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The TianQin project: Current progress on science and technology
Progress of Theoretical and Experimental Physics ( IF 3.5 ) Pub Date : 2020-08-04 , DOI: 10.1093/ptep/ptaa114
Jianwei Mei 1 , Yan-Zheng Bai 2 , Jiahui Bao 1 , Enrico Barausse 3 , Lin Cai 2 , Enrico Canuto 4 , Bin Cao 1 , Wei-Ming Chen 1 , Yu Chen 1 , Yan-Wei Ding 1 , Hui-Zong Duan 1 , Huimin Fan 2 , Wen-Fan Feng 2 , Honglin Fu 5 , Qing Gao 6 , TianQuan Gao 1 , Yungui Gong 2 , Xingyu Gou 7 , Chao-Zheng Gu 1 , De-Feng Gu 1 , Zi-Qi He 1 , Martin Hendry 8 , Wei Hong 2 , Xin-Chun Hu 2 , Yi-Ming Hu 1 , Yuexin Hu 9 , Shun-Jia Huang 1 , Xiang-Qing Huang 1 , Qinghua Jiang 7 , Yuan-Ze Jiang 1 , Yun Jiang 1 , Zhen Jiang 10, 11 , Hong-Ming Jin 2 , Valeriya Korol 12 , Hong-Yin Li 2 , Ming Li 1 , Ming Li 9 , Pengcheng Li 13 , Rongwang Li 5 , Yuqiang Li 5 , Zhu Li 1 , Zhulian Li 5 , Zhu-Xi Li 2 , Yu-Rong Liang 2 , Zheng-Cheng Liang 2 , Fang-Jie Liao 1 , Qi Liu 1 , Shuai Liu 1 , Yan-Chong Liu 2 , Li Liu 2 , Pei-Bo Liu 1 , Xuhui Liu 7 , Yuan Liu 1 , Xiong-Fei Lu 1 , Yang Lu 1 , Ze-Huang Lu 2 , Yan Luo 1 , Zhi-Cai Luo 2 , Vadim Milyukov 14 , Min Ming 2 , Xiaoyu Pi 5 , Chenggang Qin 2 , Shao-Bo Qu 2 , Alberto Sesana 15 , Chenggang Shao 2 , Changfu Shi 1 , Wei Su 2 , Ding-Yin Tan 2 , Yujie Tan 2 , Zhuangbin Tan 1 , Liang-Cheng Tu 1, 2 , Bin Wang 16 , Cheng-Rui Wang 2 , Fengbin Wang 9 , Guan-Fang Wang 1 , Haitian Wang 17 , Jian Wang 1 , Lijiao Wang 7 , Panpan Wang 2 , Xudong Wang 7 , Yan Wang 2 , Yi-Fan Wang 18, 19 , Ran Wei 20 , Shu-Chao Wu 2 , Chun-Yu Xiao 2 , Xiao-Shi Xu 1 , Chao Xue 1 , Fang-Chao Yang 2 , Liang Yang 1 , Ming-Lin Yang 1 , Shan-Qing Yang 1 , Bobing Ye 1 , Hsien-Chi Yeh 1 , Shenghua Yu 11 , Dongsheng Zhai 5 , Caishi Zhang 1 , Haitao Zhang 5 , Jian-dong Zhang 1 , Jie Zhang 2 , Lihua Zhang 9 , Xin Zhang 21 , Xuefeng Zhang 1 , Hao Zhou 2 , Ming-Yue Zhou 2 , Ze-Bing Zhou 2 , Dong-Dong Zhu 2 , Tie-Guang Zi 1 , Jun Luo 1, 2
Affiliation  

TianQin is a planned space-based gravitational wave (GW) observatory consisting of three earth orbiting satellites with an orbital radius of about $10^5~{\rm km}$. The satellites will form a equilateral triangle constellation the plane of which is nearly perpendicular to the ecliptic plane. TianQin aims to detect GWs between $10^{-4}~{\rm Hz}$ and $1~{\rm Hz}$ that can be generated by a wide variety of important astrophysical and cosmological sources, including the inspiral of Galactic ultra-compact binaries, the inspiral of stellar-mass black hole binaries, extreme mass ratio inspirals, the merger of massive black hole binaries, and possibly the energetic processes in the very early universe or exotic sources such as cosmic strings. In order to start science operations around 2035, a roadmap called the 0123 plan is being used to bring the key technologies of TianQin to maturity, supported by the construction of a series of research facilities on the ground. Two major projects of the 0123 plan are being carried out. In this process, the team has created a new generation $17~{\rm cm}$ single-body hollow corner-cube retro-reflector which has been launched with the QueQiao satellite on 21 May 2018; a new laser ranging station equipped with a $1.2~{\rm m}$ telescope has been constructed and the station has successfully ranged to all the five retro-reflectors on the Moon; and the TianQin-1 experimental satellite has been launched on 20 December 2019 and the first round result shows that the satellite has exceeded all of its mission requirements.

中文翻译:

天琴计划:科学技术现状

天琴是一个计划中的天基引力波(GW)天文台,由三颗地球轨道卫星组成,轨道半径约为$10^5~{\rm km}$。这些卫星将形成一个等边三角形星座,其平面几乎垂直于黄道平面。TianQin 的目标是检测 $10^{-4}~{\rm Hz}$ 和 $1~{\rm Hz}$ 之间的引力波,这些引力波可以由各种重要的天体物理和宇宙学来源产生,包括银河超致密双星、恒星质量黑洞双星的螺旋、极端质量比的螺旋、大质量黑洞双星的合并,以及可能是早期宇宙中的能量过程或外来源,如宇宙弦。为了在 2035 年左右开始科学运作,以“0123计划”为路线图,通过一系列地面研究设施的建设,使天琴的关键技术走向成熟。0123计划的两个重大项目正在实施。在这个过程中,团队创造了新一代$17~{\rm cm}$单体空心角立方回归反射器,并于2018年5月21日与雀桥卫星一起发射;一个配备 1.2~{\rm m}$ 望远镜的新激光测距站已经建成,并且该站已成功测到月球上的所有五个后向反射器;天琴一号实验卫星已于2019年12月20日发射,首轮结果显示,该卫星已超出其所有任务要求。支持在地面建设一系列研究设施。0123计划的两个重大项目正在实施。在这个过程中,团队创造了新一代$17~{\rm cm}$单体空心角立方回归反射器,并于2018年5月21日与雀桥卫星一起发射;一个配备 1.2~{\rm m}$ 望远镜的新激光测距站已经建成,并且该站已成功测到月球上的所有五个后向反射器;天琴一号实验卫星已于2019年12月20日发射,首轮结果显示,该卫星已超出其所有任务要求。支持在地面建设一系列研究设施。0123计划的两个重大项目正在实施中。在这个过程中,团队创造了新一代$17~{\rm cm}$单体空心角立方回归反射器,并于2018年5月21日与雀桥卫星一起发射;一个配备 1.2~{\rm m}$ 望远镜的新激光测距站已经建成,并且该站已成功测到月球上的所有五个后向反射器;天琴一号实验卫星已于2019年12月20日发射,首轮结果显示,该卫星已超出其所有任务要求。该团队创造了新一代$17~{\rm cm}$单体空心角立方体后向反射器,并于2018年5月21日随鹊桥卫星一起发射;一个配备 1.2~{\rm m}$ 望远镜的新激光测距站已经建成,并且该站已成功测到月球上的所有五个后向反射器;天琴一号实验卫星已于2019年12月20日发射,首轮结果显示,该卫星已超出其所有任务要求。该团队创造了新一代$17~{\rm cm}$单体空心角立方体后向反射器,并于2018年5月21日随鹊桥卫星一起发射;一个配备 1.2~{\rm m}$ 望远镜的新激光测距站已经建成,并且该站已成功测到月球上的所有五个后向反射器;天琴一号实验卫星已于2019年12月20日发射,首轮结果显示,该卫星已超出其所有任务要求。
更新日期:2020-08-04
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