Black hole evaporation in Conformal (Weyl) gravity
arXiv:1811.07309 · doi:10.1016/j.physletb.2019.04.036
Abstract
In this work, we explore all possible scenarios in the evaporation process of a spherical neutral AdS black hole in four-dimensional conformal gravity, where the equations of states are branched. In one branch, the final states correspond to the extremal black hole where the total decay time is divergent given any initial mass. In the other branch, the black holes always evaporate completely with in a finite time; the total decay time depends linearly on the AdS radius, when the mass is taken to be infinity.
6 page+references;minor corrections, references added, accepted by PLB
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Cited by in corpus (16)
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- Quasinormal Ringing and Shadows of Black Holes and Wormholes in Dark Matter-Inspired Weyl Gravity
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- Kiselev black hole and the ultra-slow evaporating behavior