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Wednesday, November 7, 2012

The 1PI Effective Action

In this post I'd like to try to understand the 1PI effective action that is often of interest. Suppose we have a QFT in some bosonic field ϕ(x) taking values in a vector space (this is important). Then its vev ϕcl(x):=ϕ(x) is just an ordinary (but possibly distributional) field on spacetime. The question is, what is the field equation satisfied by ϕcl? I.e., if we average over quantum effects by replacing all fields by their vevs, what is the action that governs this (now completely classical) theory? The 1PI effective action answers exactly this question.

Consider the generating functional
Z[J]=eS[ϕ]+ϕ,JDϕ
Then for a given source J, define the J-vev of ϕ(x) to be
ϕJ(x)=logZ[J]J.
Now let's take Γ to be the Legendre transform of logZ with respect to J:
Γ[ϕJ]=J,ϕJlogZ[J]
Then we compute:
ΓϕJ=J+JϕJϕJlogZ[J]JJϕJ=J.

Now consider the situation without a background source, i.e. J=0. Then ϕ0=ϕcl and we find
Γϕcl=0
Hence, ϕcl satisfies the Euler-Lagrange equations associated to the functional Γ. Note that from the Legendre transform, Γ takes quantum effects (i.e. Feynman diagrams with loops) into account, even though the field and the equations are purely classical!

By studying these equations, we might find instanton solutions (or solitons in Lorentz signature).

Now for the name. Some combinatorics and algebra (which I will skip!) show that Γ[ϕcl] is itself a generating functional for certain correlation functions, then 1PI correlation functions:
nΓϕ(x1)ϕ(xn)=ϕ(x1)ϕ(xn)1PI.
The 1PI subscript means that the RHS is computed in perturbation theory by summing over only the connection 1PI (1 particle irreducible) Feynman diagrams.

Warning: As usual, there are regularization issues, both in the UV and IR. UV divergences can be solved by a cutoff (if we only care about effective field theory), but IR divergences are much more technical. For this reason (and others), it is sometimes preferable to try to understand the low energy dynamics by studying the Wilsonian effective action. As the Wilsonian effective action does not take IR modes into account, it can avoid many of the difficulties of the 1PI effective action.

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