Analysis and visualization of the output mode-matching requirements for squeezing in Advanced LIGO and future gravitational wave detectors
The sensitivity of ground-based gravitational-wave (GW) detectors will be improved in the future via the injection of frequency-dependent squeezed vacuum. The achievable improvement is ultimately limited by losses of the interferometer electromagnetic field that carries the GW signal. The analysis and reduction of optical loss in the GW signal chain will be critical for optimal squeezed light-enhanced interferometry. In this work, we analyze a strategy for reducing output-side losses due to...[Show more]
|Collections||ANU Research Publications|
|Source:||Physical Review D-Particles, Fields, Gravitation and Cosmology|
|Access Rights:||Open Access|
|PhysRevD.101.102005.pdf||1.54 MB||Adobe PDF|
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