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R ENDICONTI

del

S EMINARIO M ATEMATICO

della

U NIVERSITÀ DI P ADOVA

C ARLO G RECO

Infinitely many spacelike periodic trajectories on a class of Lorentz manifolds

Rendiconti del Seminario Matematico della Università di Padova, tome 91 (1994), p. 251-263

<http://www.numdam.org/item?id=RSMUP_1994__91__251_0>

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on a

Class of Lorentz Manifolds.

CARLO

GRECO (*)

ABSTRACT - Let us consider R4

equipped

with a Lorentzian tensor g with

signa-

ture ( + , + , + , - ). In this paper we prove, under suitable

assumptions

on g, the existence of

infinitely

many

spacelike geodesics

z(s) _

(x(s), t(s))

with

the

periodicity

conditions x( s + 1) = x( s ), t( s + 1) = t( s ) + T ( T &#x3E; 0) on the Lorentz manifold

(R4 , g).

1. Introduction.

Let us consider the manifold

(R4 , g),

where

g(z)

=

g(x, t)

is a Lorentz tensor on

R4 ,

with

signature (+, +, +, -).

Let

z(s) =

=

(x(s), t(s))

be a

geodesic

on

(R4 , g),

and suppose that

t(0)

=

0,

and there exist a, T &#x3E; 0 such that

x(s

+

a)

=

x(s), t(s

+

a)

=

t(s)

+ T for every s E R. Then we shall say that z is a

o-periodic T-trajectory

on

(R4 , g ). Moreover,

if z is a

geodesic,

there exists

Ez

E R such that

I(s)] = Ez ,

and z called

spacelike,

null or timelike if

Ez

&#x3E; 0 or,

respectively, Ez

=

0, Ez

0

(see [14],

p.

69).

Suitable Lorentz manifolds are used in

Relativity theory

in order to

describe the

physical space-time. Then,

timelike

(or, respectively, null) periodic trajectories corresponds

to

periodics

orbits of a

particle

of po- sitive mass

(or, respectively,

of a

light ray). Spacelike geodesics

are not

trajectories

of

particles,

but

they

are

important

in order to

study

geo- metrical

properties

of a semiriemannian manifold.

Some

multiplicity

results for timelike

periodic trajectories

on

(R4 , g)

are

given,

for

instance,

in

[5]

and

[9]

under the

assumption

that

(*) Indirizzo dell’A.: Universita

degli

Studi di Bari,

Dipartimento

di Mate- matica,

Campus

Universitario, Via G. Fortunato, 70125 Bari,

Italy.

Work

supported by

MURST and

by

GNAFA of CNR.

(3)

the

gravitational

field vanish at

infinity,

so

that g

tends to the

Minkowski metric at

infinity (see

Remark 1.3 below for further

informations).

In this paper we consider a

completely

different behavior at

infinity

for g, and we are able to prove

that,

for any T &#x3E;

0,

there are

infinitely

many

spacelike 1-periodic T-trajectories

on the semiriemannian mani- fold

(R4 , g ).

Let {gij li, j

=1, ..., 4 be the

components

of g. We suppose

that g

not de-

pend

to the

time,

gij = gji E

C 1 (R3 , R ),

and

gi4=0

for i =

1,2,3.

We

set,

for = so

that we

have,

for every x and

every

E

R4 :

Moreover we assume that there exist &#x3E;

0, p

&#x3E; 2 and q E

]0,

p -

2[

such that for

every x, ~

E

R3 :

Then we have the

following

theorem.

THEOREM 1.1.

If (1.1)-(1.6)

are

satisfied, then, for

every T &#x3E;

0,

there exist

infinitely

many

spacelike 1-pe?iodic T-trajectories

on

(R4 , g).

REMARK 1.1. If and =

0,

it is easy to check that

z(s) = (xo , Ts)

is a trivial

periodic trajectory.

We shall see later that

the

trajectories given by

Theorem 1.1 are not

trivial,

and are

geometri-

cally

distinct.

(4)

REMARK 1.2. Condition

(1.3)

is a sort of

superquadraticity

condi-

tion at

infinity.

It has been introduced

by

P. H. Rabinowitz in the the- ory of Hamiltonian

systems. (1.4) implies

that there exists ci &#x3E; 0 such

that,

for every x E

R3 ,

with

I x I

; R:

Condition

(1.3)

means that

satisfied,

for

instance,

if

Moreover,

because of

(1.3),

there exists c2 &#x3E; 0 such that

for 1.

Infact,

let with 1. Since

we have

REMARK 1.3. The

problem

of

geodesics

for a Lorentz manifold

(M, g)

has been

recently

studied

by

many authors

(see [2]-[5], [7]-[12]).

If

particular,

in the papers

[5], [9],

are

given multiplicity

results for

timelike

periodic trajectories

on

(I~4 , g )

under the

assumption f3(x)

bounded.

The main difficult in the variational

approach

of this kind of

prob-

lems is that the action functional

is

strongly indefinite,

i.e. it is not of the form

identity

+

compact,

even

«modulo

compact perturbations».

In ordert to avoid this

difficult,

we

use the

convexity

of the functional with

respecto to i

and search for the critical

points

of a functional

f depending only

on x.

If is bounded as in

[9] (or

it is

subquadratic),

the functional

f

is

bounded from

below,

and satisfies

easily

the Palais-Smale

compactness

condition. In our case

f

is

unbounded,

so we need some

linking

argu-

ment ;

moreover more care is

required

in order to prove

compactness

conditions.

In Section 2 we expose the functional framework and we prove the

compactness

condition

using assumptions (1.1)-(1.5).

Then we prove Theorem 1.1 with a mountain pass

argument by using (1.6).

(5)

2. Proof of the results.

In the

following

we assume that

(1.1)-(1.5)

hold. Let as consider a

geodesic z(s) _ (x(s), t(s))

on

(R4 , g);

then z satisfies the

geodesic equations:

If z is a

a-periodic T-trajectory,

we shall call the minimal

period

of x, the minimal

period

of z. Notice

that,

if zl =

(xl , tl )

and z2 =

(X2, t2)

are

J-periodic T-trajectories

on

(I~4 , g),

with z, ;6 z2 , then zl and z2 are geo-

metrically

distinct.

In

fact,

if z2

(s)

= zl

(P(S))

for some

reparametrization ~(s),

from

geodesic equations

we have

p(s)

= as + b for some a, b E R

(see [14],

p.

69),

so that

t2 (s)

=

tl (as

+

b).

Since

il (s) -

0 for any s E

R,

from

tl (0) =

= 0 =

t2 (0)

= we have b =

0,

and from

aa)

=

t2 ( s

+

o~)

=

=

t2 (s)

+ + we have and a =

1,

which is im-

possible.

In

particular,

if zl and z2 have not the same minimal

period,

then its

are

geometrically

distinct.

REMARK 2.1. We observe now

that,

if

z(s) _ (x(s), t(s))

is a

k -1- periodic

Tk

-1-trajectory,

x and

i

are also

1-periodic

and

t( s

+

1 )

=

=

t(s)

+ T .

Infact,

it is easy to chek that

t( s

+

1)

=

t(s

+

( k - h )/h)

+

+

Th/k

for every h =

1, ..., k;

then z is a

1-periodic T-trajectory

on

(R4 , g),

with minimal

period

less or

equal

to

1 /k. So,

in order to prove

Theorem

1.1,

we can show that there exists

ko

E N such

that,

for every k E N with k &#x3E;

ko ,

there exists a

k-1-periodic Tk-1-trajectory z(s) =

- (x(s), t(s)),

0.

Let k E N be free for the

moment,

and let us consider the functional

defined on where is

the Sobolev space of

k-’-periodic

functions x:

R -~ R3

with

(6)

x, x E L 2 ([ 0, 1 /1~]),

and

It is easy to check

that,

if

(x, r¡)

is a critical

point

of

I,

then

s

z(s)

=

(x(s), t(s)),

where

t(s)

=

Ts/Ak +f n ds

is a critical

point

of the ac-

tion functional 0

so, it is a

1-periodic T-trajectory

on

(R4 , g),

with minimal

period

less or

equal

to

1 /k (see

Remark

2.1).

Notice

that,

because of

(1.4),

for

every x E H

---

H 1 ~ 2 (SIlk, R3 ),

the

1/k

functional is

strictly

convex, so it possess a

o

unique

minimum

point n x

E

R). Let f :

H -~ R be the functional

LEMMA 2.2. The

function

is continuous

from

H to

Lo R );

moreover

R)

acnd

so

that,

x E H is a critical

point of f if

and

only if ( x,

is a critical

point of

I.

PROOF. The

proof

is contained in

[9].

We recall it for the reader con- 1/k

venience. First of all we observe that

cause is a critical

point

of the functional i

(7)

, and then

Now,

let x, y E H.

Clearly

Moreover,

since

using (2.1)

we

get I(x,

as y - r, so

f

is continuous.

We prove now that is continuous.

Infact, arguing by

contra-

diction,

we suppose that there exist x E

H, (xn)

c H and s &#x3E; 0 such that

1 I,-

is

strictly

convex, we have

Since

(,u n)

is bounded

and rn

~ x, we

get I(x, ~u n) - I(xn ,

-~

0,

and and then we have a contradiction.

Finally,

fix x, y E

H,

and let 7 &#x3E; 0. From

(2.2)

we have

so the lemma is

REMARK 2.3. Notice that for every

(8)

In other

words,

there exists

cx E R

such that

f3(x(s))(T /k

+ 77 x

(s))

= cx for every s E R. Since 0

implies T/k

+

where M =

x ~ I

~

p ~,

and

I I

is the

Lebesgue

measure

of

I.

PROOF. Let cx be as in Remark

2.3,

so that +

’1)x(s)

=

for every s E R. If

s E I,

we have and then

Integrating

on

I,

we have:

Then

cz £

, so that the lemma is

proved. 0

LEMMA 2.5. Let 0 r p acnd

(xn)

c H be such that

0) ~

p. Then

where M = max

(9)

because of Lemma 2.4.

Moreover,

since

0) ~

r, we have p -

r ~ In ~ 1~2 ,

and the lemma follows.

In

We say that a functional

f:

H -~ R verifies the Palais-Smale-Cerami

(PSC)

condition

(see [6])

if every sequence

(xn)

c H such that -

~ c E R and

( f ’ (xn),

~ 0 possesses a

convergent

subse-

quence.

We have the

following

lemma.

LEMMA 2.6. There exists

ko

E N such

that, for every k a ko,

the

functionals f satisfies

the PSC-condition.

PROOF. Let

(R

is defined in

(1.3)),

and let

l~o

E N be such that a o -

T2 M/k6

&#x3E; 0. Fix k E N ivith k a

ko ,

and

let us consider a sequence

(xn)

c H such that c E R and

( f ’ (xn), xn~ -~

0 as n ~ ~ . First of

all,

we prove that

~~2)

is bounded

modulo

subsequences. Infact,

we

distinguish

two cases:

1) case:

for every

n E N, (modulo

subse-

quences).

Then

(Xn (s)) ~ xn (s))

for every s

(see (1.3)),

so,

from - c we

get (setting

77n *

Since

( f ’ (xn), xn) --~ 0,

we have

so that

then

(~~xn~~2)

is bounded because of

(1.2).

(10)

2)

case: for every

n E N, dist (Im (xn), 0)

R

(modulo

subse-

quences). Then,

if is

bounded,

we have

f3(xn (s)) ~ MI

for n

E N,

1/k

s E

R, so M1 T2 fk3,

and the claim follows from

o

the fact as n - oo.

So,

we can

assume IIxnIIoo

- 00. Let

In = {s E [ o,

+

1 ~;

from Lemma 2.5

(with r = R and p = R + 1 ),

we have

Then,

since - c,

so that

(see (1.1)):

claim follows.

We set now

shall prove that is bounded. In

fact,

we can assume that yin - y

weakly

in

HI,2

and

strongly

in

L °° ;

then

for n

large enough,

so

that,

since

(11)

so is bounded. Let us suppose xn - x

weakly

in

H1~ 2

and

strongly

L °° . Then

because of

(2.1)

we have that is

bounded,

so, the fact that

strongly

in

H,

and the lemma is

proved.

Let H =

R3) = R3

X

Y,

where

As well-known

(see

e.g.

[13],

p.

9),

for every y e Y we have

11?i112

a

and where a =

2kn( 1

+

4k2 n2)-1/2,

and b =

(1~12k)1 2.

We have now the

following

lemma.

LEMMA 2.7. There exist a, p &#x3E; 0 such that

f(y) &#x3E;

a

for

every y e Y with

IIyll

= P. Moreover a is

independent of

k.

PROOF. Fix c &#x3E; 0 such that ao -

ET2/V12

&#x3E; 0.

(1.5) implies

that

there exists p 1 &#x3E; 0 such that + for

lxl I

~ p 1. Set p =

p 1 /b

and

(12)

so

Since

a 2 ( a o - ~T2 b 2 /1~ 3 ) p i /b 2 &#x3E; ~

for every the lemma is

proved.

REMARK 2.8. Lemma 2.5

implies

that the functional

under

assumption (1.3)

is not

superquadratic

at

infinity

on finite-dimen- sional

subspaces

of H. This fact make not

possible

to

apply

the standard

linking

theorem

of f.

In order to avoid this

difficult,

we consider the sub- space E

= ~ x

E

H I x(s

+

1 /2k) _ - x(s)~. Clearly

E c

Y;

moreover we

have the

following

lemma.

LEMMA 2.9. Let us suppose that

(1.6)

holds.

Then,

every critical

point

x E E

of

the

functional

is a critical

point of f.

PROOF. Let x E E be a critical

point

and z E

H;

we shall prove

that ~ f ’ (x), z)

= 0. In

fact,

set z1

(s)

=

z(s) - z(s

+

1/2k),

and

Z2(S) =

=

z(s) - z1(s),

so that

ZIEE,

and Z=ZI+Z2.

Since (f’(x),zl)=O,

we have

( f ’ ( x ), z)

=

( f ’ ( x ), z2 ~.

From Remark

2.3,

there exists cx &#x3E; 0 such that + 77 x

(s))

= cx .

Since f3

is even and x E

E,

we have that Y)x

(s

+

+

1/2k)

=

77 x (s),

and then it is easy to

check, by using (1.6),

that

~ f ’ ( x ), Z2) = -(f’ ( x ), z),

and the lemma is

proved. 0

PROOF OF THEOREM 1.1. Let us suppose that

(1.1)-(1.6) hold,

let

ko

E N be as in Lemma

2.6, ~

&#x3E; 0 as in Lemma

2.7,

and such that k a

ko

&#x3E; 0. From Lemma

2.6,

the functional satis- fies the PSC condition on E. Let

sin (2kns), 0);

cleary w

E

E,

and since arP +

b,

we have

so that

(see

Remark

1.2)

+PoT 2Ik’, and f (w)

0

for r large enough (we

recall

that q

+ 2

p).

Set

(13)

Let p be as in Lemma

2.7; since f (0)

= 0 and we can assume

llwll

&#x3E; P, we have ~ ~ c + oo . From the mountain pass lemma

(see [1]),

we have

that c is a critical value for the

functionalfiE.

From Lemma 2.9 we

get

a

critical

point X

e H

of f with f(x)

= c. Since c &#x3E;

0,

we have 0. Because of Remark

2.1, z(s) = (x(s), t(s)),

where

t(s)

periodic T-trajectory

on

(R4 , g).

Finally,

in order to prove that z is

spacelike,

we observe that

so that

Ez

&#x3E;

0,

and Theorem 1.1 is

proved.0

REFERENCES

[1] A. AMROSETTI - P. H. RABINOWITZ, Dual variational methods in critical

point theory

and

applications,

J. Funct. Anal., 14 (1973), pp. 349-381.

[2] V. BENCI - D. FORTUNATO, Periodic

trajectories for

the Lorentz-metric

of

a

static

gravitational field,

in: Proc. on Variational Problems (D. BERESTICKI - J. M. CORON - E. EKELAND, Eds.), Paris (1989), pp. 13-18.

[3] V. BENCI - D. FORTUNATO, Existence

of geodesics for

the Lorentz-metric

of a stationary gravitational field,

Ann. Inst. Henri Poincaré, Anal. Non Lin- éaire, 7 (1) (1990).

[4] V. BENCI - D. FORTUNATO, On the existence

of infinitely

many

geodesic

on

space-time manifolds,

to appear on Adv. Math.

[5] V. BENCI - D. FORTUNATO - F. GIANNONI, On the existence

of multiple geodesics

in static

space-time,

Ann. Inst. Henri Poincaré, Anal. Non Linéaire, 8 (1991),

pp. 79-102.

(14)

[6] G. CERAMI, Un criterio di esistenza per i

punti

critici su varietà illimitate, Rend. Ist. Lomb. Sc. (A), 112 (1978), pp. 332-336.

[7] C. GRECO, Periodic

trajectories for

a class

of Lorentz-metrics of

a time-de-

pendent gravitational field,

Math. Ann., 287 (1990), pp. 515-521.

[8] C. GRECO, Periodic

trajectories

in static

space-times,

Proc.

Royal

Soc. Edin-

burgh,

113-A (1989), pp. 99-103.

[9] C. GRECO,

Multiple periodic trajectories

on

stationary space-times,

Ann.

Mat. Pura

Appl.,

(IV), 162 (1992), pp. 337-348.

[10] A. MASIELLO, Timelike

periodic trajectories

in

stationary

Lorentz

manifold,

Nonlin. Anal. T.M.A., 19 (1992), pp. 531-545.

[11] A. MASIELLO, On the existence

of

a closed

geodesic

on

stationary

Lorentz

manifold,

J. Diff.

Eqs.,

104 (1993), pp. 48-59.

[12] A. MASIELLO - L. PISANI, Existence

oftimelike trajectory for

a

time-dependent

Lorentz metric, Ann. Univ. Ferrara, (VII), 36 (1990), pp. 207-222.

[13] J. MAWHIN - M. WILLEM, Critical Point

Theory

and Hamiltonian

Systems, Springer-Verlag,

New York (1989).

[14] B.

O’NEILL,

Semi-Riemannian

Geometry.

With

Applications

to

Relativity,

Academic Press, London (1983).

[15] K. UHLENBECK, A Morse

theory for geodesics

on a Lorentz

manifold, Topolo-

gy, 14 (1975), pp. 69-90.

Manoscritto pervenuto in redazione il 27 novembre 1992.

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