GRB jet structure and the jet break

Author:

Lamb Gavin P1ORCID,Kann D Alexander2,Fernández Joseph John3ORCID,Mandel Ilya456ORCID,Levan Andrew J7,Tanvir Nial R1

Affiliation:

1. School of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK

2. IAA-CSIC, Glorieta de la Astronomía, s/n, E-18008 Granada, Spain

3. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK

4. Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia

5. OzGrav, Australian Research Council Centre of Excellence for Gravitational Wave Discovery, Swinburne University of Technology PO Box 218, Hawthorn, VIC 3122, Australia

6. Institute of Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, UK

7. Department of Astrophysics, Radboud University, NL-6525 AJ Nijmegen, The Netherlands

Abstract

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. We fit model and observed afterglow light curves with a smoothly-broken power-law function with a free-parameter κ that describes the sharpness of the break. We find that the jet break is sharper (κ 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 0.1 ≲ κ ≲ 4.6, whereas profiles with a smooth-edged core have a narrower range of 0.1 ≲ κ ≲ 2.2 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, whereas for smooth-edged jets, κ is more strongly dependent on the size of θc. Using a sample of 20 GRBs, we find 9 candidate smooth-edged jet structures and 8 candidate sharp-edged jet structures, while the remaining 3 are consistent with either. The shape of the jet break, as measured by the sharpness parameter κ, 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.

Funder

STFC

Australian Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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