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arXiv:2610.36438

Dynamical behaviour of the mass tensor in the lattice

Josué Calle, Diego Sanjinés, Evaristo Mamani

quant-phSubmitted Oct 27, 2026• Announced Oct 28, 2026
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Abstract

We study with the semiclassical model the dynamics of a particle moving in a orthorrombic lattice by the hopping mechanism in the presence of a static Coulomb field and a rapidly oscillating homogeneous field. Based on results for the anisotropic Kepler problem, where a chaotic trajectory arises due to different masses of the particle in the X and Y directions, and since this result is also obtained in the rectangular lattice at the continuum limit, the application of the oscillating field allows reparameterizing the effective masses so that they become equal in both directions. Thus, the result is an elliptic trajectory in the continuum limit of the lattice. This chaos-order transition is confirmed by the calculation of Lyapunov exponents for the different trajectories. It is also found that the application of an external magnetic field in the Z direction of the lattice yields chaos control which can be generalized beyond the simple case of the circular trajectory shown in this work. The previous scheme of chaos control was extended for trajectories in 3D in the continuum limit of the orthorrombic lattice which is also equivalent to the far region approximation where the particle moves with respect to the Coulomb field origin. In this case it found that the chaos control technique permits to observe two different dynamical regimes which, although consistent with Bohr-van Leeuwen theorem, suggests that an observable way to distinguish one from the other is to be sought.

AI Summary

The paper investigates whether a rapidly oscillating electric field can suppress chaotic semiclassical motion of a charged particle hopping on an orthorhombic lattice around a Coulomb impurity. The mechanism is to tune anisotropic effective masses until the continuum dynamics reduces to the isotropic Kepler problem. Starting from a nearest-neighbour tight-binding dispersion, high-frequency time averaging gives effective hoppings $\tilde A=AJ_0(\alpha)$ and $\tilde B=BJ_0(\beta)$, where $\alpha$ and $\beta$ encode the drive components. In the continuum limit, the effective mass ratio becomes $\tilde m_x/\tilde m_y=\xi J_0(\beta)/J_0(\alpha)$. For the studied anisotropy $\xi=2.94$, choosing $J_0(\alpha)/J_0(\beta)=2.94$ restores equal masses and elliptical trajectories. Numerical trajectories, angular-momentum conservation and reduced finite-time Lyapunov estimates support this transition; one example uses $\alpha=2$ and $\beta\approx2.262$. A simulation of the explicitly driven dynamics checks the averaging approximation at a drive-to-orbit frequency ratio of 2314. Away from the continuum limit, a heuristic magnetic-field extension is tested numerically for circular motion. Three-dimensional simulations with 1000 noninteracting particles compare chaotic near-impurity motion with approximately elliptical motion farther away, finding different magnetic-field time traces but approximately zero mean field at the impurity. The treatment is semiclassical rather than fully quantum. The Lyapunov algorithm does not produce nonpositive exponents for the elliptical cases. Finite-lattice control beyond circular trajectories and an experimentally observable distinction between the three-dimensional regimes are left open.

No sign of AI-generated textIncrementalOverclaimsStrong assumptionsPossible error

Central claim may not hold: Section 4 incorrectly assigns negative maximal Lyapunov exponents to regular Kepler ellipses, whose maximal asymptotic exponent is zero. Three of the six claimed equal-mass control points have negative J0(beta), whereas the stated condition at alpha=2 requires a positive value, so they do not restore an isotropic Kepler Hamiltonian. The magnetic field constructed for the circular orbit in Section 5 exactly cancels the Coulomb force in the paper's equations, implying constant quasimomenta and velocities rather than circular motion.

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

Comments
19 pages, 10 figures

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We study with the semiclassical model the dynamics of a particle moving in a orthorrombic lattice by the hopping mechanism in the presence of a static Coulomb field and a rapidly oscillating homogeneous field. Based on results for the anisotropic Kepler problem, where a chaotic trajectory arises due to different masses of the particle in the X and Y directions, and since this result is also obtained in the rectangular lattice at the continuum limit, the application of the oscillating field allows reparameterizing the effective masses so that they become equal in both directions. Thus, the result is an elliptic trajectory in the continuum limit of the lattice. This chaos-order transition is confirmed by the calculation of Lyapunov exponents for the different trajectories. It is also found that the application of an external magnetic field in the Z direction of the lattice yields chaos control which can be generalized beyond the simple case of the circular trajectory shown in this work. The previous scheme of chaos control was extended for trajectories in 3D in the continuum limit of the orthorrombic lattice which is also equivalent to the far region approximation where the particle moves with respect to the Coulomb field origin. In this case it found that the chaos control technique permits to observe two different dynamical regimes which, although consistent with Bohr-van Leeuwen theorem, suggests that an observable way to distinguish one from the other is to be sought.
The paper investigates whether a rapidly oscillating electric field can suppress chaotic semiclassical motion of a charged particle hopping on an orthorhombic lattice around a Coulomb impurity. The mechanism is to tune anisotropic effective masses until the continuum dynamics reduces to the isotropic Kepler problem.
Starting from a nearest-neighbour tight-binding dispersion, high-frequency time averaging gives effective hoppings A~=AJ0(α)\tilde A=AJ_0(\alpha)A~=AJ0​(α) and B~=BJ0(β)\tilde B=BJ_0(\beta)B~=BJ0​(β), where α\alphaα and β\betaβ encode the drive components. In the continuum limit, the effective mass ratio becomes m~x/m~y=ξJ0(β)/J0(α)\tilde m_x/\tilde m_y=\xi J_0(\beta)/J_0(\alpha)m~x​/m~y​=ξJ0​(β)/J0​(α). For the studied anisotropy ξ=2.94\xi=2.94ξ=2.94, choosing J0(α)/J0(β)=2.94J_0(\alpha)/J_0(\beta)=2.94J0​(α)/J0​(β)=2.94 restores equal masses and elliptical trajectories. Numerical trajectories, angular-momentum conservation and reduced finite-time Lyapunov estimates support this transition; one example uses α=2\alpha=2α=2 and β≈2.262\beta\approx2.262β≈2.262. A simulation of the explicitly driven dynamics checks the averaging approximation at a drive-to-orbit frequency ratio of 2314.
Away from the continuum limit, a heuristic magnetic-field extension is tested numerically for circular motion. Three-dimensional simulations with 1000 noninteracting particles compare chaotic near-impurity motion with approximately elliptical motion farther away, finding different magnetic-field time traces but approximately zero mean field at the impurity.
The treatment is semiclassical rather than fully quantum. The Lyapunov algorithm does not produce nonpositive exponents for the elliptical cases. Finite-lattice control beyond circular trajectories and an experimentally observable distinction between the three-dimensional regimes are left open.
We study the motion of a particle in a 3-dimensional lattice in the presence of a potential −V1/r, but we demonstrate semiclassicaly that the trajectories will always remain in a plane which can be taken as a rectangular lattice. The Hamiltonian model for this problem is the conservative tight-binding one with lattice constants a, b and hopping elements A, B in the XY axes, respectively. We use the semiclassical and quantum formalisms; for the latter we apply the pseudo-spectral algorithm to integrate the Schrödinger equation. Since the lattice discrete subspace is not isotropic, the angular momentum is not conserved, which has interesting consequences as chaotic trajectories and precession trajectories, similar to the astronomical precession trajectories due to non-central gravitational forces, notably, the non-relativistic Mercury’s perihelion precession. Although the elements of the mass tensor are naturally different in a rectangular lattice, these can be chosen to be still different in the continuum, which permits to study the motion with kinetic energies pi2/2mi (i = x,y). We calculate also the contour plots of an initial Gaussian wavepacket as it moves in the lattice and we propose an “intrinsec angular momentum” S associated to its asymmetrical deformation, such that the quantum and semiclassical angular momenta, Lq, Lc , respectively, could be related as Lq = Lc + αS.
The dynamics of an ensemble of two-level atoms moving through a single-mode lossless cavity is investigated in the semiclassical and rotating-wave approximations. The dynamical system for the expectation values of the atomic and field observables is considered as a perturbation to one of the following integrable versions: (i) a model with atoms moving through a spatially inhomogeneous resonant field, and (ii) a model with atoms interacting with a nonresonant eigenmode which is assumed to be homogeneous on the cavity size. We find the general exact solutions for both the models and show that they contain special solutions describing a coherent effect of population and radiation trapping. Using the Melnikov method, we prove analytically transverse intersections of stable and unstable manifolds of a hyperbolic fixed point under a small modulation of the vacuum Rabi frequency. These intersections are believed to provide the Smale horseshoe mechanism of Hamiltonian chaos. The analytical results are accompanied with direct computation of topographical maps of maximal Lyapunov exponents that give a representative image of regularity and chaos in the atom-field system in different ranges of its control parameters--the frequency detuning, the number, and the velocity of atoms.
We investigate the semiclassical Kepler/Coulomb problem using the classical constants of the motion in the framework of Nelson's stochastic mechanics. This is done by considering the eigenvalue relations for a family of coherent states (known as the atomic elliptic states) whose wave functions are concentrated on the elliptical orbit corresponding to the associated classical problem. We show that these eigenvalue relations lead to identities for the semiclassical energy, angular momentum and Hamilton–Lenz–Runge vectors in the elliptical case. These identities are then extended to include the cases of circular, parabolic and hyperbolic motions. We show that in all cases the semiclassical wave function is determined by our identities and so our identities can be seen as defining a semiclassical Kepler/Coulomb problem. The results are interpreted in terms of two dynamical systems: one a complex valued solution to the classical mechanics for a Coulomb potential and the other the drift field for a semiclassical Nelson diffusion.
Particle trajectories guided by the wave function are well-defined through Bohmian mechanics, which is a causal interpretation of quantum mechanics. Periodic and chaotic behaviours could be exhibited from the certain classical integrable systems that have been shown within this framework. In this study, we developed Mathematica programs to plot the Bohmian trajectories and Lyapunov exponents. These programs serve as computer experiments for numerical generation and illustration of the results. We show that the behaviours of commensurate two-dimensional harmonic oscillator systems are dependent on ratios of frequency.
We discuss some problems of dissipative chaos for open quantum systems in the framework of semiclassical and quantum distributions.For this goal, we propose a driven nonlinear oscillator with time-dependent coefficients, i.e. with time-dependent Kerr-nonlinearity and time-modulated driving field.This model showing both regular and chaotic dynamics in the classical limit is realized in several experimental schemes.Quantum dissipative chaos is analyzed on the base of numerical method of quantum trajectories.Three quantities are studied: the Wigner function of oscillatory mode from the point of view of quantum-assemble theory and both semiclassical Poincaré section and quantum Poincaré section calculated on a single quantum trajectory.The comparatively analysis of these distributions for various operational chaotic regimes of the models is performed, as well as scaling invariance in dissipative chaos and quantum interference effects assisted by chaos are discussed.
Abstract Chaos in Bohmian quantum mechanics is an open field of research. In general, most of the 3D Bohmian trajectories are free to wander around the 3D space. However, there are cases where the evolution of the trajectories is dictated by exact or approximate integrals of motion. A first case corresponds to partial integrability, where the trajectories (ordered and chaotic) evolve on certain integral surfaces. A second case corresponds to ordered trajectories. In this paper we extend our previous work in 3D Bohmian chaos by using both forms of integrability and discuss their physical implications.