51. Status of the LUX Dark Matter Search
- Author
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S. Fiorucci, D. S. Akerib, S. Bedikian, A. Bernstein, A. Bolozdynya, A. Bradley, D. Carr, J. Chapman, K. Clark, T. Classen, A. Curioni, E. Dahl, S. Dazeley, L. de Viveiros, E. Druszkiewicz, R. Gaitskell, C. Hall, C. Hernandez Faham, B. Holbrook, L. Kastens, K. Kazkaz, R. Lander, K. Lesko, D. Malling, R. Mannino, D. McKinsey, D. Mei, J. Mock, J. Nikkel, P. Phelps, U. Schroeder, T. Shutt, W. Skulski, P. Sorensen, J. Spaans, T. Stiegler, R. Svoboda, M. Sweany, J. Thomson, J. Toke, M. Tripathi, N. Walsh, R. Webb, J. White, F. Wolfs, M. Woods, C. Zhang, George Alverson, Pran Nath, and Brent Nelson
- Subjects
Physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,LUX ,Field (physics) ,Solar neutrino ,Dark matter ,FOS: Physical sciences ,Design elements and principles ,Astronomy ,chemistry.chemical_element ,Ranging ,Supernova ,Xenon ,chemistry ,astro-ph.CO ,Dark Matter ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Astrophysics - Cosmology and Nongalactic Astrophysics ,astro-ph.IM - Abstract
The Large Underground Xenon (LUX) dark matter search experiment is currently being deployed at the Homestake Laboratory in South Dakota. We will highlight the main elements of design which make the experiment a very strong competitor in the field of direct detection, as well as an easily scalable concept. We will also present its potential reach for supersymmetric dark matter detection, within various timeframes ranging from 1 year to 5 years or more., 4 pages, in proceedings of the SUSY09 conference
- Published
- 2010
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