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Black hole entropy in 3D gravity with torsion

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arxiv gr-qc/0601006 v2 pith:PWN6RS7Q submitted 2006-01-03 gr-qc hep-th

M. Blagojevic , B. Cvetkovic This is my paper · ORCID
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keywords blackholetorsionentropygravityagreementbekenstein-hawkingcomplete
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The role of torsion in quantum three-dimensional gravity is investigated by studying the partition function of the Euclidean theory in Riemann-Cartan spacetime. The entropy of the black hole with torsion is found to differ from the standard Bekenstein-Hawking result, but its form is in complete agreement with the first law of black hole thermodynamics.

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  1. Torsional black holes and wormholes in Einstein-Cartan-Maxwell gravity with a conformal scalar field

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    A one-parameter deformation of conformal coupling in Einstein-Cartan gravity produces exact torsional black hole and wormhole solutions with a scalar field.

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