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  • Letter

Exactly solvable model behind Bose-Hubbard dimers, Ince-Gauss beams, and aberrated optical cavities

R. Gutiérrez-Cuevas1,2,*, D. H. J. O'Dell3,†, M. R. Dennis4,‡, and M. A. Alonso2,5,6,§

  • 1Institut Langevin, ESPCI Paris, Université PSL, CNRS, 75005 Paris, France
  • 2Aix Marseille Université, CNRS, Centrale Marseille, Institut Fresnel, UMR 7249, 13397 Marseille Cedex 20, France
  • 3Department of Physics and Astronomy, McMaster University, 1280 Main Street W., Hamilton, Ontario, Canada, L8S 4M1
  • 4School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, United Kingdom
  • 5The Institute of Optics, University of Rochester, Rochester, New York 14627, USA
  • 6Laboratory for Laser Energetics, University of Rochester, Rochester, New York 14627, USA

  • *rodrigo.gutierrez-cuevas@espci.fr
  • †dodell@mcmaster.ca
  • ‡m.r.dennis@bham.ac.uk
  • §miguel.alonso@fresnel.fr

Phys. Rev. A 107, L031502 – Published 28 March, 2023

DOI: https://doi.org/10.1103/PhysRevA.107.L031502

Abstract

By studying the effects of quadratic anisotropy and quartic perturbations on two-dimensional harmonic oscillators, one arrives at a simple model, termed here the Ince oscillator, whose analytic solutions are given in terms of Ince polynomials. This one model unifies diverse physical systems, including aberrated optical cavities that are shown to support Ince-Gauss beams as their modes, and the two-mode Bose-Hubbard dimer describing two coupled superfluids. The Ince oscillator model describes a topological transition which can have very different origins: in the optical case, which is fundamentally linear, it is driven by the ratio of astigmatic to spherical mirror aberrations, whereas in the superfluid case it is driven by the ratio of particle tunneling to interparticle interactions and corresponds to macroscopic quantum self-trapping.

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