Enhanced low-energy supernova burst detection in large liquid argon time projection chambers enabled by Q-Pix
S. Kubota, J. Ho, A. D. McDonald, N. Tata, J. Asaadi, R. Guenette, J., B. R. Battat, D. Braga, 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

TL;DR
This paper demonstrates that Q-Pix technology enhances supernova neutrino detection in large liquid argon detectors by improving efficiency, lowering energy thresholds, and reducing data rates, thus advancing neutrino astrophysics.
Contribution
It introduces the application of Q-Pix 3D readout in liquid argon detectors, showing significant advantages over traditional wire-based systems for supernova neutrino detection.
Findings
Q-Pix offers higher reconstruction efficiency.
Lower energy detection threshold achieved.
Significant reduction in data rates.
Abstract
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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