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where σ α = σ α ( q ) is the relative magnetization at the wave-vector q .
Introducing this into the free-energy expression, and utilizing the condi-
tion that i cos( q · R i + ϕ )=0,if q is not a reciprocal lattice vector,
we find
J 2
F 0 ) /N = 4
σ α
f =( F
α {
2 A α −J
( q )
}
J 4
αβ
+ 8
σ α σ β ,
B αβ {
2+cos2( ϕ α
ϕ β )
}
(2 . 1 . 24)
if 4 q is different from a reciprocal lattice vector.
The coecients of
the second power are thus
=1 αα ( q =0),where
the susceptibility is evaluated at zero magnetization. As long as all the
second-order coecients are positive, at any value of q , the free energy
is at its minimum when σ α = 0, i.e. the system is paramagnetic. The
smallest of these coecients are those at q = Q ,where
∝{
2 A α −J
( q )
}
( q )hasits
maximum. In the heavy rare earths, with the exception of Gd, Q is
non-zero and is directed along the c -axis. Depending on the sign of
B 2 , the magnetic structures occurring in the heavy rare earths may be
divided into two classes, which we will discuss in turn.
J
2.1.3 Transversely ordered phases
When B 2 > 0, as in Tb, Dy, and Ho, the two basal-plane components
of χ ( Q ) both diverge at the same critical temperature T N .Usingthe
approximate high-temperature value (2.1.20) for the susceptibility, we
find that 1 ξξ ( Q =0)=1 ηη ( Q , 0) = 2 A ξ −J
( Q ) vanishes at the
temperature determined by
( Q ) 1+ 5
) B 2 /k B T N .
k B T N 3
2
)( J + 2
J ( J +1)
J
( J
(2 . 1 . 25)
Below T N ,both σ ξ and σ η are generally non-zero at the wave-vector Q ,
and the free energy f , given by (2.1.24) with σ ζ = 0, is minimized when
σ ξ ( Q )= σ η ( Q )= σ Q ,and
σ Q = J
1 / 2
( Q )
2 A ξ
4 J 2 B ξξ
π
2 ,
;
ϕ ξ − ϕ η =
±
(2 . 1 . 26 a )
corresponding to the helical ordering:
J
= Q cos ( Q · R i + ϕ )
(2 . 1 . 26 b )
J
=
±
Q sin ( Q · R i + ϕ ) .
The length of the angular-momentum vector is Q , independent of the
site considered. There are two energetically-degenerate configurations,
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