- Akerib, DS;
- Bai, X;
- Bedikian, S;
- Bernard, E;
- Bernstein, A;
- Bolozdynya, A;
- Bradley, A;
- Byram, D;
- Cahn, SB;
- Camp, C;
- Carmona-Benitez, MC;
- Carr, D;
- Chapman, JJ;
- 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, CH;
- Fiorucci, S;
- Gaitskell, RJ;
- Gibson, KR;
- Gilchriese, M;
- Hall, C;
- Hanhardt, M;
- Holbrook, B;
- Ihm, M;
- Jacobsen, RG;
- Kastens, L;
- Kazkaz, K;
- Knoche, R;
- Kyre, S;
- Kwong, J;
- Lander, R;
- Larsen, NA;
- Lee, C;
- Leonard, DS;
- Lesko, KT;
- Lindote, A;
- Lopes, MI;
- Lyashenko, A;
- Malling, DC;
- Mannino, R;
- Marquez, Z;
- McKinsey, DN;
- Mei, D-M;
- Mock, J;
- Moongweluwan, M;
- Morii, M;
- Nelson, H;
- Neves, F;
- Nikkel, JA;
- Pangilinan, M;
- Parker, PD;
- Pease, EK;
- Pech, K;
- Phelps, P;
- Rodionov, A;
- Roberts, P;
- Shei, A;
- Shutt, T;
- Silva, C;
- Skulski, W;
- Solovov, VN;
- Sofka, CJ;
- Sorensen, P;
- Spaans, J;
- Stiegler, T;
- Stolp, D;
- Svoboda, R;
- Sweany, M;
- Szydagis, M;
- Taylor, D;
- Thomson, J;
- Tripathi, M;
- Uvarov, S;
- Verbus, JR;
- Walsh, N;
- Webb, R;
- White, D;
- White, JT;
- Whitis, TJ;
- Wlasenko, M;
- Wolfs, FLH;
- Woods, M;
- Zhang, C
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. © 2012 Elsevier B.V.