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I1.)- ; .rh, . . ‘ . 5:} tut u . 5.. : .7. 300] This is to certify that the thesis entitled THE METAL FLUX SYNTHESIS AND CRYSTAL GROWTH OF BINARY AND TERNARY BORIDES presented by Britt Andrew Vanchura II has been accepted towards fulfillment of the requirements for the MS. degree in Chemistry Major Professor’s Signature flj 0 6 / Q 00 6 Date MSU is an Afiirmative Action/Equal Opportunity Institution l "TIBRARY Michigan State University —.-.—.—.-.—--.—.—.-.-.-.—.—.—.-..—A—.-o—o-c-u-o-o-t---o--u- 00-0-.----p-I-c-u-o-n-c-u-n-o-u-o-n--—.-»—.—.-.- PLACE IN RETURN Box to remove this checkout from your record. TO AVOID FINES return on or before date due. MAY BE RECALLED with earlier due date if requested. DATE DUE DATE DUE DATE DUE 2/05 p:!ClRC/DaleDue.indd-p.1 THE METAL FLUX SYNTHESIS AND CRYSTAL GROWTH OF BINARY AND TERNARY BORIDES By Britt Andrew Vanchura II A THESIS Submitted to Michigan State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Department of Chemistry 2006 ABSTRACT THE METAL FLUX SYNTHESIS AND CRYSTAL GROWTH OF BINARY AND TERNARY BORIDES By Britt Andrew Vanchura II Borides form a large class of compounds with diverse structural and physical properties. Traditionally, high-temperature furnaces, arc welders, and radiofrequency (RF) induction furnaces have been used to reach the elevated synthesis temperatures of most borides. By using a low-melting point metal as a solvent-like flux, the reaction temperatures for boride synthesis can be lowered by several hundred degrees. Our group has recently had success using molten gallium to synthesize the new borides RE3-XC28ig(Blz)3 (RE = Tb and Br) and B-SIB3, which are only obtainable through flux synthesis. Literature searches have found that molten copper and aluminum have also been used successfully as fluxes for the synthesis and crystal growth of many borides. In the present work we expanded the use of gallium as a metal flux by synthesizing and growing crystals of borides in the Cr—B, Mo—B, W—B, Mn—B, Re—B, Ho—Mn—B, and RE-Re—B (RE = Dy, Er, Yb) systems. Molten copper was used to synthesize borides from the Cr—B, Ru—B, and RE—Ru-B systems. Structural characterization by single crystal x-ray diffraction was carried out on all borides produced from the metal fluxes. The structures of the borides and general observations on the metal flux technique and its applications to boride synthesis are discussed. Copyright by Britt Andrew Vanchura H 2006 ACKNOWLEDGEMENTS I would like to thank my wife Jaime for being the wonderful person that she is. Nobody could be more supportive, encouraging, and understanding. My daughter Caroline has been an inspiration. Even on the bad days she’s there to great me with a “Da!” and hug. I could never thank my parents enough for all that they have done. I thank God everyday for giving me such a loving family. I would like to thank my advisor, Mercouri Kanatzidis, for all his help, support, and advice. The help and support from past and present Kanatzidis group members is greatly appreciated. The support staff in the chemistry department has been a tremendous help, even when things were more than a little crazy. iv TABLE OF CONTENTS LIST OF TABLES ..................................................................................................... viii LIST OF FIGURES ................................................................................................... xiii LIST OF ABBREVIATIONS .................................................................................... xv Chapter One The Metal Flux Technique in Boride Synthesis ................................ 1 A. Introduction .................................................................................. 1 B. The Metal Flux Technique ........................................................... 1 C. Structural Features in Borides ...................................................... 5 D. Chemical and Physical Properties of Borides .............................. 7 Chapter References .......................................................................................... 10 Two The Metal Flux Synthesis of Group Six Borides ............................... 13 A. Introduction .................................................................................. 13 B. Experimental ................................................................................ 15 Reagents ....................................................................................... 15 Furnaces ....................................................................................... 15 Synthesis and Isolation ................................................................ l7 Cr5B3 ...................................................................................... 17 033.; ...................................................................................... 17 CrzB3 ...................................................................................... 18 Cl‘Bz ........................................................................................ 19 M08 ....................................................................................... 19 WB ......................................................................................... 20 C. Physical Measurements ................................................................ 20 Energy Dispersive Spectroscopy ................................................. 21 Single Crystal X-ray Crystallography .......................................... 21 D. Structural Description .................................................................. 38 Cl'sB3 ...................................................................................... 38 Cr3B4 ...................................................................................... 38 0ng ...................................................................................... 38 CrBz ........................................................................................ 41 MB (M= Mo, W) ................................................................... 41 E. Results and Discussion ................................................................. 41 F. Conclusions ................................................................................... 44 References .......................................................................................... 46 Chapter Three The Metal Flux Synthesis of Group Seven Borides ........................... 48 A. Introduction .................................................................................. 48 B. Experimental ................................................................................ 49 Reagents ....................................................................................... 49 Furnaces ....................................................................................... 50 Synthesis and Isolation ................................................................ 51 Chapter Four MnB4 ...................................................................................... 52 R632 ....................................................................................... 52 HoMnB4 ................................................................................. 53 REReB4 (RE = Dy, Er, Yb) ................................................... 54 C. Physical Measurements ................................................................ 55 Energy Dispersive Spectroscopy ................................................. 55 Single Crystal X-ray Crystallography .......................................... 55 D. Structural Description .................................................................. 71 MnB ....................................................................................... 71 WE; ...................................................................................... 71 ReBz ....................................................................................... 74 HoMnB4 and REReB4 (RE = Dy, Er, Yb) ............................. 74 E. Results and Discussion ................................................................. 77 MnB ....................................................................................... 77 MnB4 ...................................................................................... 78 R632 ....................................................................................... 80 HoMnB4 ................................................................................. 80 REReB4 (RE = Dy, Er, Yb) ................................................... 80 General Discussion ...................................................................... 82 F. Conclusions ................................................................................... 83 References .................................................................................... 84 The Metal Flux Synthesis of Ruthenium Borides .............................. 86 A. Introduction .................................................................................. 86 B. Experimental ................................................................................ 87 Reagents ....................................................................................... 87 Furnaces ....................................................................................... 88 Synthesis ...................................................................................... 89 R0733, RilzB3, and RuBz ........................................................ 89 B-RuBz ................................................................................... 89 RERu434 (RE = Y, Ce, Sm, Dy, Yb) ..................................... 9O RE,‘(Ru4B4)y (RE = Pr, Nd) .................................................... 90 Isolation from flux ....................................................................... 90 C. Physical Measurments .................................................................. 91 Energy Dispersive Spectroscopy ................................................. 91 Single Crystal X-ray Crystallography .......................................... 92 D. Structural Description .................................................................. 110 RU7B3 ...................................................................................... I 10 RU233 ...................................................................................... 1 10 RuBz ....................................................................................... 110 B-RuBz ................................................................................... 114 RERu4B4 (RE = Y, Ce, Sm, Dy, Yb) ..................................... 114 E. Results and Discussion ................................................................. 116 F. Conclusions ................................................................................... 120 References .......................................................................................... 121 MnB ....................................................................................... 51 vi Chapter Five Gallium-Rich Gallides Isolated as By-Products from Molten Flux Reactions Containing Boron .......................................................................... 123 A. Introduction .................................................................................. 123 B. Experimental ................................................................................ 124 Reagents ....................................................................................... 124 Furnaces ....................................................................................... 124 Synthesis and Isolation ................................................................ 124 MnGa4,65 ................................................................................. 124 ReGa4_5 ................................................................................... 125 . NIo_57Ga4_43 .............................................................................. 126 C. Physical Measurements ................................................................ 127 Energy Dispersive Spectroscopy ................................................. 127 Single Crystal X-ray Crystallography .......................................... 127 D. Structural Description .................................................................. 136 MGa4+x (M= Mn,Re) .................................................................... 136 Nio_57Ga4_43 .................................................................................... 140 E. Results and Discussion ................................................................. 142 F. Conclusions ................................................................................... 144 References .......................................................................................... 145 Chapter Six Conclusions and Future Work ........................................................... 146 References .......................................................................................... l 50 Appendix RF Furnace Design and Setup ............................................................ 151 vii Table 2-1. Table 2-2. Table 2-3. Table 2-4. Table 2-5. Table 2-6. Table 2-7. Table 2-8. Table 2-9. Table 2-10. Table 2-11. Table 2-12. Table 2-13. Table 2-14. Table 2-15. Table 2-16. Table 2-17. LIST OF TABLES Crystal data and structure refinement for Crng, 24 Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Cr5B3. 25 Anisotropic displacement parameters (Azx 103) for Cr5B3. 25 Bond distances (A) for Cr5B3. 26 Crystal data and structure refinement for 033;. 27 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for CI'3B4. 28 Anisotropic displacement parameters (Azx 103) for 033;. 28 Bond distances (A) for Cr3B4. 29 Crystal data and structure refinement for Cr2B3. 30 Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Cr2B3. 31 Anisotropic displacement parameters (Azx 103) for CrzB3. 31 Bond distances (A) for Cr2B3. 32 Crystal data and structure refinement for CrBz. 33 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for CrBz. 34 Anisotropic displacement parameters (Azx 103) for 032. 34 Bond distances (A) for CrBz. 34 Crystal data and structure refinement for MoB and WB. 35 viii Table 2-18. Table 2-19. Table 2-20. Table 2-21. Table 3-1. Table 3-2. Table 3-3. Table 3-4. Table 3-5. Table 3-6. Table 3-7. Table 3-8. Table 3-9. Table 3-10. Table 3-11. Table 3-12. Table 3-13. Table 3-14. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103)for M03 and WB. 36 Anisotropic displacement parameters (Azx 103) for M03 and WB. 36 Bond distances (A) for M08. 37 Bond distances (A) for WB. 37 Crystal data and structure refinement for MnB. 58 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for MnB. 59 Anisotropic displacement parameters (Azx 103) for MnB. 59 Bond distances (A) for MnB. 59 Crystal data and structure refinement for MnB4. 60 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for MnB4. 61 Anisotropic displacement parameters (A2x 103) for MnB4. 61 Bond distances (A) for MnB4. 61 Crystal data and structure refinement for ReBz. 62 Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for ReBz. 63 Anisotropic displacement parameters (Azx 103) for ReBz. 63 Bond distances (A) for ReBz. 63 Crystal data and structure refinement for HoMnB4. 64 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (A2x 103) for HoMnB4. 65 ix Table 3-15. Anisotropic displacement parameters (Azx 103) for HoMnB4. 65 Table 3-16. Crystal data and structure refinement for REReB4 (RE= Dy, Er) 66 Table 3-17. Crystal data and structure refinement for YbReB4. 67 Table 3-18. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for REReB4 (RE = Dy, Er,Yb). 68 Table 3-19. Anisotropic displacement parameters (Azx 103) for REReB4 (RE = Dy, Er, Yb). 69 Table 3-20. Bond distances (A) for HoMnB4 and REReB4 (RE = Dy, Er, Yb). 70 Table 4-1. Crystal data and structure refinement for R0733. 95 Table 4-2. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for RU7B3. 96 Table 4-3. Anisotropic displacement parameters (Azx 103) for Ru7B3. 96 Table 4-4. Selected bond distances (A) for Ru7B3. 97 Table 4-5. Crystal data and structure refinement for Rung. 98 Table 4-6. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for RuzB3. 99 Table 4-7. Anisotropic displacement parameters (Azx 103) for Ru2B3. 99 Table 4-8. Selected bond distances (A) for Ru2B3. 99 Table 4-9. Crystal data and structure refinement for RuBz. 100 Table 4-10. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for RuBz. 101 Table 4-11. Anisotropic displacement parameters (A2x 103) for RuBz. 101 Table 4-12. Selected bond distances (A) for RuBz. 101 Table 4-13. Table 4-14. Table 4-15. Table 4-16. Table 4-17. Table 4-18. Table 4-19. Table 4-20. Table 4-21. Table 4-22. Table 5-1. Table 5-2. Table 5-3. Table 5-4. Table 5-5. Table 5-5. Table 5-7. Crystal data and structure refinement for B-RuBz. 102 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for B-RuBz. 103 Anisotropic displacement parameters (Azx 103) for B-RuBz. 103 Selected bond distances (A) for B-RuBz. 103 Crystal data and structure refinement for RERu4B4 (RE= Y, Ce). 104 Crystal data and structure refinement for RERu4B4 (RE= Sm, Dy). 105 Crystal data and structure refinement for YbRu484. 106 Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (A2x 103) for RERu484 (RE = Y, Ce, Sm, Dy, Yb). 107 Anisotropic displacement parameters (A2x 103) for RERu4B4 (RE = Y, Ce, Sm, Dy, Yb). 108 Bond distances (A) for RERu4B4 (RE = Y, Ce, Sm, Dy, Yb). 109 Crystal data and structure refinement for MnGa4_65 and ReGa4,5. 130 Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for MnGaMs and ReGa4_5. 131 Anisotropic displacement parameters (Azx 103) for MnGa4+x and ReGa4+x. 132 Bond distances (A) for MnGa4,65 and ReGa4_5. 133 Crystal data and structure refinement for Nio,57Ga4,43. 134 Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Nio_57Ga4,43. 135 Anisotropic displacement parameters (Azx 103) for Nio,57Ga4,43. 135 xi Table 58 Bond distances (A) for Nio,57Ga4_43. 135 xii Figure 1-1. Figure 2-1 Figure 2-2. Figure 2-3. Figure 2-4. Figure 3-1. Figure 3-2. Figure 3-3. Figure 3-4. Figure 3-5. LIST OF FIGURES Various geometric arrangements of boron atoms in borides: (a) isolated atoms (B:M < 0.5), (b) isolated pairs (B:M z 0.67), (c) zigzag chain (B:M =1), ((1) double chain (B:M z 1.3), (e) tn'ple chain (B:M = 1.5), (f) two-dimensional network (2.0 S B:M S 2.5). 6 (a) Representation of CrsB3 along the b-axis (b) Boron pairs in CrsB3 (Cr atoms omitted for clarity). 39 Double and triple chains of boron atoms in (a) 0384 and (b) 0283, respectively. 40 (a) CrBz structure seen along c-axis (b) Planar-nature of boron layers in CrBz. 42 Structure of MB (M = M0, W) viewed down the b-axis 43 (a) Structure of CrB-type MnB with boron atom chains parallel to page. The boron atom chains are perpendicular to the page in (b) FeB-type MnB and (c) CrB-type MnB. 72 (a) The structure of MnB4 viewed down the a-axis (b) Sheet of RuBz with similarly puckered hexagonal sheets of B atoms. 73 (a) Structure of ReBz and (b) an individual graphite-like layer of boron atoms. 75 (a) Structure of YCrB4-type compounds (b) View down a-axis showing alternating layers of metal atoms and boron atoms. 76 SEM micrograph of a MnB4 crystal. 79 xiii Figure 3-6. Figure 3-7. Figure 3-8. Figure 4-1. Figure 4-2. Figure 4-3. Figure 4-4. Figure 4-5. Figure 4-6. Figure 5-1. Figure 5-2. Figure 5-3. Figure 5-4. Figure 5-5. Figure A-l. Figure A-2. SEM micrograph of a cluster of ReBz crystals. 79 SEM micrograph of HoMnB4. 81 SEM micrograph of DyReB4. 81 (a) Structure of Ru783 and (b) the stellaquadrangula building unit. 111 (a) Structure of Ru2B3 and the (b) puckered boron layer and (c) planar layer of boron atoms. 112 Structure of RuBz crystallizing with the (a) RuBz-type and (b) ReBz-type structures. 113 Structure of RERu4B4 (RE = Y, Ce, Sm, Dy, Yb) shown down the b-axis. . 115 SEM micrographs of (a) RuBz and (b) B-RuBz. 117 SEM micrographs of (a) CeRu484 and (b) CeRuB4. 119 Structure of MGa4+x (M = Mn, Re) viewed down the c-axis. 137 View down the c-axis of (a) MnGa45 and (b) PdGas. 138 Connectivity along the c-axis in (a) MGa4+x and (b) PdGas. 139 (a) Structure of Nio.57Ga4,43 and (b) the parent y-brass structure. 141 SEM micrographs of (a) MnGa4 and (b) ReGa4,5. 143 Cross-sectional view of (a) BN susceptor holder and Mo susceptor along (b) vertical and (0) horizontal axes. 153 General setup for RF furnace. 154 xiv CCD SEM EDS LIST OF ABBREVIATIONS Charge Coupled Device Scanning Electron Microscope Energy Dispersive Spectroscopy Radio Frequency XV CHAPTER ONE The Metal Flux Technique in Boride Synthesis A. Introduction The metal flux technique is an interesting alternative to traditional solid state synthesis techniques. Low melting point metals are used as a solvent in this technique to facilitate greater diffusion of the reagents and to aid in single crystal growth. The application of the flux technique to the synthesis of borides has had some success, but the potential seems to be much greater. An examination of the metal flux technique, basic boride structural features, and properties of note for borides is presented. B. The Metal Flux Technique Solid state synthesis ofien requires the use of high temperature equipment. Traditionally, high-temperature furnaces, arc welders, and radio frequency (RF) induction furnaces have been used to reach the elevated temperatures at which synthesis takes place. While working at elevated temperatures may be required for any reaction to take place, it can also be very limiting. A desired ternary phase may be inaccessible in a system of reagents because more thermodynamically stable binary phases are formed. Efforts to combat binary formation include frequent grinding and reheating of reagents, using less-stable binary or ternary phase starting materials, and using very long annealing steps in heating profiles.1 The metal flux technique is a practical alternative to the traditional solid state techniques. The metal flux technique makes use of a metal with a relatively low melting point, in which the reagents of interest have some solubility, to act as a solvent for the reaction. The melting point of the metal need only be low in relation to the other reagents in use. For instance, copper, with a melting point of 1092 °C has been used successfully as a flux for many different systems containing metals with higher melting points from the d- and f-blocks. The liquid metal flux acts as a solvent and often allows for greater diffusion of the reagents, which allows the reagents to react at temperatures well below their melting points. The lower reaction temperature allows crystals to grow with fewer defects, a boon when the crystals are going to be used in properties measurements.2 Another advantage to using a metal flux is that the fluxes can getter impurities from a reaction environment, allowing a clean environment for crystal growth.3 This advantage is easily overlooked, but ensures a critical oxygen-free environment. Generally flux reactions are run at lower temperatures, so the reactivity of the reagents with oxygen is already less than that found in traditional techniques. Because most flux reactions have a large excess of the flux metal, oxygen, or any other impurity, is much more likely to react with the flux metal than the intended reagents. Disadvantages do exist in the use of metal fluxes. At times, finding an appropriate metal in which the reagents are soluble can be difficult or impossible. Because the flux is soluble with so many materials there can be unexpected incorporation of reaction vessel materials into the reactions. We have found that tantalum and quartz tubes react too readily with gallium and copper and are destroyed by these fluxes. Yet, the most challenging part of using the flux may be in how to extract the reaction products from the solvent-like flux. These problems must be taken into consideration when attempting a new molten metal flux synthesis. Our group has implemented the metal flux in exploratory synthesis for many multinary systems. Many new alumindesf’ 5 silicidesf’ 7 and germanidess’ 9 were found, which led to interest in extending the technique to systems including boron. Initial successes included the synthesis of a new binary phase, [3-SiB3,lo and a series of quaternary phases, REL3CZSig(B12)3 (RE= Y, Tb, Er).ll Further inspection of the literature showed that metal fluxes have been used successfully for the synthesis and growth of quite a few borides.”23 The first reports of growth of borides from molten metals dealt with mixtures of iron and aluminum as the flux metals.12 Iron melts near 1500 °C, but aluminum melts at only 660 °C, and boils near 2500 °C, which allows researchers a very large, and easily attainable, temperature range in which to carry out experiments. Using aluminum as the flux metal also allows the use of more accessible oxide starting reagents because the aluminum can reduce the oxides to elemental reagents while in the flux.13 The advantage of using these oxides is that the preparation for synthesis can be done out on a bench top, rather than inside a glovebox. These advantages made aluminum the flux metal of choice for borides. It has produced crystals of many different borides, ranging from simple 14-17 18 binary borides to temaries that include aluminum. One of the main problems with using aluminum as the flux metal is that it makes stable binaries, not only with many metals, but also with boron. Aluminum diboride is a common side product in flux reactions, and we have found at least three different aluminum dodecaborides that form from reactions rich in aluminum and boron. There have been no reports of true ternary borides grown from an aluminum flux that do not include aluminum in the structure. To make temaries that do not incorporate aluminum, other metals must be used as the flux. Copper has been used with some success in the flux growth of binary crystals in the Nb—B19 and W—B20 systems. In the last decade the use of a copper flux was extended to ternary RE—Rh—BZland RE—B—C22 systems and quaternary RE—Rh—B—C23 and RE—B— C—sz systems. An advantage to using copper over aluminum is that there are no known Cu—B binaries to inhibit other borides from forming. Disadvantages to using copper include its high melting temperature (1092 °C) and the inability to use oxides as reagents. Our group has found gallium to be a useful flux metal in the synthesis of RE—B— Si—C and Si—B compounds. After having difficulty isolating aluminum-free ternary silicides from an aluminum flux, our group moved to gallium and found that gallium stayed out of the ternary phases. Seeing that aluminum was also incorporated into many borides, we again moved to gallium thinking results similar to those found with silicides could follow. A new binary phase, [3-SiB3,10 and series of quaternary phases, RE|_3C2SIs(Blz)3 (RE= Y, Tb, Er),ll showed the thinking to be correct and provided a basis for a closer examination into the use of a gallium flux for the synthesis of multinary borides. Gallium has several characteristics that make it an interesting flux metal. As in aluminum, there is a very large difference between the melting (29 °C) and boiling points (2400 °C) of gallium, so there is seemingly a large range for reaction temperatures. However, boron has a very low solubility in gallium below about lOOO°C. Thus, potential components in multinary borides can form stable non-boride phases that crash out of the reaction mixture before boron has even had a chance to react. By working at 1000 °C and above we looked to determine the applicability of the gallium flux in the synthesis of a wider range of borides. If successful, this synthesis technique could prove its usefulness by providing larger, better-formed crystals than those previously made, allowing for better property analyses. In addition, the unique chemistry of boron, which is responsible for the great diversity of known borides, could be extended to previously unknown phases. C. Structural Features in Borides Borides are a large and diverse class of compounds. This diversity is readily seen in the geometric arrangement of the boron atoms in borides, shown in Figure 1-1, which varies based on the ratio of boron to metal atoms found in the compound.” 25 In metal- rich borides, in which the boron-to-metal ratio (B:M) is less than 0.5, the boron atoms are isolated from each other, as shown in Figure l-la, and only metal-metal or metal-boron bonds are formed. When more boron is incorporated into the structure, increasing B:M to approximately 0.67, boron-boron bonds begin to form, resulting in isolated boron pairs , as shown in Figure 1-1b. A further increase in B:M to 1.0 allows the isolated boron pairs to link together and form the zigzag boron atom chain shown in Figure 1-1c. These chains will link together as more boron is added, resulting in double chains (Figure 1-1d) for B:M near 1.3, and triple chains (Figure 1-1e) for B:M around 1.5. Two-dimensional networks are formed when B:M increases to between 2.0 and 2.5. These networks most commonly comprise six-membered rings of boron atoms, as shown in Figure l-lf, (a) (b) (0 Figure 1-1. Various geometric arrangements of boron atoms in borides: (a) isolated atoms (B:M < 0.5), (b) isolated pairs (B:M z 0.67), (c) zigzag chain (B:M =1), ((1) double chain [3:954 2'- 1.3), (e) triple chain (B:M = 1.5), (f) two-dimensional network (2.0 S B:M S 2.5). ‘ however, rings with five and seven boron atoms are also well known.”28 Boron-rich compounds, with B:M values greater than 2.5, contain three-dimensional networks of boron atoms. The most common polyhedra formed by the boron atoms are octahedra, icosahedra, and cubo—octahedra. The rich structural variety of borides is even more impressive when compared to that found in carbides and nitrides. Both carbides and nitrides have limited structural variety due in part to geometric factors.29 One such geometric factor is based on Hagg’s rule, which states that interstitial compounds with a ratio of nonmetal to metal radii less than 0.59 will adopt a simple structure, such as body-centered cubic, face-centered cubic, hexagonal close-packed, or hexagonal. Because carbon and nitrogen atoms have rather small radii compared to most metals, they can occupy the octahedral holes between metal atoms, creating simple structures, as predicted by Hagg. Boron atoms tend to be larger, exceeding Hagg’s 0.59-ratio rule, and prefer a trigonal prismatic coordination environment. The trigonal prismatic coordination environment and larger atom sizes bring boron atoms within bonding distance to each other, leading to the pairs, chains, etc. that are present throughout boride structural chemistry.24 D. Chemical and Physical Properties of Borides Accompanying the structural diversity in borides is an equally wide diversity of chemical and physical properties. Many borides have a great deal of chemical stability. Nowhere is this stability more evident than when borides are separated from a molten metal flux. To remove products from a copper flux, for instance, the ingot containing the now-solid flux and products is placed into an etching solution, a bath of nitric acid. Regardless of concentration, the acid has little effect on the boride crystals, but completely removes the copper. Similar results are seen in aluminum flux reactions, where the etching solution can be either hydrochloric acid or sodium hydroxide. Again, minimal damage is done to the boride crystals while completely removing the metal. In cases where the boride crystals must be dissolved, warm or boiling aqua regia is used because the dissolution is often too slow at room temperature, leaving the boride crystals intact and unharmed.10 The strong covalent bonding in borides leads to great thermal stability. This stability allows borides to be used in many high temperature applications, such as thermoelectric conversion materials.”32 Promising results have been found for boron- rich borides, and an entire thermoelectric device was recently made consisting entirely of boron-rich components.33 The current results on boride thermoelectric components are not optimized yet, so future work in this area looks to maximize effectiveness of these devices in harsh environments where other systems fail. Borides have consistently found use in harsh industrial applications because they are hard and incompressible materials. The hardness of the compounds comes from the directional covalent bonds in borides, while the incompressibility is due to electrostatic repulsion between atoms and can be correlated with the valence electron density of the compounds.34 The advantage of borides over more traditional industrial products is made apparent in their application in the cutting of iron-based metals. Boride coated tools are used instead of diamonds, which have superior hardness, but also react chemically with the iron in the metal.35 The added chemical and thermal stability of borides give them potential for many industrial applications. Superconductivity is not exactly a rare property for a boride to exhibit. However, when the critical transition temperature (Tc) associated with that superconductivity is 39 K, as in magnesium diboride,36 it is something of which to take note. Magnesium diboride had been prepared and its structure known for nearly fifiy years before it was tested for superconductivity. The T0 of 39 K is the highest known for a bulk sample outside of the copper oxides, and led to a flurry of research in borides in recent years. Our group is included in that flurry and we hope that the molten metal flux technique can help isolate a boride with an even high Tc. References 1. Prokhorov, A. M.; Lyakishev, N. P.; Burkhanov, G. S.; Dement'ev, V. A., High Purity Transition-Metal Borides: Promising Materials for Present Day Technology. Inorganic Materials 1996, 32, (11), 1195-1201. 2. Kanatzidis, M. G.; Pottgen, R.; Jeitschko, W., The Metal Flux- A Preparative Tool for Intermetallic Compounds. Angewandte Chemie International Edition 2005, 44, (43), 6996-7023. 3. Fisk, Z.; Remeika, J. P., Growth of Single Crystals from Molten Metal Fluxes. In Handbook on the Physics and Chemistry of the Rare Earths; K.A. Gschneidner, J .; Eyring, L.,Eds. Elsevier Science: 1989; Vol. 12, pp 53-70. 4. Latturner, S.; Kanatzidis, M. G., Formation of Multinary Intermetallics from Reduction of Perovskites by Aluminum Flux--M3Au6+xA126Ti (M = Ca, Sr, Yb), a Stuffed Variant of the BaHgn Type. Inorganic Chemistry 2004, 43, 2-4. 5. Latturner, S. E.; Bilc, D.; Ireland, J. R.; Kannewurf, C. R.; S.D.Mahanti; Kanatzidis, M. G., REAu3A17 (RE = rare earth): New Ternary Alumindes Grown from Aluminum Flux. Journal of Solid State Chemistry 2003, 170, (1 ), 48-57. 6. Latturner, S.; Kanatzidis, M. G., REAu4A13Si: The End Member of a New Homologous Series of Intermetallics Featuring Thick AuA12 layers. Chemical Communications 2003, (18), 2340-2341. 7. Salvador, J. R.; Malliakas, C.; Gour, J. R.; Kanatzidis, M. G., RE5C04Si14 (RE= Ho, Er, Tm, Yb): Silicides Grown from Ga Flux Showing Exceptional Resistance to Chemical and Thermal Attack. Chemistry of Materials 2005, 17, 1636-1645. 8. Wu, X.; Bilc, D.; Mahanti, S. D.; Kanatzidis, M. G., VzAlsGes: First Ternary Intermetallic in the V-Al-Ge System Accessible in Liquid Aluminum. Chemical Communications 2004, 1506-1507. 9. Wu, X.; Kanatzidis, M. G., REAuAl4Ge2 and REAuAl4(AuxGe1-x)2 (RE= rare earth element): Quaternary Intermetallics Grown in Liquid Aluminum. Journal of Solid State Chemistry 2005, 178, 3233-3242. 10. Salvador, J. R.; Bilc, D.; S.D.Mahanti; Kanatzidis, M. G., Stabilization of B-SiB3 from Liquid Ga: A Boron-Rich Binary Semiconductor Resistant to High-Temperature Air Oxidation. Angewandte Chemie International Edition 2003, 42, 1929-1932. 11. Salvador, J. R.; Bilc, D.; S.D.Mahanti; Kanatzidis, M. G., Gallium Flux Synthesis of Tb3-xC2Si3(B|2)3: A Novel Quaternary Boron-Rich Phase Containing B12 Icosahedra. Angewandte Chemie International Edition 2002, 41, (5), 844-846. 10 12. Bernard, A. US. Patent 3096149, 1963. 13. Okada, S.; Tanaka, T.; Leithe-Jasper, A.; Michiue, Y.; Gurin, V. N., Crystal Growth and Structure Analysis of a New Scandium Aluminum Boride SCZA1B6. Journal of Solid State Chemistry 2000, 154, 49-53. 14. Okada, S.; Atoda, T.; Higashi, 1., Structural Investigation of 028;, 033,, and CrB by Single-Crystal Diffractometry. Journal of Solid State Chemistry 1987, 68, 61-67. 15. Okada, S.; Atoda, T.; Higashi, 1.; Takahashi, Y., Preparation of Single Crystals of M08; by the Aluminum-flux Technique and Some of Their Properties. Journal of Materials Science 1987, 22, 2993-2999. 16. Okada, S.; Hamano, K.; Higashi, 1.; Lundstrom, T.; Tergenius, L.-E., Preparation of Single Crystals of a New Compound, Ta586 by the Aluminum Flux Method. Bulletin of the Chemical Society of Japan 1990, 63, 687-691. 17. Higashi, I.; Takahashi, Y.; Atoda, T., Crystal Growth of Borides and Carbides of Transition Metals from Molten Aluminum Solutions. Journal of Crystal Growth 1976, 33, 207-211. 18. Becher, H. J .; Krogmann, K.; Peisker, E., Uber das ternare Borid anAle. Zeitschriftfu’r anorganische und allgemeine Chemie 2004, 344, (3-4), 140-147. 19. Okada, S.; Hamano, K.; Lundstrom, T.; Higashi, I. In Crystal Growth of the New Compound Nb 23 3, and the Borides NbB, Nb 586, Nb 334, and Nsz, Using the Copper-Flux Method, Boron-Rich Solids, Albuquerque, New Mexico, 1986; Emin, D.; Aselagc, T.; Beckel, C. L.; Howard, 1. A.; Wood, C., Eds. American Institute of Physics: Albuquerque, New Mexico, 1985; pp. 456-459. 20. Okada, S.; Kudou, K.; Lundstrom, T., Preparations and Some Properties of W28, 8- WB, and WB; Crystals from High-Temperature Metal Solutions. Japanese Journal of Applied Physics 1995, 34, (1), 226-231. 21. Shishido, T.; Ye, J .; Sasaki, T.; Note, R.; Obara, K.; Takahashi, T.; Matsumoto, T.; F ukuda, T., Growth of Single Crystals in the Systems with R-Rh-B and R-Rh-B-C (R= Rare Earth Element) from Molten Copper Flux. Journal of Solid State Chemistry 1997, 133, 82-87. 22. Zhang, F. X.; Tanaka, T., Single Crystal Growth of Some Rare-Earth Boron-Rich Compounds in RE-B-C(N) and RE-B-Si Systems. Journal of Crystal Growth 2004, 271, p 159-164. 23. Ye, J .; Shishido, T.; Kimura, T.; Matsumoto, T.; F ukuda, T., End Member of the Rhodium-Based Quaternary Borocarbides, ErhaBzC. Acta Crystallographica 1998, C54, 1211-1214. 11 24. Etoumeau, J .; Hagenmuller, P., Structure and Physical Features of the Rare-Earth Borides. Philosphical Magazine B 1985, 52, (3), 589-610. 25. Lundstrom, T., Structure, Defects and Properties of Some Refractory Borides. Pure and Applied Chemistry 1985, 57, (10), 1383-1390. 26. Rogl, P., New Ternary Borides with YCrB4-type Structure. Materials Research Bulletin 1978, 13, 519-523. 27. Kuz'ma., Y. B., Crystal Structure of the compound YCrB4 and its analogs. Kristallografiya 1970, 15, 372-374. 28. Sobczak, R.; Rogl, P., Magnetic Behavior of New Ternary Metal Borides with YCrB4-type Structure. Journal of Solid State Chemistry 1979, 27, 343-348. 29. Chen, J. G., Carbide and Nitride Overlayers on Early Transition Metal Surfaces: Preparation, Characterization, and Reactivities. Chemical Reviews 1996, 96, 1447-1498. 30. Mori, T., High Temperature Thermoelectric properties of Ba Icosahedral Cluster- containing Rare Earth Boride Crystals. Journal of Applied Physics 2005, 97, 093703. 31. Nakayama, T.; Shimizu, J .; Kimura, K., Thermoelectric Properties of Metal-Doped B-Rhombohedral Boron. Journal of Solid State Chemistry 2000, 154, 13-19. 32. Imai, Y.; Mukaida, M.; Ueda, M.; Watanabe, A., Screening of the Possible Boron- based n-type thermoelectric conversion materials on the basis of the calculated densities of states of metal borides and doped B-boron. Intermetallics 2001, 9, 721-734. 33. Takeda, M.; Kurita, Y.; Yokoyama, K.; Miura, T. In Synthesis and High Temperature Thermoelectric Properties of Alkaline-Earth Metal Hexaborides MB6 (M=Ca,Sr, Ba), 2003 MRS Fall Meeting, Boston, MA. 34. Cumberland, R. W.; Weinberger, M. B.; Gilman, J. J.; Clark, S. M.; Tolbert, S. H.; Kaner, R. B., Osmium Diboride, An Ultra-Incompressible, Hard Material. Journal of the American Chemical Society 2005, 127, 7264-7265. 35. Gao, F.; Hou, L.; He, Y., Origin of Superhardness in Icosahedral B12 Materials. Journal of Physical Chemistry B 2004, 108, 13069-13073. 36. Nagamatsu, J .; Nakagawa, N.; Muranaka, T.; Zenitani, Y.; Akimitsu, J ., Superconductivity at 39K in Magnesium Diboride. Nature 2001, 410, 63-64. 12 CHAPTER TWO The Metal Flux Synthesis of Group Six Borides A. Introduction The group 6 elements form a very interesting series of binary borides. Chromium borides seem to vary in structure based on B:M ratio, as outlined earlier in this work. The boron atoms in these borides go from isolated atoms to isolated pairs, pairs to chains, chains to double chains, double chains to triple chains, triple chains to 2-D networks, and 2—D to 3-D networks with increasing B:M ratios. Molybdenum and tungsten borides follow most of the structural patterns according to B:M ratios. However, no molybdenum or tungsten borides with B:M ratios of 1.5 or 1.67 have been isolated. Interestingly, there are more borides with B:M 2 2.0 for molybdenum and tungsten than there are for chromium. Slight variations in the B:M ratios above 2.0 lead to various 2-D and 3-D boron networks for the molybdenum and tungsten borides. MoB2.,,,l Mongg,2 Mol.,,B3,3 WBz,4 and W2B52 all have layers with planar hexagonal boron rings. MozBs and W2B5 also have layers with puckered hexagonal boron rings. The structures of MoBz.x , WBz, MoB4, and WB., all have a common feature: planar layers of boron hexagons. However, in the tetraborides, these layers are linked to form a 3-D network. Pairs of boron atoms replace one-third of the molybdenum or tungsten atoms in the metal atom layers of the diboride structures, linking the boron atoms of the tetraboride structure into a 3-D networks 13 Further interest into group 6 borides came from previous results with the molten metal flux technique. A Japanese group of researchers has used aluminum as the flux metal for the synthesis of borides.“9 Initially, W2B5 was the only binary boride to grow from the flux reactions.6 Ternary phases incorporating aluminum were found in both the chromium and molybdenum systems, but no binary group 6 borides were found. Over a decade later, the same group reported that they could grow binary crystals in both the chromium—boron7 and molybdenum—boron8 systems by introducing a slow-cooling step into the heating profile following the soak at maximum temperature. Nearly twenty years after the initial research into the tungsten-boron system, two other W—B binaries, W2B and WB, were grown in molten aluminum.9 Also in the new article was the report of copper flux synthesis of W2B and WB in single-crystalline form. Armed with the knowledge that both aluminum and copper had worked as fluxes for group 6 boride syntheses, we wanted to see if we could extend the technique to include gallium as a flux metal. Extending the use of a copper flux to chromium and molybdenum borides was also of interest because of its success in forming tungsten borides. No ternary group 6 borides synthesized from a molten metal flux have been reported (excluding the aluminum-containing borides). Thus, the chance to apply the flux technique to synthesize ternary compounds was also an exciting possibility. Our initial gallium flux reactions targeted multinary group 6 borides, such as YbCr(Si,B)4, YM03B2, and NinBls. Despite many attempts targeting various ternary and quaternary borides, the only borides formed where binary phases. Copper flux reactions had similar results. While not giving up on our goal of synthesizing ternary borides from a metal flux, we did shift focus slightly, and started targeting binary borides l4 that had formed out of the multinary systems. In this chapter we describe the synthesis and structural characterization of binary borides synthesized using gallium and/or copper fluxes. B. Experimental Reagents: All reagents were used as received without further purification: (i) Boron metal, 99% purity, -325 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (ii) Chromium metal, 99.95% purity, -200 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (iii) Molybdenum metal, 99.9% purity, Cerac Specialty Inorganics, Milwaukee, WI, (iv) Tungsten metal, 99.9% purity, Cerac Specialty Inorganics, Milwaukee, WI, (v) Gallium 3-5 mm shot, 99.999% purity, Plasmaterials, Liverrnore, CA, (vi) Copper metal cuttings, Mallinckrodt Specialty Chemicals Co., Paris, KY, (vii) Dysprosium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (viii) Yttrium metal, 99.9% purity, -40 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (ix) Nickel metal powder, 98-99% purity, -325 mesh, E.H. Sargent & Company. Fumaces: Commercial tube furnaces from Applied Test Systems, Inc. were used to heat reactions sealed in quartz tubes. Furnace controllers from the Omega Company were used to program heating profiles for individual reactions. Furnace temperatures were monitored during reactions by thermocouples connected to the Omega controllers. To extend the life of the furnaces, the operating temperature for prolonged heating was limited to 1000 °C. 15 A commercial, hi gh-temperature, vertical tube furnace, with controller, from the Mellen Company was used for copper flux reactions. Heating profiles for individual reactions were programmed into the furnace controller. Thermocouples connected to the furnace controller were used to monitor furnace temperatures during reactions. To extend the life of the furnace, the operating temperature for prolonged heating was limited to 1350 °C. A Lindberg Blue hi gh-temperature, horizontal tube furnace was used for gallium and copper flux reactions. Heating profiles for individual reactions were programmed into the accompanying Lindberg UPISO furnace controller. Thermocouples connected to the furnace controller were used to monitor furnace temperatures during reactions. The maximum operating temperature for the furnace was 1500 °C. A radio frequency (RF) furnace was constructed from an Ameritherm XP7.5CE Induction Heater and fused quartz reaction chamber. A molybdenum cylinder, machined to act as a reaction crucible holder, was used as a susceptor. A boron nitride cylinder was machined to hold the molybdenum crucible in the center of the reaction chamber. Details on the RF furnace setup are given in the appendix of this work. RF furnace temperatures were controlled manually using the Ameritherm control unit. Reaction temperatures were monitored using an Ircon SA Series Infrared Thermometer. During the course of some reactions, films deposited inside the reaction chamber would prevent the IR thermometer from accurately reporting furnace temperatures. In such circumstances, reaction temperatures were approximated based on power settings for the Ameritherm control unit and a series of calibration runs conducted 16 by heating only the molybdenum cylinder. Temperatures greater than 1700 0C were easily reached with this furnace. Synthesis and Isolation: Cr5B3: Boron (2 mmol) and chromium (2 mmol) powders were mixed and added to an alumina crucible, along with dysprosium filings (1 mmol). Pieces of copper totaling 2.54 g (40 mmol) were then placed in the crucible. After the addition of a loose-fitting alumina lid, the crucible was placed in the RF furnace. The RF furnace was evacuated under vacuum to a pressure near 10'3 Torr and flushed with nitrogen. Heating was initiated with the system under vacuum. The temperature was raised to 1400 °C in approximately 25 minutes and then held at that temperature for 2 hours, at which time the power to the furnace was shut off and the furnace was allowed to cool to room temperature. After cooling, the crucible was removed from the furnace and placed into a bath of half-concentrated I'INO3. The etching solution entered the crucible through the loose- fitting lid. An overnight soak was used to completely remove the copper flux, however, many product crystals were removed from the flux after a 3- to 4-hour soak. Extended soaking in the bath was not found to damage the crystals. Silver, plate-like crystals were isolated in an estimated 20-30% percent yield based on chromium. Elemental analysis performed by EDS showed that chromium and boron were the only elements present in the plate-like crystals. The remainder of the collected product comprised elemental chromium and traces of DyB6. Cr3B4: Boron (4 mmol) and chromium (1 mmol) powders were mixed and added to an alumina crucible. Pieces of copper totaling 2.0 g were then placed in the crucible. l7 The crucible was suspended in a high-temperature tube furnace and heated under a slow flow of argon. The furnace was heated to 1300 °C in 13 hours and held at that temperature for 10 hours, at which point the power to the furnace was shut off and the furnace was allowed to cool to room temperature. After cooling, the crucible was removed from the furnace and placed into a bath of half-concentrated I'INO3 in order to remove the copper flux. An overnight soak was used to completely remove the copper flux, however, many crystals were removed from the flux after a 3- to 4-hour soak. Extended soaking in the bath was not found to damage the crystals. Silver, plate-like crystals were isolated in approximately 20 to 40% yields based on chromium. The remainder of the collected product comprised Cr2B3, CrBz, and elemental chromium. Cr2B3: Boron (2 mmol) and chromium (1 mmol) powders were mixed and added to an alumina crucible. Pieces of gallium shot totaling 1.6 g were then placed in the crucible. The alumina crucible was then placed in 13 mm diameter quartz tube, evacuated under vacuum to a pressure near 104 Torr, and then sealed using an oxygen- acetylene torch. The quartz tube was then heated in a commercial tube furnace under a heating profile that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 96 hours, and then allowed the furnace to cool to room temperature. After cooling, the quartz tube was opened and the alumina crucible was placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed after an overnight soak, but longer soaks can be used without damage to the recovered product. Silver needle-shaped crystals were isolated in approximately 40 to 18 60% yields based on chromium. The remainder of the product comprised CrBz and elemental chromium. CrBz: Boron (10 mmol) and chromium (1 mmol) powders were mixed and added to a glassy carbon crucible, along with yttrium (1 mmol). Pieces of gallium shot totaling 2.0 g were then placed in the crucible. The crucible was placed in the RF furnace, evacuated under vacuum to a pressure near 10'3 Torr, and flushed with argon. Heating was initiated under vacuum and the temperature was raised to 1300 °C in ten minutes. After holding at that temperature for 45 minutes, the power to the furnace was shutoff, and the furnace was allowed to cool to room temperature. After cooling, the crucible was removed from the furnace and placed into a bath of 3M 12 in DMF in order to remove the gallium flux. An overnight soak was found to be insufficient for removing all of the gallium, so soaking was continued for an additional 3 days. Extended soaking in the bath was not found to damage the crystals. Silver, hexagonal plate-like crystals were isolated in an estimated 30 to 40% yield based on chromium. Elemental analysis performed by EDS showed that chromium and boron were the only elements present in these crystals. MoB: Boron (3 mmol), molybdenum (1 mmol), and yttrium (0.3 mmol) were added to a graphite crucible. Pieces of gallium shot totaling 1.6 g were then added, along with a loose-fitting graphite cap, and the crucible was placed in the RF furnace. The RF furnace was evacuated under vacuum to a pressure near 10'3 Torr and flushed with argon. Heating was initiated with the system under vacuum. The temperature was raised to 1300 0C in approximately 15 minutes and then held at that temperature for 15 minutes, at 19 which time insufficient cooling water flow shut off the power to the furnace. The furnace then cooled to room temperature. After cooling, the crucible was placed in a bath of 3 M12 in DMF in order to remove the remaining gallium flux. An overnight soak was found to be insufficient for removing all of the gallium, so soaking continued for an additional 2 days. Extended soaking in the bath was not found to damage the crystals. Silver, plate-like crystals were a minor product (estimated 10 to 20% yield based on molybdenum). Purple powder and crystals of YB6 were present in 20-30% yields based on yttrium. The remainder of the product collected comprised unreacted boron powder and traces of YB6. WB: Boron (7.5 mmol), nickel (0.5 mmol), and tungsten (1 mmol) powders were mixed and added to an alumina crucible along with pieces of gallium shot totaling 1.45 g. A quartz filter was placed in the crucible which was then placed in 13mm diameter quartz tube, evacuated under vacuum to a pressure near 104 Torr, and sealed using an oxygen- acetylene torch. The tube was then heated in a commercial tube furnace under a heating profile that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to 250 0C in 60 hours. The quartz tube was removed from the furnace at 250 °C and centrifuged to remove excess gallium. After centrifugation, the tube was opened and the crucible was placed in a bath of 5 M 12in DMF in order to remove the remaining gallium flux. An overnight soak was found to be insufficient for removing all of the gallium, so soaking continued for an additional 2 days. Extended soaking in the bath was not found to 20 damage the crystals. Silver, prismatic crystals were a minor product (estimated 10-20% yield based on tungsten). Hexagonal plates of Ni2Ga3 were the major product, while rectangular prismatic crystals of NiGa4 were also a minor product (IO-20% yield based on nickel). The remainder of the product collected was unreacted boron powder and traces of a tungsten-gallium phase. C. Physical Measurements Energy Dispersive Spectroscopy: Energy dispersive spectroscopy (EDS) analyses were carried out on selected crystals to determine their chemical composition. The analyses were performed with a JEOL J SM-6400 scanning electron microscope (SEM) equipped with Noran Vantage Energy Dispersive Spectroscopy (SizLi) detector and Norvar window for standardless quantization of elements with Z Z 4. The crystals were affixed to an alumina sample holder with double-sided carbon tape. The EDS data were acquired at an accelerating voltage of 10kV with a 30 to 60 second accumulation time. Single-Crystal X-ray Crystallography: Single crystals were mounted on a glass fiber with super glue and their intensity data were collected on either a Bruker SMART platform CCD diffractometer, or a STOE IPDS H diffractometer using Mo K0: radiation at 50 kV and 40 mA. Individual frames of Cr3B4 and WB examined with the Bruker machine were collected with a 03° (1) rotation. The SMART software was used for data collection, and SAINTlo software was used for data extraction and reduction. After applying analytical 21 absorption corrections, structure solution and refinement were completed using direct methods and the SHELXTLll suite of programs. Samples examined with the STOE (Cr5B3, Cr2B3, CrB2, and MoB) had individual frames collected on a 34 cm image plate with a 60 second exposure time and a 10° a) rotation. The X-SHAPE'2 and X-RED-32l3 software packages were used for data extraction and reduction and to apply an analytical absorption correction. Direct methods and the SHELXTL suite were used to solve and refine the structures. The crystal structure refinement data for 0ng are listed in Table 2-1. Atomic parameters found in the previous structure report'4 were used as a starting point for structural refinement. The atomic positions and isotropic displacement parameters are listed in Table 2-2. Anisotropic displacement parameters for the chromium and boron atoms are found in Table 2-3. The bond distances, listed in Table 2-4, match well with those calculated from previous reports. The crystal structure refinement data for 033, are listed in Table 2-5. Atomic parameters found in previous structure reports7'15 were used as a starting point for structural refinement. The atomic positions and isotropic displacement parameters are listed in Table 2-6. Anisotropic displacement parameters for the chromium and boron atoms are found in Table 2-7. The bond distances, listed in Table 2-8, match well with those found in previous reports. The crystal structure refinement data for Cr2B3 are listed in Table 2-9. The atomic positions and isotropic displacement parameters are listed in Table 2-10. Anisotropic displacement parameters for the chromium and boron atoms are found in Table 2-11. 22 The bond distances, listed in Table 2—12, match well with those calculated from the previous report on the structure.7 The crystal structure refinement data for CrB2 are listed in Table 2-13. The atomic positions and isotropic displacement parameters are listed in Table 2-14. Anisotropic displacement parameters for the chromium and boron atoms are found in Table 2-15. The bond distances are listed in Table 2-16. The crystal structure refinement data for MoB and WB are listed in Table 2-17. Atomic parameters found for MoB were used as a starting point for structural refinement of WB. The atomic positions and isotropic displacement parameters for both compounds are listed in Table 2-18. Anisotropic displacement parameters for the all of the atoms are found in Table 2-19. The structure of WB needs further refinement to pinpoint the location of the boron atom. The anisotropic displacement parameters for this atom are quite large and would be reduced with a more accurate atom location. Additional work with absorption correction for the crystal can also help reduce the anisotropic values. The bond distances for MoB and WB, listed in Table 2-20 and Table 2-21, respectively, match well with those calculated from the previous report.2 23 Table 2-1. Crystal data and structure refinement for Cr5B3. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 36.70° Refinement method Data / restraints / parameters Goodness-of-fit on 13'2 Final R indices [I>2sigma(1)] R indices (all data) Extinction coefficient 292.43 293(2) K 0.71073 A Tetragonal I4/mcm a = 5.4334(8) A a: 90° b = 5.4334(8) A B= 90° c = 10.031(2) A y = 90° 296.14(9) A3 4 6.559 g/cm3 17.451 mm‘1 540 0.098 x 0.080 x 0.035 mm3 4.06 to 36.70° -9Sh_<_9,-8_<_k58,-1651516 2235 220 [R(int) = 0.0994] 99.1 % Full-matrix least-squares on F2 220 / 0/ 16 1.098 R1: 0.0618, wR2 = 0.1592 R1 = 0.0698, wR2 = 0.1661 0.026(7) R1 = 2 ”Fa! - IFcII / 2 IE)! and wR2 = {Z (IF.2 - FRI )2 / z (wF.2)21”2 24 Table 2-2. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Cr5B3. x y 2 U(GQ) Cr(l) 3285(1) 1715(1) 1459(1) 7(1) Cr(2) 0 O 0 7(1) B(1) 0 0 2500 8(2) B(2) -1161(12) -3839(12) 0 4(1) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. Table 2-3. Anisotropic displacement parameters (Azx 103) for Cr5B3. ull U22 u33 u23 [113 ul2 Cr(l) 7(1) 7(1) 6(1) 0(1) 0(1) 0(1) Cr(2) 6(1) 6(1) 7(1) 0 0 0 B(l) 8(3) 8(3) 7(4) 0 0 0 B(2) 5(2) 5(2) 3(3) 0 0 -3(3) The anisotropic displacement factor exponent takes the form: -21t2[ h2 3*2U11 + +2hka*b*U12] 25 Table 2-4. Bond distances (A) for Cr5B3. Crl B2 2x 2.1621(3) Crl B2 1x 2.1916(2) Crl B1 2x 2.2684(2) Crl CR1 1x 2.4127(4) Crl Cr2 2x 2.4892(3) Cr2 B2 4x 2.1786(3) Cr2 Crl 8x 2.4892(3) B l Crl 8x 2.2684(2) 82 B2 1x 1.7865(2) B2 Crl 4x 2.1621(3) B2 Cr2 2x 2.1786(3) B2 Crl 2x 2.1916(2) 26 Table 2-5. Crystal data and structure refinement for Cr3B4. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 29.05° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2$igma(l)] R indices (all data) Extinction coefficient 199.24 293(2) K 0.71073 A Orthorhombic Immm a = 2.9550(10)A a: 900 b = 2.9823(10) A 8: 90° c = 13.030(4) A y = 90° 114.83(7) A3 2 5.762 g/cm3 13.527 mm‘1 184 3.14 to 28.21° -3ShS3,-3Sks3,-l6£ls 16 689 102 [R(int) = 0.0176] 100.0 % Full-matrix least-squares on F2 102/0/17 1.072 R1 = 0.0145, wR2 = 0.0338 R1 = 0.0183, wR2 = 0.0371 0.0031(5) R1 = z IlFoI - IE“ I z IE1 and wR2 = 12 (11:3 — p.21 )2 7 z (”(3)2110 27 Table 2-6. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Cr3B4. x y 2 U(eq) Cl‘( 1) 0 0 0 2( 1) Cr(2) -5000 0 -1862(1) 2(1) 3(1) -5000 -5000 -668(3) 3(1) B(2) 5000 -5000 - 1393(3) 4(1) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. Table 2-7. Anisotropic displacement parameters (Azx 103) for Cr3B4. ull u22 1133 U23 ul3 ul2 Cr(l) 2(1) 3(1) 1(1) 0 0 O Cr(2) 1(1) 3(1) 2(1) 0 0 0 B(l) 0(2) 5(2) 4(2) 0 O 0 B(2) 5(2) 1(2) 5(2) 0 0 O The anisotropic displacement factor exponent takes the form: -27t2[ h2 a"‘2Ull + +2hka*b*U12] 28 Table 2-8. Bond distances (A) for Cr3B4. Crl 82 8x 2.2699(3) Crl B1 4x 2.3353(3) Cr2 B2 2x 2.1410(3) Cr2 B1 4x 2.1824(3) Cr2 B1 1x 2.2707(5) B1 B2 2x 1.7381(3) B1 Cr2 4x 2.1824(3) B l Cr2 1x 2.2707(5) Bl Crl 2x 2.3353(3) B2 B1 2x 1.7381(3) 82 B2 1x 1.7561(4) B2 Cr2 2x 2.1410(3) B2 Crl 4x 2.2699(3) 29 Table 2-9. Crystal data and structure refinement for Cr2B3. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 29.13° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2sigma(1)] R indices (all data) Extinction coefficient 136.43 293(2) K 0.71073 A Orthorhombic Cmcm a = 3.0059(6) A a: 90° b = 18.084(4) A [3: 90° c = 2.9436(6) A y = 90° 160.01(6) A3 4 5.663 g/cm3 12.949 mm-1 252 2.25 to 29.13° 45hs4,-245ks24,-45153 737 145 [R(int) = 0.0286] 98.6 % Full-matrix least-squares on F2 145/0/22 1.257 R1 = 0.0316, wR2 = 0.0503 R1 = 0.0320, wR2 = 0.0503 0.066(6) R1 = z ||F0| — |F.|| / z |F0| and wR2 = [z (|F.,2 — F.2l )2 / Z (wFo2)2]“2 30 Table 2-10. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Cr2B3. x y z U(eq) Cr( 1) 0 4276(1) 2500 2(1) Cr(2) 0 7036(1) 2500 2(1) B( l) 0 8280(5) 2500 5(2) B(2) 0 1 191(5) 2500 4(2) B(3) 0 235(5) 2500 3(2) U(eq) is defined as one third of the trace of the orthogonalized UiJ' tensor. Table 2-11. Anisotropic displacement parameters (Azx 103) for Cr2B3. ull {)2 [)33 [)23 ul3 U12 Cr(l) 4(1) 1(1) 2(1) 0 0 0 Cr(2) 2(1) 1(1) 2(1) 0 0 0 B(2) 0(5) 4(4) 8(5) 0 0 O B(3) 3(5) 2(4) 4(4) 0 0 O B(l) 8(6) 6(4) 2(4) 0 0 0 The anisotropic displacement factor exponent takes the form: ~27t2[ h2 a"‘2Ull + +2hka*b*U12] 31 Table 2-12. Bond distances (A) for Cr2B3. Crl B2 4x 2.2654(3) Crl B3 4x 2.2817(3) Crl B3 2x 2.2936(3) Crl B1 2x 2.3433(3) Cr2 B2 2x 2.1462(3) Cr2 B 1 4x 2.1808(3) Cr2 B1 1x 2.2548(4) B1 B2 2x 1.7555(3) B1 Cr2 4x 2.1808(3) Bl Cr2 1x 2.2548(4) B1 Crl 2x 2.3433(3) B2 B3 1x 1.7247(3) B2 B 1 2x 1.7555(3) B2 Cr2 2x 2.1462(3) B2 Crl 4x 2.2654(3) B3 B3 2x 1.6990(3) B3 B2 1x 1.7247(3) B3 Crl 4x 2.2817(3) B3 Crl 2x 2.2936(3) 32 Table 2-13. Crystal data and structure refinement for CrB2. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 29.02° Refinement method Data/ restraints / parameters Goodness-of-fit on F2 Final R indices [I>281gma(1)] R indices (all data) Extinction coefficient 73.62 100(2) K 0.71073 A Hexagonal P6/mmm a = 2.9604(4) A a: 90° b = 2.9604(4) A B= 90° c = 3.0574(6) A y = 120° 23.205(6) A3 2 10.536 g/cm3 22.350 mm'1 68 6.66 to 29.02° 45h54,—35k53,—45154 219 24 [R(int) = 0.0289] 100.0 % Full-matrix least-squares on F’2 24/0/6 1.296 R1 = 0.0163, wR2 = 0.0402 R1 = 0.0163, wR2 = 0.0402 1.0(5) R1 = Z ||F..| - |F.|| / Z |F0| and wR2 = [z (|F.,2 — F..2| )2 / z (wF02)2]'/2 33 Table 2-14. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for CrB2. x y z U(eq) Cr(l) 0 0 5000 1(1) 13(1) -3333 3333 0 1(1) U(eq) is defined as one third of the trace of the orthogonalized UiJ' tensor. Table 2-15. Anisotropic displacement parameters (Azx 103) for CrB2. U11 u22 u33 U23 ul3 {112 Cr(l) 1(1) 1(1) 0(1) 0 0 1(1) 3(1) 1(1) 1(1) 0(2) 0 0 0(1) The anisotropic displacement factor exponent takes the form: -27t2[ h2 a"‘2U11 + +2hka*b*U12] Table 2-16. Bond distances (A) for CrB2. Crl B 1 12x 2.2943(3) B1 Bl 3x 1.7069(2) B1 Crl 6x 2.2943(2) 34 Table 2-17. Crystal data and structure refinement for MoB and WB Formula Formula weight Crystal system Space group Unit cell dimensions Volume Z, Density (calculated) Absorption coefficient F(000) Crystal size, mm Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to 0mm, Refinement method Data / restraints / parameters Goodness-of-fit on F’2 Final R indices [I>20(I)] R indices (all data) Extinction coefficient MoB 106.75 Tetragonal 141/amd a = 3.1103(4) A b = 3.1103(4) A = 16.899(3) A 163.48(4) A3 8, 8.674 g/cm3 14.713 mm'1 376 0.004 x 0.052 x 0.096 4.73 to 29.11° 4 5 h 5 3. 4 5 k 5 3, -21 5 1 5 21 679 76 [R(int) = 0.0454] 100.0 % WB 194.66 Tetragonal 141/amd a = 3.1138(8) A b = 3.1138(8) A = 16.929(9) A 164.14(10) A3 8, 15.755 g/cm3 139.427 mm1 632 0.004 x 0.072 x 0.106 4.71 to 28.30° -35h53 -35k53 -21 5 1 5 21 524 65 [R(int) = 0.0435] 91.5% Full-matrix least-squares on E2 76/ 0 / 9 1.075 R1 = 0.0206, wR2 = 0.0456 R1 = 0.0308, wR2 = 0.0469 0.013(2) 65/ 0/ 10 1.384 R1 = 0.0663, wR2 = 0.1680 R1 = 0.0669, wR2 = 0.1688 0.015(5) R1 = Z ||F.,| — |F..|| / z |F0| and wR2 = [2 (pa,2 — Ffl )2 / z (6)5521"? 35 Table 2-18. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103)for MoB and WB. x y 2 U(EQ) M0(1) 0 2500 721(1) 3(1) B(2) -5000 2500 -309(6) 4(2) W( 1) 0 2500 724(1) 4(2) B( 1) -5000 -2500 300(40) 40(30) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. Table 2-19. Anisotropic displacement parameters (Azx 103) for MoB and WB. U11 U22 U33 U23 U13 U12 Mo(l) 2(1) 2(1) 6(1) 0 0 1(1) 3(1) 4(5) 3(5) 6(4) 0 0 0(1) W(1) 6(2) 5(2) 0(2) 0 0 0 3(1) 0(40) 130(80) 0(30) 0 0 0 The anisotropic displacement factor exponent takes the form: -27t2[ h2 a*2Ull + +2hka*b*U12] 36 Table 2-20. Bond distances (A) for MoB. M01 B2 4x 2.3070(2) Mol B2 2x 2.3353(3) Mol B2 1x 2.4826(5) B2 B2 2x 1.8739(2) BZ M01 4x 2.3070(2) B2 Mol 2x 2.3353(3) B2 Mol 1x 2.4826(5) Table 2.21. Bond distances (A) for WB. W1 Bl 4x 2.3153(4) W1 Bl 2x 2.3307(7) W1 B1 1x 2.4979(13) B1 B1 2x 1.8604(4) B1 W1 4x 2.3153(4) Bl W1 2x 2.3307(7) Bl W1 lx 2.4979(13) 37 D. Structural Description Cr5B3: The structure of Cr5B3 (Figure 2-1a) was first reported by Bertaut and Blum,l4 and came to be the representative of its own structure type. A common characteristic for the structure type is the formation of dumbbell-like pairs of atoms, shown in Figure 2-1b. An investigation of the coordination environments of the atoms reveals elongated octahedra of boron atoms around Crl and antiprisms of chromium atoms around B1. The trigonal prismatic coordination commonly found for boron atoms is seen in the chromium atoms around B2. Cr3B4: The structure of Cr3B4 belongs to the T a3B4-structure type and was first described by researchers in Sweden.15 The structure type is characterized by double chains of boron atoms that link together to form a series of side-sharing hexagons (Figure 2-2a). The structure can also be described, as in the work by Okada, et al.,7 by stacking sheets of AlB2-type structure. A V2, 1/2, 0 unit cell translation of the A1B2 structure builds the Cr3B4 structure. The sheets forming the structure are then interconnected through Cr-Cr bonds. Cr2B3: A description of the Cr2B3 structure, which belongs to the V2B3-structure type, was given by Okada, et al., in the first account on the structure of the compound.7 As with Cr3B4, the structure can be built by V2, 1/2, 0 unit cell translations of an A1B2-type structure. In this compound, triple chains of boron atoms link together and form two columns of hexagons (Figure 2-2b). The previous structural description by Okada also points out that the interatomic distances between chromium atoms (2.62 A) are larger than the distance in the elemental metal (2.498 A), suggesting that Cr—B and B—B bonds hold the sheets in the structure together. 38 Figure 2-1 (a) Representation of Cr5B3 along the b-axis. (b) Boron pairs in Cr5B3 (Cr atoms omitted for clarity). 39 c c “3‘ 3:3”? 8}: ~ c c c c :g' 4 c t (b) Figure 2-2. Double and triple chains of boron atoms in (a) Cr3B4 and (b) Cr2B3, respectively. 40 CrB2: Like most transition metal diborides, CrB2 crystallizes with the A1B2- structure type. This structure-type comprises lamellar sheets of boron atoms in a graphite-like arrangement and hexagonally close-packed metal atoms. The structure of CrB2 is shown in Figure 2-3a and the planar nature of the graphite-like boron layers are emphasized in Figure 2-3b. MB (M=Mo, W): The monoborides of molybdenum and tungsten both crystallize in the MOB-structure type (Figure 2-4). The structure, first described by Kiessling,2 features infinite zigzag chains of boron atoms running parallel to the a-axis in one sheet and parallel to the b-axis in the next. The metal atoms form trigonal prisms around the boron atoms. E. Results and Discussion As mentioned, the molten metal flux technique has been used to synthesize group 6 borides with copper and aluminum as the flux metals, so we were interested in extending the technique to include gallium. The synthesis and growth of Cr2B3, CrB2, MoB, and WB from a gallium flux indicates initial success in our extension of the technique. These results are encouraging, but they have been limited to binary borides. The chromium borides can be formed from systems containing just chromium, boron, and gallium, so the influence of varying the chromium to boron ratio on the resulting borides was briefly investigated. One of the most interesting things found was that CrB2 was the only boride formed at the most boron-rich ratios. Though it was expected that CrB4 would form at some point, that was not the case, even when the B:Cr 41 \ £5 \ aces". a‘nmnmm~ “V‘V "“\' waxes-er - ° W fi. nu! ‘ 32!". 1;?{zliji{?1—z :":;T-‘ :7:."'. ' ‘u-I- ‘— ‘Cl’ “La 1811 _ * ca 391712." i.‘.‘_ -._ 1... , . . I - _ A ‘1’ an ‘- ‘I' u u I" ' r I. I! ' _-' - if ,I‘." -‘,-_ 2.1. . - -— v r ‘ s ' r I'— r V l I" I r I _ ' """‘-"z‘~._I. ..«-‘- ‘- '- Figure 2-3. (a) CrB2 structure seen along c-axis (b) Planar-nature of boron layers in CrB2. 42 “'4‘. 6%.. b‘i/OU‘O“ M WB L. Q‘bca shown ratio reached 10:1. It was also slightly troubling that more borides with lower B:Cr ratios were not found. An expanded study looking at more B:Cr ratios should help determine which borides can be synthesized from the gallium flux. The results of the previous aluminum flux studies also imply that cooling rates for the reactions must also be studied. Our limited attempts to synthesize ternary borides from a gallium flux were unsuccessful. However, monoborides of the heavier group 6 members from these reactions aimed at ternary species were synthesized. Subsequent attempts to isolate these borides from systems containing only the metal, boron, and gallium have not been successful. However, further investigations varying the B:M ratios and heating profiles are needed for a complete study. Varying the heating profiles and reagent ratios may also help in forming ternary group 6 borides when other metals are included in the reactions. Crystals of Cr5B3, Cr3B4, and Cr2B3 have been successfully grown from reactions utilizing a molten copper flux. The latter two borides were grown from systems containing only chromium, boron, and copper, so there is potential that other borides will be found from similar reactions that vary the B:Cr ratio and heating profiles. While we were unable to isolate borides of the heavier group 6 elements or ternary borides with any group 6 members from copper flux reactions, further studies may be made more successful by varying the reagent stoichiometry and/or heating profiles. F. Conclusions The molten metal flux technique has successfully been applied to the synthesis of Group VI borides. Both gallium and copper have been used as the flux metal in the synthesis of Cr2B3. Molybdenum monoboride, tungsten monoboride, and chromium 44 diboride have been synthesized from gallium flux reactions. 0ng and Q33, have been synthesized from reactions utilizing molten copper. We have not synthesized any ternary Group VI borides from either gallium or copper, but our investigations into these systems are rather limited. We believe that further investigations into the flux reactions are merited and necessary based on these initial results. 45 References 1. Klesnar, H.; Aselage, T. L.; Morosin, B.; Kwei, G. H.; Lawson, A. C., The Diboride Compounds of Molybdenum: MoB2.x and M02B5-y. Journal of Alloys and Compounds 1996, 241, 180-186. 2. Kiessling, R., The Crystal Structure of Molybdenum and Tungsten Borides. Acta Chemica Scandinavica 1947, 1, 893-916. 3. Lundstrom, T.; Rosenberg, I., The Crystal Structure of the Molybdenum Boride M01433. Journal of Solid State Chemistry 1973, 6, 299-305. 4. Lundstrom, T., The Structure of RU283 and WB2”, as determined by single-crystal diffractometry, and some notes on the W-B system. Arkivfbr Kemi 1969, 30, 115-127. 5. Romans, P. A.; Krug, M. P., Composition and Crystallographic Data for the Highest Boride of Tungsten: Acta Crystallographica 1966, 20, 313-315. 6. Hi gashi, 1.; Takahashi, Y.; Atoda, T., Crystal Growth of Borides and Carbides of Transition Metals from Molten Aluminum Solutions. Journal of Crystal Growth 1976, 33, 207-211. 7. Okada, S.; Atoda, T.; Higashi, 1., Structural Investigation of Cr2B3, Cr3B4, and CrB by Single-Crystal Diffractometry. Journal of Solid State Chemistry 1987, 68, 61-67. 8. Okada, S.; Atoda, T.; Higashi, I.; Takahashi, Y., Preparation of Single Crystals of MoB2 by the Aluminum-flux Technique and Some of Their Properties. Journal of Materials Science 1987, 22, 2993-2999. 9. Okada, S.; Kudou, K.; Lundstrom, T., Preparations and Some Properties of W2B, 5-WB, and WB2 Crystals from Hi gh-Temperature Metal Solutions. Japanese Journal of Applied Physics 1995, 34, (1), 226-231. 10. Sheldrick, G. M. SAINT, Version 4; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI. 11. Sheldrick, G. M. SHELXTL Structure Determination Program, Version 5.0; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI, 1995. 12. X-SHAPE, Version 2.05; STOE & Cie GmbH: 2004. 13. X-RED 32, Version 1.10; STOE & Cie GmbH: 2004. 14. Bertaut, F.; Blum, P., Etude des borures de chrome. Comptes Rendus Hebdomadaires des Seances de l'Academie des Sciences 1953, 236, 1055-1056. 46 15. Elfstrom, M., The Crystal Structure of Cr3B4. Acta Chemica Scandinavica 1961, 15, (5), 1178. 47 CHAPTER THREE The Metal Flux Synthesis of Group Seven Borides A. Introduction There are many similarities between the borides of chromium and the borides of manganese. Both metals have borides that display the interesting series of boron atom configurations from isolated boron atoms to a three-dimensional network found only in CrB4 and MnB4.l Several reports have even mentioned a manganese monoboride that crystallizes with the CrB-type structure, instead of its normal FeB-type structure.2‘ 3 However, several manganese analogs are “missing” when compared to the chromium system, such as Mn5B3 and Mn2B3. We became interested in whether it was possible to use the metal flux to isolate these “missing” borides. The literature for flux syntheses of manganese borides returned only a ternary phase that incorporated aluminum from the flux, Mn2AlB2.4 This was a bit surprising, due to the success of the flux technique with the group 6 metalss'8 During the literature search we also checked for reports on flux synthesis of rhenium borides. Again, we found no previous work done in the area, but the overall lack of work done in the Re-B system did not make this overly surprising. The Re-B system has produced Re3B,9 ReB2,10 and Re7B3,ll and only Re3B had structural characterization performed on a single crystal. Rather large single crystals of 48 ReB2 were recently grown using the floating zone method, however, the growth temperature was near 2400°C, well above temperatures the equipment in our labs can attain consistently. The lower temperatures used in our flux reactions would be very attractive for producing crystals of any of these compounds. Single crystals are useful when looking for anisotropic behavior of properties in a compound. The magnetism in Mn3B4 is a fine example of this anisotropy, as ferromagnetism is detected in the ac-plane and antiferromagnetism is found between layers along the b-axis.”’ 13 Discovering and studying similar phenomena in other compounds would be greatly simplified by using single crystals. The nature of the 14, 15 may also be better understood when single superconductivity in rhenium borides crystals are used in the physical measurements. The use of single crystals limits the possibility of minor phases negatively influencing results, while these minor phases may go undetected in powdered samples. We report here our attempts to use the molten metal flux technique in the synthesis of group 7 borides. A molten gallium flux has been used to synthesize three binary borides, MnB, MnB4, and ReBz, and four ternary borides, HoMnB4, DyReB4, ErReB4, and YbReB4. Our attempts to use alternate flux metals in the syntheses of these compounds are also discussed. B. Experimental Section Reagents: All reagents were used as received without further purification: (i) Boron metal, 99% purity, -325 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (ii) Rhenium 49 powder, 99.99% purity, Strem Chemicals, Newburyport, MA, (iii) Gadolinium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (iv) Dysprosium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (v) Erbium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (vi) Gallium 3-5 mm shot, 99.999% purity, Plasmaterials, Liverrnore, CA, (vii) Manganese powder, 99.9% purity, -50 mesh, Aldrich Chemical Company, Milwaukee, WI, (viii) Tantalum powder, 99.9% purity, Cerac Specialty Inorganics, Milwaukee, WI. Furnaces: A Lindberg Blue high-temperature, horizontal tube furnace was used with a continuous argon flow of approximately 0.1 L/min. Heating profiles for individual reactions were programmed into the accompanying Lindberg UP150 furnace controller. Thermocouples connected to the furnace controller were used to monitor fiimace temperatures during reactions. The maximum operating temperature for the furnace was 1500 °C. A radio frequency (RF) furnace was constructed from an Ameritherm XP7.5CE Induction Heater and fused quartz reaction chamber. A molybdenum cylinder, machined to act as a reaction crucible holder, was used as a susceptor. A boron nitride cylinder was machined to hold the molybdenum crucible in the center of the reaction chamber. Details on the RF furnace setup are given in the appendix of this work. RF furnace temperatures were controlled manually using the Ameritherm control unit. Reaction temperatures were monitored using an Ircon SA Series Infrared Thermometer. During the course of some reactions, films deposited inside the reaction 50 chamber would prevent the IR thermometer from accurately reporting furnace temperatures. In such circumstances, reaction temperatures were approximated based on power settings for the Ameritherm control unit and a series of calibration runs conducted by heating only the molybdenum cylinder. Temperatures greater than 1700 °C were easily reached with this furnace. Synthesis and Isolation: MnB: Boron (4 mmol), tantalum (1 mmol), and manganese (2 mmol) powders were mixed and added to an alumina crucible along with pieces of gallium shot totaling 1.67 g. A quartz filter was placed in the crucible which was then placed in 13 mm diameter quartz tube, evacuated under vacuum to a pressure near 10'4 Torr, and sealed using an oxygen-acetylene torch. The tube was then heated in a commercial tube furnace under a heating profile that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to 250 °C in 60 hours. The quartz tube was removed from the furnace at 250 °C and centrifuged to remove excess gallium. After centrifugation, the tube was opened and the crucible was placed in a bath of 5M 12 in DMF in order to remove the remaining gallium flux. An overnight soak was found to be insufficient for removing all of the gallium, so soaking continued for an additional 2 days. Extended soaking in the bath was not found to damage the crystals. Silver, prismatic crystals were produced in about 40% yields, based on manganese. Visual distinction between MnB and MnSi crystals is nearly impossible, so EDS analysis was used to differentiate crystals. Elemental analysis performed by EDS 51 using an SEM showed that manganese and boron were the only elements present in the crystal used for diffraction study. Besides the MnSi, the collected product also contained MnGa4 and MnGa4_5. MnB4: Boron and manganese powder were mixed and added to alumina crucibles in millimolar quantities in boron-to-manganese ratios between 2:1 and 5:1. Pieces of gallitnn shot totaling between 1.5 g and 2.5 g were then placed in the crucibles. The alumina crucibles were then placed in 13 mm diameter quartz tubes and evacuated under vacuum to a pressure near 10'4 Torr. The quartz tubes were then sealed using an oxygen-acetylene torch. The quartz tubes were placed in mullite tubes, then heated in commercial tube furnaces under heating profiles that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 0C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to room temperature in 60 hours. After cooling, the quartz tubes were opened and the alumina crucibles were placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed after an overnight soak, but longer soaks were used without damage to the recovered product. Silver, plate-like crystals with ridges (later found to be twinned crystals) were produced in 30-40% yields. Elemental analysis performed by EDS using an SEM showed that manganese and boron were the only elements present in the crystals. The remainder of the product comprised MnGa4 and MnGa4,5. ReBz: Boron and rhenium powder were mixed and added to alumina crucibles in millimolar quantities in boron-to-rhenium ratios between 2:1 and 5:1. Pieces of gallium shot totaling between 1.5 g and 2.5 g were then placed in the crucibles. The alumina 52 crucibles were then placed in 13 mm diameter quartz tubes and evacuated under vacuum to a pressure near 10'4 Torr. The quartz tubes were then sealed using an oxygen- acetylene torch. The quartz tubes were placed in mullite tubes, then heated in commercial tube furnaces under heating profiles that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to room temperature in 60 hours. After cooling, the quartz tubes were opened and the alumina crucibles were placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed afier an overnight soak, but longer soaks were used without damage to the recovered product. Silver, hexagonal plates are produced in 40-50% yields, based on rhenium. Elemental analysis performed by EDS using a SEM showed that rhenium and boron were the only elements present in the crystals. The remainder of the product comprised ReGa4_5. HoMnB4: Boron (3.5 mmol) and manganese (0.5 mmol) powders were mixed and added to an alumina crucible along with holmium (1.5 mmol) filings. Pieces of gallium shot totaling 1.5 g were added to the crucible before it was placed in a 13 mm diameter quartz tube and evacuated under vacuum to a pressure near 10'4 Torr. The quartz tube was then sealed using an oxygen-acetylene torch and placed in a mullite tube. Heating took place in a commercial tube furnace under a heating profiles that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for 53 an additional 48 hours, and then allowed the furnace to cool to room temperature in 60 hours. After cooling, the quartz tubes were opened and the alumina crucibles were placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed after an overnight soak, but longer soaks were used without damage to the recovered product. Silver, plate-like crystals are a minor product (20-30% yields, based on manganese). Elemental analysis performed by Energy Dispersive Spectroscopy (EDS) using a Scanning Electron Microscope (SEM) showed that holmium, manganese, and boron were the only elements present in the crystals. The remainder of the product comprised MnGa4, MnGars, traces of HoB6, and unreacted boron. REReB4 (RE= Dy, Er, Yb): Boron and rhenium powders were added to alumina crucibles, along with filings from an ingot of a rare-earth metal, in millimolar quantities in a 1.5:] :4 ratio of RE:Re:B. Pieces of gallium shot totaling 2 g were placed atop the reagents in the crucibles. The alumina crucibles were then placed in an alumina boat, which was in turn place inside an alumina tube. The alumina tube was placed in a high- temperature tube furnace and heated under a slow flow of argon. The furnace was heated to 1400 °C in 8 hours and held at that temperature for 10 hours, then cooled to 1200 °C in 5 hours and held at that temperature for 10 hours, and finally cooled to 500 °C in 36 hours, at which point the power to the furnace was shut off and the furnace was allowed to cool to room temperature. After cooling, the crucibles were removed from the boats in the tube and placed in a half-concentrated HCl bath in order to remove excess the gallium. An overnight soak 54 was adequate to remove the gallium. DyReB4 and ErReB4 were collected in estimated 30-50% yields based on rhenium. YbReB4 was collected in an estimated 20-40% yield based on rhenium. Side products in the DyReB4 reaction included ReGa4_5 and DyB6. Side products in the ErReB4 reaction included ReGa4_5 and ErB6. Side products in the YbReB4 reaction included ReGa4,5 and YbB6. C. Physical Measurements Energy Dispersive Spectroscopy: Energy dispersive spectroscopy (EDS) analyses were carried out on selected crystals to determine their chemical composition. The analyses were performed with a J EOL J SM-6400 scanning electron microscope (SEM) equipped with Noran Vantage Energy Dispersive Spectroscopy (SizLi) detector and Norvar window for standardless quantization of elements with Z Z 4. The crystals were affixed to an alumina sample holder with double-sided carbon tape. The EDS data were acquired at an accelerating voltage of 10 kV with a 30 to 60 second accumulation time. Single-Crystal X-ray Crystallography: Single crystals were mounted on a glass fiber with super glue and their intensity data were collected on either a Bruker SMART platform CCD diffractometer, or a STOE IPDS II diffractometer using Mo K01 radiation at 50 kV and 40 mA. Individual frames of REReB4 (RE= Dy, Er, Yb) examined with the Bruker machine were collected with a 03° 0) rotation. The SMART software was used for data collection, and SAINTl6 software was used for data extraction and reduction. After 55 applying analytical absorption corrections, structure solution and refinement were completed using direct methods and the SHELXTLl7 suite of programs. Samples examined with the STOE (MnB, MnB4, ReB2, and HoMnB4) had individual frames collected on a 34 cm image plate with a 60 second exposure time and a 10° 0) rotation. The X-SHAPEl8 and X-RED19 sofiware packages were used for data extraction and reduction and to apply an analytical absorption correction. Direct methods and the SHELXTL suite were used to solve and refine the structures. The crystal structure refinement data for MnB are found in Table 3-1. Atomic parameters previously reported5 for CrB were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 3-2. AnisotrOpic displacement parameters for the atoms are found in Table 3-3. The bond lengths in MnB and a count of those bonds are listed in Table 3-4. The refinement data for MnB4 are found in Table 3-5. The atomic parameters from CrB420 were used as a starting point for refinement of the structure. Parameters 21. 22 apply to the monoclinic space group from previous reports on the structure of MnB4 C2/m (a = 5.5029, b = 5.3669, c = 2.9487, [3 = 122.71) and are not useful in the orthorhombic Immm space group. Atomic positions and isotropic parameters found in this study of W., are given in Table 3-6. Anisotropic displacement parameters for the atoms are listed in Table 3-7. The values for these parameters are quite high and may be the result of the twinning in the crystal or a modulated structure. The bond lengths in MnB4 and a count of those bonds in the unit cell are listed in Table 3-8. The crystal structure refinement data for ReB2 are listed in Table 3-9. The atomic parameters reported in the first structural reportlo were used as a starting point for the 56 refinement of the structure from our data. The atomic positions and isotropic displacement parameters we have found are listed in Table 3-10. Anisotropic displacement parameters for the atoms are listed in Table 3-11. Bond lengths and a count of those bonds in the structure are found in Table 3-12. The crystal structure refinement data for HoMnB4 are listed in Table 3-13. The atomic positions and isotropic displacement parameters for HoMnB4 are listed in Table 3-14. The manganese atoms were distributed over split positions, so anisotropic parameters were not carried out for these atoms. Anisotropic displacement parameters for the remaining atoms are listed in Table 3-15. The anisotropic displacement parameters are high, especially for the boron atoms. Inadequate absorption correction, modulated structure, and a twinned crystal may all play a role in creating these high values. Given the similar crystal morphology between HoMnB4 and MnB4, crystal twinning is likely present. The refinement data for REReB4 (RE = Dy, Er) are listed in Table 3-16. The refinement data for YbReB4 are listed in Table 3-17. The atomic parameters for YCrB423 were used as a starting point for the refinement of our data, as all of these compounds are members of the YCrB4 structure type. The atomic parameters and isotropic displacement parameters for REReB4 (RE = Dy, Er, Yb) are listed in Table 3-18. The anisotropic displacement parameters for REReB4 (RE = Dy, Er, Yb) are listed in Table 3-19. Inadequate absorption corrections are most likely responsible for the low values of the parameters for the heavy atoms in all of these compounds. The bond distances for HoMnB4 and REReB4 (RE = Dy, Er, Yb) are listed in Table 3-20. 57 Table 3-1. Crystal data and structure refinement for MnB. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 34.65° Refinement method Data / restraints / parameters Goodness-of-fit on F 2 Final R indices [I>28igma(1)] R indices (all data) Extinction coefficient 65.75 293(2) K 0.71073 A Orthorhombic Cmcm a=3.0113(6)A or= 90° b = 7.6733(15) A B= 90° c = 2.9610(6) A y = 90° 6842(2) A3 4 6.383 g/cm3 17.695 mm“ 120 5.31 to 34.65° -45h54,-125k512,-45154 444 92 [R(int) = 0.0299] 91.1 % Full-matrix least-squares on F2 92/ 0/ 10 1.230 R1 = 0.0135, wR2 = 0.0324 R1 = 0.0135, WR2 = 0.0324 035(4) R1 = z ”Fol — mu /2 |F0| and wR2 = [2 (IF,2 — FCZI )2 / Z (wFo2)2]"2 58 Table 3-2. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for MnB. x y z U(eq) Mn(l) 5000 1438(1) 2500 4(1) 8(1) 0 663(3) -2500 5(1) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 3-3. Anisotropic displacement parameters (Azx 103) for MnB. U11 U22 u33 U23 U13 ulz Mn(1) 4(1) 4(1) 4(1) 0 0 0 8(1) 5(1) 5(1) 4(1) 0 0 O The anisotropic displacement factor exponent takes the form: -21r2[ h2 a"'2Ull + + 2 h k a“ b* 012 ]. Table 3-4. Bond distances (A) for MnB. Mnl B1 4x 2.1937(3) Mnl Bl 2x 2.2059(3) Mnl B1 1x 2.2245(4) Bl Bl 2X 1.7966(3) Bl Mnl 4x 2.1937(3) Bl Mnl 2x 2.2059(3) B1 Mnl 1x 2.2245(4) 59 Table 3-5. Crystal data and structure refinement for MnB4, Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 36.51 ° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>231gma(l)] R indices (all data) Extinction coefficient 98.18 293(2) K 0.71073 A Orthorhombic Im a = 2.9380(6) A or= 90° b = 4.6104(9) A B= 90° c = 5.3528(11) A y = 90° 7251(3) A3 2 4.497 g/cm3 8.403 mm'1 90 5.84 to 36.51° 45h$4,-7Sk$7,-8Sl$8 589 119 [R(int) = 0.0512] 96.7 % Full-matrix least-squares on F2 119 / 0/ 11 1.255 R1 = 0.0355, wR2 = 0.0854 R1 = 0.0355, wR2 = 0.0854 0.61(13) R1 = Z “Fol - IFcII /Z IFoI and Wm = 12 (IF: — Fczl )2/z(wF.2)21“2 60 Table 3-6. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for MnB4. x y 2 U(CQ) Mn(l) 0 0 0 8(1) 3(1) 0 1995(13) 3440(11) 28(1) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. Table 3-7. Anisotropic displacement parameters (A2x 103) for MnB4_ ull U22 U33 U23 [113 [112 Mn(l) 22(1) 2(1) 1(1) 0 0 0 13(1) 3(1) 45(3) 35(2) -38(2) 0 0 The anisotropic displacement factor exponent takes the form: -21t2[h2 a"'2Ull + + 2 h k at b“ [112 ] Table 3-8. Bond distances (A) for MnB4, Mnl Bl 4X 2.0580(3) Mnl Bl 8x 2.1853(3) Bl 131 lx 1.6706(3) 131 Bl 1x 1.8391(4) Bl Bl 2x 1.8403(3) 61 Table 3-9. Crystal data and structure refinement for ReB2, Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 35.9l° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>231gma(1)] R indices (all data) Extinction coefficient 207.82 293(2) K 0.71073 A Hexagonal P63/mmc a = 2.8891(4) A or= 90° b = 2.8891(4) A [3: 90° c = 7.4606(15) A 'y = 120° 53.930(15) A3 2 12.798 g/cm3 11 1.675 M'1 170 0.140 x 0.140 x 0.010 mm3 8.17 to 35.91° -1 ShS4,-4Sk$4,-8SIS 11 270 66 [R(int) = 0.0842] 89.9 % F ull-matrix least-squares on F2 66 / 0 / 7 1.352 R1 = 0.0218, wR2 = 0.0509 R1 = 0.0263, wR2 = 0.0517 0.091(17) RI = z llFol — chll / z w and sz = 12 0F: - F31 )2 / z (wFffrm 62 Table 3-10. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for ReB2. x y z U(eq) Re(1) 6667 3333 2500 2(1) 3(1) 6667 3333 5460(20) 1(2) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 3-11. Anisotropic displacement parameters (A2x 103) for ReB2, ull U22 u33 U23 1113 ulz Re(1) 1(1) 1(1) 5(1) 0 0 1(1) 8(1) 1(3) 1(3) 0(4) 0 0 1(2) The anisotropic displacement factor exponent takes the form: -2n2[ h2 a"‘2Ull + + 2 h k a* b* U12 ] Table 3-12. Bond distances (A) for ReB2, Rel Bl 2x 2.2094(4) Rel Bl 6x 2.2573(3) 81 81 3x 1.8045(2) Bl Rel 1x 2.2094(4) Bl Rel 3x 2.2573(3) 63 Table 3-13. Crystal data and structure refinement for HoMnB4, Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 36.07° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2sigma(1)] R indices (all data) Extinction coefficient 263.1 1 293(2) K 0.71073 A Orthorhombic Pbam a = 5.8946(12) A or= 90o b=11.411(2)A 8=90° c = 3.4041(7) A y= 90° 228.96(8) A3 4 7.633 g/cm3 39.388 mm" 448 4.97 to 36.07° -9Sh$9,-17Sk$18,-551$4 3176 606 [R(int) = 0.1861] 97.9 % Full-matrix least-squares on F 2 606 / 0 / 38 1.1 18 R1 = 0.0949, wR2 = 0.2203 R1 = 0.1477, wR2 = 0.2535 0.033(8) RI = 2: “For — 1F.“ / z 181 and wR2 = 12 0F} — F21 )2 / z (mem 64 Table 3-14. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for HoMnB4_ x y z U(eq) Occupancy Mn(l) 871 1(10) 5846(5) -5000 10(1) 0.86728 Mn(15) 8400(60) 6470(30) -5000 10(1) 0.13272 Ho(1) 6278(3) 3495(1) 5000 14(1) B(2) 8700(100) 4520(30) 0 19(8) B(3) 6480(1 10) 5350(50) 0 35(15) B(4) 71 10(70) 6830(30) 0 14(6) B(5) 10200(50) 693 0(40) 0 18(7) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. Table 3-15. Anisotropic displacement parameters (Azx 103) for HoMnB4, ull U22 u33 U23 {113 ulz Ho(l) 16(1) 15(1) 10(1) 0 0 0(1) B(2) 50(20) 5(1 1) 2(9) 0 0 19(18) B(3) 60(30) 40(20) 4(1 1) 0 0 60(3 0) B(4) 31(18) 6(11) 6(11) 0 0 8(13) 3(5) 0(9) 30(19) 24(18) 0 0 10(1 1) The anisotropic displacement factor exponent takes the form: -21'C2[ h2 a"'2Ull + + 2 h ka* b* U12] 65 Table 3-16. Crystal data and structure refinement for REReB4 (RE= Dy, Er). F orrnula Formula weight Crystal system Space group Unit cell dimensions Volume Z, Density (calculated) Absorption coefficient F(000) Crystal size, mm Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to 0mm, Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [1>20'(1)] R indices (all data) Extinction coefficient DyReB4 391.94 Orthorhombic Pbam a = 5.9710(12) A b = 11.545(2) A c = 3.5980(7) A 248.03(9) A3 4, 10.496 g/cm3 78.259 mm'1 644 0.044 x 0.044 x 0.064 3.53 to 28.06° -7 S h S 7, -14 S k S 15, -4 S l S 4 2410 340 [R(int) = 0.0490] 97.7 % ErReB4 396.70 Orthorhombic Pbam a = 5.9490(12) A b = 11.508(2) A c = 3.5820(7) A 245.23(8) A3 4, 10.745 g/cm3 82.905 mrn'l 652 0.038 x 0.046 x 0.050 3.54 to 28.08° -7 S h _<_ 7. -14 S k S 15, -4 S l S 4 2459 335 [R(int) = 0.0559] 97.1 % F ull-matrix least-squares on F2 340 / 0 / 38 1.064 R1 = 0.0275, wR2 = 0.0788 R1 = 0.0278, wR2 = 0.0790 0.0324 (18) 335 / 0 / 38 1.131 R1 = 0.0395, wR2 = 0.0887 R1 = 0.0413, wR2 = 0.0898 0.00138(1 1) R1 = Z llFol — 1F.” / 2 IF.) and sz = 1: (IF: — FEI )2 / z (wFozflm 66 Table 3-17. Crystal data and structure refinement for YbReB4, Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges . Reflections collected Independent reflections Completeness to theta = 28.28° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>25igma(1)] R indices (all data) Extinction coefficient 402.48 273(2) K 0.71073 A Orthorhombic Pbam a = 5.9273(9) A or= 90° b = 11.4497(18) A 8= 90° c = 3.5617(6) A y = 90° 241 .72(7) A3 4 11.060 g/cm3 88.080 mm'1 660 0.052 x 0.052 x 0.104 mm3 3.56 to 28.28° -7ShS7,-14SkS 15,-45154 2363 333 [R(int) = 0.0605] 96.2 % F ull-matrix least-squares on F 2 333 / 0 / 38 1.143 R1 = 0.0431, wR2 = 0.1076 R1 = 0.0448, wR2 = 0.1088 0.0134(13) R1 = 2 117.1 - 1F.” /2 IF.) and sz = 12 0F: - F}: )2/Z(wFoz)21”2 67 Table 3-18. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for REReB4 (RE = Dy, Er,Yb). x y z U(eq) Re(l) 1328(1) 4133(1) 0 2(1) Dy(2) 1264(1) 1504(1) 0 2(1) B(l) 2860(30) 3183(14) -5000 3(3) B(2) -240(3 0) 3087(15) -5000 6(3) B(3) -1 130(3 0) 4520(17) -5000 7(3) B(4) 363 0(3 0) 4703(16) -5000 6(3) Re(l) 1335(1) 4131(1) 0 0(1) Er(2) 1267(2) 1502(1) 0 0(1) B( l) 2860(40) 3 140(20) 5000 1(4) B(2) 3850(40) 490(20) 5000 2(5) B(3) 4770(40) 1920(20) 5000 1(5) B(4) 365 0(40) 4700(20) 5000 3(5) Yb(1) 1271(2) 1501(1) 0 0(1) Re(2) 1339(2) 4132(1) 0 2(1) B(l) 3610(50) 4690(20) 5000 4(6) B(2) 1 120(50) 5510(30) 5000 3(6) B(3) 283 0(5 0) 3 140(30) 5000 4(6) B(4) -170(60) 3070(30) 5000 9(6) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. 68 Table 3-19. Anisotropic displacement parameters (Azx 103) for REReB4 (RE = Dy, Er, Yb). U1 l U22 u33 U23 ul3 ulz Re(l) 2(1) 0(1) 4(1) 0 0 0(1) Dy(2) 1(1) 0(1) 4(1) 0 0 0(1) 8(1) 4(7) 0(8) 6(8) 0 0 -3(6) B(2) 4(7) 0(7) 1 3(8) 0 0 0(6) B(3) 5(7) 4(8) 1 1(9) 0 0 5(6) B(4) 2(7) 6(9) 1 1(8) 0 0 0(6) Re(l) 0(1) 0(1) 0(1) 0 0 1(1) Er(2) 0(1) 0(1) 0(1) 0 0 0(1) B(l) 3(11) 0(11) 0(11) 0 0 0(9) B(2) 1(11) 5(11) 0(11) 0 0 -5(9) B(3) 0(10) 0(11) 3(11) 0 0 5(8) B(4) 0(10) 0(1 1) 8(12) 0 0 1(8) Yb(l) 0(1) 1(1) 0(1) 0 0 0(1) Re(2) 2(1) 4(1) 0(1) 0 0 1(1) 3(1) 11(13) 0(12) 0(12) 0 0 15(11) B(2) 7(14) 0(12) 3(13) 0 0 0(10) B(3) 11(14) 0(12) 0(13) 0 0 2(11) B(4) 18(16) 0(13) 10(15) 0 0 -4(12) The anisotropic displacement factor exponent takes the form: -21t2[ h2 a"'2UH + + 2 h kalt bar: U12] 69 Table 3-20. Bond distances (A) for HoMnB4 and REReB4 (RE = Dy, Er, Yb). HoMnB4 DyReB4 ErReB4 YbReB4 RE(1)—M(1) 276(3) 3.0359(11) 3.0230(13) 3.0115(14) M(1)—M(1) 2.457(11) 2.5537(11) 2.5546(17) 2.545(2) M(1)—B(1) 228(2) 2.298(1 1) 2.309(16) 232(2) M(1)—B(2) 222(5) 2.361(11) 2.364(15) 2.340(19) M(1)—B(3) 225(2) 2.366(10) 2.357(16) 2.290(19) M(1)—B(4) 228(3) 2.357(10) 2.352(15) 233(2) RE(1)—B(1) 251(4) 2.737(12) 2.734(18) 274(2) RE(1)—B(2) 272(4) 2.718(13) 2.632(19) 262(2) RE(1)—B(3) 265(3) 2.655(13) 2.699(19) 274(2) RE(1)—B(4) 261(3) 2.750(14) 2.739(19) 267(3) B(1)—B(2) 161(7) 186(3) 180(4) 180(7) B(1)—B(4) 178(5) 181(2) 186(4) 183(4) B(2)—B(3) 183(5) 174(3) 174(4) 174(4) B(3)—B(3) 1.92(15) 175(4) 184(4) 177(6) B(3)—B(4) 173(7) 174(2) 174(3) 172(5) B(4)—B(4) 1.89(12) 178(3) 175(5) 182(5) 70 D. Structural Description MnB: The structure of MnB, shown in Figure 3-la, is composed of trigonal prisms of manganese atoms centered by a zigzag chain of boron atoms. The most interesting feature of the structure is the arrangement of the prisms and chains. Normally, MnB crystallizes with the F eB-type structure (Figure 3-lb), where the prisms share corners. We have isolated a variant phase of MnB that crystallizes in the CrB structure- type (Figure 3-1c) where the prisms in each layer share trigonal faces. The layers in the CrB-type MnB are more distinct, but overall, the two structure types are very similar. Actually, the volume of this MnB phase is only 0.3% less than the volume of the F eB- type. As mentioned in the introduction to this chapter, CrB-type MnB has been reported.2’ 3 However, the powder pattern in each of the previous reports also showed lines attributed to FeB-type MnB. We saw no evidence of disorder in our diffraction data suggesting a mix of the FeB and CrB-structure types, as seen by Kanaizuka.2 Manganese was the only metal atom detected by the refinement of the atom occupancy during refinement. EDS analyses on the single crystals confirm this finding. MnB4: The structure of MnB4 reported here is analogous to that first found for CrB4,20 and may be the “semi-MnB4” structure described by Burdett and Canadell.l The defining feature in the structure of MnB4 (Figure 3-2a) is a three-dimensional network of boron atoms. The network comprises boron atom rectangles lying parallel to the bc-plane that bond to boron atoms in other rectangles, extending the network in all three dimensions. The manganese atoms sit in the middle of channels formed by six neighboring rectangles. 71 .—¥ _1, .3 :1“ \ Figure 3-1. (a) Structure of CrB-type MnB with boron atom chains parallel to page. The boron atom chains are perpendicular to the page in (b) F eB-type MnB and (c) CrB-type MnB. 72 ....d .1 .% -axis (b) Sheet of RuB -2. (a) The structure of n An alternate way to consider the structure is in terms of layers. From this perspective, the structure is made of puckered hexagonal layers of boron atoms, with layers of manganese atoms centering the boron hexagons. The boron layers are puckered in the boat-type confirmation, which is very similar to the boron layers found in RuB2 (Figure 3-2b). The interlayer bonds, which would need to break to completely reduce the M., structure into separate RuB2-type layers, are longer than the intralayer bonds by about 8%. ReB2: Rhenium diboride has a structure, seen in Figure 3-3a, built along the c-axis by puckered hexagonal layers of boron atoms and metal atom layers where rhenium atoms sit directly above the boron atoms in the l, 3, and 5 positions of the hexagon in one layer and above the atoms in the 2, 4, and 6 positions in the next boron layer. The layers in ReB2 (Figure 3-3b) display hexagons in a chair conformation, in contrast to the planar hexagons in AlB2-type structures and the boat conformation for boron hexagons in RuB2-type structures. The distance between rhenium atoms in the c-direction is larger than the bonding distance for rhenium—rhenium bonds. Similarly, the distances between successive boron layers are larger than boron—boron bonding distances, suggesting that the structure is held together along the c-axis only through rhenium—boron bonds. HoMnB4 and REReB4 (RE = Dy, Er, Yb): The group 7 ternary borides we have synthesized all crystallize in the YCrB4 structure type. This structure type (Figure 3-4a) has an interesting 2-D network of boron atoms. The boron atoms form both 5- and 7- membered rings that sit in one planar layer. The metal atoms in the structure reside in their own layer, halfway between boron layers. The rare earth atoms sit below the 74 (b) Figure 3-3. (a) Structure of ReB2 and (b) an individual graphite-like layer of boron atoms. 75 Figure 3-4. (a) Structure of YCrB4-type compounds (b) View down a-axis showing alternating layers of metal atoms and boron atoms. 76 centers of the 7-membered rings, while the transition metals sit below the centers of the 5-membered rings. Generally, when the B:M ratio reaches 2.0, a layered structure results. The boron atoms in these layers typically have a hexagonal arrangement, planar or puckered conformation depending on the metal. The rare earth atoms and transition metals in the YCrB4 structure type have such different radii that the rings must also be of different sizes. The boron atoms accommodate the metals by moving from 6-membered rings to the 5- and 7-membered rings. E. Results and Discussion All of the compounds described in this chapter have been previously synthesized using traditional solid state methods. However, single crystals have not been previously isolated for all of these compounds. Our group has used the molten metal flux technique in the synthesis and crystallization of all these compounds. Gallium was the only molten metal from which the group 7 borides would grow. Reactions using aluminum, copper, indium, or tin as the flux metal did not yield borides as a product. The products from these reactions were generally binary phases of either manganese or rhenium and the flux metal. Our success using a gallium flux should be seen as a starting point for further research, because our synthesis procedures were not optimized. MnB: One of the main problems encountered in the synthesis of MnB was in picking the crystals out from the entire reaction product. The majority of the product from the initial MnB reaction was actually MnSi. The alumina crucibles used for this reaction had a cement bottom and we concluded that the gallium flux pulled silicon out of 77 the cement and into the reaction. The crystals for MnB and MnSi look nearly identical, so EDS on the crystal is necessary to ensure that only manganese and boron are present in the crystal. Reactions with identical conditions were carried out again, except in purely alumina crucibles. These reactions produced some crystals, but still in low yields. In these reactions, the major products were manganese gallides, which will be discussed in a later chapter of this work. Crystals of the gallides can also look like the MnB phase, so again it was difficult to separate boride crystals from the product mixtures. MnB4: The crystals of M4, while easier to identify, do not form single crystals. We believe that the crystals we have isolated are a series of thin plates stacked atop each other. This stacking leads to the ridged appearance of the crystals (Figure 3-5). For the “single crystal” diffraction study a specimen with the smoothest faces possible was selected. The most intense peaks were used to index the unit cell. While this technique was in no way an ideal method, the results do give some structural insight. As noted, the crystal were indexed in an orthorhombic cell to match CrB4, rather than the monoclinic cell used in previous studies on MnB.1.2"22 The previous studies found a 03° deviation from a 90° angle for the B angle when the cell was transformed to the orthorhombic 1 setting. In our crystal, the largest deviation from 90° was approximately 015°, changing slightly when different orientations of the cell were used. These findings are inconclusive because of the aforementioned imperfections of the specimen. The quality of the data from previous studies has also been questioned.1 Further research is needed to see whether MnB4 really crystallizes in the orthorhombic 1 setting, or if our metal flux synthesis is trapping a metastable phase of the compound. 78 20 1,1111 Figure 3-6. SEM micrograph of a cluster of ReBz crystals. 79 ReB2: At a lower flux reaction temperature (lOOO°C) ReB2 crystals are thin hexagonal plates. The plates turn into hexagonal prisms at a higher flux reaction temperature (1400°C), with the prisms narrowing toward each end. The hexagonal plates will often grow together, forming clusters of plates (Figure 3-6). Single plates are often available, but they can be manually broken from these clusters if needed. An optimized synthesis would help increase yields of the plates, making physical property measurements easier. Property measurements have not been carried out because of the time consuming separation of enough crystals for measurement. HoMnB4: The synthesis of HoMnB4 is very similar to W., and faces similar obstacles to single crystal isolation. Crystals of HoMnB4 (Figure 3-7) are thin plates and appear to also have the ridges seen in the WB., crystals. The diffraction data did not show any obvious signs of twinned or intergrown crystals, but the quality of the refinement data is not as high as is expected for a true single crystal. Reactions specifically targeting this compound are needed to obtain better crystals, not only for better diffraction studies, but also for other physical properties measurements, especially magnetic measurements. REReB4 (RE = Dy, Er, Yb): The ternary rhenium borides were first seen in reactions heated to 1000°C, but the crystals were very small and poorly formed. Reactions were repeated at 1400°C and the crystals grew larger and better formed despite shorter soaking and cooling times. A crystal of DyReB4 is shown in Figure 3-8. Reactions including other rare earth elements yielded similar looking products, but a short scan on the single crystal machine revealed that the rare earth tetraboride had 80 7. SEM micrograph of HoMnB4. Figure 3 Figure 3-8. SEM micrograph of DyReB4. 81 formed. Rhenium diboride and rhenium gallides, which are discussed later in this work, also crystallized from these reactions. The refinements on the single crystals of these ternary rhenium borides are consistently accurate. Problems do arise are in the displacement parameters, both isotropic and anisotropic. These problems were a bit unexpected since the crystal faces were measured, indexed, and then used to make an analytical absorption correction. Low temperature diffraction studies may be needed to reduce the thermal motion of the atoms. General Discussion: The gallium flux is a useful medium in the synthesis of group 7 borides. The exploratory nature of our research in this group changed after finding MnB and M.,, focusing more on repeating and optimizing reactions aimed at these products. While some improvements were made, there is still a great deal of synthesis refinement to be done. Further research should also be carried out, searching for the “missing” Mnng and Mn2B3 phases mentioned in the introduction to this chapter. Ternary systems with the rare earths should also continue to yield results. Even if the structures have been reported before, very few have had any physical properties measured. The large crystals grown from molten gallium would be ideal specimens to investigate. The only binary rhenium boride we focused on was ReB2, so further research into this system needs to consider Re3B and Re7B3. Exploratory work should also be carried out to see if the flux can isolate other phases that traditional syntheses can not. This work should also carry-over into the synthesis of ternary systems, especially since it has been successfully performed with rare earth metals. As with manganese, compounds have been structurally characterized, but their physical properties remain unmeasured. 82 F. Conclusions In this chapter we successfully used a molten gallium as a solvent to synthesize and grow crystals of MnB, MnB4, ReB2, HoMnB4, DyReB4, ErReB4, and YbReB4. While the structural characterization of some compounds needs additional work, the overall picture is encouraging. The synthesis of ternary borides is especially encouraging, since the technique was unsuccessful with group 6 borides. These results set a foundation for continued research into group 7 borides using the metal flux technique. 83 References 1. Burdett, J. K.; Canadell, E., GB, and MnB4: Electronic Structures of Two Unusual Systems Containing the Tetragonal Carbon Net. Inorganic Chemistry 1988, 27, 4437- 4444. 2. Kanaizuka, T., Phase Diagram of Pseudobinary CrB-MnB and MnB-FeB Systems: Crystal Structure of the Low Temperature Modification of FeB. Journal of Solid State Chemistry 1982, 41, 195-204. 3. Papesch, G.; Nowotny, H.; Benesovsky, F., Untersuchungen in den Systemen: Chrom- Bor-Kohlenstoff, Mangan-Bor-Kohlenstoff und Mangan-Germanium-Kohlenstoff. Monatsheftefur Chemie 1973, 104, 933-942. 4. Becher, H. J .; Krogrnann, K.; Peisker, E., Uber das terniire Borid Mn2AlB2. Zeitschrift filr anorganische und allgemeine Chemie 1966, 344, (3-4), 140-147. 5. Okada, S.; Atoda, T.; Higashi, 1., Structural Investigation of Cr2B3, Cr3B4, and CrB by Single-Crystal Diffractometry. Journal of Solid State Chemistry 1987, 68, 61-67. 6. Okada, S.; Atoda, T.; Higashi, 1.; Takahashi, Y., Preparation of Single Crystals of MoB2 by the Aluminum-flux Technique and Some of Their Properties. Journal of Materials Science 1987, 22, 2993-2999. 7. Higashi, 1.; Takahashi, Y.; Atoda, T., Crystal Growth of Borides and Carbides of Transition Metals from Molten Aluminum Solutions. Journal of Crystal Growth 1976, 33, 207-211. 8. Okada, S.; Kudou, K.; Lundstrfim, T., Preparations and Some Properties of W2B, 8- WB, and WB2 Crystals from High-Temperature Metal Solutions. Japanese Journal of Applied Physics 1995, 34, (1), 226-231. 9. Aronsson, B.; Backman, M.; Rundqvist, S., The Crystal Structure of Re3B. Acta Chemica Scandinavica 1960, 14, 1001-1005. 10. Placa, S. L.; Post, B., The Crystal Structure of Rhenium Diboride. Acta Crystallographica 1962, 15, 97-99. 11. Aronsson, B.; Stenberg, E.; Aselius, J ., Borides of Rhenium and the Platinum Metals. Acta Chemica Scandinavica 1960, 14, 733-741. 12. Ishii, T.; Shimada, M.; Koizumi, M.; Sakakibara, T.; Date, M., Magnetic Properties of Mn3B4 Under High Magnetic Field. Solid State Communications 1984, 51, (2), 103- 105. 13. Ishii, T.; Shimada, M.; Koizumi, M., Synthesis and Magnetic Properties of (Mn). xCr,‘)3B4 and (Mn1-xMox)3B4. Inorganic Chemistry 1982, 21, 1670-1674. 84 14. Kawano, A.; Mizuta, Y.; Takagiwa, H.; Muranaka, T.; Akimitsu, J ., The Superconductivity in Re-B System. Journal of the Physical Society of Japan 2003, 72, (7), 1724-1728. 15. Strukova, G. K.; Degtyareva, V. F.; Shovkun, D. V.; Zverev, V. N.; Kiiko, V. M.; Ionov, A. M.; Chaika, A. N., Superconductivity in the Re-B System. eprint arXiv:cond- mat/0105293 2001. 16. Sheldrick, G. M. SAINT, Version 4; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI. 17. Sheldrick, G. M. SHELXT L Structure Determination Program, Version 5.0; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI, 1995. 18. X-SHAPE, Version 2.05; STOE & Cie GmbH: 2004. 19. X-RED 32, Version 1.10; STOE & Cie GmbH: 2004. 20. Andersson, S.; Lundstrdm, T., The Crystal Structure of CrB4. Acta Chemica Scandinavica 1968, 22, 3103-3110. 21. Andersson, S., A Note on the Crystal Structure of mm. Acta Chemica Scandinavica 1969, 23, (2), 687-688. 22. Andersson, S.; Carlsson, J .-O., The Crystal Structure of M.,. Acta Chemica Scandinavica 1970, 24, (5), 1791-1799. 23. Kuz'ma., Y. B., Crystal Structure of the compound YCrB4 and its analogs. Kristallografiya 1970, 15, 372-374. 85 CHAPTER FOUR The Metal Flux Synthesis of Ruthenium Borides A. Introduction The structure and composition of many binary borides have been reported for the past half-century. However, few of the physical properties of these compounds have ever been reported. The discovery of superconductivity in MgB2 in 20011 has renewed interest in binary borides of all kinds. This finding led to a study of group 8 borides by the Kaner group in 2005, who first reported on the hardness and incompressibility of osmium diboride.2 While the structures of OsB2 and RuB2 were first reported in 1962,3 property studies have been limited to a single report on their superconductivity in 19754 and a few reports on the electronic structures of the compoundss'7 in the past decade. Chapnik8 actually called for further study on these unique compounds, and we were interested in preparing single crystals to investigate the unknown physical properties of group 8 binary borides. Physical measurements carried out on single crystals are advantageous in eliminating minor phases in powdered samples and allow researchers to search for anisotropy in the properties of the compound. Single crystals of the ruthenium borides have been isolated from arc-melted pellets, but we were interested in using the molten metal flux technique to grow higher quality crystals. Our success in synthesizing and crystallizing borides from groups 6 and 7 and reports of ternary rhodium borides grown 86 from flux9 led us to believe that the technique could also work for ruthenium borides. The reports of ternary rhodium borides from flux synthesis also inspired us to investigate ternary ruthenium borides as well. In this chapter we report on the synthesis and crystal growth of the known compounds RU7B3, RU2B3, RuB2, and RERu4B4 (RE = Y, Ce, Sm, Dy, and Yb). A new phase of ruthenium diboride, B-RuB2, crystallizing in the ReB2-type structure is presented. A brief report on two ternary borides, Pr,,(Ru4B4)y and Ndx(Ru4B4)y, with modulated structures follows as well. B. Experimental Reagents: All reagents were used as received without further purification: (i) Boron metal, 99% purity, -325 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (ii) Ruthenium metal, 99.95% pruity, -325 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (iii) Copper shot, 99% purity, -3 +14 mesh, Aldrich Chemical Company, Milwaukee, WI, (iv) Yttrium metal, 99.9% purity, -40 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (v) Dysprosium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (vi) Cerium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (vii) Samarium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (viii) Ytterbium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (ix) Erbium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (x) Lanthanum 87 metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (xi) Erbium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (xii) Praseodymiurn metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (xiii) Neodymium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (xiv) Holmium metal (filed from ingot) 99.9% purity, Chinese Rare Earth Information Center, Inner Mongolia, China, (xv) Boron metal, 99.9% purity, typically 1 um or less, Cerac Specialty Inorganics, Milwaukee, WI. Furnaces: A Lindberg Blue high-temperature, horizontal tube furnace was used with a continuous argon flow of approximately 0.1 L/min. Heating profiles for individual reactions were programmed into the accompanying Lindberg UP150 fumace controller. Thermocouples connected to the furnace controller were used to monitor fumace temperatures during reactions. The maximum operating temperature for this furnace was 1500 °C. A radio frequency (RF) furnace was constructed from an Ameritherm XP7.5CE Induction Heater and fused quartz reaction chamber. A molybdenum cylinder, machined to act as a reaction crucible holder, was used as a susceptor. A boron nitride cylinder was machined to hold the molybdenum crucible in the center of the reaction chamber. Details on the RF fumace setup are given in the appendix of this work. RF furnace temperatures were controlled manually using the Ameritherm control unit. Reaction temperatures were monitored using an Ircon SA Series Infrared Thermometer. During the course of some reactions, films deposited inside the reaction 88 chamber would prevent the IR thermometer fi'om accurately reporting furnace temperatures. In such circumstances, reaction temperatures were approximated based on power settings for the Ameritherm control unit and a series of calibration runs conducted by heating only the molybdenum cylinder. Temperatures greater than 1700 °C were easily reached with this furnace. Synthesis: Ru7B3, RuzB3, and RuB2: Boron and ruthenium powders were added in millimolar quantities, with B:M ratios from 0.25 to 4, to alumina crucibles and topped with 40 mmol of copper shot. The crucibles were capped individually with alumina lids and then place into rectangular alumina boats. The boats were loaded into the mullite tube of a commercial high temperature furnace preheated to 500 °C. The furnace was then heated to 1450 °C in 10 hours, held for 48 hours at that temperature, and then cooled to 1100 °C in 24 hours. Upon reaching 1100°C, the furnace was turned off, allowing the products to cool to 500 °C (a preset hold temperature for the fiirnace), at which time the alumina boats were removed. B-RuB2: Boron (10 mmol) and ruthenium (1 mmol) powders were added to an alumina crucible along with holmium (2 mmol) filings. Copper shot (40 mmol) was then added to the crucible, as was an alumina lid. The RF furnace was evacuated under vacuum and flushed with N2. Heating was initiated with the RF fumace under dynamic vacuum. Over 30 minutes the furnace temperature was raised to 1400 °C. After holding for 30 minutes at 1400 °C, the power to the furnace was shutoff due to mechanical problems. The furnace cooled to room temperature over the course of 1 hour, at which time the reaction crucible was removed. 89 RERu4B4 (RE = Y, Ce, Sm, Dy, Yb): Boron (1—4 mmol) and ruthenium (1 mmol) powders and rare earth metal (0.5—l mmol) filings were added to alumina crucibles. After adding copper shot (40 mmol) and alumina lids to the crucibles, the crucibles were placed in the RF furnace. The RF furnace was evacuated under vacuum and flushed with N2. Heating was initiated with the RF furnace under dynamic vacuum. Over 30 minutes the furnace temperature was raised to 1350 °C or 1400 °C. After holding for 60 minutes at the maximum temperature, the power to the furnace was shutoff and the furnace was allowed to cool to room temperature. RE,,(Ru..B.1)y (RE = Pr, Nd): Boron (3 mmol), ruthenium (1 mmol), and the rare earth metal (2.5 mmol) were added to an alumina crucible. After adding copper shot (40 mmol) and lids, the crucibles were placed in an alumina boat. The boat was loaded into the mullite tube of a commercial high temperature furnace preheated to 500 °C. The furnace was then heated to 1450 °C in 8 hours, held for 33 hours at that temperature, and then the furnace was turned off, allowing the products to cool to 500 °C (a preset hold temperature for the furnace), at which time the alumina boat was removed. Isolation from flux: When fully cooled to room temperature, crucibles were placed in individual baths of half-concentrated HNO3 in order to remove the copper flux. An overnight soak was used to completely remove the copper flux, however, many crystals were removed from the flux after a 2-3 hour soak. Extended soaking in the bath was not found to damage the crystals. The crystals were filtered from the acid bath, washed with H20, and dried with ethanol. The well-faceted crystals were easily distinguishable from the spherical elemental ruthenium that remained in most reactions. 90 The products from reactions aimed at binary borides all contained unreacted elemental ruthenium, with the amount of residual ruthenium decreasing as the B:M ratio increased. The yield of Ru7B3 from reactions with a B:M ratio of 0.25, 0.33, 0.5, and 1.0 was between 70% and 80%, based on boron. Ru7B3 was found as a minor product in the reactions with B:M ratios of 2.0, 3.0, and 4.0. RU2B3 was the major product from the B:M =2.0 reaction, with an estimated yield of 60%, based on ruthenium. RuB2 was a minor product in the B:M = 2.0 reaction, but was the major product in the B:M = 3.0 and 4.0 reactions. The yield of RuB2 was approximately 75% in the B:M = 3.0 reaction and nearly 90% in the B:M = 4.0 reaction, based on ruthenium. The new B-RuB2 phase was collected in an estimated 25% yield, based on ruthenium. The ordinary RuB2 phase was present in approximately the same ratio. The remainder of the collected product was unreacted ruthenium and boron. The RERu4B4 compounds were collected in an estimated 50% yield, based on ruthenium. The side products in the reactions producing these compounds were RERuB4, traces of REB5 and Ru7B3, and elemental ruthenium. YRu3B2 was a minor side product in the reaction producing YRu484. C. Physical Measurements Energy Dispersive Spectroscopy: Energy dispersive spectroscopy (EDS) analyses were carried out on selected crystals to determine their chemical composition. The analyses were performed with a JEOL ISM-6400 scanning electron microscope (SEM) equipped with Oxford Inca Energy Dispersive Spectroscopy (SizLi) detector and Norvar window for standardless 91 quantization of elements with Z 2 4. The crystals were affixed to an alumina sample holder with double-sided carbon tape. The EDS data were acquired at an accelerating voltage of 10kV with a 30 to 60 second accumulation time. Single-Crystal X-ray Crystallography: Single crystals were mounted on a glass fiber with super glue and their intensity data were collected on either a Bruker SMART platform CCD diffractometer, or a STOE IPDS Il diffractometer using Mo K01 radiation at 50 kV and 40 mA. Individual frames of R0733, Ru2B3,RERu4B4 (RE = Y, Ce, Sm, Yb) and RE,,(Ru4B4)y (RE = Pr, Nd) examined with the Bruker machine were collected with a 03° 0) rotation. The SMART software was used for data collection, and SAINT software was used for data extraction and reduction. After applying analytical absorption corrections, structure solution and refinement were completed using direct methods and the SHELXTL suite of programs. Samples examined with the STOE (RuB2, and DyRu4B4) had individual fiames collected on a 34 cm image plate with a 60 second exposure time and a 10° to rotation. The X-SHAPE and X-RED-32 software packages were used for data extraction and reduction and to apply an analytical absorption correction. Direct methods and the SHELXTL suite were used to solve and refine the structures. The crystal structure refinement data for Ru7B3 are found in Table 4-1. Previously reported10 atomic parameters were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 4-2. Anisotropic displacement parameters for the atoms are found in Table 4-3. Selected bond lengths in RU7B3 and a count of those bonds are listed in Table 4-4. 92 The crystal structure refinement data for Ru2B3 are found in Table 4-5. Previously reported” atomic parameters were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 4-6. Anisotropic displacement parameters for the atoms are found in Table 4-7. Selected bond lengths in Ru2B3 and a count of those bonds are listed in Table 4-8. The crystal structure refinement data for RuB2 are found in Table 4-9. Previously reported3 atomic parameters were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 4-10. Anisotropic displacement parameters for the atoms are found in Table 4-11. Selected bond lengths in Ru2B3 and a count of those bonds are listed in Table 4-12. The crystal structure refinement data for B-RuB2 are found in Table 4-13. Atomic parameters for ReB2l2 were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 4-14. Anisotropic displacement parameters for the atoms are found in Table 4-15. Selected bond lengths in Ru2B3 and a count of those bonds are listed in Table 4-16. The crystal structure refinement data for YRu4B4 and CeRu4B4 are found in Table 4-17, in Table 4-18 for SmRu484 and DyRu4B4, and in Table 4-19 for YbRu434. Previously reported atomic parameters for LuRu4B4l3 were used as a starting point for the refinement of the structure. The atomic positions and isotropic displacement parameters are listed in Table 4-20. Anisotropic displacement parameters for the atoms are found in Table 4-21. The bond distances for RERu4B4 (RE = Y, Ce, Sm, Dy, Yb) are listed in Table 4-22. 93 Initial indexing of the single crystal data for RE,((Ru.1B4)y (RE = Pr, Nd): suggested that these compounds crystallized with the LaRmB4 structure.14 However, during refinement, it became obvious that this suggestion was incorrect. When examining the reciprocal lattice, two distinct lattices became visible along the c-axis. One lattice corresponds to a c-axis length of 3.67 A and the other corresponds to a length of 4.04 A. While we found no reports of incommensurate ruthenium borides, several reports on 15, 16 incommensurate iron borides with similar cell (and substructure) parameters exist. Further data collection is necessary for complete structural characterization. 94 Table 4-1. Crystal data and structure refinement for Ru7B3. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 28.23° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2sigma(1)] R indices (all data) Absolute structure parameter Extinction coefficient Largest diff. peak and hole 739.92 293(2) K 0.71073 A Hexagonal P63mc a = 7.4570(11) A or: 900 b = 7.4570(11) A B= 90° c = 4.7140(9) A y= 120o 227.01(6) A3 2 10.825 g/cm3 22.466 mm“ 646 0.052 x 0.052 x 0.326 mm3 3.15 to 28.23° -9ShS9,-9_<_I(S9,-6_<_IS6 2328 226 [R(int) = 0.0316] 99.2 % F ull-matrix least-squares on F 2 226/ 1 / 23 1.273 R1 = 0.0116, WR2 = 0.0288 R1 = 0.0116, WR2 = 0.0288 0.1(4) 0.0254(8) 0.512 and -0.573 e.A'3 R1 = 2 MRI — chll /2 IFol and wR2 = [z (1F.2 - F31 )2 / 5; (WF02)2]V2 95 Table 4-2. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for RU7B3. x y z U(eq) Ru( 1) 3333 6667 9527(3) 6(1) Ru(2) 1226(1) 8774(1) 7754(1) 5(1) Ru(3) 5429(1) 4571(1) 9623(1) 7(1) B(l) 1891(6) 8109(6) 11911(l8) 9(2) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 4-3. Anisotropic displacement parameters (Azx 103) for Ru7B3. ull U22 [)33 U23 ul3 ulz Ru(l) 6(1) 6(1) 6(1) 0 0 3(1) Ru(2) 4(1) 4(1) 6(1) 0(1) 0(1) 2(1) Ru(3) 7(1) 7(1) 7(1) 0(1) 0(1) 3(1) 13(1) 6(2) 6(2) 12(4) 1(2) -1(2) -1(3) The anisotropic displacement factor exponent takes the form: -21t2[ h2 a"‘2Ull + + 2 h k a” b" U12 ] 96 Table 4-4. Selected bond distances (A) for Ru7B3. Rul Bl 3x 2.1756(2) Ru2 B1 1x 2.1395(3) Ru2 B1 2x 2.1825(2) Ru3 B 1 2x 2.1637(2) Rul Ru3 3x 2.7075(4) Rul Ru3 3x 2.8105(4) Rul Ru2 3x 2.8472(3) Rul Ru3 3x 2.8852(4) Ru2 Ru2 2x 2.7427(4) Ru2 Ru3 2x 2.7913(3) Ru2 Ru2 4x 2.8395(4) Ru2 Rul 1x 2.8472(3) Ru2 Ru3 2x 2.8539(4) Ru3 Ru3 2x 2.6049(4) Ru3 Rul lx 2.7075(3) Ru3 Ru3 2x 2.7680(4) Ru3 Ru2 2x 2.7913(3) Ru3 Rul 1x 2.8105(4) Ru3 Ru2 2x 2.8539(4) Ru3 Rul 1x 2.8852(4) 97 Table 4-5. Crystal data and structure refinement for Ru2B3. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 27.76° Refinement method Data / restraints / parameters Goodness-of-fit on F 2 Final R indices [I>23igma(l)] R indices (all data) Extinction coefficient Largest diff. peak and hole 234.57 293(2) K 0.71073 A Hexagonal P63/mmc a = 2.9029(4) A or= 90° b = 2.9029(4) A 8: 90° c=12.814(3)A y=120° 93.51(3) A3 2 8.331 g/cm3 15.613 mm'1 206 0.038 x 0.084 x 0.084 mm3 3.18 to 27.76° -3ShS3,-3Sk£3,-16SIS 16 899 65 [R(int) = 0.0327] 95.4 % Full-matrix least-squares on F2 65 / 0/ 10 1.211 R1 = 0.0148, WR2 = 0.0353 R1 = 0.0163, WR2 = 0.0366 0.169(13) 0.751 and -0.503 e.A'3 RI = z llFol — chll / z W and we = [2 (IF: — 18.21 )2 / 2 mafia” 98 Table 4-6. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (Azx 103) for Ru2B3. X y Z U(CQ) Ru(l) 6667 3333 1400(1) 3(1) B(l) 6667 3333 9697(7) 4(2) B(2) 6667 3333 7500 5(3) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 4-7. Anisotropic displacement parameters (Azx 103) for Ru2B3. ull U22 u33 U23 ul3 ul2 Ru(l) 3(1) 3(1) 1(1) 0 0 2(1) 8(1) 5(3) 5(3) 3(4) 0 0 2(1) B(2) 5(4) 5(4) 5(6) 0 0 2(2) The anisotropic displacement factor exponent takes the form: -21t2[ h2 a*2U1 ‘ + + 2 h k a* b* U12 ] Table 4-8. Selected bond distances (A) for Ru2B3. Rul 131 1x 2.1821(4) Rul Bl 3x 2.1871(3) Rul BZ 3x 2.1901(3) B1 Bl 3x 1.8474(2) Bl Rul 1x 2.1821(4) Bl Rul 3X 2.1871(3) 82 Rul 6x 2.1901(3) 99 Table 4-9. Crystal data and structure refinement for RuB2. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 36.3 8° Refinement method Data / restraints / parameters Goodness-of-fit on F7- Final R indices [I>28igma(1)] R indices (all data) Extinction coefficient Largest diff. peak and hole 122.69 293(2) K 0.71073 A Orthorhombic Pmmn a = 4.6322(9) A or= 90° b = 2.8542(6) A 8: 90° c = 4.0292(8) A y = 90° 53.271(19) A3 2 7.649 g/cm3 13.716 mrn'l 108 0.031 x 0.040 x 0.048 mm3 5.06 to 36.38° -7ShS7,-4$k$4,-6SIS6 863 165 [R(int) = 0.0595] 100.0 % F ull-matrix least-squares on F2 165 / 0/ 12 1.210 R1 = 0.0157, WR2 = 0.0341 R1 = 0.0165, WR2 = 0.0344 0.200(16) 1.204 and -1.l41e.A'3 R1 = 2 “FA — 1F.” / z |F0| and wR2 = [z (IF,2 — 18.21 )2 / z (wF,2)2]'” 100 Table 4-10. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (Azx 103) for RuB2. x y 2 U(CCI) Ru(l) 2500 2500 6512(1) 1(1) 3(1) 5550(8) -2500 8615(6) 4(1) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 4-11. Anisotropic displacement parameters (Azx 103) for RuB2. U” U22 U33 U23 U13 U12 Ru(l) 1(1) 1(1) 1(1) 0 0 0 B(l) 4(1) 4(1) 3(1) 0 0(1) 0 The anisotropic displacement factor exponent takes the form: -21t2[ h7- a*2U” + + 2 h k a* b* 1112 ] Table 4-12. Selected bond distances (A) for RuB2. Rul 81 2x 2.1612(4) Rul 81 4x 2.1796(3) Rul 81 2x 2.2547(4) 81 81 1x 1.8067(4) 81 81 2x 1.8818(3) 81 Rul 1x 2.1612(4) 81 Rul 2x 2.1796(3) 81 Rul 1x 2.2547(4) 101 Table 4-13. Crystal data and structure refinement for B-RuB2. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 27.73° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2sigma(1)] R indices (all data) Extinction coefficient Largest diff. peak and hole 122.69 273(2) K 0.71073 A Hexagonal P63/mmc a = 2.9142(4) A or= 900 b = 2.9142(4) A 0: 90° C = 7.283(2) A y = 120° 53.56509) A3 2 7.607 g/cm3 13.640 mm" 108 0.008 x 0.084 x 0.090 mm3 5.60 to 27.73° -3Sh$3,-3Sk$3,-9SIS9 475 38 [R(int) = 0.0276] 94.7 °/o Full-matrix least-squares on F 2 38 / 0 / 7 0.936 R1 = 0.0239, WR2 = 0.0820 R1 = 0.0276, WR2 = 0.0880 007(4) 0.789 and -1.243 e.A'3 R1 = 2 “F01 — chlI / Z W and wR2 = [2 (IF,2 — Ffl )2 / 2 008,621"2 102 Table 4-14. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (A2x 103) for B-RuB2. x y z U(eq) Ru(l) 3333 6667 7500 5(1) B(2) 6667 3333 5590(30) 8(4) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 4-15. Anisotropic displacement parameters (Azx 103) for B-RuB2. ull U22 1133 U23 ul3 ulZ Ru(l) 4(1) 4(1) 6(1) 0 0 2(1) B(2) 8(7) 8(7) 7(8) 0 0 4(3) The anisotropic displacement factor exponent takes the form: -21t2[ h2 a*2U” + + 2 h k a* 8* U12 ] Table 4-16. Selected bond distances (A) for B-RuB2. Rul B2 6x 2.1838(3) Rul B2 2x 2.2493(7) B2 B2 3x 1.8882(2) B2 Rul 3x 2.1838(3) BZ Rul 1x 2.2493(7) 103 Table 4-17. Crystal data and structure refinement for RERu4B4 (RE= Y, Ce). Formula Formula weight Temperature Crystal system Space group Unit cell dimensions Volume Z, Density (calculated) Absorption coefficient F(000) Crystal size, mm Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to 0max Refinement method Data / restraints / parameters Goodness-of-fit on F 2 Final R indices [I>20(I)] R indices (all data) Extinction coefficient Largest diff. peak & hole YRu4B4 536.43 297(2) K Tetragonal 141/acd a = 7.4525(14) A c = 14.988(6) A 832.4(4) A3 8, 8.560 g/cm3 27.561 mm'1 1880 0.050 x 0.150 x 0.150 4.73 to 28.3l° -9 S h _<_ 9. -9 S k S 9. -18 S l S 19 3793 253 [R(int) = 0.0413] 96.9 % CeRu4B4 587.64 297(2) K Tetragonal 141/acd a = 7.4744(4) A c = 15.0642(19) A 841 .59(12) A3 8, 9.276 g/cm3 24.417 mm'1 2032 0.028 x 0.066 x 0.066 4.71 to 28.30° -9 S h S 9. -9 S k S 9. -19 S l S 18 3898 257 [R(int) = 0.0317] 97.0 % F ull-matrix least-squares on F2 253 / 0 / 23 1.337 R1 = 0.0271, wR2 = 0.1355 R1 = 0.0274, wR2 = 0.1358 0.0053(8) 2.084 & -l .244 e.A'3 257 / 0 / 23 1.013 R1 = 0.0185, wR2 = 0.0599 R1 = 0.0193, wR2 = 0.0604 0.00236(18) 1.106 & -0.916 e.A'3 RI = z 181 — chll / z 181 and sz = [z (“.02 - r121 )2 I 2: 012.2121“ 104 Table 4-18. Crystal data and structure refinement for RERu4B4 (RE= Sm, Dy). Formula Formula weight Temperature Crystal system Space group Unit cell dimensions Volume Z, Density (calculated) Absorption coefficient F(000) Crystal size, mm Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to emax Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2o(I)] R indices (all data) Extinction coefficient Largest diff. peak & hole SmRu4B4 597.87 297(2) K Tetragonal I4./acd a = 7.4801(4) A c = 15.0375(l8) A 841.38(12) A3 8, 9.440 g/cm3 27.761 mm‘1 2064 0.050 x 0.150 x 0.150 4.71 to 28.97° -10 S h S 10, -10 S k S 9. -20 S l S 19 4297 278[R(int) = 0.1325] 97.5 % DyRu4B4 610.02 100(2) K Tetragonal 141/acd a = 7.4195(10) A c = 14.930(3) A 821.9(2) A3 8, 9.860 g/cm3 32.109 mm"1 2096 0.070 x 0.079 x 0.080 4.75 to 36.59° -12 S h _<_ 12, -9 S k S 12, -24 S l S 20 6128 511 [R(int) = 0.0760] 99.0 % F ull-matrix least-squares on F2 278 / 0 / 23 1.202 R] =0.0304, wR2 =0.0928 R1 = 0.0304, wR2 = 0.0928 0.0038(4) 2.288 & -2.497 e.A‘3 511 / 0 / 23 1.317 R1 = 0.0450, wR2 = 0.1397 R1 = 0.0491, wR2 = 0.1733 0.0039(6) 6.458 & -12.129 e.A'3 RI = 2 118.1 - 1F.” / z rm and wR2 = [>3 (IRE — FA )2 / 2 682121": 105 Table 4-19. Crystal data and structure refinement for YbRu4B4. Formula weight Temperature Wavelength Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F(000) Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 29. 15° Refinement method Data / restraints / parameters Goodness-of-fit on F 2 Final R indices [I>2sigma(1)] R indices (all data) Extinction coefficient Largest diff. peak and hole 620.56 297(2) K 0.71073 A Tetragonal 141/acd a = 7.418500) A or= 90° b = 7.4185(10) A 0= 90° c = 14.9570) A y = 90° 823.2(2) A3 8 10.015 g/cm3 36.626 M'1 2128 4.75 to 29.15° -10$h59,-9Sk59,-20$1$19 4234 272 [R(int) = 0.0369] 96.1 °/o F ull-matrix least-squares on F 2 272 / 0 / 23 0.945 R1 = 0.0183, WR2 = 0.0425 R1 = 0.0188, WR2 = 0.0427 0.0054(2) 0.957 and -0.969 e.A'3 R1 = Z IIFol — IFcll / Z IE1 and wR2 = [z (IF,2 — F31 )2 / 2 (1111252)"2 106 Table 4-20. Atomic coordinates ( x 104) and equivalent isotropic displacement parameters (A2x 103) for RERmB4 (RE = Y, Ce, Sm, Dy, Yb). x y 2 U(CCI) Y(1) 0 2500 1250 8(1) Ru(l) -3519(1) 3654(1) 1867(1) 6(1) B(l) -3329(12) 3920(13) 433(7) 9(2) Ce(l) 0 2500 1250 4(1) Ru(l) -3520(1) 1355(1) 1864(1) 3(1) B(l) -3533(11) 4174(10) 2068(6) 5(1) Sm(1) 0 2500 1250 2(1) Ru(l) 3844(1) 1033(1) 633(1) 2(1) 3(1) 1675(14) -1058(13) 438(8) 3(2) Dy(l) 0 2500 1250 5(1) Ru(l) 3846(1) 3982(1) 632(1) 4(1) B( l) 6662(15) 3889(15) 425(8) 4(2) Yb(l) 0 2500 1250 3(1) Ru(l) 3504(1) 1347(1) 1868(1) 2(1) B(l) 1410(10) 836(11) 2941(6) 4(1) U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. 107 Table 4-21. Anisotropic displacement parameters (Azx 103) for RERmB4 (RE = Y, Ce, Sm, Dy, Yb). ull U22 {)3 U23 [113 1112 Y(1) 8(1) 8(1) 8(1) 0 0 2(1) Ru(l) 5(1) 6(1) 6(1) 0(1) -10) 0(1) 3(1) 0(4) 18(5) 9(4) 13(3) -8(4) 4(3) Ce(1) 4(1) 4(1) 3(1) 0 0 -1(1) Ru(l) 4(1) 3(1) 2(1) 0(1) -1(1) 0(1) B( 1) 9(4) 1(3) 3(3) 0(3) -10(3) 1(3) Sm(1) 3(1) 3(1) 0(1) 0 0 0(1) Ru(l) 3(1) 3(1) 1(1) -10) 0(1) 0(1) 8(1) 3(4) 5(4) 1(3) 6(3) -1(3) 1(3) Dy(l) 3(1) 3(1) 7(1) 0 0 1(1) Ru(l) 3(1) 3(1) 5(1) 0(1) 0(1) 0(1) B( 1) 5(4) 7(4) 0(4) 8(3) 3(3) 2(3) Yb(1) 4(1) 4(1) 3(1) 0 0 1(1) Ru(l) 3(1) 2(1) 1(1) 0(1) 1(1) 0(1) 3(1) 4(3) 3(3) 5(3) 3(3) 4(3) -4(3) The anisotropic displacement factor exponent takes the form: -21t2[ h2 a"‘2Ull + + 2 h ka“ 8* 1112] 108 Table 4-22. Bond distances (A) for RERu4B4 (RE = Y, Ce, Sm, Dy, Yb). YRu484 CeRu4B4 SmRu484 DyRu4B4 YbRu4B4 RE—Ru 2.9109(9) 2.9170(6) 2.9315(7) 2.8981(9) 2.8884(9) RE—B 2.962(7) 2.983(7) 2.973(10) 2.952(1 1) 2.9467(9) 3.006(10) 3.031(9) 3.029(12) 2.972(13) 3.0025(9) Ru—B 2.127(10) 2.130(8) 2.138(10) 2.114(11) 2.1102(9) 2.163(11) 2.176(9) 2.165(12) 2.165(11) 2.1462(9) 2.216(10) 2.258(8) 2.229(10) 2.185(11) 2.2075(9) 2.273(10) 2.259(8) 2.273(1 1) 2.265(10) 2.2622(9) 2.269(10) 2.259(8) 2.279(1 l) 2.284(13) 2.2655(9) Ru—Ru 2.7089(11) 2.7087(9) 2.7103(1 l) 2.6989(14) 2.7100(9) 2.7612(13) 2.7879(11) 2.7687(14) 2.7484(16) 2.7511(9) 2.7979(12) 2.7980(10) 2.7943(13) 2.7869(15) 2.8024(9) 2.9770(14) 2.9876(1 1) 2.9316(7) 2.8981(9) 2.9529(9) 3.1047(12) 3.1178(10) 3.1246(13) 3.0910(16) 3.0824(9) B—B 1.79(2) 1.793(18) 1.81(2) 1.78(2) 1.810(10) 109 D. Structural Description R0783: The structure of Ru7B3 (Figure 4-la) comprises ruthenium tetrahedra and octahedra and isolated boron atoms.lo The structure can also be described with a more complex building unit known as a stellaquadrangula.l7 The stellaquadrangula (Figure 4-1b) comprises a central tetrahedron sharing each face with another capping tetrahedron. The central tetrahedron in the stellaquadrangula has a corner pointing into the page, and the fourth capping tetrahedron has a corner coming out of the page. In Ru7B3, the stellaquadrangula share comers with the octahedra to form a 3-D network of ruthenium atoms. The boron atoms reside in cavities in the framework. Ru2B3: A structural description of Ru283 was first reported in 1962. The structure (F igurer 4-2a) is made of alternating metal and boron atom layers. The metal atoms are hexagonally close-packed. The boron atoms form two distinct layers, one with puckered hexagonal rings (Figure 4-2b), and the other with a hexagonally packed layer of non-bonding atoms (Figure 4-2c). The structure is quite different from the Cr2B3 structure reported in Chapter 2. In the Ru2B3 structure, the boron atoms form 2-D networks instead of the triple chains seen in Cr2B3 and expected based on the B:M ratio of 1.5. A previous report'8 on Ru2B3 suggests that the larger ruthenitun atoms would force unreasonably short boron-boron bonds should the compound crystallize with the Cr2B3 structure. The puckered layers in Ru2B3 distance the boron atoms from each other sufficiently. RuB2: The structure of RuB2, first reported in 1962,3 contains corrugated layers of boron atoms (Figure 4-3a). The corrugated boron rings are limited to RuB2 and OsB2 among diborides. The ruthenium atoms in the structure appear to be two separate layers, 110 (b) Figure 4-1. (a) Structure of Ru7B3 and (b) the stellaquadrangula building unit. 111 ‘Ru .8 g \ B\2—B2 2.9029A ‘ O (b) (c) Figure 4-2. (a) Structure of Ru2B3 and the (b) puckered boron layer and (c) planar layer of boron atoms. 112 (b) Figure 4-3. Structure of RuBz crystallizing with the (a) RuB2-type and (b) ReB2- type structures. 113 as they alternately center boron rings above and below one metal atom layer. Recent quantum mechanical studies suggest that the corrugated layers are a result of limited electron donation from the ruthenium atoms to the boron layers.7 B-RuB2: This phase of RuB2 crystallizes in the ReB2-structure type12 described in Chapter 3. In this newly discovered phase, the boron atoms are in puckered hexagonal rings, with the “chair” conformation. In the known RuB2, the layers are more corrugated, with the boron atoms sitting in the “boat” conformation of a hexagonal ring. B-RuB2, shown in Figure 4-3b, crystallizes in the hexagonal space group P63/mmc, rather than the orthorhombic Pmmn space group of the known RuB2. RERu484 (RE= Y, Ce, Sm, Dy, Yb): All of these compounds crystallize in the LuRmB4 structure type13 (Figure 4-4). The ruthenium atoms in these compounds form tetrahedra that bond to each other in a zigzag fashion. A distorted NaCl lattice is formed as the centers of the ruthenium tetrahedra reside on the anion sites and the rare earth atoms reside on the cation sites. Boron atoms are found in pairs throughout the voids of this distorted face-centered cubic lattice. 114 Figure 44. Structure of RERu4B4 (RE = Y, Ce, Sm, Dy, Yb) shown down the b-axis. 115 E. Results and Discussion After initially synthesizing RuB2 from a copper flux reaction in the RF firrnace, we decided to do a study on the ruthenium borides that would grow from a copper flux at varying BzRu ratios. Seven reactions with varying BzRu ratios from 0.25 to 4.0. Ru7B3 crystallized from all metal rich reactions and traces of the compound were still found in reactions with BzRu ratios up to 2.0. Ru2B3 was more limited, crystallizing only when the BzRu ratio was 2.0. Crystals of RuB2 were found beginning in the reaction with a BzRu ratio of 2.0 and became the major product for B:M = 3.0 and B:M = 4.0 reactions. Elemental ruthenimn was found in all products, though the amount decreased as the BzRu ratio increased. Surprisingly, no Ru) (B3 or RuB 1,) crystals were found during the study. Reactions targeted specifically at these reported phases yielded mostly Ru7B3 and Ru2B3. Further research using more varied BzRu ratios and different heating profiles should be conducted before the flux synthesis of more ruthenium boride phases can be discounted. To see further varying of B:M ratios is necessary, we need only look at the synthesis of B-RuB2. Our study on binary ruthenium borides would have produced this phase had we extended the BzRu ratio to 10.0. The initial synthesis of B-RuB2 was quite unexpected, as the reaction was aimed at producing an analog to the TthBro phases found by the Jeitschko group.l9 Finding that RuB2 can crystallize with the ReB2 structure should not be quite as surprising. There are a couple of reports of molybdenum- and tungsten-substituted RuB2 and OsB2 crystallizing in the ReB2 structure.” 2' Despite several reports on the stability of the RuB2 structure versus the A1B2-type structure} 7 we found no reports comparing the 116 (a) 100 11m 0’) Figure 4-5. SEM micrographs of (a) RuB2 and (b) B-RIIBz. 117 RuB2 and ReB2 structures. It would be interesting to conduct a study on both RuB2 phases to see if the structure really depends on how many electrons the ruthenium atoms donate to the boron layers. Crystals of RuB2 and B-RuB2 are shown in Figures 4-5a and 4-5b, respectively. Synthesis of the RERmB4 compounds was fairly easy for most rare earths with the aid of the flux. In addition to the compounds reported here, LaRu4B4 and ErRu4B4 were also synthesized. Most reactions containing a rare earth metal, ruthenium and boron, regardless of the stoichiometry, would produce a RERU4B4 compound. Unfortunately, RERuB4 compounds also crystallized along with the RERu4B4 compounds, sometimes with very similar crystal morphology. Figure 4-6 clearly displays the similar morphology of CeRu4B4 and CeRuB4 crystals. The synthesis of incommensurate ruthenium borides was very interesting. The previous report on LuRu4B4 compoundsI3 did not mention any problems in synthesizing Pr or Nd members of the series. Because we were able to synthesize the Ce member of the series, we feel the size of the rare earth should not be a factor in determining whether or not the structure is incommensurate. Heating profiles do seem to play a decisive role in determining which phase is produced. The reaction temperature producing incommensurate phases was at least 50°C greater than in reactions producing the commensurate phases. The reaction time for the reactions yielding incommensurate phases was also quite extended when compared to the reaction times for reactions yielding the commensurate phases. It should be noted, however, that reactions at lower temperatures and run for a shorter duration failed to produce any ternary borides for either Pr or Nd. 118 -1_OO 1117—1 (5) Figure 4-6. SEM micrographs of (a) CeRu434 and (b) CeRuB4. 119 F. Conclusions Presented here are the details of the copper flux synthesis and crystallographic studies on single crystals of the known binary ruthenium borides Ru7B3, Ru2B3, and RuB2. A new binary phase, B-RuB2, was synthesized and crystals of the compound were grown from a copper flux. The crystallographic data and atomic positions for B-RuBz are reported here for the first time. We successfully targeted and synthesized YRu434, CeRu484, SmRu4B4, DyRu4B4, and YbRu4B4. Single crystals of these compounds, all known compounds of the LuRu4B4-structure type, were grown from a copper flux. The first report of incommensurate ternary ruthenium borides is also presented here. We have learned that varying reaction parameters can have quite an effect on compounds isolated from the flux. For instance, by increasing the BzRu ratio to 10.0 a new phase of ruthenium diboride, B-RuB2 was isolated. Additionally, increased flux reaction temperatures also play a role in the formation of incommensurate phases of PrRu4B4 and NdRu4B4. Further investigations into the synthesis adjustments that create these variations should be able to pinpoint a stronger cause and effect relationship to the molten flux synthesis techniques. 120 References 1. Nagamatsu, J.; Nakagawa, N.; Muranaka, T.; Zenitani, Y.; Akimitsu, J., Superconductivity at 39K in Magnesium Diboride. 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Pallas, A.; Larsson, K., Structure Determination of the 4d Metal Diborides: A Quantum Mechanical Study. Journal of Physical Chemistry B 2006, 110, 5367-5371. 8. Chapnik, I. M., On the Possibility of Semiconducting Properties in Diborides ReB2, TcB2, OsB2, and RuB2. Physica Status Solidi 1977, A41, K71-K73. 9. Shishido, T.; Ye, J .; Sasaki, T.; Note, R.; Obara, K.; Takahashi, T.; Matsumoto, T.; F ukuda, T., Growth of Single Crystals in the Systems with R-Rh-B and r-Rh-B-C (R= Rare Earth Element) from Molten Copper Flux. Journal of Solid State Chemistry 1997, 133, 82-87. 10. Aronsson, B., The Crystal Structure of Ru7B3. Acta Chemica Scandinavica 1959, 13, 109-114. 11. Lundstrfim, T., The Structure of Ru2B3 and WB20, as determined by single-crystal diffractometry, and some notes on the W-B system. Arkivfbr Kemi 1969, 30, 115-127. 12. Placa, S. L.; Post, B., The Crystal Structure of Rhenium Diboride. Acta Crystallographica 1962, 15, 97-99. 13. Johnston, D. C., Superconductivity in a New ternary Structure Class of Boride Compounds. Solid State Communications 1977, 24, 699-702. 121 l4. Grilttner, A.; Yvon, K., Lanthanum Ruthenium Boride, LaRu4B4. Acta Crystallographica 1979, B35, 451-453. 15. Bezinge, A.; Yvon, K.; Braun, H. F .; Muller, J .; Nissen, H.-U., Ndee4B4: A composition-modulated compound with incommensurate composite crystal structure. Physical Review B 1987, 36, (3), 1406-1414. 16. Gubich, I. B.; Zavalii, P. Y.; Kuz'ma, Y. B., H020(Fe4B4)17 Boride- A New Representatuve of Disproportionate Structures. Inorganic Materials 1993, 29, (2), 301- 303. 17. Nyman, H.; Andersson, S., The Stella Quadrangula as a Structure Building Unit. Acta Crystallographica 1979, A35, 934-937. 18. Aronsson, B., The Crystal Structure of RuB2, OsB2, and IrBL35 and Some General Comments on the Crystal Shemistry of Borides in the Composition Range MeB-MeBg. Acta Chemica Scandinavica 1963, 17, 2036-2050. 19. Konrad, T.; Jeitschko, W., The Thorium transition Metal Borides Th2TBro (T = Fe, Co, Ni) with a Structure Very Similar to that of CaB(,. Zeitschriftfur Naturforschung 1995, 50b, 1195-1199. 20. Rogl, P.; Nowotny, H.; Benesovsky, F ., Komplexboride mit ReB2-Struktur. Monatsheftefu'r Chemie 1970, 101, 27-31. 21. Rogl, P.; Rudy, B., New Complex Borides with ReB2- and M02IrB2-type Structure. Journal of Solid State Chemistry 1978, 24, 175-181. 122 Chapter Five Gallium-Rich Gallides Isolated as By-Products from Molten Flux Reactions Containing Boron A. Introduction One of the main obstacles to overcome in the molten flux technique is the formation of binary phases containing one reagent and the flux metal." 2 These binaries are often so stable that it is nearly impossible to form the intended products. During the course of our research on synthesizing borides from a metal flux we frequently encountered this problem due to the limited solubility of boron in the flux metals. The other reagents in the reaction would react with the flux metal before boron had a chance to dissolve in the flux. This was especially true when gallium was used as the flux metal. We have had a good deal of success in synthesizing borides from a gallium flux, producing Cr2B3, CrB2, MoB, WB, MnB, MnB4, ReB2, and HoMnB4. However, even in reactions producing these borides, gallides were a side product, if not the main product. Many of the gallides we have encountered throughout our research, such as V2Ga5,3 MGa4 (M = Cr, Mn),4 MGa3 (M = Fe, Co, Ru),5 and Ni2Ga3,6 have been known for some time and have been well studied. Given the amount of research done on gallium systems, we were fairly surprised to find several binary gallides that had little, if any structural characterization. In this chapter we will discuss the synthesis, single crystal growth, and 123 characterization of gallium-rich compounds from the Mn—Ga, Re—Ga, and Ni—Ga systems. B. Experimental Reagents: All reagents were used as received without further purification: (i) Boron metal, 99% purity, -325 mesh, Cerac Specialty Inorganics, Milwaukee, WI, (ii) Rhenium powder, 99.99% purity, Strem Chemicals, Newburyport, MA, (iii) Manganese powder, 99.9% purity, -50 mesh, Aldrich Chemical Company, Milwaukee, WI, (iv) Gallium 3-5 mm shot, 99.999% purity, Plasmaterials, Liverrnore, CA, (v) Tungsten metal, 99.9% purity, Cerac Specialty Inorganics, Milwaukee, WI, (vi) Nickel metal powder, 98-99% purity, -325 mesh, E.H. Sargent & Company. Furnaces: Commercial tube furnaces from Applied Test Systems, Inc. were used to heat reactions sealed in quartz tubes. Furnace controllers from the Omega Company were used to program heating profiles for individual reactions. Furnace temperatures were monitored during reactions by thermocouples connected to the Omega controllers. To extend the life of the fumaces, the operating temperature for prolonged heating was limited to 1000 °C. Synthesis and Isolation: MnGa4,65: Boron and manganese powder were mixed and added to alumina crucibles in millimolar quantities in boron-to-manganese ratios between 2:1 and 5:1. Pieces of gallium shot totaling between 1.5 g and 2.5 g were then placed in the crucibles. The alumina crucibles were then placed in 13 mm diameter quartz tubes and evacuated 124 under vacutun to a pressure near 10'4 Torr. The quartz tubes were then sealed using an oxygen-acetylene torch. The quartz tubes were placed in mullite tubes, then heated in commercial tube furnaces under heating profiles that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to room temperature in 60 hours. After cooling, the quartz tubes were opened and the alumina crucibles were placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed after an overnight soak, but longer soaks were used without damage to the recovered product. Silver, octahedral crystals were recovered in 50-60% yields, based on manganese. Elemental analysis performed by Energy Dispersive Spectroscopy (EDS) using a Scanning Electron Microscope (SEM) showed that manganese and gallium were the only elements present in the crystals. M4 and MnGa4 were side products in these reactions. Elemental boron also remained in the collected products ReGa4,5: Boron and rhenium powder were mixed and added to alumina crucibles in millimolar quantities in boron-to-rhenium ratios between 2:1 and 5:1. Pieces of gallium shot totaling between 1.5 g and 2.5 g were then placed in the crucibles. The alumina crucibles were then placed in 13 mm diameter quartz tubes and evacuated under vacuum to a pressure near 10'4 Torr. The quartz tubes were then sealed using an oxygen- acetylene torch. The quartz tubes were placed in mullite tubes and then heated in commercial tube furnaces under heating profiles that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to 125 cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to room temperature in 60 hours. After cooling, the quartz tubes were opened and the alumina crucibles were placed in a half-concentrated HCl bath in order to remove the excess gallium. Most of the gallium was removed after an overnight soak, but longer soaks were used without damage to the recovered product. Silvery, octahedral crystals were recovered in 50-60% yields. Elemental analysis performed by EDS using an SEM showed that rhenium and gallium were the only elements present in the crystals. ReB2 was a side product in these reactions. N1057Ga4,43: Boron (7.5 mmol), nickel (0.5 mmol), and tungsten (1 mmol) powders were mixed and added to an alumina crucible along with pieces of gallium shot totaling 1.45 g. A quartz filter was placed in the crucible which was then placed in a 13 mm diameter quartz tube, evacuated under vacuum to a pressure near 10'4 Torr, and sealed using an oxygen-acetylene torch. The tube was then heated in a commercial tube furnace under a heating profile that increased the furnace temperature to 1000 °C in 10 hours, held the temperature constant for 48 hours, allowed the furnace to cool to 850 °C in 5 hours, held the temperature constant for an additional 48 hours, and then allowed the furnace to cool to 250 °C in 60 hours. The quartz tube was removed from the furnace at 250 °C and centrifuged to remove excess gallium. After centrifugation, the tube was opened and the crucible was placed in a bath of 5M 12 in DMF in order to remove the remaining gallium flux. An overnight soak was found to be insufficient for removing all of the gallium, so soaking was continued for an additional 2 days. A subsequent investigation still found remaining gallium, so an overnight soak in half-concentrated HCl was used to finally remove all 126 gallium. Silver, rectangular prisms are a minor product (IO-20% yield). Ni2Ga3 and WB were side products in this reaction. Elemental boron was also present in the collected product. C. Physical Measurements Energy Dispersive Spectroscopy: Energy dispersive spectroscopy (EDS) analyses were carried out on selected crystals to determine their chemical composition. The analyses were performed with a JEOL J SM-6400 scanning electron microscope (SEM) equipped with Noran Vantage Energy Dispersive Spectroscopy (SizLi) detector and Norvar window for standardless quantization of elements with Z Z 4. The crystals were affixed to an alumina sample holder with double-sided carbon tape. The EDS data were acquired at an accelerating voltage of 10 kV with a 30 to 60 second accumulation time. Single-Crystal X-ray Crystallography: Single crystals were mounted on a glass fiber with super glue and their intensity data were collected on either a Bruker SMART platform CCD diffractometer, or a STOE IPDS II diffractometer using Mo K01 radiation at 50 kV and 40 mA. Samples examined with the STOE (MnGa4,65 and ReGa4_5) had individual frames collected on a 34 cm image plate with a 60 second exposure time and a 10° to rotation. The X-SHAPE and X-RED-32 software packages7’ 8 were used for data extraction and reduction and to apply an analytical absorption correction. Direct methods and the SHELXTL suite were used to solve and refine the structures. 127 Individual frames of Nio_57Ga4,43 examined with the Bruker machine were collected with a 03° a) rotation. The SMART software was used for data collection, and SAINT software9 was used for data extraction and reduction. After applying analytical absorption corrections, structure solution and refinement were completed using direct methods and the SHELXTL suite of programs.10 '1’ '2 suggested that the space group for MnGa6 was either Ccc2 or Previous reports Cccm. The value of IE2—1| was 0.863 for MnGa4_55 and 0.972 for ReGa45, indicating a centrosymmetric structure, so Cccm was chosen. During initial indexing of the cell we noticed weaker satellite reflections in the reciprocal lattice, as described previously by another group.ll We have not yet attempted to include these satellites for a solution of the supercell structure. During refinement we encountered a problem in placing gallium atom G35. The most stable position for the atom leads to Ga—Ga bonds of unacceptably short lengths (1.58 A). The occupancy of the Ga5 atom was refined to nearly 50%, making the short “bond” distance more acceptable. The real atom is assumed to be in one of the Ga5 locations in half of the structure, and in the other site in the remaining half of the structure. Despite these adjustments, the anisotropic displacement parameters for Ga5 are quite large. Gallium atom Ga4 also has large anisotropic thermal parameters, but these are most likely a result of the problems with Ga5. The crystal structure refinement data for MnGa4,65 and ReGa45 are listed in Table 5-1. The atomic positions and isotropic displacement parameters are listed in Table 5-2. Anisotropic displacement parameters for the atoms are listed in Table 5-3. Bonding distances for MnGa4,65 and ReGa4_5 are listed in Table 5-4. 128 The crystal structure solution and refinement for Nio,57Ga4,43 were based on parameters from a previous structural report from powder diffraction data.‘3 The refinement data for our study are listed in Table 5-5. During refinement we found that the Nil site had a mixed occupancy of nickel and gallium atoms. Occupancy refinements on this crystal showed the site contained 57% nickel, though results likely vary from crystal to crystal. Atomic parameters and isotropic displacement parameters are listed in Table 5-6. Anisotropic refinement was performed on the non-mixed sites, and the results are listed in Table 5-7. Bonding distances for Nio,57Ga4,43 are listed in Table 5-8. 129 Table 5-1. Crystal data and structure refinement for MnGa4_65 and ReGa4,5. Formula Formula weight Crystal system Space group Unit cell dimensions Volume Z, Density (calculated) Absorption coefficient F(000) Crystal size, mm Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to 0m... Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>20'(I)] R indices (all data) Extinction coefficient MnGa4.6s 368.68 Orthorhombic Cccm a = 8.8323(18) A b = 8.9523(18) A c = 9.939(2) A 785.8(3) A3 8, 6.232 g/cm3 33.309 mm‘1 1316 0.144 x 0.179 x 0.185 3.83 to 34.54° 0 S h S 14. 0 S k S 14. 0 S l S 15 5655 875[R(int) = 0.2593] 99.4 % ReGa4.s 499.94 a = 9.007708) A b = 9.0618(18) A c = 10.158(2) A 829.2(3) A3 8, 8.009 g/cm3 57.695 mm‘1 1716 0.157 x 0.164 x 0.260 4.50 to 36.00° 0 S h S 14, 0 S k S 14, 0 S 1 S 16 3898 1027[R(int) = 0.1536] 99.2 °/o F ull-matrix least-squares on F2 875 / 0 / 35 1.068 R1 = 0.1020, wR2 = 0.1590 R1 = 0.0274, wR2 = 0.1358 0.0026(9) 1027 / 0 / 35 1.079 R1 = 0.0825, wR2 = 0.1866 R1 = 0.1451, wR2 = 0.2032 0.0022(3) R1 = Z ”Fol — Well /2 IR! and wR2 = 12: (IF.2 - all >2 / 2 017.2121” 130 Table 5-2. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (A2x 103) for MnGa4_65 and ReGa4_5. x y z U(eq) Occupancy Mn(1) 2500 2500 3458(3) 4(1) Ga(l) 1164(4) 4293(4) 5000 12(1) Ga(2) 71 1(4) 1 150(4) 5000 14(1) Ga(3) 2407(4) O 2500 14(1) Ga(4) 0 2588(5) 2500 50(2) Ga(S) 2500 2500 817(1 1) 48(3) 0.65 Re(l) 2500 2500 3461(1) 9(1) Ga(l) 1187(5) 4369(4) 5000 15(1) Ga(2) 623(5) 1 182(5) 5000 18(1) Ga(3) 2383(5) 0 2500 20(1) Ga(4) 0 2607(6) 2500 33(1) Ga(S) 2500 2500 751(7) 33(2) 0.50 U(eq) is defined as one third of the trace of the orthogonalized U11 tensor. 131 Table 5-3. Anisotropic displacement parameters (Azx 103) for MnGa4,65 and ReGa4,5. ull U22 u33 U23 ul3 [J12 Mn(l) 7(1) 2(1) 3(1) 0 0 -1(1) Ga(l) 12(1) 13(1) 10(1) 0 0 10(1) Ga(2) 12(1) 16(1) 15(2) 0 0 -11(1) Ga(3) 16(1) 8(1) 17(1) -10(1) 0 0 Ga(4) 56(3) 22(2) 71(4) 0 -57(3) 0 Ga(5) 99(9) 18(4) 28(5) 0 0 -16(5) Re(l) 17(1) 8(1) 3(1) 0 0 -l(1) Ga(l) 16(2) 12(2) 16(2) 0 0 8(1) Ga(2) 1 8(2) 1 6(2) 19(2) 0 0 -9(2) Ga(3) 24(2) 15(1) 21(1) -11(1) 0 0 Ga(4) 42(2) 21 (2) 35(2) 0 -28(2) 0 Ga(5) 60(7) 29(5) 9(3) 0 0 -8(6) The anisotropic displacement factor exponent takes the form: -27r2[ h2 a"'2Ull + + 2 h k a* b* U12 ] 132 Table 5-4. Bond distances (A) for MnGa4_65 and ReGa45. MnGaw ReGa4.s M—M 3.066(7) 3.1276(19) M—Ga(1) 2.513(3) 2.591(3) M—Ga(2) 2.512(3) 2.594(3) M—Ga(3) 2.4334(14) 2.4689(6) M—Ga(4) 2.4057(14) 2.4562(6) Ga(l)—Ga(1) 2.415(6) 2.424(7) Ga(1)—Ga(2) 2.788(5) 2.917(6) Ga(l)—Ga(3) 2.858(2) 2.905(3) Ga(2)—Ga(2) 2.412(6) 2.419(8) Ga(2)—Ga(4) 2.868(3) 2.904(3) Ga(3)—Ga(5) 2.796(6) 2.881(5) Ga(4)—Ga(5) 2.772(6) 2.870(5) Ga(5)—Ga(5) 1.620) 1.52605) 133 Table 5-5. Crystal data and structure refinement for NiO.57Ga443. Empirical formula Formula weight Temperature Crystal system Space group Unit cell dimensions Volume Z Density (calculated) Absorption coefficient F (000) Crystal size Theta range for data collection Index ranges Reflections collected Independent reflections Completeness to theta = 28.26° Refinement method Data / restraints / parameters Goodness-of-fit on F2 Final R indices [I>2sigma(1)] R indices (all data) Absolute structure parameter Extinction coefficient Largest diff. peak and hole Ga4.43 NiO.57 342.30 296(2) K Cubic 123 a = 8.424000) A a= 90° b = 8.4240(10) A 8: 90° c = 8.4240(10) A y = 90° 597.80(12) A3 8 7.607 g/cm3 42.607 mm" 1226 0.082 x 0.072 x 0.072 mm3 3.42 to 28.26°. -11ShS11,-10SkS11,-11S1S10 2475 245 [R(int) = 0.0504] 96.8 % F ull-matrix least-squares on F 2 245 / 0/ 18 1.093 R1 = 0.0329, wR2 = 0.0739 R1 = 0.0445, WR2 = 0.0780 0.5(4) 0.0022(3) 1.534 and -2.056 e.A'3 R1 = z ||Fo| — 1F.“ / 2 IE] and wR2 = [z (1F,2 — F31 )2 / z (wFfflm 134 Table 5-6. Atomic coordinates (x 104) and equivalent isotropic displacement parameters (AZX 103) for N10,57Ga4_43. x y z U(eq) Occupancy Ni(1) -1617(5) 1617(5) 1617(5) 3(1) 0.57 Ga(ll) ' -1617(5) 1617(5) 1617(5) 3(1) 0.43 Ga(l) 1610(5) 1610(5) 1610(5) 4(1) Ga(2) 0 3506(2) 0 1 1(1) Ga(3) 0 5000 2499(2) 1 1(1) U(eq) is defined as one third of the trace of the orthogonalized Uij tensor. Table 5-7. Anisotropic displacement parameters (Azx 103) for NiO.57Ga443. ull U22 u33 023 ul3 ulz Ga(l) 4(1) 4(1) 4(1) 1(1) 1(1) 1(1) Ga(2) 12(1) 10(1) 12(1) 0 9(2) 0 Ga(3) 15(1) 15(1) 3(1) 0 0 -3(3) The anisotropic displacement factor exponent takes the form: -21r2[ h2 a"‘2Ull + + 2 h ka“ 8* U12] Table 5-8. Bond distances (A) for Nio,5yGa4,43. Ni—Ga(1 ) Ni—Ga(1 ) Ga( 1 )——Ga(2) Ga(2)—Ga(2) Ga(2)—Ga(3) Ga(2)—Ga(3) Ga(3)—Ga(3) 2.7184(16) 2.587(3) 2.496(2) 2.518(3) 2.4540(17) 2.4532(17) 2.9783(4) 135 D. Structural Description MGa4,5 (M = Mn, Re): The MGa4+x compounds have a structure (Figure 5-1) that is caught between the PtHg4 structure of the MGa4 compounds (Figure 5-2a) and the PdGas structure (Figure 5-2b). In the PtHg4 structure, the metals reside in the center of gallium cubes. As more gallium is incorporated into the structure, the metal-centered cubes distort into metal-centered square antiprisms connecting along the c-axis (Figure 5- 3a,b). The squares of the antiprisms in the MGa4,5 structure are not quite offset by 45 degrees, as they are in the PdGas structure. This distortion may not be exactly the same for every antiprism, and may lead to the satellite reflections we found in the reciprocal lattice and the superstructure reflections mentioned by Girgis and Schulz.ll In the MGa4_5 structure, gallium atoms Gal and Ga2 form intra-square bonds (2.788 A) in one of the antiprism squares. The atoms in the other square, atoms Ga3 and Ga4, are separated beyond Ga—Ga bonding distance (3.1445 A). In the PdGas structure, all intra-square gallium atoms are separated from each other beyond Ga—Ga bonding distance (3.472 A). There is inter-square Ga—Ga bonding in both the MGa4+x (Gal—Ga3 2.858 A, Gal—Ga4 2.858 A, and Ga2—Ga4 2.868 A) and PdGas structures (Ga2—Ga2 2.858 A). The antiprisms in PdGa5 connect to form a rectangular prism that is centered by a gallium atom. In the MnGa4,5 structure, the rectangular prism is elongated and centered by a pair of gallium atoms. However, during refinement of the MnGa4_5 structure we found that the Ga5 atoms forming this pair are approximately half-occupied. Attempts to place a fully occupied atom at the center of this pair have not been successful. 136 mm L0 (b) -axis of (a) MnGa4 and (b) PdGas. Figure 5-3. Connectivity along the c-axis in (a) MGa4,5 and (b) PdGas. 139 NiosyGa443: The NiO.57Ga443 structure is based on the y-brass structure.13 The structures are composed of a series of body-centered cubes and chains of intersecting rhombi. NiO.57Ga4,43 (Figure 5-la) and y-brass (Figure 5-1b) crystallize in different space groups, 123 and 143m respectively, because of the position the nickel atoms occupy in NiO.57Ga443. As shown in Figure 5-1a, the nickel atoms (Nil) occupy two comers of the central body-centered cube in the Nio_57Ga4,43 structure, while gallium atoms (Gal) occupy the other two corners . This lowers the degree of the rotation axis along the b- axis from a 4-fold axis to 2-fold axis. This in turn lowers the space group symmetry of Nio_57Ga4,43 from 143m to 123. Through occupancy refinements we found that the Nil position was split between nickel atoms and gallium atoms. If the Gal position had the same mixed occupancy of the Nil position, the 143m symmetry of the parent y—brass structure would be preserved. The 143m symmetry could also be preserved if the mixed occupancy site were in the Ga2 position. However, our occupancy refinements for both of these positions found them to be completely occupied by gallium atoms. The original structural report of NiGa4 describes the structure as a vacancy controlled y-brass phase.'3 The vacancies in the structure arise because the Ga3 atoms in NiGa4 would reside in the 12d position of 143m, instead of the 24g position that the Zn2 atom occupies in the y—brass structure. This reduces the number of atoms in the unit cell from 52 to 40. 140 E. Results and Discussion As mentioned in Chapter Three, manganese gallides have been isolated from every reaction targeting a manganese boride. Crystals of MnGa4 are often rectangular plates or prisms (Figure 5-5a), so they can be mistaken for crystals of boride phases we have seen. While we have seen some needle-like and larger prismatic crystals of MnGa4,65, the crystals of this phase often have an octahedral morphology. These octahedral crystals are indistinguishable from crystals of silicon, another common, unintended side product in many of our gallium flux reactions. We were quite lucky to choose a gallide crystal when picking octahedral crystals on which to perform EDS analysis, otherwise, we may have completely overlooked the compound. After fortuitously finding MnGaMs, we knew to check the octahedral crystals from rhenium-containing reactions, hoping to find the ReGa4,5 analog. We were a bit surprised to find that the rectangular plates and prisms (Figure 5-5b) formed in these reactions were not ReGa4, because the rhenium- and manganese-containing reactions were carried out under identical conditions. The prisms and plates were the same ReGa4,5 phase as the octahedral crystals. The synthesis of Nio_57Ga4,43 was also a chance occurrence. Our synthesis targeting NiW2B15 happened to have a heating profile that ended with a hold at 250 °C in order to centrifuge the reaction tube and remove the excess gallium. Our literature search on NiGa, later revealed that the compound forms near 250 °C, though single crystals had not yet been isolated.“ '3 This may explain why we have not found this product in other reactions, as the centrifugation step was removed from most of the later reaction parameters. The absence of NiGa4 from other reaction products indicates that the 142 20 um (b) Figure 5-5. SEM micrographs of (a) MnGa4 and (b) ReGa4,5. 143 reaction temperature is the most important reaction parameter, and not necessarily the stoichiometry. The goal of this project was to synthesize borides using the metal flux technique. Therefore, as unintended products to these reactions, the gallides reported here are an interesting side-note to the main focus of this research. We have not yet initiated reactions targeting only these compounds, however such reactions will likely be carried out in the future. Possible physical and electronic properties measurements should provide even more inspiration to conduct further research on this interesting group of gallides. F. Conclusions We have synthesized and grown single crystals of MnGaMs, ReGa45, and Nio,5yGa4,43 from gallium flux reactions originally targeting borides. The first structural refinement on MnGa4,65 and ReGa4,5 shows that the compounds have an intermediate structure between the PtHg4 and PdGas structures. Single crystal x-ray diffiaction analysis of a Nio_5yGa4_43 crystal confirms the results of previous work by J inkui and Sishen on powder data. 144 References l. Fisk, Z.; Remeika, J. P., Growth of Single Crystals from Molten Metal Fluxes. In Handbook on the Physics and Chemistry of the Rare Earths, ed.; K.A. Gschneidner, J .; Eyring, L., Eds. Elsevier Science: 1989; Vol. 12, pp 53-70. 2. Kanatzidis, M. G.; P6ttgen, R.; Jeitschko, W., The Metal F lux- A Preparative Tool for Intermetallic Compounds. Angewandte Chemie International Edition 2005, 44, (43), 6996-7023. 3. Lobring, K. C.; Check, C. B; Zhang, J .; Li, S.; Zheng, C.; Rogacki, K., Single Crystal Growth, Bonding Analysis and Superconductivity of V2Ga5. Journal of Alloys and Compounds 2002, 347, 72-78. 4. Haussermann, U.; Viklund, P.; Bostrtim, M.; Sirnak, S. I., Bonding and Physical Properties of Hume-Rothery Compounds with the PtHg4 Structure. Physical Review B 2001, 63, (12), 125118. 5. Haussermann, U.; Bostrtim, M.; Viklund, P.; Rapp, O.; Bjtirnangen, T., FeGa3 and RuGa3-Semiconducting Intermetallic compounds. Journal of Solid State Chemistry 2002, 165, 94-99. 6. Feschotte, P.; Eggimann, P., Les Systemes Binaries Cobalt-Gallium et Nickel-Gallium - Etude Comparee. Journal of Less-Common Metals 1974, 63, 15-30. 7. X-SHAPE, Version 2.05; STOE & Cie GmbH: 2004. 8. X-RED 32, Version 1.10; STOE & Cie GmbH: 2004. 9. Sheldrick, G. M. SAINT, Version 4; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI. 10. Sheldrick, G. M. SHELXT L Structure Determination Program, Version 5.0; Siemens Analytical X-Ray Instruments, Inc.: Madison, WI, 1995. 11. Girgis, K.; Schulz, H., A Gallium-rich Mn-Ga Compound. Naturwissenschaften 1971, 58, (2), 95. 12. Meissner, H. G.; Schubert, K.; Ananthraman, T. R., The Constitution and Structure of Manganese-Galliurn Alloys. Proceedings of the Indian Academy of Sciences 1965, 56A, (16), 340-367. 13. Jingkui, L.; Sishen, X., The Structure of NiGa4 Crystal-a New vacancy Controlled y- Brass Phase. Scientia Sinica 1983, 26A, (12), 1305-1313. 145 CHAPTER SIX Conclusions and Future Work When we began this research, we knew that the metal flux technique had been used with some degree of success in boride synthesis. Much of the preliminary work on metal flux boride synthesis covered the use of aluminum as the flux metal. Our goals were to extend the flux technique to include gallium, and to expand on the work using copper as a flux for boride synthesis. Not only have we synthesized borides using metal fluxes, but we have also learned some of the limitations to using either gallium or copper as a flux. While we have tried to use gallium to synthesize borides for most of the transition metals, our success has been limited to groups 6 and 7. Crystals of Cr2B3, CrB2, MoB, and WB all grew from reactions targeting ternary borides. We have not yet synthesized a ternary boride from group 6; however, we have grown crystals of group 7 ternary borides. Gallium was used to grow crystals of HoMnB4, DyReB4, ErReB4, and YbReB4. Binary group 7 borides synthesized in flux reactions are MnB, MnB4, and ReB2. Further research on gallium flux synthesis of group 6 and 7 borides should begin with a focus on reproducing all known binaries for each metal in the groups. This may seem like a trivial task at first, but our synthesis of new phases for MnB and RuB2 illustrate the possibilities when using a flux to grow known compounds. Exploratory 146 syntheses of “missing” analogs to known phases can also be carried out during this study. After the binary systems are well analyzed, the ternary systems can be targeted. The remaining YCrB4-type borides for manganese and rhenium should be among the first ternary targets. Commensurate and incommensurate RETM4B4 phases are reported for both manganese and rhenium,I so the influence of the flux on which phases formed in this stoichiometry would be an interesting study. Exploratory synthesis in ternary systems should also be carried out because of the flux’s ability to trap metastable phases that are inaccessible using other synthesis techniques. When gallium flux reactions were used with metals outside of groups 6 and 7, they tended to include the first row metals. Further research with gallium should include more of the second- and third-row transition metals. Reactions with rhodium, iridium, and platinum would be particularly interesting, since several borides from these metals also include gallium in their structures.2 Preliminary reactions with rhodium and iridium have produced thin plates too fragile to study with EDS or single-crystal diffraction. Rhodium and iridium are also the next metals we would like to investigate using a copper flux. Several ternary rhodium borides have been synthesized using a copper flux,3 but similar work with iridium has not yet been reported. Research targeting just binary borides could be as fi'uitful as our work with ruthenium. A potential complication is that copper forms ternary borides with rhodium and iridium.4 Further research into the ruthenium system still needs to be conducted. Despite synthesizing Ru7B3, Ru2B3, and two phases of RuB2, we were unable to isolate Ru) 133 or RuB“. Our studies with the copper flux varied the BzRu ratio in 1.0 increments. Ru) .B3 and RuB” have empirical formulas close enough to other phases that a 1.0 difference in 147 the B:M ratios between reactions can easily bypass favorable reaction stoichiometries for these phases. Future studies should decrease the difference between B:M ratios of reactions to 0.5 or 0.25. To study properties of the new B-RuB2 phase, a little crystal engineering needs to be done. We looked into having microhardness and incompressibility measurements conducted on this phase, but our crystals were too small. Magnetic measurements can also be performed once more crystals are isolated. Electronic structure calculations should be carried out to determine the stability of the ReB2-structure versus the RuB2- structure for ruthenium and other metal diborides. The primary goal in further copper flux syntheses of ternary ruthenium borides should be completing the series of LuRu4B4-type compounds. It will be interesting to see if the entire series can be synthesized from a copper flux. Reactions temperatures need to be varied to determine whether Pr and Nd always form the modulated phases from a flux, or if the commensurate phases can be isolated under different reaction parameters. Substitution of other metals for ruthenium presents possible extension of our work. After synthesizing the LuRu4B4-type compounds, more of their physical properties need to be measured. The magnetic properties of these compounds have already been determined from bulk samples, but single crystals will allow us to examine the system more thoroughly, searching for anisotropy in the magnetic ordering. It will also be interesting to compare the results of these studies with a study on LaRu4B4, to see if the different connectivity in the Ru, tetrahedra influences the magnetic properties. Copper flux growth of binary niobium borides has been reported,5 and we have grown needle-like crystals of Nb3Co4B7, These results indicate that more group 5 borides 148 should be targeted in copper flux reactions. A few reactions targeting vanadium or tantaltnn analogs to Nb3Co4B7 have not been successful. Initial attempts to synthesize binary vanadium borides have been unsuccessful, yielding only large crystals of V-doped boron. Initial attempts to synthesize other ternary niobium borides have only produced Nb3B4. One of the most challenging tasks in metal flux synthesis of boride is finding a suitable flux metal for the late first-row transition metals. We were fairly surprised that the copper flux did not produce iron or cobalt borides, considering that both ruthenium and rhodium borides grow from that metal flux. Aluminum, gallium, indium, and tin , though unsuccessful so far, are the metals most likely to produce borides. Canfield has also used Ni2B to grow quaternary nickel borocarbides,‘5 however the isolation calls for decanting the flux while above 1000 °C. The results presented in this work set a foundation for continued research into the metal flux synthesis of borides. The above suggestions for future work are just a brief glimpse of what could be done in this field. 149 References 1. Zavalii, P. Y.; Mikhalenko, S. I.; Kuz'ma, Y. B., New incommensurate structures of the borides Pr4)(Mn4B4)35 and Pr7(Re4B4)6. Journal of Alloys and Compounds 1994, 203, 55-59. 2. Klitnter, W.; Jung, W., Gaglr4B - ein Gallium-Iridiumborid mit isolierten, annfihemd quadratisch planaren Ir4B-Gruppen in einer vom CaF2-Typ abgeleiteten Struktur. Zeitschriftfiir anorganische und allgemeine Chemie 1995, 621, 197-200. 3. Shishido, T.; Ye, J.; Sasaki, T.; Note, R.; Obara, K.; Takahashi, T.; Matsumoto, T.; F ukuda, T., Growth of Single Crystals in the Systems with R-Rh-B and r-Rh-B-C (R= Rare Earth Element) from Molten Copper Flux. Journal of Solid State Chemistry 1997, 133, 82-87. 4. Klunter, W.; Jung, W., The Copper Iriditun Boride Cu2Ir4B3 with a Layered Structure Derived from teh ZnIr4B3 Type. Zeitschriftfur anorganische und allgemeine Chemie 2000, 626, 502-505. 5. Okada, S.; Hamano, K.; Lundstrém, T.; Higashi, I. In Crystal Growth of the New Compound Nb 2B 3, and the Borides NbB, Nb 586, Nb 334, and NbB2, Using the Copper-Flux Method, Boron-Rich Solids, Albuquerque, New Mexico, 1986, 1985; Emin, D.; Aselage, T.; Beckel, C. L.; Howard, 1. A.; Wood, C., Eds. American Institute of Physics: Albuquerque, New Mexico, 1985; pp 456-459. 6. Canfield, P. C.; Fisher, 1. R., High-Temperature Solution Growth of Intermetallic Single Crystals and Quasicrystals. Journal of Crystal Growth 2001, 225, 155-161. 150 Appendix RF Furnace Design and Setup The RF furnace has been a vital instrument for high-temperature synthesis in our group for a number of years. However, several issues repeatedly arose and led to a redesign of the furnace. A brief examination of the previous design and the associated problems help illustrate the benefits of the new design. In the previous design, a thin sheet of molybdenum foil was wrapped around a reaction crucible to act as a susceptor to the magnetic fields generated by the copper induction coil. The crucible and susceptor were then balanced in a small mullite tube packed with insulating wool. The tube was placed into a pyrex reaction chamber, which was also packed with insulating wool. A flow of argon was introduced into the reaction chamber and upon turning on the power to the induction coil heating commenced. The main problem with the previous design was that the crucible and susceptor would frequently tip over and contact the reaction chamber. The reaction chamber would then crack because of the extreme heat of the susceptor. The chamber also cracked a few times because the insulating wool was packed too tightly and expanded slightly on heating. Another small problem was that the molybdenum foil became brittle after several reactions, and new pieces had to be used often. These problems and the inability to run reactions under vacuum led to the new furnace design. 151 The new RF furnace has a reaction chamber made of fused quartz, which is more thermally stable than the previous pyrex chamber. A boron nitride cylinder (Figure A-la) has replaced the insulating wool and mullite tube from the previous furnace. The cylinder is centered along the central axis of the reaction chamber by a small dimple in the floor of the chamber. Instead of using molybdenum foil as a susceptor, we machined a crucible holder from a molybdenum cylinder (Figure A-lb,c) capable of holding crucibles of different sizes. The crucible holder sits on the BN cylinder and is more stable than the molybdenum foil. Many reactions have been run and the new crucible holder / susceptor is still working quite well. In order to run reactions under vacuum, we installed a three-way valve that opens the reaction chamber to a gas flow or a vacuum pump. With this design the chamber can be filled and purged several times before the reaction is initiated. T-joints have been added to the gas lines, allowing for argon, nitrogen, or a mix of the two to be used for flushing the chamber or during reactions. Running reactions under dynamic vacuum slows the deposition of fihns on the inside of the reaction chambers. This allows the thermometer to have a clear view of the crucible and susceptor, resulting in more accurate temperature monitoring. While the design of several components has changed, the overall setup of the RF furnace has not changed (Figure A-2). The reaction chamber is placed in the induction coil, with the susceptor located in the middle of the induction coil. The induction coil is connected to a remote power station, which is controlled by the main control unit. The reaction temperatures are monitored with an IR thermometer aimed between the copper tubing and reported on a furnace controller connected to the thermometer. 152 (a) (b) (c) Figure A-l. Cross-sectional view of (a) BN susceptor holder and Mo susceptor along (b) vertical and (c) horizontal axes. 153 E 533 wczoou H Seam wagon 8053— EofitoE< UDJSE “ED .8250 EcofitoE< y \xlmJJ 2m \II} 62 0 DUDDDU mafia :U \\? 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