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Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru

Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru

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4 Scattering Formulation<br />

Andreev Billiards 137<br />

In the step-function model (6) the excitation spect<strong>ru</strong>m of the coupl<strong>ed</strong> electronhole<br />

quasiparticles can be express<strong>ed</strong> entirely in terms of the scattering matrix<br />

of normal electrons [24].<br />

The scattering geometry is illustrat<strong>ed</strong> in Fig. 4. It consists of a finite<br />

normal-metal region N adjacent <strong>to</strong> a semi-infinite superconducting region S.<br />

The metal region represents the Andreev billiard. To obtain a well-defin<strong>ed</strong><br />

scattering problem we insert an ideal (impurity-free) normal lead between N<br />

and S. We assume that the only scattering in the superconduc<strong>to</strong>r consists of<br />

Andreev reflection at the NS interface (no disorder in S). The superconduc<strong>to</strong>r<br />

may then also be represent<strong>ed</strong> by an ideal lead. We choose a coordinate system<br />

so that the normal and superconducting leads lie along the x-axis, with the<br />

interface at x =0.<br />

S N<br />

0<br />

x<br />

c- e<br />

ch<br />

+<br />

c e + ch -<br />

Fig. 4. Normal metal (N) containing an Andreev billiard, coupl<strong>ed</strong> <strong>to</strong> a superconduc<strong>to</strong>r<br />

(S) by an ideal lead. The dash<strong>ed</strong> line represents the NS interface. Scattering<br />

) are indicat<strong>ed</strong> schematically<br />

states c in =(c + e ,c −<br />

h )andcout =(c − e ,c +<br />

h<br />

We first const<strong>ru</strong>ct a basis for the scattering matrix. In the normal lead N<br />

the eigenfunctions of the BdG equation (1) can be written in the form<br />

Ψ ± � �<br />

n,e(N) =<br />

10 1<br />

�k Φn(y, z)exp(±ik<br />

e<br />

n<br />

e nx) , (10a)<br />

Ψ ±<br />

� �<br />

n,h (N) =<br />

01 1<br />

�k Φn(y, z)exp(±ik<br />

h<br />

n<br />

h nx) , (10b)<br />

where the wavenumbers k e n and k h n are given by<br />

k e,h<br />

n =<br />

√ 2m<br />

� (EF − En + σ e,h E) 1/2 , (11)

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