Relativistic Effects in LaBi$_2$ Thin Films
Reiley Dorrian, Sungmin Song, Jinwoong Kim, Mizuki Ohno, Seung-Hoon Jhi, Nicholas Kioussis, Joseph Falson
TL;DR
The study addresses how strong spin-orbit coupling (SOC) shapes growth, structure, and electronic transport in LaBi$_2$ thin films within the LaPn$_2$ square-net family. It combines layer-by-layer MBE growth on MgO(001) with extensive structural, transport, and first-principles analyses (SOC-inclusive DFT, Wannier90/EPW, Boltzmann transport) to link band-structure modifications to reduced phonon scattering and improved growth. The key findings are that LaBi$_2$ stabilizes in a monoclinic Yb-monoclinic stacking, supports intrinsic superconductivity at $T_c \approx 0.55$ K, and exhibits higher metallicity than LaSb$_2$ due to SOC-induced band shifts and lower surface energy. This work shows SOC as a tunable parameter for thin-film growth and electronic properties in pnictide intermetallics, with implications for surface engineering and superconductivity in related materials.
Abstract
Chemical substitution in crystalline quantum materials is a powerful way to explore the consequences of strong spin-orbit coupling on their structural and electronic properties. In this work, we present an investigation of thin films of the La$\textit{Pn}_2$ ($\textit{Pn}$~=~Sb, Bi) class of layered square-net intermetallics. We report the growth of LaBi$_2$ with a pristine layer-by-layer growth mode, classifying it as a good metal displaying superconductivity at $\sim$0.55~K. Compared to LaSb$_2$, we attribute the enhanced metallic behavior and improved growth dynamics of LaBi$_2$ to significant relativistic corrections to its electronic band structure and the resulting impact on both surface energy and intrinsic phonon scattering.
