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. Yamada; M. 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

doi:10.1103/PhysRevLett.93.021802

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. Yamada

M. 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

Physics and Astronomy

University of California at Irvine
The University of Tokyo
Boston University
Harvard University
California State University Dominguez Hills
Chonnam National University
George Mason University
Gifu University
University of Hawai'i at Mānoa
High Energy Accelerator Research Organization, Tsukuba
The University of Chicago
Kobe University
Kyoto University
Los Alamos National Laboratory
Louisiana State University
University of Maryland, College Park
Massachusetts Institute of Technology
University of Minnesota Duluth
Stony Brook University
University of Utah
Brookhaven National Laboratory
Nagoya University
Niigata University
The University of Osaka
Seoul National University
International and Cultural Studies
Shizuoka University
Sungkyunkwan University
Tohoku University
Tokai University
Institute of Science Tokyo
University of Warsaw
University of Washington

Research output: Contribution to journal › Article › peer-review

88 Scopus citations

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	https://doi.org/10.1103/PhysRevLett.93.021802
State	Published - Jul 9 2004

Access to Document

10.1103/PhysRevLett.93.021802

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. Article 021802. https://doi.org/10.1103/PhysRevLett.93.021802

@article{ba920476e4b2470f801516943dba6143,

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

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.",

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

year = "2004",

month = jul,

day = "9",

doi = "10.1103/PhysRevLett.93.021802",

language = "English",

volume = "93",

pages = "021802--1--021802--5",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "2",

}

Liu, DW, 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, MD, Stone, JL, Sulak, LR, Walter, CW, Wang, W, Barszczak, T, Casper, D, Cravens, JP, Gajewski, W, Kropp, WR, Mine, S, Smy, MB, Sobel, HW, Sterner, CW, Vagins, MR, Ganezer, KS, Hill, J, Keig, WE, Kim, JY, Lim, IT, Ellsworth, RW, Tasaka, S, Kibayashi, A, Learned, JG, Matsuno, S, Takemori, D, Hayato, Y, Ichikawa, AK, Ishida, T, Ishii, T, Iwashita, T, Kameda, J, Kobayashi, T, Maruyama, T, Nakamura, K, Nitta, K, Oyama, Y, Sakuda, M, Totsuka, Y, Suzuki, AT, Hasegawa, M, Hayashi, K, Inagaki, T, Kato, I, Maesaka, H, Morita, T, Nakaya, T, Nishikawa, K, Sasaki, T, Ueda, S, Yamamoto, S, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Blaufuss, E, Goodman, JA, Guillian, G, Sullivan, GW, Turcan, D, Scholberg, K, Habig, A, Ackermann, M, Jung, CK, 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, HI, Kim, SB, Yoo, J, Okazawa, H, Ishizuka, T, Choi, Y, Seo, HK, 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, KK, Washburn, K & Wilkes, RJ 2004, 'Limits on the neutrino magnetic moment using 1496 days of Super-Kamiokande-I solar neutrino data', Physical Review Letters, vol. 93, no. 2, 021802, pp. 021802-1-021802-5. https://doi.org/10.1103/PhysRevLett.93.021802

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.

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 - https://www.scopus.com/pages/publications/80051545191

U2 - 10.1103/PhysRevLett.93.021802

DO - 10.1103/PhysRevLett.93.021802

M3 - Article

AN - SCOPUS:80051545191

SN - 0031-9007

VL - 93

SP - 021802-1-021802-5

JO - Physical Review Letters

JF - Physical Review Letters

IS - 2

M1 - 021802

ER -

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

Abstract

Access to Document

Other files and links

Fingerprint

Cite this