Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

S. Fukuda; Y. Fukuda; M. Ishitsuka; Y. Itow; T. Kajita; J. Kameda; K. Kaneyuki; K. Kobayashi; Y. Koshio; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; T. Namba; A. Okada; N. Sakurai; M. Shiozawa; Y. Suzuki; H. Takeuchi; Y. Takeuchi; Y. Totsuka; S. Yamada; S. Desai; M. Earl; E. Kearns; M. D. Messier; J. L. Stone; L. R. Sulak; C. W. Walter; M. Goldhaber; T. Barszczak; D. Casper; W. Gajewski; W. R. Kropp; S. Mine; D. W. Liu; M. B. Smy; H. W. Sobel; M. R. Vagins; A. Gago; K. S. Ganezer; W. E. Keig; R. W. Ellsworth; S. Tasaka; A. Kibayashi; J. G. Learned; S. Matsuno; D. Takemori; Y. Hayato; T. Ishii; T. Kobayashi; T. Maruyama; K. Nakamura; Y. Obayashi; Y. Oyama; M. Sakuda; M. Yoshida; M. Kohama; T. Iwashita; A. T. Suzuki; A. Ichikawa; T. Inagaki; I. Kato; T. Nakaya; K. Nishikawa; T. J. Haines; S. Dazeley; S. Hatakeyama; R. Svoboda; E. Blaufuss; M. L. Chen; J. A. Goodman; G. Guillian; G. W. Sullivan; D. Turčan; K. Scholberg; A. Habig; M. Ackermann; J. Hill; C. K. Jung; M. Malek; K. Martens; C. Mauger; C. McGrew; E. Sharkey; B. Viren; C. Yanagisawa; T. Toshito; C. Mitsuda; K. Miyano; C. Saji; T. Shibata; Y. Kajiyama; Y. Nagashima; K. Nitta; M. Takitat; H. I. Kim; S. B. Kim; J. Yoo; H. Okazawa; T. Ishizuka; M. Etoh; Y. Gando; T. Hasegawa; K. Inoue; K. Ishihara; J. Shirai; A. Suzuki; M. Koshiba; Y. Hatakeyama; Y. Ichikawa; M. Koike; K. Nishijima; H. Ishino; M. Morii; R. Nishimura; Y. Watanabe; D. Kielczewska; H. G. Berns; S. C. Boyd; A. L. Stachyra; R. J. Wilkes

doi:10.1016/S0370-2693(02)02090-7

Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

S. Fukuda, Y. Fukuda, M. Ishitsuka, Y. Itow, T. Kajita, J. Kameda, K. Kaneyuki, K. Kobayashi, Y. Koshio, M. Miura, S. Moriyama, M. Nakahata, S. Nakayama, T. Namba, A. Okada, N. Sakurai, M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. TakeuchiY. Totsuka, S. Yamada, S. Desai, M. Earl, E. Kearns, M. D. Messier, J. L. Stone, L. R. Sulak, C. W. Walter, M. Goldhaber, T. Barszczak, D. Casper, W. Gajewski, W. R. Kropp, S. Mine, D. W. Liu, M. B. Smy, H. W. Sobel, M. R. Vagins, A. Gago, K. S. Ganezer, W. E. Keig, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, T. Ishii, T. Kobayashi, T. Maruyama, K. Nakamura, Y. Obayashi, Y. Oyama, M. Sakuda, M. Yoshida, M. Kohama, T. Iwashita, A. T. Suzuki, A. Ichikawa, T. Inagaki, I. Kato, T. Nakaya, K. Nishikawa, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, M. L. Chen, J. A. Goodman, G. Guillian, G. W. Sullivan, D. Turčan, K. Scholberg, A. Habig, M. Ackermann, J. Hill, C. K. Jung, M. Malek, K. Martens, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, C. Saji, T. Shibata, Y. Kajiyama, Y. Nagashima, K. Nitta, M. Takitat, H. I. Kim, S. B. Kim, J. Yoo, H. Okazawa, T. Ishizuka, M. Etoh, Y. Gando, T. Hasegawa, K. Inoue, K. Ishihara, J. Shirai, A. Suzuki, M. Koshiba, Y. Hatakeyama, Y. Ichikawa, M. Koike, K. Nishijima, H. Ishino, M. Morii, R. Nishimura, Y. Watanabe, D. Kielczewska, H. G. Berns, S. C. Boyd, A. L. Stachyra, R. J. Wilkes

Physics & Astronomy (Duluth)

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Abstract

A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar ⁸B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference Δm² between the two mass eigenstates ranges from about 3 to 19 × 10^-5 eV², while the mixing angle θ is in the range of tan²θ ≈ 0.25-0.65.

Original language	English (US)
Pages (from-to)	179-187
Number of pages	9
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	539
Issue number	3-4
DOIs	https://doi.org/10.1016/S0370-2693(02)02090-7
State	Published - Jul 18 2002

Bibliographical note

Funding Information:
We gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. The Super-Kamiokande detector has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the US Department of Energy, and the US National Science Foundation.

Keywords

Neutrino
Solar neutrino
Super-Kamiokande

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Fukuda, S., Fukuda, Y., Ishitsuka, M., Itow, Y., Kajita, T., Kameda, J., Kaneyuki, K., Kobayashi, K., Koshio, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Namba, T., Okada, A., Sakurai, N., Shiozawa, M., Suzuki, Y., Takeuchi, H., ... Wilkes, R. J. (2002). Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 539(3-4), 179-187. https://doi.org/10.1016/S0370-2693(02)02090-7

Fukuda, S, Fukuda, Y, Ishitsuka, M, Itow, Y, Kajita, T, Kameda, J, Kaneyuki, K, Kobayashi, K, Koshio, Y, Miura, M, Moriyama, S, Nakahata, M, Nakayama, S, Namba, T, Okada, A, Sakurai, N, Shiozawa, M, Suzuki, Y, Takeuchi, H, Takeuchi, Y, Totsuka, Y, Yamada, S, Desai, S, Earl, M, Kearns, E, Messier, MD, Stone, JL, Sulak, LR, Walter, CW, Goldhaber, M, Barszczak, T, Casper, D, Gajewski, W, Kropp, WR, Mine, S, Liu, DW, Smy, MB, Sobel, HW, Vagins, MR, Gago, A, Ganezer, KS, Keig, WE, Ellsworth, RW, Tasaka, S, Kibayashi, A, Learned, JG, Matsuno, S, Takemori, D, Hayato, Y, Ishii, T, Kobayashi, T, Maruyama, T, Nakamura, K, Obayashi, Y, Oyama, Y, Sakuda, M, Yoshida, M, Kohama, M, Iwashita, T, Suzuki, AT, Ichikawa, A, Inagaki, T, Kato, I, Nakaya, T, Nishikawa, K, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Blaufuss, E, Chen, ML, Goodman, JA, Guillian, G, Sullivan, GW, Turčan, D, Scholberg, K, Habig, A, Ackermann, M, Hill, J, Jung, CK, Malek, M, Martens, K, Mauger, C, McGrew, C, Sharkey, E, Viren, B, Yanagisawa, C, Toshito, T, Mitsuda, C, Miyano, K, Saji, C, Shibata, T, Kajiyama, Y, Nagashima, Y, Nitta, K, Takitat, M, Kim, HI, Kim, SB, Yoo, J, Okazawa, H, Ishizuka, T, Etoh, M, Gando, Y, Hasegawa, T, Inoue, K, Ishihara, K, Shirai, J, Suzuki, A, Koshiba, M, Hatakeyama, Y, Ichikawa, Y, Koike, M, Nishijima, K, Ishino, H, Morii, M, Nishimura, R, Watanabe, Y, Kielczewska, D, Berns, HG, Boyd, SC, Stachyra, AL & Wilkes, RJ 2002, 'Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 539, no. 3-4, pp. 179-187. https://doi.org/10.1016/S0370-2693(02)02090-7

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title = "Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data",

abstract = "A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar 8B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference Δm2 between the two mass eigenstates ranges from about 3 to 19 × 10-5 eV2, while the mixing angle θ is in the range of tan2θ ≈ 0.25-0.65.",

keywords = "Neutrino, Solar neutrino, Super-Kamiokande",

author = "S. Fukuda and Y. Fukuda and M. Ishitsuka and Y. Itow and T. Kajita and J. Kameda and K. Kaneyuki and K. Kobayashi and Y. Koshio and M. Miura and S. Moriyama and M. Nakahata and S. Nakayama and T. Namba and A. Okada and N. Sakurai and M. Shiozawa and Y. Suzuki and H. Takeuchi and Y. Takeuchi and Y. Totsuka and S. Yamada 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 M. Goldhaber and T. Barszczak and D. Casper and W. Gajewski and Kropp, {W. R.} and S. Mine and Liu, {D. W.} and Smy, {M. B.} and Sobel, {H. W.} and Vagins, {M. R.} and A. Gago and Ganezer, {K. S.} and Keig, {W. E.} and Ellsworth, {R. W.} and S. Tasaka and A. Kibayashi and Learned, {J. G.} and S. Matsuno and D. Takemori and Y. Hayato and T. Ishii and T. Kobayashi and T. Maruyama and K. Nakamura and Y. Obayashi and Y. Oyama and M. Sakuda and M. Yoshida and M. Kohama and T. Iwashita and Suzuki, {A. T.} and A. Ichikawa and T. Inagaki and I. Kato and T. Nakaya and K. Nishikawa and Haines, {T. J.} and S. Dazeley and S. Hatakeyama and R. Svoboda and E. Blaufuss and Chen, {M. L.} and Goodman, {J. A.} and G. Guillian and Sullivan, {G. W.} and D. Tur{\v c}an and K. Scholberg and A. Habig and M. Ackermann and J. Hill and Jung, {C. K.} and M. Malek and K. Martens 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 C. Saji and T. Shibata and Y. Kajiyama and Y. Nagashima and K. Nitta and M. Takitat and Kim, {H. I.} and Kim, {S. B.} and J. Yoo and H. Okazawa and T. Ishizuka and M. Etoh and Y. Gando and T. Hasegawa and K. Inoue and K. Ishihara and J. Shirai and A. Suzuki and M. Koshiba and Y. Hatakeyama and Y. Ichikawa and M. Koike and K. Nishijima and H. Ishino and M. Morii and R. Nishimura and Y. Watanabe and D. Kielczewska and Berns, {H. G.} and Boyd, {S. C.} and Stachyra, {A. L.} and Wilkes, {R. J.}",

note = "Funding Information: We gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. The Super-Kamiokande detector has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the US Department of Energy, and the US National Science Foundation.",

year = "2002",

month = jul,

day = "18",

doi = "10.1016/S0370-2693(02)02090-7",

language = "English (US)",

volume = "539",

pages = "179--187",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier",

number = "3-4",

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TY - JOUR

T1 - Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

AU - Fukuda, S.

AU - Fukuda, Y.

AU - Ishitsuka, M.

AU - Itow, Y.

AU - Kajita, T.

AU - Kameda, J.

AU - Kaneyuki, K.

AU - Kobayashi, K.

AU - Koshio, Y.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakayama, S.

AU - Namba, T.

AU - Okada, A.

AU - Sakurai, N.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeuchi, H.

AU - Takeuchi, Y.

AU - Totsuka, Y.

AU - Yamada, S.

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 - Goldhaber, M.

AU - Barszczak, T.

AU - Casper, D.

AU - Gajewski, W.

AU - Kropp, W. R.

AU - Mine, S.

AU - Liu, D. W.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Vagins, M. R.

AU - Gago, A.

AU - Ganezer, K. S.

AU - Keig, W. E.

AU - Ellsworth, R. W.

AU - Tasaka, S.

AU - Kibayashi, A.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Takemori, D.

AU - Hayato, Y.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Maruyama, T.

AU - Nakamura, K.

AU - Obayashi, Y.

AU - Oyama, Y.

AU - Sakuda, M.

AU - Yoshida, M.

AU - Kohama, M.

AU - Iwashita, T.

AU - Suzuki, A. T.

AU - Ichikawa, A.

AU - Inagaki, T.

AU - Kato, I.

AU - Nakaya, T.

AU - Nishikawa, K.

AU - Haines, T. J.

AU - Dazeley, S.

AU - Hatakeyama, S.

AU - Svoboda, R.

AU - Blaufuss, E.

AU - Chen, M. L.

AU - Goodman, J. A.

AU - Guillian, G.

AU - Sullivan, G. W.

AU - Turčan, D.

AU - Scholberg, K.

AU - Habig, A.

AU - Ackermann, M.

AU - Hill, J.

AU - Jung, C. K.

AU - Malek, M.

AU - Martens, K.

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 - Saji, C.

AU - Shibata, T.

AU - Kajiyama, Y.

AU - Nagashima, Y.

AU - Nitta, K.

AU - Takitat, M.

AU - Kim, H. I.

AU - Kim, S. B.

AU - Yoo, J.

AU - Okazawa, H.

AU - Ishizuka, T.

AU - Etoh, M.

AU - Gando, Y.

AU - Hasegawa, T.

AU - Inoue, K.

AU - Ishihara, K.

AU - Shirai, J.

AU - Suzuki, A.

AU - Koshiba, M.

AU - Hatakeyama, Y.

AU - Ichikawa, Y.

AU - Koike, M.

AU - Nishijima, K.

AU - Ishino, H.

AU - Morii, M.

AU - Nishimura, R.

AU - Watanabe, Y.

AU - Kielczewska, D.

AU - Berns, H. G.

AU - Boyd, S. C.

AU - Stachyra, A. L.

AU - Wilkes, R. J.

N1 - Funding Information: We gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. The Super-Kamiokande detector has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the US Department of Energy, and the US National Science Foundation.

PY - 2002/7/18

Y1 - 2002/7/18

N2 - A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar 8B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference Δm2 between the two mass eigenstates ranges from about 3 to 19 × 10-5 eV2, while the mixing angle θ is in the range of tan2θ ≈ 0.25-0.65.

AB - A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar 8B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference Δm2 between the two mass eigenstates ranges from about 3 to 19 × 10-5 eV2, while the mixing angle θ is in the range of tan2θ ≈ 0.25-0.65.

KW - Neutrino

KW - Solar neutrino

KW - Super-Kamiokande

UR - http://www.scopus.com/inward/record.url?scp=0037130349&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0037130349&partnerID=8YFLogxK

U2 - 10.1016/S0370-2693(02)02090-7

DO - 10.1016/S0370-2693(02)02090-7

M3 - Article

AN - SCOPUS:0037130349

SN - 0370-2693

VL - 539

SP - 179

EP - 187

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

IS - 3-4

ER -

Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

Abstract

Bibliographical note

Keywords

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