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Optimization problem for 2D horizontal solidification of an alloy138

6.5 Numerical Examples - Optimization Problem

6.5.2 Optimization problem for 2D horizontal solidification of an alloy138

The first optimization considered is the design of time history of the external mag-netic field for convection damping during a two-dimensional horizontal solidification of a Pb-Sn alloy, which was previously addressed in Section 6.4.2. The problem is characterized by strong thermosolutal buoyancy forces and severe convection driven macrosegregation in the solidifying alloy. The optimization problem was solved us-ing 4 and 5 design variables that use third and fourth degree Bezier-Bernstein curves, respectively. The tolerance during the optimization process for terminating the non-linear CG iterations was chosen as 10−3. The time interval under consideration is given by t ∈ [0, 120]. ˆt obeys ˆt ∈ [0, 1] with tmax in Eq. (6.23) being 120 seconds.

Figs. 6.9(a) and 6.9(b) show the cost functional variation for both 4 and 5 design variables. Figs. 6.10(a) and 6.10(b) show the variation of the optimal magnetic field under the time interval considered here for both cases. The optimal magnetic field is captured well by both design space discretizations. It is higher in the initial stages

CG Iterations

Figure 6.9: Cost functional versus CGM iteration for Example 6.5.2 (a) 4 design variables (b) 5 design variables.

Time (s)

Figure 6.10: Plot of the optimal magnetic field for Example 6.5.2 (a) 4 design variables (b) 5 design variables.

577.2

Figure 6.11: (a) Temperature (K) (b) Solute concentration (c) Liquid volume frac-tion and velocity at t = 120 s (optimal time varying magnetic field) for Example 6.5.2.

to counter the strong thermosolutal buoyancy force, prevalent initially. Under the combined influence of thermosolutal and Lorentz forces the convection weakens with time and the magnetic field decreases with time accordingly. The magnetic field ap-proaches a final asymptotic value, lower than its starting magnitude, towards the end of the time interval that is required to suppress weaker thermosolutal convec-tion in the later stages. This eliminates the need to maintain a constant high field throughout the solidification process.

Table 6.9 shows the difference between the maximum and minimum solute con-centrations, ∆C, at two different times. Figs. 6.11(a)-6.11(c) show different field variables under the influence of the optimal magnetic field at t = 120 s. From these figures, it is clear that the application of the optimal magnetic field helps in damp-ing out thermosolutal convection significantly. From Fig. 6.11(b) and Table 6.9, it is evident that macrosegregation is suppressed to a large extent and the solute concentration profile in the solidifying alloy is more uniform in the presence of the

Table 6.9: Comparison of ∆C at two different times for Example 6.5.2 with no and optimal magnetic fields (∆C = Cmax− Cmin).

∆C (%Sn) ∆C (%Sn)

(t = 60 s) (t = 120 s)

No magnetic field 13.35 17.57

Optimal magnetic field 0.92 1.52

z

Figure 6.12: Problem domain for Example 6.5.3 involving 3D directional solidifica-tion of a Pb-Sn alloy. G = 1000 K/m, r = 0.0167 K/s, C0 = 10 wt. % Sn and T0 = Tliq.

optimal field than that observed in Fig 6.5(i)(b) in the absence of any field.

6.5.3 Optimization problem for 3D directional solidification of an alloy

The second optimization problem considered involves designing the time history of the applied magnetic field during the three-dimensional directional solidification of a Pb-Sn alloy addressed previously in Section 3.4.3 of Chapter 3. The time interval

CG Iterations

Costfunctional

0 1 2 3 4 5 6 7

0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

Figure 6.13: Cost functional versus CG iteration for Example 6.5.3.

considered here is given by t ∈ [0, 800] with tmax being 800 seconds. The tolerance during the optimization process for terminating the non-linear CG iterations was chosen as 10−3. Fig. 6.13 shows the cost functional and Fig. 6.14 shows the variation of the optimal magnetic field under the time interval considered. The time variation is very similar to that observed in the previous example. The magnitude of the applied field, which is higher in the initial stages to suppress stronger thermosolutal buoyancy forces, decreases with time. Towards the end, there is a marginal increase in magnetic field to suppress residual solutal convection in the melt, but it is lower than the starting magnitude. This marginal increase is required to counter the residual solutal convection that is responsible for freckle formation and growth at later times. Figs. 6.15(a)-6.15(b) show the solute concentration and liquid volume fraction fields for the optimal magnetic field. In the absence of a magnetic field, channel formation occurs in the bulk leading to the formation of freckle defects where solute concentration differs greatly compared to the bulk as observed from Figs.

6.16(a)-6.16(b). The optimal magnetic field is successful in suppressing channel formation and inhibiting macrosegregation that were observed in Figs.

6.16(a)-Time (s)

Optimalmagneticfield(T)

0 200 400 600 800

3 3.5 4 4.5 5 5.5 6 6.5

Figure 6.14: Plot of the optimal magnetic field for Example 6.5.3.

6.16(b) and also in Table 6.10, where ∆C values at two different times are tabulated, in the absence of any magnetic field. The need to maintain a constant high magnetic field throughout the solidification process is also eliminated.

6.6 Summary

A numerical study of the effect of magnetic fields on solidification of metallic alloys with significant mushy zones was presented. The direct problem was based on a single domain volume-averaged model for alloy solidification under the influence of magnetic fields. Based on this, a continuum sensitivity based finite dimensional optimization problem was formulated for designing the time history of externally imposed magnetic fields. The main objective here was to use an optimal magnetic field to suppress thermosolutal convection and inhibit macrosegregation during alloy solidification. The orientation of the applied magnetic field was fixed and only the magnitude was chosen to vary with time. For metallic alloys considered here, the Lorentz force arising due to the application of magnetic fields on moving melts

X Y

Figure 6.15: (a) Solute concentration (b) Liquid volume fraction at t = 800 s (op-timal time varying magnetic field) for Example 6.5.3.

X Y

Figure 6.16: (a) Solute concentration (b) Liquid volume fraction at t = 800 s (no magnetic field) for Example 6.5.3.

Table 6.10: Comparison of ∆C at two different times for for Example 6.5.3 with no and optimal magnetic fields (∆C = Cmax− Cmin).

∆C (%Sn) ∆C (%Sn)

(t = 400 s) (t = 800 s)

No magnetic field 5.97 7.40

Optimal magnetic field 0.40 1.65

is the primary damping force. The cost functional minimization was carried out using a non-linear conjugate gradient method that utilized finite element solutions of the continuum direct and sensitivity problems. The magnetic field was tailored so as to capture variations in thermosolutal convection during solidification of the alloy. The magnitude of the optimal magnetic field was higher during the initial stages of solidification and decreased with time before approaching an asymptotic value for the 2D example in Section 6.5.2 or increasing slightly towards the end of the time interval considered for the 3D example in Section 6.5.3. During 3D directional solidification, this increase is required to counter the solutal convection that is responsible for freckle formation and growth at later times. The use of an optimal magnetic field alleviates the need to use a magnetic field with a high magnitude throughout the solidification process, which in turn translates into power and energy savings. Optimization examples in both two and three dimensions were considered to highlight the efficacy and dimension independent nature of the design simulator.

Chapter 7

Conclusions and suggestions for the future research

A stabilized finite element based numerical methodology has been developed in this thesis to address alloy solidification processes based on a single domain volume av-eraged continuum mathematical model. The main aim here is to model alloy solidi-fication processes characterized by strong convection that leads to macrosegregation or large scale solute redistribution in the solidifying alloy. Macrosegregation leads to the presence of various kinds of defects in solidifying alloys. The numerical scheme is first validated using an example involving solidification of ammonium chloride and water mixture where thermosolutal buoyancy forces are very strong. It is then extended to model the combined effect of buoyancy and shrinkage driven flows. The developed numerical scheme is general in nature and suitable for modeling a wide class of solidification problems in both two and three dimensions. The formation of segregation defects like freckles and channels, and surface defects in metallic al-loys due to different types of convection is of special interest here. Towards this end, we explore certain techniques to control macrosegregation or related defects in

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solidifying alloys.

The role of uneven surface topography on transport phenomena occurring during alloy solidification is explored next. We focus on solidification of an aluminum-copper alloy from sinusoidal cavities and the effect of uneven surface topography on convection and macrosegregation during horizontal and vertical alloy solidification.

The volume-averaged solidification model is then coupled with a hypoelastic rate dependent small deformation model to study stresses developing in the mushy zone and solid as solidification occurs from a sinusoidal cavities. Non-uniform contact at the metal-mold interface leads to air-gap formation that results in a dynamic variation of the heat flux at the metal-mold junction. Inverse segregation that occurs at the casting bottom due to shrinkage driven flows is also affected by changes in topography. A parametric analysis is then performed to determine the effect of various process variables like mold surface wavelength, melt superheating, solute concentration and mold materials on air-gap evolution at the metal-mold interface and stress development in the mushy and solid zones. With maximum equivalent stress and growth front unevenness (a surface defect) as the criteria, an optimal wavelength is determined from the parametric analysis.

The role of magnetic fields in damping convection and suppressing macrosegre-gation during solidification of metallic alloys is examined. The application of a mag-netic field on a moving fluid produces Lorentz force that opposes fluid motion. An finite dimensional optimization problem is formulated based on the continuum sen-sitivity method (CSM) to design the time history of the externally applied magnetic field to damp thermosolutal convection and suppress macrosegregation. Both two and three dimensional optimization problems are addressed. In particular, freckle suppression during directional solidification of a lead-tin alloy in three dimensions

using time varying optimal magnetic fields is demonstrated.

The model described in this thesis is valid only on the macroscale and does not take into account nucleation and microstructure evolution. The underlying microstructure in a solidifying alloy has profound influence on properties on the macroscale. A more complete picture will emerge when the continuum model on the macro scale is coupled to a dendritic evolution model on the microscale to study the effects of microstructure on macroscopic variables. This aspect is addressed briefly next.

7.1 Multi-length scale framework for alloy solidi-fication processes

A multi-length scale model that takes into account nucleation and microstructure evolution on the microscale will give a more realistic picture of the alloy solidification process. The microstructure evolution model can be further coupled with a proba-bilistic nucleation models to predict grain growth and orientation in the solid phase [103]. The envisaged multi-length scale framework will involve the current single domain model on the macroscale with a dendritic evolution model based on ex-tended finite element (XFEM) method [104] on the micro scale. Effective averaging techniques are required to transfer information from the micro to the macro scale.

Towards this end, homogenization based upscaling methods can be used as effective tools for property predictions [105]. These methods are superior compared to simple averaging techniques for obtaining property estimates from smaller scales. Effective micro-macro coupling strategies need to be developed so as to represent physics of scales smaller than the computational mesh in a consistent manner [105]. The use

of homogenization upscaling methods will enable us to study the fluctuation of field variables on different length scales [105]. Development of this framework will allow us to address a multi-length scale design problem where the main objective will be to obtain a desired microstructure by controlling macroscopic process parameters like boundary heat flux or magnetic fields.

Appendix A

Material properties

Important material properties used in various numerical examples in Chapters 2-6 are listed in Tables A.1-A.3.

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Table A.1: Important physical parameters for ammonium-chloride water system [8].

Symbol Value

Solid thermal conductivity ks 3.93 × 10−4 kW m−1K−1 Liquid thermal conductivity kl 4.68 × 10−2 kW m−1K−1 Solid specific heat cs 1.87 kJkg−1K−1

Liquid specific heat cl 3.249 kJkg−1K−1 Latent heat of fusion hf 313.8 kJkg−1 Equilibrium partition ratio κp 0.30

Thermal expansion coefficient βT 3.832 × 10−4 K−1 Solutal expansion coefficient βC 0.257 (kg/kg)−1

Solid density ρs 1078.0 kgm−3

Liquid density ρl 1078.0 kgm−3

Viscosity of the liquid µ 1.3 × 10−3 kgm−1s−1 Eutectic temperature Te 257.75 K

Melting point Tm 633.59 K

Acceleration due to gravity g 9.81 ms−2 Slope of the liquidus line mliq −4.68 Kwt%−1 Liquid solute diffusivity Dl 1.5 × 10−9 m2s−1

Table A.2: Important physical parameters for lead-tin alloys [28, 56].

Symbol Value

Solid thermal conductivity ks 1.855 × 10−2 kW m−1K−1 Liquid thermal conductivity kl 1.855 × 10−2 kW m−1K−1 Solid specific heat cs 0.167 kJkg−1K−1

Liquid specific heat cl 0.167 kJkg−1K−1 Latent heat of fusion hf 37.6 kJkg−1 Equilibrium partition ratio κp 0.31

Thermal expansion coefficient βT 1.2 × 10−4 K−1 Solutal expansion coefficient βC 0.515 (kg/kg)−1

Solid density ρs 1.01 × 104 kgm−3

Liquid density ρl 1.01 × 104 kgm−3

Viscosity of the liquid µ 2.495 × 10−3 kgm−1s−1 Eutectic temperature Te 456.0 K

Eutectic concentration of Sn Ce 61.9 wt.%

Melting point of lead Tm 600.0 K

Initial temperature Ti 580.0 K

Ambient temperature T 298 K

Acceleration due to gravity g 9.81 ms−2 Slope of the liquidus line mliq −2.33 Kwt%−1 Liquid solute diffusivity Dl 3 × 10−9 m2s−1 Liquid electrical conductivity σe 1.5 × 106 Ohm−1m−1

Table A.3: Important physical parameters for aluminum-copper alloys,[41, 43].

Symbol Value

Solid thermal conductivity ks 0.1925 kW m−1K−1 Liquid thermal conductivity kl 0.0826 kW m−1K−1 Solid heat capacity cs 1.06 kJkg−1K−1 Liquid heat capacity cl 1.06 kJkg−1K−1 Latent heat of melting hf 397.5 kJkg−1 Equilibrium partition ratio κ 0.17

Thermal expansion coefficient βT 4.95 × 10−5 K−1 Solutal expansion coefficient βC −2.0 (kg/kg)−1 Shrinkage coefficient βsh 0.10417

Solid density ρs 2650 kgm−3

Liquid density ρl 2400 kgm−3

Liquid viscosity µ 0.003 kgm−1s−1

Eutectic temperature Te 821.0 K Melting temperature of Al Tm 933.0 K Ambient temperature Tamb 298.0 K Eutectic concentration of Cu Ce 33.2 wt.%

Acceleration due to gravity g 9.81 ms−2

Slope of the liquidus line mliq −3.3735 Kwt%−1 Liquid solute diffusivity Dl 3 × 10−9 m2s−1

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