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

Jutta Kunz·Francisco Navarro-Lerida
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Abstract

5-dimensional Einstein-Maxwell-Chern-Simons theory with Chern-Simons coefficient $λ=1$ 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 $λ>1$ a rotational instability arises, where counterrotating black holes appear, whose horizon rotates in the opposite sense to the angular momentum. For $λ>2$ black holes are no longer uniquely characterized by their global charges, and rotating black holes with vanishing angular momentum appear.

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Jutta Kunz, Francisco Navarro-Lerida. 2005-10-28. D=5 Einstein-Maxwell-Chern-Simons Black Holes. https://doi.org/10.1103/physrevlett.96.081101

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