Experimental demonstration of a squeezing enhanced power recycled   Michelson interferometer for gravitational wave detection
  Interferometric gravitational wave detectors are expected to be limited by shot noise at some frequencies. We experimentally demonstrate that a power recycled Michelson with squeezed light injected into the dark port can overcome this limit. An improvement in the signal-to-noise ratio of 2.3dB is measured and locked stably for long periods of time. The configuration, control and signal readout of our experiment are compatible with current gravitational wave detector designs. We consider the application of our system to long baseline interferometer designs such as LIGO. 
Kirk McKenzie, Ben C. Buchler, Daniel A. Shaddock, Ping Koy Lam and   David E. McClelland