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dc.contributor.author한인식*
dc.date.accessioned2019-08-22T16:30:12Z-
dc.date.available2019-08-22T16:30:12Z-
dc.date.issued2019*
dc.identifier.issn0031-9007*
dc.identifier.issn1079-7114*
dc.identifier.otherOAK-25213*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/251246-
dc.description.abstractWe present new constraints on the dark matter-induced annual modulation signal using 1.7 years of COSINE-100 data with a total exposure of 97.7 kg yr. The COSINE-100 experiment, consisting of 106 kg of NaI(Tl) target material, is designed to carry out a model-independent test of DAMA/LIBRA's claim of WIMP discovery by searching for the same annual modulation signal using the same NaI(Tl) target. The crystal data show a 2.7 cpd/kg/keV background rate on average in the 2-6 keV energy region of interest. Using a chi-squared minimization method we observe best fit values for modulation amplitude and phase of 0.0092 +/- 0.0067 cpd/kg/keV and 127.2 +/- 45.9 d, respectively.*
dc.languageEnglish*
dc.publisherAMER PHYSICAL SOC*
dc.titleSearch for a Dark Matter-Induced Annual Modulation Signal in NaI(Tl) with the COSINE-100 Experiment*
dc.typeArticle*
dc.relation.issue3*
dc.relation.volume123*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.journaltitlePHYSICAL REVIEW LETTERS*
dc.identifier.doi10.1103/PhysRevLett.123.031302*
dc.identifier.wosidWOS:000476695900002*
dc.identifier.scopusid2-s2.0-85069900265*
dc.author.googleAdhikari, G.*
dc.author.googleAdhikari, P.*
dc.author.googlede Souza, E. Barbosa*
dc.author.googleCarlin, N.*
dc.author.googleChoi, S.*
dc.author.googleDjamal, M.*
dc.author.googleEzeribe, A. C.*
dc.author.googleHa, C.*
dc.author.googleHahn, I. S.*
dc.author.googleJeon, E. J.*
dc.author.googleJo, J. H.*
dc.author.googleJoo, H. W.*
dc.author.googleKang, W. G.*
dc.author.googleKang, W.*
dc.author.googleKauer, M.*
dc.author.googleKim, G. S.*
dc.author.googleKim, H.*
dc.author.googleKim, H. J.*
dc.author.googleKim, K. W.*
dc.author.googleKim, N. Y.*
dc.author.googleKim, S. K.*
dc.author.googleKim, Y. D.*
dc.author.googleKim, Y. H.*
dc.author.googleKo, Y. J.*
dc.author.googleKudryavtsev, V. A.*
dc.author.googleLee, H. S.*
dc.author.googleLee, J.*
dc.author.googleLee, J. Y.*
dc.author.googleLee, M. H.*
dc.author.googleLeonard, D. S.*
dc.author.googleLynch, W. A.*
dc.author.googleMaruyama, R. H.*
dc.author.googleMouton, F.*
dc.author.googleOlsen, S. L.*
dc.author.googlePark, B. J.*
dc.author.googlePark, H. K.*
dc.author.googlePark, H. S.*
dc.author.googlePark, K. S.*
dc.author.googlePitta, R. L. C.*
dc.author.googlePrihtiadi, H.*
dc.author.googleRa, S. J.*
dc.author.googleRott, C.*
dc.author.googleShin, K. A.*
dc.author.googleScarff, A.*
dc.author.googleSpooner, N. J. C.*
dc.author.googleThompson, W. G.*
dc.author.googleYang, L.*
dc.author.googleYu, G. H.|COSINE-100 Collaboration*
dc.contributor.scopusid한인식(7201832280;57205469686;57192312712)*
dc.date.modifydate20240415134453*


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