The comprehensive statistical analysis of Swift X-ray light-curves, collecting data from six years of operation, revealed the existence of a universal scaling among the isotropic energy emitted in the rest frame 10-10^4 keV energy band during the prompt emission (E_{ gamma,iso}), the peak of the prompt emission energy spectrum (E_{ pk}), and the X-ray energy emitted in the 0.3-10 keV observed energy band (E_{ X,iso}). In this paper we show that this three-parameter correlation is robust and does not depend on our definition of E_{ X,iso}. It is shared by long, short, and low-energetic GRBs, differently from the well-known E_{ gamma,iso}-E_{ pk} correlation. We speculate that the ultimate physical property that regulates the GRB properties is the outflow Lorentz factor.
Categories: astro-ph.HE astro-ph.CO