We propose using optomechanical interaction to narrow the bandwidth of filter cavities for achieving frequency-dependent squeezing in advanced gravitational-wave detectors, inspired by the idea of optomechanically induced transparency. This can allow us to achieve a cavity bandwidth on the order of 100 Hz using small-scale cavities. Additionally, in contrast to a passive Fabry-Pérot cavity, the resulting cavity bandwidth can be dynamically tuned, which is useful for adaptively optimizing the detector sensitivity when switching amongst different operational modes. The experimental challenge for its implementation is a stringent requirement for very low thermal noise of the mechanical oscillator, which would need a superb mechanical quality f...
International audienceWith the recent detection of gravitational waves, non-classical light sources ...
International audienceThe astrophysical reach of current and future ground-based gravitational-wave ...
We examine the use of optomechanically generated squeezing to obtain a sensitivity enhancement for i...
We propose using optomechanical interaction to narrow the bandwidth of filter cavities for achieving...
Detections of gravitational waves (GW) in the frequency band 35 to 500 Hz have led to the birth of G...
Cavities with an extremely narrow linewidth of 10–100 Hz are required for realizing frequency-depend...
Advanced interferometric gravitational-wave detectors use optical cavities to resonantly enhance the...
This electronic version was submitted by the student author. The certified thesis is available in th...
The sensitivity of future gravitational wave interferometers is expected to be limited throughout th...
The ongoing global effort to detect gravitational waves continues to push the limits of precision me...
International audienceEarth-based gravitational-wave detectors will be limited by quantum noise in a...
Earth-based gravitational-wave detectors will be limited by quantum noise in a large part of their s...
International audienceEarth-based gravitational-wave detectors will be limited by quantum noise in a...
Quantum vacuum fluctuations impose strict limits on precision displacement measurements, those of in...
International audienceWith the recent detection of gravitational waves, non-classical light sources ...
International audienceThe astrophysical reach of current and future ground-based gravitational-wave ...
We examine the use of optomechanically generated squeezing to obtain a sensitivity enhancement for i...
We propose using optomechanical interaction to narrow the bandwidth of filter cavities for achieving...
Detections of gravitational waves (GW) in the frequency band 35 to 500 Hz have led to the birth of G...
Cavities with an extremely narrow linewidth of 10–100 Hz are required for realizing frequency-depend...
Advanced interferometric gravitational-wave detectors use optical cavities to resonantly enhance the...
This electronic version was submitted by the student author. The certified thesis is available in th...
The sensitivity of future gravitational wave interferometers is expected to be limited throughout th...
The ongoing global effort to detect gravitational waves continues to push the limits of precision me...
International audienceEarth-based gravitational-wave detectors will be limited by quantum noise in a...
Earth-based gravitational-wave detectors will be limited by quantum noise in a large part of their s...
International audienceEarth-based gravitational-wave detectors will be limited by quantum noise in a...
Quantum vacuum fluctuations impose strict limits on precision displacement measurements, those of in...
International audienceWith the recent detection of gravitational waves, non-classical light sources ...
International audienceThe astrophysical reach of current and future ground-based gravitational-wave ...
We examine the use of optomechanically generated squeezing to obtain a sensitivity enhancement for i...