Within the fireshell model, Gamma Ray Bursts (GRBs) originate from an optically thick e plasma created by vacuum polarization process during the formation of a Black Hole (BH). Here we briefly recall the basic features of this model, then we show how it is possible to interpret GRB observational properties within it. In particular we present, as a specific example, the analysis of GRB 050904 observations of the prompt emission light curve and spectrum in the Swift BAT energy band (15-150 keV).
Black Holes in Gamma Ray Bursts / Patricelli, Barbara; Bernardini, MARIA GRAZIA; Bianco, Carlo Luciano; Caito, Letizia; DE BARROS, Gustavo; Izzo, Luca; Ruffini, Remo. - In: AIP CONFERENCE PROCEEDINGS. - ISSN 0094-243X. - STAMPA. - 1279:(2010), pp. 406-408. (Intervento presentato al convegno International Symposium Deciphering the Ancient Universe with Gamma-Ray Bursts tenutosi a Kyoto, JAPAN nel APR 19-23, 2010) [10.1063/1.3509327].
Black Holes in Gamma Ray Bursts
PATRICELLI, BARBARA;BERNARDINI, MARIA GRAZIA;BIANCO, Carlo Luciano;CAITO, LETIZIA;DE BARROS, GUSTAVO;IZZO, LUCA;RUFFINI, Remo
2010
Abstract
Within the fireshell model, Gamma Ray Bursts (GRBs) originate from an optically thick e plasma created by vacuum polarization process during the formation of a Black Hole (BH). Here we briefly recall the basic features of this model, then we show how it is possible to interpret GRB observational properties within it. In particular we present, as a specific example, the analysis of GRB 050904 observations of the prompt emission light curve and spectrum in the Swift BAT energy band (15-150 keV).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
