paper

Gamma-Ray Burst Precursors as the Remnant of the Thermal Radiation Initially Trapped in the Fireball

arXiv:astro-ph/0703144 · doi:10.1111/j.1365-2966.2007.12083.x

Abstract

In the standard fireball model of gamma-ray bursts (GRBs), the fireball starts with an optically thick phase. As it expands, the fireball becomes optically thin at some stage. The thermal radiation trapped in the originally opaque fireball then leaks out, producing a transient event. The appearance of the event is investigated in the framework of a homogeneous, spherically symmetric, and freely expanding fireball produced instantly by an explosive process without continuous injection of mass and energy. We find that, generally, the event has a time-duration shorter than that of the main burst, which is presumably produced by the internal shock after the fireball becomes optically thin. The event is separated from the main burst by a quiescent time-interval, and is weaker than the main burst at least in a high energy band. Hence, the event corresponds to a GRB precursor. The precursor event predicted by our model has a smooth and FRED (Fast Rise and Exponential Decay) shape lightcurve, and a quasi-thermal spectrum. Typically, the characteristic blackbody photon energy is in the X-ray band. However, if the distortion of the blackbody spectrum by electron scattering is considered, the characteristic photon energy could be boosted to the gamma-ray band. Our model may explain a class of observed GRB precursors--those having smooth and FRED-shape lightcurves and quasi-thermal spectra.

arXiv comment18 pages, including 13 figures. MNRAS accepted. An error in the boundary of the integral over theta for the flux density, luminosity etc is corrected. Figs. 5-13 are replotted. Main conclusions are not changed

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