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1
Annamaria Petrozza
Hybrid Perovskite Solar Cells
Milan, Novembre 27th, 2015
"ORGANIC ELECTRONICS : principles, devices and applications"
2
B X
A
Perovskite Crystal with ABX3 stoichiometry
I-V-O3, II-IV-O3 and III-III-O3 e.g KTaO3, SrTiO3 and GdFeO3
I-II-X3, e.g. CsSnI3, CH3NH3PbI3,
3
B X
A
It is not only a matter of stoichiometry….
The Goldschmidt tolerance factor:
)(2 XB RR
RRt XA
t< 0.7 the perovskite falls apart t >1 towards 2D structures…
4
CH3NH3PbI3 (CH3NH3)2PbI4
(C10H21NH3)2PbI4 (CH3NH3)4PbI6*H2O
Playing with Dimensionality
5
CH3NH3PbI3 (CH3NH3)2PbI4
(C10H21NH3)2PbI4 (CH3NH3)4PbI6*H2O
5 Ishihara, J. Lum, 1994.
Dielectric Confinement
6
Organo-Metal Halide Crystalline Perovskite
A= Pb2+
X= I-, Cl-, Br-
B = (CH3NH3+)x
ABX3
7
Organo-Metal Halide Crystalline Perovskite
Eric Hoke et al, Chem Sci, 2015
Filip et al, Nat Comm, 2014
8
Organo-Metal Halide Crystalline Perovskite
9
CH3NH3+ :Orientational disorder and Polarizability
Hydrogen Bonds Dipole “nearly” free to move
10
Modular Structure
11
Prone to a variety of processing
methods
Type II Hetero-Junction
Excitonic Solar Cells
13
Intrinsic Loss in Excitonic Solar Cells
1.0 1.2 1.4 1.6 1.80.4
0.6
0.8
1.0
1.2-0.6eV-0.4eV-0.2eVVoc = BG
CIGS
CdTe
ncSi
CZTSS
aSi
Vo
c (V
)
Bandgap (eV)
OPV
DSC
MSSCGaAs
Si
Hybrid Crystals in DSSC Devices
h u h
Hole transfer
e- injection
H. S. Kim et al. Sci Rep. 2: 591 (2012)
CH3NH3PbI3 perovskite as light
antenna in the DSSC concept
Glass
FTO
HTL
Silver Perovskite role:
• Absorber
• Electron-transporter
M.Lee et al. Science 338, 643 (2012)
TiO2
Al2O3
Hybrid Crystals in Hybrid Solar Cells
16
Which is their strength?
17
18
Optoelectronic Devices
Tan et al, Nat Nanotech, 2014
Zhu et al, Nat Mat, 2015
19
Designing the Device Architecture
TiO2/Al2O3 scaffold+ Perovskite
Perovkite capping layer Perovkite capping
layer
HTM HTM HTM
Nano-structured vs Thin Film J. Ball, EES, 2013
Designing the Device Architecture
• Light Absorption • Charge Generation • Photo-carriers Transport
Designing the Device Architecture
• Light Absorption • Charge Generation • Photo-carriers Transport
Light Absorption
Silicon
In direct band-gap Phonon assisted
um range sun light penetration depth
thick solar cells
no light emission
GaAs
direct band-gap
excitonic effects at absorption edge good light penetration depth
Dyes/conjugated polymers
localized states excitonic effects large absorption cross-section/ efficient carrier recombination
Silicon
In direct band-gapPhonon assisted um range visible light penetration dept thick solar cells no light emission
GaAs Dyes/conjugated polymers
direct band-gap
excitonic effects at absorption edge good light penetration depth
Light Absorption
localized states excitonic effects large absorption cross-section/ efficient carrier recombination
Silicon
In direct band-gapPhonon assisted um range visible light penetration dept thick solar cells no light emission
Hybrid Perovskites
Dyes/conjugated polymers
1.50 1.53 1.56 1.59 1.62 1.65 1.68 1.71 1.74 1.77 1.800.5
1.0
Energy (eV)
4.2K
290K
Op
tica
l D
en
sity (
a.u
.)
direct band-gap
excitonic effects at absorption edge good light penetration depth
Light Absorption
localized states excitonic effects large absorption cross-section/ efficient carrier recombination
25
“ ..is a quasi-particle that represents a collective excited state of an ensable of atoms or molecules. It is represented by a wavepacket for which we can define mass and speed which transports Energy”
Exciton
26
Binding energy
Oscillator strength
Delocalization
Lifetime
Singlet
Triplet
How many kind of excitons??
Wannier-Mott Frenkel
27
Frenkel Exciton
• Solids made by weakly interacting units (e.g organic crystals, inter-molecular coupling weaker than the intra-molecular ones).
• General case of a Molecular Excitation (DSSC)
• The wavefunction squared amplitude is the probability of finding the excited state in the lattice.
G. Lanzani, “The Photophysics behind Photovoltaics and Photonics” Wiley-VCH
De e
E
g
u
Wannier-Mott • Solids with tightly bounded atoms
• Low Screening Coulomb attraction does not allow the generation of FREE e-h pairs
• Hydrogenoid system.
• Center of Mass/Exciton radius (LARGER than the lattice constant)
E1
Eg
K
E
rh
re
RX kh
ke
O
he
XbgnK
mm
K
n
EEE
X
22
2,
G. Lanzani, “The Photophysics behind Photovoltaics and Photonics” Wiley-VCH
• Energy spent in the exciton dissociation
Why do we need to know the details?
• Energy spent in the exciton dissociation • Absoprtion cross section enhancement
Why do we need to know the details?
3)(
1
B
Xa
Elliott’s Theory (1963)
• Energy spent in the exciton dissociation • Absoprtion cross section enhancement
Why do we need to know the details?
n
nx
eh
Tk
n
n
nnn
FC
Tk
E
B
exc
FC
excFC
B
b
2/3
2)
2(
32
Exciton Vs Free Charges
at the Thermodynamic Equilibrium
Saha-Langmiur equation
@ RT PV regime
Total excitation density Excitons
Free charges
D’Innocenzo et al, Nat Comm. 5, 3586, 2014
Law of mass action
4 2
2 2 22 2B
B
eE
a
e
2
2
eaB
e
Bohr Radius
Exciton Reduced mass
Dielectric constant
Exciton Binding Energy
The golden rule:
“the Bohr orbital frequency (Eb/h) must be compared with the optical phonon frequency”
he
he
mm
mm
Dielectric constant (ε):
A measure of a substance’s ability to insulate charges from
each other.
Screening in solids: basic concept
E0
E=0 Ed
𝐸𝑑 =𝐸 0𝜀
METAL DIELECTRIC
Screening mechanisms
Electronic Polarizability (Electron Cloud Distortion) 1015 s-1
Dipole Re Orientation (Langevin Mechanism) 108- 1010 s-1
Ions Displacement (Optical Phonons)
1010- 100 s-1
Screening mechanisms
Dielectric constant of GaAs. Why it is so easy
e0 (T) = 12.4 + 0.00012*T
LO = 36meV TO = 38meV
20 e
e
Dielectric constants of CH3NH3PbI3, real and imaginary parts
Dielectric constants of CH3NH3PbI3, real and imaginary parts
1KHz
41
)exp(1Tk
Ek
B
bD uu
Eb (upper limit)= 50meV
Exciton Binding Energy
(I) Direct Measurement of Exciton Binding Energy in CH3NH3PbI3
hD
D’Innocenzo et al, Nat Comm. 5, 3586, 2014
Limitations: It is assumed that exciton-phonon interaction induces only exciton dissociation though in a limited range – it assumes the exciton binding energy constant in T
42
TkE
TTB
B
ek
Tkk 0
1T
1
12 2
1
T
1
T
2T
1
D
(I) Direct Measurement of Exciton Binding Energy in CH3NH3PbI3
43
(II) Direct Measurement of Exciton Binding Energy in CH3NH3PbI3
Numerical modelling of band-edge absorption by using Elliot’s theory of Wannier excitons
43
Eb = 25meV
Saba et al, Nat Comm. 5, 5049, 2014
Note: This simple formalism does not consider the frequency dependance of the exciton-phonon interaction
44
m*= 0.1m ; Eb = 16meV
Miyata et al, Nature Physics 11, 582–587 (2015)
n
REE gn
)*
()2/1()(m
eBNEBE g
At 4K
e 9
(III) Direct Measurement of Exciton Binding Energy in CH3NH3PbI3
45
Eb 10 meV
Miyata et al, Nature Physics 11, 582–587 (2015)
n
REE gn
)*
()2/1()(m
eBNEBE g
At 161K
e > 9
(III) Direct Measurement of Exciton Binding Energy in CH3NH3PbI3
Organic-Inorganic Interplay: Raman Spectroscopy as a probe
60 80 100 120 140 160 180 200 220 240 260 280 3000.0
0.2
0.4
0.6
0.8
1.0 Meso
Flat
Ra
ma
n I
(n
orm
.un
its)
Raman shift (cm-1)
Grancini G et al, JPC Letters, 5, 3836, 2014
• Light Absorption • Charge Generation • Photo-carriers Transport
48
Exciton Vs Free Charges
at the Thermodynamic Equilibrium
Saha-Langmuir equation n
nx
eh
k
n
n
nnn
FC
kB
exc
FC
excFC
B
T
E
2/3
2
b
)T2
(
Total excitation density Excitons
Free charges
Are there excitons around? MAPbI3
Room Temperature, in the typical PV regime ph <1016 cm-3 :
free carriers only
THz conductivity spectra are Drude-like in accordance with the presence of free charge carriers. Wehrefenning et al, Adv Mater, 26, 1584, 2014, Milot et al, Adv Funct Mater, 2015 DOI: 10.1002/adfm.201502340, PL dynamics are dictated by bimolecular recombination processes. Yamada, Y J. Am. Chem. Soc. 2014, 136, 11610. Stranks, Phys. Rev. Appl. 2014, 2 034007. fs-TA spectra show band filling effect and Varnshi –shift. Kamat et al, Nature Photonics, 2014; Grancini&Kandada et al, Nature Photonics 2015
The deal for PV is: we exploit the presence of the exciton transition for light harvesting without paying in charge dissociation
Are there excitons around? MAPbI3
Low Temperature, Exciton population is detectable.
THz spectra probe localization effects as a consequence of exciton formation below 80K. Milot et al, Adv Funct Mater, 2015 DOI: 10.1002/adfm.201502340, fs-TA spectra show a modulation of the photo-bleach as a result of exciton-exciton interaction. Grancini&Kandada et al, Nature Photonics 2015
1014
1015
1016
1017
1018
1019
1020
1021
1022
0.0
0.2
0.4
0.6
0.8
1.0
290K
170K
70K
Excitation Density (cm-3)
x (
nF
C/n
TO
T)
5 meV
WARNING: The Exciton binding energy increases (the dielectric constant decreases) when cooling down! Miyata et al, Nature Physics 11, 582–587 (2015)
MAPbI3 Local order/ microstructure
D’Innocenzo et al, Nat Comm. 5, 3586, 2014 Grancini&Kandada et al, Nature Photonics 2015
Designing the Device Architecture
• Light Absorption • Charge Generation • Photo-carriers Transport
53
500 600 700 8000.0
0.2
0.4
0.6
0.8
O.D
.
Wavelength (nm)
CH3NH
3PbI
3-xCl
x/PMMA
0.0
0.5
1.0
PL (
norm
.)
Photo-carriers Diffusion Length
54
Glass
+ - + -
Silica Selective Quencher
Diffusion constant Natural decay rate (no quencher)
Electron-Hole Diffusion Lengths
By Photoluminescence Quenching
55
Electron-Hole Diffusion Lengths
By Photoluminescence Quenching
Science , 342,341, 2013
DT (ne+nh)
CB
VB
56
Perovskite Species D (cm2s-1) LD (nm)
CH3NH3PbI3-xClx Electrons 0.042 ± 0.016 1094 ± 210
Holes 0.054 ± 0.022 1242 ± 250
CH3NH3PbI3 Electrons 0.017 ± 0.009 117 ± 29
Holes 0.012 ± 0.005 96 ± 22
0 50 100 150 20010
-2
10-1
100
PL
(norm
.)
Time after excitation (ns)
PMMA
Spiro-OMeTAD
PCBM
CH3NH3PbI3-xClx
0 10 20 30 40 5010
-2
10-1
100
PL
(n
orm
.)
Time after excitation (ns)
PMMA
Spiro-OMeTAD
PCBM
CH3NH3PbI3
Electron-Hole Diffusion Lengths
By Photoluminescence Quenching
Science , 3
42
,34
1, 2
01
3
57
Time-resolved Photoluminescence
Yamada, Y J. Am. Chem. Soc. 2014, 136, 11610. Stranks, Phys. Rev. Appl. 2014, 2 034007. Saba, M.; Nat. Commun. 2014, 5 No. 5049. D’Innocenzo, J. Am. Chem. Soc. 2014, 136 (51), pp 17730–1773 Deschler, J. Phys. Chem. Lett. 2014, 5, 1421.
Stranks et al
Deschler, et al
58
Time-resolved Photoluminescence
D’Innocenzo et al. JACS, 2014, 136 (51), pp 17730–1773
59
Time-resolved Photoluminescence
D’Innocenzo et al. JACS, 2014, 136 (51), pp 17730–1773
100 1000 10000
760
762
764
766
768
770
772
774
776
778
780
782
Band Edge Position
cwPL Peak Position
Avarage crystallite size (nm)
Spe
ctra
l po
siti
on
(n
m)
CBBB
G
E TkGi
EphphGrad
de
En
dvER
ee
eeee
e )(1
1)()(
)()()()(
Filippetti, et al. J.Phys.Chem, 2014, doi:10.1021/jp507430x
Measuring Charge-Transport in Perovskites Terahertz/Microwave Spectroscopy
Simple sample preparation Only informative on short length-scale
Time-of-flight Relevant over longer length-scale
Time-scales difficult to measure in thin-film
Space-charge limited current Relevant to optoelectronic devices
Needs highly-selective non-limiting contacts
Hall-effect Simultaneously get free-carrier density Like THz, only band mobility obtained
Q. Dong et al., Science (2015)
Q. Dong et al., Science (2015) C. Wehrenfennig et al., Adv. Mat. (2013)
C. Stoumpos et al., Inorg. Chem. (2013)
μ ~ 10 cm2/Vs
μ ~ 25 cm2/Vs
μ ~ 25-165 cm2/Vs
μ ~ 66 cm2/Vs
The room temperature structure of MAPbX3 is a fluctuating structure where titling and
distortion of the octahedral networks and rotations and polarizability of the molecular dipole can strongly affect the optoelectronic
properties of the semiconductor.
Take-home Message
Open Questions
Which is the secret of the low recombination rate Elucidation of the photo-carriers cooling Role of phonons Nature of carriers, localization vs delocalization Carriers transport mechanism
Vs Structural Properties
Technology
Technology
Zhang et al, Mater. Horiz., 2015, 2, 315–322
Technology
Perovskite PV at IIT
p I n
TiOx/PCBM
MAPbI3
Spiro MeOTAD
Aumento efficienza fotovoltaico tradizionale
Fotovoltaico leggero e flessibile, a basso costo di produzione e
energetico
17.6 %
p I n
Processi a bassa temperatura < 120 °C
Celle «TANDEM»
67
Technology Development
Perovskite PV at IIT
Further Developments
Interface Engineering Stability Toxicity ..