| Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications | |
| Li LF(李丽仿); Cao, Zhoujian | |
| Source Publication | GENERAL RELATIVITY AND GRAVITATION
 |
| 2023-06 | |
| Volume | 55Issue:6Pages:76 |
| ISSN | 0001-7701 |
| Abstract | Binary compact objects will be among the important sources for the future space-based gravitational wave detectors. Such binary compact objects include stellar massive binary black hole, binary neutron star, binary white dwarf and mixture of these compact objects. Regarding to the relatively low frequency, the gravitational interaction between the two objects of the binary is weak. Post-Newtonian approximation of general relativity is valid. Previous works about the waveform model for such binaries in the literature consider the dynamics for specific situations which involve detailed complicated matter dynamics between the two objects. We here take a different idea. We adopt the trick used in pulsar timing detection. For any gravity theories and any detailed complicated matter dynamics, the motion of the binary can always be described as a post-Keplerian expansion. And a post-Keplerian gravitational waveform model will be reduced. Instead of object masses, spins, matter's equation of state parameters and dynamical parameters beyond general relativity, the involved parameters in our post-Keplerian waveform model are the Keplerian orbit elements and their adiabatic variations. Respect to current planning space-based gravitational wave detectors including LISA, Taiji and Tianqin, we find that the involved waveform model parameters can be well determined. And consequently the detail matter dynamics of the binary can be studied then. For binary with purely gravitational interactions, gravity theory can be constrained well. |
| Keyword | Gravitational wave Post-Keplerian waveform model Binary compact object Tidal interaction Mass transfer |
| DOI | 10.1007/s10714-023-03123-6 |
| Indexed By | SCI |
| Language | 英语 |
| WOS ID | WOS:001007099100002 |
| WOS Research Area | Astronomy & Astrophysics ; Physics, Multidisciplinary ; Physics, Particles & Fields |
| Funding Organization | National Key Research and Development Program of China [2021YFC2203001] ; CAS Project for Young Scientists in Basic Research [YSBR-006] |
| Classification | 二类 |
| Ranking | 1 |
| Contributor | Cao, ZJ (corresponding author), Chinese Acad Sci, Inst Appl Math, Acad Math & Syst Sci, Beijing 100190, Peoples R China. ; Cao, ZJ (corresponding author), UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China. |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://dspace.imech.ac.cn/handle/311007/92386 |
| Collection | 微重力重点实验室 |
| Affiliation | 1.{Li Li-Fang} Chinese Acad Sci Inst Mech Beijing 100190 Peoples R China 2.{Cao Zhoujian} Chinese Acad Sci Inst Appl Math Acad Math & Syst Sci Beijing 100190 Peoples R China 3.{Cao Zhoujian} UCAS Hangzhou Inst Adv Study Sch Fundamental Phys & Math Sci Hangzhou 310024 Peoples R China |
| Recommended Citation GB/T 7714 | Li LF,Cao, Zhoujian. Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications[J]. GENERAL RELATIVITY AND GRAVITATION,2023,55,6,:76.Rp_Au:Cao, ZJ (corresponding author), Chinese Acad Sci, Inst Appl Math, Acad Math & Syst Sci, Beijing 100190, Peoples R China., Cao, ZJ (corresponding author), UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China. |
| APA | 李丽仿,&Cao, Zhoujian.(2023).Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications.GENERAL RELATIVITY AND GRAVITATION,55(6),76. |
| MLA | 李丽仿,et al."Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications".GENERAL RELATIVITY AND GRAVITATION 55.6(2023):76. |
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| Jp2023A172.pdf（474KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Download | |
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