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Equations of Motion and Initial and Boundary Conditions for Gamma-ray Burst
C.L. Bianco,G.V. Vereshchagin,R. Ruffini,S.-S. Xue 한국물리학회 2006 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.49 No.2I
We compare and contrast the three different approaches to the optically thick adiabatic phase of Gamma-ray Burst(GRB) all the way to transparency. Special attention is given to the role of the rate equation in self-consistently solving the rate equation with the relativistic hydrodynamic equations. The works of Shemi and Piran [1], Piran, Shemi and Narayan [2], M´esz´aros, Laguna and Rees [3] and Ruffini, Salmonson, Wilson and Xue [4,5] are compared and contrasted. The roles of the baryonic loading in these three treatments are pointed out. The constraints on initial conditions for the fireball produced by an electro-magnetic black hole are obtained.