The influence of the crystal sponge framework on guest molecule conformation

12 July 2024, Version 1
This content is a preprint and has not undergone peer review at the time of posting.

Abstract

The crystalline sponge (CS) method has become an important technique for structural elucidation of compounds that are challenging to crystallise. However, the impact of the CS environment on guest molecule conformations has not been systematically studied. We present a computational investigation of the conformations of organic molecules of varying flexibility in a set of experimentally determined CS structures, comparing them to gas phase conformers and, where available, pure and co-crystal structures. Via solid state and molecular density functional theory calculations, we quantify the total relative energy, conformational energy, and intramolecular strain of guest molecules, as well as framework strain. Our results show that while CS structures induce some distortion in guest geometries (total relative energies up to 41 kJ/mol), they generally adopt low-energy conformations, often within 2 kJ/mol of the global energy minimum. Intramolecular strain in CS structures is often lower than in conventional crystal structures, suggesting a more neutral packing environment where molecules are closer to their favoured isolated-molecule geometries. We also observe that multiple guests can influence each other's geometries, even in the absence of direct guest-guest interactions. These findings provide a quantification of conformational distortion that can form the basis for interpreting molecular geometries obtained from CS structures.

Keywords

structure
molecular structure
crystallography
crystal sponge
metal organic framework

Supplementary materials

Title
Description
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Title
Supporting Information and Results
Description
Details of crystal and molecular geometry optimisations, conformational searches, calculated strain, conformational, and total relative energies for all molecules, correlation between strain energy and molecular geometry changes.
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