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On energy conservation in extended magnetohydrodynamics

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arxiv 1406.2745 v1 pith:WCMEN726 submitted 2014-06-11 physics.plasm-ph astro-ph.SRphysics.space-ph

Keiji Kimura , P. J. Morrison This is my paper · ORCID
classification physics.plasm-phastro-ph.SRphysics.space-ph
keywords energyconservationextendedmodelsneglectedcommonlyconserveelectron
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A systematic study of energy conservation for extended magnetohydrodynamic (MHD) models that include Hall terms and electron inertia is performed. It is observed that commonly used models do not conserve energy in the ideal limit, i.e., when viscosity and resistivity are neglected. In particular, a term in the momentum equation that is often neglected is seen to be needed for conservation of energy.

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Cited by 1 Pith paper

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  1. Radiative Back-Reaction on Charged Particle Motion in the Dipole Magnetosphere of Neutron Stars

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    Radiative back-reaction makes charged particles under an attractive Lorentz force fall onto a magnetized neutron star, while under a repulsive force they either widen their orbits or fall, depending on the starting latitude.

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