Solar neutrino results in Super-Kamiokande-III

Abe, K.; Hayato, Y.; Iida, T.; Ikeda, M.; Ishihara, C.; Iyogi, K.; Kameda, J.; Kobayashi, Kazuyoshi; Koshio, Y.; Kozuma, Y.; Miura, M.; Moriyama, S.; Nakahata, M.; Nakayama, S.; Obayashi, Y.; Ogawa, Hiroshi; Sekiya, H.; Shiozawa, M.; Suzuki, Y.; Takeda, A.; Takenaga, Y.; Ueno, K.; Ueshima, K.; Watanabe, H.; Yamada, S.; Yokozawa, T.; Hazama, S.; Kaji, H.; Kajita, T.; Kaneyuki, K.; C. Mclachlan, T.; Okumura, K.; Shimizu, Yuki; Tanimoto, N.; R. Vagins, M.; Labarga, L.; M. Magro, L.; Dufour, Frédéric; Kearns, E.; Litos, M.; L. Raaf, J.; L. Stone, J.; Sulak, L.; Wang, W.; Goldhaber, M.; Bays, K.; Casper, D.; P. Cravens, J.; R. Kropp, W.; Mine, S.; Regis, C.; Renshaw, A.; Smy, M.; W. Sobel, H.; S. Ganezer, K.; Hill, J.; E. Keig, W.; S. Jang, J.; Y. Kim, J.; T. Lim, I.; Albert, J.; Wendell, R.; Wongjirad, T.; Scholberg, K.; W. Walter, C.; Ishizuka, T.; Tasaka, S.; G. Learned, J.; Matsuno, S.; Watanabe, Y.; Hasegawa, T.; Ishida, Toru; Ishii, T.; Kobayashi, T.; Nakadaira, T.; Nakamura, K.; Nishikawa, K.; Nishino, H.; Oyama, Y.; Sakashita, K.; Sekiguchi, T.; Tsukamoto, T.; Suzuki, Y.; Takeuchi, Y.; Minamino, A.; Nakaya, T.; Fukuda, Y.; Itow, Y.; Mitsuka, G.; Tanaka, Takayuki; K. Jung, C.; Lopez, G.; McGrew, C.; Terri, R.; Yanagisawa, C.; Tamura, N.; Ishino, H.; Kibayashi, A.; Mino, S; Mori, T.; Sakuda, M.; Toyota, H.; Kuno, Y.; Yoshida, M.; B. Kim, S.; S. Yang, B.; Ishizuka, T.; Okazawa, H.; Choi, Y.; Nishijima, K.; Yokosawa, Y.; Koshiba, M.; Totsuka, Y.; Yokoyama, M.; Chen, S.; K. Heng, Y.; Yang, Z.; Zhang, H.; Kiełczewska, D.; Mijakowski, P.; Connolly, K.; Dziomba, M.; Thrane, E.; J. Wilkes, R.

doi:10.1103/physrevd.83.052010

Public

Solar neutrino results in Super-Kamiokande-III

Published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology • Mar 24, 2011

Authors:

K. Abe

Y. Hayato

T. Iida

Abstract

The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results. With improved detector calibrations, a full detector simulation, and improved analysis methods, the systematic uncertainty on the total neutrino flux is...

Subject

Physics

Super-Kamiokande

Neutrino oscillation

Research Assistant

AI chat, annotations, notes & similar papers

Finding related papers...

Discussions

(0)

No comments yet

Be the first to share your thoughts!