The Large Underground Xenon (LUX) Experiment

Bibliographic Details
Main Author: LUX collaboration (94 authors)
Publication Date: 2012
Other Authors: de Viveiros, L., Lindote, A., Lopes, M.I., Neves, F., Silva, C., Solovov, V.N.
Format: Article
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://dx.doi.org/10.1016/j.nima.2012.11.135
http://hdl.handle.net/10400.26/26329
Summary: The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles(WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross section per nucleon of $2\times 10^{-46}$ cm$^{2}$, equivalent to $\sim$1 event/100 kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have $<$1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.
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spelling The Large Underground Xenon (LUX) ExperimentThe Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles(WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross section per nucleon of $2\times 10^{-46}$ cm$^{2}$, equivalent to $\sim$1 event/100 kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have $<$1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.Repositório ComumLUX collaboration (94 authors)de Viveiros, L.Lindote, A.Lopes, M.I.Neves, F.Silva, C.Solovov, V.N.2019-02-03T21:51:12Z2012-112019-02-03T21:51:11Z2012-11-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1016/j.nima.2012.11.135http://hdl.handle.net/10400.26/26329enginfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2025-05-14T13:05:15Zoai:comum.rcaap.pt:10400.26/26329Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-29T07:18:57.833446Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv The Large Underground Xenon (LUX) Experiment
title The Large Underground Xenon (LUX) Experiment
spellingShingle The Large Underground Xenon (LUX) Experiment
LUX collaboration (94 authors)
title_short The Large Underground Xenon (LUX) Experiment
title_full The Large Underground Xenon (LUX) Experiment
title_fullStr The Large Underground Xenon (LUX) Experiment
title_full_unstemmed The Large Underground Xenon (LUX) Experiment
title_sort The Large Underground Xenon (LUX) Experiment
author LUX collaboration (94 authors)
author_facet LUX collaboration (94 authors)
de Viveiros, L.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
author_role author
author2 de Viveiros, L.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
author2_role author
author
author
author
author
author
dc.contributor.none.fl_str_mv Repositório Comum
dc.contributor.author.fl_str_mv LUX collaboration (94 authors)
de Viveiros, L.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
description The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles(WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross section per nucleon of $2\times 10^{-46}$ cm$^{2}$, equivalent to $\sim$1 event/100 kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have $<$1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.
publishDate 2012
dc.date.none.fl_str_mv 2012-11
2012-11-01T00:00:00Z
2019-02-03T21:51:12Z
2019-02-03T21:51:11Z
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dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1016/j.nima.2012.11.135
http://hdl.handle.net/10400.26/26329
url http://dx.doi.org/10.1016/j.nima.2012.11.135
http://hdl.handle.net/10400.26/26329
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