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Search for MeV electron recoils from dark matter in EXO-200

DC Field Value Language
dc.contributor.authorAl, Kharusi S.-
dc.contributor.authorAnton, G.-
dc.contributor.authorBadhrees, I.-
dc.contributor.authorBarbeau, P.S.-
dc.contributor.authorBeck, D.-
dc.contributor.authorBelov, V.-
dc.contributor.authorBhatta, T.-
dc.contributor.authorBreidenbach, M.-
dc.contributor.authorBrunner, T.-
dc.contributor.authorCao, G.F.-
dc.contributor.authorCen, W.R.-
dc.contributor.authorChambers, C.-
dc.contributor.authorCleveland, B.-
dc.contributor.authorCoon, M.-
dc.contributor.authorCraycraft, A.-
dc.contributor.authorDaniels, T.-
dc.contributor.authorDarroch, L.-
dc.contributor.authorDaugherty, S.J.-
dc.contributor.authorDavis, J.-
dc.contributor.authorDelaquis, S.-
dc.contributor.authorDer, Mesrobian-Kabakian A.-
dc.contributor.authorDevoe, R.-
dc.contributor.authorDilling, J.-
dc.contributor.authorDolgolenko, A.-
dc.contributor.authorDolinski, M.J.-
dc.contributor.authorEchevers, J.-
dc.contributor.authorFairbank, W.-
dc.contributor.authorFairbank, D.-
dc.contributor.authorFarine, J.-
dc.contributor.authorFeyzbakhsh, S.-
dc.contributor.authorFierlinger, P.-
dc.contributor.authorFu, Y.S.-
dc.contributor.authorFudenberg, D.-
dc.contributor.authorGautam, P.-
dc.contributor.authorGornea, R.-
dc.contributor.authorGratta, G.-
dc.contributor.authorHall, C.-
dc.contributor.authorHansen, E.V.-
dc.contributor.authorHoessl, J.-
dc.contributor.authorHufschmidt, P.-
dc.contributor.authorHughes, M.-
dc.contributor.authorIverson, A.-
dc.contributor.authorJamil, A.-
dc.contributor.authorJessiman, C.-
dc.contributor.authorJewell, M.J.-
dc.contributor.authorJohnson, A.-
dc.contributor.authorKarelin, A.-
dc.contributor.authorKaufman, L.J.-
dc.contributor.authorKoffas, T.-
dc.contributor.authorKrucken, R.-
dc.contributor.authorKuchenkov, A.-
dc.contributor.authorKumar, K.S.-
dc.contributor.authorLan, Y.-
dc.contributor.authorLarson, A.-
dc.contributor.authorLenardo, B.G.-
dc.contributor.authorDouglas, Leonard-
dc.contributor.authorLi, G.S.-
dc.contributor.authorLi, S.-
dc.contributor.authorLi, Z.-
dc.contributor.authorLicciardi, C.-
dc.contributor.authorLin, Y.H.-
dc.contributor.authorMaclellan, R.-
dc.contributor.authorMcElroy, T.-
dc.contributor.authorMichel, T.-
dc.contributor.authorMong, B.-
dc.contributor.authorMoore, D.C.-
dc.contributor.authorMurray, K.-
dc.contributor.authorNjoya, O.-
dc.contributor.authorNusair, O.-
dc.contributor.authorOdian, A.-
dc.contributor.authorOstrovskiy, I.-
dc.contributor.authorPerna, A.-
dc.contributor.authorPiepke, A.-
dc.contributor.authorPocar, A.-
dc.contributor.authorRetiere, F.-
dc.contributor.authorRobinson, A.L.-
dc.contributor.authorRowson, P.C.-
dc.contributor.authorRuddell, D.-
dc.contributor.authorRunge, J.-
dc.contributor.authorSchmidt, S.-
dc.contributor.authorSinclair, D.-
dc.contributor.authorSkarpaas, K.-
dc.contributor.authorSoma, A.K.-
dc.contributor.authorStekhanov, V.-
dc.contributor.authorTarka, M.-
dc.contributor.authorThibado, S.-
dc.contributor.authorTodd, M.-
dc.contributor.authorTolba, T.-
dc.contributor.authorTotev, T.I.-
dc.contributor.authorTsang, R.H.M.-
dc.contributor.authorVeenstra, B.-
dc.contributor.authorVeeraraghavan, V.-
dc.contributor.authorVogel, P.-
dc.contributor.authorVuilleumier, J.-L.-
dc.contributor.authorWagenpfeil, M.-
dc.contributor.authorWatkins, J.-
dc.contributor.authorWen, L.J.-
dc.contributor.authorWichoski, U.-
dc.contributor.authorWrede, G.-
dc.contributor.authorWu, S.X.-
dc.contributor.authorXia, Q.-
dc.contributor.authorYahne, D.R.-
dc.contributor.authorYang, L.-
dc.contributor.authorYen, Y.-R.-
dc.contributor.authorZeldovich, O. Ya.-
dc.contributor.authorZiegler, T.-
dc.date.accessioned2024-01-19T22:01:37Z-
dc.date.available2024-01-19T22:01:37Z-
dc.date.created2023-04-03-
dc.date.issued2023-01-
dc.identifier.issn2470-0010-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/14675-
dc.description.abstractWe present a search for electron-recoil signatures from the charged-current absorption of fermionic dark matter using the EXO-200 detector. We report an average electron-recoil background rate of 6.8×104 cts kg-1 yr-1 keV above 4 MeV and find no statistically significant excess over our background projection. Using a total Xe136 exposure of 234.1 kg yr, we exclude new parameter space for the charged-current absorption cross section for dark matter masses between mχ=2.6-11.6 MeV with a minimum of 6×1051 cm2 at 8.3 MeV at the 90% confidence level.-
dc.language영어-
dc.publisherAmerican Physical Society-
dc.titleSearch for MeV electron recoils from dark matter in EXO-200-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.wosid000950501000011-
dc.identifier.scopusid2-s2.0-85147419989-
dc.identifier.rimsid80399-
dc.contributor.affiliatedAuthorDouglas, Leonard-
dc.identifier.doi10.1103/PhysRevD.107.012007-
dc.identifier.bibliographicCitationPhysical Review D, v.107, no.1-
dc.relation.isPartOfPhysical Review D-
dc.citation.titlePhysical Review D-
dc.citation.volume107-
dc.citation.number1-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
Appears in Collections:
Center for Underground Physics(지하실험 연구단) > 1. Journal Papers (저널논문)
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