Pan Wangab,
Yunyun Maab,
Zhibin Liuab,
Youguo Yanab,
Xiaoli Sun*a and
Jun Zhang*ab
aCollege of Science, China University of Petroleum, 266580 Qingdao, Shandong, People's Republic of China. E-mail: sunxiaoli@upc.edu.cn; zhangjun.upc@gmail.com
bKey Laboratory of New Energy Physics & Materials Science in Universities of Shandong, China University of Petroleum, 266580 Qingdao, Shandong, People's Republic of China
First published on 14th January 2016
The formation of vesicles has been a hot topic because of their many potential applications, ranging from cell membranes to drug delivery. However, determining essential information for further development, such as molecular arrangement and interaction, is still experimentally challenging. In this study, coarse-grained molecular dynamics simulation (CGMD) was carried out to study the formation of vesicles in a cationic cetyltrimethylammonium chloride (CTAC) and anionic sodium dodecyl sulfate (SDS) system. In the mixtures, a series of morphologies was obtained as the mixed ratio changed. When the ratio of SDS was equal to that of CTAC, a vesicle was formed by disk-like bilayer curling and the entropy was the driving force. We hold that the bending energy of the bilayer is the resisting force and the electrostatic forces play a significant role in aggregate shape. Therefore, the surfactant distribution in different parts of disk-like bilayer aggregates were studied in the vesicle formation process. These studies put forward a new understanding of vesicle formation and brought to light the microscopic details of the bilayer–vesicle transition of catanionic mixtures.
In earlier studies, vesicles were produced by phospholipid molecules constituted by double-chained amphiphiles, and the formation of vesicles required mechanical methods, such as sonication or extrusion.12,13 However, these vesicles had a fatal drawback; they were unstable, which inherently restricted their potential applications. In 1989, Kaler et al.14 reported that stable vesicles could be found in aqueous mixtures of cationic–anionic (catanionic) surfactants that mimic the structure of phospholipids through the electrostatic interaction of their polar head groups. Unlike the phospholipids, catanionic surfactant vesicles can be formed spontaneously and exhibit high stability. Since then, more and more researchers have paid close attention to catanionic surfactant mixture systems,15–17 and a mountain of work about spontaneous vesicle formation in these mixture systems has been reported.9,18–20
Most of the investigations on catanionic surfactant mixture systems have been by experiment. Yatcilla et al.15 reported the phase behavior and aggregate morphologies of the cationic cetyltrimethylammonium bromide (CTAB) and anionic sodium octyl sulfate (SOS) mixture, and they found that the composition and chain length asymmetry had a great effect on the stability of the vesicles. After that, increasing interest was focused on the composition of the mixtures21–24 and the chain length asymmetry.25–29 Recently, some researchers began to investigate responsive vesicles via changing the external environments in the original basis of surfactant mixture systems, such as temperature30 and pH,31 which have more value in practical applications. In any case, self-assembly is one of the most fundamental scientific problems. In contrast to the continuous finds in environmental responsive vesicles, the essential answer on how the composition of the mixtures triggers distinct assemblies is still not clear. Atomic-level structural details of self-assembly processes and subtle molecular interactions are crucial to giving insight into self-assembly phenomena, but unfortunately, the information is challenging or impossible to probe experimentally.
Molecular dynamic (MD) simulation, which can provide microscopic details, has been applied in extensive fields.32–35 Mesoscopic molecular dynamics technologies, including coarse-grained molecular dynamics (CGMD) and dissipative particle dynamics (DPD) and so on, improve performance when handling larger lengths and timescales, and are powerfully exploited to investigate surfactant self-assembly in solutions. Wu et al.7 and Shillcock et al.8 applied CGMD and DPD, respectively, to studying the spontaneous vesicle self-assembly, and they both revealed the process of vesicle formation. Li et al.9 showed the effects of salt, temperature, and selective solvents on micelle–vesicle transition by DPD, and revealed the transition mechanism induced by various conditions from the microscopic point of view. de Vries et al.36 adopted CGMD models to analyze the properties of intermediate structures in detail and reflect the features of the vesicle formation processes. Markvoort et al.37 studied the bilayer–vesicle transition by CGMD, and revealed that the transition is entropy driven, after going deep into studying the potential energy. Although many simulation studies on vesicle formation or transition have been made, exploration of the mechanism of vesicle self-assembly by catanionic surfactant mixtures is still sparse, and further research on this topic is urgently needed.
In our work, we employed CGMD simulation to investigate vesicle formation in catanionic mixtures composed of sodiumdodecyl sulfate (SDS) and cetyltrimethylammoniumchloride (CTAC). Various morphologies of surfactant aggregates were obtained at different CTAC/SDS ratios and the vesicles were formed when the mixed ratio was 1:
1. Furthermore, the formation process and mechanism were studied from the micro-perspective. These studies put forward a new understanding of vesicle formation, and brought to light the microscopic details of the bilayer–vesicle transition of catanionic mixtures.
Our simulation work was performed by the Gromacs 4.5.5 (ref. 41) package. The simulations of the surfactant mixture in aqueous solution were accomplished in a cubic box with periodic boundary conditions along three directions. The side length of the box was 200 Å. The canonical ensemble NPT was performed at 298 K and 1 atm for each system, the integration step was set as 20 fs. The temperature was controlled by the Berendsen thermostat,42 and the pressure coupling was set by the Berendsen barostat.42 The cut-off for nonbonded interactions was set at 12 Å with the standard shift functions of Gromacs, where the van der Waals interaction was shifted from 0.9 to 1.2 nm, and the electrostatic interaction was shifted from 0 to 1.2 nm. All simulations were carried out for 1 μs to reach the equilibrium state.
Fig. 2 shows the snapshots of equilibrium morphologies of surfactant aggregates at different CTAC/SDS ratios. If there was only CTAC in the solution, as in system I shown in Fig. 2(a), spherical micelles were formed. Once 1/6 CTAC was replaced by SDS in this system, in other words, when CTAC/SDS was 5:
1, we got a spherical micelle and a rod-like micelle, as shown in Fig. 2(b). If there was more SDS in the system, a huge disc-like micelle was formed as shown in Fig. 2(c), when the ratio of CTAC/SDS was 3
:
1 in system III. Just like system III, a disc-like micelle was also obtained at the CTAC/SDS ratio 2
:
1 in system IV, shown in Fig. 2(d). Comparing the cross-section of the rod-like micelle with that of the disc-like micelle, the disc-like micelle was well-ordered and dense. When the ratio of CTAC/SDS was 1
:
1, a single vesicle was formed, as shown in system V. With the further increase of SDS content, we also got disc-like micelles at the CTAC/SDS ratio 1
:
2 and 1
:
3 in systems VI and VII, respectively, which was similar to systems III and IV. When the amount of SDS continued to increase, we got a “sandwich” micelle, which was stacked up by two disc-like micelles. From the cross-section of the sandwich micelle, a well-ordered bilayer arranged by SDS and CTAC formed between two disc-like micelles, which was considered to be due to the electrical charge effect. In the SDS system, we got the mixture of rod-like micelles and spherical micelles as shown in Fig. 2(g). Thus, it is concluded that a mixed ratio is a key factor in the shapes of aggregates in the mixed surfactant system. With the increase of the CTAC/SDS ratio from 6
:
0, 5
:
1, 3
:
1, 2
:
1, 1
:
1, 1
:
3, 1
:
2, 1
:
5 to 0
:
6, a number of aggregates with different morphologies can be formed, such as rod-like, disc-like, vesicle, and stacking disc-like micelles, and all these aggregates have been observed by experiment.15,43,44 It is worth mentioning that vesicles were formed, when the ratio of CTAC/SDS was 1
:
1.
In order to understand the processes of mixed surfactant self-assembly in aqueous solution, the evolution of the number of clusters (N) and max. cluster size (Nm) at different ratios were calculated as shown in Fig. 3. N and Nm were collected during 1 μs simulation and the flat line at each end of these curves demonstrated that our simulation systems were close to equilibrium. As shown in Fig. 3(a), N decreases sharply to a relatively stable value in the simulation process, which shows that clusters gather rapidly at first. In addition, Nm also shows a sudden increase in the initial stage. The evolution of Nm can be further divided into three stages, depending on the increase rate and number. In this first stage, Nm almost increases sharply, since randomly scattered surfactant molecules quickly gather into small clusters due to the hydrophobic effect of surfactant tails, and it only takes about 50 ns. In the second stage, Nm increases, which is owing to the fusion of small micelles. This stage lasts several hundred nanoseconds until the curve becomes flat, which is much longer than the first stage because the fusion of micelles needs a longer time than molecule aggregation. The final stage is the flat part of the curve, in which the system achieved “quasi-equilibrium”. Therefore, from this microscopic point of view, we think that the self-assembly of surfactants starts with the aggregation of molecules, followed by the formation and fusion of micelles.
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Fig. 3 Evolution of the number of clusters (a) and max cluster size (b) at different ratios. I to IX are the same as Fig. 2. |
Compared with the equilibrium morphologies of surfactant aggregates at different CTAC/SDS ratios, not only the shapes of aggregates vary, but the numbers of aggregates are also different. Table 1 shows the number of clusters (N) and max cluster size (Nm) at different surfactant ratios. N and Nm changed significantly in different mixed surfactant systems. In system I, eight spherical aggregates were formed in cationic surfactant CTAC aqueous solution. When a little SDS was added to the cationic surfactant aqueous solution as shown in system II, N was reduced to 2, and Nm sharply increased to 408, which means that the aggregates that do form grow relatively large. As the ratio of CTAC/SDS reduced to 3:
1, there was no change in N, while Nm increased to 528. When the ratio of CTAC/SDS was 2
:
1 or 1
:
2, all surfactants aggregated into disc-like micelles. In system V, where the number of cationic surfactants was equal to that of anionic surfactants, we got the unique morphology-vesicle, and all surfactants were self-assembled into a single vesicle. If the SDS content was increased continually, N increased to 2 and Nm decreased to 521 in system VII. From system VI to IX, with increasing SDS quantity, Nm became fewer and N was more. When there was only anionic surfactant SDS in system IX, six micelles were obtained. Thus, it was concluded that the ratio of cationic surfactants and anionic surfactants is a significant factor impacting surfactant self-assembly. We speculate that the electrostatic interaction between anionic surfactants and cationic surfactants leads to the behaviour of micellar aggregation. In the following, the process of the vesicle formation will be discussed in detail and the formation mechanism of the vesicles is analyzed from the view of charge distribution.
System | I | II | III | IV | V | VI | VII | VIII | IX |
CTAC/SDS | 6![]() ![]() |
5![]() ![]() |
3![]() ![]() |
2![]() ![]() |
1![]() ![]() |
1![]() ![]() |
1![]() ![]() |
1![]() ![]() |
0![]() ![]() |
Number of clusters (N) | 8 | 2 | 2 | 1 | 1 | 1 | 2 | 2 | 6 |
Max cluster size (Nm) | 106 | 408 | 528 | 600 | 600 | 600 | 521 | 343 | 216 |
Fig. 4 shows snapshots of the morphologies at different times. The process of vesicle formation shows three stages: the first is the nucleating stage, in which surfactant molecules aggregate to form small clusters and this stage only lasts a short time, about 20 ns. In the second stage, small micelles fuse into bilayer disk-like aggregates, and this lasts for a longer time than the first stage. Then, bilayer disk-like aggregates curl up into closed vesicles in the final stage. The duration of curling is about 30 ns, as shown in Fig. 4, which means that once the disk-like micelles formed, the vesicles soon turn out via curling. After that, the vesicles are kept at the steady state. Throughout the whole process, the fusion of micelles in the second stage takes the most time.
The self-assembly process for surfactants is always accompanied a change in energy. In order to understand this procedure, the energy of these systems was calculated. As shown in Fig. 5, the black line presents the system energy with time, which shows a clear downward trend, and the red line is the evolution of max cluster size (Nm) during simulation. In the fusion stage, the change in system energy also is shown as a “ladder”, which is consistent with the change in Nm. This means that the occurrence of fusion always goes with the decrease in energy. In the curling stage, the energy maintains a stable development until the end. We therefore think that the bilayer–vesicle transition is driven by entropy, and further analysis will be presented in the following.
To get further information about vesicles, the cross-sections of vesicles and the radial distribution functions (RDFs) of each group of surfactant and water as a function of distance from the vesicle's mass centre are shown in Fig. 6. Intuitively, the head groups at the inner surface are more compact than those at the outer surface (Fig. 6(a)). More quantitatively, the numbers of cationic and anionic surfactants are 62 and 66 in the inner, and 238 and 234 in the outer leaflets of the vesicle, respectively. The peaks of the head groups are found to be 1.7 nm and 4.1 nm for the inner and outer leaflets of the vesicle (Fig. 6(b)), respectively. Thus, the surface areas per head group are 0.28 nm2 and 0.45 nm2, respectively. The head group of the inner and outer leaflets have a different compactness due to the formation process of vesicles via the curling of bilayer disk-like micelles.
Since the driving force for the bilayer–vesicle transition is entropy, it was confusing that the bilayer disk-like aggregates in the systems III, V, VI, and VII did not curl into vesicles, even when the simulation time was extended. We therefore set out to determine what the resistance force was for the transition. We determined that the bending energy of the bilayer47 is the resistance force and the electrostatic repulsion interactions play a very important role. In order to make this clear and easy to be analyzed, we designed a pre-assembled bilayer disk-like aggregate, with a diameter of approximately 120 Å, as shown in Fig. 8; the length of the sides of the box was 200 Å. There were 59400 W beads and 6600 antifreeze particles (BW beads, colored in green). The total number of surfactants was 600. The pre-assembled aggregates contained three different proportions of CTAC and SDS, 3
:
1, 1
:
1, 1
:
3. In these initial configurations of bilayer disk-like aggregates, CTAC and SDS were arranged randomly. The simulation parameters were the same as those in the first section, except that the total simulation time was 500 ns.
Fig. 9 shows the equilibrium morphology of the pre-assembled disk-like bilayer membrane at three different ratios. They are disk-like bilayer, vesicle, disk-like bilayer, as the ratio changes from 3:
1, 1
:
1 to 1
:
3, respectively. As we have seen, the pre-assembled equilibrium morphologies consisted of self-assembled morphologies, which demonstrated the rationality of the pre-assembly method. Among these equilibrium morphologies, vesicles were only formed at the ratio of 1
:
1. The disk-like bilayer membranes were divided into several parts to study the effect of different molar fractions of surfactants on vesicle formation. A segmentation map of disk-like bilayer membranes is shown in Fig. 10. A disk-like bilayer with radius of 76 Å was divided into a cylinder with 19 equal intervals of concentric cylinders. Fig. 10(a) shows the top view, and Fig. 10(b) shows the side view of the segmentation map. The red cross is the center of the disk-like bilayer, the red line shows the central axis, and the yellow lines express the cylinder segmentation. In order to reveal the difference among these three disk-like bilayers, we compared the mole fractions of the two surfactants at different concentric cylinders.
![]() | ||
Fig. 10 Segmentation map of the disk-like bilayer membrane. (a) The top view of the segmentation map. (b) The side view of the segmentation map. |
We defined a parameter R to represent the mole fraction of SDS at each part. The relationship is as follows,
![]() | (1) |
Fig. 11(a) shows the evolution of the mole fraction at the ratio of 3:
1. In the initial situation, the distribution of SDS in each section is homogeneous and the mole fraction remained at around 0.25 as shown in Fig. 11(a) by the black line. As time went on, the mole fraction of SDS in the center region rose to 0.5, while R near the edge of the disk-like bilayer remained at around 0.25. This was because the positively charged SDS and negatively charged CTAC attracted each other to form ion pairs, and they tended to gather in the center to lower the energy of the system. This rearrangement maintained the stability of the structure, while the excess CTAC was located in the edge region and did not form ion pairs. Thus, outer cylinders were positively charged to prevent the curling of the bilayer into a vesicle, so the electrostatic force played a significant role in the surfactant distribution and aggregate shape. In Fig. 11(b), the mole fraction of SDS was about 0.5 at the ratio of 1
:
1, and it was maintained at 0.5 during the whole simulation. This means that the disk-like bilayer membrane was in a neutral morphology before the vesicle was formed. The same quantity of SDS and CTAC made all surfactants form ion pairs. In Fig. 11(c), the evolution was similar to Fig. 11(a). Ion pairs were formed near the center, and excess SDS gathered in the edge region. The non-uniform distribution of excess surfactants was attributed to the initial maldistribution of headgroups (Fig. 12), which are denser in the central zones of the bilayer than in the edge regions. In this situation, the excess surfactants were much more vulnerable to gathering in the edge regions, due to the electrostatic repulsion effect, so the disk-like bilayer membrane was negatively charged. Eventually, we got three different disk-like bilayer membranes. While only the uncharged disk-like bilayer at the ratio of 1
:
1 could form vesicles, it verified that preventing electrostatic repulsion played an important role in the process of preventing the disk-like bilayer from curling into a vesicle.
![]() | ||
Fig. 12 The initial distribution of head groups. The head groups are displayed by the quicksurf method. |
The disc-like bilayers formed in the systems III, IV, VI and VII did not curl into vesicles and electrostatic repulsion interactions played a key role. If the system is given enough surfactants, the bending energy and electrostatic repulsion interactions would be reduced and the disk-like bilayer could potentially be curled into vesicles. To illustrate this, a pre-assembled bilayer disk-like aggregate with more surfactants (N = 1200) was constructed and the proportions of CTAC and SDS were 3:
1, 2
:
1, 1
:
2; and 1
:
3. The larger bilayers were converted into vesicles when the proportions were 2
:
1 and 1
:
2, but the proportions of 1
:
3 or 3
:
1 were not (data not shown). Hence, we obtained the following main results: firstly, in the process of bilayer–vesicle transition, the increase of entropy, which originated from the excluded volume overlapping itself, is the driving force. Secondly, the bending energy of the bilayer, in which preventing the electrostatic repulsion plays an important role, is the resistance force.
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