[SNO logo] [SNO pt 20 MeV Source]

A.W.P. Poon§ &, M.C. Browne§, N.P. Kherani, R.J. Komar&, H.-B. Mak#, R.G.H. Robertson§ and C.E. Waltham&

§Nuclear Physics Laboratory, University of Washington, Seattle, WA 98195, USA
& Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, Canada V6T 1Z1
Ontario Hydro Technologies, 800 Kipling Avenue, Toronto, ON, Canada M8Z 5S4
#Department of Physics, Queen's University, Kingston, ON, Canada K7L 3N6


The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cerenkov detector being constructed near Sudbury, Ontario, Canada. The SNO detector is located two kilometres underground in the Creighton Mine owned by INCO Limited.

Details of the technical specifications of the SNO detector can be found here.

Our group works on the construction of a high energy calibration gamma-ray source for energy calibration of the SNO detector. The gamma-rays are generated through proton capture on tritium, which has a Q-value of 19.8 MeV. This high energy gamma-ray source is shown in the picture below.

[SNO pt 20 MeV Source pic]

Features of this source:


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Comments regarding this WWW site may be addressed to Alan Poon (poon@npl.washington.edu)

Last Updated: April 1, 1997