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Radiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector

dc.contributor.authorAkerib, D.S. et al. (80 authors)
dc.contributor.authorde Viveiros, L.
dc.contributor.authorLindote, A.
dc.contributor.authorLopes, M.I.
dc.contributor.authorNeves, F.
dc.contributor.authorSilva, C.
dc.contributor.authorSolovov, V.N.
dc.date.accessioned2019-02-04T00:17:49Z
dc.date.available2019-02-04T00:17:49Z
dc.date.issued2015-03
dc.date.updated2019-02-04T00:17:49Z
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 $(2.6\pm0.2_{\textrm{stat}}\pm0.4_{\textrm{sys}})\times10^{-3}$~events~keV$_{ee}^{-1}$~kg$^{-1}$~day$^{-1}$ in a 118~kg fiducial volume. The observed background rate is $(3.6\pm0.4_{\textrm{stat}})\times10^{-3}$~events~keV$_{ee}^{-1}$~kg$^{-1}$~day$^{-1}$, consistent with model projections. The expectation for the radiogenic background in a subsequent one-year run is presented.
dc.description.versionPeer Reviewed
dc.identifierAstropart.Phys. 62 (2015) 33-46; DOI 10.1016/j.astropartphys.2014.07.009
dc.identifier.urihttp://dx.doi.org/10.1016/j.astropartphys.2014.07.009
dc.identifier.urihttp://hdl.handle.net/10400.26/26545
dc.language.isoeng
dc.titleRadiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector
dc.typejournal article
dspace.entity.typePublication
oaire.awardURIinfo:eu-repo/grantAgreement/FCT/5876-PPCDTI/CERN%2FFP%2F123610%2F2011/PT
oaire.fundingStream5876-PPCDTI
project.funder.identifierhttp://doi.org/10.13039/501100001871
project.funder.nameFundação para a Ciência e a Tecnologia
rcaap.rightsopenAccesspt
rcaap.typearticle
relation.isProjectOfPublication85c74552-6703-42ad-a85d-809b627b13d4
relation.isProjectOfPublication.latestForDiscovery85c74552-6703-42ad-a85d-809b627b13d4

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