Cooper pairs at room temperature 257
In the literature, one can find a fewpapers reporting superconductivity above
room temperature. The results of most of these papers represent USOs (see
Chapter 1). However, at least two works seem to report genuine results or, it is
better to say, almost genuine results (see below why). The first report presents
results of resistivity and dc magnetic susceptibility measurements performed
in a thin surface layer of the complex material Ag
x
Pb
6
CO
9
(0.7 <x<1) [64].
The data indicate that in Ag
x
Pb
6
CO
9
at 240–340 K there is a transition rem-
iniscent of a superconducting transition. The authors suggest that the crystal
structureofAg
x
Pb
6
CO
9
is quasi-one-dimensional.
The second work reports evidence for superconductivity above 600 K in
single-walled carbon nanotubes, based on transport, magnetoresistance, tun-
neling and Raman measurements [38]. The Raman measurements have been
performed on single-walled carbon nanotubes containing small amounts of the
magnetic impurity Ni:Co (≤ 1.3 %). In single-walled carbon nanotubes, the
energy gap obtained in tunneling measurements is about ∆ 100 meV [38].
As described in Chapter 3, bulk superconductivity was already observed in
single-walled carbon nanotubes at 15 K [36].
As was discussed a few moments earlier, the electron pairing occurs in some
organic materials at ∼ 550 K. Since both these materials, Ag
x
Pb
6
CO
9
and
the nanotubes, contain carbon, it is most likely that these reports present evi-
dence for electron pairing above room temperature, not for bulk superconduc-
tivity. Of course, fluctuations of phase coherence may always exist locally. On
the basis of these results, the reader can conclude once more that, for room-
temperature superconductivity, the onset of long-range phase coherence will
be the bottleneck, not the quasiparticle pairing.
3.1 Pairing energy in a room-temperature superconductor
Let us estimate the value of pairing energy in a room-temperature supercon-
ductor at T = 0. First of all, it is worth to recall that, in a superconductor, the
pairing energy (gap) ∆
p
(0), generally speaking, has no relation with a critical
temperature T
c
. The pairing energy ∆
p
(0) is proportional to T
pair
, the pairing
temperature. In conventional superconductors, ∆
p
(0) ∝ T
c
because the onset
of long-range phase coherence in the BCS-type superconductors occurs due to
the overlap of Cooper-pair wavefunctions and, therefore, T
pair
T
c
.How-
ever, in a general case, T
c
≤ T
pair
. For example, in the cuprate Bi2212 at any
doping level, 1.3T
c
<T
pair
, as shown in Fig. 6.11.
According to the fourth principle of superconductivity presented in Chap-
ter 4, the pairing energy gap must be ∆
p
(0) >
3
4
k
B
T
c
. For the case T
c
=
350 K, this condition yields ∆
p
> 23 meV. Figure 8.2 shows the pairing gap
∆
p
(0) as a function of T
pair
. In the plot, the energy scale
3
4
k
B
T marks the
lowest allowed values of ∆
p
(0) at a given temperature. It is worth noting that