Probing supermassive black hole binaries with orbital resonances of laser-ranged satellites | |
Du MH(杜明辉); Deng Q(邓琼); Bian YF(卞艺帆); Luo ZR(罗子人)![]() | |
发表期刊 | EUROPEAN PHYSICAL JOURNAL C
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2023-06-30 | |
卷号 | 83期号:6页码:554 |
ISSN | 1434-6044 |
摘要 | Coalescing supermassive black hole binaries (SMBHBs) are the primary source candidates for low frequency gravitational wave (GW) detections, which could bring us deep insights into galaxy evolutions over cosmic time and violent processes of spacetime dynamics. Promising candidates had been found based on optical and X-ray observations, which claims for new and ready-to-use GW detection approaches before the operations of space-borne antennas. We show that, satellite laser ranging (SLR) missions could serve as probes of coalescing SMBHBs through the GW-induced resonant effects. Lasting and characteristic imprints caused by such resonances in the residual distances or accelerations from SLR measurements are studied, and the detection SNR is analyzed with both the current and future improved ranging precisions. Within redshift z similar to 1, the threshold SNR = 5 requires 1-2 years of accumulated data for the current precision and months of data for improved precision, which are workable for the data processing of SLR missions. Meanwhile, joint detections with multiple SLR missions could further improve the total SNR and the confidence level. Such a detection scheme could fulfill the requirement of a tentative SMBHB probe during the preparing stage of LISA and Taiji, and it requires no further investment to any new and advanced facilities. It is also worthwhile to look back and re-process the archived data from the past decades, in where resonant signals from SMBHBs might be hidden. |
DOI | 10.1140/epjc/s10052-023-11748-9 |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:001022393100002 |
WOS研究方向 | Physics |
WOS类目 | Physics, Particles & Fields |
项目资助者 | National Key Research and Development Program of China [2020YFC2200601, 2021YFC2201901] |
论文分区 | 二类/Q1 |
力学所作者排名 | 1 |
RpAuthor | Xu, P (corresponding author), Chinese Acad Sci, Inst Mech, Ctr Gravitat Wave Expt, Natl Micrograv Lab, Beijing 100190, Peoples R China. ; Xu, P (corresponding author), Lanzhou Univ, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China. ; Xu, P (corresponding author), Univ Chinese Acad Sci, Taiji Lab Gravitat Wave Universe Beijing Hangzhou, Beijing 100049, Peoples R China. ; Xu, P (corresponding author), Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Hangzhou 310124, Peoples R China. |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://dspace.imech.ac.cn/handle/311007/92598 |
专题 | 微重力重点实验室 |
作者单位 | 1.{Du, Minghui, Deng, Qiong, Luo, Ziren, Xu, Peng} Chinese Acad Sci, Inst Mech, Ctr Gravitat Wave Expt, Natl Micrograv Lab, Beijing 100190, Peoples R China 2.{Deng, Qiong, Bian, Yifan, Xu, Peng} Lanzhou Univ, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China 3.{Luo, Ziren, Xu, Peng} Univ Chinese Acad Sci, Taiji Lab Gravitat Wave Universe Beijing Hangzhou, Beijing 100049, Peoples R China 4.{Luo, Ziren, Xu, Peng} Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Hangzhou 310124, Peoples R China |
推荐引用方式 GB/T 7714 | Du MH,Deng Q,Bian YF,et al. Probing supermassive black hole binaries with orbital resonances of laser-ranged satellites[J]. EUROPEAN PHYSICAL JOURNAL C,2023,83,6,:554.Rp_Au:Xu, P (corresponding author), Chinese Acad Sci, Inst Mech, Ctr Gravitat Wave Expt, Natl Micrograv Lab, Beijing 100190, Peoples R China., Xu, P (corresponding author), Lanzhou Univ, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China., Xu, P (corresponding author), Univ Chinese Acad Sci, Taiji Lab Gravitat Wave Universe Beijing Hangzhou, Beijing 100049, Peoples R China., Xu, P (corresponding author), Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Hangzhou 310124, Peoples R China. |
APA | 杜明辉,邓琼,卞艺帆,罗子人,&徐鹏.(2023).Probing supermassive black hole binaries with orbital resonances of laser-ranged satellites.EUROPEAN PHYSICAL JOURNAL C,83(6),554. |
MLA | 杜明辉,et al."Probing supermassive black hole binaries with orbital resonances of laser-ranged satellites".EUROPEAN PHYSICAL JOURNAL C 83.6(2023):554. |
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