Open Access Article
Sofia S.
Kantorovich
*ab,
Alexey O.
Ivanov
b,
Lorenzo
Rovigatti
a,
Jose M.
Tavares
cd and
Francesco
Sciortino
e
aUniversity of Vienna, Sensengasse 8, 1090, Vienna, Austria. E-mail: sofia.kantorovich@univie.ac.at
bUral Federal University, Lenin Av. 51, 620000, Ekaterinburg, Russia
cCentro de Física Teórica e Computacional da Universidade de Lisboa, Faculdade de Ciências, Campo Grande, 1749-016 Lisboa, Portugal
dInstituto Superior de Engenharia de Lisboa-ISEL, Rua Conselheiro Emídio Navarro 1, 1950-062 Lisboa, Portugal
eUniversity of Rome La Sapienza, Piazzale Aldo Moro 2, I-00185, Roma, Italy
First published on 29th May 2015
With the help of a unique combination of density functional theory and computer simulations, we discover two possible scenarios, depending on concentration, for the hierarchical self-assembly of magnetic nanoparticles on cooling. We show that typically considered low temperature clusters, i.e. defect-free chains and rings, merge into more complex branched structures through only three types of defects: four-way X junctions, three-way Y junctions and two-way Z junctions. Our accurate calculations reveal the predominance of weakly magnetically responsive rings cross-linked by X defects at the lowest temperatures. We thus provide a strategy to fine-tune magnetic and thermodynamic responses of magnetic nanocolloids to be used in medical and microfluidics applications.
Notwithstanding the way the surface of a magnetic nanoparticle is treated (be it special funtionalisation, steric or electrostatic stabilisation) there is an inevitable long-range, anisotropic dipolar interaction between nanoparticles' magnetic moments. This interaction introduces a preferred head-to-tail orientation of dipole moments and, if strong enough to compete with thermal fluctuations, leads to a directional self-assembly of particles in linear flexible chains.26–31 Of course, controlling self-assembly in magnetic nanocolloids is not restricted by magnetic forces only. Van der Waals, electrostatic or chemical interactions of functionalised particle surfaces, solvophilicity/solvophobicity of nanoparticle shells; all these and many others can result in versatile self-assembly scenarios.32–34 It is interesting to observe in this respect the analogies between the anisotropically interacting dipolar nanoparticles and patchy colloids with a reduced valence.35,36 Indeed, restricting the particle–particle relative orientations that result in a bond, leads to self-assembly processes that resemble the one occurring in dipolar nanoparticles, suggesting the possibility to extend the recent investigations of patchy colloids to dipolar fluids. For example, many novel and technologically-relevant phases, such as open lattices,37,38 equilibrium gels39,40 and reentrant gas–liquid phase separations,41,42 can be produced by a fine tuning of the patchy colloids parameters.
Along with an impressively rich spectrum of phases and structures induced by the aforementioned short-ranged or screened long-range interparticle interactions, magnetic nanocolloids, even if only magnetic forces are considered, experience a much more complex self-assembly scenario than that of linear chains: ring structures43,44 and networks of nanoparticles can form in these systems.45,46 Experimentally, these microstructures can be observed in solution using cryogenic electron microscopy47 and atomic force microscopy of assemblies at cross-linkable oil–water interfaces.48 On the numerical side, various simulation studies have been brought forward to describe self-assembly in magnetic nanocolloids by using simple models of dipolar hard- or soft-spheres.45,49,50 Recently, we showed that in highly diluted gas of dipolar hard spheres, chains turn into rings as temperature decreases.51 This structural transition provided a possible solution to a long-lasting debate about the non-monotonic temperature dependence of initial magnetic susceptibility in the suspensions of magnetic nanoparticles.52,53 However, at higher concentrations of magnetic nanoparticles, the assumption of non-interacting chains and rings is not valid any more, and one needs to take into account the next hierarchical step: self-assembly of chains and rings (in the following referred to as primary structures) into more complex branched structures and, eventually, into networks. One of the first attempts to handle branched structures in dipolar hard-sphere systems was introduced in ref. 54, 55, where a transition from pure chains to a system of branching chains (the gas of Y-junctions) was predicted. Even though Y-junctions are clearly one of the main branching mechanisms in dipolar hard spheres, their importance and abundance decrease dramatically with temperature.56
To shed light on the scenario of temperature-induced structural transitions in magnetic nanocolloids at moderate concentrations, we develop a theoretical approach and perform extensive Monte Carlo simulations, the result of which we present herein. Our theoretical approach is based on density-functional theory, where single nanoparticles can self-assemble in “defect-free” chains and rings as well as in “defect structures”, in which primary structures are merged with the help of specific “defect particles”. All these basic units are presented in Fig. 1. After a thorough numerical and visual analysis of simulation results,56 we identify three (and only three) defect particles, labeled in this paper as Y, X and Z defects. Defects Y include Safran's branching.54 The defects of types X and Y (see, Fig. 1) act as cross-linkers between primary structures. Defects of type Z do not link primary structures, rather they can be considered as internal defects of isolated chains and rings.
In this paper we limit our theoretical analysis to the clusters that contain at most one defect. Even though our approach can in principle be extended to multiple defects, it is essential to understand the first steps of the hierarchical self-assembly of dipolar nanoparticles, namely the aggregation of single particles into primary structures and the subsequent merging of the latter into single-defect clusters. Focusing on the different defect types, we observe a clear hierarchy in the structures formed on cooling: first, when the thermal fluctuations are still comparable to the dipolar interactions, only short linear chains form. Then, when the thermal energy becomes smaller, depending on the concentration, two different sequences of structural transitions take place: mostly chains and rings form in the dilute regime, while chains, rings and branches appear in denser systems. Finally, at very high dipolar strength (or, conversely, at very low temperature) most of the Y defects are replaced by more energetically advantageous and infinitesimally magnetoresponsive defect structures made of two rings cross-linked by one X defect. Fig. 2 provides a cartoon of these different aggregation pathways.
![]() | ||
| Fig. 2 Cartoon sketching the temperature-induced structural transitions we observe at intermediate concentrations. | ||
![]() | (1) |
ij| is the inter-particle distance and d is the particle diameter. Vdd is the dipole–dipole interaction, defined as follows:![]() | (2) |
k is the magnetic moment of particle k;
. All the particle magnetic moments have the same magnitude μ.
In the text, kB is the Boltzmann constant, β = 1/T, lengths is measured in units of the particle diameter d and energy in units of μ2/d3. Therefore, temperature is measured in units of kBd3/μ2.
In our model, defect particles do not interact with each other; rather they interact with “regular” particles. The latter can form chains and rings and as such connect defect particles. One can also think of our system as being composed by four different types of particles: one type can only form chains and rings, the other type (Z) can attach to a ring or to a chain, but cannot connect any of the two to some other cluster, whereas the other two (Y and X) connect chains and rings, effectively serving as cross-linkers with a fixed valency.
In Fig. 1 we showed the nine classes of structures that contain up to one defect particle. The free energy (F) per unit volume of this system can be obtained by summing up the free energies of these classes. In the following, we denote their equilibrium concentrations as g(·).
![]() | (3) |
containing the information about not only the size of the cluster but also about its topology, i.e. = (n, k1, k2, mY, mX, mz) |
for primary structures and 1 for the branches). In addition, the partition function of each class also depends on
: Q(
). Finally, v(
) is a characteristic volume, which allows us to express the partition functions in a simple factorised way (see, Table 1). The parameter K(
) is a combinatorial factor, representing the number of entropically distinguishable clusters from the same class, having the same
and with the same partition function Q(
). The free energy can thus be computed by minimising the functional (3) taking into account the mass-balance condition:![]() | (4) |
| Class |
|
v( ) |
N( ) |
Q( ) |
K( ) |
|---|---|---|---|---|---|
| a Here, the factor 2 reflects the possibility of Y defect to have a charge 1 or −1; [·] means the integer part of the argument. | |||||
| I | (n,0,0,0,0,0) | v | n |
|
1 |
| II | (0,k1,0,0,0,0) | v | k 1 |
|
1 |
| III | (n,0,0,1,0,0) |
|
n + 1 |
|
|
| IV | (n,k1,0,1,0,0) |
|
n + k1 + 1 |
|
2(k1 + 1)a |
| V | (n,0,0,0,1,0) |
|
n + 1 |
|
|
| VI | (n,k1,0,0,1,0) |
|
n + k1 + 1 |
|
(n − 1)(k1 + 1) |
| VII | (0,k1,k2,0,1,0) |
|
k 1 + k2 + 1 |
|
k 1 + k2 + 1 |
| VIII | (n,0,0,0,0,1) |
|
n + 1 |
|
n − 1 |
| IX | (0,k1,0,0,0,1) |
|
k 1 + 1 |
|
k 1 + 1 |
This condition constraints the total number of particles in a unit volume (ϕ/v, ϕ being regular particle volume fraction, v standing for particle volume). Note that the total number of regular particles in a cluster of class i is given by N(i) = n + k1 + k2 + mYsY + mXsX + mZsZ, where a defect particle depending on its type contains sY, sX or sZ regular particles. These parameters are used to simplify the description of the cluster formation. As shown in ref. 56, the number of particles in the defects can vary from one to four, however, the actual internal structure is irrelevant. Thus, we can unify the treatment and limit the number of defect particle types.
Minimisation using Lagrange multipliers method leads to a solution with a “traditional” functional form:
![]() | (5) |
The main complexity of the problem is condensed in the analytical calculation of Q(
), due to the long-range magnetic dipole–dipole interactions between nanoparticle magnetic moments. Here, we put forward an approach that makes use of the following assumptions:
• Each bond is described by an effective free energy: εL for a linear chain segment, εR for a ring segment; εYL(YR) for a bond between the member of a chain (ring) segment and a defect particle Y; εXL(XR) for a bond between the member of a chain (ring) segment and a defect particle X; εZL(ZR) for a bond between the member of a chain (ring) segment and a defect particle Z; εl, l = X, Y, Z is the free energy loss of forming a defect l compared to a bond between regular particles.
• The partition function Q(
) can be factorised as a product of the aforementioned effective bond free energies and thus be computed as a function of the number of monomers and temperature, for details see ref. 51;
• The factorisation of Q(
) has a peculiarity, namely, even though it is presented as a product of effective free energies, these free energies actually do depend on the lengths of corresponding segments; in this way we can consider the interactions beyond the limit of the nearest neighbours;
• Entropic contributions are calculated with respect to the entropy of a chain, which is why the factor 1/k3v+1 is included in partition functions of ring containing clusters to capture the difference in entropy between chains and rings arising from the k ways of opening a ring to form a chain, where v = 0.588 is the self-avoiding random walk exponent; the difference number of self-avoiding paths of chains and rings is proportional to k3v.57
Building upon past results,51 we know that the bonding free energies associated to rings and chains are respectively given by
![]() | (6) |
![]() | (7) |
stands for the residual of division, and [·] has the meaning of the integer part of the expression in the brackets. The low-T dimer partition function q (note that C(1) = 0, C(2) = 1), derived first by de Gennes and Pincus,58 is![]() | (8) |
) = vY; analogously, for i = V, VI, VII the normalising volume is v(
) = vX and for i = VIII, IX we set v(
) = vZ. In addition, we introduce three parameters:| y = εYv/ṽY; x = εXv/ṽX; z = εZv/ṽZ. |
In the general case x, y, z are slowly changing functions of T*, and from previous investigations56 we know that x < y < z ≪ 1 for any temperature. Here, however, we neglect their temperature dependence and fit their values by matching the internal energy in simulations and theory, obtaining x = 0.003, y = 0.005 and z = 0.006. We performed an extensive analysis changing the values of these parameters by up to 60 per cent and discovered, that the microscopic characteristics as well as the thermodynamic quantities are not sensitive to such variations of x, y and z.
For the sake of simplicity, we fix sX = sZ = sY = 1. To justify the latter, we have carefully checked simulation results, finding that the amount of particles in defects is very small in comparison to the number of particles in ring and chain segments. We provide the expression for all the terms in the free energy functional (3) under these assumptions in Table 1.
Using this table, one can minimise the free energy of the system and obtain the Lagrange multiplier p as a function of temperature and nanoparticle concentration.
It is worth noting that, using the approach described above, we can introduce more complicated structures, that can be hierarchically obtained by combining the basic nine elements, as shown in Fig. 3. One can keep adding up defects following this approach to eventually build a percolating network of branched structures. The table can be relatively easily extended for this case, however, the calculation of the K values becomes more cumbersome. In any case, before dealing with the network itself it is crucially important to understand how the initial stage of branching occurs, which structures are more probable at low temperatures and what are the main tendencies in branching for different particle concentrations. In other words, we aim at understanding the second step (the first being the formation of primary structures, namely chains and rings) of the hierarchical self-assembly, thus elucidating the thermodynamics of the aggregation of primarily formed chains and rings into small branched clusters.
• a structure containing two single-bonded particles connected by particles having two neighbours is labelled as a chain;
• a ring is a cluster containing only particles having two neighbours;
• any other kind of aggregate is a branched cluster.
At high temperature, the overwhelming majority of particles is aggregated in chains, regardless of the concentration. As soon as the temperature decreases and the concentration grows, the first defect structures appear: chains begin to develop internal defects. As the system is further cooled down, Y structures first start to emerge and then slowly disappear in favour of X-structures. At the same time, rings with internal defects and tennis-racket-like structures (IV) are clearly overtaken by rings with two chain tails. If we cool the system further down, basically all defect-cluster fractions exhibit a clear maximum and start rapidly decreasing. For low concentrations, the majority of magnetic nanoparticles is aggregated in rings. For higher concentrations, though, the fraction of particles in rings has a maximum, signalling a transition towards the formation of higher-order defect clusters such as those in the VII class, i.e. double rings. These double rings thus form at temperatures lower than single rings, but at relatively high nanoparticle concentration they clearly become the dominant class. Another interesting aspect shown by Fig. 5 is that the fractions of chain-only defects decrease faster on cooling than those with at least one ring segment. This is a clear reminiscence of the low-concentration structural transitions on cooling, where the complete redistribution from chains into rings is observed in the same temperature range.51
Several conclusions can be drawn when looking at Fig. 6. At any concentration the internal energy has an inflection point, which generates a maximum in the T dependence of the constant volume specific heat CV.60 The position of the maximum in CV, as shown in the inset, shifts towards low temperatures as the concentration decreases. Independently from concentration, there is only one specific heat maximum, whose position is in close correlation with the temperature of the first structural transition, be that chain-ring or chain-defect transition (compare to Fig. 4).
Taking advantage of the theoretical approach, one can compute the free energy and estimate its change across the various structural transitions. First we estimate the thermodynamic driving force which leads to the ring formation by calculating the free energy difference between a system composed by only chains and a system with chains and rings. At low concentrations, the possibility of forming rings drives to a dramatic decrease of the free energy and the contribution of rings to the system free energy becomes dominant at low temperature. These results are plotted with dashed lines in Fig. 7. For denser systems, though, the free energy gain due to ring formation is marginal. As a second step, we consider the free energy difference between a system composed only by chains and rings and a system composed of chains, rings and defects. The resulting driving force for branching is plotted with solid lines in the same figure (Fig. 7). The results show that, indeed, there is a significant driving force for branching, but only at intermediate and high densities in the studied range of temperature. This result confirms that the loss in the translational entropy of primary clusters on branching becomes less-and-less relevant with increasing density in comparison to the energetic contribution of the additional interaction.
![]() | ||
| Fig. 7 Free energy difference in units of T* calculated per particle. Dashed lines describe the free energy gain due to the ring formation in the model system with chains and rings only.51 The free energy gain obtained through the formation of branched structures (within the framework of the model proposed here) is plotted with solid lines. The legend for different nanoparticle concentrations is provided. | ||
Footnote |
| † We consider single particles to be chains of unit length. |
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