Using the Swift data of GRB 050315, we progress in proving the uniqueness of our theoretically predicted Gamma-Ray Burst (GRB) structure as composed by a proper-GRB, emitted at the transparency of an electron-positron plasma with suitable baryon loading, and an afterglow comprising the "prompt radiation" as due to external shocks. Detailed light curves for selected energy bands are theoretically fitted in the entire temporal region of the Swift observations ranging over 106 seconds. © 2006 American Institute of Physics.
GRB 050315: A step in the proof of the uniqueness of the overall GRB structure / Ruffini, Remo; BERNARDINI M., G; Chardonnet, P; Fraschetti, F; Guida, R; Xue, S. S.; Bianco, Carlo Luciano. - In: AIP CONFERENCE PROCEEDINGS. - ISSN 0094-243X. - 836:(2006), pp. 103-108. (Intervento presentato al convegno Gamma-Ray Bursts in the Swift Era - 16th Maryland Astrophysics Conference tenutosi a Washington; United States nel November 29-December 2, 2005) [10.1063/1.2207866].
GRB 050315: A step in the proof of the uniqueness of the overall GRB structure
RUFFINI, Remo;BIANCO, Carlo Luciano
2006
Abstract
Using the Swift data of GRB 050315, we progress in proving the uniqueness of our theoretically predicted Gamma-Ray Burst (GRB) structure as composed by a proper-GRB, emitted at the transparency of an electron-positron plasma with suitable baryon loading, and an afterglow comprising the "prompt radiation" as due to external shocks. Detailed light curves for selected energy bands are theoretically fitted in the entire temporal region of the Swift observations ranging over 106 seconds. © 2006 American Institute of Physics.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
