On the Time-Frequency Downward Drifting of Repeating Fast Radio Bursts
文献类型:期刊论文
作者 | Wang, Weiyang1,2,3,4; Zhang, Bing5; Chen, Xuelei1,2,6; Xu, Renxin3,4,7,8 |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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出版日期 | 2019-05-01 |
卷号 | 876期号:1页码:5 |
关键词 | pulsars: general radiation mechanisms: non-thermal radio continuum: general stars: neutron |
ISSN号 | 2041-8205 |
DOI | 10.3847/2041-8213/ab1aab |
英文摘要 | The newly discovered second repeating fast radio burst (FRB) source, FRB 180814.J0422+73, was reported to exhibit a time-frequency downward drifting pattern, which is also seen in the first repeater FRB 121102. We propose a generic geometrical model to account for the observed downward drifting of sub-pulse frequency, within the framework of coherent curvature radiation by bunches of electron positron pairs in the magnetosphere of a neutron star (NS). A sudden trigger event excites these coherent bunches of charged particles, which stream outward along open field lines. As the field lines sweep across the line of sight, the bunches seen later travel farther into the less-curved part of the magnetic field lines, thus emitting at lower frequencies. We use this model to explain the time-frequency downward drifting in two FRB generation scenarios, the transient pulsar-like sparking from the inner gap region of a slowly rotating NS, and the externally triggered magnetosphere reconfiguration known as the "cosmic comb." |
WOS关键词 | EMISSION ; SPARKS |
资助项目 | MoST[2016YFE0100300] ; CAS[QYZDJ-SSW-SLH017] ; CAS[XDB 23040100] ; CAS[XDB23010200] ; National Key R&D Program of China[2017YFA0402602] ; NSFC[11673002] ; NSFC[U1531243] ; NSFC[11473044] ; NSFC[11653003] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000466902900005 |
出版者 | IOP PUBLISHING LTD |
资助机构 | MoST ; MoST ; CAS ; CAS ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; MoST ; MoST ; CAS ; CAS ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; MoST ; MoST ; CAS ; CAS ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; MoST ; MoST ; CAS ; CAS ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC |
源URL | [http://ir.bao.ac.cn/handle/114a11/26061] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Wang, Weiyang |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100101, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Peking Univ, Sch Phys, Beijing 100871, Peoples R China 4.Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China 5.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA 6.Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China 7.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 8.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, Weiyang,Zhang, Bing,Chen, Xuelei,et al. On the Time-Frequency Downward Drifting of Repeating Fast Radio Bursts[J]. ASTROPHYSICAL JOURNAL LETTERS,2019,876(1):5. |
APA | Wang, Weiyang,Zhang, Bing,Chen, Xuelei,&Xu, Renxin.(2019).On the Time-Frequency Downward Drifting of Repeating Fast Radio Bursts.ASTROPHYSICAL JOURNAL LETTERS,876(1),5. |
MLA | Wang, Weiyang,et al."On the Time-Frequency Downward Drifting of Repeating Fast Radio Bursts".ASTROPHYSICAL JOURNAL LETTERS 876.1(2019):5. |
入库方式: OAI收割
来源:国家天文台
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