In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a squeezed-light laser [1]. Recently, a non-classically enhanced measurement sensitivity of GEO 600 was reported [2]. In this paper, a characterization of the squeezed-light laser is presented. Thereupon, the status of the integration into GEO 600 is reviewed, focussing on the sources of optical loss limiting the shot noise reduction by squeezing at the moment. Finally, the possibilities for a future loss reduction are discussed
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...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
Abstract. In the course of the high-frequency upgrade of GEO 600, its optical configuration was exte...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Abstract. The next upgrade of the GEO 600 gravitational wave detector is scheduled for 2010 and will...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Currently, the German/British gravitational wave detector GEO600 is being upgraded in course of the ...
This contribution reviews our recent progress on the generation of squeezed light [1], and also the ...
We report on the demonstration of broadband squeezed laser beams that show a frequency-dependent ori...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Currently, the German/British gravitational wave (GW) detector GEO 600 is being upgraded within the ...
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...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
Abstract. In the course of the high-frequency upgrade of GEO 600, its optical configuration was exte...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a ...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Abstract. The next upgrade of the GEO 600 gravitational wave detector is scheduled for 2010 and will...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Currently, the German/British gravitational wave detector GEO600 is being upgraded in course of the ...
This contribution reviews our recent progress on the generation of squeezed light [1], and also the ...
We report on the demonstration of broadband squeezed laser beams that show a frequency-dependent ori...
The next upgrade of the GEO 600 gravitational-wave detector is scheduled for 2010 and will, in parti...
Currently, the German/British gravitational wave (GW) detector GEO 600 is being upgraded within the ...
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...