Black hole masking and black hole thermodynamics

Details Black hole masking and black hole thermodynamics Black hole masking and black hole thermodynamics

2011-02-20

arxiv.org/abs/1102.4056v1

Grav.Cosmol.17:276-279,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages. To appear in Gravitation and Cosmology

Scientific paper

10.1134/S020228931103011X

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.

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