Polarization Predictions in the GRB Prompt Phase with the Internal Shock Model

no code implementations • 4 Mar 2021 • Mi-Xiang Lan, Hao-Bing Wang, Siyao Xu, Siming Liu, Xue-Feng Wu

Therefore, we conclude that the energy dependence of PD can be used to distinguish these two models for the GRB prompt emission.

High Energy Astrophysical Phenomena