Abstract

Rotating spheres in cylindrical channels roll or slide along the channel depending on the physical and geometric conditions. For a thorough investigation of the phenomenon, finite-element modelling is utilized to obtain the resistance coefficients for the motion of a sphere in a cylindrical channel, with an emphasis on near-wall motion. Extracted coefficients are compared with the data in the literature and utilized in exploring the conditions for rolling versus sliding along the channel. Sliding occurs due to the pressure build-up in the nip region between the wall and the rotating sphere in small confinement ratios, whereas rolling occurs when the shearing forces on the sphere are dominant in larger ratios. According to numerical results, a flow reversal takes place in the nip region and reduces the shear as well. Rolling versus sliding is demonstrated in experiments by using magnetic spherical particles, which are rotated by means of an external magnetic field inside cylindrical channels filled with viscous fluids. Faster axial velocities are observed in narrow channels while sliding than in wider channels while rolling for the same rotation rate of the sphere. Experiment observations are compared with the velocities evaluated from the resistance coefficients, showing that the distance between the sphere and the wall, which is dominated by roughness, plays an important role in the velocity of the sphere.

Highlights

  • The motion of spherical particles in channels is a quintessential problem in fluid mechanics and has been studied extensively in the literature with a range of applications in many 935 A9-1H.O

  • Bungay & Brenner (1973) studied the motion of spherical particles in a tightly fitting cylindrical conduit and proposed an improvement on the existing lubrication theories, which is still widely used in the cases where the sphere and the channel wall are in close proximity

  • Our study aims to understand the effects of geometric parameters and to elucidate the rolling and sliding of spheres in cylindrical channels

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Summary

Introduction

The motion of spherical particles in channels is a quintessential problem in fluid mechanics and has been studied extensively in the literature with a range of applications in many 935 A9-1H.O. Basset (1888), Boussinesq (1903) and Oseen (1927) studied the motion of a sphere settling under the gravity force in a quiescent fluid In such a fluid, disturbance to the flow occurs solely due to the settling motion of the sphere, which is of low Reynolds number, and this allows the deduction of the resulting fluid force on the sphere using the Stokes equations (Maxey & Riley 1983). Brenner & Happel (1958) investigated the frictional drag on a confined sphere subjected to a Poiseuille flow using the method of reflections They concluded that the drag is minimized at an optimal distance away from the cylindrical channel boundaries. Bungay & Brenner (1973) studied the motion of spherical particles in a tightly fitting cylindrical conduit and proposed an improvement on the existing lubrication theories, which is still widely used in the cases where the sphere and the channel wall are in close proximity Their data show that the resistance to rotation increases logarithmically as the confinement increases. Bungay & Brenner (1973) studied the motion of spherical particles in a tightly fitting cylindrical conduit and proposed an improvement on the existing lubrication theories, which is still widely used in the cases where the sphere and the channel wall are in close proximity

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