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arXiv · astro-ph/9906404

Overall Evolution of Realistic Gamma-ray Burst Remnant and Its Afterglow

Y. F. Huang·Z. G. Dai·T. Lu
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Abstract

Conventional dynamic model of gamma-ray burst remnants is found to be incorrect for adiabatic blastwaves during the non-relativistic phase. A new model is derived, which is shown to be correct for both radiative and adiabatic blastwaves during both ultra-relativistic and non-relativistic phase. Our model also takes the evolution of the radiative efficiency into account. The importance of the transition from the ultra-relativistic phase to the non-relativistic phase is stressed.

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Y. F. Huang, Z. G. Dai, T. Lu. 1999-08-21. Overall Evolution of Realistic Gamma-ray Burst Remnant and Its Afterglow. https://doi.org/10.1088/0256-307x%2F16%2F10%2F027

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