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Itinerant Spin Dynamics in Structures of ... - Jacobs University

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Chapter 5: <strong>Sp<strong>in</strong></strong> Hall Effect 91<br />

as soon as the system size L exceeds the elastic mean free path l e . In the case <strong>of</strong> δ-<br />

function potential and pure l<strong>in</strong>ear Rashba SOC <strong>in</strong> the thermodynamic limit this result is<br />

even <strong>in</strong>dependent<strong>of</strong> theimpurity strength, as discovered by Schwab andRaimondi[RS05] by<br />

us<strong>in</strong>gselfconsistentBornapproximation: Thevertex correction <strong>in</strong>theladderapproximation<br />

cancel exactly the term com<strong>in</strong>g from the one-loop part. Follow<strong>in</strong>g Rashba, Ref.[Ras04], this<br />

can be understood as follows: Correspond<strong>in</strong>g to Eq.(5.10) and Eq.(5.22) we have, at low<br />

fill<strong>in</strong>g, positive contribution to σ SH due to <strong>in</strong>terbranch transitions between the occupied<br />

(E + ) and unoccupied (E − ) states. Add<strong>in</strong>g a perturbation by apply<strong>in</strong>g an <strong>in</strong>f<strong>in</strong>itesimal<br />

small magnetic field, <strong>in</strong>trabranch transitions at the Fermi energy give rise to a negative<br />

contribution. Surpris<strong>in</strong>gly, this additional contribution cancels the first and we are left<br />

with zero SHC. This counter<strong>in</strong>tuitive f<strong>in</strong>d<strong>in</strong>g led to several controversies because the first<br />

numerical calculations <strong>in</strong> this field showed f<strong>in</strong>ite SHC when extrapolated to <strong>in</strong>f<strong>in</strong>ite large<br />

samples[NSJ + 05]. However, new numerical results, e.g. Ref.[NSJ + 06] as an erratum to<br />

Ref.[NSJ + 05], showed agreement with the analytical predictions. In contrast, tak<strong>in</strong>g <strong>in</strong>to<br />

account also sp<strong>in</strong>-orbit terms which are cubic <strong>in</strong> momentum, as they are present <strong>in</strong> any<br />

system with broken <strong>in</strong>version symmetry (cubic Dresselhaus terms), or <strong>in</strong> quantum wells<br />

with strongly asymmetric conf<strong>in</strong>ement (cubic Rashba terms), the sp<strong>in</strong> Hall conductance<br />

has a quite universal value, <strong>of</strong> σ SH = Ne 2 /(8π), where N is the number <strong>of</strong> times the sp<strong>in</strong>orbit<br />

field B SO (k) w<strong>in</strong>ds around a circle, as the momentum is moved once around the Fermi<br />

surface[Sch06].<br />

Resonant Impurities<br />

The effect <strong>of</strong> resonant impurities and <strong>of</strong> magnetic impurities on the SHC has<br />

not been studied yet <strong>in</strong> that detail[LX06, WLZ07a]. Especially, it is unclear how large<br />

its magnitude is, when the Fermi energy is <strong>in</strong> the vic<strong>in</strong>ity <strong>of</strong> the resonant levels close to<br />

the metal-<strong>in</strong>sulator transition, where it has been observed that the sp<strong>in</strong> relaxation rate is<br />

m<strong>in</strong>imal[DKK + 02], mak<strong>in</strong>g it a potentially attractive regime for sp<strong>in</strong>tronic applications.<br />

In the follow<strong>in</strong>g we analyze the reduction <strong>of</strong> the SHC <strong>in</strong> a f<strong>in</strong>ite system with periodic<br />

boundary conditions <strong>in</strong> presence <strong>of</strong> non-magnetic impurities <strong>of</strong> b<strong>in</strong>ary type, i.e. on-site<br />

potential V i = p i V where p i = 1 for impurity sites and p i = 0 otherwise. The lattice is<br />

assumed to be contam<strong>in</strong>ated with 10% <strong>of</strong> impurities. To have a better understand<strong>in</strong>g <strong>of</strong><br />

how the SHC changes with the strength <strong>of</strong> impurities, V, we first calculate the DOS. The

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