2023MNRAS.518.1522D

Studies of gamma-ray bursts (GRBs) and their multiwavelength afterglows have led to insights in electron acceleration and emission properties from relativistic, high-energy astrophysical sources. Broad-band modelling across the electromagnetic spectrum has been the primary means of investigating the physics behind these sources, although independent diagnostic tools have been developed to inform and corroborate assumptions made in particle acceleration simulations and broad-band studies. We present a methodology to constrain three physical parameters related to electron acceleration in GRB blast waves: the fraction of shock energy in electrons, ϵ_e; the fraction of electrons that gets accelerated into a power-law distribution of energies, ξ_e; and the minimum Lorentz factor of the accelerated electrons, γ_m. These parameters are constrained by observations of the peaks in radio afterglow light curves and spectral energy distributions. From a sample of 49 radio afterglows, we are able to find narrow distributions for these parameters, hinting at possible universality of the blast wave microphysics, although observational bias could play a role in this. Using radio peaks and considerations related to the prompt gamma-ray emission efficiency, we constrain the allowed parameter ranges for both ϵ_e and ξ_e to within about one order of magnitude, 0.01 ≲ ϵ_e ≲ 0.2 and 0.1 ≲ ξ_e ≲ 1. Such stringent constraints are inaccessible for ξ_e from broad-band studies due to model degeneracies.