@Article{SilvaAlbeBarrCorr:2017:RaCoCa,
author = "Silva, Washington Barbosa da and Albernaz, Alessandra F. and
Barreto, Patr{\'{\i}}cia Regina Pereira and Correa, Eberth",
affiliation = "Instituto Federal de Educa{\c{c}}{\~a}o, Ci{\^e}ncia e
Tecnologia de Goi{\'a}s and {Universidade de Bras{\'{\i}}lia
(UnB)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidade de Bras{\'{\i}}lia (UnB)}",
title = "Rate constant calculations of the C2 + HCN \→ CCCN+H
addition via the Master Equation",
journal = "Journal of Molecular Modeling",
year = "2017",
volume = "23",
number = "4",
month = "Apr.",
keywords = "C2+HCN addition, Master equation, Pathways, PES, Rate constant.",
abstract = "The addition of C2 to HCN is of relevant interest in
astrochemistry. We studied the pathways of this addition to
produce CCCN and estimated its reaction rate using the Master
Equation in the circumstellar environment. From the results of
this study, it was possible to show that a different pathway in
the Surface Potential Energy-PES can also be investigated. In a
circumstellar envelop environment, with temperatures varying
between 1000 K and 2000 K, the abundances of these species are
favorable to this kind of addition, and our branching ratio for
the rate constant showed that the new pathway is more favorable in
comparison with other possibilities for this range of temperatures
in this environment, and must be taken into account in any
computation of the rate constant.",
doi = "10.1007/s00894-017-3305-0",
url = "http://dx.doi.org/10.1007/s00894-017-3305-0",
issn = "1610-2940",
language = "en",
targetfile = "silva_rate.pdf",
urlaccessdate = "25 abr. 2024"
}