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Updated: May 17, 2026

Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry
Published on: April 8, 2020
Helium nanodroplet isolation spectroscopy and ab initio calculations of HO3-(O2)n clusters
Tao Liang1, Paul L Raston, Gary E Douberly
1Department of Chemistry, University of Georgia, Athens, GA 30602, USA.
Abstract:
HO3-(O2)n clusters are formed by the sequential addition of the hydroxyl radical and O2 molecules to superfluid helium nanodroplets. IR laser spectroscopy in the fundamental OH stretching region reveals the presence of several bands assigned to species as large as n=4. Detailed ab initio calculations are carried out for multiple isomers of cis- and trans-HO3-O2, corresponding to either hydrogen- or oxygen-bonded van der Waals complexes. Comparisons to theory suggest that the structure of the HO3-O2 complex formed in helium droplets is a hydrogen-bonded (4)A' species consisting of a trans-HO3 core. The computed binding energy of the complex is approximately 240 cm(-1). Despite the weak interaction between trans-HO3 and O2, nonadditive redshifts of the OH stretching frequency are observed upon successive solvation by O2 to form larger clusters with n>1.
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Noble Gases
The elements in group 18 are noble gases (helium, neon, argon, krypton, xenon, and radon). They earned the name “noble” because they were assumed to be nonreactive since they have filled valence shells. In 1962, Dr. Neil Bartlett at the University of British Columbia proved this assumption to be false.

