Intermediate Energy Solar Neutrinos
E. Calabresu, G. Fiorentini, M. Lissia, B. Ricci
Abstract
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 with solar models, both standard and non standard ones. Finally we discuss the expectations for Borexino, both in the case of standard and non standard neutrinos.
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