Gravitational Stability of Suspensions of Attractive Colloidal Particles

Chanjoong Kim, Yaqian Liu, Angelika Kühnle, Stephan Hess, Sonja Viereck, Thomas Danner, L. Mahadevan, and David A. Weitz
Phys. Rev. Lett. 99, 028303 – Published 11 July 2007

Abstract

Colloidal suspensions are susceptible to gravitationally induced phase separation. This can be mitigated by the formation of a particle network caused by depletion attraction. The effectiveness of this network in supporting the buoyant weight of the suspension can be characterized by its compressional modulus. We measure the compressional modulus for emulsion networks induced by depletion attraction and present a model that quantitatively predicts their gravitational stability. We also determine the relationship between the strength of the depletion attraction and the magnitude of the compressional modulus.

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  • Received 15 February 2007

DOI:https://doi.org/10.1103/PhysRevLett.99.028303

©2007 American Physical Society

Authors & Affiliations

Chanjoong Kim1,2, Yaqian Liu3, Angelika Kühnle3,*, Stephan Hess3, Sonja Viereck3, Thomas Danner3, L. Mahadevan2, and David A. Weitz1,2

  • 1Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
  • 2DEAS, Harvard University, Cambridge, Massachusetts 02138, USA
  • 3BASF AG, 67056 Ludwigshafen, Germany

  • *Present address: Department of Physics, University of Osnabrück, 49076 Osnabrück, Germany.

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Vol. 99, Iss. 2 — 13 July 2007

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