# Local orthorhombicity in the magnetic $C_4$ phase of the hole-doped   iron-arsenide superconductor Sr$_{1-x}$Na$_{x}$Fe$_2$As$_2$

**Authors:** Benjamin A. Frandsen, Keith M. Taddei, Ming Yi, Alex Frano, Zurab, Guguchia, Rong Yu, Qimiao Si, Daniel E. Bugaris, Ryan Stadel, Raymond Osborn,, Stephan Rosenkranz, Omar Chmaissem, and Robert J. Birgeneau

arXiv: 1706.03279 · 2017-11-17

## TL;DR

This study reveals that local orthorhombic distortions exist within the magnetic $C_4$ phase of Sr$_{1-x}$Na$_{x}$Fe$_2$As$_2$, indicating strong nematic fluctuations that persist across different phases of this iron-based superconductor.

## Contribution

It provides the first direct evidence of local orthorhombic regions within the magnetic $C_4$ phase, highlighting the role of nematic fluctuations in iron-based superconductors.

## Key findings

- Local orthorhombic regions are about 2 nm in size.
- Orthorhombic fluctuations are present even in the tetragonal phase.
- The results suggest a large nematic susceptibility in the material.

## Abstract

We report temperature-dependent pair distribution function measurements of Sr$_{1-x}$Na$_{x}$Fe$_2$As$_2$, an iron-based superconductor system that contains a magnetic phase with reentrant tetragonal symmetry, known as the magnetic $C_4$ phase. Quantitative refinements indicate that the instantaneous local structure in the $C_4$ phase is comprised of fluctuating orthorhombic regions with a length scale of $\sim$2 nm, despite the tetragonal symmetry of the average static structure. Additionally, local orthorhombic fluctuations exist on a similar length scale at temperatures well into the paramagnetic tetragonal phase. These results highlight the exceptionally large nematic susceptibility of iron-based superconductors and have significant implications for the magnetic $C_4$ phase and the neighboring $C_2$ and superconducting phases.

## Full text

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## Figures

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## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1706.03279/full.md

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Source: https://tomesphere.com/paper/1706.03279