Abstract
Recently, a golden colored, dense polymorph of titanium sesquioxide, TiO with a ThS-type structure, has been synthesized at high-pressure high-temperature conditions. In this paper, we present results of investigations of structural, optical, and electronic transport properties of this unusual golden polymorph of TiO under high pressure. Several experimental techniques were used, including x-ray diffraction studies using synchrotron radiation, Raman spectroscopy, electrical resistivity, and thermoelectric power. The structural studies showed that the ThS-type lattice is conserved under pressure, while it is subjected to an isostructural phase transition with a ∼0.7 volume drop at 38.5 GPa. We speculated that this transition could be driven by the electron transfer in the Ti atoms. For the ThS-type TiO, we have established a bulk modulus value, 258.3 GPa at 4.1. A full profile analysis of the diffraction patterns allowed us to discover anomalies in the compression behavior of the ThS-type structure. The bond valence sums method suggested that at ambient conditions the Ti cations have predominantly Ti oxidation state, but applied pressure stimulates a partial charge disproportionation between the Ti1 and Ti2 sites achieving the maximal effect—reduction of the Ti1 cations to ∼Ti and oxidation of the Ti2 ones to ∼Ti near 14 GPa. Pressure evolution of Raman spectra across the above crossovers showed distinct changes corroborating the above findings. The high-pressure electronic transport studies confirmed that the ThS-type TiO remains semiconducting up to 21 GPa at ambient and low temperatures down to 4.2 K. These studies found additional features, e.g., in the activation energy curve near 7 GPa, that is accompanied by inversion of the dominant conductivity type from electron to hole. The intriguing high-pressure behavior of TiO with the ThS-type structure can contribute to better understanding of high-pressure properties of transition-metal sesquioxides.
4 More- Received 22 January 2013
DOI:https://doi.org/10.1103/PhysRevB.88.184106
©2013 American Physical Society