Left-Right Symmetric Model of Neutrino Dark Energy

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dc.creatorBhatt, Jitesh R.
dc.creatorGu, Pei-Hong
dc.creatorSarkar, Utpal
dc.creatorSingh, Santosh K.
dc.date2007-11-18
dc.date2008-04-02
dc.date.accessioned2026-07-07T11:54:15Z
dc.date.available2026-07-07T11:54:15Z
dc.descriptionWe implemented the neutrino dark energy proposal in a left-right symmetric model. Unlike earlier models of mass varying neutrinos, in the present model the mass parameter that depends on the scalar field (acceleron) remains very light naturally. The required neutrino masses then predicts the U(1)_R breaking scale to be in the TeV range, providing new signals for LHC. Compared to all other neutrino dark energy proposals, this model has the added advantage that it can also be embedded into a grand unified theory. In this scenario leptogenesis occurs through decays of scalars at very high energy.
dc.description4 pages. Revised version. Accepted by PLB
dc.identifierhttps://arxiv.org/abs/0711.2728
dc.identifierhttp://arxiv.org/abs/0711.2728
dc.identifierPhys.Lett.B663:83-85,2008
dc.identifierdoi:10.1016/j.physletb.2008.03.059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204829
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLeft-Right Symmetric Model of Neutrino Dark Energy
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