English

System Size Dependence of Collisionless Reconnection Rate

Plasma Physics 2026-04-22 v1 Solar and Stellar Astrophysics Space Physics

Abstract

It is a widely accepted paradigm that collisionless magnetic reconnection proceeds at a universal fast rate of 0.1\sim0.1 when normalized to a properly defined reconnecting magnetic field and Alfv\'en speed, effectively independent of the macroscopic system size. This conclusion, derived primarily from kinetic simulations of classical Harris current sheets with kinetic-scale thickness, stands in contrast to results from forced reconnection and island coalescence, where the rate significantly depends on the system size. Here, we reconcile this disparity by performing a rigorous scaling study using both particle-in-cell and Hall magnetohydrodynamic simulations. We demonstrate that when the global magnetic configuration is self-consistently preserved by scaling the initial current sheet thickness proportionally with the system size, the ``universal'' fast rate disappears. Instead, the reconnection rate decreases as the system size increases. These results indicate that dependence on macroscopic scales is not peculiar to specific geometries but is a fundamental property of collisionless reconnection, effectively unifying the Harris sheet with other configurations exhibiting size-dependence.

Keywords

Cite

@article{arxiv.2604.18787,
  title  = {System Size Dependence of Collisionless Reconnection Rate},
  author = {Yi-Min Huang and Naoki Bessho and Li-Jen Chen and Judith T. Karpen and Amitava Bhattacharjee},
  journal= {arXiv preprint arXiv:2604.18787},
  year   = {2026}
}