2017
DOI: 10.1021/acs.jpca.6b10094
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A Quantum Mechanical Study of the kj and k′–j′ Vector Correlations for the H + LiH → Li + H2 Reaction

Abstract: We have characterized the stereodynamics of the H + LiH (v = 0, j = 0-1) reactive collisions leading to H formation through the quantum mechanical analysis of the k-j and k'-j' vector correlations that describe the polarization of the reactants and products, respectively. Our results, which cover the collision energy interval between 10 and 1 eV, are unexpectedly complex given the apparent simplicity and featureless nature of the potential energy surface for the LiH system and point toward the existence of a d… Show more

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Cited by 7 publications
(2 citation statements)
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“…The WCBG-PES, PMM-PES, and YHC-PES were widely used in recent years. Specifically, the dynamics properties of the reaction were studied in detail based on these PESs, including reaction probability, , integral cross section (ICS), ,, differential cross section (DCS), ,,, thermal rate constant, ,,, and stereodynamics, ,, among others. In contrast, the reaction has received limited theoretical attention.…”
Section: Introductionmentioning
confidence: 99%
“…The WCBG-PES, PMM-PES, and YHC-PES were widely used in recent years. Specifically, the dynamics properties of the reaction were studied in detail based on these PESs, including reaction probability, , integral cross section (ICS), ,, differential cross section (DCS), ,,, thermal rate constant, ,,, and stereodynamics, ,, among others. In contrast, the reaction has received limited theoretical attention.…”
Section: Introductionmentioning
confidence: 99%
“…Given its important role in stellar evolution and the galactic lithium production of the primitive universe, the past few decades have witnessed progressive interest in the gas-phase lithium chemistry system, such as LiH 2 [1][2][3][4] and LiH 2 + . [5][6][7][8] Indeed, LiH and its ionic variants are primarily formed by the radiative association process during the recombination era and LiH + is more abundant than LiH due to the fact that the latter is mainly ionized at low redshifts.…”
Section: Introductionmentioning
confidence: 99%