5.2 Spin Transport Equations
If the spin degree of freedom of the electrons and the holes is considered, one can
write the same set of transport equations (as was mentioned in the section 5.1)
for the corresponding up(down)-spin in silicon [173, 174, 134]. In this
work the analysis for only the electron spin is discussed, as the analysis
for the holes can be perfromed in an analogous way. Thus, the acceptor
doping is neglected and the Poisson equation Equation 5.1 can be rewritten
as
| (5.15) |
where the up(down)-spin concentration is expressed as n↑(n↓). The electron
concentration n and the spin density s can be expressed as
| (5.16a) |
| (5.16b) |
5.2.1 Spin Continuity Equation
The continuity equations for the up(down)-spin electrons in the channel
including the spin-flip term [173] is revealed below. An additional electron
generation-recombination process can be neglected because the considered system
is n-doped only (unipolar).
| (5.17a) |
| (5.17b) |
Here, J↑(J↓) represents the up(down)-spin current density, τ↑↓-1 is the rate at
which up-spin flips to down-spin, and τ↓↑-1 is the rate at which down-spin flips to
up-spin. δn↑ (δn↓) represents the up(down)-spin density deviation from its
thermal equilibrium value, denoted by n↑eql(n
↓eql).
The structure under scrutiny consists of a ferromagnetic semiconductor
(FMS), which inherently has an effective spin polarization, sharing a junction
with silicon which does not. Therefore, one must introduce a non-zero bulk
spin polarization P in the FMS. The total electron concentration at the
thermal equilibrium is n = ND by considering all the dopants to be ionized.
The equilibrium up(down)-spin concentration can thus be expressed as
n↑(↓)eql = 0.5(1 + (-)P)N
D in the FMS, and n↑(↓)eql = 0.5N
D in Si. Then the
up(down)-spin and the total spin density deviation (δs) can be expressed as
The expressions for the electron (carrier) current density (Jn) and the spin
current density (Js) are given by [173]
| (5.19a) |
| (5.19b) |
One can relate the spin-flip rates τ↑↓-1 and τ
↓↑-1 with the total spin relaxation
time by using the Matthiessen rule
| (5.20) |
The continuity equation for the spin current density is obtained by subtracting
Equation 5.17b from Equation 5.17a and can be expressed as
| (5.21) |
5.2.2 Spin Drift-Diffusion
In accordance with Equation 5.14a, the up(down)-spin current density can be
expressed as
| (5.22a) |
| (5.22b) |
Here, the up(down)-spin diffusion coefficient is D↑ (D↓), and the corresponding
mobility is μ↑ (μ↓). These are related by D↑ = VT μ↑ (D↓ = VT μ↓). EC,↑ (EC,↓)
represents the conduction band edge for the up(down)-spin.
5.2.3 Discretized Form
In order to discretize the in general multi-dimensional transport equations the
following steps are used.
Poisson Equation
To solve the partial differential equations numerically, they must be discretized.
For that reason, the domain where the equations are posed has to be
partitioned into a finite number of sub-domains i, which are usually obtained by
a Voronoi tessellation. In order to obtain the solution with a desired accuracy,
the equation system is approximated in each of these sub-domains by
algebraic equations. The unknowns of this system are approximations of the
continuous solutions at the discrete grid points in the domain [182]. It has
been found to be advantageous to apply the finite boxes discretization
scheme for semiconductor device simulation [182] [185]. This method
considers the integral form of the equation for each sub-domain, which
is the so-called control volume i associated with the node the point
i.
One can rewrite the Poisson equation (c.f. Equation 5.15) by using the Gauss’
integral theorem.
| (5.23) |
where is the outward pointing local normal vector of the enclosing surface
Ã.
Finally, the discretized equation for point i with neighbor points j can be
written implicitly as
| (5.24) |
where V i(V j) is the potential at the ith(jth) node, N
D,i is the doping at the
ith node, d
i,j is the distance between ith and jth node points, and A
i,j is
the interface area between the domains i and j. is the volume of
the domain i. For a position dependent permittivity, one can use an
average, e.g. ϵij = , where () is the permittivity at the node point i
(j).
Figure 5.1: The two-dimensional representation of the Voronoi box is shown.
The domain contains the mesh point i and is surrounded by six adjacent
mesh points. Ai,j represents the boundary between the box around the ith
node and its neighbor j. di,j implies the distance between the ith and the jth
nodes.
A two-dimensional realization of the above mentioned box integration process
can be found in Figure 5.1. In this case, representes the area surrounding the ith
node, di,j represents the distance between ith and an adjacent jth node point, and
Ai,j is the interface length as shown.
Spin Continuity Equation
One can also apply the Gauss’ integral theorem to rewrite the continuity
equations Equation 5.17a and Equation 5.17b. If steady-state analysis is under
investigation, = 0. Again, in order to derive a rather simplified analytical
solution for the spin density later in this chapter to make comparisons with the
simulated results, τ↑↓ = τ↓↑ = 2τs is considered (c.f. Equation 5.20). Because each
spin flip contributes to relaxation of both up- and down-spin, the spin relaxation
becomes twice as fast.
| (5.25a) |
| (5.25b) |
Then, considering the same Voronoi box around the ith node,
| (5.26a) |
| (5.26b) |
Here, J↑,i,j (J↓,i,j) represents the up(down)-spin current density flowing from
ith to jth node. δn
↑,i (δn↓,i) represents the up(down)-spin density deviation at the
ith node.
Spin Drift-Diffusion
The Scharfetter-Gummel (SG) discretization scheme for the carrier current
density provides an optimum way to discretize the drift-diffusion equation for
particle transport [186]. This discretization scheme can be applied as well to
rewrite the expression for the up(down)-spin current densities (c.f. Equation 5.22a
and Equation 5.22b) into their discretized form. One can discretize the spin
drift-diffusion equations by following the steps as explained in [187, 183]. In the
non-degenerate transport regime, the diffusion constant, the mobility,
and the conduction band edge are spin-independent [174]. Therefore,
D↑ = D↓, μ↑ = μ↓, and EC,↑ = EC,↓. For simplicity one can assume a
homogeneous position-independent electronic conduction band edge in
the channel. Again, the bulk spin polarization P term can be inserted
in the SG discretization scheme via the expressions of n↑eql and n
↓eql.
| (5.27a) |
| (5.27b) |
with
| (5.28a) |
| (5.28b) |
Here, Pi is the bulk spin polarization at the ith node (=P for the FMS, =0 for
silicon), μn,i,j represents the average mobility between ith and jth node, and a
good approximation is μn,i,j = . The effective density of states of electrons
(NC) in ith (jth) node is represented as N
c,i (Nc,j). The average equilibrium
electron concentration (i.e. the donor concentration) between two neighboring
points i and j is represented by ND,i,j, and thus the average equilibrium
up(down)-spin concentration can be considered as 0.5ND,i,j. The expression for
the term ND,i,j is described in the next section. B denotes the Bernoulli
function
| (5.29) |
When spin transport only in a silicon bar is considered, the electron density of
states NC becomes position-independent, and thus △i,j(1) = △
i,j.
5.2.4 Transport Channel
In order to predict the impact of a space-charge layer on the spin transport in
silicon, a one-dimensional transport channel is assumed. However, the same
predictions will be valid for a multi-dimensional structure as well. The
semiconducting channel of length W contains a semiconductor ferromagnet (FMS,
-<x<0) and silicon (Si, 0<x<), sharing a junction at x=0 (c.f. Figure 5.2).
Now, to enable a violated or restored charge neutral source of spin injection in
silicon, the following two assumptions are under consideration in this
work.
- The ferromagnetic semiconductor FMS can be considered to be doped
to a concentration, which is a factor K1 of the value in Si. Thus, when
K1>1 (K1<1), one can introduce a charge accumulated (depleted)
source of spin injection into Si (c.f. text in Figure 5.2). Indeed when
K1=1, the charge neutrality condition is restored.
- One can consider a homogeneous electronic density of states in the
FMS, which is a factor K2 of the homogeneous density of states in
Si. Thus, when K2>1 (K2<1), one can introduce a charge depleted
(accumulated) source of spin injection into Si.
|
|
Parameters | Values |
|
|
Electron mobility in Si | μn=1400cm-2V-1s-1 [50] |
Donor doping in Si | ND=1016cm-3 |
Intrinsic spin diffusion length | Li=1μm [181] |
Temperature | T=300K |
Doping ratio between the ferromagnetic
semiconductor and Si | K1 |
Ratio between the electronic density of states
among the ferromagnetic semiconductor and Si | K2 |
|
|
|
Table 5.1: The simulation parameters for the spin drift-diffusion equations
are listed.
For a one-dimensional channel = , where di,j is the distance
between ith and jth nodes, and A
i,j=1. As the space-charge effect on the spin
transport is under scrutiny the charge screening length, also known as the Debye
length (λD), puts a strict limitation on the choice of the mesh size near the
interface in both the ferromagnetic and silicon sides [188]. The Debye length
relates to the measure of a charge carrier’s net electrostatic effect, and it is
the length over which the carrier density in a semiconductor changes
by a factor [189]. λD in an n-doped semiconductor can be expressed
as
| (5.30) |
where ϵSi is the silicon permittivity. The value of λD is 40nm for the parameters
listed in Table 5.1. Thus, a good approximation is to use a step value (i.e. di,j) of
10nm near the interface in this particular simulation set up. In such a
case, the node points i and j are close enough and ND,i,j =
can be considered. The mobility is assumed to be homogeneous in the
channel.