Abstract

We present the non-adiabatic, conical-intersection quantum dynamics of the title collision where reactants and products are in the ground electronic states. Initial-state-resolved reaction probabilities, total integral cross sections, and rate constants of two H2 vibrational states, v0 = 0 and 1, in the ground rotational state (j0 = 0) are obtained at collision energies Ecoll ≤ 3 eV. We employ the lowest two excited diabatic electronic states of and their electronic coupling, a coupled-channel time-dependent real wavepacket method, and a flux analysis. Both probabilities and cross sections present a few groups of resonances at low Ecoll, whose amplitudes decrease with the energy, due to an ion-induced dipole interaction in the entrance channel. At higher Ecoll, reaction probabilities and cross sections increase monotonically up to 3 eV, remaining however quite small. When H2 is in the v0 = 1 state, the reactivity increases by ~2 orders of magnitude at the lowest energies and by ~1 order at the highest ones. Initial-state resolved rate constants at room temperature are equal to 1.74 × 10−14 and to 1.98 × 10−12 cm3s−1 at v0 = 0 and 1, respectively. Test calculations for H2 at j0 = 1 show that the probabilities can be enhanced by a factor of ~1/3, that is ortho-H2 seems ~4 times more reactive than para-H2.

Highlights

  • Atomic Hydrogen and Helium are the dominant chemical species of the early Universe (Galli andPalla, 2013) and of the interstellar medium, and are ionized by cosmic rays

  • We have taken into account the non-adiabatic conical intersection (CI) coupling between the first two excited diabatic potential energy surface (PES) of HeH+2

  • Dynamical calculations are performed for the ground and first excited vibrational states of H2, for investigating vibrational effects on the DCT dynamics, and collision energies up to 3 eV are considered

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Summary

Introduction

Atomic Hydrogen and Helium are the dominant chemical species of the early Universe (Galli andPalla, 2013) and of the interstellar medium, and are ionized by cosmic rays. A few works have theoretically investigated the dynamics of the DCT collision since 1994, when Aguillon (1994) employed a semiclassical coupled wavepacket (WP) method and the analytical diabatic PESs of Aguado et al (1993) for computing ICSs for ground and excited vibrational states v0 of H2, up to v0 = 4 and in the Ecoll range from 2 to 10 eV.

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