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dc.creatorSenent, M. L.en_US
dc.creatorBrites, V.en_US
dc.creatorHochlaf, M.en_US
dc.date.accessioned2010-07-12T14:16:55Z
dc.date.available2010-07-12T14:16:55Z
dc.date.issued2010en_US
dc.identifier2010-TI-02en_US
dc.identifier.urihttp://hdl.handle.net/1811/46292
dc.descriptionAuthor Institution: Departamento de Astrofisica Molecular e Infrarroja; Instituto de Estructura de la Materia, C.S.I.C., Serrano 121; Madrid 28006, SPAIN; Universite Paris-Est, Laboratoire de Modelisation et; Simulation Multi Echelle, MSME FRE 3160 CNRS, 5 boulevard Descartes; 77454 Marne-la-Vallee, FRANCEen_US
dc.description.abstractUsing state-of-the-art theoretical methods, we investigate the stable isomers of $C_4^-$, $C_4$H and $C_4H^-$. Three of them are relevant for astrophysics and astrochemistry. These computations are performed using interaction configuration ab initio methods and the aug-cc-pVXZ (X=T,Q) basis sets. In addition to the linear isomers, we predict the existence of several cyclic and branched forms for these molecules. For all the molecular species of interest here, sets of spectroscopic parameters are determined with perturbation theory, which compare quite well with experiment. For $\it{l}-C_4H^- (X^1\Sigma^+)$, the quartic force field is computed at the coupled cluster level of theory. This force field is derived from full nine-dimensional potential energy surface generated close to the equilibrium geometry of this anion. Finally, we treat the photochemistry processes of the hydrogen attachment and the electron attachment reactions that may lead to the formation of the $C_4H^-$ from either $C_4^-$ or $C_4H$.en_US
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleCHARACTERIZATION AND FORMATION PROCESSES OF $C_4^-$, $C_4H$ and $C_4H^-$en_US
dc.typeArticleen_US
dc.typeImageen_US
dc.typePresentationen_US


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