Observable bound for Gaussian illumination

Su-Yong Lee, Yonggi Jo, Taek Jeong, Junghyun Kim, Dong Hwan Kim, Dongkyu Kim, Duk Y. Kim, Yong Sup Ihn, and Zaeill Kim
Phys. Rev. A 105, 042412 – Published 8 April 2022

Abstract

We propose observable bounds for Gaussian illumination to maximize the signal-to-noise ratio, which minimizes the discrimination error between the presence and absence of a low-reflectivity target using Gaussian states. The observable bounds are achieved with mode-by-mode measurements. In the quantum regime using a two-mode squeezed vacuum state, our observable receiver outperforms the other feasible receivers whereas it cannot approach the quantum Chernoff bound. The corresponding observable cannot be implemented with heterodyne detections due to the additional vacuum noise. In the classical regime using a thermal state, a receiver implemented with a photon number difference measurement approaches its bound regardless of the signal mean photon number, while it asymptotically approaches the classical bound in the limit of a huge idler mean photon number.

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  • Received 24 June 2021
  • Accepted 24 March 2022

DOI:https://doi.org/10.1103/PhysRevA.105.042412

©2022 American Physical Society

Physics Subject Headings (PhySH)

Quantum Information, Science & Technology

Authors & Affiliations

Su-Yong Lee*, Yonggi Jo, Taek Jeong, Junghyun Kim, Dong Hwan Kim, Dongkyu Kim, Duk Y. Kim, Yong Sup Ihn, and Zaeill Kim

  • Agency for Defense Development, Daejeon 34186, Korea

  • *suyong2@add.re.kr
  • yonggi@add.re.kr

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Issue

Vol. 105, Iss. 4 — April 2022

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