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.
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]
- and others
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}
}
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}
}