Status of direct determination of solar neutrino fluxes after Borexino

Abstract

We determine the solar neutrino fuxes from the global analysis of the most up-to-date terrestrial and solar neutrino data including the fnal results of the three phases of Borexino. The analysis are performed in the framework of three-neutrino mixing with and without accounting for the solar luminosity constraint. We discuss the independence of the results on the input from the Gallium experiments. The determined fuxes are then compared with the predictions provided by the latest Standard Solar Models. We quantify the dependence of the model comparison with the assumptions about the normalization of the solar neutrino fuxes produced in the CNO-cycle as well as on the particular set of fuxes employed for the model testing.