Repository logo


Structural evolution of trimethylacetonitrile under pressure: a combined X‑ray diffraction and computational study

Abstract

Three high-pressure phases of trimethylacetonitrile, a compound of potential interest in the context of Titan’s atmospheric chemistry, have been investigated using single-crystal X-ray diffraction, periodic density functional theory, and CrystalExplorer intermolecular energy calculations. A disordered tetragonal P4/nmm phase is formed between 0.07 and 0.29 GPa (denoted hp-I). Compression to 0.43 GPa forms an ordered orthorhombic Pnma phase (hp-II), which transforms to a monoclinic P21/m phase (hp-III) at 1.52 GPa. The hp-III phase persists to at least 3.34 GPa. Phase transitions are driven by densification of the crystal and facilitated by rearrangement of the supramolecular hydrogen-bonding network, with 180° reorientation of half the molecules. Compression of each phase is associated with slight shortening of the intermolecular hydrogen bonds, with gradual destabilization of the cohesive energy to 3.34 GPa. © 2024 American Chemical Society.

Description

Citation

Blake, R. M., Stapleton, N. D., Jones, I. M., Brookes, J. R., Turner, G. F., Bird, S. A., Riboldi-Tunnicliffe, A., Williamson, R. M., Young, R., Maynard-Casely, H. E., Spagnoli, D., & Moggach, S. A. (2024). Structural evolution of trimethylacetonitrile under pressure: a combined X‑ray diffraction and computational study. ACS Earth and Space Chemistry, 8(9), 1693–1699. doi:10.1021/acsearthspacechem.4c00202

Collections

Endorsement

Review

Supplemented By

Referenced By