Black holes as gases of punctures with a chemical potential: Bose-Einstein condensation and logarithmic corrections to the entropy
Olivier Asin, Jibril Ben Achour, Marc Geiller, Karim Noui, Alejandro, Perez

TL;DR
This paper investigates black hole thermodynamics within loop quantum gravity by modeling black holes as gases of punctures with a chemical potential, revealing conditions for Bose-Einstein condensation and logarithmic entropy corrections.
Contribution
It introduces a detailed analysis of black hole microstates as Bose gases with holographic degeneracy, highlighting the role of chemical potential and conditions for semi-classical regimes.
Findings
Logarithmic corrections to entropy in the holographic limit
Bose-Einstein condensation of punctures at ground state spin
Semi-classical regime characterized by minimal spin punctures
Abstract
We study the thermodynamical properties of black holes when described as gases of indistinguishable punctures with a chemical potential. In this picture, which arises from loop quantum gravity, the black hole microstates are defined by finite families of half-integers spins coloring the punctures, and the near-horizon energy measured by quasi-local stationary observers defines the various thermodynamical ensembles. The punctures carry excitations of quantum geometry in the form of quanta of area, and the total horizon area is given by the sum of these microscopic contributions. We assume here that the system satisfies the Bose-Einstein statistics, and that each microstate is degenerate with a holographic degeneracy given by and . We analyze in detail the thermodynamical properties resulting from these inputs,…
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