7 papers
The reaction, solar neutrinos and the age of the globular clusters
S. Degl'Innocenti, G. Fiorentini, B. Ricci +1
We discuss implications of a new measurement of concerning solar neutrinos, solar models and globular cluster dating. Predictions for the gallium and chlorine…
Helioseismic tests of diffusion theory
G. Fiorentini, M. Lissia, B. Ricci
We present a quantitative estimate of the accuracy of the calculated diffusion coefficients, by comparing predictions of solar models with observational data provided by helioseism…
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…
Last Hope for an astrophysical solution to the solar neutrino problem
V. Berezinsky, G. Fiorentini, M. Lissia
We discuss what appears the last hope for an astrophysical solution to the solar neutrino problem: a correlated variation of the astrophysical factors for the helium burning cross…
Where are the beryllium neutrinos?
S. Degl'Innocenti, G. Fiorentini, M. Lissia
We show that present experiments imply that neutrinos are nonstandard at the 87\% C.L., independently of solar or nuclear physics. Moreover, if neutrinos are standard, the Be f…
The MSW solution to the solar neutrino problem for non-standard solar models
V. Berezinsky, G. Fiorentini, M. Lissia
The difficulties for non-standard solar models (NSSM) in resolving the solar neutrino problem are discussed stressing the incompatibility of the gallium--Kamiokande data, and of th…