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Statistical Mechanics and Black Hole Entropy

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arxiv gr-qc/9509024 v2 pith:GDMV27QW submitted 1995-09-13 gr-qc hep-th

S. Carlip This is my paper · ORCID
classification gr-qchep-th
keywords blackholeentropyapproachboundaryexplaingravitationalhorizon
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I review a new (and still tentative) approach to black hole thermodynamics that seeks to explain black hole entropy in terms of microscopic quantum gravitational boundary states induced on the black hole horizon.

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Cited by 2 Pith papers

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

  1. Spacetime structure near generic horizons and soft hair

    hep-th 2019-08 conditional novelty 6.0 of 10

    A family of horizon boundary conditions labeled by s yields BMS-like algebras with spin-s supertranslations, while another choice gives a non-linear Heisenberg-like algebra whose generators build the BMS-like ones.

  2. Embedding into flat spacetime and black hole thermodynamics

    gr-qc 2019-08 conditional novelty 4.0 of 10

    Black hole temperature and area-law entropy are reproduced from a higher-dimensional flat spacetime embedding, mapping static observers to accelerating observers and counting scalar edge states.

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