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In classical electromagnetism, magnetization is the that expresses the of permanent or induced magnetic dipole moments in a magnetic material. Accordingly, physicists and engineers usually define magnetization as the quantity of per unit volume.

It is represented by a M. Magnetization can be compared to electric polarization, which is the measure of the corresponding response of a material to an in .

Magnetization also describes how a material responds to an applied as well as the way the material changes the magnetic field, and can be used to calculate the that result from those interactions.

The origin of the magnetic moments responsible for magnetization can be either microscopic resulting from the motion of in , or the spin of the electrons or the nuclei. Net magnetization results from the response of a material to an external .

materials have a weak induced magnetization in a magnetic field, which disappears when the magnetic field is removed. and materials have strong magnetization in a magnetic field, and can be magnetized to have magnetization in the absence of an external field, becoming a . Magnetization is not necessarily uniform within a material, but may vary between different points.


Definition
The magnetization field or M-field can be defined according to the following equation: \mathbf M = \frac{\mathrm{d}\mathbf m}{\mathrm{d}V}

Where \mathrm{d}\mathbf{m} is the elementary and \mathrm{d}V is the ; in other words, the M-field is the distribution of magnetic moments in the region or concerned. This is better illustrated through the following relation: \mathbf m=\iiint \mathbf M\,\mathrm{d}V where m is an ordinary magnetic moment and the triple integral denotes integration over a volume. This makes the M-field completely analogous to the electric polarization field, or P-field, used to determine the electric dipole moment p generated by a similar region or manifold with such a polarization: \mathbf P = {\mathrm{d}\mathbf p \over \mathrm{d}V}, \quad \mathbf p = \iiint \mathbf P\,\mathrm{d}V , where \mathrm{d}\mathbf{p} is the elementary electric dipole moment.

Those definitions of P and M as a "moments per unit volume" are widely adopted, though in some cases they can lead to ambiguities and paradoxes.

The M-field is measured in per (A/m) in .


In Maxwell's equations
The behavior of ( B, H), ( E, D), ( ρ), and ( J) is described by Maxwell's equations. The role of the magnetization is described below.


Relations between B, H, and M
The magnetization defines the auxiliary magnetic field H as
\mathbf{B}=\mu_0(\mathbf{H + M}) ()
\mathbf{B} = \mathbf{H} + 4 \pi \mathbf{M} ()
which is convenient for various calculations. The vacuum permeability μ0 is, approximately, ).

A relation between M and H exists in many materials. In and , the relation is usually linear:

\mathbf{M} = \chi\mathbf{H}, \, \mathbf{B} = \mu\mathbf{H}=\mu_0 (1+\chi)\mathbf{H},
where χ is called the volume magnetic susceptibility, and μ is called the magnetic permeability of the material. The per unit volume (i.e. magnetic ) of the paramagnet (or diamagnet) in the magnetic field is:
-\mathbf{M} \cdot \mathbf{B}=-\chi\mathbf{H} \cdot \mathbf{B}=-\frac{\chi}{1+\chi}\frac{\mathbf{B}^2}{\mu_0},
the negative gradient of which is the magnetic force on the paramagnet (or diamagnet) per unit volume (i.e. force density).

In diamagnets (\chi <0) and paramagnets (\chi >0), usually |\chi|\ll 1, and therefore \mathbf{M} \approx \chi\frac{\mathbf{B}}{\mu_0}.

In there is no one-to-one correspondence between M and H because of magnetic hysteresis.


Magnetic polarization
Alternatively to the magnetization, one can define the magnetic polarization, (often the symbol is used, not to be confused with current density).
\mathbf{B}=\mu_0\mathbf{H} + \mathbf{I} ().

This is by direct analogy to the electric polarization, \mathbf{D}=\varepsilon_0\mathbf{E} + \mathbf{P}. The magnetic polarization thus differs from the magnetization by a factor of :

\mathbf{I}=\mu_0\mathbf{M} ().

Whereas magnetization is given with the unit ampere/meter, the magnetic polarization is given with the unit tesla.


Magnetization current
The magnetization M makes a contribution to the J, known as the magnetization current.

\mathbf{J}_\mathrm{m} = \nabla \times \mathbf{M}
and for the bound surface current:
\mathbf{K}_\mathrm{m} = \mathbf{M} \times \mathbf{\hat{n}}
so that the total current density that enters Maxwell's equations is given by
\mathbf{J} = \mathbf{J}_\mathrm{f} + \nabla \times \mathbf{M} + \frac{\partial\mathbf{P}}{\partial t}
where Jf is the electric current density of free charges (also called the free current), the second term is the contribution from the magnetization, and the last term is related to the electric polarization P.


Magnetostatics
In the absence of free electric currents and time-dependent effects, Maxwell's equations describing the magnetic quantities reduce to
\begin{align}
\mathbf{\nabla\times H} &= \mathbf{0}\\
\mathbf{\nabla\cdot H} &= -\nabla\cdot\mathbf{M}
     
\end{align}

These equations can be solved in analogy with problems where

\begin{align}
\mathbf{\nabla\times E} &= \mathbf{0} \\
 \mathbf{\nabla\cdot E} &= \frac{\rho}{\epsilon_0}
     
\end{align}

In this sense −∇⋅ M plays the role of a fictitious "magnetic charge density" analogous to the electric charge density ρ; (see also demagnetizing field).


Dynamics
The time-dependent behavior of magnetization becomes important when considering nanoscale and nanosecond timescale magnetization. Rather than simply aligning with an applied field, the individual magnetic moments in a material begin to precess around the applied field and come into alignment through relaxation as energy is transferred into the lattice.


Reversal
Magnetization reversal, also known as switching, refers to the process that leads to a 180° (arc) re-orientation of the magnetization with respect to its initial direction, from one stable orientation to the opposite one. Technologically, this is one of the most important processes in that is linked to the magnetic data storage process such as used in modern hard disk drives.

As it is known today, there are only a few possible ways to reverse the magnetization of a metallic magnet:

  1. an applied
  2. via a beam of particles with spin
  3. magnetization reversal by circularly polarized light;

i.e., incident electromagnetic radiation that is circularly polarized


Demagnetization
Demagnetization is the reduction or elimination of magnetization. One way to do this is to heat the object above its Curie temperature, where thermal fluctuations have enough energy to overcome exchange interactions, the source of ferromagnetic order, and destroy that order. Another way is to pull it out of an electric coil with alternating current running through it, giving rise to fields that oppose the magnetization.

One application of demagnetization is to eliminate unwanted magnetic fields. For example, magnetic fields can interfere with electronic devices such as cell phones or computers, and with machining by making cuttings cling to their parent.


See also

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