Intermediate-mass ratio inspirals in merging elliptical galaxies
文献类型：期刊论文
| 作者 | Vazquez-Aceves, Veronica4; Amaro Seoane, Pau1,2,3,5,6,7; Kuvatova, Dana7; Makukov, Maxim7; Omarov, Chingis7; Yurin, Denis7 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2023 |
| 卷号 | 518期号:2页码:2113-2118 |
| ISSN号 | 0035-8711 |
| 关键词 | gravitational waves methods: analytical stars: black holes galaxies: interactions |
| DOI | 10.1093/mnras/stac3286 |
| 英文摘要 | Close encounters between two initially unbound objects can result in a binary system if enough energy is released as gravitational waves (GWs). We address the scenario in which such encounters occur in merging elliptical galaxies. There is evidence that elliptical galaxies can harbour intermediate-mass black holes (IMBHs). Therefore, these systems are potentially the breeding grounds of sources of GWs corresponding to inspiraling compact objects onto a massive black hole due to the dynamics, the large densities, and the number of compact remnants they contain. We show that this process is efficient for IMBHs with masses ranging from M is an element of (10(3), 10(5)) M-circle dot and results in the formation of intermediate-mass ratio inspirals (IMRIs). We consider a set of IMBIIs and smaller black holes with masses m(2) is an element of (10, 10(3)) M-circle dot to estimate the IMRI formation rate. We find rates ranging between 10(-8) and 10(-5) yr(-1), and the IMRI formation rate per comoving volume in merging galaxies as a function of the redshift. The peak frequencies of the gravitational radiation emitted when these IMRIs are formed are within the detection band of space-borne detectors such as the Laser Interferometer Space Antenna (LISA) and TianQin; taking into account the observable volume of these detectors, the total amount of IMRI detections per year is significant. |
| 资助项目 | Science Committee of the Ministry of Education and Science of the Republic of Kazakhstan[AP09259383] ; CAS-TWAS President's PhD Fellowship Program of the Chinese Academy of Sciences ; World Academy of Sciences ; National Key R&D Program of China[2016YFA0400702] ; National Science Foundation of China[11721303] ; 111 Project[B20063] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000898989100002 |
| 源URL | [http://ir.amss.ac.cn/handle/2S8OKBNM/60482]  |
| 专题 | 中国科学院数学与系统科学研究院 |
| 通讯作者 | Vazquez-Aceves, Veronica |
| 作者单位 | 1.Lanzhou Univ, Sch Phys Sci & Technol, Key Lab Theoret Phys Gansu Prov, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China 2.Lanzhou Univ, Inst Theoret Phys, Lanzhou 730000, Peoples R China 3.Lanzhou Univ, Res Ctr Gravitat, Lanzhou 730000, Peoples R China 4.Chinese Acad Sci, Inst Appl Math, Acad Math & Syst Sci, Beijing 100190, Peoples R China 5.Univ Politecn Valencia, Inst Multidisciplinary Math, Valencia 46022, Spain 6.Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 7.Fesenkov Astrophys Inst, Alma Ata 050020, Kazakhstan |
| 推荐引用方式 GB/T 7714 | Vazquez-Aceves, Veronica,Amaro Seoane, Pau,Kuvatova, Dana,et al. Intermediate-mass ratio inspirals in merging elliptical galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,518(2):2113-2118. |
| APA | Vazquez-Aceves, Veronica,Amaro Seoane, Pau,Kuvatova, Dana,Makukov, Maxim,Omarov, Chingis,&Yurin, Denis.(2023).Intermediate-mass ratio inspirals in merging elliptical galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,518(2),2113-2118. |
| MLA | Vazquez-Aceves, Veronica,et al."Intermediate-mass ratio inspirals in merging elliptical galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 518.2(2023):2113-2118. |
入库方式： OAI收割
来源：数学与系统科学研究院
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