Gravitational stability of inflatons and torsion in Einstein-Cartan-Klein-Gordon Cosmology

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dc.creatorde Andrade, L. C. Garcia
dc.date2002-01-14
dc.date.accessioned2026-07-07T04:12:58Z
dc.date.available2026-07-07T04:12:58Z
dc.descriptionGravitational stability of torsion and inflaton potential in a four-dimensional spacetime de Sitter solution in scalar-tensor cosmology where Cartan torsion propagates is investigated in detail. Inflaton and torsion evolution equations are derived by making use of a Lagrangean method. Stable and unstable modes for torsion and inflatons are found. Present astrophysical observations favour a stable mode for torsion since this would explain why no relic torsion imprint has been found on the Cosmic Background Radiation in the universe.
dc.descriptionLatex file
dc.identifierhttps://arxiv.org/abs/hep-th/0201082
dc.identifierhttp://arxiv.org/abs/hep-th/0201082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51091
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational stability of inflatons and torsion in Einstein-Cartan-Klein-Gordon Cosmology
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