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Journal of High Energy Physics

, 2019:104 | Cite as

Black hole remnants

  • Ali H. ChamseddineEmail author
  • Viatcheslav Mukhanov
  • Tobias B. Russ
Open Access
Regular Article - Theoretical Physics
First Online:
  • 71 Downloads

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.

Keywords

Black Holes Classical Theories of Gravity Spacetime Singularities 
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Notes

Open Access

This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited

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Copyright information

© The Author(s) 2019

Authors and Affiliations

  1. 1.Physics DepartmentAmerican University of BeirutBeirutLebanon
  2. 2.Theoretical PhysicsLudwig Maxmillians UniversityMunichGermany
  3. 3.MPI for PhysicsMunichGermany
  4. 4.School of PhysicsKorea Institute for Advanced StudySeoulKorea

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