PeV-ZeV 宇宙射线源的多信使特征
高能天体物理现象
2019-01-23 v2
摘要
我们讨论了 eV 范围内宇宙射线的可能来源，以及其可能产生的极高能中微子和伽马射线特征，这些特征可用于识别这些源并约束其物理。在这些源中，我们特别讨论了低光度伽马射线暴，包括噎爆和激波突破天体、潮汐瓦解事件以及白矮星并合。在旨在同时进行次级多信使探测的努力中，我们讨论了 AMON 计划。
引用
@article{arxiv.1703.00890,
title = {Multi-Messenger Signatures of PeV-ZeV Cosmic Ray Sources},
author = {Peter Mészáros and Kohta Murase and Katsuaki Asano and Nicholas Senno and Di Xiao},
journal= {arXiv preprint arXiv:1703.00890},
year = {2019}
}
备注
9 pages; Based on a talk given at the Origin of Cosmic Rays: Beyond the Standard Model 2016 conference in San Vito di Cadore, Dolomites; This is not a comprehensive review; it is weighted towards work the author has been more personally involved with. Fig 3 has been updated to reflect the published work