Very High-Energy GRB Afterglow Fits with Neural-Network Emulation and Bayesian inference

Edilberto Aguilar-Ruiz, Jessica Saldívar Talavera, Ramandeep Gill +1

The very high-energy ($E>100$ GeV) afterglow emission in gamma-ray bursts (GRBs) can be explained by synchrotron self-Compton (SSC). Modeling this emission accurately requires fu…