Thermodynamics and remnants of Kiselev black holes in Rainbow gravity
P. H. Morais, G. V. Silva, J. P. Morais Gra\c{c}a, V. B. Bezerra
TL;DR
This paper investigates the thermodynamics of Kiselev black holes within Rainbow gravity, finding no general evidence for black hole remnants except in specific cases, thus challenging previous assumptions about remnants in such models.
Contribution
It provides a detailed analysis of black hole thermodynamics in Rainbow gravity with various cosmic fluids, highlighting the absence of remnants in most scenarios.
Findings
No evidence of black hole remnants in Rainbow gravity generally
Remnants appear only in peculiar, specific cases
Thermodynamics behavior varies with different cosmic fluids
Abstract
We do a detailed study of the thermodynamics of black holes in Rainbow gravity in the framework of the Kiselev metric, taking into account different cosmic fluids which can mimic several kinds of dark energy scenarios. A discussion related to the appearance of black hole remnants is presented and, unlike other studies on the same topic, we found no evidence of the appearance of remnants in Rainbow gravity, except in peculiar cases.
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