Rotating Einstein-Maxwell black holes in odd dimensions
Rhucha Deshpande, Oleg Lunin

TL;DR
This paper constructs higher-dimensional rotating Einstein-Maxwell black holes with Chern-Simons couplings, demonstrating explicit solutions in all odd dimensions and showing that the Klein-Gordon equation is separable on these backgrounds.
Contribution
It provides explicit solutions for rotating Einstein-Maxwell black holes in all odd dimensions with Chern-Simons couplings, extending known four-dimensional results.
Findings
Explicit geometries in all odd dimensions
Klein-Gordon equation is fully separable on these backgrounds
Generalization of higher-dimensional Kerr-Newman solutions
Abstract
To construct higher-dimensional counterparts of the Kerr-Newman black holes, we consider Einstein's equations sourced by a vector field and a negative cosmological constant. In contrast to the four-dimensional case, the Maxwell's equations are modified by sources generated by topological Chern-Simons couplings, the situation already encountered in the minimal five dimensional supergravity. After constructing explicit geometries in all odd dimensions, we demonstrate that the Klein-Gordon equation on the new backgrounds is fully separable.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Relativity and Gravitational Theory · Cosmology and Gravitation Theories
