Beating the Standard Sensitivity-Bandwidth Limit of Cavity-Enhanced Interferometers with Internal Squeezed-Light Generation.

Beating the Standard Sensitivity-Bandwidth Limit of Cavity-Enhanced Interferometers with Internal Squeezed-Light Generation.
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DOI:
10.1103/physrevlett.118.143601
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发表时间:
2017-02
影响因子:
8.6
通讯作者:
M. Korobko;L. Kleybolte;S. Ast;H. Miao;Yanbei Chen;R. Schnabel
M. Korobko;L. Kleybolte;S. Ast;H. Miao;Yanbei Chen;R. Schnabel
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
M. Korobko;L. Kleybolte;S. Ast;H. Miao;Yanbei Chen;R. Schnabel

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The shot-noise limited peak sensitivity of cavity-enhanced interferometric measurement devices, such as gravitational-wave detectors, can be improved by increasing the cavity finesse, even when comparing fixed intracavity light powers. For a fixed light power inside the detector, this comes at the price of a proportional reduction in the detection bandwidth. High sensitivity over a large span of signal frequencies, however, is essential for astronomical observations. It is possible to overcome this standard sensitivity-bandwidth limit using nonclassical correlations in the light field. Here, we investigate the internal squeezing approach, where the parametric amplification process creates a nonclassical correlation directly inside the interferometer cavity. We theoretically analyze the limits of the approach and measure 36% increase in the sensitivity-bandwidth product compared to the classical case. To our knowledge, this is the first experimental demonstration of an improvement in the sensitivity-bandwidth product using internal squeezing, opening the way for a new class of optomechanical force sensing devices.