Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo
文献类型:期刊论文
| 作者 | Li Z(李志)2,3,4; Yu, Jiancheng1 |
| 刊名 | EUROPEAN PHYSICAL JOURNAL C
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| 出版日期 | 2025-10-19 |
| 卷号 | 85期号:10 |
| ISSN号 | 1434-6044 |
| DOI | 10.1140/epjc/s10052-025-14911-6 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Article |
| 英文摘要 | This study investigates the accretion process and observational signatures of thin accretion disks around a Schwarzschild black hole (BH) embedded in a Dehnen-type dark matter (DM) halo. We examine the influence of the density rho s\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\rho _{s}$$\end{document} and radius rs\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$r_{s}$$\end{document} of the DM halo on key disk properties, including the energy flux, temperature distribution, and emission spectrum. Our results show that all three of these quantities decrease with increasing rho s\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\rho _{s}$$\end{document} or rs.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$r_{s}.$$\end{document} Furthermore, by generating and analyzing both direct and secondary images of the accretion disk, we explore how the observational inclination angle and the DM halo parameters rho s\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\rho _{s}$$\end{document} and rs\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$r_{s}$$\end{document} affect image profiles. Finally, the observed flux distributions are presented for different inclination angles. Our findings indicate that the accretion disk becomes colder and dimmer as the DM halo parameters increase, highlighting the significant role of DM in shaping BH observables. |
| 学科主题 | 天文学 ; 天体物理学 ; 高能天体物理学 |
| URL标识 | 查看原文 |
| 出版地 | ONE NEW YORK PLAZA, SUITE 4600, NEW YORK, NY, UNITED STATES |
| WOS关键词 | ACCRETION DISKS ; ROTATION ; IMAGE |
| 资助项目 | National Natural Science Foundation of China[2021YFA1600400/2021YFA1600402]; National Key R&D Program of China[12133011]; National Key R&D Program of China[12288102]; National Natural Science Foundation of China[202302AN360001]; International Centre of Supernovae, Yunnan Key Laboratory |
| WOS研究方向 | Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:001595911600002 |
| 出版者 | SPRINGER |
| 资助机构 | National Natural Science Foundation of China[2021YFA1600400/2021YFA1600402] ; National Key R&D Program of China[12133011, 12288102] ; National Natural Science Foundation of China[202302AN360001] ; International Centre of Supernovae, Yunnan Key Laboratory |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28659] ![]() |
| 专题 | 云南天文台_恒星物理研究组 |
| 通讯作者 | Li Z(李志) |
| 作者单位 | 1.College of Physics, Guizhou University, Guiyang, 550025, China 2.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People’s Republic of China; 3.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, People’s Republic of China; 4.International Centre of Supernovae, Yunnan Key Laboratory, Kunming, 650216, People’s Republic of China; |
| 推荐引用方式 GB/T 7714 | Li Z,Yu, Jiancheng. Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo[J]. EUROPEAN PHYSICAL JOURNAL C,2025,85(10). |
| APA | 李志,&Yu, Jiancheng.(2025).Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo.EUROPEAN PHYSICAL JOURNAL C,85(10). |
| MLA | 李志,et al."Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo".EUROPEAN PHYSICAL JOURNAL C 85.10(2025). |
入库方式: OAI收割
来源:云南天文台
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