宇宙粒子、中微子和外来物质的探测器

H. Kolanoski, N. Wermes
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引用次数: 0

摘要

天体粒子物理学使用与粒子物理学类似的探测方法来研究宇宙辐射,然而,大多数情况下使用的是完全不同的探测器布置。在本章中,介绍了不同类型的宇宙起源辐射的探测原理,包括带电粒子、伽马辐射、中微子和可能存在的暗物质。就中微子而言,也包括在加速器和反应堆上的实验。给出了探测器及其性质的典型例子,这些例子适用于不同的领域。宇宙射线探测设备是用气球或卫星部署在大气层之上,或在地面上使用大气作为量热计,高能宇宙射线在其中形成阵雨,或在地下地区,包括水和冰中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Detectors for cosmic particles, neutrinos and exotic matter
Astroparticle physics deals with the investigation of cosmic radiation using similar detection methods as in particle physics, however, mostly with quite different detector arrangements. In this chapter the detection principles for the different radiation types with cosmic origin are presented, this includes charged particles, gamma radiation, neutrinos and possibly existing Dark Matter. In the case of neutrinos also experiments at accelerators and reactors are included. Examples, which are typical for the different areas, are given for detectors and their properties. For cosmic ray detection apparatuses are deployed above the atmosphere with balloons or satellites or on the ground using the atmosphere as calorimeter in which high-energy cosmic rays develop showers or in underground areas including in water and ice.
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