Vector field theories in cosmology

dc.creatorTartaglia, A.
dc.creatorRadicella, N.
dc.date2007-08-05
dc.date.accessioned2026-07-07T11:18:25Z
dc.date.available2026-07-07T11:18:25Z
dc.descriptionRecently proposed theories based on the cosmic presence of a vectorial field are compared and contrasted. In particular the so called Einstein aether theory is discussed in parallel with a recent proposal of a strained space-time theory (Cosmic Defect theory). We show that the latter fits reasonably well the cosmic observed data with only one, or at most two, adjustable parameters, whilst other vector theories use much more. The Newtonian limits are also compared. Finally we show that the CD theory may be considered as a special case of the aether theories, corresponding to a more compact and consistent paradigm.
dc.description19 pages, 1 figure, to appear on Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0708.0675
dc.identifierhttp://arxiv.org/abs/0708.0675
dc.identifierPhys.Rev.D76:083501,2007
dc.identifierdoi:10.1103/PhysRevD.76.083501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193339
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleVector field theories in cosmology
dc.typetext

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