Universal thermodynamics of an SU($N$) Fermi-Hubbard Model

Abstract

The SU(2) symmetric Fermi-Hubbard model (FHM) plays an essential role in strongly correlated fermionic many-body systems. In the one particle per site and strongly interacting limit U/t 1, it is effectively described by the Heisenberg Hamiltonian. In this limit, enlarging the spin and extending the typical SU(2) symmetry to SU(N ) has been predicted to give exotic phases of matter in the ground state, with a complicated dependence on N . This raises the question of what -if any -are the finite-temperature signatures of these phases, especially in the currently experimentally relevant regime near or above the superexchange energy. We explore this question for thermodynamic observables by numerically calculating the thermodynamics of the SU(N ) FHM in the two-dimensional square lattice near densities of one particle per site, using determinant Quantum Monte Carlo and Numerical Linked Cluster Expansion. Interestingly, we find that for temperatures above the superexchange energy, where the correlation length is short, the energy, number of on-site pairs, and kinetic energy are universal functions of N . Although the physics in the regime studied is well beyond what can be captured by low-order high-temperature series, we show that an analytic description of the scaling is possible in terms of only one-and two-site calculations.

Projection of Infinite-$U$ Hubbard Model and Algebraic Sign Structure

“…While numerical methods may provide important hints [14,17], disputes still exist on questions such as which phase is the true ground state of large-U SU (N ) Hubbard model on several lattices [18][19][20][21][22]. Recently large-U SU (N ) Hubbard model are getting more and more attention in ultracold atom simulations [23][24][25][26][27][28][29][30].…”