Four Quantum Conservation Laws on Black Hole Equilibrium Radiation Process and Quantum Black Hole Entropy
General Relativity and Quantum Cosmology
2007-05-23 v1
Abstract
The 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.
Keywords
Cite
@article{arxiv.gr-qc/9903087,
title = {Four Quantum Conservation Laws on Black Hole Equilibrium Radiation Process and Quantum Black Hole Entropy},
author = {S. Q. Wu and X. Cai},
journal= {arXiv preprint arXiv:gr-qc/9903087},
year = {2007}
}
Comments
10 Pages, in Latex, no figure