Hamiltonian approach to black hole entropy: Kerr-like spacetimes

B. Cvetkovi\'c; M. Blagojevi\'c

Hamiltonian approach to black hole entropy: Kerr-like spacetimes

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arxiv 1905.04928 v4 pith:QUF2RMF5 submitted 2019-05-13 gr-qc hep-th

Hamiltonian approach to black hole entropy: Kerr-like spacetimes

M. Blagojevi\'c , B. Cvetkovi\'c This is my paper

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keywords blackentropyholespacetimeskerr-likesolutionsapproachcanonical

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Black hole entropy of the Kerr-like family of spacetimes is introduced as the canonical charge on the horizon. Treating these spacetimes in the framework of Poincar\'e gauge theory either as Riemannian solutions or as solutions with torsion, it is shown that these geometrically different setups lead to the same black hole entropy.

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Near-horizon geometry with torsion: Kerr-AdS black hole
gr-qc 2025-11 conditional novelty 6.0

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.