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HEP Seminar: New opportunities with solar neutrinos

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Shirley Li, Ohio State University
When
12 October 2016 from 1:30 PM to 2:30 PM
Where
339 Davey Laboratory
Contact Name
Kohta Murase
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Crucial questions about solar neutrinos remain unanswered.   Our knowledge of stellar fusion processes and neutrinos themselves is incomplete.  Neutrino detectors such as Super-Kamiokande have the exposure needed, but backgrounds are limiting.  A leading background is the beta decays of isotopes produced by cosmic-ray muons and their secondary particles, which initiate nuclear spallation reactions.  I will discuss my comprehensive studies of the spallation backgrounds, from calculating their production rates, to understanding their production mechanisms, to how to implement better background rejection methods.  I will also discuss how our work will enable better probes of both solar and neutrino physics.

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