# Ab Initio Path Integral Monte Carlo Approach to the Static and Dynamic   Density Response of the Uniform Electron Gas

**Authors:** Simon Groth, Tobias Dornheim, Jan Vorberger

arXiv: 1903.11970 · 2019-06-19

## TL;DR

This paper introduces a new ab initio path integral Monte Carlo method to accurately compute the static and dynamic density response functions of the uniform electron gas, providing insights relevant for warm dense matter and correlated electron systems.

## Contribution

The paper details a novel reconstruction method for the dynamic local field correction from PIMC data and thoroughly investigates related correlation functions, expanding the understanding of electron gas responses.

## Key findings

- Accurate dynamic structure factors for various densities and temperatures.
- Comparison of static response functions with dielectric theories.
- New insights into the high-frequency behavior of the local field correction.

## Abstract

In a recent Letter [T. Dornheim et al., Phys. Rev. Lett. 121, 255001 (2018)] we have presented the first ab initio results for the dynamic structure factor $S(\mathbf{q},\omega)$ of the uniform electron gas for conditions ranging from the warm dense matter regime to the strongly correlated electron liquid. This was achieved on the basis of exact path integral Monte Carlo data by stochastically sampling the dynamic local field correction $G(\mathbf{q},\omega)$. In this paper, we introduce in detail this new reconstruction method and provide several practical demonstrations. Moreover, we thoroughly investigate the associated imaginary-time density--density correlation function $F(\mathbf{q},\tau)$. The latter also gives us access to the static density-response function $\chi(\mathbf{q})$ and static local field correction $G(\mathbf{q})$, which are compared to standard dielectric theories like the widespread random phase approximation. In addition, we study the high-frequency limit of $G(\mathbf{q},\omega)$ and provide extensive new results for the dynamic structure factor for different densities and temperatures. Finally, we discuss the implications of our findings for warm dense matter research and the interpretation of experiments.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1903.11970/full.md

## Figures

37 figures with captions in the complete paper: https://tomesphere.com/paper/1903.11970/full.md

## References

134 references — full list in the complete paper: https://tomesphere.com/paper/1903.11970/full.md

---
Source: https://tomesphere.com/paper/1903.11970