4.2 Spin Hot Spots and Spin Precession
As the spin hot spot condition is characterized by a strong increase of the mixing
of the up- and down-spin states, the equivalent subband splitting at the spin hot
spots is purely determined by the effective spin-orbit term, which is in turn linear
with △SO, where kx and ky are the components of the in-plane electron
wave vector. This linear dependence of the splitting is similar to the Zeeman
splitting in a magnetic field [152]. Therefore, the spin-orbit interaction term
△SO with =(kx, -ky) can be interpreted as an effective magnetic field
known as spin-orbit field (SOF), while the pairs of states (X1, ↑), (X2′,
↓) and (X2′, ↑), (X1, ↓) it couples have similarities with the Zeeman
up- and down-spin states split because of the effective field [152]. It is
now obvious that the angle ϕ1 defined in the section 3.4 represents the
direction of the SOF. The spin injection orientation impacts the spin
precession at the spin hot spots and some of the related effects are now
studied.
4.2.1 Spin Expectation Value
One can estimate the spin expectations which depend on the spin injection
orientation. The spin Pauli matrices for the two [001] valleys can be written as,
Now one can express the expectation values of the spin projection on the
coordinate axes, denoted as (n=1,2 and p ∈ x,y,z),
| (4.7) |
The total spin expectation can be represented as,
| (4.8) |
When spin is injected along OZ-axis (Θ=0), ==0 but =1. It
is spotted that at spin hot spots, the value also drops to zero. When spin is
injected along OX-axis (Θ = , Φ=0), ==0 but =1. On the
contrary at the spin hot spots [153, 154],
thus making = sin arctan . When spin is injected along an
arbitrary direction on the XZ-plane, one can obtain at the spin hot spots,
and hence
| (4.11) |