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

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dc.creatorWu, S. Q.
dc.creatorCai, X.
dc.date2000-04-13
dc.date.accessioned2026-07-07T03:24:52Z
dc.date.available2026-07-07T03:24:52Z
dc.descriptionFour 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.
dc.descriptionLatex, 8 pages, no figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0004040
dc.identifierhttp://arxiv.org/abs/gr-qc/0004040
dc.identifierNuovo Cim. B115 (2000) 143-150
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33504
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneralized Laws of Black Hole Thermodynamics and Quantum Conservation Laws on Hawking Radiation Process
dc.typetext

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