Carbon blacks are made up of near-spherical elementary colloidal particles
chained together in small clusters known as aggregates. These unique morpho
logical characteristics have complicated their particle size characterizati
on by conventional techniques. In this study the potential of mercury poros
imetry for the generation of primary particle size distributions (PPSD) of
carbon blacks is investigated. Two literature theories (Mayer-Stowe and Smi
th-Stermer) were applied to derive PPSD curves from mercury porosimetry ana
lyses of six ASTM standard reference blacks (series SRB A5-F5) covering a w
ide range of particle sizes. Good agreement was found between particle size
s expected from electron microscopy and those determined by mercury porosim
etry. The advantages of the latter technique for the routine evaluation of
continuous PPSD curves are discussed.