Luminosity correlations for gamma-ray bursts and implications for their   prompt and afterglow emission mechanisms
  We present the relation between the ($z-$ and $k-$corrected) spectral lags, $\tau$, for the standard Swift energy bands 50-100 keV and 100-200 keV and the peak isotropic luminosity, $L_{\mathrm{iso}}$ (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, $L_X$, 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, $T_{\mathrm{brk}}$. We also present the $L_X-T_{\mathrm{brk}}$ relation using only the bursts common in the two samples. The two relations exhibit a significant degree of correlation ($\rho = -0.65$ for the $L_{\mathrm{iso}}-\tau$ and $\rho = -0.88$ for the $L_{X} - T_{\mathrm{brk}}$ relation) and have surprisingly similar best-fit power law indices ($-1.19 \pm 0.17$ for $L_{\mathrm{iso}}-\tau$ and $-1.10 \pm 0.03$ for $L_{X} - T_{\mathrm{brk}}$). Even more surprisingly, we noted that although $\tau$ and $T_{\mathrm{brk}}$ represent different GRB time variables, it appears that the first relation ($L_{\mathrm{iso}}-\tau$) extrapolates into the second one for timescales $\tau \simeq T_{\mathrm{brk}}$. 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. 
Joseph Sultana, Demosthenes Kazanas, Keigo Fukumura
astro-ph.HE