Luminosity correlations for gamma-ray bursts and implications for their prompt and afterglow emission mechanisms
arXiv:1208.1680 · doi:10.1088/0004-637X/758/1/32
Abstract
We present the relation between the ( and corrected) spectral lags, , for the standard Swift energy bands 50-100 keV and 100-200 keV and the peak isotropic luminosity, (a relation reported first by Norris et al.), for a subset of 12 long Swift GRBs taken from a recent study of this relation by Ukwatta et al. The chosen GRBs are also a subset of the Dainotti et al. sample, a set of Swift GRBs of known redshift, employed in establishing a relation between the (GRB frame) luminosity, , of the shallow (or constant) flux portion of the typical XRT GRB-afterglow light curve and the (GRB frame) time of transition to the normal decay rate, . We also present the relation using only the bursts common in the two samples. The two relations exhibit a significant degree of correlation ( for the and for the relation) and have surprisingly similar best-fit power law indices ( for and for ). Even more surprisingly, we noted that although and represent different GRB time variables, it appears that the first relation () extrapolates into the second one for timescales . This fact suggests that these two relations have a common origin, which we conjecture to be kinematic. This relation adds to the recently discovered relations between properties of the prompt and afterglow GRB phases, indicating a much more intimate relation between these two phases than hitherto considered.
References in corpus (4)
Cited by in corpus (13)
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