# Permeability (electromagnetism)

In electromagnetism, permeability is the measure of the ability of a material to support the formation of a magnetic field within itself. In other words, it is the degree of magnetization that a material obtains in response to an applied magnetic field. Magnetic permeability is typically represented by the Greek letter μ. The term was coined in September 1885 by Oliver Heaviside. The reciprocal of magnetic permeability is magnetic reluctivity.

In SI units, permeability is measured in henries per meter (H·m−1), or newtons per ampere squared (N·A−2). The permeability constant (μ0), also known as the magnetic constant or the permeability of free space, is a measure of the amount of resistance encountered when forming a magnetic field in a classical vacuum. The magnetic constant has the exact (defined) value µ0 = 4π×10−7 H·m−1≈ 1.2566370614…×10−6 H·m−1 or N·A−2).

A closely related property of materials is magnetic susceptibility, which is a measure of the magnetization of a material in addition to the magnetization of the space occupied by the material.

## Explanation

In electromagnetism, the auxiliary magnetic field H represents how a magnetic field B influences the organization of magnetic dipoles in a given medium, including dipole migration and magnetic dipole reorientation. Its relation to permeability is

$\mathbf {B} =\mu \mathbf {H} ,$ where the permeability, μ, is a scalar if the medium is isotropic or a second rank tensor for an anisotropic medium.

In general, permeability is not a constant, as it can vary with the position in the medium, the frequency of the field applied, humidity, temperature, and other parameters. In a nonlinear medium, the permeability can depend on the strength of the magnetic field. Permeability as a function of frequency can take on real or complex values. In ferromagnetic materials, the relationship between B and H exhibits both non-linearity and hysteresis: B is not a single-valued function of H, but depends also on the history of the material. For these materials it is sometimes useful to consider the incremental permeability defined as

$\Delta \mathbf {B} =\mu _{\Delta }\Delta \mathbf {H} .$ This definition is useful in local linearizations of non-linear material behavior, for example in a Newton–Raphson iterative solution scheme that computes the changing saturation of a magnetic circuit.

Permeability is the inductance per unit length. In SI units, permeability is measured in henries per metre (H·m−1 = J/(A2·m) = N A−2). The auxiliary magnetic field H has dimensions current per unit length and is measured in units of amperes per metre (A m−1). The product μH thus has dimensions inductance times current per unit area (H·A/m2). But inductance is magnetic flux per unit current, so the product has dimensions magnetic flux per unit area. This is just the magnetic field B, which is measured in webers (volt-seconds) per square-metre (V·s/m2), or teslas (T).

B is related to the Lorentz force on a moving charge q:

$\mathbf {F} =q(\mathbf {E} +\mathbf {v} \times \mathbf {B} ).$ The charge q is given in coulombs (C), the velocity v in meters per second (m/s), so that the force F is in newtons (N):

$q\mathbf {v} \times \mathbf {B} =C\cdot {\dfrac {m}{s}}\cdot {\dfrac {V\cdot s}{m^{2}}}={\dfrac {C\cdot (J/C)}{m}}={\dfrac {J}{m}}=N$ H is related to the magnetic dipole density. A magnetic dipole is a closed circulation of electric current. The dipole moment has dimensions current times area, units ampere square-metre (A·m2), and magnitude equal to the current around the loop times the area of the loop. The H field at a distance from a dipole has magnitude proportional to the dipole moment divided by distance cubed, which has dimensions current per unit length.

## Relative permeability and magnetic susceptibility

Relative permeability, sometimes denoted by the symbol μr, is the ratio of the permeability of a specific medium to the permeability of free space, μ0:

$\mu _{r}={\frac {\mu }{\mu _{0}}},$ where μ0 = 4π × 10−7 N A−2. In terms of relative permeability, the magnetic susceptibility is

$\chi _{m}=\mu _{r}-1.$ χm, a dimensionless quantity, is sometimes called volumetric or bulk susceptibility, to distinguish it from χp (magnetic mass or specific susceptibility) and χM (molar or molar mass susceptibility).

## Diamagnetism

{{#invoke:main|main}} Diamagnetism is the property of an object which causes it to create a magnetic field in opposition of an externally applied magnetic field, thus causing a repulsive effect. Specifically, an external magnetic field alters the orbital velocity of electrons around their nuclei, thus changing the magnetic dipole moment in the direction opposing the external field. Diamagnets are materials with a magnetic permeability less than μ0 (a relative permeability less than 1).

Consequently, diamagnetism is a form of magnetism that a substance exhibits only in the presence of an externally applied magnetic field. It is generally a quite weak effect in most materials, although superconductors exhibit a strong effect.

## Paramagnetism

{{#invoke:main|main}} Paramagnetism is a form of magnetism which occurs only in the presence of an externally applied magnetic field. Paramagnetic materials are attracted to magnetic fields, hence have a relative magnetic permeability greater than one (or, equivalently, a positive magnetic susceptibility). The magnetic moment induced by the applied field is linear in the field strength and rather weak. It typically requires a sensitive analytical balance to detect the effect. Unlike ferromagnets, paramagnets do not retain any magnetization in the absence of an externally applied magnetic field, because thermal motion causes the spins to become randomly oriented without it. Thus the total magnetization will drop to zero when the applied field is removed. Even in the presence of the field there is only a small induced magnetization because only a small fraction of the spins will be oriented by the field. This fraction is proportional to the field strength and this explains the linear dependency. The attraction experienced by ferromagnets is non-linear and much stronger, so that it is easily observed, for instance, in magnets on one's refrigerator.

## Gyromagnetism

For gyromagnetic media (see Faraday rotation) the magnetic permeability response to an alternating electromagnetic field in the microwave frequency domain is treated as a non-diagonal tensor expressed by:

{\begin{aligned}\mathbf {B} (\omega )&={\begin{vmatrix}\mu _{1}&-i\mu _{2}&0\\i\mu _{2}&\mu _{1}&0\\0&0&\mu _{z}\\\end{vmatrix}}\mathbf {H} (\omega )\\\end{aligned}} ## Values for some common materials

The following table should be used with caution as the permeability of ferromagnetic materials varies greatly with field strength. For example 4% Si steel has an initial relative permeability (at or near 0T) of 2,000 and a maximum of 35,000 and, indeed, the relative permeability of any material at a sufficiently high field strength trends toward 1.

Magnetic susceptibility and permeability data for selected materials
Medium Susceptibility χm
(volumetric SI)
Permeability μ [H/m] Relative permeability μ/μ0 Magnetic field Frequency max.
Metglas Template:Val Template:Val at 0.5 T 100 kHz
Iron (99.95% pure Fe annealed in H) Template:Val Template:Val
Nanoperm Template:Val Template:Val at 0.5 T 10 kHz
Mu-metal Template:Val Template:Val at 0.002 T
Mu-metal Template:Val Template:Val
Cobalt-Iron (high permeability strip material) Template:Val Template:Val
Permalloy Template:Val Template:Val Template:Val at 0.002 T
Iron (99.8% pure) Template:Val Template:Val
Electrical steel Template:Val Template:Val at 0.002 T
Ferritic stainless steel (annealed) Template:Val - Template:Val 1000–1800
Martensitic stainless steel (annealed) Template:Val - Template:Val 750–950
Ferrite (manganese zinc) >Template:Val 640 (or more) 100 kHz ~ 1 MHz
Ferrite (nickel zinc) Template:ValTemplate:Val 16–640 100 kHz ~ 1 MHz{{ safesubst:#invoke:Unsubst \$B=

{{#invoke:Category handler|main}}{{#invoke:Category handler|main}}[citation needed] }}

Carbon Steel Template:Val 100 at 0.002 T
Nickel Template:Val - Template:Val 100 – 600 at 0.002 T
Martensitic stainless steel (hardened) Template:Val - Template:Val 40–95
Austenitic stainless steel Template:Val - Template:Val 1.003–7  [note 1]
Neodymium magnet Template:Val 1.05
Platinum Template:Val Template:Val
Aluminum Template:Val Template:Val Template:Val
Wood Template:Val Template:Val
Air Template:Val Template:Val 
Concrete (dry) 1
Vacuum 0 4π × 10−70) 1, exactly
Hydrogen Template:Val Template:Val Template:Val
Teflon Template:Val Template:Val
Sapphire Template:Val Template:Val Template:Val
Copper Template:Val
or Template:Val
Template:Val Template:Val
Water Template:Val Template:Val Template:Val
Bismuth Template:Val Template:Val Template:Val
Superconductors −1 0 0

A good magnetic core material must have high permeability.

For passive magnetic levitation a relative permeability below 1 is needed (corresponding to a negative susceptibility).

Permeability varies with magnetic field. Values shown above are approximate and valid only at the magnetic fields shown. They are given for a zero frequency; in practice, the permeability is generally a function of the frequency. When frequency is considered, the permeability can be complex, corresponding to the in phase and out of phase response.

Note that the magnetic constant μ0 has an exact value in SI units (that is, there is no uncertainty in its value) because the definition of the ampere fixes its value to 4π × 10−7 H/m exactly.

## Complex permeability

A useful tool for dealing with high frequency magnetic effects is the complex permeability. While at low frequencies in a linear material the magnetic field and the auxiliary magnetic field are simply proportional to each other through some scalar permeability, at high frequencies these quantities will react to each other with some lag time. These fields can be written as phasors, such that

$H=H_{0}e^{j\omega t}\qquad B=B_{0}e^{j\left(\omega t-\delta \right)}$ where $\delta$ is the phase delay of $B$ from $H$ . Understanding permeability as the ratio of the magnetic flux density to the magnetic field, the ratio of the phasors can be written and simplified as

$\mu ={\frac {B}{H}}={\frac {B_{0}e^{j\left(\omega t-\delta \right)}}{H_{0}e^{j\omega t}}}={\frac {B_{0}}{H_{0}}}e^{-j\delta },$ so that the permeability becomes a complex number. By Euler's formula, the complex permeability can be translated from polar to rectangular form,

$\mu ={\frac {B_{0}}{H_{0}}}\cos \delta -j{\frac {B_{0}}{H_{0}}}\sin \delta =\mu ^{\prime }-j\mu ^{\prime \prime }.$ The ratio of the imaginary to the real part of the complex permeability is called the loss tangent,

$\tan \delta ={\frac {\mu ^{\prime \prime }}{\mu ^{\prime }}},$ which provides a measure of how much power is lost in a material versus how much is stored.