New Research In
Physical Sciences
Social Sciences
Featured Portals
Articles by Topic
Biological Sciences
Featured Portals
Articles by Topic
- Agricultural Sciences
- Anthropology
- Applied Biological Sciences
- Biochemistry
- Biophysics and Computational Biology
- Cell Biology
- Developmental Biology
- Ecology
- Environmental Sciences
- Evolution
- Genetics
- Immunology and Inflammation
- Medical Sciences
- Microbiology
- Neuroscience
- Pharmacology
- Physiology
- Plant Biology
- Population Biology
- Psychological and Cognitive Sciences
- Sustainability Science
- Systems Biology
Structure of superhard tungsten tetraboride: A missing link between MB2 and MB12 higher borides
Edited by Zachary Fisk, University of California, Irvine, CA, and approved February 3, 2015 (received for review August 13, 2014)

Significance
Superhard materials are those with hardness competitive with diamond. This study investigates tungsten tetraboride, a superhard metallic compound, and a promising candidate to revolutionize cutting tools and to succeed the “hard metals,” such as tungsten carbide, that are commonly used. Unfortunately, the structure of this material has been contested for over half a century. Previous attempts at its solution have lacked comprehensiveness, as they have not used techniques, such as neutron diffraction, which are capable of differentiating between light and heavy elements (boron and tungsten, respectively). Utilizing both X-ray and neutron diffraction, this study reveals that tungsten tetraboride is actually an interesting ‘new’ structural hybrid between lower and higher borides, a missing link that further confirms the structural regularity among borides.
Abstract
Superhard metals are of interest as possible replacements with enhanced properties over the metal carbides commonly used in cutting, drilling, and wear-resistant tooling. Of the superhard metals, the highest boride of tungsten—often referred to as WB4 and sometimes as W1–xB3—is one of the most promising candidates. The structure of this boride, however, has never been fully resolved, despite the fact that it was discovered in 1961—a fact that severely limits our understanding of its structure–property relationships and has generated increasing controversy in the literature. Here, we present a new crystallographic model of this compound based on refinement against time-of-flight neutron diffraction data. Contrary to previous X-ray–only structural refinements, there is strong evidence for the presence of interstitial arrangements of boron atoms and polyhedral bonding. The formation of these polyhedra—slightly distorted boron cuboctahedra—appears to be dependent upon the defective nature of the tungsten-deficient metal sublattice. This previously unidentified structure type has an intermediary relationship between MB2 and MB12 type boride polymorphs. Manipulation of the fractionally occupied metal and boron sites may provide insight for the rational design of new superhard metals.
As demand increases for new superhard materials, the introduction of transition metal borides as candidate compounds has recently attracted a great deal of attention (1⇓⇓–4). This trend is at least partially driven by a need for greater efficiency in cutting tools compared with tungsten carbide (which is not superhard), as well as the shortcomings of the traditional superhard compounds—diamond (which is unusable for cutting ferrous materials) (5) and cubic boron nitride (which is very expensive to synthesize and difficult to shape) (6). Within the rapidly growing family of superhard borides, tungsten tetraboride (or WB4) is of specific interest due to its excellent mechanical properties and its relatively lower cost compared with borides such as ReB2, OsB2, RuB2, and RhB2, which contain platinum group metals (3, 7⇓⇓⇓–11). For instance, tungsten tetraboride demonstrates an extremely high indentation hardness of ∼43 GPa by the Vickers method (under an applied load of 0.49 N) (8) and ∼41.7 GPa by nanoindentation (maximum, at a penetration depth of 95.25 nm; Fig. 1), and can sustain a differential stress (a lower-bound estimate of compressive yield strength) of up to ∼19.7 GPa (12). More dramatically, it is like ReB2 (2), capable of scratching natural diamond (11). We have, furthermore, previously shown that the hardness of this compound may be enhanced by the creation of solid solutions with other transition metals (9). However, to understand the underlying mechanisms for the hardness enhancements observed in WB4 solid solutions, as well as to guide the design of new superhard borides with tailored mechanical properties, it is crucial to understand the crystal structure of this compound.
Plot of average nanoindentation hardness versus displacement for WB4, indicating superhardness (hardness above 40 GPa) from ∼60 nm displacement to ∼250 nm. The average hardness over this range is 40.9 ± 1.1 GPa with a maximum value of 41.7 ± 1.3 GPa at 95.25 nm. The shaded area represents the 95% confidence interval. (Inset) The full hardness curve from 0 to 850 nm. The average value of hardness from 60 to 850 nm is 39.7 ± 0.8 GPa. Numbers following the ± sign represent SDs.
Perhaps surprisingly for a simple binary compound, the structure of tungsten tetraboride has been a contentious issue since its discovery by Chretien and Helgorsky in 1961, who assumed it to be related to borides of the ThB4 type (tetragonal, a = 6.34 Å and c = 4.50 Å) (13). Currently, no fewer than four distinct structures have been proposed for this compound (Table 1), the three most plausible of which are illustrated in Fig. 2. Because of the discrepancies among published structural models, the present study was undertaken with the goal of revisiting the structure of this boride using the additional resource of neutron diffraction, a technique that is complementary to X-ray diffraction. Thermal neutrons, interacting in this case entirely with atomic nuclei, have a very high scattering cross-section for boron-11. This situation is opposite from that in X-ray diffraction, where scattering is dictated by electron clouds, and is thus dominated by the considerably more electron-dense tungsten atoms.
Summary of previous WB4 models
Comparison of the various proposed structures of WB4. (A) The structure of WB4 by Romans and Krug (15). (B) The structure of W1.83B9 according to Nowotny et al. (16). (C) The structure of “W1-xB3” following Rosenberg and Lundström (17) and Zeiringer et al. (14) Green spheres represent boron atoms and gray spheres represent tungsten atoms. Partial occupancy is indicated by partial sphere filling. Bonds are shown to clarify the spatial arrangement only.
Having simultaneously refined against data obtained from these two methods, we have produced what we believe to be the definitive structural model for the highest boride of tungsten. As a result, the structure reported here, which contains some elements already known from previous X-ray–only investigations, introduces several previously unidentified ones that are observable only with the more detailed information derived from neutron data. Most importantly, however, this model provides insight into the rational causes of the extremely high hardness and solid solution hardening behavior observed in this boride. The history of previous attempts has already been explored in the recent work of Zeiringer et al. (14), and therefore will be only briefly summarized here.
Arguably the most cited of the structural solutions for WB4, and the first for which atomic coordinates were assigned, was produced by Romans and Krug (15) in 1965. This structure (Fig. 2A) was based on refinement of powder diffraction data against a lower volume (148.47 vs. 180.88 Å3) hexagonal unit cell (space group P63/mmc, a = 5.200 Å and c = 6.340 Å) versus the tetragonal assumption of Chretien and Helgorsky. After assigning the tungsten sites, having assumed them to be fully occupied, they accommodated their measured stoichiometry (WB4 – WB5) by designating Wyckoff positions 12(i) and 4(f) as boron sites. This assumption produced reasonable B—B bond lengths, but resulted in the imposition of B—B dimers, or “dumbbells” within the tungsten layers.
Independently, Nowotny et al. explored the system in 1967 using tungsten borides isolated from eutectic melts of MB—WB4—B (M = Ni, Rh, Pd, Pt), and assigned the formula W2−xB9 to the highest boride (approximate composition W1.83B9 or WB4.92). Perhaps due to indexing a few contaminating X-ray lines (discussed below), they assigned it to the low-symmetry trigonal group P-3 with a = 5.206 Å and c = 6.335 Å (Fig. 2B) (16). Instead of dumbbells, their structure includes B6 octahedra inserted among the ordered tungsten vacancy positions. The Nowotny et al. model is probably most notable for being the first to anticipate fractional occupancy at the tungsten 2(b) site.
To settle the already clear incongruity of the above structures, Rosenberg and Lundström attempted a definitive solution for the positions of the boron atoms in 1973 using computerized least-squares refinement and Fourier difference map techniques (17). To minimize the scattering power mismatch between metal atoms and boron, they refined, as proxy, the presumably isomorphous molybdenum phase denoted Mo1−xB3 (x ∼ 0.20) (Fig. 2C). Although this work confirmed the partial occupancy at one of the metal sites, the possibility of boron atoms filling vacancies in the structure was rejected, leaving voids in the structure. This model has been lent even more support by a recent single-crystal investigation by Zeiringer et al., who worked directly with the tungsten phase, referring to it analogously as W1−xB3 (P63/mmc, a = 5.2012 Å and c = 6.3315 Å) (14), seemingly settling the matter.
Outside the X-ray crystallographic community, however, this issue has also attracted significant attention from theoretical groups. Within the past five years, there has been a rapid succession of computational papers with the goal of identifying the structural origin of the properties of WB4 (18⇓⇓⇓⇓⇓⇓⇓⇓⇓–28). Although the correctness of the Romans and Krug model was initially assumed (24), it was quickly noticed that such a structure should be unstable (26). This lead to the theoretical confirmation that the structure and properties of the highest boride of tungsten are better accommodated if the B2 dimers are removed (21, 23, 27), producing a composition of WB3. Most recently, several exotic models have appeared with larger unit cells (18, 29) and varying stacking orders (28) of the metal layers. So far, all of these models still appear inconsistent with the experimental evidence. Thus, although nearly all current experimentally derived models agree that partial occupancy plays a role in the structure of WB4, computational support is still weak (21). This situation may change as computing resources increase (enabling, for instance, much larger supercell models), but as it stands, the calculations so far reported only further highlight the structural ambiguity of this compound and do not themselves offer a viable alternative consistent with experiment.
Results and Discussion
The ambiguity in experimental determinations of the highest boride of tungsten stems primarily from difficulties in refining X-ray diffraction data for a compound containing closely associated elements that are near the extremes of being electron poor (boron; Z = 5) and electron rich (tungsten; Z = 74). Although the ratio of boron to tungsten is large, it is not so large that boron’s core-electron contribution dominates the structure factor. This situation is exacerbated by three further issues: (i) the imprecision with which the compound’s stoichiometry is known, (ii) the synthetic necessity to include excess boron to avoid WB2 impurities; and (iii) partial occupancy at sites in the tungsten layer.
Fortunately, the disparity between the diffraction contributions of the two elements can be significantly decreased using thermal neutron diffraction, where the scattering power for both elements is roughly comparable. Thus, by simultaneous refinement of patterns obtained using both diffraction techniques, it becomes possible to distinguish between several possible atomic arrangements that all appear consistent with X-ray data alone. This approach is similar to the rationale used by Rosenberg and Lundström, whose modeling was based on an analogous compound, Mo1−xB3, where the lower atomic number of molybdenum was used to enhance the contribution of boron to the X-ray structure factor. Nevertheless, we believe the present method to be superior because we work with the native compound and therefore avoid assumptions about similarities between the W and Mo borides.
However, because we have found that the approximate eutectic composition W:B = 1:12 most reliably produces “WB4” without additional tungsten-containing phases (8), our approach is still complicated by the presence of superstoichiometric amounts of boron. This excess boron crystallizes exclusively as the β-rhombohedral phase without crystallographically identifiable dissolution of tungsten (as found here and corroborated by ref. 30), and its grains are found throughout arc-melted ingots (Fig. 3A). Unfortunately, the extreme chemical inertness and mechanical robustness of crystalline boron precludes its separation from the tungsten phase, necessitating the simultaneous refinement of both. Furthermore, boron is strongly adhered even to the macroscopic crystallites (Fig. 3B), reducing the possibility of obtaining high quality single-crystal data, particularly in the case of neutron diffraction.
(A) SEM image of a sectioned W11B12 ingot in backscattered electron (compositional) mode indicating compositional uniformity of WB4.2 (bright) grains. (B) Backscattered electron SEM image of a fractured ingot of an arc-melted sample in the ratio W:B of 1:12. Light regions are the tungsten-containing phase.
Although β-boron produces only trivial interference with the X-ray diffraction data, its presence poses a more formidable challenge for the analysis of the neutron data: its many intense peaks heavily overlap those of the tungsten phase. Moreover, the structure of β-boron is imprecisely known due to a large amount of structural disorder at the interstices between icosahedra (31⇓⇓⇓⇓⇓–37). Accordingly, the neutron diffraction experiment produces an exceptionally complex pattern from strong diffraction of the secondary β-rhombohedral boron phase, necessitating its simultaneous refinement. Nevertheless, the structure of the β-rhombohedral boron phase was found to be satisfactorily modeled by a slight modification of the atomic coordinates proposed by Hoard et al. (35) (see SI Appendix for details).
The powder X-ray diffraction pattern of a crushed ingot of nominal composition WB12 made with isotopically enriched 11B (i.e., W11B12), may be readily indexed against a hexagonal unit cell with dimensions a = 5.2001 Å and c = 6.3388 Å in the space groups P62c, P63mc, or P63 /mmc. A few contaminating lines are noticeable and fully indexable against β-rhombohedral boron, as would be expected given the large molar excess of boron in the reaction mixture. Most of these lines, with the exceptions of those at 11.92° 2θ [(102)boron], 16.19° 2θ [(110)boron], 17.56° 2θ [(104)boron], and 19.09° 2θ [(201)boron], are of similar magnitude (<1%) to those of residual CuKβ radiation diffracted by the WBx phase. Although we have found no evidence supporting the P-3 trigonal structure proposed by Nowotny et al. (16), comparison of our X-ray diffractographs to reflections presented in their work indicates the probable misassignment of the highest intensity β-boron peak (observable in our data at 17.56° 2θ in Fig. 4B) to the tungsten boride pattern. Using our data, we can readily replicate this reduction in symmetry, thus accounting for the discrepancy.
(A) Neutron and (B) X-ray powder diffraction patterns for the highest boride of tungsten. Red points indicate observed data; the green line represents the fit against the final model. The difference between the two is shown beneath (magenta line). The background has been subtracted for clarity. (C) The best fit to the neutron diffraction data without the inclusion of the trigonal boron clusters. (D) Three-dimensional Fourier difference map (yellow) from the neutron refinement overlaid on the boron-deficient model structure lacking interstitial boron. Please see SI Appendix for enlarged plots.
Here, we have chosen the highest symmetry group, P63 /mmc, in which there are three crystallographic positions [Wyckoff 2(b), 2(c), and 2(d)] that may be occupied by tungsten atoms. One of these positions [Wyckoff 2(d)] is completely unoccupied, and thus one-third of the maximum possible tungsten atoms are systematically absent, leaving “voids” in the structure. Rietveld analysis against a model consisting only of tungsten atoms and a hexagonal net of boron yielded a fractional occupancy of ∼2/3 for the tungsten atom at Wyckoff 2(b) at (0, 0, 1/4). The last remaining tungsten site, Wyckoff 2(c), is fully occupied at (1/3, 2/3, 1/4).
Among the previous work on this subject, the structure derived by Zeiringer et al. (and related to that proposed by Rosenberg and Lundström) from single crystal data is the most similar to ours. However, repeated attempts at refining this model, where only voids are left for the partially occupied tungsten site, against the neutron powder diffraction data made clear that it does not fully account for the observed peak intensities (Fig. 4C). Fourier difference maps (Fig. 4D) subsequently revealed significant diffraction density on Wyckoff 6(h) at approximately (0.24, 0.12, 1/4) and (0.26, 0.13, 1/4). A boron atom inserted into either of these positions refined to (0.24, 0.12, 1/4) with an occupancy of ∼1/3. The resulting model thoroughly accounts for the observed X-ray and neutron diffraction intensities and is compatible with our own single crystal measurements. Intriguingly, Rosenberg and Lundström mentioned peaks in their own Fourier mapping corresponding to at least ∼17% boron occupancy of the Wyckoff 6(h), but the potential for occupancy at this position was not explored. One might speculate that conclusions similar to those presented here might be reached if data for Mo1−xB3 were to be further refined against a model having such sites occupied.
The structure resulting from our analysis, presented in Fig. 5 (crystallographic parameters listed in Table 2), implies a stoichiometry of approximately WB4.2. From this solution, we may draw some structural conclusions that have not been previously reported. Specifically, we find that a trigonal cluster of boron randomly fills the crystallographic position around the partially occupied tungsten 2(b) site. Due to the relative site occupancies of these atoms [2/3 at 2(b) for W and 1/3 at 6(h) for B], as well as the unrealistically short bond distance that would result if both were present simultaneously, it is best to consider them a singular unit that is never partially occupied, but always filled by either tungsten or the boron trimer. This arrangement, where the boron atoms are well within bonding distance to the hexagonal boron nets, gives rise to a subset of slightly distorted cuboctahedra, or portions thereof, distributed between tungsten planes. The average incidence of these random cuboctahedra can be calculated as approximately one for every three cellular units (two trimers per cell). The effective void space in this structure is thus much smaller than that anticipated in other models, and the presence of boron between layers has the potential to provide bonding between boron layers.
The proposed structure of the highest boride of tungsten.
Relevant crystallographic data for the highest boride of tungsten
Isolated boron dimers, such as those in the practically canonical Romans and Krug structure (15), are a rare crystallographic entity for borides with M:B ratios greater than ∼3:2 or lesser than ∼1:12, with few examples available in the literature. Their presence in this intermediate region contradicts the rule first described by Kiessling as early as 1951 (38)—that the structural connectivity of boron transitions from isolated atoms (e.g., W2B) (39), to chains (e.g., WB) (39), to nets (e.g., WB2) (39), to interconnected polyhedra (or portions thereof) as boron content increases. In fact, exceptions to this trend, such as the compound IrB∼1.35 (wherein apparent dimerization of boron is brought about by what can be imagined as a Peierls-type distortion of the boron chain) (40), often serve better to demonstrate the law-likeness of Kiessling’s rule than to contradict it. In those cases where isolated B2 dimers do occur, such as for some borides of ratio M:B = 3:2 (e.g., W2CoB2) (41), they do so as a result of their intermediate stoichiometry between that of isolated-atom borides (M:B = 2:1) and chain-forming borides (M:B = 1:1). As such, they can be viewed as short chain fragments, with the trend continuing for M:B = 4:3, e.g., W3CoB3 (42) (three-atom chains), and so on.
Following that, the structure proposed here might itself be imagined as such an intermediate. For example, if all of the possible tungsten sites were to be fully occupied, an AlB2-type (P6/mmc) structure with nearly ideal W–W and B–B distances would result. Conversely, if the absent tungsten sites are taken to give rise to the opportunistic formation of slightly distorted cuboctahedral cages, a hexagonal variation of the UB12-type (Fm-3m) would be formed when all partially occupied tungsten sites are replaced (limiting stoichiometry = MB9). This view is additionally satisfying in light of the stoichiometric position of WB4.2 between MB2-type compounds, which contain exclusively boron nets, and MBx phases with x > 2, such as UB12, where polyhedral subunits are increasingly dominant. The analogy can be further emphasized when a (somewhat fictionalized) representation of a tungsten boride having all 6(h) sites occupied is compared against the cubic packing of a scaled UB12 unit cell, as in Fig. 6. It can be rationalized that no higher tungsten boride having a “true” UB12 structure exists by noting that the formation of dodecaborides containing well-ordered cuboctahedra depends strongly on the radius of the metal atom, with Y (1.80 Å) (43) and Zr (1.60 Å) (43) being respectively, the largest and smallest metals to do so under ambient pressure (44). In comparison, the radius of W is only 1.39 Å (43), which is too small to accommodate one cuboctahedral cage per metal atom, as would be required. Notably, although, the second-neighbor M–M distances in WB4.2 are ∼5.200 Å, versus the nearest distance of ∼5.236 Å for ZrB12 (45).
(A) Occurrence of a cuboctahedron at the intersection of three unit cells. (B) Overlay of the UB12 structure type on WB4.2, showing a close similarity.
This model is further supported by data recently presented by Cheng et al. (20), who, using aberration corrected high-resolution transmission electron microscopy, claim to have visualized “interstitial boron” in WB4. Nevertheless, the authors hypothesized that the true formula for the compound is WB3, a composition they arrived at using particle swarm computational methods. In light of the microscopic evidence, they were forced to modify this formula to WB3+x (x ∼ 0.343–0.375) and further showed that this composition is compatible with their 2 × 2 × 2 supercell. We speculate that, had the authors combined this information further and provided a crystallographic position for their interstitial boron, they may have found that full occupancy for both tungsten and boron in the sites they visualized is mutually exclusive. Indeed, assuming the interstitial boron to be a crystallographic feature would have allowed for refinement against the X-ray diffraction data reported in their work, where the partial occupancy at tungsten 2(b) becomes especially apparent. Had this last piece of information been included in their formula, it would have become W0.833B3.34 – W0.833B3.375 = WB4.01 – WB4.05, which is close to the value of WB4.2 reported here.
Finally, it is hoped that the model presented here might serve to unify the computational and experimental interpretations on this compound, as we do not find real contradiction between them. Indeed, although it is an experimental fact that one of the tungsten sites is partially occupied, it is simultaneously true that this same position is fully occupied, as this site is also the center of mass of the boron trimer that replaces it. In this way, the overall structure of the compound may be stable, even when calculations (without boron trimers) show fractional occupancy at tungsten 2(b) to be unfavorable. Furthermore, we leave open the possibility of a range of stoichiometries for the highest boride of tungsten, and perhaps of other metals as well, all based on various degrees of polyhedral substitution at a metal site, with the formula derived here (WB4.2) being only an end member. This observation may in fact turn out to be relatively common, and we might venture to propose that additional scrutiny of other nonstoichiometric borides with apparent homogeneity ranges above MB2 could reveal similar phenomena. Indeed, there is already evidence of at least one other polyhedral replacement compound, where metal atoms are replaced instead by dimerically linked half-icosahedra, in the series Mg2M1-xB6+2x (M = Rh, Ir, 0.25 < x < 0.4) of the Y2ReB6 structure type (46, 47).
Conclusions
In this work, we have presented a new crystal structure for the highest boride of tungsten, obtained by the simultaneous refinement of X-ray and neutron scattering data. The structure of this material has been debated for more than half a century, but the need for a definitive solution has increased dramatically in recent years with the discoveries that WB4.2 is both superhard and can serve as the parent phase for a large family of solid solutions that are even harder (8, 9, 11). Although the crystal structure reported here contains some elements postulated previously—sites that are only partly occupied by tungsten, for example (14, 16, 17, 21)—the structure presents previously unidentified elements as well. The most important of these is the fact that the partially occupied tungsten sites that do not contain W atoms contain boron trimers, and these trimers are within the appropriate distance to couple with the boron layers, producing slightly distorted cuboctahedral boron cages. We postulate that this cage structure is the primary bonding motif responsible for the remarkable hardness of WB4.2.
We conclude by considering the implications of this new crystal structure to the hardness of WB4.2. As mentioned above, WB4.2 is capable of hosting a wide range of solute atoms, and these solute atoms can have a profound effect on hardness, even at very low concentrations (9). Having an accurate model for WB4.2 provides valuable insight toward understanding these phenomena and more directly predicting the means of manipulating the crystal chemistry of this compound. For a low volume, high symmetry, binary compound, the unit cell of WB4.2 contains an unusually large number of unique crystallographic sites. By carefully tailoring a solid solution scheme, it may be possible to select specific guest atoms to replace only the fully occupied tungsten site, only the partially occupied site, or both. It may further be possible to introduce other metals or heteroatoms at the vacant 2(d) position, replacing the cuboctahedra with metal atoms or, conversely, enhancing the frequency and regularity with which they occur (9). Changes in the spatial distribution of boron cuboctahedra upon doping with metal heteroatoms could possibly be the basis for the extraordinary changes in hardness that can be achieved at doping levels of just a few percent. Perhaps most importantly, however, the existence of an accurate crystal structure for WB4.2 should aid in the rational design of new superhard solid solutions using computational methods. As such, this previously unreported crystal structure has potential to lead to improvements in next generation superhard materials.
Materials and Methods
Samples for X-ray and neutron diffraction were prepared in parallel from the same batch of reagents and using the same methodology. High-purity powders of tungsten (99.95%; Strem Chemicals) and crystalline 11B (99.9%, 98.2% 11B enriched; Ceradyne) were manually mixed in the atomic ratio 1:12 using an agate mortar and pestle and consolidated into pellets by means of a hydraulic jack press (Carver). The pellets were placed on a water-cooled copper hearth inside a bell jar and purged several times with ultra-high-purity argon before being arc melted under ∼100-A DC current from a nonconsumable tungsten cathode; ingots containing WB4 platelets cool directly from the placental melt. The samples were crushed to powders using a hardened steel mortar and pestle (Humboldt) and wet ground under methanol/ethylene glycol at low speed in a planetary mill (Pulverisette 5/2; Fritsch) using stainless steel media until the majority passed through a 635 mesh (20 μm) screen (Humboldt). The sieved powders were stirred under three successive aliquots of excess HCl to remove residue from the grinding media. The submicron fraction of each sample was separated by repeated suspension in methanolic ammonia, the fastest settling fraction being retained. This procedure was found to minimize contamination to below the detection limit of the energy dispersive X-ray spectroscopic analyzer (EDAX; EDAX Inc.) mounted on our SEM (JEOL JSM 6700 F).
Nanoindentation was performed using an MTS Nano Indenter XP (MTS) with a Berkovich diamond tip. After calibration of the indenter with a standard silica block, the samples were indented automatically overnight to a depth of 900 nm at 20 randomly determined points and the resulting load versus displacement plots were averaged. The nanoindentation hardness of the material was determined from the loading curves by the method of Oliver and Pharr (48).
Samples for powder X-ray diffraction were deposited directly from methanolic suspension onto silicon (511) “zero-background” plates. Excess sample was removed by a razor blade until nearly perfectly flat. Diffraction patterns were collected from 10° to 156° 2θ using an X’Pert Pro Bragg-Bentano geometry laboratory X-ray diffractometer (PANalytical), using nickel filtered CuKα radiation (λKα1 = 1.540593 Å, λKα2 = 1.5444274 Å) (49), rotating sample stage, 0.04 rad Soller slits, and X'Celerator position sensitive detector.
Neutron diffraction data were collected from the High-Pressure Preferred Orientation beam line at Los Alamos Neutron Science Center (LANCSE), Los Alamos National Lab, Los Alamos New Mexico. This is a neutron time-of-flight machine using five banks of 3H-detector tube panels. Because of the extremely high thermal neutron absorption cross-section of residual 10B, as well as that of natural W, this beam-line was selected due to its very high flux. Powdered samples ∼1 cm3 in volume were loaded into vanadium foil “cans” and irradiated by water-moderated neutrons collimated to 1 cm diameter, while data were collected for a cumulative collection time of 6 h. Powder X-ray and neutron diffraction data were subjected to simultaneous Rietveld refinement (50) using the EXPGUI (51) front-end to the GSAS (52) Rietveld refinement software package.
A single crystal of WB4.2 containing natural boron was isolated from a crushed ingot obtained using the same arc-melting procedure described above. The crystal, having approximate dimensions 250 × 50 × 5 microns, was mounted on a loop filament on an APEX-II CCD diffractometer (Bruker). Using the Olex2 (53) structure solution program, the structure was solved by the charge flipping method and refined using Gauss–Newton minimization with eight parameters and without restraints.
Acknowledgments
The authors thank Drs. Sven Vogel, Luke Deamon, and Helmut Reike at the Lujan Center of the Los Alamos National Laboratory for their help with neutron diffraction experiments; Dr. Saeed Khan for assistance with single-crystal X-ray diffractometry; and Professor Jeng-Ming Yang at the University of California, Los Angeles, Department of Materials Science and Engineering for use of his nanoindentation instrumentation. Ceradyne generously provided materials support through their provision of isotopically enriched 11B, which we gratefully acknowledge. This research was supported financially by the National Science Foundation under Grant 1106364 (to S.H.T. and R.B.K.), the University of California Proof of Concept Program, and the Department of Energy under LANSCE Grant 20112198. Crystal-chemical illustrations in this work were made using the software package VESTA (54).
Footnotes
- ↵1To whom correspondence should be addressed. Email: kaner{at}chem.ucla.edu.
Author contributions: A.T.L. and R.M. designed research; A.T.L. and C.L.T. performed research; A.T.L. analyzed data; and A.T.L., C.L.T., R.M., S.H.T., and R.B.K. wrote the paper.
The authors declare no conflict of interest.
This article is a PNAS Direct Submission.
This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1415018112/-/DCSupplemental.
References
- ↵
- ↵.
- Chung H-Y, et al.
- ↵.
- Kaner RB,
- Gilman JJ,
- Tolbert SH
- ↵
- ↵
- ↵
- ↵
- ↵.
- Mohammadi R, et al.
- ↵
- ↵
- ↵
- ↵
- ↵.
- Chretien A,
- Helgorsky J
- ↵.
- Zeiringer I, et al.
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵.
- Cheng X-Y,
- Chen X-Q,
- Li D-Z,
- Li Y-Y
- ↵
- ↵.
- Emin D,
- Aselage T,
- Beckel CL,
- Howard IA,
- Wood C
- Bullett DW
- ↵.
- Bullett DW
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵.
- Kiessling R
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵
- ↵.
- Kennard CHL,
- Davis L
- ↵
- ↵.
- Alekseeva AM, et al.
- ↵.
- Oliver WC,
- Pharr GM
- ↵
- ↵
- ↵
- ↵.
- Larson AC,
- Von Dreele RB
- ↵
- ↵
Citation Manager Formats
Sign up for Article Alerts
Article Classifications
- Physical Sciences
- Chemistry