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压力对快速过冷锆熔体结晶的影响。

The effect of pressure on the crystallization of rapidly supercooled zirconium melts.

作者信息

Zhang Haitao, Mo Yunfei, Tian Zean, Liu Rangsu, Zhou Lili, Hou Zhaoyang

机构信息

School of Physics and Electronics, Hunan University, Changsha, 410082, China.

出版信息

Phys Chem Chem Phys. 2017 May 17;19(19):12310-12320. doi: 10.1039/c7cp00865a.

Abstract

Molecular dynamics simulations have been performed to explore the effect of pressure (P) on the crystallization of zirconium (Zr) under rapid cooling. The structural evolutions have been analysed in terms of the system energy, the pair distribution function and the largest standard cluster analysis. It was found that at the cooling rate of 1.0 × 10 K s, which can crystallize Zr melts into hcp crystals via the bcc intermediate state under zero pressure, the critical pressure (P) for vitrification is about 28.75 GPa, and the larger the pressure, the higher the glass transition temperature T. At P < P the Ostwald's step rule is applied to Zr melts. Crystallization of rapidly super-cooled Zr melts under pressure always begins with the bcc phase and ends in the hcp crystal; the higher the pressure, the lower the onset temperature (T) of crystallization. Unlike the single-intermediate-state crystallization (SisC) under zero pressure, multiple-intermediate-state crystallization (MisC) is usually observed under pressure. Structural analysis reveals that if nucleation is essentially completed at the end of the first crystalline (bcc-dominated) stage, MisC will occur; otherwise, SisC occurs. The origin of such an observation is also discussed from the effect of pressure upon the thermodynamics and kinetics factors. These findings are useful for comprehensively understanding the solidification of metals under pressure.

摘要

已进行分子动力学模拟,以探究压力(P)对快速冷却下锆(Zr)结晶的影响。已根据系统能量、对分布函数和最大标准团簇分析对结构演变进行了分析。结果发现,在冷却速率为1.0×10 K/s时,在零压力下Zr熔体可通过体心立方中间态结晶为密排六方晶体,玻璃化的临界压力(P)约为28.75 GPa,压力越大,玻璃化转变温度T越高。在P < P时,奥斯特瓦尔德阶跃规则适用于Zr熔体。快速过冷的Zr熔体在压力下的结晶总是始于体心立方相并终止于密排六方晶体;压力越高,结晶起始温度(T)越低。与零压力下的单中间态结晶(SisC)不同,压力下通常观察到多中间态结晶(MisC)。结构分析表明,如果在第一个结晶(以体心立方为主)阶段结束时形核基本完成,就会发生MisC;否则,就会发生SisC。还从压力对热力学和动力学因素的影响方面讨论了这种观察结果的起源。这些发现有助于全面理解压力下金属的凝固过程。

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