Polyol–water
clusters provide a template to probe ionization
and solvation processes of paramount interest in atmospheric and interstellar
chemistry. We generate glycerol water clusters in a continuous supersonic
jet expansion and interrogate the neutral species with synchrotron-based
tunable vacuum ultraviolet photoionization mass spectrometry. A series
of glycerol fragments (m/z 44, 61,
62, and 74) clustered with water are observed. A judicious combination
of backing pressure, nozzle temperature, and water vapor pressure
allows for tuning the mol % of glycerol. The recorded appearance energies
of the water cluster series m/z 62
and 74 are similar to that observed in pure glycerol, while the m/z 61 series shows a dependence on cluster
composition. Furthermore, this series also tracks the water concentration
of the beam. Theoretical calculations on neutral and ionized clusters
visualize the hydrogen bond network in these water clusters and provide
an assessment of the number of glycerol–glycerol, glycerol–water,
and water–water hydrogen bonds in the cluster, as well as their
interaction energies. This method of bond counting and interaction
energy assessment explains the changes in the mass spectrum as a function
of mol % and offers a glimpse of the disruption of the hydrogen bond
network in glycerol–water clusters. The calculations also reveal
interesting barrierless chemical processes in photoionized glycerol
water clusters that are either activated or do not occur without the
presence of water. Examples include spontaneous intramolecular proton
transfer within glycerol to form a distonic ion, nonactivated breaking
of a C–C bond, and spontaneous proton transfer from glycerol
to water. These results appear relevant to radiation-induced chemical
processing of alcohol–water ices in the interstellar medium.