2006
DOI: 10.1086/500723
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Physical Processes Shaping Gamma‐Ray Burst X‐Ray Afterglow Light Curves: Theoretical Implications from theSwiftX‐Ray Telescope Observations

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Cited by 1,050 publications
(1,711 citation statements)
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References 127 publications
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“…Then, there is only one choice -the shock parameters should evolve with time. If we take q ∼ 0.5 (which is suggested by the recent Swift XRT data, see Zhang et al 2006), a ∼ 1, b ∼ 0, then the flux would be nearly a constant, which is agreement with the observation.…”
Section: The Case Of Grb940217supporting
confidence: 86%
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“…Then, there is only one choice -the shock parameters should evolve with time. If we take q ∼ 0.5 (which is suggested by the recent Swift XRT data, see Zhang et al 2006), a ∼ 1, b ∼ 0, then the flux would be nearly a constant, which is agreement with the observation.…”
Section: The Case Of Grb940217supporting
confidence: 86%
“…However, there are increasing evidences that the shock energy may increase with time during some period. One good example is the discovery of the "shallow decay phase" in the early X-ray light curves of many GRBs, which is usually attributed to the energy injection (Zhang et al 2006;Nousek et al 2006). Now we consider the case that there is significant continuous energy injection into the fireball, so the fireball decelerates less rapidly and the afterglow emission will show a shallow decline.…”
Section: The Ssc Emission With Energy Injection and Evolving Shock Pamentioning
confidence: 99%
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