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Tidal Disruptions of Stars by Supermassive and Intermediate-mass Black Hole Binaries: The Effects of the First-order Post-Newtonian Cross Terms

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成果类型:
期刊论文
作者:
Wu, Xiao-Jun;Luo, Yan;Li, Jie;Yuan, Ye-Fei;Lin, Wenbin
通讯作者:
Yuan, YF
作者机构:
[Wu, Xiao-Jun] China Jiliang Univ, Coll Modern Sci & Technol, Yiwu 322000, Zhejiang, Peoples R China.
[Lin, Wenbin; Li, Jie; Wu, Xiao-Jun] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
[Wu, Xiao-Jun] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
[Luo, Yan; Yuan, Ye-Fei] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China.
[Luo, Yan; Yuan, Ye-Fei] Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China.
通讯机构:
[Yuan, YF ] U
Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China.
Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China.
语种:
英文
期刊:
ASTROPHYSICAL JOURNAL
ISSN:
0004-637X
年:
2025
卷:
981
期:
1
页码:
23
基金类别:
the National Natural Science Foundation of China [12475057, 12433008]; National Natural Science Foundation of China [2020SKA0120300]; National SKA Program of China [XDB0550200]; Strategic Priority Research Program of the Chinese Academy of Sciences
机构署名:
本校为其他机构
院系归属:
核科学技术学院
数理学院
摘要:
In the vicinity of galactic nuclei, stars orbiting supermassive black hole (SMBH) binaries can undergo tidal disruption events (TDEs) due to the Lidov–Kozai mechanism and three-body interactions. While numerical simulations have incorporated post-Newtonian (PN) corrections up to 2.5PN order, they have not accounted for the 1PN cross-term effects among the three bodies. In this study, we employ N -body simulations to investigate the impact of the 1PN cross terms on the orbits of stars around an intermediate-mass black hole (IMBH) perturbed by a...

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