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Paper DOI

A Stable, Recursive Auxiliary Field Quantum Monte Carlo Algorithm in the Canonical Ensemble: Applications to Thermometry and the Hubbard Model

Tong Shen, Hatem Barghathi, Jiangyong Yu, Adrian Del Maestro, Brenda M. Rubenstein

arXiv:2212.08654

Abstract

Many experimentally-accessible, finite-sized interacting quantum systems are most appropriately described by the canonical ensemble of statistical mechanics. Conventional numerical simulation methods either approximate them as being coupled to a particle bath, or use projective algorithms which may suffer from non-optimal scaling with system size or large algorithmic prefactors. In this paper, we introduce a highly stable, recursive Auxiliary Field Quantum Monte Carlo approach that can directly simulate systems in the canonical ensemble. We apply the method to the fermionic Hubbard model in one and two spatial dimensions in a regime known to exhibit a significant "sign" problem and find improved performance over existing approaches including rapid convergence to ground state expectation values. The effects of excitations above the ground state are quantified using an estimator-agnostic approach including studying the temperature dependence of the purity and overlap fidelity of the canonical and grand canonical density matrices. As an important application, we show that thermometry approaches often exploited in ultra-cold atoms that employ an analysis of the velocity distribution in the grand canonical ensemble may be subject to errors leading to an under-estimation of extracted temperatures with respect to the Fermi temperature.

Description

This repository includes links, code, scripts, and data to generate the figures in a paper.

Requirements

The data in this project was generated via a new auxiliary-field quantum Monte Carlo algorithm in the canonical ensemble: CanEnsAFQMC. Everything included in the data directory was processed from the raw data on Zenodo DOI.

Script dependencies are listed in a Project.toml file.

Support

The creation of these materials was supported in part by the NSF CTMC CAREER Award 2046744 and the NSF under Grant No. DMR-2041995.

Figures

Figure 01: Stability of Different Approaches to Computing a Non-Interacting Fermionic Partition Function

Figure 02: Runtime Comparison Between Projection and APF Method

Figure 03: Energy Comparison Between Ensembles

Figure 04: Purity Comparison Between Ensembles

Figure 05: Fidelity Demonstrating Convergence to the Ground State

Figure 06: Fermionic Sign Conmparison Between Ensembles

Figure 07: Comparison of Charge Structure Factors