Journal
ASTROPARTICLE PHYSICS
Volume 21, Issue 6, Pages 667-687Publisher
ELSEVIER
DOI: 10.1016/j.astropartphys.2004.05.001
Keywords
dark matter; WIMPs; neutron background; neutron flux; spontaneous fission; (alpha-n) reactions; radioactivity; cosmic-ray muons underground; photomultipliers
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Simulations of the neutron background for future large-scale particle dark matter detectors are presented. Neutrons were generated in rock and detector elements via spontaneous fission and (alpha, n) reactions, and by cosmic-ray muons. The simulation techniques and results are discussed in the context of the expected sensitivity of a generic liquid xenon dark matter detector. Methods of neutron background suppression are investigated. A sensitivity of 10(-9)-10(-10) pb to WIMP-nucleon interactions can be achieved by a tonne-scale detector. (C) 2004 Elsevier B.V. All rights reserved.
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