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

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 $\ln 3$".