Angular Energy Distribution of Jets from Collapsas

Details Angular Energy Distribution of Jets from Collapsas Angular Energy Distribution of Jets from Collapsas

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1133..106m&link_type=abstract

GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP Conference Proceedings, Volume 1133, pp. 106-108 (2009).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Approximation Methods, Equations Of Motion, Supernovae

Scientific paper

The highly relativistic jets from collapsars are studied in the contect of the gamma-ray burst (GRB). The angular energy distribution of the jets after the eruption from the stellar surface is well fitted by the smoothly broken power law. The distribution of the jets from light progenitor models is steeper than that of the jets injected in more massive progenitor stars. The cocoon property of the jet in the progenitor decides this characteristics of the jet.

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