A new solution to the solar neutrino deficit

Alexander Friedland, Andrei Gruzinov

    Research output: Contribution to journalArticlepeer-review


    We reexamine the transition magnetic moment solution to the solar neutrino problem. We argue that the absence of large time variations in the Super-Kamiokande rate provides strong evidence against spin-flavor flip in the solar convective zone. Spin-flavor flip could, however, occur in the primordial magnetic field in the radiative zone. We compute the longest-lived toroidal mode for this field and show that spin-flavor flip in the radiative zone can account for all available solar data.

    Original languageEnglish (US)
    Pages (from-to)575-582
    Number of pages8
    JournalAstroparticle Physics
    Issue number4
    StatePublished - Jul 2003

    ASJC Scopus subject areas

    • Astronomy and Astrophysics


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