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 | |
发表期刊 | PHYSICAL REVIEW D |
ISSN | 2470-0010 |
卷号 | 96期号:4页码:23 |
摘要 | 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 |
语种 | 英语 |
资助项目 | 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研究方向 | Astronomy & Astrophysics ; Physics |
WOS类目 | Astronomy & Astrophysics ; Physics, Particles & Fields |
WOS记录号 | WOS:000408207500001 |
出版者 | AMER PHYSICAL SOC |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.amss.ac.cn/handle/2S8OKBNM/26274 |
专题 | 应用数学研究所 |
通讯作者 | Cao, Zhoujian |
作者单位 | 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 |
推荐引用方式 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. |
条目包含的文件 | 条目无相关文件。 |
个性服务 |
推荐该条目 |
保存到收藏夹 |
查看访问统计 |
导出为Endnote文件 |
谷歌学术 |
谷歌学术中相似的文章 |
[Cao, Zhoujian]的文章 |
[Han, Wen-Biao]的文章 |
百度学术 |
百度学术中相似的文章 |
[Cao, Zhoujian]的文章 |
[Han, Wen-Biao]的文章 |
必应学术 |
必应学术中相似的文章 |
[Cao, Zhoujian]的文章 |
[Han, Wen-Biao]的文章 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论