Constraint preserving boundary conditions for the Ideal Newtonian MHD equations
arXiv:0801.2140 · doi:10.1016/j.cpc.2008.04.015
Abstract
We study and develop constraint preserving boundary conditions for the Newtonian magnetohydrodynamic equations and analyze the behavior of the numerical solution upon considering different possible options.
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- Evolutions of Magnetized and Rotating Neutron Stars
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- A divergence-cleaning scheme for cosmological SPMHD simulations
- Pulsar magnetospheres in General Relativity
- Covariant Hyperbolization of Force-free Electrodynamics
- A novel scheme for simulating the force-free equations: boundary conditions and the evolution of solutions towards stationarity
- Astrophysical jets from boosted compact objects