Shadow and accretion disk images of the rotation loop quantum black bounce
文献类型:期刊论文
| 作者 | He, Ke-Jian6; Ye, Huan5; Zeng, Xiao-Xiong4; Li, Li-Fang3; Xu, Peng1,2,3 |
| 刊名 | CHINESE PHYSICS C
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| 出版日期 | 2025-12-01 |
| 卷号 | 49期号:12页码:16 |
| 关键词 | black hole shadow black hole image loop quantum cosmology |
| ISSN号 | 1674-1137 |
| DOI | 10.1088/1674-1137/adf4a2 |
| 通讯作者 | Li, Li-Fang(lilifang@imech.ac.cn) |
| 英文摘要 | In this study, we investigate the shadow and observational image of the Kerr-like Loop Quantum Gravity (LQG) inspired black bounce with the help of the celestial light and thin disk sources by employing the backward ray-tracing method. The results indicate that both the LQG parameter alpha and rotation parameter a contribute to a reduction in the shadow size. However, the influence of a is predominant, whereas that of alpha is supplementary. For the accretion disk model, we extend its inner edge to the black hole's event horizon, and the motion of particles is different in the regions inside and outside the innermost stable circular orbit. We find that the correlation parameters ( ), along with the observer's inclination angle, affect the image's asymmetry and the distortion of the inner shadow. As the inclination increases, the direct and lensed images diverge, creating a structure resembling a hat. Moreover, we investigate the redshift distribution of the direct lensed images of the accretion disk under different parameters and observation angles. The results show that the redshift distribution and observed intensity are evidently related to the behavior of accretion flow. These results may provide a potential approach for limiting black hole parameters, detecting quantum gravity effects, and distinguishing the LQG black hole from other black hole models. |
| WOS关键词 | HOLE ; GRAVITY ; SINGULARITY ; APPEARANCE ; PLASMA |
| WOS研究方向 | Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:001580222200001 |
| 源URL | [http://dspace.imech.ac.cn/handle/311007/104107] ![]() |
| 专题 | 力学研究所_国家微重力实验室 |
| 通讯作者 | Li, Li-Fang |
| 作者单位 | 1.Univ Chinese Acad Sci, Taiji Lab Gravitat Wave Universe Beijing Hanzhou, Beijing 100049, Peoples R China 2.Lanzhou Univ, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China 3.Chinese Acad Sci, Inst Mech, Ctr Gravitat Wave Expt, Natl Micrograv Lab, Beijing 100190, Peoples R China 4.Chongqing Normal Univ, Coll Phys & Elect Engn, Chongqing 401331, Peoples R China 5.Chongqing Jiaotong Univ, Sch Mat Sci & Engn, Chongqing 400074, Peoples R China 6.Chongqing Jiaotong Univ, Dept Mech, Chongqing 400000, Peoples R China |
| 推荐引用方式 GB/T 7714 | He, Ke-Jian,Ye, Huan,Zeng, Xiao-Xiong,et al. Shadow and accretion disk images of the rotation loop quantum black bounce[J]. CHINESE PHYSICS C,2025,49(12):16. |
| APA | He, Ke-Jian,Ye, Huan,Zeng, Xiao-Xiong,Li, Li-Fang,&Xu, Peng.(2025).Shadow and accretion disk images of the rotation loop quantum black bounce.CHINESE PHYSICS C,49(12),16. |
| MLA | He, Ke-Jian,et al."Shadow and accretion disk images of the rotation loop quantum black bounce".CHINESE PHYSICS C 49.12(2025):16. |
入库方式: OAI收割
来源:力学研究所
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