Reines Lecture Colloquium: The Science of the Sudbury Neutrino Observatory (SNO) and SNOLAB

Printer-friendly versionPrinter-friendly version
Speaker: 
Arthur B. McDonald
Institution: 
Queens Univ.
Email: 
art@snolab.ca
Speaker Link: 
Arthur B. McDonald
Date: 
Thu, 03/02/2017
Time: 
3:30 pm
Location: 
RH 101
 

 
 
ABSTRACT:
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. 
 

 
Learn more about the Reines Lecture Series at:  http://ps.uci.edu/rls
 
 
CLICK HERE to register for the 2017 Reines Lecture:  
 
A Deeper Understanding of the Universe From 2 Kilometers Underground
March 1, 2017
7:30 - 8:30 PM 
​Irvine Barclay Theatre
​4242 Campus Drive
Irvine, CA 92612 
 
 
 
 
 
 
 
Host: 
Henry Sobel