# Magnetic and orbital correlations in multiferroic CaMn$_7$O$_{12}$   probed by x-ray resonant elastic scattering

**Authors:** K. Gautam, S. S. Majid, S. Francoual, A. Ahad, K. Dey, M. C. Rahn, R., Sankar, F.C. Chou, D. K. Shukla

arXiv: 1908.00371 · 2020-06-30

## TL;DR

This study uses x-ray resonant elastic scattering to investigate magnetic and orbital correlations in multiferroic CaMn$_7$O$_{12}$, revealing a previously unknown orbital order splitting and complex temperature-dependent behaviors.

## Contribution

It demonstrates the application of polarization-resolved XRES to distinguish magnetic and orbital orders and uncovers a new low-temperature orbital phase in CaMn$_7$O$_{12}.

## Key findings

- Discovered a split in orbital order superstructure peaks at low temperature.
- Identified a second-harmonic orbital signal with distinct polarization dependence.
- Revealed temperature-driven orbital re-ordering possibly due to exchange interactions.

## Abstract

The quadruple perovskite CaMn$_7$O$_{12}$ is a topical multiferroic, in which the hierarchy of electronic correlations driving structural distortions, modulated magnetism, and orbital order is not well known and may vary with temperature. x-ray resonant elastic scattering (XRES) provides a momentum-resolved tool to study these phenomena, even in very small single crystals, with valuable information encoded in its polarization- and energy-dependence. We present an application of this technique to CaMn$_7$O$_{12}$. By polarization analysis, it is possible to distinguish superstructure reflections associated with magnetic order and orbital order. Given the high momentum resolution, we resolve a previously unknown splitting of an orbital order superstructure peak, associated with a distinct \textit{locked-in} phase at low temperatures. A second set of orbital order superstructure peaks can then be interpreted as a second-harmonic orbital signal. Surprisingly, the intensities of the first- and second-harmonic orbital signal show disparate temperature and polarization dependence. This orbital re-ordering may be driven by an exchange mechanism, that becomes dominant over the Jahn-Teller instability at low temperature.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1908.00371/full.md

## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1908.00371/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1908.00371/full.md

---
Source: https://tomesphere.com/paper/1908.00371