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Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars

文献类型：期刊论文

作者Feng, Wen-Fan7,8; Chen, Jie-Wen5,6; Liu, Tan3,4,7,8; Wang, Yan7,8; Mohanty, Soumya D.1,2
刊名PHYSICAL REVIEW D
出版日期2024-02-21
卷号109期号:4页码:8
ISSN号2470-0010
DOI10.1103/PhysRevD.109.043033
英文摘要Neutron star (NS) binaries can be potentially intriguing gravitational wave sources, with both high- and low-frequency radiation from the possibly aspherical individual stars and the binary orbit, respectively. The successful detection of such a dual-line source could provide fresh insights into binary geometry and NS physics. In the absence of electromagnetic observations, we develop a strategy for inferring the spin-orbit misalignment angle using the tight dual-line double NS system under the spin-orbit coupling. Based on the four-year joint detection of a typical dual-line system with the Laser Interferometer Space Antenna and Cosmic Explorer, we find that the misalignment angle and the NS moment of inertia can be measured with subpercentage and 5% accuracy, respectively.
WOS关键词DOUBLE COMPACT OBJECTS ; EQUATION-OF-STATE ; X-RAY BINARIES ; CONSTRAINTS ; INERTIA ; MOMENT ; POPULATION ; PRECESSION ; EXPLOSION ; SYSTEM
资助项目National Key Research and Development Program of China[2022YFC2205201] ; National Key Research and Development Program of China[2020YFC2201400] ; National Natural Science Foundation of China (NSFC)[11973024] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; Guangdong Major Project of Basic and Applied Basic Research[2019B030302001] ; U.S. National Science Foundation (NSF)[PHY-2207935]
WOS研究方向Astronomy & Astrophysics ; Physics
语种英语
WOS记录号WOS:001186268100002
出版者AMER PHYSICAL SOC
资助机构National Key Research and Development Program of China ; National Key Research and Development Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guangdong Major Project of Basic and Applied Basic Research ; Guangdong Major Project of Basic and Applied Basic Research ; U.S. National Science Foundation (NSF) ; U.S. National Science Foundation (NSF) ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guangdong Major Project of Basic and Applied Basic Research ; Guangdong Major Project of Basic and Applied Basic Research ; U.S. National Science Foundation (NSF) ; U.S. National Science Foundation (NSF) ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guangdong Major Project of Basic and Applied Basic Research ; Guangdong Major Project of Basic and Applied Basic Research ; U.S. National Science Foundation (NSF) ; U.S. National Science Foundation (NSF) ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Guangdong Major Project of Basic and Applied Basic Research ; Guangdong Major Project of Basic and Applied Basic Research ; U.S. National Science Foundation (NSF) ; U.S. National Science Foundation (NSF)
源URL[http://210.72.145.45/handle/361003/14738]  
专题国家授时中心_守时理论与方法研究室
通讯作者Liu, Tan
作者单位1.IIT Hyderabad, Dept Phys, Kandi 502284, India
2.Univ Texas Rio Grande Valley, Dept Phys & Astron, Brownsville, TX 78520 USA
3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
4.UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
5.Chinese Acad Sci, Key Lab Time & Frequency Primary Stand, Xian 710600, Peoples R China
6.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China
7.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Peoples R China
8.Huazhong Univ Sci & Technol, Dept Astron, MOE Key Lab Fundamental Phys Quant Measurements,Hu, PGMF, Wuhan 430074, Peoples R China
推荐引用方式
GB/T 7714		 Feng, Wen-Fan,Chen, Jie-Wen,Liu, Tan,et al. Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars[J]. PHYSICAL REVIEW D,2024,109(4):8.
APA Feng, Wen-Fan,Chen, Jie-Wen,Liu, Tan,Wang, Yan,&Mohanty, Soumya D..(2024).Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars.PHYSICAL REVIEW D,109(4),8.
MLA Feng, Wen-Fan,et al."Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars".PHYSICAL REVIEW D 109.4(2024):8.

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