Energy calibration of the Sudbury neutrino observatory using monoenergetic gamma-ray sources
The Sudbury Neutrino Observatory (SNO) is a new 1000-tonne D₂O Cerenkov detector. It will shed some light on the long-standing solar neutrino problem by detecting all flavours of neutrinos originating from the Sun. A high energy gamma-ray source is needed to calibrate SNO beyond the ⁸B solar neut...
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| Language: | English |
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2009
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| Online Access: | http://hdl.handle.net/2429/9581 |