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, Yusuke 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 & 92 others 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, Hirokazu 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

Research output: Contribution to journalArticle

122 Citations (Scopus)

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.

Original languageEnglish
Article number78
JournalAstrophysical Journal
Volume742
Issue number2
DOIs
Publication statusPublished - Dec 1 2011

Fingerprint

weakly interacting massive particles
muons
sun
neutrinos
cross section
scattering
stopping
scattering cross sections
energy
particle
analysis

Keywords

  • dark matter
  • neutrinos

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande. / Tanaka, T.; Abe, K.; Hayato, Y.; Iida, T.; Kameda, J.; Koshio, Yusuke; 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, J. L.; Stone, J. L.; Sulak, L. R.; Cravens, J. P.; Bays, K.; Kropp, W. R.; Mine, S.; Regis, C.; Smy, M. B.; Sobel, H. W.; Ganezer, K. S.; Hill, J.; Keig, W. E.; Jang, J. S.; Kim, J. Y.; Lim, I. T.; Albert, J. B.; Scholberg, K.; Walter, C. W.; Wendell, R.; Wongjirad, T.; Ishizuka, T.; Tasaka, S.; Learned, J. G.; 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, A. T.; Takeuchi, Y.; Ikeda, M.; Minamino, A.; Nakaya, T.; Labarga, L.; Fukuda, Y.; Itow, Y.; Mitsuka, G.; Jung, C. K.; McGrew, C.; Lopez, G.; Yanagisawa, C.; Tamura, N.; Ishino, Hirokazu; Kibayashi, A.; Sakuda, Makoto; Kuno, Y.; Yoshida, M.; Kim, S. B.; Yang, B. S.; 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, R. J.

In: Astrophysical Journal, Vol. 742, No. 2, 78, 01.12.2011.

Research output: Contribution to journalArticle

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
Tanaka, T. ; Abe, K. ; Hayato, Y. ; Iida, T. ; Kameda, J. ; Koshio, Yusuke ; 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, J. L. ; Stone, J. L. ; Sulak, L. R. ; Cravens, J. P. ; Bays, K. ; Kropp, W. R. ; Mine, S. ; Regis, C. ; Smy, M. B. ; Sobel, H. W. ; Ganezer, K. S. ; Hill, J. ; Keig, W. E. ; Jang, J. S. ; Kim, J. Y. ; Lim, I. T. ; Albert, J. B. ; Scholberg, K. ; Walter, C. W. ; Wendell, R. ; Wongjirad, T. ; Ishizuka, T. ; Tasaka, S. ; Learned, J. G. ; 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, A. T. ; Takeuchi, Y. ; Ikeda, M. ; Minamino, A. ; Nakaya, T. ; Labarga, L. ; Fukuda, Y. ; Itow, Y. ; Mitsuka, G. ; Jung, C. K. ; McGrew, C. ; Lopez, G. ; Yanagisawa, C. ; Tamura, N. ; Ishino, Hirokazu ; Kibayashi, A. ; Sakuda, Makoto ; Kuno, Y. ; Yoshida, M. ; Kim, S. B. ; Yang, B. S. ; 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, R. J. / An indirect search for weakly interacting massive particles in the sun using 3109.6days of upward-going muons in super-kamiokande. In: Astrophysical Journal. 2011 ; Vol. 742, No. 2.
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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.",
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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, Yusuke

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, Hirokazu

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

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

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JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

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