Classical Electrodynamics · Problem 5.20

Maxwell Equations, Macroscopic Electromagnetism, Conservation Laws — John David Jackson

Physics — E&M · magnetized-body-force

Problem

(a) Starting from the force equation (5.12) and the fact that a magnetization M\mathbf{M} inside a volume VV bounded by a surface SS is equivalent to a volume current density JM=(∇×M)\mathbf{J}_M = (\nabla \times \mathbf{M}) and a surface current density (M×n)(\mathbf{M} \times \mathbf{n}), show that in the absence of macroscopic conduction currents the total magnetic force on the body can be written F=−∫V(∇⋅M)Be d3x+∫S(M⋅n)Be da\mathbf{F} = -\int_V (\nabla \cdot \mathbf{M})\mathbf{B}_e\, d^3x + \int_S (\mathbf{M} \cdot \mathbf{n})\mathbf{B}_e\, da where Be\mathbf{B}_e is the applied magnetic induction (not including that of the body in question). The force is now expressed in terms of the effective charge densities ρM\rho_M and σM\sigma_M. If the distribution of magnetization is not discontinuous, the surface can be at infinity and the force given by just the volume integral. (b) A sphere of radius RR with uniform magnetization has its center at the origin of coordinates and its direction of magnetization making spherical angles θ0\theta_0, ϕ0\phi_0. If the external magnetic field is the same as in Problem 5.11, use the expression of part a to evaluate the components of the force acting on the sphere.

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