Origin of the bright prompt optical emission in the naked eye burst

Details Origin of the bright prompt optical emission in the naked eye burst Origin of the bright prompt optical emission in the naked eye burst

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..258h&link_type=abstract

DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 258-260 (2010).

Astronomy and Astrophysics

Astronomy

1

Gamma-Ray Sources (Astronomical), Synchrotron Radiation, Shock Waves, Gamma-Ray Sources, Gamma-Ray Bursts, Synchrotron Radiation, Planetary Bow Shocks, Interplanetary Shocks

Scientific paper

The huge optical brightness of GRB 080319B (the ''Naked Eye Burst'') makes this event really challenging for models of the prompt GRB emission. In the framework of the internal shock model, we investigate a scenario where the dominant radiative process is synchrotron emission and the high optical flux is due to the dynamical properties of the relativistic outflow : if the initial Lorentz factor distribution in the jet is highly variable, many internal shocks will form within the outflow at various radii. The most violent shocks will produce the main gamma-ray component while the less violent ones will contribute at lower energy, including the optical range.

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