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Spectroscopy of Low Energy Neutrinos from the Sun

Carlo Broggini
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Abstract

Two methods are discussed for the solar neutrino spectroscopy in the sub-MeV region: absorption in a loaded liquid scintillator and elastic scattering in a TPC. The different neutrino oscillation solutions predict a strong effect in this energy region where the largest fraction (\sim 98%) of solar neutrinos lies. Both projects have reached the stage where they have to prove their capability to attain a background low enough for solar neutrino detection.

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Carlo Broggini. 2001-10-15. Spectroscopy of Low Energy Neutrinos from the Sun. https://arxiv.org/abs/hep-ex/0110026

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