KMS Of Academy of mathematics and systems sciences, CAS
| Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism | |
Cao, Zhoujian1,2 ; Han, Wen-Biao3,4
| |
| 2017-08-23 | |
| Source Publication | PHYSICAL REVIEW D
 |
| ISSN | 2470-0010 |
| Volume | 96Issue:4Pages:23 |
| Abstract | Binary black hole systems are among the most important sources for gravitational wave detection. They are also good objects for theoretical research for general relativity. A gravitational waveform template is important to data analysis. An effective-one-body-numerical-relativity (EOBNR) model has played an essential role in the LIGO data analysis. For future space-based gravitational wave detection, many binary systems will admit a somewhat orbit eccentricity. At the same time, the eccentric binary is also an interesting topic for theoretical study in general relativity. In this paper, we construct the first eccentric binary waveform model based on an effective-one-body-numerical-relativity framework. Our basic assumption in the model construction is that the involved eccentricity is small. We have compared our eccentric EOBNR model to the circular one used in the LIGO data analysis. We have also tested our eccentric EOBNR model against another recently proposed eccentric binary waveform model; against numerical relativity simulation results; and against perturbation approximation results for extreme mass ratio binary systems. Compared to numerical relativity simulations with an eccentricity as large as about 0.2, the overlap factor for our eccentric EOBNR model is better than 0.98 for all tested cases, including spinless binary and spinning binary, equal mass binary, and unequal mass binary. Hopefully, our eccentric model can be the starting point to develop a faithful template for future space-based gravitational wave detectors. |
| DOI | 10.1103/PhysRevD.96.044028 |
| Language | 英语 |
| Funding Project | NSFC[11690023] ; NSFC[11622546] ; NSFC[11375260] ; NSFC[U1431120] ; Fundamental Research Funds for the Central Universities ; Youth Innovation Promotion Association CAS ; CAS[QYZDB-SSW-SYS016] |
| WOS Research Area | Astronomy & Astrophysics ; Physics |
| WOS Subject | Astronomy & Astrophysics ; Physics, Particles & Fields |
| WOS ID | WOS:000408207500001 |
| Publisher | AMER PHYSICAL SOC |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.amss.ac.cn/handle/2S8OKBNM/26274 |
| Collection | 应用数学研究所 |
| Corresponding Author | Cao, Zhoujian |
| Affiliation | 1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 2.Chinese Acad Sci, Acad Math & Syst Sci, Inst Appl Math, Beijing 100190, Peoples R China 3.Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 4.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China |
| Recommended Citation GB/T 7714 | Cao, Zhoujian,Han, Wen-Biao. Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism[J]. PHYSICAL REVIEW D,2017,96(4):23. |
| APA | Cao, Zhoujian,&Han, Wen-Biao.(2017).Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism.PHYSICAL REVIEW D,96(4),23. |
| MLA | Cao, Zhoujian,et al."Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism".PHYSICAL REVIEW D 96.4(2017):23. |
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