Simplified Model To Describe The Dissociative Recombination Of Linear Polyatomic Ions Of Astrophysical Interest
Abstract
We present results of a theoretical study on dissociative recombination of the HCNH+, HCO+ and N2H+ linear polyatomic ions at low energies using a simple theoretical model. In the present study, the indirect mechanism for recombination proceeds through the capture of the incoming electron in excited vibrational Rydberg states attached to the degenerate transverse modes of the linear ions. The strength of the non-adiabatic coupling responsible for dissociative recombination is determined directly from the near-threshold scattering matrix obtained numerically using the complex Kohn variational method. The final cross sections for the process are compared with available experimental data. It is demonstrated that at low collision energies, the major contribution to the dissociative recombination cross section is due to the indirect mechanism.
Publication Date
1-1-2015
Publication Title
EPJ Web of Conferences
Volume
84
Document Type
Article; Proceedings Paper
Personal Identifier
scopus
DOI Link
https://doi.org/10.1051/epjconf/20158407003
Copyright Status
Unknown
Socpus ID
84922183517 (Scopus)
Source API URL
https://api.elsevier.com/content/abstract/scopus_id/84922183517
STARS Citation
Douguet, N.; Fonseca Dos Santos, S.; Kokoouline, V.; and Orel, A. E., "Simplified Model To Describe The Dissociative Recombination Of Linear Polyatomic Ions Of Astrophysical Interest" (2015). Scopus Export 2015-2019. 1728.
https://stars.library.ucf.edu/scopus2015/1728