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Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band

文献类型：期刊论文

作者Tang, Wenlin1,2,3; Xu, Peng2; Hu, Songjie1; Cao, Jianfeng1; Dong, Peng4; Bu, Yanlong1; Chen, Lue1,5,6; Han, Songtao1,5; Gong, Xuefei2; Li, Wenxiao5,6
刊名ADVANCES IN SPACE RESEARCH
出版日期2017-09-15
卷号60期号:6页码:1315-1326
关键词Chang'e lunar mission Doppler tracking data Stochastic background of gravitational waves
ISSN号0273-1177
DOI10.1016/j.asr.2017.06.008
英文摘要The Doppler tracking data of the Chang'e 3 lunar mission is used to constrain the stochastic background of gravitational wave in cosmology within the 1 mHz to 0.05 Hz frequency band. Our result improves on the upper bound on the energy density of the stochastic background of gravitational wave in the 0.02-0.05 Hz band obtained by the Apollo missions, with the improvement reaching almost one order of magnitude at around 0.05 Hz. Detailed noise analysis of the Doppler tracking data is also presented, with the prospect that these noise sources will be mitigated in future Chinese deep space missions. A feasibility study is also undertaken to understand the scientific capability of the Chang'e 4 mission, due to be launched in 2018, in relation to the stochastic gravitational wave background around 0.01 Hz. The study indicates that the upper bound on the energy density may be further improved by another order of magnitude from the Chang'e 3 mission, which will fill the gap in the frequency band from 0.02 Hz to 0.1 Hz in the foreseeable future. (C) 2017 COSPAR. Published by Elsevier Ltd. All rights reserved.
资助项目Strategic Priority Research Program of the Chinese Academy of Sciences[XDB23030100] ; National Natural Science Foundation of China[11173005] ; National Natural Science Foundation of China[11171329] ; National Natural Science Foundation of China[61304233] ; National Natural Science Foundation of China[41590851] ; National Basic Research Program of China[2015CB857101]
WOS研究方向Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
WOS记录号WOS:000410018100016
出版者ELSEVIER SCI LTD
源URL[http://ir.amss.ac.cn/handle/2S8OKBNM/26399]  
专题应用数学研究所
国家数学与交叉科学中心
通讯作者Lau, Yun-Kau; Tang, Geshi
作者单位1.Beijing Aerosp Control Ctr, Sci & Technol Aerosp Flight Dynam Lab, Beijing, Peoples R China
2.Chinese Acad Sci, Acad Math & Syst Sci, Inst Computat Math, Inst Appl Math,Morningside Ctr Math & LESC, Beijing, Peoples R China
3.Beihang Univ, Sch Astronaut, Dept Aerosp Guidance Nav & Control, Beijing, Peoples R China
4.Beijing Inst Aerosp Control Devices, Beijing, Peoples R China
5.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
6.Univ Chinese Acad Sci, Beijing, Peoples R China
推荐引用方式
GB/T 7714		 Tang, Wenlin,Xu, Peng,Hu, Songjie,et al. Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band[J]. ADVANCES IN SPACE RESEARCH,2017,60(6):1315-1326.
APA Tang, Wenlin.,Xu, Peng.,Hu, Songjie.,Cao, Jianfeng.,Dong, Peng.,...&Tang, Geshi.(2017).Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band.ADVANCES IN SPACE RESEARCH,60(6),1315-1326.
MLA Tang, Wenlin,et al."Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band".ADVANCES IN SPACE RESEARCH 60.6(2017):1315-1326.

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来源：数学与系统科学研究院

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