Simulation study on high energy cosmic electron detection by shower image

R. Xu, J. Chang, S. Torii, K. Kasahara, T. Tamura, K. Yoshida
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Abstract

Many projects have recently been carried out and proposed for observing high energy electrons since it is realized that cosmic ray electrons are very important when studying the dark matter particles and the acceleration mechanism of cosmic rays. An imaging calorimeter, BETS (Balloon-borne Electron Telescope with Scintillator fiber), has been developed for this purpose. Using pattern analysis of the shower development, the electrons can be selected from those primary cosmic ray proton events with flux heights one-tenth that of the electrons. The Monte-Carlo simulation is indispensable for the instrument design, the signal trigger and the data analysis. We present different shower simulation codes and compare the simulation results with the beam test and the flight data of BETS. We conclude that the code FLUKA2002 gives the most consistent results with the experimental data.
星雨图像高能宇宙电子探测的模拟研究
由于认识到宇宙射线电子在研究暗物质粒子和宇宙射线加速机制时的重要作用,近年来开展和提出了许多观测高能电子的项目。一种成像量热计,BETS(带有闪烁体纤维的气球载电子望远镜),已经为此目的而开发。利用星雨发展的模式分析,可以从通量高度为电子十分之一的初级宇宙射线质子事件中选择电子。在仪器设计、信号触发和数据分析中,蒙特卡罗仿真是必不可少的。提出了不同的阵雨模拟程序,并将模拟结果与光束试验和BETS的飞行数据进行了比较。我们得出结论,FLUKA2002代码给出了与实验数据最一致的结果。
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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