Theory of off-axis and gravitational wave events
Hendrik Jan van Eerten

TL;DR
This paper discusses the complex electromagnetic counterparts of GW170817, focusing on off-axis gamma-ray bursts, jet dynamics, and recent developments in multi-messenger astrophysics following the event.
Contribution
It provides a summary of recent theoretical and observational insights into off-axis gamma-ray bursts and jet emissions related to gravitational wave events.
Findings
Off-axis gamma-ray bursts exhibit diverse emission signatures.
Jet success and failure impact electromagnetic counterparts.
Recent literature advances understanding of multi-messenger signals.
Abstract
GW170817 was not merely an absolute breakthrough in gravitational wave astrophysics and a first in multi-messenger astronomy. The quality and diversity of the electro-magnetic counterpart emission is staggering on its own as well, including unprecedented kilonova spectra and a broadband off-axis gamma-ray burst afterglow that has progressed along a trajectory of rise and decay and by now has even been measured using very large baseline interferometry. For these proceedings, I will summarize the points for discussion that I presented during the workshop regarding off-axis short gamma-ray bursts and their (un-)successful jets and their emission. Given that developments are currently moving very fast in the field, I also touch on some results that have appeared in the literature following the Vulcano meeting.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations
