Non-ideal magnetohydrodynamics on a moving mesh I: ohmic and ambipolar diffusion

• Published in: Monthly notices of the Royal Astronomical Society 2024-01, Vol.527 (1), p.1563-1579
• Main Authors: Zier, Oliver, Springel, Volker, Mayer, Alexander C
• Format: Article
• Language: English
• Subjects: Ambipolar diffusion; Damping; Diffusion rate; Electromagnetism; Hall effect; Interface stability; Magnetic diffusion; Magnetic fields; Magnetohydrodynamic waves; Magnetohydrodynamics; Protostars; Spatial resolution
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stad3200

ABSTRACT Especially in cold and high-density regions, the assumptions of ideal magnetohydrodynamics (MHD) can break down, making first order non-ideal terms such as ohmic and ambipolar diffusion as well as the Hall effect important. In this study, we present a new numerical scheme for the first two resistive terms, which we implement in the moving-mesh code arepo using the single-fluid approximation combined with a new gradient estimation technique based on a least-squares fit per interface. Through various test calculations including the diffusion of a magnetic peak, the structure of a magnetic C-shock, and the damping of an Alfvén wave, we show that we can achieve an accuracy comparable to the state-of-the-art code athena++ . We apply the scheme to the linear growth of the magnetorotational instability and find good agreement with the analytical growth rates. By simulating the collapse of a magnetized cloud with constant magnetic diffusion, we show that the new scheme is stable even for large contrasts in the spatial resolution. Thanks to the Lagrangian nature of the moving mesh method the new scheme is thus well suited for intended future applications where a high resolution in the dense cores of collapsing protostellar clouds needs to be achieved. In a forthcoming work, we will extend the scheme to include the Hall effect.