Euclidean quantum gravity for Kerr-Newman Spacetimes

Published 11 Dec 2019 in gr-qc | (1912.05674v2)

Abstract: It is very important to calculate the amount of radiation from a black hole as the radiation from a black hole contributes to its entropy. In this paper I have calculated the Entropy of a black hole from the action. I have used path integral formalism to calculate the second order perturbation of the metric in the action for a generalized Kerr-Newman metric.

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Rohan Raha

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