Late-time oscillatory behaviour for self-gravitating scalar fields

dc.creatorRendall, Alan D.
dc.date2006-11-16
dc.date2006-11-27
dc.date.accessioned2026-07-07T10:22:01Z
dc.date.available2026-07-07T10:22:01Z
dc.descriptionThis paper investigates the late-time behaviour of certain cosmological models where oscillations play an essential role. Rigorous results are proved on the asymptotics of homogeneous and isotropic spacetimes with a linear massive scalar field as source. Various generalizations are obtained for nonlinear massive scalar fields, $k$-essence models and $f(R)$ gravity. The effect of adding ordinary matter is discussed as is the case of nonlinear scalar fields whose potential has a degenerate zero.
dc.description17 pages, additional references
dc.identifierhttps://arxiv.org/abs/gr-qc/0611088
dc.identifierhttp://arxiv.org/abs/gr-qc/0611088
dc.identifierClass.Quant.Grav.24:667-678,2007
dc.identifierdoi:10.1088/0264-9381/24/3/010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175369
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleLate-time oscillatory behaviour for self-gravitating scalar fields
dc.typetext

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