Evidence for an oscillatory signature in atmospheric neutrino oscillations

Y. Ashie; J. Hosaka; K. Ishihara; Y. Itow; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; T. Namba; R. Nambu; Y. Obayashi; M. Shiozawa; Y. Suzuki; Y. Takeuchi; K. Taki; S. Yamada; M. Ishitsuka; T. Kajita; K. Kaneyuki; S. Nakayama; A. Okada; K. Okumura; T. Ooyabu; C. Saji; Y. Takenaga; S. Desai; E. Kearns; S. Likhoded; J. L. Stone; L. R. Sulak; C. W. Walter; W. Wang; M. Goldhaber; D. Casper; J. P. Cravens; W. Gajewski; W. R. Kropp; D. W. Liu; S. Mine; M. B. Smy; H. W. Sobel; C. W. Sterner; M. R. Vagins; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; R. W. Ellsworth; S. Tasaka; G. Guillian; A. Kibayashi; J. G. Learned; S. Matsuno; D. Takemori; M. D. Messier; Y. Hayato; A. K. Ichikawa; T. Ishida; T. Ishii; T. Iwashita; 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. W. Sullivan; D. Turcan; K. Scholberg; A. Habig; Y. Fukuda; C. K. Jung; T. Kato; K. Kobayashi; M. Malek; C. Mauger; C. McGrew; A. Sarrat; E. Sharkey; C. Yanagisawa; T. Toshito; K. Miyano; N. Tamura; J. Ishii; Y. Kuno; Y. Nagashima; M. Takita; M. Yoshida; 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; Y. Nakajima; K. Nishijima; T. Harada; H. Ishino; R. Nishimura; Y. Watanabe; D. Kielczewska; J. Zalipska; H. G. Berns; R. Gran; K. K. Shiraishi; A. Stachyra; K. Washburn; R. J. Wilkes

doi:10.1103/PhysRevLett.93.101801

Evidence for an oscillatory signature in atmospheric neutrino oscillations

Y. Ashie
, J. Hosaka
, K. Ishihara
, Y. Itow
, J. Kameda
, Y. Koshio
, A. Minamino
, C. Mitsuda
, M. Miura
, S. Moriyama
, M. Nakahata
, T. Namba
, R. Nambu
, Y. Obayashi
, M. Shiozawa
, Y. Suzuki
, Y. Takeuchi
, K. Taki
, S. Yamada
, M. Ishitsuka

T. Kajita, K. Kaneyuki, S. Nakayama, A. Okada, K. Okumura, T. Ooyabu, C. Saji, Y. Takenaga, S. Desai, E. Kearns, S. Likhoded, J. L. Stone, L. R. Sulak, C. W. Walter, W. Wang, M. Goldhaber, D. Casper, J. P. Cravens, W. Gajewski, W. R. Kropp, D. W. Liu, S. Mine, M. B. Smy, H. W. Sobel, C. W. Sterner, M. R. Vagins, K. S. Ganezer, J. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, R. W. Ellsworth, S. Tasaka, G. Guillian, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, M. D. Messier, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, 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. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, Y. Fukuda, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. Mauger, C. McGrew, A. Sarrat, E. Sharkey, C. Yanagisawa, T. Toshito, K. Miyano, N. Tamura, J. Ishii, Y. Kuno, Y. Nagashima, M. Takita, M. Yoshida, 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, Y. Nakajima, K. Nishijima, T. Harada, H. Ishino, R. Nishimura, Y. Watanabe, D. Kielczewska, J. Zalipska, H. G. Berns, R. Gran, K. K. Shiraishi, A. Stachyra, K. Washburn, R. J. Wilkes

Physics & Astronomy (Duluth)

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

688 Scopus citations

Abstract

The survival probability of muon neutrinos was analyzed as a function of L/E using atmospheric neutrino events observed in Super-Kamiokande. Alternative models that could explain the zenith angle and energy dependent deficit of the atmospheric muon neutrinos were disfavored. The neutrino energy was estimated from the total energy of charged particles observed in the inner detector (ID). It was concluded that the observed L/E distribution gives the first direct evidence that the neutrino survival probability obeys the sinusoidal function as predicted by neutrino flavor oscillations.

Original language	English (US)
Article number	101801
Pages (from-to)	101801-1-101801-6
Journal	Physical review letters
Volume	93
Issue number	10
DOIs	https://doi.org/10.1103/PhysRevLett.93.101801
State	Published - Sep 3 2004

Bibliographical note

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

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10.1103/PhysRevLett.93.101801

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Ashie, Y., Hosaka, J., Ishihara, K., Itow, Y., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Namba, T., Nambu, R., Obayashi, Y., Shiozawa, M., Suzuki, Y., Takeuchi, Y., Taki, K., Yamada, S., ... Wilkes, R. J. (2004). Evidence for an oscillatory signature in atmospheric neutrino oscillations. Physical review letters, 93(10), 101801-1-101801-6. Article 101801. https://doi.org/10.1103/PhysRevLett.93.101801

Ashie, Y, Hosaka, J, Ishihara, K, Itow, Y, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Namba, T, Nambu, R, Obayashi, Y, Shiozawa, M, Suzuki, Y, Takeuchi, Y, Taki, K, Yamada, S, Ishitsuka, M, Kajita, T, Kaneyuki, K, Nakayama, S, Okada, A, Okumura, K, Ooyabu, T, Saji, C, Takenaga, Y, Desai, S, Kearns, E, Likhoded, S, Stone, JL, Sulak, LR, Walter, CW, Wang, W, Goldhaber, M, Casper, D, Cravens, JP, Gajewski, W, Kropp, WR, Liu, DW, Mine, S, Smy, MB, Sobel, HW, Sterner, CW, Vagins, MR, Ganezer, KS, Hill, J, Keig, WE, Jang, JS, Kim, JY, Lim, IT, Ellsworth, RW, Tasaka, S, Guillian, G, Kibayashi, A, Learned, JG, Matsuno, S, Takemori, D, Messier, MD, Hayato, Y, Ichikawa, AK, Ishida, T, Ishii, T, Iwashita, T, 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, Sullivan, GW, Turcan, D, Scholberg, K, Habig, A, Fukuda, Y, Jung, CK, Kato, T, Kobayashi, K, Malek, M, Mauger, C, McGrew, C, Sarrat, A, Sharkey, E, Yanagisawa, C, Toshito, T, Miyano, K, Tamura, N, Ishii, J, Kuno, Y, Nagashima, Y, Takita, M, Yoshida, M, Kim, SB, Yoo, J, Okazawa, H, Ishizuka, T, Choi, Y, Seo, HK, Gando, Y, Hasegawa, T, Inoue, K, Shirai, J, Suzuki, A, Koshiba, M, Nakajima, Y, Nishijima, K, Harada, T, Ishino, H, Nishimura, R, Watanabe, Y, Kielczewska, D, Zalipska, J, Berns, HG, Gran, R, Shiraishi, KK, Stachyra, A, Washburn, K & Wilkes, RJ 2004, 'Evidence for an oscillatory signature in atmospheric neutrino oscillations', Physical review letters, vol. 93, no. 10, 101801, pp. 101801-1-101801-6. https://doi.org/10.1103/PhysRevLett.93.101801

@article{379fd9cfe4794ffab7f7e20da9e440f1,

title = "Evidence for an oscillatory signature in atmospheric neutrino oscillations",

abstract = "The survival probability of muon neutrinos was analyzed as a function of L/E using atmospheric neutrino events observed in Super-Kamiokande. Alternative models that could explain the zenith angle and energy dependent deficit of the atmospheric muon neutrinos were disfavored. The neutrino energy was estimated from the total energy of charged particles observed in the inner detector (ID). It was concluded that the observed L/E distribution gives the first direct evidence that the neutrino survival probability obeys the sinusoidal function as predicted by neutrino flavor oscillations.",

author = "Y. Ashie and J. Hosaka and K. Ishihara and Y. Itow 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 R. Nambu and Y. Obayashi and M. Shiozawa and Y. Suzuki and Y. Takeuchi and K. Taki and S. Yamada and M. Ishitsuka and T. Kajita and K. Kaneyuki and S. Nakayama and A. Okada and K. Okumura and T. Ooyabu and C. Saji and Y. Takenaga and S. Desai and E. Kearns and S. Likhoded and Stone, \{J. L.\} and Sulak, \{L. R.\} and Walter, \{C. W.\} and W. Wang and M. Goldhaber and D. Casper and Cravens, \{J. P.\} and W. Gajewski and Kropp, \{W. R.\} and Liu, \{D. W.\} 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 Jang, \{J. S.\} and Kim, \{J. Y.\} and Lim, \{I. T.\} and Ellsworth, \{R. W.\} and S. Tasaka and G. Guillian and A. Kibayashi and Learned, \{J. G.\} and S. Matsuno and D. Takemori 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. 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 Sullivan, \{G. W.\} and D. Turcan and K. Scholberg and A. Habig and Y. Fukuda and Jung, \{C. K.\} and T. Kato and K. Kobayashi and M. Malek and C. Mauger and C. McGrew and A. Sarrat and E. Sharkey and C. Yanagisawa and T. Toshito and K. Miyano and N. Tamura and J. Ishii and Y. Kuno and Y. Nagashima and M. Takita and M. Yoshida 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 Y. Nakajima and K. Nishijima and T. Harada and H. Ishino and R. Nishimura and Y. Watanabe 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.\}",

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

year = "2004",

month = sep,

day = "3",

doi = "10.1103/PhysRevLett.93.101801",

language = "English (US)",

volume = "93",

pages = "101801--1--101801--6",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "10",

}

TY - JOUR

T1 - Evidence for an oscillatory signature in atmospheric neutrino oscillations

AU - Ashie, Y.

AU - Hosaka, J.

AU - Ishihara, K.

AU - Itow, Y.

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 - Nambu, R.

AU - Obayashi, Y.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeuchi, Y.

AU - Taki, K.

AU - Yamada, S.

AU - Ishitsuka, M.

AU - Kajita, T.

AU - Kaneyuki, K.

AU - Nakayama, S.

AU - Okada, A.

AU - Okumura, K.

AU - Ooyabu, T.

AU - Saji, C.

AU - Takenaga, Y.

AU - Desai, S.

AU - Kearns, E.

AU - Likhoded, S.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Walter, C. W.

AU - Wang, W.

AU - Goldhaber, M.

AU - Casper, D.

AU - Cravens, J. P.

AU - Gajewski, W.

AU - Kropp, W. R.

AU - Liu, D. W.

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 - Jang, J. S.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Ellsworth, R. W.

AU - Tasaka, S.

AU - Guillian, G.

AU - Kibayashi, A.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Takemori, D.

AU - Messier, M. D.

AU - Hayato, Y.

AU - Ichikawa, A. K.

AU - Ishida, T.

AU - Ishii, T.

AU - Iwashita, T.

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 - Sullivan, G. W.

AU - Turcan, D.

AU - Scholberg, K.

AU - Habig, A.

AU - Fukuda, Y.

AU - Jung, C. K.

AU - Kato, T.

AU - Kobayashi, K.

AU - Malek, M.

AU - Mauger, C.

AU - McGrew, C.

AU - Sarrat, A.

AU - Sharkey, E.

AU - Yanagisawa, C.

AU - Toshito, T.

AU - Miyano, K.

AU - Tamura, N.

AU - Ishii, J.

AU - Kuno, Y.

AU - Nagashima, Y.

AU - Takita, M.

AU - Yoshida, M.

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 - Nakajima, Y.

AU - Nishijima, K.

AU - Harada, T.

AU - Ishino, H.

AU - Nishimura, R.

AU - Watanabe, Y.

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.

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

PY - 2004/9/3

Y1 - 2004/9/3

N2 - The survival probability of muon neutrinos was analyzed as a function of L/E using atmospheric neutrino events observed in Super-Kamiokande. Alternative models that could explain the zenith angle and energy dependent deficit of the atmospheric muon neutrinos were disfavored. The neutrino energy was estimated from the total energy of charged particles observed in the inner detector (ID). It was concluded that the observed L/E distribution gives the first direct evidence that the neutrino survival probability obeys the sinusoidal function as predicted by neutrino flavor oscillations.

AB - The survival probability of muon neutrinos was analyzed as a function of L/E using atmospheric neutrino events observed in Super-Kamiokande. Alternative models that could explain the zenith angle and energy dependent deficit of the atmospheric muon neutrinos were disfavored. The neutrino energy was estimated from the total energy of charged particles observed in the inner detector (ID). It was concluded that the observed L/E distribution gives the first direct evidence that the neutrino survival probability obeys the sinusoidal function as predicted by neutrino flavor oscillations.

UR - https://www.scopus.com/pages/publications/20844449061

UR - https://www.scopus.com/pages/publications/20844449061#tab=citedBy

U2 - 10.1103/PhysRevLett.93.101801

DO - 10.1103/PhysRevLett.93.101801

M3 - Article

AN - SCOPUS:20844449061

SN - 0031-9007

VL - 93

SP - 101801-1-101801-6

JO - Physical review letters

JF - Physical review letters

IS - 10

M1 - 101801

ER -

Evidence for an oscillatory signature in atmospheric neutrino oscillations

Abstract

Bibliographical note

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