Molecular dynamics simulation of vacancy cluster formation in β- and α-Si3N4

https://doi.org/10.1016/j.commatsci.2020.109632Get rights and content

Highlights

  • MD simulation shows Si3N4 polymorphs can accommodate up to ~12% atomic vacancies.

  • Due to energy and volume minimization atomic vacancies tend to form large clusters.

  • High concentration of vacancies (25%) in α results in α to β transformation at 1900 K.

  • Vacancy clustering results in significant fluctuation of lattice constants of β and α.

Abstract

Molecular dynamics simulation is used to study vacancy cluster formation in β- and α-Si3N4 with varying vacancy contents (0–25.6 at%). Vacancies are randomly created in supercells, which were subsequently heat-treated for 114 ns. The results show that both β and α can tolerate vacancies up to 12.8 at% and form clusters, confirming previous experimental data indicating 8 at% vacancy in α-Si3N4. However, 25.6 at% vacancy in β results in complete amorphization, while the same amount in α results in a transformation of a semi-amorphous α phase to a defective β phase, leading to the removal of the clusters in newly formed β. This clearly explains why cluster vacancies are not experimentally observed in β, considering that β-Si3N4 ceramics are produced from α. Furthermore, the lattice parameters of both modifications increase with increasing vacancy content, revealing the cause of different lattice constants that were previously reported for α-Si3N4.

Introduction

Silicon nitride (Si3N4) possesses excellent high-temperature stability, high thermal shock resistance, good creep behavior, and good corrosion and oxidation resistance [1], [2], [3]. It is very well known that lattice defects, particularly Schottky defects, play an important role in determining the overall properties of Si3N4 ceramics [4], [5]. The Schottky defects are either caused by the introduction of oxygen as an impurity or thermal annealing that results in the formation of simultaneous Si and N vacancies [6]. In the case of oxygen impurity, vacancies are created to maintain the overall charge neutrality of the lattice [7]. Although α-Si3N41 initially was assumed to be established by oxygen impurity, but later research showed that nearly pure α-Si3N4 can be synthesized [7]. For α-Si3N4, previous researches showed the presence of vacancy clusters (as large as 30 nm) or dislocation loops [8]. Such clusters or loops are not yet detected in β-Si3N4, seemingly due to the unstrained lattice of β-Si3N4 (while α-Si3N4 is strained) impeding Schottky defects formation. Moreover, it is assumed that Si and N mobilities are higher in β-Si3N4 than in α-Si3N4, so vacancies are assumed to get vanished in the later during high-temperature sintering [9]. This reasoning is based on the diffusion data of Kijima and co-workers [10], which are controversial, since, in spite of all similarities of β and α modifications, the activation energies of N diffusion in the former and latter are measured as 778 and 235 kJ/mol, respectively. Wang et al. [11] calculated the amount of Schottky defects in α-Si3N4 sintered at 1973 K to be 0.08 at%. This calculation is only based on a large cluster of vacancies (~25 nm in diameter), ignoring the smaller ones. Accordingly, using DN=4DvVSi3N4, in which DN, Dv, and VSi3N4 are diffusion coefficient of N, diffusion coefficient of vacancy (estimated as 2 × 10−18 m2/s), and volumetric vacant fraction of Si3N4, respectively, Wang et al. [11] calculated the DN in α-Si3N4 as 6 × 10−21 m2/s. This is stated to be close to that obtained by extrapolation of Kajima’s data at 2000 K (10−19 m2/s) [10], although being two orders of magnitude different. Additionally, the extrapolation of Kajima’s data seems to be considerably (three orders of magnitude) miscalculated, since extrapolation of Kajima’s work yields diffusion coefficient of N as ~10−22 m2/s at 2000 K. The recent more accurate measurement by Schmidt [12] demonstrated that DN and DSi in both modifications are in the same orders of magnitude and DN in α-Si3N4 is ~6 × 10−19 m2/s at ~2000 K. Putting this in the formulae that Wang used, and considering Dv as 2 × 10−18 m2/s, the VSi3N4 is estimated as ~8 at%. Considering these discrepancies, in the present study, we have used molecular dynamics simulation (MD) to investigate the tolerance of both modification of silicon nitride to contain varying content of Si and N vacancies (0–25.6 at%) as well as their tendency to form cluster when heat-treated for long time (114 ns).

Section snippets

Simulation procedure

MD simulation was carried out by QuantumATK (classical forcefield) package [13], with Virtual NanoLab (VNL) for visualization. The forcefield used in this study is Marian-Gastreich two-body potential [14], which is used quite frequently for simulation of silicon nitride ceramics [15], [16], [17], [18]. Furthermore, it was compared recently [19] with other existing forcefields for silicon nitride ceramics and was shown to be the best for reproducing properties of amorphous and crystalline

Results

Fig. 1 shows the lattice of different systems of β-Si3N4 with various contents of defects. Except in 0 and 25.6 systems, in the rest, for better illustration of the cluster vacancy formation, Si atoms with a coordination number of 4 and N atoms with a coordination number of 3 are deleted4. Therefore, the atoms left in these figures are either under-coordinated or over-coordinated. These atoms form

Conclusion

The current results clearly indicate that both α and β are capable of containing a considerable content of Schottky defects (up to 12.8 at%) without lattice destruction, confirming the recalculated data of Wang and co-workers (~8 at%). In both structures, these vacancies form considerably large-size vacancy clusters, although in β the cluster sizes are larger than in α. Introduction of more vacancies (25.6 at%) causes lattice destruction and complete amorphization in β, while in α such vacancy

CRediT authorship contribution statement

Esmaeil Adabifiroozjaei: Conceptualization, Funding acquisition, Data curation, Investigation, Software, Validation, Formal analysis, Writing - original draft, Writing - review & editing. S.S. Mofarah: Visualization, Writing - review & editing, Investigation. H. Ma: Software, Visualization, Writing - review & editing. Y. Jiang: Visualization, Writing - review & editing. M. Hussein N. Assadi: Visualization, Formal analysis, Writing - review & editing. T.S. Suzuki: Funding acquisition, Project

Declaration of Competing Interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Acknowledgment

E.A. acknowledges the financial support (JSPS KAKENHI Grant Number: 18F18064) provided by the Japan Society for the Promotion of Science (JSPS).

Conflict of interest

The authors declare no competing interests.

Data availability statement

All relevant data are available upon request from corresponding authors ([email protected]).

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