Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession

Details Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession

1998-12-16

arxiv.org/abs/hep-ph/9812390v1

Braz.J.Phys. 30 (2000) 594-601

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, 3 figures

Scientific paper

Taking into account the stringent limits from helioseismology observations on possible matter density fluctuations described by magnetohydrodynamics theory, we find the corresponding time variations of solar neutrino survival probability due to the resonant spin-flavor precession phenomenon with amplitude of order O(10%). We discuss the physics potential of high statistics real time experiments, like as Superkamiokande, to observe the effects of such magnetohydrodynamics fluctuations on their data. We conclude that these observations could be thought as a test of the resonant spin-flavor precession solution to the solar neutrino anomaly.

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