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Exact solutions for supersymmetric stationary black hole composites

Brandon Bates
(
- Columbia U.
)
,
Frederik Denef
(
- Rutgers U., Piscataway
)

Apr, 2003

13 pages

Published in:

JHEP 11 (2011) 127

e-Print:

hep-th/0304094 [hep-th]

DOI:

10.1007/JHEP11(2011)127

Report number:

RUNHETC-2003-10

View in:

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Abstract:

Four dimensional N=2 supergravity has regular, stationary, asymptotically flat BPS solutions with intrinsic angular momentum, describing bound states of separate extremal black holes with mutually nonlocal charges. Though the existence and some properties of these solutions were established some time ago, fully explicit analytic solutions were lacking thus far. In this note, we fill this gap. We show in general that explicit solutions can be constructed whenever an explicit formula is known in the theory at hand for the Bekenstein-Hawking entropy of a single black hole as a function of its charges, and illustrate this with some simple examples. We also give an example of moduli-dependent black hole entropy.

Note:

13 pages, 1 figure

black hole: bound state
bound state: BPS
supergravity
black hole: entropy
charge: nonlocal
field equations: solution
moduli: dependence

References(18)

Figures(0)

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