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

Chapter 2: Spin Dynamics: Overview and Analysis of 2D Systems 17
S y
0.5 0 0.5
0.5
0.5
0
0
S z
154L SO 2
x
154L SO
Figure 2.4: The spin density for linear Rashba coupling which is a solution of the spin
diffusion equation with the relaxation rate 7/16τ s . The spin points initially in the x − y-
plane in the direction (1,1,0).
over all currents in its vicinity which are directed towards that position. Thus, j(r,t) =
〈vρ(r−∆x)〉 where an angular average over all possible directions of the velocity v is taken.
Expandingin∆x = l e v/v, andnotingthat〈vρ(r)〉 = 0, onegets j(r,t) = 〈v(−∆x)∇ρ(r)〉 =
−(v F l e /2)∇ρ(r) = −D e ∇ρ(r). For the classical spin diffusion current of spin component S i ,
as defined by j Si (r,t) = vS i (r,t), there is the complication that the spin keeps precessing
as it moves from r −∆x to r, and that the spin-orbit field changes its direction with the
direction of the electron velocity v. Therefore, the 0-th order term in the expansion in ∆x
does not vanish, rather, we get
j Si (r,t) = 〈vS k i (r,t)〉−D e∇S i (r,t), (2.25)
where Si k is the part of the spin density which evolved from the spin density at r − ∆x
moving with velocity v and momentum k. Noting that the spin precession on ballistic scales
t ≤ τ is governed by the Bloch equation, Eq.(2.17), we find by integration of Eq.(2.17),
that Si k = −τ [B SO (k)×S] i
so that we can rewrite the first term yielding the total spin
diffusion current as
j Si = −τ〈v F [B SO (k)×S] i
〉−D e ∇S i . (2.26)
Thus, we can rewrite the spin diffusion equation in terms of this spin diffusion current and