4.7 Article

Axisymmetric smoothed particle magnetohydrodynamics

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 518, Issue 3, Pages 4115-4131

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac3328

Keywords

hydrodynamics; MHD; methods: numerical

Funding

  1. Ministerio de Asuntos Economicos y Transformacion Digital (MINECO) Spanish project [PID2020-117252GB-100]
  2. Swiss Platform for Advanced Scientific Computing (PASC) project SPH-EXA2: Optimizing Smooth Particle Hydrodynamics for Exascale Computing
  3. National Infrastructure for High Performance Computing and Data Storage in Norway, UNINETT Sigma2 [NN9477K]
  4. Research Council of Norway through NFR Young Research Talents Grant [276043]
  5. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [101002352]

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This study proposes a novel axisymmetric MHD hydrodynamic code to tackle the gap in the scientific literature, and demonstrates that it can produce similar results to standard 3D-SPMHD codes with less computational load.
Many astrophysical and terrestrial scenarios involving magnetic fields can be approached in axial geometry. Although the smoothed particle hydrodynamics (SPH) technique has been successfully extended to magnetohydrodynamics (MHD), a well-verified, axisymmetric MHD scheme based on such technique does not exist yet. In this work, we fill that gap in the scientific literature and propose and check a novel axisymmetric MHD hydrodynamic code, that can be applied to physical problems which display the adequate geometry. We show that the hydrodynamic code built following these axisymmetric hypothesis is able to produce similar results than standard 3D-SPMHD codes with equivalent resolution but with much lesser computational load.

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