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 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.

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Publication Details

Journal
ACS Earth and Space Chemistry
Published
2024-08-23
DOI
https://doi.org/10.1021/acsearthspacechem.4c00202
Citations
2
Primary Topic
Crystallography and molecular interactions
Type
article
Field-Weighted Citation Impact
0.89

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article

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

Rachel Williamson, Nicholas Stapleton, Isabelle Jones, Alan Riboldi‐Tunnicliffe et al.
2 citations
ACS Earth and Space Chemistry
Crystallography and molecular interactions
0.89
article

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

Rachel Williamson, Nicholas Stapleton, Isabelle Jones, Alan Riboldi‐Tunnicliffe, Stephen A. Moggach, Rosemary J. Young, Dino Spagnoli, Helen E. Maynard‐Casely, James Brookes, Gemma F. Turner, Stephanie A. Bird, Rebecca M. Blake
article en
2 citations

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.

ACS Earth and Space ChemistryVol. 8(9)
Australian Nuclear Science and Technology Organisation (AU), The University of Western Australia (AU), Australian Synchrotron (AU)
Australian Research Council
Openalex Percentile: Top 22%
Crystallography and molecular interactions
0.89
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