Universal asymptotic solution of the Fokker-Planck equation with time-dependent periodic potentials

TL;DR

This paper derives a universal asymptotic solution for the Fokker-Planck equation with time-dependent periodic potentials, revealing a common form involving a Boltzmann weight and Gaussian envelope, applicable to various complex systems.

Contribution

It introduces a universal asymptotic form for the probability distribution in time-dependent periodic potentials and provides a method to determine the Boltzmann weight for diverse potentials.

Findings

The asymptotic solution has a universal form involving Boltzmann weight and Gaussian envelope.

The Boltzmann weight can be determined by solving a partial differential equation.

Numerical and analytical methods confirm the validity of the solution.

Abstract

Brownian motion, as one of the most fundamental concepts in statistical physics, has everlasting interests in interdisciplinary fields in the past century. Although this motion with static potentials have been widely explored, its physics in time-dependent periodic potentials are far less well understood. Here we generalize this motion to the realm of time-dependent periodic potentials, showing that the asymptotic solution of the probability distribution function (PDF) can have a universal form, that is, a Boltzmann weight multiplied by a Gaussian envelope function. We derive a partial equation for this Boltzmann weight and demonstrate that many different potentials can give the same Boltzmann weight. We first present an exact solvable model to illustrate the validity of our solution. For the periodic potential with a time-dependent tilt potential, we can determine the Boltzmann weight by numerical solving the partial equation. These results are confirmed by solving the Langevin equation numerically. With this idea, we can determine the asymptotic solution of the Fokker-Planck equation, in which the entropy satisfies the thermodynamic law. Our results can have wide applications, including quasi-periodic potentials, two-dimensional potentials and even with models with inertia, which should greatly broaden our perspective of Brownian motion.