The detailed description of chemical transformations in the interstellar medium allows deciphering the origin of a number of small and medium - sized organic molecules. We present density functional theory analysis of proton transfer from the trihydrogen cation and the ethenium cation to benzonitrile, a recently discovered species in the Taurus Molecular Cloud 1. Detailed energy transformations along the reaction paths were analyzed using the interacting quantum atoms methodology, which elucidated how the proton carrier influences the lightness to deliver the proton to benzonitrile's nitrogen atom. The proton carriers' deformation energy represents the largest destabilizing effect, whereas a proton's promotion energy, the benzonitrile-proton Coulomb attraction, as well as non-classical benzonitrile-proton and carrier-proton interaction are the dominant stabilizing energy components. As two ion-molecule reactions proceed without energy barriers, rate constants were estimated using the classical capture theory and were found to be an order of magnitude larger for the reaction with the trihydrogen cation compared to that with the ethenium cation (∼10 and 10 cm s, respectively). These results were obtained both with quantum chemical and molecular dynamics simulations (the latter performed at 10 K and 100 K), confirming that up to 100 K both systems choose energetically undemanding routes by tracking the corresponding minimum energy paths. A concept of a turning point is introduced, which is an equivalent to the transition state in barrierless reactions.

Download full-text PDF

Source
http://dx.doi.org/10.1039/d1cp04338bDOI Listing

Publication Analysis

Top Keywords

trihydrogen cation
8
ethenium cation
8
energy
6
proton
5
proton leap
4
leap shuttling
4
shuttling protons
4
protons benzonitrile
4
benzonitrile detailed
4
detailed description
4

Similar Publications

We present a new analytical potential energy surface (PES) for the interaction between the trihydrogen cation and a He atom, , in its electronic ground state. The proposed PES has been built as a sum of two contributions: a polarization energy term due to the electric field generated by the molecular cation at the position of the polarizable He atom, and an exchange-repulsion and dispersion interactions represented by a sum of "atom-bond" potentials between the three bonds of and the He atom. All parameters of this new PES have been chosen and fitted from data obtained from high-level ab-initio calculations.

View Article and Find Full Text PDF

The H-H molecular dimer is of fundamental importance in the study of chemical interactions because of its unique bonding properties and its ability to model more complex systems. The trihydrogen cation H is also a key intermediate in a range of chemical processes in interstellar environments, such as the formation of various organic molecules and early stars. However, the unexpected high abundance of H in molecular clouds remains challenging to explain.

View Article and Find Full Text PDF

The light-driven formation of trihydrogen cation has been attracting considerable attention because of its important role as an initiator of chemical reactions in interstellar clouds. To understand the formation dynamics, most previous studies focused on creating H or D from unimolecular reactions of various organic molecules. Here we observe and characterize the ultrafast formation dynamics of D from a bimolecular reaction, using pump-probe experiments that employ ultrashort laser pulses to probe its formation from a D-D dimer.

View Article and Find Full Text PDF

The detailed description of chemical transformations in the interstellar medium allows deciphering the origin of a number of small and medium - sized organic molecules. We present density functional theory analysis of proton transfer from the trihydrogen cation and the ethenium cation to benzonitrile, a recently discovered species in the Taurus Molecular Cloud 1. Detailed energy transformations along the reaction paths were analyzed using the interacting quantum atoms methodology, which elucidated how the proton carrier influences the lightness to deliver the proton to benzonitrile's nitrogen atom.

View Article and Find Full Text PDF
Article Synopsis
  • The trihydrogen cation is crucial in interstellar chemistry for forming water and complex organic molecules essential for life.
  • Recent research has shifted from using organic materials to generating the trihydrogen cation from just water in a controlled environment using silica nanoparticles and femtosecond laser pulses.
  • This study suggests that natural environments in space, similar to the lab setup, could facilitate the formation of complex molecules through interactions with cosmic rays and solar wind.
View Article and Find Full Text PDF

Want AI Summaries of new PubMed Abstracts delivered to your In-box?

Enter search terms and have AI summaries delivered each week - change queries or unsubscribe any time!