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Deep Learning-Based $^{14}$C Pile-Up Identification in the JUNO Experiment

High Energy Physics - Experiment 2026-03-03 v1

Abstract

Measuring neutrino mass ordering (NMO) poses a fundamental challenge in neutrino physics. To address this, the Jiangmen Underground Neutrino Observatory (JUNO) experiment is scheduled to commence data collection in late 2024, with the ambitious goal of determining the NMO at a 3-sigma confidence level within a span of 6 years. A key factor in achieving this is ensuring a high-quality energy resolution of positrons. However, the presence of residual 14^{14}C isotopes in the liquid scintillator introduces pile-up effects that can impact the positron energy resolution. Mitigating these pile-up effects requires the identification of pile-up events, which presents a significant challenge. The signal from 14^{14}C is considerably smaller compared to the positron signal, making its identification difficult. Additionally, the close event time and vertex between a positron and a 14^{14}C further compound the identification challenge. This contribution focuses on the application of deep learning models for the identification of 14^{14}C pile-up events. It encompasses a range of models, including convolution-based models and advanced transformer models. Through performance evaluation, it shows the deep learning-based methods is promising to identify the pile-up events.

Keywords

Cite

@article{arxiv.2603.01419,
  title  = {Deep Learning-Based $^{14}$C Pile-Up Identification in the JUNO Experiment},
  author = {Wenxing Fang and Weidong Li and Wuming Luo and Zhaoxiang Wu and Miao He},
  journal= {arXiv preprint arXiv:2603.01419},
  year   = {2026}
}

Comments

For ACAT2024 conference

R2 v1 2026-07-01T10:58:28.563Z