High-Energy Multi-Messenger Transient Astrophysics
arXiv:1907.12506 · doi:10.1146/annurev-nucl-101918-023510
Abstract
The recent discoveries of high-energy cosmic neutrinos and gravitational waves from astrophysical objects have led to the new era of multi-messenger astrophysics. In particular, electromagnetic follow-up observations triggered by these cosmic signals proved to be highly successful and brought about new opportunities in the time-domain astronomy. Here 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.
36 pages, 8 figures, invited review article accepted for publication in ARNPS
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