Strong cosmic censorship for T^2-symmetric spacetimes with cosmological constant and matter

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dc.creatorSmulevici, Jacques
dc.date2007-10-06
dc.date2009-04-07
dc.date.accessioned2026-07-07T13:00:28Z
dc.date.available2026-07-07T13:00:28Z
dc.descriptionWe address the issue of strong cosmic censorship for T^2-symmetric spacetimes with positive cosmological constant. In the case of collisionless matter, we complete the proof of the C^2 formulation of the conjecture for this class of spacetimes. In the vacuum case, we prove that the conjecture holds for the special cases where the area element of the group orbits does not vanish on the past boundary of the maximal Cauchy development.
dc.description29 pages, 6 figures, v2 is the version published in Annales Henri Poincare
dc.identifierhttps://arxiv.org/abs/0710.1351
dc.identifierhttp://arxiv.org/abs/0710.1351
dc.identifierAnnalesHenriPoincare9:1425-1453,2008
dc.identifierdoi:10.1007/s00023-008-0391-7
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/225848
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAnalysis of PDEs
dc.subjectDifferential Geometry
dc.titleStrong cosmic censorship for T^2-symmetric spacetimes with cosmological constant and matter
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