主要内容:
更多的是很多疑问。
提出两个模型:X射线余辉可能是外流体本身的耗散辐射,而不是外籍波;暴本身在共动系里可能就是集束的。
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文章信息:
- · arXiv e-print (arXiv:0911.0349)
- · References in the Article
- · Citations to the Article (7) (Citation History)
- · Refereed Citations to the Article
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Title: |
| Gamma Ray Bursts: back to the blackboard |
Authors: |
| Lyutikov, Maxim |
Publication: |
| eprint arXiv:0911.0349 |
Publication Date: |
| 11/2009 |
Origin: |
| ARXIV |
Keywords: |
| Astrophysics - High Energy Astrophysical Phenomena |
Comment: |
| 28 pages, proceedings of the The Shocking Universe meeting, Venice, September 2009 |
Bibliographic Code: |
| 2009arXiv0911.0349L |
Abstract
Exceptional observational breakthroughs in the field of Gamma Ray Burst research are not paralleled by theoretical advances. In this review, based on the introductory talk given at the "The Shocking Universe" meeting, I argue that any present day model of GRBs, especially of Short type, is grossly incomplete. I will highlight various contradictions with observations that many models face and briefly mention a number of ideas that might or might not work. In particular, I will discuss (i) a possibility that early X-ray afterglows are coming from internal dissipation, and not from the forwards shock; (ii) that prompt radiation is beamed in the outflow frame.
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