English

On Quasilinear Perpendicular Diffusion

Astrophysics 2007-05-23 v1

Abstract

Quasilinear perpendicular diffusion of charged particles in fluctuating electromagnetic fields is the focus of this paper. A general transport parameter for perpendicular diffusion is presented being valid for an arbitrary turbulence geometry and a plasma wave dispersion relation varying arbitrarily in wavevector. The new diffusion coefficient is evaluated in detail for slab turbulence geometry for two special cases: (1) Alfv\'enic turbulence and (2) dynamical magnetic turbulence. Furthermore, perpendicular diffusion in 2D geometry is considered for a purely dynamical magnetic turbulence. The derivations and numerical calculations presented here cast serious doubts on the applicability of quasilinear theory for perpendicular diffusion. Furthermore, they emphasize that nonlinear effects play a crucial role in the context of perpendicular diffusion.

Keywords

Cite

@article{arxiv.astro-ph/0503576,
  title  = {On Quasilinear Perpendicular Diffusion},
  author = {O. Stawicki},
  journal= {arXiv preprint arXiv:astro-ph/0503576},
  year   = {2007}
}

Comments

19 pages, 2 figures