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Gravitational wave astronomy with TianQin
Li, En-Kun1,2,3; Liu, Shuai4; Torres-Orjuela, Alejandro5,6; Chen, Xian7; Inayoshi, Kohei7; Wang, Long1; Hu, Yi-Ming1,2,3; Amaro-Seoane, Pau8; Askar, Abbas9; Bambi, Cosimo10,11,12; Capelo, Pedro R.; Chen, Hong-Yu1,2,3; Chua, Alvin J. K.13,14; Condes-Brena, Enrique7; Dai, Lixin6; Das, Debtroy10,11; Derdzinski, Andrea15,16; Fan, Hui-Min17; Fujii, Michiko18; Gao, Jie1,2; Garg, Mudit; Ge HW(葛宏伟)19,20,21; Giersz, Mirek9; Huang, Shun-Jia22; Hypki, Arkadiusz9,35; Liang, Zheng-Cheng3; Liu, Bin23; Liu, Dongdong; Liu, Miaoxin; Liu, Yunqi; Mayer, Lucio; Napolitano, Nicola R.24; Peng, Peng7; Shao, Yong25; Shashank, Swarnim10,11; Shen, Rongfeng1; Tagawa, Hiromichi26; Tanikawa, Ataru7,27; Toscani, Martina28,34; Vazquez-Aceves, Veronica7; Wang, Hai-Tian; Wang, Han1,2,3; Yi, Shu-Xu1,2,29; Zhang, Jian-dong1,2,3; Zhang, Xue-Ting1,2,3; Zhu, Lianggui7; Zwick, Lorenz30; Huang, Song31; Mei, Jianwei1,2,3; Wang, Yan32; Xie, Yi33; Zhang, Jianjun; Luo, Jun3
发表期刊REPORTS ON PROGRESS IN PHYSICS (IF:14.257[JCR-2017],16.214[5-Year])
2025-05-01
卷号88期号:5
DOI10.1088/1361-6633/adc9be
产权排序第19完成单位
收录类别SCI
关键词gravitational wave astronomy TianQin
摘要The opening of the gravitational wave window has significantly enhanced our capacity to explore the Universe's most extreme and dynamic sector. In the mHz frequency range, a diverse range of compact objects, from the most massive black holes at the farthest reaches of the Universe to the lightest white dwarfs in our cosmic backyard, generate a complex and dynamic symphony of gravitational wave signals. Once recorded by gravitational wave detectors, these unique fingerprints have the potential to decipher the birth and growth of cosmic structures over a wide range of scales, from stellar binaries and stellar clusters to galaxies and large-scale structures. The TianQin space-borne gravitational wave mission is scheduled for launch in the 2030s, with an operational lifespan of five years. It will facilitate pivotal insights into the history of our Universe. This document presents a concise overview of the detectable sources of TianQin, outlining their characteristics, the challenges they present, and the expected impact of the TianQin observatory on our understanding of them.
资助项目Sinergia[2019B030302001]; Guangdong Major Project of Basic and Applied Basic Research[2020YFC2201400]; National Key Research and Development Program of China[12250610185]; National Key Research and Development Program of China[12261131497]; Natural Science Foundation of China[22ZR1403400]; Natural Science Foundation of Shanghai[CRSII5_213497]; Swiss National Science Foundation under the Sinergia[AST-2319441]; National Science Foundation[21BAA00619]; National Science Foundation[12233013]; National Science Foundation[2023HYSPT0706]; National Natural Science Foundation of China[CMS-CSST-2021-A04]; National Natural Science Foundation of China[CMS-CSST-2021-A06]; China Manned Space Project[2021YFA1600403]; National Key R&D Program of China[2023A1515030116]; Guangdong Basic and Applied Basic Research Foundation[GZC20242112]; Postdoctoral Fellowship Program of CPSF[2021/43/P/ST9/03167]; Foreign Scholar Research Program of Peking University[2021/41/B/ST9/01191]; Polish National Science Center (NCN)[945339]; European Union Framework Programme for Research and Innovation Horizon 2020[12288102]; European Union Framework Programme for Research and Innovation Horizon 2020[12125303]; European Union Framework Programme for Research and Innovation Horizon 2020[12173081]; NSFC[ZDBS-LY-7005]; Key Research Program of Frontier Sciences, CAS[202101AV070001]; Yunnan Fundamental Research Projects[241216104168995]; Zhaoqing City Science and Technology Innovation Guidance Project[qn202518]; Young Faculty Research Funding Project of Zhaoqing University; Fundamental Research Funds for the Central Universities[22hytd09]; Sun Yat-sen University; China Scholarship Council (CSC)
项目资助者Sinergia[2019B030302001] ; Guangdong Major Project of Basic and Applied Basic Research[2020YFC2201400] ; National Key Research and Development Program of China[12250610185, 12261131497] ; Natural Science Foundation of China[22ZR1403400] ; Natural Science Foundation of Shanghai[CRSII5_213497] ; Swiss National Science Foundation under the Sinergia[AST-2319441] ; National Science Foundation[21BAA00619, 12233013, 2023HYSPT0706] ; National Natural Science Foundation of China[CMS-CSST-2021-A04, CMS-CSST-2021-A06] ; China Manned Space Project[2021YFA1600403] ; National Key R&D Program of China[2023A1515030116] ; Guangdong Basic and Applied Basic Research Foundation[GZC20242112] ; Postdoctoral Fellowship Program of CPSF[2021/43/P/ST9/03167] ; Foreign Scholar Research Program of Peking University[2021/41/B/ST9/01191] ; Polish National Science Center (NCN)[945339] ; European Union Framework Programme for Research and Innovation Horizon 2020[12288102, 12125303, 12173081] ; NSFC[ZDBS-LY-7005] ; Key Research Program of Frontier Sciences, CAS[202101AV070001] ; Yunnan Fundamental Research Projects[241216104168995] ; Zhaoqing City Science and Technology Innovation Guidance Project[qn202518] ; Young Faculty Research Funding Project of Zhaoqing University ; Fundamental Research Funds for the Central Universities[22hytd09] ; Sun Yat-sen University ; China Scholarship Council (CSC)
语种英语
学科领域天文学 ; 物理学
文章类型Review
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0034-4885
URL查看原文
WOS记录号WOS:001489434800001
WOS研究方向Physics
WOS类目Physics, Multidisciplinary
关键词[WOS]BLACK-HOLE MERGERS ; QUASI-PERIODIC ERUPTIONS ; ACTIVE GALACTIC NUCLEI ; M-CIRCLE-DOT ; WHITE-DWARF BINARIES ; X-RAY BINARIES ; COMMON ENVELOPE EVOLUTION ; INITIAL MASS FUNCTION ; DENSE STAR-CLUSTERS ; LONG-TERM EVOLUTION
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文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/28307
专题大样本恒星演化研究组
作者单位1.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai Campus, Zhuhai 519082, Peoples R China;
2.Sun Yat Sen Univ, MOE Lab Tianqin Mission, TianQin Res Ctr Gravitat Phys, Zhuhai Campus, Zhuhai 519082, Peoples R China;
3.Sun Yat Sen Univ, Frontiers Sci Ctr TianQin, Gravitat Wave Res Ctr CNSA, Zhuhai Campus, Zhuhai 519082, Peoples R China;
4.Zhaoqing Univ, Sch Elect & Elect Engn, Zhaoqing 526061, Peoples R China;
5.Beijing Inst Math Sci & Applicat, Beijing 101408, Peoples R China;
6.Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong, Peoples R China;
7.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China;
8.Univ Politecn Valencia, Inst Mutidisciplinary Math, Valencia 46022, Spain;
9.Polish Acad Sci, Nicolaus Copernicus Astron Ctr, PL-00716 Torun, Poland;
10.Fudan Univ, Ctr Astron & Astrophys, Shanghai 200438, Peoples R China;
11.Fudan Univ, Dept Phys, Shanghai 200438, Peoples R China;
12.New Uzbekistan Univ, Sch Nat Sci & Humanities, Tashkent 100007, Uzbekistan;
13.Natl Univ Singapore, Dept Phys, Singapore 117551, Singapore;
14.Natl Univ Singapore, Dept Math, Singapore 119076, Singapore;
15.Fisk Univ, Dept Life & Phys Sci, Nashville, TN 37208 USA;
16.Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA;
17.Hebei Univ, Coll Phys Sci & Technol, Hebei 071002, Peoples R China;
18.Waseda Univ, Dept Astron, Tokyo 1130033, Japan;
19.Chinese Acad Sci, Yunnan Observat, Kunming 650216, Peoples R China;
20.Yunnan Key Lab, Int Ctr Supernovae, Kunming 650216, Peoples R China;
21.Univ Chinese Acad Sci, Beijing 100049, Peoples R China;
22.Zhejiang Univ, Sch Phys, Zhejiang 310027, Peoples R China;
23.Yangzhou Univ, Ctr Gravitat & Cosmol, Yangzhou 225009, Peoples R China;
24.Univ Federico II, Dept Phys, I-80131 Naples, Italy;
25.Univ Sci & Technol China, Sch Astron & Space Sci, Nanjing 210093, Peoples R China;
26.Shanghai Astron Observ, Shanghai 200030, Peoples R China;
27.Fukui Prefectural Univ, Ctr Informat Sci, Fukui 9170003, Japan;
28.Univ Studi Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy;
29.Inst High Energy Phys, Beijing 100049, Peoples R China;
30.Niels Bohr Inst, DK-2200 Copenhagen, Denmark;
31.Tsinghua Univ, Dept Astron, Tsinghua 100084, Peoples R China;
32.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Peoples R China;
33.Purple Mt Observ, Nanjing 210034, Peoples R China;
34.INFM, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, Italy;
35.Adam Mickiewicz Univ, Fac Math & Comp Sci, Uniwersytetu Poznanskiego 4, PL-61614 Poznan, Poland
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GB/T 7714
Li, En-Kun,Liu, Shuai,Torres-Orjuela, Alejandro,et al. Gravitational wave astronomy with TianQin[J]. REPORTS ON PROGRESS IN PHYSICS,2025,88(5).
APA Li, En-Kun.,Liu, Shuai.,Torres-Orjuela, Alejandro.,Chen, Xian.,Inayoshi, Kohei.,...&Luo, Jun.(2025).Gravitational wave astronomy with TianQin.REPORTS ON PROGRESS IN PHYSICS,88(5).
MLA Li, En-Kun,et al."Gravitational wave astronomy with TianQin".REPORTS ON PROGRESS IN PHYSICS 88.5(2025).
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