Non-singular Stiff Fluids

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dc.creatorFernández-Jambrina, L.
dc.creatorGonzález-Romero, L. M.
dc.date2009-04-08
dc.date.accessioned2026-07-07T13:01:44Z
dc.date.available2026-07-07T13:01:44Z
dc.descriptionIn this talk the possibility of constructing geodesically complete inhomogeneous stiff fluid cosmologies is discussed. A family with infinite parameters is derived. A wide and easy to implement sufficient condition for geodesic completeness is shown.
dc.description4 pp, ws-procs
dc.identifierhttps://arxiv.org/abs/0904.1359
dc.identifierhttp://arxiv.org/abs/0904.1359
dc.identifierProceedings of the Tenth Marcel Grossmann Meeting on General Relativity. Ed: M. Novello, S. Perez Bergliaffa. World Scientific, Singapore, 1764-6 (2006)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226245
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNon-singular Stiff Fluids
dc.typetext

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