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This analysis identifies mass thresholds affecting Hawking evaporation in black holes, suggesting implications for quantum gravity theories.
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 Schrödinger-type equation with an effective short-range potential barrier for massless fields of spins 0, 1/2, 1 and 2.
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Menezes et al. (2025) studied this question.
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