论文标题
稀疏能量对在广泛的空气阵雨中产生的带电颗粒的波动的变化
Thinning Energy Effect on the Fluctuations of Charged Particles Lateral Distribution Produced in Extensive Air Showers
论文作者
论文摘要
在这项工作中，通过在各种宇宙射线颗粒的极高能量下估算横向分布函数（LDF）来描述广泛的空气淋浴（EAS）的影响。模拟了LDF的电荷颗粒，例如电子和正电子对的产生，γ，MUON和所有带电的颗粒在非常高的能量10^16、10^18和10^19 eV上。使用空气淋浴模拟器系统（AIRES）2.6.0进行了模拟。考虑了EAS中产生的带电的LDF颗粒的主要颗粒，能量，变薄的能量和天顶角的影响。比较带电颗粒的估计的LDF，例如电子和正电子对的产生，以及Sciutto的模拟结果和Yakutsk EAS天文台的实验结果的比较，在0和10 Zenith Angles的能量10^19 eV上进行了良好的接受。
In this work, the effects of the extensive air showers (EAS) were described by estimating the lateral distribution function (LDF) at very high energies of various cosmic ray particles. LDF was simulated for charged particles such as the electron and positron pair production, gamma, muons and all charged particles at very high energies 10^16, 10^18 and 10^19 eV. The simulation was performed using air shower simulator system (AIRES) version 2.6.0. The effect of primary particles, energies, thinning energy and zenith angle on the charged LDF particles produced in the EAS was taken into account. The comparison of the estimated LDF of charged particles such as the electron and positron pair production and muons with the simulated results by Sciutto and experimental results by Yakutsk EAS observatory gives a good acceptance at the energy 10^19 eV for 0 and 10 zenith angles.
