Skip to main content
Article thumbnail
Location of Repository

Black hole masking and black hole thermodynamics

By Oleg B. Zaslavskii

Abstract

Masking of black holes means that, for given total mass and Hawking temperatures, these data may correspond to either "pure" black hole or a black hole of a lesser mass surrounded by a massive shell. It is shown that there is one-to one correspondence between this phenomenon and thermodynamics of a black hole in a finite size cavity: masking of black holes is possible if and only if there exists at least one locally unstable black hole solution in the corresponding canonical ensemble.Comment: 7 pages. To appear in Gravitation and Cosmolog

Topics: General Relativity and Quantum Cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Theory
Year: 2011
DOI identifier: 10.1134/S020228931103011X
OAI identifier: oai:arXiv.org:1102.4056
Download PDF:
Sorry, we are unable to provide the full text but you may find it at the following location(s):
  • http://arxiv.org/abs/1102.4056 (external link)
  • Suggested articles


    To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.