2001/10/15 by C. Broggini, Carlo Broggini, Broggini, Carlo
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #hep-ex #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ex/0110026
9 LaTeX pages, 7 postscript figures, uses epsfig and pdproc. Talk presented at the NO-VE Int. Workshop, Venezia, ITALY, 24-26 July 2001. To be published in the Workshop Proceedings
arxiv created 2001/10/15 · openalex publication_date 2001/10/15 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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 (∼ 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.