Non-classical Sources of Light and Their Applications to Gravitational Wave Detection

D.E. McClelland

doi:10.1364/CLEO_AT.2017.JTh3G.5

Conference on Lasers and Electro-Optics
OSA Technical Digest (online) (Optica Publishing Group, 2017),
paper JTh3G.5
•https://doi.org/10.1364/CLEO_AT.2017.JTh3G.5

Non-classical Sources of Light and Their Applications to Gravitational Wave Detection

D.E. McClelland and L.S. Collaboration

CLEO: Science and Innovations 2017

San Jose, California United States
14–19 May 2017
ISBN: 978-1-943580-27-9

From the session
Symposium on Optomechanics: Towards the Second Quantum Revolution I (JTh3G)

Open Access

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D. E. McClelland and , "Non-classical Sources of Light and Their Applications to Gravitational Wave Detection," in Conference on Lasers and Electro-Optics, OSA Technical Digest (online) (Optica Publishing Group, 2017), paper JTh3G.5.

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Abstract

Audio-band laser interferometer gravitational-wave detectors are massive optomechanical devices. Quantum enhancement requires sources at the operating wavelength with more than a factor of 10 squeezing from 1 Hz to 10 kHz, in a frequency-tailored quadrature.

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