Squeezed states of the optical field were theoretically described in the early 1970s and first observed in the mid 1980s. The measured photon number of a squeezed state is correlated with the measured photon numbers of all other squeezed states of the same ensemble, providing sub-Poissonian statistics. Today all gravitational-wave observatories use squeezed light as the cost-efficient alternative to further scaling up the light power. This user application of quantum correlations was made possible through dedicated research and development of squeezed light between 2002 and 2010.Comment: Proceedings paper of the invited talk at the 56th Rencontres de Moriond 2022 on Gravitation in La Thuile, Aosta Valley, Italy, January 30 - February 6,...
Intensity squeezed light was successfully generated using semiconductor lasers with sub-Poissonian p...
Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sen...
Quantum noise will be the dominant noise source for the advanced laser interferometric gravitational...
This contribution reviews our recent progress on the generation of squeezed light [1], and also the ...
The engineering of strongly squeezed vacuum states of light is a key technology for the reduction of...
Squeezing of light's quantum noise requires temporal rearranging of photons. This again corresponds ...
It is shown that squeezed states of primordial gravitational waves are inevitably produced in the co...
Currently, the German/British gravitational wave detector GEO600 is being upgraded in course of the ...
Recent experiments have demonstrated that squeezed vacuum states can be injected into gravitational ...
We report the experimental realization of squeezed quantum states of light, tailored for new applica...
In this article, the possibility of generating non-classical light due to Planck-scale effects is co...
The field of squeezed states for gravitational-wave (GW) detector enhancement is rapidly maturing. ...
We report on the first long-term application of squeezed vacuum states of light to improve the shot-...
Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sen...
The first detections of gravitational waves have opened an exciting new field of astronomy. One of t...
Intensity squeezed light was successfully generated using semiconductor lasers with sub-Poissonian p...
Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sen...
Quantum noise will be the dominant noise source for the advanced laser interferometric gravitational...
This contribution reviews our recent progress on the generation of squeezed light [1], and also the ...
The engineering of strongly squeezed vacuum states of light is a key technology for the reduction of...
Squeezing of light's quantum noise requires temporal rearranging of photons. This again corresponds ...
It is shown that squeezed states of primordial gravitational waves are inevitably produced in the co...
Currently, the German/British gravitational wave detector GEO600 is being upgraded in course of the ...
Recent experiments have demonstrated that squeezed vacuum states can be injected into gravitational ...
We report the experimental realization of squeezed quantum states of light, tailored for new applica...
In this article, the possibility of generating non-classical light due to Planck-scale effects is co...
The field of squeezed states for gravitational-wave (GW) detector enhancement is rapidly maturing. ...
We report on the first long-term application of squeezed vacuum states of light to improve the shot-...
Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sen...
The first detections of gravitational waves have opened an exciting new field of astronomy. One of t...
Intensity squeezed light was successfully generated using semiconductor lasers with sub-Poissonian p...
Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sen...
Quantum noise will be the dominant noise source for the advanced laser interferometric gravitational...