| Literature DB >> 11497878 |
Q R Ahmad1, R C Allen, T C Andersen, J D Anglin, G Bühler, J C Barton, E W Beier, M Bercovitch, J Bigu, S Biller, R A Black, I Blevis, R J Boardman, J Boger, E Bonvin, M G Boulay, M G Bowler, T J Bowles, S J Brice, M C Browne, T V Bullard, T H Burritt, K Cameron, J Cameron, Y D Chan, M Chen, H H Chen, X Chen, M C Chon, B T Cleveland, E T Clifford, J H Cowan, D F Cowen, G A Cox, Y Dai, X Dai, F Dalnoki-Veress, W F Davidson, P J Doe, G Doucas, M R Dragowsky, C A Duba, F A Duncan, J Dunmore, E D Earle, S R Elliott, H C Evans, G T Ewan, J Farine, H Fergani, A P Ferraris, R J Ford, M M Fowler, K Frame, E D Frank, W Frati, J V Germani, S Gil, A Goldschmidt, D R Grant, R L Hahn, A L Hallin, E D Hallman, A Hamer, A A Hamian, R U Haq, C K Hargrove, P J Harvey, R Hazama, R Heaton, K M Heeger, W J Heintzelman, J Heise, R L Helmer, J D Hepburn, H Heron, J Hewett, A Hime, M Howe, J G Hykawy, M C Isaac, P Jagam, N A Jelley, C Jillings, G Jonkmans, J Karn, P T Keener, K Kirch, J R Klein, A B Knox, R J Komar, R Kouzes, T Kutter, C C Kyba, J Law, I T Lawson, M Lay, H W Lee, K T Lesko, J R Leslie, I Levine, W Locke, M M Lowry, S Luoma, J Lyon, S Majerus, H B Mak, A D Marino, N McCauley, A B McDonald, D S McDonald, K McFarlane, G McGregor, W McLatchie, R Meijer Drees, H Mes, C Mifflin, G G Miller, G Milton, B A Moffat, M Moorhead, C W Nally, M S Neubauer, F M Newcomer, H S Ng, A J Noble, E B Norman, V M Novikov, M O'Neill, C E Okada, R W Ollerhead, M Omori, J L Orrell, S M Oser, A W Poon, T J Radcliffe, A Roberge, B C Robertson, R G Robertson, J K Rowley, V L Rusu, E Saettler, K K Schaffer, A Schuelke, M H Schwendener, H Seifert, M Shatkay, J J Simpson, D Sinclair, P Skensved, A R Smith, M W Smith, N Starinsky, T D Steiger, R G Stokstad, R S Storey, B Sur, R Tafirout, N Tagg, N W Tanner, R K Taplin, M Thorman, P Thornewell, P T Trent, Y I Tserkovnyak, R Van Berg, R G Van de Water, C J Virtue, C E Waltham, J X Wang, D L Wark, N West, J B Wilhelmy, J F Wilkerson, J Wilson, P Wittich, J M Wouters, M Yeh.
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).Entities:
Year: 2001 PMID： 11497878 DOI： 10.1103/PhysRevLett.87.071301
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161