Relative permeability
In physics, in particular in magnetostatics, the relative permeability is an intrinsic property of a magnetic material. It is usually denoted by μr. For simple magnetic materials, using SI units, μr is related to the proportionality constant between the magnetic flux density B and the magnetic field H, namely B = μr μ0 H, where μ0 is the magnetic constant. The relative permeability describes the ease by which a magnetic medium may be magnetized.
A related quantity is the magnetic susceptibility, denoted by χm, related to the magnetic permeability in SI units by:[1]
The force exerted between infinitesimal current elements from two loops carrying currents Ii and Ij and immersed in a magnetic medium with relative permeability μr is changed by a factor μr. The infinitesimal current elements have vector components Iidℓi and Ijdℓj where the incremental lengths are directed along the wire at the location of the element, and pointing in the direction of the current. Grassmann's law for the force between current elements is:
as is readily derived from the Biot-Savart law, and is consistent with space-time symmetry. Here
ûij is a unit vector pointing along the line joining element j to element i and rij the length of this line. The force element is second order because it is a product of two infinitesimals.
Empirically it is observed that the force may increase or decreases due to the presence of the magnetic medium, hence the relative permittivity μr may be greater than or less than 1. For simple media, if μr < 1, the medium is termed diamagnetic; if > 1 paramagnetic. Only classical vacuum has μr = 1 (exact). A typical diamagnetic susceptibility is about −10−5, while a typical paramagnetic susceptibility is about 10−4. It should be noted that the use of a constant as the relative permeability of a substance is an approximation, even for quantum vacuum. A more complete representation recognizes that all media exhibit departures from this approximation, in particular, a dependence on field strength, a dependence upon the rate of variation of the field in both time and space, and a dependence upon the direction of the field. In many materials these dependencies are slight; in others, like ferromagnets, they are pronounced.
Notes
- ↑ For example see Yehuda Benzion Band. Light and matter: electromagnetism, optics, spectroscopy and lasers. John Wiley and Sons, p. 242. ISBN 0471899313.