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Title: Surface backgrounds in the DEAP-3600 dark matter experiment

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3579572· OSTI ID:21513196
; ;  [1];  [2]
  1. Department of Physics, Queen's University, Kingston, ON K7L 3N6 (Canada)
  2. Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario, P3E 2C6, and SNOLAB, Lively, Ontario, P3Y 1M3 (Canada)

DEAP-3600 is a dark matter experiment using 3.6 tons of liquid argon to search for Weakly Interacting Massive Particles (WIMPs), with a target sensitivity to the spin-independent WIMP-nucleon cross-section of 10{sup -46} cm{sup 2}. The detector is designed to allow for a three year background-free run with a 1-ton fiducial volume. We identify in this paper the potential sources of surface contamination. We require {sup 238}U and {sup 232}Th contaminations on the order of 10{sup -12} g/g or less, a level achieved by the SNO experiment, and {sup 210}Pb not significantly out of equilibrium with {sup 238}U, i.e., 10{sup -20} g/g or less {sup 210}Pb in the acrylic vessel or TPB wavelength shifter, which should be achievable with appropriate control of exposure to radon.

OSTI ID:
21513196
Journal Information:
AIP Conference Proceedings, Vol. 1338, Issue 1; Conference: LRT-2010: Topical workshop on low radioactivity techniques, Sudbury (Canada), 28-29 Aug 2010; Other Information: DOI: 10.1063/1.3579572; (c) 2011 American Institute of Physics; ISSN 0094-243X
Country of Publication:
United States
Language:
English