Chapter 4 Cosmic-ray Physics
Chapter 4 Cosmic-ray Physics
复制标题
第四章宇宙射线物理
DOI：
10.1088/1674-1137/ac3faa
复制
发表时间：
2021
影响因子：
3.6
通讯作者：
D. Della Volpe
中科院分区：
文献类型：
--
作者：
B. D’Ettorre Piazzoli;Siming Liu;D. Della Volpe
在本章的第一部分中，概述了从1013 eV和1020 eV之间的宇宙射线观测中获得的知识的现状。这并不是一个完整的审查，而是一个涉及宇宙射线的相关过程，包括它们发生的天体物理环境的广泛概述。本概述主要涉及实验结果及其解释的现象学方面，因此没有给出实验描述，但在文本中提供了大量参考书目的参考。一些尝试，以解决最流行的理论模型提供的解释。第二部分是专门描述的LHAASO的性能和它的能力，以提供一个回答几个悬而未决的问题，仍然没有答案，关于宇宙射线以上1013 eV，突出了在这一领域的主要步骤，可以采取从LHAASO的观测。
In the first part of this Chapter the present state of knowledge from the observations of cosmic rays between 1013 eV and 1020 eV is summarized. This is not intended to be a complete review, but rather a broad overview of the relevant processes involving cosmic rays, including the astrophysical environments in which they take place. This overview mainly concerns experimental results and phenomenological aspects of their interpretation, therefore experiments’ description is not given but references to the vast bibliography are provided in the text. Some attempt is made to address the most popular explanations offered by theoretical models. The second part is devoted to the description of the LHAASO performance and of its capability to provide a response to several open questions, still unanswered, concerning cosmic rays above 1013 eV, highlighting which major steps forward in this field could be taken from LHAASO observations.