CERN Colloquium

The Science of the Sudbury Neutrino Observatory (SNO) and SNOLAB

by A.B. McDonald (Queen’s University, Kingston, Canada)

500-1-001 - Main Auditorium (CERN)

500-1-001 - Main Auditorium


Show room on map

A description of the science associated with the Sudbury Neutrino Observatory 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. The experiments include SNO+, in which the central element of the SNO detector will be liquid scintillator with Te dissolved for neutrino-less double beta decay; DEAP, using about 3300 kg of liquid argon for single phase direct Dark Matter detection; SuperCDMS, a solid state bolometer system to start construction at SNOLAB in the near future; PICO, a direct Dark Matter experiment using bubble formation for detection and NEWS, a direct Dark Matter detector using high pressure gasses for low-mass WIMP detection.

Organized by

W. Lerche/TH-SP....................................................... Tea and coffee will be served at 16h00

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