Solar Antineutrinos from Fluctuating Magnetic Fields at Kamiokande


We consider the effect of a strongly chaotic magnetic field at the narrow bottom of the convective zone of the Sun together with resonant matter oscillations on the production of electron Majorana antineutrinos. Even for moderate levels of noise, we show that it is possible to obtain a small but significant probability for ν e → ν e conversions (1-3%) at… (More)


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