Ab initio determination of magnetic ground state of pyrochlore YMnO
arXiv:2006.15002 · doi:10.1103/PhysRevB.102.125105
Abstract
There are two discrepant experimental results on the magnetic ground state of YMnO, one study proposes a spin glass state, while another introduces the material as a ferromagnet. In this study, we attempt to resolve this issue by employing density functional theory and Monte Carlo simulations. We derive different spin models by varying the Hubbard parameter in ab initio GGA+ calculations. For the most range of Hubbard , We obtain that the leading terms in the spin Hamiltonian are bi-quadratic and the nearest neighbor Heisenberg exchange interactions. By comparing Monte Carlo simulations of these models with the experiments, we find a ferromagnetic ground state for YMnO as the most compatible with experiments. We also consider YMoO as a prototype of the defect-free pyrochlore system with spin-glass behavior and compare it with YMnO. The orbital degrees of freedom are considered as a leading factor in converting a defect-free pyrochlore such as YMnO to a spin glass system. By changing the orbital occupations of Mo atoms, our GGA+ calculations for YMoO indicate many nearly degenerate states with different orbital orientations which reveals orbital degrees of freedom in this material. While for YMnO, we find a single ground state with a fixed orbital orientation. Consequently, all of our ab initio approaches confirm YMnO as a ferromagnetic system.
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