Sequences of extremal radially excited rotating black holes

Abstract

In Einstein-Maxwell-Chern-Simons theory the extremal Reissner-Nordström solution is no longer the single extremal solution with vanishing angular momentum, when the Chern-Simons coupling constant reaches a critical value. Instead a whole sequence of rotating extremal J=0 solutions arises, labeled by the node number of the magnetic U(1) potential. Associated with the same near horizon solution, the mass of these radially excited extremal solutions converges to the mass of the extremal Reissner-Nordström solution. On the other hand, not all near horizon solutions are also realized as global solutions

5 pages, 6 figures

References in corpus (4)

• Charged Rotating Black Holes in Odd Dimensions
• Near-horizon geometries of supersymmetric AdS(5) black holes
• Extremal dyonic black holes in D=4 Gauss-Bonnet gravity
• Charges from Attractors

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• Supersymmetric rotating black hole spacetime tested by geodesics
• Charged rotating black holes in Einstein--Maxwell--Chern-Simons theory with a negative cosmological constant
• Radially excited rotating black holes in Einstein-Maxwell-Chern-Simons theory
• Angular momentum-area proportionality of extremal charged black holes in odd dimensions
• Einstein-Maxwell-Chern-Simons Black Holes
• Spinning extremal dyonic black holes in $\gamma =1$ Einstein-Maxwell-dilaton theory
• Extremal rotating black holes in Einstein-Maxwell-Chern-Simons theory: radially excited solutions and non-uniqueness
• Radially Excited AdS${}_5$ Black Holes in Einstein--Maxwell--Chern--Simons Theory