Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data

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dc.creatorBarranco, J.
dc.creatorMiranda, O. G.
dc.creatorRashba, T. I.
dc.creatorSemikoz, V. B.
dc.creatorValle, J. W. F.
dc.date2002-07-26
dc.date2003-07-02
dc.date.accessioned2026-07-07T10:33:07Z
dc.date.available2026-07-07T10:33:07Z
dc.descriptionWe show that spin flavor precession solutions to the solar neutrino problem, although preferred by the latest solar data, are ruled out by the first results from the KamLAND reactor experiment, at more than 3_sigma. An illustrative chi2 plot comparing these descriptions with oscillations is given.
dc.descriptionnew appendix added discussing the impact of the KamLAND data. This updates the one published in Phys.Rev.D66:093009,2002
dc.identifierhttps://arxiv.org/abs/hep-ph/0207326
dc.identifierhttp://arxiv.org/abs/hep-ph/0207326
dc.identifierPhys.Rev.D66:093009,2002
dc.identifierdoi:10.1103/PhysRevD.66.093009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178996
dc.subjectHigh Energy Physics - Phenomenology
dc.titleConfronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data
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