Abstract

Ionization and subsequent isomerization of organic molecules has been suggested as an important source of trihydrogen H_{3}^{+} cations in outer space. The high interest in such reactions has initiated many experimental and theoretical studies for various molecules. Here, we report measurements as well as abinitio molecular dynamics simulations on the fragmentation of dicationic methanol monomers and clusters ionized by low-energy (90eV) electrons. Experimentally, for dicationic monomers, a fragmentation channel for the formation of H_{3}^{+} in coincidence with a COH^{+} cation is observed. The simulations show that an intermediate neutral H_{2} is formed in the first step, and its roaming around the dication ends in the formation of H_{3}^{+}. The entire reaction takes about 100-500fs. The calculated kinetic energy release for the H_{3}^{+}+COH^{+} ion pair is in excellent agreement with the experimental result. In contrast, for the dicationic clusters, due to the possibility of distributing the two charges onto different molecules, several fast dissociation channels occur and suppress the roaming of H_{2} and formation of H_{3}^{+}. The present Letter suggests that the quenching of H_{3}^{+} formation by the chemical environment is a general phenomenon in dicationic clusters of organic molecules.

Highlights

  • The trihydrogen Hþ3 cation is the most prevalent molecular ion in interstellar space and plays an important role in astrochemistry due to its high activity in initiating various chemical reactions in interstellar clouds [1]

  • The present Letter suggests that the quenching of Hþ3 formation by the chemical environment is a general phenomenon in dicationic clusters of organic molecules

  • The fast separation inhibits the roaming mechanism of H2 in ðM-HÞþ. These results indicate that the direct Coulomb explosion (CE) and PTMCE processes in the dicationic dimers are faster than the roaming mechanism of H2 and quench the production of Hþ3

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Summary

Published by the American Physical Society

NH3, and CH3OH) by ultraviolet (UV) photons in the laboratory has produced a suite of organic molecules including amino acids, amphiphiles, quinones, and nucleobases [31]. Thereby, in our molecular dynamics calculations of methanol dimers and larger clusters, we consider the charge-delocalized Mþ · Mþ dication as the initial state. In principle, this state can be produced by other ionization mechanisms like the intermolecular Coulombic decay [43,44,45] or by sequential ionization where the projectile electron successively kicks out one electron from each molecule of the methanol dimer and, leads to the Mþ · Mþ state. We start the dynamical simulation from the obtained initial atomic configuration and a vertical transition to the electronic ground state of the doubly charged methanol molecule (Mþþ) or dimer or larger cluster (Mþ · Mþ).

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