# Fermi surface reconstruction by a charge-density-wave with finite   correlation length

**Authors:** Yuval Gannot, Brad J. Ramshaw, and Steven A. Kivelson

arXiv: 1905.03261 · 2019-07-31

## TL;DR

This paper studies how finite correlation length in charge-density-waves affects Fermi surface reconstruction and quantum oscillations, with implications for understanding cuprate superconductors.

## Contribution

It introduces an effective Dingle factor considering finite correlation length and analyzes its impact on Fermi surface reconstruction in cuprates.

## Key findings

- Finite correlation length suppresses quantum oscillations exponentially.
- Bidirectional CDW correlation lengths are too short to explain observed reconstructions.
- Unidirectional CDW correlation lengths are sufficient for Fermi surface reconstruction.

## Abstract

Even a small amplitude charge-density-wave (CDW) can reconstruct a Fermi surface, giving rise to new quantum oscillation frequencies. Here, we investigate quantum oscillations when the CDW has a finite correlation length $\xi$ -- a case relevant to the hole-doped cuprates. By considering the Berry phase induced by a spatially varying CDW phase, we derive an effective Dingle factor that depends exponentially on the ratio of the cyclotron orbit radius, $R_c$, to $\xi$. In the context of YBCO, we conclude that the values of $\xi$ reported to date for bidirectional CDW order are, prima facie, too short to account for the observed Fermi surface reconstruction; on the other hand, the values of $\xi$ for the unidirectional CDW are just long enough.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1905.03261/full.md

## References

34 references — full list in the complete paper: https://tomesphere.com/paper/1905.03261/full.md

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Source: https://tomesphere.com/paper/1905.03261