Squeezing in Gravitational Wave Detectors

被引:19
作者
Dwyer, Sheila E. [1 ]
Mansell, Georgia L. [1 ,2 ,3 ]
McCuller, Lee [2 ,4 ]
机构
[1] LIGO Hanford Observ, Richland, WA 99352 USA
[2] MIT, LIGO, Cambridge, MA 02139 USA
[3] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA
[4] CALTECH, LIGO, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
gravitational waves; squeezed states; quantum optics; interferometer; quantum noise; 2-PHOTON QUANTUM OPTICS; COHERENT STATES; VACUUM STATES; LIGHT; NOISE; FORMALISM;
D O I
10.3390/galaxies10020046
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Injecting optical squeezed states of light, a technique known as squeezing, is now a tool for gravitational wave detection. Its ability to reduce quantum noise is helping to reveal more gravitational wave transients, expanding the catalog of observations in the last observing run. This review introduces squeezing and its history in the context of gravitational-wave detectors. It overviews the benefits, limitations and methods of incorporating squeezing into advanced interferometers, emphasizing the most relevant details for astrophysics instrumentation.
引用
收藏
页数:16
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