Evaluation of cosmogenic production of and for rare-event physics using underground argon
arXiv:2202.06403 · doi:10.1016/j.astropartphys.2022.102733
Abstract
Underground argon (UAr) with lower cosmogenic activities of and has been planned as a detector in detecting scintillation light and charge collection using time projection chambers for dark matter searches and as a veto detector in suppressing backgrounds for neutrinoless double beta decay (0) experiments. Long-lived radioactive isotopes, and , can also be produced on the surface when UAr is pumped out from a deep well. Understanding the production of long-lived isotopes in Ar is important for utilizing UAr for dark matter and 0 experiments in terms of its production, transportation, and storage. Ar exposure to cosmic rays at sea-level is simulated using Geant4 for a given cosmic ray muon, neutron, and proton energy spectrum. We report the simulated cosmogenic production rates of , , and other long-lived isotopes at sea-level from fast neutrons, high energy muons, and high energy protons. Total production rates of 938.53/kgday and 5.8110/kgday for Ar and Ar are found from our simulation. Utilizing these production rates, we set a time limit of 954 days constrained by the production of Ar for UAr to be on the surface before it compromises the sensitivity for a dark matter experiment. Similarly, a time limit of 1702 days constrained by the production of Ar is found for a 0 experiment.
arXiv comment12 pages, 3 figures, and 2 tables
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