English

Incommensurate spin density wave as a signature of spin-orbit coupling

Strongly Correlated Electrons 2016-12-28 v1

Abstract

Close to half filling and in the limit of strong interactions the Hubbard model leads a spin Hamiltonian. In its original isotropic form this is the Heisenberg model with antiferromagnetic coupling JJ. On a square lattice there is no frustration and the ground state is a classical antiferromagnet denoted by the commensurate order vector Q=(π,π){\bf Q}=(\pi,\pi). In this work we show that the inclusion of spin orbit coupling (SOC) in the fermionic Hubbard model on a square lattice leads to an incommensurate spin density wave (ISDW) in the strong interactions limit at half filling. In this limit the Hubbard model leads to a non-diagonal and anisotropic spin Hamiltonian which exhibits the incommensurate spin order as its classical ground state. We note that an ISDW can be found in systems regardless of spin orbit-coupling due to nesting and lattice distortion. These effects, however, can usually be recognized by experimental probes.

Keywords

Cite

@article{arxiv.1402.4093,
  title  = {Incommensurate spin density wave as a signature of spin-orbit coupling},
  author = {Aaron Farrell and P. -K. Wu and Y. -J. Kao and T. Pereg-Barnea},
  journal= {arXiv preprint arXiv:1402.4093},
  year   = {2016}
}

Comments

Main Text: 5 pages, 3 figures. Supplementary material: 3 pages, 2 figures