主要内容:
给出了产生UHECR所要面对的几个问题。
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文章信息:
- · arXiv e-print (arXiv:1003.5318)
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Title: |
| GRBs as ultra-high energy cosmic ray sources: clues from Fermi |
Authors: |
| Dermer, C. |
Publication: |
| eprint arXiv:1003.5318 |
Publication Date: |
| 03/2010 |
Origin: |
| ARXIV |
Keywords: |
| Astrophysics - High Energy Astrophysical Phenomena |
Comment: |
| 9 pages, to appear in the Proceedings of "The Shocking Universe: Gamma Ray Bursts and High Energy Shock Phenomena," Venice, Italy, 14-18 September 2009 |
Bibliographic Code: |
| 2010arXiv1003.5318D |
Abstract
If gamma-ray bursts are sources of ultra-high energy cosmic rays, then radiative signatures of hadronic acceleration are expected in GRB data. Observations with the Fermi Gamma-ray Space Telescope offer the best means to search for evidence of UHECRs in GRBs through electromagnetic channels. Various issues related to UHECR acceleration in GRBs are reviewed, with a focus on the question of energetics.
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