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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 In electromagnetism, current density is the amount of charge per unit time that flows through a unit area of a chosen cross section. The current density vector is defined as a vector whose magnitude is the electric current per cross-sectional a ...
, 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

The scalar potential is a useful quantity in describing the magnetic field, especially for
permanent magnet A magnet is a material or object that produces a magnetic field. This magnetic field is invisible but is responsible for the most notable property of a magnet: a force that pulls on other ferromagnetic materials, such as iron, steel, nic ...
s. Where there is no free current, :\nabla\times\mathbf = 0, so if this holds in
simply connected domain In topology, a topological space is called simply connected (or 1-connected, or 1-simply connected) if it is path-connected and every path between two points can be continuously transformed (intuitively for embedded spaces, staying within the sp ...
we can define a ''magnetic scalar potential'', ''ψ'', as :\mathbf = -\nabla\psi. The dimensions of ''ψ'' in SI base units are \mathrm. Using the definition of H: :\nabla\cdot\mathbf = \mu_\nabla\cdot\left(\mathbf + \mathbf\right) = 0, it follows that :\nabla^2 \psi = -\nabla\cdot\mathbf = \nabla\cdot\mathbf. Here, acts as the source for magnetic field, much like acts as the source for electric field. So analogously to bound electric charge, the quantity :\rho_m = -\nabla\cdot\mathbf is called the ''bound magnetic charge'' density. Magnetic charges \textstyle 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 ''qm'' in a magnetic scalar potential is :Q = \mu_0\,q_m\psi, and of a magnetic charge density distribution ''ρm'' in space :Q = \mu_0\int \rho_m\psi\,\mathrmV, where ''µ0'' is the vacuum permeability. This is analog to the energy Q=qV_E of an electric charge ''q'' in an electric potential V_E. If there is free current, one may subtract the contributions of free current per Biot–Savart law from total magnetic field and solve the remainder with the scalar potential method.


See also

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Magnetic vector potential In classical electromagnetism, magnetic vector potential (often called A) is the vector quantity defined so that its curl is equal to the magnetic field: \nabla \times \mathbf = \mathbf. Together with the electric potential ''φ'', the magnetic ...


Notes


References

* * *{{Cite book , isbn = 1-4020-2699-4 , last = Vanderlinde , first = Jack , title = Classical Electromagnetic Theory , year = 2005 , doi = 10.1007/1-4020-2700-1 , bibcode = 2005cet..book.....V , url = http://cds.cern.ch/record/1250088 Potentials Magnetism