Abstract
The electronic, magnetic, and optical properties of the double perovskite (SCIO) under biaxial strain are explored in the framework of density functional theory, including a Hubbard term and spin-orbit coupling in combination with absorption spectroscopy measurements on epitaxial thin films. While the end member is a semimetal with a quenched spin and orbital moment and bulk is a ferromagnetic (FM) metal with spin and orbital moment of 2.50 and 0.13 , respectively, the double perovskite SCIO emerges as an antiferromagnetic Mott insulator with antiparallel alignment of Co, Ir planes along the [110] direction. Co exhibits a spin and enhanced orbital moment of and , respectively. Most remarkably, Ir acquires a significant spin and orbital moment of 1.21–1.25 and 0.13 , respectively. Analysis of the orbital occupation indicates an electronic reconstruction due to a substantial charge transfer from minority to majority spin states in Ir and from Ir to Co, signaling an , configuration. Biaxial strain, varied from through 0% to , affects the orbital polarization of the states and leads to a nonmonotonic change of the band gap between 163 and 235 meV. The absorption coefficient reveals a two-plateau feature due to transitions from the valence to the lower-lying narrow and the higher-lying broader bands. Inclusion of many-body effects, in particular, excitonic effects by solving the Bethe-Salpeter equation, increases the band gap by and improves the agreement with the measured spectrum concerning the position of the second peak at .
3 More- Received 8 June 2021
- Revised 17 September 2021
- Accepted 14 October 2021
DOI:https://doi.org/10.1103/PhysRevB.104.205126
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