The Yamabe invariant for axially symmetric two Kerr black holes initial data

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dc.creatorAvila, Gastón A.
dc.creatorDain, Sergio
dc.date2008-05-18
dc.date.accessioned2026-07-07T11:50:53Z
dc.date.available2026-07-07T11:50:53Z
dc.descriptionAn explicit 3-dimensional Riemannian metric is constructed which can be interpreted as the (conformal) sum of two Kerr black holes with aligned angular momentum. When the separation distance between them is large we prove that this metric has positive Ricci scalar and hence positive Yamabe invariant. This metric can be used to construct axially symmetric initial data for two Kerr black holes with large angular momentum.
dc.description14 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0805.2754
dc.identifierhttp://arxiv.org/abs/0805.2754
dc.identifierClass.Quant.Grav.25:225002,2008
dc.identifierdoi:10.1088/0264-9381/25/22/225002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203712
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Yamabe invariant for axially symmetric two Kerr black holes initial data
dc.typetext

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