Black hole remnants

Abstract

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.

Keywords

• Black Holes
• Classical Theories of Gravity
• Spacetime Singularities