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A One-Dimensional Relativistic Shock Model for the Light Curve of Gamma-ray Bursts
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作者 Cheng-Yue Su Yi-Ping Qin +1 位作者 Jun-Hui Fan zhang-yu han 《Chinese Journal of Astronomy and Astrophysics》 CSCD 2006年第3期323-330,共8页
We investigate the forming of gamma-ray burst pulses with a simple onedimensional relativistic shock model. The mechanism is that a "central engine" drives forward the nearby plasma inside the fireball to generate a... We investigate the forming of gamma-ray burst pulses with a simple onedimensional relativistic shock model. The mechanism is that a "central engine" drives forward the nearby plasma inside the fireball to generate a series of pressure waves. We give a relativistic geometric recurrence formula that connects the time when the pressure waves are produced and the time when the corresponding shocks occurred. This relation enables us to relate the pulse magnitude with the observation time. Our analysis shows that the evolution of the pressure waves leads to a fast rise and an exponential decay pulses. In determining the width of the pulses, the acceleration time is more important than that of the deceleration. 展开更多
关键词 gamma-ray: bursts - profiles - hydrodynamics - shock waves - methods:numerical
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