English

Complex magnetic order in nickelate slabs

Strongly Correlated Electrons 2019-05-13 v1

Abstract

Magnetic ordering phenomena have a profound influence on the macroscopic properties of correlated-electron materials, but their realistic prediction remains a formidable challenge. An archetypical example is the ternary nickel oxide system RNiO3 (R = rare earth), where the period-four magnetic order with proposals of collinear and non-collinear structures and the amplitude of magnetic moments on different Ni sublattices have been subjects of debate for decades. Here we introduce an elementary model system - NdNiO3 slabs embedded in a non-magnetic NdGaO3 matrix - and use polarized resonant x-ray scattering (RXS) to show that both collinear and non-collinear magnetic structures can be realized, depending on the slab thickness. The crossover between both spin structures is correctly predicted by density functional theory and can be qualitatively understood in a low-energy spin model. We further demonstrate that the amplitude ratio of magnetic moments in neighboring NiO6 octahedra can be accurately determined by RXS in combination with a correlated double cluster model. Targeted synthesis of model systems with controlled thickness and synergistic application of polarized RXS and ab-initio theory thus provide new perspectives for research on complex magnetism, in analogy to two-dimensional materials created by exfoliation.

Keywords

Cite

@article{arxiv.1905.04160,
  title  = {Complex magnetic order in nickelate slabs},
  author = {Matthias Hepting and Robert J. Green and Zhicheng Zhong and Martin Bluschke and Y. Eren Suyolcu and Sebastian Macke and Alex Frano and Sara Catalano and Marta Gibert and Ronny Sutarto and Feizhou He and Georg Cristani and Gennady Logvenov and Yi Wang and Peter A. van Aken and Philipp Hansmann and Matthieu Le Tacon and Jean-Marc Triscone and George A. Sawatzky and Bernhard Keimer and Eva Benckiser},
  journal= {arXiv preprint arXiv:1905.04160},
  year   = {2019}
}

Comments

This is the accepted version of the manuscript. The revised manuscript according to peer reviews was published online in Nature Physics on July 23, 2018

R2 v1 2026-06-23T09:02:52.637Z