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.
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ArXiv ePrint: 1908.03498
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Chamseddine, A.H., Mukhanov, V. & Russ, T.B. Black hole remnants. J. High Energ. Phys. 2019, 104 (2019). https://doi.org/10.1007/JHEP10(2019)104
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DOI: https://doi.org/10.1007/JHEP10(2019)104