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Nuclear physics inputs needed for geo-neutrino studies
G. Bellini, G. Fiorentini, A. Ianni +3
Geo-neutrino studies are based on theoretical estimates of geo-neutrino spectra. We propose a method for a direct measurement of the energy distribution of antineutrinos from decay…
The solar neutrino spectrum derived from electron scattering and charged current interactions
G. Fiorentini, F. L. Villante
We provide a method for extracting information on the energy spectrum of solar neutrinos directly from the spectrum of scattered electrons. As an example, we apply it to the publis…
A few comments after the charged current measurement at the Sudbury Neutrino Observatory
G. Fiorentini, F. L. Villante, B. Ricci
The comparison of the SNO charged current result with the solar neutrino signal measured by Super-Kamiokande has provided, for the first time, the evidence of a non electron flavou…
Atmospheric neutrino flux and muon data
G. Fiorentini, V. A. Naumov, F. L. Villante
We present a new one-dimensional calculation of low and intermediate energy atmospheric muon and neutrino fluxes, using up-to-date data on primary cosmic rays and hadronic interact…
Solar neutrinos (almost) without standard solar models
G. Fiorentini, B. Ricci
We extract information on the fluxes of Be and CNO neutrinos directly from solar neutrino experiments, with minimal assumptions about solar models. Next we compare these results wi…