Neural networks for TeV cosmic electrons identification on the DAMPE experiment

D. Droz, A. Tykhonov, Xin Wu, M. Deliyergiyev
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Abstract

The past decades have witnessed the deployment of a new generation of cosmic ray (CR) observatories with unprecedented sensitivity and complexity, pushing towards ever-higher energies. To face the challenges of the multi-TeV domain, such instruments must be accompanied by equally powerful analysis techniques, able to exploit as much information as available. For example, the machine learning tool set may provide the needed techniques. We present a neural network optimised for the identification of multi-TeV electrons on DAMPE, a calorimetric spaceborne CR observatory with among other objectives the measurement of cosmic electrons up to 10 TeV. This constitutes a particularly challenging endeavour due to both the soft electron spectrum and the large proton background. The developed neural network significantly outperforms the more traditional cut-based approach, achieving a much lower proton contamination in the multi-TeV domain with a high signal efficiency, and retains its accuracy when transposed from Monte Carlo to real data.
DAMPE实验中TeV宇宙电子识别的神经网络
过去几十年见证了新一代宇宙射线(CR)观测站的部署,它们具有前所未有的灵敏度和复杂性,朝着更高的能量发展。为了面对多tev领域的挑战,这些仪器必须配备同样强大的分析技术,能够利用尽可能多的信息。例如,机器学习工具集可以提供所需的技术。我们提出了一个优化的神经网络,用于识别DAMPE上的多TeV电子,DAMPE是一个量热星载CR天文台,其目标之一是测量高达10 TeV的宇宙电子。由于软电子谱和大质子背景,这构成了一个特别具有挑战性的努力。开发的神经网络显著优于传统的基于切割的方法,在多tev域中实现了更低的质子污染,具有高信号效率,并且在从蒙特卡罗转换到实际数据时保持其准确性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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