Coalescence of Rotating Black Holes on Eguchi-Hanson Space

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dc.creatorMatsuno, Ken
dc.creatorIshihara, Hideki
dc.creatorKimura, Masashi
dc.creatorTomizawa, Shinya
dc.date2007-07-12
dc.date.accessioned2026-07-07T12:04:39Z
dc.date.available2026-07-07T12:04:39Z
dc.descriptionWe 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.
dc.description20 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/0707.1757
dc.identifierhttp://arxiv.org/abs/0707.1757
dc.identifierPhys.Rev.D76:104037,2007
dc.identifierdoi:10.1103/PhysRevD.76.104037
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/208163
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCoalescence of Rotating Black Holes on Eguchi-Hanson Space
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