X-Ray and high energy flares from late internal shocks of gamma-ray bursts
arXiv:0811.1068 · doi:10.1088/0004-637X/692/1/133
Abstract
We study afterglow flares of gamma-ray bursts (GRBs) in the framework of the late internal shock (LIS) model based on a careful description for the dynamics of a pair of shocks generated by a collision between two homogeneous shells,. First, by confronting the model with some fundamental observational features of X-ray flares, we find some constraints on the properties of the pre-collision shells that are directly determined by the central engine of GRBs. Second, high energy emission associated with X-ray flares, which arises from synchrotron self-Compton (SSC) emission of LISs, is investigated in a wide parameter space. The predicted flux of high energy flares may reach as high as , which is likely to be detectable with the Large Area Telescope (LAT) aboard \textit{the Fermi Space Telescope}
18 pages, 7 figures, accepted for publication in ApJ
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- Flares in gamma-ray burst X-ray afterglows as prompt emission from slightly misaligned structured jets
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- A New Correlation Between GRB X-Ray Flares And The Prompt Emission
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- The Low-Energy Spectral Index of Gamma-Ray Burst Prompt Emission from Internal Shocks
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- GeV Emission during X-Ray Flares from Late Internal Shocks: Application to GRB 100728A
- Internal shock model for the X-ray flares of Swift J1644+57
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