Solar models and neutrino deficit

Simple item page
dc.creatorConforto, G.
dc.creatorGrimani, C.
dc.creatorMartelli, F.
dc.creatorVetrano, F.
dc.date1998-07-09
dc.date.accessioned2026-07-07T04:04:15Z
dc.date.available2026-07-07T04:04:15Z
dc.descriptionThe existing measurements of the solar neutrino flux are compared with the predictions of all models capable of reproducing the other solar observables. These predictions are supplemented by the hypothesis of neutrino oscillations with mass differences large enough to render energy-independent the depletion of the solar nu(e) flux. It is concluded that the data are consistent with this hypothesis and that an energy-dependence of the solar neutrino deficit must be regarded as an attractive possibility but not as a compelling reality.
dc.description9 pages, 2 figures, contributed paper to the XVIII Int. Conf. on Neutrino Physics and Astrophysics, Takayama, Japan, 4-9 June 1998
dc.identifierhttps://arxiv.org/abs/hep-ph/9807306
dc.identifierhttp://arxiv.org/abs/hep-ph/9807306
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48016
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolar models and neutrino deficit
dc.typetext

Files

Collections

arXiv