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Slow axial drift in three-dimensional granular tumbler flow

Authors :
Paul B. Umbanhowar
Umberto D'Ortona
Richard M. Lueptow
Julio M. Ottino
Zafir Zaman
Departement of Chemical and Biological Engineering
Northwestern University
Laboratoire de Mécanique, Modélisation et Procédés Propres (M2P2)
Centre National de la Recherche Scientifique (CNRS)-École Centrale de Marseille (ECM)-Aix Marseille Université (AMU)
Department of Mechanical Engineering [Evanston]
Northwestern University [Evanston]
Northwestern Institute on Complex Systems (NICO)
Aix Marseille Université (AMU)-École Centrale de Marseille (ECM)-Centre National de la Recherche Scientifique (CNRS)
Source :
Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, American Physical Society, 2013, 88 (1), pp.012208. ⟨10.1103/PhysRevE.88.012208⟩, Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, 2013, 88 (1), pp.012208. ⟨10.1103/PhysRevE.88.012208⟩
Publication Year :
2013
Publisher :
HAL CCSD, 2013.

Abstract

International audience; Models of monodisperse particle flow in partially filled three-dimensional tumblers often assume that flow along the axis of rotation is negligible. We test this assumption, for spherical and double cone tumblers, using experiments and discrete element method simulations. Cross sections through the particle bed of a spherical tumbler show that, after a few rotations, a colored band of particles initially perpendicular to the axis of rotation deforms: particles near the surface drift toward the pole, while particles deeper in the flowing layer drift toward the equator. Tracking of mm-sized surface particles in tumblers with diameters of 8-14 cm shows particle axial displacements of one to two particle diameters, corresponding to axial drift that is 1-3% of the tumbler diameter, per pass through the flowing layer. The surface axial drift in both double cone and spherical tumblers is zero at the equator, increases moving away from the equator, and then decreases near the poles. Comparing results for the two tumbler geometries shows that wall slope causes axial drift, while drift speed increases with equatorial diameter. The dependence of axial drift on axial position for each tumbler geometry is similar when both are normalized by their respective maximum values.

Details

Language :
English
ISSN :
15393755 and 15502376
Database :
OpenAIRE
Journal :
Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, American Physical Society, 2013, 88 (1), pp.012208. ⟨10.1103/PhysRevE.88.012208⟩, Physical Review E : Statistical, Nonlinear, and Soft Matter Physics, 2013, 88 (1), pp.012208. ⟨10.1103/PhysRevE.88.012208⟩
Accession number :
edsair.doi.dedup.....40fff262192d3d3a32dc78917e2a0b98
Full Text :
https://doi.org/10.1103/PhysRevE.88.012208⟩