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The Kerr–Newman–Gödel black hole

C A R Herdeiro

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By applying a set of Hassan–Sen transformations and string dualities to the Kerr–Gödel solution of minimal D = 5 supergravity we derive a four-parameter family of five-dimensional solutions in type II string theory. They describe rotating, charged black holes in a rotating background. For zero background rotation, the solution is D = 5 Kerr–Newman; for zero charge it is Kerr–Gödel. In a particular extremal limit the solution describes an asymptotically Gödel BMPV black hole.


PACS

04.70.-s Physics of black holes

04.65.+e Supergravity

11.25.Tq Gauge/string duality

04.50.-h Higher-dimensional gravity and other theories of gravity

MSC

83E50 Supergravity

83C57 Black holes

83E30 String and superstring theories (See also 81T30)

Subjects

Gravitation and cosmology

Particle physics and field theory

Dates

Issue 22 (21 November 2003)

Received 13 August 2003

Published 6 October 2003



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