Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I

M. E.C. Swanson; K. Abe; J. Hosaka; T. Iida; K. Ishihara; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; Y. Obayashi; H. Ogawa; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takeuchi; K. Ueshima; I. Higuchi; C. Ishihara; M. Ishitsuka; T. Kajita; K. Kaneyuki; G. Mitsuka; S. Nakayama; H. Nishino; A. Okada; 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. P. Cravens; 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. E. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; 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. 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; J. Cooley; K. B.M. Mahn; A. Habig; Y. Fukuda; T. Sato; Y. Itow; T. Koike; C. K. Jung; T. Kato; K. Kobayashi; M. Malek; C. McGrew; A. Sarrat; R. Terri; C. Yanagisawa; N. Tamura; 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; H. Ishii; K. Nishijima; H. Ishino; Y. Watanabe; M. Koshiba; D. Kielczewska; J. Zalipska; H. G. Berns; R. Gran; K. K. Shiraishi; A. Stachyra; E. Thrane; K. Washburn; R. J. Wilkes

doi:10.1086/507983

Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I

M. E.C. Swanson^*, K. Abe, J. Hosaka, T. Iida, K. Ishihara, J. Kameda, Y. Koshio, A. Minamino, C. Mitsuda, M. Miura, S. Moriyama, M. Nakahata, Y. Obayashi, H. Ogawa, M. Shiozawa, Y. Suzuki, A. Takeda, Y. Takeuchi, K. Ueshima, I. HiguchiC. Ishihara, M. Ishitsuka, T. Kajita, K. Kaneyuki, G. Mitsuka, S. Nakayama, H. Nishino, A. Okada, 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. P. Cravens, 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. E. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, 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. 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, J. Cooley, K. B.M. Mahn, A. Habig, Y. Fukuda, T. Sato, Y. Itow, T. Koike, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. McGrew, A. Sarrat, R. Terri, C. Yanagisawa, N. Tamura, 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, H. Ishii, K. Nishijima, H. Ishino, Y. Watanabe, M. Koshiba, D. Kielczewska, J. Zalipska, H. G. Berns, R. Gran, K. K. Shiraishi, A. Stachyra, E. Thrane, K. Washburn, R. J. Wilkes

^*この研究の対応する著者

研究成果: Article › 査読

20 被引用数 (Scopus)

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Many astrophysical models predict a diffuse flux of high-energy neutrinos from active galactic nuclei and other extragalactic sources. At muon energies above 1 TeV, the upward-going muon flux induced by neutrinos from active galactic nuclei is expected to exceed the flux due to atmospheric neutrinos. We have performed a search for this astrophysical neutrino flux by looking for upward-going muons in the highest energy data sample from the Super-Kamiokande detector using 1679.6 live days of data. We found one extremely high energy upward-going muon event, compared with an expected atmospheric neutrino background of 0.46 ± 0.23 events. Using this result, we set an upper limit on the diffuse flux of upward-going muons due to neutrinos from astrophysical sources in the muon energy range 3.16-100 TeV.

本文言語	English
ページ（範囲）	206-215
ページ数	10
ジャーナル	Astrophysical Journal
巻	652
号	1 I
DOI	https://doi.org/10.1086/507983
出版ステータス	Published - 2006 11月 20
外部発表	はい

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.1086/507983

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Swanson, M. E. C., Abe, K., Hosaka, J., Iida, T., Ishihara, K., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Obayashi, Y., Ogawa, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takeuchi, Y., Ueshima, K., ... Wilkes, R. J. (2006). Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I. Astrophysical Journal, 652(1 I), 206-215. https://doi.org/10.1086/507983

Swanson, MEC, Abe, K, Hosaka, J, Iida, T, Ishihara, K, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Obayashi, Y, Ogawa, H, Shiozawa, M, Suzuki, Y, Takeda, A, Takeuchi, Y, Ueshima, K, Higuchi, I, Ishihara, C, Ishitsuka, M, Kajita, T, Kaneyuki, K, Mitsuka, G, Nakayama, S, Nishino, H, Okada, A, 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, Cravens, JP, Dunmore, J, Kropp, WR, Liu, DW, Mine, S, Regis, C, Smy, MB, Sobel, HW, Vagins, MR, Ganezer, KS, Hill, JE, Keig, WE, Jang, JS, Kim, JY, Lim, IT, Scholberg, K, Tanimoto, N, Walter, CW, Wendell, R, Ellsworth, RW, Tasaka, S, Guillian, G, 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, 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, Cooley, J, Mahn, KBM, Habig, A, Fukuda, Y, Sato, T, Itow, Y, Koike, T, Jung, CK, Kato, T, Kobayashi, K, Malek, M, McGrew, C, Sarrat, A, Terri, R, Yanagisawa, C, Tamura, N, 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, Ishii, H, Nishijima, K, Ishino, H, Watanabe, Y, Koshiba, M, Kielczewska, D, Zalipska, J, Berns, HG, Gran, R, Shiraishi, KK, Stachyra, A, Thrane, E, Washburn, K & Wilkes, RJ 2006, 'Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I', Astrophysical Journal, vol. 652, no. 1 I, pp. 206-215. https://doi.org/10.1086/507983

@article{ff9f6c81369542968771647469372a40,

title = "Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I",

abstract = "Many astrophysical models predict a diffuse flux of high-energy neutrinos from active galactic nuclei and other extragalactic sources. At muon energies above 1 TeV, the upward-going muon flux induced by neutrinos from active galactic nuclei is expected to exceed the flux due to atmospheric neutrinos. We have performed a search for this astrophysical neutrino flux by looking for upward-going muons in the highest energy data sample from the Super-Kamiokande detector using 1679.6 live days of data. We found one extremely high energy upward-going muon event, compared with an expected atmospheric neutrino background of 0.46 ± 0.23 events. Using this result, we set an upper limit on the diffuse flux of upward-going muons due to neutrinos from astrophysical sources in the muon energy range 3.16-100 TeV.",

keywords = "Galaxies: active, Gamma rays: bursts, Neutrinos",

author = "Swanson, {M. E.C.} and K. Abe and J. Hosaka 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 Y. Obayashi and H. Ogawa and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takeuchi and K. Ueshima and I. Higuchi and C. Ishihara 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 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 Cravens, {J. P.} 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 Hill, {J. E.} and Keig, {W. E.} and Jang, {J. S.} and Kim, {J. Y.} and Lim, {I. T.} 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. 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 J. Cooley and Mahn, {K. B.M.} and A. Habig and Y. Fukuda and T. Sato and Y. Itow and T. Koike 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 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 H. Ishii 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 E. Thrane and K. Washburn and Wilkes, {R. J.}",

year = "2006",

month = nov,

day = "20",

doi = "10.1086/507983",

language = "English",

volume = "652",

pages = "206--215",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1 I",

}

TY - JOUR

T1 - Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I

AU - Swanson, M. E.C.

AU - Abe, K.

AU - Hosaka, J.

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 - Obayashi, Y.

AU - Ogawa, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Takeuchi, Y.

AU - Ueshima, K.

AU - Higuchi, I.

AU - Ishihara, C.

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 - 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 - Cravens, J. P.

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. E.

AU - Keig, W. E.

AU - Jang, J. S.

AU - Kim, J. Y.

AU - Lim, I. T.

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 - 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 - Cooley, J.

AU - Mahn, K. B.M.

AU - Habig, A.

AU - Fukuda, Y.

AU - Sato, T.

AU - Itow, Y.

AU - Koike, 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 - 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 - Ishii, H.

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 - Thrane, E.

AU - Washburn, K.

AU - Wilkes, R. J.

PY - 2006/11/20

Y1 - 2006/11/20

N2 - Many astrophysical models predict a diffuse flux of high-energy neutrinos from active galactic nuclei and other extragalactic sources. At muon energies above 1 TeV, the upward-going muon flux induced by neutrinos from active galactic nuclei is expected to exceed the flux due to atmospheric neutrinos. We have performed a search for this astrophysical neutrino flux by looking for upward-going muons in the highest energy data sample from the Super-Kamiokande detector using 1679.6 live days of data. We found one extremely high energy upward-going muon event, compared with an expected atmospheric neutrino background of 0.46 ± 0.23 events. Using this result, we set an upper limit on the diffuse flux of upward-going muons due to neutrinos from astrophysical sources in the muon energy range 3.16-100 TeV.

AB - Many astrophysical models predict a diffuse flux of high-energy neutrinos from active galactic nuclei and other extragalactic sources. At muon energies above 1 TeV, the upward-going muon flux induced by neutrinos from active galactic nuclei is expected to exceed the flux due to atmospheric neutrinos. We have performed a search for this astrophysical neutrino flux by looking for upward-going muons in the highest energy data sample from the Super-Kamiokande detector using 1679.6 live days of data. We found one extremely high energy upward-going muon event, compared with an expected atmospheric neutrino background of 0.46 ± 0.23 events. Using this result, we set an upper limit on the diffuse flux of upward-going muons due to neutrinos from astrophysical sources in the muon energy range 3.16-100 TeV.

KW - Galaxies: active

KW - Gamma rays: bursts

KW - Neutrinos

UR - http://www.scopus.com/inward/record.url?scp=33845286498&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33845286498&partnerID=8YFLogxK

U2 - 10.1086/507983

DO - 10.1086/507983

M3 - Article

AN - SCOPUS:33845286498

SN - 0004-637X

VL - 652

SP - 206

EP - 215

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 I

ER -

Search for diffuse astrophysical neutrino flux using ultra-high-energy upward-going muons in super-kamiokande I

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