On the parameters of the Kerr-NUT-(anti-)de Sitter space-time

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dc.creatorGriffiths, J. B.
dc.creatorPodolsky, J.
dc.date2007-02-07
dc.date.accessioned2026-07-07T11:21:44Z
dc.date.available2026-07-07T11:21:44Z
dc.descriptionDifferent forms of the metric for the Kerr-NUT-(anti-)de Sitter space-time are being widely used in its extension to higher dimensions. The purpose of this note is to relate the parameters that are being used to the physical parameters (mass, rotation, NUT and cosmological constant) in the basic four dimensional situation.
dc.description4 pages. To appear as a Note in Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/gr-qc/0702042
dc.identifierhttp://arxiv.org/abs/gr-qc/0702042
dc.identifierClass.Quant.Grav.24:1687-1690,2007
dc.identifierdoi:10.1088/0264-9381/24/6/N02
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194348
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleOn the parameters of the Kerr-NUT-(anti-)de Sitter space-time
dc.typetext

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