Leyre Gomez1, Junhao Lin2, Chris de Weerd1, Lucas Poirier1, Simon C Boehme3, Elizabeth von Hauff3, Yasufumi Fujiwara4, Kazutomo Suenaga2, Tom Gregorkiewicz1. 1. Institute of Physics, University of Amsterdam , Science Park 904, 1098 XH Amsterdam, The Netherlands. 2. National Institute of Advanced Industrial Science and Technology (AIST) , AIST Central 5, Tsukuba 305-8565, Japan. 3. Department of Physics and Astronomy, Vrije Universiteit Amsterdam , De Boelelaan 1081, 1081 HV Amsterdam, The Netherlands. 4. Division of Materials and Manufacturing Science, Graduate School of Engineering, Osaka University , 2-1 Yamadaoka, Suita, Osaka 565-0871, Japan.
Abstract
All-inorganic cesium lead halide perovskite nanocrystals are extensively studied because of their outstanding optoelectronic properties. Being of a cubic shape and typically featuring a narrow size distribution, CsPbX3 (X = Cl, Br, and I) nanocrystals are the ideal starting material for the development of homogeneous thin films as required for photovoltaic and optoelectronic applications. Recent experiments reveal spontaneous merging of drop-casted CsPbBr3 nanocrystals, which is promoted by humidity and mild-temperature treatments and arrested by electron beam irradiation. Here, we make use of atom-resolved annular dark-field imaging microscopy and valence electron energy loss spectroscopy in a state-of-the-art low-voltage monochromatic scanning transmission electron microscope to investigate the aggregation between individual nanocrystals at the atomic level. We show that the merging process preserves the elemental composition and electronic structure of CsPbBr3 and takes place between nanocrystals of different sizes and orientations. In particular, we reveal seamless stitching for aligned nanocrystals, similar to that reported in the past for graphene flakes. Because the crystallographic alignment occurs naturally in drop-casted layers of CsPbX3 nanocrystals, our findings constitute the essential first step toward the development of large-area nanosheets with band gap energies predesigned by the nanocrystal choice-the gateway to large-scale photovoltaic applications of inorganic perovskites.
All-inorganic cesium lead halideperovskite nanocrystals are extensively studied because of their outstanding optoelectronic properties. Being of a cubic shape and typically featuring a narrow size distribution, CsPbX3 (X = Cl, Br, and I) nanocrystals are the ideal starting material for the development of homogeneous thin films as required for photovoltaic and optoelectronic applications. Recent experiments reveal spontaneous merging of drop-casted CsPbBr3 nanocrystals, which is promoted by humidity and mild-temperature treatments and arrested by electron beam irradiation. Here, we make use of atom-resolved annular dark-field imaging microscopy and valence electron energy loss spectroscopy in a state-of-the-art low-voltage monochromatic scanning transmission electron microscope to investigate the aggregation between individual nanocrystals at the atomic level. We show that the merging process preserves the elemental composition and electronic structure of CsPbBr3 and takes place between nanocrystals of different sizes and orientations. In particular, we reveal seamless stitching for aligned nanocrystals, similar to that reported in the past for graphene flakes. Because the crystallographic alignment occurs naturally in drop-casted layers of CsPbX3 nanocrystals, our findings constitute the essential first step toward the development of large-area nanosheets with band gap energies predesigned by the nanocrystal choice-the gateway to large-scale photovoltaic applications of inorganic perovskites.
Metalhalide semiconductors
with a perovskite structure currently captivate much interest because
of their attractive optical and electrical properties (broad range
of band gap energy values, high emission efficiency, high carrier
mobilities, and simple and low-cost synthesis). Most research effort
is focused on hybrid organic–inorganic perovskites (e.g., CH3CH3PbI3, CH3NH3PbI3, etc.). For large-scale applications, in photovoltaics
(PV) for instance, excellent long-term (chemical and structural) stability
under operating conditions is an absolute necessity. However, this
represents a considerable challenge for the hybrid perovskites.Recently, the synthesis of all-inorganic cesium lead halideperovskite
nanocrystals (CsPbX3 with X = Cl, Br, and I; IP-NCs) has
been developed.[1] This material combines
the advantages of perovskites (low-temperature/low-cost production
and band gap tuning by composition) with the typical NC characteristics
induced by quantum confinement (band gap tuning by size, energy transfer,
and a possibility of surface functionalization).[2,3] Furthermore,
IP-NCs feature a high photoluminescence quantum yield (PL QY = 50–90%)
and narrow emission bands with a tunability over the whole visible
range.[4,5] At the same time, being free from any organic
element, the IP-NCs are more stable than hybrid perovskites, which
makes them attractive for PV as well as optoelectronic applications:
solar cells, LEDs, lasers, and detectors.[6−9] Although IP-NCs allow for the
engineering of electronic states, carrier interactions, and dynamics,
their conductivity in quantum solids built of semiconductor NCs is
typically rather poor because of the presence of a confining potential,
which introduces a barrier for carrier transport. This serious disadvantage
has prevented a broader application of semiconductor NCs for solar
cells in the past. However, the recent demonstration of a stable solar cell based on CsPbI3 NCs forming thin layers with superior electrical properties[9−11] offers a new hope. This development directly illustrates that to
fabricate a superior device based on NCs and in particular on IP-NCs,
they need to form stable thin layers with good electrical contact
between individual NCs of the highest quality.The sintering
of metal nanoparticles by different processes (high-temperature, pressure-driven,
microwave or laser radiation, etc.),[12−15] even at room temperature,[16−18] has been investigated in the past. Similarly, aggregation of semiconductor
NCs into 2D sheets has been reported.[19,20] Nevertheless,
the spontaneous merging of IP-NCs passivated by long-alkyl chain ligands
is considered as a structural instability[21,22] rather than the initial step for the formation of homogeneous thin
layers—to the best of our knowledge. From our previous investigations
of IP-NCs, we concluded that the effective coupling between proximal
CsPbBr3 NCs in an ensemble leads to their band structure
modification[23] and to an efficient energy
transfer.[24] Therefore, IP-NCs are excellent
candidates for custom-designed quantum structures and solids which
could be realized by purposeful assemblage of individually characterized
and selected NCs serving as building blocks.[25] Because of their cubic shape and a narrow size distribution, IP-NCs
are ideally suited to form close-packed layers and/or multilayer structures.
Moreover, closely packed proximal IP-NCs merge together, forming larger
structures. We conclude that IP-NCs with a high “defect tolerance”[26] could possibly be used for the development of
thin films, which are highly attractive for solar cells and optoelectronic
applications.In the present work, we investigate the aggregation
process of individual IP-NCs at the atomic scale. By using state-of-the-art
annular dark-field (ADF) imaging and electron energy loss spectroscopy
(EELS) in an aberration-corrected scanning transmission electron microscope
(STEM), we show the microscopic details of the stitching between individual
IP-NCs of different sizes and crystallographic orientations. This
finding constitutes the first and the most essential step toward the
development of high-quality thin films of IP-NCs, whose properties
can be tuned by selecting appropriate NCs. More generally, the event
of the well-controlled aggregation of NCs paves the way toward advanced
concepts of purposeful assemblage of nano-objects into larger structures.
Materials and Methods
Materials
Cesium carbonate (Cs2CO3 99.9%, Sigma-Aldrich), octadecene (ODE 90%, Sigma-Aldrich), oleic
acid (OA 90%, Sigma-Aldrich), oleylamine (OLA 80–90%, Acros),
lead(II) bromide (PbBr2 98%, Sigma-Aldrich), and toluene
(ACS reagent ≥99.5%, Sigma-Aldrich) were used with no further
purification, except for the drying period reported in the synthesis
procedure.
Synthesis of CsPbBr3 NCs
First, Cs-oleate was prepared by the reaction
of 814 mg of Cs2CO3 with 40 mL of ODE and 2.5
mL of OA at 150 °C; the reactants were previously dehydrated
for 1 h at 120 °C. For the production of CsPbBr3 NCs,
30 mL of ODE and 700 mg of PbBr2 were dried for 1 h at
120 °C under a N2 atmosphere. After water removal,
5 mL of dried OLA and 5 mL of dried OA were added to the reaction
flask, and the temperature was raised up to 160 °C. After complete
solvation of the PbBr2 salt, 4 mL of Cs-oleate solution
previously warmed was injected. A few seconds later, the NC solution
was quickly cooled down with an ice bath. The product was purified
by repeated centrifugation and redispersion in toluene.
Merging Experiments
We drop-casted the IP-NC samples
on amorphous carbon/graphene TEM grids and stored them at room conditions
for the spontaneous merging of NCs to occur. Room conditions refer
to a typical ambient environment with moderate humidity. To probe
the effect of humidity, we drop-casted the same amount of colloidal
NC solution onto two identical grids and stored them separately under
lower (∼20%) and higher (∼60%) relative humidity (RH)
conditions, at room temperature. To test the effect of temperature,
we used a cooling or heating in situ sample holder (Gatan) to reach
the temperature ranges between −110 °C to 90 °C
and 90 °C to 260 °C, respectively. The electron beam-irradiated
samples/areas were exposed to the electron beam directly after drop-casting
and subsequent cooling or heating.For the electrical measurements,
the films were fabricated by drop-casting the NC dispersion onto Au-interdigitated
electrodes with a 5 μm channel width (DropSens G-IDEAU5). Immediately
before drop-casting, the electrodes were electrochemically cleaned
in H2SO4.
Characterization
The optical density was measured in a LAMBDA 950 UV/VIS/NIR spectrophotometer
(PerkinElmer). A combination of tungsten-halogen and deuterium lamps
was used together with PMT and Peltier-cooled PbS detectors, to provide
a detection range of Edet = 0.4–5.6
eV. For reference, the absorption of the solvent was measured separately
and subsequently subtracted from that of the colloid dispersion.The PL spectra were recorded using a Jobin Yvon FluoroLog spectrofluorometer
(Horiba) equipped with a 450 W xenon lamp (250–700 nm) coupled
to a monochromator to provide a range of selective excitation wavelengths.
The emission was collected in right-angle geometry and automatically
corrected for the spectral sensitivity of the setup. To determine
the PL QY, the samples were placed in an integrating sphere, using
a 150 W xenon lamp coupled to a spectrometer (Solar, MSA-130) as an
excitation source. The PL emission and excitation lights were scattered
diffusively in the integrating sphere and were detected by a CCD (Hamamatsu).Scanning transmission electron microscopy (STEM)–EELS spectra
were obtained in a low-voltage JEOL-2100F with a double delta corrector,
which has a probe size of around 1.4 Å, and in a low-voltage
JEOL-ARM60 with a double Wien filter monochromator offering an ultrahigh
spatial and energy resolutions of around 1.4 Å and 50 meV, respectively.
Current–voltage measurements were performed at a scan rate
of 47 mV/s, with a Keithley 2400 source meter and a home-made LabVIEW
program.Frequency-resolved electrical measurements were performed
in the dark, at a bias voltage of 0 V and an ac amplitude of 20 mV,
using a Metrohm-Autolab electrochemical impedance spectroscopy setup
(PGSTAT302N) equipped with a FRA32M module.
Preliminaries
The
synthesis of CsPbBr3 NCs was carried out following the
protocol reported by Protesescu et al.,[1] which was slightly modified. The green-emitting perovskites, stabilized
with OLA and OA on their surface, show a narrow emission band centered
at 520 nm (2.38 eV), with a small Stokes shift from the corresponding
absorption spectrum (Figure a). Figure b shows the energy-dispersive X-ray spectrometry (EDXS) spectrum
indicating the presence of Cs, Pb, and Br in a 1:1:3 ratio, hence
confirming the perovskite ABX3 elemental composition.[27] A fresh sample, drop-casted on an amorphous
carbon/graphene grid, reveals the presence of cubic IP-NCs with a
narrow size distribution of 8.1 ± 1.2 nm (Figure a). The NCs arrange themselves in ordered
square geometries, in some analogy to the honeycomb superlattices
of PbSe NCs.[28] Despite being clearly separated
by surface ligand layers, neighboring IP-NCs effectively couple, modifying
the energy structure of each other.[23] When
stored at room conditions, the NC layer spontaneously aggregates,
with individual IP-NCs merging into larger structures (Figure b). Eventually, after a sufficiently
long time, a semicontinuous layer of rather poor homogeneity is formed
(Figure c). In the
case of a NC layer of low density, isolated nanoplatelets appear.
When the storage time is increased to 6 months (Figure d), the NCs can arrange in very long nanowires
(aspect ratios of ∼100 and higher), although individual NCs
are still visible; to grow a large homogenous film of merged NCs,
other parameters (humidity, temperature, etc.) should be considered
as we will reveal along this paper. We have observed this aggregation
process in the layers of IP-NCs of different sizes and chemical compositions.
It is important to note that upon merging, their chemical composition
is maintained (see Figure S1 of the Supporting Information), which implies that no chemical reactions are
involved and that larger IP platelets are created. At the same time,
we observe that the merging of individual IP-NCs changes the optical
properties of a layer, red-shifting its PL spectrum and absorption
edge. We evaluated this effect using a drop-casted layer of CsPbBr3 NCs on a quartz substrate (Figure S2). In addition, the merging process leads to a reduction of the PL
QY (Figure S3). The effect of exposure
to light and air on the NC aggregation has also been observed (Figures S4). The sample stored for 1 week in
the dark in an inert gas atmosphere exhibited a negligible change
in the PL QY, whereas the sample stored in air while being constantly
illuminated showed a major QY decrease, by a factor of 6.[21]
Figure 1
Optical spectroscopy and structural characterization of
ensemble CsPbBr3 NCs. (a) Absorption and PL spectra of
colloidal NCs in toluene. (b) EDXS spectra confirming the ideal perovskite
composition Cs:Pb:Br = 1:1:3 (integrated area under the respective
peaks), without a notorious presence of Cs4PbBr6.[27]
Figure 2
ADF–STEM images of drop-casted CsPbBr3 NCs on an
amorphous carbon/graphene grid. (a) Fresh drop-casted sample. (b)
Same sample after being stored at room conditions for a week. (c)
Another region of merged NCs; the inset shows the fast Fourier transformation
pattern, demonstrating the misorientation from different small domains.
(d) Sample stored at room conditions for 6 months.
Optical spectroscopy and structural characterization of
ensemble CsPbBr3 NCs. (a) Absorption and PL spectra of
colloidal NCs in toluene. (b) EDXS spectra confirming the ideal perovskite
composition Cs:Pb:Br = 1:1:3 (integrated area under the respective
peaks), without a notorious presence of Cs4PbBr6.[27]ADF–STEM images of drop-casted CsPbBr3 NCs on an
amorphous carbon/graphene grid. (a) Fresh drop-casted sample. (b)
Same sample after being stored at room conditions for a week. (c)
Another region of merged NCs; the inset shows the fast Fourier transformation
pattern, demonstrating the misorientation from different small domains.
(d) Sample stored at room conditions for 6 months.Also, the electrical properties are influenced
by the merging. To investigate that, we drop-casted IP-NCs on interdigitated
electrodes (5 μm width) and measured the current–voltage
characteristics after 1 h, 1 day, and 9 days of storage in air (see Figure S5). We note that while the fresh drop-casted
film is conductive, the NC aggregation increases its resistivity,
as the merging of individual IP-NCs into larger clusters leads to
the formation of voids, which disrupt the percolative pathways across
the 5 μm distance between the electrodes. This problem could
possibly be addressed by adding successive layers of NCs to fill in
those voids.
Microscopic Investigations
and Discussion
To understand the merging process of IP-NCs
in some detail, we performed experiments at a microscopic level. For
that purpose, a CsPbBr3 NC dispersion in toluene has been
drop-casted on an amorphous carbon/graphene TEM grid for high-resolution
ADF–STEM imaging.We start the investigation comparing
the EELS spectra of fresh drop-casted (Figure a) and merged (Figure b) IP-NCs. Using EELS, it is possible to
measure the band-to-band absorption of individual NCs. The EELS spectrum
shows a characteristic onset, which arises from the excitation of
a valence band electron to the conduction band, defining the band
gap energy.[23] For a fresh drop-casted film,
before merging, the accumulated EELS signal measured at different
points of the layer represents the sum of the (averaged) absorption
by neighboring NCs. The EELS spectra showing the measurements collected
at different points for the fresh drop-casted NC layer and for the
semiuniform film formed by merging are presented in Figure c. The EELS data for both configurations
feature a similar absorption behavior, with the characteristic onset
at the band gap energy, in analogy to the optical density of a bulk
semiconductor. Comparing the two spectra, the band gap energy slightly
red-shifts (∼60 meV) upon merging (Efresh = 2.45 eV and Emerged = 2.39 eV), approaching
the bulk value[29] (Ebulk = 2.32 eV). We note that the aggregated IP film still
exhibits a small quantum confinement induced by its nanometer-range
thickness.[23]
Figure 3
Comparison of the absorption
of a fresh drop-casted sample and a 1 week old region of the film,
investigated by EELS. (a) ADF–STEM image of the fresh drop-casted
CsPbBr3 NCs. (b) Similar but different region (unexposed
to the electron beam) of the sample after 1 week of storage at room
conditions after which the NCs have merged. (c) Local low-loss (LL)-EELS
spectra averaged over the regions shown in panels a (blue spectrum)
and b (red spectrum), with the band gap energy values extracted from
their first derivatives, 2.45 and 2.39 eV, respectively.
Comparison of the absorption
of a fresh drop-casted sample and a 1 week old region of the film,
investigated by EELS. (a) ADF–STEM image of the fresh drop-casted
CsPbBr3 NCs. (b) Similar but different region (unexposed
to the electron beam) of the sample after 1 week of storage at room
conditions after which the NCs have merged. (c) Local low-loss (LL)-EELS
spectra averaged over the regions shown in panels a (blue spectrum)
and b (red spectrum), with the band gap energy values extracted from
their first derivatives, 2.45 and 2.39 eV, respectively.Subsequently, we zoom-in to reveal more details
of the merging between individual IP-NCs. Figure a shows a high-resolution ADF–STEM
image of a dense layer of fresh drop-casted NCs. For some NCs, linear
defects can be distinguished, as indicated by the arrows; these could
indicate the NC growth process. The merging process is very evident
when we inspect the film that was stored for a week. Figure b,c shows that the aggregation
process connects NCs not only of the same but also of a different
orientation and that the size of joining NCs does not seem to play
a role. A more careful inspection of the images reveals that the new
structures appear to be of high crystallinity, without borders between
the merging NCs (Figure b), whereas for some connecting NCs, clear boundaries are present
(Figure c).
Figure 4
High-resolution
images of a dense layer of CsPbBr3 NCs. (a) Line defects
are found in some NCs, identified with arrows. (b) Connected NCs share
the same orientation, in this case, along the [001] direction. (c)
Boundaries at the connections are clearly visualized.
High-resolution
images of a dense layer of CsPbBr3 NCs. (a) Line defects
are found in some NCs, identified with arrows. (b) Connected NCs share
the same orientation, in this case, along the [001] direction. (c)
Boundaries at the connections are clearly visualized.The ultimate illustration of the aggregation process
is provided by imaging at a single-NC level. Figure a shows a large IP-NC, with the edge exceeding
50 nm. For reference, also a 6 nm edge size NC from the originally
drop-casted layer is shown (Figure b). We conclude that in this case, the merge is ideal,
creating an apparently monocrystalline structure throughout the whole
cluster. A similar seamless stitching has been reported before for
graphene flakes, in which case, the mutual orientation of the individual
flakes was crucial.[30] Here, the necessary
alignment of individual IP-NCs with respect to each other is conveniently
facilitated by spontaneous formation of the square superlattice in
the drop-casted layer (see Figure a). Figure also illustrates that, as noticed already before, merging
of individual NCs can also occur in other configurations, with a tilted
angle (Figure c,d)
or with a different zone axis (Figure e). Therefore, we conclude that the stitching can occur
between all neighboring NCs, independently of their sizes and orientations.
This random stitching could be advantageous because it means that
all neighboring NCs will fuse, creating a continuous thin perovskite
film. A noncrystalline surface layer, which we identify with the stabilizing
ligands, can be observed around the newly formed structures. This
implies that the ligands do not disappear upon merging but merely
relocate, increasing the amount of hydrocarbon chains at the edge
of the larger assemblies. We conclude that the growth of clusters
and also the subsequent development of large structures, such as long
nanowires and extensive semicontinuous thin films of IP-NCs, proceed
by sequential merging of individual NCs and not by, for example, Ostwald
ripening, as the NCs merge together and not gradually dissolve in
one another.
Figure 5
High-resolution ADF–STEM images of single and merged
IP-NCs. (a) Large CsPbBr3 NC made by the merging of small
NCs. (b) Original NC synthesized by wet chemistry. (c) NCs merged
with the same crystal orientation but a different tilting angle. (d)
Small and large NCs merged with a different tilting angle. (e) Two
NCs of a similar size merged with a different zone axis.
High-resolution ADF–STEM images of single and merged
IP-NCs. (a) Large CsPbBr3 NC made by the merging of small
NCs. (b) Original NC synthesized by wet chemistry. (c) NCs merged
with the same crystal orientation but a different tilting angle. (d)
Small and large NCs merged with a different tilting angle. (e) Two
NCs of a similar size merged with a different zone axis.Although the formation of perfectly uniform and
crystalline large structures is possible by seamless stitching, as
illustrated in Figure , in general, the merged IP-NC film can be viewed as a large plate
with numerous smaller and larger (mono)crystalline domains formed
by aggregation, with their grain boundaries containing multiple structural
imperfections (Figure c).[31] Using the superior spatial resolution
of EELS, we can now investigate the effect of these grain-boundary-related
defects on the electronic band structure of the film. To achieve that,
we select a particular “imperfectly” merged cluster
(with clear boundaries between connecting NCs) and monitor the EELS
spectrum as we scan the electron beam between individual grains, across
the interface. The experiment shows that the absorption spectra obtained
by the locally conducted EELS are practically identical over the whole
investigated trajectory within the IP cluster. This is illustrated
in Figure , which
compares three different spectra taken in the middle of the two adjacent
grains and at their interface; a very close similarity is evident.
Moreover, we notice that the EELS measurements of the merged film
yield spectra that are practically unaltered from those of individual
IP-NCs which we reported previously.[23] A
particularly striking feature is that the interface apparently does
not introduce significant amounts of defects in the band gap nor disturbs
the band structure close to the band edges. This implies that even
the obviously imperfect boundary arising upon layer formation does
not yield defects which would strongly influence the transport properties
of the film and its performance in a solar cell (see also Figure S6). This truly microscopic finding is
essential for the photovoltaic potential of IP layers created by aggregation
of NCs. In the broader context of all perovskite materials currently
vividly explored for solar cells, this finding provides also an important
clue concerning the microscopic origin of the good mobilities and
apparent defect tolerance of these materials. We conclude that the
spontaneous orderly aggregation of IP-NCs offers a unique opportunity
to create nanosheets (nanometer thick IP layers exhibiting quantum
confinement-related effects) whose characteristics can be predefined
(tuned) by the properties of the used IP-NCs. In the future, the deposition
of IP-NC layers could be conveniently controlled by jetting.[32,33]
Figure 6
EELS
scan across the boundaries between merged NCs. (a) ADF image of merged
CsPbBr3 NCs with visible boundaries and (b) their corresponding
EELS spectra. There is no noticeable difference in the absorption
behavior and band gap energy observed, where the boundary of merged
NCs (green) and a smooth part of the film (blue and red) are compared.
EELS
scan across the boundaries between merged NCs. (a) ADF image of merged
CsPbBr3 NCs with visible boundaries and (b) their corresponding
EELS spectra. There is no noticeable difference in the absorption
behavior and band gap energy observed, where the boundary of merged
NCs (green) and a smooth part of the film (blue and red) are compared.Having established the microscopic
formation mechanism of IP nanosheets and their remarkable characteristics,
we turn our attention to the practical aspects of the merging process.
In general, the self-assembly of NCs drop-casted or spin-coated on
a substrate from a colloidal solution is governed by interactions
between the NCs and with the substrate, solution/substrate interface,
drying kinetics (solvent- and temperature-dependent), among others.[34−36] The contact between colloidal semiconductor NCs themselves is facilitated
by van der Waals forces, which are weak and can easily be overcome
by steric repulsions using stabilizing ligands.[37] Nevertheless, the highly dynamic behavior of the IP-NC
surface ligands (the binding is not strong, and they can move and
be easily lost, mainly during the purification process) besides the
ionic character of the IP-NC structure makes this material breakable
in polar solvents.[38] These characteristics
are important for manipulating and eventually controlling the assemblage
of IP-NCs. In the following section, we present how electron bean
irradiation, humidity, and thermal annealing at different temperatures
influence the aggregation process.Electron irradiation can
affect the ligands that are present at the surface of the deposited
IP-NCs, leading to the formation of intermolecular C=C bonds
between them and also between the ligands and the carbonaceous grid;[39] in both cases, the IP-NC stability would be
enhanced. This is indeed confirmed in our experiments: Figure a,b shows the images of drop-casted
IP-NC stored for 1 week at room conditions; the left part is exposed
to an electron beam directly after deposition, whereas the right-hand
side is not. As can be seen, the NC aggregation has taken place only
in the nonirradiated part of the sample, thus illustrating the stabilizing
action of the electron beam.
Figure 7
Influence of electron beam irradiation and mild-temperature
annealing on the IP-NCs merging. (a) One week-aged high-IP-NCs density
layer sample, being partially irradiated with electrons just after
deposition—left side of the image, and without previous irradiation—right
side of the iamge. (b) Lower IP-NCs density layer annealed at 90 °C
for 1 h, being partially irradiated with electrons just after deposition—left
side of the image, and no previous irradiation—right side of
the image. (c) IP-NCs annealed at 90 °C for 1 h without previous
electron irradiation. (d) Zoom-in of the sample in c.
Influence of electron beam irradiation and mild-temperature
annealing on the IP-NCs merging. (a) One week-aged high-IP-NCs density
layer sample, being partially irradiated with electrons just after
deposition—left side of the image, and without previous irradiation—right
side of the iamge. (b) Lower IP-NCs density layer annealed at 90 °C
for 1 h, being partially irradiated with electrons just after deposition—left
side of the image, and no previous irradiation—right side of
the image. (c) IP-NCs annealed at 90 °C for 1 h without previous
electron irradiation. (d) Zoom-in of the sample in c.Typically, aggregation processes are strongly temperature-dependent,
and this is also the case for the IP-NC layers, with their merging
being accelerated by mild-temperature treatments due to the removal
of surface ligands.[21] At the macroscopic
level, this is evidenced by the fact that IP-NC films on quartz treated
at mild temperatures show a decrease of the emission intensity and
PL QY because of the defect formation (see Figure S7), in agreement with previous reports.[21,40] Here, we investigate this effect at the microscopic level. Figure b shows the behaviors
of electron-irradiated and nonirradiated regions of a low-concentration
IP-NC layer, annealed at 90 °C for 1 h. Whereas the NCs in the
electron-irradiated region remain isolated, the merging process in
the untreated part of the sample is clearly enhanced. When the initial
NC density is high, the same treatment results in a complete fusion
of individual NCs into a semicontinuous film (Figure c,d). For the development of high-quality
layers, the annealing temperature will need to be optimized, as high-temperature
treatments destroy the IP-NCs (see Figure S8). In Figure a, small
clusters of 14 NCs are imaged directly after drop-casting; an amorphous
layer of ligands is clearly visible on the individual NC surface.
The electron irradiation stabilizes the ligands, as discussed before,
arresting the possible merging. Figure b shows the same cluster after being heated at 260
°C for 1 h: the IP-NCs have been completely destroyed, with a
small metallic nanoparticle being formed from the IP-NC debris, whereas
the residual shell of ligands remains, now around the empty spaces.
Figure 8
Effect
of annealing IP-NCs at a high temperature. (a) ADF–STEM image
of 14 CsPbBr3 NCs. (b) Same IP-NCs after 1 h of annealing
treatment at 260 °C; just remaining the residual ligands and
a metallic nanoparticle (bright dot).
Effect
of annealing IP-NCs at a high temperature. (a) ADF–STEM image
of 14 CsPbBr3 NCs. (b) Same IP-NCs after 1 h of annealing
treatment at 260 °C; just remaining the residual ligands and
a metallic nanoparticle (bright dot).Past research has shown that ethanol influences the growth
of IP-NCs through surface ligand destabilization[41] and can induce partial dissolution and subsequent recrystallization
of IP-NCs—the effect which can serve for healing of the film.[42] To investigate the effect of water vapor on
the NC merging, we compared two samples stored for 1 week in dry (RH
= 20%) and high-humidity atmospheres (RH = 60%). The results (Figure ) clearly show that
the water vapor accelerates the NC fusion process. Because water actually
dissolves the perovskites and in that way destroys the IP-NCs, specific
investigations are necessary to determine the optimal RH level for
the merging process, similarly as for the thermal treatment.
Figure 9
Effect of the
RH on the merging of IP-NCs. ADF–STEM images of drop-casted
CsPbBr3 NCs stored for 1 week in (a) a vacuum chamber with
RH = 20% and (b) in a humidifier with RH = 60%.
Effect of the
RH on the merging of IP-NCs. ADF–STEM images of drop-casted
CsPbBr3 NCs stored for 1 week in (a) a vacuum chamber with
RH = 20% and (b) in a humidifier with RH = 60%.
Conclusions
Colloidal IP-NCs drop-casted
on a substrate form spontaneously a semihomogeneous thin film. A thorough
microscopic investigation by our state-of-the-art ADF microscopy and
EELS reveals that the layer formation proceeds by merging of individual
NCs. We show that the fusion is accelerated by mild-temperature annealing
in a humid atmosphere. Surface ligands play an active role in the
aggregation process, which is arrested or totally prevented by their
stabilization, for example, upon electron irradiation. Most importantly,
at the atomic level, we find that the merging process does not introduce
an appreciable defect concentration in the band gap or at the band
edges, and even near-perfect seamless stitching between the aligned
NCs is possible. Because crystallographic alignment naturally arises
in drop-casted dense layers of IP-NCs, this implies that in the future,
this process could be explored for formation of thin IP films of superior
quality. Our results demonstrate the fundamental condition growth
for the development of these sheets, the seamless stitching; future
research must show whether it is also “sufficient”;
that is, if it can be extended to grow long thin films. In that way,
the current findings certify the high potential of IP-NCs for practical
applications in future thin-film PV. In a broader context, they pave
the way toward dedicated engineering of high-quality thin IP films,
creating custom-designed quantum structures by purposeful assemblage
of individually characterized and selected NCs.
Authors: M P Boneschanscher; W H Evers; J J Geuchies; T Altantzis; B Goris; F T Rabouw; S A P van Rossum; H S J van der Zant; L D A Siebbeles; G Van Tendeloo; I Swart; J Hilhorst; A V Petukhov; S Bals; D Vanmaekelbergh Journal: Science Date: 2014-05-29 Impact factor: 47.728
Authors: Jonathan De Roo; Maria Ibáñez; Pieter Geiregat; Georgian Nedelcu; Willem Walravens; Jorick Maes; Jose C Martins; Isabel Van Driessche; Maksym V Kovalenko; Zeger Hens Journal: ACS Nano Date: 2016-01-26 Impact factor: 15.881
Authors: Alexandre Teulle; Michel Bosman; Christian Girard; Kargal L Gurunatha; Mei Li; Stephen Mann; Erik Dujardin Journal: Nat Mater Date: 2014-10-26 Impact factor: 43.841
Authors: He Huang; Maryna I Bodnarchuk; Stephen V Kershaw; Maksym V Kovalenko; Andrey L Rogach Journal: ACS Energy Lett Date: 2017-08-10 Impact factor: 23.101
Authors: Francisco Palazon; Francesco Di Stasio; Quinten A Akkerman; Roman Krahne; Mirko Prato; Liberato Manna Journal: Chem Mater Date: 2016-04-19 Impact factor: 9.811
Authors: Biplab K Patra; Harshal Agrawal; Jian-Yao Zheng; Xun Zha; Alex Travesset; Erik C Garnett Journal: ACS Appl Mater Interfaces Date: 2020-06-30 Impact factor: 9.229