Revisiting the Magnetic Structure and Charge Ordering in La$_{1/3}$Sr$_{2/3}$FeO$_3$ by Neutron Powder Diffraction and M\"ossbauer Spectroscopy

TL;DR

This study investigates the magnetic structure and charge ordering in La$_{1/3}$Sr$_{2/3}$FeO$_3$ using neutron diffraction and M"ossbauer spectroscopy, proposing two possible magnetic models and analyzing charge disproportionation.

Contribution

It provides a detailed analysis of the magnetic structures, proposing both chiral helical and collinear models, and discusses charge ordering phenomena in La$_{1/3}$Sr$_{2/3}$FeO$_3$.

Findings

Both magnetic models fit the neutron diffraction data equally well.

M"ossbauer spectroscopy indicates charge disproportionation below the magnetic transition.

The Fe ions exhibit a charge state around Fe$^{3.66+}$ above the transition.

Abstract

The magnetic ordering of La$_{1/3}$Sr$_{2/3}$FeO$_3$ perovskite has been studied by neutron powder diffraction and $^{57}$Fe M\"ossbauer spectroscopy down to 2 K. From symmetry analysis, a chiral helical model and a collinear model are proposed to describe the magnetic structure. Both are commensurate, with propagation vector k = (0,0,1) in R-3c space group. In the former model, the magnetic moments of Fe adopt the magnetic space group P3$_{2}$21 and have helical and antiferromagnetic ordering propagating along the c axis. The model allows only one Fe site, with a magnetic moment of 3.46(2) $\mu_{\rm{B}}$ at 2 K. In the latter model, the magnetic moments of iron ions adopt the magnetic space group C2/c or C2'/c' and are aligned collinearly. The model allows the presence of two inequivalent Fe sites with magnetic moments of amplitude 3.26(3) $\mu_{\rm{B}}$ and 3.67(2) $\mu_{\rm{B}}$, respectively. The neutron diffraction pattern is equally well fitted by either model. The M\"ossbauer spectroscopy study suggests a single charge state Fe$^{3.66+}$ above the magnetic transition and a charge disproportionation into Fe$^{(3.66-\zeta)+}$ and Fe$^{(3.66+2\zeta)+}$ below the magnetic transition. The compatibility of the magnetic structure models with the M\"ossbauer spectroscopy results is discussed.