Detector Simulation Studies for the proposed Gamma-Ray and AntiMatter Survey (GRAMS)

Mihir Shetty
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Abstract

GRAMS is a proposed balloon and satellite-borne gamma ray and antimatter detector aimed at exploring the MeV energy bandgap as well as indirectly detecting dark matter. This study addresses the MeV detection capabilities of GRAMS via truth-level GEANT4 simulations, as a function of detector geometry and response. In particular, we examine Compton scattering as the vehicle for point source detection. As a first study, we applied the simple backprojection algorithm of Compton cameras to accurately reconstruct point source location and energy and examined the all-sky angular resolution of GRAMS, using truth-level detector information. We also calculated the point source sensitivity against a power-law isotropic background spectrum as observed by COMPTEL
伽玛射线和反物质巡天(GRAMS)探测器模拟研究
GRAMS是一种气球和卫星携带的伽马射线和反物质探测器,旨在探索MeV能量带隙以及间接探测暗物质。本研究通过真值级GEANT4模拟解决了GRAMS的MeV检测能力,作为探测器几何形状和响应的函数。特别地,我们研究了康普顿散射作为点源探测的载体。作为第一个研究,我们利用康普顿相机的简单反向投影算法精确地重建了点源位置和能量,并利用真值级探测器信息检查了GRAMS的全天角分辨率。我们还计算了在COMPTEL观测到的幂律各向同性背景光谱下的点源灵敏度
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