The structure of caustic aluminate solutions in relation to the precipitati
on of gibbsite was investigated using vibrational spectroscopy and molecula
r dynamics simulations. Results from the molecular dynamics simulations ind
icate that aluminate ions form clusters as a function of time and that thes
e clusters are stabilised by sodium ions. While the method used has the lim
itation that bond formation is forbidden, the predicted clustering would ce
rtainly facilitate polyaluminate anion formation. It, is proposed that obse
rved additional bands in vibrational spectra of concentrated aluminate solu
tions, as compared with those of dilute solutions, result from vibrations o
f these clusters (and any polyaluminate ions which arise from them). The ab
sence of spectral features characteristic of a distinct interfacial alumina
te layer at the growing crystal surface is explained by clustering througho
ut the bulk solution, and the participation of such clusters (and polyanion
s) in the growth process.