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- W1573536828 abstract "The magnetic field in the solar convective zone has a random small-scale component with the r.m.s. value substancially exceeding the strength of a regular large-scale field. For two Majorana neutrino flavors and two helicities in the presence of a neutrino transition magnetic moment and nonzero neutrino mixing we analize the displacement of the allowed (Delta m^2 - sin^2 2theta)-parameter region reconciled for all Underground experiments with solar neutrinos in dependence on the r.m.s. magnetic field value b. In contrary with the RSFP scenario with a regular large-scale magnetic field, we find an effective production of electron antineutrinos in the Sun even for small neutrino mixing through the cascade conversions like nu_eL -> bar{nu}_muR -> bar{nu}_eR. It was found that usual SMA and LMA MSW parameter regions maybe forbidden while opening LOW MSW as the allowed one from the non-observation of bar{nu}_eR in the SK experiment if random magnetic fields have strengths b > 100 kG and correlation lengths shorter than L_0 < 1000 km." @default.
- W1573536828 created "2016-06-24" @default.
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- W1573536828 date "2000-02-01" @default.
- W1573536828 modified "2023-09-26" @default.
- W1573536828 title "Neutrino spin-flavor conversions and emission from the sun with random magnetic field" @default.
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- W1573536828 doi "https://doi.org/10.1016/s0920-5632(99)00867-1" @default.
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