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 143<br />
the Thouless energy ET � �/τdwell. (We assume that ET is less than the gap<br />
∆ in the bulk superconduc<strong>to</strong>r.) In this context the dwell time τdwell is the<br />
mean time between Andreev reflections (being the life time of an electron or<br />
hole quasiparticle). The condition τerg ≪ τdwell of weak coupling is therefore<br />
sufficient <strong>to</strong> be able <strong>to</strong> apply RMT <strong>to</strong> the entire relevant energy range.<br />
6.1 Effective Hamil<strong>to</strong>nian<br />
The excitation energies Ep of the Andreev billiard in the discrete part of the<br />
spect<strong>ru</strong>m are the solutions of the determinantal (22), given in terms of the<br />
scattering matrix S(E) in the normal state (i.e. when the superconduc<strong>to</strong>r is<br />
replac<strong>ed</strong> by a normal metal). This equation can alternatively be written in<br />
terms of the Hamil<strong>to</strong>nian H of the isolat<strong>ed</strong> billiard and the M × N coupling<br />
matrix W that describes the N-mode point contact. The relation between S<br />
and H, W is [3, 10]<br />
�<br />
T<br />
S(E) =1− 2πiW E − H + iπW W T �−1 W. (30)<br />
The N × N matrix W T W has eigenvalues wn given by<br />
wn = Mδ<br />
π2 �<br />
2 − Γn − 2<br />
Γn<br />
� �<br />
1 − Γn , (31)<br />
where δ is the mean level spacing in the isolat<strong>ed</strong> billiard and Γn ∈ [0, 1] is<br />
the transmission probability of mode n =1, 2,...N in the point contact. For<br />
a ballistic contact, Γn = 1, while Γn ≪ 1 for a tunneling contact. Both the<br />
number of modes N and the level spacing δ refer <strong>to</strong> a single spin direction.<br />
Substituting (30) in<strong>to</strong>(22), one arrives at an alternative determinantal<br />
equation for the discrete spect<strong>ru</strong>m [37]:<br />
Det [E −H+ W(E)] = 0 , (32)<br />
�<br />
H 0<br />
H =<br />
0 −H∗ �<br />
, (33)<br />
� �<br />
π<br />
T T<br />
EWW ∆W W<br />
W(E) = √ . (34)<br />
∆2 − E2 The density of states follows from<br />
∆W W T EWW T<br />
ρ(E) =− 1<br />
π Im Tr (1 + dW/dE)(E + i0+ −H+ W) −1 . (35)<br />
In the relevant energy range E < ∼ ET ≪ ∆ the matrix W(E) becomes energy<br />
independent. The excitation energies can then be obtain<strong>ed</strong> as the eigenvalues<br />
of the effective Hamil<strong>to</strong>nian [38]<br />
�<br />
H<br />
Heff =<br />
−πWW T<br />
−πWW T −H∗ �<br />
. (36)