KMS Of Academy of mathematics and systems sciences, CAS
| The missing link in gravitational-wave astronomy A summary of discoveries waiting in the decihertz range | |
| Sedda, Manuel Arca1; Berry, Christopher P. L.2,3; Jani, Karan4; Amaro-Seoane, Pau5,6,7,8; Auclair, Pierre9; Baird, Jonathon10; Baker, Tessa11; Berti, Emanuele12; Breivik, Katelyn13; Caprini, Chiara9; Chen, Xian6,14; Doneva, Daniela15; Ezquiaga, Jose M.16; Ford, K. E. Saavik17,18; Katz, Michael L.2; Kolkowitz, Shimon19; McKernan, Barry17,18; Mueller, Guido20; Nardini, Germano21; Pikovski, Igor22,23; Rajendran, Surjeet12; Sesana, Alberto24; Shao, Lijing6,25; Tamanini, Nicola26; Warburton, Niels27; Witek, Helvi28; Wong, Kaze12; Zevin, Michael2 | |
| 2021-04-29 | |
| Source Publication | EXPERIMENTAL ASTRONOMY
 |
| ISSN | 0922-6435 |
| Pages | 14 |
| Abstract | Since 2015 the gravitational-wave observations of LIGO and Virgo have transformed our understanding of compact-object binaries. In the years to come, ground-based gravitational-wave observatories such as LIGO, Virgo, and their successors will increase in sensitivity, discovering thousands of stellar-mass binaries. In the 2030s, the space-based LISA will provide gravitational-wave observations of massive black holes binaries. Between the similar to 10-10(3) Hz band of ground-based observatories and the similar to 10(-4)-10(- 1) Hz band of LISA lies the uncharted decihertz gravitational-wave band. We propose a Decihertz Observatory to study this frequency range, and to complement observations made by other detectors. Decihertz observatories are well suited to observation of intermediate-mass (similar to 10(2)-10(4)M(circle dot)) black holes; they will be able to detect stellar-mass binaries days to years before they merge, providing early warning of nearby binary neutron star mergers and measurements of the eccentricity of binary black holes, and they will enable new tests of general relativity and the Standard Model of particle physics. Here we summarise how a Decihertz Observatory could provide unique insights into how black holes form and evolve across cosmic time, improve prospects for both multimessenger astronomy and multiband gravitational-wave astronomy, and enable new probes of gravity, particle physics and cosmology. |
| Keyword | Gravitational waves Decihertz observatories Multiband gravitational-wave astronomy Multimessenger astronomy Space-based detectors Black holes Neutron stars White dwarfs Stochastic backgrounds Binary evolution Intermediate-mass black holes Tests of general relativity Voyage 2050 |
| DOI | 10.1007/s10686-021-09713-z |
| Indexed By | SCI |
| Language | 英语 |
| Funding Project | Alexander von Humboldt Foundation ; Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)[138713538 - SFB 881] ; CIERA Board of Visitors Research Professorship ; Ramon y Cajal Programme of the Ministry of Economy, Industry and Competitiveness of Spain ; National Key R&D Program of China[2016YFA0400702] ; National Science Foundation of China[11721303] ; Royal Society[URF\R1\180009] ; National Science Foundation (NSF)[PHY-1912550] ; National Science Foundation (NSF)[AST-1841358] ; NASA ATP Grants[17-ATP17-0225] ; NASA ATP Grants[19-ATP19-0051] ; NSF-XSEDE Grant[PHY-090003] ; Amaldi Research Center - MIUR program Dipartimento di Eccellenza[CUP: B81I18001170001] ; European Union[690904] ; Emmy Noether Research Group - German Research Foundation (DFG)[DO 1771/1-1] ; Eliteprogramme for Postdocs - Baden-Wurttemberg Stiftung ; NASA through the NASA Hubble Fellowship grant - Space Telescope Science Institute[HST-HF2-51435.001-A] ; NASA[NAS5-26555] ; NSF[DGE-0948017] ; Chateaubriand Fellowship from the Office for Science & Technology of the Embassy of France in the United States ; ROMFORSK grant[302640] ; Society in Science, The Branco Weiss Fellowship ; European Union's H2020 ERC Consolidator Grant Binary massive black hole astrophysics[818691] ; National Natural Science Foundation of China[11721303] ; National Natural Science Foundation of China[11975027] ; National Natural Science Foundation of China[11991053] ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology[2018QNRC001] ; Max Planck Partner Group Program - Max Planck Society ; Royal Society-Science Foundation Ireland University Research Fellowship[UF160093] ; COST Action GWverse[CA16104] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000645168500001 |
| Publisher | SPRINGER |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.amss.ac.cn/handle/2S8OKBNM/58645 |
| Collection | 中国科学院数学与系统科学研究院 |
| Corresponding Author | Berry, Christopher P. L. |
| Affiliation | 1.Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Monchofstr 12-14, Heidelberg, Germany 2.Northwestern Univ, Dept Phys & Astron, Ctr Interdisciplinary Explorat & Res Astrophys CI, 2145 Sheridan Rd, Evanston, IL 60208 USA 3.Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow G12 8QQ, Lanark, Scotland 4.Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37212 USA 5.Univ Politecn Valencia, IGIC, Valencia, Spain 6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 7.Chinese Acad Sci, Acad Math & Syst Sci, Inst Appl Math, Beijing 100190, Peoples R China 8.TU Berlin, Zentrum Astron & Astrophys, Hardenbergstr 36, D-10623 Berlin, Germany 9.Univ Paris Diderot, CNRS, UMR 7164, Lab Astroparticule & Cosmol, 10 Rue Alice Domon & Leonie Duquet, F-75013 Paris, France 10.Imperial Coll London, Phys Dept, Blackett Lab, High Energy Phys Grp, Prince Consort Rd, London SW7 2BW, England 11.Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England 12.Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA 13.Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 1A7, Canada 14.Peking Univ, Sch Phys, Astron Dept, Beijing 100871, Peoples R China 15.Eberhard Karls Univ Tubingen, Theoret Astrophys, D-72076 Tubingen, Germany 16.Univ Chicago, Enrico Fermi Inst, Kavli Inst Cosmol Phys, 5640 S Ellis Ave, Chicago, IL 60637 USA 17.CUNY, BMCC, 199 Chambers St, New York, NY 10007 USA 18.Amer Museum Nat Hist, Dept Astrophys, New York, NY 10028 USA 19.Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA 20.Univ Florida, Dept Phys, POB 118440, Gainesville, FL 32611 USA 21.Univ Stavanger, Fac Sci & Technol, N-4036 Stavanger, Norway 22.Stevens Inst Technol, Dept Phys, Hoboken, NJ 07030 USA 23.Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden 24.Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy 25.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 26.Max Planck Inst Gravitat Phys, Albert Einstein Inst, Muhlenberg 1, D-14476 Potsdam, Germany 27.Univ Coll Dublin, Sch Math & Stat, Dublin 4, Ireland 28.Kings Coll London, Dept Phys, London WC2R 2LS, England |
| Recommended Citation GB/T 7714 | Sedda, Manuel Arca,Berry, Christopher P. L.,Jani, Karan,et al. The missing link in gravitational-wave astronomy A summary of discoveries waiting in the decihertz range[J]. EXPERIMENTAL ASTRONOMY,2021:14. |
| APA | Sedda, Manuel Arca.,Berry, Christopher P. L..,Jani, Karan.,Amaro-Seoane, Pau.,Auclair, Pierre.,...&Zevin, Michael.(2021).The missing link in gravitational-wave astronomy A summary of discoveries waiting in the decihertz range.EXPERIMENTAL ASTRONOMY,14. |
| MLA | Sedda, Manuel Arca,et al."The missing link in gravitational-wave astronomy A summary of discoveries waiting in the decihertz range".EXPERIMENTAL ASTRONOMY (2021):14. |
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