2. Main Part
Let us consider a functional integral for the generating functional of Green functions of some generic theory (this can be QCD or QED or any other theory):
where
is the integration measure of the functional integral
including all allowed types of the fields
of the theory.
are sources of these fields.
J in
is the full set of
.
is the free Lagrangian and
is the interaction Lagrangian of the considered theory.
g is the coupling constant of interacrions of the theory.
N is the standard normalization factor. Generalization to the case of several coupling constants of interactions is completely straightforward.
Of course the generating functional (
1) is not completely defined by the defining the Lagrangiann
only. One should also define which types of the fields
are allowed in the integration measure. If one allows integration over all possible configurations of the fields
, then it is not possible to reproduce the perturbative fields propagators of the necessary forms, i.e. with the correct ’
’ prescription of the type
.
To obtain the perturbative propagators of the correct forms one should impose on the integrated fields the known boundary conditions. For example, one has the following boundary conditions for the gluon fields in QCD:
where the incoming gluon fields
contain only the positive frequency part and, in opposite, the outgoing asymptotic gluon fields
contain the negative frequency part:
Here
,
are the polarization vectors of the gluons. In (
3) sums over gluon polarizations
are assumed.
These are the known Feynman boundary conditions of emission. They ensure the correct forms of perturbative propagators of the fields of the type
) with the necessary plus
prescription, see [
8].
Hence the gluon fields (the quark fields also) in QCD with emission boundary conditions oscillate at time infinities. Making transition to the Euclidean space with the help of the Wick rotation
one gets that the fields decrease at time infinities. Thus it is easy to see that in the Euclidean space total derivatives in the Lagrangian are zero within perturbation theory. This allows, in particular, to solve [
3] the Strong CP problem without involving hypothetical exotic particles like axions; for the review of axions see [
9].
One can write perturbative boundary conditions (
2) for all fields
of the considered theory (
1) symbolically as follows:
This short notation is used below to formulate the functional intergal for the generating functional of Green functions as a uniquely defined compact formula.
We will devide all fields in two classes: perturbative and non-perturbative. Let us call the fields with the boundary conditions (
4) as pertubative fields and the rest of fields (including in particular instantons) as non-perturbative fields.
If one defines the generating functional with integrations over all possible field configurations, then one should also integrate over the non-perturbative fields like instantons [
4] in addition to the perturbative fields with emission boundary conditions. These non-perturbative fields produce only non-perturbative contributions and do not effect the perturbative propagators. But then one comes to uncertainties since there can be, in principle, other non-perturbative solutions like instantons and it is not known in advance how many of them exist.
That is why it seems to be natural to use the boundary conditions of emission (
4) for all fields
over which the integration in the the functional integral (
1) proceeds. Then, in particular, all fields decrease in the Euclidean space at the time infinities. Hence total derivatives in the Lagrangian are nullified and this, in particular, solves [
3] the strong CP problem. Besides, this definition of the boundary conditions allows to formulate uniquely the complete generating functional integral of Green functions of the theory as an exact compact mathematical formula:
It turns out that this expression for the generating functional integral contains only perturbative contributions and does not contain non-perturbative ones. Let us demonstrate it.
The standard perturbation expansion of Green functions of the generating functional (
5) at the point
produces after renormalizations well defined perturbative series with finite coefficients (which are known to be asymptotic series). This excludes non-perturbative contributions to Green functions of the type
, etc, since they would produce unrenormalized infinities at
.
One can expand the generating functional (
5) in the perturbative series in the coupling constant
g also at the point
in the same way as one expands at the point
. (One expands the exponential integrand of the functional integral (
5) and performs integrations over fields with the boundary conditions (
4) similarly to the case
.) The expansion is again well defined. This is the perturbation theory with the finite coefficients (the counterterms are assumed to be included into the Lagrangian) since integrations in the functional integral (
5) proceed only over the fields with perturbative boundary conditions (
4). It excludes the presence of the non-perturbative contributions of the type
since otherwise the expansion would produce infinities at the point
.
Let us consider the integral function
as an example. The formal expansion of this function generates the known asymptotic series:
here the expansion can be performed both at the point
and at
with the same result for the asymptotic series.
One can also analize an expansion of the functional integral (
5) at the point
. Again the coefficients of the expansion will be finite on the same reasons as above. This excludes the presence of the non-perturbative terms of the type
since infinities would be generated otherwise.
More generally, to demonstrate the absence of the non-perturbative terms of the type
, where
x is an arbitrary positive number, one can consider an expansion at the point
. The expansion is finite. This demonstrates the absence of the non-perturbative contributions in the generating functional (
5).
There is the question of the so called non-perturbative vacuum quark and gluon condensates used in the method of the QCD sum rules [
2] for calculation of hadronic properties. These condensates have the values
and at the normalization point of the order of . Here q is the quark field, is the gluon strength tensor, , where is the strong coupling constant in the QCD Lagrangian.
But, in principle, one can generate these condensates within perturbation theory with massive perturbative propagators after the summations of the complete asymptotic perturbative series for the corresponding vacuum expectation values.