基于机器学习的轻暗物质探测锗探测器块体和表面事件分辨技术

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
P. Zhang , H. Ma , L. Yang , Z. Zeng , Q. Yue , J. Cheng
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引用次数: 0

摘要

在使用 p 型点接触锗探测器进行的光暗物质探测实验中,表现出电荷收集不完全的表面事件是一个重要的背景源。我们提出了一种基于机器学习的算法,可根据脉冲形状特征识别体事件和表面事件。我们利用部分 γ 源校准数据构建训练集和测试集,并将波形的上升沿作为模型输入。我们使用测试集和另一部分 γ 源校准数据对该方法进行了验证。结果表明,该方法在两个数据集上都有良好的表现,并对大量事件的比例和数据集的大小具有鲁棒性。与之前的方法相比,CDEX-1B 物理数据在能量阈值附近的不确定性降低了 16%。此外,通过挖掘该算法,还验证了在波形中识别出的关键模式与其物理本质是一致的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Machine learning-based discrimination of bulk and surface events of germanium detectors for light dark matter detection

Surface events that exhibit incomplete charge collection are an essential background source in the light dark matter detection experiments with p-type point-contact germanium detectors. We propose a machine learning-based algorithm to identify bulk and surface events according to their pulse shape features. We construct the training and test set with part of the γ-source calibration data and use the rising edge of the waveform as the model input. This method is verified with the test set and another part of the γ-source calibration data. Results show that this method performs well on both datasets, and presents robustness against the bulk events’ proportion and the dataset size. Compared with the previous approach, the uncertainty is reduced by 16% near the energy threshold on the physics data of CDEX-1B. In addition, the key pattern identified in the waveform is verified to be consistent with its physical nature by digging into this algorithm.

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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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