Dark Energy and Neutrino Model in SUSY

dc.creatorTakahashi, Ryo
dc.creatorTanimoto, Morimitsu
dc.date2006-10-26
dc.date2006-10-30
dc.date.accessioned2026-07-07T10:25:48Z
dc.date.available2026-07-07T10:25:48Z
dc.descriptionWe discuss the effect of the supersymmetry breaking on the Mass Varying Neutrinos(MaVaNs) scenario. Especially, the effect mediated by the gravitational interaction between the hidden sector and the dark energy sector is studied. A model including a chiral superfield in the dark sector and the right-handed neutrino superfield is proposed. Evolutions of the neutrino mass and the equation of state parameter are presented in the model.
dc.description4 pages, 3 figures, comments added, to appear in Proceedings of SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006
dc.identifierhttps://arxiv.org/abs/hep-ph/0610347
dc.identifierhttp://arxiv.org/abs/hep-ph/0610347
dc.identifierAIPConf.Proc.903:656-659,2007
dc.identifierdoi:10.1063/1.2735269
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176663
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark Energy and Neutrino Model in SUSY
dc.typetext

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