Study of Advective Energy Transport in the Inflow and Outflow of Super-Eddington Accretion Flows
文献类型：期刊论文
| 作者 | Jiao,Cheng-Liang1,2,3; Jiao CL(焦承亮) ; Jiao CL(焦承亮)
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| 刊名 | The Astrophysical Journal
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| 出版日期 | 2023-09-01 |
| 卷号 | 955期号:1 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/aceaf5 |
| 通讯作者 | Jiao,Cheng-Liang() |
| 英文摘要 | Abstract Photon trapping is believed to be an important mechanism in super-Eddington accretion, which greatly reduces the radiative efficiency as photons are swallowed by the central black hole before they can escape from the accretion flow. This effect is interpreted as the radial advection of energy in one-dimensional height-integrated models, such as the slim-disk model. However, when multidimensional effects are considered, the conventional understanding may no longer hold. In this paper, we study the advective energy transport in super-Eddington accretion based on a new two-dimensional inflow–outflow solution with radial self-similarity, in which the advective factor is calculated self-consistently by incorporating the calculation of radiative flux instead of being set as an input parameter. We found that radial advection is actually a heating mechanism in the inflow due to compression, and the energy balance in the inflow is maintained by cooling via radiation and vertical (θ-direction) advection, which transports entropy upward to be radiated closer to the surface or carried away by the outflow. As a result, fewer photons are advected inward, and more photons are released from the surface, so that the mean advective factor is smaller and the emergent flux is higher than the fluxes predicted by the slim-disk model. The radiative efficiency of super-Eddington accretion thus should be higher than that of the slim-disk model, which agrees with the results of some recent numerical simulations. |
| 语种 | 英语 |
| 出版者 | The American Astronomical Society |
| WOS记录号 | IOP:APJ_955_1_20 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/26331]  |
| 专题 | 云南天文台_双星与变星研究组 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 | Jiao,Cheng-Liang; Jiao CL(焦承亮) |
| 作者单位 | 1.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China 3.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China; jiaocl@ynao.ac.cn |
| 推荐引用方式 GB/T 7714 | Jiao,Cheng-Liang,Jiao CL,Jiao CL. Study of Advective Energy Transport in the Inflow and Outflow of Super-Eddington Accretion Flows[J]. The Astrophysical Journal,2023,955(1). |
| APA | Jiao,Cheng-Liang,Jiao CL,&焦承亮.(2023).Study of Advective Energy Transport in the Inflow and Outflow of Super-Eddington Accretion Flows.The Astrophysical Journal,955(1). |
| MLA | Jiao,Cheng-Liang,et al."Study of Advective Energy Transport in the Inflow and Outflow of Super-Eddington Accretion Flows".The Astrophysical Journal 955.1(2023). |
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来源：云南天文台
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