# Anisotropic spin-density distribution and magnetic anisotropy of   strained La$_{1-x}$Sr$_x$MnO$_3$ thin films: Angle-dependent x-ray magnetic   circular dichroism

**Authors:** G. Shibata, M. Kitamura, M. Minohara, K. Yoshimatsu, T. Kadono, K., Ishigami, T. Harano, Y. Takahashi, S. Sakamoto, Y. Nonaka, K. Ikeda, Z. Chi,, M. Furuse, S. Fuchino, M. Okano, J.-i. Fujihira, A. Uchida, K. Watanabe, H., Fujihira, S. Fujihira, A. Tanaka, H. Kumigashira, T. Koide, A. Fujimori

arXiv: 1706.05183 · 2018-02-01

## TL;DR

This study uses angle-dependent x-ray magnetic circular dichroism to reveal how strain influences the anisotropic spin-density distribution and magnetic anisotropy in La$_{1-x}$Sr$_x$MnO$_3$ thin films, clarifying surface orbital occupation effects.

## Contribution

It provides direct experimental evidence of strain-dependent in-plane and out-of-plane spin-density anisotropy in LSMO thin films using XMCD, resolving previous ambiguities from XLD measurements.

## Key findings

- Spin-density distribution anisotropy aligns with magnetic anisotropy.
- Tensile strain induces in-plane spin-density anisotropy.
- Compressive strain induces out-of-plane spin-density anisotropy.

## Abstract

Magnetic anisotropies of ferromagnetic thin films are induced by epitaxial strain from the substrate via strain-induced anisotropy in the orbital magnetic moment and that in the spatial distribution of spin-polarized electrons. However, the preferential orbital occupation in ferromagnetic metallic La$_{1-x}$Sr$_x$MnO$_3$ (LSMO) thin films studied by x-ray linear dichroism (XLD) has always been found out-of-plane for both tensile and compressive epitaxial strain and hence irrespective of the magnetic anisotropy. In order to resolve this mystery, we directly probed the preferential orbital occupation of spin-polarized electrons in LSMO thin films under strain by angle-dependent x-ray magnetic circular dichroism (XMCD). Anisotropy of the spin-density distribution was found to be in-plane for the tensile strain and out-of-plane for the compressive strain, consistent with the observed magnetic anisotropy. The ubiquitous out-of-plane preferential orbital occupation seen by XLD is attributed to the occupation of both spin-up and spin-down out-of-plane orbitals in the surface magnetic dead layer.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1706.05183/full.md

## References

33 references — full list in the complete paper: https://tomesphere.com/paper/1706.05183/full.md

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Source: https://tomesphere.com/paper/1706.05183