Mahmoud Samadpour1, Arezo Golchini1, Karim Abdizadeh2, Mahsa Heydari3, Mozhdeh Forouzandeh3,4, Zahra Saki3, Nima Taghavinia3,5. 1. Department of Physics, K. N. Toosi University of Technology, Tehran 19697 Iran. 2. Material Science and Engineering Faculty, Sharif University of Technology, Tehran 14588, Iran. 3. Nanoparticles and Coating Lab, Department of Physics, Sharif University of Technology, Tehran 14588, Iran. 4. Department of Basic Sciences, Tarbiat Modares University, Tehran 17514115, Iran. 5. Institute for Nano Science and Nanotechnology, Sharif University of Technology, Tehran 14588, Iran.
Abstract
Antisolvent crystallization is known as an effective approach for the deposition of pinhole-free solution-processed perovskite layers for high-performance solar cells. Here, we introduce a modified antisolvent dripping method by adding tetra ethyl orthosilicate (TEOS) into chlorobenzene as a conventional antisolvent. Through TEOS modification, perovskite solar cells show efficiencies as high as 16% with more than 85% retention after 290 h storage at ambient conditions in comparison to 20% in pristine cells. This significant enhancement in efficiency and stability mainly related to the decrement of the density of surface defects, which is confirmed by considerably enhanced photoluminescence of perovskite layers. Also, electrochemical impedance spectroscopy results show lower charge recombination at interfaces in modified cells. Regarding the obtained results, our modified antisolvent approach is a simple and promising route to prepare high-quality perovskite layers for solar cell applications.
Antisolvent crystallization is known as an effective approach for the deposition of pinhole-free solution-processed perovskite layers for high-performance solar cells. Here, we introduce a modified antisolvent dripping method by adding tetra ethyl orthosilicate (TEOS) into chlorobenzene as a conventional antisolvent. Through TEOS modification, perovskite solar cells show efficiencies as high as 16% with more than 85% retention after 290 h storage at ambient conditions in comparison to 20% in pristine cells. This significant enhancement in efficiency and stability mainly related to the decrement of the density of surface defects, which is confirmed by considerably enhanced photoluminescence of perovskite layers. Also, electrochemical impedance spectroscopy results show lower charge recombination at interfaces in modified cells. Regarding the obtained results, our modified antisolvent approach is a simple and promising route to prepare high-quality perovskite layers for solar cell applications.
Increasing from 3.8% to
more than 25% efficiency, hybrid organometallic
halideperovskite solar cells (PSCs) have attracted excessive attention
in recent years.[1] Hybrid perovskites with
an ABX3 structure, include an organic cation, A = methylammonium
(MA) or formamidinium (FA), divalent metals, B = Pb2+ and
Sn2+, and anions like X = Cl–, I–, and Br–.[2−4] The high performance
of PSCs have been ascribed to desirable properties such as a marked
extinction coefficient, a tunable band gap, and the proper dynamics
of charge transport at interfaces and whole devices.[5−8] In spite of exponential increase in efficiency, still there are
many concerns about the severe instabilities in perovskite solar cells.
In addition to the characteristic of the hole/electron transport layers
(HTLs/ETLs) and contacts, the stability of PSCs is mainly attributed
to the perovskite layer properties.[3,9−14] In this context, structural phase transition, light-induced trap
states, halide segregation, and moisture/thermal-induced degradations
have been widely investigated recently.[15−18] Concerning the stability issue,
a variety of novel HTLs/ETLs are introduced; also, a considerable
research is conducted to make more stable, uniform, pinhole-free,
and highly crystalline perovskite layers.[19−22]For example, utilizing
perovskites with mixed cations and halides
not only improved the performance of the primary MAPbX3 perovskite layers but also increased the stability by hindering
the volatile nature of MA molecules.[23] Annealing-free
vacuum-deposited perovskite absorbers were investigated by Zhao et
al.[24] Solvent-annealing was established
as an effective route to improve the crystallinity, and the charge
carrier diffusion length of trihalideperovskite materials was increased
to over 1 μm.[25,26] Sequential deposition is widely
used as a route to high-performance perovskite-sensitized solar cells.[27] More thermally stable with less phase impurities,
perovskites were made by addition of inorganic cesium in triple-cation
perovskite compositions.[13] More recently
flash infrared annealing has been utilized to improve the properties
of the perovskite layers.[28]Regarding
the wet chemical deposition methods, numerous studies
are performed to optimize the composition of solvents of perovskite
precursors. As an instance, extremely uniform and dense perovskite
layers were obtained by mixed solvent of γ-butyrolactone and
dimethylsulphoxide (DMSO) followed by toluene drop-casting.[29]Among the various approaches, the antisolvent
technique is currently
one of the most preferred methods to make highly crystalline, markedly
smooth and pinhole-free perovskite layers.[30−32]It is known
that the quality of the perovskite layer is mostly directed by the
nucleation and crystal growth stages. The antisolvent method produces
many nuclei by abruptly reducing the precursor’s solubility
following by crystal growth. Until now various antisolvent materials
such as chlorobenzene, hexane, toluene, ethyl acetate, diethyl ether,
isobutanol, isopropyl alcohol, and chloroform are utilized and investigated
in details.[33−36]Among the large number of possible antisolvents, chlorobenzene is
much widely utilized to make high-performance solar cells.[37,38] In addition to the considerable advantages, recently even more studies
have been conducted to better control the unpredictable crystal formation
in the antisolvent method. For instance, mixed solvents were utilized
to make more homogeneous perovskite layers.[39,40] Through PMMA addition into the chlorobenzene /toluene, not only
the electronic quality of perovskite layers was exponentially improved,
but also the stability was improved remarkably.[41]Recently tetra ethyl orthosilicate (TEOS) was directly
added in
the precursor solutions of the perovskite and spin coated on the TiO2 substrates by Zhou et al.[42] Their
results indicated that silica encapsulates the grain boundaries of
the perovskite layer and improves the efficiency and stability of
cells. In spite of the superior properties, the explained method is
applicable to the perovskite layers with formamidinium-based structures.After that various research studies utilized TEOS antisolvent in
order to modify the simple MAPbI3 structures in both planar
n-i-p and p-i-n structures.[43,44] Despite the improved
photovoltaic properties, the intrinsic structural and thermal instability,
in addition to the severe degradation of MAPbI3 structures
upon contact with moisture, hinders the practical applications.[10,11,45]In this work, we have introduced
a modified chlorobenzene (CB)
antisolvent procedure for enhancing the performance of the triple-cation
perovskite active layers by improving their electronic properties.
Here, TEOS was incorporated into the CB antisolvent, in order to decrease
the surface defects during the fast nucleation and growth of perovskite
grains. A remarkable decrement in surface trap states of perovskite
layers were confirmed through highly enhanced photoluminescence of
perovskite layers. This was further confirmed by studying the capacitive
properties of the perovskite layer between the contacts by electrochemical
impedance spectroscopy (IS) measurements. In addition to the improved
photovoltaic properties, more stable devices were obtained by the
proposed antisolvent method.
Results and Discussion
With regards to the hydrolysis and condensation reactions in the
presence of distilled water in antisolvent, TEOS will turn into silica
gel according to the following reactions as explained elsewhere.[43]It is
noteworthy that antisolvent pouring induces a considerable
drop in the solubility of the perovskite precursors, providing a high
density of nucleation sites followed by an effective crystal growth.
With regards to the TEOS-incorporated antisolvents, crystallization
of the perovskite grains and the precipitation of silica will take
place simultaneously. Therefore, the dynamics of the perovskite crystallization
could to be affected by the silica oligomers in the antisolvent.The crystalline structure of the pristine and modified perovskite
films was characterized by X-ray diffraction (XRD), as illustrated
in Figure . The diffraction
peaks at 14.10, 20.03, 24.56, 28.43, 31.86, 40.64, and 43.28o corresponding to the crystalline planes of the photoactive black
phase of the Cs0.05 (MA0.17 FA0.83)0.95 Pb(I0.83 Br0.17)3 perovskite layer.[13]
Figure 1
XRD spectra of pristine
and modified perovskite films on FTO-coated
glass/TiO2 substrates. Perovskite, PbI2, and
FTO/TiO2 diffraction peaks are indicated by α, *, and #, respectively.
XRD spectra of pristine
and modified perovskite films on FTO-coated
glass/TiO2 substrates. Perovskite, PbI2, and
FTO/TiO2 diffraction peaks are indicated by α, *, and #, respectively.Meanwhile, there is no diffraction peak from the undesired photo-inactive
delta phase of FAPbI3 at 11.61o, which is a
common and not preferred side structure in three cationic perovskite
layers. This could be originated by Cs ions as explained before.[13] The full width at half maximum (FWHM) of the
main perovskite peak at 14.10o was obtained through fitting
and was very similar, 0.19 and 0.20, respectively, for reference and
TEOS-modified perovskite layers. The crystallite size of the perovskite
layers estimated by the Scherrer equation from the most intense peak
at 14.1o slightly reduced from 43 to 40.2 nm. Regarding
the same position of perovskite diffraction peaks in reference and
modified perovskite (PS) layers and a mere difference of FWHM, the
provided results indicate that the structure of the PS film remained
unchanged after the mentioned modification. This could propose the
same antisolvent crystallization processes in both reference and modified
antisolvents.In addition to the fluorine-doped tin oxide (FTO)/TiO2 diffraction patterns, cubic PbI2 peaks were distinguished
at both pristine and modified perovskite layers with a mere difference
in intensity, which could be from the incomplete conversion of precursors
to the black perovskite phase as the deposition is performed in an
atmosphere environment here. It is known that PbI2 could
passivate the defects and enhance the device performance, nevertheless
excessive PbI2 content in the films adversely distress
device performance by its poor optoelectronic properties.[46] Furthermore, no diffraction patterns of incorporated
silica were identified. This reveals that amorphous silica is integrated
with the perovskite layer through the hydrolysis reaction of TEOS.Concerning the morphology, scanning electron microscopy (SEM) images
of the pristine and TEOS-modified perovskite layers in two different
scales are provided in Figure . Apparent from this figure, a negligible difference could
be observed in surface morphology and large grain sizes are evident
in both layers with or without TEOS modifications.
Figure 2
SEM image of (a, b) pristine
and (c, d) TEOS-modified PS layers.
Scale bar is 1 micron in figures (a, c) and 200 nm in figures (b,
d).
SEM image of (a, b) pristine
and (c, d) TEOS-modified PS layers.
Scale bar is 1 micron in figures (a, c) and 200 nm in figures (b,
d).According to the elemental mapping
of the perovskite layer, Si
is distributed in the whole layer (Figure ), which indicates that an amorphous silica
has encapsulated the entire perovskite layer while just a grain boundary
encapsulation was observed through adding TEOS to perovskite precursors.[42]
Figure 3
Elemental mapping of the perovskite layer. The scale bar
is 2.5
micron in all figures.
Elemental mapping of the perovskite layer. The scale bar
is 2.5
micron in all figures.Moreover, the ultraviolet–visible
(UV–vis) absorption
spectra of perovskite films were measured and are presented in Figure a. A glance at the
given figure reveals a mere difference between the pristine and modified
PS films absorption spectrum. Furthermore, concerning the Tauc plot
shown in Figure b,
the pristine and TEOS-modified PS band gaps are comparable, approximately
1.61 eV for both structures. These observations reveal that the TEOS
modification has no marked effect on the Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 PS layer in terms of the optical
properties.
Figure 4
(a) UV–vis absorption spectra of the reference and TOES-modified
Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 film. (b) Tauc
plots derived from absorbance spectra of pristine and modified PS
films.
(a) UV–vis absorption spectra of the reference and TOES-modified
Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 film. (b) Tauc
plots derived from absorbance spectra of pristine and modified PS
films.In order to explore the effect
of TEOS-modified perovskite layers
on the photovoltaic properties of PSCs, here reference and TEOS-modified
cells were prepared. Figure , indicates the J–V curves of cells prepared with chlorobenzene
and TEOS-modified chlorobenzene antisolvent. We name these cells reference
(R-Cell) and modified cells (M-Cell), respectively. Here, antisolvent
dripping was performed in various time intervals from 1–50
min after TEOS addition to chlorobenzene and stirring. The photovoltaic
parameters of cells are summarized in Table , concerning an apparent explanation. According
to the results provided, an open circuit voltage (Voc) of 1.03 V, a short circuit current (Jsc) of 22.32 mA.cm–2, a fill factor
(FF) of 62.49%, and a power conversion efficiency (PCE) of 14.36%
are obtained in R-cells. It is noteworthy that our cells are made
under the ambient environment and their efficiency is expected to
be lower than the record efficiencies of more than 20% of triple-cation
perovskite solar cells which are made under inert atmospheres like
N2 or Ar.[13] The modified cell,
with 2 min stirring time reveals a higher Jsc of 22.78 mA/cm2, Voc of 1.03
V, and a considerably raised FF of 71.25%, resulting in an improved
efficiency of 16.72%.
Figure 5
J–V curves of solar cells which are made with chlorobenzene
(reference cells which are denoted by R-Cell) and TEOS-modified antisolvent
(M-Cells). Here, antisolvent dripped from the solutions which are
stirred in various time intervals after TEOS addition (1–50
min).
Table 1
Photovoltaic Parameters
of Cells: Photocurrent jsc, Open Circuit
Voltage Voc, Fill Factor FF, and Efficiency PCE for Reference and Modified
Cells as a Function of Stirring
Time in TEOS Contained Antisolvents
cell type
Voc(V)
Jsc(mA/cm2)
FF (%)
PCE (%)
reference
1.03
22.32
62.49
14.36 ± 0.22
M-Cell (1 min)
1.03
22.27
63.12
14.48 ±
0.13
M-Cell
(2 min)
1.03
22.78
71.25
16.72 ± 0.14
M-Cell (3 min)
1.02
23.07
69.82
16.43 ± 0.09
M-Cell (5 min)
1.02
22.81
68.62
15.96 ±
0.24
M-Cell
(10 min)
1.01
22.66
63.73
14.58 ± 0.11
M-Cell (20 min)
1.02
21.83
64.03
14.26 ± 0.12
M-Cell (30 min)
1.01
22.44
62.10
14.07 ±
0.15
M-Cell
(40 min)
1.04
22.72
59.69
14.10 ± 0.11
M-Cell (50 min)
1.00
21.44
64.52
13.83 ± 0.17
J–V curves of solar cells which are made with chlorobenzene
(reference cells which are denoted by R-Cell) and TEOS-modified antisolvent
(M-Cells). Here, antisolvent dripped from the solutions which are
stirred in various time intervals after TEOS addition (1–50
min).A glance at the graph
and Table reveals
the superior photovoltaic properties of modified
cells in comparison to pristine ones, primarily the significant increase
in the FF (from 62.49% in R-Cells to 71.25% in optimized M-cells)
while the Voc and Jsc have a small difference.It is noteworthy that a high
polymerization degree of the silica
oligomers in the antisolvent could constrain the perovskite crystallization
and consequently drop the photovoltaic properties of cells as it is
apparent from inferior performance of cells with long stirring times
of more than 10 min (Table ). The efficiency of cells with 1 min stirring time (14.48%)
was very close to the reference cells which indicates that a longer
time is needed for noticeable hydrolysis and condensation reactions
in solution as explained before. Furthermore, the photovoltaic performance
of cells with 3 min stirring time (16.43%) was less than that of optimized
cells with 2 min stirring time.Concerning the energy levels
in PS layers and in order to evaluate
the origin of the improvement in photovoltaic properties of modified
cells, steady-state photoluminescence (PL) measurements were conducted
on pristine and modified PS layers. Figure a shows the PL spectra of the pristine and
modified Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 PS
films. For both cells, the PL peak was located at 765 nm, while the
PL intensity is markedly increased after modification. These results
suggests a considerable drop in the density of trap states in the
PS layers as nonradiative recombination centers while the bulk properties
of the layer is unchanged as shown in Figures , 2, and 4.
Figure 6
(a) Comparison of photoluminescence emission spectra of
pristine
Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 PS and TEOS-modified
PS films. (b) Current- voltage properties of the hole-only devices
with ITO/NiO/perovskite/CIS/Au structure
as presented at the inset of the figure.
(a) Comparison of photoluminescence emission spectra of
pristine
Cs0.05 (MA0.17 FA0.83)0.95 Pb (I0.83 Br0.17)3 PS and TEOS-modified
PS films. (b) Current- voltage properties of the hole-only devices
with ITO/NiO/perovskite/CIS/Au structure
as presented at the inset of the figure.The density of trap states was measured through the space-charge-limited
current (SCLC) experiment (Figure b), which was carried out on the hole-only devices
with ITO/NiOx/perovskite/CIS/Au structure (inset of Figure b).Density
of the trap states was determined be by the trap-filled-limit
voltage (VTFL) in the equation[47]VTFL = 0.5 eDtrapL2ε–1ε0–1, where e, ε0, ε, L, and Dtrap are elementary
charge, vacuum permittivity, relative dielectric constant (28.8 for
PS layer[48]), thickness of the PS layer,
and the density of trap states, respectively. The corresponding trap
densities were obtained 3.32 × 1016 cm–3 and 1.38 × 1016 cm–3 for pristine
and TEOS-modified devices, respectively, indicating the improved quality
of PS films by TEOS modification.It is known that the prominent
drop of charge carriers arises from
the imperfections located at the perovskite surface, which can trap
free charges and increase the recombination.[49−51] Amorphous silica
passivate the perovskite surface, which significantly reduce the defect
states as the carrier recombination centers. Therefore, employing
TEOS additive into the antisolvent could moderate the recombination,
consequently improving cell performance.The reduced surface
trap states, which originated by the integrated
amorphous silica in PS layers[44,52] could explain the improved
fill factors and consequently higher efficiencies in TEOS-modified
cells as explained before in Table .In order to understand the properties of charge
carriers transport
in the whole devices, electrochemical impedance spectroscopy was performed
at open circuit voltage. Figure presents the Nyquist plots of reference and modified
cells. For both samples, two distinguishable arcs were observed at
high and low frequencies, respectively. Nyquist plots were fitted
by the equivalent circuit model presented in the inset of Figure . Here, Rs is the series resistance, and C1 and R1 are associated with the
high-frequency arc in the Nyquist plot. C1 is the geometric capacitance of the perovskite in between the contact
layers. R1 corresponds to the conductivity
of the perovskite layer and also can be affected by the transport
resistance of the HTL.
Figure 7
(a) Nyquist plot and the fitting results (fitting curves
are denoted
by “F”) of the cells with pristine (R-Cell) and modified
perovskite layers (M-Cell). The equivalent circuit model for fitting
the IS results is apparent in the inset of (a). (b) Plot of the capacitance
versus frequency.
(a) Nyquist plot and the fitting results (fitting curves
are denoted
by “F”) of the cells with pristine (R-Cell) and modified
perovskite layers (M-Cell). The equivalent circuit model for fitting
the IS results is apparent in the inset of (a). (b) Plot of the capacitance
versus frequency.C2 and R2 are related to the low-frequency
arc of the Nyquist plot shown in Figure . C2 originates
from electronic and ionic charge accumulation
at the electrode interfaces. R2 is associated
with the recombination at the perovskite interface with contacts.[53]The fitting curves of the pristine and TEOS-modified
cells are presented in Figure a also.According to the fitting results by the equivalent
circuit model,
almost same values of R1, 94.41 and 97.22
Ωcm2 for pristine and modified cells, were, respectively,
obtained. Regarding the same HTL layer in both structures, it is concluded
that the bulk properties of the perovskite layer is preserved through
the antisolvent modification.On the other hand, devices with
a modified antisolvent layer have
higher R2 values (156.06 Ωcm2) than pristine (76.95 Ωcm2) cells which
explain the lower charge recombination at the interfaces of the perovskite
layer and contacts. The lower recombination at interfaces led to improved
fill factors in modified cells (Table ).In order to evaluate the capacitive processes
in cells, the capacitance–frequency
(C–f) plot of cells is presented in Figure . According to the provided figure, modified
cells, give a lower capacitance especially in mid-frequency ranges.
The capacitive behavior in mid- and low-frequency ranges is attributed
to the charge accumulation at interfaces as explained before.[51]This proves the reduced interfacial charge
accumulation at modified
cells and consequently improved photovoltaic properties (Table ). It is noticeable
that the reduced interfacial charge accumulation in modified cells
is in good agreement with considerably lower density of trap states
(higher PL intensities) in modified perovskite layers as shown in Figure . In addition to
the efficiency, by far the ambient stability is the most concerned
subject in PS solar cells. In this context, the long-term stability
of pristine and modified cells was explored under ambient conditions,
relative humidity of 40 ± 2% and 27 ± 1 °C temperature
(Figure ). Receiving
to near 20% of the initial efficiency after 290 h, pristine cells
lost 80% of their initial performance. In the stark contrast, more
than 85% of efficiency in TEOS-modified cells was achieved in the
same time. Given stability results, reveals the effective passivation
of perovskite layers by amorphous silica in modified cells.
Figure 8
Long-term stability
of reference and modified cells under ambient
conditions, relative humidity of 40 ± 2% and 27 ± 1 °C
temperature.
Long-term stability
of reference and modified cells under ambient
conditions, relative humidity of 40 ± 2% and 27 ± 1 °C
temperature.
Conclusions
Here,
a simple modified antisolvent method was introduced for improving
the performance of PSCs. According to our results the crystalline
structure and the optical properties of the perovskite layer was preserved
after modification while the surface trap states were decreased markedly.
A considerable improvement in fill factors was obtained which is originated
by the lower charge recombination in modified cells as confirmed by
IS measurements. Furthermore, the long-term stability of cells under
ambient conditions was noticeably improved in TEOS-modified cells.
As a general conclusion, here a simple modified antisolvent method
is introduced to deposit perovskite layers with superior properties
for high-efficiency PSCs.
Experimental Section
Materials and Synthesizing Methods
Fluorine-doped tin
oxide (FTO, Solaronix, 15 Ω/square)-coated glass substrates
were patterned with zinc powder and diluted hydrochloric acid. Provided
substrates were successively cleaned by sonication in 2% Hellmanex
water solution, deionized water, ethanol, acetone, and isopropanol
for 10 min. After sintering at 450 °C for 15 min, UV-ozone treatment
was performed to remove the possible residual contaminants.In order to deposit a TiO2 hole-blocking layer on FTO
substrates, a 0.15 M TTIP (97% Merck, Germany) solution in ethanol
was spin-coated at 2000 rpm, for 30 s and followed by sintering at
500 °C for 1 h. Afterward, a commercial TiO2 paste
(IRASOL PST-20 T) diluted in ethanol (1:5.5 W ratio) and was spin-coated
on the FTO/compact TiO2 layer at 4000 rpm for 30 s and
annealed at 500 °C for 30 min. Before perovskite deposition,
FTO/block-TiO2/meso-TiO2 substrates were treated
with the UV-ozone for 5 min.In order to prepare the perovskite
precursor solution, PbI2 (1.1 M), FAI (1 M), MABr (0.2
M), CsI (0.05 M), and PbBr2 (0.22 M) were dissolved in
anhydrous DMF: DMSO solvent (4:1
volume ratio). The Cs0.05 (MA0.17 FA0.83)0.95 Pb(I0.83 Br0.17)3 perovskite layer was coated on FTO/compact TiO2/ mesoporous
substrates through a two-step spin-coating at 1000 rpm for10s and
4000 rpm for 20s, respectively. The chlorobenzene antisolvent was
gently poured at the final 5 s of the second step. Also, some perovskite
layers were prepared by utilizing a modified antisolvent material.
Modified antisolvent was prepared by stirring chlorobenzene, TEOS,
and deionized water with volume ratios of 2000, 15, and 3, respectively.
The as-prepared perovskite layers were heated at 100 °C for 1
h. A thin layer of Spiro-OMeTAD hole-transport layer was spin-coated
at 500 rpm for 30 s from a solution containing 72.3 mg Spiro-OMeTAD
(99.5%, Borun Co, China) in 1 mL of chlorobenzene, 28.8 μL 4-tert-butylpyridin (Sigma-Aldrich), and 17.5 μL of
a 1.8 M LiTFSI solution in acetonitrile. Finally, gold contacts (∼100
nm thickness) were thermally deposited to complete the devices.
Characterization Methods
X-ray diffraction
patterns
were acquired by X’Pert Pro MPD equipment with Cu Kα
(λ = 1.54 Å) radiation. SEM micrographs were recorded using
a MIRA3 TESCAN field-emission scanning electron microscope. Optical
properties of the perovskite layers were taken with a PerkinElmer
Lambda 25 spectrophotometer. The photocurrent–voltage measurements
were performed under standard AM 1.5 (1000 W/m2) simulated
light radiation by a Sharif solar SIM-1000 system (calibrated by a
Thorlabs photodiode). The J–V curves were recorded by a Keithley
2400 digital SourceMeter while the cells were masked during the measurement
with an active area of 0.09 cm2. SCLC measurements were
conducted on the hole-only devices with an ITO/NiOx/perovskite/CIS/Au
architecture. NiO and CIS layers were
prepared according to the methods that we explained before.[54,55] For the steady-state photoluminescence (PL) measurements, samples
were excited by a 350 nm laser, and emissions were acquired by an
Avaspec 2048 TEC spectrophotometer. Electrochemical impedance spectroscopy
(EIS) measurements were performed using Sharif Solar PGE-18 potentiostat/galvanostat
in open circuit voltage and a frequency range between 1 Hz and 1 MHz
with an AC amplitude of 20 mV. Extracted Nyquist plots from the EIS
measurements were fitted with appropriate equivalent circuit models
in Zview software.
Authors: Yu Yu; Songwang Yang; Lei Lei; Qipeng Cao; Jun Shao; Sheng Zhang; Yan Liu Journal: ACS Appl Mater Interfaces Date: 2017-01-18 Impact factor: 9.229
Authors: Julian Burschka; Norman Pellet; Soo-Jin Moon; Robin Humphry-Baker; Peng Gao; Mohammad K Nazeeruddin; Michael Grätzel Journal: Nature Date: 2013-07-10 Impact factor: 49.962
Authors: Eric T Hoke; Daniel J Slotcavage; Emma R Dohner; Andrea R Bowring; Hemamala I Karunadasa; Michael D McGehee Journal: Chem Sci Date: 2014-11-04 Impact factor: 9.825