Technical results from the surface run of the LUX dark matter experiment
- Case Western Reserve Univ., Cleveland, OH (United States). Dept. of Physics
- South Dakota School of Mines and Technology, Rapid City, SD (United States)
- Yale Univ., New Haven, CT (United States). Dept. of Physics
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of South Dakota, Vermillion, SD (United States). Dept. of Physics
- Brown Univ., Providence, RI (United States). Dept. of Physics
- Univ. of Maryland, College Park, MD (United States). Dept. of Physics
- Univ. of Rochester, NY (United States). Dept. of Physics and Astronomy
- Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of Coimbra, Rua Larga, Coimbra (Portugal). LIP-Coimbra, Dept. of Physics
- Texas A & M Univ., College Station, TX (United States). Dept. of Physics
- Univ. of California, Davis, CA (United States). Dept. of Physics
- Harvard Univ., Cambridge, MA (United States). Dept. of Physics
- 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
Web of Science
Liquid noble gases for dark matter searches: An updated survey
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journal | September 2015 |
DARWIN: towards the ultimate dark matter detector
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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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