Resonant Spin-Flavor Precession of Neutrinos As a Possible Solution to the Solar Neutrino Problem

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dc.creatorAkhmedov, Eugeni
dc.date1992-05-29
dc.date.accessioned2026-07-07T03:55:36Z
dc.date.available2026-07-07T03:55:36Z
dc.descriptionRecent developments of the resonant neutrino spin-flavor precession scenario and its applications to the solar neutrino problem are reviewed. We discuss in particular the possibilities of reconciliation of strong time variations of the solar neutrino flux observed in the Homestake ${}^{37}\$Cl experiment with little or no time variation seen in the Kamiokande II experiment.
dc.description12 pages, 1 figure (not included), SISSA-49/92/EP
dc.identifierhttps://arxiv.org/abs/hep-ph/9205244
dc.identifierhttp://arxiv.org/abs/hep-ph/9205244
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44616
dc.subjectHigh Energy Physics - Phenomenology
dc.titleResonant Spin-Flavor Precession of Neutrinos As a Possible Solution to the Solar Neutrino Problem
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