Stability of dancing Volvox. (25th November 2020)

• Record Type: Journal Article
• Authors: Ishikawa, Takuji; Pedley, T. J.; Drescher, Knut; Goldstein, Raymond E.
• Is Part Of: Journal of fluid mechanics. Volume 903(2020)
• Publication Date: 2020-11-25
• Subjects: micro-organism dynamics, -- swimming/flying; Fluid mechanics -- Periodicals; 532.005
• DOI: 10.1017/jfm.2020.613
• Languages: English
• ISSNs: 0022-1120

Abstract

Abstract: Abstract : Biflagellate algal cells of the genus Volvox form spherical colonies that propel themselves, vertically upwards in still fluid, by the coordinated beating of thousands of flagella, that also cause the colonies to rotate about their vertical axes. When they are swimming in a chamber of finite depth, pairs (or more) of Volvox carteri colonies were observed by Drescher et al. ( Phys. Rev. Lett., vol. 102, 2009, 168101) to exhibit hydrodynamic bound states when they are close to a rigid horizontal boundary. When the boundary is above, the colonies are attracted to each other and orbit around each other in a 'waltz'; when the boundary is below they perform more complex 'minuet' motions. These dances are simulated in the present paper, using a novel 'spherical squirmer' model of a colony in which, instead of a time-independent but $\theta$ -dependent tangential velocity being imposed on the spherical surface (radius $a$ ; $\theta$ is the polar angle), a time-independent and uniform tangential shear stress is applied to the fluid on a sphere of radius $(1+\epsilon )a, \epsilon \ll 1$, where $\epsilon a$ represents the length of the flagella. The fluid must satisfy the no-slip condition on the sphere at radius $a$ . In addition to the shear stress, the motions depend on two dimensionless parameters that describe the effect of gravity on a colony: $F_g$, proportional to the ratio of the sedimentation speed of a non-swimming colony to its swimming speed, and $G_{bh}$, that represents the fact that colonies are bottom heavy; $G_{bh}$ is the ratio of the time scale to swim a distance equal to the radius, to the time scale for gravitational reorientation of the colony's axis to the vertical when it is disturbed. In addition to reproducing both of the dancing modes, the simulations are able to determine values of $F_g$ and $G_{bh}$ for which they are stable (or not); there is reasonable agreement with the experiments. A far-field model for the minuet motions is also shown to have qualitative agreement, but does not describe some features that are reproduced in the full simulations.