Entanglement-assisted detection of fading targets via correlation-to-displacement conversion
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PhysRevA.107.062405.pdf
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Affiliation
Department of Electrical and Computer Engineering, University of ArizonaJames C. Wyant College of Optical Sciences, University of Arizona
Issue Date
2023-06-05
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American Physical SocietyCitation
Chen, Xin, and Quntao Zhuang. "Entanglement-assisted detection of fading targets via correlation-to-displacement conversion." Physical Review A 107.6 (2023): 062405.Journal
Physical Review ARights
© 2023 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Quantum illumination utilizes an entanglement-enhanced sensing system to outperform classical illumination in detecting a suspected target, despite the entanglement-breaking loss and noise. However, practical and optimal receiver design to fulfill the quantum advantage has been a long open problem. Recently, Shi et al. [arXiv:2207.06609 (2022)] proposed the correlation-to-displacement ('C - D') conversion module to enable an optimal receiver design that greatly reduces the complexity of the previous known optimal receiver [Q. Zhuang, Z. Zhang, and J. H. Shapiro, Phys. Rev. Lett. 118, 040801 (2017)10.1103/PhysRevLett.118.040801]. There, the analyses of the conversion module assume an ideal target with a known reflectivity and a fixed return phase. In practical applications, however, targets often induce a random return phase; moreover, their reflectivities can have fluctuations obeying a Rayleigh distribution. In this paper, we extend the analyses of the C - D module to realistic targets and show that the entanglement advantage is maintained albeit reduced. In particular, the conversion module allows exact and efficient performance evaluation despite the non-Gaussian nature of the quantum channel involved. © 2023 American Physical Society.Note
Immediate accessISSN
2469-9926Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1103/PhysRevA.107.062405
