Origin of G-type Antiferromagnetism and Orbital-Spin Structures in ${\rm LaTiO}_3$
Abstract
The possibility of the distortion of octahedra is examined theoretically in order to understand the origin of the G-type antiferromagnetism (AFM(G)) and experimentally observed puzzling properties of . By utilizing an effective spin and pseudospin Hamiltonian with the strong Coulomb repulsion, it is shown that AFM(G) state is stabilized through the lift of the -orbital degeneracy accompanied by a tiny -distortion . The estimated spin-exchange interaction is in agreement with that obtained by the neutron scattering. Moreover, the level-splitting energy due to the distortion can be considerably larger than the spin-orbit interaction even when the distortion becomes smaller than the detectable limit under the available experimental resolution. This suggests that the orbital momentum is fully quenched and the relativistic spin-orbit interaction is not effective in this system, in agreement with recent neutron-scattering experiment.
Keywords
Cite
@article{arxiv.cond-mat/0105135,
title = {Origin of G-type Antiferromagnetism and Orbital-Spin Structures in ${\rm LaTiO}_3$},
author = {Masahito Mochizuki and Masatoshi Imada},
journal= {arXiv preprint arXiv:cond-mat/0105135},
year = {2009}
}
Comments
9 pages, 6 figures