Added to Favorites

Related Searches

Definitions

In a paramagnetic material the magnetization of the material is (approximately) directly proportional to an applied magnetic field. However, if the material is heated, this proportionality is reduced: for a fixed value of the field, the magnetization is (approximately) inversely proportional to temperature. This fact is encapsulated by Curie's law:## Derivation with quantum statistical mechanics

### Two-state (spin-1/2) paramagnetons

### General case

## Derivation with classical statistical mechanics

## Applications

It is the basis of operation of magnetic thermometers, which are used to measure very low temperatures.
## See also

- $mathbf\{M\}\; =\; C\; cdot\; frac\{mathbf\{B\}\}\{T\},$

where

- $mathbf\{M\}$ is the resulting magnetisation

- $mathbf\{B\}$ is the magnetic field, measured in teslas

- $T$ is absolute temperature, measured in kelvins

- $C$ is a material-specific Curie constant

This relation was discovered experimentally (by fitting the results to a correctly guessed model) by Pierre Curie. It only holds for high temperatures, or weak magnetic fields. As the derivations below show, the magnetization saturates in the opposite limit of low temperatures, or strong fields.

A simple model of a paramagnet concentrates on the particles which compose it, call them paramagnetons, which do not interact with each other. Each paramagneton has a magnetic moment given by $vec\{mu\}$. The energy of a magnetic moment in a magnetic field is given by

- $E=-vec\{mu\}cdotvec\{B\}$

To simplify the calculation, we are going to work with a 2-state paramagneton: the particle may either align its magnetic moment with the magnetic field, or against it. So the only possible values of magnetic moment are then $mu$ and $-mu$. If so, then such a particle has only two possible energies

- $E\_0\; =\; -\; mu\; B$

and

- $E\_1\; =\; mu\; B$

When one seeks the magnetization of a paramagnet, one is interested in the likelihood of a paramagneton to align itself with the field. In other words, one seeks the expectation value of the magnetization $mu$:

- $leftlanglemurightrangle\; =\; mu\; Pleft(muright)\; +\; (-mu)\; Pleft(-muright)$

- $Z\; =\; sum\_\{n=0,1\}\; e^\{-E\_nbeta\}\; =\; e^\{\; mu\; Bbeta\}\; +\; e^\{-mu\; Bbeta\}\; =\; 2\; coshleft(mu\; Bbetaright)$

Therefore, in this simple case we have:

- $leftlanglemurightrangle\; =\; mu\; tanhleft(mu\; Bbetaright)$

This is magnetization of one paramagneton, the total magnetization of the solid is given by

$M\; =\; Nleftlanglemurightrangle\; =\; N\; mu\; tanhleft(\{mu\; Bover\; k\; T\}right)$The formula above is known as the Langevin paramagnetic equation. Pierre Curie found an approximation to this law which applies to the relatively high temperatures and low, magnetic fields used in his experiments. Let's see what happens to the magnetization as we specialize it to large $T$ and small $B$. As temperature increases and magnetic field decreases, the argument of hyperbolic tangent decreases. Another way to say this is

- $left(\{mu\; Bover\; k\; T\}right)\; ll\; 1$

this is sometimes called the Curie regime. We also know that if $|x|\; ll\; 1$, then

- $tanh\; x\; approx\; x$

- $mathbf\{M\}(Trightarrowinfty)=\{Nmu^2over\; k\}\{mathbf\{B\}over\; T\}$

Q.E.D., with a Curie constant given by $C=\; Nmu^2/k$. Also, in the opposite regime of low temperatures or high fields, $M$ tends to a maximum value of $Nmu$, corresponding to all the paramagnetons being completely aligned with the field.

When the paramagnetons have an arbitrary spin (any number of spin states), the formula is a bit more complicated. For this more general formula and its derivation, see the article: Brillouin function. As the spin approaches infinity, the formula for the magnetization approaches the classical value derived in the following section.

An alternative treatment applies when the paramagnetons are imagined to be classical, freely-rotating magnetic moments. In this case, their position will be determined by their angles in spherical coordinates, and the energy for one of them will be:

- $E\; =\; -\; mu\; Bcostheta,$

where $theta$ is the angle between the magnetic moment and the magnetic field (which we take to be pointing in the $z$ coordinate.) The corresponding partition function is

- $Z\; =\; int\_0^\{2pi\}\; dphi\; int\_0^\{pi\}dtheta\; sintheta\; exp(mu\; Bbeta\; costheta).$

We see there is no dependence on the $phi$ angle, and also we can change variables to $y=costheta$ to obtain

- $Z\; =\; 2pi\; int\_\{-1\}^\; 1\; d\; y\; exp(mu\; Bbeta\; y)\; =$

Now, the expected value of the $z$ component of the magnetization (the other two are seen to be null (due to integration over $phi$), as they should) will be given by

- $leftlanglemu\_z\; rightrangle\; =\; \{1\; over\; Z\}\; int\_0^\{2pi\}\; dphi\; int\_0^\{pi\}dtheta\; sintheta\; exp(mu\; Bbeta\; costheta)\; left[mucosthetaright]\; .$

To simplify the calculation, we see this can be written as a differentiation of $Z$:

- $leftlanglemu\_zrightrangle\; =\; \{1\; over\; Z\; B\}\; partial\_beta\; Z.$

Carrying out the derivation we find

- $leftlanglemu\_zrightrangle\; =\; mu\; L(mu\; Bbeta),$

where $L$ is the Langevin function:

- $L(x)=\; coth\; x\; -\{1\; over\; x\}.$

This function would appear to be singular for small $x$, but it is not, since the two singular terms cancel each other. In fact, its behavior for small arguments is $L(x)\; approx\; x/3$, so the Curie limit also applies, but with a Curie constant three times smaller in this case. Similarly, the function saturates at $1$ for large values of its argument, and the opposite limit is likewise recovered.

Wikipedia, the free encyclopedia © 2001-2006 Wikipedia contributors (Disclaimer)

This article is licensed under the GNU Free Documentation License.

Last updated on Sunday August 03, 2008 at 19:01:21 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

This article is licensed under the GNU Free Documentation License.

Last updated on Sunday August 03, 2008 at 19:01:21 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

Copyright © 2014 Dictionary.com, LLC. All rights reserved.