)/21 dt, 

*^ t-Q •' < = 

whepe cosh c =^a. Hence show that this area is (sinh 2 c)/4 — c/2. 
e^(te. 81. y sinh2a;<ia;. 34. J (e*H-l)2(te. 

29. J e-^dx. 32. J* coahSxdx. 36. ^ (e*+3)r«dx. 

30. ye2* da;. 33. f sinh2 x (te. 86. f (e^+^ + 1) dx. 

68. Compound Interest Law. The fact proved in the Ex. 3 
of § 67 is of great importance in science: 
If a variable quantity y has a rate of increase 

with respect to an independent variable x proportional to y 

itself, then 

(2) y = Ce^, 

where C is an arbitrary constant. 

The equation (2) between two variables x and y was 
called by Lord Kelvin the ''Compound Interest Law" 
on account of its crude analogy to compound interest on 
money. For the larger the amount y (of principal and in- 
terest) grows the faster the interest accumulates. 

In science instances of a rate of growth which grows as the 

total grows are frequent. 

Example 1. Work in Expanding Gas, The example used to illus- 
trate Ex. 3, § 67, can be put in this form. Since, in the work W done in 
the expansion at constant temperature of a gas of volume v, we found 
dW/dv = k/v, it follows that dv/dW = v/k; hence v = ile^/*, which 
agrees with the result of § 67. 



VIII, § 68] LOGARITHMS 111 

Example 2. Cooling in a Moving Fluid, If a heated object is 
cooled in running water or moving air, and if ^ is the varying difference, 
in temperature between the heated object and the fluid, the rate of 
change of (per second) is assumed to be proportional to 6: 

de ,^ 
di^-^'^ 

where t is the time and where the negative sign indicates that is de- 
creasing. It follows that ^ = C-e^**. [Newton's Law of Cooling.] 

Such an equation may also be thrown in the form of § 67; in this 
example, dt/dd = ^ l/(kd)y whence t = — {l/k)'\ogeO + c, and the 
time taken to cool from one temperature ^i to another temperature O2 is 

where $ is the temperature of the body above the temperature of the 
surrounding fluid. 

The law for the dying out of an electric current in a conductor when 
the power is cut off is very similar to the law for cooling in this example. 
See Ex. 19, p. 114. 

Example 3. 'Bacterial Growth. If bacteria grow freely in the pres- 
ence of unhmited food, the increase per second in the number in a cubic 
inch of culture is proportional to the number present. Hence 

^^kN,N^ Ce^, t = JlogeiV + c, 

where N is the number of thousands per cubic inch, t is the time, and k 
is the rate of increase shown by a colony of one thousand per cubic inch. 
The time consumed in increase from one number Ni to another number 
N2 is 

JNi *^ Nik N k ^ Jati k ** Ni 

If N2 = 10 ATi, the time consumed is (I/A;) log^ 10 = l/{kM). This 
fact is used to determine ky since the time consumed in increasing N ten- 
fold can be measured (approximately). If this time is T, then T = 
l/(kM)y whence k = 1/{TM), where T is known and M = 0.43 (nearly). 

Nmnerous instances similar to this occur in vegetable growth and in 
organic chemistry. For this reason the equation (2) on p. 110 is often 
callecf the ''law of organic growth, ' ' (See Exs. 20, 21, p. 114.) 



{ 



112 THE CALCULUS [VIII, § 68 

Example 4. Atmospheric Pressure. The air pressure near the sur- 
face of the earth is due to the weight of the air above. The pressure at 
the bottom of 1 eu. ft. of air exceeds that at the top by the weight of 
that cubic foot of air. If we assume the temperature constant, the 
volume of a given amount is inversely proportional to the pressure, 
hence the amount of air in 1 cu. ft. is directly proportional to the pres- 
sure, and therefore the weight of 1 cu. ft. is proportional to the pressure. 
It follows that the rate of decrease of the pressure as we leave the earth 's 
surface is proportional to the pressure itself. 

^ = - fcp, p = Cer^y A = - ^loge p + c, 

where h is the height above the earth, and, as in Exs. 2 and 3, the dif- 
ference in the height which would change the pressure from pi to ps is 

Since A]^, and pt and pi can be found by experiment, k is determined 
by the last equation. 

69. Percentage Rate of Increase. The principle stated in 
§68 may be restated as follows: In the case of bacterial 
growth, for example, while the total rate of increase is clearly- 
proportional to the total nimiber in thousands to the cubic 
inch of bacteria, the percentage rate of increase is constant. 

In any case the percentage rate of increasej rp, is obtained 
by dividing 100 times the total rate of increase by the total 
amount of the quantity y 100 • {dy/dx) -r- y; and since the equa- 
tion dy/dx = ky gives (dy/dx) -i- y = ky it is clear that the 
percentage rate of increase in any of these problems is a constant. 
The quotient (dy/dx) -r- y, that is, 1/100 of the percentage 
rate of increase, will be called the relative rate of increasey and 
will be denoted by rr. 

In some of the exercises which follow, the statements are 
phrased in terms of percentage rate of increase, r^, or the relar- 
live rate of increase, r, = r^, -5- 100. 



VIII, §69] LOGARITHMS 113 

£X£RCIS£S 

Find dyldx and {dy/dx) -5- y for each of the following functions: 

1. 7 63*. 4. ^\ 7. ^ax + h)^. 

2. 4er2.to 5. e4«+5. 8. {x^ + pz-\- q)^, 

3. ice*. 6. (a;2 + 2)e«. 9. (3x + 2)e-*'. 

10. If a body cools in moving air, according to Newton's law, dd/dt 
= — kdj where t is the time (in seconds) and 6 is the difference in tem- 
peratm-e between the body and the air, find A; if ^ falls from 40® C. to 
30** C. in 200 seconds. 

11. How soon will the difference in temperature in Ex. 10 fall to 
10® C? 

12. In measuring atmospheric pressure, it is usual to express the pres- 
sure in millimeters (or in inches) of mercury in a barometer. Find C in 
the formula of Ex. 4, § 68? if p == 762 mm. when h = (sea level). Find 
C if p = 30 in. when A = 0. 

13. Using the value of C found in Ex. 12, find k in the formula for at- 
mospheric pressure if p = 24 in. when h = 5830 ft.; if p = 600 mm. 
when h = 1909 m. Hence find the barometric reading at a height of 
3000 ft. ; 1000 m. Find the height if the barometer reads 28 in. ; 650 mm. 

[Note. Pressure in pounds per square inch = 0.4908 X barometer 
reading in inches.] 

14. If a rotating wheel is stopped by water friction, the rate of de- 
crease of angular speed, dos/dt, is proportional to the speed. Find co in 
terms of the time, and find the factor of proportionality if the speed of 
the wheel diminishes 50% in one minute. 

15. If a wheel stopped by water friction has its speed reduced at a 
constant rate of 2% (in revolutions per second and seconds), how long 
will it take to lose 50% of the speed? 

16. The length Z of a rod when heated expands at a constant rate per 
cent ( = 100 k). Show that dl/dd = kly where is the temperature; if the 
percentage rate of increase is .001% (in feet and degrees C), how much 
longer will it be when heated 200° C? At what temperature will the rod 
be 1% longer than it was originally? 

[Note. This value of A; is about correct for cast iron.] 



114 THE CALCULUS [VIII, § 69 

17. The coefficient of expansion of a metal rod is the increase in 
length per degree rise in temperature of a rod of unit length. Show that 
the coefficient of expansion of any rod is the relative rate of increase in 
length with respect to the temperature. 

18. When a belt passes around a pulley, if T is the tension (in 
pounds) at a distance s (in feet) from the point where the belt leaves the 
pulley, r the radius of the pulley, and /i the coefficient of friction, then 
dt/ds = /iT/r, Express T in terms of s. If T ^ 30 lb. when a = 0, 
what is T when « = 5 ft., if r = 7 ft., and /j. = 0.3? 

19. When an electric circuit is cut off, the rate of decrease of the cur- 
rent is proportional to the current C Show that C = Coer^t where Co 
is the value of C when t — 0. 

(Note. The assumption made is that the electric pressure, or electro- 
motive force, suddenly becomes zero, the circuit remaining unbroken. 
This is approximately realized in one portion of a circuit which is 
short-circuited. The effect is due to self-induction: k = R/L, where R 
is the resistance and L the self-induction of Uie circuit.] 

20. Radium automatically decomposes at a constant (relative) rate. 
Show that the quantity remaining after a time t is q = qoe'^, where 
^0 is the original quantity. Find k from the fact that half the original 
quantity disappears in 1800 yrs. How much disappears in 100 yrs.? 
in one year? 

21. Many other chemical reactions — for example, the formation of 
invert sugar from sugar — proceed approximately in a manner similar 
to that described in Ex. 20. Show that the quantity which remains is 
q = qoer^ and that the amount transformed is A = qo — q — qQ(l ^ e"**). 
Show that the quantities which remain after a series of equal intervals 
of time are in geometric progression. 

22. The amount of light which passes through a given thickness of 
glass, or other absorbing material, is found from the fact that a fixed per 
cent of the total is absorbed by any absorbing material. Express the 
amount which will pass through a given thickness of glass. 

70. Logarithmic Differentiation. Relative Increase. In § 69 
we defined the relative rate of increase rr of a quantity y with 
respect to x as the total rate of increase {dy/dx) divided by y. 
If y is given as a function of x, 

(1) y=f(x), 



VIII, §70] LOGARITHMS 115 

the relative rate of increase 

dy 

can be obtained by taking the logarithms of both sides 
of (1),* 

(2) \0gey = \0gef{x), 

and then differentiating both sides with respect to x: 

(3) y _1 <^y ^ dlogey __ dlogef(x) 

^ ^ y' dx dx dx ' 

This process is often called logarithmic differentiation: the 
logarithmic derivative of a function is its relative rate of in- 
crease, rr, or 1/100 of its percentage rate of increase. 

Example 1. Given y = Ce**, to find n = (dy/dx) -^ y. Taking log- 
arithms on both sides: 

loge y = loge C + kx; 

differentiating both sides with respect to x, 

^' dx ' ^ dx ~^' 

The result of Ex. 3, § 68, may be restated as follows: the 
only fmiction of x whose relative rate of change (logarithmic 
derivative) is constant is Ce**. 

Example 2. Given y = x^+3x + 2,to find rr. 

Method2. rr-^^v ^ ^ x2+3x+2 ' 

* Since log N is defined only for positive values of N, aU that follows holds 
only for positive values of the quantities whose logarithms are v^ed. 

t Here and hereafter the symbol log will be used to mean a logarithm to 
the base e. 



116 THE CALCULUS [YIII, § 71 

71. Logarifhmic Methods. The process of logarithmic dif- 
ferentiation is often used apart from its meaning as a relative 
rate, simply as a device for obtaining the usual derivative. 
We shall first apply this method to prove the rule for dif- 
ferentiating any constant power of a variable. The equation 

gives 

logy = n log X. 

Differentiating with respect to x, we have 

Idy 1 

--f- = n •- 
yax X 



or 



dy y x^ 

-f- = n '-^n- — 
ax X X 

In this proof, n may be any constant whatever. (See §§ 17, 
21.) 

The logarithmic method is useful also in such examples as 
those that follow. 

Example 1. Given y = {2x^+ 3)104»-i. 
Method 1. Ordinary Differentiation. 

I = (2x2 + 3)^(104-1) +104^-1^(2 x2 + 3) 
= (2x2 + 3)-4.-^104»-i + 104«-i.4x 

= 4 . 104*-i r(2 a;2 + S)/M + xl, where M = logioe = 0.434. 

Method 2. Logarithmic Method. 

Since log y = log (2 a;2 + 3) + (4 x — 1) log 10, we have 
I dy 4x , ^ 1 in 



VIII, §71] LOGARITHMS 117 

or ^ = y[2^^ + 41ogl0] = 4.1()4i^-i[x + (2x2 + 3)logl0], 

which agrees with the preceding result, since loge 10 =.l/logioe = 1/Af. 

Example 2. Given y = {3 x^ -\- 1)^+^^ to find dy/dx. Since no rule 
has been given for a variable to a variable power, ordinary differentiation 
cannot be used advantageously. Taking logarithms, however, we find 
logy = (2 a: + 4) log (3 a;2 + 1), 

whence i • ^ = 21og (3x2 + D + -f^TT (2 a; + 4), 
y ax o a;^ -f- 1 



or 



g=(3a:2 + l)2x+4J21og(3a:2 + l)+^j^(2x + 4)[. 



The use of the logarithmic method is the only expeditious way to find 
the derivative in this example. 

EXERCISES 

Find the logarithmic derivatives (relative rates of increase) of each 
of the following functions, by each of the two methods of § 71. 

1. ^2*. 6. 0.1ei«-5. 9. (r2 + i)e-r». 

2. 4e4«. 6. 102aj+3. 10. (2 - 3 <2) eM»-i. 

3. e»+2. 7. er^Vtof'. n. (1 - f2 _j- ^) ioi'+^. 

4. ff^, 8. 2<2e-7<. 12. e^. 

Find the derivative of each of the following functions by the loga- 
rithmic method. 

13. (1 + aj)i+*. 16. x^^ 17. (1+ x) (1+ 2 x) (1+ 3 x). 

i4. («2 + 1)2*-H3. 16. if^, 18. \^rT^ ^ vTT^^. 

19. If y = uvj show that dy -i- y — du ■¥ u -^ dv -^ v. In general 
show that the relative rate of increase of a product is the sum of the 
relative rates of increase of the factors. 

20. If a rectangular sheet of metal is heated, show that the relative 
rate of increase in its area is twice the coefficient of expansion of the 
material [see Ex. 17, List XXXI]. 

21. Extend the rule of Ex. 19 to the case of any number of factors. 
Apply this to the expansion of a heated block of metal. 

22. Show directly, and also by use of Ex. 21, that the relative rate of 
increase of x** with respect to x, where n is an integer, is n/x. 



118 THE CALCULUS [VIII, § 71 

23. Compare the functions e^ and e2*+3; compare their relative 
rates of increase; compare their derivatives; compare their second 
derivatives. 

Compare the following pairs of functions, their logarithmic deriv- 
atives, their ordinary derivatives, and their second derivatives. 

24. ^ and 1(F. 27. e^ and e+<«. 

25. ^ and eo*+*. 28. ff-^ and sech x, 

26. ^ and 10**. 29. c-*' and 1 -^ (a + 6x2). 

30. Can k be found so that hff^ and 10** coincide? Prove this by- 
comparing their logarithmic derivatives, and find 6 in terms of a. 

31. If the logarithmic derivative {dy/dx) -f- y is equal to 3 + 4 x, 
show that log y = 3 x + 2x2 -f const., or y = A;e3a;+2x\ 

32. If (d2//(ir) ^y=f{x) show that y = a/^^"^^ *^- 

Find y if the logarithmic derivative has any one of the following 
values: 

33. 1 — x. 36. n/x, 37. e*. 

34. ax + bxK 86. a + n/x. 88. e* + n/x. 



CHAPTER IX 



TRIGONOMETRIC FUNCTIONS 

■ 

72. Limit of (sdn B)IB as ^ approaches Zero. To find the de- 
rivatives of sin X and cos x, we shall make use of the limit 

sin B 



lim 



B 



Let B be the angle A05, Fig. 27, and let us draw a circle 

about as center with a radius r = OA, 

cutting OB at P. Draw PP' and fi5' 

perpendicular to OA and draw OP' B'. 

Then 

(1) PP'< arc Pi4P'<BB', 
or 

(2) 2 r sin ^ < 2 r • ^ < 2 r tan ^, Fia. 27. 

since arc PAP' = 2 r • ^ if ^ is measured in circular measure. 
Dividing by 2 r sin 6, we have 

e ^ I 




(3) 



1< 



sin B cos 6 

But cos 6 approaches 1 as ^ approaches zero. Hence 
^/sin 6 must also approach 1. It follows that 



(4) 



,. sin e ^ 
hm -— = 1, 



provided, as above, that 6 is measured in circular measure.* 

*0n account of the simplicity of this formula and those that result 
from it, we shall assmne henceforth that all angles are measured m circular 
measure. 

119 



120 THE CALCULUS [IX, § 73 

73. Derivatives of sdn x and cos x. Given the equation 
(1) y = sin Xy 

we proceed to find dy/dx by the fundamental process of § 17. 
We have, using the notation of § 17, 

(A) 2/ + Ay = sin {x + Ax) 

(B) Ay = sin {x + Ax) — sin a; 

^ f , Ar\ . Ax 
= 2 cosyx + y^ sin y , 

by formula 13, Tables, II, G. Dividing both sides by Ax, 



(C) g — G + f) 



. Ax 
sm- 



Ax ' 

2 

.- Ax 

or, if we put ^ — -K- i 

Ay r X n\ sin B 

- = cos(x + ^)-^. 

Hence, by § 72, 

(D) -^ = lim -^ = cos X, 

ax tf-+o Ax 

and we have the formula 

[X] — -2 = COS X. 

ax 

Similarly, starting with y = cos x, we obtain the formula 

r«rTi d COS X 

[XI] — 5 — = — sm X. 

dx 

By means of formula VII, § 22, these formulas may be 
rewritten in the form 
.^v dsint^ dsint^ du du 

.^x d cos u __ dcost/ ^ _ _ • ^ 

dx du dx dx 



IX, § 74] TRIGONOMETRIC FUNCTIONS ' 121 

Example 1. Differentiate y = sin vT+^. 

dy dsinVl-f-a;2 r^— — grfVl+x2 x ^/3— : — 5 

-—■ = 3 = cos V 1 -h x2 = —. cos V 1 4- x2. 

dz dx dx Vl -\-x^ 

Example 2. Differentiate y = cos e^. 

dw dcose** . ^jde^' o ^ • ♦« 

3^ = — 1 = — sin e*' -J— - — 2x^ sin e**. 

dx dx dx 

74. Derivatives of tan x, ctn x, sec x, esc x. Given y = tan x, 

we may write 

jSina: dsinx . dcosa: 

J , ^ a cos X — ; sin x — 7 — ^ 

ot/ a tan a: cosx dx dx 1 



dx dx dx cos^a; cos^a: 

[^^] ^^ =7::^ai: = sec'x. 



Similarly, 



(fx cos'x 



jCOSX 

a — 



nrTTTi rfctnx sma: 1 ,^ 



rrrr^n d SeC X COS X Sm X 

[XIV] — := — = — • — = — s— = secx tanx. 

ax dx cos^ X 



r^ri d CSC X sm X — cos X . 

[XV] ^ = ; = — r-s = - CSC X Ctn X. 

dx dx 8w?x 

These may be combined with formula VII, § 22, as in § 73. 

Example 1. Differentiate y = cos^a;. 

Setting u = cos x, we have y = u^, and 

^2/ rfw3 ^ ^du _ 5 d cos x ^ „ 

j^=-3-=3w2— =3 cos* x — J — = — 3 cos2 x sin x, 
ax dx ax ax 

Example 2. Differentiate y = cos^ (2 x^ + 1). 
Setting u = cos (2 a;2 + 1), we have y = w', and 

:^=-^ ^^^ :iZ =3C0S2(2X2 + I).;;r-. 

dx dx dv dx 



122 THE CALCULUS [IX, § 74 

But 

dx- di -sin (2x2 -hi) _ 

= - 4a;sin(2a;2 + l). 
Hence 

^ = [3 cos2 (2 a;2 + 1)] [- 4 x sin (2 x2 + 1)] 
= - 12x cos2 (2x2 -h 1) sin (2x2 + 1). 

EXERCISES 

Find the derivatives of : , - 

1. sin 4 X. 5. sin x^. 9. x coe x. 

2. cos {e/Z), 6. tan (3 — 20. 10. e» ctn $, 

3. tan (— 2 ^). 7. cos (— 3 e). 11. log sec x. 

4. sin2x. 8. sec(x/2). 12. cose~*. 

13. sin X — 4 cos 2 X. 17. c* cos2 (3 « — 1). 

14. c'sin (ir/10 - 2 0- 18. ei+2< gin (3 t - ir/4). 
16. (1 -|-x2)sin(3-2x). 19. e'/io (cos < - 4 sin 3 0. 
16. logsec6s*»»*. 20. cos log tan f*. 

21. Find the area under the curve y = sin x from x = to x = 7r/2; 
test the correctness of your result by rough comparison with the cir- 
cumscribed rectangle. 

22. Find the area bounded by the two axes and the curve y = cos x, 
in the first quadrant. 

Find the maxima and minima, and the points of inflexion (if any 
exist) on each of the following curves. 

23. y = sin x. 26. y — x cos x. 29. y = e~* sin x. 

24. 2/ = cos X. 27. y = 1 — sin 2 x. 30. y = e"2« sin x. 

25. y = tan x. 28. y = sin x + cos x. 31. j/ = cos (2 x + ir/6). 

Find the derivative of each of the following pairs of functions, and 
draw conclusions concerning the functions. 

32. cos X and sin (ir/2 — x). 35. sin 2 x and 2 sin x cos x. 

33. cos2 X and 1 — sin2x. 36. cos 2 x and — 2 sin2 x, 
94, s^c ;^ and gee (— x). 37. tan2 x and sec2 ;j;^ 



IX, § 74] TRIGONOMETRIC FUNCTIONS 123 

Integrate the following expressions; in case the limits are stated, 
evaluate the integrals, and represent them graphically as areas. 

38. / sin X dx, 40. / sec^ x dx. 42. / cos (3 t + 7r/6) dt. 

/-Hr/2 ^ ^ 

cos x dx, 41. / sin 2 a; dx. 43. / tan ^ sec ^ dU 

ir/2 •/ J 



44. f (1 4- sin a;) dx. 
Jo 

45. J(co8 X 4- 3 sin 2 a;) dx. 



46. /cos^x da;. 



. Hint. 2 cos^ a; = 1 + cos 2 a;. 



47. y(cos 2 X - 1) dx. 48. /*' sin^ x dx. 

49. Find the derivative of sin x by showing that 

sin (x + Ax) — sin X = sin x (cos Ax — 1) + cos x • sin Ax 
and remarking that, as Ax-»0, 

lim[(cos Ax — 1) -5- Ax] = and Iim[(sin Ax) -5- Ax] = 1. 

60. Find the derivative of cos x as in Ex. 49. 

61. Find the derivatives of the two functions 

(a) vers x = 1 — cos x. (6) exsec x = sec x — 1. 

62. Differentiate some of the answers in the list of formulas, Tablesy 
IV, Eo, Eft. What should the result of your differentiation be? 

[The teacher will indicate which formulas should be thus tested.] 
Find the speed of a moving particle whose motion is given in terms 

of the time t by one of the pairs of parameter equations which follow; 

and find the path in each case. 



*• <a; = 3 cos 2^. __ (x = sm< 
) 2/ = 3 sm 2 ^. (y = ami. 

-. Jx = 2cos4<. _g (x=sec<. 
* J y = 3 sin 4 <. (y = tan t 



+ cos^ 



67. A flywheel 5 ft. in diameter makes 1 revolution per second. 
Find the horizontal and the vertical speed of a point on its rim 1 ft. 
above the center. 

68. A point on the rim of a flywheel of radius 5 ft. which is 3 ft. 
above the center has a horizontal speed of 20 ft. per second. Find the 
angular speed, and the total linear speed of a point on the rim. 



124 



THE CALCULUS 



[IX, § 75 



76. Simple Harmonic Motion. If a point M moves with 
constant speed in a circular path, the projection P of that 

point on any straight line is said to be 
in simple harmonic motion. 

Let the circle have a radius a; let 
the constant speed be v] and let the 
straight line be taken as the x-axis. 
We may suppose the center of the 
circle lies on the straight line, since 
the projection of the moving point on 
either of two parallel straight lines 
Let the center of the circle be the 




Fig. 28. 



has the same motion, 
origin. Then we have 

(1) X = OP = a cos ^, or x = a cos (s/^), 

where s = arc AM, since 6 = s/a. Moreover, since the 
speed V is constant, v = s/Tyii T is the time since M was at 
A; or V = s/(t — U) if t is measured from any instant what- 
ever, and to is the value of t when Af is at A. We have 
therefore 



(2) 



X = a cos - = a cos - (i — fo) = a cos [W + c]; 



where k = v/a, and € = — fcfo = — vto/a. 
From (2), the speed dx/dt of P along BA is 



(3) 



dx d[a co8(kt + e)] i * m t \ 



and the acceleration of P is 



(4) 
or, 

(5) 



3t 



dfi 



= — dk^ cos(kt + «) = — k^'Xf 



cPx 



jT-i-X — ^-i-X « ; 



IX, § 76] TRIGONOMETRIC FUNCTIONS 125 

thcU is, the acceleration of x divided by x, is a negative constant, 
— fc2. We shall see that much of the unportance of sunple 
harmonic motion arises from this fact. 

It is important to notice that (2) may be written in the 
form 

x = a cos (kt + €) = a [cos e cos kt — sin € sin kt], 

or 

(6) x = A sin kt + B cos kt, 

where A = — a sin € and S = + a cos e are both constants. 
The form (6) may be used to derive (5) directly. 

The simplest forms of the equation (6) result when fc = 1 
and either A = and 5 = 1, or A = 1 and B = 0: 

.^. fx = sin <; if fc = 1, A = 1, fi = 0, i.e. a = 1, € = 3 ir/2. 
\x = cost; if fc = 1, A = 0, B = 1, i.e. a = 1, € = 0. 

The formulas (2) and (6) are general formulas for simple har- 
monic motion; (7) represent two specially simple cases. 

76. Vibration. The importance of simple harmonic mo- 
tion, based on its property (5) of § 75, is evident in vibrating 
bodies, such as vibrating cords or wires, the prongs of a tuning 
fork, the atoms of water in a wave, a weight suspended by a 
spring. 

In all such cases, it is natural to suppose that the force 
which tends to restore the vibrating particle to its central 
position increases with the distance from that central posi- 
tion, and is proportional to that distance. (Compare 
Hooke's law in Physics.) 

It is a standard law of physics, equivalent to Newton's 
second law of motion, that the acceleration of any particle 
is proportional to the force acting upon it. 



126 THE CALCULUS [IX, § 76 

In the case of vibration, therefore, the acceleration, being 
proportional to the force, is proportional to the distance, 
Xy from the central position; it follows that, in ordinary 
vibrations, the relative acceleration is a negative constant, — 
negative, because the acceleration is opposite to the positive 
direction of motion. For this reason, each particle of a 
vibrating body is supposed to have a simple harmonic mo- 
tion, unless disturbing causes, such as air friction, enter to 
change the result. Neglecting such frictional effects tempo- 
rarily, the distance x from the central position is, as in § 75, 

X = a cos (kt + e) = A sin kt-\- B cos kt, 

where t denotes the time measured from a starting time to 
seconds before the particle is at a: = a, and where € = — tjc. 
Moreover, from § 75 and also from what precedes, 

dx^ 



dfi 



= — k^x. 



The quantity a is called the amplitude, 27r/fc is called the 
period, and to= — e/k is called the phase, of the vibration. 

EXERCISES 

Find the speed and the acceleration of a particle whose displace- 
ment X has one of the following values: compare the acceleration with 
the original expression for the displacement. 

1. a; = sin 2 ^ 6. a; = sin 2 ^ -|- 0.15 sin 6 t. 

2. X = sin {t/2 — ir/4). 6. x = sin ^ — J sin 3 ^ + i sin 5 ^ 

3. a; = sin < — } sin 2 ^ 7. a; = a sin {kt + e). 

4. X = cos t + icosSt. S. X = A cos kt -^ B sin kt 

9. Determine the angular acceleration of a hair spring if it vibrates 
according to the law 6 — .2 sin 10 irt; what is the amplitude of one 
vibration, the period and the extreme value of the acceleration? ^^ 

/ 



IX, § 76] TRIGONOMETRIC FUNCTIONS 127 

Show that each of the following functions satisfies an equation of 
the form d^u/dl^ + Aj^w ^ or d^u/dP^ — k^u = 0; in each case determine 
the value of k. 

10. w = 10 sin 2 ^ 16. w = 6 cos (t/S - ir/12). 

11. u = 0.7 cos 15 1. 16. M = 12 cos 3 ^ — 5 sin 3 <. 

12. w = 3 e^K 17. w = 3 sin 6 / + 4 cos 6 «. 

13. w = 20 e-^. 18. w = Ci sin 3 < + C2COS 3 /. 

14. w = sin (3 « + ir/3). 19. w = Cie^' + C2e-7'. 

20. Show that the function u = A sin kt-\-B cos kt always satisfies 
the equation cPu/di^ + k^u = for any values of A and B. Check by 
substituting various positive and negative values for ky Ay B. 

21. Show that u = A^ + Ber^ always satisfies the equation 



d& 



k^u = 0. 



22. When an electrical condenser discharges through a negligible re- 
sistance the current C follows the law d^C/d^ = — a^Cy where a is a con- 
stant. Express the current in terms of the time. When a = 1000, what 
is the frequency (number of alternations) per second? 

23. Any ordinary alternating electric current varies in intensity ac- 
cording to the law C = a sin kt; find the maximum current and the 
time-rate of change of the current. 

24. When a pendulum of length I swings through a small angle 9, 
its motion is represented by the equation d^d/dt^ = — gO/l, very nearly, 
I being in feet, in radians, t in seconds. Show that 

= Ci sin kt -h C2 cos kt, 

where k = ^g/L Find Ci and C2 if ^ = a and the angular speed cj 
= when t = 0; and find the time required for one full swing. 

25. A needle is suspended in a horizontal position by a torsion fila- 
ment. When the needle is turned through a small angle from its posi- 
tion of equilibrium, the torsional restoring force produces an angular 
acceleration nearly proportional to the angular displacement. Neglect- 
ing resistances, what will be the nature of the motion? 



128 THE CALCULUS [IX, § 77 

77. Inverse Trigonometric Functions. The equation 

(1) y = sm~^x, • 
is equivalent to the equation 

(2) sin y = X. 
Differentiating each side with respect to x, we find 

(3) co8j/f?=l,or^ = ^- = ^i=.. 

ax ax cos y y/\ _ ^ 

Hence we have the formula 

[XVI] ^^-'^ 1 



It is evident that the radical in these expressions should 
have the same sign as cos y, i.e, plus when y is in the first or 
in the fourth quadrant, minus when y is in the second or in 
the third quadrant. 

Combining XVI with VII, § 22, we may write 

. . s d sin~^ u 1 du 

^ dx " Vl — u^dx' 

In a similar manner, we find from formulas XI, XII, 
XIII, XIV, XV, the formulas 

[XVII] ^ ^^^"'^ - 1 



(radical + in 1st and 2d quadrants). 



[XVIII] —^ — = (all quadrants). 

'■^^^ — dx — ^ 1 I ya (^11 quadrants). 



[XX] 



d sec-^x 1 



(radical + in 1st and 3d quadrants). 



IX, § 79] TRIGONOMETRIC FUNCTIONS 129 

(fcsc-ix -1 



[XXX] 



[xxn] 



(radical + in 1st and 3d quadrants), 
tfvers~^x 1 

(radical + in 1st or 2d quadrants). 



Each of these fonnulas may be combined with VII, § 22, 
as in equation (4) above. 

78. Illustrative Examples. 

Example 1. 1 = . = : ^ = , 

dx Vl — (a;2)2 dx Vl — x* 

Example 2. 



da; 1 + (e^)2 <ic 1 + e 

Example 3. ^^ ^ = 3 (sec-i a;)2 , « 

<ic da; 

=3(8ec-ia;)2 ^ 



.2x 



a;Va;2 - 1 

T,_ . d log (cos"i a;) Id cos~i x 

Example 4. — ^-^ ^ = — -^ 3 . 

da; cos ^x dx 

1 - 1 



cos~i X Vl — a;2 

79. Integrals of Irrational Functions. By reversal of the 
formulas for the derivatives of the inverse trigonometric 
functions, XVI-XXII, we obtain the integrals of certain 
important irrational functions. 

dx . , . ^ . dsin~*x 1_ 

X' 



[XVIji I .- -_ = sm^ X + C, smce — 3 = , 

J V 1 - JC cte VI — 



dx ^ ;„ , ri -:>..- d tan-^ a; _ 1 



[XVn],- r ^ . ^^a = ta»~* JC + C, since 



2> 



130 THE CALCULUS [IX, § 79 



since - 



[XX]/ J ^^l—-^ = sec-^x + C, si] 

[xxn],J 



(fo a; Vx^ — 1 ' 

</x , . ^ • d vers"* a: 1 

/^ o = vers~i X + C, since — ^ = > , 

V2x-x» ctr V2x-a:2' 

where C in each case denotes an arbitrary constant. Since 
&in~* X + cos~* X = 7r/2, the student may show that [XVII] 
leads to the same result as [XVI]. 

Example. To find the area under the curve j/ = 1/(1 + a;2) from 
the point where x = to the point where a; = 1. 

Since A =fydx,we have 

= / T-r-^dx = tan-i x\ = -r/4 - = 7r/4. 
x=-0 ^x=0 l+iC'* Jx=0 

The fact that we are using radian measure far angles appears very 
prominently here. Draw the curve (by first drawing y = 1 -|- a;2) on a 
large scale on millimeter paper and actually count the gmall squares as a 
check on this result. 

EXERCISES 

Differentiate each of the following functions. 

1. sin~i x/^, 6. sin~i Vl — x^, 9. log tan~i x, 

2. cos~i (1 — x). 6. a; sin~i x. 10. cos"i {xe^). 

3. sin-i (i/a;). 7. tan"! (l/x^). 11. x^ tan'i 2Vi- 

4. tan-i (3 a;). 8. c* cos~i x, 12. sec-^aJ^ + !)• 

13. csc-i VrT^2. 17. cos-i Vl - x2. 21. (log tan-i a;)3. 

14. ctn-i (|-i^y 18. sec-i Gog tan a;). 22. ^^j^- 
16. cos-i (e"*"^). 19- e^^~^^. 23. ^"^ ^ 



a; 



-1. 



16. tan-i (log e*). 20. 10 ^ \ 



IX, § 79] TRIGONOMETRIC FUNCTIONS 131 

Integrate the following functions; in case limits are staited, evaluate 
the integral. 

Jo l+a;2 '*'• Ji 



eV^-l 



dt ^^ r dx 



26. f -j^=' 28. f:r^7-2' [Sett* = 2x.] 

^1/2 Vl — ^ J l+4a;2 

26. f^'r^' 29. r , ^ ♦ [Setti=2a:.] 



Integrate after making the change of letters u = 1 — x. 

dx ^^ r dx m^ r dx 



«»• f^,-n-.W '*• f i + a-x)^ - **• / 



Vl - (1 - a;)2 * J IH- (1 - a;)2 'J V2 x - x* 

Find the areas between the x-axis and each of the following curves, 
between the limits stated. 

33. 2/2 = 1-1- a;2y2; a; == to X = 1/2; a; = - 1/2 to x = + 1/2. 

34. 2/ + ^^y = l;ic = Otoa; = l;x=Otoa;=a. 

36. 2/2 = 1 ^_ 4 x'iy^; a; = to x = 1/4; x = - 1/4 to x = + 1/4. 

36. 4 x22/ + 2/ + 1 = 0; X = 1 to X = 2; X = - 1 to X = 4- 1. 

37. Show that the derivative of tan-i[(c* — e-*)/2] is 2/(e* +6"*). 
[Note. The function tan"i[(e* — e~*)/2], or tan"i (ginh x), is called 

the Giidermannian of x and is denoted by j^cf x: gdx = tan'i (sinh x). 
It follows from this exercise that d gd x/dx = sech x.] 

38. From the fact that d (sinh x) = cosh x c2x, show that the deriv- 
ative of the inverse hyperbolic sine (x = sinh"! t^ if t^ = ginh x) is 

given by the equation d (sinh"! w) = ± du/ Vl + v^. [See foot of 
p. 108.] 

39. Show that d cosh"! u =± du/ \/w2 — 1. 

40. Show that d tanh"! u = du/{l - w2). 




132 THE CALCULUS [IX, § 80 

80. Collection of Formulas for Differentiation. For convenience 
in reference we shall restate all of the formulas for differen- 
tiation, combining each of them with [VII] when it is de- 
sirable to do so. 

- (fc ^ „ dC'U du 

dJU_+V)^dU dv^ dun^ du 

dx dx dx dx dx 

X*,, dx dx __- duv dv , du 

V- -^ ^ — VI. _=„^+„^. 

Vii. $^ = ^-^- Vila. ^ = $^^^ 

dx du dx dx dt dt 

,^ dB" y> . n du --- rfe« du 

n. _ = 5-logB.^. IXa. ^ = e.^^. 

X. _^ = co8«^. XI. -^ = -8m«^. 

XIL ^ = sec«ug. Xin. ^ = -csc««g. 

XIV. — J — = seciitanii^-- XV. — ^ — = — csciictnu j-- 
dx dx dx dx 

±1 du 



XX XXI tfj8^c-'"U ±1 



±1 du 
~^dx 



du 
dx 



XXII. jT vers * u = . 3- 

dx V2u-u*o« 



CHAPTER X 



APPLICATIONS TO CURVES 
LENGTH — CURVATURE 

81. Introduction. The formulas obtained in Chapters VIII 
and IX make possible many new applications to curves. 
We shall treat some of these in this Chapter. 

82. Length of an Arc of a Curve. Let s (x) denote the length 
of the arc of a given curve y =/(x), from a fixed point F 
to a variable point P. 

When X increases by ^ 

an amount Ax, let 
As = arc PQ be the 
corresponding increase 
in s, and let Ac = chord 
PQ. Then 

(1) Ac^ = Ax^ + A^^ 
whence 



and 
(3) 




x^x^Lx 



As 

Ax 



'^hM-t 



We now require the following fundamental axiom, which 
forms the basis of the mensuration of curved lines. 

As the chord and its arc approach zero, their ratio approadies 
1, i.e. 

(4) 

133 



lim T- = 1. 
Ac-*oAc 



134 THE CALCULUS [X, § 82 

Combining (3) and (4), and passing to the limit as Ax 
approaches zero, we have 

where m = dy/dx is the slope of the curve. 

It follows that the total change in s between any two 
fixed points x = a and x = 6, is 

(6) Total length = si ' ° * = /" ° Vl + m* dx. 

83. Parameter Forms. When the equation of a curve is 
given in parameter form 

(1) x=f(t), y = <t>(t), 

we may square both sides of (5), § 82, and multiply by dx^. 
This gives the formula 

(2) c/s« = c/x» + dy*, 

which is called the Pythagorean differential formula. It is 
readily remembered by reference to the triangle PQR, 
Fig. 29. If we divide both sides of (2) by dt^, we find * 

») ©'- ey+ ©' 

From (3) we have 

whence 

whicn gives the length of the curve (1) between any two of 
its points. 

* This expresses the fact that the square of the total speed ds/dt is the 
sum of the squares of the horizontal speed dx/dt and the vertical speed dy/dt. 
This fact, proved in § 40, might have been used as the point of departure, 
and all of the formula? of %\ 82-83 might have been deduced from it. 



X, § 84] APPLICATIONS TO CURVES 13 J 

84. Illustrative Examples. While the square root which 
occurs in the formulas of §§ 82-83 renders the integrations 
rather difficult in general, the work is quite easy in some 
examples, as illustrated below. 

Example 1. Find the length of the curve y^ = x^ from the origin 
to the point where x —h. 

From 2^ = x3 we find y = »8/2^ whence 

and 

335 



•]:::-jrV'^¥-i('+?-n::- 



27 



8 



Example 2. Find the length of the catenary (§ 67) 

» = — 2- 

from the origin to the point where x ^\. 
We find immediately 

dx 2' da;VV2//' 

which reduces algebraically to the form 

ds ^ / ggg -f- 2 + e"^ V^^ _ e^ + g"^ 
dx \ ^ J 2 ' 

hence 

^ (2.718-0,368) ^ ^^^^ (^^^^jy^ 

Compare § 67, and Tables III, E, and V, C. 

Example 3. Find the length of one arch of the cycloid (Tables 

III, G). 

a; = a (< — sin 0, y = a (1 — cos Q. 
We find 

cte = (a — a cos ^i dy = o sin t dty 

d8= Vdx'^ + dy^ = a V2 - 2 cos < d« = 2 a sin|d<, 
whence 

= 1 2 a sin 7i d< = — 4 a cos « I = — 4 a [cos x — cos 0] 
i«o Jo 2 2jo 

= -4a[-l-l] =8a. 



136 THE CALCULUS [X, § 84 

EXERCISES 

Determine by integration the lengths of the following curves, each 
between the limits x = ltoa; = 2, x=2tox=4, x=atoa; = 6. 
Check the first three geometrically. 

1. y = 3 X - 1. Z. y ^mx+c. 6. y = J (2 x - 1)V2. 

2. y = 3 +2x. 4. 2/ = f (x - 1)V2. 6. y = i (4x - 1)V2. 

Find da, the speed v, and the length s of the path of each of the follow- 
ing motions, between the given limits. 

7. x = l+^, y = l-^;^ = 0to< = 2. 

8. X = (1 + 0V2, y = (1 - t)y^; t = to t ^ 1. 

9. X = (1 - 0^ y = 8 ^/2/3; < = to < = 9. 

10. X = 1 + ^2, y = < ~ ^/3; < = to < = 5. 

11. X = 2A y = t + 1/(3 ^3); ^ = a to ^ = 6. 

12. Find the length of the cycloid (Ex. 3, § 84) for half of one arch, 
i.e., from ( = to < = ir; for the portion from < = to < = ir/2; from 
< = to « = t/3. 

18. Show that the element of length for the cardioid (Tables III, G4) 

X = 2 a cos ^ — a cos 2 d, y = 2 a sin ^ — a sin 2 ^, 
is 

d« = 2a[2-2 (cos2 dcos $ + sin 2 dsin e)]^/^de = 2a (2-2 cos 6) ^^dB, 

Hence show that the entire length of the cardioid, from ^ = to 
d = 2 IT is 16 a. Show that the^length of the part of the cardioid from 
d = 0tod = ir/2is4a(2~ V2). 

14. The equation of a circle about the orjgin may be replaced by 
the parameter equations 

X = o cos ^, y = a sin ^, 

where a is the radius. Hence find by integration the length of the entire 
circumference. 

16. Show that the element of length of the four-cusped hypocycloid 

(Tables III, Ge) 

X = a cos' By y = a sin' ^, 

is (is == 3 a sin ^ cos 9 (29 = I a sin 2 d (29. 

Hence show that the length of one quarter of this curve is 3 a/2. 



X, §85] 



APPLICATIONS TO CURVES 



137 



16. Show that the length of the general catenary 



y = 



2a 



y 



y'-fix) 



from the origin to any point x = x is (e^ — e"**)/2 a. 

17. Writing the equation of the simple catenary in the form used 
in § 67, y = cosh a;, show that its length between the origin and any 
point X = XyVa sinh x. 

85. Areas of Surfaces of Revolution. Consider the surface 
generated when the arc 
KL of the curve 

(1) 2/=/(x) 
(Fig. 30) revolves about 
the X-axis. Let us denote 
by S{x) the area of the 
surface generated by the 
arc KP, and by AS the area 
of the surface generated by the arc PQ = As. If the curve 
rises from P to Q we may write, with entire accuracy, 

(2) 2^^y^s<^S<2'K{y + ^y) As. 

Hence, dividing by Ax and passing to the limit, we may write 








Fia. 30. 



(3) 



S = '"S— 'Nl' + (g; 



whence the area of the surface of revolution from x = a to 
a; = 6 is 

«' ^]:::=r-'.^-r'->Rir'"- 

Similarly, if the curve is revolved about the 2/-axis, the 
area between y = c and y = dis 

ds 



(5) -S 



]:::-r-'i*-r-»>KW*- 



138 



THE CALCULUS 



[X, §85 



Finally, if the equation of the curve is written in parameter 
form 

a;=/(0, y = <t>(.t), 

we divide (2) by At, and let At approach zero, obtaining 
dS 



(30 



dt 



-^'»|-^'W(I)'+(I)' «83.) 



Hence the area of the surface of revolution formed by 
revolving the curve about the x-axis, between points at 
which t = ^1, and < = fe, is 



(6) 



S 



];>r-»-=r-»^(S)'+©'- 



A similar formula can be written if the revolution is about 
the t/-axis. 

Example 1. Find the surface of the cone generated when the seg- 

ment of the straight line y = x — 2 from 
^ a; = 2tox = 5 revolves about the x-axis. 




S 



dx 



Fig. 31. 



= y^ 2 IT (x - 2) VTTTdx 
= 2 TrV2f (x — 2)dx 

.2;V2(f-2x)J=9,v^ 



Qieck this solution by finding the area of this cone by elementary 
geometry. 

Example 2. Find the area of the surface generated when the seg- 
ment of the curve whose parameter equations are 

a:=i(4« + l)3/2, y = «2+5 
between t » 1 and ^ = 2 is rotated about the o^-axis. 



X, § 86] APPLICATIONS TO CURVES 139 



(fo2 =(ir2H-d2/2 = (4 < + 1+4^) d^ = (2^ + 1)2 («2 
2iryds =2ir f {ti-\-5)(2t + l)dt 

1-1 •/! 

"^'[^■^^■^^^^"^^ <]^= 2 T [40| - lOf] = 5»| T. 

EXERCISES 

Find the area of the surface generated by each of the following 
lines when revolved about the x-axis, from x = 1 to x = 2; from 
X = 2 to x = 4; from x = a to x = 6. 

1. 2/ = 2x-l. 2. 2/ = 3+4x. 3. y = 3x+2. 

Find the area of the surface generated by each of the following 
curves when revolved about the x-axis, between the limits indicated. 

4. y = Vl — x2; x = to x = 1; x = } to x = 1. 



5. y = V4 x--x2; x=0tox=4; x = ltox = 3. 

6. 2/ = V7 -f 6 X — x2; x = — ltox = 7; x = 2tox=5. 

7. Find the area of the surface generated by rotating the arc of the 
catenary 

» = — 2— 
about the x-axis, between the points where x = and x = 1. 

8. Find the area of the siu^ace generated by rotating the arc of the 
curve whose parameter equations are x = 8 ^/2/3, y = (i — ^)2 about 
the X-axis, between the points where t = and t = 1, 

9. Find the area of the surface generated by the arc of the curve 

2 
whose parameter equations are 3? = 7 , y = t-\-l/(Sfi) about the 

ovaxis between the points where ^ = 1 and t = 2, 

86. Curvature. A very important concept for any plane 
curve is its rate of bending, or curvature. 
The.^exion(§39,p. 61), 

(1) b = -^^ 



140 



THE CALCULUS 



[X, § 86 



is not a satisfactory measure of the bending; since it evidently 
depends upon the choice of axes, and changes when the axes 
are rotated, for example. 

If we consider the rate of 
change of the inclination of the 
tangent, a = tan~im, with respect 
to the length of arc s, that is, 

AcK da 




(2) 



A9->oAs as 



Fia. 32. 



it is evident that we have a 
measure of bending which does 
not depend on the choice of axes, since Aa and As are the 
same, even though the axes are moved about arbitrarily, or, 
indeed, before any axes are drawn. The quantity da/ds is 
called the curvature of the curve at the point P, and is de- 
noted by the letter K: the curvature is the instantaneous rate 
of change of a per unit length of arc. 

Since a = tan~i ^^ gj^d since ds^ = dx^ + dy^ (§ 83, p. 134), 

we have, 

1 



da=s d tan~i m = 



dm, ds = Vl + m^ dx, 



l + m2 
where m = dy/dx; hence the curvature K is 

1 , dm 

(3) V _da 1 + m 






T,dm 



2 



Vl+m^dx 



dx 
(1 + m^)«/^ 



(1 + m«)»/«' 



where 6 = d^y/dx^ (= flexion), and m = dy/dx (= slope). It 
appears therefore that the flexion 6 when multiplied by the 
corrective factor 1/(1 + m2)3/2 gives a satisfactory measure 
of the bending, since K is independent of the choice of 



axes. 



X, § 86] 



APPLICATIONS TO CURVES 



141 



The reciprocal of K grows larger as the curve becomes 
flatter; it is called the radius of curvaturey and is denoted 
by the letter iZ: 

(4) ^ = -K-t-^^^^' 

It should be noticed that this concept agrees with the ele- 
mentary concept of radius 
in the case of 
since As = rAa 
circle of radius r. Hence 
ds/da = r. 

Substituting the values 

of 6 and m, formulas (3) 

and (4) may be written in 

the forms 

cPy 



a circlej 
in any 



(5) K = 



dx^ 



[ 



1 + 



/dyY-|8/2' 




\dx/ J 



Fig. 33. 



(6) 



R = 



b + m" 



dx^ 



It is preferable, however, to calculate m and 6 first, and 
then substitute these values in (3) and (4). 

Since vT+rn^ = g^^ ^^ the formulas may also be written 
in the form K = 1/R = b cos^ a. 

It is usual to consider only the numerical values of K, that 
is \K\, without regard to sign. Since K and b have the 
same sign, the value of K given by (3) will be negative when 
& is negative, i.e. when the curve is concave downwards 
(§ 41, p. 65). The same remarks apply to R, since R = 1/K. 



142 



THE CALCULUS 



K §87 



87. Center of Curvature. Evolute of a Curve. The center of 

curvature Q of a curve, corre- 
sponding to a point P on that 
curve, is obtained by drawing 
the normal to the curve at P 
and laying off the distance R 
(the radius of curvature) along 
this normal from P toward the 
concave side of the curve. Thus, 
in Fig. 34, denoting the co- 
ordinates of P by (x, y), and 
those of Q by (a, j8), we have 

(1) a= OB = OA - BA = X - R sin 0, 

(2) p = BQ = AP + CQ = y + /2cos0, 

where <t> is the angle which the tangent PT makes with the 
X-axis, 

(3) 
whence 

(4) 




_^ _dy 



tan = m = 



dx' 



sm0 = 



m 



Vl + m2 ' 
It follows that we may write 

(5) a = x-'"(*+'"*> 

where 



COS0 = 



y/l + nfi 



= y + 



1 + m* 



b ' ^ - ^ b ' 

m = dy/dx, h = d!^y/dx^. 
As the point P moves along the given curve, the point Q 
also describes a curve, which is called the evolute of the 
given curve. The parameter equations of the evolute are 
precisely the equations (5), in which (a, j8) are the variable 
coordinates of the point on the evolute, x is a parameter, and 
2/ is to be replaced by its value in terms of x from the equa- 
tion of the given curve. 



X, § 87] 



APPLICATIONS TO CURVES 



143 



In particular examples, it is possible to eliminate the 
parameter x between the 
two equations (5) after 
having substituted for i/, 
/n, and 6 their values 
found from the equation 
of the given curve. This 
gives the equation of the 
evolute as a single equa- 
tion between the variables 
a and j3. 

Example 1. Find the values of K, Rj a, /3, and find the equation 
of the evolute for the curve y = x^/4. 
Here m = x/2, b = 1/2. Hence 

1/2 4 




iC = 



(1 H- a;2/4) 3/2 (4 + a;2)8/2 ' 



jy 1 (4 -f x2)3/2 

^^K 4 

a; 1 -f gV4 
**"* 2 1/2 ' 



4 ' 



/5 = y + 



1 + gV4 _a:2 



:i. 4-2 4-— = 
4 ^ ^2 



x^ 3x2 



+ 2. 



1/2 4 • " • 2 4 

EUminating x between the last two equations, we find the equation 
of the evolute in the variables a and fi, 

27 a2 =4(/3-2)3. 

Example 2. Find the values of K^ R/a, fi, and the parameter 
equations of the evolute for the cycloid 

x = cr (^ — sin ^), y = a (1 — cos $), 



dx dx/d e a (1 



a sin d .6 

cos d) 2 ' 



- 1 



\K\ = 



dx dx/d e o (1 - cos ^)2 
-1 



4 a sin^ ^ 



-o+^-r 



sin^^ 
1 



4 a Sin ^ 



144 



THE CALCULUS 



[X, § S7 






4 a sm ^ , 



e 



^l+ctn2^ 
sin e) + ctn = ^ = a (^ + sin e), 



4 a sin* ^ 



l+ctn2| 
fi = a(l — CO8 0) j = — a (1 — cos d). , 



4 a sin* ^ 



Cycloid 




Fig. 36. 

These equations for a and fi are the parameter equations of the 
evolute; they represent a new cycloid, similar to the given one, but 
situated as shown in Fig. 36. 

EXERCISES 

Calculate X, i2, a, fi for each of the following curves; sketch the curve 
and its evolute: 
, 1. y — x^, 2. y = sc^. 3. y2 = 4 qx, 

4. xy — a2. 6. 2/ = sin X. 6. y = e^. 

7. y = (e* -f 6-«)/2 = cosh x. 8. y = (e* - e^)/2 = sinh x. 

9. x2/a2 4. y2/52 = 1. 10. x2/a2 - 2/2/62 = 1. 

11. Vx + V^ = Vo. 12. x2/3 + 2/2/3 = ^2/3, 

J- J -, = a cos' df 



13. 



16. 



19. 



j a? = a cos ^, 

< y = a sin d. 
(x = <2, 

ly = t-fi/Z, 
(x = 2 + 3^, 
ly^fi-i. 



14. j^^f ^' 16. j^ = «^! 

/ 2/ = 2 cos ^. / y = a si 

17. j* = y*' 18. ^^ = 

20. j* = *'.'«' -^ 
(y = sm < — 



sin' e. 
= sec tf 
tan ^. 
+ < sin <, 

t COS ^ 



X, § 89] APPLICATIONS TO CURVES 145 

88. Properties of the Evolute. If the point P (x, y) lies 
on a curve y = / (x), and the point Q (a, 0) is the correspond- 
ing point of the evolute, we have 

m + m^ ^ , l + rn? 
a = x ^ — , j8 = yH ^ 

Let m' be the slope of the evolute at Q; then 

da da/dx 
But we have 

dp , 6-2 w6 - (1 + m2) db/dx 
di = ^ + p 

3mb^-(l+ Tffi) db/dx 

da __ b (1 + 3 nfi) & -- (m + m^) db/dx 
dx~~ 62 

__ ~ 3 m262 + (^ + ^^) db/dx 
" P 

It follows that 

doL m 

Hence the normal to the curve at P is the tangent to its 
evolute at Q. Hence the radius of curvature of the curve 
at C is tangent to the evolute at Q. (See Fig. 35.) 

89. Length of the Evolute. As Q moves along on the evo- 
lute, the rate of change of R is the rate of change of the arc 
of the evolute. For, since we have, in Fig. 34, 

(1) /22 = Pq2=(^_«)2+(2,_^)2, 

it follows that 

(2) fi d/2 = (x - a) (dx - del) + (y - fi) (dy - dfi). 

But we have 

m = ^ = - |3-|> or (x-a)dx+(y'- 0) dy = 0. 



146 THE CALCULUS [X, § 89 

Hence (2) may be written in the form 

(3) dR = (^ -oQda+jy- jyd fi^ 

V(x - «)2 + (j/ - ^)2 
By § 88, we have 

da m X — a 

Substituting this in (3), we find 

da-\-y^dfi da + ^dfi 

(4) dR , '^ " = I . - = Vdcfi+d0^. 



>i'+c^fy >!'+©' 



This result, however, is precisely ds, where s is the length of 
the arc of the evolute. Hence we have 

dR = \ ds, or R2 — Ri = S2 — Sii 

R = Ri ./«-«i 

that is: the rate of growth of the radius of curvature is equal 
to the rate of growth of the arc of the evolute; and the 
difference between two radii of curvature is the same as the 
length of the arc of the evolute which separates them. 

This fact gives rise to an interesting method of drawing 
the original curve (the involute) from the evolute: Imagine 
a string wound along the convex portion of the evolute, 
fastened at some point (say Q, Fig. 35, p. 143) and then 
stretched taut. If a pencil is inserted at any point (say P, 
Fig. 35) in the string, the pencil will traverse the involute as 
the string, still held taut, is unwound from the evolute. 

As exercises, the lengths of the portions of the evolutes 
of curves given in the preceding list of exercises may be 
found. 



CHAPTER XI 



P =/(<?). 



POLAR COORDINATES 

90. Introduction. Since the equations of curves in polar 
coordinates often involve trigonometric functions, the equa- 
tions of curves have been written in rectangular coordinates 
throughout the earlier part of this book. We shall now 
show how to extend many of the results already foimd for 
curves whose equations are written in rectangular coordinates 
to curves whose equations are written in polar coordinates. 

91. Ani^e between Radius Vector and Tangent Let C 
(Fig. 37) be a curve whose equation in polar coordinates is 

(1) 

Consider the angle ^ 

between the radius 

vector OPR and the 

tangent PT to C at 

P. Let Q be a 

second point on C, 

with coordinates 

p + Ap> + A^, and ^^ ^^ 

let be the angle 

between the radius vector OQD and the secant PQS. As Ad 

approaches zero, i,e, as Q approaches P along C, we shall 

have 




(2) 



}p = lim 0, and tan yp = lim tan 0. 

147 



148 



THE CALCULUS 



[XI, § 91 



Draw AP perpendicular to OQ; then we shall have 

AP AP psm^e 



(3) tan 4> = 
and 



AQ OQ - OA 



(4) tan \[/ = lim 



p sin Ad 



p + Ap — p cos A^ 
p sin A^ 



= lim 



A^->op + Ap— pcosA^ A«->op(l — cos A^) +Ap 

To evaluate this limit, divide both numerator and de- 
nominator by A^ and note that 



(5) 
and 

(6) 



,. sin A^ ^ 



2 sm2 — - 

,. 1 — cos A^ ,. ^ 

lim T-z = lim — T-^ — 

^-»0 Au Ad-»0 i^" 



lim 



. A^" 
. A^ ^^^ -2 
«^^2'"Ar" 



= 01 = 0. 



It follows that 



sin Ad 






(7) 


tan^ = 


= lim — 
P' 


1 — cog 
A^ 




Ap 
A0 


P 
dp 

d0 


and therefore 












(8) 




tanyf/ = 


p d^ 
dp ^dp 
de 







The angle a between the a>axis and the tangent PT can 
be found, after ^ has been found, by means of the relation 



(9) 



a=« + ^. 



XI, § 91] POLAR COORDINATES 149 

ExASfPLE 1. Given the curve p = e*, to find tan ^, and ^ itself. 

Since p = e^, dp Id = efiy and tan ^ = p -s- {dp/d d) = \. Hence 
^ = tan~i 1 = ir/4 = 45°. It follows that this curve cuts every radius 
vector at the fixed angle of 45°. 

Example 2. Given the curve p = sin 2 ^, find ^ at the point where 

e = gr/8. 

tan ^ = p -r- {dp/d ^) = sin 2 ^ -r- 2 cos 2 d = (1/2) tan 2 6. 
When e = gr/8, tan ^ = 1/2, and ^ = 26° 34', approximately. 

EXERCISES 

Plot each of the following curves in polar coordinates; find the value 
of tan ^ in general, and the value of ^ in degrees when = 0, t/6, 

x/4, ir/2, TT, 

1. p = 4 sin 0. ft. p = 0. 11. p = sin 3 0. 

2. p = 6 cos — 5. 7. p = ^. 12. p = 2 cos 3 0. 

3. p=3 + 4cos0. 8. p = l/0. 13. p = 3sin(3d + 2T/3). 

4. p = tan e, 9. p = e^^. 14. p = 3 cos d -|- 4 sin (?. 
6. p = 2 + tan2 ^. 10. p = e^**. 16. p = 2/(1 - cos e), 

16. Show that tan ^ is constant for the curve p = A;e^. 
Find tan ^ for each of the following curves: 

17. p = p/(l — e cos d) (conic). 19. p = a (1 + cos 6) (cardioid). 

18. p = o sec d ± 6 (conchoid). 20. p2 = 2 a^ cos 2 ^ (lemniscate). 

92. Areas in Polar Coordinates. Let KL be an arc of a 
curve whose equation in polar coordinates is 

(1) P=/W. 

Consider first the area of the sector OKP bounded by the 
radius vector OK, for which B = d\, any other radius vector 
OP for which 6 =^ B, and the intercepted arc KP of the 
curve. The area is a function of the angle 6) let us denote 
itbyil(^). 



150 



THE CALCULUS 



[XI, § 92 






Now let increase by an amount A^ = Z POQ, and let 
PS and TQ be circular arcs whose radii are p ( = OP) and 
p + Ap (= OQ), respectively. Then we shall have 

(2) sector POS < sector POQ < sector TOQ, 

if p increases with 6. If p 
decreases when increases, 
the inequality signs must 
be reversed in (2) and in 
what follows. 

The area of any circular 
sector is equal to half the 
product of the angle (in 
circular measure) and the 
square of the radius. The 
sector POQ is the amount 
of increase in the area A ; 
let us call it A A (6) . Then 




Fig. 38. 



(2) becomes 

(3) 



p2A^ 



<Ail(^)< 



(p + Ap)2A^ 



Dividing through by A^, we have 

(4) 
whence 

(5) 



P^ AAjS) (p + Ap)2 
2 ^ A^ ^ 2 



lim 



AA(e) pf 

2 



dA 



= TT , or 



2 



A^ 2 ' ^* do 

It follows that the area of the sector bounded by the 
curve and the radii vectores for which d = di, and d = $2, 
respectively, is given by the formula 



(6) 






J< 



P^dS. 



XI, § 92] 



POLAR COORDINATES 



151 



Example 1. Find the area of the sector bounded by the curve 
p — \/.e and by the radii corresponding to 6 — t/3 and — t/2. 

The curve may be plotted readily by taking corresponding values of 
p and By as in the following table. 



e 





ir/6 


ir/3 


ir/2 


2ir/3 


5ir/6 


IT 


etc. 


p 


00 


1.91 


0.95 


0.64 


0.47 


0.38 


0.32 


etc. 



The required area is 




Fig. 39. 



-l-K 

-c(-r-(i)"'] 

= ;5^ = 0.16+. 

Example 2. Find the area 
of the sector bounded by the 
curve p = tan d, and by the 
radii corresponding to ^ = 45° 
and e = 60°. 

netf* 1 yT/3 1 yT/3 1 yr/S , . 

J45*> 2Jt/4 2Jt/4 2 Jt/4 

=i (tan <? - (?) I^J' =i [(V3 - ir/3) - (1 - t/4)] 
= 5 ( >/3 - 1 - x/12) = .2351 + 

EXERCISES 

Calculate the area formed by each of the following curves and tlie 
indicated radii, and check graphically. 
1. p = ^; d = to T. 2. p = 6/^; ^ = x/3 to gr/2. 

3. p = VS; d = T to 2 T. 4. p = -j^?; « = to 2 T. 

6. p = 4:/\l'e\ ^ = ir/8 to IT. 6. p = 1 + V^; = x/4 to ir. 

7. p = Vr+7; d = 1 to 3. 8. p = Vl + ^; d = to 3. 



152 



THE CALCULUS 



[XI, § 93 



9. p = (^ - 1)2; ^ = 1 to 6. 10. p = (1 + e)l^\ e = 180° to 360** 

11. p = sin ^; ^ = to x/2. 12. p = cos ^; ^ = x to 2 ir. 

13. p = sec e\ e = 7r/4 to ir/3. 14. p = 1 + sin ^; ^ = to x/2. 

Find the area bounded by each of the following curves: 

16. p = 4 cos d. 16. p = 4 cos 2 d. 

17. p2 = 4 cos 2e. 18. p = 1 — sin e. 

93. Lengths of Curves in Polar Coordinates. Let the equa- 
tion of a curve in polar coordinates b^ 

(1) p =/(«). 

and let s denote the length of arc from a fixed point X to a 
variable point P. Then s is a function of d. We shall show 



AS 




K{e=-k) 



Fig. 40. 



(2) 

we find 

(3) 



As _ As 
A^~ Ac 



first how to obtain ds/d$, 
whence we may proceed to 
find s itself by an integration. 
Let the coordinates of P be 
(p, 6), and those of a second 
point Q be (p + Ap, 6 + A^). 
Denote the arc PQ by A^, and 
the chord PQ by Ac. Then 
from the identity 

Ac 
' A^ 



^ = lim^! = lim^.f^ = limf?. See (4), §82. 

A^ A«-*o A^ 



dd Afl-ToA^ Ad^oAc 
From the law of cosines, 

Ac= Vp2 + (p + Ap)2 - 2p (p + Ap) cos A^ 

= •v^2(p2 + pA p) (1 - cos A^) + V. 

It follows that 

U^ ^^ L 2 _i_ A ^ 2( 1 - cos A^) /Ap\2 



XI, § 93] 



POLAR COORDINATES 



153 



But we have * 



(5) 



lim 



2(1 - COS Ad) 



1 and lim -A = -^ 
A->o A^ dS 



Hence, by (3) and (4), 

Integrating both sides of equation (6) with respect to 6, 
we find the important formula 



(7) 



5 



»; 




Fig. 41 



Equation (6) may be supplied 
by squaring both sides and then 
multiplying both sides by {dsy. 
The resulting formula 

(8) d^ = p^d0 + dp^ 

is the P3rthagorean differential 
formula in polar coordinates. 
(See § 83.) 

Example. Find the length of the curve p = 1 — cos d. 

dp = sin dd9. 

ds/de = V((fp/(|gp + p^. 

= Vsin^ 5 + (1 - cos ^)2. 

= V2 (1 - cos e) = 2 sin {e/2). 
The complete curve is traced when varies from to 2 t. 
Hence 

]2t y2T . , . ^ ^n2T 

= / 2 sin {e/2) de = -4 cos^ = 8. 
Jo ^Jo 

. * See and compare (6), p. 148. In this case we have 

2 (1 - cos Ag) 4 sin« Y / sm y 



A9> 



A0» 






154 THE CALCULUS [XI, § 94 

EXERCISES 

Find the length of each of the following curves, or of the portion 
specified. 

1. p = 5 sin ^. 6. p = o CSC e; = 45** to 90**. 

2. p = 3 cos 0. 7. p — Bin + COB 0; ^ to w, 

3. p = 6«; ^ = to t/2. 8. log p = ^; ^ « 2 to 3. 

4. p = ea«; ^ = to X. 9. log p = 3 + 2 d; tf = to 1. 
6. p = sec ^; ^ = } to 1. 10. p = 1 + sin 0, 

94. Curvature in Polar Coordinates. By the definition of 
the cxirvature K of any curve (§86), we have 

^^ Js" ds/do' 

Since a = ^ + ^ (§ 91), we have da/dS =1 + #/d^. De- 
noting dp/ do by p' and d^p/dS^ by p", we have 



(2) ^^ = tan-i _e^ ^ 

P 



/Q\ d^ __ ^ . ^^_i P^ 1 _d / P\ 

^^^ d^ "" de ^^"^ p' ~ 1 + (p/p02 ' ds \p7 

_ 1 p'' - PP'' ^ p'' - PP" 

i + (p/p02' p'^ f^+p'^ ' 

It follows that 

m d« 1 , # 1 , P^^-P/^ p2 + 2p^^-pp^^ 

Also, from (6), §93, 

(5) 1=^^+^ 

Hence we have 

/AN j^_da/dg_ p» + 2p^»-pp" 

^^^ ds/d^ "" [p* + p;*i'/* * 

Example 1. Find the curvature for any point on the curve p = e^^. 
Since p' = dp/d0 = 2 f2e, and p" = cPp/d^ = 4 e^», we have 



K = 



(e4<? 4- 4 e4<?)3/2 .^^2* 



XI, § 94] POLAR COORDINATES 155 

Example 2. Find the curvature at any point of the circle p = a sin ^. 

Here we find p' =^ a cos e, and p" — — a sin B. Therefore 

^ fl^ sin2 g -f 2 gg cos^ B -\- a^ sin^ g 

(a2 sin2 ^ + a2 cos2 ^)V2 
^ 2 02 (sin2 g -f C082 g) ^2 
a3 (sin2 ^ + cos2 ^)3/2 a* 

This is the reciprocal of the radius. (§ 86.) 

EXERCISES 

Find the radius of curvature of each of the following curves: 

1. p = 6?. 4. p = cos B, 7. p = o(l -|- cos B), 

2. p = aP, 6. p = sin 3 d. 8. p = 2/(1 -|- cos B), 

3. pB = a. 6. p = a sec 2 9. 9. p » a + & cos 9. 



CHAPTER XII 

TECHNIQUE OF INTEGRATION 

95. Question of Technique. Collection of Fonnulas. The 
discovery of indefinite integrals as reversed differentials was 
treated briefly, for certain algebraic functions, in Chap- 
ter VII. We proceed to show how to integrate a variety of 
functions, but the majority are referred to tables of integrals, 
since no list can be exhaustive. See Tables, IV, A-H. 

To every differential formula (pp. 44, 132) there corre- 
sponds a formula of integration: 

if d4> {x) =fix) dx, then f/ W dx = 4> W + C. 

The numbers assigned to the following formulas corre- 
spond to the number of the differential formula from which 
they come. Certain omitted numbers correspond to rela- 
tively unimportant formulas. 

FUNDAMENTAL INTEGRALS 

[I]i If ^ = 0, then y = constant. [See § 52, p. 86.] 

[The arbitrary constant C in each of the other rules results from this rule.] 

[II], fhf{x) dx = kff{x) dx. 

[Ill], /{/ {x) +it>{x)]dx =ff (x) dx +f<t> (x) dx. 

[TV]i (xn dx = 5^ + C, when n 5^ - 1. (See VIII.) 

166 



XII, § 95] TECHNIQUE OP INTEGRATION 157 

[VI]i uv = Cd{uv)^ Cudv+Cv du. ["Parts"] 

[The corresponding formula [V]i for quotients is seldom used. See § 103.] 

[VlIji J/(ti) du]^ ^ ^^^^ =Jf [<!> (X)] d<t> (X) 

[Substitution] = (f[<t>{x) ] ^^ dx. 
[Vni]i r^ = log X + C. [IX]i C&^ dx = e* + c. 

[X]i I cosxc/jc = sinjc + C. [XI]i | sinxdx = -cosx + C. 

[Xn]i jsec* X c/x = tan X + C. 

[Xinii fcsc* X dx = - ctn X + C. 

[XlVji J sec X tan x dx = sec x + C. 

[XV]i J CSC X ctn X dx = — esc x + C. 

[XVIji J-7== = sin-i x + C= -cos-ix + C. [xvn]i 
[XVra]i rj^ = tan-ix + C= -ctn-ix + C [XIX]i 
[XX]i r--^== = sec-ix + C= -csc"-ix + C'. [XXI]i 

[XXn]i r-7=^== = vers -ix + C 

The remaining differential formulas referred to on p. 132 
give rise to other integral formulas; these will be found in 
the short table of integrals, Tables, IV, A-H. 



158 THE CALCULUS [XII, § 96 

96. Polynomials. Other Simple Forms. The rules [II], 
[III], [IV] are evidently sufficient without further explana- 
tion to integrate any polynomials and indeed many simple 
radical expressions. This work has been practiced in 
Chapter VII extensively. 

Attention is called especially to the fact that the rules [II] 
and [III] show that integration of a sum is in general simpler 
than integration of a<product or a quotient. If it is possible, 
a product or a quotient should be replaced by a sum unless 
the integration can be performed easily otherwise. Thus 
the integrand (1 + x^)lx should be written 1/x + a;; (1 + o^Y 
should be written 1 + 2 a;^ + a;*; and so on. This principle 
appears frequently in what follows. 

97. Substitution. Use of [VII]. As we have already done 
in simple cases in Chapters VII and VIII, substitution of a 
new letter may be used extensively, based on Rule [VII]. 

dx 
Va2 — x^ 
Set u = xla^ then du = 3x1 a, or dx = a dUy and 

/dx r adu r du • _i , ^ • -i^c . ^ 

Va2 — x2 J Vo2 — a2w2 J Vl — w2 a 

^ , ' ^x 1 J /x\ dx/a dx 

Check. d sin"^ - = j i i _ — 



/dx 
-v//i2 — 



a \ x^ \^/ I x^ 

\^~a2 \^"-a2 



Vo2 - a;2 



Example 2. To find f Bm2xdx. 
Method 1. Direct Svbstitution, 

rsin2xdx = jTsin (2 x) d (2 x) = - }[cos2a; + C] 

= - J cos 2 a; + C. 
Check, d (— J cos 2 a;) = — } d cos (2 x) 

= + J sin (2 x) d{2x) = sin 2xdx, 

Method 2. Trigonometric Transformation and Svbstitution, 
fain 2xdx = y 2 sin x cos xdx = — 2 /^cos x d (cos x) 
= - (cos x)^ + K =-coa^x+ K, 



XII, § 98] TECHNIQUE OF INTEGRATION 159 

Notice that cos^ x -^ K =^ (1/2) cos 2 a; + C since cos 2 a; = 2 cos^ x 
— 1. Do not be discouraged if an answer obtained seems dififerent 
from an answer given in some table or book ; two apparently quite 
different answers both may be correct, as in this example, for they may 
diif er only by some constant.* 

Whenever a prominent part of an integral is accompanied 
by its derivative as a coefficient of dx, there is a strong indication 
of a desirable substitution; thus if sin x occurs prominently 
and is accompanied by cos x dx, substitute m = sin x; if log 
X is prominent and is accompanied by (l/x)dXy set u = log a;; 
if any function / (x) occurs prominently and is accompanied 
by df (x),setu=f (x) . This is further illustrated in exercises 
below. 

98. Substitutions in Definite Integrals. In evaluating defi- 
nite integrals, the new letter introduced by a substitution may 
either be replaced by the original one after integration, or the 
values of the new letter which correspond to the given limits 
of integration may be substituted directly without returning 
to the original letter. 

Example 1. Compute / sin a; cos x dx. 

Method 1. Let u = sin x. 

sin X cos X dx ^ I udu 

fi-^x^T/2 sin2a;n*-»/* 1 



Method 2. 



_ w2-|a;-T/2_ gin2 a;-|«. 
"■2Jx-o 2~Jx. 



/ sm a; cos a; ox = / udu ^ -^\ = ^ , 

Jx»o Ju^o ^Jk-o ^ 

since w ( = sin x) =0 when x = 0, and w = 1 when x = ir/2. 

Care must be exercised to avoid errors when double-valued functions 
occur. The best precaution is to sketch a figure showing the relation 
between the old letter and the new one. In case there seems to be any 
doubt, it is safer to return to the original letter. 

* Occasionally it is really difficult to show that two answers do actually 
differ by a constant in any other way than to show that the work in each case 
is correct and then appeal to the fundamental theorem ($ 52). 



160 THE CALCULUS [XII, § 98 

EXERCISES 

Integrate each of the following expressions: 

1. /(l-a;)(H-a;2)cte. 6. /(e* - e-«)2 cte. 

2. / =-! dx. 6. / dx. 

J x^ J X 

3. J{a-\-hxYdx, 7. f{l-2x)'^Vidx. 

4. /^-^^^ <^. 8. /(a^ - 2) (a;i/2 + a;2/8) <to. 

In the following integrals, carry out the indicated substitution; in 
answers, the arbitrary constant is here omitted for convenience in 
printing. 

9. y V3 a; + 2 cte; set w = 3 a; + 2. Ana, f ^3/2 = j(3a; + 2)3/2. 

.0. f^^-2 = i log (3a; +2) = log ^3 a; +2. 

^' /nR^ + 2)5 = i^«^"'(3x + 2). 

,2. fx V4+a;2 cte; set w = 4 + a;2. Ans, w3/2/3 = (4 + a;2)3/2/3. 

3- /^^2 = * log (4 +a:2) = log Vr+T^. 

,4. /sin X Vcosx dx; set w = cos x. Ans. — 2 W8/2/3 - — 2{gos^^x)/S. 

6. y cos a; Vsin a; dx = 2 (sin8/2a;)/3. 

6. /cos X (1 + 4 sin X + 9 sin2 x) dx = sin x + 2 sin2x + 3 sin^ x. 

,7. /sin3 X dx = /sin x(l — cos2x)dx = — cos x + (cos^ x)/3. 

8. ycos (3 X - 2) sin (3 X - 2) dx; = J sin2 (3 a;- 2). 

,9. ysin (1 - 3 x) cos5/2 (1 - 3 x) dx = A cos7/2 (i - 3 a;). 

20. / o ■ o ; e^t tt = -• Ans, f - tan~^ w = - tan~i - • 
•/ o2 -J- x2 ' ^ a I a a a 



XII, § 98] TECHNIQUE OF INTEGRATION 161 

In the following integrals, find a substitution by inspection and 
complete the integration. 

21. /4^73=5log(4a:+3)=log(4x+3)i/4. 

22. y V3 - 4 a; dx = - (3 - 4 x)^/^/6. 

23. ysin (4 a: - 3) cte = - } cos (4 a; - 3). 

26. ycos8 a; da? = sin a; - (sin^ a;)/3. (See Ex. 17.) 

26. J 008 X sin^ xdx — (sin^ x)/b. 

27. ^2 a; cos (1 + x2) da; = sin (1+ a;2). 

28. Aan3 x sec^ xdx=^ (tan*a;)/4. (« = tan ».) 

29. fctn^ X csc2 a; dx = — (ctn* a;)/4. {u = ctn a;.) 

30. ycos2 X dx =y [(1 + cos 2 a;)/2] da; = a;/2 + (sin 2 a;)/4. 

31. ysin2 X dx ^f[{l - cos 2 a;)/2] da; = a;/2 - (sin 2 a;)/4. 

32. Jcos^ xdx = sin a; — 2 (sin^ a;)/3 -|- (sin** x)/5. 

33. y ctn X dx = Acos a;/sin a;) da? = log sin x, (Put t* = sin a;). 

34. Ttan x dx = — log cos x = log sec x. 

^^ r dx 1 r dx lx_i/a;\ 

•^ Vl2-4a;2 ^J y/3^^ 2®"^ \V3/ 



162 THE CALCULUS [XII, § 98 



Compute the values of each of the following definite integrals. 

* Jx-o 3+a;2 V3 *° VsJ^-o vl ^ V3 6V3' 
39. / , = sin-i ( -F I = sin-i 1 = -5- 

*0- T"^ ^^2 == i I0& (3 + ^')T"^= i (loge 12 - lofo 3) = log.2. 

Jx-O o + X-* Jx-0 

41. f'^-^^= ^ « V2ir72T"' = - (vT- V2) = .4142 +. 

y^x^x/2 r nx-T/2 

sin3 x da; = - cos a; + (cos' a;)/3 = 2/3. 

z-O L Jx-O 

43. f'^x^dx-- €^/2T"^ = e/2 - 1/2 = .8591 +. 

Jx^O Jz-0 

y.if-2 ^-1 ^ 

yr^-2 ^x-2 1 + 2a; 

e-2«(to. 49. r ^-^5:^ da;. 

a»» 1 •/ X" 1 X -J" X^ 

^-ir/3 ^x-t/4 

46. / sin^ a; cos a; da;. 60. / cos^ a; dx. 



*/6 /•*-ir/4 

sin 3 a; (2a;. 61. / cos' a; da;. 



Jx-^o 



62. Find the area under the witch y = l/(o + 6a;2) for a = 9, 
6 = 1, from a; = to a; = i; for o = 8, 6 = 2, from a; = 1 to a; = 10. 
See Tables, III, J. 

63. Find the volmne of the solid of revolution formed by revolving 
one arch of the curve 2/ = sin a; about the a>-axis. 

64. Find the area under the general catenary 

y = a cosh (x/a) = a(e*/«+e-*/«)/2 
from a; = to a; = a. 

66. Find the area of one arch of the cycloid 

a; = a (^ — sin ^), y == a (1 — cos 0), 

66. Find the volume of the solid of revolution formed by revolving 
one arch of the cycloid about the x-axis. 

67. Compare the area of one arch of the curve y = sin a; with that of 
one arch of the curve y = sin 2 a;; with that of one arch of y = sin^ x. 



XII, § 99] TECHNIQUE OF INTEGRATION 163 

68. Show how any odd power of sin x or of cos x can be integrated by 
the device used in Ex. 17. 

69. Show how any power of sin x multiplied by an odd power of cos x 
can be integrated. 

99. Integration by Parts. Use of Rule [VII. — One of the 
most useful formulas in the reduction of an integral to a 
known form is [VI], which we here rewrite in the form 

[VI T J'u dv = uv —fv du 

called the formula for integration by parts. Its use is illus- 
trated sufficiently by the following examples: 

Example 1. J'x Binxdx, Put u ^ x^ dv — sin x dx; then du = dx 
and t; =y sin X cte = — cos x; hence, 

Jx sin xdx = — x cos x + /cos xdx = — x cos x + sin x] {check). 

Example 2. yiog x dx. Put log a; = w, dx = dv; then du = (l/x) dx, 
V = Xf and 

Jlogxdx = xlogx — fx'-'dx = a;logx — J dx 

— X logx — X + C; {check). 
Example 3. y Va^ — x^ dx. Put u = Vq2 — a:^, dv=dx; then v = Xj 
du= ^ ^^ - dx.gmdfVa^-x^dx =xVa^-x^-^ r_ j^dx_ 

but, by Algebra, f f^ = - f\^a^ -x^dx + f-^^; 

hence 

(j^'dx 



x^ 



J, . /» a^ ax 

V a2 - x2 rfx = x Va2 - x^ + I ^-^-- 

= X Va2 - x^ + a2 sin-i (-^ + C. 

This important' integral gives, for example, the area of the circle 
J?' -\-y^ — a^f since one fourth of that area is 

f^'^'^a^ - a;2 dx = i fx Va^ - x2 + a2 sin"! /5\T"'' 

21 2j 4 



164 THE CALCULUS [XII, § 99 

EXERCISES 
Carry out each of the following integrations: 

1. Jx cosxdx = X sin X + cos X + C. 

2. J'xeF dx = eF (x — 1) + C. [Hint, u = x, dv = eF dx.] 

3. fxlogxdx =- xV4 + (x2 log x)/2 + C. 

4. fx^logxdx=-- x*/lQ + (x^ log x)/4 + C. 

6. fx^dx = e» (x2 - 2x + 2) + C. [Hint. Use [VI] twice.] 

6. ysin"! X dx = X sin~i x + Vl — a;2 + C. [Hint, u = sin-i ^jj 

7. ytan-i X (ix = X tan-i x — log (1 + x2) V2 ^- c. 

8. yx2 tan-i X dx = (x^ tan-i x)/3 - xV6 + log (1 + x2)V6 + c. 

9. yx (e* — e~')/2 dx —Jx sinh x dx = x cosh x — sinh x + C. 

10. fx^e^' dx=^(9x^-6x-h 2)/27 + C. 

11. /e* sin X dx = e* (sin x — cos x)/2. [Set w = e*; use [VI] twice.] 

12. fe^ cos 3 X dx = e2x (3 sin 3 X + 2 cos 3 x)/13. 

15. y^^ sin 3 X dx = — e-* (3 cos 3 X + sin 3 x)/10. 

14. fe^ cos nxdx = e^ (w sin nx + a cos nx)/(cfi + n^), 

16. Show that yP (x) tan"^ x dx, where P (x) is any pol3momial, re- 
duces to an algebraic integral by means of [VI]. Show how to integrate 
the remaining integral. 

16. Show that yP (x) log x dx, where P (x) is any polynomial, re- 
duces to an algebraic integral by means of [VI]. Show how to integrate 
the remaining integral. 

17. Express J^x^ e^ dx in terms of fx^"^ 6"* dx. Hence show that 
yP (x)e«* dx can be integrated, where P (x) is any polynomial. 



XII, § 100] TECHNIQUE OF INTEGRATION 165 

Carry out each of the following integrations: 

18. f{2 - 4 a; + 3 a;2) log X dx. 20. fix^ - x)e-^' dx, 

19. fi3 a;2 + 4 X + 1) tan-i x dx. 21. f{x^ - 6)e** dx, 

22. From the rule foi^ the derivative of a quotient, derive the formula 
J*(l/v)du = u/v +y (w/y2) dv. Show that this rule is equivalent to [VI] 
if u and v in [VI] are replaced by 1/v and w, respectively. 

23. Integrate ye" sin x dx by applying [VI] once with w = e*, then 
with u^sinx, and adding. 

24. Integrate J^e^ sin nxdx by the scheme of Ex. 23. 
Find the values of each of the following definite integrals: 

26. r^"*log X dx. 28. r" (1+3 x^) tan'i x dx. 

y^-2 y^-T/2 

26. / xcdx. 29. / e-^'cosZxdx. 

Jx^-l J x^O 

^-1/2 ^-2 

27. / sin"i X dx. SO. / (e* — e"*) dx. 

31. Find the area under the curve y = e"» sin x from x = to x = t. 

Find the area under each of the following curves, from x = to x = 1. 

32. y = X6-*. 33. y = x^e-*. 34. 2/ = x^e^. 

36. Compare the area beneath the curve y = log x from x = 1 to 
X = e with the area between this curve and the y-axis, and the lines 
2/ =0 and y = 1. 

36. Show that the sum of the area beneath the curve 2/ = sin x from 
X = to X = A; and that beneath the curve y = sin"^ x from x = 
to X = sin A; is the area of a rectangle whose diagonal joins (0,0) and 
(k, sin k). 

100. Rational Fractions. Method of Partial Fractions. A frac- 
tion N/D, whose numerator and denominator are poly- 
nomials, is called a rational fraction. If such a rational 
fraction is to be integrated, we first note whether or not the 
degree of N is less than the degree of D. If not, we divide 



166 THE CALCULUS [XII, § 100 

N by D, to obtain a quotient Q and a remainder R whose 
degree is less than that of D. 

Example, yr = ^— , = 2 x H =— ; . 

D x^ -{-X . 3^ -\-x 

The integration of Q can be carried out at once. It 
remains only to consider the integration of rational fractions 
of the form R/D, where the degree of R is less than that of 
D, We shall proceed to discuss the integration of such 
forms, and we shall divide the discussion into several cases. 

101. Case I. Denominator Linear or a Power of a Linear Form. 
If the denominator of the fraction R/D (§ 100) is linear, or 
is a power of a linear form, i,e. if 

D = dx + b, or D = (ax + 6)", 
the substitution u = ax + b transforms the integral of R/D 
into a new form which is readily integrated. For this reason, 
we shall reduce other cases to this case whenever possible. 

102. Case n. Denominator the Product of Several Linear 
Factors. If the denominator of the fraction R/D (§ 100) 
is the product of several linear factors, the fractions R/D 
may be replaced by a sum of simpler fractions. The 
simpler fractions which compose this sum are called partial 
fractions. Each linear factor ax + b oi D gives rise to one 
such partial fraction, whose denominator is ax + b and 
whose numerator is a constant. Each of these partial 
fractions can be integrated as in § 101. The process is 
illustrated by the following example. 

Example. Evaluate the integral / 7 777 — r— pr? — t-ft: ^• 

J {x — l)(a; + l)(a; +2) 

The numerator of the integrand is already of less degree than the 

denominator. . We first set down the partial fraction sum just described: 

6a:2+3a;-15 _ A B C 



(x-l)(a;H-l)(a;+2) a; - 1 ' a; + 1 ' x + 2' 



XII, § 103] TECHNIQUE OF INTEGRATION 167 

where the constants A^ Bj C are as yet unknown. To find them, we 
clear of fractions, obtaining the equation 

6x2 + 3x - 15 = A(x + l)(x + 2) + J5(x-l)(x+2) + C(x-l)ix +1), 

which must hold for every value of x. If any three values of x are sub- 
stituted for X in turn, we obtain three equations that may be solved for 
A, B, and C, Values that are particularly simple are x = 1, x = —1, 
and X = — 2. Substituting each of these in turn, we get A = — 1, 
B = Q, C = h It follows that we may write 

Qx^ + Sx-15 _ 1 6 1 . 



(x- l)(a; + l)(a;+2) x - 1 ' x + 1 ' a; +2* 

Each of the fractions on the right may be integrated readily as in 
§ 101. Hence 

6x2+3x-15 ^ /---Ij ./• 6 J .rNl 



^ (x"l)(xH-l)(x + 2)'^ ^x-l'^^^x + l'^^^ 



dx 
x+2 

= - log (x- 1) +61og (x + 1) +log (x +2) 

(X + 1)6 (X + 2) 



= log 



X- 1 



103. Case m. Repeated Linear Factors. If one of the linear 
factors of the denominator D (§ 100) is repeated, i.e., if there 
is a factor of D of the form (dx + 6)**, that factor gives rise 
to several partial fractions of the form 



ax + b ' (ax + by ' (ax + by ' ' {ax + by 

Otherwise the process remains as in § 102. This case is 
illustrated by the following example, 

/3 /p2 — X 4- 1 
( 4-2V — 2')3 ^' 

According to the processes described in §§ 102-103, we first write 
3x2-x + l _ A B C D 



(x-|-2)(x-3)3 x-f-2 ' X--3 ' (x-3)2 ' (x - 3)3 * 
To find AyByCy and D, we clear of fractions 

3 x2 - X + 1 = A(x - 3)3 + B{x + 2)(x - 3)2 + C(x + 2)(x - 3) 

+ D{x + 2) 



168 THE CALCULUS [XII, § 103 

and then substitute for x, in turn, any four values of x. If we take 
a; = - 2, 0, 1, and 3, in turn, we find A = - 3/25, B = 3/25, C = 
12/5, D = 5. Hence 

r 3a;2--g + l , 
J (x + 2)(x-3)8^ 

/ — Sdx r Sdx r \2dx . r 5dx 

25(a; + 2) "^^ 25(x - 3) "^ ^ 5(x - 3)2 "^ ^ (a; - 3)3 

= --7^1og(a;+2)+llog(^-3)- ^^ ^ 



25 ^' . -/ . 25*^e»v-' -/ 5(2; _ 3) 2(a;-3)2 

=:Ai a; — 3 24 a; — 47 
25^^ a; + 2 10 (a: - 3)2 * 

104. Case IV. Quadratic Factors. If the denominator D 
(§ 100) contains a quadratic factor aa^ + bx + c which can- 
not be factored into real linear factors, we insert in the sum 
of partial fractions one fraction whose denominator is that 
quadratic factor and whose numerator is a linear expression 
Ax + B. The resulting fraction 

Ax + B 

as? + 6x + c 

can always be integrated. The process is illustrated in the 
example which follows, and in exercises in the following list. 
The general case is treated in the Tables, IV, B, No. 21, 
p. 38. 

( — lU 2 4-4.\ ^' 

We first write 

10a: -5 _ A Bx -^ C 



(x- l)(a;2+4) a;--l ' a;2+4 * 
Clearing of fractions, we have 

10 a; - 5 = A(a:2 + 4) + (x - 1) (Bx + C). 
Setting a: = 1, 0, — 1, in turn, we find A = 1, 5 = — 1, C = 9. Hence 

/ 10 a; — 5 ^ _ f dx f x — 9 , 

(a;- l)(a:2+4)^"^ a; - 1 J x^ + ^^' 



XII, § 105] TECHNIQUE OF INTEGRATION 169 

The first integral on the right is easily evaluated by § 101. The second 
integral on the right may be broken up into two parts which can be 
integrated separately: 

fj^4, ^ = ^ *^"^ i (S®® ^- 20, p. 160.) 

Collecting all these partial results, we have 

106. Case V. Repeated Quadratic Factors. If the denominator 
D (§ 100) contains a quadratic factor to a power, i.e., if D has 
a factor of the form {cu? + 6x + c)**, we insert among the par- 
tial fractions a set of fractions analogous to those of § 103, 
but with numerators that are linear, and with denominators 
that are successive powers of the quadratic: 

Ax + B . Bx + D , , Lx + M 



ax^ + bx + c {ax? + 6x + c)^ {ax? + bx H-c)" ' 

The determination of the unknown constants A, B, (7, etc., 
is performed as before. In general, the resulting partial 
fractions can always be integrated, but the problems become 
more and more difficult as the exponent n increases. The 
method of integration essentially depends on the process of 
§99 {integration by parts). Difficult examples should not 
be attempted without the assistance of the Tables, where 
the results of integration by parts are given in the general 
formulas 23 and 25, p. 38.* These, together with formulas 

* Even when it is desired to proceed without the use of tables, it is best, 
for difficult examples, to derive such formulas as 23 and 25, p. 38 (Tables), 
once for all, by integration by parts, and then to use these formulas instead 
of repeating the work in each example. 



170 THE CALCULUS [XII, § 105 

21, 22, and 24, p. 38, are sufficient to integrate any such 
expression. The process is illustrated by the following 
example. 

Example. Evaluate the integral f -. o\/ o i o\o <^' 

J {x — 2) (a;2 -j- 3)2 

As indicated above, we first set 

10 3:3 4- 7 a; -f 4 A Bx + C Dx + E 

(a:-2)(a;2H-3)2 a: - 2 "*" x'^+Z "^(2:2+3)2 

Clearing of fractions and determining the constants as before, we find 
^ = 2, -5 = - 2, C = 6, D = 6, and £? = - 11. It follows that 

r 10xM-_7^jf4 , _ f 2 /' -2a; + 6 r Gx-ll 

^ (a;-2)(x2-f 3)2'^"y a;--2'^"^^ x^ + 3 '^ "+" 7 (a;2 + 3)2 '^• 

The first integral on the right can be evaluated by § 101. The 
second one can be evaluated as shown in the example of § 104. The last 
integral may be evaluated either by an integration by parts, or by use 
of the formulas 22 and 23 on p. 38 of the Tables. 

EXERCISES 

Carry out each of the following integrations. 

^ r dx 1 /•/ 1 1 \j 1, «-i 

r dx \ y X + a 

f dx _ f dx _ 1 _, a; + 1 

*• J x'i+2x + 10 J {x + 1)^+9 3 3 

»• / x^ + 6^ + 10 °^°"(-+ ^)- 

r__dx___ _ f dx ^lif.«?ZlJ: 

^- 7a:24.2x--3"^ (a; + l)2-4 4'''^a;+3' 

/'___i£_-ll 2x-2 ^ 1 . x-1 
^' •/4a;2+4x--8"l2 ^^2x + 4 12 ^x + 2* 



XII, § 105] TECHNIQUE OF INTEGRATION 171 

In each of the following integrals, first prepare the integrand for in- 
tegration as in §§ 101-105 ; then complete the integrations. 

9. / ^ai'^s'^ + G ^ =log (^-2) +2Iog (x-3) =log [(x- 2) (x-Sn 

^ , , dx ^ x + tan~i x, 

12. / » frV ,, (te = log Vx2 + 2a;H-2 - 2 tan"! (1 + x). 
•/ x^ -|- J X -|- J 

<• /• <^ 1 X _i a; 1, ,x 

14. / 4:=f d^. 16. f- ' ^ 

J x^-'2x *^ X 



2+3X+2 

1A f__xdx__ ^- r x^dx 

^^' J x'^-bx + % J x«--4* 



x3+x ^^x3-7xH-6 

^x3H-2x2* ^2x3H-7x2 + 6x' 

^^- /(x--l)2(x--2)' ^'- /(X--1)(X2 + 1)" 

« . /• X dx OK ^2x2 -f 1 

^ 7 (x+2)(x+3)» - "• JirfW^- 

^- J {x + l)(x-2)^'^- ^- yF^=T6' 

28- J (a.2 _ 9)2- =*»• Ja;*-5x« + 4*'- 

Derive each of the following formulas. 

30 r ^ ^i— loK "^+". 

•/ (oa; 4- 6) (ma +n) an — bm " <tx+b 

•1 /• a;<fa: _ I . (x + o)» 

~. /• « <ir 5 , Vji' + o J. Va . „_, 

«*• / fx» + aHx + fe) °^+^^°gT+r^^q:^*^' 



X 



(x2 + a)(x + 6) a + 62"6 a;-|-6 a-|-62 ^ 



172 THE CALCULUS [XII, § 105 

33. Derive each of the formulas Nos. 18-24, Tables , IV, A. 



dx. 



Evaluate each of the following definite integrals. 

^«- 12 a; (a;- 4) 
So. / -p jrr^ dx. 

[Note. Further practice in definite integration may be had by insert- 
ing various limits in the previous exercises.] 

Carry out each of the following integrations after reducing them to 
algebraic form by a proper substitution. 

^_ r ainx , -,« /• cos a: , <,^ r ^ dx 

37. / zr-y o- ^' 38. / -. ^-5- dx, 39. / :; 5- • 

^ 1 + cos2 X J ^ — sm2 X •/ 1 — 62» 

.- /• , /• cosa; , 1, 1 4-sin a; , . /x , xX 

40. I secxdc - I z j-^— oc = olog:i -. — = log tan I -+- I • 

J ~'l — sm^x 2 *=•! — sma; ® \4 2/ 

41. JcBCxdc, 42. jBechxdc. 43. J each xdc. 

.. c sec* a; , a^ C^ ^ ^~* ^ 

J tan a; — tan^ x J eF +e~* 

106. Rationalization of Linear Radicals. If the integrand 
is rational except for a radical of the form Vox + 6, the sub- 
stitution of a new letter for the radical 

r = y/ax + h 
renders the new integrand rational. 

Example. Find / — t-j—: — cLc- 

Setting r = Vx + 2, we have x = r2 — 2 and cte = 2 r dr; hence 

= 2/(r + 1 - f:^)^^ = r^ +2r-- 21og(r + 1) + C 
= a; + 2 + 2 VxT2 - 2 log (VJT2 + 1) + C. 



XII, § 107] TECHNIQUE OF INTEGRATION 173 

The same plan — substitiUion of a new letter for the essential 
radical — is successful in a large number of cases, including 
all those in which the radical is of one of the forms: 



«.,,(^ + „v.,(^J- 



+ 

where n is an integer. Integral powers of the essential radiqal 
may also occur in the integrand. 



107. Quadratic Irrationals: Va + 6x d= x^. If the integral 
involves a quadratic irrational, either of several methods 
may be successful, and at least one of the following always 
succeeds: 

{A) If the quadratic Q = a + 6x i x? can be factored 
into real factors, we have 

K a "T" iC 

and the method of § 106 can be used. The resulting expres- 
sions are sometimes not so simple, however, as those found by 
one of the following processes. 

{B) If the term in x^ is positive, either of the substitutions 

VQ = t + x, \/Q = f-a:, 

will be found advantageous. One of these substitutions may 
lead to simpler forms than the other in a given example. 

(C) Completing the square imder the radical sign throws 
the radical in the form 

VQ = Vztfc=fc(a:=tc)2; 

the substitution x zt c = y certainly simplifies the integral, 
and may throw it in a form which can be recognized instantly. 



174 THE CALCULUS PQI, § 107 

(Z>) After completing the square under the radical sign, 
the radical will take one of the forms Vfc2 — a;^, Vfc^ + x^, 
Vx^ — fc^. Then a trigonometric substitution often leads 
to a simple form. Thus: 

ii X ^ k sin 0, Vk'^ — x^ becomes k cos 0; 

ii X = k tan 0, Vk^ + x^ becomes k sec 0; 

if X = fc sec ^, Vx2 — fc2 becomes k tan 0, 

Example. Let Vq = Vx^ ± a^; show the efifect of substituting 
Vq-^t-x, 

U Va;2 ± o2 = < - a;, we find 

and the transformed integrand is surely rational. Carrying out these 
transformations in the simple examples which follow, we find 



(i) 



(ii) 



= log (x + Vq) + C, where Q = x^ ± aK 



>s 



'^±flog*=^±|log(x + v/Q) + C. 



These integrals are important and are repeated in the Table of In- 
tegrals, Tables, IV, C, 33, 45a. Many other integrals can be reduced 
to these two or to that of Ex. 3, p. 163, or to Rules [XVI] or [XX] by 
process (C) above. 



EXERCISES 

1. fx Vx^n. dx = (1/15) (6 » + 4) (a: - 1)8/2. 

2. / ■ — dx -2 Vx + 1 + log , • 



3. f — r^ — = 2 tan-i Vx - 1. 
•^ xVx— 1 

4. / J]^ dx = vT=T2 + sin-i X. 
^ \1 -\-x 



XII, § 107] TECHNIQUE OF INTEGRATION 175 

6 f ^ ^ -J- f,,n-l \^Th 

J (ox + 2 6) Vox -\-h aVh \ 6 ' 

/■ (to _ ViTl 1 v^Ti + 1 

7. /(a + &a;)3/2 d^ = ^ (« + 5a;)6/2. 

A f ^ ■= 2 

''•^ (a + 6x)3/2 hVT+bi' 

Carry out each of the following integratioDS. 
9. fxVTTidx. 10. f ^L^ 

jj r dx ^2 r fr+ 

"•/>(^'^- "•/>i?r'*«- 

17. /x ^r+^(to. 18. fx yl3x + 7dx. 



dx 

^ X 

- dx. 

X 



^ (1 + x)3/2 ^0 1 — V5 

+ y/T+~x 



26. r'-^^dx, 26. r- 



Carry out each of the following integrations by first making an ap- 
propriate substitution. 



„f_^osx^ 3^ r_smxvc 

^ 3- Vsmx ^ 1-2V 



X Vcosx 



cosx 



dx. 



28. /^^3. 31. f'-±^^cosxdx. 

QQ r sec2 X (to ^„ /• sin x (to 



V2 + 3tanx ' -^ (2 + 3 cos x)3/2 



176 THE CALCULUS [XII, § 107 

Substitution of a new letter for the essential radical is immediately 
successful in the following integrals. 

S3. fxVl+x^dx, 86. f (^+^)/^ . 39. fx^Va + bx^dx. 



V2 H- 2 a; + a;2 
7^ dx ^^ r xdx ,^ r ^ 



36. /'x(H-x2)8/2dx.38. / , ff^wo ' *!• / r"'"^ ' 

•^ ^ (a + 6a:2)p/« y Va + te» 

Carry out each of the following integrations. 

/dx ____^^^ 

V^^n = log (* + VS?^^) . 



dx. 



s^ r dx .1, Va:2 — a^ 

43. / — , = - tan-i — =^ 

^ X V a;2 — a? a a 

' -^ (X + a) Va2 - a;2 a \o + x 

46. f ^ ^ = tan-i — ^=. 

•^ (l+2a;2) Vl+a;2 V52T1 

/3J "4" 1 ^—— 

^/r-^-^ dx = sin-ix - Vl - x\ 

4S. f , '^ ■ 49./ , '^ • 60./ '^ 



V4 x2 + 1 * "^ a; V4 a;2 + 1 * -^ a;2 V4a;2 + 1 

61. / dx, 62. / 5 — dx. 63. / ■ , dx. 

J X . J X^ J Vl — x2 

The following integrations may be performed by the methods of 
§ 107; note especially method (C), which consists in completing the 
square under the radical. 

/dfX _^_^^_^_^_ 

:^^=^==log(2x~H-2Va:2-a: + I). 

56. /•-_^==sin-i2^. 

66. f , = sin~^ ^ ^ = vers'^o [+ const.]. 

^ V4a;--a;2 2 2 



XII, § 108] TECHNIQUE OF INTEGRATION 177 

67. / — - == sm 1 7=r- 

68. / — = sm 1 — -. 

^ xy/lx^-\-Qx-l 4a; 

69. /- , ^ . 60. r , ^ > 61. /-- ^ 

•^ v2»2H-a; + l •^vH-a;-2x2- -^ Vl--2a;-a;2 

62. / ^ ^ 66. /'Vl4-xH-a;25i. 

•^ V6a: — x2--5 "^ 



63. r , 66. rVSxa + lOx + Oda;. 

•^ X Va;2 + 2 a; + 3 "^ 

64. f ^ 67. f X Vr^\^xTx^ dx, 

•^ (xH-4)Va;2+3a;-4 -^ 

Integrate by parts, [VI], each of the following integrals. 

68. /"x sin-i X dx. 71. J {Zx — 2) sin"! x (ix. 

^- /•sin~ix, -„ /•2+x2 

69. / 2~ ^- ^^* J — 2~ ^^ * ^• 

70. jx cos~i X dx, 73. j (sin~i x + 2 x cos~i x) dx. 

108. Trigonometric Integrals. A number of trigonometric 
integrals have been evaluated in the preceding lists of exer- 
cises. The processes explained in Exs. 14, 15, 17, 25, 26, 
28, 29, 30, 31, pp. 160-61, may be generalized and stated in 
the form of standard processes. They depend chiefly upon 
the use of well known relations between the trigonometric 
functions. (See Tables, pp. 12-13.) 

Since it is desirable to avoid the introduction of radicals 
that were not present in the original example, we do not 
ordinarily use the trigonometric formulas that involve a 
square root. But' it is desirable to notice that 

(a) Any even power of sin x can be changed into a sum of 
powers of cos x by the relation sin^x + cos^x = 1. 

(6) Any even power of cos x can be changed into a sum of 
powers of sin x by the same relation. 



178 THE CALCULUS [XII, § 108 

(c) Similarly, sums of even powers of tan x may be changed 
into simis of even powers of sec x, and conversely, by the 
relation sec^x = 1 + tan^x. 

(d) All the trigonometric functions may be changed into 
forms in sinx and cosx without introducing any new 
radicals. 

(e) The square of sin x and the square of cos x may be 
expressed in terms of the first power of cos 2 a; by means of 
the formula cos 2 x = cos^ x — sin^ x, 

(/) All the trigonometric functions can be expressed 
rationally in terms of tan (x/2). 

109. Integration of Odd Powers of sin x or of cos-x. Any 
odd power of sin x may be integrated, as in Ex. 17, p. 160, 
by the substitution u = cos x. 

Likewise, any odd power of cosx may be integrated by 
means of the substitution u = sin x. (See Ex. 25, p. 161.) 

More generally any integral of the form . 



/ 



sin" X cos*" X dx 



can be integrated if either m or n is an odd integer. If n is 
odd, set u = cos x; if m is odd, set i* = sin x. This process 
is illustrated by Exs. 14, 15, 16, 18, 19, p. 160; and by the 
following example. 

Example. Evaluate the integral J* sin3/2 x cos^ x dx. 
Set w = sin a;; then 

/ sin8/2a; cos^ xdx = /^sin3/2 x(l — sin^ a;)cos x dx 

= y w3/2 (1 _ y2) du 

= % w6/2 - ? w«/2 = ? gin6/2 x-\ sin9/2 X. 
5 9 O U 



XII, § no] TECHNIQUE OF INTEGRATION 179 

110. Reduction Formulas. If the integrand is an even 
power of sin x (or of cos x) we may use § 108 (e), as in Exs. 
30, 31, p. 161, or we may proceed by integration by parts, 
as follows. Let us first write 

J sin" xdx = I sin"~^ a: sin a: dx 

and then integrate by parts (§ 99) by taking 

u = sin""^ Xy dv = sin x dx, 

du = {n — 1) sin**"^ x cos xdx,v = — cos x. 
Then we obtain 

y^sin** X dx = — cos x sin"~^ x+ (n — 1) Jsin^-^x cos^ x dx. 

Replacing cos^x by 1 — sin^x in the last integral and breaking 
it up into two integrals, we have, 

J&in^x dx = — cos x sin""^x + (n — 1) Jsin^^^^xdx 

— (n —l)fsm^xdx. 

Transposing the last integral and dividing by n, we find the 
formula {Tables, IV, E, 57) 

(1) fsin" xdx^- ^osx^n^-^x n-1 T .^„_,^ ^ 
J n n J 

Repeated applications of this formula reduce the left-hand 
side to integrals that involve sin'*"*^, sin""* ^, • • *, down to 
sinx if n is odd, or to sin^x (= 1) if n is even. In either 
case, the integration can be completed by the use of a stand- 
ard formula. 

Ixx a similar manner, we obtain the formula {Tables, IV, E, 
60) 

(2) fcos-x dx = ^^^^^^^""^ + ^^^ fcos-^xdx. 
J n n J 



180 THE CALCULUS [XII, § 110 

By solving these formulas for the integral on the right-hand 
side, we obtain 

(3) fsin'^-'xdx = ""^^ »'"""' ^ + -?L_ fsin-a; dx; 
J n — 1 n — IJ 

and 

(4) fcos"-'' X dx = - ^^^^0^]-'^ + _??_ fcos" X dx. 
J n— 1 n — IJ 

These formulas raise the exponent in the integrand. Hence 
they are useful in integrating negative powers of sinx and 
cos Xy i.e, positive powers of esc x and of sec x. 

An analogous integration by parts leads to the formula 
(Tables, IV, E, 64) 



(5) fsin" 



X Qo^^xdx 



Sin""*"^ X COS*" ^X ^ m — I C ' n m-2 J 

. ; — I sm"a: cos*" ^xdx 

m + n m + nJ 

sin"~^a; cos*""*"^x , n — \ C - n-2 m j 
— . — I sm" ^x cos*" X dx, 

m + nJ 



m + n 

The proof of this formula is left as an exercise for the student. 
If either m or ti in (5) is an odd integer, the process of § 109 
is usually quicker. But if both m and n are even integers, 
the formula (5) is very useful. 

Example 1. Evaluate J* cos* x dx. 

/. , cos3 X8mx , S r „ , 
cos* xdx — -T — + 7 / cos2 X dx 

cos3 a; sin a; , 3 fcos x sin a: , 1 f ■, "] 
= i +iL 2—+2J'^j 

cos^ re sin a; , 3 . ,3 

= -: h Q cos xsmx -i-QX. 

4 o o 



XII, § 111] TECHNIQUE OF INTEGRATION 181 

If, in this example, we should follow the method suggested under 
(e) of § 108, we would write 

+ COS 2x\^ 



A t 9 ^9 /l+oos2a:\' 

= ^ (1+2 COS 2 a: + cos2 2 x) 

1 /i I o o , 1 + cos 4 a;\ 
= I ^1 + 2 cos 2 a: H ^ ) 



Then 



3 a; . sin 2 a: . sin 4 a: 



/. J d a; , sm z a: , 
cos* xdx — -^ -\ -^ h 



8 ' 4 ' 32 



Example 2. Evaluate f sec^ x dx. 

By (4), with n = — 1, we find 

//* sin X cos"^ X ■"" 1 /* 
sec' xdx = J cos""3 xdx = ^-^ f- —-^ J cos~i x dx 



sin X sec^ x , 1 /* 
2 "^2^ 



sec X dx. 



The integration may now be completed by means of Ex. 40, p. 172, 
which is essentially an application of § 109. 

Example 3. Evaluate ysin^ x cos* x dx. 
By the second part of (5), we have 

/• 9 A J sinarcos^a; , 1 /• . , 
sm2 X cos* xdx — ^ \- ^1 cos* x dx. 

The example may now be completed by following Example 1. 

111. Powers of tan x and of sec x. Any even power of tan x 
naay be reduced to a sum of even powers of sec a; (§ 108 
(c) ). This may be integrated by the method mentioned in 

§110. 

Another method of integrating any even power of sec x 
consists in making the substitution u = tan x. Since 
du = sec2 X dxy and since even powers of sec x may be 
reduced to a sum of even powers of tan x (§ 108 (c) ), the 
integration becomes very simple, as is illustrated by Exam- 
ple 1 below. 



182 THE CALCULUS [XII, § 111 

Odd powers of sec x can be most readily integrated by the 
method of § 110, as shown in Example 2, § 110. 

Any positive integral power of tan x may be integrated by 
reducing it to one of the two integrals: 

{\)fi2iiixdx= — log cos x= log sec x. (See Exs. 33, 34, p. 161.) 
{2)ft2Ji^xdx =f{^Q? X — 1) dx = tan x — x, 
by means of the reduction formula (see Tables IV, E, 70) : 
(3) I tan" xdx= ^^_ ^ — | tan'*-^ x dx. 

This reduction formula is obtained as follows: 

Jtsin^ xdx = Jta,n^~^ x tan^ xdx= fidJi^'^ x (sec^ x — l)dx 

= JtdM^'^x sec^xdx —JiBXi^'^x dx. 

If we set u = tan x in the first integral on the right-hand 
side, we obtain the formula (3). 

Example 1. Evaluate the integral ysec* x dx. 

Put u = tan x\ then du — sec^ x dx, and we may write 

/ sec* xdx =J sec2 x sec^ x dx —JO- + tan^ x) sec^ x dx 

= J (I +v^)du ^u + -^ = tan x-\ 5 — • 

Example 2. Evaluate y tan* x dx. 
As indicated above, we may write 

/^tan* X dx = /^(sec^ x—l)^dx = /^(sec* x — 2 sec* x-^1) dx 

= /^sec* X dx — 2 tan x-\-x. 

The remaining integral may be integrated as in Example 1. The stu- 
dent should also apply the reduction formula (3) to this integral. 

Example 3. Evaluate y tan^ x dx. 
Applying (3) we have 

/tan' xdx ^ r — /tan xdx = 7 + log cos x. 
n— I •^ n — 1° 



XII, § 112] TECHNIQUE OF INTEGRATION 183 

EXERCISES 

Evaluate the following integrals. 

1. / sin* X dx. 2. fsin^ x cos^ x dx. 3. /^tan* x dx. 

4. / tan^ X dx. 6. Jsec^ x tan* x dx. 6. Jca(^ x dx. 

7. Jta,n X sec* xdx. 8. / esc* x dx. 9. Jcsc^ x dx. 

10. /^cot* X dx. 11. fcot^ X dx. 12. Ttan^ x csc^ a: da;. 

13. fcSCXCOt^Xdx. 14. /-: • 16. /-: r— • 

^ ^ sin a; cos x ^ sin a? cos^ x 

le. / .^'fe ^ ■ 17. /?«L^±^dr. 18. /• ^ '^ ■ 
^ sin* a; cos* a; J suxx J Vsin x cos* x 

//* /"COS^ X 

sin2 a: cos* a: efcr. 20. / sin* x cos^ a: dx, 21. / . , dx. 
J J sin^a; 

22. f^^dx. 23. fsm^xco^xdx. 24. f . ^^ , - 

J sin2 X •/ ^ sm2 a: cos* a: 

^_ rsin* xdx g.^ r%\v^ x , «_ rcos^ x , 

25. / 26. / — ^-dx. 27. I . ^ dx. 

J cos a; J cos^ a: ^ sin* x 

28. /^sin* a; cos* a; da;. 29. /^sin 4a: cos Sa^dir. 30. fainSx cos 4a; dx. 

31. Verify formula 111 of Table IV, E. 

32. Verify formula 112 of Table IV, E. 

112. Elliptic and Other Integrals. If the only irrationality 

is VQ, where Q is a polynomial of the third or fourth de- 
gree, the integral is called an elliptic integral. While no 
treatment of these integrals is given here, they are treated 
briefly in tables of integrals, and their values have been com- 
puted in the form of tables.* See Tables, V, D, E. 

* Some idea of these quantities may be obtained by imagining some per- 
son ignorant of logarithms. Then y (l/x) dx would be beyond his powers, 
and we should tell him ** values of the integral f (1/x) dk can he found taJtrw- 
lated" which is precisely what is done in tables of Napierian logarithms. 
Of course as little as possible is tabulated; other allied forms are reduced 
to those tabulated by means of special formulas, given in the tables. 



184 THE CALCULUS [XII, § 113 

The discussion of such integrals, as well as of those in 
which Q is of degree higher than four, is beyond the scope 
of this book. 

113. Binomial Differentials. Among the forms which are 
shown in tables of integrals to be reducible to simpler ones are 
the so-called binomial differentials: 

f (ax"" + hy^xT dx. 

It is shown by integration by parts that such forms can be 
replaced by any one of the following combinations, where u 
stands for (ax*^ + b) : 

(1) /w^x*» dx = (Ai) u^x"^-^' + (Bi) fu^-'oT dx, 

(2) /ii^x"» dx = (A2) i^^+'x^+^ + {B2) /w^+'x^ dx, 

(3) / w^x"» dx = (A3) u^'-^'sT-^^ + (Bs) / w^x^+" dx, 

(4) / w^x*" dx = (A4) i^^+^a:^-~+^ + (B^) /w^x"*-" dx, 

where Ai, A2, Az, A^, Bi, B2, B3, B^, are certain constants. 

These rules may be used either by direct substitution from 
a table of integrals in which the values of the constants are 
given in general * (see Tables, IV, D, 51-54), or we may 
denote the unknown constants by letters and find their 
values by differentiating both sides and comparing coeffi- 
cients. 

* Such formulas are called reduction formulas; many other such for- 
mulas — notably for trigonometric functions — are given in tables of inte- 
grals. (See Tables, IV, Ea, 57, 60, 64, etc.) It is strongly advised that no 
effort be made to memorize any of these forms, — not even the skeleton 
forms given above. A far more profitable effort is to grasp the essential 
notion of the types of changes which can be made in these and other in- 
tegrals, so that good judgment is formed concerning the possibility of 
integrating given expressions. Then the actual integration is usually per- 
formed by means of a table. See also Tables, IV, Ea, 78, 82 (&) ; Eft, 85, 
86; Ec, 92-94; Ed, 98, 106; B, 17 (6), 25; etc. 



XII, § 114] TECHNIQUE OF INTEGRATION 185 

Example 1./^-^^-^^ = ^_^__ + B/_^__,by (2). 

Differentiating and comparing coefficients of x'^ and a;0, we find 5=0 
and A — 1/6; hence 

/ (0x2+6)3/2 = 2,V(i+6) ' ^'^'*' 

Example 2. J ^^^ ^ ^^3/^ = (^2+6)1/2 +^7 (00^2 +6)3/2' by (4). 

Here A = 1/a, 5 = - 2 6/a, 

J /• x^dx _ ax^ + 26 



(0x2 + 5)3/2 o2V(ax2 + 6) * 

114. General Remarks. The student will see that integra- 
tion is largely a trial process, the success of which is dependent 
upon a ready knowledge of algebraic and trigonometric trans- 
formations. Skill will come only from constant practice. 
A very considerable help in this practice is a table of integrals 
(see Tables y IV, A-H). The student should apply his intelli- 
gence in the use of such tables, testing the results there 
given, endeavoring to see how they are obtained, studying 
the classification of the table; in brief, mastering the table, 
not becoming a slave to it. 

In the list which follows, many examples can be done by 
the processes mentioned above. The exercises 43-97 may 
be reserved for practice in using a table of integrals. 

REVIEW EXERCISES 

^'J(x+2)^'^' ' J (2a: + 3)2 ^' 

« f ^ A. r x2 + 1 J 

^ J a:3+3x2* *• J i^^ '^^• 



(a;-2)3 • J (x + l)(x-l)2 

' a;3 + i /' a;3+2a;2. 

;c2 - 3 X + 3 J X^-Ti'^ 



J 



186 THE CALCULUS [XII, § 114 

Q f ^ lA c ^ 11 r ^ 

J (1 - x2)2' "• ^ 4 a;4 + 5 x2 + 1* ^ ^ 16 - x^' 

^A /* x^ + 3 X J ^^ /* x^rfa; ^. /*_^xMx_ 

"• y a:2 + 3a: + 4'^- ^^- 7 x4-2a:2 + l' ^*- ^ (5 - 7 x3)3- 

xdx ^» r x^dx --/• dx 



"• f^^- "• fwT2jn' "• Z:^ 



(ix. 



a;2 + 2a; + 5 -^ a:2 + 4a; + 2 

18. fxy/JT2dx. 19. f—%=^ 20. f-r^=^' 

^ ^ x^x—\ ^ V ax + 6 

21 r ^ ^ . 22 r /^ . 23. c^m^i^, 

^ V(a + 6x)3 -^ V(a+x)3 -^ (x- 1)3/2 

/' (2+x)cfo /- x2rfx /-(Ijfv^ 

2*- 7 ^3"^ • 2^- 7 (a + 6x3)3/2- 26. ^ ^/2 

27. f , /^ w ' 28. / 3^!Ji » 29. fxylzlTpIdx. 

'"• ^ (9x2-3)3/4* ^^- J Vf3^ ^ X(X2- 1)3/2* 

^- J xHi- x2)3/2 ^- 7 vrT^+ ^rvx 

35. f-fi%- 36. /-^. 37. Z-,^^^. 

38. f l'^^ dx, 39. /"x ^3x + 7(Zx. 40. /x ^'a + 6x2 dx. 

41. y x3 (a + x2)i/3 dx 42. ^ xS (1 + x3)i/3 cte. 

In the following integrations, use Table IV freely. 

f dx .. C dx -- f 3x + 2 , 

«• J p+l)2- **• 7 (x2 + 5)3* ***• 7 (a;2 + 3)3^- 

AA r 5x-3 , -- r rfx .^ r a?<fa? 

***• ^ (2 X2 - 1)2^^- *'• ^ (x2 + 2X + 5)2* ***• ^ (x + l)2(x+2)2 

49. / . 60. / . 61. I .>- , . o^o/a ' 

y a;3 y/x^ - 4 -^ Vx2 - a2 ^ (7 + 4 x3)2/3 

62. / (a2 - x2)3/2 dx, 63. / (x2 - a2)3/2 dx, 64. f —^^—^. 

^^' J {a^ 6x2)3/2- °^- J (1 - a;2)3/2' "''7 (« + 6x2)6/2* 



XII, § 114] TECHNIQUE OF INTEGRATION 187 

68. f^^^-^dx, 59. f^^^-r—dx. 60. f Bin^ x cos^ x dx, 

•/ sin a; •/ cos^ x J 

^^' J 2 + sin^* ^^ J 2- 3 cos ^*' ^* ^ 2 + 5 sin ^' 

64. f cos« a da. 65. ^ ctn2 Sxdx, 66. ^ sin8/2 ^ cos^ ^ d^. 

^0 (ic — 2)2 Ji (2 X — 1)» Jo 2 a;2 + 3 

70. / ,5—5 — xcte. 71. / — 7==- 72. / . dx. 

Jo 2a;2 — 3 •^2 a;v2a; + 3 -'^ v a;2 — 3 

^3^(l±£l^. 74Y-7^=- 76./^^=^. 

Jo V4 — x2 Ji Va;2 + 1 Ji Va;2 — 1 

^^' Jo (2 a: + 1) (0:2 + 2)* ^7- J _^ Vx^-Sx 

Find the values of the following definite integrals by using the tabu- 
lated numerical values: Tables^ V, A-H: 

ei'dx. 84. / — 7^ — dx = I cosh x dx. 

z-O J x=0 ^ •/sr-0 

yr,2-2.5 ^=2.3 

e2»(ir. 86. / sinha;cte. 

x-1.2 ^x-o 

y^x=1.4 >r=2 ^ -lx-2 

e-^' (to. 86. / , = cosh-i x 

x-O Jx«l Vx2— 1 J«-l 

-dx. 87. / /^ =sinh-ia; . 

x-i a? ^x-o va;2 + 1 Jx-o 

— ^dx. 88. r ,Z1_ =co8h-i^ 

x-3.5 X — Z Jx-2 Va;2 — 4 2Jx-2 

^x-3.2 1 ^-14.4 dx . , ,a;T-i4-4 

83. / -s — 7(to. 89. / ■ . = sinh~^ » 

Jx-2.1 a:^ — 1 Jx=o Vajz + Q ojx-o 

a ^ 30** j/i 

90. r = = /^ (J, 30°), Tables, V, D. 
Je»o- Vl- (l/4)sin2^ 

91. r^'*^ Vl- (l/4)sin2^dd = E (J, 45°), Taftfes, V, E. 

=■ 93. f Vl - .25 sin2 ^ dd. 

5=16" Vl — .04sin2^ Jtf-30«» 

y.=r-l/2 ^^ J^ ^-30- J^ 

./x-O Vl — ^2 Vl — 9K ^2 Jfl-0» 



^y-O Vl-x2Vl-,25»2 J^-o' Vl-.25sin2^' 

if X = sin d. 



188 



THE CALCULUS 



[XII, § 114 



- .36 a;2 






a;2 
(2x 



(^x 



.9-90<> 



= /* Vl - .36sm2 ^ dd, if a; = sin tf. 



^X-V2/2 \ 1 — 



-.16x2 



cte. 



a;- 1/2 Vl — a:2 Vl — .49 a;2 J x^-nf^ \ i — x^ 

[Note. Many of the exercises in preceding lists may be used for 
additional practice in use of the tables.] 

115. Limits Infinite. Horizontal Asymptote. If a curve 
approaches the x-axis as an asymptote, it is conceivable that 
the total area between the x-axis, the curve, and a left-hand 
vertical boundary may exist; by this total area we mean the 

limit of the area from the left-hand 
boundary out to any vertical line 
X = m, as m becomes infinite. 

Example 1. The area under the 
curve y = e"* from the ^-axis to the 



























\ 
























^ 


V 








y 


= 


c-^ 












\ 
























\ 


V 
























\ 
























1 


'^ 
























i 




^ 


^ 


^ 























z= 


-.m 



























































ordinate a; = m is 

e"^ dx = 1 — e"». 



Fig. 42. 



-|a;=»oo ^- 



*ao 



>-» 



dx 



]X^m y,-U- 

= f 

As m becomes infinite e~"» approaches 
zero; hence 

e-* dx — lim (1 — 6~*») = 1, 

... _. X^Q fflp-MO 

and we say that the total area under the curve y = e~* from a; = 
to x = + 00 is 1. 

Example 2. The area imder the hyperbola y = 1/x from a; = 1 to 
a: = m is 

A \ = / — = log a: = log w. 

Jx"! Jx'^l X Jx-i 

As m becomes infinite, log m becomes infinite, and 

lim ] A \ [ = lim log m 

does not exist; hence we say that the total area between the a>axis and 
the hyperbola from a; = 1 to a: = oo does not exist* 

*This is the standard short expression to denote what is quite obvious, — 
that the area up to a; =m becomes infinite as m becomes infinite. This result 
makes any consideration of the area up to a; = x perfectly useless; hence the 
expression "fails to exist," which is slightly more general- 



XII, § 116] TECHNIQUE OF INTEGRATION 



m 



116. Integrand Infinite. Vertical Asymptotes. If the func- 
tion to be integrated becomes infinite, the situation is pre- 
cisely similar to that of § 115; graphically, the curve whose 
area is represented by the integral has in this case a vertical 
asymptote. 

If / (x) becomes infinite at one of the limits of integration, 
x = bywe define the integral, as in § 115, by a limit process: 



J'*x = 6 rb-c 

f (x) dx = lim I / (x) dx. 
x=a c— >0 ^ a 



A similar definition applies if / {x) becomes infinite at the 
lower limit, as in the following example. 

Example 1. The area between the curve y = 1/VS and the two 
axes, from a; = to a; = 1, is 

= / — p dx = lim / —7= dx 
x=0 •/a;«0 y/x c->0 L*^x=c Va; J 

= lim \2^/x\ '"' = lim [2 - 2Vcl = 2. 

c— »0 L J x-c c-*0 L J 



Example 2. The area between the 
hyperbola y = 1/a;, the vertical line 
x = 1, and the two axes, does not 
exist For, 

/ - cte = log a; = — log c, 

but lim (— log c) as c-*0 does not 
exist, for — log c becomes infinite as 
c->0. 

Example 3. The ar ea between 
the curve 2/ = 1/ Va; — 1, its asymp- 
tote a; = 1, and the line a; = 2 is 































' 










t 
















y 






y 


= 


1 

X 


















, 


























\ 


























^ 


























^\ 
























1 


^\ 
























1 


^^ 


S. 


^ 






















^^ 








^ 


^ 


.^. 


^ 










C 


1 










( 








X 


























^mmmi 





Fig. 43. 



/ 



'2 dx 



= lim (^ 



dx 



-^= - X.... . 3, = |lim (1 - c2/3) = ? 



190 



THE CALCULUS 



[XII, S U6 



£!xAMPLE 4. Show that f 1/x^ dz docs not exist. The ordinate 

y '^ l/z^becomeainfiaiteaaxapproacheszero, i.e. the ^-axia is a vertical 
asymptote. Hence to find the given integral we must l^roceed as 

above, breaking the original integral 

into two parts: 

1-11-1 







y ■ IJ 












1 


- 
































' 








- 


■ 


. -, -^ 






t 










-T- ^ 


i 


'l_ 




/ 


- 












> 






± j_ 










-a::H^ 



I. 



The limit of neither exists since 1/c 
becomes infinite as c = 0; hence the 
given iat«gral does not exist. 

Carelessness in such cases results In 
absurdly false answers; thus if no atten- 
tion were paid to the nature of the 
''^' **■ curve, some person might write: 

which is ridiculous (see Fig. 44). 

The only general rule is to follow the principles of 
§§ 115-116 in all cases of infinite hmits or discontinuous 
integrands. Sucii integrals are called improper integrals. 
EZERCISSS 



-^i::!:- 



Verify each of the following results. 




'■/.TS' 



non-exist«Dt. 



t. r — ^^ = 

Ji.sV2z-3 
'■/,'.2 



IS non-existent 



! determinate if n < 1, 
non-existent if n £ 1. 



XII, § 116] TECHNIQUE OF INTEGRATION 191 



dx 



State a similar i*ule for / 77 — ri \ 

J a {hx + ky 



9 



Va2 — 0:2 2 * Jo Vox — x^ ^ 



^ xdx __ - -n /'^^ cte 

Vl — a;2 "" ' * J-i a;2+5a:+4 



10. /* , = 1. 12. /* o ■ ^ . ^ is non-existent. 

Jo Vl — a:2 •/ -1 



IT IT » 

.2 ^2 ^2 



13. Show that the integrals f tan x dx, f ctn a; (is, f sec x dx, 

Jo Jo Jo 

y— are all non-existent. 
X 

Verify each of the following results: 

/•* dx 1 /•* dx 

-a7=: is non-existent. 17. f 77-^ — ttt? is non-existent. 

/** ^ ' j determinate if n > 1, 
* Jo (1 -\-x)^ J non-existent if n ^ 1. 

19. I ^rn — s = o* 22. / (ix is non-existent. 

Jo l+aj2 2 Ji a; 

20. r*T^2=J^- 23. f^e-^dx^l 
Ja cfi +x^ 4a Jo 

,r = 1. 24. r 

1 a;2va;2 — 1 Jo 



e2* do; is non-existent. 



Determine the area between each of the following curves, the x- 
ajda, and the ordinates at the values of x indicated. 

25. 2/3(a:— 1)* = 1; a; = to9. Ans, 9. 

26. aJ2/2 (1 +a:)2 = 4; a; = to 4. Ans, 4 tan-i 2. 

27. 2/2a:4 (l+x) = 1; a; = to 3. Ans. 00. 

28. x^y^ (a;2 - 1) = 9; a; = 1 to 2. Ans. 2 x. 

29. 2/3 (a; _ 1)2 = 8 x3; a; = to 3. ilrw. 9 yl2 +9/2. 

30. a;22/2 (a;2 + 9) = 1; a; = 4 to 00. Ans. | log 2. 

31. j/2 (1 4. a;)4 = a?; a; = to 00 . Arw. x. 

32. 2/3(a: + l)2 = l;a; = 0to «. Ans, 00. 



CHAPTER XIII 
INTEGRALS AS LIMITS OF SUMS 

117. Step-by-step Process. The total amount of a variable 
quantity whose rate of change (derivative) is given [i.e. the 
integral of the rate] can be obtained in another way. The 
method about to be explained has many theoretical ad- 
vantages and one decidedly practical advantage, namely in 
its application to the approximate evaluation of integrals 
when the indicated integration cannot be carried out. 

For example, imagine a train whose speed is increasing. 
The distance it travels cannot be found by multiplying the 
speed by the time; but we can get the total distance approxi- 
mately by steps, computing (approximately) the distance 
traveled in each second as if the train were actually going at 
a constant speed during that second, and adding all these 
results to form a total distance traveled. 

If the speed increases steadily from zero to 30 mi. per hour, 
in 44 sec, that is, from zero to 44 ft. per second in 44 sec, 
the increase in speed each second (acceleration) is 1 ft. per 
second. Hence the speeds at the beginnings of each of the 
seconds are 0, 1, 2, 3, • • •, etc. 

If we use as the speed during each second the speed at 
the beginning of that second, we should find the total distance 
(approximately) 

s = + l + 2 + 3+--+42 + 43 = ^^-^ = 946, 

which is evidently a little too low. 

192 



XIII, § 117] INTEGRALS AS LIMITS OF SUMS 193 

If we use as the speed during each second the speed at the 
end of that second, we should get (approximately) 

44-45 
s = l + 2 + 3 + 4+... +43 + 44 = — 2— = 990, 

which is evidently too high. But these values differ only 
by 44 ft. ; and we are sure that the desired distance is between 
946 and 990 ft. 

If we reduce the length of the intervals, the result will be 
still more accurate; thus if, in the preceding example, the 
distances be computed by half seconds, it is easily shown 
that the distance is between 957 ft. and 979 ft.; if the 
steps are taken 1/10 second each, the distance is foimd to 
be between 965.8 ft. and 970.2 ft. 

Evidently, the exact distance is the limit approached by 
this step-by-step summation as the steps A^ approach zero: 



= 1 vdt= \ tdt= ^\ 
t^o Jt=o Jt^o 2J<=o 



968. 



We note particularly that the two results for s are surely 
equal; hence we obtain the important result: 

r°^\df = limit;] -Ai + t;] -A^ + vl -A/H [• 

118. Approximate Summation. This step-by-step process of 
sununation to find a given total is of such general application, 
and is so valuable even in cases where no limit is taken, that 
we shall stop to consider a few examples, in which the methods 
employed are either obvious or are indicated in the discussion 
of the example. 

Thus, areas are often computed approximately by dividing 
them into convenient strips. We have seen in § 55 that 
if A denotes the area under a curve between x = a and 



194 



THE CALCULUS 



[XIII, § 118 



x=b, then the rate of increase of A is the height h of the 

curve: 

dA 



y=R{x) 




dx 



= h = R(x), 



Fig. 46. 



where R (x) is the rate 
of increase of il, and is 
also the height of the 
curve. 
For a parabola, /i =a^, we may find the area A approxi- 
mately between x = — 1 and x = 2 by dividing that interval 
into smaller pieces and computing 
(approximately) the areas which 
stand on those pieces as if the height 
h were constant throughout each 
piece. If, for example, we divide 
the area A into six strips of equal 
width, each 1/2 unit wide, and if we 
take the height throughout each one 
to be the height at the left-hand 
corner, the total area is (approxi- 
mately) 

+ (f)*i = 19/8, 

whereas, if we take the height equal to the height at the 
right-hand comer we get 31/8. The area is really 3, as we 
find by § 55. Taking still smaller pieces, the result is of 
course better; thus with 30 pieces each yV ^^^^ wide, the 
left-hand heights give 2.855, the right-hand heights 3.155. 
With still more numerous (smaller) pieces these approximate 
results approach the true value of the area. (See § 119, p. 196.) 



















/ 


\ 








y 








r 




y 














1 






\ 






o 


y 




c« 


/ 






\ 






o 








/ 






\ 




n 






/ 








\ 




1 






y 










\ 




1 






/ 












^ 


1 




J 














\ 


^ 


_^ 


/ 












— 


I 







• 




4" 

4 

























Fig. 46. 



Xin, § 118] INTEGRALS AS LIMITS OF SUMS 195 

EXERCISES 

Approximate to about 1% the areas under the following curves, be- 
tween the limits indicated. Estimate the answers roughly in advance. 
Use judgment with regard to scales to gain accuracy by having the 
figure as large as convenient. Express each area as a definite integral 
and check by integration when possible. 

1. y = z^ — 4:x; a; = 2 to 6. 2. y = 1/x; a; = 10 to 20. 

8. i/ = »-2; a; = 1 to 5. 4. y = a;-3/2; a; = 2 to 4. 

5. y = — ^^— ; a; = 2 to 4. 6. y = rX"^ ' a? = to 2. 

7. y = 1/ Vl2 — x; x = 3 to 8. S. y = V9 — x; a; = to 5. 

9. y = I/V9 - a;2; a; = Oto 1.5. 10. y = V9 + x^; a; = to 4. 

11. y = ;— 1 — r-5— ; a; = Oto t/2. 12. y = — -, ; a; = to 1. 

'^ i + sm2 X* ' ^ e» + e-* ' 

^' y = (4 + a;2)3/2; ^ = 0*<^2. 14. 2/ - ^^^==; a; =0 to .5. 
15. y = V9+x4; a; = Oto 2. 16. y = (l-cosx)3/2;a;=0to2ir. 

17. y = r ; a; = to ir/6. 18. 2/ = tan~i x\ a; = to 1. 

V 4 — sin2 X 

^^- y l+si^a; > a;=0toir/2.20. l/^^f^aJ a; = 0to.5. 

21. y = e"^*; a; = to 1. 22. y = a; e~*'; a; = to 1. 

Approximate to about 1% the distance passed over between the indi- 
cated time limits, when the speed is as below; express each distance as a 
definite integral, and check by integration when possible. 

28. » = 4 < + «2; < = 1 to 3. 24. V = j^ ; < = to 50. 

26. V = ^}, ^ ; < = 1 to 4. 26. v = — ^^ ; < = to 100. 

2t + &' 1 + v^ 

27. V = o4-^ * < - 1 to 3. 28. V = ^r+l2; < = 10 to 20. 



196 



THE CALCULUS 



pan, 5 118 



29. Show how to lind the volume of a cone approximately, by adding 
together hyen perpendicular to it£ axis. 

30. Find the volume of a sphere by imagining it divided into small 
pyriunids with their vertices at the center and their bases in the surface, 
as in elementary geometry. 

31. The volume of a ship is computed by means of the areas of cross 
sections at small distances from each other; show how the result is cal- 
culated. Show how to make a more accurate computation by the same 
method. 



119. Exact Results. 



lummatioii Formula. Any definite 
integral 

CD §"j^'>'^ 
may be thought of as the 
area under a curve 
(2) l/=/{x) 

between the ordinates x = o 
and x = h. 

If the interval AB from 
x = aiox = bhe divided 
into n parts, each of width 
Ax, the whole area is approximately as ia § 118, 
{Z)S = ^x■f{a) + ^x^f{a-\-Ax)+■■■+^x■S{a + {n~l)^x). 
The term Ax-f(a) is the area of the rectangle ADiNiP, 
since f(a) = AP. Likewise Ax-f{a + Ax) is the area of 
DiD^sMi, etc. Hence the sum S represents the shaded 
area in Fig. 47. 

If the curve is rising from x = a io x = h, asm. Fig. 47, 
S is smaller than the area under the curve. On the other 
hand the similar sum 
(4) R = Ax-/(a + Ax) + ix-/(o + 2 Ai) + • ■ ■ • 

+ Ax-/(a + (n - 1) Ax) + Aj;-/(()) 





XIII, 1 120] INTEGRALS AS LIMITS OF SUMS 197 

is represented by the shaded area in Fig. 48, and R is too 

large if the curve is rising. 

Hence 

R>f''f(x)dx>S 

if the curve is rising. But, 
subtracting (3) from (4), we 
have 

(5) R~S = 

Ax[f{b)-f{<i)], 
and this approaches zero as 
Ax approaches zero. It 
follows that the true value of the int^ral is the limit of either 
R OT S m Ax approaches zero, i.e., as n becomes infinite, and 
we may write * 

(6) J/(x) dx=lim ^AxJ(a)+Axf{a + Ax) +■■■ 

+ Axfia + {n-l)Ax)^, 

at least if the curve rises from x = ato x = b. 

Similarly, the formula (6) is true also if the curve falls from 
X = a to X = b. Finally, if the curve alternately rises and 
falls, we may prove (6) by separating the interval into several 
parts, in some of which it rises and in some of which it falls. 

The formula (6) is called the summation formula of the 
integral calculus. 

120. fotegrals as Limits of Sums. By far the greater num- 
ber of integrations appear more naturally as limits of sums 
than as reversed rates. 



198 THE CALCULUS [XIII, § 120 

Thus, as a matter of fact, even the area A under a curve, 
treated in § 55 as a reversed rate, probably appears more 
naturally as the limit of a siun, as in (6), § 119. Of course 
the two are equivalent, since (6), § 119, is true; in any case 
the results are calculated always either approximately, as 
in the exercises under § 118, or else precisely by the methods 
of §§ 52-54. Hence the method of § 54 was given first, 
because it is used for each calculation even when the problem 
arises by a smnmation process. 

On account of the frequent occurrence of the sununation 
process, we may say that an integral really means* a limit of a 
sum, but when absolutely precise results are wanted it is 
calculated as a reversed differentiation. The S5rmbol J* is 
really a large S somewhat conventionalized, while the dx of 
the symbol is to remind us of the Ax which occurs in the 
step-by-step sunmiation. 

EXERCISES 

Express each of the following integrals as the limit of a sum, as in 
(6), § 119. Find its approximate value to about 1%, and check by in- 
tegration. 

1. f^^^^dx. 2. f^^rr-odX' 3- f^ ^^Tx^dx. 

J2 x—1 Jo l+x^ Jo 

4. / yl+xdx. 6. / sin xdx. 6. / cos a; dx. 

tgjixdx, 8. / sec xdx, 9. / logioxor. 

Jo «/io 

* It is really a waste of time to discuss at great length here which fact 
about integrals is used as a definition, and which one is proved; to satisfy 
the demand for formal definition, the integral may be defined in either way, — 
as a limit of a sum, or as a reversed differentiation. The important fact is that 
the two ideas coincide* which is the fact stated in the Summation Formula. 



I 
/ 
) 



XIII, § 121] INTEGRALS AS LIMITS OF SUMS 199 

Express each of the following quantities as the limit of a sum; find 
its approximate value to about 1%; check by integration. 

10. The area under the curve y = x2 from x == 1 to x = 3; from 
a: = — 3toa;=3. 

11. The area imder the curve y = 3^ from x =0 to x = 2; from 
a; = — ltoa; = H-l. 

12. The area under the curve x^y — 1 from x = 2 to a? = 6. 

18. The distance passed over by a body whose speed is v = 4 i + 10 
from < = to < = 3. 

14. The distance passed over by a falling body (v = gt) from t = 2 
to< =6. 

15. The increase in speed of a falling body from the fact that the 
acceleration is g = 32.2, from < = to < = 5. 

16. The increase in th§ speed of a train which moves so that its accel- 
eration isj = i/lQOj between the times < = and t — 6. The distance 
passed over by the same train, starting from rest, during the same in- 
terval of time. 

17. The number of revolutions made in 5 min. by a wheel which 
moves with an angular speed « = ^/lOOO (radians per second). 

18. The time required by the wheel of Ex. 17 to malce the first ten 
revolutions. 

19. Repeat Ex. 18 for a wheel for which w = 100 — 10 1 (degrees per 
second). Find the time required for the first revolution after < = 0; 
note that the speed is decreasing. 

20. The weight of a vertical column of air 1 sq. ft. in cross section and 
1 mi. high, given that the weight of air per cubic foot at a height of h feet 
is .0805 ~ .00000268 h pounds. 

121. Volume of any Frastum. To illustrate the ease of 
application of this process, consider again the volume of a 
frustum of a solid. (See § 57.) 

If such a frustiun be divided up into layers of thickness 
A«, by planes parallel to the base, and if As represents the 
area of any section at a distance s from the lower bounding 



200 



THE CALCULUS 



[XIII, § 121 



plane, the volume of each layer is, approximately, the 
product of its thickness As times the area A, of the bottom 
of the layer: 

(1) Volume of one layer = AgASj approximately. 

Now if we replace x in (3), § 119, by s, and if Ag = /(s), the 
sum of all such layers would be, approximately, 

AS'fia) + Ax'f(a + As) + + As'f(a+{n - l)As). 

Hence, by (6), § 119, the exact total volume is 

Asds= I f(s)ds. 

This formula is the same as that derived in § 57. It may 

be used to find the 
volume of any solid, 
if we know how to 
Ing^g^Ag find the areas of 
any such complete 
set of parallel cross 
sections. 

In particular, if 
the solid is a solid 
of revolution, the 




\8^S 



xs^a 



8^0 



Fig. 49. 

preceding formula reduces to formula (4) of § 56. 

122. Surface of a Solid of Revolution. Similarly any such 
formula is readily derived, and easily remembered by means 
of this new process. Thus the formula for the surface of a 
solid of revolution was derived in § 85. To obtain that 
formula, or to remember it, we may remark that the curved 
area of any short section is approximately 

AA = 2 Try As, 
since the ciured area is approximately the area of a section 



XIII, § 123] INl^GRALS AS LIMITS OF SUMS 



201 




Fig. 50. 



of a cone. It follows readily that the total area of such a 
surface is 

A = \2Tryds 

123. Water Pres- 
sure. As another 
typical instance, con- 
sider the water pres- 
sure on a dam or on 
any container. The 
pressure in water in- 
creases directly with 

the depth A, and is equal in all directions at any point. 
The pressure p on unit area is 

(1) p = k'h 

where h is the depth and k is the weight per cubic unit 

(about 6.24 lb. per cubic foot). 

Suppose water flowing in a paraboUc channel, Fig. 51, 

whose vertical sec- 
tion is the parabola 

x^ = 225 y. 

Let a be the depth 
of the water in the 
channel. If a cut- 
off gate be placed 
across the channel, 
let it be required 




-H 1 * — f^ 

-200 -160 -100 -W O 



60 

Fig. 51. 



150 200 a; 



to calculate the total pressure on the gate. 



202 THE CALCULUS [XIII, § 123 

Consider a horizontal strip of height Ah, whose upper 
edge is h below the surface. The area of such a strip is its 
width, Wy times its height, Ah, Hence the pressure on the 
strip is, approximately, 

pressure on horizontal strip = (k - h)w - Ah 

In this example, w? = 2x = 2 V225y = SOy^^, h = a — y, and 
Ay = Aft. Hence 

pressure on horizontal strip = 30 fc (a — y)y^^^ Ay, 

and the sum of the pressures on all such strips is the sum of 
such terms as this one. Hence, by (6), § 119, the correct 
total pressure is 

P = 30 fc P*^"* (a - y) y'^Hy 

= 3« ' [w - 5T2J0 = « *-'^' 

where fc = 62.4 lb., and a is the total depth of the water. 

EXERCISES 

1. Find the volume generated by revolving Vx + Vy = Va about 
the ic-axis, from x = to a; = a. 

2. Find the volume of the paraboloid z = x^/a^ + y^/b, from 2 = 
to h. 

3. Find the volume of the cone z^ = x^/a^ -f y^/i^, from 2 = to ft. 

4. Find the volume of a regular pjo-amid of base B and height ft. 

6. On a system of parallel chords of a circle are constructed equi- 
lateral triangles whose bases are those chords and whose planes are 
perpendicular to the plane of the circle. Find the volume in which 
all these triangles are contained. 

6. On the double ordinates of an ellipse are constructed triangles 
of fixed height ^, with planes perpendicular to the plane of the ellipse. 
Find the volume contaming all these triangles. 

7. Find the volume generated by a variable square whose center 
moves along the x-axis from a; = to ir, the plane of the square being 
perpendicular to the x-axis, and the side proportional to sin x. 



XIII, § 124] INTEGRALS AS LIMITS OF SUMS 203 

8. Find the surface of the spheroid generated by revolving the 
ellipse y2 ~ (1 _ g2) ((,2 -_ a;2) about the x-axis. 

9. Find the surface generated by revolving the catenary y = 
(e» -\-e~*)/2 about the x-axis, from x = to a. 

10. As in Ex. 9 for the hypocycloid x^/a + y2/8 = aP/8^ from x = 
—a to a. 

11. As in Ex. 9 for one arch of the cycloid. 

12. Find the surface generated by revolving p = a cos B about the 
initial line. 

18. As in Ex. 12 for the cardioid p =» a(l + cos B), 

Calculate the following pressures: 

14. On one side of the gate of a dry dock, the wet area of the gate 
being a rectangle 80 ft. long and 30 ft. deep. 

15. * One side of a board 10 ft. long and 2 ft. wide, which is submerged 
vertically in water with the upper end 10 ft. below the surface. 

16. On an equilateral triangle 20 ft. on a side, submerged in water 
with its plane vertical and one side in the surface. 

17. On one side of a square tank 10 ft. high and 5 ft. on a side, the 
tank being filled with a liquid of specific gravity .8. 

18. On one face of a square 10 ft. on a side, submerged so that one 
diagonal is vertical and one comer in the surface. 

19. On one end of a parabolic trough filled with water, the depth 
being 3 ft. and the width across the top 4 ft. 

20. On one side of an isosceles trapezoid whose upper base is 10 ft. 
long, parallel to the surface and 10 ft. below it, whose lower base is 
20 ft. and altitude 12 ft. 

21. What is the effect on the pressure if all dimensions given in Ex. 20 
are multiplied by a constant c? 

124. CavaUeri's Theorem. The Prismoid Formula. If two 
solids contained between the same two parallel planes have 
all their corresponding sections parallel to these planes equal, 
i.e. if the area A\ of such a section for the first solid is the 
same as the area A'\ of the second, it follows from § 57 that 
their total volumes are equal, since the two volumes are 
given by the same integral. 



204 THE CALCULUS [XIII, § 124 

This fact, known as Cavalieri's Theorem, is often useful in 
finding the volumes of solids. 

If the area Ag of any section of a frustum is a quadratic 
function of s: * 
(1) As = as^ + bs + c, 

where, as in § 57, s represents the distance of the section Ag 
from one of the two parallel truncating planes, the voliune is 

= I (as^ + bs + c)ds^\a'- + b% + cs\ 

»-0 Je-0 L O Z J»-0 

ah" , bh" , , 

where h is the total height of the frustum. 

The area B of the base of the frustum, the area T of the top, 
and the area Af of a section midway between the top and 
bottom are 

B =^]^_Q = [«s^ -\-bs + c^^ = c; 

T =A,'\ = {a^ + bs + c\ = aA* + bh + c: 

J|f=^l =ras2 + 6s + cl =a^+b^ + c. 

If we take the average of 5, T, and 4 times M: 

B + T + 4M _ah^ bh 

6 -3^2"^^' 

this average section multiplied by the total height h turns 
out to be exactly the entire volume: 



,^. B+T + 4.M ^. aK" bh^ . , n*-A 

* It is shown in Ex. 3, p. 206, that the results of this section hold also 
when Aa is any cubic function of «; A, = as* -}- fes^ + c« + d. Notice also 
that any linear function &« -|~ c is a special case of (1), for a » 0. 



XIII, § 124] INTEGRALS AS LIMITS OF SUMS 



205 



This fact is known as the prismoid formula. It is easy to 
see by actually checking through the various formulas, 
that this formula holds for every solid whose volume is given in 
elementary geometry; the same formula holds for a great 
variety of other solids* But the chief use to which the 
formula is put is for practical approximate computation 
of volumes of objects in nature: it is reasonably certain that 
any hill, for example, can be approximated to rather closely 
either by a frustum of a cone, or of a sphere, or of a cylinder, 
or of a pyramid, or of a paraboloid; since the prismoid 
formula holds for all these frusta, it is quite safe to use the 
formula mihout even troubling to see which of these solids 
actually approximates to the hill. Similar remarks apply 
to many other solids, such as metal castings, though it may 
be necessary to use the formula several times on separate 
portions of such a complicated object as the pedestal of a 
statue, or a large bell with attached support and tongue. 

Example. The prismoid formula 
applies to any frustum of an 
ellipsoid of revolution cut off by 
planes perpendicular to the axis 
of revolution. 

Let the origin be situated on one 
of the truncating planes of the frus- 
tum, and let the axis of x be the 
axis of revolution. Then the equa- Fig. 52. 

* The formula holds also, for example, for any prismoid, i.e. for a solid 
with any base and top sections whatever, with sides formed by straight 
lines joining points of the base to points of the top section. For example, 
any wedge, even if the base be a polygon or a curve, is a prismoid. The 
solids defined by (1) include all these and many others; for example, spheres 
and paraboloids, which are not prismoids. The formula holds for all these sol- 
ids and even (see Ex. 3, p. 206) for all cases where A, is any cubic function 
of 8. One advantage of the formula is that it is easy to remember: even 
the formula for the volume of a sphere is most readily remembered by re- 
membering that the prismoid formula holds. 




206 THE CALCULUS [XIII, § 124 

tion of the generating ellipse is of the form Ax^ -f By^ -f Da; + F = 0. 
The area A^ of a section parallel to the bases is inp'^ since the section is 
a circle whose radius is y. Hence 

which is a quadratic function of the distance x from one of the truncating 
planes of the frustum. Therefore the prismoid formula holds. 

Beware of applying the prismoid formula, as anything but an ai>- 
proximation formula, without knowing that the area of a section is a 
quadratic function of s, or (Ex. 3, p. 206) a cubic function of «. 



EXERCISES 

[This list includes a number of exercises which are intended for 
reviews.] 

1. Show that the prismoid formula holds for each of the following 
elementary soUds; hence calculate the volume of each of them by that 
formula: (a) sphere; (6) cone; (c) cylinder; (d) pyramid; (e) frustum 
of a sphere; (/) frustum of a cone. See Tables, II, F. 

2. Calculate the volume of the solid formed by revolving the area 
between the curve y = x^ and the x-axis about the x-axis, between 
X = 1 and a; = 3. Find the same volume (approximately) by the 
prismoid formula, and show that the error is about 0.6%. 

3. Calculate the volume of a frustum of a solid bounded by planes 
^ = and h — HjH the area As of a parallel cross section is a cubic 
function aA^ _^ 5^2 _j_ ^^ -f rf of the distance h from one base, first by 
direct integration, then by the prismoid formula. Hence prove the 
statement of the footnote, p. 205. 

4. In which of the exercises relating to volumes on p. 97 does the 
prismoid formula give a precise answer? 

5. How much is the percentage error made in computing the volume 
in Ex. 7, p. 97, from a; = 1 to a; = 3, by use of the prismoid formula? 

6. Show, by analogy to § 64, that the area under any curve whose 
ordinate y is any quadratic function (or any cubic function) of x, between 
a; = a and a; = 6, is 

^ [VA + ^VM + 2/bI, 

where y^, 2/b, yM represent the values of 2/ at a; = a, a; = 6, a; = (a + 6) /2, 
respectively. 



XIII, § 124] INTEGRALS AS LIMITS OF SUMS 207 

Calculate, first by direct integration, and then by the rule of Ex. 6, 
the areas under each of the following curves: 

7. y=x^ + 2x-\-S between x = 1 and a; = 5. 

8. y=x^ — 5x + 4: between a; = and x = 5. 

9. y =x^ + 5x between x = 2 and x — 4, 

10. Calculate approximately the area under the curve j/ = x* between 
ic = 1 and a; = 3 by the rule of Ex. 6. Show that the error is about .55%. 

11. Show that any integral whose integrand/ (x) is a quadratic (or a 
cubic) function of x, can be evaluated by a process analogous to the pris- 
moid rule: 

12. Evaluate the integral^ (l/x^) dx between x = 1 and a; = 5 approx- 
imately, first by the rule of Ex. 11; then by applying the same rule 
twice in intervals half as wide; then by applying the rule to intervals of 
unit width. 

18. Show that any integraiy/ (x) dx can be computed approximately 
by using Ex. 11 with an even number of intervals of small width Ax: 

y""" /(a;) dz =r/(a) +4/(a + Aa;) +2/(a + 2 Ax) +4/(a + 3 Aa;) 

+ --+/(6)]f • 

[This rule is called Simpson's Rule.] 

Calculate the following integrals approximately by Simpson's Rule. 
Notice that some of them cannot be evaluated otherwise at present. 



14. f^T^dx, 16. f \/xdx. 18. C vT+^^ci 

^0 •'0 •'0 

(1/x) dx. 17. / V 1 4- X dx. 19. / sm x dx. 



20. Find approximately the length of the arc of the curve y = x^ from 
x = to X = J; from x = J to x = 1. 

21. Find approximately the area of the convex surface of that portion 
of the paraboloid formed by revolving the curve y = Vx about the x-axis 
which is cut off by the planes x = and x = J; by x = J and x = 1, 



CHAPTER XIV 

MULTIPLE INTEGRALS —APPLICATIONS 

126. Repeated Integration. Repeated integrations may be 
performed with no new principles. Thus 

\ -^dx = he; and If f- cjdx = — log x + cx+ c\ 

The final answer might be called the second integral of 1/x^. 
Thus, in the case of a falling body, the tangential accelera- 
tion is constant: 

dv 

where g is the constant; hence 

^ = Sjrdt + const. = — gfi + c; 
but since v = ds/dty 
s =J'vdt + const, =y(— gt + c) cK + const. = —^ + ct + c\ 

If the body falls from a height of 100 ft., with an initial 
speed zero, s = 100 and t; = when ^ = 0; hence c = and 
c' = 100, whence we find 

s = - gt^l2 + 100. 

The equations s = fv dt + const., v = J'jr dt + const., just 

obtained, apply in any motion problem, where jr is the 

tangential accelerationj v is the speed, and s is the distance 

passed over. 

208 



XIV, §126] MULTIPLE INTEGRALS— APPLICATIONS 209 



126. Successive Integration in Two Letters. A distinctly 
different case of successive integration which can be per- 
formed without further rules is that in which the second 
integration is performed with respect to a different letter. 

Thus, the volume of any solid is (§ 57), 



(1) 



rh==b 



As dh, 



where Ag is the area of a section perpendicular to the direc- 
tion in which h is measured, and where h = a and h = b de- 
note planes which bound the solid. 

In many cases it is convenient first to find A, by a first 
integration, by the methods of § 55, and then integrate 
As to find V by (1), this second 
integration being with respect 
to the height h. 

Example 1. Find the volume of 
the parabolic wedge 

2/2 = x (1 - 2)2 

between the planes 2 = and 2 = 1 
and between the planes x = and 
a; = 1. 

The area A, of a section by any 
plane z = h parallel to the xy-plsme is twice the area between the curve 

y = (I — h) Vx and the a;-axis: 




Fig. 63. 






x=\ 
x^O 



= 3(1-^), 



hence this volume, by (1), is 

]»=! ^A=i 4 /.»=! , „ 4/, A2\n*=i 2 

Notice that A, during the first integration, was essentially constant. 



210 THE CALCULUS [XIV, § 126 

Combining the formulas used in this example, the volume 
V may be written 

This result is usually written without the brackets on the 

right: 

-[fc-i rh^i rx=i y- 

V\ =2 {l-h)Vidxdh. 

Such double integrals in two letters are very common in 
applications. 

Examples of triple integrals will be found further on in 
this chapter. 

127. Volumes. Double Integrals. Analogous to the problem 
of finding the area under a given portion of a curve, 
(§§ 55, 119), there is the problem of finding the volume under 
a given portion of a surface.* This leads to double integrals. 

Let A'B'C'D' be a portion of a curved surface whose 
equation is 

z = F(x, y). 

Let ABCD be the projection of A'B'C'D' on the xy 
plane, curve CD being the projection of curve CD', 

The problem is to express the volume between the portion 
A'B'C'D' of the surface and its projection on the a:2/-plane. 

Divide this volume into slices of thickness PQ = Ax, by 
planes parallel to the i/z-plane, and further subdivide the 
slices into prismatic columns by planes parallel to the 
an/-plane spaced at intervals Ay, 

The area of the section PSS'P' depends on the position 

* See Tables, I, b, for formulas from Solid Analytic Geometry. 




XIV, 5127] MULTIPLE INTEGRALS— APPUCATIONS 211 

of P, hence on x, and is therefore a function of x. Therefore 
by the frustum formula {§ 57), 
the required volume is 

]x-b fi-b 
^ ^= I ^A^dx. 

But the area Ax is the area 
under the curve P'S' whose 
ordiuates (heights above xy- 
plane) are 2 = F{x, y), where 
X has the fixed value OP and 
y alone varies from y = to 
y = PS =f{x), this being Fw. 64. 

the equation of curve DC, supposed given. 
Hence 

Then 

<" ''J. " J... X-o f(^.l')*<^- 

This is essentially the same sort of problem as that 

discussed in § 126. 

This double int^ral may be written as the limit of a 

double sum. For if we consider the prismatic column on Ax Aj/ 

as base, its volume approximately is s ir Ay or F{x, y) Ay Ai. 
This su^ests the double sum 

or, as it is usually written, 



212 THE CALCULUS [XIV, § 127 

Here the limit of the inner summation is merely A, and then 
the limit of the outer summation is the integral of A or the 
volume. Hence we write the formula 



(2) iimi:::i:ro'>(a:,j/)Aj/Ax 



Ai/-»0 



x=h >,y-/(x) 






dx. 



This is the fundamental summation formula for double 
integrals. 

Example. Determine the volume under the surface z = x^+y^ 
between the xa-plane, the planes x = 0, a; = 1, and y = 0, and the 
cylinder y = Vx. 



z=x^ 



z= 




Fig. 55. 



/ {x^+y^)dydx 

J x=o L Jo 

= y ra;5/2 + (1/3) a;3/2"| da; = 44/105. 



XIV, § 127] MULTIPLE INTEGRALS— APPLICATIONS 213 

EXERCISES 

1. Determine a function y — f (x) whose second derivative d^/dx^ 
is 6 X. Ans. y = x^ + CiX + C2. 

2. Determine the speed v and the distance s passed over by a particle 
whose tangential acceleration cPs/dfi is 12 t. Find the values of the arbi- 
trary constants if t; = and s = when ^ = 0; if v = 100 and « = 
when ^ = 0. 

Find the general expressions for functions whose derivatives have 
the following values: 

3. d^/dx^ = 6 x2. 6. dh/d0!^ = l/Vl - d. 9. d^/dx^ = ef. 

4. d^a/dfi = 3 + 2 <. 7. dh/de^ ^6^-29, 10. d^s/dfi = sec2 1. 

6. d^a/dfi = Vl-t. 8. dh/du^ = 1 - m2. 11. dh/du^ = l/w2. 

Determine the speed v and distance s passed over in time t, when 
the tangential acceleration jV and initial conditions are as below: 

12. JT = sin <; t; = and 8=0 when ^ = 0. 

13. ir = ^ + cos t; v = and « = when ^ = 0. 

14. jj. = VY+1; v = 3 and 8 = when t = 0. 
16. JT = t/Vl + ^2j t; = 1 and 8 = when < = 0. 

Evaluate each of the following integrals, taking the inner integral 
sign with the inner differential: 

16. / / xydydx. 21. f f f -^drdsdt. 



/ 6 a;2(2 - 2/)d2/ dx. 22. / / (x-{-y)dydx. 

xasQ •^ y—1 •/a:=-l •/y=—i» 

/ (x2 + l)(4-2/2)(i2/dx. 23. / / (x -{- y)^ dy dx. 

x=*0 •/v«2 •/ x=0 •/y=l 

/ Vu + vdudv. 24. / / / (x-{-y+2)dzdydx. 

20. /^°' f^^'' ^^^ dy dx, 26. T' T'' r ^r^amdded<t>dr. 

J x-\ Jv=o X Jo Jo Jo 

26. Find the volume of the part of the elliptic paraboloid 4 x^ + 
9 2^2 — 35 between the planes 2 = and 3 = 1; between the planes 
a = a and 3 = 6. 



214 THE CALCULUS [XIV, § 127 

27. Find the volume of the part of the cone 3 x^ -f 9 2/^ = 27 a? 
between the planes 2 = and 3 = 2; between 3 == a and z = b. 

28. Find the volume of the part of the cylinder a;2 + 2/2 = 25 between 
the planes 3 = and 3 = x; between the planes a = x/2 and 3 = 2 a;. 

29. A parabola, in a plane perpendicular to the x-axis and with its 
axis parallel to the 3-axis, moves with its vertex along the x-axis. Its 
latus rectum is alwa3rs equal to the oK^oordinate of the vertex. Find 
the volume inclosed by the surface so generated, from 3 = to s = 1 
and from x = to x = 1. 

30. Find the volume of the part of the cylinder a;* + j/* = 9 lying 
within the sphere x^ -\- y^ ■}- z^ = 16. 

31. For a beam of constant strength the deflection y is given by the 
fact that the flexion is constant: b = cPy/da:^ = const, if the beam is of 
uniform thickness. Find y in terms of x and determine the arbitrary 
constants if y = when x = ± 1/2. [This will occur if the beam is of 
length If and is supported freely at both ends.] 

32. Determine the arbitrary constants in the case of the beam of 
Ex. 31, if y = and dy/dx = when x =0. [This will occur if the beam 
is rigidly embedded at one end.] 

33. For a beam of uniform cross section loaded at one end and rigidly 
embedded at the other, b = d^/dx^ = k(l — x) where I is the length of 
the beam, x is the distance from one end, and A; is a known constant 
which is determined by the load and the cross section of the beam. Find 
y in terms of x, and determine the arbitrary constants. 

Find y in terms of x in each of the following cases: 

34. d^y/dx^ = A;(P - 2 te + x^); y = 0, dy/dx = when x-0. 
[Beam rigidly embedded at one end, loaded uniformly.] 

36. d^/dx^ = a + &r; 2/ = 0, dy/dx = when a; = 0. 
[Beam of uniform strength of thickness proportional to (a + bx)^^, 
embedded at one end.] 

36. d^/dx^ = A;(P/8 - x*/2); y = when x = ± 1/2. 
[Beam supported at both ends, loaded uniformly.] 

37. d^/dx^ = k/x^; y = 0, dy/dx = at x = Z. 

[Beam of uniform strength of thickness proportional to x^, embedded 
at x = L] 

88. Find the angular speed co and the total angle 6 through which a 
wheel turns in time t, if the angular acceleration is « = d^O/dl^ = 2 <, 
and if ^ = w = when < = 0. 



XIV, § 129] MULTIPLE INTEGRALS— APPLICATIONS 215 

128. Triple and Multiple Integrals. There is no difficulty 
in extending the ideas of §§ 126-7 to threefold integrations 
or to integrations of any order. Following the same reason- 
ing, it is possible to show that, ii w = F{Xyy, z) 

1«^ lilZ JZ'^ liZl w^xAyAz 

Ax— *0 
Az-*0 

I I F (x, y, z) dx dy dz, 

where the three integrations are to be carried out in succes- 
sion, where the limits for x may depend on y and 2, and where 
the limits for y may depend on z\ but the limits for z are, of 
course, constants. 

Thus it is readily seen that the volume mentioned in 
§ 127 may be computed by dividing up the entire volume by 
three sets of equally spaced planes parallel to the three coor- 
dinate planes. Then the total volume is, approximately, 
the sum of a large number of rectangular blocks, the volume 
of each of which is Ax Ly Lz\ and its exact value is 

Ax— >0 

Air-^ 

A«->0 

I I dzdy dx, 

which reduces to the result of § 127, if we note that 

dz = z\ = F{x, y). 

129. Plane Areas by Double Integration. To find the area 
bounded by a closed curve C, we divide it into small ele- 
ments of area, either by lines drawn parallel to the coordinate 
axes if the equation of C is given in rectangular coordinates. 



216 THE CALCULUS [XIV, 1 129 

or by a system of radial lines and concentric circles if the 
equation of C is given in polar coordinates. (Figures 56, 57.) 





75=^^-- 




w 




\ 


: t 




^y 


lil J 








J _ 


- 5^ 




_^^ 


t''' 


n 






In Fig. 56 let any ordinate whose abscissa is x meet the 
boundary of the area in P and Q, the corresponding values 
of 3/ being j/i and y-x- Let the extreme values of x between 
which the oval lies be i = a and x = 6. Then the area will be 

(1) 



A = lim E^ „ E" "' Am Ai = I I dy dx. 



This is merely a special case of (2), § 127, when Fix, y) = 1, 
because the volume of a right cylinder of height 1 equals the 
area of the cross section. 

In Fig. 57 let any radius vector whose angle is 8 meet the 
boundary of the area in P and Q, the corresponding values 
of p being OP = pi, OQ = pj. Let the extreme values of 
Ohe d = a and 6 = ^. Then the element of area is approxi- 
mately pA6 ■ Ap and the total area is 

(2) A - Iimy\*:fr'I"pApA(J= f'^" f''^'"pdpd$. 



XIV, S129] MULTIPLE INTEGRALS— APPLICATIONS 217 

In fonnulas (1) and (2) the first integration can be carried 
out at once, giving 
(1') A=J\y^-y,)dx (2') A = fj (p^- pv') dff. 

The last results may also be derived from the formula of 

§ 55 and § 92, so formulas (1) and (2) may be dispensed with 
so far as the mere calculation of plane areas is concerned. 
We shall, however, find the idea of a plane area as the limit 
of a double sum very useful in the following sections. 

Example 1. Find the area between the parabola j/' = 4 (x — 1) and 
theline!/ = a;-l. {Fig. 58.) 

The extreme values of x are found to be x = 1 and x = 5. Hence 

^ = fll /"" _' dydx=f r2v7^n-(j;-I)"j(ir 

= [4/3 {X - l)»/s - l(r - !)»]'= 8/3. 



IE 




Fro. 68. 

ExAUPij; 2. Find the area between the circle p = cob 6 and the car- 
dioid p - 1 + COB 8, from fl = to 45°. (Fig. 69.) 

= f''*h [(1 + coa e)s - C03! fl] de 

= if'^*il + 2 COB e) rffl = i {t/4 +V2). 



218 THE CALCULUS [XIV, § 129 

EXERCISES — DOUBLE INTEGRALS 

1. Find the volume under the surface s = x^ -f ^2 between the x&- 
plane, the planes a; = and x = 1, and the cylinder whose base is the 
curve J/ — a;2. 

Find the volume between the a:^-plane and each of the following 
surfaces cut off by the planes and surfaces mentioned in each case: 

2. « = X + J/ cut off by y = 0, X = 0, X = 1, J/ = Vx. 

3. a = x2 H- y cut off by y = 0, X = 1, X = 3, y == x2. 

4. 2 — x^ cut off by 2/ = 0, X = 2, X = 4, J/ = x2 -f 1, 
6. a = xj/ + j/2 cut off by y = 0, X = 1, X = 5, J/ = x*. 

6. 2 = y -\- y/x cut off by 2/ = 0, X = 0, X = 1, y = x^. 

7. 3 = x2 + y3 cut off by X = 0, y = 1, y = 4, y2 =aj. 

8. a = Vx +y cut off by X = 0, y = 2, y = 5, y = X. 

9. s = x2 + 4 y2 cut off by y = and y = 1 — x^. 

10. 2 = xy cut off by y = x^ and y = 1. 

11. a = x2 — y2 cut off by y = x^ and y = x. 

12. Find the volume of the portion of the paraboloid a == 1 — x^ — 
4 2/2 which lies in the first octant. 

13. If two plane cuts are made to the same point in the center of a 
circular cylindrical log, one perpendicular to the axis and the other mak- 
ing an angle of 46° with it, what is the volume of the wedge cut out? 

14. Show that the volume common to two equal cylinders of radius a 
which intersect centrally at right angles is 16 a^/S. 

16. Show that the volume of the ellipsoid x2/16 + y2/9 + a?/4 = 1 
is 32 IT. 

16. How much of the ellipsoid in Ex. 15 lies within a cube whose 
center is at the origin and whose edges are 6 units long and parallel to the 
coordinate axes? 

17. Where should a plane perpendicular to the x-axis be drawn so as 
to divide the volume of the ellipsoid in Ex. 15 in the ratio 2:1? 

Calculate by double integration the areas bounded by the following 
curves: 

18. 2/ = x2 and y = Vx. 22. x = 0, 2/ = sin x, and y = cos x. 

19. 2/ = a;2 and y =x8. 23. 2/ = 0, 2/^ = x, and x2 — y2 = 2. 

20. 2/ = a;2 and — x2 + 2/^ = 2. 24. y = 2 x, 2/ = 0, and y = 1 — x. 

21. x2 + 2/2 = 12 and y == x2. 26. 2/2 = x, and y = 1 — x. 



XIV, §130] MULTIPLE INTEGRALS— APPLICATION 219 



Determine the entire area, or the specified portion of the area, 
bounded by each of the following curves, whose equations are given in 
polar coordinates: 

26. p = 2 cos e. 27. One loop of p = sin 2 ^. 

28. One loop of p = sin 3 ^. 29. The cardioid p = 1 — cos d. 

30. The lenmiscate p^ = cos 2d. 31. The spiral p = 6, from ^ = to ir. 

32. The spiral pd = 1, from 6 = ir/4 to ir/2. 

33. p = 1 H- 2 cos dy from ^ = to ir. 

34. p = tan 6, from ^ = to 45°. 

36. p =a^, one turn. 36. p = 3 cos d + 2. 

37. p = a sin ^ cos 9/(am^ d + cos^ 0); folium: the loop. 

130. Moment of Inertia. When a particle of mass m re- 
volves in a plane about a point 0, 
with given angular speed w, its speed 
is t; = rw, and its kinetic energy is 
E = 1/2 mv^ = 1/2 mr'u)^ The mo- 
ment of inertia of m about is 
defined as the product of the mass m 
by the square of its distance from 0, Fig. 60. 

I = 7^m. Thus E is easily foimd where / is known. 

Given now a thin plate of 
metal of uniform density and 
thickness, whose boundary C is 
a given curve, let us divide the 
plate into small squares by lines 
equally spaced parallel to two 
rectangular axes through 0. 
Let P be a point in any one of 
these squares and let OP = r = 
V?+^. Then the mass of 




V 
















^ 


^ 








^ 












/ 












> 


J. 




• ■ 


J 
















A 




A^ 


f 






Pj 


f 






i 


! 


f 








/ 








I 




i 






/ 










J 








V 




J 


r 








y 


f 








> 


\^ 


f 








y 


r 












r 


^ 






y 













/ 


/ 


> 


t 
















i 


t^ 


c-^ 






X 



Fig. 61. 



220 THE CALCULUS [XIV, § 130 

the square is k- Ay Ax where k denotes the constant surface 
density {i.e. the mass per square unit) ; and the moment of 
inertia of this square about is, approximately, k-r^ Ay Ax. 
Hence the moment of inertia / of the entire plate about is: 

Ax-»0 

The limits of integration are to be taken so as to cover 
the area, as in § 129. 

Thus the moment of inertia of a plate bounded by the 
two curves i/ = (1 — x^) and y ={x^ — 1), about the origin 
(draw the figure) is: 

I (x^ + y^)dydx 

where k is the surface density. 

The moment of inertia about an axis is defined similarly, the 
distance r being replaced by the distance of P from the 
given axis. Thus the moments of inertia of the plate in 
the figure about the x- and i/-axes are, respectively, 

Ix = kJJy^dydx; Iy = kj'j^x^dydx. 

The radius of gyration of an area, whether about a point or 
about an axis, is defined by 

radius of gyration = K = Vl/M. 

If the boundary of the plate is given in polar coordinateSj 
the moment of inertia about is calculated by dividing the 
area into elements rABAr. (See § 129.) Then 



XIV, §131] MULTIPLE INTEGRALS— APPLICATIONS 221 

Thus for a circle whose center is 0, r = / (6) = a, the 
radius. Hence the moment of inertia of a circular disk 
about its center is: 

J 0=0 L4 Jp=o J tf=o 4 2 2 

where fc is the surface density, and M = kra^ is the mass of 
disk. 

131. Moments of Inertia in General. The moment of inertia 
of any mass about a given point may be defined as follows. 

Divide the mass M into elements of mass Am; multiply 
each element Am by the square of its distance, r^, from the 
given point; the limit of the sum of these products is the 
required moment of inertia: 

(1) / = lim 2] ^Am = fr^dm, 

Am->0 

When M is a plate we take Am = kAA, where k is the 
mass per unit area, and AA = Ay Ax or rA ^ Ar, as in § 129. 

When Af is a thin wire bent into the form of a given 
curve, Am = fcAs, where k is the mass per unit length and 
As the element of length. 
Then 

(2) 7=2 kr^ As = kfr^ ds, 

the limits being taken to cover the given curve. For ds we 
use (1) of § 82 or (1) of § 93. 

When ilf is a solid body, we take Am = kAV, where k is 
the mass per unit volume and AF is the element of volume, 
Ax Ay Az. 
Then 

(3) / = lim *^E2m r^AxAyAz = kfffr^ dx dy dz. 

Ax—*0 
Aa-»0 



222 



THE CALCULUS 



[XIV, § 131 



The limits of integration are to be taken to cover the given 
volume. 

For the moment of inertia about an axis we let r in forms 
(1), (2), (3), be the distance of Am from that axis. 

Example 1. Find / for a wire bent into the form of a circular 
quadrant, about the center. 

Using polar coordinates, ds —rddj and 

I -^k f r^dd='kr^ I dd 
JO Jo 

= At3 t/2 = Mr^y since M = kv r/2. 





/ 






^__i 



Fig. 62. 




Fig. 63. 



Example 2. Find / for a circular cylinder of height H and radius 
R about the center of one base. 

The equation of the surface is a;2 + ^ = R^^ if the 2-axis is the axis 
of the cylinder. Then, by symmetry, 

/ / (x^ + y^ -h z^) dz dy dx, 

x^O J v»0 J c=0 

x—0 J I/-0 

^4tkH f (x2 2/ + 2/8/3 + i^ 2//3) dx 

•/ a:=0 

^4tkH f'''\x^ Vi22-a;2 + (i22 - a;2)3/2/3 + [p VR^ - xVZ) dx. 



XIV, §131] MULTIPLE INTEGRALS— APPLICATIONS 223 
Let X = i2 sin ^. Then 

ir/2 

7=4 kHE^f (722 sinZ 6 cos2 (? + 722 cos^ B/Z + ff2 cos2 e/2) de 

= 4 A;iyiE2 (722 ^/i6 + igs ^/i6 + 16 + fl2 ^/i2) 
= A;^i22 (3 i22 + 2 iy«) (ir/6). 

EXERCISES 

Calculate / about the origin for the areas bounded by the following 
curves (Density = A; = 1): 

1. y = x^ and y = Vx, 6. a; = 0, 2/ = sin x, and y = coax 

2. 2/ = x2 and 2/ = a:^. 6. 2/ = 0, 2/2 = x, and a;2 - 2/2 = 2. 

3. 2/ = a;2 and — x^ + y^ = 2. 7. 2/ = 2 x, 2/ = 0, and 2/ = 1 — a;. 

4. a;2 + 2/2 = 12 and 2/ = x^. 8. 2/^ = x, and 2/ = 1 — a;. 

Find the moment of inertia and radius of gyration of each of the 
following shapes of thin plate: 

9. A square about a diagonal. About a comer. 

10. A right triangle about a side. About the vertex of the right angle. 

11. A circle about its center. 

12. An ellipse about either axis. About the center. 

13. A circle about a diameter. 

14. A triangle of given base and height, about the base. 

15. A trapezoid about one of its parallel sides. 

16. A thin circular plate, about a point on the circumference. 

17. A thin plate bounded by two concentric circles, about the center. 

18. An equilateral triangle, about its center. 

19. An equilateral triangle, about one vertex. 

20. p = 2 cos d. 

21. One loop of p = sin 2 0, 

22. One loop of p = sin 3 6. 

23. The cardioid p = 1 — cos 0. 

24. The lemniscate p2 = cos 2 0, 



224 



THE CALCULUS 



[XIV, § 131 



26. The spiral p = 6, from ^ = to ir. 

26. The spiral pd = 1, from d = ir/4 to t/2. 

27. p = 1 + 2 cos ^, from ^ = to x. 

28. p = tan ^, from ^=0 to 45^ 

29. Calculate the moment of inertia of a cube about a comer, 

30. Calculate the moment of inertia of a rectangular parallelopiped 
about a comer. 

Calculate the moment of inertia about the origin of each of the 
solids bounded by the following surface and lying above the xy-p]a.ne. 
(SeeExs. 2-11, p. 218.) 

31. z=x+y; y = 0; x = 0; x = 1; y = Vx. 

32. z = xy; y = x^; y- 1. 

33. 2 = a;2 + y; y = 0; x-1; x = S] y = x\ 

34. z=^xy'y 2/ = 0; a; = 1; a; = 2; j/ = aj2 + 1. 
36. 3 = x2 — 2/^; y == a;2; y — x. 

132. Average Value. Centroid. Let there be given a function 

/ {x, y) of two independent 
^ -^ — ■- variables. At any point of 

the x2/-plane, that is, for a 
given pair of values of x and 
2/, this function will have a 
definite value. 

What will be the average 
value of / (x, y) over a given 
region fl? Divide the region 
into small squares, note 
the value of the function at some point of each square 
(for convenience at the corner nearest the origin). Let 
there be n complete squares in the region iZ, the fractional 
parts around the border being disregarded. 



O 




x 



Fig. 64. 



XIV, §133] MULTIPLE INTEGRALS— APPLICATIONS 225 

Then the average value of / (x, y) at the corners of the 

squares will be 

Sum of values of / (x, y) 2) / (x, y) 
Number of these values n 

Multiplying both sides by the element of area Ail, and 

putting 

n^A = AA + AA + AA + = S AA, 

we have 2) / (x, y) A A 

S AA 

and the limit of this, as n increases and Ax and At/ decrease, 
is called the average value of f(x, y) over the region R. 
Thus 

n^ 4« vnj r^fft^ .A/.«^rP / / {x, y) dA fff (x, y) dx dy 
(1) Av. Val. of fix, y) over R = ^ ^^ — j^j^^^^^ 

The denominator is simply the area of R; the limits are to 
be taken to cover the region R, 

In polar coordinates, replace dA by rdddr, and /(x, y) by 

133. Centroid or Center of Gravity of an Area. The centroid, 
(Xyy), of a plane area, as R in the above figure, is the point 
whose coordinates are the average values of the coordinates 
of the points of 72, that is 

^^^ '' = llfA'''''^^^JdA' 

For a material plate of uniform thickness and of mass k 
per unit area, the element of. mass is dM = kdA and its 
centroid is defined by 

(o\ • _ fxdM ^ _ fydM 

^ ^ ^^ fdM ' ^" fdM 

Here the density factor k may be a given function Oi x and y; 

if k is constant it cancels out and we get the same result as 
for a plane area 



226 



THE CALCULUS 



[XIV, § 134 



134. Centroid of a Curved Arc. Similarly, the centroid of a 

curved arc is defined as the 
point whose coordinates are 
the average values of the co- 
ordinates of the points of the 
arc. Thus if AB is the arc, 
we divide it into n equal 
segments As, and note the 
^ values of x and y for some 
point of each As. The aver- 




FiG. 65. 



ages of these n values of x and y are, respectively, 
a?! + a;2 + X3 + - - + a;„ ^ yi + ^2 + 1/3 + • " + l/i 



n 



n 



Multiplying numerator and denominator by As and allowing 
n to increase, we have 

2xAs fxds 



(3) 



X = Urn _, . 



fds' 



^ fds 



136. Centroid of a Volume. Similarly, by dividing a volume 
into elements, and noting the coordinates (x, y, z) of a point 
of each element of volimie, we obtain 

^^^ ^ fxdV ^ fydV , fzdV 



z = 



fdV ' ^" fdV ' " fdV 

In general we may take dV = dxdydz, and so express 
(4) in terms of triple integrals. In numerous applications 
it is simpler, however, to take for dV a slice of the volume; 
thus in finding x cut the volume by a plane perpendicular 
to the avaxis, forming a section of area A^; then take dV = 
Axdx, 

136. Definition of Centroid in Mechanics. From the stand- 
point of mechanics the centroid is defined in a different 



XIV, §136] MULTIPLE INTEGRALS— APPLICATIONS 227 




manner that turns out to be equivalent to what we have 
done. Suppose the xy- 
plane to be horizontal and 
a wire bent into the form 
of any curve as AB to lie 
in this plane and to be 
balanced on a knife-edge 
MNy falling on the ordi- 
nate whose abscissa is j, ^^ 
X = X. Divide the wire 

into elements of mass Am = k As, multiply each Am by its 
distance from the knife-edge and form the sum of the 
moments 2 A;(x — x)As, The limit of this sum must be zero 
if the wire is balanced, so we have k J* (x ^ x) ds = 0, 
Hence J*xds = J*xdSyOTy since x is a fixed value, x J* ds = 
S X ds. Hence x = J* x ds/fds. Likewise we get y by sup- 
posing the wire to be balanced on a knife-edge parallel to 
the avaxis. The same considerations apply to a thin plate, 
except that As is replaced by AA. For a solid we pass 
planes parallel to the coordinate planes such that the sum 
of the moments of the elements of mass, i,e,, the products 
(i — a:) Am, (y — y)Am, (z — z) Am, shall have the limit 
zero. 



EXERCISES 

Find the average value of each of the following functions, over the 
area under the curve y = 1 — x*, from aj = to 1. 



3. a;2. 



4. 2/2 



1. X, 2. y. 

6. 1/(1+ x). 6. e*. 

Find the average value of each of the following functions in the vol- 
ume bounded by the coordinate planes and the plane x •}• y -{' z = 1, 

7. / (Xy y, z) = X, or y, or z, 8. / (x, y, z) = xyz, 

9. /(x, y, z) = xy. 10. /(x, y, z) ^x^ + y^ + sl^. 



228 THE CALCULUS [XIV, § 136 

11. Find the average ordinate of j/ = cos x, from a; = to ir/2. 

12. Find the average ordinate of a semicircle. 

13. Find the average distance of the points of the area of a circular 
quadrant from the center. (Use polar coordinates.) 

14. Find the average density of a rod in which the density varies as 
the distance from one end. 

Find the centroids of the following figures: 

16. Of the segment of the parabola y2 = 4 ox, from x = Otoh, 

16. Of a semicircle. 

17. Of the first quadrant of an ellipse. 

18. Of the area under y = cos x, from a; = to v/2, 

19. Of a right circular cone. 

20. Of a regular pyramid. (Use sections parallel to the base.) 

21. Of a semiellipsoid of revolution. 

22. Of a circular quadrantal arc. 

23. Of a circular arc of angle 2 a. 

24. Of the arc of a;2/3 -f- yVs = ^2/3^ in the first quadrant. 

26. Of the arc of y == (e* + e^)/2, from a; = to 1. 

Find the centroids (x, y) for the areas bounded by the following 
curves: 

26. y=x^ and y = Vx. 27. y=x'^ and y= a^, 

28. a;2 + 2/2 = 12 and y = x\ 29. 2/2 = ^j and 2/ = 1 - a;. 

30. 2/ = 2 x, 2/ = 0, and y = 1 — x. 

31. p = 2 cos B. 32. One loop of p = sin 2 B, 

33. The cardioid, p = 1 — cos B, 34. The lemniscate, p2 = cos 2 B. 
36. The spiral, p = ^, from ^ = to t. 
36. p = 1 + 2 cos ^, from ^ = to t. 



XIV, §136] MULTIPLE INTEGRALS— APPLICATIONS 229 

GENERAL REVIEW EXERCISES 

Find the areas bounded by each of the following curves, or the part 
specified: 

1. p =^ a cos ^ + 6. 2. p = a cos 3 0, 

3. fj^ia — x) = a^ [cissoid]; to its asymptote x = a. 

4. y2 = a;2 (4 — a;) : the loop. 

Find the volume generated by revolving each of the following curves 
about the line specified: 

. 6. y = 5 x/(2 + 3 x); about y = 0] x = to x = 1, 

6. 2 a;2 + 5 y2 = 8; about 2/ = 0; total solid. 

7. y = b sin (x/a); about y = 0; x = to x = w, 

5. y = a cosh (x/a); about y = 0; x = i^ x = a, 
9. (x — a)2 + y2 = r2; about a; = 0; total solid. 

10. The cycloid 5 about base; one arch. 

11. The cycloid; about tangent at maximum; one arch. 

12. The tractrix; about asymptote; total. 

13. X = a cos3 tj y = a sin' t; about y = 0; total solid. 

Find the area, its centroid, and its moment of inertia about the 
origin, for each of the following curves, between the limits indicated: 

14. y == a (1— x2/62); 1st quadrant. 
16. y = x/(l + x2); X = to a; = 1. 

16. The sine curve; one arch. 

17. The cycloid; one arch. 

18. x2/8 + ^2/3 = a2/3[or X = a cos' t^ y = a sin' t]; first quadrant. 

19. Between the two circles p = a cos d and p = 6 cos d;h > a. 

20. X = 2 a sin2 0, y = 2a sin2 ^ tan 0; between the curve and its 
asymptote. 

Find the centroid of each of the following frusta: 

21. Of the paraboloid x^ +y^ = ^ az by the plane a = c. 

22. Of a hemisphere. 

23. Of the upper half of the ellipsoid of revolution 

4 a;2 + 4 2/2 -I- 9 22 = 36. 



230 THE CALCULUS [XIV, § 136 

24. Of the upper half of the ellipsoid x2 + 4 3/2 + 9 ^2 = 36. 

26. Of the solid of revolution formed by revolving half of one arch 
of a cycloid about its base. 

26. Obtain a formula for the volume of a spherical segment of 
height h. 

27. Show that the volume of an elUpsoid of three unequal semiaxes, 
a, 6, c, is 4 vabc/Z, 

ff 

28. Show that the volume bounded by the cylinder a;2 + y2 = ckC; 
the paraboloid a;2 + 1/2 = bz, and the xy-plAue is (3/32) (va^/h), 

29. Find the volume common to a sphere and a cone whose vertex 
lies on the surface and whose axis coincides with a diameter of the 
sphere. 

Find the lengths of the arcs of each of the following curves, between 
the points specified: 

30. y = log x; X = a to X = h, 

31. e" cos x = l;a; = Otoa; = a;. 

32. x = fiyy = 2at (or 2/2 = 4 aH); « = <i to «=<^. 

33. One arch of a cycloid. 

34. p == a (1 + cos 0) [cardioid]; total length. 

35. Calculate the moment of inertia I for a right circular cone about 
its axis. Ans, (3/10) mass • square of radius. 

36. Calculate the moment of inertia and the radius of gyration for 
the rim of a flywheel about its axis, the inner and outer radii being 

37. The moment of inertia of an ellipsoid about any one of its axes is 
(1/5) (mass) (sum of the squares of the other two semi-axes). 

38. Calculate the moment of inertia for a spherical segment about 
the axis of the segment. 

39. Show that, for any body, 2 /o •=/* + /» + /«, where /o, /*, /y, 
Tg denote respectively its moments of inertia about a point and three 
rectangular axes through that point. 

40. Show that for any figure in the xy-plane, /, = /« + /y, where /„ 
Ipf It denote its moments of inertia about the three coordinate axes 
respectively. 



XIV, §136] MULTIPLE INTEGRALS— APPLICATIONS 231 

41. Show that the total pressure on a rectangle of height h feet and 
width h feet immersed vertically in water so that its upper edge is a feet 
below the surface and parallel to it, is 62.4 hh (a + h/2). Show that the 
depth of the center of pressure is at (6 a^ -|- 6 aA + 2 ^2)/(6 a _|_ 3 ^), 

42. Show that the total pressure on a circle of radius r, immersed 
vertically in water so that its center is at a depth a + ^, is 62.4 jtr^ {a-\'r). 
Show that the depth of the center of pressure is a + r + r2/(4 r + 4 a) . 

43. Show that the total pressure on a semicircle, immersed vertically 
in water with its bounding diameter in the surface, is 41.6 r^. Show 
that the depth of the center of pressure is 3 irr/16. 

44. Calculate the water pressure to within 1 % on a circular disk 10 ft. 
in diameter, if its plane is vertical and center 10 feet below the surface. 

45. Show that if a triangle is immersed in a liquid with its plane 
vertical and one side in the surface, the center of pressiu^ is at the 
middle of the median drawn to the lowest vertex. 

46. Show that if a triangle is immersed in a liquid with its plane 
vertical and one vertex in the surface, the opposite side being parallel 
to the surface, the center of pressure divides the median drawn from the 
highest vertex in the ratio 3:1. 

47. Calculate the mean ordinate of one arch of a sine-curve. The 
mean square ordinate. [Effective E. M. F. in an alternating electric 
current.] 

48. Calculate the average distance of the points of a square from one 
corner. 

49. What is the average distance of the points of a semicircular arc 
from the bounding diameter? 

60. When a liquid flows through a pipe of radius -R, the speed of 
flow at a distance r from the center is proportional to i22 — r®. What is 
the average speed over a cross section? What is the quantity of flow 
per imit time across any section? 

61. The kinetic energy ^ of a moving mass is Km S Am • i^/2, where 
Am is the element of mass moving with speed v. Show that for a disk 
rotating with angular speed w, ^ = (j^I/2, Calculate E for a solid car 
wheel of steel, 30 in. in diameter and 4 in. thick when the car is going 
20m./hr. 



232 



THE CALCULUS 



[XIV, § 136 



52. Show that the kinetic energy ^ of a sphere rotating about a 
diameter with angular speed w is (1/5) (mass) r'^oy^, 

63. Calculate the kinetic energy in foot-pounds of the rim of a fly- 
wheel whose inner diameter is 3 ft., cross section a square 6 in. on a side, 
if its angular speed is 100 R. P. M. and its density is 7. 

54. The x-component of the attraction between two particles m and 
m', separated by a distance r, is (fc • w • m^/r^) cos (r, x) where cos (r, x) 
denotes the cosine of the angle between r and the x-axis. Hence the 
a;-component of the attraction between two elementary parts of two 
solids M and Af' is {k • AM • AM'/r^) cos(r, x). Show that the total 
attraction between the two solids is expressible by a six-fold integral. 

55. A uniform rod attracts an external particle m. Calculate the 
components of the attraction parallel and perpendicular to the rod; 
the resultant attraction and its direction. 

[Hint. Let AM be an element of the rod; then aF = kAM • m/r^ is 
the force due to AM acting on w, r being the distance from AM to m; 
then the components of AF are AX = AF cos a and AY = AF sin o, where 
a is the angle between r and the rod. Hence 



X 



-s 



kmdM 



cos a, and Y = 



/ 



kmdM 



sin a,] 



56. Show that in spherical coordinates, (r, 6, <f>)j the volume of a 

solid is given by an integral of 
the form 

ffff^ cos 4>d4>dd dr. 

[Hint. Let P be a point on 
a sphere of radius r, the longi- 
tude of P being d and its 
latitude <^. It is usual to let 
the xjz-section of the sphere be 
the equator and the xa-section 
the prime meridian. Then P 
is the point (r, dj 4>), PS and 
QR are two adjacent meridians 
and PQj SR are two adjacent 
Fig. 67. parallels. Then 

= (r, ^ -h AS, 4>), R -- (r, d + Ad, <l> + A<^), S = (r, d, <!> + A<l>). 

Also PS = rA<l> and PQ = O'P • A^ = r cos <^ A^. 




XIV, § 136] MULTIPLE INTEGRALS— APPLICATIONS 233 



Suppose r to increase tor -{-Ar so that P, Q, R, S move out to P', 
Q', R\ /S' respectively. In this way is formed the element of volume in 
spherical coordinates. Its approximate volume is 

PS PQ ' PP' = r A^ • r cos <^ A^ • Ar = r^ cos <^ A^ A<^ Ar.] 

67. Calculate the volume of a sphere, using spherical coordinates. 

68. Calculate the volume cut from a cone of angle 2 a by two con- 
centric spheres with centers at the vertex of the cone. 

69. Show that, in cylindrical coordinates (r, ^, 2), the volume of a 
soUd is given by an integral of the 
form 



///' 



rdddrdz. 



Here r denotes distance from the 
s-axis. 

[Hint. The coordinates of P = 
(r, e, z) are OM =r, xOM = e, MP=z.] 

e = (r, ^ + A^,s); 

R = (r, ^ + A^, s + As); 

S = (r, ByS+Az). 

Increase r to r + Ar, so that we 
have an element of volume whose 
approximate volume is 

PQ'PS' PP' = r A^ • As • Ar. 

60. Calculate the volume of a sphere using cylindrical coordinates. 

61. Determine the part of the cylinder r = sin 2 ^ which lies between 
the planes a = and z = y. 

62. Determine the part of the cylinder r = sin 2 ^ which lies between 
the planes 3 = and x -f y + s = V2. 




Fig. 68. 



CHAPTER XV 

EMPIRICAL CURVES — INCREMENTS — 
INTEGRATING DEVICES 

137. Empirical Curves. Some of the methods used in 
science to draw the curves which represent simultaneous 
values of two related quantities and to obtain an equation 
which represents that relation approximately are given in 
Analytic Geometry. Usually the pairs of corresponding 
values are plotted on squared .paper first; in all that follows 
it is assumed that this has been done in each case. 

'138. Polynomial Approximations. It is advantageous to 
have equations which are as simple as possible. From 
experimental results, it is not to be expected that absolutely 
precise equations can be found, and the attempt is made to 
get an equation of simple form which approximately repre- 
sents the facts, in so far as the facts themselves are known. 
One simple kind of function which often does approximately 
express the facts is a polynomial: 

(1) y = a + bx + cx^ + da^ + • • • + fcx**. 

139. Logarithmic Plotting. The preceding forms of equa- 
tions may not represent the facts very well imless a large 
niunber of terms (1), § 138, are used. 

If the first graph resembles one of the curves y = x^, 

y = x?,y = x^y etc., or y = x^^^, y = x^^^, etc., or y = 1/x, 

y = l/x2, etc., it is advantageous to plot the common 

logarithms of the quantities measured instead of the actual 

values of those quantities. 

234 



XV, § 139] EMPIRICAL CURVES ' 235 

If X and y represent the quantities measured, and u = 
logioo:, V = logioi/ are their common logarithms, the values 
of u and v may lie very nearly on a straight line, 

(1) v = a + few, 

where a and 6 are found by drawing the straight line which 
on the whole seems to approximate best to the points 
(w, \)) and measuring its slope, 6, and the t;-intercept, a. 
Then from (1), since u = logio^;, ^ = logioy, 

(2) logio 2/ = a + 6 logio ^ = logio fc + logio ^ = logio Q^^) , 
where logio A: = «; hence 

(3) y = W. 

This f onn of equation is very convenient for computation and 
is used in practice very extensively wherever the logarithmic 
graph' is approximately a straight line.* This work applies 
equally well for negative and fractional values of 6. 

In many cases where the process just described fails, it is 
sometimes advantageous to assiune that the equation has 
the form (y — B) = k(x — A)^ which evidently has a 
horizontal tangent at the point (A, B) if n > 1, or a vertical 
tangent if n < 1. If the first graph (in x and y) shows such 
a vertical or horizontal tangent, that point (A, B) may be 

* To avoid the trouble of looking up the logarithms, a special paper 
usually described in Analytic Geometry may be purchased which is ruled 
with logarithmic intervals. No particular explanation of this paper is 
necessary except to say that it is so made that if the values of x and y are 
plotted directly, the graph is identical with that described above. To se- 
cure this result the successive rulings are drawn at distances proportional 
to log 1 (=0), log 2, log 3, • • • from one comer, both horizontally and ver- 
tically. 

Explanations and numerous figures are to be found in many books; see, 
e,g., Kent, "Mechanical Engineers' Pocket Book" (Wiley, 1910), p. 85; 
Trautwine, "Civil Engineers' Pocket Book" (Wiley), (Chapter on Hy- 
draulics). 



236 THE CALCULUS [XV, § 139 

selected as a new origin, and the values x'=^x-tA and 
y'= X — B should be used; thus we would plot the values of 

u = logioa:' = logio ix-A), v = logioy' = logio iy-E), 

in the manner described above. The values of A and B are 
found from the first graph (in x and y) ; the values of k and 
n are found from the logarithmic graph as above. 

140. Semi-logaritfamic Plotting. Variations of this process 
of § 139 are illustrated in the exercises below. In par- 
ticular, if the quantities are supposed to follow a com/pound 
interest laWy y = k^^, it is advantageous to take logarithms 
of both sides: 

logio y = logio k + bx logio e, 

and then plot u = x, v = logio 2/; if the facts are approxi- 
mately represented by any compound interest law, the 
experimental graph (in u and v) should coincide (approxi- 
mately) with the straight line , 

V = A + BUy 

where A = logio k and B = b logio e. After A and B have 
been measured, k and b [ = B log« 10 = 2.303 B] can be 
found. 

EXERCISES 

1. Find the equation of a straight line through the points (— 1, 3) 
and (2, 5); through (2, - 3) and (4, 5). 

2. Plot the data of Exercises 37-42, page 68; draw a straight line 
as closely as possible through all the points without giving preference 
to any of them; determine the equation from this graph; compare with 
former results. 

I' 

Plot each of the following curves logarithmically, — either by plot- 
ting logic X and logic y, or else by using logarithmic paper: 

3. 2/ = 2 0^3. 5. 2/ = .4 ofi-^. 7. 2/ = 5.7 x«. 



XV, §140] 



EMPIRICAL CURVES 



237 



In each of the following tables, the quantities are the results of 
actual experiments; the two variables are supposed theoretically to be 
connected by an equation of the form y = fcx". Draw a logarithmic 
graph and determine k and n, approximately: 

9. [Steam pressure; v — volume, p = pressure.] [Saxelby.] 



V 


2 


4 


6 


8 


10 


p 


68.7 


31.3 


19.8 


14.3 


J1.3 



IC 


\. [Gas 


engine 


mixture 


i; notation as above.] 


[Gibson.] 




V 


3.54 


4.13 


4.73 


5.35 


5.94 


6.55 


7.14 


7.73 


8.04 


V 


141.3 


115 


95 


81.4 


71.2 


63.5 


54.6 


50.7 


45 



11. [Head of water A, and time t of discharge of a given amount.] 
[Gibson.] 



h 


0.043 


0.057 


0.077 


0.095 


0.100 


t 


1260 


540 


275 


170 


138 



12. [Heat conduction, asbestos; 6 = temperature (F.), C = coefE- 
-'^ient of conductivity.] [Kent.] 






32** 


212** 


392** 


572** 


752** 


1112** 


c 


1.048 


1.346 


1.451 


1.499 


1.548 


1.644 



13. 


[Track records: d = distance, t 


= record time (intercollegiate).] 


d 


100 yd. 


220 yd. 


440 yd. 


880 yd. 


1 mi. 


2 mi. 


t 


0:09t 


0:21i 


0:48t 


1:56 


4:17t 


9:27f 



[Note. See Kennelly, Fatigue, etc., Proc. Amer. Acad. Sc. XLII, 
No. 15, Dec. 1906; and Popular Science Monthly , Nov. 1908.] 



238 THE CALCULUS [XV, § 140 

Plot the following cunres, using logarithmic values of one quantity 
and natural values of the other: 

14. y^€F. 16. j/ = 1063». le. y=:4e-«. 17. y = .le-*^. 

Discover a formula of the t3rpe y=kef^ for each of the following sets 
of data: 



18. 


x: 


.2 


.4 


.6 


.8 


1.0 




y- 


4.5 

* 


6.6 


9.9 


15.0 


22.2 


19. 


x: 


.6 


- 1.2 


1.8 


2.4 


3.0 




y- 


1.5 


2.2 


3.3 


6.0 


7.4 


20. 


x: 


.31 


.63 


.94 


1.26 


1.57 




y- 


2.44 


2.98 


3.64 


4.46 


5.44 


21. 


x: 


.2 


.8 


2.0 


4.0 






y- 


8.2 


4.5 


1.3 


0.2 




22. 


x: 


.63 


1.26 


2.51 


3.77 


5.03 




y- 


4.02 


2.70 


1.20 


0.54 


0.24 


23. 


x: 


1 


2 


3 


4 


5 




y- 


3.26 


2.68 


2.16 


1.80 


1.46 


24. 


A: 


is the amplitude of vibration of a long pendulum 


, t is the time 


since i 


it was set swinging. Show that they are connected by a law of 


the form A — ke~^. 










A 


in. = 


= 10 


4.97 


2.47 1.22 


.61 


.30 .14 


t min. = 





1 


2 3 


4 


5 6 



141. Method of Increments. A method adapted to the 
case where (1) of § 138 has the form 

(1) y = a + bx + cx2, 

is as follows. From two pairs of values of x and y, say 
(x, y) and {x + Ax, 2/ + Ay) given by experiment, we should 
have 

(2) y = a + hx + cx^^y + Ay = a + b (x + Ax) + c (x + Ax)^, 
whence 

(3) Ay = bAx + 2cxAx + c A?. 



XV, §141] 



EMPIRICAL CURVES 



239 



If Ax is constant, i.e. if points axe selected at equal x-in- 
tervals on the crudely sketched cursre drawn through the 
experimental points, we might write 

(4) y= Ay = (bh + chPj + 2 ch-x = A + Bx 

where h = Ax. If we should actually plot this equation, 
Y = A+ Bx, we would get (approximately) a straight 
line. Now Ay = F is the difference of two values of y; it can 
be f oimd for each of the values of x selected above, and the 
(approximate) straight line can be drawn, so that A and B 
can be measured. 

We may repeat the preceding process; from (4) we obtain, 
as above, 

(5) AY = BAx = 2 cA2, (h = Ax), 

whence AF is constant if h was taken constant. Now AY is 
the difference between two values of Y; that is, AF is the 
difference between two values of Ay: 

AY=A{Ay)=A^y, 

and for that reason is called a second difference, or a second 
increment. If the second differences are reasonably con- 
stant, we conclude that an equation of the form (1) will 
reasonably represent the facts and we find c directly by 
solving equation (5). 

Example 1. With a certain crane it is found that the forces / 
measured in pounds which will just overcome a weight w are 



/ 


8.5 


12.8 


17.0 


21.4 


25.6 


29.9 


34.2 


38.5 


w 


100 


200 


300 


400 


600 


600 


700 


800 



What is the law connecting force with the weight that it just overcomes? 

[Perry.] 

Plotting the values of / and w, it appears that the points are very 



240 



THE CALCULUS 



[XV, § 141 



nearly on a straight line f — a-\- bw. If they were on a straight line, 
Af/Aw would be constant and equal to df/dw = b. As a matter of fact, 
for each increase of weight, Af/Aw varies only from .042 to .044, its 
average value being 30/700 = .0429 Taking this value for 6, one gets 
for the equation of the line, and hence for the relation between force 
and weight: 

/ = 4.21 + .0429 w, 4.21 = 8.5 - 100 X .0429 

Here 4.21 appears to be the force needed to start the crane if no load 
were to be lifted. 

Example 2. If is the melting point (Centigrade) of an alloy of 
lead and zinc containing x% of lead, it is found that 



a; = % lead 


40 


50 


60 


70 


80 


90 


= melting point 


186 


205 


226 


250 


276 


304 



/ 



Plotting the points (a;, 0) will show them not to lie in a straight line as 
is also shown by the difference A0. But A(A^) or A*^ does run imi- 
formly. Therefore one tries a quadratic function of z for 0, that is 

= a-\-hx +cxK 

It is evident that A0 = lOh + c(20x + 100), 

and A2 ^ = 200 c. 

The average value of A^ is 2.25 Hence c = .01 125 If we subtract 
cx^ from 0j we find — ca^ = a + hx. These values can be calculated 
from the data and from a = .01125; they will be found to lie on a straight 
line; hence a and b can be found by any one of several preceding methods. 
The student will readily obtain, approximately, 

^ = 133 + .875 X + .01125 x\ 

a formula which represents reasonably the melting point of any zinc- 
lead alloy. [Saxelbt.] 

EXERCISES 

1. Express f{x) as a quadratic function of x, when 

x: 0.5 1.0 1.5 2.0 2.5 3.0 

fix): 2.6 1.9 1.6 1.5 1.7 2.1 2.8 

2. Express / (x) as a cubic function of x, when 

x: .02 .04 .06 .08 .10 .12 .14 

fix): .020 ,042 .064 .087 .111 .136 .163 



XV, §141] EMPIRICAL CURVES 241 

3. Express (m) as a cubic in m, when 

m: .01 .02 .03 .04 .05 .06 .07 .08 
<t>{m): .00010.00041 .00093 .00166 .00260 .00385 .00530 .00690 

4. The specific heat S of water, at ^° C, is 

^: 5 10 15 20 25 30 

S: 1.0066 1.0038 1.0015 1.0000 0.9995 1.0000 1.002 

Express S in terms of $. 

6. Determine a relation between the vapor pressure P of mercury, 
and the temperature C, from the data below: 

^: 60 90 120 150 180 210 240 

P:.03 .16 .78 2.93 9.23 25.12 58.8 

6. The resistance R, in ohms per 1000 feet, of copper wire of diame- 
ter D mils, is 

D: 289 182 102 57 32 18 10 

/J: .126 .317 1.010 3.234 10.26 32.8 105.1 

Find a relation between R and D, 

7. The Brown and Sharpe gauge numbers N of wire of diameter D 
mils, are 

N: 1 5 10 15 20 25 30 

D: 289 182 102 57 32 18 10. 

Express D in terms of N. 

8. Find a relation between the speed S of a. train in kilometers per 
hour, and the horse-power (H. P.) of the engine from the data below: 

H.P.:550 650 750 850 

S: 26 .35 52 70. 

9. The energy consmned in overcoming molecular friction when iron 
is magnetized and demagnetized (hysteresis, H, — measured in watts 
per cycle per liter of iron) is given below in terms of the strength of the 
magnetic field (B, — measured in lines per square centimeter). What 
is the relation between them? 

B: 2000 4000 6000 8000 10000 14000 16000 18000 
H: .022 .048 .085 .138 .185 .320 .400 .475 

10. Proceed as in Ex. 15, for cobalt, the hysteresis loss H being now 
measured in ergs per cycle per second: 

B: 900 2350 3100 4100 4600 5200 5850 6500 
H: 450 2450 3950 6300 7400 8950 10950 13250. 



242 



THE CALCULUS 



[XV, § 141 



The table below contains some data on the comparison of a tung- 
sten lamp with a tantalum lamp. The voltage or electrical pressure F, 
is in volts, the resistance R, in ohms, the current consumed in watts per 
candle power; C denotes candle power, and W watts per candle power. 



11. Tungsten 



12. Tantalum 



Voltage 


C. P. 


Watts 


Resistance 


C.P. 


Watts 


Resistance 






per C. P. 




per C. P. 




V 


C 


W 


R 


C 


W 


R 


80 


14 


2.51 


166 


5 


3.80 


260 


90 


24 


1.83 


173 


10 


2.85 


265 


100 


36 
52 


1.49 


182 


18 


2.05 


275 


110 


1.23 


190 


25 


1.65 


283 


120 


71 


1.10 


197 


38 


1.35 


290 


130 


95 


0.96 


202 


50 


1.15 


300 


140 


128 


0.83 


210 


62 


0.95 


308 


150 


160 


0.76 


216 


78 


0.85 


315 


160 


196 


0.58 


222 


100 


0.75 


323 


170 


230 


0.52 


227 


122 


0.70 


327 


180 


270 


0.50 


232 


156 


0.70 


332 


190 


312 


0.48 


238 


190 


0.60 


340 


200 


340 


0.47 


242 


235 


0.55 


345 



For each lamp, express each of the quantities C, W, R, in terms of V. 

• 

142. Integrating Devices. It is important in many prac- 
tical cases to know approximately the areas of given closed 
curves. Thus the volume of a ship is found by finding the 
areas of cross sections at small intervals. Besides the methods 
described above, the following devices are employed: 

A. Counting squares on cross-section paper. 

B. Weighing the figures cut from a heavy cardboard of 
uniform known weight per square inch. 

C. Integraphs. These are machines which draw the inte- 
gral curve mechanically; from it values of the area may be 
read off as heights. 



XV, §142] 



EMPIRICAL CURVES 



243 



y-fM 



The simplest such machine is that invented by Abdank-Abakano- 
wicz. A heavy carriage CDEF on large rough rollers, Ry R' is placed on 
the pap)er so that CE is 
parallel to the 2/-axis. 

Two sliders S and /S' 
move on the parallel 
sides DF and CE\ to S 
is attached a pointer P 
which follows the curve 
y ^ f(x). A grooved rod 
AB slides over a pivot 
at Af which lies on the 
X-axis, and is fastened by 
pivot B to the slider S, 
A parallelogram mechan- 
ism forces a sharp wheel 
W attached to the slider 
S^ to remain parallel to 
AB, A marker Q draws 
a new curve i = 0(x), 

which obviously has a tangent parallel to W, that is, to AB, If AB 
makes an angle a with Ox, tan a is the slope of the new curve; but 
tan a is the height of S divided by the fixed horizontal distance h between 
A andB: 

d<t>(x) _,^ _ heighto{S _f(x), 
dx "^^'^'' h "T 




Fig. 69. 



whence 



1 ^«-x 
» - io = ^ y ^ f(x)dx; 



where a is the value of x at P when the machine starts, and io denotes 
the vertical height of the new curve at the corresponding point. 

D. Polar Planimeters. — There are machines which read 
oflf the area directly (for any smooth closed curve of simple 
shape) on a dial attached to a rolling wheel. 

The simplest such machine is that invented by Amsler. 

Let us first suppose that a moving rod ab of length I always remains 
jjerpendicular to the path described by its center C. The path of C 
may be regarded as the limit of an inscribed polygon, and the area 
swept over by the rod may be thought of as the limit of the sum of small 



244 



THE CALCULUS 



[XV, § 142 




quadrilaterals, the area AA of each of which is lAp, approximately, 

where Ap is the length of 
the corresponding side of 
the polygon inscribed in 
the path of C. Hence the 
total area A swept over 
by the rod is evidently Zp, 
where p is the total length 
Pjq <7q of the path of C. 

But if the rod does not 
remain perpendicular to the path of C during the motion, and if ^ is the 
angle between the rod and that path, the area AA becomes Z sin ^ • Ap, 
approximately. The expression sin ^ • Ap 
may be thought of as the component of Ap in 
a direction perpendicular to the rod. Calling 
thid component As, we have AA = lAs, ap- 
proximately; and the total area A swept over 
by the rod is precisely lim 2 AA = lim 2 1! As 
=J*ld8 = lj*d8 = Is, where s =J*d8 is the 
total motion of C in a direction perpendicular 
to the rod. 

The quantity s =J*d8 can be measured me- 
chanically by means of a wheel of which the 
rod is the axle, attached to the rod at C; for if 
e is the total angle through which the wheel 
turns during the motion, s = rd, where r is the 
radius of the wheel, and d is measured in 
radians. Hence A = fe = Ird; the value of d 
is read off from a dial attached to the wheel; 
I and r are known lengths. 

In Am8ler*8 polar planimeter, one end h of the rod ab is forced to 
trace once around a given closed curve whose area is desired; the other 
end a is mechanically forced to move back and forth along a circular 
arc by being hinged at a to another rod Oa, which in its turn is hinged 
to a heavy metal block at O. As 6 describes that part of the given curve 
which lies farthest from 0, the rod ah sweeps over an area between the 
circular arc traced by a and the outer part of the given curve; as 6 
describes the part of the curve nearest to 0, ab sweeps back over a 
portion of the area covered before, between the circle and the inner 
part of the given curve. This latter area does not count in the final 
total, since it has been swept over twice in opposite directions. Hence 




Fig. 71. 



XV, S 142] 



EMPIRICAL CURVES 



the quantity A = IrB, given by the reading of the dial 
is precisely the desired area al the given closed 
curve, which has been swept over just once by 
the moving rod ob. 

In practicing with such a machine, begin 
with curves of known area. The machine ia 
useful not only in finding areafl of irregular 
curves whose equations are not known, but 
also in checking integrations performed by the 
standard methods, and in giving at least 
approximate values for integrals whose evalu- 
ation is difficult or impossible. 

For further information on int«grating 
devices, see: Abdank-Abakanowicz, Les in- 
legrajthes (Paris, Gautliier-Villars); Henrici, 
Report on Planimeters (British Assoc. 189^ 
Mechanical Inlegrato? 
Encyklopadie der Math. Wisa,, Vol. II. Catalogues of dealers 
stnunenta also contain much really valuable information. 




Fig. 72. 

196-523); Shaw, 
(Proc. Inst. Civ. Engs. 1885, pp. 76-143); 



EXERCISES 

1. Cottstruct a figure of each of the types mentioned below, with di- 
mensions selected at random, and find their areas approximately by 
counting squares; by Simpson's rule; by the planimeter, if one is avail- 
able. (1) A right triangle; (2) An equilateral triangle; (3) A circle; 
(4) An eUipse. (Draw it with a thread and two pins.) (5) An arch of 
a sine curve; (6) An arch of a cycloid. 

2. The figures below are repro- 
ductions of indicator cards, taken 
from three different types of en- 
gines. The dotted curves are en- 
tirely separate from the full lines. 
The average pressure on the piston 
is the area of one of these curves 
divided by the length of stroke. 
Find this value in each case, where 

the stroke is 12 in. in the first figure, and 8 in. in each of the others. 

(Unit of area = I large square.) 




Pia. 73 (a). 



THE CALCULUS 



(Note. The uwfc done ia precisely the area in question, on a proper 
scale, since the work is the average pieeaure times the length of stroke.] 




:n 




,l|:j 


!-riir| 






J.--, -+ ri 


1: 




uht^ 


=e* 


W 


--L 















CHAPTER XVI 



LAW OF THE MEAN — TAYLOR'S FORMULA — SERIES 
143. RoUe's Theorem. Let us consider a curve 

where / (x) is single-valued and continuous, and where the 
curve has at every point 
a tangent that is not ver- 
tical. If such a curve 
cuts the a;-axis twice, at 
X = a and a; = 6, it surely 
either has a maximum or 




Fig. 74. 



a minimum at at least one point x = c between a and b. 
It was shown in § 33, p. 54, that the derivative at c is zero: 

[A] If /(a) =/(&)= 0, then [^]^^^= 0, (fl<c<&); 

this fact is known as Rolle's Theorem. 

144. The Law of the Mean. Rollers Theorem is quite evi- 
dent geometrically in the form: An arc of a simple smooth 
curve cut off by the x-axis has at least one horizontal tangent. 

The precise nature of the 
necessary restrictions is 
given in § 129. 

Another similar state- 
ment, which is true under 
the same restrictions and 
Fig. 75. is equally obvious geo- 

metrically, is: An arc of a simple smooth curve cut off by any 

secant has at least one tangent parallel to thai secant, 

247 




248 THE CALCULUS [XVI, § 144 

If the curve is j/ = / (x) , and if the secant S cuts it at points 
P:[a,/(a)] and Q: [6, /(&)], the slope of S is 

Ay-hAx = [/(&) -f(a)] ^ (& - a). 

The slope of the tangent CT at a; = c is equal to this: 

This statement is called the law of the mean or the theorem 
of finite differences. 

It is easy to prove this statement algebraically from 
RoUe's Theorem. For if we subtract the height of the secant 
S from the height of the curve, we get a new curve whose 
height is: 

D{x) =/(x) - ['^^^{^ (x-a) +/(a)]. 

Now D(x) is zero when x = a and when x = b. It follows 
by § 143 that d D {x)/dx = at x = c, (a < c < 6) : 

which is nothing but a restatement of [B], 

145. Increments. The law of the mean is used to detenninc 
increments approximately, and to evaluate small errors. 
If y =zf (x) is a given function, we have, by § 144, 

In practice this law is used to estimate the extreme limit of 
errors, that is, the extreme limit of the nimierical value of Ay, 
It is evident that 

[B*] |Ay|<Mi.|Ax|, 

where Mi is the maximum of the numerical value of dy/dx be- 
tween a and a + Ax. When Ax is very small, the slope dy/dx 



XVI, § 145] LAW OF THE MEAN 249 

is practically constant from a to a + Ax in most instances, 
and Ml is practically the same as the value of dy/dx at any 
point between a and a + Ax. 

Example 1. To find the correct increments in a five-place table of 
logarithms. 

The usual logarithm table contains values of L = logio ^ at intervals 
of size AN = .001. Hence 

where iV<c<iV + . 001. 

Logarithms are ordinarily given from N = I to N = 10. Hence AL 
will vary from .00043 at the beginning of the table to .00004 at the end 
of the table. This agrees with the " differences" column in an ordinary 
logarithm table. 

Example 2. The reading of a certain galvanometer is proportional 
to the tangent of the angle through which the magnetic needle swings. 
Find the effect of an error in reading the angle on the computed value of 
the electric current measured. We have 

C = A; tan $, 

where C is the current and d the angle reading. Hence the error Ec in 
the computed current is 

where Ec is the error in the computed value of the current, and A^ is 
the error made in reading the angle 6. Since A^ is very small, 
Ec = k sec2 e • Ady approximately. The error Ec is extremely large if 
e is near 90°, even if A^ is small; hence this form of galvanometer is not 
used in accurate work. 



EXERCISES 

1. At what point on the parabola y — x^ \& the tangent parallel to 
the secant drawn through the points where x = and a; = 1? 

2. Proceed as in Ex. 1 for the curve y = sin x, and the points where 
a; = 60° and a; = 75°. 

3. Proceed as in Ex. 1 for the curve y = log (1 + x), for a; = 1 and 
a; =3. 



250 THE CALCULUS [XVI, § 145 

4. Discuss the differences in a four-place table of natural sines, the 
argument interval being 10'. 

6. Proceed as in Ex. 4 for a similar table of natural cosines; of 
natural tangents. 

6. Discuss the differences in a four^place table of logarithmic sines, 
the entries being given for intervals of 10'. 

7. Proceed as in Ex. 6 for a table of logarithmic tangents. 

8. Calculate the difference in a seven-place table of logio sin x at the 
place where x = 30°; where x = 60°; where x = 85°. 

9. Discuss the effect of a small change in x on the function 

y = log (1 + 1/x). 

10. If logio N = 1.2070 ± .0002, what is the uncertainty in N? [The 
term ± .0002 indicates the uncertainty in the value 1.2070.] 

11. If the angle of elevation of a mountain peak, as measured from 
a point in the plain 5 mi. distant from it, is 5° 20' ± 5', what is the un- 
certainty in the computed height of the peak? 

12. The horizontal range of a gun is R = (V^/g) sin 2 a, where V is 
the muzzle speed and a the angle of elevation of the gun. If F = 1200 
ft. /sec, discuss the effect upon R of an error of 5' in the angle of ele- 
vation. 

13. T he distance to the sea horizon from a point h ft. above sea level 
is D = V2 Rh + h^, where R is the radius of the earth. Discuss the 
change in D due to a change of one foot in h. (Z), -B, and h are all to 
be taken in the same units.) If D is tabulated for values of h at inter- 
vals of one foot, what is the tabular difference at the place where h = 60? 

14. If the boiling point of water at height H ft. above sea level is T, 
H = 517 (212° - T) - (212° - T)^, T being the boUing temperature 
in degrees F. Discuss the uncertainty m H^ \i T can be measured to 
1°. If H be tabulated with argument T at intervals of 1°, what is the 
tabular entry and the tabular difference when T — 200°? 

16. When a pendulum of length I (feet) swings through a small angle 
a (radians), the time (seconds) of one swing is T = vVlfg (1 + a2/16). 
What is the effect on T of a change in a, say from 5° to 6°? Of a change 
in I from 36 in. to 37 in.? Of a change in g from 32,16 to 3^.3? 



XVI, § 146] 



LAW OF THE MEAN 



251 



16. The viscosity of water at 0° C. is P = 1/(1 + .0337 d + .00022 ^). 
Discuss the change in P due to a small change in d. What is the average 
value of P from ^ = 20° to ^ = 30°? 

17. The quantity of heat (measured in calories) required to raise one 
kgm. of water from 0° C. to ^° C. is 27 = 94.21 (365 - ^)o-3i25 _}- k. How 
much heat is required to raise the temperature of one kgm. of water 1° C. 
when e = 10°? 20°? 30°? 70°? To find k, observe that H = when ^ = 0. 

18. The coefficient of friction of water flowing through a pipe of 
diameter D ^nches) with a speed V (ft. /sec.) is / = .0126 + (.0315 
— .06 D)/VV. What is the effect on / of a small change in 7? in D? 

146. Limit of Eiror. In using the formula [B] the uncer- 
tainty in the value of c is troublesome. If the value of dy/dx 
at a: = o is used in place of its value at x = c, the error made 
in finding Ay by [B] can be expressed in terms of the second 
derivative d!^y/doi^. 

We shall use the convenient notation /'(x), f" (x), etc., 
for the derivatives of / (x) : 

r (x) = ^ = ^ (the slope oiy= /(x) ). 



r(x) = 



dy(x) _ d^y _ df (x) 



(the flexion). 



dx^ dx!^ dx 
Let Af 2 denote the maximimi of the numerical value of/" (x) 
between two points V 
X = a and x = 6, so 
that 

(1)' \f"(x)\<M,. 

The area under the 
curve y = /" (x) be- 
tween X = a and any 




-f(X) 



Fig. 76 (a). 

point X = X between a and h is evidently not greater than the 
area under the horizontal line y = M2) that is, if a< x< 6, 



(2) 



I (' 7"(x)da;|< P "M-dx, or /'(a;)T"1<M2a;T ^ 



252 



THE CALCULUS 



[XVI, § 146 



since df(x)/dx =/"(x), and M2 is a constant; whence, sub- 
stituting the limits of integration in the usual manner, 
(3) \r(x)^r(a)\<M,ix^a), 

which is geometrically shown in Fig. 76 (b) . It follows that 

the area under the curve 

y =f (x) — f (a) is not 
greater than that under 
the line y = M2(x — a): 

(4) I f'^lf'ix) -ria)]dx 

^ I M2(x — a) dx; 
or since /' (a) and Af 2 are 








x^h 



Fig. 76 (6). 
constants and df{x)/dx =f(x), 

r/(x)-/'(a)..ri<3f/-^r^ 

L Jx = a| — Z Jx=a 

whence, substituting the limits in the usual manner, 

[C] \f{x) -f{a) -/'(fl)(x- fl)|< M2 ^^ , 

which holds for all values of x between x = a and x = b. 
This formula may be written even if x<a: 

[C*] fix) ^f{a) +/'(fl)(x -fl)+£2,where|£2| <M% ^^^-^, 

and E2 is the error made in using f\a) in place of /' (c) in 
formula [C]; for (x — a)^ = | a; — a | ^. 

It should be noticed that E2 is exactly the error made in 
substituting the tangent at x = a for the curve, i.e. it is the 
difference between At/[= f{x) — f(a)] and dy[= f{a) {x — a)] 
mentioned in § 26, p. 43, and shown in Fig. 8. 

The formula [B*] is exactly analogous to [C*]; since 
Ay = /(x) — f(a) if Ax = X — a, [B *] may be written 

[B *] fix) =/(a) +Ei, 1^1 1 < Ml . |x - a\. 



XVI, § 147] TAYLOR'S FORMULA 253 

Example 1. In Ex. 1, § 145, we found for L = logio AT, \ 

AL = •— ^ (nearly). 

Applying [C*], with/(iV) = logio N.a^N.x^N + ANyZ-a^AN 
= .001, we find 

where M2 is the maximum value of | /" (N) \ = Gogio e)/N^ between iV = 1 
and N = .10. Hence E2 < .00000022 The value of AL found before 
was therefore quite accurate, — absolutely accurate as far as a five-place 
table is concerned. 

ExAitPLE 2. Apply [C*] to the function /(x) = sin x, with a = 0, and 
show how nearly correct the values are for x < ir/90 = 2°. 

Since /(x) = sin x, and a = 0, [C*] becomes 

sin X = sin (0) + cos (0)- (x - 0) +E2 = x + ^2, \E2\ ^ M2^y 

where Af 2 is the maximum of | /" (x) | = | — sin x | between and ir/90. 
that is M2 = sin (ir/90) = sin 2° = .0349 Hence E2 < .0175 x2. Since 
x<ir/90, x2<ir2/8100<.0013; hence ^2<. 000023, and sinx =x is 
correct up to x 5 ir/90 within .000023 
Similarly, for a = ir/4, we have, by [C*], 

sinx = ^[l + (x-f)] + ^2, \E2\<M2^^^^\ 

where M2 < 1. If (x - ir/4) < ir/90, 1 E2I < (ir/90)2 -^ 2 = .0007 

147. Extended Law of the Mean. Taylor's Theorem. The 
formula [C*] can be extended very readily. Let/' (x), /" (x), 
/'" (x), • • • Z^**^ (x) denote the first n successive derivatives of 

^ ^^^~ dx*- " dx 

and let the maximum of the numerical value of f^^ (x) from 
X = a tQ X = fe be denoted by Mn- Then 

I /*> (X) \<Mn, 

and I n-'jin) (x)dx\^\ r"M„dx 



254 THE CALCULUS [XVI, J 147 

or !/<»-» (x) - /"-« (a) I ^ I Mn (x-a)\ 

for all values of x between a and b. Integrating again, we 
obtain, as in § 146: 

(x - ay 
2 

and, continuing this process by integrations until we reach 
/(x), we find: 



I /<"-'' (.x) -/<-*> (a) -/<"-» (a) (x - o) U 



i»f. 



[^1 



/(x) -/(a) -/' (a) (X- a) --^ (X- a)»- ... 



/(n-l) (a) 



^M,'-"'" 



nt 



or. 



[Z)*] / (X) =/ (a) +/' (a) (X - a) +^^ (x - a)» + . . . 

/(n-l) (a) 

where 



and where Af^ is the maximum of 1/^**^ (re) | between x = a and 
X = b. 

This formula is known as the extended law of the mean, or 
Taylor's Theorem, after Taylor, who first gave such approxi- 
mations as it expresses. It is one of the more important for- 
mulas of the Calculus. 

In particular, if a = 0, the formula becomes 

[D*] /(x)=/(0)+/'(0)x+^x«+... 

/(n-l) (0) • 

where \En\ ^ Mn\x^\ /n\ This special case of Taylor's 
Theorem is often called Maclaurin's Theorem. 



XVI, § 147] TAYLOR'S FORMULA 255 

The formula [D*] replaces f (x) by a polynomial of the 
nth degree, with an error En» These pol3aiomials are repre- 
sented graphically by curves, which are usually close to the 
curve which represents / (x) near x = a. See Tables, III, K. 

Since the expression for En above contains n! in the 
denominator, and since n! grows astoundingly large as n 
grows larger, there is every prospect that En will become 
smaller for larger n; hence, usually, the pol3aiomial curves 
come closer and closer tof(x) as n increases, and the approxi- 
mations are reasonably good farther and farther away from 
X = a. But it is never safe to trust to chance in this matter, 
and it is usually possible to see what does happen to En as 
n grows, without excessive work. 

Example L Find an approximating pol3momial of the third degree 
to replace sin x near x = 0, and determine the error in using it up to 
X = ir/18 = 10°. 

Since/ (x) = sin x and a = 0, we have/' (x) = cos x, /" (x) = — sin x, 
/'" (x) = - cos X, /»^ (x) = + sin x, whence/ (0) = 0, /' (0) = 1, /" (0) = 
0,/'" (0) = - 1; and [Max. |/»v (x)\] = [Max.|sinxl] = sin 10° = .1736 
between x = and x = ir/18 = 10°. Hence 

sin X = + 1 • (X - 0) + + (- 1) . ^^^^ + ^4 = X - ^ + iEf4, 

where \E^\< (.1736) • x4/4! ^ (.1736) (x/18)4 -^ 4! < .000007, when x 
lies between and ir/18. 

In general^ the approximation grows better as n grows larger, for 
[/(«) (x) I is alwajrs either [ sin x [ or 1 cos x|; hence Mn < 1, and 1 ^n I ^ 
af^/nl which diminishes very rapidly as n increases, especially if x < 1 = 
57°.3 For n = 7, the formula gives, for x > 0, 

sinx=x- J+|]+E7, \E7Kxy7i 



Example 2. Express Vl -f x as a quadratic in x and estimate the 
error if x lies between and .2 

Here /(O) ^ l;/'(0) = 1/2;/" (0) = - 1/4; M, > |/'" (©) | = 3/8. 

Hence vTT^ = 1 + x/2 - xV8 + ^s) I ^3 1 < [(3/8)/(3!)] (.2)3 = .0005 
Thus: VT2 = 1 + .1 - .005 + ^3 = 1.0950 + ^3; I ^8 1 <..0005 



256 THE CALCULUS [XVI, § 147 

EXERCISES 

1. Apply the formula (C*) to obtain an approximating polynomial 
of the first degree for tan x, with a = 0. Show that the error, when 
I X 1 < t/90, is less than .00003. Draw a figure to show the comparison 
between tan x and the approximating linear function. 

2. Apply [/)*] to obtain an approximating quadratic for cos x, with 
a = 0. Show that the error, when |a; | <ir/10 is less than (x/10)'-^3! 
Draw a figure. 

3. Apply [/)*]' to obtain an approximating cubic for cosx, near 
x = 0. Hence show that the formula found in Ex. 2 is really correct, 
when \x \ <t/10, to within (ir/lO)^ t- 4! Draw a figure. 

4. Obtain an approximation of the third degree for sin x near 
X = t/3. Show that it is correct to within (ir/10)* -J- 4! for angles 
which differ from ir/3 by less than ir/10. Draw a figure. 

Obtain an approximation of the first degree, one of the second 
degree, one of the third degree, for each of the following functions near 
the value of x mentioned; find an upper limit of the error in each case 
for values of x which differ from the value of a by the amount specified; 
draw a figure showing the three approximations in each case: 

6. e», a = 0, I X - a I < .1 9. c-*, a = 2, | x - a | < .5 

6. tan X, a = 0, 1 X — a| < ir/90. 10. sin x, a = ir/2, | x—a \ < t/45. 

7. log(l+x), a=0, |x-a|<.2 11. tanx, a = V4, |a;— a | <t/90. 

8. cosx,a = T/4, |x-a|<T/18. 12. x2+x+l,a = l, |x-al <l/5. 

13. 2 x2 - X - 1, a = 1/2, I X - a I < 1. 

14. x3-2x2-x + l, a = -2, |x-a| <.5 

16. Find a polynomial which represents sin x to seven decimal places 
(inclusive), forfx] <10°. 

16. Proceed as in Ex. 15, for cos x; for e~*, when 0<x <1. 

17. Show that x differs from sin x by less than .0001 for values of x 
less than a certain amount; and estimate this amount as well as possible. 

18. The quantity of current C (in watts) consumed per candle power 
by a certain electric lamp in terms of voltage v is C = 2.7 + 108007-.0767». 
Express C by a poljmomial in t; — 115 correct from » = 110 up to « = 
120 to within .025 watt. 



XVI, § 148] TAYLOR'S FORMULA 257 

148. Application of Taylor's Theorem to Extremes. If a 
function y = f(x) is given whose maxima and minima are to 
be found, we may find the critical points where /' (x) = 0. 
Let a be one solution of /'(x) = 0, that is, a critical value. 
Then, since/' (a) = 0, we have, by [D*], 

At/=/(x) -/(a) =0 + -^(a:-a)2+£;3, l^sl < ^3^^^'> 

where ikf 3 ^ | /'" (x) \ . Hence the sign of Ay is determined by 
the sign of /"(a) when (x — a) is sufficiently small. 

If /"(a)>0, Ay>0, and/(x) is a minimum at x = a. 

If /" (a) <0, Ai/ <0, and / (x) is a maximum at x = a. (See 
§ 42, p. 66.) 

If /"(a) = 0, the question is not decided.* But in that 
case, by [D*] : 

Ay=/(x)-/(a)=0 + 0+-^^(x-a)3+-^(x-a)4 + S^^ 

where|i?6| ^ Ms\x-a\^/5ly M^ ^ \r(x) | . From this we see 
that if/'" (a) 7^ there is neither a maximum nor a minimum, 
for (x — a)3 changes sign near x = a. But if/'" (a) = 0, then 
/*^ (a) determines the sign of Ay, as in the case of/" (a) above. 
In general, if /^*^ (a) is the first one of the successive deriva- 
tives, /'(a), /"(a), • • •, which is not zero at x = a, then there 
is: 

no extreme if k is odd; 

a maximum if k is even and /(*) (a) <0; 

a minimum if k is even and /(*> (a) > 0. 

♦ The methods which follow are logically sound and can always be car- 
ried out when the derivatives can be found. But if several derivatives 
vanish (or, what is worse, fail to exist), the method of § 34, p. 64, is better 
in practice. 



258 THE CALCULUS [XVI, § 148 

Example 1. Find the extremee for y = x*. 

Since/ (a;) = x^jf (x) = 4 x^j hence the critical values are solations of 
the equation ^xf =0, and therefore a? = is the only such critical 
value. 

Since /" (x) = 12 x^, ]"' ^^) = 24 x, /»v (x) = 24, the first derivative 
which does not vanish at x = is /*^ (x), and it is positive (= 24). It 
follows that / (x) is a minimum when x = 0; this is borne out by the 
famiUar graph of the given curve. 

EXERCISES 

Study the extremes in the following functions: 

1. x«. 6. (x + 3)6. 9. x2sinx. 

2. (x - 2)8. 6. x* (2 X - 1)3. 10. x4 cos X. 

8. 4 x3 — 3 X*. 7. sin x^. 11. x^ tan x. 

4. x3(H-x)3. 8. x-sinx. 12. e-i/^. 

18. Discuss the extremes of the curves y == x", for all positive integral 
values of n. 

14. An open tank is to be constructed with square base and vertical 
sides so as to contain 10 cu. ft. of water. Find the dimensions so that 
the least possible quantity of material will be needed. 

16. Show that the greatest rectangle that can be inscribed in a given 
circle is a square. 

[See Ex. 44, p. 59. Other exercises from § 35 may be resolved by 
the process of § 148.] 

16. What is the maximum contents of a cone that can be folded from 
a filter paper of 8 in. diameter? 

17. A gutter whose cross section is an arc of a circle is to be made by 
bending into shape a strip of copper. If the width of the strip is a, show 
that the radius of the cross section when the carrying capacity is a 
maximum is a/ir. [Osgood.] 

18. A battery of internal resistance r and E. IM. F. e sends a current 
through an external resistance R. The power given to the external 
circuit is 

{R + r)2 • 
If e = 3.3 and r = 1.5, with what value of R will the greatest power 
be given to the external circuit? [Saxelby.] 



XVI, §149] TAYLOR^S FORMULA 259 

149. Indeterminate Forms. The quotient of two functions 
is not defined at a point where the divisor is zero. Such 
quotients / (x) -5- <^ (x) at x = a, where / (a) = <t> (a) = 0, are 
called indeterminate forms* We may note that the graph 
of 

(1) ^=i§)' (/(«)=«(a)=0), 

may be quite regular near x = a; hence it is natural to make 
the definition: 

(2) ,] ^m =lual^.. 

Jx^a <t> \X)jx^a x-*a 9 W 

If we apply [D *], we obtain, 

^f(x) _ 0+r(a)(x-a)+E2' 

^ <t>{x) "0 + «'(a)(x-a) + i?2'" 
where 

\Ei'\< M2' {x - a)V2!, I £?2" I S M^" {x - a)V2!, 
and 

Mj' > |r(x) I, M2" > |«"(x) I, near X = a. 
Hence 

<^' (a) + p" M2" ^ 

where p' and p" are numbers between — 1 and +1. It 
follows that 

x->a x-^a <t> W <t> {a) 

unless <^' (a) = 0. But if <!>' (a) = 0,q becomes infinite, and 
the graph of (1) has a vertical asymptote at x = a imless 

♦If 0(a) =0 but /(a) 5*^0 the quotient q evidently becomes infinite; in 
that case the graph of (1) shows a vertical asymptote. 



260 THE CALCULUS [XVI, § 149 

/' (a) = also. If both /' (a) and 0' (a) are zero, it follows in 
precisely the same manner as above, that 

where either /^*^ (a) or 0^*^ (a) is not zero, but all preceding de- 
rivatives of both / (x) and <t> (x) are zero at x = a; and where 
MUi ^ 1/^*+'^ (x) I, Mi'+i > I «(*+^> (x) I near a: = a and where 
p' and p" are numbers between — 1 and +1. It follows 

that 

,. ,. fix) /^*> (g) 

Imi g = lim 77-^ = tott-^ , 

provided all previous derivatives of both f(x) and <t>{x) are 

zero at x = a, and provided 0^*^ (a) ^ 0. If <^^*^ (a) = 0, 

/^*^(a) 7^ 0, then q becomes infinite and the graph of (1) has a 

vertical asymptote at x = a. 

It should be noted that (3) is only a repetition of Rule [VII], p. 31. 
For if w = / (x) and v = <t> (x), since f{a) = <t> (a) = 0, 

= /W =^ fi^)—f (g) ^ 4!f =^ 4^ ^ 4?! 
^ </> (x) (x) — <i>{a) Ay Ax ' Ax ' 

where Ax = x — a; and therefore 

lim o = lim -— -^ lim — = -J- -^ 3- = iihA = -"^t^ , 

x->a Ai->oAx Ax-»oAx L«^ axjx=a L0 (^)J»-o 9(0) 

provided 0' (a) is not zero (see Theorem D, p. 15). 
Example 1. To find lim [(tan x) -r x]. 

Here / (x) = tan x, (x) = x; / (0) = (0) = 0; hence 

,. tan X /' (0) [sec2 x]««o . 

jr->0 X <t> W 1 

Draw the graph q — (tan x) -^ x and notice that this value g = 1 fits 
exactly where x = 0. 

This limit can be found directly as follows: 

,. tanfe _ .. tan {O + h) — tan (0) __ d tan x "| __ „ T __ 1 

^Z h "Ho (o + A)-(o) ~ dx 1=0"^'' ''l^o"^- 



XVI, § 150] TAYLOR'S FORMULA 261 

Example 2. To find lim (1 — cos x)/a;2. 

Here fix) = 1 - cos x, <^ (x) = x^;f(0) = <^ (0) = 0;/' (0) = sin (0) = 
and 0' (0) = 0; /" (x) = cos x, 4>" (x) = 2; hence 

,. 1 ~ cos X __ cos g "| _ 1 

a^-*0 X^ 2 Jar=iO 2 

Draw the graph of g = (1 — cos x)/x2, and note that (x = 0, g = 1/2) 
fits it well. 

150. Infinitesimals of Higher Order. When the quotient 

approaches a finite number not zero when x is infinitesimal: 

(2) lim g = lim^^ = fc 7^ 0, 

1 hen / {x) is said to be an infinitesimal of order n with respect to x. 
An infinitesimal whose order is greater than 1 is called an 
infinitesimal of higher order. 

The equation (2) may be reduced to the form 

(3) lmi[/(a;)-fcx»] = 0, 

a;-K) 

or 

(4) f(x) = (k + E)af^, 

where lim -B = 0. The quantity fcx" is called the principal 
part of the infinitesimal/ (x) . The difference/ (x) — fcx** = Eaf^ 
is evidently an infinitesimal whose order is greater than n, for 

lim (Ex'' -r-x'')=limE = 0. 

Thus by Example 2, § 149, 1 — cos x is an infinitesimal of the second 
order with respect to x; its principal part is x'^/2. Note that 

1 - cos a; = a:2/2+pa^/3 !, 

by [D*], where — 1 ^ p ^ + 1; the principal part is the first term of 
Taylor's Theorem that does not vanish. 

In general, if we have /(O) =/' (0) =/" (0) = • • • =/*-i (0) = 0, but 
/ *> (0) f^ 0, the formula [D*] gives, for a = 0, 

/ (x) = /c*) (0) . X* A I + V Mk-\-i a;*+V(A; + 1) \ 
where Ma+i ^ |/ <*+i) {x) \ near x = 0, and — 1 ^ p ^ + 1. Hence / (x) 
is an infinitesimal of order /c, and its principal part fe/^KO) x^/kL 



262 



THE CALCULUS 



[XVI, § 150 



EXERCISES 

Evaluate the indeterminate forms below, in which the notation 
<t» (x) lo means to determine the limit of 4> (x) when x = a. The vertical 
bar applies to all that precedes it. Draw the graphs as in Exs. 1, 2, above. 



1. sin x/x lo. 



2. sin 2 x/sin 3 X |o. 

.6^—1 



7. 



• x2-l 
tan 2x 



tan 3x 



8. 



^^ log(l-a; 


) 


Xv. 

smo; 




^^ x — sinx 

19. . 




X — tan X 






11. 



X 



1 — cos 2 X 



6 

9. 

12 



8. tan3x/x|o. 



X 

o» — 6» 

X 
logx2 



14 



1 + cos y X 
1 — X — log X 



16. 
19. 



X cos X — sm X 
x3 

o'*>«» — X 
logx 



17. 



sin~^ X 



20 



tan~^ X 

log (x8 - 7) 
• x2-5x + 6 



15. 
18. 



log (1 + x) 



■ I ■ ■ ■ — . — ^ 

X — sin X 



21 s^P"^ (^ — 2) 
' Vx2+x--6 



22. 



in-i Va2 - x2 



sm 



Va2 - x2 



Determine the order of each of the quantities below when the vari- 
able X is the standard infinitesimal : 



23. X — sin X. 

24. «• — «-». 
26. x2 sin x>. 

26. log(l+x)-». 

27. «" — «^». 

28. a»-L 
. log[(a + x)/(a-x)]. 



80. X cos X — sin x. 

81. sin 2 X — 2 sin X. 

82. log cos X. 

88. log (1+ e-i/»). 
84. tan~^ x — sin"i -j.^ 
86. log cos X — sin2 x. 
86. 2x — «» + c^. 



87. QQs'^{l-x)-y/2x'-xK 

151. O^er Indetenmnate Fonns. The numerator and de- 
nominator can be replaced by their derivatives not only 
when the fraction takes the form 0/0, but also when it takes 



XVI, § 151] TAYLOR'S FORMULA 263 

the form 00/ oo (see Pierpont, Functions of a Real Variable y 

p. 305). 

Since f(x)/4> {x) = [I/0 (x)] -r- [l//(a;)], any fraction that takes one 

of the two forms 0/0, 00 -5- 00 , can also be put into the other form. 

Thus, as X -♦ ir/2, tan x and sec x both become infinite, while ctn x and 

cos X approach zero; hence 

,. tan X ,. cos x ^ 
lim = lim — — = 1. 

Z^t/2 sec X x->ir/2 Ctn X 

Likewise, if / (x) -» as 4>{x) becomes infinite, their product is of the 

form X 00 , and it can be put into either of the preceding forms. 

Thus, as X -> 0, log x becomes — 00 ; so that 

lo&r X 1 /x 

lim (x log x) = lim ^rr— = lini — Ti-i = ^^ ("" ^) = 0. 

Other indetei*minate forms are 00 — 00 , 1*, OO, ooo. All these can be 
made to depend on the forms already considered. For let a, /3, 7, 5, €, 
be variables simultaneously approaching, respectively, 00, 00, 1, 0, 0. 
Then a— P, 7«, 5«, a« take, respectively, the preceding four indeter- 
minate forms. But 

lim(a-g)=lim ^/^-j/^ , 

which is of the form 0/0; while the logarithms of the others, 

log 7a = a log 7, log 6* = e log 5, log a« == e log a, 
are each of the form X 00 . 

Example 1. Thus, when x-* ir/2, (sin x)*"* takes the form 1*. But 

(sin x)^° ' = f[log sin x]/otn x 

which approaches the same limit as e"*^'/*^*', as x-* v/2, and this 
limit is evidently e^ = 1. 

Example 2. Similarly, when x becomes infinite, (l/x)^/<2a>+i) takes 
the form 0°. It may be written in the form, 

which approaches the same limit as e~^/2«, that is, the limit is gO =' 1, as 

x->oo. 

Example 3. As an example of the last form, 00 0, take (l/x)« as 
X -> 0. This becomes 

0-^~X I08 X 

and approaches e^ = 1, as x -» 0. 

Indeterminate forms in two variables cannot be evaluated, imless 
one knows a law connecting the variables as they approach their lim- 
its, which practically reduces the problem to a problem in one letter. 



264 



THE CALCULUS 



[XVI, § 151 



EXERCISES 

Evaluate each of the following indeterminate forms, where (r) |a 
means the limit of 4>(x) as x approaches a. Draw a graph in each case. 



1. ^ 



2. 



8 



00 

log ctn X 
log cos X 

secx 



r/2 



• log(ir/2~x) 



4. g 



7. 



8. 



9. 



log X 

log 2 



« 



00 



«/2 Vi 

10. a;2 ctn x |o 



5. 
6. 



oo 

log cos X 
sin2 X 

log sin^ g 
log tan3 X 



11. a;2iogx3|o. 



18. x^* 

14. (l+x)V«|o. 

16. (H-n/x)*U. 

16. (tanx)«<»*|x/2. 

17. (sinac)"*"**|o. 



12. (tan X— sec x) L/2. 18. (tanx ^ ) • 

\ 7r/2-X/\^/2 

Find the value of each of the following improper integrals, using 
Table V, F, when necessary after integrating by parts: 



00 

19. f a 

Jo 



.00 



X e~* dx. 



20. f x2 e-x dx. 
Jo 



21 



Jo 



2 6"^ dx. 



162. Infinite Series. An infinite series is an indicated sum 
of an unending sequence of terms: 

(1) Oo + ai + «2 + • • • + On + • • • ; 

this has no meaning whatever until we make a definition, for 
it is impossible to add all these terms. Let us take the simi 
of the first n terms: 

Sn = «0 + fll + ^2 + • • • + Oji-l, 

which is perfectly finite; if the limit of s„ exists as n becomes 
infinite, that limit is called the sum of the series (1) : 
(2) S = lim Sn =ao + ai H h fln H 

n-»oo 

If lim Sn = S exists, the series is called convergent; if S 

n— »oo 

does not exist, the series is called divergent; if the series 



XVI, §152] SERIES 265 

formed by taking the numerical (or absolute) values of the 
terms of (1) converges, then (1) is called absolutely con- 
vergent. Infinite series which converge absolutely are most 
convenient in actual practice, for extreme precaution is neces- 
sary in dealing with other series. (See § 154. See also 
Goursat-Hedrick, Mathematical Analysis, Vol. I, Chap. VIII.) 

Example 1, The series 1 + r -^ r^ + •••+r» + -"is called a geo- 
metric series; the number r is called the common ratio. A geometric 
series converges absolutely for any value of r numericaUy less than 1; for 

1 r" 

6'„ = 1 + r + r2 H h r^-i = -z -z , 

1 — r 1 — r 

hence 



lim 

n— wo 



1 



1-r 



= lim 
n-*oo 



1-r 



= 0, if lr|<l, 



since r»» decreases below any number we might name as n becomes in- 
finite. It follows that the sum S of the infinite series is 

/S = limsn = :j -, if|r|<l; 

and it is easy to see that the series still converges if r is negative, when 
it is replaced by its numerical value \r\. 

Example 2. Any series a© + Oi + Oa H h «n + • • • of positive num- 
bers can be compared with the geometric series of Ex. 1. Let 

<rn = «0 + Ol + O2 + • • • + On-i; 

then it is evident that a-n increases with n. Comparing with the geomet- 
ric series oo (1 + r + r^ + • • • + r» +•••)» it is clear that if 

where Sn = 1 + r + • • • + r*»~^. Hence an approaches a limit if Sn does, 
i.e. if < r < 1. It follows that the given series converges if a value of 
r < 1 can be found for which On < aor^, that is, for which an -^ On-i < r 

< 1. There are, however, some convergent series for which this test can- 
not be applied satisfactorily. It may be applied in testing any series for 
absolute convergence; or in testing any series of positive terms. For 
example, consider the series 

111 1 



266 



THE CALCULUS 



[XVI, § 152 



here a„ = 1/n!, a„-i = l/(n — 1)!, and therefore On/on-i = (n — l)!/n! 
= 1/n, Hence On/On-iK 1/2 when w > 2, 

1 



^-^^ + r! + ^! + 



+ 



>1 + 



(l+^+l 



+ 



+ 2«-2 j 



(n-i;i 

= 1 +«»-!, 

where 8»-i = 1 + r + • • • + r»-2^ r = 1/2. It follows that the given 
series converges and that its sum is less than 1+2 — 3. [Compare 
§ 154, p. 269; it results that « < 3. Compare Ex. 2, p. 268.] 



153. Taylor Series. General Convergence Test Series which 
resemble the geometric series except for the insertion of con- 
stant coeflScients of the powers of r, 



(1) 



A + Br + 07^ + 07^ + 



arise through application of Taylor's Theorem [D *], § 147, 
p. 254; such series are called Taylor series or power series. 
The properties of a Taylor series are, like those of a geometric 
series, comparatively simple. Comparing (1) with [D *], 
we see that r takes the place of (x— a), while A,B,C,D, • • • 
have the values: 

If we consider the sum of n such terms: 

^(n-1)!^^ ^^ ' 
we see by [D *], that 

fix) = Sn + En, where \En\ ^ M^ '-^^ , M^ > \r\x)\; 



n I 



or 



Sn=f{x)-En. 



XVI, §153] SERIES 267 

It follows that if En approaches zero as n becomes infinite, the 
infinite Taylor Series 

V (a) f" id) 

+ ...+-'-^(x-a)«+... 

converges, and its sum is S = lim Sn =f(x).* 
This is certainly true, for example, whenever \f^^\x) \ re- 
mains, for all values of n, less than some constant C, however 
large, for all values of x between x = a and x = b. For in 
that case 

Um |£n I < lim C • l^Zl^ = c liml^^^ = 

for all values of (x — a).t When | f^^\x) \ grows larger and 
larger without a bound as n becomes infinite, we may still 
often make | En \ approach zero by making (x — a) numeri- 
cally small. 

Example 1. Derive an infinite Taylor series in powers of x for the 
function / (x) = sin x. 

Since f(x) = sin x, we have /' (x) = cos x, /" (x) = — sin x, and, in 
general, f^^^{x) — ± sin x, or ± cos x; hence 

\/n(x)\<l,\un\En\<lim^.=0; 

therefore the infinite series [D**] for a = is 

sinx = + a; + 0-^x3 + o + ^,x5+...; 

this series certainly converges and its sum is sin x for all values of x, 
since lim \En\ = 0. 

* This result is forecasted in § 147. 

fThis results from the fact that n eventually exceeds (x—a) niuneri- 
cally; afterwards an increase in n diminishes the value of En more and more 
rapidly as n grows. 



268 THE CALCULUS [XVI, § 153 

Example 2. Derive an infinite series for e* in powers of (x — 2). 
Since / (x) = «f*. we have / (x) =«*,--•, /(">(x) = c«; hence / (2) = «?, 
f (2) = c», • • •, /(•> (2) = c», and |/t»>(x) | < & where 6 is the largest 

value of X we shall consider. Then the series 

e. = e« + e«(x-2) + ^(x-2)«+...+^(x-2)«+... 

= 6?[l + (x-2)+^(x-2)« + ...+i-,(x-2)«+...] 

conveiiges and its sum is e^, for all values of x less than 6; for 

lim|^«| < lim ^'''";^'" =0. 



Since 6 is any number we please, the series is convergent and ite sum is 
«^ for all values of x. 

EXERCISES 

Derive the following series, and show, when possible, that theyxx)n- 
verge for the indicated values of x. 

1. oosx = l-x2/2! + x4/4!-x«/6!+..; (allx). 

2. ©• = l+x + xV2!+x3/3!+---; (aUx). 
8. «-' = I-x+xV2!-x3/3!+---; (aUx). 

4. tanx=x + x3/3 + 2x5/15 + 17xV315+.--; (|x|<«'/4). 

5. log(l+x)=x-xV2+x3/3-x4/4+...; (|x|<l). 

6. sinhx = (^-c-')/2=x+x3/3! + x5/5!+---; (aUx). 

7. coshx-(c« + 6-»)/2 = l+xV2! + x4/4!+ .-•; (aUx). 

8. tanh x = sinhx/coshx = x - x3/3 + 2 x6/15 - 17 xV315 H ; 

(aUx). 

9. Show that the series of Ex. 6 can be obtained from those of | 
Exs. 2 and 3 if the terms are combined separately. i 

10. Show that the series of Ex. 3 results from the series of Ex. 2 if x 
is replaced by — x. 

11. Obtain the series for sin x in powers of (x — x/4). 

I 

12. Obtain the series for e» in terms of powers of (x — 1). 

13. Obtain the series for log x in powers of (x — 1). Compare it 
with the series of Ex. 5. 



XVI, §154] SERIES 269 

14. Obtain the series for log (1 — x) in powers of x, directly; also by 
replacing a; by — a; in Ex. 5. 

16. Using the fact that log [(1 +a;)/(l - a;)] = log (1 +a;) - log 
(1 ~ x)j obtain the series for log [(1 +a;)/(l — x)] by combining the 
separate terms of the two series of Ex. 14 and of Ex. 5. This series is 
actually used for computing logarithms. 

16. Show that the terms of the Maclaurin series for (a + x)^ in 
powers of x are precisely those of the usual binomial theorem. 

17. Show that the series for e*»+« in powers of a; is the same as the 
series for e* all multipUed by e». 

18. Show that the series for 10* is the same as the series for «» with 
X replaced by x/Mj where M = 2.30- • •. 

164. Precautions about Infinite Series. There are several 
popular misconceptions concerning infinite series which yield 
to very commonplace arguments. 

(a) Infinite series are never used in compiUation. Contrary 
to a popular belief infinite series are never used in computa- 
tion. What is actually done is to use a few terms (that is, 
a polynomial) for actual computation; one may or may 
not consider how much error is made in doing this, with an 
obvious effect on the trustworthiness of the result. 

Thus we may write 

x3 . a;6 a;2*+i 

but in practical computation, we decide to use a few terms, say sin a; = a; 
— a;3/3! -\-(jfi/5l The error in doing this can be estimated by § 147, 
p. 253. It is 1^7 1 <\x'^/7\\. For reasonably small values of x [say 
I x\ <14° <l/4 (radians)], | J^7 1 is exceedingly small. 

Many of the more useful series are so rapid in their convergence that 
it is really quite safe to use them without estimating the error made; but 
if one proceeds without any idea of how much the error amounts to, 
one usually computes more terms than necessary. Thus if it were re- 
quired to calculate sin 14° to eight decimal places, most persons would 
suppose it necessary to use quite a few terms of the preceding series, if 
they had not estimated E7. 



270 THE CALCULUS [XVI, § 154 

9 

(6) No faith can be placed in the fact that the terms are becomr 
ing smaller. The instinctive feeling that if the terms become 
quite small, one can reasonably stop and suppose the error 
small, is unfortunately not justified.* 

Thus the series 

has terms which become small rather rapidly; one instinctively feels 
that if about one hundred terms were computed, the rest would not 
affect the result very much, because the next term is .001 and the suc- 
ceeding ones are still smaller. This expectation is violently wrong. 

As a matter of fact this series diverges; we can pass any conceivable 
amount by continuing the term-adding process. For 

A -f A > 2 • A = ^, 

^ + ^ + '- +A>^'h =A, 

A ■+- lie + • • • -f liiT > 8 • xiiy = A» 

and so on; groups of terms which total more than 1/20 continue to ap- 
pear forever; twenty such groups would total over 1; 200 such groups 
would total over 10; and so on. The preceding series is therefore very 
deceptive; practically it is useless for computation, though it might 
appear quite promising to one who still trusted the instinctive- feeUng 
mentioned above. 

(c) If the terms are alternately positive and negative,, and if 
the terms are numerically decreasing with zero as their limits 
the instinctive feeling just mentioned in (b) is actually correct: 
the series a© — ai + a2 — as + • • • converges if a„ approaches 
zero; the error made in stopping with a„ is less than a„+i.t 

For, the sum Sn = Oo — ai + • • • d= On-i evidently alternates 

m 

between an increase and a decrease as n increases, and this 

* This fallacious instinctive feeling is doubtless actually used^ and it is 
responsible for more errors than any other single fallacy. The example 
here mentioned is certainly neither an unusual nor an artificial example. 

f One must, however, make quite sure that the terms actually approach 
zero, not merely that they become rather small ; the addition of .0000001 to 
each term would often have no appreciable effect on the appearance of the 
first few terms, but it would make any convergent series diverge. 



XVI, §154] SERIES 271 

alternate swinging forward and then backward dies out as n 
increases, since a„ is precisely the amount of the nth swing. 

On each swing s„ passes a point S which it again repasses 
on the return swing; and its distance from that point is 
never more than the next swing, — never more than a„-|-i. 
Since a„ approaches zero, s» approaches S, as n becomes 
infmite. 

Thus the series for sin x is particularly easy to use in calculation: the 
error made in using x — x^/3\ in place of sin x is certainly less than 
ix^/6l The test of § 147 shows, in fact, that the error {Esl <M6|a;V5!|, 
where Ms = 1. 

The similar series for e*: 

is not quite so convenient, since the swings are all in one direction for 
positive values of x; certainly the error in stopping with any term is 
greater than the first term omitted. The error can be estimated by § 147, 
p. 253; thus E5 (for a; >0) is less than Msx^/5ly where Ms is the maximum 
of f^{x) =0* between x = and a; = x, t.e. e*; hence ^6<e*x5/5!. 
Note that e» > 1 for a; > 0. 

Another means of convincing oneself that the preceding series con- 
verges for a; < 1 is by comparison with a geometric series with a ratio 
a;/2, as in Example 2, p. 265. But this method would require the com- 
putation of a vast number of terms, to make sure that the error is small. 

(d) A consistently small error in the values of a function may 
make an enormmis error in the values of its derivative. 

Thus the function y - x^ .00001 sin (100000 x) is very well ap- 
proximated b^ the single term y = x, — in fact the graphs drawn ac- 
curately on any ordinary scale will not show the slightest trace of dif- 
ference between the two curves. Yet the slope of 2/ = x is always 1, 
while the slope of y =x — .00001 sin (100000 x) oscillates between 
and 2 with extreme rapidity. Draw the curves, and find dy/dx for 
the given function. 

One advantage in Taylor series and Taylor approximating 
polynomials is the known fact — proved in advanced texts — 



272 THE CALCULUS fXVI, § 154 

that differentiation as well as integration is quite reliable on any 
valid Taylor approximation* 

Thus an attempt to expand the function y = x — .00001 sin (lOOOOOx) 
in Taylor form gives 

r 1000002 , , 1000004 _ i 

y =a;— I a; ^ — a^ -\ ^ — a^ ~ •••!» 

which would never be mistaken f or y = a; by any one; the series indeed 
converges and represents y for every value of x, but a very hasty exam- 
ination is sufficient to show that an enormous number of terms would 
have to be talcen to get a reasonable approximation, and no one would 
try to get the derivative by differentiating a single term. 

If the relation expressed by the given equation was obtained by ex- 
periment, however, no reliance can be placed in a formal differentiation, 
even though Taylor approximations are used, for minute experimental 
errors may cause large errors in the derivative. Attention is called to 
the fact that the preceding example is not an unnatural one, — pre- 
cisely such rapid minute variations as it contains occur very frequently 
in nature. 

EXERCISES 

1. Show that the series obtained by long division for 1 -5- (1 + x) 
is the same as that given by Taylor^s Series. 

2. Obtain the series for log (1 -f- x) (see Ex. 5, § 153), by inte- 
grating the terms of the series found in Ex. 1 separately. 

3. Find the first four terms of the series for sin"^ x in powers of x 
directly; then also by integration of the separate terms of the series for 

i/vr^=^. 

4. Proceed as in Ex. 3 for the functions tan~i x and 1/(1 -|- x^). 

6. Show that the series for cos x in powers of re is obtained by dif- 
ferentiating separately the terms of the series for sin x, 

6. Show that repeated differentiation or integration of the separato 
terms of the series for e* always results in the same series as the original 
one. 

7. From the series for tan~ia; compute x by using the identity 
x/4 = 4 tan-i (1/5) - tan-i (1/239). 

* See, e.g., Goursat-Hedrick, Mathematical AncUysis, Vol. I, p. 380. 



rjn, §154] SERIES 273 



2 /•* 

9. The "error integral" is P (re) = — ^ / e~^ dx. Express P (x) as a 



8. The Gudermannian of x is gd (x) — 2 tan~* e» ~ x/2; expand in 
powers of a;, calculate gd(.l) = 6° 43', and gd (.7) = 37° 11'. 

series in powers of x; calculate P(.l) = .1126, P(l) = .8427, P (2) = 
.9953+. 

10. Show that ^^^^dx =» LSI". 18. Show tha,tfdt/VT^^ = .608+. 

11. Show that J^^^dx = 1.78+ 14. Show thatyd«/VT^= 1.31 1+. 

12. Show that /*' sin ^/*xdx = .930^. 



CHAPTER XVII 
PARTIAL DERIVATIVES— APPLICATIONS 

166. Partial Derivatives. If one quantity depends upon two 
or more other quantities, its rate of change with respect to one 
of them, while all the rest remain fixed, is called a partial 
derivative.* 

If z = f (x, y) is a function of x and i/, then, for a constant 

value of i/, 1/ = fc, z is a function of x alone: z = / (x. A;) ; the 

derivative of this function of x alone is called the partid 

derivative of z with respect to x, and is denoted by any one of 

the symbols 

dz ^ df(x, y) ^ . .^^._ df{x,k) 

Aa;— ►O ^X 

A precisely similar formula defines the partial derivative 
of z with respect to y which is denoted by dz/dy. 

In* general, if w is a function of any number of variables x, 

y, z, ' - ' , and if one calculates the first derivative of u with 

respect to each of these variables, supposing all the others to 

be fixed, the results are called the first partial derivatives of 

u with respect to x, i/, z, • • • , respectively, and are denoted by 

the symbols 

du/dXj du/dy, du/dZj • • • . 

* This notion is perhaps more prevalent in the world at large than the 
notion of a derivative of a function of one variable, because quantities in 
nature usually depend upon a great many influences. The notion of par- 
tixd derivative is what is expressed in the ordinary phrases "the rate at 
which a quantity changes, everything else being supposed equal," or 
"... other things being the same." 

274 



XVII, § 156] PARTIAL DERIVATIVES— APPLICATIONS 275 

Example 1. Given 2 = x^ + 1/2, to find bzjbx and bzjdy. 
To find dg/dx, think of y as constant: y — h\ then 

ds ^ a(x2+i/2) ^ rf(x2+A;2) =2x- - =2t/ 
dx dx dx ' dy ^' 



Example 2. Given 2 = x^ sin(x +y^)j to find dsi/^x. and dz/dy. 
dz ^ a|x2sin(x+y^)l _ r <^(x2sin(xH-fc2)| 

dx dx 



r dlx^am(x + mn 

L dx Jy-i 

^ 2 X sin (x -f 2/^) -f a?^ cos (x -f y^)- 

dz ^ a(x2 8in(x4-y^)} ^ r d{k^8m(k + t^)n 
dy dy L dy Ja;-* 

=2 x2 y cos (x -f y^)- 

166. Higher Partial Derivatives. Successive differentiation 
is carried out as in the case of ©rdinary differentiation. 
There are evidently four ways of getting a second partial 
derivative: differentiating twice with respect to x; once with 
respect to x, and then once with respect to y] once with 
respect to y, and then once with respect to x; twice with re- 
spect to y. These four second derivatives are denoted, re- 
spectively, by the symbols 

dxKdxJ dx^ J^^^>y)y ey\dxJ dydx •'^^^'^z;, 

dy \dy/ " dy^ " "^^ ^^' ^^ ' dx \dyJ ' dxdy^ ^'' ^^' ^^ • 

There is no new difficulty in carrying out these operations; 
in fact the situation is simpler than one might suppose, for 
it turns out that the two cross derivatives fxy and fyx are 
always equal; the order of differentiation is immaterial,* 

A similar notation is used for still higher derivatives: 

^^ " dx3 "■ dx \dxy ' ^^"^ "■ d2/dx2 - dy \dx^)'' 

etc., and the order of differentiation is immaterial. 

♦At least if the derivatives are themselves continuous. See Goursat- 
Hedrick, Mathematical Analysis, Vol. I, p. 13. 



276 THE CALCULUS [XVII, § 156 

The ordef of a partial derivative is the total number of successive 
differentiations performed to obtain it. The partial derivatives of the 
first and second orders are very frequently represented by the letters 
V> Qy r, «, t: 

^ dx'^ dy'^ dx^'^ dxdy dydx' dy^' 

Example 1. Given z — x^ sin (x + y^), show that fxy = fyx- 
Continuing Example 2, § 155, we find: 

^=1^(1) =|;[2=^«^ (- + «'*)+-' «»(- + »*)] 

= 4 xy cos (x +y^) — 2x^y sin (x + y*). 

dx dy dx \dy/ dxt v • if / j 

^4xy C08 (x-{- y^) — 2 x^j/ sin {x + y^), 

EXERCISES 

Find the first and second partial derivatives, ds/dx, ds/dy^ d^s/dx^, 
d2 z/dx dyy d2 g/dy QXy and d^ zjdy'^ for each of the following functions. In 
each case verify the fact that d^z/dx dy = d'^z/dy dx, 

1. z=x^ — 2/2. 4. 3 = e<w+»y. 7. 3 = (x + 2/) e^i''. 

2. z^x^y-\- xy^. 6. z = tan-i iyjx), 8. s = (x^/ — 2 2/2)5/3. 
8. s = sin (x2 + 2/2). 6. 3 = e*sin2/. 9. s = log (x2 + 2/2)i/2. 

10. The volume of a right circular cylinder is v = nr2 A. Find the rate 
of change of the volume with respect to r when h is constant, and ex- 
press it as a partial derivative. Find dv/dA, and express its meaning. 

11. The pressure p, the volume v, and temperature ^ of a gas are 
connected by the relation yo — kO, where is measured from the ab- 
solute zero, — 273° C. Assuming constant, find dp/dv and express 
its meaning. If the volume is constant, express the rate of change of 
pressure with respect to the temperature as a derivative, and find its 
value. 

12. Find the rate of change of the volume of a cone with respect to its 
height, if the radius, is constant; and the rate of change of the volume 
with respect to the radius, if the height is a constant. 

18. Show that the functions in Exercises 1, 5, 6, and 9 satisfy the 
equation ^z/dx^ -f ^z/dy^ = 0. 



XVII, § 157] PARTIAL DERIVATIVES— APPLICATIONS 277 



14. A point moves parallel to the x-axis. What are the rates of 
change of its polar coordinates with respect to xl 

16. Show that the rate of change of the total surface of a right 
circular cylinder with respect to its altitude is dA/dh = 2 ir r; and that 
its rate of change with respect to its radius is dA/dr = 2irk-{-4irr. 

16. Calculate the rate of change of the hypotenuse of a right triangle 
relative to a side, the other side being fixed; relative to an angle, the 
opposite side being fixed. 

17. Two sides and the included angle of a parallelogram are a, b, C, 
respectively. Find the rate of change of the area with respect to each 
of them, the other two being fixed; the same for the diagonal opposite 
toC. 

18. In a steady electric current C = V -^ /2, where C, V, R, denote 
the current, the voltage (electric pressure), and the resistance, respec- 
tively. Find d C/d V and d C/d R, and express the meaning of each of 
them. 

157. Geometric InterpretatioiL The first partial deriva- 
tives of a function of two independent variables 

can be interpreted geometrically in a simple manner. This 
equation represents a 
surface, which may 
be plotted by erect- 
ing at each point of 
the xt/-plane a per- 
pendicular of length 
f(x, y); the upper 
ends * of these per- 
pendiculars are the 
points of the surface. 
Let ABCD be a 
portion of this sur- 




/"p<h,k,o) 



Fig. 77. 
* If 2 is negative, of course the lower end is the one to take. 



278 THE CALCULUS • [XVII, § 157 

face lying above an area abed of the x2/-plane. If x varies 
while y remains fixed, say equal to fc, there is traced on the 
surface the curve HK, the section of the surface by the plane 
y = k. The slope of this curve is dz/dx. 

Similarly, dz/dy is the slope of the curve cut from the 
surface by a plane x = A. 

168. Total Derivative. If in addition to the function 
z= f{x,y)y a relation between x and y, say y = 4>{x), is given, 
z reduces by simple svbstiiution to a function of one variable: 

z=f{x, 2/), y = (t>{x) gives z =/(x, 0(x)). 

Now any change Ax in x forces a change Ay iny; hence y 
cannot remain constant (unless, indeed, (x) = const.). 
Hence the change Az in the value of z is due both to the direct 
change Ax in a: and also to the forced change Ay in y. We 
shall call 

Az = the total change in 2 = / (x + Ax, y + Ay) — / (x, j/), 

Ax2 = the partial change due to Ax directly 

= /(x + Ax, I/) -f(x,y), 
AyZ = the partial change forced by the forced change Ay 

= Az- A^z, = /(x + Ax, 2/ + A?/) -/(x + Ax, y). 
It follows that 

(1) ^ = lim— j^lim (/(^+^.vH-Ay)-/(..y)\> 



= l^ ^ajg +AyZ { ^^m^ f f(x-{-/!iX,y)-f{x,y) 
Aa>-^ Ax < AI^->0\ ^ 

.y)Ai/\l. 



Aaj-K) 

/ (X -\-Ax, V + Ay) -/ {x +Aa; 



+ AV 



XVII, 1 158] PARTIAL DERIVATIVES— APPLICATIONS 279 
whence, if the partial derivatives exist and are continuous,* 

dz ,. ^^xz ^vz^y\ 

or, multiplying both sides by dx(=Ax), 



dz dzdy 
di'^dydx' 



(3) 



dz , dz , . J dy , 




where dy = <t> (x) dx. Since <^(x) is 
any function whatever, dy is really 
perfectly arbitrary. Hence (3) holds 
for any arbitrary values of dx and dy 
whatever, where dz = {dz/dx) dx is 
defined by (2); dz is called the 
total differential of z. 

These quantities are all repre- 
sented in the figure geometrically: ^^^^^^^ 
thus A2 = A^ + AyZ is represented st=cd^av 

by the geometric equation TQ = 'J^'XCTJ^I^q'^R^ 
SR + MQ. It should be noticed az=QoQ-PoP=tq='SR+mq 
that dz is the height of the plane '^"^ ^:^«-«+a» 
drawn tangent to the surface at P, since dz/dx and a^/dy 
are the slopes of the sections of the. surface hy y = yp and 
X = xp, respectively. [See also § 163.] 

If the curve PqQo in the xi/-plane is given in parameter 
form, X = 4>(f)y V = ^(^)» ^^ "^^^ divide both sides of (3) 
by dl and write 



(4) 



dz _dzdx .dzdy 
di " dx dt dy dt' 



since dx^di = dx/dt, dy -^ dt = dy/dt. 

*For a more detaUed proof using the law of the mean, see Goursat-Hed- 
rick, Mathematical Analysis, I, pp. 38-42. 



280 THE CALCULUS [XVII, § 159 

159. Elementary Use. In elementary cases, many of which 
have been dealt with successfully before § 158, the use of the 
formulas (2), (3), and (4) of § 158 is quite self-evident. 

Example 1. The area of a cylindrical cup with no top is 
(1) A=2irM + irr2, 

where h is the height, and r is the radius of the base. If the volume of 
the cup, Tf^ hf ia known in advance, say xr^ h = 10 (cubic inches), we 
actually do know a relation between h and r: 

o. »-^, 

whence 

(3) A=2irr^ + irr2 = -+irra 

from which dA/dr can be found. We did precisely the same work in 
Ex. 26, p. 57. In fact even then we might have used (1) instead of (3), 
and we might have written 

(4) ^ = 2 irr - +2 tA + 2 irr, or dA = 2 irr dh + (2 irh-\-2 irr) dr, 

where dh/dr is to be found from (2). 

This is precisely what formula (2), § 158, does for us; for 

(5) ^=2irA + 2^r, ^-2^r, 

^ =(2irA+2irr) + (2irr)^, or dA^ {2 Th+2 irr) dr +2 xr dL 

We used just such equations as (4) to get the critical values in finding 
extremes for dA/dr = at a critical point. We may now use (2), § 158, 
to find dA/dr] and the work is considerably shortened in some cases. 

Example 2. The derivative dy/dx can be found from (2),* § 158, if 
we know that z is constant. 

Thus in § 24, p. 39, we had the equation 
(1) a;2 + 2/2=:i, 

and we wrote: 
whence we found 



XVII, § 160] PARTIAL DERIVATIVES— APPLICATIONS 281 

This work may be thought of as follows: 
Let 2 = x2 + ^; then 

dx dx dx'^dydx '^^ dx* 

but s = 1 by (1) above; hence dz/dx = 0, and 

2x+2j,f^=0,or^ = -5. 
dx dx y 

Thus the use of the formulas of § 158 is essentially not at 
ail new; the preceding exercises and the work we have done 
in §§ 24, 29, etc., really employ the same principle. But 
the same facts appear in a new light by means of § 158; 
and the new formulas are a real assistance in many examples. 

160. Small Errors. Partial Differentials. Another appUcation 
closely allied to the work of § 145, p. 248, is found in the esti- 
mation of smaU errors. 

Example 1. The angle A of a right triangle ABC (C = 90°) may 
be computed by the formula 

tan A = Tf OT A = tan~i _^ 

where a, 6, c are the sides opposite A, B, C, If an error is made in 
measuring a or 6, the computed value of A is of course false. We may 
estimate the error in A caused by an error in measuring a, supposing 
temporarily that b is correct, by § 145; this gives approximately 

1 

dA b b 

1+52 

where d is used in place of d of i 145, since A really depends on & also, 
and we have simply supposed b constant temporarily. Likewise the 
error in A caused by an error in 6 is approximately, 

_ ^ 

62 



282 THE CALCULUS [XVII, § 160 

If errors are possible in both measurements, the total error in A is, 
approximately, the sum of these two partial errors: 

The methods of § 146, p. 251, give a means ot finding how nearly 
correct these estimates of AoA, ^A, and A A are; in practice, such 
values as those just found serve as a guide, since it is usually desired 
only to give a general idea of the amounts of such errors. 

This method is perfectly general. The differences in the 
value of a function z = f{x, y) of two variables, x and i/, which 
are caused by differences in the value of x alone, or of y alone, 
are denoted by A^a:, Ay2, respectively. The total difference 
in z caused by a change in both x and y is 

A2 =/(a: + Ax, 2/ + At/)-/(a:, i/) 

= [/(x + Ax, 2/ + Ai/) -/(x + Ax, y)] + [/(x + Ax, y) 

-fix,y)] 

as in § 158. The differences A^^ and AyZ are, approximately,* 

whence, approximately, 

Az = A^ + Ajs = £Az + ~Ay. 

♦ More precisely, these errors are 

A,^ = I • Ax + E',. A^ = %\_^^ A„ + E",. 

where | E'2 \ and | E^'t \ are less than the maximum Mt of the_yalues of all of 

the second derivatives of z near (x, y) multiplied by A?, or Ay*, respectively 

(see §146). And since dz/dj/ is itself supposed to be continuous, we may 

write 

dz ^ , dz . , „ 
Az^^^Ax+^Ay-\-E2, 

where | ^2 1 is less than Af2( | Ax | + 1 ^2/ 1 )*• [Law of the Mean. Compare 
5146.] 



XVII, § 160] PARTIAL DERIVATIVES— APPLICATIONS 283 

The products (dz/dx) dx and (dz/dy) dy are often called 
the partial differentials of z, and are denoted by 

dz dz 

b^ = -r- dXj dyZ = -r- dy, whence dz = djfi + d^z. 
ox ay 

We have therefore, approximately, 

Az = d^ + dyZy 

within an amount which can be estimated as in § 146 and in 
the preceding footnote. 

Similar formulas give an estimate of the values of the 
changes in a function u = f{x, y, z) of the variables x^y^z; 
we have, approximately, 

A ^^ A A ^^ A A ^^ A 

A.u=-Ax, AyU^^Ay, A,ii=-A., 
Au = AxU + AyU + A^u=— Ax + —Ay + — Az, 

within an amount which can be estimated as in the preceding 
footnote. The generalization to the case of more than three 
variables is obvious. 

EXERCISES 

Find dy/dx in each of the following implicit equations by method of 
Ex. 2, § 159: 

1. a;2 + 4 2/2 = 1. 3. x^ + y^''Sxy = 0. 

2. 7x2-9^2 = 36. 4. 2/2(2a-a;) =a^. 

5. If Ay By C denote the angles, and a, 6, c the sides opposite them, 
respectively, in a plane triangle, and if a, il, B are known by measure- 
ments, 6 = a sin B/sin A, Show that the error in the computed value 
of b due to an error da in measuring a is, approximately, 

dab = sin B CSC A da. 
Likewise show that 

djj) = — a sin 5 CSC A ctn Ad Ay and dsb = a cos B cac Ad B] 

and the maximum total error is, approximately, \db\ ^ \dab\4- \dAb\ 

+ I dsbl. Note that dA and dB are to be expressed in radian measure. 



284 THE CALCULUS [XVII, § 160 

6. The measured parts of a triangle and their probable errors are 

a = 100 ± .01 ft., A = 100° ± 1', B = 40° ± 1'. 

Show that the partial errors in the side h are 

dab = ± .007 ft., dAh = ± .003 ft., a^ = ± .023 ft. 

If these should all combine with like signs, the maximum total error 
would be db^ ± .033 ft. 

7. If a = 100 ft., B = 30°, A = 110°, and each is subject to an 
error of 1%, find the per cent of error in 6. 

8. Find the partial and total errors in angle B, when 

a = 100 ± .01 ft., 6 = 159 ± .01 ft., A = 30° ± 1'. 

9. The radius of the base and the altitude of a right circular cone 
being measured to 1%, what is the possible per cent of error in the 
volume? Ana. 3%. 

10. The formula for index of refraction is m = sin I'/sin r, i being the 
angle of incidence and r the angle of refraction. If i = 50° and r = 40°, 
each subject to an error of 1%, what is m, and what its actual and its 
percentage error? 

11. Water is flowing through a pipe of length L ft., and diameter 
D ft., imder a head of H ft. The flow, in cubic feet per minute, is 

Q = 2356 V jr, j-30/) * H L = 1000, D = 2, and ^ = 100, determine 

the change in Q due to an increase of 1% in H; in L; in D, Compare 
the partial differentials with the partial increments. 

161. Envelopes. The straight line 

(1) y = kx — k^y 

where fc is a constant to which various values may be assigned, 
has a different position for each value of k. All the straight 
lines which (1) represents may be tangents to some one curve. 
If they are, the point P*, (x, y) at which (1) is tangent 
to the curve, evidently depends on the value of k: 

(2) x = 0(fc), y = 4^{k); 



XVII, § 161] PARTIAL DERIVATIVES— APPLICATIONS 285 



these equations may be considered to be the parameter 
equations of the required 
curve. The motive is to 
find the functions <l>{k) and 
^(fc) if possible. 

Since Pt lies on (1) and 
on (2), we may substitute 
from (2) in (1) to obtain: 

(3) ^(fc) = k<t>{k) - P, 

which must hold for all 
values of fc. Moreover, 
since (1) is tangent to (2) at 
Ptj the values of dy/dx 
found from (1) and from (2) 
must coincide : 




(4) 



^ J from (1) ^ J from (2) 



Fig. 79. 



or fc0'(fc) = ^'(fc). 



To find 0(A;) and ^(fc) from the two equations (3) and (4), it 

is evident that it is expedient to dififerentiate both sides of (3) 

with respect to fc: 

(3*) ^'(fc) = A;0'(fc) + 0(fc) - 2 fc; 

this equation reduces by means of (4) to the form 

(5) = + 0(fc) - 2 fc, or 0(fc) = 2 fc, 
and then (3) gives 

(6) ^(fc) = fc(2fc)-fc2==fc2. 

Hence the parameter equations (2) of the desired curve are 

(7) x = 2fc, y = k\ 

and the equation in usual form results by elimination of fc: 



(8) 



X 



286 THE CALCULUS [XVII, § 161 

It is easy to show that the tangents to (8) are precisely the 
straight lines (1). 

The preceding method is perfectly general. Given any set of curves 

(1)' F (X, y, k)^0, 

where k may have various values, a curve to which they are all tangent 
is called their envelope; its equations may be written 

(2)' X = (fc), y = iA {k)\ 

whence by substitution in (1)', 

(3)' F[4> (kh ^ (k), k] = 0, 

for all values of k. Differentiating (3)' with respect to k, 

* dF{x,y,k) __dFdx dFdy , dF ^ 

^ ^ dk dx dk '^ dydk'^ dk 

Moreover, since (1)' is tangent to (2)', 



dF . dF _dyl _dy-[ 
^ ^ dx ' dy dxj ^om (1)' dxj ^om (2)' 


_dy , dx, 
dk ' dk' 


whence (3*)' reduces to the form 




(^)' af = «' 





and then (3)' and (5)' may be solved as simultaneous equations to find 
(A;) and ^ {k) as in the preceding example. 

The envelope may be found speedily by simply writing 
down the equations (1)' and (5)', and then eliminating k 
between them It is recommended very strongly that this 
should not be done until the student is familiar with the 
direct solution as shown in the preceding example. 

162. Envelope of Nonnals. Evolute. If y = /(x) is a given 
curve and if yt and m* respectively denote the ordinate and 
slope when x = fc, the equation of any normal may be 
written 

(1) 2/ - y* = - — (a^ - fc), 

or F{x, y, k) = yrriu - ytnit + x - fc = 



XVII, § 162] PARTIAL DERIVATIVES— APPLICATIONS 287 

Hence by (5'), § 161, we have, for the envelope of the system 
of lines (1) when k is regarded as a variable parameter, 

dF 



(2) 



dk 



= y • 6* - y* • fe* - w* • w* - 1 = 0. 



(Remember that in forming dF/dk, x and y are regarded 
as constant, and only k, 
w»> Vk, are regarded as 
variable. We have used 
bi to stand for dmjdk,) 

Solving (2) for y we 
have 

(3) y = y. + ^^- 

This value of y in (1) 
gives 




Fig. 80. 



(4) 



X = fc — m* 



l+m\ 



Equations (3) and (4) are the parametric equations of the 
envelope of the system of normals (1), and are precisely 
equations (1) of § 98, with only a change of notation. Hence 
the envelope of the systems of normals to a given curve is the 
evolute of that curve. 



EXERCISES 

Find the envelopes of each of the following families of curves: 

1. y =Skx'- k^. Ans, y^ = 4 sfi. 

2. y = 4 fcr — A;*. Ana, y^ = 27x^. 

3. y^ =^kx — k^, Ans. y = ± ix. 

4. y = kx ± Vl 4- k^» Ans, a;^ + ^ = 1. 

5. y^ ='J^x — 2k, Ans, xy^ = — 1. 



288 THE CALCULUS [XVII, § 162 

6. (x - A;)2 + 2r^ = 2 k. Ans. y^ ^2x + l. 

7. 4x2 + (y- A;)2 = 1 - ^2. jins. y^+8x^ = 2. 

8. X cos ^ + y sin ^ = 10. Arw. x^+y^ = 100. 

9. Show that the envelope of a family of circles through the origin 
with their centers on the parabola y^ ^ 2 x ia y^(x -\- 1) -^ 3fi — 0, 

10. Show that the envelope of the family of straight lines ax -\-by 
= 1 where a + 6 = a6, is the parabola x^ + y^ = 1. 

11. Show that the envelope of the family of parabolas represented by 
the equation y = x tan a — mx^ sec^ aiay == 1/(4 m) — mx^. 

[Note. If m = g/(2 vq^), the given equation represents the path of a 
projectile fired from the origin with initial speed vq at an angle of eleva- 
tion a.] 

12. The lemni scate (x ^ -j- 2/2)2 = ^2( 3.2 — y 2) m^y ^^ written in the 
form X = a cos t Vcos 2 1] y = Sismt Vcos 2 1, Show that the evolute 

is (x2/3 + 2/2/3)2 (a;2/3 _ ^2/3) = 4 ^2/9. 



CHAPTER XVIII 



CURVED SURFACES — CURVES IN SPACE 

163. Tangent Plane to a Surface. Let Pq be the point 
(xo 2/0, Zq) on the surface z = f(x,y). Let Po^i be the tangent 
line at Pq to the curve cut 
from the surface by the 
plane y = yo and P0T2 the 
tangent line to the curve 
cut from the surface by 
the plane x = Xq. The 
plane containing these 
two lines is the tangent 
plane to the surface at Po. 

Since this plane goes 
through Po, its equation 
can be thrown into the form 

(1) 2 - 2o = A{x - Xo)+B(y- yo). 

If we set y = yo we find the equation of Po^i in the form: 

(2) z — Zo = A{x — Xo), 

But, from § 28, p. 49, the equation of Po^i may be written in 
the form : 




Fig. 81. 



(3) 
Hence 

(4) 



= t1^ " 



likewise B — -;r\ ' 

^2/ Jo 

289 



290 THE CALCULUS [XVIII, § 163 

Thus the equation of the tangent plane is 

or, what is the same thing, 

(6) 2 - 2, = f^(x - X,) + |]^(y - j/o). 

It is important to notice the great similarity between this 
equation and the equation 

(^> '^ = S]o'^ + |].'^«' 

of § 158. Indeed (7) expresses the fact that if dx, dy are 
measured parallel to the x and y axes from the point of tan- 
gency (xo, 2/0, ^o), dz represents the height of the tangent 
plane above (xo, 2/0, ^o). Equation (7) furnishes a good 
means of remembering (6). 

164. Extremes on a Surface. If a function z — f{x^y)]& 
represented geometrically by a surface, it is evident that 
the extreme values of z are represented by the points on the 
surface which are the highest, or the lowest, points in their 
neighborhood: 

(1) / (xo, 2/0) > / (iCo + A, 2/0 + fc), if / (xo, 2/0) is a maximum^ 

(2) / (xo, 2/0) <f{xo + h,yo + k),iif (xq, yo) is a minimum^ 

for all values of h and k for which h^ + k^ is not zero and is not 
too large. 

It is evident directly from the geometry of the figure that 
the tangent plane at such a point is horizontal. 

This results also, however, from the fact that the section 
of the surface by the plane x = xo must have an extreme at 
(^0, 2/0); hence [df/dy]oy which is the slope of this section at 
{xoyo)y must be zero; likewise [df/dx]o, the slope of the 



XVIII, § 164] CURVED SURFACES 291 

section through (xo, 2/0) by the plane y = yo, must be zero. 
Hence equation (5), § 163, reduces to z — Zo = which is a 
horizontal plane. 

A point at which the tangent plane is horizontal is called 
a critical point on the surface. The following cases may 
present themselves. 

(1) The surface may cut through its tangent plane; then 
there is no extreme at (xo, 2/0). 

This is what happens at a point on a surface of the saddleback type 
shown by a hyperbolic paraboloid at the origin; a homeher example is 
the depression between the knuckles of a clenched fist. 

(2) The surface may just touch its tangent plane along a 
whole line, but not pierce through; then there is what is often 
called a weak extreme at (xo, yo); that is, z = f{x, y) has the 
same value along a whole line that it has at (xo, 2/0), but 
otherwise / (x, y) is less than [or greater than] / {xq, i/o). 

This is what happens on the top of a surface which has a rim, such as 
the upper edge of a water glass, or the highest point of an anchor ring 
lying on its side. Most objects intended to stand on a table are provided 
with a rim on which to sit; they touch the table all along this rim, but 
do not pierce through the table. 

(3) The surface may touch its tangent plane only at the point 
(^0, yo); then z = f{x, y) is an extreme at (xo, 2/0): a mini- 
mum, if the surface is wholly above the tangent plane near 
(^0, 2/0) ; a maximum, if the surface is wholly below. 

. The shape of the clenched fist gives many good illustrations of this 
type also. Examples of formal algebraic character occur below. 

Example 1. For the elliptic paraboloid s = x^ + 2/^ the tangent 
plane at (xq, 2/0, 3d) is 

2 — 30 = 2 xo (x — xo) + 2 2/0 (2/ — 2/0), , 

which is horizontal if 2 xq = 2 2/0 = 0; this gives Xq = yo = 3b = 0, 
hence (x = 0, y = 0) is the only critical point. 






292 THE CALCULUS [XVIII, § 164 

At (x = 0, y = 0), ar has the value 0; for any other values of x and j/, 
s ( = x2 + y^) is surely positive. It follows that ;? is a minimum at 
a; = 0, y = 0. 

Example 2. In experiments with a pulley block the weight «? to be 
lifted and the pull p necessary to lift it Were found in three trials to 
be (in pounds) (pj = 5, t^^i = 20), (p2 = 9, «^ = 50), {jpz = 15, 103 = 
90). Assuming that p = au> + /3, find the values of a. and /3 which 
make the sum S of the squares of the errors least. (Compare Ex. 37, 
p. 58.) 

Computing p by the formula aw + /3, the three values are p'l = 
20 a + ^, p'2 = 50 a + /3, p'a = 90 a + /3. Hence the sum of the 
squares of the errors is 

S = (p'l - pi)2 + (p'2 - P2)2 + (p'3- Pzy 

= (20 a + /3 - 5)2 + (50 a + /3 - 9)2 + (9Q a + /3 - 15)2. 
In order that a5 be a minimum, we must have 

^ = 2-[20 (20a + ^ - 5) + 50 (50a + /3- 9) +90 (90a + /3 - 15)] = 0. 
da 

^ = 2 [(20a + /3- 5) + (50 a + /3 - 9) + (90a + ^ - 15)] = 0. 
op 

that is, after reduction, 

1100 + 16 ^ - 190 = 0, a = m = .143, 

160 a + 3 /3 - 29 = 0, /3 = \%<^ = 2.03. 

If the usual graph of the values of p and w is drawn, it will be seen 
that p = aw -{- represents these values very well for a = .143, 
/3 = 2.03 and it is evident from the geometry of the figure that these 
values render S a minimum, S = .0545; for any considerable increase 
in either a or j8 very evidently makes S increase. Since this is the 
only critical point, it surely corresponds to a minimum, for the function 
S has no singularities. 

This conclusion can also be reached by thinking oi S aa represented 
by the heights of a surface over an a/3 plane, and considering the sectien 
of that surface by the tangent plane at the point just found as in Ex. 3 
below; but in this problem the preceding argument is simpler. 

It is customary to assume that the values of a and /3 which make S a 
minimum are the best compromise, or the " most probable values'* ; 
hence the most probable formula for p is p = .143 w + 2.03. 

The work based on more than three trials is quite similar; the only 
change being that S has n terms instead of 3 if n trials are made. 



The plane 

^-300 



XVIII, § 164] CURVED SURFACES 293 

Example 3. Find the most economical dimensions for a rectangular 
bin with an open top which is to hold 500 cu. ft. of grain. 

Let X, y, h represent the width, length, and height of the bin, respec- 
tively. Then the volume is xyh; hence xyh = 500; and the total area z 
of the sides and bottom is 

, . , o 1 . o I. 1 1000 , 1000 

(a) z = xy + 2hy-\-2hx=xy-] 1 • 

X y 

If this area (which represents the amount of material used) is to be a 
minimum, we must have 

,,, dz 1000 ^ dz 1000 ^ 

Substituting from the first of these the value y = lOOO/x^ in the 
second, we find 

(c) X — r^r^ = 0, whence a; = 0, or a; = 10. *' 

lo^ 

The value x = is obviously not worthy of 

any consideration; but the value x = 10 gives 

y = lOOO/x^ = 10 and h = 500/{xy) = 5. ^ i^ * 

The value of z when x = 10, 2/ = 10 is 300. If ' ^^^' ^' 

the equation (a) is represented graphically by a surface, the values of z 
being drawn vertical, the section of the surface by the plane z — 300 
is represented by the equation 

(d) xy + ^509 + 122? = 300, or x^y^ - 300 xy + 1000 (x + 2/) = 0. 

X y 

This equation is of course satisfied by x = 10, 2/ = 10. If we attempt 
to plot the curve near (10, 10), — for example, if we set y = 10 + A; 
and try to solve for x in the resulting equation: 

(10 + A;)2x2 - (300 A; + 2000) X + 1000(10 + A;) = 0, 

the usual rule for imaginary roots of any quadratic ax^ + 6x + c = 

shows that 

62 - 4 oc = - 1000 A;2 [4 A; + 30] < 

for all values of k greater than — 7.5. Hence it is impossible to find 
any other point on the curve near (10, 10). It follows that the hori- 
zontal tangent plane z = 300 cuts the surface in a single point; hence 
the surface lies entirely on one side of that tangent plane. Trial of 
any one convenient pair of values of x and y near (10, 10) shows that z 
is greater near (10, 10) than at (10, 10) ; hence the area 2 is a minimum 
when X = 10, y = 10, which gives A = 5. 



294 



THE CALCULUS 



[XVIII, § 165 



165. Final Tests. Final tests to determine whether a func- 
tion f{x, y) has a maximum or a minimum or neither, are 
somewhat diiSScult to obtain in reliable form. Comparatively 
simple and natural examples are known which escape all set 
rules of an elementary nature.* (See Example 1 below.) 

One elementary fact is often useful: if the surface has a 
maximum at (xo, 2/0), every vertical section through (xo, t/o) has a 
maximum there. Thus any critical point (xo, 2/0) may be dis- 
carded if the section by the plane x = Xo has no extreme at 
that point, or if it has the opposite sort of extreme to the 
section made by y = 2/0. 



Example 1. The surface a = (y — x^) (j/ — 2 x^) has critical points 
where 

dx 



6 X2/ + 8 a;3 = 0, ^ = 2 y - 3 a;2 = 0; 



that is, the only critical point is (x = 0, 2/ =0). The tangent plane at 
that point is a = 0. This tangent plane cuts the surface where 

(y- x^) (2/ - 2 x2) = 0; 

that is, along the two parabolas 
y = x^^y — 2x^. Atx ^ 0,y = 
1, the value of 2 is + 1 ; hence s is 
positive for points (x, y) inside 
the parabola y = 2x^. Atx = 1, 
y = Oy the value of z is + 2; 
hence 2 is positive for all points 
{Xy y) outside the parabola y = 
a;2. At the point x = 1, 2/ = 1.5, 
the value of a is — .25; hence a is 
negative between the two pa- 
rabolas. It is evident, therefore, 
that a has. no extreme at x == 0, 
Fig. 83. 2^ = 0. 

A qualitative model of this extremely interesting surface can be 
made quickly by molding putty or plaster of paris in elevations in the 

* For a detailed discussion, see Goursat-Hedrick, Maihematiccd Analysis^ 
Vol. I, p. 119. 




XVIII, § 165] CURVED SURFACES 295 

unshaded regions indicated above, with a deprescion in the shaded 
portion. 

Another interesting fact is that every vertical section of this surface 
through (0, 0) has a minimum at (0, 0); this fact shows that the rule 
about vertical sections stated above cannot be reversed. Moreover, 
this surface ehides every other known elementary test except that used 
above. 

EXERCISES 

Find the equation of the tangent plane to each of the following 
surfaces at the point specified: 

1. = x2 + 9 2/2, (2, 1, 13). Ans. z = 4:X + I8y - IS. 

2. = 2x2-42/2,(3,2,2). Ans. z =- 12 x - 16 y - 2. 

3. z = xyj (2, — 3, — 6). Ans. Sx — 2y + z = Q. 

4. 2 = (x + y)2, (1, 1, 4)* . Ans. 4x + 4y — = 4. 

5. = 2 X2/2 + 2/3, (2, 0, 0) Ans. = 0. 

6-10. The straight hne perpendicular to the tangent plane at its 
point of tangency is called the normal to the surface. 

Find the normal to each of the surfaces in Exs. 1-5, at the point 
specified. 

11. At what angle does the plane x + 2y — z -{- S = cut the 
paraboloid x2 + 2/2 = 4 at the point (6, 8, 25)? 

12. Find the angle between the surfaces of Exs. 1 and 2 at the point 
(A/i3, 1, 22). 

Find the angle between each pair of surfaces in Exs. 1-5, at some one 
of their points of intersection, if they intersect. 

13. Find the tangent plane to the sphere x2 + 2/2 + 02 = 25 at the 
point (3, 4, 0); at (2, 4, VS). 

14. At what angles does the line x = 2 2/ = 3 cut the paraboloid 
2/ = x2 + ;^? 

15. Find a point at which the tangent plane to the surface 1 is 
horizontal. 

Draw the contour lines of the surface near that point and show 
whether the point is a minimum or a maximum or neither. 



296 THE CALCULUS [XVIII, § 165 

16. Proceed as in Ex. 15 for each of the surfaces of Exs. 2-5, and 
verify the following facts: 

(2.) Horizontal tangent plane at (0, 0); no extreme. 

(3.) Horizontal tangent plane at (0, 0); no extreme. 

(4.) Horizontal tangent plane at every point on the liye x + y = 0; 
weak minimum at each point. 

(5.) Horizontal tangent plane at every point where j/ = 0; no 
extreme at any point. 

Find the extremes, if any, on each of the following surfaces: 

17. 2 =: x2 + 4 2/2 - 4 a;. (Minimum at (2, 0, - 4).) 

18. a=a:3 - 3 X - 2/2. (See Tables, Fig. Ii.) 

19. = a:3 - 3 a; + 2/2 (x - 4). (See Tables, Fig. I2.) 

20. s = [(x - a)2 + 2/2] [(x + a)2 + 2/2]. (Similar to Tables, Fig. I7.) 

21. 2 =x3 — 6 a; — ^2 (Draw auxiliary curve as for Fig. Ii.) 

22. a = x' — 4 2/2 + xy^. (Draw auxiliary curve as for Fig. I2.) 

23. 2 = X* + 2/^ — 3 xy. (Draw by rotating x2/-plane through ir/4.) 

24. Redetermine the values of a and fi in Example 2, § 164, if the 
additional information (p = 23, lo = 135) is given. 

26. Find the values of u and v for which the expression 
(aiu + biv — ci)2 + (a2U + b2V — 02)2 + (asu +bzv — ci)^ 
becomes a minimum. (Compare Ex. 24.) 

26. Show that the most economical rectangular covered box is 
cubical. 

27. Show that the rectangular parallelopiped of greatest volume that 
can be inscribed in a sphere is a cube. 

[Hint. The equation of the sphere is x2 + y^ + 2^ = 1 ; one corner o f 
the parallelopiped is at (x, y, 2); then F= 8 xyz, where a = Vl — x^ — y^.] 

28. Show that the greatest rectangular parallelopiped which can be 
inscribed in an ellipsoid x2/a2 -f- 2/2/62 -j- ^/c^ == 1 has a volume V = 

Sahc/(SV3). 

29. The points (2, 4), (6, 7), (10, 9) do not lie on a straight line. 
Under the assumptions of § 164, show that the best compromise for a 
straight Une which is experimentally determined by these values is 
24 2/ = 15X + 70. 



XVIII, § 166] CURVED SURFACES 297 

30. The linear extension E (in inches) of a copper wire stretched by 
a load W (in pounds) was found by experiment (Gibson) to be {W == 10, 
E = .06), {W = 30, E = .17), {W = m, E = .32). Find values of a 
and /3 in the formula E = aW -{- fi under the assumptions of § 164. 

31. The readings of a standard gas meter S and that of a meter T 
being tested were found to be (T = 4300, S = 500), (T = 4390, S = 
600), (T = 4475, S = 700). Find the most probable values in the 
equation T = aS + fi and explain the meaning of a and of /3. 

32. The temperatures 6° C. at a depth d in feet below the surface of 
the ground in a mine were found to be d = 100 ft., 6 = 15°.7, d = 200 
ft., = 16°.5, c? = 300 ft., = 17°.4. Find an expression for the tem- 
perature at any depth. 

33. The points (10, 3.1), (3.3, l.Q), (1.25, .7) lie very nearly on a 
curve of the form a/x + ^/y = 1. Use the reciprocals of the given 
values to find the most probable values of a and /3. 

34. The sizes of boiler flues and pressures under whiqh they collapsed 
were found by Clark to he (d = 30, p = 76), {d = 40, p = 45), (d = 50, 
p = 30). These values satisfy very nearly an equation of the form 
p = jfc . (in or log p = n log d + log A;, where d is the diameter in inches, 
and p is the pressure in pounds per square inch. Using the logarithms 
of the given numbers, find the most probable values for n and log k, 

166. Tangent Planes. Implicit Fonns. If the equation of 
a surface is given in implicit form, F(Xy y, z) = 0, taking the 
total differential we find: 

But, by virtue of F (x, y, z) = 0, any one of the variables, say 
2, is a function of the other two; hence 

(2) (fe = |dx + g%. 

Putting this in the total differential above and rearranging: 



298 THE CALCULUS [XVIII, § 166 

But dx and dy are independent arbitrary increments of x and 
of y; and since the equation is to hold for all their possible 
pairs of values, the coefficients of dx and dy must vanish 
separately. This gives 

dz dF/dx dz dF/dy 






^^^ dx dF/dz ' dy dF/dz 

substituting these values in the equation of the tangent plane, 
and clearing of fractions, we obtain 

(^) S o(^ - ^^ + f ] 0^^ - ^o) + So^^ - ^) = «' 

the equation of the tangent plane at (xq, yoy zq) to the surface 
F (x, y, z)=0, 

167. Line Normal to a Surface. The direction cosines of 
the tangent plane to a surface whose equation is given in the 
explicit form z = f(x, y) are proportional (§ 163) to 

(1) ' dz/dx]o, dz/dy]^^ and — 1. 

Hence the equations of the normal at (xq, yo, Zq) are 

(<y\ x — xq ^ y — yo ^ z — zp 

^^^ dz/dx]o dz/dy]o -1 

The direction cosines of a surface whose equation is given 
in the implicit form F (x, y, 2) = are proportional to 

(3) dF/dx]o, dF/dyh, dF/dz]o, 

* 

so that the equations of the normal to this surface are 

x — xq y-yo z-zo 



(4) 



dF/dx]o dF/dy]o dF/dz]Q 



168. Parametric Forms of Equations. A surface S may 
also be represented by expressing the coordinates of any point 
on it in terms of two auxiliary variables or parameters: 
[S] x==f(u, v), y = <t>{u, v), z = \f^(u, v). 



XVIII, § 168] CURVED SURFACES 299 

If we eliminate u and v between these equations, we obtain 
the equation of the surface in the form F (x, y, z) = 0, 

Similarly a curve C may be represented by giving x, y, z in 
terms of a single auxiliary variable or parameter t: 

[C] x=f{t),y = 4>{t),z = Ht), 

The elimination of t from each of two pairs of these equations 
gives the equations of two surfaces on each of which the 
curve lies. In particular, taking t =x gives the curve as the 
intersection of the projecting cylinders: 

[P] y = <t>{x), z = yp{x). 

If, in the parametric equations of a surface, one parameter (say u) is 
kept fixed while the other varies, a space-curve is described which lies 
on the surface. Now if u varies, this curve varies as a whole and de- 
scribes the surface. The curve on which u keeps the value k is called 
the curve u = k. Similarly, keeping v fixed while u varies gives a curve 
V = k\ The intersection of a curve u = k with a curve v = k' gives 
one or more points {k, k') on the surface. The numbers A;, k' are called 
the curvilinear coordinates of points on the surface. 

Simple examples of such coordinates are the ordinary rectangular 
coordinate system and the polar coordinate system in a plane. Thus 
(2, 3) means the point at the intersection of the hnes a; = 2, y = 3 of 
the plane; in polar coordinates, (5, 30°) means the point at the intersec- 
tion of the circle r = 5 with the line 6 ■— 30°. 

Example 1. The equations of the plane x-\-y -{-z = 1 may be 
written, in the parametric form: 

x = w, y — Vy z = l — u — v. 

Let the student draw a figure from these equations by inserting ar- 
bitrary values of u and v and finding associated values of x, y^ z. An- 
other set of parameter equations which represent the same plane is 

x=u-\-v, y = u^Vf 3 = — 2w+l. 

Thus several different sets of parameter equations may represent the 
same surface. 

In the first form, put u = k. Then, as v varies, we obtain the straight 
line 

X = k, y = Vf z - l — k^Vj 



300 THE CALCULUS [XVIII, § 168 

which lies in the given plane. As k varies this Hne varies; its different 
positions map out the entire plane. Likewise, t; = A;' is a Hne varying 
with k' and describing the plane. The intersection of two of these 
lines, one from each system, is point (k, k') of the plane. 

Example 2. The sphere x^ -\- y*^ -\- z^ = c? may be represented by 
the equations: 

2=asin^cos0, y=a sin ^ sin d, z^acos^. 

Here the parameters ^ and are respectively the co-latitude and the 
longitude. Thus = A; is a parallel of latitude; d = A;' is a meridian; 
and their intersection {k, k') is a point of co-latitude k and longitude k\ 
[If a is allowed to vary, the equationi^^of this example define polar 
coordinates in space; but 90° — <f>m often used in place of <f>.] 

I 

Example 3. The equations 

x=acoatf y=a am tf z=Uy 

represent a space curve, namely a helix drawn on a cylinder of radius 
a with its axis along the 2-axis. The total rise of the curve during 
each revolution is 2 irb. 

If a is replaced by a variable parameter w, the helix varies with m, 
and describes the surface 

x^ucoat, y=su am t, 2=&^. 

which is called a helicoid. The blade of a propeller screw is a piece 
of such a surface. 

169. Tangent Planes and Normals. Parameter Fonns. 

When a surface is given by means of parametric equations, 

(1) X = / (u, v), y = <f> (w, v), 2 = ^ (w, v)y 

the equation of the tangent plane is found as follows. Elimination of u 
and V would give the equation in the implicit form F (x, y, z) = 0. If 
the parametric values of Xj j/, z are substituted in this equation, the 
resultiag equation is identically true, since it must hold for all values of 
the independent parameters w, v; hence 

that is 

^^ dx du dy du dz du ' dx dv^ dy dv dz dv 



XVIII, § 169J CURVED SURFACES 



301 



Solving these, we find: 



(4) 



dF dF dF 
dx ' dy ' dz 



dy dz 
du du 




dz dx 
du du 




dx dy 
du du 


dy dz 
dv dv 


• 


dz dx 

dv dv 


• 


dx dy 
dv dv 



hence the equation of the tangent plane is 



(x — Xq) 



du 


dz 

du 


dy 


dz 


dv 


dv 



+ (2/ - Vo) 



dz 


dx 


du 


du 


dz 
dv 


dx 
dv 



+ (2 - 3o) 



dx 

du 


9y 

du 


dx 
dv 


dy 
dv 



while the equations of the normal are 

x — xq __ y — yp _ 



z 



So 



dy dz 




dz dx 




dx dy 


du du 




du du 




du du 


dy dz 




dz dx 




dx dy 


dv dv 





dv dv 





dv dv 



-0; 



EXERCISES 

1. Determine the tangent plane and the normal to the ellipsoid 
a;2 + 4 2/2 + 2^ = 36 at the point (4, 2, 2), first by solving for s, by the 
methods of § 163; then, without solving for z, by the methods of 

166- 167. 



Determine the tangent planes and the normals to each of the fol- 
lowing surfaces, at the points specified: 

2. x^ + y^+z^ =a^ at (xq, ^o. ^o)- 

3. a;2 - 4 2/2 + 22 = 36 at (6, 1, 2). 

4. a;2 - 4 2/2 - 9 32 = 36 at (7, 1, 1). 
6. a;2+2/2-z2=0at (3,4,5). 

6. a;3 + a;22/ - 2 22 = at (1, 1, - 1). 

7. 22 = e«+v at (0, 2, c). 

8. Find the angle between the tangent planes to the eUipsoid 
4 a;2 + 9 2/2 + 36 22 = 36 at the points (2, 1, 20) and (- 1, - 1, 21). 

9. At what angle does the 2-axis cut the surface 22 =s e*-*? 



302 



THE CALCULUS 



[XVIII, § 169 



10. Obtain the equation of the tangent plane to the helicoid 

X = u cos Vj y = usin Vf 2 = v, 
at the point w = 1, v = ir/4. 

11. Talcing the equations of a sphere in terms of the latitude and 
longitude (Example 2, § 168), find the equation of its tangent plane and 
the equations of the normal at a point where 6 = 4> ^ 45°; at a point 
where ^ = 60% = 30**. 

12. EUminate u and v from the equations x = u + Vf y — u — Vy 
z — uoyijo obtain an equation in x, y, and z. Find the equation of the 
tangent plane at a point where t* = 3, t; = 2, by the methods of § 166; 
then by the methods of § 169 directly from the given equations. 

13. Write the equation of the tangent plane to the surface used in 
Ex. 7 at any point (xq, yo, zq). At what point is the tangent plane 
horizontal? Is z an extreme at that point? 

Proceed as in Ex. 7 for each of the following surfaces: 

14. X =r cos dy y = r Bin 6, z == r, a,t r = 2, 6 = ir/4. 

^. uv -{-1 u — V uv— 1 ^ _ ^ 

16. X = — j — , y = — — , z = — i — , at w = 2, » = — 1. 

u -{-V u -{-V u -\-v ' 

16. a; = -"3w + 2v, y —2u — v, s = e**+f, at (uqj Vq), 

17. X =2 cos 6 cos 0, 2/ = 3 cos 6 sin 0, a = sin ^, at ^ = = t/4. 

18. The surfaces z = x^ — 4y^ and z = Qx intersect in a curve, 
whose equations are the two given equations. Find the tangent line 
to this curve at the point (8, 2, 48) by first finding the tangent planes to 
each of the surfaces at that point; the line of intersection of these planes 
is the required line. 

19. Find the tangent line to the curve defined by the two equations 
16x2-3^2 =4 sand 9x2+32/2-;^ = 20 at (1, 2, 1). 

170. Area of a Curved Surface. Let /S be a portion of a curved 
surface and R its projection on the X2/-plane. In R take an element 
AxAy and on it erect a prism cutting an element AS out of S. At any 
point of AS, draw a tangent plane. The prism cuts from thi? an ele- 
ment A A. The smaller Ax Ay (and therefore AS) becomes, the more 
nearly will the ratio aA/aS approach unity, since we assume that the 
limit of this ratio is 1. 



XVllI, § 170] CURVED SURFACES 



303 



Suppose now that the area i2 is all divided up into elements AxAy and 
that on each a prism is erected. 
The area S will thus be divided up 
into elements AS and there will be' 
cut from the tangent plane at a 
point of each an element AA. One 
thus gets 

(1) S = Km y. AA, 




Ax— ^0' 
Ay-»0 



But if 7 is the acute angle that 
the normal to any AA makes with 
the 2-axis, we have 




Fig. 84. 



(2) 
hence 



AA = sec 7 Aa; Ay; 



(3) iS = Um y Ail = lim T* (sec y AxAy) = f faec y dx dy. 



Ax-»0 
Ay— K) 



Ar-»0 
Ay-»0 



Of course sec 7 is a variable to be expressed in terms of x and y from the 
equation of the surface. The limits of integration to be inserted are 
the same as if the area of R were to be found by means of the integral 

ffdx dy. 

If the surface doubles back on itself, so that the projecting prisms cut 
it more than once, it will usually be best to calculate each piece sep- 
arately. 

When the equation of the surface is given in the form 2 =» / (a;, y)y 
the direction cosines of the normal are given by 

dz dz ^ 

cos a : cos j8 : cos 7 = ^ : -:r : — 1. 

dx dy 



Taking cos 7 positive, that is 7 acute, we may write 



(4) 



and 



sec 7 



S)"+ (S)"+ ■■ 



» - //VlMif^"'*- 



The determination of sec 7, when the surface is given in the form 
F(Xy y, z) = 0, is performed by straightforward transformations similar 
to those used in §§ 167-169; they are left to the student. 



304 THE CALCULUS [XVIII, § 170 

EXERCISES 

1. Calculate the area of a spiiere by the preceding method. 

2. A square hole is cut centrally through a sphere. How much of 
the spherical surface is removed? 

3. A cylinder intersects a sphere so that an element of the cylinder 
coincides with a diameter of the sphere. If the diameter of the cylinder 
equals the radius of the sphere, what part of the spherical surface hes 
within the cyHnder? 

4. How much of the surface s =xy lies within the cylinder 
a;2 + 2/2 = 1? 

6. How much of the conical surface ^ = a;^ + y^ lies above a 
square in the a^-plane. whose center is the origin? 

6. Show that if the region 22 of § 170 be referred to ordinary polar 
coordinates, AA = r sec 7 Ar A6, approximately. (See § 92, p. 149.) 

7. Using the result of Ex. 6, show that S —ffr sec 7 dr dd. 

8. Show that, for a surface of revolution formed by revolving a 
curve whose equation is s = / (x) about the z-axis, 

sec 7 = Vl 4- [rf/(r)/dr]2, where r = Vx^ + y^. 

9. By means of Exs. 7, 8, show that the area of the surface of revo- 
lution mentioned in Ex. 8 is 

-XT' nR¥J— J:'^FOT*. 

where a is the value of r at the end of the arc of the generating curve. 

10. Compute the area of a sphere by the method of Ex. 9. 

11. Find the area of the portion of the paraboloid of revolution 
formed by revolving the curve z^ = 2 mx about the x axis, from x = 
to a; = A;. 

12. Show that the area of the surface of an ellipsoid of revolution 
is 2 7r6 [6 + (<»A) sin~ie], where a and h are the semiaxes and e the 
eccentricity, of the generating ellipse. 

13. Show that the area generated by revolving one arch of a cycloid 
about its base is 64 -n-a^/S. 

14. Show that the area of the surface generated by revolving the 
curve ^2/3 -|- 2/2/3 = a^/z about one of the axes is 12 iral^/5. 



XVIII, § 172] CURVED SURFACES 



305 



171. Tangent to a Space Curve. Let the equation of the curve 
be given in parametric form a; == / (0, 2/. = (0, 2 = \A (0- Let Pq = (xq, 
2/0, 2^) be the point on the curve where t = ^. Let Q be a neighboring 
point on the curve where t = to ■{• At 

The direction cosines of the secant PqQ are proportional to Ax/At, 
Ay /At, As/At; hence its equations are 



(1) 



x 



xo _ y — yo ^ g— 2o 



Ax/At Ay I At Az/At 
As Ai -^ 0, these become 



20 



^ ^ dx/dt]Q dy/dt]Q dz/dth' 

the equations^f the tangent at 
the point Pq. 

If the curve is given as the 
intersection of two projecting 
cylinders y = fix), z = <l>(x), 
we may join to these the third 





Fia. 



equation x = x, thus conceiving of x, y, and 3 as all expressed in terms 
of x. The equations of the tangent then become 

x — xo _ y — yo _ z— zq 
1 



(3) 



dy/dx]o dz/dxlo 

If the curve is given as the intersection of two surfaces, / (x, y, z) = 0, 

F (x, y, z) =fi, and if we think of x, y, zaa depending upon a parameter 

t, we find 

^ ^^^,^dy ^dz ^ 

dt dxdt '^ dydt '^ dzdt * 



and 



dF ^ d£^,dF^dydF^dz^^ 
dt dx dt'^ dy dt'^ dz dt 



From these .equations we obtain dx/dt : dy/dt : dz/dt, and we may write 
the equations of the tangent at Pq in the form: 



X— Xo 



2/ -2/0 



z— Zo 



df df 
dy dz 




df df 

dz dx 




dx dy 


dFdF 
dy dz 





dFdF 

dz dx 





dF dF 
dx dy 



172. Length of a Space Curve. The length of the chord joining 
two points t and t +A< of the curve 

(1) a;=/(O,2/ = 0(O,s = ^(O, 



306 THE CALCULUS [XVIII, § 172 

is Ac = VAX* + Aj/* + Aar*, or^ 

r9^ A^ |ax2 , Aj/a , As*., 

(2) ^ = \a?+A^+Z?^'- 

Defining the length of a curve between two points as the limit of the 

sum of the inscribed chords, we find for that length: 

EXERCISES 

1. At what angle does a straight line joining the earth's South pole 
with a point in 40® North latitude cut the 40th parallel? 

2. At what angle does the helix x = 2 cos ^, 2/ = 2 siu ^, a = 0, cut 
the sphere a;^ + y^ _j- g2 — 9? 

3. Find the angle of intersection of the ellipse and parabola that are 
cut from the cone s^ = x^ +y^hy the planes 2z = 1 — x and a = 1 -f a; 
respectively. 

4. Show that the curves of intersection of the three surfaces 

2 = 2/, a;2 = 2/2 4. 22^ a;2 + 2/2 _j. 32 = 1^ 

cut each other mutually at right angles. 

6. Show the same for the curves of intersection of the surfaces 
4x2 + 9^2 +3632 = 36, 3a;2 + 62/2 - 6^2 = 6, 10x2 - 15y^ - 6^2 =30. 

6. Calculate the length of the curve x = tyy = fi, z = 2 ^/2, from 
^ = to < = 1. 

7. Find the length of the helix x = a cos ^, 2^ = a sin ^, a = bd, from 
5 = ^0 to ^ = ^1. What is the length of one turn? 

8. Find the length of the curve a; = sin s, y = cos a, from (1, 0, t/2) 
to (0, - 1, ir). 

GENERAL REVIEW EXERCISES 

[The exercises marked with an asterisk are of more than usual 
difficulty. Some of them contain new concepts of value for which 
it is hoped that time may be found. 'Hiose of the greatest theoretical 
value are marked f. 

Attention is called to the reviews of doul^le and 'riple integration.] 

1. Given u =^ xy, x = r cos 6, y = r ain dj find du/dr and du/dS, 
first by actually expressing u in terms of r and 6; then directly from the 
given equations. 



Xyill, § 172] CURVED SURFACES 307 

2. Proceed as in Ex. 1 for the function u — tan~^ (y/x). 

3. Given u = t^^^, x = r cos d, y — r sin dy find du/dz and du/dy 
first by expressing u in terms of x and y; then directly from the given 
equations. 

[Hint. In the second part, it is convenient here to solve the last 
two equations for r and 6 in terms of x and y. But see Ex. 4.] 

4.* lix = r cos 6 and y = r sin 0, show by differentiation that 

- = l = -cos9-r8ine-, and - =0 = -sm » + r cos 9 -■ 

Solve these equations for &r/dx and dO/dx, and show that du/dx may be 
found in Ex. 3 by means of the equation 

dx^^ dx de dx' 

6.* If, in general, tt is a function of the two variables (r, ^), show 
that the last equation in Ex. 4 hold^ true. Find a similar equation for 
du/dy, and evaluate du/dy in Ex. 3 by means of it. 

6.*t If w is a function of any two variables p and q, and if p and q 
are given in terms of x and y by two equations x — f(p, q)jy = 4>{Pj q), 
obtain du/dx and du/dy by a process analogous to that of Exs. 4, 5. 

Proceed as in Ex. 3, by the methods of Exs. 4, 5, in each of the fol- 
lowing cases: 

7. w = r^ __ cQg2 g 8. w = refi*. 9. u — d log r. 

10. Find the volume of that portion of a sphere of radius 4 ft. which 
is bounded by two parallel planes at distances 2 ft. and 3 ft., respectively, 
from the center, on the same side of the center. 

11. Determine the position of the center of mass of the solid de- 
scribed in Ex. 10. 

12. What is the nature of the field of integration in the integral 

/ fix,y)dydx7 

•^ X 

Show that the same integral may be written in the form 



I f(x,y)dydx + 1 I f {x, y) dx dy, 

"^ -^ a/V2 *^ 

13. Find the volume cut from the sphere x^ + ^ + a^ = a^ by the 
cylinder a^ -\']^ — ax =0. 



308 THE CALCULUS [XVIII, § 172 

14. Find the volume cut from the sphere a;^ + i/S -f s* = a^ by the 
cone (x — a)2 + 2/2 — a^ — Q^ 

16. Show that the surface of a zone of a sphere depends only upon 
the radius of the sphere and the height 6 — a of the zone, where the 
bounding planes are z = a and z =b. 

16. Find the area of that part of the surface kH = xy within the 
cylinder a^ + 2/* = A;*. 

17. Find the center of gravity of the portion of the surface described 
in Ex. 16, when A; = 1. 

18. Find the moment of inertia about its edge, of a wedge whose 
cross section, perpendicular to the edge, is a sector of a circle of radius 

1 and angle 30*^, if the length of the edge is 1, and the density is 1. 

19. The thrust due to water flowing against an element of a surface 
is proportional to the area of the element and to the square of the com- 
ponent of the speed perpendicular to the element. Show that the 
total thrust on a cone whose axis lies in the direction of the flow is 
A;7rrV/(r2 + A2)i. 

20. Calculate the total thrust due to water flowing against a seg- 
ment of a paraboloid of revolution whose axis lies in the direction of 
the flow. (See Ex. 19.) 

21. Show that the thrust due to water flowing against a sphere is 

2 kin^i^/S. Compare with the thrust due to the flow normally against 
a diametral plane of this sphere. 

22. Find the critical points, if any exist, for the surface z = x^ +2y2 
— 4 rr — 4 y + 10. Is the value of z an extreme at that point? Draw 
the contour lines near the point. 

23. Determine the greatest rectangular parallelopiped which can be 
inscribed in a sphere of radius a. 

24. The volume of CO2 dissolved in a given amount of water at tem- 
perature ^ is ( ^ 5 10 15, 

(v 1.80 1.45 1.18 1.00. 

Determine the most probable relation of the form v = a -{-bO. 



26. Determine the most probable relation of the form S = a +hF^ 
from the data: \P 550 650 750 850, 

S 26 35 52 70. 



I 



1 



I 



XVIII, § 172] CURVED SURFACES 309 

26. Determine the most probable relation of the form y = (m^ from 
the data: \x 1 2 3 4, 

\y .74 .27 .16 .04. 

27. The barometric pressure P (inches) at height H (thousands feet) 

P 30 28 26 24 22 20 18 16, 
H 1.8 3.8 5.9 8.1 10.5 13.2 16.0. 

Determine the most probable values of the constants in each of the 
assumed relations: (a) ^ = a + 6P; (b) H = a-hbP+cP^; (c) H = 
a + 6 log P or P = Ae^^. Which is the best approximation? 

28. t If the observed values of one quantity yaxe mi, rM2, m3, corre- 
sponding to values h, h, fe of a quantity x on which y depends, and if 
2/ = ox + 6, show that the sum 

S = {ah + 6 - mi)2 + (ofe + 6 ~ mz)^ _|- (afe _|- 6 - ;^)2 

is least when 

h {all -{-b — mi) + fc (0/2 + 6 — W2) + 13 {ah + 6 — ma) = 0, 
{all + 6 — mi) + {al2 -f & — ^2) + (a/3 +b — ms) = 0; 
that is, when 

a ' J^h^ -^b ' J^h - J^mih =Oanda. J^h -{- S b -J^mi =0, 
or 

Sj^mih — J^i'^^ 'Jj^ J^h^' ^wi — ^mi^i • J^h 

where ^ indicates the sum of such terms as that which follows it. 

[Theory of Least Squares.] 

29. Show that the equation of the tangent plane to 2 s = x^ -\- y^ &t 
{xoj yo)mz-\'3o ^xxo-\- yyo. 

30. Determine the tangent plane and normal line to the hyperboloid 
a;2 _ 4 2^ + 9 ;^ == 36 at the point (2, 1, 2). 

31. Study the surface xyz = 1. Show that the volume included be- 
tween any tangent plane and the coordinate planes is constant. 

32. Study the surface 2 = {x^ -\- y^) {x^ -]- y^ — 1). Determine the 
extremes. 

33. At what angle does a Une through the origin and equally in- 
clined to the positive axes cut the surface 2 s = x^ + y^? 



310 THE CALCULUS [XVIII, § 172 

34. Determine the tangent line and the nonnal plane at the point 
(1, 3/8, 5/8) on the curve of intersection of the surfaces x + y + a = 2 
and r^ + 4 ^ - 4 22 = 0. 

35. Detennine the tangent line and the normal plane to the curve 
X — 2 cos ty y —28inty z = fi a,t t == ir/2 and at < = ir. 

36. Find the length of one turn of the conical spiral x ^^ t cos (a log 0, 

y = / sin (a log t), z — htj starting from t = t. 

37. Determine the length of the curve x — a cos $ cos ^ y = a cos 
$ am <t>t ^ ~ <i sin 0, from = ^i to ^ = ^, where 6 is given in terms 
of 4> by the equation 5 = A; log ctn (x/4 — <f>/2). (Loxodrome on the 
sphere.) 

38,*t Show that the surfaces /(a;, y, z) = and ^ (x, y, z) =0 cut 
each other at right angles '^ fx<f*x •\- fy<l>y + f»4>s ==0. 

39.* Show that the surfaces 

xV(«2+X)+2/V(^+X)+22/(c2+X) = 1, a>6>c>0, 

are always (t) ellipsoids if X > — c^, (ii) hyperboloids of one sheet if 
— 6^ < X < — c2, (m) hyperboloids of two sheets if — a^ < X < — 6^. 

(CONFOCAL QUADRICS.) 

Show also thaji these surfaces cut each other mutually at right angles. 
If X = r cos 6 cos 4>, y — r cos 9 sin ^, z = r sin B (polar coordinates), 
find du/dfy du/ddy and du/d<t> for each of the following functions: 

40. w = x2 + 2/2 + z^, 41. w = x2 + y2 _ 22. 42. u = ae»+». 

43. Compute du/dXy du/dyy and dw/dz if w = r? (sin^ e + sin^ ^), 
where r, d, are defined as in Exs. 40-42. 

44.t Show that the centroid (x, y) of a plane area in polar coordinates 
(p, e) is 

J J p2 COS e dp de J J p2 sin ^ dp dS 

X = , y = , 

jjp dp de J J p dp de 

where the integrals are extended over the given area. 



CHAPTER XIX 
DIFFERENTIAL EQUATIONS 

PART I. ORDINARY PIFFERENTIAL EQUATIONS OF 

THE FIRST ORDER 

173. Definitions. An equation involving derivatives or 
differentials is called a differential equation. An ordinary 
differential equation is one involving only total derivatives. 
A partial differential equation is one involving partial 
derivatives. 

The order of a differential equation is the order of the 
highest derivative present in it. 

The degree of a differential equation is the exponent of 
the highest power of the highest derivative, the equation 
having been made rational and integral in the derivatives 
which occur in it. 



Examples. 






(« g-« 




(First order, first degree.) 


<« l+S-*- 




(Second order, first degree.) 


<» [' + ©7 ■ 


-»(S)' 


(Second order, second degree.) 


'« S+S-' 




(Second order, first degree.) 



Such equations constantly arise in the applications of 

mathematics to the physical sciences. Many simple examples 

have already been treated in the text. 

311 



312 THE CALCULUS pOX, § 174 

174 Elimination of Constants. Differential equations also 
arise in the elimination of arbitrary constants from an 
equation. 

Example 1. Thus, if A and B are arbitrary constants, then equation 
y = Ax + B represents a straight line in the plane, and by a proper 
choice of A and B represents any line one pleases in the plane except a 
vertical line. One differentiation gives m = dy/dx = A, which repre- 
sents all hues of slope A. A second differentiation gives 

(1) flexion = 6 = d^y/dx^ = 0, 

which represents all non-vertical lines in the plane, since all these and 
on other curves have a flexion identically zero. 

Example 2. Any circle whose radius is a given constant r is repre- 
sented by the equation 

(2) {X - A)2 + (2/ - B)2 = r2, 

from which A and B may be eliminated as in the preceding example. 
Differentiating once, 

(3) x-A + iy- B)y' = 0, 
where y' = dy/dx. Differentiating again, 

(4) 1 + 2/'2 + (2/ - B)y'' = 0, 

where y" = d!^y/dx^. Solving (3) and (4) for a; — A and y-rB and sub- 
stituting these values into (2), so as to eliminate A and B, we find 

(5) (1 + 2/'2)3 = r22/"2. 

This sayB that every one of these circles, regardless of the position of its 
center, has the curvature 1/r, — a statement which absolutely charac- 
terizes these circles. 

In general, if 

(6) Six, y, cu C2, • • • , c„) = 

is an equation involving x, y, and n independent arbitrary 
constants Ci, C2, • • •, c^, n differentiations in succession with 
regard to x give 

these equations, together with (6), form a system of w + 1 



XIX, § 175] DIFFERENTIAL EQUATIONS 



313 



equations from which the constants Ci, C2, • • • , c» may be 
eliminated. The result is a differential equation of the nth 
order free from arbitrary, constants, and of the form 
(8) 0(^,2/,2/',y", •••,2/^"^)=.0. 

Equation (6) is called the primitive or the general solution 
of (8). The term general solution is used because it can be 
shown that all possible solutions of an ordinary differential 
equation of the nth order can be produced from any solution 
that involves n independent arbitrary constants, with the ex- 
ception of certain so-called '* singular solutions" not derivable 
from the one general solution (6). 

Thus, to solve an ordinary differential equation of the nth 
order is understood to mean to find a relation between the 
variables and n arbitrary constants. These latter are called 
the constants of integration. 

If, in the general solution, particular values are assigned to 
the constants of integration, a particular solution of the dif- 
ferential equation is obtained. 

175. Integral Curves. An ordinary differential equation 
of the first order, 

(1) <t>(x> y> y') = 0, or I/' = / (x, 2/), 
where y' = dy/dx, has a general 
solution involving one arbitrary 
constant c: 

(2) F{x,y,c) = Q, 
This represents a singly infinite 
set or family of curves, there being 
in general one curve for each value 
of c. Any curve of the family can 
be singled out by assigning to the 
proper value. Fig. 86. 




314 THE CALCULUS [XIX, § 175 

The differential equation determines these curves by- 
assigning, for each pair of values of x and y, that is, at each 
point of the plane, a value of the slope y' [ = /(^, 2/)] of the 
particular curve going through that point. Thus the curves 
are outlined by the directions of their tangents in much the 
way that iron filings sprinkled over a glass plate arrange 
themselves in what seem to the* eye to be curves when a 
magnet is placed beneath the glass. Straws on water in 
motion create the same optical illusion. 

A differential equation of the second order: 

<t>(x, y, y\ 2/") =0, or y" = /(x, y, y'), 

has a general solution involving two arbitrary constants, 

F(x, y, ci, cz) = 0. 

This represents a doubly infinite or two-parameter family of 
curves; for each cqnstant, independently of the other, can 
have any value whatever. The extension of these concepts 
to equations of higher order is obvious. 

The curves which constitute the solutions are called the 
integral curves of the differential equation. 

EXERCISES 

Find the differential equations whose general solutions are the follow- 
ing, the c's denoting arbitrary constants: 

1. a;2 + y2 = q2 jIyis, X -i-yy' =0. 

2. a;2 — 1/2 = ex. Ans, x^ +'y^ = 2 xyy\ 

3. y — C&' —i (sin a; + cos x). Ans, y' = y -\-8mx, 

4. y = ex -\-€^, Ans. y = y'x + y^. 
6. y = cx+f(c). Ans. y = y'x-\-f(y'), 

6. y - Cie^' + 026^. Ans. i/" — 5 2/' + 6 y = 0. 

7. y = cie«* + Ci^ Ans. y" -- (a + h)y'+ aby = 0. 

8. xy = o-{- (^x. ' Ans. x^y^ = y'x + y. 

9' y = (ci+ x)€^ + c^. Ans. I/" - 4 1/' + 3 1/ = 2 e3*. 



XIX, § 175] DIFFERENTIAL EQUATIONS 315 

10. 2/ = cie* + o^ + C3e3*. Am, y'" — 6 2/" + 11 2/' — 6 y = 0. 

11. r ^ c sin Q, An&. r cos = r' sin d, 

12. r = e^. Ans. r log r = r'd. 

13. Assuming the differential equation found in Ex. 1, indicate the 
values of y\— — x/y) at a large number of points (x, y) by short 
straight-line segments through each point in the correct direction. 
Continue doing this at points distributed over the plane until a set of 
curves is outlined. Are these curves given in Ex. 1? 

14. Proceed as in Ex. 13 for the equation y' — yfx. Do you recog- 
nize the set of curves? Can you jirove that your guess is correct? 

16. Draw a figure to illustrate the meaning of y' == x^. Find y. 
Generalize the problem to the case y' = }{x). 

16. Find that curve of the set given in Ex. 1 which passes through 
(1,2). Find its slope (value of y') at that point. Do these three values 
of (x, y^ y') satisfy the differential equation given as the answer in No. 1? 

17. Proceed as in Ex. 16 for the equation of Ex. 2. 

18. Proceed as in Ex. 16 for the first equation of Ex. 15. 

19. Find the differential equation of all circles having their centers 
at the origin. 

20. Find the differential equation of all parabolas with given latus 
rectum and axes coincident with the a;-axis. 

21. Find the differential equation of all parabolas with axes falling 
in the x-axis. 

22. Find the differential equation of a system of confocal ellipses. 

23. Find the differential equation of a system of confocal hyperbolas. 

24. Find the differential equation of the curves in which the sub- 
tangent equals the abscissa of the point of contact of the tangent. 

26. A point is moving at each instant in a direction whose slope 
equals the abscissa of the point. Find the differential equation of all 
the possible paths. 

26. Write the differential equation of linear motion with constant 
acceleration; of Unear motion whose acceleration varies as the square of 
the displacement. The same for angular motion of rotation. 

27. A bullet is fired from a gun. Write the differential equations 
which govern its motion, air resistance being neglected. How must 
these equations be modified, if air resistance is assumed proportional to 
velocity? 



316 THE CALCULUS [XIX, § 176 

176. General Statement We shall now consider methods for 
solving dififerential equations. Since the most common proper- 
ties of curves involve slope and curvature, and since in the 
theory of motion we deal constantly with speed and ac- 
celeration, the differential equations of the first and second 
orders are of prime importance. 

Ordinary differential equations of the first order and first 
degree have the form 

(1) M + N^ = 0,oTMdx + Ndy = 0, 

where M and N are functions of x and y. 

No general method is known for solving all such differential 
equations in terms of elementary functions. We proceed to 
give some standard methods of solution in special cases. 

177. Type I. Separation of Variables. It may happen that 
M involves x only, and N involves y only. The variables are 
then said to be separated and the primitive is f oimd by direct 
integration: 

CMdx+fNdy^C, 
C being an arbitrary constant. 

Example 1. A particle is falling through air such that the resistance 
is proportional to the speed. If the particle starts from rest, what is 
its speed at any time? 

Since acceleration is dv/dt, and since this is equal to g diminished by 
a term proportional to v, we have 

dv 

Separating variables: 

g — av 
Integrating: 

a 

or fif — av = e-a(«+*). 



Separating: ^ j^ dy + -g— rr dx ^0. 



XIX, § 178] DIFFERENTIAL EQUATIONS 317 

Since the particle starts from rest we have v *« when t = 0, Sub- 
stituting these values in the last equation we have g = e~**; 
hence g — av = e-<«-at = ge~^t, 

or V = (g/a){l — e-^). 

Example 2. Given (x^ + I) (y + 1) dy +xy^dx = 0. Determine 
the relation between x and y. 

Integrating: \o%y — l/y + log Vx^ + 1 = A;. 
Let ^ = — log Cf rearrange and combine terms; the result Is 

log(cyVa;2 + l) = l/y 
or cyVs^~+l =eV». 

178. Typell. Homogeneous Equations. When M and N 
are homogeneous * in a: and y and of the same degree, the 
equation is said to be homogeneous. If we write the equation 
in the form 

dy _ _M^ 

and make the substitution 

dy , xdv 

we obtain a new equation in which the variables can be 
separated. 

Example 1. 

(1) {xy -\-y^)dx + {xy — x^) dy = 0, 

or 

(2) dy ^ xy-\-y^ 

dx x^ — xy 

Substituting as above : 

* Polynomials are homogeneous in x and y when each term is of the 
same degree. In general, / (x, y) is homogeneous if / (Ax, ky) = k^fix^ y) for 
some one value of n and for all values of k. 



318 THE CALCULUS [XLX, § 178 

(3). t; + x^=^^3^-j-^, 

dv 2v^ 



or aJ^- = 



dx 1-v' 
separating variables, ^ dt; = — 

Integrating: — 2I; "" 2 ^^^ ""^ ^^^ ^ "^ ^* 

Replacing t; by y/x, 

or logxy = 2 c; 

henoe 

(4) xy = e-*/»-2«, 
or xy = ke-'^y, 
where A; = e-^. 

Check: Differentiating both sides of (4) with respect to x, we find 

(5) ydx+xdy^ke^/y^- ^^'^'"'^^ ']^, 

dividing the two sides of (5) by the corresponding sides of (4) respectively 

x.,N r J 1 J 1 ydx — xdy 

(6) \ydx-{-xdy\-^xy^ -^ -^ ^; 

show that (6) agrees with (1). 

EXERCISES 

Solve the following exercises by separating the variables: 

1. x dy -{- y dx =^ 0. Ans. xy = c, 

2. xVm^dx - yVT+x^dy = 0. Ans. Vl+x^ = VT+¥+ c. 

3. sin ^ c?r + r cos d dd — 0. Ans. r sin ^ = c. 

4. xVl +ydx= yVl -\-x dy. 

Solve the following homogeneous equations 
6. (x-\-y)dx + {X'-' y) dy =0. Ans. x^ +2xy — f^ = c. 

6. (x2 + 2/2) cte = 2 xy dy. Ans. x^ — y^=cx. 

7. (3 x2 - 2/2) dy = 2 xy dx. Ans. x^ — y^^cifi. 

8. (x2 -\-2xy — 2/2) ctx = (x^ — 2xy — y^) dy. 

Arw. a;2 + 2/2 = c(x + y). 



XIX, § 178] DIFFERENTIAL EQUATIONS 319 

The following Exs. 9- 18 axe intended partially for practice in recog- 
nizing types: 

9. Vl — y2 dx + Vl — x^ dy = 0. Ans. sin-i x + sin"! y = c. 



10. 3fidx-\- (3 x^y + 2 y^) dy = 0. ilrw. x^-\-2y^ ^ cVx^ + y^. 

11. dy + ysmxdx = sin x cte. 12. r d^ = tan d dr. 

13. (2/ — 1) cte = (a; + 1) dt/. 14. ydx + ix — y) dy = 0. 

16. x{l +u^)dx = y(l +a;2) dy. 16. (9 x^+y^)dx=2 xy dy, 

17, ^ -^ X = c. 18. -^ 4- 2^ = x. 
dx dx 

19. In Ex. 1 above, draw a figure to represent the direction of the 
integral curves at various points. Hence solve the equation geomet- 
rically. 

20. A point moves so that the angle between the a;-axis and the di- 
rection of the motion is always double the vectorial angle. Determine 

the possible paths. . xy , ^ n 

^ ^ Am, 0,9 -cx;c>0. 

21. Proceed as in Ex. 20 for a point moving so that its radius vector 
always makes equal angles with the direction of the motion and the 
X-axis. Ans, r = c sin d. 

22. The speed of a moving point varies jointly as the displacement 
and the sine of the time. Determine the displacement in terms of the 
time. Ans, asce*"*®®"'. 

23. Find the value of y if its logarithmic derivative with respect to 
a; is a;2. 

24. Determine the curve whose subnormal is constant and which 
passes through the point (2, 5). 

26. Determine the curve whose subtangent at any point {x, y) is 
(1 + x)y and which passes through (0, 3). 

26. Determine the curve passing through (5, 4) such that the length 
of the normal at any point (§ 30) equals the distance of the point from 
the origin. 



320 THE CALCULUS [XIX, § 178 

27. When a wheel is driven by a belt the tension at P and the angle 

are connected by the equation dT/d$ = kT, 



B ^^ 


^2 


k being a known constant. 
If Ti = 200 lb.. 


*-.. \ 


> 


V k = 0.1, 




y 


1 and ACB = 60°, 
/ what is T2? 

If Ti = 500 lb., 
Ti = 550 lb.. 


^1 

Fig. 87. 




and ACB = 90°, 
what is A;? 



28. In a chemical reaction A is the quantity of active matter originally 
present, q the quantity of product at time t; these are related through 
the equation dq/dt = k (A — q). 

Express g as a function of it. 

29. In a bimolecular chemical reaction the original amounts of ac- 
tive substances are A and B; the product q formed in time i is to be 
determined from the equation 

dq/dt ^k{A-'q)(B-' q). 
Express q in terms of t. Consider the special case A =^ B 

30. The differential equation of the adiabatic expansion of a gas 
\a kp dv -\- V dp ^ Q. Show that p = cv^. Find c if A; = .001, and 

V = 100 when p = 10. 

31. The rectilinear motion of a particle under the action of a central 
force which varies as the inverse square of the distance from a fixed 
point is V dv/dt = A;^/^, where v is the speed and t the time. Express 

V in terms of t 

32. Solve Helmholtz's equation for the strength of an electric cur- 
rent, C =E/R- {L/R) idC/dt)y E, L and R being constants. If 
C = when t = 0, show that C = (E/R) (1 - 6-«/^). 

179. Type in. Linear Equations. This name is applied 
to equations of the form 

(1) l+^^=«' 



XIX, § 179] DIFFERENTIAL EQUATIONS 321 

where P and Q do not involve y, but may contain x. Its solu- 
tion can be obtained by first finding a particular solution of 
the reduced equation, 

(10 1 + ^^ = 0' 

where ^ is a new quantity introduced for convenience in what 
follows; and where Q is replaced by zero. In (1') the vari- 
ables can be- separated (see § 179), and we get 

as a particular solution, the constant C of integration being 
given the particular value 0. 
If we make the substitution 

(2) 'y = V'y, 

where t; is a function of x to be determined, the equation (1) 
becomes 

The first term vanishes by (1') leaving 



Hence 



y^ = Q, or dv = ^dx = [Qe^^'^dx. 



and 

(3) y = vy = e'^''^ \f[Qe^''^ dx + c j • 

This equation expresses the solution of any linear equation. 
It should not be used as a formula; rather, the substitution 
(2) should be made in each example. 



322 THE CALCULUS [XIX, § 179 

' Example. Given 
(1) ^ + 3x^y=3fi, 

the reduced equation in the new letter y == y/v is 

(10 ^ "*■ ^ ^^^ "" ^' whence y = er^. 

Hence the substitution y = v -y becomes 



^==«-x»^- 

and (1) takes the form 



(2) y = V e-*', whence -^ = ^~*';^ "" ^ vx^e^f 



[ 



e-^'^ - 3 wrSe-^l + 3 x^ [w^T = afi. 



This reduces, as we foresaw in general above, to the form 

.dv , dv - , 

e-*' 3- = a;6, or -r- = a:^ e«' 

aa; ax 

whence v =^J*x^^'dx + c = J [^^ ^' ~ e*'] + c, 

or, returning by (2) to y: 

(3) 2/ = ve^' = i [aj3 - 1] + ce^'. 
Check. DiflPerentiating both sides, 

(4) ^--x^-3x^ce-^; 
ehminating c by multiplying (3) by 3 x^ and adding to (4), 

The result (3) may also be obtained by direct substitution from (1). 
Sufficient practice in the direct solution, as in the preceding example, 
is strongly advised. 

180. Equations Reducible to Linear Equations. Certain 
forms of equations may be reduced to linear equations by a 
proper change of variable. No general rule can be given, 
and the proper substitution is usually to be formed by 

trial. 

dv 
Example. sec^ 2/ ;£ + 3 a^ tan y =3fi. 

Letting tan y = z, we have 

dx 
which is linear in z and has the same form as the example solved in 
§ 179. 



XIX, § 180] DIFFERENTIAL EQUATIONS 323 

The equation 

^ + Py = Qy^y (n a constant.) 

called the. extended linear equation is always reducible to 
the linear type by putting y^~^ = z. 

Example. Given 

Thus -(1/2)2/3^+1=0:2/3 

and ^-2^^-2x. 

ax X 

Here P = - ?, fpdx = - 2 log x, eJ^^^ = x-^; 

so that z = 3^ If dx-)rc\ = — 2 a;2 log a; + cx^ = y-2, 

and finally x^y^ (c — 2 log x) = 1. Check this result. 



EXERCISES 
Solve the following equations and check each answer. 

1. ^ "■ ^ ~ ^/^- ^' 5^ + y cos a; « sin 2 a;. 

2. ^+3x22/=3»5. 4. x^£+y^\ogx. 



6. 


I+I-^- 




7. 


S-2r. = r2^. 


6. 


g+. = x^. 




8. 


.2/^2-^=^- 


9. 


C082x|+y = 


tans. 


10. 


r^^ = (l+r2)sm^. 


11. 






12. 


In-.-.-. 



13. dy — ydx^mix dx. 14. sec ^ dr + (r — 1) dd = 0. 



324 THE CALCULUS [XIX, § 180 

16. (a;2 -\-l) dy ^ (xy -\-k) dx, 16. xdy -\-ydx = xy^ log x dx. 

17. The equation of a variable electric current is 

where L and R are constants of the circuit, i is the current, and e the 
electromotive force of the circuit. Calculate i in terms of /, 1**, if e is 
constant; 2°, if e = eo sin (at. 

Ans. 2** i = ,- ^Q sin (ut - 0) + ce-»</^, = arc tan (« L/i?). 

181. Other Methods. Non-linear Equations. A variety of 
other methods are given in treatises on Differential Equa- 
tions; some of these are indicated among the exercises which 
follow; Noteworthy among these are the possibility of 
making advantageous substitutions; and — what amounts 
to a special type of substitution — the possibility of writing 
the given equation in the fofrm of a total differential, dz = 0, 
where 2 is a known function of x and y which leads to the 
general solution z = constant (see Exs. 5-12, below). 

Equations not linear in y' may often be solved. If the 
given equation can be solved for y\ several values of t/' may 
be found, each of which constitutes a differential equation: 
the general solution of the given equation means the totality 
of all of the solutions of all of these new equations. 

EXERCISES 

Solve the following equations, using the indicated substitutions: 

1. y^dy + (y^+x)dx = 0, (Put v = 2/3.) 

2. 8dt — td8='2s(t'-s)dt. (Put s = tv.) 

3. xdy — ydx = (x^ — y^) dy. (Put y — vx,) 

4. u^v^ iudv -{-V du) = (v -i-iP) dv. (Put w = x, v = y,) 

6. Solve the equation (3 x^ + y) dx -\- (x -\- 3 y^) dy = 0. 

[Hint. If we put z = x^ -\- xy -\- y^, this equation reduces to cfo = 0; 
for dz = (dz/dx) dx + (dz/dy) dy. But dz = gives z = const., hence 



/ 



XIX, § 181] DIFFERENTIAL EQUATIONS 325 

35^ + a?t/ + 2/3 = c is the general solution. Such an equation as that 
given in this example is called an exact differential equation,] 

6. Solve the equation xdy — ydx =0. 

[Hint. This equation can be solved by previous methods; but it is 
easier to divide both sides by x^ and notice that the resulting equation 
is d (y/x) = 0; hence the general solution is y/x == c. A factor which 
renders an equation exact (l/x^ in this example) is called an integrating 
factor.] 

m 

7. Solve the equation {x^ + 2 xj^) dx-+ (2 a^ y -h 2/2) ^^ = q. 
lHint. Put z = x3/3 + a;22/2 + 2/3/3.] ' 

8. Solve the equation {s -\-t sin s) ds + (< — cos «) dt = 0. 

[Hint. Arrange: s cfo + [< sin s cfe — cos a dt] -{-t dt = 0) integrate 
this, knowing that the bracketed term is — d (/ cos s).] 

9. Solve the equation xdy—{y — x)dx = (), 

[Hint. Arrange: [xdy — y dx] -\- x dx =0; divide by x^t and com- 
pare Ex. 6.] 

10. Show that [/ (x) + 2 xy^ dx -\-[2 x^y + 4^ iy)] dy = can always 
be solved by analogy to Ex. 7. 

11. Show that [/ (x) -\- y] dx — X dy can always be solved by analogy 
to Ex. 9. Solve (x^ +y) dx — xdy = 0. Ans, x — y/x — c, 

12. Solve the equation (r — tan 6) dd + (r sec ^ + tan d) dr = 0. 

[Hint. Multiply both sides by the integrating factor cos d; — sin 6 
dd -i- r dr + d (r sin 6) =0; integrate term by term.] 

13. When a family of curves crosses those of another family every- 
where at right angles, the curves of either family are called the orthog- 
onal trajectories of those of the other family. 

Find the orthogonal trajectories of the family of circles 

a;2 _j_ 2^2 = j&^ 

[Hint. If the differential equation of the first family be dy/dx = 
/ (^> y)t then the differential equation of the orthogonal trajectories is 
dx/dy = — /(x, y), for any point of intersection (x, y) the slope of the 
curve of one system is the negative reciprocal of the slope of the curve 
of the other. 

In this example the differential equation of the given family is x dx + 
ydy^O. It is evident that the differential equation of the orthogonal 



326 THE CALCULUS pOX, § 181 

family is obtained by replacing dy and dxhy — dx and dy, respectively; 
hence the desired equation is xdy — ydx = 0, whence the curves are 
y '^cx, i.e. the family of all straight Unes through the origin.] 

14. Find the orthogonal trajectories of the exponential curves. 

y = e» + A;. 

[Hint. The differential equation is dy/dx = e». The orthogonal 
family is defined by the equation dy/dx = — «"*, whence the trajec- 
tories are 2/ = «~* + c. Draw the figure.] 

Determine the orthogonal trajectories of the following families, and 
draw diagrams in illustratioh of each: 

15. x + y ^k, 18. 0^ ^ ^ - 2 log a; -h c. 

16. xy==k. 19. 2a;2 4-2/2=^^2, 

17. y^=4k(x+k). 20. x^+y^:=kx. 



PART II. ORDINARY DIFFERENTIAL EQUATIONS 

OF THE SECOND ORDER 

182. Special lypes. We first .consider some very special 
forms of equations of the second order that are most fre- 
quently used in the application of mathematics to physics, 
namely: 

[I] ^^=: ±ft^y [fc = constant.] 

[II] ^^^2 + B^ + Cy ^0 [A,B,C, constants.] 

[III] il§ + B^ + Cy = F(x). [A, B, C, constants.] 

These are all special forms of the general equation of the 
second order (x, y, dy/dx^ cP y/dx^) = 0. 

[IV] We shall consider other special forms also, some of 
which include the above; namely, the cases that arise when 
one or more of the quantities x, 1/, dy/dx, are absent from the 
equation. (See § 186, p. 334.) 



XIX, § 183] DIFFERENTIAL EQUATIONS 327 

183. Type I. This type of equation arises in problems on 
motion in which the tangential acceleration cP s/dfi is propor- 
tional to the distance passed over: 

(1) S = ±fc^«' 

a form which is equivalent to [I], written in the letters s and 
t If we multiply both sides of this equation by the speed 
V = ds/dt and then integrate with respect to t, we obtain 

but we know that 

and 

hence (2) becomes* 

Case 1. If the sign before Jlt^ is +, (3) becomes 

(4) ^ = Jt^ kVW+^u 
whence i > ^ == \ kdt + C2, 

(5) log(s + Vs2 + Ci)=fc« + C2; 
or, solving for s, 

(6) s = AeM + Be-^. 

♦ This is often called the energy integral, for if we multiply through by 
the mass m, the expression mv*/2 on the left is precisely the kinetic energy 
of the body. 



328 



THE CALCULUS 



[XIX, § 183 



where 2 A = e^* and 2 J5 = — Ci c"^' are. two new arbitrary 
constants. 

By means of the hyperbolic functions sinh w = (e" — €"^)/2 
and cosh w(e" + e"")/2 this result may also be written in 
the form 

(7) s = a sinh (kt) + b cosh (kt), 

where b + a = 2A and 6 — a = 2 J5. 

Case 2. If the sign before fe* is — , Ci must be negative 
also, or else v is imaginary; hence we set Ci = — a^ and write 



(42) 



or 



V = TT = fc Va2 — s2 



whence 



sin-i ( y = fc< + Cs; 



(52) 

or solving for s: 

(62) s = fl sin (kt + C2) =A sin kt + B cos kt, 

where A = a cos C2 and J5 = a sin C2 are two new arbitrary 
constants. 

Equation (62) is the characteristic equation of simple har- 
monic motion; the amplitude of the motion is a, the period is 
2 7r/fc, and the phase is — C2/k, 

The differential equation (1) was first found in § 88, p. 155. 
We now see that the general simple harmonic motion (62) is 
the only possible motion in which the tangential acceleration 
is a negative constant times the distance from a fixed point; 
i.e. it is the only possible type of natural vibration xmder the 
assumptions of § 76, p. 125. 



XIX, § 184] DIFFERENTIAL EQUATIONS 329 

EXERCISES 
Solve each of the following equations: 
. (P8 _ ^ <P8 

6. Find the curves for which the flexion {^y/dx^) is proportional to 
the ordinate iy). 

6. Determine the motion described by the equation of Ex. 1 if the 
speed t; ( = ds/dt) and the distance traversed s are both zero when < = 0. 

7. Proceed as in Ex. 6 for Ex. 3, and explain your result. 

8. Write the solution of Ex. 1 in terms of sinh t and cosh t. Deter- 
mine the arbitrary constants by the conditions of Ex. 6, and show that 
the final answer agrees precisely with that of Ex. 6. 

9. Determine the motion described by the equation of Ex. 3 if 
t; = 2 and « = 10 when < = 0; if t; = and 5=5 when < = 0. 

18i. Type n. Homogeneous Linear Equations of the Second 
Order with Constant Coefficients. The form of this equation is 

(1) *^^'%*c,-o. 

where A, B, C are constants. 

The type just considered is a special case of this one. Fol- 
lowing the indications of the results we obtained in § 183, it 
is natural to ask whether there are solutions of any one of the 
types we found in the special case. 

Trial of e**. If we substitute y = e^'m (1) we obtain the 
equation: 

(2) [Ak^ + Bk + C]^ = 0. 

The factor e** is never zero; hence k miLst satisfy the quad- 
ratic equation 

(1*) Ak^ + Bk + C = 0, 



330 THE CALCULUS [XIX, § 184 

which is called the auxiliary equation to (1). If the roots of 
(1*) are real and distinct, i.e. if 

(3) D=J52-4AC>0, 

then ffiese roots ki and h ore possible values for k, and the gen- 
eral solution of (1) is 

(4) y = Cie*i' + C te^, 

since a trial is sufficient to convince one that the sum of two 
solutions of (1) is also a solution of (1) ; and that a constant 
times a solution is also a solution. 

Trial of y = e'^* -v. If (3) is not satisfied, the substitution 

(5) y = e** • V 
changes (1) to the form 

(6) A^, + [2KA+J5]^ + [Aic2 + J5K + C]t; = 0, 

which becomes quite simple if we determine k so that the 
term in dv/dx is zero: 

(7) 2 ic A + 5 = 0, whence ic = - B/2A) 
then (6) takes the form 

(8) X5 1-7-2 — ^ = - K^Vy 



dx" 4 A 



where K = V4 AC - By {2 A) = V- D/2 A is reoZ if 

(9) D=52-4AC^0, 
which is the case we could not solve before. 

If Z>< 0, the solutions of (8) are 

(10) t; = Ci sin (Kx) + C2 cos (Kx), 

by (62), § 183, p. 328; hence the solutions of (1) are 

(11) y = e'^ .v = e^' [Ci sin (Kx) + C» cos (Kx)], 

where k = - B/{2 A) and K = V^/{2 A) ; these values of 



XIX, § 184] DIFFERENTIAL EQUATIONS 



331 



K and K are most readily found by solving (1 *) for k, since 
the solutions of (1*) are k=(-B ± VD)/(2 A)=k±KV^. 

If Z> = 0, X = 0, and the solutions of (8) are 

(12) v^CiX + C2; 
hence the solutions of (1) are 

(13) y=e^.v = e^' [Cix + CJ, 

where k= —5/(2 A) is the solution of (1 *); since when 
D = 0, (1*) has only one root k= - B/(2 A), 

It follows that the solutions of (1) are surely of one of the 
three forms (4), (11), (13), according as D = B^ — 4 AC is 
+, — , or 0; that is, according as the roots of the auxiliary 
equation (1*) are real and distinct j imaginary, or equal; in 
r&um^: 



D = B»-4AC 


Character of 
Roots of (1*) 


Values of Roots 

OF (1*) 


Solution of (1) 


+ 


Real, unequal 


A^i, k2 


(4) 


— 


Imaginary 


K±KV-1 


(11) 





Equal 


K 


(13) 



We illustrate by some examples put, for convenience of 
comparison, in tabular form. 



Examples 


1 

• 


2 


s 


Equation (1) 


32/"-42/'+2/=0 


32/"-42/'+t2/=0 


32/"-42/'+22/ = 


Auxiliary equa- 
tion (1*) 


3A;2-4A;+I=0 


3A;2-4A;+J=0 


3A;2-4A;+2=0 


Roots of (1*) 


1, 1/3 


2/3, 2/3 


i(2±V-2) 


Solution of (1) 


y=Cie*+C2e*/3 


y=e^^Hci+(^) 


y = e2*/8 (Cl COS 

\/2 , . V2 , 
g a:-fc2sm ^ x) 



332 THE CALCULUS [XIX, § 184 

EXERCISES 

1. 2/"-42/' + 32/ = 0. ' 9. y"-92/' + 14y = 0. 

2. 2/" + 32/' + 2y = 0. 10. 22/"-32/'+2/=0. 

5. 52/"-42/' + 2/=0. 11. 6y"-13y'+62/=0. 
4. 9y" + 12|/'+4y =0. 12. 2/"-3y' = 0. 

6. 2/"-22/'+2/=0. 13. y"-4y = 0. 

6. y" + y' + 2/ = 0. 14. y" + 9y = 0. 

7. y"-22/' + 3y = 0. 16. y" + %' = 0. 

8. 3 2/" + 5 2^' + 2 2^=0. 16. y" ± A;2/ = 0. 

17. If a particle is acted on by a force that varies as the distance and 
by a resistance proportional to its speed, the differential equation of its 
motion is 

dPx/dfi + b dx/dt + ex = 0, 

where c > if the force attracts, and c < if the force repels. Solve the 
equation in each case. 

18. If in Ex. 17, 6 = c = 1, and the particle starts from rest at a 
distance 1, determine its distance and speed at any time t. Is the 
motion oscillatory? If so, what is the period? Solve when the initial 
speed is vo. 

19. If in Ex. 17, 6 = 1 and c = — 1, discuss the motion as in Ex. 18. 

185. Type m. Non-homogeneous Equations. This type is 
of the form: 

where A,BjC, are constants, and F (x) is a function of x only. 
We proceed to show that this form can be solved in a manner 
exactly analogous to § 179, p. 320. First write down the 
reduced equation in the new letter v: 



XIX, § 185] DIFFERENTIAL EQUATIONS 333 

and solve (1*) by the method of § 184. Let v = <t>{x) be any 
one particular solution of (1*) (the simpler, the better, except 
that v = is excluded). Then the substitution 

(2) y = viu 
transforms (1) into 

(3) {Av" + Bv' + Cv) u + (2Av' + Bv)^ + Av^ = F (x); 

but, since v satisfies (1*), the first term of (3) is zero; and 
if we now set du/dx = w temporarily, this equation can be 
written as the linear equation: 

(^) -dx + i Av [^^^ir> 

which is precisely of the form solved in § 179. Comparing 

(4) with (1), § 179, we have 

(5) p.2jy + B. FM. 
^ ^ Av Av 

Having found t/; by § 179, we have 

M = I wdx + Ci, y = uv = v\ I wdx + c» L 

which is the required solution of (1). 
Example 1. Given the equation 

we write the reduced equation 

this is easily solyed by the method of § 184; the simplest particular solu- 
tion is t; = er». Substituting t; = e-* in the general work above, we find 

P = T-^ — = 1 and Q = — p^ = e» sm x; 

Av Av 



334 THE CALCULUS [XIX, § 186 

heDce eS^^ = e*, and 

tt? = e-* fe^ mixdx -{-Ci = ■» e* (2 sin x - cos x) + Cier*, 

w (to + C2 = Y^j e* (sin a; — 3 cos x) — Cie~* + C2t 



y = u*v — — (sin a; — 3 cos x) — Cie~^ + C2e~*. 



EXERCISES 

1. y" — 3 y' + 2 y = cos X. 

il?w. y — ^ (cos a; — 3 sin a;) + cie* + cae^. 

2. y"-42/' + 2y = a;. 

^ns. y = i (aJ + 2) + CleC»^-^2)x 4. o^&-<2)x^ 

S. y" + 3j/' +2 2/ = e». ilns. 2/ = e*/6 — ci^-^* +' cae-^. 

4. y" — 2y' ■}- y — X, Ans. y = a: + 2 +e»(ci +caa;). 

5. 2/" + y = sin X. Ans. 2/ = — J a; cos a; + Ci sin a; + C2 cos a;. 

6. y^' — y' — 2y = sin x. 

Ans. y — ^ (cos a; — 3 sin x) + cie"* + cae^. 

7. y" + 4 y = x^ + cos X. 

Ans. 2/ = i (2 a;2 — 1) + J cos x + Ci cos 2 x + ca sin 2 x. 

8. 2/" - 2 ^' = 62x ^ 1, ^^, 2/ = ia; (e2» - 1) + ci + cae^*. 

9. ^" — 4 2/' + 3 2/ = 2 c3*. Ans. y = xe^ + cie* + c^. 

10. If a particle moves under the action of a periodic force through a 
medium resisting as the speed, the equation of motion is 

(Ps/dfi + Ads/dt = B sin C «. 

Express s and the speed in terms of ^. If A = B = C = 1, what is 
the distance passed over and the speed after 5 seconds, the particle 
starting from rest? 

186. Type IV. One of the quantities x, y^ y' absent. 

Type IV ai <l>(y") = 0. Solve for y", to obtain a solution, 
say y" = a. Then integrate twice. The general solution 
for each value of y" is of the form y = J ax^ + CiX + c^. 



XIX, § 186] DIFFERENTIAL EQUATIONS 335 

In problems of motiorij this type is equivalent to the statement that 
4> (jj) = 0, where 7 J, = cPs/dfi = dv/dL Hence jj, may have any one of 
the several constant values which satisfy <t> (J^) = 0; but if j^, = kf 
8 = kfi/2 + ci< + C2 (see Ex. 24, p. 64). 

Type TVbi y missing, ^(x, y', y") = 0. The substitution 
m = y' = d\f/dx, dm/dx = d^y/dx^ = y", reduces the given 
equation to an equation of the first order in m, Xj dm/dx. 
Solving, if possible, one gets a relation of the form 

/ (m, X, c) = 0. 
This is again an equation of the first order in x and y, and 
may be integrated by methods given in Part I, §§ 177-181. 

The interpretation in motion problems is particularly vivid and 
beautiful. Thus v = ds/dt and jj, = d/o/dt = ^s/df\ hence finy equa- 
tion in jj,i Vf t, wUh 8 ahserUf is a differential equation of the first order 
in V, Solving this, we get an equation in v and t; since v =^ ds/dt, this 
new equation is of the first order in s and t 

Example 1. l+x+a^^=0. 

Setting dy/dx = m, l+x+x^ -r- = 0. 

1 4-x 
Separating variables, — dm = — g" ^* 

Integrating, — m = 1- log a; + ci. 

X 

Integrating again, y = Ipg a; — a; log a; + (1 — ci) a; — C2. 

Interpret this as a problem in motion, with s and i in place of y and x, 
andjr = dv/dt = cPs/dfi. 

Example 2. In a certain motion the space passed over s, the speed 
», and the acceleration jr are connected with the time by the relation 
1 + v^ — jr = 0; find s in terms of t 

Placing JT = dv/dtj the equation 

1+^-1=0 

is of the first order. The variables can be separated, and the integral is 

tan-i t; = ^ -f- ci or » = tan (t + ci), 



336 THE CALCULUS [XIK, § 186 

which is itself a differential equation of the ftrst order if we replace v by 
ds/dL Integrating this new equation: 

Jds =y tan (t + Ci) d^ + C2, or 5 = — log cos (t + a) + 02. 

In such a motion problem we usually know the values of v and s for 
some value of ^. If » = and « = 10 when ^ = 0, for example, ci must be 
zero (or else a multiple of w) and Ci must be 10; henc6 

s = — log cos t + 10. 



Examples. 1 +a;f^ +0^2^ = = 1 +a;m + 



dm 

This can be written dm/dx + m/x = — l/x^, 
which is linear in m and a;, the solution being 

m = — -loga; + -- 
x X 

The second integration gives 

y - — i [log a;]2 +ci log x + C2. 

Interpret this as a motion problem, and determine ci and C2 to make 
y = 10 and m = 3 when a; = 1. 

Type IVc: X missing. <t>(y, y\ y") = 0. The substitution 

m = y' gives 

,/_^ „n^dy' _dy' dy_dm 

and the transformed equation is an equation of the first * 
order in y and m. We solve this and then restore y' in place 
of m, whereupon we have left to solve another equation 
(in X and y) of the first order. » 

This is precisely the way in which we solved Type I, § 183, 
Type I being only an important special case of Tj^e IV. 

Example 1. If the acceleration jj, is given in terms of the distance 
passed over (compare § 188), we have 

d^s ^ . . dv ^ . . 

This is transformed by the relation 

. _dv __ du^ds __ dv 
^T- dt ~ dsdt ' ds^' 



XIX, § 186] DIFFERENTIAL EQUATIONS 337 

(which is itself a moat vaLuahle formula) into 

do ^ . V 

^» = «(8) 

in which the variables can be separated; integration gives 

which is called the energy integral (see footnote, p. 327). 

The work cannot be carried further than this without knowing an 
exact expression for ^ («). When <f> («) is given, we proceed as in § 183, 
replacing v by ds/dt and integrating the new equation: 

^ v^y («) (fe + 2 c 

Unfortunately the indicated integrations are difficult in many cases; 
often they can be performed by means of a table of integrals. One case 
in which the Integrations are comparatively easy is that already done 
in § 183. 

EXERCISES ' 

1. y"2^'— 4 x2 = 0. Ans. y = ±l/3x^ + cix + eg. 

2. 2/" = Vl + 2/^2. Ans, 2 2/ = cie* + e-^/ci + C2. 

8. xy" + y' = x^. Ans. y — x^/g 4- ci log x + C2. 
4. s cPs/dfi + ds/dt = 1. Atis. s^ = ^ + ci^ + C2. 

9. ^ = rc* cos a;. 10. 



11. ^ = «• - cos 2 a;. 12. 



dx^ 


XKry 


• 


(jpy 

dx^ "■ 


^. 




dx^ 


x + Z 


sin a;. 


cPy 
dx^ 


1 + 


(1) 



13/2 



13. Show that Ex. 12 is equivalent to the problem, to find a curve 
whose radius of curvature is unity. 

14. The flexion {(^/dx^) of a beam rigidly embedded at one end, and 
loaded at the other end, which is unsupported, mki} — x)y where A; is a 
constant and I is the length of the beam. Find ^, and determine the 
constants of integration from the fact that y — Q and dy/dx = at the 
embedded end, where a; = 0. 



338 THE CALCULUS [XIX, § 186 

15. Find the form of a uniformly loaded beam of length /, embedded 
at one end only, if the flexion is proportional to P — 2 te + a^, where 
a; = at the embedded end. 

16. Find the form of a uniformly loaded beam of length I, freely 
supported at both ends, if the flexion is proportional to P — 4 a:^ in each 
half, where x is measured horizontally from the center of the beam. 



PART III. GENERALIZATIONS 

187. Ordinaxy Equations of Higher Order. An equation 
whose order is greater than two is called an equation of higher 
order; the reason for this is the comparative rarity in 
applications of equations above the second order. We shall 
state briefly the generalizations to equations of higher order, 
however, since they do occur in a few problems, and since 
it is interesting to know that pratically (he same rules apply 
in certain types for higher orders as those we foimd for 
order two. 

188. Linear Homogeneous Type. The work of § 184 can be 
generalized to any linear homogeneous equation with constant 
coefficients: 

Thus if we set y =? e**, as in § 184, we find 
(1*) fc" + aik^-' + . . . + On-ifc + a„ = 0, 

again called the auxiliary equation. Corresponding to any 
real root ki there is therefore a solution e*** ; if all the roots are 
real and distinct^ the general solution of (1) is 
(2) y = Cie*i^ + Ca 6*2^ + • • • + C„6*«^ 

where fci, fe, • • • , A;„ are the roots of (1). Curiously enough, 
the chief difficulty is not in any operation of the Calculus; 
rather it is in solving the algebraic equation (1*). 



1 



XIX, § 188] DIFFERENTIAL EQUATIONS 339 

It is easy to show by extensions of the methods of § 184 

that any pair of imaginary roots of (1*), k = kiLK V— 1 cor- 
responds to a solution of the form^ 

(3) y = e*^^ [C sin {Kx) + C" cos {Kx)], 
which then takes the place of two of the terms of (2). 

Finally, if a root k = k of (1*) occurs more than once, i.e. if 
the left-hand side of (1*) has a factor (fc — kY, the cor- 
responding solviion obtained as above should be multiplied by 
the polynomial 

(4) Bo + BiX + B2:t'+'"+ B^,^^-\ 

where p is the order of multiplicity of the root {i.e. the expo- 
nent of (fc — k)^, and where the B^s are arbitrary constants 
which replace those lost from (2) by the condensation of 
several terms into one. 

The proof is most easily effected by making the substitution y = e^'u, 
whereupon the transformed differential equation contains no derivative 
below d^u/dx^; hence u = the polynomial (4) is a solution of the new 
equation, and y = e** times the polynomial (4) is a solution of (1). This 
work may be carried out by the student in any example below in which 
(1*) has multiple roots. t 

t This fact is often made plausible by the use of the equations 
e«V-i = cos u + V— 1 sin u, e-"V-i = cos u — V— 1 sin u; 
these equations can be derived formally by using the Taylor series for e*, 
cos w, sin w, with » = wV— 1, but they remain only plausible until after a 
study of the theory of imaginary numbers. The solutions e* =*= K"^-^ are 
indicated formally by (2) ; hence it is plausible that (3) is correct. 

A more direct process which avoids any uncertainty concerning imagi- 
naries is almost as easy. For the substitution j/ = e**«w (see §184) gives a 
new equation in u and x which, together with its auxiliary, has coefficients 
of the form (d^A( k)/d k^) -r-nl, where A (k) represents the left-hand side 
of (1*). Now irV — 1 is a solution of the new auxiliary by development of 
A(:k) in powers of (k—K); hence u = sin (Kx) and u =cos (Kx) are solu- 
tions of the new differential equation, as a comparison of coefficients dem- 
onstrates. This process constitutes a rigorous proof of (3). 

t To avoid using i mag inary powers of e, if that is desired, substitute 
2/ = c** [cos (Kx ) -h V — 1 sin (Kx)]u, when the multiple root is imaginary, 
k = K + KV^^l. 



340 



THE CALCULUS 



[XIX, § 188 



These extensions of § 184 should be verified by the student by a direct 
check in each exercise. 



Example 


1 


% 


s 


(1) 


2/'" - 2/' = 


2/*^H-62/'"+12y"+82/'-0 


y'" + 82/=0 


(1*) 


A;3-A; = 


fc4 + 6A:3 + 12A;2+8A; = 


A;3 + 8 = 


k-= 


0, 1, - 1 


0,-2,-2,-2 


- 2, 1 ± V3 V- 1 


y 


Ci+cje^+cje"* 


c\ + e"^ (C2 + Cjo: + c^pt^) 


cie-2*4-e*(c2CosV3a; 
+ Cg sin y/Zx) 



189. Non-homogeneous Type. The non-homogeneous type 



(1) 



d^y 



d^ y 



(ir»''"^'dx"-^ + 



+ an-i^ + an^F(x) 



cannot be solved in general by an extension of § 185. But in 
the majority of cases*which actually arise in practice,* a suffi- 
cient method consists in differentiating both sides of (1) re- 
peatedly until an elimination of the rigfA^-hand sides becomes 
possible. The new equation will be of higher order still: 



(2) 



d^y I aS«\ I 



"T Am-i -IT 4" Am — 0, 



but its right-hand side is zero. Solve this equation by § 188 
and then substitute the result in (1) for trial; of course there 
will be too many arbitrary constants; the superfluous ones 
are determined by comparison of coefficients, as in the 
examples below. 

Example 1. y'" + j/' = sin x. 

Differentiating both sides twice and adding the result to the given 

equation: 

y^+22/'" + j/' = 0. 



* For more general methods, see any work on Differential Equations; 
eg, Forsyth, Differential Equations, 



XIX, § 189] DIFFERENTIAL EQUATIONS 341 

The auxiliary equation k^ -\- 2 k^ + k = has the roots A; = 0, A; = ± 

V— 1 (twice). Hence we first write as a trial solution yt the solution 
of the new equation: yi = ci + fe + cax) cos a: + (c4 + c^x) sin x; sub- 
stituting this in the given equation, we find — 2 ca cos x — 2 c^sinx = 
gin Xf whence ca = and c^ = — 1/2; substituting these values in the 
trial solution yt gives the general solution of the given equation: 

y = ci + C2 cos a; + (C4 — x/2) sin x, 
I 

EXERCISES 

1. 2/'" — 3 y" ^ 0. Arw. y = ci + cax + cge*". 

2. y'" — 2/" - 4 y' + 4 y = 0. Arw. y = cie» + C2e^ + cae-^*. 

8. ^^ — 16 y = 0. Atw. y = cie^ + C2e~2» + cs cos 2 a;+C4 sin 2 x, 

4. y*^ — 6 y" + 9 = 0. Arw. ^ = e* V3(ci + cax) + e-*V3(c3 + C4x). 

6. y^+62/'"+92/' = 0. 

Ans. y = ci + (c2 + cax) cos Vs x + (c4 + csx) sin VSx. 

6. y^- 162/'" + 64 2/ = 0, A;=2, 2, -1 ±iV3, -l±iV3. 
ilns. y = 6^(ci + cax) + e"* [(cs + C4a;) cos VSx + (cs + cea;) sin V3 x. 

7. 2/"-5 2/'+4 2/ = e2«. ^^. 2/ = cie»«- (l/2)e2» +p2e4*. 

8. 32/" + 42/' + 2/ = sina;. 10. 2/'" - 2/" - 4 2/' + 4 2/ = e». 

9. 2/'"- 32/" + 22/' = a;. 11. 2/*^ - 5 2/" + 4 2/ = 62«. 

12. Solve the equation 2/'" + 2/' = by first setting ^' = p. 
Solve the following equations by setting y' = p or else y" = q. 

13. 3 2/'" -4 2/" + 2^' =0. 16. 2/'" + 3 2/"+2 2/' = e». 

14. 2/'" + y" + 2/' = 0. 17. 2/*^-2/" = 0. 

16. 2/'" + 2/' = sin X. 18. 2^^ + 2/" = e». 

The following equations, though not linear, may be solved by first 
setting 2/' = p or 2/" = g or ^"' = r. 

19. 2/' = 2/" + VI + 2/"2. 21. l+x+xV = 0. 

20. 2^" + 2/"'a; = (2/")2 a^. 22. 3:2/*^ + 2/'" = a;^. 

23. Solve the equation x^y" +xy' — y = logx, 

[Hint. Put x = «•; then 
dy ^dy dz^ _\dy , ^ ^ d_ fldy\ dz _ J:/^_^Y 
dx~ dzdx " X dz' dx^ ds \a; ds/ <ia; a^ \d2^ ds/ ' 
so that the transformed equation is 

— I — y = 2, whence 2/ = cie* + 026"* — 3 = CiX + C2X~^ — log a;.] 



342 THE CALCULUS . [XIX, § 189 

Solve the equations, 

24. x^y" — xy' — Zy^O, 25. rty" — y' = log x, 

26. (a; + l)2 2/"-4(x + l)2/' + 6y = x, (x + 1 =». 

27. (a + 6x)V' + (a + 6a;)y' - 2/ = log (a + 6a;), (« + &«=«•). 

28. a;V"-6j/=l+a;. 

190. Systems of Differential Equations. Let us finally con- 
sider systems of two equations, and let us suppose the equa- 
tions to be linear in the derivatives, that is, to involve only 
the first powers of these derivatives. 

191. Linear System of the First Order. Let the equations be 

(1) 2/' = ax 4- &2/ + C2 + d, 

(2) z' = aix + biy + CiZ + di, 

where the coefficients are constant. We wish to determine 
y and z as functions of x. 
Differentiating (1) with respect to x gives 

(3) 2/" = a + 6i/' + c2'; 

then the elimination of z and 2' between the three equations 
(1;, (2), (3), gives a differential equation of the second order 
in y, which should be solved for y. 

192. dx/P = dy/Q = dz/R. Here P, Q, and R are functions 
of X, y, z. Let X, /i> v be any multipHers, either constants or 
functions of x, y, z. Then, by the laws of algebra, 

. V •dx _dy _dz _ \dx + fidy + vdz 

^^^ P~ Q^ R~ \P + ^Q+vR ' 

Suppose that we can select from these ratios (or from these 
together with others obtainable from them by giving suitable 
values to X, /i> »') two equal ratios free from 2, i.e. containing 
only x and y. Such an equation is an ordinary differential 
equation of the first order in x andt/. Solving it, we obtain 
(2) fix, 2/, ci) = 0. 



XIX, § 192] DIFFERENTIAL EQUATIONS 



343 



Suppose that a second pair of ratios can be found, free from 
another of the variables, say y. The result is an equation of 
the first order in x and z. Let its solution be 

(3) F{x,z,C2) = 0. 

Then (2) and (3) form the complete solution of the system. 
Conversely, differentiating (2) and (3) with respect to x, 
eliminating ci and Ca, and solving for dx:dy: dz, we find a 
system like (1). In selecting the second pair of ratios, the 
result (2) of the first integration may be utilized to eliminate 
the variable whose absence is desired. 



Example 1. 



dx/x^ = dy/xy = dz/^. 




The first two ratios give dx/x = dy/yy whence y = c\x. Putting this 
value of y in dy/xy = dz/:? gives dy/{ciy^) = dz/^, so that 

c\y z 

or, a = Ci2/ + ciCzyz = x + c^z. Hence 
the solutions are given by the two 
equations y = ciXy s = a; + o^z. 

Interpreted geometrically, the solu- 
tions represent a family of planes and 
a family of hyperboloids. These are 
the integral surfaces of the differ- 
ential equation. Each plane cuts 
each hyperboloid in a space curve, 
forming a doubly infinite system of 
curves, the integral curves of the 
differential equation. The system may be written dx:dy:dz =a^:xy:y^. 
But the direction cosines of the tangent to a space curve are proportional 
to dxj dy, dz. Thus the given equations define at each point a direction 
whose cosines are proportional to x^, xy^ y^. Our solution is a system of 
curves having at each point the proper direction. What curve of the 
above system goes through (4, 2, 3)? What are the angles which the 
tangent to the curve at this point malces with the coordinate axes? 







I' 



Pig. 88. 



344 THE CALCULUS [XLX, § 192 

— , ^ dx dy d% 

Example 2. = — ^- = 

y — z z — X X — y 

Let X =5 /* = y = 1. Then each of the above fractions equal 

dx -\-dy -\-dz 

m ■■■■■!■ • 


But since the given ratios are in general finite, this gives 
dx + dy + dz = Oy whence x +y + z = ci. 
Again, let X = a;, a* = j/, y = 2. This gives 

xdx -\-ydy -\-zdz = 0, whence x^ + y2 _j_ ^2 = ^j. 

Thus the integral surfaces are planes and spheres, and the integral 
curves are the circles in which they intersect. 

In this example the multipHers X, /k, v have been chosen so as to get 
exact differentials. 

Ti o dx dy dz 

Example 3. = — f— = — • 

x—y x+y z 

The first two ratios are free from z and give 

arc tan {y/x) = log [c\x^/^x^ + 2/^]. 

Using the multipliers \ — Xj /x = y, v = 0, and equating the ratio thus 
obtained to the last of the given ratios, we find ' 

xdx+ydy dz , ^ i a ^ji 

^_^y2 = 7> whence x^+y^= ^z^. 



EXERCISES 

1. x dxly^ = y dy/x^ = dz/z, Ans, a?* — ^ = ci; a? = c^ (x? + ^). 

2. dx/x = dy/y = — dz/z. Ans. yz = a; y = CiX- 

3. dx/yz = dy/xz = d&/(x -\- y). 

Ana. ^ -2{x + y) +ci;3i^ ^^ =02. 

4. dx/(y + z) = dy/(x + z) =dz (x + y), 

Ans. {x — y) = ci (x — s) 

{x — yY{x + y-\-z)^ a. 

5. dx/{x^ + ^) = dy/(2 xy) = dz/{xz + yz). 

Ans. 2 y = ci (a;2 — y^); x + y =c^. 

ft ^ — 2a?y . dz^ _. 2xz 
dx" 3^^y^ — s^' dx s? — y^ — ^ 

Ans. y = CiZ = 02 (a^ + ^ + s?). 



XIX, § 192] DIFFERENTIAL EQUATIONS 345 

„ dy _ 2 — 3a; . dz _ 2x — y 
dx~'3y-2z' dx^Sy-2z 

Ans, x + 2y + 3s = ci;a? +1^ + ^=^0i. 

8. dx == — ky dt] dy == kx dt, 

Ans, X =^ A COS kt-\-B gin kt; y = A sin kt" B cos kt, 

9. dx/dt =» 3 x — y; dy/dt =^x-\-y, 

Ans, x=^(A+Bt)&^''yy = (A''B+Bt)&^K 

10. Determine the curves in which the direction cosines of the tan- 
gent are respectively proportional to the coordinates of the point of 
contact; to the squares of those coordinates. 

11. A particle moves in a plane so that the sum of the exial compo- 
nents of the speed always equals the sum of the coordinates of the 
particle, while the difference of the components is a constant A;. De- 
termine the possible paths. Ans, x -\-y = ci<^\x — y =kt-\-Ci, 

12. If the particle in Exercise 11 is at (1, 1) when i = 0, where is it 
;rlien 2 = 5? Approximately how far has it traveled? 



INDEX TO TABLES 



Beferences to pages of the Tahles in Italic numerals. 
References to pages of the body of the book in Roman numerals. 

PA6S8 

Table I. Signs and Abbreviations IS 

Table IL Standard Formulas S-IS 

Table III. Standard Curves 19-S4 

Table IV. Standard Integrals . • . . • . • S6-60 

Table V. Numerical Tables . , • .• # • • 61-60 



m 




Greek Alphabet 






Lettsbs Nambs 


LsTTKBB Nambs 


Lettebs Names 


Lettbkg 


\ NAMB9 


Aa 


Alpha 


H 17 Eta 


N I' Nu 


Tr 


Tau 


BiS 


Beta 


e Theta 


S^ Xi 


T V 


Upsilon 


r7 


Gamma 


It lota 


Omicron 


$0 


Phi 


A8 


Delta 


E jc Kappa 


Hit Pi 


Xx 


Chi 


Ee 


Epsilon 


A X Lambda 


Pp Rho 


yfrrj, 


Psi 


zi- 


Zeta 


M/i Mu 


Z <r f Sigma 


w 


Omega 



TABLES 



[Boman page numbers refer to the body of the text ; italic page nambers refer to these 
Tables.} 

TABLE I 
SIGNS AND ABBREVIATIONS 

1. Elementary signs assumed known without explanation . 

+ ; db; T; — ; =; ay.h=^a'h = ab\ a-i-b = a/b = a : 6 = - ? 

cfi; a3; a»; a-*=l/a»; a^^^Va; aPf^^VaP; aO = l; (); []; 
a', a", ..., a(») (accents) ; ai, 02, ..., «« (subscripts). 

^ , not equal to. >, greater than or equal to. 

>, greater than. -^^ less than or equal to. 

<, less than. n\ (or |n) , factorial n = n(»— 1) •••3.2.1. 

q.p., approximately. | a |, absolute or numerical value of a. 

3. Signs peculiar to The Calculus and its Applications : 

(a) Given a plane curve y =f(x) in rectangular coordinates («, y) ; 
m = slope = dy/dx =f(x) = y' = first derivative ; see p. 19. 
[Also occasionally D^y, f^, y, p, by some writers.] 
a = angle between positive a>-axis and curve = tan-i m. 
Ay, A2y, ..., A*»y, first, second, -.., n*^ differences (or increments) of y, 
dy =f(x) . Ax, (Py =zff(x) • A?, •••, d^y =/(«)(a;) • Ax**, first, second, 
— , n*^ differentials of y. 

rr = relative rate of increase, or logarithmic derivative ; see p. 114 ; 

=/(«) -5-/(«) = (dy/dx) -J- y = d (log y)/dx = r^ -5- 100. 
Tp = percentage rate of increase = 100 • rr. 

b = flexion = d^/dx^ z=zff(x) = y" = second derivative ; see p. 62. 
d^/dx:^ =/(«)(x) = y<'») = n^ derivative. 

K= curvature =zl •%- B; .B = radius of curvature = 1 -i- JST; p. 140. 

1 



2 SIGNS AND ABBREVIATIONS [1, 3 

Sf(x) dx = indefinite integral otf(x); see p. 83. 
Cf(x)dx = f'~ /(x)da; = definite integral of /(«); see p. 87. 

= arc between x = a and x = b. 

]b -ix = b 

= A = area between y = 0, y = f(x), « = «, x = 6 ; seep. 90* 
a -lz = a 

(6) (^it?€n a cwroe p =/(^) in polar coordinates (p, ^) ; 
^ = Z (radius vector and curve) = ctn-i [(dp/d0) -5- p] 

= ctn-i[d(logp)/d^]. 
= Z (circle about and curve) = tan-i [(dp/dB) -;- p] 

= tan-i[d(logp)/d^]. 

= -4 = area between p =f(^6), 6 = a, = ^; see p. 160. 

a Jtfssa 

(c) For problems in plane motion : 

s = distance. r, = horizontal speed = projection of v on Ox. 

t = time. Vy = vertical speed = projection of v on Oy. 

m = mass. ^*, = horizontal acceleration = proj. of Jon Ox, 

v = speed. jy = vertical acceleration = proj. of J on Oy. 

V = velocity (vector), jy = normal ace. = proj. of J on the normal. 

J = ace. (vector). jj. = tangential ace. = proj. of j on the tangent 

= angle (of rotation), a = angular acceleration. 

(V = angular speed. g = acceleration due to gravity. 

(d) Problems in space; functions z =f(x, y, •••) of several variables • 
Previous notations are generalized when possible v^ithout ambiguity, 

exceptions are ^^^j^^^f^, ^^g^/^^^^. 

r = Z'^zjdx^ = /,, ; « = ^zjhx dy =f,y=^fy,', t = d^z/dy^ = fyy. 
[The notation (dz/dx)^ used by some vnriters for dz/dx is ambiguous.] 

4. Other letters commonly used with special meanings: 

IT = ratio of circumference to diameter of circle = 3.14159- ••. 

e = base of Napierian (or hyperbolic) logarithms = 2.71828-.. 

ilf = logio e = modulus of Napierian to common logarithms = 0.434-*- 

^ = " sum of such term as " ; thus : ^ '~^a^ = ai + ag* + ••• ««*• 

(«» i^j 7)» — direction angles of a line in space. 
(Z, w, n), — direction cosines ; I = cos a, etc. 

5. H.'M. — simple harmonic motion. 

e or e, — eccentricity of a conic ; also phase angle of a S. H. M. 



II, A] EXPONENTS AND LOGARITHMS 3 

a, — amplitude of a S. H. M. 

(a, 6), — semiaxes of a conic ; (a, 6, c), semiaxes of a conicoid. 

A = difference (of two values of a quantity). 

p = density ; also radius vector, radius of curvature, radius of gyration. 

6. Trigonometric, logarithmic^ hyperbolic^ and other transcendental 
functions : See Tables, II, A ; II, F, 3 ; II, G ; II, H ; and consult Index. 

6. Inverse function notations : 

If y =/(«), then f-^iy) =x; f-^ denotes an inverse function, [This 
notation is ambiguous ; confusion with {/(«)}"^ = 1 h- /(«).] 

sin-i X or arc sin x, — inverse of sin sc, or anti-sine of x, or arc sine a?, 
or angle whose sine is x. [Other inverse trigonometric functions, and 
hyperbolic functions, follow the same notations. See Tables, II, G, 18 ; 
H,7.] 

TABLE II 

STANDARD FORMULAS 

A. Exponents and I^ogarithms. 

(The letters B, 6, etc. indicate base; L, I, *- indicate logarithm; N, n, 
..• indicate number; base arbitrary when not stated. See § 69, p. 99.) 

Laws of Exponknts Rules or Logarithms 

(1) Nz=B^;in particular (1)' L = logjiVT, i.e. N = B'°»*^; andr 
1=»50; B^Bt; \/B= B^K logl = 0; loggB^i; logB(l/5)=-l. 

(2) BL.B = B^+K (2)' log (A^ . n) = log N + log n. 

(3) B^-^Bi = B^-K (3) ' log (N^n)= log N - log »u 

(4) (Bt)» = B^L^ (4)' log (iV») = n log JST. 

(5) N=B^,B = b^,N= 6*^. (5) ' logj, iV^ = logi, B . logs N, 

B^6, &=10 gives A;=0.4842945=jr=logio6; \og^^N=-M' XogtN, 
-ff=10, 6=« gives A=2.302585=l+Jf=logel0; logei^=(l-!-Jlf) logio^^. 
&=iV gives L=l/*, l=log65. loga&; «.^., log, 10=1 -i-logio«. 

L=^x gives 10«=«**-*^; e*=10** 

N^x gives log,o x^M > log, x ; log, 85= (1-f-if ) logjo x. 

(6) y = cx» gives r = nw + A;, w = logio x, t? = logi«,y. A; = logio c. 

(7) y = ce«* gives v^mx-\-k, t? = logio y, wi =« logio e = aJlf, 
* = logio c. 



STANDARD FORMULAS 



[II. B 



B. Factori. 

(1) a2 - &2 = (flf _ 5)^^ ^ 5), (2) (a ± 6)« = a* ± 2a6 + 6». 

(3) a»— 6» = (a — 6)(a»-i + a*-^ 6 + a»-«62 ^ ... ^ 5»-i). 

(4) a2»+i + 62»+i = (a + 6)(a2» - a2»-i6 + ... + fes*). 
See also Tables, IV, Nos. 16, 20, 21, 49, 60. 

(5) Polynomials : if /(a) = 0, f(x) has a factor as — a; in general ; 
f(x) -J- (x — a) gives remainder /(a) . 

(6) (a ± 6)» = a» ± -a-ift + ILilLzil a»-262 + ... + (±l)»6» 
See II, B, 1, p. 7. ^ ^ * ^ 



C. Solation of Bquations. 

(I)ax2 + 6x + c = 0, roots: x = — ^ ± :^^^Ei«£ = - A ± >^, 
^ ^ ' 2a 2a 2a 2a' 



where 

D = b^'- 4ac'j roots of (1) are 



real 

coincident 
. imaginary j 



when D 



>0 
= 
<0. 



z.; 



(2) a;» + pia:»-i ^ pax"-! + •• + p«-ix + P» = 0. Roots : Xi, Xa, — , 
then ^Xi = — 1)1, 2ja;t«,- =P2, 2jx»xyX* = — ps, etc. 

(3) /(x)— 0(x)=O: roots given by intersections of y rr/Cx), y=0(x). 
(Logarithmic chart often useful. ) Find roots approximately ; redraw 
figure on larger scale near intersection. (Generalized Horner Process.) 

(4) Simultaneous Equations : /(x, y) = 0, 0(x, y) = : roots (x, 
are points of intersection ; redraw on larger scale as in (3). 

(5) Linear Equations : 

(a) 2 equations in 2 unknowns : ^ . ^ [• 

I a2X + 62!/ = C2 J 



Solutions : x = 



y = 



cibi 
C262 

aiCi 
a^c^ 



a\b\ 
a^b^ 

aibi 
azb^ 



= (C162 — C261) -i- (ai6a — aa&i)) 



= (aiCa — aaCi) -5- (0162 — fl2&i)» 



11, D] 



FORMULAS OF ALGEBRA 



(1) n equations in n unknowns 
2f ••• f ft. 

Qi bi "• pi ••• A^i 
02 O2 • • • P2 '•• Jco 



ciiXi + biX2 + ••• + kiXn =P« ; i = 1, 



Solutions : o^ = 



where 






(^n^n'-'Pn '••^n 



■J- 7} J ^^°™° of ^'8 replaces colnmn of 1 
\ coefficients of <bj* ) 



2>= 



di 61 ••• Jfei 

G2 &2 *•• ^2 



On &«••• A^n 





6a ••• X^ 




61 ••• ki 




63 ••• ^8 




63 • • • ^8 


= ai 


• • 

• • 


-a2 


• • 

• • 




• • 

bn"'K 




• • 
bn ••• A;„ 



+ -+(-l)»-ia. 



61 ••• 


A:i 


02 ••' 


.A:2 


• 


• 


• 


• 


• 


• 


6»-i 


*.-i 



[Coefficient of a,- skips tth row of D, The last formula is a general 
definition of a determinant.] 



D. Applications of Algebra. 

1. Interest. (P = principal ; p = rate per cent ; r =p-i- 100 ; n = 
number of years ; An = amount after n years.) 

(a) Simple interest : An = P(^l + nr). 

(6) Yearly compound interest: ^ = P- (1 + r)«. 

(c) Semiannually compounded : ^, = P ( 1 + r/2)2*. 

(d) Compounded once each wth part of year : -4, = P(l + r/m)*^. 

(e) Continuously compounded i An = P lim (1 + r/m)*^ = Pe*^. 

2. udranm^ies. Depreciation. (/= yearly income (or depreciation or 
X)ayment or charge) ; n = number of years annuity, or depreciation, runs.) 

(a) Present worth Pof yearly annuity I: 

P= 7[(1 + r)n - l]-^[r(l + r)«]. 

(6) Annuity J purchasable by present amount Pj or, yearly deprecia* 
tion I of plant of value P : 

1= P[r(l + r)»»]H-[(l + r)»-l]. 

(c) Final value ^^ of n yearly payments : 

^ = I(l + r)[(l + r)«-l]+r. 



6 STANDARD FORMULAS [II, D 

3. Permutations Pn,n <^^^ Combinations Cn.ri of n things r at & time, 
without repetitions : 

(a) Pn,r = w(«— 1) •• (n — r+ 1)= «! -f-(n — r)! 
(6) C«,, = P„.,-^rI=[n(«-l)... (n-r + l)]-rl 

4. Chance and Probability. 

(a) Chance of an event = (number of favorable cases) -?- (total number 
of trials) <1. 

Chance of succeBsive (independent) events — product of separate chances <1. 
Chance of at least one of several (independent) events — sum of separate chances. 

(6) Probable value v of an observed quantity : 
V = [ymi\-^n= arithmetic mean of n measurements wi, m^^ •••, 
w„ ; probable error in « = ± .6745 \ ( ^ (^ — w*»)^) -?- w (» — 1). 

(If the observations are unequally reliable, count each one a number of times, p^, which 
represents its estimated reliability ; Jt),- = " weight " of m^). 

(c) Probable value of k in formula v = kx: 

A; = 2 XiVi -5- 2***' ^^^^ ^ measurements (a;i, «i), (iCg, W2), •••, (x«, «»); 

probable error in A; = ± .6746 \/ 5) (*^» - v»)2 -r- (n — 1) ^a^^^ g^e Exs. 
37, p. 58 ; 28, p. 309. 

(d) Probable values of A;, Z, m, •••, in formula t? = A;aj + Zy + m« + — 
are solutions of the equations : 

k 2)^*^ + ^ S ^♦^/i + wi 2^ ^'^^ "•■ **' " S^*"^< 
k ^XiZi + I 2J y»2f» + m ^Zi^ + ... = V^f^v^ 



See also Exs. 37-42, p. 58, Example 2, p. 292, and Exs. 24-31, p. 308. 
{Bules for Least Squares, See also Observational Errors^ No. Ill, J.) 



II, E] SERIES 7 

E. Series. 

1. Binomial Theorem : Expansion of (a + 6)" 

(a) n a positive integer : (a + 6)» = a'»+ 2*^^ C'„,ra"^6'' ; 

[Cn,r: see No. II, D, 8, p. 6, and also II, B, 6, p. A.] 

(6) n fractional or negative, | a | > | 6 | : 
(a -|-6)«=a» + —a^-^b + ^i^=iiia«-262+ ... + Cn,ra«-*'6'+ - (forever) 

II iB I 

(c) Special cases : 

= (1 ± «)-! — 1 T » + a^ T «»'+ «* T ••• ; ( I » I < 1). (Geometric progression.) 



l±x 



2 2«.2I 2»-81 



2. Arithmetic series : a + (a -f d) + (a + 2 d) + ... + (o + (w — l)d) ; 
last term = 2 = a +(» — l)d; sum = s = n(a + Z)/2. 

3. Geometric series : a •\- ar -\- at^ + ar^ + •••. 

(a) n terms : Z = ar^-^ ; « = ^ " ^ = a — ^ • 
^ ^ ' r-1 r-1 

(6) infinite series, | r | < 1 : « = a/ (I — r). 

4. 1 + 2+3 + 4+ ••• +(n-l)+n = n(n+ l)/2. 

5. 2 + 4 + 6 + 8 + ... +(2n-2) + 2n = n(7i + l). 

6. 1 + 3 + 5 + 7+ ... +(2?i-3) + (2n-l) = n2. 

7. 12 + 22 + 32+ ... +(w-l)2+n2 = n(n + l)(2n+l)-^31 

8. 18 + 28+38+ ... +(n-l)« + n8 = [n(» + l)/2]2. 

9. 1 + 1/1 1 + 1/2! + 1/31+ ... =lim(l + iy = 6 = 2.71828.-.. 

10. e» = l+x/l! + a;2/2i + ic«/3l... ; (all x); a* = e*i<««. 

11. log.(l ±a;) = ±a-a;2/2±a:8/3-x*/4±ic5/6 ; (-l<a;< + 1). 

12. log, [(l+x)/(l-a;)]=2[x + a;V3 + x^/6+-];(-l <«< + !). 
[Computition of log JV^: set W-(l + x)/(i - x); then oj = (iV- l)/(iV^+ 1); use II, A, 6'.] 



8 STANDARD FORMULAS [n,E 

13. sin a; = a;/l ! - xV3 ! + x^/s i - x^ll I + — ; (all x). 

14. co8a; = l-xV2I + x*/41-a^/6!+ ...;(aU«)- 

15. tan a; = a; + ie»/3 + 2x6/15 + 17x7315+ ... ; (|a;|<ir/2). 

General term : 22» (2»" - l)52n-l -i-(2»)! ; see iJ;», Tbftfo*, V, N, p. m, 

16. ctnx=l/x-x/3-x8/45-V252,_i(2x)a»-i^(2n)!; 

(0<|x|<ir). 

17. secx = 1 + xV2 ! + 6 x*/4 ! +2^ [-B2,.x2»/(2 n)l] ; ( | x |< ir/2). 

18. C8CX=l/x+x/31 + 2j[2(22«+i-l)B2n+ix2»+V(2n+2)!]; 

(0<|x|<ir). 

19. 8in-ix=ir/2-C08-ix=x+xV(2.3) + l. 3x5/(2.4. 5)+.. .;(|x|<l). 

20. tan-ix = ir/2-ctn-ix = x-xV3 + x6/5 — xV7 + ...; (|x|<l). 

21. (e« H- 6-»)/2 = cosh x = 1 + xV2 1 + x*/4 1 + x^/e !+..•; (all x). 

22. (e* - 6-*)/2 = sinh x = x + x8/3 1 + xV5 1 + xV? I + ... ; (all x). 

23. e-«* = l-x2 + x*/21-a^/3! + x8/4I ; (allx). 

24. /(x)=/(a)+/(a)(x-a)+/"(a)(x-a)V21 + ... 

+/(— i)(a)(x - a)^y{n - 1) ! +^,. 

Taylor's Theorem ; Remainder En' \Kn\< [Max. | f^^^x) I ] I (a - a)» | -»- n 1 ; 
^n =/*»la+i;(a5-a)](aj-a)n+n ! ; En =(1 -i>)«-l/^»)[a +/>(» - a)] (a? - a)Vn ! ; 
IPl<l. 

Set a - 0: /(x) -/(O) +/'(0)aj +/"(0)a5V2 ! + ••• +/(«-l>(0)a»»-V(n-l)! +i?i»; 

[JToc/owrtn]. 
Set » - r + A, a - r : /(r + A) -/(r) + A/'(r) + A«/"(r)/2 I + ... + ^«. 

25. fix + h,y + k) -/(fl5, y) + [hMx, y) + k/y(x, y)] 

+ [A?/,, + 2 A*/,„ + ifc«/„„l + 2 1 + ... + i;; 
I JT,, I < M{ |A| + |£|)"-s-ft!, if— maxim am of absolute values of all n^ deriyatiTes. 

26. If fix) — afl/2 + a^ cos + a^ cos 2 + a^ cos 8 + ... 

+ &i sin 05 + &j sin 2 » + &8 s**! 8 CD + ... ; (—«-<»< + «-). 

On = - 1 /(») cos «» rfoj ; &n = - I /(») sin «a> <to. Fourier Theorem. 

F. Qeometrlc Magnitudes. Mensuration. 

I = length (or perimeter) ; A = area ; V= volume. 



11, Fl 



MENSURATION 



9 



Dimensions ob Equations 



FOBMITXAS 




2. Trapezoid. 



3. Circle. 




Z, OEB = a/2 ; 

/_ OBT^ 90° ; 

ZFBT^a\ 

/, FBO = 90" - a 

^ =Z,FTB\ 



4. Ellipse. «<1. 




g + ||-1, (origin at 0). 

or P = ; — ^ — :;t 
'^ 1 — ecostf 

(pole at F) ; 

Foci, #, -F" ; Center ; 0. 



Sides: a^h^c. Angles: A,B,C. 
Altitude from ^ on a » A^. 

« - (a + 6 + c)/2 ; 

ir = ^ + ^+^=180<»; 

= («-«) tan (J/2) ; 
c = 6 cos J + a cos ^ ; 
<fi =^ a* + 1* - 2 ab cos C. 

h = height. &i, &j = bases. 

■ ■ — ■ ■ ■ ■ ■ ■ I — 

r «> radias ; d = diameter ; 
a = COB at center 

arc CB , ,, s 

= (radians) 

r 

180 arc CB ., 

B= (degrees) ; 

n T 

V2 = CEB, «^ = 2 a = 2>0^; 

sin a =^B -i- r = 1 -i- esc a ; 

cos a = 0F-¥- r = 1 -5- sec a ; 

tan a = 7!S -5- r = 1 -i- ctn a ; 
vers a^FC-i-r = 1 — cos a ; 
ex sec a = CT-i- r = sec a— 1. 






= a + i» + c = 2«; 
^akJ2^hhiJ2^chJ2 

=»(l/2)a&sin C, etc. 

= ra =%/« («-a)(«-&)(«~c); 
sin J sin B sin (7 



tan 



B-C 



b-c , A 
b + c 2 



:4=A(6i + &a)/2. 



I = 2 irr = ird = 2 A/r ; 
^ = wr« = jr<«V4 =- 1 r/2 ; 
arc (TiS :^r»a^ (a in radians) 

= irra/180, (a in degrees); 
Chord DB =» 2 r sin a 

=-2r8in(.^/2); 

Sector ODCB = ^ nr*, (a in 

degrees) ; 
Triangle DOB = r* sin a cos a 

= (l/2)r«sin2a-, 
Segment Di^^C- r« [ira/180 

- (sin 2 a)/2]. 



tan (a/2) ^BF^EF^ si n a/Cl + cos a ) ; 
sin (a/2) = 5F-4- iF^ =V (1 - cos tt)/2 ; 
cos (a/2) ^EF-h-EB = V(l + cos a)/2. 



a, &, semiaxes ; /*, r', radii, 
c = Va2 - Ifi ; 
« s da =- Va2"3^/a, 

(eccentricity); 
p « yt/c = a(l - eV« ; 

a «=■ tan~i { t^ ) = eccentric 

angle ; 

05 = a cos a, y = & sin a ; 

25 . , 25. 

a,»«cos^,y = 68ln — , 

CD «e a sin <^, y => & cos ^ \ 
^ = ir/2 - a. 



r + r' = const. =» 2 a. ^ — waft ; 

aft .05 



«^P-^a 



T~'"'a' 



=» rt J Vl — e»co8»a tf a : 
where cos a = aj/a. 

Arc-ffP= I \— i ~dx 

JO ^ a* — <t« 

= a r Vl-.e«sin»«^<?«^ 
Jo 

(^ s ir/2— a ; sin <^ « oj/a. 



STANDARD FORMULAS 



[II, If 





BTbolft. 


r,r''. ndil; 


r-- 1- -MBit, -2a; 
fi-BMtorOFP-^1oe(2 + «) 


f 


\Y ' 




e 




FukboU. «-l. 
V P— - 

'f M 


iAr^lstusreemm. 
OF-plt-LNH. 
j,i-2p«, (origin at 0); 


ArMOiVPJf-lVa^l/W; 
(Bee raW«, p. W, No. 4« {»). 




v|t ' 




7. Prlem. 


i-htlght. 


T-B.h. 


8 


Pn 


«mOid(SlM 


^.|o»8rl»s8(i™); 
jr-nilddleaecdoD; 
r-uppprb.ae; ft- height. 


(SMiiii«roS(«, iv,G,p. *?.) 



9. Pyramid (.ny 


A-t.tat,t\af»\ 
ft-hrtght. 


r-.i.»A 


10. Biglltcaroulap 
OyUnder. 


ft-liefglit;«-bi^<arM). 





II, F] 



MENSURATION 



11 



Dimensions os Equatiokb 



FOBICITLAB 







, 


11. Bight Circular r » rftdias of base ; 


s = \/r* + A» ; 


Cone. See Fig. 19, p. 76. 

tan a=r/h ; 
cos a=h/8 ; sin a=r/8. 


A = height ; B — base ; 

8 = slant height ; 

a = half vertex angle. 


-4 (curved )= nr \/r* -|- A« =- irr« ; 
^(total)*=irr (« + r); 
F==ir»-iA/8 = J?A/8. 




r = radius lower base ; 
R « radius upper base ; 
h = height; «= slant height. 




12. Frustum of 
Cone. 
^= lower base (area); 
7*= upper base. 


fi = V(y,;-r)« + A«; 
-4. (curved) = ir» (^ + r) ; 
F = irA {R» + Rr + f*)/S. 


13. Sphere. 

(a) Entire Sphere. 


r = radius ; d = diameter ; 
(7= great circle (area). 


^ = 4 irr» - ire«« - 4 C; 
F = 4irr»/8 = ird«/6 
«^.r/8 = 4 0/8. 


(6) Spherical Seg- 
ment. 

Other notations as 
above. 


a — radius of base of seg- 
ment; 
h Bs height of segment. 


a« = A(2r-A); 
/4 = 2 irrA = w (a« -|- A«) ; 
F= irA(8a« + A«)/6 
= irA« (8 r - A)/3. 


(c) Spherical Zone. 


h = height of zone ; 
a^h^ radii of bases. 


^ = 2 irrA ; 

F= irA (8 a« -1- 3 62 + A«)/6. 


id) Spherical Lune. 


a = angle of lune (degrees'^. 


^ = irr«a/90. 


(«) Spherical Tri- 
angle. 

Sides a, ^, y. 
Angles ^, J5, C. 

k = V[8in (« — a) sin (8 - 


E^A + B + C-lSa^; 
S=iA + B+C)/2\ 
« = (a + ^ + y)/2, 

-i8)sln(«-y)1/sln«; 


sin ^ _ sin 5 _ sin <?.. 
sin a sin p sin y ' 
cos a -■ cos jS cos y 

-f-sinjS.siny cos.<l; 


^=: \/ - cos S/lco& (aS - ^) cos {S - B) cos (-S - C)]- 


-H sin jS sin C cos a ; 
tan(^/2)=*/8in(«-a); 
tan (a/2) - JTcos {S- A). 


14. Mlipsoid. 

Semiazes, a, &, c. 


««/a« + y»/2>* + e»/c» = 1. 


r>='4nabc/8. 


16. Paraboloid of 
Bevolution. 


r » radius of base; 
A = height. 


F-irr«A/2 = ir;>A«. 


16. Anchor Bang. 


r«= radius, generating cir- 
cle; 
R = mean radius of ring. 


^-4ir»ftr; 
r^2ir*Rt*. 


v^aJ>+y»± Vr^ - e« = i?. 



[See also Standard Applications of Integration, Tables, IV, H, p. 4S.^ 



12 



STANDARD FORMULAS 



[n,G 



Q. Trigonometric Relations. For Trigonometric Mensuration For- / 
mulas, see II, F, 1, 3, 13 e, p. 9, 

1. Definitions. See also II, F, 3, p. 9, 

sin A = y/r ; cos A = x/r ; tan A = y/z ; 

CSC A = r/y ; 8ecA = r/x ; ctn ^ = r/y ; 

vers A = l — cos A ; exsec -4 = sec -4 — 1. 

2. Special Values^ Signs, etc, for sine, cosine, and tangent. 



Angle 


0«» 

±0 

1 
±0 


80«» 


46'» 


60* 


90- 

1 
±0 

±00 


ISO* 

±0 
-1 
±0 


270" 

-1 

±0 

±00 


860° ±^ 
orO'*±A 


90'*±A 


ISO* ± A 


270* ±^ 


sin 


1/2 


>/2/2 


V3/2 


±sin^ 


+ cos^ 


qpslnul 


— cos^ 


cos 


Vs/2 


V2/2 


1/2 


+ cos^ 


=F8inJl 


— cos J. 


±sinJl 


tan 


Vs/8 


1 


V3 


±t&nA 


TotnA 


d:tan^ 


Tctn Jl 



[± and ± 00 indicate that the function changes sign.] 

3. CSC A = 1/sin A; sec ^ = 1/cos A ; tan A = 1/ctn A. 

4. a;2+y2=,4; cos2^+sin2^=l; l+tan2^=sec2^;ctn2^+l=csc2A 

5. sin (A ±B)= sin AcosB ± cos A sin 5. 

6. cos (A± B)= cos -4 cos .B T sin ^ sin B. 

7. tan(Jl±5) = [tan^± tanJ?]-T-[l T tanJl tanS]. 

8. sin 2 ^ = 2 sin A cos A; sin a = 2 sin (a/2) cos (a/2). 

9. cos 2 ^ = cos2 A — 8in2 ^ = 1 - 2 sin^^ = 2 cos2 Jl — 1 ; 
cos a = cos2 (a/2) — sin2 (a/2) ; see also II, F, 3, p. 9. 

10. sin 3 -4 = 3 sin ^ — 4 sin^ A. 11. cos 3 ^ = 4 cos^ ^ — 3 cos A 

12. tan 2 ^ = 2 tan ^ ^ [1 - tan2 A]. [See also II, F, 3, p. P]. 

13. 2sin^cos-B = sin(^ + 5) + sin(^-5); 

sin a ± sin /3 = 2 sin [(a ± /3)/2] cos [(a ::f /3)/2]. 

14. 2 cos -4 cos 5 = cos (^ - 5) H- cos (A + -B) ; 

cos a + cos /3 = 2 cos [(a + /3)/2] cos [(a - /3)/2]. 

16. 2 sin ^ sin B = cos (A — B)— cos (^ + B) ; 

cos a - cos /3 = - 2 sin [(a + /3)/2] sin [(a - /8)/2]. 



11, H] 



TRIGONOMETRY 



13 



16. sin2 ^ - sin2 B = cos2 J5 - cos? ul - gin (^ + B) sin (A-B), 

17. cos2 A - sin2 B = cos^ B — sin^ ^ = cos (^ + ^) cos (^ - J5). 

18. Definitions of Inverse Trigonometric Functions: 

(a) y = sin-i x = arc sin a; = angle whose sine is x, if a; = sin j^ ; 
usually y is selected in 1st or 4tli quadrant]. 
(6) y = co8"i X = arc cos x, if x = cos y ; [take y in 1st or 2d quadrant], 
(c) y = tan-i x = arc tan x, if x = tan y ; [take y in 1st or 4th quadrant] 



19. sin-i X = t/2 — cos-i x = cos-i VI -x^ = tan-i [x/ Vl - x2] 
= csc-i (1/x) = sec-i[l/ Vn=^ = ctn-i[ vT3^/x]. 



20. cos-i X = ir/2 - sin-i x = sin-i Vl - x^ = tan-i [Vl-xV«] 

= sec-i (1/x) = csc-i [1/ >/ri^] = ctn-i [x/ VH^^]. 



21. tan-i X = ir/2 - ctn-ix = ctn-i (1/x) = sin-i [x/Vl + 2c'^] 



= cos-i [l/Vl + x2] = sec- VI + x2 = csc-i [vT+^/x], 
22. Special values, correct quadrants, etc., for inverse functions. 



Value 


+ 


— 






n/2 




1 

ir/2 


»/4 


-1 


1/2 

ir/6 
n/S 
0.46 


V2/2 


V8/2 


V8/8 


>1 


-Jk 


Bln-lflj 


UtQ 


4th Q 


-ir/2 


ir/4 


,r/8 


0.62 




- sin-l (+ k) 


cos -1 05 


UtQ 


2dQ 


w 


V4 


ir/6 


0.96 




IT — 0O8-l(+A) 


tan-lflj 

1 


UtQ 


4th Q 


-ir/4 

• 


0.62 


0.71 . 


ir/6 


>ir/4 


-tan-l(+*) 



H. H]rpeTbolic Functions. 

1. Definitions. (See figures III, E, J2, pp. 22, SO ; and V, C, p. S4, 
sinh X = («* — c-*)/2 ; cosh x = (c* + e-*)/2 ; 

tanh X = sinh x/cosh x = (e» — e-*)/(e» + e"*) ; 

etnh X = 1/tanh x ; sech x = 1/cosh x ; csch x = 1/sinh x, 

= Gudermannian of x = ^dx = tan-i (sinhx) ; tan = sinh x. 

= tan-i [(e« - c-»)/2] = 2 tan-ie« — ir/2 

2. cosh2 X — sinh2 x = 1. 3. 1 — tanh^ x = sech^ ». 

4. 1 — ctnh^x = csch2x. 

5. sinh (x±y) = sinh x cosh y ^ cosh x sinh y. 



14 STANDARD FORMULAS [II, H 

6. cosh (x±y)= cosh x cosh ^ i: sinh a; sinh y. 

7. y = sinh-^a; = arg sinh x = inverse hyperbolic sine, if as = sinh y 
[Similar inverse forms corresponding to cosh x, tanh x, etc.] 

8. sinh-ix = cosh-i Vx^ + 1 = csch i (1/a;) = log (x + Vx^ + 1). 

9. cosh-i X = sinh-i Vx^ — 1 = sech-^ (1/x) = log (x + Vx^ — 1). 

10. tanh-ix = ctnh-i (1/x) = (1/2) log [(l + x)/(l - x)]. 

11. It 4> = gd Xy sinh x = tan <p, cosh x = ctn 0, tanh x = sin 0. 

I. a. Plane Analytic Oeometry 

[(», y) or (a, 6) denote a point ; (ajj, y^) and (a-a, y,) two points ; etc.] 



1. Distance I = P1P2 = V(X2 - Xi)2 -f {y^ - yi)'^ = Vax^ + Ay^ 

2. Projection of P1P2 on Ox = Ax = X2 — xi = Z cos «, where 

a = Z(Ox, P1P2). 

3. Projection of PiP2 on Oy = Ay = ^2 — 2/i = ^ sin a, 

4. Slope of P1P2 = tan « = (^2 — yO/(^ — asi) = Ay/ Ax. 

5. Division point of P1P2 in ratio r : (xi + r Ax, yi + r Ay). 

6. Equation Ax + By -{-C = 0: straight line, 
(a) y = r?»x + b : slope, w ; y-intercept, b. 

(&) y—yo = m(x — xo): slope, m ; passes through (xo, yo). 

(c) (y-yi)/(y2-yi)=(«—«i)/(x2-xi): passes through (xi,yi), (X2,y2). 

(d) X cosa + ycos/3 =p: distance to origin, p; a^Z{Ox, n) ; 
|3 = Z(Oyy n); n = normal through origin. • 

[General equation Ax + By + C—0 reduces to this on division by \^A* + B*.} 

7. Angle between lines of slopes wi, W2=tan-i [(wi — m2)/(l+mim2)]. 
[Parallel, if mi = 7712 ; perpendicular, if l+?»iW2=0, i.e. if wi = — l/m2.] 

8. Transformation x = x' -^ h, y = y' -{• k. [Translation to (h, *).] 

9. Transformation x = ex', y = ky'. [Increase of scale in ratio c on 
X-axis ; in ratio k on y-axis. ] 

10. Transformation, x = x' cos $ — y' sin 0, y = x' sin ^ + y' cos $, 
[Rotation of axes through angle $.'] 

11. Transformation to polar coordinates (p, B): x =p cos 6, y = p sin $. 
Reverse transformation : p = Vx^ + y^, $ = tan-i (y/x). 



II, J] ANALYTIC GEOMETRY 15 

12. Circle : (x— ay + (y — by = r^; center, (a, b) ; radius, r ; or 
(« — «) = *• cos dy (y — 6) = r sin d. (d variable.) 

13. Parabola : y^ — 2px : vertex at origin ; latus rectum 2 p. 

14. Ellipse : x'^/a^ + yV^ = 1 • ce^iter at origin ; semiaxes, a, b, 
(See n, F, 4, p. 9.) 

15. Hyperbola : x^/a'^ — y^/b^ = 1 ; center at origin ; semiaxes, a, b ; 
asymptotes, x/a ± y/b = 0. See II, F, 5, p. 10. 

(a) If a = 6, x2 — 2^2 _ q2 . retaugular hyperbola. 

(b) xy = k, rectangular hyperbola ; asymptotes : the axes. 

(c) y=(ax-{-b)/{cx-{-d), rectangular hyperbola ; asymptotes: x=z^d/c, 
y = a/c, 

16. Parabolic Curves: y = ao + a\X + a2X^ + ••• H- an«* 
[Graph of polynomial ; see also Figs. A, B, pp. 19 ^ 20,'] 

17. Lagrange Interpolation Formula. Qiven y = /(x)^ the poly- 
nomial approximation of degree n — 1 [parabolic curv'^e through n points, 
(«i, yi), (X2,y2)y •-, (a?„, 2/J] is 

y = r(Qc) = ViP^ix) + y.^p^{x) + ... + VnPni^), 

where the polynomials pi(x), i?2(^)» •••» Pn(jx) are 

n,(a;) = -X*-"" ^i)(^_":.^2V- (a; - y<-i)(a; - a^f+i) ••- (a; - gn) 

(X< - Xi){Xi -X2)'" {Xi - Xi-\){Xi - Xi+{) -"{Xi-Xn) 

[Numerator skips (« — aj^) ; denominator skips (x< — Xi). Proof by 
direct check.] 

[For a variety of other curves, see Tables^ III, pp. 19-34. ] 

I. b. Solid Analytic Geometry. 

[(x, y, z) denotes a point ; (xi, y^ Zi) and (X2, Vi, 22) two points, etc. 
O denotes the origin, (0, 0, 0).] 

1. Distance : P1P2 = V(X2 - Xi)2 + (2/2 - 2/1)2 ^ (^^ _ zi)2. 

2. Distance from the origin : OP = Vx^ + y2 ^ 22. 

3. Direction cosines of a line L : cos a, cos/3, cos 7, if a, /3, 7 denote 
the angles L makes with the x, y, z axes, respectively ; and we have 

cos^a + cos2j8 + COS27 = 1. 

4. Direction cosines proportional to given numbers : 

If a: b : c = cos a : cos/3 : cos 7, .and B^ = a'^ -\- b^ -\- c^, then 
Qosa = a/JB, cos/3 = &/JB, cos 7 = c/i2. 



16 



STANDARD FORMULAS 



[11, 1 



6. Angle B between lines L and U with direction cosines (Z, m, n) and 

(r, m', n') : 

cos^ = IV + mm' + nn'. 

JAnes parallel if W + mm' -\- nn' = 1, or if i = i', m = m', n = n'. 
• Lines perpendicular if W + mm' = nn' = 0. 

6. Direction cosines of a plane P = direction cosines of any line 
perpendicular to P. 

7. Equation of a plane P : 

te + my + nz = p, or x cos a + y cos /3 + « C0S7 = p, 

where (Z, m, n) are the direction cosines of P, and p is the length of the 
perpendicular from to P. 

8. General equation of a plane : Ax + J5y + C« + D = 0. 

If 122 = ^2 4. ^ ^. C2, i = cosa = A/R, m = B/B, n= C/E, p^-B/B, 

9. Plane with intercepts a, 6, c, on the axes : 

x/a + 2//6 + z/c = 1. 

10. Plane determined by {xu Vi, ^i)? i^, 1/2, 2^2), (acj, ys» zi): 

X y z 1 

»i yi 2i 1 

X2 2/2 ^2 1 
353 2/3 23 1 

11. Angle $ between two planes (I, m, n ; p), (I, m, n ; p); 

cos $ = 11' -{- mm' + nn'. 

12. Angle ^ between planes Ax -\- By + C« -f D = and 

A'x + 2?'y + C'« + D' = ; 

cos e = ^^'H-P^^+ CC 2J2 = ^2 4. ^ 4. (72 R/2 = ^'2 + J5/2 + 0'« 

BB' . .' T T , , 

Planes paraHeZ if W + mm' + nn' = 1, or if ^ = A', B= B', C = C 
Planes petpendicuiar if A A' + 55' + CC = 0. 

13. Distance d from point (xi, yi, «i) to plane (i, m, n ; p): 

d = 1x1 + fny\ + W2i — p. 

14. Distance d from (xi, yi, 2i) to -4x + 5y + Cz + D = : 
^^Aci + 5y^+C2i + i) 222 = ^2 + ^2+02. 

15. Direction cosines (2, m, n) of a line determined by two planes 
^ + 5y + Cz + D = 0, A'x-\- B'y + C'z + D' = ; 



= 



limine 



B 


C 


• 


c 


A 


• 


A 


B 


B' 




• 


c 


A' 


• 


A' 


& 



see 4. 



n,Ji 



ANALYTIC GEOMETRY 



17 



16. Line through (xu Vu 2i) and (0521 y2i 22) • 

x — xi __ y — yi _ z^Zi ^ 
X2 - xi 2/2 - 2/1 22 — Zl 

17. Line through (xo, yoi 2©) in direction (i, m, n): 

18. Line through (xo, yo» 20) perpendicular to plane Ax-{- By -\-Cz^O: 

x — xq __ y — vo _, z — zq 
A B C ' 

19. Plane through (Xi, 2/1, Zi) perpendicular to line of fonnula 17 : 

A(x-Xi) + B(^y^ yi) + C (2 - 2i) = 0. 

20. Sphere of center (a, 6, c) and radius r : 

(X - ay + (y- 6)2 + (2 — c)2 = r«. 

21. Cones with vertex at : 

352 t/2 22 

a* 6* c2 

Imaginary J if all signs are alike ; otherwise real, and sections parallel to 
one of the reference planes are ellipses. 

22. Ellipsoids and hyperboloids with centers at O (see Tables III 

Signs on left : 

All + : ellipsoid 

One — : hyperboloid of one sheet 

Two — 

All - 

23. Paraboloids on z-axis with vertices at (see Tables III N4, 5) : 

Signs on left : 
< Alike : elliptic paraboloid 

Different : hyperbolic paraboloid 

24.. Contour lines on curved surface F(x, y, z)=0: 

Sections by z = a are F(x, y, a) = 0. 

25. Curves in space : 
(a) Intersection of two surfaces : Fi(x, y, 2)= 0, 1^2 (x, y, 2) = 0. 
(6) Solve for y and z : y =/(x), z = 0(x). 
(c) Parameter forms : x =/(0» y = 0(O» 2 = ^(Q. 

26. General cylinder with elements parallel to z-axis : /(x, y) = 0. 



X* . 2/2 . 2* 



hyperboloid of two sheets 
surface imaginary 



. x2 . 2/2 
o2 62 



18 STANDARD FORMULAS [11, J 

J. Diflerential Formulas. 

1.1/= /(x) : dy =/'(x) dc, f'(x) = dy -^ dx = dy/dx. 

2. r(x, 2/) = : F^dx + Fydy = 0, or dy = _[F, ^ F^jcte. 

3. x=f(t), y = i>(t): 

{a) dx = f (t) dt, dy = <p'(t)dt, dy/dx = <pf{t) -i-f^Ct). 

(6) d:hf/dx;^ = dldy/dxydx = dl<p' -^fydx = [0"/' -/"0'] -5- (/')«. 

(c) d8y/d:i^3 = j[^2^/da;-^]/tZx = d[(0"/' -/"0') -^ (/')^]M -/'• 

4. Transformation x = /(f) : y = 0(ic) becomes y = 0(/(O) = ^ CO* 

(a) dy/dx becomes dy/df -^/'(O »' C^^® ^ C^)]- 

(6) <r^/eix2 becomes [(c?V<^«^) '/'(O - (<^yM)/"(0] -*■ [/'(O]'; 
[see 3 (6)]. 

5. Transformation ic=f(tjU), y = ^(tfU): y = F(x) becomes 

w = *(0. 

(a) dy/dx becomes ^^^ or rM+?^ . ^"1 ^ fV+^t . ^l^ 

d« dt Idt du dtj Idt du dtj 

(6) d?y/dx'^ becomes d[dy/dx]/dt -f- dx/dt ; [compute as in 6 (a)]. 

6. Polar Transformation x = p cos ^, y = p sin ^ . 

dx = cos ^ dp — p sin ^ d^ ; d^/ = sin ddp + p cos ^ d^, 
d^x = cos 0d^p — 2 sin ddpdd — p cos ^ df^, 
(?V = sin ^d^p + 2 cos ^ dp d^ — p sin ^d^-i. 

. 7. z = F*(i€,y): dz = F^dx-\-Fj,dy=pdx + qdy; [see I, 3(d), 
p. £], 

8. Transformation x =f(u, v), y = (p(u, v) : z = F(x, y) = *(u, »). 

5w 5x Sm 5y du ' 5v 5x 5v dy dv ' 

dx du dv dy du dv 

lA, B, C, D found by solving 8 (a) for dz/dx and dz/dy.^ 

(c)^ = Af^\=Af^j?£+5?£^ 

^ "^ dx^ dx\dxj dx\ du dvl 

= A^(a^-^ + B^^] + B ^ (a^-^+ B^\. 
du \ du dvj dv\ du dv) 

[Similar expressions for d'^z/dy^ and higher derivatives.] 



STANDARD CURVES 

A Gnrves y — x" all pass through (1 1) - positive powers also through 
(0 0) nega, e powers asj mp otic to the y sjcie Spec al cases 1 




20 STANDARD CURVES ' [1 

are ■tralgbt litieB ; h = 2, 1/2 are ordinary paiabolaa ; n = — 1 
ordinary hyperbola ; n = 3/2, 2/3 are Boml-oabical parabolas. 



B. Logaritbinlo Paper ; Carves y = x", y = kx'*. Logarithmic 
paper is need cliiefly in experimentai deUrmtnation of the eonstanU k and 
n ; and for graphical tables. In Fig. B, k=l except where given. 




[See |lS9,p.334, »1>iitb; *]90 TiniMin-HB»n, ffjrfrouHo T^iblet; Trmtirine, Xa- 
gtn6eri' Handboi^k; D'Ocagne, Somoeraphit.\ Tbellnsy — »— Igiiee tbe rtcipnteak 
r/ 7in7itf'era by ilircct readlngB. 



Ill, Dl 



ELEMENTARY FUNCTIONS 



C. Trlgouometrlo Fnnctiona. The invDrHe tiigonometric innc- 
tions are given by reading y fitst. 




2.303 logi«x. The values of the expo- 
= e" are given bj reading y first. See E. 



i 


'P"-' \"'-\ 
















1 ■ U_--- ^---T~1 


-'■ Li'.'B 


rrDjius 












i. 








--■li- 


:::r|.:: 






- 


' 








- '- - ■ ^ 






^ljr"_ 












i 


//'■' 






: '"'r—A 




















•^ ■ -:- 


















i'i'ii' "^■■■M. ,i,-i..-h-riJ.-4lii^i| 



22 



STANDARD CURVES 



[III, I 



B. BzponentSal and Hyperbolic Functlona. Tbe catenaiy 

(hyperbolic cosine) [?/ = cosh i = (e* + e— )/2] and the bjrperbolic 
•Ine [y =sinha5= (e*— e-')/2] are ahown in their relation to the ei- 
pODBiitial curve* i; =e; y - e"'. Notice that both hyperbolic cnrrea 
are SHymptotic to y = e'/2. 




' is the standard damping ci 



ni, PI 



HARMONIC CURVES 



F. Haimonlc Curvea. The general type of Bimpls haimonlo Oiuv* 

is y = a sin (^kx + 1): 



».,. 


«■!■ (!« + () 


■IBZ 


O.. 


■■■a« 


(i/2)«iBCe»- 


..J 


Binplltuds 


■ a 


1 


1 


1 


1/2 




S>/* 




2ir 


w 


Jr/a 




-,/k 


• 


«/2 





o-i 



A eompoand taEumonlo cnrvs is lonned by superpoaiag aimple hur 
monies : In Fig. i\, j = Bin 2 a; + (1/2) sin (Bx- 1.2) ia drawn. 









A 






= ..n 


21 

,(Cr- 


1J2) 




r 








// 




K^ 


... 


^H' 


n{Or- 


"' 


/ 


\ 


/ 


\ 


f 




r^ 


\ 




V' 


' 




V 


A. 




^ 


A 


/ 


\\ 




\ 






y. 










y 


v/ 


^ 


1 




V. 


^ 










^ 


A 









Id theorids of rlbnUons, gonnd, elKtrleltf. 



24 



STANDARD CURVES 



The Bimplciit type of damped vlbtatloiia U 

Bhowa y — e-''*sin 3 r The general form iey—c 
damped simp e Tib a odb may be auperposed o 
damped v bratioua. 



[Ill, P 

< = «-" sin kx : Fig, Fj 
-"sin (to + Such 
. otber damped or im- 




O. The RoulettM. 

A roulette is the path of any point rigidly connected with a moving 
curve which rolls without slipping on another (fixed) curve. 
TbeCTcMd 




Figure Gi shows the ordinary cycloid, a roulette formed by a point 
P on the rim of a wheel of radius a, which rolls on a straight line OK 
See also Fig. 30, p. 144. The equations are 



jfherefl = ^ifCP 



Ill, GJ 



ROULETTES 



25 



Figure G2 shows the curves traced by a point on a spoke of the 

wheel of Fig. H, or the spoke produced. These are called trochoids ; 

their equations are 

x = ad—h sin^, 

y =z a — h cos 0^ 




Fig. G» 



Xhe Tieclioids 



where h is the distance PC, If & > a, the curve is called an epitrochoidi 
if 5 < a, a hypotrochoid. 



Figure G3 shows the epicycloid ; 

x = (a + 6) cos ^ — 5 cos 



[^'] 



y]= (a + 5) sin <? - 6 sin f^Ll^ $], 





e 




Fig. Gj 



formed by a point on the circumference of a circle of radius b rolling on 
the exterior of a circle of radius a. 



26 



STANDARD CURVES 



[III.G 



y}^ 


^ 


f c 




r 


V ^ 


y 


v^ 



Fio. G4 

Figure Gg shows the hypocycloid : 

« = (a - 6) cos^ + 6 cos ["^^^^ ^"j, 
y = (a _ 6) sin ^ - 6 sin T^i^ <?1, 



formed by a point on the circumference 
of a circle of radius 6 rolling on the 
interior of a circle of radius a. 

Hypocycloid 



Figure G4 shows the special epicycloid, a = 6, 



x — 2a cos $ — a cos 2 0, 
y = 2 a sin ^ — a sin 2 ^, 



which is called the cardloid ; its equation in 
polar coordinates (p, <p) with pole at (^ is 
p = 2a(l — COS0). 





Fig. G4 

Figure Ge shows the special hypocycloid, a = 4 6, 
x = a cos^ 0, 



1 



y = a sin8 0, 



or a;2^ + y2/8 = aa/«, 



Fig. G« 



which is called the four-cusped hypocycloid, 01 
astroid. 



H. The Tractrlz. This 
curve is the path of a particle 
P drawn by a cord PQ of fixed 
length a attached to a point 
Q which moves along the 
X-axis from to ± 00. Its 
equation is 





V 












^ 


Vp 


The Tractrix. 




^ 


^ a 


V 

X 


V 


X-:;__ 


k 











Q 


X 



FiQ. H 



x = alog^ + ^^'^y'^v^^^-3jr2. 



y 



in, I] 



CUBICS— CONTOUR LINES 



27 



I. Cubic and Quartic Curves. 

Figure Ii shows the contour lines of the surface z = ofi — ^x — y'^ cut 
out by the planes z = k^ for &=— 6, —4, —2, 0, 2, 4; that is, the 
cubic curves x^'~Zx — y'^ = k, 

• 

The surfiMse has a maximum at (»« — 1, ^ — 0; the point (e = 1, ^ « is also a critical 
point, but the surface cuts through its tangent plane there, along the curve ik = — 2 ; 
y« = a5» - 8 a; + 2. , 

These curves are drawn by means of the auxiliary curve ^'=3'*— 3», itself a type of cubic 
curve ; then y =y/q — k. is readily computed. 





Fig. Ii 



Fig. t 



Figure I2 shows the contour lines of the surface 2J=a8— 3 a;+2^« («— 4) 
for « = A; = — 6, — 4, — 2, 0, 2, 4 ; that is, the cubic curves 



y2=(ic«-3x-A:)/(4 - x). 

The Burfl&ce has a maximum at (- 1, 0). At (1, 0) the horizontal tangent plane « — -2 
cuts the surface in the strophoid y«= (a5« - 8cb -f 2)/(4 - oj) whose equation with the 
rew origin C>' is y» = a?'* (3 + aj') /(3 _ a;'). The line tp « 4 is an asymptote for each of the 
curves. 



28 



STANDARD CUftVES 



[m,i 




Figure I3 shows anothei cubic : the cissoid, 
famous for its use in the ancient problem oi 
the ** duplication of the cube/' Its equation is 



y2 = 



ofi 



2a — a; * 



or p = 2atan(^ sin^. 



It can be drawn by using an anxiliaiy carve as above ; 
or bj means of its geometric definition : OP — QB^ when 
Oy and AB are vertical tangents to the circle OQA, 



Figure I4 shows the conchoid of Nicomedes, used by the ancients in 
the problem of trisection of an angle. Its equation is 



= -a?a + 



-^ — ) , or p = a sec ^ :t 5. 
X — a/ 



FlQ. I4 



Condhohl 





Follmn 

of 
Descartes 



Fig. h 



Figure Ig shows the cubic «* + j^ — 3 axy = 0, called the Folium 
of Descartes ; see Example, p. 45. 



The ^ 
Witch ^^ 


2a ^'•«-..^,,^ 


*^"i«+4a« 


*- 





^ 

X 



Fio. Is 

Figure le shows the witch of Agnesi : y = S aV(x2 + 4 a*) ; see Ezs. 
I, 36, p. 131 J 62, p. 162 ; and see III, J, below. 



QUARTICS— CONTOUR LINES 



Figure It shows the CaBmlnlan ovals, defiaed geometrically by the 
equation FF • FFi = i* ; or by the qnartic equation, 



o)« + j/'][Ca; + a)'4-y'] = H 



where a = OF (= I in Fig. I;). The special oval Ifi = o? Is called the 
leminlKato, (i^ + y*)= = 2 a" (2= - y') or ^^ = 2 «« cos 2 S. 




which has minima at (2 = ±a, y = 0), and a critical point with r 



STANDARD CURVES 



J. Error or Probability Cmvaa. 

Figure Ji is the so-called oorve ot error, or probability ci 




where ft is i 

of precision. See Tables. 

IV, H, 148, p. SO ; and V, 



y = seeta x = 2/(e' + e-) 
In some instances thiscurve, or the witch (Fig. I«), maybeusedinplac 
ot Fig. J]. Any of 
these curves, on a 
proper scale, give 
good approzimatioiiB 
to the probable dis- 
tribution of any ac- 
cldeotal data which 
t«nd to group tLem- 
selves about a mean. Fiu. Ji 

K. PolyTtoinial Appro^mationa. 

Figure K], shows the first Taylor polynomial approxiniatloiui to tha 
CuncUoii y = sin X. (See § 147, p. 2 





APPROXIMATION CURVES 



Figure K3 shows the Slmpaon-LagreuiBe approzlmatlotU) : (1) bj 
i broken line ; (2) b; an ordinarj parabola ; (3) by a cubic, wbicb 



However degenerates 
into a parabola in this 
example. (Lagrange 
iDtcrpolation For- 
mula, Ta6(M, p. 15.) 



'^''SS^SSi 



s 



11V1.1™ point, ^ uk.n - ffil TTiTrfm-f fflTf fFf^hH ^ 

jloher together thu ■■ H4+i-|-rT I |-|4+|-T I H"|- H+|-H->+ i M-f: :44-|-hH+ 



Fio. Ki 

3*- 1.2I3» - .405ir', O^bSit. 



.it/3.w,-Sir/3,B,-i. 



L. Trlgonomettlo ApprozlniBtiaiia. 























(1) 






















.4 


/ 








^ 


\\ 


C 




, 


E'ou 


ler 


APP 


lex 


Q«tl 




// 








A 


A 


1 




1 


JU 


... 


^ 




«<0 




r 








\ 


j 




I 


/(' 


). 


'/2 


\ 


<TJ 




^ 








< 




'1 






- 


f^ 













% 




T 




} 


\ 












li 


Ap^ 


™ 


Hii 

mat 


Z" 






\ 








uy 


//(» 


1 " 


J, =2. tor 








D 


^S. 








•■H 




./; 


>-'-""i ■»•"*•"* 












i-i 




1 1 1 1 1 1 1 



Fio. L 

Fignre L shows the approximation to the two detached llne-eegmenls 

r = -x/2, (~x<ar<0),y = ir/2, (0<i<») by means ot an eipres- 

flon of the form a, + ai sin le + og siu 2 x + — + a, sin nx. See TI, E, 28. 



STANDAKD CUKVES 




\ 




ao- /60* 


i^ 


/l90" 


^S^ 




' \ 
\ 


t 


Arehlmei 


MtnBjrtraK 


\>- 


'^ 


/ ,. 


off ^ 


>/'\ 


/ 


^^ 


,^ 


\ 



m, N] SPIRALS — QUADfilC SURFACES 

U. SplralB. 




Tignies M: and Mg represent the Archimedean Spiral p = aS, and the 
Hyparbollo Spiral p$ = a, respectivety. 

Jl. Quadtic StuiaoeB. 

These are standard figures of the nsnal equatioDS. 

HTporiralatd of ons Sheat 




34 



STANDARD INTEGRALS 



[in,N 



Hyperboloid of two Sheets 








i=0O 




>h 






V7 
if 






I 



M 






V 



V 

/ 



.*Vx' 



Fig. Nt 



Elliptic Fftraboloid 







TlO. ^« 



z 
a 



Hjrperbolic Paraboloid 




TABLE IV 

STANDARD INTEGRALS 
Index ; 

A. Fundamental General Formulas, p. S5, 

B. Integrand — Rational Algebraic, p. 36 

C. Integrand Irrational, p. S9. 

(a) Linear radical r = Vaag -h 6, p . S9, 
(6) Quadratic radical V± x^ ^ ^2^ p, jp, 

D. Binomial Differentials — Reduction Formulas, o. ^1. 

is. Integrand Transcendental, p. 41. 

(a) Trigonometric, p. 41, 

(6) Trigonometric — Algebraic, p. 44- 

(c) Jnverse Trigonometric, p. 4^- 

(d) Exponential and Logarithmic, p. 45. 

F. Important Definite Integrals, p. ^6. 

G. Approximation Formulas, p. ^7. 
H. Standard Applications, p. 48. 

A. Fundamental General Formulas. 

•■ • It ^— = -r— , then w = t; + constant. [Fondanaental Theorem*. 

2. If I t« dX = I, then -^ = w. [General Check.! 

•^ da? 

3. \cudx = c\udoc. 

4. \[u + v'\dx=(udx^-(vdx. 

6. \UdV = UV—lvdU, {Parts. J 

8. r f /(u) dwl = f /[^(a5)] ^^ cfaj. :SubgtltotIon.J 

35 



36 . STANDARD INTEGRALS [IV, B 

B. Integrand — Rational Algebraic. 

7. \x^dx = — , n=7t-l, see 8. 

•^ n+l 

Notes, (a) /(Any Polynomial) das, — use 8, 4, 7. 

(b) /(Product of Two Polynomials) (to, -~ expand, then use SfA,t» 

(c) /ctto — 00, by 8, 7. 

8. f ^ = loge 05 = (logio a;)aog. 10) = (2.302685) logio x. 

Notes, (a) /(l/a5'")(fa5, — use 7 withn — - wi if m=^l ; useSif m — 1, 
(6) / [(Any Polynomial)/*"*] dx^ — use short division, then 7 and &• 

9. f-^=larctaii^ = ltan-i^ = lcte-i^ 

1 cr 

= — — Ctn-l— [+ const.]. 

a a 

L f_J^= _L log ^I^ = JL log «^=^[+ const.]. 

Note. All rational functions are integrated by reductions to 7, 8, 9. The redoe* 
tions are performed by 8, 4, 6. No. 10 and all that follow are results of this process. 

11. ((ax + b)^dx = 1 (<^^ + ^)"'^\ n^-1. (See No. 12.) [From 7.1 
J a n + 1 



12. f — ^ — = llog(ax + b), [From 8.1 
J (oic + 6) a 

Notes, (a) { "^ dx, — use long division, then 7 and 12. 



fX + b 



^ j^ |. Any Polynomial ^^^ _ ^^^ j^^^ division, then 7 and 12. 
J ax-\-b 

13. rr-^7T- = -7 .x7^ vx i >(^=?fcl)' [From 11.1 

JCox + fe)"* a (m-l)(ax+6)'"-^ -^ / l j 

14. fy-^^r-r = -^r— TT + l^S (aa + 6)1 • [From 11, 12.] 

Notes, (a) f "*" dx, — combine A times No. 14 and B times No. 18, m = 2. 
' (aa5 + b)* 

^j^ J. (Any Polynomial) ^^^j^^ i^ng division, then 7 and 14 (a); oP use 16 
J (ow + &)■ 



IV, B] RATIONAL ALGEBRAIC 37 

16. r f-^C*, ax + b) dxl = " f -^ ("— » A ^u, [From 6.] 

Notes, (a) BestaUment : put t* for ace + 6, 2LZL_ for 05,-^ for dx. 

a a 

(5) lWiax + mdx,-nsel6. ^«,.1[-1 + -1^]^^^. 
(^j f (Any Polynomial) ^ _ use 16 ; then 8 (6). 

^^j J. (Any Polynomial) ^^^^ __ ^^^ jg ^^^^^ m <8, ; but see 12 (ft), 14 (ft). 

J (005 + ft)»» 
(e) Jaj»(aaj + ft)"»<to, — use 16 if >n > «; use 7 (6) if wi<n ; see also 61-64. 

16. ? =— i — r-« ^— 1 

(aa? + ft) (ca? + d) ad — be Laoc + 6 ex + dj 

NoTBS. (a) f ^^ , — use 16, then 12. Special cases, — see 10 and 16 (6> 

-»(aa5 + b)(fix + d) 

(M r ^« ^-ff- ^^Id*. (Special case of 16 (o).) 

Ma.(aa, + 6) ftJ Laj f/a--i-ftJ *^ 

(c) r Ax + B <faj-. use 16, then long division, 12. 

^^^ f (Any Polynomial) ^^ ^^^^ jg^ ^^^ 1^^^ division, 7, 12. 
-» (aa5 + ft)(ca5 + tf) 

(«) If a£{ - ftc — 0, 18 can be used. 

17. l(Fix,ax + l»dxl ^=liF(-^, -^).^^. 
L^ J*^^^ -^ \w — a w — a/ (tt — a)* 

NoTss. (a^ Beatatsment: 

Put t* for ^1^+^; -^^for«; -^1*- for a« + ft ; -^^. forcto. 
flj t* - a «- a (t* - a)> ^ 

(jx r dx 1_ |. (u-a)"*+n-2 ^^ ^ ^^^ ^^^ g ^ 

•' «B«(aa5 + 6)"» jm+n-lJ i*"» 

/ -v f dx ^ « — g log t» .,v f dx ^ «« — 4 am- 2a«logt» . 
^^^ J «B*(aa5 + 6) " ft« * ^ ^ •'a5«(aaj + ft)'" 2ft« 

18. f— ^_ = JLtan-i«\/^,if a>0, 6>0. [See 9.] 
J ax^ + b y/ab ^ ft 

= 1 log^^"^^^,ifg>0, 6<0. [See 10.] 

N«™- («)J;i^,-usel8(2ndpart);6 — c. (ft)J-^ — 1^^. 



38 STANDARD INTEGRALS [IV, B 

19- f-^l^ = :^ log («a;2 + 6). 
J ax^ + b 2 a 

NOTB8. (a) J , — use loDg division, then 18. 

(ft) fil^iL^ da), — use 18, 19. 

. , . r(-A-ny Polynomial) , 

(c) J aa^ + ft ^05, — use long division, then 18, 19. 

20. 1 = 1 r m'^ _ mx — n n ^ 

^^""- ^^^ hmx + nnaa^ + b) ^'"^ -^*« ^0. then 12, 18, 19. 

(&) ^<g«-l--Bia;-K7 _A 1 . -» ^ , /^ ^ft^»\ 1 

(tmc + w)(oa5« + 6)^amaj + n maa5» + 6\ a m) (mx+n)(cM*+b) ' 

, . - Any Polynomial _ . ,. . . , , ^ 

^^^ J (n»fl; + 7i)(q<p« + fr) '^'*'' ~ "*® ^^"^ division, then 20 6, 12. 18, 20 a. 

21. a«2 + 6a; + c = araJ + -^T-^i=-l«^. 

L 2aJ 4a 

(c) J ^^^^^^Tg^ ^'^» — ^<>"8^ division, then 7, 21, 21 &, 18, and 19. 

/.,v r Any Polynomial , 

K"') J — Any Cubic — ' ~ ^°^ division, then find one real &ctor of cubic, then use 

81, 21 ft. [If the cubic has a double factor, set u = that ikctor, then use 17 c] 

22 f ^^ 1 1 

J (0x2 + 6)2 2aaic2 + 6' 



23 f ^^ — ^ ■ 1 r da; ., ,j> 

* J (ax2 + 6)2 2 6(ax2 + 6)'^26Jaa;2 + 6' ^''®'' ^^• 

^' L-f^ = r^ f-l > tl^«^ 7 or 8. 

25. f ^ =_- i g_ ■ 2m-8 r (fo; 

J (ax^+b)^ 2 6(w-l) (ax2 + 6)«»-i "^ 2(m - 1)6 J {ax^+b)'^-i 

Notes, (a) Use 25 repeatedly to reach 23 and thence 18. 

(6) Final forms in partial firaction reduction are of types 12, 24, 26 (by use of 21) 



IV. C] IRRATIONAL ALGEBRAIC 39 



C. (a) Integrand Irrational : involving r — Vox + h. 

26. r {Fix, y/ax + h) dx\ ^ ' =z i F (^"-^ ^ r]"^ dr. * 

27. i Vaac + 6cte= \t— dT = -—i*^ r = Vax + 6. 
•7 J a 3a 

28. J.V5^T5d. = AJ(r*-5^)dr = ^[5-|]. 

29. f ^ =gfdr = gr. 

30. r ^_ = f-M?L;use9orlO. 

-^xy/ax+b -^r^-^ 

31. f ^^- = 2 a f /^ ^ ; use 23. 

Note, ^/ax + 6 = (ooj + b)/Vax + ^ ; (Vaa5 + 6)« - (flO) + 6) V</a + b. 



(b) Integrand Irrational : involving V±x^ ± a'^. 

32. f-=_^_=:zz = arc8in-=sin-i^=-cos-i-+ [const.]- 

33. f _ -<^ap ^ ^ logCa? + >/i2±a2) = sinhi^ [+ const.] for +, 

or cosh~i - [+ const.] for — . 
a 

34. f ^^ = sin-i f ?^l^^ = - cos-i ^-^I^-^ [ + const.] 

= vers-^ (x/a) + const. 



f — ^ = Isec-i^ = -cos-ig =- Icac-ig r+ const.]. 

•7 '*'. •v/'Ka _ /,2 a a a jc a a 



35 



36 f ^^^ =-v^g^«. 38. fa;V^^^dx=::^(>/S2:=^2)8. 
• J \/a2-x2 -^ 3 

37. f /^^^ =Vx2 4-qa. 39. fa Va2 + a^da; = J {y/x^ + a2)^ 

Notes, (a) 82 and 88 Airnlsh the basis for all which follow. 

{V) 86, 87, 88, 89 follow from xdx^di9^ + const.) /2. 



40 STANDARD INTEGRALS [IV, C 

40. f_^^=-?V523:T3 + «?8in-i?. 



41. f ^^ =.llogp + ^^^^^^1. 
•^a;Va2±«2 a L a; J 

42. f ^^ =--I,Va2^xg. 

43. (a) I Va2-a;2(fa=?Va«-««+ — 8in-i^. 

•^ 2 2 a 

(6) (^^^^i^dx = V5n:F2 - a log « +^^:^. 

^ X X 

•^ x2 X a 

44 f g^^ =^Vg«4- a«T^logrx + Va^rfca«). 
•^ Vx2 ± a2 2 2 



46. f dx ^^V^2^a2^ 

46. (a) f Vx2 ± a2dx = ? Vx? ± a^ ± ^ log (x + Vx2 ± o^). 

(6) r Vx2 j:aa ^ ^ Vx2 ± a2 ± a^ C — ^ then 35 or 41. 

^ « J a; Vx2 ± a2 



(c) fvgZgdx = -^'^^^^Vf-^^^,theD32or38. 
^ x2 X ^ Vx2 ± a2 

. f /^ = ? 48. f 

•^ f Vo2 - x2^» a2 Va2 - x2 -^ 



dx _ ±« 



( Vo2 - x2)» a2 Va2 — x2 •^(Vx2ia2)» a« Vx» db a* 

NoTKS. 7V*t0ronofn0^ic Subsiitutiona. If the desired form is not found in 82-^, try 
79. Then use Nos. 65-79, see 79. {h) See also D 51-54, below. 

49. V±(ax2 + 6x + c) = Va V±w2 ± A?, where 

u = x + Aandfc2 = &i=l«£. 
2a 4a2 



IV, E] REDUCTION FORMULAS 41 



50 -x l^^ "^ ^ = , ax + b y/(ax + b)icx-{-d) ^ 

^cx + d"" V(aa; + 6)(ca; + d) .cx + d 

NoTBS. (a) Integrals containing V{ax + b)/{cx + d) : use 50, then 49, then 82-48. 

(5) Sabstttntion of u B'\/(ax + b)/(cx + d) is successftd without 50, 

D. Integrals of Binomial Differentials — Reduction Formulas. 

Symbols : u = ax* + b; a, 6, p, m, n, any numbers for which no de. 
nominator in the formula vanishes. 

51. (x^(ax^-\-h)Pdx= [7^-^Hp-{-npb xx^u^-^dx]. 

J m-\- np -\-l J 

= ^ [— ic«+iwi'+i 4- (m + TO + np + 1) (x^uP-^^ doc], 

bn(p + 1) J 

53. (af^{ax:^ + b)Pdx 

= = [a:«+iwP+i — a(m -{■ n + np + 1) \ x'^-^^uP doc]. 

{m-{-\)b J 

54. (x^{ax^ + h)P dx 

a(m + wp + 1) J 

Notes, (a) These reduotion form.ula8 useflil when p, m, or n are firaotiotial ; 
hence applications to Irrational Integrands. 

(6) Bepeated application may reduce to one of 82-48. 

(o) Do not apply if p, m, n, are all integral, unless n ^2 andp large. Note 11, 15, 17-2£^ 

Ea. Integrand Transcendental : Trigonometric Functions. 

55. Isin X dx = — cos a?. 

56. ( sin2 xdx=i—\ cos a; sin x + J » = — J sin 2 a; + J a;. 

Note. / sin* fepcfoj, — set kx =» m, and use 56. Likewise in 55-78. 

67. Uwzdx = - «'""-' '^oo^^ + a^il f gjp^a x(fa... 

Note. If » is odd, put sin« aj = 1 — cos« x and use 62. 



42 STANDARD INTEGRALS [IV, g 

58. Ccos X dx = sin x* 

6Q. ( coB^xdx = i sin xcos x + i ^ = i sin 2 x + |x. 

60. fco8»ic<te = 52«n£«nf + «nlfco8»-Sxd«. 
J n n J 

NoTB. If n is odd, put co8*(0 >■ 1 — 8in*fl9 and use 63. 

61. Isin xcosxdx=— i cos 2x = i sin^ a; [ .+ const.]. 

62. f8ina;cos»a:dx=-^^?^,n:?fc-l. 
J n + 1 

63. rsin»xcosa;dx = ^^^^^ — -,71=^—1. 
J n+1 

64. f sin" X cos- X cte = sin-+i x cos >»-i x ^ m-^1 T .^, ^ ^^^^.^ ^ ^^ 
J m + n TO + n./ 

— sin*-* X C0S"»+1X , W — 1 r„:„n-2« «A.ei»/^y7^ 

= 1 I sin*^^ X cos"* xox. 

w + n TO+ n J 

NoTK. If n is an odd Integer, set sin* a; « 1 — cos> ce and use 62. If m is odd, use 63. 

i»e C ' f \ / \j cosr(m4-n)xl cosfCm — n)x] 

66. i sin (mx) cos (nx) dx = ^^ — -^^ — -^ ;r^ r-^» 

J ^ ' ^ ^ 2(w + n) 2(m - n) 

wi T^ db «« 

66. rsin(mx)sin(nx)dx = ^^"i:(^"^)^] -- '^^"J/'^+^^^^^ 
J ^ ^ ^ ; 2(m-n) 2(w + n) 

67. rcos(mx)cos(nx)dx= »^"C(^^ ^>^3 + "^°£<"* + ")^3 , m:^±»». 

68. I tanx(Zx=— logcosx. 69. ftan2xdx = tanx — x. 

70. ('tan»xdx = ^^"**~^ ^ - f Un*-2xdx. 
J n — 1 J 

71. fctnxdx = logsinx. 72. J ctn«x(ix =— ctnx— SB. 

73. rctn»xdx=-^i?^^^-fctnn-2xdx, 
*; n— 1 ./ 

74» Jsecxifo =: Iqgtanf | + ?Uj = log(8ecx + tanx)[+con8t.]. 



IV, E] 



TRIGONOMETRIC 



43 



75. Tcsc xdx =\og tan | = — log (esc x + ctn x) [ + const. ]. 



76.1 



sec^xdx = tanx. 



■ I 



77. I csc^ xdx = — ctn x. 



78 



. ( sec"* 



xcac*^xdx 



J si 



dx 



sin* X cos"* 05 



(See also 64.) 



dx 



= — = — sec"*^i X csc«-^ X + ^"^^ — = f sec"*-2 x esc* x 
wi — 1 w — 1 J 

= = — sec"*-! X cse**-i x -|- ^"^^ ~" rsec"» x csc**^ xdx 

n— 1 n— 1 J 

NoTxs. (a) In 64 and 78 and many others, m and n may have negative valaes. 

(&) To reduce J[sin*CB/co8"*CB]<?(D take m negative in 64. 

(o) To reduce /[cos"»0/sin** x] cte take n negative in 64. 

79. Substitutions: 



0) 



(2) 



(8) 



(4) 



(ft) 



u — 



since 



costs 



tana? 



sec CD 



(0 

tan — 

2 



du 



cos (0 (f {0 



— Ainwdoi 



sec* £D ef (0 



sec CD tan (to 



-8ec«-(fflJ 



811100 



« 



Vl - U« 



u 



Vl + w« 



Vw« - 1 



u 



2tf 

1 +M« 



COS 00 



>/l -«« 



-u 



Vi + ws 



1_ 
14 



1 -!<» 
l + tf* 



tanas 



7* 


V7^ 


u* 




Vi- 


M« 


u 


t» 




Vwa- 


-1 


2u 



1 -M« 



S0 



sin-* tt 



cos-i f* 



tan"*!* 



sec-*t* 



2 tan-* 1* 



cto 



(fu 



Vi -i*« 



dfM 



Vi - t*« 



du 
1+u* 



du 



t*Vtt«- 1 



2<gu 



Replace ctn x, sec x, esc x by 1/tan x, 1/cos x, 1/sin x, respectively. 

Notes, (a) J /'(sin 0) cos cb ef «, — use 79, (1). 

(b) / ^(cos aj) sin (to, — use 79, (2). 

(0) / ^(tan x) sec« 85 efoj, — use 79, (8) . 

id) Inspection of this table shows deHrahle aubatituUona from trigonometric to 
algebraic, and conversely. Thus, if only tan (0, sin* x, cos* x appear, use 79, (8). 



44 STANDARD INTEGRALS [TV, E 

80. f ^ = ^ gin-ifc + asinx jf „*> j^ 

..^ a + 6 sin X Va' — 6* a + 6 ain a; 

= _i_ log &>V6^^^ + atan(V2)^ .^^,^ ^ 
y/l^-a^ 5 + V62 _ ^a + o tan (a;/2) 

81. f ^— = i_ tan-i rJ^EItaDq, a^>6^; 

J a + & cos a: v^2 _ 52 L ^a + 6 2 J 



V62 - a2 V6 + a -V6-atan (a;/2) ' 

82. f . ^ = 1 logtan^ilg. « = sin-i ^ ■ 

y a sm X + 6 cos X VaM-~6^ ^ Vo^ + 6* 

Notes, (a) J — . . .^ , — use 79, (1), = ^ log (» + ^ sin »)• 

* a + 2>siii(D ^ a + sinoi b ^ b •' a+6 sin aj' 

then use 82 a, 80. 

(c) Many others similar to (a) and (6) ; e.g, /[sin cp/(a + & cos a)] rfa>, — use 79, (2). 

{d) r . , , — -^z T— and like forms, — nse 79, (8) ; see 79, note d. 

^ a* sin* x + b* cos« x » v / » 

(«) As last resort, ase 79, (5), for any rational trigonometric integral. 

Hb' Integrand Transcendental : Trigonometxic-Algebraio. 

83. f x« sin ic daj = — a?» cos a; + wi f a:«-i cos x dx, 

84. j a^ cos 05 (to = a?» sin a; — TO j a:"»-i sin x dx. 

Notes, (a) JccsintB^to*? — (BcoscD + Jcos^Jcto, — use 58. 
(6) /a?* sin xdx^ — repeat 88 to reach 68. 
(e) / (Any Polynomial) sin x dx, — split up and use 88. 
(d) For cos 85 repeat (o), (6), (c). 

Q- fsin X dx — sin X ,1 f cos x ^^ ^ _j. 1 

J X~ (to — 1) X*»-l TO — 1 •/ X™-1 

gg rcoaxdx^ C08X l_Cmidx,m=^l. 

J X" (m—1) x"-! m — 1 J x"*-! 



IV. E] TRANSCENDENTAL 45 

87. C^Mdx= f fl - ^ + ^ "I dx ; see II, B, 13, p. 8, 

88. (^^^dx = f rl - £. + ^ "1 dx ; see II, B, 14, p. 8. 

J X J La5 2 1 4 1 J 

NoTS. Other trigonometrie-algebraic combinations, use 5 ; or 79 followed by 89-84. 

Be> Integrand Transcendental : Inverse Trlgonometrio. 

89. Isin-i xdx=:x sin-i x + Vl^^. [From 6.] 

90. Tcos-i xdx = x cos-i x — Vl — x^, 

91. jtan-i xdx = x tan-i x — J log (1 + x*). 

92. (xn 8in-i xdx = ?:!li^ll^ - JL f ^!ii^ , then 53 or 64, 32, 36. 
J n + 1 n-\-lJ VrZ^ 

93. rx»co8-ixdx = ^'*^'^^«''^ + ^- f^::li^,then63or64,32,36. 
J n + 1 w+1 -^ Vl— x^ 

94. Cxntaa-ixdx = ^^'^^"'^ L_ f?!!li^, then 19 (c). 

J n + 1 n + l-Jl+a;* ^'^ 

NoTKS. (a) Replace ctn-ioj by ^ - tan-ijp ; or by tan"* (l/oj) and Bubstltate l/oj — 1», 

(fj) Replace sec'ia by cos~i(l/a5), c8C~iqj by 8ln~i(l/aj) and substltate \/x = u. 
(c) /(Any Polynomial) sin~icpr7aj, split up and use 92. (Similarly for cos'ijo, etc.) 
id) i/(^) 8in-»fl8<ffl8, - use (5) with u — sln"»a). (Similarly for co8~ia and tan-i<n.) 
(«) Other Inverse Trigonometric Integrands, use 79 or 5* 

Hd' Integrand Transcendental : Exponential and Logarithmic 

96. (a^dx = -^ = -f^ logio e = rf^ 0.4848. 
J lege a logio<^ logio^ 

96. (€^dx = e». 

Notes, (a) / «*»rfa5 -= «»* -^ *. (5) Notice a* - 6(lo».«)» - e**, * - log, a. 

97. fx^e** (Zx = - x»e*» - - f x*»-ic*' dx. 
^ k kJ 

NoTKS. (a) J «■€*'(/» = a?e**/* - e**/*«. (b) ^x'^e^dx, —repeat 97 to reach 97 Ca) 

(c) /(Any Polynomial) e^'dx, split up and use 97. 



46 



STANDARD INTEGRALS 



[IV, E 



98. (—dx = — + ^ (- — dx (repeat to reach 99). 

J x"» (m — 1) a;"»~i w — 1 ^ a;"*"^ 

99. C^dx =("[- + 1 + — 4- — + •••! <^tt, u = kx; see ra6Ze«, V, H 
J X J Lu 2131 J 



Bmnxdx = e^ 



k sin nx— n cos fix 



100. fe**8i_. - ,., ^ 

J *2 + n2 

102. I logxdx = a; logx — jc. 

103. f(logx)-^ = il2£^i:±\ «=jt_l. 
J X n + 1 

104. C^= ffMM^ ti = logx; see 99 and ro6Zc«, V, H. 

105. f X" log X dx = x"+i ri?l^ 1 1 . 

J Lw + 1 (n + l)2j 

106. f e** logx(?x = - e** logx - i f — dx, see 99. 
J k kJ X 



F. Some Important Definite Integrals. 
•«cfa5 1 



108. P- 
JD a' 



a?»» f»— 1 

* dx H 



, if m > 1 (otherwise non-existent). 



2 + 62x2 2ab 



109. f *a5»»6-»cfa5 = r(n + 1) = n I if n is integral. See V, F, p. 56. 

NoTjBS. (a) In general, r (n + 1 ) = « • r (n), as for n I, If »> 0. 

(6) r(2) = r(i) = i, r(i/2) = v^. r(« + i)-n(»). 

110. fx-(l-x)ndx = i:(!?L±I)iX!L±i}. 

J» r(m + n + 2) 



■X' 



111. i sinnx-Hinmxdx 



/•n 



cosna!;co8nia;cfiz;:=0, if 9f»^n, 

if m and n are integral. 

112. J sin2 nx dx=\ em^nxdx = ir/2 ; n integral, see 56, 59. 



tV, G] DEFINITE INTEGRALS 47 

3. C^e-'^dx^l/k. 114. P[(8in nx)/aj] da;= ir/2. 

5. f *6-** sin nx dx = n/(k^ + w^) , if A; > 0. 

6. Pe-** cos mx dx = k/(Jc^ + wi^) , if A; > 0. 

7. f *e-*'x»d« = ^^^t^^ = -^ , if n is integral. See 109. 
Jo A;'*+^ A;*+i 

,8. Pe-*»'Vx = v^/(2*). 
. i e-*^* cos mx (Zx = -— , if A; > 0. 

J.) 2 A5 

20. r_l^?_=r--^^- = -^. 121. C(\o^xydx = {-\Yn\ 
Jo efct+g-te Jo cosiiA-x 2 k Jo ^ '^ ^ ^ ^ 

;. r ''^^iog sin xdx= \ ^log cos xdx = — ^ log 2. 

Jo Jo 2 

23. i 8in2«+i xdx= \ cos2»*+i xdx=i „ ^ „ — — - ( n, positive 

J. J» 3.6.7...(2»+l)\j^^^^^ 

24. f "''sin''- a;<te = ("'^os^xdx = ^I'^/'J^l'^^ H (»- P<»i«™ 
^ Jo 2.4.6...2» 2 j^j^^^^ 

Q. Approzimation Formulas. 

• ) f (^') ^x = / (c) (6 — a), a < c < 6, [Law of the Mean.] 



if 



25 
26 



28 



. (\f(x)dx = /W+/(^) (6 - a). [Trapezoid Rule— precise 

for a straight line.] 

27. I f(x)dx. lExtended Trapezoid Eule.'] 

[/(a)/2+/(a+Ax)+/(a+2Ax)+ ••• 4-/[a4-(w-l)Ax]+/(&)/2]Ax. 

. Cfi^)dx=iM±im±±3m±mi^i,^a). 

[Prlamold Rule ; or second Simpson- Lagrange ^.p^roximaXion ; precise 
/(x) is any quadratic or cubic ; see § 124, p. 202.] 

.29. £f(x)dx = ^ If (a) + 4/(a + Ax) + 2/(a + 2 Ax) 

+ 4/(a + 3 Ax)H-2/(a 4-4 Ax)+ - +/(&)]. 
[Blmpson^B Rule ; or extended prismoid rule. Ex. 13, p. 207.] 



48 STANDARD* INTEGRALS [IV, G 

130. Cf(z)dx 

[A third Simpson-Lagrange Approximation. Extend as in 129.] 

131. f /(») (to 

[A fourth Simpson-Lagrange Approximation ; see Lagrange interpola- 
tion formula, n, I, 17, p. i5.] 

H. Standard AppllcationB of Integratdon. 

132. Areas of Plane Figures : id A. 

ia\ Strips AA parallel to 2^-axls : dA — y dx. 

(2>) Strips ^A parallel to avaxls : dA — x dy, I 

(c) Rectangles ^A =^^ix^y:dA = dxdy, A = Jfdxdy, 

(d) Parameter form of equation : A =(1/2) / {x dy. — y dx). 

(e) Polar sectors bounded by radii : dA = (p'/2) d9. 

(/) Polar rectangles 6.A '^ p^p^9: dA^pdpd9\ A "UpdpdB, 

133. Lengths of Plane Curves : i ds, 

(a) Equation in form y^f(x): d% = ^/l +[/'(a5)l«cte. 
(6) Equation in form x = 4>(y) : ds = Vl +l</>'(y)P<^y. 
(c) Parameter equations : ds —y/d^ + <fy*. 
(tf) Polar equation : tf« =■ Vd^"+p«^^. 

134. Volumes of Solids : (dV. 

(a) Frustum (area of cross section A): dV'* Adh\ V^jAdh where h is the variable 
height perpendicular to the cross section A, 

(b) Solid of revolution about aj-axis : dV^ny*dx. 

(c) Solid of revolution about y-axis : <i 7 =» iraj* dy. 

(d) Bectangular coordinate divisions :dV=dxdyd0\ 

V'= J^dzdydx= ^sdydx== S{Jzdy}dx — jAd». 

(e) Polar coordinate divisions ; dV^p^sinBdpd^ dB, 



rsr,H] APPLICATIONS 49 

135. Area of a Surface : \ f sec + dx dp, 

where ^ is the angle between the element ds of the surface and its pro- 
jection dxdy, 

(a) Surface of Bevolation about avaxis : A— j 2 try da. 
(6) Sorfoce of Bevolution about y-axis : A—l^rrxds. 

136. Length of twisted arcs : i ds. 

(a) Bectaugalar Coordinates : ds =« y/d«^ + dy* + rf««. 

(&) Explicit Equations y =/ (a?) , » « {x) : rf« = v^l + [/' (»)]* + [*' (a)]*. 

(c) a-/(0, y - 0(0, « = '/'W : <?« = v^[/'(0?+[<^'(0]«+['/''(OP. 

(c?) Polar Coordinates : d« = Vrf p« + pSci^* + p* cos* citf». 

137. Mass of a body : M = \dM = fp cf F, 

where p is the density (mass per unit volume). 

(a) If p is constant : Jtf"™ p / d F; see 184. 

(jb) On any curve : c? F= rf«, if p = mass per unit length. 

(c) On any surface (or plane) : dV= dA^ if p » mass per unit area. 

138. Average value of a variable quantity q : A. V* of q* : 

(a) throughout a solid : q =»/(», y, «) ; A.V.otq.==^q dV-i- Jd V. 

(5) on an area ^ : A. V. of q. — ^qdA-i- J dA. 
(c)onanarc«: A.V»otq.^ jqds-^ ^ds. 

139. Center of Mass, (x, y, i) : sc= i x dM -i- i dM, 
with similar formulas for y and z. See dM, 137. 

{a) for a volume : <?if ■= p c? F. 

(6) for an area : dM^ p cf ul. 
(c) for an arc : dM» p da. 

139.* Theorems of Papi)«« or Guldin : 

(a) Surface generated by an arc of a plane curve revolved about an 
axis in its plane = length of arc x length of path of center of mass of arc. 

(6) Volume generated by revolving a closed plane, contour about an 
axis in its plane = area of contour x length of path of its center of mass. 

140. Moment of IneHia : I = f r2 dM. (See 137, 139.) 

{a) For plane figures, Tx + Iy^Io, where /«, ly, 1q are taken about the te-azis, the 
y-axis, the origin, respectively. 

(b) For space figures, /« + /y + /«= Tq. 

(c) /jp = /- -f (05 — fiB)«Jf, where /^ is taken about a line || to the aj-axis. 



50 STANDARD INTEGRALS [IV, H 

141. Badim of Gyration : k^^I-h M= f r8 dM -s- (dM. 

[In 140 and 141, r may be the distance flroro some fixed point, or line, or plane.] 

142. Liquid pressure : P= iph dA, 

where P is the total pressure, dA is the elementary strip parallel to the 
surface ; h is the depth below the surface ; and p is the weight per unit 
volume of the liquid. 

143. Center of liquid pressure : h= i h^dA ± KhdA. 

144. Work of a variable force : W =\f cos + ds, 

where / is the numerical magnitude of the force, ds is the element of the 
arc of the path, and yp is the angle between / and ds. 

145. Attraction exerted by a solid : F=: k f ^^^ ^ 

where k \a the attraction between two unit masses at unit distance, m is 
the attracted particle, dM is an element of the attracting body ; r is the 
distance from m to dM. 

Components Fg, Fy. F, of F along Ox, Oy, Oz are : 

^,.t™J?2i±l^, F,-kmf-!!^^, j.._fcm;22i^, 

where a, ^, y are the direction angles of a line joining m to dJf. 

146. Work in an expanding gas : W = \p dv» 

147. Distance «, speed r, tangential acceleration jr* 

Jr = I V cZ< = i I isdtX dt. 
[Similar forms for angular speed and acceleration.] 

148. Errors of observation : 

y (f CD, where y ia the 
4,.w„^„— ~-^„^, ^. w- .— ^ — . *~* 

(&) The usual formula y - (A/Vw) «-*"** gives: P- (A/Vw) J «-**** cfoj, where h 
is the so-called measure of precision. 

(c) Probability of an error between x^— a and a5-«+a; P(a)— I y dx. 

(d) Probable error = (0.477) /A =- value of a for which P(a) — 1/2. 

(fl) Mean error ^ \ «yd<r+ I y tf » =- 1 / ( An/w ) 

Jo Jo 



V. NUMERICAL TABLES 



A. TRIGONOMETRIC FUNCTIONS 

[Characteristics nf Logarithms omitted — determine by the usual rule from the value] 



Radians 


De- 


Sine 


Tangbnt 


Cotangent 


Cosine 






grees 


Value logio 


Value logio 


Value 


logio 


Value 


logio 






0000 


0° 


.0000 


— CO 


.0000 -00 


00 


00 


1.0000 


0000 


90° 


1.5708 


.0175 


1° 


.0176 


2419 


.0175 2419 


57.290 


7581 


.9998 


9999 


89° 


1.5533 


.0349 


2° 


.0349 


5428 


.0349 5431 


28.636 


4569 


.9994 


9997 


88° 


1.5359 


.0524 


3° 


.0523 


7188 


.0524 7194 


19.081 


2806 


.9986 


9994 


87° 


1.5184 


.0698 


4° 


.0698 


8436 


.0699 8446 


14.301 


1564 


.9976 


9989 


86° 


1.5010 


.0873 


5° 


.0872 


9403 


.0876 9420 


11.430 


0580 


.9962 


9983 


85° 


1.4835 


.1047 


6° 


.1046 


0192 


.1051 0216 


9.5144 


9784 


.9945 


9976 


84° 


1.4661 


.1222 


7° 


.1219 


0869 


.1228 0891 


8.1443 


9109 


.9926 


9968 


"83° 


1.4486 


.1396 


.8° 


.1392 


1436 


.1405 1478 


7.1154 


8522 


.i)903 


9958 


82° 


1.4312 


.1571 


9° 


.1564 


1943 


.1684 1997 


6.3138 


8003 


.9877 


9946 


81° 


1.4137 


.1746 


10° 


.1736 


2397 


.1763 2463 


5.6713 


7537 


.9848 


9934 


80° 


1.3963 


.1920 


11° 


.1908 


2806 


.1944 2887 


5.1446 


7113 


.9816 


9919 


79° 


1.3788 


.2094 


12° 


.2079 


3179 


.2126 3276 


4.7046 


6726 


.9781 


9904 


78° 


1.3614 


.2269 


13° 


.2250 


3521 


.2309 3634 


4.3315 


61366 


.9744 


9887 


77° 


1.3439 


.2443 


14° 


.2419 


3837 


.2493 3968 


4.0108 


6032 


.9703 


9869 


76° 


1.3266 


.2618 


15° 


.2688 


4130 


.2679 4281 


3.7321 


5719 


.9659 


9849 


75° 


1.3090 


.2793 


16° 


.2756 


4403 


.2867 4576 


3.4874 


5425 


.9613 


9828 


74° 


1.2916 


.2967 


17° 


.2924 


4669 


.3057 4853 


3.2709 


5147 


.9563 


9806 


73° 


1.2741 


.3142 


18° 


.3090 


4900 


.3249 5118 


3.0777 


4882 


.9511 


9782 


72° 


1.25(K5 


.3316 


19° 


.3256 


6126 


.3443 5370 


2.9042 


4630 


.9455 


9757 


71° 


1.2392 


.3491 


20° 


.3420 


6341 


.3640 5611 


2.7475 


4380 


.9397 


9730 


70° 


1.2217 


.3665 


21° 


.3584 


5643 


.3839 5842 


2.6051 


4158 


.9336 


9702 


69° 


1.2043 


.3840 


22° 


.3746 


5736 


.4040 6064 


2.4751 


3936 


.9272 


9672 


68° 


1.1868 


.4014 


23° 


.3907 


5919 


.4245 6279 


2.3559 


3721 


.9205 


9640 


67° 


1.1694 


.4189 


24° 


.4067 


6093 


.4452 6486 


2.2460 


3514 


.9135 


9607 


66° 


1.1519 


.4363 


25° 


.4226 


6269 


.4663 6687 


2.1445 


3313 


.9063 


9573 


65° 


1.1345 


.4538 


26° 


.4384 


6418 


.4877 6882 


2.0503 


3118 


.8988 


9537 


64° 


1.1170 


.4712 


27° 


.4540 


6570 


.5096 7072 


1.9626 


2f)28 


.8910 


9499 


63° 


1.0996 


.4887 


28° 


.46i*5 


6716 


.5317 7257 


1.8807 


2743 


.8829 


9459 


62° 


1.0821 


.6061 


29° 


.4848 


6856 


.6543 7438 


1.8040 


2562 


.8746 


9418 


61° 


1.0647 


.5236 


30° 


.5000 


6990 


.5774 7614 


1.7321 


2386 


.8660 


9375 


60° 


1.0472 


.5411 


31° 


.5150 


7118 


.6009 7788 


1.6643 


2212 


.8572 


9331 


69° 


1.0297 


.5585 


32° 


.5299 


7242 


.6249 7958 


1.6003 


2042 


.8480 


928i 


58° 


1.0123 


.5760 


33° 


.5446 


7361 


.6494 8125 


1.5399 


1875 


.8387 


9236 


67° 


.9948 


.5934 


34° 


.5592 


7476 


.6745 8290 


1.4826 


1710 


.8290 


9186 


66° 


.9774 


.6109 


a5° 


.6736 


7586 


.7002 8452 


1.4281 


1548 


.8192 


9134 


55° 


.9599 


.6283 


36° 


.5878 


7692 


.7265 8613 


1.3764 


1387 


.80^)0 


9080 


54° 


.9425 


.6468 


37° 


.6018 


7796 


.7536 8771 


1.3270 


1229 


.7986 


9023 


53° 


.9250 


.6632 


38° 


.6157 


7893 


.7813 8928 


1.2799 


1072 


.7880 


8965 


52° 


.9076 


.6807 


39° 


.6293 


7989 


.8098 9084 


1.2349 


0916 


.7771 


8905 


51° 


.8901 


.6981 


40° 


.6428 


8081 


.8391 9238 


1.1918 


0762 


.7660 


8843 


50° 


.8727 


.7166 


41° 


.6561 


8169 


.8693 9392 


1.1504 


0608 


.7547 


8778 


49° 


.8552 


.7330 


42° 


.6691 


8265 


.9004 9544 


1.1106 


0456 


.7431 


8711 


48° 


.8378 


.7606 


43° 


.6820 


8338 


.9326 9697 


1.0724 


0303 


.7314 


8641 


47° 


.8203 


.7679 


44° 


.6947 


8418 


.9667 9848 


1.0356 


0152 


.7193 


8569 


46° 


.8029 


.7864 


45° 


.7071 


8495 


1.0000 0000 


1.0000 


0000 


.7071 


8495 


45° 


.7854 






Value 


logio 


Value lopjo 


Value 


loPio 


Value 


logic 


De- 


Radians 






COSINR 


Cotangent 


Tangent 


Sine | 


grees 



51 



52 



NUMERICAL TABLES 



[V, B 



B. COMMON LOGARITHMS 



N 





1 


2 


3 


4 


5 


6 


7 


8 


9 


I> 


10 


0000 


0O43 


0086 


0128 


0170 


0212 


0253 


0294 


0334 


0374 


42 


11 


0414 


0463 


0492 


0631 


0569 


0607 


0645 


0682 


0719 


0765 


38 


12 


0792 


0828 


0864 


0899 


0934 


0969 


1004 


1038 


1072 


1106 


35 


13 


1139 


1173 


1206 


1239 


1271 


1303 


1336 


1367 


1399 


1430 


32 


14 


1461 


1492 


1523 


1553 


1584 


1614 


1644 


1673 


1703 


1732 


30 


15 


1761 


1790 


1818 


1847 


1876 


1903 


1931 


1959 


1987 


2014 


28 


16 


2041 


2068 


2095 


2122 


2148 


2175 


2201 


2227 


2253 


2279 


26 


17 


2304 


2330 


2365 


2380 


2405 


2430 


2466 


2480 


2504 


2529 


25 


18 


2563 


2577 


2601 


2625 


2648 


2672 


2696 


2718 


2742 


2765 


24 


19 


2788 


2810 


2833 


2856 


2878 


2900 


2923 


2945 


2967 


2989 


22 


20 


3010 


3032 


3064 


3075 


3096 


3118 


3139 


3160 


3181 


3201 


21 


21 


3222 


3243 


3263 


3284 


3304 


3324 


3345 


3365 


3385 


3404 


20 


22 


3424 


3444 


3464 


3483 


3602 


3622 


3541 


3660 


3579 


3698 


19 


23 


3617 


3636 


3655 


3674 


3692 


3711 


3729 


3747 


3766 


3784 


18 


24 


3802 


3820 


3838 


3856 


3874 


3892 


3909 


3927 


3945 


3962 


18 


25 


3979 


3997 


4014 


4031 


4048 


4066 


4082 


4099 


4116 


4133 


17 


26 


4150 


4166 


4183 


4200 


4216 


4232 


4249 


4265 


4281 


4298 


16 


27 


4314 


4330 


4346 


4362 


4378 


4393 


4409 


4425 


4440 


4456 


16 


28 


4472 


4487 


4502 


4518 


4533 


4648 


4664 


4579 


4694 


4609 


15 


29 


4624 


4639 


4654 


4669 


4683 


4698 


4713 


4728 


4742 


4757 


15 


30 


4771 


4786 


4800 


4814 


4829 


4843 


4867 


4871 


4886 


4900 


14 


31 


4914 


4928 


4942 


4955 


4969 


4983 


4997 


5011 


6024 


5038 


14 


32 


5051 


5065 


5079 


5092 


5105 


6119 


6132 


5145 


5169 


5172 


13 


33 


6185 


5198 


5211 


6224 


5237 


5250 


6263 


5276 


5289 


5302 


13 


34 


6316 


5328 


5340 


5363 


5366 


6378 


6391 


6403 


5416 


5428 


13 


35 


5441 


5453 


5465 


5478 


5490 


6502 


5514 


5527 


6539 


5651 


12 


36 


5663 


5575 


5687 


5699 


5611 


5623 


6635 


6647 


5658 


5670 


12 


37 


6682 


5694 


5705 


5717 


5729 


6740 


5762 


5763 


6775 


5786 


12 


38 


6798 


5809 


5821 


5832 


5843 


6866 


5866 


5877 


5888 


5899 


11 


39 


6911 


5922 


5a33 


5944 


5965 


5966 


5977 


5988 


5999 


6010 


11 


40 


6021 


6031 


6042 


6053 


6064 


60Z5 


6085 


6096 


6107 


6117 


11 


41 


6128 


6138 


6149 


6160 


6170 


6180 


6191 


6201 


6212 


6222 


10 


42 


6232 


6243 


6263 


6263 


6274 


6284 


6294 


6304 


6314 


6325 


10 


43 


6335 


6345 


6365 


6365 


6375 


6385 


6395 


6406 


6415 


6425 


10 


44 


6435 


6444 


6454 


6464 


6474 


6484 


6493 


6603 


6613 


6622 


10 


45 


6632 


6542 


6551 


6561 


6571 


6680 


6590 


6599 


6609 


■6618 


10 


46 


6628 


6637 


6646 


6666 


6665 


6675 


6684 


6693 


6702 


6712 


9 


47 


6721 


6730 


6739 


6749 


6758 


6767 


6776 


6785 


6794 


6803 


9 


48 


6812 


6821 


6830 


6839 


6848 


6867 


6866 


6875 


6884 


6893 


9 


49 


6902 


6911 


6920 


6928 


6937 


6946 


6965 


6964 


6972 


6981 


9 


50 


6990 


6998 


7007 


7016 


7024 


7033 


7042 


7050 


7069 


7067 


9 


51 


7076 


7084 


7093 


7101 


7110 


7118 


7126 


7135 


7143 


7152 


8 


52 


7160 


7168 


7177 


7185 


7193 


7202 


7210 


7218 


7226 


7235 


8 


53 


7243 


7251 


7269 


7267 


7275 


7284 


7292 


7300 


7308 


7316 


8 


54 


7324 


7332 


7340 


7348 


7356 


7364 


7372 


7380 

• 


7388 


7396 


8 



V.B] 



COMMON LOGARITHMS 



53 



N 





1 


2 


3 


4 


5 


6 


7 


8 


9 


D 

8 


55 


7404 . 


7412 


7419 


7427 


7435 


7443 


7451 


7459 


7466 


7474 


56 


7482 


7490 


7497 


7505 


7513 


7520 


7528 


7536 


7543 


7551 


8 


67 


7559 


7566 


7574 


7582 


7589 


7597 


7604 


7612 


7619 


7627 


8 


58 


7634 


7642 


7649 


7657 


76(>4 


7672 


7679 


7686 


7694 


7701 


7 


59 


7709 


7716 


7723 


7731 


7738 


7745 


7752 


7760 


7767 


7774 


7 


60 


7782 


7789 


7796 


7803 


7^10 


7818 


7825 


7832 


7839 


7846 


7 


61 


7863 


7860 


7868 


7875 


7882 


7889 


7896 


7903 


7910 


7917 


7 


62 


7924 


7931 


7938 


7945 


7952 


7959 


7966 


7973 


7980 


7987 


7 


68 


7993 


8000 


8007 


8014 


8021 


8028 


8a35 


8041 


8048 


8055 


7 


64 


8062 


8069 


8075 


8082 


8089 


8096 


8102 


8109 


8116 


8122 


7 


65 


8129 


8136 


8142 


8149 


8156 


8162 


8169 


8176 


8182 


8189 


7 


66 


8195 


8202 


8209 


8215 


8222 


8228 


8235 


8241 


8248 


8254 


7 


67 


8261 


8267 


8274 


8280 


8287 


8293 


8299 


8306 


8312 


8319 


6 


68 


8325 


8331 


8338 


8344 


8351 


8357 


8363 


8370 


8376 


8382 


6 


69 


8388 


8395 


8401 


8407 


8414 


8420 


8426 


8432 


8439 


8445 


6 


70 


8461 


8457 


8463 


8470 


8476 


8482 


8488 


8494 


8500 


8506 


6 


71 


8513 


8519 


8525 


8531 


8637 


8543 


8649 


8555 


8561 


8567 


6 


72 


8573 


8579 


8585 


8591 


8597 


8603 


8609 


8615 


8621 


8627 


6 


78 


8633 


8639 


8645 


8651 


8657 


8663 


8669 


8675 


8681 


8686 


6 


74 


8692 


8698 


8704 


8710 


8716 


8722 


8727 


8733 

• 


8739 


8745 


6 


75 


8751 


8756 


8762 


8768 


8774 


8779 


8785 


8791 


8797 


8802 


6 


76 


8808 


8814 


8820 


8825 


8831 


8837 


8842 


8848 


8864 


8859 


6 


77 


8865 


8871 


8876 


8882 


8887 


8893 


8899 


8904 


8910 


8915 


6 


78 


8i*21 


8927 


8932 


8938 


8943 


8949 


8954 


8960 


8965 


8971 


6 


79 


8976 


8982 


8987 


8993 


8998 


9004 


9009 


9016 


9020 


9025 


5 


80 


<mi 


9036 


9042 


9047 


9053 


9058 


9063 


9069 


9074 


9079 


5 


81 


9085 


9090 


9096 


9101 


9106 


9112 


9117 


9122 


9128 


9133 


6 


82 


9138 


9143 


9149 


9154 


9159 


9165 


9170 


9176 


9180 


9186 


5 


88 


9191 


9196 


9201 


9206 


9212 


9217 


9222 


9227 


9232 


9238 


5 


84 


9243 


9248 


9253 


9258 


9263 


9269 


9274 


9279 


9284 


9289 


5 


85 


9294 


9299 


9304 


9309 


9315 


9320 


9325 


9330 


9335 


9340 


6 


86 


9345 


9350 


9355 


9360 


9365 


9370 


9375 


9380 


9386 


9390 


5 


87 


9395 


9400 


9405 


9410 


9415 


9420 


9425 


9430 


9436 


9440 


5 


88 


9445 


9450 


9455 


9460 


9465 


9469 


9474 


9479 


9484 


9489 


5 


89 


9494 


9499 


9504 


9509 


9513 


9518 


9523 


9528 


9533 


9538 


5 


90 


9542 


9547 


9552 


9557 


9562 


9566 


9571 


9576 


9581 


9586 


5 


91 


9590 


9595 


9600 


9606 


9609 


9614 


9619 


9624 


9628 


9633 


5 


92 


9638 


9643 


9647 


9652 


9657 


9661 


9666 


9671 


9675 


9680 


5 


98 


9685 


9689 


9694 


9699 


9703 


9708 


9713 


9717 


9722 


9727 


5 


94 


9731 


9736 


9741 


9745 


9750 


9754 


9759 


9763 


9768 


9773 


6 


95 


9777 


9782 


9786 


9791 


9795 


9800 


9805 


9809 


9814 


9818 


6 


96 


9823 


9827 


9832 


9836 


9841 


9845 


9850 


9854 


9859 


9863 


6 


97 


9868 


9872 


9877 


9881 


9886 


9890 


9894 


9899 


9903 


9908 


4 


98 


9912 


9917 


9921 


9926 


9930 


9934 


9939 


9943 


9948 


9952 


4 


99 


9956 


9i)61 


9965 


9969 


9974 


9978 


9983 


9987 


9991 


9996 


4 



54 



NUMERICAL TABLES 



[V,C 



C. EXPONENTIAI, AHD HYPERBOLIC FUNCTIONS 







e* 


e- 


-z 


slnhat; 


eoshoo 


(0 


logeOJ 


Value 


logio 


Value 


logio 


Value 


lo&io 


Value 


loffio 


0.0 


— 00 


1.000 


0.000 


1.000 


0.000 


0.000 


— 00 


1.000 





0.1 


-2.303 


1.105 


0.043 


0.905 


9.957 


0.100 


9.001 


1.006 


0.002 


0.2 


-1.610 


1.221 


0.087 


0.819 


9.913 


0.201 


9.304 


1.020 


0.009 


0.3 


-1.204 


1.350 


0.130 


0.741 


9.870 


0.305 


9.484 


1.045 


0.019 


0.4 


-0.916 


1.492 


0.174 


0.670 


9.826 


0.411 


9.614 


1.081 


0.034 


0.5 


-0.693 


1.649 


0.217 


0.607 


9.783 


0.621 


9.717 


1.128 


0.052 


0.6 


-0.511 


1.822 


0.261 


0.549 


9.739 


0.637 


9.804 


1.185 


0.074 


0.7 


-0.367 


2.014 


0304 


0.497 


9.696 


0.769 


9.880 


1.255 


0.099 


0.8 


-0.223 


2.226 


0.347 


0.449 


9.663 


0.888 


9.948 


1.337 


0.126 


0.9 


-0.106 


2.460 


0.391 


0.407 


<f.609 


1.027 


0.011 


1.433 


0.156 


1.0 


0.000 


2.718 


0.434 


0368 


9.666 


1.175 


0.070 


1.543 


0.188 


1.1 


0.095 


3.004 


0.478 


0.333 


9.622 


1.336 


0.126 


1.669 


0.222 


1.2 


0.182 


3.320 


0.521 


0.301 


9.479 


1.609 


0.179 


1.811 


0.258 


1.3 


0.262 


3.669 


0.566 


0.273 


9.435 


1.698 


0.230 


1.971 


0.295 


1.4 


0.336 


4.055 


0.608 


0.247 


9.392 


1.904 


0.280 


2.151 


o.:«3 


1.6 


0.406 


4.482 


0.651 


0.223 


9.349 


2.129 


0.328 


2.an2 


0.372 


1.6 


0.470 


4.953 


0.695 


0.202 


9.305 


2.376 


0.376 


2.577 


0.411 


1.7 


0.631 


6.474 


0.738 


0.183 


9.262 


2.646 


0.423 


2.828 


0.452 


1.8 


0.588 


6.050 


0.782 


0.165 


9.218 


2.942 


0.469 


3.107 


0.492 


1.9 


0.642 


6.686 


0.826 


0.160 


9.175 


3.268 


0.614 


3.418 


0.534 


2.0 


0.693 


7.389 


0.869 


0.135 


9.131 


3.627 


0.660 


a762 


0.576 


2.1 


0.742 


8.166 


0.912 


0.122 


9.088 


4.022 


0.604 


4.144 


0.617 


2.2 


0.788 


9.025 


0.955 


0.111 


9.046 


4.467 


0.649 


4.668 


0.660 


2.3 


0.833 


9.974 


0.999 


0.100 


9.001 


4.937 


0.690 


5.037 


0.702 


2.4 


0.875 


11.02 


1.023 


0.091 


8.958 


6.466 


0.738 


6.657 


0.745 


2.6 


0.916 


12.18 


1.086 


0.082 


8.914 


6.060 


0.782 


6.132 


0.788 


2.6 


0.956 


13.46 


1.129 


0.074 


8.871 


6.695 


0.826 


6.769 


0.831 


2.7 


0.993 


14.88 


1.173 


0.067 


8.827 


7.406 


0.870 


7.473 


0.874 


2.8 


1.030 


16.44 


1.216 


0.061 


8.784 


8.192 


0.913 


8.253 


0.917 


2.9 


1.005 


18.17 


1.259 


0.055 


8.741 


9.060 


0.957 


9.115 


0.960 


3.0 


1.099 


20.09 


1.303 


0.050 


8.697 


10.018 


1.001 


10.068 


1.003 


3.6 


1.253 


33.12 


1.620 


0.03Q 


8.480 


16.643 


1.219 


16.673 


1.219 


4.0 


1.386 


54.60 


1.737 


0.018 


8.263 


27.290 


1.436 


27.308 


1.436 


4.5 


1.504 


90.02 


1.964 


0.011 


8.046 


46.003 


1.653 


45.014 


1.653 


6.0 


1.609 


148.4 


2.171 


0.007 


7.829 


74.203 


1.870 


74.210 


1.870 


6.0 


1.792 


403.4 


2.606 


0.002 


7.394 


201.7 


2.305 


201.7 


2.305 


7.0 


1.946 


1096.6 


3.0i0 


0.001 


6.960 


548.3 


2.739 


648.3 


2.739 


8.0 


2.079 


2981.0 


3.474 


0.000 


6.526 


1490.6 


3.173 


1490.5 


3.173 


9.0 


2.197 


8103.1 


3.909 


0.000 


6.091 


4051.6 


3.608 


4051.5 


3.608 


10.0 


2.303 


22026. 


4.343 


0.000 


6.667 


11013. 


4.041 


11013. 


4.041 



log<, X. = (logio x)-^M ; M= .4342944819. logi© e*+» = logio e* -r logio ev. 

Sinhx and coshaj approach e*/2 as x increases (see Fig. E, p. 2^). The 
formula logjo (e'/2) = M -x — logio 2 represents logjo sinh x and logjo cosh x to 
three decimal places when a; > 3.5 ; four places when a; > 5 ; to five places when 
x>6] to eight places when x > 10. 



V.E] 



ELLIPTIC INTEGRALS 



55 



D. VALUES OF 






dx 



Vl-A:2siii2e '^o V(l-a52)(l-A;2ac2) 
[Elliptic Integral of the First Kind.] 



a? = sinO 



Jb» 


<^-5o 


<f>^10P 


*-16« 


<l>=ZOP 


<^»45o 


<^»60o 


«fr-75o 


K 




-ir/ao 


=ir/18 


=ir/12 


= 7r/6 


-ir/4 


-ir/8 


-6ir/12 


«fr-90"> 


















-ir/2 


0.0 


0.087 


0.175 


0.262 


0.524 


0.786 


1.047 


1.309 


1.571 


0.1 


0.087 


0.175 


0.262 


0.524 


0.786 


1.049 


1.312 


1.575 


0.2 


0.087 


0.175 


262 


0.525 


0.789 


1.054 


1.321 


1.588 


0.3 


0.087 


0.176 


0.262 


0.526 


0.792 


1.062 


1.336 


1.610 


0.4 


0.087 


0.175 


0.262 


0.527 


0.798 


1.074 


1.358 


1.643 


0.5 


0.087 


0.175 


0.263 


0.629 


0.804 


1.090 


1.385 


1.686 


0.6 


0.087 


0.175 


0.263 


0.532 


0.814 


1.112 


1.426 


1.762 


0.7 


0.087 


0.175 


0.263 


0.536 


0.826 


1.142 


1.488 


1.854 


0.8 


0.087 


0.176 


0.264 


0.539 


0.839 


1.178 


1.566 


1.993 


0.9 


0.087 


0.175 


0.264 


0.544 


0.858 


1.233 


1.703 


2.275 


1.0 


0.087 


0.175 


0.265 


0.549 


0.881 


1.317 


2.028 


oo 



£(*, ♦) 



Jo 



E. VALUES OF 



hi sin^ e d^ 



Jo 



[Elliptic Integral of the Second Kind.] 



dx^ 



X 

u 



sine 
sin^ 



h^ 


*=6«> 


<^=10« 


<^»16o 


*=80« 


<^-46« 


«fr=60«» 


*=75"» 


JS 




=ir/86 


-ir/18 


=ir/12 


= ir/6 


= ir/4 


= ir/8 


-6ir/12 


^=90° 


















= ir/2 


0.0 


0087 


0.176 


0.262 


0.524 


0.786 


1.047 


1.309 


1.571 


0.1 


0.087 


0.176 


0.262 


0.623 


0.785 


1.046 


1.306 


1.566 


0.2 


0.087 


0.174 


0.262 


0.523 


0.782 


1.041 


1.297 


1.554 


0.3 


0.087 


0.174 


0.262 


0.521 


0.779 


1.033 


1.283 


1.533 


0.4 


0.087 


0.174 


0.261 


0.520 


0.773 


1.026 


1.264 


1.504 


0.5 


0.087 


0.174 


0.261 


0.518 


0.767 


1.008 


1.240 


1.467 


0.6 


0.087 


0.174 


0.261 


0.515 


0.759 


0.989 


1.207 


1.417 


0.7 


0.087 


0.174 


0.2(i0 


0.512 


0.748 


0.965 


1.163 


1.351 


0.8 


0.087 


0.174 


0.260 


0.509 


0.737 


0.940 


1.117 


1.278 


0.9 


0.087 


0.174 


0.259 


0.505 


0.723 


0.907 


1.053 


1.173 


1.0 


0.087 


0.174 


0.259 


0.500 


0.707 


0.866 


0.966 


1.000 



56 



NUMERICAL TABLES 

F. VALUSS OF n (p) =T (p + 1) = (e-^xPdSD 

Jo 

p A PROPER FRACTION 

[n fn) =B r (n + 1) a= n I, if n is a positive integer.] 



[V.I 





1>?»0.0 


p-0.1 


p-0.2 


p-0.8 


p-0.4 


1>»0.5 


p»0.6 


p=0.7 


p^O.S 


p=M 

0.9G2 


r(p+i)= 


1.000 


0.951 


0.918 


0.897 


0.887 


0.886=v^/2 


0.894 


0.909 


0.931 



r (* + 1) = * r (*) , if ifc > ; hence T(k + 1) can be calculated at intervals of 0.1. 
Minimum value of r(p + 1) is .88560 atp = .46163. 



6. VALUES OF THE PROBABILITY INTEGRAL: 



Vi 



Jo 



e-^^dXi 



X 


.0 


.1 


.2 


.8 


.4 


.6 


.6 


.7 


.8 


.9 


0. 

1. 

2. 


.0000 
.8427 
.9953 


.1125 

.8802 
.9970 


.2227 
.9103 
.9981 


.3286 
.9340 
.9989 


.4284 
.9523 
.9993 


.5205 
.9661 
.9996 


.6039 
.9763 
.9998 


.6778 
.9838 
.9999 


.7421 
.9891 
.99911 


.7969 

.9928 

1.0000 



H. VALUES OF THE INTEGRAL C 

[Note break at a; = 0.] 



^^dx 



<x> (C 





n»l 


n«2 


ra=s8 


n»4 


n»6 


n»6 


n=7 


n=8 


n^i 


X =*— n ♦ 
a;=— n/10 


-.2194 
-1.823 


-.0489 
— 1.223 


-.0130 
-.9057 


-.0038 
-.7024 


-.0012 
-.6598 


-.0004 
-.4544 


-.0001 
— .3738 


— .0000 
-.3106 


-.0000 

- .wa 


a;=+n/10 

x=4-n 


— 1.623 
1.895 


- .8218 
4.954 


-.3027 
9.934 


+ .1048 
19.63 


.4542 
40.18 


.7699 
85.99 


1.065 
191.5 


1.347 
440.4 


1.623 
1038 



•Note 
'« dx 



-00 



e*dx 



=—00. Values on each side of a = can be used safely. 



\ -^^ and f — dx reduce to the integral here tabulated ; see IV, 99, 104, p. 46. 
Jo log* J z* 



V.I] 



RECIPROCALS SQUARES CUBES 



57 



Ii. RECIPROCALS OF NUMBERS FROM 1 TO 9.9 



1 


.0 


.1 


.2 


.8 


.4 


.6 


.6 


.7 


.8 


.9 


1.000 


0.909 


0.833 


0.769 


0.714 


0.667 


0.625 


0.588 


0.556 


0.526 


2 


0.500 


0.476 


0.465 


0.435 


0.417 


0.400 


0.385 


0.370 


0.357 


0.345 


3 


0.333 


0.323 


0.313 


0.303 


0.294 


0.286 


0.278 


0.270 


0.263 


0.256 


4 


0.250 


0.244 


0.238 


0.233 


0.227 


0.222 


0.217 


0.213 


0.208 


0.204 


5 


0.!»0 


0.196 


0.192 


0.189 


0.185 


0.183 


0179 


0.175 


o.m 


0.169 


6 


0.167 


0.164 


0.161 


0.159 


0.156 


0.154 


0.152 


0.149 


0.147 


0.145 


7 


0.143 


0.141 


0.139 


0.137 


0.136 


0.133 


0.132 


0.130 


0.128 


0.127 


8 


0.125 


0.123 


0.122 


0.120 


0.119 


0.118 


0.116 


0.116 


0.114 


0.112 


9 


0.111 


0.110 


0.109 


0.108 


0.106 


0.105 


0.104 


0.103 


0.102 


0.101 



I2. SQUARES OF NUMBERS FROM 10 TO 99 



1 





1 


2 


S 


4 


6 


6 


7 


8 


9 


100 


121 


144 


169 


196 


226 


256 


• 289 


324 


361 


2 


400 


441 


484 


529 


576 


625 


676 


729 


784 


841 


3 


900 


961 


1024 


1089 


1156 


1225 


1296 


1369 


1444 


1621 


4 


1600 


1681 


1764 


1849 


1936 


2026 


2116 


2209 


2304 


2401 


5 


2500 


2001 


2704 


2809 


2916 


9025 


3136 


3249 


3364 


3481 


6 


3600 


3721 


3844 


3969 


4096 


4226 


4356 


4489 


4624 


4761 


7 


4900 


5041 


5184 


5329 


6476 


5626 


5776 


6929 


6084 


6241 


8 


6400 


6561 


6724 


6889 


7056 


7226 


7396 


7569 


7744 


7921 


9 


8100 


8281 


8464 


8649 


8836 


9025 


9216 


9409 


9604 


9801 



Is. CUBES OF NUMBERS FROM 1 TO 9.9 



1 


.0 


.1 


.2 


.8 


.4 


.5 


.6 


.7 


.8 


.9 


1.00 


1.33 


1.73 


2.20 


2.74 


3.37 


4.10 


4.91 


5.83 


6.86 


2 


8.00 


9.26 


10.66 


12.17 


13.82 


15.62 


17.58 


19.68 


21.96 


24.39 


3 


27.00 


29.79 


32.77 


a5.94 


39.30 


42.87 


46.66 


50.65 


64.87 


66.32 


4 


(>4.0 


68.9 


74.1 


79.5 


86.2 


91.1 


97.3 


103.8 


110.6 


117.6 


5 


125.0 


132.7 


140.6 


148.9 


157.5 


166.4 


175.6 


185.2 


195.1 


205.4 


6 


216.0 


227.0 


238.3 


250.0 


262.1 


274.6 


287.5 


300.8 


314.4 


328.5 


7 


343.0 


357.9 


373.2 


389.0 


405.2 


421.9 


439.0 


456.6 


474.6 


493.0 


8 


512.0 


631.4 


551.4 


671.8 


592.7 


614.1 


636.1 


658.6 


681.5 


705.0 


r 


729.0 


753.6 


778.7 


804.4 


830.6 


857.4 


884.7 


912.7 


941.2 


970.3 



58 



NUMERICAL TABLES 



[V,J 



Ji. SQUASE ROOTS OF NUMBERS FROM 1 TO 9.9 






.0 


.1 


.2 


.8 


.4 


.5 


.6 


.7 


.8 


.» 


0.000 


0.316 


0.447 


0.548 


0.632 


0.707 


0.775 


0.837 


0.894 


0.949 


1 


1.000 


1.049 


1.095 


1.140 


1.183 


1.225 


1.265 


1.304 


1.342 


1.378 


2 


1.414 


1.449 


1.483 


1.517 


1.549 


1.581 


1.612 


1.643 


1.673 


1.703 


8 


1.732 


1.761 


1.789 


1.817 


1.844 


1.871 


1.897 


1.924 


1J949 


1.975 


4 


2.000 


2.025 


2.049 


2.074 


2.098 


2.121 


2.145 


2.168 


2.191 


2.214 


^ 6 


2.336 


2.258 


2.280 


2.802 


2.324 


2.345 


2.366 


2.387 


2.408 


2.429 


6 


2.449 


2.470 


2.490 


2.510 


2.530 


2.560 


2.569 


2.588 


2.608 


2.627 


7 


2.646 


2.665 


2.683 


2.702 


2.720 


2.739 


2.757 


2.775 


2.793 


2.811 


8 


2.828 


2.846 


2.864 


2.881 


2.898 


2.915 


2.933 


2.950 


2.966 


2.983 


9 


3.000 


3.017 


3.033 


3.050 


3.066 


3.082 


3.098 


3.114 


3.130 


3.146 



J2. SQUARE ROOTS OF NUMBERS FROM 10 TO 99 



1 





1 


2 


8 


4 


5 


« 


7 


8 9 


3.162 


3.317 


3.464 


3.606 


3.742 


3.873 


4.000 


4.123 


4.243 4.359 


2 


4.472 


4.583 


4.690 


4.796 


4.899 


6.000 


5.099 


5.196 


5.292 6.385 


8 


5.477 


5.568 


5.657 


5.745 


5.831 


5.916 


6.000 


6.083 


6.164 6.245 


4 


6.325 


6.403 


6.481 


6.557 


6.633 


6.708 


6.782 


6.856 


6.928 7.000 


6 


7.071 


7.141 


7.211 


7.280 


7.348 


7.416 


7.483 


7.550 


7.616 7.681 


6 


7.746 


7.810 


7.874 


7.937 


8.000 


8.062 


8.124 


8.185 


8.246 8.307 


7 


8.367 


8.426 


8.485 


8.544 


8.602 


8.660 


8.718 


8.775 


8.832 8.888 


8 


8.944 


9.000 


9.055 


9.110 


9.165 


9.220 


9.274 


9.327 


9.381 9.434 


9 


9.487 


9.539 


9.592 


9.644 


9.696 


9.747 


9.798 


9.849 


9.899 9.950 



K. RADIANS TO DEGREES 



1 

2 
8 
4 
5 
6 
7 
8 
9 


Radians 


Tenths 


Hundredths 


Thousandths 


Ten-thousandths 


57°17'44".8 
114°35'29".6 
171°53'14".4 
229°10'59".2 
286°28'44".0 
343°46'28".8 
401° 4' 13" .6 
458°21'58".4 
515°39'43".3 


5°4;V46".5 
11°27'33".0 
17°11'19".4 
22°55'05".9 
28°38'52".4 
34°22'38".9 
40° 6'25".4 
45°50'11".8 
61°33'58".3 


0°34'22".6 
1° 8'45".3 
1°43'07".9 
2°17'30".6 
2°51'53".2 
3°26'15".9 
4° 0'38".5 
4°35'01".2 
5° 9'23".8 


0° 3'26".3 
0° 6'52".5 
0°10'18".8 
0°13'45".l 
0°17'11".3 
0°20'37".6 
0°24'03".9 
0°27'30".l 
0°30'56".4 


0° 0'20".6 
0° 0'41".3 
0° 1'01".9 
0° 1'22".5 
0° l'43".l 
0° 2'03".8 
0° 2'24".4 
0° 2'45".0 
0° 3'05".6 



V.M] 



CONSTANTS 



59 



L. IMPORTANT CONSTANTS AND THEIR COIIMON 

LOGARITHMS 



^=» Number 


Value of 2^ 


LoOio^A^ 


TT 


3.14159265 


0.49714987 


1-i-ir 


0.31830989 


9.60286013 


X2 


9.86960440 


0.99429975 


V¥ 


1.77245385 


0.24857494 


e = Napierian Base 


2.71828183 


0.43429448 


M=lOgio€ 


0.43429448 


9.63778431 


l-5-3f=logelO 


2.30258509 


0.36221569 


180 -f-ir = degrees in 1 radian 


67.2957795 


1.75812263 


ir -f. 180 = radians in 1° 


0.01745329 


8.24187737 


TT ^ 10800 = radians in 1' 


0.0002908882 


6.46372612 


V -*. 648000 = radians in 1" 


0.000004848136811095 


4 68567487 


sin 1" 


0.000004848136811076 


4.68557487 


tan 1" 


0.000004848136811133 


4.68657487 


centimeters in 1 ft. 


30.480 


1.4840158 


feet in 1 cm. 


0.032808 


8.6169842 


inches in 1 m. 


39.37 


1.5951654 


pounds in 1 kg. 


2.20462 


0.3433340 


kilograms in 1 lb. 


0.453693 


9.6666660 


g (average value) 


32.16 ft./sec./sec. 


1.5073 




= 981 cm./ sec/sec. 


2.9916690 


weight of 1 cu. ft. of water 


62.425 lb. (max. density) 


1.7953686 


weight of 1. cu. ft. of air 


0.0807 lb. (at 32° F.) 


8.907 


cu. in. in 1 (U. S.) gallon 


231 


2.3636120 


ft. lb. per sec. in 1 H. P. 


560. 


2.7403627 


kg. m. per sec. in 1 H. P. 


76.0404 


1.8810445 


watts in 1 H. P. 


745.957 


2.8727135 



M. DEGREES TO RADIANS 



1° 


.01745 


10° 


.17463 


100° 


1.74533 


6' 


.00175 


6" 


.00003 


2° 


.03191 


20° 


.34907 


110° 


1.91986 


r 


.00204 


7" 


.00003 


3° 


.05236 


30° 


.52360 


120° 


2.09440 


8' 


.00233 


8" 


.00004 


4° 


.06981 


40° 


.69813 


130° 


2.26893 


9' 


.00262 


9" 


.00004 


5° 


.08727 


60° 


.87266 


140° 


2.44346 


10' 


.00291 


10" 


.00006 


6° 


.10472 


60° 


1.04720 


160° 


2.61799 


20' 


.00682 


20" 


.00010 


7° 


.12217 


70° 


1.22173 


160° 


2.79253 


30' 


.00873 


30" 


.00016 


8° 


.13963 


80° 


1.39626 


170° 


2.96706 


40' 


.01164 


40" 


.00019 


9° 


.16708 


90° 


1.57080 


180° 


3.14159 


50' 


.01464 


60" 


.00024 



60 



NUMERICAL TABLES 



(V, N 



N. SHORT CONVERSION TABLES AND OTHER DATA: 
MULTIPLES, POWERS, ETC., FOR VARIOUS NUMBERS 





n»l 


n»2 


n»c8 


n=4 n=5 n=6 


»=7 


n=8 


M=9 


TT »n 


3.1416 


6.2832 


9.4248 


12.566 15.708 18.860 


21.991 


25.133 


28.274 


TT . 71^/4 


.78540 


3.1416 


7.0686 


12.666 19.635 28.274 


38.485 


60.265 


63.617 


V . n8/6 


.62360 


4.1888 


14.137 


33.610 65.450 113.10 


179.59 


268.08 


381.70 


ir-rw 


3.1416 


1.5708 


1.0472 


.78540 .62382 .52360 


.44880 


.39270 


.34907 


n-T-'f' 


.31831 


.63662 


.95493 


1.2732 1.5915 1.9099 


2.2282 


2.5465 


2.8648 


(ir/180) . n 


.01745 


.03491 


.05236 


.06981 .08727 .10472 


.12217 


.13963 


.15708 


(180/ir) . n 


67.296 


114.59 


171.89 


229.18 286.48 343.77 


401.07 


458.37 


515.66 


e'n 


2.7183 


5.4366 


8.1548 


10.873 13.591 16.310 


19.028 


21.746 


24.465 


Mn 


.43429 


.86859 


,1.3028 


1.7371 2.1714 2.6057 


3.0400 


3.4744 


3.9087 


(l-r3f).n 


2.3026 


4.6052 


6.9078 


9.2103 11.513 13.816 


16.118 


18.421 


20.723 


\-7-n 


1.0000 


.50000 


.33333 


.25000 .20000 .16667 


.14286 


.12500 


.11111 


n3 


1. 


4. 


9. 


16. 25. 36. 


49. 


64. 


81. 


n8 


1. 


8. 


27. 


84. . 125. 216. 


343. 


512. 


729. 


n* 


1. 


16. 


81. 


256. 625. 1296. 


2401. 


4096. 


€561. 


n6 


1. 


32. 


243. 


1024. 3125. 7776. 


16807. 


32768. 


59049. 


26.2* 


64. 


128. 


256. 


. 512. 1024. 2048. 


4096. 


8192. 


16384. 


3» 


3. 


9. 


27. 


81. 243. 729. 


2187. 


6561. 


19683. 


V7i 


1. 


1.4142 


1.7321 


2. 2.2361 2.4495 


2.6458 


2.8284 


3. 


3,- 


1. 


1.2599 


1.4422 


1.5874 1.7100 1.8171 


1.9129 


2. 


2.0801 


n! 


1. 


2. 


6. 


24. 120. 720. 


5040. 


40320. 


862SS0. 


l^n! 


1. 


0.5 


.16667 


.04167 .00833 .00139 


.00020 


.00002 


.000003 


^»* 


l-r6 


1. 


1^30 


5. 1-^42 61. 


l-r30 


1385. 


6-7-66 


cm. in 71 in. 


2.5400 


5.0800 


7.6200 


10.160 12.700 16.240 


17.780 


20.320 


22.860 


in. in n cm. 


.39370 


.78740 


1.1811 


1.5748 1.9685 2.3622 


2.7559 


3.1496 


3.5438t 


m. in n ft. 


.30480 


.60960 


.91440 


1.2192 1.6240 1.8288 


2.1336 


2.4384 


2.7432 


ft. in 71 m. 


3.2808 


6.5617 


9.8425 


13.123 16.404 19.685 


22.966 


26.247 


29.527 


km. in n mi. 


1.6093 


3.2187 


4.8280 


6.4374 8.0467 9.6661 


11.265 


12.875 


14.484 


mi. in n km. 


0.6214 


1.2427 


1.8641 


2.4855 3.1069 3.7282 


4.3496 


4.9710 


5.5923 


kg. in n lb. 


.45359 


.90719 


1.3608 


1.8144 2.2680 2.7216 


3.1751 


3.6287 


4.0823 


lb. in n kg. 


2.2046 


4.4092 


6.6139 


8.8185 11.023 13.228 


15.432 


17.637 


19.842 


1. in 71 qt. 


.94636 


1.8927 


2.8391 


3.7854 4.7318 6.6782 


6.6245 


7.6709 


8.5172 


qt. in 71 1. 


1.0567 


2.1134 


3.1700 


4.2267 6.2834 6.3401 


7.3968 


8.4634 


9.5101 



* Bn = nth Bernoulli number ; see II, E, 15-18, p. 8, 
1 Exact legal values in U. S. 



INDEX 



[Numbers in roman type refer to pages of the body of the book; those in 

italics refer to pages of the Tables.] 



Absolute value, 14. 

Acceleration, 60, 62; angular, 72; 
component, 63; of a reaction, 78; 
tangential, 60; total, 63. 

Algebraic functions, 24, 41. 

Amplitude of S. H. M., 126. 

Analytic geometry, formulas, 16. 
See also Curves. 

Anchor ring, 11. 

Annuity, S. 

Approximate integration, 193, 47. 

Approximation. See also Error, La- 
grange, Prismoid, Simpson, Tay- 
lor. 

Approximations, formulas for, 4'^: 
polynomial, 234, 255, SO; Simpson- 
LaGrange, 31; Taylor, 30; trigono- 
metric, 5, 31. 

Area, polar coordinates, 149; of a 
surface, 302 ; surface of revolution, 
137, 200. 

Areas, 90, 215, 4^. 

Astroid, ^6. 

Asymptotes, 188, 189. 

Atmospheric pressiu*e. 111. 

Attraction, 232, 50. 

Average value, 224, 231, 49, 

Bacterial growth. 111. 
Beams, 71, 213. 
Bernouilli numbers, 60, 
Binomial differentials, 184, 4^. 
Binomial theorem, 269, 7. 

Cardioid, 136, 26. 
Cassinian ovals, 29. 
Catenary, 108, 137, 22. 
Cavalieri's Theorem, 202. 



Center of gravity, 224, 225, 226, 49. 

Center of mass, 49. See also Center 
of gravity. 

Center of pressure, 231. 

Centroid. See Center of gravity. 

Chance, 6. 

Circle, 9, 15. 

Circular measure, 119. See also 
Radian. 

Cissoid, 229, 28. 

Coefficient of expansion, 114. 

Combinations, 6. 

Compound interest law, 110. 

Concavity, 65. 

Conchoid, 28. 

Cone, 11. 

Confocal quadrics, 310. 

Constants, 1; of integration, 313; 60. 

Continuity. See Fimctions, con- 
tinuous. 

Contour lines, 27. 

Conversion tables, 60. 

Cooling, in fluid. 111. 

Critical point, on a surface, 291. 

Critical points, for extremes, 53. 

Cubes, table of, 57. 

Curvature, 139, 154; center of, 142; 
radius of, 141. 

•Curves, 19, see also Functions; cubic, 
27; parabolic, 15, 19, see also 
Polynomials; quartic, 27. 

Curvilinear coordinates, 299. 

Cycloid, 136, 143, 24. 

Cylinder, 10; projecting, 299. 

Cylindrical coordinates, 233. 



Damping, of vibrations, 24» 
Definite integrals, 46> 



ai 



62 



INDEX 



Depreciation, 6. 

Derivative, 19; of a constant, 25; 
of a function of a function, 31 ; of a 
power, 25, 27, 34; of a product, 30; 
of a quotient, 28; of a sum, 25; 
logarithmic, see Logarithmic; par- 
tial, 274, 18; total, 278. 

Derivatives, notation for, 19; second, 
61; of inverse trigonometric func- 
tions, 128; of exponentials, 107; of 
logarithms, 103; of trigonometric 
functions, 120, 121. 

Derived. curves, 68. 

Determinant, 5. 

Difference quotient, 6. 

Differential, partial, 283; total, 279. 

Differential coefficient, 19. 

Differential equations, 82, 127, 311; 
exact, 325; extended linear, 323; 
higher order, 338; homogeneous, 
317, 329, 338; linear, 320; linear, 
constant coefficients, 338; non- 
homogeneous, 332, 340; ordinary, 
311; partial, 311; second order, 
326; separable, 316; special types, 
334; systems of, 342. 

Differential formulas, 44, 132, 15. 
See also Derivatives. 

Differentials, 43; exact, 325; notation 
for, 43; transformation of, 18. 

Differentiation, 20; formulas for, 
35, 44, 132, 15. 

Direction cosines, 16. 

Distribution of data, SO. 

Electric current, 114, 277. 

Elimination of constants, 312. 

Ellipse, 9, 15. 

Ellipsoid, 11, 14' 

Elliptic functions, 55. 

Elliptic intervals, 183. 

Empirical curves, 234. 

Energy integral, 337. 

Envelopes, 284. 

Epicycloid, ^5. 

Epitrochoid, £4- 

Equations, differential, see Differ- 
ential; in parameter form, 32, 
see also Parameter ; solution of, 4- 

Error curve, SO, 



Errors, of observation, 50, 
Evolute, 142, 145, 286. 
Explicit functions, 40. 
Exponentials, 107, 22, see also 

Logarithms; differentiations of, 

107; table of, 54. 
Exponents, S. 
Extremes, 52, 257, 290; final tests 

for, 54, 66, 294; weak, 291. 

Factors, 4- 

Falling bodies, 87, 208. 

Family, of curves, 21. 

Finite differences, 248. See cUso 

Increments. 
Flexion, 61. 
Flow of water, 308. 
Fluid pressure. See Water pressure. 

Atmospheric pressure, etc. 
Folium, 41, 28. 
Force, work done by, 50. 
Fourier's theorem, 8, SI. 
Frustum, of a cone, 11; formula, 96; 

of a solid, 95. 
Functions, 1; continuous, 11, 15; 

derived, 19; notation for, 1; 

implicit, etc., see Implicit, etc.; of 

functions, 31; algebraic, rational, 

etc., see Algebraic functions, etc.; 

classification of, 24. 

Gamma function, 56. 

Gases, expansion of, 38, 48, 78, 105, 

110, 50. 
Geometry, of space, 16. 
Graphs, 2. 

Gudermannian, 131, IS. 
Guldin and Pappus, Theorem, 4^. 
Gyration, radius of. See Radius. 

Harmonic functions, 23. See also 
Trigometrio. 

Helicoid, 300. 

Helix, 300. 

Hooke's Law, 125. 

Hyperbola, 10, 15. 

Hyperbolic functions, 108, IS, 22, 54, 
inverse, see Inverse. 

Hyperbolic logarithm. See Loga- 
rithms. 



INDEX 



63 



Hyperboloid, 33. 
Hypocycloid, S6. 
Hypotrochoid, SS. 

Implicit functions, 40. 

Improper integrals, 190. 

Increments, 4, 248; method of, 238; 
second, 239, see also Finite 
differences. 

Indeterminate forms, 259, 262. 

Inertia, moment of. See Moment. 

Infinite series. See Series. 

Infinitesimal, 14; principal part, 261. 

Infinitesimals, higher order, 261. 

Infinity, 16. 

Inflexion, point of, 65. 

Integral, as limit of sun, 192, 197; 
fundamental theorem, 86; in- 
definite, 83; notation for, 83. 

Integral curves, 313, 343. 

Integrals, definite, 87, 4^; double, 
210; elliptic, 183, 9, 66; improper, 
190; infinite limits, 188; infinite 
integrand, 189; multiple, 208, 215; 
table of, 36; triple, 208. 

Integral surfaces, of a differential 
equation, 343. 

Integrand, 83. 

Integraph, 243. 

Integrating factor, 325. 

Integration, 83; approximate, 193, 
see also Approximation; by parts, 
163, 36: by substitution, 158, 36, 
43; formulas for, 156, 36; of a 
sum, 84; of binomial differentials, 
184, 4U of irrational functions, 
129, 39; of linear radicals, 172, 39; 
of polynomials, 84, 158; of quad- 
ratic radicals, 173, 39; of rational 
functions, 165, 36; of trigonometric 
functions, 157, 172, 177-182, 41; 
reduction formulas, 184, 4^^ 4^! 
repeated, 208; successive, 209. 

Interpolation, Lagrange's formula, 
16. See also Lagrange. 

Inverse functions, 3. 

Inverse hyperbolic functions, 131, 

14, 64. 
Inverse trigonometric functions, 128. 
Involute, 146. 



Irrational functions, 25; differen- 
tiation of, 34; integration of, 164, 
172. 

Isothermal expansion, 105. 

Kinetic energy, 231. 

Lagrange interpolation formula, 16^ 

47. 
Law of the mean, 247, 47; extended, 

253, see also Taylor's theorem. 
Least squares, 58, 296, 309, 0. 
Lemniscate, S9. 
Length, 133, 4^; polar coordinates, 

152; of a space curve, 305. 
Limits, 14; arc to chord, 133; proper- 
ties of, 15; sin 6 to 0, 119. 
Liquid pressure, 50. 
Logarithmic derivative, 115. See ' 

also Rates, relative. 
Logarithmic plotting, 234, 20. 
Logarithms, computation of, 7; 

graph of, 21; hyperbolic, 102; 

Napierian, 102, 64; natural, 102; 

rules of operation, 99, 3; table of, 

62. 

Maclaurin's Theorem, 258. See also 

Taylor's Theorem. 
Mass, 49. 

Mathematical symbols, 1-3. 
Maximum, 6. See also Extremes. 
Mean square ordinate, 231. 
Mensuration, 9. 

Minimum, 6. See also Extremes. 
Modulus, of logarithms, 103. 
Moment of inertia, 219, 221, 49; 

polar coordinates, 220. 
Motion. See Speed, Acceleration, etc. 

Napierian base e, 102. See also 

Logarithms. 
Natural logarithms. See Logarithms. 
Normal, 5, 49; length of, 50; to a 

surface, 298, 300. 
Notation, 1. 
Numbers, e, M. See Logarithms. 

Organic growth, law of. 111. 
Orthogonal trajectories, 325. 



64 



INDEX 



Pappus Theorem, 49, 

Parabola, 10, See also Curves, 

parabolic. 
Paraboloid, 11, 34-, 
Parameter forms, 32, 50, 134. 
Partial derivative, 274, see dUo 

Derivative; order of, 275. 
Partial derivatives, geometric inter- 
pretation, 277; transformation, 18, 
Partial differential. See Differential. 
Partial fractions, 165. 
Pendulum, 127, 238, 250. 
Percentage rate of increase, 112. 

See also Rates. 
Period, of S. H. M., 126. 
Permutations, 6. 
Phase, of S. H. M., 126. 
Plane, equation of, 16, 
Planimeter, 243. 
Point of inflexion, 65. 
Polar coordinates, 5, 147; plane area, 

216; moment of inertia, 220; space, 

300. 
Polynomial, approximations. See 

Approximations. 
Polynomials, 24, see also Curves, 

parabolic; differentiation of, 25; 

roots of, 65; integration of, 84, 158. 
Power cvirves, 19. 
Power series. See Taylor series. 
Primitive, of a differential equation, 

313. 
Prism, 10. 

Prismoid, defined, 205. 
Prismoid rule, 202, 10, 47. 
Probability, 6, see also Least Squares, 

Error curve, 30; integral, SO, 56, 
Psrramid, 10, 
Pythagorean formula, 134. 

Quadric surfaces, 33; confocal, 310. 
Quartic curves, ;?7. 

Radian measure, table of, 61, 68, 

Radium, dissipation of, 114. 

Radius of curvature. See Curvature. 

Radius of gjn-ation, 220, 50. 

Rates, average, 18; instantaneous, 
19; percentage, 112; related, 74; 
relative, 112, 114; reversal of, 79, 
see also Integrals; time, 10, 60, 



Rational functions, 24; differenti- 
ation of, 28; integration of, 165. 

Reactions, rates of, 78, 114. 

Reciprocals, table of, 57, 

Reduction formulas, 179, 185, 41- 

Relative rate of increase, 112, 114. 
See also Rates and Logarithmic 
derivative. 

RoUe's Theorem, 247. 

Roulettes, ^4, 

Semi-logarithmic plotting, 236. 
Series, alternating, 270; convergence 

tests, 266; differentiation of, 272; 

geometric, 265, 7; infinite, 7; 

integration of, 272; precautions, 

269; Taylor, 266. 
Simple harmonic motion, 124, 328, 

^3. 
Simpson-Lagrange approximations, 

31. 
Simpson's rule, 207, 47, 
Singular solution of a differential 

equation, 313. 
Slope, 4. 

Solution of equations, 4- 
Speed, 9, 60, 62, see also Motion; 

component, 10; angular, 72; total, 

42, 134; of a reaction, 78. 
Sphere, 11. 

Spherical coordinates, 232, 300. 
Spirals, 3$. 

Square roots, table of, 58, 
Squares, table of, 57, 
Strophoid, ^7. 
Subnormal, 50. 
Subtangent, 50. 
Summation, approximate, 193 ; exact, 

196. 
Summation formula, 197. 
Surfaces, quadric, 33. 

Table of integrals, 156, 36, 
Tables. See special titles. 
Tangent, equation of, 5, 49; length 

of, 50; to a space curve, 305. 
Tangent plane, to the surface, 289, ' 

297, 300. 
Taylor series, 266, 30, 



INDEX 



65 



Taylor's Theorem, 263, 8, see also 

Law of the Mean. 
Time rates. See Rates. 
Total derivative, 278. 
Total differentials, 279. 
Tractrix, e6. 

Trajectories, orthogonal, 325. 
Transcendental functions, 25. 
Trapezoid rule, 47- 
Trigonometric functions, table of, 

12, 21,61. 
Trigonometry, 9, 
Trochoid, 24- 



Variable, 1; dependent, 1; inde- 
pendent, 1. 

Velocity, 60. See also Speed. 

Vibration, 125, 23; electric, 125. 

Volume, of frustum, 95, 199; of solid 
of revolution, 94. 

Volumes, 94, 95, 210, 48. 



Water pressure, 201, 231, SO, 
Witch, 28. 

Work, of a force, 60; on a gas, 105, 
110. 



ANSWERS TO EXERCISES 

§ 6. Page 9 
1. y = 2aj-3. 8. 8x — 2/ = ll. 6. 3x-y = 2. 7. 3x+y = 4. 

§ 9. Page 12 

8. 82 ; 114 ; 178 ; 50 + 32 T. 6. 2 ; 6 ; 40 ; 2 T. 7. 80 ; 16 ; - 80. 
9. « = 5/2 ; 8 = 100 ; c = 0. 11. 1 ; 2 « ; Vl+TPT 

§ 11. Pages 17-18 

6. 9. 7. -5/12. 9. ^-1/2. 11. (a + b)/(c + d). ' 18. 1. 

15. 0. 17. 3/5. 19. - 1/2. 23. 5/3. 26. 2. . 27. Va/p. 

§ 14. Pages 22-23 

1. 2x-4. 3. 3-3x2. 5. 8-4x3. 7. - l/(x - 1)2. 

9. -2/x3. 11. 8/(x + 2)2. 13. 4x + 9y = 24. 16. Rises 

when I X I > \/5~; falls when | x | < V5 ; slope zero when x = ± V6. 
17. Rises when x > 2 ; falls when x < 2 ; slope zero when x = 2. 
19. Hor. speed, dx/dt = 15 ; vert, speed, dy/dt='^ 32 1 + 15. 
21. 8irr; 3 a2 ; 2 irrA/3. 

§ 16. Pages 27-28 

1. 12 x3. 8. 20 x4. 6. 50 (t* + 1). 7. 12 t(t^ - 1). 

9. 18 t\l + «3). 11. 6 r (3 r + 2). 13. 2v- 1. 16. 11 rW + 12 vK 
17. 13 ayi2 _ 9 aby^. 19. mfcx«-i + nAx"-i. 21. 3 n«3n-i — (n + 2)e»+i. 
23. (-2, 0). 26. (1, 6). 27. Slopes at x = 0, 2, - 2, 4, - 4 resp. 
are 0, 12, 36, 72, 120 ; slope is 9/2 at x = 3/2 and - 1/2 ; slppe is - 3/2 
at X = 1/2. 

§ 17. Pages 29-30 

1. -l/x2. 8. 6/(x + 4)2. 6. -9/x4. 7. -28x-8-4x-3. 

9. - («4 + 2 t)/(«3 _ 1)2. 11. 4 w/(u2 _ 1)2. 18. 16/3 ^ 1/^2. 

16. 0. 17. - 6/2* - 6 2/(z2 + 1)2. 19. 2(1 - r^)/(r^ - r + 1)«. 
21. 3(l-6y2 + 2 2/3)/(«3_i)2. 28. - 6 fT -{- S tr^, 

26. -(r6+3i32)/(«4_i)2. 27. -x/(a» + 6)3. 

29. (y2-2)/(y-l)4. 31. tan-i(-3). 

1 



2 ANSWERS 

§ 20. Pages 33-34 

1.6JB2-2. 8.4X + 3. 5. 12x2-5x4-2x. 7.4x(a;«-l). 
9. 6x«(x«-3). 11. 24x(3a;S + 6)3. 18. 4(1 - 30(H-2«-3<?). 
16. 3(3 «2 - l)(«3 _ t - 4)«. 17. 8(2 rs + 3 v)(v^ + 3 u* - 2). 

19. -6 «V(«' + !)'• 21- (6a;2 - 3 x* - 18x)/(x2 + 2)1 

28. - 8 8(2 82 - 3)-3. 25. 6(2 + 4 «2 - 5t))(3r - 5)(tj2 + 2)2. 

27. 6^6+12 «H 12 «2+12. 29. 166-108X. 81. (2/5)[3(l-2x)-«+8]. 
88. 3/(2 «). 85. Horiz. tangents at X = 1/2, —4/3, -6/12. 

§ 23. Pages 37-38 

1. (4/3)xi 8. (4/3)x"*. 6. (3/4)x"^. 7. -6x-2-5x"** 

9. (22/3)«* + 7 t^. 11. - 6x-4 - (l/2)x^ + (2/8)x"i. 

13. ^ . 15. A±^. 17. -ll^ll 

2V2 + 3X 2V2 + 3U 

19. -^^-.- 81. lg''-l«^. SS. 



8(l + ««)* 2V3a;-4 

, ^ • 27. ''-^°' . 

4^x + xVx 2u2Va2-u 



2Vt2_3t 


2x-l 


2 VI -XH-X2 


«-3«3 


Vl -<2 



81. 2(xj- VI + x2)2/ Vl + x2. _ Tangents: 88. 3x + 4y=5. 

85. 2V2y - X = 2. 87. 2 V2y = 5x - 1. 89. tan-i(5/12). 

41. dp/du=-1.41fcu-2.4i. 

§ 25. Pages 41-42 

1. - 2 y/x or - 2/x«. 8. (2 X — y)/x or 1 + 6/x2. 

5. x/4i/orx/(2Vx2-36). 7. - x2/2/2 or - x2/(a» - x»)i 

9. 3(1 - x2)/(2 y) or 3(1 - x2)/2V3x-x3. 

11. (2 X - 2/2)/(2y + 2xy) or (2 + x)/2(l + x)i 18. - y/x. 

15. l/(2y). 17. -Vy/x. 19. 4«;2y = x2. 

21. « ; 27 y2 = 4(x - l)s. 23. (<2 - 1)/( 2Q ; x' + y2 = i. 

27. dy/dx > when x < and v .v. 29. o = (1/2) V2 + 2«2. 

§ 27. Pages 46-48 

1. (2ax + 6)dx. 8. 3(2ax-|-6)(ax2+6x+c)2dx. 5. -a(axH-6)-2dx. 
7. -(12t + l)d«. 9. «(a - 0K2 a - 5 t)d<. 11. (S - 2 t)dt/2VSt^. 

18. (9/2)Vt«-3«(t2-l)dt. 15. -(l+r)diV(2i5 + i?*)*. 

17. -(l+r)(2 + 3i?2 + a?8)d«/(t?3-.l)2. 19. 42/2(2 -.yS)-!^^. 



ANSWERS 3 

21. (l/2)(2H-y)(l + y)"W 28. 6nps«-i(a + 6««)P-ids. 

25. - 6np«»-ids/(a + 6«»)p+i. 27. cte/[>/x(l - Vx)2]. 

29 y^ 81. (2^^~^^-^)<^ . 33. q(g^ +y^)dg 

^ 1 — X * y + «^ * 2 y (1 — oaj) * 

35 (3^2 + 20x4- y)dx, 37 y + 6x = ll. 48. Vt72. 

2i/(a— 6x) 

45. -(2 + ^) (1 + ^)2/^. 47. 9/(2 r). 49. 2(1 - <2)/(i + ^)2 ; 

- 4 V(l + *2)2 ; 2/(1 + t2). 51. dc = (6 - tj)di)/(p - a/tj2 + 2 a6/tj3). 

§ 31. Page 52 

Tang. Norm. Subt. Subn. Tang. Norm. 

1. 9x + y = 5. x-9y = 37. 4/9. 36. 4v^/9. 4V^. 

8. 9x + 4y = 25. 9y-4x = 32. 16/9. 9. 4^97/9. V97. 

5. x + 32/=:6. 3x-y = 8. 3. 1/3. VlO. VlO/S. 

7. y = 3. X = 4. GO . 0. 00 . 3. 

Tangents : 9. y + y^ = 2 AxcXq. 11. xxq + Wo = «*• 18. ft^xx^ ± a2j/yo 
= a262. 15. axXo+ 6(xyo + Xq?/) + cyyo + ^i^ + «o) + e(y + Vo) +/ = 0. 



35. Pages 56-59 

1. 8. 5. 7. 9. 

Max. x = 0. q=i—\, y = 0. n = l. t = 2/3. 

Min. x = 4. q = 6, y =± V2. n = 3. t = 1. 

11. 18. 15. 17. 19. 

Max. 8 = 0. None. x = 4. (1 ± V6)/2. r = 2. 

.Min. « = ±V572. x = -2. x = 0. (-l±\/6)/2. r=-2. 
21. A square ; area 400. 88. (d: 7, d: 7). 25. Ht. = diam. 

27. Width = 2 X depth. 29. Depth = V3 x breadth, 81. x/6+y/8=l. 
88. Max. 3 ; Min. 1 : the variable x does not increase steadily when the 
function D^ goes through its minimum or maximum, as the general 
theory requires. 39. Compromise: 42^ a foot; average: 42.56^ a 
foot. 45. Width = 1/2 x base of A. 47. Height = (2 v%/3) x radius 

of sphere. 49. Rad. = V(6 + V5)/10 x radius of sphere. 51. 2 ab. 

§ 40. Pages 64-65 

1. 2x + 5, 2. 8. 4x-l,4. 5. 2x-6/2, 2. 

7. 6(x2 + x-6),6(2xjfl). 9. 4x3- 6 x2+ lOx , I2x»-12x + 10. 

11. 1/2 Vx + x/Vx2 + l, - l/(4\/x3)+ 1/V(x2 + 1)3. 

18. (X + 2)2(5x2 + 4x - 3), 2(x + 2)(10x2+16x + l). 16. a, 0. 



4 



ANSWERS 



17. 2 ox +6, 2 a. 19. [m(x — 6) +n(x — a)](a; - a)"»-i(aj — 6)»-i, 

[m(m — l)(x — 6)2 + 2mn(x — a)(x — 6)+ n(Ti— l)(x— a)^] 



X (X — a)'»-2(x - 6)'»-2. 

27. m = 2(3x»-7x-13)(x + 3)(x-2)2 

-llOx-10). 

88. 85. 

d/b. - 2 r3. 

0. 6 r -». 

6. 1. 

d. - 2 t-K 

V6« + (P. 

0. 

0. 

0. 



m 
6: 

V : 

J- 



Ji 



0. 



0. 
-12M 



25. m = -l/x2, 6 = 2/x3. 
6 = 2(x-2)C15x»— 10x2 

87. 

-(1 + t)ytK 

2(1 + 0V«'- 

(1 + t)-K 

-«-2. 



Vt2 + 4 



-2(1 + «)-'• 

2r«^ 

2 V(l + «)-« + t-« . 



8. 

Max. X = — 1. 

Min. X = 5. 
Infl. X = 2. 



§ 44. Page 70 

5. 

- 11/6. 

5/6. 

-1/2. 



9. 



7. 
0. 

±1. 
11. 

None. 
None. 

None. 



Max. - B/(2 A), A<0; none, ^ > 0. 
Min. None, ^ < ; - B/(2 A), A >0. 

Infl. None. 

28. 2/ = 3x2 + ox + 6; xV3 + 3x2/2 + ax+b; ox + 6. 

27. 29. 

Infl, None. x = 3 1/4. 

Max. Defl. x = ± Z/2. x = 2(1 + V33)/16. 



18. 

None. 
-2. 

2^. 



§ 46. Page 73 

1. w = 3 <2/l000 degr./sec. ; a = Q t/lOOO degr./sec.«. 
8. w=(-«3/4-l/32) rad./min. =[-«3/(8T)-l/(64ir)]rev./min. 

= (- <3/240 - 1/1920) rad./sec. 
a =— 3«2/4 rad./min.2 = - 3 tys v rev./min.2 =— t2/4800 rad./sec.2. 
7. (ir/720)(«2 - ««/46) ft. /sec. ; (ir/860)(t - t2/30) ft./sec.2. 



ANSWERS 6 

§47. Page 76 

1. 1026/(2304 r) ft./min. 3. Inversely as the cross-sections: 

dhldi : dh'/dt = r'* : r^. 5. Inversely as areas of liquid surfaces ; their 

dV dP 1 
ratio varies as the area of remaining liquid; 5 =- r'cota; 

dt dt 2 
a = half -angle of cone, r =: radius of liquid surface in the funnel. 

7. (fc/4) VS/e" cu. in./sec. 9. dy/d« = 4(4x - 1) ft./sec.; 

12 ft. /sec. ; 44 ft./sec. 11. Vy = 3 x^u, = 30 as* ft. /sec. ; 1080 ft. /sec. 

13. 8/V5 ft./sec. ; 4/\/5B ft. /sec. 15. 4 ft./sec. ; Nearly 312 ft./sec. 
17. = 17** 41', 16° 18', 10° 22' ; max. h. = 62600 sin* 20° ft. 

§ 50. Page 82 

1. 2a5* + c. 3. x» + c. 6. -2x3 + c. 7. — xV6 + c. 9. 5xV2 
+ 4x + c. 11. a = ty4 — 2 «2 4- 7 « + c. 13. y = axV2 + bx+c. 

15. y = .002x8-. 001 x4+.003x» + c. 17. y = -x-V2 4-c. 

19. »=-3/«-2/«* + c. 21. 2/=(4/3)x*-6xi + c. 

§ 51. Tage 85 

1. y = J(4 X* + 3 x)dx = 4 x'/S + 8 xV2 + c. 
3. y = Jx-«dx=— X-V2 + c. 5. y = J(4x + 6)dx = 2x2 + 5x + c. 

7. y = J9(Jx = 9x + c. 9. y= /(x* — x*)(ix =xV4 — xV6 + c. 

11. y = J(x + Vx) dx = xV2 + 2x*/3 + c. 13. xV2 + 6x + c. 

15. 3x*- 9x5/6 + c. 17. 16x + xV2- 2x3/3 + c. 

19. 2x*-4x*/6 + c. 21. 2x^/7 -2xV^ + c. 

23. x + 3x*/2 + 3x^/6 + c. 26. 4 tJ/7 + c. 27. 3u*/2-2Vu+c. 

29. - l/t» - 1/(2 «*) + c. 31. 6 «*/8 + 6 «*/2 + c. 

33. 3y"V/i3«6yJ/7 + c. 35. 12\/y+c. 37. 3u*/8 + c. 

39. x*/2 + (2/6)x*+ c. 41. t»/3-tV6 + c. 48. ax*/2 + 6x»/3 + c. 
45. ax*+i/(n+l)+6x"+V(« + 2) + c. 47. - t-i'Vl-^ + *^/2 + c. 

49. (2/3)«*+(4/7)«* + c. 

§ 54. Page 88 

1. 3000 gal. ; 1600 gal. 3. s = tV^ + c ; 4 ; 76/4. 5. 46/(8 r) . 

333/(200ir). 7. 16/6. 9. -940/3. 11. 22/3. 13. -1899. 

15. 7 a/8. 17. 0. 19. 10a»/3. 21. 729/6. 23. -2. 25. 28/3; 

27. .0002 29. 226/4. 31. s = flftV2 + 10 « ; 770. 33. lOflf; no. 



6 ANSWERS 

§ 55. Page 93 

1. 1/3; 21. 8. 2/6; 62/6. 6. 2/3 ; - 18. 7. 2(2V2-l)/3 ; 

2(5V6-2V2)/3. 9. 1/4; -226/4. 11. 6/6; (6/6)al- 18. 15/2. 
16. 32. 17. 11/6. 19. 8/3. 21. 1/3. 

§ 57. Page 97 

1. 128 7r/7; 2ir/7. 8. 856ir/106; 167r/105. 

5. For upper half of curve : For lower half of curve: 

0to2; (14/3 + 4V3)t. (22/3 - 4 V3)ir. 

- 1 to 1 ; 4 ir(l + 2 V2/3). 4 ir(l - 2 V2/3). 

7. 296ir/81; tt (3x* - 6x2 - l)/3a;8]J. 9. 8ir ; ir(x* + 3)/3x]». 

11. 4ir. 18. 778ir/6. [15. (2ir/21)(21 + 14V2 + 24v^8). 

17. 32 ir; 48 tt; 2ir(62-a2). 19. 4irahyS; 4ira26/3. 21. 20ir/3. 

28. 8V3/6; 2k/ VS. 26. Trkr^hy2i 2irkr^^h, 

§ 60. Page 101 

16. Iogio7/logioll= 0.812 17. 186.4± 19. 3.479 21. 2.862 

§ 65. Page 106 

1. i^. 8. _A^. 6. — — 7. — . 9. 2 + 21og«. 

X l + 2x l+x X 

11. ^ 18. LllMi. 15. Ml^gOf. n. . .713 

2-6t + 3^ ^ St 

19. 160.693 21. 2(e3-2)/3 + (e-2-l)/6. 28. 0.219 

25. 2.302; log A:. 27. — X"*. 29. Max., none; Min., x = l; Infl., 

none. 81. Max., none; Min., x=±2; Infl., none. 88. 11.416 

85. -0.396 87. 6.693 89. A:2 1ogc. 

§ 67. Page 109 

1. 3e3«. 8. e^i+^/(2\/rri). 5. e*(2x+x2). 7. (3 log 10)103«-m. 

9. I. 11. -2x. 18. 2e«(6* + l). 15. (e^^ + e^^)/4v^. 

19. 10.02 ; 2.36 ; sinh a. 





21. 




28. 


25. 


Max. 


None. 




None. 


x = l. 


Min. 


x=-l. 




None. 


None. 


Infl. 


x=-2. 




x = 0. 


x = 2. 


29. 0.632 


81. 1.381 


88. 


(eio _ e-io)/8 - 5, 


/2. 85. 26.762 



ANSWERS • 7 

§ 69. Page 113 

1. 21 e3» ; 3. 8. (1 4- aJ)e» ; (1 + aj)/x. 6. 4 e^^+s ; 4. 

7. (Jkoa; + fe6 + a)e*» ; (kax-\-kb + d)/(ax-\-b), 
9. (3-4»-6x2)e-«'; (3 -4a; - 6aj2)/(3aj + 2). 
11. About 963 sec. after ^ = 40°. 

13. k = (1/5830) log (6/4) ; (1/1909) log 1.27 ; 26.7 in. ; 672 min. ; 1806 
ft. ; 1266 m. 16. 60 log 2. 

§ 71. Pago 117 

1. - 2. 8. 3. 5. 10. 7. - 2 X + 3 kxK 9.-2 r^/(r^ + 1). 
11. [3(1 - <2 + t4) (t2 + 1) log 10 - 2 « + 4 t3]/(l - t3 + t4). 
13. [1 + log(l + X) ] (1 4- xy+'. 16. xV^=V2(i + log Vi). 
17.6 + 22x4-18x2. 88. A;e*-«'/2. 36. &x». 87. fee**. 

§ 74. Page 122 

1. 4 cos 4. 3.-2 sec22 ^. 6. 4 x« cos x\ 7. — 3 sin 3 ^. 

9. cosx— xsinx. 11. tanx. 18. cos x 4- 3 sin 2 x. 

16. 2xsin(3-2x)-2(l 4- x^) cos (3 - 2 x). 

17. e' cos (3 « - 1) [cos(3 t - 1) - 6 sin (3 « - 1)]. 

19. e«/io[(l/10)(co8i-4sin3 0-(sin«4.12cos3«)], 21. 1. 

Maximum Minimum Points of Inflexion 

23. X = 2 WTT 4- ir/2. 2 nir — ir. nir. 

26. none. none. mr, 

27. nir — 7r/4. nw 4- ir/4. nT/2. 
29. 2 nir 4- ir/4. (2 n 4- l)ir 4- ir/4. nir. 

81. nir - ir/12. (2 n 4- l)ir/2 - ir/12. (2 n 4- l)ir/4 - ir/12. 

83, 86, 37. The functions differ at most by a constant. 

89. 2. 41. -(l/2)cos2x4- fe. 48. sec t+k. 

46. sin X — (3/2) cos 2 x 4- k, 47. (1/2) sin 2 x — x 4- fc. 

Vg Vjf V Path. 

63. — 6 sin 2 «. 6 cos 2 1 6 x'^ + y^ = 9. 

56. cos t — sin L cos t. Vl — 2 sin t cos t 4- cosH. z^ — 2xy + y^=zl, 
67. — 2 ir ft. /sec. ; ± ir V^ ft. /sec. 

§ 76. Page 126 

1. 2 cos 2 £, — 4 sin 2t. 8. cos £ — cos 2 £, — sin 1 4- 2 sin 2 1 

6. 2cos2«4-0.9cos6«, — 4sin2 « — 6.4sin4^ 

7. ak cos (kt 4- e), — aA:2 sin (kt 4- e). 

9. cP^/d«2 = - 20 ir2 sin 10 irt ; 0.2; 1/6; ±20ir2. 28. a; ak cos kt. 

26. S. H. M. because cP0/dt^ = - k'^B, 



8* 



ANSWERS 



1. 



4x8 



9. 
15. 



1 



8. 



§ 79. Page 130 

-1 e -1 



6. 



^y/x^ - 1 



(l + x«)tan-ix 



11. 



X' 



l + 4x 



4-2xtaii-i2v'x. 



18. 



VI — C2"*°* 



17. 



19. 



e 



— 2g 
l + x* 

-1 

l + aj« 



21 3(logtan-igy 
(H- a;2) tan-i « 
27. -ir/6. 



28. 



Vl-x* 

25. x/3. 



\/l-x2 

Vl — ag/2Vx + sin-i Vx 

(1 - «)* 
29. (l/2)8in-i2x. 81. -tan-i(l-x). 

88. 7r/6; ir/3. 85. ir/12 ; ir/6. 

§ 84. Page 136 

1. ViO; 2ViO; (6-a)\/iO. 
8. Vl + m2 ; 2 Vl + w*^ ; (6 — a)VH-m2. 

6. (2/3) (4 - \/2) ; (8/3)(2V2 - 1) ; (2/3)(6i - a*) V2. 

7. 9. 11. 

(to: V2(ft. 2(1 + 0^*- (1 + M)(i«. 

s: 2\/2. 99. (6 - a) + (6-«- a-»)/3. 

tJ ; v^. 2(1 + 0. 1 + 1-«. 

§ 85. Page 139 

1. 4irV6; 20irV6; 2irV6(6- a)(6+o-l). 

8. 13irv^; 447r\/l0; irViO(6-a)(36 + 3a+4). 

5. Sir; 4 IT. 7. (7r/2)(e2 + e-» + 6). 9. 263ir/64. 



§87. Page 144 



R 

(1 + 4x2) 



a 



/3 



i 



8. 



5. 



(y» -f 4 Qg) 



4a» 
(1 4- cos^x) 



— 4x8; 



3x + 2a; 



6x2+1 



2>/x7a(2a — x). 



4 



sinx 
7. coah^x; 



« + 



1 + cos* X . 



ctnx 
^ — siDhxcoshx; 



2y. 



1 + cos'x 
cscx 



ANSWERS 



9 



9. 

11. 

18. 
15. 

17. 
19. 



ib*afi + oV)* 












2Va 
3 a sin 2 9 



OB 4- 2(x + y) ^; y + 2(x + y)-^/?. 



(1 + <*) 



i 



2^3 



0; 

oco8d(l +2sin«^) 



(l/6)(9 + 4t«)*|; 2-4«8/3; 



0. 

a sin ^(1 + 2 cos« ^). 

2«8 
3 1« - 1/2. 



§ 91. Page 149 

1. tan ^. 8. - (3/4) esc ^ — ctn 0. 5.(1 + cos« $)/(2 tan &). 

7. e/2. 9. 1/2. 11. (1/3) tan 3d. 18. (1/3) tan(3d + 2ir/3). 
15. -tan(d/2).. 17. (ecosd- l)/(esind). 19. -ctn(d/2). 

§ 92. Page 151 

1. ir8/6. 8. 3»V4. 5. 12v^T. 7. 3. 9. 626/2. 11. tt/S. 
18. (V3-l)/2. 15. 4ir. 17. 4. 

§ 93. Page 154 

1. 5ir. 8. _V2(e»/2- 1). 5. tan 1 - tan (1/2)= 1.012+. 7. irV2. 
9. (e* - e») V5. 

§ 94. Page 155 

1. py/2. 8. (a/^)(l +^)'*. 5. (1 + 8 cos* 3^)^/(10 + 8 cos* 3d). 
7. (2/3) vTo^. 9. (62-a« + 2a/))*/(2 62-2a« + 3ap). 

§ 98. Page 160 

1. a; - xy2 + xys - x*/4 + c. 8. a^x + abx^ + 62x3/3 + c ; or, 

(a+6x)«/(3 6)+c'. 5. (c^* - e-2»)/2 - 2 x + c. 

7. laji-jx^ + fx^ + c. 45. .0686 47. 1/3. 49. log 3. 

51. 5 V2/12. 58. irV2. 55. Sira*. 57. Areas : 2, 1, ir/2. 

§ 99. Page 164 

19. (2 +x + 2x« + x») tan-ix-2x-xV2 +c. 
21. e*»(32x«-24x«+12x-163)/128+c. S5. 1. 27. ir/12+VS/2-l. 
. (2-3e-»)/18. 81. (l+e-»)/2.- 88. 2-6/e. 



10 ANSWERS 

§ 105. Page 170 

16. \ogi!L±^. 17. x + log^n?. 19. 1 .^c (x-2)Kx + 8) 

27. llog^ + ltan-i?. 29. llog (^ + 1)^(^- 2), 

86. log2-41og?-^. 87. - tan-i (cosx). 89. -log^ + ^. 

41. log tan (x/2) . 43. log Izii! . 45. log (e« + e-*) . ~ 

1 -f- 6* 

§ 107. Page 174 

9. (6g- -4)(l +x)i/15. 11. 2tan-iV»=^. 18. Vx"=^ + sin-iVx. 

tK Vx + 4 . , 1, Vx + 2 — 2 1 

16. -t^-+_log_^__. „. A(4x-3)(l+x)» 

19. -(3/10)(2 x+3)(l-x)* 21. (4/3)x*-.4xi + 4taii-ixi 

28. cos-ix-2V(l-x)/(l+x). 26. -9-41og2. 
27. 61og(3-Vsinx)-2VsEx. 29. (2/3) V2 + 3 tan x." 
81. -slnx -4\/sinx-41og(l -VSnx).. 83. (l-fx2)^/3. 

36. (l+x2)V6. 87. -.(flH^x2)-V6. 89. 2(a + 6x3)*/9 6. 

Ai 2y/a + 6x» -« i V4x2 4- 1 — 1 , , 

41- :^ 49. logy^±^rJ: — L 61. Vx2-.l-.tan-iVx23T. 

53. (x-Vi3:^)V2. 69. ( V^/2) log[4x + 1 + 2 V4x2 + 2x + 2]. 

61. -cos-i^ii. 63. J-iQg ^ + V3 - V x2 + 2x4-3 



V2 V3 x-V'3-V22 + 2x + 3 

2^ + 1./ . . „ . „, . 3 

8 



66- —J— VI + a; + x2 + - log (2x + 1 + 2 Vr+T+^). 



«.« 1t^^ 2x+1^ 3 

®^- 3^ "~r~-^~i6^^s(^+2* + 2i2); 12== vr+T+^. 

69. log ^=_siir:ix 

^ 1 + VI - X2 X 

^, 6x2-8x — 3 . , 3x-8 /:; = 

71. z sm-i X H z — VI — x2. 

4 4 

78. ?-^=^Vn=^ + ^^^sin-ix + x2cos-ix. 
X 2 



ANSWERS 11 

§ 111. Page 183 

cos X sin3 X . S . ^^^^ „. . 
1. __ h-(x— cosxsinx). 

4 8 

8. (1/6) tan^x— (1/3) *an3x + tanx — X. 6. (l/5)tan6x. 

tan2x . tan^x ^ ; 2ctn3x ctn^x 
7. -^ + -j-. 9. -ctnx 3 ^. 

11. — (1/2) cot2 X — log sin x. 13. — sin x — esc x. 

16. (1/2) sec2 X + log tan x. 17. x cos a + sin a log sin x. 

19. (l/3)sin3x-(l/6)sin5x. 21. -sinx-cscz. 28. sin4x(l+cos2x)/12. 

25. (l/2)cos2x-logcosx. 27. -(l/2)(cosxcsc2x + logtanx). 

29. — (l/l4)cos7x— (l/2)cosx. 

§ 114. Page 185 

■■A- '-W'-^-r.- •■ .^^.- '«'<—' 

X* „" , (*-2)« - X , I, 1+x 

7. -+3* + logJ^--^. 9. 2(l-x^)+4l°Sl^- 

1 'i'X21 -X X .3,x — 1 

^^- ^^^^l^-^ie'*^ 2- ^^- ^-2-(irzi) + ii^^5TT- 

15. llog4=|. 17. :^log^±^^". 19. 2tan-xV?^l. 
**'-8^x« + 2 4 ^x + 2+V2 

_2 2x «^ 1 „ 

21. 23. . 26. 7^a+&x3- 

oVa4- &x Vx- 1 ^ . 

27. ^ 29. l(4x-7)(3x+7)*. 

b(n -p) \/(a + 6x)»-p ^^ 

35. 12 f^-^ + ^-^+tan-i2/\ where 2/12 = X. 
\9 7 6 o y 

87. 4(3&x-4a)(a+ 6x)</(2162). 39. (4/405) (16 x +28) (3 x +7)*. 

^ +1 
2(x2+l)^2 



41. (8/66)(4x2-3a)(a + x2)*. 43. ^T^^^Tn +otan-ix. 



12(x2+3)2 ^36 V3 8(x2 + 2 X + 6) 16 2 

*^- ^^ + r6«^«-^^ "• i(4x3-21)(7+4x3)i 

68. 2x1:^1^ vi^3:T2+'^ log (x + VS^^r52). 

o o 



12 ANSWERS 



55. 



^ 57. 69. 4 8ina;-31ogtan(^ + |y 

ay/a + bx^ Sa{a + lMfi)i ^ ^' 



61. tan^-sec^. 68. _JL ipg 2 tan(^/2) + 5- V21, 

V2r 2 tan {0/2) + 5 + V21 
66. - aj - (1/3) ctn 8 x. . 67. 7/2 - 2 log 2. 

. (3/4)log(6/3)-(2/V6)tan-iV273. 



n. j.iog (8^V59)(6 + V21) ,3^^ 75. log (2 4- V3). 

77. -log(3-V5). 79. 68.7 81. 0.833 88. 0.184 

85. 4.037 87. 0.88 89. 2.274 91. 0.767 98. 0.940 

95. 0.902 97. 0.254 

§ 118. Page 195 

1. 16/3. 8. 4/6. 5. - 1.307 7. 2. 9. ir/6. 11. ir/4. 

18. V2/8. 15. 6.89 17. 0.263 19. 0.693 21. 0.746 
88. 74/3. 25. 0.346 S7. 0.650 

§ 120. Page 198 

1. 12.4 8. 17.2 5. 2 7. 0.35 9. 67.6 

11. 4; 1/2; (abs. val.). 18. 48. 15. 161. 17. 4600/ir. 

19. 3600/3 rev., 4.7 sec, nearly. 

§ 123. Page 202 

I. iraV16. 8. rabh^/S. 5. 2V3aV3. 7. kw/2. 
9. ir(e««-e-a»+4a)/4. 11. 64iraV3. 18. 32ira«/6. 15. 18,720 lb. 
17. 12,480 lb. 19. 699 lb. nearly. 21. P* = c^P. 

§ 124. Page 206 

5. 1/2 9^. 7. 232/3. 9. 90. 15. 1.099 17. 7.912 

19. 0.298 

§ 127. Page 211 

8. xV2 + ex + c'. 5. (4/16)(l - 0^ + ct + c'. 

7. e^/QO - ^V12 + ce^ + c'0 + c". 9. e« + ex 4- C. 

II. c +&U-U log u. 18. P/2 + sin e ; t^/Q — cos e -f 1. 

15. Vl + t2; (</2) VTT^ + (1/2) log (t + VTTF). 

17. 8. 19. (4/16)(6*-6* + 3^-32). 21. 32/3. 88. 1106/2. 



ANSWERS 13 

26. irr»/3. 27. 32 ir. 29. 8/9. 81. 6(4x2-Z2)/a 

88. y = A:(3 te2 - iX^)/Q. 86. y = (3 aa;2 + 6x»)/6. 
87. y = fc[loga/x)4-aj/Z-l]. 

§ 129. Page 218 

1. 26/106. 8. 363/5. 6. (68 - 1)/16 +(5io-l)/30. 7. 20477/4. 
9. 26/36. 11. 1/70. 18. 2aV3. 17. atx = 0.904 19. 1/12. 

21. V3 + 2ir. 28. V5/3 + log (1 + V2). 26. 6V6/6. 27. ir/8; 
. 3ir/2. 81. ir»/6. 88. 3ir/2. 86. 16 aVV6. 87. o^/O. 



131. Page 223 

1. 8/20. 8. 104V'2/35. 6. >/2(irV16 - 31/18) + 16/9. 

7. 17/162. 9. ikay3 ; 2 ka'^/Z. 11. k7ra^/2. 18. kva^/^, 

16. lch\b + Zb')/\2. 17. A:T(a2* - ai4)/2. 19. 5 ikay V3 ; side = 2 a. 
21. ^kir/U, 28. 36fcir/16. 26. fc7rV20. 27. 19 A;ir/4. 

29. kaK 81. 641 A;/756. 83. 846290 A;/189. 86. 21026 ik/10395. 

§ 136. Page 227 

1. 3/8. 8. 1/6. 6. 3/4. 7. 1/4. 9. 1/20. 11. 2/ir. 

18. 2 a/3. 16. 3 VS. 17. (4a/3ir, 4 6/3ir). 

19. 3 ^/4 from vertex. 21. 3 a/8 from center, on axis of revolution a. 

28. Dist. fromcenter=2asina/(3a). 25. f-^, ^-IzL^lLniV 

\e+l 4e — 4e-i/ 

27. (3/5,12/35). 29. (1,-1/2). 81. (1,0). 88. (-5/6,0). 

86. [ (24 - 6 ir2)/ir», (2 ir* - 12)/ir2]. 

§ 136. Page 229 

1. ir(aV2 + 62); a>6. 8. 3iraV4. 6. 1.558+. 7. ira62[ir/(2 a) 
-(l/4)sin(2ir/a)]. 9. 4 7rr3/3. 11. jr^aK 18. 32iraV105. 

16. ^ = log \/2 ; « = 0.6192 ; y = 0.2059 ; I = fe(x/4 - 23/48) . 

17. ^ = 3ira2; x'=ira; y"=6a/6; I = (iraV3)(8ir2 + 5). 

19. ^ = 7r(62- a2)/4 ; « = (a2 + a6 + 62)/2(6 + a) ; 1= 3 ir(6* - a*)/32. 

21. ^ = 2c/3. 28. z=3/4. 26. x = ira/2 + 64 a/(46ir). 

29. 4 7rr3(l - cos* a)/3 ; 2 a = angle of cone. 81. log tan (x/2 + ir/4). 
88. 8 a. 86. (3/10) mass times square of radius. 

87. (1/5) mass times sum of squares of other two semi-axes. 

47. 2/x ; 1/2. 49. 2 r/ir. 61. 3025 irfc/27. 68. 382812.5 ir» ft. Ib./min. 

61. IT. 



14 ANSWERS 

§ 140. Page 236 

1. 2x = 3y-ll; 4x = y + ll. 9. u = 86.2P-w«. 11. ^i = .66 «-•». 
18. d = 14.8t««. 19. y = e2«/8. 91. y = 10e-*. 98. y = 4e--2«. 

§ 141. Page 240 

1. /(x)= 0.6x2 -1.4 aj + 2.5 8. <f>(m) = m^ -^ m\ 5. P=e^'10-^^. 
7. D = 10(»-JO/« 9. 0.012 X 10-7BI «. 

11. Tungsten: C = .00000272 F»-«o ; IT = 10300 T-i**; B = 31.6 F«». 

§ 145. Page 249 . 

1. X = 1/2. 8. X = 1.88 11. About ± 40 ft. 18. About 420 ft. 

15. T changes by about 1.1 9^, 1.4 96, .06 % respectively. 

17. 0.520, 0.530, 0.541, 0.590 calories 

§ 147. Page 256 

1. tanx = x. 8. cosx = l— xV2. 

The cubics are : 6. l+x + xV2 + xV6 ; | -E^l < .000004 
7. X - xV2 + xV3 ; I ^1 < .0004 

9. e-2[l - (X - 2) + (a; - 2)2/2 - (x - 2) V6] ;\E\< .0004 
11. 1 + 2(X - ir/4)+ 2(X - 7r/4)2 +(8/3)(x - ir/4)8 ; | -E? |< .000007 

16. X - xV6 + XV120. 17. X < 5^ 50'. 

§ 148. Page 258 
1. 8. 5. 7. 9. 

Max. none. x = 1. none. (2 nir + ir/2)». 131°. 2 etc. none. 

Min. X = 0. none. none. (2 rnr — ir/2)*. 291°.4 etc. x = 0. 

§ 150. Page 262 

1. 1. 8. 3. 5. -1. 7. 2/3. 9. log (a/6). 11. 1. 

18. - 1/2. 15. 0. 17. 1. 19. log a - 1. 21. 0. . 28. 3. 
25. 4. 27. 3. 29. 1. 81. 3. 83. x. 85. 2. 87. 3/2. 

§ 151. Page 264 

1. 0. 8.-00. 5. -1/2. 7. 0. 9. 0. 11. 0. 18. 1. 
15. e». 17. 1. 19. 1. 21. 1.102 

§ 153. Page 268 

11. (V2/2)[l + (X - t/4)-(x - )r/4)V2 ! -(x - ir/4)V8 I + — ]• 
18. (X - 1) - (x - 1)2/2 +(x-l)V3-. 



ANSWERS • 15 

§ 156. Page 276 

• The answers for Ex's. 1-9 are in the order «,,, z^y, Zyy 

1, 2, 0, - 2. 8. 2 cos (x2 + y2)- 4 x^ sin (aj2 + y2), ^4xymi(x^ + 2^), 

2cos(x2 + 2,2)-4v2sin(x^ + 2^). 5. ^^^^ (J^,^ (^^,- 

7. (6aj-h2y + 4a;» + 4a;2y)e«, 2(a; + y)(l +2aJ2^)e«, 
(2aj + 6y + 4aJ2/2 + 4y3)e« ; u = «« + y*. 

yg^ga -2xy x^-y^ . 11 «^, *. 

(«2 + y2)2' (X2 + 2/2)2' (X2 4-^2)2 1, „ 

17. Area=jr; Z«= &sin C, Z^ = asin C, Kc^ahcosC; Diag. = D; 
Da = 2(a — 6 cos 0), Dj, = 2(6 — a cos O), Do = 2 ah sin C. 

§ 160. Page 283 

1. — aj/(4y). 8. (y - x2)/(y2 — x). 7. Errors due to Aa, AB, 
A4: 19fe; .30 9^; .84 9b. 9. 3%. 11. 20.6, 19.3, 101.6 

§ 166. Page 295 

7. (x-3)/12=(2-2/)/16 = 3-2. 9. {B=y, 2 = 4. 
11. cos-i(2/\/39). 18. 3x + 42/ = 26; 2x + 4y+V62 = 26. 

16. (0, 0, 0). 26. u and tj are solutions of the '* normal equations " 
uZaxi + vSa6 = Sac ; uSa6 + rS66 = S6c ; where Soa = ai^ + au* + ^a*, 
Sa6 = ai&i + 0262 + os&a, etc. 81. a = 7/8, /3 = 11690/3. 

88. a = - 10.30, /3 = 6.48 

§ 169. Page 301 

I. 2x + 42/ + 2 = 18; (x - 4)/2 =(2/ - 2)/4 = 2 - 2. 

8. 3x-22/+2 = 18; (x- 6)/3 =(1 - 2/)/2 = 2 - 2. 

6. 3x + 42/-62 = 0; (x-3)/3=(y~ 4)/4 =(6 - 2)/6. 
.7. ex + cy4-22 = 4c; x/e =(2/ - 2)/c =(2 - c)/2. 

9. cos-i(±2/V6). _ 11. x+y-f-V2 2 = 2a, x = 2/ = 2/V2. 
\/3 X4-3 y+2 2=4 a, x/ \/3 = y/^ = 2/2. 18. xxo - y^o - 2(2 + 2©) = ; 
(0, 0, 0) ; no extreme. 16. x'^-\-i/^ = l -h z^\ -'X-\-Zy-\'Zz = l. 

17. 9jB2 + 4y2 + 362i = 36; 9x + 6y + 18>/22 = 36. 
19. 8x-3y-2 = l; 9x + 6y-2 = 20. 

§ 170. Page 304 

8. 2 a?(3 ir/4 - 2). 6. V2 a2 ; a = side of square. 

II. (2 ir/3)( Vm(2 fe + m)« - w?). 



16 ANSWERS 

§ 172. Page 306 



1. W. 8. coB-i (1/6). 7. (^1 - ^a) Vfl?TT2, 2 » Va^ + 6». 

§ 172. Page 306 (Second List) 

I. rsin.2^; f«co82d. 8. 2rc2«(co8d— sin^) ; 2fc««(cofltf + smtf). 
7. 2 cos e(r* — sin« d)/r ; 2 sin ^(r* + cos* e)/r. 

9. (^cos^— sinolog r)/r, (^ sin ^ + cos ^ log r)/r. 11. « = 286/116. 
18. 4 a«(3 IT - 4)/9. 17. (0,0). 88. The inscribed cube. 

25. iS' = -7.97 + .000107 P«. 87. (a) ff = 83.68 - 1.188 P. 

(6) ff = 31 .64 - 0.966 P - 0.0087 P«. (c) ff = 40.86 - 10.73 log P. 
88. sin-i (1/V3) and sin-i (1/3). 

86. -x/2=(y-2)/0 = (4 2-ir«)/(4ir); 

(x + 2)/0 = - y/2 = (2 - x2)/(2 r) ; 8 « - 4 jr2 + ir» = ; 
y — irz +ir» = 0. 

87. aVl + A;*(^— 0i). Value of y should be a cos sin 0. 

§ 175. Page 314 

17. aj2 - y* =- 3aj ; 6/4. 19. xdz + ydy = 0. 91. vy" + y'« = 0. 
28. x* - y« — xj/(y' ~ l/y') = a« - 62. 26. dy = xdx, 

*^- dt«~ ^' "Si"^' d^~ ^ *dt' dT* — dt 

§ 178. Page 318 

II. y = 1 4- ce^o". 18. y - 1 = c(x + 1). 16. 1 +y«= c(l + ai*). 

17. 2 y = cx« + c'. 88. |/« = cC. 96. y = 3(1 + x). 
97. Ti = 200 e»/» ; * = (2/ir) log 1.1 

99. (B - 5')/(^ - g) = e('-^)(«+«). 81. «« = c - 2 *«/<• 

§180. Page 323 

1. y = (c + x)e^/«. 8. y=2sinx-2 + ce"**"*. 5. xj/a(2 + ex) = 1. 
7. 2/r = 1 — ^ + cer^. 9. y = tan x — 1 + ce-**°». 11. 8 = c«-* — 1 + «. 

18. y = ce» — (sinx + cosx)/2. 15. y = kx-\- c Vl + x». 

§ 181. Page 324 

1. 3y5 = l— 3x + cc-8». 8. (x + y)/(x - y) = ce*i'. 

7. x» + 3 xV + y» = c. 9. xe*^* = c. 15. (a)x — y = c. 

17. y* = 4 c(x + c). 19. y^ = kx. 



ANSWERS 17 

§ 183. Page 329 

1. a = Ae^ + Be-*, 8. s = a sin (i + 6). 
5. y = A&* + Ber** oxy — a sin Qci + 6). 
7. S. H. M. with zero amplitude ; no motion. 

9. a = \/l04, 6 = tan-i6 ; a = 6, 6 = ir/2. 

§184. Page 332 

1 = cie* + C26*». 8. y = Cie» + Cje-*'». 6. y = {c\Z + C8)e». 

7. y = (ci sin ^2 « + C2 cos V2'x)e». 9. y = CiC** + Cje^.. 
11. y = cie*«/3 + C2e8»/2. . 18. y = cie^* + c^sr^, 15. y = ci + C2e-*». 
17. % = c-*</2[cicVii=iSt/2 + Cjte~>/»«=^/«], c < 6V4 ; 

X = e-w/«[ci sin V4 c — hHI'l + Cjcos V4c — 6««/2], c > ftV** 

19. X = e-'/2^5-±2^c^^/2 + ^"^e-v^/'l ; No ; 
L 10 10 J 

^ ^ ^„ ri+A/6 + 2ro^^,,^V6^1>2.o^^^,n 

L 2V6 2V6 J 

§ 186. Page 337 

5. 3 < = 2(V« - 2 c) V>/s + c + C. 7. y = e8»/4 + CiX + C2. 

9. y = 6cosa5 + 4a5sinaB — «*cosx4 ca5 + c'. 
11. yz=.^ —(1/16) C082 X + CiX* + C2X* + C3X + C4. 
15. y = fcB«(x« - 4 te 4- 6 12)/12. 

§189. Page 341 

9. y = 3x/4 + x«/4 + Cie* + CjC«* + Cs- 
11. y = cie» + cjc-* + csc-^ + (C4 + x/12)c2». 18. y = Cie» + Cje*/* + Cj. 
15. y = — Jxsinx + cicosx + C2sinx + C8. 17. y = Cie»+C2e"*+C8X4-C4. 

19. 2Vl + cc»4-log[(Vl + c€*- 1)/(V1 + ce* + 1)] + c'. 
21. y = (x — x2/2) log X + CiX* + CaX + C3. 25. y = CiX* — x logx + C2. 
27. y = (1 — 6)/62 - log (a + 6x)+ Ci(a + &x)«i + C2 (a + &x)"4, where 
mi and m^ are the roots of m* + (6 — l)m — 6* = 0. 



aiaaaii7Mak 





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