Black hole remnants
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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.
KeywordsBlack Holes Classical Theories of Gravity Spacetime Singularities
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