Jitter Mechanism as a Kind of Coherent Radiation: Constrained by the GRB 221009A Emission at 18 TeV
文献类型:期刊论文
作者 | Mao JR(毛基荣)1,2,3; Wang JC(王建成)1,2,3 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2023-04-01 |
卷号 | 946期号:2 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/acc400 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | The emission of gamma-ray burst (GRB) 221009A at 18 TeV has been detected by the large high-altitude air shower observatory. We suggest jitter radiation as a possible explanation for the TeV emission for this energetic GRB. In our scenario, the radiation field is linked to the perturbation field, and the perturbation field is dominated by kinetic turbulence. Kinetic turbulence takes a vital role in both magnetic field generation and particle acceleration. The jitter radiation can reach the TeV energy band when we consider either electron cooling or Landau damping. We further suggest that the jitter radiation in the very high-energy band is coherent emission. Our modeling results can be constrained by the observational results of GRB 221009A in the TeV energy band. This radiation mechanism is expected to have wide applications in the high-energy astrophysical research field. |
学科主题 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | EXTRAGALACTIC BACKGROUND LIGHT ; GAMMA-RAY BURSTS ; PARTICLE-ACCELERATION ; ELECTRON ACCELERATION ; MAGNETIC-FIELDS ; PROMPT EMISSION ; PLASMA ; ENERGY ; SHOCK ; GENERATION |
资助项目 | National Natural Science Foundation of China[11673062] ; Oversea Talent Program of Yunnan Province ; YunLing Scholar Award of Yunnan Province |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:000962895600001 |
资助机构 | National Natural Science Foundation of China[11673062] ; Oversea Talent Program of Yunnan Province ; YunLing Scholar Award of Yunnan Province |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25899] |
专题 | 星系类星体研究组 云南天文台_高能天体物理研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Mao JR(毛基荣) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, People's Republic of China; jirongmao@mail.ynao.ac.cn; 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, 100012 Beijing, People's Republic of China; 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, People's Republic of China |
推荐引用方式 GB/T 7714 | Mao JR,Wang JC. Jitter Mechanism as a Kind of Coherent Radiation: Constrained by the GRB 221009A Emission at 18 TeV[J]. ASTROPHYSICAL JOURNAL,2023,946(2). |
APA | Mao JR,&Wang JC.(2023).Jitter Mechanism as a Kind of Coherent Radiation: Constrained by the GRB 221009A Emission at 18 TeV.ASTROPHYSICAL JOURNAL,946(2). |
MLA | Mao JR,et al."Jitter Mechanism as a Kind of Coherent Radiation: Constrained by the GRB 221009A Emission at 18 TeV".ASTROPHYSICAL JOURNAL 946.2(2023). |
入库方式: OAI收割
来源:云南天文台
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