2.1. Introduction
Fluid flow of and mass transfer from/to drops, bubbles, and solid particles are often observed in nature and various areas of engineering. Chemical and metallurgical engineers rely on bubbles and drops for unit operations such as distillation, absorption, flotation and spray drying, while solid particles are used as catalysts or chemical reactants. In these processes, there is relative motion between bubbles, drops or particles on one hand, and a surrounding fluid on the other. In many cases, transfer of mass and/or heat is also of importance. Owing to rapid progress of computer techniques and numerical methods in fluid mechanics and transport phenomena, the application of numerical simulation has recently become increasingly popular in understanding multiphase flow and transport on a particle (a generic term including drops and bubbles) scale.
In this chapter, this topic is discussed in detail in the following six sections. Firstly, the theoretical basis and numerical methods frequently adopted are summarized in
Sections 2.2 and
2.3 respectively. We choose to focus mostly on three methods: simulation on orthogonal boundary-fitted coordinates, an improved level set method, and a mirror fluid method. This choice reflects our own background, as well as the fact that these methods are deemed successful and reliable for computing the motion and mass transfer of fluid particles (bubbles and drops) or solid particles. The validity of these methods is demonstrated and compared with the reported experimental data in
Section 2.4. Also, considering the trace quantities of surfactants unavoidable in most industrial systems, study of the motion and mass transfer of a solute to/from a single drop with a surfactant adsorbed on the interface is carried out to better understand the liquid extraction processes and for the scientific design of relevant equipment. The Marangoni effect, one of the most sophisticated interphase transport phenomena, interests researchers due to its influence on transport rates and it has been mathematically formulated and numerically simulated to shed light on these mechanisms. Recent studies relating to the Marangoni effect are presented in
Section 2.5. In
Section 2.6, numerical simulation methods on particle swarms are discussed briefly and modified cell models are introduced to examine the flow and transport behaviors of particle swarms.
Section 2.7 incorporates related progress on particle motion controlled by fluid shear or extension.
2.2. Theoretical basis
The mathematical formulation of two-phase particle flow may be exemplified using two-fluid systems in which a liquid drop or a gas bubble moves in another continuous liquid as it follows in this section. The fundamental physical laws governing the motion of and mass transfer from/to a single particle immersed in another fluid are Newton’s second law, the principle of mass conservation, and Fick’s diffusion law. So the flow field and solute transport in both fluid phases must be formulated using the first principles of fluid mechanics and transport phenomena. When a solid particle is involved, the flow in the solid domain is usually not necessary and the particle is tracked mechanically as a rigid body. In this context, two-phase flow with a solid particle is a simplified case of general two-phase systems.
2.2.1. Fluid mechanics
The motion of a small particle (drop, bubble or solid particle) of around 1 mm size under gravity through an immiscible continuous fluid phase can be resolved using the following assumptions: (1) the fluid is viscous and incompressible; (2) the physical properties of the fluid and the particle are constant; (3) the two-phase flow is axisymmetric or two-dimensional; (4) the flow is laminar at low Reynolds numbers.
The flow in each fluid phase is governed by the continuity and Navier–Stokes equations:
·u=0
(2.1)
?u?t+u·?u=-?p+?g+?·t+S
(2.2)
where t is the stress tensor defined as
=µ(?u+(?u)T)
(2.3)
and the source term S is formulated differently in different cases.
Boundary conditions for the governing equations are essential when an interface exists between the two phases. For a bubble or a drop, the normal velocity in each phase is equal at the interface. If the gas in a bubble is taken as inviscid, the bubble surface is mobile and not subject to any shear force. However, if the gas is taken as a viscous fluid, both the velocity vector and shear stress should be continuous across the interface. For a solid particle, both the normal and tangential velocity components of the continuous phase must be zero at the particle surface; that is, the solid surface should satisfy the “no-slip” condition.
For the case with constant physical properties of both fluid phases, including that on the interface, the solution for mass transfer will be decoupled from the problem of fluid flow. Thus, the information of the flow field, required for solution of convective diffusion problems, whether for steady or unsteady mass transfer, can be provided directly from numerical simulation of steady-state fluid flow only once.
2.2.2. Mass transfer
In general, the transient mass transfer to/from a drop (or a bubble) is governed by the convective diffusion equation in vector form:
c?t+u·?c=D?2c
(2.4)
in each phase subject to two interfacial conditions:
1?c1?n1=D2?c2?n2 (flux continuity at the interface)
(2.5)
2=mc1 (interfacial dissolution equilibrium)
(2.6)
In the above equations, subscript 1 indicates the continuous phase and 2 the dispersed phase. The solution of Eq.
(2.5) is reliant on the resolved fluid flow both in the dispersed and the continuous phases, as addressed by
Li and Mao (2001). In accordance with Fick
’s first law, for steady external mass transfer the local diffusive flux across the interface is calculated by
loc=-D2?c2?n2=kloc(c¯2-mc18)
(2.7)
where the remote boundary concentration 1 8 and the only available measurement of the bubble/drop concentration ¯2 (averaged over the whole drop, taking a drop as an example) are used to define the driving force and the mass transfer coefficient. The latter may be expressed in terms of dimensional concentration gradient as
loc=-D2(c¯2-mc18)?c2?n2
(2.8)
Then, the local Sherwood number is
hloc=dklocD2=-d(c¯2-mc18)?c2?n2
(2.9)
and the drop area averaged Shod is
hod=?Shlocds?ds
(2.10)
On the other hand, the overall mass transfer coefficient kod may be evaluated from the overall solute conservation based on the drop as follows:
od(c2*-c¯2)A=Vddc¯2dt
(2.11)
where ¯2 is the average concentration of the drop at any time instant, which is almost the only available measure of solute concentrations of drops in conventional experiments. If the time interval tout–tin is chosen small enough, kod may be evaluated approximately from integration of the above equation as
od=-VdA1tout-tinlnc2*-c¯2,outc2*-c¯2,in
(2.12)
where A and Vd are the volume and the surface area of the drop, and for a spherical drop Vd/A =...