A NNALES DE L ’I. H. P., SECTION A
D IEGO N OJA
A NDREA P OSILICANO
On the point limit of the Pauli-Fierz model
Annales de l’I. H. P., section A, tome 71, n
o4 (1999), p. 425-457
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425
On the point limit of the Pauli-Fierz model
Diego NOJA
AndreaPOSILICANO
a Dipartimento di Matematica, Universita di Milano, Via Saldini 50,1-20133 Milano, Italy
b Dipartimento di Scienze, Universita dell’Insubria, Via Lucini 3,1-22100 Como, Italy
Article received on 10 April 1997
~L71,n°4,1999, Physique theorique
ABSTRACT. - We continue in this paper the
analysis, begun
in(Noja
and
Posilicano, 1998),
of the classicaldynamics
of thepoint
limit ofthe Maxwell-Lorentz
system
indipole approximation (the
Pauli-Fierzmodel). Here,
as a firststep
towardsconsidering
the full nonlinearsystem,
we
study
the case in which a nonlinear external field of force ispresent.
We
study
the flow of theregularized (namely
with an extendedparticle) system,
and show that it converges in theappropriate
norm, as the radiusof the
particle
tends to zero, to the flow of a closedcoupled system
ofequations, containing
the renormalized massonly,
which soprovides
thevery definition of the
dynamics
of thesystem
in thepoint
limit. TheAbraham-Lorentz-Dirac
equation
for theparticle position
is deducedand turns out to
be,
in thisdescription,
aboundary
condition on thevector
potential, giving
the evolution of itssingularity. Moreover,
theHamiltonian structure of the limit
system
isdisplayed,
and it is shown that the standard Hamiltonian of the Pauli-Fierz model converges to the Hamiltonian of the limitsystem
heregiven.
@Elsevier,
ParisRESUME. - Nous
continuons,
dans cepapier, 1’ analyse
commenceedans
(Noja
andPosilicano, 1998),
de ladynamique classique
dusysteme
de Maxwell-Lorentz a la limite
ponctuelle
dans1’ approximation dipo-
laire
(modele
dePauli-Fierz). Ici,
commepremier
pas vers unsysteme complet nonlineaire,
nous etudions Ie cas danslequel
unchamps
exte-Annales de l’ Institut Henri Poincaré - Physique theorique - 0246-0211
Vol. 71/99/04/@ Elsevier, Paris
rieur de forces est
present.
Nous etudions Ie flot dusysteme regularise (c’ est-a-dire
avec uneparticule etendue),
et montronsqu’ il
converge dans la normeappropriee, lorsque
Ie rayon de laparticule
tends verszero,
versIe flot d’un
systeme couple d’équations,
contenant seulement la masserenormalisee,
definissant ladynamique
dusysteme
dans la limite ponc- tuelle. L’equation
de Abraham-Lorentz-Dirac pour laposition
de la par-ticule,
sepresente
comme une condition aux bords pour Iepotentiel
vec-toriel,
donnant 1’ evolution de sasingularite. Enfin,
nous donnons la struc- ture hamiltonienne dusysteme
limite et montrons que Ie hamiltonien du modele de Pauli-Fierz converge vers celui dusysteme
limite. @Elsevier,
Paris
1. INTRODUCTION
In a recent contribution
[8]
the authors succeeded indefining
thedynamics
of thesystem
constitutedby
afree charged point particle interacting
with theelectromagnetic
field in thedipole (or linearized) approximation.
As it is wellknown,
this is ahighly
nontrivialproblem
due to the fact that the Maxwell-Lorentz
system,
which of course should be used to describe thedynamics, is,
from arigorous point
ofview, meaningless
when apoint particle
is considered. Theanalogous problem
shows up in
quantum electrodynamics
too, where it is at theorigin
of thedivergences
which led to the introduction ofperturbative
renormalizationtheory.
The usual way out consists intrying
to define adynamics by taking
a suitable limit("point limit")
on aregularized
version of thesystem itself, typically
obtainedby attributing
aformfactor 03C1r
to theparticle.
Theregularized system
so obtained is often called the "Pauli- Fierz model"[9,3,2].
In[8]
it is shown how the flow of theregularized
system
converges to the flow of a well defineddynamical system
if andonly
if mass renormalization isperformed,
and a suitable constraint(conserved by
theevolution)
between the initial data of vectorpotential
and
particle velocity
isimposed.
Moreprecisely,
the limitsystem
for thevector
potential
A(which
in the Coulomb gauge is theonly
relevantvariable for the
field)
and theparticle position q
has the form(with
cAnnales de l’ Institut Henri Poincaré - Physique theorique
denoting
thespeed
oflight)
Here
Hm
is aself-adjoint operator,
bounded from below andcontaining
the renormalized mass
only;
such anoperator
turns out to be of the class of the so calledpoint
interactions[1]
and itsproperties
for thecase at hand are recalled below
(see
Theorems 2.1 and2.2). QA
is aquantity characterizing
thesingularity
of thegeneric
element A of the form domain of theoperator Hm, according
to the formulawhere Sr
denotes thesphere
of radius r about theorigin,
/~ is thecorresponding
surface measure, and e is theparticle
electriccharge.
So the
dynamics
of thesystem
iscompletely specified by solving
theabstract wave
equation
for the fieldgiven by
the first of( 1.1 ), correspond- ing
to initial data in a suitablephase
space, and thenrecovering
the timeevolution of the
particle position
from the secondequation
of thesystem ( 1.1 )
with the aid of formula( 1.2).
The main
goal
wouldbe,
of course, thestudy
of thepoint
limit forthe
complete
and relativistic Maxwell-Lorentzsystem.
But this is aproblem which,
up to now, we are not able to tackle. As a firststep,
in thepresent
paper, stillremaining
in the framework of thedipole approximation (i.e.,
linearization of theinteraction),
we consider thecase in which a
nonlinearity
is introducedthrough
an external nonlinearforce field
F(q) acting
on theparticle.
This still constitutes a non trivialgeneralization
because it is notpossible
to prove convergenceby using
the same
techniques exploited
in[8]
which wereessentially
based onlinear methods. In
particular
a fixedpoint method,
combined with someuniform
(with respect
to theparticle
radiusr) estimates,
is needed.By
the way, a furthergeneralization
is introduced in as much as itoccurs that
system ( 1.1 )
turns out to describeonly
situations in which the total linear momentumvanishes;
this is due to the fact that the constraint between initial data forparticle velocity
and vectorpotential,
which inVol. 71, n° 4-1999.
some form is necessary in order to obtain a limit at
all,
was chosen in[8]
in a form
stronger
than needed. Such a limitation will be removed here.The
procedure
of thepresent
novelapproach
can bebriefly
describedas follows.
Taking inspiration
from the Hamiltonian structure of theregularized
Pauli-Fierzequations,
we write(see (3.2))
a first ordersystem equivalent
to theoriginal
one,introducing
assupplementary
variables the total linear momentum and the electric fieldIt turns out
that, just
as in the free case, a limitsystem
exists if andonly
if mass is renormalized
according
to the traditionalprescription
where is the electrostatic energy of energy of the distribution pY ; this energy as it is well
known, diverges
to +00 asr t 0,
sothat,
as aconsequence, the bare mass mY
diverges
to -00 in the same limit. With this massrenormalization,
the limitsystem
is(see n this set 0
equations
is atamily
ot affineoperators parametrized by
total linear momentum p, and defined(see (3.3)
and Lemma4.1 )
in terms of the standardLaplacian
with onepoint interaction, namely
theoperator Hm already
studied in thequoted
paper.The
system
reduces to( 1.1 )
whenF(q)
=0,
as it isexpected,
butonly
with the initial condition po = 0.
Indeed,
asalready
mentionedabove,
the case treated in
[8]
is aparticular
onecorresponding
to solutions of thecoupled system
withvanishing
total linear momentum(see
Remark3.6).
Of course, due to the its
nonlinearity,
it is notpossible
to write downexplicitly
the flow ofsystem ( 1.4)
as it was done for the free casein
[8]. Nevertheless,
an alternative andexpressive picture
of thedynamics
l’Institut Henri Poinèare - Physique theorique
is
possible
forstrong
solutions of theCauchy problem ( 1.4).
Infact, exploiting
anequivalent
definition of the domain of theoperator
in which the
dynamics
of theparticle
appears as aboundary
condition onthe vector
potential (see
Lemma4.1 ),
it turns out that the these solutions coincide with thesolutions,
for the same initialdata,
of theCauchy problem
for thesystem (where Ào
isgiven
in Theorem2.2.)
(see
Theorem4.2).
Here0)
is the solution of the free waveequation
with the the same initial data for the field as the
system ( 1.4).
This is amore familiar
problem
in which a standard waveequation
iscoupled
withan
ordinary
differential one. Thisordinary
differentialequation
is a loworder version of the well known Abraham-Lorentz-Dirac eauation 4 7
so on one hand this much
questioned equation
is confirmed in thepresent
more
general
case, and on the other hand it is settled in aconvincing
mathematical context.
Finally,
we show that the limitsystem ( 1.4)
is in fact a Hamiltoniansystem,
and that thecorresponding
Hamiltonian function is the limit in awell defined sense of the classical Hamiltonian of the Pauli-Fierz model
(see
Theorem5.1).
Thisresult,
which answers a time honoredproblem (we quote only
the papers[6]
and[10]),
could be useful tostudy
themany open
questions
related toelectrodynamics
ofpoint particles (e.g.,
runaway
solutions, quantization...),
and couldperhaps give
valid hintsto
study
thefully
non linearsystem
withoutdipole approximation.
2. DEFINITIONS AND SOME PRELIMINARY RESULTS We
begin by recalling
some definitions and results from[8].
We denoteby
the Hilbert space of squareintegrable, divergence-free,
vectorVol. 71, n° 4-1999.
fields on
JR.3.
M will be theprojection
fromL3 (I~3),
the Hilbert space of squareintegrable
vector fields on onto and we will use thesame
symbol (’,’}(!!-
~[12
is thecorresponding
Hilbertnorm)
to denotethe scalar
products
inL 2 (1I~3 ) , L 3 (11~3 ) ,
and also to denote theobvious
pairing
between an element of and one of(the
result
being
a vector inJR3). By
the same abuse ofnotation, given
twofunctions
f
and g inL 2 (I~3 ) , by f
we will denote theoperator
in definedby f
(g)g(A)
:=f(g, A).
Moreover E?,
indicates the usual scale of Sobolev-Hilbert spaces, and themeaning
ofH3 (II~3)
and7~(!R~)
should now be clear. If y is a continuouspath
inJR3,
defined on the
compact
time interval1 (T )
:==[-T, T ], I) Y (I ~
denotesthe usual supremum norm. With we denote the space of
Lipschitz
vector fields.Finally, given
a measurablenon-negative
functionp we define its energy
E (p)
asTHEOREM 2.1
[8,
Theorem2.1]. -As r t 0, i.e., as
:=p a spherically symmetric probability density
with boundedsupport,
weakly
converges to ’80,
theself adjoint
operatorconverges in norm resolvent sense in to a
self-adjoint
operatorHm,
whereHm
has the resolventand where
If
m r = const thenHr
converges in norm resolvent sense in to -~. No otherdefinition of
therenormalized
mass mr(up
toO(r) terms)
leads to a limit
for Hr.
Annales de l’Institut Henri Poincare - Physique theorique
THEOREM 2.2
[8,
Theorem2.3]. -
The vectors A in the ’operator
domainD(Hm)
areof the
’ typeThe above
decomposition
in aregular
partA03BB, and a corresponding
$singular one, is unique, and
with A ED (Hm) of this form
one hasLet
Fm
be thequadratic form corresponding to
’Hm.
Then the vectors Ain
the form
domainD (F m)
areof the
’ typeGiven A E
D(Fm), QA can be explicitly computed by the formula
,where S,.
denotes thesphere
’of
radius r and is thecorresponding surface
measure. ’ The abovedecomposition
isunique, and
with A ED(Fm) of this form
one hasMoreover
and
where
-Ào
has athreefold degeneration
andare the
corresponding normalized eigenvectors,
where is anorthonormal basis.
Vol. 71, n ° 4-1999.
Remark 2.3. - This remark would
correspond
to Remark 2.5 in[8].
However,
here weproceed
in a different wayavoiding
the use of the fieldsX.
By
functionalcalculus,
andby
we
have,
for any X EL * (I~3 ) , ~,
>Ào
Analogously,
if À > and rsufficiently small,
we havewhere
Moreover, by
the definition ofQ A,
we haveLEMMA
2.4. - If
then
Annales de l’Institut Henri Poincaré - Physique theorique
Proof. - By (2.2)
we haveThe thesis follows
by (2.3), by Lebesque’s
dominated convergence theorem andNow we recall some results on abstract second order
equations (see [5]
for theproofs
of suchresults).
Let H be a bounded from below(this
is a necessarycondition) self-adjoint operator
onL*(1I~3),
and letF the
corresponding quadratic
form. Then Hgenerates
a cosineoperator
functioni.e.,
C is astrongly
continuous function such thatVol. 71, n ° 4-1999.
Moreover Vz E C such that
-z 2
Ep(H)
and Re z>
/B011/2
and so,
by
and
by
inverseLaplace transform, V~ ~ 0,
VA ED(N),
One defines then the sine
operator
function --+,C ( L * (II~3 ) ; L * (II~3 ) )
by
Obviously,
if H isstrictly positive, then, by
functionalcalculus,
Given
Ao, Ao
EL*(I~3),
X EC(R; L*(II~3)),
letThen A E
L * (I~3 ) ) .
IfA o Ao
E thenIf Ao
ED(H), Ao
ED(F),
X EL*(~3)),
thenAnnales de l’Institut Henri Poincaré - Physique theorique
and
A(t)
solves theinhomogeneous Cauchy problem
We will denote
by Sm(t),
andby Cr(t), Sr(t),
the cosine and sineoperator
functionscorresponding
toc2 H,~
andc2 respectively.
We conclude this section with the
following
lemma which is one of the main technicalpoints
of the paper.LEMMA 2.5. - For any y E
C(I (T ); :ae3)
o~e l~asBy
theinequality
it follows
71, n° 4-1999.
where C will be defined below. Since
and
- one has
and so
Now let C be a sequence such that
Then
Annales de l’Institut Henri Poincare - Physique theorique
and
Therefore,
ifX, := (Hm
+~, ) - 2 f ; ,
one hasand
so that
Since
in conclusions there follows
that,
for any ~ >0,
there existsj*
such that3. THE POINT LIMIT OF THE MAXWELL-LORENTZ
EQUATIONS
WITH AN EXTERNAL FORCELet us consider the
regularized
Maxwell-Lorentzsystem
in thedipole approximation
with an external forceF, i.e.,
thesystem
ofequations
onVol. 71, n° 4-1999.
L * (II~3 ) given by
Now,
as in[8],
we want tostudy
thepoint
limit0,
or p,.~ 80)
of such a
system.
At first we rewrite(3.1 )
aswhere
Fq(x)
:=F(x
+q).
Given anypath p
in R3 we define the time-dependent
operator, with domainLet us now
try
to determine thelimit,
as0,
ofHr,p.
Given ~, >Ào,
suppose that r is so small thatHr
+ À isstrictly positive,
and consider theCauchy problem
Annales de Henri Poincaré - Physique theorique
Its
(mild)
solution isgiven by
which,
after anintegration by parts,
can be rewritten as(here
and belowwe are
supposing
that p issufficiently regular)
~~B ..~/ ~yy I. / .~w 1 _1 .
By
Theorem 2.1 andby
Lemma2.5,
ifthen
where
Integrating by parts
we can rewrite the aboveexpression
asVol. 71, n° 4-1999.
This tell us that
solves the
Cauchy problem
and so
A(t)
solves theCauchy problem
This induces us to
define,
on thetime-dependent
domainthe
time-dependent
operatorgiven by
or,
alternatively, by
In the next two theorems we
give
the(local)existence
results for the twodynamical systems
definedby Eqs. (3.2)
andby
theirconjectured point
limit.
Annales de l’Institut Henri Poincaré - Physique théorique
THEOREM 3.1. - Let F E
Lip(R3; R3).
Then there , exists T >0, independent
such that theCauchy problem
has an
unique
’ mild solutionProof. -
Given T >0,
let us introduce the mapwhere
and where
~
EC(7(r); ~(R~))
nC’(/(r); L~(R~))
denotes the mildsolution of the
Cauchy problem
Vol. 71, n° 4-1999.
If we prove that
1/Ir
has anunique
fixedpoint
thengives
the solution. Let us now show that is a contraction onwhere c denotes the
Lipschitz
constant of F. Sincewe have
Since
(see (2.5))
by (2.6)
and(2.7)
it follows thatconverges,
uniformly
in t overcompact intervals,
and 0 so there ’ existsc ( T ) ,
withc(F) ~
0 asr ~ 0,
such thatAnnales de Henri Poincare - Physique " theorique "
Therefore
Since I -+
0,
we canchoose, independently of r, aT> 0
such thatand 0 the
proof
is concluded 0by
the contractionmapping principle.
DTHEOREM 3.2. - Let F E
R3).
Then there exists T > 0 such that theCauchy problem
/MM ~
Proof -
Given T >0,
let us introduce the mapwhere
~bl.71,n°4-1999.
and AY denotes the mild solution of the
Cauchy problem
with
If we prove
that 1/1
has anunique
fixedpoint y*
thengives
the solution. Let us now provethat 1/1
is a contraction.Defining
by (3.3),
AY solves theCauchy problem (3.8)
if andonly
if A solvesTherefore the solution of
(3.8)
isgiven by
which,
after anintegration by parts,
can be rewritten asAnnales de l’ Institut Henri Poincaré - Physique theorique
Therefore we have
and so there exists a T
sufficiently
small such that themap 03C8
is acontraction. The
proof
is then concludedby
the contractionmapping principle.
DBefore
stating
our convergence theorem we need thefollowing prelim- inary
result:THEOREM
3.3. - For any 03B3r
E]R3),
r >0,
T >0,
letVol. 71, n° 4-1999.
be the ’ mild solution
of the
’Cauchy problem
with ~. >
1 If
then
where A E
C(/(r);
nL*(IL~3))
is the ’ mild solutionof the
’Cauchy problem
Proof. - By proceeding
as in theproof
of[8,
Theorem2.8],
andby
the definitions of
Hr, Yr
and it will suffice to prove theanalogous
statements for the mild solutions of the
Cauchy problems (À
>Ào)
~nrt
l’Institut Henri Poincaré - Physique theorique
Proceeding
as in the calculations aboveleading
to the definition of(see
thebeginning
of thissection),
we have that the solution of the firstproblem
isgiven by
and the solution of the second one is
given by
Now, by
the knownstrong
resolvent convergence ofHr
toHm (see
Theorem
2.1),
andby
theC
1 convergence of to y, theproof
isconcluded
by
Lemma 2.5. DWe now come to the main result of this paper:
THEOREM 3.4. - Let
Lip(R3; }R3), |F(x)| M0(1+|x|), 03BB
>03BB0,
and
Eo
EL * (IIg3 ).
LetAo
EH* (II~3 ), Ao
E such thatThen there exists T > 0 such
that, if
Vol. 71,~4-1999.
denotes the ’ mild solution
of the
’Cauchy problem
then
where
denotes the ’ mild solution
of the
’Cauchy problem
Proof. -
Let us denoteby yr
andy*
the fixedpoints
of themaps ~,.
(see (3.4)) and 03C8 (see (3.7)), respectively.
If we prove thatAnnales de Henri Poincaré - Physique theorique
then, obviously,
and so the
proof
is concludedby
Theorem 3.3. Let us consider anarbitrary family
such
that!!/, - y!~ ~ 0,
y EJR3). Then, writing
by
Theorem 3.3 we haveTherefore, by
Lemma2.4,
we haveThis
gives
and so for anv n E N.
Since
y,*
=by (3.5)
and(3.6), defining
we have
Bbl.71,n° 4-1999.
Therefore,
if rand Taresufficiently small,
thenand so
These results
imply, denoting by
or 1 the common,independent
of r,constant of
contractivity
of~r and 1/1,
Therefore
(3 .11 )
is proven, and theproof
is done. 0Remark 3.5. - Here we make the connection with the results
obtained,
for the case F =
0,
in[8].
The results there stated are aparticular
caseof the ones
given
here: indeed in[8, Corollary 2.9]
the initial fieldsAo
and
Ao
are notarbitrary
elements in/~(R~)
andD(Fm), respectively, (however, they belong
toL2-dense
subsets of7~(!R~)
andD(Fm), respectively).
Moreover the convergence conditions(3.9)
are weaker than the(2.8)
used in[8].
In thepresent setting, writing Ao
=(Hr
+~,)-1~2~0,
these would
correspond,
besides(3.9),
toSince the relations
(2.8)
in[8]
are declared to be necessary and sufficient for the convergence, a contradiction seems to appear. This is not the case.Indeed in
[8]
we studied the limit of the Maxwell-Lorentzsystem
whenAnnales de l’Institut Henri Poincaré - Physique theorique
the limit total linear momentum po is
vanishing.
In fact onehas, by (2.2), (2.3),
and(3.9)
and so,
given (3.9), (3.12)
isequivalent
to po = 0. This is consistent with the fact that the limitequations (3.10) coincide,
in the case F ==0,
po =
0,
with the ones obtained in[8].
As a last remarkregarding [8]
letus
point
outthat, since,
when F =0,
the linear momentum isconserved,
the condition(3.12)
ispreserved by
the flow.4. THE LIMIT DYNAMICS
In this section we want to
give
a more detaileddescription
of thesolution of the
Cauchy problem (3.10).
Let usbegin
with an alternative characterization of the domain ofHm,p. By
Theorem 2.2 we have that the vectors inD(Hm,p)
are of thetype
This
obviously implies
Vol. 71, n° 4-1999.
and, by the definition of we have
-Since
in conclusion we have the
following
and
the following
$boundary
condition holds:Moreover
The next result is
analogous
to Theorem 3.3 in[8]:
it characterizes the solutions of the limitEq. (3.10).
THEOREM 4.2. - Given F E let
Annales de l’Institut Henri Poincare - Physique theorique
be the ’ strict solution
of the
’Cauchy problem
Then
where ,
I
the solutionof the free
waveequation
with initial dataAo, Eo,
andwhere B denotes the Heaviside
function.
MoreoverQA satisfies
theequation
Proof. -
Letwhere
denotes the retarded
potential
of the source and denotes the solution of the free waveequation
with initial dataAo,
andEo.
ThereforeA(t)
satisfies the distributionalequation
By
the Kirchhoff formula one canverify
thatA f gives
no contributionto
QA (see [8]).
ThereforeQ(t). Since, by
anelementary integration,
Vol. 71, n° 4-1999.
we have that A satisfies the
boundary
condition(4.1)
if andonly
if(4.3)
holds true.By
Lemma 4.1(applied
in the case p =0)and by [8,
Theorem
3.3]
it follows thatand so,
by
Lemma 4.1again,
we have A ED(Hm,p).
Theproof
is thenconcluded
by
the distributionalidentity
Remark 4.3. -
Alternatively
Theorem 4.2 can berephrased by saying
that the strict solution of
(4.2)
coincides with the solution of theCauchy problem
Differentiating (when possible) Eq. (4.4),
we obtain the classical Abra- ham-Lorentz-Diracequation
where to : =
2e2 3mc3.
Annales de l’Institut Henri Poincare - Physique theorique
5. THE HAMILTONIAN STRUCTURE
By
the definition(3.3),
andby D(Hm,p)
CD(Fm),
we haveTherefore,
in the case F ==2014W, Eqs. (4.2)
arenothing
but the Hamiltonequations corresponding
to the(degenerate)
Hamiltonianthis is defined on the
symplectic
vector space(D(Fm)
x xS2o),
whereS2o
denotes the standardsymplectic
formMoreover one has the
following
convergence result:THEOREM
be the ’ Hamiltonian
giving
,Eqs. (2.2), defined
on thesymplectic
vectorspace
(H;(IR3)
x xIR6,
Let E E, p )
EIR6,
andlet
Ar
E A eD(Fm) satisfy the
condition(3.9).
ThenProof. -
Let us writeSince, by (3.9)
and Lemma2.4,
one hasobviously
it will suffice to prove thatVol. 71, n ° 4-1999.
By
Remark 2.3 one obtainsBy (2.3), (2.7), (3.9),
andby
Annales de Henri Poincare - Physique " theorique "
the
proof
is done if we prove thatObviously
this isequivalent
to prove that{~/F(2014A
+À)-1 weakly
converges to zero in
L 2 (II~3 ) . Evidently
such afamily weakly
converges to zero on a dense set, and so weonly
need to prove that it is bounded inL 2 (II~3 ) .
This is truesince, by
standard S obolevestimates,
one has[1] S. ALBEVERIO, F. GESZTESY, R. HØEGH-KROHN and H. HOLDEN, Solvable Models in Quantum Mechanics, Springer, New York, 1988.
[2] A. ARAI, Rigorous theory of spectra and radiation for a model in quantum electrodynamics, J. Math. Phys. 24 (1983) 1896-1910.
[3] P. BLANCHARD, Discussion mathematique du modèle de Pauli-Fierz relatif au
catastrophe infrarouge, Commun. Math. Phys. 15 (1969) 156-172.
[4] P.A.M. DIRAC, Classical theory of
radiating
electrons, Proc. Roy. Soc. A 167 (1938)148-168.
[5] H.O. FATTORINI, Second Order Linear Differential Equations in Banach Spaces, North-Holland, Amsterdam, 1985.
[6] H.A. KRAMERS, Nonrelativistic quantum electrodynamics and the correspondence principle, in: R. Stoops, ed., Rapports et Discussions du Huitieme Conseil de
Physique Solvay, Brussels, 1950.
[7] H.A. LORENTZ, The Theory of Electrons, 2nd Ed., Dover, New York, 1952.
[8] D. NOJA and A. POSILICANO, The wave equation with one point interaction and the
(linearized) classical electrodynamics of a point particle, Ann. Inst. Henri Poincaré
68 (1998) 351-377.
[9] W. PAULI and M. FIERZ, Zur Theorie der Emission Langwelliger Lichtquanten,
Nuovo Cimento 15 (1938) 168-188.
[10] N.G. VANKAMPEN, Contributions to the quantum theory of light scattering, Kgl.
Danske. Videnskab. Selskab, Mat. Fys. Medd. 26 (15) (1951).
Vol. 71, n° 4-1999.