Effect of spin-orbit coupling on the ground state structure of mercury

被引:5
|
作者
Mishra, Vinayak [1 ]
Gyanchandani, Jyoti [2 ]
Chaturvedi, Shashank [1 ]
Sikka, S. K. [3 ]
机构
[1] Bhabha Atom Res Ctr, Computat Anal Div, Visakhapatnam 530012, Andhra Pradesh, India
[2] Bhabha Atom Res Ctr, Div Mat Sci, Bombay 400085, Maharashtra, India
[3] Govt India, Off Principle Sci Adviser, New Delhi 110011, India
关键词
Metals; Crystal structure and symmetry; Spin-orbit effects; Phase transitions; PHASE-STABILITY; PRESSURE; EXCHANGE; EQUATION; ZN; CD; HG;
D O I
10.1016/j.ssc.2014.01.025
中图分类号
O469 [凝聚态物理学];
学科分类号
070205 ;
摘要
Near zero kelvin ground state structure of mercury is the body centered tetragonal (BCT) structure (beta Hg). However, in all previously reported density functional theory (OFT) calculations, either the rhombohedral or the HCP structure has been found to be the ground state structure. Based on the previous calculations it was predicted that the correct treatment of the SO effects would improve the result. We have performed FPLAPW calculations, with and without inclusion of the SO coupling, for determining the ground state structure. These calculations determine rhombohedral structure as the ground state structure instead of BCT structure. The calculations, without inclusion of SO effect, predict that the energies of rhomboheclral and BCT structures are very close to each other but the energy of rhomboheclral structure is lower than that of BCT structure at ambient as well as high pressure. On the contrary, the SO calculations predict that though at ambient conditions the rhomboheclral structure is the stable structure but on applying a pressure of 3.2 GPa, the BCT structure becomes stable. Hence, instead of predicting the stability of BCT structure at zero pressure, the SO calculations predict its stability at 3.2 GPa. This small disagreement is expected when the energy differences between the structures are small. (C) 2014 Elsevier Ltd. All rights reserved.
引用
收藏
页码:38 / 41
页数:4
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