The
ion evaporation mechanism (IEM) is perceived to be a major
pathway for disintegration of multi-ion charged droplets found in
atmospheric and sprayed aerosols. However, the precise mechanism of
IEM and the effect of the nature of the ions in the emitted cluster
size distribution have not yet been established despite its broad
use in mass spectrometry and atmospheric chemistry over the past half
century. Here, we present a systematic study of the emitted ion cluster
distribution in relation to their spatial distribution in the parent
droplet using atomistic modeling. It is found that in the parent droplet,
multiple kosmotropic and weakly polarizable chaotropic ions (Cs+) are buried deeper within the droplet than polarizable chaotropic
ions (Cl–, I–). This differentiation
in the ion location is only captured by a polarizable model. It is
demonstrated that the emitted cluster size distribution is determined
by dynamic conical deformations and not by the equilibrium ion depth
within the parent droplet as the IEM models assume. Critical factors
that determine the cluster size distribution such as the charge sign
asymmetry that have not been considered in models and in experiments
are presented. We argue that the existing IEM analytical models do
not establish a clear difference between IEM and Rayleigh fission.
We propose a shift in the existing view for IEM from the equilibrium
properties of the parent droplet to the chemistry in the conical shape
fluctuations that serve as the centers for ion emission. Consequently,
chemistry in the conical fluctuations may also be a key element to
explain charge states of macromolecules in mass spectrometry and may
have potential applications in catalysis due to the electric field
in the conical region.