Back to Search Start Over

Sudbury neutrino observatory

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, E.I.
Fowler, M.M.
Goldschmidt, A.
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.
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, E.I.
Fowler, M.M.
Goldschmidt, A.
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.
Publication Year :
2000

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 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.

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.ocn895581167
Document Type :
Electronic Resource

Tools

Authors Abstract Subjects Details