Sudbury Neutrino Observatory (SNO)
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The Sudbury Neutrino Observatory (SNO) is a water Cherenkov detector dedicated to investigate elementary particles called neutrinos. It is located 2070 m below the surface in shaft number 9 of the INCO Creighton Nickel Mine near Sudbury, Ontario.

All of the solar neutrino experiments conducted to date have only detected only a fraction of the number of expected neutrinos from the sun. This is called the Solar Neutrino Problem.

If the experiments are correct, then either our understanding of the Sun is seriously wrong, or 'neutrino oscillations' (which imply a non-zero neutrino mass) are reducing the number of detected electron neutrinos.

SNO is designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of heavy water as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the charged- and neutral-current interaction rates.

Links

Introduction to SNO SNOLAB: The International Facility for Underground Science
Particle Physics Resources Sudbury Neutrino Observatory Main Page
SNO Group at Carleton Opportunities for Students at Carleton
Carleton SNO Physics Analysis (Password required) Software Development (Password required)

 

 
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