Titlebook: Quantum Enhancement of a 4 km Laser Interferometer Gravitational-Wave Detector; Sheon S. Y. Chua Book 2015 Springer International Publishi

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Backscattered-Light Impact in a Squeezing-Enhanced Gravitational-Wave Detectorent to the strain-sensitivity of a gravitational-wave detector. The impact of backscattered light in gravitational-wave detector readout is first introduced in Sects. . and .. After overviews of the LIGO Squeezed Light Injection Experiment environment conditions (Sect. .) and the evidence of the bac

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Gravitational Waves and the Quest for Their Direct Detections of gravitational waves and potential sources of such waves in our Universe. Section . presents an introduction to current, second generation and future ground-based interferometric detectors. Section . provides an overview of noise sources currently affecting ground based measurements.

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Book 2015esign of the squeezed light source which would be used for the experiment. The specific design is the doubly-resonant, traveling-wave bow-tie cavity squeezed light source with a new modified coherent sideband locking technique. The thesis describes the properties affecting the squeezing magnitudes a

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Overview of the LIGO Squeezed Light Injection Experimentware and modifications made for the LIGO Squeezed Light Injection Experiment. The squeezed light source for the Experiment is then covered, including specifics about the contribution from the ANU, the Optical Parametric Oscillator.

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Backscattered-Light Impact in a Squeezing-Enhanced Gravitational-Wave Detectorge displacement measurement result (Sect. .), and the consistency between the two experiments is discussed in Sect. .. Recommendations to further reduce the backscattered light impact of an installed squeezer in future gravitational-wave detectors conclude the chapter (Sect. .).