The Schwarzschild-de Sitter solution in five-dimensional general relativity briefly revisited

dc.creatorFonseca-Neto, J. B.
dc.creatorRomero, C.
dc.date2007-03-20
dc.date.accessioned2026-07-07T11:21:54Z
dc.date.available2026-07-07T11:21:54Z
dc.descriptionWe briefly revisit the Schwarzschild-de Sitter solution in the context of five-dimensional general relativity. We obtain a class of five-dimensional solutions of Einstein vacuum field equations into which the four-dimensional Schwarzschild-de Sitter space can be locally and isometrically embedded. We show that this class of solutions is well-behaved in the limit of lambda approaching zero. Applying the same procedure to the de Sitter cosmological model in five dimensions we obtain a class of embedding spaces which are similarly well-behaved in this limit. These examples demonstrate that the presence of a non-zero cosmological constant does not in general impose a rigid relation between the (3+1) and (4+1)-dimensional spacetimes, with degenerate limiting behaviour.
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0703103
dc.identifierhttp://arxiv.org/abs/gr-qc/0703103
dc.identifierClass.Quant.Grav.24:3515-3520,2007
dc.identifierdoi:10.1088/0264-9381/24/13/N01
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194402
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Schwarzschild-de Sitter solution in five-dimensional general relativity briefly revisited
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