Giant orbital magnetization in two-dimensional materials
Martin Ovesen, Thomas Olsen
TL;DR
This paper clarifies how unquenched orbital magnetization can arise in two-dimensional transition-metal compounds through a synergy of crystal-field splitting, spin-orbit coupling, and electronic correlations. It shows that a self-consistent treatment of SOC combined with a Hubbard correction is required to obtain correct orbital polarization and large magnetic anisotropy, particularly for partially filled $t_{2g}$ bands in octahedral or tetrahedral environments. By screening the C2DB, the authors identify dozens of monolayers with potentially giant orbital moments, significantly expanding known examples beyond FePS$_3$ and VI$_3$ and highlighting the impact on 2D magnetism and Néel temperature predictions. The work provides a practical framework for predicting and understanding orbital contributions to magnetism in 2D materials, with implications for designing high-temperature 2D magnets and anisotropy-driven spintronics.
Abstract
Orbital magnetization typically plays a minor role in compounds where the magnetic properties are governed by transition metal elements. However, in some cases, the orbital magnetization may be fully unquenched, which can have dramatic consequences for magnetic anisotropy and various magnetic response properties. In the present work, we start by summarizing how unquenched orbital moments arise from particular combinations of crystal field splitting and orbital filling. We exemplify this for the cases of two-dimensional (2D) VI$_3$ and FePS$_3$, and show that Hubbard corrections as well as self-consistent spin-orbit coupling are crucial ingredients for predicting correct orbital moments from first principles calculations. We then search the Computational 2D Materials Database (C2DB) for monolayers having tetrahedral or octahedral crystal field splitting of transition metal $d$-states and orbital occupancy that is expected to lead to large orbital moments. We identify 112 monolayers with octahedral crystal field splitting and 62 monolayers with tetrahedral crystal field splitting and for materials with partially filled $t_{2g}$ bands, we verify that inclusion of Hubbard corrections as well as self-consistent spin-orbit coupling typically increases the magnitude of predicted orbital moments by an order of magnitude.
