Local temperature for dynamical black holes

Details Local temperature for dynamical black holes Local temperature for dynamical black holes

2008-12-13

arxiv.org/abs/0812.2534v1

AIP Conf.Proc.1122:145-151,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, contribution to Proceedings of ERE2008

Scientific paper

10.1063/1.3141237

A local Hawking temperature was recently derived for any future outer trapping horizon in spherical symmetry, using a Hamilton-Jacobi tunneling method, and is given by a dynamical surface gravity as defined geometrically. Descriptions are given of the operational meaning of the temperature, in terms of what observers measure, and its relation to the usual Hawking temperature for static black holes. Implications for the final fate of an evaporating black hole are discussed.

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