Abstract:
The model is built in which the main global properties of classical and quasi-classical black holes become local (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 self-consistently the Einstein equations and classical (local) thermodynamics and explain in this way the "$\log3$"-puzzle.
Keywords:classical and quasi-classical black holes.