English

Non-Thermal Einstein Relations

Chaotic Dynamics 2016-08-24 v1 Statistical Mechanics

Abstract

We consider a particle moving with equation of motion x˙=f(t)\dot x=f(t), where f(t)f(t) is a random function with statistics which are independent of xx and tt, with a finite drift velocity v=fv=\langle f\rangle and in the presence of a reflecting wall. Far away from the wall, translational invariance implies that the stationary probability distribution is P(x)exp(αx)P(x)\sim \exp(\alpha x). A classical example of a problem of this type is sedimentation equilibrium, where α\alpha is determined by temperature. In this work we do not introduce a thermal reservoir and α\alpha is determined from the equation of motion. We consider a general approach to determining α\alpha which is not always in agreement with Einstein's relation between the mean velocity and the diffusion coefficient. We illustrate our results with a model inspired by the Boltzmann equation.

Keywords

Cite

@article{arxiv.1602.06059,
  title  = {Non-Thermal Einstein Relations},
  author = {Robin Guichardaz and Alain Pumir and Michael Wilkinson},
  journal= {arXiv preprint arXiv:1602.06059},
  year   = {2016}
}

Comments

5 pages, 1 figure

R2 v1 2026-06-22T12:53:34.088Z