Thermal dimensional reduction and black hole evaporation

G. B. Santos; I. P. Lobo

Thermal dimensional reduction and black hole evaporation

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arxiv 2009.08556 v2 pith:YTMKRUR2 submitted 2020-09-17 gr-qc hep-th

I. P. Lobo , G. B. Santos This is my paper · ORCID

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We analyze how a quantum-gravity-induced change in the number of thermal dimensions (through a modified dispersion relation) affects the geometry and the thermodynamics of a charged black hole. To that end we resort to Kiselev's solution as the impact such modifications have on the evaporation rate of the black hole becomes more clear. As an application, we study the case for which the thermal dimension is reduced to two.

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The Case For Black Hole Remnants: A Review
gr-qc 2024-11 unverdicted novelty 2.0 of 10

A review arguing that black hole remnants remain viable and that the species and entropy objections to them are not decisive, so remnants could resolve the information paradox.

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