A pair of extremal charged black holes on Kerr-Taub-bolt space
arXiv:1504.04203 · doi:10.1088/0264-9381/32/21/215008
Abstract
We construct asymptotically Kaluza-Klein solutions in five-dimensional Einstein-Maxwell theory which represent a pair of extremal, charged, static black holes on Kerr-Taub-bolt space. Regularity conditions require that the topology of spatial infinity and that of each black hole are not S, but different lens spaces. We show that for a given topology at spatial infinity, there are an infinite number of different horizon topologies for the black hole pair. We briefly discuss a generalization to the case with a positive cosmological constant.
24 pages, 7 figures
References in corpus (13)
- A supersymmetric black lens
- Kaluza-Klein Multi-Black Holes in Five-Dimensional Einstein-Maxwell Theory
- Black Holes on Eguchi-Hanson Space in Five-Dimensional Einstein-Maxwell Theory
- Topology Change of Coalescing Black Holes on Eguchi-Hanson Space
- On the smoothness of static multi-black hole solutions of higher-dimensional Einstein-Maxwell theory
- The Disjointed Thermodynamics of Rotating Black Holes With a NUT Twist
- Coalescence of Rotating Black Holes on Eguchi-Hanson Space
- Charged black holes on a Kaluza-Klein bubble
- Charged rotating Kaluza-Klein multi-black holes and multi-black strings in five-dimensional Einstein-Maxwell theory
- Analyticity of Event Horizons of Five-Dimensional Multi-Black Holes with Non-Trivial Asymptotic Structure
- Charged Black Holes in a Five-dimensional Kaluza-Klein Universe
- Supersymmetric Rotating Black Hole in a Compactified Spacetime
- A simple diagnosis of non-smoothness of black hole horizon: Curvature singularity at horizons in extremal Kaluza-Klein black holes