Simulation of neutron background for a dark matter search experiment at JUSL
arXiv:2011.04969 · doi:10.1088/1748-0221/16/06/P06022
Abstract
Dark matter search experiments demand low to ultralow radiation background to operate. It is very important to understand the nature of the radiation background including knowledge about the sources contributing to it. Sometimes, evaluation of the background becomes very specific to the site chosen for the experiment, and also to the experimental configuration. A dark matter search experiment is proposed to be set up at the Jaduguda Underground Science Laboratory (JUSL) in India. The laboratory will be located inside an existing mine with 555 m of vertical rock overburden. Neutrons produced from reactions, spontaneous fission of natural radioactive impurities in the rocks, and also from cosmic muon induced reactions are considered as the main background which can affect the sensitivity and outcome of the experiment. In this work, simulations based on GEANT4 are done to understand both the radiogenic neutron background caused by natural radioactivity of the surrounding rock and the cosmogenic neutron background due to interaction of the deeply penetrating cosmic muons with the rock. The muon flux in the cavern is obtained to be cms and the fluxes of radiogenic and cosmogenic neutrons above an energy threshold of 1 MeV in the cavern are obtained to be cms and cms respectively. The values obtained are comparable with estimates and measurements done for DAMA, WIPP and dark matter experiments at Boulby mine. The effectiveness of different shielding materials are also investigated to obtain the best possible neutron background reduction for a dark matter search experiment at JUSL. We also estimate the sensitivity of a CsI based detector for Weakly Interacting Massive Particle (WIMP) dark matter search at JUSL considering the estimated neutron background.
References in corpus (12)
- Planck 2015 results. XIII. Cosmological parameters
- Direct Detection of WIMP Dark Matter: Concepts and Status
- Muon-Induced Background Study for Underground Laboratories
- Evolution of the Reactor Antineutrino Flux and Spectrum at Daya Bay
- Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)
- Direct dark matter detection: the next decade
- Neutron background in large-scale xenon detectors for dark matter searches
- First limit on WIMP cross section with low background CsI(Tl) crystal detector
- Evaluation of (alpha,n) Induced Neutrons as a Background for Dark Matter Experiments
- Neutron beam test of CsI crystal for dark matter search
- The Cosmic Ray Muon Flux at WIPP
- Muon-induced neutrons do not explain the DAMA data