This topical group operates a 10-metre prototype interferometer facility located in the institute for gravitational physics. The 10-m prototype offers an environment with extremely low displacement noise, a large volume in ultra-high vacuum, a highly stable laser with a power of 35 watts, a very stable DC supply network, comprehensive detection of environmental influences, fully digital control infrastructure and sufficient flexibility to quickly change the experimental setup - if necessary.
The first and most important experiment being set up in this facility is a Michelson interferometer, which explores the interferometric standard quantum limit (SQL). To achieve the SQL, the interferometer sensitivity must be limited only by the quantum noise at the measurement frequency. The SQL can be surpassed by exploiting correlations between the amplitude and phase quantum fluctuations of the light inside the interferometer. Different approaches for surpassing the SQL will be tested and analysed.