Within 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 here present the consequences of such a scenario on the theoretical interpretation of the nature of "long" and "short" GRBs. © 2008 World Scientific Publishing Co. Pte. Ltd.
Theoretical Interpretation of "long" and "short" GRBs / BERNRDINI M., G; Caito, L; Chardonnet, P; DAINOTTI M., G; Fraschetti, F; Guida, R; Ruffini, Remo; Xue, S. S.; Bianco, Carlo Luciano. - C:(2008), pp. 1974-1977. (Intervento presentato al convegno Proceedings of the Eleventh Marcel Grossmann Meeting tenutosi a Berlin; Germany nel 23-29 July 2006) [10.1142/9789812834300_0302].
Theoretical Interpretation of "long" and "short" GRBs
RUFFINI, Remo;BIANCO, Carlo Luciano
2008
Abstract
Within 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 here present the consequences of such a scenario on the theoretical interpretation of the nature of "long" and "short" GRBs. © 2008 World Scientific Publishing Co. Pte. Ltd.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
