IMECH-IR  > 微重力重点实验室
Distinguishability of binary extreme-mass-ratio inspirals in low frequency band
Jiang, Ye; Han, WenBiao; Zhong, XingYu; Shen, Ping; Luo ZR(罗子人); Wu YL(吴岳良)
Corresponding AuthorHan, Wen-Biao([email protected])
Source PublicationEUROPEAN PHYSICAL JOURNAL C
2024-05-08
Volume84Issue:5Pages:15
ISSN1434-6044
AbstractThe inspiral of compact stellar objects into massive black holes are one of the main astrophysical sources for the Laser Interferometer Space Antenna (LISA) and Taiji. These extreme-mass-ratio inspirals (EMRIs) have great potential for cosmology and fundamental physics. A binary extreme-mass-ratio inspiral (b-EMRI) describes the case where binary black holes (BBHs) are captured by a supermassive black hole. The b-EMRIs serve as multi-band gravitational wave sources and provide insights into the dynamics of nuclei and tests of general relativity. However, if the b-EMRIs can be distinguished from the normal EMRIs or not is still not clear. In this work, with a few of assumptions, and using the Teukolsky equation, we calculate the approximate gravitational waves of b-EMRIs and assess their detectability by space-based detectors. We also decouple the secondary object information from the Teukolsky equation, enabling us to calculate the energy fluxes and generate the waveforms more conveniently. Variations in the quadrupole of the binary result in small but non-negligible changes in energy fluxes and waveforms, making it possible to distinguish b-EMRI signals with data analysis. This opens up the potential of using b-EMRIs to test gravity theories and for further astrophysical studies.
DOI10.1140/epjc/s10052-024-12841-3
Indexed BySCI
Language英语
WOS IDWOS:001219585700004
WOS KeywordEVALUATE HOMOGENEOUS SOLUTIONS ; ROTATING BLACK-HOLE ; GENERAL-RELATIVITY ; EXTENDED BODIES ; GRAVITATIONAL-WAVES ; TEUKOLSKY EQUATION ; NUMERICAL-METHODS ; DYNAMICS ; PERTURBATIONS ; ASTROPHYSICS
WOS Research AreaPhysics
WOS SubjectPhysics, Particles & Fields
Funding ProjectNational Key R &D Program of China[2021YFC2203002] ; National Key R &D Program of China[2020YFC 2201501] ; National Natural Science Foundation of China[11773059] ; National Natural Science Foundation of China[12173071] ; National Natural Science Foundation of China[12147103] ; National Natural Science Foundation of China[11821505] ; Strategic Priority Research Program of the CAS[XDA15021102]
Funding OrganizationNational Key R &D Program of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the CAS
Classification二类/Q1
Ranking3+
ContributorHan, Wen-Biao
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://dspace.imech.ac.cn/handle/311007/95352
Collection微重力重点实验室
Recommended Citation
GB/T 7714
Jiang, Ye,Han, WenBiao,Zhong, XingYu,et al. Distinguishability of binary extreme-mass-ratio inspirals in low frequency band[J]. EUROPEAN PHYSICAL JOURNAL C,2024,84,5,:15.Rp_Au:Han, Wen-Biao
APA Jiang, Ye,Han, WenBiao,Zhong, XingYu,Shen, Ping,罗子人,&吴岳良.(2024).Distinguishability of binary extreme-mass-ratio inspirals in low frequency band.EUROPEAN PHYSICAL JOURNAL C,84(5),15.
MLA Jiang, Ye,et al."Distinguishability of binary extreme-mass-ratio inspirals in low frequency band".EUROPEAN PHYSICAL JOURNAL C 84.5(2024):15.
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