Enhancing the Bandwidth of Gravitational-Wave Detectors with Unstable Optomechanical Filters

被引:69
作者
Miao, Haixing [1 ]
Ma, Yiqiu [2 ]
Zhao, Chunnong [2 ]
Chen, Yanbei [3 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Univ Western Australia, Sch Phys, Nedlands, WA 6009, Australia
[3] CALTECH, Theoret Astrophys 350 17, Pasadena, CA 91125 USA
基金
美国国家科学基金会; 澳大利亚研究理事会;
关键词
INDUCED TRANSPARENCY; LIGHT; CAVITIES; NOISE;
D O I
10.1103/PhysRevLett.115.211104
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Advanced interferometric gravitational-wave detectors use optical cavities to resonantly enhance their shot-noise-limited sensitivity. Because of positive dispersion of these cavities-signals at different frequencies pick up different phases, there is a tradeoff between the detector bandwidth and peak sensitivity, which is a universal feature for quantum measurement devices having resonant cavities. We consider embedding an active unstable filter inside the interferometer to compensate the phase, and using feedback control to stabilize the entire system. We show that this scheme in principle can enhance the bandwidth without sacrificing the peak sensitivity. However, the unstable filter under our current consideration is a cavity-assisted optomechanical device operating in the instability regime, and the thermal fluctuation of the mechanical oscillator puts a very stringent requirement on the environmental temperature and the mechanical quality factor.
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页数:5
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