Large Low Background kTon-Scale Liquid Argon Time Projection Chambers
T. Bezerra, A. Borkum, E. Church, C. Cuesta, Z. Djurcic, J. Genovesi,, J. Haiston, C. M. Jackson, I. Lazanu, B. Monreal, S. Munson, C. Ortiz, M., Parvu, S. J. M. Peeters, D. Pershey, S. S. Poudel, J. Reichenbacher, R., Saldanha, K. Scholberg, G. Sinev, S. Westerdale, J. Zennamo

TL;DR
This paper explores the potential of large, low-background liquid argon detectors to enhance sensitivity to low-energy physics phenomena like neutrinos, double beta decay, and dark matter, through design improvements and radiopurity controls.
Contribution
It demonstrates the feasibility of augmenting existing DUNE-like detectors for low-energy physics searches, including supernova neutrinos, double beta decay, and dark matter detection.
Findings
Enhanced sensitivity to supernova and solar neutrinos.
Feasibility of neutrinoless double beta decay search with $^{136}$Xe.
Competitive dark matter detection capabilities with seasonal variation signatures.
Abstract
We find that it is possible to increase sensitivity to low energy physics in a third or fourth DUNE-like module with careful controls over radiopurity and targeted modifications to a detector similar to the DUNE Far Detector design. In particular, sensitivity to supernova and solar neutrinos can be enhanced with improved MeV-scale reach. A neutrinoless double beta decay search with Xe loading appears feasible. Furthermore, sensitivity to Weakly-Interacting Massive Particle (WIMP) Dark Matter (DM) becomes competitive with the planned world program in such a detector, offering a unique seasonal variation detection that is characteristic for the nature of WIMPs.
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