Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
文献类型:期刊论文
作者 | Liu, Chang1,2; Kang, Yacheng1,2; Shao, Lijing2,3 |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 2022-07-01 |
卷号 | 934期号:1页码:11 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ac7a39 |
英文摘要 | We investigated the detection rates and early-warning parameters of binary neutron star (BNS) populations with decihertz gravitational-wave observatories in a realistic detecting strategy. Assuming the operation time of B-DECIGO is 4 yr, we classified the detectable BNSs based on parameter precision into three categories: (a) sources that merge within 1 yr, which could be localized with an uncertainty of Delta omega similar to 10(0) deg(2); (b) sources that merge in 1-4 yr, which take up three-quarters of the total events and yield the most precise angular resolution with Delta omega similar to 10(-2) deg(2) and time-of-merger accuracy with Delta t ( c ) similar to 10(-1) s; and (c) sources that do not merge during the 4 yr mission window, which enable possible early warnings, with Delta omega similar to 10(-1) deg(2) and Delta t ( c ) similar to 10(0) s. Furthermore, we compared the pros and cons of B-DECIGO with the third-generation ground-based detectors, and explored the prospects of detections using three other decihertz observatories and four BNS population models. In realistic observing scenarios, we found that decihertz detectors could even provide early-warning alerts to a source decades before its merger while their localizations are still as accurate as ground-based facilities. Finally we found a decrease of events when considering the confusion noise, but this could be partially solved by a proper noise subtraction. |
WOS关键词 | LUMINOSITY FUNCTION ; MERGERS |
资助项目 | National Natural Science Foundation of China[11975027] ; National Natural Science Foundation of China[11991053] ; National Natural Science Foundation of China[11721303] ; National SKA Program of China[2020SKA0120300] ; Max Planck Partner Group Program - Max Planck Society ; High-Performance Computing Platform of Peking University |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000830788300001 |
出版者 | IOP Publishing Ltd |
资助机构 | National Natural Science Foundation of China ; National Natural Science Foundation of China ; National SKA Program of China ; National SKA Program of China ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; High-Performance Computing Platform of Peking University ; High-Performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National SKA Program of China ; National SKA Program of China ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; High-Performance Computing Platform of Peking University ; High-Performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National SKA Program of China ; National SKA Program of China ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; High-Performance Computing Platform of Peking University ; High-Performance Computing Platform of Peking University ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National SKA Program of China ; National SKA Program of China ; Max Planck Partner Group Program - Max Planck Society ; Max Planck Partner Group Program - Max Planck Society ; High-Performance Computing Platform of Peking University ; High-Performance Computing Platform of Peking University |
源URL | [http://ir.bao.ac.cn/handle/114a11/87883] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Shao, Lijing |
作者单位 | 1.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 2.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Liu, Chang,Kang, Yacheng,Shao, Lijing. Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories[J]. ASTROPHYSICAL JOURNAL,2022,934(1):11. |
APA | Liu, Chang,Kang, Yacheng,&Shao, Lijing.(2022).Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories.ASTROPHYSICAL JOURNAL,934(1),11. |
MLA | Liu, Chang,et al."Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories".ASTROPHYSICAL JOURNAL 934.1(2022):11. |
入库方式: OAI收割
来源:国家天文台
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