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Science China Physics Mechanics and Astronomy

Revealing nonclassicality via s-ordered phase-space distribution

Yue Zhang, Shuheng Liu, Boxuan Jing, Qiongyi He, Shunlong Luo

Published Sep 19, 2022• 5 citations
Publisher
DOI
10.1007/s11433-022-1968-8

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Various phase-space distributions, from the celebrated Wigner function, to the Husimi $$Q$$ function and the Glauber–Sudarshan $$P$$ distribution, have played an interesting and important role in the phase-space formulation of quantum mechanics in general, and quantum optics in particular. A unified approach to all these distributions based on the notion of the $$s$$ -ordered phase-space distribution was introduced by Cahill and Glauber. With the intention of illuminating the physical meaning of the parameter $$s$$ , we interpret the $$s$$ -ordered phase-space distribution as the Wigner function of a state under the Gaussian noise channel, and thus reveal an intrinsic connection between the $$s$$ -ordered phase-space distribution and the Gaussian noise channel, which yields a physical insight into the $$s$$ -ordered phase-space distribution. In this connection, the parameter $$-s/2$$ (rather than the original $$s$$ ) acquires the role of the noise occurring in the Gaussian noise channel. An alternative representation of the Gaussian noise channel as the scaling-measurement preparation in a coherent states is illuminated. Furthermore, by exploiting the freedom in the parameter $$s$$ , we introduce a computable and experimentally testable quantifier for optical nonclassicality, reveal its basic properties, and illustrate it by typical examples. A simple and convenient criterion for optical nonclassicality in terms of the $$s$$ -ordered phase-space distribution is derived.

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Reply to “Comment on ‘Nonclassicality indicator for the real phase-space distribution functions’ ”

Siamak Khademi, Parvin Sadeghi, S. Nasiri

Sadeghi et al. [Phys. Rev. A 82, 012102 (2010)] presented a new nonclassicality indicator which works properly for Husimi and Rivier distribution functions as well as the Wigner distribution function. Some objections on the Sadeghi nonclassicality indicator are presented by Kenfack (preceding Comment, ``Nonclassicality indicator for the real phase-space distribution functions'', Phys. Rev. A 93, 036101 (2016). In this Reply, some misconceptions on Sadeghi's nonclassicality indicator are discussed and clarified.

Physical Review A•Mar 16, 2016•5 citations

Generalized structure of higher order nonclassicality

Amit Verma, Anirban Pathak

arXiv:0901.3193•Physics Letters A•Dec 22, 2009•50 citations
From the Wigner function to the sss-ordered phase-space distribution via a Gaussian noise channel
Various phase-space distributions, from the celebrated Wigner function, to the Husimi QQQ function and the Glauber–Sudarshan PPP distribution, have played an interesting and important role in the phase-space formulation of quantum mechanics in general, and quantum optics in particular. A unified approach to all these distributions based on the notion of the sss -ordered phase-space distribution was introduced by Cahill and Glauber. With the intention of illuminating the physical meaning of the parameter sss , we interpret the sss -ordered phase-space distribution as the Wigner function of a state under the Gaussian noise channel, and thus reveal an intrinsic connection between the sss -ordered phase-space distribution and the Gaussian noise channel, which yields a physical insight into the sss -ordered phase-space distribution. In this connection, the parameter −s/2-s/2−s/2 (rather than the original sss ) acquires the role of the noise occurring in the Gaussian noise channel. An alternative representation of the Gaussian noise channel as the scaling-measurement preparation in a coherent states is illuminated. Furthermore, by exploiting the freedom in the parameter sss , we introduce a computable and experimentally testable quantifier for optical nonclassicality, reveal its basic properties, and illustrate it by typical examples. A simple and convenient criterion for optical nonclassicality in terms of the sss -ordered phase-space distribution is derived.
We devise a method to certify nonclassical features via correlations of phase-space distributions by unifying the notions of quasiprobabilities and matrices of correlation functions. Our approach complements and extends recent results that were based on Chebyshev's integral inequality \cite{BA19}. The method developed here correlates arbitrary phase-space functions at arbitrary points in phase space, including multimode scenarios and higher-order correlations. Furthermore, our approach provides necessary and sufficient nonclassicality criteria, applies to phase-space functions beyond s -parametrized ones, and is accessible in experiments. To demonstrate the power of our technique, the quantum characteristics of discrete- and continuous-variable, single- and multimode, as well as pure and mixed states are certified only employing second-order correlations and Husimi functions, which always resemble a classical probability distribution. Moreover, nonlinear generalizations of our approach are studied. Therefore, a versatile and broadly applicable framework is devised to uncover quantum properties in terms of matrices of phase-space distributions.
Sadeghi et al. [Phys. Rev. A 82, 012102 (2010)] presented a new nonclassicality indicator which works properly for Husimi and Rivier distribution functions as well as the Wigner distribution function. Some objections on the Sadeghi nonclassicality indicator are presented by Kenfack (preceding Comment, ``Nonclassicality indicator for the real phase-space distribution functions'', Phys. Rev. A 93, 036101 (2016). In this Reply, some misconceptions on Sadeghi's nonclassicality indicator are discussed and clarified.