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Reduction of optimum light power with Heisenberg-limited photon-counting noise in interferometric gravitational-wave detectors

✍ Scribed by Constantin Brif


Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
66 KB
Volume
263
Category
Article
ISSN
0375-9601

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✦ Synopsis


We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of interferometric gravitational-wave detectors, depends on properties of input states of light. We analyze the situation with specially prepared nonclassical input states which reduce the photon-counting noise to the Heisenberg limit. This results in a great reduction of the optimum light power needed to achieve the standard quantum limit, compared to the usual configuration.