Generalized Laws of Black Hole Thermodynamics and Quantum Conservation Laws on Hawking Radiation Process
نویسندگان
چکیده
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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Four Quantum Conservation Laws for Black Hole Stationary Equilibrium Radiation Processes
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