Fermi Observations of Gamma-ray Bursts

被引：0
|
作者：
Ohno, Masanori [1 ]
机构：
[1] JAXA, Inst Space & Astronaut Sci, Chuo Ku, Kanagawa 2525210, Japan
来源：
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS | 2010年 / 1279卷
关键词：
gamma-rays:; bursts; SPECTRAL COMPONENT; EMISSION;
D O I：
10.1063/1.3509362
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The gamma-ray emission mechanism of Gamma-ray bursts (GRBs) are still unknown. Fermi Gamma-ray Space Telescope successfully detected high-energy (> 100 MeV) emission from 17 GRBs since its launch. Fermi revealed the distinct temporal behaviors and extra spectral component from high-energy emission. These new observational results are driving many theoretical implications, such as leptonic, hadronic and afterglow origin. The highest energy photon detected by Fermi gives a constraint on the bulk Lorentz factor of the ultra-relativistic jets of GRBs. The impact of the Fermi GRB observations extends not only to the GRB-related issues but also to the outside GRB physics, such as quantum gravity and model of the extra galactic background light
引用
收藏
页码：9 / 12
页数：4
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