A new solution to the solar neutrino deficit

Details A new solution to the solar neutrino deficit A new solution to the solar neutrino deficit

2002-02-11

arxiv.org/abs/hep-ph/0202095v3

Astropart.Phys.19:575-582,2003

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 5 figures, version accepted for publication in Astroparticle Physics

Scientific paper

10.1016/S0927-6505(02)00255-4

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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