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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52 Rashba spin-<strong>orbit</strong> <strong>coupling</strong> in quantum dots<br />
with parabolic confinement of energy ω 0 [108],<br />
H 0 = (p + e c A)2<br />
2m<br />
+ m 2 ω2 0(x 2 + y 2 ), (3.2)<br />
where m is the effective mass of the <strong>electron</strong>. Applying a perpendicular magnetic<br />
field in the symmetric gauge, in second quantised notation we have<br />
H 0 = ˜ω(a † xa x + a † ya y + 1) + ω c<br />
2i (a ya † x − a x a † y), (3.3)<br />
with ω c ≡ eB/mc <strong>and</strong> ˜ω 2 ≡ ω 2 0 + ω2 c/4. Introduction of a ± = 2 −1/2 (a x ∓ ia y )<br />
decouples the system into eigenmodes of frequency ω ± = ˜ω ± ω c /2.<br />
We now include the Rashba interaction of Eq. (3.1), for which the <strong>coupling</strong><br />
strength α is related to the spin precession length l SO ≡ 2 /2mα. With magnetic<br />
length l B ≡ √ /mω c , we have<br />
H SO = α˜l<br />
[<br />
]<br />
γ + (a + σ + + a † +σ − ) − γ − (a − σ − + a † −σ + ) , (3.4)<br />
with coefficients γ ± ≡ 1 ± 1 2(˜l/l B<br />
) 2 <strong>and</strong> ˜l ≡ √ /m˜ω.<br />
Adding the Zeeman term, in which we take g to be negative as in InGaAs,<br />
performing a unitary rotation of the spin such that σ z → −σ z <strong>and</strong> σ ± → −σ ∓ , <strong>and</strong><br />
rescaling energies by ω 0 we arrive at the Hamiltonian<br />
H = ω + a † +a + +ω − a † −a − + 1 2 E zσ z<br />
+ l2 [<br />
]<br />
0<br />
γ − (a − σ + + a † −σ − ) − γ + (a + σ − + a † +σ + ) , (3.5)<br />
2˜l l SO<br />
where l 0 = √ /mω 0 is the confinement length of the dot <strong>and</strong> E z =|g|m/2m e (l B /l 0 ) 2<br />
is the Zeeman energy with m e the bare mass of the <strong>electron</strong>.<br />
This single-particle picture is motivated by the good agreement between Fock-<br />
Darwin theory <strong>and</strong> experiment in the non-SO case [108], <strong>and</strong> by studies which<br />
have shown that many-body effects in QDs play only a small role at the magnetic<br />
fields we consider here [101, 102, 109].<br />
We now derive an approximate form of this Hamiltonian by borrowing the<br />
observation from quantum optics that the terms preceded by γ + in Eq. (3.5) are<br />
counter-rotating, <strong>and</strong> thus negligible under the rotating-wave approximation [33]<br />
when the SO <strong>coupling</strong> is small compared to the confinement. This decouples the<br />
ω + mode from the rest of the system, giving H = ω + n + + H JC where<br />
H JC (α) = ω − a † −a − + 1 2 E zσ z + λ(a − σ + + a † −σ − ), (3.6)