Gauri M.
Nabar§
a,
Abhilasha V.
Dehankar§
a,
Elizabeth
Jergens
a,
Benworth B.
Hansen
a,
Ezekiel
Johnston-Halperin
b,
Matthew
Sheffield
b,
Joshua
Sangoro
a,
Barbara E.
Wyslouzil
ac and
Jessica O.
Winter
*ad
aWilliam G. Lowrie Department of Chemical and Biomolecular Engineering, The Ohio State University, 151 W. Woodruff Ave., Columbus, OH 43210, USA. E-mail: winter.63@osu.edu
bDepartment of Physics, The Ohio State University, Columbus, Ohio 43210, USA
cDepartment of Chemistry and Biochemistry, The Ohio State University, 151 W. Woodruff Ave., Columbus, OH 43210, USA
dDepartment of Biomedical Engineering, The Ohio State University, 151 W. Woodruff Ave., Columbus, OH 43210, USA
First published on 12th April 2024
Superparamagnetic iron oxide nanoparticles (SPIONs) have attracted significant attention because of their nanoscale magnetic properties. SPION aggregates may afford emergent properties, resulting from dipole–dipole interactions between neighbors. Such aggregates can display internal order, with high packing fractions (>20%), and can be stabilized with block co-polymers (BCPs), permitting design of tunable composites for potential nanomedicine, data storage, and electronic sensing applications. Despite the routine use of magnetic fields for aggregate actuation, the impact of those fields on polymer structure, SPION ordering, and magnetic properties is not fully understood. Here, we report that external magnetic fields can induce ordering in SPION aggregates that affect their structure, inter-SPION distance, magnetic properties, and composite Tg. SPION aggregates were synthesized in the presence or absence of magnetic fields or exposed to magnetic fields post-synthesis. They were characterized using transmission electron microscopy (TEM), small angle X-ray scattering (SAXS), superconducting quantum interference device (SQUID) analysis, and differential scanning calorimetry (DSC). SPION aggregate properties depended on the timing of field application. Magnetic field application during synthesis encouraged preservation of SPION chain aggregates stabilized by polymer coatings even after removal of the field, whereas post synthesis application triggered subtle internal reordering, as indicated by increased blocking temperature (TB), that was not observed via SAXS or TEM. These results suggest that magnetic fields are a simple, yet powerful tool to tailor the structure, ordering, and magnetic properties of polymer-stabilized SPION nanocomposites.
Such aggregates can be generated through a variety of methods, including DNA origami for precision placement14–16 or less ordered structures through colloidal self-assembly.17,18 Colloidal aggregates are an attractive choice because of their ease of synthesis. The structure of these colloidal aggregates is primarily determined by the effective interaction potential resulting from the cumulative fundamental attraction and repulsion forces between SPIONs, such as van der Waals, steric, magnetic dipole, and electrostatic forces from attached ligands. Such forces can be leveraged to alter not only the final structure, but also any metastable structures that form during synthesis. For example, magnetic fields applied during synthesis may induce structural transformations that effect ordering in the final material, altering the collective magnetism of the aggregate. A deeper understanding of these magnetically induced structural transformations could provide opportunities to tailor 3D SPION aggregate properties through external magnetic field application. Most previous studies of SPION colloidal clusters have focused on tuning their magnetic properties through synthesis methods.4,19–22 The influence of magnetic fields applied during and post-synthesis on structural ordering has yet to be explored. Also, few of these studies examined the influence of nanoparticle magnetic ordering on the properties of the polymers used to stabilize these aggregates.
Our group has established a new route to NP aggregates via self-assembly assisted by polystyrene (PS)-b-polyethylene oxide (PEO) block copolymers (BCPs). Densely loaded aggregates formed that consist of NP aggregates coated by amphiphilic BCPs rendering them soluble in aqueous media. These structures exhibit high NP volume concentration (up to 24%) with semi-ordered packing and NP separation distances smaller than NP diameters (e.g., ∼2 nm edge-to-edge for ∼6 nm NPs).23 These loadings are well above those of commercial magnetic particles used for cell separation, which have magnetic NP packings between 5–10%.24 For example, an 80 nm diameter, densely loaded aggregate can contain up to 900 encapsulated SPIONs, making this vehicle an ideal model system for evaluating the effect of magnetic fields on emergent SPION aggregate properties and 3D superlattice formation.
Here, we leveraged the high packing volume and low inter-NP spacing of these densely loaded SPION aggregates to assess the impact of magnetic field application during and after synthesis on emergent structural and magnetic properties of SPION clusters. Nanoscale aggregate morphology was evaluated using transmission electron microscopy (TEM) and image analysis. NP packing was examined using complementary small angle X-ray scattering (SAXS) measurements of aggregate solutions. Magnetic properties, specifically coercivity and blocking temperatures, were measured using a superconducting quantum interference device (SQUID). Changes in stabilizing polymer properties, specifically Tg, were measured using differential scanning calorimetry (DSC). Morphology and changes in polymer and magnetic properties were used to establish structure–property relationships for densely loaded aggregates with differing SPION orientations, including structural and magnetic ordering induced by external magnetic fields. This work presents an investigation of magnetically induced ordering in densely loaded SPION aggregates. Such composites offer promise for applications requiring tailored magnetic ordering and fields, including magnetic resonance imaging, cell separations, and magnetic storage.
SPION nanocomposites formed in the presence of a magnetic field will be referred to as magnetically stirred SNC or denoted by SNC-St. To produce the SNC-St, an emulsion was initially generated by manual shaking in a glass vial (internal diameter = 2.3 cm) and then stirred at 60 rpm using a magnetic stir bar (Alnico, forged steel, Fig. S1, ESI‡) with a maximum magnetic flux density of 60 Oe under atmospheric conditions for 12 hours.
In both synthesis methods, unencapsulated SPIONs were eliminated by centrifugation at 4000 rcf for 1 minute. Because of the mechanism involved, the interfacial instability method yields samples that contain densely loaded aggregates,23 micelles incorporating SPIONs (i.e., SPION-micelles) and SPION free micelles (i.e., empty micelles). In densely loaded aggregates a cluster containing many SPIONs occupies the central volume of the micelle, whereas SPION-micelles exhibit a void volume with a low number of encapsulated SPIONs. Clusters were classified in TEM images using these characteristics.
We first evaluated SNCs produced at a 1:
1 NP
:
polymer molar ratio in the absence of magnetic fields. Under these conditions, both densely loaded aggregates (8.5% by number) and micelles (with or without SPIONs) (91.5%) were observed (Table 1). Densely loaded aggregate populations displayed average diameters of 62.4 ± 27.0 nm and log-normal size distribution; some internal NP ordering (i.e., chaining) was also observed with centre to centre spacing of ∼5.6 ± 0.94 nm (Fig. 2). In contrast, SPION-micelles displayed sizes of ∼25.6 ± 8.0 nm with log normal size distribution and no observed NP ordering. NPs were not tightly packed and there were heterogeneities in NP distribution throughout the micelle. The sizes reported here for both populations were not statistically different from those we reported previously23 (i.e., α = 0.05). The increased polydispersity of densely loaded aggregates compared to micelles could be explained by variation in aggregate nucleation and growth kinetics, which depends on uncontrolled factors in this system, such as local gradients in NP and polymer concentrations, interparticle distance in solution, and thermal fluctuations. The tight NP packing, as well as occasional chaining, observed within densely loaded aggregates, but not SPION micelles, is consistent with our previous small angle X-ray scattering (SAXS) analysis,23,29 in which spectra could only be fit by including a hard sphere structure factor.
Sample | N | Aggregatesb (nm) (%) | Micelles (nm) (%) |
---|---|---|---|
a Number of particles analysed. b Percent by number of nanocomposites classified as aggregates or micelles. | |||
SNC | 779 | 62.4 ± 27.0 | 25.6 ± 8.0 |
8.5 | 91.5 | ||
SNC-St | 345 | 107.0 ± 39.0 | 32.4 ± 8.0 |
24.2 | 75.8 | ||
SNC-P | 352 | 50.2 ± 21.0 | 26.2 ± 8.0 |
39.5 | 60.5 | ||
SNC-S | 1192 | 54.6 ± 22.0 | 23.2 ± 8.8 |
8.1 | 91.9 |
In addition to changes in overall composite size, we also observed striking changes to internal structure within the densely loaded aggregates. In the SNC-St samples, semi-periodic SPION arrays emerged (Fig. 4) that were not observed in the densely loaded aggregates found in the SNC samples (Fig. 2). Within a linear array, the centre-to-centre SPION distance is ∼3.72 ± 0.61 nm, but spacing between linear arrays increases to ∼7.29 ± 0.81 nm (two replicates, N > 100). This internal ordering indicates a transition to a more structured phase. Since TEM images are 2D projections of 3D objects, the radial organization of SPIONs within these structures cannot be fully evaluated. Furthermore, 2D projection effects may be largely responsible for particle centre-to-centre distances that are smaller than the diameter of individual SPIONS.
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Fig. 4 (A) TEM images of an example a SNC-St, with (B) increased ordering indicated by the formation of periodic linear arrays (yellow lines), (C) fast Fourier transform (FFT) of (A). The diffraction spots (green arrow) and outer elliptical halo indicating directional semi-periodicity (yellow) in the FFT are consistent with reports of short range order,1 (D) FFT of a SNC shown in Fig. 2. No diffraction spots are observed in these samples. |
The presence of a magnetic field likely played a strong role in aggregate formation. It has been established that field-induced increases in SPION magnetic moment strength and alignment can trigger the formation of uniformly sized, linearly aligned SPION arrays.31 During aggregation, SPIONs will spontaneously align their easy axes to minimize their free energy by dipole coupling. These SPION arrays may then form densely loaded aggregate through nucleation and growth mechanisms. SPION arrays interact via strong dipole–dipole interactions that are stronger than those of SPIONs not exposed to a magnetic field. Array aggregation will depend on the competition between dipole coupling within the existing aggregate and that with the incoming SPION array, as aggregates will attempt to minimize their overall free energy. To integrate a new SPION array into the aggregate, SPIONs must either internally realign their magnetic dipoles or physically arrange the incoming array to minimize the resulting free energy. Beyond a limiting size, strong internal dipole coupling within the existing densely loaded aggregate may repel addition of new SPION arrays. Additionally, steric limitations for SPION arrays magnetic field much higher than those for individual SPIONs. Thus, the shift from log normal to Gaussian size distribution and the increase in ordering in the presence of magnetic fields observed in densely loaded aggregates may result from SPION arrays comprised of individual SPIONs aligning their magnetization with the rotating magnetic field of the stir bar against thermal fluctuations.
In addition to the application of a magnetic field during synthesis, emulsion solutions also experienced increased and longer mixing during the solvent evaporation phase resulting from magnetic stirring compared to solutions that were left on a rocker during the solvent evaporation phase. This may have resulted in changes in emulsion droplet size, solvent evaporation rates, and solvent concentration profiles. For example, faster solvent evaporation should increase the formation of non-equilibrium structures as a result of kinetic trapping.
Thus, magnetic forces combined with enhanced mixing likely account for the statistically significant size increase observed in the densely loaded aggregates associated with SNC-Sts vs. SNCs, as aggregate growth is stabilized against thermal fluctuations by magnetic forces. This phenomenon has been previously observed in solution32 in the absence of BCPs and may be augmented by short-range, attractive van der Waals forces between NPs. Thus, the combination of the attractive magnetic and van der Waals forces, aided by the presence of BCP that serves as an entropic barrier to reconfiguration, likely stabilizes semi-ordered NP aggregates so that structure is maintained even after the external magnetic field is removed. In these structures the BCP may intercalate between linear arrays as well as coating the surface of the aggregate and intercalating within the first few NP layers. The preserved internal structuring observed here is highly desirable because increased ordering can lead to enhanced magnetism.31
The percent of densely loaded aggregates and micelles (i.e., empty or SPION) and their sizes were quantified in both SNC-P and SNC-S samples (Table 1). The percentage of densely loaded aggregates in the SNC-P sample increased (39.5%) after magnetic exposure relative to the population prior to magnetic exposure (8.5%) and the population in the SNC-S sample (8.1%). With post-synthesis magnetic field exposure, densely loaded aggregates displayed log normal size distributions with mean sizes of ∼50.2 ± 21.0 nm and ∼54.6 ± 22.0 nm for the SNC-P and SNC-S samples, respectively (Table 1). There was no statistically significant difference in mean densely packed aggregate size (significance level of α = 0.05) between the SNC-P, SNC-S, and SNC samples. Furthermore, there was no obvious difference in SPION arrangement within the densely loaded structures in either magnetically treated sample relative to the control. Thus, although magnetic field exposure post-synthesis enriched the pellet with densely loaded aggregates, it did not change mean size or visible internal ordering, unlike magnetic field exposure during synthesis. As these structures are derived from SNC samples not exposed to fields, BCP arrangement is expected to be similar with hydrophobic chains interacting with the NP aggregate surface and possible intercalating with selected NPs. Structures that appeared to have ‘fused’ via polymer bridges were occasionally seen in the SNC-P samples, but not in control samples (Fig. S4 and S5, Supplemental Results and discussion, ESI‡). Further investigation necessary to determine the origin of these fused structures is beyond the scope of this investigation.
The accumulation of more densely loaded aggregates in SNC-P is consistent with the larger magnetic force experienced by these nanocomposites compared to the smaller, individual SPIONs or SPION micelles and the higher diffusivity of the latter relative to the former. Previously, we have shown that magnetic forces on the order of 0.1–0.2 pN are required to capture similar nanocomposites33,34 and that neodymium magnets can capture particles within ∼2 μm of their surfaces.35 The absence of significant size change in the pellet or supernatant can be explained by structure stabilization engendered by strong van der Waals forces, dipole–dipole interactions between SPIONs, and entropic stabilization provided by the BCPs. These results indicate that magnetic forces applied after composite formation were not sufficient to break BCP entropic barriers to change composite size, at least at the strengths investigated here. Based on the test tube thickness and the magnet employed, exposure resulted in a magnetic field gradient of 2000 ≤ magnetic field (Oe) ≤ 5000 across the entire sample (Fig. S3, ESI‡), which would vary in the z dimension during composite diffusion. Although the densely loaded aggregate population in the SNC-P sample was enriched, the lack of complete removal of densely loaded aggregates from the SNC-S most likely resulted from field variation in the z dimension. Additional research is needed to optimize the magnetic field gradient, exposure time, and sample orientation for more efficient size-based magnetic concentration.
All samples made in the absence of a magnetic field display a peak at the same location, q = 1.10 Å−1, irrespective of whether they were exposed to a magnetic field post-synthesis. This value of q corresponds to a characteristic spacing d = 2π/q = 5.7 nm. Complementary TEM results yield an average interparticle spacing of 5.61 ± 0.94 nm for these samples. The latter value is in good agreement with the SAXS value. The full width at half max (FWHM) of these peaks are all close to ∼0.11 nm−1, suggesting the interparticle distance does not vary significantly in the particles that contribute to this peak. SPIONs are coated with an oleic acid capping ligand with a molecular size of ∼2 nm, thus nanoparticles are likely not directly touching in these samples.
In contrast, the SNC-St samples produced in the presence of the magnetic field show a peak at a slightly lower value q = 1.05 nm−1, corresponding to d = 5.98 nm. The full width at half max of these peaks is ∼0.10 nm−1. The increase in distance observed in SAXS is consistent with the presence of a longer spacing length scale observed between the adjacent chains of aligned particles. Given the broad distribution of particle spacings (Fig. 3C) and the presence of less well-organized particles within the aggregates; however, it is not surprising that we do not see two peaks – one corresponding to each interparticle spacing observed in TEM. Finally, the SAXS results confirm that the TEM images are representative of the aggregates throughout the solution.
However, when analysing SPIONs in close proximity, such as in densely loaded aggregates, dipole–dipole interactions (Edd) become relevant. As a result, TB is proportional to an additive function of Ea and Edd, and HC is also altered.39 These dipole interactions can align head-to-tail in-line or in vertical ferromagnetic (parallel) or anti-ferromagnetic (antiparallel) arrangements (Fig. 7). Effective Edd decreases (and free energy increases) in the order of head-to-tail in-line > antiferromagnetic > ferromagnetic orientation. Thus, head-to-tail in-line orientation is energetically most-favoured during SPION assembly in 1D, and results in the highest TB. Similarly, effective Ea and therefore HC for in-line or ferromagnetic orientations is higher than that of antiferromagnetic orientations. However, in a 3D cluster of SPIONs, this relationship is much more complex. Similar to TB, HC of the interacting system is also influenced by the dipole coupling between SPIONs and depends on the dipole-coupled shape anisotropy and volume.31 Thus, measurements of TB and HC can provide critical information on the structure of magnetic field treated and untreated densely loaded aggregates present in the SNCs, as well as insights into their structure–property relationships.
We investigated the difference in magnetic properties of dispersed SPIONs and SNC, SNC-St, SNC-P, and SNC-S samples (Table 2 and Fig. S6–S11, ESI‡). Individual SPIONs were dispersed in a PMMA matrix to prevent interactions during testing. Dispersed SPIONs lack ordering and have the lowest TB. The SNC samples have increased ordering and dipole–dipole interactions, and thus have a TB double that of dispersed SPIONs. SNC-St and SNC-P samples follow the same trend of increased TB with increased ordering. Interestingly, this trend is not observed in the SNC-S sample, which exhibits the same TB as the SNC sample. The differences in HC are too small to reveal statistically significant structural/magnetic insight for all the samples.
Sample | T B (K) | H C (Oe) |
---|---|---|
a Normalized standard deviation of magnetic measurement fits are reported in Table S1 (ESI). | ||
Dispersed, individual SPIONs | 8 | 50 |
SNC | 16 | 67 |
SNC-St | 20 | 78 |
SNC-P | 24 | 50 |
SNC-S | 16 | 67 |
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Fig. 8 Melting (Tm) and glass transition (Tg) temperatures for pure PS-PEO polymer, SNC, SNC-P, SNC-S, SNC-St samples, and PS-PEO micelles. |
Pure PS-PEO polymer examined as a control exhibited a melting transition at 53.4 °C, which was not observed in any of the SNC samples tested. SPION nanocomposites yielded glass transitions even with relatively slow rates of cooling, suggesting easy supercooling. The SNC sample displayed a Tg of 27.4 °C, whereas the SNC-P and SNC-S samples show Tg values of 27.4 and 26.7 °C, respectively. Since these values are largely unchanged from the SNC sample, it is likely that magnetic exposure post-synthesis does not produce a systematic change in polymer chain interactions. The SNC-St sample exhibited a Tg of 8.6 °C, a marked decrease of nearly 20 degrees from the other SNC samples investigated. Glass transitions are directly dependent on dynamic intermolecular forces, so a sharp decrease in Tg suggests that changes introduced into the structure of SNC-St either reduce the overall intermolecular force strength or increase the free volume of the system. Increased ordering seen in TEM can cause a decrease van der Waals forces, leading to the noticeable decrease in Tg. Similarly, when a sample of pure micelle structures with no SPIONs is tested, there is an increase in Tg (up to 40.9 °C) suggesting the opposite is happening. This is likely results from the lack of SPION encapsulation changing the packing and volume fractions. The observation of a single Tg suggests that the BCPs behave as statistical polymers in this confinement regime. If the different polymer domains were still distinct, we would expect the Tg to be around −55 °C (Lindeman's criterion verified by experiments of confined PEO, e.g., in ref. 40), which is not the case. These data suggest the possibility of single chain confinement between nanoparticles and nanoparticle arrays.
Although modifications in morphology and structure have previously been achieved by changing reaction conditions, such as using different stabilizing polymer compositions21 or concentrations,23 these methods are severely limited in controlling magnetic order in colloidal SPION aggregates. The use of magnetic fields provides a unique opportunity to manipulate magnetic structure, in addition to physical structure, of densely loaded aggregates that could potentially be applied to composites of differing composition. Further, diverse structural and magnetic modifications can be achieved, depending on the timing of magnetic field application (i.e., during or after synthesis), enabling experimental exploration of super-ferromagnetic and spin-glass phases of SPION assemblies. As a result, this technique offers enhanced capability to tailor 3D SPION aggregate structure and properties, by employing inherent properties of SPION constituents. As such, this approach could enable SPION aggregates to be harnessed for applications in targeted hyperthermia, separations, magnetic resonance imaging, or photonics.
Footnotes |
† Portions of this material were published in the PhD thesis of GMN36 and are cited where appropriate. |
‡ Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4sm00008k |
§ Gauri M. Nabar and Abhilasha V. Dehankar contributed equally to this work. |
This journal is © The Royal Society of Chemistry 2024 |