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Radially Excited AdS Black Holes in Einstein--Maxwell--Chern--Simons Theory
In the large coupling regime of the 5-dimensional
Einstein--Maxwell--Chern--Simons theory, charged and rotating cohomogeneity-1
black holes form sequences of extremal and non-extremal radially excited
configurations. These asymptotically global Anti-de Sitter (AdS) black
holes form a discrete set of solutions, characterised by the vanishing of the
total angular momenta, or the horizon angular velocity. However, the solutions
are not static. In this paper, we study the branch structure that contains
these excited states, and its relation with the static Reissner-Nordstr\"om-AdS
black hole. Thermodynamic properties of these solutions are considered,
revealing that the branches with lower excitation number can become
thermodynamically unstable beyond certain critical solutions that depend on the
free parameters of the configuration.Comment: 18 pages, 9 figures, invited paper for the "Entropy" special issue
"Geometry in Thermodynamics II", editor George Ruppeine
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