Black Hole Solution of Quantum Gravity

TL;DR

This paper introduces an exact quantum gravity black hole solution that resembles classical black holes at large distances and exhibits two horizons for certain masses, with an analysis of its thermodynamics.

Contribution

It provides a novel exact spherically symmetric solution to Quantum Einstein Equations, connecting quantum gravity effects with classical black hole properties.

Findings

Solution is asymptotically anti-De Sitter

Possesses two horizons for specific mass ranges

Includes thermodynamical analysis of the quantum black hole

Abstract

We present a spherically symmetric and static exact solution of Quantum Einstein Equations. This solution is asymptotically (for large $r$) identical with the black hole solution on the anti--De Sitter background and, for some range of values of the mass possesses two horizons. We investigate thermodynamical properties of this solution.