
Semiclassical Equations from
Wave
Packets 469
The terms involving the anomalous velocity Q and wave packet magnetic mo-
ment rhp can sometimes be omitted from semiclassical equations
of
motion
for
electrons. One reason is that they often vanish by symmetry. In particular, they
vanish for crystals that have both time-inversion symmetry, and spatial inversion
symmetry. Under time inversion, k, d/idr, r, and B flip sign while
E
and
%^
are
unchanged; therefore Ù(k)
=
—Çl(—k)
and
m~
k
=
—«*_-£. Under spatial inversion,
r, k,
%£
and
E
flip sign while B does not, so Q(k) = Q(—k) and
in-^
= m_^. These
two symmetries are only compatible
if
Ù and
m-
k
vanish for all k. Thus the terms
can be omitted for many monatomic solids. However, they should not be omitted in
crystals without inversion symmetry, such as GaAs, or in crystals with spontaneous
magnetic moments such as iron. The existence of such terms has been known for
a long time, since work
of
Karplus and Luttinger (1954) and Blount (1962), and
the fact that they nevertheless have often been left off is due to
a
desire for sim-
plicity. The careful development of spintronics (Section 26.5) will however require
these terms to provide an accurate account of how spin currents respond to external
fields.
Limitations of Semiclassical Dynamics. Validity of the semiclassical equations
of motion requires four conditions:
1.
The spatial scales
of
all external potentials must be much larger than inter-
atomic spacing, making it possible to construct wave packets spanning many
unit cells, but seeing the external potentials as very slowly varying.
2.
The magnitudes of the electric fields cannot be too large, or else they induce
Zener tunneling between bands. To prevent this tunneling in a solid with band
gap £„, one must require, according to Eq. (16.64),
(16.86)
Electric fields this large are impossible to obtain in metals except near points
of degeneracy where band gaps shrink to zero. With energy gaps on the order
of
1
eV, and
\/kp
on the order
of
1 Â, the electric field needs to be on the
order of
1
V/Â, or 10
10
V/m. The largest fields that actually can be generated
in
a
metal are six orders
of
magnitude smaller, because electrons are quite
effective in screening external fields out of existence.
The magnitudes
of
magnetic fields cannot be too large. The characteristic
energy of electrons in magnetic fields
is
derived from their orbital period
7
and is 2TTH/7. For free electrons, as shown in Section 21.2, T
=
2irmc/eB,
which can used to obtain the estimate 2nh/7
~
1.16- 10
_4
[Z?/T]eV, measur-
ing the magnetic induction in Tesla. By analogy with Eq. (16.86), estimate
that magnetic fields will not induce interband transitions so long as
2irh/7<^E
g
J-f-.
(16.87)