Junjie Hao‡
abe,
Peizhao Liu‡ch,
Ziming Zhou‡c,
Haochen Liu‡c,
Wei Chen
cdf,
Peter Müller-Buschbaum
fg,
Jiaji Cheng
h,
Kai Wang
c,
Xiao Wei Sun*c,
Jean-Pierre Delville
*b and
Marie-Helene Delville
*a
aUniv. Bordeaux, CNRS, Bordeaux INP, ICMCB, UMR 5026, F-33600 Pessac, France. E-mail: marie-helene.delville@icmcb.cnrs.fr
bUniv. Bordeaux, CNRS, LOMA, UMR 5798, 33405 Talence, France
cInstitute of Nanoscience and Applications, Department of Electrical and Electronic Engineering, Southern University of Science and Technology, Shenzhen, 518055, China
dCollege of Engineering Physics, Shenzhen Technology University, Shenzhen, 518118, China
eCollege of Integrated Circuits and Optoelectronic Chips, Shenzhen Technology University, Shenzhen, 518118, China
fTechnical University of Munich, TUM School of Natural Sciences, Department of Physics, Chair for Functional Materials, James-Franck-Str. 1, 85748 Garching, Germany
gHeinz Maier-Leibnitz Zentrum (MLZ), Technical University of Munich, Lichtenbergstraße 1, 85748 Garching, Germany
hKey Laboratory for the Green Preparation and Application of Functional Materials, Ministry of Education, School of Materials Science and Engineering, Hubei University, Wuhan, 430062, China
First published on 29th January 2025
Colloidal chemistry provides an assortment of synthetic tools for tuning the shape of semiconductor nanocrystals. To fully exploit the shape- and structure-dependent properties of semiconductor nanorods, high-precision control on growth and design is essential. However, achieving this precision is highly challenging due to the high temperatures (>350 °C) and short reaction times (<8 minutes) often required for these reactions. In this study, we performed the first investigation on the impact of temperature and time on the CdS-shell growth of CdSe/CdS quantum rods. Our findings demonstrate that temperature plays a pivotal role in achieving ultra-thin shell dot-in-rods, which are crucial for enhancing chiroptical properties. The two-step process proposed here explains the shell growth of CdSe/CdS dot-in-rods (DRs). It involves finely-tuned isotropic shell growth in the first stage, followed by anisotropic length growth along the [0001] rod axis in the second step. This approach has two advantages: a systematic control of the shell thickness for different aspect ratios (ARs) and batch monodispersity. These DRs, with an ultra-thin CdS shell and a high AR, after modification with L/D cysteine molecules, exhibit significant enhancement of their ligand-induced chirality, with circular dichroism (CD) g-factor values as high as 10−3.
CdSe/CdS dot-in-rods (DRs) are visible light-emitting nanocrystals that form robust systems combining a high degree of monodispersity with bright and narrow photoluminescence.37–39 However, although rapid initial progress in their development has resulted in the achievement of DRs with different aspect ratios (ARs) and colors in the visible range,40–46 improvements in the control of their morphology at the nanoscale, using conventional fast-injection-based preparations, are still under development. This is especially true for the control of a targeted ultra-thin shell.
Even if such thin shells have a positive influence on the improvement of catalytic performances47 and chirality,17,24,32 to the best of our knowledge, no investigation so far has directly focused on the synthesis of uniform quantum rods that can combine thin shells with varying ARs. Only a few publications mentioned the control of the DR shell thickness. Bawendi38 used a second over-coating process and focused on DRs with thicker shells to enhance the quantum yield (QY) to nearly 100%. She et al.48 studied the QYs and photophysical processes by systematically tuning the shell and seed sizes, including the thin shell case, but in fact, both the shell layer and length increased simultaneously. Kim et al.40 proposed a dual-diameter structure for these semiconductor nanorods exhibiting two distinctly segmented parts with different diameters and a thicker shell on the CdSe seed. Khon et al.47 obtained thin-shell DRs by etching a 0.7 nm CdS layer from the CdSe/CdS nanorods, enhancing their catalytic activity more than 3 times compared to the original CdSe/CdS DRs.
Additionally, when considering the impact of shell thickness variation on the chiral properties of CdSe/CdS nanorods, two competing effects should be taken into account: (i) the CdS shell acts as an energy barrier for holes within the CdSe core, potentially hindering their chiral electronic coupling with surface ligands and leading to a decrease in CD signals; (ii) conversely, appropriately designed CdS layers can lower the energy of holes, bringing them closer to the energetic resonance of the Highest Occupied Molecular Orbital (HOMO) of the ligand. This closer alignment enhances the CD responses, as it facilitates stronger interactions between holes and ligands. Therefore, the limitations in chirality transfer via the post-ligand exchange strategy remain to be fully understood. Nonetheless, these examples highlight the critical importance of thin shell thickness for achieving high CD and CPL activities. They also show the complexity of achieving such high-precision control in the synthesis of DRs when increasing their lengths and ARs. Obtaining DRs with both a high AR and a thin shell is a prerequisite for studying, controlling, and even increasing their ligand-induced CD and CPL activities.
Therefore in this work, we aimed to first analyse and understand the discrepancies in the literature concerning the temperature and time reaction conditions, then address the two issues mentioned above, and determine how thin the shell of a DR should be for optimal optical properties. To do so, we reinvestigated and modeled (1) the variation of the DRs' dimensions with time, (2) the effect of temperature throughout the synthesis on the DRs' shell thickness and (3) the effect of seed concentration on the aspect ratio of the thin-shell DRs. We eventually checked the influence of shell thickness on the chirality of asymmetric DRs.
All the heating mantles are made by Glas-Col but have different setups. (1) Typically, the experiments were performed by using a 180 W Series O spherical mantle (high capacity) covering both the top and the bottom of the flask to improve safety and efficiency; (2) we chose the 50% (90 W) input power controlled by the Glas-Col controller of lower power for control experiments, which decreases the heating rate (from ∼12 K min−1 to ∼5 K min−1).
Purification of the CdSe-TOP seed. The reaction mixture was cooled to 343–353 K and mixed with 50 μL (40.85 mg) of TBP; then 4 mL of ethanol was added to the above solution, which was centrifuged at 10000 rpm for 3 minutes. Then, the precipitate was dissolved in a small amount of toluene while the supernatant was discarded. After centrifugation again, the precipitate was dissolved in TOP (CdSe-TOP). Due to the TBP purification process, the CdSe seed can be better purified, removing the adsorbed ions on the surface and the by-products in the solution. This is essential for achieving uniform morphology control and high quantum yield in DRs.
The shell thickness can be controlled by changing the injection temperature, heating mantle power, or ambient temperature. CdSe/CdS DRs with different aspect ratios were also synthesized by adjusting the seed concentration and reaction time.
![]() | ||
Fig. 1 Range of shell thicknesses of CdSe/CdS DRs for given temperatures and a reaction time of 8 min based on data from Table 1. |
No. | λAbs (nm) | Seed diam. (nm) | Tinjection (K)/time (min) | DR length (nm) | DR diam. (nm) | DR AR | Shell-thickness (nm) | Ref. |
---|---|---|---|---|---|---|---|---|
a Diameter of the CdSe seed determined from the absorption spectrum using Peng's equation (nm);54b The ambient temperature was 303 K (summertime).c The ambient temperature was 291 K (wintertime); reaction time: 8 min, otherwise indicated. | ||||||||
1 | — | 3.2 | 623 | 53 ± 4 | 3.9 ± 0.2 | 13.6 | 0.35 | 41 |
2 | 3.3 | 623 | 35 ± 2 | 4.2 ± 0.4 | 8.3 | 0.50 | 41 | |
3 | 3.3 | 653 | 19 ± 1 | 5.0 ± 0.5 | 3.8 | 0.90 | 41 | |
4 | 585 | 4.0a | 623/10 | 44 ± 4 | 5.5 ± 0.2 | 8.0 | 0.75 | 38 |
5 | — | 3.9a | 638 | 28 ± 4 | 8 ± 1 | 3.5 | 2.05 | 49 |
6 | 3.4a | 623 | 44 ± 8 | 4.9 ± 0.7 | 9.0 | 0.75 | 49 | |
7 | 3.1a | 623 | 108 ± 25 | 4.6 ± 0.5 | 23.5 | 0.75 | 49 | |
8 | — | 3.4a | 653 | 37 ± 3 | 4.9 ± 0.6 | 7.6 | 0.75 | |
9 | 2.9a | 633 | 56 ± 3 | 5.3 ± 0.6 | 10.6 | 1.20 | 50 | |
10 | 536 | 2.7 | 623/20 | 22 | 7 | 3.1 | 2.15 | 45 |
11 | 623 | 22 | 4 | 5.5 | 0.65 | 45 | ||
12 | 653/20 | 35 | 7 | 5.0 | 2.15 | 45 | ||
13 | 623/40 | 58 | 7 | 8.3 | 2.15 | 45 | ||
14 | — | 4.2 | 623 | 42 | 7.5 | 5.6 | 1.65 | 45 |
15 | — | 3.5 | 623/6 | 24.0 ± 2 | 5.0 ± 0.5 | 4.8 | 0.75 | 51 |
16 | 557 | 3.2a | 623 | 36.5 | 7.3 | 5.0 | 2.05 | 52 |
17 | — | 4.2 | 593 | 49 ± 2.5 | 5.8 ± 0.5 | 8.4 | 0.8 | 53 |
18 | 653b | 30.4 ± 2.5 | 5.8 ± 0.8 | 5.2 | 1.3 | This work | ||
19 | 623b | 32.5 ± 2.0 | 4.9 ± 0.5 | 6.6 | 0.85 | This work | ||
20 | 593b | 24.3 ± 1.6 | 3.8 ± 0.4 | 6.4 | 0.35 | This work | ||
21 | 593c | 24.5 ± 2.0 | 4.4 ± 0.5 | 5.6 | 0.6 | This work |
To clarify the discrepancies between these results, we performed all the experiments with a temperature control located directly inside the solution to ensure more accurate monitoring of the reaction. Room-temperature solution injections were introduced into the solution only after it had reached and stabilized at the desired temperature.
We then decided to reinvestigate the growth of CdSe/CdS DRs by varying (i) the reaction time to follow the involved mechanisms, (ii) the reaction temperature to determine activation energies and optimize the AR range, and (iii) the concentration of CdSe seeds to offer even more versatility in the AR.
Typically, 3.2 nm wurtzite (WZ)-CdSe seeds54 were chosen as starting seed samples (λabs = 557 nm, Fig. S1†) to study the growth process over a wide range of reaction times from 30 s to 16 min, with reaction temperatures extending from 503 to 653 K, and seed concentrations ranging from 4 to 40 μM.
Here we performed the first set of experiments starting from the same CdSe seed (Ds = 3.2 nm) at a concentration of 14 μM, and at 593 K. We varied the time and analysed the growth of the resulting CdSe/CdS DRs. Fig. 2 illustrates the precise control of their morphology, and Table 2 provides detailed information on the variation of the CdS shell thickness (D − Ds/2), the overall length of the DRs (L), their overall aspect ratios (AR = L/D), and the increase in the overall volume with time.
Name | React time (s) | Length L (nm) | D (nm) | AR L/D | Shell-thickn. (D − Ds)/2 (nm) | Va (nm3) |
---|---|---|---|---|---|---|
a Overall volume V = πD2(L − D/3)/4, assuming a cylindrical part with hemispherical ends. | ||||||
DR-1 | 30 | 5.5 ± 0.9 | 3.4 ± 0.5 | 1.6 | 0.1 | 39.6 |
DR-2 | 60 | 8.0 ± 1.0 | 3.6 ± 0.5 | 2.2 | 0.2 | 69.2 |
DR-3 | 120 | 15.7 ± 3.0 | 3.6 ± 0.4 | 4.4 | 0.2 | 147.6 |
DR-4 | 240 | 21.7 ± 2.7 | 3.8 ± 0.4 | 5.7 | 0.3 | 223.8 |
DR-5 | 480 | 38.7 ± 3.5 | 3.6 ± 0.4 | 10.8 | 0.35 | 381.4 |
DR-6 | 960 | 35.8 ± 2.4 | 5.4 ± 0.8 | 6.6 | 1.1 | 778.7 |
As (i) the morphology of nanorods can be described as a cylindrical part with two hemispherical tips and (ii) cylinders and spheres have different symmetries, the growth law of the overall length L involves both axial and radial components. Then, we separate them considering that a NR, of overall length L and diameter D, can be described as a cylindrical part of length l = L − D capped by two hemispherical tips of radius D/2. Fig. 3 shows a diagram of such a nanorod, depicting the growth sequence of the length (l), diameter (D), volume (V − Vseed) of the grown CdS material, and the aspect ratio, now defined as l/D (l/D = L/D − 1) to explicitly separate symmetries, for the seeded case where CdS grows over a CdSe seed at T = 593 K; raw data corresponding to this growth are provided in Table 2.
Schematically, the growth of DRs starting from the 3.2 nm seeds in the presence of ligands grafted on the surface shows the following stages, analogous to those observed by Peng under seedless conditions.55 (i) When starting with polyhedron CdSe seeds of nearly spherical symmetry, the growth of a CdS layer on a seed remains isotropic until the emergence of facets that differentiate the surface energy properties (one CdS layer seems sufficient to induce such a differentiation). (ii) When this difference in surface energy becomes high enough,56 the asymmetric growth is triggered along the axial direction. DRs form (1D-growth), and a maximum overall aspect ratio of 10 can be reached. (iii) Eventually, these DRs undergo 3D growth with some reshaping, likely to minimize surface energy stresses in comparison to bulk ones. This reshaping is evidenced by the concomitant decrease in length observed in Fig. 3b, and by the continuous volume growth with the reaction time, as shown in Fig. 3c.
The growth kinetic mechanisms of II–VI semiconductor DRs are not yet well established, particularly for the 1D-growth regime. On the one hand, Viswanatha et al.57 investigated in detail the growth of bare CdS spherical nanoparticles during the Ostwald ripening regime and experimentally confirmed the validity of a diffusion-limited growth mechanism in this case. On the other hand, the growth mechanism of ligand-capped spherical CdSe nanoparticles remains a topic of debate. While half of the studies propose a diffusion-limited interpretation,58,59 the other half suggests a reaction-limited mechanism.60,61
Nonetheless, when looking at the broader literature concerning the growth of metallic-capped nanoparticles, particularly gold ones62 (see also references therein), it looks like the growth of ligand-capped gold nanoparticles may follow different consecutive steps and mechanisms, but they are all driven by a surface reaction-limited process. Then, following these lines and considering the symmetry of the DRs, we examine the growth of the cylindrical part and the hemispherical tips separately.
For reaction-limited growth on CdSe seeds, well before the final Ostwald ripening, i.e., in the free-growth regime during which the solute concentration at infinity ([C]∞) can be assumed constant, the growth of the DRs can be qualitatively obtained by balancing the DR volume growth rate with the reactive flux (Jreac) at the concerned surface of the DR.
Thus, axial growth occurs from the reaction flux at the spherical tips (index s) of the DRs such that we have dV/dt|D = VM·Jreacs = VM·πD2ks[C]∞, whereas radial growth occurs from the reaction flux at the cylindrical part (index c) of the DRs so that dV/dt|l = VM·Jreacc = VM·πDlkc[C]∞, where VM is the molar volume of CdS and ks,c represents the reaction rates for solute incorporation into the DRs; ks,c is classically expressed in nm s−1.62 Using the volume V = πD2(l + 2D/3)/4 of a DR, we, thus, expect the following growth rates (eqn (1)):
![]() | (1) |
Moreover, in this 1D-growth regime, the volume of the DRs corrected by the volume of the seed (V1d − Vseed), i.e., the amount of grown material, and the aspect ratio, AR1d = l1d/D1d, are also expected to behave respectively as (V1d − Vseed)(t) ≈ πl1d(t)D021d/4 = πD021dVMks[C]∞t and AR1d(t) = l1d(t)/D01d ≈ 4VMks[C]∞t/Ds, both linearly varying with time. This is experimentally determined and again confidently fitted using power-laws with respective exponents of 1.006 and 0.96 and correlations of 0.99 and 0.98. Note also that a linear fit of (V1d(t) − Vseed) ≈ πl1d(t)D021d/4 as a function of l1d before reshaping, gives a slope of πD021d/4 = (12.14 ± 0.22) nm2, from which we can deduce a statistical average diameter of D01d = (3.93 ± 0.04) nm during the 1D-growth phase. This value corresponds to the seed diameter, Ds = 3.2 nm covered with a single CdS layer (≈0.35 nm) and, thus, strongly supports the fact that the first transitory isotropic growth stage of CdS onto the spherical CdSe seeds involves the growth of just a monolayer of CdS to trigger the 1D-growth. We finally note that DRs eventually reshape when their overall aspect ratio reaches a maximum value of (l1d/D1d + 1) ≈ 11 under the present experimental conditions. However, this reshaping does not affect the growth as illustrated by the continued linear variation of the DR volume with time, despite the decrease in their length.
This dynamic thus suggests a method to consistently produce high aspect ratio NRs with the thin-shell thickness remaining around 1 CdS monolayer as long as the growth remains within the 1D-regime, i.e., up to a reaction time of 8 minutes under the present experimental conditions. Indeed, for longer reaction times, the 3D growth and reshaping increase the shell thickness and decrease the AR, explaining why many previous studies used these 6–10 min reaction times.38,41,45,49–51,63 Considering the data in Fig. 3, we also chose 8 min as the reaction time and further optimized the control over the AR by varying the reaction temperature.
The shape and composition of samples were confirmed by TEM energy dispersive spectroscopy (EDS) elemental mapping and shown for one of them (Fig. 4). The position of the CdSe seed at around 1/4 to 1/2 of the overall length shows that the temporal sequence of the seeded rod length is consistent with the literature.40,49,64–67
Name | TInjection (K) | Length L (nm) | Diameter D (nm) | AR l/D | (D − Ds)/2 (nm) | Volumea V (nm3) |
---|---|---|---|---|---|---|
a Overall volumeV = πD2(L − D/3)/4, assuming a cylindrical shape with two hemispherical ends. | ||||||
DR-7 | 503 | 6.2 ± 0.7 | 3.6 ± 0.4 | 1.7 | 0.2 | 50.9 |
DR-8 | 533 | 8.3 ± 0.8 | 3.7 ± 0.5 | 2.2 | 0.25 | 76.0 |
DR-9 | 563 | 12.0 ± 1.0 | 3.8 ± 0.4 | 3.2 | 0.3 | 121.7 |
DR-10 | 593 | 24.3 ± 1.6 | 3.8 ± 0.4 | 6.4 | 0.3 | 261.2 |
DR-11 | 623 | 32.5 ± 2.0 | 4.9 ± 0.5 | 6.6 | 0.85 | 582.1 |
DR-12 | 653 | 30.4 ± 2.5 | 5.8 ± 0.8 | 5.2 | 1.3 | 752.1 |
Fig. 5 shows that 1D-growth is preserved for at least 8 min, provided the injection temperature remains below 593 K. The shell thickness can, thus, remain very thin while the overall length L of the DRs, and consequently the overall aspect ratio L/D, can be tuned up to 6.4 under present experimental conditions.
Moreover, using the data from Table 3, and the linearity between (V1d − Vseed) and l1d in the 1D-growth regime ((V1d − Vseed)(t) ≈ πl1d(t)D021d/4), we find πD021d/4 = (12.07 ± 0.20) nm2 from which we can deduce a statistical average final diameter of D01d = (3.92 ± 0.03) nm. This value, now obtained from experiments conducted at different temperatures after an 8-minute reaction time, strengthens the fact that just a single CdS monolayer (0.35 nm) grows on the CdSe seeds (Ds = 3.2 nm) during the first growth stage, regardless of the reaction temperature.
Also, temperature investigations give access to activation energies necessary for DR growth. On the one hand, let τ1,3 denote the crossover time at which the growth switches from 1D to 3D. Then, the axial growth rate dl/dt ≅ 4VMks[C]∞ continues to predict l3d(t) ≅ 4VMks[C]∞t. Moreover, as l/D ≫ 1 at τ1,3 in Fig. 5, the radial growth rate dD/dt ≈ 2VMl/l + Dkc[C]∞ ≈ 2VMkc[C]∞ leads to D3d(t) ≈ D01d + 2VMkc[C]∞(t − τ1,3). We deduce the CdS shell thickness variation, S3d(t > τ1,3) = (D3d − D01d)/2 ≈ VMkc[C]∞(t − τ1,3). On the other hand, the DR growth reaction rate constants, ks,c, of the solute are known to follow Arrhenius' laws in temperature of the form ks,c = k0s,c exp(−Es,c/RT), where Es,c represents the growth activation energies at the DR surfaces, at their spherical tips and the cylindrical part, respectively. Consequently, at a given time and for an initial solute concentration of [C]∞, we expect: (i) l1d,3d(T) ∝ ks(T) ∝ exp(−Es/RT) during the 1D- and the 3D-growth stages and, (ii) S3d(T) ∝ kc(T) ∝ exp(−Ec/RT) for the 3D-growth stage. Thus, the temperature-dependent variations in the DR shell thickness and length should allow the determination of the corresponding axial and radial energies of activation (Fig. 5).
The axial growth exponential fitting yields Es ≈ (51 ± 8) kJ mole−1. The determination of Ec from the 3D-radial growth stage is less accurate because it is difficult to obtain much data free from DR reshaping; only an order of magnitude can be given using three shell thickness measurements. The corresponding exponential fitting yields Ec ≈ (70 ± 18) kJ mole−1. Considering the errors resulting from data fitting, Ec ∼ Es, which suggests that the energy cost for radial and axial solute incorporation is not a determinant quantity to explain the difference between 1D- and 3D-growth.
Activation energy data are scarce in the literature for comparison. For instance, Viswanatha et al.57 performed experiments on the growth of CdS nanoparticles in the absence of surface ligands and over a narrow and low-temperature range (333–373 K); they also adjusted their concentrations to maintain the growth of their CdS nanoparticles in the spherically isotropic Ostwald ripening regime. They found an activation energy of Ea ∼ 142 ± 3 kJ mole−1, i.e., typically twice as high as the Es obtained for the 3D-growth at the DR tip with the same spherical symmetry. Nonetheless, both the presence of ligands on the DR surface, which are known to reduce diffusion phenomena, and the higher reaction temperature (503–653 K) level may explain this difference in values. This hypothesis is strengthened by another work on the spherical growth of CdS nanocrystals in a hot paraffin matrix developed by Yordanov et al.68 Working in the spherically isotropic Ostwald ripening regime, they found that the growth rate was slower when using a coordinating matrix (Tri-n-octyl phosphine oxide, (TOPO)) instead of a non-coordinating one (tributylphosphine sulfide (TBP-S) in liquid paraffin). Further analysis using TBP-S gave an activation energy of Ea ∼ 51.9 kJ mole−1 within the temperature range of 473–533 K,69 comparable to our measured value (average value: Es ∼ 60 kJ mole−1).
Consequently, the reaction temperature plays a crucial role in the growth process, and 593 K seems to be an optimized value for achieving the highest aspect ratio before 3D growth and reshaping occur. Finally, this temperature-controlled investigation clarifies the dispersion in results observed in previous studies, many of which were based on reaction temperatures above 623 K.38,41,45,49–51,63
Name | [Seed]a (μM) | Length (nm) | Diam. (nm) | ARb | Shell-thickness (nm) | Vc (nm3) |
---|---|---|---|---|---|---|
a The seed concentration was calculated from the absorption spectrum using Peng's equation (nm).54b AR = L/D ((L − D)/D).c Overall volume V = πD2(L − D/3)/4, assuming a cylindrical shape with hemispherical ends. | ||||||
DR-13 | 3.7 | 74.6 ± 7.1 | 3.7 ± 0.5 | 20.2 (19.2) | 0.3 | 788.84 |
DR-14 | 7.3 | 52.7 ± 3.7 | 3.6 ± 0.4 | 14.6 (13.6) | 0.2 | 524.21 |
DR-5 | 14 | 38.7 ± 3.5 | 3.6 ± 0.4 | 10.8 (9.8) | 0.2 | 381.7 |
DR-10 | 18.8 | 24.3 ± 1.6 | 3.8 ± 0.4 | 6.4 (5.4) | 0.3 | 261.24 |
DR-15 | 36.5 | 18.3 ± 2.8 | 3.8 ± 0.6 | 4.8 (3.8) | 0.3 | 193.17 |
Table 4 shows that the shell-thickness of the DRs remains less than 1 monolayer (one monolayer of CdS having an average thickness of 0.35 nm) as the seed concentration decreases. Meanwhile, their length not only increases (Fig. 6) but also exhibits a much narrower size distribution.
These behaviors can be quantitatively understood by mass conservation at time t. Indeed, the volume of material consumed at time t for DR growth, VM[C(t)] = VM × Min{[Cd](t),[S](t)}, should be equal to the number of seeds per liter, Ns, multiplied by the increase in individual DR volume due to material consumption: Ns(V(t) − Vseed). Then, as , where
is the Avogadro number, we deduce (eqn (2)):
![]() | (2) |
Working in the 1D-growth regime, (V(t) − Vseed) ≈ (V1d − Vseed)(t) ≈ πl1d(t)(D01d)2/4, where D01d = Ds + 2CdS layers (Ds = 3.2 nm plus twice 0.35 nm). Then, at a given reaction time (8 min), temperature (593 K) and cadmium precursor concentration ([Cd] = 0.55 M), we expect from eqn (2): l1d ∝ (V1d − Vseed) ∝ [CdSe]−1, D1d = D01d ∝ [CdSe]0, and , all linear in [CdSe]−1, except D1d ∼ Ds which is fixed as the initial condition.
Moreover, the diameter D of the DRs remains constant over the investigated range of CdSe seed concentrations, corresponding to almost one order of magnitude variation. Finally, Fig. 7 shows that (V1d − Vseed) is indeed linear in l1d, and the slope of πD021d/4 = (10.75 ± 0.21) nm2, allows deducing a statistical mean diameter of D01d = (3.70 ± 0.04) nm, during 1D-growth. This value corresponds to a seed diameter of Ds = 3.2 nm covered with a single CdS layer (0.35 nm) and gives one more proof of the isotropic growth of a single CdS shell before switching to the 1D-growth regime.
In conclusion, CdSe/CdS DRs with a thin shell close to a single CdS layer can be synthesized with high accuracy and predictability when the reaction temperature is well controlled, including the influence of the initial thermal conditions (see the ESI (Tables S1 and S2)).† This approach was also extended to other CdSe seed sizes (Fig. S3 and S4 and Table S3†). Moreover, their overall aspect ratio can be continuously varied between 1 and 20 (DR13), just by adjusting the reaction time and/or seed concentration at the optimized reaction temperature. Finally, as illustrated in Fig. 3 over time and Fig. 5 with varying temperatures, the 3D-growth process enables variations and adjustments in the shell thickness as needed. Consequently, we had a set of available samples for studying in detail the influence of the envelope and length on the chiroptical properties of these CdSe/CdS nano-objects.
We chose ligand-induced chirality among the several methods for inducing chirality in QDs.2,3,16,20 Induced chirality in the aqueous phase relies on the replacement of the original achiral ligand with a chiral one on the semiconductor nanoparticles.15,16,29,30,74 Gun'ko and co-workers were the first to report the observation of circular dichroism (CD) response induced in excitonic transitions of CdS quantum dots (QDs) capped with chiral molecules.18 However, the CD g-factor they found was quite low (typically 10−4 or even 10−5).16,75–78 Since, on the one hand, the induced chiral signal intensity of the core–shell systems has been shown to increase with decreasing shell thickness,24 and on the other hand, we have recently observed that CdSe/CdS DRs have great potential for high ligand-induced chirality,16,17 we aim to use our actual control of shell thickness down to ultra-thin shell DRs to generate and study high ligand-induced chiral signals.
To prepare these chiral DRs, we extracted the organic colloidal phase using an aqueous phase with cysteine (Cys) ligands as previously discussed (Fig. 8).16,17
To do so, cysteine was dissolved in deionized (DI) water (5 mL, [Cys] = 0.1 M); the pH of the resulting solution was then adjusted to 12.0 with a 25% aqueous solution of tetramethylammonium pentahydrate (TMAH). A solution of CdSe/CdS DRs in n-hexane (5 mL, 1 μM) was added to the aqueous cysteine solution; the reaction mixture was then purged with nitrogen and stirred at room temperature, under an inert atmosphere for 24 h in the absence of light. The reaction mixture was then allowed to rest for 1 h to allow phase separation. The bottom aqueous layer, now containing the DRs, was removed with a syringe, and purified twice by precipitation with ethanol/DI water/chloroform (4:
1
:
1). As an example, purified Cys-DRs were dispersed in deionized H2O and stored at room temperature in the dark. Fig. S8† shows the luminescence of the DRs listed in Table 3; before (a and b) and after (c and d) the ligand exchange and transfer from the organic to the aqueous phase. From left to right, we observe the CdSe QDs, and DRs with different aspect ratios, respectively. The luminescence of the different DRs is well preserved, but that of the pure CdSe is almost completely quenched.
We then focused on the UV-vis and CD studies performed on samples with increasing shell thicknesses with also comparable lengths, listed in pairs in Table S4† and shown in Fig. 9.
![]() | ||
Fig. 9 CD spectra and the corresponding UV/vis absorption spectra of the L- and D-Cys-CdSe/CdS DRs with different shell thicknesses. (a) DR-10, (b) DR-11, (c) DR-12, and (d) DR-23. |
The results show that the strong CD signal observed for CdSe/CdS DRs with one or two monolayers (DR-10 and DR-11) decreases and is completely suppressed when the shell becomes thicker (DR-12 and DR-23), as expected due to the effect mediated by hole interactions with the surface. This phenomenon is independent of the DR length, as illustrated by the similar lengths of DR-10 and DR-23. The CD g-factor signal decreased by more than 5-fold as the shell thickness increased from 0.35 to 2.10 nm (one to six layers) (Fig. 10, Tables S5 and S6†), as also observed by Purcell-Milton.24
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Fig. 10 Variation of the CD g-factor of the DRs with their shell thickness (Table S4†). Green dots: additional data from ref. 16 (Tables S2 and S3†) and blue ones from ref. 34 with identical seed diameter. |
This study not only confirms, the behaviour observed by Purcell et al.24,79 in QDs for DRs, i.e., an inverse relationship between the CD g-factor and the number of shell layers (consistent with the increase in the distance between the chiral ligands and the holes localized at the CdSe core level) but also shows that this behaviour (i) takes place in a range of g-values an order of magnitude higher than in QDs, (ii) is linear, and (iii) does not follow an exponential trend.
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Fig. 11 Variation of the CD signal with the DR aspect ratio, in the 400–500 nm region of the CdS absorption (CdSe seed size Ds = 3.2 nm). (a–e) CD signal of DR-15, DR-10, DR-5, DR-14, and DR-13, from Table 3; (f) Resulting CD g-factor variation of the same DRs (lines are guides for the eyes). Blue and green data are from ref. 78 for pure CdSe QRs. Lines are also guides for the eyes. |
A closer look at Fig. 11 further highlights the significant added value of a thin CdS shell as compared to pure CdSe nanorods.78 The combined effects of the CdSe core and CdS shell generate a chiral signal for the CdSe/CdS DRs that is higher than that of pure CdSe or CdS. As the aspect ratio increases, the CdS shell gradually grows along the [001] axis, which increases the anisotropy and leads to chirality enhancement.
The reaction temperature plays a crucial role in the growth process, and 593 K appears to be the optimized value for which the highest AR is reached before 3D growth and reshaping take place. Eventually, this study on the control of the temperature elucidates the discrepancies in results observed in the aforementioned studies, where many used reaction temperatures above 623 K.
Under optimal conditions, we could achieve DRs with a thin shell thickness of approximately 0.35 nm, corresponding to a single atomic layer of CdS and ARs ranging from 4.8 to 20. Their CD g-factor values varied from 0.23 × 10−3 to 1.30 × 10−3. Notably, the CD g-factor value of 1.3 × 10−3 represents the highest ligand-induced chirality achieved to date for this type of nanorods by simply controlling their length and shell thickness. Additionally, only one type of chiral ligand was used. This approach gives these structures great potential for further applications in the chirality domain. Most of all, this study provides a platform for the exploration of various dimensions of nanostructures with controllable anisotropy. Finally, we anticipate that this ultra-thin shell adjustment strategy can be extended to other types of seed-grown semiconductor nanoparticles, enhancing their chiral signal and catalytic properties with significant practical implications.
Footnotes |
† Electronic supplementary information (ESI) available: Fig. S1. (a) UV-vis absorption spectra and (b) PL emission spectra of WZ-CdSe cores (λabs = 557 nm). Fig. S2. TEM images of DRs synthesized at different temperatures using the same CdSe cores. Table S1. Physical properties of CdSe/CdS DRs at different reaction times, with two heating power systems. Working temperature 593 K. Table S2. Physical properties of CdSe/CdS DRs at different ambient temperatures (CdSe core 3.2 nm). Table S3. Characterizations of the thin shell CdSe/CdS DRs using different sizes of CdSe cores. Fig. S3. UV-vis absorption and PL emission spectra of CdSe cores with different sizes. Fig. S4. UV-vis absorption and PL emission spectra of CdSe/CdS DRs with thin shell multi-colour. (a) DR-16 (green), (b) DR-15 (orange), (c) DR-17 (red), (d) DR-18 (red). Table S4. Physical properties of CdSe/CdS with different shell thicknesses (CdSe core (3.2 nm). Fig. S5. TEM image of DR-23 with a second over-coating process, the shell thickness is 2.0 nm. Fig. S6. UV-vis absorption and PL emission spectra of CdSe/CdS DRs with different shell thicknesses. Fig. S7. Variation of PL emission spectra of CdSe/CdS DRs with different shell thicknesses. Fig. S8. Images comparing the luminescence before and after the ligand exchange. (a) and (b) the oil phase QDs and DRs in hexane; (c) and (d) the aqueous phase QDs and DRs. Images (a) and (c), under natural light, and (b) and (d) under UV light (365 nm). From left to right: CdSe QDs, and DRs with different aspect ratios (see Table 3 for details). Table S5. The CD anisotropy factors of D-CdSe/CdS DRs with different shell thicknesses (CdSe cores (D = 3.2 nm)). Table S6. CD anisotropy factors of L-CdSe/CdS DRs with different shell thicknesses (CdSe cores (D = 3.2 nm)). Table S7. CD anisotropy factors of D-CdSe/CdS DRs at different core concentrations (CdSe cores (D = 3.2 nm)). Table S8. CD anisotropy factors of L-CdSe/CdS DRs at different core concentrations (CdSe cores (D = 3.2 nm)). See DOI: https://doi.org/10.1039/d4na01003e |
‡ These authors contributed equally. |
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