Abstract
Atmospheric new particle formation (NPF) events can be driven by iodine oxides or oxoacids via both neutral and ionic mechanisms. Photolysis of new particles likely plays a significant role in their growth mechanisms, but their spectra and their photolysis mechanisms remain difficult to characterize. We recorded UV photodissociation spectra of (I2O5)0-3(IO3-) clusters, observing O atom, I2O4, and (I2O5)1,2 fragments in the atmospherically-relevant range 300-340 nm. With increasing cluster size, absorption red shifts and generally increases in intensity, suggesting particles photolyze more frequently as they grow. Estimates of the rates indicate that even relatively small clusters are likely to undergo photolysis in ambient conditions. Vibrational spectra identify the covalent moiety I3O8- as the likely chromophore, not IO3-. The (I2O5)-loss pathway competes with particle growth while the slower O loss pathway likely produces triplet O + triplet cluster products that could drive subsequent intra-particle chemistry, particularly with co-adsorbed organic or amine species.
Supplementary materials
Title
Supplementary Information
Description
The Supporting Information contains additional experimental spectra comparisons, collision induced dissociation mass spectra, and details on how rates were calculated. Further information on singlet versus triplet calculations, adiabatic detachment energy calculations, detection efficiency correction factors, and coordinates for all of the computed clusters are also reported.
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