Spin scattering in nonmagnetic semiconductorssaykin/notes/Scatt.pdf · Spin scattering is here...
Transcript of Spin scattering in nonmagnetic semiconductorssaykin/notes/Scatt.pdf · Spin scattering is here...
Spin scattering in nonmagnetic semiconductors
Spin state
( ) ↓+↑= ↓↑ ,,, kkk ϕϕψ sWave function:
( ) ( ) ⎟⎟⎠
⎞⎜⎜⎝
⎛==
↓↓↓↑
↑↓↑↑
ρρρρ
ψψρ ss ,, kk
1112
z x ys
x y z
P P iPP iP P
ρ+ −⎛ ⎞
= ⎜ ⎟+ −⎝ ⎠
Spin density matrix:
In general, it should be
Spin polarization vector:
OR
( )ss ′′ ,;,kkρUse Wigner’s functionto get
( )ss ′,;,RKρ
( )zyx PPPP ,,=r
Local spin polarization
ΔV
X
Y
Z
x0
y0
z0
Number of electrons: N=n · ΔVMagnetic moment: M=N·μB·P
X
Y
Z
PZ(t)
P1
P2
P3
P4
P5
PSpin polarization |P|≤1
X
Y
Z ω
∆P
PZ(t)
Z
Evolution of spin polarization
Spin polarization vector
( ) ⊥−−−×= PT
PPT
BPdtPd rrrrrr
20||
1
11γBloch equation:
Spin scattering is here
Today we talk about T1 processes
Interaction with magnetic fieldInteraction with magnetic field
Hz
BH gμ=− =μH SH24
B 9.27 10μ −= × J/T
Px
t
Py
t
Pz
t
tϕ ω=
x
k
k’
No scattering!Pure dephasing.
Evolution of spin polarization vector
T2* instead of T2
T1 remains the same
Spin-orbit interactionElliot-Yafet mechanism
D’yakonov-Perel mechanism
Hyperfine interaction with nuclear spins
Exchange with holes (Bir-Aronov-Pikus)
Spin scattering
No direct interaction with phonons & non-magnetic impurities.
T1 processes We have to define basis for spin ↑ and ↓.Use small magnetic field.
Spin flip vs. spin precession
↓,k
↑,'k
νhE =
Phonon
↓,k
Impurity
↑,'k
OR
Type I
Sr
kr
phononωh
Impurity
Initialstate
Finalstate
k ′r
S ′r
Type II
Electron-hole exchange
Hyperfine interaction
)(rJSδAHexch =Exchange Hamiltonian:
Important in p-type semiconductors
)()(Hf rSIr δAH =Hyperfine Hamiltonian:
Suppressed in strong magnetic fields
Hole
Electron
momentum and J can relax
Nucleus
Electron
Elliott-Yafet mechanism
Spin states: ↑,k↓,k
k
E
( )( )
3/ 2
3/ 2
," " ( ) ( )
," " ' ( ) ' ( )
i
i
k L e u v
k L e u v
−
−
↑ = ↑ + ↓
↓ = ↓ + ↑
krk k
krk k
r r
r r
mixes pure spin up and down states
" "↑
" "↓
↓,k
↑,'k
νhE =
Phonon
↓,k
Impurity
↑,'k
Any momentum scattering can result in a spin flip.
D’yakonov-Perel’ mechanism
Sr
kr
phononωh
Impurity
Initialstate
Finalstate
k ′r
S′r
)()()( 222222yxzzxzyyzyxxSO kkkkkkkkkH −+−+−= Γ σσσα
Spin-orbit interaction:
Crystals without a center of inversion
GaAs
Fe
GaAs
S
V
GaAsFe n+
n+
Α=Α=
Α=
=
Γ
eVeV
eV
eVq
X
L
B
087.027.0
28
72.03
ααα
φ
1 μm
Region is studied
D-P scattering in a device structure, example
0.0 0.2 0.4 0.6 0.8 1.0
-2.0
-1.5
-1.0
-0.5
0.0
0.5
1.0
Pote
ntia
l, V
X, μm
Potential Profile, Vds = 2 V
Model for Monte-Carlo simulation
• Spin scattering mechanism:
• Charge transport (BTE):
• Spin density matrix evolution:
CtffVqf
tf
⎟⎟⎠
⎞⎜⎜⎝
⎛=∇⋅∇−∇⋅+
∂∂
∂∂
kv )(h
( )ds
22 )( NneV −−=∇ r
ε
hh // SOSO )()( dtiHi
dtiHi etedtt ρρ −=+
)(R yxxy kkH σση −=2
D ( )z y y x xH k k kβ σ σ= < > −
ρρ
φ
=′=′
=′
−=′
zz
yy
Bxx
EE
EE
qEE
h
h
h
/2
/2
/2
*
*
*
zz
yy
xx
Emk
Emk
Emk
′±=′
′±=′
′=′
Injection Mechanisms
Bq φ
fmE
cE
fsE
xE
xE′
eVbias
• Thermionic Emission: Bx qE φ> & spin is conserved
ΦΦ−=′
=′
=′
=′
iizz
yy
x
ee
EE
EE
E
ρρ
0
• Tunneling through the Schottky barrier: Bx qE φ<
h
h
/2
/2
0
*
*
zz
yy
x
Emk
Emk
k
′±=′
′±=′
=′Bq φ
fmE
cE
fsE
xE
tpx
)( tpc xE
eVbias
)])([22exp()(0
*tp dxExEmET
tpx
xc∫ −−=h
Tunneling probability:(WKB approximation)
Injection Mechanisms
TkEETkEE
Bfm
Bfme
eEf /)(
/)( ~1
1)( −−−+
=
• Electron distribution function:
• Equal average kinetic energy in x, y and z directions
Electrons at the Ferromagnetic Contact
• Probabilities of spin states are based on the densities of states
↑↓↓↑
↑↑ −=
+= PP
EDEDED
EP 1and)()(
)()(
Spin-orbit couplings in 3 valleys of bulk GaAs
1. Γ valley (000)
2. L valleys
3. X valleys
)()()( 222222yxzzxzyyzyxxSO kkkkkkkkkH −+−+−= Γ σσσα
⎪
⎪⎩
⎪⎪⎨
⎧
+−++−++−+−−
−++−+−+−+−
=
)()()(3/)()()(3/
)()()(3/)()()(3/
yxzzxyyzxL
yxzzxyzyxL
xyzzxyzyxL
yxzxzyzyxL
SO
kkkkkkkkkkkk
kkkkkkkkkkkk
H
σσσασσσα
σσσασσσα ( 1 1 1)
(-1-1 1)
(-1 1-1)
(1-1 -1)
⎪⎩
⎪⎨
⎧
−−−
=)()()(
yyxxX
zzxxX
yyzzX
SO
kkkkkk
Hσσασσασσα (±1 1 1)
( 1±1 1)( 1 1±1)
Dresselhaus Mechanism
Carrier ConcentrationT = 300 K, V = 2 V
The extremely high electric field at the Schottky barrier pumps the electrons onto up valleys, especially the X valley
0.00 0.05 0.10 0.151E18
1E19
1E20
1E21
1E22
1E23
conc
entra
tion,
m-3
X, um
Γ valley L valley X valley
Spin dephasing is much stronger in upper valleys due stronger SO coupling
Current Spin Polarization
T = 300 K, V = 2 V
0.00 0.05 0.10 0.150.0
0.2
0.4
0.6
0.8
1.0
Cur
rent
pol
ariz
atio
n
X, μm
Γ valley L valley X valley
0.00 0.05 0.10 0.15
1E14
1E15
1E16
Con
cent
rato
in m
-3
X, um
Gamma L X valley
T = 300 K, V = 0.5 VCarrier ConcentrationLow bias
T = 300 K, V = 0.5 V
0.00 0.05 0.10 0.150.0
0.2
0.4
0.6
0.8
1.0
Cur
rent
spi
n po
lariz
atoi
n
X, um
Gamma L X
Current Spin Polarization
T = 80 K, V = 2 VLow temperature
0.00 0.05 0.10 0.151E10
1E11
1E12
1E13
1E14
1E15
co
ncen
tratio
n, m
-3
X Axis Title
Γ valley L valley X valley
Carrier Concentration
Current Spin Polarization
T = 80 K, V = 2 VLow temperature
0.00 0.05 0.10 0.150.0
0.2
0.4
0.6
0.8
1.0
Cur
rent
pol
ariz
atio
n
X, μm
Γ valley L valley X valley
Spin-LED
GaAs (001)
p-GaAs
hν
Spin Polarizing contact
n-AlGaAsGaAs QW
p-AlGaAs
M. Yasar, PhD Thesis
A0
Do
e1
h1ħω
AlGaAs(n)
GaAs
AlGaAs (p)
ħΩ
A-
++++ +
- - - - -CBVB
X/K
Spin-LED
11600 11800 12000 12200 12400 126000
1x105
2x105
3x105
4x105
5x105
6x105
7x105
Sample 1T = 6 KCB A
EL Spectra X a XBulk
EL In
tens
ity (a
rb.u
.)
Energy (cm-1)
Electroluminescence (1,0,0)
12200 12300 12400 12500 12600
0.0
5.0x104
1.0x105
1.5x105
2.0x105
Sample 1T = 6 K
EL Spectra X a XBulk
EL In
tens
ity (a
rb.u
.)
Energy (cm-1)
ΔE~84 cm-1 = TA phonon at X
R. Mallory, et. al., Phys. Rev. B 73, 115308 (2006)
-6 -4 -2 0 2 4 6-30
-20
-10
0
10
20
30
Sample 1T = 6 K
Feature X Feature a
Pola
rizat
ion
(%)
Magnetic Field (T)
11600 11800 12000 12200 12400 12600
0.0
5.0x103
1.0x104
1.5x104
2.0x104
2.5x104
Sample 3T = 6 K
EL Spectrum X a'
XBulk Bulk feature
EL In
tens
ity (a
rb.u
.)
Energy (cm-1)
Spin-LED
Electroluminescence (1,1,0)
ΔE~105 cm-1 ~ phonon at K
Questions?