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115. Talk in Munich. Leading logs

ASTRO, HEP-TH/PH — By Dmitry Podolsky on November 28, 2008 at 11:05 pm
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Dmitry Podolsky has got his PhD from Landau Institute for Theoretical Physics. He currently works as postdoc at Case Western Reserve University. He is also one of the editors of NEQNET.

Last time I have claimed that the leading IR divergences in the loop expansion for the inflaton pair correlation function in 115. Talk in Munich. Leading logs theory contribute in the form of expansion

115. Talk in Munich. Leading logs .

Let me now show how these divergences appear. First of all, let us forget about the interaction term 115. Talk in Munich. Leading logs and show that the correlation function 115. Talk in Munich. Leading logs for the free field 115. Talk in Munich. Leading logs on dS background diverges in the IR.

We can write

115. Talk in Munich. Leading logs , (1)

where

115. Talk in Munich. Leading logs

115. Talk in Munich. Leading logs (2)

are the eigenmodes of the free scalar field on de Sitter background.

Keeping the leading term in the expansion (2) of the Hankel function, we find that the integral (1) diverges logarithmically on both upper and lower limits. The UV cutoff for the integral is given by the scale 115. Talk in Munich. Leading logs , where the Hankel function starts to oscillate rapidly. The IR cutoff for (1) is given by the value of scale factor at the very beginning of inflation, when all modes were still subhorizon: 

115. Talk in Munich. Leading logs .

We therefore find

115. Talk in Munich. Leading logs (3)

If you want to see a more accurate derivation, then I can recommend to take a look at the famous book by Andrei Linde. What I am going to talk about next is not written in any book yet 115. Talk in Munich. Leading logs

How to estimate behavior of this correlator in the interacting 115. Talk in Munich. Leading logs theory in de Sitter background?

Let us take renormalizations into account and write the effective Lagrangian as

115. Talk in Munich. Leading logs ,

where 115. Talk in Munich. Leading logs and 115. Talk in Munich. Leading logs . The equation of motion for the Heisenberg operator 115. Talk in Munich. Leading logs is

115. Talk in Munich. Leading logs . (4)

We just considered the r.h.s. of (4) as a source term and want to write the solution of this equation in the symbolic integral form:

115. Talk in Munich. Leading logs , (5)

where 115. Talk in Munich. Leading logs is the solution of the EOMs for 115. Talk in Munich. Leading logs , i.e., for the case of free field.

The Eq. (5) is called Yang-Feldman equation and we can easily construct its solution by iterations. It is easy to see that the corresponding expansion for the two point correlator has the following general (and again symbolic 115. Talk in Munich. Leading logs ) form:

115. Talk in Munich. Leading logs (6)

If we note that the most divergent contribution comes from 115. Talk in Munich. Leading logs in the integral in (5) and take (3) into account, we conclude that the small parameter in the expansion (6) is actually 115. Talk in Munich. Leading logs instead of 115. Talk in Munich. Leading logs .

This expansion is called the leading log expansion. It was first introduced by Woodard as far as I know (see for example this paper and references therein).

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