2021/09/30 by Gourav Banerjee, Binata Panda
Physics and Astronomy · #hep-th
paper · pdf · doi:10.1007/jhep11(2021)214
published as Journal of High Energy Physics 11(2021)214 · Version published in JHEP
arxiv created 2021/11/30 · arxiv updated 2021/12/01
We reviewed the field redefinition approach of Seeley-DeWitt expansion for the determination of Seeley-DeWitt coefficients from arXiv:1505.01156. We apply this approach to compute the first three Seeley-DeWitt coefficients for \saynon-minimal N=1 Einstein-Maxwell supergravity in four dimensions. Finally, we use the third coefficient for the computation of the logarithmic corrections to the Bekenstein-Hawking entropy of non-extremal black holes following arXiv:1205.0971. We determine the logarithmic corrections for non-extremal Kerr-Newman, Kerr, Reissner-Nordström and Schwarzschild black holes in \saynon-minimal N=1, d=4 Einstein-Maxwell supergravity.