Magnetic scalar potential

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Magnetic scalar potential, ψ, is a quantity in classical electromagnetism analogous to electric potential. It is used to specify the magnetic H-field in cases when there are no free currents, in a manner analogous to using the electric potential to determine the electric field in electrostatics. One important use of ψ is to determine the magnetic field due to permanent magnets when their magnetization is known. The potential is valid in any region with zero current density, thus if currents are confined to wires or surfaces, piecemeal solutions can be stitched together to provide a description of the magnetic field at all points in space.

Magnetic scalar potential[]

Magnetic scalar potential of flat cylinder magnets encoded as color from positive (fuchsia) through zero (yellow) to negative (aqua).

The scalar potential is a useful quantity in describing the magnetic field, especially for permanent magnets.

In a simply connected domain where there is no free current,

${\displaystyle \nabla \times \mathbf {H} =0,}$

hence we can define a magnetic scalar potential, ψ, as^[1]

${\displaystyle \mathbf {H} =-\nabla \psi .}$

The dimensions of ψ in SI base units are ${\displaystyle \mathrm {A} }$.

Using the definition of H:

${\displaystyle \nabla \cdot \mathbf {B} =\mu _{0}\nabla \cdot \left(\mathbf {H} +\mathbf {M} \right)=0,}$

it follows that

${\displaystyle \nabla ^{2}\psi =-\nabla \cdot \mathbf {H} =\nabla \cdot \mathbf {M} .}$

Here, ∇ ⋅ M acts as the source for magnetic field, much like ∇ ⋅ P acts as the source for electric field. So analogously to bound electric charge, the quantity

${\displaystyle \rho _{m}=-\nabla \cdot \mathbf {M} }$

is called the bound magnetic charge density. Magnetic charges ${\displaystyle \textstyle {q_{m}=\int \rho _{m}\,\mathrm {d} V}}$ never occur isolated as magnetic monopoles, but only within dipoles and in magnets with a total magnetic charge sum of zero. The energy of a localized magnetic charge q_m in a magnetic scalar potential is

${\displaystyle Q=\mu _{0}\,q_{m}\psi }$,

and of a magnetic charge density distribution ρ_m in space

${\displaystyle Q=\mu _{0}\int \rho _{m}\psi \,\mathrm {d} V}$,

where µ₀ is the vacuum permeability. This is analog to the energy ${\displaystyle Q=qV_{E}}$ of an electric charge q in an electric potential ${\displaystyle V_{E}}$.

If there is free current, one may subtract the contribution of free current per Biot–Savart law from total magnetic field and solve the remainder with the scalar potential method.

See also[]

• Magnetic vector potential

Notes[]

References[]

• Duffin, W.J. (1980). Electricity and Magnetism, Fourth Edition. McGraw-Hill. ISBN 007084111X.

• Jackson, John David (1999), Classical Electrodynamics (3rd ed.), John Wiley & Sons, ISBN 0-471-30932-X

• Vanderlinde, Jack (2005). Classical Electromagnetic Theory. Bibcode:2005cet..book.....V. doi:10.1007/1-4020-2700-1. ISBN 1-4020-2699-4.