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arXiv · hep-th/0606213

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

Z. W. Chong·M. Cvetic·H. Lu·C. N. Pope
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Abstract

Supersymmetric black holes in five-dimensional gauged supergravity must necessarily be rotating, and so in order to study the passage to black holes away from supersymmetry, it is of great interest to obtain non-extremal black holes that again have non-zero rotation. In this paper we find a simple framework for describing non-extremal rotating black holes in five-dimensional gauged supergravities. Using this framework, we are able to construct a new solution, describing the general single-charge solution of N=2 gauged supergravity, with arbitrary values for the two rotation parameters. Previously-obtained solutions with two or three equal charges also assume a much simpler form in the new framework, as also does the general solution with three unequal charges in ungauged N=2 supergravity. We discuss the thermodynamics and BPS limit of the new single-charge solutions, and we discuss the separability of the Hamilton-Jacobi and Klein-Gordan equations in these backgrounds.

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Z. W. Chong, M. Cvetic, H. Lu, C. N. Pope. 2006-10-30. Non-Extremal Rotating Black Holes in Five-Dimensional Gauged Supergravity. https://doi.org/10.1016/j.physletb.2006.11.012

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