Scattering Dynamics and Kinetic Modeling of CN + H2 Reactions Across Interstellar Conditions

Document Type : Research Article

Authors

Department of Chemistry, Yasouj University,7493475918 Yasouj, Iran.

10.24200/sci.2026.68348.11114

Abstract

This study examines the dynamics of collisions between the cyano radical CN and molecular hydrogen H2, as well as their deuterated isotopologues. The investigation employs an interpolated potential energy surface derived from QCISD(T)/6-311++G(d,p) ab initio calculations. Classical trajectory simulations were used to evaluate reaction probabilities and cross sections across a broad range of energies. These quantities were analyzed as functions of fragment translational energy, thereby facilitating the examination of how varying energy inputs affect the probability and efficiency of reaction pathways. To better understand the fundamental dynamics of collisions, we investigated the outcomes of inelastic collisions. This examination focused on the redistribution of the initial kinetic energy, analyzing whether it remained conserved as translational motion or was converted into the internal energy of the reaction products. Furthermore, the relationship between the deflection angles and both the impact parameter and the relative translational energy of the colliding entities was evaluated. Rate constants were determined from the calculated cross sections using nonlinear least-squares fitting, thereby enabling the development of quantitative models to characterize the observed kinetics. The investigation of the isotope effect was conducted by substituting deuterium for hydrogen. A method in which the effects of target and incident molecules' mass on cross sections, reaction probabilities, scattering angles, and overall reaction rates are clarified. This comprehensive approach provided an in-depth analysis of the factors influencing collisions between the cyano radical and molecular hydrogen and its isotopic variants.

Keywords

Main Subjects



Articles in Press, Accepted Manuscript
Available Online from 18 July 2026
  • Receive Date: 01 December 2025
  • Revise Date: 08 May 2026
  • Accept Date: 07 June 2026