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Momentum Equation

\[\rho \frac{D\mathbf{U}}{Dt} = -\nabla p + \mathbf{J}\times\mathbf{B} + \mu \nabla^2\mathbf{U}\]

Source lecture(s): pc368_lec05_mhd

Physical Meaning

The momentum equation balances the rate of change of fluid momentum with forces: pressure gradients, electromagnetic Lorentz force, and viscous stress.

Variable Definitions

Symbol Definition SI Units
\(\rho\) Fluid mass density kg m\(^{-3}\)
\(\mathbf{U}\) Fluid velocity m s\(^{-1}\)
\(p\) Fluid pressure Pa
\(\mathbf{J}\) Current density A m\(^{-2}\)
\(\mathbf{B}\) Magnetic field T
\(\mu\) Dynamic viscosity Pa·s

Assumptions

  • Single MHD fluid.
  • Scalar, isotropic pressure.
  • Ohmic dissipation via \(\mathbf{E} + \mathbf{U}\times\mathbf{B} = \eta\mathbf{J}\).

Derivation

Take the first velocity moment of the Boltzmann equation with collision operator that conserves momentum. The Lorentz force appears as \(\int (q/m)\mathbf{E} f d^3v + \int (q/m)\mathbf{v}\times\mathbf{B} f d^3v = \rho_c \mathbf{E} + \mathbf{J}\times\mathbf{B}\).

Applications

  • Z-pinch equilibrium: \(dp/dr = B_\theta^2/\mu_0\).
  • Tokamak force balance: Toroidal/poloidal field stresses.
  • Alfvén waves: Inertial term \(\rho \partial \mathbf{U}/\partial t\) vs. magnetic tension.

Connections to Other Equations

  • MHD: Part of the MHD system.
  • Alfvén Speed: Derived from momentum + induction.