Neutrino Oscillations and the Solar Neutrino Problem

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dc.creatorHaxton, W. C.
dc.date2000-04-23
dc.date2000-04-28
dc.date.accessioned2026-07-07T05:38:02Z
dc.date.available2026-07-07T05:38:02Z
dc.descriptionI describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications of current experiments -- including the SuperKamiokande atmospheric and LSND measurements -- and the need for additional constraints from SNO and other new detectors.
dc.descriptionReference corrected in this replacement
dc.identifierhttps://arxiv.org/abs/nucl-th/0004052
dc.identifierhttp://arxiv.org/abs/nucl-th/0004052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/81482
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino Oscillations and the Solar Neutrino Problem
dc.typetext

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