Abstract
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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 477-506 |
| Number of pages | 30 |
| Journal | Annual Review of Nuclear and Particle Science |
| Volume | 69 |
| DOIs | |
| State | Published - 2019 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
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