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Entropy of Kerr--Newman--AdS black holes with torsion

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arxiv 2203.14696 v1 pith:P52D25Q5 submitted 2022-03-24 gr-qc hep-th

Milutin Blagojević , Branislav Cvetković This is my paper · ORCID
classification gr-qchep-th
keywords blackentropyfieldholesmattermaxwelltorsionapproach
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The canonical approach to black hole entropy in Poincar\'e gauge theory without matter is extended to include Maxwell field as a matter source. The new formalism is used to calculate asymptotic charges and entropy of Kerr--Newmann--AdS black holes with torsion. The result implies that the first law, with a nontrivial contribution of the Maxwell field, takes the same form as in general relativity.

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  1. Near-horizon geometry with torsion: Kerr-AdS black hole

    gr-qc 2025-11 conditional novelty 6.0 of 10

    Covariant conditions are derived for a regular near-horizon limit with torsion, and a new Kerr-AdS black hole with torsion is constructed that satisfies them.

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