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Generalized Laws of Black Hole Thermodynamics and Quantum Conservation Laws on Hawking Radiation Process

S. Q. Wu·X. Cai
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Abstract

Four classical laws of black hole thermodynamics are extended from exterior (event) horizon to interior (Cauchy) horizon. Especially, the first law of classical thermodynamics for Kerr-Newman black hole (KNBH) is generalized to those in quantum form. Then five quantum conservation laws on the KNBH evaporation effect are derived in virtue of thermodynamical equilibrium conditions. As a by-product, Bekenstein-Hawking's relation $ S=A/4 $ is exactly recovered.

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S. Q. Wu, X. Cai. 2000-04-13. Generalized Laws of Black Hole Thermodynamics and Quantum Conservation Laws on Hawking Radiation Process. https://arxiv.org/abs/gr-qc/0004040

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