CP620, Shock Compression of Condensed Matter - 2001 edited by M. D. Furnish, N. N. Thadhani, and Y. Horie © 2002 American Institute of Physics 0-7354-0068-7/02/$ 19.00 INVESTIGATION OF LIQUID-SOLID PHASE TRANSITION USING ISENTROPIC COMPRESSION EXPERIMENTS (ICE) Jean-Paul Davis, Dennis B. Hayes, James R. Asay, Phillip W. Watts , Paul A. Flores*, and David B. Reisman1^ Sandia National Laboratories, Albuquerque, NM 87185 Bechtel Nevada - Los Alamos Operations, Los Alamos, NM 87544 1 Lawrence Livermore National Laboratory, Livermore, CA 94550 Abstract. Isentropic ramp-wave loading of materials is a novel method to study the kinetics of phase transitions, particularly in regimes that cannot be accessed by shock-loading techniques. The Sandia Saturn accelerator produces magnetically driven planar ramp waves of 200-300 ns rise time in an aluminum drive plate, which then propagate into a material sample. In this way, molten tin initially at 600-700 K was isentropically loaded to 160-220 kbar, driving it across the liquid-solid phase boundary. VISAR measurements at a sapphire window interface show possible evidence of nonequilibrium freezing in tin with a characteristic transition time around 100 ns. Improved experimental techniques are needed to verify this conclusion. INTRODUCTION USEFULNESS OF THE ICE TECHNIQUE An isentropic compression loading technique has recently been developed at Sandia National Laboratories* using fast pulsed power to provide planar magnetic loading of material samples over several hundred nanoseconds.1 Dubbed "Isentropic Compression Experiments" (ICE), this method is well-suited to the study of structural phase transitions, especially those not accessible by Hugoniot measurements. One transition of interest is freezing of metals, which, to the authors' knowledge, has never been observed experimentally under high strain-rate conditions. Liquid-solid transitions can be accessed with relative ease using the ICE technique by pre-heating low-melting-point metals such as tin to the liquid state. This paper presents some computational results for dynamic loading of molten tin as well as initial results from the first experiments on molten tin performed at Sandia. Figures 1-3 show how the ICE technique can access freezing transitions in tin that cannot be detected using shock-loading techniques. These plots present results from one-dimensional hydrodynamic calculations using an equilibrium threephase model for tin, described in the next section. In Fig. 1, phase boundaries, Hugoniot curves, and ICE loading paths are shown together in the p-T plane. Due to opposite curvature of the melting line and Hugoniot curve, the Hugoniot starting from an initial temperature of 700 K never enters the mixedphase region. The 600-K Hugoniot enters the mixed-phase region, but never completely transforms to the y-solid phase, instead returning to the liquid at about 240 kbar. Along the quasi-isentropic ICE loading paths, however, the temperature remains low and the tin can transform completely to the y-solid phase. If the transition is far from equilibrium, the ICE loading may follow a metastable path in a super-cooled liquid state as indicated in Fig. 1 for an initial temperature of 700 K. * Sandia is a multi-program laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy under Contract DE-AC04-94AL85000. 221 produces a shock wave of peak stress about 20 kbar over the equilibrium transition stress on the ICE loading path for 600 K. Even at this low overstress, the partial freezing is overdriven, obscuring information about the transition. The stress histories shown for ramp-wave loading in Fig. 3, however, give a clear indication of the stress upon entering and exiting the mixed-phase region, for propagation distances small enough to avoid shock formation. After a shock forms in the mixed-phase region, the transition is quickly overdriven as shown for a propagation distance of 0.8 mm. A thermodynamic equilibrium model of liquid - solid transition may not be valid on the time scale of an ICE ramp-wave. The nonequilibrium computational results in Fig. 4, which assume a very simple model for phase change kinetics, indicate sensitivity of the ICE technique to the characteristic time for dynamic freezing. Thus, not only can the ICE technique access phase transitions not detectable using impact experiments, it can also provide experimental data on the kinetics of phase transitions. Figure 2 shows in-situ stress-time histories in molten tin at various Lagrangian distances from an impact surface. The copper impactor at 800 m/s 1700- liquid 1500 equilibrium Hugoniot curves 1300 1100 equilibrium ICE loading paths y-solid ct(8) 500300 P-solid ct( 0 50 100 150 200 250 pressure (kbar) 300 FIGURE 1. Computed phase diagram of tin with equilibrium Hugoniot curves (dashed) and ICE loading paths (solid gray) for initial temperatures of 600 K and 700 K. uu - 0.0 5mm 80- \ 6040- 0.2mm \O.lmm / -^ THREE-PHASE MODEL FOR TIN 0.4mm The continuum calculations presented in the previous section were performed using a threephase model for tin based on assumptions introduced by Horie and Duvall2 concerning a homogeneous mixture of structural phases; common particle velocity, common pressure and temperature, and no interfacial energy between phases. The calculation method follows that developed by Andrews3 and extended to N phases by Hayes.4 Each of the 20- n0 50 100 150 200 time from impact (ns) FIGURE 2. In-situ longitudinal stress histories in tin initially at 600 K impacted by copper at 800 m/s, computed under the assumption of equilibrium freezing. 400- 200 time (ns) FIGURE 3. In-situ longitudinal stress histories at 0.2 mm intervals in tin initially at 600 K subjected to ICE ramp-wave loading, computed under the assumption of equilibrium freezing. Load profile based on real Saturn current pulse. Disturbances correspond to mixed-phase region. 200 time (ns) 250 FIGURE 4. In-situ longitudinal stress histories (at a Lagrangian distance of 0.4 mm from loading surface) for tin initially at 700 K, computed using the present kinetics model. 222 Aluminum drive (0.6mm) Pymoeeram 9608 insulator (2.0mm) phases (oc-solid, y-solid, and liquid) has its own equation of state (EOS), and extensive properties of the mixture are mass-averaged over all phases. For the EOS of each phase, a Mie-Griineisen form was assumed with constant cv, constant T/v, and the reference p(v) curve given by a Birch isotherm. Parameter and reference-state values for the three phases of tin were taken from Mabire and Hereil.5 The phase boundaries in Fig. 1 were computed by solving for states where the Gibbs free energies of two phases are equal. Kinetics were introduced by a simple phenomenological model wherein the mass fraction rate of change for a given phase is proportional to the sum of the differences in Gibbs free energy from each other phase.3 The model was implemented in the one-dimensional computer code WONDY.6 It is important to note that the present model, based solely on macroscopic thermodynamics, is not intended to illuminate the underlying physics of dynamic freezing. Rather, the goal is to connect experimental data to continuum modeling. Confidence in the present model was obtained by successful comparison (not shown) to the impact data of Mabire and Hereil,5 which indicate melting upon release from Hugoniot states. A] 1 o Stepped tin sample (0.4mm & 0.7mm) Stepped sapphire wiridow (2.3mm & 2.0mm) FIGURE 5. Sketch of experiment configuration showing thicknesses of the various material layers. turb the wave entering the molten tin. Pyroceram 9608, a glass ceramic made by Corning, was chosen because previous impact experiments7 indicated a ramp-generating behavior up to 200 kbar. This nonlinear elastic response prevents the input ramp wave from shocking up over the long propagation distance required for thermal insulation. Since Pyroceram 9608 is no longer manufactured, the present work used material from a small batch recreated by the Corning Cells Group. Results from recent impact experiments on the new Pyroceram 9608 indicate that it does not reproduce the same ramping behavior seen in the original material. Fiber-coupled velocity interferometry (VISAR) was used to measure time-resolved particle velocity of the tin/sapphire interface. EXPERIMENT CONFIGURATION A pre-molten tin sample was obtained using small 25-W resistance heater cartridges with feedback control. These heated a tubular copper boat that defined the lateral extent of a 6.9-mm diameter cell holding the molten tin. The copper was clamped between a stepped sapphire window and a ceramic insulator (12-mm diameter) to define the axial extent of the tin sample. The insulator was itself bonded to the aluminum drive plate that forms part of the anode on the Saturn accelerator. As shown in Fig. 5, magnetic loading is applied to the opposite side of the drive plate, sending an unsteady hydrodynamic stress wave into the series of material layers. Layer thicknesses are shown in Fig. 5. The most challenging requirement in these experiments is the thermal insulator between the metallic drive plate (part of an enormous heat sink in the form of Saturn's power-flow hardware) and the tin sample. Materials with low thermal conductivity tend to have high elastic limits that adversely per- RESULTS Two molten tin experiments were performed on the Saturn accelerator, using two different anode geometries (to obtain different current densities and hence different peak pressures) and different initial temperatures. Two heating cells were used on each experiment; one with the stepped tin sample, the other with a sapphire window mounted directly on Pyroceram. Figures 6-7 present VISAR data from these shots. Note that differences in signal delay times have not been accounted for. In shot 2925 (Fig. 6), an untested method was 223 1.0 time (us) uncorrected 1.1 1.2 1.3 time (us) uncorrected 1.4 1.5 FIGURE 6. VISAR velocity records from Saturn shot 2925 (peak pressure approx. 220 kbar, initial temperature 600 K). FIGURE 7. VISAR velocity records from Saturn shot 2926 (peak pressure approx. 160 kbar, initial temperature 700 K). used to bond the sapphire window to the pre-heated Pyroceram. The bond evidently failed, leaving a small gap that resulted in an impact. In shot 2926 (Fig. 7), the heater without a tin sample was left at room temperature, and the Pyroceram/sapphire bond appears to have maintained its integrity. In this case, however, a useful measurement of the ramp wave exiting the Pyroceram was prevented by early (relative to the ramp rise-time) arrival of edge waves at the probe location. This was due in part to use of two off-center probes for redundancy (shot 2925 used only one centered probe). The tin/sapphire interface velocity at which freezing is expected to initiate was computed using the model described earlier, and is indicated on each of Figures 6-7. The experimental data show a distinct two-wave structure that, based on other experiments using Pyroceram (not shown), is probably due to a disturbance generated in the new Pyroceram 9608 insulator material. In Fig. 6, the second wave is overtaking the first wave, consistent with a double-ramp wave having entered the tin from the Pyroceram. If the plateau were due to freezing, it would be expected to occur at a higher velocity in Fig. 7 due to the higher initial temperature (cf. Fig. 1); instead, it appears at the same velocity. Nonequilibrium dynamic freezing may cause the change in curvature with propagation seen at the top of the first wave. If so, then comparison to nonequilibrium computations would suggest a characteristic time for freezing on the order of 100 ns. It should be noted that, based on the results in Figures 3-4, the present experiments are only expected to detect freezing if it occurs with a charac- teristic time of less than 400-500 ns. FUTURE WORK Further experiments are planned using a sapphire insulator in place of the Pyroceram to provide an unperturbed ramp wave up to 300 kbar (within the elastic regime of sapphire under ICE loading). Though sapphire has an order of magnitude higher thermal conductivity, the heating cell was overdesigned by a wide margin. Also being considered are LiF windows to increase signal reading time. REFERENCES 1. 2. 3. 4. 5. 6. 7. 224 Hall, C. A., Phys Plasmas 7(5), 2069-2075 (2000). Horie, Y. and Duvall, G. E., "Shock-induced phase transition in iron," Behavior of Dense Media under High Dynamic Pressure, IUTAM Symposium on High Dynamic Pressure, Gordon and Breach, New York, 1968, pp. 355-359. Andrews, D.J.,7 Comp Phys 7(2), 310-326 (1971). Hayes, D.B., JAppl Phys 46(8), 3438-3443 (1975). Mabire, C. and Hereil, P. L., "Shock induced polymorphic transition and melting of tin," in Shock Compression of Condensed Matter - 1999, edited by M. D. Furnish et al, AIP Conference Proceedings 505, New York, 2000, pp. 93-96. Kipp, M. E. and Lawrence, R. J., WONDY V - A One-Dimensional Finite-Difference Wave Propagation Code, Sandia National Laboratories Report SANDS 1-0930, 1982. Asay, J. R. and Chhabildas, L. C., "Some new developments in shock wave research," in High Pressure Science and Technology, eds. Vodar, B. and Marteau, Ph., Pergamon Press, 1980, pp. 958-964.
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