This additional magnetic field may now be used for statistical considerations to calculate the mag-
netization as a function of temperature. The magnetization is the magnetic moment of the electrons
times the differnce in spin occupation (see figure 66).
M= (N 1 −N 2 )μ (83)
We can calculateN 1 andN 2 in thermal equilibrium
N 1
N
=
e
μB
kBT
e
μB
kBT +e
−μB
kBT
(84)
N 2
N
=
e−
μB
kBT
e
μB
kBT +e
−μB
kBT
(85)
Combining these equations leads to a magnetization of
M = (N 1 −N 2 )μ (86)
M = Nμ
e
μB
kBT−e
−μB
kBT
e
μB
kBT+e
−μB
kBT
(87)
M = Nμtanh(
μB
kBT
) (88)
In this result for the magnetization we can plug in the magnetic field from the mean field calculation
M=Mstanh(
Tc
T
M
Ms
) (89)
with the saturation magnetization
Ms=
NgμB
2 V
(90)
and the Curie temperture
Tc=
nnnJ
4 kB
(91)
. A well known approximation to this implicit equation is the Curie-Weiss law which is valid for
B << T(see figure 67). Expanding the hyperbolic tangent aroundTcyields
M~ = χ
μ 0
B, T > T~ c (92)
χ =
C
T−Tc
(93)
Summing up