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Solar Cells© F.-J. Haug, ETH Zürich
Cu(InGa)Se2 solar cells
n-ZnO
glass
Mo
p-CIGS
n-CdS
Efficiencies up to 18.8% (NREL, USA), 15.7% (ETHZ)
Solar Cells© F.-J. Haug, ETH Zürich
Crystallographic properties of CIGS
Diamond (element semiconductors: Ge and Si)
Zincblende (optoelectronic materials: GaAs, InP, GaN)
Photovoltaic materials: CdTe (Zincblende)CuInSe2 (Chalcopyrite) Cu
In,GaSe
a
c
Solar Cells© F.-J. Haug, ETH Zürich
Phase diagram of CuInSe2
15 20 25 30
100
300
500
700
900
Cu [at%]
t [°C
]
α
α
α+β
α+δ
δ
β
β+δ
δ
α+Cu2Se (HT)
α+Cu2Se
Cu In
Se
In2Se3
Cu2Se
CuInSe2
CuIn3Se5CuIn5Se8
Pseudo-binary cut through ternary diagram
Device quality: Cu-poor; Cu-rich: Cu2-xSe seggregations
Fearheiley, SC, 16, p. 91
Solar Cells© F.-J. Haug, ETH Zürich
Substrate and back contact
Substrate:Soda lime glass (supply of Na)steel foils (Kovar, Invar; rough surfaces)Polyimides (Kapton, Upilex, other; poor adhesion)
Back contact:Mo (formation of MoSe2, back surface field)Cr (Na barrier)Cu (CIS Cut process)TCOs (superstrate cells, reversed configuration)
Solar Cells© F.-J. Haug, ETH Zürich
Absorber layer
CuInSe2 with Ga addition Cu(In,Ga)Se2 (CIGS)
Compound formation ~400-500°C; growth ~550°C
“one stage” process: low quality material
Cu-poor material: single phase chalcopyriteCu-rich material: Cu2-xSe segregates,
conducting (undesired), flux (large grain)
“bilayer” or “three stage” superior quality
Solar Cells© F.-J. Haug, ETH Zürich
Spectral absorption
Direct bandgap (CuInSe2) Indirect bandgap (Si) (additional phonon required)
1.0 1.5 2.0 2.5 3.0
0.0
2.0x104
4.0x104
6.0x104
8.0x104
1.0x105
1.2x105
1.4x105
1.6x105
Photon energy [eV]
Abs
orpt
ion
coef
ficie
nt [c
m-1]
CuInSe2
c-Si
1.0 1.5 2.0 2.5 3.0101
102
103
104
105
Abs
orpt
ion
coef
ficie
nt [c
m-1]
Solar Cells© F.-J. Haug, ETH Zürich
Transmission (absorber layer)
1.0 1.5 2.0 2.5 3.0 3.5 4.00
20
40
60
80
100
0.2
0.25
x=0.3
CuGa3Se5
CuIn1-xGaxSe2
CuGaSe2
Tra
nsm
issi
on [%
]
Band gap energy [eV]
1200 900 600 300
Wavelength [nm]
Bandgap depends on I/(I+III) and Ga/(Ga+In) ratio
Solar Cells© F.-J. Haug, ETH Zürich
Deposition methods
co-evaporation(Best results)
Selenisation of precursors(low cost, difficulty of complete conversion)
Vacuum Multilayers(sputtering, evaporation)
Pastes(Screen printing)
Se or H2Se
Solar Cells© F.-J. Haug, ETH Zürich
Morphology of absorber layers
Cu-rich Cu-poor
“one step”
“two step”
Solar Cells© F.-J. Haug, ETH Zürich
Band offsets
Gereference
-0.32 eV
1.04 eV1.68 eV
CuIn1-xGaxSe
-0.6 eV
1.3 eV
OVC
-1.4 eV
CdS Zn1-xMgxO
-2.7 eV
3.3 eV
2.4 eV
-0.6 eV
1.5 eV
CuInS1-xSex
Schmid et.al. SEM 41/42, p. 281Klein et.al. APL 70(19), p. 1299Minemoto et.al. JAP 89(12), p. 8327
Turcu et.al. APA 73, p. 769
Solar Cells© F.-J. Haug, ETH Zürich
Band alignment (equilibrium)
ZnO CdS
OVC
CuIn0.7Ga0.3Se
“Spike” type, ~0.2 eV
Spike <0.3 uncritical
Niemegeers et.al.APL, 67(6), p. 843
Spike <0.4 favourableMinemoto et.al.SEM, 67, p. 83
Solar Cells© F.-J. Haug, ETH Zürich
Buffer layer
Formation of pn-junction
(Historically: also front contact)
Deposition of CdS in chemical bath process (CBD)
Cd(Ac)2, (H2N)2CS (Thiourea), NH3, precipitation of CdS
Alternate:In(OH)xSy, ZnSe, ZnS; (CBD process)ZnS, ZnSe; (evaporation)Cd, Zn; (partial electrolyte treatment)
Solar Cells© F.-J. Haug, ETH Zürich
Transmission (window layer)
CdS buffer absorbs at 600 nm => reduced photocurrent
1.0 1.5 2.0 2.5 3.0 3.5 4.00
20
40
60
80
100
AM 1.5 CdS (400nm)
ITO
CdS (50nm)
ZnO
Tra
nsm
issi
on [%
]
Band gap energy [eV]
1200 900 600 300
Wavelength [nm]
Solar Cells© F.-J. Haug, ETH Zürich
Buffer layer and cell efficiency
ZnO direct
CdS/ZnO
Cd-treatment
Zn-treatment
Performance of CdS buffer layer is unsurpassed
Canava et.al.TSF 361/362, p. 187
Solar Cells© F.-J. Haug, ETH Zürich
Alternate buffers
Thickness of CdS may be reduced
ZnSe and ZnS are promising
Engelhardt et. al., PPV 7, p 423
Solar Cells© F.-J. Haug, ETH Zürich
Transmission (solar cell)
1.0 1.5 2.0 2.5 3.0 3.5 4.00
20
40
60
80
100
CdS (50nm)
ZnO
x=0.3
CuIn1-xGaxSe2
Tra
nsm
issi
on [%
]
Band gap energy [eV]
1200 900 600 300
Wavelength [nm]
Absorption in CdS does not contribute to current
Solar Cells© F.-J. Haug, ETH Zürich
Transparent conducting oxides(TCOs)
Suppress absorption in visible range => Eg>3.3 eV
Oxides: ZnO, CdO, SnO2, In2O3, (CdSnO4)
Doping: ZnO: B, Al, Ga, In; SnO2: F (FTO)
Multinary compounds: In2O3-SnO2 (ITO)
n-type
ZnO:N, ZnO:N,Ga
p-typeCuGaO2, CuInO2, SrCu2O2
Difficulty to dope p-type
Solar Cells© F.-J. Haug, ETH Zürich
Spectral response
Higher mobility in ZnO:BHigher Transmission in IRHigher current density
Hagiwara et.al, SEM 67, p. 267
Solar Cells© F.-J. Haug, ETH Zürich
Module interconnectionMo P1
CIGS P2
ZnO/CdS P3
Problem: corrosion of ZnO/Mo contact
Solar Cells© F.-J. Haug, ETH Zürich
Superstrate solar cells
Reversed structure
n-ZnO
glass
Au
p-CIGS
Challenges:•thermally stable ZnO:Al•no CdS buffer layer•no Na (ZnO diffusion barrier)
n++-ZnO:Al
Efficiencies up to 12.8% (AGU, Japan), 11.2% (ETHZ)
Prospects:•low cost encapsulation•dry processing
Solar Cells© F.-J. Haug, ETH Zürich
Flexible solar cells
Challenges:•processing on polymer•low temperature•no Na supply
Prospects:•flexibility (“wearable”)•light weight
Efficiencies up to 12.8% (ETH)
Solar Cells© F.-J. Haug, ETH Zürich
Tandem solar cells
CuInSe2 and CuGaSe2 are an ideal combination
Solar Cells© F.-J. Haug, ETH Zürich
Mechanically stacked tandem
no current matching necessary separate HT from LT processes
Top cell: 15% minimum, present CGS cell ~9% on Mo
Also: Bifacial approach
Four terminal device
Solar Cells© F.-J. Haug, ETH Zürich
Monolithically integrated tandem
“blue” absorber
p++n++ tunnel junction
“red” absorber
Two terminal device
Monolithic GaInP-GaAs cells: >30%
Disadvantage: current matching required
Solar Cells© F.-J. Haug, ETH Zürich
n++
III-V tandem solar cells
Top cell (InGaP):•blue: absorption (Eg~1.7 eV)•red: transmission
Bottom cell (GaAs):•red absorption (Eg~1.0 eV)
n
pp++
n++
np
Junction:• transparent