Huang, Y. F. and Lu, T. and Cheng, K. S. (2005) GRB afterglows: Deep Newtonian phase and its application. Il nuovo cimento C, 28 (3). pp. 415-418. ISSN 1826-9885
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Abstract
Gamma-ray burst afterglows have been observed for months or even years in a few cases. It is worth noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shockaccelerated 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.
| Item Type: | Article |
|---|---|
| Additional Information: | Paper presented at the “4th Workshop on Gamma-Ray Burst in the Afterglow Era”, Rome, October 18-22, 2004. |
| Uncontrolled Keywords: | Astrophysical magnetohydrodynamics and plasmas ; Supernovae ; Black holes |
| Subjects: | 500 Scienze naturali e Matematica > 520 Astronomia e scienze connesse |
| Depositing User: | Marina Spanti |
| Date Deposited: | 16 Mar 2020 10:47 |
| Last Modified: | 16 Mar 2020 10:47 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/15675 |
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