Searching for hep Neutrinos using the Sudbury Neutrino Observatory

Details Searching for hep Neutrinos using the Sudbury Neutrino Observatory Searching for hep Neutrinos using the Sudbury Neutrino Observatory

2009-05-29

arxiv.org/abs/0906.0040v1

Physics

High Energy Physics

High Energy Physics - Experiment

Scientific paper

The Sudbury Neutrino Observatory has recently finished its third and final phase, and has accumulated over 1082 days of neutrino data, spanning the energy range from approximately 5-20 MeV. Almost all the observed neutrinos are due to the 8B reaction in the Sun. The so-called hep process (3He + p -> 4He + e + nu_e) also occurs in the Sun, but has not yet been observed. hep neutrino energy endpoint extends above the 8B spectrum. This paper describes the three phase analysis that will ultimately be the most sensitive to this reaction.

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