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. 2021 Jul 28;60(16):12158–12171. doi: 10.1021/acs.inorgchem.1c01355

Overlooked Binary Compounds Uncovered in the Reinspection of the La–Au System: Synthesis, Crystal Structures, and Electronic Properties of La7Au3, La3Au2, and La3Au4

Alexander Ovchinnikov 1, Anja-Verena Mudring 1,*
PMCID: PMC8389835  PMID: 34319098

Abstract

graphic file with name ic1c01355_0013.jpg

Although compound formation between two elements is well studied, thorough investigations make it possible to uncover new binary compounds. A re-examination of the La–Au system revealed three new phases, which were characterized with respect to their structural and electronic properties as well as thermal stability: La7Au3 (Th7Fe3 type, space group P63mc, Pearson code hP20) appears to be metastable. It can be obtained by slow crystallization from a stoichiometric melt. La3Au2 (U3Si2 type, space group P4/mbm, Pearson code tP10) is stable up to 1013 K, where it decomposes peritectically. La3Au4 (Pu3Pd4 type, space group R3̅, Pearson code hR14) is thermally stable up to at least 1273 K. In addition, the crystal structures of La2Au (anti-PbCl2 type, space group Pnma, Pearson code oP12) and α-LaAu (FeB type, space group Pnma, Pearson code oP8) could be determined by single-crystal X-ray diffraction. The electronic structures and chemical bonding have been evaluated from first principles calculations. They show that all compounds can be viewed as electron-rich, polar intermetallics.

Short abstract

Revisiting the La−Au phase diagram unveils three new binary phases

Introduction

The location of gold in the sixth period of the periodic table lends this element physical and chemical characteristics that are often strikingly different from those of the lighter congeners in group 11.1 To a large extent, these differences are associated with strong relativistic effects impacting the electronic properties of the gold valence states.1,2 In particular, relativistic stabilization of the 6s2 electronic configuration results in a high electronegativity of gold, comparable to that of iodine on the Pauling scale,3 although some recently developed electronegativity scales suggest a somewhat lower value for Au in comparison to I.4,5 For this reason, compounds of Au with other metals frequently reveal a significant transfer of the electron density to the Au atoms, which allows their description as aurides, i.e., phases with anionic Au species. Arguably, the most illustrative and well-studied example is the ionic compound (Cs+)(Au), adopting the CsCl structure type and displaying an optical band gap of 2.5 eV.68 The highly ionic nature of this salt-like material is also reflected in its ability to form crystal solvates, such as CsAu·NH3.9 Quite often, gold and iodine compounds are found to be isostructural, e.g., CsAu and CsI and oxygen-containing phases with anionic Au or I: A3XO (A = K, Rb, Cs; X = I, Au)10 and (AX)2(A3AuO2) (A = K, Rb; X = I, Au).11,12 Similar to iodine, anionic gold forms polyanions, albeit they rarely are isotypic. The Au substructures in aurides form polyanions of various dimensionalities, ranging from isolated Au atoms to three-dimensional frameworks.1 This opens up possibilities for crystal structure design, which likely have not been brought to full potential yet.

From the physics perspective, the relativistic properties of gold, for instance, strong spin–orbit coupling, may be utilized to induce and tune various physical phenomena, especially in multinary Au-containing systems, where higher structural flexibility can be achieved. Examples include topologically nontrivial electronic states13 and unconventional magnetic orders and spin dynamics in compounds of Au with magnetic elements.14

Gold-containing intermetallics are conventionally produced by annealing Au with other metals at elevated temperatures, usually close to or above the melting point of some or all of the reactants. In many cases, induction or arc furnaces are utilized for these purposes.1518 Because of the high reaction temperatures, mainly thermodynamically stable compounds are produced by such methods. Since diffusion rates drop considerably with decreasing temperature, targeting metastable or low-temperature phases is challenging, especially when various compositionally close phases exist in the system.19 Long annealing times are necessary to afford the completion of solid-state reactions at low temperatures. Alternatively, chemical activities can be increased by utilizing suitable media, e.g., low-melting metal fluxes or molten salts. Although the flux approach has yielded many intermetallic compounds not easily accessible by conventional high-temperature methods,2024 its application to Au-containing compositions remains rather limited,2527 mostly because the intended reaction partner for gold often forms stable phases with the flux constituents instead.

In this contribution, we present the synthesis and characterization of three new binary La aurides—La7Au3, La3Au2, and La3Au4—which were discovered by us first during an investigation of the ternary systems La–TM–Au, where TM is a magnetic transition metal. Our initial motivation was to design materials with unusual magnetic arrangements, such as noncollinear magnetic structures. The titular binary phases came out as a side result of those exploratory efforts. Subsequently, we targeted these compounds by re-examining the binary La–Au system. While La7Au3 appears to be metastable, La3Au2 and La3Au4 are thermodynamically stable phases, although La3Au2 exhibits a rather limited thermal stability window. In addition, we re-examined the compositionally close compounds La2Au and LaAu. Electronic structure calculations and bonding analysis reveal that all studied materials are metallic and belong to the class of polar intermetallics and hence can be described as aurides.

Experimental Section

Synthesis

All weighing and mixing procedures were carried out in an Ar-filled glovebox with a controlled atmosphere. Single-phase polycrystalline samples of La3Au2 and La3Au4 were prepared by a two-step procedure. First, stoichiometric mixtures of La (HEFA Rare Earth, 99.9 wt %) and Au (NEYCO, 99.999 wt %) were arc-melted three times to ensure homogeneity. The weight losses at this step were smaller than 0.6 wt %. The as-cast buttons were wrapped in Mo foil and sealed in evacuated fused silica tubes. The tubes were loaded in box furnaces and annealed at 973 K over a period of 10 days for La3Au2 and at 1073 K over a period of 7 days for La3Au4. To reach the target temperatures a heating rate of 200 K/h was applied. After the annealing step, the furnaces were switched off, and the samples were allowed to cool to room temperature naturally. It is worth noting that in the case of La3Au4, the sample came out single-phase directly after arc melting. Prolonged annealing helped to improve crystallinity.

The La-richest phase La7Au3 could not be prepared as single-phase. The cleanest sample containing about 30 wt % La7Au3 was produced by combining the elements with the stoichiometric ratio by arc melting and melting the as-cast pellet at 873 K in a Mo boat jacketed in an evacuated fused silica tube, followed by cooling to 773 K at a rate of 5 K/h.

To check for possible stabilization of La7Au3 by the presence of hydrogen, occasionally reported in intermetallic compounds,28 we attempted the remelting of an as-cast button with the nominal composition La7Au3 under hydrogenating conditions. For this purpose, the button was placed in an alumina crucible sealed in an evacuated fused silica tube along with a small amount of TiH2 powder (Alfa Aesar, ≥99 wt %), loaded in a separate alumina crucible and topped with quartz wool. The employed heating program was the same as the one described above for the La7Au3 sample. The reported onset of thermal decomposition of TiH2 is around 673 K.29 The used amount of TiH2 corresponded to a H2 pressure of 500 mbars at T = 873 K if complete decomposition of TiH2 into Ti metal and H2 is assumed. Of course, this value is an upper estimate. The hydrogenation reaction did not result in the formation of La7Au3, producing LaH2 and an unidentified crystalline product instead.

The crystal structures of La2Au and LaAu, the phases located in the compositional vicinity of the newly discovered binaries, were never accurately determined, which motivated us to conduct crystallographic studies for these compositions as well. Single crystals of the low-temperature modification α-LaAu were found in a sample with nominal composition La3Au2 annealed at 1273 K for 5 h and cooled to room temperature at a rate of 5 K/h. Another La-rich binary auride, La2Au, was reproducibly observed in samples during exploratory synthesis attempts. Because of their high ductility and malleability, La2Au single crystals prepared by high-temperature treatment of the elements were not of sufficient quality for X-ray diffraction analysis. Suitable crystals were grown using a La flux. A mixture of La and Au with the molar ratio 10:3, respectively, was loaded in a Ta tube sealed at one end. After that, the tube was welded shut under high-purity Ar using a custom-built arc welder and placed in an evacuated fused silica tube. The mixture was heated to 1223 K at a rate of 200 K/h, kept at this temperature for 5 h, and cooled to 773 K at a rate of 5 K/h. At this point, the heating was turned off and the sample was cooled to room temperature. The Ta tube was cut open inside the glovebox. Submillimeter-sized single crystals of La2Au were mechanically extracted from the La matrix.

For the binary compounds in this contribution, we attempted crystal growth from a Pb flux, as a more convenient alternative for long annealing in the solid state. However, in all cases, LaPb3 was the main product and no binary La–Au phases were produced.

Powder X-ray Diffraction (PXRD)

PXRD patterns were collected in reflection geometry on a PANalytical X’Pert diffractometer (Cu Kα1 λ = 1.54056 Å) and on a Bruker Phaser D2 diffractometer (filtered Cu Kα λmean = 1.5418 Å) in the 2θ range of 5–90° with a step size of 0.013°. The samples were immobilized on low-background silicon holders with vacuum grease. Rietveld refinements were carried out using the JANA2006 software.30

Single-Crystal X-ray Diffraction (SCXRD)

Suitable crystals were selected under vacuum grease and mounted on low-background plastic loops. Data collection for all studied compounds was performed at room temperature on a Bruker D8 Venture (Mo Kα λ = 0.71073 Å) equipped with a PHOTON 100 CMOS detector. In addition, a low-temperature measurement (T = 100 K) was conducted for a crystal of La3Au4. For this purpose, the crystal was cooled with a stream of nitrogen using an OxfordCryosystems cooling setup. Data integration and absorption corrections were performed using the SAINT31 and SADABS32 software, respectively. Crystal structures were solved by dual-space methods as implemented in SHELXT33 and refined by a full-matrix least-squares method on F2 with SHELXL.34 Atomic coordinates were standardized using STRUCTURE TIDY.35 Details of the data collection and selected crystallographic parameters are summarized in Tables 112 (room-temperature measurements) and S1–S3 (low-temperature measurements).

Table 1. Refinement Details and Selected Crystallographic Data for La7Au3, La3Au2, and La3Au4 (Room Temperature, Mo Kα, λ = 0.71073 Å).

refined composition La7Au3 La3Au2 La3Au4
CCDC number 2072067 2072068 2072069
fw/g mol–1 1563.27 810.66 1204.60
space group P63mc (no. 186) P4/mbm (no. 127) R3̅ (no. 148)
Z 2 2 6
a 10.5726(7) 8.431(3) 14.038(3)
c 6.5801(5) 4.0618(15) 6.2248(5)
V3 636.98(10) 288.7(2) 1062.4(5)
ρcalc/g cm–3 8.151 9.325 11.297
μMo Kα/mm–1 57.24 72.18 100.08
Rint 0.042 0.046 0.055
R1 [I > 2σ(I)]a 0.022 0.024 0.022
wR2 [I > 2σ(I)]a 0.038 0.053 0.047
R1 [all data]a 0.026 0.026 0.026
wR2 [all data]a 0.038 0.053 0.048
Flack parameter 0.029(9)    
Δρmax,min/e Å–3 1.36, −1.16 1.35, −1.38 1.72, −1.15
a

R1 = ∑||F0| – |Fc||/∑|F0|; wR2 = [∑[w(F02Fc2)2]/∑[w(F02)2]]1/2, where w = 1/[σ2F02 + (AP)2 + (BP)] and P = (F02 + 2Fc2)/3. A and B are the respective weight coefficients. (See the CIF data.)

Table 12. Selected Interatomic Distances (Å) in α-LaAu.

atoms distance
La –Au 3.1459(10)
  –Au 3.1777(10)
  –Au 3.1894(11)
  –Au × 2 3.2000(7)
  –Au × 2 3.2070(7)
  –La × 4 3.9472(6)
  –La × 2 4.0104(7)
  –La × 2 4.0671(14)
Au –Au × 2 3.0218(7)
  –La 3.1459(10)
  –La 3.1777(10)
  –La 3.1894(11)
  –La × 2 3.2000(7)
  –La × 2 3.2070(7)

Table 2. Refinement Details and Selected Crystallographic Data for La2Au and α-LaAu (Room Temperature, Mo Kα λ = 0.71073 Å).

refined composition La2Au LaAu
CCDC number 2072070 2072071
fw/g mol–1 474.79 335.88
space group Pnma (no. 62) Pnma (no. 62)
Z 4 4
a 7.5064(12) 7.6053(11)
b 5.1531(8) 4.8235(8)
c 9.5036(13) 5.9234(8)
V3 367.61(10) 217.29(6)
ρcalc/g cm–3 8.579 10.267
μMo Kα/mm–1 62.35 86.33
Rint 0.038 0.037
R1 [I > 2σ(I)]a 0.042 0.025
wR2 [I > 2σ(I)]a 0.106 0.059
R1 [all data]a 0.047 0.026
wR2 [all data]a 0.109 0.059
Δρmax,min/e Å–3 3.50, −2.49 1.74, −1.59
a

R1 = ∑||F0| – |Fc||/∑|F0|; wR2 = [∑[w(F02Fc2)2]/∑[w(F02)2]]1/2, where w = 1/[σ2F02 + (AP)2 + (BP)] and P = (F02 + 2Fc2)/3. A and B are the respective weight coefficients (see the CIF data).

Table 3. Atomic Coordinates and Equivalent Isotropic Displacement Parameters (Å2) for La7Au3.

atom site x y z Ueqa
La1 6c 0.53800(5) 1 – x 0.0245(3) 0.0220(2)
La2 6c 0.87362(5) 1 – x 0.3121(3) 0.0214(2)
La3 2b 1/3 2/3 0b 0.0217(3)
Au 6c 0.19023(3) 1 – x 0.2519(3) 0.02214(15)
a

Ueq is defined as one-third of the trace of the orthogonalized Uij tensor.

b

The z coordinate of La3 was fixed to 0 after data standardization.

Table 4. Atomic Coordinates and Equivalent Isotropic Displacement Parameters (Å2) for La3Au2.

atom site x y z Ueqa
La1 4h 0.16362(8) x + 1/2 1/2 0.0214(3)
La2 2a 0 0 0 0.0284(4)
Au 4g 0.62723(5) x – 1/2 0 0.0194(2)
a

Ueq is defined as one-third of the trace of the orthogonalized Uij tensor.

Table 5. Atomic Coordinates and Equivalent Isotropic Displacement Parameters (Å2) for La3Au4.

atom site x y z Ueqa
La 18f 0.04359(5) 0.21220(5) 0.23186(8) 0.02253(18)
Au1 18f 0.39091(3) 0.11467(3) 0.04913(6) 0.02213(15)
Au2 3b 0 0 1/2 0.0370(3)
Au3 3a 0 0 0 0.0426(3)
a

Ueq is defined as one-third of the trace of the orthogonalized Uij tensor.

Table 6. Atomic Coordinates and Equivalent Isotropic Displacement Parameters (Å2) for La2Au.

atom site x y z Ueqa
La1 4c 0.00819(18) 1/4 0.67556(14) 0.0244(4)
La2 4c 0.1515(2) 1/4 0.08642(13) 0.0260(4)
Au 4c 0.24308(13) 1/4 0.40218(9) 0.0278(3)
a

Ueq is defined as one-third of the trace of the orthogonalized Uij tensor.

Table 7. Atomic Coordinates and Equivalent Isotropic Displacement Parameters (Å2) for α-LaAu.

atom site x y z Ueqa
La 4c 0.18451 (11) 1/4 0.64246(14) 0.0174(3)
Au 4c 0.03896 (8) 1/4 0.14532(9) 0.0188(3)
a

Ueq is defined as one-third of the trace of the orthogonalized Uij tensor.

Table 8. Selected Interatomic Distances (Å) in La7Au3.

atoms distance
La1 –Au × 2 3.0761(8)
  –La1 × 2 3.5722(7)
  –La3 3.7513(9)
  –La2 × 2 3.8164(9)
  –La3 3.9166(16)
  –La2 × 2 4.0197(7)
  –La1 × 2 4.0812(15)
  –La3 4.1791(16)
La2 –Au × 2 3.0962(5)
  –Au 3.1213(12)
  –La1 × 2 3.8164(8)
  –La3 3.9863(10)
  –La2 × 2 4.0086(15)
  –La1 × 2 4.0198(7)
  –La2 × 4 4.0225(5)
La3 –Au × 3 3.1008(10)
  –La1 × 3 3.7513(8)
  –La1 × 3 3.9167(16)
  –La2 × 3 3.9862(10)
  –La1 × 3 4.1791(16)
Au –La1 × 2 3.0760(8)
  –La2 × 2 3.0962(4)
  –La3 3.1008(10)
  –La2 3.1213(12)

Table 9. Selected Interatomic Distances (Å) in La3Au2.

atoms distance
La1 –Au × 4 3.1987(8)
  –Au × 2 3.2161(11)
  –La2 × 4 3.7510(8)
  –La1 3.902(2)
  –La1 × 2 4.0618(15)
La2 –Au × 4 3.3208(3)
  –La1 × 8 3.7510(8)
  –La2 × 2 4.0618(15)
Au –Au 3.0339(13)
  –La1 × 4 3.1987(8)
  –La1 × 2 3.2161(11)
  –La2 × 2 3.3208(3)

Table 10. Selected Interatomic Distances (Å) in La3Au4.

atoms distance
La –Au1 3.0059(8)
  –Au3 3.0836(6)
  –Au1 3.1205(9)
  –Au2 3.1955(6)
  –Au1 3.2225(10)
  –Au1 3.2313(10)
  –Au1 3.3140(10)
  –Au1 3.3505(7)
  –Au1 3.4390(8)
  –La 3.6540(12)
  –La × 2 3.9696(10)
  –La × 2 4.1503(9)
  –La × 2 4.3092(11)
Au1 –La 3.0058(8)
  –Au1 3.0407(8)
  –La 3.1205(9)
  –Au1 × 2 3.1836(6)
  –La 3.2226(7)
  –La 3.2312(10)
  –La 3.3140(10)
  –La 3.3504(7)
  –La 3.4390(9)
Au2 –Au3 × 2 3.1124(8)
  –La × 6 3.1955(7)
Au3 –La × 6 3.0835(6)
  –Au2 × 2 3.1124(8)

Table 11. Selected Interatomic Distances (Å) in La2Au.

atoms distance
La1 –Au 3.1399(17)
  –Au × 2 3.2775(10)
  –La2 × 2 3.6321(14)
  –La2 3.656(2)
  –La2 × 2 3.7257(15)
  –La1 × 2 4.0110(11)
  –La2 4.0502(19)
  –La1 × 2 4.218(2)
La2 –Au 3.0678(18)
  –Au 3.0785(16)
  –Au × 2 3.2141(10)
  –La1 × 2 3.6322(14)
  –La1 3.656(2)
  –La1 × 2 3.7257(15)
  –La2 × 2 3.809(2)
  –La1 4.0502(19)
Au –La2 3.0678(18)
  –La2 3.0785(16)
  –La1 3.1399(17)
  –La2 × 2 3.2141(10)
  –La1 × 2 3.2775(10)

First-Principles Calculations

Total energy calculations were performed for the newly discovered phases and some known compounds in the La–Au binary system using the Vienna ab initio Simulation Package (VASP).36 Exchange and correlation were described in the generalized-gradient approximation (GGA) with the Perdew–Burke–Ernzerhof exchange-correlation functional (PBE).37 The plane wave energy cutoff was set to 500 eV. k-point grids with 0.1 Å–1 spacing were used to sample the Brillouin zones. The structures were fully relaxed to residual forces of less than 0.02 eV/Å. All calculations were made at the scalar-relativistic level. We also checked the effect of spin–orbit coupling (SOC) on the thermodynamic properties calculated at 0 K and found that the enthalpies of formation were affected by less than 3% with SOC included. Such small differences have no effect on the conclusions drawn from the calculations made without SOC. For this reason and due to the higher computational cost of calculations with SOC, we conducted a detailed analysis of thermodynamic stability without a consideration of spin–orbit coupling. An evaluation of the phase diagrams at 0 K was performed by employing tools available within the atomic simulation environment.38

Electronic structure calculations were performed for La7Au3, La3Au2, and La3Au4 as well as La2Au and α-LaAu at the scalar relativistic level with the TB-LMTO-ASA code.39 The von Barth–Hedin implementation of the LDA functional was employed.40 For all structures except La3Au2, an introduction of empty spheres was necessary to satisfy the atomic sphere approximation (ASA). Chemical bonding was analyzed with the aid of crystal orbital Hamilton population curves,41 generated by the dedicated module in the LMTO program.

Differential Scanning Calorimetry (DSC)

Differential scanning calorimetry (DSC) was performed with a computer-controlled Netzsch STA 449 F5 Jupiter thermal analyzer. Measurements were carried out at temperatures of up to 1273 K with a heating rate of 10 K/min under a flow of high-purity Ar (grade 5.0, 70 mL/min). The samples were placed in alumina pans covered with lids. Since the studied samples showed indications of side reactions with the crucible material above 1273 K, all measurements were made below this temperature.

Magnetization Measurements

Magnetization was measured for La3Au2 and La3Au4 between 3 and 300 K in static fields from 10 to 60 000 Oe on a Quantum Design Physical Property Measurement System (PPMS) using the vibrating sample magnetometer (VSM) option. The polycrystalline samples were enclosed in polypropylene (PP) sample containers. The data were corrected for the empty holder contribution and ferromagnetic impurities using the Honda–Owen method.42,43

Results and Discussion

Synthesis

New phases La7Au3 and La3Au4 were initially identified in samples prepared during our exploratory investigations in the La–TM–Au systems, where TM is a transition element. The La3Au2 phase was discovered for the first time in a sample targeted at the preparation of pure La7Au3. For La7Au3 and La3Au2, early synthesis attempts at temperatures T = 1073–1273 K, i.e., close to the melting points of the elements, always resulted in the phases predicted by the published La–Au phase diagram.44 However, our total energy ab initio calculations suggested that the enthalpies of decomposition for La7Au3 and La3Au2 at T = 0 K must be very small (vide infra), which motivated us to carry out our reactions at lower temperatures.

For La7Au3, annealing of the stoichiometric elemental mixtures or homogeneous pellets prepared by arc melting did not result in the formation of the target phase, even after heat treatment for 5 months at temperatures of as low as 673 K. This observation is in line with the results of a recent study on the La-rich side of the ternary La–Mg–Au phase diagram at 673 K, where the authors did not observe any unreported binary La–Au compounds close to the La:Au = 7:3 composition.45 However, we found that La7Au3 can be prepared with a reasonably high yield by slow crystallization from a melt with the same nominal composition. The samples produced this way always contained some La2Au and La, which are the phases expected to be in equilibrium at the given composition according to the published phase diagram.44 The presence of the former compound in the samples precluded accurate Rietveld refinements of the powder patterns due to the high malleability of La2Au and associated severe preferred orientation and anisotropic peak broadening (Figure 1). However, the amount of La7Au3 in these samples can be estimated to be around 30 wt % on the basis of the calculated corundum ratios for the phases present in the sample.46 Interestingly, quenching of the stoichiometric melt did not produce La7Au3, indicating that slow crystallization is essential for the formation of this phase. The failure to produce pure samples of La7Au3 is probably related to the metastability of this phase rather than stabilization by undetected foreign elements, such as hydrogen. Our attempt to prepare La7Au3 under hydrogenating conditions, as described in the Experimental Section, led to LaH2 and an unidentified air-sensitive crystalline product, as suggested by PXRD analysis, and no traces of La7Au3 were detected (Figure S1).

Figure 1.

Figure 1

Powder X-ray diffraction pattern (Cu Kα) of a sample containing about 30 wt % La7Au3. Experimental data with subtracted background and theoretical powder patterns for La7Au3, La2Au, and La are shown in gray, blue, red, and green, respectively.

Phase-pure samples of La3Au2 were initially obtained after annealing an as-cast pellet at 873 K for 30 days (Figure 2a). After the thermal stability of this phase had been established (vide infra), we managed to optimize the synthesis by increasing the annealing temperature up to 973 K, which allowed us to reduce the annealing time to 10 days.

Figure 2.

Figure 2

Powder X-ray diffraction patterns (Cu Kα1) and the respective Rietveld refinement for (a) La3Au2 and (b) La3Au4. The experimental data, theoretical pattern, and difference curve are shown in black, red, and blue, respectively. Tick marks correspond to the positions of the Bragg peaks.

In contrast to La7Au3 and La3Au2, La3Au4 can be easily prepared by arc melting of the elements. Prolonged annealing at temperatures of between 1073 and 1273 K improved the crystallinity without resulting in any decomposition (Figure 2b).

None of the studied phases displayed any appreciable homogeneity range, according to powder X-ray diffraction (PXRD).

Crystal Structures

La7Au3

The La-richest phase in the La–Au system, La7Au3, crystallizes in a noncentrosymmetric structure with the Th7Fe3 type (space group P63mc, Pearson code hP20, Figure 3). The La substructure can be viewed as consisting of isolated La4≡(La3)(La1)3 tetrahedra and columns of face-sharing [(La2)6/2] octahedra propagating along [001] (Figure 3a). The shortest La–La contacts in the tetrahedra and octahedra measure 4.081(2) and 4.009(2) Å, respectively. These values significantly exceed the shortest metal–metal contacts in elemental La (dLa–La = 3.74–3.77 Å47). The smallest La–La interatomic separation in the structure with dLa–La = 3.5722(7) Å is observed between the corners of adjacent La4 tetrahedra.

Figure 3.

Figure 3

Crystal structure of La7Au3. (a) Polyhedral representation of the La substructure consisting of isolated La4≡(La3)(La1)3 tetrahedra and face-sharing [(La2)6/2]. (b) Interlinking of the gold-centered [AuLa2/2La4/3] trigonal prisms. A single trimer composed of three edge-shared prisms is emphasized in blue. The unit cell is outlined in black.

The unique Au site in the structure is 6-fold coordinated by La, adopting a trigonal-prismatic environment, with the Au–La distances ranging from 3.0760(8) Å to 3.121(1) Å (Figure 3b). These values are close to the numbers reported in the literature for bonding contacts in other La aurides.4850 The prisms form trimers by sharing edges of the triangular bases. The trimers arrange in turn in hexagonal close packing and link by corners to build a three-dimensional structure. The shortest Au–La distance between the adjacent trimers measures 3.6512(8) Å and significantly exceeds the typical bonding contacts.

Among the gold-containing phases, the Th7Fe3 type is adopted by M7Au3 with M = Sr, Eu, and Yb,5153 i.e., the metals that have a tendency to adopt the +II oxidation state. Rare earth metals (RE) that prefer the +III oxidation state form compounds with the Th7Fe3 structure when combined with transition elements of groups 8–10.5466 In addition, binary compounds Sc7P3 and La7Ge3, containing main-group elements, were reported to crystallize in this type.67,68 From these examples, it is clear that the existence field of the Th7Fe3 structure extends over a wide region of valence electron counts. However, it is not clear at the moment if other RE7Au3 compounds exist and whether any of them are thermodynamically stable.

La3Au2

Binary auride La3Au2 adopts the U3Si2 structure type (space group P4/mbm, Pearson code tP10, Figure 4). There are two symmetrically independent La sites and a unique Au position. The La part of the structure can be visualized as consisting of La-centered [(La2)(La1)8/4] cubes, with dLa2–La1 = 3.7510(8) Å. The cubes connect by sharing faces along the [001] direction, forming columns which interlink by edge sharing. The resulting substructure hosts extended voids propagating along the c direction. These voids accommodate Au2 dumbbells with an Au–Au distance of 3.034(1) Å. Although this distance is longer than the shortest contact in elemental Au (dAu–Au = 2.88 Å69), it is in good agreement with the values reported for other structures with polyanionic Au species.70,71 The Au atoms are 6-fold coordinated by La1 (dAu–La1 = 3.1987(8)–3.216(1) Å), building trigonal prisms, similar to the Au coordination polyhedra in La7Au3. The prisms share faces, giving rise to extended double columns running along the c direction, which interlink by edge sharing. The La2 atoms cap the faces of the [Au(La1)6/6] prisms, completing the 8-fold coordination of Au, with dAu–La2 = 3.3208(3) Å. The observed La–Au distances in the La3Au2 structure are considerably longer than those in La7Au3, but fall in the range of bonding contacts determined for other compounds.50

Figure 4.

Figure 4

Crystal structure of La3Au2. Columns of face-sharing La-centered [(La2)(La1)8/4] cubes and double columns of face-sharing Au-centered [Au(La1)6/6] trigonal prisms are depicted in green and red, respectively. The coordination of one Au atom by La2 is shown in violet. The unit cell is outlined in black.

The breakdown of the La3Au2 structure into cubic and trigonal-prismatic building blocks allows its description as an intergrowth of W- and AlB2-type fragments, as was previously noted for other representatives of this prolific structural family, c.f. Figure 4.72

Whereas several Au-containing ternary derivatives of the U3Si2 type are known, such as Gd2Au2Sn,73 and Ca2Au2Pb,74 the only binary auride reported to crystallize in this type is Y3Au2.75 The latter compound was prepared by annealing the elements at a rather high temperature of 1323 K. A possible explanation for the lack of experimental data for other RE3Au2 compositions may be their apparently low thermal stability. It is worth noting that an unidentified phase tentatively assigned to the U3Si2 type was observed upon recent re-evaluation of the La–Mg–Au phase system.45 Judging from the estimated lattice parameters (a ≈ 8.3 Å, c ≈ 4.0 Å), the reported compound may actually be the binary La3Au2 phase presented here.

La3Au4

In contrast to the previously described phases, La3Au4 is a new phase identified in the gold-rich field of the phase diagram. It crystallizes in the Pu3Pd4 type (space group R3̅, Pearson code hR14, Figure 5). The three crystallographically unique Au sites are distributed between two kinds of polyanionic substructures: Au1 atoms make up a three-dimensional framework hosting large channels running along the c direction (hexagonal setting). The Au1–Au1 distances range from 3.0407(8) to 3.1836(6) Å. The channels in turn accommodate linear Au2–Au3– chains with dAu2–Au3 = 3.1124(8) Å. Both Au2 and Au3 sites are octahedrally coordinated by La, and the resulting octahedra share faces, forming infinite columns Inline graphic (Figure 5a). Short La–La contacts of 3.654(1) Å are observed between the neighboring columns. Interestingly, the equivalent isotropic displacement parameters for Au2 and Au3 were found to be about 1.7–1.9 times larger than those for Au1 and La. In particular, for Au3, this is reflected in an elongation of the thermal ellipsoid along the c direction (Figure 5b). Similar behavior for the corresponding Au sites was reported in isostructural compounds M3Au4 (M = Ca, Y, Nd).7678 This effect may be related to possible destabilization of the one-dimensional Au chains due to a Peierls distortion. To check for potential pairwise chain breaking, structure refinement was tried in polar space group R3. Although it did result in an alternation of the Au–Au distances along the chains with respective values of 3.06(1) Å and 3.16(1) Å, the displacement parameters of Au remained virtually unaffected. Partial breaking of the chains with statistically disordered oligomers or undetected modulation may explain the observed deviations of the displacement parameters. Refinement of the Au sites as split did not yield better results in either R3̅ or R3, and no obverse–reverse twinning was identified. We note that the analysis of the reciprocal space did not indicate any pronounced diffuse scattering or presence of extra reflections (Figure S2).

Figure 5.

Figure 5

Crystal structure of La3Au4. (a) Columns of face-sharing [(Au2,3)La6/2] octahedra embedded in the three-dimensional Au1 framework. The unit cell (hexagonal setting) is outlined in black. (b) Close-up view of a single column with thermal ellipsoids drawn at the 90% probability level. (c) Corner-sharing Au-centered [(Au2)(Au3)2/2(Au1)6] distorted cubes and La atoms. (d) Representation as a superstructure of the W type. La- and Au-centered distorted cubes are shown in green and orange, respectively.

Furthermore, single-crystal X-ray diffraction studies at 100 K did not indicate any pronounced distortion either (Tables S1–S3), although the elongation of the thermal ellipsoids was still observed. Therefore, we retained the original structural model in the disorder-free Pu3Pd4 type.

Although there is no direct Au–Au bonding between the Au1 framework and the (Au2, Au3) linear chains, for a better visualization of the crystal structure, it is convenient to consider the Au2-centered (Au2)(Au3)2(Au1)6 cluster as a building block. These clusters display a strongly distorted cubic shape due to the long Au2–Au1 distance of 3.7855(4) Å. The “cubes” interconnect by corner sharing, resulting in chains propagating along the c direction (Figure 5c). The La atoms occupy the distorted cubic voids between the chains. In this representation, the structure of La3Au4 can be regarded as consisting of fused AuLa8 and LaAu8 distorted cubes (Figure 5d), prompting its description as a complex superstructure of the W type. A detailed description of the structural relationship between the Pu3Pd4 and W types within the Bärnighausen tree formalism79 is given in Figure S3.

Numerous compounds containing group 10 elements were reported to crystallize in the Pu3Pd4 structure type.8085 Among the aurides, structurally well-characterized representatives of this family are limited to M3Au4 with M = Ca, Y, and Nd.7678,86 In addition, compositions with M = Ce, Pr, Gd, Sm, Tb, and Th were assigned to this structure based on the respective powder X-ray diffraction patterns without further refinements.78,8791 The M3Au4 phases with rare earth metals Pr, Nd, Gd, and Tb were found to decompose peritectically at 1523–1613 K.86,8890 In light of our experimental data, it is conceivable that La3Au4 has a similar decomposition point.

La2Au and α-LaAu

The structures of La2Au and α-LaAu were previously assigned to the Co2Si (space group Pnma, Pearson code oP12) and FeB (space group Pnma, Pearson code oP8) types, respectively, based on powder X-ray diffraction patterns.92 In this section, we provide accurate crystal structure determination for the two compounds from single-crystal X-ray diffraction data.

The La-richer phase, La2Au, can be described as crystallizing in the anti-PbCl2 structure type (space group Pnma, Pearson code oP12, Figure 6), which is isopointal to Co2Si but displays somewhat different coordination environments due to distinct geometric parameters. McMasters et al. discussed the differentiation between the two structure types in terms of chemical bonding types and argued that the intermetallic Co2Si compound bears more similarity to RE2Au when electronic interactions are concerned.92 In contrast, Chai and Corbett assigned the isostructural Y2Au to the anti-PbCl2 type referring to the similarity in the local atomic coordination.75 We prefer to adhere to the latter criterion since the equilibrium geometry of the atomic arrangement, unlike chemical bonding, is an easily measurable quantity. The structures of La2Au can be conveniently represented as based on Au-centered AuLa6 trigonal prisms which link by sharing the trigonal faces along the b direction and by edge sharing along the a direction, building up corrugated layers stacked along the c axis (Figure 6a). The Au–La distances in the prisms span from 3.068(2) to 3.842(1) Å. The latter value clearly exceeds the typical Au–La bonding distances and demonstrates only weak bonding character according to our calculations (vide infra). Disregarding these long Au–La contacts, the Au site is 7-fold coordinated by La, with three of the La atoms coming from the adjacent trigonal prisms (Figure 6b).

Figure 6.

Figure 6

Crystal structure of La2Au. (a) Layers of interlinked Au-centered [Au(La2)2/2(La1)4/4] trigonal prisms. The unit cell is outlined in black. (b) Local coordination environment of the Au site. The distances are given in angstroms. The Au–La contacts that exceed the typical bonding distances are dashed.

The assignment of the α-LaAu structure to the FeB type (space group Pnma, Pearson code oP8, Figure 7) is confirmed in our study. Similarly to La2Au, the structure can be broken down into Au-centered AuLa6 trigonal prisms with dAu–La = 3.178(1)–3.189(1) Å. The prisms connect via common rectangular faces giving rise to columns propagating along the b axis. The columns interlink by edge and corner sharing to form a three-dimensional framework (Figure 7a). The 7-fold coordination of Au by La is completed by including a La atom from a neighboring prism at a distance of 3.146(1) Å (Figure 7b). In contrast to La2Au, where no direct Au–Au interactions are observed, there are infinite zigzag Au chains with dAu–Au = 3.0218(7) Å in α-LaAu, running inside the columns along [010].

Figure 7.

Figure 7

Crystal structure of α-LaAu. (a) Three-dimensional framework emerging from columns of face-sharing Au-centered [AuLa6/6] trigonal prisms. The unit cell is outlined in black. (b) Local coordination environment of the Au site. The distances are given in angstroms.

Magnetic Properties

Magnetization measurements were performed for La3Au2 and La3Au4. The temperature dependence of the magnetic susceptibility corrected for the sample holder contribution and ferromagnetic impurities is shown in Figure 8. Because of the absence of localized magnetic moments, the magnetic response of La3Au2 and La3Au4 is weak. At low temperatures, the magnetic data are affected by paramagnetic impurities, while at high temperatures a linear increase in the magnetic susceptibility with temperature is observed. The latter effect, which is especially pronounced for La3Au2, is likely associated with the presence of peaks in the electronic density of states around the Fermi level (vide infra). To take the paramagnetic impurity and the linear behavior into account, the magnetic susceptibility was fitted with the modified Curie expression, χ(T) = χ0 + CT–1 + aT, which yielded the temperature-independent contribution χ0 of about 3.5 × 10–4 emu mol–1 for both compounds, indicating the prevalence of the Pauli paramagnetism over the diamagnetic components. Measurements under fields of as low as 10 Oe did not indicate any superconductivity down to 3 K.

Figure 8.

Figure 8

Temperature dependence of the corrected magnetic susceptibility for (a) La3Au2 and (b) La3Au4. Open circles and red lines denote the experimental data and nonlinear fits, respectively.

Thermodynamic Stability from First Principles

Total energy calculations performed with VASP for the titular phases, selected La–Au binary compounds, and elemental La and Au were used to evaluate formation energies at 0 K and construct an energy convex hull (Figure 9). From this analysis, among the La-rich phases with a La:Au ratio of up to 1:1, LaAu appears to have the highest negative enthalpy of formation per atom, which is also in line with its reportedly high thermal stability. We note here that the two modifications of LaAu, α-LaAu (FeB type) and β-LaAu (CrB type), were found to be almost degenerate in energy. Interestingly, La-richer compositions are located close to the line connecting La and LaAu, which suggests that their formation enthalpies from La and LaAu have very small absolute values. Thus, La7Au3 is located on the convex hull and is therefore predicted to be thermodynamically stable. However, its decomposition enthalpy into La and LaAu measures only 26.6 meV/atom. Various studies on the reaction enthalpies calculated with DFT methods indicate that the errors in such calculations lie between about 20 and 100 meV/atom for different classes of materials.93,94 With this in mind, it can be concluded that the stability of La7Au3 at 0 K cannot be unambiguously confirmed with DFT methods.

Figure 9.

Figure 9

Calculated convex hull for selected binary La–Au phases. Structures located on the hull and above are highlighted in green and red, respectively.

The other two La-rich phases, La2Au and La3Au2, appear to be located above the hull. In this case again, the absolute value of the decomposition enthalpy into La and LaAu is found to be below the expected error of the calculation: 12.1 meV/atom for La2Au and 19.8 meV/atom for La3Au2. The Au-richer composition La3Au4, which is predicted to be stable, also displays a moderate decomposition enthalpy into LaAu and LaAu2 of 17.7 meV/atom. The main conclusion of these computational results is that many binary phases in the La–Au system, including those experimentally confirmed to be thermodynamically stable (such as La2Au), exhibit very small decomposition enthalpies, which may result in narrow regions of thermal stability or even metastability at finite temperatures. Since the entropy factor is not taken into account in such calculations, in general, an analysis of thermodynamic stability at 0 K should always be taken with care, especially when the enthalpy differences are small.

We conclude our discussion of the DFT-derived thermodynamics with a note on the possible stabilization of the La7Au3 structure with a foreign element. Since the mentioned compound could not be prepared single-phase, a natural question to ask is whether the presence of some undetected third element is responsible for the stabilization of this phase. Our SCXRD analysis allows ruling out elements of the second period (such as carbon, nitrogen, and oxygen) and heavier elements (such as Mo from the reactor) as possible constituents of the crystal structure, since any significant amounts of these elements would be detectable. On the basis of the analysis of the X-ray diffraction data, we cannot exclude the presence of some hydrogen, which was found to be responsible for the stabilization of many seemingly binary phases in the past.28 However, our attempt to prepare La7Au3 under hydrogenating conditions resulted in the formation of LaH2 and did not produce the target phase (vide supra). It is not clear if the employed reaction conditions were too harsh, e.g., if the hydrogen pressure was too high. For this reason, we also investigated the stability of the La7Au3 structure upon incorporation of hydrogen from first principles.

As discussed above, the crystal structure of La7Au3 features some tetrahedral and octahedral voids surrounded by La atoms. These voids could potentially accommodate H atoms. To check this hypothesis using first-principle calculations, we considered three model structures: La7Au3H(tetr), with H atoms placed exclusively in the tetrahedral voids; La7Au3H(oct), with H atoms in the octahedral voids only; and La7Au3H2, with H atoms occupying both kinds of voids. The structures were fully relaxed, and their stability was checked with respect to other phases in the La–Au–H system. We found that in all cases the introduction of H into the structure has a destabilizing effect and the formation of the binary hydride LaH2 is favorable:

graphic file with name ic1c01355_m002.jpg
graphic file with name ic1c01355_m003.jpg
graphic file with name ic1c01355_m004.jpg

Two points need to be mentioned here. First, the nature of the Au-containing product in our reaction under hydrogen is not yet known, so it cannot be considered for the calculations. Second, the given absolute values of the decomposition enthalpies are not particularly high and may be regarded as lying on the upper side of the expected calculation error. Nevertheless, the observed trend suggests that placing hydrogen in the tetrahedral or octahedral voids in the structure of La7Au3 will not have a stabilizing effect. Of course, other factors such as the potential location of hydrogen in other parts of the structure or entropy stabilization of a hydride should also be considered. In conclusion, although the presence of hydrogen in the experimentally observed La7Au3 cannot be completely ruled out, our experimental data and first-principles calculations do not support this scenario.

Thermal Analysis

Results of the differential scanning calorimetry (DSC) analysis for a sample containing about 30 wt % La7Au3 are shown in Figure 10a. Upon heating, the sample undergoes incongruent melting at about 833 K, corresponding to the eutectic point between elemental La and La2Au.44 No other effects are seen below this temperature, indicating that the decomposition of La7Au3 must be too slow to occur within the time frame of the measurement. Upon cooling, the sample crystallizes with virtually no supercooling effect. No other transitions are visible below the solidification point. PXRD analysis of the sample after the DSC measurement revealed the presence of La, La2Au, and small amounts of La7Au3 (Figure S4). From the described behavior, it can be inferred that La7Au3 is a metastable phase, which forms upon crystallization from the melt in line with Ostwald’s rule and decomposes upon melting or prolonged heating at a temperature sufficient for solid-state diffusion to occur.

Figure 10.

Figure 10

Differential scanning calorimetry on heating (red) and cooling (blue) for La7Au3 (a, about 30 wt % La7Au3 in the sample), La3Au2 (b), and La3Au4 (c). Thermal events with the corresponding temperatures and explanations are indicated. See the text for details.

DSC measurements on a La3Au2 sample (Figure 10b) revealed an endothermic peak upon heating to 1013 K. No other intrinsic transitions are observed below this temperature; a small bump in the heating curve at about 963 K corresponds to the polymorphic transition (α → β) of a tiny amount of LaAu impurity in the sample. Ex situ analysis of a La3Au2 sample annealed above 1013 K suggests that a peritectic decomposition into LaAu and a La-rich melt occurs at this temperature. From the DSC analysis, the enthalpy of melting for La3Au2 was estimated to be 16.8 kJ/mol (or 34.8 meV/atom, i.e, within the error range for reaction enthalpy estimation using DFT methods). Upon cooling, the DSC curve reveals three exothermic effects: the crystallization of La3Au2 (T = 1013 K), the polymorphic β → α transition of LaAu (T = 963 K), and the crystallization of La2Au from the melt (T = 953 K).

Finally, our DSC analysis of a La3Au4 sample at temperatures of up to 1273 K did not reveal any thermal effects (Figure 10c), suggesting that the decomposition or melting occurs at higher temperatures.

With the collected data at hand, we are able to propose a refined version of the La–Au binary phase diagram in the La-rich region (Figure 11). While the phase relationships involving La3Au4 remain unclear, important updates to the published phase diagram include the incongruently melting La3Au2 and the metastable La7Au3.

Figure 11.

Figure 11

Part of the re-evaluated La–Au phase diagram. Polymorphic phase transitions in elemental La are omitted for clarity. The metastable La7Au3 is depicted with a dashed line. Selected temperatures (K) are indicated.

Electronic Structure and Chemical Bonding

A first attempt to rationalize the electronic structure and bonding of La7Au3, La3Au2, La3Au4, La2Au, and α-LaAu by applying the Zintl–Klemm formalism (which holds true for many polar intermetallics) allows rewriting the compounds’ formulas as (La3+)7(Au)3(e)18, (La3+)3(Au)2(e)7, (La3+)3(Au)4(e)5, (La3+)2(Au)(e)5, and (La3+)(Au)(e)2, respectively, if occupation of the Au(6p) states is not taken into account for the calculation of the formal charge. Thus, they would be expected to be electron-rich, polar intermetallics. In line with this simplified evaluation, the electronic densities of states (DOS) for La7Au3, La3Au2, La3Au4, La2Au, and α-LaAu (Figure 12a–c and Figure S5a,b) reveal metallic character and sizable charge transfer. At the Fermi level (EF), the DOS are dominated by the La(5d) states with a small contribution of Au(6p) and Au(5d). Unoccupied La(4f) states form a peak in the DOS centered at about EEF = 2 to 3 eV. The Au(6s) and Au(5d) components are mostly localized well below EF, confirming the anionic nature of Au. With the emergence of Au–Au bonding, the dispersion of the Au(6s) and Au(5d) states gradually increases. Thus, in La7Au3 (Figure 12a) and La2Au (Figure S5a), both lacking direct Au–Au interactions, a domain with Au(6s, 5d) character is situated below EEF = −4 eV and is separated from the bands crossing the Fermi level by an energy gap. In La3Au2 (Figure 12b) and α-LaAu (Figure S5b), with isolated Au dumbbells and zigzag Au chains, respectively, the Au(6s) and Au(5d) states broaden and the gap between these states and the higher-lying bands is reduced. Finally, in La3Au4 (Figure 12c), with an extended three-dimensional framework of Au–Au bonds, the Au(6s) and Au(5d) regions become continuous in a wide energy window, with a dip in the DOS at around EEF = −2 eV. Within the framework of the rigid band approximation, the location of the gap or the dip in the electronic spectra of La7Au3, La3Au2, La3Au4, La2Au, and α-LaAu corresponds to the removal of 18, 7, 5, 5, and 2 electrons per formula unit, respectively. These numbers are in perfect agreement with the electron excess calculated above. This shows that the electronic structure of the studied materials can be fairly well explained using, as the first approximation, simple electron counting suitable for compounds with highly localized bonding and augmenting this picture with electronic delocalization, an approach that appears to be applicable for a great number of polar intermetallic phases.95

Figure 12.

Figure 12

Total and projected electronic densities of states (DOS) and bond-averaged crystal orbital Hamilton population curves (COHP) for (a) La7Au3, (b) La3Au2, and (c) La3Au4. Dashed lines denote integrated COHP curves.

Crystal orbital Hamilton population analysis (COHP) revealed that for all studied compounds, the La–Au contacts show exclusively bonding character below EF, with some extra bonding states available just above the Fermi level, resulting in slightly underoptimized interactions (Figure 12a–c). The long La–Au contacts in the range of 3.65–3.84 Å, observed in La7Au3 and La2Au, were also examined, but were found to exhibit considerably smaller bonding contributions in comparison with the shorter La–Au pairs.

The Au–Au bonding, observed for La3Au2, La3Au4, and α-LaAu, displays a more complex electronic pattern hallmarked by a combination of bonding and antibonding states below EF. Nevertheless, the magnitude of the bond-averaged negative integrated COHP values (−ICOHP) for the Au–Au contacts at the Fermi level is comparable to that of the La–Au bonds. Interestingly, for La3Au4, all Au–Au contacts, except Au2–Au3 along the Au chains, demonstrate bonding states in the vicinity of EF. In contrast, in the case of Au2–Au3, the Fermi level crosses an extended region of antibonding character, spanning from about EEF = −2.4 to 1.1 eV (Figure S6). Although, the integration over all states below EF indicates a net attractive interaction for Au2–Au3, with an −ICOHP value close to those of other Au–Au contacts, the location of EF in the antibonding domain suggests that the Au–Au chains in La3Au4 are too electron-rich and may be prone to destabilization, such as Peierls distortion, discussed above in relation to the increased atomic displacement parameters of the Au atoms in the chains. To further study the possibility of such a distortion, we attempted geometry optimizations for La3Au4 with the VASP code starting from the ideal structure with equidistant Au chains and from a hypothetical structure with a pairwise distortion of the chains. Both optimization runs converged to essentially the same structure with identical Au–Au distances along the chain. The introduction of spin–orbit coupling did not affect this result. This observation suggests that structural distortion, if any, happens on scales larger than the size of a single unit cell. In order to spot such a distortion experimentally, crystallographic studies at helium temperatures may be necessary.

Since some of the presented structures exhibit relatively short La–La contacts, this kind of homoatomic interaction was also analyzed. Only La–La pairs with interatomic distances of less than 3.90 Å were considered. In all studied compounds, such contacts are characterized exclusively by bonding states below EF. However, due to a transfer of electron density from the La atoms to the Au species, the resulting La–La bonding interactions turn out to be too electron-deficient and consequently much weaker than the La–Au bonding, yet non-negligible. In particular, for La3Au2, the −ICOHP magnitude for the short La–La contact with dLa–La = 3.75 Å amounts to about 50% of the bond-averaged La–Au value. This bonding picture is reminiscent of that in the lanthanum subiodide LaI, which also exhibits unsaturated, but still quite pronounced, La–La bonding.96

Conclusions

In this contribution, we described three new binary phases in the La–Au system—La7Au3, La3Au2, and La3Au4—crystallizing in known structure types, which are nevertheless rather uncommon for binary gold-containing intermetallic compounds. In addition, we determined the crystal structures of known binaries La2Au and α-LaAu. An examination of the crystal and electronic structures of the listed materials suggests that the increase in the Au content is accompanied by the emergence of structural units with homoatomic Au–Au bonding, such as Au2 dimers in La3Au2, Au chains in LaAu, and extended Au frameworks in La3Au4.

Our exploratory studies, first principles calculations, and thermal analysis indicate that the La-richest phase La7Au3 is metastable and can be prepared by crystallization from a stoichiometric melt, in accordance with Ostwald’s rule. In contrast, La3Au2 and La3Au4 appear to be thermodynamically stable. The former phase decomposes peritectically at 1013 K, while the latter is stable at least up to 1273 K. Our investigations enabled a re-evaluation of the available La–Au phase diagram in the La-rich part. Taking into account the relative scarcity of detailed thermodynamic studies devoted to gold-containing intermetallics, it is not surprising that even binary systems may offer a source of new compounds with potentially interesting crystal-structural characteristics and physical properties. In this respect, the observed propensity of Au in the formation of homoatomic bonds makes it interesting to explore Au-rich phase spaces as well.

Acknowledgments

Funding from the Royal Swedish Academy of Sciences through the Göran Gustafsson Prize in Chemistry as well as Energimyndigheten through grant no. 46595 is acknowledged.

Supporting Information Available

The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acs.inorgchem.1c01355.

  • Crystal structure data for La3Au4 at T = 100 K, reciprocal space reconstruction for La3Au4, additional PXRD data, group–subgroup relationships for Pu3Pd4 and bcc structures, and supplementary electronic structure and chemical bonding analysis (PDF)

Accession Codes

CCDC 2072067–2072071 contain the supplementary crystallographic data for this paper. These data can be obtained free of charge via www.ccdc.cam.ac.uk/data_request/cif, or by emailing data_request@ccdc.cam.ac.uk, or by contacting The Cambridge Crystallographic Data Centre, 12 Union Road, Cambridge CB2 1EZ, UK; fax: +44 1223 336033.

The authors declare no competing financial interest.

Supplementary Material

ic1c01355_si_001.pdf (764.9KB, pdf)

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