Scaling attractors for quintessence in flat universe with cosmological term

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dc.creatorKiselev, V. V.
dc.date2006-11-13
dc.date2007-02-08
dc.date.accessioned2026-07-07T11:21:31Z
dc.date.available2026-07-07T11:21:31Z
dc.descriptionFor evolution of flat universe, we classify late time and future attractors with scaling behavior of scalar field quintessence in the case of potential, which, at definite values of its parameters and initial data, corresponds to exact scaling in the presence of cosmological constant.
dc.description11 pages, 16 eps-figures, revtex4, reference with comment added
dc.identifierhttps://arxiv.org/abs/gr-qc/0611064
dc.identifierhttp://arxiv.org/abs/gr-qc/0611064
dc.identifierJCAP0801:019,2008
dc.identifierdoi:10.1088/1475-7516/2008/01/019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194284
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleScaling attractors for quintessence in flat universe with cosmological term
dc.typetext

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