Non-classical sources of light and their applications to gravitational wave detection

D. E. McClelland, L. S. Collaboration

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    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.

    Original languageEnglish
    Title of host publicationCLEO
    Subtitle of host publicationApplications and Technology, CLEO_AT 2017
    PublisherOptica Publishing Group (formerly OSA)
    ISBN (Print)9781943580279
    DOIs
    Publication statusPublished - 2017
    EventCLEO: Applications and Technology, CLEO_AT 2017 - San Jose, United States
    Duration: 14 May 201719 May 2017

    Publication series

    NameOptics InfoBase Conference Papers
    VolumePart F43-CLEO_AT 2017
    ISSN (Electronic)2162-2701

    Conference

    ConferenceCLEO: Applications and Technology, CLEO_AT 2017
    Country/TerritoryUnited States
    CitySan Jose
    Period14/05/1719/05/17

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