Quantum geometry and microscopic black hole entropy

TL;DR

This paper calculates the microscopic quantum states of black holes in loop quantum gravity, confirming the Bekenstein-Hawking entropy relation and revealing new oscillatory behavior for small black holes.

Contribution

It provides a detailed state counting for quantum black holes in LQG and introduces a novel oscillatory entropy pattern at Planck scales.

Findings

Entropy is asymptotically linear with area.

Logarithmic correction with coefficient -1/2.

Oscillatory entropy behavior for small black holes.

Abstract

Quantum black holes within the loop quantum gravity (LQG) framework are considered. The number of microscopic states that are consistent with a black hole of a given horizon area $A_0$ are counted and the statistical entropy, as a function of the area, is obtained for $A_0$ up to $550 l^2_{\rm Pl}$. The results are consistent with an asymptotic linear relation and a logarithmic correction with a coefficient equal to -1/2. The Barbero-Immirzi parameter that yields the asymptotic linear relation compatible with the Bekenstein-Hawking entropy is shown to coincide with a value close to $\gamma=0.274$, which has been previously obtained analytically. However, a new and oscillatory functional form for the entropy is found for small, Planck size, black holes that calls for a physical interpretation.