Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

K. Abe; C. Bronner; Y. Hayato; M. Ikeda; K. Iyogi; J. Kameda; Y. Kato; Y. Kishimoto; Ll Marti; M. Miura; S. Moriyama; M. Nakahata; Y. Nakajima; Y. Nakano; S. Nakayama; A. Orii; G. Pronost; H. Sekiya; M. Shiozawa; Y. Sonoda; A. Takeda; A. Takenaka; H. Tanaka; S. Tasaka; T. Yano; R. Akutsu; T. Kajita; Y. Nishimura; K. Okumura; K. M. Tsui; L. Labarga; P. Fernandez; F. D.M. Blaszczyk; C. Kachulis; E. Kearns; J. L. Raaf; J. L. Stone; L. R. Sulak; S. Berkman; S. Tobayama; J. Bian; M. Elnimr; W. R. Kropp; S. Locke; S. Mine; P. Weatherly; M. B. Smy; H. W. Sobel; V. Takhistov; K. S. Ganezer; J. Hill; J. Y. Kim; I. T. Lim; R. G. Park; Z. Li; E. O'Sullivan; K. Scholberg; C. W. Walter; M. Gonin; J. Imber; Th A. Mueller; T. Ishizuka; T. Nakamura; J. S. Jang; K. Choi; J. G. Learned; S. Matsuno; J. Amey; R. P. Litchfield; W. Y. Ma; Y. Uchida; M. O. Wascko; M. G. Catanesi; R. A. Intonti; E. Radicioni; G. De Rosa; A. Ali; G. Collazuol; L. Ludovici; S. Cao; M. Friend; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; K. E. Abe; M. Hasegawa; A. T. Suzuki; Y. Takeuchi; T. Hayashino; S. Hirota; M. Jiang; M. Mori; K. E. Nakamura; T. Nakaya; R. A. Wendell; L. H.V. Anthony; N. McCauley; A. Pritchard; Y. Fukuda; Y. Itow; M. Murase; F. Muto; P. Mijakowski; K. Frankiewicz; C. K. Jung; X. Li; J. L. Palomino; G. Santucci; C. Viela; M. J. Wilking; C. Yanagisawa; D. Fukuda; H. Ishino; S. Ito; A. Kibayashi; Y. Koshio; H. Nagata; M. Sakuda; C. Xu; Y. Kuno; D. Wark; F. Di Lodovico; B. Richards; S. Molina Sedgwick; R. Tacik; S. B. Kim; A. Cole; L. Thompson; H. Okazawa; Y. Choi; K. Ito; K. Nishijima; M. Koshiba; Y. Suda; M. Yokoyama; R. G. Calland; M. Hartz; K. Martens; M. Murdoch; B. Quilain; C. Simpson; Y. Suzuki; M. R. Vagins; D. Hamabe; M. Kuze; Y. Okajima; T. Yoshida; M. Ishitsuka; J. F. Martin; C. M. Nantais; H. A. Tanaka; T. Towstego; A. Konaka; S. Chen; L. Wan; A. Minamino

doi:10.3847/2041-8213/aabaca

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

K. Abe
, C. Bronner
, Y. Hayato
, M. Ikeda
, K. Iyogi
, J. Kameda
, Y. Kato
, Y. Kishimoto
, Ll Marti
, M. Miura
, S. Moriyama
, M. Nakahata
, Y. Nakajima
, Y. Nakano
, S. Nakayama
, A. Orii
, G. Pronost
, H. Sekiya
, M. Shiozawa
, Y. Sonoda

A. Takeda, A. Takenaka, H. Tanaka, S. Tasaka, T. Yano, R. Akutsu, T. Kajita, Y. Nishimura, K. Okumura, K. M. Tsui, L. Labarga, P. Fernandez, F. D.M. Blaszczyk, C. Kachulis, E. Kearns, J. L. Raaf, J. L. Stone, L. R. Sulak, S. Berkman, S. Tobayama, J. Bian, M. Elnimr, W. R. Kropp, S. Locke, S. Mine, P. Weatherly, M. B. Smy, H. W. Sobel, V. Takhistov, K. S. Ganezer, J. Hill, J. Y. Kim, I. T. Lim, R. G. Park, Z. Li, E. O'Sullivan, K. Scholberg, C. W. Walter, M. Gonin, J. Imber, Th A. Mueller, T. Ishizuka, T. Nakamura, J. S. Jang, K. Choi, J. G. Learned, S. Matsuno, J. Amey, R. P. Litchfield, W. Y. Ma, Y. Uchida, M. O. Wascko, M. G. Catanesi, R. A. Intonti, E. Radicioni, G. De Rosa, A. Ali, G. Collazuol, L. Ludovici, S. Cao, M. Friend, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, K. E. Abe, M. Hasegawa, A. T. Suzuki, Y. Takeuchi, T. Hayashino, S. Hirota, M. Jiang, M. Mori, K. E. Nakamura, T. Nakaya, R. A. Wendell, L. H.V. Anthony, N. McCauley, A. Pritchard, Y. Fukuda, Y. Itow, M. Murase, F. Muto, P. Mijakowski, K. Frankiewicz, C. K. Jung, X. Li, J. L. Palomino, G. Santucci, C. Viela, M. J. Wilking, C. Yanagisawa, D. Fukuda, H. Ishino, S. Ito, A. Kibayashi, Y. Koshio, H. Nagata, M. Sakuda, C. Xu, Y. Kuno, D. Wark, F. Di Lodovico, B. Richards, S. Molina Sedgwick, R. Tacik, S. B. Kim, A. Cole, L. Thompson, H. Okazawa, Y. Choi, K. Ito, K. Nishijima, M. Koshiba, Y. Suda, M. Yokoyama, R. G. Calland, M. Hartz, K. Martens, M. Murdoch, B. Quilain, C. Simpson, Y. Suzuki, M. R. Vagins, D. Hamabe, M. Kuze, Y. Okajima, T. Yoshida, M. Ishitsuka, J. F. Martin, C. M. Nantais, H. A. Tanaka, T. Towstego, A. Konaka, S. Chen, L. Wan, A. Minamino

Physics and Astronomy

The University of Tokyo
STFC Rutherford Appleton Laboratory
Universidad Autónoma de Madrid
Boston University
University of British Columbia
University of California at Irvine
California State University Dominguez Hills
Chonnam National University
Duke University
Laboratoire Leprince-Ringuet
Fukuoka Institute of Technology
Gifu University
Gwangju Institute of Science and Technology
University of Hawai'i at Mānoa
Imperial College London
National Institute for Nuclear Physics
University of Rome La Sapienza
High Energy Accelerator Research Organization, Tsukuba
Kobe University
Kyoto University
University of Liverpool
Miyagi University of Education
Nagoya University
National Centre for Nuclear Research
Stony Brook University
Okayama University
The University of Osaka
University of Oxford
Queen Mary University of London
University of Regina
TRIUMF
Seoul National University
University of Sheffield
Shizuoka University of Welfare
Sungkyunkwan University
Tokai University
Institute of Science Tokyo
Tokyo University of Science
University of Toronto
Tsinghua University
Yokohama National University
University of California at Los Angeles
City University of New York

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

42 Scopus citations

Abstract

We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ∼100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is () cm^-2 for muon neutrinos (muon antineutrinos), with an error range of ±5around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of-2. The fluence limit for neutrino energies less than 100 MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6 × 10⁷ cm^-2 for anti-electron neutrinos under the assumption of a Fermi-Dirac spectrum with average energy of 20 MeV.

Original language	English
Article number	L4
Journal	Astrophysical Journal Letters
Volume	857
Issue number	1
DOIs	https://doi.org/10.3847/2041-8213/aabaca
State	Published - Apr 10 2018

Keywords

astroparticle physics
gravitational waves
neutrinos

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10.3847/2041-8213/aabaca

Cite this

Abe, K., Bronner, C., Hayato, Y., Ikeda, M., Iyogi, K., Kameda, J., Kato, Y., Kishimoto, Y., Marti, L., Miura, M., Moriyama, S., Nakahata, M., Nakajima, Y., Nakano, Y., Nakayama, S., Orii, A., Pronost, G., Sekiya, H., Shiozawa, M., ... Minamino, A. (2018). Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger. Astrophysical Journal Letters, 857(1), Article L4. https://doi.org/10.3847/2041-8213/aabaca

@article{9e69ceff67e14317a2faf60eff37db1b,

title = "Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger",

abstract = "We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ∼100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90\% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is () cm-2 for muon neutrinos (muon antineutrinos), with an error range of ±5around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of-2. The fluence limit for neutrino energies less than 100 MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6 × 107 cm-2 for anti-electron neutrinos under the assumption of a Fermi-Dirac spectrum with average energy of 20 MeV.",

keywords = "astroparticle physics, gravitational waves, neutrinos",

author = "K. Abe and C. Bronner and Y. Hayato and M. Ikeda and K. Iyogi and J. Kameda and Y. Kato and Y. Kishimoto and Ll Marti and M. Miura and S. Moriyama and M. Nakahata and Y. Nakajima and Y. Nakano and S. Nakayama and A. Orii and G. Pronost and H. Sekiya and M. Shiozawa and Y. Sonoda and A. Takeda and A. Takenaka and H. Tanaka and S. Tasaka and T. Yano and R. Akutsu and T. Kajita and Y. Nishimura and K. Okumura and Tsui, \{K. M.\} and L. Labarga and P. Fernandez and Blaszczyk, \{F. D.M.\} and C. Kachulis and E. Kearns and Raaf, \{J. L.\} and Stone, \{J. L.\} and Sulak, \{L. R.\} and S. Berkman and S. Tobayama and J. Bian and M. Elnimr and Kropp, \{W. R.\} and S. Locke and S. Mine and P. Weatherly and Smy, \{M. B.\} and Sobel, \{H. W.\} and V. Takhistov and Ganezer, \{K. S.\} and J. Hill and Kim, \{J. Y.\} and Lim, \{I. T.\} and Park, \{R. G.\} and Z. Li and E. O'Sullivan and K. Scholberg and Walter, \{C. W.\} and M. Gonin and J. Imber and Mueller, \{Th A.\} and T. Ishizuka and T. Nakamura and Jang, \{J. S.\} and K. Choi and Learned, \{J. G.\} and S. Matsuno and J. Amey and Litchfield, \{R. P.\} and Ma, \{W. Y.\} and Y. Uchida and Wascko, \{M. O.\} and Catanesi, \{M. G.\} and Intonti, \{R. A.\} and E. Radicioni and Rosa, \{G. De\} and A. Ali and G. Collazuol and L. Ludovici and S. Cao and M. Friend and T. Hasegawa and T. Ishida and T. Ishii and T. Kobayashi and T. Nakadaira and K. Nakamura and Y. Oyama and K. Sakashita and T. Sekiguchi and T. Tsukamoto and Abe, \{K. E.\} and M. Hasegawa and Suzuki, \{A. T.\} and Y. Takeuchi and T. Hayashino and S. Hirota and M. Jiang and M. Mori and Nakamura, \{K. E.\} and T. Nakaya and Wendell, \{R. A.\} and Anthony, \{L. H.V.\} and N. McCauley and A. Pritchard and Y. Fukuda and Y. Itow and M. Murase and F. Muto and P. Mijakowski and K. Frankiewicz and Jung, \{C. K.\} and X. Li and Palomino, \{J. L.\} and G. Santucci and C. Viela and Wilking, \{M. J.\} and C. Yanagisawa and D. Fukuda and H. Ishino and S. Ito and A. Kibayashi and Y. Koshio and H. Nagata and M. Sakuda and C. Xu and Y. Kuno and D. Wark and Lodovico, \{F. Di\} and B. Richards and Sedgwick, \{S. Molina\} and R. Tacik and Kim, \{S. B.\} and A. Cole and L. Thompson and H. Okazawa and Y. Choi and K. Ito and K. Nishijima and M. Koshiba and Y. Suda and M. Yokoyama and Calland, \{R. G.\} and M. Hartz and K. Martens and M. Murdoch and B. Quilain and C. Simpson and Y. Suzuki and Vagins, \{M. R.\} and D. Hamabe and M. Kuze and Y. Okajima and T. Yoshida and M. Ishitsuka and Martin, \{J. F.\} and Nantais, \{C. M.\} and Tanaka, \{H. A.\} and T. Towstego and A. Konaka and S. Chen and L. Wan and A. Minamino",

year = "2018",

month = apr,

day = "10",

doi = "10.3847/2041-8213/aabaca",

language = "English",

volume = "857",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

number = "1",

}

Abe, K, Bronner, C, Hayato, Y, Ikeda, M, Iyogi, K, Kameda, J, Kato, Y, Kishimoto, Y, Marti, L, Miura, M, Moriyama, S, Nakahata, M, Nakajima, Y, Nakano, Y, Nakayama, S, Orii, A, Pronost, G, Sekiya, H, Shiozawa, M, Sonoda, Y, Takeda, A, Takenaka, A, Tanaka, H, Tasaka, S, Yano, T, Akutsu, R, Kajita, T, Nishimura, Y, Okumura, K, Tsui, KM, Labarga, L, Fernandez, P, Blaszczyk, FDM, Kachulis, C, Kearns, E, Raaf, JL, Stone, JL, Sulak, LR, Berkman, S, Tobayama, S, Bian, J, Elnimr, M, Kropp, WR, Locke, S, Mine, S, Weatherly, P, Smy, MB, Sobel, HW, Takhistov, V, Ganezer, KS, Hill, J, Kim, JY, Lim, IT, Park, RG, Li, Z, O'Sullivan, E, Scholberg, K, Walter, CW, Gonin, M, Imber, J, Mueller, TA, Ishizuka, T, Nakamura, T, Jang, JS, Choi, K, Learned, JG, Matsuno, S, Amey, J, Litchfield, RP, Ma, WY, Uchida, Y, Wascko, MO, Catanesi, MG, Intonti, RA, Radicioni, E, Rosa, GD, Ali, A, Collazuol, G, Ludovici, L, Cao, S, Friend, M, Hasegawa, T, Ishida, T, Ishii, T, Kobayashi, T, Nakadaira, T, Nakamura, K, Oyama, Y, Sakashita, K, Sekiguchi, T, Tsukamoto, T, Abe, KE, Hasegawa, M, Suzuki, AT, Takeuchi, Y, Hayashino, T, Hirota, S, Jiang, M, Mori, M, Nakamura, KE, Nakaya, T, Wendell, RA, Anthony, LHV, McCauley, N, Pritchard, A, Fukuda, Y, Itow, Y, Murase, M, Muto, F, Mijakowski, P, Frankiewicz, K, Jung, CK, Li, X, Palomino, JL, Santucci, G, Viela, C, Wilking, MJ, Yanagisawa, C, Fukuda, D, Ishino, H, Ito, S, Kibayashi, A, Koshio, Y, Nagata, H, Sakuda, M, Xu, C, Kuno, Y, Wark, D, Lodovico, FD, Richards, B, Sedgwick, SM, Tacik, R, Kim, SB, Cole, A, Thompson, L, Okazawa, H, Choi, Y, Ito, K, Nishijima, K, Koshiba, M, Suda, Y, Yokoyama, M, Calland, RG, Hartz, M, Martens, K, Murdoch, M, Quilain, B, Simpson, C, Suzuki, Y, Vagins, MR, Hamabe, D, Kuze, M, Okajima, Y, Yoshida, T, Ishitsuka, M, Martin, JF, Nantais, CM, Tanaka, HA, Towstego, T, Konaka, A, Chen, S, Wan, L & Minamino, A 2018, 'Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger', Astrophysical Journal Letters, vol. 857, no. 1, L4. https://doi.org/10.3847/2041-8213/aabaca

TY - JOUR

T1 - Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

AU - Abe, K.

AU - Bronner, C.

AU - Hayato, Y.

AU - Ikeda, M.

AU - Iyogi, K.

AU - Kameda, J.

AU - Kato, Y.

AU - Kishimoto, Y.

AU - Marti, Ll

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakajima, Y.

AU - Nakano, Y.

AU - Nakayama, S.

AU - Orii, A.

AU - Pronost, G.

AU - Sekiya, H.

AU - Shiozawa, M.

AU - Sonoda, Y.

AU - Takeda, A.

AU - Takenaka, A.

AU - Tanaka, H.

AU - Tasaka, S.

AU - Yano, T.

AU - Akutsu, R.

AU - Kajita, T.

AU - Nishimura, Y.

AU - Okumura, K.

AU - Tsui, K. M.

AU - Labarga, L.

AU - Fernandez, P.

AU - Blaszczyk, F. D.M.

AU - Kachulis, C.

AU - Kearns, E.

AU - Raaf, J. L.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Berkman, S.

AU - Tobayama, S.

AU - Bian, J.

AU - Elnimr, M.

AU - Kropp, W. R.

AU - Locke, S.

AU - Mine, S.

AU - Weatherly, P.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Takhistov, V.

AU - Ganezer, K. S.

AU - Hill, J.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Park, R. G.

AU - Li, Z.

AU - O'Sullivan, E.

AU - Scholberg, K.

AU - Walter, C. W.

AU - Gonin, M.

AU - Imber, J.

AU - Mueller, Th A.

AU - Ishizuka, T.

AU - Nakamura, T.

AU - Jang, J. S.

AU - Choi, K.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Amey, J.

AU - Litchfield, R. P.

AU - Ma, W. Y.

AU - Uchida, Y.

AU - Wascko, M. O.

AU - Catanesi, M. G.

AU - Intonti, R. A.

AU - Radicioni, E.

AU - Rosa, G. De

AU - Ali, A.

AU - Collazuol, G.

AU - Ludovici, L.

AU - Cao, S.

AU - Friend, M.

AU - Hasegawa, T.

AU - Ishida, T.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Nakadaira, T.

AU - Nakamura, K.

AU - Oyama, Y.

AU - Sakashita, K.

AU - Sekiguchi, T.

AU - Tsukamoto, T.

AU - Abe, K. E.

AU - Hasegawa, M.

AU - Suzuki, A. T.

AU - Takeuchi, Y.

AU - Hayashino, T.

AU - Hirota, S.

AU - Jiang, M.

AU - Mori, M.

AU - Nakamura, K. E.

AU - Nakaya, T.

AU - Wendell, R. A.

AU - Anthony, L. H.V.

AU - McCauley, N.

AU - Pritchard, A.

AU - Fukuda, Y.

AU - Itow, Y.

AU - Murase, M.

AU - Muto, F.

AU - Mijakowski, P.

AU - Frankiewicz, K.

AU - Jung, C. K.

AU - Li, X.

AU - Palomino, J. L.

AU - Santucci, G.

AU - Viela, C.

AU - Wilking, M. J.

AU - Yanagisawa, C.

AU - Fukuda, D.

AU - Ishino, H.

AU - Ito, S.

AU - Kibayashi, A.

AU - Koshio, Y.

AU - Nagata, H.

AU - Sakuda, M.

AU - Xu, C.

AU - Kuno, Y.

AU - Wark, D.

AU - Lodovico, F. Di

AU - Richards, B.

AU - Sedgwick, S. Molina

AU - Tacik, R.

AU - Kim, S. B.

AU - Cole, A.

AU - Thompson, L.

AU - Okazawa, H.

AU - Choi, Y.

AU - Ito, K.

AU - Nishijima, K.

AU - Koshiba, M.

AU - Suda, Y.

AU - Yokoyama, M.

AU - Calland, R. G.

AU - Hartz, M.

AU - Martens, K.

AU - Murdoch, M.

AU - Quilain, B.

AU - Simpson, C.

AU - Suzuki, Y.

AU - Vagins, M. R.

AU - Hamabe, D.

AU - Kuze, M.

AU - Okajima, Y.

AU - Yoshida, T.

AU - Ishitsuka, M.

AU - Martin, J. F.

AU - Nantais, C. M.

AU - Tanaka, H. A.

AU - Towstego, T.

AU - Konaka, A.

AU - Chen, S.

AU - Wan, L.

AU - Minamino, A.

PY - 2018/4/10

Y1 - 2018/4/10

N2 - We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ∼100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is () cm-2 for muon neutrinos (muon antineutrinos), with an error range of ±5around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of-2. The fluence limit for neutrino energies less than 100 MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6 × 107 cm-2 for anti-electron neutrinos under the assumption of a Fermi-Dirac spectrum with average energy of 20 MeV.

AB - We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ∼100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is () cm-2 for muon neutrinos (muon antineutrinos), with an error range of ±5around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of-2. The fluence limit for neutrino energies less than 100 MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6 × 107 cm-2 for anti-electron neutrinos under the assumption of a Fermi-Dirac spectrum with average energy of 20 MeV.

KW - astroparticle physics

KW - gravitational waves

KW - neutrinos

UR - https://www.scopus.com/pages/publications/85045853820

U2 - 10.3847/2041-8213/aabaca

DO - 10.3847/2041-8213/aabaca

M3 - Article

AN - SCOPUS:85045853820

SN - 2041-8205

VL - 857

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 1

M1 - L4

ER -

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

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