Seeley-DeWitt Coefficients in Einstein-Maxwell Supergravity Theory and Logarithmic Corrections to Extremal Black Hole Entropy
arXiv:1905.13058 · doi:10.1007/JHEP08(2019)056
Abstract
We investigate the heat kernel method for one-loop effective action following the Seeley-DeWitt expansion technique of heat kernel with Seeley-DeWitt coefficients. We also review a general approach of computing the Seeley-DeWitt coefficients in terms of background or geometric invariants. We, then consider the Einstein-Maxwell theory embedded in minimal supergravity in four dimensions and compute the first three Seeley-DeWitt coefficients of the kinetic operator of the bosonic and the fermionic fields in an arbitrary background field configuration. We find the applications of these results in the computation of logarithmic corrections to Bekenstein-Hawking entropy of the extremal Kerr-Newman, Kerr and Reissner-Nordstrom black holes in minimal Einstein-Maxwell supergravity theory following the quantum entropy function formalism.
V4: the Kerr-Newman results in eqs. (6.14) and (6.15) are simplified into a topological form
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- Generalized Einstein-Maxwell theory: Seeley-DeWitt coefficients and logarithmic corrections to the entropy of extremal and non-extremal black holes
- Logarithmic corrections to black hole entropy in matter coupled Einstein-Maxwell supergravity
- Logarithmic correction to the entropy of extremal black holes in Einstein-Maxwell supergravity
- Logarithmic corrections to the entropy of non-extremal black holes in Einstein-Maxwell supergravity
- Logarithmic correction to the entropy of a Kerr-Newman family of black holes in -charged STU supergravity models
- Scattering approach for calculating one-loop effective action and vacuum energy