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The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes

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arxiv gr-qc/0409107 v3 pith:4MUSW4JF submitted 2004-09-28 gr-qc hep-th

classification gr-qchep-th
keywords blackholesmotionssphericallystationarysymmetricapproachchemical
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We generalize the work of Deser and Levin on the unified description of Hawking radiation and Unruh effect to general stationary motions in spherically symmetric black holes. We have also matched the chemical potential term of the thermal spectrum of the two sides for uncharged black holes.

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  1. 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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