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Measurement of optical response of a detuned resonant sideband extraction gravitational wave detector

2006/04/18 by O. Miyakawa, Osamu Miyakawa, Robert Ward +27 · 3 citations
Physics and Astronomy · #Advanced Frequency and Time Standards #Cold Atom Physics and Bose-Einstein Condensates #Pulsars and Gravitational Waves Research #gr-qc

paper · pdf · doi:10.1103/physrevd.74.022001

published as Phys.Rev. D74 (2006) 022001 · 6 pages, 4 figures, for submission to Phys Rev Letters

arxiv created 2006/04/18 · openalex publication_date 2006/07/06 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) interferometer with power recycling. The purpose of the detuned RSE configuration is to manipulate and optimize the optical response of the interferometer to differential displacements (induced by gravitational waves) as a function of frequency, independently of other parameters of the interferometer. The design of our interferometer results in an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a radiation pressure induced optical spring at around 41 Hz. We have developed a reliable procedure for acquiring lock and establishing the desired optical configuration. In this configuration, we have measured the optical response to differential displacement and found good agreement with predictions at both resonances and all other relevant frequencies. These results build confidence in both the theory and practical implementation of the more complex optical configuration being planned for Advanced LIGO.

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