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Thickness-dependent perovskite octahedral distortions at heterointerfaces

Invited

Abstract

The plethora of exotic physics found in transition metal oxides is no accident, it directly reflects the particularly fascinating chemistry of the d-orbitals. The d wavefunctions are highly directional and electronically very localized, leading to a strong coupling between the lattice, electronic and spin degrees of freedom. This means, therefore, that fine details of the crystal structure can have important consequences for the material properties. One famous example of this remarkable sensitivity is the family of perovskite rare earth nickelates where the temperature of their electronic and magnetic phase transitions are greatly modified by small changes of the Ni-O-Ni bond angle. The sublattice of corner connected O6 octahedra is therefore essential in driving the physics of these materials and many other perovskites like them.
Within the field of perovskite oxide heterostructures, how the oxygen sublattice reacts to the heterointerfacial constraints, as well as the contstraint of keeping the octahedra connected, is of great interest [1]. Complicating matters, however, is the difficulty in probing a light element such as oxygen when the sample volume is - by design - small and the distortions themselves may be minute.
Here we have demonstrated that the synchrotron x-ray diffraction approach successfully developed to extract the oxygen positions from half-order Bragg peaks [2] can be applied to films as thin as 2 nm [3]. Our study looks at LaNiO3 and LaAlO3 films on SrTiO3 and LaAlO3 substrates. It reveals that biaxial strain alone cannot account for the accommodation of the heterointerface when the thickness approaches the ultrathin limit and, thus, highlights layer thickness as a control parameter to adjust the lattice on the picometer scale.



[1]. J. M. Rondinelli, S. J. May and J. W. Freeland, MRS Bulletin 37 (2012)
[2]. S. J. May et al, Phys. Rev. B 82 (2010)
[3]. J. Fowlie et al, ACS Nano Lett. 19 (2019)

Presenters

  • Jennifer Fowlie

    Department of Quantum Matter Physics, University of Geneva, Department of quantum matter physics, Univ of Geneva, Univ of Geneva

Authors

  • Jennifer Fowlie

    Department of Quantum Matter Physics, University of Geneva, Department of quantum matter physics, Univ of Geneva, Univ of Geneva

  • Céline Lichtensteiger

    Univ of Geneva

  • Marta Gibert

    University of Zurich, Univ of Zurich, Physik-Institut, University of Zurich

  • Hugo Meley

    Univ of Geneva

  • Philip Willmott

    Paul Scherrer Institut

  • Jean-Marc Triscone

    Department of Quantum Matter Physics, University of Geneva, Department of quantum matter physics, Univ of Geneva, Univ of Geneva