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The model is built in which the main global properties of classical andquasi-classical black holes become local. These are the event horizon,"no-hair", temperature and entropy. Our construction is based on the featuresof a quantum collapse, discovered while studying some quantum black holemodels. But it is purely classical, and this allows to use the Einsteinequations and classical (local) thermodynamics and explain in this way the"log(3)" - puzzle.

On Classical Analogs of Quantum Schwarzschild and Reissner-Nordstrom Black Holes. Solving the "Mystery of log(3)"