General heat kernel coefficients for massless free spin-3/2 Rarita-Schwinger field
High Energy Physics - Theory
2018-04-25 v2
Abstract
We review the general heat kernel method for the Dirac spinor field as an elementary example in any arbitrary background. We, then compute the first three Seeley-DeWitt coefficients for the massless free spin-3/2 Rarita-Schwinger field without imposing any limitations on the background geometry.
Cite
@article{arxiv.1709.08063,
title = {General heat kernel coefficients for massless free spin-3/2 Rarita-Schwinger field},
author = {Sudip Karan and Shashank Kumar and Binata Panda},
journal= {arXiv preprint arXiv:1709.08063},
year = {2018}
}
Comments
13 pages