Literature DB >> 18851271

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

B Aharmim1, 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 Tesić, 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.   

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.

Entities:  

Year:  2008        PMID： 18851271     DOI： 10.1103/PhysRevLett.101.111301

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN： 0031-9007            Impact factor:   9.161


  4 in total

Review 1.  Astroparticle physics with solar neutrinos.

Authors:  Masayuki Nakahata
Journal:  Proc Jpn Acad Ser B Phys Biol Sci       Date:  2011       Impact factor: 3.493

2.  Prospects for beyond the Standard Model physics searches at the Deep Underground Neutrino Experiment: DUNE Collaboration.

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M Bonesini; M Bongrand; F Bonini; A Booth; C Booth; S Bordoni; A Borkum; T Boschi; N Bostan; P Bour; S B Boyd; D Boyden; J Bracinik; D Braga; D Brailsford; A Brandt; J Bremer; C Brew; E Brianne; S J Brice; C Brizzolari; C Bromberg; G Brooijmans; J Brooke; A Bross; G Brunetti; N Buchanan; H Budd; D Caiulo; P Calafiura; J Calcutt; M Calin; S Calvez; E Calvo; L Camilleri; A Caminata; M Campanelli; D Caratelli; G Carini; B Carlus; P Carniti; I Caro Terrazas; H Carranza; A Castillo; C Castromonte; C Cattadori; F Cavalier; F Cavanna; S Centro; G Cerati; A Cervelli; A Cervera Villanueva; M Chalifour; C Chang; E Chardonnet; A Chatterjee; S Chattopadhyay; J Chaves; H Chen; M Chen; Y Chen; D Cherdack; C Chi; S Childress; A Chiriacescu; K Cho; S Choubey; A Christensen; D Christian; G Christodoulou; E Church; P Clarke; T E Coan; A G Cocco; J A B Coelho; E Conley; J M Conrad; M Convery; L Corwin; P Cotte; L Cremaldi; L Cremonesi; J I Crespo-Anadón; E Cristaldo; R Cross; C Cuesta; Y Cui; D Cussans; 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D Franco; J Freeman; J Freestone; J Fried; A Friedland; S Fuess; I Furic; A P Furmanski; A Gago; H Gallagher; A Gallego-Ros; N Gallice; V Galymov; E Gamberini; T Gamble; R Gandhi; R Gandrajula; S Gao; D Garcia-Gamez; M Á García-Peris; S Gardiner; D Gastler; G Ge; B Gelli; A Gendotti; S Gent; Z Ghorbani-Moghaddam; D Gibin; I Gil-Botella; C Girerd; A K Giri; D Gnani; O Gogota; M Gold; S Gollapinni; K Gollwitzer; R A Gomes; L V Gomez Bermeo; L S Gomez Fajardo; F Gonnella; J A Gonzalez-Cuevas; M C Goodman; O Goodwin; S Goswami; C Gotti; E Goudzovski; C Grace; M Graham; E Gramellini; R Gran; E Granados; A Grant; C Grant; D Gratieri; P Green; S Green; L Greenler; M Greenwood; J Greer; W C Griffith; M Groh; J Grudzinski; K Grzelak; W Gu; V Guarino; R Guenette; A Guglielmi; B Guo; K K Guthikonda; R Gutierrez; P Guzowski; M M Guzzo; S Gwon; A Habig; A Hackenburg; H Hadavand; R Haenni; A Hahn; J Haigh; J Haiston; T Hamernik; P Hamilton; J Han; K Harder; D A Harris; J Hartnell; T Hasegawa; R Hatcher; 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T Usher; M R Vagins; P Vahle; G A Valdiviesso; E Valencia; Z Vallari; J W F Valle; S Vallecorsa; R Van Berg; R G Van de Water; D Vanegas Forero; F Varanini; D Vargas; G Varner; J Vasel; G Vasseur; K Vaziri; S Ventura; A Verdugo; S Vergani; M A Vermeulen; M Verzocchi; H Vieira de Souza; C Vignoli; C Vilela; B Viren; T Vrba; T Wachala; A V Waldron; M Wallbank; H Wang; J Wang; Y Wang; Y Wang; K Warburton; D Warner; M Wascko; D Waters; A Watson; P Weatherly; A Weber; M Weber; H Wei; A Weinstein; D Wenman; M Wetstein; M R While; A White; L H Whitehead; D Whittington; M J Wilking; C Wilkinson; Z Williams; F Wilson; R J Wilson; J Wolcott; T Wongjirad; K Wood; L Wood; E Worcester; M Worcester; C Wret; W Wu; W Wu; Y Xiao; G Yang; T Yang; N Yershov; K Yonehara; T Young; B Yu; J Yu; R Zaki; J Zalesak; L Zambelli; B Zamorano; A Zani; L Zazueta; G P Zeller; J Zennamo; K Zeug; C Zhang; M Zhao; Y Zhao; E Zhivun; G Zhu; E D Zimmerman; M Zito; S Zucchelli; J Zuklin; V Zutshi; R Zwaska
Journal:  Eur Phys J C Part Fields       Date:  2021-04-16       Impact factor: 4.590

Review 3.  The Sun, neutrinos and Super-Kamiokande.

Authors:  Yoichiro Suzuki
Journal:  Proc Jpn Acad Ser B Phys Biol Sci       Date:  2020       Impact factor: 3.493

4.  Different paradigms of transcranial electrical stimulation improve motor function impairment and striatum tissue injuries in the collagenase-induced intracerebral hemorrhage rat model.

Authors:  Amir Reza Heidarzadegan; Asadollah Zarifkar; Narges Sotoudeh; Mohammad Reza Namavar; Amir Hossein Zarifkar
Journal:  BMC Neurosci       Date:  2022-01-29       Impact factor: 3.288
  4 in total

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