The Novel and Common Origin of Gamma-ray Bursts: A Galactic Seed Separation with Emitting Radiations

Abstract

The mechanism of the gamma-ray burst is uncertain while the current candidates, respectively, for short and long GRBs are rather accepted. They conflict with some observed facts. Here we examine in detail the process for an energy circulation to separate to two ones by the energy circulation theory. We derive the equations of the force and the potential energy for the separation of a galactic seed. A galactic seed divides to two seeds orthogonally. If the receding speed is high enough, two seeds separate away orthogonally. If not enough, they are trapped at the energy trough, from where a subsequent flat separation occurs. The difference in the potential energy is partly emitted as gamma-ray radiations. The proposed process nicely meets the observed features of the GRBs, which the standard cosmology cannot explain. The GRBs are an important evidence to support our proposed model of galactic evolution, which includes galactic seed separations, as well as its basis; the energy circulation theory. Another key evidence, which we reported previously, is that the model predicts a constant speed of a galaxy rotation at any radial distances without dark matter.