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Independent measurement of the total active 8B solar neutrino flux using an array of 3He proportional counters at the sudbury neutrino observatory

  • B. Aharmim
  • , S. N. Ahmed
  • , J. F. Amsbaugh
  • , A. E. Anthony
  • , J. Banar
  • , N. Barros
  • , E. W. Beier
  • , A. Bellerive
  • , B. Beltran
  • , M. Bergevin
  • , S. D. Biller
  • , K. Boudjemline
  • , M. G. Boulay
  • , T. J. Bowles
  • , M. C. Browne
  • , T. V. Bullard
  • , T. H. Burritt
  • , B. Cai
  • , Y. D. Chan
  • , D. Chauhan
  • M. Chen, B. T. Cleveland, G. A. Cox-Mobrand, C. A. Currat, X. Dai, H. Deng, J. Detwiler, M. Dimarco, P. J. Doe, G. Doucas, P. L. Drouin, C. A. Duba, F. A. Duncan, M. Dunford, E. D. Earle, S. R. Elliott, H. C. Evans, G. T. Ewan, J. Farine, H. Fergani, F. Fleurot, R. J. Ford, J. A. Formaggio, M. M. Fowler, N. Gagnon, J. V. Germani, A. Goldschmidt, J. T.M. Goon, K. Graham, E. Guillian, S. Habib, R. L. Hahn, A. L. Hallin, E. D. Hallman, A. A. Hamian, G. C. Harper, P. J. Harvey, R. Hazama, K. M. Heeger, W. J. Heintzelman, J. Heise, R. L. Helmer, R. Henning, A. Hime, C. Howard, M. A. Howe, M. Huang, P. Jagam, B. Jamieson, N. A. Jelley, K. J. Keeter, J. R. Klein, L. L. Kormos, M. Kos, A. Krüger, C. Kraus, C. B. Krauss, T. Kutter, C. C.M. Kyba, R. Lange, J. Law, I. T. Lawson, K. T. Lesko, J. R. Leslie, J. C. Loach, R. MacLellan, S. Majerus, H. B. Mak, J. Maneira, R. Martin, K. McBryde, N. McCauley, A. B. McDonald, S. McGee, C. Mifflin, G. G. Miller, M. L. Miller, B. Monreal, J. Monroe, B. Morissette, A. Myers, B. G. Nickel, A. J. Noble, N. S. Oblath, H. M. O'Keeffe, R. W. Ollerhead, G. D.Orebi Gann, S. M. Oser, R. A. Ott, S. J.M. Peeters, A. W.P. Poon, G. Prior, S. D. Reitzner, K. Rielage, B. C. Robertson, R. G.H. Robertson, E. Rollin, M. H. Schwendener, J. A. Secrest, S. R. Seibert, O. Simard, J. J. Simpson, L. Sinclair, P. Skensved, M. W.E. Smith, T. D. Steiger, L. C. Stonehill, G. Tešić, P. M. Thornewell, N. Tolich, T. Tsui, C. D. Tunnell, T. Van Wechel, R. Van Berg, B. A. Vandevender, C. J. Virtue, T. J. Walker, B. L. Wall, D. Waller, H. Wan Chan Tseung, J. Wendland, N. West, J. B. Wilhelmy, J. F. Wilkerson, J. R. Wilson, J. M. Wouters, A. Wright, M. Yeh, F. Zhang, K. Zuber
  • Laurentian University
  • Queen's University
  • University of Washington
  • The University of Texas at Austin
  • MST-8, Los Alamos National Laboratory
  • Laboratório de Instrumentação
  • University of Pennsylvania School of Arts and Sciences
  • Carleton University
  • University of Alberta
  • University of Guelph
  • Ernest Orlando Lawrence Berkeley National Laboratory
  • University of Oxford
  • Massachusetts Institute of Technology
  • Louisiana State University
  • Brookhaven National Laboratory
  • University of British Columbia
  • TRIUMF
  • SNOLAB

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Résumé

The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (νx) B8 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)×106cm-2s-1, in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Δm2=7.59-0.21+0.19×10-5eV2 and θ=34.4-1.2+1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO's previous results.

langue originaleAnglais
Numéro d'article111301
journalPhysical Review Letters
Volume101
Numéro de publication11
Les DOIs
étatPublié - 9 sept. 2008
Modification externeOui

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