A NNALES DE L ’I. H. P., SECTION A
E. F ROCHAUX
New representations of the Poincaré group describing two interacting bosons
Annales de l’I. H. P., section A, tome 71, n
o2 (1999), p. 217-239
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217
New representations of the Poincaré group
describing two interacting bosons
E.
FROCHAUX1
Departement de Mathematiques, Ecole Poly technique Federale de Lausanne, CH-1015 Lausanne, Switzerland
Article received on 1 December 1997
Vol. 71, n° 2, 1999, Physique theorique
ABSTRACT. - New
representations
of the Poincare group aregiven,
which describe two bosons with interaction in four
space-time
dimen-sions. The
quantum
frame is theSchrodinger picture
in momentum space.More
precisely
we start from the relativistic free model with Hilbert spaceX where c~2 is the Lorentz invariant measure. We add to the free Hamiltonian and the free Lorentz
generators
new interaction terms, withoutchanging
the Poincarealgebra
commutationrules,
and such that thealgebra representation
can beintegrated
togive
aunitary
represen- tation of the group onL2(II~6, cr2).
Thephysics
of these models can beinvestigated through
the bound stateequation (a
relativisticSchrödinger equation)
andthrough
thescattering matrix,
which is shown to be uni-tary. Finally
wegive
anexample
for which a bound state exists and for which thescattering
matrix can be written downexplicitely.
This exam-ple
assures that interaction caneffectively
occur between theparticles.
@
Elsevier,
ParisRESUME. - Nous etablissons de nouvelles
representations
du groupe de Poincare decrivant deux bosons en interaction dans unespace-temps
a quatre dimensions. Le cadrequantique
est celui de larepresentation
de
Schrodinger
dansl’espace
des moments. Plusprecisement,
nousI E-mail: efrauchau @ worldcom.ch.
Annales de l’Institut Henri Poincaré - Physique theorique - 0246-0211 I
Vol. 71 /99/02/© Elsevier, Paris
partons
de larepresentation
decrivant deux bosonslibres,
dont1’ espace
de Hilbert des etats est X
c~2),
ou cr2 est la mesure invariante de Lorentz. Nousajoutons
a l’Hamiltonien et auxgenerateurs
de Lorentz denouveaux termes, dits
d’interaction,
sans briser lesregles
de commutation del’algèbre
dePoincare,
et de sorte que larepresentation
deFalgebre puisse s’integrer
et donner unerepresentation
unitaire du groupe,toujours
dans
L2 (II~6, c~2) .
Laphysique
de ces modeles est accessiblegrace
a uneequation
aux valeurs propres pour les etats lies(une
sorted’équation de Schrödinger relativiste)
etgrace
a 1’ existence de la matrice dediffusion, qui
s’ avere etre unitaire. Finalement nous donnons unexemple
pourlequel
un etat lie existe et pourlequel
la matrice de diffusionpeut
etre ecriteexplicitement.
Cetexemple
nous assurequ’une
interaction entreparticules peut
effectivement avoir lieu dans ces modeles. (c)Elsevier,
Paris1. INTRODUCTION
A new
family
ofunitary representations
of the Poincare group in fourspace-time
dimensions isgiven,
which describe two bosonsystems
with interaction. Thequantum
frame is theSchrodinger picture
ofQuantum
Mechanics in momentum space. The
physics
of these models can be obtained from thescattering operator
and the bound stateequation,
an
eigenvalue equation
of the kind of theSchrodinger equation.
Theexistence of a bound state and the
non-triviality
of thescattering
matrixconfirm that the interaction is effective. To our
knowledge,
this is the firstexample
of relativisticquantum
models for a finitenumber
ofinteracting particles.
Moreoverthey
admit a rathersimple
mathematical construction.The
quantum
frame of theSchrodinger picture
means that the Hilbert state space issimply
made of functions of the momenta. Inparticular
thetime variable does not appear
explicitly. However,
these modelssatisfy
the relativistic
principles,
becausethey
consist ofunitary representations
of the Poincare group. An
elementary example
of such a model isgiven by
the free model for two bosons(’free’
means withoutinteraction).
Our models are obtained
by perturbations
of the Hamiltonian and the Lorentzgenerators
of the freemodel,
in such a way that the commutation rules of the Poincarealgebra
remain satisfied. The existence of solutionsAnnales de l’Institut Poincaré - Physique theorique
to this
problem
is rathersurprising. Indeed,
such aperturbation
of theHamiltonian and the Lorentz
generators
hasalready
beenproposed by
Dirac in the late 40’s
[ 1 ],
in the framework of classical mechanics. Diracthought
that the classicaltheory
should be establishedfirst,
and that thequantum
version would be obtained afterwardsby applying
the canonicalquantization.
Therefore his paper concernsonly
classicalphysics,
and itdoes not
really
obtain aninteresting
conclusion. In theearly 60’s,
Curriecontinued this
approach,
still in the classical frame. He obtained in[2]
that,
under additional naturalassumptions,
such modifications cannotgenerate
an interaction(this
is known as the ’non-interactiontheorem’).
The
present
paper shows thatby going directly
to thequantum frame,
thisdifficulty
can be overcome.The result
given
here is thegeneralization
of similar results in 2-d(two space-time dimensions) [3]
and in 3-d[4]. Although
thefamily
of models in
[3]
is verygeneral (the
kernel of the interactionpart
of the Hamiltonian can be chosen almostarbitrarily
in the centre-of-massframe),
in 3-d and 4-d we haveonly managed
to construct models withspecial
interaction terms(excuding
local interactionsby
apotential).
Moreover,
thegeneralization
to more than twoparticles [5]
and to bosonswith different masses
[6],
which is easy in2-d,
seems difficult inhigher space-time
dimensions.Originally,
the result in2-d
wassuggested by
a newapproch
of thebound state
problem
in 2-dQuantum
FieldTheory,
see[4].
The paper is
organized
as follows. Section 2presents
afamily
ofoperators
whichformally satisfy
the commutation rules of the Poincarealgebra, provided
the ’interaction kernel’ h(the
kernel of the interaction term of theHamiltonian)
satisfies a ’fundamentalequation’.
In Section 3the
complete
set of solutions to thisequation
isgiven,
in the weakcoupling regime.
Then we focus on a subset of solutions whichsatisfy
all the
properties
we need for thefollowing proofs.
Section 4 shows that the formalrepresentations
of the Poincarealgebra
of Section 2can be
integrated
togive unitary representations
of the Poincare group.Section 5
presents
theeigenvalue equation
for the bound states(the
’relativistic
Schrodinger equation’).
Section 6 establishes the existence oftwo-particle asymptotic
states and of thescattering operator,
which appears to beunitary.
Section 7gives
asimple example (one-dimensional perturbation)
for which the bound stateequation
admits a solution and for which thescattering
matrix can be written downexplicitly
andis non-trivial.
Finally,
Section 8 collects thephysical
results of the paper.Vol. 71, n° 2-1999.
This paper follows
closely [4].
For acomplete, detailed,
and self-contained version see the
preprint,
available at mp-arc 98-305.2. THE MODELS
The Poincare group
~+
isgenerated by
the tenoperators
H(Hamil-
tonian),
P =(Pi, P2 , P3 ) (momentum),
J =(7i, ,12, J3 ) (angular
mo-mentum)
and L =(Li, L 2, L 3 ) (generators
of the Lorentz transforma-tions), satisfying
the standard commutation rules of the Liealgebra ~
of
7~.
Thisalgebra
admits two Casimiroperators,
the massoperator
M and the Pauli-Lubanskioperator W,
the squares of which aregiven by
where the dot "’" and the
wedge
"n" denote theordinary
scalar and vec- torproducts, respectively.
We start from the
representation describing
twofree, identical,
andspinless particles
of mass m >0,
in theSchrodinger picture.
Ifpl,
p2 E
R3
are the momenta of the twoparticles,
the total and relative momentaP , Q
are definedby
where
c~ ( pi )
:=p2 + m2, i
E{ 1, 2}
and(The variable Q
is defined as the momentum in the centre-of-massframe.)
In thesevariables,
theoperators
of the freerepresentation
are thefollowing
for almost all
( P , Q )
ER6
and suitable functions03C6,
where we haveput
l’Institut Henri Poincaré - Physique theorique
These
operators
define arepresentation
of thealgebra ~
which can beintegrated
togive
aunitary
and continuousrepresentation
of the group7~,
in the Hilbert spacemade of even functions with
respect
toQ (Le., ~(P, Q ) _ ~ ( P , - Q ) ),
where =
In the non-relativistic case, it is
possible
to find relative variables whichare invariant under the proper Galilean transformations. Such variables cannot be found in the relativistic case. In
(3)
the Lorentzgenerators
contain a terminvolving 7~, i.e., acting
on6.
Note thatonly
theangular
.variables of
Q
areconcerned,
becauseis Lorentz invariant. This can also be seen from the Casimir
operators,
which areonly
functions ofQ 2
and(JQ)2
To introduce an interaction we take a
symmetric operator (9,
theinteraction
operator,
on which weimpose only,
for the moment, the formal commutationproperties
The interaction
representation
is defined as followswhere we have used the notation
{A, B}
= A B + BA. The commutation rules of the Poincarealgebra formally
hold if 0 satisfies thefollowing
conditions Bbl.71,n° 2-1999.
for
all j ~ k
E{1, 2, 3}.
Thus we have to find non-trivial solutionsC~ ~ 0
to this
system.
Let us write 0 as a kernel
operator
which commutes with Pwhere
h(P, Q, Q’)
is anarbitrary
kernel(for
themoment)
which satisfiesand the
symmetry
conditionwhere the star ~ means
complex conjugation,
all these conditionsbeing
necessary for 0 to be a
symmetric operator.
The last condition of(7) imposes (formally)
The substitution of
( 10)
in(9)
leads to sixnon-linear, integro-
differential
equations
for h . To solve thissystem
we restrict ourselves to solutionssatisfying
thefollowing
conditionwhich leads
to J P h
= = 0 becauseof (11)
and( 12).
Thus( 13)
isequivalent
to therequirement
thath ( P , 6, Q’)
is function of the normsII only.
With thiscondition,
the sixequations (9)
coincide.Introducing
the differentialoperator
Dthe conditions
(9)
and( 13)
lead to thesingle equation
l’Institut Henri Poincaré - Physique theorique
This is the fundamental
equation
whichguarantees
the relativisticstructure of the
theory.
Let us sum up what we have found.PROPOSITION 1. -
Leth(P, Q, Q’) be a function of ~P~,
only
whichsatisfies ( 11 )
and( 15).
Then the operators(8),
with 0given by ( 10),
aresymmetric
andsatisfy formally
the commutation rulesof the
algebra ~.
The total Hamiltonian and Lorentzgenerators
Hand L arerepresented
in termso, f ’
hby
thefollowing integral operators:
3. EXISTENCE OF SOLUTIONS OF THE FUNDAMENTAL
EQUATION
We
give
thecomplete
set of solutions of(15) lying
in a ball of a Banachspace. Then we introduce a subset of
solutions,
whichsatisfy
also( 11 )
and
( 13),
and we establish their usefulproperties.
DEFINITION 1. - Let lC be a compact set
of R3
withLebesgue- measure |03BA| ~
0. We denoteby
03B2 the Banach spaceof
continuous and boundedfunctions h (P, Q, Q’)
with support in(P, Q, Q’)
ER3
x J’C x 1Cfor
whichDh(P, Q, Q’)
exists and is also bounded and continuous,given
the norm
.
’
where the
differential operator
D isgiven by ( 14).
Vol. 71, nO 2-1999.
The
following
result assures the existence of alarge
class of solutionsof
( 15).
PROPOSITION 2. - There exists
I~1
E(0, (0)
suchthat, for
all c Ex
J’C) satisfying
there exists one andonly
E ~8satisfying:
(1)
(2) e. Q’) for all
(3) h (P, Q, Q’) satisfies (15) for all P, Q, Q’ E
The
proposition gives
thecomplete
set of solutions h of( 15) lying
in acertain ball of
~3; they
areuniquely
definedby
their restriction to P =0,
which can be chosenarbitrarily
in a certain ball of xThus, apart
from thisanalytic condition,
the restriction of h for P = 0(centre-
of-mass
frame)
isarbitrary.
The
proof
is an easyadaptation
ofProposition
3 of[4]
to the 4-d caseand to the bilinear
operator
b defined on functions E ~6by
for all
(P, Q, 60
EObviously
b : ,t~ ~ ,t3 and satisfieswhere
and thus we can take
Kl
=m3/llCl.
Let us introduce the
following
set of functions.DEFINITION 2. - Let R > 0 and let 1C be the ball
of R3 of
cehtre 0and radius R. Let V be the set
offunctions c(Q, Q’)
EC30(03BA
x whichAnnales de l’Institut Henri Poincare - Physique theorique
satisfy c(Q, Q’)*
=c(Q’, Q),
whichdepend only
on the normsII
andII
and such thatNote that 1>
depends
on the twopositive parameters m
and R .V is made of kernels
c(Q, Q’)
withcompact support,
boundedby
aconstant
depending
on thesupport,
anddepending on ~6!! and ~Q’~ only.
These
requirements
take us away fromphysical applications.
Each c E V satisfies the
hypothesis
ofProposition
2 andwhere
L2 (l~6)
refers to theordinary Lebesgue
measure(not
the 0’2measure).
Thefollowing properties
hold on V.PROPOSITION 3. - Let c E V. The
function
h deducedfrom
cby Proposition
2 has thefollowing properties:
( 1 )
hsatisfies ( 15),
(2) h(P, Q, Q’ depends only
onthe norms
(3) for
allQ, JR.3,
thefunction
P --+h(P, Q, Q’)
isafunction of
P2 analytic
in aC-neighbourhood
--> -->(4) for
allP2
in someC-neighbourhood of R+, thefunction Q, Q’
~h(P, Q, Q’)
has compact support andbelongs
toC3(JR.6),
(5)
thepartial
derivativesof h (P, Q, Q’), of
any order with respect toP2
andof
order~3
with respect toQ, Q’, belong
to,23, (6)
hand Dhsatisfy
the estimatesPm9/:-(l)-(5)
are easyadaptations
of thecorresponding proofs
in
[4].
For(6)
we introduce the normfor all
f
E From an easy estimateinvolving
theCauchy-Schwartz inequality
weget
Vol. 71, n° 2-1999.
for all
f
E ,t3. Now recall that h = where An are defined in[4].
Let us suppose that for some n E N we know that2/3
1/20 (this
is obvious for n =0).
Then we obtainIt follows that these bounds hold for all n . Let us take the limit n 2014~ oo .
Because the convergence of An and DAn is
uniform,
the sequences~An~* and ~DAn~*
converge too(taking
theintegral
in(21 )
as aRiemann
integral).
Thus the above estimates still hold in thelimit,
whichestablishes
(20).
04. UNITARITY REPRESENTATIONS OF THE
POINCARE
GROUP
Until now, the
representations (8)
of thealgebra ~
wereonly formal,
inthe sense that the domains of the
operators
and of the commutators were notspecified.
THEOREM 4. - Let c E 1/’. Let O be the interaction operator
( 10)
withthe
deduced from
c inProposition
2. Then{77, P, J, L}, given by (8),
are the generators of aunitary
continuousrepresentation
Proof. - According
to Theorem 5 of[7], H, P, J, L
are thegenerators
of aunitary
continuousrepresentation
of~+
if thefollowing
threeconditions are satisfied:
( 1 ) they
areself-adjoint, (2) they
admit a commoninvariant dense domain D on which the commutation rules of the
algebra hold, (3)
D is a domain of essentialself-adjointness
for theoperator
1st step :
Self-adjointness of H, P, J, L.
It is clear forP
andJ .
Tostudy
H andL
we need ageneral
estimate of the norm of vectors like,
Annales de l’Institut Henri Poincare - Physique theorique
for
all ~
E ~C and forkernels ~
such thatis well defined. From the
Cauchy-Schwarz inequality
and the Fubini theorem weget
By using
theexpression
of Hgiven
inProposition
1together
with(20)
we find the
following
bound on theoperator
norm of H -Ho :
Thus H -
Ho
is bounded and H isself-adjoint
on the domain ofHo.
Using similarly
theexpression
of Lgiven by Proposition
1together
with the estimate
(24)
leads tofor
all j
E{1,2,3}.
From the Kato-Rellich theorem(Theorem
X.12of
[8])
it follows that L isself-adjoint
on the domain ofLo provided
1. This condition is indeed satisfied because from
(20)
2nd step : Invariant domain and the commutation rules. Let D be the domain
D is dense
(because
it contains and isclearly
left invariantby Ho, P, J
andLo.
To show that it is also invariant under Hand L it is sufficient to show that it is invariant under 0.Let (~
E D and let usapply
anoperator
to the vector
O03C6 (recall
thatJkO
=0).
From the Leibniz rule we find Vol. 71, nO 2-1999.for some coefficients
Ca,~ . Because ~
E D theexpression
in[ ]
is avector of 7~.
By using
the estimate(24)
we find that(27) belongs
to ?-Lif the
expression
in{ }
has a well defined.
norm, which follows fromProposition
3 and somestraightforward
estimate.By working
on D the commutation rules for{ H, P, J, L}
can bededuced from those for
{No, P, J, Lo}
withouthaving
to take care oftheir domain. Thus we
only
have to do formalcalculations,
and thus toapply Proposition
1.3th step : D is a domain
of essential self-adjointness for the
operator A. Because{P, Ho, J, Lo}
are the infinitesimalgenerators
of aunitary
continuous
representation
of a Lie group it follows from Theorem 3 of[7]
that these
operators
andare
self-adjoint
and thatthey
admit a domainDo
as common invariantdomain and common core.
However,
thelargest
common invariantdomain is
(26),
thus D is also a common core.By
the Kato-Rellich theorem(Theorem
X.12 of[8]),
ð isessentially self-adjoint
on D iffor
all ø
ED,
for some 0~i
1 and 0k2
oo .Now ð,. -
Ac
=m-2 (HZ -
+L2 - Lo. Using (24)
and(20)
andsome
straightforward
estimates we can show thatH2 - Ho
is bounded.Let us
put Lh
:=L 2014 Lo. Using
the same estimates and(25)
we findfor
all ø
E DAnnales de l’Institut Henri Poincaré - Physique theorique
for some
k3 , k~
E(0, oo) . Finally by collecting
these estimates we obtainfor some
ks
E(0, oo)
andall ~
E D.Using
some technicsexplained
in[4]
we find also
and then the constant
1~1
of(28)
can be taken asIt follows from
(20)
that~i 1 / 2
1. D5. BOUND STATES AND RELATIVISTIC
SCHRÖDINGER EQUATION
.
In a
quantum theory,
thestudy
of thephysics
of a model consistsessentially
in twoproblems, namely
the search for the bound states and the construction of thescattering operator.
In a relativistictheory,
theB~bL71,n°2-1999.
bound states are related to the discrete
part
of thespectrum
of the massoperator
M. Moreprecisely
the mass m R of a bound state is a solution tothe
eigenvalue problem M(~ = with ~
ED(M)
0. In ourmodels this
equation
takes the formwith ~
ED(M~), ~ 7~ 0,
and where S is the interaction kernel ofH2 given by
The
function ~,
when itexists,
is continuous on P(see below).
Thus onecan take P = 0
(centre-of-mass frame)
and thisequation
reduces towhere
~(6) = ~(0, 6).
Now for P =0, M2
isjust H2.
Thus thepositive
square root of the
operator
involved in(30)
iseasily
taken and leads toThe
operator M,
thepositive
square root of theoperator M2 appearing
in
(29),
satisfies thefollowing properties.
THEOREM 5. - For all c E 1> the operator M is
essentially self-adjoint
on the domain D
(26). Moreover;
its spectrum is contained in(0, oo)
where
(0, 2m )
contains at most afinite
numberof eigenvalues
m B, whichare solutions to the
eigenvalue Eq. (31 ).
Remark. -
Eq. (29) (or
its reduced forms(30), (31 ))
can be conside- red as a relativisticSchrodinger equation
because itplays
the role of theSchrodinger equation
inQuantum
Mechanics: itgenerates
the discrete structure of the bound states.Annales de l’Institut Henri Poincare - Physique theorique
Historical remark.
Looking
for a relativisticequation
for theHy- drogen
atom, Diracrejected
theequation:
which is the first natural
attempt
to a relativisticgeneralization
of theSchrodinger equation.
The reason was that it is not invariant under Lorentz transformations(see
the discussion in[9]). Now,
theanalogue
of this
equation
in our models is(31 ),
which cannotsatisfy
such aninvariance,
because it has been obtained in agiven
referential frame(moreover, Q
is not anordinary
momentum, because is Lorentzinvariant).
In fact the relativisticequation
is(29)
and its invariance is notobvious,
because it involves Lgiven by (8).
Proof of
Theorem 5. - Thespectrum
ofMo given by (6)
covers theinterval
[4m2, oo)
and isabsolutely
continuous. ThenMo
isessentially self-adjoint
on D. From(20)
and(24)
it follows thatM2 - M20
is bounded.Then
M2
isessentially self-adjoint
onD,
and so is M.Let
~(/), P)
be the simultaneousspectral
measure of HandP,
where p > 0 is the
spectral
variable associated with H . In thespectral representation
M is themultiplication by ( p2 - p2) 1/2.
Because M is aCasimir
operator,
the invariantsubspaces
are limited in the(p, P)
spaceby half-hyperboloids
p =( P 2
+K 2 ) 1 /2
with K > 0.Let us introduce the
family
of Hilbert spacesand P E
plays
the role ofparameters.
The Hilbert space 1-í is the directintegral
(see
Section 1.5 of[11]).
LetHo,p
andHP
be the restrictions ofHo
and Hto
?-~P .
For instanceHP
isgiven by
for suitable 03C6, where
H0,P03C6(Q)
=From
Proposition
3 theintegral
Vol. 71, n° 2-1999.
is well
defined,
even if wegive
a smallimaginary
value toP2.
Thus(see [4])
the essentialspectrum
of/7p
is the interval0), oo)
andit may exist a finite number of
eigenvalues
in(0, 0)),
which formcontinuous
hypersurfaces
in the(p, P)-space.
Thesehypersurfaces
haveto be
half-hyperboloids
p =( P 2
+m B ) 1 ~2
for m B E(0, 2m )
solutions tothe
eigenvalue equation
for P =0,
that is to(31 ).
06. SCATTERING STATES AND SCATTERING MATRIX A
vector 03C8
E H is said to be a "twoparticle scattering
state" if its timeevolution,
for verylarge
time(or
very smalltime),
is notdistinguishable
from the two freeparticle evolution,
thatis,
if there exist03C8out (or
in H suchthat 0/
=(or 03C8
= wherethe ’wave
operators’ U +,
U - aregiven by
Here
Ho
is the two freeparticle
Hamiltoniangiven
in(3).
When theoperators (34) exist, they
map any vector of 7 C on atwo-particle scattering
state.
PROPOSITION 6. - For all c E V the
operators U±
exist on all H.The
proof
can beeasily adapted
from thecorresponding proof
in[4].
Proposition
6 leads to the existence of twoparticle
states, defined asthe states contained in the range of the
operators U ~ .
Now twoparticle scattering
processes can be obtainedby computing
the matrix elements of thescattering operator S
:= However thequestion
of theexistence of other states
(apart
from the boundstates) naturally arises,
which is related to the
asymptotic completeness problem.
We willgive
a
partial
answer to thisquestion.
InQuantum Mechanics,
theasymptotic completeness problem
is stated once theseparation
of the centre-of-mass motion has been done. In the relativistic case, thisseparation
cannotbe
performed,
but we can restrict ourselves to aparticular frame, given by
the choice of a fixed P EII~3.
We consideragain
the Hilbert spacedecomposition (33)
and the restrictionsjHp, Ho, p, LP, JP
andacting
on suitable domains of still
given by
the sameformulas,
but withfixed P. Now for each P the "wave
operators"
can be constructed o on
~CP (their
existence ’ follows from the same ’proof
asProposition 6,
with fixed oP).
Thequestion
of theasymptotic
Annales de l’Institut Henri Poincare - Physique theorique
completeness
will be discussed inAccording
to[10],
it consistsof two statements:
( 1 )
the HamiltonianHP
has nosingular
continuousspectrum
and(2)
the ranges ofU±P
coincide with thesubspace
of?-CP
corresponding
to theabsolutely
continuouspart
of thespectrum
of7-/p.
Only
the second statement, called the"completeness
of the waveoperators",
will be considered here. We note that it is sufficient to insure theunitarity
of thescattering operator SP
:=THEOREM 7. - For all c
andfor
all P ER3, the
rangesof the U±P
coincide continuous
subs pace of HP in HP (i.e.,
thewave operators aYe
complete).
Then thescattering
operator S zsunitary.
Proof. -
Let P ER3
be fixed.Appendix
A and thepoint (4)
ofProposition
3imply
thatH p - H0,P
is trace class in Then theranges of
7-
coincide with theabsolutely
continuoussubspace
of(Kato-Rosenblum theorem,
Section6.2, [ 11 ] ).
0The full
asymptotic completeness (with
absence ofsingular
continuousspectrum)
needsprobably
more restrictions on c(see [6]
for the 2-dcase).
7. AN EXAMPLE AND THE NON-TRIVIALITY
To establish the
non-triviality
we consider anexample
for which c isthe kernel of a one-dimensional range
operator.
This has theadvantage
ofleading
toexplicit
results.Let ~
EC~([0, (0))
withsupport
in[0, R ] ,
with uniform norm boundedby
and bounded below
by
where " R and 0 m are " the
parameters appearing
£ in Definition 2.PROPOSITION 8. - Let c be
the function given by
for
all above and À E lL For 1thefunction
cis the , interaction kernel in the
centre-of-mass frame
,of a
, continuousVol. 71, . 2-1999.
unitary representation of the
Poincaré group. Thisrepresentation
admitsa mass operator M with
absolutely
continuous spectrum[2m, oo)
and atmost number
(0, 2m), unitary scattering
operator S. Moreover
(i)
(ii)
M has aneigenvalue
m B E(0, 2m )
= -1 andm/ R
> 2.Proof. -
The function(38) belongs
to V. Thus the firstpart
of theproposition
follows from Theorems4, 5, 7
andProposition
6. Moreover thecompleteness
of the waveoperators implies
that theabsolutely
continuous
spectrum
of H(of M)
is the same as forHo (for Mo).
Proof of (i).
Note that ~C carries two differentunitary
continuousrepresentations
of the Poincare group, the freerepresentation
gener-ated
by {Ho, P , J ,
and the interactionrepresentation generated by { H, P, J, L}.
BecauseHo
and P commutethey
admit a simultaneousspectral
measureP)
where E > 0 is thespectral
variable asso-ciated with
Ho.
In thespectral representation Mo
becomes themultipli-
cation
operator by ( E 2 - p 2 ) 1 /2 .
BecauseMo ~
2m thesupport
ofd ~o
is
For such
( E , P)
let us consider the space = : which appears in thespectral decomposition
of~CP
whichdiagonalizes Ho,
pwhere
s p (Ho,
thespectrum
ofHo,
p, that i s the interval[~2(P, 0) ; (0).
The
operator 5’p
restricted to P is denotedS E,
P and iscalled
the ‘scat-tering
matrix’ . The action ofLo
on the variables(E, P)
iseasily
com-puted.
For~6
E}R3, I 1, the
Lorentz boost ofspeed ~6 (from
which
Lo
are the infinitesimalgenerators)
acts as followswhere
~
is the Lorentz matrix ofspeed ~6.
It follows from(39)
that therelation between
scattering
matrix isAnnales de l’Institut Henri Poincaré - Physique - theorique
which shows that S is known once is
given.
Let us restrict ourselves to on which the interactionoperator
has one-dimensional range, that is
V003C6
=03BB(~,03C6)0~
where(. , .)o
isthe scalar
product
of andAccording to [11],
Theorem 3 of Section
6.7,
thescattering operator gives
for all v Ewhere
for all z E
C,
Imz > 0. In(41 ), (., .) E,o
is the scalarproduct
ofand is the restriction
of ~
to In factis a constant in so that
which is non-zero for all 2m E
~/7~ + 4~ (see
the definition of1])
and for all v in a
large
set ofOn
the otherhand,
for E as abovelet us
compute
the limit needed in(41 )
which has
obviously
a non-zeroimaginary part. Then SE,0 - I
is non-zero for all such E. Because the
representation
in ~-Cgenerated by
Lo}
iscontinuous,
if follows from(40)
that thescattering operator
S differs fromidentity.
From Theorem 5 with
(38)
and  = -1Eq. (31 )
can bewritten as follows
W.71,n° 2-1999.
where K is a constant. This function
belongs
toD(Mp-o)
C andis an
eigenfunction
ofprovided
theimplicit equation
admits a solution 0 m B 2m . To
study
this lastquestion
we considerthe
right
hand side of(43 )
as a function of the variable For m B = 0we
get
from(36)
.Now it follows from
(37)
that for m B = 2m theright
hand side of(43)
ismaj orized
as followswhich is > 1 for
m/ R
> 2. Thus(43)
has a(unique)
solution 0 m B2m,
which is aneigenvalue
of(31)
and then aneigenvalue
of M. 08. CONCLUSION
Let us sum up what we have found. We have constructed a
family
ofunitary,
continuousrepresentations
of the Poincare group in four space- timedimensions,
asperturbations
of the two free boson model. Thescattering operator
S can beperformed
and isunitary
and non-trivial insome cases..
The
physical
content of this mathematical construction is based onWigner’s
famousinterpretation [ 13], according
to which anelementary particle
is describedby
anirreducible, unitary,
and continuous repre- sentation of7~.
In the construction of S we have verified the existenceAnnales de l’Institut Henri Poincaré - Physique theorique
of
scattering
states,i.e.,
states which forlarge (or small)
timeapproach
the tensor
product
of two irreducibleunitary representations
of~,
in-terpreted
asdescribing
two freeparticles.
This allows us to assert thatour models
really
describe relativisticquantum systems
of twoparticles.
Moreover the
non-triviality
of S allows us to claim that the interaction between theparticles
can be effective.The absence of
particle
creation or annihilation makes these modelsinteresting
for low energyphysics,
inparticular
for the bound stateproblem.
The existence of a bound stateequation
similar to theordinary Schrodinger equation
ofQuantum
Mechanics(and
which can be calleda "relativistic
Schrodinger equation")
isprobably
thestrongest
result of the paper.However,
these results have been obtained for interactionoperators
(9 with ranges contained in thesubspace
of zeroangular
momentum(the
so-called "s-wave
subspace").
Toget
a better characterization of thislimitation,
let uscompute
thechange
of the second Casimiroperator,
the Pauli-Lubanskioperator, given by ( 1 ).
In therepresentation (8)
itbecomes
where
WJ
isgiven by (6)
andWo
nLo.
Now condition( 13) implies {0, Wo}
= 0 and thusOur interactions have no effect on the Pauli-Lubanski
operator.
ACKNOWLEDGEMENT
I would like to thank the Professors W.O.
Amrein,
P.Bader,
J.Bros,
J.
Frohlich,
G.Gallavotti,
J.-J.Loeffel,
R. Stora and S.V.Varadarajan
forfruitful discussions and useful
suggestions.
I amgrateful
to them for their interest in this work and for theirencouragements.
APPENDIX A. A CRITERIUM FOR TRACE-CLASS
OPERATORS
Let =
s)
be a Hilbert space Where s is apositive
cr-finitemeasure, and let F be an
integral operator
onHS
of kernelf : R3
xIR3
H
C,
that isVol. 71, n° 2-1999.
for all suitable " u E
LEMMA 9. -Let K be a
compact
subsetof R3
andf
E xS Q9
s)
.suchthat for
almost all x ER3 the
’function
y ~,f (x, y)
hassupport in
K. Let us suppose that the three derivativesexist in
L 2 (II~3
x}R3, S
@s ) .
ThenF, defined by (44), is
trace class.Proof. -
We follow[ 12,
SectionXI.9.32].
We use that aproduct
of twoHilbert-Schmidt
operators
is a trace classoperator.
Let k > 0 be such that K c[-k, k]3 .
Let u E From threeintegrations by parts
weget
We have written F as a
product
of two Hilbert-Schmidtoperators,
the first one of kerneland the second one of kernel
Thus F is trace class. 0
[1] P.A.M. DIRAC, Forms of relativistic dynamics, Rev. Mod. Phys. 21 (1949) 392-
399.
[2] D.G. CURRIE, Interaction contra classical relativistic Hamiltonian
particle
mechan- ics, J. Math. Phys. 4 (1963); See also E.C.G. SUDARSHAN and N. MUKUNDA, Classical Dynamics: A Modern Perspective, Wiley, New York, 1974.[3] E. FROCHAUX, Non-trivial representations of the special relativity group, Forum Math. 9 (1997) 75-102.
[4] E. FROCHAUX, Two relativistic boson models in the Schrödinger picture in three
space-time
dimensions, J. Math. Phys. 37 (1996) 2979-3000.Annales de l’Institut Henri Physique - theorique
[5] E. FROCHAUX, A relativistic quantum equation for N ~ 2 bosons in two space-time dimensions, Helv. Phys. Acta 68 (1995) 47-63.
[6] E. FROCHAUX and A. ROESSL, A relativistic
generalization
of Quantum Mechan-ics in two space-time dimensions, in preparation.
[7] E. NELSON, Analytic vectors, Ann. Math. 70 (1959) 572-615.
[8] M. REED and B. SIMON, Methods of Modern Mathematical Physics, Vol. II, Fourier Analysis and Self-Adjointness, Academic Press, New York, 1975.
[9] J. SUCHER, Relativistic invariance and the square-root Klein-Gordon equation,
J Math. Phys. 4 (1963) 17-23.
[10] M. REED and B. SIMON, Methods of Modern Mathematical Physics, Vol. III, Scattering Theory, Academic Press, Boston, 1979.
[11] D.R. YAFAEV, Mathematical Scattering Theory, General Theory, Translations of Mathematical Monographs, Amer. Math. Soc., Providence, RI, 1992.
[12] N. DUNFORD and J.T. SCHWARTZ, Linear Operators: Part II: Spectral Theory, Wiley Classical Library, Interscience, 1988.
[13] E.P. WIGNER, Unitary representations of the inhomogeneous Lorentz group, Ann.
Math. 40 (1939) 149-204.
Vol. 71, n° 2-1999.