2019/08/09 by Ali H. Chamseddine, Viatcheslav Mukhanov, Tobias B. Russ
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #Extremal black hole #Hawking radiation #Limiting #Naked singularity #Quantum Electrodynamics and Casimir Effect #Ring singularity #Singularity #White hole #astro-ph.CO #de Sitter–Schwarzschild metric #gr-qc #hep-th
paper · pdf · doi:10.1007/jhep10(2019)104
published as JHEP (2019) 104 · 4 pages
arxiv created 2019/08/09 · openalex created_date 2019/08/22 · openalex publication_date 2019/10/01 · arxiv updated 2020/08/05 · openalex updated_date 2026/08/05
A bstract 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.