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Cited by 385

The DOI matches its Crossref record; 83 of the 83 references it cites were found in a registry or an index.

Quantum metrology for gravitational wave astronomy

Open access
Schnabel, Roman, Mavalvala, Nergis, McClelland, David E., Lam, Ping K.·2010·Nature Communications
DOI 10.1038/ncomms1122
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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.

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Metadata

Authors
Schnabel, R., Mavalvala, N., McClelland, D. E., & Lam, P. K.
Venue
Nature Communications
Publisher
Springer Science and Business Media LLC
Published
2010-11-16
Volume
1
Issue
1
Pages
121-121
ISSN
2041-1723 (ISSN-L)
DOI
10.1038/ncomms1122
OpenAlex
W2007523837
Cited by
385
References
83
FWCI
7.48
Type
journal article
Language
en
Open access
bronze

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