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

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dc.contributor.authorMcClelland, David
dc.contributor.authorCollaboration, L. S.
dc.coverage.spatialSan Jose, United States
dc.date.accessioned2023-02-27T03:25:36Z
dc.date.createdMay 14-19 2017
dc.date.issued2017
dc.date.updated2021-12-19T07:17:11Z
dc.description.abstractAudio-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 quadratureen_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn9781943580279en_AU
dc.identifier.urihttp://hdl.handle.net/1885/286460
dc.language.isoen_AUen_AU
dc.publisherOptical Society of American (OSA)en_AU
dc.relation.ispartofSymposium on Optomechanics: Towards the Second Quantum Revolution I (JTh3G)en_AU
dc.relation.ispartofseries2017 Conference on Lasers and Electro-Optics (CLEO)en_AU
dc.rights© 2017 Optical Society of Americaen_AU
dc.sourceOptics InfoBase Conference Papersen_AU
dc.titleNon-classical sources of light and their applications to gravitational wave detectionen_AU
dc.typeConference paperen_AU
local.bibliographicCitation.lastpage201en_AU
local.bibliographicCitation.startpage201en_AU
local.contributor.affiliationMcClelland, David, College of Science, ANUen_AU
local.contributor.affiliationCollaboration, L. S., LIGO Scientific Collaborationen_AU
local.contributor.authoruidMcClelland, David, u8802403en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor510100 - Astronomical sciencesen_AU
local.identifier.absfor510800 - Quantum physicsen_AU
local.identifier.ariespublicationa383154xPUB6634en_AU
local.identifier.doi10.1364/CLEO_AT.2017.JTh3G.5en_AU
local.identifier.scopusID2-s2.0-85020459297
local.publisher.urlhttps://opg.optica.org/en_AU
local.type.statusPublished Versionen_AU

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