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

preprint2022arXivOpen access

Abstract

We develop finite temperature strong coupling expansions for the SU(N) Hubbard Model in powers of βtβt, w=exp⁡(−βU)w=\exp{(-βU)} and 1βU{1\over βU} 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 w→0w\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 w→0w\to 0 limit corresponds to an effective t−Jt-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=1−nδ=1-n, the deviation from one particle per site, where the leading βtβt 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.

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