We examine the Swift/X-ray Telescope (XRT) light curves from the first ∼ 150 Gamma-Ray Burst (GRB) afterglows. Although we expected to find jet breaks at typical times of 1-2 days after the GRB, we find that these appear to be extremely rare. Typical light curves have a break in the slope at about 104 s, followed by a single power law decay whose slope is much too shallow to be consistent with expectations for jet breaks. X-ray light curves typically extend out to ∼ 10 days without any further breaks, until they become too faint for the XRT to detect. In some extreme cases, light curves extend out to more than two months without evidence for jet breaks. This raises concerns about our understanding of afterglow and jet dynamics, and of GRB energetics.
|Original language||English (US)|
|Number of pages||15|
|Journal||Nuovo Cimento della Societa Italiana di Fisica B|
|State||Published - Oct 2006|
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)