1996
DOI: 10.1016/0301-0104(96)00060-2
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Diabatic excited states of the (HeH2)+ molecular ion for the charge exchange-excitation reaction: He+ + H2 → HeH+ + H∗

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Cited by 13 publications
(5 citation statements)
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“…Approximated theoretical models were also employed (Dhuicq et al, 1996) for explaining observed cross sections above 9 eV, when excited H * ( n = 2) was produced. Finally, quantum infinite-order-sudden cross sections were calculated (Martínez et al, 2000) for He + +H 2 → He+H * ( n ≥ 2)+H + at E coll ≥ 10 eV, using the accurate diabatic representation of Aguado et al (1993) and six more approximated diabatic electronic states (Sidis, 1996).…”
Section: Introductionmentioning
confidence: 99%
“…Approximated theoretical models were also employed (Dhuicq et al, 1996) for explaining observed cross sections above 9 eV, when excited H * ( n = 2) was produced. Finally, quantum infinite-order-sudden cross sections were calculated (Martínez et al, 2000) for He + +H 2 → He+H * ( n ≥ 2)+H + at E coll ≥ 10 eV, using the accurate diabatic representation of Aguado et al (1993) and six more approximated diabatic electronic states (Sidis, 1996).…”
Section: Introductionmentioning
confidence: 99%
“…Besides its relevance in the hydrogen plasma chemistry, process is a fundamental pathway for the formation of molecular hydrogen cation in the early Universe. , Concerning these last models, however, to include correctly this process in the master equation, rate constants in a collision energy range of 4 orders of magnitude should be inserted, because of the rapid adiabatic expansion (and the consequent cooling) of the Universe in its first ages after the atomic recombination era. In this range of temperatures, of course, different processes (e.g., nonadiabatic and collision-induced dynamics) of the HeH 2 + system can be relevant, so that a pure quantum mechanical approach, although extended to cover a large range of temperatures, has important limitations.…”
Section: Introductionmentioning
confidence: 99%
“…9,56−58 Concerning these last models, however, to include correctly this process in the master equation, rate constants in a collision energy range of 4 orders of magnitude should be inserted, because of the rapid adiabatic expansion (and the consequent cooling) of the Universe in its first ages after the atomic recombination era. In this range of temperatures, of course, different processes (e.g., nonadiabatic 59 and collision-induced dynamics) of the HeH 2 + system can be relevant, so that a pure quantum mechanical approach, although extended to cover a large range of temperatures, has important limitations. The present work is organized as follows: in section 2 some details of the chemical system and of the employed reaction dynamical methods are given; in section 3 the results are shown and reported in different subsections.…”
Section: Introductionmentioning
confidence: 99%
“…Compared with equation (25), reaction (32) has greater interest: as discussed in [87], it occurs on an excited adiabatic potential energy surface of the triatomic system He ‡ ‡ H 2 ; at close distances, the atom± biatom interaction becomes strongly repulsive and the adiabatic surface has avoided crossings with a sequence of upper excited, quasi-Rydberg, states, posing severe problems for the de® nition of the diabatic potentials [57] able to explain the so called R ¤ reaction and the presence of electronically excited hydrogen atoms among the reaction products.…”
Section: Manifolds Of Diabatic Statesmentioning
confidence: 99%