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Carsten Timm: Theory of superconductivity

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Note that the external legs do not represent electronic Green functions but only indicate the states <strong>of</strong> incoming<br />

and outgoing electrons. The series is very similar to the one for the RPA susceptibility. Indeed, the effective<br />

interaction is<br />

V eff (q, iν n ) = U + Uχ +−<br />

0 (q, iν n ) U + Uχ +−<br />

0 (q, iν n ) Uχ +−<br />

0 (q, iν n ) + · · ·<br />

= U + U 2 [χ +−<br />

0 (q, iν n ) + χ +−<br />

0 (q, iν n ) Uχ +−<br />

0 (q, iν n ) + · · · ]<br />

= U + U 2 χ +−<br />

RPA (q, iν n). (12.36)<br />

Typically one goes beyond the RPA at this point by including additional diagrams. In particular, also charge<br />

fluctuations are included through the charge susceptibility and the bare Green function G 0 is replaced by a<br />

selfconsistent one incorporating the effect <strong>of</strong> spin and charge fluctuations on the electronic self-energy. This leads<br />

to the fluctuation-exchange approximation (FLEX ). One could now obtain the Cooper instability due to the FLEX<br />

effective interaction in analogy to Sec. 9.1 and use a BCS mean-field theory to describe the superconducting state.<br />

However, since the system is not in the weak-coupling limit—the typical interaction times the electronic density<br />

<strong>of</strong> states is not small—one usually employs a strong-coupling generalization <strong>of</strong> BCS theory known as Eliashberg<br />

theory. Since the effective interaction is, like the spin susceptibility, strongly peaked close to (π/a, π/a), it favors<br />

d x2 −y2-wave pairing, as we have seen.<br />

The numerical result <strong>of</strong> the FLEX for T c and for the superfluid density n s are sketched here:<br />

T c<br />

n s<br />

0 doping x<br />

The curve for T c vs. doping does not yet look like the experimentally observed dome. There are several aspects<br />

that make the region <strong>of</strong> weak doping (underdoping) difficult to treat theoretically. One is indicated in the sketch:<br />

n s is strongly reduced, which indicates that <strong>superconductivity</strong> may be in some sense fragile in this regime.<br />

Furthermore, the cuprates are nearly two-dimensional solids. In fact we have used a two-dimensional model so<br />

far. If we take this seriously, we know from chapter 7 that any mean-field theory, which Eliashberg theory with<br />

FLEX effective interaction still is, fails miserably. Instead, we expect a BKT transition at a strongly reduced<br />

critical temperature. We reinterpret the FLEX critical termperature as the mean-field termperature T MF and the<br />

FLEX superfluid density as the unrenormalized superfluid density n 0 s. We have seen in chapter 7 that the bare<br />

stiffness K 0 is proportional to n 0 s. The BKT transition temperature T c is defined by K(l → ∞) = 2/π. It is thus<br />

reduced by small n 0 s, corresponding to a small initial value K(0) ≡ K 0 . This is physically clear: Small stiffness<br />

makes it easy to create vortex-antivortex pairs. T c is <strong>of</strong> course also reduced by T MF and can never be larger than<br />

T MF . A BKT theory on top <strong>of</strong> the FLEX gives the following phase diagram, which is in qualitative agreement<br />

with experiments:<br />

T<br />

ns<br />

T MF<br />

vortex<br />

fluctuations<br />

superconductor<br />

T c<br />

0 x<br />

This scenario is consistent with the Nernst effect (an electric field measured normal to both an applied magnetic<br />

field and a temperature gradient) in underdoped cuprates, which is interpreted in terms <strong>of</strong> free vortices in a broad<br />

temperature range, which we would understand as the range from T c to T MF .<br />

128

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