A closer look at how symmetry constraints and the spin-orbit coupling shape the electronic structure of Bi(111)
Marisol Alcantara-Ortigoza, Talat S. Rahman

TL;DR
This study uses relativistic density-functional theory to analyze Bi(111) thin films, revealing that surface state splitting is due to spin-orbit coupling effects rather than inversion asymmetry, and clarifies the nature of their spin textures.
Contribution
It provides a detailed theoretical analysis of the electronic structure of Bi(111), challenging previous interpretations of surface state splitting and spin textures, and demonstrates how structural perturbations induce Rashba effects.
Findings
9-nm films suffice to model bulk Bi(111)
Surface state splitting is due to spin-orbit coupling, not inversion asymmetry
Rashba effect can be induced by structural perturbations
Abstract
Relativistic density-functional-theory calculations of Bi(111) thin films are performed to revisit their band structure and that of macroscopic samples. The band structure of a our 39-bilayer film (~15~nm) shows that (1) 9-nm films are enough to describe that of Bi(111), (2) The two split surface-state metallic branches along the direction do not overlap with the bulk band at the zone boundary but lie within the A7-distortion-induced conduction-valence band gap, and (3) Neither the existence of the metallic surface states nor their observed splitting is related to inversion \emph{asymmetry}. Thus, the spin texture observed in such states is not caused by the lifting of the Kramers degeneracy and their splitting is not of the Rashba-type. We instead propose that (1) the large splitting of the metallic branches is a - splitting and…
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Taxonomy
TopicsPhysics of Superconductivity and Magnetism · Magnetic properties of thin films · Topological Materials and Phenomena
