Bridging hybrid- and full-kinetic models with Landau-fluid electrons: I. 2D magnetic reconnection

TL;DR

This study introduces a Landau-fluid electron model within hybrid-kinetic simulations to accurately replicate 2D magnetic reconnection physics, including electron micro-physics and pressure anisotropy effects, with computational efficiency.

Contribution

The paper presents a new hybrid-kinetic plasma model with a Landau-fluid electron response that closely reproduces full-kinetic magnetic reconnection dynamics, especially during the non-linear stage.

Findings

HVLF model effectively reproduces main features of 2D MR

Captures electron micro-physics and pressure anisotropy evolution

Fails to reproduce electron-cyclotron instability

Abstract

Magnetic reconnection (MR) plays a fundamental role in plasma dynamics under many different conditions, from space and astrophysical environments to laboratory devices. High-resolution in-situ measurements from space missions allow to study naturally occurring MR processes in great detail. Alongside direct measurements, numerical simulations play a key role in investigating the fundamental physics underlying MR. The choice of an adequate plasma model to be employed in numerical simulations, while also compromising with their computational cost, is crucial to efficiently address the problem. We consider a new plasma model that includes a refined electron response within the hybrid-kinetic framework (kinetic ions, fluid electrons). The extent to which this new model can reproduce a full-kinetic description of 2D MR, with particular focus on its robustness during the non-linear stage, is evaluated. We perform 2D simulations of MR with moderate guide field by means of three different plasma models: a hybrid-Vlasov-Maxwell model with isotropic, isothermal electrons, a hybrid-Vlasov-Landau-fluid (HVLF) model where an anisotropic electron fluid is equipped with a Landau-fluid closure, and a full-kinetic one. When compared to the full-kinetic case, the HVLF model effectively reproduces the main features of MR, as well as several aspects of the associated electron micro-physics and its feedback onto proton dynamics. This includes the global evolution of MR and the local physics occurring within the so-called electron-diffusion region, as well as the evolution of species pressure anisotropy. In particular, anisotropy driven instabilities (such as firehose, mirror, and cyclotron instabilities) play a relevant role in regulating electrons anisotropy during the non-linear stage of MR. As expected, the HVLF model captures all these features, except for the electron-cyclotron instability.