The symmetry of the order parameter and the magnitude of the energy gap are two of the most fundamental properties of superconductors. While there is a general agreement about the s-wave nature of superconductivity in the alkali metal fulleride compounds, the magnitude of the energy gap is not known with sufficient accuracy.
Why is the determination of the energy gap so important? Let us consider,
for example, the Eliashberg theory of phonon-mediated superconductivity, and
represent the phonons by a single Einstein mode.[1, 2]
There are two parameters in this theory: The phonon
frequency
and the coupling between electrons and phonons
.
(The latter one may be viewed as an ``effective" electron - phonon coupling
constant, incorporating the ``true"
and the electron - electron
repulsion parameter
.[1, 3]) In the weak coupling (BCS)
limit the quantity
is the only relevant
combination of parameters. In that limit the
ratio of the low temperature value of the superconducting energy
gap to the critical temperature is always
. If the coupling is strong, however, knowledge of the
critical temperature and the low temperature gap provides us with
and
. Once the magnitudes of these parameters are known,
theoretical models for the microscopic mechanism of
superconductivity [4] can be placed in the proper context.
A review of the literature reveals a great disparity
between the various measurements of the superconducting energy gap
in Rb
C
. Direct spectroscopic
methods to determine the gap include optical spectroscopy, tunneling and
photoemission. The first optical study by Rotter et al. [5]
resulted in values of
.
Fitzgerald et al. [6] obtained
from transmission measurements on thin film samples. In
more recent reflectance measurements on polycrystalline[7]
and single crystal[8] samples, Degiorgi et al. obtained
and
, respectively. Zhang et al. [9]
reported tunneling measurements yielding a value greater than 5, whereas
Jess and co-workers measured values between 2 and 4 in an STM study
[10]. Photoemission experiments by the Argonne-University of Illinois
collaboration [11] led to
. Nuclear magnetic
resonance [12, 13] and muon spin relaxation [14] yielded
values compatible with the BCS weak coupling limit. (All numerical values
summarized here apply to Rb
C
.)
An accurate determination of
, and the detailed fit of the
theoretical curves to the experimental results answers a fundamental
question: Is the coupling between the electrons weak enough for
the BCS theory to describe superconductivity?
In this Letter we report optical transmission and tunneling measurements
unambiguously demonstrating that the ratio
is
,
significantly larger than the BCS value. Since the weak coupling conditions
are not satisfied, we are able to deduce the
phonon coupling constant and the characteristic phonon frequency, obtaining
and
cm
(
meV).
The electron - phonon coupling is consistent with the value determined from DC
resistivity measurements [15]; the phonon frequency is close to the
lowest lying Raman frequency of the C
molecule [16].
Figure 1: Resistivity and resistance of the thin film and pressed pellet
samples used in the optical and tunneling measurements, respectively.
The pressed pellet
samples for the tunneling measurements were made by heating and mixing
stoichiometric amounts of Rb and C
in a quartz tube for several weeks.
According to powder X-ray diffraction, the sample contained
no secondary phases.
The material was pressed into a pellet, with four gold wires embedded for
electrical contacts. The resistivity as a function
of the temperature is shown in Figure 1. The
resistivity of the pressed pellet sample was as low as the resistivity of
single crystals[15]. The superconducting transition temperature was
30K.
The optical measurements were performed on samples prepared by deposition of
a thin C
film on a Si substrate and subsequent exposure to Rb vapor in a
sample cell mounted in a Bomem MB-155 spectrometer.[17] The composition of the
sample was monitored by observing the
vibrational mode of the C
molecule [18]. The thickness of the film was
m.
Scanning force microscope images
of the sample surface showed an irregular surface with poorly matching crystal
faces.
From room temperature to 30K there was a factor of two increase
of resistance, typical of thin film samples [19] and indicative of
granular morphology (Figure 1).
The superconducting transition occurred at 30K; a
smearing of the transition suggested a distribution of critical
temperatures, also consistent with granular morphology.
Figure 2:
(top) Far infrared transmission of the sample at
temperatures below the superconducting transition. The curves are
normalized to the transmission at T = 35K in order to eliminate the
features due to the silicon substrate. (bottom) Calculated transmission curves,
based on dirty limit BCS results.
The far-IR transmission spectra were measured as a function of temperature at the U4IR beamline of the National Synchrotron Light Source, at Brookhaven National Laboratory. The sample cell was mounted on a Helitran He flow refrigerator and the spectra were taken in a Nicolet 20F Rapid Scan FTIR spectrometer. Due to the capacitive inter-grain coupling, AC measurements (including the optical transmission) are expected to be less sensitive to the grain boundaries then the DC transport. In accordance with this expectation, the optical transmission of the film decreased upon cooling, corresponding to the increasing intrinsic conductivity of the crystallites.
The upper panel in Figure 2 shows the low temperature transmission
results, normalized to the spectrum taken in the normal state at 35K. The
pronounced peak in the optical transmission is a direct
evidence for the sharp energy gap in the real part of the optical
conductivity at
. This feature was first
observed for superconductors, and discussed in
detail, by Glover and Tinkham [20].
Figure 3: Temperature dependence of the energy gap evaluated from the
optical transmission data. The dashed line represents the BCS temperature
dependence, scaled to satisfy
.
Calculated transmission curves are shown in the lower panel of Figure
2. In the absence of readily available Eliashberg
results for the density of states and optical conductivity, we
modified the BCS result[21] to include the effects of
inelastic pair breaking[25] in a phenomenological way.
The total optical transmission t was represented in a two component model,
in the form of
,
where
is the transmissions of a Drude metal, and
, was
calculated from the Mattis-Bardeen[21] conductivity
of a superconductor. This approach also accounts for the inevitable
imperfections in the sample. In the best fits the
weight factor was about w=30% at the lowest
temperature, and it decreased as the temperature approached
.
The
energy gap as a function of the temperature, evaluated from these fits, is
shown in Figure 3. Notice that the energy gap at zero
temperature corresponds to
.
For comparison, the temperature dependence of the weak
coupling (BCS) gap, scaled to
,
is also shown in the Figure.
For the tunneling measurements
the pressed pellets were first cooled to low temperature. A break junction was
made and controlled by mechanical means. The device was similar
to the one used in the tunneling studies of high
superconductors
[22]. The sample was in He atmosphere to
prevent the degradation of the material due to the chemical reaction with
oxygen. The differential conductance of a typical junction at
T = 4.2K is shown in Figure 4. The poor thermal stability
of the junction prevented us from measuring the temperature dependence of
the tunneling.
Figure 4: Differential conductance of the break junction made of a
polycrystalline RbC
pellet (open circles). The continuous line is a three
parameter fit using a modified BCS formula for the density of states (see
text). The dashed line was obtained by including an additional leakage
conductance at zero bias, and the voltage dependence of the transmission
function of the junction.
Ideal break junctions are superconductor - insulator - superconductor (SIS)
junctions. The tunneling current is described by
where g=g(E) and g'=g(E-eV) are the densities of states and
f=f(E) and f'=f(E-eV) are Fermi functions
[23]. The simple BCS density of
states is often modified to
where the phenomenological parameter
accounts for the pair breaking
effects[25, 26]. The continuous line in
Figure 4 was obtained by adjusting
,
and the
vertical scale factor of the differential conductance. Apart from the
elevated zero bias conductance and the upturn of conductivity at larger
bias voltages, the agreement is satisfactory. (The parameters are
meV and
meV). A more complete calculation,
including an additional leakage conductance at zero bias, and a voltage
dependent tunneling rate [27], results in an even better fit
(dashed line).
Most importantly, the Figure demonstrates that the value of the energy gap is
not sensitive to the processing of the data: the peak position of the raw
data, and the two fitting procedures yield
meV, corresponding
to
The accuracy of the results and the agreement between the two principal
spectroscopic methods (optics and tunneling) leave little doubt about the
magnitude of the low temperate energy gap in Rb
C
. The ratio
is obtained, which is clearly
beyond the weak coupling value.
This result is compatible with, although more
accurate than, most of the earlier spectroscopic studies[24], and
it agrees particularly well with the photoemission study[11]. Thus
all three direct methods (tunneling, optics and photoemission) yield
very similar values.
In early NMR measurements the absence of
the Hebel-Slichter (H-S) peak in the relaxation rate was interpreted
as an evidence for strong coupling.[12, 28] More recently,
Stenger et al. [13] observed the H-S peak, and argued that
Rb
C
is in the weak coupling regime. In particular,
was excluded as too high. However, due to the many
factors influencing the magnitude of the H-S peak, smaller values of
could not be excluded. Interestingly, Stenger et al.
puts a lower bound of 200cm
on the phonon frequency, and our result is
entirely compatible with that constraint.
Kiefl et al. determined
from muon spin rotation
experiments. The interpretation of the results is similar to the NMR
relaxation rate, except the low temperature limiting behavior is
more accessible with muons. The spin relaxation rate depends on the
number of electrons in the conduction band. For BCS superconductors
these electrons are thermally activated, thus the relaxation rates
should exhibit Arrhenius temperature dependence at low T.
This straightforward interpretation becomes rather complicated
for intermediate and strong coupling. At finite temperatures, the density of
states is non-zero at the Fermi level (unlike the BCS limit).[25]
Indeed, Kiefl et al. used a broadened density of states, such as described
in Eq. 1. The value of the gap depends on the
assumptions made for the temperature dependence of
. We believe that
in this case it is crucial to use the full Eliashberg calculation to
obtain a more reliable value for
.
Notice the contrast to the direct spectroscopic studies, where the
phenomenological parameter
does not influence the numerical magnitude of the gap in any
significant way.
The dimensionless electron - phonon coupling constant and the characteristic
phonon frequency can be determined as follows. According to Carbotte
[2], for various superconductors
can be well approximated
by
The
value determined here corresponds to
. This, in turn, leads to the dimensionless coupling constant
of
(from Eq. 2 of Allen and Dynes[1]) or a slightly
larger value if the repulsive electron electron interaction is also
considered (one obtains, for example,
for
).
Two important conclusions can be drawn from our results. First, the
coupling constant is reasonably close to the
, obtained from the DC electrical transport measurements by Vareka
and Zettl[15]. Notice that for most BCS superconductors
and
are close, but the two quantities do not have to be
equal [29]. This agreement makes Rb
C
look like one of the most
simplistic materials. We have to keep in mind, however, that with
the mean free path of the electrons is actually
shorter than the lattice spacing.
The existence of metallic
conduction with such a short mean free path remains one of the mysteries of
the transport in alkali fullerides.
The second conclusion concerns the characteristic phonon frequency. It
turns out to be
cm
, which is larger than the
typical frequency of the acoustic phonons. This result
is in agreement with the photoemission studies and calculations of Gunnarson
et al.[4],
where the low lying Raman modes of the C
molecule proved to contribute
significantly to the electron - phonon coupling.
In summary, we investigated the energy gap of the superconducting state of
Rb
C
and we demonstrated that this material
cannot be described by the (weak coupling) BCS theory. The dimensionless
electron - phonon coupling constant and the typical phonon frequency were
determined.
It is expected that the Eliashberg theory, with a coupling constant in
the order of 1, fully describes the superconductivity this material.
Acknowledgments. We are indebted to P.B. Allen for enlightening discussions, to G.P. Williams and G.L. Carr for valuable advice during the measurements at the NSLS, and to S. Lindaas and C. Jacobsen for the use of the scanning atomic force microscope. This research has been supported by the Swiss National Science Foundation, by the NSF grants DMR-9501325 and INT-9414840, and by the Hungarian National Science Foundation grant OTKA-T015552. The NSLS and the U4IR beamline is supported by the US Department of energy, under the grant DEFG-0291-ER4531.
Laszlo Mihaly
Mon Nov 11 12:38:44 EST 1996