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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 | Abstract: | Gamma-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 | Services: | Forum | Review | PDF | Favorites |
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