Search for Supernova Relic Neutrinos at Super-Kamiokande

M. Malek; M. Morii; S. Fukuda; Y. Fukuda; M. Ishitsuka; Y. Itow; T. Kajita; J. Kameda; K. Kaneyuki; K. Kobayashi; Y. Koshio; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; T. Namba; A. Okada; T. Ooyabu; C. Saji; N. Sakurai; M. Shiozawa; Y. Suzuki; H. Takeuchi; Y. Takeuchi; Y. Totsuka; S. Yamada; S. Desai; M. Earl; E. Kearns; M. D. Messier; J. L. Stone; L. R. Sulak; C. W. Walter; M. Goldhaber; T. Barszczak; D. Casper; W. Gajewski; W. R. Kropp; S. Mine; D. W. Liu; M. B. Smy; H. W. Sobel; M. R. Vagins; A. Gago; K. S. Ganezer; W. E. Keig; R. W. Ellsworth; S. Tasaka; A. Kibayashi; J. G. Learned; S. Matsuno; D. Takemori; Y. Hayato; T. Ishii; T. Kobayashi; T. Maruyama; K. Nakamura; Y. Obayashi; Y. Oyama; M. Sakuda; M. Yoshida; M. Kohama; T. Iwashita; A. T. Suzuki; A. Ichikawa; T. Inagaki; I. Kato; T. Nakaya; K. Nishikawa; T. J. Haines; S. Dazeley; S. Hatakeyama; R. Svoboda; E. Blaufuss; J. A. Goodman; G. Guillian; G. W. Sullivan; D. Turcan; K. Scholberg; A. Habig; M. Ackermann; J. Hill; C. K. Jung; K. Martens; C. Mauger; C. McGrew; E. Sharkey; B. Viren; C. Yanagisawa; T. Toshito; C. Mitsuda; K. Miyano; T. Shibata; Y. Kajiyama; Y. Nagashima; K. Nitta; M. Takita; H. I. Kim; S. B. Kim; J. Yoo; H. Okazawa; T. Ishizuka; M. Etoh; Y. Gando; T. Hasegawa; K. Inoue; K. Ishihara; J. Shirai; A. Suzuki; M. Koshiba; Y. Hatakeyama; Y. Ichikawa; M. Koike; K. Nishijima; H. Ishino; R. Nishimura; Y. Watanabe; D. Kielczewska; H. G. Berns; S. C. Boyd; A. L. Stachyra; R. J. Wilkes

doi:10.1103/PhysRevLett.90.061101

Search for Supernova Relic Neutrinos at Super-Kamiokande

M. Malek
, M. Morii
, S. Fukuda
, Y. Fukuda
, M. Ishitsuka
, Y. Itow
, T. Kajita
, J. Kameda
, K. Kaneyuki
, K. Kobayashi
, Y. Koshio
, M. Miura
, S. Moriyama
, M. Nakahata
, S. Nakayama
, T. Namba
, A. Okada
, T. Ooyabu
, C. Saji
, N. Sakurai

M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, Y. Totsuka, S. Yamada, S. Desai, M. Earl, E. Kearns, M. D. Messier, J. L. Stone, L. R. Sulak, C. W. Walter, M. Goldhaber, T. Barszczak, D. Casper, W. Gajewski, W. R. Kropp, S. Mine, D. W. Liu, M. B. Smy, H. W. Sobel, M. R. Vagins, A. Gago, K. S. Ganezer, W. E. Keig, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, T. Ishii, T. Kobayashi, T. Maruyama, K. Nakamura, Y. Obayashi, Y. Oyama, M. Sakuda, M. Yoshida, M. Kohama, T. Iwashita, A. T. Suzuki, A. Ichikawa, T. Inagaki, I. Kato, T. Nakaya, K. Nishikawa, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, E. Blaufuss, J. A. Goodman, G. Guillian, G. W. Sullivan, D. Turcan, K. Scholberg, A. Habig, M. Ackermann, J. Hill, C. K. Jung, K. Martens, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, T. Toshito, C. Mitsuda, K. Miyano, T. Shibata, Y. Kajiyama, Y. Nagashima, K. Nitta, M. Takita, H. I. Kim, S. B. Kim, J. Yoo, H. Okazawa, T. Ishizuka, M. Etoh, Y. Gando, T. Hasegawa, K. Inoue, K. Ishihara, J. Shirai, A. Suzuki, M. Koshiba, Y. Hatakeyama, Y. Ichikawa, M. Koike, K. Nishijima, H. Ishino, R. Nishimura, Y. Watanabe, D. Kielczewska, H. G. Berns, S. C. Boyd, A. L. Stachyra, R. J. Wilkes

Physics & Astronomy (Duluth)

Research output: Contribution to journal › Article › peer-review

202 Scopus citations

Abstract

A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to [Formula presented]. Additionally, an upper bound of [Formula presented] was set for the supernova relic neutrino flux in the energy region [Formula presented].

Original language	English (US)
Article number	061101
Pages (from-to)	061101/1-061101/5
Number of pages	1
Journal	Physical Review Letters
Volume	90
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevLett.90.061101
State	Published - 2003

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10.1103/PhysRevLett.90.061101

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Malek, M., Morii, M., Fukuda, S., Fukuda, Y., Ishitsuka, M., Itow, Y., Kajita, T., Kameda, J., Kaneyuki, K., Kobayashi, K., Koshio, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Namba, T., Okada, A., Ooyabu, T., Saji, C., ... Wilkes, R. J. (2003). Search for Supernova Relic Neutrinos at Super-Kamiokande. Physical Review Letters, 90(6), 061101/1-061101/5. Article 061101. https://doi.org/10.1103/PhysRevLett.90.061101

Malek, M, Morii, M, Fukuda, S, Fukuda, Y, Ishitsuka, M, Itow, Y, Kajita, T, Kameda, J, Kaneyuki, K, Kobayashi, K, Koshio, Y, Miura, M, Moriyama, S, Nakahata, M, Nakayama, S, Namba, T, Okada, A, Ooyabu, T, Saji, C, Sakurai, N, Shiozawa, M, Suzuki, Y, Takeuchi, H, Takeuchi, Y, Totsuka, Y, Yamada, S, Desai, S, Earl, M, Kearns, E, Messier, MD, Stone, JL, Sulak, LR, Walter, CW, Goldhaber, M, Barszczak, T, Casper, D, Gajewski, W, Kropp, WR, Mine, S, Liu, DW, Smy, MB, Sobel, HW, Vagins, MR, Gago, A, Ganezer, KS, Keig, WE, Ellsworth, RW, Tasaka, S, Kibayashi, A, Learned, JG, Matsuno, S, Takemori, D, Hayato, Y, Ishii, T, Kobayashi, T, Maruyama, T, Nakamura, K, Obayashi, Y, Oyama, Y, Sakuda, M, Yoshida, M, Kohama, M, Iwashita, T, Suzuki, AT, Ichikawa, A, Inagaki, T, Kato, I, Nakaya, T, Nishikawa, K, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Blaufuss, E, Goodman, JA, Guillian, G, Sullivan, GW, Turcan, D, Scholberg, K, Habig, A, Ackermann, M, Hill, J, Jung, CK, Martens, K, Mauger, C, McGrew, C, Sharkey, E, Viren, B, Yanagisawa, C, Toshito, T, Mitsuda, C, Miyano, K, Shibata, T, Kajiyama, Y, Nagashima, Y, Nitta, K, Takita, M, Kim, HI, Kim, SB, Yoo, J, Okazawa, H, Ishizuka, T, Etoh, M, Gando, Y, Hasegawa, T, Inoue, K, Ishihara, K, Shirai, J, Suzuki, A, Koshiba, M, Hatakeyama, Y, Ichikawa, Y, Koike, M, Nishijima, K, Ishino, H, Nishimura, R, Watanabe, Y, Kielczewska, D, Berns, HG, Boyd, SC, Stachyra, AL & Wilkes, RJ 2003, 'Search for Supernova Relic Neutrinos at Super-Kamiokande', Physical Review Letters, vol. 90, no. 6, 061101, pp. 061101/1-061101/5. https://doi.org/10.1103/PhysRevLett.90.061101

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title = "Search for Supernova Relic Neutrinos at Super-Kamiokande",

abstract = "A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90\% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to [Formula presented]. Additionally, an upper bound of [Formula presented] was set for the supernova relic neutrino flux in the energy region [Formula presented].",

author = "M. Malek and M. Morii and S. Fukuda and Y. Fukuda and M. Ishitsuka and Y. Itow and T. Kajita and J. Kameda and K. Kaneyuki and K. Kobayashi and Y. Koshio and M. Miura and S. Moriyama and M. Nakahata and S. Nakayama and T. Namba and A. Okada and T. Ooyabu and C. Saji and N. Sakurai and M. Shiozawa and Y. Suzuki and H. Takeuchi and Y. Takeuchi and Y. Totsuka and S. Yamada and S. Desai and M. Earl and E. Kearns and Messier, \{M. D.\} and Stone, \{J. L.\} and Sulak, \{L. R.\} and Walter, \{C. W.\} and M. Goldhaber and T. Barszczak and D. Casper and W. Gajewski and Kropp, \{W. R.\} and S. Mine and Liu, \{D. W.\} and Smy, \{M. B.\} and Sobel, \{H. W.\} and Vagins, \{M. R.\} and A. Gago and Ganezer, \{K. S.\} and Keig, \{W. E.\} and Ellsworth, \{R. W.\} and S. Tasaka and A. Kibayashi and Learned, \{J. G.\} and S. Matsuno and D. Takemori and Y. Hayato and T. Ishii and T. Kobayashi and T. Maruyama and K. Nakamura and Y. Obayashi and Y. Oyama and M. Sakuda and M. Yoshida and M. Kohama and T. Iwashita and Suzuki, \{A. T.\} and A. Ichikawa and T. Inagaki and I. Kato and T. Nakaya and K. Nishikawa and Haines, \{T. J.\} and S. Dazeley and S. Hatakeyama and R. Svoboda and E. Blaufuss and Goodman, \{J. A.\} and G. Guillian and Sullivan, \{G. W.\} and D. Turcan and K. Scholberg and A. Habig and M. Ackermann and J. Hill and Jung, \{C. K.\} and K. Martens and C. Mauger and C. McGrew and E. Sharkey and B. Viren and C. Yanagisawa and T. Toshito and C. Mitsuda and K. Miyano and T. Shibata and Y. Kajiyama and Y. Nagashima and K. Nitta and M. Takita and Kim, \{H. I.\} and Kim, \{S. B.\} and J. Yoo and H. Okazawa and T. Ishizuka and M. Etoh and Y. Gando and T. Hasegawa and K. Inoue and K. Ishihara and J. Shirai and A. Suzuki and M. Koshiba and Y. Hatakeyama and Y. Ichikawa and M. Koike and K. Nishijima and H. Ishino and R. Nishimura and Y. Watanabe and D. Kielczewska and Berns, \{H. G.\} and Boyd, \{S. C.\} and Stachyra, \{A. L.\} and Wilkes, \{R. J.\}",

year = "2003",

doi = "10.1103/PhysRevLett.90.061101",

language = "English (US)",

volume = "90",

pages = "061101/1--061101/5",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "6",

}

TY - JOUR

T1 - Search for Supernova Relic Neutrinos at Super-Kamiokande

AU - Malek, M.

AU - Morii, M.

AU - Fukuda, S.

AU - Fukuda, Y.

AU - Ishitsuka, M.

AU - Itow, Y.

AU - Kajita, T.

AU - Kameda, J.

AU - Kaneyuki, K.

AU - Kobayashi, K.

AU - Koshio, Y.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakayama, S.

AU - Namba, T.

AU - Okada, A.

AU - Ooyabu, T.

AU - Saji, C.

AU - Sakurai, N.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeuchi, H.

AU - Takeuchi, Y.

AU - Totsuka, Y.

AU - Yamada, S.

AU - Desai, S.

AU - Earl, M.

AU - Kearns, E.

AU - Messier, M. D.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Walter, C. W.

AU - Goldhaber, M.

AU - Barszczak, T.

AU - Casper, D.

AU - Gajewski, W.

AU - Kropp, W. R.

AU - Mine, S.

AU - Liu, D. W.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Vagins, M. R.

AU - Gago, A.

AU - Ganezer, K. S.

AU - Keig, W. E.

AU - Ellsworth, R. W.

AU - Tasaka, S.

AU - Kibayashi, A.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Takemori, D.

AU - Hayato, Y.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Maruyama, T.

AU - Nakamura, K.

AU - Obayashi, Y.

AU - Oyama, Y.

AU - Sakuda, M.

AU - Yoshida, M.

AU - Kohama, M.

AU - Iwashita, T.

AU - Suzuki, A. T.

AU - Ichikawa, A.

AU - Inagaki, T.

AU - Kato, I.

AU - Nakaya, T.

AU - Nishikawa, K.

AU - Haines, T. J.

AU - Dazeley, S.

AU - Hatakeyama, S.

AU - Svoboda, R.

AU - Blaufuss, E.

AU - Goodman, J. A.

AU - Guillian, G.

AU - Sullivan, G. W.

AU - Turcan, D.

AU - Scholberg, K.

AU - Habig, A.

AU - Ackermann, M.

AU - Hill, J.

AU - Jung, C. K.

AU - Martens, K.

AU - Mauger, C.

AU - McGrew, C.

AU - Sharkey, E.

AU - Viren, B.

AU - Yanagisawa, C.

AU - Toshito, T.

AU - Mitsuda, C.

AU - Miyano, K.

AU - Shibata, T.

AU - Kajiyama, Y.

AU - Nagashima, Y.

AU - Nitta, K.

AU - Takita, M.

AU - Kim, H. I.

AU - Kim, S. B.

AU - Yoo, J.

AU - Okazawa, H.

AU - Ishizuka, T.

AU - Etoh, M.

AU - Gando, Y.

AU - Hasegawa, T.

AU - Inoue, K.

AU - Ishihara, K.

AU - Shirai, J.

AU - Suzuki, A.

AU - Koshiba, M.

AU - Hatakeyama, Y.

AU - Ichikawa, Y.

AU - Koike, M.

AU - Nishijima, K.

AU - Ishino, H.

AU - Nishimura, R.

AU - Watanabe, Y.

AU - Kielczewska, D.

AU - Berns, H. G.

AU - Boyd, S. C.

AU - Stachyra, A. L.

AU - Wilkes, R. J.

PY - 2003

Y1 - 2003

N2 - A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to [Formula presented]. Additionally, an upper bound of [Formula presented] was set for the supernova relic neutrino flux in the energy region [Formula presented].

AB - A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than 18 MeV. In the absence of a signal, 90% C.L. upper limits on the total flux were set for several theoretical models; these limits ranged from 20 to [Formula presented]. Additionally, an upper bound of [Formula presented] was set for the supernova relic neutrino flux in the energy region [Formula presented].

UR - https://www.scopus.com/pages/publications/0037435905

UR - https://www.scopus.com/pages/publications/0037435905#tab=citedBy

U2 - 10.1103/PhysRevLett.90.061101

DO - 10.1103/PhysRevLett.90.061101

M3 - Article

AN - SCOPUS:0037435905

SN - 0031-9007

VL - 90

SP - 061101/1-061101/5

JO - Physical Review Letters

JF - Physical Review Letters

IS - 6

M1 - 061101

ER -

Search for Supernova Relic Neutrinos at Super-Kamiokande

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