The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of ~ 10-4 Hz/ at 20 Hz rolling off to below 6 × 10-6 Hz/ above 1 kHz. It is expected that tight angular control of the reference cavity's mirrors is necessary to reach this stringent requirement
Gravitational wave detectors are highly sensitive instruments to measure gravitational waves. To inc...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
International audienceThe interrogation of an ultra-narrow clock transition of a single trapped ion ...
The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum L...
The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum L...
The AEI 10 m Prototype is in its designing phase and will provide a test-bed for very sensitive inte...
The AEI 10 m Prototype is in its designing phase and will provide a test-bed for very sensitive inte...
A century after the existence of gravitational waves was predicted by Albert Einstein in his general...
A 10 m prototype interferometer facility is currently being set up at the AEI in Hannover, Germany. ...
The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein...
Neue Technologien zur Verbesserung der Empfindlichkeit von Gravitationswellendetektoren werden weltw...
The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein...
The sensitivity of high-precision interferometric measurements can be limited by Brownian noise with...
Currently, the AEI 10 m Prototype is being set up at the Albert Einstein Institute in Hannover, Germ...
Currently, the AEI 10 m Prototype is being set up at the Albert Einstein Institute in Hannover, Germ...
Gravitational wave detectors are highly sensitive instruments to measure gravitational waves. To inc...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
International audienceThe interrogation of an ultra-narrow clock transition of a single trapped ion ...
The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum L...
The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum L...
The AEI 10 m Prototype is in its designing phase and will provide a test-bed for very sensitive inte...
The AEI 10 m Prototype is in its designing phase and will provide a test-bed for very sensitive inte...
A century after the existence of gravitational waves was predicted by Albert Einstein in his general...
A 10 m prototype interferometer facility is currently being set up at the AEI in Hannover, Germany. ...
The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein...
Neue Technologien zur Verbesserung der Empfindlichkeit von Gravitationswellendetektoren werden weltw...
The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein...
The sensitivity of high-precision interferometric measurements can be limited by Brownian noise with...
Currently, the AEI 10 m Prototype is being set up at the Albert Einstein Institute in Hannover, Germ...
Currently, the AEI 10 m Prototype is being set up at the Albert Einstein Institute in Hannover, Germ...
Gravitational wave detectors are highly sensitive instruments to measure gravitational waves. To inc...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
International audienceThe interrogation of an ultra-narrow clock transition of a single trapped ion ...