Model of heap formation in vibrated gravitational suspensions

Hiroyuki Ebata and Masaki Sano
Phys. Rev. E 92, 053016 – Published 23 November 2015

Abstract

In vertically vibrated dense suspensions, several localized structures have been discovered, such as heaps, stable holes, expanding holes, and replicating holes. Because an inclined free fluid surface is difficult to maintain because of gravitational pressure, the mechanism of those structures is not understood intuitively. In this paper, as a candidate for the driving mechanism, we focus on the boundary condition on a solid wall: the slip-nonslip switching boundary condition in synchronization with vertical vibration. By applying the lubrication approximation, we derived the time evolution equation of the fluid thickness from the Oldroyd-B fluid model. In our model we show that the initially flat fluid layer becomes unstable in a subcritical manner, and heaps and convectional flow appear. The obtained results are consistent with those observed experimentally. We also find that heaps climb a slope when the bottom is slightly inclined. We show that viscoelasticity enhances heap formation and climbing of a heap on the slope.

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  • Received 8 July 2015
  • Revised 19 October 2015

DOI:https://doi.org/10.1103/PhysRevE.92.053016

©2015 American Physical Society

Authors & Affiliations

Hiroyuki Ebata* and Masaki Sano

  • Department of Physics, Graduate School of Sciences, Kyushu University, Fukuoka 812-8581, Japan

  • *ebata@phys.kyushu-u.ac.jp
  • Also at Department of Physics, Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan; sano@phys.s.u-tokyo.ac.jp

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Vol. 92, Iss. 5 — November 2015

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