29.01.2013 Views

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

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)

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!