2009
DOI: 10.1016/j.jssc.2009.07.034
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Investigation of substitution effects and the phase transition in type-I clathrates Rb Cs8–Sn44□2 (1.3≤x≤2.1) using single-crystal X-ray diffraction, Raman spectroscopy, heat capacity and electrical resistivity measurements

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Cited by 16 publications
(8 citation statements)
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“…At room temperature, the α-A 8 Sn 44 2 phase adopts the type-I clathrate structure with a 2 × 2 × 2 superstructure (Ia3d space group) of the primitive cubic unit cell (Pm3n), which originates from a partial ordering of defects. The reversible transformation into the high-temperature β-form with the smaller unit cell with primitive symmetry occurs at the temperatures higher than 330 K [35,45,[48][49][50]. However, our SCXRD experiments performed at 200(2) K showed that some datasets could be indexed in Pm3n space group (Table 4), whereas other datasets show super-structure reflections consistent with the Ia3d model.…”
Section: Resultsmentioning
confidence: 73%
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“…At room temperature, the α-A 8 Sn 44 2 phase adopts the type-I clathrate structure with a 2 × 2 × 2 superstructure (Ia3d space group) of the primitive cubic unit cell (Pm3n), which originates from a partial ordering of defects. The reversible transformation into the high-temperature β-form with the smaller unit cell with primitive symmetry occurs at the temperatures higher than 330 K [35,45,[48][49][50]. However, our SCXRD experiments performed at 200(2) K showed that some datasets could be indexed in Pm3n space group (Table 4), whereas other datasets show super-structure reflections consistent with the Ia3d model.…”
Section: Resultsmentioning
confidence: 73%
“…The initial idea of the synthesis was to incorporate Europium into the clathrate cage as an extension of the work on Rb 8−x Eu x (In,Ge) 46 clathrates performed previously by our group [32], which proved unsuccessful (vide supra). The co-existence of both alkali metals and alkaline-earth metals, or Eu, is known for the different type-I clathrates, such as K 6 AE 2 M 5 Ge 41 (AE = Eu, Ba; M = Zn, Cd) and K 6 Eu 2 Ga 10 Ge 36 [7,33] [44,45], which show the tendency for the larger Cs to fill the larger 24-vertex cages, while the smaller Rb and K, in particular, are better suited for the smaller 20-vertex cage (Figure 2). The report on K 7.1 Ba 0.3 Ga 8.3 Sn 37.7 shows that it is possible to have Sn-bearing clathrates with guest atoms from Groups 1 and 2, where Ba occupies only one (2a) site [24].…”
Section: Resultsmentioning
confidence: 99%
“…The XRPD patterns were indexed in agreement with the reflection conditions of space group Ia $\bar{3}$ d , which is also supported by the TEM/SAED studies (Figure 3). This space group has already been known for the clathrate‐I phases M 8 Sn 44 □ 2 ( M = Rb, Cs)1820 or Ba 8 Ge 43 □ 3 ,2123 for which an ordering of vacancies leads to a 2 a 0 × 2 a 0 × 2 a 0 superstructure. In the case of compositions such as K 8 Li 2.29(16) Ge 43.47(3) □ 0.24(15) , however, the vacancy concentration is only small, so that the superstructure formation should primarily be related to an ordering of lithium atoms.…”
Section: Resultsmentioning
confidence: 91%
“…The Zn defects in Zn-Sb compounds and Cu defects Cu defects in Cu-chalcogenides are essential for decreasing lattice thermal conductivity and tuning of carrier concentrations [4][5][6][7][8][9][10]. In some Type-I clathrates, defects have been found in frameworks and the ordering of vacancies are important for the tuning of the Seebeck coefficient, electrical resistivity and thermal conductivity [11][12][13][14][15]. Defects in clathrates can also change the band structure as the bonding and antibonding orbitals of framework elements contribute to the bands near the Fermi-level [11].…”
Section: Introductionmentioning
confidence: 99%