Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method

We present a new method for evolving the equations of magnetohydrodynamics (both Newtonian and relativistic) that is capable of maintaining a divergence-free magnetic field (∇⋅B=0) on adaptively refined, conformally moving meshes. The method relies on evolving the magnetic vector potential and then...

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Main Authors: P. Chris Fragile, Daniel Nemergut, Payden L. Shaw, Peter Anninos
Format: Article
Language:English
Published: Elsevier 2019-03-01
Series:Journal of Computational Physics: X
Online Access:http://www.sciencedirect.com/science/article/pii/S2590055219300368
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spelling doaj-d92887276f4f46529037a28d8738c8942020-11-25T00:21:02ZengElsevierJournal of Computational Physics: X2590-05522019-03-012Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential methodP. Chris Fragile0Daniel Nemergut1Payden L. Shaw2Peter Anninos3Department of Physics and Astronomy, College of Charleston, Charleston, SC 29424, USA; Corresponding author.Department of Physics and Astronomy, College of Charleston, Charleston, SC 29424, USADepartment of Physics and Astronomy, College of Charleston, Charleston, SC 29424, USALawrence Livermore National Laboratory, P.O. Box 808, Livermore, CA 94550, USAWe present a new method for evolving the equations of magnetohydrodynamics (both Newtonian and relativistic) that is capable of maintaining a divergence-free magnetic field (∇⋅B=0) on adaptively refined, conformally moving meshes. The method relies on evolving the magnetic vector potential and then using it to reconstruct the magnetic fields. The advantage of this approach is that the vector potential is not subject to a constraint equation in the same way the magnetic field is, and so can be refined and moved in a straightforward way. We test this new method against a wide array of problems from simple Alfvén waves on a uniform grid to general relativistic MHD simulations of black hole accretion on a nested, spherical-polar grid. We find that the code produces accurate results and in all cases maintains a divergence-free magnetic field to machine precision. Keywords: Magnetohydrodynamics, Adaptive mesh refinement, Divergence constraint, Astrophysics, Magnetic fieldshttp://www.sciencedirect.com/science/article/pii/S2590055219300368
collection DOAJ
language English
format Article
sources DOAJ
author P. Chris Fragile
Daniel Nemergut
Payden L. Shaw
Peter Anninos
spellingShingle P. Chris Fragile
Daniel Nemergut
Payden L. Shaw
Peter Anninos
Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
Journal of Computational Physics: X
author_facet P. Chris Fragile
Daniel Nemergut
Payden L. Shaw
Peter Anninos
author_sort P. Chris Fragile
title Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
title_short Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
title_full Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
title_fullStr Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
title_full_unstemmed Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
title_sort divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method
publisher Elsevier
series Journal of Computational Physics: X
issn 2590-0552
publishDate 2019-03-01
description We present a new method for evolving the equations of magnetohydrodynamics (both Newtonian and relativistic) that is capable of maintaining a divergence-free magnetic field (∇⋅B=0) on adaptively refined, conformally moving meshes. The method relies on evolving the magnetic vector potential and then using it to reconstruct the magnetic fields. The advantage of this approach is that the vector potential is not subject to a constraint equation in the same way the magnetic field is, and so can be refined and moved in a straightforward way. We test this new method against a wide array of problems from simple Alfvén waves on a uniform grid to general relativistic MHD simulations of black hole accretion on a nested, spherical-polar grid. We find that the code produces accurate results and in all cases maintains a divergence-free magnetic field to machine precision. Keywords: Magnetohydrodynamics, Adaptive mesh refinement, Divergence constraint, Astrophysics, Magnetic fields
url http://www.sciencedirect.com/science/article/pii/S2590055219300368
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AT peteranninos divergencefreemagnetohydrodynamicsonconformallymovingadaptivemeshesusingavectorpotentialmethod
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