Black hole remnants
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...
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2019-10-01
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Online Access: | http://link.springer.com/article/10.1007/JHEP10(2019)104 |
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doaj-fa449cc020524b2e83a530d61f27fe7b2020-11-25T03:06:50ZengSpringerOpenJournal of High Energy Physics1029-84792019-10-012019101910.1007/JHEP10(2019)104Black hole remnantsAli H. Chamseddine0Viatcheslav Mukhanov1Tobias B. Russ2Physics Department, American University of BeirutTheoretical Physics, Ludwig Maxmillians UniversityTheoretical Physics, Ludwig Maxmillians UniversityAbstract 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.http://link.springer.com/article/10.1007/JHEP10(2019)104Black HolesClassical Theories of GravitySpacetime Singularities |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Ali H. Chamseddine Viatcheslav Mukhanov Tobias B. Russ |
spellingShingle |
Ali H. Chamseddine Viatcheslav Mukhanov Tobias B. Russ Black hole remnants Journal of High Energy Physics Black Holes Classical Theories of Gravity Spacetime Singularities |
author_facet |
Ali H. Chamseddine Viatcheslav Mukhanov Tobias B. Russ |
author_sort |
Ali H. Chamseddine |
title |
Black hole remnants |
title_short |
Black hole remnants |
title_full |
Black hole remnants |
title_fullStr |
Black hole remnants |
title_full_unstemmed |
Black hole remnants |
title_sort |
black hole remnants |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2019-10-01 |
description |
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. |
topic |
Black Holes Classical Theories of Gravity Spacetime Singularities |
url |
http://link.springer.com/article/10.1007/JHEP10(2019)104 |
work_keys_str_mv |
AT alihchamseddine blackholeremnants AT viatcheslavmukhanov blackholeremnants AT tobiasbruss blackholeremnants |
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1724672022148022272 |