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Solar neutrino measurements in Super-Kamiokande-IV
Authors
K. Abe,Y. Haga
Y. Hayato,M. Ikeda,K. Iyogi,J. Kameda,Y. Kishimoto,Ll. Marti,M. Miura,S. Moriyama,M. Nakahata,Tomoki NAKAJIMA,S. Nakayama,A. Orii,H. Sekiya,M. Shiozawa,Y. Sonoda,A. Takeda,H. Tanaka,Y. Takenaga,S. Tasaka,T. Tomura,K. Ueno,T. Yokozawa,R. Akutsu,T. Irvine,H. Kaji,T. Kajita,I. Kametani,K. Kaneyuki,K. Lee,Y. Nishimura,T. Mclachlan,K. Okumura,E. Richard,L. Labarga,P. Fernández,F. Blaszczyk,J. Gustafson,C. Kachulis,E. Kearns,J. Raaf,J. Stone,L. Sulak,S. Berkman,S. Tobayama,M. Goldhaber,K. Bays,G. Carminati,N. Griskevich,W. Kropp,S. Mine,A. Renshaw,M. Smy,H. Sobel,Volodymyr Takhistov,P. Weatherly,K. Ganezer,B. Hartfiel,J. Hill,W. Keig,Nguyễn Hồng,J. Kim,I. Lim,R. Park,T. Akiri,J. Albert,A. Himmel,Z. Li,Erin O’Sullivan,K. Scholberg,C. Walter,T. Wongjirad,T. Ishizuka,T. Nakamura,J. Jang,K. Choi,J. Learned,S. Matsuno,S. Smith,M. Friend,T. Hasegawa,Toru Ishida,T. Ishii,T. Kobayashi,T. Nakadaira,K. Nakamura,K. Nishikawa,Y. Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,Y. Nakano,Y. Suzuki,Y. Takeuchi,T. Yano,S. Cao,T. Hayashino,T. Hiraki,S. Hirota,K. Huang,K. Ieki,M. Jiang,T. Kikawa,A. Minamino,A. Murakami,T. Nakaya,N. Patel,Kenta Suzuki,Sentaro Takahashi,R. Wendell,Y. Fukuda,Y. Itow,G. Mitsuka,F. Muto,T. Suzuki,P. Mijakowski,K. Frankiewicz,J. Hignight,J. Imber,C. Jung,X. Li,J. Palomino,G. Santucci,Ian Taylor,C. Vilela,M. Wilking,C. Yanagisawa,D. Fukuda,H. Ishino,T. Kayano,A. Kibayashi,Y. Koshio,T. Mori,M. Sakuda,J. Takeuchi,R. Yamaguchi,Y. Kuno,R. Tacik,S. Kim,H. Okazawa,Y. Choi,Kei Ito,K. Nishijima,M. Koshiba,Y. Totsuka,Y. Suda,M. Yokoyama,C. Bronner,R. Calland,M. Hartz,K. Martens,Y. Obayashi,M. Vagins,C. Nantais,J. Martin,P. Perio,A. Konaka,S. Chen,Hongjie Sui,L. Wan,Z. Yang,H. Zhang,Yang Zhang,K. Connolly,M. Dziomba,R. Wilkes,Young-Il Choi,Thomas Mclachlan,P. Fernåndez,V. Radeka
+169 authors
,Wolfgang WalterPublished
Sep 20, 2016
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Abstract
After important upgrades to the experiment, the Super-Kamiokande collaboration returns to measuring the solar mixing angle and the mass splitting $\mathrm{\ensuremath{\Delta}}\phantom{\rule{0}{0ex}}{m}_{12}^{2}$. By focusing on low-energy ${}^{8}B$ neutrinos, the collaboration is able to single out neutrinos that undergo flavor conversion only through vacuum oscillations. The results are the currently most precise values for the mixing and mass-difference parameters relevant for vacuum solar neutrino oscillations.
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