Abstract
In layered materials, a common mode of deformation involves buckling of the layers under tensile deformation in the direction perpendicular to the layers. The instability mechanism, which operates in elastic materials from geological to nanometer scales, involves the elastic contrast between different layers. In a regular stacking of “hard” and “soft” layers, the tensile stress is first accommodated by a large deformation of the soft layers. The inhibited Poisson contraction results in a compressive stress in the direction transverse to the tensile deformation axis. The hard layers sustain this transverse compression until buckling takes place and results in an undulated structure. Using molecular simulations, we demonstrate this scenario for a material made of triblock copolymers. The buckling deformation is observed to take place at the nanoscale, at a wavelength that depends on strain rate. In contrast to what is commonly assumed, the wavelength of the undulation is not determined by defects in the microstructure. Rather, it results from kinetic effects, with a competition between the rate of strain and the growth rate of the instability.
Keywords: computational modeling, block copolymers, mechanical properties, mechanical behavior, buckling instability
The mechanical response of multiblock copolymers depends sensitively upon their constituent homopolymers segments, molecular architecture, and chain topology. Triblock copolymers, in particular, have become an attractive material for their use as thermoplastic elastomers that could be integrated in several technical and manufactural fields [copolymer styrene butadiene rubber is commercially exploited in footwear, in pressure-sensitive adhesive (K-Resine), in paving and roofing compounds, etc.]. Depending on the amount of each phase, the segregated block copolymers may present several morphologies (e.g., spherical, cylindrical, lamellar, etc.) (1). The lamellar morphologies are particularly interesting as model systems, as well-aligned specimens can be prepared by shearing. The one-dimensional aspect of the structure simplifies the analysis, and the mechanical response reveals equally the presence of both phases, whereas in other morphologies, it tends to be dominated by the majority matrix phase. In these block copolymer systems, the constituent blocks are generally chosen such that one of them is glassy and the other one is rubbery. A single copolymer chain can be shared between two different glassy lamellae, forming a rubber bridge that provides a strong coupling between phases. The resulting system combines the stiffness of the hard glassy phase and the ductility of the soft rubbery phase.
When such a lamellar copolymer sample is submitted to a tensile strain perpendicular to the layers, the glassy layer eventually buckles into a “chevron” morphology. With increasing strain the normal to the lamellae tilts away from the stretching direction, whereas the lamellar spacing remains almost constant. This behavior was demonstrated experimentally in triblock copolymers by small-angle X-ray scattering under deformation (2) and by micrographs of strongly deformed samples (3) (see Fig. 1). Similar effects are also observed in lamellar systems with alternating crystalline and glassy parts (4, 5), and in deformed semicrystalline polymers, which form locally lamellar structures of crystalline material separated by softer amorphous parts (6).
Fig. 1.
(Upper) Transmission electron micrograph shows the buckling observed in a real copolymer sample (styrene-butadiene-styrene). Reprinted from ref. 17, Copyright 2004, with permission from Elsevier. (Lower) Lamellae buckling observed by molecular dynamics simulation; snapshot is taken at ezz = 0.55. This image contains six periodic copies of the simulated system, which is enclosed in the white frame. The scale on the right is obtained by assuming a monomer size σ = 0.5 nm.
This buckling instability under strain, which is observed in many layered materials from smectic liquid crystals (7) to geological layers (8, 9), is frequently described in a qualitative way by a preference to shear compared to an extension in the direction normal to the layers, in order to preserve the lamellar spacing. A different cause for buckling is the existence of a Poisson effect. In a stacking of hard and soft layers, the soft phase accommodates most of the imposed deformation, and because the Poisson contraction is prevented by the coupling to the hard phase, it exerts a compressive stress in the transverse direction. The hard layers sustain this transverse compression until buckling takes place and results in an undulated structure. In general, elasticity predicts buckling to take place on the largest wavelength compatible with the boundary conditions imposed to the system (10). We study this generic scenario by means of molecular dynamics simulations, for a material made of triblock copolymers in their lamellar phase. The contrast in elasticity is provided by a different glass transition temperature of the different blocks. We use the ability of molecular dynamics simulations to give information on the local values of stresses and strains to explore the causes of the instability in triblock copolymers with alternating glassy and rubbery layers, without introducing an a priori description of the mechanism. Although the elastic origin of the instability is confirmed, our results demonstrate an unexpected dependence of the failure mode on strain rate. The wavelength of the undulations is determined by the deformation rate, and a characteristic size emerges even in the absence of preexisting defects in the microstructure. We discuss a general mechanism for the emergence of such a characteristic size, which results from a competition between the rate of strain and the growth rate of the buckling instability.
Evidence of the Poisson Effect
When a multilayered system is stretched perpendicularly to the layering direction, each component of the system will deform according to its own stiffness. Locally, the deformation is distributed between phases in a way that ensures the continuity of the stress. The resulting macroscale deformation is the sum of the local strain response of each phase, so that the stiffness will be dominated by the response of the soft phase. In a lamellar copolymer with alternating rubbery and glassy phases, the tensile strain will be mainly localized in the rubbery lamellae, which are essentially incompressible (Poisson ratio νrubbery ≃ 0.5). The contraction in the transverse direction that would result from the Poisson effect is however prevented by the strong coupling to the hard phase at the interface, so that the soft phase exerts a strong compressive stress in the transverse direction on the hard layers. The glassy phase becomes submitted to a tensile stress in the perpendicular direction and a compressive stress laterally. Under these conditions, and for a sufficiently large system, the buckling instability takes place to relax the lateral compressive stress.
This scenario can be checked by monitoring the local stress in a sample strained perpendicularly to the lamellae. Fig. 2 shows a map of the lateral stress (
) of a stretched copolymer sample at a true strain ezz = 0.04. The average pressure in the transverse direction is zero because uniaxial tensile conditions are imposed globally. The local stress, however, is positive in the rubbery phase, although it is negative in the glassy phase, indicating a local compression parallel to the glassy lamellae. An interesting additional feature that is apparent in Fig. 2 is the existence of noticeable fluctuations in the local stress values. Such fluctuations are expected in the response of amorphous materials, and they arise from the local heterogeneity of elastic properties in such materials; a property already well documented for glassy polymers (11). We will see below that the response of the system can become macroscopically nonuniform due to the development of an elastic instability, and it is therefore quite natural to speculate that the initial stress fluctuations serve to nucleate this instability. A related study of cavitation in glassy homopolymers showed a similar correlation between elastic fluctuations and nucleation of cavities (12).
Fig. 2.
Cartography of the lateral stress
. Snapshots were taken at a deformation ezz = 0.04. The local stress is computed within a box of size 5σ × 5σ × Ly = 102σ, where σ is the size of a monomer (typically σ = 0.5 nm, see Size and Strain Rate Dependence, p. 4). The stress in these figures was probed in a relatively small sample (Lx = 34.5σ, Ly = 102.3σ, and Lz = 34.5σ), in which buckling does not take place; however, the analysis of the stress profile clearly shows the importance of the Poisson effect, with a large contrast in the transverse stress between the compressed glassy layers and the rubbery layers under tension. The influence of the lateral dimension of the sample is discussed in the text.
Plastic Deformation Through Buckling and Cavitation
Fig. 3 illustrates the deformation process that takes place under tensile deformation in a sufficiently large sample, and the corresponding stress–strain curve is shown in Fig. 4. In this first set of results, the strain rate is
in reduced units (see Materials and Methods). The pressure is fixed to zero in the x and y directions.
Fig. 3.
Local density cartographies at several strains. The high (low) density phase corresponds to the glassy (rubbery) lamellae. The phase buckling starts before cavitation. As the deformation progresses, cavities will nucleate randomly in the rubbery phase. Cavities that are located in the tilted part of the chevron disappear rapidly; however, only cavities that are located in the hinges will survive to a high strain.
Fig. 4.
(Upper) Stress–strain curve of the sample shown in Fig. 3 under uniaxial strain conditions. The black points denote the selected configurations shown in Fig. 3. The stress release is associated with a combination of two phenomena: buckling, and nucleation and growth of cavities in the rubbery phases. (Lower) Evolution of the lateral strain 0.5(exx + ezz) under uniaxial tensile conditions. The local slope defines the Poisson ratio, and buckling is correlated to a strong change in this slope, as the sample starts deforming in an accordion-like manner.
The stress–strain curve displays three main regimes:
Elastic regime: At small strain, the stress grows linearly with the imposed deformation. This regime is limited to a very small deformation amount (less than 2%). The Young’s modulus, which can be fitted from this curve, results from a combination of the elastic behavior of each phase. The density maps show very little change in this regime.
Buckling: Beyond the elastic regime, a progressive softening is observed. This slight deviation from the elastic linear behavior is commonly interpreted by the change of molecular conformation in the rubbery phase. The buckling of the glassy phase starts at ezz = 0.06 and can be detected from a rapid change in the apparent Poisson ratio of the material. From the onset of the buckling instability, the sample starts deforming in an “accordion-like” manner, with a higher Poisson ratio than a sample with parallel layers.
Cavitation: After buckling, a strong stress drop occurs at ezz = 0.08. This drop can be correlated with the nucleation of cavities in the rubbery phase, as illustrated by the fourth density map in Fig. 3. The low-density spots in Fig. 3 correspond to the cavitation in the rubbery layers. Indeed, because of the buckling, the local deformation of the rubbery phase is not homogenous. The sample progressively adopts a chevron morphology, with different deformation states: At large strains, the cavitation is confined to a localized region in space, developing into a hinge. At the hinges of the chevron, the deformation is essentially tensile, whereas the tilted part undergoes a simple shear deformation. The latter is caused by the rotation and sliding of the hard lamella. In contrast, at the hinges of the chevron, the deformation is essentially triaxial and favors nucleation of cavities. As a result, the cavities in the rubber that initially appear randomly tend to heal in the sheared zones and nucleate preferentially where triaxial stress persists, as illustrated by the sequence of snapshots in Fig. 3.
Elastic Description of the Buckling Instability
As mentioned in the Introduction, two different theoretical descriptions of buckling of lamellae under stress are available in the literature. One approach is based on a free energy functional of the order parameter that describes the lamellar order, which explains the instability by the fact that a strained state will try to maintain the lamellar distance that minimizes this free energy (13). This approach would be appropriate for copolymers in which both phases are at equilibrium, so that the order parameter can respond to the deformation. Here one of the phases is glassy, and the explanation for the buckling instability must be searched in a different direction, involving the minimization of the total elastic energy. This description (which for some aspects goes back to early works of Biot, refs. 8, 14 and 15) has been detailed in a seminal paper by Read et al. (10). Taking for simplicity a two-dimensional geometry, the elastic energy of the sample under small strain can be written as
![]() |
[1] |
where Cij are the components of a symmetric 2 × 2 stiffness matrix of the entire system, and eij is the macroscopic deformation. In this equation, the material is considered as homogeneous and anisotropic. The indexes 1, 2 refer to the directions normal and parallel to the layers, and the coefficients Cij and G (shear modulus parallel to the layers) can be obtained from mechanical tests in different directions, or deduced from the elastic properties of each lamella.
The bending energy results from the variation of the lamellar rotation angle θ (the angle between the layer and the horizontal axis x). The associated energy density reads
![]() |
[2] |
where K is the bending modulus of the sample. Because of the serial coupling between phases, the bending modulus will be dominated by the contribution of the hard phase. The bending modulus can then be estimated from simple beam bending theory as
, where ϕh is the volume fraction of the hard phase, Eh is the Young’s modulus of the hard phase, νh is its Poisson ratio, and d is the lamellar spacing.
The total energy density results from the addition of the bulk elastic energy and the bending energy, U2D = Ubend + Umacro. It can be expressed in terms of the global deformation exx, exz, and ezz and of a local, nonaffine displacement field
that quantifies the difference between the displacement imposed at the global scale and the one observed locally.
The final expression for the free energy, written as an expansion in powers of
(10), reads
![]() |
[3] |
A linear stability analysis of this energy is performed by introducing a sinusoidal perturbation of the form observed in our simulations,
| [4] |
with k = 2nπ/L a wave vector compatible with the boundary conditions
![]() |
[5] |
where
![]() |
[6] |
The buckling instability occurs upon increasing strain when the coefficient of
in Eq. 5 becomes negative, meaning that the global gain in elastic energy overwhelms the bending energy penalty. In a 3D case, the same analysis process can be performed, which leads to a function
instead of
, where
| [7] |
To close the system, one assumes that, before the buckling begins (i.e., in the elastic regime), exx and eyy can be substituted by νezz, where ν is a global Poisson ratio. Under this assumption,
becomes a function
of ezz only. The buckling strain
can be estimated by solving this equation for a fixed wavevector kn = 2nπ/L:
| [8] |
For a given wavevector kn, buckling will become possible above a certain strain
such that
. As
is an increasing function of the strain, the wavevector corresponding to the largest wavelength (i.e., the size of the box), will become unstable at the smallest strain, according to this analysis. This reasoning implies that, for a smaller box size, a larger strain would be needed to observe buckling; as noted above, in such small systems, cavitation tends to take place before the critical strain for buckling is reached, and the elastic analysis becomes irrelevant above the cavitation threshold.
In the following, numerical comparison between simulations and this theory will be made by using for the elastic constants Cij values determined from simple linear deformations of a small sample that does not exhibit the buckling instability. These values are, for the interaction parameters and temperature mentioned below, C11 = 24.17, C33 = 7.61, C23 = C13 = 6.5, and G = 0.07 (in the same reduced units, the Young’s modulus of a glassy polymer is of order 50; see Materials and Methods). The Poisson ratio is ν = 0.178.
Size and Strain Rate Dependence, Interpretation
The discussion in the previous section shows that the boundary conditions and geometry of the sample have an important influence on the buckling instability. For example, the instability takes place for a different mode for a system with free or with periodic boundary conditions, the first one undergoing a “half-wave” instability, which is prohibited in the second case. Also, the buckling of small samples is impossible because the bending energy of the glassy phase is very high compared to the deformation energy of the bulk. Therefore, a critical size of sample can be defined as
.
, the minimal length from which the sample will be able to buckle under tensile strain before failure due to cavitation and crazing in the rubber phase, becomes dominant.
According to elastic theory, the instability will take place at smaller and smaller strains for bigger and bigger samples, and always at the largest possible wavelength allowed by the boundary conditions. This prediction, however, contradicts a number of experimental observations in which a rather well-defined wavelength of the chevron structure is observed. This discrepancy is commonly assigned to preexisting defects in the microstructure (3). Simulation provides an ideal benchmark of this hypothesis, as it allows one to study an ideal microstructure. We have therefore studied samples of various sizes, between 100 and 800σ in the y direction. Fig. 5 compares the response of all tested samples, at a strain rate 7.3 × 10-5. In terms of stress–strain relation, all samples have roughly the same mechanical behavior up to the yield point.
Fig. 5.
Snapshots of several samples with different sizes. All configurations are taken at a true strain ezz = 0.08. The samples are obtained by replication of a system with size L0 = 32.8σ. Buckling is possible only for the longer samples with Ly≥393.6. The buckling wave length seems to be size independent.
However, it is clear that the minimal length for observing buckling before cavitation is at least 200 monomer sizes σ, implying that such observations can be made only on very large (by simulation standards) systems. For samples larger than about 400σ, the onset of buckling always occurs at the same strain (ebuck = 0.06), in contradiction with the expectation from the elastic description of the previous section. Another surprising observation, illustrated in Fig. 5, is that the wavelength of the instability does not appear to increase with the size of the system.
Fig. 6 summarizes the buckling properties obtained at strain rate of 7.3 × 10-5. For each sample, the theoretical value of the buckling strain was calculated from Eq. 8, assuming an instability wavevector k = 2π/L except for the largest sample. The predicted values of
is always less than the measured one. This difference will be interpreted below as a direct consequence of kinetic factors that are not taken into account in the elastic calculation. Note, finally, that the yield strain and stress are roughly the same for all samples, and are correlated with the cavitation in the rubber phase.
Fig. 6.
Strain at buckling. Comparison for two different strain rates 7.3 × 10-5 (blue bars) and 1.4 × 10-5 (red bars) for different system sizes, with the prediction of elastic theory (yellow bars). Note that the smallest system does not exhibit buckling at high strain rate. For large samples, the buckling at high and low strain rates are observed in different modes, see Figs. 7 and 8. The comparison with the prediction of elastic theory shows that the latter is quite accurate when the buckling takes place in the largest wavelength mode, although it underestimates somewhat the buckling strain due to kinetic effects.
In order to understand the role of strain rate, we have submitted the same samples to a uniaxial tensile strain test driven at a lower strain rate (
). We find that (i) the change in the Young’s modulus is negligibly small for all samples, (ii) the yield stress and strain decrease as the strain rate decreases, and, finally, (iii) the stress softening exhibits a smooth transition (from yield to the drawing regime) at low strain rate compared to a large drop at high strain rate. Depending on sample size, the yield stress and strain are more or less affected. For the smallest sample, the decrease of the yield stress and strain is small compared to other samples. In general, the decrease of the yield threshold is strongly correlated with the change of the plastic mode from cavitation to buckling. Both cavitation and buckling result in a yield behavior, however, the yielding associated with buckling is much more progressive and smooth than the one associated with cavitation, as illustrated in Fig. 7. The most striking observation, however, is the fact that the wavelength of the buckling instability changes with strain rate. In the largest sample, it is equal to sample size, as expected from elasticity theory (see Fig. 7).
Fig. 7.
(Upper) Snapshots of samples with lateral size Ly = 492σ and Ly = 787σ driven at two different strain rates (
and
). At low strain rate , the buckling wave length is equal to the sample length, which is not the case at high strain rate. Note the imperfect aspect of the sinusoidal pattern in the first snapshot, indicative of a competition between modes with different wavelength. Note also that, for this high driving rate, cavitation and buckling take place simultaneously. (Lower) Stress–strain curves that correspond to the two different driving rates of the largest sample. The high strain rate curve is identical to the one shown in Fig. 4.
We propose an interpretation of this unexpected change of wavelength with strain rate based on a simple model of the competition between unstable modes. It has been argued above (see Elastic Description of the Buckling Instability) that the onset of buckling at a certain wavevector k is determined by the function
, where f2 is obtained from Eq. 6 or Eq. 7. Above a critical strain ec, f2(ϵ) becomes negative, and the wavevectors in the range
become linearly unstable. We propose to account for the time evolution of the amplitude Uk of a given mode through the simple linear equation
| [9] |
where Λ is a phenomenological kinetic coefficient which is assumed here, for simplicity, to be wavevector and strain-rate independent, at least in the range of strain rates investigated in our simulations. Beyond ec, the growth rate ΛF has a maximum at a finite wavevector. The key in understanding the effect of strain rate is in the time dependence of F, which is encoded in the time dependence of ezz and renders the evolution nontrivial. For small strain rates, the instability of the smallest wavevector k = 2π/L has ample time to develop before the strain increases and makes a second mode at k = 4π/L unstable. At higher strain rates, the growth rate evolves on timescales comparable to the instability itself, and a competition between modes arises. By solving numerically Eq. 9 with a value of Λ adjusted to reproduce the observed growth of the instability in one of the configurations, we found that, for the largest sample size considered in our simulations, the mode that corresponds to k = 4π/L indeed overwhelms the long wavelength mode k = 2π/L when the system is driven at the largest strain rate, before the latter mode has time to develop significantly. Therefore the second mode, rather than the first, is observed. Although the very high strain rates used in simulation (see Materials and Methods) result here in a selection of very short wavelengths of the order of nanometers, the effect is expected to be very generic and could result in the submicron chevron structures observed in experiments. These results are summarized in Fig. 8, which displays the competing mechanisms depending on sample size and strain rate.
Fig. 8.
Qualitative summary of our observations, indicating the various modes of deformation and yield depending on strain rate and sample size. The points indicate the simulated configurations, and the solid lines between regions are shown as guides to the eye.
Conclusion
The buckling instability of layered materials has been explored here by atomistic simulations, in the case on a lamellar copolymer with glassy and rubbery lamellae. This approach allows one to identify unambiguously the mechanism that drives the instability and failure of such materials, as being caused by the elastic contrast between the two phases and a Poisson ratio effect. Still, a pure elastic theory is insufficient to account for the dependence of the observed instability on strain rate, which is also reported here. A simple description of this dependence was provided by a model that involves the competition between the growth rate of linearly unstable modes with the rate of deformation. This rate dependence of the deformation mode of the microstructure, which is still to be investigated in controlled experiments, indicates the possibility of a rich and still unexplored phenomenology in the mechanical behavior of layered materials. The generality of the mechanism for buckling points to the importance of this instability as a plasticity mechanism in nanostructured polymer materials, which is expected to operate in semicrystalline materials as well as in block copolymers, and to complement more traditional mechanisms such as cavitation and crazing.
Materials and Methods
Our molecular dynamics simulations involve standard coarse-grained model polymer chains. Each chain is represented by a sequence of 50-100-50 beads of different chemical nature (A andB) interacting via covalent finitely extendable nonlinear elastic bonds and Lennard–Jones (LJ) interparticle potentials. The parameters of the LJ potentials are chosen to ensure that phase separation into a lamellar morphology takes place and that the A layers are in a glassy state, while the B layers remain rubbery at the tensile test temperature (Ttest ≃ 300 K). The method used for generating samples has been detailed in ref. 16. In terms of Lennard–Jones interaction parameters, we take ϵAA = 1, ϵBB = 0.3, and ϵAB = 0.4. The resulting glass transition temperatures are
for the A layers and
for the B layers. The diameter and mass, σ and m, are identical for all species and serve as length and mass units, respectively. Using an energy scale of 1,000 K/kB and a length scale of 0.5 nm, which are typical in the coarse-grained descriptions of standard polymers, the corresponding stress unit is of order 100 MPa, and the Young’s modulus of the glassy polymer is of the order of 1–10 GPa.
An important remark here is that the timescale that results from these choices of units, if parameters appropriate for typical polymers are used, lies in the picosecond time range. Therefore, the strain rates achieved in simulations are of the order of 107 s-1 in real units, extremely high compared to typical experimental rates. As is often the case in simulation studies involving glassy materials, the behavior observed in simulation studies must be understood as being qualitatively, rather than quantitatively, representative of the experimental reality.
Supplementary Material
Acknowledgments.
We thank Prof. D. J. Read and Prof. T. McLeish (Leeds University) for useful exchanges. Computational support by the Fédération Lyonnaise de Calcul Haute Performance and Grand Equipement National de Calcul Intensif are acknowledged. Financial support from Agence Nationale de la Recherche (Nanomeca project) and Région Rhône-Alpes (Macodev project) are also acknowledged. J.-L.B. is supported by Institut Universitaire de France. Part of the simulations were carried out using the Large Atomic Molecular Massively Parallel Simulator molecular dynamics software (http://lammps.sandia.gov).
Footnotes
The authors declare no conflict of interest.
This article is a PNAS Direct Submission.
This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1111367109/-/DCSupplemental.
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