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Electrostatics and Magnetostatics

Maxwell's equations describe electrodynamics as:

D=ρ,B=0,×E=Bt,×H=J+Dt.

Here, E and H are the electric and magnetic field intensities, D and B are the electric and magnetic flux densities, and ρ and J are the electric charge and current densities.

Electrostatics

For electrostatic problems, Maxwell's equations simplify to this form:

D=(εE)=ρ,×E=0,

where ε is the electrical permittivity of the material.

Because the electric field E is the gradient of the electric potential V, E=V., the first equation yields this PDE:

(εV)=ρ.

For electrostatic problems, Dirichlet boundary conditions specify the electric potential V on the boundary.

Magnetostatics

For magnetostatic problems, Maxwell's equations simplify to this form:

B=0,×H=J+(εE)t=J.

Because B=0, there exists a magnetic vector potential A, such that B=×A. For non-ferromagnetic materials, B = μH, where µ is the magnetic permeability of the material. Therefore,

H=μ1×A,×(μ1×A)=J.

Using the identity

×(×A)=(A)2A

and the Coulomb gauge ·A=0, simplify the equation for A in terms of J to this PDE:

2A=A=μJ.

For magnetostatic problems, Dirichlet boundary conditions specify the magnetic potential A on the boundary.

Magnetostatics with Permanent Magnets

In the case of a permanent magnet, the constitutive relation between B and H includes the magnetization M:

B=μH+μ0M.

Here, μ=μ0μr, where μr is the relative magnetic permeability of the material, and μ0 is the vacuum permeability.

Because B=0, there exists a magnetic vector potential A, such that B=×A. Therefore,

H =1μ0μrB1μrM,×H=×(1μ0μr×A1μrM)=J.

The equation for A in terms of the current density J and magnetization M is

×(1μrμ0×A)=J+×(1μrM).