Nearby SN-Associated GRB~190829A: Environment, Jet Structure, and VHE Gamma-Ray Afterglows

Understand

We present a self-consistent paradigm for interpreting the striking features of nearby low-luminosity GRB~190829A.

• Its prompt gamma-ray lightcurve has two separated pulses.
• We propose that the interaction of the hard prompt gamma-ray photons ($E_p= 624_{-303}^{+2432}$ keV) of its initial pulse with the dusty medium ($A_{\rm V}=2.33$) does not only result in the second soft gamma-ray pulse ($E_p\sim 12$ keV), but also makes a pre-accelerated $e^{\pm}$-rich medium shell via the $\gamma\gamma$ annihilation.In this paradigm, we show that the observed radio, optical, and X-ray afterglow lightcurves are well fit with the forward shock model.
• Its jet is almost isotropic ($\theta_j>1.0$ rad) with a Lorentz factor of $\sim 35$, and the electron density of the $e^{\pm}$-rich medium shell is $\sim 15$ cm$^{-3}$, about 7~times higher than the electron density of its normal surrounding medium.