Afterglow light curves from misaligned structured jets. Issue 3 (25th February 2020)

• Record Type: Journal Article
• Authors: Beniamini, Paz; Granot, Jonathan; Gill, Ramandeep
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 493:Issue 3(2020)
• Page Start: 3521
• Page End: 3534
• Publication Date: 2020-02-25
• Subjects: radiation mechanisms: general -- gamma-ray burst: general; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa538
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: GRB 170817A/GW 170817 is the first gamma-ray burst (GRB) clearly viewed far from the GRB jet's symmetry axis. Its afterglow was densely monitored over a wide range of frequencies and times. It has been modelled extensively, primarily numerically, and although this endeavour was very fruitful, many of the underlying model parameters remain undetermined. We provide analytic modelling of GRB afterglows observed off-axis, considering jets with a narrow core (of half-opening angle θc ) and power-law wings in energy per unit solid angle (ϵ = ϵc Θ − a where Θ = [1 + (θ/θc ) 2 ] 1/2 ) and initial specific kinetic energy (Γ0 − 1 = [Γc, 0 − 1]Θ − b ), as well as briefly discuss Gaussian jets. Our study reveals qualitatively different types of light curves that can be viewed in future off-axis GRBs, with either single or double peaks, depending on the jet structure and the viewing angle. Considering the light-curve shape rather than the absolute normalizations of times and/or fluxes, removes the dependence of the light curve on many of the highly degenerate burst parameters. This study can be easily used to determine the underlying jet structure, significantly reduce the effective parameter space for numerical fitting attempts and provide physical insights. As an illustration, we show that for GRB 170817A, there is a strong correlation between the allowed values of Γc, 0 and b, leading to a narrow strip of allowed solutions in the Γc, 0 – b plane above some minimal values Γc, 0 ≳ 40, b ≳ 1.2. Furthermore, the Lorentz factor of the material dominating the early light curve can be constrained by three independent techniques to be Γ0 (θmin, 0 ) ≈ 5–7.