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ANNALS OF MATHEMATICS STUDIES
Number 29
AN NALS O F M A TH EM A T IC S S T U D IE S
Edited by Emil Artin and Marston Morse 1.
Algebraic Theory of Numbers, by H e r m a n n W e y l
3.
Consistency of the Continuum Hypothesis, by K u r t G o d e l
6.
The Calculi of Lam bda-Conversion, by A l o n z o C h u r c h
7.
Finite Dimensional V ector Spaces, by P a u l R. H a l m o s
10.
Topics in Topology, by S o l o m o n L e f s c h e t z
11.
Introduction to Nonlinear M echanics, by N. K r y l o f f and N. B o g o l i u b o f f
14.
L ectu res on Differential Equations, by S o l o m o n
15.
Topological Methods in the Theory of Functions of a Complex V ariable,
L e fs c h e tz
by M a r s t o n M o r s e
16. Transcendental Numbers, by C a r l
L u d w ig
S ie g e l
17.
Probleme General de la Stabilite du Mouvem ent, by M. A. L i a p o u n o f f
19.
Fourier Transform s, by S. B o c h n e r
20.
and K .
C h a n d ra se k h a ra n
Contributions to the Theory of Nonlinear Oscillations, Vol. I, edited by S. L
efsch etz
21.
Functional Operators, Vol. I, by J o h n v o n N e u m a n n
22.
Functional O perators, Vol. II, by J o h n v o n N e u m a n n
23.
Existence Theorem s in Partial Differential Equations, by D o r o t h y
L.
B e r n s t e in
24.
Contributions to the Theory of Games, Vol. I, edited by H. W . K u h n and A. W . T u c k e r
25.
Contributions to Fourier Analysis, by A. Z y g m u n d , W . T r a n s u e , M . M o r s e , A. P. C a l d e r o n , and S. B o c h n e r
26.
A Theory of Cross-Spaces, by R o b e r t S c h a t t e n
27.
Isoperim etric Inequalities in M athem atical Physics, by G. P o l y a
and
G . Szeg o
28.
Contributions to the Theory of Games, Vol. II, edited by H . K u h n and A. W . T u ck er
29.
Contributions to the Theory of Nonlinear Oscillations, Vol. II, edited by S. L
30.
efsc h etz
Contributions to the Theory of Riemann Surfaces, edited bii L . A h l f o r s et al.
CONTRIBUTIONS TO THE THEORY OF NONLINEAR OSCILLATIONS V O L U ME I I
M. L. C A R T W R IG H T
S. LEFSCHETZ
E. A. CODDINGTON
N. LEVINSON
h
. f . De BAGGIS
j
. M cC a r t h y
H. L. T U R R I T T I N
E D IT E D BY S. LE F SC H E T Z
PR IN CE TO N P R I N C E T O N U N IV E R S IT Y PRESS
1952
Copyright, 1952, by P r inceton U ni v e r s i t y Press London: Geoffrey Cumberlege Oxford Univ e r s i t y Press
The papers i n this volume by DeBaggis, Lefschetz, and Turrittin, were prepared under contract w i t h the Office of Naval Research, and equally sponsored by the Office of Ai r Research. The p aper by Codd i n g t o n and L e v i n s o n was prepared under contract w i t h the Office of Naval Research. Reproduction, translation, publication, use and disposal in whole or i n part by or for the United States Government w i l l be permitted
Printed i n the United States of A merica
iv
PREFACE
This monograph, a s e q u e l t o Annals o f Mathematics Study No. 20, o f f e r s another c o l l e c t i o n o f co n trib u tio n s to d i f f e r e n t i a l equ atio n s. l a s t d e a l more o r l e s s w it h o s c i l l a t o r y problem s.
A l l but the
I n Mary L. C a r t w r i g h t ’ s
paper t h e r e a re g i v e n new and more a c c u r a t e e s t i m a t e s o f th e p e r io d and a m p li tude o f th e o s c i l l a t i o n o f th e van d e r Pol e q u a t io n 2
(1)
x + p ( x - i ) x
+ x=
o
f o r fi l a r g e . E. A. Coddington and Norman L ev in s o n examine s u f f i c i e n t c o n d i t i o n s f o r th e e x i s t e n c e o f p e r i o d i c s o l u t i o n s o f (2)
x = Ax + p +
(x , t , ^ )
where x i s an n - v e c t o r , A a c o n s t a n t m a t r i x , ^ a s m a ll p aram eter and f p e r i o d i c in t . DeBaggis g i v e s n . a . s . c . f o r the s t r u c t u r a l s t a b i l i t y o f a system (5 )
x = f ( x , y ), y = g ( x , y ). The paper by L e f s c h e t z c o n s i s t s o f two p a r t s .
I n the f i r s t t h e r e i s
g i v e n a co mplete d e s c r i p t i o n o f the c r i t i c a l p o i n t s o f an a n a l y t i c a l system ( 3 )- In th e second the s o l u t i o n s o f the e q u a t io n o f van d e r Pol i n th e f u l l phase p lan e a re studied ' and d e s c r i b e d . The t i t l e o f the paper by John McCarthy t e l l s
i t s own s t o r y .
H. L. T u r r i t t i n d is p o s e s c o m p le t e ly o f th e fo rm a l problem o f the s o l u t i o n o f an e q u a t iio on (b )
. x = A( t , E )x
where £ i s a param e ter, x i s an n - v e c t o r and A an n m a tr ix whose terms a re power s e r i e s i n e . He a l s o shows t h a t th e fo rm a l s o l u t i o n s a r e , under c e r t a i n con d itio n s , a ctu al so lu tion s. S. L e f s c h e t z Princeton U n iv e rs ity January, 1952
v
CONTENTS Preface
v
B y So l o m o n Lefschetz I.
V a n d er P o l ’ s E q u a t i o n for Rela x a t i o n Oscillations
3
B y M a r y L. Cartwright II.
Perturbations of L i n e a r Systems w i t h Constant Coefficients Possessing Periodic Solutions
19
B y E. A. C o d d i n g t o n and N. L e v i n s o n III.
D y n a mical Systems w i t h Stable Structures
37
B y H. F. DeBaggis IV.
Notes o n D iffer e n t i a l Equations
61
B y So l o m o n Lefschetz V.
A Method for the C a l c u l a t i o n of Limit Cycles by Successive Approximation
75
By John McCarthy
VI.
Asymptotic Expansions of Solutions of Systems of Ordinary L i n e a r D i f f e rential Equations C o n taining a Parameter B y H. L. T u r r i t t i n
81
CONTRIBUTIONS TO T HE T H E O R Y OF NO N L I N E A R OSCILLATIONS VOL. II
I.
VAN DER P O L ’ S EQ U A T I O N F O R R E LAXATION OSCILLATIONS B y M. L. Cartwright §1 .
Introduction.
(1 )
The equat i o n
x - k ( l - x
with
k
2
) x + x =
'
0
large and positive has only one periodic solution, other t h a n
x =
0,
and this is of a type usually described as a r e l a x a t i o n osc i l l a t i o n (as
1
opposed to a sinusoidal oscillation). tained a graphical solution fcr
It was discussed by v a n der Pol w h o obp k = 10 and by le Corbeiller who, using
Lienard’ s method, showed that the period
2T = 2 k (3/2 - log 2) + 0 (k), and e * k -> «» . Other authors^ have also dis4 cussed the equation, in partic u l a r D o r o d n i t s i n has obtained a n asymptotic
the greatest height f ormula for
T
h = 2 + 0 (1)
as
w i t h smaller error terms but his analysis is difficult to
follow . This pap e r Is based o n the joint w o r k of Professor J. E. Littlewood and myself, largely on w o r k w h i c h was done before that contained in our other published papers o n n onlinear differential equations. k
We shall show that as
00
(2 )
T
1 0 ge 2
) +
+
h= 2 + ^ 5
(3) where
= k (5/ 2 -
&
and
p
0
( - ^ 3)
+ ° ( ^ 75) ’
are constants determined as follows:
The eq u a t i o n
> has one and only one solution
(1) (2 ) (3 )
(4 )
*( 5 )
such that
0
as £
B. v a n d er Pol, Phil, Mag. 2 (1926), 978-992. Ph. le Corbeiller, Journal Inst. Elec. Eng., 79 (1936), 361-378. D. A. Flanders and J. J. Stoker, "The Limit Case of R e l a xation O s c i l l a t i o n s ”, i n "Studies I n N o n l inear V i b r a t i o n Theory", e d . R. Courant (Inst, f or Maths, and Mech., New Y o r k University, 19^6, typescript), J. Haag, Ann. E c . Norm. Sup. 60 (19^3), 35-111, 61 (1944), 73-117, J. P. LaSalle, Quart. App. Maths., 7 ( 1 9 ^ 9 )* 1-20. A. A. Dorodnitsin, "Prik. Mat. i. Mech.", 11 ( 1 9 ^ 7 ).
3
M. L. CARTWRIGHT
b
y ^
1,
- log hi. 2
Let 0 at some point Z in HC, th e n since h < 0 and x is continuous there is a sub-arc X Z of HC such that x = 0 and y >
0
for
x > y ^ z.
6
M. L .
CARTWRIGHT
Hence k - iHpTiT + h W
Z ..
> 2 ■ x = J x y dt > 0 '
which gives a co n tra d ic tio n , and so x { 0 for a l l X in HC. Part
(ii)
follows at once from ( i )
and the o r ig in a l eq uatio n, and
also i f h > x > y > 1 .
xy which gives
*
=
h
- x-- > k
Ixl
)? ( x
- £ ) dx = kl
-
y2 ) - log x / y .
-’y
( i v ) and the p a r tic u la r result fo llo w s .
F in a l l y •• • 2 •• *2 x = - k (x -1 ) x - 2 kxx = k ( x 2 -i ) |x| i
- 2 k x i2 > k (x
which is
-x
- 2 kx x 2 + |x|
-1 )
2 k(x-i )
( 3 ). §V.
Lemma 2 consists of one-sided in e q u a lit ie s except i n ( i i ) ,
it is obvious that nothing b etter than the left-hand in e q u a lity i n ( i i )
and can
be obtained near H , but i n order to o b ta in a more accurate estim ate of t ^ c we need in e q u a lit ie s
of the opposite k in d .
For th is purpose we need to know that
h is not too near 1 and we div ide the arc HC by points Y , LEMMA 3 .
Suppose that h >
Z and E .
and that HY is a n arc
on which x -6
(1 )
k ( x 2 -i )
where 0 < kQ ( 4 ) .
Also y =
|x|
y
I H
( 1 ) is cer ta in ly negative fo r x
c e r ta in ly e x i s t s .' Since
= 1 and x < 0 in HC, y ^ 1 . ( x 2 -i ) - x < - cJ
x dt < - k ( 2 for k > k Q , and (ii)
L E MMA 5. Suppose that Y Z is the longest arc satisfying the hypo theses of Lemma b, and that E is a point i n ZC at w h i c h
e y_ 1 + A k
2^ ,
t h e n if X is
M. L. CARTWRIGHT any point in ZE M
Ix|
A . ze Ak ° At Z (i) holds in virtue of Lemma 2 (ii) and ( 4 ), and since x < t
(iii)
it w i l l continue to hold as long as x ) if x {
0
whi c h is the case at Z by ( 5 ).
0
But
0
M
k ( x 2 - 1 ) |x| £ 2kx x 2 - ix|
0 and x is increasing so that we can repeat the argument, and (i) holds throughout ZE. Part (ii) follows at once, and
t TO- f ze
•E
^
IxI
A
1
e2 )
6.
5
K -
+- f- f
log ^
+
I
If E satisfies the hypotheses of Lemma
+ Ak
A _ and k > k (S,A). O P — 1 /*^ The two largest error terms k(e - 1 ) and A k ' come f r o m the interval
EC whi c h
wil l need special consideration. §6. We now proceed to study the arc C A ’,f raming
our
lemmas so as
to cover all solutions starting d o w n fr o m C*. L E MMA 7. If a solution starts f r o m C, and if F is a point in CA' at w h i c h f max (A1/2 k"1/3 , |c| ) ,
and
(ii)
tcf < M A 1/2 k '1/5 .
B y the energy equa t i o n for CF w e have x 2 y_ c 2 + and so |f| > max (A 1 ^ 2 k ,
_
tcf
1
- x2
|c|) w h i c h gives (i).
n
Jp TxT
dx /
C
^ Jf
It also follows that
dx_______ «
1 !2
-p / m A
(1 . x 2 ji/2 - arc
003 f ^
LE M M A 8 . If a solution starts f r o m C and reaches F w here f = 1 - A k , A > 0, t h e n
(i)
tf a , < M/(A k1/3) ,
and (ii) Put x rj y k ^
for
=
0
1
2
y
1V1
Ak-
Part (ii) follows immediately fro m the integrated eq u a t i o n §2 (3) applied to CA' . §7.
W e now jump from A ’to the arc AB w h i c h is the refl e x i o n of
A ' B 1. Whereas at C the magnitude of c made little difference to the subsequent be h a viour of the solution, after A the behaviour depends very much o n the magni tude of a. If a is very small, the p o ssibility of the solution turning do w n be fore it reaches B, or taking a very long time to reach B, cannot be ruled out, but it is of some interest to see that e v e n if a - 0 (k 1 ) the subsequent b e
M. L. CARTWRIGHT
10
2
ha v i o u r may be similar to that of the periodic solution for w h i c h a ru -k 1 /2 except that h ~ 3 1 instead of 2 and that it takes a fairly long time to get away fro m A. LEMMA
9.
A solution starting f r o m A wit h a
3 /k
reaches B with (1)
|b - a - ffcl < t ab < M i provided that k > k .
^
If further a >
fcab < F T ¥ + "Tc- for k > Let G be the point x = ^ .
T h e n in A G
increases fro m A as long as x £ ^ ka.
Since x £
G is reached wi t h t&g < ^-/a ^ x ^
>
g- k.
3
On 1
AG 2
?■ + kx(l - - x ) ^
, £k,
where £>
0 ,t h e n
ko ‘ x
^ kx
- x,
and
^ in A G and ^ ka
so x ]> ^ ,
by the integrated equation ? | A
xdt
k + T ^ l o c - ^ kx = k + l k x '
Hence g ) ^ + ^ k , and t = tag
C — fdx_ ✓ 2 _____ dx_____ . M log k for k \ k J. I T ' I + 1 kx k 0 ‘ A -’ o k + 4
Next x > i- k near G; If eve r x =
1- k
on GB, let X be the first occasion.
The n
but also x > s - SG for k
x dt > k + - p - - 1 = - ^ r - - k > E k
> 2 w h ich gives a contradiction.
So x ) ^ k o n GB, B is reached wi t h
t b K.
and (1 ) follows from the integrated eq u a t i o n §2 (3) for AB. If a >£k, since x increases in A G w e have t M while the left hand side is positive.
Hence p < M and so t^
have |b + k ( p - p 5 /3 for k > k 0 (£).
2 / 3)1
< M/(£k). p j'
= tk +
U s i n g (2) again, we
P - e L
-
|
1
1.
in PQ, we have
x = - k x(x2 - 1 ) - x
- kx
,
and so divi d i n g by x and integrating fro m P to Q we obta i n l o g ( q / p ) £ - k tpq . Hence k tpq £
2
log(£k)
f r o m w h i c h the result for t
follows. The restrictions o n 1 . L E M M A 12.
If the hypotheses of Lemmas 10 and 11 are
satisfied, t h e n t ^
< M/(ek) and
|b + k (h ’ for £ < £q , x < - x
S k Q (e, 5 ) .
and as above
- Tk -
x < M.
Since h = 0
I * dt < - M S h
f r o m w h i c h the result for t ^ follows. B y the integrated e q u a t i o n for B H we have
M. L. CARTWRIGHT
12
H J - x dt { M tb h {
|b - k (h - j h 3 - |)I =
B for
«5 < < 50 , £ < §9 .
£0
and k > k Q (t, 5 ).
We have now covered the equivalent of a half wav e H C A ’ B’ H 1, and
w e m a y review the results as follows:
in Lemma 1 we showed that a solution
starting at a m a x i m u m H not too far above x = 1 arrives at C w i t h |c| bounded b y a constant d e pending on h. I n Lemma 2 we showed that a l t hough x { 0 in HC, x remains small until x approaches 1, and consequently the s o l ution takes a long time to reach C unless h is nea r 1. Lemmas and 5 show that the one-sided estimates for x and for the time in L emma 2 do in fact give a good approximation, provided that h > and x is not too near 1. Lemma 6 deals w i t h the arc just before C, and L emma 7 wit h that just after C a s suming that the solution starts from C, and together they show that the time t a k e n to cross the strip |x - 1 | £ A k
2/ 3
is at most M A 2 k
t i o n starting fro m C reaches A ’in time M A
L emma
1/ 2
8
shows that a s o l u
k ~ 1^ 3 w i t h ja'I > |k + |c| - M
L e m m a 9 shows that a solution starting fro m A w i t h a y 3 /k rises to B in time . p 0 (log k/k) w i t h b > - 0 (k) and gives a b e tter result if a is large. Lemmas
10,
11, and 12 deal w i t h a solution rising f r o m B w i t h b large.
show that tfeh =
(log k/k), and give a formula for h d e p e nding o n t>.
0
be observed that the tran s i t i o n interval
PQ
is comparable in some ways to the
tr a n s i t i o n interval Y Z in partic u l a r the time f or each is §1 0 .
They It may
0
(log k/k).
The periodic solution traces the reflec t i o n of the hal f wave
ABHCA' b e low x =
0,
and we shall now proceed to estimate T and h b y applying
the previous lemmas w i t h this in mind. THEOREM
1.
M \
M Ak
F o r the periodic solution ,
I / m A 1 /g k 1/ 5 ’
1/ 5
(ii)
la
- | k| ^k f or k > k Q , we
w h i c h with (ii) gives (iii).
L emma 12, w e have |h - l - h 3 + || ( M i 1 / 2
,
and so if we write h = 2 + £ we have it, (3 + 2 s + j i ; 2 )i { m a
which gives (iv) provided that A
y
A 0 and k
,/2
y
k ' 1*/5 ,
kQ (A).
U s i n g this in
V AN DER P O L ’ S EQUATION
13
Finally T = tah + thc + t o a l B y Lemmas 9 ,
1 0 , 11
and
12
t -i = t ah ag / M ^ k
M £k
+
4*
t -i ~f~ "t-t + "t + t -i gb bp pq qh
M log; k k
M / M log; k £k ^ k
f o r every £ > 0 , provided that k > kQ (e). and using (iv) in Lemma 2 we have
B y Lemmas
7
and
putting e =
1
+ Ak
8
t
, (M A
1/ 2
k
tvhe
and similarly from Lemmas
3 * b,
5 and
6,
_o /*
1 D we have, as
in §5,
thc = V s M
+ tyz + tze +
M log k
^ T k
+ —
k
+ ki
.
t ec
. M A
&
3 2
21
log
■ ^173
+ “ ^T 7 3
A Q , k > k Q (A, S) = k Q (A). §11.
It remains to remove the large constant A and replace it by
constants w h i c h can be determined more precisely.
It is obvious that the
errors depending o n A originate in the arc EF, i.e. i n the strip |x - 1 | ^ A k
with x
1 as
h y p erbola
2
^ rj Q + 1 =
0,
£ ->
w e see that
+ 00
d rjQ /d^ > 0
below and to the right of the upper b r anch and d t ] Q /d£
±00 unless 2 £ »7 0 +
1
-»
.
0
.
0
above
Hence one
set of solutions descends fro m + o© as £ increases fr o m until it crosses the upper branch of the h yperbola and t h e n ascends a g a i n to + , a nother set
The curves *)0 (4 ) are shown In black w i t h the separating curve rj* o n w h i c h i]0 (£ ) — 1►
0
as
I — ►-»
thicker t h a n the o t h e r s . crosses rjo = + oo .if |
0 at
§= %Q , say, wit h d r i o /d§ = 0 0 at % + 00 i n such a w a y that lim rjQ > 0 , the n
and ascends to
and so *|0 (|) ^ 2 as 5 ± 93 • B o t h sets vary continuously wit h value of and fo r m ope n sets. There is therefore a solution, or closed set of solutions, separating the two sets, and it must lie b e t w e e n the hy p e r b o l a and r[o = 0 for negative § . It follows that o n such a s o l u t i o n ^ * d r | * / d £ > 0 , and since for fixed ^ d r ^ / d ^ increases as rf decreases, the lower solutions increase more rapidly t h a n the upper w h i c h is impossible if there is more tha n Y|Q ( 0 )
V A N DER POL'S EQUATION
15
one solution o n wh i c h % —> - ^ b e t w e e n the h y p e r b o l a and rj = 0. Hence there is a unique solution separating the classes. LE M M A 1 4 . Suppose that T) (£) satisfies (2) and that a is defined
as in Lemma 13(or
w he r e if r|(0)
> o, we have y) 1 for some £, such that - A £ % 0 for all I and 90 (i) 00 as £ for ^- A , provided that A > A q (1 d l ~
2
+
cl
S
and let
= ol + t,
.
T h e n by
~ 00 and so *)0 (£) 2 ^ £( 0. Substituting
■2 ^ 1 + ^273 ^ 2(,7o + 7i } + 5I = 0 »
w h ere ^ ( 0 ) = 0 , and since *)0 (£) 2. £ > 0 , we have
dth
. xtA)!^! + _ j _ ( ^
E-h, I
2
k 2/5 p
m +
£-
In,
where "X (A) denotes a number d epending o n A but not o n k or % . Since rj ^ (0 ) = 0 by a w e l l k n o w n me t h o d ^ it follows that for every A > 0 (6 )
h , I £ -X(A) k " 2 /J
0 and every A > 0 , provided that - A { ^ i A and k > k ( A > A 0 and k > k Q ( S , A ) . If Y)o ( 0 ) = o l - 8/2 5
=
§0
>
where
0
A b (6 ).
we also have
+
1)
S ^ *)
+ 1.
This means that the solution of (2 ) increases more rapidly t h a n the solution of (3) through the same point 2 %
+
1
low the creases.
>
0-
in the region defined by £
0,
certainly lies b e
just defined ne a r €> = 0 , and continues to lie be l o w it as £ d e It therefore reaches y = 0 for | w h i c h gives the second part. LEM M A
15*
Suppose that at and p are defined by §1 ( 5 )
and t is any positive number. T h e n if 9 ( £ ) solution of (2) for w hich |y(0) - 0 and every A > o we have I ^ | < £' for -A {
5
{ A provided that h
0, provided that A > A 0 (£), £' < £q(£,A), k > k0 ( £ , £ ' A j ) . As ^ -» - 00 , >7
k ( k Q (£,A).
T h e n (iii) follows f r o m Lemma 9.
/ 2- £^
X
R e flecting in x = 0
Putting (iii) in Lem m a
12
we
have
h - j h 5 + |+ and
pu t t i n g h As
( « + (3) k -4/ 5 = 0(k~4/ 5 ) ,
= 2 + every
£
k (| - log
2
)
) 0,A ) 0 and
(3 )
+
( oc+ (3 ) k "
k>
k
t, he = t, h y i
every £
+ tyz
s)
)2
3>
5
t l U LtfJ.
>2
> 0 ,provided that k > k Q (e). dx
?
ec
1
+ tze
, S U J S J . , k( l _ ^
f
- k(e -
(£ , A ) . B y Lemmas
*
for
1/ 5
•''c
But _1
IxI
r o d 4.
k 1/ 5 •'-A P
and so b y L emma 15 and (i ) above we have
|tec - k(e - 1
( 0 , provided that A > A 0 (£) and k > k Q (£,$,A). Putting (2) and (3) t o g ether w i t h ( 4 ), we have ’ t^c
as k
f
00
.
= k(
I
-
log
2 ) +
\
( CX. +
p
) k ' 1/ 3
+
rj ) ~ p ( 0 ) - t) = 0 .
(0 . 3 ) For
p- =
0,
the system (0 .3 ) has
rj -
0
as a s o l u t i o n . . If the J a cobian
J = det (x*j (T,fj.,rj) - E) does not v a nish at continuous solution Here det
= determinant, and E I n case
form
I] = *](p)
f(x,
for
p. =
0,
t h e n ( 0 .3 ) has a unique
| p. | sufficiently small w i t h
r^(o) =
represents the n-dimensional unit
t, (jl )does not contain t
explicitly, but
f ( x , p ) , the system ( 0 .2 ) has £ = p' as a s o l ution of period
the above hypothesis is n ever fulfilled.
0.
matrix. is of the T
so that
I n this case the t h e orem is modified,
and if (0 . 4 ) *
x' = f(x, p.)
This pa p e r was w r i t t e n in the course of w o r k sponsored by the Office of Naval Research.
19
20
C0DDINGT0N AND LEVINSON
has a periodic solution
x = p(t)
of period
T Q f or p-=
0,
and if the first
v a r i a t i o n (0 .2 ) has no more t h a n one independent solution of period T Q , ( 0 .4 ) has a periodic solution x = q(t,p.) for small 1^-1 , continuous in (t, p O . q(t,
0
The period,
T(^),
) = p(t), and
of
q(t,p)
T( 0 ) = T Q .
is continuous in ^ .
The fact that ( 0 .4 ) at p - =
only linearly independent solution of period v a n ishing of a c e r tain
TQ
the n
Moreover
0
has p ’as its
is equivalent to the n o n
(n - l )-dimensional Ja c o b i a n
J1.
In ma n y important cases the hypothesis o n the equations of the first variation, or, what is the same, the non - v a n i s h i n g requirement o n the Jacobians J and
J^,
Is not met. F o r example in case
(0.5)
w
Is a
scalar the eq u a t i o n
w" + w = p-g(w, w ’, t, ^ )
where
g
is periodic of period
2 rrin
t,
,
if it contains
t,
has f o r its
first v a r i a t i o n w" + w =
0 }
w h i c h has sin t and cos t as independent solutions the hypothesis for neither result stated above c an
of period 2 rr. Thus be met for (0.5). The cases
of equa t i o n (0.5) relevant here have b e e n treated in detail by F r i edrichs and Stoker [2]. f(x,
0
It is our purpose to consider the case whe r e f(x, t, 0 ) of (0.1 ), or ) of (0 .4 ), are of the form' Ax, wh e r e A is a constant matrix. We
show that it is possible to give sufficient conditions for the existence of p eriodic solutions of small
x
1
= A x + p-f(x, t,p.) (and
Ip-! e v e n w h e n the Jacobians
J and
J1
x* = A x + p.f(x, p.)) for
vanish.
These conditions only
involve knowledge of the solutions of the degenerate linear system As is to be expected, if case
f = f(x, p.))
for which
J
(or
f
can be solved fo r recursively. J1 )
x* = A x .
is analytic, t h e n the solutions (and period in I n the following, systems
vanish w i l l be referred to simply as systems w i t h a
vani s h i n g Jacobian. 1.
PERTURBATION OF A SYSTEM W I T H A V A N I S H I N G JACOBIAN
F o r the linear system ( 1 .1 ) where
x A
s o lution
1
= Ax,
is a constant real matrix, assume that there exists a real periodic p = p(t)
w i t h period
2 tt.
This is equivalent to the fact that
there exists at least one characteristic root wh e r e
N
is a n integer (which m a y be zero).
X
of
A
of the f o r m
N = IN
W e shall be interested in the
perturbed system (1.2)
x'=Ax+yu.f(x,
t,ju),
wh e r e it is assumed that A is the constant matr i x g i v e n in (1 .1 ), fjL is a real parameter, and f is real, periodic of period 2 TT in t. (Since 2 tt need not be the least period of e x c l u d e d ).
f
in
t
the case of subharmonic oscillations is not
PERTURBATIONS OP LINEAR SYSTEMS It is clear that if
c and
d
21
are any real constants, t h e n
is also a real periodic solution of ( 1 .1 ) w i t h period f or what values of
c
and
d,
periodic s o lution t e n ding to
,
2 tt
c p(t + d)
It is not obvious
if any, the perturbed system ( 1 .2 ) m a y have a c p(t + d)
as p--»0 .
W e can not a pply the p r o
cedure m entioned in the Introd u c t i o n f or in the case ( 1 .2 ) the relevant Ja c o b i a n
J
vanishes.
However, it is possible to give sufficient conditions
fo r the existence of periodic solutions of ( 1 .2 ) fo r
y- ^ 0
provided
A
is
i n canonical form, and it is always possible to arrange this. Setting
x = Py
wh e r e
P
is a real n o n - s ingular constant matrix,
the system ( 1 .2 ) c a n be replaced by a system for matrix B = P 1A P,
when
p- =
0,
y
w here the coefficient
is i n real canonical form.
n e w system satisfies the same assumptions as ( 1 .2 ). assumed that
(1
.3 )
A
al r e a d y has the fo l l o w i n g real canonical f o r m
A =
w h e r e the elements not s h own are zeros. ma t r i x of
Moreover, this
It w i l l therefore be
a . (
a . even)
Eac h
Ay
j =
1,
..., k,
Is a
rows and columns of the f o r m sj Sj
E2 (1 . * 0
2
w h e r e all elements are zero except
sj = n j
Nj be i n g a positive integer, (In k - d i m e nsional unit matrix 0 < k < only two rows and columns in w h i c h rows and columns, 1,
sj
and
and
0
1
the foll o w i n g E^. w ill always denote the n, and E = E n ). A m a trix Aj m a y have case it is Each ma t r i x Bj has p S3 and Is of the for m
CODDINGTON AND LEVINSON w here
B. m a y have only one row and column, in w h i c h case B. J k J m the single element 0 . The matrix C has Y = n X
(O)
0
)
■ f ( P ( 0 ) . ») n v i=1
A p( J*-1 ) + b j A p ( o )
af
(P
dx.
(o)
0) Pi
(j-i)
+ P ( j) (1 ) P(J) depends o n p ( 0 ), where That the system (2.12) has a solution f o r p (i)
d (J’ 2),
and
and
b.
v
b2,
bM
is clear.
T H E O R E M 6. U n d e r the assumptions of T h e o r e m 5 the analytic solution q of (2.1 ) c an be obtained b y solving equations (2.12) i n s u c cession for the periodic coefficients p ^ ,
of period
2ir,
of the power series (2.9) for
p(s, jjl ) = q (s (1 + T / 2 TT),p.), e x p a n s i o n (2.10) f or
T / 2 tt.
and the constants The p.(i) vx; and b^
determined in (2.12) by the requirements that p ^ ( s
+ 2 tt) = p ^ ( s ) ,
PROOF.
in the are uniquely p ( o ) (s) = e sAa,
2 TTb,
Suppose there are two functions
fying the second e q u a t i o n i n (2.12), and two constants
( 1 ), b2,
-(1 ) ~2 ,
satis-
such that
(2 ) £(2) b 2 ) there correspond to the pairs (p (1 ) respectively satisfying the third e q u a t i o n of (2.12). S ubtracting the third e q u a t i o n for one case f r o m that fo r the other case, and d e noting p (1)
b 2 = t>2 - b g ,
we have
g f 2) = A p < 2 > + b, A p l,) + b £ A p < °>
n v i=l
af dx.
(P
;o)
0) p. (1)
F r o m the second e q u a t i o n for each case follows ds Let p (1 >(o) = a (1 > each is zero. Since
=
(0) == 0.
and
A p* v0 )
and p ^2 ^( 0 ) = * ( 2 ) The second (ot1 ) p ^ 1 ^ is periodic it follows that p (1 }(s) = e aAa < ' K
component of
-
CODDINGTON AND LEVINSON
3k
w h e r e only the exceptional components of
a/
1^
c an be different f r o m zero.
Thus a ^1 ^ has at most 2k + m - 1 components that are not k n o w n to be zero. P r o m the differential equa t i o n for p ^ 2 ^, and the fact that p ^ ( o ) = p ^ 2 ^(2 tt), it follows that (E - e 2™ )
-(2) = b
2tr (* e ( 2Tr^ ) A p ( 1 ) (cr)d **r\ fo
a
'
+ b2 A J - V ^ V ^ ^ d c r +
£
•’o
- |£ _
1=1
( p ( o ) ( 0,
b p,
cr (x 1 , x 2 ) -
ap0 + " a ^ ) + °*
I n the proof of the theo r e m w e shall assume that a) and b) are not satisfied and derive a contradiction. w e m a y assume
(x°, x°)
Without loss of generality, in the proof
at the origin.
Moreover, since, by L emma 3, each crit
ical point of (A) is a n isolated point we m ay encircle the o r i g i n b y a circle of radius
r > £,
and choose
6(e)
so small that there is exactly one c r i t i
cal point of the perturbed system w i t h i n this neighborhood. Suppose first that e qua t i o n
\
2
+ ° < a 0,
A.(o, 0) > 0,
0 ],
When
no definite statement ca n be made as to the stability or unstability We shall show that if (A) is structurally stable, it cannot possess, a limit-cycle y such that h(y) = 0 . But first we shall prove the
0
following lemma w h i c h is a slight ex t e n s i o n of the continuity theo r e m wit h respect to the initial conditions. Let us wri t e the system (A) in the v e c t o r f o r m
D Y N A M I C A L SYSTEMS W I T H STABLE STRUCT U R E S (A)
^5
x = P(x)
where
x, P. denote the co l u m n vectors
> (p^-) 9 resPe c '*:^v e ^ y •
this
n o t a t i o n the perturbed system (B) becomes (B)
y = P ( y ) + p(y).
The solutions of (A), (B) are giv e n b y the equations x =