Page 111 - Optofluidics Fundamentals, Devices, and Applications
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92     Cha pte r  F i v e


               density, U is the characteristic transport speed, a is an appropriate
               size scale, and μ is the viscosity. For pure particle transport in a quies-
               cent medium, U would be the particle speed and a would be its diam-
               eter. In water then a 1-μm particle transported at 100 μm/s would
                                                     −4
               have a Reynolds number of approximately 10 . If one is considering
               an externally induced flow in a microchannel (say by the application
               of a pressure difference), U would be the average flow speed in the
               channel and a the channel height. In such a case Re can be as high as
               approximately 0.1 but is usually much less. In either case, physically
               this means that momentum transport occurs via diffusion rather than
               convection and that we can ignore the nonlinear terms in the Navier-
               Stokes equations. This also implies that the flow will reach its steady
               state velocity relatively quickly and that the transient period can be
               ignored. Under these assumptions the fluid dynamical equations
               reduce to conservation of volume [Eq. (5-1a)] and the Stokes equation
               [Eq. (5-1b)].

                                         v
                                       ∇⋅ = 0                       (5-1a)
                                       2
                                    μ∇ v  − ∇ = 0P                  (5-1b)
               where v is the velocity field and P is the pressure.

               Hydrodynamic Forces on a Particle in a Flow
               Equations (5-1a) and (5-1b) are descriptive of the fluid velocity at
               every point in a flow. Generally speaking a particle in a flow will
               experience a net pressure force (caused by pressure drop across the
               particle) and a friction force (caused by the flow of a viscous liquid
               over the surface). In the most general case the net drag force can be
               written as
                                    D ∫
                                   F = (T  F  ⋅ )dS                 (5-2a)
                                             n
                                        s
               where F = drag force
                      D
                     T = fluid stress tensor
                      F
                     n = normal vector to the surface of the particle.
               For an incompressible Newtonian fluid, the stress tensor is written
               as
                                       I + (  v + ∇ )
                                                   T
                                 T =−P    μ  ∇   v                  (5-2b)
                                  F
               where I is the isotropic tensor and ∇v is the gradient of the flow
               velocity.
                  The above forms of the hydrodynamic equations are appropriate
               for use in numerical simulations, but difficult to manipulate analyti-
               cally. Simplified versions of these equations are, however, available
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