Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande

J. Hosaka; K. Ishihara; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; T. Namba; Y. Obayashi; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takeuchi; S. Yamada; I. Higuchi; M. Ishitsuka; T. Kajita; K. Kaneyuki; G. Mitsuka; S. Nakayama; H. Nishino; A. Okada; K. Okumura; C. Saji; Y. Takenaga; S. Clark; S. Desai; E. Kearns; S. Likhoded; J. L. Stone; L. R. Sulak; W. Wang; M. Goldhaber; D. Casper; J. P. Cravens; W. R. Kropp; D. W. Liu; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; C. W. Sterner; M. R. Vagins; K. S. Ganezer; J. E. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; K. Scholberg; C. W. Walter; R. Wendell; R. W. Ellsworth; S. Tasaka; E. Guillian; A. Kibayashi; J. G. Learned; S. Matsuno; M. D. Messier; 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; 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; E. Blaufuss; J. A. Goodman; G. W. Sullivan; D. Turcan; J. Cooley; A. Habig; Y. Fukuda; T. Sato; Y. Itow; C. K. Jung; T. Kato; K. Kobayashi; M. Malek; C. Mauger; C. McGrew; A. Sarrat; C. Yanagisawa; N. Tamura; Makoto Sakuda; Y. Kuno; M. Yoshida; S. B. Kim; J. Yoo; T. Ishizuka; H. Okazawa; Y. Choi; H. K. Seo; Y. Gando; T. Hasegawa; K. Inoue; J. Shirai; A. Suzuki; K. Nishijima; H. Ishino; Y. Watanabe; M. Koshiba; D. Kielczewska; J. Zalipska; H. G. Berns; R. Gran; K. K. Shiraishi; A. Stachyra; K. Washburn; R. J. Wilkes

doi:10.1103/PhysRevD.74.032002

Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande

J. Hosaka, K. Ishihara, J. Kameda, Y. Koshio, A. Minamino, C. Mitsuda, M. Miura, S. Moriyama, M. Nakahata, T. Namba, Y. Obayashi, M. Shiozawa, Y. Suzuki, A. Takeda, Y. Takeuchi, S. Yamada, I. Higuchi, M. Ishitsuka, T. Kajita, K. KaneyukiG. Mitsuka, S. Nakayama, H. Nishino, A. Okada, K. Okumura, C. Saji, Y. Takenaga, S. Clark, S. Desai, E. Kearns, S. Likhoded, J. L. Stone, L. R. Sulak, W. Wang, M. Goldhaber, D. Casper, J. P. Cravens, W. R. Kropp, D. W. Liu, S. Mine, C. Regis, M. B. Smy, H. W. Sobel, C. W. Sterner, M. R. Vagins, K. S. Ganezer, J. E. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, K. Scholberg, C. W. Walter, R. Wendell, R. W. Ellsworth, S. Tasaka, E. Guillian, A. Kibayashi, J. G. Learned, S. Matsuno, M. D. Messier, 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, 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, E. Blaufuss, J. A. Goodman, G. W. Sullivan, D. Turcan, J. Cooley, A. Habig, Y. Fukuda, T. Sato, Y. Itow, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. Mauger, C. McGrew, A. Sarrat, C. Yanagisawa, N. Tamura, Makoto Sakuda, Y. Kuno, M. Yoshida, S. B. Kim, J. Yoo, T. Ishizuka, H. Okazawa, Y. Choi, H. K. Seo, Y. Gando, T. Hasegawa, K. Inoue, J. Shirai, A. Suzuki, K. Nishijima, H. Ishino, Y. Watanabe, M. Koshiba, D. Kielczewska, J. Zalipska, H. G. Berns, R. Gran, K. K. Shiraishi, A. Stachyra, K. Washburn, R. J. Wilkes

研究成果 › 査読

184 被引用数 (Scopus)

抄録

We report on the results of a three-flavor oscillation analysis using Super-Kamiokande I atmospheric neutrino data, with the assumption of one mass scale dominance (Δm122=0). No significant flux change due to matter effect, which occurs when neutrinos propagate inside the Earth for θ13≠0, has been seen either in a multi-GeV νe-rich sample or in a νμ-rich sample. Both normal and inverted mass hierarchy hypotheses are tested and both are consistent with observation. Using Super-Kamiokande data only, 2-dimensional 90% confidence allowed regions are obtained: mixing angles are constrained to sin 2θ13<0.14 and 0.37<sin 2θ23<0.65 for the normal mass hierarchy. Weaker constraints, sin 2θ13<0.27 and 0.37<sin 2θ23<0.69, are obtained for the inverted mass hierarchy case.

本文言語	English
論文番号	032002
ジャーナル	Physical Review D - Particles, Fields, Gravitation and Cosmology
巻	74
号	3
DOI	https://doi.org/10.1103/PhysRevD.74.032002
出版ステータス	Published - 2006
外部発表	はい

ASJC Scopus subject areas

核物理学および高エネルギー物理学
物理学および天文学（その他）

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10.1103/PhysRevD.74.032002

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Hosaka, J., Ishihara, K., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Namba, T., Obayashi, Y., Shiozawa, M., Suzuki, Y., Takeda, A., Takeuchi, Y., Yamada, S., Higuchi, I., Ishitsuka, M., Kajita, T., ... Wilkes, R. J. (2006). Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande. Physical Review D - Particles, Fields, Gravitation and Cosmology, 74(3), [032002]. https://doi.org/10.1103/PhysRevD.74.032002

Hosaka, J, Ishihara, K, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Namba, T, Obayashi, Y, Shiozawa, M, Suzuki, Y, Takeda, A, Takeuchi, Y, Yamada, S, Higuchi, I, Ishitsuka, M, Kajita, T, Kaneyuki, K, Mitsuka, G, Nakayama, S, Nishino, H, Okada, A, Okumura, K, Saji, C, Takenaga, Y, Clark, S, Desai, S, Kearns, E, Likhoded, S, Stone, JL, Sulak, LR, Wang, W, Goldhaber, M, Casper, D, Cravens, JP, Kropp, WR, Liu, DW, Mine, S, Regis, C, Smy, MB, Sobel, HW, Sterner, CW, Vagins, MR, Ganezer, KS, Hill, JE, Keig, WE, Jang, JS, Kim, JY, Lim, IT, Scholberg, K, Walter, CW, Wendell, R, Ellsworth, RW, Tasaka, S, Guillian, E, Kibayashi, A, Learned, JG, Matsuno, S, Messier, MD, 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, Kato, I, Maesaka, H, Nakaya, T, Nishikawa, K, Sasaki, T, Sato, H, Yamamoto, S, Yokoyama, M, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Blaufuss, E, Goodman, JA, Sullivan, GW, Turcan, D, Cooley, J, Habig, A, Fukuda, Y, Sato, T, Itow, Y, Jung, CK, Kato, T, Kobayashi, K, Malek, M, Mauger, C, McGrew, C, Sarrat, A, Yanagisawa, C, Tamura, N, Sakuda, M, Kuno, Y, Yoshida, M, Kim, SB, Yoo, J, Ishizuka, T, Okazawa, H, Choi, Y, Seo, HK, Gando, Y, Hasegawa, T, Inoue, K, Shirai, J, Suzuki, A, Nishijima, K, Ishino, H, Watanabe, Y, Koshiba, M, Kielczewska, D, Zalipska, J, Berns, HG, Gran, R, Shiraishi, KK, Stachyra, A, Washburn, K & Wilkes, RJ 2006, 'Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 74, no. 3, 032002. https://doi.org/10.1103/PhysRevD.74.032002

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title = "Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande",

abstract = "We report on the results of a three-flavor oscillation analysis using Super-Kamiokande I atmospheric neutrino data, with the assumption of one mass scale dominance (Δm122=0). No significant flux change due to matter effect, which occurs when neutrinos propagate inside the Earth for θ13≠0, has been seen either in a multi-GeV νe-rich sample or in a νμ-rich sample. Both normal and inverted mass hierarchy hypotheses are tested and both are consistent with observation. Using Super-Kamiokande data only, 2-dimensional 90% confidence allowed regions are obtained: mixing angles are constrained to sin 2θ13<0.14 and 0.37",

author = "J. Hosaka 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 T. Namba and Y. Obayashi and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takeuchi and S. Yamada and I. Higuchi and M. Ishitsuka and T. Kajita and K. Kaneyuki and G. Mitsuka and S. Nakayama and H. Nishino and A. Okada and K. Okumura and C. Saji and Y. Takenaga and S. Clark and S. Desai and E. Kearns and S. Likhoded and Stone, {J. L.} and Sulak, {L. R.} and W. Wang and M. Goldhaber and D. Casper and Cravens, {J. P.} and Kropp, {W. R.} and Liu, {D. W.} and S. Mine and C. Regis and Smy, {M. B.} and Sobel, {H. W.} and Sterner, {C. W.} and Vagins, {M. R.} and Ganezer, {K. S.} and Hill, {J. E.} and Keig, {W. E.} and Jang, {J. S.} and Kim, {J. Y.} and Lim, {I. T.} and K. Scholberg and Walter, {C. W.} and R. Wendell and Ellsworth, {R. W.} and S. Tasaka and E. Guillian and A. Kibayashi and Learned, {J. G.} and S. Matsuno and Messier, {M. D.} 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 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 E. Blaufuss and Goodman, {J. A.} and Sullivan, {G. W.} and D. Turcan and J. Cooley and A. Habig and Y. Fukuda and T. Sato and Y. Itow and Jung, {C. K.} and T. Kato and K. Kobayashi and M. Malek and C. Mauger and C. McGrew and A. Sarrat and C. Yanagisawa and N. Tamura and Makoto Sakuda and Y. Kuno and M. Yoshida and Kim, {S. B.} 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 J. Shirai and A. Suzuki and K. Nishijima and H. Ishino and Y. Watanabe and M. Koshiba and D. Kielczewska and J. Zalipska and Berns, {H. G.} and R. Gran and Shiraishi, {K. K.} and A. Stachyra and K. Washburn and Wilkes, {R. J.}",

year = "2006",

doi = "10.1103/PhysRevD.74.032002",

language = "English",

volume = "74",

journal = "Physical Review D",

issn = "0556-2821",

number = "3",

}

TY - JOUR

T1 - Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande

AU - Hosaka, J.

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 - Namba, T.

AU - Obayashi, Y.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Takeuchi, Y.

AU - Yamada, S.

AU - Higuchi, I.

AU - Ishitsuka, M.

AU - Kajita, T.

AU - Kaneyuki, K.

AU - Mitsuka, G.

AU - Nakayama, S.

AU - Nishino, H.

AU - Okada, A.

AU - Okumura, K.

AU - Saji, C.

AU - Takenaga, Y.

AU - Clark, S.

AU - Desai, S.

AU - Kearns, E.

AU - Likhoded, S.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Wang, W.

AU - Goldhaber, M.

AU - Casper, D.

AU - Cravens, J. P.

AU - Kropp, W. R.

AU - Liu, D. W.

AU - Mine, S.

AU - Regis, C.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Sterner, C. W.

AU - Vagins, M. R.

AU - Ganezer, K. S.

AU - Hill, J. E.

AU - Keig, W. E.

AU - Jang, J. S.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Scholberg, K.

AU - Walter, C. W.

AU - Wendell, R.

AU - Ellsworth, R. W.

AU - Tasaka, S.

AU - Guillian, E.

AU - Kibayashi, A.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Messier, M. D.

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 - 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 - Blaufuss, E.

AU - Goodman, J. A.

AU - Sullivan, G. W.

AU - Turcan, D.

AU - Cooley, J.

AU - Habig, A.

AU - Fukuda, Y.

AU - Sato, T.

AU - Itow, Y.

AU - Jung, C. K.

AU - Kato, T.

AU - Kobayashi, K.

AU - Malek, M.

AU - Mauger, C.

AU - McGrew, C.

AU - Sarrat, A.

AU - Yanagisawa, C.

AU - Tamura, N.

AU - Sakuda, Makoto

AU - Kuno, Y.

AU - Yoshida, M.

AU - Kim, S. B.

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 - Shirai, J.

AU - Suzuki, A.

AU - Nishijima, K.

AU - Ishino, H.

AU - Watanabe, Y.

AU - Koshiba, M.

AU - Kielczewska, D.

AU - Zalipska, J.

AU - Berns, H. G.

AU - Gran, R.

AU - Shiraishi, K. K.

AU - Stachyra, A.

AU - Washburn, K.

AU - Wilkes, R. J.

PY - 2006

Y1 - 2006

N2 - We report on the results of a three-flavor oscillation analysis using Super-Kamiokande I atmospheric neutrino data, with the assumption of one mass scale dominance (Δm122=0). No significant flux change due to matter effect, which occurs when neutrinos propagate inside the Earth for θ13≠0, has been seen either in a multi-GeV νe-rich sample or in a νμ-rich sample. Both normal and inverted mass hierarchy hypotheses are tested and both are consistent with observation. Using Super-Kamiokande data only, 2-dimensional 90% confidence allowed regions are obtained: mixing angles are constrained to sin 2θ13<0.14 and 0.37

AB - We report on the results of a three-flavor oscillation analysis using Super-Kamiokande I atmospheric neutrino data, with the assumption of one mass scale dominance (Δm122=0). No significant flux change due to matter effect, which occurs when neutrinos propagate inside the Earth for θ13≠0, has been seen either in a multi-GeV νe-rich sample or in a νμ-rich sample. Both normal and inverted mass hierarchy hypotheses are tested and both are consistent with observation. Using Super-Kamiokande data only, 2-dimensional 90% confidence allowed regions are obtained: mixing angles are constrained to sin 2θ13<0.14 and 0.37

UR - http://www.scopus.com/inward/record.url?scp=33746835287&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33746835287&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.74.032002

DO - 10.1103/PhysRevD.74.032002

M3 - Article

AN - SCOPUS:33746835287

SN - 0556-2821

VL - 74

JO - Physical Review D

JF - Physical Review D

IS - 3

M1 - 032002

ER -

Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande

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