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 (18)

• Relativity in space-times with short-distance structure governed by an observer-independent (Planckian) length scale
• Quintessence and black holes
• Testable scenario for Relativity with minimum-length
• Generalized Lorentz invariance with an invariant energy scale
• Loop Quantum Gravity
• Gravity's Rainbow
• Quantum Gravity: a Progress Report
• Doubly Special Relativity
• Planck-scale deformation of Lorentz symmetry as a solution to the UHECR and the TeV-$\gamma$ paradoxes
• Black Hole Remnants and the Information Loss Paradox
• Black Holes and Massive Remnants
• Black Hole Remnants and Dark Matter
• Thermodynamics of modified black holes from gravity's rainbow
• Black Hole Remnant from Gravity's Rainbow
• Cosmic rays and TeV photons as probes of quantum properties of space-time
• Thermodynamic phase transition in the rainbow Schwarzschild black hole
• Strings, Branes and Extra Dimensions
• Thermodynamics and Luminosities of Rainbow Black Holes

Cited by in corpus (7)

• Thermodynamic topology of topological black hole in $F(R)$-ModMax gravity's rainbow
• Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow
• Dark Energy Star in Gravity's Rainbow
• Relativistic Bose-Einstein condensate in the rainbow gravity
• 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