We present the observation of optical fields carrying squeezed vacuum states at sideband frequencies from 100.3em0exHz to above 350.3em0exMHz. The field was generated with type-I optical parametric oscillation below threshold at 10640.3em0exnm. A coherent, unbalanced classical modulation field at 400.3em0exMHz enabled the generation of error signals for stable phase control of the squeezed vacuum field with respect to a strong local oscillator. Broadband squeezing of approximately -40.3em0exdB was measured with balanced homodyne detection. The spectrum of the squeezed field allows a quantum noise reduction of ground-based gravitational wave detectors over their full detection band, regardless of whether homodyne readout or radio-frequency heterodyne readout is used.
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Chelkowski et al. (2007) studied this question.
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