Advances in Mathematical Physics Volume 2009, Article ID 978903,52pages doi:10.1155/2009/978903
Research Article
Spectral Theory for a Mathematical Model of the Weak Interaction—Part I: The Decay of the
Intermediate Vector Bosons W
±J.-M. Barbaroux
1, 2and J.-C. Guillot
31Centre de Physique Th´eorique, Centre National de la Recherche Scientique (CNRS), Luminy Case 907, 13288 Marseille Cedex 9, France
2D´epartement de Math´ematiques, Universit´e du Sud Toulon-Var, 83957 La Garde Cedex, France
3Centre de Math´ematiques Appliqu´ees, ´Ecole Polytechnique, UMR-CNRS 7641, 91128 Palaiseau Cedex, France
Correspondence should be addressed to J.-M. Barbaroux,barbarou@univ-tln.fr Received 28 April 2009; Accepted 13 August 2009
Recommended by Valentin Zagrebnov
We consider a Hamiltonian with cutoffs describing the weak decay of spin 1 massive bosons into the full family of leptons. The Hamiltonian is a self-adjoint operator in an appropriate Fock space with a unique ground state. We prove a Mourre estimate and a limiting absorption principle above the ground state energy and below the first threshold for a sufficiently small coupling constant. As a corollary, we prove the absence of eigenvalues and absolute continuity of the energy spectrum in the same spectral interval.
Copyrightq2009 J.-M. Barbaroux and J.-C. Guillot. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
1. Introduction
In this article, we consider a mathematical model of the weak interaction as patterned accord- ing to the Standard Model in Quantum Field Theorysee1,2. We choose the example of the weak decay of the intermediate vector bosonsW±into the full family of leptons.
The mathematical framework involves fermionic Fock spaces for the leptons and bosonic Fock spaces for the vector bosons. The interaction is described in terms of annihilation and creation operators together with kernels which are square integrable with respect to momenta. The total Hamiltonian, which is the sum of the free energy of the particles and antiparticles and of the interaction, is a self-adjoint operator in the Fock space for the leptons and the vector bosons and it has an unique ground state in the Fock space for a sufficiently small coupling constant.
The weak interaction is one of the four fundamental interactions known up to now.
But the weak interaction is the only one which does not generate bound states. As it is well
known, it is not the case for the strong, electromagnetic, and gravitational interactions. Thus we are expecting that the spectrum of the Hamiltonian associated with every model of weak decays is absolutely continuous above the energy of the ground state, and this article is a first step towards a proof of such a statement. Moreover a scattering theory has to be established for every such Hamiltonian.
In this paper we establish a Mourre estimate and a limiting absorption principle for any spectral interval above the energy of the ground state and below the mass of the electron for a small coupling constant.
Our study of the spectral analysis of the total Hamiltonian is based on the conjugate operator method with a self-adjoint conjugate operator. The methods used in this article are taken largely from3,4and are based on5,6. Some of the results of this article have been announced in7.
For other applications of the conjugate operator method see8–19.
For related results about models in Quantum Field Theory see20,21in the case of the Quantum Electrodynamics and22in the case of the weak interaction.
The paper is organized as follows. InSection 2, we give a precise definition of the model we consider. In Section 3, we state our main results and in the following sections, together with the appendix, detailed proofs of the results are given.
2. The Model
The weak decay of the intermediate bosonsWandW−involves the full family of leptons together with the bosons themselves, according to the Standard Model see 1, formula 4.139and2.
The full family of leptons involves the electrone−and the positrone, together with the associated neutrinoνeand antineutrinoνe, the muonsμ−andμtogether with the associated neutrinoνμand antineutrinoνμ,and the tau leptonsτ−andτ together with the associated neutrinoντ and antineutrinoντ.
It follows from the Standard Model that neutrinos and antineutrinos are massless particles. Neutrinos are left handed, that is, neutrinos have helicity−1/2 and antineutrinos are right handed, that is, antineutrinos have helicity1/2.
In what follows, the mathematical model for the weak decay of the vector bosons W andW−that we propose is based on the Standard Model, but we adopt a slightly more general point of view because we suppose that neutrinos and antineutrinos are both massless particles with helicity±1/2. We recover the physical situation as a particular case. We could also consider a model with massive neutrinos and antineutrinos built upon the Standard Model with neutrino mixing23.
Let us sketch how we define a mathematical model for the weak decay of the vector bosonsW±into the full family of leptons.
The energy of the free leptons and bosons is a self-adjoint operator in the correspond- ing Fock spacesee below, and the main problem is associated with the interaction between the bosons and the leptons. Let us consider only the interaction between the bosons and the electrons, the positrons, and the corresponding neutrinos and antineutrinos. Other cases are strictly similar. In the Schr ¨odinger representation the interaction is given bysee1, page 159, equation4.139and2, page 308, equation21.3.20
I
d3xΨexγα 1−γ5
ΨνexWαx
d3xΨνexγα 1−γ5
ΨexWαx∗, 2.1
whereγα,α 0,1,2,3 andγ5are the Dirac matrices andΨ·xandΨ·xare the Dirac fields fore−,e,νe,andνe.
We have Ψex
1 2π
3/2
s ±1/2
d3p
be,
p, su p, s
√p0 eip·xb∗e,−
p, sv p, s
√p0 e−ip·x , Ψex Ψex†γ0.
2.2
Herep0 |p|2m2e1/2whereme >0 is the mass of the electron, andup, sandvp, sare the normalized solutions to the Dirac equationsee1, Appendix.
The operatorsbe,p, sandb∗e,p, s resp.,be,−p, sandb∗e,−p, sare the annihilation and creation operators for the electronsresp., the positronssatisfying the anticommutation relationssee below.
Similarly we define Ψνex and Ψνex by substituting the operators cνe,±p, s and c∗νe,±p, s for be,±p, s and b∗e,±p, s with p0 |p|. The operators cνe,p, s and cν∗e,p, s resp.,cνe,−p, sandc∗νe,−p, sare the annihilation and creation operators for the neutrinos associated with the electronsresp., the antineutrinos.
For theWαfields we havesee24, Section 5.3
Wαx 1
2π
3/2
λ −1,0,1
d3k 2k0
αk, λak, λeik·x∗αk, λa∗−k, λe−ik·x
. 2.3
Herek0 |k|2m2W1/2wheremW >0 is the mass of the bosonsW±.Wis the antiparticule ofW−. The operatorsak, λanda∗k, λ resp.,a−k, λanda∗−k, λare the annihilation and creation operators for the bosonsW−resp.,Wsatisfying the canonical commutation relations. The vectorsαk, λare the polarizations of the massive spin 1 bosonsW±see24, Section 5.2.
The interaction2.1is a formal operator and, in order to get a well-defined operator in the Fock space, one way is to adapt what Glimm and Jaffe have done in the case of the Yukawa Hamiltoniansee25. For that sake, we have to introduce a spatial cutoffgxsuch thatg ∈L1R3, together with momentum cutoffsχpandρkfor the Dirac fields and the Wμfields, respectively.
Thus when one develops the interaction I with respect to products of creation and annihilation operators, one gets a finite sum of terms associated with kernels of the form
χ p1
χ p2
ρkg
p1p2−k
, 2.4
wheregis the Fourier transform ofg. These kernels are square integrable.
In what follows, we consider a model involving terms of the above form but with more general square integrable kernels.
We follow the convention described in 24, Section 4.1 that we quote: “The state- vector will be taken to be symmetric under interchange of any bosons with each other, or any bosons with any fermions, and antisymmetric with respect to interchange of any two fermions with each other, in all cases, whether the particles are of the same species or not.”
Thus, as it follows from24, Section 4.2, fermionic creation and annihilation operators of different species of leptons will always anticommute.
Concerning our notations, from now on, ∈ {1,2,3}denotes each species of leptons.
1 denotes the electrone−the positroneand the neutrinosνe,νe. 2 denotes the muons μ−,μ and the neutrinosνμandνμ, and 3 denotes the tau-leptons and the neutrinosντ andντ.
Letξ1 p1, s1be the quantum variables of a massive lepton, where p1 ∈ R3 and s1 ∈ {−1/2,1/2}is the spin polarization of particles and antiparticles. Letξ2 p2, s2be the quantum variables of a massless lepton wherep2∈R3ands2∈ {−1/2,1/2}is the helicity of particles and antiparticles, and, finally, letξ3 k, λbe the quantum variables of the spin 1 bosonsWandW−wherek ∈R3andλ ∈ {−1,0,1}is the polarization of the vector bosons see24, Section 5. We setΣ1 R3× {−1/2,1/2}for the leptons andΣ2 R3× {−1,0,1}for the bosons. ThusL2Σ1is the Hilbert space of each lepton andL2Σ2is the Hilbert space of each boson. The scalar product inL2Σj,j 1,2 is defined by
f, g
Σj
fξgξdξ, j 1,2. 2.5
Here
Σ1
dξ
s 1/2,−1/2
dp,
Σ2
dξ
λ 0,1,−1
dk,
p, k∈R3
. 2.6
The Hilbert space for the weak decay of the vector bosonsW andW− is the Fock space for leptons and bosons that we now describe.
LetSbe any separable Hilbert space. Letn
aSresp.,n
sSdenote the antisymmetric resp., symmetricnth tensor power ofS. The fermionicresp., bosonicFock space overS, denoted byFaS resp.,FsS, is the direct sum
FaS ∞
n 0
n a S
resp., FsS ∞
n 0
n
s S , 2.7
where0
aS 0
sS ≡C. The stateΩ 1,0,0, . . . ,0, . . .denotes the vacuum state inFaS and inFsS.
For every,F is the fermionic Fock space for the corresponding species of leptons including the massive particle and antiparticle together with the associated neutrino and antineutrino, that is,
F
4
Fa
L2Σ1
1,2,3. 2.8
We have
F
q≥0,q≥0,r≥0,r≥0
Fq,q,r,r 2.9
with
Fq,q,r,r q
a
L2Σ1 ⊗
⎛
⎝q
a
L2Σ1
⎞
⎠⊗ r
a
L2Σ1 ⊗ r
a
L2Σ1 . 2.10
Hereq resp.,q is the number of massive fermionic particleresp., antiparticlesandr
resp.,ris the number of neutrinosresp., antineutrinos. The vectorΩ is the associated vacuum state. The fermionic Fock space denoted byFLfor the leptons is then
FL
3 1
F, 2.11
andΩL 3
1Ωis the vacuum state.
The bosonic Fock space for the vector bosonsWandW−, denoted byFW, is then FW Fs
L2Σ2
⊗Fs
L2Σ2 Fs
L2Σ2⊕L2Σ2
. 2.12
We have
FW
t≥0,t≥0
Ft,tW , 2.13
whereFt,tW t
sL2Σ2⊗t
sL2Σ2. Heretresp.,tis the number of bosonsW−resp., W. The vectorΩWis the corresponding vacuum.
The Fock space for the weak decay of the vector bosonsWandW−, denoted byF, is thus
F FL⊗FW, 2.14
andΩ ΩL⊗ΩW is the vacuum state.
For every ∈ {1,2,3} let D denote the set of smooth vectorsψ ∈ F for which ψq,q,r,rhas a compact support andψq,q,r,r 0 for all but finitely manyq, q, r, r. Let
DL 3
1D. 2.15
Here
is the algebraic tensor product.
LetDWdenote the set of smooth vectorsφ∈FWfor whichφt,thas a compact support andφt,t 0 for all but finitely manyt, t.
Let
D DL⊗D W. 2.16
The setDis dense inF.
LetAbe a self-adjoint operator inFsuch thatD is a core forA. Its extension toFL
is, by definition, the closure inFLof the operatorA1⊗12⊗13with domainDLwhen 1, of the operator 11⊗A2⊗13 with domainDLwhen 2, and of the operator 11⊗12⊗A3with domainDLwhen 3. Here 1is the operator identity onF.
The extension ofA toFLis a self-adjoint operator for whichDLis a core and it can be extended toF. The extension ofA toFis, by definition, the closure inFof the operator A⊗1W with domainD, whereAis the extension ofA toFL. The extension ofAtoFis a self-adjoint operator for whichDis a core.
LetB be a self-adjoint operator inFW for which DW is a core. The extension of the self-adjoint operatorA⊗Bis, by definition, the closure inFof the operatorA1⊗12⊗13⊗B with domainDwhen 1, of the operator 11⊗A2⊗13⊗Bwith domainDwhen 2, and of the operator 11⊗12⊗A3⊗Bwith domainDwhen 3. The extension ofA⊗BtoFis a self-adjoint operator for whichDis a core.
We now define the creation and annihilation operators.
For each 1,2,3, b,ξ1 resp., b∗,ξ1 is the fermionic annihilation resp., fermionic creation operator for the corresponding species of massive particle when and for the corresponding species of massive antiparticle when −. The operatorsb,ξ1 andb,∗ ξ1are defined as usuallysee, e.g.,20,26; see also the detailed definitions in27.
Similarly, for each 1,2,3,c,ξ2 resp.,c∗,ξ2is the fermionic annihilationresp., fermionic creationoperator for the corresponding species of neutrino when and for the corresponding species of antineutrino when −. The operatorsc,ξ2andc∗,ξ2are defined in a standard way, but with the additional requirements that for any,,and, the operatorsb,ξ1andc,ξ2anticommutes, wherestands either for a∗or for no symbol see the detailed definitions in27.
The operatoraξ3 resp.,a∗ξ3is the bosonic annihilationresp., bosonic creation operator for the bosonW−when and for the bosonWwhen −see, e.g.,20,26, or27. Note thataξ3commutes withb, ξ1andc,ξ2.
The following canonical anticommutation and commutation relations hold:
b,ξ1, b∗,
ξ1
δδδ ξ1−ξ1
, c,ξ2, c∗,
ξ2
δδδ ξ2−ξ2
, aξ3, a∗
ξ3
δδ ξ3−ξ3
, b,ξ1, b,
ξ1
c,ξ2, c, ξ2
0, aξ3, a
ξ3 0, {b,ξ1, c,ξ2}
b,ξ1, c∗, ξ2 0, b,ξ1, aξ3
b,ξ1, a∗ξ3
c,ξ2, aξ3
c,ξ2, a∗ ξ3 0,
2.17
where we used the notationδξj−ξj δλλδk−k.
We recall that the following operators, withϕ∈L2Σ1, b,
ϕ
Σ1
b,ξϕξdξ, c,
ϕ
Σ1
c,ξϕξdξ,
b,∗
ϕ
Σ1
b∗,ξϕξdξ, c∗,
ϕ
Σ1
c∗,ξϕξdξ
2.18
are bounded operators inFsuch that b,
ϕ c,
ϕ ϕL2, 2.19
wherebresp.,cisbresp.,corb∗resp.,c∗.
The operators b, ϕand c,ϕsatisfy similar anticommutaion relations see, e.g., 28.
The free HamiltonianH0is given by H0 H01H02H03
3 1
±
w1 ξ1b∗,ξ1b,ξ1dξ13
1
±
w2 ξ2c,∗ ξ2c,ξ2dξ2
±
w3ξ3a∗ξ3aξ3dξ3,
2.20
where
w1 ξ1 p12m21/2
, with 0< m1 < m2< m3, w2 ξ2 p2,
w3ξ3
|k|2m2W1/2 ,
2.21
wheremW is the mass of the bosonsWandW−such thatmW > m3.
The spectrum ofH0is0,∞and 0 is a simple eigenvalue withΩas eigenvector. The set of thresholds ofH0, denoted byT, is given by
T
pm1qm2rm3smW;
p, q, r, s
∈N4, pqrs≥1
, 2.22
and each sett,∞,t∈T, is a branch of absolutely continuous spectrum forH0. The interaction, denoted byHI, is given by
HI
2 α 1
HIα, 2.23
where
HI1 3
1
/
G1,,ξ1, ξ2, ξ3b,∗ ξ1c,∗ ξ2aξ3dξ1dξ2dξ3
3
1
/
G1,,ξ1, ξ2, ξ3a∗ξ3c,ξ2b,ξ1dξ1dξ2dξ3,
HI2 3
1
/
G2,,ξ1, ξ2, ξ3b∗,ξ1c∗,ξ2a∗ξ3dξ1dξ2dξ3
3
1
/
G2,,ξ1, ξ2, ξ3aξ3c,ξ2b,ξ1dξ1dξ2dξ3.
2.24
The kernelsG2,,·,·,·,α 1,2, are supposed to be functions.
The total Hamiltonian is then
H H0gHI, g >0, 2.25
wheregis a coupling constant.
The operatorHI1describes the decay of the bosonsWandW−into leptons. Because ofHI2 the bare vacuum will not be an eigenvector of the total Hamiltonian for everyg >0 as we expect from the physics.
Every kernelG,,ξ1, ξ2, ξ3, computed in theoretical physics, contains aδ-distribution because of the conservation of the momentumsee1and24, Section 4.4. In what follows, we approximate the singular kernels by square integrable functions.
Thus, from now on, the kernelsGα,,are supposed to satisfy the following hypothesis.
Hypothesis 2.1. Forα 1,2, 1,2,3,, ±, we assume
Gα,,ξ1, ξ2, ξ3∈L2Σ1×Σ1×Σ2. 2.26 Remark 2.2. A similar model can be written down for the weak decay of pionsπ−andπsee 1, Section 6.2.
Remark 2.3. The total Hamiltonian is more general than the one involved in the theory of weak interactions because, in the Standard Model, neutrinos have helicity−1/2 and antineutrinos have helicity 1/2.
In the physical case, the Fock space, denoted byF, is isomorphic toFL⊗FW, with
FL 3
1
F,
F
2
a
L2Σ1 ⊗ 2
a
L2 R3 .
2.27
The free Hamiltonian, now denoted byH0, is then given by
H0 3
1
±
w1ξ1b∗,ξ1b,ξ1dξ13
1
±
R3
p2c∗, p2
c, p2
dp2
±
w3ξ3a∗ξ3aξ3dξ3,
2.28
and the interaction, now denoted by HI, is the one obtained from HI by supposing that Gαξ1,p2, s2, ξ3 0 ifs2 1/2. The total Hamiltonian, denoted by H, is then given byH H0 gHI. The results obtained in this paper forH hold true forHwith obvious modifications.
Under Hypothesis 2.1 a well-defined operator on D corresponds to the formal interactionHI as it follows.
The formal operator
G1,,ξ1, ξ2, ξ3b∗,ξ1c∗,ξ2aξ3dξ1dξ2dξ3 2.29
is defined as a quadratic form onD⊗DW×D⊗DWas c,ξ2b,ξ1ψ, G1,,aξ3φ
dξ1dξ2dξ3, 2.30
whereψ,φ∈D⊗DW.
By mimicking the proof of29, Theorem X.44, we get a closed operator, denoted by HI,,,1 , associated with the quadratic form such that it is the unique operator inF⊗FW such thatD⊗DW ⊂ DHI,,,1 is a core forHI,,,1 and
HI,,,1
G1,,ξ1, ξ2, ξ3b∗,ξ1c,∗ ξ2aξ3dξ1dξ2dξ3 2.31
as quadratic forms onD⊗DW×D⊗DW.
Similarly for the operatorHI,,,1 ∗, we have the equality as quadratic forms HI,,,1
∗
G1,,ξ1, ξ2, ξ3a∗ξ3c,ξ2b,ξ1dξ1dξ2dξ3. 2.32
Again, there exists two closed operatorsHI,,,2 andHI,,,2 ∗ such that D ⊗DW ⊂ DHI,,,2 ,D ⊗DW ⊂ DHI,,,2 ∗, andD ⊗DW is a core forHI,,,2 and HI,,,2 ∗and
such that
HI,,,2
G2,,ξ1, ξ2, ξ3b,∗ ξ1c,∗ ξ2a∗ξ3dξ1dξ2dξ3, HI,,,2
∗
G2,,ξ1, ξ2, ξ3aξ3c,ξ2b,ξ1dξ1dξ2dξ3
2.33
as quadratic forms onD⊗DW×D⊗DW.
We will still denote byHI,,,α andHI,,,α ∗α 1,2their extensions toF. The setD is then a core forHI,,,α andHI,,,α ∗.
Thus
H H0g
α 1,2
3 1
/
HI,,,α HI,,,2
∗
2.34
is a symmetric operator defined onD.
We now want to prove thatHis essentially self-adjoint onDby showing thatHI,,,α
andHI,,,α ∗are relativelyH0-bounded.
Once again, as above, for almost everyξ3 ∈ Σ2, there exists closed operators inFL, denoted byBα,,ξ3andBα,,ξ3∗such that
B,,1 ξ3 −
G1,,ξ1, ξ2, ξ3b,ξ1c,ξ2dξ1dξ2, B1,,ξ3∗
G1,,ξ1, ξ2, ξ3b∗,ξ1c∗,ξ2dξ1dξ2, B,,2 ξ3
G2,,ξ1, ξ2, ξ3b∗,ξ1c∗,ξ2dξ1dξ2, B2,,ξ3∗
−
G2,,ξ1, ξ2, ξ3b,ξ1c,ξ2dξ1dξ2
2.35
as quadratic forms onD×D.
We have that D ⊂ DBα,,ξ3 resp.,D ⊂ DB,,α ξ3∗ is a core for B,,α ξ3 resp., forBα,,ξ3∗. We still denote byBα,,ξ3andB,,α ξ3∗their extensions toFL.
It then follows that the operatorHI with domainDis symmetric and can be written in the following form:
HI
α 1,2
3 1
/
HI,,,α HI,,,α
∗
α 1,2
3 1
/
Bα,,ξ3⊗a∗ξ3dξ3
α 1,2
3 1
/
Bα,,ξ3∗
⊗aξ3dξ3.
2.36
LetNdenote the operator number of massive leptonsinF, that is,
N
b∗,ξ1b,ξ1dξ1. 2.37
The operatorN is a positive self-adjoint operator inF. We still denote byN its extension toFL. The setDLis a core forN.
We then have the following.
Proposition 2.4. For almost every ξ3 ∈ Σ2,DBα,,ξ3,DBα,,ξ3∗ ⊃ DN1/2 , and for Φ∈ DN1/2 ⊂FLone has
B,,α ξ3Φ
FL≤Gα,,·,·, ξ3
L2Σ1×Σ1
N1/2 Φ
FL,
Bα,,ξ3∗ Φ
FL≤Gα,,·,·, ξ3L2
Σ1×Σ1
N1/2 Φ
FL.
2.38
Proof. The estimates2.38are examples ofNτestimatessee25. The proof is quite similar to the proof of20, Proposition 3.7. Details can be found in27but are omitted here.
Let
H0,3
w3ξ3a∗ξ3aξ3dξ3. 2.39
ThenH0,3is a self-adjoint operator inFW, andDW is a core forH0,3. We get the following.
Proposition 2.5. One has Bα,,ξ3∗
⊗aξ3dξ3Ψ 2
≤
⎛
⎜⎝
Σ1×Σ1×Σ2
Gα,,ξ1, ξ2, ξ32
w3ξ3 dξ1dξ2dξ3
⎞
⎟⎠
N11/2⊗
H0,31/2
Ψ 2,
2.40
Bα,,ξ3⊗a∗ξ3dξ3Ψ 2
≤
⎛
⎜⎝
Σ1×Σ1×Σ2
Gα,,ξ1, ξ2, ξ32
w3ξ3 dξ1dξ2dξ3
⎞
⎟⎠
N11/2⊗
H0,31/2 Ψ
2
Σ1×Σ1×Σ2
Gα,,ξ1, ξ2, ξ32dξ1dξ2dξ3 ηN11/2⊗1Ψ2 1 4ηΨ2
2.41
for everyΨ∈ DH0and everyη >0.
Proof. Suppose thatΨ∈ DN1/2⊗DH0,31/2. Let Ψξ3 w3ξ31/2
N11/2⊗aξ3
Φ. 2.42
We have
Bα,,ξ3∗
⊗aξ3dξ3Ψ
Σ2
1
w3ξ31/2
B,,α ξ3∗
N1−1/2⊗1
Ψξ3dξ3. 2.43 Therefore, forΨ∈ DN1/2 ⊗DH0,31/2,2.40follows fromProposition 2.4.
We now have
B,,α ξ3⊗a∗ξ3Ψdξ3
2 F
B,,α ξ3⊗a ξ3
Ψ, Bα,,
ξ3
⊗aξ3Ψ
dξ3dξ3
B,,α ξ3⊗1
Ψ2dξ3, 2.44
Σ2×Σ2
Bα,,ξ3⊗a ξ3
Ψ, B,,α
ξ3
⊗aξ3Ψ dξ3dξ3
Σ2×Σ2
1 w3ξ31/2w3
ξ31/2
×
Bα,,ξ3N1−1/2⊗1 Ψ
ξ3 ,
B,,α
ξ3
N1−1/2⊗1
Ψξ3 dξ3dξ3
≤
Σ2
1 w3ξ31/2
Bα,,ξ3N1−1/2
FLΨξ3dξ3 2
≤
⎛
⎝
Σ1×Σ1×Σ2
Gαξ1, ξ2, ξ32
w3ξ3 dξ1dξ2dξ3
⎞
⎠
N11/2⊗
H0,31/2 Ψ
2.
2.45 Furthermore
Σ2
B,,α ξ3⊗1 Ψ2dξ3
Σ2
Bα,,ξ3N1−1/2⊗1
N11/2⊗1 Ψ2dξ3
≤
Σ1×Σ1×Σ2
Gα,,ξ1, ξ2, ξ32dξ1dξ2dξ3 ηN1Ψ2 1 4ηΨ2
2.46
for everyη >0.
By2.40,2.45, and2.46, we finally get2.41for everyΨ ∈ DN1/2⊗DH0,3. It then follows that2.40and2.41are verified for everyΨ∈ DH0.
We now prove thatHis a self-adjoint operator inFforgsufficiently small.
Theorem 2.6. Letg1>0 be such that 3g12
mW
1
m21 1
α 1,2
3 1
/
Gα,,2L2
Σ1×Σ1×Σ2<1. 2.47
Then for everyg satisfyingg ≤g1,His a self-adjoint operator inFwith domainDH DH0, andDis a core forH.
Proof. LetΨbe inD. We have
HIΨ2≤12
α 1,2
3 1
/
"
Bα,,ξ3∗
⊗aξ3Ψdξ3
2
B,,α ξ3
⊗a∗ξ3Ψdξ3
2
# . 2.48
Note that
H0,3Ψ≤H03Ψ≤ H0Ψ, NΨ ≤ 1
mH0,Ψ ≤ 1
m1H0,Ψ ≤ 1
m1H0Ψ,
2.49
where H0,
w1 ξ1b,∗ ξ1b,ξ1dξ1
w2 ξ2c∗,ξ2c,ξ2dξ2. 2.50
We further note that N11/2⊗
H0,31/2
Ψ 2≤ 1
2 1
m21 1 H0Ψ2 β
2m21H0Ψ2 1
2 1 8β
Ψ2 2.51
forβ >0, and
ηN1⊗1Ψ2 1
4ηΨ2≤ η
m21H0Ψ2 ηβ
m21H0Ψ2η
1 1 4β
Ψ2 1 4ηΨ2.
2.52
Combining2.48with2.40,2.41,2.51, and2.52we get forη >0,β >0
HIΨ2 ≤6
α 1,2
3 1
/
Gα,,2
× 1
2mW
1
m21 1 H0Ψ2 β
2mWm21H0Ψ2 1 2mW
1 1
4β
Ψ2 12
α 1,2
3 1
/
Gα,,2 η m21
1β
H0Ψ2
η
1 1 4β
1
4η
Ψ2 , 2.53
by noting
Σ1×Σ1×Σ2
|G,,ξ1, ξ2, ξ3|2
w3ξ3 dξ1dξ2dξ3≤ 1
mWGα,,2. 2.54 By2.53the theorem follows from the Kato-Rellich theorem.
3. Main Results
In the sequel, we will make the following additional assumptions on the kernelsGα,,. Hypothesis 3.1. iForα 1,2, 1,2,3,, ±,
Σ1×Σ1×Σ2
Gα,,ξ1, ξ2, ξ32
p22 dξ1dξ2dξ3<∞. 3.1
iiThere existsC >0 such that forα 1,2, 1,2,3,, ±,
Σ1×{|p2|≤σ}×Σ2
Gα,,ξ1, ξ2, ξ32dξ1dξ2dξ3
1/2
≤Cσ2. 3.2
iiiForα 1,2, 1,2,3,, ±, andi, j 1,2,3
iii.a
Σ1×Σ1×Σ2
$p2· ∇p2
Gα,,%
ξ1, ξ2, ξ32dξ1dξ2dξ3 <∞, iii.b
Σ1×Σ1×Σ2
p2,i2 p2,j2
∂2Gα,,
∂p2,i∂p2,jξ1, ξ2, ξ3
2
dξ1dξ2dξ3<∞.
3.3