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

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dc.creatorBianco, Carlo Luciano
dc.creatorBernardini, Maria Grazia
dc.creatorCaito, Letizia
dc.creatorDainotti, Maria Giovanna
dc.creatorGuida, Roberto
dc.creatorRuffini, Remo
dc.date2007-12-04
dc.date.accessioned2026-07-07T11:13:32Z
dc.date.available2026-07-07T11:13:32Z
dc.descriptionIn 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.
dc.description4 pages, 5 figures, in the Proceedings of the "4th Italian-Sino Workshop on Relativistic Astrophysics", held in Pescara, Italy, July 20-28, 2007, C.L. Bianco, S.-S. Xue, Editors
dc.identifierhttps://arxiv.org/abs/0712.0495
dc.identifierhttp://arxiv.org/abs/0712.0495
dc.identifierAIPConf.Proc.966:12-15,2007
dc.identifierdoi:10.1063/1.2836983
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191755
dc.subjectAstrophysics
dc.titleThe "fireshell" model and the "canonical" GRB scenario
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