# Mitigating the Sign Problem Through Basis Rotations

**Authors:** Ryan Levy, Bryan K. Clark

arXiv: 1907.02076 · 2021-06-02

## TL;DR

This paper introduces a method to optimize the basis in quantum Monte Carlo simulations to mitigate the Fermion sign problem, significantly improving simulation efficiency for large two-dimensional Hubbard systems.

## Contribution

The authors demonstrate how to use sign-free quantum Monte Carlo to optimize basis rotations, reducing the sign problem and accelerating simulations of large 2D Hubbard models.

## Key findings

- Optimized basis rotations improve the average sign in Hubbard models.
- Sign problem reduction leads to exponential speedup in simulations.
- Method applicable across various U and density parameters.

## Abstract

Quantum Monte Carlo simulations of quantum many body systems are plagued by the Fermion sign problem. The computational complexity of simulating Fermions scales exponentially in the projection time $\beta$ and system size. The sign problem is basis dependent and an improved basis, for fixed errors, lead to exponentially quicker simulations. We show how to use sign-free quantum Monte Carlo simulations to optimize over the choice of basis on large two-dimensional systems. We numerically illustrate these techniques decreasing the `badness' of the sign problem by optimizing over single-particle basis rotations on one and two-dimensional Hubbard systems. We find a generic rotation which improves the average sign of the Hubbard model for a wide range of $U$ and densities for $L \times 4$ systems. In one example improvement, the average sign (and hence simulation cost at fixed accuracy) for the $16\times 4$ Hubbard model at $U/t=4$ and $n=0.75$ increases by $\exp\left[8.64(6)\beta\right]$. For typical projection times of $\beta\gtrapprox 100$, this accelerates such simulation by many orders of magnitude.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/1907.02076/full.md

## References

39 references — full list in the complete paper: https://tomesphere.com/paper/1907.02076/full.md

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Source: https://tomesphere.com/paper/1907.02076