Experimental and theoretical studies are presented on the reactions of the isomeric radical cations H2CNH•+ and HCNH2•+ with CH4. Ionic isomers were generated selectively by VUV dissociative photoionization of azetidine and cyclopropylamine precursors respectively. Both exclusively give H2CNH2+ plus CH3• as products, but differences are observed related to a competition between stripping and complex-mediated H-transfer. Astrochemical implications for Titan’s atmosphere are briefly discussed, where the presence of methanimine (H2CNH), a key prebiotic molecule and a potential precursor for tholins, is proposed on the basis of atmospheric models and the observation of CH2NH2+ ions in Cassini mass spectrometric data.
The reactivity of methanimine radical cation (H2CNH•+) and its isomer aminomethylene (HCNH2•+) with methane / Richardson, Vincent; Alcaraz, Christian; Geppert Wolf, D; Polasek, Miroslav; Romanzin, Claire; Sundelin, David; Thissen, Roland; Tosi, Paolo; Zabka, Jan; Ascenzi, Daniela. - In: CHEMICAL PHYSICS LETTERS. - ISSN 0009-2614. - STAMPA. - 775:(2021), pp. 138611.1-138611.7. [10.1016/j.cplett.2021.138611]
The reactivity of methanimine radical cation (H2CNH•+) and its isomer aminomethylene (HCNH2•+) with methane
Richardson, Vincent;Tosi, Paolo;Ascenzi, Daniela
2021-01-01
Abstract
Experimental and theoretical studies are presented on the reactions of the isomeric radical cations H2CNH•+ and HCNH2•+ with CH4. Ionic isomers were generated selectively by VUV dissociative photoionization of azetidine and cyclopropylamine precursors respectively. Both exclusively give H2CNH2+ plus CH3• as products, but differences are observed related to a competition between stripping and complex-mediated H-transfer. Astrochemical implications for Titan’s atmosphere are briefly discussed, where the presence of methanimine (H2CNH), a key prebiotic molecule and a potential precursor for tholins, is proposed on the basis of atmospheric models and the observation of CH2NH2+ ions in Cassini mass spectrometric data.File | Dimensione | Formato | |
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