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Thermal properties in mesoscopics: physics and ... - ResearchGate

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evaluated at the normal-superconduct<strong>in</strong>g <strong>in</strong>terface. Here<br />

ˆn is the unit vector normal to the <strong>in</strong>terface <strong>and</strong> µS is the<br />

chemical potential of the superconductor. The former<br />

equation guarantees the absence of charge imbalance <strong>in</strong><br />

the superconductor, while the latter describes the vanish<strong>in</strong>g<br />

energy current <strong>in</strong>to it. For E > ∆, the usual<br />

normal-metal boundary conditions are used. Note that<br />

these boundary conditions are valid as long as the resistance<br />

of the wire by far exceeds that of the <strong>in</strong>terface; <strong>in</strong><br />

the general case, one should apply Eqs. (9).<br />

Assume now a system where a normal-metal wire is<br />

placed between normal-metal (at x = L, potential µN<br />

<strong>and</strong> temperature T = Te,N) <strong>and</strong> superconduct<strong>in</strong>g reservoirs<br />

(at x = 0, µS = 0, T = Te,S). Solv<strong>in</strong>g the Boltzmann<br />

equation (3) then yields (Nagaev <strong>and</strong> Buttiker,<br />

2001)<br />

<br />

1<br />

2<br />

f(E) =<br />

<br />

x 1 + L<br />

fN (E) + 1<br />

<br />

x<br />

2 1 − ¯fN(E),<br />

L<br />

E < ∆<br />

<br />

x 1 − L feq(E; µ = 0, Te,S) + x<br />

LfN (E), E > ∆.<br />

Here fN(E) = feq(E; µN , Te,N) <strong>and</strong><br />

(44)<br />

fN(E) ¯ =<br />

feq(E; −µN, Te,N ). This function is plotted <strong>in</strong> Fig. 2<br />

(b). In the quasiequilibrium regime, the problem can<br />

be analytically solved <strong>in</strong> the case eV, kBT ≪ ∆, i.e.,<br />

when Eqs. (43) apply for all relevant energies. Then the<br />

boundary conditions are µ = µS = 0 <strong>and</strong> ˆn · ∇Te = 0<br />

at the NS <strong>in</strong>terface. Thus, the quasiequilibrium distribution<br />

function is given by f(E, x) = f(E; µ(x), Te(x))<br />

with µ(x) = µN (1 − x/L) <strong>and</strong><br />

Te(x) =<br />

<br />

T 2 e,N<br />

+ V 2<br />

L0<br />

x<br />

<br />

L<br />

2 − x<br />

L<br />

<br />

. (45)<br />

Note that this result is <strong>in</strong>dependent of the temperature<br />

Te,S of the superconduct<strong>in</strong>g term<strong>in</strong>al.<br />

In this <strong>in</strong>coherent regime, the electrical conductance is<br />

unmodified compared to its value when the superconductor<br />

is replaced by a normal-metal electrode: Andreev reflection<br />

effectively doubles both the length of the normal<br />

conductor <strong>and</strong> the conductance for a s<strong>in</strong>gle transmission<br />

channel (Beenakker, 1992), <strong>and</strong> thus the total conductance<br />

is unmodified. Wiedemann-Franz law is violated<br />

by the Andreev reflection: there is no heat current <strong>in</strong>to<br />

the superconductor at subgap energies. However, the<br />

sub-gap current <strong>in</strong>duces Joule heat<strong>in</strong>g <strong>in</strong>to the normal<br />

metal <strong>and</strong> this by far overcompensates any cool<strong>in</strong>g effect<br />

from the states above ∆ (see Fig. 5).<br />

The SNS system <strong>in</strong> the <strong>in</strong>coherent regime has also<br />

been analyzed by Bezuglyi et al. (2000) <strong>and</strong> Pierre et al.<br />

(2001). Us<strong>in</strong>g the boundary conditions <strong>in</strong> Eqs. (43) at<br />

both NS <strong>in</strong>terfaces with different potentials of the two superconductors<br />

leads to a set of recursion equations that<br />

determ<strong>in</strong>e the distribution functions for each energy. The<br />

recursion is term<strong>in</strong>ated for energies above the gap, where<br />

the distribution functions are connected simply to those<br />

of the superconductors. This process is called the multiple<br />

Andreev reflection: <strong>in</strong> a s<strong>in</strong>gle coherent process, a<br />

13<br />

quasiparticle with energy E < −∆ enter<strong>in</strong>g the normalmetal<br />

region from the left superconductor undergoes multiple<br />

Andreev reflections, <strong>and</strong> its energy is <strong>in</strong>creased by<br />

the applied voltage dur<strong>in</strong>g its traversal between the superconductors.<br />

F<strong>in</strong>ally, when it has Andreev reflected<br />

∼ (2∆/eV ) times, its energy is <strong>in</strong>creased enough to overcome<br />

the energy gap <strong>in</strong> the second superconductor. The<br />

result<strong>in</strong>g energy distribution function is a staircase pattern,<br />

<strong>and</strong> it is described <strong>in</strong> detail <strong>in</strong> (Pierre et al., 2001).<br />

The width of this distribution is approximately 2∆, <strong>and</strong><br />

it thus corresponds to extremely strong heat<strong>in</strong>g even at<br />

low applied voltages.<br />

The superconduct<strong>in</strong>g proximity effect gives rise to two<br />

types of important contributions to the electrical <strong>and</strong><br />

thermal <strong>properties</strong> of the metals <strong>in</strong> contact to the superconductors:<br />

it modifies the charge <strong>and</strong> energy diffusion<br />

constants <strong>in</strong> Eqs. (5), <strong>and</strong> allows for f<strong>in</strong>ite supercurrent<br />

to flow <strong>in</strong> the normal-metal wires.<br />

The simplest modification due to the proximity effect is<br />

a correction to the conductance <strong>in</strong> NN’S systems, where<br />

N’ is a phase-coherent wire of length L, connected to a<br />

normal <strong>and</strong> a superconduct<strong>in</strong>g reservoir via transparent<br />

contacts. In this case, jS = T an = 0 <strong>and</strong> the k<strong>in</strong>etic<br />

equation for the charge current reduces to the conservation<br />

of jT = DT ∂xf T . This can be straightforwardly<br />

<strong>in</strong>tegrated, yield<strong>in</strong>g the current<br />

<br />

I = GN/e dEf T eq(E; V )DT (E), (46)<br />

where f T eq(E; V ) = {tanh[(E + eV )/(2kBT )] − tanh[(E −<br />

eV )/(2kBT )]}/2, T is the temperature <strong>in</strong> the normalmetal<br />

reservoir, <strong>and</strong> we assumed the normal metal <strong>in</strong><br />

potential −eV . The proximity effect can be seen <strong>in</strong> the<br />

term DT = ( L<br />

0<br />

dx<br />

DT (x;E) /L)−1 . For T = 0, the differ-<br />

ential conductance is dI/dV = DT (eV )GN . A detailed<br />

<strong>in</strong>vestigation of DT (E) requires typically a numerical solution<br />

of the retarded/advanced part of the Usadel equation<br />

(Golubov et al., 1997). In general, it depends on<br />

two energy scales, the Thouless energy ET = D/L 2 of<br />

the N’ wire <strong>and</strong> the superconduct<strong>in</strong>g energy gap ∆. The<br />

behavior of the differential conductance as a function of<br />

the voltage <strong>and</strong> of the l<strong>in</strong>ear conductance as a function<br />

of the temperature are qualitatively similar, exhibit<strong>in</strong>g<br />

the reentrance effect (Charlat et al., 1996; Golubov et al.,<br />

1997; den Hartog et al., 1997): for eV, kBT ≪ ET <strong>and</strong> for<br />

max(eV, kBT ) ≫ ET , they tend to the normal-state value<br />

GN whereas for <strong>in</strong>termediate voltages/temperatures, the<br />

conductance is larger than GN , show<strong>in</strong>g a maximum for<br />

max(eV, kBT ) of the order of ET .<br />

The proximity-effect modification to the conductance<br />

can be tuned <strong>in</strong> an Andreev <strong>in</strong>terferometer, where a<br />

normal-metal wire is connected to two normal-metal<br />

reservoirs <strong>and</strong> two superconductors (Golubov et al., 1997;<br />

Nazarov <strong>and</strong> Stoof, 1996; Pothier et al., 1994). This system<br />

is schematized <strong>in</strong> the <strong>in</strong>set of Fig. 7. Due to the<br />

proximity effect, the conductance of the normal-metal<br />

wire is approximatively of the form G(φ) = GN + δG(1 +<br />

cos(φ))/2, where φ is the phase difference between the

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