Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2005-04-20
Phys.Rev. D72 (2005) 073004
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, 3 figures
Scientific paper
10.1103/PhysRevD.72.073004
We study the effect of random magnetic fields in the spin-flavor precession of solar neutrinos in a three generation context, when a non-vanishing transition magnetic moment is assumed. While this kind of precession is strongly constrained when the magnetic moment involves the first family, such constraints do not apply if we suppose a transition magnetic moment between the second and third families. In this scenario we can have a large non-electron anti-neutrino flux arriving on Earth, which can lead to some interesting phenomenological consequences, as, for instance, the suppression of day-night asymmetry. We have analyzed the high energy solar neutrino data and the KamLAND experiment to constrain the solar mixing angle, and solar mass difference, and we have found a larger shift of allowed values.
de Holanda Pedro Cunha
Guzzo Marcelo M.
Peres Orlando L. G.
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