Design and Detection Mechanism for Gamma Rays and Antimatter Particles by a LArTPC Detector Towards Future GRAMS Mission

J. Leyva
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Abstract

The upcoming GRAMS (Gamma-Ray and AntiMatter Survey) experiment aims to provide unprecedented sensitivity to a poorly explored region of the cosmic gamma-ray spectrum from 0.1-100 MeV, often referred to as the “MeV gap”. In addition to gamma rays, the ability to detect cosmic antimatter makes GRAMS an excellent candidate for a nearly ‘background free’ indirect dark matter search. Utilizing Liquid Argon Time Projection Chamber (LArTPC) technology to detect MeV gamma rays and antimatter, GRAMS has the potential to uncover crucial details behind a variety of processes in multi-messenger astrophysics. In this poster session, the design and detection mechanism for a proof-of-concept detector called MicroGRAMS will be covered. This detector’s primary use is to evaluate the performance of the GRAMS charge and light collection systems and demonstrate the detection concept for gamma rays and antimatter particles.
面向未来gram任务的LArTPC探测器伽玛射线和反物质粒子的设计和探测机制
即将到来的GRAMS(伽马射线和反物质调查)实验旨在为0.1-100 MeV的宇宙伽马射线光谱区域提供前所未有的灵敏度,该区域通常被称为“MeV间隙”。除了伽马射线外,探测宇宙反物质的能力使gram成为几乎“无背景”的间接暗物质搜索的绝佳候选者。利用液态氩时间投影室(LArTPC)技术探测MeV伽马射线和反物质,GRAMS有可能揭示多信使天体物理学中各种过程背后的关键细节。在这个海报环节中,我们将介绍一种名为MicroGRAMS的概念验证探测器的设计和检测机制。该探测器的主要用途是评估GRAMS电荷和光收集系统的性能,并演示伽玛射线和反物质粒子的探测概念。
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