The supercritical pile model for GRBs

We present the basic notions of the “Supercritical Pile” model of Gamma Ray Bursts (GRBs). This model is motivated by the need for a process that provides the dissipation necessary in GRBs and presents a well defined scheme for converting the energy stored in the relativistic protons of the Relativistic Blast Waves (RBW) associated with GRB into radiation; at the same time it leads to spectra which exhibit a peak in the burst νFν distribution at an energy Ep ≃ 1 MeV in the observer’s frame, in agreement with observation and largely independent of the Lorentz factor Γ of the associated relativistic outflow.