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Last Updated:
5 April 2012

Low Frequency Squeezed Light


The Squeezed Light Experiment at the Centre for Gravitational Physics

Low frequency squeezed light (or low frequency 'squeezing') at GW signal frequencies (10Hz-10kHz) can be used to reduce quantum noise in GW detectors.

From our group's first demonstration of squeezing measured within the audio gravitational wave detection band using a degenerate Optical Parametric Oscillator [1], we have developed a squeezed light source that can produce and control squeezed light on timescales commensurate with GW detector science runs [2], and recently demonstrated at least 10dB of Quantum Noise reduction across the audio gravitational wave detection band [shown below - 3]

This work is done in collaboration with the ANU Quantum Optics group, the Quantum Measurement Group at MIT, USA and Albert Einstein Institute in Germany.

[1] K. McKenzie et al, Phys. Rev. Lett. 93, 161105 (2004) (paper)
[2] S. S. Y. Chua et al, Optics Letters 36, 4680-4682 (2011) (paper)
[3] M. S. Stefszky et al, paper in review

Locked squeezed spectrum (Red trace) showing at least 10dB of noise reduction below Quantum Noise (Blue trace) across the audio gravitational wave detection band (10Hz - 10kHz), and 11.6dB noise reduction above 200Hz.

Magenta trace is antisqueezed spectrum, and Black trace is electronics noise.