by Suliana
Manley
Aggregation is an important process which can be used to
control the viscoelastic properties of colloidal materials. Much has been
done to understand the effect of interparticle interactions
on aggregation. For strong attractions, aggregation can
be described as diffusion-limited, or in the case of a repulsive
barrier, reaction-limited. However, in the presence of gravity,
diffusion becomes less important as the cluster Peclet number
increases. We use a novel, CCD-based low angle dynamic light
scattering
apparatus
to investigate cluster growth under
varying buoyancy mismatch. We have also studied the growth
of the aggregates under microgravity with the
Physics of Colloids in Space project
.
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We study polystyrene and silica colloidal aggregates,
formed by destabilization by the addition of salt. At
a high volume fraction of colloids, the aggregates grow to
fill the sample volume, thus forming an
elastic network, or gel. When the buoyancy mismatch
is high, the gel cannot support its own weight and collapses in time.
This effect is seen in many gelling systems (J. R. Weeks et al., J.
Phys. Cond. Mat. 12 (2000), C. Allain et al., Phys. Rev. Lett. 74 (1995)).
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At lower volume fractions, we can watch the
effect of gravity on the aggregation itself. This leads to a change
in the shape of the measured correlation functions, because the aggregates
are displaced by both diffusion and gravity. This effect becomes more
and more pronounced as the aggregates grow, reflected in the correlation
functions which deviate more and more from a single-exponential decay characteristic
of diffusive motion. In addition, the aggregation rate increases as
the larger aggregates settle faster than the smaller ones, thereby
growing faster than they would by diffusion alone.
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