Computer Science – Sound
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1065..223b&link_type=abstract
2008 NANJING GAMMA-RAY BURST CONFERENCE. AIP Conference Proceedings, Volume 1065, pp. 223-226 (2008).
Computer Science
Sound
4
Gamma-Ray Sources, Gamma-Ray Bursts, Space-Based Ultraviolet, Optical, And Infrared Telescopes, Macrosonic Propagation, Finite Amplitude Sound, Shock Waves, Supernovae
Scientific paper
The Swift observation of GRB 060614, as well as the catalog analysis by Norris and Bonnell [1], opened the door ``on a new Gamma-Ray Bursts (GRBs) classification scheme that straddles both long and short bursts'' [2]. Within the ``fireshell'' model for the Gamma-Ray Bursts (GRBs) 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 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 also outline some implications for the theoretical interpretation of the Amati relation.
Bianco Carlo Luciano
Caito Letizia
Giovanna Dainotti Maria
Grazia Bernardini Maria
Guida Roberto
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