Black hole remnants

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dc.contributor.authorChamseddine, Ali H.
dc.contributor.authorMukhanov, Viatcheslav F.
dc.contributor.authorRuss, Tobias B.
dc.contributor.departmentDepartment of Physics
dc.contributor.facultyFaculty of Arts and Sciences (FAS)
dc.contributor.institutionAmerican University of Beirut
dc.date.accessioned2025-01-24T11:25:11Z
dc.date.available2025-01-24T11:25:11Z
dc.date.issued2019
dc.description.abstractWe 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. © 2019, The Author(s).
dc.identifier.doihttps://doi.org/10.1007/JHEP10(2019)104
dc.identifier.eid2-s2.0-85073523568
dc.identifier.urihttp://hdl.handle.net/10938/26239
dc.language.isoen
dc.publisherSpringer Verlag
dc.relation.ispartofJournal of High Energy Physics
dc.sourceScopus
dc.subjectBlack holes
dc.subjectClassical theories of gravity
dc.subjectSpacetime singularities
dc.titleBlack hole remnants
dc.typeArticle

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