On surface-symmetric spacetimes with collisionless and charged matter

dc.creatorTchapnda, Sophonie Blaise
dc.date2006-07-31
dc.date2006-12-21
dc.date.accessioned2026-07-07T11:26:26Z
dc.date.available2026-07-07T11:26:26Z
dc.descriptionSome future global properties of cosmological solutions for the Einstein-Vlasov-Maxwell system with surface symmetry are presented. Global existence is proved, the homogeneous spacetimes are future complete for causal trajectories, and the same is true for inhomogeneous plane-symmetric solutions with small initial data. In the latter case some decay properties are also obtained at late times. Similar but slightly weaker results hold for hyperbolic symmetry.
dc.description34 pages, version to be published in AHP
dc.identifierhttps://arxiv.org/abs/gr-qc/0607140
dc.identifierhttp://arxiv.org/abs/gr-qc/0607140
dc.identifierAnnalesHenriPoincare8:1221-1253,2007
dc.identifierdoi:10.1007/s00023-007-0333-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195825
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn surface-symmetric spacetimes with collisionless and charged matter
dc.typetext

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