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A search for solar axion induced signals with COSINE-100

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dc.contributor.authorAdhikari, P.-
dc.contributor.authorAdhikari, G.-
dc.contributor.authorBarbosa de Souza, E.-
dc.contributor.authorCarlin, N.-
dc.contributor.authorChoi, S.-
dc.contributor.authorDjamal, M.-
dc.contributor.authorEzeribe, A.C.-
dc.contributor.authorHa, C.-
dc.contributor.authorHahn, I.S.-
dc.contributor.authorJeon, E.J.-
dc.contributor.authorJo, J.H.-
dc.contributor.authorJoo, H.W.-
dc.contributor.authorKang, W.G.-
dc.contributor.authorKang, W.-
dc.contributor.authorKauer, M.-
dc.contributor.authorKim, G.S.-
dc.contributor.authorKim, H.-
dc.contributor.authorKim, H.J.-
dc.contributor.authorKim, K.W.-
dc.contributor.authorKim, N.Y.-
dc.contributor.authorKim, S.K.-
dc.contributor.authorKim, Y.D.-
dc.contributor.authorKim, Y.H.-
dc.contributor.authorKo, Y.J.-
dc.contributor.authorKudryavtsev, V.A.-
dc.contributor.authorLee, H.S.-
dc.contributor.authorLee, J.-
dc.contributor.authorLee, J.Y.-
dc.contributor.authorLee, M.H.-
dc.contributor.authorLeonard, D.S.-
dc.contributor.authorLynch, W.A.-
dc.contributor.authorMaruyama, R.H.-
dc.contributor.authorMouton, F.-
dc.contributor.authorOlsen, S.L.-
dc.contributor.authorPark, B.J.-
dc.contributor.authorPark, H.K.-
dc.contributor.authorPark, H.S.-
dc.contributor.authorPark, K.S.-
dc.contributor.authorPitta, R.L.C.-
dc.contributor.authorPrihtiadi, H.-
dc.contributor.authorRa, S.-
dc.contributor.authorRott, C.-
dc.contributor.authorShin, K.A.-
dc.contributor.authorScarff, A.-
dc.contributor.authorSpooner, N.J.C.-
dc.contributor.authorThompson, W.G.-
dc.contributor.authorYang, L.-
dc.contributor.authorYu, G.H.-
dc.date.accessioned2023-03-08T14:08:09Z-
dc.date.available2023-03-08T14:08:09Z-
dc.date.issued2020-01-
dc.identifier.issn0927-6505-
dc.identifier.issn1873-2852-
dc.identifier.urihttps://scholarworks.bwise.kr/cau/handle/2019.sw.cau/63452-
dc.description.abstractWe present results from a search for solar axions with the COSINE-100 experiment. We find no evidence of solar axion events from a data-set of 6,303.9 kg . days exposure and set a 90% confidence level upper limit on the axion-electron coupling, g(ae), of 1.70 x 10(-11) for an axion mass less than 1 keV/c(2). This limit excludes QCD axions heavier than 0.59 eV/c(2) in the DFSZ model and 1681 eV/c(2) in the KSVZ model. (C) 2019 Elsevier B.V. All rights reserved.-
dc.format.extent6-
dc.language영어-
dc.language.isoENG-
dc.publisherELSEVIER-
dc.titleA search for solar axion induced signals with COSINE-100-
dc.typeArticle-
dc.identifier.doi10.1016/j.astropartphys.2019.07.004-
dc.identifier.bibliographicCitationASTROPARTICLE PHYSICS, v.114, pp 101 - 106-
dc.description.isOpenAccessN-
dc.identifier.wosid000489353300012-
dc.identifier.scopusid2-s2.0-85069473427-
dc.citation.endPage106-
dc.citation.startPage101-
dc.citation.titleASTROPARTICLE PHYSICS-
dc.citation.volume114-
dc.type.docTypeArticle-
dc.publisher.location네델란드-
dc.subject.keywordAuthorSolar axion-
dc.subject.keywordAuthorCOSINE-100-
dc.subject.keywordAuthorDark matter-
dc.subject.keywordPlusINVARIANCE-
dc.subject.keywordPlusMECHANISM-
dc.subject.keywordPlusTESTS-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
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