Hawking Evaporation Time Scale of Topological Black Holes in Anti-de Sitter Spacetime - INSPIRE

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Hawking Evaporation Time Scale of Topological Black Holes in Anti-de Sitter Spacetime

Yen Chin Ong
(
- Nordita and
- Royal Inst. Tech., Stockholm and
- Stockholm U.
)

Jul 28, 2015

13 pages

Published in:

Nucl.Phys.B 903 (2016) 387-399

Published: Feb, 2016

e-Print:

1507.07845 [gr-qc]

DOI:

10.1016/j.nuclphysb.2016.01.005

View in:

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Abstract: (Elsevier)

It was recently pointed out that if an absorbing boundary condition is imposed at infinity, an asymptotically anti-de Sitter Schwarzschild black hole with a spherical horizon takes only a finite amount of time to evaporate away even if its initial mass is arbitrarily large. We show that this is a rather generic property in AdS spacetimes: regardless of their horizon topologies, neutral AdS black holes in general relativity take about the same amount of time to evaporate down to the same size of order L , the AdS length scale. Our discussion focuses on the case in which the black hole has toral event horizon. A brief comment is made on the hyperbolic case, i.e. for black holes with negatively curved horizons.

Note:

Published version

space-time: anti-de Sitter
black hole: Schwarzschild
horizon: topology
boundary condition
general relativity
black hole: evaporation
curvature

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