Explicit sufficient stability criteria and a Hall MHD energy principle for XMHD equilibria with flow, derived from energy-Casimir, dynamically accessible, and Lagrangian methods.
and then try to eliminate the explicit appearance of δBφ and δv⊥ into δ2HC by other means
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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria
Explicit sufficient stability criteria and a Hall MHD energy principle for XMHD equilibria with flow, derived from energy-Casimir, dynamically accessible, and Lagrangian methods.