Radial excitations of non-static $J=0$ black holes in Einstein-Maxwell-Chern-Simons gravity
General Relativity and Quantum Cosmology
2017-11-21 v1
Abstract
We study the generalization of the Kerr-Newmann black hole in 5D Einstein-Maxwell-Chern-Simons theory with free Chern-Simons coupling parameter. These black holes possess equal magnitude angular momenta and an event horizon of spherical topology. We focus on the extremal case with zero temperature. We find that, when the Chern-Simons coupling is greater than two times the supergravity case, new branches of black holes are found which violate uniqueness. In particular, a sequence of these black holes are non-static radially excited solutions with vanishing angular momentum. They approach the Reissner-Nordstr\"om solution as the excitation level increases.
Keywords
Cite
@article{arxiv.1602.00822,
title = {Radial excitations of non-static $J=0$ black holes in Einstein-Maxwell-Chern-Simons gravity},
author = {Jose Luis Blázquez-Salcedo and Jutta Kunz and Francisco Navarro-Lérida and Eugen Radu},
journal= {arXiv preprint arXiv:1602.00822},
year = {2017}
}
Comments
6 pages, 2 figures