Ab initio studies of the Rg-NO+(X1?+) van der Waals complexes (Rg = He, Ne, Ar, Kr, and Xe)

dc.contributor.authorOrek, Cahit
dc.contributor.authorKlos, Jacek
dc.contributor.authorLique, Francois
dc.contributor.authorBulut, Niyazi
dc.date.accessioned2026-08-12T17:32:52Z
dc.date.issued2016
dc.departmentFırat Üniversitesi
dc.description.abstractWe used the explicitly correlated variant of the coupled clusters method with single, double, and noniterative triple excitations [CCSD(T)-F12] to compute two-dimensional potential energy surfaces of van der Waals complexes formed by rare gas atoms (Rg) and NO+(X-1 Sigma(+)) cations. We used the correlation-consistent, triple-zeta (cc-pVTZ-F12) atomic basis sets, and for Kr and Xe rare gases, we employed corresponding pseudopotential cc-pVTZ-PP-F12 atomic basis sets. These basis sets were additionally augmented with mid-bond functions. The complexes are all of skewed T-shape type with Rg atom being closer to the N-side. Using analytical representation of the potentials, we have estimated zero-point energy corrected dissociation energies from anharmonic calculations with BOUND program and also from the harmonic approximation. The binding energies increase with the polarization of the Rg atom in series from He to Xe and are 196 cm(-1), 360 cm(-1), 1024 cm(-1), 1434 cm(-1), and 2141 cm(-1), respectively. Their corresponding dissociation energies are 132 cm(-1), 300 cm(-1), 927 cm(-1), 1320 cm(-1), and 1994 cm(-1) for the complexes with He to Xe, respectively. We find good agreement with previous theoretical and experimental results. The harmonic vibrational frequencies were calculated for the bending and stretching modes of the Rg-NO+ complexes. Published by AIP Publishing.
dc.description.sponsorshipScientific Research Projects Coordination Unit of Firat University [FF.15.03]; U.S. National Science Foundation [CHE-1213332]
dc.description.sponsorshipN.B. and C.O. acknowledge the support by the Scientific Research Projects Coordination Unit of Firat University, Project No. FF.15.03. J.K. acknowledges financial support from the U.S. National Science Foundation through Grant No. CHE-1213332 to M. H. Alexander.
dc.identifier.doi10.1063/1.4950813
dc.identifier.issn0021-9606
dc.identifier.issn1089-7690
dc.identifier.issue20
dc.identifier.orcid0000-0002-3854-1537
dc.identifier.orcid0000-0002-7407-303X
dc.identifier.orcid0000-0002-0664-2536
dc.identifier.orcid0000-0003-2863-7700
dc.identifier.pmid27250302
dc.identifier.scopus2-s2.0-84971291432
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1063/1.4950813
dc.identifier.urihttps://hdl.handle.net/11508/56806
dc.identifier.volume144
dc.identifier.wosWOS:000377712700032
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.indekslendigikaynakPubMed
dc.language.isoen
dc.publisherAip Publishing
dc.relation.ispartofJournal of Chemical Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260511
dc.subjectCenter-Dot-No+
dc.subjectPotential-Energy Surface
dc.subjectCationic Complexes
dc.subjectBound-States
dc.subjectPhotoelectron
dc.subjectPerturbation
dc.subjectGas
dc.titleAb initio studies of the Rg-NO+(X1?+) van der Waals complexes (Rg = He, Ne, Ar, Kr, and Xe)
dc.typeArticle

Dosyalar