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Simulation and Experimental Validation of Electroosmotic Flow in a Microfluidic Channel Seungbae Hong*, Zhongliang Tang+, Djordje Djukic++, Aurea Tucay++, Sasha Bakhru++, Richard Osgood++, James Yardley++, Alan C. West+, Vijay Modi* ++ Department of Electrical Engineering + Department of Chemical Engineering * Department of Mechanical Engineering Columbia University, New York, NY 10027 Abstract - In this paper steady electroosmotic and pressure driven flows in geometries of interest to biomacromolecular detection are considered. For both types of flow, experimental data are obtained by imaging fluorescent dye propagation. Numerical simulations are carried out using finite volume methods. Test structures are made of Polydimethylsiloxane (PDMS) mold using the negative of the desired structure fabricated by SU-8 thick negative photoresist. Steady electroosmotic flow is governed by the Laplace equation under certain idealized conditions such as when the Helmholtz-Smoluchowski relation is satisfied at the inlet and outlet boundaries, and when the zeta potential is uniform across the domain. In many of these cases, electroosmotic fluid flow can be further idealized as two-dimensional when two parallel plates confine the flow. Such conditions are frequently encountered in many microfluidic devices. In this paper, numerical solutions of such an idealized two-dimensional electroosmotic flow are obtained and compared to experimental data. Equations describing the transient dye propagation are then solved in a straight channel followed by a downstream circular well. Effects of channel size, electric field and possible pressure driven flow components are also explored. The effects of flow three- dimensionality are also examined. I. INTORDUCTION Electroosmosis becomes an increasingly efficient fluid transport mechanism as channel cross-sectional dimensions become lower than millimeter scale. If the conditions of electroosmotic flow meet certain criteria such as uniform surface zeta potential, homogeneous fluid properties, insulating and impermeable channel walls, negligibly thin Debye layer (compared to channel dimensions), and uniform total pressure on all entry and exit ports [1], the electroosmotic flow can be considered as irrotational. In this irrotational flow, velocity everywhere outside the Debye layer is proportional to the electric field gradient in the fluid. Therefore, in the ideal electroosmotic flow condition, the flow field can be obtained by the solution of Laplace equation for electric potential. Due to the nature of chip manufacturing processes such as photo-etching and surface bonding, many micro-channels on the chip can be approximated as two-dimensional networks whose actual cross section is rectangular. Since most constant depth rectangular channels do not have electric field gradients perpendicular to the chip plane, the flow that meets the ideal electroosmosis condition will indeed become two- dimensional flow. Patankar and Hu [2] conducted three dimensional electroosmotic flow simulation where the channel and fluid conditions met the conditions for ideal electroosmosis. They concluded that their numerical simulation did not have velocity component in the third dimension and the flow could be approximated as 2-D flow. This confirms our 2-D assumption on such situations. Seiler, Fan, Fluri, and Harrison[3] however suggest that a pressure driven component may be present in the flow while the conditions met the ideal electroosmosis criteria. If the channel network contains a branch with weak electric field gradient, leakage flow is induced and the electroosmotic flow field will no longer be proportional to the electric field gradient. Therefore, care needs to be exercised in the choice of ideal electroosmotic flow conditions and as a result, we limit our simulations to single inlet, single outlet systems so that no complications would arise from pressure induced flow at channel junctions. We have validated our analysis using experiment on a PDMS chip with fluorescence dye that is supplied from the inlet reservoir. For fabricating PDMS chip, the negative of the desired structure using thick SU-8 negative photoresist was first created. This is used as a molding master for creating a desired channel structure in PDMS. II. THEORY We first begin with the solution of electric field in the channel. For steady state electric potential gradient E = -∇ Φ, we use the Laplace equation: 02 =Φ∇ (1) Since the microfluidic chip and the channel wall are usually made out of silicon, glass, or polymeric materials, which are insulators for electric currents, we impose a Neumann boundary condition at the channel walls. At the electrode, a scalar voltage potential is applied. The electroosmotic velocity is proportional to the electric field gradient by the electroosmotic mobility µeo. Φ∇−= eov µ & (2) Electroosmotic mobility is a property that depends on the type of fluid and solid at their interface. For PDMS and de- ionized water, it is found to be 2.768×10-5 m2/V⋅s and mass diffusion coefficient between the dye and water is defined as DAB.= 5.5×10-10.m2/sec. Mass dispersion equation shown below is used to calculate dye propagation over time. CDCv t C AB 2)( ∇=∇⋅+ ∂ ∂ & (3) The integral forms of equation (1) and (3) are solved using the finite volume method. These are: 02 =⋅Φ∇∫ S dSn& ∫∫∫ ⋅∇=⋅+Ω∂∂ Ω SABS dSnCDdSnvCCdt &&& )( (4) Above, Ω is the volume and S is the surface area of a control volume. For numerical calculations, dimensionless forms of the above equations are solved. These equations are obtained by normalizing velocities with U, the inlet velocity, lengths with W, the channel width and concentrations with inlet concentration. An important dimensionless parameter, Peclet number or Pe given by ABD UWPe = (5) emerges from this exercise characterizing the ratio of convection to diffusion. For Pe >>1, convection will be dominant while for Pe << 1, diffusion will be dominant. For microchannels with channel cross-section dimensions of 10 ∼ 100 µm, Pe numbers vary from 1-100. III. FABRICATION PROCEDURE Rapid prototyping of microchannel structures for flow experiments was done by replica-molding PDMS from master structures created in thick negative photoresist (SU-8) by optical lithography. Commercially available standard grade mixtures of EPON SU-8 photoresist, SU-8-5 (with 52% solids), and SU-8-25 (63% solids), were spun onto Si wafer substrates at 1100 and 2000 rpm yielding 10µm and 30 µm thick films, respectively. Pre-exposure bake was done for one hour at 95°C on a precisely leveled hot plate and the samples were allowed to cool down before further processing [4]. Exposure was done using a direct laser writing system. Photolithographic setup consists of an Ar-ion laser (wavelength λ=350nm), focusing optics, and a computer controlled sample stage. The movement of the stage along all three axes (x,y,z) is achieved by stepping motors. Desired master patterns were created by scanning the samples underneath the focused laser beam to expose the outline, and then scanning across the interior to fully expose the micro- Fig. 1. SEM micrograph of the SU-8 master structure. Fig. 2. SEM micrograph of the PDMS replica of the SU-8 master structure. channel structure. Dynamical focus correction for the sample tilt with respect to the scanning laser beam was the done by on-the-fly adjustments of the distance between the focusing lens and the sample stage. Post-exposure bake was done at 95°C for 15min followed by developing in a commercial SU8 developer for 5 min. The sample was lightly stirred during developing.Fig. 1 shows a 100 µm diameter circular well structure with 30 µm wide input and output channels created in 30 µm thick SU-8. Patterns created in SU-8 were used as molding masters for replication in PDMS[5]. PDMS was prepared from the mixture of 10:1 ratio by weight of the PDMS precursor and curing agent (Sylgard 184 kit, Dow Corning). Before curing, the mixture was placed in vacuum to evacuate the bubbles formed during mixing. It was then poured over the SU-8 master, which was previously coated with a thin layer (~50nm) of chromium to improve the release of the PDMS coating after curing. Curing was done at 70°C for 12 hours. It can be seen from Fig. 2, that the PDMS replica exhibits smooth, vertical sidewalls, and the required dimensions for our microfluidic structure design. IV. EXPERIMENTAL SETUP A. Electrokinetic Flow Experiment The chip with circular well (100µm in diameter and 10-30µm high, connected to the outside reservoirs by 10-30 µm wide channels) on it is rinsed with ethanol five times and then rinsed with deionized water three times. The chip is dried by compressed air. A flat piece of PDMS is cleaned and dried in text Output reservoir Well Input reservoirW mµφ 100= (a) text W Cathode Anode 4 mm (b) Fig. 3. Top view (a) and side view (b) of the chip the same way and used as a cover to seal the chip by adhesion (Fig. 3). After it is assembled, the chip is flooded by adding electrolyte solution in one well and applying a vacuum to the other well. Both wells are cleaned and refilled with same amount of electrolyte (0.1mM KNO3). Electrodes (platinum wires) are then connected to the circuit. A fluorescence dye (calcein or bis [N, N-bis(carboxymethyl) - aminomethyl] fluorescein, excitation at 490nm, emission at 540nm, MW 622.55, Dw=5.5×10-10 m2/s [6]) is used as the probe. The assembled chip is then put under a fluorescence microscope and a voltage is applied across the channel. A CCD camera (Sensys0401E, Roper Scientific) is used to record fluorescence images at a constant time interval. The images are stored in a computer for further processing [7-9]. The fluorescence filter set used is Chroma 11001. The flow pattern inside the feature is extracted by processing the image sequence. The schematic setup of the experiment is illustrated in Fig. 3. B. Pressure Driven Flow Experiment Following the same procedure as in the electro-osmotic flow experiment section except that a pressure gradient is applied across the channel as the flow driving force instead of an electric field. The calculated pressure gradient needed to obtain a comparable flow rate to electro-osmotic flow is about 5 Pa/mm for this geometry. Thus hydraulic pressure is used in this experiment. V. RESULTS Experimental data on electroosmotic flow were obtained for two different channel sizes, 10 × 10 µm channel and a 30 × 30 µm channel leading into a 100 µm diameter circular well. The microfluidic structure is made from PDMS with a measured zeta potential of -40mV. The applied electric field inside the inlet and exit channel is 50, 100, 150 V/cm respectively. Initially, calcein (fluorescent probe) is placed in the reservoir to the right of the Fig. 4. Figure. 4a-c shows a comparison of simulated and measured flows for the 10 × 10 µm channel case and Fig. 4d for the 30 × 30 µm channel. The simulated contour plots are shown in the bottom row, and the corresponding experimental plots are shown on the top of the figure. Note that in these Figures the flow is from right to left and in each of figures. Four plots are shown at four consecutive times (from left to right) with time intervals ∆t for each case shown in the figure caption. The particular instances of time shown are chosen so that the calcein labeled solution can be observed in the well region. In each plot of Fig. 4, fluorescence intensity levels of 20, 40, 60 and 80 percent of the inlet intensity of calcein are shown. From the results it is seen that the simulations and experiments show reasonable agreement for the 10 µm square inlet channel case, whereas for the 30 µm square channel case the agreement is not as good. The asymmetries in the measured concentration contours in the 30 µm case, are believed to be errors in leveling of the chip, whereas it is hard to notice for the 10 µm thick chip. Moreover dye propagation in the 30 µm case seems to be faster as well. The reason for these differences could be the relative importance of a spurious pressure driven component, as discussed in the next section. The results also show differences in dye concentration gradients between the simulation and experiment at the side- walls. The simulations do not show a concentration gradient normal to the wall, while in the experiment a gradient a. b. c. d. W = 10 µm channel a. E = 50V/cm, v = 0.14mm/sec, ∆t = 0.8 sec (Pe = 2.6) b. E = 100V/cm, v = 0.28mm/sec, ∆t = 0.4 sec (Pe = 5.1) c. E = 150V/cm, v = 0.42mm/sec, ∆t = 0.4 sec (Pe = 7.65) W = 30 µm channel d. E = 50V/cm, v = 0.14 mm/sec, ∆t = 0.4sec (Pe = 7.53) Fig. 4. Measured (upper row) and computed (lower row) electroosmotic flows for 10 and 30 µm square channels at the wall is readily seen. We suspect that the reason for this is as follows. The electroosmotic flow is driven by effectively slip conditions that exist at all the four walls (top, bottom, and two side walls) of the PDMS structure. It is possible that the fabrication process does not lead to smooth side-walls causing electric potential gradients to be smaller at the side walls than for the top and bottom surfaces walls. The flow at the side walls could be somewhat slower and this along with the optical refraction at the walls could contribute to what appears to be a dragging effect at the side walls in Fig. 4. VI. DISCUSSION We have developed a computer program to predict the electroosmotic flow field and mass dispersion. To verify the two dimensional nature of the flow in the microchannel, we have fabricated a PDMS microchip and conducted experiments using a fluorescent dye, and observed the dye propagation through CCD camera. The microfluidic flow and dye dispersion were successfully modeled and matched with the experiment. There are some pressure driven components in the experiment which are more prevalent in the low speed electroosmotic flow and for the chips with larger dimensions. Using the equations for pipe flow, we find that an approximately 1mm height difference (h) for a 4mm (L) long channel with 30 µm (d) square cross section corresponds to 77 µm/sec (v) flow velocity, and for the 10 µm (d) square cross section corresponds 8.6 µm/sec (v) flow velocity. L dhgv µ ρ 5.28 2 = (ρ: density, g: 9.8m/s2, µ: viscosity) (6) Due to this difference of almost an order of magnitude in speed, we can observe the remnant of pressure driven component such as the asymmetrical pattern of dye dispersion in 30 µm thick channel more readily than in 10 µm thick channel in the circular channel bulge. Fig. 5 shows the dye concentration contours obtained by experiment and simulation for a pressure driven flow. These are for a hydrostatic pressure of h = 2mm of water, corresponding to a means velocity in the channel of 153 µm/sec. The Pe number for this case is 8.34. Due to the relatively low Pe numbers, i.e. high diffusion rate, there is little distinction in the dye dispersion shape between the electroosmotic and pressure driven flow for the simulation. The same applies for the experiment, but pressure driven flow shows higher dye concentration gradient. Through close examination, in both experimental and simulation cases, the pressure driven one showsa sharp angled dye front, while the electroosmotically driven flow showed round dye front. Note that the pressure driven flow in this system is necessarily three-dimensional and that the assumption of two-dimensionality in Fig. 5b may not be appropriate. Hence 3-D simulations of the same flow were also carried out. The concentration contours for this case are shown in Fig. 5c. There are no significant gradient in the channel depth direction. Overall, the simulations and experimental results show generally good quantitative agreement. Using this simulation technique, the flow behavior of a microfluidic network can be predicted accurately as long as the flow meets the ideal Fig. 5. Measured and computed pressure driven flow for 30 µm square channel [h = 2mm, v = 0.153 mm/sec, ∆t = 0.45 sec (Pe = 8.34)] electroosmosis criteria. As expected smaller channel dimensions and higher electric fields lead to lower contamination with pressure driven components and hence better agreement between computation and experiment. REFERENCES [1] E. B. Cummings, S. K. Griffiths, R.H. Nilson, “Irrotationality of Uniform Electroosmosis”, SPIE conference on Microfluidic Devices and Systems II, Santa Clara, CA, vol. 3877, page 180-189. (September 1999) [2] N. A. Partankar, H. H. Hu, “Numerical Simulation of Electroosmotic Flow”, Analytical Chemistry, vol. 70, page 1870-1881. (1998) [3] K. Seiler, Z. H. Fan, K. Fluri, D. J. Harrison, “Electroosmotic Pumping and Valveless Control of Fluid Flow within a Manifold of Capillaries on a Glass Chip”, Analytical Chemistry, vol. 66, 3485-3491, (1994) [4] H. Lorentz et al., “SU-8:a low-cost negative resist for MEMS”, J. Micromech. Microeng., 7, pp 121-124, (1997) [5] A. Folch et al., “Molding of Deep Polydimethylsiloxane Microstructures for Microfluidics and Biological Applications”, J. Biomech. Eng., 121, pp.28-34, (1999) [6] D. de Beer, P. Stoodley, Z. Lewandowski, “Measurement of Local Diffusion Coefficients in Biofilms by Microinjection and Confocal Microscopy”, Biotechnology and Bioengineering, vol. 53 151-158 (1997) [7] K.D. Kramer, K.W. Oh, C.H. Ahn and et. al., “An Optical MEMS-based Fluorescence Detection Scheme with Applications to Capillary Electrophoresis”, SPIE Conference on Microfluidic Devices (Santa Clara, CA) 76-85 (1998) [8] S.N. Brahmasandra, B.N. Johnson, J.R. Webster and et. al., “On-Chip DNA Detection in Microfabricated Separation Systems”, SPIE Conference on Microfluidic Devices (Santa Clara, CA) 242-251 (1998) [9] D.W. Arnold and P.H. Paul, “Fluorescence-based Visualization of Electroosmotic Flow in Microfabricated Systems”, SPIE Conference on Microfluidic Devices II (Santa Clara, CA) 174-179 (1999) Abstract - In this paper steady electroosmotic and pressure driven flows in geometries of interest to biomacromolecular detection are considered. For both types of flow, experimental data are obtained by imaging fluorescent dye propagation. Numerical sim A. Electrokinetic Flow Experiment B. Pressure Driven Flow Experiment
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