Direct Measurement Of The (7)Be Solar Neutrino Flux With 192 Days Of Borexino Data

C. Arpesella,H. Back,M. Balata,G. Bellini,J. Benziger,S. Bonetti,A. Brigatti,B. Caccianiga,L. Cadonati,F. Calaprice,C. Carraro,G. Cecchet,A. Chavarria,M. Chen,F. Dalnoki-Veress,D. D’Angelo,A. de Bari,A. de Bellefon,H. de Kerret,A. Derbin,M. Deutsch,A. di Credico,G. di Pietro,R. Eisenstein,F. Elisei,A. Etenko,R. Fernholz,K. Fomenko,R. Ford,D. Franco,B. Freudiger,C. Galbiati,F. Gatti,S. Gazzana,M. Giammarchi, D. Giugni,M. Goeger-Neff,T. Goldbrunner,A. Goretti,C. Grieb,C. Hagner,W. Hampel,E. Harding,S. Hardy, F. Hartman,T. Hertrich,G. Heusser,Aldo Ianni,Andrea Ianni,M. Joyce,J. Kiko,T. Kirsten,V. Kobychev,G. Korga,G. Korschinek,D. Kryn,V. Lagomarsino,P. Lamarche,M. Laubenstein,C. Lendvai,M. Leung,T. Lewke,E. Litvinovich,B. Loer,P. Lombardi,L. Ludhova,I. Machulin,S. Malvezzi,S. Manecki,J. Maneira,W. Maneschg,I. Manno,D. Manuzio,G. Manuzio,A. Martemianov,F. Masetti,U. Mazzucato,K. McCarty,D. McKinsey,Q. Meindl,E. Meroni,L. Miramonti,M. Misiaszek,D. Montanari,M. Monzani,V. Muratova,P. Musico,H. Neder,A. Nelson,L. Niedermeier, L. Oberauer,M. Obolensky,M. Orsini,F. Ortica,M. Pallavicini,L. Papp,S. Parmeggiano,L. Perasso,A. Pocar,R. Raghavan,G. Ranucci,W. Rau,A. Razeto,E. Resconi,P. Risso,A. Romani,D. Rountree,A. Sabelnikov,R. Saldanha,C. Salvo,D. Schimizzi,S. Schönert,T. Shutt,H. Simgen,M. Skorokhvatov,O. Smirnov,A. Sonnenschein,A. Sotnikov,S. Sukhotin,Y. Suvorov,R. Tartaglia,G. Testera,D. Vignaud,S. Vitale,R. Vogelaar,F. von Feilitzsch,R. von Hentig,T. von Hentig,M. Wojcik,M. Wurm,O. Zaimidoroga,S. Zavatarelli,G. Zuzel

PHYSICAL REVIEW LETTERS(2008)

引用 397|浏览72
暂无评分
摘要
We report the direct measurement of the 7 Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV (7)Be neutrinos is 49 +/- 3(stat) +/- 4(syst) counts/(day . 100 ton). The hypothesis of no oscillation for (7)Be solar neutrinos is inconsistent with our measurement at the 4 sigma C.L. Our result is the first direct measurement of the survival probability for solar P, in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of (7)Be, pp, and CNO solar v(e) and the limit on the effective neutrino magnetic moment using solar neutrinos.
更多
查看译文
关键词
beryllium,elementary particles,magnetic moments,cosmic ray,solar neutrinos,magnetic moment,neutrino oscillation,solar radiation,oscillations
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要