Mott-Hubbard gap closure and structural phase transition in the oxyhalides TiOBr and TiOCl under pressure
C. A. Kuntscher, A. Pashkin, H. Hoffmann, S. Frank, M. Klemm, S. Horn,, A. Sch\"onleber, S. van Smaalen, M. Hanfland, S. Glawion, M. Sing, R., Claessen

TL;DR
This study investigates how applying pressure causes the Mott-Hubbard gap to close and induces structural phase transitions in TiOBr and TiOCl, revealing the interplay between electronic and structural changes.
Contribution
It provides the first detailed pressure-dependent optical and structural data showing gap closure and phase transitions in TiOBr and TiOCl.
Findings
Mott-Hubbard gap closes at 14 GPa in TiOBr and 16 GPa in TiOCl.
Structural phase transition coincides with gap closure.
Similar effects observed at low temperature in TiOBr.
Abstract
Pressure-dependent transmittance and reflectance spectra of TiOBr and TiOCl single crystals at room temperature suggest the closure of the Mott-Hubbard gap, i.e., the gap is filled with additional electronic states extending down to the far-infrared range. According to pressure-dependent x-ray powder diffraction data the gap closure coincides with a structural phase transition. The transition in TiOBr occurs at slightly lower pressure (=14 GPa) compared to TiOCl (=16 GPa) under hydrostatic conditions, which is discussed in terms of the chemical pressure effect. The results of pressure-dependent transmittance measurements on TiOBr at low temperatures reveal similar effects at 23 K, where the compound is in the spin-Peierls phase at ambient pressure.
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