Home Synthesis and structural characterization of the new rare-earth borosilicates Pr3BSi2O10 and Tb3BSi2O10
Article Publicly Available

Synthesis and structural characterization of the new rare-earth borosilicates Pr3BSi2O10 and Tb3BSi2O10

  • Sebastian Bräuchle and Hubert Huppertz EMAIL logo
Published/Copyright: November 17, 2015
Become an author with De Gruyter Brill

Abstract

The rare-earth borosilicates RE3BSi2O10 (RE = Pr, Tb) were synthesized under high-temperature conditions of 1600 °C in a radio frequency furnace from praseodymium oxide, terbium oxide, silicon dioxide, silicon nitride, boron trioxide, and boric acid. The structure determinations based on powder diffraction data revealed that both phases RE3BSi2O10 (RE = Pr, Tb) are isotypic to Gd3BSi2O10 [L. Chi, H. Chen, X. Lin, H. Zhuang, J. Huang, Jiegou Huaxue1998, 17, 297]. The compounds crystallize in the orthorhombic space group Pbca (no. 61) with eight formula units and the lattice parameters a = 982.9(2), b = 714.2(2), c = 2314.4(4) pm, V = 1.6247(4) nm3, Rp = 0.0231, and Rwp = 0.0354 (all data) for Pr3BSi2O10 and a = 960.5(5), b = 692.1(3), c = 2272.4(1) pm, V = 1.5106(2) nm3 for Tb3BSi2O10. The lattice parameters of Tb3BSi2O10 could be determined, but a final refinement of the powder data has not proved satisfactory. The structure of Pr3BSi2O10 exhibits eight- (Pr1) and ninefold coordinated rare-earth cations (Pr2 and 3). Layers of ortho-silicate anions [SiO4]4– and borosilicate anions [BSiO6]5– are arranged alternatingly along the c axis and the RE cations are located in between.

1 Introduction

In the last decades, interest in compounds with mixed oxide anions like rare-earth borosilicates is increasing. The reason lies in their possible application in laser materials and luminescent phosphors [1]. Up to now, there exist three different compositions in the substance class of borosilicates: REBSiO5 (RE = La–Nd, Sm) [2–5] with stillwellite structure, RE3BSi2O10 (RE = La, Ce, Nd, Sm–Gd) [6–11], and RE5Si2BO13 (RE = La, Pr, Nd, Sm–Gd, Dy) [12–14] with a structure related to apatite. The rare-earth borosilicates with stillwellite and apatite related structures both contain [BO4]5– and [SiO4]4– groups. Nekrasov et al. [2] and Neumann et al. [5] synthesized the phases REBSiO5 (RE = La–Nd, Sm) by solid state reactions and under hydrothermal conditions. The apatite related phase RE5Si2BO13 (RE = La) was first synthesized by Mazza et al. [12]. The third composition RE3BSi2O10 (RE = La, Ce, Nd, Sm–Gd) [6–11] contains triangular [BO3]3– groups, tetrahedral [SiO4]4– groups, and three crystallographically independent rare-earth cations. Serhan et al. [15] reported an isotypic structure with the composition Nd3BGe1.08Si0.92O10, where Ge and Si atoms are distributed statistically on the tetrahedral positions. The syntheses of borosilicates with the heavier and smaller rare-earth atoms (Tb–Lu) were not successful until now. For this reason, we focused our research onto the syntheses of the rare-earth borosilicates RE3BSi2O10 with the cations Pr and Tb–Lu. In the present part, we report the high-temperature syntheses and IR spectroscopic investigations of Pr3BSi2O10 and Tb3BSi2O10 (both compounds are isotypic to Gd3BSi2O10 [10]). For Pr3BSi2O10, a Rietveld structure refinement is presented.

2 Experimental section

2.1 Syntheses

The new rare-earth borosilicates RE3BSi2O10 (RE = Pr, Tb) were synthesized from a non-stoichiometric mixture of Pr6O11 (Strem Chemicals, Newburyport, MA, USA; 99.9+ %), Tb4O7 (Smart Elements GmbH, Wien, Austria; 99.99 %), B2O3 (Strem Chemicals, Newburyport, MA, USA; 99.9+ %), H3BO3 (Merck, Darmstadt, Germany; 99.5 %), SiO2 (Sigma-Aldrich, Inc., St. Louis, MO, USA; purum p.a.), and Si3N4 (Sigma-Aldrich, Inc., St. Louis, MO, USA; predominantly the α-modification).

The starting materials were mixed in the molar ratio 3:1:5:4:2, finely ground in an agate mortar and filled into boron nitride crucibles (Henze BNP GmbH, HeBoSint® S100, Kempten, Germany). The boron nitride crucibles were placed in tungsten crucibles (Plansee Metall GmbH, Reutte, Austria) and heated in a radio frequency furnace [16] (Hüttinger Elektronik GmbH + Co. KG, Freiburg, Germany) under N2 atmosphere (dried over silica gel/KOH/molecular sieves/P2O5, and BTS catalyst) to 1400 °C in 1 h, then the temperature was further raised to 1600 °C within 2 h. In the case of Pr3BSi2O10, 1600 °C were maintained for 4 h and then the sample was quenched to room temperature by switching off the furnace. For Tb3BSi2O10, the temperature of 1600 °C was lowered to 1400 °C within 1 h. Finally, the sample was quenched to room temperature. The new compound Pr3BSi2O10 was obtained as a light green pellet, and Tb3BSi2O10 in the form of a white pellet; both are air- and water-resistant. We presume that the syntheses of the new compounds are kinetically controlled. Only with the exact composition and heating process mentioned above it was possible to synthesize the new rare-earth borosilicates RE3BSi2O10 (RE = Pr, Tb). A stoichiometric mixture or the omittance of one of the starting materials did not lead to the desired phases. Instead, well known compounds like PrBO3 [17], Pr2Si2O7 [18], PrBSiO5 [2] or a mixture of two of them, and TbBO3 [17] as well as Tb2Si2O7 [19] in the case of RE = Tb were formed. In comparison to the syntheses of other rare-earth borosilicates, which were performed in evacuated silica tubes or hydrothermally [2–14], the duration of the syntheses could be markedly reduced from approximately 2 weeks to 6 h using a radio frequency furnace. One of the reasons for the reduction of the time of syntheses could be the increase of the temperature from 1000 °C to 1600 °C leading to a better diffusion.

2.2 X-ray powder diffraction analyses and Rietveld refinement

Pr3BSi2O10 and Tb3BSi2O10 were identified by powder X-ray diffraction measurements on flat samples of the reaction products, using a Stoe Stadi P powder diffractometer with Ge(111)-monochromatized MoKα1 (λ = 70.93 pm) radiation. Both powder diffraction patterns (Figs. 1 and 2) showed reflections of the corresponding rare-earth borosilicates RE3BSi2O10 (RE = Pr, Tb) and of side products. Due to the fact that both compounds RE3BSi2O10 (RE = Pr, Tb) are isotypic to Gd3BSi2O10 [10], a full-pattern Rietveld refinement was carried out with the program Topas [20]. The structural refinement was performed by taking the positional parameters of the isotypic phase Gd3BSi2O10 as starting values. For Pr3BSi2O10, constraints were set so that the B–O distances remained close to 1.37 Å and the Si–O distance close to 1.62 Å. During the refinement, the residual impurity could be identified as SiO2 [21]. The free refinement of individual displacement parameters for boron and oxygen led to unreasonable values. Therefore, one isotropic displacement parameter was refined, and set for all atoms. The final difference Fourier syntheses did not reveal any significant peaks in the refinement. Figure 3 shows the result of the Rietveld refinement of the X-ray powder diffractogram of Pr3BSi2O10. The residual values and all relevant details of the data collection and refinement are listed in Table 1. The Tables 2 and 3 list the positional parameters and interatomic distances for Pr3BSi2O10. The refinement of the powder data of Tb3BSi2O10 did not succeed until now. The program Diamond [22] was used for the graphical representation of the structure.

Fig. 1: Top: experimental powder pattern of Pr3BSi2O10. The reflections marked with a red asterisk arise from SiO2 as a residual starting material. Bottom: theoretical powder pattern of Pr3BSi2O10 based on the modified single-crystal diffraction data of Gd3BSi2O10 (Pr3+ instead of Gd3+ and lattice parameters of Pr3BSi2O10).
Fig. 1:

Top: experimental powder pattern of Pr3BSi2O10. The reflections marked with a red asterisk arise from SiO2 as a residual starting material. Bottom: theoretical powder pattern of Pr3BSi2O10 based on the modified single-crystal diffraction data of Gd3BSi2O10 (Pr3+ instead of Gd3+ and lattice parameters of Pr3BSi2O10).

Fig. 2: Top: experimental powder pattern of Tb3BSi2O10. The reflections marked with a red asterisk arise from SiO2 of residual starting material. Bottom: theoretical powder pattern of Tb3BSi2O10 based on the modified single-crystal diffraction data of Gd3BSi2O10 (Tb3+ instead of Gd3+ and lattice parameters of Tb3BSi2O10).
Fig. 2:

Top: experimental powder pattern of Tb3BSi2O10. The reflections marked with a red asterisk arise from SiO2 of residual starting material. Bottom: theoretical powder pattern of Tb3BSi2O10 based on the modified single-crystal diffraction data of Gd3BSi2O10 (Tb3+ instead of Gd3+ and lattice parameters of Tb3BSi2O10).

Fig. 3: Calculated (black) and observed (red crosses) X-ray powder diffractogram of Pr3BSi2O10. The difference curve (observed-calculated) is plotted below (blue). The short vertical bars indicate the positions of the reflections. First row: Pr3BSi2O10 (89.2(1) wt%), second row: SiO2 (10.8(1) wt%).
Fig. 3:

Calculated (black) and observed (red crosses) X-ray powder diffractogram of Pr3BSi2O10. The difference curve (observed-calculated) is plotted below (blue). The short vertical bars indicate the positions of the reflections. First row: Pr3BSi2O10 (89.2(1) wt%), second row: SiO2 (10.8(1) wt%).

Table 1

Powder data and structure refinement of Pr3BSi2O10.

Empirical formulaPr3BSi2O10
Molar mass, g mol–1649.71
Crystal systemorthorhombic
Space groupPbca (No. 61)
a, Å9.829(2)
b, Å7.142(1)
c, Å23.144(4)
V, Å31624.7(4)
Formula units per cell8
Calculated density, g·cm–35.31
Temperature, K293(2)
Powder diffractometerSTOE Stadi P
RadiationMoKα1 (λ = 70.93 pm)
MonochromatorGe(111)
range, deg2.0–75.0
Increment, deg0.15
Profile functionPseudo-Voigt
Background functionChebychev polynomial
Weighting schemeSigma
Phases, wt%
 Pr3BSi2O1089.2(1)
 SiO210.8(1)
Number of data points7345
Number of independent parameters79
Rp0.0278
Rwp0.0355
Rexp0.0231
Goodness of fit1.54
Table 2

Atomic coordinates (Wyckoff positions 8c for all atoms) and isotropic displacement parameters Beq of Pr3BSi2O10 (space group: Pbca). Beq was set to 0.476(1) for all atoms.

Atomxyz
Pr10.49086(1)0.36157(2)0.427720(4)
Pr20.13402(1)0.32978(2)0.336760(5)
Pr30.26709(1)0.09447(2)0.182260(5)
B10.2590(2)0.3752(3)0.96783(4)
Si10.37997(6)0.35426(9)0.07882(2)
Si20.44023(5)0.31526(7)0.28027(2)
O10.2536(1)0.2631(2)0.9196(4)
O20.13087(8)0.4158(2)0.9890(5)
O30.3636(1)0.3576(2)0.00843(4)
O40.4557(1)0.1718(2)0.10209(4)
O50.2331(1)0.3438(2)0.11134(4)
O60.4614(1)0.5281(2)0.10462(5)
O70.6054(8)0.3033(2)0.27681(4)
O80.4093(1)0.3815(2)0.21127(4)
O90.3891(9)0.4576(2)0.32911(3)
O100.3397(9)0.1415(2)0.29080(4)
Table 3

Interatomic distances (pm) in Pr3BSi2O10 (space group: Pbca).

Pr1–O4237.9(1)Pr2–O1234.4(9)Pr3–O7a237.7(9)
Pr1–O2a240.0(1)Pr2–O8248.1(9)Pr3–O8a240.3(1)
Pr1–O2b244.3(1)Pr2–O10a250.0(1)Pr3–O5a242.9(1)
Pr1–O1250.3(1)Pr2–O4251.9(1)Pr3–O5b244.5(1)
Pr1–O6254.0(1)Pr2–O6259.4(1)Pr3–O8b257.0(1)
Pr1–O5254.9(1)Pr2–O10b265.0(1)Pr3–O7b260.6(1)
Pr1–O9258.4(8)Pr2–O7265.0(9)Pr3–O10263.3(9)
Pr1–O3274.0(1)Pr2–O9a267.4(8)Pr3–O4268.0(1)
Pr2–O9b267.4(9)Pr3–O6291.5(1)
Ø = 251.7Ø = 256.5Ø = 256.2
Si1–O4159.3(1)Si2–O9160.1(9)B1–O1137.5(2)
Si1–O6159.4(1)Si2–O10160.5(9)B1–O2138.2(1)
Si1–O3163.0(1)Si2–O7162.7(9)B1–O3139.8(1)
Si1–O5163.7(1)Si2–O8169.3(1)
Ø = 161.4Ø = 163.2Ø = 138.5

2.3 Vibrational spectra

The FTIR-attenuated total reflection (ATR) spectra of powders were measured with a Bruker Alpha-P spectrometer with a diamond ATR-crystal (2×2 mm), equipped with a DTGS detector in the spectral range of 400– 4000 cm–1 (spectral resolution 4 cm–1). Twenty-four scans of the sample were acquired. A correction for atmospheric influences using the Opus 7.2 software was performed.

3 Results and discussion

3.1 Crystal structure of Pr3BSi2O10

The new rare-earth borosilicate Pr3BSi2O10 crystallizes isotypically to the structure of Gd3BSi2O10 in the orthorhombic space group Pbca (no. 61) with eight formula units per cell. The structure is composed of two different types of anions: ortho-silicate anions [Si2O4]4– and borosilicate anions [BSi1O6]5–, which are arranged alternatingly along the c axis (Fig. 4). The borosilicate anions consist of a [SiO4]4– tetrahedron and a [BO3]3– group sharing a common oxygen atom (Fig. 5). The three different rare-earth ions Pr1, Pr2, and Pr3 occupy the interlayer sites and are coordinated by eight (Pr1) and nine (Pr2, Pr3) oxygen atoms (Fig. 6). The Pr–O polyhedra are linked to each other through edge-sharing.

Fig. 4: Crystal structure of Pr3BSi2O10 (space group: Pbca).
Fig. 4:

Crystal structure of Pr3BSi2O10 (space group: Pbca).

Fig. 5: The borosilicate anion in Pr3BSi2O10.
Fig. 5:

The borosilicate anion in Pr3BSi2O10.

Fig. 6: Coordination polyhedra of the rare-earth ions Pr1 (left), Pr2 (center), and Pr3 (right).
Fig. 6:

Coordination polyhedra of the rare-earth ions Pr1 (left), Pr2 (center), and Pr3 (right).

The boron-oxygen distances inside of the [BO3]3– units range between 137.5(2) and 139.8(1) pm with a mean value of 138.5(2) pm for Pr3BSi2O10. This mean value of the boron oxygen distances in the [BO3]3– units corresponds to the values of the literature, which usually range around 137 pm [23–25]. The B–O–B angles are between 112.0(1) and 121.5(2)°. The Si1–O distances vary from 159.3(1) to 163.7(2) pm with a mean value of 161.4(2) pm. The interatomic distances Si2–O are between 160.1(9) and 169.3(2) pm with a mean value of 163.2(9) pm. The bond angles range from 102.7(7) to 114.3(7)° for O–Si1–O, and from 101.0(5) to 125.5(6)° for O–Si2–O in Pr3BSi2O10. The distances of the eightfold coordinated Pr1 to the oxygen atoms are 237.9(1)–274.0(1) pm with a mean value of 251.7(8) pm. Pr2 and Pr3 are coordinated by nine oxygen atoms; the bond lenghts vary from 234.4(9) to 267.4(9) pm with a mean value of 256.5(9) pm for Pr2 and from 237.6(9) to 291.5(1) pm with a mean value of 256.2(9) pm for Pr3. The Table 3 shows the interatomic distances of Pr3BSi2O10. For a detailed description of the structure, the reader is referred to the paper of the isotypic compound Gd3BSi2O10 [10]. In this work, we briefly compare the isotypic phases RE3BSi2O10 (RE = Ce, Pr, Gd).

Due to their isotypy, there is no large difference in the structures of Pr3BSi2O10, Ce3BSi2O10, and Gd3BSi2O10. Table 4 compares the unit cells, the coordination numbers of the rare-earth metal ions, and the bond lengths. The differences of the lattice parameters a, b and c correspond to the decrease in the ionic radii from Ce3+ to Gd3+, which is based on the lanthanide contraction. Due to the fact that the size difference is marginal, no greater deviations of the bond lengths and angles are observed.

Table 4

Comparison of the isotypic structures RE3BSi2O10 (RE = Ce, Pr, Gd, and Tb).

Empirical formulaCe3BSi2O10Pr3BSi2O10Gd3BSi2O10Tb3BSi2O10
Reference[7]this work[10]this work
Molar mass, g mol–1647.3649.7698.7703.8
Unit cell dimensions
a, pm990.07(6)982.86(2)963.0(1)960.5(5)
b, pm720.36(4)714.22(1)695.9(1)692.1(3)
c, pm2329.2(2)2314.36(4)2279.2(3)2272.4(2)
Coordination number (CN)
RE18888
RE29999
RE39999
av. RE1–O distances, pm250.7(1)251.7(8)252.1(1)
av. RE2–O distances, pm261.4(1)256.5(9)249.3(1)
av. RE3–O distances, pm262.4(1)256.2(9)241.9(1)
av. Si1–O distances, pm163.3(1)161.4(1)162.1(2)
av. Si2–O distances, pm162.9(1)163.2(9)162.1(1)
av. B–O distances in [BO3]3–, pm138.5(1)138.5(2)137.4(2)

3.2 IR spectroscopy

The spectra of the FTIR-ATR measurements of Pr3BSi2O10 and Tb3BSi2O10 are displayed in Fig. 7. The assignments of the vibrational modes are based on a comparison with the experimental data of borates containing trigonal [BO3]3– groups [26–30] and of borosilicates containing tetrahedral [SiO4]4– groups [31, 32]. For borates containing [BO3]3– groups, absorption bands at 1200–1450 cm–1 (stretching vibrations) and at 600–800 cm–1 (bending vibrations) are expected. The absorption bands for tetrahedral [SiO4]4– groups in borosilicates are expected at 400–600 cm–1 (bending vibrations) and at 650–1100 cm–1 (stretching vibrations). In the FTIR spectrum of the new praseodymium and terbium borosilicates, the expected [BO3]3– modes are detected between 1200 and 1450 cm–1 and between 600 and 800 cm–1. The [SiO4]4– modes are between 400 and 600 cm–1 and between 650 and 1100 cm–1. Furthermore, no bands for OH groups or water could be detected in the range of 3000 to 3600 cm–1.

Fig. 7: FT-IR reflectance spectrum of Pr3BSi2O10 (red) and Tb3BSi2O10 (black).
Fig. 7:

FT-IR reflectance spectrum of Pr3BSi2O10 (red) and Tb3BSi2O10 (black).

4 Conclusions

With the synthesis of Pr3BSi2O10, the list of the known compounds in the system RE3BSi2O10 could be extended by an additional compound. It crystallizes in the space group Pbca, being isotypic to the structure of Gd3BSi2O10. The main structural characteristics are the ortho-silicate anion [SiO4]4– and the borosilicate anion [BSiO6]5–, which form alternating layers along the c axis, with the RE cations located in between. Pr1 is surrounded by eight oxygen atoms while Pr2 and Pr3 are coordinated by nine oxygen atoms. The synthesis of the isotypic compound Tb3BSi2O10 was also successful, but up to now, a successful Rietveld refinement of the powder data failed.


Corresponding author: Hubert Huppertz, Institut für Allgemeine, Anorganische und Theoretische Chemie, Leopold-Franzens-Universität Innsbruck, Innrain 80–82, A-6020 Innsbruck, Austria, e-mail:

References

[1] S. Yu. Stefanovich, V. N. Sigaev, A. V. Dechev, A. V. Mosunov, V. R. Samygina, N. I. Leonyuk, P. D. Sarkisov, Izv. Ross. Akad. Nauk Ser. Neoorgan. Mater. 1995, 31, 819.Search in Google Scholar

[2] I. Ya. Nekrasov, R. A. Nekrasova, Dokl. Akad. Nauk SSSR1971, 201, 1202.Search in Google Scholar

[3] J. McAndrew, T. R. Scott, Nature1955, 176, 509.10.1038/176509b0Search in Google Scholar

[4] A. A. Voronkov, Y. A. Pyatenko, Kristallografiya1967, 12, 241.Search in Google Scholar

[5] H. Neumann, S. Bergstol, B. Nilssen, Norsk. Geol. Tidsskr. 1966, 46, 327.Search in Google Scholar

[6] H. Müller-Bunz, Th. Schleid, Z. Kristallogr. 1998, Suppl. 15, 48.Search in Google Scholar

[7] H. Müller-Bunz, H. Grossholz, Th. Schleid, Z. Anorg. Allg. Chem. 2001, 627, 1436.10.1002/1521-3749(200107)627:7<1436::AID-ZAAC1436>3.0.CO;2-#Search in Google Scholar

[8] L. Chi, H. Chen, S. Deng, H. Zhuang, J. Huang, Acta Crystallogr. 1996, C52, 2385.10.1107/S0108270196005069Search in Google Scholar

[9] L. Chi, H. Chen, S. Deng, H. Zhuang, J. Huang, J. Alloys Compd. 1996, 242, 1.10.1016/0925-8388(96)02301-8Search in Google Scholar

[10] L. Chi, H. Chen, X. Lin, H. Zhuang, J. Huang, Jiegou Huaxue1998, 17, 297.Search in Google Scholar

[11] E. Shavanskii, N. I. Leonyuk, G. Bocelli, L. Right, J. Solid State Chem. 2000, 154, 312.10.1006/jssc.2000.8855Search in Google Scholar

[12] D. Mazza, M. Tribaudino, A. Delmastro, B. Lebech, J. Solid State Chem. 2000, 155, 389.10.1006/jssc.2000.8929Search in Google Scholar

[13] J. Yuan, Z. Zhang, X. Wang, H. Chen, J. Zhao, G. Zhang, C. Shi, J. Solid State Chem. 2007, 180, 1365.10.1016/j.jssc.2007.01.033Search in Google Scholar

[14] S. Asiri Naidu, U. V. Varadaraju, B. Raveau, J. Solid State Chem. 2010, 183, 1847.10.1016/j.jssc.2010.05.034Search in Google Scholar

[15] K. Serhan, M. Taibi, J. Aride, A. Boukhari, J. Darriet, G. Le Flem, J. Solid State Chem. 1994, 110, 384.10.1006/jssc.1994.1183Search in Google Scholar

[16] W. Schnick, H. Huppertz, R. Lauterbach, J. Mater. Chem. 1999, 9, 289.10.1039/a803900cSearch in Google Scholar

[17] R. Velchuri, B. V. Kumar, V. R. Devi, G. Prasad, D. J. Prakash, M. Vithal, Mater. Res. Bull. 2011, 46, 1219.10.1016/j.materresbull.2011.04.006Search in Google Scholar

[18] J. Felsche, Z. Kristallogr. 1971, 133, 364.10.1524/zkri.1971.133.133.364Search in Google Scholar

[19] M. E. Fleet, X. Y. Liu, Z. Kristallogr. 2003, 218, 795.10.1524/zkri.218.12.795.20550Search in Google Scholar

[20] Topas (version 4.2), Bruker Analytical X-ray Instruments Inc., Madison, Wisconsin (USA) 2009.Search in Google Scholar

[21] K. Ogata, Y. Takeuchi, Y. Kudoh, Z. Kristallogr. 1987, 179, 403.10.1524/zkri.1987.179.1-4.403Search in Google Scholar

[22] K. Brandenburg, Diamond (version 3.2i), Crystal and Molecular Structure Visualization, Crystal Impact-H. Putz & K. Brandenburg GbR, Bonn (Germany) 2012. See also: http://www.crystalimpact.com/diamond/.Search in Google Scholar

[23] F. C. Hawthorne, P. C. Burns, J. D. Grice, in Boron: Mineralogy, Petrology and Geochemistry, (Ed.: E. S. Grew), Mineralogical Society of America, Washington, DC, 1996.Search in Google Scholar

[24] E. Zobetz, Z. Kristallogr. 1982, 160, 81.10.1524/zkri.1982.160.1-2.81Search in Google Scholar

[25] E. Zobetz, Z. Kristallogr. 1990, 191, 45.10.1017/S0362152900012733Search in Google Scholar

[26] J. P. Laperches, P. Tarte, Spectrochim. Acta, 1966, 22, 1201.10.1016/0371-1951(66)80023-1Search in Google Scholar

[27] H. Böhlhoff, U. Bambauer, W. Hoffmann, Z. Kristallogr. 1971, 133, 386.10.1524/zkri.1971.133.133.386Search in Google Scholar

[28] K. Machida, H. Hata, K. Okune, G. Adachi, J. Shiokawa, J. Inorg. Nucl. Chem. 1979, 41, 1425.Search in Google Scholar

[29] A. Haberer, H. Huppertz, J. Solid State Chem. 2009, 182, 888.10.1016/j.jssc.2009.01.023Search in Google Scholar

[30] A. Haberer, M. Enders, R. Kaindl, H. Huppertz, Z. Naturforsch. 2010, 65b, 1213.10.1515/znb-2010-1006Search in Google Scholar

[31] J. Kristof, J. Mink, E. Horvath, M. Gabor, Vibrat. Spectrosc. 1993, 5, 61.10.1016/0924-2031(93)87055-XSearch in Google Scholar

[32] M. Handke, W. Mozgawa, Vibrat. Spectrosc. 1993, 5, 75.10.1016/0924-2031(93)87057-ZSearch in Google Scholar

Received: 2015-9-1
Accepted: 2015-9-10
Published Online: 2015-11-17
Published in Print: 2015-12-1

©2015 by De Gruyter

Downloaded on 30.9.2025 from https://www.degruyterbrill.com/document/doi/10.1515/znb-2015-0143/html
Scroll to top button