Search for Solar Flare Neutrinos with the KamLAND Detector

Kamland Collaboration; 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. K. Ichikawa; A. Kozlov; D. Chernyak; Y. Takemoto; S. Yoshida; S. Umehara; K. Fushimi; 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/ac35d1

Search for Solar Flare Neutrinos with the KamLAND Detector

Kamland Collaboration, 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. KinoshitaM. 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. K. Ichikawa, A. Kozlov, D. Chernyak, Y. Takemoto, S. Yoshida, S. Umehara, K. Fushimi, 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

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Abstract

We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. This large exposure allows us to explore previously unconstrained parameter space for solar flare neutrinos. We found no statistical excess of neutrinos and established 90% confidence level upper limits of 8.4 × 107 cm-2 (3.0 × 109 cm-2) on the electron antineutrino (electron neutrino) fluence at 20 MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity.

Original language	English
Article number	103
Journal	Astrophysical Journal
Volume	924
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/ac35d1
Publication status	Published - 2022 Jan 10

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/ac35d1

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Collaboration, K., 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., ... Dell'Oro, S. (2022). Search for Solar Flare Neutrinos with the KamLAND Detector. Astrophysical Journal, 924(2), [103]. https://doi.org/10.3847/1538-4357/ac35d1

Collaboration, K, 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, Ichikawa, AK, Kozlov, A, Chernyak, D, Takemoto, Y, Yoshida, S, Umehara, S, Fushimi, K, 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 2022, 'Search for Solar Flare Neutrinos with the KamLAND Detector', Astrophysical Journal, vol. 924, no. 2, 103. https://doi.org/10.3847/1538-4357/ac35d1

@article{8786222c8562450d832ab83849e1ff67,

title = "Search for Solar Flare Neutrinos with the KamLAND Detector",

abstract = "We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. This large exposure allows us to explore previously unconstrained parameter space for solar flare neutrinos. We found no statistical excess of neutrinos and established 90% confidence level upper limits of 8.4 × 107 cm-2 (3.0 × 109 cm-2) on the electron antineutrino (electron neutrino) fluence at 20 MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity.",

author = "Kamland Collaboration and 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 Ichikawa, {A. K.} and A. Kozlov and D. Chernyak and Y. Takemoto and S. Yoshida and S. Umehara and K. Fushimi 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",

note = "Funding Information: Original content from this work may be used under the terms of the . Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. MEXT ∣ Japan Society for the Promotion of Science (JSPS) https://doi.org/10.13039/501100001691 19H05803 U.S. Department of Energy (DOE) https://doi.org/10.13039/100000015 DE-AC02-05CH11231 National Science Foundation (NSF) https://doi.org/10.13039/100000001 NSF-1806440 National Science Foundation (NSF) https://doi.org/10.13039/100000001 NSF-2012964 yes � 2022. The Author(s). Published by the American Astronomical Society. Creative Commons Attribution 4.0 licence Publisher Copyright: {\textcopyright} 2022. The Author(s). Published by the American Astronomical Society.",

year = "2022",

month = jan,

day = "10",

doi = "10.3847/1538-4357/ac35d1",

language = "English",

volume = "924",

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TY - JOUR

T1 - Search for Solar Flare Neutrinos with the KamLAND Detector

AU - Collaboration, Kamland

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 - Ichikawa, A. K.

AU - Kozlov, A.

AU - Chernyak, D.

AU - Takemoto, Y.

AU - Yoshida, S.

AU - Umehara, S.

AU - Fushimi, 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.

N1 - Funding Information: Original content from this work may be used under the terms of the . Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. MEXT ∣ Japan Society for the Promotion of Science (JSPS) https://doi.org/10.13039/501100001691 19H05803 U.S. Department of Energy (DOE) https://doi.org/10.13039/100000015 DE-AC02-05CH11231 National Science Foundation (NSF) https://doi.org/10.13039/100000001 NSF-1806440 National Science Foundation (NSF) https://doi.org/10.13039/100000001 NSF-2012964 yes � 2022. The Author(s). Published by the American Astronomical Society. Creative Commons Attribution 4.0 licence Publisher Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

PY - 2022/1/10

Y1 - 2022/1/10

N2 - We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. This large exposure allows us to explore previously unconstrained parameter space for solar flare neutrinos. We found no statistical excess of neutrinos and established 90% confidence level upper limits of 8.4 × 107 cm-2 (3.0 × 109 cm-2) on the electron antineutrino (electron neutrino) fluence at 20 MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity.

AB - We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. This large exposure allows us to explore previously unconstrained parameter space for solar flare neutrinos. We found no statistical excess of neutrinos and established 90% confidence level upper limits of 8.4 × 107 cm-2 (3.0 × 109 cm-2) on the electron antineutrino (electron neutrino) fluence at 20 MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity.

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UR - http://www.scopus.com/inward/citedby.url?scp=85123899172&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ac35d1

DO - 10.3847/1538-4357/ac35d1

M3 - Article

AN - SCOPUS:85123899172

SN - 0004-637X

VL - 924

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 103

ER -

Search for Solar Flare Neutrinos with the KamLAND Detector

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