English

A Reduced-Speed-of-Light Formulation of the Magnetohydrodynamic-Particle-in-Cell Method

High Energy Astrophysical Phenomena 2022-09-20 v2 Astrophysics of Galaxies Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics Plasma Physics

Abstract

A reduced-speed-of-light (RSOL) approximation is a useful technique for magnetohydrodynamic (MHD)-particle-in-cell (PIC) simulations. With a RSOL, some "in-code" speed-of-light c~\tilde{c} is set to much lower values than the true cc, allowing simulations to take larger timesteps (which are restricted by the Courant condition given the large CR speeds). However, due to the absence of a well-formulated RSOL implementation from the literature, with naive substitution of the true cc with a RSOL, the CR properties in MHD-PIC simulations (e.g.\ CR energy or momentum density, gyro radius) vary artificially with respect to each other and with respect to the converged (c~c\tilde{c} \rightarrow c) solutions with different choices of a RSOL. Here, we derive a new formulation of the MHD-PIC equations with a RSOL, and show that (1) it guarantees all steady-state properties of the CR distribution function and background plasma/MHD quantities are {\em independent} of the RSOL c~\tilde{c} even for c~c\tilde{c} \ll c, (2) ensures that the simulation can {\em simultaneously} represent the real physical values of CR number, mass, momentum, and energy density, (3) retains the correct physical meaning of various terms like the electric field, and (4) ensures the numerical timestep for CRs can always be safely increased by a factor c/c~\sim c/\tilde{c}. This new RSOL formulation should enable greater self-consistency and reduced CPU cost in simulations of CR-MHD interactions.

Keywords

Cite

@article{arxiv.2111.14704,
  title  = {A Reduced-Speed-of-Light Formulation of the Magnetohydrodynamic-Particle-in-Cell Method},
  author = {Suoqing Ji and Philip F. Hopkins},
  journal= {arXiv preprint arXiv:2111.14704},
  year   = {2022}
}

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published by MNRAS