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Time variation of the solar-neutrino flux and the resonant spin-flavor rotation mechanism

Abstract:

The recent observation at the Cl37 experiment suggests that the (anti) correlation between the solar-neutrino flux and the sunspot activity seems to be real. We analyze the characteristic features of the time variation of the solar-neutrino flux in terms of the resonant spin-flavor rotation mechanism. Implications for the ongoing Kamiokande II experiment are discussed. © 1991 The American Physical Society.

Año de publicación:

1991

Keywords:

    Fuente:

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    scopusscopus

    Tipo de documento:

    Article

    Estado:

    Acceso restringido

    Áreas de conocimiento:

    • Física de partículas

    Áreas temáticas:

    • Física moderna
    • Cuerpos y fenómenos celestes específicos

    Contribuidores:

    Nunokawa H.Nunokawa H.
    Hisakazu MinakataHisakazu Minakata