Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory - INSPIRE

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Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory

L.J. Romans
(
- Caltech, JPL
)

Aug, 1991

21 pages

Published in:

Nucl.Phys.B 383 (1992) 395-415

Published: 1992

e-Print:

hep-th/9203018 [hep-th]

DOI:

10.1016/0550-3213(92)90684-4

Report number:

PRINT-92-0114 (JPL,CAL-TECH)

View in:

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Abstract:

In flat space, the extreme Reissner-Nordstr\o m (RN) black hole is distinguished by its coldness (vanishing Hawking temperature) and its supersymmetry. We examine RN solutions to Einstein-Maxwell theory with a cosmological constant

\Lambda

, classifying the cold black holes and, for positive

\Lambda

, the ``lukewarm" black holes at the same temperature as the de Sitter thermal background. For negative

\Lambda

, we classify the supersymmetric solutions within the context of

N=2

gauged supergravity. One finds supersymmetric analogues of flat-space extreme RN black holes, which for nonzero

\Lambda

differ from the cold black holes. In addition, there is an exotic class of supersymmetric solutions which cannot be continued to flat space, since the magnetic charge becomes infinite in that limit.

Einstein-Maxwell equation: solution
black hole
supersymmetry
thermodynamics

References(43)

Figures(0)

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