Solar models and solar neutrino oscillations

Abstract

We provide a summary of the current knowledge, theoretical and experimental, of solar neutrino fluxes and of the masses and mixing angles that characterize solar neutrino oscillations. We also summarize the principal reasons for doing new solar neutrino experiments and what we think may be learned from the future measurements.

Comments: Submitted to the Neutrino Focus Issue of New Journal of Physics at http://www.njp.org