The ``fireshell'' model and the ``canonical GRB'' scenario. Implications for the Amati relation

Details The ``fireshell'' model and the ``canonical GRB'' scenario. Implications for the Amati relation The ``fireshell'' model and the ``canonical GRB'' scenario. Implications for the Amati relation

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111..587b&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

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Supernova Remnants, Gamma-Ray Sources, Gamma-Ray Bursts, Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

Within the ``fireshell'' model for GRBs we define a ``canonical GRB'' light curve with two sharply different components: the Proper-GRB (P-GRB), emitted when the optically thick fireshell reaches transparency, and the extended afterglow, emitted due to the collision between the remaining optically thin fireshell and the CircumBurst Medium (CBM). We here outline our ``canonical GRB'' scenario, which implies three different GRB classes: the ``genuine'' short GRBs, the ``fake'' or ``disguised'' short GRBs and the other (so-called ``long'') GRBs. We will also outline the corresponding implications for the Amati relation, which are opening its use for cosmology.

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