1088 P.S. Riseborough,G.M. Schmiedeshoff,and J.L.Smith
duction electrons scatter off of a set of independent
disordered magnetic moments. In this temperature
regime, the thermal conductivity from the electrons
may be calculated perturbatively [267].Theresult for
the Lorentz number L(T) can be approximately ex-
pressed in the form
L(T)=
1
e
2
T
I
(2)
I
(0)
−
I
(1)
I
(0)
2
, (19.156)
where I
(n)
is defined by Eq. (19.141). The Lorentz
number is also expected to depend strongly on the
crystalfieldsplittings [268].Thecrystalfieldsplitting
in CeCu
2
Si
2
is assumed to give rise to a minimum in
the Lorentz number at the temperature around 80 K.
In this high temperature regime, the Lorentz num-
ber can be appreciably greater than L
0
. This result
is caused by the large temperature induced shift of
the f density of states away from the Fermi energy
for T > T
K
.The experiments are consistent with this
trend: However, the lattice contribution to
L
is no
longer negligible and may be several times greater
than the quasi-particle contribution. This hypothe-
sis is supported by the comparison of measurements
on CeCu
2
Si
2
with the reference material LaCu
2
Si
2
.
In fact, if the phonon contribution
L
is completely
ignored in the data analysis, the Lorentz number is
about a factor oftwenty times greater than L
0
.Thein-
ferredpresence of a large phonon contribution is also
supported by the conclusion that the theoretical cal-
culated values of L(T),using the independent Kondo
impuritymodel,areunabletoaccountforelectronic
contributions to L(T) ofthismagnitude.Likewise,for
UPt
3
,the phonon contribution has been identified as
being important above3.5 K [29] and may be respon-
sible for up to a maximum of 4.5 L
0
of the Lorentz
number at T = 24 K inferredfrom the raw data [216].
The Lorentz number for CeCu
6
, in the high temper-
ature regime [269] qualitatively resembles L(T)for
UPt
3
, having a maximum at T ∼ 20 K where it at-
tains a value of about 2.5 L
0
but falls towards L
0
at
higher temperatures.
Ultrasonic Attenuation
Ultrasonic experiments measure the attenuation and
velocities of sound waves and, through the electron–
phonon interaction, provide information about the
electronic system. At temperatures much lower than
the Debye temperature, the attenuation of the sound
wave due to anharmonic phonon interactions should
be negligible, and the electron–phonon interaction
should provide the dominant contribution to the at-
tenuation.In this case,oneexpects a strongsimilarity
between the ultrasonic attenuation coefficient and
the electrical conductivity. Just like the optical con-
ductivity (!) yields the lifetime of a photon, the
ultrasonic attenuation ˛
q, ˆ
(!) yields the lifetime of
a phonon. This similarity is expected since, for many
purposes, the effect of a phonon can be interpreted
in terms of the effect of the accompanying electric
field. In analogy with the conductivity, one expects
that in the limit q → 0, the renormalization of the
scattering rate will cancel with the mass enhance-
ment. Thus, in the long wavelength limit, the ultra-
sonic attenuation is expected to be unrenormalized.
The most noticeable difference between ultrasonic
attenuation and optical absorption occurs through
the extremely different magnitudes of the velocities
of the corresponding waves. If the conditions allow
the heavy quasi-particles to co-move with the sound
wave, it becomes possible for the quasi-particles to
surf-ride and continuously absorb energy from the
sound wave. For example, if a longitudinally polar-
ized sound wave with phase velocity
!
q
propagates
through a gas of heavy quasi-particles, it strongly
perturbs the quasi-particles with velocities almost
parallel and almost equal to the phase velocity of
the wave. In the frame of reference traveling with
the wave, the quasi-particle is at rest and experiences
an essentially time independent electric field. The
electric field continuously transfers energy from the
wave to the quasi-particles that have the same ve-
locity. If there is a slight mismatch in the velocities,
quasi-particles with lower velocities than the wave
draw energy from the wave and accelerate, whereas
quasi-particles that are moving faster lose energy
and slow down. This results in the rate of energy
loss of the wave being proportional to the derivative
of the distributionof quasi-particle velocities,which
is evaluated at the velocity of sound.At temperatures
below those at which the heavy quasi-particles are
being formed, the Fermi velocity is comparable to