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Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band
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; Ping, Jinsong5; Lau, Yun-Kau2; Tang, Geshi1
2017-09-15
Source PublicationADVANCES IN SPACE RESEARCH
Volume60Issue:6Pages:1315-1326
AbstractThe 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.
SubtypeArticle
KeywordChang'e Lunar Mission Doppler Tracking Data Stochastic Background Of Gravitational Waves
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationStrategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; National Natural Science Foundation of China(11173005 ; National Natural Science Foundation of China(11173005 ; National Basic Research Program of China(2015CB857101) ; National Basic Research Program of China(2015CB857101) ; 11171329 ; 11171329 ; 61304233 ; 61304233 ; 41590851) ; 41590851) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; National Natural Science Foundation of China(11173005 ; National Natural Science Foundation of China(11173005 ; National Basic Research Program of China(2015CB857101) ; National Basic Research Program of China(2015CB857101) ; 11171329 ; 11171329 ; 61304233 ; 61304233 ; 41590851) ; 41590851)
DOI10.1016/j.asr.2017.06.008
Indexed BySCI
Language英语
Funding OrganizationStrategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; National Natural Science Foundation of China(11173005 ; National Natural Science Foundation of China(11173005 ; National Basic Research Program of China(2015CB857101) ; National Basic Research Program of China(2015CB857101) ; 11171329 ; 11171329 ; 61304233 ; 61304233 ; 41590851) ; 41590851) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB23030100) ; National Natural Science Foundation of China(11173005 ; National Natural Science Foundation of China(11173005 ; National Basic Research Program of China(2015CB857101) ; National Basic Research Program of China(2015CB857101) ; 11171329 ; 11171329 ; 61304233 ; 61304233 ; 41590851) ; 41590851)
WOS Research AreaAstronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
WOS SubjectAstronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences
WOS IDWOS:000410018100016
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20090
Collection月球与深空探测研究部
Affiliation1.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
Recommended Citation
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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