Topological Hall effect and emergent skyrmion crystal at manganite-iridate oxide interfaces

Narayan Mohanta, Elbio Dagotto, Satoshi Okamoto

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50 Scopus citations

Abstract

Scalar spin chirality is expected to induce a finite contribution to the Hall response at low temperatures. We study this spin-chirality-driven Hall effect, known as the topological Hall effect, at the manganite side of the interface between La1-xSrxMnO3 and SrIrO3. The ferromagnetic double-exchange hopping at the manganite layer, in conjunction with the Dzyaloshinskii-Moriya (DM) interaction which arises at the interface due to broken inversion symmetry and strong spin-orbit coupling from the iridate layer, could produce a skyrmion-crystal (SkX) phase in the presence of an external magnetic field. Using the Monte Carlo technique and a two-orbital spin-fermion model for manganites, supplemented by an in-plane DM interaction, we obtain phase diagrams which reveal at low temperatures a clear SkX phase and also a low-field spin-spiral phase. Increasing temperature, a skyrmion-gas phase, precursor of the SkX phase upon cooling, was identified. The topological Hall effect primarily appears in the SkX phase, as observed before in oxide heterostructures. We conclude that the manganite-iridate superlattices provide another useful platform to explore a plethora of unconventional magnetic and transport properties.

Original languageEnglish
Article number064429
JournalPhysical Review B
Volume100
Issue number6
DOIs
StatePublished - Aug 30 2019

Funding

The authors gratefully acknowledge John Nichols, Elizabeth M. Skoropata, and Ho Nyung Lee for discussions on their related experiments. All members of this collaboration were supported by the US Department of Energy (DOE), Office of Science, Basic Energy Sciences (BES), Materials Sciences and Engineering Division. This research used resources of the Compute and Data Environment for Science (CADES) at the Oak Ridge National Laboratory, which is supported by the Office of Science of the US Department of Energy. This research was supported in part by an appointment to the Oak Ridge National Laboratory ASTRO Program, sponsored by the U.S. Department of Energy and administered by the Oak Ridge Institute for Science and Education.

FundersFunder number
Data Environment for Science
US Department of Energy
U.S. Department of Energy
Office of Science
Basic Energy Sciences
Oak Ridge Institute for Science and Education
Cades Foundation
Division of Materials Sciences and Engineering

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