Solar neutrino measurements in Super-Kamiokande-II

J. P. Cravens; K. Abe; T. Iida; K. Ishihara; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Ogawa; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takeuchi; K. Ueshima; H. Watanabe; S. Yamada; I. Higuchi; C. Ishihara; M. Ishitsuka; T. Kajita; K. Kaneyuki; G. Mitsuka; H. Nishino; K. Okumura; C. Saji; Y. Takenaga; S. Clark; S. Desai; F. Dufour; E. Kearns; S. Likhoded; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; W. Wang; M. Goldhaber; D. Casper; J. Dunmore; W. R. Kropp; D. W. Liu; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; M. R. Vagins; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; M. Fechner; K. Scholberg; N. Tanimoto; C. W. Walter; R. Wendell; R. W. Ellsworth; S. Tasaka; G. Guillian; J. G. Learned; S. Matsuno; M. D. Messier; Y. Watanabe; Y. Hayato; A. K. Ichikawa; T. Ishida; T. Ishii; T. Iwashita; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nitta; Y. Oyama; Y. Totsuka; A. T. Suzuki; M. Hasegawa; K. Hiraide; I. Kato; H. Maesaka; T. Nakaya; K. Nishikawa; T. Sasaki; H. Sato; S. Yamamoto; M. Yokoyama; T. J. Haines; S. Dazeley; S. Hatakeyama; R. Svoboda; G. W. Sullivan; D. Turcan; A. Habig; Y. Fukuda; T. Sato; Y. Itow; T. Koike; T. Tanaka; C. K. Jung; T. Kato; K. Kobayashi; M. Malek; C. McGrew; A. Sarrat; R. Terri; C. Yanagisawa; N. Tamura; Y. Idehara; M. Ikeda; M. Sakuda; M. Sugihara; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; J. Yoo; T. Ishizuka; H. Okazawa; Y. Choi; H. K. Seo; Y. Gando; T. Hasegawa; K. Inoue; Y. Furuse; H. Ishii; K. Nishijima; H. Ishino; M. Koshiba; S. Chen; Z. Deng; Y. Liu; D. Kielczewska; H. Berns; R. Gran; K. K. Shiraishi; A. Stachyra; E. Thrane; K. Washburn; R. J. Wilkes

doi:10.1103/PhysRevD.78.032002

Solar neutrino measurements in Super-Kamiokande-II

J. P. Cravens
, K. Abe
, T. Iida
, K. Ishihara
, J. Kameda
, Y. Koshio
, A. Minamino
, C. Mitsuda
, M. Miura
, S. Moriyama
, M. Nakahata
, S. Nakayama
, Y. Obayashi
, H. Ogawa
, H. Sekiya
, M. Shiozawa
, Y. Suzuki
, A. Takeda
, Y. Takeuchi
, K. Ueshima

H. Watanabe, S. Yamada, I. Higuchi, C. Ishihara, M. Ishitsuka, T. Kajita, K. Kaneyuki, G. Mitsuka, H. Nishino, K. Okumura, C. Saji, Y. Takenaga, S. Clark, S. Desai, F. Dufour, E. Kearns, S. Likhoded, M. Litos, J. L. Raaf, J. L. Stone, L. R. Sulak, W. Wang, M. Goldhaber, D. Casper, J. Dunmore, W. R. Kropp, D. W. Liu, S. Mine, C. Regis, M. B. Smy, H. W. Sobel, M. R. Vagins, K. S. Ganezer, J. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, M. Fechner, K. Scholberg, N. Tanimoto, C. W. Walter, R. Wendell, R. W. Ellsworth, S. Tasaka, G. Guillian, J. G. Learned, S. Matsuno, M. D. Messier, Y. Watanabe, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nitta, Y. Oyama, Y. Totsuka, A. T. Suzuki, M. Hasegawa, K. Hiraide, I. Kato, H. Maesaka, T. Nakaya, K. Nishikawa, T. Sasaki, H. Sato, S. Yamamoto, M. Yokoyama, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, G. W. Sullivan, D. Turcan, A. Habig, Y. Fukuda, T. Sato, Y. Itow, T. Koike, T. Tanaka, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. McGrew, A. Sarrat, R. Terri, C. Yanagisawa, N. Tamura, Y. Idehara, M. Ikeda, M. Sakuda, M. Sugihara, Y. Kuno, M. Yoshida, S. B. Kim, B. S. Yang, J. Yoo, T. Ishizuka, H. Okazawa, Y. Choi, H. K. Seo, Y. Gando, T. Hasegawa, K. Inoue, Y. Furuse, H. Ishii, K. Nishijima, H. Ishino, M. Koshiba, S. Chen, Z. Deng, Y. Liu, D. Kielczewska, H. Berns, R. Gran, K. K. Shiraishi, A. Stachyra, E. Thrane, K. Washburn, R. J. Wilkes

Physics and Astronomy

University of California at Irvine
The University of Tokyo
High Energy Accelerator Research Organization, Tsukuba
Boston University
Pennsylvania State University
Brookhaven National Laboratory
California State University Dominguez Hills
Chonnam National University
Duke University
George Mason University
Gifu University
University of Hawai'i at Mānoa
Indiana University Bloomington
Kanagawa University
Kobe University
Kyoto University
TRIUMF
Los Alamos National Laboratory
Louisiana State University
University of Maryland, College Park
University of Minnesota Duluth
Miyagi University of Education
Nagoya University
Stony Brook University
Niigata University
Okayama University
The University of Osaka
Seoul National University
Shizuoka University
Shizuoka University of Welfare
Sungkyunkwan University
Tohoku University
Tokai University
Institute of Science Tokyo
Tsinghua University
University of Warsaw
University of Washington

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

280 Scopus citations

Abstract

The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured B8 total flux is (2.38±0.05(stat.)-0.15+0.16(sys.))×106cm-2s-1 and the day-night difference is found to be (-6.3±4.2(stat.)±3.7(sys.))%. There is no evidence of systematic tendencies between the first and second phases.

Original language	English
Article number	032002
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	78
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevD.78.032002
State	Published - Aug 6 2008

Access to Document

10.1103/PhysRevD.78.032002

Cite this

Cravens, J. P., Abe, K., Iida, T., Ishihara, K., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Ogawa, H., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takeuchi, Y., ... Wilkes, R. J. (2008). Solar neutrino measurements in Super-Kamiokande-II. Physical Review D - Particles, Fields, Gravitation and Cosmology, 78(3), Article 032002. https://doi.org/10.1103/PhysRevD.78.032002

@article{5584c3c765d241afb33754b7c678187a,

title = "Solar neutrino measurements in Super-Kamiokande-II",

abstract = "The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured B8 total flux is (2.38±0.05(stat.)-0.15+0.16(sys.))×106cm-2s-1 and the day-night difference is found to be (-6.3±4.2(stat.)±3.7(sys.))\%. There is no evidence of systematic tendencies between the first and second phases.",

author = "Cravens, \{J. P.\} and K. Abe and T. Iida and K. Ishihara and J. Kameda and Y. Koshio and A. Minamino and C. Mitsuda and M. Miura and S. Moriyama and M. Nakahata and S. Nakayama and Y. Obayashi and H. Ogawa and H. Sekiya and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takeuchi and K. Ueshima and H. Watanabe and S. Yamada and I. Higuchi and C. Ishihara and M. Ishitsuka and T. Kajita and K. Kaneyuki and G. Mitsuka and H. Nishino and K. Okumura and C. Saji and Y. Takenaga and S. Clark and S. Desai and F. Dufour and E. Kearns and S. Likhoded and M. Litos and Raaf, \{J. L.\} and Stone, \{J. L.\} and Sulak, \{L. R.\} and W. Wang and M. Goldhaber and D. Casper and J. Dunmore and Kropp, \{W. R.\} and Liu, \{D. W.\} and S. Mine and C. Regis and Smy, \{M. B.\} and Sobel, \{H. W.\} and Vagins, \{M. R.\} and Ganezer, \{K. S.\} and J. Hill and Keig, \{W. E.\} and Jang, \{J. S.\} and Kim, \{J. Y.\} and Lim, \{I. T.\} and M. Fechner and K. Scholberg and N. Tanimoto and Walter, \{C. W.\} and R. Wendell and Ellsworth, \{R. W.\} and S. Tasaka and G. Guillian and Learned, \{J. G.\} and S. Matsuno and Messier, \{M. D.\} and Y. Watanabe and Y. Hayato and Ichikawa, \{A. K.\} and T. Ishida and T. Ishii and T. Iwashita and T. Kobayashi and T. Nakadaira and K. Nakamura and K. Nitta and Y. Oyama and Y. Totsuka and Suzuki, \{A. T.\} and M. Hasegawa and K. Hiraide and I. Kato and H. Maesaka and T. Nakaya and K. Nishikawa and T. Sasaki and H. Sato and S. Yamamoto and M. Yokoyama and Haines, \{T. J.\} and S. Dazeley and S. Hatakeyama and R. Svoboda and Sullivan, \{G. W.\} and D. Turcan and A. Habig and Y. Fukuda and T. Sato and Y. Itow and T. Koike and T. Tanaka and Jung, \{C. K.\} and T. Kato and K. Kobayashi and M. Malek and C. McGrew and A. Sarrat and R. Terri and C. Yanagisawa and N. Tamura and Y. Idehara and M. Ikeda and M. Sakuda and M. Sugihara and Y. Kuno and M. Yoshida and Kim, \{S. B.\} and Yang, \{B. S.\} and J. Yoo and T. Ishizuka and H. Okazawa and Y. Choi and Seo, \{H. K.\} and Y. Gando and T. Hasegawa and K. Inoue and Y. Furuse and H. Ishii and K. Nishijima and H. Ishino and M. Koshiba and S. Chen and Z. Deng and Y. Liu and D. Kielczewska and H. Berns and R. Gran and Shiraishi, \{K. K.\} and A. Stachyra and E. Thrane and K. Washburn and Wilkes, \{R. J.\}",

year = "2008",

month = aug,

day = "6",

doi = "10.1103/PhysRevD.78.032002",

language = "English",

volume = "78",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

issn = "1550-7998",

number = "3",

}

Cravens, JP, Abe, K, Iida, T, Ishihara, K, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Nakayama, S, Obayashi, Y, Ogawa, H, Sekiya, H, Shiozawa, M, Suzuki, Y, Takeda, A, Takeuchi, Y, Ueshima, K, Watanabe, H, Yamada, S, Higuchi, I, Ishihara, C, Ishitsuka, M, Kajita, T, Kaneyuki, K, Mitsuka, G, Nishino, H, Okumura, K, Saji, C, Takenaga, Y, Clark, S, Desai, S, Dufour, F, Kearns, E, Likhoded, S, Litos, M, Raaf, JL, Stone, JL, Sulak, LR, Wang, W, Goldhaber, M, Casper, D, Dunmore, J, Kropp, WR, Liu, DW, Mine, S, Regis, C, Smy, MB, Sobel, HW, Vagins, MR, Ganezer, KS, Hill, J, Keig, WE, Jang, JS, Kim, JY, Lim, IT, Fechner, M, Scholberg, K, Tanimoto, N, Walter, CW, Wendell, R, Ellsworth, RW, Tasaka, S, Guillian, G, Learned, JG, Matsuno, S, Messier, MD, Watanabe, Y, Hayato, Y, Ichikawa, AK, Ishida, T, Ishii, T, Iwashita, T, Kobayashi, T, Nakadaira, T, Nakamura, K, Nitta, K, Oyama, Y, Totsuka, Y, Suzuki, AT, Hasegawa, M, Hiraide, K, Kato, I, Maesaka, H, Nakaya, T, Nishikawa, K, Sasaki, T, Sato, H, Yamamoto, S, Yokoyama, M, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Sullivan, GW, Turcan, D, Habig, A, Fukuda, Y, Sato, T, Itow, Y, Koike, T, Tanaka, T, Jung, CK, Kato, T, Kobayashi, K, Malek, M, McGrew, C, Sarrat, A, Terri, R, Yanagisawa, C, Tamura, N, Idehara, Y, Ikeda, M, Sakuda, M, Sugihara, M, Kuno, Y, Yoshida, M, Kim, SB, Yang, BS, Yoo, J, Ishizuka, T, Okazawa, H, Choi, Y, Seo, HK, Gando, Y, Hasegawa, T, Inoue, K, Furuse, Y, Ishii, H, Nishijima, K, Ishino, H, Koshiba, M, Chen, S, Deng, Z, Liu, Y, Kielczewska, D, Berns, H, Gran, R, Shiraishi, KK, Stachyra, A, Thrane, E, Washburn, K & Wilkes, RJ 2008, 'Solar neutrino measurements in Super-Kamiokande-II', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 78, no. 3, 032002. https://doi.org/10.1103/PhysRevD.78.032002

TY - JOUR

T1 - Solar neutrino measurements in Super-Kamiokande-II

AU - Cravens, J. P.

AU - Abe, K.

AU - Iida, T.

AU - Ishihara, K.

AU - Kameda, J.

AU - Koshio, Y.

AU - Minamino, A.

AU - Mitsuda, C.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakayama, S.

AU - Obayashi, Y.

AU - Ogawa, H.

AU - Sekiya, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Takeuchi, Y.

AU - Ueshima, K.

AU - Watanabe, H.

AU - Yamada, S.

AU - Higuchi, I.

AU - Ishihara, C.

AU - Ishitsuka, M.

AU - Kajita, T.

AU - Kaneyuki, K.

AU - Mitsuka, G.

AU - Nishino, H.

AU - Okumura, K.

AU - Saji, C.

AU - Takenaga, Y.

AU - Clark, S.

AU - Desai, S.

AU - Dufour, F.

AU - Kearns, E.

AU - Likhoded, S.

AU - Litos, M.

AU - Raaf, J. L.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Wang, W.

AU - Goldhaber, M.

AU - Casper, D.

AU - Dunmore, J.

AU - Kropp, W. R.

AU - Liu, D. W.

AU - Mine, S.

AU - Regis, C.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Vagins, M. R.

AU - Ganezer, K. S.

AU - Hill, J.

AU - Keig, W. E.

AU - Jang, J. S.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Fechner, M.

AU - Scholberg, K.

AU - Tanimoto, N.

AU - Walter, C. W.

AU - Wendell, R.

AU - Ellsworth, R. W.

AU - Tasaka, S.

AU - Guillian, G.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Messier, M. D.

AU - Watanabe, Y.

AU - Hayato, Y.

AU - Ichikawa, A. K.

AU - Ishida, T.

AU - Ishii, T.

AU - Iwashita, T.

AU - Kobayashi, T.

AU - Nakadaira, T.

AU - Nakamura, K.

AU - Nitta, K.

AU - Oyama, Y.

AU - Totsuka, Y.

AU - Suzuki, A. T.

AU - Hasegawa, M.

AU - Hiraide, K.

AU - Kato, I.

AU - Maesaka, H.

AU - Nakaya, T.

AU - Nishikawa, K.

AU - Sasaki, T.

AU - Sato, H.

AU - Yamamoto, S.

AU - Yokoyama, M.

AU - Haines, T. J.

AU - Dazeley, S.

AU - Hatakeyama, S.

AU - Svoboda, R.

AU - Sullivan, G. W.

AU - Turcan, D.

AU - Habig, A.

AU - Fukuda, Y.

AU - Sato, T.

AU - Itow, Y.

AU - Koike, T.

AU - Tanaka, T.

AU - Jung, C. K.

AU - Kato, T.

AU - Kobayashi, K.

AU - Malek, M.

AU - McGrew, C.

AU - Sarrat, A.

AU - Terri, R.

AU - Yanagisawa, C.

AU - Tamura, N.

AU - Idehara, Y.

AU - Ikeda, M.

AU - Sakuda, M.

AU - Sugihara, M.

AU - Kuno, Y.

AU - Yoshida, M.

AU - Kim, S. B.

AU - Yang, B. S.

AU - Yoo, J.

AU - Ishizuka, T.

AU - Okazawa, H.

AU - Choi, Y.

AU - Seo, H. K.

AU - Gando, Y.

AU - Hasegawa, T.

AU - Inoue, K.

AU - Furuse, Y.

AU - Ishii, H.

AU - Nishijima, K.

AU - Ishino, H.

AU - Koshiba, M.

AU - Chen, S.

AU - Deng, Z.

AU - Liu, Y.

AU - Kielczewska, D.

AU - Berns, H.

AU - Gran, R.

AU - Shiraishi, K. K.

AU - Stachyra, A.

AU - Thrane, E.

AU - Washburn, K.

AU - Wilkes, R. J.

PY - 2008/8/6

Y1 - 2008/8/6

N2 - The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured B8 total flux is (2.38±0.05(stat.)-0.15+0.16(sys.))×106cm-2s-1 and the day-night difference is found to be (-6.3±4.2(stat.)±3.7(sys.))%. There is no evidence of systematic tendencies between the first and second phases.

AB - The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured B8 total flux is (2.38±0.05(stat.)-0.15+0.16(sys.))×106cm-2s-1 and the day-night difference is found to be (-6.3±4.2(stat.)±3.7(sys.))%. There is no evidence of systematic tendencies between the first and second phases.

UR - https://www.scopus.com/pages/publications/49349088871

U2 - 10.1103/PhysRevD.78.032002

DO - 10.1103/PhysRevD.78.032002

M3 - Article

AN - SCOPUS:49349088871

SN - 1550-7998

VL - 78

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

IS - 3

M1 - 032002

ER -

Solar neutrino measurements in Super-Kamiokande-II

Abstract

Access to Document

Other files and links

Fingerprint

Cite this