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Horizon thermodynamics and spacetime mappings

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arxiv 1401.1189 v1 pith:CG36TL7L submitted 2014-01-06 gr-qc astro-ph.CO

Valerio Faraoni , Vincenzo Vitagliano This is my paper · ORCID
classification gr-qcastro-ph.CO
keywords horizonsblackdynamicalholesthermodynamicstransformationsapparentarguments
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When black holes are dynamical, event horizons are replaced by apparent and trapping horizons. Conformal and Kerr-Schild transformations are widely used in relation with dynamical black holes and we study the behaviour under such transformations of quantities related to the thermodynamics of these horizons, such as the Misner-Sharp-Hernandez mass (internal energy), the Kodama vector, surface gravity, and temperature. The transformation properties are not those expected on the basis of naive arguments.

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  1. Thermodynamic parameters of fluids on conformally connected spacetimes

    gr-qc 2025-05 conditional novelty 6.0 of 10

    For conformally related Einstein spacetimes, equilibrium fluid temperature and chemical potential both scale as the inverse conformal factor, preserving the ratio μ/T.

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