Calculate $\hbar \ln$ Gaussian Path Integral w/Einstein Summation

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Homework Help Overview

The discussion revolves around calculating a Gaussian path integral involving the Einstein summation convention. The original poster presents an expression for the integral and an expected result, while expressing uncertainty about the next steps in the calculation.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants explore the implications of the Fourier transform and the treatment of variables s and r, questioning why they may be treated differently in the context of the integral.

Discussion Status

The discussion is ongoing, with participants providing insights and questioning the assumptions made in the original formulation. Some guidance is offered regarding the interpretation of the variables involved, but no consensus has been reached.

Contextual Notes

There are references to specific equations and properties from a paper by R. Golestanian, which may influence the understanding of the problem. Participants also note potential issues with the original poster's interpretation of the integral.

MadMax
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Einstein summation convention employed throughout

We want to calculate

\hbar \ln \int D x_i \exp[\frac{1}{32 \pi^3} \int ds \int d^3 r x_i(-is,r) M_{ij}(s,r) x_j(is,r)]

The answer is

\hbar \int \frac{ds}{2\pi} \ln \det[M_{ij}\delta^3(r-r')]

I know that

\int d^3 x_i e^{\frac{1}{2}x_i B_{ij} x_j} = \sqrt{\frac{(2\pi)^n}{\det B_{ij}}}

and that standard logarithmic properties will be used. Also the \delta^3(r-r') means that a Fourier transform involving that delta function will be employed at some point.

Beyond that I'm at a complete loss as to how to continue. One question is why we don't need to employ a Fourier transform involving a \delta(s-s')]. Any help would be much appreciated.
 
Last edited:
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I was hoping someone else would tackle this one, but here goes ...

The answer doesn't make sense to me. I don't see why s should be fundamentally different than r. I think you should have a \delta(s+s'), with + rather than - because the arguments have opposite sign, and that there should be no integral over s.

But perhaps there is something about the definition of x(is,r) that you haven't told us that would change this ...
 
Thanks.

What kind of things might make s different to r in that way?

Perhaps these? "is" is wick rotated frequency; and started out as the Fourier transform of time. r is real space. r is a vector and s is a scalar.
 
Last edited:
MadMax said:
What kind of things might make s different to r in that way?
Perhaps these? "is" is wick rotated frequency; and started out as the Fourier transform of time. r is real space. r is a vector and s is a scalar.

No, none of that should matter.

Is this from a book? If so, which one?
 
He's just being sloppy. His eq.(1) is wrong, and should be what I said. Then he trades log det for Tr log, and the integral over zeta in eq.(3) is part of the trace, just like the integrals over r.
 
Ahh brilliant. Thanks again. :)
 

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