Rheology of moderated dilute suspensions of star colloids: the shape factor

Fuente: arXiv
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Main Authors: Usabiaga, F. Balboa, Ellero, M.
Format: Preprint
Published: 2023
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author Usabiaga, F. Balboa
Ellero, M.
author_facet Usabiaga, F. Balboa
Ellero, M.
contents Star colloids are rigid particles with long and slender arms connected to a central core. We show numerically that the colloid shapes control the rheology of their suspensions. In particular, colloids with curved arms and hooks can entangle with neighbor particles and form large clusters that can sustain high stresses. When a large cluster permeates the whole system the viscosity increases many fold. Contrary to the case of spherical colloids we observe that these effects are very strong even at moderate volumes fraction over a wide range of Péclet numbers.
format Preprint
id arxiv_https___arxiv_org_abs_2311_14166
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Rheology of moderated dilute suspensions of star colloids: the shape factor
Usabiaga, F. Balboa
Ellero, M.
Soft Condensed Matter
Star colloids are rigid particles with long and slender arms connected to a central core. We show numerically that the colloid shapes control the rheology of their suspensions. In particular, colloids with curved arms and hooks can entangle with neighbor particles and form large clusters that can sustain high stresses. When a large cluster permeates the whole system the viscosity increases many fold. Contrary to the case of spherical colloids we observe that these effects are very strong even at moderate volumes fraction over a wide range of Péclet numbers.
title Rheology of moderated dilute suspensions of star colloids: the shape factor
topic Soft Condensed Matter
url https://arxiv.org/abs/2311.14166