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MG12 - Talk detail
 

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 Participant 

de Barros, Gustavo

Institution

La Sapienza - ICRA  - Piazzale Aldo Moro - Roma - RM - Italy

Session

Talk

Abstract

GRB4

Radial density distribution in optically thick ultrarelativistic expanding plasma

Relativistic Eulerian code is developed which allows solution of spherically symmetric hydrodynamic equations. We apply this code to the case of GRBs with the special attention to the structure of energy density and matter density radial distribution formed when the bulk of the plasma is accelerated to large Lorentz factors. Different initial radial distributions and various baryonic loading are studied.

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