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Tuning the Néel Temperature of Hexagonal Ferrites by Structural Distortion

https://doi.org/10.1103/PhysRevLett.121.237203

Sinha, Kishan ; Wang, Haohan ; Wang, Xiao ; Zhou, Liying ; Yin, Yuewei ; Wang, Wenbin ; Cheng, Xuemei ; Keavney, David J. ; Cao, Huibo ; Liu, Yaohua ; et al ( December 2018 , Physical Review Letters)
Electronic structure and direct observation of ferrimagnetism in multiferroic hexagonal YbFeO3

https://doi.org/10.1103/PhysRevB.95.224428

Cao, Shi ; Sinha, Kishan ; Zhang, Xin ; Zhang, Xiaozhe ; Wang, Xiao ; Yin, Yuewei ; N'Diaye, Alpha T. ; Wang, Jian ; Keavney, David J. ; Paudel, Tula R. ; et al ( June 2017 , Physical Review B)
Electronic Structure and Band Alignment of LaMnO 3 /SrTiO 3 Polar/Nonpolar Heterojunctions

https://doi.org/10.1002/admi.201801428

Kaspar, Tiffany C. ; Sushko, Peter V. ; Spurgeon, Steven R. ; Bowden, Mark E. ; Keavney, David J. ; Comes, Ryan B. ; Saremi, Sahar ; Martin, Lane ; Chambers, Scott A. ( November 2018 , Advanced Materials Interfaces)

Abstract
The behavior of polar LaMnO₃(LMO) thin films deposited epitaxially on nonpolar SrTiO₃(001) (STO) is dictated by both the LMO/STO band alignment and the chemistry of the Mn cation. Using in situ X‐ray photoelectron spectroscopy, the valence band offset (VBO) of LMO/STO heterojunctions is directly measured as a function of thickness, and found that the VBO is 2.5 eV for thicker (≥3 u.c.) films. No evidence of a built‐in electric field in LMO films of any thickness is found. Measurements of the Mn valence by MnL‐edge X‐ray absorption spectroscopy and by spatially resolved electron energy loss spectra in scanning transmission electron microscopy images reveal that Mn²⁺is present at the LMO surface, but not at the LMO/STO interface. These results are corroborated by density functional theory simulations that confirm a VBO of ≈2.5 eV for both ideal and intermixed interfaces. A model is proposed for the behavior of polar/nonpolar LMO/STO heterojunctions in which the polar catastrophe is alleviated by the formation of oxygen vacancies at the LMO surface.

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