Maximal neutrino oscillation solution to the solar neutrino problem

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dc.creatorFoot, R.
dc.creatorVolkas, R. R.
dc.date1995-10-17
dc.date.accessioned2026-07-07T03:58:20Z
dc.date.available2026-07-07T03:58:20Z
dc.descriptionWe discuss a simple predictive solution to the solar neutrino problem based on maximal vacuum neutrino oscillations. The solution can be motivated by the exact parity symmetric model which predicts that the neutrino mass eigenstates are maximal mixtures of ordinary and mirror weak eigenstates (if neutrinos are massive). We show that this proposed solution to the solar neutrino problem is in reasonable agreement with the experiments, and that in the near future this scheme may be either ruled out or tested more precisely as statistics improve for the SAGE and GALLEX experiments. Predictions are also given for the upcoming Superkamiokande, SNO and Borexino experiments.
dc.description12 pages, LaTeX, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9510312
dc.identifierhttp://arxiv.org/abs/hep-ph/9510312
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45772
dc.subjectHigh Energy Physics - Phenomenology
dc.titleMaximal neutrino oscillation solution to the solar neutrino problem
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