English

GRB jet structure and the jet break

High Energy Astrophysical Phenomena 2021-08-12 v2

Abstract

We investigate the shape of the jet break in within-beam gamma-ray burst (GRB) optical afterglows for various lateral jet structure profiles. We consider cases with and without lateral spreading and a range of inclinations within the jet core half-opening angle, θc\theta_c. We fit model and observed afterglow lightcurves with a smoothly-broken power-law function with a free-parameter κ\kappa that describes the sharpness of the break. We find that the jet break is sharper (κ\kappa is greater) when lateral spreading is included than in the absence of lateral spreading. For profiles with a sharp-edged core, the sharpness parameter has a broad range of 0.1κ4.60.1\lesssim\kappa\lesssim4.6, whereas profiles with a smooth-edged core have a narrower range of 0.1κ2.20.1\lesssim\kappa\lesssim2.2 when models both with and without lateral spreading are included. For sharp-edged jets, the jet break sharpness depends strongly on the inclination of the system within θc\theta_c, whereas for smooth-edged jets, κ\kappa is more strongly dependent on the size of θc\theta_c. Using a sample of 20 GRBs we find nine candidate smooth-edged jet structures and eight candidate sharp-edged jet structures, while the remaining three are consistent with either. The shape of the jet break, as measured by the sharpness parameter κ\kappa, can be used as an initial check for the presence of lateral structure in within-beam GRBs where the afterglow is well-sampled at and around the jet-break time.

Keywords

Cite

@article{arxiv.2104.11099,
  title  = {GRB jet structure and the jet break},
  author = {Gavin P Lamb and D. Alexander Kann and Joseph John Fernández and Ilya Mandel and Andrew J. Levan and Nial R. Tanvir},
  journal= {arXiv preprint arXiv:2104.11099},
  year   = {2021}
}

Comments

13 pages, 5 figures, accepted for publication in MNRAS 15/07/21

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