This chapter discusses the physics of solar neutrinos with detailed treatment of the following: thermonuclear energy production, standard solar models, model-independent constraints on solar neutrino fluxes, Homestake experiment, Gallium experiments (GALLEX/GNO and SAGE), water Cherenkov detectors (Kamiokande, Super-Kamiokande, and SNO), vacuum oscillations, resonant flavour transitions in the Sun, and regeneration of solar electron neutrinos in the Earth. This chapter also provides a global fit of solar neutrino data.
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