Non-Gaussianity from superselection rules
quant-ph
Submitted: 2026-03-21
Updated: 2026-10-10
Comments: Comments are welcome, including suggestions of any relevant references we may have overlooked
Journal ref: Phys. Rev. Lett. 137, 050203 (2026)
DOI: 10.1103/5fl9-89j4
License: http://creativecommons.org/licenses/by/4.0/
The gist: The quantum theory of the electromagnetic field enables the description of multiphoton states exhibiting nonclassical statistical properties, often reflected in non-Gaussian phase-space distributions.
Terminology
Abstract
The quantum theory of the electromagnetic field enables the description of multiphoton states exhibiting nonclassical statistical properties, often reflected in non-Gaussian phase-space distributions. While non-Gaussianity alone does not fully characterize quantum states, several classifications have been proposed to hierarchize non-Gaussian states according to physically or informationally relevant resources. Here, we provide a physical interpretation of non-Gaussianity and connect it to a computational perspective by showing how a prominent classification-the stellar rank-emerges as a limiting case of the roots of polynomials that univocally represent bosonic states defined with a quantized phase reference, namely the Majorana polynomials. A direct consequence of our results is a revised interpretation of both the stellar rank and non-Gaussianity itself: when superselection rules are properly taken into account, quadrature non-Gaussianity - and nonzero stellar rank - act as witnesses of particle entanglement, rather than being linked with photon addition to Gaussian states as previously assumed. In addition, we show that because the stellar rank depends on a specific choice of coherent states, its relation to computational resources and potential quantum advantage is inherently basis-dependent, being naturally tied to quadrature eigenstates as the computational basis. Motivated by this observation, we generalize the notion of stellar rank to arbitrary computational bases, thereby establishing it as a genuine witness of bosonic resources that may enable quantum advantage.
Sources
- Witnesses of non-Gaussian features as lower bounds of stellar rank
- Phase-space representation of classical simulability for arbitrary bosonic encodings
- From Discrete to Continuous-Variable Systems via Jordan-Schwinger Tomographic Transformation
- Equivalence of continuous- and discrete-variable gate-based quantum computers with finite energy
- The quantum sky of Majorana stars
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