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Related papers: Arnold diffusion in the planar elliptic restricted…

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Traditional analytical theories of celestial mechanics are not well-adapted when dealing with highly elliptical orbits. On the one hand, analytical solutions are quite generally expanded into power series of the eccentricity and so limited…

Earth and Planetary Astrophysics · Physics 2016-06-14 Guillaume Lion , Gilles Métris

The genericity of Arnold diffusion in the analytic category is an open problem. In this paper, we study this problem in the following a priori unstable Hamiltonian system with a time-periodic perturbation…

Dynamical Systems · Mathematics 2023-06-06 Qinbo Chen , Rafael de la Llave

We introduce and analyze a model for the transport of particles or energy in extended lattice systems. The dynamics of the model acts on a discrete phase space at discrete times but has nonetheless some of the characteristic properties of…

Mathematical Physics · Physics 2015-06-12 Raphael Lefevere

We apply Arnold's theory of generic smooth plane curves to Stark-Zeeman systems. This is a class of Hamiltonian dynamical systems that describes the dynamics of an electron in an external electric and magnetic field, and includes many…

Symplectic Geometry · Mathematics 2018-11-08 Kai Cieliebak , Urs Frauenfelder , Otto van Koert

We provide an illustration of a mechanism for Arnold's diffusion following a nonvariational approach and find explicit estimates for the diffusion time.

chao-dyn · Physics 2008-02-26 Giovanni Gallavotti

We prove the existence of "Arnold diffusion orbits" in cusp-generic nearly integrable a priori stable systems on ${\mathbb A}^3$. The result relies on the cusp-generic existence of chains in nearly integrable a priori stable systems, proved…

Dynamical Systems · Mathematics 2016-02-09 Jean-Pierre Marco

We provide numerical evidence of global diffusion occurring in slightly perturbed integrable Hamiltonian systems and symplectic maps. We show that even if a system is sufficiently close to be integrable, global diffusion occurs on a set…

Chaotic Dynamics · Physics 2007-05-23 Massimiliano Guzzo , Elena Lega , Claude Froeschle'

The theory of the post-Newtonian (PN) planar circular restricted three-body problem is used for numerically investigating the orbital dynamics of a test particle (e.g., a comet, asteroid, meteor or spacecraft) in the planar Sun-Jupiter…

Earth and Planetary Astrophysics · Physics 2018-03-21 Euaggelos E. Zotos , F. L. Dubeibe

This paper concerns the restricted 3-body problem. By applying topological methods we give a computer assisted proof of the existence of some classes of periodic orbits, the existence of symbolic dynamics and we give a rigorous lower…

Dynamical Systems · Mathematics 2009-11-07 Gianni Arioli

General properties of the three-body problem in a model of modified dynamics are investigated. It is shown that the three-body problem in this model shares some characters with the similar problem in Newtonian dynamics. Moreover, the planar…

Astrophysics of Galaxies · Physics 2023-04-14 Hossein Shenavar

We study a three-dimensional rapidly rotating convection model featuring tall columnar structures, in the absence of thermal diffusion. We establish the global existence and uniqueness of weak solutions, as well as the Hadamard…

Analysis of PDEs · Mathematics 2025-07-23 Chongsheng Cao , Yanqiu Guo , Edriss S. Titi

We consider the planar circular restricted three-body problem (PCRTBP), as a model for the motion of a spacecraft relative to the Earth-Moon system. We focus on the Lagrange equilibrium points $L_1$ and $L_2$. There are families of Lyapunov…

Dynamical Systems · Mathematics 2022-01-12 Marian Gidea , Rafael de la Llave , Maxwell Musser

When dealing with satellites orbiting a central body on a highly elliptical orbit, it is necessary to consider the effect of gravitational perturbations due to external bodies. Indeed, these perturbations can become very important as soon…

Earth and Planetary Astrophysics · Physics 2016-05-26 Guillaume Lion , Gilles Métris , Florent Deleflie

The goal of this paper is to obtain an approximate solution of the restricted three-body problem in the case of small perturbations in the vicinity of, but not in exact resonance. In this paper, we study the restricted threebody problem…

Earth and Planetary Astrophysics · Physics 2025-11-11 Alexey Rosaev , Eva Plavalova , Pavel Nesterov

We assume that a symplectic real-analytic map has an invariant normally hyperbolic cylinder and an associated transverse homoclinic cylinder. It is well known that such cylinder is preserved under small perturbations. We prove that for a…

Dynamical Systems · Mathematics 2014-12-02 Vassily Gelfreich , Dmitry Turaev

The problem of nonintegrability of the circular restricted three-body problem is very classical and important in the theory of dynamical systems. It was partially solved by Poincare in the nineteenth century: He showed that there exists no…

Dynamical Systems · Mathematics 2024-03-05 Kazuyuki Yagasaki

We prove, under suitable non-resonance and non-degeneracy ``twist'' conditions, a Birkhoff-Lewis type result showing the existence of infinitely many periodic solutions, with larger and larger minimal period, accumulating onto elliptic…

Dynamical Systems · Mathematics 2007-05-23 Massimiliano Berti , Luca Biasco , Enrico Valdinoci

The Hannay angle has been previously studied for a celestial circular restricted three-body system by means of an adiabatic approach. In the present work, three main results are obtained. Firstly, a formal connection between perturbation…

Astrophysics · Physics 2009-11-10 A. Spallicci , A. Morbidelli , G. Metris

Space debris mitigation guidelines represent the most effective method to preserve the circumterrestrial environment. Among them, end-of-life disposal solutions play a key role. A growing effort is devoted to exploit natural perturbations…

Dynamical Systems · Mathematics 2024-03-05 Elisa Maria Alessi , Inmaculada Baldomá , Mar Giralt , Marcel Guardia

The restricted three-body problem describes the motion of a massless particle under the influence of two primaries of masses $1-\mu$ and $\mu$ that circle each other with period equal to $2\pi$. For small $\mu$, a resonant periodic motion…

Dynamical Systems · Mathematics 2014-08-28 D. Viswanath