Range of biquadratic and triquadratic Heisenberg effective couplings deduced from multiorbital Hubbard models

TL;DR

This study derives bounds on higher-order Heisenberg couplings from multiorbital Hubbard models, showing that biquadratic and triquadratic interactions are limited in strength, which constrains effective spin models for correlated materials.

Contribution

It provides a systematic analysis of how multiorbital Hubbard parameters influence higher-order spin couplings, establishing quantitative bounds on their ratios.

Findings

J2/J1 < 0.4, J3/J1 < 0.2, indicating limited higher-order couplings.

Mapping Hubbard models to effective Heisenberg models with specific multi-spin interactions.

Results guide the construction of realistic effective spin models for strongly correlated systems.

Abstract

We studied a multi-orbital Hubbard model at half-filling for two and three orbitals per site on a two-site cluster via full exact diagonalization, in a wide range for the onsite repulsion $U$, from weak to strong coupling, and multiple ratios of the Hund coupling $J_H$ to $U$. The hopping matrix elements among the orbitals were also varied extensively. At intermediate and large $U$, we mapped the results into a Heisenberg model. For two orbitals per site, the mapping is into a $S=1$ Heisenberg model where by symmetry both nearest-neighbor $(\mathbf{S}_{i}\cdot\mathbf{S}_{j})$ and $(\mathbf{S}_{i}\cdot\mathbf{S}_{j})^{2}$ are allowed, with respective couplings $J_1$ and $J_2$. For the case of three orbitals per site, the mappping is into a $S=3/2$ Heisenberg model with $(\mathbf{S}_{i}\cdot\mathbf{S}_{j})$, $(\mathbf{S}_{i}\cdot\mathbf{S}_{j})^{2}$, and $(\mathbf{S}_{i}\cdot\mathbf{S}_{j})^{3}$ terms, and respective couplings $J_1$, $J_2$, and $J_3$. The strength of these coupling constants in the Heisenberg models depend on the $U$, $J_H$, and hopping amplitudes of the underlying Hubbard model. Our study allows to establish bounds on how large the ratios $J_2/J_1$ and $J_3/J_1$ can be. We show that those ratios are severely limited and, as a crude guidance, we conclude that $J_2/J_1$ is less than 0.4 and $J_3/J_1$ is less than 0.2, establishing bounds on effective models for strongly correlated Hubbard systems.