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arXiv · 2504.06964

Thermodynamics of effective loop quantum black holes

Abstract

We study the thermodynamics of a non-singular black hole model with effective quantum corrections motivated by Loop Quantum Gravity (LQG). The effective geometry has a transition surface that connects trapped and anti-trapped regions with the same mass. There is a minimum mass for which the horizon temperature and Komar energy are zero, and the black hole stops its Hawking evaporation. For horizons above this limit, we present the grey-body factors, emission spectra, and the mass loss rate, solving a one-dimensional Schrdinger-type equation with an effective short-range potential barrier for massless fields of spins 0, 1/2, 1 and 2.

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F. G. Menezes, H. A. Borges, I. P. R. Baranov, S. Carneiro. 2025-04-09. Thermodynamics of effective loop quantum black holes. https://doi.org/10.1088/1361-6382%2Fadf936

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