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Phys. Rev. B 81, 085112 (2010) [10 pages]

Electronic structure and stability of hexagonal Ba3Ti2RuO9

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G. Radtke1,*, C. Maunders2, A. Saúl3, S. Lazar4, H. J. Whitfield5, J. Etheridge5, and G. A. Botton2
1Institut Matériaux Microélectronique Nanosciences de Provence, UMR 6242 CNRS, Faculté des Sciences de Saint-Jérôme, Université Paul Cézanne-Aix Marseille III, Case 262, 13397 Marseille Cedex 20, France
2Canadian Centre for Electron Microscopy, McMaster University, Hamilton, Ontario, Canada L8S 4L8
3Centre Interdisciplinaire de Nanoscience de Marseille, UPR 3118 CNRS, Campus de Luminy, Case 913, 13288 Marseille Cedex 9, France
4FEI Electron Optics, Eindhoven, The Netherlands
5Monash Centre for Electron Microscopy, Monash University, Clayton, Victoria, Australia

Received 23 September 2009; revised 7 January 2010; published 18 February 2010

We investigated the electronic structure and stability of the hexagonal perovskite Ba3Ti2RuO9 using high-resolution electron energy loss spectroscopy and first-principles band structure calculations. The comparison between experimental and theoretical results leads to a coherent picture of the electronic structure of this compound where both Ti and Ru ions are tetravalent, the first unoccupied states being of Ru 4d character. Structural relaxations performed on four variants of this compound allowed a detailed investigation of the influence of the Ru atoms location in the hexagonal unit cell and clarified the origin of the stabilization of this phase at room temperature. Two structures without inversion symmetry built, respectively, with two TiRuO9 units (space group P63mc, 186) or with one Ru2O9 and one Ti2O9 unit (P6̅ m2,187) are found to be the most stable. The stabilization of the first structure occurs through the polarization of the partially filled Ru 4d bands, whereas a direct metal-metal bonding interaction taking place between the two Ru atoms in the Ru2O9 unit lowers the total energy of the second. The influence of the exchange correlation functional used to perform these calculations on the relative stability of the four variants is discussed.

© 2010 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.81.085112
DOI:
10.1103/PhysRevB.81.085112
PACS:
79.20.Uv, 61.66.Fn, 71.20.Ps

*guillaume.radtke@im2np.fr