Thermodynamics and remnants of Kiselev black holes in Rainbow gravity

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.

References in corpus (1)

• Thermodynamic phase transition in the rainbow Schwarzschild black hole

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• Three-dimensional energy-dependent $C$-metric: black hole solutions
• Black hole solutions surrounded by anisotropic fluid in f(T,T) gravity
• Einstein-Yang-Mills Regular Black Holes in Rainbow Gravity