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

doi:10.1016/j.asr.2017.06.008

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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, Peng 2; Hu, Songjie 1; Cao, Jianfeng 1; Dong, Peng 4; Bu, Yanlong 1; Chen, Lue 1,5,6; Han, Songtao 1,5; Gong, Xuefei2 ; Li, Wenxiao 5,6; Ping, Jinsong 5; Lau, Yun-Kau2 ; Tang, Geshi 1
	2017-09-15
发表期刊	ADVANCES IN SPACE RESEARCH
ISSN	0273-1177
卷号	60 期号:6 页码:1315-1326
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.
关键词	Chang'e lunar mission Doppler tracking data Stochastic background of gravitational waves
DOI	10.1016/j.asr.2017.06.008
语种	英语
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
WOS类目	Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences
WOS记录号	WOS:000410018100016
出版者	ELSEVIER SCI LTD
引用统计
文献类型	期刊论文
条目标识符	http://ir.amss.ac.cn/handle/2S8OKBNM/26400
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.