A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts

S. Abe; S. Asami; A. Gando; Y. Gando; T. Gima; A. Goto; T. Hachiya; K. Hata; K. Hosokawa; K. Ichimura; S. Ieki; H. Ikeda; K. Inoue; K. Ishidoshiro; Y. Kamei; N. Kawada; Y. Kishimoto; T. Kinoshita; M. Koga; N. Maemura; T. Mitsui; H. Miyake; K. Nakamura; Kengo Nakamura; R. Nakamura; H. Ozaki; T. Sakai; H. Sambonsugi; I. Shimizu; J. Shirai; K. Shiraishi; A. Suzuki; Y. Suzuki; A. Takeuchi; K. Tamae; M. Eizuka; M. Kurasawa; T. Nakahata; S. Futagi; H. Watanabe; Y. Yoshida; S. Obara; A. K. Ichikawa; S. Yoshida; S. Umehara; K. Fushimi; B. E. Berger; B. K. Fujikawa; J. G. Learned; J. Maricic; S. N. Axani; J. Smolsky; C. Laber-Smith; L. A. Winslow; Z. Fu; J. Ouellet; Y. Efremenko; H. J. Karwowski; D. M. Markoff; W. Tornow; A. Li; J. A. Detwiler; S. Enomoto; M. P. Decowski; C. Grant; H. Song; T. O'Donnell; S. Dell'Oro

doi:10.3847/1538-4357/ac4e7e

A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts

S. Abe, S. Asami, A. Gando, Y. Gando, T. Gima, A. Goto, T. Hachiya, K. Hata, K. Hosokawa, K. Ichimura, S. Ieki, H. Ikeda, K. Inoue, K. Ishidoshiro, Y. Kamei, N. Kawada, Y. Kishimoto, T. Kinoshita, M. Koga, N. MaemuraT. Mitsui, H. Miyake, K. Nakamura, Kengo Nakamura, R. Nakamura, H. Ozaki, T. Sakai, H. Sambonsugi, I. Shimizu, J. Shirai, K. Shiraishi, A. Suzuki, Y. Suzuki, A. Takeuchi, K. Tamae, M. Eizuka, M. Kurasawa, T. Nakahata, S. Futagi, H. Watanabe, Y. Yoshida, S. Obara, A. K. Ichikawa, S. Yoshida, S. Umehara, K. Fushimi, B. E. Berger, B. K. Fujikawa, J. G. Learned, J. Maricic, S. N. Axani, J. Smolsky, C. Laber-Smith, L. A. Winslow, Z. Fu, J. Ouellet, Y. Efremenko, H. J. Karwowski, D. M. Markoff, W. Tornow, A. Li, J. A. Detwiler, S. Enomoto, M. P. Decowski, C. Grant, H. Song, T. O'Donnell, S. Dell'Oro

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Abstract

We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts (GRBs) from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of ±500 s plus the duration of each GRB, no statistically significant excess above the background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the GRB source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.

Original language	English
Article number	69
Journal	Astrophysical Journal
Volume	927
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ac4e7e
Publication status	Published - 2022 Mar 1

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ac4e7e

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Abe, S., Asami, S., Gando, A., Gando, Y., Gima, T., Goto, A., Hachiya, T., Hata, K., Hosokawa, K., Ichimura, K., Ieki, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Kamei, Y., Kawada, N., Kishimoto, Y., Kinoshita, T., Koga, M., ... Dell'Oro, S. (2022). A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts. Astrophysical Journal, 927(1), [69]. https://doi.org/10.3847/1538-4357/ac4e7e

Abe, S, Asami, S, Gando, A, Gando, Y, Gima, T, Goto, A, Hachiya, T, Hata, K, Hosokawa, K, Ichimura, K , Ieki, S , Ikeda, H , Inoue, K , Ishidoshiro, K, Kamei, Y, Kawada, N, Kishimoto, Y, Kinoshita, T, Koga, M, Maemura, N, Mitsui, T, Miyake, H, Nakamura, K, Nakamura, K, Nakamura, R, Ozaki, H, Sakai, T, Sambonsugi, H, Shimizu, I, Shirai, J, Shiraishi, K, Suzuki, A, Suzuki, Y, Takeuchi, A, Tamae, K, Eizuka, M, Kurasawa, M, Nakahata, T, Futagi, S, Watanabe, H, Yoshida, Y, Obara, S, Ichikawa, AK, Yoshida, S, Umehara, S, Fushimi, K, Berger, BE, Fujikawa, BK, Learned, JG, Maricic, J, Axani, SN, Smolsky, J, Laber-Smith, C, Winslow, LA, Fu, Z, Ouellet, J, Efremenko, Y, Karwowski, HJ, Markoff, DM, Tornow, W, Li, A, Detwiler, JA, Enomoto, S, Decowski, MP, Grant, C, Song, H, O'Donnell, T & Dell'Oro, S 2022, 'A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts', Astrophysical Journal, vol. 927, no. 1, 69. https://doi.org/10.3847/1538-4357/ac4e7e

@article{89e9016ce2b34192b2eddaa5dbf39049,

title = "A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts",

abstract = "We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts (GRBs) from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of ±500 s plus the duration of each GRB, no statistically significant excess above the background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the GRB source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.",

author = "S. Abe and S. Asami and A. Gando and Y. Gando and T. Gima and A. Goto and T. Hachiya and K. Hata and K. Hosokawa and K. Ichimura and S. Ieki and H. Ikeda and K. Inoue and K. Ishidoshiro and Y. Kamei and N. Kawada and Y. Kishimoto and T. Kinoshita and M. Koga and N. Maemura and T. Mitsui and H. Miyake and K. Nakamura and Kengo Nakamura and R. Nakamura and H. Ozaki and T. Sakai and H. Sambonsugi and I. Shimizu and J. Shirai and K. Shiraishi and A. Suzuki and Y. Suzuki and A. Takeuchi and K. Tamae and M. Eizuka and M. Kurasawa and T. Nakahata and S. Futagi and H. Watanabe and Y. Yoshida and S. Obara and Ichikawa, {A. K.} and S. Yoshida and S. Umehara and K. Fushimi and Berger, {B. E.} and Fujikawa, {B. K.} and Learned, {J. G.} and J. Maricic and Axani, {S. N.} and J. Smolsky and C. Laber-Smith and Winslow, {L. A.} and Z. Fu and J. Ouellet and Y. Efremenko and Karwowski, {H. J.} and Markoff, {D. M.} and W. Tornow and A. Li and Detwiler, {J. A.} and S. Enomoto and Decowski, {M. P.} and C. Grant and H. Song and T. O'Donnell and S. Dell'Oro",

note = "Funding Information: The KamLAND experiment is supported by JSPS KAKENHI grant 19H05803; the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan; Netherlands Organization for Scientific Research (NWO); and under the US Department of Energy (DOE) contract No. DE-AC02-05CH11231, National Science Foundation (NSF) Nos. NSF-1806440, and NSF-2012964, the Heising‒Simons Foundation, as well as other DOE and NSF grants to individual institutions. The Kamioka Mining and Smelting Company has provided services for activities in the mine. We acknowledge the support of NII for SINET4. Publisher Copyright: {\textcopyright} 2022. The Author(s). Published by the American Astronomical Society.",

year = "2022",

month = mar,

day = "1",

doi = "10.3847/1538-4357/ac4e7e",

language = "English",

volume = "927",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "1",

}

TY - JOUR

T1 - A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts

AU - Abe, S.

AU - Asami, S.

AU - Gando, A.

AU - Gando, Y.

AU - Gima, T.

AU - Goto, A.

AU - Hachiya, T.

AU - Hata, K.

AU - Hosokawa, K.

AU - Ichimura, K.

AU - Ieki, S.

AU - Ikeda, H.

AU - Inoue, K.

AU - Ishidoshiro, K.

AU - Kamei, Y.

AU - Kawada, N.

AU - Kishimoto, Y.

AU - Kinoshita, T.

AU - Koga, M.

AU - Maemura, N.

AU - Mitsui, T.

AU - Miyake, H.

AU - Nakamura, K.

AU - Nakamura, Kengo

AU - Nakamura, R.

AU - Ozaki, H.

AU - Sakai, T.

AU - Sambonsugi, H.

AU - Shimizu, I.

AU - Shirai, J.

AU - Shiraishi, K.

AU - Suzuki, A.

AU - Suzuki, Y.

AU - Takeuchi, A.

AU - Tamae, K.

AU - Eizuka, M.

AU - Kurasawa, M.

AU - Nakahata, T.

AU - Futagi, S.

AU - Watanabe, H.

AU - Yoshida, Y.

AU - Obara, S.

AU - Ichikawa, A. K.

AU - Yoshida, S.

AU - Umehara, S.

AU - Fushimi, K.

AU - Berger, B. E.

AU - Fujikawa, B. K.

AU - Learned, J. G.

AU - Maricic, J.

AU - Axani, S. N.

AU - Smolsky, J.

AU - Laber-Smith, C.

AU - Winslow, L. A.

AU - Fu, Z.

AU - Ouellet, J.

AU - Efremenko, Y.

AU - Karwowski, H. J.

AU - Markoff, D. M.

AU - Tornow, W.

AU - Li, A.

AU - Detwiler, J. A.

AU - Enomoto, S.

AU - Decowski, M. P.

AU - Grant, C.

AU - Song, H.

AU - O'Donnell, T.

AU - Dell'Oro, S.

N1 - Funding Information: The KamLAND experiment is supported by JSPS KAKENHI grant 19H05803; the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan; Netherlands Organization for Scientific Research (NWO); and under the US Department of Energy (DOE) contract No. DE-AC02-05CH11231, National Science Foundation (NSF) Nos. NSF-1806440, and NSF-2012964, the Heising‒Simons Foundation, as well as other DOE and NSF grants to individual institutions. The Kamioka Mining and Smelting Company has provided services for activities in the mine. We acknowledge the support of NII for SINET4. Publisher Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

PY - 2022/3/1

Y1 - 2022/3/1

N2 - We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts (GRBs) from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of ±500 s plus the duration of each GRB, no statistically significant excess above the background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the GRB source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.

AB - We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts (GRBs) from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of ±500 s plus the duration of each GRB, no statistically significant excess above the background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the GRB source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.

UR - http://www.scopus.com/inward/record.url?scp=85126716194&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85126716194&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ac4e7e

DO - 10.3847/1538-4357/ac4e7e

M3 - Article

AN - SCOPUS:85126716194

SN - 0004-637X

VL - 927

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 69

ER -

A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts

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