Probing Magnetic Fields of GRB X-Ray Flares with Polarization Observations
文献类型:期刊论文
作者 | Geng, Jin-Jun1,2,3; Huang, Yong-Feng1,2; Wu, Xue-Feng4; Song, Li-Ming5,6; Zong, Hong-Shi3 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2018-08-01 |
卷号 | 862期号:2页码:8 |
ISSN号 | 0004-637X |
关键词 | gamma-ray burst: general polarization radiation mechanisms: non-thermal relativistic processes |
DOI | 10.3847/1538-4357/aacd05 |
英文摘要 | X-ray flares, lasting for similar to 100-1000 s in the X-ray band, are often observed following gamma-ray bursts (GRBs). The physical origin of X-ray flares is still unknown merely with the temporal/spectral information. On the other hand, some polarimeters are expected to be launched within several years, thanks to the increasing interest on astronomical X-ray polarimetry. Here, by assuming that X-ray flares are synchrotron radiation from relativistic spherical shells, we show that the linear polarization degree during the rising phase of an X-ray flare is much higher for the emitting region with toroidal magnetic fields than for that with random magnetic fields. In the decay phase of the flare, the evolution of the polarization degree is determined by the curvature effect of the emitting shell, which is a natural feature of jet scenarios for flares. Therefore, the measurement of the polarization of X-ray flares would provide a useful tool to probe the configuration of magnetic fields in the emission region, and may even help to test the curvature effect. The information on the magnetic configuration can further help us to understand the properties of GRB jets. |
WOS关键词 | INTERNAL SHOCK MODEL ; DOUBLE RADIO-SOURCES ; LIGHT CURVES ; LINEAR-POLARIZATION ; MILLISECOND PULSARS ; OPTICAL AFTERGLOWS ; EMISSION MECHANISM ; BURST EMISSION ; ACCRETION DISK ; EVOLUTION |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000440304800004 |
源URL | [http://libir.pmo.ac.cn/handle/332002/21667] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Geng, Jin-Jun |
作者单位 | 1.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Jiangsu, Peoples R China 2.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Jiangsu, Peoples R China 3.Nanjing Univ, Dept Phys, Nanjing 210093, Jiangsu, Peoples R China 4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 5.Chinese Acad Sci, Key Lab Particle Astrophys, Beijing 100049, Peoples R China 6.Chinese Acad Sci, Inst High Energy Phys, Particle Astrophys Div, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Geng, Jin-Jun,Huang, Yong-Feng,Wu, Xue-Feng,et al. Probing Magnetic Fields of GRB X-Ray Flares with Polarization Observations[J]. ASTROPHYSICAL JOURNAL,2018,862(2):8. |
APA | Geng, Jin-Jun,Huang, Yong-Feng,Wu, Xue-Feng,Song, Li-Ming,&Zong, Hong-Shi.(2018).Probing Magnetic Fields of GRB X-Ray Flares with Polarization Observations.ASTROPHYSICAL JOURNAL,862(2),8. |
MLA | Geng, Jin-Jun,et al."Probing Magnetic Fields of GRB X-Ray Flares with Polarization Observations".ASTROPHYSICAL JOURNAL 862.2(2018):8. |
入库方式: OAI收割
来源:紫金山天文台
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