The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range
文献类型：期刊论文
| 作者 | Sedda, Manuel Arca18; Berry, Christopher P. L.19,20; Jani, Karan21; Amaro-Seoane, Pau22,23,24,25; Auclair, Pierre26; Baird, Jonathon27; Baker, Tessa17; Berti, Emanuele1; Breivik, Katelyn29; Burrows, Adam28 |
| 刊名 | CLASSICAL AND QUANTUM GRAVITY
 |
| 出版日期 | 2020-11-05 |
| 卷号 | 37期号:21页码:36 |
| 关键词 | gravitational-wave detectors decihertz observatories compact binaries multiband gravitational-wave astronomy intermediate-mass black holes tests of general relativity early universe physics |
| ISSN号 | 0264-9381 |
| DOI | 10.1088/1361-6382/abb5c1 |
| 英文摘要 | The gravitational-wave astronomical revolution began in 2015 with LIGO's observation of the coalescence of two stellar-mass black holes. Over the coming decades, ground-based detectors like laser interferometer gravitational-wave observatory (LIGO), Virgo and KAGRA will extend their reach, discovering thousands of stellar-mass binaries. In the 2030s, the space-basedlaser interferometer space antenna(LISA) will enable gravitational-wave observations of the massive black holes in galactic centres. Between ground-based observatories and LISA lies the unexplored dHz gravitational-wave frequency band. Here, we show the potential of adecihertz observatory(DO) which could cover this band, and complement discoveries made by other gravitational-wave observatories. The dHz range is uniquely suited to observation of intermediate-mass (similar to 10(2)-10(4)M(circle dot)) black holes, which may form the missing link between stellar-mass and massive black holes, offering an opportunity to measure their properties. DOs will be able to detect stellar-mass binaries days to years before they merge and are observed by ground-based detectors, providing early warning of nearby binary neutron star mergers, and enabling measurements of the eccentricity of binary black holes, providing revealing insights into their formation. Observing dHz gravitational-waves also opens the possibility of testing fundamental physics in a new laboratory, permitting unique tests of general relativity (GR) and the standard model of particle physics. Overall, a DO would answer outstanding questions about how black holes form and evolve across cosmic time, open new avenues for multimessenger astronomy, and advance our understanding of gravitation, particle physics and cosmology. |
| 资助项目 | Alexander von Humboldt foundation ; Deutsche Forschungsgemeinschaft (DFG, German research foundation)[138713538 -SFB 881] ; CIERABoard of VisitorsResearch Professorship ; NationalNatural Science Foundation of China[11975027] ; NationalNatural Science Foundation of China[11991053] ; NationalNatural Science Foundation of China[11721303] ; Young Elite Scientists Sponsorship Program by the China Association for Science and Technology[2018QNRC001] ; Royal Society[URF\R1\180009] ; Ramon y Cajal Programme of the Ministry of Economy, Industry and Competitiveness of Spain ; COST Action GWverse[CA16104] ; National Key R&D Program of China[2016YFA0400702] ; National Science Foundation of China[11721303] ; NSF[PHY-1912550] ; NSF[AST-1841358] ; NASA ATP Grants[17-ATP17-0225] ; NASA ATP Grants[19-ATP19-0051] ; NSF-XSEDE Grant[PHY090003] ; Amaldi Research Center - MIUR program 'Dipartimento di Eccellenza'[CUP: B81I18001170001] ; European Union's Horizon 2020 research and innovation programme under the Marie SklodowskaCurie grant[690904] ; Emmy Noether Research Group - German Research Foundation (DFG)[DO 1771/1-1] ; Eliteprogramme for Postdocs - Baden-Wurttemberg Stiftung ; NASAthrough theNASAHubble Fellowship grant - Space Telescope Science Institute[HST-HF2-51435.001A] ; NASA[NAS5-26555] ; National Science Foundation[DGE-0948017] ; Chateaubriand Fellowship from the Office for Science & Technology of the Embassy of France in the United States ; Society in Science, The Branco Weiss Fellowship ; European Union's H2020 ERC Consolidator Grant 'Binary massive black hole astrophysics'[818691-B Massive] ; Royal Society-Science Foundation Ireland University Research Fellowship[UF160093] |
| WOS研究方向 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:000576064200001 |
| 出版者 | IOP PUBLISHING LTD |
| 源URL | [http://ir.amss.ac.cn/handle/2S8OKBNM/52298]  |
| 专题 | 中国科学院数学与系统科学研究院 |
| 通讯作者 | Sedda, Manuel Arca |
| 作者单位 | 1.Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA 2.Kings Coll London, Dept Phys, London WC2R 2LS, England 3.Univ Coll Dublin, Sch Math & Stat, Dublin 4, Ireland 4.Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA 5.Max Planck Inst Gravitat Phys, Albert Einstein Inst, Muhlenberg 1, D-14476 Potsdam, Germany 6.Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy 7.Stockholm Univ, Oskar Klein Ctr, Dept Phys, Stockholm, Sweden 8.Stevens Inst Technol, Dept Phys, Hoboken, NJ 07030 USA 9.Univ Stavanger, Fac Sci & Technol, N-4036 Stavanger, Norway 10.Univ Florida, Dept Phys, POB 118440, Gainesville, FL 32611 USA |
| 推荐引用方式 GB/T 7714 | Sedda, Manuel Arca,Berry, Christopher P. L.,Jani, Karan,et al. The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range[J]. CLASSICAL AND QUANTUM GRAVITY,2020,37(21):36. |
| APA | Sedda, Manuel Arca.,Berry, Christopher P. L..,Jani, Karan.,Amaro-Seoane, Pau.,Auclair, Pierre.,...&Zevin, Michael.(2020).The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range.CLASSICAL AND QUANTUM GRAVITY,37(21),36. |
| MLA | Sedda, Manuel Arca,et al."The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range".CLASSICAL AND QUANTUM GRAVITY 37.21(2020):36. |
入库方式： OAI收割
来源：数学与系统科学研究院
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