Four Quantum Conservation Laws for Black Hole Stationary Equilibrium Radiation Processes

Details Four Quantum Conservation Laws for Black Hole Stationary Equilibrium Radiation Processes Four Quantum Conservation Laws for Black Hole Stationary Equilibrium Radiation Processes

2000-09-12

arxiv.org/abs/hep-th/0009088v1

Int.J.Theor.Phys. 39 (2000) 2215-2220

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, no figure, Revtex in 12pt

Scientific paper

The classical first law of thermodynamics for a Kerr-Newman black hole (KNBH) is generalized to a law in quantum form on the event horizon. Then four quantum conservation laws on the KNBH equilibrium radiation process are derived. The Bekenstein-Hawking relation ${\cal{S}}={\cal{A}}/4$ is exactly established. It can be inferred that the classical entropy of black hole arises from the quantum entropy of field quanta or quasi-particles inside the hole.

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