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

Stony Brook University
Institute of Science Tokyo
Tokyo University
Boston University
Brookhaven National Laboratory
University of California at Irvine
California State University Dominguez Hills
George Mason University
Gifu University
University of Hawaii
High Energy Accelerator Research Organization (KEK)
Kobe University
Kyoto University
Physics Division
Louisiana State University
University of Maryland
Massachusetts Institute of Technology
University of Minnesota Duluth
Nagoya University
Niigata University
Osaka University
Seoul National University
International and Cultural Studies
Shizuoka University
Tohoku University
Tokai University
University of Warsaw
University of Washington

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

20 Citas (Scopus)

Resumen

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].

Idioma original	Inglés
Páginas (desde-hasta)	5
Número de páginas	1
Publicación	Physical Review Letters
Volumen	90
N.º	6
DOI	https://doi.org/10.1103/PhysRevLett.90.061101
Estado	Publicada - 2003
Publicado de forma externa	Sí

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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), 5. https://doi.org/10.1103/PhysRevLett.90.061101

@article{4be620ee2c7d43feb6b67a9ba4d15795,

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",

volume = "90",

pages = "5",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "6",

}

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, n.º 6, pp. 5. https://doi.org/10.1103/PhysRevLett.90.061101

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/85038266945

U2 - 10.1103/PhysRevLett.90.061101

DO - 10.1103/PhysRevLett.90.061101

M3 - Article

AN - SCOPUS:85038266945

SN - 0031-9007

VL - 90

SP - 5

JO - Physical Review Letters

JF - Physical Review Letters

IS - 6

ER -

Search for Supernova Relic Neutrinos at Super-Kamiokande

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