Koushik Saikiaa,
Debasis Senb,
Subhasish Mazumderb and
Pritam Deb*a
aAdvanced Functional Material Laboratory (AFML), Tezpur University (Central University), Tezpur, India. E-mail: pdeb@tezu.ernet.in
bSolid State Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India
First published on 24th November 2014
Nanoparticle clusters have become attractive secondary nanostructures due to their collective physical properties, which can be modulated as a function of their internal structure. In this study, a reassembling strategy of iron oxide nanoparticles prior to the formation of nearly identical nanoclusters of size 80 ± 20 nm as the secondary nanostructures is reported, where ordered arrangement of nanoparticle subunits with a narrow distribution of interparticle spacing is observed. Oleic acid capped iron oxide nanoparticles (IONPs@OA) with sizes of 5 ± 2 nm are used as the primitive assembly of subunits. Post-functionalization of these nanoparticles with surfactant cetyltrimethyl ammonium bromide (CTAB) and subsequently with polyelectrolyte polyacrylic acid (PAA) result in irregular aggregation of nanoparticles (IOagg@CTAB) and nanoparticle clusters (IONPCs@PAA) respectively. The orderly oriented carboxylate groups of PAA play an important role in dense packing of nanoparticles with an ordered arrangement inside the clusters. The observed fractal morphologies give an indication of interparticle interactions for all three systems irrespective of assembly, aggregation and reassembly. Henkel plots show the dipolar type of interaction for all three systems. The dominant effect of the interparticle spacing distribution over size on the modification of effective anisotropy energy barrier distribution is realized from the observed trend of ZFC (zero-field cooled) magnetization peak broadening and shifting.
Properties of the magnetic nanoparticles are believed to be dependent directly on their sizes.6–8 It is due to the modification of magnetic anisotropy energy with the size, which can even lead to the critical state like ‘superparamagnetic state’ below a particular size limit.9,10 In reality, it is not feasible to study the properties of a completely isolated magnetic nanoparticle. We can only deal with the assemblies of magnetic nanoparticles having different type of interparticle interactions, which can be of dipolar type or exchange type of interactions.11 The study on the related magnetic properties for such assemblies is challenging because here both the size and interparticle interactions have to be taken into consideration. In this scenario, development of assembly of nanoparticles with narrow size distribution and well-defined morphologies is of prime importance to control efficiently their physical properties. Apart from different secondary self-assembly strategies, there are few established synthesis techniques, which can lead to in situ formation of magnetic nanoparticles assemblies. Among these, thermal decomposition of organometallic complexes in presence of suitable capping agents,12 polyol synthesis method,13 co-precipitation of iron salts in highly basic medium14 etc. are commonly used. Assembly structures achieved through these routes solely depend on the nature of the capping molecules and reaction parameters like temperature, pressure etc. However, the fundamental concern of these in situ assemblies is retaining of similar size and morphologies of the nanoparticles with the variation of reaction parameters and the employed capping molecules.
In this aim, this work reports a novel strategy for the controlling of interparticle spacing during the formation of secondary nanostructures, keeping individual particle size, shape and phase identical. The process is achieved through an aggregation step followed by a reassembling step of iron oxide nanoparticles with the help of cationic surfactant CTAB and polyelectrolyte PAA. Polymer functional groups are utilized as the orderly oriented motifs, where positively charged CTAB functionalized nanoparticles are attached densely for resulting nanoparticle clusters. However, there are few reports on the clustering of iron oxide nanoparticles using polyelectrolyte-neutral block copolymers15 and different hydrogels,16 these methods are complicated and time consuming. In contrast, our reassembling based method is facile and cost effective for the preparation of nanoparticles clusters, where the strength of interparticle interaction and spatial arrangement play the important roles in determining the collective properties. The primitive assembly of iron oxide nanoparticles is prepared through in situ capping with oleic acid, where interparticle spacing seems to be least. Along with the direct microscopic tool like high resolution transmission electron microscopy (HRTEM), the small angle X-ray scattering (SAXS) technique is employed to estimate the size and interparticle spacing distribution in the assembly state, aggregation state and finally in the reassembling state. Since, SAXS gives the overall structural informations unlike HRTEM, it is more appropriate to correlate the SAXS data to collective magnetic properties for a reliable structure–property correlation. The collective magnetic properties of all three systems are explained based on the observed variation in interparticle interaction related to the change in interparticle spacing. Moreover, the change in spatial arrangement of the nanoparticles in the aggregation and reassembling is directly related to the collective magnetic properties.
The crystalline phase of the nanoparticles were studied with Rigaku X-ray diffractometer (XRD) equipped with intense CuKα radiation (λ = 0.154 nm). The XRD data at room temperature were collected over a 2θ scattering range 10–70° with a step 0.05°. High resolution transmission electron microscopy (HRTEM) images were recorded on a JEOL 2100 electron microscope operating at an accelerating voltage of 200 kV. For this characterization, the colloidal solution of nanoparticles were deposited on to carbon coated grids and then dried at gentle temperature to evaporate the solvents. Statistical analysis was carried out with the help of the ImageJ software. For each sample, particle size distribution was calculated on about 200 nanoparticles from multiple images in bright field mode and fitted with a log-normal function
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Atomic force microscopy (AFM) images of nanoparticles were recorded using Nanonics-AFM equipped with MultiView 1000 head intermittent contact mode. An N-type Si probe with tip radius <75 nm and resonance frequency 47–76 kHz was mounted to a standard silicon AFM tip mount. The scan was performed based on laser feedback mechanism with lower scanner movement. The Raman spectra of the samples were recorded using a Renishaw In-Via Raman spectrometer (Renishaw, UK) at a resolution of 0.3 cm−1. Ar+ laser of 514.5 nm wavelength is used for excitation. The used laser power was 0.1 mW and passed through a 50× objective for illuminating the samples. Magnetic characterizations such as field dependent magnetizations (M–H) and temperature dependent magnetizations (M–T) were studied using a Quantum design Dynacool PPMS (Physical Property Measurement System) equipped with a vibrating sample magnetometer and superconducting coil which produces magnetic fields in the range of −9 T to +9 T. Temperature dependent magnetizations were measured using ZFC (zero field cooling) and FC (field cooling) protocols. For ZFC, the sample was cooled in zero magnetic field from 300 K temperature to 10 K and subsequently magnetization was measured while warming the sample again to 300 K with a probe field 500 Oe. In contrast for FC, the sample was cooled in presence same probe field before measuring the magnetization with warming. For FC (M–H) measurement, the sample was cooled in presence of 5 T magnetic field to the measurement temperature (5 K) and then magnetization measurement was performed similar to normal M–H. The field dependence of remanent magnetization was measured using IRM (isothermal remanent magnetization) and DCD (direct current demagnetization) methods. For IRM, the sample was cooled to low temperature at zero field. After cooling, a small field was applied for 10 s, and then it was switched off and remanence was measured. The process was repeated with increasing magnitude of applied field up to 5 T. On the other hand, for DCD, after cooling the sample at zero magnetic field to low temperature, 5 T field was applied for 10 s, and then a small field was applied in the negative direction. After 10 s, it was switched off and the remanence was measured. The process was repeated with increasing field up to −5 T. Thermogravimetric analysis was carried out using a thermogravimetric analyzer (TGA, Perkin Elmer STA 6000). Measurements were performed in nitrogen atmosphere keeping the nitrogen flow rate of 20 ml min−1 and in the temperature range 50–750 °C with heating rate 30 °C min−1. The capping characteristics of the nanoparticles were characterized with Nicolet Fourier transforms infrared (FTIR) spectrometer. Zeta potential measurements were carried out with a Micromeritics NanoPlus zeta/nano particle analyzer.
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Fig. 2 TGA weight loss comparison of IONPs@OA, (b) IOagg@CTAB (c) IONPCs@PAA. Inset shows the comparison of first two samples in double y plot. |
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Fig. 3 AFM height images of (a) IONPs@OA, (b) IOagg@CTAB and (c) IONPCs@PAA with their respective height distributions. The inset in figure c shows two identical clusters (scale bar is 120 nm). |
In the second step, these CTAB functionalized nanoparticles are further functionalized with electrolyte PAA to get the nanoparticle clusters. The idea is that, the cationic nature of polar head groups (N+(CH3)3) of CTAB molecules over the nanoparticles might prefer the electrostatic binding with carboxylate group (COO−) of PAA. The measured zeta potential for the so-prepared CTAB functionalized is +46 mV (ESI2†). In contrast, PAA solution (1.2 w/v) has shown negative value of zeta potential in the whole pH range 3.00 to 12.00. Based on the zeta potential results, the neutral pH (pH = 7.00) is identified as the optimized condition for effective PAA functionalization of the CTAB capped nanoparticles. The resultant solution of PAA functionalized nanoparticles has showed the zeta potential value +27 mV. This decrement of the zeta potential could be due to the neutralization of some amount positive charges over the CTAB functionalized nanoparticles by negatively charged carboxylate groups of PAA, which is according to our expected mechanism. After washing for unbound PAA and drying, the PAA functionalized nanoparticles are re-dispersed in water for TEM and AFM characterizations. TEM shows distribution of nearly spherical shaped clusters of size 80 ± 20 nm with significant intercluster separation (shown in Fig. 1c and f). AFM topography image also corroborates the TEM result as shown in the Fig. 3c (shown in inset). Interestingly, the high magnification TEM micrograph shows a measurable interparticle spacing among nanoparticles inside the clusters (shown in Fig. 1i), which is not observed for CTAB functionalized aggregate system (shown in Fig. 1h). Since, through this functionalization process a measurable interparticle spacing has been regained similar to the primitive nanoparticles assembly, so, this functionalization step is termed as the reassembling process. Moreover, the wrapping nature of the long chain polymer has resulted in the nearly spherical shape of the nanoparticle clusters with dense packing morphology. The dominant contribution of PAA in the cluster system is confirmed from the significant amount of weight loss (∼39%) with characteristics two steps in TGA (shown in Fig. 2). Based on the above observations, a model has been proposed for the said reassembling process as shown in the Scheme 1. The model shows that, the negatively charged PAA carboxylate groups are functioning like orderly oriented motifs, where positively charged nanoparticles are bound to attach densely with a definite interparticle spacing due to strong electrostatic interaction.
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F(q,R) = 3[sin(qR) − qR![]() | (3) |
The size distribution ρ(R)dR represents the probability of finding a particle with radius R to R + dR and has been assumed as log normal distribution function.
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The nature of the profile at low q regime is determined by the nature of structure factor. For an attractive potential, the intensity at low q increases because of the formation of aggregated structure of the particles. In low q region of the SAXS profiles, the power law dependence of I(q) on q (i.e., linear relation in double logarithmic scale) and with non-integer exponent of power law indicate fractal like morphologies in all the three systems, irrespective of assembling, aggregation and reassembling. In reality, power law scattering is manifested in a limited q range determined by upper and lower cut-off lengths between which the system behaves as a fractal.24,25
So, scattering curves are modelled using the form factor of a polydisperse spheres (subunit or monomer) and a mass fractal structure factor26
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Fig. 4a shows the transmission corrected scattered intensity profiles along with fitted curves. The fitted parameters such as fractal dimensions (Dm) of the systems and their basic subunit size (μ), polydispersity index (σ) and the approximate interparticle distance (2r) for all three systems are listed in the Table 1. The SAXS curves for the IONPs@OA and IONPCs@PAA are fitted with two contributions; (i) basic nanoparticles with fractal morphology and (ii) a very small length scale (∼2 nm) which could be due to oleic acid capping over the nanoparticles. Fig. 4c shows the size distribution profiles of the subunits which is almost corroborating with the same obtained from TEM (size distribution histogram is shown in Fig. 1). Also, the interparticle spacing measured from the high magnification TEM images are corroborating well with the SAXS results. It is worth mentioning here that the interparticle spacing distribution profiles are approximated from the average interparticle spacing and width of the particle size distribution obtained from SAXS. However, the slight dissimilarities in the trend of size distribution, polydispersity index and mean size can be attributed to the fact that the applied scattering tools are believed to give the overall structural informations about the system, while TEM provides the selective informations based on the region of interest. In this scenario, it will be more reliable for the explanation of magnetic properties on the basis of structural information obtained from scattering data, as the measured magnetic properties are the collective properties of the systems.
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Fig. 4 (a) SAXS and (b) SANS profiles in double logarithmic scale (solid lines represent the fitted curves) (c) is the lognormal size distributions nanoparticles obtained from SAXS data. |
System | Fractal dimension (Dm) | Median size (μ) of the NPs (nm) | Polydispersity index (σ) | Interparticle distance (2ro) (nm) | |||
---|---|---|---|---|---|---|---|
HRTEM | SAXS | HRTEM | SAXS | HRTEM | SAXS | ||
IONPs@OA | 2.43 ± 0.01 | 5.0 | 5.40 ± 0.02 | 0.206 | 0.20 ± 0.01 | 6.3 | 5.8 |
IOagg@CTAB | 2.59 ± 0.01 | 5.3 | 5.68 ± 0.03 | 0.186 | 0.28 ± 0.01 | 4.9 | 4.8 |
IONPCs@PAA | 2.39 ± 0.01 | 5.4 | 5.58 ± 0.02 | 0.169 | 0.26 ± 0.01 | 5.5 | 5.6 |
For knowing the structural informations at larger length scale, SANS was employed for three systems of nanoparticles. Looking into the SANS intensity profiles (shown in Fig. 4b) carefully, it is easily noticeable that SANS profiles of IONPs@OA and IONPCs@PAA are replicating each other in the region q > 0.1 nm−1. In contrast, for the system IOagg@CTAB, it is deviated slightly in the intermediate q range (0.01–0.05 nm−1). These observations can be related to the reassembly mediated regaining of the overall system structure at larger length scale. Table shown in ESI3† gives the obtained length scales from SANS data, which are corroborating with the TEM results. However, interaction at these larger length scales may be ignored here for its correlation with magnetic properties.
Γ = A1g + Eg + 3T2g + T1g + 2A2u + 2Eu + 5T1u + 2T2u | (8) |
Fig. 5a–c show the Raman spectra of these three systems of nanoparticles taken in ambient conditions, where the characteristics bands of both magnetite and maghemite phases are observed. The deconvolution of different bands has been achieved by fitting the spectra with Lorentzian profile. The positions and assignments of all bands are listed in table (ESI6†). Thus, from the Raman and FTIR results a core–shell structure (predominant magnetite phase) of the constituent nanoparticles can be assumed, considering a thin maghemite shell formed due to the symmetric surface oxidation.
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Fig. 5 Raman spectra comparison of (a) IONPs@OA, (b) IOagg@CTAB and (c) IONPCs@PAA, where, Lorentzian deconvolutions show positions of magnetite and maghemite phases. |
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Fig. 6 TGA corrected M–H plots of IONPs@OA, IOagg@CTAB and IONPCs@PAA at 300 K (a) and 5 K (b). Insets show magnifications of M–H plots for Hc and Mr measurements. |
Sample | Total weight lossa (%) | Msb (emu g−1) | Hc (Oe) | (Mr/Ms)c | Dead layer thickness DL (nm) | |||
---|---|---|---|---|---|---|---|---|
300 K | 5 K | 300 K | 5 K | 300 K | 5 K | |||
a Total weight loss determined by TGA.b Corrected saturation magnetization values using TGA weight losses.c Reduced remanence. | ||||||||
IONPs@OA | 14.0 | 73.13 | 83.45 | 20.05 | 188.43 | 0.02 | 0.16 | 0.20 |
IOagg@CTAB | 8.2 | 72.48 | 84.30 | 35.57 | 196.88 | 0.04 | 0.17 | 0.21 |
IONPCs@PAA | 39.0 | 82.36 | 86.24 | 19.41 | 181.20 | 0.03 | 0.17 | 0.11 |
The thickness of magnetic dead layers (DL) has been calculated for the three systems using the eqn (9).38
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Interestingly, for the IONPs@OA and IOagg@CTAB the dead layer thickness are obtained almost same (∼0.2 nm) and for the third system it is obtained significantly less (∼0.1 nm) as shown in the Table 2. It is worth mentioning that like the first two systems TGA corrected Ms value (82.36 emu g−1) of IONPCs@PAA is found not much lesser than the bulk magnetite Ms (92 emu g−1). Ideally, it should not be significantly higher in comparison to the earlier two systems, because same initial iron oxide nanoparticles were used. If it would have been found significantly smaller, the explanation could be given as: two steps functionalization might be responsible for this decrement. In this situation, the only reason that can be responsible for the observed enhancement of Ms is the enhanced interparticle interaction in the cluster system. However, it cannot be ignored that, for the calculation of the dead layer thickness the collective magnetization (Ms) values (after TGA correction) have been used, which are already affected by the interparticle interaction.
The blocking phenomenon of the magnetic moments and its dependency on the interparticle interaction have been studied with ZFC (zero field cooled) and FC (field cooled) magnetization measurements as shown in the Fig. 8a–c. ZFC and FC curves show the distinct features like broad ZFC peaks with maxima Tmax and that the ZFC and FC coincide at high temperatures but split at a temperature Tirr (irreversible temperature) for all three systems. For non-interacting magnetic nanoparticles, Tmax is directly proportional to the average blocking temperature 〈TB〉 through Tmax = β〈TB〉 (where, β is the proportionality constant depending on the type of size distribution in the order of 1.5 to 2.0 (ref. 40)) marks a crossover region where average anisotropy barrier energy and the energy caused by thermal energy (kBT) are comparable. When the anisotropy energy is predominant (for T < Tmax) it is blocked state and for its opposite (T > Tmax) the superparamagnetic state starts. Generally, for a particle of volume V, blocking temperature TB is defined as the temperature at which relaxation time described by the Neel relaxation time , where the anisotropy energy barrier height EB = KV, becomes equal to the measuring time tm. Tirr signifies the highest blocking temperature, i.e. at this temperature the relaxation time of the biggest particle in the assembly is comparable to the measurement time tm.41 Thus, both TB and Tirr are distribution dependent parameters and the difference between Tmax and Tirr is bound to provide a qualitative width of the energy barrier distribution related to the distribution of particle size. In absence of any broad size distribution the only factor that can affect these parameters significantly is the interparticle interactions. In fact, the SAXS results show narrow and similar size distribution profile of nanoparticles in all three systems (Fig. 4c). So, the observed broadening and separation between Tirr and Tmax could be related to modification of energy barrier distribution due to enhanced interparticle interactions in the aggregated and cluster systems. The approximate interparticle distance distributions obtained from SAXS results are corroborating with the trend of ZFC peak broadening for the three systems as shown in the Fig. 8a–d. This implies the significant role of interparticle spacing distribution for the modification of energy barrier distribution. Another noticeable observation is the up-shifting of Tmax for the aggregated and the cluster systems, which again signifies the enhanced interparticle interaction. This type of behaviours such as ZFC broadening and higher temperature shifting of average blocking temperature 〈TB〉 and hence Tmax due to enhanced interparticle interaction with increasing concentration of magnetic nanoparticles were observed in both experimental and simulation studies.42,43 Interestingly, here the up-shift for IOagg@CTAB was observed maximum (∼88 K), while for IONPCs@PAA it was reverted back (∼24 K). This can be correlated to the influence of dipolar interaction due to the change in interparticle spacing for aggregation and cluster systems. When particles are in direct contact (i.e., 2ro ≤ μ) for aggregation system, the Tmax is shifted to higher temperature and again it is reverted back for the cluster system, where a measured interparticle spacing is obtained (i.e., 2ro ≥ μ). For the IONPCs@PAA system, the increased separation among the nanoparticles due to their oriented binding to the polymer carboxylate group should result for intermediate dipolar strength. However, the Henkel plots show its value maximum for this system. The obtained strongest dipolar strength could be resulted from the comparatively more random orientation of magnetization easy axis as explained in earlier discussion. The retaining of similar overall shape of all ZFC curves irrespective of the assembly type nullifies the possibility of any percolation during cluster formation, because above the percolation limit ZFC curves show some distinctive shape due to the formation of coherent ferromagnetic clusters.44 Moreover, the possibility of the formation of any superspin-glass state among the nanoparticles after aggregation and clustering is discarded from the observed monotonic decrement of FC magnetizations with increase of temperature below Tmax. Because, for spin-glasses, FC curves show some plateau like feature below Tmax.45
Another noticeable feature in the ZFC and FC curves is the appearance of a kink in the irreversible region above the Tmax and the position of which is almost same for all three systems. This type of kink may be correlated to the difference in spin states of core and shell in a core–shell composite. Here, the core–shell nanoparticle is of ferrimagnetic magnetite core and ferrimagnetic maghemite shell. Maghemite shell is assumed to be formed due to symmetric surface oxidation of smaller size magnetite nanoparticles. It is known that FC and ZFC magnetization curves of strongly exchange coupled core–shell system do not show separate signature as the spins of their core and shell are strongly correlated, however, core–shell systems with weak spin coupling at the interface can exhibit some features. Thus, the observed kink in M–T is not unusual, as in our core–shell nanoparticles there should not be strong exchange coupling. The weak exchange coupling is confirmed from the zero exchange bias effect in all three systems as shown in the Fig. 9. Similar kink feature in M–T measurement was reported for Fe3O4/γ-Mn3O4 core–shell system also, where the presence of weak exchange coupling was justified with zero exchange bias effect.46
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra12115e |
This journal is © The Royal Society of Chemistry 2015 |