2015
DOI: 10.1039/c5sm01551k
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Depletion, melting and reentrant solidification in mixtures of soft and hard colloids

Abstract: We present extensive experimental and theoretical investigations on the structure, phase behavior, dynamics and rheology of model soft-hard colloidal mixtures realized with large, multiarm star polymers as the soft component and smaller, compact stars as the hard one. The number and length of the arms in star polymers control their softness, whereas the size ratio, the overall density and the composition are additional parameters varied for the mixtures. A coarse-grained theoretical strategy is employed to pre… Show more

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Cited by 26 publications
(34 citation statements)
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“…We present a comparative rheological investigation of different states of asymmetric binary softhard colloid mixtures. Using the same system studied before [61], [62], we extend our earlier studies and report on the transient nonlinear rheology (evolution and relaxation of stress under constant shear, response to large amplitude oscillatory shear deformation) of RG, APS and DG states. We discuss the phenomenological link of the rheological properties to morphology and compare simple repulsive glasses from hard spheres, microgels and stars.…”
Section: Introductionmentioning
confidence: 87%
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“…We present a comparative rheological investigation of different states of asymmetric binary softhard colloid mixtures. Using the same system studied before [61], [62], we extend our earlier studies and report on the transient nonlinear rheology (evolution and relaxation of stress under constant shear, response to large amplitude oscillatory shear deformation) of RG, APS and DG states. We discuss the phenomenological link of the rheological properties to morphology and compare simple repulsive glasses from hard spheres, microgels and stars.…”
Section: Introductionmentioning
confidence: 87%
“…In general, the increase of   with particle concentration is attributed to the reduced free volume due to crowding [68]. Furthermore, in the DG state both depletants and depleted particles freeze, the elastic modulus increases sharply ( Figure 6) while the soft stars shrink due to the osmotic pressure exerted by the HS-like stars [62]. Indeed, taking into account the mean-field pressure exerted by the HS-like stars [62] for cHS>40 % wt, soft stars become dramatically squeezed and assume a collapsed configuration akin to that observed under poor solvency conditions.…”
Section: Iii1 Linear Viscoelasticitymentioning
confidence: 99%
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