Electronic structure of the band-filling-controlled CaVO3 and LaVO3 compounds.
| Autor: | Mossanek RJ; Departamento de Física, Universidade Federal do Paraná, Caixa Postal 19081, 81531-990 Curitiba PR, Brazil., Abbate M, Yoshida T, Fujimori A, Yoshida Y, Shirakawa N, Eisaki H, Kohno S, Fonseca PT, Vicentin FC |
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| Jazyk: | angličtina |
| Zdroj: | Journal of physics. Condensed matter : an Institute of Physics journal [J Phys Condens Matter] 2010 Mar 10; Vol. 22 (9), pp. 095601. Date of Electronic Publication: 2010 Feb 10. |
| DOI: | 10.1088/0953-8984/22/9/095601 |
| Abstrakt: | We studied the electronic structure of the band-filling CaVO(3) and LaVO(3) compounds. The experimental techniques were photoemission (PES) and x-ray absorption (XAS) spectroscopy. The experimental results were analyzed using an extended cluster model. The ground states of CaVO(3) and LaVO(3) are highly covalent and contain a considerable 3d(n + 1)L contribution. The CaVO(3) compound is in the charge transfer regime (Δ < U), whereas the LaVO(3) material is in the intermediate regime (Δ ∼ U). The spectral weight distributions reveal that CaVO(3) is a coherent metal and that LaVO(3) is a p-d insulator. The photoemission of CaVO(3) shows the coherent peak (3d(1)C) and the incoherent feature (3d(1)L). The spectrum of insulating LaVO(3) presents only the incoherent structure (3d(2)L), whereas the coherent peak is replaced by the Mott-Hubbard screening (3d(2)D). This transfer of spectral weight is responsible for the opening of the experimental bandgap. The incoherent feature contains a considerable O 2p character and cannot be attributed to the lower Hubbard band. Further, the relative V 3d-O 2p cross section helps to explain the photon energy dependence of the PES spectra. The addition spectra of both CaVO(3) and LaVO(3) are dominated by the 3d(n + 1) final state configuration. The distribution of spectral weight is mainly dictated by intra-atomic exchange and crystal field splittings. The coherent contribution is less important than in photoemission, and is greatly diminished in the O 1s x-ray absorption spectra. (© 2010 IOP Publishing Ltd) |
| Databáze: | MEDLINE |
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