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Optical Gravitational Wave Antenna with Increased Power Handling Capability
Andrey B. Matsko, Mikhail V. Poplavskiy, Hiroaki Yamamoto +1
Fundamental sensitivity of an optical interferometric gravitational wave detector increases with increase of the optical power which, in turn, limited because of the opto-mechanica…
The noise in gravitational-wave detectors and other classical-force measurements is not influenced by test-mass quantization
Vladimir B. Braginsky, Mikhail L. Gorodetsky, Farid Ya. Khalili +3
It is shown that photon shot noise and radiation-pressure back-action noise are the sole forms of quantum noise in interferometric gravitational wave detectors that operate near or…
Conversion of conventional gravitational-wave interferometers into QND interferometers by modifying their input and/or output optics
H. J. Kimble, Yuri Levin, Andrey B. Matsko +2
The LIGO-II gravitational-wave interferometers (ca. 2006--2008) are designed to have sensitivities at about the standard quantum limit (SQL) near 100 Hz. This paper describes and a…