“…The successful launch of the Swift satellite did open a new window to reveal what happens in the early GRB afterglow phase. As summarized in Zhang et al (2006) and Nousek et al (2006), in a canonical Swift GRB X-ray afterglow lightcurve some interesting features are emerging, including the very early sharp decline (i.e., phase-I), a shallow decline of the X-ray afterglow (i.e., phase-II), and the energetic X-ray flares (i.e., phase-V). The interpretation and the implication of these features have been discussed in great detail (see Mészáros 2006;Piran & Fan 2007;Zhang 2007 for recent reviews).…”