Figure 77: (a) Ground state of a linear ferromagnetic chain at zero temperature, (b) excited state
where one spin is flipped, (c) excite state where the spin flip is equally distributet among
all available spins resulting in a spin wave. [from Kittel]
To calculate the dispersion relation for Magnons we examine thekthspin in equation 135
Uk=− 2 JS~k·(S~k− 1 +S~k+1) (141)
. Inserting the relation between magnetic moment and spin~μ=γS~=−gμBS~into this relation we
obtain
Uk=−~μk·(
− 2 J
gμB
(S~k− 1 +S~k+1)) (142)
. Because the potential energy of a magnetic dipole isU=−~μ·B~we may interpret
B~k=−^2 J
gμB
(S~k− 1 +S~k+1) (143)
as the effective magnetic field on spin k due to the nearest neighbors. The rate of change of angular
momentum is the torqueT~ =d
~S
dt =~μ×
B~. Using the torque we set up equations of motion for the
spin
d
dt
S~k = −gμB
~
S~k×B~k (144)
=
2 J
~
(S~k×S~k− 1 +S~k×S~k+1) (145)
. The cartesian components of this relation are
d
dt
S~xk =^2 J
~
(Sky(Szk− 1 +Skz+1)−Szk(Sky− 1 +Sky+1)) (146)
d
dt
S~ky =^2 J
~
(Skz(Skx− 1 +Skx+1)−Skx(Skz− 1 +Skz+1)) (147)
d
dt
S~kz =^2 J
~
(Skx(Syk− 1 +Syk+1)−Sky(Sxk− 1 +Skx+1)) (148)
. One way to solve these nonlinear set of equations it is to linearize them. This is valid in the low
energy limit since we already know that low-lying excitations have a form of 77 (c) and therefore