A NNALES DE L ’I. H. P., SECTION A
E DWARD P. O SIPOV
The Yukawa quantum field theory : linear N
τbound, locally Fock property
Annales de l’I. H. P., section A, tome 30, n
o3 (1979), p. 159-192
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159
The Yukawa2 quantum field theory :
linear N03C4 bound, locally Fock property
Edward P. OSIPOV
Department of Theoretical Physics, Institute for Mathematics, 630090, Novosibirsk, 90, USSR
Henri Poincaré, Vol. XXX, 1~3, 1979
Section A : Physique ’ théorique.
ABSTRACT. - The Yukawa
quantum
fieldtheory
in two-dimensionalspace-time
is considered.Using
the Matthews-Salamintegral
represen- tation a linearNr
bound isproved.
As a consequence, this boundimplies
that the
Yukawa2 theory
in the infinite volume islocally
Fock.RESUME. - On considere la theorie
quantique
deschamps
de Yukawadans un
espace-temps
de dimension 2. Unemajoration
lineaire pourNt
est demontree en utilisant la
representation integrale
de Matthews et Salam.En
consequence,
cettemajoration implique
que la theorie deYukawa2
dans Ie volume infini est localement Fock.
CONTENTS
1. Introduction ... 160
2. Integral representation of Matthews-Salam... 162
3. Estimates for functions S1", GT... 163
4. Estimates for some integral operators ... 171
5. 03C4 - Integrability of some functions ... 172
6. Upper bound on detren (1 + K(A)) ... 175
7. Bounds on Schwinger functions, linear NT bound ... 188
References... 190
Annales de l’Institut Henri Poincaré - Section A - Vol. XXX, 0020-2339/1979/159/$ 4.00/
(Ç) Gauthier-Villars 8
160 E. P. OSIPOV
1. INTRODUCTION
In the
present
paper we prove thelocally
Fockproperty (the
definitionof the
locally
Fockproperty
see[1])
for the(renormalized) Yukawa2
interaction
( = Y2)
in the two-dimensionalspace-time
with the free orperiodic (in
thespatial direction) boundary
conditions. For the main results and references on theY2 theory,
see, for instance[2-6, 7~, 77, 13, 22, 23, 26, 24, 27].
The
locally
Fockproperty
for models has first beenproved by
Glimm and Jaffe
[1, 7].
For the
Y2 theory
thelocally
Fockproperty
has beenproved by
Schra-der
[3] (for
the freeboundary
conditions and under some restrictions onthe smoothness of the space
cut-off).
In the
present
paper weget
rid of these restrictions and alsogive
a new(semi-)
Euclideanproof
which is valid both for the free and for theperiodic boundary
conditions.Namely,
thefollowing
theorem is valid :THEOREM 1.1. - The
Y2 theory
withthe free or periodic boundary
tions is
locally
Fock.Theorem 1.1 is used in the
proof
of the Lorentz invariance of theY2 theory
with theperiodic boundary
conditions[24].
Since the
locally
Fockproperty is,
infact,
a consequence of the linearN~
bound,
see[1, 7, 2, 3],
so we shall notgive
theproof
of this theorem and fix our attention on theproof
of the linearN~
bound.Let an ultraviolet cut-off in the
spatial
direction begiven by
a function~(p2/a),
where11(.) E 9’(rR)
and1](0)
= 1.Let be the interval
[a - 1/2,
a +1/2].
Let: =
cardinality
ofg’.
We suppose that our space cut-offssatisfy
the
following
conditions :i)
Eii) uniformly in g ~ I
a
where
[xag] ~ ~k)
is the Fourier transform of xag.THEOREM 1.2. - Let
03C3)
be the(renormalized) cut-off Yukawa2
Hamiltonian with the
free
orperiodie boundary
conditions. Let z 1.for
some a >0, depending
on zonly,
uniformly
ir2 g, cr, 1 6 oo.l’Institut Henri Poincaré - Section A
161
THE YUKAWA2 QUANTUM FIELD THEORY
- We note that Theorerns 1.1 and 1.2 are also valid for
P(c~~2
+Y2
models. Theproofs
are in this case the same as for thecase of pure
Y2 theory.
To obtain a linear
NT
bound we use the(semi-)
Euclidean formalism ofMatthews-Salam,
Seiler[8-10, 5, 26, 28]
in which the fermions have beenintegrated
out. The idea of theproof
consists in thefollowing.
Werewrite
expressions
like(F,
exp( - t(H(g, cr)
- with thehelp
ofthe Matthews-Salam
integral representation
with the Gaussian measurecorresponding
to theperturbed two-point
functionand then we use the
technique
of Refs.[4, 6, 10, 77] to
obtain the boundson
detren ( 1
+K).
Here thecomplications
appear, which are connected with the fact that the Gaussian measure has no Markovproperty
in thespatial
direction.Nevertheless,
theperturbed two-point
function decreasesexponentially
onlarge (Euclidean)
distances. This decrease allows us,similarly
to Refs.[6, 72],
to obtain linear bounds.The
proof
of the Matthews-Salamformulas,
which weneed,
has been considered in Ref.[28].
The
exposition
is made in thefollowing
way. In Sec. 2 we formulate the Matthews-Salamintegral representation
for thetheory
with the Hamil- tonianH(g, 7) 2014
In Sec.3,4
we obtain the estimates which we need for the(perturbed)
functionsGr, St
and for theintegral operators
connected with them. In Sec. 5 we obtain some necessary estimates of the functionalintegral
over the(perturbed)
measure 03C4 and in Sec.6,7
we prove the linearNt bound,
i. e. Theorem 1.2.Since the
proofs
of the linearNT
bound for the free andperiodic boundary
conditions coincide
essentially,
so wegive
the detailed version for the freeboundary
conditions and make some remarks for thechanges
needed forthe case of the
periodic boundary
conditions.In the
following f ~ , f "
denote the direct and inverse Fourier transform of thefunction!
We definedetn
asBy p
we denote the set of compact operators with the normP: = 2014
i (the gradient operator),
... denotestrictly positive
constantspossibly depending
on unessential variables.XXX, nO 3 - 1979.
162 E. P. OSIPOV
2. INTEGRAL REPRESENTATION OF MATTHEWS-SALAM
We want to obtain the
integral representation
of the Matthews-Salamtype
for the Hamiltonianexpressions
of the formwhere F is either a fermion
field 03C8
or its Diracconjugate 03C8 : =
or a function of the boson field
0 x)
at time zerois the
(renormalized, cut-off)
Hamiltonian of theY2 theory perturbed by
the « number ))
operator
with ’r 1 and the constant a > 0 is chosen such thatWe want to consider the
(cut-off)
interactions of the formand
7(~) = ~(2014 x)
is a function from9’(IR). Let,
forsimplicity,
W beeither a bounded
analytic
real-valued function on IR or/J, W
1 Eand an ultraviolet be made with the
help
of a function from9’(IR).
Let 03C4
be the Gaussian mean zero measure on9"((R2)
with thetwo-point
function
We remark that the Gaussian measure Jlt is
hypercontractive
and hasthe Markov
property
in thetemporal
direction[l4],
but it has no Markovproperty
in thespatial
direction[15].
We also introduce the
(perturbed, Euclidean)
fermiontwo-point
functionThe
following
£ theorem is valid.Annales de Henri Poincare - Section A
163
THE YUKAWA2 QUANTUM FIELD THEORY
THEOREM 2.1. -
( Matthews-Salam formulas).
Let H’ begiven by (2 . 2)- (2.3).
Then the Hamiltonianobjects (2.1)
aregiven by
Matthews-Salamformulas
with the Gaussian measure /It and thefermion two-point function (2 . 5).
This theorem is
proved
in[28].
3. ESTIMATES ON FUNCTIONS
St, Gt
In this section we consider
properties
of the functionsSt
andGt
and ofsome
integral operator
connected withSf
andGt.
It follows from the definition
(2.5)
thatwhere
The
following
lemmas contain the mainproperties
of the functionsS~
and
G~.
LEMMA 3.1.
Proof of Lemma
3.1. 2014 In the sense of distributionsand, thus,
as it can beeasily
seenin the sense of distributions. Since the
integrals
in(3.2)
areconvergent,
eq.(3.2)
is valid in the sense of usual functions. To estimate the firstintegral
we write
Vol. XXX, nO 3 - 1979.
164 E. P. OSIPOV
and, thus,
thisintegral
is estimatedby
To estimate the second
integral
we divide the domain of theintegration
into two subdomains
where
A;’ = ~k; , 0).
The contribution of domain I is less thanHolder’s
inequality gives RB[-1,1] dk’1(.) ~
const.and so the
integral
over domain I is estimatedby
The
integral
over domain II is less thanBut
sup |k’1 |-1 ~ c(k2
+1) -1/2,
and theintegral
is less thanand so the
integral
over domain II is less thanTo prove the lemma we
join together
the obtained estimates. Lemma 3.1 isproved.
We need the estimates of the functions and its hermitian
adjoint
with some localization conditions in x - space.
Moreover,
since we wantto obtain the estimates uniform in
cut-offs,
we need the uniform estimates of the fermionpropagator
with cut-offs.Let
,,(.) E 9’(IR), ~(0) = 1
and an ultra-Annales de l’Institut Henri Poincaré - Section A
165
THE YUKAWA2 QUANTUM FIELD THEORY
violet cut-off in the
temporal
(11 andspatial
(12directions.
Let 1 -((~,
~(p) E ~(1~2),
where~(p)
= 1for I ~ ,
and~(p~
= 0 for~ ! ~ ~
-f-1,
be an infrared
(low momentum)
cut-off.The estimates we need are formulated in the
following
lemma:LEMMA 3.2. - Let
I(k)
be oneo.f the functions St(k), S+~t or
Then
a) «
ct exp( -
forh(x) E C~«(IRB{ O})
x~)~
d = dist
({O},
supph) ;
b) II (ki
+ cl exp(- c2d)
forji(x2)
E0
~),
d = dist({
0~,
supph),
0 ~ r1 ;
c) 11 h(x)1 ^(x) ~Lp ~
cl exp(- c2d)
forhtx)
EC~0(R2B{
0}),
d -dist
( {
0~,
supph),
2 s p 00.Lf’
thefunction Sr- (k)
isreplased by
the,func,~tion St- (k)r~~(k)(I - ~(k)),
then the estimates
a), b), c)
are valid with theexponential
decreasebeing replaced by
the decreasefaster
than any power and the estimates areuniform
in ultraviolet
eut-off
o~for
1 ~ 61, 2 ~ 00.Remark. The
replacement
of theexponential
decreaseby
the decrease faster than any power in the case with cut-offs is connected with the decrease faster than any power of the functionsProof of
Lemma 3.2. Let us first consider the caseb)
of the lemmafot
the function We shall obtain the
representation
for the function Srin the form of a contour
integral.
The statements will follow from thisrepresentation.
In the sense of distributions
Let us denote the
complex
variablek2 by ~.
We cut thecomplex plane ( by ( - foo,
-im]
and and choose the branches of theanalytic
functions
((2
+m2)n2, (~2
+T~22) ~12
such thatthey
would bepositive
onthe real semiaxis.
Let,
fordefiniteness,
supp h lie in thehalf-plane
x2 O.Let
C(5, 03C6)
be the contour chosen inFig. 1,
where 03B4and 03C6
aresufficiently
small
positive
numbers whichdepend only
on m and r and which will bechosen later
(for
x2 > 0 we should choose the contour in the lower half-plane 03B6).
We assert that for
sufficiently
small 03B4 and 03C6in and on the contour
C(5, ~p)
for some constant c > 0.Vol. XXX, no 3 - 1979.
166 E. P. OSIPOV
To prove this
inequality
it is sufficient to show thatin and on the contour
C(~, ~p),
whereWe write
Since
b(Re ()
>0,
soheRe 0 ~
~3 > 0. In the domain boundedby
thecontour
C(5, I
c2, where theconstant c2
isindependent
of5,
~p forsufficiently
small 5 and ~p.Thus,
in the domainand thus in this domain
inequality (3.6)
is fulfilled forsufficiently
small 03B4.Since
and since in the domain bounded
by
the contourC(5, ~p)
so in this domain
Thus,
in the domain boundedby
the contourC(5, ~)
forI
>5
But this is
greater
than apositive
" constant forsufficiently
small5,
cp.These ’
arguments
and 0 eqs.(3 . 2), (3.3) imply
that the functionST (k 1, 0
Annales de l’Institut Henri Poincare - Section A
167
THE YUKAW A2 QUANTUM FIELD THEORY
is
analytic
in and on the contour~p)
forsufficiently
small5,
~p. It is easy to see,making
estimates of the term0
forcomplex’
EC(5, ~p)
in the same way in the
proof
of Lemma 3.1 for realk2,
thatfor |03B61-+ 00, (
EC(b, cp),
may benonuniformly
inkl.
But then theintegral
of
()
over the arcs of the circleentering
the contourC(5, ~p)
tendsto zero when the radius of the circle increases. Let
C’(5, ~p)
be the contourshown in
Fig.
2(or,
in the case x2 >0,
theanalogous
contour in the lowerhalf-plane). Then, by Cauchy’s
theoremUsing
estimate(3 . 5)
it is easy to see that(the
term0
is estimated in the same way, as in theproof
of Lemma3.1)
where
c(1 , I)
is a functionincreasing
slower than apolynomial. Thus,
in the sense of distributions
and
which proves the
part b)
of the lemma for the functionSt’
In the same way we consider the functions
Si
and(k2
+m2)~’2S~ N Si .
Now,
we consider the casea~
of the lemma for the functionSt.
Fordefiniteness,
we suppose that supp h lies in thehalf-plane
xl 0.Then,
in the sense of distributions
where
We use the relation lim
(k
±i E) -1 -
P. V.k -1
:p which is valid in the sense ofdistributions,
see[16].
We want to write the
integral
overkl and k2
as theintegrals
over somecontours in the
complex planes ’1
1 and’2’
Vol. XXX, no 3 - 1979.
168 E. P. OSIPOV
First we consider the
integral
overA;i.
We cut thecomplex plane 03B61 by
Then the
integrand
is ananalytic
function in the upper half-plane
with the cut. Theintegrand
in(3.8)
decreases in’1
in the upperhalf-plane as I ’1 1-+
oo . This is evident for the functionsS;«(1, k ~ ), s~~ (~1, k2)
and for theintegral
overkl
it follows from the estimatesNow, choosing
the contour, as it is shown inFig. 3,
it is easy to see that theintegral
over the arcs of the circle tends to zeroand, by Cauchy’s theorem,
theintegral of k
over the real axis isequal
to theintegral
over the contourC’~k2).
As a resultIt is easy to see that the
right
side of(3.9)
isanalytic in 03B62
forsufficiently small I 1m ’2 I (in particular,
for theintegral
overk 1,
theanalyticity
inthis
domain
follows from the factthat small). Besides,
the inte-gral
of(3.9) over’ 2
over the intervalsfor
sufficiently
smallpositive 5 tends,
as it is easy to see, to zero when R -+ oo.So,
the contour of theintegration over ’2 may be
shifted up ordown, depending
on thesign
of x2. As aresult,
Annales de l’Institut Henri Poincare - Section A
THE YUKAWA2 QUANTUM FIELD THEORY 169
the
integral over (2
converges due to theproperties
of the contourC’«(2).
This
expression
defines a function smooth in x(this
can beeasily proved by interchanging
the order of the differentiation and theintegration), increasing exponentially
in Xl and x2,and, thus,
in x for 0.Thus,
norms of derivatives of this function
satisfy
the bound ci exp(- c2d)
and
by
theHausdorff-Young inequality
normssatisfy
the sameinequality.
Thus,
the casea)
of the lemma isproved
for the functionSt’
In the same way we consider the other functions.
Consider the case
c). By a)
andb)
We have used the Holder and
Hausdorff-Young inequalities.
The obtainedinequality
proves the casec)
of the lemma.In the case with cut-offs it is necessary to
estimate,
forexample,
the caseb~
with an ultraviolet
cut-off,
theexpression
of the formLet {
ei be apartition
ofunity
in the variable y2 obtainedby
thetranslations of a fixed
C~
function with thesupport
in[ - 3/4~3/4~]
sosupp ei ~
[(i
-3/4)d, (i
+ We insert thispartition
ofunity
betweenr~~
andSt’
After that the termis estimated
by
where .
. is some norm on the Schwartz space in variables ~2~2’Taking
the location of thesupports
into account, it is easy to see that the aboveexpression
is less thanuniformly
i n 6 for 03C3 > 1.Vol. XXX, n° 3 - 1979.
170 E. P. OSIPOV
The terms
are estimated
similarly
to theprevious
oneby
theTaking
the sum over i we obtain power estimate for the cut-off propa-gator.
The estimate for the case
b)
with a lower momentum cut-off is obtained with the use of atwo-dimensional partition
ofunity
and the bounda)
ofthe lemma.
In the same way we consider the case
a)
with cut-offs. Lemma 3.2 isproved.
LEMMA 3.3. -
The function G03C4(x) ~ Lp(d2x),
1~ p
oo .The following
estimates are valid
where
Proof of Lemma
3.3. Theproof
isanalogous
to theproof
of Lemma 3.2.The
integral
overkl
is takenexplicitly,
and theintegral
overk2
may be rewritten as theintegral
over the contour of the formC’(~, Fig.
2.Lemma 3.3 is
proved.
LEMMAS
3.1y-3.3y.
- The boundscorresponding to the
boundsof Lemmas
3.1-3.3 are also valid in the case
of
theperiodic boundary conditions,
theseestimates are
uniform in
the boxcut-off
V ~ 1(naturally, I x2| V/2).
~.7v-~.~y.
- Lemma3.1v
may beproved
in the sameway as Lemma 3.1.
The statements of Lemma
3.2y
and3.3y
follow from Lemmas 3.2 and3.3,
from theinequality
for anorm II and
from the relationswhere the series converges in the sense of distributions and where
f
is oneof the functions
Gt, St’ [(k~
+m2) 1 ~2 Si N Si ] "
or these functions with cut-offs andIv
is thecorresponding
function in theperiodic boundary
conditions case.
Let us
consider,
forinstance,
the caseb)
of Lemma 3.2. In this case~2)~([-V/2,V/2]B{0})and
Annales de Henri Poincare - Section A
171
THE YUKAWA2 QUANTUM FIELD THEORY
Then
In the same way we consider the other cases. Lemmas 3.1
v-3.3y
areproved.
4. ESTIMATES FOR SOME INTEGRAL OPERATORS
In this section we consider trace-norms of some
integral operators.
With the
help
of Lemma 3.2 we prove Theorem 4.1(an analogue
of Theo-rem 2.2 of Ref.
[4])
which allows us to estimate contributions of theseparate
squares.THEOREM 4. l. Let xa, a E
Z2,
be the characteristicfunction of
the square with center at oc and side 1. Fixq >_
1.Suppose
operatorsA,
B aregiven
with
Ax«(P2
+ E~R,
and(p2
+ E~9.. for
someE > 0 and where
q’-1
-E-q’~-1 _ q-l.
Then, for
all rx,/3
Eq,
whereI(P)
is an operatorof multipli-
cation on one
of
thefunctions Si , S; - , ( p2
-E-m2)
1/2S; - ST ,
andIf the function Sz (p)isreplacedby the function with cut-offs~a(p)(1- 03B6(p))S~03C4(p),
then the assertion
of
the theorem is valid with thereplacement of
the exponen- tial decreaseby
the power decrease witharbitrarily large degree,
and thisdegree of
the decrease isuniform
in the ultravioletcut-off 03C3 for
ffi 1,2 ~ 1.Proof of Theorem
4.1. Theproof
uses Lemmas3.1, 3.2
and is an ana-logue
of that of Theorem 2.2 Ref.[4].
Let |I G( - 03B2I
sv/2 (i.
e.touehing squares),
thenNow,
the assertion follows from Holder’sinequality
foroperators
and from the boundedness of theoperator
in the square brakets(Lemma 3.1).
Now, let
I a -B/2 (i.
e.non-touching squares),
then eitherI ¿ 2 or 1, ! ~ - ~2 ! I
>2. Let h be afunction with support in
( - B/2 - ~, ý2
+5) identically
onein (- B/2, B/2),
where 5 is chosen withÝ2
+ 5 2.Now, if /31 r
>_2,
thenVol. XXX, no 3 - 1979.
172 E. P. OSIPOV
and
The assertion follows from Holder’s
inequality
for trace-norms of opera- tors and from the boundedness of theoperator
in the square brackets(Lemma 3.2a).
and
Again
the assertion follows from Holder’sinequality
for operators, from the boundedness of theoperator
from Lemma 3.2 and from the
inequality I x 2014 ~ ~
1+
a2 -~2 ! I
for
I
~1.Theorem 4.1 is
proved.
5. Jit -INTEGRABILITY OF SOME FUNCTIONS
In this section we prove some
integrability
results for the Gaussianmeasure which is
given by
thetwo-point
functiony) (formula (2.4)),
and obtain some bounds.THEOREM 5.1. >- 2 and
v, )B,
> 0 with( v
+~,)q >
1.the Gaussian mean zero measure on
G’(R2)
which isgiven by
the covariancey) (2.4)).
LetA(03C6) = (p2
+ + linearmap from
somesubspace of G’(R2) to operators.
Here A E ond hasa Then A(03C6) is 03C4 almost
everywhere in q.
Proof of Theorem
J.7. Consider first the case q = 2k with k aninteger.
Acting
as in theproof
of Theorem 3.4 Ref.(see
also Ref.[77],
Theo-rem
9.1
andusing
Lemma 3.3 it is easy to see thatWhen q
is not an eveninteger,
we can,following
Seiler and Simon[4],
use the
interpolation
theorem. For theproof
of theinterpolation
theoremsee
Gohberg,
Krein[18,
p.137-139).
Theorem 5.1 isproved.
Annales de Henri Section A
173
THE YUKAWA2 QUANTUM FIELD THEORY
THEOREM 5.2. Let
~( . )
E bea function
with a boundedsupport.
77!~
belongs to 1
/It almosteverywhere
’ and ’X E
C~([R2)
andequal to
one on supp % Aand , C is trace class in the Hilbert space
Proof of
Theorem 5.2. - Let y be aCo (f~2)
function which satisfies 0 x 1 and o isidentically
one ’ on supp % A and o zero o onThen L =
so,
by
Lemma2.1, M,
M e~2. Then, by
Theorem5.1,
N e~2 ~
almostanc~
where C is trace class in
namely,
where
G T
and E are theoperators
ofmultiplication
in the momentumspace
by
thefunctions, respectively,
andwhere p t = p ±
k/2.
Using
the numberinequality
we obtain
Theorem 5.2 is
proved.
We also need some estimates for
integrals
of Wick monoms which aresimilar to the estimates of
Dimock,
Glimm[12,
Lemma2.4]
andGlimm,
Jaffe and
Spencer [17,
Theorem9.4].
In contrast to the bound of Lemma 2.4Vol. XXX, nO 3 - 1979.
174 E. P. OSIPOV
by
Dimock and Glimm[12]
we need an estimate in which the kernel isLp(d2x)
functionwith p
> 1and p -
1 is small(see
also Ref.[17]).
We want to consider functions on
g’(1R2)
of the formwhere the normal
ordering
is made withrespect
to the measure 03C4and,
forsimplicity,
all have the form =p(v, k)x), ~
E9’(1R2),
1,
or all are~
=k)~?(P(v~ ’1 E 9’(~),
1
(a
moregeneral
case ofdinerent
cut-offs in different direc- tions can also beconsidered).
We remark that for ultraviolet cut-oifs of the form the normalordering
withrespect
to the measure 03C4 and withrespect
to the free boson measure with the mass mb coincide.We suppose that the
support w
lies in a set of the formwhere
c~(v)
el~2
and whereA~. c: [R~
is the square with side 1 and centerat j ~ 1Z2.
Let~j
be the characteristic function of0394j
and let n* = sup ny.Let,
also~={1_..,N}, I,={(~1),...~
The set of all
possible graphs
on I is denotedr(I),
the set of all vacuumgraphs
is denotedro(I)
and let[1]
=~I03BD
be the set of alllegs [72].
where
Proof of Lemma
5.3. Theproof is
the same as that ofProposition
9.3[77] ]
or of Lemma 2.1
[12]
with thereplacement
of Schwarz’sinequality by
Holder’s
inequality.
5.3 isproved.
We define a
function 03C9(.)
on[I] k))
= andfor j ~ Z2
defineTHEOREM 5.4. - Let w E p > 1. have the
a,f’orementioned form
and infp(v, k)
= p >0, then, as above for 03B4
E[0, 1)
_ .
Annales de l’Institut Henri Poincare - Section A
THE YUKAWA QUANTUM FIELD THEORY 175
Proof of
Theorem 5.4. Theproof
of this theorem is the same as that of Lemma 2.4 of Ref.[12].
Someslight
modifications appear in theproof
of estimates for the kernel
G~(y, y’) only,
to which the kernely’) corresponds
in notations of Dimock and Glimm[12].
But these estimatescan
easily
be obtained.Since the function
Gt(x)
has anexponential
falloff forlarge
distances(Lemma 3.3)
and since for each n the uniform inp(v, k)
forinf
p(v, k)
= p > 0 estimate (v ,k )E[I]is valid. So
On the other
hand,
for//M~ S:
2 thefollowing
estimate is valid! G, ~ 11c;1- * Gz
*~,, (Hausdorff-Young inequality)
for r
(2//~)~.
These estimates and the
arguments
of Ref.[/2] imply
Theorem 5.4.Theorem 5.4 is
proved.
6. UPPER BOUND ON
detren (1
1 +K(A))) I
In this section we prove the main technical result of this paper.
The
operator S03C4039303C6
enters the Matthews-Salam formulas.Here, A(x)
is a
space-time
cut-off. The idea to consider thisoperator
in the Hilbert spaceL2((p2
+t’I’i2)1~2C~2p)
Q(;2 belongs
to Seiler[10].
In the Hilbertspace
([2
thisoperator
has the formThe
operator
with cut-offsK(A, (7)
isgiven by
theanalogous expression.
We define
infinite boson mass renormalizations and 2,03C4(,03C3)
= 1 2d03C4K(, 03C3)2
is thesecond order Euclidean renormalization.
Vol. XXX, no 3 - 1979.
176 E. P. OSIPOV
Let be a
space-time
cut-off. Let xa be thepartition
of(R2
on squares with centres in a El~2
and side 1. We defineand we shall
identify
A’ andLet I A I
: =cardinality
of ABaEA’
We suppose that
space-time
cut-offssatisfy
thefollowing
conditions :i) A(x)
Eii) uniformly in ~ I
We remark
that,
inparticular,
the indicator of arectangle
satisfies thecondition
i), ii)
and ifg(x2)
satisfies the conditionsi), ii)
of Sec.1,
thenxp,b(xl)g(x2),
where ~a,b 1S the indicator of[a, b],
satisfies the condi- tionsi), ii).
THEOREM 6.1. - Let
A(x) satisfy
the above conditionsi), ii). Then, for
any p there is a constant c so that
uniformly
in ultravioletcut-offs
The similar assertion is also valid in the
case of the periodic boundary
tions.
Proof of
Theorem 6.1. 2014 To prove the theorem we, as Seiler and Simon[77, 4] split
theoperator
K into twoparts
withlarge
and small momenta. Let~(p)
be apositive
Coofunction, equal
to 1 on the E1R2 I ~ },
and
equal
to 0 on theset {p
EI 2 ,
+ 1}.
The function03B6(p) gives
a low momentum cut-off. Thepositive constant’
will be determined later.Let where
Taking
in theinequality
of Theorem 4.1[4]
A =H,
B =0,
C = L we obtain the estimatewhere
b
= 1 +e$l4
=4,4
... , A = H + H* +A+
is its non-negative part
and A- - itsnegative part. Similarly
we defineA(03C3),
etc.Annales de l’Institut Henri Poincare - Section A
THE YUKAWA2 QUANTUM FIELD THEORY 177
It is easy to see that the
right
side ofinequality (6.1)
may be rewritten in the formwhere
To prove the theorem it is sufficient to show that for
each p
E[1, oo),
!’=1,2,3
.... ,.,uniformly
in Q.First,
we consider the factor v 1.By
Theorem 5.2Since 1/2
forsufficiently
small5, depending only on and p,
so for such ð 1 -2p03B4C
is apositive operator
inand
by
a direct calculation of the Gaussianintegrals (cf. [~D,
Lemma3.3], [13,
Lemma2.1])
we obtain the boundEstimating
the determinant we have used theinequality
Lemma 2.1
[4]
and eq.(5.1) imply
thatThe
operator
C ingiven by
eq.(5.2).
In correspon- dence with theunitary equivalence
in the Hilbert spaceL2(d2p)
theoperator
C has the formWe note that the
operator
E is theoperator
of convolution(see (5.3)) by
the function whereVol. XXX, nO 3 - 1979.
178 E. P. OSIPOV
To estimate
CC
1 norm of theoperator
C we writeand
So the linear bound for the
factor 03BD1
is obtained.Now we
proceed
to the Gaussian factor v2.To estimate this factor we cancel the
divergences
in theexplicit
form.For this purpose we rewrite this factor in the
following
formHere
where B is a
positive (for large ()
Hilbert-Schmidtoperator
in the Hilbert space(see below)
andB(6)-the corresponding operator
with ultraviolet cut-offs. Theoperator
B isequal
towhere
Greg
is theoperator
ofmultiplication
in the momentum spaceby
the function
Here,
~± == ~ ±k/2, S~(~) = (1 2014 ~(p))ST (p)
is theperturbed two-point
fermion function with a low momentum
cut-off, Sp
is theoperation
oftaking
the trace overspinor
indices and we have written the counterterm of the boson mass renormalization for theYukawa2
interaction withFurthermore,
i r
are the second order Euclidean renormalization with and without a low momentum cut-off.
It is easy to see that
uniformly
in u and 0 A.Annales de , l’Institut Henri Poincaré - Section A
179
THE YUKAWA2 QUANTUM FIELD THEORY
In
addition,
if B ~0,
thenThus,
to obtain a linear estimate for the Gaussian factors it is sufficientto prove that B > 0 for
sufficiently large’
and to prove a linear bound for the square of the Hilbert-Schmidt norm of B.Let us show that for
sufficiently large’
B is apositive
Hilbert-Schmidtoperator. Writing S-r
=So
+S4,
whereSo
is the usual Euclideantwo-point
fermion
function,
andusing
eqs.(3.1)
and the estimate of Lemma3.1,
we see that the function
is bounded
by
a constantuniformly
in~. Estimating
the second item in(6.3)
in the same way as in[11]
we obtain thatSo the
operator
B ispositive
forsufficiently large’.
Now we estimate the Hilbert-Schmidt norm of the
operator
B in thespace
replace
the spaceand write
Aa :
=where ~03B1
is the indicator of the squares with center in ex E~2
and side 1. Thenwhere
It is easy to see that
Let us consider
operators
First we show that E~2.
It is easy tosee that
Vol. XXX, nO 3 - 1979.
180 E. P. OSIPOV
Since
(6.3)
isbounded,
so the direct calculation(see
Seiler[3,
A12])
andthe
triangle inequality give
Then
where we use Schwarz’s and
Young’s inequalities
to obtain the last expres- sion. Now the conditionii)
for Aimplies
thatB03B103B2
E2.
Now
To prove a linear estimate it is sufficient to prove that
where 03B15 = 03B11. This estimate follows from the
equality
and from the estimate
B03B1103B12 ~ 2
and Ch.XL8,
exercise D.49c[21] imply
thatLet h be a function with
support in (- V2 - ð, ý2
+ð)
iden-tically
onein (- ~/2, B/2)
where b > 0 is chosen withy2
+ b 2.Now, if
Xi 2014a2 f > y2, ( ~c2
-~3 ! I
>yi (non-touching squares),
then it is easy to see that
(6.5)
is the limit of theanalogous expression
inwhich is
replaced by Greg(r, ~).
wherex)
is a function obtainedby performing
an ultraviolet cut-off in the fermionpropagators (i.
e. tobound the
integration
domain in(6 . 2)). Thus,
we haveAnnales de l’Institut Henri Poincare - Section A
181
THE YUKAWA2 QUANTUM FIELD THEORY
where
In the same way we can
replace
the functionby A"(~
whereA(x)
=h( ~ x ~ I -
a2 -a3 ’
Thus in the case ofnon-touching
squares
Using inequality (6.4)
we see thatIn the same way we consider the other cases of mutual locations of
o 0~.
uniformly in I A I.
The
estimation
of the Gaussian factors is finished.Now we
proceed
to the factor v3.Estimating
this factor we shall follow in the main theproof
ofProposition
II.1given by Magnen
and Seneor[6]
(remark
that we follow theproof
ofProposition
II.1 which wasgiven
inthe
preprint only).
Let
~3(cr)
be the factor u3 with an ultraviolet cut-off r.First,
we showthat
~3(cr)
defines Pt measurable function for (72014~00. Theorem5.1,
theexpansion ST
=So
+S4’
eqs.(3.1)
and the estimates of Lemma 3.1imply
that H E /? >
2,
Pt almosteverywhere. Thus,
to show thatv3{a)
definesfit measurable function for (y 2014~ 00 it is sufficient to show that
Vol. XXX, n° 3 - 1979.
182 E. P. OSIPOV
for o- 2014~ oo . For this it is sufficient to show that the
operator B1
is Hilbert-Schmidt in But
Bi
whereGreg
and
Freg
are theoperators
ofmultiplication by functions, respectively, (6.2)
andIn the Hilbert space
B1
= + Since eqs.(3.1),
the estimates of Lemma 3.1 and Seiler’s calculations
[I0, Appendix] imply
that
Greg
+Freg
is a boundedoperator
and Lemma 2.1[4] implies
thatG1/203C4
E so theoperator B1
is Hilbert-Schmidt.Moreover, it can
beshown,
as above for the kernelGreg,
that forI
oc- {3 I
>V2
theoperator
has the kernelwhich satisfies the estimate
c1 | 03B1(x)03B2(y) (1 + 03B1 - 03B2 B)-4.
Theproof
of this estimate is similar to that of Lemma 3.2.
In the
following
we shall not write down the ultraviolet cut-off cr,keeping
in mind that our bounds are uniform in 03C3 ~ oo .
We introduce an
increasing
sequence of cut-offs po, ... , pn, ... with 03C10 = 0 and pn = 1. Let the values of ultraviolet cut-offske belong
to this sequence. We also define cut-off fields
by
where =
and ~
is apositive
Coofunction,
= 1 forI 1/2,
0 1 for1/2 I 2, r~(k)
= 0 for 2 k.Then,
fora
set { k039403B1 }03B1~Z2
of localized cut-offs we defineWe write
We use the
inequality
Annales de Henri Poincaré - Section A
183
THE YUKAWAg QUANTUM FIELD THEORY
for
A~ >: 2014 1,
and Lemma 6.2 to obtain the boundApplying
Seiler’s arguments[10,
Lemma3.2
we obtain the boundLEMMA 6.2. -
(Seiler [10], Magnen,
Seneor[6] ) .
LetA,
B E4 be
twoself-adjoint
operators, thenSince the
proof
of Lemma 6.2given by Magnen
and Seneor[6,
LemmaIII.1] is
containedonly
in thepreprint,
wegive
here itsproof.
Proof of Lemma
6.2[6, preprint,
Lemma111.1].
2014 It is sufficient to prove theinequality
foroperators
of finiterank,
then theproof
followsby approxi-
mations. Let
~,i
and/17
be theeigenvalues
ofA+,
andB+
form a decreas-in
sequence, then withwe have
Vol. XXX, nO 3 - 1979.
184 E. P. OSIPOV
Since 1 +
v ~(t )
;:::1,
sol
Since
a~~ 4
and are subsets of the sets of theeigen-values
ofA4
andB4, thus, by applying
thegeneralization
of Lidskii’s theorem(Kato [19,
II Theo-rem 6.10 and
6.11]
and Seiler[10,
Lemma3.2])
we haveLemma 6.2 is
proved.
Eqs. (3.1),
Lemma 3.1 and Seiler’s calculations[10, Appendix A] imply
that
A
uniformly
in aspace-time
cut-off A.We transform the
expression (6.6)
in thefollowing
way.Any
differenceterm between
quantities
with and without ultraviolet cut-offs isdeveloped
as a sum of terms
containing
the difference H -Hk,
orH* -
or4>
-~k. Using linearity
in thefields,
wereplace
each field4> by ~
andA use the
triangle inequality
Now each
c~
localized in A with an ultraviolet cut-offka
= for someE will be
decomposed
in(this
is not done for thefields 4> - c~k)
with
= =
~2/P))
andwhere ~
is defined above.After this we also use
linearity
in the fields or thetriangle inequality
to rewrite ’ each localized
expression
as a sum overi 1, i2,
...Annales de # Henri Section A