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Excited State Trends in Bidirectionally Expanded Closed-Shell PAH and PANH Anions.
Ryan C Fortenberry1, Megan M Moore1, Timothy J Lee2
1Department of Chemistry, Georgia Southern University , Statesboro, Georgia 30460, United States.
Closed-shell polycyclic aromatic hydrocarbons (PAHs) and nitrogen-containing PAHs (PANHs) can exhibit unique excited states. This study identifies the structural requirements for these valence excited states in PAHs and PANHs.
Area of Science:
- Physical Chemistry
- Astrochemistry
- Quantum Chemistry
Background:
- Certain anions possess intrinsic excited states, independent of external influences.
- These states arise from the stabilization of valence orbitals, where electron binding energy exceeds valence excitation energy.
- Closed-shell anions are prime candidates due to their inherent stability from spin-paired ground states.
Purpose of the Study:
- To determine the critical structural features in deprotonated polycyclic aromatic hydrocarbons (PAHs) and nitrogen-containing PAHs (PANHs) that lead to valence excited states.
- To establish a general trend for the occurrence of these excited states in PAHs/PANHs of varying sizes and dimensionalities.
Main Methods:
- Theoretical analysis of electronic structure and stability of closed-shell anions.
- Investigation of valence accepting orbital stabilization and electron binding energies.
- Establishing a correlation between molecular size (number of six-membered rings) and the onset of valence excited states.
Main Results:
- A general trend for the emergence of valence excited states in PAHs/PANHs is established, applicable to various sizes and dimensions.
- Valence excited states are present in PAHs/PANHs once they comprise seven six-membered rings.
- For most PAH/PANH classes, this critical number of rings is closer to four.
Conclusions:
- Deprotonated, closed-shell PAHs and PANHs can exhibit intrinsic valence excited states.
- The size and structure of PAHs/PANHs dictate the presence of these excited states, with a general threshold identified.
- Despite potentially weak absorption, the abundance of PAHs in astronomical environments suggests their significant contribution to observed spectra.
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