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Gravitational wave emission from close-in strange quark planets around strange stars with magnetic interactions
Zhang, Xiao-Li1; Zou, Ze-Cheng2; Huang, Yong-Feng2,3; Gao, Hao-Xuan4; Wang, Pei5,6; Cui, Lang7; Liu, Xiang7
2024-06-14
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume531Issue:4Pages:3905-3911
Contribution Rank7
AbstractAccording to the strange quark matter hypothesis, strange planets may exist, which are planetary mass objects composed of almost equal numbers of up, down, and strange quarks. A strange planet can revolve around its host strange star in a very close-in orbit. When it finally merges with the host, strong gravitational wave emissions will be generated. Here, the gravitational waveforms are derived for the merging process, taking into account the effects of the strange star's magnetic field on the dynamics. Effects of the inclination angle are also considered. Templates of the gravitational waveforms are derived. It is found that the magnetic interactions significantly speed up the merging process. Coalescence events of such strange planetary systems occurring in our Galaxy as well as in local galaxies can be effectively detected by current and future gravitational experiments, which may hopefully provide a new method to test the strange quark matter hypothesis and probe the magnetic field of compact stars.
Keywordgravitational waves exoplanets planet-star interactions binaries: general stars: magnetic fields stars: neutron
DOI10.1093/mnras/stae1400
Indexed BySCI
Language英语
WOS KeywordNEUTRON-STAR ; WHITE-DWARF ; COALESCENCE ; PROBE
Funding ProjectNational Natural Science Foundation of China[12233002] ; National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[U2031117] ; National Natural Science Foundation of China[2020SKA0120300] ; National Natural Science Foundation of China[2020SKA0120200] ; National Natural Science Foundation of China[2022SKA0120102] ; National Square Kilometer Array Program of China[2021YFA0718500] ; National Square Kilometer Array Program of China[2023YFE0102300] ; National Key Research and Development Program of China[2021-XBQNXZ-005] ; Chinese Academy of Sciences 'Light of West China' Program ; Xinjiang Tianshan Talent Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001247548400008
PublisherOXFORD UNIV PRESS
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Square Kilometer Array Program of China ; National Key Research and Development Program of China ; Chinese Academy of Sciences 'Light of West China' Program ; Xinjiang Tianshan Talent Program
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Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6809
Collection中国科学院新疆天文台
Corresponding AuthorHuang, Yong-Feng
Affiliation1.Nanjing Univ, Dept Phys, Nanjing 210093, Peoples R China
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
3.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China
4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
6.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
7.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Zhang, Xiao-Li,Zou, Ze-Cheng,Huang, Yong-Feng,et al. Gravitational wave emission from close-in strange quark planets around strange stars with magnetic interactions[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,531(4):3905-3911.
APA Zhang, Xiao-Li.,Zou, Ze-Cheng.,Huang, Yong-Feng.,Gao, Hao-Xuan.,Wang, Pei.,...&Liu, Xiang.(2024).Gravitational wave emission from close-in strange quark planets around strange stars with magnetic interactions.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,531(4),3905-3911.
MLA Zhang, Xiao-Li,et al."Gravitational wave emission from close-in strange quark planets around strange stars with magnetic interactions".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 531.4(2024):3905-3911.
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