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phase (but not if spontaneous ordering occurs), the magnetic moment
of the system per unit volume, neglecting the anisotropy, is given by
Curie's law (1.2.32):
g 2 µ 2 B J ( J +1)
3 k B T
N
V
M =
( H + H eff ) .
(1 . 5 . 8)
For a uniform system, we may write
N
j
1
g 2 µ 2 B
V
( ij ) M = J
( 0 )
g 2 µ 2 B
V
N M ,
H eff =
J
(1 . 5 . 9)
recalling that
( q )=
j
( ij ) e −i q · ( R i R j ) ,
J
J
(1 . 5 . 10)
and the susceptibility is therefore
1
1
g 2 µ 2 B J ( J +1)
3 k B T
N
V
J
( 0 ) J ( J +1)
3 k B T
C
χ MF =
θ ,
(1 . 5 . 11)
T
where C is the Curie constant (1.2.32), and the paramagnetic Curie
temperature is
θ = J
( 0 ) J ( J +1)
3 k B
.
(1 . 5 . 12)
From the Curie-Weiss law (1.5.11) it is apparent that, if nothing else
happens, the susceptibility diverges at θ , which is therefore also the
Curie temperature T C
at which spontaneous ferromagnetism occurs in
this model.
The bulk magnetic properties of the rare earths are summarized
in Table 1.6, where the moments are given in units of µ B /ion, and the
temperatures in K . The theoretical paramagnetic moments per ion are
µ = g
1 / 2 µ B , and are compared with values deduced from
the linear magnetic susceptibilities in the paramagnetic phases, using
(1.5.11). The theoretical saturation moments per ion are B J ,from
(1.2.30), and are compared with low-temperature values, in fields high
enough essentially to saturate the magnetization, or in the highest fields
in which measurements have been made (McEwen et al. 1973). θ
{
J ( J +1)
}
and θ
are the paramagnetic Curie temperatures, deduced from measurements
with a field applied respectively parallel and perpendicular to the c -
axis, and using (1.5.11). As we shall see in Section 2.1.1, there are
corrections to this expression at finite temperatures, which give rise to a
non-linearity in the inverse susceptibility. A simple linear extrapolation
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