The causal boundary of product spacetimes

dc.creatorAlana, V.
dc.creatorFlores, J. L.
dc.date2007-04-24
dc.date2007-04-25
dc.date.accessioned2026-07-07T11:20:22Z
dc.date.available2026-07-07T11:20:22Z
dc.descriptionThe new formulation of the causal completion of spacetimes suggested in [1], and modified later in [2], is tested by computing the causal boundary for product spacetimes of a Lorentz interval and a Riemannian manifold. This is particularized for two important families of spacetimes, conformal to the previous ones: (standard) static spacetimes and Generalized Robertson-Walker spacetimes. As consequence, it is shown that this new approach essentially reproduces the structure of the conformal boundary for multiple classical spacetimes: Reissner-Nordstrom (including Schwarzschild), Anti-de Sitter, Taub and standard cosmological models as de Sitter and Einstein Universe.
dc.description21 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/0704.3148
dc.identifierhttp://arxiv.org/abs/0704.3148
dc.identifierGen.Rel.Grav.39:1697-1718,2007
dc.identifierdoi:10.1007/s10714-007-0492-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193940
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe causal boundary of product spacetimes
dc.typetext

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