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arXiv:2608.23316 · APL Quantum

Exact Quasiprobability Hierarchy of the Double-Morse Oscillator: From Potential Geometry to Operator Ordering

Firoz Chogle, Berihu Teklu, Mauro F. Pereira

quant-phSubmitted Aug 24, 2026• Announced Aug 25, 2026• 0 citations• Revised Sep 20, 2026 (v4)
v1 · Aug 24, 2026v2 · Aug 25, 2026v3 · Aug 29, 2026v4 · Sep 20, 2026v5 · Oct 5, 2026
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Abstract

Phase-space and quasiprobability methods now play operational roles in quantum technologies, characterizing localization, non-Gaussianity, nonclassical resources, and coarse-graining. We develop an exact, representation-consistent analysis of the lowest quasi-exact ground state of the symmetric double-Morse oscillator. In the double-Morse potential, the dimensionless parameter $A$ controls the separation of the minima and the central barrier, thereby changing the physical ground state. At fixed $A$, the Cahill--Glauber parameter $s$ labels the quasiprobability $W_A^{(s)}(q,p)$: $s=0$, $-1$, and $1$ give the Wigner, Husimi $Q$, and Glauber--Sudarshan $P$ representations, respectively. Although the potential is double-welled for $0<A<1$, the exact ground-state amplitude is single-peaked at the origin and lies above the barrier; as $A$ approaches unity, the merged well remains locally quartic rather than harmonic. Closed analytical expressions are obtained for the Wigner function and Weyl characteristic function. The Wigner function displays the $A$-dependent exchange between position and momentum localization and retains negative regions, certifying nonclassicality and, for this pure state, non-Gaussianity. The Weyl function is its Fourier dual, generates symmetrically ordered moments and cumulants, and yields the full $s$-ordered hierarchy. For $s<0$, isotropic Gaussian smoothing suppresses fine sign-changing structure while preserving the large-scale localization envelope. The Husimi endpoint is nonnegative without implying classicality, whereas the $P$ representation remains distributional. Thus, $A$ controls the physical phase-space geometry, while $s$ controls how the same non-Gaussian and nonclassical state is resolved across complementary representations.

Comments
15 pages, 5 figures

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Abstract We present a comparative phase-space analysis of the Wigner function W , the Husimi distribution H , and a normalized auxiliary diagnostic derived from the Wigner function, | W | , for a one-dimensional quantum system undergoing a transition from a single-well to a symmetric double-well potential. Using the quasi-exactly solvable sextic oscillator as a benchmark, we analyze the two-dimensional phase-space structure of these quantities, together with their marginals and associated information-theoretic measures. We show that W uniquely captures phase-space interference, negativity, and the strongest information-theoretic signatures associated with the emergence of the double-well structure, whereas | W | and H primarily highlight geometric splitting and coarse-grained delocalization. In particular, | W | provides a sign-suppressed structural diagnostic that lies between the fully oscillatory Wigner description and the Gaussian-smoothed Husimi picture. These results clarify the distinct information retained by standard and derived phase-space characterizations of the state under continuous deformation of the confining potential.
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.
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