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Search for Solar Flare Neutrinos with the KamLAND Detector

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dc.contributor.authorCollaboration, K.
dc.contributor.authorAbe, S.
dc.contributor.authorAsami, S.
dc.contributor.authorGando, A.
dc.contributor.authorKozlov, A.
dc.contributor.authorКозлов, Александр Анатольевич
dc.date.accessioned2024-12-26T08:20:31Z
dc.date.available2024-12-26T08:20:31Z
dc.date.issued2022
dc.description.abstract© 2022. The Author(s). Published by the American Astronomical Society.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.
dc.identifier.citationSearch for Solar Flare Neutrinos with the KamLAND Detector / Collaboration, K. [et al.] // Astrophysical Journal. - 2022. - 924. - № 2. - 10.3847/1538-4357/ac35d1
dc.identifier.doi10.3847/1538-4357/ac35d1
dc.identifier.urihttps://www.doi.org/10.3847/1538-4357/ac35d1
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85123899172&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000743309900001
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/28724
dc.relation.ispartofAstrophysical Journal
dc.titleSearch for Solar Flare Neutrinos with the KamLAND Detector
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue2
oaire.citation.volume924
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