Monte Carlo Characterization of the Cosmic Ray Muon Flux in Subsurface Geological Repositories
Harish Gadey, Stylianos Chatzidakis, Abi T. Farsoni

TL;DR
This paper develops a Monte Carlo methodology to characterize cosmic ray muon fluxes at depths of geological repositories, exploring their potential for passive, non-invasive safeguards monitoring of nuclear materials underground.
Contribution
It introduces a new Monte Carlo-based approach to model muon fluxes and proposes parametrizations for detector-specific safeguards applications in geological repositories.
Findings
Muon flux decreases with depth but remains detectable.
Parametrizations enable practical muon monitoring at various depths.
Potential for muon-based detection of cask movement or excavation.
Abstract
Recent challenges in monitoring subsurface geological repositories call for new, innovative concepts that are facility independent, cost-effective, passive, and reliable. Inspection and verification of future disposal facilities will exert significant pressure on the limited safeguards resources. Compared to aboveground facilities, subsurface geological repositories cannot be directly monitored. Once nuclear material is in place in these facilities, reverifying the inventory may no longer be feasible if continuity of knowledge is lost or updated safeguards information on the contents (or lack thereof) becomes available to inspectors. Using cosmic ray muons presents several potential advantages over conventional photon/neutron signatures, and their use in safeguards applications has only recently received attention. However, there have been limited efforts to explore the integration of…
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Taxonomy
TopicsParticle Detector Development and Performance · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
