Low energy background in the NCD phase of the Sudbury Neutrino Observatory
<p>The Sudbury Neutrino Observatory (SNO) was a 1 kilotonne heavy water Č{C}erenkov detector. Evidence for flavour changing neutrino oscillations was found by comparing the rate of Charged Current interactions with that of Neutral Current (NC) interactions. </p> <p>This thes...
Prif Awdur: | O'Keeffe, HM |
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Awduron Eraill: | Jelley, NA |
Fformat: | Traethawd Ymchwil |
Iaith: | English |
Cyhoeddwyd: |
2008
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Pynciau: |
Eitemau Tebyg
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Determining the Low Energy Backgrounds at the Sudbury Neutrino Observatory
gan: O'Keeffe, H, et al.
Cyhoeddwyd: (2011) -
Simulation of the Sudbury Neutrino Observatory neutral current detectors
gan: Wan Chan Tseung, H
Cyhoeddwyd: (2008) -
Looking for matter enhanced neutrino oscillations via day v. night asymmetries in the NCD phase of the Sudbury Neutrino Observatory
gan: Ott, Richard Anthony, III
Cyhoeddwyd: (2013) -
The Sudbury Neutrino Observatory
gan: Boger, J, et al.
Cyhoeddwyd: (2000) -
The Sudbury Neutrino Observatory
gan: Jelley, N, et al.
Cyhoeddwyd: (2009)