M.A., F.R.S., PROFESSOR OK MATHEMATICS IN" THE ARTILLERY COLLEGE, WOOLWICH ... seventy years old, has scarcely yet made its way into the ...
Edward Bright
Mathematics Dept
THE APPLICATIONS OF ELLIPTIC FUNCTIONS.
THE APPLICATIONS OF
ELLIPTIC FUNCTIONS
BY
ALFRED GEORGE GREENHILL M.A., F.R.S.,
PROFESSOR OK MATHEMATICS
IN"
THE ARTILLERY COLLEGE, WOOLWICH
MACMILLAN AND AND XETT YORK 1892 [All riyhlft reserved]
CO.
AY*
CONTENTS. PAGE
INTRODUCTION,
vii
CHAPTER THE ELLIPTIC FUNCTIONS,
-
-
I.
-
CHAPTER
1
II.
THE ELLIPTIC INTEGRALS,
-
CHAPTER GEOMETRICAL AND MECHANICAL FUNCTIONS,
-
III.
ILLUSTRATIONS
THE
OF
ELLIPTIC
-
66
CHAPTER THE ADDITION THEOREM FOR
IV.
ELLIPTIC FUNCTIONS,
CHAPTER THE ALGEBRAICAL FORM
IN
-
-
112
V. 142
VI. -
-
175
-
200
-
254
VII.
GENERAL AND THEIR APPLICATIONS,
CHAPTER THE DOUBLE PERIODICITY
-
OF THE SECOND AND THIRD KIND,
CHAPTER THE ELLIPTIC INTEGRALS
-
OF THE ADDITION THEOREM,
CHAPTER THE ELLIPTIC INTEGRALS
30
VIII.
OF THE ELLIPTIC FUNCTIONS,
781468
-
-
CONTENTS.
vi
CHAPTER
IX. PAGE
THE RESOLUTION
OF THE
INTO FACTORS AND
ELLIPTIC FUNCTIONS
...
SERIES,
CHAPTER
X.
THE TRANSFORMATION OF ELLIPTIC FUNCTIONS,
APPENDIX, INDEX,
277
-
-
-
305
-
-
340
353
INTRODUCTION.
"L
ETUDE approfondie de
la
nature est
la
source
la plus
feconde des decouvertes mathematiques.
Non
seulement cette etude, en offrant aux recherches un but
determine a Favantage d exclure ,
calculs sans issue 1
;
elle est
Analyse elle-meme,
importe
le
et
questions vagues et les
les
encore un
moyen
d en decouvrir
les
assure de former
elements qu
il
nous
plus de connaitre et que cette science doit toujours
conserves
Ces ele ments fondamentaux sont ceux qui se reproduisent dans tous les effets naturels." (Fourier.)
These words of Fourier are taken as the text of the present treatise, which is addressed principally to the student of ApjDlied Mathematics,
who
will in general acquire his
matical equipment as he wants definite actual
problem
;
and
it
it is
mathe
for the solution of
some
in the interest of such
students that the following Applications of Elliptic Functions
have been brought together, to enable them to see how the purely analytical formulas may be considered to arise in the discussion of definite physical questions.
The Theory of Elliptic Functions, as developed by Abel and Jacobi, beginning about 1826, although now nearly *-~~^^*~ seventy years old, has scarcely yet made its way into the "
THE APPLICATIONS OF ELLIPTIC FUNCTIONS.
viii
ordinary curriculum of mathematical study in this country
and
is still
;
considered too advanced to be introduced to the
student in elementary text-books. In consequence of this omission,
many
of the
most interest
ing problems in Dynamics are left unfinished, because the
complete solution requires the use of the Elliptic Functions these could not be introduced without a long digression, unless a considerable knowledge is presupposed of a course
;
of Pure Mathematics in this subject.
But by developing the Analysis
as
it is
required for some
particular problem in hand, the student of Applied
Mathe
matics will obtain a working knowledge of the subject of Elliptic Functions, such as
he would probably never acquire
from a study of a treatise like Jacobi s Fundamenta Nova, where the formulas are established and the subject is in
developed
Mathematical application
they
of
originate
strictly
order
logical
without
Analysis,
the formulas,
any
Pure
of
on
digression
the
on the manner in which
or
independently,
branch
a
as
the
as
some
of
expression
physical law.
we
In introducing these applications
are following, to
some
extent, the
plan of Durege s excellent treatise on Elliptic Functions (Leipsic, Teubner); and also of Halphen s Traite
des fonctions
elliptiqucs
et
de
leurs
applications
(Paris,
1886-1891).
But while volume
I.
of
Halphen s
treatise
to the establishment of the formulas
of the functions,
volume
II.
;
is
devoted entirely
and analytical properties
and the applications are not discussed
in the following pages
it
is
till
proposed to develop
immediately from some definite physical or and the reader who wishes to follow geometrical problem the formulas
;
up the purely analytical development of the subject to such treatises as
Abel
s
(Euvres, Jacobi s
is
referred
Fundamenta Nova,
INTRODUCTION.
i
x
already mentioned, or the Treatises on Elliptic Functions of Cayley, Enneper,
Kb nigsberger,
The following works
also
H. Weber,
etc.
be mentioned as having been
may
consulted in the preparation of this
work
:
Legendre: Theorie des fauctions elliptiques ; 1825. Thomas Abriss einer Theorie der complexen Functionen :
und der Tketafunctionen einer Verdnderlichen 1873. Schwarz: Formeln und Lehrsdtze zum Gebrauche der ;
elliptischen Functionen.
Klein (Morrice)
:
Lectures on the Icosahedron
;
1888.
Klein und Fricke; Vorlesungen uber die Theorie der ellip
Modalfunctionen ; 1890. Darboux: Cours de niecanique ; 1886. Despeyrous tischen
et
R A. Roberts
:
Integral Calculus
1887.
;
Bjerknes: Niels Hendrik Abel; tableau de sa vie action scientifique
We
shall begin
;
by the discussion ,
of the
and
an idea
and importance.
Pendulum could only be
circular functions, small,
Problem of the
to give the student
Previously to the introduction of the the Circular
de son
as the problem best calculated to
define the Elliptic Functions, of their nature
et
1885.
by considering the
and by assimilating
its
Elliptic
treated
Functions,
by means
of the
oscillations as indefinitely
motion to that of Huygens
Cycloidal Pendulum, of 1673.
But now the employment
of the Elliptic Functions renders
the ordinary discussion of the Cycloidal
and of mere
historical interest,
such expressions as "reducible
"
Pendulum antiquated
and banishes from our
an integral which cannot be
to a matter of quadrature" in describing
integral, expressions
found,"
an
which aroused the indignation of
Mathematical Papers,
p. 562).
treatises
or
elliptic
Clifford
THE APPLICATIONS OF ELLIPTIC FUNCTIONS.
x
According to the
new
in
May
regulations for the
come
Tripos at Cambridge, to
1893, the schedule
II.
of Part
I.
includes
"
Elementary
excluding the Theta Functions and the
Elliptic Functions,
"
theory of Transformation
to be
hoped that this Functions into the ordinary mathe
reintroduction of Elliptic
;
so it
is
receive
more
Applications
have
matical curriculum will cause the subject
general
Mathematical
into force in the examination
and
attention
These
study.
to
been put together with the idea of covering this ground by exhibiting their practical importance in Applied Mathematics,
and of securing the
interest of the student, so that he
may
if
he wishes follow with interest the analytical treatises already mentioned.
We
begin with Abel
elliptic integral of
the
idea of the inversion of Legendre s
s
first
kind, and employ Jacobi
s
notation,
with Gudermann s abbreviation, for a considerable extent at the outset.
The more modern notation
of Weierstrass
is
introduced
subsequently, and used in conjunction with the preceding notation,
and not
to its exclusion
;
as
it
will be
sometimes one notation and sometimes the other
found that is
the more
suitable for the problem in hand.
At the same time explanation
is
given of the methods by
which a change from the one to the other notation can be speedily carried out. It has
been considered
sufficient in
many places,
in the reduction of the Integrals in Chapter
for instance
II.,
down the results without introducing the intermediate as the trained mathematical student to
whom
this
to write
analysis
book
;
is
addressed will have no difficulty in supplying the connecting steps,
and
this
work
will at the
exercises in the subject
students,
many
;
and
same time provide instructive
further, in the interest of such
important problems have been introduced in
INTRODUCTION.
XI
the text, forming immediate applications of theorems already
developed previously. I have to thank Mr. A. G. Hadcock for his assistance in preparing the diagrams, and in drawing them carefully to scale.
ERRATA. Page
6.
Line 9 from bottom, read Huygeiis. 1
*/ -. V x-y
42.
Line
48.
Line 5 from bottom, read -
64.
Line
99.
The diagram must be replaced by the one given below. The Xodoid in fig. 12, p. 99, was described by a point which was not a focus of the rolling hyperbola.
107.
138. 158.
205.
213.
227. 282.
328.
6,
read
19,
sin"
read Fonctions
4tt-(9e-
-r
4/r)
J .
elliptiques.
Line 2 from bottom, delete minus sign before radical. 2 ctf/D. Equation (7), read (r., Line 12, read 3QX(x, y). + v). Line 6 from bottom, read $(u - v) Line 7 from bottom, read G + Lx - X(yz - y ~] with the corresponding subsequent corrections. Line 7, read P s/-Y i + Q\ -Y 2 = $>(u
;
-
Line 5 from top, for rectangle read ribbon. Line 12 from bottom, read Pw. L. M. .?., IX.
ABBREVIATIONS. Quarterly Journal of Mathematics. S., Proceedings of the London Mathematical Society. Proc. G. P. $., Proceedings of the Cambridge Philosophical Society. Q. J. M.,
Proc. L.
Am.
J.
M.
M.,
F. E.,
Math. Ann., Phil.
Mag.,
American Journal
of
Mathematics.
Fonctions elliptiques (Legendre and Halphen). Mathematische Annalen.
Phil. Trail*.
Philosophical Magazine. Philosophical Transactions of the Royal Society of London.
Berlin Sitz.,
Sitzungsberichte der Berliner Akademie.
CHAPTEK
I.
THE ELLIPTIC FUNCTIONS. 1.
The Pendulum;
introducing Elliptic Functions into
Dynamics.
When a pendulum OP swings through a finite angle about a horizontal axis 0, the determination of the motion introduces the Elliptic Functions in such an elementary and straight forward manner, that
we may
take the
elliptic functions as
by pendulum motion, and begin the investigation of their use and theory by their application to this problem. Denote by the weight in Ib. of the pendulum, and let = OG h (feet), where G is the centre of gravity let Wk 2 denote defined
W
;
the
moment
of inertia of the
pendulum about the horizontal
+k )
axis through G, so that W(h* about the parallel axis through
2
is
the
moment
of inertia
(fig. 1).
OG makes
with the vertical OA an angle 6 radians at the time t seconds, reckoned from an instant at which the pendulum was vertical and if we employ the absolute unit
Then
if
;
of force, the
poundal, and denote by g (32
celoes,
roughly)
the acceleration of gravity, the equation of motion obtained
by taking moments about
is
since the impressed force of gravity is G so that ; vertically through
or,
on putting
G.E.F.
h + k*/h = I,
Wg
poundals, acting
THE ELLIPTIC FUNCTIONS.
to
THE ELLIPTIC FUNCTIONS.
3
If the gravitation unit of force, the force of
employed, then the equation of motion
w fr/TO 2
(A.
J lft
+&2 )-p = 7
.
is
a pound,
is
written
TTTf sm 0, Wh
O\*-^ v/
/\
"
reducing to (1) as before. 2.
Producing
OG
OP =
to P, so that
GP = k /h, 2
l,
P is
the point
called the centre of oscillation (or of percussion) and is called the length of the simple equivalent pendulum, because ;
AP
P
oscillates on the circle the point manner as a small plummet suspended
2); as along the arc
is
(fig.
the
same
by a fine thread from
seen immediately by resolving tangentially = s = l9 when the equation of motion of
AP
)
=
is
plummet
in exactly the
2
or
2
I(d 0/dt
-g sin#; ........................ (1) = C-gversO ......................... (2)
)= 2
and
g sin#=
integrating, U(dO/dt) These theorems are explained in treatises on Analytical Mechanics, such as Kouth s Rigid Dynamics, or Bartholomew Price s Infinitesimal Calculus, vol. IV., and might have been assumed here but now we proceed further, to the complete ;
integration of equation 3.
First suppose the
oscillation
BO A +AOB
of oscillation
is
Navez
Ballistic
church
bell,
oscillations,
books
;
in
(2).
pendulum
to oscillate, the angle of
being denoted by 2a
purposely
made
(fig. 2);
the angle
large, as in early clocks, in the
Pendulum, in a swing, or as in ringing a
so as to emphasize the difference from small the only case usually considered in the text
fig.
2 the angle of oscillation is made 300. when 6 = a, so that in equation (2)
Then dO/dt =
(7=# versa
and now denoting
g/l
2 by n
,
so that
;
n
is
what
Sir
W. Thomson
calls the
speed (angular) of the pendulum, 2 = n 2 ( vers a vers 0) ^(dO/dt)
= 2?i2 (sin2 Ja-sin ^), .............................. (3) vers = 2 sin 2 J0 2 dO/dt = 27i x/(sin ia -sin i0), 2
since
;
_ 2
and
nt-f
^
-..
.
..(4)
THE ELLIPTIC FUNCTIONS.
4,
and (4) is called by Legendre an elliptic integral of kind ; it is not expressible by any of the algebraical,
the first
circular,
or hyperbolic functions of elementary mathematics. 4.
To reduce
this elliptic integral to the
standard form con
by Legendre, we put
sidered
sinA0 = sinJa sin 0, by equivalent geometrically to denoting the angle as diameter, touching is the circle on (fig. 2), where in Q. BBf in D, and cutting the horizontal line
ADQ
AD
AQD
For, in the circle and, in the circle
PN
AP,
AQ,
AN= \AD vers 2$ = AD sin =I
Now
sin2 \ a
vers a sin
2
2
= 21 sin2 |a sin2 0.
= sin2 |a cos 0, ~ J$ = sin (sin Ja sin 0), 2
sin 2 J$
1
and
dle=
so that
*ft,2 v .^i*.* snrja sm 0)
^/(l
nt =
-
r~r ^r-, Jfr^/(1-siu iasm
and therefore
>
2
2
^,)
which is now an elliptic integral of the standard form employed by Legendre.
(Fonctions Elliptiques, 5.
In Legendre 2
ic sin
t. I.,
chap VI.)
replaced by ic; the quantity or A(0, K) and the integral
s notation, sin-Jet is
is. ,
K) for
Table IX.)
Legendre spent a long
life in investigating the properties of the elliptic integral of the first kind but the subject was revolutionised by the single remark of Abel (in
the function
Fc/>,
;
THE ELLIPTIC FUNCTIONS. 1823), that
is
of the nature of
.5
an inverse function
F(j>
we put u
then
;
and that
we should study
the properties of 0, the amplitude, as a function of u, and not of u as a function of as carried out by Legendre in his Fonctions Elliptiques. if
F(f>,
,
= am u, or am(it, /c) when Jacobi proposed the notation to be the modulus K is required put in evidence and now, 6.
;
we have
considered as functions of u, cos
Jacobi
= cos am u, sin = sin am u,
s
= A am u,
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p
p
THE ELLIPTIC FUNCTIONS.
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p
p O p Lt O
ut
p
ip
p
p
11
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