Shlomo Dado, Arnon Dar
Published 2013-03-12, updated 2013-08-23Version 3
The 'jet-break' in the X-ray afterglow of gamma ray bursts (GRBs) appears to be correlated to other properties of the X-ray afterglow and the prompt gamma ray emission, but the correlations are at odds with those predicted by the conical fireball model of GRBs. The correlations are in good agreement, however, with those predicted by the Cannonball model of GRBs.
Comments: Accepted for publication in Astronomy and Astrophysics
Journal: A&A 558, A115 (2013)
Origin of $10^{15}-10^{16}$G Magnetic Fields in the Central Engine of Gamma Ray Bursts
Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
Spectral Softening in X-ray Afterglow of GRB 130925A as Predicted by Dust Scattering Model
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