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Lowering threshold of NaI(Tl) scintillator to 0.7 keV in the COSINE-100 experiment

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dc.contributor.authorG.H. Yu-
dc.contributor.authorCarlin, N.-
dc.contributor.authorJ.Y. Cho-
dc.contributor.authorJ.J. Choi-
dc.contributor.authorChoi, S.-
dc.contributor.authorEzeribe, A.C.-
dc.contributor.authorFranca, L.E.-
dc.contributor.authorHa, C.-
dc.contributor.authorI.S. Hahn-
dc.contributor.authorHollick, S.J.-
dc.contributor.authorE.J. Jeon-
dc.contributor.authorJoo, H.W.-
dc.contributor.authorW.G. Kang-
dc.contributor.authorKauer, M.-
dc.contributor.authorB.H. Kim-
dc.contributor.authorKim, H.J.-
dc.contributor.authorKim, J.-
dc.contributor.authorK.W. Kim-
dc.contributor.authorS.H. Kim-
dc.contributor.authorKim, S.K.-
dc.contributor.authorW.K. Kim-
dc.contributor.authorY.D. Kim-
dc.contributor.authorY.H. Kim-
dc.contributor.authorY.J. Ko-
dc.contributor.authorLee, D.H.-
dc.contributor.authorE.K. Lee-
dc.contributor.authorH. Lee-
dc.contributor.authorH.S. Lee-
dc.contributor.authorH.Y. Lee-
dc.contributor.authorI.S. Lee-
dc.contributor.authorJ. Lee-
dc.contributor.authorLee, J.Y.-
dc.contributor.authorM.H. Lee-
dc.contributor.authorS.H. Lee-
dc.contributor.authorLee, S.M.-
dc.contributor.authorLee, Y.J.-
dc.contributor.authorD.S. Leonard-
dc.contributor.authorLuan, N.T.-
dc.contributor.authorMachado, V.H.A.-
dc.contributor.authorManzato, B.B.-
dc.contributor.authorMaruyama, R.H.-
dc.contributor.authorNeal, R.J.-
dc.contributor.authorS.L. Olsen-
dc.contributor.authorB.J. Park-
dc.contributor.authorPark, H.K.-
dc.contributor.authorPark, H.S.-
dc.contributor.authorPark, J.C.-
dc.contributor.authorK.S. Park-
dc.contributor.authorPark, S.D.-
dc.contributor.authorPitta, R.L.C.-
dc.contributor.authorPrihtiadi, H.-
dc.contributor.authorS.J. Ra-
dc.contributor.authorRott, C.-
dc.contributor.authorK.A. Shin-
dc.contributor.authorCavalcante, D.F.F.S.-
dc.contributor.authorSon, M.K.-
dc.contributor.authorSpooner, N.J.C.-
dc.contributor.authorTruc, L.T.-
dc.contributor.authorYang, L.-
dc.date.accessioned2025-01-14T05:00:32Z-
dc.date.available2025-01-14T05:00:32Z-
dc.date.created2024-12-23-
dc.date.issued2024-12-
dc.identifier.issn1748-0221-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/16160-
dc.description.abstractCOSINE-100 is a direct dark matter search experiment, with the primary goal of testing the annual modulation signal observed by DAMA/LIBRA, using the same target material, NaI(Tl). In previous analyses, we achieved the same 1 keV energy threshold used in the DAMA/LIBRA's analysis that reported an annual modulation signal with 11.6σ significance. In this article, we report an improved analysis that lowered the threshold to 0.7 keV, thanks to the application of Multi-Layer Perception network and a new likelihood parameter with waveforms in the frequency domain. The lower threshold would enable a better comparison of COSINE-100 with new DAMA results with a 0.75 keV threshold and account for differences in quenching factors. Furthermore the lower threshold can enhance COSINE-100's sensitivity to sub-GeV dark matter searches. © 2024 IOP Publishing Ltd and Sissa Medialab. All rights, including for text and data mining, AI training, and similar technologies, are reserved.-
dc.language영어-
dc.publisherInstitute of Physics-
dc.titleLowering threshold of NaI(Tl) scintillator to 0.7 keV in the COSINE-100 experiment-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.scopusid2-s2.0-85212120046-
dc.identifier.rimsid84759-
dc.contributor.affiliatedAuthorG.H. Yu-
dc.contributor.affiliatedAuthorJ.Y. Cho-
dc.contributor.affiliatedAuthorJ.J. Choi-
dc.contributor.affiliatedAuthorE.J. Jeon-
dc.contributor.affiliatedAuthorW.G. Kang-
dc.contributor.affiliatedAuthorB.H. Kim-
dc.contributor.affiliatedAuthorK.W. Kim-
dc.contributor.affiliatedAuthorS.H. Kim-
dc.contributor.affiliatedAuthorW.K. Kim-
dc.contributor.affiliatedAuthorY.D. Kim-
dc.contributor.affiliatedAuthorY.H. Kim-
dc.contributor.affiliatedAuthorY.J. Ko-
dc.contributor.affiliatedAuthorE.K. Lee-
dc.contributor.affiliatedAuthorH. Lee-
dc.contributor.affiliatedAuthorH.S. Lee-
dc.contributor.affiliatedAuthorH.Y. Lee-
dc.contributor.affiliatedAuthorI.S. Lee-
dc.contributor.affiliatedAuthorJ. Lee-
dc.contributor.affiliatedAuthorM.H. Lee-
dc.contributor.affiliatedAuthorS.H. Lee-
dc.contributor.affiliatedAuthorD.S. Leonard-
dc.contributor.affiliatedAuthorS.L. Olsen-
dc.contributor.affiliatedAuthorB.J. Park-
dc.contributor.affiliatedAuthorK.S. Park-
dc.contributor.affiliatedAuthorS.J. Ra-
dc.contributor.affiliatedAuthorK.A. Shin-
dc.identifier.doi10.1088/1748-0221/19/12/P12013-
dc.identifier.bibliographicCitationJournal of Instrumentation, v.19, no.12-
dc.relation.isPartOfJournal of Instrumentation-
dc.citation.titleJournal of Instrumentation-
dc.citation.volume19-
dc.citation.number12-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.subject.keywordAuthorDark Matter detectors (WIMPs, axions, etc.)-
dc.subject.keywordAuthorAnalysis and statistical methods-
dc.subject.keywordAuthorGamma detectors (scintillators, CZT, HPGe, HgI etc)-
dc.subject.keywordAuthorData reduction methods-
Appears in Collections:
Center for Underground Physics(지하실험 연구단) > 1. Journal Papers (저널논문)
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