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Enhanced low-energy supernova burst detection in large liquid argon time projection chambers enabled by Q-Pix

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arxiv 2203.12109 v3 pith:D4Q53L4G submitted 2022-03-23 hep-ex physics.ins-det

S. Kubota , J. Ho , A. D. McDonald , N. Tata , J. Asaadi , R. Guenette , J. B. R. Battat , D. Braga
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M. Demarteau Z. Djurcic M. Febbraro E. Gramellini S. Kohani C. Mauger Y. Mei F. M. Newcomer K. Nishimura D. Nygren R. Van Berg G. S. Varner K. Woodworth
This is my paper · ORCID
classification hep-exphysics.ins-det
keywords detectionargondetectorsliquidlowerneutrinoneutrinosq-pix
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The detection of neutrinos from core-collapse supernovae may reveal important process features as well as neutrino properties. The detection of supernova neutrinos is one of the main science drivers for future kiloton-scale neutrino detectors based on liquid argon. Here we show that for such detectors the intrinsically 3D readout in Q-Pix offers numerous advantages relative to a wire-based readout, such as higher reconstruction efficiency, lower energy threshold, considerably lower data rates, and potential pointing information.

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  1. Opportunities and challenges to study solar neutrinos with a Q-Pix pixel readout

    hep-ex 2025-07 conditional novelty 6.0 of 10

    Simulations show a Q-Pix liquid argon detector could, in a low-background underground scenario, see boron-8 and hep solar neutrinos above about 5 MeV if poorly understood gamma and alpha-capture backgrounds are controlled.

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