Simulations of neutron background in a time projection chamber relevant to dark matter searches
arXiv:hep-ex/0503017 · doi:10.1016/j.nima.2005.03.121
Abstract
Presented here are results of simulations of neutron background performed for a time projection chamber acting as a particle dark matter detector in an underground laboratory. The investigated background includes neutrons from rock and detector components, generated via spontaneous fission and (alpha, n) reactions, as well as those due to cosmic-ray muons. Neutrons were propagated to the sensitive volume of the detector and the nuclear recoil spectra were calculated. Methods of neutron background suppression were also examined and limitations to the sensitivity of a gaseous dark matter detector are discussed. Results indicate that neutrons should not limit sensitivity to WIMP-nucleon interactions down to a level of (1 - 3) x 10^{-8} pb in a 10 kg detector.
arXiv comment27 pages (total, including 3 tables and 11 figures). Accepted for publication in Nuclear Instruments and Methods in Physics Research - Section A
References in corpus (8)
- A Unified Approach to the Classical Statistical Analysis of Small Signals
- Neutron Flux at the Gran Sasso Underground LaboratoryRevisited
- Predicting Neutron Production from Cosmic-ray Muons
- Angular Signatures for Galactic Halo WIMP Scattering in Direct Detectors: Prospects and Challenges
- Neutron background in large-scale xenon detectors for dark matter searches
- Simulations of muon-induced neutron flux at large depths underground
- Measurements of muon flux at 1070 metres vertical depth in the Boulby underground laboratory
- Neutron background at the Canfranc Underground Laboratory and its contribution to the IGEX-DM dark matter experiment
Cited by in corpus (13)
- The case for a directional dark matter detector and the status of current experimental efforts
- Muon simulation codes MUSIC and MUSUN for underground physics
- A novel large-volume Spherical Detector with Proportional Amplification read-out
- Optimizing WIMP directional detectors
- Low energy neutron propagation in MCNPX and GEANT4
- Markov Chain Monte Carlo analysis to constrain Dark Matter properties with directional detection
- Determining the WIMP mass from a single direct detection experiment, a more detailed study
- First Results from the DRIFT-IIa Dark Matter Detector
- Directional Statistics for WIMP direct detection II: 2-d read-out
- The expected background spectrum in NaI dark matter detectors and the DAMA result
- Consequences of statistical sense determination for WIMP directional detection
- Measuring the Cosmic Ray Muon-Induced Fast Neutron Spectrum by (n,p) Isotope Production Reactions in Underground Detectors
- Radiation shielding for underground low-background experiments