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Do Afterglow Synchrotron Radiations Follow the L<sub>p,iso</sub>–E<sub>p,z</sub>–Γ<sub>0</sub> Relation of Gamma-Ray Bursts? The Cases of GRBs 190114C, 130427A, and 180720B
Bimodal spectral energy distributions (SEDs) of gamma-ray burst (GRB) afterglow of GRBs 190114C, 130427A and 180720B confirm that they are originated from the synchrotron emission (Syn) and synchrotron self-Compton Scattering process (SSC) of electrons accelerated in the jets. The radiation mechanism and the physics of the observed spectrum-luminosity/energy relations of …