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A NNALES DE L ’I. H. P., SECTION A

J OÃO -P AULO D IAS

M ARIO F IGUEIRA J EFFREY R AUCH

Scattering for a one-sided Klein-Gordon equation in quantum gravity

Annales de l’I. H. P., section A, tome 61, n

o

1 (1994), p. 75-86

<http://www.numdam.org/item?id=AIHPA_1994__61_1_75_0>

© Gauthier-Villars, 1994, tous droits réservés.

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Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques

http://www.numdam.org/

(2)

75

Scattering for

a

one-sided Klein-Gordon

equation in quantum gravity

João-Paulo

DIAS,

Mario FIGUEIRA

Jeffrey

RAUCH

CMAF,

University

of Lisdon, Av. Prof. Gama Pinto, 1699 Lisboa Codex, Portugal

Department of Mathematics, University of

Michigan,

Ann Arbor, MI 48109-1003, U.S.A.

Vol. 61, n° 1,1994 Physique theorique

ABSTRACT. - In this paper we consider a Klein-Gordon

equation

in

one space dimension with a class of smooth

positive increasing potentials

V motivated

by

a model in

quantum gravity.

For

large

times the wave

propagate freely

to the left. We prove

decay

in time estimates and

asymptotic completeness justifying

this

phrase.

Dans cet article nous considerons une

equation

de Klein-

Gordon dans une dimension

d’espace

avec une classe de

potentiels reguliers positifs

et croissants V motivee par un modele en

gravite quantique.

Pour

des

grandes

valeurs du

temps

l’onde se prop age librement a

gauche.

Nous donnons des estimations de decroissance

temporelle

et prouvons la

completude asymptotique

en

justifiant

cette

phrase.

Annales de l’Institut Henri Poincaré - Physique theorique - 0246-0211

Vol. 61/94/01/$

(3)

1.

INTRODUCTION

AND MAIN RESULTS

This paper is motivated

by

the results obtained in

[2]

on the

decay

of

the solutions of the

following equation

where p E R is a constant and

(z, y)

E

1R2.

This

equation

is

obtained, by

the transformation u

(z, ?/)

=

(x, y),

z =

log

x, x &#x3E;

0,

from the

simplified

Wheeler-DeWitt

equation

with a

massless

single

scalar

field y (cf [4])

where x E

R+

is a scale factor

(radius

of the

Universe),

p E R is a constant which reflects the

factor-ordering ambiguity and 03C8

:

IR+

x R ~ is the

wave function of the Universe for the

minisuperspace

model.

As a consequence of the results in this paper we conclude

that,

for

large

values of ~/, the wave

function ~ propagates freely

near the

origin,

that is

the term is

negligable,

and is very small for

large

values of x.

We

study

the

asymptotic

behaviour and

scattering properties

of the

solutions of the Klein-Gordon

equation

where the

potential

V satisfies

It is well known that the

operator Ao :

D --&#x3E;

L~ (~)

defined

by

Annales de l’Institut Henri Poincaré - Physique theorique

(4)

with domain

is

self-adjoint

in

LZ (R).

Let

~ = {u

E

H1

E

LZ (ff8)}

with its natural norm and

put

It is easy to see that the

operator A,

with domain D

(A),

is

self-adjoint

in

H.

Denote

by e-itA

the

unitary

group in ~-l

generated by

2014zA

For cp =

(uo,

E D

(~4),

denote

by

t6

(t)

=

e-itA

cp the

corresponding

solution of the

Cauchy problem ( ~(0)

= uo,

-~2014 (0)

= for the

equation ( 1.2).

Let

(~)

x

L2 (P~),

B :

D(B) -. D (B)

x

H1,

where B is the

self-adjoint operator

in defined

by

Denote

by

the

(free) unitary

group in

xo generated by

2014zB. The

operator

B has constant

coefficients,

D

(A)

c D

(B) and,

on D

(~4),

The estimates of

[2]

show that the solutions of

( 1.2)

are small in x &#x3E; 0 for t ~ oo. Our main result asserts that the solutions are

asymptotically equal

to solutions of the free Klein-Gordon

equation

which travel to the left. For t ~ oo, it is free waves

travelling

to the

right (for

time

increasing)

with intervenue. In a sense this is a three space

scatteririg theory.

Write the finite energy free solutions as

The f term has group

velocity equal

to

T~!/(~).

The waves with

plus sign

travel to the left and those with a minus to the

right.

For

example,

if

a+ E

Co (R B 0)

then the

plus

term has

LZ (]0, +00 [)

norm which tends

(5)

to zero faster than any power of

1/t

as t tends to +00. The same is true

for all derivatives

(apply

the results in app. 1 to XI.3 in

[6]).

The energy in is

equal

to

Thus

?~o

=

~+ EB 1-

~_ where denotes the space of solutions with

a~ _

0. One has

Thus

(t6o,

E = Note the familiar Hilbert

transform

sgn (D).

The

following

result has a

proof

similar to the

proof

of theorem 2 in

[2].

THEOREM 1. - Assume cp =

(l6o, Ul)

E

D (A2).

Then

By

an

adaptation

of the

proof

of the theorem 3 in

[2]

we will prove the

following:

THEOREM 2. -

Assume 03C6

=

(uo,

E

(D(R))2.

Then u E

C4(R2), u (~, t) at ~~’ t~

E

In

addition,

COROLLARY. -

(i) If

~p E

(D ( I~ ) ) 2 and, for

a E

IR, Ha

=

H 1 (] a, -f- oo ~)

X

L2 (] a, +~[),

then lim

~e-itA 03C6~Ha

= p.

(ii) If Pac

=

Pac (A)

denote

the

orthogonal projection of

H onto the

subspace of

absolute

continuity for A,

then

Pa~

= Id .

The first

part

of the

corollary

is an immediate consequence of theorems 1 and

2 , since dV dx ~

a 1 &#x3E; 0 in

[ a

,

+oo[ [ [by ( 1.3)].

The second

part

will be

provided

as a consequence of

( 1.7).

Annales de l’Institut Henri Poincare - Physique theorique

(6)

Similar results can be

proved

for the

corresponding Schrodinger equation

i

~v ~t

+

20142014 -

V v = 0

(cf [3]

for the

special

case V

(x)

=

Choose

It is easy to see that

Our main results are

THEOREM 3

(Existence

of the wave

operators). -

For each C{J E

~=p

there

exists a

unique (resp.

in H such that

We have cp~ ~ = M~ ~p = lim

eiAt

x

e-iBt

cp in ~L and the maps M~ :

?~C~ --~

?-~ are bounded.

THEOREM 4

(Completeness

of the wave

operators). -

For

each ~

E ~-C

there exists a

unique ~_ (resp. ~+)

in

~~

such that

We

lim

eiBt e-iAt 03C8 in H0,

and the

maps 03C8 ~ 03C8~

are

bounded inverses

of

the maps M-=f

defined in

theorem 3. In

addition, if Y (x)

=

e~x, ~

&#x3E;

0,

then the

map S

=

(M+)-1 M- :

?~. -~

an

isometry..

-

For the

proof

of theorems

3, 4,

we use the

asymetric

Birman-Kato

theory,

more

precisely

the theorem in

[5],

and

(for

theorem

4)

the

corollary

of theorems 1 and 2. Note that the

asymmetry

of the

problem

forces us

to use the Birman-Kato

theory

two

times,

once for existence

and,

in a different way, for

completeness. Analogous

results can be

proved

for the

Schrodinger equation

Vol. 61, n° 1-1994.

(7)

using decay

estimates

extending

those of

[3] proved

for the

special

case

VM - e4x.

The two first authors were

supported by

the JNICT

project

PMCT/C/CEN/18/90 and

by

the Gulbenkian

Foundation/Deptm.

of

Mathematics of the

University

of Lisbon

project.

The third author was

supported by

the NSF

grant

DMS 8601783 and

by

the ONR

grant

NO 01492J1245.

2. PROOF OF THEOREM 2

Assume cp

=

ul) - ~(0))

E

(D (~))z

c

D (A4).

Since V E

C3

it is easy to see that the

corresponding

solution of the

Cauchy problem u belongs

to

C4 (1R2)

and that for

each t, t6(’, t)

E

Co ~~ ~ ~ ~ ~ ~ have, for

v =

d~,

Multiply

the

equation (2.1) by -.,

then

integrate

in .r E R and take the real

part.

This

yields,

with

Thus,

for

~ 0,~

&#x3E;

0,

Annales de l’Institut Henri Poincaré - Physique theorique

(8)

Now, multiply

the

equation (2.1) by 2014, integrate

in x E R and take

the real

part

to iind

and

Hence,

and so,

by ( 1.3),

Now, (2.2)

and

(2.3) yield,

with a suitable 03B4 &#x3E;

0,

On the other

hand,

it is easy to see that the

proof

of

proposition

3.1

in

[2] yields

Hence, using (2.3), 2.4

and

2.5

we obtain

Vol. 61, n° 1-1994.

(9)

Taking

the t derivative in

equation (2.1), replacing

v

by ~v ~t

-- ~ ~x(~u ~t) and

imitating

the

proof using (2.5), yields

The two

inequalities (2.6), (2.7)

with a classical

argument employed

for

example

in the

proof

of the theorem 2 in

[2], imply

Time

reversibility completes

the

proof

of theorem 2..

PROOF OF PART

(ii)

OF THE COROLLARY. - For cP E

(P (~))2

a dense subset of

7~,

we have

The second

part

of theorem 2

implies

that the l.h.s.

belongs

to

L2 (R).

Therefore,

the Fourier transform of the bounded measure

~p) belongs

to

L2 (R).

Thus the measure is

absolutely

continuous so

Pa~

=

.

3. PROOF OF THEOREMS 3 AND 4

PROOF OF THEOREM 3. - Let

111 = H 2

X

H1 (R), 112

== 11 =

Hv

X

L2,

Hl

=

H2

= A and J :

111

2014~

112

the linear continuous

operator

defined

by

J =

where x

is the function defined in

( 1.8).

We

have, for cp

E

H3

x

H2,

with y

=

H103C6

E

Furthermore,

c and

[extended

to as an element of

~2)].

Annales de l’Institut Henri Poincaré - Physique theorique

(10)

On the other

hand,

we have

Thus, ( u, v )

E we

get

Theorem 3.2 in

[ 1 ] implies

that the

operator H2 J - JH1

is a trace class

operator

from into

7~2.

This and the theorem in

[5] imply

that the limits

exist in

~2

= ~.

By density

we can take cp E

xo

=

H1

x

L2,

and it follows

immediatelly that,

if =

eiAt

x

e-iBt

cp,

To prove

unicity,

suppose that 03C6 E

H+

and 0 = 03C6+ =

lim ezAt

in x. Then

Moreover,

Hence,

PROOF OF THEOREM 4. - Let =

D ~ AZ ~ , ~ 2

=

~0

X

£2,

H1

=

H2

= Band 0 -4

~C2

defined

by

J = where

61, n°

(11)

Since the

projection (in

onto the

subspace

of absolute

continuity

for

HI

is

Pac|H1

=

Id,

we

have, for cp

E D

(A3),

with 03C8

=

H103C6

# E

Furthermore,

=

(u, v)

E we obtain

(by extending

£

H2

J-

JHl

To estimate the last term write

/ 2 B

where we have used the fact that v G D

[ 2014 2014-

+ 1 +

VJ implies

that

2014 (-d2 dx2

+ 1 + e

L2

and the map from D

(-d2 dx2

+ 1 +

v)

to

L2

so defined is continuous

(the proof

is

exactly

as for the case

V

(~r)

=

e4x

which is

presented

in section 3 of

[3]).

We

conclude, by

the

theorem 3.2 in

[1]

that the

operator ~2

~ ~

JHl

is a trace class

operator

from

~1

into

7~2. Hence, by

the theorem in

[5]

we conclude that the limits

exist in

~C2

=

By density,

the same limits exist for

Annales de l’Institut Henri Poincare - Physique theorique

(12)

For such y~, let

The next

step

is to prove that

This

implies

that

and so cp+ E

H+

and =

~eiBt e-iAt 03C6~H0 ~ 11’P111t.

Choose cpn E

(D (1R))2,

n =

1,2, ... ,

such that cpn ~ cp in ~‘~C. We have

Since,

for each n, and

by

the

corollary

of theorems 1 and

2, part (i),

~(1 2014 x)

cpn 20142014~

0,

we

conclude, by

standard

arguments,

that ---7 o.

Now,

we derive

are

therefore, by

similar

arguments,

Finally,

let S =

(M+)-1 M- .

7~ 2014~

?~+

which is

bijective

and

bicontinuous. Assume

V(x)

=

e03BBx, 03BB

&#x3E; 0.

Let 03C8

=

Since

D (A2)

is dense in 7l we can

assume ~

E

Hence, by

theorem 1 and since

2014 = AV,

we

get

61, n°

(13)

Moreover,

we have ’P-J: = lim

eitB

in

~fo

and so

t2014~+oo

[1] E. B. DAVIES and B. SIMON, Scattering Theory for Systems with Different Spatial Asymptotics

on the Left and Right, Commun. Math. Phys., Vol. 63, 1978, pp. 277-301.

[2] J. P. DIAS and M. FIGUEIRA, On a class of solutions for the simplified Wheeler-DeWitt

equation with a massless single scalar field, to appear in Ricerche di Matematica.

[3] J. P. DIAS and M. FIGUEIRA, On a singular limit for a class of solutions for the simplified

Wheeler-DeWitt equation with a massless single scalar field, Rendic. di Mat., Vol. 13, 1993, pp. 529-542.

[4] G. W. GIBBONS and L. P. GRISHCHUK, What is a typical wave function for the Universe?, Nucl. Phys. B, Vol. 313, 1989, pp. 736-748.

[5] D. B. PEARSON, A Generalization of the Birman Trace Theorem, J. Funct. Anal., Vol. 28, 1978, pp. 182-186.

[6] M. REED and B. SIMON, Methods of Modern Mathematical Physics, III: Scattering Theory, Academic Press, New York, 1979.

(Manuscript received July 12, 1993;

revised version received October 10, 1993.)

Annales de Henri Poiricare - Physique theorique

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