Non-linear extension of the dynamical linear response of spins; extended Heisenberg model
arXiv:2105.03035 · doi:10.7566/JPSJ.90.094710
Abstract
We introduce a new extended Heisenberg model. The model contains the orbital-dependent spins together with the retarded effects of spin torque. The model is directly derived from the dynamical linear response functions on the transversal spin fluctuation. Our model allows us to address effects which are not accessible via the usual Heisenberg model. With the model, we can describe not only the relaxation effects due to the Landau damping caused by the Stoner excitations, but also the nesting effects of the Fermi surface. We discuss possibilities of the extended Heisenberg model based on the high-resolution plots of the spin susceptibility for Fe.
References in corpus (5)
- Spin wave dispersion based on the quasiparticle self-consistent method: NiO, MnO and -MnAs
- Quasiparticle self-consistent GW method based on the augmented plane-wave and muffin-tin orbital method
- Intersublattice magnetocrystalline anisotropy using a realistic tight-binding method based on maximally localized Wannier functions
- Formulation of the augmented plane-wave and muffin-tin orbital method
- Fast acquisition of spin-wave dispersion by compressed sensing