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Abstracts - KTH Mechanics

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The evolution of energy in flow driven through rising bubbles<br />

Enrico Calzavarini ∗ , Detlef Lohse † ,IreneMazzitelli ‡ and Federico Toschi §<br />

We investigate by direct numerical simulations the flow that rising bubbles cause<br />

in initially quiescent fluid. We employ the Eulerian-Lagrangian 1 method and embody<br />

the two-phase coupling by retaining the bubbles like point sources (see figure 1(a)).<br />

The effects of added mass, buoyancy, drag and lift are included in the model equation<br />

for the bubble dynamics. The possibility of bubble-bubble interaction (4-way<br />

coupling) is analyzed in detail. Our analysis is confined to bubble of small Reynolds<br />

number, Reb ∼ O(1), corresponding to micro-bubbles in water.<br />

The present results suggest that a large scale motion is generated in the initial stages<br />

of the flow evolution, owing to an inverse energy cascade from the small to the large<br />

scale, later on the flow reaches a statistically steady condition where no relevant large<br />

scale fluctuations are present, see figure 1(b). Our analysis at relatively low gaseous<br />

volume fractions, α 1%, suggests that the vorticity induced by the gas on the liquid<br />

phase is not strong enough to enhance bubble accumulation in vortices and therefore<br />

bubbles remain spreaded. The lift force and collision term play a major role in<br />

reducing the degree of clusterization in the high vorticity regions of the flow.<br />

∗Department of Applied Physics, University of Twente, 7500 AE Enschede, The Netherlands.<br />

† Department of Applied Physics, University of Twente, 7500 AE Enschede, The Netherlands.<br />

‡ Department of Applied Physics, University of Twente, 7500 AE Enschede, The Netherlands.<br />

§ Istituto per le Applicazioni del Calcolo, CNR, Viale del Policlinico 137, I-00161 Roma, Italy.<br />

1I. M. Mazzitelli, D. Lohse and F. Toschi, J. Fluid Mech. 483, 283 (2003) and Phys. Fluids 15,<br />

L5-L8 (2003).<br />

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Figure 1: (a) Effect of the bubble feedback on still fluid, vertical section of the velocity<br />

field. (b) Evolution of the velocity spectra in a typical run, void fraction α =0.016, a<br />

transient characterized by relatively large velocity fluctuations (solid line) is followed<br />

by a state of almost equi-partition of energy (the time evolution is as follows: dashed,<br />

dotted and dot-dashed lines).<br />

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