High-Energy Neutrino Astronomy Using Upward-going Muons in Super-Kamiokande I

High-Energy Neutrino Astronomy Using Upward-going Muons in Super-Kamiokande I
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DOI：
10.1086/508016
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发表时间：
2006-06
期刊：
The Astrophysical Journal
影响因子：
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通讯作者：
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;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. Raaf;J. Stone;L. Sulak;W. Wang;M. Goldhaber;D. Casper;J. P. Cravens;J. Dunmore;W. Kropp;D. Liu;S. Mine;C. Regis;M. Smy;H. Sobel;M. Vagins;K. Ganezer;J. Hill;W. Keig;J. Jang;J. Kim;I. Lim;K. Scholberg;N. Tanimoto;C. Walter;R. Wendell;R. Ellsworth;S. Tasaka;G. Guillian;J. Learned;S. Matsuno;M. Messier;Y. Hayato;A. Ichikawa;T. Ishida;T. Ishii;T. Iwashita;T. Kobayashi;T. Nakadaira;K. Nakamura;K. Nitta;Y. Oyama;Y. Totsuka;A. Suzuki;M. Hasegawa;K. Hiraide;I. Kato;H. Maesaka;T. Nakaya;K. Nishikawa;T. Sasaki;H. Sato;S. Yamamoto;M. Yokoyama;T. Haines;S. Dazeley;S. Hatakeyama;R. Svoboda;G. Sullivan;D. Turcan;M. Swanson;A. Clough;A. Habig;Y. Fukuda;T. Sato;Y. Itow;T. Koike;C. 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. Kim;B. 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. Kiełczewska;J. Zalipska;H. Berns;R. Gran;K. Shiraishi;A. Stachyra;E. Thrane;K. Washburn;R. Wilkes
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;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. Raaf;J. Stone;L. Sulak;W. Wang;M. Goldhaber;D. Casper;J. P. Cravens;J. Dunmore;W. Kropp;D. Liu;S. Mine;C. Regis;M. Smy;H. Sobel;M. Vagins;K. Ganezer;J. Hill;W. Keig;J. Jang;J. Kim;I. Lim;K. Scholberg;N. Tanimoto;C. Walter;R. Wendell;R. Ellsworth;S. Tasaka;G. Guillian;J. Learned;S. Matsuno;M. Messier;Y. Hayato;A. Ichikawa;T. Ishida;T. Ishii;T. Iwashita;T. Kobayashi;T. Nakadaira;K. Nakamura;K. Nitta;Y. Oyama;Y. Totsuka;A. Suzuki;M. Hasegawa;K. Hiraide;I. Kato;H. Maesaka;T. Nakaya;K. Nishikawa;T. Sasaki;H. Sato;S. Yamamoto;M. Yokoyama;T. Haines;S. Dazeley;S. Hatakeyama;R. Svoboda;G. Sullivan;D. Turcan;M. Swanson;A. Clough;A. Habig;Y. Fukuda;T. Sato;Y. Itow;T. Koike;C. 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. Kim;B. 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. Kiełczewska;J. Zalipska;H. Berns;R. Gran;K. Shiraishi;A. Stachyra;E. Thrane;K. Washburn;R. Wilkes
中科院分区：
其他
文献类型：
--
作者：
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;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. Raaf;J. Stone;L. Sulak;W. Wang;M. Goldhaber;D. Casper;J. P. Cravens;J. Dunmore;W. Kropp;D. Liu;S. Mine;C. Regis;M. Smy;H. Sobel;M. Vagins;K. Ganezer;J. Hill;W. Keig;J. Jang;J. Kim;I. Lim;K. Scholberg;N. Tanimoto;C. Walter;R. Wendell;R. Ellsworth;S. Tasaka;G. Guillian;J. Learned;S. Matsuno;M. Messier;Y. Hayato;A. Ichikawa;T. Ishida;T. Ishii;T. Iwashita;T. Kobayashi;T. Nakadaira;K. Nakamura;K. Nitta;Y. Oyama;Y. Totsuka;A. Suzuki;M. Hasegawa;K. Hiraide;I. Kato;H. Maesaka;T. Nakaya;K. Nishikawa;T. Sasaki;H. Sato;S. Yamamoto;M. Yokoyama;T. Haines;S. Dazeley;S. Hatakeyama;R. Svoboda;G. Sullivan;D. Turcan;M. Swanson;A. Clough;A. Habig;Y. Fukuda;T. Sato;Y. Itow;T. Koike;C. 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. Kim;B. 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. Kiełczewska;J. Zalipska;H. Berns;R. Gran;K. Shiraishi;A. Stachyra;E. Thrane;K. Washburn;R. Wilkes

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我们展示了利用 Super-Kamiokande I（1996 年 4 月-2001 年 7 月）中微子引起的上行 μ 子数据寻找高能中微子天体物理来源的几项研究的结果。该数据集由 2359 个最小能量为 1.6 GeV 的事件组成，其中 1892 个在探测器内通过，467 个在探测器内停止。提出了几个独立分析的结果，包括使用方向和时间信息搜索点源，以及搜索宇宙射线与向上运动的μ子中的星际介质相互作用的特征。没有发现点源或来自银河系平面的任何漫射通量的统计显着证据，因此计算了可能的点源通量的具体限制。位于南半球且始终位于超级神冈地平线以下的天文源的向上 μ 介子通量的 90% 置信度 (CL) 上限约为 × 10-15 cm-2 s-1。
We present the results from several studies used to search for astrophysical sources of high-energy neutrinos using the Super-Kamiokande I (1996 April-2001 July) neutrino-induced upward-going muon data. The data set consists of 2359 events with minimum energy 1.6 GeV, of which 1892 are through-going and 467 stop within the detector. The results of several independent analyses are presented, including searches for point sources using directional and temporal information and a search for signatures of cosmic-ray interactions with the interstellar medium in the upward-going muons. No statistically significant evidence for point sources or any diffuse flux from the plane of the Galaxy was found, so specific limits on fluxes from likely point sources are calculated. The 90% confidence level (CL) upper limits on upward-going muon flux from astronomical sources that are located in the southern hemisphere and always under the horizon for Super-Kamiokande are ~ × 10-15 cm-2 s-1.