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The Sudbury Neutrino Observatory

Abstract

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 D{sub 2}O 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.
Authors:
Boger, J; Hahn, R L; Rowley, J K; Carter, A L; Hollebone, B; Kessler, D; Blevis, I; Dalnoki-Veress, F; DeKok, A; Farine, J; Grant, D R; Hargrove, C K; Laberge, G; Levine, I; McFarlane, K; Mes, H; Noble, A T; Novikov, V M; O'Neill, M; Shatkay, M; Shewchuk, C; Sinclair, D; Clifford, E T.H.; Deal, R; Earle, E D; Gaudette, E; Milton, G; Sur, B; Bigu, J; Cowan, J H.M.; Cluff, D L; Hallman, E D; Haq, R U; Hewett, J; Hykawy, J G; Jonkmans, G; Michaud, R; Roberge, A; Roberts, J; Saettler, E; Schwendener, M H; Seifert, H; Sweezey, D; Tafirout, R; Virtue, C J; Beck, D N; Chan, Y D; Chen, X; Dragowsky, M R; Dycus, F W; Gonzalez, J; Isaac, M C.P.; Kajiyama, Y; Koehler, G W; Lesko, K T; Moebus, M C; Norman, E B; Okada, C E; Poon, A W.P.; Purgalis, P; Schuelke, A; Smith, A R; Stokstad, R G; Turner, S; Zlimen, I; Anaya, J M; Bowles, T J; Brice, S J; Esch, Ernst-Ingo; Fowler, M M; Goldschmidt, Azriel; Hime, A; McGirt, A F; Miller, G G; Teasdale, W A; Wilhelmy, J B; Wouters, J M; Anglin, J D; Bercovitch, M; Davidson, W F; Storey, R S; Biller, S; Black, R A; Boardman, R J; Bowler, M G; Cameron, J; Cleveland, B; Ferraris, A P; Doucas, G; Heron, H; Howard, C; Jelley, N A; Knox, A B; Lay, M; Locke, W; Lyon, J; Majerus, S; Moorhead, M; Omori, M; Tanner, N W; Taplin, R K; Thorman, M; Wark, D L; West, N; Barton, J C; Trent, P T; Kouzes, R; Lowry, M M; Bell, A L; Bonvin, E; Boulay, M; Dayon, M; Duncan, F; Erhardt, L S; Evans, H C; Ewan, G T; Ford, R; Hallin, A; Hamer, A; Hart, P M; Harvey, P J; Haslip, D; Hearns, C A.W.; Heaton, R; Hepburn, J D; Jillings, C J; Korpach, E P; Lee, H W; Leslie, J R; Liu, M -Q; Mak, H B; McDonald, A B; MacArthur, J D; McLatchie, W; Moffat, B A; Noel, S; Radcliffe, T J; Robertson, B C; Skensved, P; Stevenson, R L; Zhu, X; Gil, S; Heise, J; Helmer, R L; Komar, R J; Nally, C W [1] 
  1. and others
Publication Date:
Jul 11, 2000
Product Type:
Journal Article
Resource Relation:
Journal Name: Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment; Journal Volume: 449; Journal Issue: 1-2; Other Information: PII: S0168900299014692; Copyright (c) 2000 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved; Country of input: Ukraine; PBD: 11 Jul 2000
Subject:
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; CHERENKOV COUNTERS; HE-3 COUNTERS; HEAVY WATER; NEUTRINO OSCILLATION; SOLAR NEUTRINOS; SPECIFICATIONS; SUDBURY NEUTRINO OBSERVATORY
OSTI ID:
20369611
Country of Origin:
Netherlands
Language:
English
Other Identifying Numbers:
Journal ID: ISSN 0168-9002; NIMAER; TRN: NL03S0614051353
Submitting Site:
NLN
Size:
page(s) 172-207
Announcement Date:
Aug 16, 2003

Citation Formats

Boger, J, Hahn, R L, Rowley, J K, Carter, A L, Hollebone, B, Kessler, D, Blevis, I, Dalnoki-Veress, F, DeKok, A, Farine, J, Grant, D R, Hargrove, C K, Laberge, G, Levine, I, McFarlane, K, Mes, H, Noble, A T, Novikov, V M, O'Neill, M, Shatkay, M, Shewchuk, C, Sinclair, D, Clifford, E T.H., Deal, R, Earle, E D, Gaudette, E, Milton, G, Sur, B, Bigu, J, Cowan, J H.M., Cluff, D L, Hallman, E D, Haq, R U, Hewett, J, Hykawy, J G, Jonkmans, G, Michaud, R, Roberge, A, Roberts, J, Saettler, E, Schwendener, M H, Seifert, H, Sweezey, D, Tafirout, R, Virtue, C J, Beck, D N, Chan, Y D, Chen, X, Dragowsky, M R, Dycus, F W, Gonzalez, J, Isaac, M C.P., Kajiyama, Y, Koehler, G W, Lesko, K T, Moebus, M C, Norman, E B, Okada, C E, Poon, A W.P., Purgalis, P, Schuelke, A, Smith, A R, Stokstad, R G, Turner, S, Zlimen, I, Anaya, J M, Bowles, T J, Brice, S J, Esch, Ernst-Ingo, Fowler, M M, Goldschmidt, Azriel, Hime, A, McGirt, A F, Miller, G G, Teasdale, W A, Wilhelmy, J B, Wouters, J M, Anglin, J D, Bercovitch, M, Davidson, W F, Storey, R S, Biller, S, Black, R A, Boardman, R J, Bowler, M G, Cameron, J, Cleveland, B, Ferraris, A P, Doucas, G, Heron, H, Howard, C, Jelley, N A, Knox, A B, Lay, M, Locke, W, Lyon, J, Majerus, S, Moorhead, M, Omori, M, Tanner, N W, Taplin, R K, Thorman, M, Wark, D L, West, N, Barton, J C, Trent, P T, Kouzes, R, Lowry, M M, Bell, A L, Bonvin, E, Boulay, M, Dayon, M, Duncan, F, Erhardt, L S, Evans, H C, Ewan, G T, Ford, R, Hallin, A, Hamer, A, Hart, P M, Harvey, P J, Haslip, D, Hearns, C A.W., Heaton, R, Hepburn, J D, Jillings, C J, Korpach, E P, Lee, H W, Leslie, J R, Liu, M -Q, Mak, H B, McDonald, A B, MacArthur, J D, McLatchie, W, Moffat, B A, Noel, S, Radcliffe, T J, Robertson, B C, Skensved, P, Stevenson, R L, Zhu, X, Gil, S, Heise, J, Helmer, R L, Komar, R J, and Nally, C W. The Sudbury Neutrino Observatory. Netherlands: N. p., 2000. Web. doi:10.1016/S0168-9002(99)01469-2.
Boger, J, Hahn, R L, Rowley, J K, Carter, A L, Hollebone, B, Kessler, D, Blevis, I, Dalnoki-Veress, F, DeKok, A, Farine, J, Grant, D R, Hargrove, C K, Laberge, G, Levine, I, McFarlane, K, Mes, H, Noble, A T, Novikov, V M, O'Neill, M, Shatkay, M, Shewchuk, C, Sinclair, D, Clifford, E T.H., Deal, R, Earle, E D, Gaudette, E, Milton, G, Sur, B, Bigu, J, Cowan, J H.M., Cluff, D L, Hallman, E D, Haq, R U, Hewett, J, Hykawy, J G, Jonkmans, G, Michaud, R, Roberge, A, Roberts, J, Saettler, E, Schwendener, M H, Seifert, H, Sweezey, D, Tafirout, R, Virtue, C J, Beck, D N, Chan, Y D, Chen, X, Dragowsky, M R, Dycus, F W, Gonzalez, J, Isaac, M C.P., Kajiyama, Y, Koehler, G W, Lesko, K T, Moebus, M C, Norman, E B, Okada, C E, Poon, A W.P., Purgalis, P, Schuelke, A, Smith, A R, Stokstad, R G, Turner, S, Zlimen, I, Anaya, J M, Bowles, T J, Brice, S J, Esch, Ernst-Ingo, Fowler, M M, Goldschmidt, Azriel, Hime, A, McGirt, A F, Miller, G G, Teasdale, W A, Wilhelmy, J B, Wouters, J M, Anglin, J D, Bercovitch, M, Davidson, W F, Storey, R S, Biller, S, Black, R A, Boardman, R J, Bowler, M G, Cameron, J, Cleveland, B, Ferraris, A P, Doucas, G, Heron, H, Howard, C, Jelley, N A, Knox, A B, Lay, M, Locke, W, Lyon, J, Majerus, S, Moorhead, M, Omori, M, Tanner, N W, Taplin, R K, Thorman, M, Wark, D L, West, N, Barton, J C, Trent, P T, Kouzes, R, Lowry, M M, Bell, A L, Bonvin, E, Boulay, M, Dayon, M, Duncan, F, Erhardt, L S, Evans, H C, Ewan, G T, Ford, R, Hallin, A, Hamer, A, Hart, P M, Harvey, P J, Haslip, D, Hearns, C A.W., Heaton, R, Hepburn, J D, Jillings, C J, Korpach, E P, Lee, H W, Leslie, J R, Liu, M -Q, Mak, H B, McDonald, A B, MacArthur, J D, McLatchie, W, Moffat, B A, Noel, S, Radcliffe, T J, Robertson, B C, Skensved, P, Stevenson, R L, Zhu, X, Gil, S, Heise, J, Helmer, R L, Komar, R J, & Nally, C W. The Sudbury Neutrino Observatory. Netherlands. https://doi.org/10.1016/S0168-9002(99)01469-2
Boger, J, Hahn, R L, Rowley, J K, Carter, A L, Hollebone, B, Kessler, D, Blevis, I, Dalnoki-Veress, F, DeKok, A, Farine, J, Grant, D R, Hargrove, C K, Laberge, G, Levine, I, McFarlane, K, Mes, H, Noble, A T, Novikov, V M, O'Neill, M, Shatkay, M, Shewchuk, C, Sinclair, D, Clifford, E T.H., Deal, R, Earle, E D, Gaudette, E, Milton, G, Sur, B, Bigu, J, Cowan, J H.M., Cluff, D L, Hallman, E D, Haq, R U, Hewett, J, Hykawy, J G, Jonkmans, G, Michaud, R, Roberge, A, Roberts, J, Saettler, E, Schwendener, M H, Seifert, H, Sweezey, D, Tafirout, R, Virtue, C J, Beck, D N, Chan, Y D, Chen, X, Dragowsky, M R, Dycus, F W, Gonzalez, J, Isaac, M C.P., Kajiyama, Y, Koehler, G W, Lesko, K T, Moebus, M C, Norman, E B, Okada, C E, Poon, A W.P., Purgalis, P, Schuelke, A, Smith, A R, Stokstad, R G, Turner, S, Zlimen, I, Anaya, J M, Bowles, T J, Brice, S J, Esch, Ernst-Ingo, Fowler, M M, Goldschmidt, Azriel, Hime, A, McGirt, A F, Miller, G G, Teasdale, W A, Wilhelmy, J B, Wouters, J M, Anglin, J D, Bercovitch, M, Davidson, W F, Storey, R S, Biller, S, Black, R A, Boardman, R J, Bowler, M G, Cameron, J, Cleveland, B, Ferraris, A P, Doucas, G, Heron, H, Howard, C, Jelley, N A, Knox, A B, Lay, M, Locke, W, Lyon, J, Majerus, S, Moorhead, M, Omori, M, Tanner, N W, Taplin, R K, Thorman, M, Wark, D L, West, N, Barton, J C, Trent, P T, Kouzes, R, Lowry, M M, Bell, A L, Bonvin, E, Boulay, M, Dayon, M, Duncan, F, Erhardt, L S, Evans, H C, Ewan, G T, Ford, R, Hallin, A, Hamer, A, Hart, P M, Harvey, P J, Haslip, D, Hearns, C A.W., Heaton, R, Hepburn, J D, Jillings, C J, Korpach, E P, Lee, H W, Leslie, J R, Liu, M -Q, Mak, H B, McDonald, A B, MacArthur, J D, McLatchie, W, Moffat, B A, Noel, S, Radcliffe, T J, Robertson, B C, Skensved, P, Stevenson, R L, Zhu, X, Gil, S, Heise, J, Helmer, R L, Komar, R J, and Nally, C W. 2000. "The Sudbury Neutrino Observatory." Netherlands. https://doi.org/10.1016/S0168-9002(99)01469-2.
@misc{etde_20369611,
title = {The Sudbury Neutrino Observatory}
author = {Boger, J, Hahn, R L, Rowley, J K, Carter, A L, Hollebone, B, Kessler, D, Blevis, I, Dalnoki-Veress, F, DeKok, A, Farine, J, Grant, D R, Hargrove, C K, Laberge, G, Levine, I, McFarlane, K, Mes, H, Noble, A T, Novikov, V M, O'Neill, M, Shatkay, M, Shewchuk, C, Sinclair, D, Clifford, E T.H., Deal, R, Earle, E D, Gaudette, E, Milton, G, Sur, B, Bigu, J, Cowan, J H.M., Cluff, D L, Hallman, E D, Haq, R U, Hewett, J, Hykawy, J G, Jonkmans, G, Michaud, R, Roberge, A, Roberts, J, Saettler, E, Schwendener, M H, Seifert, H, Sweezey, D, Tafirout, R, Virtue, C J, Beck, D N, Chan, Y D, Chen, X, Dragowsky, M R, Dycus, F W, Gonzalez, J, Isaac, M C.P., Kajiyama, Y, Koehler, G W, Lesko, K T, Moebus, M C, Norman, E B, Okada, C E, Poon, A W.P., Purgalis, P, Schuelke, A, Smith, A R, Stokstad, R G, Turner, S, Zlimen, I, Anaya, J M, Bowles, T J, Brice, S J, Esch, Ernst-Ingo, Fowler, M M, Goldschmidt, Azriel, Hime, A, McGirt, A F, Miller, G G, Teasdale, W A, Wilhelmy, J B, Wouters, J M, Anglin, J D, Bercovitch, M, Davidson, W F, Storey, R S, Biller, S, Black, R A, Boardman, R J, Bowler, M G, Cameron, J, Cleveland, B, Ferraris, A P, Doucas, G, Heron, H, Howard, C, Jelley, N A, Knox, A B, Lay, M, Locke, W, Lyon, J, Majerus, S, Moorhead, M, Omori, M, Tanner, N W, Taplin, R K, Thorman, M, Wark, D L, West, N, Barton, J C, Trent, P T, Kouzes, R, Lowry, M M, Bell, A L, Bonvin, E, Boulay, M, Dayon, M, Duncan, F, Erhardt, L S, Evans, H C, Ewan, G T, Ford, R, Hallin, A, Hamer, A, Hart, P M, Harvey, P J, Haslip, D, Hearns, C A.W., Heaton, R, Hepburn, J D, Jillings, C J, Korpach, E P, Lee, H W, Leslie, J R, Liu, M -Q, Mak, H B, McDonald, A B, MacArthur, J D, McLatchie, W, Moffat, B A, Noel, S, Radcliffe, T J, Robertson, B C, Skensved, P, Stevenson, R L, Zhu, X, Gil, S, Heise, J, Helmer, R L, Komar, R J, and Nally, C W}
abstractNote = {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 D{sub 2}O 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.}
doi = {10.1016/S0168-9002(99)01469-2}
journal = []
issue = {1-2}
volume = {449}
journal type = {AC}
place = {Netherlands}
year = {2000}
month = {Jul}
}