Signatures of spontaneously broken r parity and solar neutrino oscillations
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Signatures of spontaneously broken r parity and solar neutrino oscillations

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Signatures of spontaneously broken r parity and solar neutrino oscillations

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Santamaria, Arcadi Perfil; Furtado Valle, José Wagner Perfil
Aquest document és un/a article, creat/da en: 1989
Matter-enhanced neutrino-oscillation parameters can be probed in a variety of conventional experiments in supergravity models where the small neutrino mass arises from spontaneous R-parity violation. A combined analysis of astrophysical and laboratory limits tends to exclude regions of oscillation parameters where the high-energy neutrinos are adiabatically converted. This suggests the possibility of a large reduction in the pp and Be7 neutrino flux even for a mildly reduced B8 neutrino flux, thus stressing the importance of gallium experiments.

    Santamaria, Arcadi; Furtado Valle, José Wagner (1989) Signatures of spontaneously broken r parity and solar neutrino oscillations Physical Review D 39 6 1780
http://dx.doi.org/10.1103/PhysRevD.39.1780
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