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25 April 2024
 
  » arxiv » astro-ph/0502555

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GRB afterglows: deep Newtonian phase and its application
Y.F. Huang ; T. Lu ; K.S. Cheng ;
Date 26 Feb 2005
Subject astro-ph
AbstractGamma-ray burst afterglows have been observed for months or even years in a few cases. It deserves noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shock-accelerated electrons will no longer be highly relativistic. To calculate the afterglows, we must assume that the electrons obey a power-law distribution according to their kinetic energy, not simply the Lorentz factor.
Source arXiv, astro-ph/0502555
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