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dc.contributor.author한인식*
dc.date.accessioned2024-02-15T05:12:14Z-
dc.date.available2024-02-15T05:12:14Z-
dc.date.issued2023*
dc.identifier.issn0031-9007*
dc.identifier.issn1079-7114*
dc.identifier.otherOAK-34700*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/267884-
dc.description.abstractWe search for energetic electron recoil signals induced by boosted dark matter (BDM) from the galactic center using the COSINE-100 array of NaI(Tl) crystal detectors at the Yangyang Underground Laboratory. The signal would be an excess of events with energies above 4 MeV over the well-understood background. Because no excess of events are observed in a 97.7 kg center dot yr exposure, we set limits on BDM interactions under a variety of hypotheses. Notably, we explored the dark photon parameter space, leading to competitive limits compared to direct dark photon search experiments, particularly for dark photon masses below 4 MeV and considering the invisible decay mode. Furthermore, by comparing our results with a previous BDM search conducted by the Super-Kamionkande experiment, we found that the COSINE-100 detector has advantages in searching for low-mass dark matter. This analysis demonstrates the potential of the COSINE-100 detector to search for MeV electron recoil signals produced by the dark sector particle interactions.*
dc.languageEnglish*
dc.publisherAMER PHYSICAL SOC*
dc.titleSearch for Boosted Dark Matter in COSINE-100*
dc.typeArticle*
dc.relation.issue20*
dc.relation.volume131*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.journaltitlePHYSICAL REVIEW LETTERS*
dc.identifier.doi10.1103/PhysRevLett.131.201802|http://dx.doi.org/10.1103/PhysRevLett.131.201802*
dc.identifier.wosidWOS:001163660900002*
dc.identifier.scopusid2-s2.0-85178344362*
dc.author.googleAdhikari, G.*
dc.author.googleCarlin, N.*
dc.author.googleChoi, J. J.*
dc.author.googleChoi, S.*
dc.author.googleEzeribe, A. C.*
dc.author.googleFranca, L. E.*
dc.author.googleHa, C.*
dc.author.googleHahn, I. S.*
dc.author.googleHollick, S. J.*
dc.author.googleJeon, E. J.*
dc.author.googleJo, J. H.*
dc.author.googleJoo, H. W.*
dc.author.googleKang, W. G.*
dc.author.googleKauer, M.*
dc.author.googleKim, B. H.*
dc.author.googleKim, H. J.*
dc.author.googleKim, J.*
dc.author.googleKim, K. W.*
dc.author.googleKim, S. H.*
dc.author.googleKim, S. K.*
dc.author.googleKim, W. K.*
dc.author.googleKim, Y. D.*
dc.author.googleKim, Y. H.*
dc.author.googleKo, Y. J.*
dc.author.googleLee, D. H.*
dc.author.googleLee, E. . K.*
dc.author.googleLee, H.*
dc.author.googleLee, H. S.*
dc.author.googleLee, H. Y.*
dc.author.googleLee, I. S.*
dc.author.googleLee, J.*
dc.author.googleLee, J. Y.*
dc.author.googleLee, M. H.*
dc.author.googleLee, S. H.*
dc.author.googleLee, S. M.*
dc.author.googleLee, Y. J.*
dc.author.googleLeonard, D. S.*
dc.author.googleLuan, N. T.*
dc.author.googleManzato, B. B.*
dc.author.googleMaruyama, R. H.*
dc.author.googleNeal, R. J.*
dc.author.googleNikkel, J. A.*
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.googlePark, S. D.*
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.googleCavalcante, D. F. F. S.*
dc.author.googleScarff, A.*
dc.author.googleSpooner, N. J. C.*
dc.author.googleThompson, W. G.*
dc.author.googleYang, L.*
dc.author.googleYu, G. H.*
dc.contributor.scopusid한인식(7201832280;57205469686;57192312712)*
dc.date.modifydate20240502144901*
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사범대학 > 과학교육과 > Journal papers
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