A Second Order Godunov Method for Multidimensional Relativistic Magnetohydrodynamics

TL;DR

This paper introduces a second-order Godunov method for multidimensional relativistic magnetohydrodynamics that improves stability and accuracy using advanced flux computation and correction techniques, with applications to jets and turbulence.

Contribution

It presents a novel, stable, and accurate second-order Godunov algorithm for RMHD that incorporates constrained transport and correction steps, enhancing simulation fidelity.

Findings

Riemann solvers with contact and rotational discontinuities increase magnetic field strength in jets.

The new method improves spectral resolution in RMHD turbulence simulations.

Corrections significantly enhance stability despite their rarity.

Abstract

We describe a new Godunov algorithm for relativistic magnetohydrodynamics (RMHD) that combines a simple, unsplit second order accurate integrator with the constrained transport (CT) method for enforcing the solenoidal constraint on the magnetic field. A variety of approximate Riemann solvers are implemented to compute the fluxes of the conserved variables. The methods are tested with a comprehensive suite of multidimensional problems. These tests have helped us develop a hierarchy of correction steps that are applied when the integration algorithm predicts unphysical states due to errors in the fluxes, or errors in the inversion between conserved and primitive variables. Although used exceedingly rarely, these corrections dramatically improve the stability of the algorithm. We present preliminary results from the application of these algorithms to two problems in RMHD: the propagation of supersonic magnetized jets, and the amplification of magnetic field by turbulence driven by the relativistic Kelvin-Helmholtz instability (KHI). Both of these applications reveal important differences between the results computed with Riemann solvers that adopt different approximations for the fluxes. For example, we show that use of Riemann solvers which include both contact and rotational discontinuities can increase the strength of the magnetic field within the cocoon by a factor of ten in simulations of RMHD jets, and can increase the spectral resolution of three-dimensional RMHD turbulence driven by the KHI by a factor of 2. This increase in accuracy far outweighs the associated increase in computational cost. Our RMHD scheme is publicly available as part of the Athena code.