Gao XF, Xie JC, Li H, Meng X, Wu Y, Tian SX. Direct observation of long-lived cyanide anions in superexcited states.
Commun Chem 2021;
4:13. [PMID:
36697555 PMCID:
PMC9814559 DOI:
10.1038/s42004-021-00450-0]
[Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/25/2020] [Accepted: 01/07/2021] [Indexed: 01/28/2023] Open
Abstract
The cyanide anion (CN-) has been identified in cometary coma, interstellar medium, planetary atmosphere and circumstellar envelopes, but its origin and abundance are still disputed. An isolated CN- is stabilized in the vibrational states up to ν = 17 of the electronic ground-state 1Σ+, but it is not thought to survive in the electronic or vibrational states above the electron autodetachment threshold, namely, in superexcited states. Here we report the direct observation of long-lived CN- yields of the dissociative electron attachment to cyanogen bromide (BrCN), and confirm that some of the CN- yields are distributed in the superexcited vibrational states ν ≥ 18 (1Σ+) or the superexcited electronic states 3Σ+ and 3Π. The triplet state can be accessed directly in the impulsive dissociation of BrCN- or by an intersystem transition from the superexcited vibrational states of CN-. The exceptional stability of CN- in the superexcited states profoundly influences its abundance and is potentially related to the production of other compounds in interstellar space.
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