A NNALES DE L ’I. H. P., SECTION A
A. O STENDORF
Feynman rules for Wightman functions
Annales de l’I. H. P., section A, tome 40, n
o3 (1984), p. 273-290
<http://www.numdam.org/item?id=AIHPA_1984__40_3_273_0>
© Gauthier-Villars, 1984, tous droits réservés.
L’accès aux archives de la revue « Annales de l’I. H. P., section A » implique l’accord avec les conditions générales d’utilisation (http://www.numdam.
org/conditions). Toute utilisation commerciale ou impression systématique est constitutive d’une infraction pénale. Toute copie ou impression de ce fichier doit contenir la présente mention de copyright.
Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques
http://www.numdam.org/
273
Feynman rules
for Wightman functions
A. OSTENDORF
Fakultat fur Physik, Universitat Bielefeld 4800, Bielefeld, 1 RFA
Vol. 40, n° 3, 1984, Physique theorique
ABSTRACT. 2014 We consider the vacuum
expectation
values ofpartially
time ordered
products
of field operators. For these wegive graphical computation
rulesanalogous
to theFeynman
rules. As aspecial
casethis includes the
Wightman
functions. It is shown that these functionssatisfy
theWightman
conditions as formulated inWightman’s
reconstruc- tiontheorem,
exceptpositivity.
RESUME . - On considere les valeurs moyennes dans Ie vide de
produits partiellement
ordonnes en tempsd’operateurs
dechamp.
On donne pour celles-ci desregles
de calculgraphiques analogues
auxregles
deFeynman.
Les fonctions de
Wightman
sont incluses comme casparticulier.
On montreque ces fonctions satisfont les conditions de
Wightman
tellesqu’elles
sont formulees dans Ie theoreme de reconstruction de
Wightman,
al’excep-
tion de la
positivite.
1. INTRODUCTION
In
studying
theproperties
of localquantum
field theories theWightman
functions are
important tools,
because the basicassumptions («
axioms»)
of the
theory
areeasily
translated intoproperties
of them[7] ] [2 ].
Sinceexact non-trivial models are hard to come
by,
we arelargely dependent
on
approximation schemes,
one of the more useful of which still is per- turbationtheory.
It is therefore desirable to findexplicit
rules for theAnnales de l’Institut Henri Poincaré - Physique theorique - Vol. 40, 0246-0211
calculation of
perturbative Wightman
functions which arecomparable
in
simplicity
to theFeynman
rules for the time-ordered functions. In the present paper suchFeynman-like diagrammatic
rules forWightman
functions will be derived for the
example
of the(~-theory.
It is convenientto solve a somewhat more
general problem, namely
that offinding
dia-grammatic
rules for the « sector r-functions », definedby
T : time order operator
They
include the usual ~--functions and theWightman
functions asspecial
cases. Their existence in
perturbation theory
as distributions has beenproved
in[3 ],
withoutgiving
anexplicit representation
of the typepresented
here.
Let
and
W~
be the term of order o- in theperturbative expansion
of Wandsimilarly
for the sector ’[-functions. Our construction is based on the follow-ing
conditions :a) W~
satisfies the linearWightman
conditions[2] ]
b)
InI ...
the sector boundaries can bedropped
betweenadjacent
sectors, if their arguments are in the proper timeordering:
if
c)
For... , xn)
the usualFeynman
rules are valid.Alternatively
we couldreplace
conditionc) by
therequirement
thatthe
I ... satisfy appropriate equations
of motion.The
plan
of the paper is as follows. In sections 2 and 3 we derive unrenor-malized
diagrammatic
rulessatisfying
conditionsb)
andc).
In section 4we show that the ultraviolett
divergences
can be removedby
standardrenormalization
procedures.
In section 5 we demonstrate that theproposed
rules indeed
satisfy
the linearWightman
conditions.Positivity is,
of course, notexpected
to hold in finite-orderperturbation theory.
The rules
given
here can beeasily generalized
to other local field theories.However,
in theories with masslessparticles
we are then confronted withAnnales de l’Institut Henri Poincaré - Physique theorique
-
infrared
divergent subgraphs. Examples
inQED
show that these diver- gences willprobably
cancel between differentgraphs,
but we have nogeneral proof
of this assertion.2. RECURSIVE DEFINITION OF SECTOR 03C4-FUNCTIONS
To
simplify
the discussion and to facilitateunderstanding
let us firsthandle the unrenormalized case. The essential ideas will become evident in this part. Later on we shall treat renormalization with the BPHZ for- malism. We make the
following
ansatz for the sector 03C4-functions in per- turbationtheory :
We start
the
recursion with the freefield,
i. e.where
0 # - i0394F
for i’ = i,0 # - A+
for i’ i.In addition we set
T~(0) = ð(1o, i~(x)
= 0.(2.1) comprises
the wellknown recurrence relation for 1:-functions as aspecial
case, since 03C4-functions are sector r-functions without sector boundaries.In the
following
we shallgive
aproof
of the timeordering property
mentioned before underb) by
induction.Zeroth order :
We know that
fAF(~--);)=~-~)A+(~--y)+0(~-~)A+(~-~). (2.3)
This
implies
Therefore boundaries between time ordered sectors can be discarded in zeroth order.
6-th order
Let us call
Ik(u)
theintegrand
ofthe
right
hand side ofequation (2.1)
and theintegrand
ofWe have to handle the cases k =1 and A; > 1
separately.
The
integrands
and readaccording
to(2 .1 )
From the induction
assumption
follows thatunder the condition that >
xo~~2~.
We obtainSince
x°, x?-~ > xo,~2~
there exists ay°
withx°, ~-’~ > 3~°
>xo,~2>.
We
distinguish
two cases :. We assume " that the sector 03C4-functions are " invariant under
permutations
Annales de l’Institut Henri Poincare - Physique theorique
of the arguments within a sector. This will be shown later on. With the induction
assumption
we obtainSince
x°
>u°
we have We obtainWe see that for k = 1 the
integrands
are identical for thegiven
time order.With the same
technique
as described above it is easy to show that all contributionscancel,
soIk(u) -
= 0 forany k.
It follows that for thegiven
time order both sector T-functions differ at most in the uninte-grated
terms of the recursionequation (2.1).
For these weproceed
in thesame way as above until sector r-functions with no or one
argument
remain.These terms are
equal
to zero.Since
equation (2.1)
reduces forordinary
r-functions to the usual recur-sion
equation
we see that theperturbative
sector 03C4-functions have in fact the timeordering properties
one wouldexpect
for the VEVs ofpartially
time ordered
products
of field operators(condition b)).
3. RULES .
FOR EVALUATING SECTOR 03C4-FUNCTION GRAPHS In this section we
give
anexplicit
solution of(2 .1 )
in terms ofFeynman
like
graphs.
First we need some definitions.
A
graph corresponding
to... , xn)
in~p4 theory
consists of n externalpoints
and 6 four line vertices. NA
graph corresponding
to.. J XJ
also consists of n= ~ ~
external
points
and 6 four line vertices. Furthermore everygraph
getsan additional structure which we call sector
partition.
We will define sectorpartitions
in thefollowing.
To every external
point
and to every vertex we relate a real number called sector number. The sector numbers for internal vertices are for the presentarbitrary. Every
externalpoint
gets the number of its sector, i. e. EXi
gets sector number i. Forgraphs
we extend the definition ofa sector as the set of all external
points
and vertices which have the samesector number. The sectors must have the
following properties :
External sectors are sectors which contain external
points.
Each of its vertices is connected to at least one externalpoint
within this sector.Internal sectors are sectors which contain no external
point. They
areconnected.
We call two sectors
adjoining
if there exists a vertex in one sector which is connected to a vertex in the other sectorby
a line.Every partition
of thegraph
into sectors is called sectorpartition.
We call a sectorpartition
proper if every internal sector has a number between the
highest
and thelowest sector number of the
adjoining
sectors. This intermediate value ruleimplies
that all sectors have a number between 1 and N.Sector
partitions
define anordering
of the vertices because we can order the vertices after the numerical value of their sector numbers. Two sectorpartitions
are calledequivalent
when theordering
of allpairs
ofadjoining
vertices are the same.
An
example
of different sectorpartitions
of agiven graph
is shown infig.
1. With these definitions we can formulate the rules forcomputing
sector 03C4-functions with
graphs ;
we compute ... as follows : 1. Draw all distinctdiagrams
with n externalpoints x 11 ~, ...,~~
andvertices
t=l
To every
diagram
draw all versions withnon-equivalent
proper sectorpartitions.
2. Now set for each vertex a
factor - i,
for each lineconnecting
thevertices yi
and yj
with sectornumbers ai and aj
a factorai = aj, a factor
0 +( yi - Yj) if ai aj,
and a factor if ai > a~.3.
Every diagram
G has to be dividedby
a combinatorial factory(G)
=g2~(3 !)~ - °2y,
where a is the number of double lines(pairs
of vertices connectedby
twolines), ~3
the number oftriple
lines(pairs
of vertices connectedby
threelines),
y the number of linesconnecting
a vertex withitself
and g
the number ofautomorphism
of thediagram (permutation
ofAnnales de l’Institut Henri Poincaré - Physique theorique
FiG.l 1
vertices which leave the
diagram unchanged) [4 ].
In addition every dia- gramgets
a factor( - 1)~, where 11
is the number of internal sectors.4. Sum up for each
diagram
all sectorpartitions, integrate
over all i~and sum up all
diagrams.
Let us consider an
example
of a second ordergraph ~2.~3 ! I x4),
a contribution to
~2~3! ~0)’
We have to sum over all
possible
sector numbers for Miand u2
whichlead to different proper sector
partitions.
The sectorpartitions
infig.
2are all proper sector
partitions
for x2,x3 ~ ~4)-
c reads for
example
FIG. 2
where
FiG.3
Annales de Henri Poincaré - Physique theorique
Proof of the
rules :We can write the recursion
equation
in thegraphical
form shown infig.
3.We will prove the rules
by
induction. In zeroth order the rules lead to the correctexpressions
because for everygraph
existsonly
one sectorpartition
since there are no innervertices,
and these sectorpartitions obviously
lead to the correct propagators.Now suppose the rules are true in all orders up 1. Let us first consider the
integral
term of theright
hand side of eq.(2.1). Obviously equivalent
sectorpartitions
lead to the sameanalytic expressions
fora
graph
because it isonly
the order of the sector numbers ofadjoining
vertices which determines the kind of propagator between them. In the
graphical
form we have chosenS(A) == 1, 1. 5,
...,N20140.5,
N. Thisspecial
selection can lead to
improper
sectorpartitions
and to arepetition
ofthe same
graph
for different sector numbersS(A).
Forexample
the sectorpartitions
shown infig.
4 are of the form shown infig.
5.FIG. 4
Fio.5
The
graphs
withS(A)
=1.5, 2,
2.5 haveequivalent
sectorpartitions,
the
graphs
withS(A)
=2,
4 haveimproper
sectorpartitions.
We will prove that
graphs
withimproper
sectorpartitions
cancel andthat
equivalent
sectorpartitions
sum up toyield
onegraph
with propersign.
For this purpose we have to answer the
following question :
How oftendo we get
equivalent
sectorpartitions
for agiven graph,
whenS(A)
runsthrough
the valuesS(A)
=1, 1. 5, ... , N ?
LEMMA. - Let G be a
graph
with sectorpartitions SG,
y an internalsector of G with sector number
S(y).
There exists an intervallly)
C IRsuch that we can find a sector
partition equivalent
toSG
withS’(y)
insteadof
S(y)
iffS’(y)
E(ky, ly),
whereky and ly
are sector numbers of externalpoints.
Proof
2014 The internal sectors 03B3iof SG
are restrictedby
a number ofinequa-
lities like k
l,
where due to the intermediate value rule k and are sector numbers of externalpoints.
For agiven
sec-tor y there exists a
highest k
such that kS(y)
and a lowest l such thatS(y)
1. We call thesebounds ki and li
for a sector 03B3i, sothat ki S(yi) li.
Only
ifS’(y)
is within these bounds we can find anequivalent
sector par- tition withS’(y)
instead ofS(y).
It remains to be shown that for everyS’(y)
E(ky, ly)
there exists a sectorpartition equivalent
toSo. Suppose
that
S’(y) S(y).
Then the sectorpartition
withS’(yi)
=is
equivalent
toSG
if ~, E(0,1 ],
and ~, can beadjusted
such thatS’(y) _ (1 - ~.)k
+~S(y). If S’(y)
>S(y)
chooseS’(yi) _ (1- ~,)l~ + ~,S(yi).
With this lemma we can
complete
theproof
of theFeynman
rules forthe sector ~-functions.
For a
given
sectorpartition
A is part of a sectory(A)
with sector numberS(A) (see fig. 6).
If
y(A)
is external the sectorpartitions
for other values ofS(A)
will bedifferent. We see from the induction
assumption
that theresulting
sectorpartition
has theright properties.
If
y(A)
is internal andS(A)
satisfies the intermediate value rule we know from the lemma thatfor ky S(A) ly
we obtainequivalent
sector par-titions, where ky and ly
are the sector numbers of externalpoints
whichare all
integer.
SinceS(A)
runsthrough integer
andhalfinteger
valuesthis
implies
that there are an odd number ofgraphs
withequivalent
sectorpartitions.
Due to thealternating sign
the sum of them results in onegraph
withnegative sign.
Ify(A)
consists of Aalone, y(A)
is a new internall’Institut Henri Poincare - Physique theorique
sector, and the
negative sign
isappropriate.
The sector numbers inside of can be chosen such thatthey
areunequal
toS(A),
so that all internal sectors are connected. Ify(A)
consists of more vertices than Athis implies
that
y(A)
is an external sector with respect to It follows thaty(A)
is a new internal sector of La and the
negative sign
isagain appropriate.
In addition it is
connected, following
from the connectednessproperties
of external sectors.
If
y(A)
is internal and does notsatisfy
the intermediate value rule weobtain
equivalent
sectorpartitions
for kS(y) ~
N. The lemmaapplies
for the part of the
graph belonging
to Therefore k isinteger,
sothat the number of
equivalent
sectorpartitions
is even. Due to thealternating sign
their sum vanishes.For the
unintegrated
terms in(2.1)
we repeat thisprocedure
until Ta with no or one argument remain. These areequal
to zero.We see from our rules that the sequence of arguments
1 ...
within a sector has no influence on the
graphs contributing
to1 ...
Therefore the arguments can be
permuted
within a sector withoutchanging
the sector r-function.
4. RENORMALIZATION
OF SECTOR T-FUNCTION GRAPHS
Until now
everything
has been done without renormalization. To get well defined results a renormalization is necessary and the renormalization scheme we shall use is that of BPHZ[4] ] [5 ].
We are
mainly
interested in the subtraction of infinities and shall commenton the renormalization conditions and finite renormalization later on.
The BPHZ renormalization scheme is formulated
in p-space.
We thereforehave to transform the
Feynman
rules into this space. We use the unsymme- tric Fourier transformA connected
diagram
in p-space is evaluated in thefollowing
way : We have to set an overall factor + ... externalvariables ;
for every line a factor
0 # (p), depending
on the sectorpartition;
for every vertex a factor - i. In every vertex momentum is conserved and to everyindependent
closedloop
we associate anintegration
variableki
and and 4k
integration
measure(27T)
. We have to sum over all sector
partitions
analogous
to the rules in x-space.The renormalization of a proper
diagram
G(i.
e. a connecteddiagram
which remains connected when an
arbitrary
internal line iscut)
is donein the usual
theory
in thefollowing
way :The
integrand
of everysuperficial divergent diagram
is subtractedby
anumber of counterterms. We do not
give
ageneral
definition ofsuperficial divergence here,
weonly
need that in~4 theory
everysubdiagram
withfour external lines has
superficial divergence
ofdegree 0,
i. e. islogarithmi- cally divergent,
and everydiagram
with two external lines hassuperficial divergence
ofdegree 2,
i. e. isquadratically divergent ( [4 ],
forexample).
Here we use the definition of a
subdiagram
of agraph
G as a subset ofvertices of G and of all
lines joining
them in G. Asubdiagram
must haveat least 2 vertices.
We
replace
theintegrand Ia
of aFeynman graph by
U is the forest of renormalization parts,
G/y
is thegraph
weobtain,
whenwe
replace
y in Gby
apoint,
andTyIG
=IG/03B3T03B3I03B3
is defined as theintegrand
of the
Graph G,
whereTyly
is inserted inplace
ofIy.
The first step is to translate this renormalization scheme to sector T-func- tions. We shall see that we can
apply exactly
the sameprocedure
to them.This is based on the
following
twoproperties :
1. every
integral
over aloop
notcompletely
within one sector is finite2. every renormalization part y not
completely
within one sector satisfiesthe
equation TyIy
= 0.So
only
thosesubgraphs
of a sector functiongraph
need a renorma-lization which consist of
purely i0394F propagators. Seagull
terms, i. e. sub-diagrams
connected to thediagram only by
asingle
vertex, vanish in thecourse of
renormalization,
becausethey
do notdepend
on external momenta.Therefore,
we shall omit them in thefollowing.
Let us first prove
property
1. Consider the sector with lowest sector number within theloop,
so that all linescoming
out of the sectors corres-pond
to0 + propagators.
If we call k theintegration
variable in theloop
momentum conservation
implies
that there exist two lines with propa- gatorst~ + (k)
and0 + (p - k), respectively.
But theproduct
has its support in a finite
region
withrespect
to k. It follows that no UVdivergences
appear.To prove the second
property
wesimilarly
consider the sector withthe lowest sector number in the renormalization
part.
Let us first assume that theTaylor operator
hasdegree
zero which means that the external momenta of thesubgraph
y are set to zero. Thisimplies
that the sum ofall momenta of the
outgoing
lines of the sector isequal
to zero. Since alll’lnstitut Henri Poincaré - Physique theorique
these momenta
belong
to0+
propagatorsTyIy
= 0. This remains true~ if the external momenta vary in a small
neighbourhood
of zero. Hence every derivation in the external momenta ofIy
at theorigin
is zero andTyly=0
is satisfied.
At last we have to examine wether
G/y
leads to a finiteintegral
in all cases.Due to
point
2 above this isonly important
if y consists ofonly
one sector.If y has four external lines
G/y
has a new four line vertex with the sectornumber of A instead of the
sub graph
y and we see that this isagain
anordinary
sector 03C4-functiongraph.
Things
are different when y has two external lines. We obtain a new type of vertex with two lines forG/y.
This kind of vertex occurs also in thecourse of mass renormalization.
This two line vertex leads to an undefined
product
of propagators suchas or
0 + ( p)0 + ( p).
We canhope
that the summation of these undefinedproducts
leads to a well definedexpression.
Let us thereforeconsider a reduced
graph
with m -1 two line vertices between two four line vertices.We assume the sector number of the four line vertex on the left hand to be lower than that on the
right
hand and take into account all proper sectorpartitions
of the two linevertices, holding
the rest of the sectornumbers fixed. Due to the intermediate value rule we obtain
only 0 +
and
i0394F
propagators. There are mpositions
for one1! +
propagator,(;) for
two propagators and so on.
Using
thesign
rule we obtain : ,where we used = With the formula
we obtain
as well as can be
potentiated
asboundary
values of holo-morphic
functions. Themultiplication
with does not cause any diffi- culties.Apart
from this obviousdifficulty
withselfenergy
insertions we have not considered theproblem
of the local existence in p-space of our inte-grals,
i. e. thequestion corresponding
to the existence of the s 2014 > 0 limit inordinary Feynman graphs [6 ].
We feel that this is adifficult,
but nota serious
problem.
In any case the sum over allgraphs
of agiven
ordermust exist
by
the results of[3 ],
hence apossible
localdivergence
of indi-vidual
graphs
can beeasily
curedby
a suitableregularization.
Thus we have the result that R
= fl ( - T03B3)IG
is a well defined expres-U y
sion both for ’[-functions and for sector 03C4-functions.
Only
for the ’[-functionsubgraphs
counterterms are necessary. Zimmermannproved
thatthey
lead to finite
expressions
when theintegrations
areperformed. Integration
over
loops
with vertices in different sectors arealways
finite as we showedabove. So the whole
integration
can beperformed
and is finite.The time
ordering property
mentioned in part 1 underb)
is true alsofor the renormalized ’[-functions. This can be
easily
seen with the multi-plicative
renormalization scheme. Weregularize
all propagatorsby setting 0#(x ; ~) -~ 0#(x ; m) - 0# (x ; M)(Pauli-Villars).
Theargumentation given
in part 2 can beapplied then,
because thereparametrization
of thetheory by Z, U,
and 5~ does not influence the timeordering property.
In the BPHZ renormalization scheme renormalization conditions can
be
imposed
as usual with thehelp
of finite counter vertices.5. DEMONSTRATION OF WIGHTMAN PROPERTIES FOR THE PERTURBATIVE WIGHTMAN FUNCTIONS In this section we show that our
expression
for W satisfies the linearWightman properties.
a)
RelativisticT ransformation
LayvTranslation invariance : In the
equations only
differences between twoarguments
occur, differences between two exterior variables(x - y)
anddifferences between external variables and
integration
variablesor An addition of a constant vector vanishes or can be absorbed in a translation of the
integration
variables.Lorentz invariance :
Ap, 0 +
and A. are invariant to Lorentz transfor-mations. The
integration
measuredx0dx1dx2dx3
isinvariant, just
as theintegration region
which is the whole1R4.
de l’Institut Henri Poincaré - Physique theorique
b) Spectral
ConditionWe shall prove a
slightly
stronger statement,namely
Consider an
arbitrary graph I ...
of order 6together
with agiven
sectorpartition.
Let us cut every line for which one vertex has sector number less orequal k
and the other greater than k. Then thegraph
disinte-grates into two
pieces,
which are notnecessarily
connected. Due to the intermediate value rule onepiece
has sector numbers less than k and the otherbigger
than k. If we call the momenta of the lines between the twopieces
q 1, ... , qs, then to every linecorresponds
a propagator0 + ( qi).
S
This
implies
thatG"
vanishes ifany qi~ V+
andparticulary
ifV+ .
s k
i= 1
Due to momentum
conservation
which proves theSpectral
Condition.i= 1 i= 1
c) Hermiticity
ConditionAt first
sight
this seems to be easy to prove, but it turns out to bequite
involved. The reason
for
this is that has arelatively complicated algebraic
relation to(eq. 4 . 5).
We shall use the relationand
proceed again by
induction.In zeroth order the
hermiticity
property is obvious becauseIn
higher
orders we first consider the unrenormalized butregularized graphs. ...
denotes agraph together
with all sectorpartitions
and we define
D6 - I ... ... !
In the
following
we willexpand I ...
frombehind,
i. e. withrespect
to x 1. This caneasily
be done with thehelp
of thegraphical
rulesfor the sector ’[-functions. We obtain :
The second term of
D 6 yields, using
the inductionassumption
andFrom
equation (4.3)
we know that similarequation
holds for
G6
+G6, namely
This can
easily
be seenby distinguishing
the casesu°
>x° and u0 x0i.
Using equation (5 . 5)
several terms cancel and we obtain after somesimple
calculation
Annales de Henri Physique theorique
Transformation into p-space
yields
We know that
I
...I
p"I
pl -kl -k2, kl, k2)
has supportinpl
EV -,
whereasd + (p 1 )
has support in p 1 EV+ .
Hence theproduct
vanishes and the same is true for the second term in(5.6).
It follows thatD6
= 0. Inthe same way as in part 4 we can conclude that the
hermiticity
conditionis satisfied also for the
non-regularized
and renormalized sector 03C4-functions.d )
LocalCommutativity
From
(a)
we know the relativistic invariance of the sector ’[-functions. HenceWe choose L such that
(Lx - Lxj + 1)0
> 0. This isalways possible
if(x~ - x J + 1 )2
0. Thenwhere we used the fact that we can permute arguments within a sector.
Now we choose L’ E
L~
such thatL’Xj+ 1)0
0. ThenThe main
point
in theproof
is that every sector ’[-function is Lorentz inva- riant for every selection of boundaries.At last we have to prove the Cluster
Decomposition Property.
Wecan
completely
mimic the axiomaticproof.
The essentialassumptions
are
locality,
spectrum condition and the fact that theWightman
functionsare
tempered
distribution.By
the results of this section..., xn)
is theboundary
value ofan
analytic
function in a forward tube[1 ]. W~
is thusuniquely
determinedby
its values in the open real> ~
> > ...> ~ },
where it mustcoincide with
... , xn).
Hence our solution of theproblem posed
inthe introduction is
unique.
ACKNOWLEDGMENT
It is a
pleasure
for me to thank Professor Dr O. Steinmann for manystimulating
discussions and his continuous support.[1] A. S. WIGHTMAN, Quantum Field Theory in Terms of Vacuum Expectation Values, Phys. Rev., t. 101, 1956, p. 860.
[2] R. STREATER and A. WIGHTMAN, PCT, Spin and Statistics, and All That, New York, 1964.
[3] H. EPSTEIN and V. GLASER, The role of locality in perturbation Theory, Ann.
Inst.Henri Poincaré, t. 19, 1973, p. 3.
[4] W. ZIMMERMANN, Local Operator Products and Renormalization in Quantum Field Theory, in Lectures on Elementary Particle Physics and Quantum Field Theory,
Brandeis University, Summer Institute in Theoretical Physics; MIT Press, Cambridge, 1970.
[5] W. ZIMMERMANN, Convergence of Bogoliubov’s Method of Renormalization in Momentum Space, Comm. Math. Phys., t. 15, 1969, p. 208.
[6] K. HEPP, Proof of the Bogoliubov-Parasiuk Theorem on Renormalization, Comm.
Math. Phys., t. 2, 1966, p. 301.
( M anuscrit reçu le 24 avril 1983)
Annales de l’Institut Henri Poincare - Physique theorique .