Cazorla C, Gillan M J, Taioli S, Alfè D
Department of Physics and Astronomy, London Centre for Nanotechnology, UCL, London WC1H OAH, United Kingdom.
J Chem Phys. 2007 May 21;126(19):194502. doi: 10.1063/1.2735324.
Ab initio calculations of the melting curve of molybdenum for the pressure range 0-400 GPa are reported. The calculations employ density functional theory (DFT) with the Perdew-Burke-Ernzerhof exchange-correlation functional in the projector augmented wave (PAW) implementation. Tests are presented showing that these techniques accurately reproduce experimental data on low-temperature body-centered cubic (bcc) Mo, and that PAW agrees closely with results from the full-potential linearized augmented plane-wave implementation. The work attempts to overcome the uncertainties inherent in earlier DFT calculations of the melting curve of Mo, by using the "reference coexistence" technique to determine the melting curve. In this technique, an empirical reference model (here, the embedded-atom model) is accurately fitted to DFT molecular dynamics data on the liquid and the high-temperature solid, the melting curve of the reference model is determined by simulations of coexisting solid and liquid, and the ab initio melting curve is obtained by applying free-energy corrections. The calculated melting curve agrees well with experiment at ambient pressure and is consistent with shock data at high pressure, but does not agree with the high-pressure melting curve deduced from static compression experiments. Calculated results for the radial distribution function show that the short-range atomic order of the liquid is very similar to that of the high-T solid, with a slight decrease of coordination number on passing from solid to liquid. The electronic densities of states in the two phases show only small differences. The results do not support a recent theory according to which very low dT(m)dP values are expected for bcc transition metals because of electron redistribution between s-p and d states.
本文报道了在0-400 GPa压力范围内钼熔化曲线的从头算计算结果。计算采用密度泛函理论(DFT),并在投影增强波(PAW)方法中使用了Perdew-Burke-Ernzerhof交换关联泛函。文中给出的测试表明,这些技术能够准确再现低温体心立方(bcc)结构钼的实验数据,并且PAW方法的结果与全势线性缀加平面波方法的结果非常接近。这项工作试图通过使用“参考共存”技术来确定熔化曲线,以克服早期DFT计算钼熔化曲线时固有的不确定性。在该技术中,将一个经验参考模型(这里是嵌入原子模型)精确拟合到关于液体和高温固体的DFT分子动力学数据上,通过共存固体和液体的模拟确定参考模型的熔化曲线,并通过应用自由能校正获得从头算熔化曲线。计算得到的熔化曲线在常压下与实验结果吻合良好,在高压下与冲击数据一致,但与静态压缩实验推导的高压熔化曲线不一致。径向分布函数的计算结果表明,液体的短程原子序与高温固体非常相似,从固体转变为液体时配位数略有降低。两相的电子态密度仅显示出微小差异。结果不支持最近的一种理论,该理论认为由于s-p和d态之间的电子重新分布,bcc结构的过渡金属预期具有非常低的dT(m)dP值。