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A gravitational wave observatory operating beyond the quantum shot-noise limit

Date: 
2011-09-11
Author(s): 

The LIGO. Scientific Collaboration, LSC. (J. Abadie, R. Schnabel et al. )

Reference: 

Nature Physics 7, 962–965, (2011)

Around the globe several observatories are seeking the first direct detection of gravitational waves (GWs). These waves are predicted by Einsteins general theory of relativity and are generated, for example, by black-hole binary systems. Present GW detectors are Michelson-type kilometre-scale laser interferometers measuring the distance changes between mirrors suspended in vacuum. The sensitivity of these detectors at frequencies above several hundred hertz is limited by the vacuum (zero-point) fluctuations of the electromagnetic field.

Rainer Blatt receives DPG's Stern-Gerlach-Medaille

Summary: 

The highest prize for experimental physics of the German Physical Society DPG goes to AQUTE member Rainer Blatt.

Read the full story (in German).

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