Quantum metrology for gravitational wave astronomy

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Schnabel, Roman; Mavalvala, Nergis; McClelland, David E.; Lam, Ping K.: Quantum metrology for gravitational wave astronomy. In: Nature Communications 1 (2010), 121. DOI: https://doi.org/10.1038/ncomms1122

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To cite the version in the repository, please use this identifier: https://doi.org/10.15488/1635

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Sum total of downloads: 381




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Abstract: 
Einstein's general theory of relativity predicts that accelerating mass distributions produce gravitational radiation, analogous to electromagnetic radiation from accelerating charges. These gravitational waves (GWs) have not been directly detected to date, but are expected to open a new window to the Universe once the detectors, kilometre-scale laser interferometers measuring the distance between quasi-free-falling mirrors, have achieved adequate sensitivity. Recent advances in quantum metrology may now contribute to provide the required sensitivity boost. The so-called squeezed light is able to quantum entangle the high-power laser fields in the interferometer arms, and could have a key role in the realization of GW astronomy.
License of this version: CC BY 4.0 Unported
Document Type: article
Publishing status: publishedVersion
Issue Date: 2010
Appears in Collections:Fakultät für Mathematik und Physik

distribution of downloads over the selected time period:

downloads by country:

pos. country downloads
total perc.
1 image of flag of Germany Germany 304 79.79%
2 image of flag of United States United States 13 3.41%
3 image of flag of China China 12 3.15%
4 image of flag of Chile Chile 9 2.36%
5 image of flag of United Kingdom United Kingdom 6 1.57%
6 image of flag of Sweden Sweden 5 1.31%
7 image of flag of France France 5 1.31%
8 image of flag of No geo information available No geo information available 4 1.05%
9 image of flag of Korea, Republic of Korea, Republic of 4 1.05%
10 image of flag of Russian Federation Russian Federation 3 0.79%
    other countries 16 4.20%

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