Astronomy and Astrophysics – Astronomy
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005newar..49..315r&link_type=abstract
New Astronomy Reviews, v. 49, iss. 2-6 [SPECIAL ISSUE], p. 315-321.
Astronomy and Astrophysics
Astronomy
Scientific paper
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 (α,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.
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