2000/04/13 by S. Q. Wu, X. Cai
Physics and Astronomy · #gr-qc
published as Nuovo Cim. B115 (2000) 143-150 · Latex, 8 pages, no figure
arxiv created 2000/04/13 · arxiv updated 2009/11/30
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.