Please use this identifier to cite or link to this item: http://hdl.handle.net/10316/95851
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dc.contributor.authorAkerib, D. S.-
dc.contributor.authorAlsum, S.-
dc.contributor.authorAraújo, H. M.-
dc.contributor.authorBai, X.-
dc.contributor.authorBalajthy, J.-
dc.contributor.authorBaxter, A.-
dc.contributor.authorBernard, E. P.-
dc.contributor.authorBernstein, A.-
dc.contributor.authorBiesiadzinski, T. P.-
dc.contributor.authorBoulton, E. M.-
dc.contributor.authorB. Boxer, B.-
dc.contributor.authorBrás, P.-
dc.contributor.authorManalaysay, A.-
dc.contributor.authorMarangou, N.-
dc.contributor.authorMcKinsey, D. N.-
dc.contributor.authorMei, D.-M.-
dc.contributor.authorM. Moongweluwan, M.-
dc.contributor.authorMorad, J. A.-
dc.contributor.authorMurphy, A. St. J.-
dc.contributor.authorNaylor, A.-
dc.contributor.authorNehrkorn, C.-
dc.contributor.authorNelson, H. N.-
dc.contributor.authorNeves, F.-
dc.contributor.authorNilima, A.-
dc.contributor.authorOliver-Mallory, K. C.-
dc.contributor.authorPalladino, K. J.-
dc.contributor.authorPease, E. K.-
dc.contributor.authorRiffard, Q.-
dc.contributor.authorRischbieter, G. R. C.-
dc.contributor.authorRhyne, C.-
dc.contributor.authorRossiter, P.-
dc.contributor.authorShaw, S.-
dc.contributor.authorShutt, T. A.-
dc.contributor.authorSilva, C.-
dc.contributor.authoret al.-
dc.date.accessioned2021-09-29T08:29:13Z-
dc.date.available2021-09-29T08:29:13Z-
dc.date.issued2021-06-22-
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029-
dc.identifier.urihttp://hdl.handle.net/10316/95851-
dc.description11 pages, 6 figurespt
dc.description.abstractThe Large Underground Xenon (LUX) dark matter search was a 250-kg active mass dual-phase time projection chamber that operated by detecting light and ionization signals from particles incident on a xenon target. In December 2015, LUX reported a minimum 90% upper C.L. of 6e-46 cm^2 on the spin-independent WIMP-nucleon elastic scattering cross section based on a 1.4e4 kg*day exposure in its first science run. Tension between experiments and the absence of a definitive positive detection suggest it would be prudent to search for WIMPs outside the standard spin-independent/spin-dependent paradigm. Recent theoretical work has identified a complete basis of 14 independent effective field theory (EFT) operators to describe WIMP-nucleon interactions. In addition to spin-independent and spin-dependent nuclear responses, these operators can produce novel responses such as angular-momentum-dependent and spin-orbit couplings. Here we report on a search for all 14 of these EFT couplings with data from LUX's first science run. Limits are placed on each coupling as a function of WIMP mass.pt
dc.language.isoengpt
dc.publisherAmerican Physical Societypt
dc.relationPTDC/FIS-NUC/1525/2014pt
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleAn Effective Field Theory Analysis of the First LUX Dark Matter Searchpt
dc.typearticlept
degois.publication.issue12pt
degois.publication.titlePhysical Review Dpt
dc.relation.publisherversionhttps://journals.aps.org/prd/pdf/10.1103/PhysRevD.103.122005pt
dc.peerreviewedyespt
dc.identifier.doihttp://arxiv.org/abs/2003.11141v1-
dc.identifier.doi10.1103/PhysRevD.103.122005-
degois.publication.volume103pt
dc.date.embargo2021-06-22*
dc.identifier.urlhttp://arxiv.org/abs/2003.11141v1-
uc.date.periodoEmbargo0pt
item.languageiso639-1en-
item.fulltextCom Texto completo-
item.grantfulltextopen-
crisitem.author.deptFaculty of Sciences and Technology-
crisitem.author.parentdeptUniversity of Coimbra-
crisitem.author.researchunitLIP – Laboratory of Instrumentation and Experimental Particle Physics-
crisitem.author.orcid0000-0002-1771-1517-
Appears in Collections:I&D CFis - Artigos em Revistas Internacionais
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