English

Finite Temperature Strong Coupling Expansions for the SU(N) Hubbard Model

Strongly Correlated Electrons 2022-08-04 v2

Abstract

We develop finite temperature strong coupling expansions for the SU(N) Hubbard Model in powers of βt\beta t, w=exp(βU)w=\exp{(-\beta U)} and 1βU{1\over \beta U} for arbitrary filling. The expansions are done in the grand canonical ensemble and are most useful at a density of one particle per site, where for UU larger than or of order the Bandwidth, the expansions converge over a wide temperature range t2/U  T  10Ut^2/U \ \lesssim \ T \ \lesssim \ 10 U. By taking the limit w0w\to 0, valid at temperatures much less than UU, the expansions turn into a high temperature expansion for a dressed SU(N) Heisenberg model that includes nearest-neighbor exchange, further neighbor exchanges and ring exchanges known from the T=0T=0 perturbation theory of the SU(2) Hubbard model. Below a filling of one particle per site, the w0w\to 0 limit corresponds to an effective tJt-J model. The onset of strong correlations can be identified by a plateau-like behavior in the entropy as a function of temperature. At small deviations from one particle per site, the expansions can be arranged in powers of a small parameter δ=1n\delta=1-n, the deviation from one particle per site, where the leading βt\beta t dependent terms correspond to holes sloshing around in a disordered SU(N) background. We use these expansions to calculate the thermodynamic properties of the model at moderate and high temperatures over a wide parameter range.

Keywords

Cite

@article{arxiv.2201.06677,
  title  = {Finite Temperature Strong Coupling Expansions for the SU(N) Hubbard Model},
  author = {Rajiv R. P. Singh and Jaan Oitmaa},
  journal= {arXiv preprint arXiv:2201.06677},
  year   = {2022}
}

Comments

8 pages 7 figures

R2 v1 2026-06-24T08:52:58.458Z