English

Extended space and time correlations in strongly magnetized plasmas

Plasma Physics 2021-04-21 v1

Abstract

Molecular dynamics simulations are used to show that strong magnetization significantly increases the space and time scales associated with interparticle correlations. The physical mechanism responsible is a channeling effect whereby particles are confined to move along narrow cylinders with a width characterized by the gyroradius and a length characterized by the collision mean free path. The predominant interaction is 180180^\circ collisions at the ends of the collision cylinders, resulting in a long-range correlation parallel to the magnetic field. Its influence is demonstrated via the dependence of the velocity autocorrelation functions and self-diffusion coefficients on the domain size and run time in simulations of the one-component plasma. A very large number of particles, and therefore domain size, must be used to resolve the long-range correlations, suggesting that the number of charged particles in the collection must increase in order to constitute a plasma. Correspondingly, this effect significantly delays the time it takes to reach a diffusive regime, in which the mean square displacement of particles increases linearly in time. This result presents challenges for connecting measurements in non-neutral and ultracold neutral plasma experiments, as well as molecular dynamics simulations, with fluid transport properties due to their finite size.

Keywords

Cite

@article{arxiv.2102.04289,
  title  = {Extended space and time correlations in strongly magnetized plasmas},
  author = {Keith R. Vidal and Scott D. Baalrud},
  journal= {arXiv preprint arXiv:2102.04289},
  year   = {2021}
}

Comments

14 pages, 11 figures

R2 v1 2026-06-23T22:56:43.069Z