Supporting information
Crystallographic Information File (CIF) https://doi.org/10.1107/S205322961401612X/fn3175sup1.cif | |
Structure factor file (CIF format) https://doi.org/10.1107/S205322961401612X/fn3175Isup2.hkl |
CCDC reference: 1013352
During exploratory syntheses of quasicrystals and approximants in the Ca–Au–Tr system (Tr = Ga, In, Ge, Sn; Lin & Corbett, 2007, 2008a,b, 2010a,b), the 1:1:1 phases were sometimes the minor products in interesting e/a (electron count per atom) regions. These phases were generally well characterized by single-crystal X-ray diffraction. According to the literature, both CaAuGa (Cordier et al., 1993) and CaAuIn (Kußmann et al., 1998) show SrMgSi-type (or TiNiSi-type) structures (space group Pnma). In comparison, the same 1:1:1 ratio yielded polymorphs when group 13 elements (Ga, In) were replaced by group 14 elements (Ge, Sn). For example, two polymorphs of CaAuGe were reported, i.e. a threefold superstructure (space group Pnma) of the SrMgSi-type (Merlo et al., 1998; Kußmann et al., 1998) and a monoclinic derivative (space group C2/m) (Merlo et al., 1998), whereas CaAuSn exhibits a fivefold superstructure (space group Pnma) of the SrMgSi-type parent structure (Kußmann et al., 1998). The formation of all these superstructures is incurred by different ordering between Au and Sn. In this work, we report another CaAuSn phase, which belongs to the EuAuGe-type (space group Imm2) structure (Pöttgen, 1995) and can also be considered as a parent of the CaAuSn superstructure.
High-purity elements of Ca, Au and Sn (all from Alfa Aesar, >99.99%) were weighed in the desired stoichiometries in an Ar-filled glove-box, and the mixtures were sealed in Ta containers using an arc melter under Ar. The Ta containers were then enclosed in SiO2 tubes, which were evacuated down to 10 -6 Torr (1 Torr = 133.322 Pa). The samples were heated from room temperature to 1123 K at a rate of 120 K h-1, kept at 1073 K for 1 d, slowly cooled to 773 K at a rate of 2 K h-1, annealed at this temperature for three weeks and finally quenched in water. High-yield (> 95%) phase products were obtained from various loadings of CaAu1+xSn1-x (x ≤ ±0.2) proportions. All products are fragile, inert to air at room temperature and with a metallic luster.
A single crystal attached to a glass fiber was mounted on a Bruker SMART APEX CCD area-detector diffractometer equipped with Mo Kα (λ = 0.71069 Å) radiation. An exposure time of 10 s per frame at room temperature was adopted. The reflection intensities were integrated using the SAINT-Plus program in the SMART software package (Bruker, 2013). Empirical absorption corrections were accomplished with the aid of the SADABS subprogram (Sheldrick, 1996). The noncentrosymmetric space group was determined by the |E2 - 1| test in XPREP within SHELXTL (Sheldrick, 2008). The structure was solved with the aid of direct methods and subsequently refined on |F2| with a combination of least-squares refinement and difference Fourier maps.
The Au and Sn sites were directly identified by direct methods. After a few cycles of least-square refinements, two independent sites with distances to the Au and Sn sites of ~3.05–3.10 Å were yielded by the difference Fourier map, so Ca was assigned to both sites. Final least-square refinements, with anisotropic displacement parameters, a secondary extinction correction and a constraint of an inversion twin for the noncentric symmetry, yielded R1 = 0.0276, wR2 = 0.0720 and a goodness-of-fit of 1.171 for 23 parameters refined from 330 observed independent data.
The present CaAuSn structure features two puckered layers, in which Au and Sn alterate along the c axis. There are two sets of Au—Sn bond distances in the puckered layers, i.e. 2.628 (1) and 2.663 (3) Å, the two shortest interatomic separations in the structure. Viewed along the a axis, adjacent puckered layers are connected by homo-atomic Au—Au [3.090 (2) Å] and Sn—Sn [2.746 (5) Å] interlayer bonds, as shown in Fig. 1(a), whereas the electropositive Ca atoms are located in the large eight-membered rings. From another viewpoint, the Au–Sn three-dimensional framework can be considered as interlinked ladders (circled with a red line in Fig. 1a), which consist of the above-mentioned interlayer bonds. This structure differs from the SrMgSi-type by the `coloring' with regard to the interlayer bonds (or ladders). As shown in Fig. 1(b), the SrMgSi-type structure consists only of hetero-atomic interlayer bonds.
It turns out that the EuAuGe- and SrMgSi-type structures, both ordered derivatives of the KHg2-type (or CeCu2-type) structure (Hoffmann & Pöttgen, 2001), represent the two basic structural motifs for all the above-mentioned superstructures and others, which are actually intergrowth structures consisting of various proportions of the building blocks of the EuAuGe- and SrMgSi-type structures. Using A and B to represent the ladders of the EuAuGe- and SrMgSi-type structures, respectively, CaAuGe (Merlo et al., 1998; Kußmann et al., 1998) can be considered as a 4A+2B intergrowth structure, as shown in Fig. 2(a). Similarly, the structure of CaAuSn (Kußmann et al., 1998) is a 4A+6B intergrowth structure (Fig. 2b), EuAuSn (Pöttgen et al., 1997) is a 6A+4B intergrowth (Fig. 2c) and YPdSi (Prots' et al., 1998) is a 2A+2B intergrowth structure (Fig. 2d). Apparently, similar phases with other A+B combinations could exist and are to be discovered.
Data collection: SMART (Bruker, 2002); cell refinement: SAINT-Plus (Bruker, 2013); data reduction: SAINT-Plus (Bruker, 2013); program(s) used to solve structure: SHELXS97 (Sheldrick, 2008); program(s) used to refine structure: SHELXL2013 (Sheldrick, 2008); molecular graphics: DIAMOND (Brandenburg, 2000); software used to prepare material for publication: SHELXTL2013 (Sheldrick, 2008).
CaAuSn | Dx = 9.362 Mg m−3 |
Mr = 355.74 | Mo Kα radiation, λ = 0.71073 Å |
Orthorhombic, Imm2 | Cell parameters from 330 reflections |
a = 4.5261 (7) Å | θ = 3.9–28.2° |
b = 7.1356 (11) Å | µ = 69.58 mm−1 |
c = 7.8147 (11) Å | T = 273 K |
V = 252.39 (7) Å3 | Irregular, metallic |
Z = 4 | 0.03 × 0.02 × 0.02 mm |
F(000) = 596 |
Bruker SMART APEXII CCD area-detector diffractometer | 326 reflections with I > 2σ(I) |
Radiation source: Mo Ka | Rint = 0.024 |
ω scans | θmax = 28.2°, θmin = 3.9° |
Absorption correction: empirical (using intensity measurements) (SADABS; Sheldrick, 1996) | h = −5→5 |
Tmin = 0.16, Tmax = 0.27 | k = −4→9 |
769 measured reflections | l = −10→9 |
330 independent reflections |
Refinement on F2 | Secondary atom site location: difference Fourier map |
Least-squares matrix: full | w = 1/[σ2(Fo2) + (0.036P)2 + 7.6305P] where P = (Fo2 + 2Fc2)/3 |
R[F2 > 2σ(F2)] = 0.028 | (Δ/σ)max < 0.001 |
wR(F2) = 0.072 | Δρmax = 2.68 e Å−3 |
S = 1.17 | Δρmin = −1.85 e Å−3 |
330 reflections | Extinction correction: SHELXL2013 (Sheldrick, 2008), Fc*=kFc[1+0.001xFc2λ3/sin(2θ)]-1/4 |
23 parameters | Extinction coefficient: 0.0072 (10) |
1 restraint | Absolute structure: Refined as an inversion twin (Flack, 1983) |
Primary atom site location: structure-invariant direct methods | Absolute structure parameter: 0.31 (3) |
CaAuSn | V = 252.39 (7) Å3 |
Mr = 355.74 | Z = 4 |
Orthorhombic, Imm2 | Mo Kα radiation |
a = 4.5261 (7) Å | µ = 69.58 mm−1 |
b = 7.1356 (11) Å | T = 273 K |
c = 7.8147 (11) Å | 0.03 × 0.02 × 0.02 mm |
Bruker SMART APEXII CCD area-detector diffractometer | 330 independent reflections |
Absorption correction: empirical (using intensity measurements) (SADABS; Sheldrick, 1996) | 326 reflections with I > 2σ(I) |
Tmin = 0.16, Tmax = 0.27 | Rint = 0.024 |
769 measured reflections |
R[F2 > 2σ(F2)] = 0.028 | 1 restraint |
wR(F2) = 0.072 | Δρmax = 2.68 e Å−3 |
S = 1.17 | Δρmin = −1.85 e Å−3 |
330 reflections | Absolute structure: Refined as an inversion twin (Flack, 1983) |
23 parameters | Absolute structure parameter: 0.31 (3) |
Geometry. All e.s.d.'s (except the e.s.d. in the dihedral angle between two l.s. planes) are estimated using the full covariance matrix. The cell e.s.d.'s are taken into account individually in the estimation of e.s.d.'s in distances, angles and torsion angles; correlations between e.s.d.'s in cell parameters are only used when they are defined by crystal symmetry. An approximate (isotropic) treatment of cell e.s.d.'s is used for estimating e.s.d.'s involving l.s. planes. |
Refinement. Refined as an inversion twin. |
x | y | z | Uiso*/Ueq | ||
Au | 0.0000 | 0.21650 (14) | 0.68259 (7) | 0.0106 (5) | |
Sn | 0.0000 | 0.3076 (4) | 0.0130 (3) | 0.0163 (6) | |
Ca1 | 0.5000 | 0.5000 | 0.8058 (15) | 0.0083 (18) | |
Ca2 | 0.0000 | 0.5000 | 0.3876 (16) | 0.0109 (19) |
U11 | U22 | U33 | U12 | U13 | U23 | |
Au | 0.0111 (6) | 0.0074 (6) | 0.0133 (6) | 0.000 | 0.000 | 0.0007 (7) |
Sn | 0.0145 (14) | 0.0191 (10) | 0.0153 (13) | 0.000 | 0.000 | 0.0004 (9) |
Ca1 | 0.010 (5) | 0.006 (4) | 0.009 (4) | 0.000 | 0.000 | 0.000 |
Ca2 | 0.014 (6) | 0.007 (4) | 0.012 (5) | 0.000 | 0.000 | 0.000 |
Au—Sni | 2.6282 (13) | Ca1—Snxvi | 3.103 (7) |
Au—Snii | 2.6282 (13) | Ca1—Sniii | 3.103 (7) |
Au—Sniii | 2.663 (3) | Ca1—Snxvii | 3.103 (7) |
Au—Ca2 | 3.067 (9) | Ca1—Snii | 3.171 (9) |
Au—Auiv | 3.090 (2) | Ca1—Snxviii | 3.171 (9) |
Au—Ca2v | 3.174 (6) | Ca1—Auxix | 3.185 (4) |
Au—Ca2vi | 3.174 (6) | Ca1—Auxii | 3.185 (4) |
Au—Ca1vii | 3.185 (4) | Ca1—Auxx | 3.185 (4) |
Au—Ca1 | 3.185 (4) | Ca1—Auxviii | 3.325 (11) |
Au—Ca1viii | 3.325 (11) | Ca1—Auii | 3.325 (11) |
Sn—Auix | 2.6282 (13) | Ca2—Auxii | 3.067 (9) |
Sn—Aux | 2.6282 (13) | Ca2—Aux | 3.174 (6) |
Sn—Auxi | 2.663 (3) | Ca2—Auxxi | 3.174 (6) |
Sn—Snxii | 2.746 (5) | Ca2—Auxxii | 3.174 (6) |
Sn—Ca1xiii | 3.103 (7) | Ca2—Auix | 3.174 (6) |
Sn—Ca1xi | 3.103 (7) | Ca2—Snxii | 3.233 (12) |
Sn—Ca1viii | 3.171 (9) | Ca2—Snxviii | 3.301 (4) |
Sn—Ca2 | 3.233 (12) | Ca2—Sni | 3.301 (4) |
Sn—Ca2viii | 3.301 (4) | Ca2—Snii | 3.301 (4) |
Sn—Ca2xiv | 3.301 (4) | Ca2—Snxxiii | 3.301 (4) |
Ca1—Snxv | 3.103 (7) | ||
Sni—Au—Snii | 118.87 (9) | Snxv—Ca1—Auxix | 50.09 (5) |
Sni—Au—Sniii | 120.33 (5) | Snxvi—Ca1—Auxix | 85.44 (6) |
Snii—Au—Sniii | 120.33 (5) | Sniii—Ca1—Auxix | 163.2 (3) |
Sni—Au—Ca2 | 70.38 (8) | Snxvii—Ca1—Auxix | 113.27 (9) |
Snii—Au—Ca2 | 70.38 (8) | Snii—Ca1—Auxix | 102.8 (3) |
Sniii—Au—Ca2 | 124.60 (17) | Snxviii—Ca1—Auxix | 48.85 (10) |
Sni—Au—Auiv | 86.25 (6) | Au—Ca1—Auxix | 144.8 (4) |
Snii—Au—Auiv | 86.25 (6) | Snxv—Ca1—Auxii | 113.27 (9) |
Sniii—Au—Auiv | 104.13 (6) | Snxvi—Ca1—Auxii | 163.2 (3) |
Ca2—Au—Auiv | 131.27 (15) | Sniii—Ca1—Auxii | 85.44 (6) |
Sni—Au—Ca2v | 146.78 (8) | Snxvii—Ca1—Auxii | 50.09 (5) |
Snii—Au—Ca2v | 66.97 (18) | Snii—Ca1—Auxii | 102.8 (3) |
Sniii—Au—Ca2v | 68.2 (2) | Snxviii—Ca1—Auxii | 48.85 (10) |
Ca2—Au—Ca2v | 134.46 (14) | Au—Ca1—Auxii | 78.87 (11) |
Auiv—Au—Ca2v | 60.88 (7) | Auxix—Ca1—Auxii | 90.57 (13) |
Sni—Au—Ca2vi | 66.97 (18) | Snxv—Ca1—Auxx | 85.44 (6) |
Snii—Au—Ca2vi | 146.78 (8) | Snxvi—Ca1—Auxx | 50.09 (5) |
Sniii—Au—Ca2vi | 68.2 (2) | Sniii—Ca1—Auxx | 113.27 (9) |
Ca2—Au—Ca2vi | 134.46 (14) | Snxvii—Ca1—Auxx | 163.2 (3) |
Auiv—Au—Ca2vi | 60.88 (7) | Snii—Ca1—Auxx | 48.85 (10) |
Ca2v—Au—Ca2vi | 91.0 (2) | Snxviii—Ca1—Auxx | 102.8 (3) |
Sni—Au—Ca1vii | 65.30 (16) | Au—Ca1—Auxx | 90.57 (13) |
Snii—Au—Ca1vii | 143.71 (12) | Auxix—Ca1—Auxx | 78.87 (11) |
Sniii—Au—Ca1vii | 63.4 (2) | Auxii—Ca1—Auxx | 144.8 (4) |
Ca2—Au—Ca1vii | 78.95 (14) | Snxv—Ca1—Auxviii | 48.12 (15) |
Auiv—Au—Ca1vii | 129.44 (6) | Snxvi—Ca1—Auxviii | 75.1 (2) |
Ca2v—Au—Ca1vii | 131.5 (4) | Sniii—Ca1—Auxviii | 75.1 (2) |
Ca2vi—Au—Ca1vii | 69.50 (12) | Snxvii—Ca1—Auxviii | 48.12 (15) |
Sni—Au—Ca1 | 143.71 (12) | Snii—Ca1—Auxviii | 163.9 (3) |
Snii—Au—Ca1 | 65.30 (16) | Snxviii—Ca1—Auxviii | 108.51 (7) |
Sniii—Au—Ca1 | 63.4 (2) | Au—Ca1—Auxviii | 124.3 (2) |
Ca2—Au—Ca1 | 78.95 (14) | Auxix—Ca1—Auxviii | 88.43 (13) |
Auiv—Au—Ca1 | 129.44 (6) | Auxii—Ca1—Auxviii | 88.43 (13) |
Ca2v—Au—Ca1 | 69.50 (12) | Auxx—Ca1—Auxviii | 124.3 (2) |
Ca2vi—Au—Ca1 | 131.5 (4) | Snxv—Ca1—Auii | 75.1 (2) |
Ca1vii—Au—Ca1 | 90.57 (14) | Snxvi—Ca1—Auii | 48.12 (15) |
Sni—Au—Ca1viii | 61.51 (5) | Sniii—Ca1—Auii | 48.12 (15) |
Snii—Au—Ca1viii | 61.51 (5) | Snxvii—Ca1—Auii | 75.1 (2) |
Sniii—Au—Ca1viii | 166.45 (12) | Snii—Ca1—Auii | 108.51 (7) |
Ca2—Au—Ca1viii | 69.0 (2) | Snxviii—Ca1—Auii | 163.9 (3) |
Auiv—Au—Ca1viii | 62.31 (10) | Au—Ca1—Auii | 88.43 (13) |
Ca2v—Au—Ca1viii | 102.76 (15) | Auxix—Ca1—Auii | 124.3 (2) |
Ca2vi—Au—Ca1viii | 102.76 (15) | Auxii—Ca1—Auii | 124.3 (2) |
Ca1vii—Au—Ca1viii | 124.3 (2) | Auxx—Ca1—Auii | 88.43 (13) |
Ca1—Au—Ca1viii | 124.3 (2) | Auxviii—Ca1—Auii | 55.4 (2) |
Auix—Sn—Aux | 118.87 (9) | Auxii—Ca2—Au | 82.5 (3) |
Auix—Sn—Auxi | 118.23 (5) | Auxii—Ca2—Aux | 134.46 (13) |
Aux—Sn—Auxi | 118.23 (5) | Au—Ca2—Aux | 93.35 (6) |
Auix—Sn—Snxii | 93.75 (6) | Auxii—Ca2—Auxxi | 93.35 (6) |
Aux—Sn—Snxii | 93.75 (6) | Au—Ca2—Auxxi | 134.46 (13) |
Auxi—Sn—Snxii | 104.13 (6) | Aux—Ca2—Auxxi | 119.4 (4) |
Auix—Sn—Ca1xiii | 156.94 (10) | Auxii—Ca2—Auxxii | 93.35 (6) |
Aux—Sn—Ca1xiii | 70.37 (16) | Au—Ca2—Auxxii | 134.46 (13) |
Auxi—Sn—Ca1xiii | 66.55 (19) | Aux—Ca2—Auxxii | 58.25 (13) |
Snxii—Sn—Ca1xiii | 63.74 (7) | Auxxi—Ca2—Auxxii | 91.0 (2) |
Auix—Sn—Ca1xi | 70.37 (16) | Auxii—Ca2—Auix | 134.46 (13) |
Aux—Sn—Ca1xi | 156.94 (10) | Au—Ca2—Auix | 93.35 (6) |
Auxi—Sn—Ca1xi | 66.55 (19) | Aux—Ca2—Auix | 91.0 (2) |
Snxii—Sn—Ca1xi | 63.74 (7) | Auxxi—Ca2—Auix | 58.25 (13) |
Ca1xiii—Sn—Ca1xi | 93.7 (3) | Auxxii—Ca2—Auix | 119.4 (4) |
Auix—Sn—Ca1viii | 65.84 (7) | Auxii—Ca2—Sn | 163.9 (3) |
Aux—Sn—Ca1viii | 65.84 (7) | Au—Ca2—Sn | 113.61 (8) |
Auxi—Sn—Ca1viii | 122.06 (18) | Aux—Ca2—Sn | 48.42 (14) |
Snxii—Sn—Ca1viii | 133.81 (16) | Auxxi—Ca2—Sn | 75.5 (2) |
Ca1xiii—Sn—Ca1viii | 133.07 (11) | Auxxii—Ca2—Sn | 75.5 (2) |
Ca1xi—Sn—Ca1viii | 133.07 (11) | Auix—Ca2—Sn | 48.42 (14) |
Auix—Sn—Ca2 | 64.61 (6) | Auxii—Ca2—Snxii | 113.61 (8) |
Aux—Sn—Ca2 | 64.61 (6) | Au—Ca2—Snxii | 163.9 (3) |
Auxi—Sn—Ca2 | 169.01 (14) | Aux—Ca2—Snxii | 75.5 (2) |
Snxii—Sn—Ca2 | 64.88 (11) | Auxxi—Ca2—Snxii | 48.42 (14) |
Ca1xiii—Sn—Ca2 | 106.53 (16) | Auxxii—Ca2—Snxii | 48.42 (14) |
Ca1xi—Sn—Ca2 | 106.53 (16) | Auix—Ca2—Snxii | 75.5 (2) |
Ca1viii—Sn—Ca2 | 68.9 (2) | Sn—Ca2—Snxii | 50.2 (2) |
Auix—Sn—Ca2viii | 134.14 (13) | Auxii—Ca2—Snxviii | 48.58 (11) |
Aux—Sn—Ca2viii | 61.05 (16) | Au—Ca2—Snxviii | 102.4 (3) |
Auxi—Sn—Ca2viii | 63.2 (2) | Aux—Ca2—Snxviii | 164.2 (3) |
Snxii—Sn—Ca2viii | 131.67 (7) | Auxxi—Ca2—Snxviii | 48.51 (4) |
Ca1xiii—Sn—Ca2viii | 68.86 (12) | Auxxii—Ca2—Snxviii | 108.36 (8) |
Ca1xi—Sn—Ca2viii | 129.7 (4) | Auix—Ca2—Snxviii | 89.12 (6) |
Ca1viii—Sn—Ca2viii | 75.76 (15) | Sn—Ca2—Snxviii | 123.4 (3) |
Ca2—Sn—Ca2viii | 123.4 (3) | Snxii—Ca2—Snxviii | 89.22 (13) |
Auix—Sn—Ca2xiv | 61.05 (16) | Auxii—Ca2—Sni | 102.4 (3) |
Aux—Sn—Ca2xiv | 134.14 (13) | Au—Ca2—Sni | 48.58 (11) |
Auxi—Sn—Ca2xiv | 63.2 (2) | Aux—Ca2—Sni | 48.51 (4) |
Snxii—Sn—Ca2xiv | 131.67 (7) | Auxxi—Ca2—Sni | 164.2 (3) |
Ca1xiii—Sn—Ca2xiv | 129.7 (4) | Auxxii—Ca2—Sni | 89.12 (6) |
Ca1xi—Sn—Ca2xiv | 68.86 (12) | Auix—Ca2—Sni | 108.36 (8) |
Ca1viii—Sn—Ca2xiv | 75.76 (15) | Sn—Ca2—Sni | 89.22 (13) |
Ca2—Sn—Ca2xiv | 123.4 (3) | Snxii—Ca2—Sni | 123.4 (3) |
Ca2viii—Sn—Ca2xiv | 86.54 (14) | Snxviii—Ca2—Sni | 145.5 (4) |
Snxv—Ca1—Snxvi | 52.52 (15) | Auxii—Ca2—Snii | 102.4 (3) |
Snxv—Ca1—Sniii | 117.1 (4) | Au—Ca2—Snii | 48.58 (11) |
Snxvi—Ca1—Sniii | 93.7 (3) | Aux—Ca2—Snii | 108.36 (8) |
Snxv—Ca1—Snxvii | 93.7 (3) | Auxxi—Ca2—Snii | 89.12 (6) |
Snxvi—Ca1—Snxvii | 117.1 (4) | Auxxii—Ca2—Snii | 164.2 (3) |
Sniii—Ca1—Snxvii | 52.52 (15) | Auix—Ca2—Snii | 48.51 (4) |
Snxv—Ca1—Snii | 133.07 (11) | Sn—Ca2—Snii | 89.22 (13) |
Snxvi—Ca1—Snii | 94.03 (5) | Snxii—Ca2—Snii | 123.4 (3) |
Sniii—Ca1—Snii | 94.03 (5) | Snxviii—Ca2—Snii | 83.34 (14) |
Snxvii—Ca1—Snii | 133.07 (11) | Sni—Ca2—Snii | 86.55 (14) |
Snxv—Ca1—Snxviii | 94.03 (5) | Auxii—Ca2—Snxxiii | 48.58 (11) |
Snxvi—Ca1—Snxviii | 133.07 (11) | Au—Ca2—Snxxiii | 102.4 (3) |
Sniii—Ca1—Snxviii | 133.07 (11) | Aux—Ca2—Snxxiii | 89.12 (6) |
Snxvii—Ca1—Snxviii | 94.03 (5) | Auxxi—Ca2—Snxxiii | 108.36 (7) |
Snii—Ca1—Snxviii | 87.6 (3) | Auxxii—Ca2—Snxxiii | 48.51 (4) |
Snxv—Ca1—Au | 163.2 (3) | Auix—Ca2—Snxxiii | 164.2 (3) |
Snxvi—Ca1—Au | 113.27 (9) | Sn—Ca2—Snxxiii | 123.4 (3) |
Sniii—Ca1—Au | 50.09 (5) | Snxii—Ca2—Snxxiii | 89.22 (13) |
Snxvii—Ca1—Au | 85.44 (6) | Snxviii—Ca2—Snxxiii | 86.55 (14) |
Snii—Ca1—Au | 48.85 (10) | Sni—Ca2—Snxxiii | 83.34 (14) |
Snxviii—Ca1—Au | 102.8 (3) | Snii—Ca2—Snxxiii | 145.5 (4) |
Symmetry codes: (i) −x−1/2, −y+1/2, z+1/2; (ii) −x+1/2, −y+1/2, z+1/2; (iii) x, y, z+1; (iv) −x, −y, z; (v) x+1/2, y−1/2, z+1/2; (vi) x−1/2, y−1/2, z+1/2; (vii) x−1, y, z; (viii) x−1/2, y−1/2, z−1/2; (ix) −x+1/2, −y+1/2, z−1/2; (x) −x−1/2, −y+1/2, z−1/2; (xi) x, y, z−1; (xii) −x, −y+1, z; (xiii) x−1, y, z−1; (xiv) x+1/2, y−1/2, z−1/2; (xv) −x+1, −y+1, z+1; (xvi) x+1, y, z+1; (xvii) −x, −y+1, z+1; (xviii) x+1/2, y+1/2, z+1/2; (xix) −x+1, −y+1, z; (xx) x+1, y, z; (xxi) x+1/2, y+1/2, z−1/2; (xxii) x−1/2, y+1/2, z−1/2; (xxiii) x−1/2, y+1/2, z+1/2. |
Experimental details
Crystal data | |
Chemical formula | CaAuSn |
Mr | 355.74 |
Crystal system, space group | Orthorhombic, Imm2 |
Temperature (K) | 273 |
a, b, c (Å) | 4.5261 (7), 7.1356 (11), 7.8147 (11) |
V (Å3) | 252.39 (7) |
Z | 4 |
Radiation type | Mo Kα |
µ (mm−1) | 69.58 |
Crystal size (mm) | 0.03 × 0.02 × 0.02 |
Data collection | |
Diffractometer | Bruker SMART APEXII CCD area-detector diffractometer |
Absorption correction | Empirical (using intensity measurements) (SADABS; Sheldrick, 1996) |
Tmin, Tmax | 0.16, 0.27 |
No. of measured, independent and observed [I > 2σ(I)] reflections | 769, 330, 326 |
Rint | 0.024 |
(sin θ/λ)max (Å−1) | 0.664 |
Refinement | |
R[F2 > 2σ(F2)], wR(F2), S | 0.028, 0.072, 1.17 |
No. of reflections | 330 |
No. of parameters | 23 |
No. of restraints | 1 |
Δρmax, Δρmin (e Å−3) | 2.68, −1.85 |
Absolute structure | Refined as an inversion twin (Flack, 1983) |
Absolute structure parameter | 0.31 (3) |
Computer programs: SMART (Bruker, 2002), SAINT-Plus (Bruker, 2013), SHELXS97 (Sheldrick, 2008), SHELXL2013 (Sheldrick, 2008), DIAMOND (Brandenburg, 2000), SHELXTL2013 (Sheldrick, 2008).