The "fireshell" model and the "canonical" GRB scenario

Details The "fireshell" model and the "canonical" GRB scenario The "fireshell" model and the "canonical" GRB scenario

2007-12-04

arxiv.org/abs/0712.0495v1

AIPConf.Proc.966:12-15,2007

Astronomy and Astrophysics

Astrophysics

4 pages, 5 figures, in the Proceedings of the "4th Italian-Sino Workshop on Relativistic Astrophysics", held in Pescara, Italy

Scientific paper

10.1063/1.2836983

In the "fireshell" model we define a "canonical GRB" light curve with two sharply different components: the Proper-GRB (P-GRB), emitted when the optically thick fireshell of electron-positron plasma originating the phenomenon reaches transparency, and the afterglow, emitted due to the collision between the remaining optically thin fireshell and the CircumBurst Medium (CBM). We outline our "canonical GRB" scenario, originating from the gravitational collapse to a black hole, with a special emphasis on the discrimination between "genuine" and "fake" short GRBs.

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