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1.
Eu3+ and Eu2+ in Oxides of the Composition MBeLn2O5: SrBeEu2O5 and EuBeNd2O5 Single crystals of (I): SrBeEu2O5 and (II): EuBeNd2O5 were prepared by CO2-LASER (I) in air and plasma torch (II) technique in H2 atmosphere. X-ray investigations led to orthorhombic symmetry, space group D-Pnma; (I): a = 9.488, b = 7.156, c = 6.495 Å; (II): a = 9.534, b = 7.225, c = 6.544 Å, Z = 4. Sr2+ and Eu3+ as well as Eu2+ and Nd3+ are in statistical distribution within a Kagomé framework. Both compounds are discussed with respect to the monoclinic form of MBeLn2O5.  相似文献   

2.
About a Mixed Valence Oxoniobate: Sr5Nb34+Nb25+O16 The hitherto unknown compound Sr5Nb5O16 was prepared and examined by X-ray single crystal work. It crystallizes with orthorhombic symmetry (space group D–Pmn21, a = 3.992(1), b = 32.476(10), c = 5.677(2) Å; Z = 2). Sr5Nb5O16 consists of stacked perovskite-like blocks cut by a plane perpendicular to the cube face diagonal of the perovskite structure. The coordination relations of the intersections between those blocks and the distribution of Nb5+ and Nb4+ are discussed.  相似文献   

3.
The Crystal Structure of Perovskites A NiIIMVIO6. II. Sr2NiWO6 The results of an X-ray single crystal study of the perovskite Sr[NiIIWVI](6)O6, ordered in the octahedral sites, are given. While Sr[NiIITeVI](6)O6 crystallizes in a monoclinically deformed structure of the perovskite (elpasolite) type, showing a phase transition to a tetragonal lattice at 675 °K, Sr[NiIIWVI](6)O6 is tetragonal already at 298°K (space group: C; a = b = 5.559 Å; c = 7.918 Å; Z = 2). The Ni? O distances found for the tungsten compound are nearly identical with those of the tellurium perovskite. In contradiction to crystal field theory very different values of the ligand field parameter Δ (ca. 25%) are observed for these two compounds however. Obviously this effect is caused by the rather different kind of bonding within the NiO6 polyhedra in the two compounds. On the basis of the structural results the Ni? O-bonding in the two perovskites is discussed in dependence of the next nearest cationic environment.  相似文献   

4.
Compound Formation MeO: M2O3. VI. Synthesis and Structure Determination of Sr1,33 Pb0,67 Al6O11 Single crystal of Sr1,33Pb0.67Al6O11 could be prepared with a PbO flux. (Space group D–Pnnm, a = 22.13, b = 4.88, c = 8.42 Å, Z = 4) Sr2+ and Pb2+ are statistically intercalated into a framework of AlO6 octahedra and AlO4 tetrahedra. The typical coordination of Sr2+ and Pb2+ is realized by occupying different positions in the same cavern.  相似文献   

5.
On Ordered Perovskites with Cationic Vacancies. IX. Compounds of the Type Sr2Sr1/4B □1/4WO6?Sr8SrB ?W4O24 (BIII ? La, Pr, Nd, Sm–Tm, Y) The compounds Sr2Sr1/4B□1/4WO6?Sr8SrB?W4O24 belong to the group of perovskites with octahedral cationic vacancies (cation/vacancy ratio (CN 6) ?:1). For the larger BIII ions (La, Pr, Nd, Sm–Dy) different ordering effects are observed. The perovskites with BIII ? Sm, Eu, Gd are polymorphic too (HT modification: higher ordered cubic perovskite (BIII ? Gd: a = 2X8.234 Å); LT modification: hexagonal perovskite stacking polytype (BIII ? Gd: a = 9.954 Å; c = 19.04 Å)). With the smaller BIII ions (Ho, Er, Tm and Y) a cubic, 1:1 ordered perovskite type is observed.  相似文献   

6.
On the Atomic Distribution in Ba2SrIn2O6 with a Contribution to the Existence of the Calciumferrite-Type of Oxoindates (I) Ba2SrIn2O6 and (II) Sr0.93Ba0.07In2O4 were prepared and investigated by single crystal X-ray technique. I crystallizes with tetragonal symmetry, space group D – I4/mmm, a = 4.168; c = 21.290 Å; Z = 2; II belongs to the orthorhombic space group D – Pnma, a = 9.858; b = 3.273; c = 11.520 Å; Z = 4. I shows in respect to the formerly investigated compound BaSr2In2O6 an unexpected statistically distribution of Ba2+ and Sr2+ with the La2SrCu2O6 type. II marks the range of existence of the calciumferrite type within the alkaline earth oxoindates in direction of large radii of M2+ ions.  相似文献   

7.
Photoluminescence of Trivalent Rare Earths in Perovskite Stacking Polytypes Ba2La2?x RE MgW2□O12, Ba6Y2?x RE W3□O18, and Sr8SrGd2?xRE W4□O24 Rhombohedral 12 L stacking polytypes Ba2La2?xREMgW2□O12 show with RE3+ = Pr, Sm, Eu, Tb, Dy, Ho, Er, Tm; the 18 L stacking polytypes Ba6Y2?xREW3□O18 and the polymorphic perovskites Sr8SrGd2?xREW4□O24 with RE3+ = Sm, Eu, Dy, Ho, Er visible photoluminescence. The concentration dependence and the influence of the coordination number of the rare earth are reported.  相似文献   

8.
A New Mixed Valence Strontium Niobium Oxide Sr7Nb24+Nb45+O21 \documentclass{article}\pagestyle{empty}\begin{document}$ \widehat = $\end{document} Sr1.167NbO3.5 The unknown compound Sr7Nb6O21 kristallisiert nach Einkristall-Röntgenbeugungsdaten rhomboedrisch (Raumgruppe C? R3 ; a = 16,450(5) Å, α = 19,85(1)° trigonale Aufstellung: a = 5,670(1), c = 48,364(13) Å). The compound is built up by perovskite blocks with a width of 6 octahedra. The crystal chemistry especially of the interspace between those blocks is discussed in respect to related compounds.  相似文献   

9.
On Hexagonal Perovskites with Cationic Vacancies. XXXI. Systems BaO? Re2O7? M O5 with MV = Nb, Ta In the systems BaO? Re2O7? MO5 three quaternary oxides are formed, which belong to the perovskite stacking polytypes with cationic vacancies: Ba8Re7/2M□3O24 (MV = Nb, Ta; rhombohedral 24 L type; sequence (hhhhchhc)3; space group R3 m), Ba4Re9/8Ta13/85/4O12 (rhombohedral 12 L type; sequence (hhcc)3; space group R3 m) and the phases Ba5BaRe3/2?xM □O15?xx (MV = Nb, Ta; variants of a hexagonal 5 L type).  相似文献   

10.
The first Alkaline Alkaline-Earth Oxocuprate (II, III): NaBa2Cu22+Cu3+O6 The compound NaBa2Cu3O6 was prepared by heating of Na2O2, BaO2, Cu2O in closed Ag-tubes. X-ray single crystal investigations led to orthorhombic symmetry, space group D-Fmmm; a = 8.4229; b = 11.4418; c = 14.4063 Å; Z = 8. Cu2+ and Cu3+ show square planar polygones of four and Na+ trigonal prisms of six O2?. The two barium point positions show coordination numbers C.N. = 8 and 6 + 4. The crystal structure is discussed.  相似文献   

11.
An MP4(full,SDTQ)/6-311++G(d,p)//MP2(full)/6-311++G(d,p) ab initio study was performed of the reactions of formyl and isoformyl cations with H2O and NH3, which play an important role in flame and interstellar chemistries. Two different confluent channels were located leading to CO+H3O+/NH. The first one corresponds to the approach of the neutral molecule to the carbon atom of the cations. The second one leads to the direct proton transfer from the cations to the neutrals. At 900 K the separate products CO+H3O+/NH are the most stable species along the Gibbs energy profiles for the processes. For the reaction with H2O the reaction channel leading to HC(OH) (protonated formic acid) is disfavored with respect to the two CO+H3O+ channels in agreement with the experimental evidence that H3O+ is the major ion observed in hydrocarbon flames. According to our calculations, NH+H2O are considerably more stable in Gibbs energy than NH3+H3O+;NH will predominate in the reaction zone when ammonia is added to CH4+Ar diffusion flame, as experimentally observed. At 100 K the most stable structures are the intermediate complexes CO…HOH/HNH. Particularly the CO…HOH complex has a lifetime large enough to be detected and, therefore, could play a certain role in interstellar chemistry. ©1999 John Wiley & Sons, Inc. J Comput Chem 20: 1432–1443, 1999  相似文献   

12.
On Ordered Perovskites with Cationic Vacancies. X. Compounds of Type A B B □1/4MVIO6 ? A BIIB □M O24 with AII, BII = Ba, Sr, Ca and MVI = U, W Perovskites of type Ba8BIIB2III□UO24 show polymorphic phase transformations of order disorder type. An 1:1 ordered orthorhombic HT form is transformed into a higher ordered LT modification with a fourfold cell content (four formula units Ba8BIIB□U4O24), compared to cubic 1:1 ordered perovskites A2BMO6. In the series Ba8BaB□W4O24 and Sr8SrB□W4O24 different ordering phenomena are observed. In comparison with 1:1 ordered cubic perovskites A2BMO6, the cell contains eight formula units ABIIB□W4O24. The higher ordered cells with UVI and WVI are face centered, which has its origin in an ordering of cationic vacancies.  相似文献   

13.
Crystal Structure and Properties of Calcium and Strontium Hexathiodiphosphate(IV), Ca2P2S6 and Sr2P2S6, with a Contribution on Ca5P8 and Pb2P2S6 Ca2P2S6 and Sr2P2S6 were prepared from metal and a mixture of red phosphorus and sulfur (molar ratio M:P:S = 1:1:3) in 2 corundum crucibles inserted in quartz ampullae under vacuum (20 d 900°C). The compounds were obtained as colourless, crystalline powders containing single crystals. They crystallize in the Sn2P2S6 (high temperature form) type structure (P21/c, Z = 2): Ca2P2S6 a = 653.2(2)pm, b = 728.1(2)pm, c = 1110.1(4)pm, β = 124.00(4)°, d = 2.50(2); Sr2P2S6 a = 664.3(2)pm, b = 755.7(3)pm, c = 1139.7(3)pm, β = 124.07(2)°, d = 2.97(2). The anions P2S have staggered confirmation and are arranged with the motif of a cubic close-packing. Sr2+ is coordinated by 8S which form a twofold face-capped trigonal prism and belong to 4P2S. Structure calculations clearly show that Pb2P2S6 also crystallizes in P21/c and not in Pc [1]. Also, Raman- and IR-spectra of Ca5P8 were recorded at 20°C. The stretching vibrations of P were assigned in analogy to those of P2S in alkaline earth hexathiodiphosphates(IV). The range of their frequencies (480 to 340 cm?1) is essentially smaller and shifted to smaller values compared with P2S in Ca2P2S6 and Sr2P2S6 (620 to 390 cm?1). The symmetry of P is not D3d but C2h as in the case of P2S.  相似文献   

14.
The Structures of the Hexagonal Elpasolite-Type Compounds Ba3NiSb2O9 and Ba3CuSb2O9 The results of an X-ray single crystal study of the hexagonal elpasolite Ba(NiSb2)(6)O9 are given. (Space group: C; a = b = 5.837 Å, c = 14.392 Å; Z = 2). The structure can be described by close-packed BaO3 layers alternating in the sequence c c h c c h … (hex. BaTiO3 type). Groups of two octahedra with common faces are connected by SbO6 octahedra via common corners. They are occupied alternately by Ni and Sb. The final reliability index was R = 3.0%. The Cu2+-compound is of the same structural type. The ligand field and EPR spectra are discussed in comparison with related Ni2+ and Cu2+ compounds.  相似文献   

15.
A Contribution on Sr3Nd4O9 The metastable compound Sr3Nd4O9 was prepared by high temperature reactions and investigated by X-ray single crystal methods. It crystallizes with monoclinic symmetry: a = 1147.4; b = 723.8; c = 1324.6 pm and β = 115.6°: space group C? Cs. The metal positions show a nearly statistical distribution of Sr2+ and Nd3+. The network of the polyhedrals characterizes a new structure type, which in spite of the statistical metal distribution does not belong to the high temperature X-modification of the Rare Earth sesquioxides.  相似文献   

16.
On a Novel Alkaline Earth Metal Oxothallate: Sr4Tl2O7 The hitherto unknown compound Sr4Tl2O7 was prepared and investigated by X-ray single crystal methods. Sr4Tl2O7 crystallizes in the tetragonal space group C? P42nm (a = 5.006, c = 18.73 Å). Sr2+ has a trigonal prismatic surrounding whereas Tl3+ shows 2+2 oxygen neighbours. The crystal structure is completely described.  相似文献   

17.
CuTb[B5O10]: The first “Metaborate” with a [B5O10]5? Anion Single crystals of the new compound CuTb[B5O10] were obtained by a B2O3 flux-technique. They crystallize in a so far unknown structure. X-ray investigations on single crystals led to the space group C–I ba2 (Nr. 45); a = 6.294(1) Å; b = 8.406(8) Å; c = 12.733(2) Å; Z = 4. The structure contains [B5O10]5? chains isolated from each other. These chains include twelf membered rings of boron and oxygen. Each ring consists of two tetrahedral BO4 and two planar B2O5 groups and is connected with the next one via the BO4 units. Tb3+ is eightfold- and Cu2+ elongated octahedraly coordinated by oxygen.  相似文献   

18.
The Crystal Chemistry of Copper Rare-Earth Oxotungstates: (I): triclinic-α-CuTbW2O8, (II): monoclinic-CuInW2O8 and (III): monoclinic-CuYW2O8 Single crystals of (I), (II) and (III) were prepared by recrystallisation in closed systems and examined by X-ray technique. (I): space group C? P1 , a = 7.3080, b = 7.8945, c = 7.1476 Å, α = 115.23, β = 116.21, γ = 56.98°, Z = 2; (II): space group C? C2/c, a = 9.6576, b = 11.6496, c = 4.9863 Å, β = 91.17°, Z = 4; (III): space group C? P2/n, a = 10.0504, b = 5.8214, c = 5.0224 Å, β = 94.23°, Z = 2. The crystal structures are discussed with respect to calculations of the coulombterms of lattice energy and possible valence states of Cu2+ and Mo5+.  相似文献   

19.
Single Crystal X-Ray Analysis of Sr3TiGa10O20 Single crystals of Sr3TiGa10O20 were prepared by recrystallisation of a molten oxide mixture and investigated by X-Ray technique. It crystallizes with monoclinic symmetry, space group C–C2/m, a = 15.451, b = 11.579, c = 5.051 Å, β = 108.57°, Z = 2. Sr3TiGa10O20 belongs to the Pb3GeAl10O20 type, showing Ga3+ in tetrahedral and octahedral coordination. The octahedral coordinated point positions are occupied by Ga3+ and Ti4+ statistically.  相似文献   

20.
The First Alkalinc Alkaline Earth Oxoniccolate(II,III): NaBa2Ni22+Ni3+O6 Single crystals of NaBa2Ni22+Ni3+O6 were prepared by solid state reaction. X-ray investigations led to orthorhombic symmetry, space group D-Fmmm; a = 8.310; b = 11.220; c = 14.397 Å; Z = 8. Na+ is coordinated by six O2? in form of a trigonal prism and the two Ba2+ point positions show different coordination numbers C.N. = 6 + 4 and 8. The Ni2+ /Ni3+ ions are in square planar polygons, six of them are forming a so far unknown closed macro polyhedra.  相似文献   

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