Loredana Protesescu1,2, Sergii Yakunin1,2, Olga Nazarenko1,2, Dmitry N Dirin1,2, Maksym V Kovalenko1,2. 1. Institute of Inorganic Chemistry, Department of Chemistry and Applied Bioscience, ETH Zürich, Vladimir Prelog Weg 1, CH-8093 Zürich, Switzerland. 2. Laboratory for Thin Films and Photovoltaics, Empa-Swiss Federal Laboratories for Materials Science and Technology, Überlandstrasse 129, CH-8600 Dübendorf, Switzerland.
Abstract
Lead halide perovskites of APbX3 type [A = Cs, formamidinium (FA), methylammonium; X = Br, I] in the form of ligand-capped colloidal nanocrystals (NCs) are widely studied as versatile photonic sources. FAPbBr3 and CsPbBr3 NCs have become promising as spectrally narrow green primary emitters in backlighting of liquid-crystal displays (peak at 520-530 nm, full width at half-maximum of 22-30 nm). Herein, we report that wet ball milling of bulk APbBr3 (A = Cs, FA) mixed with solvents and capping ligands yields green luminescent colloidal NCs with a high overall reaction yield and optoelectronic quality on par with that of NCs of the same composition obtained by hot-injection method. We emphasize the superiority of oleylammonium bromide as a capping ligand used for this procedure over the standard oleic acid and oleylamine. We also show a mechanically induced anion-exchange reaction for the formation of orange-emissive CsPb(Br/I)3 NCs.
Lead halide perovskites of APbX3 type [A = Cs, formamidinium (FA), methylammonium; X = Br, I] in the form of ligand-capped colloidal nanocrystals (NCs) are widely studied as versatile photonic sources. FAPbBr3 and CsPbBr3 NCs have become promising as spectrally narrow green primary emitters in backlighting of liquid-crystal displays (peak at 520-530 nm, full width at half-maximum of 22-30 nm). Herein, we report that wet ball milling of bulk APbBr3 (A = Cs, FA) mixed with solvents and capping ligands yields green luminescent colloidal NCs with a high overall reaction yield and optoelectronic quality on par with that of NCs of the same composition obtained by hot-injection method. We emphasize the superiority of oleylammonium bromide as a capping ligand used for this procedure over the standard oleic acid and oleylamine. We also show a mechanically induced anion-exchange reaction for the formation of orange-emissive CsPb(Br/I)3 NCs.
Bottom-up
synthesis methods with surfactant (ligand)-capped colloidal
nanocrystals (NCs), such as high-temperature hot injection or heating
methods, have afforded an unprecedented variety of NC compositions
and morphologies, with a high level of uniformity and narrow size
distribution.[1−5] Colloidal synthesis in apolar solvents has enabled the development
and recent commercial applications of colloidal semiconductor NCs
(also known as quantum dots, QDs) composed of typical binary compound
semiconductors: II–VI (CdS, CdSe, CdTe),[1] III–V (InP, InAs, InSb),[6−9] and IV–VI (PbS, PbSe, PbTe).[10−19] In addition, QDs with high structural complexity have been achieved,
with the most notable examples being core–shell QDs (CdSe/ZnS[5,20] and PbX/CdX,[21−23] X = S, Se, Te), nanowires,[24] nanodisks,[25] nanoplatelets (NPLs),[26] rods, and tetrapots.[27]Unsurprisingly, the most recent addition to the family of
colloidal
QDs, NCs of lead halide perovskites [LHPs; APbX3-type;
A = Cs, formamidinium (FA), methylammonium (MA); X = Br, I] were initially
approached with the same experimental mindset.[28] For example, the first synthesis of CsPbX3 NCs
was accomplished by injecting a Cs precursor into a PbX2 solution at elevated temperatures.[29] Similarly,
highly luminescent FA- and MA-based LHPs were synthesized by injecting
the sources of MA and FA cations.[30,31] Colloidal
Cs- and FA-based LHP NCs[29,31,32] exhibit broadly tunable photoluminescence (PL), spanning the entire
visible spectral range (410–700 nm), small PL line widths (full
width at half-maximum, fwhm, 12–40 nm for blue-to-red), and
high PL quantum yields (QYs, 50%–90%), thus providing a broad
color gamut.LHPs are ionic and are characterized by low formation
and lattice
energies; therefore, they do not require thermal activation during
formation to achieve high crystallinity. Subsequent studies have shown
that the synthesis of colloidal LHP NCs involves a surfactant-controlled
coprecipitation of ions that proceeds with fast kinetics even at room
temperature (RT). Facile formability of LHP NCs has been successfully
achieved using an alternative strategy, the reprecipitation method,
wherein an ionic solution of the respective ions (A+, Pb2+, and X–) in a polar solvent is rapidly
destabilized by mixing with a nonsolvent, inducing a burst of nucleation.
This method was originally proposed for MAPbBr3 NCs[33] and has since been extended to Cs and FA systems.
Noncuboidal shapes, such as NPLs, nanosheets, and nanowires, can also
be obtained using both methods.[34−37]The soft nature of LHPs and their facile crystallization
suggest
that top-down methods might also be applicable for LHP NC preparation.
In this study, we report a simple mechanochemical synthesis of LHP
NCs using a commercial ball mill. Such a synthesis essentially involves
simple mechanical grinding of bulk APbX3 materials or AX
+ PbX2 mixtures in the presence of a solvent (mesitylene)
and ligand (oleylammonium halide, OAmX, or mixture of oleic acid,
OA, and oleylamine, OLA). These ligands are chosen based on their
success in hot-injection synthesis methods.[29,31]High-energy ball milling is a type of mechanical grinding
of materials.
This process can be conducted in a dry (without solvents) or wet (with
solvents) fashion. Laboratory-scale ball milling (5–100 mL
scale) is a batch process, whereas industrial ball mills can be operated
in a continuous mode, thus offering a very high synthesis throughput.
The milling occurs due to mechanical friction between the grinding
medium, such as balls of the same or various sizes, and the ground
material (Figure ).
The container (bowl) and the grinding balls are typically made of
the same, high-hardness material (zirconia, corundum, or stainless
steel). Mechanical energy is provided to the system by the rotary
motion of the bowl, as in the case of a planetary ball mill. The rotation
of the bowl and the speed are optimized such that the maximum speed,
the speed at which balls do not move within the bowl, is not exceeded.
The milling can have diverse effects on the ground material: different
extents of downsizing of the final powder (from microns to tens of
nanometers), efficient mixing (e.g., production of slurries in battery
manufacturing or preparation of pigments), solid-state chemical transformation
(mechanochemical synthesis), or a combination of these effects.[38,39] Wet ball milling is also considered to be a green chemistry approach,
as it does not require high temperatures (energy saving) and consumes
minimal quantities of solvents.[40] Ball
milling has been popular since the 1970s for producing oxide dispersions
such as Al2O3, Y2O3, and
ThO2. Grinding techniques are also widely used for alloying
materials,[41] in the synthesis of metal
oxides,[39,42,43] and for mechanical
exfoliation of graphene.[44] However, in
terms of the synthesis of semiconductor NCs, ball milling has achieved
very limited success (examples include CdSe[45] and CdTe[46]) due to the lack of bright
emission from the resulting QDs. This is because, on the one hand,
ball milling generates numerous structural defects in rigid lattices
of these materials, and on the other hand, it does not allow surface
passivation. The combined effect of the trap states, which are abundant
on the pristine (uncoated) NC surfaces, and other structural defects
leads to very low PL QYs. Therefore, it is necessary to coat conventional
QDs with wide-bandgap materials, such as in the canonical example
of core–shell CdSe-CdZnS NCs, thereby decoupling the excitonic
recombination from the detrimental surface states.
Figure 1
Photographs of (a) a
typical planetary ball mill, (b) zirconia
bowl filled with zirconia balls, and (c) crystals of bulk CsPbBr3 used as starting materials. (d) Schematic of the working
principle of the planetary ball mill showing the horizontal cross-section
of the bowl during the wet ball-milling experiments. The bowl undergoes
two motions: orbital rotation of the entire ball and its simultaneous
spinning. (e) Schematic of the processes occurring during the mechanochemical
synthesis of LHP NCs. Photographs showing the colloid of CsPbBr3 NCs (f) directly after the ball-milling experiment and (g)
after dilution with toluene and filtration (taken under visible light
and under a UV lamp, λ = 365 nm). (h) TEM image of the resulting
CsPbBr3 NCs.
Photographs of (a) a
typical planetary ball mill, (b) zirconia
bowl filled with zirconia balls, and (c) crystals of bulk CsPbBr3 used as starting materials. (d) Schematic of the working
principle of the planetary ball mill showing the horizontal cross-section
of the bowl during the wet ball-milling experiments. The bowl undergoes
two motions: orbital rotation of the entire ball and its simultaneous
spinning. (e) Schematic of the processes occurring during the mechanochemical
synthesis of LHP NCs. Photographs showing the colloid of CsPbBr3 NCs (f) directly after the ball-milling experiment and (g)
after dilution with toluene and filtration (taken under visible light
and under a UV lamp, λ = 365 nm). (h) TEM image of the resulting
CsPbBr3 NCs.On the contrary, LHP NCs are unique in that they do not require
surface passivation with epitaxial wide-bandgap semiconductor layers
for exhibiting bright emission in the green-red spectral region. This
is one of the manifestations of the rare phenomenon of defect tolerance:
structural defects are nearly fully benign with respect to the carrier
dynamics. Theoretical calculations indicate that dominant point defects,
primarily vacancies, in the bulk material,[47] at grain boundaries,[48] and on the NC
surfaces,[49] are all shallow or intraband
(in the valence or conduction bands). Other defects, for instance,
those of the antisite or interstitial type, are not common in perovskites
due to their crystal structure and ionic bonds. Defect tolerance makes
LHPs vastly different from all known types of colloidal QDs and enables
many synthesis pathways for LHP NCs. Besides the mechanochemical synthesis
presented here and by others (see further discussion in the next section),[50,51] perovskite NCs with bright PL were obtained by sonication,[52] microwave irradiation,[53,54] or templating of crystallization using the nanoscale pores of mesoporous
silica.[55]
Results
and Discussion
The goal of this study was to produce highly
luminescent CsPbBr3 and FAPbBr3 NCs in one step
by ball milling. Both
of these nanomaterials can be readily synthesized on microfluidic
platforms[56] and by the hot-injection colloidal
method,[29,31,57,58] ultrasonication,[52] the
reprecipitation method at RT,[59,60] and microwave-assisted
growth.[53,54,61] Mechanochemical
syntheses were initially used only for MAPbI3,[51,62] wherein relatively large micro- and nanoparticles (>200 nm) are
formed on Al2O3 carrier particles. In a recent
report,[50] dry ball milling of CsX and PbX2 powders followed by the addition of OLA yielded luminescent
colloidal NCs. In our own experiments, we were unable to produce stable
and bright colloids with only OLA as the ligand. Also, dry-milling
was ineffective in our experiments, irrespective of the ligands used
afterward or whether bulk APbX3 or AX + PbX2 mixtures were used as starting precursors. Below, we detail our
own study, wherein different ligand systems were used: (i) a mixture
of OLA and OA and (ii) OAmX. These ligand systems are typically used
in colloidal syntheses of perovskite NCs, and the general consensus
is that OAm+ coordinates the surface anions, whereas Br– or oleate anions locate themselves close to surface
cations, thereby maintaining the overall charge neutrality of the
NC.[49,63,64]The
ball-milling method (Figure ) employs two rotational movements: one of the milling
bowl and the other of the supporting disk (on which the bowl with
NCs is mounted). The combined effect enables the efficient movement
of the balls within the bowl, causing grinding of the material. If
only circular motion of the bowl was employed, such as in centrifuges,
all components of the mixture would be statically held by the centrifugal
force. As precursor materials, either a bulk APbX3 compound
or an equimolar mixture of AX and PbX2 is used. The combined effect
of milling and the presence of the capping ligands and solvents allows
for a simple one-step conversion of bulk precursors into colloids
of APbX3 NCs. The optimal milling time at RT and 500 rpm
is dependent on the material: 2 h for CsPbBr3 and 1 h for
FAPbBr3.In a typical experiment (see Methods section
for the detailed protocols), 0.035 mmol of CsPbBr3 or 0.04
mmol of FAPbBr3 was loaded into a zirconia bowl with 25
zirconia balls (4 mm and 5 mm in diameter). OAmBr (0.03 mmol) was
added as the ligand, and 0.4 mL of mesitylene was added as the solvent.
The milling speed was set to 500 rpm and milling time to 2 h (for
CsPbBr3) and 1 h (for FAPbBr3), as found to
be optimal for obtaining NCs (Figure b). Powder X-ray diffraction (XRD) patterns confirmed
the complete conversion of the precursors into nanogranular products
with the expected crystal structure (orthorhombic for CsPbBr3 and cubic for FAPbBr3).
Figure 2
(a) Powder XRD patterns of bulk CsPbBr3 (orange pattern)
used for the ball-milling experiment, and the resulting CsPbBr3 NCs (green pattern) showing an identical orthorhombic perovskite
crystal structure (Pnma space group); (b) photograph
showing the obtained colloidal CsPbBr3 NCs diluted in toluene;
(c) photograph showing the initial bulk CsPbBr3 crystals;
(d) comparison of the XRD patterns of bulk FAPbBr3 (orange
pattern) used for the ball-milling experiment and the resulting FAPbBr3 NCs (green pattern), indicating the retention of the cubic
lattice; (e–h) TEM images of CsPbBr3 NCs and FAPbBr3 NCs at various magnifications.
(a) Powder XRD patterns of bulk CsPbBr3 (orange pattern)
used for the ball-milling experiment, and the resulting CsPbBr3 NCs (green pattern) showing an identical orthorhombic perovskite
crystal structure (Pnma space group); (b) photograph
showing the obtained colloidal CsPbBr3 NCs diluted in toluene;
(c) photograph showing the initial bulk CsPbBr3 crystals;
(d) comparison of the XRD patterns of bulk FAPbBr3 (orange
pattern) used for the ball-milling experiment and the resulting FAPbBr3 NCs (green pattern), indicating the retention of the cubic
lattice; (e–h) TEM images of CsPbBr3 NCs and FAPbBr3 NCs at various magnifications.The ball-to-material weight ratio, wherein “material”
is the mixture of precursors, ligands, and solvents, is an important
parameter for obtaining uniform NCs: the higher the ratio, the shorter
the time required for complete milling of the bulk materials. A broad
range for this parameter is reported in the literature for various
materials (from 1 to 220).[38,65,66] By keeping the number of balls constant and changing the amount
of material, the ball-to-material ratio was varied from 21.7 to 167
(Figure S1). The optimal ball-to-material
weight ratio was found to be 80 [∼10 balls (4 mm) and 15 balls
(5 mm), 0.035 mmol CsPbBr3 (0.04 mmol for FAPbBr3), 0.1 g of OAmBr, 0.4 mL of mesitylene], yielding PL fwhm = 27 nm
for CsPbBr3 NCs (PL peak at 510 nm) after 2 h of milling.
Very long milling times often caused the emergence of mixed shapes,
in particular, a large fraction of NPLs. NPLs were apparent in the
blue-shifted bands in the PL spectra (Figure S2a, Figure S4). For example, for FAPbBr3, NCs with an emission peak at 537 nm could be readily obtained
within 1 h (Figure a). A longer milling (ca. 2 h) time led to the appearance of an emission
peak at 450 nm. This band was dominant in the PL spectrum after 3
h (Figure S2b). OAmBr was the most suitable
ligand for both perovskite materials, giving stable colloidal dispersions
and narrow emission line widths. When only OLA was used, no NCs were
formed (no PL was observed), whereas using OA as the sole ligand yielded
bright suspensions but unstable colloids with fast decay of the PL
QY upon storage. A mixture of OA and OLA allowed the fabrication of
stable colloids of FAPbBr3, but with broader PL line widths
(Figure S3b, fwhm = 34 nm), most likely
due to acid/base equilibrium reactions between the ligands; therefore,
the existence of protonated and unprotonated species in the same time
increased the probability to obtain NCs with a broader size distribution.
The attempts to form CsPbBr3 NCs with OA and OLA resulted
in a mixture of NCs and NPLs (Figure S3a). Other ligands, such as tetraoctylammonium bromide, induced the
formation of bright FAPbBr3 NCs but without satisfactory
colloidal stability (Figure S3). Mesitylene
was identified as the best solvent for colloidal stability; other
tested solvents included octadecene, toluene, diphyl, hexane, and
chloroform. Dry milling, for example, without solvents and ligands,
leads only to poorly luminescent microcrystalline powders.
Figure 3
(a) Absorbance
and PL spectra for CsPbBr3 NCs (green)
and FAPbBr3 NCs (black) obtained using the ball-milling
method. (inset) Photograph of CsPbBr3 NCs under UV lamp
(λ = 365 nm), (b) time-resolved PL of CsPbBr3 NCs
(green) and FAPbBr3 NCs (black) measured in solutions,
(c) absolute QY of CsPbBr3 NCs (green) and FAPbBr3 NCs (black) measured in solutions and films, and (d) decay time
for CsPbBr3 NCs (green) and FAPbBr3 NCs (black)
measured in solutions and films.
(a) Absorbance
and PL spectra for CsPbBr3 NCs (green)
and FAPbBr3 NCs (black) obtained using the ball-milling
method. (inset) Photograph of CsPbBr3 NCs under UV lamp
(λ = 365 nm), (b) time-resolved PL of CsPbBr3 NCs
(green) and FAPbBr3 NCs (black) measured in solutions,
(c) absolute QY of CsPbBr3 NCs (green) and FAPbBr3 NCs (black) measured in solutions and films, and (d) decay time
for CsPbBr3 NCs (green) and FAPbBr3 NCs (black)
measured in solutions and films.Time-resolved PL traces of both CsPbBr3 and FAPbBr3 samples were characterized by multiexponential decay behavior
(Figure b). This could
be explained by the broad size and shape distribution of the NCs after
ball milling. This was also consistent with the broader emission band
observed for NCs obtained by ball milling than for NCs obtained by
hot injection.[29] For CsPbBr3 NCs, the fastest decay component in the biexponential fitting model
was at least 2 times longer than nearly monoexponential decay parameter
for NCs produced by hot injection (10.6 vs 5 ns). FAPbBr3 NCs, however, showed notably faster relaxation times than colloidally
synthesized NCs of the same composition.[31] We associate this to the larger fraction of smaller NCs in the ball-milled
FAPbBr3 product. In smaller NCs, higher quantum confinement
accelerates the radiative rate. The acceleration due to surface states
(the effect is rather common for II–VI QDs) can be ruled out
by the observation of PL QYs. PL QYs were high and similar in solutions
(>75% for CsPbBr3 NCs, >80% for FAPbBr3 NCs).
Films of FAPbBr3 NCs nearly retained their high PL QYs
(>70%), whereas CsPbBr3 NC films exhibited a significant
decrease to 45% (Figure c). High initial QY and better stability in film for FAPbBr3 NCs can be attributed to the better tolerance to defects, lower
density of defects, and also higher defect formation energy.[67] In films of FAPbBr3 NCs, the relaxation
speed was slower than in the solution, as opposed to CsPbBr3 NC, where relaxation is slightly faster than in the corresponding
solution (Figure d).
Such different behavior of NC with organic and inorganic cations can
be explained by the higher tendency of FAPbBr3 NCs to sintering
at room temperature (bulk material has lower melting point) and higher
density of surface defects in CsPbBr3 with lower defect
formation energy.[68]Attempts to compositionally
tune the bandgap by methods such as
milling bulk CsPbBr3 and oleylammonium iodide (OAmI) as
starting materials showed limited success, as the resulting NCs exhibited
low PL QYs. A better approach was to conduct an anion-exchange reaction[32] by adding OAmI to CsPbBr3 NCs (Figure ).
Figure 4
Example of an anion-exchange
reaction performed by adding OAmI
to the bowl immediately after the synthesis of CsPbBr3 NCs
(520 nm). Within several minutes, the PL peak shifted from 520 to
580 nm, indicating the formation of CsPb(Br/I)3 NCs.
Example of an anion-exchange
reaction performed by adding OAmI
to the bowl immediately after the synthesis of CsPbBr3 NCs
(520 nm). Within several minutes, the PL peak shifted from 520 to
580 nm, indicating the formation of CsPb(Br/I)3 NCs.The results of the mechanochemical
synthesis using CsBr and PbBr2 as precursors are illustrated
in Figure and compared
with those of the identical
procedure using the CsPbBr3 precursor. Even after 14 h,
the fwhm of the obtained NCs was 49 nm (centered at ca. 500 nm), indicating
that it was very important to use a bulk ternary compound as a precursor
rather than the mixture of two binary. Using two precursors, we can
expect two simultaneous phenomena: the mechanical downsizing of the
precursors and the chemical reaction between CsBr and PbBr; the nucleation
of CsPbBr3 NCs could be initiated any time during those
processes, and therefore different NCs will have different growth
history, yielding polydisperse ensemble or remanence of some bulk
material. If a shorter ball-milling reaction time is considered (1
h), the obtained NCs with emission at 522 and fwhm of 27 nm were not
colloidally stable. This suspension contained most of the material
in the nonluminescent bulk phase. After it was centrifuged and filtered,
only a highly dilute colloid was obtained (≤1 mg/mL, <5%
of theoretical reaction yield). Hence, the narrow PL band could be
attributed to the strong reabsorption of PL by the bulk material.
Unbalanced kinetics of the formation of new NCs and downsizing of
the earlier formed NCs eventually led to a very broad PL peak.
Figure 5
Comparison
between ball-milling synthesis of CsPbBr3 NCs employing
bulk CsPbBr3 and that employing a mixture
of CsBr and PbBr2 as precursors.
Comparison
between ball-milling synthesis of CsPbBr3 NCs employing
bulk CsPbBr3 and that employing a mixture
of CsBr and PbBr2 as precursors.Finally, we would like to point out that this ball-milling
synthesis
method was essentially inapplicable to iodide systems (CsPbI3 and MAPbI3, Figure S5).
Conclusions
In summary, this study explored the utility
of wet mechanical grinding
for obtaining colloidal NCs of lead halide perovskite. The method
yielded FAPbBr3 and CsPbBr3 NCs with optoelectronic
quality on par with that required for application in the backlighting
of liquid-crystal displays (as the green primary color). The utmost
simplicity and speed of mechanochemical synthesis indicated its utility
for future research. For instance, the fast downsizing achieved by
this synthesis could be used as a general method for testing whether
certain bulk materials, such as soft metal halides, can become bright
emitters in the form of NCs.
Methods
Synthesis
of Bulk CsPbBr3, Adapted from Ref (69)
Bulk CsPbBr3 crystals were obtained from dimethyl sulfoxide (DMSO, 99.8%,
Fluka) solution at 110 °C. First, CsBr (Aldrich, 99.9%) and PbBr2 (99.999%, ABCR) were dissolved in DMSO with [Cs] and [Pb]
of 0.5 and 1 M, respectively. This solution was filtered at RT and
then slowly heated to 110 °C. Typically, numerous sub-millimeter
crystals appeared just above 90 °C and continued to grow with
increasing temperature. After ∼4 h of growth, the crystals
were taken out of the solution, wiped with filter paper to remove
the solvent, and dried overnight in a vacuum oven at 50 °C. Synthesis of bulk FAPbBr3. FA acetate (3.2 mmol,
0.33 g, Aldrich, 99%) was dissolved in 1 mL of HBr (48%, aqueous solution,
Aldrich). PbBr2 (3.2 mmol, 1.174 g, 99.99%, Aldrich) was
dissolved in 2 mL of HBr, and this solution was heated to 80 °C
to fully dissolve the salts. To this warm solution, the FA solution
was added, forming a red precipitate. The mixture was cooled to RT
and centrifuged. The precipitate was rinsed with diethyl ether several
times to remove the residual acid and dried on a filter paper.
Synthesis
of Bulk MAPbI3, Adapted from Ref (70)
Pb(OAc)2·3H2O (11.33 mg, 0.03 mmol, ≥99.99%, Aldrich)
was dissolved in 38.7 mL of hydroiodic acid (HI, 57 wt %, stabilized
with 1.5% H3PO2, ABCR or Aldrich) and heated
to 100 °C in an oil bath. Then, a mixture of 2.52 g of methylamine
aqueous solution (40 wt %, Fluka) and 8.45 mL of HI was added. Small-grained
black powder precipitated within a few minutes. Then, the solution
was cooled to 75 °C and maintained at this temperature for 1
d. The obtained powder was washed with diethyl ether and dried in
vacuum at 25 °C.
Preparation of Oleylammonium Halide (OAmX)[32]
Ethanol (100 mL, Aldrich, absolute,
>99.8%) and
OLA (12.5 mL, Acros Organics, 80%–90%) were combined in a 250
mL two-necked flask and vigorously stirred. The reaction mixture was
cooled in an ice–water bath, and 8.56 mL of HBr (48% aqueous
solution, Aldrich) for preparing OAmBr or 10 mL of HI (HI 57%, Aldrich,
no stabilizer) for preparing OAmI was added. The reaction mixture
was left to react overnight under N2 flow. Then, the solution
was dried under vacuum, and the obtained product was purified by rinsing
several times with diethyl ether. The product (white powder) was obtained
after vacuum-drying at 80 °C overnight.
Mechanochemical Synthesis
of CsPbBr3 NCs
Bulk CsPbBr3 (0.02 g,
0.035 mmol, prepared as described
above) was loaded into a zirconia bowl with 25 zirconia balls (4 mm
and 5 mm) and with OAmBr (0.01 g, 0.03 mmol, prepared as described
above), and 0.4 mL of mesitylene (98%, Sigma-Aldrich). Another tested
ligand system was a mixture of OA (0.05 mL, Sigma-Aldrich, 90%) and
OLA (0.05 mL, Strem, 95%). Other tested solvents were octadecene (Sigma-Aldrich,
90%), Dowtherm A (diphyl, eutectic mixture of 26% diphenyl + 73.5%
dipheniloxide), toluene (Sigma-Aldrich, 99.5%), hexane (>95%, Sigma-Aldrich),
and chloroform (HPLC grade, Fisher Chemicals). The bowl was mounted
on a planetary ball mill (Fritsch, Pulverisette 7, classic line),
and the speed was set to 500 rpm. The time was varied from 30 min
to 24 h. After the milling, a bright green suspension was obtained,
which was diluted with toluene (2 mL) and used as-obtained or precipitated
one time with acetonitrile (0.5 mL, 99.8%, Aldrich). The precipitate
was redispersed in 2 mL of toluene.Alternatively, CsBr (0.011
g, 0.05 mmol, Aldrich, 99.9%) and PbBr2 (0.018 g, 0.05
mmol) were loaded into a zirconia bowl with 25 zirconia balls (4 mm
and 5 mm) and with 1.6 mL of mesitylene and 0.01 g of OAmBr (0.03
mmol). The subsequent milling lasted 2 h at 500 rpm. The bright green
crude solution was diluted with 2 mL of toluene.
Mechanochemical
Synthesis of FAPbBr3 NCs
Bulk FAPbBr3 (0.02 g, 0.04 mmol, prepared as described)
was loaded into a zirconia bowl with 25 zirconia balls (4 mm and 5
mm) and with OAmBr (0.01 g, 0.03 mmol) and 0.4 mL of mesitylene as
the solvent. Other tested ligand systems were a mixture of OA (0.1
mL) and OLA (0.05 mL) and tetraoctylammonium bromide (0.01 g, Aldrich,
98%). The bowl was mounted on a planetary ball mill, and the speed
was set to 500 rpm. The milling time was varied from 30 min to 3 h.
After the milling, a bright green suspension was obtained, which was
diluted with toluene (2 mL) and used as-is or precipitated one time
with acetonitrile (0.5 mL). The precipitate was redispersed in 2 mL
of toluene.
Anion-Exchange Procedure
CsPbBr3 NCs were
prepared as described above. After the ball-milling experiment was
completed, an additional 0.02 g of OAmI (0.05 mmol) was added to the
crude solution, and the ball-milling experiment was continued for
1 h at 500 rpm. A bright-orange suspension was obtained.
Film Preparation
Toluene solution of the perovskite
NCs (10 mg/mL) was filtered using a 0.45 μm poly(tetrafluoroethylene)
(PTFE) filter and drop-casted onto acetone/ethanol-cleaned glass slides.
Characterization
UV–Vis absorption spectra for
the colloidal solutions were recorded using a Jasco V670 spectrometer
in transmission mode. PL and absolute QY measurements were performed
using a Fluorolog iHR 320 Horiba Jobin Yvon spectrofluorimeter equipped
with a photomultiplier tube (PMT) detector, used to acquire steady-state
PL spectra from solutions and films. QY values from NC dispersions
were estimated according to the standard procedure using fluorescein
as the reference.[71] Powder XRD patterns
were recorded using a STOE STADI P powder diffractometer, operating
in transmission mode. A germanium monochromator, Cu Kα1 irradiation,
and a silicon strip detector, Dectris Mythen, were used. Transmission
electron microscopy images were recorded using a Philips CM 12 microscope
operating at 120 kV. Time-resolved PL measurements were performed
using a time-correlated single-photon counting setup, equipped with
an SPC-130-EM counting module (Becker & Hickl GmbH) and an IDQ-ID-100-20-ULN
avalanche photodiode (Quantique) for recording the decay traces. The
emission of the perovskite NCs was excited by a BDL-488-SMN laser
(Becker & Hickl) with a pulse duration of 50 ps, wavelength of
488 nm, and continuous-wave (CW) power equivalent of ∼0.5 mW,
externally triggered at a 1 MHz repetition rate. PL emission from
the samples was passed through a long-pass optical filter with an
edge at 500 nm to reject the excitation laser line. Average radiative
lifetimes were determined as , where A and τ are corresponding
amplitudes and exponential decay parameters in biexponential analysis.
PL QY measurements of the films were conducted using a method similar
to that reported by Semonin et al.[72] With
an integrating sphere (IS200-4, Thorlabs) with a short-pass filter
(FES450, Thorlabs), the absorbance was corrected to reflectance, and
the scattering losses were estimated. A CW laser diode with a wavelength
of 405 nm and a power of 0.2 W modulated at 30 Hz was used as the
excitation source. The emitted light was measured using long-pass
filters (FEL450, Thorlabs). The light intensity was measured by a
broadband (0.1–20 μm) UM9B-BL-DA pyroelectric photodetector
(Gentec-EO). The modulated signal from the detector was recovered
by a lock-in amplifier (SR 850, Stanford Research). The ratio between
the emitted and absorbed light gave the energy yield. The PL QY was
obtained from the value of the energy yield, corrected to the ratio
of photon energies of the laser beam and PL bands. The effect of emission
reabsorption was taken into account in the final calculation.
Authors: Jeffrey M Pietryga; Richard D Schaller; Donald Werder; Michael H Stewart; Victor I Klimov; Jennifer A Hollingsworth Journal: J Am Chem Soc Date: 2004-09-29 Impact factor: 15.419
Authors: He Huang; Yanxiu Li; Yu Tong; En-Ping Yao; Maximilian W Feil; Alexander F Richter; Markus Döblinger; Andrey L Rogach; Jochen Feldmann; Lakshminarayana Polavarapu Journal: Angew Chem Int Ed Engl Date: 2019-09-26 Impact factor: 15.336
Authors: Bogdan M Benin; Dmitry N Dirin; Viktoriia Morad; Michael Wörle; Sergii Yakunin; Gabriele Rainò; Olga Nazarenko; Markus Fischer; Ivan Infante; Maksym V Kovalenko Journal: Angew Chem Int Ed Engl Date: 2018-07-30 Impact factor: 15.336