UV photodissociation action spectra of protonated formylpyridines

Author:

McKinnon Benjamin I.1ORCID,Marlton Samuel J. P.1ORCID,Dezalay Jordan2,Soorkia Satchin2ORCID,Blanksby Stephen J.3ORCID,Trevitt Adam J.1ORCID

Affiliation:

1. Molecular Horizons and School of Chemistry and Molecular Bioscience, University of Wollongong, Wollongong, New South Wales 2522, Australia

2. Institut des Sciences Molećulaires d’Orsay (ISMO), CNRS, Université Paris-Sud, Université Paris-Saclay, F-91405 Orsay, France

3. Central Analytical Research Facility and the School of Chemistry and Physics, Queensland University of Technology, Brisbane 4001, Australia

Abstract

The first ππ* transition for protonated 2-, 3-, and 4-formylpyridine (FPH+) ( m/z 108) is investigated by mass spectrometry coupled with photodissociation action spectroscopy at room temperature and 10 K. The photoproduct ions are detected over 35 000–43 000 cm−1, and the major product channel for 3-FPH+ and 4-FPH+ is the loss of CO forming protonated pyridine at m/z 80. For 2-FPH+, the CO loss product is present but a more abundant photoproduct arises from the loss of CH2O to form m/z 78. Plausible potential energy pathways that lead to dissociation are mapped out and comparisons are made to products arising from collision-induced dissociation. Although, in all cases, the elimination of CO is the overwhelming thermodynamically preferred pathway, the protonated 2-FPH+ results suggest that the CH2O product is kinetically driven and competitive with CO loss. In addition, for each isomer, radical photoproduct ions are detected at lower abundances. SCS-CC2/aug-cc-pVTZ Franck–Condon simulations assist with the assignment of vibrionic structure and adiabatic energies (0–0) for 2-FPH+ at 36 560 cm−1, 37 430 cm−1 for 3-FPH+, and 36 140 cm−1 for 4-FPH+, yielding an accurate prediction, on average, within 620 cm−1.

Funder

Australian Research Council

Publisher

AIP Publishing

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

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