Equilibrium Configuration of Black Holes and the Inverse Scattering Method

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dc.creatorVarzugin, G. G.
dc.date2000-04-24
dc.date.accessioned2026-07-07T11:34:18Z
dc.date.available2026-07-07T11:34:18Z
dc.descriptionThe inverse scattering method is applied to the investigation of the equilibrium configuration of black holes. A study of the boundary problem corresponding to this configuration shows that any axially symmetric, stationary solution of the Einstein equations with disconnected event horizon must belong to the class of Belinskii-Zakharov solutions. Relationships between the angular momenta and angular velocities of black holes are derived.
dc.descriptionLaTeX, 14 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0004073
dc.identifierhttp://arxiv.org/abs/gr-qc/0004073
dc.identifierTheor.Math.Phys.111:667,1997; Teor.Mat.Fiz.111:345-355,1997
dc.identifierdoi:10.1007/BF02634055
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198202
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEquilibrium Configuration of Black Holes and the Inverse Scattering Method
dc.typetext

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