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electrostatics and magnetostatics

maxwell's equations describe electrodynamics as:

∇⋅d=ρ,∇⋅b=0,∇×e=−∂b∂t,∇×h=j ∂d∂t.

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=∇⋅(ε e)=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:

−∇⋅(ε ∇v)=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=μ−1∇×a,∇×(μ−1∇×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 =1μ0μrb−1μrm,∇×h=∇×(1μ0μr×a−1μrm)=j.

the equation for a in terms of the current density j and magnetization m is

∇×(1μrμ0∇×a)=j ∇×(1μrm).

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