Theoretical Characterization of C 3 H and C 5 H and Their Anions
Highly correlated ab initio calculations are employed for the structural and spectroscopic characterization of small odd chains of type C 2n+1 H, considering neutral forms, cations, and giving special attention to the anions. This work confirms the stability of the linear carbon chains and carbon cl...
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Veröffentlicht in: | The Astrophysical journal 2019-02, Vol.871 (2), p.255 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Highly correlated ab initio calculations are employed for the structural and spectroscopic characterization of small odd chains of type C
2n+1
H, considering neutral forms, cations, and giving special attention to the anions. This work confirms the stability of the linear carbon chains and carbon clusters containing three-body rings. The smallest species, C
3
H, displays three stable structures, whereas C
5
H possesses at least 8 neutral isomers and 11 and 10 isomers with a negative or a positive charge. The equilibrium geometries, which can be candidates for laboratory and astrophysical detection, are studied using the RCCSD(T)-F12 and MRCI/CASSCF levels of theory, specifying properties for various electronic states. Four different stable isomers are confirmed for the C
5
H
−
anion. They are two rings and two chains, all showing singlet ground electronic states. The viability of the triplet linear form of C
5
H
−
(
(X
3
Σ
−
)) postulated in previous works, is not confirmed because it appears to be really dependent on the electron correlation energy denoting instability. A quasi-linear singlet (C
s
(X
1
A
′)) represents a secondary minimum. Electronic state crossing occurs close to the linear structure where spin–orbit effects are negligible. The most stable structure of C
5
H
−
is a three-carbon cycle in which rotational constants have been determined to be
A
0
= 35479.86 MHz,
B
0
= 3618.29 MHz, and
C
0
= 3280.10 MHz. Its dipole moment is relatively large (6.4086 D). |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.3847/1538-4357/aafa76 |