Classical analog of quantum Schwarzschild black hole: local vs global, and the mystery of log(3)

Details Classical analog of quantum Schwarzschild black hole: local vs global, and the mystery of log(3) Classical analog of quantum Schwarzschild black hole: local vs global, and the mystery of log(3)

2010-06-02

arxiv.org/abs/1006.0362v1

Int.J.Mod.Phys.A26:161-178,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

20 pp, no figures, preprint IHES/P/10/15, submitted to Classical and Quantum Gravity

Scientific paper

10.1142/S0217751X11051135

The model is built in which the main global properties of classical and quasi-classical black holes become local. These are the event horizon, "no-hair", temperature and entropy. Our construction is based on the features of a quantum collapse, discovered when studying some quantum black hole models. But our model is purely classical, and this allows to use selfconsistently the Einstein equations and classical (local) thermodynamics and explain in this way the log(3)-puzzle.

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