Sk
Tahmid Shahriar
a,
Chris
Feltman
b,
Sean
Machler
c and
Nabila
Tanjeem
*c
aDepartment of Mechanical Engineering, California State University, Fullerton, Fullerton, California 92831, USA
bDepartment of Mathematics, California State University, Fullerton, Fullerton, California 92831, USA
cDepartment of Physics, California State University, Fullerton, Fullerton, California 92831, USA. E-mail: ntanjeem@fullerton.edu
First published on 16th May 2025
We investigate two-dimensional crystal assemblies formed by a binary mixture of colloidal particles with a size ratio of 0.88 and driven by short-ranged depletion interactions. Our experiments show that the orientational order of the assembly decreases with an increasing fraction of impurity particles, reaching up to 18% reduction in a 1
:
1 binary mixture compared to a monodisperse suspension. We observe slower growth rate and arrested dynamics in the binary mixture, whereas the monodisperse sample follows a two-step nucleation and growth mechanism. We performed molecular dynamics simulations to calculate the minimum energy states for different size ratios and number ratios of the binary mixture. The simulation results predict a compromised translational order but sustained orientational order in a binary mixture with a size ratio as high as 0.88. From the combined experimental and numerical results, we conclude that the disordered assemblies found in a binary mixture originate from the frustration in assembly kinetics rather than topological frustration when there is a marginal mismatch between the two particle sizes.
An important determinant of colloidal self-assembly is the nature of the interparticle interaction potential. While hard sphere assembly has been a common choice for studying phase behavior, assembly mechanisms that involve engineering the attractive potential between particles by tuning electrostatic, DNA-hybridization, and depletion interactions have become increasingly popular.21–23 Specifically, self-assembly driven by depletion forces allows for tuning the strength and the range of the attractive interaction potential simply by varying the assembly components, hence it has been employed for programming the structures of colloidal clusters.24–28 Another important aspect of depletion interaction is that its strength depends on the geometry of the particles and the nearby surfaces; this property allows the formation of two-dimensional colloidal crystals on a surface whose curvature is smaller than the particle curvature.29,30 Therefore, depletion-induced self-assembly has been an attractive choice for investigating 2D colloidal crystallization mechanisms on flat and curved surfaces.31,32 Such systems have a diverse set of applications involving photonic crystals,27,33 semiconducting particle assembly,34 chiral nanomaterials,31,35 photonic balls,36,37 and colloidal epitaxy.10,38 Despite significant interest, it is yet unknown how depletion-driven 2D colloidal crystallization is affected by particle polydispersity, the simplest case of which is a binary system comprised of two different particle sizes.
Here, we investigate two-dimensional binary colloidal self-assembly driven by a short-ranged depletion interaction potential, where the ratio of the small particle diameter to the large particle diameter is
, and the range of the attractive interaction potential is only 4% of the particle diameter. Prior work on binary colloidal self-assembly in the presence of depletion interactions investigated the phase behavior in bulk,39–41 observed eutectic crystallization,42,43 and the formation of colloidal gels.44,45 Toyotama et al. found phase-separated eutectic crystals for a size ratio of particles (0.83) that was closer to our system but driven by a long-ranged interaction potential (80% of particle diameter). Pandey et al. investigated self-assembly with short-ranged depletion interaction (4% of particle diameter) in a binary mixture of particles with a size ratio of 0.49 and observed the formation of 3D colloidal gels and arrested particle dynamics. To our knowledge, no experiments have explained the formation of 2D binary crystals driven by short-ranged depletion interactions, especially in the presence of a small asymmetry in the particle sizes. Therefore, we performed a combination of experimental and computational investigation to elucidate how the size ratio and the relative concentrations of the two particle species determine the structural order and the assembly kinetics.
We found that the orientational hexatic order parameter of the self-assembled binary monolayer reduces by 18% in a 1
:
1 binary mixture compared to a monodisperse suspension. Additionally, the binary mixture exhibits much slower growth kinetics that is accompanied by cooperative particle motion. To explain the experimental findings, we developed a molecular dynamics simulation model to identify the minimum energy states of a 2D binary assembly driven by a short-range attractive interaction potential. The model shows that for a mixture with a greater particle size difference, i.e.,
, the hexatic order parameter decreases with an increasing fraction of impurity particles and reaches the minimum value for the 1
:
1 mixture. However, for a binary mixture where the particle sizes are much closer, i.e.,
, the orientational hexatic order parameter in the 1
:
1 mixture ratio sample remains the same as the sample with minimal impurity. However, in this case, a reduction in the translational order, as characterized by the average bond length, is observed. The disagreement between the computational and experimental results can be attributed to the assembly kinetics that distinguish the 1
:
1 mixture from a monodisperse sample. Although both samples grow in amorphous states during the first part of the assembly process, the monodisperse sample starts forming stable crystallites following two-step nucleation,30 whereas the binary sample continues to grow in the amorphous state until the assembly attains high surface coverage and the particles become dynamically arrested. Our results provide a new insight into binary assemblies in cases where the mismatch in the particle sizes is marginal—the frustration in assembly kinetics, rather than the topological frustration, is the key factor that determines the structural order of the assembly.
Monodisperse sample: the green beads (Fluoro-Max G700) with a diameter of d1 = 700 nm were used to study the self-assembly of a monodisperse suspension. Five μL of the 1% particle suspension was mixed with an equal volume of 73 mM of SDS. 1
:
1 binary mixture: 10 μL of 73 mM SDS solution was mixed with 5 μL of 700 nm green beads and 5 μL of 790 nm red beads. 9
:
1 binary mixture: 9 μL of 700 nm green beads and 1 μL of 790 nm red beads were mixed with 10 μL of 73 mM SDS solution. 19
:
1 binary mixture: 19 μL of 700 nm green beads and 1 μL of 790 nm red beads were mixed with 20 μL of 73 mM SDS solution. 39
:
1 binary mixture: 39 μL of 700 nm green beads and 1 μL of 790 nm red beads were mixed with 40 μL of 73 mM SDS solution.
The number ratios of the two particles in a binary mixture can be calculated based on the volume ratios of the two mixtures
, particle sizes (Dp), the density of the particles (ρb) and the fluid (ρf) using the following equation:
![]() | (1) |
The sample cells were imaged using an optical microscope immediately after sealing them. The imaging was performed using an inverted Olympus ix83 microscope equipped with a 100× (N.A. = 1.45) objective lens. Images were captured using the open-source software Fiji and its plug-in Micro-Manager 2.0. The green particles were captured using a 470 nm/525 nm (excitation/emission) filter set, and the red particles were captured using a 560 nm/630 nm filter set.
The expected number ratios of the two particles in the mixture
calculated using eqn (1), and the observed number ratios measured from the self-assembled monolayers are summarized in Table 1.
, where θjk is the angle between the vector rjk that connects particle k to particle j, and the x-axis. An existing Python library (PairCorrelation) was used to calculate the radial distribution function g(r) from colloidal crystal images.
| χ4(t) = N [〈Q(t)2〉t − 〈Q(t)〉t2] |
A particle was defined as mobile if its displacement at a time interval Δt is greater than a threshold displacement
, where d is the average particle diameter. The temporal fluctuations of Q(t) was calculated from 100 images captured at every 30 s of time intervals.
![]() | (2) |
Interaction between type 2 (large) particles:
![]() | (3) |
Interaction between type 1 (small) and type 2 (large) particles:
![]() | (4) |
The finite diameters of the smaller and the larger particles were represented by Δ1 + σ and Δ2 + σ, respectively. Five different size ratios m = 0.80, 0.82, 0.84, 0.86, 0.88 were applied to simulate different degrees of asymmetry in particle sizes. The values of Δ2 and
were calculated for each m and for a fixed value of Δ1 (all parameters listed in Table 2). The value of σ was calculated from the experimental estimate of the range of depletion interaction – 4% of the diameter of the smaller particles, i.e.,
. Since the ratio of the interaction strengths,
is true for depletion forces, ε2 and
were calculated from the values of ε1 and m. The cutoff distance rc was chosen to be approximately 1.5 [(Δ1 + σ) + (Δ2 + σ)] to reduce the computation time.
cases. The following equations were solved to calculate N1 and N2.![]() | (5) |
000 is the total area covered by all particles in the simulation box, and![]() | (6) |
N
1 : N2 (small : large) |
N 1 | N 2 | |
|---|---|---|---|
| m = 0.80 | 90 : 1 |
24 713 |
273 |
9 : 1 |
21 420 |
2381 | |
1 : 1 |
9808 | 9827 | |
| m = 0.82 | 90 : 1 |
24 727 |
272 |
9 : 1 |
21 572 |
2353 | |
1 : 1 |
10 102 |
10 077 |
|
| m = 0.84 | 90 : 1 |
24 727 |
272 |
9 : 1 |
21 757 |
2449 | |
1 : 1 |
10 836 |
10 840 |
|
| m = 0.86 | 90 : 1 |
24 732 |
273 |
9 : 1 |
21 769 |
2435 | |
1 : 1 |
10 607 |
10 639 |
|
| m = 0.88 | 90 : 1 |
24 727 |
283 |
9 : 1 |
21 947 |
2459 | |
1 : 1 |
10 976 |
10 984 |
|
to
over a period of 5 × 105 iterations, with the time step of each iteration, τ = 0.001 s. We confirmed that closely packed crystalline structures were found at the end of the simulation period for every set of parameters (Table 3). We found that the energy reaches the minimum for all simulations that were performed for longer than 105 iterations (for both τ = 0.01 and τ = 0.001). The minimum energy value was also consistent with the one found using conjugate gradient energy minimization on LAMMPS (Fig. S1, ESI†).
We find no evidence of self-assembly at SDS concentrations below 30 mM (Fig. S2, ESI†). The particles remain in a fluid phase with SDS concentration of 30 mM and in a fluid-crystal co-existent phase at 32 mM (Fig. 1a). We observe the formation of polycrystalline monolayers that cover the entire glass surface with higher SDS concentration of 34 mM (estimated particle–particle bond energy Eb ≈ −Umin ≈ 5.6kBT, ESI,† Section S2) and 36.5 mM (Eb ≈ 6.1kBT). The particle–particle interaction is even stronger at 38 mM and 42 mM of SDS, resulting in gel formation. From the phase behavior, we conclude that equilibrium assembly can take place through multiple particle binding and unbinding events only when the SDS concentration is in the range of 34–36.5 mM. We estimated the range of the attractive interaction to be about 4.84% of particle diameter by analysing a snapshot of the assembled colloidal crystals (Fig. S3, ESI†). The average center-to-center distance between nearest neighbors was found to be about 734 nm, only 34 nm larger than the particle diameter (700 nm).
Next, we studied 2D binary assemblies by mixing 34 mM of SDS with polystyrene microspheres of two different diameters, d1 = 700 nm and d2 = 790 nm, (Fig. 1b and c). The polydispersity index of the polystyrene particles was less than 3%, as reported by the supplier. Both particles, small and large, remain stable in the suspension at the applied concentration (0.5% w/w, volume fraction ϕ = 0.005) on their own as well as when mixed with each other (Fig. S4 and S5, ESI†). The structure and dynamics of the self-assembled monolayers were observed in real-time using an optical microscope (Olympus ix83) equipped with fluorescence imaging capabilities and a 100× oil immersion objective lens (NA = 1.45). Particles with diameter d1 = 700 nm and d2 = 790 nm were identified from their fluorophore labels – green and red colors, respectively. The self-assembled monolayers formed after leaving the mixture solution in a sealed sample chamber for several hours (Fig. 1d). Since the height of our sample cell (about 360 μm) was much larger than the particle diameter, we do not expect to observe any effect of the hydrodynamic interactions resulting from the spatial confinement. The observed number ratio of the two particles
in the self-assembled monolayer was found to be very close to the expected number ratio calculated from the volume ratio of the two suspensions (Table 1). The small difference could be due to the marginally stronger interaction potential between the larger particles and their lower diffusivity and higher sedimentation rate.
We investigated how the mixing ratio of the two types of particles impact the crystalline order of the formed layers. The difference in crystalline order is evident from the corresponding Voronoi diagrams and the radial distribution function g(r), as shown in Fig. 2. The 1
:
1 mixture (700 nm
:
790 nm) sample exhibit more 5- and 7-fold defects (Fig. 2a) and reduced heights in higher-order peaks compared to the 39
:
1 (700 nm
:
790 nm) mixture sample (Fig. 2b). The hexatic order parameter can be used to quantify the degree of six-fold rotational symmetry around every particle,
. The average
was calculated from micrographs of particles at five different positions in a sample, each consisting of about 7500 particles, after 22 h of observation. While the polycrystalline structures in the 39
:
1 mixture had a higher average hexatic order of
, the 1
:
1 mixture showed a much lower value of
(distributions of |ψ6| shown in in Fig. S6, ESI†). The lack of crystalline order was consistently observed in samples with different particle concentrations –
in a 0.13% (w/w) particle suspension and
in a 0.25% (w/w) suspension (Fig. S7, ESI†). This result clearly indicates that the self-assembled structures transition from crystalline to amorphous for a higher fraction of impurities and thereby offers a mechanism for precise tuning of the crystalline order in 2D colloidal assemblies.
Although it may not be surprising that the addition of impurities frustrates crystalline order in binary assemblies, there are two possible mechanisms behind this frustration. The first one is a topological frustration induced by the size mismatch that would reduce the crystallinity of the equilibrium states. And the second one is a kinetic frustration induced by the specific crystal growth mechanism that restricts the assembly from reaching its equilibrium state.
To investigate the possibility of topological frustration, we developed a molecular dynamics simulation model that allows us to identify the equilibrium assembly structures for a wider range of parameters. The simulation was performed using the open-source molecular dynamics simulation package LAMMPS.53 The different sizes of the particles were implemented by using shifted Lennard-Jones (LJ) potentials (eqn (2)–(4)), where Δ1 + σ represents the diameter of the smaller particles (green) and and Δ2 + σ represents the diameter of the larger particles (red).54 The range of the attractive interaction potential was fixed at 4% of the smaller particle diameter to mimic the experimental range of attractive potential (about 34 nm).48,55 The shapes of the applied LJ potential between different particle pairs are shown in Fig. 3a.
We identified the minimum energy states of the 2D assembly for different size ratios,
by performing simulated annealing. We observe a reduction in the average hexatic order,
, with increasing fractions of impurities, specifically for cases where the difference in the particle sizes was larger (smaller m). For example,
decreases from 0.89 to 0.69 as the mixture ratio varies from 90
:
1 to 1
:
1 when the simulation is performed at m = 0.80 (Fig. 3b). However, the average hexatic order
does not decrease when two particle types have closely matched diameters, i.e., m = 0.88 – a size ratio that represents the experimental sample. The assembled structures found at the minimum energy states are shown in Fig. 3c – polycrystalline structures and clearly separated grain boundaries form when the fraction of impurities is small (90
:
1) for both m = 0.80 and m = 0.88. In contrast, randomly distributed defects and voids are observed in the 50% mixture ratio (1
:
1) sample (Voronoi diagrams in Fig. S8, ESI†). The constant
value in the 1
:
1 and the 90
:
1 mixture for m = 0.88 indicates that the energy cost of the grain boundaries in the 90
:
1 mixture matches the energy cost of the voids in the 1
:
1 mixture. As the mismatch in particle diameters becomes larger, e.g., for m = 0.80, the number of defects increases, causing a significant reduction (22%) in the average hexatic order. The computational results indicate that the formation of amorphous solids in the presence of a large size mismatch can be explained primarily from the energetics of the system. This finding is consistent with prior experiments that observed glass formation in binary samples with a size ratio of 0.77 and 0.81.47,56
Additionally, we quantified the translational order of the assembled structures by quantifying the distributions of the center-to-center distance between neighboring particles, DB. As shown in Fig. 3d and e, the average
and the standard deviation of the distribution, δDB gradually increases with the increasing fraction of impurities (both for = 0.80 and m = 0.88). This increase is more prominent in the presence of large size mismatch as demonstrated in Fig. 3f. The finding indicates that the translational order is more sensitive to marginal mismatches in particle diameters than the orientational hexatic order. Although the asymmetric bond lengths between particle pairs reduce the average translational order, the deviation is not high enough to compromise the mean orientational order in the 1
:
1 binary mixture for m = 0.88. Therefore, the simulation results confirm that a marginal size mismatch (such as m = 0.88) cannot introduce enough topological frustration to reduce the hexatic order of a binary mixture sample as high as 18%.
To strengthen our conclusion, we examined the hexatic order for the m = 0.88 sample numerically for an even shorter range of attractive interaction – 0.22% of the particle diameter. We found that the hexatic order shows only a 2% reduction when the number ratio varies from 90
:
1 to 1
:
1 (Fig. S9, ESI†), much smaller compared to the 18% reduction observed in the experiment. We also examined the thermodynamic equilibrium states by exciting the ground state crystal structures with an increased temperature of kBT. We found that the hexatic orders of all mixture ratios (90
:
1, 9
:
1, and 1
:
1) decrease equally from 0.89 to 0.82 at room temperature, yet any notable reduction was absent in the 1
:
1 sample compared to the 90
:
1 sample (Fig. S9, ESI†). Therefore, we conclude that the near equilibrium structures computed in the simulations do not explain why we observe a large reduction of
(18%) in the m = 0.88 sample when the mixture ratio changes from 90
:
1 to 1
:
1.
Therefore, we shift our focus to the investigation of the crystal growth mechanism to explore the possibility of kinetic frustration. In Fig. 4a, the mean hexatic order plot is shown for samples with a few different volume ratios – 39
:
1, 19
:
1, 9
:
1, and 1
:
1, observed at different times and assembled with different SDS concentrations (i.e., different bond energy). We find the general trend of gradually decreasing
with increasing fraction of “impurity” (790 nm, red) particles. We also notice that the addition of impurities slows down the crystallization process. The sample with a higher SDS concentration (36.5 mM, Eb ≈ 6.1kBT) reaches its maximum crystalline state within about 90 min for all mixture ratios. In contrast, the sample with lower SDS concentration (34 mM, Eb ≈ 5.6kBT) crystallizes slowly, especially when impurities are added (compare the dark blue and cyan curves on Fig. 4a). In this case, a monodisperse sample crystallizes with
within only 3 h; however, the 19
:
1 mixture ratio takes about 22 h to obtain a similarly higher magnitude of
. It is expected that the average hexatic order for a sample with higher bond energy will be slightly smaller, because of the more frequent nucleation from different sites (the black curve is situated lower than the dark blue curve). Notably, we observe that the hexatic order of the 1
:
1 mixture is low for both SDS concentrations, regardless of the long observation time of up to 22 h. Upon close examination of the assembled structures in the 19
:
1 sample (Eb ≈ 5.6kBT after 22 h), we notice that the ordered regions of the assembly consist mostly of the 700 nm particles (green) while the 790 nm particles (red) locate themselves in between the boundaries of different crystalline grains. All these observations indicate that the crystallization pathway is different in a suspension with large number of impurities compared to a monodisperse suspension.
Colloidal crystallization driven by short-ranged depletion interaction is known to follow a two-step nucleation pathway, distinct from the mechanism explained in the classical nucleation theory.30 Savage et al. found that especially at a high area fraction, the assembly first forms amorphous clusters and grows in that state until a sudden increase in the hexatic order occurs resulting a crystalline state. The mechanism behind this two-step nucleation was explained by the reduction of the line tension in the intermediate amorphous phase that compensates for the lower bulk energy caused by the short interaction range. This is indeed what we observe in the crystallization pathway of the monodisperse sample (Fig. 4b and c) – the assembly first grows in the amorphous state, and then stable crystallites start developing at about 40 min, which eventually grow and form boundaries between multiple crystalline grains (at t = 60 min, Fig. 4c). However, in the binary sample, growth in this amorphous state continues for the entire timespan of the assembly, as depicted by the slow growth curve in Fig. 4b and the snapshots in Fig. 4c. The absence of two-step nucleation is binary mixtures is likely due to the size mismatch that causes a further reduction of the bulk energy in a binary simple compared to a monodisperse sample – as evident from the calculation of higher nucleation barrier in binary systems.57 From the hexatic order plots during the early stage of crystal growth (0–60 min, Fig. 4b), we observe the signature of a two-step growth mechanism only in the monodisperse suspension. Both the monodisperse and the binary mixture show a linear growth for the first 20 min, followed by a non-linear growth in the monodisperse sample and a continued linear growth in the binary sample (full field of view images and longer time growth characterization shown in Fig. S10 and S11, ESI†). We also examined different intermediate mixture ratios, such as 9
:
1, 5
:
1, and 3
:
1 (Fig. S12, ESI†) – although we observe the formation of stable grains via two-step nucleation in the 9
:
1 mixture sample, it becomes a rarer event when the fraction of the impurities increases in the 5
:
1 and 3
:
1 mixtures. From all the observations, it is reasonable to conclude that the second step of nucleation is much more likely to occur in a region where a critical number of particles with the same size can gather. Since it takes long time for this gathering to occur in the presence of the impurities, the 19
:
1 and 9
:
1 mixtures exhibit slower rates of growth in reaching their maximum
value (Fig. 4a), and the 1
:
1 mixture remain frustrated for the entire timespan of observation (with a maximum
of only 0.63 after 22 h, Fig. 4a).
We verified that the major impact caused by the impurities is the two-step nucleation, and not the difference in deposition rate or the formation of second layers. The rate at which the particles attach to the surface, i.e., the deposition rate remains equal for both samples during the early stage of growth (Fig. S13, ESI†). The growth only slows down after 40 min for the binary sample due to the lack of available space for deposition. Therefore, we can conclude that the deposition rate is not the cause of kinetic frustration in the binary samples. Furthermore, the growth of second layers is only observed on top of a highly crystalline first layer, which acts a solid surface and induce a depletion interaction between the first layer and the second layer (Fig. S14a, ESI†). We do not observe any second layer formation in the 1
:
1 binary sample because of the highly amorphous first layer, indicating that the second layer cannot induce the kinetic frustration either.
Finally, we quantify the particle dynamics in the amorphous layer of the 1
:
1 binary mixture to identify any signature of arrested dynamics. The microscopic dynamics of the amorphous state was captured after the assembly continued for 80 min (Movie S1, ESI†). While freely diffusing particles before assembly take 1 s to move 1 μm2 (mean-squared displacement), the particles in the assembled layer of the binary sample take about 970 s to move only 0.1 μm2 (Fig. 5a). Additionally, we observe multiple partial vacancies in the assembly and cooperative particle movement adjacent to the locations of the partial vacancies. An example of the cooperative motion is presented and quantified in Fig. 5c. Because of the remarkably short interaction range, particles fail to interact with each other across a partial vacancy and continue to rearrange their positions locally due to their Brownian motions. These local movements result in continuous hopping of the vacancy locations (Fig. 5c and Movie S1, ESI†). Because of the high surface coverage, the fluctuating particles can support the relocation of their nearest neighbors, causing the cooperative movement observed in certain spots. Particle motion of this nature contributes to the overall arrested dynamics, which is a common feature observed near glass transition.58,59 The four-point susceptibility, χ4, calculated from a 50 μm × 30 μm region of the sample (Fig. S15, ESI†) shows a peak near 600 s (Fig. 5b), demonstrating the signature of spatiotemporal heterogeneity in colloidal glasses.47 Furthermore, when a stronger interaction potential is applied by increasing the concentration of the depletant micelles, the binary sample forms colloidal gels (Fig. S16, ESI†), transitioning from one nonequilibrium phase to another.
:
1 binary mixture compared to the monodisperse suspension. The order reduces gradually as the fraction of the impurity particles increases in the binary mixture. By carefully examining the crystallization kinetics, we find that the two-step nucleation mechanism that drives crystallization in the presence of short-ranged depletion interaction is responsible for the observed phenomenon. After growing in the amorphous state during the first step, the monodisperse sample enters the second nucleation step to rapidly form stable crystallites while the binary sample continues to grow in the amorphous state until the particle dynamics becomes arrested. These results have important implications for our general understanding of the mechanisms behind amorphous solid formation that originate from thermodynamic, kinetic, or topological conditions. Our findings on 2D binary assembly demonstrate that the frustration in growth kinetics can dominate over the topological frustration when a small mismatch in particle size is introduced. Leveraging this kinetic pathway of colloidal glass formation can stimulate progress in the fundamental studies on glass transitions59–62 as well as applications focused on photonic glasses.63–65 In addition, the binary mixtures with intermediate volume ratios (19
:
1 and 9
:
1) allow the nucleation of small crystallites whose growth is then inhibited by the presence of the impurities. Applications of this self-limiting formation of crystal grains could enable the design of polycrystalline and epitaxial colloidal materials10,66–69 with precisely tuned optical and mechanical properties.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5sm00433k |
| This journal is © The Royal Society of Chemistry 2025 |