Autores
B Aharmim, SN Ahmed, JF Amsbaugh, AE Anthony, J Banar, N Barros, EW Beier, Alain Bellerive, B Beltran, M Bergevin, SD Biller, K Boudjemline, Mark Guy Boulay, TJ Bowles, MC Browne, TV Bullard, TH Burritt, B Cai, YD Chan, D Chauhan, M Chen, BT Cleveland, GA Cox-Mobrand, CA Currat, X Dai, H Deng, J Detwiler, M DiMarco, PJ Doe, G Doucas, P-L Drouin, CA Duba, FA Duncan, M Dunford, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, F Fleurot, RJ Ford, JA Formaggio, MM Fowler, N Gagnon, JV Germani, A Goldschmidt, JTM Goon, K Graham, E Guillian, S Habib, RL Hahn, AL Hallin, ED Hallman, AA Hamian, GC Harper, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, R Henning, A Hime, C Howard, MA Howe, M Huang, P Jagam, B Jamieson, NA Jelley, KJ Keeter, JR Klein, LL Kormos, M Kos, A Krüger, C Kraus, CB Krauss, T Kutter, CCM Kyba, R Lange, J Law, IT Lawson, KT Lesko, JR Leslie, JC Loach, R MacLellan, S Majerus, HB Mak, J Maneira, R Martin, K McBryde, N McCauley, AB McDonald, S McGee, C Mifflin, GG Miller, ML Miller, B Monreal, J Monroe, B Morissette, A Myers, BG Nickel, AJ Noble, NS Oblath, HM O’Keeffe, RW Ollerhead, GD Orebi Gann, SM Oser, RA Ott, SJM Peeters, AWP Poon, G Prior, SD Reitzner, K Rielage, BC Robertson, RGH Robertson, E Rollin, MH Schwendener, JA Secrest, SR Seibert, O Simard, JJ Simpson, L Sinclair, P Skensved, MWE Smith, TD Steiger, LC Stonehill, G Tešić, PM Thornewell, N Tolich, T Tsui, CD Tunnell, T Van Wechel, R Van Berg, BA VanDevender, CJ Virtue, TJ Walker, BL Wall, D Waller, H Wan Chan Tseung, J Wendland, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, JM Wouters, A Wright, M Yeh, F Zhang, K Zuber
Fecha de publicación
2008/9/9
Revista
Physical Review Letters
Volumen
101
Número
11
Páginas
111301
Editor
American Physical Society
Descripción
The Sudbury Neutrino Observatory (SNO) used an array of He 3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (ν x) B 8 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)× 10 6 cm− 2 s− 1, in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Δ m 2= 7.59− 0.21+ 0.19× 10− 5 eV 2 and θ= 34.4− 1.2+ 1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO’s previous results.
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Artículos de Google Académico
B Aharmim, SN Ahmed, JF Amsbaugh, AE Anthony… - Physical Review Letters, 2008
