Authors
Jea Boger, RL Hahn, JK Rowley, AL Carter, B Hollebone, D Kessler, I Blevis, F Dalnoki-Veress, A DeKok, J Farine, DR Grant, CK Hargrove, G Laberge, I Levine, K McFarlane, H Mes, AT Noble, VM Novikov, M O'Neill, M Shatkay, C Shewchuk, D Sinclair, ETH Clifford, R Deal, ED Earle, E Gaudette, G Milton, B Sur, J Bigu, JHM Cowan, DL Cluff, ED Hallman, RU Haq, J Hewett, JG Hykawy, G Jonkmans, R Michaud, A Roberge, J Roberts, E Saettler, MH Schwendener, H Seifert, D Sweezey, R Tafirout, CJ Virtue, DN Beck, YD Chan, X Chen, MR Dragowsky, FW Dycus, J Gonzalez, MCP Isaac, Y Kajiyama, GW Koehler, KT Lesko, MC Moebus, EB Norman, CE Okada, AWP Poon, P Purgalis, A Schuelke, AR Smith, RG Stokstad, S Turner, I Zlimen, JM Anaya, TJ Bowles, SJ Brice, Ernst-Ingo Esch, MM Fowler, Azriel Goldschmidt, A Hime, AF McGirt, GG Miller, WA Teasdale, JB Wilhelmy, JM Wouters, JD Anglin, M Bercovitch, WF Davidson, RS Storey, S Biller, RA Black, RJ Boardman, MG Bowler, J Cameron, B Cleveland, AP Ferraris, G Doucas, H Heron, C Howard, NA Jelley, AB Knox, M Lay, W Locke, J Lyon, S Majerus, M Moorhead, M Omori, NW Tanner, RK Taplin, M Thorman, DL Wark, N West, JC Barton, PT Trent, R Kouzes, MM Lowry, AL Bell, E Bonvin, M Boulay, M Dayon, F Duncan, LS Erhardt, HC Evans, GT Ewan, R Ford, A Hallin, A Hamer, PM Hart, PJ Harvey, D Haslip, CAW Hearns, R Heaton, JD Hepburn, CJ Jillings, EP Korpach, HW Lee, JR Leslie, M-Q Liu, HB Mak, AB McDonald, JD MacArthur, W McLatchie, BA Moffat, S Noel, TJ Radcliffe, BC Robertson, P Skensved, RL Stevenson, X Zhu, S Gil, J Heise, RL Helmer, RJ Komar, CW Nally, HS Ng, CE Waltham, RC Allen, G Bühler
Publication date
2000/7/11
Journal
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume
449
Issue
1-2
Pages
172-207
Publisher
North-Holland
Description
The Sudbury Neutrino Observatory is a second-generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of D2O 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. In this paper the physical properties, construction, and preliminary operation of the Sudbury Neutrino Observatory are described. Data and predicted operating parameters are provided whenever possible.
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Scholar articles
J Boger, RL Hahn, JK Rowley, AL Carter, B Hollebone… - Nuclear Instruments and Methods in Physics Research …, 2000