The effect of relativity on stability of Copernicium phases, their electronic structure and mechanical properties
Hana \v{C}en\v{c}arikov\'a, Dominik Legut

TL;DR
This study uses first-principles calculations to explore how relativistic effects influence the stability, electronic structure, and mechanical properties of Copernicium's various crystalline phases, highlighting the importance of spin-orbit coupling.
Contribution
It provides a detailed analysis of relativistic effects on Copernicium's phase stability and mechanical properties, emphasizing the role of spin-orbit interaction in stabilizing the bcc structure.
Findings
Spin-orbit coupling stabilizes the bcc phase.
fcc and rh structures are mechanically unstable.
Pressure induces a transition between sc and bcc phases.
Abstract
The phase stability of the various crystalline structures of the super-heavy element Copernicium was determined based on the first-principles calculations with different levels of the relativistic effects. We utilized the Darwin term, mass-velocity, and spin-orbit interaction with the single electron framework of the density functional theory while treating the exchange and correlation effects using local density approximations. It is found that the spin-orbit coupling is the key component to stabilize the body-centered cubic () structure over the hexagonal closed packed () structure, which is in accord with Sol. Stat. Comm. 152 (2012) 530, but in contrast to Sol. Stat. Comm. 201 (2015) 88, Angew. Chem. 46 (2007) 1663, Handbook of Elemental Solids Z=104-112 (Springer 2015). It seems that the main role here is the correct description of the semi-core relativistic …
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