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

M. Korobko, L. Kleybolte, S. Ast, H. Miao, Y. Chen, and R. Schnabel
Phys. Rev. Lett. 118, 143601 – Published 7 April 2017
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Abstract

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.

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  • Received 12 February 2017

DOI:https://doi.org/10.1103/PhysRevLett.118.143601

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & OpticalGravitation, Cosmology & Astrophysics

Authors & Affiliations

M. Korobko1,*, L. Kleybolte1, S. Ast2, H. Miao3, Y. Chen4, and R. Schnabel1

  • 1Institut für Laserphysik und Zentrum für Optische Quantentechnologien, Universität Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
  • 2Institut für Gravitationsphysik, Leibniz Universität Hannover and Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Callinstraße 38, 30167 Hannover, Germany
  • 3Institute of Gravitational Wave Astronomy, University of Birmingham, Birmingham B15 2TT, United Kingdom
  • 4Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, California 91125, USA

  • *mikhail.korobko@physnet.uni-hamburg.de

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Issue

Vol. 118, Iss. 14 — 7 April 2017

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