ece 663 so far, we looked at equilibrium charge distributions. the end result was np = n i 2 when...
TRANSCRIPT
![Page 1: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/1.jpg)
ECE 663
• So far, we looked at equilibrium charge distributions. Theend result was np = ni
2
• When the system is perturbed, the system tries to restoreitself towards equilibrium through recombination-generation
• We will calculate the steady-state rates
• This rate will be proportional to the deviation fromequilibrium, R = A(np-ni
2)
R-G processes
![Page 2: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/2.jpg)
ECE 663
h
h
Real spaceEnergy space
Direct Band-to-band recombination
Lasers, LEDs, ..
![Page 3: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/3.jpg)
ECE 663
h
h
Real spaceEnergy space
Direct excitonic recombination
Organic Solar cells, CNTs, wires (1-D systems)
![Page 4: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/4.jpg)
ECE 663
R-G for a Direct Band-gap
Conserve momentum and Energy
1. Eg = h
2. k = kphoton = 2/c
= Eg/ħc
Eg ~ 1.2 eV
k ~ 6/m << BZ = 2/a [Å]
Optical transitions almost vertical !!
![Page 5: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/5.jpg)
ECE 663
Indirect Band-gap
Since photons make vertical transitions,they won’t conserve momentum for indirect band-gaps (Si, Ge)
![Page 6: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/6.jpg)
ECE 663
Indirect Band-gap: What about phonons?
Conserve momentum and Energy
1. Ephonon = hphonon
2. k = kphonon = 2phonon/vsound
= Ephonon/ħvsound ≈ 2/a [Å]
Because they involve atomic Displacements, wavelengths arecomparable
But energy very small (~ 10-100 meV).Not sufficient
![Page 7: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/7.jpg)
ECE 663
Indirect Band-gap: Involving traps
Two step process !!
ktrap ≈ 2/a
![Page 8: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/8.jpg)
ECE 663
Phonons Phonons
Real spaceEnergy space
Indirect (Trap-assisted) recombination
Nonradiative Recombination(Ge, Si FETs, solar cells )
![Page 9: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/9.jpg)
ECE 663
Shockley-Read-Hall
![Page 10: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/10.jpg)
ECE 663
Phonon Phonon
Real spaceEnergy space
Auger Recombination
III-Vs, highly doped samples(Opposite process is impact ionization)
XX
![Page 11: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/11.jpg)
ECE 663
Real spaceEnergy space
Impact Ionization
Si, Ge, InP Lasers, FETs
X
X
![Page 12: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/12.jpg)
ECE 663
The capture process
NT = nT + pT
5 2 35 3 2
![Page 13: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/13.jpg)
ECE 663
The capture rate
Assume these c’s don’t change under bias
![Page 14: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/14.jpg)
ECE 663
Net Recombination Rates
TpTpGR
P
TnTnGR
N
pepnctp
r
nenpctn
r
(1-f)
![Page 15: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/15.jpg)
ECE 663
Net Recombination Rates
TpTpGR
P
TnTnGR
N
pepnctp
r
nenpctn
r
![Page 16: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/16.jpg)
ECE 663
Problem Solving Strategy
•Look at equilibrium
en
•Steady-state: Set rN = rP
nT
•Plug back in:
R = rN, rP
Similar
prescription
in ECE 687
toget ballistic
current,
except
R = A(n-f),
not A(np-ni
2)
![Page 17: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/17.jpg)
ECE 663
Look at Equilibrium first
Detailed Balance
![Page 18: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/18.jpg)
ECE 663
Look at Equilibrium first
rN = rP = 0
en = cnpT0n0/nT0 = cnn1
ep = cpnT0p0/pT0 = cpp1
n1 = nie(E’T-Ei)/kT
p1 = nie(Ei-E’T)/kT
Charge densities if trapspin Fermi energy
![Page 19: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/19.jpg)
ECE 663
)(
)(
1
1
pppnctp
r
nnnpctn
r
TTpGR
P
TTnGR
N
Substituting:
![Page 20: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/20.jpg)
ECE 663
Now look at steady-state
![Page 21: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/21.jpg)
ECE 663
Detailed Balance, Steady State
No net clockwise flow Steady clockwise flow
![Page 22: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/22.jpg)
ECE 663
… and TransientsUnsteady flow
![Page 23: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/23.jpg)
ECE 663
Steady State
TTT
TTpTTn
TTpPTTnN
nNp
pppncnnnpc
pppncrnnnpcr
)()(
)()(
11
11
)()( 11
1
ppcnnc
pNcnNcn
pn
TpTnT
![Page 24: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/24.jpg)
ECE 663
Steady State Recombination Rate R
• Use:
• And
• And
)(
)(
1
1
pppncr
or
nnnpcr
TTpP
TTnN
211 i
TTT
npn
nNp
)()( 11
1
ppcnnc
pNcnNcn
pn
TpTnT
![Page 25: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/25.jpg)
ECE 663
Steady State Recombination Rate R
)()( 11
2
ppnnnnp
rrRnp
iPN
Tnn Nc
1Tp
p Nc1
n1 = nie(E’T-Ei)/kT p1 = nie(Ei-E’T)/kT ci=ivth
![Page 26: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/26.jpg)
Typical #s
NT ET TN TP SN SP
Material [cm-3] [eV] [m2] [m2] [m/s] [m/s]
Si, Ge 1e13 0.0 1e-15 1e-15 0.0 0.0
III-Vs 2e16 0.4 1e-14 1e-13 0.0 0.0
![Page 27: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/27.jpg)
ECE 663
Let’s look at a few limits
n = n0 + n, n << n0
p = p0 + p, p << p0 << n0
Low-level injection, n-type material
n ~ pFew traps
Deep traps (midgap) n1 ≈ p1 ≈ ni
![Page 28: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/28.jpg)
ECE 663
Low level injection
)()())((
)()(
1010
200
11
2
pppnnnnppnn
R
ppnnnnp
R
np
i
np
i
• Set n0p0 = ni2 cancels term in numerator
• Drop np term in numerator• n0p >> p0n in numerator for n-type material• Keep only n0 related term in denominator
![Page 29: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/29.jpg)
ECE 663
• For n-type:
• For p-type
p
pR
n
nR
Low level injection
We’ll frequently adopt this approximation
![Page 30: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/30.jpg)
ECE 663
Surface Recombination
Lattice periodicity broken at surface/interface – mid-gap E levelsCarriers generated-recombined per unit area
![Page 31: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/31.jpg)
ECE 663
Surface States
Reconstruction
Expt (Akiyama et al, PRB 2000) Theory (Rakshit/Liang/Ghosh/Hersam/Datta, PRB 2005)
![Page 32: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/32.jpg)
ECE 663
• Processes and descriptions analogous to bulk R-G using surface parameters
• For a single energy level surface state:
)(
)(
1
1
pppncr
nnnpcr
TTpP
TTnN
)(
)(
1
1
sTsssTpsPs
sTssTsnsNs
pppncr
nnnpcr
kTEEi
kTEEi
Ti
iT
epp
enn/)(
1
/)(1
'
'
kTEE
i
kTEEis
ITi
iIT
epp
enn/)(
1
/)(1
'
'
)()( 11
2
ppnnnnp
Rnp
i
)(1
)(1
11
2
ssn
ssp
iss
pps
nns
npnR
Surface Recombination
![Page 33: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/33.jpg)
ECE 663
Surface Recombination
)(1
)(1
11
2
ssn
ssp
iss
pps
nns
npnR
CAVEAT !! sn and sp have units of length/time – surface recombination velocity for single level surface states
Tsnsn Ncs Tspsp Ncs
![Page 34: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/34.jpg)
ECE 663
Multi-Level (more realistic)
DIT(E) – density of interface traps (per unit area-energy)DIT(E)dE – density of IT between E and E+dE (replaces NTs)
dEEDpp
cnn
c
npnR IT
E
Ess
nsss
ps
issC
V
)()(
1)(
111
2
![Page 35: ECE 663 So far, we looked at equilibrium charge distributions. The end result was np = n i 2 When the system is perturbed, the system tries to restore](https://reader035.vdocuments.site/reader035/viewer/2022062717/56649e4c5503460f94b41e74/html5/thumbnails/35.jpg)
In summary• R-G processes drive system towards equilibrium
R (np – ni2)
(In ECE687, restoration will be driven by the contacts)
• For indirect band-gap materials, SRH dominates
• Coeffs depend on minority carrier lifetime, a critical concept for this course
• Minority carrier lifetime depends on trap cross-section (size), trap density and electron thermal velocity
• When computing current, the drive forces (drift-diffusion) in the next chapter will be countered by these RG forces