High-Energy Multimessenger Transient Astrophysics
High-Energy Multimessenger Transient Astrophysics
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DOI：
10.1146/annurev-nucl-101918-023510
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发表时间：
2019-07
影响因子：
12.4
通讯作者：
K. Murase;I. Bartos
中科院分区：
文献类型：
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作者：
K. Murase;I. Bartos
最近从天体物理对象中发现的高能宇宙中微子和引力波引领了一个多信使天体物理学的新时代。特别是由这些宇宙信号引发的电磁跟踪观测已经被证明是非常成功的，并为时域天文学带来了新的机遇。我们回顾了与黑洞和中子星相关的各种天体物理瞬态现象中高能粒子的产生，并讨论了如何利用高能发射来揭示中微子和引力波源的潜在物理特性。
The recent discoveries of high-energy cosmic neutrinos and gravitational waves from astrophysical objects have led to a new era of multimessenger astrophysics. In particular, electromagnetic follow-up observations triggered by these cosmic signals have proved to be highly successful and have brought about new opportunities in time-domain astronomy. We review high-energy particle production in various classes of astrophysical transient phenomena related to black holes and neutron stars, and discuss how high-energy emission can be used to reveal the underlying physics of neutrino and gravitational-wave sources.