![[SNO pt 20 MeV Source]](pt_banner.gif)
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.
Features of this source:
- Compact and Portable
It is compact enough to go down the calibration port connected to
the acrylic vessel of the SNO detector. In fact, it fits inside a 10
inch diameter by 24 inch stainless steel capsule for lowering into the
heavy water volume during calibration. Power to the source is delivered
by cable from external power supplies.
- "No" Maintenance
To ensure that the radioactive contamination from tritium be
minimal, no maintenance is required to the tritiated parts of the
source. There is no external vacuum pump or gas bottle attached to the
source.
- Low Operating Voltage
The source has an adequate gamma-ray production rate for energy calibration
at SNO at a beam energy of as low as 20 keV.
Related Links
Comments regarding this WWW site may be addressed to
Alan Poon (poon@npl.washington.edu)
Last Updated: April 1, 1997