Instability of charged black holes in Anti-de Sitter space - INSPIRE

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Instability of charged black holes in Anti-de Sitter space

Steven S. Gubser
(
- Princeton U.
)
,
Indrajit Mitra
(
- Princeton U.
)

Sep, 2000

6 pages

Part of Strings 2001: Proceedings, Strings 2001 Conference, Tata Institute of Fundamental Research, Mumbai, India, January 5-10, 2001, 221

Published in:

Clay Math.Proc. 1 (2002) 221

Contribution to:

Strings 2001: International Conference, 221

e-Print:

hep-th/0009126 [hep-th]

Report number:

PUPT-1953

View in:

ADS Abstract Service

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Abstract:

We exhibit a tachyonic mode in a linearized analysis of perturbations of large anti-de Sitter Reissner-Nordstrom black holes in four dimensions. In the large black hole limit, and up to a 0.7% discrepancy which is probably round-off error in the numerical analysis, the tachyon appears precisely when the black hole becomes thermodynamically unstable.

black hole: Reissner-Nordstroem
space-time: anti-de Sitter
tachyon
perturbation theory: linear
field theory: conformal
black hole: stability

References(27)

Figures(0)

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