High-energy neutrinos in the context of multimessenger astrophysics
High-energy neutrinos in the context of multimessenger astrophysics
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DOI：
10.1016/j.physrep.2007.10.006
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发表时间：
2007-10
期刊：
影响因子：
--
通讯作者：
J. Becker
中科院分区：
文献类型：
--
作者：
J. Becker
天体粒子物理学领域目前正在迅速发展，因为新的实验挑战了我们对已经研究过的过程的理解。三种信使可以用来提取天体物理源的属性信息：光子，带电宇宙射线和中微子。本文对高能中微子（Eν>100GeV）的研究进行了综述。
The field of astroparticle physics is currently developing rapidly, since new experiments challenge our understanding of processes that have been investigated. Three messengers can be used to extract information on the properties of astrophysical sources: photons, charged Cosmic Rays and neutrinos. This review focuses on high-energy neutrinos (Eν>100GeV) with the main topics as follows.