Coalescence of Rotating Black Holes on Eguchi-Hanson Space

Abstract

We obtain new charged rotating multi-black hole solutions on the Eguchi-Hanson space in the five-dimensional Einstein-Maxwell system with a Chern-Simons term and a positive cosmological constant. In the two-black holes case, these solutions describe the coalescence of two rotating black holes with the spatial topologies of S^3 into a single rotating black hole with the spatial topology of the lens space S^3/Z_2. We discuss the differences in the horizon areas between our solutions and the two-centered Klemm-Sabra solutions which describe the coalescence of two rotating black holes with the spatial topologies of S^3 into a single rotating black hole with the spatial topology of S^3.

20 pages, 9 figures

References in corpus (7)

• Rotating Black Holes at Future Colliders. III. Determination of Black Hole Evolution
• A Rotating Kaluza-Klein Black Hole with Squashed Horizons
• Black Holes on Eguchi-Hanson Space in Five-Dimensional Einstein-Maxwell Theory
• Dilaton black holes with squashed horizons and their thermodynamics
• Topology Change of Coalescing Black Holes on Eguchi-Hanson Space
• Kaluza-Klein black holes with squashed horizons and $d=4$ superposed monopoles
• Cosmological Black Holes on Taub-NUT space in Five-Dimensional Einstein-Maxwell Theory

Cited by in corpus (9)

• Evolution of perturbations of squashed Kaluza-Klein black holes: escape from instability
• Charged Rotating Kaluza-Klein Black Holes in Five Dimensions
• Charged Black Holes in a Rotating Gross-Perry-Sorkin Monopole Background
• Charged Rotating Kaluza-Klein Black Holes Generated by G2(2) Transformation
• Cosmological rotating black holes in five-dimensional fake supergravity
• Multi-Black Rings on Eguchi-Hanson Space
• Stability analysis of Squashed Kaluza-Klein Black Holes with Charge
• Charged Black Holes in a Five-dimensional Kaluza-Klein Universe
• NUT Solutions in Einstein-Maxwell-scalar-Gauss-Bonnet Gravity