首页 | 本学科首页   官方微博 | 高级检索  
相似文献
 共查询到20条相似文献,搜索用时 11 毫秒
1.
On Ordered Perovskites with Cationic Vacancies. XI. Compounds of Type A B B □1/4WVIO6 ? A BIIB □W O24 with AII, BII = Ba, Sr Depending on the ionic radii of the two and three valent cations in the perovskites of type ABB □1/4WVIO6 ?; ABIIB □WO24 order disorder phenomena are present. The results of the x-ray and vibrational spectroscopic investigations as well as the diffuse reflectance spectra and the visible photoluminescence are reported.  相似文献   

2.
On Hexagonal Perovskites with Cationic Vacancies. I. Compounds of the Type Ba2B □2/3ReVIIO6 Compounds of Type Ba2B□2/3ReVIIO6 are formed with BIII = Sm? Gd Ho? Lu, Y, Sc, In (yellow); Tb (black-brown); Dy (yellow-orange). They crystallize with BIII = Sm? Lu, Y and Sc in a rhombohedral layer structure of 12 L-type (space group R3 m; sequence: cchhcchhcchh) with 6 formula units in the unit cell.  相似文献   

3.
On Hexagonal Perovskites with Cationic Vacancies. III. Structure Determination on Compounds of Type Ba2B □2/3 ReVIIO6 Compounds of Type Ba2B □2/3 ReVIIO6 with BIII = rare earth, Y. Sc, In belong to the group of hexagonal perovskite stacking polytypes. For BIII = Gd, Y structure determinations with powder data have been performed. The refined R′ factors are 9.11% for Ba2Gd1/3□2/3ReO6 and 12.07% for Ba2Y1/3□2/3ReO6. The structure represents a rhombohedral 12 L type (space group R3 m) with the sequence hhcchhcchhcc. The lattice contains groups of three octahedra connected by common faces which are linked together by a single octahedron via common vertices. In the block of three face-sharing octahedra the central octahedral lattice site is vacant and the two outer positions are occupied by the rhenium atoms. According to this distribution direct contact of occupied face-sharing octahedra is absent.  相似文献   

4.
On Hexagonal Perovskites with Cationic Vacancies. X. Compounds of Type Ba4BIII(ReW□O12) – New Rhombohedral 12 L-Stacking Polytypes Compounds of type Ba4BIII(ReW□O12) are described for BIII = Sc, In, Lu, Yb. They crystallize in the rhombohedral 12 L-stacking poly/type (space group R3 m, sequence (3)(1) ? hhcc).  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 Hexagonal Perovskites with Cationic Vacancies. XXXIII. Compounds of Type Ba6?xSrxB2?y3+SEy3+W3□O18 In the series Ba6?xSrxLu2?ySEy3+W3□O18 a substitution of Sr2+ for Ba2+ is possible. According to intensity calculations on powder data of BaSr5Lu1,6Ho0,4W3□O18 the compounds crystallize in a rhombohedral 18 L type with the sequence (hhcccc)3; space group R3 m. The refined, intensity related R' value is 11.5%. The differences in properties (diffuse reflectance spectra, photoluminescence) between the hexagonal modifications Ba6B2?y3+SEy3+W3□O18 (B3+ ? Gd, Y, Lu; SE3+ ? Sm, Eu, Tb, Dy, Ho, Er, Tm) and the corresponding cubic HT modifications are discussed.  相似文献   

7.
On Hexagonal Perovskites with Cationic Vacancies. XI. Stacking Polytype Ba6W42O18 The white Ba6W42O18, with a cation/vacancy ratio of 2:1 for the octahedral holes, is the first representative of a new stacking polytype for this formula type. It crystallizes in a rhombohedral six layer-structure with ahex = 10.130 Å chex = 13.960 Å Z = 3 (ρexp = 7.38 g/cm3; ρcalc = 7.418 g/cm3).  相似文献   

8.
On Hexagonal Perovskites with Cationic Vacancies. XII. Structure Determination on Ba6W42O18 The stacking polytype Ba6W42O18 is the first oxidic variant of the Cs3Tl2Cl9-type. The structure determination gave for the space group R3 c with the sequence (h)6, Z = 3, the refined, intensity related R′ value of 6.8%. The octahedral net consists of groups of two face sharing WO6 octahedra (W2O6/2;O6), which are in the (110) plane displaced against each other. In the doublé octahedra the tungsten atoms are shifted away from their ideal central position (W–W: 2.327 Å) with the result, that the W–W distance has increased to 2.905 Å.  相似文献   

9.
Compounds of the Type Ba3BIIM O9 with BII ? Mg, Ca, Sr, Ba, and MV ? Nb, Ta The hexagonal perovskites Ba3BIIMO9 (MV ? Nb, Ta) crystallize with BII ? Mg Ca in a 3 L structure (sequence (c)3) and BII ?; Sr in the hexagonal BaTiO3 type (6 L; sequence (hcc)2) with an 1:2 order for the B and M ions. Intensity calculations for Ba3SrNb2O9 and Ba3SrTa2O9 gave in the space group P63/mmc a refined, intensity related R′ value of 8.4% (Nb) and 9.0% (Ta) respectively. For BII ? Ba the perovskite Ba3BaTa2O9 has an orthorhombic distorted 6 L structure and forms with Ba3SrTa2O9 a continuous series of mixed crystals (Ba3Sr1?xBaxTa2O9). In the system Ba3Sr1?xBaxNb2O9 the range of existence of the hexagonal BaTiO3 type is confined to the Sr richer end. The pure Ba compound possesses a proper structure type (5 L: Ba5BaNb3□O13.51.5).  相似文献   

10.
On Hexagonal Perovskites with Cationic Vacancies. XIV. The Rhombohedral 12 L-Stacking Polytypes Ba2La2BII(W □O12) Rhombohedral 12 L-stacking polytypes with cationic vacancies of type Ba2La2BII-(W□O12) are reported for BII = Mg, Zn (white), Ni(light brown) and Co(brown). They crystallize in the space group R3 m, sequences (3 )(1) ? (hhcc)3. For BII = Cu, as a consequence of the Jahn Teller effect, a triclinic distorted lattice is observed.  相似文献   

11.
On Ordered Perovskites with Cationic Vacancies III. Ba2CeSb4/51/5O6, the First Representant of a New Perovskite Variant The lemon coloured Ba2CeSb4/51/5O6 is polymorphic. The HT modification has a cubic face centered (a = 8.539 Å) and the TT form a cubic primitive lattice (a = 8.531 Å). According to the density measurement there are 4 formula units of Ba2CeSb4/51/5O6 in the unit cell.  相似文献   

12.
On Hexagonal Perovskites with Cationic Vacancies. XVI. Rhombohedral 12 L-Stacking Polytypes Ba3AIIIM □O12 with MV = Nb, Ta The white quaternary oxides Ba3LaM□O12 with MV = Nb, Ta belong to the group of hexagonal perovskites with cationic vacancies. They crystallize in a rhombohedral 12 L-structure (sequence (hhcc)3; space group R3 m) with a = 5.751 Å; c = 28.11 Å (MV = Nb); a = 5.746 Å; c = 28.20 Å (Ta) and Z = 3. Signs for the formation of isotypic compounds with AIII = Pr, Nd could be obtained as well.  相似文献   

13.
On Oxygen Perovskites with Pentavalent Ruthenium A BIIIRuVO6 with AII = Ba, Sr The perovskites Ba2BIIIRuVO6 with BIII = La, Nd, Sm, Eu, Gd, Dy, Y, are cubic (BIII = La: a = 8,544 Å; Y: a = 8,337 Å); with a partial order for BIII and RuV. The Sc compound, Ba2ScRuO6, has a hexagonal 6 L structure (a = 5.795 Å; c = 14.229 Å; sequence (hcc)2)2. The lattice of the Sr perovskites, Sr2BIIIRuVO6, with BIII = Eu, Gd, Dy, Y is rhombic distorted. The IR and FRI spectra are discussed.  相似文献   

14.
On Hexagonal Perovskites with Cationic Vacancies. VII. Vibrational Spectroscopie investigations on the Rhombohedral 12 L-Stacking Polytypes Ba4BII(Re2□O12) and Ba4B □1/3 (Re2 □ O12) For the rhombohedral 12 L stacking polytypes Ba4BII(Re2□O12) and Ba4B□1/3(Re2□O 12), space group R3 m, sequence (3)(1), the lattice consists of groups of three face sharing octahedra with the composition Re2□O12. They are isolated from each other by the Ba and B ions.The vibrational spectra are interpreted according to the factor group analysis. For the Re2□O12 unit (symmetry D3d) the results of a complete vibrational analysis and the calculation of the force constants are reported.  相似文献   

15.
On ordered perovskites with cationic vacancies. VIII. Structure investigations on Ba2Ba7/81/8UO57/81/8 The reddish brown Ba2Ba7/81/8UO57/81/8 belongs to the group of oxygen perovskites with an ordered distribution of cationic vacancies. It crystallized tetragonally (a = 12.624 Å; c = 17.534 Å) with 16 formula units in the unit cell: Ba32Ba142U16O942. For the space group I4/mmm intensity calculations on powder data gave a refined, intensity related R′ value of 13.4%. The octahedrally coordinated barium an uranium atoms are 1:1 ordered; both cationic vacancies are located in the barium sublattice and form a body centered arrangement. For the 94 oxygen atoms and the two oxygen vacancies a statistical distribution was chosen. In the lattice all cations neighbouring the cationic vacancies are dislocated: The corresponding barium atoms in the close packed sheets move by ~0.55 Å in direction of the holes, on the contary the uranium atoms concerned are shifted away by ~0.17 Å and ~0.26 Å respectively.  相似文献   

16.
On Hexagonal Perovskites with Cationic Vacancies. XV. Ba9Nb6W□2O27 – the First Perovskite Stacking Polytype of Rhombohedral 27 L-Type The perovskite stacking polytype Ba9NbWVI2O27(white) is the first representative of a rhombohedral 27 L-type. The lattice parameters (trigonal setting) are: a = 5.793 Å; c = 63.41 Å; Z = 3 (?exp = 6.46 g/cm3; ?calc = 6.512 g/cm3). The corresponding TaV -compound is isotypic; it tends to develop stacking faults.  相似文献   

17.
On Hexagonal Perovskites with Cationic Vacancies. XX. Ba6Nb4Zr□o18 - a New Stacking Polytype with a Rhombohedra1 18 L Structure The white Ba6Nb4Zr□O18 crystallizes in a rhombohedral 18 L structure (a = 5.821 Å; c = 42.63 Å; space group R3 m) with three formula units for the trigonal setting (?exp = 6.05 g/cm3; ?calc = 6.271 g/cm3). The corresponding TiIV and HfIV compounds, Ba6Nb4Zr□O18 and Ba6Nb4Hf□O18, are isotypic.  相似文献   

18.
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   

19.
On Ordered Perovskites with Cationic Vacancies. II. The Incorporation of NbV in Ba2Gd0,670,33UO6 In Ba2Gd0.670.33UO6 a complete substitution of UVI by NbV is possible by filling the cationic vacancies (x-phase: Ba2Gd0.67+0.33xU1?xNbxO6). For the y-Phase (Ba2Gd0.67U1?yNbyO6?0.5y) solid solutions are formed only for y ? 0.5. The properties of both phases are studied by x-ray and spectroscopic methods. In Ba2GdNbO6 – in contrary to the complete ordered Ba2GdTaO6 – the order of gadolinium and niobium id partial.  相似文献   

20.
On Hexagonal Perovskites with Cationic Vacancies. XXIX. Structure of Ba4ScReW□O12 On the Function of Octahedral Cationic Vacancies in Perovskite Stacking Polytypes The hexagonal perovskite stacking polytype Ba4ScReW□O12 crystallizes in a rhombohedral 12 L structure (space group R3 m; sequence (hhcc)3). The refined, intensity related R′ value is 6.6%. The octahedral net consists of blocks of three face connected octahedra with a central vacancy, in the two outer positions the rhenium and tungsten atoms are located; this units are linked via common corners by single octahedra, occupied with scandium.  相似文献   

设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号