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Radiogenic and muon-induced backgrounds in the LUX dark matter detector
Affiliation:1. Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA, USA;2. Pacific Northwest National Laboratory, Richland, WA, USA;3. Department of Physics and Astronomy, University of South Carolina, Columbia, SC, USA;4. Oak Ridge National Laboratory, Oak Ridge, TN, USA;5. National Research Center “Kurchatov Institute” Institute for Theoretical and Experimental Physics, Moscow, Russia;6. Joint Institute for Nuclear Research, Dubna, Russia;7. Department of Physics, Duke University, Durham, NC, USA;8. Triangle Universities Nuclear Laboratory, Durham, NC, USA;9. Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, WA, USA;10. Department of Physics, University of South Dakota, Vermillion, SD, USA;11. South Dakota School of Mines and Technology, Rapid City, SD, USA;12. Los Alamos National Laboratory, Los Alamos, NM, USA;13. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN, USA;14. Research Center for Nuclear Physics and Department of Physics, Osaka University, Ibaraki, Osaka, Japan;15. Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC, USA;p. Department of Physics, North Carolina State University, Raleigh, NC, USA;q. Department of Physics, Black Hills State University, Spearfish, SD, USA;r. Tennessee Tech University, Cookeville, TN, USA;s. Department of Nuclear Engineering, University of California, Berkeley, CA 94720, US;t. Department of Physics, University of South Dakota, Vermillion, SD, USA;u. Department of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Canada
Abstract:
Keywords:LUX  Dark matter  Radioactive background  Material screening  Simulation
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