Jitter radiation as a possible mechanism for Gamma-Ray Burst afterglows. Spectra and lightcurves

Details Jitter radiation as a possible mechanism for Gamma-Ray Burst afterglows. Spectra and lightcurves Jitter radiation as a possible mechanism for Gamma-Ray Burst afterglows. Spectra and lightcurves

2007-03-09

arxiv.org/abs/astro-ph/0703209v1

Astrophys.J.666:339-345,2007

Astronomy and Astrophysics

Astrophysics

16 pages, 1 figure

Scientific paper

10.1086/520701

The standard model of GRB afterglows assumes that the radiation observed as a delayed emission is of synchrotron origin, which requires the shock magnetic field to be relatively homogeneous on small scales. An alternative mechanism -- jitter radiation, which traditionally has been applied to the prompt emission -- substitutes synchrotron when the magnetic field is tangled on a microscopic scale. Such fields are produced at relativistic shocks by the Weibel instability. Here we explore the possibility that small-scale fields populate afterglow shocks. We derive the spectrum of jitter radiation under the afterglow conditions. We also derive the afterglow lightcurves for the ISM and Wind profiles of the ambient density. Jitter self-absorption is calculated here for the first time. We find that jitter radiation can produce afterglows similar to synchrotron-generated ones, but with some important differences. We compare the predictions of the two emission mechanisms. By fitting observational data to the synchrotron and jitter afterglow lightcurves, it can be possible to discriminate between the small-scale vs large-scale magnetic field models in afterglow shocks.

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