by
Remo Ruffini(Rome University "La Sapienza" and ICRANet)
→
Europe/Stockholm
FA32
FA32
Description
The fireshell model studies GRBs within a consistent approach spanning from the original electron positron plasma formation to the reaching of transparency with the P-GRB emission and the prompt phases encompassing the peak of the extended afterglow. Such an approach allows to locate specific emission process with the thermal and the power law components in the observed spectra. The case of GRB 090618 and GRB 101023 will be discussed as prototypes.
