2019
DOI: 10.1021/acs.jpca.9b01879
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Why Do Large Ionized Polycyclic Aromatic Hydrocarbons Not Lose C2H2?

Abstract: The reaction mechanisms for the loss of C2H2 from the ions of anthracene, phenanthrene, tetracene, and pyrene were calculated at the B3-LYP/6-311++G­(2d,p) level of theory and compared to that previously published for ionized naphthalene. A common pathway emerged involving the isomerization of the molecular ions to azulene-containing analogues, followed by the contraction of the seven-member ring into a five- and four-member fused ring system, leading to the cleavage of C2H2. The key transition state was found… Show more

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Cited by 33 publications
(39 citation statements)
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“…With regard to the loss of a C 2 H 2 unit, pathways similar to those described by Trinquier et al (2017b) and West et al (2019) for Pyr + were verified. Like Pyr + , 1EtyPyr + features direct routes for the loss of C 2 H 2 from an inner ring or from an outer one (respectively dissociation types 1 and 2 in Trinquier et al 2017b).…”
Section: Theoretical Dissociation Pathssupporting
confidence: 76%
“…With regard to the loss of a C 2 H 2 unit, pathways similar to those described by Trinquier et al (2017b) and West et al (2019) for Pyr + were verified. Like Pyr + , 1EtyPyr + features direct routes for the loss of C 2 H 2 from an inner ring or from an outer one (respectively dissociation types 1 and 2 in Trinquier et al 2017b).…”
Section: Theoretical Dissociation Pathssupporting
confidence: 76%
“…34,35 Furthermore, many studies on the larger PAH species have shown a trend for smaller and irregular PAHs to be more likely to lose [2C,2H] than H or H 2 upon photofragmentation. [36][37][38][39][40][41][42] It would thus be of great interest to find out if phenylium follows this trend.…”
Section: Introductionmentioning
confidence: 99%
“…However, for pericondensed PAHs, including pyrene, loss of C 2 H 2 is inhibited because a key transition state is too high in energy. 10 Indeed, experiments reveal that for PAHs in the astrophysically-relevant size range (50-100 carbon atoms), fragmentation is dominated by hydrogen-loss until mostif not all -hydrogen atoms are lost. 8,10,11 For completeness, we mention that in regions with high atomic hydrogen density and low UV fields, interstellar PAHs can be superhydrogenated (i.e.…”
Section: Introductionmentioning
confidence: 99%
“…10 Indeed, experiments reveal that for PAHs in the astrophysically-relevant size range (50-100 carbon atoms), fragmentation is dominated by hydrogen-loss until mostif not all -hydrogen atoms are lost. 8,10,11 For completeness, we mention that in regions with high atomic hydrogen density and low UV fields, interstellar PAHs can be superhydrogenated (i.e. some or all of the edge carbon atoms have acquired an additional hydrogen atom).…”
Section: Introductionmentioning
confidence: 99%