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Global optimization for light concentrators of a Geiger-mode cosmic-ray Cherenkov calorimeter

机译:盖革模式宇宙射线切伦科夫量热仪光聚光器的全局优化

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Light concentrators are crucial devices for photon-counting instruments, the optical characteristics of which affect the photoelectric response for the sensors. The designs that only aim to the light transmission have been proved far from optimum for the Geiger-mode calorimeters due to the significant influence from the angle-dependent reflectance, versatile light trajectories, and saturation of fired avalanche photodiodes (APD5). In this paper, we took into account these coupling effects, presented a novel approach to solve the problems in global optimization for light concentrators in combination with silicon photomultiplier (SiPM). In addition, a new probability method is studied and used to restore the photon counting for precise reconstruction of cosmic-ray air showers. The Monte-Carlo experiment verified that the new system design features a high accurate energy scaling for cosmic-ray measurement. The results also indicate that the precision is able to be improved by at least one order in magnitude. (C) 2021 Optical Society of America under the terms of the OSA Open Access Publishing Agreement
机译:光聚光器是光子计数仪器的关键设备,其光学特性会影响传感器的光电响应。由于角度相关反射率、多功能光轨迹和发射雪崩光电二极管 (APD5) 饱和度的显着影响,仅针对透光率的设计已被证明远非盖革模式量热仪的最佳设计。本文考虑了这些耦合效应,提出了一种新的方法来解决硅光电倍增管(SiPM)组合的光聚光器全局优化问题。此外,还研究了一种新的概率方法,用于恢复光子计数,以精确重建宇宙射线空气阵雨。蒙特卡洛实验验证了新系统设计具有用于宇宙射线测量的高精度能量缩放。结果还表明,精度能够提高至少一个数量级。(C) 2021 年美国光学学会根据 OSA 开放获取出版协议的条款

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