Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos

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dc.creatorBi, Xiao-Jun
dc.creatorFeng, Bo
dc.creatorLi, Hong
dc.creatorZhang, Xinmin
dc.date2004-12-01
dc.date2005-11-02
dc.date.accessioned2026-07-07T06:38:16Z
dc.date.available2026-07-07T06:38:16Z
dc.descriptionIn this paper we consider the cosmological implications of dark energy models with a coupled system of a dynamical scalar field (the quintessence) and the neutrinos. By detailed numerical calculations we study the various possibilities on the evolution and the fates of the universe in this class of models. Our results show that due to the interaction with quintessence, neutrinos could be dominant over the quintessence in the future universe, however would eventually decay away.
dc.descriptionOne typographical error corrected, references updated and presentation improved
dc.identifierhttps://arxiv.org/abs/hep-ph/0412002
dc.identifierhttp://arxiv.org/abs/hep-ph/0412002
dc.identifierPhys.Rev. D72 (2005) 123523
dc.identifierdoi:10.1103/PhysRevD.72.123523
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/100679
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Theory
dc.titleCosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
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