English

Origin of G-type Antiferromagnetism and Orbital-Spin Structures in ${\rm LaTiO}_3$

Strongly Correlated Electrons 2009-09-25 v1

Abstract

The possibility of the D3dD_{3d} distortion of TiO6{\rm TiO}_6 octahedra is examined theoretically in order to understand the origin of the G-type antiferromagnetism (AFM(G)) and experimentally observed puzzling properties of LaTiO3{\rm LaTiO}_3. 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 t2gt_{2g}-orbital degeneracy accompanied by a tiny D3dD_{3d}-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