Repository logo


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

dc.contributor.authorBlake, RMen_AU
dc.contributor.authorStapleton, NDen_AU
dc.contributor.authorJones, IMen_AU
dc.contributor.authorBrookes, JRen_AU
dc.contributor.authorTurner, GFen_AU
dc.contributor.authorBird, SAen_AU
dc.contributor.authorRiboldi-Tunnicliffe, Aen_AU
dc.contributor.authorWilliamson, RMen_AU
dc.contributor.authorYoung, Ren_AU
dc.contributor.authorMaynard-Casely, HEen_AU
dc.contributor.authorSpagnoli, Den_AU
dc.contributor.authorMoggach, SAen_AU
dc.date.accessioned2026-08-11T07:19:31Zen_AU
dc.date.issued2024-08-23en_AU
dc.date.statistics2026-01-06en_AU
dc.description.abstractThree 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.en_AU
dc.description.sponsorshipR.M.B., N.D.S., and J.R.B. acknowledge the Australian Government and the University of Western Australia for the provision of a Research Training Program Scholarship. R.M.B. acknowledges the support of an AINSE Ltd. Honours Scholarship, and N.D.S acknowledges the support of an AINSE Ltd. Postgraduate Research Award (PGRA). S.A.M. acknowledges the Australian Research Council (ARC) for the provision of a Future Fellowship (FT200100243) and a Discovery Project (DP220103690). I.M.J. was funded by FT200100243, and G.F.T. was funded by DP220103690. R.M.B., J.R.B., D.S., and N.D.S. acknowledge the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia for providing resources for carrying out calculations. All authors acknowledge the Australian Synchrotron for the provision of beamtime on MX1 and the International Space Center at UWA.en_AU
dc.identifier.citationBlake, 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.4c00202en_AU
dc.identifier.issn2472-3452en_AU
dc.identifier.issue9en_AU
dc.identifier.journaltitleACS Earth and Space Chemistryen_AU
dc.identifier.pagination1693-1699en_AU
dc.identifier.urihttps://doi.org/10.1021/acsearthspacechem.4c00202en_AU
dc.identifier.urihttps://apo.ansto.gov.au/handle/10238/17309en_AU
dc.identifier.volume8en_AU
dc.languageEnglishen_AU
dc.language.isoenen_AU
dc.publisherAmerican Chemical Society (ACS)en_AU
dc.subjectCompressionen_AU
dc.subjectCrystalsen_AU
dc.subjectCrystal structureen_AU
dc.subjectMoleculesen_AU
dc.subjectPressure rangeen_AU
dc.subjectDiffractionen_AU
dc.subjectHydrogenen_AU
dc.subjectX-ray diffractionen_AU
dc.subjectDensity functional methoden_AU
dc.titleStructural evolution of trimethylacetonitrile under pressure: a combined X‑ray diffraction and computational studyen_AU
dc.typeJournal Articleen_AU

Files

License bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
license.txt
Size:
1.66 KB
Format:
Plain Text
Description:

Collections