Development of a Measuring Method of Cosmic-Ray Muon Momentum Distribution Using Drift Chambers

Pub Date : 2024-04-22 DOI:10.14407/jrpr.2023.00423
Naoto Nakagami, Satoko Kamei, Shoichiro Kawase, Akira Sato, Yukinobu Watanabe
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Abstract

Background: Soft errors in semiconductor devices caused by cosmic rays have been recognized as a significant threat to the reliability of electronic devices on the ground. Recently, concerns about soft errors induced by cosmic-ray muons have increased. Some previous studies have indicated that low-energy negative muons have a more significant contribution to the occurrence of soft errors than positive muons. Thus, charge-identified low-energy muon flux data on the ground are required for accurate evaluation of the soft error rate. However, there are no such experimental data in the low-energy region. Materials and Methods: We designed a new muon detector system to measure low-energy muon flux data with charge identification. The major components consist of two drift chambers and a permanent magnet. The charge and momentum of detected muon can be identified from the deflection of the muon trajectory in the magnetic field. An algorithm to estimate the muon momentum is developed using numerical optimization by combining the classical Runge-Kutta and quasi-Newton methods. The momentum search algorithm is applied to event-by-event data of positive and negative muons obtained by Monte Carlo simulations with Particle and Heavy Ion Transport code System, and its performance is examined. Results and Discussion: The momentum search algorithm is fully applicable even in the case of an inhomogeneous magnetic field. The precision of the momentum determination is evaluated by considering the stochastic fluctuation caused by multiple scattering and the position resolution of the drift chambers. It was found that multiple scattering has a significant contribution to the precision in the momentum region below 50 MeV/c, while the detector position resolution considerably affects the precision above that. Conclusion: It was confirmed that the momentum search algorithm works well with a sufficient precision of 15% in the low-momentum region below 100 MeV/c, where no muon flux data exist.
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利用漂移室开发宇宙射线μ介子动量分布测量方法
背景:宇宙射线在半导体器件中引起的软误差已被认为是对地面电子器件可靠性的重大威胁。最近,人们对宇宙射线μ介子引起的软误差的关注有所增加。之前的一些研究表明,与正μ介子相比,低能负μ介子对发生软误差的影响更大。因此,需要地面上电荷识别的低能μ介子通量数据来准确评估软误差率。然而,在低能区还没有这样的实验数据。材料和方法:我们设计了一个新的μ介子探测器系统,用于测量带电荷识别的低能μ介子通量数据。主要部件包括两个漂移室和一块永磁体。探测到的μ介子的电荷和动量可以通过μ介子在磁场中的轨迹偏转来识别。通过结合经典的 Runge-Kutta 和准牛顿方法,利用数值优化开发了一种估算μ介子动量的算法。将该动量搜索算法应用于利用粒子和重离子输运代码系统进行蒙特卡罗模拟所获得的正负μ介子的逐次事件数据,并对其性能进行了检验。结果与讨论:即使在磁场不均匀的情况下,动量搜索算法也完全适用。通过考虑多重散射引起的随机波动和漂移室的位置分辨率,对动量确定的精度进行了评估。结果发现,在低于 50 MeV/c 的动量区域,多重散射对精确度的影响很大,而探测器的位置分辨率则对高于该值的精确度有很大影响。结论:在没有μ介子通量数据的 100 MeV/c 以下低动量区,动量搜索算法运行良好,精度达到 15%。
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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