Spin-orbit coupling and electron-phonon scattering - Fachbereich ...
Spin-orbit coupling and electron-phonon scattering - Fachbereich ...
Spin-orbit coupling and electron-phonon scattering - Fachbereich ...
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3.2 Introduction to quantum dots <strong>and</strong> various derivations 59<br />
theory. Then, we treat the charging properties by extending the theory to the<br />
few-<strong>electron</strong> case using the constant interaction model. This simple but powerful<br />
model provides a basic underst<strong>and</strong>ing of a few-<strong>electron</strong> dot <strong>and</strong> enables one to<br />
comprehend the effects of SO interaction which are reviewed later in this chapter.<br />
The one-<strong>electron</strong> spectra of a QD are well described by means of the Fock–<br />
Darwin theory. This exactly solvable model assumes a parabolically confined QD<br />
in two dimensions with perpendicular magnetic field (B = Bê z ),<br />
(<br />
p +<br />
e<br />
H 0 = c<br />
A ) 2<br />
+ m 2m 2<br />
0( ω2 x 2 + y 2) , p = (p x , p y ,0). (3.10)<br />
To underst<strong>and</strong> the effect of SO <strong>coupling</strong> which we shall present in Sec. 3.2.3, we<br />
derive the spectrum of Hamiltonian (3.10) in some detail. By choosing symmetric<br />
gauge for the vector potential, A = (−y,x,0)B/2, we can rewrite Eq. (3.10) as<br />
H 0 = p2 x + p 2 y<br />
2m<br />
+ m 2 ˜ω2( x 2 + y 2) + ω c<br />
2 (xp y − yp x ), (3.11)<br />
with ω c = eB/mc <strong>and</strong> ˜ω 2 = ω 2 0 + ω2 c/4. We now define oscillator operators,<br />
a x = √ 1 (<br />
2<br />
x˜l + i ˜l )<br />
p x , a † x = √ 1 (<br />
2<br />
x˜l − i ˜l )<br />
p x , [a i ,a † j ] = δ i j, (3.12)<br />
where ˜l = (/m˜ω) 1/2 (y-component is analogously defined). This leads to<br />
(<br />
)<br />
H 0 = ˜ω a † xa x + a † ya y + 1 + ω ( )<br />
c<br />
a y a † x − a x a † y . (3.13)<br />
2i<br />
The introduction of<br />
a ± = 2 − 1 2 (ax ∓ ia y ) (3.14)<br />
decouples x <strong>and</strong> y oscillators into eigenmodes of frequency ω ± = ˜ω ± ω c /2,<br />
(<br />
H 0 = ω + n + + 1 ) (<br />
+ ω − n − + 1 )<br />
, n ± = a †<br />
2<br />
2<br />
±a ± . (3.15)<br />
Although this representation of the Hamiltonian is convenient to discuss the effect<br />
of SO <strong>coupling</strong> in the next section, it is customary to rewrite the decoupled modes<br />
in terms of radial <strong>and</strong> angular momentum quantum numbers,<br />
n := min(n + ,n − ), l := n − − n + , (3.16)<br />
leading to a spectrum known as the Fock–Darwin states [123, 124],<br />
E nl = (2n + |l| + 1)˜ω − 1 2 l ω c. (3.17)