Abstract
A recent theoretical study has shown that hexagonal is dynamically unstable and distorts into a stable orthorhombic structure. In this paper, we show theoretically that the orthorhombic phase is energetically more stable than the hexagonal phase in the low-temperature region, while the phonon entropy stabilizes the hexagonal phase thermodynamically in the high-temperature region. The orthorhombic-to-hexagonal phase transition temperature is K, which is determined using self-consistent phonon calculations. We investigate the magnetocrystalline anisotropy energy (MAE) using self-consistent and non-self-consistent (force theorem) calculations with spin-orbit interaction (SOI) along with the Hubbard correction. Then, we find that the orthorhombic phase has MAE, orbital moment, and orbital moment anisotropy values that are similar to those of the hexagonal phase when the self-consistent calculation with SOI is performed. Since the orthorhombic phase still gives magnetic properties comparable to those found in experiments, the orthorhombic distortion is potentially realized in the low-temperature region, which awaits experimental exploration.
- Received 6 January 2023
- Accepted 10 July 2023
DOI:https://doi.org/10.1103/PhysRevB.108.014304
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