Search for Supernova Neutrino Bursts at Super-Kamiokande
Search for Supernova Neutrino Bursts at Super-Kamiokande
复制标题
寻找超级神冈探测器的超新星中微子爆发
DOI：
10.1086/521547
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发表时间：
2007-06
期刊：
影响因子：
--
通讯作者：
中科院分区：
文献类型：
--
作者：
我们报告的结果搜索中微子爆发超新星爆炸使用超级神冈探测器。Super-Kamiokande通过观察中微子的排放对核心坍缩超新星爆炸很敏感。这样的爆发事件的预期数量约为104，中微子的平均能量在我们银河系典型距离（10 kpc）的核心坍缩超新星爆炸的几十MeV范围内;这个强信号意味着我们银河系内任何地方的探测效率都应该是100%。我们研究了从1996年5月至2001年7月，从2002年12月至2005年10月，对应于2589.2活天的数据集。然而，在数据采集期间没有这样的超新星爆炸的证据。90% C. L。在100千秒差距范围内，核心坍缩超新星爆炸速率的上限为0.32 SN yr-1。
We report the results of a search for neutrino bursts from supernova explosions using the Super-Kamiokande detector. Super-Kamiokande is sensitive to core-collapse supernova explosions via observation of their neutrino emissions. The expected number of events comprising such a burst is ~104, and the average energy of the neutrinos is in the range of a few tens of MeV for a core-collapse supernova explosion at a typical distance in our galaxy (10 kpc); this strong signal means that the detection efficiency anywhere within our galaxy and well past the Magellanic Clouds should be 100%. We examined a data set taken from 1996 May to 2001 July, and from 2002 December to 2005 October, corresponding to 2589.2 live days. However, there is no evidence of such a supernova explosion during the data-taking period. The 90% C.L. upper limit on the rate of core-collapse supernova explosions out to distances of 100 kpc is found to be 0.32 SN yr-1.
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DOI：
10.1016/s0920-5632(02)01489-5
发表时间：
2002-01
期刊：
--
影响因子：
--
作者：
G. Raffelt
通讯作者：
G. Raffelt
影响因子：
5
作者：
Keitaro Takahashi;Mariko Watanabe;Katsuhiko Sato;T. Totani
通讯作者：
Keitaro Takahashi;Mariko Watanabe;Katsuhiko Sato;T. Totani
影响因子：
8.6
作者：
HIRATA, K;KAJITA, T;CORTEZ, BG
通讯作者：
CORTEZ, BG
DOI：
10.1086/508016
发表时间：
2006-06
期刊：
The Astrophysical Journal
影响因子：
--
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
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
影响因子：
8.6
作者：
BIONTA, RM;BLEWITT, G;WUEST, C
通讯作者：
WUEST, C