Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data

D. W. Liu, Y. Ashie, S. Fukuda, Y. Fukuda, K. Ishihara, Y. Itow, Y. Koshio, A. Minamino, M. Miura, S. Moriyama, M. Nakahata, T. Namba, R. Nambu, Y. Obayashi, N. Sakurai, M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, S. YamadaM. Ishitsuka, T. Kajita, K. Kaneyuki, S. Nakayama, A. Okada, T. Ooyabu, C. Saji, S. Desai, M. Earl, E. Kearns, M. D. Messier, J. L. Stone, L. R. Sulak, C. W. Walter, W. Wang, T. Barszczak, D. Casper, J. P. Cravens, W. Gajewski, W. R. Kropp, S. Mine, M. B. Smy, H. W. Sobel, C. W. Sterner, M. R. Vagins, K. S. Ganezer, J. Hill, W. E. Keig, J. Y. Kim, I. T. Lim, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, J. Kameda, T. Kobayashi, T. Maruyama, K. Nakamura, K. Nitta, Y. Oyama, M. Sakuda, Y. Totsuka, A. T. Suzuki, M. Hasegawa, K. Hayashi, T. Inagaki, I. Kato, H. Maesaka, T. Morita, T. Nakaya, K. Nishikawa, T. Sasaki, S. Ueda, S. Yamamoto, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, J. A. Goodman, G. Guillian, G. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, M. Ackermann, C. K. Jung, T. Kato, K. Kobayashi, K. Martens, M. Malek, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, T. Shibata, J. Ishii, Y. Kajiyama, Y. Kuno, Y. Nagashima, M. Takita, M. Yoshida, H. I. Kim, S. B. Kim, J. Yoo, H. Okazawa, T. Ishizuka, Y. Choi, H. K. Seo, Y. Gando, T. Hasegawa, K. Inoue, J. Shirai, A. Suzuki, M. Koshiba, T. Hashimoto, Y. Nakajima, K. Nishijima, H. Ishino, M. Morii, R. Nishimura, Y. Watanabe, D. Kielczewska, J. Zalipska, R. Gran, K. K. Shiraishi, K. Washburn, R. J. Wilkes

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Abstract

A study on neutrino magnetic movement was presented using solar neutrino data obtained from Super Kamiokandel (SK). The distortions to the energy spectrum of recoil electrons from magnetic scattering by nonzero neutrino magnetic movement were also studied. The systematic uncertainty of the reconstructed energy of electrons between 5 and 20 MeV was found to be less than 0.64%. The limits on the neutrino magnetic moment were also obtained by analyzing the SK day-night energy spectra.

Original languageEnglish
Article number021802
Pages (from-to)021802-1-021802-5
JournalPhysical Review Letters
Volume93
Issue number2
DOIs
Publication statusPublished - Jul 9 2004

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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  • Cite this

    Liu, D. W., Ashie, Y., Fukuda, S., Fukuda, Y., Ishihara, K., Itow, Y., Koshio, Y., Minamino, A., Miura, M., Moriyama, S., Nakahata, M., Namba, T., Nambu, R., Obayashi, Y., Sakurai, N., Shiozawa, M., Suzuki, Y., Takeuchi, H., Takeuchi, Y., ... Wilkes, R. J. (2004). Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data. Physical Review Letters, 93(2), 021802-1-021802-5. [021802]. https://doi.org/10.1103/PhysRevLett.93.021802