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High-Energy Multimessenger Transient Astrophysics
- Kohta Murase1,2, and Imre Bartos3
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View Affiliations Hide AffiliationsAffiliations: 1Department of Physics, Department of Astronomy and Astrophysics, and Center for Particle and Gravitational Astrophysics, Institute for Gravitation and the Cosmos, Pennsylvania State University, University Park, Pennsylvania 16802, USA; email: [email protected] 2Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan 3Department of Physics, University of Florida, Gainesville, Florida 32611, USA; email: [email protected]
- Vol. 69:477-506 (Volume publication date October 2019) https://doi.org/10.1146/annurev-nucl-101918-023510
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Copyright © 2019 by Annual Reviews. All rights reserved
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.
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2019-10-19
2024-04-24
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/content/journals/10.1146/annurev-nucl-101918-023510
High-Energy Multimessenger Transient Astrophysics
Annual Review of Nuclear and Particle Science 69, 477 (2019); https://doi.org/10.1146/annurev-nucl-101918-023510
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