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This paper investigates the geometric structure of Gaussian quantum states, specifically deriving the Bures metric's behavior near uncertainty limits and its transition to classical Fisher-Rao geometry. By analyzing spectral boundaries and potential functions for bosonic systems, it clarifies how relative quantum corrections vanish at large symplectic eigenvalues, offering rigorous mathematical insights into the interface between quantum and classical statistical regimes.
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The Global Geometry of the Gaussian Bures Manifold: Admissible Domain, Spectral Boundary, and Asymptotic Classicality

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arXiv:2609.17563v1 Announce Type: new Abstract: We construct the covariance-sector Bures geometry of centered bosonic Gaussian states from the Gaussian symmetric-logarithmic-derivative equation and determine its quantum-admissible domain. At the Williamson uncertainty floor, the boundary geometry is anisotropic: spectrum-changing radial coefficients diverge, whereas squeezing and rotation directions along the pure Gaussian orbit remain finite. Dually, the covariance cometric acquires an exact \(m^2\)-dimensional kernel when \(m\) modes become pure, yet the boundary remains at finite radial Bures distance. We derive the potential \[ \Phi=-\tfrac12\sum_k\log(\nu_k^2-\tfrac14), \] which generates fixed-frame covariance dilation and equals \(\beta F\) on fixed-Hamiltonian thermal families. At large symplectic eigenvalue, the relative quantum correction is \(O(\hbar^2/\nu^2)\), recovering covariance Fisher--Rao geometry. This intrinsic classical regime differs from the pure-state boundary, where classical statistics require a specified measurement channel. As a secondary comparison, the normalized Bures, Fisher--Rao, and action-matched Bures--Wasserstein determinant densities possess an exact one-mode junction at \[ (x,\eta)=(\sqrt{\varphi},\sqrt{\varphi}),\qquad x=2\nu/\hbar. \] This junction is kinematic, and its branch interpretation is conditional. At a prescribed finite nonzero compression rate, the Bures action diverges while the Bures--Wasserstein cost remains finite; a bounded Bures budget instead enforces radial deceleration.

Abstract:We construct the covariance-sector Bures geometry of centered bosonic Gaussian states from the Gaussian symmetric-logarithmic-derivative equation and determine its quantum-admissible domain. At the Williamson uncertainty floor, the boundary geometry is anisotropic: spectrum-changing radial coefficients diverge, whereas squeezing and rotation directions along the pure Gaussian orbit remain finite. Dually, the covariance cometric acquires an exact \(m^2\)-dimensional kernel when \(m\) modes become pure, yet the boundary remains at finite radial Bures distance. We derive the potential \[ \Phi=-\tfrac12\sum_k\log(\nu_k^2-\tfrac14), \] which generates fixed-frame covariance dilation and equals \(\beta F\) on fixed-Hamiltonian thermal families. At large symplectic eigenvalue, the relative quantum correction is \(O(\hbar^2/\nu^2)\), recovering covariance Fisher--Rao geometry. This intrinsic classical regime differs from the pure-state boundary, where classical statistics require a specified measurement channel. As a secondary comparison, the normalized Bures, Fisher--Rao, and action-matched Bures--Wasserstein determinant densities possess an exact one-mode junction at \[ (x,\eta)=(\sqrt{\varphi},\sqrt{\varphi}),\qquad x=2\nu/\hbar. \] This junction is kinematic, and its branch interpretation is conditional. At a prescribed finite nonzero compression rate, the Bures action diverges while the Bures--Wasserstein cost remains finite; a bounded Bures budget instead enforces radial deceleration.

arXiv:2609.17563 [quant-ph]

(or arXiv:2609.17563v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2609.17563 Focus to learn more arXiv-issued DOI via DataCite

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