Hamiltonian Dynamics and Diffusion Mechanisms
Summary
Hamiltonian dynamics form the mathematical framework for systems in which energy is conserved and motion evolves on a symplectic phase space. In integrable cases, the motion is confined to invariant tori on which the actions remain constant. Small perturbations of such integrable systems give rise to a rich tapestry of phenomena: most invariant tori survive according to Kolmogorov–Arnold–Moser (KAM) theory, but gaps appear around resonances where frequencies satisfy integer relations. Through these gaps, slow drift of the action variables can occur, a process known as Arnold diffusion. This mechanism enables trajectories to wander across large regions of phase space on very long timescales, with profound implications for the stability of celestial systems, the confinement of charged particles in magnetic fields and transport in condensed-matter models. The interplay between local resonances, global scattering maps and variational structures underpins modern understanding of diffusion mechanisms in nearly integrable Hamiltonian systems, while advances in geometric and analytic techniques continue to clarify the conditions under which energy exchange and instability arise.
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Hamiltonian Dynamics and Diffusion Mechanisms publication trend
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Technical terms
Hamiltonian system: A dynamical system governed by a function (the Hamiltonian) representing total energy, whose flow preserves a symplectic form.
Invariant torus: A compact, toroidal subset of phase space on which motion is quasi-periodic and action variables remain constant.
KAM theorem: A result assuring the persistence of many non-resonant invariant tori under small, smooth perturbations of an integrable Hamiltonian.
Arnold diffusion: A slow drift mechanism allowing trajectories to traverse gaps between invariant tori via resonance channels, leading to large-scale instability.
Resonance: A condition in which two or more natural frequencies of a system satisfy an integer relation, creating opportunities for enhanced energy exchange.
References
- Why are inner planets not inclined?. Publications mathématiques de l'IHÉS (2024).
- The dynamics of pseudographs in convex Hamiltonian systems. Journal of the American Mathematical Society (2008).
- Analytic genericity of diffusing orbits in a priori unstable Hamiltonian systems. Nonlinearity (2022).
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