Some Properties of a New Solution of the Ernst Equation

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dc.creatorGariel, J.
dc.creatorMarcilhacy, G.
dc.creatorSantos, N. O.
dc.date2001-09-25
dc.date.accessioned2026-07-07T11:46:17Z
dc.date.available2026-07-07T11:46:17Z
dc.descriptionFrom a particularly simple solution of the Ernst equation, we build a solution of the vacuum stationary axisymmetric Einstein equations depending on three parameters. The parameters are associated to the total mass of the source and its angular momentum. The third parameter produces a topological deformation of the ergosphere making it a two-sheet surface, and for some of its values forbids the Penrose process.
dc.description17 pages, LaTeX, 10 EPS figures, uses graficx.sty
dc.identifierhttps://arxiv.org/abs/gr-qc/0109086
dc.identifierhttp://arxiv.org/abs/gr-qc/0109086
dc.identifierClass.Quant.Grav.19:2157-2170,2002
dc.identifierdoi:10.1088/0264-9381/19/8/307
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202174
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSome Properties of a New Solution of the Ernst Equation
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