Simulation of neutrons produced by high-energy muons underground

Abstract

This article describes the Monte Carlo simulation used to interpret the measurement of the muon-induced neutron flux in the Boulby Underground Laboratory (North Yorkshire, UK), recently performed using a large scintillator veto deployed around the ZEPLIN-II WIMP detector. Version 8.2 of the GEANT4 toolkit was used after relevant benchmarking and validation of neutron production models. In the direct comparison between Monte Carlo and experimental data, we find that the simulation produces a 1.8 times higher neutron rate, which we interpret as over-production in lead by GEANT4. The dominance of this material in neutron production allows us to estimate the absolute neutron yield in lead as (1.31 +/- 0.06) x 10^(-3) neutrons/muon/(g/cm^2) for a mean muon energy of 260 GeV. Simulated nuclear recoils due to muon-induced neutrons in the ZEPLIN-II target volume (~1 year exposure) showed that, although a small rate of events is expected from this source of background in the energy range of interest for dark matter searches, no event survives an anti-coincidence cut with the veto.

13 Pages, 11 Figures, 3 Tables. To appear in Astroparticle Physics. Version 2 has minor corrections and clarifications. Figures 1 and 3 now include neutron yields obtained with FLUKA-2008

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• Design and Construction of the DEAP-3600 Dark Matter Detector
• No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results
• Muon-induced background in the EDELWEISS dark matter search
• Measurement and simulation of the muon-induced neutron yield in lead
• The neutron background of the XENON100 dark matter experiment
• Radioactivity Backgrounds in ZEPLIN-III
• The ZEPLIN-III Anti-Coincidence Veto Detector
• Performance of the veto detector incorporated into the ZEPLIN-III experiment
• The Muon-Induced Neutron Indirect Detection EXperiment, MINIDEX
• Neutron Production by Cosmic-Ray Muons in Various Materials
• Muon-induced neutrons in lead and copper at shallow depth
• Signatures of muonic activation in the Majorana Demonstrator
• Measurement of cosmic muon-induced neutron background with ISMRAN detector in a non-reactor environment