查看“︁居里-外斯定律”︁的源代码

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{{translating|[[:en:Curie-weiss law]]|time=2019-05-05}}
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|T=zh-hans:居里-韦斯定律;zh-cn:居里-韦斯定律;zh-hk:居禮-外斯定律;zh-tw:居禮-外斯定律;
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|1=zh-hans:居里;zh-cn:居里;zh-hk:居禮;zh-tw:居禮;
|2=zh-hans:居里-韦斯定律;zh-cn:居里-韦斯定律;zh-hk:居禮-外斯定律;zh-tw:居禮-外斯定律;
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'''居禮-外斯定律'''為[[居里定律]]的修正公式，用來補足該公式的不足。當一物質的溫度大於[[居里溫度]](<math>T_{c}</math>)時，其磁化率<math>\chi</math>與溫度<math>T</math>的關係式為：
:<math>\chi = \frac{C}{T - T_{c}}</math>
其中：
:<math>C</math>是該物質的居禮常數
:<math>T</math>是絕對溫度，單位為<math>K</math>
:<math>T_{c}</math>是該物質的居禮溫度，單位為<math>K</math>

根據該定律，當<math>T=T_{c}</math>時，[[磁化率]]為無窮大。而當低於此溫度時，鐵磁性物質將會[[自發磁化]]。

==基本概念==

一個磁性物質的[[磁化強度|磁化向量]](或稱磁化強度)代表單位體積該物質的磁矩強度。而磁矩可能由原子內的電子運動或者是[[自旋]]所產生。而淨磁化向量可能由外加磁場誘導產生，甚至可能不需要施加外加磁場也能產生磁化向量(例如足夠低溫狀態下的鐵)，其中後者被稱之為[[自發磁化]]。<br>

而其他與鐵擁有同樣性質的物質，如[[鎳]]與[[磁鐵礦]]，被稱之為[[鐵磁性|鐵磁性物質]]。鐵磁性物質在足夠低的溫度下將會不須施加外部磁場也會產生磁性，而該臨界溫度稱之為[[居禮溫度]]。
== 局限性 ==

有许多材料的磁化特性在居里点附近显现出明显的敏感性，而由于居里-韦斯定律基于[[平均场理论|平均场近似]]而无法描述这种现象。

{{TransH}}
In many materials the Curie–Weiss law fails to describe the susceptibility in the immediate vicinity of the Curie point, since it is based on a [[mean field theory|mean-field approximation]]. Instead, there is a [[critical behavior]] of the form

:<math>
\chi \sim \frac{1}{(T - T_{c})^\gamma}
</math>

with the [[critical exponent]] {{math| <var>&gamma;</var>}}. However, at temperatures {{math| <var>T ≫ T<sub>c</sub></var>}} the expression of the Curie–Weiss law still holds true, but with {{math| <var>T<sub>c</sub></var>}} replaced by a temperature {{math| <var>&Theta;</var>}} that is somewhat higher than the actual Curie temperature. Some authors call {{math| <var>&Theta;</var>}} the '''Weiss constant''' to distinguish it from the temperature of the actual Curie point.

== Classical approaches to magnetic susceptibility and Bohr–van Leeuwen theorem ==

According to [[Bohr–van Leeuwen theorem]] when statistical mechanics and classical mechanics are applied consistently, the thermal average of the magnetization is always zero. Magnetism cannot be explained without quantum mechanics. However we list some classical approaches to it as they are easy to understand and relate to even though they are incorrect.

The magnetic moment of a free atom is due to the orbital angular momentum and spin of its electrons and nucleus. When the atoms are such that their shells are completely filled they do not have any net magnetic dipole moment in the absence of external magnetic field. When present, such field distorts the trajectories (classical concept) of the electrons so that the applied field could be opposed as predicted by the [[Lenz's law]]. In other words the net magnetic dipole induced by the external field is in the opposite direction and such materials are repelled by it. These are called [[diamagnetic]] materials.

Sometimes an atom has a net magnetic dipole moment even in the absence of an external magnetic field. The contributions of the individual electrons and nucleus to the total angular momentum do not cancel each other. This happens when the shells of the atoms are not fully filled up ([[Hund's Rule]]). A collection of such atoms however may not have any net magnetic moment as these dipoles are not aligned. An external magnetic field may serve to align them to some extent and develop a net magnetic moment per volume. Such alignment is temperature dependent as thermal agitation acts to disorient the dipoles. Such materials are called [[paramagnetic]].

In some materials, the atoms (with net magnetic dipole moments) can interact with each other to align themselves even in the absence of any external magnetic field when the thermal agitation is low enough. Alignment could be parallel ([[ferromagnetism]]) or anti-parallel. In case of anti-parallel, the dipole moments may or may not cancel each other ([[antiferromagnetism]], [[ferrimagnetism]]).


== Density matrix approach to magnetic susceptibility ==

We take a very simple situation in which each atom can be approximated as a two state system. The thermal energy is so low that the atom is in ground state. In this ground state the atom is assumed to have no net orbital angular momentum but only one unpaired electron to give it a spin of half. In the presence of an external magnetic field the ground state will split into two states having energy difference proportional to the applied field. The spin of the unpaired electron is parallel to the field in the higher energy state and anti-parallel in the lower one.

A [[density matrix]], <math> \rho </math>, is a matrix that describes a quantum system in a mixed state, a statistical ensemble of several quantum states (here several similar 2-state atoms). This should be contrasted with a single state vector that describes a quantum system in a pure state. The expectation value of a measurement, <math> A </math>, over the ensemble is <math> \langle A \rangle = Tr (A \rho) </math>. In terms of a complete set of states, <math> |i\rangle </math>, one can write
: <math>
\rho = \sum_{ij}
\rho_{ij} |i\rangle \langle j| .
</math>

Von Neumann’s equation tells us how the density matrix evolves with time.
: <math>
i \hbar \frac d {dt} \rho (t) = [H, \rho(t)]
</math>

In equilibrium,
one has <math> [H, \rho] = 0 </math>, and the allowed density matrices are 
<math> f(H) </math>.
The canonical ensemble has 
<math> \rho = \exp(-H/T)/Z </math>
where
<math> Z = Tr \exp(-H/T) </math>.

For the 2-state system, we can write
<math> H = -\gamma \hbar B \sigma_3 </math>.
Here <math> \gamma </math> is the [[gyromagnetic ratio]].
Hence <math> Z = 2 \cosh(\gamma \hbar B/(2T)) </math>, and
:<math>
\rho(B,T) = \frac 1 {2 \cosh(\gamma \hbar B/(2T))} 
\begin{pmatrix}
\exp (-\gamma \hbar B/(2T)) & 0 \\
0 & \exp (\gamma \hbar B/(2T))
\end{pmatrix}.
</math>

From which 
:<math>
\langle J_x \rangle = 
\langle J_y \rangle = 0, 
\langle J_z \rangle = - \frac \hbar 2 \tanh (\gamma \hbar B/(2T)).
</math>

== Explanation of para and diamagnetism using perturbation theory ==

In the presence of a uniform external magnetic field <math> B </math> along the z-direction, the Hamiltonian of the atom changes by
:<math>
\Delta H = \alpha J_z B + \beta B^2 \sum_i (x_i^2 + y_i^2 ),
</math>
where <math> \alpha, \beta </math> are positive real numbers which are independent of which atom we are looking at but depends on the mass and the charge of the electron. <math> i </math> corresponds to individual electrons of the atom.

We apply second order [[perturbation theory]] to this situation. This is justified by the fact that even for highest presently attainable field strengths, the shifts in the energy level due to <math> \Delta H </math> is quite small w.r.t. atomic excitation energies. Degeneracy of the original Hamiltonian is handled by choosing a basis which diagonalizes <math> \Delta H </math> in the degenerate subspaces. Let <math> |n\rangle </math> be such a basis for the state of the atom (rather the electrons in the atom). Let <math> \Delta E_n </math> be the change in energy in <math> |n \rangle </math>. So we get
:<math>
\Delta E_n = \langle n | \Delta H | n \rangle + \sum_{m, E_m \neq E_n} 
\frac
{| \langle n | \Delta H | m \rangle |^2}
{E_n - E_m}
.
</math>
In our case we can ignore <math> B^3 </math> and higher order terms. We get
:<math>
\Delta E_n = \alpha B \langle n | J_z | n \rangle
+
\alpha^2 B^2 \sum_{m, E_m \neq E_n} 
\frac
{| \langle n | J_z | m \rangle |^2}
{E_n - E_m}
+
\beta
B^2 \sum_i \langle n | x_i^2 + y_i^2 | n \rangle
.
</math>

In case of diamagnetic material, the first two terms are absent as they don't have any angular momentum in their ground state. In case of paramagnetic material all the three terms contribute.
== Adding spin-spin interaction in the Hamiltonian: Ising model ==

So far we have assumed that the atoms do not interact with each other. Even though this is a reasonable assumption in case of diamagnetic and paramagnetic substances, this assumption fails in case of ferromagnetism where the spins of the atom try to align with each other to the extent permitted by the thermal agitation. In this case we have to consider the Hamiltonian of the ensemble of the atom. Such a Hamiltonian will contain all the terms described above for individual atoms and terms corresponding to the interaction among the pairs of atom. [[Ising model]] is one of the simplest approximation of such pairwise interaction.
:<math>
H_{\text{pairs}} = 
- \frac 1 2
\sum_{R,R'}
S(R) \cdot S(R') J (R - R')
</math>

Here the two atoms of a pair are at <math> R, R' </math>. Their interaction <math> J </math> is determined by their distance vector <math> R - R' </math>. In order to simplify calculation it is often assumed that interaction happens between neighboring atoms only and <math> J </math> is a constant. The effect of such interaction is often approximated as a [[mean field]] and in our case the [[Weiss field]].

== Modification of Curie Law due to Weiss field ==

The Curie-Weiss Law is an adapted version of Curie's Law, which for a paramagnetic material may be written in SI units as<ref name=Hall205>{{harvnb|Hall|1994|pp=205–206}}</ref>

:<math>\chi = \frac{M}{H} =\frac{M \mu_0}{B} =\frac{C}{T} .</math>

Here µ<sub>0</sub> is the [[permeability of free space]];  ''M'' the [[magnetization]] ([[magnetic moment]] per unit volume), {{math|''B''{{=}}''µ''<sub>0</sub>''H''}} is the [[magnetic field]], and ''C'' the material-specific [[Curie constant]]:

:<math>C = \frac{\mu_0 \mu_B^2}{3 k_B}N g^2 J(J+1),</math>
where {{math|''k''<sub>B</sub>}} is [[Boltzmann's constant]], {{math|''N''}} the number of magnetic atoms (or molecules) per unit volume, {{math|''g''}} the [[Landé g-factor]], {{math|''&mu;''<sub>B</sub>}} the [[Bohr magneton]],  {{math|''J''}} the [[angular momentum]] quantum number.<ref name=Levy201>{{harvnb|Levy|1968|pp=201–202}}</ref>

For the Curie-Weiss Law the total magnetic field is {{math|''B+λM''}} where {{math|''λ''}} is the Weiss molecular field constant and then

:<math>\chi =\frac{M \mu_0}{B}</math> → <math>\frac{M \mu_0}{B+\lambda M} =\frac{C}{T}</math>

which can be rearranged to get

:<math>\chi = \frac{C}{T - \frac{C \lambda }{\mu_0}}</math>

which is the Curie-Weiss Law

:<math>
\chi = \frac{C}{T - T_{c}}
</math>
where the [[Curie Temperature]] {{math|''T''<sub>C</sub>}} is

:<math>T_C = \frac{C \lambda }{\mu_0}</math>

==参见==
*[[Curie's law]]
*[[Paramagnetism]]
*[[Pierre Curie]]
*[[Pierre-Ernest Weiss]]
*[[Exchange interaction]]
{{TransF}}
== 注释 ==

{{reflist}}

==参考资料==

*{{cite book|last=Kittel|first=Charles|title=Introduction to solid state physics|year=1996|publisher=Wiley|location=New York [u.a.]|isbn=978-0471111818|edition=7th}}
*{{cite book|last=Hall|first=H. E. Hook, J. R.|title=Solid state physics|year=1994|publisher=Wiley|location=Chichester|isbn=0471928054|edition=2nd |ref=harv}}
*{{cite book|last=Levy|first=Robert A|title=Principles of Solid State Physics|url=https://archive.org/details/principlesofsoli00levy|year=1968|publisher=Academic Press |isbn=978-0124457508|ref=harv}}
*{{cite book|author= [[Neil Ashcroft]], [[David Mermin]] |title=Solid State Physics|year= 1976 |url= https://archive.org/details/solidstatephysic00ashc }}
*http://theory.tifr.res.in/~sgupta/courses/qm2013/hand5.pdf {{Wayback|url=http://theory.tifr.res.in/~sgupta/courses/qm2013/hand5.pdf |date=20190716123323 }}

{{居禮夫婦}}
[[Category:磁序]]
[[Category:皮埃尔·居里]]