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通过第一性原理超晶胞方法研究了氧(O)原子在体心立方(BCC)难熔金属Nb,Ta,Mo,W中不同间隙位置的占位稳定性和原子结构以及电子结构.杂质形成能结果表明,O原子占据在Nb,Ta的八面体间隙最稳定;与之相反,O原子占据在Mo,W的四面体间隙位置最稳定.进一步的,O原子在BCC难熔金属的杂质形成能由低到高的顺序为Nb<Ta<Mo<W,这表明金属中溶解氧容易顺序为Nb>Ta>Mo>W.此外,分析了O对难熔金属Nb,Ta,Mo,W原子结构的影响.利用电子结构态密度解释了氧原子在Nb,Ta八面体间隙和Mo,W四面体间隙的最稳定性原因.

参考文献

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