The agglomeration of titania particles with radii ranging from 20 to 40 nm
was simulated based on the colloidal stability using van der Waals attracti
on and the electrostatic repulsion energy. With an increase in particle rad
ius from 20 to 40 nm, the shape of the energy barrier was changed to allow
the bigger particles to agglomerate more easily. For the zeta potential inc
rease from 4.5 to 16.8 mV, both the height and width of the energy barrier
increased to make the dispersed state stable. This tendency explains the ex
perimentally observed agglomeration behaviour where smaller particles with
higher zeta potential exhibited higher stability but formed bigger and hard
er agglomerates with irregular shapes after drying.