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arXiv · hep-ph/0202095

A new solution to the solar neutrino deficit

Alexander Friedland·Andrei Gruzinov
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Abstract

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.

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Alexander Friedland, Andrei Gruzinov. 2002-12-04. A new solution to the solar neutrino deficit. https://doi.org/10.1016/s0927-6505(02)00255-4

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