A theoretical study of the dissociative recombination of SH with electrons through the states of SH
arXiv:2405.20147 · doi:10.1063/1.4983690
Abstract
A quantitative theoretical study of the dissociative recombination of SH with electrons has been carried out. Multireference, configuration interaction calculations were used to determine accurate potential energy curves for SH and SH. The block diagonalization method was used to disentangle strongly interacting SH valence and Rydberg states and to construct a diabatic Hamiltonian whose diagonal matrix elements provide the diabatic potential energy curves. The off-diagonal elements are related to the electronic valence-Rydberg couplings. Cross sections and rate coefficients for the dissociative recombination reaction were calculated with a step-wise version of the multichannel quantum defect theory, using the molecular data provided by the block diagonalization method. The calculated rates are compared with the most recent measurements performed on the TSR ion storage ring in Heidelberg, Germany.
17 pages, 15 figures, 4 tables
References in corpus (5)
- The chemistry of ions in the Orion Bar I. - CH+, SH+, and CF+: The effect of high electron density and vibrationally excited H2 in a warm PDR surface
- Chemical probes of turbulence in the diffuse medium: the TDR model
- Rotational transitions induced by collisions of HD ions with low energy electrons
- Dissociative recombination, and vibrational excitation of CO: model calculations and comparison with experiment
- Dissociative recombination and vibrational excitation of BF in low energy electron collisions
Cited by in corpus (5)
- Low-energy electron impact dissociative recombination and vibrational transitions of N
- Electron-induced excitation, recombination and dissociation of molecular ions initiating the formation of complex organic molecules
- Dissociative recombination of the CH molecular ion at low energy
- Dissociative recombination and rotational transitions of D in collisions with slow electrons
- Population of ground and lowest excited states of Sulfur via the dissociative recombination of SH+ in the diffuse interstellar medium