Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru
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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Andreev Billiards 141<br />
Equation (25) for the Andreev map has the same form as (22) for the Andreev<br />
billiard (with α → −i). In particular, both equations have roots that lie<br />
symmetrically around zero.<br />
A specific realization of the Andreev map is the Andreev kick<strong>ed</strong> rota<strong>to</strong>r.<br />
(See [30] for a different realization, bas<strong>ed</strong> on the kick<strong>ed</strong> Harper model.) The<br />
normal kick<strong>ed</strong> rota<strong>to</strong>r has Floquet opera<strong>to</strong>r [31]<br />
�<br />
F =exp i �τ0<br />
× exp<br />
4I0<br />
�<br />
i �τ0<br />
4I0<br />
∂2 ∂θ2 � �<br />
exp −i KI0<br />
∂ 2<br />
∂θ 2<br />
�<br />
cos θ<br />
�τ0<br />
�<br />
. (27)<br />
It describes a particle that moves freely along the unit circle (cos θ, sin θ) with<br />
moment of inertia I0 for half a period τ0, is then kick<strong>ed</strong> with a strength K cos θ,<br />
and proce<strong>ed</strong>s freely for another half period. Upon increasing K the classical<br />
dynamics varies from fully integrable (K = 0) <strong>to</strong> fully chaotic [K > ∼ 7, with<br />
Lyapunov exponent α ≈ ln(K/2)]. For K < 7 stable and unstable motion<br />
coexist (mix<strong>ed</strong> phase space). If ne<strong>ed</strong><strong>ed</strong>, a magnetic field can be introduc<strong>ed</strong><br />
in<strong>to</strong> the model as describ<strong>ed</strong> in [32].<br />
The transition from classical <strong>to</strong> quantum behavior is govern<strong>ed</strong> by the effective<br />
Planck constant heff ≡ �τ0/2πI0. For1/heff ≡ M an even integer, F<br />
can be represent<strong>ed</strong> by an M × M unitary symmetric matrix. The angular<br />
coordinate and momentum eigenvalues are θm =2πm/M and pm = �m, with<br />
m =1, 2,...M, so phase space has the <strong>to</strong>pology of a <strong>to</strong><strong>ru</strong>s. The NS interface<br />
is an annulus around the <strong>to</strong><strong>ru</strong>s, either in the θ-direction or in the p-direction.<br />
(The two configurations give equivalent results.) The const<strong>ru</strong>ction (23) produces<br />
a 2M × 2M Floquet opera<strong>to</strong>r F, which can be diagonaliz<strong>ed</strong> efficiently<br />
in O(M 2 ln M) operations [rather than O(M 3 )] by combining the Lanczos<br />
technique with the fast-Fourier-transform algorithm [33].<br />
6 Random-Matrix Theory<br />
An ensemble of isolat<strong>ed</strong> chaotic billiards, const<strong>ru</strong>ct<strong>ed</strong> by varying the shape at<br />
constant area, corresponds <strong>to</strong> an ensemble of Hamil<strong>to</strong>nians H with a particular<br />
distribution function P (H). It is convenient <strong>to</strong> think of the Hamil<strong>to</strong>nian as<br />
a random M × M Hermitian matrix, eventually sending M <strong>to</strong> infinity. The<br />
basic postulate of random-matrix theory (RMT) [9] is that the distribution is<br />
invariant under the unitary transformation H → UHU † , with U an arbitrary<br />
unitary matrix. This implies a distribution of the form<br />
P (H) ∝ exp[−Tr V (H)] . (28)<br />
If V (H) ∝ H 2 , the ensemble is call<strong>ed</strong> Gaussian. This choice simplifies some of<br />
the calculations but is not essential, because the spectral correlations become