Andrew Joseph
Christofferson‡
a,
George
Yiapanis§‡
a,
Jing Ming
Ren
b,
Greg Guanghua
Qiao
b,
Kotaro
Satoh
c,
Masami
Kamigaito
c and
Irene
Yarovsky
*a
aSchool of Aerospace, Mechanical and Manufacturing Engineering, RMIT University, GPO Box 2476, VIC 3001, Australia. E-mail: irene.yarovsky@rmit.edu.au
bDepartment of Chemical and Biomolecular Engineering, University of Melbourne, Melbourne, VIC 3010, Australia
cDepartment of Applied Chemistry, Nagoya University, Chikusa-ku, Nagoya 464-8603, Japan
First published on 1st December 2014
In this study, by using X-ray powder diffraction profiles as blueprints, we successfully mapped the most probable molecular-level structural arrangement of the PMMA super-helix stereocomplexes through molecular dynamic simulations. Molecular-level resolution of the PMMA triple-helix supramolecule was not previously achievable by experimental methods. After constructing molecular models of stereo-regular complexes composed of linear it- and st-PMMAs, our all-atom molecular dynamics simulations identified the stereocomplex structure that best reproduces experimental diffraction profiles and thermodynamic properties as a double helix of isotactic (it-)PMMA with a helical pitch of 1.8 nm and 9 units per turn surrounded by a single helix of syndiotactic (st-)PMMA with an average helical pitch of 0.9 nm and 20 units per turn. The it-/st- complexing stoichiometry in the PMMA triple-helix is therefore 9:20. This presents the first all-atom model of the it-/st-PMMA triple-helix stereocomplex that accurately fits experimental X-ray diffraction profiles. In addition, the simulation results revealed the outer st-PMMA helix of the PMMA stereocomplex has a fiber diameter of at least 1.85 nm and adopts a non-ideal helical geometry. Furthermore, through dynamic simulations, surprising new sights into the effect of the structural configuration of the PMMA stereocomplex (i.e., helical pitch and direction, and tilt angle) on the physical properties of their crystal structures were obtained. Those crystal properties include X-ray diffraction profile, packing density, chain–chain spacing, chain width and cohesive energy density.
One of the most intriguing synthetic super-helix is perhaps the poly(methyl methacrylate) (PMMA) stereocomplex, as multiple-strand synthetic helices are very rare. The unique supramolecular architecture provides the PMMA stereocomplex with useful properties for a number of potential applications in life science and nanotechnology. For instance, PMMA stereocomplex formation has been exploited as an assembly mode for the fabrication of ultrathin films,4,5 nanoparticles,6,7 network and gel formations,8 as well as fibers9 and dialysis membranes.10 Moreover, other interesting and remarkable characteristics of PMMA stereocomplexes that have been explored, include stereospecific polymerization-templating,5 molecular recognition capability11,12 and helix-sense stereo-complexation.6
The structures of PMMA stereocomplexes have been studied since the 1950s, but to date, the exact structural arrangements of PMMA stereocomplexes at the molecular level still remain elusive.
In complexing solvents such as acetonitrile or acetone, isotactic PMMA (it-PMMA) can self-aggregate to form a double-stranded helix with definitive crystalline characteristics.13,14 Its aggregation depends strongly on the degree of stereoregularity, the nature of the solvent and on temperature.15 Many attempts were made to elucidate the crystal structure using X-ray diffraction analysis, but due to the amorphous nature of the supramolecular assembly, conflicting results were obtained. For many years, the consensus based on X-ray results16–18 and early molecular models was that the it-PMMA structure consisted of two 101 helices (10 repeating MMA units per turn) of it-PMMA chains intertwined to form a double helix in the crystal with a helical pitch of 2.1 nm.
In addition to the double helix, it-PMMA can be combined with syndiotactic PMMA (st-PMMA) to form a stereocomplex.13,19,20 With an it:st complexing ratio (monomer ratio in the stereoregular region of the polymer) of 1:2,21 Schomaker and Challa proposed a model based on X-ray fiber diffraction of a 91 double-stranded helix of it-PMMA and st-PMMA in a 1:2 monomer ratio.22 While X-ray fiber diffraction gave a fiber identity period of 1.84 nm,22,23 consistent with a 91 helix, due to the poor quality of the diffraction patterns resulting from an inherently disordered structure a quantitative analysis was not possible and the proposed model was recommended as a starting point for further investigations. Interestingly, the authors found that stereocomplexes of atactic and isotactic PMMA gave fiber X-ray diffraction patterns with the main characteristics of the it-/st-PMMA stereocomplex diffraction pattern still present, suggesting that the degree of tacticity of the st-PMMA is not critical to stereocomplexation.22
More recently, the introduction of the Langmuir–Blodgett technique coupled with atomic force microscopy (AFM) analysis has enabled the direct observation of the it-/st-PMMA stereocomplex.24,25 Based on their observations, Yashima and colleagues proposed a model of a 91 it-PMMA double-stranded helix with a helical pitch of 1.84 nm surrounded by a single helix of 181 st-PMMA with a helical pitch of 0.92 nm. These early works demonstrated that the exact arrangement of the supramolecular complex proved difficult to resolve based upon experimental methods.
In this work, we discovered that by using the X-ray diffraction profiles of the PMMA stereocomplex crystals as blueprints, the most probable molecular-level arrangements of the PMMA super-helix stereocomplexes can be successfully mapped through molecular dynamic (MD) simulations. Due to stereo-association being dominated by non-covalent interactions, MD simulation provides a unique method for resolving structural features of it-/st-PMMA crystals and this becomes the only way to obtain an all-atom structural model compatible with X-ray diffraction results. More specifically, we constructed models of it-PMMA and st-PMMA crystals comprising double-stranded helices of it-PMMA and single-stranded st-PMMA with varying helical pitch and direction in excellent agreement with experimentally obtained diffraction data. Our results show that an average of 20 PMMA repeating units are required to form one helix turn for the st-PMMA in the triple-helix stereocomplex structure and this is distinguished from any previously reported results. Through MD simulation, other than mapping the structural features of the PMMA stereocomplexes, we obtained new insights into the effect of helical pitch and helix direction on the molecular structure and stability of it- and st-PMMA crystals by analyzing the following properties: X-ray diffraction profiles, density, chain–chain spacing, chain width, and cohesive energy density.
The procedure for synthesis of st-PMMA was adopted from previously published literature with modifications,28–30 and the full details may be found elsewhere.27 In brief, copper(I) bromide (CuBr, 36.0 mg, 0.25 mmol) and copper(II) bromide (CuBr2, 5.6 mg, 0.025 mmol) were added to a dry round-bottom flask equipped with a 3-way stopcock in a glovebox, followed by addition (under dry N2) of 1,1,1,3,3,3-hexafluoro-2-phenyl-2-propanol (PhC(CF3)2OH, 8.4 mL), MMA (2.7 mL, 25.2 mmol), 2,2′-bipyridyl (bpy, 495 mM in toluene, 1.0 mL) and prop-2-ynyl 2-bromo-2-methylpropanoate (PgBr, 503 mM in toluene, 0.50 mL). The reaction was conducted at 0 °C with samples taken periodically under N2. The polymerization was terminated after 11 h by cooling the reaction to −78 °C. A sample was extracted for 1H NMR spectroscopic analysis, and the remaining product was diluted with ethyl acetate (EtOAc, 200 mL), washed with 1 M HCl (100 mL × 2), then distilled water (150 mL × 2). The extracted product was collected, concentrated and then precipitated in hexane, followed by drying in vacuo to afford the st-PMMA (st-L4k) as a white solid, 0.88 g (87.8%); 1H NMR: MMA conversion = 33% (theoretical Mn = 3.5 kDa); GPC: Mn = 4.2 kDa, Mw/Mn = 1.34; 13C NMR: mm/mr/rr (%) = 2/26/72; DSC: Tg = 98.6 °C and Tm = 99.5 °C.
The general procedure employed for the synthesis of the PMMA stereocomplex was as follows:31 the st-PMMA (10 mg) and it-PMMA (10 mg) precursors were separately dissolved in an acetonitrile/water mixture (MeCN:H2O = 9:1) at concentrations of 2 mg mL−1 and combined to an it:st molar ratio of 1:2. The solutions were left to stand at room temperature for 24 h. After removing the solvent in vacuo, the st-L4k/it-L10k stereocomplexes were dried under reduced vacuum (0.05 mmHg) for 24 h before DSC and XRD analysis; Tm = 126.4 °C.32
Single-stranded helices of 181 st-PMMA with a helical pitch of 0.92 nm were constructed based on reported bond lengths, bond angles and internal rotation angles from the proposed Yashima model for the triple helix stereocomplex.24 Similar to the it-PMMA, the fiber axes of the chains were oriented in the z-direction and each st-PMMA fragment was connected to its periodic image in the z-direction, mimicking an infinite PMMA crystal (Fig. 2). For this model (91-it-/181-st-PMMA) only the Right Down packing motif was employed. In order to more closely reproduce the experimental stereocomplex synthesized in this work, additional st-PMMA fragments of 40 PMMA units were constructed, labeled 40mer-st, corresponding to the l-st-PMMA (st-L4k) fragments. Each cell contained two it-PMMA double helices surrounded by a single st-PMMA helix of the same sense and direction in a hexagonal packing arrangement with initial cell dimensions of 3.98 and 2.36 nm in the x- and y-directions. The length along the z-direction depended on the helical pitch of the it-PMMA double helix; 2.10 and 1.84 nm for the 101-it/40mer-st and 91-it/40mer-st models respectively. For the 101-it/40mer-st model only the Rright Ddown packing motif was employed, while for the 91-it/40mer-st model all four packing motifs (Fig. 1b) were employed.
Fig. 2 a) Initial model crystal structure of the 91-it-/181-st-PMMA stereocomplex, (b) schematic representations of the three triple helix stereocomplex systems. |
For all models, we initially performed energy minimization with unit cell dimensions fixed and a force convergence criterion of 0.01 kcal mol−1 Å−1. Subsequently, we undertook molecular dynamics (MD) simulations in the NPT ensemble (constant number of particles, pressure and temperature) for a total of 40 ns. For the it-/st-PMMA stereocomplex simulations, atom coordinates of the it-PMMA were fixed for the first 20 ns, followed by 20 ns of simulation with all coordinates varying. The temperature and pressure were maintained at 298 K and 1 atm respectively using the Nose-Hoover thermostat and barostat.42,43 A time step of 1 fs was implemented, with atomic coordinates and thermodynamic quantities recorded every 10000 steps. The models were considered equilibrated when the energy and density attained a steady value (standard deviation within 1%). The geometry of the equilibrated models was optimized by energy minimization with a force convergence criterion of 0.001 kcal mol−1 Å−1 and the optimized structures were used for analysis of density, structural parameters, cohesive energy density and calculated X-ray diffraction profiles.
Fig. 3 Wide angle X-ray scattering profiles obtained from powder diffraction experiments and molecular dynamics simulations for the it-PMMA double helix in the Right Down packing motif. |
The experimental peak at 1.04 nm, which arises from the chain–chain spacing in the x- and xy-directions (see Fig. 4), is reproduced by both the 91 and 101 models, but the former generates a greater peak intensity. The peak at 0.60–0.63 nm is likely associated with the chain–chain spacing in the y-direction and the pitch spacing along the fiber axis. The pitch spacing can be calculated from the helical pitch multiplied by the cosine of the tilt angle, where the tilt angle for an ideal helix is the helix diameter multiplied by π and divided by the helical pitch.44 For a calculated tilt angle of 54° and helical pitch of 1.81 nm for the 91 double helix, the pitch spacing equals 0.73 nm. For the 101 double helix model, the tilt angle is closer to 50° and the pitch spacing is 0.80 nm. Based on these values we can conclude that while the peak is associated with the pitch spacing, it does not directly correspond to it.
Fig. 4 Model of the optimized crystal structure of 91 it-PMMA in the Right Down packing motif. The chain–chain spacing (left) and pitch spacing (right) are shown in light blue. |
The peak at 0.52 nm arises primarily due to reflections from the x-plane. Finally, the peak at 0.31 nm corresponds to the inter-monomer spacing along the axis of the helix. Fig. 3 shows that for the 91 it-PMMA model this particular peak is positioned just below 30°, in line with the experimental X-ray diffraction data, while for the 101 it-PMMA model the peak is positioned just above 30°.
We should note here that the peak intensities reflect contributions from various crystallographic planes, which makes it difficult to precisely determine the exact contribution to each peak. In general, however, we see an excellent agreement between the simulated and experimentally obtained diffraction patterns validating our models.
Table 1 summarizes the simulated model properties and compares them with the experimental values available. For both the 91 and 101 double helixes, densities ranged from 1.220 to 1.255 g cm−3, comparing well to an experimental density of 1.23 g cm−3.45 To compare the relative thermodynamic stability of the model structures we calculated the cohesive energy density which is equal to the internal energy divided by the molar volume of a system, and describes the amount of energy required to remove a unit volume of molecules from their neighbors to infinite separation.47
Description | Packing motif | Density (g cm−3) | Helical pitch (nm) | Cohesive energy density (J cm−3) |
---|---|---|---|---|
a Experimental cohesive energy density of PMMA with unspecified tacticity.46 | ||||
Experiment | — | 1.23 (ref. 45) | 1.84 (91)24 | 361a |
2.10 (101)16 | ||||
91 it-PMMA | RD | 1.235 ± 0.007 | 1.80 ± 0.01 | 385 ± 12 |
RD/RU | 1.240 ± 0.014 | 1.79 ± 0.01 | 281 ± 12 | |
RD/LD | 1.220 ± 0.001 | 1.81 ± 0.01 | 221 ± 1 | |
RD/LU | 1.240 ± 0.028 | 1.80 ± 0.03 | 285 ± 4 | |
101 it-PMMA | RD | 1.225 ± 0.007 | 2.01 ± 0.09 | 302 ± 3 |
RD/RU | 1.215 ± 0.007 | 1.95 ± 0.15 | 281 ± 1 | |
RD/LD | 1.235 ± 0.021 | 2.05 ± 0.01 | 227 ± 36 | |
RD/LU | 1.255 ± 0.007 | 2.06 ± 0.01 | 271 ± 22 |
The 91 it-PMMA exhibits a larger cohesive energy density than the 101 it-PMMA in every case, with the Right Down 91 model at 385 ± 12 J cm−3 compared to 302 ± 3 J cm−3 for the 101. Interestingly, there was a range in cohesive energy density values for both the 91 and 101 models, with the Right Down packing motif providing the largest values for both models, although there appear to be no obvious trends between cohesive energy density and other properties, including structural parameters, density, and the experimental X-ray diffraction profiles for the different packing motifs.
In summary, based on the analyses of X-ray diffraction data, density, structural parameters and cohesive energy densities, the model that best agrees with the experimental data is a 91 it-PMMA double helix with a helical pitch of 1.80 ± 0.01 nm, a tilt angle of 54°, and a pitch spacing of 0.73 nm.
It can be seen from Fig. 5 that the 91-it/181-st stereocomplex model (infinite st-PMMA with 18 units per turn complexed with infinite it-PMMA with 9 units per turn) failed to reproduce the experimental X-ray diffraction data. Most notably the experimentally observed peak of 2.08 nm is shifted to a shorter d-spacing of 1.86 nm. This suggests that the chain width of this model is too narrow, resulting in a crystal that is overly compact. This is further supported by a density of 1.240 ± 0.001 g cm−3 calculated for this structure compared to the experimental density of 1.215 g cm−3.45 In addition, this model fails to reproduce the helical pitch of the st-PMMA, with a value of 0.97 ± 0.016 nm for the model, compared to the experimentally measured value of 0.92 ± 0.02 nm.24 This is reflected by a shift in the associated peak d-spacing to 0.89 nm, compared to the experimental peak at 0.78 nm.
Previous ab initio calculations6 suggested that the helical pitch ratio for it-PMMA and st-PMMA is not exactly 2:1. Based on this, we constructed models of infinite it-PMMA with 40-unit st-PMMA fragments (40mer-st) which is in line with the size of the st-PMMA fragments used in our X-ray diffraction experiments. These 40mer-st fragments exhibited an average helical pitch of 20 MMA units, with gaps of approximately 1–2 units between fragments in the z-direction.
While the 101 it-PMMA complexed with 40-unit st-PMMA model (101-it-/40mer-st) maintains the 1:2 it:st complexing ratio, the model fails to reproduce the experimental helical pitch and experimental X-ray diffraction peak at 0.78 nm. Similar to the infinite triple helix model (91-it/181-st), this peak is shifted to the left, associated with an increased pitch spacing. The density of this model was found to be 1.185 ± 0.007 g cm−3, well below the experimental value.
Fig. 5 demonstrates that the 91 it-PMMA complex with 40-unit st-PMMA fragment model (91-it/40mer-st) exhibits the best agreement with experimental X-ray diffraction profiles. The density range of 1.200–1.215 g cm−3 for the four packing motifs is also in a good agreement with experiment, and the cohesive energy density range for this model is 387–399 J cm−3, compared to values of 362 ± 18 J cm−3 and 287 ± 9 J cm−3 for the 101-it/40mer-st and 91-it/181-st models, respectively (Table 2).
Fig. 5 Wide angle X-ray scattering data obtained from powder diffraction experiments and molecular dynamic simulation for the it-/st-PMMA stereocomplex in the Right Down packing motif. |
Description | Packing motif | Density (g cm−3) | Helical pitch st-PMMA (nm) | Cohesive energy density (J cm−3) | Chain width (nm) | Sum of differencesa (nm) |
---|---|---|---|---|---|---|
a Sum of differences refers to the sum of the numerical value differences between the peak positions of the simulated structures and the experimental X-ray diffraction. Thus, a smaller value indicates a better agreement with experiment. b Experimental cohesive energy density of PMMA with unspecified tacticity.46 | ||||||
Experiment | — | 1.215 (ref. 45) | 0.92 ± 0.02 (ref. 24) | 361b | ||
91-it/181-st | RD | 1.240 ± 0.001 | 0.97 ± 0.016 | 287 ± 9 | 1.68 ± 0.018 | 0.39 |
101-it/40mer-st | RD | 1.185 ± 0.007 | 0.96 ± 0.007 | 362 ± 18 | 1.84 ± 0.007 | 0.27 |
91-it/40mer-st | RD | 1.215 ± 0.007 | 0.90 ± 0.004 | 398 ± 2 | 1.85 ± 0.001 | 0.08 |
91-it/40mer-st | RD/RU | 1.210 ± 0.001 | 0.89 ± 0.006 | 399 ± 1 | 1.85 ± 0.001 | 0.16 |
91-it/40mer-st | RD/LD | 1.200 ± 0.001 | 0.90 ± 0.004 | 387 ± 1 | 1.86 ± 0.011 | 0.17 |
91-it/40mer-st | RD/LU | 1.210 ± 0.001 | 0.90 ± 0.008 | 398 ± 2 | 1.84 ± 0.010 | 0.17 |
Unlike the it-PMMA structures, there was little difference in density, cohesive energy density, or X-ray diffraction for the different packing motifs of the stereocomplex (Table 2). The average st-PMMA helical pitch of this model is 0.90 ± 0.005 nm, in good agreement with the AFM measurements of 0.92 ± 0.02,24 with approximately 20 MMA units per turn. While this results in an it:st complexing ratio of 9:20, it is important to note that the established it:st stoichiometric ratio of 1:2 is merely the best mixing ratio for complexation, and different mixing ratios still result in the same final stereocomplex.21 Additionally, the it-PMMA helical pitch of ∼1.80 nm is in good agreement with the fiber X-ray diffraction experiments that show a fiber identity period of 1.84 nm.22,23 The optimized structure of the 91-it/40mer-st model is shown in Fig. 6.
When Yashima and colleagues proposed the triple helix model, they also proposed a quadruple helix model that could correspond to their AFM results with two strands of st-PMMA wrapped around an it-PMMA double helix.24 We constructed models of the quadruple helix with 40-unit st-PMMA and both 91 and 101 it-PMMA (Fig. S1, ESI†), but the X-ray diffraction profiles and calculated densities of these models were in a lesser agreement with experiment (Fig. S2, Table S1, ESI†). While both the triple helix and quadruple helix models can in principle satisfy the AFM results as well as explain the observed weakness of the first-layer-line reflection (corresponding to a spacing of 1.84 nm) of the fiber X-ray diffraction,22,24 only the triple helix model fully reproduces the experimental density and powder X-ray diffraction profile.
Interestingly, the st-PMMA helix of the 91-it/40mer-st model exhibits a distinct deviation from ideal helical geometry, not seen in either the 101-it/40mer-st or 91-it/181-st models (Fig. 7). This non-ideal helical geometry is characterized by a broader distribution in backbone internal angles and torsions, as well as a small number of torsions evenly distributed approximately every 20 monomer units (2 per turn) of the st-PMMA chain that deviate widely from the standard values of around 180° for an ideal helix comprising 18 units per turn (Fig. 8). Notably, this non-ideal geometry is required to reproduce the experimental X-ray diffraction peak at 0.78 nm, and is similar to the geometry found in the recently discovered and characterized stereocomplex of a cyclic form of 18-unit st-PMMA with linear double helix it-PMMA27 (Fig. 7c), which also exhibits an X-ray diffraction peak at 0.78 nm. The cyclic triple helix stereocomplex also has a similar fiber diameter to that of the 91-it/40mer-st model (the linker unit of the cyclic st-PMMA corresponds to roughly two MMA units) and a corresponding X-ray diffraction peak at 2.08 nm.
To further examine the PMMA stereocomplexation ratio, we constructed models of 36-unit st-PMMA fragments with infinite 91-it-PMMA double helices (91-it/36mer-st). While these systems maintained the 9:18 it- to st-PMMA monomer ratio of the Yashima model, the resulting structure had a density of 1.16 g cm−3; far below the predicted value. Interestingly, the overall structure resembled the non-ideal helical geometry of 91-it/40mer-st model, but with wide gaps between the st-PMMA fragments.
We noted that the gap between successive st-PMMA fragments in the 91-it/40mer-st model roughly corresponds to two MMA units. We thus constructed models of infinite st-PMMA with 21 units per turn. This 91-it/211-st model exhibited a similar structure and X-ray diffraction profile to the 91-it/40mer-st model, but had a cohesive energy density of 245 ± 21 J cm−3; far smaller than the predicted value. This further emphasizes that the helical pitch ratio cannot be exactly 2:1 (i.e. the st-PMMA cannot complete exactly two full turns in the distance required for the it-PMMA to complete one full turn).
In order to gain a better understanding of the interactions driving the stability of the supramolecular assembly, we determined the st:it contact area and total free volume of the 91-it/40mer-st and 91-it/181-st models. Our results show that both models exhibit similar free volume (approximately 10% of the total volume) and st:it contact area (approximately 35–36% of the total st-PMMA surface area is in contact with it-PMMA for both models). This suggests that the observed differences in thermodynamic and structural properties are not due to differences in the packing of the stereocomplexes. A decomposition of the cohesive energy density for the two models reveals that in particular the electrostatic interactions between the st- and it-PMMA of the 91-it/181-st model are strongly unfavorable. Because the it- and st-PMMA have different helical pitches, a deviation from ideal helical geometry is necessary to maximize the non-bond interactions as seen in the 91-it/40mer-st model.
The molecular dynamics simulations described in this study provide a vital tool to resolve molecular-level arrangement of complex molecular structures, when experimental means are inadequate. Furthermore, the reported molecular mapping technique is expected to have a wide scope of applications in macro(supra)molecular chemistry, including design and synthesis, structural characterization and property simulation.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4sc02971b |
‡ A.C. and G.Y. contributed equally. |
§ Current address: IBM Research Australia, 5/204 Lygon St, Melbourne, Victoria 3001, Australia. |
This journal is © The Royal Society of Chemistry 2015 |