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Black hole entropy from the boundary conformal structure in 3D gravity with torsion

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arxiv gr-qc/0606086 v2 pith:QN3E7MUS submitted 2006-06-20 gr-qc hep-th

Black hole entropy from the boundary conformal structure in 3D gravity with torsion

classification gr-qc hep-th
keywords blackboundaryconformalentropygravityholestructuretorsion
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Asymptotic symmetry of the Euclidean 3D gravity with torsion is described by two independent Virasoro algebras with different central charges. Elements of this boundary conformal structure are combined with Cardy's formula to calculate the black hole entropy.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Non-Relativistic Chern-Simons Supergravity with Torsion

    hep-th 2026-04 unverdicted novelty 7.0

    A parameterized family of non-relativistic supergravity theories with torsion is obtained in three dimensions from the semigroup expansion of an N=2 supersymmetric Mielke-Baekler algebra.

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

    hep-th 2026-05 unverdicted novelty 6.0

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