Microstructure Design of Mechanically Alloyed Materials ARCHIVES by Zachary C. Cordero B.S. Physics Massachusetts Institute of Technology, 2010 MASSACHUSETTS INSTITUTE OF TECHNOLOGY- OCT 28 2015 LIBRARIES SUBMITTED TO THE DEPARTMENT OF MATERIALS SCIENCE & ENGINEERING IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN MATERIALS SCIENCE & ENGINEERING AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY SEPTEMBER 2015 0 2015 Massachusetts Institute of Technology Signature redacted Signature of Author: C Defartment of Materials Science & Engineering August 14, 2015 Signature redacted Certified by: D Accepted by: , en Christopher A. Schuh d Danae and Vasilis Sal apatas Professor of Metallurgy Thesis Supervisor Signature redacted \Z w Donald Sadoway John F. Elliott Professor of Materials Chemistry hair, Departmental Committee on Graduate Students 77 Massachusetts Avenue Cambridge, MA 02139 MITLibranes h-tp://'ibraries.mit.edu/ask DISCLAIMER NOTICE Due to the condition of the original material, there are unavoidable flaws in this reproduction. We have made every effort possible to provide you with the best copy available. Thank you. The first 61 pages are un-numbered. The remaining pages (62-120) have pagination numbers. Microstructure Design of Mechanically Alloyed Materials by Zachary C. Cordero Submitted to the Department of Materials Science and Engineering on August 14, 2015 in Partial Fulfillment of the Requirements for the Degree of the Doctor of Philosophy in Materials Science and Engineering ABSTRACT Nanocrystalline metals have exceptional mechanical properties that make them attractive for structural applications. However, these materials' properties tend to degrade due to grain growth when they are exposed to high temperatures; this makes producing bulk, nanocrystalline components particularly difficult as the most promising synthesis methods involve high temperature densification of powders or foils. Several alloy design strategies have been developed to overcome these thermal stability issues, but their efficacy depends on the spatial distribution of the stabilizing element in the feedstock materials, which are typically prepared using extensive plastic deformation or mechanical alloying. There is thus a need to predict the chemical mixity of mechanically alloyed materials, and this thesis seeks to address this need. To this end, phase strength effects are incorporated into a kinetic Monte Carlo simulation of a mechanically-driven, binary alloy, which can provide quantitative insight into the combination of processing and material parameters that dictate the steady state chemical mixity. Using such simulations, dynamical phase diagrams are generated that predict temperatures and compositions at which a couple with a given phase strength mismatch should chemically homogenize during mechanical alloying. Several of these dynamical phase diagrams are validated using mechanical alloying experiments, in which tungsten-transition metal couples with various phase strength mismatches are mechanically alloyed in a high energy ball mill. This thesis also describes an alloy design case study in which the insights from these simulations and experiments are used to develop a nanocrystalline W-based (W-7Cr-9Fe, at%) alloy powder that can be rapidly compacted to high relative densities while maintaining ultrafine grain sizes. Two-phase compacts made from the alloy exhibit microhardnesses of 13 GPa and dynamic compressive strengths in excess of 4 GPa. Furthermore, postmortem images of compressed micropillars machined out of these compacts suggest that this alloy deforms by shear localization. The penetration performance of this alloy is explored in sub-scale ballistic tests into concrete targets, and is found to be at least as good as current state-of-the-art penetrator materials. Thesis Supervisor: Christopher A. Schuh Title: Department Head and Danae and Vasilis Salapatas Professor of Metallurgy Acknowledgments First and foremost, I owe a big thank you to my adviser, Prof. Chris Schuh, for showing me how to do cutting-edge scientific research, how to communicate my results through presentations and manuscripts, how to develop and pursue research ideas, how to manage collaborations, and how to lead a research group. I feel very fortunate to have had the opportunity to work with him these past four years. I also want to acknowledge the support and guidance of my committee members, Profs. Tom Eagar and Michael Demkowicz. I especially want to thank Prof. Demkowicz for allowing me to TA Mechanics of Materials for him. This was one of the most rewarding experiences that I had in my time at MIT. This thesis would not have possible without the guidance of my unofficial, fourth committee member, Dr. Brian Schuster of the Army Research Laboratory. I enjoyed collaborating with him very much and hope to continue this collaboration in the future. His semi-serious taunt that I would end up a metallographer at NIST gave me nightmares that motivated me to work harder. In addition to developing a novel penetrator material together, I'm pretty sure that we also invented the shelfie, i.e., a selfie with a shellfish. Only time will tell which of these two innovations is the more lasting. Thanks also go to the other members of the DMSE faculty who have mentored me along the way. In particular, I am indebted to Prof. Jeff Grossman for introducing me to materials science when I was an undergrad. When he hired me as a UROP, he set off a chain reaction that ultimately led to me pursuing a doctorate. One step in this chain reaction was the year that I spent at Berkeley, where early on I stumbled into James Wu's powder processing lab. When I was a clueless physicist, James took me under his wing and showed me how to press, sinter, heat-treat, arc melt, machine, and roll. He molded me into the card-carrying metallurgist that I am today, and for that, I am eternally grateful. Back at MIT, the past four years were made exponentially more fun by the people I interacted with every day. The other Schuh groupers are a great bunch who inspired me to work harder, be smarter, present better, and be a better person. Some of my best memories from the past four years are from board game nights with the Schuh groupers who helped me get started in my graduate studies: Samwell Humpfree Baker, Alan The Lai Guy, and Lil' Stian Ueland. Matt Humbert and Mike Tarkanian are two more MIT people who had a tremendous positive impact on my graduate studies and my engineering abilities; when I'm asked what makes MIT special, I say the people and give those two as examples. Finally, there are my training buddies on the MIT masters swim team: Bill Paine, Wishy Washy Joshy, Sebby Binx, Derrick Cow, and Johnny McKelleher. Swimming with all of them helped keep me focused. My parents, Ella and Pedro, put me on this planet and have always given me with their love and unwavering support. They passed their crazy on to me, and instilled in me the drive to work hard on meaningful things. Both of these were essential to me starting and then finishing this dissertation. My brother Ben is a big ball of joy who kept me in check when I needed it most these past couple of years. Finally, there's the newest member of the Cordero clan, Margaret. Meeting her was the best thing to happen to me during my PhD. I feel blessed to have you all as my family. And last but not least, I want to express my gratitude to the US for paying for my graduate studies through the NDSEG fellowship. I think the US made a good investment, but again, only time will tell. Table of Contents Acknow ledgm ents .......................................................................................................................... 3 Table of Contents ........................................................................................................................... 5 List of Figures ................................................................................................................................ 7 List of Tables ............................................................................................................................... 12 1. Introduction .......................................................................................................................... 13 2. Phase Strength Effects on Chemical Mixing in Extensively Deformed Alloys...............26 2.1. M aterials and M ethods .......................................................................................... 27 2.1.1. Powder Processing ............................................................................................. 27 2.1.2. M icro structural and Chem ical Characterization ............................................... 28 2.1.3. Mechanical Testing.............................................................................................31 2.2. M icrostructure and Hardness Evolution............................................................... 31 2.3. Factors A ffecting Deform ation-Induced M ixing.................................................. 44 2.4. Generalized Phase Strength Effects...................................................................... 45 2.4.1. Bi-stability and History-Dependent Steady States............................................. 48 2.4.2. M icrostructure and M ixing Kinetics................................................................. 50 2.4.3. Tem perature and Com position Effects ............................................................... 52 2.5. Concluding Rem arks ............................................................................................ 57 3. Guidelines for the Microstructure Design of Mechanically Alloyed Materials................59 4. Powder-Route Synthesis and Mechanical Testing of Ultrafine Grain Tungsten Alloys......68 4.1. M aterials and M ethods .......................................................................................... 69 4.1.1. Powder Processing and Consolidation............................................................... 69 4.1.2. M icrostructural Characterization ........................................................................ 70 4.1.3. M echanical Testing............................................................................................. 71 4.2. Powder Characterization......................................................................................... 72 4.3. Com paction and Com pact M icrostructure............................................................. 75 4.4. M echanical Properties ............................................................................................ 82 4.4.1. Strengthening Contributions ............................................................................... 82 4.4.2. M icropillar Com pression ................................................................................... 85 4.4.3. High Strain Rate Deforn ation .......................................................................... 87 4.5. 5. 6. Concluding Remarks .............................................................................................. Sub-Scale Ballistic Testing of an Ultrafine Grained Tungsten Alloy .............................. 88 90 5.1. Experimental M ethods........................................................................................... 90 5.2. Sub-Scale Ballistic Testing into Concrete ............................................................. 93 5.3. Concluding Remarks ............................................................................................ 98 C o n c lu sio n s .......................................................................................................................... 99 Appendix A: Aggregated Hall-Petch Data ................................................................................ 102 References............................................................................................ 107 List of Figures Figure 1.1 - Engineering stress-strain curves from microcompression tests on micropillars machined out of W powder particles with a grain size of ~10 nm. .............................................. 13 Figure 1.2 - Ashby map comparing the predicted performance of different kinetic penetrator materials. The grey lines are isocontours of constant kinetic energy density, which indicate similar ballistic performance for a given penetrator geometry. Nanocrystalline tungsten's exceptionally high strength and density make it ideal for penetration applications................. 14 Figure 1.3 - Effective temperature as a function of ambient temperature under a constant intensity driving force. At high temperatures, Teii and T are similar because thermally activated processes outpace processes related to the driving force, while at low temperatures, Terr and T diverge because the thermally activated processes are suppressed. ......................................... 18 Figure 1.4 - Cross-section of a 3-dimensional phase diagram [45]. The axes indicate the concentration on each of the four, interpenetrating simple cubic sublattices of a face-centered cubic metal. To identify the steady-state order parameter of an irradiated material with this diagram, follow the arrows from a starting order parameter to one of the steady state order 21 parameters indicated by the triangle, diamond, or square. ...................................................... Figure 1.5 - Cross-sections from kinetic Monte Carlo simulations of mechanical alloying [70]. Above each of the cross-sections is the shearing rate and temperature used in the simulation. The black dots indicate atoms of one of the alloying elements. The cross-sections show that with decreasing shearing frequency, the alloy is able to phase separate. ......................................... 23 Figure 1.6 -MD simulations of shear-induced mixing in a (a) Cu-Ag and a (b) Cu-V nanocomposite [77]. Both of the simulations began with all of the solute in a single precipitate, and both volume elements have accumulated plastic strains of 60. The solute atoms are colored to indicate their local chemical environment, with green atoms indicating solute surrounded by solute nearest neighbors. The simulations reveal that the V precipitate is still relatively in-tact, while the Ag precipitate is nearly completely dissolved. ......................................................... 24 Figure 2.1 - Fe contamination as measured using EDS in the initially pure W and W-transition metal powders as a function of milling time. The W, W 5 oCr5 o, and W5 oNb50 powders are harder than the W5 oNi5 o, W 50 Hf50 , and W50 Zr5 Opowders, and abrade more Fe as a result. ................ 28 Figure 2.2 - XRD patterns from the a) W 5oCr5o and b) W5 oZr5o powders with increasing milling time. The region around the W (110) Bragg peaks is highlighted to emphasize how, in the W5 oCr 50 patterns, the W and Cr peaks gradually merge with increasing milling time, whereas in the W5 oZr5 o patterns, the W peak essentially remains unmoved................................................... 33 Figure 2.3 - a) The BCC W phase's lattice parameter measured using Rietveld refinement for the various W5 oTM50 couples with increasing milling time. b) Solute concentration in the BCC W phase normalized by the total solute concentration as function of milling time for the same couples. These values were calculated from the BCC W phase's lattice parameter and the data in Fig. 2.1 using a modified Vegard's law as described in the text. c) Average integrated intensities of the W Bragg peaks in the W-Ni/Zr/Hf couples' XRD patterns, I, normalized by their integrated intensities after m illing for one hour, 10 ................................................................... 34 Figure 2.4 - Grain size of the initially pure W phase as a function of milling time measured using the Williamson-Hall technique. Fits to the raw data using Eqn 2.3 are shown as well. The similar rate of grain refinement among the three powders suggests that, at least for short milling times, the W domains are being plastically strained similarly in all three powders.......... 35 Figure 2.5 - SEM micrographs of the a-d) W 5oCr5o and e-h) W5 oZr50 powders milled for the times indicated; scale bars are all 200 nm. The light regions contain W and the dark regions contain either Cr or Zr. Note the lamellar and particulate morphologies of the W5 oCrso and W5 oZr50 couples' microstructures, respectively. Additionally, the lack of contrast in the micrograph of the W 5oCr5s powder milled for 15 hours suggests that this powder is chemically homogeneous, in agreement with the XRD results. i) Mean spacing measured using Eqn. 2.2 of the W5 oCr5 o and W5 oZr5o powders milled for 1, 3 and 5 hours; the data points at 0 hours correspond to the mean particle diameters of the starting powder. Also shown are fits to the mean spacing versus time data using Eqn. 5 in Reference [26]................................................. 37 Figure 2.6 - a) Dark field STEM micrograph of a W 5oZr5o powder particle milled for 45 hours. The white regions are residual W particles in a dark, Zr matrix. b) Cumulative distribution of the W particles' circular equivalent diameters along with an integrated log-normal fit to the diameter data. The mean diameter of the fit is 8 nm, in agreement with the W grain size measured using X R D .............................................................................................................................................. 39 Figure 2.7 - a) Hall-Petch plots for the initially pure W, Cr, and Zr powders. All of the initially pure powders' hardnesses increase, to varying degrees, with milling time, mainly due to grain refinement. Also shown are Hall-Petch trendlines for Ni [ l ], Hf [110], and Nb [1 12] taken from the literature. b) Hardness as a function of milling time for the W 5 oCr5 o and W5 oZr5 O powders along with spline fits to the W, Cr, and Zr powders' hardnesses. The W50Cr50 powder's hardness increased until it was nearly the same as the initially pure W powder, whereas the hardness of the W5 oZr50 powder actually decreased until it is was the same as that of the initially p u re Zr p o w d er.............................................................................................................................. 41 Figure 2.8 - Micrographs of nanoindentations using a cube corner tip into a,b) W50 Cr5 Oand c,d) W 5oZr50 powder particles that were milled for 15 hours. Both powders' pile-up patterns exhibit non-homogeneous plastic deformation (i.e., shear localization). In the W 5oZr5o powder's pile-up, the shear offsets appear to be skirting around the larger W particles in the regions indicated by th e arro w s...................................................................................................................................... 43 Figure 2.9 - a) Evolution in the order parameter a for kinetic Monte Carlo simulations using two different temperatures in a couple with no difference in strength. The two lines that converge for each temperature correspond to two different starting configurations. b) The same set of simulations but using a couple having a large difference in strength between the phases. Note that in the low temperature simulations, the initially segregated and chemically mixed curves do not converge. The insets are two-dimensional slices across the low temperature simulation cells with the A atoms colored grey and the B atoms invisible. ...................................................... 49 Figure 2.10 - Steady state unit cells of A5 oB50 simulations with a-c) no difference in strength and d-f) a large difference in strength. The simulations were performed using the temperatures indicated, and the color scheme is the same as in Figure 2.9. All of the simulations were initialized w ith a segregated m icrostructure. ........................................................................... 52 Figure 2.11 - Evolution in order parameter a during simulations following a cooling trajectory while shearing, using the A's and c's indicated. Note that with increasing c, a large difference in strength is no longer sufficient for preventing mixing: when c equals 0.8, all of the simulations hom ogen ize b y 2 30 K . .................................................................................................................. 53 Figure 2.12 - Dynamical phase diagrams for systems studied as a function of temperature and composition. The regions below the lines correspond to the temperatures at which the various simulations homogenized during the simulated anneals. With increasing phase strength mismatch A, a two-phase region opens up where certain couples remain segregated if they start as such. The open circles on the x-axis indicate compositions that remained dual phase over the range of temperatures studied. Experimental compositions are placed on these diagrams at their expected locations based on the strength differential in a fine nanocrystalline structure from F ig u re 2 .7 ...................................................................................................................................... 55 Figure 3.1 - E1/(D/b2) of binary alloys processed by high-energy ball milling. All of the couples are expected to form single phase solid solutions. While experiments show that the couples colored red do in fact form solid solutions, the couples colored blue form simple m ech an ical m ix tu res. .................................................................................................................... 62 Figure 3.2 - Aggregated Hall-Petch data for pure Cu and Ag. The solid dots indicate the maxim um strength of pure, as-milled Cu and Ag...................................................................... 63 Figure 3.3 - A values for various metal-metal couples whose mixing behaviors have been studied in d eta il.......................................................................................................................................... 65 Figure 3.4 - A values for all metals whose grain size strengthening behavior has been studied. The red and blue squares indicate couples expected to be either mechanically miscible or immiscible, respectively. The grey squares indicate couples that could exhibit either behavior. 66 Figure 4.1 - a) Set of XRD scans taken from the feedstock and W-7Cr-9Fe powder milled for 10 and 20 hrs. Note the disappearance of the Cr (110) Bragg peak in the highlighted region after 10 hrs of milling. This, along with the change in W lattice parameter, suggests the formation of a solid solution. b) Williamson-Hall and Rietveld analysis give the W-rich BCC phase's grain size and lattice parameter as a function of milling time for both alloys. ......................................... 73 Figure 4.2 - Representative TEM micrographs of the as-milled a) W-7Cr-9Fe and b) W-9Fe powders illustrating the powders' nanocrystalline grain structure. The inset electron diffraction patterns feature the uniform rings characteristic of nanocrystalline materials. ........................ 74 Figure 4.3 - Punch displacement curves measured during the heating ramp-up phase for the two alloys, under an applied stress of 100 M Pa............................................................................... 75 Figure 4.4 - Stereological porosity after compaction experiments at a variety of soak temperatures and two soak times, I and 20 minutes................................................................. 76 Figure 4.5 - Backscatter electron micrographs of a) W-7Cr-9Fe and b) W-9Fe compacts consolidated at 1673 K (1400 'C) for 20 minutes. These samples had the coarsest microstructures of all the compacts. The p-phase precipitates in both samples are generally darker than the BCC solid solution due to the lower W content. The precipitates are also distributed randomly throughout the BCC solid solution, which itself is composed of many individual grains. The black dots in both micrographs are residual pores............................... 78 Figure 4.6 - Volume fraction intermetallic predicted by THERMOCALC and measured using stereology for compacts consolidated at temperatures greater than 1373 K. All of the predicted and experimental volume fractions are within 3 vol% of each other, which is reasonable given uncertainties in the global stoichiometry of the powder and the stereology measurements......... 80 Figure 4.7 - Grain sizes of compacts made from both alloys and consolidated at various soak temperatures and two soak times, 1 and 20 minutes. Also shown for comparison is the grain size 81 of th e as-m illed p ow d er. ............................................................................................................... Figure 4.8 - a) Low- and b) high-magnification secondary electron micrographs of the optimized W-7Cr-9Fe compact consolidated using the 20 mm die at 1473 K for 1 min. The lowmagnification micrograph illustrates the distribution of porosity (black regions) and the p-phase intermetallic (darker grey contrast). The high-magnification micrograph illustrates this sample's ultrafine grain structure (D - 130 nm )........................................................................................ 82 Figure 4.9 - Hall-Petch plot for compacts made with both alloys, from samples compacted at various times and temperatures to densities in excess of 98%. Microhardness values from Vashi et al. on nominally pure W compacted to 95% relative density are also presented for comparison [222]. According to Vashi et al., the hardness of their W specimens was independent of load between loads of 0.2 and 2 kgf, and the data shown is the average of the hardnesses measured using loads of 0.2, 0.3 and 2 kgf. The data point labeled with a star is the hardness of the W-7Cr9Fe sam ple consolidated with the 20 m m die.......................................................................... 83 Figure 4.10 - Some typical engineering stress-strain curves from micropillar compression tests on pillars preferentially milled from the BCC solid solution phase. Inset shows a shear offset in a m icropillar loaded to 6.3 G Pa. ............................................................................................... 86 Figure 4.11 - An engineering stress-time curve collected during a Kolsky bar test conducted at a strain rate of 600 s-. The test specimen was cut from the W-7Cr-9Fe compact consolidated at 1473 K using the 20 mm die. The accompanying high speed photographs were taken at the times indicated by the lines. The arrows next to the first frame indicate the loading direction, and the test specimen's orientation is the same in all of the photographs............................................. 87 Figure 5.1 - Schematics of the a) cemented carbide and b) W-8Cr-4Fe penetrators............... 91 Figure 5.2 - a) Radiographs of cemented carbide rounds that struck the targets at the velocities indicated. The crater region is highlighted in the radiograph of the penetrator that had an incident velocity of 720 m/s. b) Cemented carbide rounds' depths of penetration as a function of incident velocity. The dashed line is the best fit to the data using Eqn 5.4, and the grey shaded region indicates the 95% confidence intervals.......................................................................... 95 Figure 5.3 - a) Radiographs of W-8Cr-4Fe rounds embedded in the concrete targets. b) Depth of penetration of the W-8Cr-4Fe penetrators as a function of incident velocity. The rigid body depth of penetration predicted using Eqn 5.4 is shown as well................................................. 96 Figure 5.4 - a) Radiographs of cemented carbide penetrators that shattered on impact. b) Incident velocity versus angle of incidence, y, of the W alloy and cemented carbide shots with the cemented carbide shots that fractured indicated by crosses...................................................... 97 Figure A.1 - Hall-Petch data for the FCC metals. The horizontal grey line indicates the metal's theoretical strength and the vertical gray line indicates the grain size that the pure as-milled po wders w ill d ev elo p .................................................................................................................. 102 Figure A.2 - Hall-Petch data for the BCC metals. ..................................................................... 104 Figure A.3 - Hall-Petch data for the HCP metals....................................................................... 106 List of Tables Table 2.1 - aFe and asolue values used in Eqn 2. 1. The Zr lattice parameter was estimated by extrapolating the P-phase's lattice parameter at 862 'C (3.609 A) to room temperature using the P-phase's coefficient of thermal expansion reported in Reference [104]. The Hf lattice parameter was estimated from P-stabilized alloys [105]. The Ni lattice parameter was estimated from its FCC lattice parameter using the procedure outlined in Reference [106]................................... 30 Table 3.1 - Mechanical alloying behaviors reported for positive heat of mixing metal-metal c o u p le s . ......................................................................................................................................... 60 Table 3.2 - Steady state grain sizes of pure metals during high energy ball milling at room temperature and estimated strength of the pure, as-milled powders from their grain size strengthening data. Grain sizes were either taken from [82-84] or estimated using the trends reported in those References..................................................................................................... 64 Table 4.1 - Compact properties after densification, including specific gravity, p (relative uncertainty: 0.5%), porosity measured using stereology (relative uncertainty: 50%), and porosity calculated from the relative density (relative uncertainty: 20%) for each compact. ................ 77 Table 5.1 - Properties of the cemented carbide and tungsten alloy penetrators....................... 94 1. Introduction The strength of a metal, a, is related to its grain size, D, through the Hall-Petch equation: O (1.1) where o-o and k are material-dependent constants [1]. In Eqn 1, the reciprocal square root dependence on grain size suggests that there should be a dramatic increase in strength as the grain size is refined to the nanoscale. This expectation has been validated in mechanical tests on nanocrystalline materials, where strengths approaching theoretical values have been observed [2]. Figure 1, for example, shows engineering stress-strain curves from microcompression tests on micron-scale pillars ion-milled out of nanocrystalline W powder particles. These stress-strain curves give an average 0.2% offset yield stress of 6.5 GPa, which is ~70% of W's theoretical yield strength [3,4]. 8 6 ~144 2 0 i I strain I i 4% Figure 1. 1 - Engineering stress-strain curves from microcompression tests on micropillars machined out of W powder particles with a grain size of~-10 nm. Because of their high strengths, nanocrystalline materials are very attractive for use in structural applications, and nanocrystalline tungsten in particular would make an ideal penetrator material because it also has a high density. We can illustrate the full potential of nanocrystalline tungsten penetrators by plotting them alongside other penetrator materials in an Ashby map like that shown in Fig. 1.2. Here the x-axis is the density of the penetrator material and the y-axis is the striking velocity at which the penetrator material should transition from rigid body to eroding during penetration into concrete. For a given penetrator geometry, materials that are closer to the upper-right corner of Figure 1.2 can deliver a larger kinetic energy to the target and achieve a greater depth of penetration as a result. Figure 1.2 therefore shows that nanocrystalline tungsten could far outperform currently available penetrator materials such as cemented carbides and high strength steels. 2.0 nanocrystalline_...* tungsten 1.5Limit Velocity (km/s) 1.0- 38 GJ/m cemented carbides 3 15 GJ/m 3 high-strength steels 0.55 3 KE Density = 3 GJ/m 10 15 20 ) Density (103 kg/m 3 Figure 1.2 - Ashby map comparing the predicted performance of different kinetic penetrator materials. The grey lines are isocontours of constant kinetic energy density, which indicate similar ballistic performance for a given penetrator geometry. Nanocrystalline tungsten's exceptionally high strength and density make it ideal for penetration applications. Despite their promise, nanocrystalline materials' commercial applications at the time of this writing tend to be mostly as hard, wear-resistant coatings. This is because their microstructures tend to degrade when exposed to high temperatures due to grain growth [5], which makes producing bulk nanostructured materials particularly difficult as the most promising synthesis method is high temperature densification of powders or foils. To overcome these thermal stability issues, two groups of alloying strategies have been developed. The first group of alloying strategies reduce the soak time and temperature required to sinter a green compact by accelerating low-temperature densification processes [6-8]. The second group of alloying strategies slow or altogether prevent grain growth at elevated temperatures. This is accomplished through the addition of inert second phases that pin the grain boundaries (i.e., Zener pinning) or grain boundary segregating solute elements that reduce either the driving force for grain growth or the grain boundary mobility [9-13]. Since alloying is critical to retaining a fine grain size, high energy ball milling is an important processing step in the powder-route synthesis of bulk nanocrystalline materials because it can simultaneously refine a metal's grain size and introduce a solute element [14-17]. In this process, metal powders and grinding media are sealed in a vial that is then agitated vigorously. Powder particles that get trapped between the grinding media during milling are subjected to plastic strains on the order of 100%, and with an increasing number of such collision events, the powder particles can accumulate very large plastic strains [18-20]. The microstructures that develop as a result of these large plastic strains depend on the milling parameters and the properties of the powders being milled, but in general, they are determined by a competition between plastic deformation and recovery processes. This competition is illustrated most simply with pure metal powders, which all exhibit the same monotonic decrease in grain size to a steady state value during milling [21,22]. In this case, the competition that determines the steady state grain size is between grain refinement, which depends on the milling intensity, and recrystallization, which depends on material properties and the ambient milling temperature. Increasing the ambient milling temperature accelerates recrystallization processes, which in turn leads to higher steady state grain sizes. This was demonstrated by Atzmon et al. in experiments on iron, in which as-milled iron powder's steady state grain size increased by a factor of -2 when the milling temperature was increased from 25 to 160 'C [23]. Because these mechanically alloyed powders possess non-equilibrium steady-state microstructures that result from a dynamic competition between deformation and recovery processes, they are considered driven materials. This same basic competition between plastic deformation and recovery processes also determines the steady state microstructure of alloy powders processed by high energy ball milling, but in an alloy, there can be an additional competition between shear-induced chemical mixing and thermally activated chemical diffusion. As a result, and in contrast with the relatively simple behavior of pure metals, there is a diversity of possible microstructures that can emerge when two or more metals are mechanically alloyed. Some mechanically alloyed powders will mix and form single phase solid solutions, while others will forn dual-phase mechanical mixtures [24]. What is more, even if two metals do not mix completely, they might still dissolve in one another such that they form supersaturated solid solutions [25]. Further, negative heat of mixing couples can form intermetallics [26] or even undergo solid state amorphization reactions [27]. Predicting which of these microstructures will result is critical when designing nanocrystalline alloy powders for consolidation, since the efficacy of the alloying strategies mentioned earlier depend not just on the specific alloying elements, but also on the alloying element's spatial distribution in the base metal. There are three main challenges in predicting the microstructural evolution of a mechanically alloyed powder that are common to all driven materials: 1) Driven materials can develop multiple, distinct steady-state microstructures under a given set of processing conditions [28]. 2) Identifying the steady-state microstructure that a driven material will settle into requires solving an initial value problem in which the initial microstructure evolves with time according to some master equation that is often challenging to develop [28,29]. 3) This master equation is typically noisy, making it difficult to predict which steady state microstructure a driven alloy will settle into when the microstructure starts near a manifold that separates basins containing distinct steady states. What is more, because the magnitude of the noise varies with the instantaneous microstructure, linear stability analyses of steady states cannot be trusted [30-33]. Much of the work addressing these challenges has focused on irradiated materials, which are another type of driven material. So we now turn our attention to the tools that have been developed to describe irradiated materials and mention how these tools have been adapted to mechanical alloying. The earliest attempts at describing the microstructural evolution of irradiated materials mainly focused on solving mass transport equations at hetero-phase interfaces [34,35]. A notable example of this approach is Ref [35], in which Frost and Russell modeled how a precipitate's size evolves under radiation. These investigators developed a mass conservation equation, with a source term that accounted for radiation-induced ballistic mixing, which they then solved in the matrix region adjacent to the precipitate using a mean field approximation. In this way, Frost and Russell were able to predict radiation conditions under which the precipitates would dissolve, coarsen, or even pattern, i.e., shrink or grow to some uniform size. Though this approach could explain several behaviors seen in irradiated materials containing precipitates, it suffered from several deficiencies, including the fact that the solute concentration was not conserved. Adapting this approach to mechanically alloyed materials has also proven difficult because it is unclear how to account for shear-induced chemical mixing in a conservation equation. A more general framework for describing irradiated materials was proposed by Martin, who added a ballistic mixing term to Cahn's free energy functional and then studied what this new functional predicted for the steady-state microstructure under irradiation [36-38]. Using this modified functional, Martin showed how the phases present in a driven material are the same ones present at some elevated, effective temperature, Ter, given by Teff = T(1 + 0) (1.2) where T is the actual temperature of the irradiated material, and 0 reflects the competition between ballistic mixing and thermally activated recovery and is always positive. For an irradiated material, Martin demonstrated that 0 = Db,rad/Dt (1.3) where Dt is the classic interdiffusivity that follows an Arrehnius-law temperature dependence, and Db,rad is a ballistic diffusivity that accounts for chemical homogenization due to irradiation. Figure 1.3 shows the effective temperature as a function of temperature for a material subjected to a constant intensity driving force. Here T and Tef are nearly equal above ~500 K because Dt is much larger than Db,rad so that 6 is approximately 0. T and Terr diverge at lower temperatures, since Dt's exponential dependence on temperature causes it to decrease dramatically with decreasing temperature, thereby causing 0 to blow up. At temperatures below the minimum in the Tetf curve, decreasing the temperature or increasing the driving force's intensity result in higher effective temperatures, which in turn correspond to non-equilibrium microstructures with higher free energies. To help explain his "rule of corresponding states," Martin suggested that radiation, or any other driving force, contributes an additional entropy-like term to the free energy, which stabilizes high temperature phases at low ambient temperatures. With this rule-ofthumb, Martin successfully explained a number of phenomena observed during the irradiation of alloys, such as the disordering of ordered compounds, the formation of supersaturated solid solutions, and the amorphization of certain alloys [39]. 1200 800 TO (K) Te = T(1 + 0) 400 400 800 T (K) 1200 Figure 1.3 - Effective temperature as a function of ambient temperature under a constant intensity driving force. At high temperatures, Teti and T are similar because thermally activated processes outpace processes related to the driving force, while at low temperatures, Tety and T diverge because the thermally activated processes are suppressed. Two mechanical alloying studies have demonstrated that Martin's rule of corresponding states can also be extended to certain materials subjected to extensive plastic deformation. In the first of these studies, Pochet et al. mechanically milled an FeAl intermetallic at various temperatures and intensities and then measured the as-milled powder's long range order parameter (LRO) [40]. These investigators found that they could decrease the LRO, in other words drive the intenmetallic from its equilibrium state, by either increasing the milling intensity at constant temperature or by lowering the temperature at constant milling intensity. They rationalized the effects that these processing changes had on the LRO with Martin's effective temperature concept by replacing Dbrad in Eqn 1.2 with a new ballistic diffusivity, Db,MA, that accounts for shear-induced chemical mixing. In this case, increases in the milling intensity, which increase DbMA, or decreases in temperature, which decrease Dt, both translate to higher effective temperatures that correspond to non-equilibrium microstructures with a smaller LRO. In another mechanical alloying study whose results support the rule of corresponding states, Klassen et al. investigated the effect of ambient milling temperature on the chemical mixity of Ag 5oCu 5o alloy powders [41]. In these experiments, Klassen et al. mechanically alloyed the powders at temperatures between 85 and 473 K and found that the solubility in the terminal solid solutions increased with decreasing temperature, until at low enough temperatures, the alloy homogenized. Since this alloy is dual-phase with negligible solid solubility in either phase at equilibrium at room temperature, by lowering the milling temperature, Klassen and coworkers were driving the alloy into a non-equilibrium, high-temperature configuration. Their explanation of this behavior followed that of Pochet et al.: by decreasing the milling temperature, they were decreasing Dt, which in turn raised the effective temperature, thereby stabilizing the phases' high-temperature solid solubilities. The results from both of these mechanical alloying studies are well described by the effective temperature framework because the systems studied obey one of Martin's core assumptions: the driving force affects both components of the alloy equally. This assumption, however, is invalid for many mechanically driven materials, particularly those with initial microstructures that contain two phases, since there can be strain localization in one of the phases. Such strain localization does not affect the FeAl intermetallic studied by Pochet et al. because it is already chemically homogeneous, nor does it affect the Cu-Ag couple studied by Klassen and coworkers because these alloying elements have similar strengths when nanocrystalline and so co-deform; however, one must account for the fact that the driving force can have a stronger effect on one of the components in order to generalize the effective temperature concept to all mechanically alloyed systems. Besides the rule of corresponding states, which serves well as a qualitative rule-of-thumb, other theoretical tools have been developed that provide more quantitative descriptions of driven materials. Of these tools, many of which are adapted from the physical chemistry field of dissipative systems, the master equation initially found the most use [42]. The master equation is a differential equation that describes the time evolution of the microstructure, and its steady state solutions correspond to the steady state microstructures. The first master equation describing an irradiated material was developed by Bellon and Martin in their work on electron-irradiated Ni 4 Mo [29]. This particular system was of interest because it had been experimentally studied in detail by Urban and coworkers and was known to exhibit several interesting behaviors, including bi-stability and path-dependent steady state order parameters [43,44]. To describe these behaviors, Bellon and Martin first developed equations that gave the probability of transitions between different states of ordering. They then incorporated these transition probabilities into a master equation, with which they developed a dynamical potential whose maximum indicated the order parameter most likely to be observed. Following Bellon and Martin, Haider et al. developed another master equation that described a different ordered compound [45-47]. These investigators used their master equation to generate maps like that shown in Figure 1.4. With one of these maps, one can identify the microstructures that an irradiated alloy will eventually settle into by tracing the arrows from a starting point, which corresponds to the initial order parameter, to a steady state order parameter. In their study on the mechanical milling of FeAl, Pochet et al. developed a master equation for mechanically alloyed materials [40]. With this master equation, these investigators calculated dynamical phase diagrams that indicated milling conditions under which the alloy should disorder. 00 %% %-% % .0.0% //ef%%* a .&o tI - % I'. 'tV OX3 Figure 1.4 - Cross-section of a 3-dimensional phase diagram [451. The axes indicate the concentration on each of the four, interpenetrating simple cubic sublattices of a facecentered cubic metal. To identify the steady-state order parameter of an irradiated material with this diagram, follow the arrows from a starting order parameter to one of the steady state order parameters indicated by the triangle, diamond, or square. In addition to the master equation, fixed-lattice, kinetic Monte Carlo simulations have been borrowed from the dissipative systems community and adapted to describe driven materials [4851]. The advantage of kinetic Monte Carlo simulations over the master equation is that the simulations better capture the stochastic nature of the driving process [52-55]. The kinetic Monte Carlo simulations of driven materials that Bellon and colleagues have developed all feature the same two competing dynamics: a temperature-dependent vacancy migration mechanism and an athermal mixing mechanism. The specific mixing mechanism depends on the system being studied, but in kinetic Monte Carlo simulations of irradiated materials, it involves random exchanges of atoms [55-58]. With these kinetic Monte Carlo simulations, Bellon and colleagues have studied how the order parameter of compounds as well as the chemical mixity of positive heat of mixing, immiscible alloys evolve under irradiation [59-61]. In general, the simulation results have aligned well with Martin's rule of corresponding states: higher effective temperatures achieved by lowering the temperature or increasing the rate of ballistic exchanges correspond to microstructures with higher excess free energies. However, the simulations have also revealed behaviors that could not have been predicted by the effective temperature concept such as patterning [62-67], which have recently been demonstrated in experiments [68]. The kinetic Monte Carlo simulations use a different mixing mechanism to model mechanically alloyed materials: instead of exchanging randomly selected atoms, the simulation cell is sheared along two randomly selected glide planes in the same slip system [69,70]. From a historic perspective, it is interesting to note the similarity between this shearing mechanism and that from simulations used by the fatigue community in the 70's and 80's to model precipitate dissolution during the low-cycle fatigue of age-hardened materials [71,72]. In one of these earlier fatigue studies, Lee et al. even went so far as to build a two-dimensional physical model of the BellonAverback kinetic Monte Carlo simulations [72]! Historical notes aside, these kinetic Monte Carlo simulations of mechanical alloying have been used to study the evolution in chemical mixity of binary, phase-separating alloys. In line with expectations, the simulations demonstrate that the steady-state chemical mixity is determined by a competition between shear-induced mixing and thermally activated phase separation and that it is possible to tune the chemical mixity of the simulation cell by independently changing the rate of either process. Figure 1.5, for example, shows cross-sections of simulation cells that had reached their steady state chemical mixity. Each of these simulations were conducted at the same temperature but with different shearing frequencies, as indicated. The black dots in the cross-sections correspond to one of the alloying elements, and they are clearly more homogeneously distributed in the solvent in the simulations with higher shearing frequencies. Another behavior seen in these Bellon-Averback simulations was that domains of the two phases developed a characteristic length scale that depended on the effective temperature. Such patterning behavior was subsequently demonstrated in Cu-Ag alloys mechanically alloyed at elevated temperatures [73,74]. In general, the mixing phenomenology seen in the simulations matches closely that seen in CuAg alloys, but not most other couples. This is because the classical Bellon-Averback simulations share the same deficiency as Martin's law of corresponding states: they do not account for strain localization. In fact, these kinetic Monte Carlo simulations ignore essentially all of the mechanisms of plastic deformation in a nanocomposite. In a real nanocomposite prepared by high energy ball milling, there are line defects, incoherent heterophase interfaces, and high angle grain boundaries separating misoriented grains, and all of these features influence the plastic deforiation behavior and as a result the rate of shear-induced chemical mixing. By contrast, in these kinetic Monte Carlo simulations, there are no defects and only one deformation mode, shearing of one plane of atoms over another. y = 10, ST = 400 K y = 10 3 sO T = 400 K y = 1 s1 T = 400 K Figure 1.5 - Cross-sections from kinetic Monte Carlo simulations of mechanical alloying [70]. Above each of the cross-sections is the shearing rate and temperature used in the simulation. The black dots indicate atoms of one of the alloying elements. The crosssections show that with decreasing shearing frequency, the alloy is able to phase separate. To develop a better understanding of how mixing proceeds in reality, researchers have studied the deformation of dual-phase nanocomposites in molecular dynamics (MD) simulations [7579]. In these simulations, the atoms are not constrained to a lattice so the mixing processes more closely reflect reality, revealing behaviors that could not have manifested in the kinetic Monte Carlo simulations. For example, the MD simulations have revealed that the character of a heterophase interface influences the rate of shear induced mixing across that interface [79], an effect that is absent from the kinetic Monte Carlo simulations since there are no interfaces per se. The simulations have also highlighted the dramatic effect that differences in the constituent phases' strengths can have on their mixing behaviors. This is illustrated by Figure 1.6, taken from Ref [77], which shows results from MD simulations in which precipitates of Ag and V are being dissolved in a Cu matrix through cyclic plastic straining. In Figure 1.6, the atoms' colors indicate their local chemical environment, with atoms colored green representing solute atoms whose nearest neighbors are also all solute atoms. Since the initial volume fraction of the precipitate was the same in both simulations and both simulations received the same total plastic strain, the much larger fraction of green atoms in Fig 1.6b relative to Fig 1.6a demonstrates that shear-induced mixing proceeds faster in the Cu-Ag couple than in the Cu-V couple. This can be explained by the much smaller fractional difference in strength between Cu and Ag than between Cu and V when nanocrystalline. This results in less strain localization in the matrix in the Cu-Ag couple and faster shear-induced mixing as a result. Hence, these MD simulations reproduce the strain localization behaviors that are absent from the kinetic Monte Carlo simulations and Martin's law of corresponding states, but that are expected intuitively and that play a very important role in the microstructural evolution of mechanically alloyed materials. Cu-Ag Cu-V Figure 1.6 -MD simulations of shear-induced mixing in a (a) Cu-Ag and a (b) Cu-V nanocomposite [771. Both of the simulations began with all of the solute in a single precipitate, and both volume elements have accumulated plastic strains of 60. The solute atoms are colored to indicate their local chemical environment, with green atoms indicating solute surrounded by solute nearest neighbors. The simulations reveal that the V precipitate is still relatively in-tact, while the Ag precipitate is nearly completely dissolved. Although these MD simulations are very useful for studying the mechanisms of mixing, they are not without drawbacks: they simulate timescales on the order of nanoseconds; do not include thermally-activated recovery phenomena; and are therefore incapable of predicting the steadystate microstructure of a mechanically alloyed powder. The preceding discussion has highlighted the important role that mechanical alloying plays in the powder-route synthesis of bulk nanostructured materials, and the need to predict the as-milled powders' chemical mixity in order to design powders that can be consolidated. As the preceding discussion also makes clear, all of the current tools and frameworks that predict the chemical mixity of mechanically alloyed materials have drawbacks that limit their usefulness: - the core assumption of the rule of corresponding states does not apply to materials that exhibit strain localization; - the master equation is often difficult to develop and is deterministic, while the actual mechanical alloying processes are stochastic; - the MD simulations do not incorporate important thermally activated recovery processes; - and the kinetic Monte Carlo simulations treat plastic deformation too simplistically. This thesis aims to enable the microstructure design of mechanically alloyed materials by addressing the deficiencies of the classical Bellon-Averback Monte Carlo simulations with insights provided by mechanical alloying experiments as well as the MD simulations in the open literature. This thesis then seeks to apply the lessons learned from these improved simulations in an engineering application: the synthesis of a nanocrystalline alloy powder with a specific microstructure that enables its rapid consolidation into bulk, ultrafine grained articles. These two, complementary goals are addressed in the following chapters which are organized as follows: * Mechanical alloying experiments on tungsten-transition metal couples with various fractional differences in strength are described in Chapter 2. Learning from these experiments, we then modify the classical Bellon-Averback kinetic Monte Carlo simulations to account for phase strength effects, thereby making them better predictors of an extensively deformed material's chemical mixity. " In Chapter 3, maps are generated that are based on insights from our improved simulations and that indicate couples expected to mix to a chemically homogeneous state under different processing conditions. " A specific nanocrystalline W-Cr-Fe alloy powder is introduced and its consolidation behavior explored in detail in Chapter 4. Because of this powder's highly non- equilibrium, as-milled microstructure, it can be compacted into fully dense parts with a high strength and specific gravity that are ideal for penetration applications. 0 Results from preliminary ballistic tests on rounds made from this alloy are described in Chapter 5. 2. Phase Strength Effects on Chemical Mixing in Extensively Deformed Alloys Although there are examples of immiscible couples (e.g., Cu-Co [80] and Ag-Cu [81]) that form solid solutions during mechanical alloying, others remain phase separated over a range of compositions despite being milled at low homologous temperatures (e.g., Cu-W [82] and Cu-Ta [83]). One reason that some couples remain dual phase, which was described in detail in the Introduction, is that plastic deformation occurs preferentially in the softer phase, and as a result, atoms are not sheared across the interphase interface [75,77]. Thus, alloying elements must codeform for deformation-induced mixing to occur, and one way to encourage co-deformation is to mechanically alloy elements with "similar" mechanical properties [24]. For dual phase metallic systems with coarse microstructures, it is also well established that the amount of co-deformation depends not just on the individual phases' mechanical properties but also on microstructure, and specifically the two phases' volume fractions and geometries [84-87]. For example, in alloys with a small volume fraction of a hard element, the softer element can flow around the hard element without the hard element deforming; however, this becomes more difficult as the volume fraction of the hard element increases [88]. Hong and Fultz [25] and others [89,90] have suggested that microstructure and mechanical properties can influence the amount of deformation-induced mixing during mechanical alloying. There have also been several recent molecular dynamics studies investigating the effect of the alloying elements' mechanical properties on the mechanisms of deformation-induced mixing [76-79]. But while there are many isolated data points, some empirical rules-of-thumb, and qualitative discussion about the roles of the constituent phases' mechanical properties and the couple's microstructure in mechanical alloying, we are not aware of a general quantitative heuristic by which mixable couples (or conditions under which couples can become mixable) can be predicted. Our purpose in this Chapter is to provide a step towards such a view through systematic study by both experiment and simulation. Experimentally, we track the microstructure, mechanical properties, and amount of co-defornation and mixing in several Wtransition metal couples subjected to mechanical alloying. Computationally, we adapt a classical Bellon-Averback kinetic Monte Carlo simulation of mechanical alloying [69,70,91] to demonstrate how a difference in phase strength leads to multiply stable steady states. The results together point to the possibility of understanding preferred conditions for forced mechanical mixing. 2.1. Materials and Methods 2. 1.1. Powder Processing Elemental W, Cr, and Zr as well as several equiatomic W50 TM50 alloys (TM = Cr, Nb, Ni, Hf, or Zr) were milled in a SPEX 8000 high-energy ball mill. The powders were acquired from Alfa Aesar, and had the following purity and sizing: W, 99.95%, -200+325 mesh; Cr, 99+%, -325 mesh; Zr, 99.6%, -325 mesh; Nb, -325 mesh, 99.8%; Ni, 99.996%, -120 mesh; Hf, 99.6%, -325 mesh. We selected W as the base alloying element because the maximum temperature encountered in a SPEX ball mill (~100 'C [92]) is just 10% of its melting temperature. As a result, interdiffusion in the W9 oTM 5 o couples is, to a good approximation, kinetically suppressed, and structural evolution only proceeds through plastic deformation. The alloying elements were selected because their maximum hardnesses (once refined into a nanocrystalline state) ranged from a low of 6 GPa (Zr [93]), to a high of 16 GPa (Cr), as compared to 22 GPa for W. M 25- WwNbw +.4 WsoCrso 20V U_ Z150- y4WwNiw 5 V* V * + W 5 Hf 25 30 01, 0 5 10 15 20 Time (hrs) Figure 2.1 - Fe contamination as measured using EDS in the initially pure W and Wtransition metal powders as a function of milling time. The W, W5oCr5 o, and W 50Nb5 O powders are harder than the W 5oNi5 o, W5oHf5o, and W50Zr5 o powders, and abrade more Fe as a result. The W 50 TM 50 alloys were prepared by mechanically alloying elemental feedstock powders. All of the milling runs were conducted using a steel vial and grinding media with a ball-to-powder ratio of 5:1 (10 g powder). To prevent oxidation, the milling was performed in a glovebox maintained under an ultra-high purity Ar atmosphere. To monitor the structural evolution of the powder particles, -0.2 g of the powder were removed periodically for subsequent characterization. 2.1.2. Microstructuraland Chemical Characterization The grain size and lattice parameter of the W-rich, BCC phase was tracked with milling time using X-ray diffraction (XRD). XRD patterns were collected using a Cu-Ka source Panalytical X'Pert Pro operated at 45 kV and 40 mA. The lattice parameter, which can be used to infer the amount of solute dissolved in the W and therefore the degree of mixing, was measured using Rietveld refinement. The grain size was calculated from the peak broadening using a Williamson-Hall analysis after correcting out the contribution from instrumental broadening using a NIST LaB6 standard. Following XRD, the powders were cold-mounted in epoxy, rough ground, and polished; polishing concluded with a colloidal silica suspension. Energy dispersive spectroscopy (EDS) was performed on these mounted samples using a JEOL 6610-LV scanning electron microscope (SEM) operated at 20kV, to measure the amount of Fe contamination due to abrasion of the steel vial and media. The total amount of Fe contamination as a function of milling time for the various couples and pure W is shown in Figure 2.1. We highlight the W, W 5 oCr5 o, and W5 oNb5 O data in red to emphasize that these powders had a similar amount of Fe contamination, which was greater than that of the W 5oZrso, W5oHf5O, and W50 Ni50 powders, highlighted blue. The concentration of solute, x, dissolved in the BCC W phase was calculated from the measured lattice parameter using Vegard's law: = (a, -- a.,) (a.,. -a,) (2.1) xFB(ae-ar) (a,. -a,) where xFe is the concentration of Fe dissolved in the W and aw, aFe, asolite, and aBcc are the pure W, pure Fe, pure solute, and measured lattice parameters, respectively. The first term in this expression is the standard form of Vegard's law for a binary couple, and the second term is added as a correction to account for the pickup of iron from the milling media and vial. The alloying elements' lattice parameters are given in Table 1; note that estimated BCC lattice parameters were used for the non-BCC alloying elements: Zr, Hf, and Ni. We estimated xFe by multiplying the global concentration of Fe in the as-milled powder (Figure 2.1) by the fraction of Fe dissolved in the W phase. The fraction of Fe dissolved in the W phase was calculated from a control experiment in which we milled initially pure W, and measured the global concentration of Fe using EDS and the concentration of Fe in the W lattice using Vegard's law with milling time. The ratio of these quantities gave the fraction of Fe dissolved in the W, which we assumed to be the same for pure W and the W 50 TM50 couples for a given milling time. The W5 oCr5o and W5 oZr5 Ocouples were down-selected for a more in-depth investigation of their microstructure using SEM and dark field STEM. These couples were selected for two reasons. First, the W5 oCr5 o and W5 oZr5 o couples' behaviors are representative of systems that either do or do not mix, respectively, after long milling times, as will be seen shortly. Second, the difference in atomic number between W and either Cr or Zr is such that, prior to atomic mixing, there is sufficient contrast in either SEM or dark field STEM to qualitatively gauge chemical inhomogeneity. For milling times up to ~5 hours, the chemical inhomogeneity of the W 5oCr5 o and W5 oZr5 O couples could be monitored using back scatter imaging in a FEI Helios Nanolab 600 SEM operated at 5 kV. The mean spacing, X, between nominally pure W regions inside the powder particles was measured using I = (2.2) NL where Vw is the volume fraction of W and NI is the number of interceptions of W per unit test line [94]. We found that negligible atomic mixing occurs up to 5 hours (as will be seen in the next section), so Vtw could be assumed constant and equal to that for the elemental powder mixture of W 50 TM50 (Vw = 0.57 for W5 0 Cr5O; Vw= 0.41 for W5 oZro). The mean W spacing, k, is also proportional to the mean intercept length of the W regions [94], with a proportionality constant of 0.8 and 1.4 identified for W-Cr and W-Zr couples respectively. Table 2.1 - ape and aSolte values used in Eqn 2.1. The Zr lattice parameter was estimated by extrapolating the P-phase's lattice parameter at 862 'C (3.609 A) to room temperature using the p-phase's coefficient of thermal expansion reported in Reference 1951. The Hf lattice parameter was estimated from P-stabilized alloys [961. The Ni lattice parameter was estimated from its FCC lattice parameter using the procedure outlined in Reference 1971. Element aVelaIe (A) Ref. Fe 2.866 [97] Cr 2.885 [97] Nb 3.301 [97] Zr 3.57 [95] Ni 2.793 [97] Hf 3.50 [96] Beyond 5 hours of milling, it became difficult to resolve the individual phases using the SEM. Therefore, samples milled for 45 hours were inspected using dark field STEM in a JEOL 2010F operated at 200 kV. TEM specimens were prepared from individual powder particles using the FIB liftout technique [98] so as not to distort the as-milled microstructure. 2.1.3. Mechanical Testing Nanoindentation was also performed on as-milled W, Cr, Zr, W5oCr5 o and W 5 oZr5 O powders to correlate the evolution in microstructure with that in mechanical properties. The Zr, Cr, and WSoZr5 o nanoindentation test specimens were prepared in the same manner as that used for the SEM specimens. A different mounting material (solder glass EG2934 VWG from Ferro Corp.) was used for the W and W 50Cr5 0 powders to minimize substrate compliance effects in mechanical testing. The molten glass (~700 'C) was poured onto powder in a steel retaining ring, which was then quenched in brine. The maximum temperature during this process was well below the temperatures at which thermally activated relaxation processes become noticeable in pure W [99], and the time of thermal exposure was only a few seconds. XRD and TEM were used to confirm that there was no grain growth, segregation, or substantial oxidation during mounting. Nanoindentation tests were performed using a Hysitron Triboindenter 950 with a diamond Berkovich tip. The tip's area function and the frame compliance were calibrated using a fused silica standard. The Oliver-Pharr method [100] was used to extract hardness and reduced modulus from the load-displacement curves. Additional nanoindentation tests were performed using a cube corner tip to augment the pile-up patterns, and these nanoindentations were inspected by SEM. 2.2. Microstructure and Hardness Evolution Inspection of the five W 50 TM50 couples' XRD patterns suggests that these couples exhibit one of two main alloying behaviors, either forming a solid solution or remaining phase separated after long milling times. These two behaviors are typified by W-Cr and W-Zr in Figure 2.2a and 2.2b, respectively. In the W5 0 Cr50 and W 50Nb5 Ocouples' XRD patterns, the W and Cr/Nb Bragg peaks broadened and gradually merged with milling time (Figure 2.2a). The merging Bragg peaks reflect a homogenization of the two BCC phases' lattice parameters as the W and Cr/Nb dissolved in each other to form a single BCC solid solution. In the other couples' (W5 oZr5o, W 50 Hf5 0 , and W 5oNi 5o) XRD patterns, the W Bragg peaks broadened as well, but their integrated intensities decreased and their positions did not change appreciably with milling time. Simultaneously, the low angle Zr/Hf/Ni Bragg peaks broadened and merged into a single broad hump (Figure 2.2b), characteristic of an amorphous solute-rich phase [101]. These latter couples were clearly still dual phase after milling, and the stationary W Bragg peaks suggest that a limited amount of solute dissolved in the W phase. Applying our modified Vegard's law (Eqn 2. 1) to the W lattice parameter data shown in Figure 2.3a gives the amount of solute dissolved in the BCC W phase. Figure 2.3b contains these calculated solute contents normalized by the global non-ferrous solute content, xO. The values in Figure 2.3b provide an indication of the powder's chemical homogeneity: the limiting values of zero and one correspond to phase-separated and chemically homogeneous alloys, respectively. Thus the results in Figure 2.3b support the interpretation that the W 50 Cr5 o and W5 oNb5 o couples formed a solid solution when milled in excess of 15 hours, whereas in the W 5 oNi5 o, W 5 oHfO, and W5 oZr5 o couples, there was negligible solute in the W phase even after 25 hours of milling. a. .OW e Cr 1 hr 3 C 25 01 -15 25 b Wr 1 hr Zr C C5 015 50 75 100 Position (020) Figure 2.2 - XRD patterns from the a) W5 oCr5 o and b) W5oZr5o powders with increasing milling time. The region around the W (110) Bragg peaks is highlighted to emphasize how, in the W 5oCr5 o patterns, the W and Cr peaks gradually merge with increasing milling time, whereas in the W5oZrso patterns, the W peak essentially remains unmoved. To a good approximation, changes in integrated intensity are proportional to changes in the volume fraction of a phase during mechanical alloying [101]. Therefore, normalizing the integrated intensities of the W Bragg peaks at later milling times by their integrated intensities after milling for one hour as done in Figure 2.3c, gives a rough measure of relative changes in the BCC W phase fraction. According to Figure 2.3c, the decreasing integrated intensity of the W Bragg peaks in the W5 oZr5o, W 5oHf5 o, and W50Ni50 XRD patterns suggest that some W was lost from the BCC W phase and thus dissolved into the second phase (rich in the alloying M- element) in each of these couples. Additionally, the volume fraction of W in the W5oZr5o and W50Hf5 O couples started to plateau value after -15 hours of milling. As for the W 5oNi 5o couple, the W volume fraction appears to continue decreasing even after 15 hours of milling but this is most likely due to the comparatively larger Fe contamination in this system that continues to alter the global powder composition. a3.2 0 S-- I- *el- 4) 3.1 5 E ,q~---~ W5 Hf50 - -- W,0Nb 0 ==-I WeZr5O WVNi5 ------ W5Ni50 qW 3.1 0 - 3.0 5 -qW b. 1. U 50rs mixed LI 0. 8- X 0. 6- X* 0. 40. 2 -0 C. 0.8 0.6 unmixed + 0 0. 0 1. 0 0 t 1 10 V 0.4. 0.2-I A' . 0I 0 10 a 20 Time (hrs) I 30 Figure 2.3 - a) The BCC W phase's lattice parameter measured using Rietveld refinement for the various W5 oTM5 o couples with increasing milling time. b) Solute concentration in the BCC W phase normalized by the total solute concentration as function of milling time for the same couples. These values were calculated from the BCC W phase's lattice parameter and the data in Fig. 2.1 using a modified Vegard's law as described in the text. c) Average integrated intensities of the W Bragg peaks in the WNi/Zr/Hf couples' XRD patterns, I, normalized by their integrated intensities after milling for one hour, 10. It is significant that in the above systems, W appears to dissolve into the second element, while the evidence suggests little dissolution of the second element in the BCC W. Similar asymmetric mixing kinetics have been observed in other mechanically alloyed couples (Mo-Ni [102,103] and W-Ni [101]), and Ashkenazy et al. [77] demonstrated using molecular dynamics simulations that asymmetric mixing is likely a general feature of mechanical alloying in couples with a large difference in strength. 80 V W * W50Cr50 * E W 50Zr5 60 1 N (n, C - 40 I 20 1 0 5 10 Time (hrs) 15 Figure 2.4 - Grain size of the initially pure W phase as a function of milling time measured using the Williamson-Hall technique. Fits to the raw data using Eqn 2.3 are shown as well. The similar rate of grain refinement among the three powders suggests that, at least for short milling times, the W domains are being plastically strained similarly in all three powders. The peak broadening in all of the couples' XRD patterns was due predominantly to grain refinement and microstrain with some contribution from chemical heterogeneity as evidenced by the W Bragg peaks' asymmetric shapes. The grain size of the BCC W phase measured using the Williamson Hall technique for the pure W, W5 oCrjo, and W5 oZr50 powders are shown in Figure 2.4 as a function of milling time. Note that the Williamson-Hall technique does not account for chemical heterogeneity's contribution to peak broadening, so the grain size at later milling times in Figure 2.4 may be artificially small. All of the grain sizes exhibit a typical exponential refinement trend given by [104] (2.3) D=DF+(DO -DF)e-" where Do is the starting grain size, DF is the final grain size, t is the total time milled, and k1 is a rate constant that depends on both the milling parameters and material properties; fits to the data using Eqn. 2.3 are included in Figure 2.4. The three sets of data indicate that the W grain size refines at a similar rate, but to a slightly different steady state grain size depending on the presence and type of alloying element. Because grain size is inversely proportional to the accumulated plastic strain during the early stages of mechanical alloying [104,105], the data in Figure 2.4 also reveal that, at least for short milling times, the W is co-deforming along with the Zr. The grain size of the second phases could not be accurately tracked in any of these systems because of their small diffraction signatures. 1 hr 3 hrs 5 hrs 15 hrs L 4 10 0 W50Zr. + Cr 10 3 ) 102 C 101 1 0 1 2 Time (hrs) 4 6 Figure 2.5 - SEM micrographs of the a-d) W 5 oCr5 o and e-h) W 5oZr5o powders milled for the times indicated; scale bars are all 200 nm. The light regions contain W and the dark regions contain either Cr or Zr. Note the lamellar and particulate morphologies of the W5 oCr5 o and W 50 Zr5 O couples' microstructures, respectively. Additionally, the lack of contrast in the micrograph of the W5 0 Cr5 0 powder milled for 15 hours suggests that this powder is chemically homogeneous, in agreement with the XRD results. i) Mean spacing measured using Eqn. 2.2 of the W5 oCr5 o and W 50 Zr50 powders milled for 1, 3 and 5 hours; the data points at 0 hours correspond to the mean particle diameters of the starting powder. Also shown are fits to the mean spacing versus time data using Eqn. 5 in Reference [26]. For the WsoCrso and W5 oNb5 O couples, the amount of solute dissolved in the W phase exhibited a typical sigmoidal time-dependence (cf. Figure 2.3b), with an incubation period prior to the onset of substantial shear-induced mixing [106,107]. During the incubation period, the individual powder particles consisted of nominally pure solute and W regions. The evolution in the W regions' shape, mean spacing, and size provides insight into the degree of co-deformation, and is explored in the series of SEM micrographs in Figure 2.5. For example, the W regions in the W5 oCr5 o couple maintained a lamellar structure for milling times up to 5 hours, indicating that the W and Cr were deforming compatibly (Figures 2.5a-c). Over this same period, the W regions in the W5 oZr5 o couple were comminuted into smaller particles suggesting that the much softer Zr was undergoing large plastic straining and that the W, unable to deform compatibly, fractured instead (Figures 2.5e-g). Aning et al. observed a similar break-up of the W regions in their study of mechanically alloyed W-Ni [101]. b. 1.0 afit data U- 0.5 L-I 0.5 :-XRD 0.0 0 j-------_A 10 Particle Diameter (nm) - " 20 Figure 2.6 - a) Dark field STEM micrograph of a W5oZr5 o powder particle milled for 45 hours. The white regions are residual W particles in a dark, Zr matrix. b) Cumulative distribution of the W particles' circular equivalent diameters along with an integrated lognormal fit to the diameter data. The mean diameter of the fit is 8 nm, in agreement with the W grain size measured using XRD. Despite the couples' different morphologies, their mean spacings and domain sizes initially refined at similar rates as shown in Figure 2.5i, only diverging after the onset of mixing in the W 5oCr5o couple at -5 hours of milling. The onset of mixing in the W5oCr5o couple occurred because refinement in the mean thickness of the W lamellae in the W 5oCr5o couple led to a concomitant increase in the amount of interface between the W and Cr domains. This in turn led to an increase in the rate of mixing because there was more material that could be carried across the interface between the two phases by plastic deformation. In contrast to the gradual dissolution of the W regions in the W5 oCr5o powder, the mean diameter of the W regions in the W5oZr5 O powder was refined until it reached a lower limit, namely the W grain size. This is illustrated by the dark field STEM micrograph shown in Figure 2.6a of a W 5 0Zr5 O powder particle after milling for 45 hours. residual W particles dispersed in a dark Zr matrix. In this micrograph, the light regions are The cumulative distribution of the W particles' circular equivalent diameters is given in Figure 2.6b along with an integrated lognormal fit with a mean particle diameter of 8 nm, consistent with the W grain size measured using XRD (9 nm). Similar microstructures have been observed during severe plastic deformation studies of Cu-Nb alloys [108,109]. Although the sample in Figure 2.6a was milled for 45 hours, we estimate that the particle diameter and grain size reach similar values between 5 and 10 hours of milling based on the time dependencies measured in Figures 2.4 and 2.5i. The elemental W, Cr, and Zr powders' hardnesses increased rapidly during milling, before plateauing after roughly 5 hours. These elemental powders are predominantly grain size strengthened, so this trend in hardness can be attributed to their grain refinement. We demonstrate this by plotting the powders' hardness against their reciprocal square root grain size in Figure 2.7a; the Cr and Zr data both conform to a Hall-Petch scaling. As for the W data, there is a slight, negative deviation from the expected linear dependence on reciprocal square root grain size at the smallest grain sizes, which we ascribe to the presence of Fe that softens the W powder. For comparison purposes, Figure 2.7a also contains Hall-Petch trendlines for Hf [110], Ni [111], and Nb [112] taken from the literature. Figure 2.7b shows the behavior of the mixed elemental powders, which contrast with the uniform behavior of the elemental powders. The WsoCr5o powder's hardness increased with milling time until it was similar to that of the W powder, whereas the W5 oZr5 Opowder's hardness actually decreased until it was similar to that of the Zr powder. From the microstructure of the W5 oCr5 o powder, these powders are both grain size and solid solution strengthened. Thus, the W5 0 Cr5 O particles are an additional ~4 GPa harder than the as-milled Cr particles [113]. The W5oZr5 o powder's decreasing hardness with milling time reflects a decreasing amount of co-deformation. The convergence of the W5 oZr5 o and Zr hardnesses after 15 hours of milling suggests that, by this point, plastic deformation was accommodated solely in the softer Zr phase and that this Zr phase has a similar hardness to that of pure Zr (in a milled, refined state). Grain Size (nm) a. 100 25 11 -OW -o Cr 20 09 [50] .Nb, - 15 - -2 10- -Hf, CO [48] V de AZr Ni, [49] - 5 5 0.2 0.1 b. 2 (nm)-1 2 D 1/ *W 0.3 5Cr0 W50Zr50 - - 20- 1--- 15 /C' W -- -, Cr (D C . - ~20 Zr 50 5 10 Time (hrs) 15 Figure 2.7 - a) Hall-Petch plots for the initially pure W, Cr, and Zr powders. All of the initially pure powders' hardnesses increase, to varying degrees, with milling time, mainly due to grain refinement. Also shown are Hall-Petch trendlines for Ni [1111, Hf [110], and Nb [112] taken from the literature. b) Hardness as a function of milling time for the W 5 oCr5 O and W5 oZr5 o powders along with spline fits to the W, Cr, and Zr powders' hardnesses. The W 5oCr5o powder's hardness increased until it was nearly the same as the initially pure W powder, whereas the hardness of the W5 OZr5 O powder actually decreased until it is was the same as that of the initially pure Zr powder. We examined the pile-up around nanoindentations in the WsoCr5 o and W5oZr5o powders milled for 15 hours, in order to better appreciate the nature of the deformation in these systems when they are structurally quite refined. The lower magnification SEM micrographs shown in Figures 2.8a and 2.8b indicate that both alloys deform by shear localization after long milling times. The higher magnification SEM micrograph of the pileup around the nanoindentation into WSOCrO shown in Figure 2.8c lacks phase contrast, suggesting a chemically homogeneous powder. In contrast, closer inspection of the edge of the indentation in the pile-up region in Figure 2.8d reveals clear phase contrast, with the W-rich regions appearing lightly colored, and the Zr-rich second phase dark. Additionally, the shear bands in this sample show highly serrated faulting that seems to skirt around the W regions; places where this deflection behavior is particularly evident are marked with arrows. Figure 2.8 - Micrographs of nanoindentations using a cube corner tip into a,b) W5oCr5o and c,d) W5 oZr5 o powder particles that were milled for 15 hours. Both powders' pile-up patterns exhibit non-homogeneous plastic deformation (i.e., shear localization). In the W5 oZr5o powder's pile-up, the shear offsets appear to be skirting around the larger W particles in the regions indicated by the arrows. Courtney et al. [114] observed that Fe contamination during mechanical alloying provides an indirect measure of a powder's hardness: harder particles are more abrasive resulting in more Fe contamination. This observation is consistent with the present work in which we measured substantially more Fe contamination in the harder W and W 50 Cr5 O powders than in the comparatively soft W5 oZr5 O powder (Figure 2.1). W5 0TM50 Inspection of Figure 2.1 suggests that the couples' hardnesses divide roughly into two groups: the couples that homogenize (i.e., W 5 0Nb50 and WsoCr5 o) are similarly hard, whereas the couples that remain dual phase (i.e., W5 oNi50 , W 5 oZr5 o, and W5 oHf5 o) are similarly soft. 2.3. Factors Affecting Deformation-Induced Mixing Considering all of the characterizations in the previous section together, we conclude that in these W 5 oTM5 0 couples, differences in the strength of the two alloying elements, and the subsequent two phases that they evolve into, clearly affect the mode and amount of codeformation and atomic mixing. In the W-Cr couple, for example, nanocrystalline W and Cr phases would differ in strength by about 30% (cf. Figure 2.7b). This difference is small enough that when W and Cr are mechanically alloyed, plastic strain is partitioned between the W and Cr domains even at longer milling times, as evidenced by the lamnellar microstructure in Figures 2.5a-c. This in turn promotes deformation-induced mixing and the eventual formation of a homogeneous BCC solid solution, with W and Cr phases shearing into each other. Similarly, milled phases of W and Nb have a strength mismatch of about 40% (cf. Figure 2.7a), which we infer is not enough to prevent co-deformation and subsequent atomic mixing to a solid solution. In contrast is the W-Zr couple, for which the milled phases differ in strength by 70%. This large strength mismatch contributes to plastic strain localization in the softer Zr phase. This in turn leads to minimal mixing that is also more acutely asymmetric (practically no Zr dissolves in W, while some W dissolves in Zr). Similar conclusions are reached for W-Ni. That a difference in strength can play an important role in the amount of deformation-induced mixing is intuitive and has been noted by many others [25,89,90,115,116], but the W-transition metal couples studied here demonstrate this effect vividly. Although in this study the only alloying elements that completely mix with BCC W have BCC crystal structures themselves, in general, both elements do not need to have the same crystal structure for there to be complete homogenization during mechanical alloying. Of the many examples supporting this statement, two specific ones are Cu5 oFe5 o, a positive heat of mixing FCC-BCC couple that forms an FCC solid solution when mechanically alloyed [117-119], and Ni 5 oNb50 , a negative heat of mixing FCC-BCC couple that forms a homogeneous amorphous alloy when mechanically alloyed [120]. There are also examples of couples where both elements have the same crystal structure but do not homogenize even when milled at low homologous temperatures (e.g., Ni-Ag) [121]. These results suggest that nuanced effects like local interface structure might be less relevant given the random and repeated nature of deformation in mechanical alloying. For example, Vo et al. used molecular dynamics simulations of the Nb-Cu couple to demonstrate that certain interphase interfaces with special crystallographic orientations have enhanced resistance to deformation-induced mixing [78,79,122], but averaging over time during milling, many weak interfaces might be expected to be sampled as well. We speculate that crystal structure mismatch may correlate with the mixing behavior for a different reason, namely, because the Hall-Petch coefficient of FCC or HCP metals tends to be smaller than that of BCC metals [123]. Consequently, an initial difference in the coarse-grained metals' strengths in a BCC-HCP/FCC couple typically increases to a greater extent than the same initial difference in a BCC-BCC couple as the two alloying elements' grain sizes are refined. At least for the present W-TM couples studied here, crystal structure correlates with mixing behavior primarily because it affects the difference in phase strength at later milling times. A parameter that apparently did not influence the amount of deformation-induced mixing in these W-transition metal couples was the heat of mixing: W-Zr/Hf/Ni are all systems with mildly negative heats of mixing (AH = -8 kJ/mol; AH = -6 kJ/mol; AH' = -2 kJ/mol [124]), but their as-milled powders remain dual phase because interdiffusion is kinetically suppressed and their differences in strengths preclude much deformation-induced mixing. In contrast, W-Cr has a modest positive heat of mixing (AHi = +8 kJ/mol [125]) and thus prefers to segregate but forms a homogeneous solid solution instead. 2.4. Generalized Phase Strength Effects Our experimental results demonstrate that a difference in strength strongly influences the amount of chemical mixing attained during mechanical alloying, but they are limited in that only one combination of composition and ambient milling temperature was studied for each couple, and the gradual pickup of Fe during milling works against the study of steady-state structural conditions in these experiments. Furthermore, as noted in the Introduction, although there are theoretical constructs from driven alloy theory to rationalize mechanical mixing in systems that intrinsically mix to the atomic level, these do not generally include the role of mechanical strength on mixing. For these reasons, we adapt a kinetic Monte Carlo simulation of forced atomic mixing during mechanical milling. This Bellon-Averback type model captures the competition between deformation-induced mixing and thermally activated diffusion during mechanical alloying [69,70,91]. Following Refs. [69,70,91], we simulate a system containing a single vacancy and two types of atoms (given labels A and B for the stronger and weaker phases, respectively). The atoms have an FCC crystal structure, and the simulation unit cell is a rhombohedron with the faces parallel to FCC { 11 planes, 30 atoms along each of its edges, and periodic boundary conditions. To be consistent with previous simulations [70], the atoms' interaction energy, that CAA + EBB - 2&B = I-= -0.05533 eV, where EA CAB, was selected such and BB are the atoms' respective cohesive energies and were assumed to be equal. This interaction energy results in the system having a symmetric miscibility gap with a critical temperature at 1573 K. At each Monte Carlo step, either the vacancy exchanges positions with one of its nearest neighbors or the simulation cell is sheared, according to a residence time algorithm. The vacancy exchange frequency was configuration- and temperature-dependent, whereas the shearing frequency, 0, was held constant at 103 s- . The vacancy exchange frequency was calculated using w = vexp{-(E +Ea)IkBT} (2.4) where kB is the Boltzmann constant, T is the temperature in Kelvin, v is an attempt frequency (1015 s-'), EO is a configuration-independent energy set equal to 0.8 eV, andEN =En/2is an energy that reflects the local environment of each of the vacancy's nearest neighbor atoms, which we label exchange atoms [126]. The variable n is the number of each exchange atoms' nearest neighbors that are of the opposite species. After a number of Monte Carlo steps, the deformation-induced mixing and vacancy-mediated segregation processes typically reach a dynamic equilibrium. The resulting simulation cell's microstructure has a characteristic amount of chemical mixing, which we measured using the first Warren-Cowley short-range order parameter, a [127], normalized such that the limiting values of 0 and I correspond to a homogeneous solid solution and a completely segregated, dual phase alloy, respectively. Values of a intermediate to 0 and I reflect an increased number of dissimilar nearest neighbors, and can be attributed to either roughening of the interphase interface or dissolution of one element into the other [55]. We can estimate the temperature at which simulations with no difference in strength should be completely homogenized, TH, by setting the shearing and maximum diffusion frequencies equal and solving for T to give: T (E0 +3e) in kB 12v (2.5) where the factor of 12 comes from the coordination number. For our simulations, TH is 244 K. During a shearing event, two glide planes in the same slip system were selected, and the material between the planes was displaced by a Burgers vector in a random slip direction. The slip system and two glide planes were selected as follows: first, the slip system (i.e., family of glide planes and direction) was selected from one of the 12 possibilities using a uniform probability distribution, such as might be expected for randomly applied shears that would occur in ball milling. Next, two glide planes in this slip system were selected using a probability distribution function that accounts for each of the planes' strengths. The probability of selecting a given glide plane P(/) was calculated using Pj)=N (2.6) i-4 where the summation in the denominator is over all of the glide planes in a given slip system and Rj is defined as: R v=exp{-[N +N B(1-A)+Naj(1-A/2)]/kBT1 (2.7) where Ni, NB, and NB are the respective number of A-A, B-B, and A-B bonds across the slip plane j; A is the fractional difference between the pure A and B phases' strength; and X is a constant (2.4 x 1022 J) that gives the work required to move a dislocation across the plane j when multiplied by the other terms in the exponent's numerator. After the first glide plane was selected, the probability distribution was recalculated, omitting the plane that was already selected. According to Eqns. 2.6 and 2.7, setting A closer to unity makes selecting planes containing a larger number of B-B bonds more likely, so by adjusting A, we influence the strain partitioning (i.e., the A and B phases' difference in strength). For comparison with experimental results, we can interpret A as the fractional difference between the A and B atoms' shear moduli when information on the alloying elements' strengths is unavailable, because for nanocrystalline metals, the maximum strength is roughly proportional to shear modulus [113]. Moreover, by using an exponential in Eqn. 2.7, the probability distribution function is sufficiently steep that in a couple with A - 1, a small cluster of A atoms is unlikely to be sheared. In addition to varying the temperature and A, we also controlled the concentration, c, of A. Note that increasing the temperature tends to distribute the shearing events among the planes more uniformly by making the shearing of harder planes more probable. This effect is most significant among planes with similar strengths. 2.4. 1. Bi-stability and History-DependentSteady States When there is no difference in strength (i.e., A = 0), the present model devolves to become identical with that of Bellon and Averback [70], and the results match theirs in detail. Specifically, the steady state chemical mixity is path-independent and determined solely by the shearing rate and the vacancy exchange rate, which is in turn a function of the temperature. This is demonstrated in Figure 2.9a where, for a given temperature, a converges to the same value regardless of the starting configuration for an A 50B 50 alloy. This path-independence in couples with little to no difference in strength aligns with experimental results such as those of Klassen et al. [41] (for Cu-Ag), and is consistent with Martin's "rule of corresponding configurations" for driven alloys, which states that an alloy should attain a unique steady state chemical mixity for a given intensity of the driving force and ambient temperature [36]. In contrast, our simulations suggest that when there is a large difference in strength (i.e., A = 1), the steady state chemical mixity becomes path dependent, at least if the temperature is sufficiently low. Figure 2.9b, for example, depicts the evolution in chemical mixing for two different starting configurations, completely segregated and chemically mixed, at two different temperatures in a couple with a large difference in strength. In the high temperature simulation, the a's converge as before, but interestingly, in the low temperature simulation, the initially segregated and chemically mixed configurations remain as such. The insets in Figure 2.9b are two-dimensional slices across the initially segregated and chemically mixed simulation cells that illustrate their disparate initial and steady state amounts of chemical mixing. a. 1.0 0.8 350 K A - 0.6 a 0.4 300 K 0.2 0.0 b. 1.0 a 300 K 0.4 0.2 0.C 0 1 2 3 MCS (107) Figure 2.9 - a) Evolution in the order parameter a for kinetic Monte Carlo simulations using two different temperatures in a couple with no difference in strength. The two lines that converge for each temperature correspond to two different starting configurations. b) The same set of simulations but using a couple having a large difference in strength between the phases. Note that in the low temperature simulations, the initially segregated and chemically mixed curves do not converge. The insets are two-dimensional slices across the low temperature simulation cells with the A atoms colored grey and the B atoms invisible. In Figure 2.9b, both the low temperature segregated and chemically mixed states appear to be stable steady states. The segregated state is stable because shearing occurs preferentially in the softer phase and will not lead to mixing so long as there are two glide planes containing only B atoms parallel to each plane in the { IlI} set. One set of these planes was missing from the starting configuration, but it formed during the first 107 Monte Carlo steps as evidenced by the dip in a. The disordered state is also stable because all planes in the simulation cell are equally likely to be sheared so shearing does lead to mixing, and the vacancy exchanges are sufficiently infrequent relative to shearing events that the A atoms cannot segregate into larger, unshearable precipitates. At higher temperatures, however, the vacancy exchange frequency increases so the A atoms can segregate into particles that subsequently coarsen. This is why both the initially segregated and chemically mixed simulations arrive at the same steady state a value in the 350 K simulation. Though the simulations are of positive heat of mixing couples, the negative heat of mixing (W-Zr/Hf/Ni) couples that we studied experimentally also appear to be bi-stable. In the case of W 5oZr5 o, for example, the steady state microstructure is dual phase when elemental W and Zr powders are mechanically alloyed. If, however, the W and Zr were first reacted to form an intermetallic and then this intermetallic was mechanically milled, the steady state microstructure would in all likelihood be single phase. There are many examples of multi-stability and path-dependent steady states in the literature on driven systems [31,39,42]. In irradiated alloys, for example, Banerjee et al. irradiated Ni 4Mo with high-energy electrons at various temperatures and found that the alloy either developed short-range order (SRO) or long-range order (LRO) depending on its state prior to irradiation [44]. Bellon and Martin subsequently explained this phenomenon by modeling the competition between irradiation-induced disordering and thermally activated reordering [29]. The authors concluded that bi-stability emerges because the SRO and LRO structures have different sensitivities to radiation damage: the SRO structure is less sensitive to irradiation-induced disordering than the LRO structure but the alloy's thermodynamic ground state has LRO. Both this example and our simulations demonstrate that bi-stability emerges when the driving force affects one phase disproportionately. That Martin's rule of corresponding configurations breaks down for these systems is reasonable; its assumption that the driving force affects both phases equally is not met. 2.4.2. Microstructureand Mixing Kinetics In the initially segregated simulations, the microstructure that emerged after holding a simulation for many MCS at a constant temperature was also affected by a difference in strength. In simulations where there is no difference in strength, Bellon and Averback [70] and others [69,9 1] observed interfacial roughening and compositional patterning as the temperature was decreased and vacancy exchanges suppressed. A 5 0B 50 We observed similar behavior in our simulations of an alloy equilibrated at various temperatures. As shown in Figures 2.10a-c, the characteristic length scales of the A and B regions decreased in step with the temperature. An analogous dependence of microstructural length scales on the ambient milling temperature has been confirmed experimentally in the Cu 5 oAg5o system using atom probe [74,128] and TEM/STEM [73,129]. When we introduced a difference in strength, the microstructures no longer featured interfacial roughening. Instead, the A regions organized into smaller aggregates with flat faces along the {1 11 } planes. Atoms that jutted out from these faces tended to be sheared off the surface into the B matrix, and once inside the B matrix, were shuttled about, sometimes rejoining the A cluster in a more stable position. Figures 2.10d-f demonstrate the development of these flat faces as the simulation cell temperature was dropped from 400 to 300 K. This lack of roughening, "chipping away" of A atoms at the interphase interface, and resultant asymmetric mixing kinetics are all broadly consistent with molecular dynamics simulations of deformation-induced mixing of hard, BCC precipitates in softer FCC matrices [77]. They are also consistent with the microstructure and mode of mixing exhibited by our W50 Zr5 O couple; in that couple the steady state microstructure featured nanoscale, equiaxed W particles in a Zr matrix and the W atoms were sheared into the Zr matrix without an equal but opposite flux of Zr atoms into the W particles. A=0 a. A 1 = 400 K 350 K C. 300 K Figure 2.10 - Steady state unit cells of A 50 B50 simulations with a-c) no difference in strength and d-f) a large difference in strength. The simulations were performed using the temperatures indicated, and the color scheme is the same as in Figure 2.9. All of the simulations were initialized with a segregated microstructure. 2.4.3. Temperature and Composition Effects Knowing that the steady state chemical mixity is path dependent for some combinations of temperature, A, and c, it is of particular interest to know at what temperatures a system with given A and c will homogenize if the starting microstructure is initially segregated, as is generally the case in high energy milling. The temperature at which this occurs provides an upper bound, below which the most likely stable state is the completely homogenized one. To identify this temperature, we performed simulations in which an initially phase-separated cell containing a single particle of the minority phase was cooled from 430 to 220 K by decrementing the temperature by 0.05 K every 104 steps. We selected this temperature range because over it, a couple with no strength mismatch (i.e., A = 0) transitions from phase-separated to chemically homogeneous. parameter space. The composition and A were systematically varied to explore the entire c-A Temperature (K) 380 330 280 230 1.0 0.6 - 0.8 a 0.4> - 0.6 0.20 0.4- A=ON 0.2- c = 0.20 0.0 0 2 MCS (101) c 4 0.50 2 MCS (107) c 4 0.80 2 MCS (107) 4 Figure 2.11 - Evolution in order parameter a during simulations following a cooling trajectory while shearing, using the A's and c's indicated. Note that with increasing c, a large difference in strength is no longer sufficient for preventing mixing: when c equals 0.8, all of the simulations homogenize by 230 K. Results from several simulations are shown in Figure 2.11 and two features are immediately apparent. First, adding a strength mismatch depresses the onset temperature for deformationinduced mixing, and for small c's, large differences in strength prevent mixing altogether. From inspection of the microstructure, the A clusters in these latter simulations essentially behave like unshearable dispersoids. Second, the relationship between A and the onset of mixing becomes less significant as c increases. Above a threshold c, all of the simulations mix at roughly the same temperature regardless of A because the atoms become geometrically constrained to codeform and mix. This trend is consistent with the experiments of Gaffet and coworkers [82] who mechanically alloyed several compositions of W and Cu, a couple with an 80% difference in strength when both metals are nanocrystalline [130,131]. The authors found that although the powder remained dual phase after milling, more Cu dissolved in the W as the volume fraction of W in the starting charge increased. The link between c, A, and the amount of mixing is also consistent with the behavior of dual phase metallic materials with coarse microstructures, in which co-deformation becomes more likely as the volume fraction of the harder phase increases. Co-deformation and atomic mixing should also occur more easily at all c's as the phase strength mismatch decreases, as is the case in our simulations and in experiments. For example, nanocrystalline Fe and Cu have an ~8 GPa difference in hardness [132,133], less than half that of W-Cu, and when the two are mechanically alloyed, they torm a solid solution at all compositions other than FeCu(I\) (60 < x < 80) [134]. Based on these observations, we conclude that the only requirement for a stable dual phase rnicrostructure in these simulations is that there be two "easy glide" planes parallel to each axis. The most trivial approximation of this condition would be if the easy glide planes comprised only B atoms, for which we can calculate a maximum concentration of A atoms, cvax, as C 8 L 24 L 2 3 L=--+ 32 (2.8) L where L is the number of atoms along an edge of the simulation cell; Eqn. 2.8 gives 0.76 for our simulations, which agrees reasonably with the simulation output in Figure 2.11, where at higher concentrations near c ~ 0.7, mixing is geometrically forced no matter the strength mismatch. In an experimental context there may be no threshold concentration above which mixing is forced, because the geometric constraint on deformation-induced mixing is not as strict in reality as it is in our simulations: when non-planar slip is possible, plastic deformation can deflect around the harder phase as suggested by the pileup pattern in W50 Zr5 Oin Figure 2.8. Finally, in Figures 2.12a-d, we summarize and generalize our simulation results for four different values of A by first scaling the temperatures at which the atoms completely mixed by TH and then plotting them as a function of the concentration of the harder A atoms, which can be compared with the concentration (or volume fraction) of W in our experiments. The data points here, and more specifically the shaded regions below them, delineate the combinations of temperature and concentration for which the simulations formed solid solutions. First examining the case where no strength mismatch is employed, i.e., A = 0 in Figure 2.12a, we observe that homogeneously mixed states are produced at all concentrations, when the temperature is low enough to prevent diffusional phase separation. The boundary separating the dual phase and solid solution regions is symmetric about a volume fraction of 0.5, and resembles the re-entrant miscibility gap that Martin [36] and Enrique and Bellon [135] predicted for irradiated alloys with a miscibility gap. This behavior is expected, because without a significant difference in strength, shearing, like irradiation, affects both phases equally. However, the limiting case of zero phase strength mismatch is not one often occurring in experimental alloys, and none of the present experiments are comparable to this simulated condition. 1.5 - a. =0 1.5 bA = 0.3 dual phase TT1.0- TH 1.0 0 0 solid solution 0.2 0.4 0.6 0.2 0.8 0.6 0.4 1.5 - C. A=0.4 1.5 d. A=0.7 W50 Hf50 + 1.0 T1.0 TH W W5Nb 0.2 0.6 0.4 C 0 WZr TH 0.5 0.8 C C 0.8 0.5 0.2 0.4 0Ni 0.6 0.8 C Figure 2.12 - Dynamical phase diagrams for systems studied as a function of temperature and composition. The regions below the lines correspond to the temperatures at which the various simulations homogenized during the simulated anneals. With increasing phase strength mismatch A, a two-phase region opens up where certain couples remain segregated if they start as such. The open circles on the x-axis indicate compositions that remained dual phase over the range of temperatures studied. Experimental compositions are placed on these diagrams at their expected locations based on the strength differential in a fine nanocrystalline structure from Figure 2.7. Figure 2.12b illustrates the mixing behavior of couples with A = 0.3, which can be reasonably compared with the W-Cr system, which has a 30% strength mismatch in the fine nanocrystalline regime (cf. Figure 2.7b). Near the terminal compositions, the data in Figure 2.12b also show the development of a re-entrant miscibility gap, much as we saw in Figure 2.12a. However, the strength mismatch suppresses the ability of the system to mix for some intermediate compositions between about 40 and 50% A atoms; the open data points show systems that remained phase separated in a steady-state condition even at low temperatures. The emergence of a low temperature dual phase region bookended by solid solution regions is encouraging because most mechanically alloyed transition metal couples exhibit this type of mixing behavior [24]. It also supports Xu et al.'s hypothesis that the positions of such phase boundaries in a dynamical phase diagram are partly determined by the mechanical properties of the constituent phases [90]. What is more, it reasonably compares with our observations for the W-Cr system, which is the most closely comparable to these simulations among our experiments. As shown by the arrow at the bottom of Figure 2.12b, W5 OCr5 O lies within the region of the map where mixing is expected, as indeed it is seen to occur in the experiments (cf. Figure 2.3b). Figures 2.12c and 2.12d expand the discussion to larger phase strength mismatches of A = 0.4 and 0.7, respectively. These values are comparable to that of our W-Nb couple, and the three couples W-Zr, W-H f, and W-Ni, respectively. The tendency of strain partitioning increases with A, expanding the range of the dual phase region to a compositional width of about 20% at A 0.4, and to a width of ~50% at A = 0.7. The dual phase region also becomes more asymmetrical with A, skewing towards the A-lean side of the diagram. These simulations correctly align with the experimental observations that the W 5oZr5 O, W50 Hfso, and W50Ni5O couples should remain dual phase during mechanical alloying. According to these simulations, a couple with W 5ONb 5 O's strength mismatch and volume fraction of W should remain dual phase, which is nominally at odds with what we found experimentally. However, this apparent discrepancy is explained by the accumulation of Fe in the as-milled powder, which after 25 hrs of milling consists of 25 at% Fe (cf. Figure 2.1). The presence of Fe is expected to promote homogenization of the W and Nb because it decreases the volume fraction of W, thereby shifting the position of the W 5oNb50 couple in Figure 2.12c from c ~ 0.46 to ~ 0.38, bringing it closer to the A-lean solid solution region. Dissolution of Fe into both the Nb and W should also promote homogenization by decreasing A due to solid solution strengthening and softening effects in the W and Nb, respectively. For example, in the powder milled for 25 hrs containing 25 at% Fe, if the Fe completely dissolved in equal proportions in nanocrystalline W and Nb, then A would decrease from 0.4 to -0.3 [113]. When both the change in the W concentration and the expected decrease in A are accounted for, then the W50Nb 5 O couple lies in the solid solution region of the dynamical phase diagram in Figure 2.12b, which brings alignment between the experiments and the model. 2.5. Concluding Remarks The objective of this research was to clarify the effects of a phase strength mismatch between the input materials on the steady state chemical mixity during extensive plastic straining of alloys; some alloy pairs mix during straining and others do not, and the steady-state after large strains was explored here in several W-transition metal couples treated by high energy ball milling. Two contrasting sets of behavior were observed: the W-Cr/Nb couples formed homogeneous solid solutions after 15 hours of milling, whereas the W-Zr/Hf/Ni couples remained dual phase even after 25 hours of milling. In the latter couples, the mixing kinetics appeared to be asymmetric in that more W dissolved in the alloying element than alloying element dissolved in W. A more in-depth investigation of the evolution in the W5 oCr5 o and W 5 oZr5o couples' hardness and microstructure demonstrated that the root cause of the two groups' disparate mixing behaviors was the magnitude of the strength mismatch between the phases. In the W 5 oCr5 O couple a comparatively small fractional difference in phase strength encouraged co-deformation and consequent mixing. That the W and Cr were co-deforming was indirectly evidenced by the lamellar phase morphology in the as-milled, WsoCr 5 O powders. In contrast, nanocrystalline W and Zr's large difference in strength led to strain localization in the softer Zr phase and a consequent lack of deformation-induced mixing. To further explore the effects of a strength mismatch in the context of a driven alloy framework, we adapted a kinetic Monte Carlo simulation of mechanical alloying to account for differences in phase strength in a model system. The simulations were able to reproduce several salient features of our experimental results, such as the asymmetric mixing kinetics of the W-Zr/Hf/Ni couples and the particulate morphology of the W regions in the W 50 Zr50 powder. The simulations also enabled a more general, parametric study of the effects of composition and processing parameters on the development of a solid solution. The dynamical phase diagrams of mechanically alloyed pairs tend to show re-entrant miscibility at low temperatures, where diffusion is suppressed and mechanical strain tends to promote mixing. Phase strength mismatch, however, works against mechanical mixing, and decreases the degree of re-entrant miscibility; the trends seen in the dynamical phase diagrams also align with the experimental results for the various W-TM couples. These dynamical phase diagrams and the emergence of multi-stability and path-dependent steady states in simulations of couples with a large strength mismatch highlight the need to appropriately modify the classical driven alloy framework when describing systems in which the potency of the mixing process is environment dependent. 3. Guidelines for the Microstructure Design of Mechanically Alloyed Materials In the preceding chapter, we demonstrated that A, or the fractional difference in the alloying elements' strengths when they are nanocrystalline, is related to the degree of strain localization during mechanical alloying. We also showed that the degree of strain localization in turn determines the as-milled powder's steady state chemical mixity. In this chapter, we further explore the relationships between A, plastic strain localization, and the steady-state chemical mixity of mechanically alloyed powders through a survey of the grain size strengthening and mechanical alloying literature. This survey was motivated by the abundance of relevant data in the open literature: there have been mechanical alloying studies on nearly 100 different metalmetal couples, and the strengths needed to calculate A for most of these couples can be estimated using results from Hall-Petch studies. To begin, we summarize the results from mechanical alloying studies on positive heat of mixing couples in Table 3.1. Included in Table 3.1 are descriptions of the microstructures that the different couples developed after long milling times, and based on these mixing behaviors, we divided the couples into two groups. The couples labeled mechanically immiscible are ones that remain dual-phase across a wide range of compositions even after long milling times. By contrast, the couples labeled mechanically miscible are either ones shown to mix completely at all of the compositions studied, or couples that contain alloying elements with dissimilar crystal structures and that are therefore dual-phase over a small range of compositions as they transition between the crystal structures of the two terminal solid solutions. Table 3.1 - Mechanical alloying behaviors reported for positive heat of mixing metal-metal couples. Compositions Couples Coup Studied (at% (A-B) B) mechanically immiscible Mixing Behavior Refs. SAED patterns collected from as-milled powders suggest dual-phase microstructures at all compositions studied [136] ______________________________ Ag-Co 40, 80, 94 Ag-Fe 50 Ag-Ni XRD measurements of the Ni lattice parameter indicate that only the Ag-95Ni alloy homogenizes SEM micrographs show W particles in a Ag matrix XRD indicates that the Al phase can dissolve up to 20 at% Zn [121,136,141] Ag-W Al-Zn 30, 50, 70, 90, 95 60 1, 4, 78 Cd-Zn 16,30,42 XRD measurements revealed that the as-milled powder is still dual- [145] Cr-Cu 30, 50, 70 Cu-Mo 1, 7, 70 Cu-Nb Cu-Ta Mossbauer spectroscopy indicate Fe nanograins sit dispersed in an [137-140] Ag matrix '__'_phase, [142] [143,144] but that there is enhanced solid solubility XRD of powders milled in argon reveal that the alloy is still dual- [146,147] XRD reveals Bragg peaks due to both Mo and Cu [148,149] 1, 5, 10, 20, 50 XRD reveals that the alloy is still dual phase but that the FCC Cu phase can [150-153] 10, 30, 50, 70, 90 XRD reveals that the alloy remains dual phase after milling for long times. Some studies claimed the alloy amorphizes during milling but phase at all compositions tested dissolve up to 10 at% Nb [83,154,155] this is likely due to contamination by the milling atmosphere Cu-V 30, 50, 70 Cu-W 2, 4, 6, 10, 13, 18, 25, 30, 50, 60, 75 XRD patterns reveal 2 sets of Bragg peaks corresponding to nanocrystalline W and nanocrystalline Cu Fe-Mg 5, 10, 15, 20, 80 XRD and Mossbauer spectroscopy show that the Mg can dissolve up to 5 at% Fe and that up to 15 at% Mg can dissolve in the Fe but that 8 [156] [82,157-160] [161-163] I the alloy is otherwise dual-phase 15, 20, 65, 85, XRD measurements of the lattice parameter show that up to 3 at% 90, 95 I Mg-I ,i I I Mg can dissolve in the Ti but that the alloy remains dual-phase at , _______Mg-Ti EXAFS and XRD reveal that this alloy is dual-phase when milled in Ar I [164-169] I I I Ag-Cu 20 30, 40, 50, 60, 70, 80 Ag-Pd 5, 10, 15, 30, 50, 60, 70, 80, 85 10, 25, 60, 75, 90, 100 Co-Cu most compositions XRD, FIM, and DSC measurements indicate that the alloy forms a single-phase FCC solid solution at all compositions. Alloy must be milled at liauid nitrogen temperatures to suppress phase separation. XRD indicates that the alloy forms a single phase solid solutionn at all compositions XRD, TEM, and atom probe all indicate that Cu-Co form a metastable FCC solid solution at all compositions, though some magnetic measurements indicate that the alloy is dual-phase at the [75,91,106,170, 171] [172,173] [80,106,174180] nanoscale. mechanically miscible Co-Ni 30, 40, 50, 60, XRD results indicate that this alloy forms single phase solid solution [181-184] Cr-Mo 25, 50, 75 Lattice parameter measurements with XRD indicate that the alloy is [185] Cr-Ni 60, 80 XRD patterns suggest the formation of a single-phase solid solution [186] Cr-W 50 70 chemically homogeneous XRD and electron microscopy indicate that the alloy mixed atomically Chapter 2 Cu-Fe 30, 40, 50, 70, 90 XRD, Mossbauer, and EXAFS show that the alloy forms a single phase FCC solid sol'n with up to 60 at% Fe dissolved in the Cu, is dual-phase between between 60 and 80 at% Fe, and forms a single phase BCC solid solution with up to 20 at% Cu in Fe [25,118,134,13 8,187,188] CuNi 10, 30, 50, 60, Lattice parameter measurements with XRD indicate that the alloy is [189191] Fe-V 40, 50, 60 XRD and Mossbauer spectroscopy have shown that the alloy [192-195] Mo-W 13, 25, 50, 75, 87 XRD suggests that all compositions homogenize during mechanical alloying XRD measurements indicate that the alloy mixes to a chemically [196,197] 70, 80, 90 Nb-Zr I at all compositions I 40, 45, 50 chemically homogeneous homogenizes during mechanical alloying I homogeneous state [189__91] [198] A first approach to explaining the disparate mixing behaviors in Table 3.1 can be made with the classic Bellon-Averback framework, which ignores strain localization effects. According to this framework, thermally activated phase separation and shear-induced chemical mixing compete to Which of these two processes determine the alloy's steady state chemical mixity [199]. dominates is indicated by the dimensionless quantity e/(Deff/b2 ), where b is the Burgers vector, Detf is an effective diffusivity that accounts for grain-boundary, short-circuit diffusion, Since grain boundary diffusion and t is the average macroscopic plastic strain rate [69]. dominates lattice diffusion over the range of grain sizes and temperatures typically encountered during mechanical alloying, DeI can be estimated as follows Deff f=Dgb (3.1) where Dgh is the grain boundary diffusivity, L the grain size, and t the grain boundary thickness, which we approximate as being twice the average of the two alloying elements' Burgers vectors. The activation energy and pre-factor that are required to calculate Dgb can be estimated from lattice diffusivity data: the grain boundary diffusivity's activation energy is typically half that of the lattice diffusivity, while the pre-factors of the lattice and grain boundary diffusivities are roughly the same [200,201]. According to the classic Bellon-Averback framework, when an alloy is processed such that t/(Deff/b 2 ) >> 1, the rate of shear-induced chemical mixing is expected to be greater than that of thermally activated phase separation, and as a result, the alloy should chemically homogenize even if it would energetically prefer to de-mix [70]. mechanically immiscible 100 I I I iCO Cu-Ag Ag-Pd Ni-Cu I 1010 ICo-Cu 1 IW-Cr 2 a, i/D~ Ui(D,/b2 | W-Fe ) 4&I Cr-Cu Cu-Nb Ni-Ag Fe-Ag Cd-Zn Zn-Al I 1M5 1 T = 100 *C i = 104 s- Cu-W Mo-Cr mechanically miscible Figure 3.1 - ei/(D/b 2 ) of binary alloys processed by high-energy ball milling. All of the couples are expected to form single phase solid solutions. While experiments show that the couples colored red do in fact form solid solutions, the couples colored blue form simple mechanical mixtures. 62 Figure 3.1 shows values of 9/(Deff/b 2 ) for the transition metal couples in Table 3.1 when they are mechanically alloyed in a SPEX high energy ball mill. The couples in Figure 3.1 were selected because their interdiffusivity data are available in the open literature. In this figure, 9 is taken as 104 s4 and the ambient temperature used to calculate Dej is 100 'C, in line with estimates of the t and temperature rise encountered during ball milling [18,92]. In Figure 3.1, - those couples with t/(Deff/b 2 ) >> 1 are all - including the mechanically immiscible ones expected to homogenize according to the Bellon-Averback framework [24]. Since Figure 3.1 shows that this expectation is not realized in experiments, we conclude that /(Deff/b 2 ) > 1 is a necessary condition for two elements to mechanically alloy, but it is not sufficient. 1.5 A 0.5 1.0 Cu 0 Ag 0.5 0 0.1 0.2 1 2 D- 0.3 0.4 (nM 1 2 ) 0 Figure 3.2 - Aggregated Hall-Petch data for pure Cu and Ag. The solid dots indicate the maximum strength of pure, as-milled Cu and Ag. In light of this clear discrepancy between the classic Bellon-Averback metric and the experimental results, we next correlate the mixing behaviors in Table 3.1 with the couples' respective A values. To calculate A for each of these couples, we first reviewed the mechanical alloying literature to identify the steady state grain size of the pure metals when they are mechanically alloyed at room temperature. Subsequently, we estimated the strength of the 63 metals at this grain size with data from Hall-Petch studies. Figure 3.2, for example, shows the aggregated Hall-Petch data for pure copper and silver, and the solid dots indicate the expected strength of the pure, as-milled powders. These strengths were the values used to calculate this couple's A. For metals that do not have Hall-Petch data at the finest grain sizes, we estimated the as-milled powder's strength by extrapolating the available grain size strengthening data. Table 3.2 lists the strengths used to calculate A in the following discussion, and Appendix I includes the aggregated Hall-Petch data for each of the metals in this Table. Table 3.2 - Steady state grain sizes of pure metals during high energy ball milling at room temperature and estimated strength of the pure, as-milled powders from their grain size strengthening data. Grain sizes were either taken from 121,22,2021 or estimated using the trends reported in those References. Element Ag Al Au Be Cd Co Cr Cu Fe Mg Mo Nb Ni Pd Ta Ti V W Zn Zr Grain Size (nm) 25 25 17 11 30 14 9 21 10 39 9 9 14 8 7 14 8 7 25 13 Strength (GPa) 0.4 0.6 0.7 5.3 0.08 1.7 5.3 0.8 2.9 0.3 6.2 4 2.3 1 5 1.8 3.8 7.3 0.2 1.8 Figure 3.3 shows values of A for couples with t/(Deff/b2 ) >> I when they are mechanically alloyed. Here, the mechanically miscible and immiscible couples separate into two regions that overlap only slightly: couples with A less than 0.6 are all mechanically miscible, those with A greater than 0.75 are mechanically immiscible, while in the range 0.6 < A < 0.75, there are both 64 mechanically miscible and immiscible couples. This Figure demonstrates that A and /(Deff/ b 2 ) can be used together to identify a couple's mixing behavior. mechanically immiscible Mb-Cu Fe-Ag ,u 0511 ) 0. T1V-Fe V-Ag Ni-Co W-Mo Mo-Cr Cu-Cr i I M o-Cu W-Ag Ni-g 1.0 Zr-Nb Cu-Co Pd-Ag Cu-Ag Ni-Cr Ni-Cu mechanically miscible Figure 3.3 - A values for various metal-metal couples whose mixing behaviors have been studied in detail. In order to facilitate the microstructure design of mechanically alloyed materials, we calculated A for all of the binary combinations of the metals listed in Table 3.2 and aggregated these A values in Figure 3.4. Each square in Figure 3.4 corresponds to a specific couple and the square's color indicates whether that couple is mechanically miscible (A < 0.6), immiscible (A > 0.75), or indeterminate (0.6 < A < 0.75). With this table, it is possible to predict the mixing behaviors of couples that have yet to be studied. 65 > ZI--mom ON M<«<Q..O-NZW W Mo Cr Be Ta Nb V Fe Ni Zr Ti Co Pd Cu Au Ag Mg Zn Cd UA < 0.6 (mech. __0.75< miscible) 0.6 < A < 0.75 A (mech. immiscible) Figure 3.4 - A values for all metals whose grain size strengthening behavior has been studied. The red and blue squares indicate couples expected to be either mechanically miscible or immiscible, respectively. The grey squares indicate couples that could exhibit either behavior. Returning our attention to Figure 3.3, we can use results from continuum plasticity to explain why the transition between the mechanically miscible and immiscible couples occurs at A's between 0.6 and 0.75. Support for using continuum plasticity to describe the micromechanics of plastic deformation in a mechanically alloyed material is provided by the nanoindentation experiments described in the previous chapter. These tests showed that the hardness of the asmilled W5 oZr5o powder was nearly identical to that of the as-milled Zr powder after long milling times, despite the fact that the alloy powder contained nearly 50 vol% tungsten in the form of 10 nm diameter dispersoids. Such a complete lack of dispersion-strengthening, while initially surprising because it departs from the behavior of traditional, microcrystalline materials, is actually consistent with the theorems of limit analysis in continuum plasticity and their prediction of the limit load for a composite material featuring isolated rigid particles in an elastic-perfectly plastic matrix. These W-Zr powders - and possibly other powders of mechanically immiscible couples prepared by high energy ball milling - might behave like such idealized particulate composites for three main reasons. First, dislocations cannot accumulate in the nanoscale grains of the matrix so that the matrix exhibits minimal work-hardening and is 66 therefore nearly elastic-perfectly plastic. Second, much higher stresses are required to nucleate and propagate dislocations in the W nanoparticles than in the Zr matrix so that the particles are effectively rigid. Third, and most importantly, the length of the dislocations in the matrix and the distance that they travel is limited by the grain size of the matrix. This is why the matrix behaves like a plastic continuum even at the nanoscale. In materials with A smaller than that of W-Zr, the second justification listed above can break down and the particles may deform along with matrix. In this case, the nanocomposite can still be described using continuum plasticity, but instead of approximating the particles as rigid, they can be modeled as elastic-perfectly plastic. Such dual-phase particulate composites in which both the dispersoid and the matrix are elastic-perfectly plastic have been studied in detail by Bao et al. using finite element simulations, and their results can help explain the trends in Figure 3.3 [203]. These investigators showed that the plastic strain is uniform throughout the composite regardless of the volume fraction of the hard phase when A is less than 0.5, that the strain starts to localize in the softer phase when A is greater than 0.5, and that the particles stop deforming altogether when A is larger than 0.6. Comparing these results with Figure 3.3, we therefore speculate that the transition from mechanically miscible to immiscible behavior starting at a A of roughly 0.6 can be explained by modeling mechanically alloyed materials as dual-phase elastic-perfectly plastic particulate composites. The survey conducted in this chapter showed that predicting the mixing behavior of a given binary alloy requires knowledge of both A and /(Deff/b 2 ). In light of this, we aggregated the data needed to calculate A for most metal-metal couples into a heat map that can help guide alloying decisions during the microstructure design of mechanically alloyed materials. In addition, we explained certain features of this map with the help of continuum plasticity results. 67 4. Powder-Route Synthesis and Mechanical Testing of Ultrafine Grain Tungsten Alloys As mentioned in the Introduction, ultrafine grain tungsten's high density, compressive strength, and propensity for shear banding make it an attractive material for penetration applications, but the amount of available data supporting its unique mechanical properties remains limited due to processing constraints [204,205]. One major constraint has been the limited dimensions of W specimens whose grain sizes are refined by severe plastic deformation techniques such as wire drawing and high pressure torsion [99,206-209]. For example, Wei and coworkers used high pressure torsion to prepare a W specimen whose grain size was refined to about 170 nm, but this technique is limited to specimen geometries of -1 mm thickness and ~10 mm diameter [209,210], while much higher aspect ratio specimens are required for traditional ballistic testing [211]. Furthermore, severe plastic deformation techniques capable of yielding larger specimens (e.g., cold rolling and equal channel angular extrusion) have generally produced W specimens with coarser ultimate grain sizes (>500 nm) [208,212,213]. It is thus of interest to synthesize ultrafine grain W specimens using more readily scalable methods, for example based on powder processing. Previous efforts to synthesize ultrafine grain W articles using powder processing have generally found that pressure-assisted sintering and alloying are necessary for achieving high relative densities without grain growth [208,214-221]. Hot isostatic pressing, for example, was used to consolidate 50 nm W particles to >95% relative density between 1093 and 1193 K [222]. Because these temperatures are below the grain growth onset temperature of unalloyed tungsten (1273-1373 K), grain growth was suppressed, and the compacts retained grain sizes as small as 150 nm [223]. Attempts to replicate these results with other pressure-assisted sintering techniques such as field assisted sintering (FAS) used lower stresses: the hot isostatic pressing study used an isostatic pressure of I GPa, whereas the maximum uniaxial stress reported in FAS studies is 266 MPa [208,218-221]. Consequently, these FAS studies generally required higher soak temperatures (>1273 K) or longer hold times to achieve similar relative densities. Despite FAS's fast ramp rates, the higher thermal excursion led to coarse (>1 pm) grains and 68 commensurately degraded mechanical properties. Hence, pressure-assisted sintering and rapid ramp rates, although beneficial, cannot guarantee low porosity and ultrafine grains. In addition to merely increasing consolidation pressure and thermal excursion, it is also desirable to consider W alloys containing elements that accelerate densification at lower temperatures and/or retard grain growth, thereby decreasing the necessary soak temperature and allowing longer hold times at higher temperatures. This, in turn, can reduce the need for very high consolidation pressures. Accordingly, this is the approach that we took in this chapter, in which we describe a specific nanocrystalline, W-based alloy powder (W-7Cr-9Fe, at%) that can consolidate to high relative densities without excessive grain growth during FAS. Because of their relatively small fractional differences in strength, W, Cr, and Fe mix to a chemically homogeneous state when mechanically alloyed and then phase separate on heating. Two-phase, ultrafine grain compacts made from the powder exhibit high hardness and dynamic compressive strengths, as well as a tendency to shear localize. Examination of the structure and properties of these materials also provides directions for the improvement of future generations of ultrafine grain W-based materials. 4.1. Materials and Methods 4.1.1. Powder Processing and Consolidation Nanocrystalline powder with a W to Cr atomic ratio of 10:1 was prepared by milling the appropriate ratio of feedstock powders (99.95% W, -200+325 mesh; 99+% Cr, -325 mesh) in a SPEX 8000 high energy ball mill. For comparison purposes, initially unalloyed W was milled as well. The W and W-Cr powders were milled for up to 20 hours in a hardened steel vial with steel media and a ball-to-powder ratio of 5:2 (20 g of powder). In order to prevent oxidation, milling was conducted in a glovebox kept under an ultra-high purity argon atmosphere. The amount of Fe pickup in the powder due to abrasion of the vial and media was measured using energy dispersive spectroscopy (EDS) in a JEOL 661 OLV scanning electron microscope (SEM) operated at 20 kV. Prior to compaction, the as-milled powder's homogeneity and microstructure were assessed using X-ray diffraction (XRD) and transmission electron microscopy (TEM). The grain size and lattice parameter were calculated from XRD profiles collected using Cu-Ka radiation in a Panalytical X'Pert Pro diffractometer. The grain size was measured from the XRD pattern 69 using a Williamson-Hall analysis of the peak broadening after correcting for instrumental broadening using a NIST LaB6 standard. The Williamson-Hall method was used in the present work because it has been shown to measure the grain size more accurately than techniques that do not account for microstrain, i.e. the Scherrer equation, which tend to underestimate the grain size [224]. The lattice parameter of the BCC W phase was measured using Rietveld refinement. TEM was used to confirm the XRD grain size. TEM specimens were prepared by mixing the powder in epoxy, manually grinding a powder-epoxy disk until it was less than 10 tm thick, and then argon ion polishing the disk to electron transparency in a Fischione 1010 ion mill. During ion polishing, the specimen was cooled to 183 K using a liquid nitrogen cold finger. Bright field TEM micrographs were collected in a JEOL 2010F operating at 200 kV. Individual grains were manually traced and their spherical-equivalent diameters measured. The milled powders were subsequently consolidated in a Dr. Sinter SPS-515S hot pressing (FAS) apparatus, using various soak times and temperatures to identify the optimal processing parameters for minimizing both porosity and grain growth. Except for samples used subsequently for micropillar compression and Kolsky bar tests, all of the samples were consolidated using an 8 mm diameter graphite punch and die set. The Kolsky bar and micropillar compression specimens were machined from a larger compact consolidated with a 20 mm punch and die set. Both the 8 and 20 mm compacts were consolidated under a uniaxial stress of 100 MPa. During consolidation, the temperature was ramped from room temperature to 843 K (570 'C) in 3 minutes and then from 843 K to the soak temperature at 100 K/min. The soak temperature was systematically varied from 1373 to 1673 K in increments of 100 K, and soak times of I and 20 minutes were used at each temperature. During consolidation, the hot zone was held under a vacuum of at least 0.2 mbar. Following consolidation, the temperature in the water-cooled consolidation chamber initially decreased at a rate of ~200 K/min, eventually slowing to <40 K/min after dropping below 1073 K. The compacts were rough ground to remove any carbide from their surfaces and sectioned using electro discharge machining (EDM) for microstructural characterization and mechanical testing. 4.1.2. Microstructural Characterization The porosity, volume fraction of phases present, and mean grain size of the W-rich BCC phase were quantified in as-compacted samples using standard stereological techniques. A section of 70 each compact was mounted, ground, and polished prior to collecting SEM images for stereological measurements. Metallographic preparation concluded with a suspension of colloidal silica in dilute chromic acid (0.03 M) to enhance grain boundary relief. The micrographs used for grain size measurements were taken in secondary electron mode, whereas those used for volume fraction and porosity measurements were taken in backscatter electron mode. The volume fraction of intermetallic was manually measured using the point counting technique described in ASTM standard E562-11 [225]. The porosity was measured following the image analysis procedure outlined in ASTM E1245-03 [226]. The mean grain size was measured in accordance with the circular intercept procedure for specimens containing two phases as described in ASTM standard El 12-12 [227]. To validate the stereological porosity measurements, the compacts' relative densities were also estimated. Their specific gravities were measured using the Archimedes method in deionized water. Each sample's specific gravity was measured five times giving a relative uncertainty of 0.5%. The compacts' theoretical densities were calculated by summing the product of each phase's theoretical density and stereological volume fraction. 4.1.3. Mechanical Testing Microhardness was measured using a Leco DM-400FT Microhardness Tester with a 1 kg load and a 15 s hold time. Compact as well as individual phase mechanical properties were measured by instrumented nanoindentation using a MTS Nanoindenter XP with a diamond Berkovich tip. The tip's area function was calibrated on a fused silica standard. Indentations were performed at a nominal strain rate of 0.05 s- to a maximum depth of 1 ptm. The hardness and reduced modulus were calculated from the load-displacement data using the Oliver-Pharr method [228]. The Young's modulus was then calculated using standard values for the elastic properties of diamond and the Poisson's ratio of W (vw = 0.28) [229]. Select specimens were subjected to additional small scale mechanical testing. After polishing the sample's surface, micropillars with diameter and length of 5 and 10 pm, respectively, were fabricated using the lathe technique in a FEI Nova 600i dual-beam focused ion beam [230]. The micropillars were compressed in the same MTS Nanoindenter XP with a square, 30 x 30 tm flat punch diamond tip. The loading rates in the load-controlled nanoindenter were prescribed to provide nominal strain rates of ~104 s-1. Engineering stress and strain for each 71 test were calculated from the applied load and cross-head displacement data collected by the nanoindenter. In addition, the samples were observed post-mortem using an SEM. High strain rate uniaxial compression experiments were conducted on select samples using a 3/8 inch diameter maraging steel Kolsky bar system. Details of a comparable experimental setup can be found in Reference [29]. For these experiments, cuboidal samples were cut from the bulk materials using a wire EDM and polished to a cross sectional geometry of 2.2 x 2.2 mm and lengths from 1.8-2 mm. Impedance-matched tungsten carbide platens were used to protect the ends of the bars due to the test specimens' high strengths. In addition, Cu pulse shapers were used to produce ramped loading conditions in order to ensure stress equilibrium was achieved within the sample prior to failure. Several specimens were recorded during loading using an Imacon 200 high speed camera. The specimens were illuminated by a Photogenic Powerlight 2500DR flash, and the images were captured with a 2 pis exposure time at a framing rate of 2.2 pts. 4.2. Powder Characterization Abrasive wear of the steel vial and media during milling was the source of iron in the present alloys; milling changed the average stoichiometry of the W 9 oCrio and W powders to W 84.1 Cr7.1 Fe8 .8 and W 90.5Fe9 .5, as measured by EDS. The two alloys are referred to as W-7Cr9Fe and W-9Fe for simplicity. Previous studies on mechanical alloying of W reported similar Fe pickup and so this was expected [114]. Here, the addition of Fe modified the equilibrium phases present at the soak temperatures used. Inspection of the ternary W-Cr-Fe phase diagram shows that W and W-IOCr lie in a single-phase, BCC solid solution field at temperatures greater than 1373 K; W-7Cr-9Fe and W-9Fe alloys lie in a two-phase field linking the BCC solid solution with a pt-phase intermetallic [231]. The intermetallic p-phase precipitated during consolidation. XRD patterns of the feedstock W- I OCr powder and the W-7Cr-9Fe powder milled for 10 and 20 hours are shown in Figure 4. 1a. The elemental W and Cr powders diffract differentiable sets of BCC Bragg peaks. With increasing time milled, the Cr peaks disappear, while the W peaks broaden due to grain refinement and shift to higher 20 indicating a change in lattice parameter. The disappearance of the Cr peaks and the change in W's lattice parameter suggest that the W, Cr, and Fe form a metastable solid solution, in line with previous reports on mechanically 72 alloyed W-Cr and W-Fe couples and as expected based on the map (Figure 3.2) presented in Chapter 3 [232,233]. Similarly to the W-7Cr-9Fe powder, the W lattice parameter in the initially pure W powder changes as Fe dissolves into the W lattice. a. * tungsten v chromium feedstock powder Cd milled 10 hrs milled 20 hrs * I * I 100 80 60 40 . Position (020) b. 60 - W-7Cr-9Fe o W-9Fe E N ''C 40 20 ,3.16 3.15 a. .1 3.13 0 I- .1 I * 5 10 * 03.14 15 20 Time Milled (hrs) Figure 4.1 - a) Set of XRD scans taken from the feedstock and W-7Cr-9Fe powder milled for 10 and 20 hrs. Note the disappearance of the Cr (110) Bragg peak in the highlighted region after 10 hrs of milling. This, along with the change in W lattice parameter, suggests the formation of a solid solution. b) Williamson-Hall and Rietveld analysis give the W-rich BCC phase's grain size and lattice parameter as a function of milling time for both alloys. 73 Figure 4. 1b shows the change in the W-rich solid solution lattice parameter and grain size with time milled for the W-7Cr-9Fe and W-9Fe powders. The evolution in both powders' micro strain, as measured using the Williamson-Hall method, is in agreement with that previously reported by Wagner et al. for mechanically milled W, plateauing after 10 hrs of milling at -0.8 % [234]. Both samples' rate of grain size reduction slowed after 10 hrs of milling; however, their lattice parameters, indicators of the powder's chemical homogeneity, only started to change appreciably after 10 hrs of milling. 20 hrs of milling was chosen as a suitable compromise between achieving a terminal grain size, chemically homogenizing the powder, and avoiding excessive Fe pickup. The mean grain sizes of the 20 hr milled W-7Cr-9Fe and W-9Fe powders were 17 5 and 15 5 nm, as measured using TEM (Figure 4.2). These values were validated by the XRD measurements of grain size by the Williamson-Hall method (Figure 4.1b). The as-milled powders' grain sizes are in line with what has been reported in other studies of high energy ball milled W (-5 to 15 nm) [10 1,234-237]. b. Figure 4.2 - Representative TEM micrographs of the as-milled a) W-7Cr-9Fe and b) W9Fe powders illustrating the powders' nanocrystalline grain structure. The inset electron diffraction patterns feature the uniform rings characteristic of nanocrystalline materials. 74 4.3. Compaction and Compact Microstructure Punch displacements measured during some typical consolidation runs with both alloys are shown in Figure 4.3. The curves were collected while ramping from 843 to 1673 K at 100 K/s under a compaction pressure of 100 MPa. The onset of significant punch displacement at around 1173 K indicates that both alloys are beginning to densify, and the densification accelerates before slowing at ~1448 K where, presumably, full density is being approached. Although both alloys densify over the same temperature range, the Cr-free alloy appears to densify more rapidly at lower temperatures than the Cr-bearing alloy. W-9Fe W-7Cr-9Fe -- 0.6 - E E 0.40,2 / ~0.2 0.0S 1100 I 1200 * I 1300 * I 1400 * I 1500 Temperature (K) Figure 4.3 - Punch displacement curves measured during the heating ramp-up phase for the two alloys, under an applied stress of 100 MPa. The trends in the punch displacement data noted above agree with the stereological porosity versus soak temperature curves presented in Figure 4.4. As expected, the samples consolidated at soak temperatures of 1473 K or higher all had less than 2 vol% porosity and so were nearly full density. In addition, the W-9Fe alloy densified more rapidly at lower temperatures. Each compact's specific gravity, porosity measured using stereology, and porosity calculated from its relative density are shown in Table 1. For clarity, the two measures of porosity are presented in adjacent columns; the agreement is good. 75 - 8 1 min -W-7Cr-9Fes- 6 a_1 min W-9Fes- - 0 0 4 0) 0 u)2 20 min -W-7Cr-9Fem1- \W-9Feww ------ . 0 1300 1400 1500 1600 Temperature (K) Figure 4.4 - Stereological porosity after compaction experiments at a variety of soak temperatures and two soak times, I and 20 minutes. Although Figure 4.4 shows that the samples compacted at 1373 K for 20 minutes had porosities equivalent to those of samples consolidated at higher temperatures, we found that they were relatively friable and not well bonded at interparticle interfaces. In light of this, 1473 K at 1 minute was identified as the combination of time and temperature that minimized the thermal excursion while still achieving near full relative density and good interparticle bonding. 76 Table 4.1 - Compact properties after densification, including specific gravity, p (relative uncertainty: 0.5%), porosity measured using stereology (relative uncertainty: 50%), and porosity calculated from the relative density (relative uncertainty: 20%) for each compact. Alloy, Die Temp. Time p Porosity 100*(]-p/pi) Diameter (K ("C)) (min.) (g/cc) (%) (%) 1 17.7 4.5 3.5 20 18.1 0.5 1.1 1 18.1 0.6 1.1 20 18.1 0.3 1.4 1 18.1 1 1.3 20 18.1 0.8 1.4 1 18.1 1 1.4 20 18.1 1.3 1.5 1 16.1 7 8.5 20 17.3 0.9 1.5 1 17.3 0.5 1.8 20 17.3 0.8 1.5 1 17.3 1.1 1.5 20 17.4 0.8 1.2 1 17.5 0.9 0.9 20 17.6 1 0.6 1 17.0 1.7 3.3 1373 1473 W-9Fe, 8 mm 1573 1673 1373 1473 W-7Cr-9Fe, 8 mm 1573 1673 W-7Cr-9Fe, 20 mm 1473 Rapid, low temperature densification comparable to that reported above has been previously observed in two other studies of ball milled W and W alloys [215,238]. Oda and coworkers ball milled pure W powder and subsequently FAS consolidated the as-milled powder to near full density at 1273 K (1000 'C) and 50 MPa for 30 minutes [215]. Oda et al. did not assess the extent of Fe pickup after milling; however, in an independent W-Fe mechanical alloying study that used milling equipment similar to Oda et al.'s, Herr and Samwer observed that the Fe 77 pickup increased linearly with milling time and reached -70 at% after 80 hrs of milling whenever there was less than 70 at% Fe in the starting charge [239]. Thus, after accounting for the difference in ball to powder ratio used in the two studies, we estimate that there might be as much as perhaps -20 at% Fe in the powders made by Oda et al. after milling for 100 hrs. In addition, Xiang et al. mechanically alloyed a mixture of W, Ni, and Fe (W-7Ni-3Fe wt%) powders that they consolidated to 95% relative density using the same pressure, 50 MPa, but holding for only 8 minutes at a higher temperature, 1473 K [238]. The present results are in line with these other reports, although we achieve higher relative densities than Xiang et al. and use a significantly shorter soak time than Oda et al. The p-phase intermetallic precipitated during consolidation and was present in all of the compacts along with the majority BCC solid solution phase. EDS was performed on the samples consolidated at 1673 K for 20 minutes to determine both phases' compositions. In the W-7Cr-9Fe samples, the intermetallic and BCC phases had respective stoichiometries of W 4 6Cr1 6 Fe38 and W 92 Cr3Fe 5 , whereas in the W-9Fe compacts, the same phases had compositions of W5 oFe5o and Wq 8 Fe2 . In addition, we performed nanoindentation on the intermetallic in these samples to measure its hardness, which was determined to be about 17.4 GPa averaging over 8 indents. a. b. BCC solid sol'n p-phas 10 pm 10_pm Figure 4.5 - Backscatter electron micrographs of a) W-7Cr-9Fe and b) W-9Fe compacts 78 consolidated at 1673 K (1400 C) for 20 minutes. These samples had the coarsest microstructures of all the compacts. The p-phase precipitates in both samples are generally darker than the BCC solid solution due to the lower W content. The precipitates are also distributed randomly throughout the BCC solid solution, which itself is composed of many individual grains. The black dots in both micrographs are residual pores. There was a larger volume fraction of the p-phase in the Cr-bearing samples, but both alloys' compacts had qualitatively similar microstructures: regions of the W-rich, BCC solid solution phase containing many individual grains were interspersed with intermetallic precipitates as demonstrated by the micrographs in Figure 4.5. For soak temperatures greater than 1373 K, the volume fraction of the pt-phase that precipitated during compaction was, within error, equal to that predicted by the equilibrium phase diagram (as assessed by THERMOCALC software) given the alloys' stoichiometries (Figure 4.6) [240]. For the samples consolidated at 1373 K, the intermetallic volume fraction was greater than 10% but could not be more accurately measured because of difficulties resolving the two phases. The residual porosity, also evident in the micrographs in Figure 4.5, was located predominantly at triple junctions in the W-rich, BCC solid solution phase, the intermetallic-BCC phase boundaries, and the centers of larger regions of intermetallic. The samples consolidated at 1673 K for 20 minutes shown in Figure 5 had the coarsest microstructures of all of the compacts, and most of the other samples had similar microstructures, albeit on a finer length-scale. In the samples consolidated at 1373 K for 1 minute, individual powder particles were separated by pockets of porosity and could be clearly delineated. 79 W-7Cr-9Fe THERMOCALC 0.20- CL t - W-7Cr- 9Fe 1 min 0 2min 020 rmin 0-0 0 L-0.15E20Ominmm W-9Fe 1 mino-E E w W-9Fe THERMOCALC 0.10 1 1400 1500 1600 Temperature (K) Figure 4.6 - Volume fraction intermetallic predicted by THERMOCALC and measured using stereology for compacts consolidated at temperatures greater than 1373 K. All of the predicted and experimental volume fractions are within 3 vol% of each other, which is reasonable given uncertainties in the global stoichiometry of the powder and the stereology measurements. The compacts' grain sizes (D) are plotted against their soak temperatures in Figure 4.7. Even at the lowest soak temperature and shortest hold time (1373 K for 1 min), the grain size in both alloys was considerably larger than for the as-milled powder. The observed onset of grain growth at temperatures below 1373 K is in agreement with past reports of grain boundary migration in heavily worked W alloys [99,207]. In a study of warm-drawn, K-doped W wire, for example, Meieran and Thomas observed grain boundary migration at temperatures as low as 1 73 [99]. In our samples, the grain boundaries are sufficiently mobile by 1673 K that the grains rapidly coarsen to micron dimensions. It is also evident from the results in Figure 4.7 that Cr supports a finer grain structure in the W- 7Cr-9Fe samples relative to the W-9Fe samples. Cr appears to slow grain growth most at the lower soak temperatures. For example, the W-7Cr-9Fe samples consolidated at 1373 K for 1 and 20 minutes have 50% smaller mean linear intercept grain sizes than the similarly processed W-9Fe samples, whereas by 1673 K, the W-7Cr-9Fe and W-9Fe samples have effectively the same grain size. Additionally, one prior study of Cr-doped W reported that a W-30Cr alloy compact had a -5x smaller grain size than similarly processed pure W compacts after sintering 80 [232]. The Cr can inhibit grain growth in two ways. First, Cr is expected to segregate to grain boundaries in W and thereby lower the driving force for grain growth as well as the grain boundary mobility; this is specifically the case at 1373 K [11]. Second, if the p-phase exerts a pinning force on mobile grain boundaries in the W-rich, BCC phase, the larger volume fraction of p-phase in the Cr-bearing sample would result in more sluggish grain growth. 20 min *-W-9Fe 2.0 -'W-7Cr-9Fe E 1.5 1 min - EJ-QW-9Fe ioW-7Cr-9Fe (. 0.5 01 -As-milled n 0 Powder U I 1500 1600 Temperature (K) - 300 1 400 S 1700 * 0 1800 Figure 4.7 - Grain sizes of compacts made from both alloys and consolidated at various soak temperatures and two soak times, I and 20 minutes. Also shown for comparison is the grain size of the as-milled powder. From a practical perspective, it is of interest that the grain growth kinetics are sufficiently slow in the Cr-bearing sample that the powders can be consolidated at 1473 K for I minute to near full density and still retain ultrafine grains (D ~130 nm). These samples are therefore singled out for the micropillar compression and Kolsky bar experiments described later. We include additional low- and high-magnification SEM micrographs of this material in Figure 4.8 to illustrate the distribution of the intermetallic, the porosity, and the refined grain structure. 81 Figure 4.8 - a) Low- and b) high-magnification secondary electron micrographs of the optimized W-7Cr-9Fe compact consolidated using the 20 mm die at 1473 K for 1 min. The low-magnification micrograph illustrates the distribution of porosity (black regions) and the p-phase internetallic (darker grey contrast). The high-magnification micrograph illustrates this sample's ultrafine grain structure (D -130 nm). 4.4. Mechanical Properties 4.4.1. Strengthening Contributions Consistent with other reports of grain-size strengthening in W and W alloys, the compacts' microhardnesses conform to a Hall-Petch scaling, as shown in Figure 4.9. For comparison purposes, the data collected in this study are plotted alongside microhardness measurements on nominally pure W compacts fabricated by hot isostatic pressing W nanopowders from 82 Reference [20]. Numerical values for the Hall-Petch slopes are shown in the figure, and the extrapolation of the trend to infinite grain size is shown at the y-intercept. The slopes are similar among the three alloys, and the y-intercepts suggest that the W-7Cr-9Fe and W-9Fe compacts are respectively about 1.6 and 1.0 GPa harder than a nominally pure W compact, independently of grain size effects. 4.00 14 Grain Size (prm) 0.44 0.25 1.00 0.16 0 W-7Cr-9Fe ,12 M E W-9Fe W, [20]-- E )10-,'' 3.2 4.' 0.0 3.2 G P ap M1 . I 0.5 I 1.0 1.5 2.0 2.5 plot for compacts made with both alloys, from samples Figure 4.9 -Hall-Petch compacted at various times and temperatures to densities in excess of 98%. Microhardness values from Vashi et al. on nominally pure W compacted to 95% relative density are also presented for comparison [222]. According to Vashi et al., the hardness of their W specimens was independent of load between loads of 0.2 and 2 kgf, and the data shown is the average of the hardnesses measured using loads of 0.2, 0.3 and 2 kgf. The data point labeled with a star is the hardness of the W-7Cr-9Fe sample consolidated with the 20 mm die. One possible explanation for the higher hardness of the Fe- and Cr- bearing alloys is classical solid solution strengthening of the BCC W-rich phase. using the Fleischer equation: 83 We estimate solid solution hardening 3/2 1 AH=33 12 G~cl 700 dG G, d dG 1 1 2G, dc (4.1) 3 da a dc where the 33/2 prefactor is used to convert shear stress to hardness, Gw is W's shear modulus, G is the alloy's shear modulus, a is the lattice parameter, and c is the solute concentration [241]. If we assume that there are no solute-solute interactions so that the strengthening effects of Fe and Cr are additive, then using the solute concentrations given earlier and the material properties listed in References [44] and [45], we estimate that solid solution strengthening would increase the hardness in both the W-7Cr-9Fe and W-9Fe compacts by ~20 MPa relative to a nominally pure W compact. The solid solution strengthening contribution is thus two orders of magnitude too small to explain the >1 GPa hardening seen in the present alloys. Although solid solution strengthening effects have been found to be dramatically enhanced in extremely fine grain nanomaterials [113], the grain sizes in the present alloys are too big to permit such an explanation here. A more likely explanation for the high hardnesses of our alloys relative to pure W is the presence of the hard intermetallic pt-phase. This intermetallic's hardness (~17 GPa) is much higher than that of even the hardest nominally pure W compacts from the study of Vashi et al. in Figure 4.9 (~1 3 GPa). Its presence at volume fractions up to 20% can adequately explain the alloy hardness; using the model of Gurland and Lee [242] we can estimate the hardening factor as: AH = (H, - Hf,)f.m C,. (4.2) where H, is the intermetallic's hardness, Hw is the hardness of pure W, fim is the volume fraction of the intermetallic (equal to 14 and 20% in the W-9Fe and W-7Cr-9Fe alloys, respectively), and Cim is a contiguity parameter for the intermetallic (defined in Reference [48] and estimated as CIM z 0.6 based on its volume fraction and the random, homogeneous, and isotropic microstructure) [243]. Using the y-intercept from Vashi et al.'s data, i.e., Hw = 3.7 GPa, the AH values for the W-7Cr-9Fe and W-9Fe compacts are 1.6 and 1.2 GPa, respectively. These align with the measured values of 1.6 and 1.0 reasonably well. 84 We conclude that the alloy compacts are clearly substantially strengthened because of grain size refinement (cf. Figure 4.9), but with a non-negligible contribution from the presence of the intermetallic. 4.4.2. Micropillar Compression Micropillar compression tests were used to measure the yield strength and study the deformation behavior of the ultrafine grain BCC phase. We therefore made efforts to avoid larger p-phase precipitates and pores when machining the microcompression pillars, but cannot rule out the possible presence of some p-phase content in them. Engineering stress-strain curves from several microcompression experiments are shown in Figure 4.10. The Young's modulus, taken from a linear fit of the elastic region of the stress-strain curve, was ~50% of the nanoindentation value (~355 GPa). This difference is ascribed to the compliance of the pillar's base and a non-zero angle (< 1) between the pillar's longitudinal axis and the platen's face normal [244]. Although micropillar compression experiments are generally not well suited for accurate measurement of the Young's modulus, the engineering stress and yield strength values can be reliably measured. The average 0.2% offset yield strength was 5.15 GPa, with apparent hardening to an ultimate engineering stress of about 6 GPa followed by a plateau in the stressstrain response. The plateau is associated with the development of a single shear band within the pillar. An example of a shear offset, captured just before failure at an applied stress level of 6.3 GPa, is shown in the inset of Figure 4.10. - 6 cc C 4- U)Shear Offset C 0) 2 '5 C w 0 0.02 0.04 0.06 Engineering Strain 85 0.08 Figure 4. 10 - Some typical engineering stress-strain curves from micropillar compression tests on pillars preferentially milled from the BCC solid solution phase. Inset shows a shear offset in a micropillar loaded to 6.3 GPa. We are not aware of any other reports on the micropillar compression testing of ultrafine grain W, but our pillars are large (~5x10 pm) compared to the grain size (0.13 prm) and can thus be compared to bulk compression tests. It is particularly instructive to highlight two differences between our results and those from quasi-static compression tests on bulk coarse and ultrafine grain W specimens. First, the pillars' average yield strength of 5.15 GPa is substantially higher than the 3.1 GPa yield strength exhibited by a high pressure torsion specimen reported by Wei et al. [209] This increment in strength is most likely due to better alignment of our specimen with the loading axis, as the high pressure torsion specimen had a similar grain size (170 nm) and microhardness (11 GPa), and Wei et al. reported issues with specimen misalignment and buckling during loading [209]. Second, the shear localization observed in our micropillar compression specimens is consistent with another recent report by Butler et al. of shear localization during quasi-static compression testing of bulk ultrafine grained WI-Re, (x = 5, 10, 25 at%) compacts [245]. These W-Re compacts were also synthesized by powder processing and had porosities similar to our Kolsky bar specimens', but had slightly larger grain sizes (200 to 350 nm). Although Butler et al.'s W-Re samples exhibited lower yield strengths than ours, their post-mortem analysis of the compression specimens showed evidence of shear localization. Apart from the work by Butler et al. described above, W test specimens with grain sizes ranging from 50 prm to 170 nm were reported to have only deformed by homogeneous plastic deformation and axial cracking along grain boundaries [209,212,246]; the only other reports of shear localization in W were from high strain rate tests of ultrafine grain specimens [208,209,212,213,247]. In such high strain rate tests, the shear localization has been most commonly attributed to adiabatic heating that causes localized softening on planes of maximum shear stress. The low strain rates used in both Butler et al.'s and our quasi-static tests are not consistent with this kind of adiabatic shear localization, and instead argue for a structural origin of shear softening. This more closely resembles that seen during quasi-static compression 86 testing of ultrafine grain Fe [248], Ta [249], and Fe-lOCu [250]. In these other materials, shear localization occurs because grain rotation leads to geometric softening [251,252]. 4.4.3. High Strain Rate Deformation A representative engineering stress versus time curve from a Kolsky bar test conducted at a strain rate of 600 s-1 is shown in Figure 4.11. Note that engineering strain values are not reported because these specimens failed at very low strains, which are difficult to measure accurately with a Kolsky bar system. The specimen was loaded until failure, followed by rapid unloading. Accompanying the stress-time curve are images collected using high-speed videography, which serve to illustrate the specimen's brittle mode of failure at 76 pIs. The average failure stress was 4.14 GPa, which is in rough agreement with the Tabor estimate based on the measured microhardness value reported earlier (a ~ H/3 = 13.5 / 3 GPa = 4.5 GPa). 4- 3 q Ca) 2 U) 1 (1 0 20 40 Time (ps) 60 Figure 4.11 - An engineering stress-time curve collected during a Kolsky bar test conducted at a strain rate of 600 s-1. The test specimen was cut from the W-7Cr-9Fe 87 compact consolidated at 1473 K using the 20 mm die. The accompanying high speed photographs were taken at the times indicated by the lines. The arrows next to the first frame indicate the loading direction, and the test specimen's orientation is the same in all of the photographs. Coarse-grained W strained at high rates deforms by a combination of homogeneous plastic deformation and axial cracking [246], and ultrafine grain W has been reported to exhibit adiabatic shear localization [208,209,212,213,247]. In our samples, the residual pores act as stress risers and crack nucleation sites, while the brittle intermetallic p-phase lowers the compact's toughness. Together, these two microstructural features likely contributed to the onset of fracture events at high rates. Based on our samples' grain size and the micropillar compression results on the W-rich BCC phase reported in the previous section, we speculate that the BCC phase would favor shear localization under both quasi-static and high strain rate testing. This is because other ultrafine grain BCC metals that exhibit structural shear localization during quasi-static compression tests also typically exhibit shear localization in high strain rate tests [248]. Therefore it is expected that further tuning of the alloy composition and consolidation schedule to reduce the volume fraction of the intermetallic and the porosity could permit some tuning of the propensity for shear localization versus cracking. 4.5. Concluding Remarks Nanocrystalline W-rich alloy (W-9Fe and W-7Cr-9Fe) powders have been synthesized via mechanical alloying, and the microstructure and mechanical properties of compacts made from the powder systematically investigated. The main results of this work are as follows: " Ultrafine grain W-rich compacts with high relative densities were achieved by suppressing the rate of grain growth during consolidation, by (1) minimizing the thermal excursion during consolidation, thereby slowing thermally activated grain growth, and (2) alloying with Cr, an element expected to reduce grain boundary energy and mobility in W. Dense compacts with grain sizes as small as 130 nm were synthesized. " The ultrafine grain compacts' hardnesses were greater than 12 GPa due to grain size strengthening in the W-rich, BCC phase, and followed the Hall-Petch scaling. A second significant contribution to their hardnesses (-1-2 GPa) came from the hard intermetallic tphase that precipitated during compaction. 88 * The ultrafine grain compacts exhibited very high quasi-static and dynamic compressive failure strengths measured using micropillar compression and Kolsky bar tests, respectively. During micropillar compression experiments, pillars that were ion-milled out of a compact began to yield at 5 GPa and eventually failed by shear localization upon loading to 6 GPa. During Kolsky bar tests on bulk specimens machined out of the same compacts, the samples failed at an average stress of 4.14 GPa. 89 5. Sub-Scale Ballistic Testing of an Ultrafine Grained Tungsten Alloy The high-density, ultrafine grain alloys described in the previous chapter possesses a unique set of mechanical properties that make them very attractive kinetic penetrator materials for rigid body penetration into concrete and geomaterials. Their high strengths, for instance, suggest that they should remain elastic at striking velocities where penetrators made from softer materials, e.g., high strength steels, start to deform plastically [209,253,205,208,254-256,2]. In this chapter, we evaluate the ballistic performance of these ultrafine grain tungsten alloy using subscale ballistic tests into concrete targets. This sub-scale test method departs from many of the standard protocols for characterizing penetration performance, which call for penetrators with large dimensions. For example, the classic Forrestal framework for evaluating the performance of rigid body penetrators into concrete was originally developed for penetrators with lengths upwards of 9 cm and diameters of at least 1 cm [257]. Our results demonstrate the potential of sub-scale ballistic testing as a means of characterizing next-generation kinetic penetrator materials as well as the potential of this specific tungsten alloy in ballistic applications. 5.1. Experimental Methods We studied the ballistic performance of two different penetrator materials: a tungsten carbide cermet (WC-12Co, wt%) and a powder-processed, ultrafine-grained W alloy. A schematic of the cemented carbide penetrator is shown in Figure 5.1 a. We used these conical nose cemented carbide rounds to calibrate the penetration equations described below. Quasi-static compression tests on specimens machined from these cemented carbide rounds gave an average failure stress of 3.8 GPa, with the samples failing by brittle fracture. 90 a. 10.4 mm 4.0 mm 550 14.2 mm b. 8.0 mm 4.0 mm R, 10.0 mm 14.0 mm Figure 5.1 - Schematics of the a) cemented carbide and b) W-8Cr-4Fe penetrators. We also prepared sub-scale rounds from an ultrafine-grained W-Cr-Fe alloy whose chemistry and processing schedule are related to the optimized alloy described in Chapter 4. The material used in this study was prepared by 6 hours of attrition milling of elemental feedstock powders of W and Cr (99.95 pct W -100 mesh; 99+ pct Cr, -325 mesh) with an initial stoichiometry of W-lOCr, at%. Milling was performed under an Ar atmosphere using 200 g of powder, steel media, and a ball to powder ratio of 10:1. The final chemistry of the as-milled powder was W8Cr-4Fe, at% as measured by energy dispersive spectroscopy, where the Fe was introduced due to abrasion of the milling equipment. Note that this is a different chemistry from that reported in Chapter 4 and this difference is due to the fact that we used attritor mill, as opposed to a SPEX mill, to produce larger quantities of powder for these ballistic tests. We consolidated the as-milled powder using a Dr. Sinter SPS-515S hot press, a graphite punch and die having a diameter of 24 mm, and the preferred consolidation parameters identified in Chapter 4: a ramp rate of 100 K/min, a consolidation pressure of 100 MPa, a soak time of 1 min, and a soak temperature of 1200 'C. We centerless ground samples electro-discharge machined from the center of these compacts into ogive nose rounds with the dimensions given in Figure 5.1b. We mounted in epoxy, cross-sectioned, and polished one of these W-8Cr-4Fe rounds using standard metallographic techniques, and characterized the microstructure of this cross-sectioned round using a JEOL 6610LV scanning electron microscope (SEM) operated at 20 kV and equipped with an energy dispersive spectrometer. 91 We also measured this cross-sectioned round's Vickers microhardness using a LECO microhardness tester with a load of 50 gf and a hold time of 15 s. These microstructural investigations revealed that the W-8Cr-4Fe penetrators had a bimodal grain size distribution: approximately 85 vol% of the penetrator had a grain size of 200 nm, while the remaining material was coarse grained, with an average grain size exceeding 10 tm. As a result of their different grain sizes, the coarse- and fine-grained regions had different mechanical properties, with the fine grained regions having an average Vickers hardness of 10.8 GPa, more than double the Vickers hardness of the softer, coarse-grained regions. The coarse- and fine-grained regions also had different chemistries, with the coarsegrained regions containing no solute and the fine grained regions containing Fe and Cr, with an average stoichiometry of W-IOCr-6Fe as measured by energy dispersive spectroscopy. That only the fine grained regions contained Fe and Cr supports our claim in Chapter 4 that these alloying elements are critical for retaining a fine grain size. This penetrator's average stereological porosity was 6%, and its density was 16.1 g/cm 3 as measured by the Archimedes method using high purity water as a reference liquid. We fired the projectiles from a 5.56 mm diameter powder gun with a 1:7 twist and a 0.5 m long barrel, and varied the incident velocity between 500 to 1100 m/s by using different amounts of gun powder. We monitored the incident velocity as well as the pitch and yaw at impact using flash x-radiography [258]. Based on these measurements, we adjusted the muzzle-to-target distance between 3.3 and 3.9 m to minimize the pitch and yaw at impact, and only included tests with angles of incidence less than 4' in our analysis. We fired all of the shots into targets prepared from the same batch of well-cured concrete. The concrete had a density of 2.2 g/cm 3 and contained aggregate with a volume-average, circular equivalent diameter of 2 mm. Cylindrical compression specimens with a 5 cm diameter and an aspect ratio of 2.5 that were cored from several targets had an average, unconfined compressive failure strength of 48 MPa. The concrete targets had cross-section dimensions of 20 by 20 cm and a thickness of 13 cm. The maximum depth of penetration was roughly half the thickness of the target and there was no scabbing seen on the back face of the target after impact, so these targets could be approximated as semi-infinite. The reported depths of penetration are the average of two measurements from radiographs taken at right angles to one another, which were always in good agreement. 92 l+g[ ]+4R 5.2. Sub-Scale Ballistic Testing into Concrete Forrestal and coworkers used experiments and theory to develop a framework describing rigid body penetration into concrete and geomaterials [257,259-270]. Using penetrators with on- board accelerometers [267,268,270], these researchers showed that the axial force on a projectile during impact can be described by the following relationships: 4R (5.la) z > 4R (5.1b) z F = -cz F = -7rR 2 (US + NpV 2 ) where Eqns 5.1 a and 5.1 b describe the force equations during the cratering and tunneling phases of impact, respectively, and with z the instantaneous depth of penetration, R the radius of the penetrator, U the unconfined compressive stress of the concrete target, p the density of the concrete, and V the instantaneous velocity of the penetrator. The pre-factor c in Eqn 5.1 a is a constant that depends on the incident velocity, VsK, as follows: (5.2) C = wR Sa + mVsNp 4 m + 47rR3Np) The constant N accounts for the shape of the penetrator's nose. For conical-nose penetrators, N is given by N = sin(p) 2 (5.3) where (p is half the nose angle [271], and for ogive-nose penetrators, N is calculated using N = (5.4) 81P-1 241p2 where ip = r/2R with r being the ogive radius [257]. Table 1 summarizes the properties of the cemented carbide and W-8Cr-4Fe penetrators that are necessary for evaluating Eqns 5.1 to 5.4. The constant S in Eqns 5.la, 5.1b, and 5.2 is a fitting parameter that accounts for the strengthening of the concrete due to the hydrostatic compressive stress and high strain rates at the tip of the penetrator. Evaluating the equations of motion using Eqn 5.1a and 5.1b and the initial condition that V = V, at z = 0 gives the following relationship between the incident velocity and the depth of penetration _____ (5.5)P = 2 27rR pN Sum+NpmVS 3 Sa(m+47R Np) 1 93 which can be fitted to experimental data to calibrate S. Table 5.1 - Properties of the cemented carbide and tungsten alloy penetrators. m (g) N WC-Co 2.1 0.21 W-8Cr-4Fe, at% 2.3 0.13 Forrestal and coworkers have shown that Eqns 5.1 through 5.5 apply to penetrators with lengths ranging from 9 to 53 cm and diameters between 1.3 and 8 cm [257,267,268,270]. To test if they apply to sub-scale penetrators as well, we compared their predictions with the behavior of the much smaller cemented carbide penetrators. Because these cemented carbide penetrators are two orders of magnitude stronger than the concrete targets, it was expected that they would remain elastic during impact given the incident velocities used in this study. This expectation was confirmed by radiographs of these cemented carbide rounds embedded in concrete targets, like those shown in Figure 5.2a, which reveal a lack of plastic deformation (though there is evidence of fracturing which we discuss later). These radiographs also reveal distinct cratering and tunneling regions in the wake of the penetrator, with the average depth of the craters being I cm, or roughly twice the diameter of the penetrator. The morphology of this impact zone is consistent with Forrestal et al.'s previous reports of penetration into concrete [257,263,264,268]. In Figure 5.2b, we plotted the cemented carbide penetrators' incident velocities against their depths of penetration, as well as a best fit to these results using Eqn 5.4. The agreement between the fit and the results is quite good, confirming that the Forrestal equations work very well even with these small-caliber penetrators. From this fit, we found S= 24, which is twice that predicted by Forrestal et al. for concrete with a compressive strength of 48 MPa [257,264,266]. The reason for this discrepancy is the small ratio of the penetrator diameter to aggregate diameter in our work; the smaller this ratio, the larger S is for a given strength concrete, as noted by Beth [272] and others [267]. 94 b. a. Y= cemented carbide shots - 10 720 m/s -00 C Rigid body penetration, Eqn 5.5 j_ 1> crater 82- 820m~0 1 M C 4-5 -W 910 m/s ~00 0.6 0.8 1.0 1.2 Incident Velocity (km/s) Figure 5.2 - a) Radiographs of cemented carbide rounds that struck the targets at the velocities indicated. The crater region is highlighted in the radiograph of the penetrator that had an incident velocity of 720 m/s. b) Cemented carbide rounds' depths of penetration as a function of incident velocity. The dashed line is the best fit to the data using Eqn 5.4, and the grey shaded region indicates the 95% confidence intervals. In light of these cemented carbide results, we next evaluated the penetration behavior of the W8Cr-4Fe rounds, which still performed well in these ballistic tests despite their processing defects, e.g., porosity, regions of coarse-grained material, and chemical heterogeneity. Figure 5.3a shows a set of radiographs of the concrete targets containing embedded W-8Cr-4Fe penetrators, which have dimensions similar to those of the as-received penetrators, excluding the 620 m/s shot. To test for rigid body behavior, we plotted the W-8Cr-4Fe penetrator's depth of penetration as a function of incident velocity alongside the depth of penetration predicted by Eqn 5.5 in Figure 5.3b. Aside from a slight deviation between the predicted and measured depths of penetration at the highest striking velocity, which we can ascribe to the larger angle of incidence of that penetrator at impact (~2.5o), the measured and predicted values agree quite well, confirming rigid body penetration and attesting to the high strength of this ultrafine grained alloy. 95 b. ultrafine grain W shots 10 620 msC- Rigid body penetration, Eqn 5.5 4). 5 1070 ms 01 0.6 1 CIncident 0.8 1.0 Velocity (km/s) 1.2 Figure 5.3 - a) Radiographs of W-8Cr-4Fe rounds embedded in the concrete targets. b) Depth of penetration of the W-8Cr-4Fe penetrators as a function of incident velocity. The rigid body depth of penetration predicted using Eqn 5.4 is shown as well. Of more engineering significance is the fact that the W-8Cr-4Fe penetrators appear to be more tolerant of oblique impact at high velocities than the cemented carbide penetrators. This is illustrated by Figures 5.4a and 5.4b which show radiographs of shattered cemented carbide penetrators and the angle of incidence versus the incident velocity of the different penetrators, respectively. In Figure 5.4b, the cemented carbide penetrators that fractured during impact are indicated by crosses. Figure 5.4b suggests that the cemented carbide rounds are more likely to fracture than the W-8Cr-4Fe penetrators under equivalent or less severe impact conditions (i.e., either smaller angles of incidence or lower incident velocities or both), though the data is limited and a direct comparison between the cemented carbide and W-8Cr-4Fe penetrators is complicated by their different nose geometries. 96 a. WC-Co penetrators, V = 820 m/s b. * W-8Cr-4Fe * WC-Co X shattered WC-Co 3 X 930 m/s CD CD 1 1030 m/s ee 00 0 0.6 1 cm X I I 0.8 1.0 Incident Velocity (km/s) 1.2 Figure 5.4 - a) Radiographs of cemented carbide penetrators that shattered on impact. b) Incident velocity versus angle of incidence, y, of the W alloy and cemented carbide shots with the cemented carbide shots that fractured indicated by crosses. We can use the results from these sub-scale ballistic tests to compare the different penetrator materials by estimating limit velocities above which these small scale penetrators should transition from rigid body to eroding behavior. From Eqns 5.1 a and 5.1 b, we can estimate the forces acting on the rounds during penetration. By normalizing these forces by the penetrator's cross-sectional area, we can then estimate the nominal stresses that the rounds experience. The maximum nominal stress that the rounds experience during impact is then given by Gmax = Sm + mVs2 Np 3 (5.6) m + 47rR Np Setting Eqn 5.6 equal to the yield strength of the penetrator material and solving for V gives a rough estimate of the limit velocity, Vmax. Note that this V,,x represents an optimistic estimate since it assumes perfectly normal incidence; in reality, fracture or plastic flow may occur at lower velocities due to bending moments generated by oblique impact, for example. With Vnax, we can then calculate a kinetic energy density, p(Vjax)2 , where p is the density of the penetrator material. This kinetic energy density can be used as a figure of merit for comparing different penetrator materials. 97 As an example of how to apply these concepts, we use them to compare our W-8Cr-4Fe material with high strength steel, the standard material used in concrete penetration. Our ultrafine grained W-8Cr-4Fe alloy has a dynamic compressive strength of 2.8 GPa as measured by Kolsky pressure bar experiments, so penetrators made from this alloy with the geometry shown in Figure 5.1b should start to yield at incident velocities of 2.2 km/s. By contrast, high strength steel penetrators with the same geometry and a yield strength of 1.5 GPa should start to yield at much lower incident velocities, around 1.2 km/s. Combined with the ~8 g/cc density of steel, these limit velocities indicate that penetrators made from our ultrafine grained W-8Cr-4Fe alloy should be capable of delivering 7 times the kinetic energy of a high strength steel round before transitioning from rigid body to eroding behavior. 5.3. Concluding Remarks Sub-scale ballistic tests into concrete have been performed using cemented carbide and ultrafine grained tungsten alloy penetrators. We found that the penetration behavior of these small- caliber rounds was well-described by the Forrestal equations. After calibrating the fitting parameter in these equations, we were able to evaluate the performance of the ultrafine grained tungsten alloy penetrators and quantitatively demonstrate that they essentially behave as a rigid body penetrators over the range of velocities tested. In addition, this tungsten alloy appears to be less likely to fracture due to oblique impact at high velocities than the cemented carbide calibrant penetrators. These results together demonstrate the promise of this particular tungsten alloy as well as the potential of sub-scale ballistic testing as a tool for rapidly screening novel ballistic materials. 98 6. Conclusions High energy ball milling is not a new processing technique; it was developed in the late 1960's and is currently used to manufacture large quantities of oxide dispersion strengthened superalloys [17]. Despite this, the process's effects on microstructure are still poorly understood, so using it to synthesize materials with tailored microstructures remains a trial-anderror endeavor. The same is true for most of the other severe plastic deformation processing techniques such as high-pressure torsion and equal channel angular pressing. Removing some of the empiricism associated with these techniques was the main objective of this thesis. A second, related objective was using this improved understanding of mechanical alloying to guide the microstructure design of a powder capable of being consolidated into bulk ultrafine grained parts. The following summary highlights the main contributions of this thesis: " The process of mechanical alloying has been studied in several tungsten-transition metal couples in order to develop a better understanding of phase strength effects on shearinduced chemical mixing. One group of binary alloys (W 5 oCr5 o, W 5oNb5 O) is found to rapidly mix to a chemically homogeneous state, while a second group (W5oNi 5o, W 5 oHf5 o, W5 oZr5o) is found to remain dual-phase despite prolonged milling. The two groups' disparate mixing behaviors are directly linked to strain localization due to differences in the base alloying elements' relative strengths using nanoindentation experiments on individual power particles and SEM observations of the pile-up around these nanoindentations. These experiments also revealed asymmetric mechanical mixing in the couples that remained dual-phase, wherein some W dissolved in the second alloying element while the W remained relatively pure. " The results from these experiments are incorporated into classical Bellon-Averback type kinetic Monte Carlo simulation of mechanical alloying so that they better account for strain localization effects. With these improved simulations, we reproduce the asymmetric mixing and channeling behaviors observed during the high energy ball milling of W 50 Ni50 , W 50 Hf5 0 , and W5 oZr50 strength. - couples with large fractional differences in We also use these simulations to generate dynamical phase diagrams which 99 feature an asymmetric dual-phase region with a width that is directly proportional to the alloying elements' fractional difference in strength. Finally, we demonstrate with simulations of low-temperature mechanical alloying that couples with large fractional differences in strength should exhibit path-dependent steady state microstructures. Though such a path dependence has been observed in other dissipative systems, it has not previously been demonstrated in mechanically alloyed materials. This result also runs counter to the conventional wisdom of Martin's rule of corresponding states, which holds that a driven alloy has a unique steady state chemical mixity under a given set of processing conditions. " An analysis is introduced that builds on insights from these mechanical alloying experiments and simulations and that enables one to predict the microstructures that will emerge in extensively deformed materials. This analysis is calibrated using studies available in the open literature, and takes into account the effects of strain localization as well as the competition between shear-induced mixing and thermally activated phase separation. With the output of this analysis, it is straightforward to identify mechanically immiscible, mechanically miscible, and nanopatterning couples. " We describe a nanocrystalline tungsten-based alloy powder that forms a homogeneous solid solution during high energy ball milling, and explore the consolidation behavior of this nanocrystalline powder in detail, demonstrating that it can be compacted into dense ultrafine grained articles under one set of processing conditions. Using a battery of characterization techniques, we also show that compacts prepared with this optimized set of processing parameters exhibit a suite of properties - high strength, specific gravity, and relative density - that make this alloy ideal for penetration applications. * The penetration performance of this material is evaluated with sub-scale ballistic testing into concrete targets. Despite defects in the rounds, they still perform favorably, remaining rigid body at the highest striking velocities, ~1100 km/s. As the preceding summary illustrates, the topics explored in this thesis run the gamut from materials science (e.g., the theory of mechanically driven alloys) to materials engineering (e.g., the synthesis and testing of a new and improved ballistic material). Possible avenues for future research in each of the topics covered in this thesis are summarized below: 100 * It would be interesting to experimentally verify that there are path dependent steady state microstructures in mechanically alloyed materials. The best candidates for exhibiting this behavior are the mechanically immiscible couples identified in the map in Chapter 3. * The dynamical phase diagrams should be further calibrated with additional mechanical alloying experiments. To systematically test the effects of temperature on the steady state chemical mixity, I have developed jackets capable of maintaining the vial at temperatures between 77 and 500 K and plan to conduct variable temperature milling experiments in the future. It would also be interesting to experimentally identify the volume fraction at which alloys become "geometrically constrained" to co-deform and mix. Studying how this volume fraction varies with A could shed light on the length scales associated with plastic deformation in particulate, nanocomposite materials. " With a better understanding of strain localization in nanocomposites, it should be possible to improve the analysis in Chapter 3. Here one possible research direction will be to describe plastic deformation in these nanocomposite materials, which have negligible capacity to work-harden, with load-bounding or slip line field theories. " The ultrafine grain tungsten compacts described in Chapter 4 possess a suite of very attractive properties; however, their ductility and, relatedly, toughness should be improved if large penetrators made from this alloy are to survive high-angle, oblique impact or the relief stress pulses generated during penetrator launch. It will be important to improve these properties without sacrificing relative density, specific gravity, or strength, and one way to go about doing this is to minimize the volume fraction of the intermetallic. * More ballistic testing is needed in order to fully evaluate the effects of obliquity, nose shape, target material, etc. on the performance of the small-caliber rounds described in Chapter 5. 101 ...... ......... .. ..... Appendix A: Aggregated Hall-Petch Data Al Cu (DMAn 4 4 (DMA~min 3 3 a- 0Omax 0 -- ------ 02 2 Omax 1 1 UP 0 .0 0.3 . a 0.2 0.1 0.2 0.3 0.4 D112 (nm"2) (nm r) D-1/ Au Ni ---------------- 4 0.1 0.0 0.4 (DMA min 4 - Omax 3 3 b 2 02 0~ 00max 1 (DA (D)MA min) nI 0.0 1 2 0 0.3 0.2 2 D-1 (nM-1 ).0 0.4 (D MAm ) 0.4 4 11 2 3 3 - - Omax 0 0 2 I (DMA,m n Omax --- -- - - - - - - - - - - - - I 1 ni 0.0 0.3 Pd 4 0 2 0.2 D12 (M-1/) Ag 0 0.1 2 ) 0.1 0.1 0.2 0.3 U 0.0 0.4 I 0.1 0.2 0.3 0.4 0.5 0.6 D" 2 (nm-1 2) D" 2 (nm-1 2 ) ----L------------- 1 -- Figure A. 1 - Hall-Petch data for the FCC metals. The horizontal grey line indicates the 102 metal's theoretical strength and the vertical gray line indicates the grain size that the pure as-milled powders will develop. 103 8 - I I I I Cr I I I I I 8 iI 0 .max - 0 Max 6 6 4 0-4 (DMAmi 2 1/2 I- 2. (DMAmn 0.1 0.4 0.2 0.3 D-1 2 (nm 1 2 0.1 8 0.2 D-1 ) 0.0 Nb 0.3 0.4 (nm-1 2 ) 00.0 Oh 112: -V 8 (DMAm)12 (DMAmi) 6 6 0 0-4 4 0 0max 0.1 0.2 12 D- 8 0.3 - 0 0 .0 0.1 0.2 D 1 /2 --- 0.3 1 (nm- 2 0.4 Mo 8 m)'2 --- - - - -F Ta (D 2 0.4 (nm-" 2 -- ) 0 0. 0 ) 2 ------------------- Max-- -- -- -- -- -- -- -- - 0 7 max - 6 ------- - 6 - -- - - - - -- - - - A----- 0- Omax 4 112 (DMA.Mi)1 2 2 o 0.0 / Al 0.1 0.2 0.3 0.0 0.4 12 D- (nm-') a a 3 3 0.1 0.2 a 3 0.3 1 2 D- (nm" 2 ) 0 4 Figure A.2 - Hall-Petch data for the BCC metals. 104 0.4 ...... ................................. x.. ......... Fe 8 - 6 a. 0,max 2 -(DM 0.1 0.2 0.3 D- 2 12 (nm 112 0.4 ) 0 0.0 minY Figure A.3 (cont.) - Hall-Petch data for the BCC metals. 105 . .......................... ....... ........... .. ............. I II Be ----____-_-.-------- ---- Mg - 8_ I aOmax 4 (D MA.mtn))1I2 6 -. 3 0 0 (4'-4 02 - 0 COmax 2 1 -- - --- ---- - - ------ (DMAmn)1/2 '.r-7--- 0 0.0 0.1 0.3 0.2 0 0.4 0.3 0.2 D-1 2 (nm- 12 0.1 ).0 ) Ti Co 4 0.4 ) D" 2 (nm-" 2 4 CY,max 3 - D -3 CL 0 C0 0 0max 02 2 1 I 1 1-2 :(DMA minY (DMA mm) a 0 0 .0 0.1 0.2 2 a 0.4 0 D.0 0.3 0.2 2 D-" (nm") 0.1 (nm 112 ) D" a 0.3 1/ 2 0.4 Zr Zn 4 - 4 (D MAim) 112 3 -3 - 0 1! 0 2 0Omax -- - omax - 0 02 1 0 0.1 0.2 D-1 2 0.3 0.0 0.4 (nm-1 2 Figure A.4 - Hall-Petch data for the HCP metals. 106 . ......... 1/ (DMAmi1 A 0.1 0.3 0.2 D" ) 0.0 V 2 (nm-"2) 0.4 References [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] E.O. Hall, The Deformation and Ageing of Mild Steel: 11 Discussion of Results, Proc. Phys. Soc. Sect. B. 64 (1951) 747. Z.C. Cordero, E.L. Huskins, M. Park, S. Livers, M. Frary, B.E. Schuster, et al., PowderRoute Synthesis and Mechanical Testing of Ultrafine Grain Tungsten Alloys, Metall. 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