Backscatter tolerant squeezed light source for advanced gravitational-wave detectors

Sheon S.Y. Chua; Michael S. Stefszky; Conor M. Mow-Lowry; Ben C. Buchler; Sheila Dwyer; Daniel A. Shaddock; Ping Koy Lam; David E. McClelland

doi:10.1364/OL.36.004680

Backscatter tolerant squeezed light source for advanced gravitational-wave detectors

Sheon S.Y. Chua^*, Michael S. Stefszky, Conor M. Mow-Lowry, Ben C. Buchler, Sheila Dwyer, Daniel A. Shaddock, Ping Koy Lam, David E. McClelland

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

51 Citations (Scopus)

Abstract

We report on the performance of a dual-wavelength resonant, traveling-wave optical parametric oscillator to generate squeezed light for application in advanced gravitational-wave interferometers. Shot noise suppression of 8.6 ± 0.8dB was measured across the detection band of interest to Advanced LIGO, and controlled squeezing measured over 5900 s. Our results also demonstrate that the traveling-wave design has excellent intracavity back-scattered light suppression of 47 dB and incident backscattered light suppression of 41 dB, which is a crucial design issue for application in advanced interferometers.

Original language	English
Pages (from-to)	4680-4682
Number of pages	3
Journal	Optics Letters
Volume	36
Issue number	23
DOIs	https://doi.org/10.1364/OL.36.004680
Publication status	Published - 1 Dec 2011

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title = "Backscatter tolerant squeezed light source for advanced gravitational-wave detectors",

abstract = "We report on the performance of a dual-wavelength resonant, traveling-wave optical parametric oscillator to generate squeezed light for application in advanced gravitational-wave interferometers. Shot noise suppression of 8.6 ± 0.8dB was measured across the detection band of interest to Advanced LIGO, and controlled squeezing measured over 5900 s. Our results also demonstrate that the traveling-wave design has excellent intracavity back-scattered light suppression of 47 dB and incident backscattered light suppression of 41 dB, which is a crucial design issue for application in advanced interferometers.",

author = "Chua, \{Sheon S.Y.\} and Stefszky, \{Michael S.\} and Mow-Lowry, \{Conor M.\} and Buchler, \{Ben C.\} and Sheila Dwyer and Shaddock, \{Daniel A.\} and Lam, \{Ping Koy\} and McClelland, \{David E.\}",

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doi = "10.1364/OL.36.004680",

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AU - Chua, Sheon S.Y.

AU - Stefszky, Michael S.

AU - Mow-Lowry, Conor M.

AU - Buchler, Ben C.

AU - Dwyer, Sheila

AU - Shaddock, Daniel A.

AU - Lam, Ping Koy

AU - McClelland, David E.

PY - 2011/12/1

Y1 - 2011/12/1

N2 - We report on the performance of a dual-wavelength resonant, traveling-wave optical parametric oscillator to generate squeezed light for application in advanced gravitational-wave interferometers. Shot noise suppression of 8.6 ± 0.8dB was measured across the detection band of interest to Advanced LIGO, and controlled squeezing measured over 5900 s. Our results also demonstrate that the traveling-wave design has excellent intracavity back-scattered light suppression of 47 dB and incident backscattered light suppression of 41 dB, which is a crucial design issue for application in advanced interferometers.

AB - We report on the performance of a dual-wavelength resonant, traveling-wave optical parametric oscillator to generate squeezed light for application in advanced gravitational-wave interferometers. Shot noise suppression of 8.6 ± 0.8dB was measured across the detection band of interest to Advanced LIGO, and controlled squeezing measured over 5900 s. Our results also demonstrate that the traveling-wave design has excellent intracavity back-scattered light suppression of 47 dB and incident backscattered light suppression of 41 dB, which is a crucial design issue for application in advanced interferometers.

UR - https://www.scopus.com/pages/publications/82955227994

U2 - 10.1364/OL.36.004680

DO - 10.1364/OL.36.004680

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VL - 36

SP - 4680

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JO - Optics Letters

JF - Optics Letters

IS - 23

ER -

Backscatter tolerant squeezed light source for advanced gravitational-wave detectors

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