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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
  • 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 

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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