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Black Hole Remnants

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.

7 nodes7 linksoverview previewBlack Hole Remnants
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Black Hole Remnants7 visible / 7 total nodes / 10 links
Co-authorshipCo-authorshipCo-authorshipAuthorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalRelated contextWBlack Hole Remnantspreprint / 2019AAli H. ChamseddineResearcherAViatcheslav MukhanovResearcherATobias B. RussResearcherTastro-ph.CO6979 worksTgr-qc10727 worksThep-th13268 works
PaperSignal 106 links

Black Hole Remnants

preprint / 2019

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