Classical analogue of a quantum Schwarzschild black hole: "Standard model" and beyond

Details Classical analogue of a quantum Schwarzschild black hole: "Standard model" and beyond Classical analogue of a quantum Schwarzschild black hole: "Standard model" and beyond

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012tmp...170...71b&link_type=abstract

Theoretical and Mathematical Physics, Volume 170, Issue 1, pp.71-82

Mathematics

Mathematical Physics

Quantum Black Hole, Thermodynamics, Quasinormal Frequency

Scientific paper

We build a model in which the main global properties of classical and semiclassical 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 particular quantum black hole models. But our model is purely classical, and this allows using the Einstein equations and classical (local) thermodynamics self-consistently and, in particular, solving the "puzzle of log 3."

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