D=5 Einstein-Maxwell-Chern-Simons Black Holes

Details D=5 Einstein-Maxwell-Chern-Simons Black Holes D=5 Einstein-Maxwell-Chern-Simons Black Holes

2005-10-28

arxiv.org/abs/hep-th/0510250v1

Phys.Rev.Lett. 96 (2006) 081101

Physics

High Energy Physics

High Energy Physics - Theory

4 pages, 4 figures, RevTeX style

Scientific paper

10.1103/PhysRevLett.96.081101

5-dimensional Einstein-Maxwell-Chern-Simons theory with Chern-Simons coefficient $\lambda=1$ has supersymmetric black holes with vanishing horizon angular velocity, but finite angular momentum. Here supersymmetry is associated with a borderline between stability and instability, since for $\lambda>1$ a rotational instability arises, where counterrotating black holes appear, whose horizon rotates in the opposite sense to the angular momentum. For $\lambda>2$ black holes are no longer uniquely characterized by their global charges, and rotating black holes with vanishing angular momentum appear.

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