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Solar neutrino interactions: Using charged currents at SNO to tell neutral currents at Super-Kamiokande
F. L. Villante, G. Fiorentini, E. Lisi
In the presence of flavor oscillations, muon and tau neutrinos can contribute to the Super-Kamiokande (SK) solar neutrino signal through the neutral current process ν_{μ,τ} e^{-}\t…
Neutrino masses and mixing
S. M. Bilenky, C. Giunti, W. Grimus
We present a short review of the present status of the problem of neutrino masses and mixing. The existing experimental results indicate that there are at least four massive neutri…
Vacuum oscillations and variations of solar neutrino rates in SuperKamiokande and Borexino
B. Faid, G. L. Fogli, E. Lisi +1
The vacuum oscillation solution to the solar neutrino problem predicts characteristics variations of the observable neutrinos rates, as a result of the L/E_nu dependence of the nu_…
Discriminating MSW solutions to the solar neutrino problem with flux-independent information at SuperKamiokande and SNO
G. L. Fogli, E. Lisi, D. Montanino
The two possible Mikheyev-Smirnov-Wolfenstein (MSW) solutions of the solar neutrino problem (one at small and the other at large mixing angle), up to now tested mainly through abso…
Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations
G. Fiorentini, E. Lisi, Subir Sarkar +1
We present a simple method for determining the (correlated) uncertainties of the light element abundances expected from big bang nucleosynthesis, which avoids the need for lengthy…