Magnetohydrodynamic-guiding-center-particle-in-cell Method for Multiscale Plasma Kinetic Simulations
Zitao Hu, Xue-Ning Bai, Xiaochen Sun
TL;DR
The work develops the MHD-gPIC framework that couples magnetohydrodynamic fluid dynamics with guiding-center particles to simulate multiscale plasma kinetics while mitigating gyro-scale constraints. By deriving Galilean-invariant particle equations, incorporating perpendicular particle pressure into the fluid pressure, and carefully formulating particle backreaction, the method enables large-scale MHD dynamics with non-thermal particle feedback. Validation across trajectory tests, wave-particle interactions, noise-reduction tests, and magnetic reconnection scenarios demonstrates accurate particle transport, energy transfer, and acceleration predominantly via Fermi mechanisms in plasmoid-dominated reconnection, with ions strongly influencing the MHD environment. This approach offers a robust, scalable path toward realistic, multi-scale plasma simulations on the Athena++ platform, with implications for cosmic-ray transport, solar flares, and related astrophysical processes.
Abstract
We present the formulation, algorithm and numerical tests of the magnetohydrodynamic-particle-in-cell (MHD-PIC) method with particles treated under the guiding center approximation, which we term the MHD-gPIC method, and it is implemented in the Athena++ MHD code. The new MHD-gPIC model consists of thermal (cold) fluid and high-energy particles whose dynamics are integrated through guiding center equations including drift motion, with carefully evaluated source terms as particle backreaction. The code is validated with a series of tests, and it is expected to be primarily applicable to study particle acceleration and transport in systems where gyro-resonance is considered insignificant. We also present preliminary studies of particle acceleration during non-relativistic magnetic reconnection.
