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Inferring binary parameters with dual-line gravitational wave detection from tight inspiraling double neutron stars
Feng, Wen-Fan1,2; Chen, Jie-Wen3,4; Liu, Tan1,2,5,6; Wang, Yan1,2; Mohanty, Soumya D.7,8
2024-02-21
发表期刊PHYSICAL REVIEW D
ISSN2470-0010
卷号109期号:4页码:8
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.
资助者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)
DOI10.1103/PhysRevD.109.043033
关键词[WOS]DOUBLE COMPACT OBJECTS ; EQUATION-OF-STATE ; X-RAY BINARIES ; CONSTRAINTS ; INERTIA ; MOMENT ; POPULATION ; PRECESSION ; EXPLOSION ; SYSTEM
语种英语
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]
资助者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)
WOS研究方向Astronomy & Astrophysics ; Physics
WOS类目Astronomy & Astrophysics ; Physics, Particles & Fields
WOS记录号WOS:001186268100002
出版者AMER PHYSICAL SOC
引用统计
文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/14738
专题守时理论与方法研究室
通讯作者Liu, Tan
作者单位1.Huazhong Univ Sci & Technol, Dept Astron, MOE Key Lab Fundamental Phys Quant Measurements,Hu, PGMF, Wuhan 430074, Peoples R China
2.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Peoples R China
3.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China
4.Chinese Acad Sci, Key Lab Time & Frequency Primary Stand, Xian 710600, Peoples R China
5.UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
6.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
7.Univ Texas Rio Grande Valley, Dept Phys & Astron, Brownsville, TX 78520 USA
8.IIT Hyderabad, Dept Phys, Kandi 502284, India
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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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