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Black Hole Remnants

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arxiv 1908.03498 v1 pith:HU7DH4UB submitted 2019-08-09 hep-th astro-ph.COgr-qc

Ali H. Chamseddine , Viatcheslav Mukhanov , Tobias B. Russ This is my paper · ORCID
classification hep-thastro-ph.COgr-qc
keywords blackhawkingholeremnantsasymptoticallycurvatureevaporationfree
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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.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Constructing regular black holes from multi-polytropic equations of state

    gr-qc 2025-02 reject novelty 5.0 of 10

    Two regular black hole metrics are derived from anisotropic multi-polytropic TOV equations; one reduces to the known Hayward geometry and the other is new, with repulsive-gravity regions outside the horizon for partic...

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