Gravitational Collapse of Colloidal Gels

S. Manley, J. M. Skotheim, L. Mahadevan, and D. A. Weitz
Phys. Rev. Lett. 94, 218302 – Published 3 June 2005

Abstract

We present a unified framework for understanding the compaction of colloidal gels under their own weight. The dynamics of the collapse are determined by the value of the gravitational stress σg, as compared to the yield stress σY of the network. For σg<σY, gels collapse poroelastically, and their rate of compression decays exponentially in time. For σg>σY, the network eventually yields, leading to rapid settling. In both cases, the rate of collapse is backflow limited, while its overall magnitude is determined by a balance between gravitational stress and network elastic stress.

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  • Received 13 December 2004

DOI:https://doi.org/10.1103/PhysRevLett.94.218302

©2005 American Physical Society

Authors & Affiliations

S. Manley, J. M. Skotheim, L. Mahadevan, and D. A. Weitz

  • Department of Physics & DEAS, Harvard University, Cambridge, Massachusetts 02138, USA

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Vol. 94, Iss. 21 — 3 June 2005

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