Black hole remnants
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Springer Verlag
Abstract
We show that in asymptotically free mimetic gravity with limiting curvature the black hole singularity can be resolved and replaced by a static patch of de Sitter space. As a result of Hawking evaporation of these non-singular black holes, there remain stable remnants with vanishing Hawking temperature. © 2019, The Author(s).
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Keywords
Black holes, Classical theories of gravity, Spacetime singularities