4. Results and Discussion
Molecular dynamics simulations were conducted at a temperature of 300 K to validate atomistic potentials that can be used to model the phase transition pressure. For simulating the phase transformation of Mg, we considered two atomistic potentials, as follows: the potential by Sun et al. [
14], which is the most widely used potential for Mg, and the potential developed by Wilson and Mendelev [
19]. The latter corrects the tensile instability artifacts observed under spall conditions, caused by the potential by Sun et al., under high tensile stresses. Our work focused on high pressures (compressive stresses), so simulations using either potential are expected to align with the experimental results on phase transformation in magnesium at room temperature.
Simulated results obtained from three thermodynamic ensembles were assessed. The critical pressure for phase transformation was consistent between all the aforementioned ensembles. The kinetics of phase transition were expected to be different from one ensemble to another since differences in the ability of the ensembles to exchange thermal energy and mechanical work between the system and the surroundings are naturally expected to change the conditions for phase transition evolution.
Figure 3 shows a series of snapshots taken at different times during a representative simulation of a phase transition. The simulation was conducted at an initial pressure of 48 GPa and a temperature of 300 K. In the figure, the blue atoms represent the HCP phase, while the green atoms belong to the BCC phase. The maroon-colored atoms within the HCP phase are disordered (CNA = 5). When viewed along the
direction, the simulation results show the motion of a HCP-BCC phase boundary or a phase transition front. The boundary is composed of atoms a few layers thick, and the atoms within the boundary are disordered.
Figure S1 shows the same result when viewed along
direction. In this direction, stacking faults are seen in the basal plane of HCP Mg propagating ahead of the phase boundary. Stacking faults on the basal plane of HCP magnesium is an energetically favorable deformation mechanism [
20]. Within the BCC phase in
Figure 3, a planar boundary was observed to be left behind by the propagating phase boundary. This boundary, colored in red, is a grain boundary made up of several layers of thick atoms, and it is mobile.
The displacement and velocity histories from the HCP-BCC phase boundary (indicated by an arrow on the right side of
Figure 3) are shown in
Figure S2. The velocity history oscillates due to the nucleation of defects that dissipate energy behind (in BCC) and ahead (in HCP) of the propagating phase boundary. Additionally, the overall velocity decreases over time because the overall pressure in the system decreases as the HCP-to-BCC transformation progresses. Furthermore, the energy of the system reduces while maintaining a constant temperature via the NVT ensemble.
The phase boundary propagates under relatively pure hydrostatic pressure. This hydrostatic condition was further verified by plotting the evolution of the normal stress field in
Figure S3, which shows that the pressure ahead of the phase boundary remains uniform. However, the stress state behind the phase boundary is no longer purely hydrostatic.
Figure S4 shows a shear wave behind the moving phase boundary on the right. The stress tensor components were calculated using the virial stress formulation and time-averaged over 1 ps. The shear wave in
Figure S4 (on the right) is traveling in the -ve Z-direction and coincides with the normal wave in
Figure S3. Both the fronts of the shear and normal waves coincide with the position of the phase boundary. Due to the phase transformation from HCP to BCC, there is a jump in the shear stress and the normal stress components across the HCP-BCC phase boundary. The phase transformation leads to a reduction in the magnitude of pressure in the BCC phase. However, in the BCC domain, the magnitude of the normal stress components is unequal, resulting in finite shear stress, as seen in
Figure S4. This shear stress component is likely responsible for defects, such as twin boundaries in the (BCC phase) wake of the moving HCP-BCC phase boundary.
Figure 4 shows the velocity of a phase boundary with pressure. The propagation velocity starts at 46 GPa and increases to 650 m/s at 48 GPa. Between pressures of 48–49 GPa, a jump in the velocity is observed, reaching about 2500 m/s at 49 GPa. This jump is qualitatively similar to the non-monotonous kinetics of a twin boundary, which is caused by the nucleation of new mechanisms of plastic deformation (dislocations and twin boundaries) that influence the mode of propagation of the boundary (as reported in Daphalapurkar et al., 2014 [
21]). This MD result indicates a non-monotonous dependence of phase boundary velocity on the pressure. Beyond pressures of 49 GPa to 54 GPa, the velocity of propagation increases, reaching about 3000 m/s. However, there is a slight decreasing trend in the velocity from 49 GPa to 50 GPa.
In
Figure 5, snapshots from simulations conducted at different initial pressures (46 GPa to 56 GPa) show the planar boundary that was left behind in the BCC structure by propagating two phase boundaries. At a critical pressure of 46 GPa, a few layers of BCC atoms were nucleated. However, despite the nucleation of the phase boundary, no motion was observed in the boundary. The motion of the phase boundary was observed at and above 47 GPa pressure. The agreement between the predicted phase transformation pressure using the potential by Sun et al. [
14] and the experimental prediction [
16] is satisfactory. The results are shown for the constant volume and temperature ensemble, while the results using two other ensembles (constant volume and energy; constant pressure and temperature) resulted in similar values for the critical pressure at which phase boundary propagation commences.
We further provide observations on the activated planar faults from the MD results. It was found that the density of planar faults left behind by the phase boundary increases with the initial pressure, as seen in
Figure 5. Two types of planar boundaries (vertical and inclined) were observed; they are topologically different from each other. The non-planar boundaries, which are made up of several layers of thick atoms and colored in red, are the grain boundaries in BCC Mg that were left behind by the propagating HCP-BCC phase boundary.
Figure S5 shows a comparison between the motion of the phase boundary at two initial pressures of 48 GPa and 51 GPa. The magnitudes of average velocity indicate propagation of the phase boundary under a reasonably constant value of statistically averaged pressure and temperature conditions. At 51 GPa, the phase boundary travels at an average velocity of 2.3 ± 0.23 nm/ps (or 2300 ± 230 m/s), which is higher than the velocity of 0.63 ± 0.11 nm/ps (or 630 ± 110 m/s) at 48 GPa.
Next, the propagation modes of the phase boundary were identified.
Figure 5 shows snapshots from simulations conducted at different initial pressures ranging from 46 GPa to 56 GPa. These snapshots show planar boundaries left behind in the BCC structure by propagating phase boundaries. The jump in the propagation velocity above 49 GPa from
Figure 4 confirms that a new plastic deformation (twin) system was activated, which helped in faster propagation of the phase boundary. Previous studies have shown that the presence of dislocations in the original phase impacts the formation of the phase boundary (for example, [
22]).
To the author’s knowledge, these are the first results to demonstrate the role of plastic deformation in the newly transformed phase (in the wake of the phase boundary) in modulating the phase transformation kinetics. Two types of boundaries, namely a grain boundary and a twin boundary, were identified in BCC Mg. In BCC metals, twins are created by multi-layer stacking faults resulting from the movement of
dislocations on successive
planes [
23]; where
a represents the BCC lattice constant. This process can be explained in the crystallographic
direction. The twin formation happens by shearing consecutive
planes of a BCC crystal. The glide of the first
dislocation on a
plane causes the creation of a one-layer stacking fault. When the second and third dislocations glide on successive
planes, two- and three-layer stacking faults are created, respectively. The twin growth occurs when the dislocations glide beyond the third layer on successive
planes. It is important to note that the twin boundaries in these simulations are mobile, and the subsequent time snapshots in
Figure S1 demonstrate that the grain boundaries are mobile, as well.
The critical pressure for nucleation of the phase boundary was 47 GPa, and although BCC atoms a few layers thick were nucleated (on the left side), there was no motion of the phase boundary. Phase boundary motion was observed at all pressures above 47 GPa. The agreement between the MD-predicted phase transformation pressure (47 GPa) using the potential by Sun et al. [
14] and the experimental prediction (50 GPa) [
16] is satisfactory.
The density of planar faults left behind by the phase boundary increases with initial pressure. Two types of planar boundaries are observed—vertical and inclined; these are grain boundaries and twin boundaries, respectively, as viewed along the
direction of BCC Mg.
Figure 6 shows snapshots showing the propagation of phase boundaries, along with histories of displacement and velocity, for an initial pressure of 51 GPa. An algorithm was used to calculate the average X-position of atoms belonging to an HCP-BCC phase boundary, which were identified using CNA analysis. The left phase boundary leaves behind vertical planar faults (grain boundaries). On the other hand, the right phase boundary leaves both types of planar faults in its wake. After 21 ps, the propagating phase boundary appears to suppress the inclined planar faults (twin boundaries). Thus, the activation of inclined planar faults (twin boundaries) facilitated the relatively higher propagation velocity of the right phase boundary compared to the left phase boundary. This observation is also true when looking at snapshots of simulations in
Figure 5, which show the presence of inclined planar faults (twin boundaries) for simulations with initial pressure higher than 49 GPa. These twin boundaries result from the activation of slip systems depending on the magnitude of the resolved shear stress on the slip system, which is favorable for twinning.
The study conducted nine simulations with superimposed shear stress from 20 megapascal to 1000 megapascal (MPa) with an initial pressure of 46 GPa. It is known that the shear stress modulates the phase transformation pressure [
9]. In all cases of simulations, results indicated the critical pressure for the propagation of the phase boundary was reduced in the presence of shear stress. Such high levels of shear stress may be experienced under shock-loading conditions and in anisotropic crystals. At 46 GPa pressure, the phase boundary propagated in the presence of a superimposed 500 MPa shear stress, which otherwise failed to propagate under the pure hydrostatic case. In addition, under 1000 MPa shear stress, the BCC phase nucleated, and the phase boundary propagated a significant distance at pressures as low as 40 GPa, which is almost 14% lower than the critical pressure under purely hydrostatic conditions (47 GPa pressure). Thus, the shear stress provides additional thermodynamic force for the motion of the phase boundary.
This work successfully demonstrated the feasibility of simulating the transformation from hexagonal close-packed (HCP) to body-centered cubic (BCC) phase that occurs at and above 47 GPa and at room temperature (300 K), using an intermolecular potential developed for pure Magnesium by Sun et al. [
14]. Using molecular dynamics, we developed a model to examine the kinetics of phase transformation under controlled initial pressure conditions. The simulated results for the critical phase transformation pressure are consistent with experimental results [
16] at 300 K temperature. Finally, this work compared simulations of phase transformation under several different hydrostatic pressures and characterized the kinetics relation, i.e., the velocity of a moving phase boundary as a function of pressure. The molecular dynamics result suggests a non-monotonic dependence of the phase boundary velocity on pressure, indicating the need for further development of models of the kinetics of phase transformation to account for the activation of defects that enable high-speed boundary velocities.