2022
DOI: 10.3390/molecules27103198
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Spectral Signatures of Protonated Noble Gas Clusters of Ne, Ar, Kr, and Xe: From Monomers to Trimers

Abstract: The structures and spectral features of protonated noble gas clusters are examined using a first principles approach. Protonated noble gas monomers (NgH+) and dimers (NgH+Ng) have a linear structure, while the protonated noble gas trimers (Ng3H+) can have a T-shaped or linear structure. Successive binding energies for these complexes are calculated at the CCSD(T)/CBS level of theory. Anharmonic simulations for the dimers and trimers unveil interesting spectral features. The symmetric NgH+Ng are charactized by … Show more

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Cited by 7 publications
(12 citation statements)
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“…This frequency is close to that of the corresponding ν H + band for Ar 2 H + , which is at 989 cm −1 . 35,38,41,43 Furthermore, combination bands involving ν int + ν H + and 2ν int + ν H + are seen as bands at 1121 cm −1 and 1424 cm −1 . On the other hand, the ν NN band is seen as a moderate peak at 2370 cm −1 .…”
Section: ■ Results and Discussionmentioning
confidence: 92%
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“…This frequency is close to that of the corresponding ν H + band for Ar 2 H + , which is at 989 cm −1 . 35,38,41,43 Furthermore, combination bands involving ν int + ν H + and 2ν int + ν H + are seen as bands at 1121 cm −1 and 1424 cm −1 . On the other hand, the ν NN band is seen as a moderate peak at 2370 cm −1 .…”
Section: ■ Results and Discussionmentioning
confidence: 92%
“…20,35−44 In addition to the bright ν H + band, our past simulations have shown that a strong progression of combination bands (nν int + ν H + ), which involves ν H + and multiple quanta of the A•••A intermolecular stretch nν int is observed for symmetric PBDs. Such combination bands are very pronounced in NgH + Ng 35,41,43 and N 2 H + N 2 . 13,20 In the present work, theoretical simulations were performed to investigate the vibrational structure of N 2 H + Ng, Ng = {He, Ne, Ar, Kr, Xe, and Rn}.…”
Section: ■ Introductionmentioning
confidence: 95%
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“…The recent astronomical observations of HeH + and ArH + have increased the interest in molecules bearing noble atoms . Several molecules of this type that could form in the interstellar medium (ISM) have been studied since these detections. New searches for the noble gas species have also been carried out in recent years …”
Section: Introductionmentioning
confidence: 99%