"The Science of the Sudbury Neutrino Observatory (SNO) and SNOLAB"
Presented by Art McDonald, Queens University
Monday, December 17, 2018, 3:30 pm — Large Seminar Room, Bldg. 510
A description of the science associated with the Sudbury Neutrino Observatory, performed with substantial contributions from BNL scientists, and its relation to other neutrino measurements will be given, along with a discussion of the new set of experiments that are at various stages of development or operation at SNOLAB. These experiments will perform measurements of neutrino properties and seek direct detection of Weakly-Interacting Massive Particles (WIMPS) as Dark Matter candidates. Specific examples will include SNO+ (with BNL participation), in which the central element of the SNO detector will now be liquid scintillator with Te dissolved for neutrino-less double beta decay and DEAP-3600 using liquid argon for single phase direct Dark Matter detection. Future directions for Dark Matter detection with liquid argon will also be discussed.
Hosted by: David Asner
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