Resumen
The recent interstellar detections of ArH+ and HeH+ have increased the interest in noble molecules. In this work, we develop potential energy surfaces (PESs) at a high level of theory for the HeHHe+ + He, ArHAr+ + He, and NeHNe+ + He complexes and study the collision dynamics. A large number of ab initio energies are computed at the coupled-cluster with single, double, and perturbative triple excitations level of theory for the systems. A grid of energies at the complete basis set limit is fitted to an analytical function for each complex. These PESs are then employed in close-coupling calculations at low collision energies. The rotational state-to-state rate coefficients of HeHHe+ by collision He are compared with previous studies, and an excellent agreement is found. Furthermore, the available quenching rate coefficients for ArH+, HeH+, and NeH+, by He, are compared with those computed in this work, and the rotational de-excitations of the diatoms are more efficient than with the triatomic systems. Finally, a set of rate coefficients for ArHAr+ + He, HeHHe+ + He, and NeHNe+ + He at low temperatures is reported.
| Idioma original | Inglés |
|---|---|
| Páginas (desde-hasta) | 1924-1929 |
| Número de páginas | 6 |
| Publicación | ACS Earth and Space Chemistry |
| Volumen | 6 |
| N.º | 7 |
| DOI | |
| Estado | Publicada - 21 jul. 2022 |
Áreas temáticas de ASJC Scopus
- Geoquímica y petrología
- Ciencias atmosféricas
- Ciencias planetarias y espacial
Huella
Profundice en los temas de investigación de 'Quantum Inelastic Scattering of ArHAr+, HeHHe+, and NeHNe+with He on New Potential Energy Surfaces'. En conjunto forman una huella única.Citar esto
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