Abstract
We clarify the origin of the strikingly different spectroscopic properties of the chemically similar compounds and . Our first-principle, many-body analysis demonstrates that the highly sensitive physics of these two materials is controlled by their proximity to an adjacent Hund’s-Mott insulating phase. Although oxides are mildly correlated, we show that the cooperative action of intraorbital repulsion and Hund’s exchange becomes the dominant physical mechanism in these materials if their shell is half filled. Small material specific details hence result in an extremely sharp change of the electronic mobility, explaining the surprisingly different properties of the paramagnetic high-temperature phases of the two compounds.
- Received 15 October 2019
- Revised 10 May 2020
- Accepted 25 August 2020
DOI:https://doi.org/10.1103/PhysRevLett.125.166402
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