Hydrodynamics of Relativistic Blast Waves in a Density-Jump Medium and Their Emission Signature

Details Hydrodynamics of Relativistic Blast Waves in a Density-Jump Medium and Their Emission Signature Hydrodynamics of Relativistic Blast Waves in a Density-Jump Medium and Their Emission Signature

2001-11-23

arxiv.org/abs/astro-ph/0111454v3

Astronomy and Astrophysics

Astrophysics

minor changes, accepted for publication in ApJ Letters

Scientific paper

10.1086/339418

We analyze in detail the hydrodynamics and afterglow emission of an ultrarelativistic blast wave when it expands in a density-jump medium. Such a medium is likely to appear in the vicinity of gamma-ray bursts (GRBs) associated with massive stars. The interaction of the blast wave with this medium is described through a reverse shock and a forward shock. We show that the reverse shock is initially relativistic if the factor of a density jump ($\alpha$) is much larger than 21, and Newtonian if $1<\alpha\ll 21$. We also calculate light curves of the afterglow emission during the interaction if the reverse shock is relativistic, and find that the optical flux density initially decays abruptly, then rises rapidly, and finally fades based on a power-law, which could be followed by an abrupt decay when the reverse shock has just crossed the originally swept-up matter. Therefore, one property of an afterglow occurring in a large-density-jump medium is an abrupt drop followed by a bump in the light curve and thus provides a probe of circumburst environments. In addition, this property could not only account for the optical afterglows of GRB 970508 and GRB 000301C but also explain the X-ray afterglow of GRB 981226.

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