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Taylor's chiral microswimmer

Harsh Soni

  • Department of Physics, Indian Institute of Science, Bangalore 560 012, India and School of Physical Sciences, IIT Mandi, Kamand, Mandi, HP 175005, India

Phys. Rev. Fluids 8, 044201 – Published 28 April, 2023

DOI: https://doi.org/10.1103/PhysRevFluids.8.044201

Abstract

In order to understand the rotational motion of a microswimmer in a Newtonian fluid, we model it as an infinite cylinder with a helical, propagating surface wave. Using the method of series expansion, we calculate the linear and angular velocities of the cylinder, assuming that the wave amplitude is much smaller than the wavelength. To the first order in the wave amplitude, for the first mode of a purely azimuthal wave (that is, when the wavelength equals the cylinder's circumference), the cylinder moves along a circular path in the plane normal to its axis. Otherwise, the first-order velocities of the cylinder are zero, like the Taylor sheet. The time-averaged motion of the cylinder is determined by calculating the second-order velocities; the axial component of the wave vector leads to the linear motion of the cylinder along its axis and the azimuthal component to the angular motion around the axis. With the same stroke, the cylinder is always slower and less efficient than the Taylor sheet.

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