YNAO OpenIR  > 大样本恒星演化研究组
Alternative TitleFormation of Binary Black Hole Through Stable Mass Transfer Channel
Source Publication天文学进展(Progress In Astronomy)
Contribution Rank第1完成单位
Indexed ByCSCD ; 核心
Keyword大质量恒星 双星 黑洞 恒星演化

由于缺乏足够的观测数据,大质量恒星的研究进展缓慢,到目前为止大质量恒星演化和黑洞详细的形成过程还存在较大争议。LIGO首次探测到恒星级双黑洞并合产生的引力波信号,这不但验证了爱因斯坦20世纪的预言,而且还证实了大质量双黑洞的存在。研究工作采用恒星演化程序MESA (Modules for Experiments in Stellar Astrophysics)计算孤立双星的演化,主星初始质量为20 M⊙~80 M⊙,金属丰度为0.000 1~0.002,初始双星质量比为0.7~0.9。双星系统通过稳定物质转移通道,形成总质量(15~110) M⊙范围内的双黑洞。形成双黑洞的并合时标强烈依赖于初始轨道周期,只有初始轨道周期不大于5 d的双星系统演化形成的双黑洞,通过引力波辐射损失角动量,最终可能在哈勃时标内并合。研究工作得到的结果可以解释部分现阶段已经探测到的引力波事件。

Other Abstract

Due to the lack of observational constraints, progresses in the field of massive stars has been small, leading to controversy regarding their evolution, as well as how black holes are formed. Following LIGO's discovery of binary black hole systems, a better understanding of the formation of massive binary black hole systems is required. In this paper, we use MESA (Modules for Experiments in Stellar Astrophysics) to simulate the evolution of isolated massive binaries, taking into account processes such as stellar wind, mass transfer, and supernova explosions. In our work, we consider binaries with primary masses of 20 to 80 solar masses, mass ratios of 0.7 to 0.9, and metallicities of 0.000 1 to 0.002. We find that binaries that undergo stable mass transfer can form binary black holes with total masses of 15 to 110 solar masses. We also find that the gravitational merging timescales of the simulated binaries are strongly dependent on their initial orbital periods; in our sample, which does not include systems that undergo common envelope evolution, binaries with initial orbital periods of less than 5 days can merge within Hubble time, while those with initial orbital periods of more than 5 days cannot. Our results can explain the origin of some objects that have been observed by LIGO and Virgo.

Funding Project国家自然科学基金[11773065]
Funding Organization国家自然科学基金[11773065]
Subject Area天文学 ; 恒星与银河系 ; 恒星物理学 ; 恒星形成与演化
MOST Discipline Catalogue理学::天文学
Citation statistics
Document Type期刊论文
Corresponding Author李槛杉
Affiliation1.中国科学院云南天文台, 昆明, 650011
2.中国科学院大学, 北京, 100049
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
李槛杉. 稳定物质转移通道形成双黑洞[J]. 天文学进展(Progress In Astronomy),2020,38(3):293-310.
APA 李槛杉.(2020).稳定物质转移通道形成双黑洞.天文学进展(Progress In Astronomy),38(3),293-310.
MLA 李槛杉."稳定物质转移通道形成双黑洞".天文学进展(Progress In Astronomy) 38.3(2020):293-310.
Files in This Item:
File Name/Size DocType Version Access License
稳定物质转移通道形成双黑洞_李槛杉.pd(2036KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[李槛杉]'s Articles
Baidu academic
Similar articles in Baidu academic
[李槛杉]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[李槛杉]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 稳定物质转移通道形成双黑洞_李槛杉.pdf
Format: Adobe PDF
All comments (0)
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.