Observation of a kilogram-scale oscillator near its quantum ground state

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dc.identifier.uri http://dx.doi.org/10.15488/1304
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/1329
dc.contributor.author Aufmuth, Peter
dc.contributor.author Danzmann, Karsten
dc.contributor.author Hage, B.
dc.contributor.author Kwee, P.
dc.contributor.author Lueck, H.
dc.contributor.author Meier, Tobias
dc.contributor.author Thuering, A.
dc.contributor.author Willke, Benno
dc.contributor.author et al.
dc.date.accessioned 2017-04-06T08:24:40Z
dc.date.available 2017-04-06T08:24:40Z
dc.date.issued 2009
dc.identifier.citation Aufmuth, P.; Danzmann, K.; Hage, B.; Kwee, P.; Lueck, H. et al. (LIGO Scientific Collaboration): Observation of a kilogram-scale oscillator near its quantum ground state. In: New Journal of Physics 11 (2009), 73032. DOI: https://doi.org/10.1088/1367-2630/11/7/073032
dc.description.abstract We introduce a novel cooling technique capable of approaching the quantum ground state of a kilogram-scale system-an interferometric gravitational wave detector. The detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) operate within a factor of 10 of the standard quantum limit (SQL), providing a displacement sensitivity of 10(-18) m in a 100 Hz band centered on 150 Hz. With a new feedback strategy, we dynamically shift the resonant frequency of a 2.7 kg pendulum mode to lie within this optimal band, where its effective temperature falls as low as 1.4 mu K, and its occupation number reaches about 200 quanta. This work shows how the exquisite sensitivity necessary to detect gravitational waves can be made available to probe the validity of quantum mechanics on an enormous mass scale. eng
dc.description.sponsorship United States National Science Foundation
dc.description.sponsorship Science and Technology Facilities Council of the United Kingdom
dc.description.sponsorship Max-Planck-Society
dc.description.sponsorship State of Niedersachsen
dc.description.sponsorship Australian Research Council
dc.description.sponsorship Council of Scientific and Industrial Research of India
dc.description.sponsorship Istituto Nazionale di Fisica Nucleare of Italy
dc.description.sponsorship Spanish Ministerio de Educacion y Ciencia
dc.description.sponsorship Conselleria d’Economia Hisenda i Innovacio of the Govern de les Illes Balears
dc.description.sponsorship Scottish Funding Council
dc.description.sponsorship Scottish Universities Physics Alliance
dc.description.sponsorship National Aeronautics and Space Administration
dc.description.sponsorship Carnegie Trust
dc.description.sponsorship Leverhulme Trust
dc.description.sponsorship David and Lucile Packard Foundation
dc.description.sponsorship Research Corporation
dc.description.sponsorship Alfred P. Sloan Foundation
dc.language.iso eng
dc.publisher Bristol : IOP Publishing Ltd.
dc.relation.ispartofseries New Journal of Physics 11 (2009)
dc.rights CC BY-NC-SA 3.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by-nc-sa/3.0/
dc.subject radiation-pressure eng
dc.subject back-action eng
dc.subject cavity eng
dc.subject interferometer eng
dc.subject micromirror eng
dc.subject resonator eng
dc.subject mirror eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Observation of a kilogram-scale oscillator near its quantum ground state
dc.type Article
dc.type Text
dc.relation.essn 1367-2630
dc.relation.doi https://doi.org/10.1088/1367-2630/11/7/073032
dc.bibliographicCitation.volume 11
dc.bibliographicCitation.firstPage 73032
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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