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arXiv:2610.32249

Bose-Einstein condensate in a shell: nonlinear modes and symmetry breaking

Alexander Wolf, Vladimir V. Konotop, Maxim A. Efremov

cond-mat.quant-gasnlin.PSquant-phSubmitted Oct 23, 2026• Announced Oct 26, 2026• 0 citations
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Abstract

The state of a quantum particle confined to a spherical surface is commonly described using spherical harmonics, which play a crucial role in solving many scientific problems featuring spherical symmetry. A mean-field description of a system of many interacting quantum particles confined to a spherical shell naturally leads to nonlinear generalizations of spherical harmonics. In this study, we analyze the emergence of such nonlinear modes in a shell-shaped Bose-Einstein condensate with both repulsive and attractive two-particle interactions. We find several classes of nonlinear modes. The first kind is an analytical continuation of a single spherical harmonic or their superposition for nonvanishing atom-atom interaction. Some of these solutions have planar counterparts in the form of Townes solitons and Townes vortices, which either appear stable even in the case of attractive interactions or can be stabilized by three-particle interactions. The second kind originate from symmetry-breaking bifurcations in the case of a repulsive interaction, and therefore have no linear counterparts. Moreover, we demonstrate the existence of a breathing dynamics that oscillates primarily between an unstable soliton and a stable vortex necklace state. Our findings show that the physics of nonlinear matter waves on curved geometries differs substantially from that in planar systems, suggesting the feasibility of observing these unconventional wave patterns experimentally.

AI Summary

The paper studies how interactions modify spherical-harmonic modes of a Bose–Einstein condensate confined to a thin spherical shell, and which stationary patterns and dynamics arise through symmetry breaking. It uses the angular Gross–Pitaevskii equation $i\partial_t\psi=\tfrac12L^2\psi+G|\psi|^2\psi$, with unit normalization and $G\approx4\pi aN/\Delta R$. Stationary states are computed by nonlinear eigenvalue iteration, stability by Bogoliubov–de Gennes spectra, and dynamics by direct simulations and spherical-harmonic Galerkin truncations. Nonlinear continuations of individual harmonics and selected degenerate superpositions exhibit stability windows for repulsive and attractive interactions. The homogeneous state has an analytical excitation spectrum and is dynamically stable for $G>-2\pi$. At $G=-2\pi$, a localized branch breaks rotational symmetry and approaches the planar Townes-soliton norm $|G|\approx5.85$. Attractive localized solitons and vortices are unstable in the cubic model but can be stabilized by repulsive quintic terms; the reported vortex example requires $\delta=30$. For repulsion, symmetry-breaking branches form vortex necklaces: the branch from the $l=1,m=0$ dark soliton appears near $G=26.3$ and has an extended stability interval. At $G=40$, an unstable dark soliton repeatedly evolves into a four-vortex configuration and approximately returns. Three spherical harmonics contain approximately 95% of the population; few-mode models reproduce the dynamics qualitatively but develop timing errors. The treatment assumes frozen radial motion, requiring interaction energies below the radial excitation gap. Mode families are explored selectively, largely through $l\leq4$. Experimental preparation routes are proposed, but no experimental verification is reported.

Little sign of AI-generated textIncrementalOverclaimsPossible error

Error found: The claimed breathing between an unstable soliton and a stable stationary vortex necklace is supported only by recurrence, modal populations, and qualitative resemblance, not by a demonstrated close approach to the stable stationary necklace. The localized charge-one solution retains an opposite-winding zero at the other pole under the paper’s own ansatz, so it is not a single vortex without an antivortex partner.

Written by gpt-6.1-sol from the paper's full text. Automated: it can be wrong.

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The state of a quantum particle confined to a spherical surface is commonly described using spherical harmonics, which play a crucial role in solving many scientific problems featuring spherical symmetry. A mean-field description of a system of many interacting quantum particles confined to a spherical shell naturally leads to nonlinear generalizations of spherical harmonics. In this study, we analyze the emergence of such nonlinear modes in a shell-shaped Bose-Einstein condensate with both repulsive and attractive two-particle interactions. We find several classes of nonlinear modes. The first kind is an analytical continuation of a single spherical harmonic or their superposition for nonvanishing atom-atom interaction. Some of these solutions have planar counterparts in the form of Townes solitons and Townes vortices, which either appear stable even in the case of attractive interactions or can be stabilized by three-particle interactions. The second kind originate from symmetry-breaking bifurcations in the case of a repulsive interaction, and therefore have no linear counterparts. Moreover, we demonstrate the existence of a breathing dynamics that oscillates primarily between an unstable soliton and a stable vortex necklace state. Our findings show that the physics of nonlinear matter waves on curved geometries differs substantially from that in planar systems, suggesting the feasibility of observing these unconventional wave patterns experimentally.
The paper studies how interactions modify spherical-harmonic modes of a Bose–Einstein condensate confined to a thin spherical shell, and which stationary patterns and dynamics arise through symmetry breaking. It uses the angular Gross–Pitaevskii equation i∂tψ=12L2ψ+G∣ψ∣2ψi\partial_t\psi=\tfrac12L^2\psi+G|\psi|^2\psii∂t​ψ=21​L2ψ+G∣ψ∣2ψ, with unit normalization and G≈4πaN/ΔRG\approx4\pi aN/\Delta RG≈4πaN/ΔR. Stationary states are computed by nonlinear eigenvalue iteration, stability by Bogoliubov–de Gennes spectra, and dynamics by direct simulations and spherical-harmonic Galerkin truncations.
Nonlinear continuations of individual harmonics and selected degenerate superpositions exhibit stability windows for repulsive and attractive interactions. The homogeneous state has an analytical excitation spectrum and is dynamically stable for G>−2πG>-2\piG>−2π. At G=−2πG=-2\piG=−2π, a localized branch breaks rotational symmetry and approaches the planar Townes-soliton norm ∣G∣≈5.85|G|\approx5.85∣G∣≈5.85. Attractive localized solitons and vortices are unstable in the cubic model but can be stabilized by repulsive quintic terms; the reported vortex example requires δ=30\delta=30δ=30. For repulsion, symmetry-breaking branches form vortex necklaces: the branch from the l=1,m=0l=1,m=0l=1,m=0 dark soliton appears near G=26.3G=26.3G=26.3 and has an extended stability interval.
At G=40G=40G=40, an unstable dark soliton repeatedly evolves into a four-vortex configuration and approximately returns. Three spherical harmonics contain approximately 95% of the population; few-mode models reproduce the dynamics qualitatively but develop timing errors.
The treatment assumes frozen radial motion, requiring interaction energies below the radial excitation gap. Mode families are explored selectively, largely through l≤4l\leq4l≤4. Experimental preparation routes are proposed, but no experimental verification is reported.
In this work we study spherical shell dark soliton states in three-dimensional atomic Bose-Einstein condensates. Their symmetry is exploited in order to analyze their existence, as well as that of topologically charged variants of the structures, and, importantly, to identify their linear stability Bogoliubov--de Gennes spectrum. We compare our effective one-dimensional spherical and two-dimensional cylindrical computations with the full three-dimensional numerics. An important conclusion is that such spherical shell solitons can be stable sufficiently close to the linear limit of the isotropic condensates considered herein. We have also identified their instabilities leading to the emergence of vortex line and vortex ring cages. In addition, we generalize effective particle pictures of lower-dimensional dark solitons and ring dark solitons to the spherical shell solitons concerning their equilibrium radius and effective dynamics around it. In this case too, we favorably compare, qualitatively and quantitatively, the resulting predictions such as the shell equilibrium radius with full numerical solutions in three dimensions.
The form and stability of quantum vortices in Bose-Einstein condensates with attractive atomic interactions is elucidated. They appear as ring bright solitons, and are a generalization of the Townes soliton to nonzero winding number m. An infinite sequence of radially excited stationary states appear for each value of m, which are characterized by concentric matter-wave rings separated by nodes, in contrast to repulsive condensates, where no such set of states exists. It is shown that robustly stable as well as unstable regimes may be achieved in confined geometries, thereby suggesting that vortices and their radial excited states can be observed in experiments on attractive condensates in two dimensions.
In the present work, we revisit two-component Bose-Einstein condensates in their fully three-dimensional (3D) form. Motivated by earlier studies of dark-bright solitons in the 1D case, we explore the stability of these structures in their fully 3D form in two variants. In one the dark soliton is planar and trapping a planar bright (disk) soliton. In the other case, a dark spherical shell soliton creates an effective potential in which a bright spherical shell of atoms is trapped in the second component. We identify these solutions as numerically exact states (up to a prescribed accuracy) and perform a Bogolyubov-de Gennes linearization analysis that illustrates that both structures can be dynamically stable in suitable intervals of sufficiently low chemical potentials. We corroborate this finding theoretically by analyzing the stability via degenerate perturbation theory near the linear limit of the system. When the solitary waves are found to be unstable, we explore their dynamical evolution via direct numerical simulations which, in turn, reveal wave forms that are more robust. Finally, using the SO(2) symmetry of the model, we produce multi-dark-bright planar or shell solitons involved in pairwise oscillatory motion.
The stability of nonlinear waves on curved surfaces is a problem of widespread interest across physics. Here, we establish the stability criteria for dark solitons on a spherical Bose-Einstein condensate. We demonstrate a sharp instability threshold in the nonlinear parameter, beyond which solitons decay into vortex dipoles via snake instabilities. Analytically and numerically, we prove this decay is dictated by a single unstable mode for each angular momentum m≥2m \geq 2m≥2, which is a universal mechanism that controls the resulting vortex state. Unlike in the full three-dimensional case, where snake instabilities lead to vortex rings, a dark soliton confined to the surface of a bubble can only decay into vortex pairs.
The novel phenomena arising from Bose-Einstein condensates with spatially and spatiotemporally modulated nonlinearities in external potential is reviewed from a theoretical viewpoint. We first present theoretical analysis and numerical studies of the localized nonlinear matter waves in one-dimensional single and two-component BECs with spatially and spatiotemporally modulated nonlinearities, respectively. It is shown that the spatially or spatiotemporally modulated nonlinearity can support stable novel localized nonlinear matter waves such as the breathing solitons and moving solitons. Then the quasi-two-dimensional BEC with spatially modulated nonlinearity is investigated and we show that all of the BECs, similar to the linear harmonic oscillator, can have an arbitrary number of localized nonlinear matter waves with discrete energies. Their properties are determined by the principal quantum number and secondary quantum number. Moreover, we investigate the quantized vortices in a rotating BEC with spatiotemporally modulated interaction in harmonic and anharmonic potentials, respectively. The exact quantized vortex and giant vortex solutions are constructed explicitly by similarity transformation. Their stability behavior is examined by numerical simulation, which shows that a new series of stable vortex states which are defined by radial and angular quantum numbers, can be supported by the spatiotemporally modulated interaction in this system. We find that there exist stable quantized vortices with large topological charges in repulsive condensates with spatiotemporally modulated interaction.
We consider the stability and dynamics of multiple dark solitons in cigar-shaped Bose-Einstein condensates. Our study is motivated by the fact that multiple matter-wave dark solitons may naturally form in such settings as per our recent work [Phys. Rev. Lett. 101, 130401 (2008)]. First, we study the dark soliton interactions and show that the dynamics of well-separated solitons (i.e., ones that undergo a collision with relatively low velocities) can be analyzed by means of particle-like equations of motion. The latter take into regard the repulsion between solitons (via an effective repulsive potential) and the confinement and dimensionality of the system (via an effective parabolic trap for each soliton). Next, based on the fact that stationary, well-separated dark multisoliton states emerge as a nonlinear continuation of the appropriate excited eigenstates of the quantum harmonic oscillator, we use a Bogoliubov-de Gennes analysis to systematically study the stability of such structures. We find that for a sufficiently large number of atoms, multiple soliton states are dynamically stable, while for a small number of atoms, we predict a dynamical instability emerging from resonance effects between the eigenfrequencies of the soliton modes and the intrinsic excitation frequencies of the condensate. Finally, we present experimental realizations of multisoliton states including a three-soliton state consisting of two solitons oscillating around a stationary one and compare the relevant results to the predictions of the theoretical mean-field model.