The Heat Kernel in Riemann Normal Coordinates and Multiloop Feynman Graphs in Curved Spacetime
Igor Carneiro, Gero von Gersdorff

TL;DR
This paper develops a formalism using the heat kernel method to compute multi-loop Feynman graphs in curved spacetime, specifically calculating off-diagonal heat kernel components in Riemann normal coordinates up to second order in curvature.
Contribution
It introduces a novel approach for evaluating complex Feynman graphs in curved spacetime by explicitly computing heat kernel components in Riemann normal coordinates.
Findings
Derived off-diagonal heat kernel components up to second order in curvature.
Provided a systematic method for multi-loop Feynman graph calculations in curved backgrounds.
Enhanced the computational toolkit for quantum field theory in curved spacetime.
Abstract
We present a formalism for computing arbitrary multi-loop Feynman graphs in curved spacetime using the heat kernel approach. To this end, we compute the off-diagonal components of the heat kernel in Riemann normal coordinates up to second order in the curvature.
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Taxonomy
Topicsadvanced mathematical theories · Cosmology and Gravitation Theories · Advanced Mathematical Theories and Applications
