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Experimental Separability Geometry

Pasquale Kaboth

Published Aug 25, 2026• 0 citations
Publisher
DOI
10.5281/zenodo.22100169

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The effect of boundary deformation on the non-separable entanglement which appears in the classical elec- tromagnetic field is considered. A quantum chaotic billiard geometry is used to explore the influence of a mechanical modification of the optical fiber cross-sectional geometry on the production of non-separable entan- glement within classical fields. For the experimental realization of our idea, we propose an optical fiber with a cross section that belongs to the family of Robnik chaotic billiards. Our results show that a modification of the fiber geometry from a regular to a chaotic regime can enhance the transverse mode entanglement. Our proposal can be realized in a very simple experimental set-up which consists of a specially designed optical fiber where non-entangled light enters at the input end and entangled light propagates out at the output end after interacting with a fiber boundary that is known to generate chaotic behavior.
Description:A geometric analysis of GHZ–Mermin experiments that separates deterministic parity obstruction, classical Bell constraints, and independent attenuation mechanisms using the incidence structure of K4K_4K4​. The paper derives an exact edge-cone compatibility criterion, proves uniqueness of attenuation failure, establishes the sharp tradeoff W≤3+e−δAW\le 3+e^{-\delta_A}W≤3+e−δA​, extends the construction to KnK_nKn​, and develops a coarse-grained KL/Fisher framework for statistical separation and experimental design. Keywords:GHZ–Mermin experiments; Bell nonlocality; incidence geometry; edge cones; parity obstruction; attenuation models; Mermin inequality; contextuality; Kullback–Leibler divergence; Fisher information; experimental design; statistical separation; complete graphs.
We study the phase separation configurations and their rotational properties for a mixture of two interacting charged Bose-Einstein condensates subject to a magnetic field trapped in disc and Corbino geometries. We calculate the ground state energies of azimuthal and radial phase separation configurations using the Gross-Pitaevskii and the Thomas-Fermi approximations. We show that the results for experimentally relevant system parameters from both approaches are in good agreement. The immiscible mixture in both geometries with equal intracomponent interactions favors the azimuthal phase separation for any intercomponent interactions. Only an imbalance in the intracomponent interactions can result in a transition to the radial phase separation, for which the transition becomes sensitive to the shape of the trap. We present phase diagrams as function of the inter and intracomponent interactions. While the radial phase separation is widely favoured in disc geometry, the azimuthal phase separation is favoured for narrower Corbino geometries. We explore the rotational properties of the spatially separated condensates under the magnetic field, studying their angular momenta and velocity fields. The quantization of circulation breaks down for the azimuthal phase separation. In this case, the bulk region of the condensate continues to display superfluid flow behavior whereas the velocity field shows a rigid body behavior along the phase boundaries.