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Title: Technical results from the surface run of the LUX dark matter experiment

Journal Article · · Astroparticle Physics
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  1. Case Western Reserve Univ., Cleveland, OH (United States). Dept. of Physics
  2. South Dakota School of Mines and Technology, Rapid City, SD (United States)
  3. Yale Univ., New Haven, CT (United States). Dept. of Physics
  4. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  5. Univ. of South Dakota, Vermillion, SD (United States). Dept. of Physics
  6. Brown Univ., Providence, RI (United States). Dept. of Physics
  7. Univ. of Maryland, College Park, MD (United States). Dept. of Physics
  8. Univ. of Rochester, NY (United States). Dept. of Physics and Astronomy
  9. Univ. of California, Berkeley, CA (United States). Dept. of Physics
  10. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  11. Univ. of Coimbra, Rua Larga, Coimbra (Portugal). LIP-Coimbra, Dept. of Physics
  12. Texas A & M Univ., College Station, TX (United States). Dept. of Physics
  13. Univ. of California, Davis, CA (United States). Dept. of Physics
  14. Harvard Univ., Cambridge, MA (United States). Dept. of Physics
  15. Univ. of California, Santa Barbara, CA (United States). Dept. of Physics

We present the results of the three-month above-ground commissioning run of the Large Underground Xenon (LUX) experiment at the Sanford Underground Research Facility located in Lead, South Dakota, USA. LUX is a 370 kg liquid xenon detector that will search for cold dark matter in the form of Weakly Interacting Massive Particles (WIMPs). The commissioning run, conducted with the detector immersed in a water tank, validated the integration of the various sub-systems in preparation for the underground deployment. Using the data collected, we report excellent light collection properties, achieving 8.4 photoelectrons per keV for 662 keV electron recoils without an applied electric field, measured in the center of the WIMP target. We also find good energy and position resolution in relatively high-energy interactions from a variety of internal and external sources. Finally, we have used the commissioning data to tune the optical properties of our simulation and report updated sensitivity projections for spin-independent WIMP-nucleon scattering.

Research Organization:
University of California, Berkeley, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
Nuclear Science & Security Consortium (NNSC)
Grant/Contract Number:
NA0000979; FG02-08ER41549; FG02-91ER40688; FG02-95ER40917; FG02-91ER40674; FG02-11ER41738; FG02-11ER41751; AC52-07NA27344; PHY-0750671; PHY-0801536; PHY-1004661; PHY-1102470; PHY-1003660; RA0350; AC02-05CH11231
OSTI ID:
1454541
Alternate ID(s):
OSTI ID: 1511361
Journal Information:
Astroparticle Physics, Vol. 45, Issue C; ISSN 0927-6505
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 38 works
Citation information provided by
Web of Science

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Cited By (7)

Liquid noble gases for dark matter searches: An updated survey journal September 2015
DARWIN: towards the ultimate dark matter detector journal November 2016
Dark compact objects: An extensive overview journal March 2019
DARWIN: towards the ultimate dark matter detector text January 2016
Liquid noble gas detectors for low energy particle physics text January 2012
Results from a search for dark matter in the complete LUX exposure text January 2016
Calibration, event reconstruction, data analysis and limits calculation for the LUX dark matter experiment text January 2017

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