2023
DOI: 10.1021/acsearthspacechem.2c00302
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Rotational State-to-State Rate Coefficients of HeHNe+ by Collision with He at Low Temperatures

Abstract: The HeHNe+ molecule is expected to have, after NeH+, the strongest neon bond found so far. Furthermore, formation mechanisms in the interstellar medium (ISM) have been proposed for this molecule. If HeHNe+ is detected, the collisional rate coefficients of this species with the most abundant constituents of the ISM will be critical for employing nonlocal thermodynamic equilibrium (non-LTE) models. Therefore, the main goals of this work are to study the interaction of HeHNe+ with He and to report a set of rotati… Show more

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“…The first evidence of gaseous cationic species dates back to 1925, 1 when Hogness and Lunn detected the simplest HeH + and HeH 2 + from ionized He/H 2 mixtures. Over the years, the gas-phase chemistry of the Ng m H n + (Ng = He–Xe; m , n ≥ 1) turned out to be rich and varied, 2 and the rejuvenated interest that it is currently enjoying 3–13 is also stimulated by the actual detection of ArH + and HeH + in various galactic and extragalactic regions. 14–18 Neutral compounds with Ng–H bonds emerged first in 1995, 19 when Räsänen and his coworkers identified the strong infrared absorbers originating from the photodissociation of hydrogen halides in Kr and Xe matrices as the “inserted” compounds HXeI, HXeBr, HXeCl, and HKrCl.…”
Section: Introductionmentioning
confidence: 99%
“…The first evidence of gaseous cationic species dates back to 1925, 1 when Hogness and Lunn detected the simplest HeH + and HeH 2 + from ionized He/H 2 mixtures. Over the years, the gas-phase chemistry of the Ng m H n + (Ng = He–Xe; m , n ≥ 1) turned out to be rich and varied, 2 and the rejuvenated interest that it is currently enjoying 3–13 is also stimulated by the actual detection of ArH + and HeH + in various galactic and extragalactic regions. 14–18 Neutral compounds with Ng–H bonds emerged first in 1995, 19 when Räsänen and his coworkers identified the strong infrared absorbers originating from the photodissociation of hydrogen halides in Kr and Xe matrices as the “inserted” compounds HXeI, HXeBr, HXeCl, and HKrCl.…”
Section: Introductionmentioning
confidence: 99%
“…86 The He-solvated dimers, such as HHe 3 + , HNe 2 + •He, HAr 2 + •He, and HHeNe + •He, have also been playing a crucial role in testing collisional and nonlocal thermodynamic equilibrium models. 87,88 A common structural motif of the four proton-bound rare-gas dimers mentioned is that their chromophores are triatomic, formally linear cations. If a linear molecule, whose quadrupole moment dominates its multipole expansion, 89 interacts with a single solvating atom, the resulting dimer forms a (nearly) T-shaped global minimum (GM), though linear secondary minima (SM) might also be present on the potential energy surface (PES).…”
Section: Introductionmentioning
confidence: 99%
“…The structures and vibrations of larger HAr n + complexes ( n = 3–7) have also been studied via gas-phase infrared spectroscopy . The He-solvated dimers, such as HHe 3 + , HNe 2 + ·He, HAr 2 + ·He, and HHeNe + ·He, have also been playing a crucial role in testing collisional and nonlocal thermodynamic equilibrium models. , A common structural motif of the four proton-bound rare-gas dimers mentioned is that their chromophores are triatomic, formally linear cations.…”
Section: Introductionmentioning
confidence: 99%