Entropy of Reissner-Nordström-like black holes

In Poincaré gauge theory, black hole entropy is defined canonically by the variation of a boundary term ΓH, located at horizon. For a class of static and spherically symmetric black holes in vacuum, the explicit formula reads δΓH=TδS, where T is black hole temperature and S entropy. Here, we analyze...

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Bibliographic Details
Main Authors: M. Blagojević, B. Cvetković
Format: Article
Language:English
Published: Elsevier 2022-01-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269321007553