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Semiempirical Potential in Kinetics Calculations on the HC3N + CN Reaction
Authors:Emília Valena Ferreira de Arago  Luca Mancini  Noelia Faginas-Lago  Marzio Rosi  Dimitrios Skouteris  Fernando Pirani
Institution:1.Master-Tec Srl, Via Sicilia 41, 06128 Perugia, Italy; (E.V.F.d.A.); (D.S.);2.Dipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi di Perugia, 06123 Perugia, Italy; (L.M.); (F.P.);3.Dipartimento di Ingegneria Civile ed Ambientale, Università degli Studi di Perugia, 06125 Perugia, Italy
Abstract:The reaction between the cyano radical CN and cyanoacetylene molecule HC3N is of great interest in different astronomical fields, from star-forming regions to planetary atmospheres. In this work, we present a new synergistic theoretical approach for the derivation of the rate coefficient for gas phase neutral-neutral reactions. Statistic RRKM calculations on the Potential Energy Surface are coupled with a semiempirical analysis of the initial bimolecular interaction. The value of the rate coefficient for the HC3N + CN → H + NCCCCN reaction obtained with this method is compared with previous theoretical and experimental investigations, showing strengths and weaknesses of the new presented approach.
Keywords:astrochemistry  ab initio calculations  semiempirical potential energy surface  Improved Lennard–  Jones  chemical reactions  chemical calculations
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