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Updated: May 2, 2026

The Diffusion of Passive Tracers in Laminar Shear Flow
Published on: May 1, 2018
Stochastic approach to diffusion inside the chaotic layer of a resonance
Martín F Mestre1, Armando Bazzani2, Pablo M Cincotta1
1Grupo de Caos en Sistemas Hamiltonianos, Facultad de Ciencias Astronómicas y Geofísicas, UNLP, Argentina and Instituto de Astrofísica de La Plata (CCT La Plata - CONICET, UNLP), Argentina.
We modeled chaotic diffusion in a four-dimensional (4D) symplectic map using a theorem for stochastically perturbed systems. Our findings on diffusion coefficients offer insights into slow diffusion in celestial mechanics and accelerator physics.
Area of Science:
- Physics
- Applied Mathematics
- Dynamical Systems
Background:
- Chaotic diffusion is a key phenomenon in Hamiltonian systems.
- Understanding diffusion in high-dimensional systems is crucial for fields like celestial mechanics and accelerator physics.
Purpose of the Study:
- To model and analyze chaotic diffusion in a 4D symplectic map.
- To develop a seminumerical method for calculating diffusion coefficients.
- To investigate the applicability of Fokker-Planck equations in describing diffusion processes.
Main Methods:
- Utilizing a theorem for stochastically perturbed integrable Hamiltonian systems.
- Explicitly defining a map coupling a free rotator (FR) and a standard map (SM).
- Calculating the diffusion coefficient for the action I of the FR.
Main Results:
- A seminumerical method was developed to compute the diffusion coefficient.
- The probability density function for action I was well-interpolated by a Fokker-Planck (FP) equation in the case of a thick chaotic layer.
- A nonconstant time shift was observed with respect to the FP solution in the case of a thin chaotic layer, suggesting anomalous diffusion.
Conclusions:
- The study provides a method for calculating diffusion coefficients in 4D symplectic maps.
- Results indicate that Fokker-Planck equations can describe chaotic diffusion, but anomalous time scales may arise.
- The findings contribute to understanding slow diffusion in celestial mechanics and accelerator physics.
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