Please use this identifier to cite or link to this item: http://hdl.handle.net/10316/27830
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dc.contributor.authorAkerib, D. S.-
dc.contributor.authorAraújo, H. M.-
dc.contributor.authorBai, X.-
dc.contributor.authorBailey, A. J.-
dc.contributor.authorBalajthy, J.-
dc.contributor.authorBernard, E.-
dc.contributor.authorBernstein, A.-
dc.contributor.authorBradley, A.-
dc.contributor.authorByram, D.-
dc.contributor.authorCahn, S. B.-
dc.contributor.authorCarmona-Benitez, M. C.-
dc.contributor.authorChan, C.-
dc.contributor.authorChapman, J. J.-
dc.contributor.authorChiller, A. A.-
dc.contributor.authorChiller, C.-
dc.contributor.authorCoffey, T.-
dc.contributor.authorCurrie, A.-
dc.contributor.authorViveiros, L. de-
dc.contributor.authorDobi, A.-
dc.contributor.authorDobson, J.-
dc.contributor.authorDruszkiewicz, E.-
dc.contributor.authorEdwards, B.-
dc.contributor.authorFaham, C. H.-
dc.contributor.authorFiorucci, S.-
dc.contributor.authorFlores, C.-
dc.contributor.authorGaitskell, R. J.-
dc.contributor.authorGehman, V. M.-
dc.contributor.authorGhag, C.-
dc.contributor.authorGibson, K. R.-
dc.contributor.authorGilchriese, M. G. D.-
dc.contributor.authorHall, C.-
dc.contributor.authorHertel, S. A.-
dc.contributor.authorHorn, M.-
dc.contributor.authorHuang, D. Q.-
dc.contributor.authorIhm, M.-
dc.contributor.authorJacobsen, R. G.-
dc.contributor.authorKazkaz, K.-
dc.contributor.authorKnoche, R.-
dc.contributor.authorLarsen, N. A.-
dc.contributor.authorLee, C.-
dc.contributor.authorLindote, A.-
dc.contributor.authorLopes, M. I.-
dc.contributor.authorMalling, D. C.-
dc.contributor.authorMannino, R.-
dc.contributor.authorMcKinsey, D. N.-
dc.contributor.authorMei, D.-M.-
dc.contributor.authorMock, J.-
dc.contributor.authorMoongweluwan, M.-
dc.contributor.authorMorad, J.-
dc.contributor.authorMurphy, A. St. J.-
dc.contributor.authorNehrkorn, C.-
dc.contributor.authorNelson, H.-
dc.contributor.authorNeves, F.-
dc.contributor.authorOtt, R. A.-
dc.contributor.authorPangilinan, M.-
dc.contributor.authorParker, P. D.-
dc.contributor.authorPease, E. K.-
dc.contributor.authorPech, K.-
dc.contributor.authorPhelps, P.-
dc.contributor.authorReichhart, L.-
dc.contributor.authorShutt, T.-
dc.contributor.authorSilva, C.-
dc.contributor.authorSolovov, V. N.-
dc.contributor.authorSorensen, P.-
dc.contributor.authorO’Sullivan, K.-
dc.contributor.authorSumner, T. J.-
dc.contributor.authorSzydagis, M.-
dc.contributor.authorTaylor, D.-
dc.contributor.authorTennyson, B.-
dc.contributor.authorTiedt, D. R.-
dc.contributor.authorTripathi, M.-
dc.contributor.authorUvarov, S.-
dc.contributor.authorVerbus, J. R.-
dc.contributor.authorWalsh, N.-
dc.contributor.authorWebb, R.-
dc.contributor.authorWhite, J. T.-
dc.contributor.authorWitherell, M. S.-
dc.contributor.authorWolfs, F. L. H.-
dc.contributor.authorWoods, M.-
dc.contributor.authorZhang, C.-
dc.date.accessioned2014-12-09T15:01:57Z-
dc.date.available2014-12-09T15:01:57Z-
dc.date.issued2015-03-
dc.identifier.citationAKERIB, D. S. [et. al] - Radiogenic and muon-induced backgrounds in the LUX dark matter detector. "Astroparticle Physics". ISSN 0927-6505. Vol. 62 (2015) p. 33–46por
dc.identifier.issn0927-6505-
dc.identifier.urihttp://hdl.handle.net/10316/27830-
dc.description.abstractThe Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The radiogenic backgrounds in the LUX detector have been measured and compared with Monte Carlo simulation. Measurements of LUX high-energy data have provided direct constraints on all background sources contributing to the background model. The expected background rate from the background model for the 85.3 day WIMP search run is (2.6±0.2stat±0.4sys)×10-3 events View the MathML source in a 118 kg fiducial volume. The observed background rate is (3.6±0.4stat)×10-3 events View the MathML source, consistent with model projections. The expectation for the radiogenic background in a subsequent one-year run is presented.por
dc.language.isoengpor
dc.publisherElsevierpor
dc.rightsopenAccesspor
dc.subjectLUXpor
dc.subjectDark matterpor
dc.subjectRadioactive backgroundpor
dc.subjectMaterial screeningpor
dc.subjectSimulationpor
dc.titleRadiogenic and muon-induced backgrounds in the LUX dark matter detectorpor
dc.typearticlepor
degois.publication.firstPage33por
degois.publication.lastPage46por
degois.publication.titleAstroparticle Physicspor
dc.relation.publisherversionhttp://www.sciencedirect.com/science/article/pii/S0927650514001054por
dc.peerreviewedYespor
dc.identifier.doi10.1016/j.astropartphys.2014.07.009-
degois.publication.volume62por
item.grantfulltextopen-
item.languageiso639-1en-
item.fulltextCom Texto completo-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
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