Precise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I
Precise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I
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DOI:
10.1103/physrevd.69.011104
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发表时间:
2004-01
影响因子:
5
通讯作者:
M. Smy;M. Earl;T. Iwashita;J. Kameda;G. Sullivan;N. Sakurai;K. Ishihara;D. Kiełczewska;K. Inoue;A. Stachyra;S. Dazeley;H. Takeuchi;S. Fukuda;Y. Choi;A. Suzuki;T. Maruyama;W. Gajewski;H. Ishino;K. Miyano;L. Sulak;Y. Totsuka;Y. Takeuchi;C. Saji;J. Zalipska;M. Koshiba;K. Ganezer;A. Habig;M. Sakuda;T. Ooyabu;R. Ellsworth;H. Kim;J. Shirai;W. Keig;S. Nakayama;E. Kearns;T. Nakaya;Y. Fukuda;Y. Koshio;D. Turcan;Y. Nagashima;R. Wilkes;J. Hill;S. Mine;M. Vagins;T. Namba;T. Kajita;M. Shiozawa;K. Martens;R. Nishimura;I. Lim;J. Goodman;Y. Gando;W. Wang;H. Sobel;T. Toshito;M. Nakahata;Tetsuya Kobayashi;R. Svoboda;K. Nishijima;B. Viren;R. Nambu;T. Inagaki;K. Scholberg;M. Miura;A. Gago;Michitoshi Yoshida;I. Kato;C. Jung;M. Ishitsuka;M. Koike;D. Casper;M. Etoh;G. Guillian;A. Ichikawa;A. Okada;S. Yamada;J. Kim;T. Ishizuka;M. Ackermann;S. Hatakeyama;T. Kato;D. Takemori;Y. Obayashi;S. Matsuno;E. Blaufuss;K. Nakamura;Y. Hayato;C. Mcgrew;S. Kim;M. Goldhaber;J. Yoo;J. Stone;T. Ishii;H. Berns;D. Liu;Y. Oyama;T. Barszczak;C. Yanagisawa;A. Kibayashi;M. Takita;S. Boyd;T. Shibata;S. Moriyama;C. Mitsuda;A. Suzuki;C. Walter;Y. Itow;W. Kropp;M. Małek;H. Seo;Y. Kajiyama;J. Learned;S. Desai;K. Kaneyuki;Y. Ashie;K. Nishikawa;A. Minamino;Y. Ichikawa;K. Kobayashi;Y. Hatakeyama;K. Nitta;H. Okazawa;C. Mauger;M. Morii;Y. Suzuki;Y. Watanabe;T. Haines;T. Hasegawa;E. Sharkey;S. Tasaka
中科院分区:
文献类型:
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作者:
M. Smy;M. Earl;T. Iwashita;J. Kameda;G. Sullivan;N. Sakurai;K. Ishihara;D. Kiełczewska;K. Inoue;A. Stachyra;S. Dazeley;H. Takeuchi;S. Fukuda;Y. Choi;A. Suzuki;T. Maruyama;W. Gajewski;H. Ishino;K. Miyano;L. Sulak;Y. Totsuka;Y. Takeuchi;C. Saji;J. Zalipska;M. Koshiba;K. Ganezer;A. Habig;M. Sakuda;T. Ooyabu;R. Ellsworth;H. Kim;J. Shirai;W. Keig;S. Nakayama;E. Kearns;T. Nakaya;Y. Fukuda;Y. Koshio;D. Turcan;Y. Nagashima;R. Wilkes;J. Hill;S. Mine;M. Vagins;T. Namba;T. Kajita;M. Shiozawa;K. Martens;R. Nishimura;I. Lim;J. Goodman;Y. Gando;W. Wang;H. Sobel;T. Toshito;M. Nakahata;Tetsuya Kobayashi;R. Svoboda;K. Nishijima;B. Viren;R. Nambu;T. Inagaki;K. Scholberg;M. Miura;A. Gago;Michitoshi Yoshida;I. Kato;C. Jung;M. Ishitsuka;M. Koike;D. Casper;M. Etoh;G. Guillian;A. Ichikawa;A. Okada;S. Yamada;J. Kim;T. Ishizuka;M. Ackermann;S. Hatakeyama;T. Kato;D. Takemori;Y. Obayashi;S. Matsuno;E. Blaufuss;K. Nakamura;Y. Hayato;C. Mcgrew;S. Kim;M. Goldhaber;J. Yoo;J. Stone;T. Ishii;H. Berns;D. Liu;Y. Oyama;T. Barszczak;C. Yanagisawa;A. Kibayashi;M. Takita;S. Boyd;T. Shibata;S. Moriyama;C. Mitsuda;A. Suzuki;C. Walter;Y. Itow;W. Kropp;M. Małek;H. Seo;Y. Kajiyama;J. Learned;S. Desai;K. Kaneyuki;Y. Ashie;K. Nishikawa;A. Minamino;Y. Ichikawa;K. Kobayashi;Y. Hatakeyama;K. Nitta;H. Okazawa;C. Mauger;M. Morii;Y. Suzuki;Y. Watanabe;T. Haines;T. Hasegawa;E. Sharkey;S. Tasaka
The time variation of the elastic scattering rate of solar neutrinos with electrons in Super-Kamiokande-I was fit to the variations expected from active two-neutrino oscillations. The best fit in the Large Mixing Angle solution has a mixing angle of tan^2theta=0.55 and a mass squared difference of Deltam^2=6.3times10^-5eV^2 between the two neutrino mass eigenstates. The fitted day/night asymmetry of -1.8+-1.6(stat)+1.3-1.2(syst)% has improved statistical precision over previous measurements and agrees well with the expected asymmetry of -2.1%.