Abstract
Numerical results for ground-state and excited-state properties (energies, double occupancies, and Matsubara-axis self-energies) of the single-orbital Hubbard model on a two-dimensional square lattice are presented, in order to provide an assessment of our ability to compute accurate results in the thermodynamic limit. Many methods are employed, including auxiliary-field quantum Monte Carlo, bare and bold-line diagrammatic Monte Carlo, method of dual fermions, density matrix embedding theory, density matrix renormalization group, dynamical cluster approximation, diffusion Monte Carlo within a fixed-node approximation, unrestricted coupled cluster theory, and multireference projected Hartree-Fock methods. Comparison of results obtained by different methods allows for the identification of uncertainties and systematic errors. The importance of extrapolation to converged thermodynamic-limit values is emphasized. Cases where agreement between different methods is obtained establish benchmark results that may be useful in the validation of new approaches and the improvement of existing methods.
10 More- Received 9 May 2015
DOI:https://doi.org/10.1103/PhysRevX.5.041041
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Published by the American Physical Society
Popular Summary
The two-dimensional Hubbard model is one of the simplest models for interacting fermions: Its Hamiltonian consists of a single band of electrons. The potential energy contribution is modeled by an on-site interaction, and the kinetic energy contribution is modeled by nearest-neighbor and next-nearest-neighbor hopping terms. This Hamiltonian is believed to model the low-energy behavior of cuprate superconductors, and it can be emulated using ultracold fermionic gases. In two dimensions, no analytical solutions to this Hamiltonian are known beyond the perturbative limit, despite the simplicity of the Hamiltonian, and solutions derived from numerical methods have proven to be challenging. Here, we present numerical solutions obtained from a wide range of numerical methods, for widely different parts of phase space of the model, in the thermodynamic limit.
We consider a Hubbard model defined on a two-dimensional square lattice, and we calculate the properties of systems with many interacting electrons using different numerical methods and considering strong, intermediate, and weak on-site repulsion. We pay particular attention to the estimation of the errors introduced by approximations employed by the different methods, and we systematically control these errors wherever possible. We find that errors arise from extrapolating to a thermodynamic limit and that some models diverge in the regime of intermediate coupling. The resulting data yield a summary of the state of the art of the field and delineate areas of parameter space of the model that are known very well and areas where additional improvement is necessary.
Our results constitute a stringent set of reference (i.e., benchmark) data with which future results from numerical methods can be compared and tested.