An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande

T. Tanaka; K. Abe; Y. Hayato; T. Iida; J. Kameda; Y. Koshio; Y. Kouzuma; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; K. Ueno; K. Ueshima; S. Yamada; T. Yokozawa; C. Ishihara; S. Hazama; H. Kaji; T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; F. Dufour; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; J. P. Cravens; K. Bays; W. R. Kropp; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. B. Albert; K. Scholberg; C. W. Walter; R. Wendell; T. Wongjirad; T. Ishizuka; S. Tasaka; J. G. Learned; S. Matsuno; S. Smith; K. Martens; M. Vagins; Y. Watanabe; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; H. Nishino; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; M. Ikeda; A. Minamino; T. Nakaya; L. Labarga; Y. Fukuda; Y. Itow; G. Mitsuka; C. K. Jung; C. McGrew; G. Lopez; C. Yanagisawa; N. Tamura; H. Ishino; A. Kibayashi; Makoto Sakuda; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; H. Okazawa; Y. Choi; K. Nishijima; Y. Yokosawa; M. Koshiba; Y. Totsuka; M. Yokoyama; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; E. Thrane; R. J. Wilkes

doi:10.1088/0004-637X/742/2/78

An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande

T. Tanaka, K. Abe, Y. Hayato, T. Iida, J. Kameda, Y. Koshio, Y. Kouzuma, M. Miura, S. Moriyama, M. Nakahata, S. Nakayama, Y. Obayashi, H. Sekiya, M. Shiozawa, Y. Suzuki, A. Takeda, Y. Takenaga, K. Ueno, K. Ueshima, S. YamadaT. Yokozawa, C. Ishihara, S. Hazama, H. Kaji, T. Kajita, K. Kaneyuki, T. McLachlan, K. Okumura, Y. Shimizu, N. Tanimoto, F. Dufour, E. Kearns, M. Litos, J. L. Raaf, J. L. Stone, L. R. Sulak, J. P. Cravens, K. Bays, W. R. Kropp, S. Mine, C. Regis, M. B. Smy, H. W. Sobel, K. S. Ganezer, J. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, J. B. Albert, K. Scholberg, C. W. Walter, R. Wendell, T. Wongjirad, T. Ishizuka, S. Tasaka, J. G. Learned, S. Matsuno, S. Smith, K. Martens, M. Vagins, Y. Watanabe, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nishikawa, H. Nishino, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki, Y. Takeuchi, M. Ikeda, A. Minamino, T. Nakaya, L. Labarga, Y. Fukuda, Y. Itow, G. Mitsuka, C. K. Jung, C. McGrew, G. Lopez, C. Yanagisawa, N. Tamura, H. Ishino, A. Kibayashi, Makoto Sakuda, Y. Kuno, M. Yoshida, S. B. Kim, B. S. Yang, H. Okazawa, Y. Choi, K. Nishijima, Y. Yokosawa, M. Koshiba, Y. Totsuka, M. Yokoyama, S. Chen, Y. Heng, Z. Yang, H. Zhang, D. Kielczewska, P. Mijakowski, K. Connolly, M. Dziomba, E. Thrane, R. J. Wilkes

研究成果 › 査読

150 被引用数 (Scopus)

抄録

We present the result of an indirect search for high energy neutrinos from Weakly Interacting Massive Particle (WIMP) annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Data sets from SKI-SKIII (3109.6days) were used for the analysis. We looked for an excess of neutrino signal from the Sun as compared with the expected atmospheric neutrino background in three upmu categories: stopping, non-showering, and showering. No significant excess was observed. The 90% C.L. upper limits of upmu flux induced by WIMPs of 100GeV c^-2 were 6.4 × 10^-15cm ^-2s^-1 and 4.0 × 10^-15cm ^-2s^-1 for the soft and hard annihilation channels, respectively. These limits correspond to upper limits of 4.5 × 10 ^-39cm^-2 and 2.7 × 10^-40cm^-2 for spin-dependent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively.

本文言語	English
論文番号	78
ジャーナル	Astrophysical Journal
巻	742
号	2
DOI	https://doi.org/10.1088/0004-637X/742/2/78
出版ステータス	Published - 12月 1 2011

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

文献へのアクセス

10.1088/0004-637X/742/2/78

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引用スタイル

Tanaka, T., Abe, K., Hayato, Y., Iida, T., Kameda, J., Koshio, Y., Kouzuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueno, K., Ueshima, K., ... Wilkes, R. J. (2011). An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande. Astrophysical Journal, 742(2), [78]. https://doi.org/10.1088/0004-637X/742/2/78

Tanaka, T, Abe, K, Hayato, Y, Iida, T, Kameda, J, Koshio, Y, Kouzuma, Y, Miura, M, Moriyama, S, Nakahata, M, Nakayama, S, Obayashi, Y, Sekiya, H, Shiozawa, M, Suzuki, Y, Takeda, A, Takenaga, Y, Ueno, K, Ueshima, K, Yamada, S, Yokozawa, T, Ishihara, C, Hazama, S, Kaji, H, Kajita, T, Kaneyuki, K, McLachlan, T, Okumura, K, Shimizu, Y, Tanimoto, N, Dufour, F, Kearns, E, Litos, M, Raaf, JL, Stone, JL, Sulak, LR, Cravens, JP, Bays, K, Kropp, WR, Mine, S, Regis, C, Smy, MB, Sobel, HW, Ganezer, KS, Hill, J, Keig, WE, Jang, JS, Kim, JY, Lim, IT, Albert, JB, Scholberg, K, Walter, CW, Wendell, R, Wongjirad, T, Ishizuka, T, Tasaka, S, Learned, JG, Matsuno, S, Smith, S, Martens, K, Vagins, M, Watanabe, Y, Hasegawa, T, Ishida, T, Ishii, T, Kobayashi, T, Nakadaira, T, Nakamura, K, Nishikawa, K, Nishino, H, Oyama, Y, Sakashita, K, Sekiguchi, T, Tsukamoto, T, Suzuki, AT, Takeuchi, Y, Ikeda, M, Minamino, A, Nakaya, T, Labarga, L, Fukuda, Y, Itow, Y, Mitsuka, G, Jung, CK, McGrew, C, Lopez, G, Yanagisawa, C, Tamura, N, Ishino, H, Kibayashi, A, Sakuda, M, Kuno, Y, Yoshida, M, Kim, SB, Yang, BS, Okazawa, H, Choi, Y, Nishijima, K, Yokosawa, Y, Koshiba, M, Totsuka, Y, Yokoyama, M, Chen, S, Heng, Y, Yang, Z, Zhang, H, Kielczewska, D, Mijakowski, P, Connolly, K, Dziomba, M, Thrane, E & Wilkes, RJ 2011, 'An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande', Astrophysical Journal, vol. 742, no. 2, 78. https://doi.org/10.1088/0004-637X/742/2/78

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title = "An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande",

abstract = "We present the result of an indirect search for high energy neutrinos from Weakly Interacting Massive Particle (WIMP) annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Data sets from SKI-SKIII (3109.6days) were used for the analysis. We looked for an excess of neutrino signal from the Sun as compared with the expected atmospheric neutrino background in three upmu categories: stopping, non-showering, and showering. No significant excess was observed. The 90% C.L. upper limits of upmu flux induced by WIMPs of 100GeV c-2 were 6.4 × 10-15cm -2s-1 and 4.0 × 10-15cm -2s-1 for the soft and hard annihilation channels, respectively. These limits correspond to upper limits of 4.5 × 10 -39cm-2 and 2.7 × 10-40cm-2 for spin-dependent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively.",

keywords = "dark matter, neutrinos",

author = "T. Tanaka and K. Abe and Y. Hayato and T. Iida and J. Kameda and Y. Koshio and Y. Kouzuma and M. Miura and S. Moriyama and M. Nakahata and S. Nakayama and Y. Obayashi and H. Sekiya and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takenaga and K. Ueno and K. Ueshima and S. Yamada and T. Yokozawa and C. Ishihara and S. Hazama and H. Kaji and T. Kajita and K. Kaneyuki and T. McLachlan and K. Okumura and Y. Shimizu and N. Tanimoto and F. Dufour and E. Kearns and M. Litos and Raaf, {J. L.} and Stone, {J. L.} and Sulak, {L. R.} and Cravens, {J. P.} and K. Bays and Kropp, {W. R.} and S. Mine and C. Regis and Smy, {M. B.} and Sobel, {H. W.} and Ganezer, {K. S.} and J. Hill and Keig, {W. E.} and Jang, {J. S.} and Kim, {J. Y.} and Lim, {I. T.} and Albert, {J. B.} and K. Scholberg and Walter, {C. W.} and R. Wendell and T. Wongjirad and T. Ishizuka and S. Tasaka and Learned, {J. G.} and S. Matsuno and S. Smith and K. Martens and M. Vagins and Y. Watanabe and T. Hasegawa and T. Ishida and T. Ishii and T. Kobayashi and T. Nakadaira and K. Nakamura and K. Nishikawa and H. Nishino and Y. Oyama and K. Sakashita and T. Sekiguchi and T. Tsukamoto and Suzuki, {A. T.} and Y. Takeuchi and M. Ikeda and A. Minamino and T. Nakaya and L. Labarga and Y. Fukuda and Y. Itow and G. Mitsuka and Jung, {C. K.} and C. McGrew and G. Lopez and C. Yanagisawa and N. Tamura and H. Ishino and A. Kibayashi and Makoto Sakuda and Y. Kuno and M. Yoshida and Kim, {S. B.} and Yang, {B. S.} and H. Okazawa and Y. Choi and K. Nishijima and Y. Yokosawa and M. Koshiba and Y. Totsuka and M. Yokoyama and S. Chen and Y. Heng and Z. Yang and H. Zhang and D. Kielczewska and P. Mijakowski and K. Connolly and M. Dziomba and E. Thrane and Wilkes, {R. J.}",

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doi = "10.1088/0004-637X/742/2/78",

language = "English",

volume = "742",

journal = "Astrophysical Journal",

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TY - JOUR

T1 - An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande

AU - Tanaka, T.

AU - Abe, K.

AU - Hayato, Y.

AU - Iida, T.

AU - Kameda, J.

AU - Koshio, Y.

AU - Kouzuma, Y.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakayama, S.

AU - Obayashi, Y.

AU - Sekiya, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Takenaga, Y.

AU - Ueno, K.

AU - Ueshima, K.

AU - Yamada, S.

AU - Yokozawa, T.

AU - Ishihara, C.

AU - Hazama, S.

AU - Kaji, H.

AU - Kajita, T.

AU - Kaneyuki, K.

AU - McLachlan, T.

AU - Okumura, K.

AU - Shimizu, Y.

AU - Tanimoto, N.

AU - Dufour, F.

AU - Kearns, E.

AU - Litos, M.

AU - Raaf, J. L.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Cravens, J. P.

AU - Bays, K.

AU - Kropp, W. R.

AU - Mine, S.

AU - Regis, C.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Ganezer, K. S.

AU - Hill, J.

AU - Keig, W. E.

AU - Jang, J. S.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Albert, J. B.

AU - Scholberg, K.

AU - Walter, C. W.

AU - Wendell, R.

AU - Wongjirad, T.

AU - Ishizuka, T.

AU - Tasaka, S.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Smith, S.

AU - Martens, K.

AU - Vagins, M.

AU - Watanabe, Y.

AU - Hasegawa, T.

AU - Ishida, T.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Nakadaira, T.

AU - Nakamura, K.

AU - Nishikawa, K.

AU - Nishino, H.

AU - Oyama, Y.

AU - Sakashita, K.

AU - Sekiguchi, T.

AU - Tsukamoto, T.

AU - Suzuki, A. T.

AU - Takeuchi, Y.

AU - Ikeda, M.

AU - Minamino, A.

AU - Nakaya, T.

AU - Labarga, L.

AU - Fukuda, Y.

AU - Itow, Y.

AU - Mitsuka, G.

AU - Jung, C. K.

AU - McGrew, C.

AU - Lopez, G.

AU - Yanagisawa, C.

AU - Tamura, N.

AU - Ishino, H.

AU - Kibayashi, A.

AU - Sakuda, Makoto

AU - Kuno, Y.

AU - Yoshida, M.

AU - Kim, S. B.

AU - Yang, B. S.

AU - Okazawa, H.

AU - Choi, Y.

AU - Nishijima, K.

AU - Yokosawa, Y.

AU - Koshiba, M.

AU - Totsuka, Y.

AU - Yokoyama, M.

AU - Chen, S.

AU - Heng, Y.

AU - Yang, Z.

AU - Zhang, H.

AU - Kielczewska, D.

AU - Mijakowski, P.

AU - Connolly, K.

AU - Dziomba, M.

AU - Thrane, E.

AU - Wilkes, R. J.

PY - 2011/12/1

Y1 - 2011/12/1

N2 - We present the result of an indirect search for high energy neutrinos from Weakly Interacting Massive Particle (WIMP) annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Data sets from SKI-SKIII (3109.6days) were used for the analysis. We looked for an excess of neutrino signal from the Sun as compared with the expected atmospheric neutrino background in three upmu categories: stopping, non-showering, and showering. No significant excess was observed. The 90% C.L. upper limits of upmu flux induced by WIMPs of 100GeV c-2 were 6.4 × 10-15cm -2s-1 and 4.0 × 10-15cm -2s-1 for the soft and hard annihilation channels, respectively. These limits correspond to upper limits of 4.5 × 10 -39cm-2 and 2.7 × 10-40cm-2 for spin-dependent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively.

AB - We present the result of an indirect search for high energy neutrinos from Weakly Interacting Massive Particle (WIMP) annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Data sets from SKI-SKIII (3109.6days) were used for the analysis. We looked for an excess of neutrino signal from the Sun as compared with the expected atmospheric neutrino background in three upmu categories: stopping, non-showering, and showering. No significant excess was observed. The 90% C.L. upper limits of upmu flux induced by WIMPs of 100GeV c-2 were 6.4 × 10-15cm -2s-1 and 4.0 × 10-15cm -2s-1 for the soft and hard annihilation channels, respectively. These limits correspond to upper limits of 4.5 × 10 -39cm-2 and 2.7 × 10-40cm-2 for spin-dependent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively.

KW - dark matter

KW - neutrinos

UR - http://www.scopus.com/inward/record.url?scp=81255147981&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=81255147981&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/742/2/78

DO - 10.1088/0004-637X/742/2/78

M3 - Article

AN - SCOPUS:81255147981

SN - 0004-637X

VL - 742

JO - Astrophysical Journal

JF - Astrophysical Journal

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M1 - 78

ER -