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Talk1 h 18 min

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

A.B. McDonald · CERN

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About

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. .

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The talk

  1. The Science of the Sudbury Neutrino Observatory (SNO) and SNOLAB 2017-09-04 · 1 h 18 min · CERN's player

Credits and licence

Institution
CERN
Department
CERN Colloquium
Speaker
A.B. McDonald
Year
2017
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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