Quantum Black Holes. Black Hole Temperature without a Black Hole

TL;DR

This paper proposes a quantum model of black holes based on quantum thin dust shells, extending classical 'no hair' properties to a quantum context, and finds that the model exhibits Hawking temperature.

Contribution

It introduces a classical analog of quantum black holes derived from quantum thin dust shells, connecting quantum properties with classical black hole thermodynamics.

Findings

The model exhibits Hawking temperature exactly.

Quantum features extend classical 'no hair' properties.

The analog is heated, consistent with black hole thermodynamics.

Abstract

The model is constructed, some features of which comes from quantum thin dust shells and is, in fact, an extension of the "no hair" property of classical black hole on a quantum level. It appears that the proposed classical analog of quantum black hole is heated, the temperature being exactly the Hawking's temperature.