High-Pressure Crystallization and Compression of Isobutyronitrile

  • Rebecca M. Blake
  • , Nicholas D. Stapleton
  • , James R. Brookes
  • , Isabelle M. Jones
  • , Gemma F. Turner
  • , Stephanie A. Bird
  • , Alan Riboldi-Tunnicliffe
  • , Rachel M. Williamson
  • , Rosemary J. Young
  • , Helen E. Maynard-Casely
  • , Dino Spagnoli
  • , Stephen A. Moggach

Research output: Contribution to journalArticlepeer-review

Abstract

The structural response of a high-pressure phase of isobutyronitrile up to 6.12 GPa was studied by using high-pressure single-crystal X-ray diffraction, periodic density functional theory (DFT), and CrystalExplorer calculations. This phase is isostructural with a known low-temperature phase. Compression involves distortion of packing arrangements and shortening of hydrogen bonds. However, interaction energy calculations show stabilization from enhanced hydrogen bonds is offset by increasing steric repulsion. Steric contacts cause transient incompressibility between 1.88 and 2.17 GPa, overcome by higher pressure. Volume reduction, not hydrogen bonding, primarily drives compressibility. Significant steric repulsion develops by 5.21 GPa, preceding crystallinity degradation above 6.12 GPa.

Original languageEnglish
Pages (from-to)2837-2845
Number of pages9
JournalACS Earth and Space Chemistry
Volume9
Issue number12
Early online date9 Dec 2025
DOIs
Publication statusPublished - 18 Dec 2025

Funding

FundersFunder number
ARC Australian Research Council FT200100243, DP220103690

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