G0900098-v1 L-V Meeting2 Motivation  High power operation in future detectors  Biggest remaining technical risk (after DC readout)  Squeezing allows for lower laser power  Squeezer technology now ready  7 dB of squeezing down to 10 Hz  Has been demonstrated on a bench and on interferometers (40M) Missing: Low frequency noise demonstration  Planned Experiments  GEO600: prototype for long baseline interferometers  Hanford H1: low noise at low frequency
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