Abstract
| Nucleation of neutral iodine particles has recently
been found to involve both iodic acid (HIO3) and iodous acid
(HIO2). However, the precise role of HIO2 in iodine oxoacid
nucleation remains unclear. Herein, we probe such a role by
investigating the cluster formation mechanisms and kinetics of
(HIO3)m(HIO2)n (m = 0−4, n = 0−4) clusters with quantum
chemical calculations and atmospheric cluster dynamics modeling.
When compared with HIO3, we find that HIO2 binds more strongly
with HIO3 and also more strongly with HIO2. After accounting for
ambient vapor concentrations, the fastest nucleation rate is
predicted for mixed HIO3−HIO2 clusters rather than for pure
HIO3 or HIO2 ones. Our calculations reveal that the strong binding
results from HIO2 exhibiting a base behavior (accepting a proton
from HIO3) and forming stronger halogen bonds. Moreover, the binding energies of (HIO3)m(HIO2)n clusters show a far more
tolerant choice of growth paths when compared with the strict stoichiometry required for sulfuric acid−base nucleation. Our
predicted cluster formation rates and dimer concentrations are acceptably consistent with those measured by the Cosmic Leaving
Outdoor Droplets (CLOUD) experiment. This study suggests that HIO2 could facilitate the nucleation of other acids beyond HIO3
in regions where base vapors such as ammonia or amines are scarce. |