Two-component electronic phase separation in the doped Mott insulator Y1−xCaxTiO3

S. Hameed, J. Joe, D. M. Gautreau, J. W. Freeland, T. Birol, M. Greven

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Abstract

One of the major puzzles in condensed matter physics has been the observation of a Mott-insulating state away from half-filling. Several theoretical proposals aimed to elucidate this phenomenon have been put forth, a notable one being phase separation and an associated percolation-induced Mott insulator-metal transition. In the present work we study the prototypical doped Mott-insulating rare-earth titanate YTiO3, in which the insulating state survives up to a large hole concentration of 35%. Single crystals of Y1-xCaxTiO3 with 0≤x≤0.5, spanning the insulator-metal transition, are grown and investigated. Using x-ray absorption spectroscopy, a powerful technique capable of probing element-specific electronic states, we find that the primary effect of hole doping is to induce electronic phase separation into hole-rich and hole-poor regions. The data reveal the formation of electronic states within the Mott-Hubbard gap, near the Fermi level, which increase in spectral weight with increasing doping. From a comparison with DFT+U calculations, we infer that the hole-poor and hole-rich components have charge densities that correspond to the insulating x=0 and metallic x∼0.5 states, respectively, and that the new electronic states arise from the metallic component. Our results indicate that the doping-induced insulator-metal transition in Y1-xCaxTiO3 is indeed percolative in nature, and thus of inherent first-order character.

Original languageEnglish (US)
Article number045112
JournalPhysical Review B
Volume104
Issue number4
DOIs
StatePublished - Jul 9 2021

Bibliographical note

Funding Information:
We thank Damjan Pelc for valuable comments on the manuscript and Chris Leighton for the use of sample-polishing equipment. The work at University of Minnesota was funded by the Department of Energy through the University of Minnesota Center for Quantum Materials, under DE-SC0016371. This research used resources of the Advanced Photon Source, a US Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. Part of this work was carried out in the Characterization Facility, University of Minnesota, which receives partial support from the NSF through the MRSEC (Award No. DMR-2011401) and the NNCI (Award No. ECCS-2025124) programs.

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© 2021 American Physical Society.

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