4.6 Article

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

Journal

NEW JOURNAL OF PHYSICS
Volume 11, Issue -, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1367-2630/11/7/073032

Keywords

-

Funding

  1. United States National Science Foundation
  2. Science and Technology Facilities Council of the United Kingdom
  3. Max-Planck-Society
  4. State of Niedersachsen/Germany
  5. Australian Research Council
  6. Council of Scientific and Industrial Research of India
  7. Istituto Nazionale di Fisica Nucleare of Italy
  8. Spanish Ministerio de Educacion y Ciencia
  9. Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears
  10. Scottish Funding Council
  11. Scottish Universities Physics Alliance
  12. The National Aeronautics and Space Administration
  13. Carnegie Trust
  14. Leverhulme Trust
  15. David and Lucile Packard Foundation
  16. Research Corporation
  17. Alfred P Sloan Foundation
  18. Science and Technology Facilities Council [PP/F00110X/1, PP/F001096/1, PP/E001203/1, ST/G504284/1, PP/F001118/1] Funding Source: researchfish
  19. Direct For Mathematical & Physical Scien
  20. Division Of Physics [0653653, 0757058] Funding Source: National Science Foundation
  21. Division Of Physics
  22. Direct For Mathematical & Physical Scien [0905184, 855313] Funding Source: National Science Foundation
  23. STFC [PP/E001203/1, PP/F001096/1, PP/F00110X/1, ST/G504284/1, PP/F001118/1] Funding Source: UKRI

Ask authors/readers for more resources

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.

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