A High-Order Relativistic Two-Fluid Electrodynamic Scheme with Consistent Reconstruction of Electromagnetic Fields and a Multidimensional Riemann Solver for Electromagnetism

TL;DR

This paper introduces a high-order relativistic two-fluid electrodynamic scheme that accurately models plasma-electromagnetic interactions in astrophysics, ensuring divergence-free magnetic fields and consistent electric field reconstruction, with strong coupling and high accuracy.

Contribution

The paper presents three innovations: divergence-free magnetic field reconstruction, a multidimensional upwinded strategy for electromagnetic field updates, and an efficient high-order coupling scheme for fluid and electromagnetic solvers.

Findings

Method achieves high accuracy in MHD and electromagnetic wave limits.

Successfully models relativistic plasma interactions in astrophysical scenarios.

Demonstrates robustness with challenging high-energy astrophysics test problems.

Abstract

In various astrophysics settings it is common to have a two-fluid relativistic plasma that interacts with the electromagnetic field. While it is common to ignore the displacement current in the ideal, classical magnetohydrodynamic limit, when the flows become relativistic this approximation is less than absolutely well-justified. In such a situation, it is more natural to consider a positively charged fluid made up of positrons or protons interacting with a negatively charged fluid made up of electrons. The two fluids interact collectively with the full set of Maxwell's equations. As a result, a solution strategy for that coupled system of equations is sought and found here. Our strategy extends to higher orders, providing increasing accuracy. Three important innovations are reported here. In our first innovation, the magnetic field within each zone is reconstructed in a divergence-free fashion while the electric field within each zone is reconstructed in a form that is consistent with Gauss' law. In our second innovation, a multidimensionally upwinded strategy is presented which ensures that the magnetic field can be updated via a discrete interpretation of Faraday's law and the electric field can be updated via a discrete interpretation of the generalized Ampere's law. Our third innovation consists of an efficient design for several popular IMEX schemes so that they provide strong coupling between the finite-volume-based fluid solver and the electromagnetic fields at high order. Several accuracy analyses are presented showing that our method meets its design accuracy in the MHD limit as well as in the limit of electromagnetic wave propagation. Several stringent test problems are also presented. We also present a relativistic version of the GEM problem, which shows that our algorithm can successfully adapt to challenging problems in high energy astrophysics.