# Crystal structure and the magnetic properties of the 5d transition metal   oxide AOsO4 (A = K, Rb, Cs)

**Authors:** Jun-ichi Yamaura, Zenji Hiroi

arXiv: 1906.08519 · 2019-06-21

## TL;DR

This study synthesizes and characterizes the structure and magnetic properties of AOsO4 (A = K, Rb, Cs), revealing diverse magnetic behaviors and structural transitions linked to their distorted diamond lattice structures and spin-orbit coupling effects.

## Contribution

It provides the first detailed structural and magnetic analysis of AOsO4 compounds, highlighting the influence of lattice distortion and spin-orbit coupling on their magnetic properties.

## Key findings

- K and Rb compounds exhibit antiferromagnetic order with specific transition temperatures.
- Cs compound shows a structural transition without magnetic order above 2 K.
- The Os magnetic moments are reduced, likely due to antiparallel orbital moments.

## Abstract

We synthesized the 5d1-transition metal oxides AOsO4 (A = K, Rb, Cs) by solid-state reaction, and performed structure determination and magnetic and heat capacity measurements. It was found that they crystallize in a scheelite (A = K and Rb) or a quasi-scheelite structure (A = Cs) comprising of distorted diamond lattices of septivalent Os (d1) ions tetrahedrally coordinated by four oxide ions without local inversion symmetry; hence an antisymmetric spin-orbit coupling is expected in the crystals. The K and Rb compounds have Weiss temperatures of theta = -66 and -18 K, effective magnetic moments of mu_eff = 1.44 and 1.45 mu_B/Os, and antiferromagnetic transition temperatures of T_N = 36.9 and 21.0 K, respectively. In contrast, the Cs compound has theta = 12 K and mu_eff = 0.8 mu_B/Os without magnetic transition above 2 K, instead exhibiting a first-order structural transition at T_s = 152.5 K. The decline of the Os moment from 1.73 mu_B/Os for the simple d1 spin, particularly for Cs, is likely to originate from the antiparallel orbital moment, although the spin-orbit coupling is generally quenched in the low-lying e orbitals.

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Source: https://tomesphere.com/paper/1906.08519