DEASA在空间物理和介子断层扫描中的研究和应用

Sonali Bhatnagar
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引用次数: 0

摘要

进入地球大气层的高能宇宙射线揭示了天体粒子和粒子物理学的许多方面。这项工作概述了基于印度阿格拉的小型阵列DEASA对这些高能初级的调查学习。DEASA (Dayalbagh教育风淋阵列)由八个塑料闪烁体组成,每个闪烁体的面积为1平方米。该天线阵占地260平方米,是我国北部地区的首个天线阵。这些高能粒子的一个现实应用是找到最好的材料来保护宇航员免受银河宇宙射线(GCR)的伤害。采用基于Geant4的强子二元模型对幻影、车辆、太阳高能粒子(SEP)和GCR屏蔽层进行了仿真。SEP屏蔽材料固定为水,GCR屏蔽材料有铝、聚苯乙烯和聚乙烯三种。由于含有大量的氢(H)和较低的原子序数(Z),聚乙烯材料被发现是最好的。在这项工作中,与其他材料相比,聚苯乙烯材料沉积在GCR屏蔽体中的等效剂量最小(107西弗)。在第二个应用中,研究了高能μ子通过μ子层析成像核盒。在蒙特卡罗模拟中,用一定能量的μ子轰击装有不同数量的UO2棒的干桶容器,测量了μ子的散射,计算出了能量损失、辐射长度和散射角等参数,可以对这些容器进行校准,以正确识别核废物。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
DEASA studies and applications to space physics and muon tomography
The high energy cosmic rays entering the Earth’s atmosphere throw light upon many aspects of Astroparticle and Particle Physics. This work outlines investigative learning about these high energy primaries based on a mini array DEASA in Agra,India. DEASA (Dayalbagh Educational Air Shower Array) consists of eight plastic scintillators each with an area of 1 square meter. This array covers an area of 260 square meters and is the first array in the northern part of our country. A real-life application of these highly energetic particles has been to find the best material to protect the astronaut from them in form of galactic cosmic rays (GCR). Geant4 based hadronic binary model was used in simulation of phantom, vehicle, SEP (Solar Energetic Particles) and GCR shield. The SEP shielding material was fixed as water and GCR shield was varied among aluminum, Polystyrene and Polyethylene. The poly materials were found to be the best due to large amount of hydrogen (H) and low atomic number (Z). In this work the equivalent dose deposited in the phantom with Polystyrene material for GCR shield was calculated to be minimum (107 sievert) as compared to the other materials.In the second application, the high energy muons have been studied to image nuclear caskets through muon tomography.In this Monte Carlo based simulation, a dry cask container containing different number of the UO2 rods have been bombarded with definite energy muons to measure the muon scattering .The parameters computed in this work are energy loss,radiation length and scattering angle which can calibrate these containers for correct identification of nuclear wastage.
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