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Paper detail

On the Counter-jet Emission in GRB Afterglows

We investigate the dynamical evolution of double-sided jets and present detailed numerical studies on the emission from the receding jet of gamma-ray bursts. It is found that the receding jet emission is generally very weak and only manifests as a plateau in the late time radio afterglow light curves. Additionally, we find that the effect of synchrotron self-absorption can influence the peak time of the receding jet emission significantly.

preprint2010arXivOpen access
Xin WangY. F. Huang
astro-ph.HE
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Xin WangY. F. Huang

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