Solar mass-varying neutrino oscillations

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dc.creatorBarger, V.
dc.creatorHuber, Patrick
dc.creatorMarfatia, Danny
dc.date2005-02-21
dc.date2005-09-30
dc.date.accessioned2026-07-07T11:04:43Z
dc.date.available2026-07-07T11:04:43Z
dc.descriptionWe propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaVaNs). This scenario elucidates solar neutrino data beautifully while remaining comfortably compatible with atmospheric neutrino and K2K data and with reactor antineutrino data at short and long baselines (from CHOOZ and KamLAND). We find that the survival probability of solar MaVaNs is independent of how the suppression of neutrino mass caused by the acceleron-matter couplings varies with density. Measurements of MeV and lower energy solar neutrinos will provide a rigorous test of the idea.
dc.description4 pages, 3 figures. Version to appear in PRL
dc.identifierhttps://arxiv.org/abs/hep-ph/0502196
dc.identifierhttp://arxiv.org/abs/hep-ph/0502196
dc.identifierPhys.Rev.Lett.95:211802,2005
dc.identifierdoi:10.1103/PhysRevLett.95.211802
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188988
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Experiment
dc.subjectNuclear Experiment
dc.subjectNuclear Theory
dc.titleSolar mass-varying neutrino oscillations
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