Abstract
The microscopic origin of the topological magnon band gap in ferromagnets has been a subject of controversy for years since two main models with distinct characteristics, i.e., Dzyaloshinskii-Moriya (DM) and Kitaev, provided possible explanations with different outcome implications. Here, we investigate the angular magnetic field dependence of the magnon gap of by elucidating what main contributions play a major role in its generation. We implement stochastic atomistic spin-dynamics simulations to compare the impact of these two spin interactions on the magnon spectra. We observe three distinct magnetic field dependencies between these two gap opening mechanisms. First, we demonstrate that the Kitaev-induced magnon gap is influenced by both the direction and amplitude of the applied magnetic field, while the DM-induced gap is solely affected by the magnetic field direction. Second, the position of the Dirac cones within the Kitaev-induced magnon gap shifts in response to changes in the magnetic field direction, whereas they remain unaffected by the magnetic field direction in the DM-induced gap scenario. Third, we find a direct-indirect magnon band gap transition in the Kitaev model by varying the applied magnetic field direction. These differences may distinguish the origin of topological magnon gaps in and other van der Waals magnetic layers. Our findings pave the way for exploration and engineering topological gaps in van der Waals materials.
- Received 15 December 2023
- Revised 8 March 2024
- Accepted 15 April 2024
- Corrected 22 May 2024
DOI:https://doi.org/10.1103/PhysRevB.109.174425
©2024 American Physical Society
Physics Subject Headings (PhySH)
Corrections
22 May 2024
Correction: The second sentence of Sec. V contained an error in wording and has been fixed. The omission of an acknowledgment statement and a support statement in the Acknowledgments have been fixed.