Polarization-dependent magnetic properties of periodically driven -RuCl
arXiv:2112.04690 · doi:10.1103/PhysRevB.104.214413
Abstract
We study magnetic properties of a periodically driven Mott insulator with strong spin-orbit coupling and show some properties characteristic of linearly polarized light. We consider a -orbital Hubbard model driven by circularly or linearly polarized light with strong spin-orbit coupling and derive its effective Hamiltonian in the strong-interaction limit for a high-frequency case. We show that linearly polarized light can change not only the magnitudes and signs of the exchange interactions, but also their bond anisotropy even without the bond-anisotropic hopping integrals. Because of this property, the honeycomb-network spin system could be transformed into weakly coupled zigzag or step spin chains for the light field polarized along the - or -axis, respectively. Then, analyzing how the light fields affect several magnetic states in a mean-field approximation, we show that linearly polarized light can change the relative stability of the competing magnetic states, whereas such a change is absent for circularly polarized light. We also analyze the effects of both the bond anisotropy of nearest-neighbor hopping integrals and a third-neighbor hopping integral on the magnetic states and show that the results obtained in a simple model, in which the bond-averaged nearest-neighbor hopping integrals are considered, remain qualitatively unchanged except for the stability of zigzag states in the non-driven case and the degeneracy lifting of the zigzag or stripy states.
24 pages, 15 figures, 1 table; published
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Cited by in corpus (5)
- Symmetry analysis of light-induced magnetic interactions via Floquet engineering
- Symmetry-protected difference between spin Hall and anomalous Hall effects of a periodically driven multiorbital metal
- From linear to circular polarized light -- Floquet engineering in Kitaev-Heisenberg materials with Lissajous figures
- Scalar spin chirality induced by a circularly polarized electric field in a classical kagome magnet
- Photoinduced Pseudospin Polarization in a Three-Orbital Hubbard Model