Search for low-mass dark matter with CsI(Tl) crystal detectors
DC Field | Value | Language |
---|---|---|
dc.contributor.author | H. S. Lee | - |
dc.contributor.author | H. Bhang | - |
dc.contributor.author | J. H. Choi | - |
dc.contributor.author | S. Choi | - |
dc.contributor.author | Kevin Insik, Hahn | - |
dc.contributor.author | E. J. Jeon | - |
dc.contributor.author | H.W. Joo | - |
dc.contributor.author | Woon Gu Kang | - |
dc.contributor.author | B. H. Kim | - |
dc.contributor.author | G. B. Kim | - |
dc.contributor.author | H. J. Kim | - |
dc.contributor.author | J. H. Kim | - |
dc.contributor.author | K.W. Kim | - |
dc.contributor.author | S. C. Kim | - |
dc.contributor.author | S. K. Kim | - |
dc.contributor.author | Yeongduk Kim | - |
dc.contributor.author | Yong Hamb Kim | - |
dc.contributor.author | J. H. Lee | - |
dc.contributor.author | J. K. Lee | - |
dc.contributor.author | S. J. Lee | - |
dc.contributor.author | D. S. Leonard | - |
dc.contributor.author | Jin Li | - |
dc.contributor.author | J. Li | - |
dc.contributor.author | Y. J. Li | - |
dc.contributor.author | X. R. Li | - |
dc.contributor.author | S. S. Myung | - |
dc.contributor.author | S. L. Olsen | - |
dc.contributor.author | J.W. Park | - |
dc.contributor.author | I. S. Seong | - |
dc.contributor.author | Jungho So | - |
dc.contributor.author | Q. Yue | - |
dc.date.available | 2015-04-21T09:04:42Z | - |
dc.date.created | 2014-11-26 | ko |
dc.date.issued | 2014-09 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/1473 | - |
dc.description.abstract | We present a search for low-mass (≤ 20 GeV=c2) weakly interacting massive particles (WIMPs), strong candidates of dark matter particles, using the low-background CsI(Tl) detector array of the Korea Invisible Mass Search experiment. With a total data exposure of 24,524.3 kg days, we search for WIMP interaction signals produced by nuclei recoiling from WIMP-nuclear elastic scattering with visible energies between 2 and 4 keVee (electron-equivalent energy). The observed energy distribution of candidate events is consistent with null signals, and upper limits of the WIMP-proton spin-independent interaction are set with a 90% confidence level. The observed limit covers most of the low-mass region of parameter space favored by the DAMA annual modulation signal assuming the standard halo model. | - |
dc.language | 영어 | - |
dc.publisher | American Physical Society | - |
dc.title | Search for low-mass dark matter with CsI(Tl) crystal detectors | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000342147500001 | - |
dc.identifier.scopusid | 2-s2.0-84907588732 | - |
dc.identifier.rimsid | 16562 | ko |
dc.date.tcdate | 2018-10-01 | - |
dc.contributor.affiliatedAuthor | E. J. Jeon | - |
dc.contributor.affiliatedAuthor | Woon Gu Kang | - |
dc.contributor.affiliatedAuthor | Yeongduk Kim | - |
dc.contributor.affiliatedAuthor | Yong Hamb Kim | - |
dc.contributor.affiliatedAuthor | Jin Li | - |
dc.contributor.affiliatedAuthor | Jungho So | - |
dc.identifier.doi | 10.1103/PhysRevD.90.052006 | - |
dc.identifier.bibliographicCitation | Physical Review D - Particles, Fields, Gravitation and Cosmology, v.90, no.5, pp.052006-1 - 052006-6 | - |
dc.relation.isPartOf | Physical Review D - Particles, Fields, Gravitation and Cosmology | - |
dc.citation.title | Physical Review D - Particles, Fields, Gravitation and Cosmology | - |
dc.citation.volume | 90 | - |
dc.citation.number | 5 | - |
dc.citation.startPage | 052006-1 | - |
dc.citation.endPage | 052006-6 | - |
dc.date.scptcdate | 2018-10-01 | - |
dc.description.wostc | 18 | - |
dc.description.scptc | 16 | - |
dc.description.journalClass | 1 | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | N | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Physics, Particles & Fields | - |
dc.subject.keywordPlus | SIMULATION | - |
dc.subject.keywordPlus | EMISSION | - |