Heat Kernel Expansions for Distributional Backgrounds
High Energy Physics - Theory
2009-10-31 v1
Abstract
Heat kernel expansion coefficients are calculated for vacuum fluctuations with distributional background potentials and field strengths. Terms up to and including t^5/2 are presented.
Cite
@article{arxiv.hep-th/0007185,
title = {Heat Kernel Expansions for Distributional Backgrounds},
author = {Ian G Moss},
journal= {arXiv preprint arXiv:hep-th/0007185},
year = {2009}
}
Comments
6 pages, ReVTeX