Structural Evolution of Trimethylacetonitrile under Pressure: A Combined X‑ray Diffraction and Computational Study

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 disorder...

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Veröffentlicht in:ACS earth and space chemistry 2024-09, Vol.8 (9), p.1693-1699
Hauptverfasser: Blake, Rebecca M., Stapleton, Nicholas D., Jones, Isabelle M., Brookes, James R., Turner, Gemma F., Bird, Stephanie A., Riboldi-Tunnicliffe, Alan, Williamson, Rachel M., Young, Rosemary, Maynard-Casely, Helen E., Spagnoli, Dino, Moggach, Stephen A.
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Sprache:eng
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Zusammenfassung: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.
ISSN:2472-3452
2472-3452
DOI:10.1021/acsearthspacechem.4c00202