Energy Distribution of Relativistic GRB Jets

Details Energy Distribution of Relativistic GRB Jets Energy Distribution of Relativistic GRB Jets

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1000..467m&link_type=abstract

GAMMA-RAY BURSTS 2007: Proceedings of the Santa Fe Conference. AIP Conference Proceedings, Volume 1000, pp. 467-471 (2008).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Interstellar Medium And Nebulae In External Galaxies, Jets, Outflows, And Bipolar Flows

Scientific paper

We investigate relativistic jet propagation in the collapsar and interstellar medium, using 2-dimensional relativistic hydrodynamic simulations. The jet is assumed to be initially thermal dominated plasma and have half opening angle (5 degrees). Realistic progenitor models are adopted and the difference of the outflow properties by different progenitor models are studied. There is not significant difference, especially in the energy distribution in unit solid angle as a function of the angle between jet and line of site.

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