General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity

Details General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity

2005-06-02

arxiv.org/abs/hep-th/0506029v1

Phys.Rev.Lett.95:161301,2005

Physics

High Energy Physics

High Energy Physics - Theory

revtex, 4 pages

Scientific paper

10.1103/PhysRevLett.95.161301

We construct the general solution for non-extremal charged rotating black holes in five-dimensional minimal gauged supergravity. They are characterised by four non-trivial parameters, namely the mass, the charge, and the two independent rotation parameters. The metrics in general describe regular rotating black holes, providing the parameters lie in appropriate ranges so that naked singularities and closed timelike curves (CTC's) are avoided. We calculate the conserved energy, angular momenta and charge for the solutions, and show how supersymmetric solutions arise in a BPS limit. These have naked CTC's in general, but for special choices of the parameters we obtain new regular supersymmetric black holes or smooth topological solitons.

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