Media contact

Dr.  Benjamin  Knispel
Dr. Benjamin Knispel
Press Officer AEI Hannover
Phone:+49 511 762-19104Fax:+49 511 762-17182

Science contact

Dr.  Henning Vahlbruch
Dr. Henning Vahlbruch
Phone:+49 511 762-17092Fax:+49 511 762-17182

Further information

AEI scientist honoured in New York

International prize for Dr. Henning Vahlbruch

August 11, 2009

AEI scientist Dr. Henning Vahlbruch was honoured in New York with the THESIS Prize of the Gravitational Wave International Committee (GWIC) for the world’s best doctoral thesis in the area of gravitational wave research. The prize is awarded annually for outstanding theses. Henning Vahlbruch was thus able to prevail against competitors from MIT (Massachusetts Institute of Technology) and from the renowned CALTECH (California Institute of Technology).

In his research work, Vahlbruch has described how a new, highly precise measuring technology can be implemented in gravitational wave research with the help of squeezed light. He works in the Research Group led by Prof. Dr. Roman Schnabel, where the way was paved for this procedure. “Squeezed light means that the temporal, naturally random and irregular distance between light particles, the photons, can be influenced,” explains Dr. Henning Vahlbruch. “We squeeze the photons into rank and file, tame them so to speak, and thereby raise the measurement accuracy and range of the gravitational wave detectors.” Untamed photons, conversely, cause a “shot noise” that seriously reduces the measurement accuracy.

In gravitational wave detectors, laser light is used to measure tiny expansions and compressions of space-time that arise when passing through a gravitational wave. When a gravitational wave passes through a detector, the arm length of the laser beam changes, and thus the intensity of the laser light at the output of the detector. In step with the gravitational wave, a corresponding photocurrent is generated via the photoelectric effect, the data of which is stored and which can be processed. Thus, the laser light itself should show no fluctuations in its intensity, so that even the very tiniest signals can be measured.

Already today, gravitational wave detectors of the first generation, e.g. the German-British GEO600 detector in Ruthe near Hannover, can precisely measure a measuring distance of 10-19 m - which is comparable to one 10,000th of the diameter of a proton. Thanks to such measurement accuracy, neutron stars can be observed up to a distance of 40 million light years from Earth. The thereby accessible part of the universe encompasses several dozen galaxies.

For the first time ever, the installation of squeezed light in a gravitational wave detector, in GEO600, is currently underway in Hannover. GEO600 is a project of the AEI, which is also partner of the QUEST Excellence Cluster. The detector is a think-tank and technological pioneer in gravitational wave research. The bestowal of the GWIC Thesis Prize on Dr. Henning Vahlbruch is a further attestation to this.

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