Solar Neutrino Decay

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dc.creatorAcker, Andy
dc.creatorPakvasa, Sandip
dc.date1993-10-01
dc.date.accessioned2026-07-07T13:02:37Z
dc.date.available2026-07-07T13:02:37Z
dc.descriptionWe re-examine the neutrino decay solution to the solar neutrino problem in light of the new data from Gallex II and Kamiokande III. We compare the experimental data with the solar models of Bahcall and Pinsonneault and Turck-Chieze and find that neutrino decay is ruled out as a solution to the solar neutrino problem at better than the 98\% c.l. even when solar model uncertainties are taken into account.
dc.description10 pages, UH-511-774-93
dc.identifierhttps://arxiv.org/abs/hep-ph/9310207
dc.identifierhttp://arxiv.org/abs/hep-ph/9310207
dc.identifierPhys.Lett.B320:320-322,1994
dc.identifierdoi:10.1016/0370-2693(94)90663-7
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226509
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolar Neutrino Decay
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