A theoretical investigation of the possible detection of C24 in space

Bibcode
2020FNCN...28..637S
DOI
10.1080/1536383X.2020.1731735
Sadjadi, SeyedAbdolreza; Kwok, Sun; Cataldo, Franco; García-Hernández, D. A.; Manchado, Arturo
Bibliographical reference

Fullerene Nanotubes and Carbon Nanostructures

Advertised on:
8
2020
Number of authors
5
IAC number of authors
2
Citations
4
Refereed citations
4
Description
Astronomical infrared spectral features at ~6.6, 9.8 and 20 micronm have recently been suggested as being due to the planar graphene form of C24 carbon cluster. Here we report density functional theory and coupled cluster calculations on wavefunctions stability, relative energies, and infrared spectra of four different types of C24 isomers, including the graphene and fullerene forms. The types of vibrational motions under these bands are also discussed. Among the four isomers, we find that the astronomical data are best approximated by the graphene form of C24.
Related projects
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Nucleosynthesis and molecular processes in the late stages of Stellar Evolution

Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars are important contributors to the enrichment of the

Domingo Aníbal
García Hernández
In progress
Type
Refereed
Exoplanetary Systems & Solar System (SEYSS)
Stellar & Interstellar Physics (FEEI)
The Milky Way and the Local Group (MWLG)

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