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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)

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