Min
Zhu
,
Xu-Tang
Tao
and
Sheng-Qing
Xia
*
State Key Laboratory of Crystal Materials, Institute of Crystal Materials, Shandong University, Jinan, Shandong 250100, People's Republic of China. E-mail: shqxia@sdu.edu.cn; Fax: +(531) 883-62519; Tel: +(531) 883-62519
First published on 2nd August 2016
A series of new magnesium copper pnictide intermetallics, A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As) and Eu5Mg2.39Cu16.61As12, were synthesized through high temperature flux reactions. By the single-crystal X-ray diffraction technique, their structures were accurately determined. Sr2Mg3Cu9P7, Eu2Mg3Cu9P7, Sr2Mg3Cu9As7 and Eu2Mg3Cu9As7 crystallize in the Zr2Fe12P7 structure type (S.G. P
, no. 174) with cell parameters: a = 9.7736(19)/9.7417(7)/10.0550(10) Å/10.0410(8) Å, c = 3.9280(16)/3.9008(5)/4.0544(9)/4.0364(6) Å, respectively, while Eu5Mg2.39Cu16.61As12 adopts the Zr5Co19P12 structure type (S.G. P
2m, no. 189) with cell parameters of a = 13.2521(6) Å and c = 4.0910(3) Å. These compounds can be viewed as an extensive branch of the ternary RE−M−Pn system (RE = rare-earth elements; M = transition metals; Pn = pnictogen) with the metal-to-nonmetal ratio being close or equal to 2
:
1. Interestingly, with the divalent alkaline-earth cations being introduced, these metal-rich phases exhibit electron deficiency according to the DFT calculations. Eu2Mg3Cu9As7 is metallic based on the resistivity measurement, consistent with theoretical prediction, and the magnetic susceptibility data of Eu2Mg3Cu9As7 confirmed the divalent oxidation state and weak ferromagnetic coupling for the europium cations.
The Re–M–Pn ternary phases (RE = rare-earth elements; M = transition metals; Pn = pnictides) belong to a huge intermetallic system, with which interesting physical properties such as catalysis and magnetic properties were frequently investigated.17,18 Among these compounds, the metal-rich analogues, whose metal-to-nonmetal ratio is close or equal to 2
:
1, represent a large family bearing various derivative structures related to the binary phosphide M2P. As a typical extensive branch, Zr2Fe12P7-type compounds were also frequently probed recently for their possible ordered structures when the Fe sites are occupied by two different transition metals.19 Although there have been many ternary members of such a structure, to date there are only a few examples of the quaternary pnictide phases, i.e., RE2M3M′9Pn7 (RE = Gd, Er; M = Cr, W; M′ = Fe, Co; Pn = P, As).20 It was not until recently that the ordered rare-earth variants RE2Mn3Cu9Pn7 (Pn = P, As) have been reported21 and no such alkaline-earth examples have been discovered to date.
In this work, we successfully obtained four structure-ordered quaternary pnictide compounds, A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As). The substitution of the trivalent rare-earth elements by divalent cations results in electron deficiency in the compound, according to the electronic band structure calculations. With the above success, we continued to extend the synthesis and interestingly, discovered a new compound Eu5Mg2.39Cu16.61As12, derived from the parent structure Ln5Cu19P12 (Ln = La, Ce) which typically forms with trivalent rare-earth cations.22 These new quaternary phases are very interesting since they probably imply new applications such as thermoelectrics for their tunable structures. Moreover, the replacement of the rare-earth cations by alkaline-earth cations will also provide easy cases for the studies of electronic band structures of these phases, as it is obvious that the handling of rare-earth cations in theoretical calculations is much more complicated. Magnetic and electrical conducting properties of Eu2Mg3Cu9As7 are reported as well.
Pb-flux reactions were utilized to synthesize the title compounds. Initially, Eu2Mg3Cu9As7 was obtained from the reaction mixture with the atomic ratio Eu
:
Mg
:
Cu
:
As
:
Pb = 0.4
:
0.6
:
1
:
1
:
15, which was loaded in an alumina crucible and then subsequently sealed in a silica tube by using a flame under vacuum. The reaction mixture was first heated to 1173 K at a rate of 200 K h−1 and then kept at this temperature for 24 h; after this homogenization process, the furnace was slowly cooled down to 773 K at a rate of 5 K h−1 and at this temperature the excess molten lead was decanted quickly by centrifugation. After the structures and compositions of these compounds were accurately determined by single-crystal X-ray diffraction, they were all reproduced with the stoichiometric ratio of A2Mg3Cu9Pn7. However, an optimization of the reaction procedure with a slightly different ratio of Eu
:
Mg
:
Cu
:
As
:
Pb = 0.2
:
0.3
:
0.8
:
0.7
:
10 also resulted in the discovery of a new phase Eu5Mg2.39Cu16.61As12. Attempts to synthesize other analogues with such a structure type failed. The products of these compounds are typically black needle-shaped crystals. Although various synthetic procedures have been tried, large crystals suitable for property measurements can only be obtained from the compound Eu2Mg3Cu9As7.
For compound Eu2Mg3Cu9As7, a non-centrosymmetric space group P
(no. 174) was suggested by the program and the structure was solved by direct methods. These results are also consistent with the previous structure solution on the rare-earth cation analogues. For compound Eu5Mg2.39Cu16.61As12, a chiral space group P3 was first suggested, and the structure refinements with anisotropic thermal parameters were converged quickly to a small R value with a reasonable Flack parameter as well. However, later checking by using the PLATON program with the WinGx system, ver. 1.15
25 indicates higher symmetry in a new space group P
2m, which turns the structure exactly into the Ln5Cu19P12 type, but with the Cu4 site statistically occupied by 0.203(8) Cu and 0.797(8) Mg. Note that the structure solution based on the lower symmetric space group P3 also leads to a similar disorder in the structure. The site occupancies of all atoms except for the mixed Mg/Cu were checked with the freed occupancies, which are very close to 100%.
Important information on the data collection and structure refinement of A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As) and Eu5Mg2.39Cu16.61As12 is summarized in Table 1. Standardized atomic coordinates and isotropic atomic displacement parameters of Eu2Mg3Cu9As7 and Eu5Mg2.39Cu16.61As12 are collected in Table 2. The atomic coordinates and isotropic displacement parameters of Sr2Mg3Cu9P7, Sr2Mg3Cu9As7 and Eu2Mg3Cu9P7 are provided in the ESI.† Further information in the form of CIF has been deposited with Fachinformationszentrum Karlsruhe, 76344 Eggenstein-Leopoldshafen, Germany, (fax: (49) 7247-808-666; e-mail: crysdata@fiz-karlsruhe.de) – depository CSD-number 431458-431462 for Eu2Mg3Cu9As7, Eu2Mg3Cu9P7, Sr2Mg3Cu9As7, Sr2Mg3Cu9P7, and Eu5Mg2.39Cu16.61As7, respectively. Important bonding distances are tabulated in Tables 3 and 4.
| a R 1 = ∑||Fo| − |Fc||/∑|Fo|; wR2 = [∑[w(Fo2 − Fc2)2]/∑[w(Fo2)2]]1/2, and w = 1/[σ2Fo2 + (A·P)2 + B·P], P = (Fo2 + 2Fc2)/3; A and B are weight coefficients. | |||||
|---|---|---|---|---|---|
| Formula | Sr2Mg3Cu9P7 | Sr2Mg3Cu9As7 | Eu2Mg3Cu9P7 | Eu2Mg3Cu9As7 | Eu5Mg2.39Cu16.61As12 |
| fw/g mol–1 | 1036.82 | 1344.47 | 1165.50 | 1473.15 | 2772.34 |
| T/K | 296(2) | ||||
| Radiation | Mo-Kα, 0.71073 Å | ||||
| Space group |
P (no. 174) |
P (no. 174) |
P (no. 174) |
P (no. 174) |
P 2m (no. 189) |
| Cell dimensions | |||||
| a/Å | 9.7736(19) | 10.0550(10) | 9.7417(7) | 10.0410(8) | 13.2521(6) |
| c/Å | 3.9280(16) | 4.0544(9) | 3.9008(5) | 4.0364(6) | 4.0910(3) |
| V/Å3 | 324.95(16) | 354.99(9) | 320.59(5) | 352.43(7) | 622.20(6) |
| ρ calc./g cm−3 | 5.298 | 6.289 | 6.037 | 6.941 | 7.399 |
| μ Mo Kα/ cm−1 | 1.750 | 2.262 | 1.980 | 4.021 | 4.556 |
| Final R indicesa [I > 2σ(I)] | R 1 = 0.0410 | R 1 = 0.0234 | R 1 = 0.0218 | R 1 = 0.0258 | R 1 = 0.0183 |
| wR2 = 0.0704 | wR2 = 0.0413 | wR2 = 0.0439 | wR2 = 0.0495 | wR2 = 0.0416 | |
| Final R indicesa [all data] | R 1 = 0.0590 | R 1 = 0.0283 | R 1 = 0.0246 | R 1 = 0.0306 | R 1 = 0.0190 |
| wR2 = 0.0774 | wR2 = 0.0425 | wR2 = 0.0461 | wR2 = 0.0512 | wR2 = 0.0418 | |
| Atoms | Wyckoff | x | y | z | U eq.a (Å2) |
|---|---|---|---|---|---|
| a U eq. is defined as one-third of the trace of the orthogonalized Uijtensor. | |||||
| Eu2Mg3Cu9As7 | |||||
| Eu1 | 1f | 2/3 | 1/3 | 0.5 | 0.0109(3) |
| Eu2 | 1c | 1/3 | 2/3 | 0 | 0.0087(3) |
| Mg | 3k | 0.2251(6) | 0.1097(6) | 0.5 | 0.0125(12) |
| Cu1 | 3k | 0.3793(2) | 0.4310(2) | 0.5 | 0.0136(4) |
| Cu2 | 3j | 0.1597(2) | 0.2860(2) | 0 | 0.0125(4) |
| Cu3 | 3j | 0.4225(3) | 0.0556(3) | 0 | 0.0151(5) |
| As1 | 3k | 0.1165(2) | 0.41123(19) | 0.5 | 0.0086(3) |
| As2 | 3j | 0.4196(2) | 0.30701(19) | 0 | 0.0078(3) |
| As3 | 1a | 0 | 0 | 0 | 0.0081(5) |
| Eu5Mg2.39Cu16.61As12 | |||||
| Eu1 | 3g | 0.80974(4) | 0 | 0.5 | 0.00848(15) |
| Eu2 | 2c | 1/3 | 2/3 | 0 | 0.00906(18) |
| Cu1 | 6k | 0.36067(11) | 0.48053(11) | 0.5 | 0.0142(3) |
| Cu2 | 6j | 0.18242(10) | 0.37656(11) | 0 | 0.0138(2) |
| Cu3 | 3g | 0.27944(12) | 0 | 0.5 | 0.0129(3) |
| Cu4/Mg4 | 3f | 0.4300(2) | 0 | 0 | 0.0086(9) |
| Cu5 | 1a | 0 | 0 | 0 | 0.0102(6) |
| As1 | 6k | 0.17035(8) | 0.48024(8) | 0.5 | 0.0084(2) |
| As2 | 3f | 0.17749(11) | 0 | 0 | 0.0082(3) |
| As3 | 3f | 0.63341(10) | 0 | 0 | 0.0090(3) |
| Atom pairs | Distances (Å) | ||||
|---|---|---|---|---|---|
| Sr2Mg3Cu9P7 | Sr2Mg3Cu9As7 | Eu2Mg3Cu9P7 | Eu2Mg3Cu9As7 | ||
| A1– | Pn2 × 6 | 3.062(4) | 3.136(1) | 3.010(3) | 3.105(1) |
| A2– | Pn1 × 6 | 3.069(4) | 3.158(1) | 3.032(3) | 3.132(1) |
| Mg1– | Pn1 | 2.583(8) | 2.681(4) | 2.577(6) | 2.690(5) |
| Pn2 × 2 | 2.733(6) | 2.827(3) | 2.728(4) | 2.818(4) | |
| Pn3 × 2 | 2.738(4) | 2.816(3) | 2.724(3) | 2.812(4) | |
| Cu1– | Pn1 | 2.419(6) | 2.504(2) | 2.404(4) | 2.493(3) |
| Pn1 | 2.506(6) | 2.554(2) | 2.494(4) | 2.545(2) | |
| Pn2 × 2 | 2.416(4) | 2.503(1) | 2.428(3) | 2.508(2) | |
| Cu2– | Pn1 × 2 | 2.450(3) | 2.535(1) | 2.441(2) | 2.527(1) |
| Pn2 | 2.404(6) | 2.503(2) | 2.428(4) | 2.510(3) | |
| Pn3 | 2.404(2) | 2.486(1) | 2.403(2) | 2.493(2) | |
| Cu3– | Pn1 × 2 | 2.482(4) | 2.546(1) | 2.480(3) | 2.547(2) |
| Pn2 | 2.403(5) | 2.492(2) | 2.402(4) | 2.480(3) | |
| Pn2 | 2.513(5) | 2.551(2) | 2.464(4) | 2.539(3) | |
| Atom pairs | Distances (Å) | Atom pairs | Distances (Å) | ||
|---|---|---|---|---|---|
| Eu1– | As2 × 4 | 3.185(1) | Eu2– | As1 × 5 | 3.101(1) |
| As3 × 2 | 3.106(1) | As1 | 3.101(1) | ||
| Cu1– | As1 | 2.511(2) | Cu3– | As1 × 2 | 2.484(1) |
| As1 | 2.520(2) | As2 × 2 | 2.451(1) | ||
| Cu2– | As1 × 2 | 2.513(1) | Cu4/Mg4– | As1 × 4 | 2.867(1) |
| As2 | 2.535(2) | As3 | 2.696(3) | ||
| As3 | 2.509(1) | Cu5– | As2 × 3 | 2.352(1) | |
Eu5Mg2.39Cu16.61As12 was discovered incidentally in the reactions aiming at optimizing the synthetic procedure of Eu2Mg3Cu9As7. The structure of this compound can be viewed as derived from the Zr5Co19P12 type.31 The flexibility of valence electrons in such ternary intermetallics has been well demonstrated by previous references.32–36 The components of these compounds are various, for example, the cations can be rare-earth, alkaline-earth or transition metals, whereas the anions may come from the pnictogen or tetrel elements. Typical ternary analogues include but are not limited to RE5Ir19P12,32 RE5Ru19P12,33 and Ca5T19P12 (RE = rare-earth metals; T = Rh, Ir),34 to name just a few. In particular, compound Sr5Mg19Ge12 can be described as a Zintl phase with the electrons rationalized precisely, [Sr2+]5[Mg2+]19[Ge4−]12,35 and small homogeneity ranges were also suggested on the alkaline-earth positions for A5+xMg18−xTt13 (A = Sr, Ba; Tt = Si, Ge).36 Compared to other transition metals, the RE–Cu–Pn ternary systems were rarely investigated and only two phosphides, Ln5Cu19P12 (Ln = La, Ce), were reported.22 In addition, the related quaternary derivatives of RE5M3M′16Pn12 were also very few, and only the Ln5Zr3Ni16As12 (Ln = La and Y) series was probed so far.37 With the above successes in configuring the ordered structure of A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As), the Eu5Mg2.39Cu16.61As12 is also interesting since in this compound, the mixing between Mg and Cu atoms is significant and also the existence of the non-stoichiometric composition of this compound may indicate a similar electron deficiency in the structure, governed by the Mg/Cu concentrations at the mixed site.
A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As) and Eu5Mg2.39Cu16.61As12 all crystallize in hexagonal crystal systems, while their space groups are different in that the former belongs to P
(no. 174), the latter belongs to P
2m (no. 189), and their crystallographic data are presented in Table 1. They all represent a large family bearing various derivative structures related to the binary phosphide M2P, whose metal-to-nonmetal ratio is close or equal to 2
:
1. The pnictides A2Mn3Cu9Pn7 (Pn = P, As) are quaternary derivatives of the hexagonal Zr2Fe12P7-type structure, and the copper-rich Eu5Mg2.39Cu16.61As12 adopts the Zr5Co19P12 structure type. Their structures viewed in projection down the c-axis are shown in Fig. 1, in which CuPn4 tetrahedrons define the overall framework of the structure. These CuPn4 tetrahedral units are connected through a corner- or edge-sharing manner. In both structures, tunnels form along the c-axis with the alkaline-earth cations filled into the cavities in the anionic framework. Although these two structures are similar in the anionic fragments, their cation coordination environments are subtly different. For A2Mg3Cu9Pn7, the Mg and Cu atoms are ordered, and occupy different crystallographic sites and feature very different coordination geometries, whereas for Eu5Mg2.39Cu16.61As12, the Mg cations are partially substituted by Cu atoms and in such a case, this structure can be readily viewed as derived from the Zr5Co19P12 type31 with the Mg/Cu statistically disordered at the Co sites.
![]() | ||
| Fig. 1 Polyhedral and ball-and-stick view of crystal structure of A2Mg3Cu9Pn7 (A = Sr, Eu; Pn = P, As) (a) and Eu5Mg2.39Cu16.61As12 (b), viewed in the projection down the c-axis. | ||
A more clear illustration of the coordination geometries of various cations as well as the Cu atoms is presented in Fig. 2. For typical alkaline-earth or rare-earth cations such as Sr and Eu, they all exhibit a trigonal prismatic coordination fashion with CN = 6 in both structures. Interestingly, Mg has a relatively smaller coordination number (CN = 5) in these compounds, which adopts the square pyramidal coordination geometry and is reasonable in consideration of its relatively smaller cationic size compared to Sr or Eu. The Cu atoms generally form strong covalent bonds with the pnictide anions coordinated and they prefer the tetrahedral sites with CN = 4. As a typical transition metal, Cu atoms may also act as cations such as in Eu5Mg2.39Cu16.61As12, for which the square pyramidally coordinated Mg can be partially substituted by Cu. As mentioned above, the atomic numbers between Mg and Cu are significantly different, which makes the structure solution of these phases by X-ray diffraction easily conducted. In addition, the possible Cu/Mg mixing at other tetrahedral or trigonal planar sites can be evidentially ruled out. The composition of Eu5Mg2.39Cu16.61As12 from the crystallographic data coincides with the results of EDX analyses as well.
All CuPn4 tetrahedrons in A2Mg3Cu9Pn7 are slightly distorted and the corresponding Cu–As distances fall into the reasonable single-bond distances: d(Cu1–Pn) = 2.404(4)–2.5536(18) Å, d(Cu2–Pn) = 2.4034(15)–2.5351(11) Å and d(Cu3–Pn) = 2.402(4)–2.551(2) Å, respectively. However, for Eu5Mg2.39Cu16.61As12 the Cu atoms also feature square pyramidal and trigonal planar coordination besides the tetrahedral fashion, as illustrated by Cu4 and Cu5 atoms in Fig. 2b. The Cu–As bonding distances in this compound are also in a relatively broad range of 2.3522(14)–2.8671(8) Å. Compared with the regular interatomic distances of Cu–As pairs in other copper-rich analogues such as 2.411–2.595 Å in BaCu8As4,38 2.222(2) Å in Ba2Cu16.33As10,39 these values are still reasonable except for the Cu4–As1 (2.8671(8) Å) and Cu4–As3 (2.696(3) Å). However, taking into account the special square pyramidal coordination geometry of the Cu4 cation, these interactions obviously cannot be simply treated as covalent single bonds. According to references, displacive disorder was also found in this type of structure with the transition metals at the same Wyckoff position.40,41 In the current case, the Cu4 site in Eu5Mg2.39Cu16.61As12 was statistically occupied by 0.203(8) Cu and 0.797(8) Mg, suggested by the single crystal X-ray diffraction data and EDX analyses.
![]() | ||
| Fig. 4 Calculated electronic band structures of the Sr2Mg3Cu9As7 (a) and Eu5Cu19As12 (b). Fermi level is chosen as the energy reference. | ||
The calculated total and projected density of states (TDOS and PDOS) are shown in Fig. 3a. Both compounds show a pseudo-gap in the TDOS curves and below the energy gap the valence bands are crossed by the Fermi level, indicating an electron deficient character for these structures. In the vicinity of the Fermi level, all constituent atoms have significant contributions except for Cu. In addition, the d-orbitals of Cu atoms are almost localized in an energy region from −5.0 to −2.0 eV. Such a characteristic indicates that in these compounds, the Cu anion can be readily treated as Cu+ and based on such a conclusion, the electron counting of these compounds can be established, which results in electron-deficient rationalization in both cases: [Sr2+]2[Mg2+]3[Cu+]9[As3−]7 and [Eu2+]5[Cu+]19[As3−]12. The former is only 2-electron deficient, but the latter will be 7-electron deficient according to this hypothetical mode. In such a situation, if the Cu+ is substituted by Mg2+ as in Eu5Mg2.39Cu16.61As12, the electron-deficiency numbers can be reduced to 4.61. If normalized by the compounds’ formulae, the deficiency numbers are 0.10 and 0.13 per atom for Sr2Mg3Cu9As7 and Eu5Mg2.39Cu16.61As12, respectively, which are still comparable to each other.
The electron deficiency in these compounds can be more informative with the bonding analysis of these compounds. As illustrated in the corresponding COHP curves (Fig. 3b), all Cu–As bonds are well optimized in both structures, however, for the interactions between the alkaline-earth or rare-earth cations and pnictogen anions, the Fermi level crosses a region with significantly bonding interactions. These results indicate that the electron deficiency mainly involves the bonds of A–As, and the physical properties of these compounds should be predominantly governed by the alkaline-earth and pnictogen atoms in the compounds. The electron deficiency can be further illustrated by the calculated electronic band structures, as shown in Fig. 4. It is very clear that the Fermi level crosses the top of the valence bands with a pocket open at G. According to the band structure, the band gaps are almost close in both compounds, corresponding to the pseudo-gaps appearing in their DOS curves. This means that these compounds may be poor-metallic or semi-conducting. Since for LDA or GGA calculations, the underestimation of the band gap is very common, these discrepancies do not impede the assertion that these phases can be considered as Zintl phases.
45 and Eu3Ga2P4.46 The calculated effective magnetic moment is 8.05μB per Eu atom, which is a little different from, but still in good agreement with the Hund's rule derived value of 7.94μB for the free-ion Eu2+ with total angular momentum J = 7/2 and the Landé g factor = 2. These results also rule out the possibility that mixed valency may exist for the europium cations in these compounds.
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| Fig. 5 Temperature dependence of the magnetic susceptibility data of Eu2Mg3Cu9As7, measured under an applied field of 500 Oe. Inset shows the inverse of susceptibility versus temperature. | ||
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| Fig. 6 Temperature-dependent electrical resistivity data measured on a single crystal of Eu2Mg3Cu9As7 by the four-probe method. | ||
Footnote |
| † Electronic supplementary information (ESI) available: EDX analysis on the single crystals of Eu5Mg2.39Cu16.61As12; crystallographic data on Sr2Mg3Cu9P7, Sr2Mg3Cu9As7 and Eu2Mg3Cu9P7; powder X-ray diffraction patterns of Eu2Mg3Cu9As7. See DOI: 10.1039/c6qi00221h |
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