Electronic phase separation at LaAlO3/SrTiO3 interfaces tunable by oxygen deficiency

V. N. Strocov, A. Chikina, M. Caputo, M.-A. Husanu, F. Bisti, D. Bracher, T. Schmitt, F. Miletto Granozio, C. A. F. Vaz, and F. Lechermann
Phys. Rev. Materials 3, 106001 – Published 7 October 2019
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Abstract

Electronic phase separation is crucial for the fascinating macroscopic properties of the LaAlO3/SrTiO3 (LAO/STO) paradigm oxide interface, including the coexistence of superconductivity and ferromagnetism. We investigate this phenomenon using angle-resolved photoelectron spectroscopy (ARPES) in the soft-x-ray energy range, where the enhanced probing depth combined with resonant photoexcitation allow us access to fundamental electronic structure characteristics – momentum-resolved spectral function, dispersions and ordering of energy bands, Fermi surface – of buried interfaces. Our experiment uses x-ray irradiation of the LAO/STO interface to tune its oxygen deficiency, building up a dichotomic system where mobile weakly correlated Tit2g electrons coexist with localized strongly correlated Tieg ones. The ARPES spectra dynamics under x-ray irradiation shows a gradual intensity increase under constant Luttinger count of the Fermi surface. This fact identifies electronic phase separation (EPS) where the mobile electrons accumulate in conducting puddles with fixed electronic structure embedded in an insulating host phase, and allows us to estimate the lateral fraction of these puddles. We discuss the physics of EPS invoking a theoretical picture of oxygen-vacancy clustering, promoted by the magnetism of the localized Tieg electrons, and repelling of the mobile t2g electrons from these clusters. Our results on the irradiation-tuned EPS elucidate the intrinsic one taking place at the stoichiometric LAO/STO interfaces.

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  • Received 12 June 2019

DOI:https://doi.org/10.1103/PhysRevMaterials.3.106001

©2019 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

V. N. Strocov1, A. Chikina1, M. Caputo1, M.-A. Husanu1,2, F. Bisti1, D. Bracher1, T. Schmitt1, F. Miletto Granozio3, C. A. F. Vaz1, and F. Lechermann4

  • 1Swiss Light Source, Paul Scherrer Institute, CH-5232 Villigen-PSI, Switzerland
  • 2National Institute of Materials Physics, Atomistilor 405A, RO-077125 Magurele, Romania
  • 3CNR-SPIN, Complesso universitario di Monte S. Angelo, Via Cintia, I-80126 Naples, Italy
  • 4Institut für Theoretische Physik, Universität Hamburg, Jungiusstr. 9, DE-20355 Hamburg, Germany

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Issue

Vol. 3, Iss. 10 — October 2019

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