Polarization Evolution of Gamma-Ray Burst Prompt Emission with Bulk Acceleration
文献类型:期刊论文
| 作者 | Zhong, Qian1; Liu, Hong-Bang1; Cheng, Kangfa2; Feng, Zu-Ke1; Tuo, Jiang-Chuan1; Mai, Qian-Nan1; Mao JR(毛基荣)3,4,5 ; Liang, En-Wei1
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2025-06-10 |
| 卷号 | 986期号:1 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/add0ac |
| 产权排序 | 第3完成单位 |
| 文献子类 | Article |
| 英文摘要 | During the prompt phase, Poynting-flux-dominated jets undergo acceleration accompanied by magnetic dissipation. By using an outward-propagating thin-shell model, where bulk Lorentz factors Gamma increase with radius and the magnetic field strength decay is related to the acceleration and the energy conversion rate, this process can be investigated through time-resolved polarization analysis. Faster acceleration produces a greater flux, steeper light-curve growth followed by a sharper decline, and polarization degree decreases sharply. With a fixed acceleration index, lower energy conversion rates are associated with lower flux, shallower rises and declines in light curves, lower polarization degree, smoother decline for on-beam (q = theta(v)/theta(j) < 1) emission, and sharper decline for off-beam (q > 1) emission in polarization curves. Both jet acceleration and magnetic dissipation enhance the likelihood of polarization angle flips in observations with small viewing angles, while also leading to higher polarization degrees after the flip in observations with larger viewing angles. The joint analysis of light curves and polarization provides valuable insights into gamma-ray burst motion and energy conversion processes. Rapid decline in the light curve indicates fast acceleration and high energy conversion rates, while gradual light-curve decline coupled with polarization angle flips (for small viewing angles) or the higher polarization degree after flipping (for large viewing angles) suggests acceleration accompanied by magnetic dissipation. Otherwise, the jet is coasting or slowly accelerating at this time. |
| 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 | DECAYING MAGNETIC-FIELD ; RECONNECTION ; AFTERGLOWS ; MODELS ; TURBULENCE ; RADIATION ; OUTFLOWS ; I. |
| 资助项目 | National Key R&D Program of China; National Natural Science Foundation of China[12027803]; National Natural Science Foundation of China[U1731239]; National Natural Science Foundation of China[12133003]; National Natural Science Foundation of China[U1938201]; National Natural Science Foundation of China[12273005]; Guangxi Talent Program (Highland of Innovation Talents); |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001503787100001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | National Key R&D Program of China ; National Natural Science Foundation of China[12027803, U1731239, 12133003, U1938201, 12273005] ; Guangxi Talent Program (Highland of Innovation Talents) ; [2024YFA1611700] ; [2021YFA071850X] ; [2021YFA071840X] |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28336] ![]() |
| 专题 | 星系类星体研究组 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 | Liu, Hong-Bang |
| 作者单位 | 1.Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Nanning 530004, People's Republic of China; liuhb@gxu.edu.cn; 2.School of Mathematics and Physics, Guangxi Minzu University, Nanning 530006, People's Republic of China; 3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, Yunnan Province, People's Republic of China; 4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China; 5.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Zhong, Qian,Liu, Hong-Bang,Cheng, Kangfa,et al. Polarization Evolution of Gamma-Ray Burst Prompt Emission with Bulk Acceleration[J]. ASTROPHYSICAL JOURNAL,2025,986(1). |
| APA | Zhong, Qian.,Liu, Hong-Bang.,Cheng, Kangfa.,Feng, Zu-Ke.,Tuo, Jiang-Chuan.,...&Liang, En-Wei.(2025).Polarization Evolution of Gamma-Ray Burst Prompt Emission with Bulk Acceleration.ASTROPHYSICAL JOURNAL,986(1). |
| MLA | Zhong, Qian,et al."Polarization Evolution of Gamma-Ray Burst Prompt Emission with Bulk Acceleration".ASTROPHYSICAL JOURNAL 986.1(2025). |
入库方式: OAI收割
来源:云南天文台
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