The Kerr-Newman-Godel Black Hole

Details The Kerr-Newman-Godel Black Hole The Kerr-Newman-Godel Black Hole

2003-07-20

arxiv.org/abs/hep-th/0307194v2

Class.Quant.Grav. 20 (2003) 4891-4900

Physics

High Energy Physics

High Energy Physics - Theory

12 pages, LaTeX, no figures; v2: one reference added, very minor changes; to appear in CQG

Scientific paper

10.1088/0264-9381/20/22/013

By applying a set of Hassan-Sen transformations and string dualities to the Kerr-Godel 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-Godel. In a particular extremal limit the solution describes an asymptotically Godel BMPV black hole.

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