作者
DS Akerib, X Bai, S Bedikian, E Bernard, A Bernstein, A Bolozdynya, A Bradley, D Byram, SB Cahn, C Camp, MC Carmona-Benitez, D Carr, JJ Chapman, A Chiller, C Chiller, K Clark, T Classen, T Coffey, A Curioni, E Dahl, S Dazeley, L De Viveiros, A Dobi, E Dragowsky, E Druszkiewicz, B Edwards, CH Faham, S Fiorucci, RJ Gaitskell, KR Gibson, M Gilchriese, C Hall, M Hanhardt, B Holbrook, M Ihm, RG Jacobsen, L Kastens, K Kazkaz, R Knoche, S Kyre, J Kwong, R Lander, NA Larsen, C Lee, DS Leonard, KT Lesko, A Lindote, MI Lopes, A Lyashenko, DC Malling, R Mannino, Z Marquez, DN McKinsey, D-M Mei, J Mock, M Moongweluwan, M Morii, H Nelson, F Neves, JA Nikkel, M Pangilinan, PD Parker, EK Pease, K Pech, P Phelps, A Rodionov, P Roberts, A Shei, T Shutt, C Silva, W Skulski, VN Solovov, CJ Sofka, P Sorensen, J Spaans, T Stiegler, D Stolp, R Svoboda, M Sweany, M Szydagis, D Taylor, J Thomson, M Tripathi, S Uvarov, JR Verbus, N Walsh, R Webb, D White, JT White, TJ Whitis, M Wlasenko, FLH Wolfs, M Woods, C Zhang
发表日期
2013/3/11
期刊
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
卷号
704
页码范围
111-126
出版商
North-Holland
简介
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.
学术搜索中的文章
DS Akerib, X Bai, S Bedikian, E Bernard, A Bernstein… - Nuclear Instruments and Methods in Physics Research …, 2013