2004
DOI: 10.1016/s0927-6505(04)00075-1
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Neutron background in large-scale xenon detectors for dark matter searches

Abstract: 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 b… Show more

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Cited by 2 publications
(2 citation statements)
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References 13 publications
(25 reference statements)
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“…This flux is comparable to measurements and simulations of the (α, n) neutron flux in other underground labs [63,64]. No attempt was made to measure the intrinsic background of the detector, but based on its material composition and an estimate of the intrinsic radioactivity, the contribution is expected to be very small.…”
Section: Underground Measurementsupporting
confidence: 73%
“…This flux is comparable to measurements and simulations of the (α, n) neutron flux in other underground labs [63,64]. No attempt was made to measure the intrinsic background of the detector, but based on its material composition and an estimate of the intrinsic radioactivity, the contribution is expected to be very small.…”
Section: Underground Measurementsupporting
confidence: 73%
“…The soft- Table 6: Calculated contaminations for a sample of resistors screened using both Chaloner and Lunehead. A high level of agreement is seen across the 238 U chain with the exception of 210 Pb which has a measured specific activity 58× higher than those isotopes above it in the chain (determined using the combined Lunehead/Chaloner measurement of 226 ware has been modified to extend the energies of α-particles from the original energy cut of 6.5 MeV to 10 MeV [31], and to improve the cross-section library for a large number of materials [32,33,34], with newly added cross-sections calculated using the EMPIRE-2.19 code [35]. In the worst case scenario, we assume that all the measured contamination in the surface mount resistors is confined to the ceramic.…”
Section: Significant Disequilibrium At 210 Pbmentioning
confidence: 90%