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dc.contributor.authorAxani, Spencer Nicholas
dc.contributor.authorWinslow, Lindley
dc.contributor.authorFu, Z.
dc.contributor.authorOuellet, J.
dc.date.accessioned2022-05-05T14:09:32Z
dc.date.available2022-05-05T14:09:32Z
dc.date.issued2022-01-01
dc.identifier.urihttps://hdl.handle.net/1721.1/142353
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>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 × 10<jats:sup>7</jats:sup> cm<jats:sup>−2</jats:sup> (3.0 × 10<jats:sup>9</jats:sup> cm<jats:sup>−2</jats:sup>) 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.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/1538-4357/ac35d1en_US
dc.rightsCreative Commons Attribution 4.0 International Licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleSearch for Solar Flare Neutrinos with the KamLAND Detectoren_US
dc.typeArticleen_US
dc.identifier.citationWinslow, Lindley. 2022. "Search for Solar Flare Neutrinos with the KamLAND Detector." The Astrophysical Journal, 924 (2).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-05-05T14:05:01Z
dspace.orderedauthorsAbe, 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, Sen_US
dspace.date.submission2022-05-05T14:05:02Z
mit.journal.volume924en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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