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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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140 C.W.J. Beenakker<br />

A stroboscopic model of an Andreev billiard was const<strong>ru</strong>ct<strong>ed</strong> by Jacquod<br />

et al. [27], building on an existing model for open normal billiards call<strong>ed</strong> the<br />

open kick<strong>ed</strong> rota<strong>to</strong>r [28]. The Andreev kick<strong>ed</strong> rota<strong>to</strong>r possesses the same phenomenology<br />

as the Andreev billiard, but is much more tractable numerically. 3<br />

In this subsection we discuss how it is formulat<strong>ed</strong>. Some results obtain<strong>ed</strong> by<br />

this numerical method will be compar<strong>ed</strong> in subsequent sections with results<br />

obtain<strong>ed</strong> by analytical means.<br />

A compact unitary map is represent<strong>ed</strong> in quantum mechanics by the Floquet<br />

opera<strong>to</strong>r F , which gives the stroboscopic time evolution u(pτ0) =F pu(0) of an initial wave function u(0). (We set the stroboscopic period τ0 =1in<br />

most equations.) The unitary M × M matrix F has eigenvalues exp(−iεm),<br />

with the quasi-energies εm ∈ (−π, π) (measur<strong>ed</strong> in units of �/τ0). This describes<br />

the electron excitations above the Fermi level. Hole excitations below<br />

the Fermi level have Floquet opera<strong>to</strong>r F ∗ and wave function v(p) =(F∗ ) pv(0). The mean level spacing of electrons and holes separately is δ =2π/M.<br />

An electron is convert<strong>ed</strong> in<strong>to</strong> a hole by Andreev reflection at the NS interface,<br />

with phase shift −i for ε ≪ τ0∆/� [cf. (20)]. In the stroboscopic<br />

description one assumes that Andreev reflection occurs only at times which<br />

are multiples of τ0. TheN × M matrix P projects on<strong>to</strong> the NS interface. Its<br />

elements are Pnm =1ifm = n ∈{n1,n2,...nN } and Pnm = 0 otherwise. The<br />

dwell time of a quasiparticle excitation in the normal metal is τdwell = M/N,<br />

equal <strong>to</strong> the mean time between Andreev reflections.<br />

Putting all this <strong>to</strong>gether one const<strong>ru</strong>cts the quantum Andreev map from<br />

the matrix product<br />

�<br />

F 0<br />

F = P<br />

0 F ∗<br />

� �<br />

T T 1 − P P −iP P<br />

, P =<br />

−iP TP 1 − P T �<br />

. (23)<br />

P<br />

(The superscript “T” indicates the transpose of a matrix.) The particle-hole<br />

wave function Ψ =(u, v) evolves in time as Ψ(p) =F pΨ(0). The Floquet<br />

opera<strong>to</strong>r can be symmetriz<strong>ed</strong> (without changing its eigenvalues) by the unitary<br />

transformation F→P−1/2FP1/2 , with<br />

� √ �<br />

1 T 1<br />

1 − (1 − 2)P P −i<br />

P 1/2 =<br />

−i 1<br />

2<br />

√<br />

T<br />

2<br />

2 2P P<br />

√ √<br />

T 1 T 2P P 1 − (1 − 2 2)P P<br />

. (24)<br />

The quantization condition det(F −e−iε ) = 0 can be written equivalently<br />

as [27]<br />

Det [1 + S(ε)S(−ε) ∗ ]=0, (25)<br />

in terms of the N × N scattering matrix [28, 29]<br />

S(ε) =P [e −iε − F (1 − P T P )] −1 FP T . (26)<br />

3 The largest simulation <strong>to</strong> date of a two-dimensional Andreev billiard has N =30,<br />

while for the Andreev kick<strong>ed</strong> rota<strong>to</strong>r N =10 5 is within reach, cf. Fig. 24.

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