What determines the structure of short gamma-ray burst jets?

TL;DR

This study uses numerical simulations to explore how the initial structure, luminosity, and duration of short gamma-ray burst jets influence their final structure and observable afterglow emissions, especially in off-axis scenarios like GRB 170817A.

Contribution

It demonstrates that the initial jet structure significantly affects the final jet configuration and afterglow, emphasizing the need for combined simulation and propagation studies.

Findings

Final jet structure depends on initial conditions and environment.

Long-lasting jets preserve initial structure; short jets are strongly modified.

Structured jets can explain GRB 170817A afterglow observations.

Abstract

The discovery of GRB 170817A, the first unambiguous off-axis short gamma-ray burst arising from a neutron star merger, has challenged our understanding of the angular structure of relativistic jets. Studies of the jet propagation usually assume that the jet is ejected from the central engine with a top-hat structure and its final structure, which determines the observed light curve and spectra, is primarily regulated by the interaction with the nearby environment. However, jets are expected to be produced with a structure that is more complex than a simple top-hat, as shown by global accretion simulations. We present numerical simulations of short GRBs launched with a wide range of initial structures, durations and luminosities. We follow the jet interaction with the merger remnant wind and compute its final structure at distances $\gtrsim 10^{11}$~cm from the central engine. We show that the final jet structure, as well as the resulting afterglow emission, depend strongly on the initial structure of the jet, its luminosity and duration. While the initial structure at the jet is preserved for long-lasting SGRBs, it is strongly modified for jets barely making their way through the wind. This illustrates the importance of combining the results of global simulations with propagation studies in order to better predict the expected afterglow signatures from neutron star mergers. Structured jets provide a reasonable description of the GRB 170817A afterglow emission with an off-axis angle $\theta_{\rm obs} \approx 22.5^\circ$.