Search for supernova neutrino bursts at super-kamiokande

M. Ikeda; A. Takeda; Y. Fukuda; M. R. Vagins; K. Abe; T. Iida; K. Ishihara; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; Y. Obayashi; H. Ogawa; H. Sekiya; M. Shiozawa; Y. Suzuki; Y. Takeuchi; K. Ueshima; H. Watanabe; S. Yamada; I. Higuchi; C. Ishihara; M. Ishitsuka; T. Kajita; K. Kaneyuki; G. Mitsuka; S. Nakayama; H. Nishino; 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; K. S. Ganezer; J. 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; H. Maesaka; T. Nakaya; K. Nishikawa; T. Sasaki; S. Yamamoto; M. Yokoyama; T. J. Haines; S. Dazeley; S. Hatakeyama; R. Svoboda; G. W. Sullivan; D. Turcan; A. Habig; T. Sato; Y. Itow; T. Koike; T. Tanaka; C. K. Jung; T. Kato; K. Kobayashi; M. Malek; C. Mcgrew; A. Sarrat; R. Terri; C. Yanagisawa; N. Tamura; Y. Idehara; 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; Y. Furuse; H. Ishii; K. Nishijima; H. Ishino; Y. Watanabe; M. Koshiba; S. Chen; Z. Deng; Y. Liu; D. Kielczewska; J. Zalipska; H. Berns; R. Gran; K. K. Shiraishi; A. Stachyra; E. Thrane; K. Washburn; R. J. Wilkes

doi:10.1086/521547

Search for supernova neutrino bursts at super-kamiokande

M. Ikeda
, A. Takeda
, Y. Fukuda
, M. R. Vagins
, K. Abe
, T. Iida
, K. Ishihara
, J. Kameda
, Y. Koshio
, A. Minamino
, C. Mitsuda
, M. Miura
, S. Moriyama
, M. Nakahata
, Y. Obayashi
, H. Ogawa
, H. Sekiya
, M. Shiozawa
, Y. Suzuki
, Y. Takeuchi

K. Ueshima, H. Watanabe, S. Yamada, I. Higuchi, C. Ishihara, M. Ishitsuka, T. Kajita, K. Kaneyuki, G. Mitsuka, S. Nakayama, H. Nishino, 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, K. S. Ganezer, J. 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, H. Maesaka, T. Nakaya, K. Nishikawa, T. Sasaki, S. Yamamoto, M. Yokoyama, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, G. W. Sullivan, D. Turcan, A. Habig, T. Sato, Y. Itow, T. Koike, T. Tanaka, C. K. Jung, T. Kato, K. Kobayashi, M. Malek, C. Mcgrew, A. Sarrat, R. Terri, C. Yanagisawa, N. Tamura, Y. Idehara, 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, Y. Furuse, H. Ishii, K. Nishijima, H. Ishino, Y. Watanabe, M. Koshiba, S. Chen, Z. Deng, Y. Liu, D. Kielczewska, J. Zalipska, H. Berns, R. Gran, K. K. Shiraishi, A. Stachyra, E. Thrane, K. Washburn, R. J. Wilkes

Physics and Astronomy

Okayama University
The University of Tokyo
Miyagi University of Education
University of California at Irvine
Boston University
Pennsylvania State University
Brookhaven National Laboratory
California State University Dominguez Hills
Chonnam National University
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High Energy Accelerator Research Organization, Tsukuba
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Los Alamos National Laboratory
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University of Maryland, College Park
University of Minnesota Duluth
Nagoya University
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Seoul National University
Shizuoka University
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Tohoku University
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University of Warsaw
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Research output: Contribution to journal › Article › peer-review

148 Scopus citations

Abstract

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% CL. 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.

Original language	English
Pages (from-to)	519-524
Number of pages	6
Journal	Astrophysical Journal
Volume	669
Issue number	1
DOIs	https://doi.org/10.1086/521547
State	Published - Nov 1 2007

Keywords

Galaxies: individual (Milky Way, LMC, SMC)
Neutrinos
Supernovae: general

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10.1086/521547

Cite this

Ikeda, M., Takeda, A., Fukuda, Y., Vagins, M. R., Abe, K., Iida, T., Ishihara, K., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Obayashi, Y., Ogawa, H., Sekiya, H., Shiozawa, M., Suzuki, Y., ... Wilkes, R. J. (2007). Search for supernova neutrino bursts at super-kamiokande. Astrophysical Journal, 669(1), 519-524. https://doi.org/10.1086/521547

@article{7e7b656295cc454293ad8accd59ad211,

title = "Search for supernova neutrino bursts at super-kamiokande",

abstract = "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\% CL. 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.",

keywords = "Galaxies: individual (Milky Way, LMC, SMC), Neutrinos, Supernovae: general",

author = "M. Ikeda and A. Takeda and Y. Fukuda and Vagins, \{M. R.\} and K. Abe 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 H. Sekiya and M. Shiozawa and Y. Suzuki and Y. Takeuchi and K. Ueshima and H. Watanabe and S. Yamada 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 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 Ganezer, \{K. S.\} and J. Hill 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 H. Maesaka and T. Nakaya and K. Nishikawa and T. Sasaki 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 A. Habig and T. Sato and Y. Itow and T. Koike and T. Tanaka 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 Y. Idehara 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 Y. Furuse and H. Ishii and K. Nishijima and H. Ishino and Y. Watanabe and M. Koshiba and S. Chen and Z. Deng and Y. Liu and D. Kielczewska and J. Zalipska and H. Berns and R. Gran and Shiraishi, \{K. K.\} and A. Stachyra and E. Thrane and K. Washburn and Wilkes, \{R. J.\}",

year = "2007",

month = nov,

day = "1",

doi = "10.1086/521547",

language = "English",

volume = "669",

pages = "519--524",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "1",

}

Ikeda, M, Takeda, A, Fukuda, Y, Vagins, MR, Abe, K, Iida, T, Ishihara, K, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Obayashi, Y, Ogawa, H, Sekiya, H, Shiozawa, M, Suzuki, Y, Takeuchi, Y, Ueshima, K, Watanabe, H, Yamada, S, Higuchi, I, Ishihara, C, Ishitsuka, M, Kajita, T, Kaneyuki, K, Mitsuka, G, Nakayama, S, Nishino, H, 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, Ganezer, KS, Hill, J, 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, Maesaka, H, Nakaya, T, Nishikawa, K, Sasaki, T, Yamamoto, S, Yokoyama, M, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Sullivan, GW, Turcan, D, Habig, A, Sato, T, Itow, Y, Koike, T, Tanaka, T, Jung, CK, Kato, T, Kobayashi, K, Malek, M, Mcgrew, C, Sarrat, A, Terri, R, Yanagisawa, C, Tamura, N, Idehara, Y, 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, Furuse, Y, Ishii, H, Nishijima, K, Ishino, H, Watanabe, Y, Koshiba, M, Chen, S, Deng, Z, Liu, Y, Kielczewska, D, Zalipska, J, Berns, H, Gran, R, Shiraishi, KK, Stachyra, A, Thrane, E, Washburn, K & Wilkes, RJ 2007, 'Search for supernova neutrino bursts at super-kamiokande', Astrophysical Journal, vol. 669, no. 1, pp. 519-524. https://doi.org/10.1086/521547

TY - JOUR

T1 - Search for supernova neutrino bursts at super-kamiokande

AU - Ikeda, M.

AU - Takeda, A.

AU - Fukuda, Y.

AU - Vagins, M. R.

AU - Abe, K.

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 - Sekiya, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeuchi, Y.

AU - Ueshima, K.

AU - Watanabe, H.

AU - Yamada, S.

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 - 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 - Ganezer, K. S.

AU - Hill, J.

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 - Maesaka, H.

AU - Nakaya, T.

AU - Nishikawa, K.

AU - Sasaki, T.

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 - Habig, A.

AU - Sato, T.

AU - Itow, Y.

AU - Koike, T.

AU - Tanaka, 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 - Idehara, Y.

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 - Furuse, Y.

AU - Ishii, H.

AU - Nishijima, K.

AU - Ishino, H.

AU - Watanabe, Y.

AU - Koshiba, M.

AU - Chen, S.

AU - Deng, Z.

AU - Liu, Y.

AU - Kielczewska, D.

AU - Zalipska, J.

AU - Berns, H.

AU - Gran, R.

AU - Shiraishi, K. K.

AU - Stachyra, A.

AU - Thrane, E.

AU - Washburn, K.

AU - Wilkes, R. J.

PY - 2007/11/1

Y1 - 2007/11/1

N2 - 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% CL. 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.

AB - 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% CL. 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.

KW - Galaxies: individual (Milky Way, LMC, SMC)

KW - Neutrinos

KW - Supernovae: general

UR - https://www.scopus.com/pages/publications/39049152843

U2 - 10.1086/521547

DO - 10.1086/521547

M3 - Article

AN - SCOPUS:39049152843

SN - 0004-637X

VL - 669

SP - 519

EP - 524

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

ER -

Search for supernova neutrino bursts at super-kamiokande

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