High-Energy Multi-Messenger Transient Astrophysics

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.

arXiv comment36 pages, 8 figures, invited review article accepted for publication in ARNPS

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• Post-Merger Jets from Supermassive Black Hole Coalescences as Electromagnetic Counterparts of Gravitational Wave Emission
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• High-energy neutrino signatures from pulsar remnants of binary neutron-star mergers: coincident detection prospects with gravitational waves
• New results on the gamma-ray burst variability-luminosity relation
• Optimal Gravitational-wave Follow-up Tiling Strategies Using a Genetic Algorithm
• All-Sky Search for Transient Astrophysical Neutrino Emission with 10 Years of IceCube Cascade Events
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• Strong Lensing of High-Energy Neutrinos
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• Time-integrated constraint on neutrino flux of CHIME fast radio burst sources with 10-year IceCube point-source data
• Neutrino emission from FRB-emitting magnetars
• Transient electromagnetic sources can detect solitary black holes in Milky Way galaxy
• Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
• On the Spectral Changes of OJ 287: The Lowest X-ray state Spectrum -- extended at Optical-UV and Hard at X-rays