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The next detectors for gravitational wave astronomy
by
BLAIR David JU Li ZHAO ChunNong WEN LinQing MIAO HaiXing CAI RongGen GAO JiangRui LIN XueChun LIU Dong WU Ling-An ZHU ZongHong HAMMOND Giles PAIK Ho Jung FAFONE Viviana ROCCHI Alessio BLAIR Carl MA YiQiu QIN JiaYi PAGE Michael
in
Angular resolution
/ Astronomy
/ China
/ Classical and Continuum Physics
/ Control stability
/ Detectors
/ Gravitation
/ Gravitational waves
/ Grounds
/ Instability
/ Invited Review
/ Observations and Techniques
/ Physics
/ Physics and Astronomy
/ Room temperature
/ Sensitivity analysis
/ Sensitivity enhancement
/ Sensors
/ Special Topic: the Next Detectors for Gravitational Wave Astronomy
/ Stability
/ Suspension systems
/ Thermal compensation
/ 天文探测器
/ 引力波
/ 探测器阵列
/ 操作技术
/ 测量技术
/ 灵敏度分析
/ 量子测量
/ 面探测器
2015
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The next detectors for gravitational wave astronomy
by
BLAIR David JU Li ZHAO ChunNong WEN LinQing MIAO HaiXing CAI RongGen GAO JiangRui LIN XueChun LIU Dong WU Ling-An ZHU ZongHong HAMMOND Giles PAIK Ho Jung FAFONE Viviana ROCCHI Alessio BLAIR Carl MA YiQiu QIN JiaYi PAGE Michael
in
Angular resolution
/ Astronomy
/ China
/ Classical and Continuum Physics
/ Control stability
/ Detectors
/ Gravitation
/ Gravitational waves
/ Grounds
/ Instability
/ Invited Review
/ Observations and Techniques
/ Physics
/ Physics and Astronomy
/ Room temperature
/ Sensitivity analysis
/ Sensitivity enhancement
/ Sensors
/ Special Topic: the Next Detectors for Gravitational Wave Astronomy
/ Stability
/ Suspension systems
/ Thermal compensation
/ 天文探测器
/ 引力波
/ 探测器阵列
/ 操作技术
/ 测量技术
/ 灵敏度分析
/ 量子测量
/ 面探测器
2015
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The next detectors for gravitational wave astronomy
by
BLAIR David JU Li ZHAO ChunNong WEN LinQing MIAO HaiXing CAI RongGen GAO JiangRui LIN XueChun LIU Dong WU Ling-An ZHU ZongHong HAMMOND Giles PAIK Ho Jung FAFONE Viviana ROCCHI Alessio BLAIR Carl MA YiQiu QIN JiaYi PAGE Michael
in
Angular resolution
/ Astronomy
/ China
/ Classical and Continuum Physics
/ Control stability
/ Detectors
/ Gravitation
/ Gravitational waves
/ Grounds
/ Instability
/ Invited Review
/ Observations and Techniques
/ Physics
/ Physics and Astronomy
/ Room temperature
/ Sensitivity analysis
/ Sensitivity enhancement
/ Sensors
/ Special Topic: the Next Detectors for Gravitational Wave Astronomy
/ Stability
/ Suspension systems
/ Thermal compensation
/ 天文探测器
/ 引力波
/ 探测器阵列
/ 操作技术
/ 测量技术
/ 灵敏度分析
/ 量子测量
/ 面探测器
2015
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Journal Article
The next detectors for gravitational wave astronomy
2015
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Overview
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.
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