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Intermediate Energy Solar Neutrinos
E. Calabresu, G. Fiorentini, M. Lissia +1
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…
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…
Time-Variation of Newton's Constant and the Age of Globular Clusters
S. Degl'Innocenti, G. Fiorentini, G. G. Raffelt +2
A variation of Newton's constant over cosmological time scales would modify the main-squence time of globular cluster (GC) stars. We have calculated the evolution of low-mass s…
The fate of Li and Be in stars and in the laboratory
V. Castellani, G. Fiorentini, O. Straniero +1
We connect the observed under-abundances of Li and Be in dwarfs, with recent results on nuclear cross sections at low energies: for collisions of protons with atomic or molecular t…