The Large Underground Xenon (LUX) Experiment
arXiv:1211.3788 · doi:10.1016/j.nima.2012.11.135
Abstract
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 cm, equivalent to 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.
50 pages, 16 figures
References in corpus (7)
- Dark Matter Results from 225 Live Days of XENON100 Data
- The ZEPLIN-III dark matter detector: instrument design, manufacture and commissioning
- Evaluation of (alpha,n) Induced Neutrons as a Background for Dark Matter Experiments
- Technical Results from the Surface Run of the LUX Dark Matter Experiment
- Performance and Fundamental Processes at Low Energy in a Two-Phase Liquid Xenon Dark Matter Detector
- Limits on spin-dependent WIMP-nucleon cross-sections from the first ZEPLIN-II data
- A simple high-sensitivity technique for purity analysis of xenon gas