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Updated: Aug 9, 2026

Generation and Coherent Control of Pulsed Quantum Frequency Combs
Published on: June 8, 2018
D = 5 Einstein-Maxwell-Chern-Simons black holes
Jutta Kunz1, Francisco Navarro-Lérida
1Institut für Physik, Universität Oldenburg, Postfach 2503, D-26111 Oldenburg, Germany.
Abstract:
Five-dimensional Einstein-Maxwell-Chern-Simons theory with a Chern-Simons coefficient lambda = 1 has supersymmetric black holes with a 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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