Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

S. Abe; S. Asami; A. Gando; Y. Gando; T. Gima; A. Goto; T. Hachiya; K. Hata; S. Hayashida; 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; K. Ueshima; Y. Wada; H. Watanabe; Y. Yoshida; S. Obara; A. Kozlov; D. Chernyak; Y. Takemoto; S. Yoshida; S. Umehara; K. Fushimi; A. K. Ichikawa; K. Z. Nakamura; M. Yoshida; B. E. Berger; B. K. Fujikawa; J. G. Learned; J. Maricic; S. N. Axani; 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; T. O'Donnell; S. Dell'Oro

doi:10.3847/1538-4357/abd5bc

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

S. Abe, S. Asami, A. Gando, Y. Gando, T. Gima, A. Goto, T. Hachiya, K. Hata, S. Hayashida, K. Hosokawa, K. Ichimura, S. Ieki, H. Ikeda, K. Inoue, K. Ishidoshiro, Y. Kamei, N. Kawada, Y. Kishimoto, T. Kinoshita, M. KogaN. 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, K. Ueshima, Y. Wada, H. Watanabe, Y. Yoshida, S. Obara, A. Kozlov, D. Chernyak, Y. Takemoto, S. Yoshida, S. Umehara, K. Fushimi, A. K. Ichikawa, K. Z. Nakamura, M. Yoshida, B. E. Berger, B. K. Fujikawa, J. G. Learned, J. Maricic, S. N. Axani, 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, T. O'Donnell, S. Dell'Oro

研究成果: Article › 査読

7 被引用数 (Scopus)

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We present the results of a search for MeV-scale electron antineutrino events in KamLAND coincident with the 60 gravitational wave events/candidates reported by the LIGO/Virgo collaboration during their second and third observing runs. We find no significant coincident signals within a 500 s timing window from each gravitational wave and present 90% C.L. upper limits on the electron antineutrino fluence between 108 and 1013 cm-2 for neutrino energies in the energy range of 1.8-111 MeV.

本文言語	English
論文番号	116
ジャーナル	Astrophysical Journal
巻	909
号	2
DOI	https://doi.org/10.3847/1538-4357/abd5bc
出版ステータス	Published - 2021 3月 10

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.3847/1538-4357/abd5bc

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Abe, S., Asami, S., Gando, A., Gando, Y., Gima, T., Goto, A., Hachiya, T., Hata, K., Hayashida, S., Hosokawa, K., Ichimura, K., Ieki, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Kamei, Y., Kawada, N., Kishimoto, Y., Kinoshita, T., ... Dell'Oro, S. (2021). Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events. Astrophysical Journal, 909(2), [116]. https://doi.org/10.3847/1538-4357/abd5bc

Abe, S, Asami, S, Gando, A, Gando, Y, Gima, T, Goto, A, Hachiya, T, Hata, K, Hayashida, S, 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, Ueshima, K, Wada, Y, Watanabe, H, Yoshida, Y, Obara, S, Kozlov, A, Chernyak, D, Takemoto, Y, Yoshida, S, Umehara, S, Fushimi, K, Ichikawa, AK, Nakamura, KZ, Yoshida, M, Berger, BE, Fujikawa, BK, Learned, JG, Maricic, J, Axani, SN, Winslow, LA, Fu, Z, Ouellet, J, Efremenko, Y, Karwowski, HJ, Markoff, DM, Tornow, W, Li, A, Detwiler, JA, Enomoto, S, Decowski, MP, Grant, C, O'Donnell, T & Dell'Oro, S 2021, 'Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events', Astrophysical Journal, vol. 909, no. 2, 116. https://doi.org/10.3847/1538-4357/abd5bc

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abstract = "We present the results of a search for MeV-scale electron antineutrino events in KamLAND coincident with the 60 gravitational wave events/candidates reported by the LIGO/Virgo collaboration during their second and third observing runs. We find no significant coincident signals within a 500 s timing window from each gravitational wave and present 90% C.L. upper limits on the electron antineutrino fluence between 108 and 1013 cm-2 for neutrino energies in the energy range of 1.8-111 MeV.",

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 S. Hayashida 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 K. Ueshima and Y. Wada and H. Watanabe and Y. Yoshida and S. Obara and A. Kozlov and D. Chernyak and Y. Takemoto and S. Yoshida and S. Umehara and K. Fushimi and Ichikawa, {A. K.} and Nakamura, {K. Z.} and M. Yoshida and Berger, {B. E.} and Fujikawa, {B. K.} and Learned, {J. G.} and J. Maricic and Axani, {S. N.} 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 T. O'Donnell and S. Dell'Oro",

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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 - Hayashida, S.

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 - Ueshima, K.

AU - Wada, Y.

AU - Watanabe, H.

AU - Yoshida, Y.

AU - Obara, S.

AU - Kozlov, A.

AU - Chernyak, D.

AU - Takemoto, Y.

AU - Yoshida, S.

AU - Umehara, S.

AU - Fushimi, K.

AU - Ichikawa, A. K.

AU - Nakamura, K. Z.

AU - Yoshida, M.

AU - Berger, B. E.

AU - Fujikawa, B. K.

AU - Learned, J. G.

AU - Maricic, J.

AU - Axani, S. N.

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 - O'Donnell, T.

AU - Dell'Oro, S.

PY - 2021/3/10

Y1 - 2021/3/10

N2 - We present the results of a search for MeV-scale electron antineutrino events in KamLAND coincident with the 60 gravitational wave events/candidates reported by the LIGO/Virgo collaboration during their second and third observing runs. We find no significant coincident signals within a 500 s timing window from each gravitational wave and present 90% C.L. upper limits on the electron antineutrino fluence between 108 and 1013 cm-2 for neutrino energies in the energy range of 1.8-111 MeV.

AB - We present the results of a search for MeV-scale electron antineutrino events in KamLAND coincident with the 60 gravitational wave events/candidates reported by the LIGO/Virgo collaboration during their second and third observing runs. We find no significant coincident signals within a 500 s timing window from each gravitational wave and present 90% C.L. upper limits on the electron antineutrino fluence between 108 and 1013 cm-2 for neutrino energies in the energy range of 1.8-111 MeV.

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DO - 10.3847/1538-4357/abd5bc

M3 - Article

AN - SCOPUS:85103252980

VL - 909

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 116

ER -

Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events

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