2009
DOI: 10.1063/1.3212625
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Synthesis of interstellar 1,3,5-heptatriynylidyne, C7H(X Π2), via the neutral-neutral reaction of ground state carbon atom, C(P3), with triacetylene, HC6H (X Σ1g+)

Abstract: The reaction of ground-state carbon atom with a polyyne, triacetylene (HC6H) is investigated theoretically by combining ab initio calculations for predicting reaction paths, RRKM theory to yield rate constant for each path, and a modified Langevin model for estimating capturing cross sections. The isomerization and dissociation channels for each of the five collision complexes are characterized by utilizing the unrestricted B3LYP/6-311G(d,p) level of theory and the CCSD(T)/cc-pVTZ calculations. Navigating with… Show more

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Cited by 17 publications
(11 citation statements)
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“…For the biological properties of thiourea derivatives, see; Sun et al (2006); Figueiredo et al (2006). For a related structure, see: Othman et al (2010); For standard bond lengths, see: Allen et al (1987).…”
Section: Related Literaturementioning
confidence: 99%
See 1 more Smart Citation
“…For the biological properties of thiourea derivatives, see; Sun et al (2006); Figueiredo et al (2006). For a related structure, see: Othman et al (2010); For standard bond lengths, see: Allen et al (1987).…”
Section: Related Literaturementioning
confidence: 99%
“…The continuing work on the synthesis of thiourea derivatives is driven by their chemical and biological properties (Sun et al ,2006). Some thiourea derivatives such as N- [1-(4R)…”
Section: Data Collectionmentioning
confidence: 99%
“…However, one of the isomers of SiC 3 , which contains a transannular C–C bond (rhomboidal geometry) has been confirmed in the evolved carbon star, IRC + 10216 based on laboratory rest frequencies . Within C 5 H 2 elemental composition, the elusive aromatic carbene, 2-methylenebicyclo[1.1.0]­but-1(3)-en-4-ylidene ( 9 ; see Figure ), also contains a transannular C–C bond but less attention has been paid to this molecule. Of note, for the confirmation of four C n H 2 carbenes in nonterrestrial environments, identification of the same in laboratories (terrestrial environments) is a crucial factor. ,, Therefore, considering the astrochemical relevance, available laboratory astrophysics data, and enhancing our understanding of structure and bonding of various C n H 2 isomers, where, n = 2, 3, ,,,, 4, ,, 5, 6, ,, 7, ,, 8, ,,, 9, ,,,,…”
Section: Introductionmentioning
confidence: 99%
“…However, we affirm that at the CCSDT(Q)/CBS level of theory including zero-point vibrational energy (ZPVE) corrections at the fc-CCSD(T)/cc-pVTZ level of theory, the linear isomer (1) is the most stable structure (Table 1) on the C 5 H 2 PES. The poor performance of density functional theory (DFT) for similar relative energies has been previously noted in the case of C 7 H 2 isomers, in particular for the low-lying non-linear isomers [59,60,61,62] (see also ref. [63] for a comprehensive survey of the performance of a wide range of DFT methods for challenging structural relative energies).…”
Section: Resultsmentioning
confidence: 73%