C. Zagorec-Marks | Searcharxiv

arXiv2026

Vibrational Quantum-State-Controlled Reactivity in the O2+ + C3H4 Reaction

Quantum-state-controlled reactivity is a long-standing goal in the field of physical chemistry. In this work, we explore the vibrational-state-dependent behavior of the ion-molecule reaction between O2+ in distinct vibrational states and two isomers of C3H4, allene (H2C3H2) and propyne (H3C3H). While most products are formed regardless of the vibrational state of O2+, the branching ratios are influenced by vibrational excitation, and a new product, C2O+, appears exclusively in the excited-state reactions. This selective formation of C2O+ demonstrates that vibrational excitation can effectively activate a reaction pathway, providing direct evidence of quantum-state control in reactivity. These results represent an important step towards the goal of quantum-state-controlled chemistry in molecular systems.

physics.chem-ph↗

arXiv2025

Termination of bottom-up interstellar aromatic ring formation at C6H5+

The aromatic molecule benzene is considered the essential building block for larger polycyclic aromatic hydrocarbons (PAHs) in space. Despite benzene's importance in the formation of PAHs, the formation mechanisms of interstellar benzene are not well understood. A single ion-molecule reaction sequence is considered when modeling the formation of benzene in the interstellar medium, beginning with the protonation of acetylene. Although this process has been used to model the initial steps for formation of PAHs, it has not been experimentally measured. To explore this reaction mechanism, we have carried out the first experimental study of sequential ion-molecule reactions beginning with protonation of acetylene at single-collision conditions. Surprisingly, we find that the reaction sequence does not result in benzene and instead terminates at C6H5+, which is unreactive toward both acetylene and hydrogen. This result disproves the previously proposed mechanism for interstellar benzene formation, critically altering our understanding of interstellar PAH formation.

astro-ph.GA↗