Superhydrogenation of pentacene: the reactivity of zigzag-edges

Investigating the hydrogenation of carbonaceous materials is of interest in a wide range of research areas including electronic device development, hydrogen storage, and, in particular, astrocatalytic formation of molecular hydrogen in the universe. Polycyclic Aromatic Hydrocarbons (PAHs) are ubiqui...

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Veröffentlicht in:Physical chemistry chemical physics : PCCP 2020-01, Vol.22 (3), p.1557-1565
Hauptverfasser: Campisi, Dario, Simonsen, Frederik Doktor S, Thrower, John D, Jaganathan, Rijutha, Hornekær, Liv, Martinazzo, Rocco, Tielens, Alexander G. G. M
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Sprache:eng
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Zusammenfassung:Investigating the hydrogenation of carbonaceous materials is of interest in a wide range of research areas including electronic device development, hydrogen storage, and, in particular, astrocatalytic formation of molecular hydrogen in the universe. Polycyclic Aromatic Hydrocarbons (PAHs) are ubiquitous in space, locking up close to 15% of the elementary carbon. We have used thermal desorption measurements to study the hydrogenation sequence of pentacene from adding one additional H to the fully hydrogenated pentacene species. The experiments reveal that hydrogenated species with an even number of excess H atoms are highly preferred over hydrogenated species with an odd number of H atoms. In addition, the experiments show that specific hydrogenation states of pentacene with 2, 4, 6, 10, 16 and 22 extra H atoms are preferred over other even numbers. We have investigated the structural stability and activation energy barriers for the superhydrogenation of pentacene using Density Functional Theory. The results reveal a preferential hydrogenation pattern set by the activation energy barriers of the hydrogenation steps. Based on these studies, we formulate simple concepts governing the hydrogenation that apply equally well for different PAHs. Studies of pentacene hydrogenation reveal a preferential hydrogenation sequence. The guiding concepts apply more broadly to aromatic carbonaceous systems and may be crucial in catalytic formation of molecular hydrogen in interstellar space.
ISSN:1463-9076
1463-9084
DOI:10.1039/c9cp05440e