Four Quantum Conservation Laws on Black Hole Equilibrium Radiation Process and Quantum Black Hole Entropy

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dc.creatorWu, S. Q.
dc.creatorCai, X.
dc.date1999-03-23
dc.date.accessioned2026-07-07T03:33:04Z
dc.date.available2026-07-07T03:33:04Z
dc.descriptionThe classical first law of thermodynamic for Kerr-Newmann black hole (KNBH) is generalized to that in quantum form on event horizon. Then four quantum conservation laws on the KNBH equilibrium radiation process are derived, and Bekenstein-Hawking's relation S=A/4 is recovered. It can be argued that the classical entropy of black hole arise from the quantum entropy of field quanta or quasi-particles inside the hole.
dc.description10 Pages, in Latex, no figure
dc.identifierhttps://arxiv.org/abs/gr-qc/9903087
dc.identifierhttp://arxiv.org/abs/gr-qc/9903087
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36477
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFour Quantum Conservation Laws on Black Hole Equilibrium Radiation Process and Quantum Black Hole Entropy
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