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Akerib, D.S.; Bai, X.; Bedikian, S.; Bernard, E.; Bernstein, A.; Bolozdynya, A.; Bradley, A.; Byram, D.; Cahn, S.B.; Camp, C.; Carmona-Benitez, M.C.; Carr, D.; Chapman, J.J.; Chiller, A.; Chiller, C.; Clark, K.; Classen, T.; Coffey, T.; Curioni, A.; Dahl, E.; Dazeley, S.; de Viveiros, L.; Dobi, A.; Dragowsky, E.; Druszkiewicz, E.; Edwards, B.; Faham, C.H.; Fiorucci, S.; Gaitskell, R.J.; Gibson, K.R.; Gilchriese, M.; Hall, C.; Hanhardt, M.; Holbrook, B.; Ihm, M.; Jacobsen, R.G.; Kastens, L.; Kazkaz, K.; Knoche, R.; Kyre, S.; Kwong, J.; Lander, R.; Larsen, N.A.; Lee, C.; Leonard, D.S.; Lesko, K.T.; Lindote, A.; Lopes, M.I.; Lyashenko, A.; Malling, D.C.; Mannino, R.; Marquez, Z.; McKinsey, D.N.; Mei, D.-M.; Mock, J.; Moongweluwan, M.; Morii, M.; Nelson, H.; Neves, F.; Nikkel, J.A.; Pangilinan, M.; Parker, P.D.; Pease, E.K.; Pech, K.; Phelps, P.; Rodionov, A.; Roberts, P.; Shei, A.; Shutt, T.; Silva, C.; Skulski, W.; Solovov, V.N.; Sofka, C.J.; Sorensen, P.; Spaans, J.; Stiegler, T.; Stolp, D.; Svoboda, R.; Sweany, M.; Szydagis, M.; Taylor, D.; Thomson, J.; Tripathi, M.; Uvarov, S.; Verbus, J.R.; Walsh, N.; Webb, R.; White, D.; White, J.T.; Whitis, T.J.; Wlasenko, M.; Wolfs, F.L.H.; Woods, M.; Zhang, C.
Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 03/2013, Volume: 704Journal Article
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 2×10−46cm2, equivalent to ∼1event/100kg/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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