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 language | English |
---|---|
Article number | 021802 |
Pages (from-to) | 021802-1-021802-5 |
Journal | Physical review letters |
Volume | 93 |
Issue number | 2 |
DOIs | |
Publication status | Published - 2004 Jul 9 |
ASJC Scopus subject areas
- Physics and Astronomy(all)
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Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data. / 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.; Yamada, S.; Ishitsuka, M.; Kajita, T.; Kaneyuki, K.; Nakayama, S.; Okada, A.; Ooyabu, T.; Saji, C.; Desai, S.; Earl, M.; Kearns, E.; Messier, M. D.; Stone, J. L.; Sulak, L. R.; Walter, C. W.; Wang, W.; Barszczak, T.; Casper, D.; Cravens, J. P.; Gajewski, W.; Kropp, W. R.; Mine, S.; Smy, M. B.; Sobel, H. W.; Sterner, C. W.; Vagins, M. R.; Ganezer, K. S.; Hill, J.; Keig, W. E.; Kim, J. Y.; Lim, I. T.; Ellsworth, R. W.; Tasaka, S.; Kibayashi, A.; Learned, J. G.; Matsuno, S.; Takemori, D.; Hayato, Y.; Ichikawa, A. K.; Ishida, T.; Ishii, T.; Iwashita, T.; Kameda, J.; Kobayashi, T.; Maruyama, T.; Nakamura, K.; Nitta, K.; Oyama, Y.; Sakuda, M.; Totsuka, Y.; Suzuki, A. T.; Hasegawa, M.; Hayashi, K.; Inagaki, T.; Kato, I.; Maesaka, H.; Morita, T.; Nakaya, T.; Nishikawa, K.; Sasaki, T.; Ueda, S.; Yamamoto, S.; Haines, T. J.; Dazeley, S.; Hatakeyama, S.; Svoboda, R.; Blaufuss, E.; Goodman, J. A.; Guillian, G.; Sullivan, G. W.; Turcan, D.; Scholberg, K.; Habig, A.; Ackermann, M.; Jung, C. K.; Kato, T.; Kobayashi, K.; Martens, K.; Malek, M.; Mauger, C.; McGrew, C.; Sharkey, E.; Viren, B.; Yanagisawa, C.; Toshito, T.; Mitsuda, C.; Miyano, K.; Shibata, T.; Ishii, J.; Kajiyama, Y.; Kuno, Y.; Nagashima, Y.; Takita, M.; Yoshida, M.; Kim, H. I.; Kim, S. B.; Yoo, J.; Okazawa, H.; Ishizuka, T.; Choi, Y.; Seo, H. K.; Gando, Y.; Hasegawa, T.; Inoue, K.; Shirai, J.; Suzuki, A.; Koshiba, M.; Hashimoto, T.; Nakajima, Y.; Nishijima, K.; Ishino, H.; Morii, M.; Nishimura, R.; Watanabe, Y.; Kielczewska, D.; Zalipska, J.; Gran, R.; Shiraishi, K. K.; Washburn, K.; Wilkes, R. J.
In: Physical review letters, Vol. 93, No. 2, 021802, 09.07.2004, p. 021802-1-021802-5.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data
AU - Liu, D. W.
AU - Ashie, Y.
AU - Fukuda, S.
AU - Fukuda, Y.
AU - Ishihara, K.
AU - Itow, Y.
AU - Koshio, Y.
AU - Minamino, A.
AU - Miura, M.
AU - Moriyama, S.
AU - Nakahata, M.
AU - Namba, T.
AU - Nambu, R.
AU - Obayashi, Y.
AU - Sakurai, N.
AU - Shiozawa, M.
AU - Suzuki, Y.
AU - Takeuchi, H.
AU - Takeuchi, Y.
AU - Yamada, S.
AU - Ishitsuka, M.
AU - Kajita, T.
AU - Kaneyuki, K.
AU - Nakayama, S.
AU - Okada, A.
AU - Ooyabu, T.
AU - Saji, C.
AU - Desai, S.
AU - Earl, M.
AU - Kearns, E.
AU - Messier, M. D.
AU - Stone, J. L.
AU - Sulak, L. R.
AU - Walter, C. W.
AU - Wang, W.
AU - Barszczak, T.
AU - Casper, D.
AU - Cravens, J. P.
AU - Gajewski, W.
AU - Kropp, W. R.
AU - Mine, S.
AU - Smy, M. B.
AU - Sobel, H. W.
AU - Sterner, C. W.
AU - Vagins, M. R.
AU - Ganezer, K. S.
AU - Hill, J.
AU - Keig, W. E.
AU - Kim, J. Y.
AU - Lim, I. T.
AU - Ellsworth, R. W.
AU - Tasaka, S.
AU - Kibayashi, A.
AU - Learned, J. G.
AU - Matsuno, S.
AU - Takemori, D.
AU - Hayato, Y.
AU - Ichikawa, A. K.
AU - Ishida, T.
AU - Ishii, T.
AU - Iwashita, T.
AU - Kameda, J.
AU - Kobayashi, T.
AU - Maruyama, T.
AU - Nakamura, K.
AU - Nitta, K.
AU - Oyama, Y.
AU - Sakuda, M.
AU - Totsuka, Y.
AU - Suzuki, A. T.
AU - Hasegawa, M.
AU - Hayashi, K.
AU - Inagaki, T.
AU - Kato, I.
AU - Maesaka, H.
AU - Morita, T.
AU - Nakaya, T.
AU - Nishikawa, K.
AU - Sasaki, T.
AU - Ueda, S.
AU - Yamamoto, S.
AU - Haines, T. J.
AU - Dazeley, S.
AU - Hatakeyama, S.
AU - Svoboda, R.
AU - Blaufuss, E.
AU - Goodman, J. A.
AU - Guillian, G.
AU - Sullivan, G. W.
AU - Turcan, D.
AU - Scholberg, K.
AU - Habig, A.
AU - Ackermann, M.
AU - Jung, C. K.
AU - Kato, T.
AU - Kobayashi, K.
AU - Martens, K.
AU - Malek, M.
AU - Mauger, C.
AU - McGrew, C.
AU - Sharkey, E.
AU - Viren, B.
AU - Yanagisawa, C.
AU - Toshito, T.
AU - Mitsuda, C.
AU - Miyano, K.
AU - Shibata, T.
AU - Ishii, J.
AU - Kajiyama, Y.
AU - Kuno, Y.
AU - Nagashima, Y.
AU - Takita, M.
AU - Yoshida, M.
AU - Kim, H. I.
AU - Kim, S. B.
AU - Yoo, J.
AU - Okazawa, H.
AU - Ishizuka, T.
AU - Choi, Y.
AU - Seo, H. K.
AU - Gando, Y.
AU - Hasegawa, T.
AU - Inoue, K.
AU - Shirai, J.
AU - Suzuki, A.
AU - Koshiba, M.
AU - Hashimoto, T.
AU - Nakajima, Y.
AU - Nishijima, K.
AU - Ishino, H.
AU - Morii, M.
AU - Nishimura, R.
AU - Watanabe, Y.
AU - Kielczewska, D.
AU - Zalipska, J.
AU - Gran, R.
AU - Shiraishi, K. K.
AU - Washburn, K.
AU - Wilkes, R. J.
N1 - Funding Information: The authors gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. Super-Kamiokande has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the U.S. Department of ?>Energy, and the U.S. National Science Foundation. This work was partially supported by the Korean Research Foundation (BK21) and the Korea Ministry of Science and Technology.
PY - 2004/7/9
Y1 - 2004/7/9
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=80051545191&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=80051545191&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.93.021802
DO - 10.1103/PhysRevLett.93.021802
M3 - Article
C2 - 15323899
AN - SCOPUS:80051545191
VL - 93
SP - 021802-1-021802-5
JO - Physical Review Letters
JF - Physical Review Letters
SN - 0031-9007
IS - 2
M1 - 021802
ER -