Iodic acid (IA) has
recently been recognized as a key driver for
new particle formation (NPF) in marine atmospheres. However, the knowledge
of which atmospheric vapors can enhance IA-induced NPF remains limited.
The unique halogen bond (XB)-forming capacity of IA makes it difficult
to evaluate the enhancing potential (EP) of target compounds on IA-induced
NPF based on widely studied sulfuric acid systems. Herein, we employed
a three-step procedure to evaluate the EP of potential atmospheric
nucleation precursors on IA-induced NPF. First, we evaluated the EP
of 63 precursors by simulating the formation free energies (ΔG) of the IA-containing dimer clusters. Among all dimer
clusters, 44 contained XBs, demonstrating that XBs are frequently
formed. Based on the calculated ΔG values,
a quantitative structure–activity relationship model was developed
for evaluating the EP of other precursors. Second, amines and O/S-atom-containing
acids were found to have high EP, with diethylamine (DEA) yielding
the highest potential to enhance IA-induced nucleation by combining
both the calculated ΔG and atmospheric concentration
of considered 63 precursors. Finally, by studying larger (IA)1–3(DEA)1–3 clusters, we found that
the IA-DEA system with merely 0.1 ppt (2.5×106 cm–3) DEA yields comparable nucleation rates to that of
the IA–iodous acid system.