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Article ; Online: Evidence of Antineutrinos from Distant Reactors Using Pure Water at SNO.

Allega, A / Anderson, M R / Andringa, S / Antunes, J / Askins, M / Auty, D J / Bacon, A / Barros, N / Barão, F / Bayes, R / Beier, E W / Bezerra, T S / Bialek, A / Biller, S D / Blucher, E / Caden, E / Callaghan, E J / Cheng, S / Chen, M /

Cleveland, B / Cookman, D / Corning, J / Cox, M A / Dehghani, R / Deloye, J / Deluce, C / Depatie, M M / Dittmer, J / Dixon, K H / Di Lodovico, F / Falk, E / Fatemighomi, N / Ford, R / Frankiewicz, K / Gaur, A / González-Reina, O I / Gooding, D / Grant, C / Grove, J / Hallin, A L / Hallman, D / Heintzelman, W J / Helmer, R L / Hu, J / Hunt-Stokes, R / Hussain, S M A / Inácio, A S / Jillings, C J / Kaluzienski, S / Kaptanoglu, T / Khaghani, P / Khan, H / Klein, J R / Kormos, L L / Krar, B / Kraus, C / Krauss, C B / Kroupová, T / Lam, I / Land, B J / Lawson, I / Lebanowski, L / Lee, J / Lefebvre, C / Lidgard, J / Lin, Y H / Lozza, V / Luo, M / Maio, A / Manecki, S / Maneira, J / Martin, R D / McCauley, N / McDonald, A B / Mills, C / Morton-Blake, I / Naugle, S / Nolan, L J / O'Keeffe, H M / Orebi Gann, G D / Page, J / Parker, W / Paton, J / Peeters, S J M / Pickard, L / Ravi, P / Reichold, A / Riccetto, S / Richardson, R / Rigan, M / Rose, J / Rosero, R / Rumleskie, J / Semenec, I / Skensved, P / Smiley, M / Svoboda, R / Tam, B / Tseng, J / Turner, E / Valder, S / Virtue, C J / Vázquez-Jáuregui, E / Wang, J / Ward, M / Wilson, J R / Wilson, J D / Wright, A / Yanez, J P / Yang, S / Yeh, M / Yu, S / Zhang, Y / Zuber, K / Zummo, A

Physical review letters

2023 Volume 130, Issue 9, Page(s) 91801

Abstract: The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240 km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with ... ...

Abstract	The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240 km away in Ontario, Canada. This analysis uses events with energies lower than in any previous analysis with a large water Cherenkov detector. Two analytical methods are used to distinguish reactor antineutrinos from background events in 190 days of data and yield consistent evidence for antineutrinos with a combined significance of 3.5σ.
Language	English
Publishing date	2023-02-24
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.130.091801
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Article: Constraints on nucleon decay via invisible modes from the Sudbury Neutrino Observatory.

Ahmed, S N / Anthony, A E / Beier, E W / Bellerive, A / Biller, S D / Boger, J / Boulay, M G / Bowler, M G / Bowles, T J / Brice, S J / Bullard, T V / Chan, Y D / Chen, M / Chen, X / Cleveland, B T / Cox, G A / Dai, X / Dalnoki-Veress, F / Doe, P J /

Dosanjh, R S / Doucas, G / Dragowsky, M R / Duba, C A / Duncan, F A / Dunford, M / Dunmore, J A / Earle, E D / Elliott, S R / Evans, H C / Ewan, G T / Farine, J / Fergani, H / Fleurot, F / Formaggio, J A / Fowler, M M / Frame, K / Frati, W / Fulsom, B G / Gagnon, N / Graham, K / Grant, D R / Hahn, R L / Hall, J C / Hallin, A L / Hallman, E D / Hamer, A S / Handler, W B / Hargrove, C K / Harvey, P J / Hazama, R / Heeger, K M / Heintzelman, W J / Heise, J / Helmer, R L / Hemingway, R J / Hime, A / Howe, M A / Jagam, P / Jelley, N A / Klein, J R / Kos, M S / Krumins, A V / Kutter, T / Kyba, C C M / Labranche, H / Lange, R / Law, J / Lawson, I T / Lesko, K T / Leslie, J R / Levine, I / Luoma, S / MacLellan, R / Majerus, S / Mak, H B / Maneira, J / Marino, A D / McCauley, N / McDonald, A B / McGee, S / McGregor, G / Mifflin, C / Miknaitis, K K S / Miller, G G / Moffat, B A / Nally, C W / Neubauer, M S / Nickel, B G / Noble, A J / Norman, E B / Oblath, N S / Okada, C E / Ollerhead, R W / Orrell, J L / Oser, S M / Ouellet, C / Peeters, S J M / Poon, A W P / Robertson, B C / Robertson, R G H / Rollin, E / Rosendahl, S S E / Rusu, V L / Schwendener, M H / Simard, O / Simpson, J J / Sims, C J / Sinclair, D / Skensved, P / Smith, M W E / Starinsky, N / Stokstad, R G / Stonehill, L C / Tafirout, R / Takeuchi, Y / Tesić, G / Thomson, M / Thorman, M / Van Berg, R / Van de Water, R G / Virtue, C J / Wall, B L / Waller, D / Waltham, C E / Tseung, H Wan Chan / Wark, D L / West, N / Wilhelmy, J B / Wilkerson, J F / Wilson, J R / Wittich, P / Wouters, J M / Yeh, M / Zuber, K

Physical review letters

2004 Volume 92, Issue 10, Page(s) 102004

Abstract: Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n-->3nu. The analysis was based on a search for gamma rays from the deexcitation of the residual nucleus that would result ...

Abstract	Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n-->3nu. The analysis was based on a search for gamma rays from the deexcitation of the residual nucleus that would result from the disappearance of either a proton or neutron from 16O. A limit of tau(inv)>2 x 10(29) yr is obtained at 90% confidence for either neutron- or proton-decay modes. This is about an order of magnitude more stringent than previous constraints on invisible proton-decay modes and 400 times more stringent than similar neutron modes.
Language	English
Publishing date	2004-03-12
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.92.102004
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Measurement of the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity.

Dosanjh, R S / Doucas, G / Dragowsky, M R / Duba, C A / Duncan, F A / Dunford, M / Dunmore, J A / Earle, E D / Elliott, S R / Evans, H C / Ewan, G T / Farine, J / Fergani, H / Fleurot, F / Formaggio, J A / Fowler, M M / Frame, K / Fulsom, B G / Gagnon, N / Graham, K / Grant, D R / Hahn, R L / Hall, J C / Hallin, A L / Hallman, E D / Hamer, A S / Handler, W B / Hargrove, C K / Harvey, P J / Hazama, R / Heeger, K M / Heintzelman, W J / Heise, J / Helmer, R L / Hemingway, R J / Hime, A / Howe, M A / Jagam, P / Jelley, N A / Klein, J R / Kos, M S / Krumins, A V / Kutter, T / Kyba, C C M / Labranche, H / Lange, R / Law, J / Lawson, I T / Lesko, K T / Leslie, J R / Levine, I / Luoma, S / MacLellan, R / Majerus, S / Mak, H B / Maneira, J / Marino, A D / McCauley, N / McDonald, A B / McGee, S / McGregor, G / Mifflin, C / Miknaitis, K K S / Miller, G G / Moffat, B A / Nally, C W / Nickel, B G / Noble, A J / Norman, E B / Oblath, N S / Okada, C E / Ollerhead, R W / Orrell, J L / Oser, S M / Ouellet, C / Peeters, S J M / Poon, A W P / Robertson, B C / Robertson, R G H / Rollin, E / Rosendahl, S S E / Rusu, V L / Schwendener, M H / Simard, O / Simpson, J J / Sims, C J / Sinclair, D / Skensved, P / Smith, M W E / Starinsky, N / Stokstad, R G / Stonehill, L C / Tafirout, R / Takeuchi, Y / Tesić, G / Thomson, M / Thorman, M / Van Berg, R / Van de Water, R G / Virtue, C J / Wall, B L / Waller, D / Waltham, C E / Tseung, H Wan Chan / Wark, D L / West, N / Wilhelmy, J B / Wilkerson, J F / Wilson, J R / Wouters, J M / Yeh, M / Zuber, K

Physical review letters

2004 Volume 92, Issue 18, Page(s) 181301

Abstract: The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability. The measurements were made with dissolved NaCl in heavy water to ... ...

Abstract	The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability. The measurements were made with dissolved NaCl in heavy water to enhance the sensitivity and signature for neutral-current interactions. The flux is found to be 5.21 +/- 0.27(stat)+/-0.38(syst) x 10(6) cm(-2) s(-1), in agreement with previous measurements and standard solar models. A global analysis of these and other solar and reactor neutrino results yields Deltam(2)=7.1(+1.2)(-0.6) x 10(-5) eV(2) and theta=32.5(+2.4)(-2.3) degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations.
Language	English
Publishing date	2004-05-07
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.92.181301
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Independent measurement of the total active 8B solar neutrino flux using an array of 3He proportional counters at the Sudbury Neutrino Observatory.

Aharmim, B / Ahmed, S N / Amsbaugh, J F / Anthony, A E / Banar, J / Barros, N / Beier, E W / Bellerive, A / Beltran, B / Bergevin, M / Biller, S D / Boudjemline, K / Boulay, M G / Bowles, T J / Browne, M C / Bullard, T V / Burritt, T H / Cai, B / Chan, Y D /

Chauhan, D / Chen, M / Cleveland, B T / Cox-Mobrand, G A / Currat, C A / Dai, X / Deng, H / Detwiler, J / DiMarco, M / Doe, P J / Doucas, G / Drouin, P-L / Duba, C A / Duncan, F A / Dunford, M / Earle, E D / Elliott, S R / Evans, H C / Ewan, G T / Farine, J / Fergani, H / Fleurot, F / Ford, R J / Formaggio, J A / Fowler, M M / Gagnon, N / Germani, J V / Goldschmidt, A / Goon, J T M / Graham, K / Guillian, E / Habib, S / Hahn, R L / Hallin, A L / Hallman, E D / Hamian, A A / Harper, G C / Harvey, P J / Hazama, R / Heeger, K M / Heintzelman, W J / Heise, J / Helmer, R L / Henning, R / Hime, A / Howard, C / Howe, M A / Huang, M / Jagam, P / Jamieson, B / Jelley, N A / Keeter, K J / Klein, J R / Kormos, L L / Kos, M / Krüger, A / Kraus, C / Krauss, C B / Kutter, T / Kyba, C C M / Lange, R / Law, J / Lawson, I T / Lesko, K T / Leslie, J R / Loach, J C / MacLellan, R / Majerus, S / Mak, H B / Maneira, J / Martin, R / McBryde, K / McCauley, N / McDonald, A B / McGee, S / Mifflin, C / Miller, G G / Miller, M L / Monreal, B / Monroe, J / Morissette, B / Myers, A / Nickel, B G / Noble, A J / Oblath, N S / O'Keeffe, H M / Ollerhead, R W / Gann, G D Orebi / Oser, S M / Ott, R A / Peeters, S J M / Poon, A W P / Prior, G / Reitzner, S D / Rielage, K / Robertson, B C / Robertson, R G H / Rollin, E / Schwendener, M H / Secrest, J A / Seibert, S R / Simard, O / Simpson, J J / Sinclair, L / Skensved, P / Smith, M W E / Steiger, T D / Stonehill, L C / Tesić, G / Thornewell, P M / Tolich, N / Tsui, T / Tunnell, C D / Van Wechel, T / Van Berg, R / VanDevender, B A / Virtue, C J / Walker, T J / Wall, B L / Waller, D / Tseung, H Wan Chan / Wendland, J / West, N / Wilhelmy, J B / Wilkerson, J F / Wilson, J R / Wouters, J M / Wright, A / Yeh, M / Zhang, F / Zuber, K

Physical review letters

2008 Volume 101, Issue 11, Page(s) 111301

Abstract: The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (nu_x) 8B solar neutrino flux. This technique is independent of ...

Abstract	The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (nu_x) 8B solar neutrino flux. This technique is independent of previous methods employed by SNO. The total flux is found to be 5.54_-0.31;+0.33(stat)-0.34+0.36(syst)x10(6) cm(-2) s(-1), in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Deltam2=7.59_-0.21;+0.19x10(-5) eV2 and theta=34.4_-1.2;+1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO's previous results.
Language	English
Publishing date	2008-09-12
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.101.111301
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory.

Ahmad, Q R / Allen, R C / Andersen, T C / D Anglin, J / Barton, J C / Beier, E W / Bercovitch, M / Bigu, J / Biller, S D / Black, R A / Blevis, I / Boardman, R J / Boger, J / Bonvin, E / Boulay, M G / Bowler, M G / Bowles, T J / Brice, S J / Browne, M C /

Bullard, T V / Bühler, G / Cameron, J / Chan, Y D / Chen, H H / Chen, M / Chen, X / Cleveland, B T / Clifford, E T H / Cowan, J H M / Cowen, D F / Cox, G A / Dai, X / Dalnoki-Veress, F / Davidson, W F / Doe, P J / Doucas, G / Dragowsky, M R / Duba, C A / Duncan, F A / Dunford, M / Dunmore, J A / Earle, E D / Elliott, S R / Evans, H C / Ewan, G T / Farine, J / Fergani, H / Ferraris, A P / Ford, R J / Formaggio, J A / Fowler, M M / Frame, K / Frank, E D / Frati, W / Gagnon, N / Germani, J V / Gil, S / Graham, K / Grant, D R / Hahn, R L / Hallin, A L / Hallman, E D / Hamer, A S / Hamian, A A / Handler, W B / Haq, R U / Hargrove, C K / Harvey, P J / Hazama, R / Heeger, K M / Heintzelman, W J / Heise, J / Helmer, R L / Hepburn, J D / Heron, H / Hewett, J / Hime, A / Howe, M / Hykawy, J G / Isaac, M C P / Jagam, P / Jelley, N A / Jillings, C / Jonkmans, G / Kazkaz, K / Keener, P T / Klein, J R / Knox, A B / Komar, R J / Kouzes, R / Kutter, T / Kyba, C C M / Law, J / Lawson, I T / Lay, M / Lee, H W / Lesko, K T / Leslie, J R / Levine, I / Locke, W / Luoma, S / Lyon, J / Majerus, S / Mak, H B / Maneira, J / Manor, J / Marino, A D / McCauley, N / McDonald, A B / McDonald, D S / McFarlane, K / McGregor, G / Meijer Drees, R / Mifflin, C / Miller, G G / Milton, G / Moffat, B A / Moorhead, M / Nally, C W / Neubauer, M S / Newcomer, F M / Ng, H S / Noble, A J / Norman, E B / Novikov, V M / O'Neill, M / Okada, C E / Ollerhead, R W / Omori, M / Orrell, J L / Oser, S M / Poon, A W P / Radcliffe, T J / Roberge, A / Robertson, B C / Robertson, R G H / Rosendahl, S S E / Rowley, J K / Rusu, V L / Saettler, E / Schaffer, K K / Schwendener, M H / Schülke, A / Seifert, H / Shatkay, M / Simpson, J J / Sims, C J / Sinclair, D / Skensved, P / Smith, A R / Smith, M W E / Spreitzer, T / Starinsky, N / Steiger, T D / Stokstad, R G / Stonehill, L C / Storey, R S / Sur, B / Tafirout, R / Tagg, N / Tanner, N W / Taplin, R K / Thorman, M / Thornewell, P M / Trent, P T / Tserkovnyak, Y I / Van Berg, R / Van de Water, R G / Virtue, C J / Waltham, C E / Wang, J-X / Wark, D L / West, N / Wilhelmy, J B / Wilkerson, J F / Wilson, J R / Wittich, P / Wouters, J M / Yeh, M

Physical review letters

2002 Volume 89, Issue 1, Page(s) 11301

Abstract: Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported. Using the neutral current (NC), elastic scattering, and charged current reactions and assuming the standard 8B shape, the nu(e) component of ... ...

Abstract	Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported. Using the neutral current (NC), elastic scattering, and charged current reactions and assuming the standard 8B shape, the nu(e) component of the 8B solar flux is phis(e) = 1.76(+0.05)(-0.05)(stat)(+0.09)(-0.09)(syst) x 10(6) cm(-2) s(-1) for a kinetic energy threshold of 5 MeV. The non-nu(e) component is phi(mu)(tau) = 3.41(+0.45)(-0.45)(stat)(+0.48)(-0.45)(syst) x 10(6) cm(-2) s(-1), 5.3sigma greater than zero, providing strong evidence for solar nu(e) flavor transformation. The total flux measured with the NC reaction is phi(NC) = 5.09(+0.44)(-0.43)(stat)(+0.46)(-0.43)(syst) x 10(6) cm(-2) s(-1), consistent with solar models.
Language	English
Publishing date	2002-07-01
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.89.011301
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters.

Ahmad, Q R / Allen, R C / Andersen, T C / Anglin, J D / Barton, J C / Beier, E W / Bercovitch, M / Bigu, J / Biller, S D / Black, R A / Blevis, I / Boardman, R J / Boger, J / Bonvin, E / Boulay, M G / Bowler, M G / Bowles, T J / Brice, S J / Browne, M C /

Physical review letters

2002 Volume 89, Issue 1, Page(s) 11302

Abstract: The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted 8B spectrum, the night minus day rate is 14.0%+/-6.3%(+1.5%)(-1.4%) of the average rate. If the ...

Abstract	The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted 8B spectrum, the night minus day rate is 14.0%+/-6.3%(+1.5%)(-1.4%) of the average rate. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the nu(e) asymmetry is found to be 7.0%+/-4.9%(+1.3%)(-1.2%). A global solar neutrino analysis in terms of matter-enhanced oscillations of two active flavors strongly favors the large mixing angle solution.
Language	English
Publishing date	2002-07-01
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.89.011302
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article: Measurement of the rate of nu(e) + d --> p + p + e(-) interactions produced by (8)B solar neutrinos at the Sudbury Neutrino Observatory.

Ahmad, Q R / Allen, R C / Andersen, T C / Anglin, J D / Bühler, G / Barton, J C / Beier, E W / Bercovitch, M / Bigu, J / Biller, S / Black, R A / Blevis, I / Boardman, R J / Boger, J / Bonvin, E / Boulay, M G / Bowler, M G / Bowles, T J / Brice, S J /

Browne, M C / Bullard, T V / Burritt, T H / Cameron, K / Cameron, J / Chan, Y D / Chen, M / Chen, H H / Chen, X / Chon, M C / Cleveland, B T / Clifford, E T / Cowan, J H / Cowen, D F / Cox, G A / Dai, Y / Dai, X / Dalnoki-Veress, F / Davidson, W F / Doe, P J / Doucas, G / Dragowsky, M R / Duba, C A / Duncan, F A / Dunmore, J / Earle, E D / Elliott, S R / Evans, H C / Ewan, G T / Farine, J / Fergani, H / Ferraris, A P / Ford, R J / Fowler, M M / Frame, K / Frank, E D / Frati, W / Germani, J V / Gil, S / Goldschmidt, A / Grant, D R / Hahn, R L / Hallin, A L / Hallman, E D / Hamer, A / Hamian, A A / Haq, R U / Hargrove, C K / Harvey, P J / Hazama, R / Heaton, R / Heeger, K M / Heintzelman, W J / Heise, J / Helmer, R L / Hepburn, J D / Heron, H / Hewett, J / Hime, A / Howe, M / Hykawy, J G / Isaac, M C / Jagam, P / Jelley, N A / Jillings, C / Jonkmans, G / Karn, J / Keener, P T / Kirch, K / Klein, J R / Knox, A B / Komar, R J / Kouzes, R / Kutter, T / Kyba, C C / Law, J / Lawson, I T / Lay, M / Lee, H W / Lesko, K T / Leslie, J R / Levine, I / Locke, W / Lowry, M M / Luoma, S / Lyon, J / Majerus, S / Mak, H B / Marino, A D / McCauley, N / McDonald, A B / McDonald, D S / McFarlane, K / McGregor, G / McLatchie, W / Meijer Drees, R / Mes, H / Mifflin, C / Miller, G G / Milton, G / Moffat, B A / Moorhead, M / Nally, C W / Neubauer, M S / Newcomer, F M / Ng, H S / Noble, A J / Norman, E B / Novikov, V M / O'Neill, M / Okada, C E / Ollerhead, R W / Omori, M / Orrell, J L / Oser, S M / Poon, A W / Radcliffe, T J / Roberge, A / Robertson, B C / Robertson, R G / Rowley, J K / Rusu, V L / Saettler, E / Schaffer, K K / Schuelke, A / Schwendener, M H / Seifert, H / Shatkay, M / Simpson, J J / Sinclair, D / Skensved, P / Smith, A R / Smith, M W / Starinsky, N / Steiger, T D / Stokstad, R G / Storey, R S / Sur, B / Tafirout, R / Tagg, N / Tanner, N W / Taplin, R K / Thorman, M / Thornewell, P / Trent, P T / Tserkovnyak, Y I / Van Berg, R / Van de Water, R G / Virtue, C J / Waltham, C E / Wang, J X / Wark, D L / West, N / Wilhelmy, J B / Wilkerson, J F / Wilson, J / Wittich, P / Wouters, J M / Yeh, M

Physical review letters

2001 Volume 87, Issue 7, Page(s) 71301

Abstract: Solar neutrinos from (8)B decay have been detected at the Sudbury Neutrino Observatory via the charged current (CC) reaction on deuterium and the elastic scattering (ES) of electrons. The flux of nu(e)'s is measured by the CC reaction rate to be straight ...

Abstract	Solar neutrinos from (8)B decay have been detected at the Sudbury Neutrino Observatory via the charged current (CC) reaction on deuterium and the elastic scattering (ES) of electrons. The flux of nu(e)'s is measured by the CC reaction rate to be straight phi(CC)(nu(e)) = 1.75 +/- 0.07(stat)(+0.12)(-0.11)(syst) +/- 0.05(theor) x 10(6) cm(-2) s(-1). Comparison of straight phi(CC)(nu(e)) to the Super-Kamiokande Collaboration's precision value of the flux inferred from the ES reaction yields a 3.3 sigma difference, assuming the systematic uncertainties are normally distributed, providing evidence of an active non- nu(e) component in the solar flux. The total flux of active 8B neutrinos is determined to be 5.44+/-0.99 x 10(6) cm(-2) s(-1).
Language	English
Publishing date	2001-08-13
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.87.071301
Database	MEDical Literature Analysis and Retrieval System OnLINE

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