Revisited precipitation process in dilute Mg-Ca-Zn alloys

被引:14
|
作者
Li, Z. H. [1 ,2 ]
Cheng, D. [3 ]
Wang, K. [3 ]
Hoglund, E. R. [3 ]
Howe, J. M. [3 ]
Zhouc, B. C. [3 ]
Sasaki, T. T. [1 ,4 ]
Ohkubo, T. [1 ]
Hono, K. [1 ,2 ]
机构
[1] Natl Inst Mat Sci, 1-2-1 Sengen, Tsukuba 3050047, Japan
[2] Univ Tsukuba, Grad Sch Pure & Appl Sci, Tsukuba 3058577, Japan
[3] Univ Virginia, Dept Mat Sci & Engn, Charlottesville, VA 22904 USA
[4] Kyoto Univ, Ctr Elements Strategy Initiat Struct Mat ESISM, Yoshida Honmachi, Kyoto 6068501, Japan
基金
美国国家科学基金会;
关键词
Magnesium alloys; Precipitation; HAADF-STEM; 3DAP; First-principles calculation; TOTAL-ENERGY CALCULATIONS; CRYSTAL-STRUCTURE; GD-ZN; MAGNESIUM ALLOYS; PHASE; 1ST-PRINCIPLES; STABILIZATION; STABILITY; STRENGTH; GAMMA'';
D O I
10.1016/j.actamat.2023.119072
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
To obtain thorough understandings of precipitation process in heat-treatable Mg-Ca-Zn alloy, we revisited the precipitation process of a Mg-0.3Ca-0.6 Zn (at.%) dilute alloy during isothermal aging at 200 degrees C using an aberration-corrected scanning transmission electron microscope, atom probe tomography, and first-principles calculations. The monolayer G.P. zones form on the (0002)& alpha; plane in the peak-aged condition and transform into tri-atomic layer & eta;'' and & eta;' plates with a thickness of a single unit-cell height. The & eta;' plates, then, form in pairs and stacks with energetically favorable 4-5 atomic layers of pure magnesium between the plates. While such a transformation path is similar to that seen in Mg-RE-Zn alloys (RE: rare-earth elements), the unique structure of coarse & eta;1 plates that precipitate after the & eta;' plates leads to a different precipitate microstructure evolution from the Mg-RE-Zn system. The & eta;1 phase (Mg7Ca2Zn3) is unevenly distributed in the matrix after 100 h of aging and finally evolves to the equilibrium & eta; phase (Mg10Ca3Zn6) phase with a hexagonal structure. First-principles calculations of energetics were performed to further identify the crystal structure and stability of the precipitates, supporting the following new precipitation sequence: S.S.S.S. & RARR; G.P. zones & RARR; & eta;'' & RARR; & eta;' & RARR; & eta;' pairs and stacks / & eta;1 & RARR; & eta;
引用
收藏
页数:15
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