The next detectors for gravitational wave astronomy
文献类型：期刊论文
| 作者 | Blair, D; Ju, L; Zhao, CN; Wen, LQ; Miao, HX; Cai, RG ; Gao, JR; Lin, XC; Liu, D; Wu, LA
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| 刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
 |
| 出版日期 | 2015 |
| 卷号 | 58期号:12页码:120405 |
| 关键词 | future gravitational wave detectors opto-mechanics quantum limit |
| 通讯作者 | Blair, D (reprint author), Univ Western Australia, Sch Phys, Crawley, WA 6009, Australia. |
| 英文摘要 | This paper focuses on the next detectors for gravitational wave astronomy which will be required after the current ground based detectors have completed their initial observations, and probably achieved the first direct detection of gravitational waves. The next detectors will need to have greater sensitivity, while also enabling the world array of detectors to have improved angular resolution to allow localisation of signal sources. Sect. 1 of this paper begins by reviewing proposals for the next ground based detectors, and presents an analysis of the sensitivity of an 8 km armlength detector, which is proposed as a safe and cost-effective means to attain a 4-fold improvement in sensitivity. The scientific benefits of creating a pair of such detectors in China and Australia is emphasised. Sect. 2 of this paper discusses the high performance suspension systems for test masses that will be an essential component for future detectors, while sect. 3 discusses solutions to the problem of Newtonian noise which arise from fluctuations in gravity gradient forces acting on test masses. Such gravitational perturbations cannot be shielded, and set limits to low frequency sensitivity unless measured and suppressed. Sects. 4 and 5 address critical operational technologies that will be ongoing issues in future detectors. Sect. 4 addresses the design of thermal compensation systems needed in all high optical power interferometers operating at room temperature. Parametric instability control is addressed in sect. 5. Only recently proven to occur in Advanced LIGO, parametric instability phenomenon brings both risks and opportunities for future detectors. The path to future enhancements of detectors will come from quantum measurement technologies. Sect. 6 focuses on the use of optomechanical devices for obtaining enhanced sensitivity, while sect. 7 reviews a range of quantum measurement options. |
| 学科主题 | Physics |
| 类目[WOS] | Physics, Multidisciplinary |
| 关键词[WOS] | PARAMETRIC OSCILLATORY INSTABILITY ; INDUCED TRANSPARENCY ; OPTICAL CAVITIES ; SEISMIC NOISE ; INTERFEROMETER ; SENSITIVITY ; SILICA ; LIGHT ; RESONATORS ; DEPENDENCE |
| 收录类别 | SCI |
| 语种 | 英语 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/20777]  |
| 专题 | 理论物理研究所_理论物理所1978-2010年知识产出 |
| 推荐引用方式 GB/T 7714 | Blair, D,Ju, L,Zhao, CN,et al. The next detectors for gravitational wave astronomy[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2015,58(12):120405. |
| APA | Blair, D.,Ju, L.,Zhao, CN.,Wen, LQ.,Miao, HX.,...&Page, M.(2015).The next detectors for gravitational wave astronomy.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,58(12),120405. |
| MLA | Blair, D,et al."The next detectors for gravitational wave astronomy".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 58.12(2015):120405. |
入库方式： OAI收割
来源：理论物理研究所
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