Solar Photovoltaics & Energy Systems · Summary: Organic Semiconductors... have a huge potential...
Transcript of Solar Photovoltaics & Energy Systems · Summary: Organic Semiconductors... have a huge potential...
Solar Photovoltaics & Energy SystemsLecture 6. Emerging Technologies
ChE-600
Wolfgang Tress, May 2016
1
Energy Payback Time (EPBT)
2
Record Efficiencies
3
NREL Chart
4
Organic Solar Cells
5https://3dprint.com
10..100 nm
Steps of Energy Conversion
[1] Tang, Appl. Phys. Lett. 48, 183 (1986)[2] Hiramoto et al. Appl. Phys. Lett. 58, 1062 (1991)[3] B. Maennig et al., Appl. Phys. A 79, 1 (2004)
Steps of energy conversion
Exciton generation via light absorption
Exciton migration (diffusion)
Exciton separation and dissociation
Charge carrier transport
Charge carrier collection/injection
[3]
Donor Acceptor
energy
-
+
-
-
+
electrode
electrode
Challenges
• Disorder, poor charge transport
• Excited states hard to split
• Low fill factor
• High recombination, low voltage
• Narrow absorption, but broad onset
• Low long-term stability
6
Bulk Heterojunction: Morphology
• Tune amount of mixing/demixing
• Energy vs. entropy
• Annealing
• Solvents
7
TEM tomography
Nano Lett., 2009, 9 (2), pp 853–855 DOI: 10.1021/nl803676e
Absorption and EQE
8
• Narrow absorption bands
EQE and JV-curve
9
Jph depends on voltage
Charge collection problem
Reduces fill factor
p-HTL
n-ETL
Light Management
10
Thin film optics: interference
Beer-Lambert law does not apply
Meta
l
HTL
D:A
ETL
ITO
Meta
l
HTL
D:A
ETL
50 nm
Microcavity and Plasmonics:Marc Schiffler
p-HTL
n-ETL
Tandem Solar Cells
• Current matching
11
How to Increase Current and Voltage
12
EFn
EFp
eVoc
+
-
“HOMO”
“LUMO”
E
+
-
EgDA
Donor Acceptor
Current: Low band gap materials Broad absorption spectra Complementary
absorption of donor and acceptor
push-pull molecules
Voltage: Reduce “offset” energies Combination of donor
and acceptor Decrease recombination
Tuning Absorption in Polymers
13
Working Principle and Role of Contacts
14
→ Provide built-in potential due to difference in work functions
E
+
-
HTL Donor Acceptor Al
HTL = hole
transport layer
Energy diagrams at short circuit:
ITO Donor Acceptor Al
+
-
EVac
EF
HTL Donor Acceptor Al
+
-
Donor Acceptor
EVac
WF
anode
EF
WF
cathode
EF
Model-system
Flat vs. Bulk Heterojunction
15
→ Build selective device!
E
+
-
HTL Donor Acceptor Al
+
-
HTL Donor Acceptor Al
EVac
HTL = hole
transport layer
Energy diagrams at short circuit:
+
-
Acceptor 40 nm
Donor 8 nm
D:A 30 nm
diffusion
recombination
blocked
HTL Donor:Acceptor Al
no changes of Voc
decrease of Voc
Missaligned contacts → S-Shape
Geminate Recombination
Donor Acceptor
-
+
-
-
+
electrode
electrode
Geminate recombination
+
-
Non-geminaterecombination
16
Charge Transfer States: hot, (de)localized?
Donor Acceptor
-
+
-
-
+
electrode
electrode
Coulombically bound?
hot
energy
Vandewal et al. Nature Materials 2014
17
Charge Transfer State: Delocalized?
18
Compare to TD DFT simulations
In collaboration with U. Roethlisberger, EPFL
1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9
10-4
10-3
10-2
10-1
100
energy / eV
EQ
E F
TP
S s
cale
d
ZnPc
1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9
10-4
10-3
10-2
10-1
100
energy / eV
EQ
E F
TP
S s
cale
d
0.0 : 2.0 : 3
ZnPc
ZnF4Pc:ZnPc:C
60
Charge Transfer State and Voc
19
Charge-transferabsorption
Donor absorption
𝑉oc,rad = 1.0 V
𝑉oc,rad = 1.2 V
𝐽ph = 𝑒 EQE 𝐸 𝛷AM1,5g 𝐸 𝑑𝐸
𝑉oc,rad =𝑘B𝑇
𝑒ln
𝐽ph
𝐽em,0+ 1
𝐽em,0 = 𝑒 EQE 𝐸 𝜙BB 𝑇0 𝑑𝐸
State-of-the-Art Efficiencies
• Single junction η > 11 %
• Triple η > 13 %20
Fullerene free
Jsc = 16 mA/cm2
Fabrication
• Low-Cost: Roll-to-roll
• Printing
• Slot die coating
• Evaporation
21
popupcity.net
penscetriaru.5hark.net
https://www.tu-ilmenau.de/
Organic Photovoltaics State of the Art
Building integrated, Flexible, Colorful, Semitransparent
Record 13.2 %
o Stability
- In module ? %
- Not really in market yet
- Efficiency
22
Future Applications
23
Pictures: heliatek and Konarka
Summary: Organic Semiconductors
... have a huge potential• low cost roll to roll and solution processability• large area and ultra-thin devices• variety of different hydrocarbons
… are well suited for solar cells• low energy input• different dyes• abundant
… are different• film consists of weakly bound molecules• mostly amorphous and even intermixed films• optical excitation is localized• charge transport occurs mainly via hopping• optical and electrical gap decoupled
24
Dye-Sensitized Solar Cells
25
www.asknature.org
Dye-Sensitized Solar Cell: Ingredients
26Hardin, Slideshare
Dye-Sensitized Solar Cell: Schematics
• Absorption on monolayer of dye, decoupled from transport
• Meso or nanostructure increased surface area27
Dye-Sensitized Solar Cell: Energetics
• Redox potential of electrolyte fixed28
Maçaira, J., Andrade, L. & Mendes, A. Modeling, simulation and design of dye sensitized solar cells. RSC Adv. 4, 2830–2844 (2013).
History and State of the Art
29
• 1980s sensitization of TiO2
• 1991 Nature paper: η = 7 %
• Solid state DSC
• Now: η = 13 %
• Dye with designated (broad or IR) spectrum
• Electrolyte for high voltage (I Co)
Applications
30
www.connect-green.com
• Consumer: indoor?
• Building integrated
• Challenges: Efficiency, Stability, Upscaling
Is there room for further technologies?
31
Perovskite Solar Cells
32http://cleantechnica.com
What is Perovskite?
• 1839: perovskite = CaTiO3 discovered
• 1958: CsPbX3 (X = Cl, Br, or I) perovskite structure determined
• 1978 Cs cation replaced by methylammoniumcations CH3NH3
+ organic–inorganic hybrid
perovskites
• Last two decades: perovskite researched in electronics
Møller, C. K. Nature 182, 1436 (1958).
Mitzi, D. B. Synthesis, Structure and Properties of Organic–Inorganic Perovskites and Related Materials: Progress in Inorganic Chemistry Vol. 48 (ed. Karlin, K. D.) 1–121 (J. Wiley & Sons, 1999).
Ishihara, T. Optical properties of PbI-based perovskite structures. Journal of Luminescence 60–61, 269–274 (1994).
33
Weber, D. Z. Naturforsch. 33b, 1443–1445 (1978). Weber, D. Z. Naturforsch. 33b, 862–865 (1978).
History
1. Perovskite replaces dye
Solution processing route on TiO2
2009 2012 2013 2014 2015
Miyasaka, Park, Graetzel, Snaith, Seok, Bolink …
Fabrication:PbI2 + CH3NH3I
3.5 %6.5 %
12 %15 %
20 %
16 %18 %
34
The First Solar Cells
• perovskite replaces the molecular sensitizer in dye sensitized solar cell (DSSC)
• unstable (10 minutes operation), dissolves in liquid electrolyte
35
Kojima, A., Teshima, K., Shirai, Y. & Miyasaka, T. Organometal Halide Perovskites as Visible-Light Sensitizers for Photovoltaic Cells. J. Am. Chem. Soc. 131, 6050–6051 (2009).
CH3NH3PbI3
CH3NH3PbBr3
3.8 %2009
Structure of dye-sensitized solar cell
CH3NH3Pb-Halide as Pigment in DSSC
36
Im, J.-H., Lee, C.-R., Lee, J.-W., Park, S.-W. & Park, N.-G. 6.5% efficient perovskite quantum-dot-sensitized solar cell. Nanoscale 3, 4088–4093 (2011).
CH3NH3PbI36.5 %
2011
• perovskite replaces the molecular sensitizer in dye sensitized solar cell (DSSC)
• unstable (10 minutes operation), dissolves in liquid electrolyte
History
37
1. Perovskite replaces dye
2. Solid state device
Solution processing route on TiO2
2009 2012 2013 2014 2015
Miyasaka, Park, Graetzel, Snaith, Seok, Bolink …
Fabrication:PbI2 + CH3NH3I
3.5 %6.5 %
12 %15 %
20 %
16 %18 %
3. Sequential deposition
Sequential Deposition
• Better control of crystal morphology and conformal coating
• Tuning of dipping time, concentration, solvent, temperature etc.
• Correlation of perovskite loading, conversion and thickness
Use of a two-step technique to form the hybrid perovskite:
38
Burschka, J. et al. Sequential deposition as a route to high-performance perovskite-sensitized solar cells. Nature 499, 316–319 (2013)
PbI2 + CH3NH3I CH3NH3PbI3
Cross Sectional SEM
P
i
nanocomposite
n
39
Burschka, J. et al. Sequential deposition as a route to high-performance perovskite-sensitized solar cells. Nature 499, 316–319 (2013).
sublimation in vacuum
History
40
1. Perovskite replaces dye
2. Solid state device
4. Solvent engineering
5. Composition engineering
Solution processing route on TiO2
2009 2012 2013 2014 2015
Miyasaka, Park, Graetzel, Snaith, Seok, Bolink …
Fabrication:PbI2 + CH3NH3I
3.5 %6.5 %
12 %15 %
20 %
16 %18 %
Co
mp
act
film
s w
ith
larg
e cr
ysta
ls
planar architectures
3. Sequential deposition
CH3NH3PbI3: A Good Solar Cell Material
*Stranks, S. D. et al. Electron-Hole Diffusion Lengths Exceeding 1 Micrometer in an Organometal Trihalide PerovskiteAbsorber. Science 342, 341–344 (2013); Xing, G. et al. Long-Range Balanced Electron- and Hole-Transport Lengths in Organic-Inorganic CH3NH3PbI3. Science 342, 344–347 (2013).
• High crystallinity• Absorption coefficient of 104 … 105 cm-1
• Band gap of 1.6 eV, valence band edge at -5.4 eV • Ambipolar semiconductor with high charge carrier mobilities*• Wannier excitons with fast dissociation at room temperature, high dielectric
constant• Low defect density, even if solution processed• Characterized in stacks similar to solar cells many intrinsic parameters and
influence of morphology and grain boundaries not extensively quantified
41
Goldschmidt Tolerance Factor
t = 0.89–1.0 cubic structure
t = 0.8-1.0 3 D perovskite
42
ABX3
NATURE PHOTONICS DOI: 10.1038/NPHOTON.2014.134
MA: methylammonium (CH3NH3+)
EA: ethylammonium (CH3CH2NH3+)
FA: formamidinium (NH2CH=NH2+)
Band Gap Engineering
Valence band formed by orbitals from B and X43
http://onlinelibrary.wiley.com/doi/10.1002/smll.201402767/full#smll201402767-fig-0002
Certification
44
PCE of 21 %> 1.1 V
19.5 % on 1 cm2
Luminescence and Open-Circuit Voltage
• If there is absorption, there will be emission.
• The solar cell in the dark is in thermal equilibrium with its surroundings,
meaning that it absorbs and thus emits:
𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸
Emission spectrum can be predicted from absorption
45
absorber Black body emitter at 300 K
0 0.2 0.4 0.60
1
2
3
4
x 1023
energy /eV
photo
n flu
x / m
-2 s
-1
Black body radiation at T = 300 K
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d s
pe
ctr
al p
ho
ton
flu
x
1.5 1.6 1.7 1.80
0.5
1
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d E
QE
PV
experimental data
model
experimental data
model T = 320 K
model T = 300 K
model T = 350 K
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d s
pe
ctr
al p
ho
ton
flu
x
1.5 1.6 1.7 1.80
0.5
1
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d E
QE
PV
experimental data
model T = 320 K
model T = 300 K
model T = 350 K
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d s
pe
ctr
al p
ho
ton
flu
x
1.5 1.6 1.7 1.80
0.5
1
1.5 1.55 1.6 1.65 1.7 1.75 1.8
10-3
10-2
10-1
100
energy / eV
no
rma
lize
d E
QE
PV
experimental data
model T = 320 K
model T = 300 K
model T = 350 K
Spectra of Perovskite Device
46
Tress, W. et al. Predicting the Open-Circuit Voltage of CH3NH3PbI3 Perovskite Solar Cells Using Electroluminescence and Photovoltaic Quantum Efficiency Spectra: the Role of Radiative and Non-Radiative Recombination. Adv. Energy Mater. (2015). doi:10.1002/aenm.201400812
emission EQE ∝ absorption
Steep absorption onset, Urbach energy of approx. 15 meV
Luminescence and Open-Circuit Voltage
• If there is absorption, there will be emission.
• The solar cell in the dark is in thermal equilibrium with its surroundings,
meaning that it absorbs and thus emits:
𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸
Emission spectrum can be predicted from absorption
• Under illumination (thermodynamic limit):
𝑉oc,rad =𝑘B𝑇
𝑒ln
𝐽ph
𝐽em,0+ 1
47
𝑒 𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸 𝑑𝐸
Rau, U. Reciprocity relation between photovoltaic quantum efficiency and electroluminescent emission of solar cells. Phys. Rev. B 76, 085303 (2007).
1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9
10-3
10-2
10-1
100
energy / eV
scale
d E
QE
PV
Compared to Organics
Steeper absorption onset higher Voc
Charge-transfer-state absorption
Donor (ZnPc)absorption
𝑉oc,rad = 1.0 V
𝑉oc,rad = 1.2 V
𝑉oc,rad = 1.33 V
48
Shockley Queisser Limit
In theory:
CH3NH3PbI3 can reach 30 %
49
0.5 1 1.5 2 2.5 3 3.5 4 4.50
5
10
15
20
25
30
35
bandgap Eg [eV]
eff
icie
ncy
[%
]
(c)
SiGaAs
CIGS perovskite
0 0.2 0.4 0.6 0.8 1 1.2
-25
-20
-15
-10
-5
0
5
10
voltage [V]
cu
rre
nt d
en
sity [m
A / c
m 2]
0 0.2 0.4 0.6 0.8 1 1.2
-60
-40
-20
0
20
extr
acta
ble
po
we
r [m
W/c
m2]
(a)
Eg = 1.6 eV
VOC
= 1.32 V
JSC
= 25 mA/cm2
FF = 90.5 % = 30 %
MPP
𝑉oc =𝐸g
𝑒−𝑘B𝑇
𝑒ln
𝑁𝐶𝑁𝑉
𝑛𝑝
𝜂 = 𝑉oc𝐽scFF
𝑉oc
𝐽sc
Luminescence and Open-Circuit Voltage
• If there is absorption, there will be emission.
• The solar cell in the dark is in thermal equilibrium with its surroundings, meaning that it absorbs and thus emits:
𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸
Emission spectrum can be predicted from absorption
• Under illumination (thermodynamic limit):
𝑉oc,rad =𝑘B𝑇
𝑒ln
𝐽ph
𝐽em,0+ 1
50
𝑒 𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸 𝑑𝐸
Rau, U. Reciprocity relation between photovoltaic quantum efficiency and electroluminescent emission of solar cells. Phys. Rev. B 76, 085303 (2007).
Recombination
-
+
Φem
-
+
-
via defects (SRH type)
trap
CB
VB
Au
-
at surfaces (wrong electrode)
radiativeelectron-hole
-
+
CB
VB
Auger recombination
-
non-radiative recombination
enters thermodynamic
limit
pure, defect-free material
passivation, reduction of contact area
material property (indirect
semiconductor)
51
to be avoidedunavoidable in absorber
Luminescence and Open-Circuit Voltage
• If there is absorption, there will be emission.
• The solar cell in the dark is in thermal equilibrium with its surroundings, meaning that it absorbs and thus emits:
𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸
Emission spectrum can be predicted from absorption
• Under illumination (thermodynamic limit):
𝑉oc,rad =𝑘B𝑇
𝑒ln
𝐽ph
𝐽em,0+ 1
𝑉oc,real=𝑘B𝑇
𝑒ln EQEEL
𝐽ph
𝐽0+ 1
52
𝑒 𝑎 𝐸 𝛷BB 𝑇 = 300K, 𝐸 𝑑𝐸
solarcell
light
operate as LED
EQEEL =
Rau, U. Reciprocity relation between photovoltaic quantum efficiency and electroluminescent emission of solar cells. Phys. Rev. B 76, 085303 (2007).
Driving the solar cell as LED
EL reaches 0.5 %, non-rad. recombination dominant
53
JV curve in the dark, emitted photon flux and the resulting quantum efficiency of EL
𝐽inj = 𝐽0 exp𝑒𝑉
𝒏 𝑘B𝑇− 1
Bi, D. et al. Efficient luminescent solar cells based on tailored mixed-cation perovskites. Science Advances 2, e1501170 (2016).
Arun Paraecattil
ideality factor
Recombination Mechanisms
54
𝑉oc =𝐸g
𝑒−𝑘B𝑇
𝑒ln
𝑁𝐶𝑁𝑉
𝑛𝑝
𝛽𝑛𝑝
𝐺0 = 𝛼 𝐸 𝛷BB 𝐸 𝑑𝐸 = 𝛽𝑛0𝑝0 = 𝛽𝑛i2
𝛽 ≈ 10−11cm3s−1
radiativeelectron-hole
-
+
Φem
-
+
-
via defects (SRH type)
trap
CB
VB
n = 1 n = 2
𝑘𝑛 =1
𝜏𝑛
𝑑𝑛
𝑑𝑡= −𝛽𝑛2(𝑡) −
1
𝜏𝑛(𝑡)
Ideally:
Measure Recombination Rates
Long PL lifetime reduced non-radiative recombination
55
𝑑𝑛
𝑑𝑡= −𝛽𝑛2(𝑡) −
1
𝜏𝑛(𝑡)
𝛽 ≈ 10−11cm3s−1
PL decay
Bi, D. et al. Efficient luminescent solar cells based on tailored mixed-cation perovskites. Science Advances 2, e1501170 (2016).
𝜏 = 350 ns
Hysteresis: Backward and Forward Scan
-1 -0.5 0 0.5 1
-20
-15
-10
-5
0
voltage / V
curr
ent density / m
A c
m-2
10 mV/s
100 mV/s
1,000 mV/s
10,000 mV/s
100,000 mV/s
(a)
1 sun
• Result depends on• preconditioning
• scan direction
-1 -0.5 0 0.5 1
-20
-15
-10
-5
0
voltage / V
cu
rre
nt d
en
sity / m
A c
m-2
JV curve not sufficient to accurately determine efficiencyHysteresis related to long-term instability and device degradation?
56
-1 -0.5 0 0.5 1
-20
-15
-10
-5
0
voltage / V
cu
rre
nt d
en
sity / m
A c
m-2
10 mV/s
100 mV/s
1,000 mV/s
10,000 mV/s
100,000 mV/s
1 sun
Hysteresis: Voltage Sweep Rates
• Result depends on• preconditioning• scan direction• scan rate
Device has “short-term memory”
• 2 possible reasons:• Displacement
current• Modified
photocurrent
57
-0.2 0 0.2 0.4 0.6 0.8
-20
-15
-10
-5
0
5
10
15
voltage / V
curr
ent density / m
A c
m-2
100 mV/s
1,000 mV/s
10,000 mV/s
30,000 mV/s
100,000 mV/s
1 sun
(a)
Charge carrier collection efficiency recombination
Tress, W. et al. Understanding the rate-dependent J–V hysteresis, slow time component, and aging in CH3NH3PbI3 perovskite solar cells: the role of a compensated electric field. Energy Environ. Sci. 8, 995–1004 (2015).
without TiO2 blocking layerLight induced structural changes?
Deep (surface) traps?Ferroelectrics?Ion migration?
…?
Hysteresis: What Happens?
58
Solar cell works as a pin device with built-in potential Vbi dropping over the approx. intrinsic perovskite layer**Bergmann, V. W. et al. Real-space observation of unbalanced charge distribution inside a perovskite-sensitized solar cell. Nat Commun 5, (2014).
Tress, W. et al. Understanding the rate-dependent J–V hysteresis, slow time component, and aging in CH3NH3PbI3 perovskite solar cells: the role of a compensated electric field. Energy Environ. Sci. 8, 995–1004 (2015).
CH3NH3PbI3
perovskite
-
+
CB -3.8 eV
VB -5.4 eV
-5.2 eV
-4.0 eV
1.6 eV
TiO2
HTM
Hysteresis: What Happens?
-1 -0.5 0 0.5 1
-20
-18
-16
-14
-12
-10
-8
-6
-4
-2
0
voltage / V
curr
ent density / m
A c
m-2
-0.5 0 0.5 1
-20
-15
-10
100,000 mV/s
100,000 mV/s
10,000 mV/s
200,000 mV/s
50,000 mV/s
10 mV/s
(a)
100,000 mV/s
59
Solar cell works as a pin device with built-in potential Vbi dropping over the approx. intrinsic perovskite layer**Bergmann, V. W. et al. Real-space observation of unbalanced charge distribution inside a perovskite-sensitized solar cell. Nat Commun 5, (2014).
Tress, W. et al. Understanding the rate-dependent J–V hysteresis, slow time component, and aging in CH3NH3PbI3 perovskite solar cells: the role of a compensated electric field. Energy Environ. Sci. 8, 995–1004 (2015).
Solar cell works as a pin device with built-in potential Vbi dropping over the approx. intrinsic perovskite layer*
Hysteresis: What Happens?
-1 -0.5 0 0.5 1
-20
-18
-16
-14
-12
-10
-8
-6
-4
-2
0
voltage / V
curr
ent density / m
A c
m-2
-0.5 0 0.5 1
-20
-15
-10
100,000 mV/s
100,000 mV/s
10,000 mV/s
200,000 mV/s
50,000 mV/s
10 mV/s
(a)
100,000 mV/s
-0.2 0 0.2 0.4 0.6 0.8-20
-15
-10
-5
0
5
10
voltage / V
curr
ent density / m
A c
m-2
-0.3 V
0.25 V
0.5 V
0.75 V
(b)
100,000 mV/s
*Bergmann, V. W. et al. Real-space observation of unbalanced charge distribution inside a perovskite-sensitized solar cell. Nat Commun 5, (2014).
60
without TiO2 blocking layer
Perovskite Solar Cells: Outlook
61
Costs• Solution processing
• Towards low-T processes• Absorber material low-cost
• Encapsulation?
Lifetime / Stability
Efficiency
• Theoretical SQ limit with 1.57 eV gap: η = 31 %
1 2 3 40
5
10
15
20
25
30
35
bandgap Eg [eV]
eff
icie
ncy
[%
]
• Considering the predicted max. Voc (incl. tail) of 1.32 V, 24 mA/cm2
η = 29 %, (VMPP = 1.2 V, FF ≈ 90 %)
• Considering state-of-the-art recombination (SRH): Voc = 1.2 V, FF = 83 % η = 24 %
CH3NH3PbI3
• Toxicity?• Acceptance?
• Sensitive to humidity• Stable when encapsulated?
• Upscaling?
Third Generation Concepts
62
http://www.solarroadways.com/
Overcoming the SQ Limit
63
http://www.intechopen.com/books/solar-cells-research-and-application-perspectives/optimization-of-third-generation-nanostructured-silicon-based-solar-cells
Intermediate Band Solar Cells
• Experimental trials: InAs QDs in GaAs not yet very successful
64
cstec.engin.umich.edu
• Maintain high voltage
• Increase current
• 3 quasi Fermi levels
Hot Carrier Solar Cells
• Avoiding thermalization by introducing “phonon bottleneck”
• Energy selective contacts
not yet successfully realized
65
web.stanford.edu
Up- and Down Conversion
• Effects shown, however with low yield66
www.intechopen.com
Fraunhofer ISE
There is always room for new ideas…
67
http://www.solarroadways.com/
Wattways
World Solar Challenge Australia