Startseite Flux-growth synthesis and structural characterization of R 6Nb4Al43 (R = Sm, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu)
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Flux-growth synthesis and structural characterization of R 6Nb4Al43 (= Sm, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu)

  • Shrenik Patha , Soham Bhatt , Daniel S. Tortorella , Connor Donnelly und Svilen Bobev EMAIL logo
Veröffentlicht/Copyright: 20. Februar 2025

Abstract

Presented are the flux-growth synthesis and the structural characterization of the series of ternary aluminides R 6Nb4Al43, with R representing the rare-earth elements Sm, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu. Although not new compounds, the structures of R 6Nb4Al43 have not been unequivocally established to date. This study showcases comprehensive structural work that has been carried out using single-crystal X-ray diffraction methods. The nine title compounds are shown to be isotypic and to crystallize in a hexagonal crystal system with space group P63/mcm (no. 193). The crystal structure is rather complex and the structure type adopted is known as Ho6Mo4Al43 (Pearson symbol hP106). Structural refinements from single-crystal X-ray diffraction data in all cases help establish the long range crystallographic ordering and no homogeneity width in any of the R 6Nb4Al43 crystals. There is a monotonic decrease in lattice parameters and unit cell volume with increasing the R-element atomic number, corresponding to the lanthanide contraction and the atomic size reduction across the 4f-series. Anomalous behavior in Yb6Nb4Al43 is observed though, whereby a divergence from this trend in decreasing in the unit cell volume is detected. Although not corroborated by magnetic measurements, we posit that the larger than expected the unit cell volume in Yb6Nb4Al43 is likely due to Yb2+/Yb3+ mixed-valent state, where the closed-shell 4f14 electronic configuration for Yb2+ affects the structural parameters, causing the deviation from the rest of the structures with R 3+ ions.

1 Introduction

In the realm of ternary aluminides, the R 6 T 4Al43 series (R = rare-earth element, T = early transition metal) constitutes a relatively large class of compounds. 1 , 2 , 3 , 4 , 5 , 6 , 7 , 8 , 9 , 10 , 11 , 12 , 13 , 14 , 15 Although a number of R 6 T 4Al43 phases were discovered nearly simultaneously in the early 1990s by teams from Ukraine, Switzerland, and Germany, the structure of Ho6Mo4Al43 is now known as the prototype of this family. 1 , 2 , 3 , 4 This likely plays homage to Niemann and Jeitschko, who identified it, and also conducted extensive pioneering research on a lot of “6–4–43” aluminides. 1 , 2 The phase space covered in their exploratory work included the rare-earth metals Nd, Sm, Gd–Lu, as well as Y, Th, and U, and the transition metals Ti, V, Cr, Nb, Mo, Ta, and W. This initial work not only found various compounds within the Ho6Mo4Al43 family exhibiting complex structural features and interesting magnetic correlations, but also have since proven instrumental in establishing a baseline understanding of the structural and electronic complexities of aluminides. The key findings from the now 30-year old works have been consistently observed in later research on other ternary and quaternary Al-rich phases. 6 , 7 , 8 , 9 , 10 , 11 , 12 , 13 , 14

The subsequent identification of more ternary compounds that are analogous to Ho6Mo4Al43 revealed further significant insights, particularly regarding the stability and unique structural features of this complicated hexagonal crystal structure (Pearson symbol hP106). In recent years, research on the R 6 T 4Al43 series has been extended, highlighting the compounds’ distinct structural and magnetic properties. 16 , 17 , 18 , 19 , 20 From surveying the literature though, one will notice that while most works provide the lattice constants from powder X-ray diffraction and reasonably close basic estimations of magnetic moments, the expectations that the crystal structures will be unequivocally established, frequently are not met. We will also draw attention to the fact that while several papers have reported physical properties of ternary R–Nb–Al compounds, 7 , 9 there appear to be no entries in the crystallographic database validating their structures. 21 Considering that some prior structure refinements from single-crystal X-ray diffraction have indicated a measurable degree of T–Al atomic disordering, such as in Yb6Cr4+x Al43–x (x = 1.15–1.76) and even the Ho6Mo4Al43 prototype, the structure of which has been published with ca. 97/3 % mixing of Al and Mo on site Al6 (vide infra), 1 , 2 , 3 , 4 we posit that there is a need to further synthesize “6–4–43” aluminides and carefully characterize compounds’ structural features. Accordingly, our research goals sought to append our understanding of the nuances of the R 6Nb4Al43 crystal structure through experimental work focused on flux-growth synthesis and characterization by single-crystal X-ray diffraction (SCXRD) methods. By focusing on SCXRD, it was anticipated that the previously mentioned discrepancies between the ideal and the real crystal structure that may arise from an undetected (small or large) degree of atomic disordering, would be avoided.

2 Materials and methods

2.1 Synthesis

All starting materials were pure elements sourced from Thermo Scientific with a stated purity 99.9 %wt. or higher. They were stored and handled inside an argon-filled glovebox (p(O2) ≤ 1 ppm). Each element was weighed to the stoichiometric ratio 1:1:20. After weighing, the elements were put in Coorstek 2 cm3 alumina crucibles, which were subsequently transferred to fused silica tubes and capped with quartz wool. The tubes were evacuated and flamed-sealed in order to maintain an oxygen-free and airtight environment during the heat treatment. The sealed tubes were placed upright in muffle furnaces equipped with programmable temperature controllers. The heating profile included a gradual increase in temperature to 1,373 K at a rate of 100 K/h, where the temperature was maintained for 24 h. Following this, the temperature was decreased to 1,023 K at a rate of 50 K/h and held for 3 h before the remaining molten Al was centrifuged while still orange-hot.

This process effectively separated the R 6Nb4Al43 crystals from the aluminum growth medium, although not to the fullest extent. Residual Al metal was partially removed by soaking the samples in concentrated NaOH solutions for several hours and washing them thoroughly with distilled water. This harsh treatment did not appear to affect the R 6Nb4Al43 crystals, although we note that their surfaces were left tarnished post-treatment. The crystallographic quality of such pieces was not severely diminished, although we preferred to use untreated crystals for our crystallography work.

The as-grown crystals of all title phases exhibit metallic luster. They are stable in air over periods greater than 6 months.

2.2 Structural characterization

The synthesized samples were initially characterized by powder X-ray diffraction (PXRD) to confirm phase purity. Small portions of each sample were ground into a fine powder before undergoing PXRD analysis. The collected powder patterns (a Rigaku MiniFlex diffractometer operating in Bragg-Brentano configuration and equipped with a sealed Cu-source energized at 450 W of power) were cross-referenced with the custom structure database to confirm the outcome of each synthesis. Once phase identifications were verified by PXRD, crystals from each sample were subjected to single-crystal X-ray diffraction (SCXRD) in order to gather precise structural data. SCXRD analysis provided detailed insights into the spatial arrangement of atoms within the unit cell, and helped establish all structures as disorder-free, which allows for a comprehensive understanding of the crystal structure and ensured robust structural characterization.

All single-crystal X-ray diffraction experiments were done on a Bruker APEX III diffractometer equipped with monochromatized Mo Kα radiation (λ = 0.71073 Å). Data were collected at 200 K, a temperature that was maintained by a cryostat using cold flow of gas evaporated from liquid nitrogen. Suitable-sized single crystals were selected under the microscope and mounted on plastic loops. Raw data processing, including absorption corrections, was performed with the Bruker-supplied software. Standard coordinates from the known structure of Ho6Mo4Al43 were used as a starting model for refinements, which were performed with the full-matrix least-squares methods on F 2 implemented in the program SHELXL. 22 The refinements converged quickly to low conventional residuals and featureless difference Fourier maps, confirming the validity of the model. Refinements of site occupation factors showed no statistically significant deviations from 100 %, which is indicative of all structures exhibiting long-range ordering without measurable defects and/or admixing of atoms on the same sites, as suggested previously for some “6–4–43” aluminides, particularly those with Cr. 1 , 2 , 3 , 4

Selected details of the data collection and crystallographic parameters are provided in Tables 13.

Table 1:

Selected data collection details and crystallographic data for Sm6Nb4Al43, Gd6Nb4Al43, and Tb6Nb4Al43.

Sm6Nb4Al43 Gd6Nb4Al43 Tb6Nb4Al43
Space group P63/mcm P63/mcm P63/mcm
Fw/g mol−1 2,433.88 2,475.28 2,485.30
a/Å 11.1353(4) 11.1088(4) 11.0941(4)
c/Å 17.9450(10) 17.8862(10) 17.8468(10)
V/Å3 1926.98(15) 1911.54(14) 1902.28(14)
Z 2 2 2
ρ calc/g cm−3 4.20 4.30 4.34
μ/cm−1 111.2 124.1 131.6
Collected: Independent reflections 15,117:1,054 14,662:1,005 15,447:1,089
Goodness of fit 1.069 1.029 1.032
R 1 (I > 2σ(I))a 0.0251 0.0266 0.0256
wR 2 (I > 2σ(I))a 0.0416 0.0504 0.0420
R 1 (all data)a 0.0370 0.0422 0.0368
wR 2 (all data)a 0.0439 0.0548 0.0447
Δρ max,min/e Å−3 1.11,−0.85 0.96,−0.95 0.81,−0.83
CCDC deposition number 2409524 2409521 2409522
  1. a R 1 = Σ ∣ ∣F o∣−∣F c∣ ∣/ΣF o∣; wR 2 = (Σ [w(F o 2 − F c 2)2]/ΣwF o 4)1/2, w = 1/[σ2(F o 2) + (AP)2 + (BP)], where P = (F o 2 + 2F c 2)/3; A and B are weight coefficients.

Table 2:

Selected data collection details and crystallographic data for Dy6Nb4Al43, Ho6Nb4Al43, and Er6Nb4Al43.

Dy6Nb4Al43 Ho6Nb4Al43 Er6Nb4Al43
Space group P63/mcm P63/mcm P63/mcm
Fw/g mol−1 2,506.78 2,521.36 2,535.34
a/Å 11.0804(4) 11.0733(4) 11.0633(4)
c/Å 17.8123(7) 17.7888(9) 17.7612(8)
V/Å3 1893.92(12) 1889.00(14) 1882.66(13)
Z 2 2 2
ρ calc/g cm−3 4.40 4.43 4.45
μ/cm−1 138.5 145.9 154.0
Collected: Independent reflections 14,786:1,001 14,555:999 14,565:991
Goodness of fit 1.037 1.060 1.071
R 1 (I > 2σ(I))a 0.0242 0.0217 0.0246
wR 2 (I > 2σ(I))a 0.0353 0.0375 0.0419
R 1 (all data)a 0.0336 0.0318 0.0371
wR 2 (all data)a 0.0371 0.0395 0.0443
Δρ max,min/e Å−3 1.01,−1.04 1.02,−0.85 0.96,−0.99
CCDC deposition number 2409523 2409525 2409527
  1. a R 1 = Σ ∣ ∣F o∣−∣F c∣ ∣/ΣF o∣; wR 2 = (Σ [w(F o 2 − F c 2)2]/ΣwF o 4)1/2, w = 1/[σ2(F o 2) + (AP)2 + (BP)], where P = (F o 2 + 2F c 2)/3; A and B are weight coefficients.

Table 3:

Selected data collection details and crystallographic data for Tm6Nb4Al43, Yb6Nb4Al43, and Lu6Nb4Al43.

Tm6Nb4Al43 Yb6Nb4Al43 Lu6Nb4Al43
Space group P63/mcm P63/mcm P63/mcm
Fw/g mol−1 2,545.36 2,570.02 2,581.60
a/Å 11.0610(6) 11.0872(4) 11.0425(7)
c/Å 17.7389(14) 17.8344(9) 17.6895(16)
V/Å3 1879.5(3) 1898.60(14) 1868.0(3)
Z 2 2 2
ρ calc/g cm−3 4.50 4.50 4.59
μ/cm−1 161.9 167.9 179.0
Collected: Independent reflections 15,137:1,077 14,620:1,002 15,137:1,068
Goodness of fit 1.077 1.051 1.061
R 1 (I > 2σ(I))a 0.0223 0.0273 0.0277
wR 2 (I > 2σ(I))a 0.0384 0.0451 0.0518
R 1 (all data)a 0.0295 0.0409 0.0295
wR 2 (all data)a 0.0399 0.0482 0.0542
Δρ max,min/e Å−3 0.82,−0.71 1.47,−1.10 1.07,−0.88
CCDC deposition number 2409526 2409528 2409520
  1. a R 1 = Σ ∣ ∣F o∣−∣F c∣ ∣/ΣF o∣; wR 2 = (Σ [w(F o 2 − F c 2)2]/ΣwF o 4)1/2, w = 1/[σ2(F o 2) + (AP)2 + (BP)], where P = (F o 2 + 2F c 2)/3; A and B are weight coefficients.

3 Results and discussions

3.1 Synthesis

The initial observation for the formation of a ternary R–Nb–Al compound was made during the attempt to synthesize another rare-earth metal-containing compound from Al flux in a crucible made from Nb tubing. The experiment was conducted because the standard-design Al2O3 crucibles would crack at high temperature and the contents would leak, causing failures. Using a metallic crucible was considered, and Nb was chosen because the laboratory uses 3/8˝ tubing for other types of experiments. Under the stated conditions (see Experimental), crystals of R 6Nb4Al43 could be indentified in several batches, which prompted our attention to systematically work out the flux-synthesis of all possible R 6Nb4Al43 phases. So far, we have succeeded in obtaining 9 of the possible 14 (all metals from La through Lu, excluding the radioactive Pm).

Extensive attempts to make R 6Nb4Al43 from stoichiometric melts were not made during this study. Only several tries employing an arc melter can be noted here. This method (without subsequent annealing) only led to the formation of binary phases, such as NbAl2 and RAl3, rather than the target ternary aluminides. It is possible that the very high temperatures of the arc caused partial volatilization, preventing the formation of the desired phase. An alternative synthesis in welded Nb-tubes involving an induction furnace and rection temperature of 1,373 K also failed, which points at the high melting point of niobium as the possible culprit. We speculate that much longer reaction times may be required for such experiments to succeed. Of course, it is also possible that R 6Nb4Al43 are metastable phases and that excess Al creates a favorable reaction medium and allows for the crystallization of R 6Nb4Al43 at lower temperatures, where it does not “compete” with thermodynamically stable binaries.

Attempts to make R 6Nb4Al43 for R = La, Ce, Pr, Nd were also made, both by flux and direct reaction methods, but were not successful. Powder X-ray diffraction patterns from these samples were indicative of multi-phase products. The diffraction data also point at the possible formation of ternary phases, whose structures remain unresolved to date.

We will also note here that the synthesis of Lu6Nb4Al43 was particularly challenging. The observation that during synthesis, multi-phase mixtures will always result, and that their relative amounts would vary from one experiment to another, points at the need for more careful control of the reaction condition in this case. Despite these challenges, crystals of Lu6Nb4Al43 were successfully grown and analyzed, showcasing the expected lattice contraction and density increase. We posit that due to Lu’s small atomic radius, other interatomic contacts within the structure become “strained”. The reverse may also be true for the lighter R-elements, whose atoms are larger, which can cause less tighter packing, potentially leading to structural instabilities. Another possible explanation for the synthetic challenges encountered during the synthesis of Lu6Nb4Al43 is the very high melting point of Lu, and/or its solubility in molten Al. This also underscores the impact of R on the crystal formation and stability, highlighting the need for tailored synthesis approaches to maintain structural fidelity when working with the elements from the lanthanide series.

3.2 Crystal structure and bonding

The archetype structure for the reported compounds is well known and does not require an extensive description in this article. In the following paragraphs, we will provide only a brief account, focusing on several important structural details.

Selected crystallographic data for R 6Nb4Al43 (R = Sm, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu) can be found in Tables 13. Additionally, Table 4 displays the atomic coordinates and the equivalent displacement for the atoms in the asymmetric unit of Sm6Nb4Al43, chosen as a representative example. As seen from Table 4, there are 10 crystallographically independent atoms, all in special positions except Al1, which takes the 24l position with no symmetry constraints. A schematic view of this rather complicated structure is shown in Figure 1.

Table 4:

Refined atomic coordinates and equivalent isotropic displacement parameters (U eq a) for Sm6Nb4Al43.

Atom Wyckoff Symmetry x y z U eq /2
Sm1 12k . . m 0.52845(3) 0 0.09538(1) 0.0076(1)
Nb1 6g m2m 0.72870(6) 0 1/4 0.0056(2)
Nb2 2b 3 . m 0 0 0 0.0053(3)
Al1 24l 1 0.1590(1) 0.3950(1) 0.16373(6) 0.0093(3)
Al2 12k . . m 0.1591(2) 0 0.61548(9) 0.0096(4)
Al3 12k . . m 0.2551(2) 0 0.02965(9) 0.0090(4)
Al4 12j m . . 0.1487(2) 0.5946(2) 1/4 0.0091(4)
Al5 12i . . 2 0.24736(9) 0.4947(2) 0 0.0093(4)
Al6 8h 3 . . 1/3 2/3 0.1260(1) 0.0088(4)
Al7 6g m2m 0.1480(2) 0 1/4 0.0089(5)
  1. a U eq is defined as one-third of the trace of the orthogonalized U ij tensor.

Figure 1: 
Ball-and-stick representation of the hexagonal crystal structure of Sm6Nb4Al43, viewed down the [0001] direction. Cylinders represent Al–Al contacts 3.1 Å and shorter (for clarity, only Al–Al bonding is taken into consideration here). Al atoms are drawn in turquoise, Nb atoms are in light green, and the atoms of the rare-earth metal are magenta colored. Unit cell is outlined.
Figure 1:

Ball-and-stick representation of the hexagonal crystal structure of Sm6Nb4Al43, viewed down the [0001] direction. Cylinders represent Al–Al contacts 3.1 Å and shorter (for clarity, only Al–Al bonding is taken into consideration here). Al atoms are drawn in turquoise, Nb atoms are in light green, and the atoms of the rare-earth metal are magenta colored. Unit cell is outlined.

As one might infer from the chemical formula, and the abundance of Al sites (seven), there is extensive Al–Al bonding, which is what we emphasize in Figure 1. Overall, the structure can be viewed as a framework of fused Al polyhedra, the largest ones hosting the rare-earth metal and Nb atoms. From the figure, one ought to be able to distinguish various Al6-octahedra and trigonal prisms, Al5-square prisms, as well as larger Al12-icosahedral fragments. The most unusual polyherdron is perhaps that around Al6, which is showing 9 nearest Al neighbors (Figure 2). When three close by rare-earth metals are considered, the environment of Al6 becomes an icosahedron. It is noteworthy that the Al6 site in many analogs of Ho6Mo4Al43 is known to host admixtures of Al and transition metal atoms. 1 , 2 , 3 , 4 For instance, in Yb6Cr4+x Al43–x , Al6 is reported as 56 % Al and 44 % Cr. 4 In all of our refined structures, however, Al6 does not show contributions from Nb mixing in.

Figure 2: 
Schematic view of the pseudo-icosahedral environment around Al6 in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Sm−Al contacts 3.5 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the atoms of the rare-earth metal are colored in magenta.
Figure 2:

Schematic view of the pseudo-icosahedral environment around Al6 in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Sm−Al contacts 3.5 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the atoms of the rare-earth metal are colored in magenta.

The polyhedron around the largest atom in the structure, Sm, on the representative example Sm6Nb4Al43, is understandably the largest. According to the structural representation shown in Figure 3, Sm has 15 nearby Al atoms. Including into a consideration one Nb atom and one additional Sm atom, both located within 3.5 Å, makes for a polyhedron that has 17 vertices. Notably, two such Sm-centered polyhedra are integrown, sharing a “hexagonal” face made by four Al5 and two Al3 atoms.

Figure 3: 
Schematic view of the pseudo-icosahedral environment around Sm in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Sm−Al contacts 3.5 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the atoms of the rare-earth metal are colored in magenta.
Figure 3:

Schematic view of the pseudo-icosahedral environment around Sm in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Sm−Al contacts 3.5 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the atoms of the rare-earth metal are colored in magenta.

The polyhedra around the two independent Nb atoms in the structure are both with coordination number (CN) 12. Nb2, which occupies the more symmetric position with Wyckoff symbol 2b at the origin, has a nearly perfect icosahedron around itself (Figure 4a). The 12 vertices are Al2 and Al3 atoms only. The packing of the Nb2-centered, Al6-centered, and the Sm-centered polyhedra on the ab-plane is depicted in Figure 4b.

Figure 4: 
Schematic view of the icosahedral environment around Nb2 in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Nb–Al contacts 3.1 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the Nb are colored in light green. (a) Nb2 atoms at the centers of icosahedra at the unit corners. (b) A slab of approximate thickness 8 Å, cut parallel to (0001) at z ∼ 0.05 and showing how the polyhedra around Sm, Nb2 and Al6 at packed.
Figure 4:

Schematic view of the icosahedral environment around Nb2 in the structure of Sm6Nb4Al43. Cylinders represent Al–Al contacts 3.1 Å and shorter; Nb–Al contacts 3.1 Å and shorter are depicted with thin solid lines. Al atoms are drawn in turquoise, and the Nb are colored in light green. (a) Nb2 atoms at the centers of icosahedra at the unit corners. (b) A slab of approximate thickness 8 Å, cut parallel to (0001) at z ∼ 0.05 and showing how the polyhedra around Sm, Nb2 and Al6 at packed.

Finally, we will briefly comment on the polyhedron around the Nb1 atoms in the structure, which are also with CN 12, but this count includes two neighboring rare-earth atoms. From the chosen representation on Figure 5, one can see how these less-regularly shaped icosahedra share corners and are intergrown together with the Al6-centered icosahedra, which also include three rare-earth metal atoms. The space around is packed with “empty” Al-polyhedra of smaller size (prisms and octahedra).

Figure 5: 
Schematic view of the icosahedral environment around Nb1 in the structure of Sm6Nb4Al43. Al and Nb atoms are drawn in turquoise and light green, respectively. The Sm atoms are colored in magenta. A slab of approximate thickness 8 Å, cut parallel to (0001) at z ∼ 0.25 shows showing how the polyhedra around Nb1 and Al6 at packed together.
Figure 5:

Schematic view of the icosahedral environment around Nb1 in the structure of Sm6Nb4Al43. Al and Nb atoms are drawn in turquoise and light green, respectively. The Sm atoms are colored in magenta. A slab of approximate thickness 8 Å, cut parallel to (0001) at z ∼ 0.25 shows showing how the polyhedra around Nb1 and Al6 at packed together.

3.3 Periodic trends

The lanthanide contraction is a prominent trend in this study, as evidenced by a systematic reduction in lattice parameters and unit cell volume as atomic number increases from Sm to Lu (Tables 13). This is the consequence from the limited shielding provided by f-electrons, which allows the nucleus to exert a stronger pull on outer electrons, effectively reducing the atomic radius. Moving across the lanthanide series, lattice parameters decrease steadily, which makes all Al–Al, Nb–Al, R–Al, and RR contacts contract. The inability to synthesize R 6Nb4Al43 for = La, Ce, Pr, Nd showcases how the atomic size of the rare-earth metal influences overall crystal packing and underpins the stability of the crystal structure across the series. This trend also implies that structural and potentially electronic properties may vary predictably with the choice of R-element.

A clear deviation from the lanthanide contraction trend is the compound Yb6Nb4Al43, presenting a slightly larger lattice parameter and unit cell volume than expected for its position in the series (Figure 6). The lattice parameters for Yb6Nb4Al43 are larger relative to its neighbors in the series, a behavior likely stemming from Yb’s unique ability to exist in both 4f13 (Yb3+) and 4f14 (Yb2+) electronic configurations. This is suggestive that all, or a part of the Yb ions in Yb6Nb4Al43 are Yb2+, having closed-shell electron arrangement that affects its atomic radius, and effectively causing this phase to behave differently than the other isotypic materials where the rare-earth elements have partially filled f-orbitals (except the case of Lu of course). Similar mixed-valent Yb2+/Yb3+ behavior has been reported for the isotypic Yb6V4Al43 and Yb6Ta4Al43 phases. 7

Figure 6: 
Relationship between unit cell volume (V) and atomic number (Z) for the R
6Nb4Al43 series. The values are those from Tables 1–3, obtained by single-crystal X-ray diffraction methods. A general decrease in volume with increasing atomic number is observed, consistent with lanthanide contraction. An anomaly at Yb (Z = 70) indicates that all, or part of, the Yb ions in Yb6Nb4Al43 are Yb2+.
Figure 6:

Relationship between unit cell volume (V) and atomic number (Z) for the R 6Nb4Al43 series. The values are those from Tables 13, obtained by single-crystal X-ray diffraction methods. A general decrease in volume with increasing atomic number is observed, consistent with lanthanide contraction. An anomaly at Yb (Z = 70) indicates that all, or part of, the Yb ions in Yb6Nb4Al43 are Yb2+.

4 Conclusions

Although R 6Nb4Al43 compounds have been reported before, to date, their crystal structures have not been systematically ascertained. This study’s findings shed light on the crystal growth and crystal structures of nine members of the R 6Nb4Al43 series, providing valuable insights into the crystallography of these ternary aluminides with the hexagonal Ho6Mo4Al43-type structure. Specifically, none of the refined crystal structures exhibited signs of positional or occupational disorder. The systematic analysis across different rare-earth elements revealed a clear trend of decreasing lattice parameters with increasing atomic number, consistent with the lanthanide contraction.

Within the entrire R 6Nb4Al43 series, the periodic trend in unit cell parameters is disrupted by Yb6Nb4Al43, which displays an anomalous increase in volume. This deviation is a likely a telltale sign of Yb valence instabilities, suggesting that this phase could exhibit unique physical properties. This knowledge adds to the foundation for advancing our understanding of complex aluminides and optimizing their properties. Overall, the results from this work pave the way for future research to explore the magnetic anisotropy and electronic behavior of these and related materials.


Corresponding author: Svilen Bobev, Department of Chemistry and Biochemistry, University of Delaware, Newark, DE 19716, USA, E-mail:

Funding source: United States Department of Energy, Office of Science, Basic Energy Sciences

Award Identifier / Grant number: #DE-SC0008885

Acknowledgments

The authors are indebted to Dr. M. O. Ogunbunmi, Dr. K. Ghosh and Mrs. S. Rahman for their help with the operation of the single-crystal X-ray diffractometer.

  1. Research ethics: All authors have read and agreed to the published version of the manuscript.

  2. Informed consent: Not applicable.

  3. Author contributions: Methodology, conceptualization S.B. (Svilen Bobev); investigation, S.P., S.B. (Soham Bhatt), and C.D.; validation, D.T.; formal analysis, S.P., S.B. (Soham Bhatt), C.D., and D.T.; data curation, S.P., S.B. (Soham Bhatt), and D.T.; writing – original draft preparation, S.P., S.B. (Soham Bhatt), and D.T.; visualization, S.P., S.B. (Soham Bhatt), D.T., and S.B. (Svilen Bobev); writing – review and editing, S.B. (Svilen Bobev); supervision, project administration, funding acquisition S.B. (Svilen Bobev).

  4. Use of Large Language Models, AI and Machine Learning Tools: None declared.

  5. Conflict of interest: The authors declare no conflicts of interest.

  6. Research funding: Financial support from the United States Department of Energy, Office of Science, Basic Energy Sciences, under Award #DE-SC0008885 is gratefully acknowledged.

  7. Data availability: The corresponding crystallographic information files (CIF) have been deposited with the Cambridge Crystallographic Database Centre (CCDC) with the following depository numbers: 2409520–2409528. The files can be obtained free of charge via https://www.ccdc.cam.ac.uk/ or by sending an email to .

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Received: 2025-01-03
Accepted: 2025-01-24
Published Online: 2025-02-20
Published in Print: 2025-03-26

© 2025 the author(s), published by De Gruyter, Berlin/Boston

This work is licensed under the Creative Commons Attribution 4.0 International License.

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